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1

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Gasoline and Diesel Fuel Update (EIA)

176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY...

2

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Gasoline and Diesel Fuel Update (EIA)

0.00-1.99 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 18. Average Price of Natural Gas Delivered to U.S. Onsystem Industrial Consumers, 1996 (Dollars per Thousand Cubic Feet) Figure 19. Average Price of Natural Gas Delivered to U.S. Electric Utilities, 1996 (Dollars per Thousand Cubic Feet) Figure Sources: Federal Energy Regulatory Commission (FERC), Form FERC-423, "Monthly Report of Cost and Quality of Fuels for Electric Plants," and Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." Note: In 1996, consumption of natural gas for agricultural use

3

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Gasoline and Diesel Fuel Update (EIA)

accomplishments accomplishments are impressive in themselves, and associ- ated with each milestone is the expansion of future produc- tion opportunities as another technical barrier is overcome. The extension of recovery opportunities into deep water has established the deep offshore as an area of considerable national significance. A second source of increased supply is gas from coalbed formations. Natural gas production from coalbed methane fields continued to grow in 1996 as projects initiated mainly in the early to mid 1990's matured through the dewatering phase into higher rates of gas production. Coalbed forma- tions contribute almost 1 trillion cubic feet, roughly 5 per- cent, to total U.S. production. Continued production growth from coalbeds is not likely in light of the precipitous drop in new wells completed in coalbed formations since the termination of the production tax

4

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Annual Energy Outlook 2012 (EIA)

857, "Monthly Report of Natural Gas Purchases and Deliveries to Consumers." 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 15. Average City Gate Price of Natural...

5

IL  

Office of Legacy Management (LM)

:; / 2. ' :; / 2. ' b-:-"y .",...4 * .-.a 2 IL !< :. 34 --' -, ' ' < I ,-. g Tvo"l r . . .-i- :- " .1-. . . . . NC0 /L ' J,, ' ;.' , -_I( + ? CENTRAL FILES c -&' { ' c;$y ;;j*' E ,J): ' i' Z, 1; p -^ r-raL-r.nuzT".Fn., , ,..-y - -' -ie .". iJ.&:~e!ct.;;' sf ' ;;i_is ,trip ' JG,' go f-Jj;~ey~ 2123 -:s Cc::!<:\.& a k,ea 1:1,:r a;::: zzft:k-~ .sl.x"fe:; an:: , I to a&-isc 2n tiie g Tc;t?z ~,;~~~,;;'

6

Weights and Measures State Directors IL  

Science Conference Proceedings (OSTI)

State Directors IL. Idaho. Mailing Address, Contact Information. ISDA Bureau of Weights & Measures PO Box 790 Boise, ID 83701. ...

2013-05-07T23:59:59.000Z

7

27-ID and 35-ID Construction Schedule | Advanced Photon Source  

NLE Websites -- All DOE Office Websites (Extended Search)

27-ID and 35-ID Past 27-ID and 35-ID Long Range Schedule (pdf) 27-ID and 35-ID, Construction Schedule Electrical and PSS work continues on 35-ID-B and C. Will not run the main...

8

Type Ia Supernovae Project at NERSC  

NLE Websites -- All DOE Office Websites (Extended Search)

Type Ia Supernovae Type Ia Supernovae Supernova-1.jpg Update: Recent Berkeley Lab Computing Sciences News about supernovae: read more... Key Challenges: Understanding Type Ia...

9

BLDG. ID NAME  

NLE Websites -- All DOE Office Websites (Extended Search)

a: main site Building Inventory 2006 appendices BLDG. ID NAME (B)UILDING (T)RAILER MAP GRID REF SIzE (GSF) 002 Advanced Materials Lab B D&24; &24;5,506 002A Central Chemical Storage B D&24;...

10

Category:Mason, IA | Open Energy Information  

Open Energy Info (EERE)

IA IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Mason, IA" The following 16 files are in this category, out of 16 total. SVQuickServiceRestaurant Mason IA MidAmerican Energy Co (Iowa).png SVQuickServiceRestaura... 64 KB SVFullServiceRestaurant Mason IA MidAmerican Energy Co (Iowa).png SVFullServiceRestauran... 64 KB SVHospital Mason IA MidAmerican Energy Co (Iowa).png SVHospital Mason IA Mi... 73 KB SVLargeHotel Mason IA MidAmerican Energy Co (Iowa).png SVLargeHotel Mason IA ... 72 KB SVLargeOffice Mason IA MidAmerican Energy Co (Iowa).png SVLargeOffice Mason IA... 73 KB SVMediumOffice Mason IA MidAmerican Energy Co (Iowa).png SVMediumOffice Mason I... 69 KB SVMidriseApartment Mason IA MidAmerican Energy Co (Iowa).png

11

LAX XXlCfl jX?iK, Idd+?KYLViG?IA  

Office of Legacy Management (LM)

f f , : I~&l, samtier cipwati8Aa CffUm - . Jiux.lCJ d,# 1754 - - _- - .- t :; . Jesse e. ahizmn*~*ter -2.' -------- - _ &tV' hi@A l f izau Bkteriala ;' . . 1 -7 I _' i' . Fpr&G& r&Q Q,&& fu &fI& L;&& -l&d 2;,i' iI,;/Qi' rIGN CQ&GgJy p;E& p;~p>gyf LAX XXlCfl jX?iK, Idd+?KYLViG?IA i-icfer~~o is &o ta yaw rwarandu3;: l P iimwmbec L?, 1953, reque&in~ a d&q.&ti of khority tA A&sister prog= for th+zz developmrrrl, Ii-&k& & acyui8itti ef c;uYletit*type and reswitlitc-type urtim bi:aPing eres and far t3-u jx*uctim and acquisitian 6f W ;aniU CCm- csa:ratc~ fhzi awes wit2n Lhe Six&e of Pemlsyzvania. 1 da not b&i- the projscrt fmr the pkcch2670 +S eroa from i&d.&

12

Il.-'",.'  

Office of Legacy Management (LM)

,,.. .r' ,,.. .r' +p,o~ ,!,*' A;>$, :.::> ,' ; ,.;I:- : ~ ", ,r .,,. ' , ' i.,l<, ~ ,1* .iT ,.~~~~~~~I~ _,L :,~.:/: .,,.,,,.,' ,, ;, ,, ,, I .. ,(: _ : ; . , y.,+ lar&f&r!rj&~+ ,id) L"'w#~~~~* I. ,& f ;";.y,m; ,I @ & **t&,y%:iis ;*a k' q&t ,:.: ;,I,' ,,, ,_ *, . ,. ,,&S_ ;, , (, t+ I . 1. -. ' ,' ~' i"'i,!..l + *I .(, h," ,rz ,. ,' :' ,' . :,' . ,.' _-#I_ ,. ,I. :, ,.' , ..I>. Xi,,? ,I. , ,r c/i' ,"" >.:1.. .>,. w/.&q:r*x Il.-'",.' !,.~~,,,~~iyY;~~~aj' ,~,,~~~~~~~~~ri~ *~i..iz~~ri~~~J~illi~;' ~(l~.~~i:)i9:ll~,-' i ?, ".' a? ,,?J,?" ~~~~I~~.~,~~~~~~~~.~~~~~~~~~~~~~-~ +q86?,r$w4t .r:~:@o:, " .", ' 1 j/ +$+. : WJl @+&?+&&w ' . 2 _ ._ b )., .;,a. :,. I .b.i.:.,*. A'

13

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

INL/EXT-08-13979 INL/EXT-08-13979 U.S. Department of Energy Office of Electricity Delivery and Energy Reliability Enhancing control systems security in the energy sector NSTB National SCADA Test Bed Common Cyber Security Vulnerabilities Observed in Control System Assessments by the INL NSTB Program November 2008 November 2008 INL/EXT-08-13979 Common Cyber Security Vulnerabilities Observed in Control System Assessments by the INL NSTB Program November 2008 Idaho National Laboratory Idaho Falls, Idaho 83415 http://www.inl.gov Prepared for the U.S. Department of Energy Office of Electricity Delivery and Energy Reliability Under DOE Idaho Operations Office Contract DE-AC07-05ID14517 Common Cyber Security Vulnerabilities Observed in Control System Assessments by the INL NSTB

14

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

INEEL/EXT-04-02423 INEEL/EXT-04-02423 ABB SCADA/EMS System INEEL Baseline Summary Test Report J. R. Davidson M. R. Permann B. L. Rolston S. J. Schaeffer November 2004 Prepared by: Idaho National Engineering and Environmental Laboratory INEEL/EXT-04-02423 ABB SCADA/EMS System INEEL Baseline Summary Test Report J. R. Davidson M. R. Permann B. L. Rolston S. J. Schaeffer November 2004 Idaho National Engineering and Environmental Laboratory INEEL National Security Division Idaho Falls, Idaho 83415 Prepared for the U.S. Department of Energy Office of Energy Assurance Under DOE Idaho Operations Office Contract DE-AC07-99ID13727 ABB SCADA/EMS System INEEL Baseline Summary Test Report INEEL/EXT-04-02423 November 2004 ABSTRACT The Idaho National Engineering and Environmental Laboratory

15

4-ID-D Instrumentation  

NLE Websites -- All DOE Office Websites (Extended Search)

4-ID-D Instrumentation Detectors Integrating Counting Area Diffractometors 8-Circle 4Tesla Magnet 13 Tesla Magnet Focussing Zone Plate Optics K-B Mirror System Temperature Control...

16

DOE-ID Operations Summary  

NLE Websites -- All DOE Office Websites (Extended Search)

September 10, 2013 DOE-ID Operations Summary For the Period August 12, 2013 through August 26, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho...

17

Prospective Type Ia supernova surveys from Dome A  

E-Print Network (OSTI)

Prospective Type Ia Supernova Surveys From Dome A A. Kim a ,are conducive toward Type Ia supernova surveys forheterogeneities within the Type Ia supernova class, reducing

Kim, A.

2010-01-01T23:59:59.000Z

18

Category:Boise, ID | Open Energy Information  

Open Energy Info (EERE)

ID ID Jump to: navigation, search Go Back to PV Economics By Location Media in category "Boise, ID" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Boise ID Idaho Power Co.png SVFullServiceRestauran... 61 KB SVHospital Boise ID Idaho Power Co.png SVHospital Boise ID Id... 62 KB SVLargeHotel Boise ID Idaho Power Co.png SVLargeHotel Boise ID ... 66 KB SVLargeOffice Boise ID Idaho Power Co.png SVLargeOffice Boise ID... 58 KB SVMediumOffice Boise ID Idaho Power Co.png SVMediumOffice Boise I... 63 KB SVMidriseApartment Boise ID Idaho Power Co.png SVMidriseApartment Boi... 61 KB SVOutPatient Boise ID Idaho Power Co.png SVOutPatient Boise ID ... 62 KB SVPrimarySchool Boise ID Idaho Power Co.png SVPrimarySchool Boise ... 62 KB SVQuickServiceRestaurant Boise ID Idaho Power Co.png

19

RL·721 Document ID Number:  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Document ID Number: Document ID Number: REV 3 NEPA REVIEW SCREENING FORM DOE/CX-00045 . J.proj(;l~t Titl~: - - - -- - - - - - - - - - - - - - - - - - -- --------- ------_. . _ - - - - - - - - - - - - - . - - - - - - - - - - - - - - - - - - - LIMITED FIREBREAK MAINTENANCE ON THE HANFORD SITE DURING CALENDAR YEAR 2012 II. Project Description and Location (including Time Period over which proposed action will occur and Project Dimensions· e.g., acres displaced/disturbed, excavation length/depth, etc.): The Department of Energy (DOE) proposes to perform firebreak maintenance in selected areas of the Hanford Site during calendar year 2012 with limited use of physical, chemical, and prescribed burning methods. Prescribed burning will be performed by the Hanford Fire Department under approved burn plans and permits; and only in previously disturbed

20

DOE-ID Operations Summary  

NLE Websites -- All DOE Office Websites (Extended Search)

June 5, 2013 June 5, 2013 DOE-ID Operations Summary For the Period May 16, through May 30, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho National Laboratory, managed by DOE- Idaho Operations Office. It has been compiled in response to a request from stakeholders for more information on health, safety and environmental incidents at DOE facilities in Idaho. It also includes a brief summary of accomplishments at the Site. POC - Shannon Brennan, DOE-ID, (208) 526-3993. Advanced Mixed Waste Treatment Project (AMWTP) [No items to Report] Idaho Cleanup Project (ICP) May 15 - 30, 2013: CH2M-WG Idaho, LLC discovered three instances of new information at the Integrated Waste Treatment Unit (IWTU) which have the potential to impact the nuclear safety analysis

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Document ID Number: RL-721  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Document ID Number: Document ID Number: RL-721 REV 4 NEPA REVIEW SCREENING FORM DOE/CX-00066 I. Project Title: Nesting Bird Deterrent Study at the 241-C Tank Farm CX B3.8, "Outdoor Terrestrial Ecological and Environmental Research" II. Project Description and Location (including Time Period over which proposed action will occur and Project Dimensions - e.g., acres displaced/disturbed, excavation length/depth, area/location/number of buildings, etc.): Washington River Protection Solutions LLC (WRPS) will perform an outdoor, terrestrial ecological research study to attempt to control and deter nesting birds at the 241-C Tank Farm. This will be a preventative study to test possible methods for controlling &/or minimizing the presence and impacts of nesting birds inside the tank farm. A nesting bird

22

IL.26  

Office of Legacy Management (LM)

ixa6-q ?k.m+~ ixa6-q ?k.m+~ @ lo3 IL.26 -ORNL/TM-11552 OAK RIDGE NATIONAL LABORATORY PRELIMINARY RESULTS OF THE RADIOLOGICAL SURVEY AT THE FORMER DOW CHEMICAL COMPANY SITE, MADISON, ILLINOIS c W . D. Cottrell J. K. W illiams OPERATED BY MARTIN MARIETTA ENERGY SYSTEMS, INC. FOR THE UNITED STATES DEPARTMENT OF ENERGY This report has been reproduced directly from the best available copy. Available to DOE and DOE contractors from the Office of Scientific and Techni- cal Information, P.O. Box 62. Oak Ridge, TN 37831; prices available from (615) 5766401, PTS 626-840 1. Availabie to the public from the National Technical Information Service, U.S. Department of Commerce, 5285 Port Royal Rd., Springfield, VA 22161. I I This report was prepared as an account of work sponsored by an agency of

23

Federal ID Credential Security Standard Strengthens ...  

Science Conference Proceedings (OSTI)

Federal ID Credential Security Standard Strengthens Authentication, Extends To Mobile Devices. From NIST Tech Beat: September 5, 2013. ...

2013-09-17T23:59:59.000Z

24

Turbulent Combustion in Type Ia Supernova Models  

E-Print Network (OSTI)

We review the astrophysical modeling of type Ia supernova explosions and describe numerical methods to implement numerical simulations of these events. Some results of such simulations are discussed.

F. K. Roepke; W. Hillebrandt

2006-09-15T23:59:59.000Z

25

New approaches for modeling type Ia supernovae  

SciTech Connect

Type Ia supernovae (SNe Ia) are the largest thermonuclearexplosions in the Universe. Their light output can be seen across greatstances and has led to the discovery that the expansion rate of theUniverse is accelerating. Despite the significance of SNe Ia, there arestill a large number of uncertainties in current theoretical models.Computational modeling offers the promise to help answer the outstandingquestions. However, even with today's supercomputers, such calculationsare extremely challenging because of the wide range of length and timescales. In this paper, we discuss several new algorithms for simulationsof SNe Ia and demonstrate some of their successes.

Zingale, Michael; Almgren, Ann S.; Bell, John B.; Day, Marcus S.; Rendleman, Charles A.; Woosley, Stan

2007-06-25T23:59:59.000Z

26

Theoretical cosmic Type Ia supernova rates  

E-Print Network (OSTI)

The aim of this work is the computation of the cosmic Type Ia supernova rates at very high redshifts (z>2). We adopt various progenitor models in order to predict the number of explosions in different scenarios for galaxy formation and to check whether it is possible to select the best delay time distribution model, on the basis of the available observations of Type Ia supernovae. We also computed the Type Ia supernova rate in typical elliptical galaxies of different initial luminous masses and the total amount of iron produced by Type Ia supernovae in each case. It emerges that: it is not easy to select the best delay time distribution scenario from the observational data and this is because the cosmic star formation rate dominates over the distribution function of the delay times; the monolithic collapse scenario predicts an increasing trend of the SN Ia rate at high redshifts whereas the predicted rate in the hierarchical scheme drops dramatically at high redshift; for the elliptical galaxies we note that the predicted maximum of the Type Ia supernova rate depends on the initial galactic mass. The maximum occurs earlier (at about 0.3 Gyr) in the most massive ellipticals, as a consequence of downsizing in star formation. We find that different delay time distributions predict different relations between the Type Ia supernova rate per unit mass at the present time and the color of the parent galaxies and that bluer ellipticals present higher supernova Type Ia rates at the present time.

R. Valiante; F. Matteucci; S. Recchi; F. Calura

2008-07-15T23:59:59.000Z

27

Steamboat IA Geothermal Facility | Open Energy Information  

Open Energy Info (EERE)

IA Geothermal Facility IA Geothermal Facility Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Steamboat IA Geothermal Facility General Information Name Steamboat IA Geothermal Facility Facility Steamboat IA Sector Geothermal energy Location Information Location Washoe, Nevada Coordinates 40.5608387°, -119.6035495° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.5608387,"lon":-119.6035495,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

28

APS Beamline 6-ID-D  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees 6-ID-D Home Recent Publications Beamline Info Optics Instrumentation Software User Info Beamline 6-ID-D Beamline 6-ID-D is operated by the Magnetic Materials Group in the X-ray Science Division (XSD) of the Advanced Photon Source. This is a high energy (50 - 130 keV) beamline used for structural studies primarily on single crystal materials. Recent Research Highlights LuFeO Unlikely route to ferroelectricity May 16, 2012 A new type of ferroelectric, LuO2Fe4, has been investigated at the APS by a research team from Julich research center. XAS & XMCD studies on beamline 4-ID-C determined the Fe magnetism and valence, while single crystal x-ray scattering measurements at 6-ID-B & 6-ID-D probed the associated structural and charge ordering.

29

DOE-ID Operations Summary  

NLE Websites -- All DOE Office Websites (Extended Search)

26, 2013 26, 2013 DOE-ID Operations Summary For the Period July 29, 2013 through August 12, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho National Laboratory, managed by DOE- Idaho Operations Office. It has been compiled in response to a request from stakeholders for more information on health, safety and environmental incidents at DOE facilities in Idaho. It also includes a brief summary of accomplishments at the Site. POC -Danielle Miller, (208) 526-5709. Advanced Mixed Waste Treatment Project (AMWTP) July 31, 2013: The Idaho Treatment Group, LLC (ITG), the managing contractor for the Advanced Mixed Waste Treatment Project received a warning letter from the State of Idaho's Department of Environmental quality regarding self- reported RCRA permit violations which

30

DOE-ID Operations Summary  

NLE Websites -- All DOE Office Websites (Extended Search)

18, 2013 18, 2013 DOE-ID Operations Summary For the Period September 30, 2013 through October 31, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho National Laboratory, managed by DOE- Idaho Operations Office. It has been compiled in response to a request from stakeholders for more information on health, safety and environmental incidents at DOE facilities in Idaho. It also includes a brief summary of accomplishments at the Site. POC -Danielle Miller, (208) 526-5709. Advanced Mixed Waste Treatment Project (AMWTP) October 15, 2013: A manager at the Advanced Mixed Waste Treatment Project (AMWTP) determined that the AMWTP Safety Analysis process required review due to an operational trend of fire/combustion events in the Treatment Facility (TF) box lines. Safety analysis for the TF is

31

DOE-ID Operations Summary  

NLE Websites -- All DOE Office Websites (Extended Search)

January 6, 2014 January 6, 2014 DOE-ID Operations Summary For the Period November 01, 2013 through November 30, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho National Laboratory, managed by DOE- Idaho Operations Office. It has been compiled in response to a request from stakeholders for more information on health, safety and environmental incidents at DOE facilities in Idaho. It also includes a brief summary of accomplishments at the Site. POC -Danielle Miller, (208) 526-5709. Advanced Mixed Waste Treatment Project (AMWTP) Nothing to Report Notable Accomplishments: Contracting companies supporting EM's cleanup program and the Office of Nuclear Energy at the Idaho site volunteered to be among the first to use a new DOE

32

II.CONTRACT ID CODE  

National Nuclear Security Administration (NNSA)

1 1 II.CONTRACT ID CODE ~AGE 1 of AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT PAGES AC 5. PROJECT NO. (If applicable) 3. EFFECTNE DATE 2. AMENDMENTfMODIFICA TION NO. 4. REQUISITIONIPURCHASE REQ. NO. See Block 16c. NOPR 7. ADMINISTERED BY (If other than Item 6) CODE 05008 6. ISSUED BY CODE 05008 U.S. Department of Energy National Nuclear Security Administration U.S. Department of Energy National Nuclear Security Administration P.O. Box 2050 Oak Ridge, TN 37831 P.O. Box 2050 Oak Ridge, TN 37831 9A. AMENDMENT OF SOLICITATION NO. 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) Babcock & Wilcox Technical Services Y-12, LLC P.O. Box 2009 MS 8014 9B. DATED (SEE ITEM 11) Oak Ridge, TN 37831-8014 lOA. MODIFICATION OF CONTRACT/ORDER NO.

33

The progenitors of subluminous type Ia supernovae  

DOE Green Energy (OSTI)

We find that spectroscopically peculiar subluminous SNe Ia come from an old population. Of the thirteen subluminous SNe Ia known, nine are found in E/S0 galaxies, and the remainder are found in early-type spirals. The probability that this is a chance occurrence is only 0.1%. The finding that subluminous SNe Ia are associated with an older stellar population indicates that for a sufficiently large lookback time (already accessible in current high redshift searches) they will not be found. Due to a scarcity in old populations, hydrogen and helium main sequence stars and He red giant stars that undergo Roche lobe overflow are unlikely to be the progenitors of subluminous SNe Ia. Earlier findings that overluminous SNe Ia (DELTA m{sub 15} (B) < 0.94) come from a young progenitor population are confirmed. The fact that subluminous SNe Ia and overluminous SNe Ia come from different progenitor populations and also have different properties is a prediction of the CO white dwarf merger progenitor scenario.

Howell, D. Andrew

2001-02-01T23:59:59.000Z

34

APS Beamline 6-ID-B,C  

NLE Websites -- All DOE Office Websites (Extended Search)

B,C Home B,C Home Recent Publications Beamline Info Optics Instrumentation Software User Info Beamline 6-ID-B,C Beamline 6-ID-B,C is operated by the Magnetic Materials Group in the X-ray Science Division (XSD) of the Advanced Photon Source. Research on this beamline centers on general x-ray scattering studies of materials. The beamline has 2 end-stations: 6-ID-B: Psi -Diffractomter & In-Field Studies 6-ID-C: UHV in-situ growth Recent Research Highlights LSMO pictures Searching for Next-Generation Electronic Materials December 14, 2009 A new class of layered oxide materials discovered thanks to research at the beamline 6-ID-B offers scientists unprecedented opportunities for creating the next generation of electronic devices. Local Contact: Phil Ryan Local Contacts: Philip Ryan (Surface Diffraction) 630.252.0252 ryan@aps.anl.gov

35

Rates and progenitors of type Ia supernovae  

SciTech Connect

The remarkable uniformity of Type Ia supernovae has allowed astronomers to use them as distance indicators to measure the properties and expansion history of the Universe. However, Type Ia supernovae exhibit intrinsic variation in both their spectra and observed brightness. The brightness variations have been approximately corrected by various methods, but there remain intrinsic variations that limit the statistical power of current and future observations of distant supernovae for cosmological purposes. There may be systematic effects in this residual variation that evolve with redshift and thus limit the cosmological power of SN Ia luminosity-distance experiments. To reduce these systematic uncertainties, we need a deeper understanding of the observed variations in Type Ia supernovae. Toward this end, the Nearby Supernova Factory has been designed to discover hundreds of Type Ia supernovae in a systematic and automated fashion and study them in detail. This project will observe these supernovae spectrophotometrically to provide the homogeneous high-quality data set necessary to improve the understanding and calibration of these vital cosmological yardsticks. From 1998 to 2003, in collaboration with the Near-Earth Asteroid Tracking group at the Jet Propulsion Laboratory, a systematic and automated searching program was conceived and executed using the computing facilities at Lawrence Berkeley National Laboratory and the National Energy Research Supercomputing Center. An automated search had never been attempted on this scale. A number of planned future large supernovae projects are predicated on the ability to find supernovae quickly, reliably, and efficiently in large datasets. A prototype run of the SNfactory search pipeline conducted from 2002 to 2003 discovered 83 SNe at a final rate of 12 SNe/month. A large, homogeneous search of this scale offers an excellent opportunity to measure the rate of Type Ia supernovae. This thesis presents a new method for analyzing the true sensitivity of a multi-epoch supernova search and finds a Type Ia supernova rate from z {approx} 0.01-0.1 of r{sub V} = 4.26{sub -1.93 -0.10}{sup +1.39 +0.10} h{sup 3} x 10{sup -4} SNe Ia/yr/Mpc{sup 3} from a preliminary analysis of a subsample of the SNfactory prototype search. Several unusual supernovae were found in the course of the SNfactory prototype search. One in particular, SN 2002ic, was the first SN Ia to exhibit convincing evidence for a circumstellar medium and offers valuable insight into the progenitors of Type Ia supernovae.

Wood-Vasey, William Michael

2004-08-16T23:59:59.000Z

36

State Laboratory Contacts IL  

Science Conference Proceedings (OSTI)

State Laboratory Contact Information IL. Idaho. ... State of Iowa Metrology Laboratory Ellsworth Community College 1100 College Ave. ...

2013-11-07T23:59:59.000Z

37

Rolling Hills (IA) | Open Energy Information  

Open Energy Info (EERE)

Rolling Hills (IA) Rolling Hills (IA) Jump to: navigation, search Name Rolling Hills (IA) Facility Rolling Hills (IA) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Company Developer MidAmerican Energy Company Energy Purchaser MidAmerican Energy Company Location Massena IA Coordinates 41.230443°, -94.75459° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.230443,"lon":-94.75459,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

38

Department of Energy Idaho - Inside DOE-ID  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-ID Mission and Vision Brief History of the Idaho National Laboratory (INL) Strategic Plan Idaho Operations Office (DOE-ID) - 888 KB DOE-ID Agreement in Principle...

39

Property:WFSPTurbineID | Open Energy Information  

Open Energy Info (EERE)

WFSPTurbineID WFSPTurbineID Jump to: navigation, search Property Name WFSPTurbineID Property Type Number This is a property of type Number. Pages using the property "WFSPTurbineID" Showing 25 pages using this property. (previous 25) (next 25) A Alleghany High School Wind Project + 110,608 + Appanoose Elementary School Wind Project + 108,442 + Auburn-Washburn Wind Project + 105,237 + Avery County High School Wind Project + 110,607 + B Bancroft-Rosalie Public Schools Wind Project + 108,812 + Bloomfield Public Schools Wind Project + 110,699 + Burlington High School Wind Project + 107,678 + C CAES Wind Project + 105,329 + Cedar Rapids Wind Project + 105,272 + Cherry Valley Elementary School Wind Project + 120,342 + Concordia High School Wind Project + 108,482 +

40

1-ID: Sector 1, Insertion Device Beamline  

NLE Websites -- All DOE Office Websites (Extended Search)

1-ID beamline schematic 1-ID beamline schematic ID on-axis brilliance values 1-ID - Sector 1, Insertion Device Beamline Responsible Scientists Jon Almer, phone: (630) 252-1049, e-mail: almer@aps.anl.gov Sarvjit Shastri, phone: (630) 252-0129, e-mail: shastri@aps.anl.gov John Okasinski, phone: (630) 252-0162, e-mail: okasinski@aps.anl.gov Peter Kenesei, phone: (630) 252-0133, e-mail: kenesei@aps.anl.gov Scientific Programs Coupled high-energy SAXS/WAXS studies (HE-SAXS/WAXS) High-energy diffraction microscopy (HEDM) Single-grain studies Stress/strain/texture studies Pair-distribution function (PDF) measurements High-energy fluorescence Source Characteristics Upstream insertion device: APS Undulator A No. of Poles 72 Undulator Period 3.3 cm Device Length 2.4 m Minimum Gap 11 mm Downstream insertion device

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

IPS: IDS or IPS: what is best?  

Science Conference Proceedings (OSTI)

Intrusion detection systems (IDS) have become one of the most common countermeasures in the network security arsenal. But while other technologies such as firewalls and anti-virus provide proactive protection, most current IDSs are passive; detection ...

Maria Papadaki; Steven Furnell

2004-07-01T23:59:59.000Z

42

On the Brightness of Supernova Ia  

E-Print Network (OSTI)

Before 1998 the universe expansion was thought to be slowing down. After 1998 the universe expansion is thought to be accelerating up. The key evidence came from the observed brightness of high redshift supernovae Ia in 1998. Astronomers found that the observed brightness of high redshift supernovae Ia is fainter than expected. Astronomers believe this means that the universe expansion is accelerating up. In this paper it is argued that if the ionized gas in the universe space is taken into account, then the brightness of the high redshift supernova Ia should be fainter than expected. The universe expansion does not need to be accelerating up. The exotic form of energy (dark energy) does not need to be introduce

Yijia Zheng

2013-10-01T23:59:59.000Z

43

Spectral diversity of Type Ia Supernovae  

E-Print Network (OSTI)

We use published spectroscopic and photometric data for 8 Type Ia supernovae to construct a dispersion spectrum for this class of object, showing their diversity over the wavelength range 3700A to 7100A. We find that the B and V bands are the spectral regions with the least dispersion, while the U band below 4100A is more diverse. Some spectral features such as the Si line at 6150A are also highly diverse. We then construct two objective measures of 'peculiarity' by (i) using the deviation of individual objects from the average SN Ia spectrum compared to the typical dispersion and (ii) applying principle component analysis. We demonstrate these methods on several SNe Ia that have previously been classified as peculiar.

J. Berian James; Tamara M. Davis; Brian P. Schmidt; Alex G. Kim

2006-05-05T23:59:59.000Z

44

EIA-802  

U.S. Energy Information Administration (EIA)

Product Code (202) 586-1076 OR ... Hawaii IA Iowa ID Idaho IL ... Quantities entered below should be the weekly equivalent of those reported monthly to the Energy ...

45

Annual Planning Summaries: Idaho Operations Office (ID) | Department...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Marketing Administration Other Agencies You are here Home Annual Planning Summaries: Idaho Operations Office (ID) Annual Planning Summaries: Idaho Operations Office (ID)...

46

Id-1 and Id-2 genes and products as markers of epithelial cancer  

DOE Patents (OSTI)

A method for detection and prognosis of breast cancer and other types of cancer. The method comprises detecting expression, if any, for both an Id-1 and an Id-2 genes, or the ratio thereof, of gene products in samples of breast tissue obtained from a patient. When expressed, Id-1 gene is a prognostic indicator that breast cancer cells are invasive and metastatic, whereas Id-2 gene is a prognostic indicator that breast cancer cells are localized and noninvasive in the breast tissue.

Desprez, Pierre-Yves (El Cerrito, CA); Campisi, Judith (Berkeley, CA)

2008-09-30T23:59:59.000Z

47

Visualizing Buoyant Burning Bubbles in Type Ia Supernovae at...  

NLE Websites -- All DOE Office Websites (Extended Search)

Burning in Supernovae Buoyant Burning Bubbles in Type Ia Supernovae bubble-s.jpeg Flame ignition in type Ia supernovae leads to isolated bubbles of burning buoyant fluid. As a...

48

Location-based security for ID document and ID card enrollment stations  

Science Conference Proceedings (OSTI)

Much of today's security for financial assets, services, facilities, personal information, immigration, employment and travel is provided in the form of a variety of ID instruments such as passports, credit cards, ID badges, access cards, and other similar ... Keywords: RFID, identity management systems, identity verification, location-based security, physical unclonable functions

Eugene P. Gerety; Khaled M. Elleithy

2011-04-01T23:59:59.000Z

49

APS Beamline 6-ID-D  

NLE Websites -- All DOE Office Websites (Extended Search)

D Home D Home Recent Publications Beamline Info Optics Instrumentation Software User Info Beamline 6-ID-D Beamline 6-ID-D is operated by the Magnetic Materials Group in the X-ray Science Division (XSD) of the Advanced Photon Source. This is a high energy (50 - 130 keV) beamline used for structural studies primarily on single crystal materials. Recent Research Highlights A New Family of Quasicrystals A New Family of Quasicrystals June 24, 2013 Scientists from the U.S. Department of Energy's Ames Laboratory and Iowa State University have used the high energy x-rays available on beamline 6-ID-D, to confirm the structure of the only known magnetic rare earth icosahedral binary quasicrystals. Contacts: Alan Goldman & Paul Canfield - Iowa State Univ. & Ames Lab Local Contacts:

50

Requesting a Digital ID | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Requesting a Digital ID Requesting a Digital ID Requesting a Digital ID Step One - Registering with MIS To request a DOE Digital Identity you must first register in DOE's Management Information System (MIS) by going to https://mis.doe.gov, selecting "Requesting Access" and following the onscreen instructions. Note: DOE Federal employees are already registered and do not need to complete this step, they may skip to step 2. During the registration process you will be required to search for, and select, a DOE sponsor. Your DOE sponsor is the DOE federal employee that is certifying that you have a recognized relationship with the Department and have a valid need for a DOE Digital Identity. For contractors this person is often your Contract Task Manager, Contracting Officer's Representatives

51

LINKING TYPE Ia SUPERNOVA PROGENITORS AND THEIR RESULTING EXPLOSIONS  

Science Conference Proceedings (OSTI)

Comparing the ejecta velocities at maximum brightness and narrow circumstellar/interstellar Na D absorption line profiles of a sample of 23 Type Ia supernovae (SNe Ia), we determine that the properties of SN Ia progenitor systems and explosions are intimately connected. As demonstrated by Sternberg et al., half of all SNe Ia with detectable Na D absorption at the host-galaxy redshift in high-resolution spectroscopy have Na D line profiles with significant blueshifted absorption relative to the strongest absorption component, which indicates that a large fraction of SN Ia progenitor systems have strong outflows. In this study, we find that SNe Ia with blueshifted circumstellar/interstellar absorption systematically have higher ejecta velocities and redder colors at maximum brightness relative to the rest of the SN Ia population. This result is robust at a 98.9%-99.8% confidence level, providing the first link between the progenitor systems and properties of the explosion. This finding is further evidence that the outflow scenario is the correct interpretation of the blueshifted Na D absorption, adding additional confirmation that some SNe Ia are produced from a single-degenerate progenitor channel. An additional implication is that either SN Ia progenitor systems have highly asymmetric outflows that are also aligned with the SN explosion or SNe Ia come from a variety of progenitor systems where SNe Ia from systems with strong outflows tend to have more kinetic energy per unit mass than those from systems with weak or no outflows.

Foley, Ryan J.; Kirshner, Robert P. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Simon, Joshua D.; Burns, Christopher R. [Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Hamuy, Mario [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Morrell, Nidia I.; Phillips, Mark M. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Shields, Gregory A. [Department of Astronomy, University of Texas, Austin, TX 78712 (United States); Sternberg, Assaf, E-mail: rfoley@cfa.harvard.edu [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching (Germany)

2012-06-20T23:59:59.000Z

52

National ID project of Nepal: future challenges  

Science Conference Proceedings (OSTI)

Nepal is a small, landlocked and developing country in South Asia. It is bordered by China at North and India at South, East and West. The Government of Nepal, in order to achieve good governance and social-economic development, has initiated the e-Government ... Keywords: Nepal, challenges, government, national ID

Ganesh Prasad Adhikari

2011-09-01T23:59:59.000Z

53

Category:Des Moines, IA | Open Energy Information  

Open Energy Info (EERE)

IA IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Des Moines, IA" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVFullServiceRestauran... 64 KB SVQuickServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVQuickServiceRestaura... 64 KB SVHospital Des Moines IA MidAmerican Energy Co (Iowa).png SVHospital Des Moines ... 73 KB SVLargeHotel Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeHotel Des Moine... 72 KB SVLargeOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeOffice Des Moin... 73 KB SVMediumOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVMediumOffice Des Moi... 69 KB SVMidriseApartment Des Moines IA MidAmerican Energy Co (Iowa).png

54

Property:DSIRE/Id | Open Energy Information  

Open Energy Info (EERE)

Property Property Edit with form History Facebook icon Twitter icon » Property:DSIRE/Id Jump to: navigation, search This is a property of type String. DSIRE Incentive Code. Pages using the property "DSIRE/Id" Showing 25 pages using this property. (previous 25) (next 25) 2 2003 Climate Change Fuel Cell Buy-Down Program (Federal) + US04F + 3 30% Business Tax Credit for Solar (Vermont) + VT31F + A AEP (Central and North) - CitySmart Program (Texas) + TX141F + AEP (Central and North) - Residential Energy Efficiency Programs (Texas) + TX116F + AEP (Central and SWEPCO) - Coolsaver A/C Tune Up (Texas) + TX119F + AEP (Central, North and SWEPCO) - Commercial Solutions Program (Texas) + TX141F + AEP (SWEPCO) - Residential Energy Efficiency Programs (Texas) + TX138F +

55

Property:GBIG/GreenButtonID | Open Energy Information  

Open Energy Info (EERE)

GreenButtonID Jump to: navigation, search This is a property of type String. Retrieved from "http:en.openei.orgwindex.php?titleProperty:GBIGGreenButtonID&oldid509348" What...

56

Microsoft Word - DOE-ID-INL-11-005.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

protective equipment (PPE) where practical. DOE-ID NEPA CX DETERMINATION IDAHO NATIONAL LABORATORY Page 2 of 2 CX Posting No.: DOE-ID-INL-11-005 Releasing Contaminants - Diesel...

57

Microsoft Word - DOE-ID-INL-12-015.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

direction of Waste Generator Services (WGS). DOE-ID NEPA CX DETERMINATION IDAHO NATIONAL LABORATORY Page 2 of 2 CX Posting No.: DOE-ID-INL-12-015 Releasing Contaminants - The...

58

Microsoft Word - DOE-ID-INL-13-028.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

and therefore, waste associated DOE-ID-NEPA CX DETERMINATION Idaho National Laboratory Page 2 of 2 CX Posting No.: DOE-ID-INL-13-028 with project activities is...

59

Guided Summarization Results GOOGLE Google Inc Run ID ...  

Science Conference Proceedings (OSTI)

Page 1. Guided Summarization Results GOOGLE Google Inc Run ID: GOOGLE1 Overall Responsiveness 1.000 Overall ...

2012-02-27T23:59:59.000Z

60

Microsoft Word - DOE-ID-INL-13-025.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

2 of 4 EC Document No.: DOE-ID-INL-13-025 DOE-ID-NEPA CX DETERMINATION Idaho National Laboratory Page 3 of 4 EC Document No.: DOE-ID-INL-13-025 All conduit located on the...

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

DOE - Office of Legacy Management -- Titus Metals - IA 04  

Office of Legacy Management (LM)

from consideration under FUSRAP Also see Documents Related to TITUS METALS IA.04-1 - Argonne National Laboratory Memorandum; Lonergan to Novak; Subject: Extrusion of Billets,...

62

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

Turbulence-Flame Interactions in Type Ia Supernovae A. J.Normalised time (e) Normalised flame speed Normalised time (length scale (cm) Laminar flame width Gibson scale Cell

Aspden, Andrew J; Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (Authors 1, 2 & 3); Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (Author 4); Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (Author 5)

2008-01-01T23:59:59.000Z

63

DOE - Office of Legacy Management -- Bendix Aviation Corp Pioneer Div - IA  

Office of Legacy Management (LM)

Bendix Aviation Corp Pioneer Div - Bendix Aviation Corp Pioneer Div - IA 05 FUSRAP Considered Sites Site: BENDIX AVIATION CORP., PIONEER DIV. (IA.05 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Pioneer Division, Bendix Aviation Corporation Bendix Aviation Corporation Bendix Pioneer Division IA.05-1 IA.05-2 IA.05-3 Location: Davenport , Iowa IA.05-1 Evaluation Year: 1990 IA.05-2 IA.05-4 Site Operations: Conducted studies to investigate the feasibility of using sonic cleaning equipment to decontaminate uranium contaminated drums. IA.05-1 Site Disposition: Eliminated - Potential for contamination considered remote based on limited operations at the site IA.05-2 IA.05-4 IA.05-5 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IA.05-1

64

Conformal cosmological model and SNe Ia data  

SciTech Connect

Now there is a huge scientific activity in astrophysical studies and cosmological ones in particular. Cosmology transforms from a pure theoretical branch of science into an observational one. All the cosmological models have to pass observational tests. The supernovae type Ia (SNe Ia) test is among the most important ones. If one applies the test to determine parameters of the standard Friedmann-Robertson-Walker cosmological model one can conclude that observations lead to the discovery of the dominance of the {Lambda} term and as a result to an acceleration of the Universe. However, there are big mysteries connected with an origin and an essence of dark matter (DM) and the {Lambda} term or dark energy (DE). Alternative theories of gravitation are treated as a possible solution of DM and DE puzzles. The conformal cosmological approach is one of possible alternatives to the standard {Lambda}CDM model. As it was noted several years ago, in the framework of the conformal cosmological approach an introduction of a rigid matter can explain observational data without {Lambda} term (or dark energy). We confirm the claim with much larger set of observational data.

Zakharov, A. F., E-mail: zakharov@itep.ru [National Astronomical Observatories of Chinese Academy of Sciences (China); Pervushin, V. N. [Joint Institute for Nuclear Research, Bogoliubov Laboratory for Theoretical Physics (Russian Federation)

2012-11-15T23:59:59.000Z

65

The Distant Type Ia Supernova Rate  

DOE R&D Accomplishments (OSTI)

We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample, which surveyed about 12 square degrees, thirty-eight supernovae were detected at redshifts 0.25--0.85. In a spatially flat cosmological model consistent with the results obtained by the Supernova Cosmology Project, we derive a rest-frame Type Ia supernova rate at a mean red shift z {approx_equal} 0.55 of 1.53 {sub -0.25}{sub -0.31}{sup 0.28}{sup 0.32} x 10{sup -4} h{sup 3} Mpc{sup -3} yr{sup -1} or 0.58{sub -0.09}{sub -0.09}{sup +0.10}{sup +0.10} h{sup 2} SNu(1 SNu = 1 supernova per century per 10{sup 10} L{sub B}sun), where the first uncertainty is statistical and the second includes systematic effects. The dependence of the rate on the assumed cosmological parameters is studied and the redshift dependence of the rate per unit comoving volume is contrasted with local estimates in the context of possible cosmic star formation histories and progenitor models.

Pain, R.; Fabbro, S.; Sullivan, M.; Ellis, R. S.; Aldering, G.; Astier, P.; Deustua, S. E.; Fruchter, A. S.; Goldhaber, G.; Goobar, A.; Groom, D. E.; Hardin, D.; Hook, I. M.; Howell, D. A.; Irwin, M. J.; Kim, A. G.; Kim, M. Y.; Knop, R. A.; Lee, J. C.; Perlmutter, S.; Ruiz-Lapuente, P.; Schahmaneche, K.; Schaefer, B.; Walton, N. A.

2002-05-28T23:59:59.000Z

66

Entity Name: ABC Company Entity ID:  

Gasoline and Diesel Fuel Update (EIA)

Entity Name: Entity Name: ABC Company Entity ID: 00000 Data Year: 2013 State Include or exclude pre-arranged interruptions? 1 2 3 Do you capture outage records for events that initiate outside your system (customer system that causes di 4 5 6 7 8 Point to calculation in P1782: use percentages weighted based upon the classification of the circuit. 9 10 11 12 REWORD: The percent of customers automatically reported when they have lost power? e.g. SCADA, AMI, Etc. 13 SAIDI value (w/o Major Events included) FORM EIA-861 OMB No. 1905-0129 ANNUAL ELECTRIC POWER INDUSTRY REPORT

67

u.s. DEPARTlIlENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERlIlINATION  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

lincoln lincoln u.s. DEPARTlIlENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERlIlINATION Pagc 1 of3 STATE: NE PROJECT TITLE: EECBG DE- EE 0000664 City of Lincoln Statement of Work Template (S) {Activities 1, 2, 3 , 4, 5 , 6 , 7 , 8, 10 & 14 on SOW; Add'i CX for 9,13,15,16,17] Funding Opportunity Announ<:ement Number PrCKurement Instrument Number NEPA Control Number cm Number DE-FOA-OOOOO13 DE-EEOOOO664 0 Based OD my review of the information con<:erning the proposed a<:tion, as NEPA Complian<:e Offi<:er (authorized under DOE Order 451.IA), I have made the following determination: CX, EA, EIS APPENDIX AND NUMBER: Description: A9 Information gathering (including, but not limited 10, literature surveys, inventories, audits), data analysis (including

68

Burning Thermals in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

Burning Thermals in Type Ia Supernovae A. J. Aspden1 , J. B. Bell1 , S. Dong2 , and S. E. Woosley2 ABSTRACT We develop a one-dimensional theoretical model for thermals burning in Type Ia supernovae based for the burning and for the expansion of the thermal due to changes in the background stratification found

Bell, John B.

