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Note: This page contains sample records for the topic "mm dd yy" 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.


1

cession Numb Main Entry Title Description Restrictions Material type Extent in container Location Slides Map Case M/A Date MM/DD/YY Accession date Notes Folder List 81-002 Froman, Lenore Photographs, 1959  

E-Print Network [OSTI]

Slides Map Case M/A Date MM/DD/YY Accession date Notes Folder List 81-002 Froman, Lenore Photographs, 1959 Five color 35mm slides depicting the departure of R/V Stranger on Naga Expedition, 15 June 1959. Photographs 5 items Slides 1A 1A 7/21/1981 1981 Not Needed 81-003 SIO Ship Operations and Marine Technical

Russell, Lynn

2

Summary of Decisions - MM DD YYYY - MM DD YYYY | Department of Energy  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankCombustion |Energy Usage »of Energy Strain Rate4 RecoveryJuly 1, 2013 - July 5,3, 2013 - JuneMM DD

3

Student Name: ______________________________ Birthdate (MM/DD/YY): ____________ PART I SCREENING: Please answer the following questions  

E-Print Network [OSTI]

Seychelles Sierra Leone Singapore Solomon Islands Somalia South Africa Sri Lanka Sudan Suriname Swaziland

4

Name and Contact Information * Indicates a required field * Date of Birth (MM/DD/YYYY)  

E-Print Network [OSTI]

Name and Contact Information * Indicates a required field * Date of Birth (MM/DD/YYYY) * o Female o courses offered as part of a certificate or diploma program are exempt from GST, even if you are only certificates and diplomas for eligible students. If you have any questions or requests about the collection

5

Complete one form for each person seeking Wisconsin COMMERCIAL Pesticide Applicator Certification. Last Name First Name Middle Initial Date of Birth (mm/dd/yyyy)  

E-Print Network [OSTI]

Complete one form for each person seeking Wisconsin COMMERCIAL Pesticide Applicator Certification. Last Name First Name Middle Initial Date of Birth (mm/dd/yyyy) Company Name Company Unit taking the pesticide applicator certification exam. A personalized training/reference manual

Mladenoff, David

6

BB UU LL GG AA RR II AA NN AA CC AA DD EE MM YY OO FF SS CC II EE NN CC EE SS IINNSSTTIITTUUTTEE OOFF IINNFFOORRMMAATTIIOONN AANNDD CCOOMMMMUUNNIICCAATTIIOONN TTEECCHHNNOOLLOOGGIIEESS  

E-Print Network [OSTI]

Library (ITIL) ­ essence development, open problems Abstract: This article aims to give an overview over the ITIL framework objective. It is going to explain the rapidly growing IT business needs which had caused the development of this library. We are also going to follow the ITIL evolution history and find the circumstances

Mustakerov, Ivan

7

Kelly Scientific Resources Kelly Scientific Resources yy BIOTECHNOLOGY DRUG &  

E-Print Network [OSTI]

Kelly Scientific Resources Kelly Scientific Resources yy BIOTECHNOLOGY DRUG & PHARMACEUTICAL · What Kelly Scientific Resources or staffing agencies are and how they work?they work? · How to work Role: ­ Northern California Recruiting and Business efforts for Kelly Scientific Resources ­ Promote

Puglisi, Joseph

8

Revue Franaise de Gestion Industrielle Vol. xx, n yy  

E-Print Network [OSTI]

Revue Franaise de Gestion Industrielle Vol. xx, n yy A LA RECHERCHE D'UNE MUTUALISATION DES LIVRAISONS EN MILIEU URBAIN : LE CAS DU GROUPE NMPP1 Jess GONZALEZ-FELIU* , Jolle MORANA presse, tel que le cas d'tude ici considr, le groupe Nouvelles Messageries de la Presse Parisienne

Boyer, Edmond

9

Page 1 of 3 HR; Version: 16/Date: 1/12/09  

E-Print Network [OSTI]

Dates* of Visit to LBNL: - . * Berkeley Lab reserves the right to change dates at any times. (mm/dd/yy) - (mm/dd/yy) Do you plan to visit LBNL intermittently during your expected dates as stated above? Yes No (e.g. visit LBNL for 2 consecutive weeks, leave LBNL the following week, and return to LBNL for 3

Knowles, David William

10

YY1 Regulates Melanocyte Development and Function by Cooperating with MITF  

E-Print Network [OSTI]

Studies of coat color mutants have greatly contributed to the discovery of genes that regulate melanocyte development and function. Here, we generated Yy1 conditional knockout mice in the melanocyte-lineage and observed ...

Li, Juying

11

100% DD Energy Model Update  

SciTech Connect (OSTI)

The Miami Science Museum energy model has been used during DD to test the building??s potential for energy savings as measured by ASHRAE 90.1-2007 Appendix G. This standard compares the designed building??s yearly energy cost with that of a code-compliant building. The building is currently on track show 20% or better improvement over the ASHRAE 90.1-2007 Appendix G baseline; this performance would ensure minimum compliance with both LEED 2.2 and current Florida Energy Code, which both reference a less strict version of ASHRAE 90.1. In addition to being an exercise in energy code compliance, the energy model has been used as a design tool to show the relative performance benefit of individual energy conservation measures (ECMs). These ECMs are areas where the design team has improved upon code-minimum design paths to improve the energy performance of the building. By adding ECMs one a time to a code-compliant baseline building, the current analysis identifies which ECMs are most effective in helping the building meet its energy performance goals.

None

2011-06-30T23:59:59.000Z

12

Liquid-gas Phase Transition in Strange Hadronic Matter with Weak Y-Y Interaction  

E-Print Network [OSTI]

The liquid-gas phase transition in strange hadronic matter is reexamined by using the new parameters about the $\\Lambda - \\Lambda$ interaction deduced from recent observation of $^{6}_{\\Lambda\\Lambda}He$ double hypernucleus. The extended Furnstahl-Serot-Tang model with nucleons and hyperons is utilized. The binodal surface, the limit pressure, the entropy, the specific heat capacity and the Caloric curves are addressed. We find that the liquid-gas phase transition can occur more easily in strange hadronic matter with weak Y-Y interaction than that of the strong Y-Y interaction.

Li Yang; Shao Yu Yin; Wei Liang Qian; Ru-keng Su

2005-06-19T23:59:59.000Z

13

The secondary minimum in YY Her: Evidence for a tidally distorted giant  

E-Print Network [OSTI]

We present and analyze quiescent UBVRI light curves of the classical symbiotic binary YY Her. We show that the secondary minimum, which is clearly visible only in the quiescent VRI light curves, is due to ellipsoidal variability of the red giant component. Our simple light curve analysis, by fitting of the Fourier cosine series, resulted in a self-consistent phenomenological model of YY Her, in which the periodic changes can be described by a combination of the ellipsoidal changes and a sinusoidal changes of the nebular continuum and line emission.

J. Mikolajewska; E. A. Kolotilov; S. Yu. Shugarov; B. F. Yudin

2002-06-23T23:59:59.000Z

14

PART 1. Student background University ID Social Security number Birthdate (mm/dd/yyyy)  

E-Print Network [OSTI]

Support Resources. Do not return this form to your college or academic department. Return this form to: Academic Support Resources By U.S. Postal Service mail Academic Support Resources 20 Fraser Hall 106 from no less than 20 percent post-consumer waste. Please recycle.*OTR161* updated by date for office

Amin, S. Massoud

15

Electron assisted $dd$ reactions in metals  

E-Print Network [OSTI]

The electron assisted low energy $dd$ reactions in deuterized metals are investigated. It is shown that if a metal is irradiated with slow, free deuterons then the $e+d+d\\rightarrow e^{\\prime }+p+t$ and $e+d+d\\rightarrow e^{\\prime }+n+$ $^{3}He$\\ electron assisted $dd$ processes will have measurable probabilities even in the case of slow deuterons. The cross sections and the yields in an irradiated sample are determined. The results are associated with the so called anomalous screening effect. It is concluded that the electron $dd$ processes have to be taken into account when evaluating the experimental data of low energy fusion reactions in metals.

Pter Klmn; Tams Keszthelyi

2014-02-19T23:59:59.000Z

16

Web Intelligence: New Frontiers of Exploration Yiyu (Y.Y.) Yao  

E-Print Network [OSTI]

Web Intelligence: New Frontiers of Exploration Yiyu (Y.Y.) Yao Department of Computer Science://www.cs.uregina.ca/yyao Abstract-- Web Intelligence (WI) deals with the scientific exploration of the new territories of the Web in the context of the Web, and goes beyond each of them. From several perspectives of the Web, we investigate

Yao, Yiyu

17

Registration and Fees Confirmation Form For Full-Time McMaster Students on a Letter of Permission  

E-Print Network [OSTI]

; and disclosure to or on behalf of the applicable McMaster student government. This information is protected and is being collected pursuant to section 39(2) and section 42 of the Freedom of Information and Protection/05/09 Course Name (ie. History) Course Code (ie. 2EA3E) Start Date (dd/mm/yy) End Date (dd/mm/yy) #12;

Hitchcock, Adam P.

18

INEL D&D long-range plan  

SciTech Connect (OSTI)

This Long-Range Plan presents the Decontamination and Dismantlement (D&D) Program planning status for facilities at the Idaho National Engineering Laboratory (INEL). The plan provides a general description of the D&D Program objectives, management criteria, and policy; discusses current activities; and documents the INEL D&D Program cost and schedule estimate projections for the next 15 years. Appendices are included that provide INEL D&D project historical information, a comprehensive descriptive summary of each current D&D surplus facility, and a summary database of all INEL contaminated facilities awaiting or undergoing the facility transition process.

Buckland, R.J.; Kenoyer, D.J.; LaBuy, S.A.

1995-09-01T23:59:59.000Z

19

INEL D&D Long-Range Plan  

SciTech Connect (OSTI)

This Long-Range Plan presents the Decontamination and Decommissioning (D&D) Program planning status for facilities at the Idaho National Engineering Laboratory (INEL). The plan provides a general description of the D&D Program objectives, management criteria, and philosophy; discusses current activities; and documents the INEL D&D Program cost and schedule estimate projections for the next 15 years. appendices are included that provide INEL D&D project historical information and a comprehensive descriptive summary of each current surplus facility.

Buckland, R.J.; Kenoyer, D.J.; Preussner, D.H.

1993-10-01T23:59:59.000Z

20

D-D Nuclear Fusion Using Different Size Pyroelectric Crystals  

E-Print Network [OSTI]

D-D Nuclear Fusion Using Different Size Pyroelectric Crystals A. M. Kovanen, D. J. Gillich, T. Z the conditions for D-D fusion in pyroelectric crystal accelerators. Three different pyroelectric crystal sizes are with the Department of Mechanical, Aerospace and Nuclear Engineering, Rensselaer Polytechnic Institute, Troy, NY. A. M

Danon, Yaron

Note: This page contains sample records for the topic "mm dd yy" 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

Design Computing and Cognition DCC'12. J.S. Gero (ed), pp. xx-yy. Springer 2012  

E-Print Network [OSTI]

Design Computing and Cognition DCC'12. J.S. Gero (ed), pp. xx-yy. © Springer 2012 1 Role Grenoble, F-38031, France Elicitation of requirements is a key step of the design activity. The building of a shared understanding of design requirements is essential to the performance of the design. Personas

Paris-Sud XI, Université de

22

Design Computing and Cognition DCC'12. J.S. Gero (ed), pp. xx-yy. Springer 2012  

E-Print Network [OSTI]

Design Computing and Cognition DCC'12. J.S. Gero (ed), pp. xx-yy. © Springer 2012 1 Understanding Analogical Reasoning in Biomimetic Design: An Inductive Approach Hyunmin Cheong, Gregory Hallihan, and L designers ap- ply biological analogies to solve design problems. We recorded the discourse of fourth

Shu, Lily H.

23

Water Tanks Demolition and Deactivation (D&D) Project (4589)...  

Broader source: Energy.gov (indexed) [DOE]

Water Tanks Demolition and Deactivation (D&D) Projects (4589) Program or Field Office: Y-12 Site Office Location(s) (CityCountyState): Oak Ridge, Anderson County, Tennessee...