69

Visualizing Type Ia Supernova Explosions at NERSC  

NLE Websites -- All DOE Office Websites (Extended Search)

Supernova Explosions Supernova Explosions Visualizing Type Ia Supernova Explosions Childs1a-Supernovasm.png Deep inside a dying star in a galaxy far, far away, a carbon fusion flame ignites. Ignition may happen in the middle or displaced slightly to one side, but this simulation explores the consequences of central ignition. In a localized hot spot, represented here by a deformed sphere with an average radius of 100 km, carbon is assumed to have already fused to iron, producing hot ash (~10 billion K) with a density about 20% less than its surroundings. As the burning progresses, this hot buoyant ash rises up and interacts with cold fuel. Rayleigh-Taylor fingers give rise to shear and turbulence, which interacts with the flame, causing it to move faster. In about 2 seconds, the energy released blows the entire white dwarf star up,

70

Facility Representative Program ID Selects FR of the Year  

NLE Websites -- All DOE Office Websites (Extended Search)

Facility Representative Program ID Selects Facility Representative Program ID Selects FR of the Year John Martin DOE-ID Facility Representative John Martin DOE-ID Facility Representative of the Year. John Martin was selected as DOE-ID's Facility Representative of the Year and the office's nominee for the 2007 DOE Facility Representative of the Year Award. John was selected from an exceptional field of candidates to represent DOE-ID at the Facility Representative Annual Workshop in Las Vegas this May. Each year the Department of Energy recognizes the Facility Representative whose achievements during the calendar year are most exemplary. A panel of senior personnel representing the Office of Health, Safety and Security (HSS) National Nuclear Security Administration (NNSA), Environmental Management (EM), Science (SC), Nuclear Energy (NE) and at least five

71

Microsoft Word - DOE-ID-INL-12-015.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

15 15 SECTION A. Project Title: Materials and Fuels Complex Underground and Aboveground Storage Tank Replacement SECTION B. Project Description: The purpose of this project is to permanently close and remove the Materials and Fuels Complex (MFC) 4,000 gallon bio-diesel underground storage tank (UST) [Site ID# 7230/Facility ID # 6-120614/Tank ID # 99ANL00013] and remove the 1,000 gallon E-85 aboveground storage tank (AST) [Site ID# 7230/Facility ID# 6-120614/Tank ID# 05MFC00035] and replace the two tanks with a 10,000 gallon aboveground storage tank (AST) split tank (5,000 gallons for bio-diesel/5,000 gallons for E-85). The 4,000 gallon bio-diesel UST and the 1,000 gallon E-85 AST are located in the parking lot area near building MFC-701.

72

Beamline 6-ID-D Publications  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 2011 2010 2009 2008 All Sector 6 Pubs. APS Pubs. Database Recent 6-ID-D Publications Publications 2013:(24) "Controlling Size-Induced Phase Transformations Using Chemically Designed Nanolaminates," Matt Beekman, Sabrina Disch, Sergei Rouvimov, Deepa Kasinathan, Klaus Koepernik, Helge Rosner, Paul Zschack, Wolfgang S. Neumann, David C. Johnson, Angew. Chem. Int. Ed. 52, 13211 (2013). "Thermophysical and Structural Measurements of Liquid Metallic Alloys Using Electrostatic Levitation," James Christopher Bendert, Ph.D.-Thesis, Washington University , 2013. "Pair distribution function analysis of X-ray diffraction from amorphous spheres in an asymmetric transmission geometry: application to a Zr58.5Cu15.6Ni12.8Al10.3Nb2.8 glass," J.C. Bendert, N.A. Mauro, K.F. Kelton, J. Appl. Crystallogr. 46, 999

73

Mo Year Report Period: EIA ID NUMBER:  

U.S. Energy Information Administration (EIA) Indexed Site

Version No: 2013.01 Mo Year Report Period: EIA ID NUMBER: http://www.eia.gov/survey/form/eia_14/instructions.pdf Mailing Address: Secure File Transfer option available at: (e.g., PO Box, RR) https://signon.eia.doe.gov/upload/noticeoog.jsp Electronic Transmission: The PC Electronic Zip Code - Data Reporting Option (PEDRO) is available. If interested in software, call (202) 586-9659. Email form to: OOG.SURVEYS@eia.doe.gov - - - - Fax form to: (202) 586-9772 Mail form to: Oil & Gas Survey Email address: U.S. Department of Energy Ben Franklin Station PO Box 279 Washington, DC 20044-0279 Questions? Call toll free: 1-800-638-8812 PADD 4 Type of Report (Check One ): (Thousands of dollars) (Thousands of barrels) PADD 2 PADD 3 PAD DISTRICT (a) Revision to Report:

74

Beamline 4-ID-D Publications  

NLE Websites -- All DOE Office Websites (Extended Search)

2012 2012 2011 2010 2009 2008 All Sector 4 Pubs. APS Pubs. Database Recent 4-ID-D Publications Publications 2013:(13) "Classical and quantum phase transitions revealed using transport and x-ray measurements," Arnab Banerjee, Ph.D.-Thesis, University of Chicago, 2013. "Charge transfer and multiple density waves in the rare earth tellurides," A. Banerjee, Yejun Feng, D.M. Silevitch, Jiyang Wang, J.C. Lang, H.-H. Kuo, I.R. Fisher, T.F. Rosenbaum, Phys. Rev. B 87, 155131 (2013). "Local structure, stripe pinning, and superconductivity in La1.875Ba0.125CuO4 at high pressure," G. Fabbris, M. Hücker, G.D. Gu, J.M. Tranquada, D. Haskel, Phys. Rev. B 88, 060507(R) (2013). "Different routes to pressure-induced volume collapse transitions in

75

SLAC Dosimeter / ID Request Form A  

NLE Websites -- All DOE Office Websites (Extended Search)

Feb 2009 (updated 13 May 2010) SLAC-I-760-0A07J-006-R010 1 of 2 Feb 2009 (updated 13 May 2010) SLAC-I-760-0A07J-006-R010 1 of 2 SLAC Dosimeter / ID Request Form A (For applicants who have completed SLAC Environment, Safety, and Health Training) Sections 1-5 completed by applicant. Section 1: Contact Information Last name: First name: MI: Male Female Birth year (yyyy): Job title: Contact information/mailing address: City: State: Zip code: Country: Dept/Group: Phone number: Mail stop: Users or non-SLAC employees only: List employer, company, or university : Section 2: Identification Badge Request I am applying for my first SLAC identification badge; I have successfully completed the following ES&H training (indicate all that apply): SON SOC EOESH GERT RWT I RWT II

76

DOE - Office of Legacy Management -- Iowa Army Ammunition Plant - IA 02  

Office of Legacy Management (LM)

Army Ammunition Plant - IA 02 Army Ammunition Plant - IA 02 FUSRAP Considered Sites Iowa Army Ammunition Plant, IA Alternate Name(s): Burlington Ordnance Plant Iowa Ordnance Plant Silas Mason Company IA.02-3 Location: Located in Township 70 North, Range 3 West, Section 32, 5th Principal Meridian, Des Moines County, Burlington, Iowa IA.02-1 IA.02-5 Historical Operations: Assembled nuclear weapons, primarily high explosive components and conducted explosives testing using the high explosive components and depleted uranium. AEC and ERDA operations conducted under permit from the Department of the Army. IA.02-3 IA.02-4 Eligibility Determination: Eligible IA.02-5 Radiological Survey(s): Assessment Survey IA.02-2 Site Status: Cleanup pending by U.S. Army Corps of Engineers. IA.02-6

77

Mobile ID Device Best Practice Recommendation Version 1.0  

Science Conference Proceedings (OSTI)

Page 1. Mobile ID Device Best Practice Recommendation Version 1.0 Shahram Orandi R. Michael McCabe Information Access Division ...

2012-03-11T23:59:59.000Z

78

,"Eastport, ID Natural Gas Pipeline Imports From Canada (MMcf...  

U.S. Energy Information Administration (EIA) Indexed Site

Of Series","Frequency","Latest Data for" ,"Data 1","Eastport, ID Natural Gas Pipeline Imports From Canada (MMcf)",1,"Annual",2012 ,"Release Date:","172014" ,"Next...

79

Late Light Curves of Normally-Luminous Type Ia Supernovae  

E-Print Network (OSTI)

The use of Type Ia supernovae as cosmological tools has reinforced the need to better understand these objects and their light curves. The light curves of Type Ia supernovae are powered by the nuclear decay of $^{56}Ni \\to ^{56}Co \\to ^{56}Fe$. The late time light curves can provide insight into the behavior of the decay products and their effect of the shape of the curves. We present the optical light curves of six "normal" Type Ia supernovae, obtained at late times with template image subtraction, and the fits of these light curves to supernova energy deposition models.

J. C. Lair; M. D. Leising; P. A. Milne; G. G. Williams

2006-01-05T23:59:59.000Z

80

UMore Ph IA CR Report 7-8-10.pdf  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

PHASE IA ARCHAEOLOGICAL AND PHASE IA ARCHAEOLOGICAL AND ARCHITECTURAL HISTORY SURVEY FOR THE UMORE PARK RESEARCH WIND TURBINE PROJECT, DAKOTA COUNTY, MINNESOTA SHPO File No. Pending Client No. Pending The 106 Group Project No. 10-18 Submitted to: Barr Engineering Company 4700 West 77th Street Minneapolis, MN 55435-4803 Submitted by: The 106 Group Ltd. The Dacotah Building 370 Selby Avenue St. Paul, MN 55102 Principal Investigators: AnneKetz, M.A., RPA Greg Mathis, M.C.R.P. Report Authors: Mark Doperalski, B.S. Miranda Van Vleet, M.H.P July 2010 UMore Park Wind Turbine Project Phase IA Archaeological and Architectural History Survey Page i MANAGEMENT SUMMARY During May of 2010, The 106 Group Ltd. (106 Group) conducted a Phase IA archaeological and architectural history survey for the University of Minnesota Outreach, Research, and

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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81

TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM  

SciTech Connect

Owing to their utility for measurements of cosmic acceleration, Type Ia supernovae (SNe Ia) are perhaps the best-studied class of SNe, yet the progenitor systems of these explosions largely remain a mystery. A rare subclass of SNe Ia shows evidence of strong interaction with their circumstellar medium (CSM), and in particular, a hydrogen-rich CSM; we refer to them as SNe Ia-CSM. In the first systematic search for such systems, we have identified 16 SNe Ia-CSM, and here we present new spectra of 13 of them. Six SNe Ia-CSM have been well studied previously, three were previously known but are analyzed in depth for the first time here, and seven are new discoveries from the Palomar Transient Factory. The spectra of all SNe Ia-CSM are dominated by H{alpha} emission (with widths of {approx}2000 km s{sup -1}) and exhibit large H{alpha}/H{beta} intensity ratios (perhaps due to collisional excitation of hydrogen via the SN ejecta overtaking slower-moving CSM shells); moreover, they have an almost complete lack of He I emission. They also show possible evidence of dust formation through a decrease in the red wing of H{alpha} 75-100 days past maximum brightness, and nearly all SNe Ia-CSM exhibit strong Na I D absorption from the host galaxy. The absolute magnitudes (uncorrected for host-galaxy extinction) of SNe Ia-CSM are found to be -21.3 mag {<=} M{sub R} {<=} -19 mag, and they also seem to show ultraviolet emission at early times and strong infrared emission at late times (but no detected radio or X-ray emission). Finally, the host galaxies of SNe Ia-CSM are all late-type spirals similar to the Milky Way, or dwarf irregulars like the Large Magellanic Cloud, which implies that these objects come from a relatively young stellar population. This work represents the most detailed analysis of the SN Ia-CSM class to date.

Silverman, Jeffrey M. [Department of Astronomy, University of Texas, Austin, TX 78712-0259 (United States); Nugent, Peter E. [Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States); Gal-Yam, Avishay; Arcavi, Iair; Ben-Ami, Sagi [Benoziyo Center for Astrophysics, Weizmann Institute of Science, Rehovot 76100 (Israel); Sullivan, Mark [School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom); Howell, D. Andrew; Graham, Melissa L. [Las Cumbres Observatory Global Telescope Network, Goleta, CA 93117 (United States); Filippenko, Alexei V.; Bloom, Joshua S.; Cenko, S. Bradley; Clubb, Kelsey I. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Cao, Yi; Horesh, Assaf; Kulkarni, Shrinivas R. [Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Chornock, Ryan; Foley, Ryan J. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Coil, Alison L. [Department of Physics, University of California, San Diego, La Jolla, CA 92093 (United States); Griffith, Christopher V. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Kasliwal, Mansi M., E-mail: jsilverman@astro.as.utexas.edu [Observatories of the Carnegie Institution of Science, Pasadena, CA 91101 (United States); and others

2013-07-01T23:59:59.000Z

82

A database of anomalous traffic for assessing profile based IDS  

Science Conference Proceedings (OSTI)

This paper aims at proposing a methodology for evaluating current IDS capabilities of detecting attacks targeting the networks and their services. This methodology tries to be as realistic as possible and reproducible, i.e. it works with real attacks ... Keywords: KDD'99, ROC curves, attack traces, statistical evaluation of IDS

Philippe Owezarski

2010-04-01T23:59:59.000Z

83

VELOCITY EVOLUTION AND THE INTRINSIC COLOR OF TYPE Ia SUPERNOVAE  

SciTech Connect

To understand how best to use observations of Type Ia supernovae (SNe Ia) to obtain precise and accurate distances, we investigate the relations between spectra of SNe Ia and their intrinsic colors. Using a sample of 1630 optical spectra of 255 SNe, based primarily on data from the CfA Supernova Program, we examine how the velocity evolution and line strengths of Si II {lambda}6355 and Ca II H and K are related to the B - V color at peak brightness. We find that the maximum-light velocity of Si II {lambda}6355 and Ca II H and K and the maximum-light pseudo-equivalent width of Si II {lambda}6355 are correlated with intrinsic color, with intrinsic color having a linear relation with the Si II {lambda}6355 measurements. Ca II H and K does not have a linear relation with intrinsic color, but lower-velocity SNe tend to be intrinsically bluer. Combining the spectroscopic measurements does not improve intrinsic color inference. The intrinsic color scatter is larger for higher-velocity SNe Ia-even after removing a linear trend with velocity-indicating that lower-velocity SNe Ia are more 'standard crayons'. Employing information derived from SN Ia spectra has the potential to improve the measurements of extragalactic distances and the cosmological properties inferred from them.

Foley, Ryan J.; Sanders, Nathan E.; Kirshner, Robert P., E-mail: rfoley@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2011-12-01T23:59:59.000Z

84

The Rate of Type Ia Supernovae at High Redshift  

E-Print Network (OSTI)

We derive the rates of Type Ia supernovae (SNIa) over a wide range of redshifts using a complete sample from the IfA Deep Survey. This sample of more than 100 SNIa is the largest set ever collected from a single survey, and therefore uniquely powerful for a detailed supernova rate (SNR) calculation. Measurements of the SNR as a function of cosmological time offer a glimpse into the relationship between the star formation rate (SFR) and Type Ia SNR, and may provide evidence for the progenitor pathway. We observe a progressively increasing Type Ia SNR between redshifts z~0.3-0.8. The Type Ia SNR measurements are consistent with a short time delay (t~1 Gyr) with respect to the SFR, indicating a fairly prompt evolution of SNIa progenitor systems. We derive a best-fit value of SFR/SNR 580 h_70^(-2) M_solar/SNIa for the conversion factor between star formation and SNIa rates, as determined for a delay time of t~1 Gyr between the SFR and the Type Ia SNR. More complete measurements of the Type Ia SNR at z>1 are necessary to conclusively determine the SFR--SNR relationship and constrain SNIa evolutionary pathways.

Brian J. Barris; John L. Tonry

2005-09-22T23:59:59.000Z

85

The diversity of Type Ia Supernovae: evidence for systematics?  

E-Print Network (OSTI)

The photometric and spectroscopic properties of 26 well observed Type Ia Supernovae (SNeIa) were analyzed with the aim to explore SNIa diversity. The sample includes (Branch-)normal SNe as well as extreme events like SNe 1991T and 1991bg, while the truly peculiar SNIa, SN2000cx and SN2002cx are not included in our sample . A statistical treatment reveals the existence of three different groups. The first group (FAINT) consists of faint SNeIa similar to SN1991bg, with low expansion velocities and rapid evolution of SiII velocity. A second group consists of ``normal'' SNeIa, also with high temporal velocity gradient (HVG), but with brighter mean absolute magnitude =-19.3 and higher expansion velocities than the FAINT SNe. The third group includes both ``normal'' and SN1991T-like SNeIa: these SNe populate a narrow strip in the SiII velocity evolution plot, with a small velocity gradient (SVG), but have absolute magnitudes similar to HVGs. While the FAINT and HVG SNeIa together seem to define a relation between RSi(II) and Dm15(B), the SVG ones either do not conform with that relation or define a new, looser one. The RSi(II) pre-maximum evolution of HVGs is strikingly different from that of SVGs. The impact of this evidence on the understanding of SNIa diversity, in terms of explosion mechanisms, degree of ejecta mixing, and ejecta-CSM interaction, is discussed.

S. Benetti; E. Cappellaro; P. A. Mazzali; M. Turatto; G. Altavilla; F. Bufano; N. Elias-Rosa; R. Kotak; G. Pignata; M. Salvo; V. Stanishev

2004-11-02T23:59:59.000Z

86

IDS Climate Change and Development Centre Resources | Open Energy  

Open Energy Info (EERE)

IDS Climate Change and Development Centre Resources IDS Climate Change and Development Centre Resources Jump to: navigation, search Tool Summary Name: IDS Climate Change and Development Centre Resources Agency/Company /Organization: Institute of Development Studies Sector: Energy, Land Topics: Policies/deployment programs Resource Type: Workshop, Publications, Training materials, Lessons learned/best practices References: Institute of Development Studies CCDC[1] Logo: IDS Climate Change and Development Centre Resources CCDC promotes "collaborative research and policy analysis, delivering high quality research programmes, knowledge services, teaching and training." References ↑ "Institute of Development Studies CCDC" Retrieved from "http://en.openei.org/w/index.php?title=IDS_Climate_Change_and_Development_Centre_Resources&oldid=375095"

87

Il Vopiscus di Lucio Afranio.  

E-Print Network (OSTI)

??In un quadro bibliografico molto ridotto, il presente lavoro si prefigge di ricercare un metodo per proporre un testo, una traduzione e un commento esegetico, (more)

BEDINI, FILIPPO

2011-01-01T23:59:59.000Z

88

IL Wted States Government  

Office of Legacy Management (LM)

Tis&: p/WI-3 Tis&: p/WI-3 . IL Wted States Government ' 1, -1. \ k. 4 4L La. -iF 1 I ' __, 7, Department of Energy memorandum

89

u.s. DEPARTlIlENT OF ENERGY EERE PROJECT M ANAGE MENT CEN T  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DEPARTlIlENT OF ENERGY DEPARTlIlENT OF ENERGY EERE PROJECT M ANAGE MENT CEN T ER NEPA DETERlIlINATION Page 1 of2 STATE: NC PROJECT TITLE : Charlotte Activity 3 * 1-485 Park & Ride Energy Efficiency Lighting Pilot ARRA-EECBG Strategy-Only Funding Opportunity Announcement Number DE·FOA-OOOOO13 Pr()(urement Instrument Number DE-EEOOO0765.001 NEPA Control Number elO Number o BaRd on my re",iew of the information concerning the proposed action, as NEPA Compliance Officer (authoriud under DOE Order 451.IA), I have made the following ddumination: ex, EA, EIS APPENDIX AN» NUMBER: Description: 82.5 Safety and environmental improvements of a facility , including replacement and upgrade of facility components, that do not result in a significant change in the expected useful life, design capacity, or function of the facility and during which

90

DISTRIBUTED FLAMES IN TYPE Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

At a density near a few x10{sup 7} g cm{sup -3}, the subsonic burning in a Type Ia supernova (SN) enters the distributed regime (high Karlovitz number). In this regime, turbulence disrupts the internal structure of the flame, and so the idea of laminar burning propagated by conduction is no longer valid. The nature of the burning in this distributed regime depends on the turbulent Damkoehler number (Da{sub T}), which steadily declines from much greater than one to less than one as the density decreases to a few x10{sup 6} g cm{sup -3}. Classical scaling arguments predict that the turbulent flame speed s{sub T} , normalized by the turbulent intensity u-check, follows s{sub T}/u-check = Da{sub T}{sup 1/2} for Da{sub T} {approx}burns as a turbulently broadened effective unity Lewis number flame. This flame burns locally with speed s{sub l}ambda and width l{sub l}ambda, and we refer to this kind of flame as a lambda-flame. The burning becomes a collection of lambda-flames spread over a region approximately the size of the {integral} scale. While the total burning rate continues to have a well-defined average, s{sub T}{approx}u-check, the burning is unsteady. We present a theoretical framework, supported by both one-dimensional and three-dimensional numerical simulations, for the burning in these two regimes. Our results indicate that the average value of s{sub T} can actually be roughly twice u-check for Da{sub T} {approx}> 1, and that localized excursions to as much as 5 times u-check can occur. We also explore the properties of the individual flames, which could be sites for a transition to detonation when Da{sub T} {approx} 1. The lambda-flame speed and width can be predicted based on the turbulence in the star (specifically the energy dissipation rate epsilon*) and the turbulent nuclear burning timescale of the fuel tau {sup T}{sub nuc}. We propose a practical method for measuring s{sub l}ambda and l{sub l}ambda based on the scaling relations and small-scale computationally inexpensive simulations. This suggests that a simple turbulent flame model can be easily constructed suitable for large-scale distributed SNe flames. These results will be useful both for characterizing the deflagration speed in larger full-star simulations, where the flame cannot be resolved, and for predicting when detonation occurs.

Aspden, A. J.; Bell, J. B. [Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (United States); Woosley, S. E. [Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (United States)

2010-02-20T23:59:59.000Z

91

Property:HPBD/ProjectId | Open Energy Information  

Open Energy Info (EERE)

ProjectId ProjectId Jump to: navigation, search This is a property of type Number. Pages using the property "HPBD/ProjectId" Showing 25 pages using this property. (previous 25) (next 25) H High Performance Buildings Database + 203 + High Performance Buildings Database + 358 + High Performance Buildings Database + 71 + High Performance Buildings Database + 833 + High Performance Buildings Database + 247 + High Performance Buildings Database + 20 + High Performance Buildings Database + 498 + High Performance Buildings Database + 132 + High Performance Buildings Database + 194 + High Performance Buildings Database + 323 + High Performance Buildings Database + 50 + High Performance Buildings Database + 785 + High Performance Buildings Database + 223 +

92

Redshift-Independent Distances to Type Ia Supernovae  

E-Print Network (OSTI)

We describe a procedure for accurately determining luminosity distances to Type Ia supernovae (SNe Ia) without knowledge of redshift. This procedure, which may be used as an extension of any of the various distance determination methods currently in use, is based on marginalizing over redshift, removing the requirement of knowing $z$ a priori. We demonstrate that the Hubble diagram scatter of distances measured with this technique is approximately equal to that of distances derived from conventional redshift-specific methods for a set of 60 nearby SNe Ia. This indicates that accurate distances for cosmological SNe Ia may be determined without the requirement of spectroscopic redshifts, which are typically the limiting factor for the number of SNe that modern surveys can collect. Removing this limitation would greatly increase the number of SNe for which current and future SN surveys will be able to accurately measure distance. The method may also be able to be used for high-$z$ SNe Ia to determine cosmological density parameters without redshift information.

Brian J. Barris; John L. Tonry

2004-08-04T23:59:59.000Z

93

DOE - Office of Legacy Management -- Chicago North IL Site - IL 05  

Office of Legacy Management (LM)

North IL Site - IL 05 North IL Site - IL 05 FUSRAP Considered Sites Chicago North, IL Alternate Name(s): National Guard Armory 124th Field Artillery Armory Illinois National Guard Armory Site IL.05-4 IL.05-5 Location: 5200 Cottage Grove Avenue, Chicago, Illinois IL.05-4 Historical Operations: Processed and stored uranium metal, resulting in uranium metal and dry uranium oxide contamination. Metallurgical operations were conducted by the University of Chicago, an MED contractor. IL.05-5 IL.05-7 IL.05-8 Eligibility Determination: Eligible IL.05-1 IL.05-2 IL.05-3 Radiological Survey(s): Assessment Surveys, Verification Surveys IL.05-6 IL.05-7 Site Status: Certified-Certification Basis, Federal Register Notice Included IL.05-7 Long-term Care Requirements: Long-Term Surveillance and Maintenance Requirements for Remediated FUSRAP Sites S07566_FUSRAP

94

US ENC IL Site Consumption  

U.S. Energy Information Administration (EIA) Indexed Site

IL IL Site Consumption million Btu $0 $500 $1,000 $1,500 $2,000 $2,500 US ENC IL Expenditures dollars ALL ENERGY average per household (excl. transportation) 0 2,000 4,000 6,000 8,000 10,000 12,000 US ENC IL Site Consumption kilowatthours $0 $250 $500 $750 $1,000 $1,250 $1,500 US ENC IL Expenditures dollars ELECTRICITY ONLY average per household * Illinois households use 129 million Btu of energy per home, 44% more than the U.S. average. * High consumption, combined with low costs for heating fuels compared to states with a similar climate, result in Illinois households spending 2% more for energy than the U.S. average. * Less reliance on electricity for heating, as well as cool summers keeps average site electricity consumption in the state low relative to other parts of the U.S.

95

US ENC IL Site Consumption  

Gasoline and Diesel Fuel Update (EIA)

IL IL Site Consumption million Btu $0 $500 $1,000 $1,500 $2,000 $2,500 US ENC IL Expenditures dollars ALL ENERGY average per household (excl. transportation) 0 2,000 4,000 6,000 8,000 10,000 12,000 US ENC IL Site Consumption kilowatthours $0 $250 $500 $750 $1,000 $1,250 $1,500 US ENC IL Expenditures dollars ELECTRICITY ONLY average per household * Illinois households use 129 million Btu of energy per home, 44% more than the U.S. average. * High consumption, combined with low costs for heating fuels compared to states with a similar climate, result in Illinois households spending 2% more for energy than the U.S. average. * Less reliance on electricity for heating, as well as cool summers keeps average site electricity consumption in the state low relative to other parts of the U.S.

96

2010 Annual Planning Summary for Idaho Operations Office (ID...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

to be prepared in the next 24 months, and the planned cost and schedule for each NEPA review identified. 2010 Annual Planning Summary for Idaho Operations Office (ID) More...

97

Category:Chicago, IL | Open Energy Information  

Open Energy Info (EERE)

IL IL Jump to: navigation, search Go Back to PV Economics By Location Media in category "Chicago, IL" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Chicago IL Commonwealth Edison Co.png SVFullServiceRestauran... 74 KB SVHospital Chicago IL Commonwealth Edison Co.png SVHospital Chicago IL ... 68 KB SVLargeHotel Chicago IL Commonwealth Edison Co.png SVLargeHotel Chicago I... 75 KB SVLargeOffice Chicago IL Commonwealth Edison Co.png SVLargeOffice Chicago ... 76 KB SVMediumOffice Chicago IL Commonwealth Edison Co.png SVMediumOffice Chicago... 73 KB SVMidriseApartment Chicago IL Commonwealth Edison Co.png SVMidriseApartment Chi... 77 KB SVOutPatient Chicago IL Commonwealth Edison Co.png SVOutPatient Chicago I... 74 KB SVPrimarySchool Chicago IL Commonwealth Edison Co.png

98

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star  

E-Print Network (OSTI)

The absolute magnitudes of Type IA supernovae. Astrophys. J.in a Sublu- o minous Type Ia Supernova: SpectropolarimetryL. Could There Be a Hole in Type Ia Super- novae? Astrophys.

2008-01-01T23:59:59.000Z

99

DOE - Office of Legacy Management -- Granite City IL Site - IL 28  

Office of Legacy Management (LM)

Granite City IL Site - IL 28 Granite City IL Site - IL 28 FUSRAP Considered Sites Granite City, IL Alternate Name(s): Granite City Steel General Steel Industries General Steel Casings Corporation New Betatron Building IL.28-3 Location: 1417 State Street, Granite City, Illinois IL.28-3 Historical Operations: Under subcontract with Mallinckrodt and using a government-owned Betatron (magnetic induction electron accelerator), x-rayed natural uranium ingots and dingots to detect metallurgical flaws. Contamination from rubbing off of oxidized uranium during handling. IL.28-3 IL.28-5 Eligibility Determination: Eligible IL.28-1 IL.28-2 Radiological Survey(s): Assessment Surveys, Verification Survey IL.28-6 IL.28-7 IL.28-8 Site Status: Certified - Certification Basis, Federal Register Notice included IL.28-9

100

Nucleosynthesis in type Ia supernovae driven by asymmetric thermonuclear ignition  

Science Conference Proceedings (OSTI)

Type Ia Supernovae (SNe Ia) are believed to be thermonuclear explosions of a white dwarf. They can be used as mature cosmological standardized candles, leading to the discovery of the accelerating expansion of the Universe. However, the explosion mechanism has not yet been fully clarified. In this paper, we first present nucleosynthetic features of a leading explosion scenario, namely a delayed-detonation scenario. Based on this, we propose a new and strong observational constraint on the explosion mechanism through emission lines from neutron-rich Fe-peaks. Especially, we show that an asymmetry in the explosion is likely a generic feature. We further argue that the diversity arising from various viewing angles can be an origin of observational diversities of SNe Ia seen in their spectral features (suspected possible biases in cosmology) and colors (related to the extinction estimate in cosmology). Using these new insights could open up a possibility of using SNe Ia as more precise distance indicators than currently employed.

Maeda, Keiichi [Institute for the Physics and Mathematics of the Universe (IPMU), Todai Institutes for Advanced Study (TODIAS), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

2012-11-12T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

Balanced binary trees for ID management and load balance in distributed hash tables  

Science Conference Proceedings (OSTI)

We present a low-cost, decentralized algorithm for ID management in distributed hash tables (DHTs) managed by a dynamic set of hosts. Each host is assigned an ID in the unit interval [0, 1). At any time, the set of IDs splits the interval into disjoint ... Keywords: DHT, ID management, P2P, binary tree, distributed hash table, load balance, peer to peer

Gurmeet Singh Manku

2004-07-01T23:59:59.000Z

102

Property:EiaUtilityId | Open Energy Information  

Open Energy Info (EERE)

EiaUtilityId EiaUtilityId Jump to: navigation, search This is a property of type String. Pages using the property "EiaUtilityId" Showing 25 pages using this property. (previous 25) (next 25) 3 3 Phases Energy Services + 21093 + 4 4-County Electric Power Assn + 6641 + A A & N Electric Coop + 84 + A & N Electric Coop (Virginia) + 84 + AEP Generating Company + 343 + AEP Texas Central Company + 3278 + AEP Texas North Company + 20404 + AES Eastern Energy LP + 134 + AGC Division of APG Inc + 261 + AP Holdings LLC + 56571 + AP Holdings LLC (New York) + 56571 + APN Starfirst, L.P. + 50153 + APN Starfirst, L.P. (Illinois) + 50153 + APN Starfirst, L.P. (Ohio) + 50153 + APN Starfirst, L.P. (Texas) + 50153 + APNA Energy + 55841 + ARCO Products Co-Watson + 867 +

103

Intergral Drive Systems AG IDS | Open Energy Information  

Open Energy Info (EERE)

Intergral Drive Systems AG IDS Intergral Drive Systems AG IDS Jump to: navigation, search Name Intergral Drive Systems AG (IDS) Place Zurich, Swaziland Zip CH-8005 Sector Wind energy Product Zurich based producer of power electronics systems for wind turbines, PV plants, and propulsion systems. Coordinates 47.37706°, 8.53955° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":47.37706,"lon":8.53955,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

104

Building Energy Software Tools Directory: ID-Spec Large  

NLE Websites -- All DOE Office Websites (Extended Search)

ID-Spec Large ID-Spec Large ID-Spec Large is software for the electrical installation design of industrial and tertiary buildings. It helps to design a green electrical installation by enabling the user to: - Assess the impact of selecting energy efficiency solutions like power factor correction and low losses transformers in terms of cost savings - Reduce power losses and consequently carbon emissions in the electrical installation by optimizing equipment locations - Reduce investment cost while using less raw materials by optimizing length and cross-section of cables - Assess the percentage of recyclable materials for cables and busbar trunking systems. Screen Shots Keywords Electrical installation design, power losses assessment, CO2 emissions, quantity of conductors

105

Microsoft Word - DOE-ID-INL-13-006.docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

ID-NEPA CX DETERMINATION ID-NEPA CX DETERMINATION Idaho National Laboratory Page 1 of 3 EC Document No.: DOE-ID-INL-13-006 SECTION A. Project Title: Power Line Configuration 2013-1 SECTION B. Project Description: This project will install temporary distribution-level power lines between Materials and Fuels Complex (MFC) and Critical Infrastructure Test Range Complex (CITRC) to support research and development and testing using electric power infrastructure. Two circuits of three-phase distribution lines will be installed from Power Burst Facility (PBF)-613 to the MFC test pad. Standard new crossarms and insulators will be installed on the existing 138kV H structures (underbuild) to support standard aluminum conductors steel reinforced (ACSR) conductors for the majority of the configuration change (approximately from Pole 40E to Pole 127E - an

106

Category:Springfield, IL | Open Energy Information  

Open Energy Info (EERE)

IL IL Jump to: navigation, search Go Back to PV Economics By Location Media in category "Springfield, IL" The following 16 files are in this category, out of 16 total. SVQuickServiceRestaurant Springfield IL Commonwealth Edison Co.png SVQuickServiceRestaura... 75 KB SVFullServiceRestaurant Springfield IL Commonwealth Edison Co.png SVFullServiceRestauran... 75 KB SVHospital Springfield IL Commonwealth Edison Co.png SVHospital Springfield... 67 KB SVLargeHotel Springfield IL Commonwealth Edison Co.png SVLargeHotel Springfie... 75 KB SVLargeOffice Springfield IL Commonwealth Edison Co.png SVLargeOffice Springfi... 76 KB SVMediumOffice Springfield IL Commonwealth Edison Co.png SVMediumOffice Springf... 74 KB SVMidriseApartment Springfield IL Commonwealth Edison Co.png

107

Optical Spectra of Type Ia Supernovae at z=0.46 and z=1.2  

E-Print Network (OSTI)

We present optical spectra, obtained with the Keck 10-m telescope, of two high-redshift type Ia supernovae (SNe Ia) discovered by the High-z Supernova Search Team: SN 1999ff at z=0.455 and SN 1999fv at z~1.2, the highest-redshift published SN Ia spectrum. Both SNe were at maximum light when the spectra were taken. We compare our high-z spectra with low-z normal and peculiar SNe Ia as well as with SNe Ic, Ib, and II. There are no significant differences between SN 1999ff and normal SNe Ia at low redshift. SN 1999fv appears to be a SN Ia and does not resemble the most peculiar nearby SNe Ia.

Coil, A L; Filippenko, A V; Leonard, D C; Tonry, J; Riess, A G; Challis, P M; Clocchiatti, A; Garnavich, P M; Hogan, C J; Jha, S; Kirshner, R P; Leibundgut, B; Phillips, M M; Schmidt, B P; Schommer, R A; Smith, R C; Soderberg, A M; Spyromilio, J; Stubbs, C; Suntzeff, N B; Woudt, P A; Coil, Alison L.; Matheson, Thomas; Filippenko, Alexei V.; Leonard, Douglas C.; Tonry, John; Riess, Adam G.; Challis, Peter; Clocchiatti, Alejandro; Garnavich, Peter M.; Hogan, Craig J.; Jha, Saurabh; Kirshner, Robert P.; Schmidt, Brian P.; Schommer, Robert A.; Soderberg, Alicia M.; Stubbs, Christopher; Suntzeff, Nicholas B.; Woudt, Patrick

2000-01-01T23:59:59.000Z

108

Progenitors of type Ia supernovae in elliptical galaxies  

Science Conference Proceedings (OSTI)

Although there is a nearly universal agreement that type Ia supernovae are associated with the thermonuclear disruption of a CO white dwarf, the exact nature of their progenitors is still unknown. The single degenerate scenario envisages a white dwarf accreting matter from a non-degenerate companion in a binary system. Nuclear energy of the accreted matter is released in the form of electromagnetic radiation or gives rise to numerous classical nova explosions prior to the supernova event. We show that combined X-ray output of supernova progenitors and statistics of classical novae predicted in the single degenerate scenario are inconsistent with X-ray and optical observations of nearby early type galaxies and galaxy bulges. White dwarfs accreting from a donor star in a binary system and detonating at the Chandrasekhar mass limit can account for no more than {approx}5% of type Ia supernovae observed in old stellar populations.

Gilfanov, M.; Bogdan, A.

2011-09-21T23:59:59.000Z

109

Learning from the scatter in type ia supernovae  

SciTech Connect

Type Ia Supernovae are standard candles so their mean apparent magnitude has been exploited to learn about the redshift-distance relationship. Besides intrinsic scatter in this standard candle, additional scatter is caused by gravitational magnification by large scale structure. Here they probe the dependence of this dispersion on cosmological parameters and show that information about the amplitude of clustering, {sigma}{sub s}, is contained in the scatter. In principle, it will be possible to constrain {sigma}{sub s} to within 5% with observations of 2000 Type Ia Supernovae. They identify three sources of systematic error--evolution of intrinsic scatter, baryon contributions to lensing, and non-Gaussianity of lensing--which will make this measurement difficult.

Dodelson, Scott; /Fermilab /Chicago U., Astron. Astrophys. Ctr.; Vallinotto, Alberto; /Fermilab /Chicago U.

2005-11-01T23:59:59.000Z

110

Type Ia Supernova Spectral Line Ratios as LuminosityIndicators  

SciTech Connect

Type Ia supernovae have played a crucial role in thediscovery of the dark energy, via the measurement of their light curvesand the determination of the peak brightness via fitting templates to theobserved lightcurve shape. Two spectroscopic indicators are also known tobe well correlated with peak luminosity. Since the spectroscopicluminosity indicators are obtained directly from observed spectra, theywill have different systematic errors than do measurements usingphotometry. Additionally, these spectroscopic indicators may be usefulfor studies of effects of evolution or age of the SNe~;Ia progenitorpopulation. We present several new variants of such spectroscopicindicators which are easy to automate and which minimize the effects ofnoise. We show that these spectroscopic indicators can be measured byproposed JDEM missions such as snap and JEDI.

Bongard, Sebastien; Baron, E.; Smadja, G.; Branch, David; Hauschildt, Peter H.

2005-12-07T23:59:59.000Z

111

u.s. DEPARTlIlENT OF ENERGY EERE PROJECT MANAGEM ENT CENT ER  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DEPARTlIlENT OF ENERGY DEPARTlIlENT OF ENERGY EERE PROJECT MANAGEM ENT CENT ER NEPA DFTFRlIllNATION Page 1 of2 RECIPIENT:City of Cleveland· Division of Engineering & Construction STATE: OH PROJECT TITLE: Cleveland City ARRA·EECBG Act 9 (Lake-to--Lake Bikeway) Funding Opportunity Announcement Number Procurement Instrument Number NEPA Control Number cm Number OE·EEOOOO705 0 Based on my review oflhe information concerning the proposed action, as NEPA Compliance Officer (authorized under DOE Order 451.IA), [have made the following determination: CX, EA, E[S APPENDIX AND NUMBER: Description: A11 Technical advice and planning assistance to internaUonal, national, stale, and local organizations, A9 Information gathering (including, but not limited to, literature surveys, inventories, audits), data analysis (including

112

ORNL 2011-G00219/jcn UT-B ID 201002414  

E-Print Network (OSTI)

ORNL 2011-G00219/jcn UT-B ID 201002414 08.2011 Catalytic Conversion of Bioethanol to Hydrocarbons dilute bio-mass produced alcohols, such as those found in a biomass fermentation reactor. Conventional of traditional ethanol fermentation into fungible fuel applications Potential Applications · Hydrocarbon products

Pennycook, Steve

113

An adaptive architecture of applying vulnerability analysis to IDS alerts  

Science Conference Proceedings (OSTI)

With increasing intrusions and attacks on the Internet, there is an urgent need to develop techniques for network security. Current standalone network security products, such as the firewall systems, the Intrusion Detection System (IDS), the anti-virus ... Keywords: alert, intrusion detection, network security, predicate-based evaluation, vulnerability analysis

Xuejiao Liu; Xin Zhuang; Debao Xiao

2008-07-01T23:59:59.000Z

114

ORNL 2010-G00390/jcn UT-B ID 200802041  

E-Print Network (OSTI)

from Water Technology Summary Developing the technology to generate energy from waste and renewableORNL 2010-G00390/jcn UT-B ID 200802041 Microbial Fuel Cells Generate Energy While Clearing Biowaste materials is becoming an increasingly important priority in the United States, as energy derived from fossil

Pennycook, Steve

115

ORNL 2011-G00218/jcn UT-B ID 200701859  

E-Print Network (OSTI)

be wasted energy inside a hybrid electric vehicle engine. The invention, a mechanical flywheel coupledORNL 2011-G00218/jcn UT-B ID 200701859 07.2011 Flywheel Energy Storage Device for Hybrid to a rotor inside the engine, stores rotational energy during engine performance, subsequently feeding

Pennycook, Steve

116

ORNL 2010-G00385/jcn UT-B ID 200301297  

E-Print Network (OSTI)

billion annually in lost productivity. Waste energy from deceleration could be captured and storedORNL 2010-G00385/jcn UT-B ID 200301297 Nanostructured Carbon Shows Promise for Energy Storage energy storage demands of modern supercapacitors. Short power interruptions cost U.S. industry $80

Pennycook, Steve

117

ORNL 2010-G00405 UT-B ID 200902330  

E-Print Network (OSTI)

Industrial Effluents Technology Summary A vast amount of energy is wasted in the United States from of such previously wasted energy from relatively low temperature (ORNL 2010-G00405 UT-B ID 200902330 Novel Nanopore Membrane Technology Recovers Energy from

Pennycook, Steve

118

ID-based proxy signature scheme with message recovery  

Science Conference Proceedings (OSTI)

A proxy signature scheme, introduced by Mambo, Usuda and Okamoto, allows an entity to delegate its signing rights to another entity. Identity based public key cryptosystems are a good alternative for a certificate based public key setting, especially ... Keywords: Bilinear pairing, ID-based signature, Mobile agent, Proxy signature, Signature with message recovery

Harendra Singh; Girraj Kumar Verma

2012-01-01T23:59:59.000Z

119

UW China Hong Kong Entrance Scholarship University of Waterloo ID#  

E-Print Network (OSTI)

UW ­ China Hong Kong Entrance Scholarship Name: University of Waterloo ID#: Program Applied of Waterloo who currently lives in or who previously lived in Hong Kong or mainland China. Candidates must also intend to return to Hong Kong or China after graduation. Selection will be based on academic

Le Roy, Robert J.

120

Investigating the Flame Microstructure in Type Ia Supernovae  

E-Print Network (OSTI)

We present a numerical model to study the behavior of thermonuclear flames in the discontinuity approximation. This model is applied to investigate the Landau-Darrieus instability under conditions found in Type Ia supernova explosions of Chandrasekhar mass white dwarfs. This is a first step to explore the flame microstructure in these events. The model reproduces Landau's linearized stability analysis in early stages of the flame evolution and the stabilization in a cellular flame structure in the nonlinear stage.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2002-04-02T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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121

Reflections on Reflexions: I. Light Echoes in Type Ia Supernovae  

E-Print Network (OSTI)

In the last ten years, observational evidences about a possible connection between Type Ia Supernovae (SNe) properties and the environment where they explode have been steadily growing. In this paper I discuss, from a theoretical point of view but with an observer's perspective, the usage of light echoes (LEs) to probe the CSM around SNe of Type Ia since, in principle, they give us a unique opportunity of getting a three-dimensional description of the SN environment. In turn, this can be used to check the often suggested association of some Ia's with dusty/star forming regions, which would point to a young population for the progenitors. After giving a brief introduction to the LE phenomenon in single scattering approximation, I derive analytical and numerical solutions for the optical light and colour curves for a few simple dust geometries. A fully 3D multiple scattering treatment has also been implemented in a Monte Carlo code, which I have used to investigate the effects of multiple scattering. In particu...

Patat, F

2004-01-01T23:59:59.000Z

122

Could There Be A Hole In Type Ia Supernovae?  

E-Print Network (OSTI)

In the favored progenitor scenario, Type Ia supernovae arise from a white dwarf accreting material from a non-degenerate companion star. Soon after the white dwarf explodes, the ejected supernova material engulfs the companion star; two-dimensional hydrodynamical simulations by Marietta et. al. show that, in the interaction, the companion star carves out a conical hole of opening angle 30-40 degrees in the supernova ejecta. In this paper we use multi-dimensional Monte Carlo radiative transfer calculations to explore the observable consequences of an ejecta-hole asymmetry. We calculate the variation of the spectrum, luminosity, and polarization with viewing angle for the aspherical supernova near maximum light. We find that the supernova looks normal from almost all viewing angles except when one looks almost directly down the hole. In the latter case, one sees into the deeper, hotter layers of ejecta. The supernova is relatively brighter and has a peculiar spectrum characterized by more highly ionized species, weaker absorption features, and lower absorption velocities. The spectrum viewed down the hole is comparable to the class of SN 1991T-like supernovae. We consider how the ejecta-hole asymmetry may explain the current spectropolarimetric observations of SNe Ia, and suggest a few observational signatures of the geometry. Finally, we discuss the variety currently seen in observed SNe Ia and how an ejecta-hole asymmetry may fit in as one of several possible sources of diversity.

Daniel Kasen; Peter Nugent; R. C. Thomas; Lifan Wang

2003-11-01T23:59:59.000Z

123

Biolog(TM) ID as compared to 16S ribosomal RNA ID for environmental isolates from the deep subsurface  

SciTech Connect

The U.S. Dept of Energy (DOE) Subsurface Microbial Culture Collection (SMCC) contains nearly 10,000 strains of microorganisms isolated from terrestrial subsurface environments. Many of the aerobic, gram-negative, chemoheterotrophs isolated from the DOE Savannah River Site (SRS) have previously been identified by phylogenetic analysis of 16S ribosomal RNA (rRNA) gene nucleotide sequences. These SMCC isolates are currently being examined using Biolog GN Microplates and the Biolog Microstation System in order to gain knowledge of their metabolic capabilities and to compare Biolog IDs with 16S IDs. To accommodate the particular needs of these subsurface isolates, which are often incapable of growing under high-nutrient conditions, Biolog's recommendations for inoculating isolates into Biolog GN Microplates have been altered. The isolates are grown on low nutrient media, sodium thioglycolate (3mM) is added to the culture media to inhibit capsule formation, and a low density of bacteria is inoculated into the microplate. Using these altered inoculation criteria, 60 percent of these SMCC isolates have a Biolog genus ID that matches the 16S rRNA ID. These results indicate that the Biolog System can be a good means of identifying unusual environmental isolates, even when recommended inoculation procedures are altered to accommodate particular isolate needs.

McKinsey, P.C.

2000-05-05T23:59:59.000Z

124

Quantitative analysis of IL-2 and IL-15 signal transduction in T lymphocytes  

E-Print Network (OSTI)

IL-2 and IL-15 are common y-chain family cytokines critically involved in regulation of T cell differentiation and homeostasis. Both cytokines signal through a heterotrimeric surface receptor complex (IL-2/15R) composed ...

Arneja, Abhinav

2013-01-01T23:59:59.000Z

125

THE SDSS-II SUPERNOVA SURVEY: PARAMETERIZING THE TYPE Ia SUPERNOVA RATE AS A FUNCTION OF HOST GALAXY PROPERTIES  

Science Conference Proceedings (OSTI)

Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.

Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7530, Cape Town (South Africa); Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX (United Kingdom); Dilday, Benjamin [Las Cumbres Observatory Global Telescope Network, 6740 Cortona Dr., Suite 102, Goleta, CA 93117 (United States); Marriner, John; Frieman, Joshua [Center for Particle Astrophysics, Fermilab, P.O. Box 500, Batavia, IL 60510 (United States); Kessler, Richard [Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Ave, Chicago, IL 60637 (United States); Bassett, Bruce [African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg 7945 (South Africa); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); Garnavich, Peter [Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers, State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Lampeitl, Hubert [Astrophysics, Cosmology and Gravity Centre (ACGC), Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701 (South Africa); Sako, Masao [Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Sollerman, Jesper, E-mail: matsmith2@gmail.com [Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, SE-106 91 Stockholm (Sweden)

2012-08-10T23:59:59.000Z

126

Microsoft Word - DOE-ID-INL-12-018.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

8 8 SECTION A. Project Title: Rexburg Bus Lot (B60-1789-D-NE) Lease Termination SECTION B. Project Description: The proposed activity will terminate the lease of approximately four bus spaces at the Rexburg Parking Lot (B60-1789-D-NE) at South 5 th West in Rexburg, ID on or about July 31, 2012 for cost savings and consolidation to the existing lot at Rigby, ID. A facility walkthrough by BEA personnel will be performed in order to ensure the facility is ready for turnover back to the owner. Approximate cost associated with the activity is estimated at $1,500.00. SECTION C. Environmental Aspects / Potential Sources of Impact: Transacting real property in Rexburg, Idaho and moving four buses to a lot in Rigby, Idaho will not affect any INL environmental

127

Microsoft Word - DOE-ID-INL-12-021.docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DOE-ID-INL-12-021 DOE-ID-INL-12-021 SECTION A. Project Title: High Frequency Sounder - Permanent Installation at Water Reactor Research Test Facility (WRRTF) SECTION B. Project Description: The scope of this project is to construct and operate a 150-watt high frequency (HF) radio antenna (both transmit and receive) within the fenced area of the former Water Reactor Research Test Facility (WRRTF) to support various wireless test bed (WTB) activities and increase WTB capabilities by measuring the ionospheric characteristics of the region. The measurements are used to generate propagation maps of the ionosphere to graphically illustrate what HF frequencies are effective for communications. Construction is scheduled to take place in the August-September 2012 timeframe with operation beginning in October 2012.

128

Microsoft Word - DOE-ID-INL-12-003.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

EC Document No.: DOE-ID-INL-12-003 EC Document No.: DOE-ID-INL-12-003 SECTION A. Project Title: Auxiliary Canal Fill Project at Test Reactor Area (TRA)-670 SECTION B. Project Description: Although the ATR canal meets all design basis criteria, lessons learned following the earthquake and tsunami events at the Fukushima- Daiichi Nuclear Power Plant in March of 2011 indicate that an auxiliary water supply to the fuel storage canal with a fill connection located outside of the facility would have been valuable following the beyond design basis event. As a result of these lessons learned, the Department of Energy (DOE) has allocated additional funding to the Idaho National Laboratory (INL) to mitigate beyond design basis events similar to the Fukushima-Daiichi disaster. The Auxiliary Canal Fill Project is one of the projects being funded from this

129

Microsoft Word - DOE-ID-INL-12-012.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

ECX Posting No.: DOE-ID-INL-12-012 ECX Posting No.: DOE-ID-INL-12-012 SECTION A. Project Title: Film Processing Project at Test Reactor Area (TRA)-678 SECTION B. Project Description The proposed action is to install a silver recovery unit to the film processor in the film processing area at TRA-678 for the purpose of minimizing waste generation and implementing pollution prevention. The proposed film processor (Kodak M-35A) generates approximately 90 ml of developer and 140 ml of fixer effluents per 17 inch film and approximately 40 gallons per hour of rinse water effluent. Developer and fixer effluents from the current film processing equipment are being collected in a Satellite Accumulation Area (SAA). The new equipment would eliminate the need for storing the effluent in the SAA by filtering silver from the effluent for recycling. The remaining

130

Microsoft Word - DOE-ID-INL-10-020.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-ID-INL-10-020 DOE-ID-INL-10-020 SECTION A. Project Title: Idaho National Laboratory (INL) Routine Maintenance Activities (Overarching) SECTION B. Project Description: The purpose of this overarching Environmental Checklist (EC) is to address activities that would meet the intent of the categorical exclusion (CX) B1.3 as described in 10 CFR 1021, Appendix B to Subpart D. These activities would consist of typical and non-typical types of actions, such as routine maintenance, minor modifications, and custodial service activities required to support safe and efficient plant operation, even if performed on an infrequent basis, and would occur on the INL Site and at those in town (Idaho Falls) facilities. These activities would be performed by INL Facility and Site Services personnel or off-site contractors. None of these activities would

131

Microsoft Word - DOE-ID-INL-13-007.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

8 8 EC Document No.: DOE-ID-INL-13-007 SECTION A. Project Title: Seismic Monitoring for Seismic Hazards Analyses SECTION B. Project Description: The Idaho National Laboratory (INL) Probabilistic Seismic Hazards Analysis (PSHA) Phase I - Data Collection and Evaluation project is being conducted by Battelle Energy Alliance (BEA) at the request of the U.S. Department of Energy Idaho Operations office (DOE-ID) and INL Management. The project is being conducted from FY-2013 to FY-2017. Earthquake data will be collected at seismic stations located near INL facility areas for at least two years using seismometers and for the long-term using accelerometers. Installation of the seismic stations is being funded by the INL PSHA - Data Collection and Evaluation project and, following completion of this project,

132

Microsoft Word - DOE-ID-INL-10-017.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DOE-ID-INL-10-017 DOE-ID-INL-10-017 SECTION A. Project Title: ATR Complex Dial Room. SECTION B. Project Description: The proposed project is to construct and operate a new dial room at the Advanced Test Reactor Complex (ATR Complex) (formerly known as the Test Reactor Area [TRA]) in order to meet the U.S. Department of Energy Office of Nuclear Energy programmatic needs and to provide ongoing critical support at the Idaho National Laboratory (INL). The existing telecommunication and data systems located at the ATR Complex need to be updated to ensure the protection and continuity of telecommunications hardware and software property and provide reliability of communications and data connectivity. The new modular dial room facility will replace existing telecommunications systems equipment (telephony, optical transport, and data network infrastructure

133

Microsoft Word - DOE-ID-INL-10-020.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DOE-ID-INL-10-020 DOE-ID-INL-10-020 SECTION A. Project Title: Idaho National Laboratory (INL) Routine Maintenance Activities (Overarching) SECTION B. Project Description: The purpose of this overarching Environmental Checklist (EC) is to address activities that would meet the intent of the categorical exclusion (CX) B1.3 as described in 10 CFR 1021, Appendix B to Subpart D. These activities would consist of typical and non-typical types of actions, such as routine maintenance, minor modifications, and custodial service activities required to support safe and efficient plant operation, even if performed on an infrequent basis, and would occur on the INL Site and at those in town (Idaho Falls) facilities. These activities would be performed by INL Facility and Site Services personnel or off-site contractors. None of these activities would

134

Microsoft Word - DOE-ID-INL-12-016.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

No.: DOE-ID-INL-12-016 No.: DOE-ID-INL-12-016 SECTION A. Project Title: Reverse Osmosis System Removal SECTION B. Project Description: The project will remove a reverse osmosis water treatment system (FU-HA-101) from TAN 681 room 182. The system is out-of-service, with no intent of future use. Work will involve removal of the reverse osmosis system, and associated plumbing/piping and electrical lines and conduit. The project will clear the area of obstacles and tripping hazards associated with unused/unnecessary equipment and utilities. SECTION C. Environmental Aspects / Potential Sources of Impact: Generating and Managing Waste: Project activities will result in generation of an estimated 90 cubic ft. of low-level radioactive waste. Wastes will be characterized and dispositioned through Waste Generator Services. Reuse and recycling of materials will be practiced

135

Microsoft Word - DOE-ID-INL-12-021.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-ID-INL-12-021 DOE-ID-INL-12-021 SECTION A. Project Title: High Frequency Sounder - Permanent Installation at Water Reactor Research Test Facility (WRRTF) SECTION B. Project Description: The scope of this project is to construct and operate a 150-watt high frequency (HF) radio antenna (both transmit and receive) within the fenced area of the former Water Reactor Research Test Facility (WRRTF) to support various wireless test bed (WTB) activities and increase WTB capabilities by measuring the ionospheric characteristics of the region. The measurements are used to generate propagation maps of the ionosphere to graphically illustrate what HF frequencies are effective for communications. Construction is scheduled to take place in the August-September 2012 timeframe with operation beginning in October 2012.

136

Microsoft Word - DOE-ID-INL-13-007.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

8 8 EC Document No.: DOE-ID-INL-13-007 SECTION A. Project Title: Seismic Monitoring for Seismic Hazards Analyses SECTION B. Project Description: The Idaho National Laboratory (INL) Probabilistic Seismic Hazards Analysis (PSHA) Phase I - Data Collection and Evaluation project is being conducted by Battelle Energy Alliance (BEA) at the request of the U.S. Department of Energy Idaho Operations office (DOE-ID) and INL Management. The project is being conducted from FY-2013 to FY-2017. Earthquake data will be collected at seismic stations located near INL facility areas for at least two years using seismometers and for the long-term using accelerometers. Installation of the seismic stations is being funded by the INL PSHA - Data Collection and Evaluation project and, following completion of this project,

137

DOE-ID Procurement Services � the action team  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-ID Procurement Services � the action team DOE-ID Procurement Services � the action team Passage of the American Recovery and Reinvestment Act of 2009 included billions of dollars in additional funding for energy efficiency improvements to U.S. homes and businesses. By early July, the U.S. Department of Energy was hard pressed to get that funding to the communities who needed it to reduce their power bills. That�s when DOE�s Office of Energy Efficiency asked the department�s Idaho Operations Office for support from DOE-ID�s Procurement Services team. Rapid response Pat Alexander-Johnson (top) and Jeff Fogg (bottom) are two highly-trained and experienced contract specialists with the U.S. Department of Energy's Idaho Operations Office. Within moments of receiving its orders, the 10-member team shifted into

138

Microsoft Word - DOE-ID-INL-12-024..doc  

NLE Websites -- All DOE Office Websites (Extended Search)

PostingNo.: DOE-ID-INL-12-024 PostingNo.: DOE-ID-INL-12-024 SECTION A. Project Title: Rigby Bus Lot Northwest Entrance SECTION B. Project Description: The purpose of the proposed action is to provide an additional bus entrance to the Rigby Park and Ride Bus Lot. A portion of chain link fencing (running east to west) on the northwest corner of the Rigby Park and Ride Bus Lot would be relocated to allow an opening off of the City of Rigby dirt access road so that buses may enter the Rigby Park and Ride Lot from the northwest. The existing fence material would then be placed across the City of Rigby dirt access road (running north and south). The new entrance would be for buses only. Approximately 4 to 6 buses would use this entrance. No personnel vehicles will have access. Buses would start using the new

139

Microsoft Word - DOE-ID-INL-12-012.docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

ECX Posting No.: DOE-ID-INL-12-012 ECX Posting No.: DOE-ID-INL-12-012 SECTION A. Project Title: Film Processing Project at Test Reactor Area (TRA)-678 SECTION B. Project Description The proposed action is to install a silver recovery unit to the film processor in the film processing area at TRA-678 for the purpose of minimizing waste generation and implementing pollution prevention. The proposed film processor (Kodak M-35A) generates approximately 90 ml of developer and 140 ml of fixer effluents per 17 inch film and approximately 40 gallons per hour of rinse water effluent. Developer and fixer effluents from the current film processing equipment are being collected in a Satellite Accumulation Area (SAA). The new equipment would eliminate the need for storing the effluent in the SAA by filtering silver from the effluent for recycling. The remaining

140

Microsoft Word - DOE-ID-INL-12-018.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

8 8 SECTION A. Project Title: Rexburg Bus Lot (B60-1789-D-NE) Lease Termination SECTION B. Project Description: The proposed activity will terminate the lease of approximately four bus spaces at the Rexburg Parking Lot (B60-1789-D-NE) at South 5 th West in Rexburg, ID on or about July 31, 2012 for cost savings and consolidation to the existing lot at Rigby, ID. A facility walkthrough by BEA personnel will be performed in order to ensure the facility is ready for turnover back to the owner. Approximate cost associated with the activity is estimated at $1,500.00. SECTION C. Environmental Aspects / Potential Sources of Impact: Transacting real property in Rexburg, Idaho and moving four buses to a lot in Rigby, Idaho will not affect any INL environmental

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

File:INL-geothermal-id.pdf | Open Energy Information  

Open Energy Info (EERE)

id.pdf id.pdf Jump to: navigation, search File File history File usage Idaho Geothermal Resources Size of this preview: 380 × 600 pixels. Full resolution ‎(3,458 × 5,456 pixels, file size: 1.67 MB, MIME type: application/pdf) Description Idaho Geothermal Resources Sources Idaho National Laboratory Authors Patrick Laney; Julie Brizzee Related Technologies Geothermal Creation Date 2003-11-01 Extent State Countries United States UN Region Northern America States Idaho File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 12:24, 16 December 2010 Thumbnail for version as of 12:24, 16 December 2010 3,458 × 5,456 (1.67 MB) MapBot (Talk | contribs) Automated upload from NREL's "mapsearch" data

142

DOE - Office of Legacy Management -- Chicago South IL Site - IL 06  

NLE Websites -- All DOE Office Websites (Extended Search)

South IL Site - IL 06 South IL Site - IL 06 FUSRAP Considered Sites Chicago South, IL Alternate Name(s): University of Chicago Charles Herbert Jones Chemical Laboratory Ryerson Physical Laboratory Eckhart Hall Kent Chemical Laboratory Ricketts Laboratory IL.06-3 Location: University of Chicago, Ellis Avenue and East 58th Street, Chicago, Illinois IL.06-3 Historical Operations: Performed activities associated with (1) production and purification of plutonium, which involved the handling and processing of uranium compounds; (2) demonstrating the self-sustaining nature of the fission process and the production of Pu-239 from U-238 (nuclear fission and Chicago Pile-1); and (3) health effects (metal toxicology and radiation effects). IL.06-5 IL.06-6 IL.06-7 Eligibility Determination: Eligible IL.06-1

143

DOE - Office of Legacy Management -- Chicago South IL Site - IL 06  

Office of Legacy Management (LM)

South IL Site - IL 06 South IL Site - IL 06 FUSRAP Considered Sites Chicago South, IL Alternate Name(s): University of Chicago Charles Herbert Jones Chemical Laboratory Ryerson Physical Laboratory Eckhart Hall Kent Chemical Laboratory Ricketts Laboratory IL.06-3 Location: University of Chicago, Ellis Avenue and East 58th Street, Chicago, Illinois IL.06-3 Historical Operations: Performed activities associated with (1) production and purification of plutonium, which involved the handling and processing of uranium compounds; (2) demonstrating the self-sustaining nature of the fission process and the production of Pu-239 from U-238 (nuclear fission and Chicago Pile-1); and (3) health effects (metal toxicology and radiation effects). IL.06-5 IL.06-6 IL.06-7 Eligibility Determination: Eligible IL.06-1

144

RENEWABLE ENERGY FROM SWINE WASTE Bingjun He, University of Idaho, Moscow, ID 1  

E-Print Network (OSTI)

RENEWABLE ENERGY FROM SWINE WASTE Bingjun He, University of Idaho, Moscow, ID 1 Yuanhui Zhang, Ted of Idaho, Moscow, ID 83844. Phone: 208.885.7714, fax: 208.885.7908, email: . 2Yuanhui Zhang

He, Brian

145

GRR/Section 13-ID-a - Land Use Assessment | Open Energy Information  

Open Energy Info (EERE)

ID-a - Land Use Assessment < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 13-ID-a - Land Use...

146

Microsoft Word - DOE-ID-INL-13-002 _INL-13-008_.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-ID NEPA CX DETERMINATION Idaho National Laboratory Page 2 of 2 CX Posting No.: DOE-ID-INL-13-002 If objects of potential archaeological or historical significance (e.g.,...

147

Microsoft Word - DOE-ID-INL-12-025-1.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

would be recycled to the extent practicable. DOE-ID NEPA CX DETERMINATION Idaho National Laboratory Page 2 of 2 CX Posting No.: DOE-ID-INL-12-025 SECTION D. Determine the...

148

Microsoft Word - DOE-ID-INL-12-007_INL-12-033_.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

personal protective equipment (PPE) where practical. DOE-ID NEPA CX DETERMINATION IDAHO NATIONAL LABORATORY Page 2 of 2 CX Posting No.: DOE-ID-INL-12-007 Releasing...

149

U-063: RSA SecurID Software Token for Windows DLL Loading Error...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

3: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code U-063: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote...

150

THE DIFFUSE GAMMA-RAY BACKGROUND FROM TYPE Ia SUPERNOVAE  

SciTech Connect

The origin of the diffuse extragalactic gamma-ray background (EGB) has been intensively studied but remains unsettled. Current popular source candidates include unresolved star-forming galaxies, starburst galaxies, and blazars. In this paper, we calculate the EGB contribution from the interactions of cosmic rays accelerated by Type Ia supernovae (SNe), extending earlier work that only included core-collapse SNe. We consider Type Ia events not only in star-forming galaxies, but also in quiescent galaxies that lack star formation. In the case of star-forming galaxies, consistently including Type Ia events makes little change to the star-forming EGB prediction, so long as both SN types have the same cosmic-ray acceleration efficiencies in star-forming galaxies. Thus, our updated EGB estimate continues to show that star-forming galaxies can represent a substantial portion of the signal measured by Fermi. In the case of quiescent galaxies, conversely, we find a wide range of possibilities for the EGB contribution. The dominant uncertainty we investigated comes from the mass in hot gas in these objects, which provides targets for cosmic rays; total gas masses are as yet poorly known, particularly at larger radii. Additionally, the EGB estimation is very sensitive to the cosmic-ray acceleration efficiency and confinement, especially in quiescent galaxies. In the most optimistic allowed scenarios, quiescent galaxies can be an important source of the EGB. In this case, star-forming galaxies and quiescent galaxies together will dominate the EGB and leave little room for other contributions. If other sources, such as blazars, are found to have important contributions to the EGB, then either the gas mass or cosmic-ray content of quiescent galaxies must be significantly lower than in their star-forming counterparts. In any case, improved Fermi EGB measurements will provide important constraints on hot gas and cosmic rays in quiescent galaxies.

Lien, Amy; Fields, Brian D. [Department of Physics, University of Illinois, Urbana, IL 61801 (United States)

2012-03-10T23:59:59.000Z

151

Reflections on Reflexions: I. Light Echoes in Type Ia Supernovae  

E-Print Network (OSTI)

In the last ten years, observational evidences about a possible connection between Type Ia Supernovae (SNe) properties and the environment where they explode have been steadily growing. In this paper I discuss, from a theoretical point of view but with an observer's perspective, the usage of light echoes (LEs) to probe the CSM around SNe of Type Ia since, in principle, they give us a unique opportunity of getting a three-dimensional description of the SN environment. In turn, this can be used to check the often suggested association of some Ia's with dusty/star forming regions, which would point to a young population for the progenitors. After giving a brief introduction to the LE phenomenon in single scattering approximation, I derive analytical and numerical solutions for the optical light and colour curves for a few simple dust geometries. A fully 3D multiple scattering treatment has also been implemented in a Monte Carlo code, which I have used to investigate the effects of multiple scattering. In particular, I have explored in detail the LE colour dependency from time and dust distribution, since this is a promising tool to determine the dust density and derive the effective presence of multiple scattering from the observed properties. Finally, again by means of Monte Carlo simulations, I have studied the effects of multiple scattering on the LE linear polarization, analyzing the dependencies from the dust parameters and geometry. Both the analytical formalism and MC codes described in this paper can be used for any LE for which the light curve of the central source is known.

F. Patat

2004-09-28T23:59:59.000Z

152

Turbulence-Flame Interactions in Type Ia Supernovae  

SciTech Connect

The large range of time and length scales involved in type Ia supernovae (SN Ia) requires the use of flame models. As a prelude to exploring various options for flame models, we consider, in this paper, high-resolution three-dimensional simulations of the small-scale dynamics of nuclear flames in the supernova environment in which the details of the flame structure are fully resolved. The range of densities examined, 1 to 8 x 107 g cm-3, spans the transition from the laminar flamelet regime to the distributed burning regime where small scale turbulence disrupts the flame. The use of a low Mach number algorithm facilitates the accurate resolution of the thermal structure of the flame and the inviscid turbulent kinetic energy cascade, while implicitly incorporating kinetic energy dissipation at the grid-scale cutoff. For an assumed background of isotropic Kolmogorov turbulence with an energy characteristic of SN Ia, we find a transition density between 1 and 3 x 107 g cm-3 where the nature of the burning changes ualitatively. By 1 x 107 g cm-3, energy diffusion by conduction and radiation is exceeded, on the flame scale, by turbulent advection. As a result, the effective Lewis Number approaches unity. That is, the flame resembles a laminar flame, but is turbulently broadened with an effective diffusion coefficient, D_T \\sim u' l, where u' is the turbulent intensity and l is the integral scale. For the larger integral scales characteristic of a real supernova, the flame structure is predicted to become complex and unsteady. Implications for a possible transition to detonation are discussed.

Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (Authors 1, 2& 3); Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (Author 4); Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (Author 5); Aspden, Andrew J; Aspden, Andrew J.; Bell, John B.; Day, Marc S.; Woosley, Stan E.; Zingale, Mike

2008-05-27T23:59:59.000Z

153

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

The large range of time and length scales involved in type Ia supernovae (SN Ia) requires the use of flame models. As a prelude to exploring various options for flame models, we consider, in this paper, high-resolution three-dimensional simulations of the small-scale dynamics of nuclear flames in the supernova environment in which the details of the flame structure are fully resolved. The range of densities examined, 1 to $8 \\times 10^7$ g cm$^{-3}$, spans the transition from the laminar flamelet regime to the distributed burning regime where small scale turbulence disrupts the flame. The use of a low Mach number algorithm facilitates the accurate resolution of the thermal structure of the flame and the inviscid turbulent kinetic energy cascade, while implicitly incorporating kinetic energy dissipation at the grid-scale cutoff. For an assumed background of isotropic Kolmogorov turbulence with an energy characteristic of SN Ia, we find a transition density between 1 and $3 \\times 10^7$ g cm$^{-3}$ where the nature of the burning changes qualitatively. By $1 \\times 10^7$ g cm$^{-3}$, energy diffusion by conduction and radiation is exceeded, on the flame scale, by turbulent advection. As a result, the effective Lewis Number approaches unity. That is, the flame resembles a laminar flame, but is turbulently broadened with an effective diffusion coefficient, $D_T \\sim u' l$, where $u'$ is the turbulent intensity and $l$ is the integral scale. For the larger integral scales characteristic of a real supernova, the flame structure is predicted to become complex and unsteady. Implications for a possible transition to detonation are discussed.

A. J. Aspden; J. B. Bell; M. S. Day; S. E. Woosley; M. Zingale

2008-11-17T23:59:59.000Z

154

Northern Illinois Gas Co IL  

Gasoline and Diesel Fuel Update (EIA)

Northern Northern Illinois Gas Co ............................ IL 254,574,988 4.60 Southern California Gas Co ...................... CA 233,632,354 6.89 Columbia Gas Dist Co............................... OH,KY,PA,MD 196,322,935 6.64 Pacific Gas and Elec Co............................ CA 190,864,262 5.83 Consumers Pwr Co ................................... MI 188,587,672 4.81 Michigan Consol Gas Co........................... MI 160,809,168 5.16 East Ohio Gas Co ..................................... OH 146,802,045 5.44 Pub Svc Elec and Gas Co......................... NJ 140,712,209 6.62 Peoples Gas Lt and Coke Co.................... IL 126,356,925 6.40 Brooklyn Union Gas Co............................. NY 106,349,594 9.43 Atlanta Gas Lt Co ...................................... GA 106,075,815 6.66 Lone Star Gas Co......................................

155

U-063: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

3: RSA SecurID Software Token for Windows DLL Loading Error 3: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code U-063: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code December 16, 2011 - 8:00am Addthis PROBLEM: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code. PLATFORM: RSA SecurID Software Token 4.1 for Microsoft Windows ABSTRACT: A remote user can cause the target application to execute arbitrary code on the target user's system. reference LINKS: SecurityTracker Alert ID: 1026426 ESA-2011-039 Secunia Advisory: SA45665 Securityfocus Advisory CVE-2011-4141 RSA Online Fraud Resource Center IMPACT ASSESSMENT: High Discussion: A vulnerability was reported in RSA SecurID Software Token. A remote user

156

U-063: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

63: RSA SecurID Software Token for Windows DLL Loading Error 63: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code U-063: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code December 16, 2011 - 8:00am Addthis PROBLEM: RSA SecurID Software Token for Windows DLL Loading Error Lets Remote Users Execute Arbitrary Code. PLATFORM: RSA SecurID Software Token 4.1 for Microsoft Windows ABSTRACT: A remote user can cause the target application to execute arbitrary code on the target user's system. reference LINKS: SecurityTracker Alert ID: 1026426 ESA-2011-039 Secunia Advisory: SA45665 Securityfocus Advisory CVE-2011-4141 RSA Online Fraud Resource Center IMPACT ASSESSMENT: High Discussion: A vulnerability was reported in RSA SecurID Software Token. A remote user

157

Institute of Development Studies (IDS) | Open Energy Information  

Open Energy Info (EERE)

Institute of Development Studies (IDS) Institute of Development Studies (IDS) Jump to: navigation, search Logo: Institute of Development Studies Name Institute of Development Studies Address Library Road, Brighton, East Sussex Place Brighton, UK Zip BN1 9RE Number of employees 201-500 Year founded 1966 Phone number +44 (0)1273 606261 Coordinates 50.8659583°, -0.0901136° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":50.8659583,"lon":-0.0901136,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

158

Microsoft PowerPoint - IEEE IAS PES 102313.pptx  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE's ARRA DOE's ARRA Smart Grid Program Steve Bossart, Senior Energy Analyst IEEE IAS/PES Pittsburgh Section October 23, 2013 ‹#› Topics * OE ARRA Smart Grid Program * OE ARRA Smart Grid Progress * Results and Case Studies * Life After ARRA Smart Grid ‹#› DOE OE ARRA Smart Grid Program ‹#› American Recovery and Reinvestment Act ($4.5B) * Smart Grid Investment Grants (99 projects) - $3.4 billion Federal; $4.7 billion private sector - > 800 PMUs covering almost 100% of transmission - ~ 8000 distribution automation circuits - > 15 million smart meters * Smart Grid Demonstration Projects (32 projects) - $685 million Federal; $1 billion private sector - 16 storage projects - 16 regional demonstrations Smart Grid ARRA Activities ‹#› Smart Grid investment from ARRA field projects

159

Type Ia Supernova: Burning and Detonation in the Distributed Regime  

E-Print Network (OSTI)

A simple, semi-analytic representation is developed for nuclear burning in Type Ia supernovae in the special case where turbulent eddies completely disrupt the flame. The speed and width of the ``distributed'' flame front are derived. For the conditions considered, the burning front can be considered as a turbulent flame brush composed of corrugated sheets of well-mixed flames. These flames are assumed to have a quasi-steady-state structure similar to the laminar flame structure, but controlled by turbulent diffusion. Detonations cannot appear in the system as long as distributed flames are still quasi-steady-state, but this condition is violated when the distributed flame width becomes comparable to the size of largest turbulent eddies. When this happens, a transition to detonation may occur. For current best estimates of the turbulent energy, the most likely density for the transition to detonation is in the range 0.5 - 1.5 x 10^7 g cm^{-3}.

S. E. Woosley

2007-09-26T23:59:59.000Z

160

DEPARThIl!NT OF ENERGY EERE PROJECT MANAGEMENT CENTER NllPA DEl'ER}.fiNATION  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DEPARThIl!NT OF ENERGY DEPARThIl!NT OF ENERGY EERE PROJECT MANAGEMENT CENTER NllPA DEl'ER}.fiNATION RECIPIENT:Cortiand County Business Development Corporation PROJE(.T TITLE : Energy Independent Agri-Business Outreach Page I of2 STATE: NY Funding Opportunity Announcement Number DE-EOOO3110 Procurement Instrument Number EEOOO3110 NEPA Control Number em Number GFO-10-573 0 Based on my review orlbe information concerning the proposed action, as N[PA Compliance Officer (autborized under DOE Order 4SI.IA),1 have made tbe follol'iing determination: ex, EA, EIS APPENDIX AND NUMBER: Description: A9 Information gathering (including, bul nollimiled 10, literature surveys. inventories, audits), data analysis (including computer modeling), document preparation (such as conceptual design or feasibility studies, analytical energy supply

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161

U.S. DEP.-\RTUENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERl\ilNATION  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

'""c-.-n. '""c-.-n. j!." OJ . U.S. DEP.-\RTUENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERl\ilNATION RECIPIENT:James Hardie Building Products PROJECT TITLE: XLD Reject Reclamation STATE: IL Page 1 of2 / ~ ~,' .' unding Opportunity AnnounCEment Number Procurement Instrument Numbu NEPA Control Number CID Number DE-FOA-OOOOOS2 EEOOOO119 GFO-1Q.-322 EE119 Baud on my rnitw oftht information concerning the proposed action, 85 NEPA Compliance Officer (authorized under DOE Order 451.IA), I have made the following determination: ex, EA, EIS APPENDIX AND NUMBER: Description: 85.1 Actions to conserve energy, demonstrate potential energy conservation, and promote energy-efficiency that do not increase the indoor concentrations of potentially harmful substances. These actions may involve financial and technical

162

C:\\ANNUAL\\VENTCHAP.V8\\NGA.VP  

Gasoline and Diesel Fuel Update (EIA)

4 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99...

163

C:\\ANNUAL\\VENTCHAP.V8\\NGAla1109.vp  

Gasoline and Diesel Fuel Update (EIA)

0 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Sources: Energy...

164

NGA98fin5.vp  

Annual Energy Outlook 2012 (EIA)

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99...

165

U-120: RSA SecurID Software Token Converter Unspecified Buffer Overflow  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

0: RSA SecurID Software Token Converter Unspecified Buffer 0: RSA SecurID Software Token Converter Unspecified Buffer Overflow Vulnerability U-120: RSA SecurID Software Token Converter Unspecified Buffer Overflow Vulnerability March 8, 2012 - 7:00am Addthis PROBLEM: RSA SecurID Software Token Converter Unspecified Buffer Overflow Vulnerability PLATFORM: RSA SecurID Software Token Converter 2.x ABSTRACT: Successful exploitation may allow execution of arbitrary code. reference LINKS: Secunia Advisory SA48297 CVE-2012-0397 IMPACT ASSESSMENT: High Discussion: A vulnerability has been reported in RSA SecurID Software Token Converter, which can be exploited by malicious people to compromise a user's system. Impact: An unspecified error can be exploited to cause a buffer overflow. Solution: Update to version 2.6.1. Addthis Related Articles

166

Type Ia Supernovae Rates and Galaxy Clustering from the CFHT Supernova Legacy Survey  

E-Print Network (OSTI)

The Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS) has created a large homogeneous database of intermediate redshift (0.2 rates, properties, and host galaxy star formation rates. The SNLS SN Ia database has now been combined with a photometric redshift galaxy catalog and an optical galaxy cluster catalog to investigate the possible influence of galaxy clustering on the SN Ia rate, over and above the expected effect due to the dependence of SFR on clustering through the morphology-density relation. We identify three cluster SNe Ia, plus three additional possible cluster SNe Ia, and find the SN Ia rate per unit mass in clusters at intermediate redshifts is consistent with the rate per unit mass in field early-type galaxies and the SN Ia cluster rate from low redshift cluster targeted surveys. We also find the number of SNe Ia in cluster environments to be within a factor of two of expectations from the two component SNIa rate model.

M. L. Graham; C. J. Pritchet; M. Sullivan; S. D. J. Gwyn; J. D. Neill; E. Y. Hsiao; P. Astier; D. Balam; C. Balland; S. Basa; R. G. Carlberg; A. Conley; D. Fouchez; J. Guy; D. Hardin; I. M. Hook; D. A. Howell; R. Pain; K. Perrett; N. Regnault; S. Baumont; J. Le Du; C. Lidman; S. Perlmutter; P. Ripoche; N. Suzuki; E. S. Walker; T. Zhang

2008-01-31T23:59:59.000Z

167

Microsoft Word - DOE-ID-INL-12-022.docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

IDAHO NATIONAL LABORATORY Page 1 of 3 CX Posting No.: DOE-ID-INL-12-022 SECTION A. Project Title: Radiological Dispersal Device (RDD)/Improvised Nuclear Device (IND) Material Training Activities and Evaluations Using Radiation Emitting Sources/Material/Devices - Overarching SECTION B. Project Description This Environmental Checklist (EC) will be an overarching EC for future training as described in this EC. Work Description The purpose of this overarching EC is to plan, prepare, coordinate, ship materials off-site, observe, and conduct training for response to radiological incidents at the Idaho National Laboratory (INL) locations and non-INL customer-hosted locations (such as Armed Forces installations). Only work performed at the INL is covered under this EC. Training at non-INL customer-hosted locations may be subject

168

Microsoft Word - DOE-ID-INL-13-008.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DOEID NEPA CX DETERMINATION DOEID NEPA CX DETERMINATION Idaho National Laboratory Page 1 of 2 EC Document No.: DOE-ID-INL-13-008 SECTION A. Project Title: Materials and Fuels Complex (MFC) Diversion Dam SECTION B. Project Description: There is a flood control dam about 2000 ft south of MFC. The dam is at risk of failure during a large runoff event. This project will reinforce the flood control dam with additional earthen material and a concrete headwall around the culvert inlet. The workscope consists of 1) Removing riprap from the existing slope around the culvert area. 2) Installing a concrete headwall structure around the culvert inlet. 3) Increase the slope of the dam at the culvert inlet and around the headwall to a 3:1 slope. 4) Replace riprap around headwall.

169

AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT I '. CONTRACT ID CODE  

National Nuclear Security Administration (NNSA)

SOLICITATIONIMODIFICATION OF CONTRACT I '. SOLICITATIONIMODIFICATION OF CONTRACT I '. CONTRACT ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, VA 24506 PAGE I OF 12 PAGES Albuquerque, NM 871 85-5400 I Amarillo, TX 79120 I I 90. DATED (SEE ITEM 1 1 ) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) I 10A. MODIFICATION OF CONTRACTIORDER NO. 2. AMENDMENT/MODIFICATION NO. MI67 9A. AMENDMENT OF SOLICITATION NO. I 1 DE-AC04-00AL66620 100. DATED (SEE ITEM 13) 3. EFFECTIVE DATE See Block 16C Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the

170

Microsoft Word - DOE-ID-INL-13-008.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

DOEID NEPA CX DETERMINATION DOEID NEPA CX DETERMINATION Idaho National Laboratory Page 1 of 2 EC Document No.: DOE-ID-INL-13-008 SECTION A. Project Title: Materials and Fuels Complex (MFC) Diversion Dam SECTION B. Project Description: There is a flood control dam about 2000 ft south of MFC. The dam is at risk of failure during a large runoff event. This project will reinforce the flood control dam with additional earthen material and a concrete headwall around the culvert inlet. The workscope consists of 1) Removing riprap from the existing slope around the culvert area. 2) Installing a concrete headwall structure around the culvert inlet. 3) Increase the slope of the dam at the culvert inlet and around the headwall to a 3:1 slope. 4) Replace riprap around headwall.

171

Material Safety Data Sheet MSDS ID NO.: 0137SPE012  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Material Safety Data Sheet Material Safety Data Sheet MSDS ID NO.: 0137SPE012 Revision date: 05/25/2011 1. CHEMICAL PRODUCT AND COMPANY INFORMATION Product name: Speedway E85 Synonym: Speedway ED75/ED85; E-75; E75; E-85; E85; Ethanol/Gasoline Fuel Blend; Fuel Ethanol ED75/ED85 Chemical Family: Gasoline/Ethanol Formula: Mixture Manufacturer: Speedway LLC P.O. Box 1500 Enon, OH 45501 Other information: 419-421-3070 Emergency telephone number: 877-627-5463 2. COMPOSITION/INFORMATION ON INGREDIENTS E85 is a mixture of ethyl alcohol and gasoline that is approved for use in an automobile spark ignition engine. Can contain small amounts of dye and other additives (>0.02%) which are not considered hazardous at the concentrations used. Product information: Name CAS Number

172

Microsoft Word - DOE-ID-INL-12-023.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Environmental Checklist Environmental Checklist Page 1 of 1 CX Posting No.: DOE-ID-INL-12-023 SECTION A. Project Title: Idaho Falls Power - Willow Creek Building (WCB) Conduit Installation SECTION B. Project Description: The purpose of this project is to provide the Idaho National Laboratory (INL) a communications pathway from the Willow Creek Building (WCB) northeast parking lot handhole to the handhole north of Research and Education Campus (REC)-617. INL and the City of Idaho Falls have an existing easement agreement that allows INL to place private telecommunications infrastructure in the City easement. Idaho Falls Power would provide and install a 1" conduit with pull rope for future INL use. Idaho Falls Power would provide and install a fiber patch panel, pull the fiber coiled in the WCB northeast parking lot handhole, and terminate and test the fiber to provide connectivity

173

Microsoft Word - DOE-ID_INL-13-010.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

0 0 SECTION A. Project Title: North Boulevard Annex Lease Termination SECTION B. Project Description: The proposed activity would terminate the current lease of the North Boulevard Annex (IF-613) at 2095 North Boulevard in Idaho Falls, ID on or about July 31, 2013 for cost savings and footprint reduction purposes. A facility walkthrough by BEA personnel will occur prior to the lease termination to ensure the facility is ready for turnover back to the owner. Approximate cost associated with these activities is estimated at $2,000.00. SECTION C. Environmental Aspects or Potential Sources of Impact: Generating and Managing Waste: Various quantities of industrial waste (non-hazardous, non-radioactive) such as office trash are removed from the building for pickup and transportation by garbage collection services prior to lease termination.

174

Microsoft Word - DOE-ID-INL-13-019.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

9 9 SECTION A. Project Title: University Boulevard Water Meter Installation SECTION B. Project Description: This project would install water meters for the purpose of measuring water use at each of four University Boulevard (UB) buildings at 535, 655, 625, and 595 University Boulevard (IF-680 (UB1), IF-681 (UB2), IF-682 (UB3), and IF-684 (UB4)) in Idaho Falls, ID during the projected time period of August and September, 2013 at an approximate cost of $20 K - $95 K depending upon whether the work can be completed from inside the building(s) or must be performed exterior to the building(s). SECTION C. Environmental Aspects or Potential Sources of Impact: Air Emissions: If excavation is required, the activity has the potential to generate fugitive dust. All reasonable precautions shall be

175

Microsoft Word - DOE-ID-INL-13-012.docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4 4 CX Posting No.: DOE-ID-INL-13-012 SECTION A. Project Title: Water Security Test Bed (WSTB) SECTION B. Project Description: This project was extensively described in Environmental Checklists (ECs) Idaho National Laboratory (INL)-13-014 (Overarching [OA] 5) and INL-13-014 Revision (R) 1 (OA 5). Upon review, it was determined that additional planning and detail was required to fully describe the project and associated activities. Both INL-13-014 and R1 to that EC are canceled; this EC will replace them. Future revisions may address additional project details regarding design, construction, and operational details and limitations as they become known through the project planning process. Background Since its inception, the Environmental Protection Agency's (EPA) Homeland Security Research Program (Sponsor) has been providing

176

Microsoft Word - DOE-ID-INL-13-006.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 EC Document No.: DOE-ID-INL-13-006 SECTION A. Project Title: Power Line Configuration 2013-1 SECTION B. Project Description: This project will install temporary distribution-level power lines between Materials and Fuels Complex (MFC) and Critical Infrastructure Test Range Complex (CITRC) to support research and development and testing using electric power infrastructure. Two circuits of three-phase distribution lines will be installed from Power Burst Facility (PBF)-613 to the MFC test pad. Standard new crossarms and insulators will be installed on the existing 138kV H structures (underbuild) to support standard aluminum conductors steel reinforced (ACSR) conductors for the majority of the configuration change (approximately from Pole 40E to Pole 127E - an

177

Microsoft Word - DOE-ID-INL-12-022.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

IDAHO NATIONAL LABORATORY Page 1 of 3 CX Posting No.: DOE-ID-INL-12-022 SECTION A. Project Title: Radiological Dispersal Device (RDD)/Improvised Nuclear Device (IND) Material Training Activities and Evaluations Using Radiation Emitting Sources/Material/Devices - Overarching SECTION B. Project Description This Environmental Checklist (EC) will be an overarching EC for future training as described in this EC. Work Description The purpose of this overarching EC is to plan, prepare, coordinate, ship materials off-site, observe, and conduct training for response to radiological incidents at the Idaho National Laboratory (INL) locations and non-INL customer-hosted locations (such as Armed Forces installations). Only work performed at the INL is covered under this EC. Training at non-INL customer-hosted locations may be subject

178

IdJOO2 UNITED STATES ENVIRONMENTAL PROTECTION AGENCY  

NLE Websites -- All DOE Office Websites (Extended Search)

6/2004 13:39 FAX 6/2004 13:39 FAX IdJOO2 UNITED STATES ENVIRONMENTAL PROTECTION AGENCY WASHINGTON, D.C. 20460 MAR 26 2004 OFFICE OF AIR AND RADIATION R. Paul Detwiler, Acting Manager Carlsbad Field Office U.S. Department of Energy P.O. Box 3090 Carlsbad, NM 88221-3090 Dear Dr. Detwiler: This letter announces the U.S. Environmental Protection Agency's (EPA's) final decision to approve the Department of Energy's (DOE's) remote handled (RH) transuranic (TRU) Waste Characterization Program Implementation Plan (WCPIP), Revision aD, and the RH TRU Waste Characterization Plan for the Waste Isolation Pilot Plant (WIPP). We have detenDined that these documents provide an adeql.late general framework for the characterization ofRH waste for disposal at WIPP, while allowing flexibility for DOE to develop characterization programs

179

Microsoft Word - DOE-ID-INL-13-022.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

Idaho National Laboratory Idaho National Laboratory Page 1 of 2 CX Posting No.: DOE-ID-INL-13-022 SECTION A. Project Title: Global Threat Reduction Initiative (GTRI) Irradiated Experiment Shipping Capability SECTION B. Project Description: The General Electric (GE) 2000 Model Cask is currently used to support the Global Threat Reduction Initiative (GTRI) irradiated experiment shipments from the Advanced Test Reactor (ATR) at Idaho National Laboratory's (INL) ATR Complex to the Hot Fuel Examination Facility (HFEF) at INL's Materials and Fuels Complex (MFC). However, due to changes in GE-Hitachi's business model, the continued availability of the GE Model 2000 cask is not guaranteed. Furthermore, the internal cavity of the GE Model 2000 cask is too short to support shipment of some larger GTRI experiments. The purpose of the proposed action is to develop and implement a

180

Microsoft Word - DOE-ID-INL-12-023.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

Environmental Checklist Environmental Checklist Page 1 of 1 CX Posting No.: DOE-ID-INL-12-023 SECTION A. Project Title: Idaho Falls Power - Willow Creek Building (WCB) Conduit Installation SECTION B. Project Description: The purpose of this project is to provide the Idaho National Laboratory (INL) a communications pathway from the Willow Creek Building (WCB) northeast parking lot handhole to the handhole north of Research and Education Campus (REC)-617. INL and the City of Idaho Falls have an existing easement agreement that allows INL to place private telecommunications infrastructure in the City easement. Idaho Falls Power would provide and install a 1" conduit with pull rope for future INL use. Idaho Falls Power would provide and install a fiber patch panel, pull the fiber coiled in the WCB northeast parking lot handhole, and terminate and test the fiber to provide connectivity

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

Microsoft Word - DOE-ID-INL-12-006.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

6 6 SECTION A. Project Title: International Way Office Building Lease Termination SECTION B. Project Description: The proposed activity will terminate the current lease of the International Way Office Building (IF-674, IWB) at 1690 International Way in Idaho Falls, ID on or about March 28, 2012 for cost savings and footprint reduction purposes. A facility walkthrough by BEA personnel will occur on or about March 26 to ensure the building is ready for turnover back to the owner. Approximate cost associated with these activities is estimated at $2,500.00. SECTION C. Environmental Aspects / Potential Sources of Impact: Generating and Managing Waste: Small amounts of industrial waste (non-hazardous, non-radioactive) such as office trash are

182

Automatic ID heat load generation in ANSYS code  

SciTech Connect

Detailed power density profiles are critical in the execution of a thermal analysis using a finite element (FE) code such as ANSYS. Unfortunately, as yet there is no easy way to directly input the precise power profiles into ANSYS. A straight-forward way to do this is to hand-calculate the power of each node or element and then type the data into the code. Every time a change is made to the FE model, the data must be recalculated and reentered. One way to solve this problem is to generate a set of discrete data, using another code such as PHOTON2, and curve-fit the data. Using curve-fitted formulae has several disadvantages. It is time consuming because of the need to run a second code for generation of the data, curve-fitting, and doing the data check, etc. Additionally, because there is no generality for different beamlines or different parameters, the above work must be repeated for each case. And, errors in the power profiles due to curve-fitting result in errors in the analysis. To solve the problem once and for all and with the capability to apply to any insertion device (ID), a program for ED power profile was written in ANSYS Parametric Design Language (APDL). This program is implemented as an ANSYS command with input parameters of peak magnetic field, deflection parameter, length of ID, and distance from the source. Once the command is issued, all the heat load will be automatically generated by the code.