24

BUSINESS ADMINISTRATION -PLAN OF STUDY CATALOG YEAR: 2014-2015 Name________________________________________ PeopleSoft ID#____________________ Anticipated Date of Completion (MM/YY)_________  

E-Print Network [OSTI]

Page 1 BUSINESS ADMINISTRATION - PLAN OF STUDY CATALOG YEAR: 2014-2015 Name-approved Business elective BADM 4075W MKTG 3101 MGMT 4902 Advisor-approved Business elective MGMT 3101 OPIM 3104 Extended core requirement Advisor-approved Business elective OPIM 3103 Extended core requirement Extended

Alpay, S. Pamir

25

BUSINESS DATA ANALYTICS -PLAN OF STUDY CATALOG YEAR: 2014-2015 Name__________________________________________ PeopleSoft ID#________________ Anticipated Date of Completion (MM/YY) _________  

E-Print Network [OSTI]

Page 1 BUSINESS DATA ANALYTICS - PLAN OF STUDY CATALOG YEAR: 2014-2015 Name OPIM 3104 3000/4000 level Business elective 3000/4000 level Business elective FNCE 3101 OPIM 3505 3000/4000 level Business elective MGMT 4902 OPIM 3103 BADM 4075W BADM 4072 1 ACCT 2101: Recommended to take

Alpay, S. Pamir

26

D.D. Sentman Geophysical Institute  

E-Print Network [OSTI]

clip) Camera 1: Starlight Xpress MX716 CCD Sony ICX249AL 752x580x8.6 m 16 bit samples, 2x2 binning 10s 6mm f/1.2 Recorder: Sony Digital Video Walkman miniDV recorder #12;GOES-8 IR4 (10-12m) weather

California at Berkeley, University of

27

D&D Waste Estimate Validation  

SciTech Connect (OSTI)

Rocky Flats Closure Project (Site) includes several multi-year decontamination and decommissioning (D&D) projects which, over the next four years, will dismantle and demolish four major plutonium facilities, four major uranium facilities, and over 400 additional facilities of different types. The projects are currently generating large quantities of transuranic, low-level, mixed, hazardous, and sanitary wastes. A previous paper described the initial conceptual estimates and methods, and the evolution of these methods based on the actual results from the decommissioning of a ''pilot'' facility. The waste estimating method that resulted from that work was used for the waste estimates incorporated into the current Site baseline. This paper discusses subsequent developments on the topic of waste estimating that have occurred since the baseline work. After several months of operation under the current Site baseline, an effort was initiated to either validate or identify improvements to the waste basis-of-estimate. Specific estimate and estimating method elements were identified for additional analysis based on the element's potential for error and the impact of that error on Site activities. The analysis took advantage of actual, more detailed data collected both from three years additional experience in decommissioning a second plutonium facility and from experience in deactivating certain non-plutonium facilities. It compared the actual transuranic and low-level waste generation against their respective estimates based on overall distribution and for individual media (i.e. equipment type), and evaluated trends. Finally, it projected the quantity of lead-characteristic low-level mixed waste that will be generated from plutonium building decommissioning and upgraded the decommissioning waste estimates of the non-plutonium buildings.

Sanford, P. C.; Templeton, J. H.; Stevens, J. L.; Dorr, K.

2002-02-25T23:59:59.000Z

28

mm-Wave Phase Shifters and Switches  

E-Print Network [OSTI]

4.1.1 Slow wave transmissioncombiners . . . . . . . . . . . 5.3 mm-Wave implementationfailed to predict current mm-wave design trend [1] . . . . .

Adabi Firouzjaei, Ehsan

2010-01-01T23:59:59.000Z

29

DEFLECTION MEASUREMENTS OF 25 mm ALUMINUM COLLARS  

E-Print Network [OSTI]

MEASUREMENTS OF 25 mm ALUMINUM COLLARS C. Peters LawrenceMEASUREMENTS OF 25 mm ALUMINUM COLLARS" C. Peters Lawrenceinch thick 7075- T6 aluminum alloy plate. Inside corners

Peters, C.

2010-01-01T23:59:59.000Z

30

Deactivation & Decommissioning Knowledge Management Information Tool (D&D KM-IT)  

Broader source: Energy.gov [DOE]

The Deactivation and Decommissioning Knowledge Management Information Tool (D&D KM-IT) serves as a centralized repository providing a common interface for all D&D related activities.

31

First observation of the decay B-0 -> D*D+*(-)  

E-Print Network [OSTI]

We have observed four fully reconstructed B-0 --> D*+D*- candidates in 5.8 x 10(6) Y(4S) --> B (B) over bar decays recorded with the CLEO detector. The background is estimated to be 0.31 +/- 0.10 events. The probability that the background could...

Ammar, Raymond G.; Baringer, Philip S.; Bean, Alice; Besson, David Zeke; Coppage, Don; Davis, Robin E. P.; Kotov, S.; Kravchenko, I.; Kwak, Nowhan; Zhou, L.

1999-04-01T23:59:59.000Z

32

Summary of the D&D Engineering Operations  

E-Print Network [OSTI]

mandatory! · Clear responsibility and accountability! ! #12;Conduct of Operations WORK CONTROL CENTER DKeith Rule Summary of the D&D Engineering Operations Princeton Plasma Physics Laboratory #12&D operations ! Maximum single individual external dose of 573 mRem (5.73 mGy) attributed to the sheer

33

a 3.37 mm length b 3.32 mm diameter  

E-Print Network [OSTI]

5.2 ml retinal subtense 300 µm/deg retinal arc 51 mm retinal area* 1024 ± 184 mm2 total.3 µl retinal subtense 31 µm/deg retinal arc 4.9 mm retinal area 15.6 mm2 cone:rod ratio 0/deg retinal arc 10.6 mm retinal area 52 mm2 cone:rod ratio mean cone density* mm-2 mean rod

Marc, Robert E.

34

Web-based Support Systems for Sustainable Communities W.N. Liu J.T. Yao L. Fan Y.Y. Yao X.D. Yang  

E-Print Network [OSTI]

present an architecture of Web-based support systems for sustainable communities. The architectureWeb-based Support Systems for Sustainable Communities W.N. Liu J.T. Yao L. Fan Y.Y. Yao X.D. Yang,fan,yyao,yang}@cs.uregina.ca ABSTRACT This paper studies Web-based support systems for sustain- able communities. A sustainable

Yao, JingTao

35

The giant star of the symbiotic system YY Her: Rotation, Tidal wave, Solar-type cycle and Spots  

E-Print Network [OSTI]

We analyze the historical light curve of the symbiotic star YY Her, from 1890 up to December 2005. A secular declining trend is detected, at a rate of ~.01 magn in 1000 d, suggesting that the system could belong to the sub-class of symbiotic novae. Several outburst events are superposed on this slow decline. Three independent periodicities are identified in the light curve. A quasi-periodicity of 4650.7 d is detected for the outburst occurrence. We suggest that it is a signature of a solar-type magnetic dynamo cycle in the giant component. A period of 593.2 d modulates the quiescent light curve and it is identified as the binary period of the system. During outburst events the system shows a stable periodic oscillation of 551.4 d. We suggest that it is the rotation period of the giant.The secondary minima detected at some epochs of quiescence are probably due to dark spots on the surface of the rotating giant. The difference between the frequencies of these two last periods is the frequency of a tidal wave in the outer layers of the giant. A period which is a beat between the magnetic cycle and the tidal wave period is also apparent in the light curve. YY Her is a third symbiotic system exhibiting these cycles in their light curve, suggesting that a magnetic dynamo process is prevalent in the giant components of symbiotic stars, playing an important role in the outburst mechanism of some of these systems.

Liliana Formiggini; Elia M. Leibowitz

2006-09-17T23:59:59.000Z

36

Data:B2df03dd-411d-469c-9605-28160068dd2c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2 No revision has38865d08 No revision has been28a07c58 No revision has-28160068dd2c No revision has been

37

D-D fusion experiments using fast Z pinches  

SciTech Connect (OSTI)

The development of high current (I > 10 MA) drivers provides the authors with a new tool for the study of neutron-producing plasmas in the thermal regime. The imploded deuterium mass (or collisionality) increases as I{sup 2} and the ability of the driver to heat the plasma to relevant fusion temperatures improves as the power of the driver increases. Additionally, fast (<100 ns) implosions are more stable to the usual MHD instabilities that plagued the traditional slower implosions. The authors describe experiments in which deuterium gas puffs or CD{sub 2} fiber arrays were imploded in a fast z-pinch configuration on Sandia`s Saturn facility generating up to 3 {times} 10{sup 12} D-D neutrons. These experiments were designed to explore the physics of neutron-generating plasmas in a z-pinch geometry. Specifically, the authors intended to produce neutrons from a nearly thermal plasma where the electrons and ions have a nearly Maxwellian distribution. This is to be clearly differentiated from the more usual D-D beam-target neutrons generated in many dense plasma focus (DPF) devices.

Spielman, R.B.; Baldwin, G.T.; Cooper, G. [and others

1998-03-01T23:59:59.000Z

38

Environmental Health and Safety  

E-Print Network [OSTI]

Environmental Health and Safety Approved by Document No. Version Date Replaces Page EHS EHS-FORM-072 1.0 15-May-2008 N/A 1 of 4 Laboratory Safety Orientation Checklist Name (Print) Department Supervisor Date (DD/MM/YY) A Laboratory Safety Orientation Checklist should be completed within one month

Shoubridge, Eric

39

VICE CHANCELLOR Signature of Head of School  

E-Print Network [OSTI]

VICE CHANCELLOR Signature of Head of School Date (dd/mm/yy) Following is a report on the professional and consultative work of my School/section over the twelve months of (year) School/Section One. Yes No (Nil Return) Total number of staff within School/Section at year end who are eligible to engage

Tobar, Michael

40

[OMB # 0648-0327 EXP 07-31-2015] NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION  

E-Print Network [OSTI]

Phone No. ( ) City State Zip Code Fax Phone No. ( ) Email Address Website Cell Phone No. ( ) SECTION 2 No. ( ) Email Address Birth Date (mm/dd/yy) Cell Phone No. ( ) SECTION 4 - ADDITIONAL FEDERAL - ADDITIONAL FACILITIES (add additional sheets if necessary) Business Name Daytime Phone No. Fax Phone No

Note: This page contains sample records for the topic "mm dd yy" 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

Address for applications only: International School for Graduate Studies (ISGS)  

E-Print Network [OSTI]

Family Name First Name Sex/ Date of Birth Place of Birth Citizenship Male Female dd/mm/yy 3/ Zip code Town Country Email Phone/ Fax Please attach photo here #12;2 5. YOUR EDUCATIONAL BACKGROUND of the Certificates! 5.1 School Education What is the highest level of your secondary education? 5.2 Higher Education

Madlener, Klaus

42

Application for Admission: Collaborative Academic Training Program  

E-Print Network [OSTI]

Immigration Status o Study Permit Citizenship(s): YY MM DD Address for correspondence regarding-secondary institutions previously or currently attended, including the University of Calgary. Failure to report all post University of Petroleum (Beijing) p China University of Petroleum (East China) p Xi'an Jiaotong University p

de Leon, Alex R.

43

Application for admission to german university for international applicants with foreign academic qualifikation  

E-Print Network [OSTI]

Female Date of birth . . 19 (dd, mm, 19yy) Place of birth . Nationality/Nationalities . 3. Postal adress or English) of your certificates. Please submit these together with this application. Important: Some universities accept certificates in other languages besides German or English. (Enquire at the university

Heermann, Dieter W.

44

Application for admission to German university for international applicants with foreign academic qualification  

E-Print Network [OSTI]

Female Date of birth . . 19 (dd, mm, 19yy) Place of birth . Nationality/Nationalities . 3. Postal address to substantiate the data below with certified copies and translations (German or English) of your certificates. Please submit these together with this application. Important: Some universities accept certificates

Knüpfer, Christian

45

SECTION 1 -CERTIFICATION BY AUTHORISED DEPARTMENTAL OFFICER  

E-Print Network [OSTI]

SECTION 1 - CERTIFICATION BY AUTHORISED DEPARTMENTAL OFFICER Earnings Code Description Rate No Ext. Employee ID Surname Given Names Title Date of Birth (dd/mm/yy) Sex (tick one) male female Home Phone No. Postal Address (for group certificates, etc) Postcode Is an Employment Declaration Form

Tobar, Michael

46

Address for applications only: International School for Graduate Studies  

E-Print Network [OSTI]

of Birth Place of Birth Citizenship Male Female dd/mm/yy 3 CORRESPONDENCE ADDRESS (Address to which/ attested certificates and documents and officially certified/ attested German or English translations! Please do not send the originals of the Certificates! 5.1 School Education What is the highest level

Pinnau, René

47

UNISTART is a new program designed for Aboriginal and Torres Strait Islander people wishing to gain entry into a university degree. A student-centred program, UNISTART offers you holistic development -culturally, personally  

E-Print Network [OSTI]

the appropriate box Gender: OtherFemaleMale Date of birth: dd/mm/yy CONTACT DETAILS City: PERSONAL DETAILS Torres by another name/s? (please state) N.B Documentation is required to prove changes in name i.e name at birth centre? Please list them and include copies of any certificates you have with this form #12;DECLARATION I

University of Technology, Sydney

48

Fusion Technologies for Tritium-Suppressed D-D Fusion White Paper prepared for FESAC Materials Science Subcommittee  

E-Print Network [OSTI]

1 Fusion Technologies for Tritium-Suppressed D-D Fusion White Paper prepared for FESAC Materials for tritium-suppressed D-D fusion and the understanding of the turbulent pinch in magnetically confined plasma pathway. Tritium- suppressed D-D fusion eliminates the need to breed fuel from lithium, reduces the damage

49

Maximizing the Benefit from the D&D Technology Development Program  

Broader source: Energy.gov [DOE]

The Office of Deactivation and Decommissioning (D&D)/Facility Engineering (FE) is charged with reducing the technical risk and uncertainty of D&D activities across the Environmental...

50

D&D Toolbox Robotic Deployment of High Resolution Laser Imaging for Characterization  

Broader source: Energy.gov [DOE]

The characterization of complex and/or hazardous facilities for the purposes of planning D&D projects can be excessively time consuming and present unacceptable hazards for personnel who enter...