Wang, Zhibi

1992-04-30T23:59:59.000Z

183

Idaho National Laboratory Supervisory Control and Data Acquisition Intrusion Detection System (SCADA IDS)  

SciTech Connect

Current Intrusion Detection System (IDS) technology is not suited to be widely deployed inside a Supervisory, Control and Data Acquisition (SCADA) environment. Anomaly- and signature-based IDS technologies have developed methods to cover information technology-based networks activity and protocols effectively. However, these IDS technologies do not include the fine protocol granularity required to ensure network security inside an environment with weak protocols lacking authentication and encryption. By implementing a more specific and more intelligent packet inspection mechanism, tailored traffic flow analysis, and unique packet tampering detection, IDS technology developed specifically for SCADA environments can be deployed with confidence in detecting malicious activity.

Jared Verba; Michael Milvich

2008-05-01T23:59:59.000Z

184

A Role for Id-1 in the Aggressive Phenotype and Steroid ...  

Desprez, P. Y., Hara E., Bissell, M. J., and Campisi, J. Suppression of mammary epithelial cell differentiation by the helix-loop-helix protein Id-1. Mol. Cell.

185

Fitting Type Ia supernovae with coupled dark energy  

E-Print Network (OSTI)

We discuss the possible consistency of the recently discovered Type Ia supernovae at z>1 with models in which dark energy is strongly coupled to a significant fraction of dark matter, and in which an (asymptotic) accelerated phase exists where dark matter and dark energy scale in the same way. Such a coupling has been suggested for a possible solution of the coincidence problem, and is also motivated by string cosmology models of "late time" dilaton interactions. Our analysis shows that, for coupled dark energy models, the recent data are still consistent with acceleration starting as early as at $z=3$ (to within 90% c.l.), although at the price of a large "non-universality" of the dark energy coupling to different matter fields. Also, as opposed to uncoupled models which seem to prefer a ``phantom'' dark energy, we find that a large amount of coupled dark matter is compatible with present data only if the dark energy field has a conventional equation of state w>-1.

Amendola, L; Piazza, F; Amendola, Luca; Gasperini, Maurizio; Piazza, Federico

2004-01-01T23:59:59.000Z

186

Mtrologie des supernovae de type Ia pour la cosmologie : instrumentation et analyse calorimtrique.  

E-Print Network (OSTI)

??L'utilisation des supernovae de type Ia comme indicateurs de distance est un pilier du modle de concordance actuel en cosmologie. Le travail d'instrumentation prsent dans (more)

Juramy, Claire

2006-01-01T23:59:59.000Z

187

Toward Exascale Computing of Type Ia and Ib,c Supernovae: V&V...  

NLE Websites -- All DOE Office Websites (Extended Search)

Toward Exascale Computing of Type Ia and Ib,c Supernovae: V&V of Current Models PI Name: Don Lamb PI Email: lamb@oddjob.uchicago.edu Institution: University Of Chicago Allocation...

188

Last Revision Date: 8/16/2010 Last Merged Filing ID:  

NLE Websites -- All DOE Office Websites (Extended Search)

Revision Date: 8/16/2010 Last Merged Filing ID: Revision Date: 8/16/2010 Last Merged Filing ID: Tariffs, Rate Schedules, and Other Tariff Documents Southwestern Power Administration Tariffs, Rate Schedules, and Other Tariff Documents Document Generated On: 10/1/2010 Contents TABLE OF CONTENTS ....................................................................................................................................1 PREAMBLE: AUTHORITIES AND OBLIGATIONS .............................................................................................1

189

SAT(ID): satisfiability of propositional logic extended with inductive definitions  

Science Conference Proceedings (OSTI)

We investigate the satisfiability problem, SAT(ID), of an extension of propositional logic with inductive definitions. We demonstrate how to extend existing SAT solvers to become SAT(ID) solvers, and provide an implementation on top of MiniSat. We also ...

Maarten Marin; Johan Wittocx; Marc Denecker; Maurice Bruynooghe

2008-05-01T23:59:59.000Z

190

Diversity of supernovae Ia determined using equivalent widths of Si II 4000  

E-Print Network (OSTI)

Spectroscopic and photometric properties of low and high-z supernovae Ia (SNe Ia) have been analyzed in order to achieve a better understanding of their diversity and to identify possible SN Ia sub-types. We use wavelet transformed spectra in which one can easily measure spectral features. We investigate the \\ion{Si}{II} 4000 equivalent width ($EW_w\\lbrace\\ion{Si}{II}\\rbrace$). The ability and, especially, the ease in extending the method to SNe at high-$z$ is demonstrated. We applied the method to 110 SNe Ia and found correlations between $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ and parameters related to the light-curve shape for 88 supernovae with available photometry. No evidence for evolution of $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ with redshift is seen. Three sub-classes of SNe Ia were confirmed using an independent cluster analysis with only light-curve shape, colour, and $EW_w\\lbrace\\ion{Si}{II}\\rbrace$. SNe from high-$z$ samples seem to follow a similar grouping to nearby objects. The $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ value measured on a single spectrum may point towards SN Ia sub-classification, avoiding the need for expansion velocity gradient calculations.

V. Arsenijevic; S. Fabbro; A. M. Mourao; A. J. Rica da Silva

2008-09-18T23:59:59.000Z

191

DOE - Office of Legacy Management -- Madison - IL 26  

Office of Legacy Management (LM)

Madison - IL 26 Madison - IL 26 FUSRAP Considered Sites Madison, IL Alternate Name(s): Spectrulite Consortium, Inc. Former Dow Chemical Company Site IL.26-3 IL.26-4 Location: Intersection of College and Weaver Streets, Madison, Illinois IL.26-4 Historical Operations: Conducted experimental work in natural uranium metal extrusion. IL.26-4 IL.26-5 Eligibility Determination: Eligible IL.26-1 IL.26-2 Radiological Survey(s): Assessment Survey, Verification Survey IL.26-4 LTSM00011565 LTSM00013029 LTSM00011563 Site Status: Cleanup Complete LTSM00011565 Long-term Care Requirements: Long-Term Surveillance and Maintenance Requirements for Remediated FUSRAP Sites S07566_FUSRAP Also see Madison, Illinois, Site Documents Related to Madison, IL FACT SHEET The Madison, Illinois, Site is located northeast of and

192

T-642: RSA SecurID update to Customers | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

2: RSA SecurID update to Customers 2: RSA SecurID update to Customers T-642: RSA SecurID update to Customers June 9, 2011 - 12:45am Addthis PROBLEM: Certain characteristics of the attack on RSA indicated that the perpetrator's most likely motive was to obtain an element of security information that could be used to target defense secrets and related IP, rather than financial gain, PII, or public embarrassment. PLATFORM: RSA SecurID implementations ABSTRACT: RSA investigation has revealed that the attack resulted in certain information being extracted from RSA's systems. Some of that information is related to RSA's SecurID two-factor authentication products. reference LINKS: Open Letter to RSA Customers (update) CVE-2011-0322 RSA Fraud Resource Center RSA Security Practice DOE-CIRC T-640: RSA Access Manager Server CVE-2011-0322 Update

193

GRR/Section 3-ID-d - Land Use Permit | Open Energy Information  

Open Energy Info (EERE)

d - Land Use Permit d - Land Use Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 3-ID-d - Land Use Permit 03-ID-d - Land Use Permit.pdf Click to View Fullscreen Contact Agencies Idaho Department of Lands Triggers None specified Click "Edit With Form" above to add content 03-ID-d - Land Use Permit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Lands issues Land Use Permits for non-invasive exploration on a case by case basis. 3-ID-d.1 to 3-ID-d.2 - Will Non-Invasive Exploration Be Preformed on State Lands? A Land Use Permit is required to preform non-invasive exploration on state

194

Finding Utility Companies Under a Given Utility ID | OpenEI Community  

Open Energy Info (EERE)

Finding Utility Companies Under a Given Utility ID Finding Utility Companies Under a Given Utility ID Home > Groups > Developer Jayhuggins's picture Submitted by Jayhuggins(15) Member 22 June, 2012 - 09:39 Utility+Utility Access Map Here's a quick way to find all the utility company pages under a given utility id. From the Special Ask page, in the query box enter the following: [[Category:Utility Companies]][[EiaUtilityId::15248]] substituting your utility id of interest for 15248, and click "Find results". Groups: Developer Login to post comments Jayhuggins's blog Latest blog posts Rmckeel The utility rate database version 1 API is now deprecated Posted: 6 Sep 2013 - 14:00 by Rmckeel Jweers New Robust References! Posted: 7 Aug 2013 - 18:23 by Jweers 1 comment(s) 1 of 10 ›› Groups Menu You must login in order to post into this group.

195

AMENDMENT OF SOLICITATIONIMODIFICATION OF CONTRACT I '. CONTRACT ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

I '. I '. CONTRACT ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, VA 24506 PAGE I OF 12 PAGES Albuquerque, NM 871 85-5400 I Amarillo, TX 79120 I I 90. DATED (SEE ITEM 1 1 ) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) I 10A. MODIFICATION OF CONTRACTIORDER NO. 2. AMENDMENT/MODIFICATION NO. MI67 9A. AMENDMENT OF SOLICITATION NO. I 1 DE-AC04-00AL66620 100. DATED (SEE ITEM 13) 3. EFFECTIVE DATE See Block 16C Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

196

DOE - Office of Legacy Management -- Podbeilniac Corp - IL 22  

Office of Legacy Management (LM)

Podbeilniac Corp - IL 22 Podbeilniac Corp - IL 22 FUSRAP Considered Sites Site: PODBEILNIAC CORP. (IL.22) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Chicago , Illinois IL.22-1 Evaluation Year: 1990 IL.22-2 Site Operations: MED used equipment for a uranium extraction experiment in 1957. IL.22-1 Site Disposition: Eliminated - Potential for contamination considered remote due to limited scope of activities performed at the site IL.22-2 IL.22-3 IL.22-4 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IL.22-1 Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to PODBEILNIAC CORP. IL.22-1 - Report, Ross to Quigley; Trip Report to Podbeilniac Corp.,

197

DOE - Office of Legacy Management -- Fansteel Metallurgical Corp - IL 16  

NLE Websites -- All DOE Office Websites (Extended Search)

Fansteel Metallurgical Corp - IL 16 Fansteel Metallurgical Corp - IL 16 FUSRAP Considered Sites Site: Fansteel Metallurgical Corp. (IL.16 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Chicago , Illinois IL.16-1 Evaluation Year: 1987 IL.16-3 Site Operations: Sole producer and supplier of tantalum and columbium metals to the MED. IL.16-1 IL.16-3 Site Disposition: Eliminated - No radioactive materials handled at this site IL.16-2 IL.16-3 Radioactive Materials Handled: No Primary Radioactive Materials Handled: None IL.16-2 Radiological Survey(s): No Site Status: Eliminated from further consideration under FUSRAP Also see Documents Related to Fansteel Metallurgical Corp. IL.16-1 - MED Memorandum; Greninger to the File; Subject: Visit to

198

Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra  

SciTech Connect

We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispersion using high signal-to-noise ratio Keck-I/LRIS-B spectroscopy for a sample of 36 events at intermediate redshift (z=0.5) discovered by the Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS). We introduce a new method for removing host galaxy contamination in our spectra, exploiting the comprehensive photometric coverage of the SNLS SNe and their host galaxies, thereby providing the first quantitative view of the UV spectral properties of a large sample of distant SNe Ia. Although the mean SN Ia spectrum has not evolved significantly over the past 40percent of cosmic history, precise evolutionary constraints are limited by the absence of a comparable sample of high-quality local spectra. The mean UV spectrum of our z~;;=0.5 SNe Ia and its dispersion is tabulated for use in future applications. Within the high-redshift sample, we discover significant UV spectral variations and exclude dust extinction as the primary cause by examining trends with the optical SN color. Although progenitor metallicity may drive some of these trends, the variations we see are much larger than predicted in recent models and do not follow expected patterns. An interesting new result is a variation seen in the wavelength of selected UV features with phase. We also demonstrate systematic differences in the SN Ia spectral features with SN light curve width in both the UV and the optical. We show that these intrinsic variations could represent a statistical limitation in the future use of high-redshift SNe Ia for precision cosmology. We conclude that further detailed studies are needed, both locally and at moderate redshift where the rest-frame UV can be studied precisely, in order that future missions can confidently be planned to fully exploit SNe Ia as cosmological probes.

Nugent, Peter E; Ellis, R.S.; Sullivan, M.; Nugent, P.E.; Howell, D.A.; Gal-Yam, A.; Astier, P.; Balam, D.; Balland, C.; Basa, S.; Carlberg, R.; Conley, A.; Fouchez, D.; Guy, J.; Hardin, D.; Hook, I.; Pain, R.; Perrett, K.; Pritchet, C.J.; Regnault, N.

2008-02-28T23:59:59.000Z

199

THE FIRST MAXIMUM-LIGHT ULTRAVIOLET THROUGH NEAR-INFRARED SPECTRUM OF A TYPE Ia SUPERNOVA  

Science Conference Proceedings (OSTI)

We present the first maximum-light ultraviolet (UV) through near-infrared (NIR) Type Ia supernova (SN Ia) spectrum. This spectrum of SN 2011iv was obtained nearly simultaneously by the Hubble Space Telescope at UV/optical wavelengths and the Magellan Baade telescope at NIR wavelengths. These data provide the opportunity to examine the entire maximum-light SN Ia spectral energy distribution. Since the UV region of an SN Ia spectrum is extremely sensitive to the composition of the outer layers of the explosion, which are transparent at longer wavelengths, this unprecedented spectrum can provide strong constraints on the composition of the SN ejecta, and similarly the SN explosion and progenitor system. SN 2011iv is spectroscopically normal, but has a relatively fast decline ({Delta}m{sub 15}(B) = 1.69 {+-} 0.05 mag). We compare SN 2011iv to other SNe Ia with UV spectra near maximum light and examine trends between UV spectral properties, light-curve shape, and ejecta velocity. We tentatively find that SNe with similar light-curve shapes but different ejecta velocities have similar UV spectra, while those with similar ejecta velocities but different light-curve shapes have very different UV spectra. Through a comparison with explosion models, we find that both a solar-metallicity W7 and a zero-metallicity delayed-detonation model provide a reasonable fit to the spectrum of SN 2011iv from the UV to the NIR.

Foley, Ryan J.; Marion, G. Howie; Challis, Peter; Kirshner, Robert P.; Berta, Zachory K. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kromer, Markus; Taubenberger, Stefan; Hillebrandt, Wolfgang; Roepke, Friedrich K.; Ciaraldi-Schoolmann, Franco; Seitenzahl, Ivo R. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, D-85748 Garching bei Muenchen (Germany); Pignata, Giuliano [Departamento de Ciencias Fisicas, Universidad Andres Bello, Avda. Republica 252, Santiago (Chile); Stritzinger, Maximilian D. [Department of Physics and Astronomy, Aarhus University, Ny Munkegade, DK-8000 Aarhus C (Denmark); Filippenko, Alexei V.; Li Weidong; Silverman, Jeffrey M. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Folatelli, Gaston [Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa 277-8583 (Japan); Hsiao, Eric Y.; Morrell, Nidia I. [Carnegie Observatories, Las Campanas Observatory, La Serena (Chile); Simcoe, Robert A., E-mail: rfoley@cfa.harvard.edu [MIT-Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, 37-664D Cambridge, MA 02139 (United States); and others

2012-07-01T23:59:59.000Z

200

DOE - Office of Legacy Management -- Precision Extrusion Co - IL 20  

NLE Websites -- All DOE Office Websites (Extended Search)

Precision Extrusion Co - IL 20 Precision Extrusion Co - IL 20 FUSRAP Considered Sites Site: PRECISION EXTRUSION CO. (IL.20) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: 720 East Green Avenue , Bensenville , Illinois IL.20-1 Evaluation Year: 1987 IL.20-2 Site Operations: 1956-1959, metal fabrication - extruded uranium billets. IL.20-1 Site Disposition: Eliminated - Potential for contamination considered remote based on limited quantities of materials handled at the site IL.20-2 Radioactive Materials Handled: Yes IL.20-1 Primary Radioactive Materials Handled: Uranium IL.20-1 Radiological Survey(s): Yes IL.20-3 Site Status: Eliminated from further consideration under FUSRAP Also see Documents Related to PRECISION EXTRUSION CO.

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

GRR/Section 8-ID-a - State Transmission | Open Energy Information  

Open Energy Info (EERE)

8-ID-a - State Transmission 8-ID-a - State Transmission < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 8-ID-a - State Transmission 08IDAStateTransmission.pdf Click to View Fullscreen Contact Agencies Idaho Public Utilities Commission Regulations & Policies IC §67-6508: Local Land Use Planning Duties IC §61-526: Certificate of Public Convenience and Necessity Triggers None specified Click "Edit With Form" above to add content 08IDAStateTransmission.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative 8-ID-a.1 - Will the Transmission Project Be Undertaken by a Public Utility?

202

GRR/Section 6-ID-b - Construction Storm Water Permit | Open Energy  

Open Energy Info (EERE)

6-ID-b - Construction Storm Water Permit 6-ID-b - Construction Storm Water Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 6-ID-b - Construction Storm Water Permit 06IDBConstructionStormwaterPermit.pdf Click to View Fullscreen Contact Agencies United States Environmental Protection Agency Triggers None specified Click "Edit With Form" above to add content 06IDBConstructionStormwaterPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative 6-ID-b.1 - EPA Construction General Permit Idaho does not have authority from the United States Environmental Protection Agency to issue a construction storm water permit. See Flowchart

203

GRR/Section 1-ID-a - Land Use Considerations | Open Energy Information  

Open Energy Info (EERE)

GRR/Section 1-ID-a - Land Use Considerations GRR/Section 1-ID-a - Land Use Considerations < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 1-ID-a - Land Use Considerations 01IDALandUseConsiderations.pdf Click to View Fullscreen Triggers None specified Click "Edit With Form" above to add content 01IDALandUseConsiderations.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Add Text Print PDF Retrieved from "http://en.openei.org/w/index.php?title=GRR/Section_1-ID-a_-_Land_Use_Considerations&oldid=685536" Categories: Regulatory Roadmap State Sections Geothermal Regulatory Roadmap Sections

204

Comments on Docket ID: DOE-HQ-2011-0014 | Department of Energy  

NLE Websites -- All DOE Office Websites (Extended Search)

on Docket ID: DOE-HQ-2011-0014 on Docket ID: DOE-HQ-2011-0014 Comments on Docket ID: DOE-HQ-2011-0014 This letter comprises the comments of the Pacific Gas and Electric Company (PG&E), Southern California Gas Company (SCGC), San Diego Gas and Electric (SDG&E), and Southern California Edison (SCE) in response to the U.S. Department of Energy's (DOE) Request for Information on Regulatory Burden. The signatories of this letter, collectively referred to herein as the California Investor Owned Utilities (CA IOUs) represent some of the largest utility companies in the Western United States, serving over 35 million customers. Comments on Docket ID: DOE-HQ-2011-0014 More Documents & Publications FINAL CA IOU Comment Letter RFI Regulatory Burden O:\IM-20\E-Government Program Office\FDMS\FDMS

205

GRR/Section 4-ID-a - State Exploration Process | Open Energy Information  

Open Energy Info (EERE)

4-ID-a - State Exploration Process 4-ID-a - State Exploration Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 4-ID-a - State Exploration Process 04IDAStateExplorationProcess.pdf Click to View Fullscreen Contact Agencies Idaho Department of Water Resources Triggers None specified Click "Edit With Form" above to add content 04IDAStateExplorationProcess.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative _ 4-ID-a.1 - Has the Environmental Process been Completed for Exploration? If an EA/EIS has not yet been completed for this portion of the project, the developer must first complete the applicable environmental process.

206

Comments on Docket ID: DOE-HQ-2011-0014 | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Comments on Docket ID: DOE-HQ-2011-0014 Comments on Docket ID: DOE-HQ-2011-0014 Comments on Docket ID: DOE-HQ-2011-0014 This letter comprises the comments of the Pacific Gas and Electric Company (PG&E), Southern California Gas Company (SCGC), San Diego Gas and Electric (SDG&E), and Southern California Edison (SCE) in response to the U.S. Department of Energy's (DOE) Request for Information on Regulatory Burden. The signatories of this letter, collectively referred to herein as the California Investor Owned Utilities (CA IOUs) represent some of the largest utility companies in the Western United States, serving over 35 million customers. Comments on Docket ID: DOE-HQ-2011-0014 More Documents & Publications FINAL CA IOU Comment Letter RFI Regulatory Burden O:\IM-20\E-Government Program Office\FDMS\FDMS

207

Microsoft Word - 2013 (05-22-13) DOE-ID Operations Summary-13...  

NLE Websites -- All DOE Office Websites (Extended Search)

was restored to the E-3 diesel bus from commercial power, and equipment lost due to the power outage was restored. NE-ID--BEA-ATR-2013-0012 3 April 17: (Notification) As a...

208

RL-721 Document ID Number: REV4 NEPA REVIEW SCREENING FORM  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

of InitiatorEGO signed NRSF to DOE NCO for information only. DOE NCO Page 1 of2 RL-721 Document ID Number: REV4 NEPA REVIEW SCREENING FORM (continued) DOECX-00126, Rev 0 V....

209

RL-721 REV4 Document ID Number: NEPA REVIEW SCREENING FORM  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

9405630, HCRC2003-200-044, & DOERL-97-56 R1 Additional Attachments: Page 1 of 2 RL-721 Document ID Number: REV4 NEPA REVIEW SCREENING FORM (continued) DOECX-00094 Rev 0 IV....

210

(SE-33)Intelligent ID-Based threshold system by an encryption and decryption from bilinear pairing  

Science Conference Proceedings (OSTI)

We suggest a new intelligent ID-based threshold secure system by an encryption and decryption protocol using (k, n)-threshold scheme which only k agents or more are engaged to reconstruct an encrypted data for a mobile intelligent ...

Young Whan Lee; Byung Mun Choi

2005-09-01T23:59:59.000Z

211

Microsoft Word - 2013 (05-22-13) DOE-ID Operations Summary-13...  

NLE Websites -- All DOE Office Websites (Extended Search)

May 16, 2013 DOE-ID Operations Summary For the Period April 1 to May 16, 2013 EDITOR'S NOTE: The following is a summary of contractor operations at the Idaho National Laboratory,...

212

GRR/Section 14-ID-d - Section 401 Water Quality Certification...  

Open Energy Info (EERE)

GRRSection 14-ID-d - Section 401 Water Quality Certification Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of...

213

Spectral Modeling of SNe Ia Near Maximum Light: Probing the Characteristics of Hydro Models  

E-Print Network (OSTI)

We have performed detailed NLTE spectral synthesis modeling of 2 types of 1-D hydro models: the very highly parameterized deflagration model W7, and two delayed detonation models. We find that overall both models do about equally well at fitting well observed SNe Ia near to maximum light. However, the Si II 6150 feature of W7 is systematically too fast, whereas for the delayed detonation models it is also somewhat too fast, but significantly better than that of W7. We find that a parameterized mixed model does the best job of reproducing the Si II 6150 line near maximum light and we study the differences in the models that lead to better fits to normal SNe Ia. We discuss what is required of a hydro model to fit the spectra of observed SNe Ia near maximum light.

E. Baron; S. Bongard; David Branch; Peter H. Hauschildt

2006-03-03T23:59:59.000Z

214

IL.06-123 057 I I  

Office of Legacy Management (LM)

IL.06-123 057 I I IL.06-123 057 I I 7 Bechtel National. Inc Systems Engmeers - Constructors Jackson Plaza Tower e 800 Oak Ridge Turnpike Oak Ridge. Tennessee 37830 AII.il Addr.u P.O 80.350. 0.' R,dg_. 7N 3713' .0350 7.'-. 3785873 NOV 1 5 . . u.s. Department of Energy Oak Ridge Operations Post Office Box E Oak Ridge, Tennessee 37831 Attention: Peter J. Gross, Director Technical Services Division Subject: Bechtel Job No. 14501, FUSRAP Project DOE Contract No. DE-AC05-810R20722 Revised Letter Characterization Report for the George Herbert Jones Chemical Laboratory at the Unive sity of Chicago Site, Chicago, Illinois Code: 7330/WBS: 131 Dear Mr. Gross: Radiological characterization and remedial action activities were performed by Bechtel National, Inc. (BNI) at George

215

THE LOW-VELOCITY, RAPIDLY FADING TYPE Ia SUPERNOVA 2002es  

SciTech Connect

SN 2002es is a peculiar subluminous Type Ia supernova (SN Ia) with a combination of observed characteristics never before seen in an SN Ia. At maximum light, SN 2002es shares spectroscopic properties with the underluminous SN 1991bg subclass of SNe Ia, but with substantially lower expansion velocities ({approx}6000 km s{sup -1}) more typical of the peculiar SN 2002cx subclass. Photometrically, SN 2002es differs from both SN 1991bg-like and SN 2002cx-like supernovae. Although at maximum light it is subluminous (M{sub B} = -17.78 mag), SN 2002es has a relatively broad light curve ({Delta}m{sub 15}(B) = 1.28 {+-} 0.04 mag), making it a significant outlier in the light-curve width versus luminosity relationship. We estimate a {sup 56}Ni mass of 0.17 {+-} 0.05 M{sub Sun} synthesized in the explosion, relatively low for an SN Ia. One month after maximum light, we find an unexpected plummet in the bolometric luminosity. The late-time decay of the light curves is inconsistent with our estimated {sup 56}Ni mass, indicating that either the light curve was not completely powered by {sup 56}Ni decay or the ejecta became optically thin to {gamma}-rays within a month after maximum light. The host galaxy is classified as an S0 galaxy with little to no star formation, indicating that the progenitor of SN 2002es is likely from an old stellar population. We also present a less extensive data set for SN 1999bh, an object which shares similar photometric and spectroscopic properties. Both objects were found as part of the Lick Observatory Supernova Search, allowing us to estimate that these objects should account for 2.5% of SNe Ia within a fixed volume. Current theoretical models are unable to explain the observed characteristics of SN 2002es.

Ganeshalingam, Mohan; Li Weidong; Filippenko, Alexei V.; Silverman, Jeffrey M.; Shen, Ken J. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Chornock, Ryan; Foley, Ryan J.; Kirshner, Robert P.; Calkins, Mike [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Matheson, Thomas [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Milne, Peter, E-mail: mganesh@astro.berkeley.edu [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)

2012-06-01T23:59:59.000Z

216

EARLY PHASE OBSERVATIONS OF EXTREMELY LUMINOUS TYPE Ia SUPERNOVA 2009dc  

Science Conference Proceedings (OSTI)

We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is DELTAm{sub 15}(B) = 0.65 +- 0.03, which is one of the slowest among SNe Ia. The peak V-band absolute magnitude is estimated to be M{sub V} = -19.90 +- 0.15 mag if no host extinction is assumed. It reaches M{sub V} = -20.19 +- 0.19 mag if we assume the host extinction of A{sub V} = 0.29 mag. SN 2009dc belongs to the most luminous class of SNe Ia, like SNe 2003fg and 2006gz. Our JHK{sub s} -band photometry shows that this SN is also one of the most luminous SNe Ia in near-infrared wavelengths. We estimate the ejected {sup 56}Ni mass of 1.2 +- 0.3 M{sub sun} for the no host extinction case (and of 1.6 +- 0.4 M{sub sun} for the host extinction of A{sub V} = 0.29 mag). The C II lambda6580 absorption line remains visible until a week after the maximum brightness, in contrast to its early disappearance in SN 2006gz. The line velocity of Si II lambda6355 is about 8000 km s{sup -1} around the maximum, being considerably slower than that of SN 2006gz. The velocity of the C II line is similar to or slightly less than that of the Si II line around the maximum. The presence of the carbon line suggests that the thick unburned C+O layer remains after the explosion. Spectropolarimetric observations by Tanaka et al. indicate that the explosion is nearly spherical. These observational facts suggest that SN 2009dc is a super-Chandrasekhar mass SN Ia.

Yamanaka, M.; Arai, A.; Chiyonobu, S.; Fukazawa, Y.; Ikejiri, Y.; Itoh, R.; Komatsu, T.; Miyamoto, H. [Department of Physical Science, Hiroshima University, Kagamiyama 1-3-1, Higashi-Hiroshima 739-8526 (Japan); Kawabata, K. S. [Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Kinugasa, K.; Hashimoto, O.; Honda, S. [Gunma Astronomical Observatory, Takayama, Gunma 377-0702 (Japan); Tanaka, M. [Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan); Imada, A.; Kuroda, D. [Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata, Asakuchi-shi, Okayama 719-0232 (Japan); Maeda, K.; Nomoto, K. [Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa (Japan); Kamata, Y. [National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588 (Japan); Kawai, N. [Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Konishi, K., E-mail: myamanaka@hiroshima-u.ac.j [Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa, Chiba, 277-8582 (Japan)

2009-12-20T23:59:59.000Z

217

International Degree (ID) and Engineering For complete information and admission requirements for the ID, refer to the "Passport to the International  

E-Print Network (OSTI)

credits which apply toward the degree. The ID program advisor works closely with each student to help develop a unique program that meets their needs and future goals. Students will also work with a thesis a structural engineer on the Hanford vitrification design-build project How can I get started

Escher, Christine

218

DOE - Office of Legacy Management -- Blockson Chemical Co - IL 07  

Office of Legacy Management (LM)

Blockson Chemical Co - IL 07 Blockson Chemical Co - IL 07 FUSRAP Considered Sites Site: Blockson Chemical Co. (IL.07) Eliminated from consideration under FUSRAP - Referred to US EPA Region V and the State of Illinios Designated Name: Not Designated Alternate Name: Olin Corporation IL.07-1 Location: Patterson Road , Joliet , Illinois IL.07-2 Evaluation Year: 1985 IL.07-1 Site Operations: Process development studies and pilot plant testing of uranium recovery from phosphoric acid during the 1950s. Site Disposition: Eliminated - No Authority IL.07-1 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium Radiological Survey(s): Yes IL.07-2 Site Status: Eliminated from consideration under FUSRAP - Referred to US EPA Region V and the State of Illinios IL.07-1

219

DOE - Office of Legacy Management -- Kankakee Ordnance Plant - IL 32  

Office of Legacy Management (LM)

Kankakee Ordnance Plant - IL 32 Kankakee Ordnance Plant - IL 32 FUSRAP Considered Sites Site: KANKAKEE ORDNANCE PLANT (IL.32 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Kankakee , Illinois IL.32-1 Evaluation Year: 1991 IL.32-1 Site Operations: Kankakee Ordnance Plant was cited as a possible location for the disposal of radioactive waste material. There is no indication that any radioactive waste was brought to Kankakee. IL.32-1 IL.32-2 Site Disposition: Eliminated - No indication that radioactive materials were handled at this site IL.32-1 Radioactive Materials Handled: None Indicated IL.32-1 Primary Radioactive Materials Handled: None Radiological Survey(s): No Site Status: Eliminated from further consideration under FUSRAP

220

DOE - Office of Legacy Management -- Rock Island Arsenal - IL 09  

NLE Websites -- All DOE Office Websites (Extended Search)

Rock Island Arsenal - IL 09 Rock Island Arsenal - IL 09 FUSRAP Considered Sites Site: ROCK ISLAND ARSENAL ( IL.09 ) Eliminated from consideration under FUSRAP - Referred to DOD Designated Name: Not Designated Alternate Name: None Location: Rock Island , Illinois IL.09-1 Evaluation Year: 1987 IL.09-2 Site Operations: Site located on a DOD facility and operated under AEC control. Exact nature or time period of operations not clear. No indication that radioactive materials were involved. Contract work with Albuquerque Operations office performed. IL.09-1 IL.09-2 Site Disposition: Eliminated - No Authority - Referred to DOD IL.09-2 Radioactive Materials Handled: None Indicated IL.09-2 Primary Radioactive Materials Handled: None Indicated Radiological Survey(s): None Indicated

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

DOE - Office of Legacy Management -- Kaiser Aluminum Corp - IL 19  

NLE Websites -- All DOE Office Websites (Extended Search)

Kaiser Aluminum Corp - IL 19 Kaiser Aluminum Corp - IL 19 FUSRAP Considered Sites Site: KAISER ALUMINUM CORP. (IL.19 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Dolton , Illinois IL.19-2 Evaluation Year: 1987 IL.19-2 Site Operations: Performed limited duration work extruding uranium billets into three CP-5 fuel elements, circa 1959. IL.19-2 Site Disposition: Eliminated - Potential for contamination considered remote due to limited scope of activities IL.19-3 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IL.19-2 Radiological Survey(s): Yes - health and safety monitoring during operations IL.19-4 Site Status: Eliminated from further consideration under FUSRAP

222

u.s. DEPARTMENT OF ENERGY EERE PROJECT MANAG EMEN T CENTER NEPA DETERl\ilNATION  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

City of Noriolk City of Noriolk u.s. DEPARTMENT OF ENERGY EERE PROJECT MANAG EMEN T CENTER NEPA DETERl\ilNATION Page 1 of2 STATE: VA PROJECT TITLE: Green Vision Community Energy Program and Evergreen Municipal Energy Efficiency Program- SOW (5) Funding Opportunity Announcement Number Proc:urt:mtnt Instrument Number NEPA Control Number CID Number DE-FOA-OOOOO13 OE-EEOOOO880/000 0 Based on my review of the information concerning the proposed action, as NEPA Compliance Officer (authorized under DOE Order 451.IA), I have made the following determination: ex, EA, EIS APPENDIX AND NUMBER: Description: 85.1 Actions to conserve energy, demonstrate potential energy conservation, and promote energy-efficiency that do not increase the indoor concentrations of potentially harmful substances. These actions may involve financial and technical

223

Final Technical Report: Discovering the Nature of Dark Energy: Towards Better Distances from Type Ia Supernovae  

Science Conference Proceedings (OSTI)

The final technical report from the project "Discovering the Nature of Dark Energy: Towards Better Distances from Type Ia Supernovae" led at Rutgers the State University of New Jersey by Prof. Saurabh W. Jha is presented, including all publications resulting from this award.

Saurabh W. Jha

2012-10-03T23:59:59.000Z

224

Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook  

E-Print Network (OSTI)

Symbiotic stars are interacting binaries in which the first-formed white dwarf accretes and burns material from a red giant companion. This paper aims at presenting physical characteristics of these objects and discussing their possible link with progenitors of type Ia supernovae.

Miko?ajewska, J

2011-01-01T23:59:59.000Z

225

g-MODE EXCITATION DURING THE PRE-EXPLOSIVE SIMMERING OF TYPE Ia SUPERNOVAE  

SciTech Connect

Prior to the explosive burning of a white dwarf (WD) that makes a Type Ia supernova (SN Ia), the star 'simmers' for {approx}10{sup 3} yr in a convecting, carbon-burning region. I estimate the excitation of g-modes by convection during this phase and explore their possible effect on the WD. As these modes propagate from the core of the WD toward its surface, their amplitudes grow with decreasing density. Once the modes reach nonlinear amplitudes, they break and deposit their energy into a shell of mass {approx}10{sup -4} M{sub sun}. This raises the surface temperature by {approx}4 x 10{sup 8} K, which is sufficient to ignite a layer of helium, as is expected to exist for some SN Ia scenarios. This predominantly synthesizes {sup 40}Ca, but some amount of {sup 28}Si, {sup 32}S, and {sup 44}Ti may also be present. These ashes are expanded out with the subsequent explosion up to velocities of {approx}20, 000 km s{sup -1}, which may explain the high velocity features (HVFs) seen in many SNe Ia. The appearance of HVFs would therefore be a useful discriminant for determining between progenitors, since a flammable helium-rich layer will not be present for accretion from a C/O WD as in a merger scenario. I also discuss the implications of {sup 44}Ti production.

Piro, Anthony L., E-mail: piro@caltech.edu [Theoretical Astrophysics, California Institute of Technology, 1200 E California Blvd., M/C 350-17, Pasadena, CA 91125 (United States)

2011-09-01T23:59:59.000Z

226

Flames in Type Ia Supernova: Deflagration-Detonation Transition in the Oxygen Burning Flame  

E-Print Network (OSTI)

Flames in Type Ia Supernova: Deflagration-Detonation Transition in the Oxygen Burning Flame S. E structure which, de- pending on density, may involve separate regions of carbon, oxygen and silicon burning, all propagating in a self-similar, subsonic front. The separation between these three burning regions

227

A Test for the Nature of the Type Ia Supernova Explosion Mechanism  

E-Print Network (OSTI)

Currently popular models for Type Ia supernovae (SNe Ia) fall into two general classes. The first comprises explosions of nearly pure carbon/oxygen (C/O) white dwarfs at the Chandrasekhar limit which ignite near their centers. The second consists of lower-mass C/O cores which are ignited by the detonation of an accreted surface helium layer. Explosions of the latter type produce copious Fe, Co and Ni K-alpha emission from 56Ni and 56Co decay in the detonated surface layers, emission which is much weaker from Chandrasekhar-mass models. The presence of this emission provides a simple and unambiguous discriminant between these two models for SNe Ia. Both mechanisms may produce 0.1-0.6 solar masses of 56Ni, making them bright gamma-ray line emitters. The time to maximum brightness of 56Ni decay lines is distinctly shorter in the sub-Chandrasekhar mass class of model (approximately 15 days) than in the Chandrasekhar mass model (approximately 30 days), making gamma-ray line evolution another direct test of the explosion mechanism. It should just be possible to detect K-shell emission from a sub-Chandrasekhar explosion from SNe Ia as far away as the Virgo cluster with the XMM Observatory. A 1 to 2 square meter X-ray telescope such as the proposed Con-X Observatory could observe K-alpha emission from sub-Chandrasekhar mass SNe Ia in the Virgo cluster, providing not just a detection, but high-accuracy flux and kinematic information.

Philip A. Pinto; Ronald G. Eastman; Tamara Rogers

2000-08-21T23:59:59.000Z

228

WHITE DWARF/M DWARF BINARIES AS SINGLE DEGENERATE PROGENITORS OF TYPE Ia SUPERNOVAE  

SciTech Connect

Limits on the companions of white dwarfs in the single-degenerate scenario for the origin of Type Ia supernovae (SNe Ia) have gotten increasingly tight, yet igniting a nearly Chandrasekhar mass C/O white dwarf from a condition of near hydrostatic equilibrium provides compelling agreement with observed spectral evolution. The only type of non-degenerate stars that survive the tight limits, M{sub V} {approx}> 8.4 on the SN Ia in SNR 0509-67.5 and M{sub V} {approx}> 9.5 in the remnant of SN 1572, are M dwarfs. While M dwarfs are observed in cataclysmic variables, they have special properties that have not been considered in most work on the progenitors of SNe Ia: they have small but finite magnetic fields and they flare frequently. These properties are explored in the context of SN Ia progenitors. White dwarf/M dwarf pairs may be sufficiently plentiful to provide, in principle, an adequate rate of explosions even with slow orbital evolution due to magnetic braking or gravitational radiation. Even modest magnetic fields on the white dwarf and M dwarf will yield adequate torques to lock the two stars together, resulting in a slowly rotating white dwarf, with the magnetic poles pointing at one another in the orbital plane. The mass loss will be channeled by a 'magnetic bottle' connecting the two stars, landing on a concentrated polar area on the white dwarf. This enhances the effective rate of accretion compared to spherical accretion. Luminosity from accretion and hydrogen burning on the surface of the white dwarf may induce self-excited mass transfer. The combined effects of self-excited mass loss, polar accretion, and magnetic inhibition of mixing of accretion layers give possible means to beat the 'nova limit' and grow the white dwarf to the Chandrasekhar mass even at rather moderate mass accretion rates.

Wheeler, J. Craig, E-mail: wheel@astro.as.utexas.edu [Department of Astronomy, University of Texas at Austin, Austin, TX 78712 (United States)

2012-10-20T23:59:59.000Z

229

DOE - Office of Legacy Management -- Crane Co - IL 13  

Office of Legacy Management (LM)

Crane Co - IL 13 Crane Co - IL 13 FUSRAP Considered Sites Site: Crane Co. (IL.13 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Chicago , Illinois IL.13-2 Evaluation Year: 1987 IL.13-2 Site Operations: MED activities during late-1940s to early/mid-1950s included the development of valves and possibly the use of test quantities of normal uranium in the development process. IL.13-4 Site Disposition: Eliminated - Potential for contamination remote due to limited scope of operations IL.13-3 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IL.13-2 Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to Crane Co.

230

DOE - Office of Legacy Management -- Swenson Evaporator Co - IL 23  

NLE Websites -- All DOE Office Websites (Extended Search)

Swenson Evaporator Co - IL 23 Swenson Evaporator Co - IL 23 FUSRAP Considered Sites Site: SWENSON EVAPORATOR CO. (IL.23 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Harvey , Illinois IL.23-1 Evaluation Year: 1987 IL.23-1 Site Operations: Scheduled a raffinate spray drying test that was later cancelled. IL.23-1 Site Disposition: Eliminated - No indication that radioactive materials were handled at this site IL.23-1 Radioactive Materials Handled: None Indicated Primary Radioactive Materials Handled: None Radiological Survey(s): None Indicated Site Status: Eliminated from further consideration under FUSRAP Also see Documents Related to SWENSON EVAPORATOR CO. IL.23-1 - Memorandum/Checklist; D.Levine to the File; Subject:

231

GRR/Section 3-ID-a - State Lands Commercial Geothermal Lease | Open Energy  

Open Energy Info (EERE)

3-ID-a - State Lands Commercial Geothermal Lease 3-ID-a - State Lands Commercial Geothermal Lease < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 3-ID-a - State Lands Commercial Geothermal Lease 03IDAStateLandsCommercialGeothermalLease (1).pdf Click to View Fullscreen Contact Agencies Idaho Department of Lands Idaho State Board of Land Commissioners Regulations & Policies Original Administrative Rule Draft Rules Leasing of Public Lands 58-301 et seq Geothermal Resources 47-1605 IX, Section 8 of Idaho's Constitution Triggers None specified Click "Edit With Form" above to add content 03IDAStateLandsCommercialGeothermalLease (1).pdf 03IDAStateLandsCommercialGeothermalLease (1).pdf Error creating thumbnail: Page number not in range.

232

GRR/Section 12-ID-a - State Flora & Fauna Considerations | Open Energy  

Open Energy Info (EERE)

GRR/Section 12-ID-a - State Flora & Fauna Considerations GRR/Section 12-ID-a - State Flora & Fauna Considerations < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 12-ID-a - State Flora & Fauna Considerations 12IDAFloraFaunaConsiderations.pdf Click to View Fullscreen Contact Agencies Idaho Department of Fish & Game Regulations & Policies Idaho Statutes 36.103 Triggers None specified Click "Edit With Form" above to add content 12IDAFloraFaunaConsiderations.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Fish & Game preserves wildlife against any direct take, including wild animals, birds, and fish under Idaho Statutes 36.103.

233

GRR/Section 14-ID-c - Underground Injection Control | Open Energy  

Open Energy Info (EERE)

4-ID-c - Underground Injection Control 4-ID-c - Underground Injection Control < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 14-ID-c - Underground Injection Control 14IDCUndergroundInjectionControlPermit.pdf Click to View Fullscreen Contact Agencies Idaho Department of Water Resources Regulations & Policies IDAPA 37.03.04 IDAPA 37.03.03 Triggers None specified Click "Edit With Form" above to add content Potential Roadblocks Extensive public comments can stretch the timeline since IDWR must respond to all comments, potentially hold a Fact Finding Hearing, and thoroughly review the input received in these processes prior to making a decision to issue or deny the permit. 14IDCUndergroundInjectionControlPermit.pdf

234

GRR/Section 18-ID-d - Solid Waste Management Facilities | Open Energy  

Open Energy Info (EERE)

8-ID-d - Solid Waste Management Facilities 8-ID-d - Solid Waste Management Facilities < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 18-ID-d - Solid Waste Management Facilities 18IDDSolidWasteManagementFacilities (2).pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Regulations & Policies IDAPA 58.01.06 Triggers None specified Click "Edit With Form" above to add content 18IDDSolidWasteManagementFacilities (2).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Idaho considers transfer stations, composting operations, incinerators and landfills solid waste management facilities. The state does not require a

235

GRR/Section 18-ID-a - Underground Storage Tank Systems | Open Energy  

Open Energy Info (EERE)

GRR/Section 18-ID-a - Underground Storage Tank Systems GRR/Section 18-ID-a - Underground Storage Tank Systems < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 18-ID-a - Underground Storage Tank Systems 18IDAUndergroundStorageTankSystems.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Regulations & Policies IDAPA 58.01.07 Rules Regulating Underground Storage Tank Systems Triggers None specified Click "Edit With Form" above to add content 18IDAUndergroundStorageTankSystems.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Environmental Quality (DEQ) requires notification

236

GRR/Section 14-ID-f - 401 NPDES Water Quality Certification | Open Energy  

Open Energy Info (EERE)

ID-f - 401 NPDES Water Quality Certification ID-f - 401 NPDES Water Quality Certification < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 14-ID-f - 401 NPDES Water Quality Certification 14IDFSection401NPDESWaterQualityCertification.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality United States Environmental Protection Agency U S Army Corps of Engineers Regulations & Policies Idaho Environmental Protection and Health Act Idaho Administrative Procedure Act Triggers None specified Click "Edit With Form" above to add content 14IDFSection401NPDESWaterQualityCertification.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range.