51

Data:1fb894cb-3e2c-4dba-8e17-dd8dd9321d94 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision5af6d400c2d No529a57c00c0 No revision has75f38de27d No revision has7-dd8dd9321d94 No

52

ARM - Campaign Instrument - 5mm-mwr  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary)morphinanInformation Desert SouthwestTechnologies |NovemberARMContactsARMFacilitiesCERAgovInstruments5mm-mwr

53

SS OO UU TT HH AA FF RR II CC AA SS QQ UU AA RR EE KK II LL OO MM EE TT RR EE AA RR RR AA YY SKA South Africa Project Office  

E-Print Network [OSTI]

South Africa Project Office 12 March 2012 BIDS AWARDED CIVIL WORKS FOR THE CONSTRUCTION OF ROADS@ska.ac.za / mabela@ska.ac.za 1st Floor 17 Baker Street Rosebank Johannesburg South Africa 2196 Tel: +27 (0) 11 442

Jarrett, Thomas H.

54

SS OO UU TT HH AA FF RR II CC AA SS QQ UU AA RR EE KK II LL OO MM EE TT RR EE AA RR RR AA YY SKA South Africa Project Office  

E-Print Network [OSTI]

South Africa Project Office 05 July 2012 BIDS AWARDED PROCUREMENT OF VEHICLES FOR THE OPERATION@ska.ac.za 1st Floor 17 Baker Street Rosebank Johannesburg South Africa 2196 Tel: +27 (0) 11 442 2434 Fax: +27

Jarrett, Thomas H.

55

SS OO UU TT HH AA FF RR II CC AA SS QQ UU AA RR EE KK II LL OO MM EE TT RR EE AA RR RR AA YY SKA South Africa Project Office  

E-Print Network [OSTI]

South Africa Project Office 04 July 2012 BIDS AWARDED KAT 7 AND MEERKAT BUILDING MANAGEMENT SYSTEM, 2 March 2012 at 11:00 Name of the Successful Bidders: Schneider- Electric South Africa Ceiling Price: tcheetham@ska.ac.za / mabela@ska.ac.za 1st Floor 17 Baker Street Rosebank Johannesburg South Africa 2196 Tel

Jarrett, Thomas H.

56

SS OO UU TT HH AA FF RR II CC AA SS QQ UU AA RR EE KK II LL OO MM EE TT RR EE AA RR RR AA YY SKA South Africa Project Office  

E-Print Network [OSTI]

South Africa Project Office 1st Floor The Park 17 Baker Street 3rd Floor Rosebank Park Rd Johannesburg Pinelands South Africa South Africa 2196 7405 Tel: +27 (0) 11 442 2434 +27 (0)21 506 7300 Fax: +27 (0) 11

Jarrett, Thomas H.

57

Experimental Determination of DT Yield in High Current DD Dense Plasma Focii  

SciTech Connect (OSTI)

Dense Plasma Focii (DPF), which utilize deuterium gas to produce 2.45 MeV neutrons, may in fact also produce DT fusion neutrons at 14.1 MeV due to the triton production in the DD reaction. If beam-target fusion is the primary producer of fusion neutrons in DPFs, it is possible that ejected tritons from the first pinch will interact with the second pinch, and so forth. The 2 MJ DPF at National Security Technologies Losee Road Facility is able to, and has produced, over 1E12 DD neutrons per pulse, allowing an accurate measurement of the DT/DD ratio. The DT/DD ratio was experimentally verified by using the (n,2n) reaction in a large piece of praseodymium metal, which has a threshold reaction of 8 MeV, and is widely used as a DT yield measurement system1. The DT/DD ratio was experimentally determined for over 100 shots, and then compared to independent variables such as tube pressure, number of pinches per shot, total current, pinch current and charge voltage.

Lowe, D. R. [National Security Technologies, LLC; Hagen, E. C. [National Security Technologies, LLC; Meehan, B. T. [National Security Technologies, LLC; Springs, R. K. [University of Nevada, Las Vegas; O'Brien, R. J. [University of Nevada, Las Vegas

2013-06-18T23:59:59.000Z

58

Polarized mm And sub-mm Emission From Sgr A* At The Galactic Center  

E-Print Network [OSTI]

The recent detection of significant linear polarization at mm and sub-mm wavelengths in the spectrum of Sgr A* (if confirmed) will be a useful probe of the conditions within several Schwarzschild radii ($r_S$) of the event horizon at the Galactic Center. Hydrodynamic simulations of gas flowing in the vicinity of this object suggest that the infalling gas circularizes when it approaches within $5-25 r_S$ of the black hole. We suggest that the sub-mm ``excess'' of emission seen in the spectrum of Sgr A* may be associated with radiation produced within the inner Keplerian region and that the observed polarization characteristics provide direct evidence for this phenomenon. The overall spectrum from this region, including the high-energy component due to bremsstrahlung and inverse Compton scattering processes, is at or below the recent {\\it Chandra} measurement, and may account for the X-ray source if it turns out to be the actual counterpart to Sgr A*.

Fulvio Melia; Siming Liu; Robert Coker

2001-01-18T23:59:59.000Z

59

direction. Three different pipette solutions were used: Cs-gluconate solution (150 mM CsOH, 5 mM CsCl, 135 mM sucrose, 10 mM HEPES, 1.5 mM EGTA and 1.5 mM EDTA  

E-Print Network [OSTI]

was varied from 20 mM to 5 mM by addition of the corresponding amount of 1 M CaCl2 stock solution into one-Tris solution (205 mM HEPES (pH 7.2 with Trisma base)). Bath solution with 105 mM [Ca2þ ]c (105 mM CaCl2 solution) contained 105 mM CaCl2, 10 mM HEPES (pH 7.2 with Trisma base or NaOH). This solution

Scholey, Jonathan

60

Search for D?-D?? mixing in D? --> K? [pi]? [pi]? [pi]? decays  

E-Print Network [OSTI]

We present results of a search for D?-D?? mixing by analyzing D? --> K? [pi]? [pi]? [pi]? decays from events in 230.4 fb-1 e+e- data recorded by BABAR. Assuming CP conservation, we measure the time-integrated mixing rate ...

Zheng, Yi, Ph. D. Massachusetts Institute of Technology

2008-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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

Appendix D: Coal Gasifier Control: A Process Engineering Approach 208 DD.. CCOOAALL GGAASSIIFFIIEERR CCOONNTTRROOLL  

E-Print Network [OSTI]

Appendix D: Coal Gasifier Control: A Process Engineering Approach 208 DD.. CCOOAALL 24 June 1998 Coventry University #12;Appendix D: Coal Gasifier Control: A Process Engineering Approach 209 Coal Gasifier Control: A Process Engineering Approach B N Asmar, W E Jones and J A Wilson

Skogestad, Sigurd

62

40 MM Grenade Launcher Qualification Requirements at Department...  

Office of Environmental Management (EM)

launcher, which utilizes high explosive ammunition to defeat adversary personnel and equipment. A number of Department sites have procured these weapons. 40 MM Grenade...

63

Study of charge symmetry breaking in dd collisions with WASA-at-COSY  

SciTech Connect (OSTI)

Charge symmetry is an approximate symmetry of the strong interaction. Studies of its breaking can yield information on the u and d quark mass difference. A theoretical collaboration is currently working on the description of charge symmetry breaking mechanisms for dd{yields}{alpha}{pi}{sup 0} and np{yields}d{pi}{sup 0} within Chiral Perturbation Theory, using the data from TRI-UMF and IUCF. One of the items in the program of the WASA-at-COSY collaboration is to extend the data base for the dd{yields}{alpha}{pi}{sup 0} reaction to higher energies, which would allow the extraction of the information on the p-wave. Status of the analysis of experimental data along with the preliminary results from the pilot run will be presented here.

Wronska, Aleksandra [Institute of Physics, Jagiellonian University, Cracow, Reymonta 4, 30-059 Cracow (Poland)

2011-10-24T23:59:59.000Z

64

Improving D&D Planning and Waste Management with Cutting and Packaging Simulation  

SciTech Connect (OSTI)

The increased amount of decontamination and decommissioning (D&D) being performed throughout the world not only strains nuclear cleanup budgets, but places severe demands on the capacities of nuclear waste disposal sites. Although budgets and waste disposal sites have been able to accommodate the demand thus far, the increasing number of large facilities being decommissioned will cause major impacts to the waste disposal process. It is thus imperative that new and innovative technologies are applied within the D&D industry to reduce costs and waste disposal requirements for the decommissioning of our inventory of large and aging nuclear facilities. One of the most significant problems reactor owners deal with is the accurate determination of the types and volumes of wastes that will be generated during decommissioning of their facilities. Waste disposal costs, restrictions, and transportation issues can account for as much as 30% of the total costs to decommission a facility and thus it is very important to have accurate waste volume estimates. The use of simulation technologies to estimate and reduce decommissioning waste volumes provides a new way to manage risks associated with this work. Simulation improves the process by allowing facility owners to obtain accurate estimates of the types and amounts of waste prior to starting the actual D&D work. This reduces risk by permitting earlier and better negotiations with the disposal sites, and more time to resolve transportation issues. While simulation is a tool to be used by the D&D contractors, its real value is in reducing risks and costs to the reactor owners.

Richard H. Meservey; Jean-Louis Bouchet

2005-08-01T23:59:59.000Z

65

Constraining smoothness parameter and the DD relation of Dyer-Roeder equation with supernovae  

SciTech Connect (OSTI)

Our real universe is locally inhomogeneous. Dyer and Roeder introduced the smoothness parameter ? to describe the influence of local inhomogeneity on angular diameter distance, and they obtained the angular diameter distance-redshift approximate relation (Dyer-Roeder equation) for locally inhomogeneous universe. Furthermore, the Distance-Duality (DD) relation, D{sub L}(z)(1+z){sup ?2}/D{sub A}(z) = 1, should be valid for all cosmological models that are described by Riemannian geometry, where D{sub L} and D{sub A} are, respectively, the luminosity and angular distance distances. Therefore, it is necessary to test whether if the Dyer-Roeder approximate equation can satisfy the Distance-Duality relation. In this paper, we use Union2.1 SNe Ia data to constrain the smoothness parameter ? and test whether the Dyer-Roeder equation meet the DD relation. By using ?{sup 2} minimization, we get ? = 0.92{sub ?0.32}{sup +0.08} at 1? and 0.92{sub ?0.65}{sup +0.08} at 2?, and our results show that the Dyer-Roeder equation is in good consistency with the DD relation at 1?.

Yang, Xi; Yu, Hao-Ran; Zhang, Tong-Jie, E-mail: yangwds@mail.bnu.edu.cn, E-mail: yu@bnu.edu.cn, E-mail: tjzhang@bnu.edu.cn [Department of Astronomy, Beijing Normal University, Beijing 100875 (China)

2013-06-01T23:59:59.000Z

66

Course Outline ENG 2MM3 Electrical Circuits & Power  

E-Print Network [OSTI]

-Phase Induction Motor; 5. DC Generators & DC Motors; 6. Efficiency/Heating of Electric Machines; 7. ActiveCourse Outline ENG 2MM3 Electrical Circuits & Power Winter 2010 Instructor: Prof. Matiar Howlader Web Page: www.ece.mcmaster.ca/~mrhowlader/ENG2MM3Notes Text Books: 1. Electrical Power and Controls

Haykin, Simon

67

Course Outline ENG 2MM3 Electrical Circuits & Power  

E-Print Network [OSTI]

-Phase Induction Motor; 5. DC Generators & DC Motors; 6. Efficiency/Heating of Electric Machines; 7. ActiveCourse Outline ENG 2MM3 Electrical Circuits & Power Fall 2010 Instructor: Prof. Matiar Howlader Web Page: www.ece.mcmaster.ca/~mrhowlader/ENG2MM3Notes Text Books: 1. Electrical Power and Controls

Haykin, Simon

68

1.25 mM NaH2PO4, 1 mM CaCl2, 1 mM MgCl2, 26 mM NaHCO3 and 10 mM dextrose, bubbled with 95% O2/5% CO2 (pH 7.4). Slices (300400 mm thick) were prepared with a  

E-Print Network [OSTI]

1.25 mM NaH2PO4, 1 mM CaCl2, 1 mM MgCl2, 26 mM NaHCO3 and 10 mM dextrose, bubbled with 95% O2/5% CO cerebrospinal fluid (ACSF: 124 mM NaCl, 2 mM KCl, 1.5 mM MgSO4, 1.25 mM NaH2PO4, 2.5 mM CaCl2, 26 mM NaHCO3, 10

Zuker, Charles

69

Waste management regulatory compliance issues related to D&D activities at Oak Ridge National Laboratory (ORNL)  

SciTech Connect (OSTI)

The waste management activities at ORNL related to the decontamination and decommissioning (D&D) of radioactively contaminated buildings are divided into four categories: Operational facilities, inactive or surplus facilities, future facilities planning, and D&D activities. This paper only discusses regulatory issues related to inactive or surplus facilities. Additionally, rather than attempting to address all resulting waste streams and related regulations, this paper highlights only a few of the ORNL waste streams that present key regulatory issues.