237

GRR/Section 3-ID-c - Encroachment Permit | Open Energy Information  

Open Energy Info (EERE)

3-ID-c - Encroachment Permit 3-ID-c - Encroachment Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 3-ID-c - Encroachment Permit 03IDCEncroachmentPermit.pdf Click to View Fullscreen Contact Agencies Idaho Transportation Department Regulations & Policies IDAPA 39.03.42 Triggers None specified Click "Edit With Form" above to add content 03IDCEncroachmentPermit.pdf 03IDCEncroachmentPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative A developer needs an Encroachment Permit from the Idaho Transportation Department (ITD) to add, modify, relocate, maintain, or remove an encroachment on the state highway or within the state highway rights-of way

238

DOI-BLM-ID-220-2009-EA-3709 | Open Energy Information  

Open Energy Info (EERE)

ID-220-2009-EA-3709 ID-220-2009-EA-3709 Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-220-2009-EA-3709 EA at Raft River Geothermal Area for Geothermal/Exploration Raft River Geothermal Drilling Project General NEPA Document Info Energy Sector Geothermal energy Environmental Analysis Type EA Applicant Agua Caliente, LLC Consultant EMPSi Geothermal Area Raft River Geothermal Area Project Location Idaho Project Phase Geothermal/Exploration Techniques Exploration Drilling Time Frame (days) Participating Agencies Lead Agency BLM Funding Agency none provided Managing District Office BLM Twin Falls District Office Managing Field Office Burley Field Office Funding Agencies none provided Surface Manager BLM Mineral Manager BLM

239

GRR/Section 14-ID-b - NPDES Permitting Process | Open Energy Information  

Open Energy Info (EERE)

GRR/Section 14-ID-b - NPDES Permitting Process GRR/Section 14-ID-b - NPDES Permitting Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 14-ID-b - NPDES Permitting Process 14IDBNPDESPermittingProcess.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality United States Environmental Protection Agency Triggers None specified Click "Edit With Form" above to add content 14IDBNPDESPermittingProcess.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative 'National Pollutant Discharge Elimination System Permits' The NPDES program requires facilities discharging from a point source into

240

GRR/Section 6-ID-a - Transportation Permit | Open Energy Information  

Open Energy Info (EERE)

GRR/Section 6-ID-a - Transportation Permit GRR/Section 6-ID-a - Transportation Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 6-ID-a - Transportation Permit 06IDATransportationPermit.pdf Click to View Fullscreen Contact Agencies Idaho Transportation Department Regulations & Policies IDAPA 39.03.21 Triggers None specified Click "Edit With Form" above to add content 06IDATransportationPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Overlegal permits are issued to protect the "safety and convenience of the general public." The Idaho Transportation Department is also concerned with

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

GRR/Section 5-ID-a - Drilling and Well Development | Open Energy  

Open Energy Info (EERE)

ID-a - Drilling and Well Development ID-a - Drilling and Well Development < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 5-ID-a - Drilling and Well Development 05IDADrillingWellDevelopment.pdf Click to View Fullscreen Contact Agencies Idaho Department of Water Resources Regulations & Policies IC §42-233: Appropriation of Water, Geothermal IC §42-4003: Permits IC §42-4004: Processing Applications IC §42-4011: Name of Owner Triggers None specified Click "Edit With Form" above to add content Best Practices Community outreach Talk to the local county Potential Roadblocks Incomplete applications result in longer approval times by IDWR 05IDADrillingWellDevelopment.pdf Error creating thumbnail: Page number not in range.

242

DOI-BLM-ID-I020-2012-0017-CX | Open Energy Information  

Open Energy Info (EERE)

DOI-BLM-ID-I020-2012-0017-CX DOI-BLM-ID-I020-2012-0017-CX Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-I020-2012-0017-CX CX at Abraham Hot Springs Geothermal Area for Geothermal/Exploration {{{NEPA_Name}}} General NEPA Document Info Environmental Analysis Type CX Applicant Idaho Geological Survey Geothermal Area Abraham Hot Springs Geothermal Area Project Location Utah Project Phase Geothermal/Exploration Techniques Time Frame (days) Application Time 272 Participating Agencies Lead Agency BLM Funding Agency none provided Managing District Office BLM Idaho Falls District Office Managing Field Office BLM Pocatello Field Office Funding Agencies none provided Surface Manager BLM Mineral Manager BLM Selected Dates Application Date 10/21/2011

243

GRR/Section 7-ID-c - Certificate of Public Convenience and Necessity | Open  

Open Energy Info (EERE)

GRR/Section 7-ID-c - Certificate of Public Convenience and Necessity GRR/Section 7-ID-c - Certificate of Public Convenience and Necessity < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 7-ID-c - Certificate of Public Convenience and Necessity 07IDCCertificateOfPublicConvenienceAndNecessity (1).pdf Click to View Fullscreen Contact Agencies Idaho Public Utilities Commission Regulations & Policies Idaho Code 61-526 IDAPA 31.01.01 Triggers None specified Click "Edit With Form" above to add content 07IDCCertificateOfPublicConvenienceAndNecessity (1).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Electrical corporations must receive a Certificate of Public Convenience

244

GRR/Section 9-ID-a - State Environmental Process | Open Energy Information  

Open Energy Info (EERE)

9-ID-a - State Environmental Process 9-ID-a - State Environmental Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 9-ID-a - State Environmental Process 09IDAStateEnvironmentalProcess.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Triggers None specified Click "Edit With Form" above to add content 09IDAStateEnvironmentalProcess.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Idaho has no state-specific EA/EIS equivalent for renewable energy projects. Idaho does have an environmental assessment process for proposed wastewater and drinking water construction projects, but only when grant

245

DOI-BLM-ID-T020-2012-0003-CX | Open Energy Information  

Open Energy Info (EERE)

DOI-BLM-ID-T020-2012-0003-CX DOI-BLM-ID-T020-2012-0003-CX Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-T020-2012-0003-CX CX at Abraham Hot Springs Geothermal Area for Geothermal/Exploration {{{NEPA_Name}}} General NEPA Document Info Energy Sector Geothermal energy Environmental Analysis Type CX Applicant Agua Caliente LLC Geothermal Area Abraham Hot Springs Geothermal Area Project Location Utah Project Phase Geothermal/Exploration Techniques Seismic Techniques Time Frame (days) Participating Agencies Lead Agency BLM Funding Agency none provided Managing District Office BLM Twin Falls District Office Managing Field Office BLM Burley Field Office Funding Agencies none provided Surface Manager BLM Mineral Manager BLM Selected Dates

246

GRR/Section 14-ID-d - Section 401 Water Quality Certification | Open Energy  

Open Energy Info (EERE)

GRR/Section 14-ID-d - Section 401 Water Quality Certification GRR/Section 14-ID-d - Section 401 Water Quality Certification < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 14-ID-d - Section 401 Water Quality Certification 14IDDSection401WaterQualityCertificationProcess.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality United States Environmental Protection Agency U S Army Corps of Engineers Regulations & Policies Idaho Environmental Protection and Health Act Idaho Administrative Procedure Act Triggers None specified Click "Edit With Form" above to add content 14IDDSection401WaterQualityCertificationProcess.pdf 14IDDSection401WaterQualityCertificationProcess.pdf Error creating thumbnail: Page number not in range.

247

GRR/Section 18-ID-c - Wastewater Pretreatment Permit | Open Energy  

Open Energy Info (EERE)

8-ID-c - Wastewater Pretreatment Permit 8-ID-c - Wastewater Pretreatment Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 18-ID-c - Wastewater Pretreatment Permit 18IDCWastewaterPretreatmentPermit.pdf Click to View Fullscreen Triggers None specified Click "Edit With Form" above to add content 18IDCWastewaterPretreatmentPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Industrial wastewater permits are issued at the local level. If wastewater is not discharged into a municipal sewer system, the nonpoint source and NPDES permit inquiries are sufficient. A common approach to wastewater treatment is to treat on-site. See Idaho's

248

GRR/Section 11-ID-a - State Cultural Considerations | Open Energy  

Open Energy Info (EERE)

-ID-a - State Cultural Considerations -ID-a - State Cultural Considerations < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 11-ID-a - State Cultural Considerations 11IDAStateCulturalConsiderations (2).pdf Click to View Fullscreen Contact Agencies Idaho State Historical Society Regulations & Policies Idaho's Protection of Graves Statute IS 27-503 Triggers None specified Click "Edit With Form" above to add content 11IDAStateCulturalConsiderations (2).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Idaho has a statute that provides state law protection to cairns and grave sites. The Idaho State Historical Society administers the protections

249

GRR/Section 14-ID-a - Nonpoint Source Pollution | Open Energy Information  

Open Energy Info (EERE)

GRR/Section 14-ID-a - Nonpoint Source Pollution GRR/Section 14-ID-a - Nonpoint Source Pollution < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 14-ID-a - Nonpoint Source Pollution 14IDANonpointSourcePollution.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality United States Environmental Protection Agency Regulations & Policies Clean Water Act Idaho Code Triggers None specified Click "Edit With Form" above to add content 14IDANonpointSourcePollution.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Environmental Quality (IDEQ) developed Idaho's

250

GRR/Section 15-ID-b - Air Quality Permit - Tier II Operating Permit | Open  

Open Energy Info (EERE)

GRR/Section 15-ID-b - Air Quality Permit - Tier II Operating Permit GRR/Section 15-ID-b - Air Quality Permit - Tier II Operating Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 15-ID-b - Air Quality Permit - Tier II Operating Permit 15IDBAirQualityPermitTierIIOperatingPermit.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Regulations & Policies IDAPA 58.01.01 Triggers None specified Click "Edit With Form" above to add content 15IDBAirQualityPermitTierIIOperatingPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative Tier II Operating Permits are issued to facilities or stationary sources

251

GRR/Section 15-ID-a - Air Quality Permit - Permit to Construct | Open  

Open Energy Info (EERE)

15-ID-a - Air Quality Permit - Permit to Construct 15-ID-a - Air Quality Permit - Permit to Construct < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 15-ID-a - Air Quality Permit - Permit to Construct 15IDAAirQualityPermitPermitToConstruct (1).pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Regulations & Policies IDAPA 58.01.01 Triggers None specified Click "Edit With Form" above to add content 15IDAAirQualityPermitPermitToConstruct (1).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Environmental Quality (DEQ) requires an air quality

252

DOI-BLM-ID-110-2009-3825-CE | Open Energy Information  

Open Energy Info (EERE)

DOI-BLM-ID-110-2009-3825-CE DOI-BLM-ID-110-2009-3825-CE Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-110-2009-3825-CE CX at Crane Creek Geothermal Area for Geothermal/Exploration {{{NEPA_Name}}} General NEPA Document Info Energy Sector Geothermal energy Environmental Analysis Type CX Applicant Agua Caliente LLC Geothermal Area Crane Creek Geothermal Area Project Location Idaho Project Phase Geothermal/Exploration Techniques Time Frame (days) Application Time 113 Participating Agencies Lead Agency BLM Funding Agency none provided Managing District Office Boise Managing Field Office BLM Four Rivers Field Office Funding Agencies none provided Surface Manager BLM Mineral Manager none provided Selected Dates Application Date 6/4/2009

253

GRR/Section 19-ID-a - Water Access and Water Rights | Open Energy  

Open Energy Info (EERE)

19-ID-a - Water Access and Water Rights 19-ID-a - Water Access and Water Rights < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 19-ID-a - Water Access and Water Rights 19IDAWaterAccessAndWaterRightsIssues.pdf Click to View Fullscreen Contact Agencies Idaho Department of Water Resources Regulations & Policies Idaho Code Title 42 Triggers None specified Click "Edit With Form" above to add content 19IDAWaterAccessAndWaterRightsIssues.pdf 19IDAWaterAccessAndWaterRightsIssues.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Water Resources (IDWR) has the exclusive authority for regulation of appropriation of the public surface and ground waters of

254

GRR/Section 18-ID-b - Hazardous Waste Permit Process | Open Energy  

Open Energy Info (EERE)

GRR/Section 18-ID-b - Hazardous Waste Permit Process GRR/Section 18-ID-b - Hazardous Waste Permit Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 18-ID-b - Hazardous Waste Permit Process 18IDBHazardousWastePermitProcess.pdf Click to View Fullscreen Contact Agencies Idaho Department of Environmental Quality Regulations & Policies Idaho Hazardous Waste Management Act IDAPA 58.01.05 Rules and Standards for Hazardous Waste 40 CFR 124.31 Pre-application public meeting and notice 40 CRF 124.10 Public notice of permit actions and public comment period 40 CFR 124.12 Public hearings 40 CFR 270.13 Contents of Part A of the permit application Triggers None specified Click "Edit With Form" above to add content 18IDBHazardousWastePermitProcess.pdf 18IDBHazardousWastePermitProcess.pdf

255

DOI-BLM-ID-B010-2010-0083-CX | Open Energy Information  

Open Energy Info (EERE)

ID-B010-2010-0083-CX ID-B010-2010-0083-CX Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-B010-2010-0083-CX CX at {{{GeothermalArea}}} for Geothermal/Exploration, {{{NEPA_Name}}} General NEPA Document Info Energy Sector Geothermal energy Environmental Analysis Type CX Applicant Agua Caliente Geothermal Area {{{GeothermalArea}}}"{{{GeothermalArea}}}" cannot be used as a page name in this wiki. Project Location Project Phase Geothermal/Exploration Techniques Thermal Gradient Holes Comments ROW across BLM managed lands for access to TGH locations Time Frame (days) Participating Agencies Lead Agency Idaho Funding Agency none provided Managing District Office Boise Managing Field Office BLM Four Rivers Field Office

256

GRR/Section 20-ID-a - Well Abandonment Process | Open Energy Information  

Open Energy Info (EERE)

GRR/Section 20-ID-a - Well Abandonment Process GRR/Section 20-ID-a - Well Abandonment Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 20-ID-a - Well Abandonment Process 20IDAWellAbandonmentProcess.pdf Click to View Fullscreen Contact Agencies [[Idaho Department of Water Resources]] Regulations & Policies Drilling for Geothermal Resources Rule 45 Triggers None specified Click "Edit With Form" above to add content 20IDAWellAbandonmentProcess.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative This flowchart illustrates the well abandonment procedures in the state of Idaho. The director of the Idaho Department of Water Resources

257

Microsoft Word - DOE-ID-INL-12-028-1.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

EC Document No.: DOE-ID-INL-12-028 EC Document No.: DOE-ID-INL-12-028 SECTION A. Project Title: National Oceanic and Atmospheric Administration (NOAA) Birch Creek Canyon Wind Study SECTION B. Project Description: The National Oceanic and Atmospheric Administration (NOAA) Birch Creek Valley Wind Study would be conducted under the umbrella of the NOAA/Idaho National Laboratory (INL) Meteorological Research Partnership Memorandum of Agreement between NOAA and the Idaho Office of the U.S. Department of Energy (DOE-ID). The project would use a location near the northeast corner of the Test Area North (TAN) perimeter fence just north of the old TAN parking lot adjacent to the road to the Initial Engine Test (IET) facility and a remote site along Birch Creek near the point where Birch Creek crosses Idaho Highway 22. Field setup would occur as

258

RL-721 Document ID Number: REV4 NEPA REVIEW SCREENING FORM  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

ID Number: ID Number: REV4 NEPA REVIEW SCREENING FORM DOE/CX-00125, Rev 0 I. Project Title: MSA Annual Categorical Exclusion for Actions to Conserve Energy or Water under 10 CFR 1021, Subpart D, Appendix B, B5.1 II. Project Description and location (including Time Period over which proposed action will occur and Project Dimensions - e.g., acres displaced/disturbed, excavation length/depth, area/location/number of buildings, etc.): Mission Support Alliance (MSA) and its subcontractors perform actions to conserve energy or

259

Jong-Woo Kim  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Jong-Woo Kim Argonne National Laboratory 9700 S. Cass Ave 432/B008 Argonne, Il 60439 Phone: 252-0248 Fax: 252-7392 E-Mail: jwkim@aps.anl.gov Education/Experience: 2007 - present: Assistant Physicist, Advanced Photon Source, Argonne National Lab. 2005-2007: Postdoctoral Research Associate, APS/μ-CAT, Ames Laboratory, Argonne, IL. Ph. D. Condensed Matter Physics; Iowa State University, Ames, IA; 2005 M.S. Physics; Yongsei University, Seoul, Korea; 2000

260

Doug Robinson  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Doug Robinson Argonne National Laboratory 9700 S. Cass Ave 432/B007 Argonne, Il 60439 Phone: 252-0247 Fax: 252-7392 E-Mail: drobinsn@aps.anl.gov Education/Experience: 2009 - present: Physicist, Argonne National Lab. 1997 -2009: Beamline Scientist, APS/μ-CAT, Ames Laboratory, Argonne, IL. 1988-1997: Staff Scientist, Microelectronics Research Center, Iowa State University, Ames, IA Ph.D. Condensed Matter Physics, University of Illinois, Urbana,

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
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261

File:USDA-CE-Production-GIFmaps-IA.pdf | Open Energy Information  

Open Energy Info (EERE)

IA.pdf IA.pdf Jump to: navigation, search File File history File usage Iowa Ethanol Plant Locations Size of this preview: 776 × 600 pixels. Full resolution ‎(1,650 × 1,275 pixels, file size: 303 KB, MIME type: application/pdf) Description Iowa Ethanol Plant Locations Sources United States Department of Agriculture Related Technologies Biomass, Biofuels, Ethanol Creation Date 2010-01-19 Extent State Countries United States UN Region Northern America States Iowa External links http://www.nass.usda.gov/Charts_and_Maps/Ethanol_Plants/ File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 16:13, 27 December 2010 Thumbnail for version as of 16:13, 27 December 2010 1,650 × 1,275 (303 KB) MapBot (Talk | contribs) Automated bot upload

262

IA REP0 SAND85-2809 Unlimited Release UC-92A  

Office of Scientific and Technical Information (OSTI)

IA REP0 SAND85-2809 Unlimited Release UC-92A IA REP0 SAND85-2809 Unlimited Release UC-92A Printed July 1986 High Energy Gas Fracture Experiments in Fluid-Filled Boreholes-Potential Geothermal Application J. F. Cuderman, T. Y. Chu, J. Jung, R. D. Jacobson Prepared by Sandia National Laboratories Albuquerque, New Mexico 87 185 and Livermore, California 94550 for the United States Department of Energy under Contract DE-AC04-76DP00789 DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency Thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process

263

Constraining the spin-down timescale of the white-dwarf progenitors of Type Ia supernovae  

E-Print Network (OSTI)

Justham (2011) and DiStefano et al.\\ (2011) proposed that the white-dwarf progenitor of a Type Ia supernova (SN Ia) may have to spin down before it can explode. As the white dwarf spin-down timescale is not well known theoretically, we here try to constrain it empirically (within the framework of this spin-down model) for progenitor systems that contain a giant donor and for which circumbinary material has been detected after the explosion: we obtain an upper limit of a few $10^{\\rm 7} {\\rm yr}$. Based on the study of Di Stefano & Kilic (2012) this means that it is too early to rule out the existence of a surviving companion in SNR 0509-67.5.

Meng, Xiangcun

2013-01-01T23:59:59.000Z

264

th e american bir d conse rvan c y g u id e to bird conservation  

E-Print Network (OSTI)

th e american bir d conse rvan c y g u id e to bird conservation by daniel j. lebbin, michael j CONSERVATION 1886 George Grinnell founds the first Audubon So- ciety. 1896 Harriet Hemenway, her cousin Minna conservation for waterfowl and other birds. 1934 Roger Tory Peterson publishes his landmark Field Guide

McReynolds, Ben

265

TEXAS GRANT Statement of Student Eligibility Last Name First Name UT Arlington Student ID  

E-Print Network (OSTI)

TEXAS GRANT Statement of Student Eligibility 2012-2013 Last Name First Name UT Arlington Student ID Effective September 1, 2010, all institutions are required to collect a statement from each TEXAS Grant. TEXAS Grant funds will not disburse to your student account until the statement below is signed

Huang, Haiying

266

TEXAS GRANT Statement of Student Eligibility Last Name First Name UT Arlington Student ID  

E-Print Network (OSTI)

TEXAS GRANT Statement of Student Eligibility 2010-2011 Last Name First Name UT Arlington Student ID Effective September 1, 2010, all institutions are required to collect a statement from each TEXAS Grant. TEXAS Grant funds will not disburse to your student account until the statement below is signed

Corley, Bill

267

TEXAS GRANT Statement of Student Eligibility Last Name First Name UT Arlington Student ID  

E-Print Network (OSTI)

TEXAS GRANT Statement of Student Eligibility 2011-2012 Last Name First Name UT Arlington Student ID Effective September 1, 2010, all institutions are required to collect a statement from each TEXAS Grant. TEXAS Grant funds will not disburse to your student account until the statement below is signed

Corley, Bill

268

IDS: Thermodynamic-kinetic-empirical tool for modelling of solidification, microstructure and material properties  

Science Conference Proceedings (OSTI)

IDS (InterDendritic Solidification) is a thermodynamic-kinetic-empirical tool for simulation of solidification phenomena of steels including phase transformations from melt down to room temperature. In addition, important thermophysical material properties ... Keywords: Continuous casting, Inclusions, Material properties, Microstructure, Solidification

J. Miettinen; S. Louhenkilpi; H. Kytnen; J. Laine

2010-03-01T23:59:59.000Z

269

Integral Airframe Structures (IAS)---Validated Feasibility Study of Integrally Stiffened Metallic Fuselage Panels for Reducing Manufacturing Costs  

Science Conference Proceedings (OSTI)

The Integral Airframe Structures (IAS) program investigated the feasibility of using "integrally stiffened" construction for commercial transport fuselage structure. The objective of the program was to demonstrate structural performance and weight equal ...

Munroe J.; Wilkins K.; Gruber M.

2000-05-01T23:59:59.000Z

270

In vivo cofactor biosynthesis and maintenance in the class Ia ribonucleotide reductase small subunit of Escherichia coli  

E-Print Network (OSTI)

The small subunit ([beta]2) of Escherichia coli class Ia ribonucleotide reductases (RNRs) contains a diferric tyrosyl radical (Y*) cofactor essential for the conversion of nucleotides to deoxynucleotides that are needed ...

Wu, Chia-Hung, Ph. D. Massachusetts Institute of Technology

2009-01-01T23:59:59.000Z

271

Generation of a stable, aminotyrosyl radical-induced ?2?2 complex of Escherichia coli class Ia ribonucleotide reductase  

E-Print Network (OSTI)

Ribonucleotide reductase (RNR) catalyzes the conversion of nucleoside diphosphates to deoxynucleoside diphosphates (dNDPs). The Escherichia coli class Ia RNR uses a mechanism of radical propagation by which a cysteine in ...

Minnihan, Ellen Catherine

272

SELF-SHIELDING OF SOFT X-RAYS IN TYPE Ia SUPERNOVA PROGENITORS  

SciTech Connect

There are insufficient super-soft ({approx}0.1 keV) X-ray sources in either spiral or elliptical galaxies to account for the rate of explosion of Type Ia supernovae (SNe Ia) in either the single-degenerate or the double-degenerate scenarios. We quantify the amount of circumstellar matter that would be required to suppress the soft X-ray flux by yielding a column density in excess of 10{sup 23} cm{sup -2}. We summarize evidence that appropriate quantities of matter are extant in SNe Ia and in recurrent novae that may be supernova precursors. The obscuring matter is likely to have a large, but not complete, covering factor and to be substantially non-spherically symmetric. Assuming that much of the absorbed X-ray flux is re-radiated as blackbody radiation in the UV, we estimate that {approx}<100 sources might be detectable in the Galaxy Evolution Explorer All-sky Survey.

Wheeler, J. Craig [Department of Astronomy, University of Texas at Austin, Austin, TX (United States)] [Department of Astronomy, University of Texas at Austin, Austin, TX (United States); Pooley, D., E-mail: wheel@astro.as.utexas.edu [Department of Physics, Sam Houston State University, Huntsville, TX (United States)

2013-01-10T23:59:59.000Z

273

Restframe I-band Hubble diagram for type Ia supernovae up toredshift z ~; 0.5  

SciTech Connect

We present a novel technique for fitting rest frame I-bandlight curves on a data set of 42 type Ia supernovae (SNe Ia). Using the result of the fit, we construct a Hubble diagram with 26 SNe from the subset at 0.01 < z < 0.1. Adding two SNe at z {approx} 0.5 yields results consistent with a flat Lambda-dominated ''concordance universe'' (OmegaM,Omega Lambda) = (0.25, 0.75). For one of these, SN 2000fr, new near infrared data are presented. The high redshift supernova NIR data are also used to test for systematic effects in the use of SNe Ia as distance estimators. A flat, Lambda = 0, universe where the faintness of supernovae at z {approx} 0.5 is due to grey dust homogeneously distributed in the intergalactic medium is disfavored based on the high-z Hubble diagram using this small data-set. However, the uncertainties are large and no firm conclusion may be drawn. We explore the possibility of setting limits on intergalactic dust based on B - I and B - V color measurements, and conclude that about 20 well measured SNe are needed to give statistically significant results. We also show that the high redshift restframe I-band data points are better fit by light curve templates that show a prominent second peak, suggesting that they are not intrinsically underluminous.

Nobili, S.; Amanullah, R.; Garavini, G.; Goobar, A.; Lidman, C.; Stanishev, V.; Aldering, G.; Antilogus, P.; Astier, P.; Burns, M.S.; Conley, A.; Deustua, S.E.; Ellis, R.; Fabbro, S.; Fadeyev, V.; Folatelli,G.; Gibbons, R.; Goldhaber, G.; Groom, D.E.; Hook, I.; Howell, D.A.; Kim,A.G.; Knop, R.A.; Nugent, P.E.; Pain, R.; Perlmutter, S.; Quimby, R.; Raux, J.; Regnault, N.; Ruiz-Lapuente, P.; Sainton, G.; Schahmaneche, K.; Smith, E.; Spadafora, A.L.; Thomas, R.C.; Wang, L.

2005-04-01T23:59:59.000Z

274

Observational constraints from SNe Ia and Gamma-Ray Bursts on a clumpy universe  

E-Print Network (OSTI)

The luminosity distance describing the effect of local inhomogeneities in the propagation of light proposed by Zeldovich-Kantowski-Dyer-Roeder (ZKDR) is tested with two probes for two distinct ranges of redshifts: supernovae Ia (SNe Ia) in 0.015 gamma-ray bursts (GRBs) in 1.547 < z < 3.57. Our analysis is performed by a Markov Chain Monte Carlo (MCMC) code that allows us to constrain the matter density parameter \\Omega_m as well as the smoothness parameter $\\alpha$ that measures the inhomogeneous-homogeneous rate of the cosmic fluid in a flat \\LambdaCDM model. The obtained best fits are (\\Omega_m=0.285^{+0.019}_{-0.018}, \\alpha= 0.856^{+0.106}_{-0.176}) from SNe Ia and (\\Omega_m=0.259^{+0.028}_{-0.028}, \\alpha=0.587^{+0.201}_{-0.202}) from GRBs, while from the joint analysis the best fits are (\\Omega_m=0.284^{+0.021}_{-0.020}, \\alpha= 0.685^{+0.164}_{-0.171}) with a \\chi^2_{\\rm red}=0.975. The value of the smoothness parameter $\\alpha$ indicates a clumped universe however it does not have an impact on the amount of dark energy (cosmological constant) needed to fit observations. This result may be an indication that the Dyer-Roeder approximation does not describe in a precise form the effects of clumpiness in the expansion of the universe.

Nora Bretn; Ariadna Montiel

2013-03-06T23:59:59.000Z

275

The Cellular Burning Regime in Type Ia Supernova Explosions - I. Flame Propagation into Quiescent Fuel  

E-Print Network (OSTI)

We present a numerical investigation of the cellular burning regime in Type Ia supernova explosions. This regime holds at small scales (i.e. below the Gibson scale), which are unresolved in large-scale Type Ia supernova simulations. The fundamental effects that dominate the flame evolution here are the Landau-Darrieus instability and its nonlinear stabilization, leading to a stabilization of the flame in a cellular shape. The flame propagation into quiescent fuel is investigated addressing the dependence of the simulation results on the specific parameters of the numerical setup. Furthermore, we investigate the flame stability at a range of fuel densities. This is directly connected to the questions of active turbulent combustion (a mechanism of flame destabilization and subsequent self-turbulization) and a deflagration-to-detonation transition of the flame. In our simulations we find no substantial destabilization of the flame when propagating into quiescent fuels of densities down to ~10^7 g/cm^3, corroborating fundamental assumptions of large-scale SN Ia explosion models. For these models, however, we suggest an increased lower cutoff for the flame propagation velocity to take the cellular burning regime into account.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2003-12-03T23:59:59.000Z

276

Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z \\lesssim 0.3, of which 270 (52%) are spectroscopically identified as SNe Ia. The remaining 246 SNe Ia were identified through their light curves; 113 of these objects have spectroscopic redshifts from spectra of their host galaxy, and 133 have photometric redshifts estimated from the SN light curves. Based on consideration of 87 spectroscopically confirmed non-Ia SNe discovered by the SDSS-II SN Survey, we estimate that 2.04+1.61-0.95 % of the photometric SNe Ia may be misidentified. The sample of SNe Ia used in this measurement represents an order of magnitude increase in the statistics for SN Ia rate measurements in the redshift range covered by the SDSS-II Supernova Survey. If we assume a SN Ia rate that is constant at low redshift (z < 0.15), then the SN observations can be used t...

Dilday, Benjamin; Bassett, Bruce; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Filippenko, Alexei V; Frieman, Joshua A; Galbany, Lluis; Garnavich, Peter M; Goobar, Ariel; Hopp, Ulrich; Ihara, Yutaka; Jha, Saurabh W; Kessler, Richard; Lampeitl, Hubert; Marriner, John; Miquel, Ramon; Molla, Mercedes; Nichol, Robert C; Nordin, Jakob; Riess, Adam G; Sako, Masao; Schneider, Donald P; Sollerman, Jesper; Wheeler, J Craig; Ostman, Linda; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Pan, Kaike; Simmons, Audrey; Snedden, Stephanie

2010-01-01T23:59:59.000Z

277

DOE - Office of Legacy Management -- Heavy Minerals Inc - IL...  

Office of Legacy Management (LM)

Subject: FUSRAP Considered Site Recommendation; July 9, 1990. IL.14-2 - Heavy Minerals Co. Letter; Wyatt to Faulkner; Subject: Crude Thorium Hydroxide Proposal; December 1, 1954...

278

Weasel ID  

NLE Websites -- All DOE Office Websites (Extended Search)

question for you. (You showed up on page 1 of a Yahoo search on "weasel") Our cat recently killed (but didn't mangle) a small mammal of the weasel family (it looks in...

279

DOE-ID FOIA Type A Accident Investigation Board Report - July 28, 1998  

NLE Websites -- All DOE Office Websites (Extended Search)

Electronic Reading Room Documents Electronic Reading Room Documents Freedom of Information Act (FOIA) More on FOIA/Privacy Act Electronic Request Form Frequently Ask Questions Frequently Requested Documents Guides Helpful Links Points of Contact and Privacy Act Advisory Privacy Act Reading Room DOE-ID Public Reading Room Research Library You are here: DOE-ID Home > FOIA > Type A Accident Investigation Board Report - July 28, 1998 Type A Accident Investigation Board Report - July 28, 1998 Fatality and Multiple Injuries Resulting From Release of Carbon Dioxide at Building 648, Test Reactor Area Idaho National Engineering and Environmental Laboratory Files are provided in Adobe Acrobat format. If you experience problems reading these files please download the latest Adobe Acrobat reader at http://get.adobe.com/reader/ Download Acrobat Reader . Adobe Acrobat file Reader will allow you to view, navigate, and print these PDF files on all major computing platforms.

280

DOI-BLM-ID-B010-2010-??-CX | Open Energy Information  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » DOI-BLM-ID-B010-2010-??-CX Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: DOI-BLM-ID-B010-2010-??-CX CX at Weiser Geothermal Area for Geothermal/Exploration {{{NEPA_Name}}} General NEPA Document Info Environmental Analysis Type CX Applicant Agua Caliente LLC Geothermal Area Weiser Geothermal Area Project Location Idaho Project Phase Geothermal/Exploration Techniques Time Frame (days) Participating Agencies Lead Agency BLM Funding Agency none provided Managing District Office Boise Managing Field Office BLM Four Rivers Field Office Funding Agencies none provided Surface Manager BLM Mineral Manager none provided Selected Dates Decision Document Date 9/30/2010

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

GRR/Section 17-ID-a - Aesthetic Resource Assessment | Open Energy  

Open Energy Info (EERE)

form form View source History View New Pages Recent Changes All Special Pages Semantic Search/Querying Get Involved Help Apps Datasets Community Login | Sign Up Search Page Edit with form History Facebook icon Twitter icon » GRR/Section 17-ID-a - Aesthetic Resource Assessment < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 17-ID-a - Aesthetic Resource Assessment 17IDAAestheticResourceAssessment.pdf Click to View Fullscreen Triggers None specified Click "Edit With Form" above to add content 17IDAAestheticResourceAssessment.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative

282

GRR/Section 3-ID-b - State Land Access | Open Energy Information  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » GRR/Section 3-ID-b - State Land Access < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 3-ID-b - State Land Access 03IDBStateLandAccess (1).pdf Click to View Fullscreen Contact Agencies Idaho Department of Lands Regulations & Policies IDAPA 20.03.08 -Easements on State-Owned Lands Leasing of Public Lands 58-301 et seq Geothermal Resources 47-1605 Triggers None specified Click "Edit With Form" above to add content 03IDBStateLandAccess (1).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative

283

Ronald E. Gill (NE), Scoville, ID - Level I Curtis Roth (EM), Idaho  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

E. Gill (NE), E. Gill (NE), Scoville, ID - Level I Curtis Roth (EM), Idaho Falls, ID - Level I Jared T. Howerton (NNSA), Oak Ridge, TN - Level I Richard L. Person (NNSA), DOE HQ - Level I Phillip (Tony) A. Polk (EM), Aiken, SC (Savannah River) - Level IV Jane Powell-Dolan (LM), Cincinnati, OH - Level I Eric M. Thompson (NNSA), Oak Ridge, TN - Level II Congratulations to our newly certified FPDs! The Certification Review Board (CRB or 'the Board') convened on Friday, Sep- tember 24 to review certifi- cation candidates and dis- cuss several topics. The Department of Energy (DOE) met the FY2010 tar- gets for the Root Cause Analysis, Corrective Action Plan metrics 7 and 8, as fol- lows: DOE surpassed the target for Metric #7 (95% of pro-

284

GRR/Section 19-ID-b - Change Application Process | Open Energy Information  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » GRR/Section 19-ID-b - Change Application Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 19-ID-b - Change Application Process 19IDBChangeApplicationProcess (2).pdf Click to View Fullscreen Contact Agencies Idaho Department of Water Resources Regulations & Policies Idaho Code 42-222 Triggers None specified Click "Edit With Form" above to add content 19IDBChangeApplicationProcess (2).pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative A water right transfer is a change to a water right's point of diversion,

285

Microsoft Word - DOE-ID-12-011 RESL XRF EC.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 SECTION A. Project Title: DOE-ID/RESL Wavelength-Dispersive X-Ray Spectrometer for Chemistry Research & Development SECTION B. Project Description The DOE-ID Radiological & Environmental Sciences Laboratory (RESL) has a need for a complete state-of-the-art fully automated sequential wavelength-dispersive X-ray fluorescence (WD-XRF) spectrometer system. The WD-XRF spectrometer system will be primarily used for elemental analyses of soil, liquids (waters), air filters, unknown precipitates, and other environmental samples, as well as for quality control of other materials used in the preparation of performance testing materials for radiological and inorganic testing programs. SECTION C. Environmental Aspects / Potential Sources of Impact

286

Microsoft Word - DOE-ID-12-011 RESL XRF EC.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

1 1 SECTION A. Project Title: DOE-ID/RESL Wavelength-Dispersive X-Ray Spectrometer for Chemistry Research & Development SECTION B. Project Description The DOE-ID Radiological & Environmental Sciences Laboratory (RESL) has a need for a complete state-of-the-art fully automated sequential wavelength-dispersive X-ray fluorescence (WD-XRF) spectrometer system. The WD-XRF spectrometer system will be primarily used for elemental analyses of soil, liquids (waters), air filters, unknown precipitates, and other environmental samples, as well as for quality control of other materials used in the preparation of performance testing materials for radiological and inorganic testing programs. SECTION C. Environmental Aspects / Potential Sources of Impact

287

11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT  

National Nuclear Security Administration (NNSA)

11. CONTRACT ID CODE 11. CONTRACT ID CODE PAGE OF PAGES I AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1 I 2. AMENDMENTIMODIFICATION NO. 258 6. ISSUED BY CODE 3. EFFECTIVE DATE See Block 16C 05008 4. REQUISITION/PURCHASE REQ. NO. 7. ADMINISTERED BY (If other than Item 6) 15. PROJECT NO. (If applicable) CODE 1 0 5 0 0 8 NNSA/Oakridge Site Office NNSA/Oakridge Site Office U.S. Department of Energy U. S. Department of Energy NNSA/Y-12 Site Office NNSA/Y-12 Site Office P.O. Box 2050 P.O. Box 2050 Building 9704-2 Building 9704-2 Oak Ridge TN 37831 Oak Ridge TN 37831 8. NAME AND ADDRESS OF CONTRACTOR (No., str**t, county, SIal. and ZIP Code) ABCOCK & WILCOX TECHNICAL SERVICES Y-12, ttn: WILLIE J. WILSON o BOX 2009 02 SCARBORO RD. , Nl.149/MS 8004 AK RIDGE TN 378318004

288

File:USDA-CE-Production-GIFmaps-ID.pdf | Open Energy Information  

Open Energy Info (EERE)

ID.pdf ID.pdf Jump to: navigation, search File File history File usage Idaho Ethanol Plant Locations Size of this preview: 776 × 600 pixels. Full resolution ‎(1,650 × 1,275 pixels, file size: 212 KB, MIME type: application/pdf) Description Idaho Ethanol Plant Locations Sources United States Department of Agriculture Related Technologies Biomass, Biofuels, Ethanol Creation Date 2010-01-19 Extent State Countries United States UN Region Northern America States Idaho External links http://www.nass.usda.gov/Charts_and_Maps/Ethanol_Plants/ File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 16:13, 27 December 2010 Thumbnail for version as of 16:13, 27 December 2010 1,650 × 1,275 (212 KB) MapBot (Talk | contribs) Automated bot upload

289

Microsoft Word - DOE-ID-INL-13-004 R1.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

EC Document No.: DOE-ID-INL-13-004 R1 EC Document No.: DOE-ID-INL-13-004 R1 SECTION A. Project Description: High Density Fuel Material for Light Water Reactors (LWRs) SECTION B. Project Description: This project proposes to install glove boxes, laboratory equipment and laboratory hoods in the east wing of the Experimental Fuels Facility (EFF), building 794, at the Materials and Fuels Complex (MFC) at the Idaho National Laboratory (INL). The building was previously known as the Contaminated Equipment Storage Building (CESB). The purpose of this project is to support a high density fuel material development activity for Light Water Reactors (LWRs). The proposed action transfers process equipment from the Idaho Nuclear Technology and Engineering Center (INTEC) Chemical Process Plant (CPP)-1634 to EFF. Activities at CPP-1634 were

290

DOE - Office of Legacy Management -- W E Pratt Manufacturing Co - IL 12  

Office of Legacy Management (LM)

E Pratt Manufacturing Co - IL 12 E Pratt Manufacturing Co - IL 12 FUSRAP Considered Sites Site: W.E. PRATT MANUFACTURING CO. (IL.12) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: William E. Pratt Manufacturing Co. Klassing Handbrake Company IL.12-1 IL.12-2 Location: 18 Henderson Street , Joliet , Illinois IL.12-3 Evaluation Year: 1990 IL.12-4 IL.12-5 Site Operations: Performed metal fabrication tasks (machining and grinding). IL.12-1 IL.12-4 Site Disposition: Eliminated - Radiation levels below criteria IL.12-3 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium Metal IL.12-1 IL.12-3 Radiological Survey(s): Yes IL.12-3 Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to W.E. PRATT MANUFACTURING CO.

291

Notes on the compatibility of type Ia supernovae data and varying--$G$ cosmology  

E-Print Network (OSTI)

Observational data for type Ia supernovae, shows that the expansion of the universe is accelerated. This accelerated expansion can be described by a cosmological constant or by dark energy models like quintessence. An interesting question may be raised here. Is it possible to describe the accelerated expansion of universe using varying--$G$ cosmological models? Here we shall show that the price for having accelerated expansion in slow--varying--$G$ models (in which the dynamical terms of $G$ are ignored) is to have highly non--conserved matter and also that it is in contradiction with other data.

Shojai, F

2013-01-01T23:59:59.000Z

292

On the hydrogen emission from the type Ia supernova 2002ic  

DOE Green Energy (OSTI)

The discovery of SN 2002ic by the Supernova Factory and the subsequent spectroscopic studies have led to the surprising finding that SN 2002ic is a type Ia supernova with strong ejecta-circumstellar interaction. Here we show that nearly 1 year after the explosion the supernova has become fainter overall, but the H-alpha emission has brightened and broadened dramatically compared to earlier observations. We have obtained spectropolarimetry data which show that the hydrogen-rich matter is highly aspherically distributed. These observations suggest that the supernova exploded inside a dense, clumpy, disk-like circumstellar environment.

Wang, Lifan; Baade, Dietrich; Hoflich, Peter; Wheeler, J. Craig; Kawabata, Koji; Nomoto, Ken'ichi

2003-12-10T23:59:59.000Z

293

U.S. Energy Information Administration | Annual Energy Outlook...  

Gasoline and Diesel Fuel Update (EIA)

1 Regional maps Figure F4. Oil and gas supply model regions Figure F4. Oil and Gas Supply Model Regions Atlantic WA MT WY ID NV UT CO AZ NM TX OK IA KS MO IL IN KY TN MS AL FL GA...

294

DOE - Office of Legacy Management -- Quality Hardware and Machine Co - IL  

NLE Websites -- All DOE Office Websites (Extended Search)

Quality Hardware and Machine Co - Quality Hardware and Machine Co - IL 11 FUSRAP Considered Sites Site: QUALITY HARDWARE AND MACHINE CO. (IL.11) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Ravenswood Venture Marden Manufacturing Co. IL.11-1 IL.11-2 Location: 5823/5849 North Ravenswood Avenue , Chicago , Illinois IL.11-3 Evaluation Year: 1990 IL.11-4 IL.11-5 Site Operations: From 1944 to 1945, entered into subcontracts with the University of Chicago to furnish personnel, facilities, and equipment to produce special tools, dies, fixtures, etc., from materials furnished by the University; was involved in the Hanford slug canning process. IL.11-10 IL.11-6 IL.11-7 IL.11-8 IL.11-9 Site Disposition: Eliminated - Radiation levels below criteria IL.11-11

295

DOE - Office of Legacy Management -- Lindsay Light and Chemical Co - IL 10  

Office of Legacy Management (LM)

Lindsay Light and Chemical Co - IL Lindsay Light and Chemical Co - IL 10 FUSRAP Considered Sites Site: LINDSAY LIGHT AND CHEMICAL CO. ( IL.10 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: West Chicago , Illinois IL.10-3 Evaluation Year: 1995 IL.10-4 Site Operations: Processed thorium ores - chiefly monazite sands - for thorium and rare earth metals. IL.10-1 IL.10-2 Site Disposition: Eliminated - No Authority - NRC licensed operation IL.10-4 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Thorium IL.10-2 Radiological Survey(s): Yes IL.10-2 IL.10-5 Site Status: Eliminated from consideration under FUSRAP IL.10-4 Also see Documents Related to LINDSAY LIGHT AND CHEMICAL CO. IL.10-1 - Lindsay Light & Chemical Letter; J. Murray to E. Lintner;

296

DOE - Office of Legacy Management -- GSA 39th Street Warehouse - IL 02  

Office of Legacy Management (LM)

GSA 39th Street Warehouse - IL 02 GSA 39th Street Warehouse - IL 02 FUSRAP Considered Sites Site: GSA 39TH STREET WAREHOUSE (IL.02 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: 1716 West Pershing Road , Chicago , Illinois IL.02-1 Evaluation Year: 1985 IL.02-2 IL.02-3 Site Operations: Stored radioactive materials. IL.02-1 IL.02-2 Site Disposition: Eliminated - Radiation levels below criteria IL.02-1 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Unknown IL.02-2 Radiological Survey(s): Yes IL.02-1 IL.02-4 Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to GSA 39TH STREET WAREHOUSE IL.02-1 - Report (DOE/EV-0005/9); Formerly Utilized MED/AEC Sites Remedial Action Program Radiological Survey of the Former GSA 39th Street

297

Photometric Observations of the Type Ia SN 2002er in UGC 10743  

E-Print Network (OSTI)

Extensive light and colour curves for the Type Ia supernova SN 2002er are presented as part of the European Supernova Collaboration. We have collected UBVRI photometry from ten different telescopes covering the phases from 7 days before until 619 days after maximum light. Corrections for the different instrumental systems and the non-thermal spectrum of the supernova (S-corrections) have been applied. With the densely sampled light curves we can make detailed comparisons to other well-observed objects. SN 2002er most closely resembles SN 1996X after maximum, but clearly shows a different colour evolution before peak light and a stronger shoulder in V and R bands compared to other well-observed SNe Ia. In particular, the rise time appears to be longer than what is expected from rise-time vs.decline-rate relation. We use several methods to determine the reddening towards SN 2002er based on the colour evolution at near peak and at late phases. The uvoir (bolometric) light curve shows great similarity with SN 199...