Hitch, J.P.; Arnold, S.E.; Burwinkle, T.; Daugherty, D.

1994-09-01T23:59:59.000Z

70

MATERIALS MANAGEMENT OFFICE SUPPLY REQUEST FORM -MM-4  

E-Print Network [OSTI]

MATERIALS MANAGEMENT OFFICE SUPPLY REQUEST FORM - MM-4 REQUESTER'S NAME: DEPARTMENT: TTILE: MAIL. Include the justification with this form when faxing or mailing to Materials Management. Fax 679: ________________ University Director of Materials Management: _________________________________________________________ Date

Oliver, Douglas L.

71

Proceedings of the 2007 ANS Topical Meeting on Decommissioning, Decontamination, and Reutilization - DD and R 2007  

SciTech Connect (OSTI)

The American Nuclear Society (ANS) Topical Meeting on Decommissioning, Decontamination, and Reutilization (DD and R 2007), 'Capturing Decommissioning Lessons Learned', is sponsored by the ANS Decommissioning, Decontamination and Reutilization; Environmental Sciences; and Fuel Cycle and Waste Management Divisions. This meeting provides a forum for an international exchange of technical knowledge and project management experience gained from the ongoing process of decommissioning nuclear facilities. Of particular note is the number of projects that are approaching completion. This document gathers 113 presentations given at this meeting.

NONE

2008-01-15T23:59:59.000Z

72

2-D Spatial Distribution of D-D and D-T Neutron Emission in JET ELMy H-mode Plasmas with Tritium Puff  

E-Print Network [OSTI]

2-D Spatial Distribution of D-D and D-T Neutron Emission in JET ELMy H-mode Plasmas with Tritium Puff

73

PHOTOSWITCHR Photoelectric Sensors General Purpose 18mm Cylindrical Style  

E-Print Network [OSTI]

(Sensor) DC Micro For NPN type tie the load to Brown (+). For PNP type tie the load to Blue Beam Load Load Load Load Load Load Light Source Unit Protection Supply Voltage Current Consumption Photoelectric Sensors 42CA General Purpose 18mm Cylindrical Style R146 Typical Response Curve 100 1 0.1 0 1 (3

Allen, Gale

74

M/M/1 Queueing System with Delayed Controlled Vacation  

E-Print Network [OSTI]

M/M/1 Queueing System with Delayed Controlled Vacation Yonglu Deng , Zhongshan University W. John systems using a time division multiple access (TDMA) scheme (Frey and Takahashi, [7]). Researchers have that of a server's cold switch-on. The case of delayed vacation has also very recently been studied by Frey

Zhao, Yiqiang Q.

75

Design and testing of a dual 8-T 380-mm/12-T 220-mm split superconducting solenoid for ORNL  

SciTech Connect (OSTI)

A superconducting high field magnet facility has recently been prepared for operation at the Oak Ridge National Laboratory (ORNL). The facility consists of a background NbTi coil and an insert coil made of Nb/sub 3/Sn tape. The background coil produces an 8-T central field, with a peak field of 8.8 T, in a bore of 380 mm and contains radial access ports of 67-mm diam. Details of magnet design both for the background coil and insert coil will be presented. The protection scheme will be discussed and test results will be given.

Ballou, J.K.; Brown, R.L.; Fietz, W.A.; Forseman, J.W.; Gray, W.H.; Kenney, W.J.; Wysor, R.B.; Markiewicz, W.D.; Van Alstyne, R.G.

1981-01-01T23:59:59.000Z

76

Data:9772770c-c71d-418c-a771-711260dd8714 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No789501c8a3b5d3f-8637-e4b2dd7a939911260dd8714 No revision has been

77

Data:83dd866f-1ad1-4738-be83-cdba19e39264 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300acbfcc-59082908dd3e No063dd1c7a Nocdba19e39264 No

78

Sub-mm clues to elliptical galaxy formation  

E-Print Network [OSTI]

There is growing evidence that, at the S(850) 2.5, with a mean redshift z = 3.5. While radio selection raises concerns about bias, I argue that our current knowledge of the brightest (S(850) ~ 10 mJy) sub-mm sources detected in unbiased SCUBA imaging surveys indicates that they are also largely confined to this same high-z regime. Consequently, while the most recent number counts imply such extreme sources can contribute only 5-10% of the sub-mm background, their comoving number density (in the redshift band 3 < z < 5) is 1-2 x 10^{-5} per cubic megaparsec, sufficient to account for the formation of all ellipticals of comparable mass to radio galaxies (~4L-star) in the present-day universe.

James S. Dunlop

2000-11-03T23:59:59.000Z

79

Preliminary measurements of neutrons from the D-D reaction in the COMPASS tokamak  

SciTech Connect (OSTI)

Recent results of measured fast neutrons created in the D-D reaction on the COMPASS tokamak during ohmic discharges are presented in this paper. Two different type detectors were used during experiment. He-3 detectors and bubble detectors as a support. The measurements are an introduction for neutron diagnostic on tokamak COMPASS and monitoring neutrons during discharges with Neutral Beam Injection (NBI). The He-3 counters and bubble detectors were located in two positions near tokamak vacuum chamber at a distance less than 40 cm to the centre of plasma. The neutrons flux was observed in ohmic discharges. However, analysis of our results does not indicate any clear source of neutrons production during ohmic discharges.

Dankowski, J., E-mail: jan.dankowski@ifj.edu.pl; Kurowski, A.; Twarog, D. [The Henryk Niewodnicza?ski Institute of Nuclear Physics Polish Academy of Sciences, Radzikowskiego 152 Str., PL-31-342 Krakw (Poland); Janky, F.; Stockel, J. [Institute of Plasma Physics AS CR, v.v.i. Za Slovankou 1782/3, 182 00 Prague 8 (Czech Republic)

2014-08-21T23:59:59.000Z

80

Standard Model Predictions and New Physics Sensitivity in B->DD Decays  

E-Print Network [OSTI]

An extensive model-independent analysis of B->DD decays is carried out employing SU(3) flavour symmetry, including symmetry-breaking corrections. Several theoretically clean observables are identified which allow for testing the Standard Model. These include the known time-dependent CP asymmetries, the penguin pollution of which can be controlled in this framework, but notably also quasi-isospin relations which are experimentally well accessible and unaffected by symmetry-breaking corrections. Theoretical assumptions can be kept to a minimum and controlled by additional sum rules. Available data are used in global fits to predict the branching ratio for the B0->DsDs decay as well as several CP asymmetries which have not been measured so far, and future prospects are analyzed.

Jung, Martin

2014-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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.


81

Public Can Comment on Proposed D&D and Waste Disposition Plans for EM's Portsmouth Site Through March 11  

Broader source: Energy.gov [DOE]

WAVERLY, Ohio Approximately 150 neighbors, community leaders, workers, and other interested people participated in a public meeting Nov. 17 near the Portsmouth Gaseous Diffusion Plant site to hear from EM and its decontamination and decommissioning (D&D) contractor, Fluor-B&W Portsmouth LLC, about options for future cleanup of the site.

82

The redshifts of bright sub-mm sources  

E-Print Network [OSTI]

One of the key goals in observational cosmology over the next few years will be to establish the redshift distribution of the recently-discovered sub-mm source population. In this brief review I discuss and summarize the redshift information which has been gleaned to date for the ~ 50 bright sub-mm sources which have been uncovered via the six main classes of survey performed with SCUBA on the JCMT over the last 2-3 years. Despite the biases inherent in some of these surveys, and the crudeness of the redshift information available in others, I conclude that all current information suggests that only 10-15 % of luminous sub-mm sources lie at z < 2, and that the median redshift of this population is z ~ 3. I suggest that such a high median redshift is arguably not unexpected given current theories designed to explain the correlation between black-hole mass and spheroid mass found at low redshift. In such scenarios, peak AGN emission is expected to correspond to, or even to cause termination of major star-formation activity in the host spheroid. In contrast, maximum dust emission is expected to occur roughly half-way through the star-formation process. Given that optical emission from bright quasars peaks at z = 2.5, dust-emission from massive ellipticals might be reasonably expected to peak at some point in the preceding ~ 1 Gyr, at z ~ 3. Confirmation or refutation of this picture requires significantly-improved redshift information on bright samples of SCUBA sources.

James S. Dunlop

2001-01-17T23:59:59.000Z

83

Businss Operations Calendar: YY 2015  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAboutScienceCareersEnergy,ServicesBurningOperations

84

Measurement of the Enhanced Screening Effect of the d+d Reactions in Metals  

E-Print Network [OSTI]

The investigation of the d+d fusion reactions in metallic environments at sub-Coulomb energies demands especially adapted techniques beyond standard procedures in nuclear physics. The measurements which were performed with an electrostatic accelerator at different self-implanted metallic target materials show an enhancement of the reaction cross-section compared to the gas target experiments. The resulting electron screening energy values are about one order of magnitude larger relative to the gas target experiments and exceed significantly the theoretical predictions. The measurements on deuterium inside metals are heavily affected by the interference of two peculiarities of this system: the possibly very high mobility of deuterium in solids and the formation of surface contamination layers under ion beam irradiation in high vacuum systems. Thorough investigations of these processes show their crucial influence on the interpretation of the experimental raw data. The differential data acquisition and analysis method employed to it is outlined. Non observance of these problems by using standard procedures results in fatal errors for the extraction of the screening energies.

A. Huke; K. Czerski; P. Heide

2007-01-26T23:59:59.000Z

85

Measurement of the Neutron Spectrum of a DD Electronic Neutron Generator  

SciTech Connect (OSTI)

A Cuttler-Shalev (C-S) 3He proportional counter has been used to measure the energy spectrum of neutrons from a portable deuterium-deuterium electronic neutron generator. To improve the analysis of results from the C-S detector digital pulse shape analysis techniques have been used to eliminate neutron recoil artifacts in the recorded data. Data was collected using a 8-GHz, 10-bit waveform digitizer with its full scale corresponding to approximately 6-MeV neutrons. The measurements were made with the detector axis perpendicular to the direction of ions in the ENG in a plane 0.5-m to the side of the ENG, measuring neutrons emitted at an angle from 87.3? to 92.7? with respect to the path of ions in the ENG. The system demonstrated an energy resolution of approximately 0.040 MeV for the thermal peak and approximately 0.13 MeV at the DD neutron energy. In order to achieve the ultimate resolution capable with this type of detector it is clear that a higher-precision digitizer will be needed.

D. L. Chichester; J. T. Johnson; E. H. Seabury

2010-08-01T23:59:59.000Z

86

ORNL Soils Remediation and Slabs Removal The Bridge from D&D to Redevelopment  

SciTech Connect (OSTI)

The landscape of the Oak Ridge National Laboratory (ORNL) has dramatically changed over the past 2 years with demolition of aging facilities in the Central Campus. Removal of these infrastructure legacies was possible due to an influx of DOE-Environmental Management funding through the American Recovery and Reinvestment Act of 2009 (ARRA). Facility D&D traditionally removes everything down to the building slab, and the Soils and Sediments Program is responsible for slabs, below-grade footers, abandoned waste utilities, and soils contaminated above certain risk levels that must be removed before the site can be considered for redevelopment. , DOE-EM has used a combination of base and ARRA funding to facilitate the clean-up process in ORNL s 2000 Area. Demolition of 13 buildings in the area was funded by the ARRA. Characterization of the remaining slabs, underground pipelines and soils was funded by DOE-EM base funding. Additional ARRA funding was provided for the removal of the slabs, pipelines and contaminated soils. Removal work is in progress and consists of removing and disposing of approximately 10,000 cubic yards (CY) of concrete, 2,500 CY of debris, and 500 CY of contaminated soil. The completion of this work will allow the site to be available for redevelopment and site reuse efforts at ORNL.

Conger, M Malinda [ORNL; Schneider, Ken R [ORNL

2012-01-01T23:59:59.000Z

87

Large-scale Demonstration and Deployment Project for D&D of Fuel Storage Canals and Associated Facilities at INEEL  

SciTech Connect (OSTI)

The Department of Energy (DOE) Office of Science and Technology (OST), Deactivation and Decommissioning Focus Area (DDFA), sponsored a Large Scale Demonstration and Deployment Project (LSDDP) at the Idaho National Engineering and Environmental Laboratory (INEEL) under management of the DOE National Energy Technology Laboratory (NETL). The INEEL LSDDP is one of several LSDDPs sponsored by DOE. The LSDDP process integrates field demonstrations into actual decontamination and decommissioning (D&D) operations by comparing new or improved technologies against existing baseline technologies using a side-by-side comparison. The goals are (a) to identify technologies that are cheaper, safer, faster, and cleaner (produce less waste), and (b) to incorporate those technologies into D&D baseline operations. The INEEL LSDDP reviewed more than 300 technologies, screened 141, and demonstrated 17. These 17 technologies have been deployed a total of 70 times at facilities other than those where the technology was demonstrated, and 10 have become baseline at the INEEL. Fifteen INEEL D&D needs have been modified or removed from the Needs Management System as a direct result of using these new technologies. Conservatively, the ten-year projected cost savings at the INEEL resulting from use of the technologies demonstrated in this INEEL LSDDP exceeds $39 million dollars.

Whitmill, Larry Joseph

2001-12-01T23:59:59.000Z

88

Digital Frequency Domain Multiplexer for mm-Wavelength Telescopes  

SciTech Connect (OSTI)

An FPGA based digital signal processing (DSP) system for biasing and reading out multiplexed bolometric detectors for mm-wavelength telescopes is presented. This readout system is being deployed for balloon-borne and ground based cosmology experiments with the primary goal of measuring the signature of inflation with the Cosmic Microwave Background Radiation. The system consists of analog superconducting electronics running at 250 mK and 4 K, coupled to digital room temperature backend electronics described here. The digital electronics perform the real time functionality with DSP algorithms implemented in firmware. A soft embedded processor provides all of the slow housekeeping control and communications. Each board in the system synthesizes multi-frequency combs of 8 to 32 carriers in the MHz band to bias the detectors. After the carriers have been modulated with the sky-signal by the detectors, the same boards digitize the comb directly. The carriers are mixed down to base-band and low pass filtered. The signal bandwidth of 0.050Hz-100 Hz places extreme requirements on stability and requires powerful filtering techniques to recover the sky-signal from the MHz carriers.

Spieler, Helmuth G; Dobbs, Matt; Bissonnette, Eric; Spieler, Helmuth G.

2007-07-23T23:59:59.000Z

89

Data:Dd4c985c-73c7-4f1b-a774-9964f2dd7ce5 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision has been approved

90

Implementation of DOE/NFDI D&D Cost Estimating Tool (POWERtool) for Initiative Facilities at the Savannah River Site  

SciTech Connect (OSTI)

The Savannah River Site (SRS) has embarked on an aggressive D&D program to reduce the footprint of excess facilities. Key to the success of this effort is the preparation of accurate cost estimates for decommissioning. SRS traditionally uses ''top-down'' rough order-of-magnitude (ROM) estimating for decommissioning cost estimates. A second cost estimating method (POWERtool) using a ''bottoms-up'' approach has been applied to many of the SRS excess facilities in the T and D-area. This paper describes the use of both estimating methods and compares the estimated costs to actual costs of 5 facilities that were decommissioned in 2002.

Austin, W. E.; WSRC; Baker, S. B. III, Cutshall, C. M.; Crouse, J. L.

2003-02-26T23:59:59.000Z

91

Data:6133353e-33af-4276-a282-3daf0dd8a3ba | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved for thisbade-2c5cfacaa2ee No revisiondaf0dd8a3ba No revision has been

92

Data:52eabb28-cd1d-43dd-80d2-219739044111 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b Nobfef8fa58cf74865627f783eabb28-cd1d-43dd-80d2-219739044111 No revision has been

93

Data:9bdf2d28-2c28-4026-adb9-dd6567952019 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision has been approved for7a-a33e-3aa1431a0b90 No revision6-adb9-dd6567952019 No

94

Data:D9d93ea5-7031-4192-8814-92268dd664a0 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has beenadf9-4884-b0c1-529b3bb19f9c No2-d6f420785d1d No revision has been68dd664a0 No revision

95

Data:Dd970074-b298-4754-91a4-b28077373b20 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5bac6-bfb65e3d4028b28077373b20 No

96

Data:838f1203-9378-4f83-bfcc-59082908dd3e | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300acbfcc-59082908dd3e No revision has been approved for

97

Data:8772df9b-032c-41bd-98da-19dd3cb485dc | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revisionb27d098e Nod173ef850e7b37914bbdf Noc-54044054ab55 No19dd3cb485dc No

98

Data:3ecdc92f-5486-4912-a5dd-927eddd17c1c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has been approved64ec514 Noc707c3a4d4cdc3dd4086bc-36c3421918ca

99

Heat Transfer -2 A pure platinum wire with diameter D = 3 mm and length L = 20 mm is placed outside on a day when air temperature  

E-Print Network [OSTI]

Heat Transfer - 2 A pure platinum wire with diameter D = 3 mm and length L = 20 mm is placed outside on a day when air temperature T = 10o C. The heat transfer coefficient at the wire's surface h equation that includes all heat transfer mechanisms involved in this problem. Write this energy balance

Virginia Tech

100

A Polarizable QM/MM Explicit Solvent Model for Computational Electrochemistry in Water  

E-Print Network [OSTI]

We present a quantum mechanical/molecular mechanical (QM/MM) explicit solvent model for the computation of standard reduction potentials E[subscript 0]. The QM/MM model uses density functional theory (DFT) to model the ...

Wang, Lee-Ping

Note: This page contains sample records for the topic "mm dd yy" from the National Library of EnergyBeta (NLEBeta).
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We encourage you to perform a real-time search of NLEBeta
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101

Breakdown of 2mm symmetry in electron diffraction from multiwalled carbon nanotubes  

E-Print Network [OSTI]

Breakdown of 2mm symmetry in electron diffraction from multiwalled carbon nanotubes Zejian Liu of single-walled carbon nanotubes always have 2mm symmetry regardless if the nanotubes them- selves have such symmetry. We here show that, for the case of multiwalled carbon nanotubes, the 2mm symmetry can break down

Qin, Lu-Chang

102

450 mm dual frequency capacitively coupled plasma sources: Conventional, graded, and segmented electrodes  

E-Print Network [OSTI]

450 mm dual frequency capacitively coupled plasma sources: Conventional, graded, and segmented fabrication will soon transition from 300 to 450 mm at a time when excitation frequencies for capacitively of processing. The increase in diameter to 450 mm is likely to exacerbate these effects, perhaps requiring

Kushner, Mark

103

Observation of the {psi}(4415){yields}DD{sub 2}*(2460) Decay Using Initial-State Radiation  

SciTech Connect (OSTI)

We report measurements of the exclusive cross section for e{sup +}e{sup -}{yields}D{sup 0}D{sup -}{pi}{sup +} over the center-of-mass energy range 4.0 GeV to 5.0 GeV with initial-state radiation and the first observation of the decay {psi}(4415){yields}D{sup 0}D{sup -}{pi}{sup +}. From a study of the resonant substructure in {psi}(4415) decay we conclude that the {psi}(4415){yields}D{sup 0}D{sup -}{pi}{sup +} decay is dominated by {psi}(4415){yields}DD{sub 2}*(2460). We obtain B({psi}(4415){yields}D{sup 0}D{sup -}{pi}{sub nonresonant}{sup +})/B({psi}(4415){yields}DD{sub 2}*(24 = 60){yields}D{sup 0}D{sup -}{pi}{sup +})<0.22 at 90% C.L. The analysis is based on a data sample collected with the Belle detector with an integrated luminosity of 673 fb{sup -1}.

Pakhlova, G.; Balagura, V.; Chistov, R.; Danilov, M.; Liventsev, D.; Medvedeva, T.; Mizuk, R.; Pakhlov, P.; Tikhomirov, I.; Uglov, T. [Institute for Theoretical and Experimental Physics, Moscow (Russian Federation); Adachi, I.; Brodzicka, J.; Haba, J.; Hazumi, M.; Itoh, R.; Iwasaki, Y.; Kibayashi, A.; Kichimi, H.; Krokovny, P.; Nakao, M. [High Energy Accelerator Research Organization (KEK), Tsukuba (Japan)] (and others)

2008-02-15T23:59:59.000Z

104

Data:836e7240-8724-4fc7-8925-9dd9d3e233a9 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300ac Noc1e69d7992f-3f3dd886bf1c1dc0188f0dd9d3e233a9 No

105

Data:83be13c0-5016-4add-881b-ba3063dd1c7a | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300acbfcc-59082908dd3e No063dd1c7a No revision has been

106

Data:83ca2721-b57a-43eb-891b-dd84c6a300c7 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300acbfcc-59082908dd3e No063dd1c7a No revision has

107

X-Ray Measurements Of A Thermo Scientific P385 DD Neutron Generator  

SciTech Connect (OSTI)

Idaho National Laboratory is experimenting with electrical neutron generators, as potential replacements for californium-252 radioisotopic neutron sources in its PINS prompt gamma-ray neutron activation analysis (PGNAA) system for the identification of military chemical warfare agents and explosives. In addition to neutron output, we have recently measured the x-ray output of the Thermo Scientific P385 deuterium-deuterium neutron generator. X rays are a normal byproduct from neutron generators, but depending on their intensity and energy, x rays can interfere with gamma rays from the object under test, increase gamma-spectrometer dead time, and reduce PGNAA system throughput. The P385 x-ray energy spectrum was measured with a high-purity germanium (HPGe) detector, and a broad peak is evident at about 70 keV. To identify the source of the x rays within the neutron generator assembly, it was scanned by collimated scintillation detectors along its long axis. At the strongest x-ray emission points, the generator also was rotated 60 deg. between measurements. The scans show the primary source of x-ray emission from the P385 neutron generator is an area 60 mm from the neutron production target, in the vicinity of the ion source. Rotation of the neutron generator did not significantly alter the x-ray count rate, and its x-ray emission appears to be axially symmetric. A thin lead shield, 3.2 mm (1/8 inch) thick, reduced the 70-keV generator x rays to negligible levels.

Wharton, C. J.; Seabury, E. H.; Chichester, D. L.; Caffrey, A. J. [Idaho National Laboratory, 2525 N. Freemont Avenue, Idaho Falls, Idaho 83415 (United States); Simpson, J.; Lemchak, M. [Thermo-Fisher Scientific/MF Physics, 5074 List Drive, Colorado Springs, Colorado 80919 (United States)

2011-06-01T23:59:59.000Z

108

Data:28d59351-f16b-4707-bbb7-d7ad1dd3342a | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 Noc7e1a8ffe No revision has been approved7af2e2cf0e85488a7fe3a3badf5 Noedc47ab2bbb7-d7ad1dd3342a

109

Microsoft Word - WH-MM-818B-819B NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

8B & WH-MM-819B Title: Repair WH Brine Tanks, WHT-14 & WHT-15 Description: Subcontractor shall shall provide all materials, tools, equipment, supplies, transportation, facilities,...

110

Compact D-D Neutron Source-Driven Subcritical Multiplier and Beam-Shaping Assembly for Boron Neutron Capture Therapy  

SciTech Connect (OSTI)

This work assesses the feasibility of using a small, safe, and inexpensive keff 0.98 subcritical fission assembly [subcritical neutron multiplier (SCM)] to amplify the treatment neutron beam intensity attainable from a compact deuterium-deuterium (D-D) fusion neutron source delivering [approximately]1012 n/s. The objective is to reduce the treatment time for deep-seated brain tumors to [approximately]1 h. The paper describes the optimal SCM design and two optimal beam-shaping assemblies (BSAs) - one designed to maximize the dose rate and the other designed to maximize the total dose that can be delivered to a deep-seated tumor. The neutron beam intensity amplification achieved with the optimized SCM and BSA results in an increase in the treatment dose rate by a factor of 18: from 0.56 Gy/h without the SCM to 10.1 Gy/h. The entire SCM is encased in an aluminum structure. The total amount of 20% enriched uranium required for the SCM is 8.5 kg, and the cost (not including fabrication) is estimated to be less than $60,000. The SCM power level is estimated at 400 W when driven by a 1012 n/s D-D neutron source. This translates into consumption of only [approximately]0.6% of the initially loaded 235U atoms during 50 years of continuous operation and implies that the SCM could operate continuously for the entire lifetime of the facility without refueling. Cooling the SCM does not pose a challenge; it may be accomplished by natural circulation as the maximum heat flux is only 0.034 W/cm2.