Pignata, G; Benetti, S; Blinnikov, S; Hillebrandt, W; Kotak, R; Leibundgut, B; Mazzali, P A; Meikle, P; Qiu, Y; Ruiz-Lapuente, P; Smartt, S; Sorokina, E; Stritzinger, M; Stehle, M; Turatto, M; Marsh, T; Martin-Luis, F; McBride, N; Mndez, J; Morales-Rueda, L; Narbutis, D; Street, R

2004-01-01T23:59:59.000Z

298

The Cellular Burning Regime in Type Ia Supernova Explosions - II. Flame Propagation into Vortical Fuel  

E-Print Network (OSTI)

We investigate the interaction of thermonuclear flames in Type Ia supernova explosions with vortical flows by means of numerical simulations. In our study, we focus on small scales, where the flame propagation is no longer dominated by the turbulent cascade originating from large-scale effects. Here, the flame propagation proceeds in the cellular burning regime, resulting from a balance between the Landau-Darrieus instability and its nonlinear stabilization. The interaction of a cellularly stabilized flame front with a vortical fuel flow is explored applying a variety of fuel densities and strengths of the velocity fluctuations. We find that the vortical flow can break up the cellular flame structure if it is sufficiently strong. In this case the flame structure adapts to the imprinted flow field. The transition from the cellularly stabilized front to the flame structure dominated by vortices of the flow proceeds in a smooth way. The implications of the results of our simulations for Type Ia Supernova explosion models are discussed.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2003-12-08T23:59:59.000Z

299

Flame Evolution During Type Ia Supernovae and the Deflagration Phase in the Gravitationally Confined Detonation Scenario  

E-Print Network (OSTI)

We develop an improved method for tracking the nuclear flame during the deflagration phase of a Type Ia supernova, and apply it to study the variation in outcomes expected from the gravitationally confined detonation (GCD) paradigm. A simplified 3-stage burning model and a non-static ash state are integrated with an artificially thickened advection-diffusion-reaction (ADR) flame front in order to provide an accurate but highly efficient representation of the energy release and electron capture in and after the unresolvable flame. We demonstrate that both our ADR and energy release methods do not generate significant acoustic noise, as has been a problem with previous ADR-based schemes. We proceed to model aspects of the deflagration, particularly the role of buoyancy of the hot ash, and find that our methods are reasonably well-behaved with respect to numerical resolution. We show that if a detonation occurs in material swept up by the material ejected by the first rising bubble but gravitationally confined to the white dwarf (WD) surface (the GCD paradigm), the density structure of the WD at detonation is systematically correlated with the distance of the deflagration ignition point from the center of the star. Coupled to a suitably stochastic ignition process, this correlation may provide a plausible explanation for the variety of nickel masses seen in Type Ia Supernovae.

D. M. Townsley; A. C. Calder; S. M. Asida; I. R. Seitenzahl; F. Peng; N. Vladimirova; D. Q. Lamb; J. W. Truran

2007-06-07T23:59:59.000Z

300

Flame-driven deflagration-to-detonation transitions in Type Ia supernovae?  

E-Print Network (OSTI)

Although delayed detonation models of thermonuclear explosions of white dwarfs seem promising for reproducing Type Ia supernovae, the transition of the flame propagation mode from subsonic deflagration to supersonic detonation remains hypothetical. A potential instant for this transition to occur is the onset of the distributed burning regime, i.e. the moment when turbulence first affects the internal flame structure. Some studies of the burning microphysics indicate that a deflagration-to-detonation transition may be possible here, provided the turbulent intensities are strong enough. Consequently, the magnitude of turbulent velocity fluctuations generated by the deflagration flame is analyzed at the onset of the distributed burning regime in several three-dimensional simulations of deflagrations in thermonuclear supernovae. It is shown that the corresponding probability density functions fall off towards high turbulent velocity fluctuations much more slowly than a Gaussian distribution. Thus, values claimed to be necessary for triggering a detonation are likely to be found in sufficiently large patches of the flame. Although the microphysical evolution of the burning is not followed and a successful deflagration-to-detonation transition cannot be guaranteed from simulations presented here, the results still indicate that such events may be possible in Type Ia supernova explosions.

F. K. Roepke

2007-09-26T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Verifying the Cosmological Utility of Type Ia Supernovae:Implications of a Dispersion in the Ultraviolet Spectra  

SciTech Connect

We analyze the mean rest-frame ultraviolet (UV) spectrum ofType Ia Supernovae(SNe) and its dispersion using high signal-to-noiseKeck-I/LRIS-B spectroscopyfor a sample of 36 events at intermediateredshift (z=0.5) discoveredby the Canada-France-Hawaii TelescopeSupernova Legacy Survey (SNLS). Weintroduce a new method for removinghost galaxy contamination in our spectra,exploiting the comprehensivephotometric coverage of the SNLS SNe and theirhost galaxies, therebyproviding the first quantitative view of the UV spectralproperties of alarge sample of distant SNe Ia. Although the mean SN Ia spectrumhas notevolved significantly over the past 40 percent of cosmic history,preciseevolutionary constraints are limited by the absence of acomparable sample ofhigh quality local spectra. The mean UV spectrum ofour z 0.5 SNe Ia and itsdispersion is tabulated for use in futureapplications. Within the high-redshiftsample, we discover significant UVspectral variations and exclude dust extinctionas the primary cause byexamining trends with the optical SN color. Although progenitormetallicity may drive some of these trends, the variations we see aremuchlarger than predicted in recent models and do not follow expectedpatterns.An interesting new result is a variation seen in the wavelengthof selected UVfeatures with phase. We also demonstrate systematicdifferences in the SN Iaspectral features with SN lightcurve width inboth the UV and the optical. Weshow that these intrinsic variations couldrepresent a statistical limitation in thefuture use of high-redshift SNeIa for precision cosmology. We conclude thatfurther detailed studies areneeded, both locally and at moderate redshift wherethe rest-frame UV canbe studied precisely, in order that future missions canconfidently beplanned to fully exploit SNe Ia as cosmological probes.

Ellis, R.S.; Sullivan, M.; Nugent, P.E.; Howell, D.A.; Gal-Yam,A.; Astier, P.; Balam, D.; Balland, C.; Basa, S.; Carlberg, R.G.; Conley,A.; Fouchez, D.; Guy, J.; Hardin, D.; Hook, I.; Pain, R.; Perrett, K.; Pritchet, C.J.; Regnault, N.

2007-11-02T23:59:59.000Z

302

Alternative Muon Front-end for the International Design Study (IDS)  

E-Print Network (OSTI)

We discuss alternative designs of the muon capture front end of the Neutrino Factory International Design Study (IDS). In the front end, a proton bunch on a target creates secondary pions that drift into a capture channel, decaying into muons. A sequence of RF cavities forms the resulting muon beams into strings of bunches of differing energies, aligns the bunches to (nearly) equal central energies, and initiates ionization cooling. This design is affected by limitations on accelerating gradients within magnetic fields. The effects of gradient limitations are explored, and mitigation strategies are presented

Alekou, A; Martini, M; Prior, G; Rogers, C; Stratakis, D; Yoshikawa, C; Zisman, M

2010-01-01T23:59:59.000Z

303

LATE-TIME SPECTRAL OBSERVATIONS OF THE STRONGLY INTERACTING TYPE Ia SUPERNOVA PTF11kx  

SciTech Connect

PTF11kx was a Type Ia supernova (SN Ia) that showed time-variable absorption features, including saturated Ca II H and K lines that weakened and eventually went into emission. The strength of the emission component of H{alpha} gradually increased, implying that the SN was undergoing significant interaction with its circumstellar medium (CSM). These features, and many others, were blueshifted slightly and showed a P-Cygni profile, likely indicating that the CSM was directly related to, and probably previously ejected by, the progenitor system itself. These and other observations led Dilday et al. to conclude that PTF11kx came from a symbiotic nova progenitor like RS Oph. In this work we extend the spectral coverage of PTF11kx to 124-680 rest-frame days past maximum brightness. The late-time spectra of PTF11kx are dominated by H{alpha} emission (with widths of full width at half-maximum intensity Almost-Equal-To 2000 km s{sup -1}), strong Ca II emission features ({approx}10,000 km s{sup -1} wide), and a blue 'quasi-continuum' due to many overlapping narrow lines of Fe II. Emission from oxygen, He I, and Balmer lines higher than H{alpha} is weak or completely absent at all epochs, leading to large observed H{alpha}/H{beta} intensity ratios. The H{alpha} emission appears to increase in strength with time for {approx}1 yr, but it subsequently decreases significantly along with the Ca II emission. Our latest spectrum also indicates the possibility of newly formed dust in the system as evidenced by a slight decrease in the red wing of H{alpha}. During the same epochs, multiple narrow emission features from the CSM temporally vary in strength. The weakening of the H{alpha} and Ca II emission at late times is possible evidence that the SN ejecta have overtaken the majority of the CSM and agrees with models of other strongly interacting SNe Ia. The varying narrow emission features, on the other hand, may indicate that the CSM is clumpy or consists of multiple thin shells.

Silverman, Jeffrey M. [Department of Astronomy, University of Texas, Austin, TX 78712-0259 (United States); Nugent, Peter E.; Filippenko, Alexei V.; Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, The Weizmann Institute of Science, Rehovot 76100 (Israel); Sullivan, Mark [School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom); Howell, D. Andrew [Las Cumbres Observatory Global Telescope Network, Goleta, CA 93117 (United States); Pan, Yen-Chen; Hook, Isobel M., E-mail: jsilverman@astro.as.utexas.edu [Department of Physics (Astrophysics), University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom)

2013-08-01T23:59:59.000Z

304

A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data  

Science Conference Proceedings (OSTI)

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; /Pennsylvania U.; Sako, M.; /Pennsylvania U.; Corlies, L.; /Pennsylvania U. /Columbia U.; Folatelli, G.; /Tokyo U. /Carnegie Inst. Observ.; Frieman, J.; /Chicago U., KICP /Chicago U., Astron. Astrophys. Ctr.; Holtzman, J.; /New Mexico State U.; Jha, S.W.; /Rutgers U., Piscataway; Kessler, R.; /Chicago U., Astron. Astrophys. Ctr. /Chicago U., KICP; Marriner, J.; /Fermilab; Phillips, M.M.; /Carnegie Inst. Observ.; Stritzinger, M.; /Aarhus U. /Stockholm U., OKC /Bohr Inst. /Carnegie Inst. Observ.

2012-06-01T23:59:59.000Z

305

A PRECISION PHOTOMETRIC COMPARISON BETWEEN SDSS-II AND CSP TYPE Ia SUPERNOVA DATA  

SciTech Connect

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; Sako, M.; Corlies, L. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Folatelli, G. [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Frieman, J.; Kessler, R. [Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Holtzman, J. [Department of Astronomy, MSC 4500, New Mexico State University, P.O. Box 30001, Las Cruces, NM 88003 (United States); Jha, S. W. [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, J. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Phillips, M. M.; Morrell, N. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Stritzinger, M. [Oskar Klein Centre for Cosmo Particle Physics, AlbaNova University Center, 106 91 Stockholm (Sweden); Schneider, D. P., E-mail: jmosher@sas.upenn.edu [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States)

2012-07-15T23:59:59.000Z

306

A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data  

E-Print Network (OSTI)

Consistency between Carnegie Supernova Project (CSP) and SDSS-II supernova (SN) survey ugri measurements has been evaluated by comparing SDSS and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 magnitude level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 magnitudes in ugri, with rms scatter ranging from 0.043 to 0.077 magnitudes. The u band agreement is promising, with the caveat that only four of the nine supernovae are well-observed in u and these four exhibit an 0.038 magnitude supernova-to-supernova scatter in this filter.

Mosher, J; Corlies, L; Folatelli, G; Frieman, J; Holtzman, J; Jha, S W; Kessler, R; Marriner, J; Phillips, M M; Stritzinger, M; Morrell, N; Schneider, D P

2012-01-01T23:59:59.000Z

307

Analysis of Reaction-Diffusion Systems for Flame Capturing in Type Ia Supernova Simulations  

E-Print Network (OSTI)

We present a study of numerical behavior of a thickened flame used in Flame Capturing (FC, Khokhlov (1995)) for tracking thin unresolved physical flames in deflagration simulations. We develop a steady-state procedure for calibrating the flame model used, and test it against analytical results. We observe numerical noises generated by original realization of the technique. Alternative artificial burning rates are discussed, which produce acceptably quiet flames. Two new quiet models are calibrated to yield required "flame" speed and width, and further studied in 2D and 3D setting. Landau-Darrieus type instabilities of the flames are observed. One model also shows significantly anisotropic propagation speed on the grid, both effects increasingly pronounced at larger matter expansion as a result of burning; this makes the model unacceptable for use in type Ia supernova simulations. Another model looks promising for use in flame capturing at fuel to ash density ratio of order 3 and below. That "Model B" yields f...

Zhiglo, Andrey V

2009-01-01T23:59:59.000Z

308

Executive Bios: Dr. Yoon Il Chang - Nuclear Engineering Division (Argonne)  

NLE Websites -- All DOE Office Websites (Extended Search)

Yoon Il Chang Yoon Il Chang Director's Welcome Organization Achievements Awards Patents Professional Societies Highlights Fact Sheets, Brochures & Other Documents Multimedia Library About Nuclear Energy Nuclear Reactors Designed by Argonne Argonne's Nuclear Science and Technology Legacy Opportunities within NE Division Visit Argonne Work with Argonne Contact us For Employees Site Map Help Join us on Facebook Follow us on Twitter NE on Flickr Celebrating the 70th Anniversary of Chicago Pile 1 (CP-1) Argonne OutLoud on Nuclear Energy Argonne Energy Showcase 2012 Distinguished Fellows Bookmark and Share Dr. Yoon Il Chang Dr. Yoon Il Chang Senior Technical Advisor Distinguished Fellow PhD, Engineer Nuclear Engineering Division Argonne Experts: Y.I. Chang Dr. Chang joined Argonne National Laboratory in 1974 and has been

309

ASD(NII)/DoD CIO SUBJECT: Defense Industrial Base (DIB) Cyber Security/Information Assurance (CS/IA) Activities  

E-Print Network (OSTI)

directing the conduct of DIB CS/IA activities to protect unclassified DoD information, as defined in the Glossary, that transits or resides on unclassified DIB information systems and networks. 2. APPLICABILITY. This Instruction applies to OSD, the Military Departments, the Office of

unknown authors

2010-01-01T23:59:59.000Z

310

EARLY RADIO AND X-RAY OBSERVATIONS OF THE YOUNGEST NEARBY TYPE Ia SUPERNOVA PTF 11kly (SN 2011fe)  

SciTech Connect

On 2011 August 24 (UT) the Palomar Transient Factory (PTF) discovered PTF11kly (SN 2011fe), the youngest and most nearby Type Ia supernova (SN Ia) in decades. We followed this event up in the radio (centimeter and millimeter bands) and X-ray bands, starting about a day after the estimated explosion time. We present our analysis of the radio and X-ray observations, yielding the tightest constraints yet placed on the pre-explosion mass-loss rate from the progenitor system of this supernova. We find a robust limit of M-dot {approx}<10{sup -8}(w/100 km s{sup -1}) M{sub sun} yr{sup -1} from sensitive X-ray non-detections, as well as a similar limit from radio data, which depends, however, on assumptions about microphysical parameters. We discuss our results in the context of single-degenerate models for SNe Ia and find that our observations modestly disfavor symbiotic progenitor models involving a red giant donor, but cannot constrain systems accreting from main-sequence or sub-giant stars, including the popular supersoft channel. In view of the proximity of PTF11kly and the sensitivity of our prompt observations, we would have to wait for a long time (a decade or longer) in order to more meaningfully probe the circumstellar matter of SNe Ia.

Horesh, Assaf; Kulkarni, S. R.; Carpenter, John; Kasliwal, Mansi M.; Ofek, Eran O. [Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Fox, Derek B. [Astronomy and Astrophysics, Eberly College of Science, Pennsylvania State University, University Park, PA 16802 (United States); Quimby, Robert [IPMU, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa-shi, Chiba (Japan); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); De Bruyn, A. G. [Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, NL-7990 AA Dwingeloo (Netherlands); Kamble, Atish; Wijers, Ralph A. M. J. [Center for Gravitation and Cosmology, University of Wisconsin, Milwaukee, WI 53211 (United States); Van der Horst, Alexander J. [Universities Space Research Association, NSSTC, Huntsville, AL 35805 (United States); Kouveliotou, Chryssa [Space Science Office, VP-62, NASA-Marshall Space Flight Center, Huntsville, AL 35805 (United States); Podsiadlowski, Philipp; Sullivan, Mark; Maguire, Kate [Department of Physics (Astrophysics), University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom); Howell, D. Andrew [Las Cumbres Observatory Global Telescope Network, Santa Barbara, CA 93117 (United States); Nugent, Peter E. [Computational Cosmology Center, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Gehrels, Neil [NASA-Goddard Space Flight Center, Greenbelt, MD 20771 (United States); and others

2012-02-10T23:59:59.000Z

311

Photometric Observations of the Type Ia SN 2002er in UGC 10743  

E-Print Network (OSTI)

Extensive light and colour curves for the Type Ia supernova SN 2002er are presented as part of the European Supernova Collaboration. We have collected UBVRI photometry from ten different telescopes covering the phases from 7 days before until 619 days after maximum light. Corrections for the different instrumental systems and the non-thermal spectrum of the supernova (S-corrections) have been applied. With the densely sampled light curves we can make detailed comparisons to other well-observed objects. SN 2002er most closely resembles SN 1996X after maximum, but clearly shows a different colour evolution before peak light and a stronger shoulder in V and R bands compared to other well-observed SNe Ia. In particular, the rise time appears to be longer than what is expected from rise-time vs.decline-rate relation. We use several methods to determine the reddening towards SN 2002er based on the colour evolution at near peak and at late phases. The uvoir (bolometric) light curve shows great similarity with SN 1996X, but also indications of a higher luminosity, longer rise time and a more pronounced shoulder 25 days past maximum. The interpretation of the light curves was done with two independent light curve codes. Both find that given the luminosity of SN 2002er the 56Ni mass exceeds 0.6 Msun with prefered values near 0.7 Msun. Uncertainties in the exact distance to SN 2002er are the most serious limitation of this measurement. The light curve modelling also indicates a high level of mixing of the nickel in the explosion of SN 2002er.

G. Pignata; F. Patat; S. Benetti; S. Blinnikov; W. Hillebrandt; R. Kotak; B. Leibundgut; P. A. Mazzali; P. Meikle; Y. Qiu; P. Ruiz-Lapuente; S. Smartt; E. Sorokina; M. Stritzinger; M. Stehle; M. Turatto; T. Marsh; F. Martin-Luis; N. McBride; J. Mendez; L. Morales-Rueda; D. Narbutis; R. Street

2004-08-12T23:59:59.000Z

312

Direct Analysis of Spectra of the Peculiar Type Ia Supernova 2000cx  

E-Print Network (OSTI)

The Type Ia SN 2000cx exhibited multiple peculiarities, including a lopsided B-band light-curve peak that does not conform to current methods for using shapes of light curves to standardize SN Ia luminosities. We use the parameterized supernova synthetic-spectrum code SYNOW to study line identifications in the photospheric-phase spectra of SN 2000cx. Previous work established the presence of Ca II infrared-triplet features forming above velocity about 20,000 km/s, much higher than the photospheric velocity of about 10,000 km/s. We find Ti II features forming at the same high velocity. High-velocity line formation is partly responsible for the photometric peculiarities of SN 2000cx: for example, B-band flux blocking by Ti II absorption features that decreases with time causes the B light curve to rise more rapidly and decline more slowly than it otherwise would. SN 2000cx contains an absorption feature near 4530 A that may be H-beta, forming at the same high velocity. The lack of conspicuous H-alpha and P-alpha signatures does not necessarily invalidate the H-beta identification if the high-velocity line formation is confined to a clump that partly covers the photosphere and the H-alpha and P-alpha source functions are elevated relative to that of resonance scattering. The H-beta identification is tentative. If it is correct, the high-velocity matter must have come from a nondegenerate companion star.

D. Branch; R. C. Thomas; E. Baron; D. Kasen; K. Hatano; K. Nomoto; A. V. Filippenko; W. Li; R. J. Rudy

2004-01-15T23:59:59.000Z

313

NUCLEOSYNTHESIS IN TWO-DIMENSIONAL DELAYED DETONATION MODELS OF TYPE Ia SUPERNOVA EXPLOSIONS  

SciTech Connect

For the explosion mechanism of Type Ia supernovae (SNe Ia), different scenarios have been suggested. In these, the propagation of the burning front through the exploding white dwarf (WD) star proceeds in different modes, and consequently imprints of the explosion model on the nucleosynthetic yields can be expected. The nucleosynthetic characteristics of various explosion mechanisms are explored based on three two-dimensional explosion simulations representing extreme cases: a pure turbulent deflagration, a delayed detonation following an approximately spherical ignition of the initial deflagration, and a delayed detonation arising from a highly asymmetric deflagration ignition. Apart from this initial condition, the deflagration stage is treated in a parameter-free approach. The detonation is initiated when the turbulent burning enters the distributed burning regime. This occurs at densities around 10{sup 7} g cm{sup -3}-relatively low as compared to existing nucleosynthesis studies for one-dimensional spherically symmetric models. The burning in these multidimensional models is different from that in one-dimensional simulations as the detonation wave propagates both into unburned material in the high-density region near the center of a WD and into the low-density region near the surface. Thus, the resulting yield is a mixture of different explosive burning products, from carbon-burning products at low densities to complete silicon-burning products at the highest densities, as well as electron-capture products synthesized at the deflagration stage. Detailed calculations of the nucleosynthesis in all three models are presented. In contrast to the deflagration model, the delayed detonations produce a characteristic layered structure and the yields largely satisfy constraints from Galactic chemical evolution. In the asymmetric delayed detonation model, the region filled with electron capture species (e.g., {sup 58}Ni, {sup 54}Fe) is within a shell, showing a large off-set, above the bulk of {sup 56}Ni distribution, while species produced by the detonation are distributed more spherically.

Maeda, K. [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Roepke, F.K.; Fink, M.; Hillebrandt, W.; Travaglio, C. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching (Germany); Thielemann, F.-K., E-mail: keiichi.maeda@ipmu.j [Department Physik, Universitaet Basel, CH-4056 Basel (Switzerland)

2010-03-20T23:59:59.000Z

314

DOE - Office of Legacy Management -- Great Lakes Carbon Corp - IL 21  

Office of Legacy Management (LM)

Great Lakes Carbon Corp - IL 21 Great Lakes Carbon Corp - IL 21 FUSRAP Considered Sites Site: GREAT LAKES CARBON CORP. ( IL.21 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: 333 North Michigan Avenue , Chicago , Illinois IL.21-1 Evaluation Year: 1987 IL.21-1 Site Operations: Facility performed a limited amount of nuclear fuel fabrication in the 1950s. Facility also developed graphite production under an AEC contract. IL.21-1 IL.21-3 Site Disposition: Eliminated - Potential for contamination considered remote due to limited scope of activities performed IL.21-1 Radioactive Materials Handled: Yes IL.21-3 Primary Radioactive Materials Handled: Uranium, Thorium IL.21-3 Radiological Survey(s): Yes IL.21-3

315

DOE - Office of Legacy Management -- American Machine and Metals Inc - IL  

NLE Websites -- All DOE Office Websites (Extended Search)

Machine and Metals Inc - Machine and Metals Inc - IL 24 FUSRAP Considered Sites Site: American Machine and Metals Inc (IL.24 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: E. Moline , Illinois IL.24-1 Evaluation Year: 1994 IL.24-2 IL.24-3 Site Operations: Tested process for dewatering green salt by centrifugation. IL.24-1 IL.24-2 Site Disposition: Eliminated - Potential for contamination considered remote due to limited amount of radioactive materials handled IL.24-1 IL.24-2 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium Oxide (Green Salt) IL.24-1 Radiological Survey(s): Health and Safety Monitoring IL.24-1 Site Status: Eliminated from consideration under FUSRAP Also see

316

DOE - Office of Legacy Management -- Wyckoff Drawn Steel Co - IL 0-09  

Office of Legacy Management (LM)

Drawn Steel Co - IL 0-09 Drawn Steel Co - IL 0-09 FUSRAP Considered Sites Site: Wyckoff Drawn Steel Co (IL 0-09) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Chicago , Illinois IL.0-09-1 Evaluation Year: 1987 IL.0-09-3 Site Operations: Experimentation on centerless grinding of uranium rods in 1943. IL.0-09-2 IL.0-09-3 Site Disposition: Eliminated - Potential for contamination considered remote based on the limited scope of activities at the site IL.0-09-1 IL.0-09-3 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IL.0-09-2 Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to Wyckoff Drawn Steel Co IL.0-09-1 - DOE Letter; Wagoner to Daley; Subject: Wycoff Steel Co.

317

Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z {approx}< 0.3, of which 270 (52%) are spectroscopically identified as SNe Ia. The remaining 246 SNe Ia were identified through their light curves; 113 of these objects have spectroscopic redshifts from spectra of their host galaxy, and 133 have photometric redshifts estimated from the SN light curves. Based on consideration of 87 spectroscopically confirmed non-Ia SNe discovered by the SDSS-II SN Survey, we estimate that 2.04{sub -0.95}{sup +1.61}% of the photometric SNe Ia may be misidentified. The sample of SNe Ia used in this measurement represents an order of magnitude increase in the statistics for SN Ia rate measurements in the redshift range covered by the SDSS-II Supernova Survey. If we assume a SN Ia rate that is constant at low redshift (z < 0.15), then the SN observations can be used to infer a value of the SN rate of r{sub V} = (2.69{sub -0.30-0.01}{sup +0.34+0.21}) x 10{sup -5} SNe yr{sup -1} Mpc{sup -3} (H{sub 0}/(70 km s{sup -1} Mpc{sup -1})){sup 3} at a mean redshift of {approx} 0.12, based on 79 SNe Ia of which 72 are spectroscopically confirmed. However, the large sample of SNe Ia included in this study allows us to place constraints on the redshift dependence of the SN Ia rate based on the SDSS-II Supernova Survey data alone. Fitting a power-law model of the SN rate evolution, r{sub V} (z) = A{sub p} x ((1+z)/(1+z{sub 0})){sup {nu}}, over the redshift range 0.0 < z < 0.3 with z{sub 0} = 0.21, results in A{sub p} = (3.43{sub -0.15}{sup +0.15}) x 10{sup -5} SNe yr{sup -1} Mpc{sup -3} (H{sub 0}/(70 km s{sup -1} Mpc{sup -1})){sup 3} and {nu} = 2.04{sub -0.89}{sup +0.90}.

Dilday, Benjamin; /Rutgers U., Piscataway /Chicago U. /KICP, Chicago; Smith, Mathew; /Cape Town U., Dept. Math. /Portsmouth U.; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Becker, Andrew; /Washington U., Seattle, Astron. Dept.; Bender, Ralf; /Munich, Tech. U. /Munich U. Observ.; Castander, Francisco; /Barcelona, IEEC; Cinabro, David; /Wayne State U.; Filippenko, Alexei V.; /UC, Berkeley; Frieman, Joshua A.; /Chicago U. /Fermilab; Galbany, Lluis; /Barcelona, IFAE; Garnavich, Peter M.; /Notre Dame U. /Stockholm U., OKC /Stockholm U.

2010-01-01T23:59:59.000Z

318

AMENDMENT OF SOLICITATIONIMODIFICATlON OF CONTRACT ( I- CONTRACT ID CODE PAGE I OF 2  

National Nuclear Security Administration (NNSA)

( ( I- CONTRACT ID CODE PAGE I OF 2 PAGES I . . Babcock & Wilcox Technical Services Pantex, LLC PO Box 30020 Amarillo, TX 79120 2. AMENDMENTIMODIFICATION NO. M I 51 Albuquerque, NM 87185-5400 I Amarillo, TX 79120 90. DATED (SEE ITEM 11) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) 3. EFFECTIVE DATE See Block 16C 9A. AMENDMENT OF SOLICITATION NO. extended. 6 . ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center Property and M&O Contract Su~pport Department P.O. Box 5400 CODE FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning -

319

Header Sheet Doc ID Z OAK RIDGE NATIONAL LABORATORY M. E. Murray  

Office of Legacy Management (LM)

Dames & Moore Dames & Moore Header Sheet Doc ID Z OAK RIDGE NATIONAL LABORATORY M. E. Murray MANAGED BY LOCKHEED MARTIN rNERGY RESEARCH CORPORATION PHONE: (423) 574-5838 FOR THE U.S. DEPARTMENT OF ENERGY FAX: (423) POST OFFICE Box 2 INTERNET: r'0 March 31, 1997 Mr. Andrew Meloy DuPont Environmental Remediation Services DuPont Chambers Works Route 130, Anti-Knocks Building G Deepwater, New Jersey 08023 Dear Mr. Meloy: Radiological Sampling Requirements for the B Ditch Remediation Project, DuPont Chamber Works Site, Deepwater, New Jersey During the week of March 10, staff members of the Oak Ridge National Laboratory, Life Sciences Division, made surface radiation measurcments along the B ditch from 6+00' to the 11+00' markers. These measurements were performed to better define the subsurface

320

Microsoft Word - DOE-ID-INL-12-007_INL-12-033_.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Page 1 of 2 CX Posting No.: DOE-ID-INL-12-007 SECTION A. Project Title: Geotechnical Core Drilling for USGS 138 SECTION B. Project Description: . The U.S. Geological Survey (USGS) proposes to drill a 1,000-foot deep geotechnical corehole (USGS 138) into the eastern Snake River Plain aquifer. The location of the corehole will be about 4.0 mile(s) east of the city Howe and about 8.5 mile(s) north of the Naval Reactors Facility at the Southeast Quarter of the Southwest Quarter, Section 7, Township 5 North, Range 30 East; lattitude/longitude (WGS84) 43 46 16.1 N / 112 55 27.7W (fig. 1). The purpose of this geotechnical borehole is to obtain geologic, stratigraphic, and hydraulic data to characterize flow in the eastern Snake River Plain aquifer.

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321

Report Period: EIA ID NUMBER: Appendix A: Mailing Address: Appendix B:  

U.S. Energy Information Administration (EIA) Indexed Site

Report Period: Report Period: EIA ID NUMBER: Appendix A: Mailing Address: Appendix B: Zip Code - Secure File Transfer option available at: - - - - Email form to: OOG.SURVEYS@eia.doe.gov Fax form to: (202) 586-9772 Email address: Oil & Gas Survey U.S. Department of Energy Ben Franklin Station PO Box 279 Washington, DC 20044-0279 Questions? Call toll free: 1-800-638-8812 1. Total Acquisitions (Enter the total volume of foreign crude oil acquired during the report month for importation into the United States. This is the sum of column (l), Part III, excluding resubmission.) 2. Offshore Inventories (Enter the total volume of foreign oil owned by the firm, for eventual importation into the United States which is held in storage outside the United States and/or is enroute to the United States as of the

322

GRR/Section 3-ID-e - Term Easement | Open Energy Information  

Open Energy Info (EERE)

e - Term Easement e - Term Easement < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 3-ID-e - Term Easement 03IDGTermEasement.pdf Click to View Fullscreen Contact Agencies Idaho Department of Lands Regulations & Policies IDPA 20.03.08 Idaho Code 58-603 Triggers None specified Click "Edit With Form" above to add content 03IDGTermEasement.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative The Idaho Department of Lands (IDL) requires a Term Easement for access across state lands and for right of ways across state lands. Note, an easement is not required for lands covered under a Geothermal Lease.

323

AMENDMENT OF SOLICITATIONIMODIFICATlON OF CONTRACT ( I- CONTRACT ID CODE PAGE I OF 2  

NLE Websites -- All DOE Office Websites (Extended Search)

( ( I- CONTRACT ID CODE PAGE I OF 2 PAGES I . . Babcock & Wilcox Technical Services Pantex, LLC PO Box 30020 Amarillo, TX 79120 2. AMENDMENTIMODIFICATION NO. M I 51 Albuquerque, NM 87185-5400 I Amarillo, TX 79120 90. DATED (SEE ITEM 11) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) 3. EFFECTIVE DATE See Block 16C 9A. AMENDMENT OF SOLICITATION NO. extended. 6 . ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center Property and M&O Contract Su~pport Department P.O. Box 5400 CODE FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning -

324

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT ( I. ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

( ( I. ID CODE / DE-ACO4-OOAL6662O ' 10s. DATED (SEE ITEM 13) PAGE I OF 2 PAGES Babcock & W ~ ~ C O X Technical Services Pantex, LLC 800 Main Street Lynchburg, VA 24505 9B. DATED (SEE ITEM 11) 10A. MODIFICATION OF CONTRACTIORDER NO. Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR ACKNOWLEDGMENT TO BE RECEIVED AT THE PLACE DESIGNATED FOR THE RECEIPT OF OFFERS PRIOR TO THE HOUR AND DATE

325

RL·721 Do~)nt ID Number: REV4 NEPA REVIEW SCREENING FORM  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Do~)nt ID Number: REV4 NEPA REVIEW SCREENING FORM " 8)( ... /){)(!) 7 !J --Jil.P:G-3·&-'1-2-0·0~~ 1. Project Title: CH2MHill Plateau Remedia t'ion co. - Routine Maintenance and Custodial Services August 2012 to August 2013 11. Project Description and Location (Including Time Period over which proposed action will occur and Project Dimensions -e.g., acres displaced/disturbed, excavation length/depth, area/location/number of buildings, etc.): CH2MHill Plateau Remediation Company (PRC) will conduct routine maintenance and custodial services on and near the Hanford Site in accordance with the categorical exclusion (CX) referenced in 10 CF'R 1021, Appendix B, ex Bl. 3, nRoutine Maintenance Servj.ces" and "Routine

326

Report Period: EIA ID NUMBER: Instructions: (e.g., Street Address, Bldg, Floor, Suite)  

U.S. Energy Information Administration (EIA) Indexed Site

Report Period: Report Period: EIA ID NUMBER: Instructions: (e.g., Street Address, Bldg, Floor, Suite) Secure File Transfer option available at: (e.g., PO Box, RR) Electronic Transmission: The PC Electronic Data Reporting Option (PEDRO) is available. Zip Code: - If interested in software, call (202) 586-9659. Email form to: Fax form to: (202) 586-9772 - - Mail form to: Oil & Gas Survey - - U.S. Department of Energy Ben Franklin Station PO Box 279 Washington, DC 20044-0279 Questions? Call toll free: 1-800-638-8812 OOG.SURVEYS@eia.doe.gov Contact Name: Version No.: 2013.01 Date of this Report: Mo Day State: Year Phone No.: DOMESTIC CRUDE OIL FIRST PURCHASE REPORT Company Name: A completed form must be filed by the 30th calendar day following the end of the report

327

Microsoft Word - DOE-ID-INL-13-009 R1.docx  

NLE Websites -- All DOE Office Websites (Extended Search)

09 R1 09 R1 SECTION A. Project Title: National Oceanic and Atmospheric Administration (NOAA) Project Sagebrush Atmospheric Tracer Dispersion Study Revision 1 SECTION B. Project Description: This revision of this EC is being prepared to provide estimated quantities of tracer emissions to account for greenhouse gas (GHG) emissions and to clarify that the National Oceanic and Atmospheric Administration (NOAA) would report GHG emissions as required by Executive Order (EO) 13514. The National Oceanic and Atmospheric Administration's (NOAA) Atmospheric Tracer Dispersion Study, formally called Project Sagebrush, would be conducted under the umbrella of the NOAA/Idaho National Laboratory (INL) Meteorological Research Partnership Memorandum of Agreement (MOA) between NOAA and the Idaho Office of the U.S. Department of Energy (DOE-ID). This MOA

328

Final PHP bench-scale report for the DOE-ID/SAIC sole source contract  

SciTech Connect

The Plasma Hearth Process (PHP) Technology Development Project was established to develop, test, and evaluate a new concept for treating mixed waste. The new concept uses direct current (dc) transferred-arc plasma torch technology to process mixed waste into a glass-like end-product. Under the cognizance of the US Department of Energy (DOE) Office of Technology Development (OTD) Mixed Waste Focus Area (MWFA), the technology is being explored for its potential to treat mixed waste. Because it is a mature technology, well-understood and commercially available, it is expected to develop rapidly in this new application. This report summarizes the radioactive bench-scale system activities funded under PHP Sole Source Contract DE-AC07-94ID13266 through the end of the contract.

1997-04-01T23:59:59.000Z

329

North Portal Fuel Storage System Fire Hazard Analysis-ESF Surface Design Package ID  

SciTech Connect

The purpose of the fire hazard analysis is to comprehensively assess the risk from fire within the individual fire areas. This document will only assess the fire hazard analysis within the Exploratory Studies Facility (ESF) Design Package ID, which includes the fuel storage system area of the North Portal facility, and evaluate whether the following objectives are met: 1.1.1--This analysis, performed in accordance with the requirements of this document, will satisfy the requirements for a fire hazard analysis in accordance with U.S. Department of Energy (DOE) Order 5480.7A. 1.1.2--Ensure that property damage from fire and related perils does not exceed an acceptable level. 1.1.3--Provide input to the ESF Basis For Design (BFD) Document. 1.1.4 Provide input to the facility Safety Analysis Report (SAR) (Paragraph 3.8).

N.M. Ruonavaara

1995-01-18T23:59:59.000Z

330

Environmental Science and Research Foundation annual technical report to DOE-ID, January , 1995--December 31, 1995  

Science Conference Proceedings (OSTI)

The foundation conducts an environmental monitoring and surveillance program over an area covering much of the upper Snake River Plain and provide environmental education and support services related to INEL natural resource issues. Also, the foundation, with its university affiliates, conducts ecological and radioecological research on the Idaho National Environmental Research Park. This research benefits major DOE-ID programs including waste management, environmental restoration, spent nuclear fuels, and land management issues. Major accomplishments during CY1995 can be divided into five categories: environmental surveillance program, environmental education, environmental services and support, ecological risk assessment, and research benefitting the DOE-ID mission.

NONE

1996-06-01T23:59:59.000Z

331

DOE - Office of Legacy Management -- Granite City Army Depot - IL 0-02  

Office of Legacy Management (LM)

Granite City Army Depot - IL 0-02 Granite City Army Depot - IL 0-02 FUSRAP Considered Sites Site: GRANITE CITY ARMY DEPOT ( IL.0-02 ) Eliminated from consideration under FUSRAP - Referred to DOD Designated Name: Not Designated Alternate Name: None Location: Granite City , Illinois IL.0-02-1 Evaluation Year: 1987 IL.0-02-1 Site Operations: Site was used for storage of GSA thorium residues until circa 1964. IL.0-02-1 Site Disposition: Eliminated - Referred to DOD IL.0-02-1 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Thorium IL.0-02-1 Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP - Referred to DOD IL.0-02-1 Also see Documents Related to GRANITE CITY ARMY DEPOT IL.0-02-1 - DOE Letter; J.Fiore to C.Schafer; Information regarding

332

LOGGING IN TO UI-INTEGRATE SELF-SERVICE First-time users must get their Enterprise ID and Enterprise ID Password before logging in to UI-Integrate  

E-Print Network (OSTI)

screen allows you to enter multiple search criteria to narrow your search. Click "Submit" at the bottom the Urbana-Champaign campus. #12;2 2. Once you have selected your campus, enter your Enterprise ID or seniors). · Curriculum (your degree, college, major). 7. To begin registration, Select a Term. Select

Anastasio, Thomas J.

333

Secretary Bodman Highlights Advanced Energy Initiative in Peoria, IL |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Bodman Highlights Advanced Energy Initiative in Peoria, Bodman Highlights Advanced Energy Initiative in Peoria, IL Secretary Bodman Highlights Advanced Energy Initiative in Peoria, IL April 6, 2006 - 10:15am Addthis PEORIA, IL - Secretary of Energy Samuel W. Bodman today highlighted the goals of President Bush's Advanced Energy Initiative after consulting on an energy savings assessment at Caterpillar Inc.'s manufacturing facility in Peoria, Illinois. To answer President Bush's call for Americans to be more energy efficient, the Department of Energy (DOE) is conducting no-cost energy assessments at 200 of the nation's most energy-intensive manufacturing facilities to identify energy- and money-saving opportunities. "President Bush has called on all Americans to be more energy efficient. Private industry is joining the federal government in taking a leading role

334

Constraints on SN Ia progenitor time delays from high-z SNe and the star formation history  

E-Print Network (OSTI)

We re-assess the question of a systematic time delay between the formation of the progenitor and its explosion in a type Ia supernova (SN Ia) using the Hubble Higher-z Supernova Search sample (Strolger et al. 2004). While the previous analysis indicated a significant time delay, with a most likely value of 3.4 Gyr, effectively ruling out all previously proposed progenitor models, our analysis shows that the time-delay estimate is dominated by systematic errors, in particular due to uncertainties in the star-formation history. We find that none of the popular progenitor models under consideration can be ruled out with any significant degree of confidence. The inferred time delay is mainly determined by the peak in the assumed star-formation history. We show that, even with a much larger Supernova sample, the time delay distribution cannot be reliably reconstructed without better constraints on the star-formation history.

F. Frster; C. Wolf; Ph. Podsiadlowski; Z. Han

2006-01-19T23:59:59.000Z

335

A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z {le} 0.17 and 27 SN events in 492 maxBCG clusters at 0.1 {le} z {le} 0.3. We find values for the cluster SN Ia rate of (0.37{sub -0.12-0.01}{sup +0.17+0.01}) SNur h{sup 2} and (0.55{sub -0.11-0.01}{sup +0.13+0.02}) SNur h{sup 2} (SNux = 10{sup -12}L{sub x{circle_dot}}{sup -1} yr{sup -1}) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be (0.31{sub -0.12-0.01}{sup +0.18+0.01}) SNur h{sup 2} and (0.49{sub -0.11-0.01}{sup +0.15+0.02}) SNur h{sup 2} in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be (2.04{sub -1.11-0.04}{sup +1.99+0.07}) SNur h{sup 2} and (0.36{sub -0.30-0.01}{sup +0.84+0.01}) SNur h{sup 2} in C4 and maxBCG clusters, respectively. The ratio of the SN Ia rate in cluster early-type galaxies to that of the SN Ia rate in field early-type galaxies is 1.94{sub -0.91-0.015}{sup +1.31+0.043} and 3.02{sub -1.03-0.048}{sup +1.31+0.062}, for C4 and maxBCG clusters, respectively. The SN rate in galaxy clusters as a function of redshift, which probes the late time SN Ia delay distribution, shows only weak dependence on redshift. Combining our current measurements with previous measurements, we fit the cluster SN Ia rate data to a linear function of redshift, and find r{sub L} = [(0.49{sub -0.14}{sup +0.15}) + (0.91{sub -0.81}{sup +0.85}) x z] SNuB h{sup 2}. A comparison of the radial distribution of SNe in cluster to field early-type galaxies shows possible evidence for an enhancement of the SN rate in the cores of cluster early-type galaxies. With an observation of at most 3 hostless, intra-cluster SNe Ia, we estimate the fraction of cluster SNe that are hostless to be (9.4{sub -5.1}{sup +8.3})%.

Dilday, Benjamin; /Rutgers U., Piscataway /Chicago U. /KICP, Chicago; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Becker, Andrew; /Washington U., Seattle, Astron. Dept.; Bender, Ralf; /Munich, Tech. U. /Munich U. Observ.; Castander, Francisco; /Barcelona, IEEC; Cinabro, David; /Wayne State U.; Frieman, Joshua A.; /Chicago U. /Fermilab; Galbany, Lluis; /Barcelona, IFAE; Garnavich, Peter; /Notre Dame U.; Goobar, Ariel; /Stockholm U., OKC /Stockholm U.; Hopp, Ulrich; /Munich, Tech. U. /Munich U. Observ. /Tokyo U.

2010-03-01T23:59:59.000Z

336

Prospects for Type Ia Supernova explosion mechanism identification with gamma rays  

E-Print Network (OSTI)

The explosion mechanism associated with thermonuclear supernovae (SNIa) is still a matter of debate. There is a wide agreement that high amounts of of radioactive nuclei are produced during these events and they are expected to be strong gamma-ray emitters. In the past, several authors have investigated the use of this gamma-ray emission as a diagnostic tool. In this paper we have done a complete study of the gamma-ray spectra associated with all the different scenarios currently proposed. This includes detonation, delayed detonation, deflagration and the off-center detonation. We have performed accurate simulations for this complete set of models in order to determine the most promising spectral features that could be used to discriminate among the different models. Our study is not limited to qualitative arguments. Instead, we have quantified the differences among the spectra and established distance limits for their detection. The calculations have been performed considering the best current response estimations of the SPI and IBIS instruments aboard INTEGRAL in such a way that our results can be used as a guideline to evaluate the capabilities of INTEGRAL in the study of type Ia supernovae. For the purpose of completeness we have also investigated the nuclear excitation and spallation reactions as a possible secondary source of gamma-rays present in some supernova scenarios. We conclude that this mechanism can be neglected due to its small contribution.