Francesco Ganda; Jasmina Vujic; Ehud Greenspan; Ka-Ngo Leung

2010-12-01T23:59:59.000Z

111

CC II RR EE DD 18th International Conference on Electricity Distribution Turin, 6-9 June 2005 Session No 4  

E-Print Network [OSTI]

CC II RR EE DD 18th International Conference on Electricity Distribution Turin, 6-9 June 2005 CIRED Kingdom P.Vovos@ed.ac.uk INTRODUCTION Electricity networks are called on to accommodate more and more by adjusting their reactive power output, as it may destabilise the automatic Load Tap Changers (LTCs

Harrison, Gareth

112

PPPL-3207, Preprint: October 1996, UC-420, 421, 423, 426 Core V and Ti Profiles and Transport in TFTR DD and DT  

E-Print Network [OSTI]

/wall interactions relative to performance of advanced tokamaks. The effects of lithium on plasma performance were in TFTR DD and DT Plasmas with Lithium Conditioning C. E. Busha, R. E. Bellb, B. LeBlancb, D. K with lithium (Li) conditioned graphite walls in TFTR. Values of E > 300 ms have been obtained with neutron

113

PPPL3207, Preprint: October 1996, UC420, 421, 423, 426 Core Vf and T i Profiles and Transport in TFTR DD and DT  

E-Print Network [OSTI]

/wall interactions relative to performance of advanced tokamaks. The effects of lithium on plasma performance were in TFTR DD and DT Plasmas with Lithium Conditioning C. E. Bush a , R. E. Bell b , B. LeBlanc b , D. K neutral beam heating with lithium (Li) conditioned graphite walls in TFTR. Values of tE > 300 ms have been

114

Vapor deposition of platinum alloyed nickel aluminide coatings Z. Yu , K.P. Dharmasena, D.D. Hass, H.N.G. Wadley  

E-Print Network [OSTI]

Vapor deposition of platinum alloyed nickel aluminide coatings Z. Yu , K.P. Dharmasena, D.D. Hass at high temperature. It requires the chemical vapor deposition of aluminum on a nickel rich superalloy substrate that has been pre-coated with several microns of electrodeposited platinum. Here, we show

Wadley, Haydn

115

Evaluation of Offshore Wind Simulations with MM5 in the Japanese and Danish Coastal Waters  

E-Print Network [OSTI]

Evaluation of Offshore Wind Simulations with MM5 in the Japanese and Danish Coastal Waters Teruo to evaluate the accuracy of offshore wind simulation with the mesoscale model MM5, long-term simulations to simulate offshore wind conditions in the Japanese coastal waters even using a mesoscale model, compared

Heinemann, Detlev

116

Hybrid QM/MM Car-Parrinello Simulations of Catalytic and Enzymatic Reactions  

E-Print Network [OSTI]

1 Hybrid QM/MM Car-Parrinello Simulations of Catalytic and Enzymatic Reactions MariaCarola Colombo, we review some recent applications of hybrid Car-Parrinello simulations of chemical and biological recently developed a combination of these two techniques into a hybrid QM/MM Car-Parrinello scheme [4

Guidoni, Leonardo

117

MECHANICAL TEST RESULTS ON DIPOLE MODEL C-l 25 mm ALUMINUM COLLARS  

E-Print Network [OSTI]

P~. FI'9 . ~ C.C rv'IW\\ 707~-Th ALUMINUM ' ~LAI2.. o Pl.ATTDIPOLE MODEL C-1 25 mm ALUMINUM COLLARS C. Peters FebruaryON DIPOLE MODEL C-I 25 mm ALUMINUM COLLARS Craig Peters

Peters, C.

2010-01-01T23:59:59.000Z

118

Geometry Optimization with QM/MM, ONIOM, and Other Combined Methods. I. Microiterations  

E-Print Network [OSTI]

Geometry Optimization with QM/MM, ONIOM, and Other Combined Methods. I. Microiterations calculation, have been very successful in describing large systems. Geometry optimization methods can take). A series of microit- erations can be employed to fully optimize the MM region for each optimization step

Schlegel, H. Bernhard

119

The near-infrared Hubble diagram for sub-mm galaxies  

E-Print Network [OSTI]

Determing the nature of the bright sub-mm sources and their role in the process of galaxy formation is likely to be a major focus of extra-galactic research over the next few years. In particular, we would like to know if these sources are the progenitors of today's massive elliptical galaxies, or alternatively arise from short-lived, albeit spectacular starbursts within haloes of unexceptional mass. This question can be addressed from a number of different directions, one of which is to compare the masses of sub-mm host galaxies with those of other known massive high-redshift objects. Here I make a first attempt to do this by exploring whether the few well-studied sub-mm/mm sources are consistent with the well-established K-z relation for powerful radio galaxies. Out to z = 3 this appears to be the case, providing evidence that bright sub-mm sources are indeed destined to be massive ellipticals. At higher redshifts there is a suggestion that sub-mm galaxies are signficantly fainter at K than their radio-selected counterparts, but at present it is unclear whether this indicates a significant difference in stellar mass or the increasing impact of dust obscuration on the rest-frame light from the sub-mm hosts.

James S. Dunlop

2002-03-12T23:59:59.000Z

120

Of horseshoes and heliotropes: Dynamics of dust in the Encke Gap M.M. Hedman a,  

E-Print Network [OSTI]

Of horseshoes and heliotropes: Dynamics of dust in the Encke Gap M.M. Hedman a, , J.A. Burns a located within the Cassini Division's Laplace Gap demonstrates ``heliotropic'' behavior: its geometric

Hamilton, Douglas P.

Note: This page contains sample records for the topic "mm dd yy" 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.


121

MagLab - Cell 15: 45.1 Tesla / 32 mm Hybrid Magnet  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Magnets & Facilities Arrow Cell 15: 45.1 Tesla 32 mm Hybrid Magnet The labs flagship magnet, the 45 T Hybrid, is composed of a 33.5 T resistive magnet nested in an 11.5 T...

122

Optical rotation in RbTiOAsO4 (point group mm2) W. Kaminsky*, I  

E-Print Network [OSTI]

Optical rotation in RbTiOAsO4 (point group mm2) W. Kaminsky*, I , P. A. ThomasII and A. M. Glazer, UK Received March 5, 2001; accepted September 13, 2001 Abstract. Measurement of optical rotation in RbTiOAsO4 (RTA) with the tilter method resulted in an optical rotation of r12 ¼ þ17ð3? /mm

Kaminsky, Werner

123

A compact proton spectrometer for measurement of the absolute DD proton spectrum from which yield and ?R are determined in thin-shell inertial-confinement-fusion implosions  

SciTech Connect (OSTI)

A compact, step range filter proton spectrometer has been developed for the measurement of the absolute DD proton spectrum, from which yield and areal density (?R) are inferred for deuterium-filled thin-shell inertial confinement fusion implosions. This spectrometer, which is based on tantalum step-range filters, is sensitive to protons in the energy range 1-9 MeV and can be used to measure proton spectra at mean energies of ?1-3 MeV. It has been developed and implemented using a linear accelerator and applied to experiments at the OMEGA laser facility and the National Ignition Facility (NIF). Modeling of the proton slowing in the filters is necessary to construct the spectrum, and the yield and energy uncertainties are <10% in yield and 120?keV, respectively. This spectrometer can be used for in situ calibration of DD-neutron yield diagnostics at the NIF.

Rosenberg, M. J., E-mail: mrosenbe@mit.edu; Zylstra, A. B.; Frenje, J. A.; Rinderknecht, H. G.; Gatu Johnson, M.; Waugh, C. J.; Sguin, F. H.; Sio, H.; Sinenian, N.; Li, C. K.; Petrasso, R. D. [Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States); Glebov, V. Yu.; Hohenberger, M.; Stoeckl, C.; Sangster, T. C. [Laboratory for Laser Energetics, University of Rochester, Rochester, New York 14623 (United States); Yeamans, C. B.; LePape, S.; Mackinnon, A. J.; Bionta, R. M.; Talison, B. [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States); and others

2014-10-15T23:59:59.000Z

124

Data:1fe29ef0-91ee-4ab5-924d-b3c7ea445dd6 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision5af6d400c2d No529a57c00c0 No revision has75f38de27dd-9676-67406d29c468d-b3c7ea445dd6

125

Data:4bb04cdd-cba8-46dd-a0d5-1da64b6a4bcf | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revisione66e17fc7f7d25b394 Noc98dd29320 No11301ee4674-46dd-a0d5-1da64b6a4bcf No

126

Data:A44de58c-11bd-4e36-b8e1-dd2e360e5d46 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05a97219c78 Noa9b16c55c7a0 Noed1f5fc9 No-b8e1-dd2e360e5d46 No

127

Development and application of QM/MM methods to study the solvation effects and surfaces  

SciTech Connect (OSTI)

Quantum mechanical (QM) calculations have the advantage of attaining high-level accuracy, however QM calculations become computationally inefficient as the size of the system grows. Solving complex molecular problems on large systems and ensembles by using quantum mechanics still poses a challenge in terms of the computational cost. Methods that are based on classical mechanics are an inexpensive alternative, but they lack accuracy. A good trade off between accuracy and efficiency is achieved by combining QM methods with molecular mechanics (MM) methods to use the robustness of the QM methods in terms of accuracy and the MM methods to minimize the computational cost. Two types of QM combined with MM (QM/MM) methods are the main focus of the present dissertation: the application and development of QM/MM methods for solvation studies and reactions on the Si(100) surface. The solvation studies were performed using a discreet solvation model that is largely based on first principles called the effective fragment potential method (EFP). The main idea of combining the EFP method with quantum mechanics is to accurately treat the solute-solvent and solvent-solvent interactions, such as electrostatic, polarization, dispersion and charge transfer, that are important in correctly calculating solvent effects on systems of interest. A second QM/MM method called SIMOMM (surface integrated molecular orbital molecular mechanics) is a hybrid QM/MM embedded cluster model that mimics the real surface.3 This method was employed to calculate the potential energy surfaces for reactions of atomic O on the Si(100) surface. The hybrid QM/MM method is a computationally inexpensive approach for studying reactions on larger surfaces in a reasonably accurate and efficient manner. This thesis is comprised of four chapters: Chapter 1 describes the general overview and motivation of the dissertation and gives a broad background of the computational methods that have been employed in this work. Chapter 2 illustrates the methodology of the interface of the EFP method with the configuration interaction with single excitations (CIS) method to study solvent effects in excited states. Chapter 3 discusses the study of the adiabatic electron affinity of the hydroxyl radical in aqueous solution and in micro-solvated clusters using a QM/EFP method. Chapter 4 describes the study of etching and diffusion of oxygen atom on a reconstructed Si(100)-2 x 1 surface using a hybrid QM/MM embedded cluster model (SIMOMM). Chapter 4 elucidates the application of the EFP method towards the understanding of the aqueous ionization potential of Na atom. Finally, a general conclusion of this dissertation work and prospective future direction are presented in Chapter 6.

Dibya, Pooja Arora

2010-05-16T23:59:59.000Z

128

450 mm dual frequency capacitively coupled plasma sources: Conventional, graded, and segmented electrodes  

SciTech Connect (OSTI)

Wafer diameters for microelectronics fabrication will soon transition from 300 to 450 mm at a time when excitation frequencies for capacitively coupled plasmas (CCPs) are increasing to 200 MHz or higher. Already for 300 mm tools, there is evidence that wave behavior (i.e., propagation, constructive, and destructive interference) affects the uniformity of processing. The increase in diameter to 450 mm is likely to exacerbate these effects, perhaps requiring nontraditional tool designs. This is particularly important in dual frequency (DF) CCP tools in which there are potential interactions between frequencies. In this paper, results from a two-dimensional computational investigation of Ar plasma properties in a 450 mm DF-CCP reactor, incorporating a full-wave solution of Maxwell's equations, are discussed. As in 300 mm DF-CCP reactors, the electron density collapses toward the center of the reactor with increasing high frequency (HF), however, with more pronounced finite wavelength effects. Graded conductivity electrodes with multilayer of dielectrics are computationally demonstrated as a possible means to suppress wave effects thereby increasing plasma uniformity. Segmentation of the HF electrode also improves the plasma uniformity by making the electrical distance between the feeds and the sheath edges as uniform as possible.

Yang Yang [Department of Electrical and Computer Engineering, Iowa State University, Ames, Iowa 50011 (United States); Kushner, Mark J. [Department of Electrical Engineering and Computer Science, University of Michigan, 1301 Beal Avenue, Ann Arbor, Michigan 48109-2122 (United States)

2010-12-01T23:59:59.000Z

129

THE CREATIVE APPLICATION OF SCIENCE TECHNOLOGY & WORK FORCE INNOVATIONS TO THE D&D OF PLUTONIUM FINISHING PLANT (PFP) AT THE HANFORD NUCLEAR RESERVATION  

SciTech Connect (OSTI)

The Plutonium Finishing Plant (PFP) consists of a number of process and support buildings for handling plutonium. Building construction began in the late 1940's to meet national priorities and became operational in 1950 producing refined plutonium salts and metal for the United States nuclear weapons program. The primary mission of the PFP was to provide plutonium used as special nuclear material for fabrication into a nuclear device for the war effort. Subsequent to the end of World War II, the PFP's mission expanded to support the Cold War effort through plutonium production during the nuclear arms race. PFP has now completed its mission and is fully engaged in deactivation, decontamination and decommissioning (D&D). At this time the PFP buildings are planned to be reduced to ground level (slab-on-grade) and the site remediated to satisfy national, Department of Energy (DOE) and Washington state requirements. The D&D of a highly contaminated plutonium processing facility presents a plethora of challenges. PFP personnel approached the D&D mission with a can-do attitude. They went into D&D knowing they were facing a lot of challenges and unknowns. There were concerns about the configuration control associated with drawings of these old process facilities. There were unknowns regarding the location of electrical lines and process piping containing chemical residues such as strong acids and caustics. The gloveboxes were highly contaminated with plutonium and chemical residues. Most of the glovebox windows were opaque with splashed process chemicals that coated the windows or etched them, reducing visibility to near zero. Visibility into the glovebox was a serious worker concern. Additionally, all the gloves in the gloveboxes were degraded and unusable. Replacing gloves in gloveboxes was necessary to even begin glovebox cleanout. The sheer volume of breathing air needed was also an issue. These and other challenges and PFP's approach to overcome these challengers are described. Many of the challenges to the D&D work at PFP were met with innovative approaches based on new science and/or technology and many were also based on the creativity and motivation of the work force personnel.

CHARBONEAU, S.L.

2006-02-01T23:59:59.000Z

130

Observed Multi-Decade DD and DT Z-Pinch Fusion Rate Scaling in 5 Dense Plasma Focus Fusion Machines  

SciTech Connect (OSTI)

Dense Plasma Focus (DPF) machines are in use worldwide or a wide variety of applications; one of these is to produce intense, short bursts of fusion via r-Z pinch heating and compression of a working gas. We have designed and constructed a series of these, ranging from portable to a maximum energy storage capacity of 2 MJ. Fusion rates from 5 DPF pulsed fusion generators have been measured in a single laboratory using calibrated activation detectors. Measured rates range from ~ 1015 to more than 1019 fusions per second have been measured. Fusion rates from the intense short (20 50 ns) periods of production were inferred from measurement of neutron production using both calibrated activation detectors and scintillator-PMT neutron time of flight (NTOF) detectors. The NTOF detectors are arranged to measure neutrons versus time over flight paths of 30 Meters. Fusion rate scaling versus energy and current will be discussed. Data showing observed fusion cutoff at D-D fusion yield levels of approximately 1?1012, and corresponding tube currents of ~ 3 MA will be shown. Energy asymmetry of product neutrons will also be discussed. Data from the NTOF lines of sight have been used to measure energy asymmetries of the fusion neutrons. From this, center of mass energies for the D(d,n)3He reaction are inferred. A novel re-entrant chamber that allows extremely high single pulse neutron doses (> 109 neutrons/cm2 in 50 ns) to be supplied to samples will be described. Machine characteristics and detector types will be discussed.

Hagen, E. C. [National Security Technologies, LLC; Lowe, D. R. [National Security Technologies, LLC; O'Brien, R. [University of Nevada, Las Vegas; Meehan, B. T. [National Security Technologies, LLC

2013-06-18T23:59:59.000Z

131

Polystyrene PS648 outlet optical birefringence pattern, piston speed 1.0mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 1.0 mm/s at 170C. Video shows the outlet flow (from top to bottom)....

Hassell, David

2008-08-27T23:59:59.000Z

132

Polystyrene PS648 inlet optical birefringence pattern, piston speed 1.4mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 1.4 mm/s at 170C. Video shows the inlet flow (from bottom to top)....

Hassell, David

2008-08-27T23:59:59.000Z

133

Polystyrene PS648 inlet optical birefringence pattern, piston speed 1.0mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 1.0 mm/s at 170C. Video shows the inlet flow (from bottom to top)....

Hassell, David

2008-08-27T23:59:59.000Z

134

Polystyrene PS648 outlet optical birefringence pattern, piston speed 1.4mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 1.4 mm/s at 170C. Video shows the outlet flow (from top to bottom)....

Hassell, David

2008-08-27T23:59:59.000Z

135

Polystyrene PS648 outlet optical birefringence pattern, piston speed 0.16mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 0.16 mm/s at 170C. Video shows the outlet flow (from top...

Hassell, David

2008-08-27T23:59:59.000Z

136

Polystyrene PS648 inlet optical birefringence pattern, piston speed 0.16mm/s  

E-Print Network [OSTI]

The optical birefringence pattern obtained from polystyrene PS648 flowing through a narrow slit. Experiment conducted on the Cambridge Multi Pass Rheometer (MPR4) at a piston speed of 0.16 mm/s at 170C. Video shows the inlet flow (from bottom to top)....

Hassell, David

2008-08-27T23:59:59.000Z

137

Greenland ice sheet surface mass balance variability (1988-2004) from calibrated Polar MM5 output*  

E-Print Network [OSTI]

1 Greenland ice sheet surface mass balance variability (1988-2004) from calibrated Polar MM5 output in Environmental Sciences, University of Colorado, Boulder, CO, USA 4 National Snow and Ice Data Center, University coherent regional patterns of Greenland ice sheet surface mass balance (SMB) change over a 17-year period

Howat, Ian M.

138

ALUMINUM SITING IN THE ZSM-22 AND THETA-1 ZEOLITES REVISITED: A QM/MM STUDY  

E-Print Network [OSTI]

ALUMINUM SITING IN THE ZSM-22 AND THETA-1 ZEOLITES REVISITED: A QM/MM STUDY Stepan SKLENAKa1. 73, Nos. 6­7, pp. 909­920 Aluminum Siting in the ZSM-22 and Theta-1 Zeolites Revisited 909 © 2008

Sklenak, Stepan

139

AbstractLarge (>458 mm) striped bass (Morone saxatilis) are dominant  

E-Print Network [OSTI]

fishes and anadromous herrings (Alosa spp.) also contibuted large percentages of striped bass diet of striped Dorazio et al., 1994). After spawning, bass experienced drastic declines in the these fish leave414 AbstractLarge (>458 mm) striped bass (Morone saxatilis) are dominant predators in Chesapeake

140

M.M. AbdouAbdou TBWGTBWG--13 Meeting13 Meeting  

E-Print Network [OSTI]

M.M. AbdouAbdou TBWGTBWG--13 Meeting13 Meeting July 7July 7--9, 20049, 2004 Presentations from-TBM Abdou (5 min.) Wong (20 min.) Sze (10 min.) Ying (15 min.) Kurtz (10 min.) #12;TBM's and Port Allocation

Abdou, Mohamed

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141

Data:F07da1bd-bc5a-4394-8ace-306f2c4e47dd | Open Energy Information  

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Data:F8ff6edc-1305-4ebb-9d20-4f531dd485d6 | Open Energy Information  

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Data:67a97277-3fcd-4328-8b35-cb2e14dd4964 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approvedea02758d3 No revision has1574de6f No revisionb70f702c53ceb35-cb2e14dd4964

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Data:6d95a822-320e-495a-b33a-afbb242dd536 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approvedea02758d3f49fa2694613-b89b-a700bd7943d5 No revision has beenafbb242dd536

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Data:7250c0fb-9c9e-43e9-ad6a-374255d20dd6 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision has been approved for this779a9a2a3278ad6a-374255d20dd6 No

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Data:73395af2-de6c-4ae2-9da5-3a8401dd879a | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision has beenb9c6b19f89f3 No revision hasda5-3a8401dd879a No revision

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Data:734e918e-80d0-45ed-a31b-dd794e3e5c4a | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision has beenb9c6b19f89f3 No revision hasda5-3a8401dd879add794e3e5c4a

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Data:77ae1593-d949-46be-94b3-089dd26da1ce | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision8390-f3c1d17c852d Nof0ac113123b15ccc3573012fcf8e No9dd26da1ce No

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Data:77b10539-46bd-442d-84e3-3dd53615e097 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision8390-f3c1d17c852d Nof0ac113123b15ccc3573012fcf8e No9dd26da1ce

150

Data:906c3e21-af90-40fc-919f-cab204dd88bb | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation,f31366697 Noa332baf71bac Noc2-4eb2d7ab908a No919f-cab204dd88bb

151

Data:Acb988dd-1e30-4e5b-90ac-6a4926210312 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation,f31366697Acb988dd-1e30-4e5b-90ac-6a4926210312 No revision has

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Data:Ad6565e0-c2cb-4dd1-88e6-aa87547cfbe1 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation,f31366697Acb988dd-1e30-4e5b-90ac-6a4926210312 No revision

153

Data:1f2841bf-ff8e-4487-89e0-608dd570394d | Open Energy Information  

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Data:2627a18c-ed1f-4899-818e-1e1858dd2f6f | Open Energy Information  

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Data:28b54f08-c941-4fd0-93d1-2a577e3dd598 | Open Energy Information  

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156

Data:B0f7ee6d-3f73-4104-9dc1-ec5083dd1c49 | Open Energy Information  

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Data:B24a8a69-b6a7-4ba0-a71b-cf889bd688dd | Open Energy Information  

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161

Data:56dd8b89-9ec3-4da7-b115-0f494067cb5b | Open Energy Information  

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Data:5751e555-0721-44ff-93dd-ea0b82b105de | Open Energy Information  

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Data:42f77724-394f-4af3-873a-ae25dd294a91 | Open Energy Information  

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Data:527ff887-485e-441d-b096-edce50dd6d83 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b Nobfef8fa58cf74865627f783 Noaad3-ec22188355fa No341c9c4152dd958 No

177

Data:5305deef-c23c-4c07-b36d-d2aa91b58cef | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b Nobfef8fa58cf74865627f783eabb28-cd1d-43dd-80d2-219739044111b17be4b No revision has

178

Data:0a710392-0262-4cde-a5ba-d1dd41e15527 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable-1a29da98863b No revision has beencde-a5ba-d1dd41e15527 No revision has been

179

Data:118d7d07-14f6-4962-b5dd-6741a324e875 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has been approved for720c8ec90dbaf6-4962-b5dd-6741a324e875 No revision has been

180

Data:15661511-101e-483c-b379-c9ee26f7dd9a | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 No revision78ced93e0 No52ca No5d8683238e931b74ee26f7dd9a No

Note: This page contains sample records for the topic "mm dd yy" 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

Data:17c9c9ef-1c18-4fd8-af1a-0c4b993dd5af | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 Nob97eb4d202d0d9aabb1ca46d No revisionc4b993dd5af No revision has

182

Data:17e9f8fb-dd13-43e1-88cd-3d94fd371b7c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 Nob97eb4d202d0d9aabb1ca46d No revisionc4b993dd5aff5c690625b6d

183

Data:A137d5f1-efe0-4518-b209-069dd1fd7c05 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05 No revision has been approved for this page. It is

184

Data:A28606df-43b5-40dd-8f64-6ab6b7ed51bc | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05 Nod0a-20a071f2b985 No revision

185

Data:A2cbda74-2dd8-4c49-923c-3e35bd842b10 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05 Nod0a-20a071f2b985 Noab0-1e2015cab1b0 No revision

186

Data:A442b48a-53fb-459d-8234-7a0d70af1dd6 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05a97219c78 Noa9b16c55c7a0 Noed1f5fc9 No revision has

187

Data:A626f719-5123-4939-86c1-470fe535dd99 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 Noddefe0-db39-48c0-ac98-7941b3451e3cf8e56363f No revision hasfe535dd99 No revision has

188

Data:A64044db-dd8c-4dbb-9ec5-98b3d4e872cf | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 Noddefe0-db39-48c0-ac98-7941b3451e3cf8e56363f No revision hasfe535dd99ec5-98b3d4e872cf

189

Data:Aa7f412f-07b5-4554-a50e-4c95f24dd14d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44f-4cd6-87d8-e9253aab8d9c No0a794995ed1-8279-0f89b49fba66 No revision hasc95f24dd14d No

190

Data:Fc3c902f-2e59-422b-ba1b-0db4740dd3e9 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved for thisd785796ade4709e636e4428acdb15335744 No230126bedfda No revisionb-0db4740dd3e9 No

191

Data:Fcf9b74e-611f-41b8-8dd8-2ca51ef75828 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved forcd976b98236 No revisionFcf9b74e-611f-41b8-8dd8-2ca51ef75828 No revision has been

192

Data:Fd6d8aa6-e915-454b-b401-5bbf391c0dd0 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved forcd976b98236 Noa566193f57 No revision has been approved foreac124aadbc No5bbf391c0dd0

193

Data:Fdd5e97c-2797-4524-bec8-62dd17acfac5 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved forcd976b98236 Noa566193f57Fdd2d0f5-4736-45f8-b32e-89158106d400 No revision2dd17acfac5

194

Data:Ffe2fb55-352f-473b-a2dd-50ae8b27f0a6 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has beenFfe2fb55-352f-473b-a2dd-50ae8b27f0a6 No revision has been approved for this page. It is currently

195

Data:9409b7c1-0714-4f02-aac6-d9cea0dd153b | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No revisionedead8-4241-4b53-933a-90a289b19506aac6-d9cea0dd153b No

196

Data:9637e7b9-de03-4c04-89dd-afcb2c2e8cfb | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No789501c8a3b5 Noc60f0b1242e7ca4dccba98d7 No revision-89dd-afcb2c2e8cfb

197

Data:96d3125f-4bbc-4d3f-8637-e4b2dd7a9399 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No789501c8a3b5d3f-8637-e4b2dd7a9399 No revision has been approved for

198

Data:9be3db16-e125-45ae-afef-ff8fb999dd27 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision has been approved for7a-a33e-3aa1431a0b90 No revision6-adb9-dd6567952019

199

Data:9c1eb185-cb94-4501-a6f5-0dd9ec16325f | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision has been approved for7a-a33e-3aa1431a0b90e07303b6b3e1-0dd9ec16325f No

200

Data:C5936b43-9507-4cef-b654-02d2a7a90dd1 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742 No revision has4dc5b1450a No revision873cfacc637 No revision hasd60de67e02d2a7a90dd1 No

Note: This page contains sample records for the topic "mm dd yy" 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

Data:Cc8427b3-92d4-4cac-ade1-5dd9fb0b039c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742e80b26cc4 No revision has been930896a No revision2-643305872f4e No revision5dd9fb0b039c

202

Data:Cebf9be9-865b-4dd4-8836-92d409cfdd0d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742e80b26cc4Cebf9be9-865b-4dd4-8836-92d409cfdd0d No revision has been approved for this

203

Data:D47c30f0-58e7-45d2-88c2-ac95dd308151 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has been approved97069579d6 No revision has993fca7f315dd308151 No revision has been approved for

204

Data:D48c3616-8527-403d-ac82-dd96cc373c32 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has been approved97069579d6 No revision has993fca7f315dd308151 No revision has been approved