Jordi Gomez-Gomar; Jordi Isern; Pierre Jean

1997-09-05T23:59:59.000Z

337

EVALUATING SYSTEMATIC DEPENDENCIES OF TYPE Ia SUPERNOVAE: THE INFLUENCE OF CENTRAL DENSITY  

SciTech Connect

We present a study exploring a systematic effect on the brightness of Type Ia supernovae using numerical models that assume the single-degenerate paradigm. Our investigation varied the central density of the progenitor white dwarf at flame ignition, and considered its impact on the explosion yield, particularly the production and distribution of radioactive {sup 56}Ni, which powers the light curve. We performed a suite of two-dimensional simulations with randomized initial conditions, allowing us to characterize the statistical trends that we present. The simulations indicate that the production of Fe-group material is statistically independent of progenitor central density, but the mass of stable Fe-group isotopes is tightly correlated with central density, with a decrease in the production of {sup 56}Ni at higher central densities. These results imply that progenitors with higher central densities produce dimmer events. We provide details of the post-explosion distribution of {sup 56}Ni in the models, including the lack of a consistent centrally located deficit of {sup 56}Ni, which may be compared to observed remnants. By performing a self-consistent extrapolation of our model yields and considering the main-sequence lifetime of the progenitor star and the elapsed time between the formation of the white dwarf and the onset of accretion, we develop a brightness-age relation that improves our prediction of the expected trend for single degenerates and we compare this relation with observations.

Krueger, Brendan K.; Jackson, Aaron P.; Calder, Alan C. [Department of Physics and Astronomy, State University of New York-Stony Brook, Stony Brook, NY (United States); Townsley, Dean M. [Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL (United States); Brown, Edward F. [Department of Physics and Astronomy, Michigan State University, East Lansing, MI (United States); Timmes, Francis X., E-mail: brendan.krueger@stonybrook.edu [Joint Institute for Nuclear Astrophysics, Notre Dame, IN (United States)

2012-10-01T23:59:59.000Z

338

Phenomenology for Supernova Ia Data Based on a New Cosmic Time  

E-Print Network (OSTI)

A new phenomenological theory for the expansion of our universe is presented. Because fundamental supporting theory is still in development, its discussion is not presented in this paper. The theory is based on a new algebraic expression for cosmic time G Rho t^2=3/32Pi, which correctly predicts the WMAP measured cosmological constants and the fundamental Hubble parameter H(t) for the expansion of the universe. A replacement for dark matter, called here "dark mass", is proposed which scales as with the expansion and incorporated. It does not react with ordinary matter, except gravitationally, and produces flat rotational curves for spiral galaxies. Also a new expression for the approaching velocity of radiation in a closed 3-sphere expanding universe is given that accounts for the early degrading negative approach of radiation for z > 1.7. The expression is v = Hr-c. Combining these three elements produces a luminosity distance dL that successfully predicts the apparent magnitude of exploding supernova Ia stars and even the new gamma ray bursts with no need for dark energy or acceleration of the expansion of the universe.

Charles B. Leffert

2007-07-26T23:59:59.000Z

339

HIGH-RESOLUTION SIMULATIONS OF CONVECTION PRECEDING IGNITION IN TYPE Ia SUPERNOVAE USING ADAPTIVE MESH REFINEMENT  

E-Print Network (OSTI)

We extend our previous three-dimensional, full-star simulations of the final hours of convection preceding ignition in Type Ia supernovae to higher resolution using the adaptive mesh refinement capability of our low Mach number code, MAESTRO. We report the statistics of the ignition of the first flame at an effective 4.34 km resolution and general flow field properties at an effective 2.17 km resolution. We find that off-center ignition is likely, with radius of 50 km most favored and a likely range of 4075 km. This is consistent with our previous coarser (8.68 km resolution) simulations, implying that we have achieved sufficient resolution in our determination of likely ignition radii. The dynamics of the last few hot spots preceding ignition suggest that a multiple ignition scenario is not likely. With improved resolution, we can more clearly see the general flow pattern in the convective region, characterized by a strong outward plume with a lower speed recirculation. We show that the convective core is turbulent with a Kolmogorov spectrum and has a lower turbulent intensity and larger integral length scale than previously thought (on the order of 16 km s?1 and 200 km, respectively), and we discuss the potential consequences for the first flames. Key words: convection hydrodynamics methods: numerical nuclear reactions, nucleosynthesis, abundances supernovae: general white dwarfs Online-only material: color figures 1.

A. Nonaka; A. J. Aspden; M. Zingale; A. S. Almgren; J. B. Bell; S. E. Woosley

2012-01-01T23:59:59.000Z

340

Direct numerical simulations of type Ia supernovae flames II: The Rayleigh-Taylor instability  

Science Conference Proceedings (OSTI)

A Type Ia supernova explosion likely begins as a nuclear runaway near the center of a carbon-oxygen white dwarf. The outward propagating flame is unstable to the Landau-Darrieus, Rayleigh-Taylor, and Kelvin-Helmholtz instabilities, which serve to accelerate it to a large fraction of the speed of sound. We investigate the Rayleigh-Taylor unstable flame at the transition from the flamelet regime to the distributed-burning regime, around densities of 10e7 gm/cc, through detailed, fully resolved simulations. A low Mach number, adaptive mesh hydrodynamics code is used to achieve the necessary resolution and long time scales. As the density is varied, we see a fundamental change in the character of the burning--at the low end of the density range the Rayleigh-Taylor instability dominates the burning, whereas at the high end the burning suppresses the instability. In all cases, significant acceleration of the flame is observed, limited only by the size of the domain we are able to study. We discuss the implications of these results on the potential for a deflagration to detonation transition.

Bell, J.B.; Day, M.S.; Rendleman, C.A.; Woosley, S.E.; Zingale, M.

2004-01-12T23:59:59.000Z

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341

Constraining deflagration models of Type Ia supernovae through intermediate-mass elements  

E-Print Network (OSTI)

The physical structure of a nuclear flame is a basic ingredient of the theory of Type Ia supernovae (SNIa). Assuming an exponential density reduction with several characteristic times we have followed the evolution of a planar nuclear flame in an expanding background from an initial density 6.6 10^7 g/cm3 down to 2 10^6 g/cm3. The total amount of synthesized intermediate-mass elements (IME), from silicon to calcium, was monitored during the calculation. We have made use of the computed mass fractions, X_IME, of these elements to give an estimation of the total amount of IME synthesized during the deflagration of a massive white dwarf. Using X_IME and adopting the usual hypothesis that turbulence decouples the effective burning velocity from the laminar flame speed, so that the relevant flame speed is actually the turbulent speed on the integral length-scale, we have built a simple geometrical approach to model the region where IME are thought to be produced. It turns out that a healthy production of IME invol...

Garca-Senz, D; Cabezon, R M; Woosley, S E

2006-01-01T23:59:59.000Z

342

Direct numerical simulations of type Ia supernovae flames I: The landau-darrieus instability  

SciTech Connect

Planar flames are intrinsically unstable in open domains due to the thermal expansion across the burning front--the Landau-Darrieus instability. This instability leads to wrinkling and growth of the flame surface, and corresponding acceleration of the flame, until it is stabilized by cusp formation. We look at the Landau-Darrieus in stability for C/O thermonuclear flames at conditions relevant to the late stages of a Type Ia supernova explosion. Two-dimensional direct numerical simulations of both single-mode and multi-mode perturbations using a low Mach number hydrodynamics code are presented. We show the effect of the instability on the flame speed as a function of both the density and domain size, demonstrate the existence of the small scale cutoff to the growth of the instability, and look for the proposed breakdown of the non-linear stabilization at low densities. The effects of curvature on the flame as quantified through measurements of the growth rate and computation of the corresponding Markstein number. While accelerations of a few percent are observed, they are too small to have any direct outcome on the supernova explosion.

Bell, J.B.; Day, M.S.; Rendleman, C.A.; Woosley, S.E.; Zingale, M.

2003-11-24T23:59:59.000Z

343

FLAMES IN TYPE Ia SUPERNOVA: DEFLAGRATION-DETONATION TRANSITION IN THE OXYGEN-BURNING FLAME  

Science Conference Proceedings (OSTI)

The flame in a Type Ia supernova is a conglomerate structure that, depending on density, may involve separate regions of carbon, oxygen, and silicon burning, all propagating in a self-similar, subsonic front. The separation between these three burning regions increases as the density declines until eventually, below about 2 x 10{sup 7} g cm{sup -3}, only carbon burning remains active, the other two burning phases having 'frozen out' on stellar scales. Between 2 and 3 x 10{sup 7} g cm{sup -3}, however, there remains an energetic oxygen-burning region that trails the carbon burning by an amount that is sensitive to the turbulence intensity. As the carbon flame makes a transition to the distributed regime (Karlovitz number {approx}> 10), the characteristic separation between the carbon- and oxygen-burning regions increases dramatically, from a fraction of a meter to many kilometers. The oxygen-rich mixture between the two flames is created at a nearly constant temperature, and turbulence helps to maintain islands of well-mixed isothermal fuel as the temperature increases. The delayed burning of these regions can be supersonic and could initiate a detonation.

Woosley, S. E. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Kerstein, A. R. [Combustion Research Facility, Sandia National Laboratories, Livermore, CA 94551 (United States); Aspden, A. J., E-mail: woosley@ucolick.org, E-mail: arkerst@sandia.gov, E-mail: ajaspden@lbl.gov [Center for Computational Sciences and Engineering, Lawrence Berkeley National Laboratory, CA 94720 (United States)

2011-06-10T23:59:59.000Z

344

TYPE Ia SUPERNOVAE: CALCULATIONS OF TURBULENT FLAMES USING THE LINEAR EDDY MODEL  

SciTech Connect

The nature of carbon burning flames in Type Ia supernovae is explored as they interact with Kolmogorov turbulence. One-dimensional calculations using the Linear Eddy Model of Kerstein elucidate three regimes of turbulent burning. In the simplest case, large-scale turbulence folds and deforms thin laminar flamelets to produce a flame brush with a total burning rate given approximately by the speed of turbulent fluctuations on the integral scale, U{sub L} , This is the regime where the supernova explosion begins and where most of its pre-detonation burning occurs. As the density declines, turbulence starts to tear the individual flamelets, making broader structures that move faster. For a brief time, these turbulent flamelets are still narrow compared to their spacing and the concept of a flame brush moving with an overall speed of U{sub L} remains valid. However, the typical width of the individual flamelets, which is given by the condition that their turnover time equals their burning time, continues to increase as the density declines. Eventually, mixed regions almost as large as the integral scale itself are transiently formed. At that point, a transition to detonation can occur. The conditions for such a transition are explored numerically and it is estimated that the transition will occur for densities near 1 x 10{sup 7} g cm{sup -3}, provided the turbulent speed on the integral scale exceeds about 20% sonic. An example calculation shows the details of a detonation actually developing.

Woosley, S. E. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Kerstein, A. R.; Sankaran, V. [Combustion Research Facility, Sandia National Laboratory, Livermore, CA 94551 (United States); Aspden, A. J. [Center for Computational Science and Engineering, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States); Roepke, F. K., E-mail: woosley@ucolick.or, E-mail: arkerst@sandia.go, E-mail: AJAspden@lbl.go, E-mail: fritz@mpa-Garching.mpg.d [Max Planck Institut fuer Astrophysik, Garching (Germany)

2009-10-10T23:59:59.000Z

345

ON THE NATURE OF THE PROGENITOR OF THE Type Ia SN2011fe IN M101  

SciTech Connect

The explosion of a Type Ia supernova, SN2011fe, in the nearby Pinwheel galaxy (M101 at 6.4 Mpc) provides an opportunity to study pre-explosion images and search for the progenitor, which should consist of a white dwarf (WD), possibly surrounded by an accretion disk, in orbit with another star. We report on our use of deep Chandra observations and Hubble Space Telescope observations to limit the luminosity and temperature of the pre-explosion WD. It is found that if the spectrum was a blackbody, then pre-SN WDs with steady nuclear burning of the highest possible temperatures and luminosities are excluded assuming moderate n{sub H} values, but values of kT between roughly 10 eV and 60 eV are permitted even if the WD was emitting at the Eddington luminosity. This allows the progenitor to be an accreting nuclear-burning WD with an expanded photosphere 4-100 times the WD itself, or a super-critically accreting WD blowing off an optically thick strong wind, or possibly a recurrent nova with luminosities an order of magnitude lower than Eddington. The observations are also consistent with a double degenerate scenario, or a spinning down WD that has been spun up by accretion from the donor.

Liu Jifeng [National Astronomical Observatory of China, Beijing 100012 (China); Di Stefano, Rosanne; Wang Tao; Moe, Maxwell [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-04-20T23:59:59.000Z

346

Capturing the Fire: Flame Energetics and Neutronizaton for Type Ia Supernova Simulations  

E-Print Network (OSTI)

We develop and calibrate a realistic model flame for hydrodynamical simulations of deflagrations in white dwarf (Type Ia) supernovae. Our flame model builds on the advection-diffusion-reaction model of Khokhlov and includes electron screening and Coulomb corrections to the equation of state in a self-consistent way. We calibrate this model flame--its energetics and timescales for energy release and neutronization--with self-heating reaction network calculations that include both these Coulomb effects and up-to-date weak interactions. The burned material evolves post-flame due to both weak interactions and hydrodynamic changes in density and temperature. We develop a scheme to follow the evolution, including neutronization, of the NSE state subsequent to the passage of the flame front. As a result, our model flame is suitable for deflagration simulations over a wide range of initial central densities and can track the temperature and electron fraction of the burned material through the explosion and into the expansion of the ejecta.

A. C. Calder; D. M. Townsley; I. R. Seitenzahl; F. Peng; O. E. B. Messer; N. Vladimirova; E. F. Brown; J. W. Truran; D. Q. Lamb

2006-11-01T23:59:59.000Z

347

MEMORANDUM TO: FILE F3on: A 6 IL  

Office of Legacy Management (LM)

F3on: A 6 IL F3on: A 6 IL ---A------------ ALTERNATE CITY: l4v+&a ------- _-__------___-___ STATE: -~-~-- if yes, date contacted _____ & Development a Facility Type 0 Prndurtion scale testing 0 Pilot Scale 0 Makfacturing .a Bench Scale 0 0 Process University 0 0 Theoretical Studies Reseaich Organization cl Sample & Analysis 0 Gopernment Sponsored Facility 0 Other -~~-~~~--_-~~-__----- 0 Production I 0 Disposal/Storage TYPE OF CONTRACT ~------__--_____ q Prime q Subcontract& u Purchase Order Cl Other'infcrmation (i.e., cost + fixed fee, unit price; time & material, +r) ------- ' 'Con+act/Purchase Order # nls.vP ---------------------------- --------------------_____________ CONTRACTING P=3IOD- -----------w-=---T- h,Jn<, ------------------------------- _

348

Proceedings of the 2008 International Conference on Electrical Machines Paper ID 1434 DFIG-Based Wind Turbine Fault Diagnosis  

E-Print Network (OSTI)

Proceedings of the 2008 International Conference on Electrical Machines Paper ID 1434 DFIG for electrical and mechanical fault diagnosis in a DFIG-based wind turbine. The investigated technique Generator (DFIG), Discrete Wavelet Transform (DWT), fault diagnosis. I. INTRODUCTION Wind energy conversion

Paris-Sud XI, Université de

349

ABSTRACT FINAL ID: PP21D-03; TITLE: Quantifying Kinetic Isotope Effect in Speleothems Through Clumped and Oxygen  

E-Print Network (OSTI)

ABSTRACT FINAL ID: PP21D-03; TITLE: Quantifying Kinetic Isotope Effect in Speleothems Through Clumped and Oxygen Isotopes in Laboratory Precipitation Experiments SESSION TYPE: Oral SESSION TITLE: PP21 INSTITUTIONS (ALL): 1. Dept. of Geology & Geophysics, Yale University, New Haven, CT, United States. 2. Inst

350

The Joint Efficient Dark-energy Investigation (JEDI): Measuring the cosmic expansion history from type Ia supernovae  

E-Print Network (OSTI)

JEDI (Joint Efficient Dark-energy Investigation) is a candidate implementation of the NASA-DOE Joint Dark Energy Mission (JDEM). JEDI will probe dark energy in three independent methods: (1) type Ia supernovae, (2) baryon acoustic oscillations, and (3) weak gravitational lensing. In an accompanying paper, an overall summary of the JEDI mission is given. In this paper, we present further details of the supernova component of JEDI. To derive model-independent constraints on dark energy, it is important to precisely measure the cosmic expansion history, H(z), in continuous redshift bins from z \\~ 0-2 (the redshift range in which dark energy is important). SNe Ia at z > 1 are not readily accessible from the ground because the bulk of their light has shifted into the near-infrared where the sky background is overwhelming; hence a space mission is required to probe dark energy using SNe. Because of its unique near-infrared wavelength coverage (0.8-4.2 microns), JEDI has the advantage of observing SNe Ia in the rest frame J band for the entire redshift range of 0 energy are discussed, with special emphasis on the improved precision afforded by the rest frame near-infrared data.

M. M. Phillips; Peter Garnavich; Yun Wang; David Branch; Edward Baron; Arlin Crotts; J. Craig Wheeler; Edward Cheng; Mario Hamuy; for the JEDI Team

2006-06-28T23:59:59.000Z

351

A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey  

E-Print Network (OSTI)

ABRIDGED We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z <0.17 and 27 SN events in 492 maxBCG clusters at 0.1 < z < 0.3$. We find values for the cluster SN Ia rate of $({0.37}^{+0.17+0.01}_{-0.12-0.01}) \\mathrm{SNu}r h^{2}$ and $({0.55}^{+0.13+0.02}_{-0.11-0.01}) \\mathrm{SNu}r h^{2}$ ($\\mathrm{SNu}x = 10^{-12} L_{x\\sun}^{-1} \\mathrm{yr}^{-1}$) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be $({0.31}^{+0.18+0.01}_{-0.12-0.01}) \\mathrm{SNu}r h^{2}$ and $({0.49}^{+0.15+0.02}_{-0.11-0.01})$ $\\mathrm{SNu}r h^{2}$ in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be $({2.04}^{+1.99+0.07}_{-1.11-0.04}) \\mathrm{SNu}r h^{2}$ and $({0.36}^{+0.84+0.01}_...

Dilday, Benjamin; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Frieman, Joshua A; Galbany, Llus; Garnavich, Peter; Goobar, Ariel; Hopp, Ulrich; Ihara, Yutaka; Jha, Saurabh W; Kessler, Richard; Lampeitl, Hubert; Marriner, John; Miquel, Ramon; Moll, Mercedes; Nichol, Robert C; Nordin, Jakob; Riess, Adam G; Sako, Masao; Schneider, Donald P; Smith, Mathew; Sollerman, Jesper; Wheeler, J Craig; stman, Linda; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Pan, Kaike; Simmons, Audrey; Snedden, Stephanie

2010-01-01T23:59:59.000Z

352

DOE - Office of Legacy Management -- Eimco Corp - IL 0-01  

Office of Legacy Management (LM)

Eimco Corp - IL 0-01 Eimco Corp - IL 0-01 FUSRAP Considered Sites Site: Eimco Corp. (IL.0-01 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Palatine , Illinois IL.0-01-1 Evaluation Year: 1987 IL.0-01-1 Site Operations: Conducted laboratory leaf filtration tests IL.0-01-1 Site Disposition: Eliminated - Potential for contamination considered remote based on the limited scope of activities at the site IL.0-01-1 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Test Quantities of Uranium (Yellow Cake Uranium). IL.0-01-1 Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to Eimco Corp. IL.0-01-1 - Memorandum/Checklist; Levine to the File; Subject:

353

DOE - Office of Legacy Management -- Era Tool and Engineering Co - IL 29  

NLE Websites -- All DOE Office Websites (Extended Search)

Era Tool and Engineering Co - IL 29 Era Tool and Engineering Co - IL 29 FUSRAP Considered Sites Site: Era Tool and Engineering Co. (IL.29 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Audi-Tex Industries, Incorporated IL.29-1 Location: 4555 West Addison Street , Chicago , Illinois IL.29-2 Evaluation Year: 1989 IL.29-3 Site Operations: From February 1944 through June 1944, provided personnel, facilities, and equipment to produce machined parts for special equipment, tools, jigs, fixtures, etc., from materials furnished by the University of Chicago IL.29-4 IL.29-5 Site Disposition: Eliminated - Radiation levels below criteria IL.29-2 Radioactive Materials Handled: None indicated Primary Radioactive Materials Handled: None indicated

354

The Rise and Fall of Type Ia Supernova Light Curves in the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We analyze the rise and fall times of Type Ia supernova (SN Ia) light curves discovered by the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. From a set of 391 light curves k-corrected to the rest-frame B and V bands, we find a smaller dispersion in the rising portion of the light curve compared to the decline. This is in qualitative agreement with computer models which predict that variations in radioactive nickel yield have less impact on the rise than on the spread of the decline rates. The differences we find in the rise and fall properties suggest that a single 'stretch' correction to the light curve phase does not properly model the range of SN Ia light curve shapes. We select a subset of 105 light curves well observed in both rise and fall portions of the light curves and develop a '2-stretch' fit algorithm which estimates the rise and fall times independently. We find the average time from explosion to B-band peak brightness is 17.38 {+-} 0.17 days, but with a spread of rise times which range from 13 days to 23 days. Our average rise time is shorter than the 19.5 days found in previous studies; this reflects both the different light curve template used and the application of the 2-stretch algorithm. The SDSS-II supernova set and the local SNe Ia with well-observed early light curves show no significant differences in their average rise-time properties. We find that slow-declining events tend to have fast rise times, but that the distribution of rise minus fall time is broad and single peaked. This distribution is in contrast to the bimodality in this parameter that was first suggested by Strovink (2007) from an analysis of a small set of local SNe Ia. We divide the SDSS-II sample in half based on the rise minus fall value, t{sub r} - t{sub f} {approx} 2 days, to search for differences in their host galaxy properties and Hubble residuals; we find no difference in host galaxy properties or Hubble residuals in our sample.

Hayden, Brian T.; /Notre Dame U.; Garnavich, Peter M.; /Notre Dame U.; Kessler, Richard; /KICP, Chicago /Chicago U., EFI; Frieman, Joshua A.; /KICP, Chicago /Chicago U. /Fermilab; Jha, Saurabh W.; /Stanford U., Phys. Dept. /Rutgers U., Piscataway; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Cinabro, David; /Wayne State U.; Dilday, Benjamin; /Rutgers U., Piscataway; Kasen, Daniel; /UC, Santa Cruz; Marriner, John; /Fermilab; Nichol, Robert C.; /Portsmouth U., ICG /Baltimore, Space Telescope Sci. /Johns Hopkins U.

2010-01-01T23:59:59.000Z

355

AMENDMENT OF SOlLICITATION/MODIFICATlON OF CONTRACT I I. CONTRACr ID CODE  

National Nuclear Security Administration (NNSA)

SOlLICITATION/MODIFICATlON OF CONTRACT I SOlLICITATION/MODIFICATlON OF CONTRACT I I. CONTRACr ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, VA 24506 PAGE I OF 2 PAGES Albuquerque, NM 871 85-5400 I Amarillo, TX 79120 9B. DATED (SEE ITEM 1 1 ) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) DE-AC04-00AL66620 I I IOB. DATED (SEE ITEM 13) 2. AMENDMENTIMODIFICATION NO. MI41 9A. AMENDMENT OF Sol-ICITATION NO. CODE I ~ H L I L I I Y L U U ~ I I - 11. THlS ITEM ONLY APPLIES TO AMENDMENTS OF SOLICITATIONS 1. l l is not The above numbered solicitation is amended as set forth in Item 14. The hour and date specified- receipt of Offers is extendec 3. EFFECTIVE DATE See Block 16C . - extended. 6. ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center

356

DOE-ID Bi-Weekly Summary For June 15 to July 6, 2009  

NLE Websites -- All DOE Office Websites (Extended Search)

6, 2009 6, 2009 EDITOR'S NOTE: The following is a regular summary of operations at DOE's Idaho Site. It has been compiled in response to a request from stakeholders for more information on health, safety and environmental incidents at DOE facilities in Idaho. It also includes a brief summary of accomplishments at the laboratory. The report is broken down by contractor: Advanced Mixed Waste Treatment Project (AMWTP), Idaho Cleanup Project (ICP) and Idaho National Laboratory (INL). This summary will be sent to everyone on INL's regular news release distribution list every other week. To be added to this distribution list, please call Brad Bugger at (208) 526-0833. Advanced Mixed Waste Treatment Project June 15: While retrieving waste at the Advanced Mixed Waste Treatment Project, workers discovered a waste bin that was labeled as potentially containing unexploded ordnance. Previous information about the container indicated it probably did not contain unexploded ordnance, but because of the labeling, that information was not considered definitive. An exclusion zone was established around the container, using guidance from INL explosives experts. Additional information is being gathered to definitively determine the contents of the container. (EM-ID-BBWI-AMWTF-2009-0008).

357

File:03-ID-d - Land Use Permit.pdf | Open Energy Information  

Open Energy Info (EERE)

d - Land Use Permit.pdf d - Land Use Permit.pdf Jump to: navigation, search File File history File usage Metadata File:03-ID-d - Land Use Permit.pdf Size of this preview: 463 × 599 pixels. Other resolution: 464 × 600 pixels. Full resolution ‎(1,275 × 1,650 pixels, file size: 28 KB, MIME type: application/pdf) File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 13:56, 22 August 2013 Thumbnail for version as of 13:56, 22 August 2013 1,275 × 1,650 (28 KB) Abergfel (Talk | contribs) 13:47, 22 August 2013 Thumbnail for version as of 13:47, 22 August 2013 1,275 × 1,650 (27 KB) Abergfel (Talk | contribs) You cannot overwrite this file. Edit this file using an external application (See the setup instructions for more information)

358

AUG-31-04 15,22 FROM,L AND M TECH ID,5052347038 PAGE  

NLE Websites -- All DOE Office Websites (Extended Search)

31-04 15,22 FROM,L AND M TECH 31-04 15,22 FROM,L AND M TECH ID,5052347038 PAGE 3/15 [TX/RX NO 6044] 141003 08/31/2004 TOE 15:22 PAGE 4/15 IC,5052347038 AUG-31-04 15,22 FROM,L AND M TECH PAGE 1 of 9 Supplement Analysis for USE OF THE IO-160B TRANSPORTATION CASK FOR RH-TRUWASTE SHIPMENTS TO WIPP 1.0 INTRODUCTION The U.S. Department of Energy (DOE) is propo~ing to use the CNS lO-160B, Type B Shipping Cask (referred to in this document simply as the lO-160B) to transport remote handled (RH) transuranic (TRU) wastes to the Waste Isolation Pilot Plant (WIPP). DOE originally examined the impacts ofWlPP operations in the Waste Isolation Pilot Plant Disposal Phase Final Supplemental Environmental Impact Statement, DOE/EIS-OO26-S-2, (SEIS~II). This Supplement Analysis (SA) discusses environmental impacts associated with

359

AMENDMENT OF SOlLICITATION/MODIFICATlON OF CONTRACT I I. CONTRACr ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

SOlLICITATION/MODIFICATlON OF CONTRACT I SOlLICITATION/MODIFICATlON OF CONTRACT I I. CONTRACr ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, VA 24506 PAGE I OF 2 PAGES Albuquerque, NM 871 85-5400 I Amarillo, TX 79120 9B. DATED (SEE ITEM 1 1 ) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) DE-AC04-00AL66620 I I IOB. DATED (SEE ITEM 13) 2. AMENDMENTIMODIFICATION NO. MI41 9A. AMENDMENT OF Sol-ICITATION NO. CODE I ~ H L I L I I Y L U U ~ I I - 11. THlS ITEM ONLY APPLIES TO AMENDMENTS OF SOLICITATIONS 1. l l is not The above numbered solicitation is amended as set forth in Item 14. The hour and date specified- receipt of Offers is extendec 3. EFFECTIVE DATE See Block 16C . - extended. 6. ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center

360

THE DETONATION MECHANISM OF THE PULSATIONALLY ASSISTED GRAVITATIONALLY CONFINED DETONATION MODEL OF Type Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

We describe the detonation mechanism composing the 'pulsationally assisted' gravitationally confined detonation (GCD) model of Type Ia supernovae. This model is analogous to the previous GCD model reported in Jordan et al.; however, the chosen initial conditions produce a substantively different detonation mechanism, resulting from a larger energy release during the deflagration phase. The resulting final kinetic energy and {sup 56}Ni yields conform better to observational values than is the case for the 'classical' GCD models. In the present class of models, the ignition of a deflagration phase leads to a rising, burning plume of ash. The ash breaks out of the surface of the white dwarf, flows laterally around the star, and converges on the collision region at the antipodal point from where it broke out. The amount of energy released during the deflagration phase is enough to cause the star to rapidly expand, so that when the ash reaches the antipodal point, the surface density is too low to initiate a detonation. Instead, as the ash flows into the collision region (while mixing with surface fuel), the star reaches its maximally expanded state and then contracts. The stellar contraction acts to increase the density of the star, including the density in the collision region. This both raises the temperature and density of the fuel-ash mixture in the collision region and ultimately leads to thermodynamic conditions that are necessary for the Zel'dovich gradient mechanism to produce a detonation. We demonstrate feasibility of this scenario with three three-dimensional (3D), full star simulations of this model using the FLASH code. We characterized the simulations by the energy released during the deflagration phase, which ranged from 38% to 78% of the white dwarf's binding energy. We show that the necessary conditions for detonation are achieved in all three of the models.

Jordan, G. C. IV; Graziani, C.; Weide, K.; Norris, J.; Hudson, R.; Lamb, D. Q. [Flash Center for Computational Science, University of Chicago, Chicago, IL 60637 (United States); Fisher, R. T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States); Townsley, D. M. [Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487 (United States); Meakin, C. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Reid, L. B. [NTEC Environmental Technology, Subiaco WA 6008 (Australia)

2012-11-01T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

Three-dimensional numerical simulations of Rayleigh-Taylorunstable flames in type Ia supernovae  

SciTech Connect

Flame instabilities play a dominant role in accelerating the burning front to a large fraction of the speed of sound in a Type Ia supernova. We present a three-dimensional numerical simulation of a Rayleigh-Taylor unstable carbon flame, following its evolution through the transition to turbulence. A low Mach number hydrodynamics method is used, freeing us from the harsh time step restrictions imposed by sound waves. We fully resolve the thermal structure of the flame and its reaction zone, eliminating the need for a flame model. A single density is considered, 1.5x107 gm/cc, and half carbon/half oxygen fuel--conditions under which the flame propagated in the flamelet regime in our related two-dimensional study. We compare to a corresponding two-dimensional simulation, and show that while fire-polishing keeps the small features suppressed in two dimensions, turbulence wrinkles the flame on far smaller scales in the three-dimensional case, suggesting that the transition to the distributed burning regime occurs at higher densities in three dimensions. Detailed turbulence diagnostics are provided. We show that the turbulence follows a Kolmogorov spectrum and is highly anisotropic on the large scales, with a much larger integral scale in the direction of gravity. Furthermore, we demonstrate that it becomes more isotropic as it cascades down to small scales. Based on the turbulent statistics and the flame properties of our simulation, we compute the Gibson scale. We show the progress of the turbulent flame through a classic combustion regime diagram, indicating that the flame just enters the distributed burning regime near the end of our simulation.

Zingale, M.; Woosley, S.E.; Rendleman, C.A.; Day, M.S.; Bell, J.B.

2005-01-28T23:59:59.000Z

362

Constraining deflagration models of Type Ia supernovae through intermediate-mass elements  

E-Print Network (OSTI)

The physical structure of a nuclear flame is a basic ingredient of the theory of Type Ia supernovae (SNIa). Assuming an exponential density reduction with several characteristic times we have followed the evolution of a planar nuclear flame in an expanding background from an initial density 6.6 10^7 g/cm3 down to 2 10^6 g/cm3. The total amount of synthesized intermediate-mass elements (IME), from silicon to calcium, was monitored during the calculation. We have made use of the computed mass fractions, X_IME, of these elements to give an estimation of the total amount of IME synthesized during the deflagration of a massive white dwarf. Using X_IME and adopting the usual hypothesis that turbulence decouples the effective burning velocity from the laminar flame speed, so that the relevant flame speed is actually the turbulent speed on the integral length-scale, we have built a simple geometrical approach to model the region where IME are thought to be produced. It turns out that a healthy production of IME involves the combination of not too short expansion times, t_c > 0.2 s, and high turbulent intensities. According to our results it could be difficult to produce much more than 0.2 solar masses of intermediate-mass elements within the deflagrative paradigma. The calculations also suggest that the mass of IME scales with the mass of Fe-peak elements, making it difficult to conciliate energetic explosions with low ejected nickel masses, as in the well observed SN1991bg or in SN1998de. Thus a large production of Si-peak elements, especially in combination with a low or a moderate production of iron, could be better addressed by either the delayed detonation route in standard Chandrasekhar-mass models or, perhaps, by the off-center helium detonation in the sub Chandrasekhar-mass scenario.

D. Garcia-Senz; E. Bravo; R. M. Cabezon; S. E. Woosley

2006-09-15T23:59:59.000Z

363

Revealing Type Ia supernova physics with cosmic rates and nuclear gamma rays  

E-Print Network (OSTI)

Type Ia supernovae (SNIa) remain mysterious despite their central importance in cosmology and their rapidly increasing discovery rate. The progenitors of SNIa can be probed by the delay time between progenitor birth and explosion as SNIa. The explosions and progenitors of SNIa can be probed by MeV nuclear gamma rays emitted in the decays of radioactive nickel and cobalt into iron. We compare the cosmic star formation and SNIa rates, finding that their different redshift evolution requires a large fraction of SNIa to have large delay times. A delay time distribution of the form t^{-1.0 +/- 0.3} provides a good fit, implying 50% of SNIa explode more than ~ 1 Gyr after progenitor birth. The extrapolation of the cosmic SNIa rate to z = 0 agrees with the rate we deduce from catalogs of local SNIa. We investigate prospects for gamma-ray telescopes to exploit the facts that escaping gamma rays directly reveal the power source of SNIa and uniquely provide tomography of the expanding ejecta. We find large improvements relative to earlier studies by Gehrels et al. in 1987 and Timmes & Woosley in 1997 due to larger and more certain SNIa rates and advances in gamma-ray detectors. The proposed Advanced Compton Telescope, with a narrow-line sensitivity ~ 60 times better than that of current satellites, would, on an annual basis, detect up to ~ 100 SNIa (3 sigma) and provide revolutionary model discrimination for SNIa within 20 Mpc, with gamma-ray light curves measured with ~ 10 sigma significance daily for ~ 100 days. Even more modest improvements in detector sensitivity would open a new and invaluable astronomy with frequent SNIa gamma-ray detections.

Shunsaku Horiuchi; John F. Beacom

2010-06-30T23:59:59.000Z

364

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I CONTRACT ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

CONTRACT ID CODE CONTRACT ID CODE Babcock & Wilcox Technical Services Pantex, LLC 9B. DATED (SEE ITEM 11) PO Box 30020 Amarillo, T X 79120 PAGE 1 OF 2 PAGES Albuquerque, NM 87185-5400 I Amarillo, TX 79120 I I DE-AC04-00AL66620 10B. DATED (SEE ITEM 13) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) 2. AMENDMENTIMODIFICATION NO. MI74 9A. AMENDMENT OF SOLICITATION NO. extended. CODE I FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

365

Microsoft Word - DOE-ID-INL-13-006 R1-(INL-13-019 R1-redline).docx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

EC Document No.: DOE-ID-INL-13-006 R1 EC Document No.: DOE-ID-INL-13-006 R1 SECTION A. Project Title: Power Line Configuration - 2013-1 R1 SECTION B. Project Description: Rev 1 Based on recommendations by the Idaho National Laboratory (INL) Cultural Resource Management (CRM) Office, the route of the insulated cables on the ground has been changed. The new route replaces Fig 1 in the original Environmental Checklist (EC) and is shown in the figure, below. The new route has been surveyed by both the INL CRM Office and Biological Resources personnel. All Environmental Aspects and Work Activities identified in the original EC remain valid. All requirements and conditions identified in the original EC remain effective. Original EC This project will install temporary distribution-level power lines between Materials and Fuels Complex (MFC) and Critical Infrastructure

366

KT McDonald IDS-NF Plenary Meeting (RAL) Apr 6, 20132 1 Engineering Issues for the  

E-Print Network (OSTI)

Diagnostics Controls and Interlocks Health and Safety Mechanical Decommissioning Remote Handling and Hot Cells 10,730,099 1.06.07 - Remote Handling Systems 14,348,362 1.06.08 - Controls 3,076,899 1.06.09 - Beam. #12;KT McDonald IDS-NF Plenary Meeting (RAL) Apr 6, 20132 19 We must have an activated-air handling

McDonald, Kirk

367

Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations  

E-Print Network (OSTI)

The light curve of a type Ia supernova decays at a rate set by the beta-decay lifetimes of the Ni-56 and Co-56 produced in the explosion. This makes such a light curve sensitive to the value of the Fermi constant G_F at the time of the supernova. Using data from the CfA Supernova Archive, we measure the dependence of the light curve decay rate on redshift and place a bound on the time variation of G_F of |(dG_F/dt)/G_F| < 10^(-9) / y.

Ferrero, Alejandro

2010-01-01T23:59:59.000Z

368

Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey  

E-Print Network (OSTI)

We use type-Ia supernovae (SNe Ia) discovered by the SDSS-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host galaxy center, using the distance as a proxy for local galaxy properties (local star-formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light-curves using both MLCS2k2 and SALT2, and determine color (AV, c) and light-curve shape (delta, x1) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4-sigma level) finding is that the average fitted AV from MLCS2k2 and c from SALT2 decrease with the proj...

Galbany, Lluis; Ostman, Linda; Brown, Peter J; Cinabro, David; D'Andrea, Chris B; Frieman, Joshua; Jha, Saurabh W; Marriner, John; Nichol, Robert C; Nordin, Jakob; Olmstead, Matthew D; Sako, Masao; Schneider, Donald P; Smith, Mathew; Sollerman, Jesper; Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Simmons, Audrey; Shelden, Alaina

2012-01-01T23:59:59.000Z

369

Metodi per il miglioramento continuo della qualit. Il caso di Cesab Carrelli elavatori S.p.A (gruppo Toyota Material Handling).  

E-Print Network (OSTI)

??La tesi affronta diversi argomenti, legati ai metodi e agli strumenti per il miglioramento continuo della Qualit all'intern del mondo Toyota. Ho approfondito dunque i (more)

Dal Pra', Sarah

2010-01-01T23:59:59.000Z

370

The IL-9 receptor gene (IL9R): Genomic structure, chromosomal localization in the pseudoautosomal region of the long arm of sex chromosomes, and identification of IL9R pseudogenes at 9qter, 10pter, 16pter, 18pter  

Science Conference Proceedings (OSTI)

Cosmids containing the human IL-9 receptor (R) gene (IL9R) have been isolated from a genomic library using the IL9R cDNA as a probe. We have shown that the human IL9R gene is composed of 11 exons and 10 introns, stretching over {approx} 17 kb, and is located within the pseudoautosomal region of the Xq and Yq chromosome, in the vicinity of the telomere. Analysis of the 5` flanking region revealed multiple transcription initiation sites as well as potential binding motifs for AP1, AP2, AP3, Sp1, and NF-kB, although this region lacks a TATA box. Using the human IL9R cosmid as a probe to perform fluorescence in situ hybridization, additional signals were identified in the subtelomeric regions of chromosomes 9q, 10p, 16p, and 18p. IL9R homologs located on chromosomes 9 and 18 were partially characterized, while those located on chromosomes 16 and 10 were completely sequenced. Although they are similiar to the IL9R gene ({approx} 90% identity), none of these copies encodes a functional receptor: none of them contains sequences homologous to the 5` flanking region or exon 1 of the IL9R gene, and the remaining ORFs have been inactivated by various point mutations and deletions. Taken together, our results indicate that the IL9R gene is located at Xq28 and Yq12, in the long arm pseudoautosomal region, and that four IL9R pseudogenes are located on 9q34, 10p15, 16p13.3 and 18p11.3, probably dispersed as the result of translocations during evolution. 42 refs., 6 figs., 3 tabs.

Kermouni, A.; Godelaine, D.; Lurquin, C.; Szikora, J.P. [Ludwig Institute for Cancer Research, Brussels (Belgium)] [and others

1995-09-20T23:59:59.000Z

371

Job Title Organization Name Type End Date Job ID Intern -Industrial Engineer Jabil Circuit, Inc. Intern 8/15/2012 36012  

E-Print Network (OSTI)

Job Title Organization Name Type End Date Job ID Intern - Industrial Engineer Jabil Circuit, Inc HVAC Equipment Technical Support Tom Barrow Co. Full-time 7/31/2012 36332 Internship HQ Inc Intern 9

Meyers, Steven D.

372

T-559: Stack-based buffer overflow in oninit in IBM Informix Dynamic Server (IDS) 11.50 allows remote execution  

Energy.gov (U.S. Department of Energy (DOE))

Stack-based buffer overflow in oninit in IBM Informix Dynamic Server (IDS) 11.50 allows remote execution attackers to execute arbitrary code via crafted arguments in the USELASTCOMMITTED session environment option in a SQL SET ENVIRONMENT statement

373

6/10/12 Researchers Develop New Method to Measure Bubble Size Distribution in Pipelines 1/2www.azomining.com/news.aspx?newsID=6367  

E-Print Network (OSTI)

.azomining.com/news.aspx?newsID=6367 0 Posted in | Natural Gas | Oil Shale Read in | English | Español | Français | Deutsch | Português

Sóbester, András

374

Enter Search Term Enter Drill Deeper or ED Online ID Home Subscribe Back Issues Design FAQs Ideas for Design Power Analog  

E-Print Network (OSTI)

Enter Search Term Enter Drill Deeper or ED Online ID Home Subscribe Back Issues Design FAQs Ideas Subscribe to Electronic Design UPDATE (Archive) Email: Enter Email Click to view this week's welcome screen

Rogers, John A.

375

DOE - Office of Legacy Management -- Morse Chemical Co - IL 0-05  

Office of Legacy Management (LM)

Morse Chemical Co - IL 0-05 Morse Chemical Co - IL 0-05 FUSRAP Considered Sites Site: MORSE CHEMICAL CO. (IL.0-05 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: 8 South Michigan Avenue , Chicago , Illinois IL.05-1 Evaluation Year: 1987 IL.05-3 Site Operations: Submitted a bid to AEC for thorium work; proposal was not accepted; no indication work done for a DOE predecessor at this site. IL.05-3 Site Disposition: Eliminated - No Authority - No work for a DOE predecessor was done at the site IL.05-2 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Thorium Radiological Survey(s): None Indicated Site Status: Eliminated from consideration under FUSRAP Also see Documents Related to MORSE CHEMICAL CO.

376

FAILED-DETONATION SUPERNOVAE: SUBLUMINOUS LOW-VELOCITY Ia SUPERNOVAE AND THEIR KICKED REMNANT WHITE DWARFS WITH IRON-RICH CORES  

SciTech Connect

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosions of carbon-oxygen (C-O) white dwarfs (WDs). The single-degenerate scenario is a well-explored model of SNe Ia where unstable thermonuclear burning initiates in an accreting, Chandrasekhar-mass WD and forms an advancing flame. By several proposed physical processes, the rising, burning material triggers a detonation, which subsequently consumes and unbinds the WD. However, if a detonation is not triggered and the deflagration is too weak to unbind the star, a completely different scenario unfolds. We explore the failure of the gravitationally confined detonation mechanism of SNe Ia, and demonstrate through two-dimensional and three-dimensional simulations the properties of failed-detonation SNe. We show that failed-detonation SNe expel a few 0.1 M{sub Sun} of burned and partially burned material and that a fraction of the material falls back onto the WD, polluting the remnant WD with intermediate-mass and iron-group elements that likely segregate to the core forming a WD whose core is iron rich. The remaining material is asymmetrically ejected at velocities comparable to the escape velocity from the WD, and in response, the WD is kicked to velocities of a few hundred km s{sup -1}. These kicks may unbind the binary and eject a runaway/hypervelocity WD. Although the energy and ejected mass of the failed-detonation SN are a fraction of typical thermonuclear SNe, they are likely to appear as subluminous low-velocity SNe Ia. Such failed detonations might therefore explain or are related to the observed branch of peculiar SNe Ia, such as the family of low-velocity subluminous SNe (SN 2002cx/SN 2008ha-like SNe).

Jordan, George C. IV; Van Rossum, Daniel R. [Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637 (United States); Perets, Hagai B. [Physics Department, Technion, Israel Institute of Technology, Haifa 32000 (Israel); Fisher, Robert T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States)

2012-12-20T23:59:59.000Z

377

TYPE Ia SUPERNOVA PROPERTIES AS A FUNCTION OF THE DISTANCE TO THE HOST GALAXY IN THE SDSS-II SN SURVEY  

Science Conference Proceedings (OSTI)

We use Type Ia supernovae (SNe Ia) discovered by the Sloan Digital Sky Survey-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host-galaxy center, using the distance as a proxy for local galaxy properties (local star formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light curves using both MLCS2K2 and SALT2, and determine color (A{sub V} , c) and light-curve shape ({Delta}, x{sub 1}) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4{sigma} level) finding is that the average fitted A{sub V} from MLCS2K2 and c from SALT2 decrease with the projected distance for SNe Ia in spiral galaxies. We also find indications that supernovae (SNe) in elliptical galaxies tend to have narrower light curves if they explode at larger distances, although this may be due to selection effects in our sample. We do not find strong correlations between the residuals of the distance moduli with respect to the Hubble flow and the galactocentric distances, which indicates a limited correlation between SN magnitudes after standardization and local host metallicity.

Galbany, Lluis; Miquel, Ramon; Oestman, Linda [Institut de Fisica d'Altes Energies, Universitat Autonoma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Brown, Peter J.; Olmstead, Matthew D. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); D'Andrea, Chris B.; Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX (United Kingdom); Frieman, Joshua [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellise Avenue, Chicago, IL 60637 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, John [Center for Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Nordin, Jakob [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720 (United States); Sako, Masao [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7535, Cape Town (South Africa); Sollerman, Jesper [Oskar Klein Centre, Department of Astronomy, AlbaNova, SE-106 91 Stockholm (Sweden); Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard, E-mail: lluis.galbany@ist.utl.pt [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); and others

2012-08-20T23:59:59.000Z

378

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rat...

Dilday, Benjamin; Frieman, J A; Holtzman, J; Marriner, J; Miknaitis, G; Nichol, R C; Romani, R; Sako, M; Bassett, B; Becker, A; Cinabro, D; De Jongh, F; Depoy, D L; Doi, M; Garnavich, P M; Hogan, C J; Jha, S; Konishi, K; Lampeitl, H; Marshall, J L; McGinnis, D; Prieto, J L; Riess, A G; Richmond, M W; Schneider, D P; Smith, M; Takanashi, N; Tokita, K; van der Heyden, K; Zheng, N Yasuda C; Barentine, J; Brewington, H; Choi, C; Crotts, A; Dembicky, J; Harvanek, M; Im, M; Ketzeback, W; Kleinman, S J; Krzesi?ski, J; Long, D C; Malanushenko, E; Malanushenko, V; McMillan, R J; Nitta, A; Pan, K; Saurage, G; Snedden, S A; Watters, S; Wheeler, J C; York, D

2008-01-01T23:59:59.000Z

379

Blockage of IL-6 secretion in glia by lead and mercury  

E-Print Network (OSTI)

Mercury (Hg) and lead (Pb) are toxic to the development and function of the central nervous system (CNS). Interleukin-6 (IL 6) produced by astroglia protects neurons from damage in many progressive degenerative disorders. IL-6 secretion is chaperoned by a 78 kD glucose-regulated protein (GRP78), which is an ER-chaperone protein involved in protein folding, assembly, and trafficking. We hypothesized that Pb and Hg could target GRP78 and thereby block IL-6 secretion from astroglia. In this report, we constructed an IL-6-EGFP chimera and transiently transfected rat C6 glioma cells and rat primary astroglia. IL-6-EGFP signal in transfected cultures exposed to Pb, Hg, or anti-oligos against GRP78 was detected with a bio-image fluorescence microscope. Data of the bio-image analysis showed that the retention of IL-6-EGFP in both astroglia and C6 cells transfected with IL-6-EGFP was at an undetectable level. However, the IL-6-EGFP signal in these cultures, while exposed to Pb (0-10 ?M) or Hg (0-10 ?M) for 24 hours, apparently increased, suggesting that Pb or Hg could block IL-6 secretion from astroglia. Furthermore, when these transfected cultures were exposed to anti-oligos against GRP78, as expected, the retention of IL-6-EGFP within the cultures increased. In order to quantify the increase of IL-6-EGFP retention, we used ELISA to detect IL-6 levels in the medium of non-transfected astroglia exposed to Pb (0-100 ?M) and Hg (0-10 ?M). Data showed that IL-6 levels in the medium decreased when the primary astrocyte cultures were exposed to Pb or Hg, suggesting that the increased retention results in part from a decrease in IL-6 secretion. We used an immunocytochemistry assay as an additional approach for quantifying IL-6 amounts of cells treated or not treated with metals. The immunocytochemistry data concurred with the ELISA findings. These data, together with our previous studies, suggest that Pb and Hg may target GRP78, thereby reducing the amount of IL-6 secreted from astroglia. The decrease in IL-6 secretion prevents this cytokine from doing its job of protecting and restoring neighboring neural tissue.

Pourrajabi, Nima Matthew

2003-01-01T23:59:59.000Z

380

Making the Standard Candle: A study of how the progenitor white dwarf modulates the peak luminosity of type Ia supernovae  

SciTech Connect

The goals of the proposed research as stated in the proposal were to: Build a suite of one-dimensional initial models of different metallicities and central densities. Using the improved flame capturing scheme, simulate the explosion of a white dwarf with embedded Lagrangian tracer particles, and post-process the thermal histories of the tracers to reconstruct the nucleosynthesis of the explosion. Survey the effects of a changing progenitor metallicity on the isotopic yields. Of particular interest is 1) whether the linear relation between the mass of 56Ni synthesized and the pro- genitor metallicity is moderated by the effect of electron captures in the core; and 2) how a varying central density alters the relation between metallicity and 56Ni mass. Using these results, examine how the observed metallicity distribution would affect the brightness distribution of SNe Ia and the isotopic ratios about the Fe-peak.

Brown, Edward F [Michigan State University

2010-01-21T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
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381

Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae  

E-Print Network (OSTI)

We estimate the solar system motion relative to the cosmic microwave background using type Ia supernovae (SNe) measurements. We take into account the correlations in the error bars of the SNe measurements arising from correlated peculiar velocities. Without accounting for correlations in the peculiar velocities, the SNe data we use appear to detect the peculiar velocity of the solar system at about the 3.5 sigma level. However, when the correlations are correctly accounted for, the SNe data only detects the solar system peculiar velocity at about the 2.5 sigma level. We forecast that the solar system peculiar velocity will be detected at the 9 sigma level by GAIA and the 11 sigma level by the LSST. For these surveys we find the correlations are much less important as most of the signal comes from higher redshifts where the number density of SNe is insufficient for the correlations to be important.

Christopher Gordon; Kate Land; Anze Slosar

2007-11-27T23:59:59.000Z

382

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I I, CONTRACT ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

I, CONTRACT ID CODE I, CONTRACT ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, V A 24506 PAGE I OF 2 PAGES Albuquerque, NM 87185-5400 I Amarillo, TX 79120 9B. DATED (SEE ITEM I I ) 8. NAME AND ADDRESS OF CONTRACTOR (No.. street, county, state, ZIP Code) I ( DE-AC04-00AL66620 10B. DATED (SEE ITEM 13) 2. AMENDMENTIMODIFICATION NO. M I 3 8 9A. AMENDMENT OF SOLICITATION NO. extended. 3. EFFECTIVE DATE See Block 16C CODE I FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

383

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I I. CONTRA'T ID CODE  

National Nuclear Security Administration (NNSA)

CONTRA'T ID CODE CONTRA'T ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, V A 24506 PAGE I OF 2 PAGES Albuquerque, NM 871 85-5400 / Amarillo, TX 79120 I I 9B. DATED (SEE ITEM 11) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) I 10A. MODIFICATION OF CONTRACTIORDER NO. 2. AMENDMENTIMODIFICATION NO. M I 0 8 9A. AMENDMENT OF SOLICITATION NO. DE-AC04-00AL66620 1 1 108. DATED (SEE ITEM 13) 3. EFFECTIVE DATE See Block 16C Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

384

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I I. CONTRA'T ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

CONTRA'T ID CODE CONTRA'T ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, V A 24506 PAGE I OF 2 PAGES Albuquerque, NM 871 85-5400 / Amarillo, TX 79120 I I 9B. DATED (SEE ITEM 11) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) I 10A. MODIFICATION OF CONTRACTIORDER NO. 2. AMENDMENTIMODIFICATION NO. M I 0 8 9A. AMENDMENT OF SOLICITATION NO. DE-AC04-00AL66620 1 1 108. DATED (SEE ITEM 13) 3. EFFECTIVE DATE See Block 16C Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

385

Electromagnetics - DC/Low Frequency  

Science Conference Proceedings (OSTI)

... GA [200403- 0] ID. Idaho National Laboratory -Calibration Services Dept., Idaho Falls, ID [200115- 0] IL. S. Himmelstein ...

2013-07-26T23:59:59.000Z

386

Il fenomeno dei fan nel mercato della musica. Analisi netnografica dei seguaci italiani di Bruce Springsteen.  

E-Print Network (OSTI)

??Lo studio ha ad oggetto la comunit dei fan italiani di Bruce Springsteen. Dopo aver analizzato la letteratura e descritto il fenomeno dei fan e (more)

Gallo, Sara

2007-01-01T23:59:59.000Z

387

Structural comparison and chromosomal localization of the human and mouse IL-13 genes  

SciTech Connect

The genomic structure of the recently described cytokine IL-13 has been determined for both human and mouse genes. The nucleotide sequence of a 4.6-kb DNA segment of the human gene is described. The human IL-13 gene (IL 13) occurs as a single copy in the haploid genome and maps to human chromosome 5. A 4.3-kb DNA fragment of the mouse IL-13 gene (Il 13) has been sequenced and found to occur as a single copy, mapping to mouse chromosome 11. Intrachromosomal mapping studies revealed that both genes contain four exons and three introns and show a high degree of sequence identify throughout their length. Potential recognition sequences for transcription factors that are present in the 5'-flanking region and are conserved between both genes include IFN-responsive elements, binding sites for AP-1, AP-2, and AP-3, an NF-lL 6 site, and a TATA-like sequence. Both genes map to chromosomal locations adjacent to genes encoding other cytokines, including IL-3, GM-CSF, IL-5, and IL-4 suggesting that IL-13 is another member of this cytokine gene family that may have arisen by gene duplication. 26 refs., 5 figs., 3 tabs.

McKenzie, A.N.J.; Sato, A.; Doyle, E.L.; Zurawski, G. (DNAX Research Institute of Cellular and Molecular Biology, Palo Alto, CA (United States)); Li, X.; Milatovich, A.; Francke, U. (Stanford Univ. Medical School, CA (United States)); Largaespada, D.A.; Copeland, N.G.; Jenkins, N.A. (National Cancer Institute, Frederick, MD (United States))

1993-06-15T23:59:59.000Z

388

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I CONTRACT ID CODE  

National Nuclear Security Administration (NNSA)

I CONTRACT ID CODE Babcock & Wilcox Technical Services Pantex, LLC 9B. DATED (SEE ITEM 11) PO Box 30020 Amarillo, T X 79120 PAGE 1 OF 2 PAGES Albuquerque, NM 87185-5400 I Amarillo, TX 79120 I I DE-AC04-00AL66620 10B. DATED (SEE ITEM 13) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) 2. AMENDMENTIMODIFICATION NO. MI74 9A. AMENDMENT OF SOLICITATION NO. extended. CODE I FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

389

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT ID PAGE I OF 2  

NLE Websites -- All DOE Office Websites (Extended Search)

/ ' / ' ID PAGE I OF 2 PAGES - . Albuquerque, NM 87185-5400 I Amarillo, TX 79120 I ( DE-AC04-00AL66620 10B. DATED (SEE ITEM 13) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) Babcock & W ~ ~ C O X Technical Services Pantex, LLC 800 Main Street Lynchburg, VA 24505 2 . AMENDMENTIMODIFICATION NO. MI50 9A. AMENDMENT OF SOLICITATION NO. 9B. DATED (SEE ITEM 11) 10A. MODIFICATION OF CONTRACTIORDER NO. Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

390

RESULTS OF RADIOLOGICAL I'IEASUREMENTS HIGHT{AYS 18 AI.ID IO4 IN NIAGARA  

Office of Legacy Management (LM)

9s' 9s' RESULTS OF RADIOLOGICAL I'IEASUREMENTS HIGHT{AYS 18 AI.ID IO4 IN NIAGARA az76 rl//.ry' ORNL/RASA.85/ 40 TAKEN AT JUNCTION FALLS, NEH YORK Accesr to the information in thit rcport ir limiled to tho!' inOllateO on tho dl3tribution li3t and to OePartment ot Encrgy and Oepartmcnt ol Enotgy Gontracton This report was prepared as an account of work sponsored by an agency of the United States Government. Neitherth€ U nited StatesGovernment norany agency thereof, nor any of their employees, makes any warranty, express or implied' or assumes any legal liability or responsibility for the accuracy, completenessi or usefulness of any information, apparatus, product, or,process disclosed, or represents that its usewould not inlringe privately owned rights" Reference herein

391

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT I ' CONTRACT ID CODE  

National Nuclear Security Administration (NNSA)

' ' CONTRACT ID CODE BWXT Pantex, LLC Route 726, Mt. Athos Road Lynchburg, VA 24506 PAGE 1 OF 12 PAGES 9B. DATED (SEE ITEM 11) 5. PROJECT NO. (If applicable) 4. REQUlSlTlONlPURCHASE REQ. NO. 2. AMENDMENTIMODIFICATION NO. MI39 extended. 6. ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center Property and M&O Contract Support Department P.O. Box 5400 Albuquerque, NM 871 85-5400 3. EFFECTIVE DATE See Block 16C CODE I FACILITY CODE Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the

392

AMENDMENT OF SOLlClTATlONlMODlFlCATlON OF CONTRACT ID PAGE I OF 2  

National Nuclear Security Administration (NNSA)

/ ' / ' ID PAGE I OF 2 PAGES - . Albuquerque, NM 87185-5400 I Amarillo, TX 79120 I ( DE-AC04-00AL66620 10B. DATED (SEE ITEM 13) 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) Babcock & W ~ ~ C O X Technical Services Pantex, LLC 800 Main Street Lynchburg, VA 24505 2 . AMENDMENTIMODIFICATION NO. MI50 9A. AMENDMENT OF SOLICITATION NO. 9B. DATED (SEE ITEM 11) 10A. MODIFICATION OF CONTRACTIORDER NO. Offers must acknowledge receipt of this amendment prior to the hour and date specified in the solicitation as amended, by one of the following methods: (a) By completing Items 8 and 15, and returning - copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR

393

#iWNCD W ONTAININO Il@MQWm;  

Office of Legacy Management (LM)

decontmlmtlon proceam takee longer than originally anticipated decontmlmtlon proceam takee longer than originally anticipated 'U&e order .are urgently required to prevent a shutdown. "Z, mo-1 ' 2lda.p - from 4a6-55 to a possible 4-5-55 based on the receipt of vendor's plantby 1-22-55. #iWNCD W ONTAININO Il@MQWm; ;g hours worked; Hours worked will be observed and under the control of . . M%-.'E.Section . (Copy of Vendorts letter of quotation dated l/5/55 is VAWNWWXlINALORDEt :Y $ u(,507.60 upoDRpuiI9APPROPAk &movND* 0 3375.00 (rllaxlmum) Field approval contained in .!lT Savannah.A L, 1 Not required., Gosney to Hutton. (The Operating Departmeni Ato& Bad-~ Cadeaiaa agrees on the urgency and the need for autho -,. ,n - this premiumpayment.) l-13-55 loiD. 365 duPont l topa 4-26-55 pa and the faettbat

394

A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae  

E-Print Network (OSTI)

The dynamics of the explosive burning process is highly sensitive to the flame speed model in numerical simulations of type Ia supernovae. Based upon the hypothesis that the effective flame speed is determined by the unresolved turbulent velocity fluctuations, we employ a new subgrid scale model which includes a localised treatment of the energy transfer through the turbulence cascade in combination with semi-statistical closures for the dissipation and non-local transport of turbulence energy. In addition, subgrid scale buoyancy effects are included. In the limit of negligible energy transfer and transport, the dynamical model reduces to the Sharp-Wheeler relation. According to our findings, the Sharp-Wheeler relation is insuffcient to account for the complicated turbulent dynamics of flames in thermonuclear supernovae. The application of a co-moving grid technique enables us to achieve very high spatial resolution in the burning region. Turbulence is produced mostly at the flame surface and in the interior ash regions. Consequently, there is a pronounced anisotropy in the vicinity of the flame fronts. The localised subgrid scale model predicts significantly enhanced energy generation and less unburnt carbon and oxygen at low velocities compared to earlier simulations.

W. Schmidt; J. C. Niemeyer; W. Hillebrandt; F. K. Roepke

2006-01-23T23:59:59.000Z

395

Early and late time VLT spectroscopy of SN 2001el - progenitor constraints for a type Ia supernova  

E-Print Network (OSTI)

We present early time high-resolution (VLT/UVES) and late time low-resolution (VLT/FORS) optical spectra of the normal type Ia supernova, SN 2001el. The high-resolution spectra were obtained 9 and 2 days before (B-band) maximum light in order to detect narrow hydrogen and/or helium emission lines from the SN CSM. No such lines were detected in our data. We therefore use photoionisation models to derive upper limits of 1x10^-5 and 6x10^-5 Msol/yr, assuming wind velocities of 10 and 50 km/s, respectively, for the mass loss rate from the progenitor system of SN 2001el. This excludes a symbiotic star in the upper mass loss rate regime from being the progenitor of SN 2001el. The low-resolution spectrum was obtained in the nebular phase of the supernova, \\~400 days after the maximum light, to search for any hydrogen rich gas originating from the SN progenitor system. However, we see no signs of Balmer lines in our spectrum. Therefore, we model the late time spectra to derive an upper limit of ~0.03 Msol for solar a...

Mattila, S; Sollerman, J; Kozma, C; Baron, E; Fransson, C; Leibundgut, B; Nomoto, K

2005-01-01T23:59:59.000Z

396

Enter Search Term Enter ED Online ID Advanced Search | Help Electronic Design Home Recent Articles Back Issues Featured Vendors Discussion Forums Subscribe / Renew  

E-Print Network (OSTI)

Enter Search Term Enter ED Online ID Advanced Search | Help Electronic Design Home Recent Articles- analyzer vendors have kept pace with industry demands in terms of speed and functionality. However, in many tools. Logic- analyzer vendors have kept pace with industry demands in terms of speed and functionality

LaMeres, Brock J.

397

Signaling thresholds govern heterogeneity in IL-7-receptor-mediated responses of nave CD8? T cells  

E-Print Network (OSTI)

Variable sensitivity to T-cell-receptor (TCR)- and IL-7-receptor (IL-7R)-mediated homeostatic signals among nave T cells has thus far been largely attributed to differences in TCR specificity. We show here that even when ...

Palmer, Megan Joan

398

Ionizing radiation induces IL-6-production by human fibroblasts involving activation of nuclear factor-. kappa. B  

Science Conference Proceedings (OSTI)

The authors report that human lung fibroblasts respond to X-ray treatment with release of interleukin (IL) -6. Synthesis of IL-6 upon ionizing radiation is preceded by an increase of IL-6 transcript levels resulting from transcriptional activation of the IL-6 gene. Analysis of deleted fragments of the IL-6 promoter revealed that transcriptional induction of the IL-6 promoter is due to enhanced binding activity of the transcription factor NF-kB. Although AP-1 does not participate in the rapid induction of the IL-6 promoter its binding activity is also enhanced upon XRT. In contrast to binding kinetics observed with NF-kB, AP-1 binding upon XRT. In contrast to binding kinetics observed with NF-kB- and the AP-1 recognition sequence, conferred inducibility by XRT to a heterologous promoter, with reporter gene activity being maximal 24 hours or 48 hours upon XRT, respectively. Sequential activation of two distinct transcription factors might thus contribute to synchronize transcriptional activation of different genes participating in the X-ray response.

Brach, M.A.; Gruss, H.J.; Kaisho, Tsuneyasu; Asano, Yoshinobu; Vos, Sven de; Mertelsmann, R.; Hirano, Toshio; Herrmann, F. (Univ. of Freiburg (Germany) Osaka Univ. (Japan))

1992-02-26T23:59:59.000Z

399

TCL: Comandi utili versione 2.1. [open stringa mode] restituisce il descrittore di un file aperto (di nome stringa) in modalit "riscrittura" (se mode w) o in  

E-Print Network (OSTI)

TCL: Comandi utili versione 2.1. [open stringa mode] restituisce il descrittore di un file aperto]) restituisce il nome del file .tcl corrente [$ns get-ns-traceall] restituisce il descrittore del file di trace

Bregni, Stefano

400

EVOLUTION OF POST-IMPACT COMPANION STARS IN SN Ia REMNANTS WITHIN THE SINGLE-DEGENERATE SCENARIO  

Science Conference Proceedings (OSTI)

The nature of the progenitor systems of Type Ia supernovae is still uncertain. One way to distinguish between the single-degenerate scenario and double-degenerate scenario is to search for the post-impact remnant star. To examine the characteristics of the post-impact remnant star, we have carried out three-dimensional hydrodynamic simulations of supernova impacts on main-sequence-like stars. We explore the evolution of the post-impact remnants using the stellar evolution code MESA. We find that the luminosity and radius of the remnant star dramatically increase just after the impact. After the explosion, post-impact companions continue to expand on a progenitor-dependent timescale of {approx}10{sup 2.5}-10{sup 3} years before contracting. It is found that the time evolution of the remnant star is dependent not only on the amount of energy absorbed but also on the depth of the energy deposition. We examine the viability of the candidate star Tycho G as the possible remnant companion in Tycho's supernova by comparing it to the evolved post-impact remnant stars in our simulations. The closest model in our simulations has a similar effective temperature, but the luminosity and radius are twice as large. By examining the angular momentum distribution in our simulations, we find that the surface rotational speed could drop to {approx}10 km s{sup -1} if the specific angular momentum is conserved during the post-impact evolution, implying that Tycho G cannot be completely ruled out because of its low surface rotation speed.

Pan, Kuo-Chuan; Ricker, Paul M. [Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States); Taam, Ronald E., E-mail: kpan2@illinois.edu, E-mail: pmricker@illinois.edu, E-mail: taam@northwestern.edu [Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 (United States)

2012-11-20T23:59:59.000Z

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

NGA_99fin.vp  

Gasoline and Diesel Fuel Update (EIA)

9 9 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 18. Average Price of Natural Gas Delivered to U.S. Onsystem Industrial Consumers, 1999 (Dollars per Thousand Cubic Feet) Figure 19. Average Price of Natural Gas Delivered to U.S. Electric Utilities, 1999 (Dollars per Thousand Cubic Feet) Figure Sources: Federal Energy Regulatory Commission (FERC), Form FERC-423, "Monthly Report of Cost and Quality of Fuels for Electric Plants," and Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental

402

C:\ANNUAL\VENTCHAP.V8\NGAla1109.vp  

Gasoline and Diesel Fuel Update (EIA)

Energy Energy Information Administration / Natural Gas Annual 2000 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Note: Commercial prices include natural gas delivered for use as vehicle fuel. Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." 0.00-1.99 2.00-3.99 4.00-5.99 6.00-7.99 8.00-9.99 10.00-11.99 12.00+ 0.00-1.99 2.00-3.99 4.00-5.99 6.00-7.99 8.00-9.99 10.00-11.99 12.00+ 17. Average Price of Natural Gas Delivered to U.S. Residential

403

NGA98fin5.vp  

Gasoline and Diesel Fuel Update (EIA)

8 8 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 18. Average Price of Natural Gas Delivered to U.S. Onsystem Industrial Consumers, 1998 (Dollars per Thousand Cubic Feet) Figure 19. Average Price of Natural Gas Delivered to U.S. Electric Utilities, 1998 (Dollars per Thousand Cubic Feet) Figure Sources: Federal Energy Regulatory Commission (FERC), Form FERC-423, "Monthly Report of Cost and Quality of Fuels for Electric Plants," and Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental

404

C:\ANNUAL\VENTCHAP.V8\NGAla1109.vp  

Gasoline and Diesel Fuel Update (EIA)

2000 2000 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-3.99 4.00-5.99 6.00-7.99 8.00-9.99 10.00-11.99 12.00+ NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-3.99 4.00-5.99 6.00-7.99 8.00-99.99 10.00-11.99 12.00+ 19. Average Price of Natural Gas Delivered to U.S. Onsystem Industrial Consumers, 2000 (Dollars per Thousand Cubic Feet) Figure 20. Average Price of Natural Gas Delivered to U.S. Electric Utilities, 2000 (Dollars per Thousand Cubic Feet) Figure Sources: Federal Energy Regulatory Commission (FERC), Form FERC-423, "Monthly Report of Cost and Quality of Fuels for Electric Plants," and Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural

405

NGA_99fin.vp  

Gasoline and Diesel Fuel Update (EIA)

9 9 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Note: Commercial prices include natural gas delivered for use as vehicle fuel. Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 16. Average Price of Natural Gas Delivered to U.S. Residential Consumers, 1999 (Dollars per Thousand Cubic Feet) Figure

406

C:\ANNUAL\VENTCHAP.V8\NGA.VP  

Gasoline and Diesel Fuel Update (EIA)

8 8 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Note: Commercial prices include natural gas delivered for use as vehicle fuel. Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 16. Average Price of Natural Gas Delivered to U.S. Residential Consumers, 1997 (Dollars per Thousand Cubic Feet) Figure

407

NGA98fin5.vp  

Gasoline and Diesel Fuel Update (EIA)

1998 1998 NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC Note: Commercial prices include natural gas delivered for use as vehicle fuel. Source: Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 16. Average Price of Natural Gas Delivered to U.S. Residential Consumers, 1998 (Dollars per Thousand Cubic Feet) Figure

408

DFPARThIl!NT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERlIfiNA...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DFPARThIlNT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERlIfiNATION Page 1 of3 RECIPIENT :State of Hawaii DBEOT STATE : HI PROJECf TITLE: Loan Loss Reserve Funding...

409

Bakken Formation Producing Wells W il sto nBa North Dakota ...  

U.S. Energy Information Administration (EIA)

USA CANADA SD MT ND Saskatchewan Manitoba Dunn Ward Dawson McLean McKenzie Morton W il ams Stark Richland R os ev lt Mountrail Divide Prairie McHenry Burke Sheridan

410

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

822 822 Idaho National Laboratory Stand-Off Experiment (SOX) Range Environmental Assessment Final March 2011 DOE/EA-1822 Idaho National Laboratory Stand-Off Experiment (SOX) Range Environmental Assessment Final March 2011 Prepared for the U.S. Department of Energy Idaho Operations Office i CONTENTS ACRONYMS ............................................................................................................................................... iii GLOSSARY ................................................................................................................................................. v EXECUTIVE SUMMARY ........................................................................................................................ vii

411

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Data Report on Data Report on Corrosion Testing of Stainless Steel SNF Storage Canisters Prepared for U.S. Department of Energy Used Fuel Disposition Campaign D.G. Enos, C.R. Bryan, and K. M. Norman Sandia National Laboratories September 30, 2013 FCRD-UFD-2013-000324 SAND2013-8314P Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04- 94AL85000. DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty,

412

Beamline 29-ID  

NLE Websites -- All DOE Office Websites (Extended Search)

IEX Milestones(4/29/2013) IEX Milestones(4/29/2013) • Spring 2012 ✓ Completion of the IEX EM-VPU insertion device (photos) ✓ Installation of EM-VPU in the storage ring (photo1, photo2) ✓ Installation of high heat-load mirrors M0/M1 (photo) • Summer 2012 ✓ Testing of various polarization mode of EM-VPU with stored beam ✓ Installation of vacuum transport, support tables and diagnostic component; implementation of beamline controls and safety systems (cleanroom, FOE progress, FOE progress2) • Fall 2012 ✓ FDR approval (October 15) ✓ Installation of first optical enclosure components (photo) ✓ First light and testing of white/pink beam components (photo1, photo2) • Winter/Spring 2013 - White beam commissioning ✓ Alignment of mirrors with synchrotron beam ✓ Installation and alignment of support tables (photo)

413

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

76 76 Idaho National Laboratory Radiological Response Training Range Environmental Assessment Final October 2010 DOE/EA-1776 Idaho National Laboratory Radiological Response Training Range Environmental Assessment Final October 2010 Prepared for the U.S. Department of Energy Idaho Operations Office i CONTENTS GLOSSARY ................................................................................................................................................ iii EXECUTIVE SUMMARY .......................................................................................................................... v 1.0 PURPOSE AND NEED ..................................................................................................................... 1 2.0 ALTERNATIVES .............................................................................................................................. 2

414

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Used Fuel Disposition Used Fuel Disposition Campaign Preliminary Quality Assurance Implementation Plan Prepared for U.S. Department of Energy Used Fuel Disposition Campaign December FCR&D-USED-2011-000019 Used Fuel Disposition Preliminary Quality Assurance Implementation Plan Prepared for U.S. Department of Energy Campaign December 2010 000019 DISCLAIMER This information was prepared as an account of work sponsored by an

415

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Research, Development, Research, Development, and Demonstration Roadmap for Deep Borehole Disposal Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Bill W. Arnold, Palmer Vaughn, Robert MacKinnon, Jack Tillman, Dennis Nielson, Patrick Brady, William Halsey, and Susan Altman Sandia National Laboratories August 31, 2012 FCRD-USED-2012-000269 SAND2012-8527P Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy"s National Nuclear Security Administration under contract DE-AC04-94AL85000. DISCLAIMER

416

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Disposal Options for Research and Development for Spent Nuclear Fuel and High Basis for Identification of Disposal Options for Research and Development for Spent Nuclear Fuel and High-Level Waste Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Rob P. Rechard Barry Goldstein Larry H. Brush Sandia National Laboratories James A. Blink Mark Sutton Lawrence Livermore National Laboratory

417

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

RD&D Study Plan for RD&D Study Plan for Advancement of Science and Engineering Supporting Geologic Disposal in Bedded Salt- March 2013 Workshop Outcomes Prepared for U.S. Department of Energy Used Nuclear Fuel S. David Sevougian, SNL Robert J. MacKinnon, SNL Bruce A. Robinson, LANL Christi D. Leigh, SNL Douglas J. Weaver, LANL May 31, 2013 FCRD-UFD-2013-000161, Rev. 0 SAND2013-4386P Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. Los Alamos National Laboratory is an equal opportunity employer operated by

418

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

754 754 Online Monitoring Technical Basis and Analysis Framework for Emergency Diesel Generators-Interim Report for FY 2013 Binh T. Pham Nancy J. Lybeck Vivek Agarwal December 2012 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise,

419

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Generic Deep Geologic Generic Deep Geologic Disposal Safety Case Prepared for U.S. Department of Energy Used Fuel Disposition Campaign G. Freeze, M. Voegele, P. Vaughn, J. Prouty, W.M. Nutt, E. Hardin, S.D. Sevougian Sandia National Laboratories Argonne National Laboratory August 2013 Revision 1 FCRD-UFD-2012-000146 SAND2013-0974P Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty,

420

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

13 Summary Report: 13 Summary Report: Post-Irradiation Examination of Zircaloy-4 Samples in Target Capsules and Initiation of Bending Fatigue Testing for Used Nuclear Fuel Vibration Integrity Investigations Prepared for U.S. Department of Energy Used Fuel Disposition Campaign R. H. Howard, Y. Yan, J. Wang, L. J. Ott, R. L. Howard Oak Ridge National Laboratory September 30, 2013 FCRD-UFD-2013-000369 Oak Ridge National Laboratory is a multi-program laboratory managed and operated by UT-Battelle, LLC for the U.S. Department of Energy under contract DE-AC05-00OR22725. DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty,

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421

wyp_brochure.id  

NLE Websites -- All DOE Office Websites (Extended Search)

scientific and technical staff scientific and technical staff are eager to celebrate with your students. Classroom presentations are free of charge. Contact Nancy Lanning, edreg@fnal.gov or 630-840-5588. Please provide: * Your name, telephone and e-mail address. * Presentation requested. * Date of request. * Grade level and number of students. * School name. * A map to the school. Coinciding with the 100th anniversary

422

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Update of the Used Fuel Update of the Used Fuel Disposition Campaign Implementation Plan Prepared for U.S. Department of Energy Used Fuel Disposition Kevin McMahon Sandia National Laboratories September 2012 FCRD-UFD-2012-000334 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise,

423

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

6 6 Idaho National Laboratory Radiological Response Training Range Environmental Assessment Final October 2010 DOE/EA-1776 Idaho National Laboratory Radiological Response Training Range Environmental Assessment Final October 2010 Prepared for the U.S. Department of Energy Idaho Operations Office i CONTENTS GLOSSARY ................................................................................................................................................ iii

424

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

22 22 Idaho National Laboratory Stand-Off Experiment (SOX) Range Environmental Assessment Final March 2011 DOE/EA-1822 Idaho National Laboratory Stand-Off Experiment (SOX) Range Environmental Assessment Final March 2011 Prepared for the U.S. Department of Energy Idaho Operations Office i CONTENTS ACRONYMS ............................................................................................................................................... iii

425

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Recommended Practices Guide For Securing Recommended Practices Guide For Securing ZigBee Wireless Networks in Process Control System Environments Draft April 2007 Author Ken Masica Lawrence Livermore National Laboratory Ken Masica page 1 LLNL Recommended Practices Guide Securing ZigBee Wireless Networks in Process Control System Environments ( D R A F T ) Ken Masica Vulnerability & Risk Assessment Program (VRAP) Lawrence Livermore National Laboratory (LLNL) for DHS US CERT Control Systems Security Program (CSSP) April 2007 This work was performed under the auspices of the U.S. Department of Energy by University of California, Lawrence Livermore National Laboratory under Contract W- 7405-Eng-48. This document was prepared as an account of work sponsored by an agency of the

426

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

54 54 Draft Environmental Assessment for the Resumption of Transient Testing of Nuclear Fuels and Materials Draft November 2013 DOE/EA-1954 Draft Environmental Assessment for the Resumption of Transient Testing of Nuclear Fuels and Materials Draft November 2013 U.S. Department of Energy DOE Idaho Operations Office ii CONTENTS LIST OF FIGURES ..................................................................................................................... iii LIST OF TABLES....................................................................................................................... iv ACRONYMS .............................................................................................................................. v

427

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4 4 Guidance for Deployment of Mobile Technologies for Nuclear Power Plant Field Workers Ronald K. Farris Heather Medema September 2012 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation,

428

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Gap Analysis to Support Extended Storage of Used Nuclear Fuel Rev. 0 Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Brady Hanson (PNNL) Halim Alsaed (INL) Christine Stockman (SNL) David Enos (SNL) Ryan Meyer (PNNL) Ken Sorenson (SNL) January 31, 2012 FCRD-USED-2011-000136 Rev. 0 PNNL-20509 USED FUEL DISPOSITION CAMPAIGN Gap Analysis to Support Extended Storage of Used Nuclear Fuel Rev. 0 ii JANUARY 31, 2012 Disclaimer This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy,

429

11. CONTRACT ID CODE  

NLE Websites -- All DOE Office Websites (Extended Search)

1 PAGE 1 OF2 AMENDMENT OF SOLICITATION/MODIFICATION OF CONTRACT PAGES 2. AMENDMENT/MODIFICATION NO. I 3. EFFECTIVE DATE M191 See Block 16C 4. REQUISITION/PURCHASE I 5. PROJECT NO. (If applicable) REQ. NO. 6.ISSUED BY CODE U.S. Department of Energy National Nuclear Security Administration Service Center Property and M&O Contract Support Department P.O. Box 5400 Albuquerque, NM 87185-5400 7. ADMINISTERED BY (If other than Item 6) CODE U.S. Department of Energy National Nuclear Security Administration Manager, Pantex Site Office P.O. Box 30030 Amarillo, TX 79120 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) Babcock & Wilcox Technical Services Pantex, LLC PO Box 30020 Amarillo, TX 79120 CODE I FACILITY CODE SA. AMENDMENT OF SOLICITATION NO.

430

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

US US ED FUEL DIS P OS ITION CAMPAIGN Us e d Nu c le a r Fu e l Lo a d in g a n d S tru c tu ra l P e rfo rm a n c e Un d e r No rm a l Co n d itio n s o f Tra n s p o rt - Mo d e lin g, S im u la tio n a n d Exp e rim e n ta l In te g ra tion RD&D P la n P re p a re d fo r U.S . De p a rtme n t of En e rg y Us e d Fu e l Dis p o s itio n Ca m p a ig n Ap ril 1, 2013 FCRD-UFD-2013-000135 USED FUEL DISPOSITION CAMPAIGN Used Nuclear Fuel Loading and Structural Performance Under Normal Conditions of Transport - Modeling, Simulation and Experimental Integration RD&D Plan ii APRIL 1, 2013 Disclaimer This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility

431

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Public Preferences Related to Public Preferences Related to Consent-Based Siting of Radioactive Waste Management Facilities for Storage and Disposal: Analyzing Variations over Time, Events, and Program Designs Prepared for US Department of Energy Nuclear Fuel Storage and Transportation Planning Project Hank C. Jenkins-Smith Carol L. Silva Kerry G. Herron Kuhika G. Ripberger Matthew Nowlin Joseph Ripberger Center for Risk and Crisis Management, University of Oklahoma Evaristo "Tito" Bonano Rob P. Rechard Sandia National Laboratories February 2013 FCRD-NFST-2013-000076 SAND 2013-0032P Public Preferences Related to Consent Based Siting of Radioactive Waste Management Facilities ii February 2013 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a

432

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

0 0 Advanced LWR Nuclear Fuel Cladding System Development Trade-off Study Kristine Barrett Shannon Bragg-Sitton Daniel Galicki September 2012 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation,

433

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Integrated Tool Development Integrated Tool Development for Used Fuel Disposition Natural System Evaluation - Phase I Report Prepared for U.S. Department of Energy Used Fuel Disposition Yifeng Wang & Teklu Hadgu Sandia National Laboratories Scott Painter, Dylan R. Harp & Shaoping Chu Los Alamos National Laboratory Thomas Wolery Lawrence Livermore National Laboratory Jim Houseworth Lawrence Berkeley National Laboratory September 28, 2012 FCRD-UFD-2012-000229 SAND2012-7073P DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy,

434

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Deep Borehole Disposal Deep Borehole Disposal Research: Demonstration Site Selection Guidelines, Borehole Seals Design, and RD&D Needs Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Bill W. Arnold, Patrick Brady, Susan Altman, Palmer Vaughn, Dennis Nielson, Joon Lee, Fergus Gibb, Paul Mariner, Karl Travis, William Halsey, John Beswick, and Jack Tillman Sandia National Laboratories October 25, 2013 FCRD-USED-2013-000409 SAND2013-9490P Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.

435

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Experimental and Modeling Experimental and Modeling Investigation of Radionuclide Interaction and Transport in Representative Geologic Media Prepared for U.S. Department of Energy Used Fuel Disposition Yifeng Wang, Andy Miller, Edward Matteo Sandia National Laboratories Paul Reimus, Mei Ding, Timothy Dittrich Los Alamos National Laboratory Liange Zheng, James Houseworth Lawrence Berkeley National Laboratory Pihong Zhao, Annie Kersting, Zurong Dai, Mavrik Zavarin Lawrence Livermore National Laboratory September 15, 2013 FCRD-UFD-2013-000314 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for

436

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Degradation: Degradation: Experimental and Modeling Report (FCRD-UFD-2013-000404) Prepared for U.S. Department of Energy Used Fuel Disposition Campaign David C. Sassani, Carlos F. Jové Colón, Philippe Weck (Sandia National Laboratories) James L. Jerden Jr., Kurt E. Frey, Terry Cruse, William L. Ebert (Argonne National Laboratory) Edgar C. Buck, Richard S. Wittman (Pacific Northwest National Laboratory) October 17, 2013 SAND2013- 9077P Prepared by: Sandia National Laboratories Albuquerque, New Mexico 87185 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.

437

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

2/308 2/308 FCRD-FCT-2012-000232 Categorization of Used Nuclear Fuel Inventory in Support of a Comprehensive National Nuclear Fuel Cycle Strategy December 2012 Prepared by John C. Wagner, ORNL Joshua L. Peterson, ORNL Don E. Mueller, ORNL Jess C. Gehin, ORNL Andrew Worrall, ORNL Temitope Taiwo, ANL Mark Nutt, ANL Mark A. Williamson, ANL Mike Todosow, BNL Roald Wigeland, INL William G. Halsey, LLNL Ronald P. Omberg, PNNL Peter N. Swift, SNL Joe T. Carter, SRNL DOCUMENT AVAILABILITY Reports produced after January 1, 1996, are generally available free via the U.S. Department of Energy (DOE) Information Bridge. Web site http://www.osti.gov/bridge Reports produced before January 1, 1996, may be purchased by members of the public from the

438

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Coupled Thermal-Hydrological-Mechanical Processes in Salt Coupled Thermal-Hydrological-Mechanical Processes in Salt ii November 15, 2012 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe

439

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

BRINE MIGRATION EXPERIMENTAL BRINE MIGRATION EXPERIMENTAL STUDIES FOR SALT REPOSITORIES Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Florie A. Caporuscio, Hakim Boukhalfa, Michael C. Cheshire, Amy B. Jordan, and Mei Ding Los Alamos National Laboratory September 25, 2013 FCRD-UFD-2013-000204 Los Alamos National Laboratory-Approved for public release- 'LA-UR-13-27240' DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe

440

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

FUEL ASSEMBLY FUEL ASSEMBLY SHAKER TEST for Determining Loads on a PWR Assembly under Surrogate Normal Conditions of Truck Transport Prepared for U.S. Department of Energy Used Fuel Disposition Campaign Paul McConnell, Gregg Flores, Robert Wauneka, Greg Koenig, Doug Ammerman, John Bignell, Sylvia Saltzstein, Ken Sorenson Sandia National Laboratories SAND2013-5210P, Rev. 0.1 FCRD-UFD-2013-000190 June 30, 2013 (revised December 1, 2013) DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process

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While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Laboratory operated by Battelle Energy Alliance INL/EXT-12-27155 Revision 0 Evaluation of Computer- Based Procedure System Prototype Johanna Oxstrand Katya Le Blanc Seth Hays September 2012 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise,

442

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

TSPA Model Development TSPA Model Development and Sensitivity Analysis of Processes Affecting Performance of a Salt Repository for Disposal of Heat-Generating Nuclear Waste Prepared for U.S. Department of Energy Used Nuclear Fuel S. David Sevougian, SNL Geoff A. Freeze, SNL Michael B. Gross, SNL Joon Lee, SNL Christi D. Leigh, SNL Paul Mariner, SNL Robert J. MacKinnon, SNL Palmer Vaughn, SNL September 28, 2012 FCRD-UFD-2012-000320, Rev. 0 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.

443

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Appendix E Appendix E FCT Document Cover Sheet *Note: In some cases there may be a milestone where an item is being fabricated, maintenance is being performed on a facility, or a document is being issued through a formal document control process where it specifically calls out a formal review of the document. In these cases, documentation (e.g., inspection report, maintenance request, work planning package documentation or the documented review of the issued document through the document control process) of the completion of the activity along with the Document Cover Sheet is sufficient to demonstrate achieving the milestone. QRL for such milestones may be also be marked N/A in the work package provided the work package clearly specifies the requirement to use the Document Cover

444

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Review of Used Nuclear Fuel Storage and Transportation Technical Gap Analyses Prepared for U.S. Department of Energy Used Fuel Disposition Campaign July 31, 2012 FCRD-USED-2012-000215 PNNL-21596 USED FUEL DISPOSITION CAMPAIGN Review Of Used Nuclear Fuel Storage and Transportation Technical Gap Analyses ii July 31, 2012 Disclaimer This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed or represents that its use

445

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

INL/MIS-12-27161 Revision 0 Summary Report on Industrial and Regulatory Engagement Activities Ken Thomas September 2012 DISCLAIMER This information was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, expressed or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness, of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. References herein to any specific commercial product, process, or service by trade name, trade mark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation,

446

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Integration of EBS Integration of EBS Models with Generic Disposal System Models (FCRD-UFD-2012-000277) Prepared for U.S. Department of Energy Used Fuel Disposition Campaign David C. Sassani, Carlos F. Jové Colón, Philippe Weck (Sandia National Laboratories) James L. Jerden Jr., Kurt E. Frey, Terry Cruse, William L. Ebert (Argonne National Laboratory) Edgar C. Buck, Richard S. Wittman, Frances N. Skomurski, Kirk J. Cantrell, Bruce K. McNamara, Chuck Z. Soderquist (Pacific Northwest National Laboratory) September 07, 2012 SAND2012-7762 P Prepared by: Sandia National Laboratories Albuquerque, New Mexico 87185 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of

447

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

forming. He also has specialized FEA experience in electromagnetic analyses to support improvements to performance of radiation detector arrays and field enhancement for...

448

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

This includes the storage, transportation, and disposal of low level waste (LLW), used nuclear fuel (UNF), and high level waste (HLW). The Office of Fuel Cycle Technologies...

449

elementbingo_all.id  

NLE Websites -- All DOE Office Websites (Extended Search)

Jefferson National Accelerator Facility - Office of Science Education http:education.jlab.org Thomas Jefferson National Accelerator Facility - Office of Science Education http:...

450

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

of providing the power required for acceleration. Also, the battery's ability to accept energy from regenerative braking decreased significantly during the operating period....

451

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

... 5 2. Arizona Public Service residential electricity rates for summer peak months ... 5 3. Vehicle to grid scenario...

452

DOE/ID  

NLE Websites -- All DOE Office Websites (Extended Search)

materials, often expressed as Biological Oxygen Demand (BOD) and Chemical Oxygen Demand (COD), from 1 Figure 1. Thermal stratification of a hydropower reservoir the watershed...

453

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Coupled Thermal-Hydrological-Mechanical Processes in Salt ii November 15, 2012 Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia...

454

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

RH Remote-Handled radioactive waste SNF Spent Nuclear Fuel SRD Salt R&D Study T Thermal processes TMI Three-Mile Island Tr Radionuclide transport processes TRU Transuranic...

455

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4 Guidance for Deployment of Mobile Technologies for Nuclear Power Plant Field Workers Ronald K. Farris Heather Medema September 2012 DISCLAIMER This information was prepared as an...

456

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

Streamflows and Power Potentials for Alaska and Hawaii Kristine L. Verdin SAICEROS Data Center May 2004 Idaho National Engineering and Environmental Laboratory Bechtel BWXT...

457

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Nuclear Waste Technical Review Board (NWTRB), the U.S. Nuclear Regulatory Commission (NRC), the Electric Power Research Institute (EPRI), and the International Atomic Energy...

458

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

... 29 Modification of ACRR and Construction of New Hot Cell- ...29 Routine Maintenance and Operations at ACRR...

459

DOE/ID-Number  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

y). Irradiated pre-hydrided metallic materials will generate baseline data to benchmark hot-cell testing of high-burnup used fuel cladding at relatively low cost, and more...

460

DOE/ID-Number  

NLE Websites -- All DOE Office Websites (Extended Search)

Funding Project as they were the only electric vehicles available for leasing from vehicle manufacturers at the time. Federal Fleet Acquisitions of Electric Vehicles 0 2 4 6...

Note: This page contains sample records for the topic "id il ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Beamline 29-ID  

NLE Websites -- All DOE Office Websites (Extended Search)

Rosenberg Dr. George Srajer IEX - Advisory Committee Dr Dario Arena (Brookhaven National Lab, NSLS) Dr. Steve Hulbert (Brookhaven National Lab, NSLS) Dr Zahid Hussain...

462

11. CONTRACT ID CODE  

National Nuclear Security Administration (NNSA)

30030 Amarillo, TX 79120 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county,