205

Data:D495ab52-c999-44a4-af72-2fea73dd9e96 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has been approved97069579d6 No revision has993fca7f315dd308151 No revision has been

206

Data:D5c9d832-d960-4e80-89fd-be71456dd7da | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has been approved97069579d6 Nob2d2-b9d0456a138a No9855-451273353a58 No9fd-be71456dd7da No

207

Data:Dbb8ded7-5c5e-45fc-83c0-882caf7f9dd1 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision hasDafcf4ac-ca67-414f-9d31-84001343bbeb NoDbb8ded7-5c5e-45fc-83c0-882caf7f9dd1 No revision has

208

Data:Dd576956-48ce-4d67-8b2b-1294f1a3e40c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision has been

209

Data:Dd5a5cb0-c416-4d2c-8361-0fe1ba286aa7 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision has beenba286aa7 No

210

Data:Dd5d1fe0-1d39-4447-84fc-eda0914fb91d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision has beenba286aa7

211

Data:Dd603d1f-9704-4ff8-8a7b-582373fb194b | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision has

212

Data:Dd64eff6-8d85-423e-ae35-e8d1eb4296b7 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revision

213

Data:Dd6b2688-4a9c-4558-aadb-4d7abeba0790 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revisionabeba0790 No

214

Data:Dd739449-fc9d-425a-998f-cb67c9dfd12b | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No revisionabeba0790

215

Data:Dd791421-9638-4d46-9113-41f7c766b564 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5 No

216

Data:Dd79dec2-80d6-4d49-aa4f-6ef025d4b758 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5

217

Data:Dd7f0f03-1407-4d0a-bac6-bfb65e3d4028 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5bac6-bfb65e3d4028 No revision

218

Data:Dd8dda17-2b18-4e7e-a002-1ab52a69793d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5bac6-bfb65e3d4028

219

Data:Dd98c2ec-2371-4b18-a704-cc297cdd5bd2 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approvedf2dd7ce5bac6-bfb65e3d4028b28077373b20

220

Data:Df85b9b4-bde2-474a-a2e1-28b897dd813d | Open Energy Information  

Open Energy Info (EERE)

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Note: This page contains sample records for the topic "mm dd yy" 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

Data:78f18e44-a572-4e7d-adf2-f6929d8dd1bb | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b Nof667a9d7d88 No revision has929d8dd1bb No revision has been approved for

222

Data:78f4c0e7-dd49-4386-81e2-1c902c5eb5fd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b Nof667a9d7d88 No revision has929d8dd1bb No revision has been approved

223

Data:7905f3d8-b1ce-4f4d-ba10-7dd0110efd93 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b Nof667a9d7d88 No revision has929d8dd1bb No revision has been

224

Data:81c3c537-65ea-4e6f-8fbb-3dbff9dd3b8d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300ac No revisiondbff9dd3b8d No revision has been

225

Data:81ce1edd-eea7-4dea-9611-307366c2dd34 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300ac No revisiondbff9dd3b8d No

226

Data:831a3fae-8ea2-4bf8-965f-3f3dd886bf1c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has9-c45258b300ac Noc1e69d7992f-3f3dd886bf1c No revision has been

227

Data:8afd9aa1-538e-409b-b702-95fd1ae300dd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No18fed1db5 No revision has been7a5-b5d93ded2d08 No revision95fd1ae300dd No

228

Data:3dc474c2-3d38-4ba9-a267-faab96e42dd7 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has been approved64ec514 No revision has been approved for thisfaab96e42dd7

229

Data:3e9cc325-5999-4e83-808c-c5c3dd4086bc | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has been approved64ec514 Noc707c3a4d4cdc3dd4086bc No revision has been

230

THE MAGNETIC FIELD MORPHOLOGY OF THE CLASS 0 PROTOSTAR L1157-mm  

SciTech Connect (OSTI)

We present the first detection of polarization around the Class 0 low-mass protostar L1157-mm at two different wavelengths. We show polarimetric maps at large scales (10'' resolution at 350 {mu}m) from the SHARC-II Polarimeter and at smaller scales (1.''2-4.''5 at 1.3 mm) from the Combined Array for Research in Millimeter-wave Astronomy (CARMA). The observations are consistent with each other and show inferred magnetic field lines aligned with the outflow. The CARMA observations suggest a full hourglass magnetic field morphology centered about the core; this is only the second well-defined hourglass detected around a low-mass protostar to date. We apply two different methods to CARMA polarimetric observations to estimate the plane-of-sky magnetic field magnitude, finding values of 1.4 and 3.4 mG.

Stephens, Ian W.; Looney, Leslie W.; Kwon, Woojin; Crutcher, Richard M. [Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801 (United States); Hull, Charles L. H.; Plambeck, Richard L. [Astronomy Department and Radio Astronomy Laboratory, 601 Campbell Hall, University of California, Berkeley, CA 94720 (United States); Chapman, Nicholas; Novak, Giles; Matthews, Tristan [Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 (United States); Davidson, Jacqueline [School of Physics, University of Western Australia, 35 Stirling Hwy, Crawley, WA 6009 (Australia); Vaillancourt, John E. [SOFIA Science Center, Universities Space Research Association, NASA Ames Research Center, MS 232-11, Moffett Field, CA 94035-0001 (United States); Shinnaga, Hiroko, E-mail: stephen6@illinois.edu [Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, HI 96720 (United States)

2013-05-20T23:59:59.000Z

231

A Magnetic Dynamo Origin For The Sub-mm Excess In Sgr A*  

E-Print Network [OSTI]

The sub-mm bump observed in the spectrum of Sgr A* appears to indicate the existence of a compact emitting component within several Schwarzschild radii, $r_S$, of the nucleus at the Galactic Center. This is interesting in view of the predicted circularized flow within $\\sim 5-10 r_S$, based on detailed multi-dimensional hydrodynamic simulations of Bondi-Hoyle accretion onto this unusual object. In this paper, we examine the physics of magnetic field generation by a Keplerian dynamo subject to the conditions pertaining to Sgr A*, and show that the sub-mm bump can be produced by thermal synchrotron emission in this inner region. This spectral feature may therefore be taken as indirect evidence for the existence of this circularization. In addition, the self-Comptonization of the sub-mm bump appears to produce an X-ray flux exceeding that due to bremsstrahlung from this region, which may account for the X-ray counterpart to Sgr A* discovered recently by {\\it Chandra}. However, the required accretion rate in the Keplerian flow is orders of magnitude smaller than that predicted by the Bondi-Hoyle simulations. We speculate that rapid evaporation, in the form of a wind, may ensue from the heating associated with turbulent mixing of gas elements with large eccentricity as they settle down into a more or less circular (i.e., low eccentricity) trajectory. The spectrum of Sgr A* longward of $\\sim 1-2$ mm may be generated outside of the Keplerian flow, where the gas is making a transition from a quasi-spherical infall into a circularized pattern.

Fulvio Melia; Siming Liu; Robert Coker

2001-05-27T23:59:59.000Z

232

A 15 15 mm, 1 A, Reliable Sensor-Net Module: Enabling Application-Specific Nodes  

E-Print Network [OSTI]

-simokw, tanaka-t, kuriyama, kshimada, k_yano}@crl.hitachi.co.jp 1. INTRODUCTION ZN1 is an ultra-small, low-power sensor-net module. ZN1 integrates MCU, RF, and RTC into an ultra-small 15 ? 15-mm module with an ultra-low standby current less than 1 µA. Its ultra- small feature enables application-specific sensor nodes

Savvides, Andreas

233

Correlated Sub-mm and X-ray Variability in Sgr A*  

E-Print Network [OSTI]

PAPER WITHDRAWN. The recent detection of Sgr A* in the X-ray band, together with the radio polarization measurements conducted over the past few years, offer the best constraints yet for understanding the nature of the emitting gas within several Schwarzschild radii ($r_S$) of this supermassive black hole candidate at the Galactic Center. Earlier, we showed that the sub-mm radiation from this source may be associated with thermal synchrotron emission from an inner Keplerian region within the circularization radius of the accreting plasma. In this paper, we extend this analysis in a very important way, by calculating the implied high-energy emission of Sgr A* associated with the orbiting, hot, magnetized gas. We find that for the accretion rate inferred from the fits to the sub-mm data, the dominant contribution to Sgr A*'s X-ray flux is due to self-Comptonization of the radio photons, rather than from bremsstrahlung. The latter is a two-body process, which would produce significant X-ray emission only at much higher accretion rates. This picture leads to the testable prediction that the physical conditions within the inner $\\sim5r_S$ are variable on a time scale of order a year. In particular, the accretion rate $\\dot M$ appears to have changed by about 15% between the sub-mm measurements in 1996 and 1999. Given that the radio and self-Comptonized fluxes are strongly correlated in this picture, the upcoming second generation Chandra observations of Sgr A* may provide the direct evidence required to test this model.

Fulvio Melia; Siming Liu; Marco Fatuzzo

2002-05-28T23:59:59.000Z

234

L1448-MM OBSERVATIONS BY THE HERSCHEL KEY PROGRAM, ''DUST, ICE, AND GAS IN TIME'' (DIGIT)  

SciTech Connect (OSTI)

We present Herschel/Photodetector Array Camera and Spectrometer (PACS) observations of L1448-MM, a Class 0 protostar with a prominent outflow. Numerous emission lines are detected at 55 1000 K) environment, indicative of a shock origin. For OH, IR-pumping processes play an important role in the level population. The molecular emission in L1448-MM is better explained with a C-shock model, but the atomic emission of PACS [O I] and Spitzer/Infrared Spectrograph [Si II] emission is not consistent with C-shocks, suggesting multiple shocks in this region. Water is the major line coolant of L1448-MM in the PACS wavelength range, and the best-fit LVG models predict that H{sub 2}O and CO emit (50%-80%) of their line luminosity in the PACS wavelength range.

Lee, Jinhee; Lee, Jeong-Eun [Department of Astronomy and Space Science, Kyung Hee University, Yongin-shi, Kyungki-do 449-701 (Korea, Republic of); Lee, Seokho [Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul 151-742 (Korea, Republic of); Green, Joel D.; Evans, Neal J. II [Department of Astronomy, University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712-1205 (United States); Choi, Minho [Korea Astronomy and Space Science Institute, 776 Daedeokdaero, Yuseong, Daejeon 305-348 (Korea, Republic of); Kristensen, Lars [Harvard-Smithsonian Center for Astrophysics, MS78, Cambridge, MA 02138 (United States); Dionatos, Odysseas; Jrgensen, Jes K., E-mail: jeongeun.lee@khu.ac.kr [Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, ster Voldgade 5-7, 1350 Copenhagen (Denmark); Collaboration: DIGIT Team

2013-11-01T23:59:59.000Z

235

Fe/Al2O3 C2H4 Hata mm/10 min  

E-Print Network [OSTI]

Fe/Al2O3 C2H4 () () () () () () () * () 1. (SWNT) SWNT (CVD) (CNT)[1] Hata mm/10 min SWNT (Super Growth)[2]Al2O3 Fe C2H4 SWNT Fe/Al2O3 C2H4 CVD SWNT CNT CNT 2 SiO2 Al2O3 20 (RBM) 1350 cm-1 (D-Band)Fe G/D RBM Fe SWNT Al 15 nm Fe 0.6 nm CVD TEM Fig. 3 3 nm SWNT

Maruyama, Shigeo

236

Sub-mm tests of the gravitational inverse-square law  

E-Print Network [OSTI]

Sub-mm tests of the gravitational inverse-square law are interesting from several quite different perspectives. This paper discusses work by the Eot-Wash group performed since the publication of our initial result in February 2001. We find no evidence for short-range Yukawa interactions. Our results provide an upper limit of 200 micrometers on the size of the largest ``extra'' dimension, and for the unification scenario with 2 large extra dimensions, set an upper limit of 150 micrometers on the size of those dimensions.

E. G. Adelberger

2002-02-02T23:59:59.000Z

237

A QM/MM Study on the Aqueous Solvation of theTetrahydroxouranylate [UO(OH)]  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary)morphinanInformation Desert SouthwestTechnologies |November 2011A First LookMicroscopyComplex Ion. | EMSL QM/MM

238

Investigation of temperature dependence of neutron yield and electron screening potential for the d(d, n){sup 3}He reaction proceeding in deuterides ZrD{sub 2} and TiD{sub 2}  

SciTech Connect (OSTI)

The temperature dependence of the enhancement factor for the dd reaction proceeding in TiD{sub 2} and ZrD{sub 2} is investigated. The experiments were carried out at the Hall pulsed ion accelerator (INP, Polytechnic University, Tomsk, Russia) in the deuteron energy interval 7.0-12.0 keV and at temperatures ranging from 20 to 200 Degree-Sign C. The values obtained for the electron screening potentials indicate that the dd reaction enhancement factor does not depend on the target temperature in the range 20-200 Degree-Sign C. This result contradicts the conclusions drawn by the LUNA Collaboration from their work.

Bystritsky, V. M., E-mail: bystvm@jinr.ru [Joint Institute for Nuclear Research (Russian Federation); Bystritskii, Vit. M. [University of California, Department of Physics and Astronomy (United States); Dudkin, G. N. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Filipowicz, M. [AGH, University of Science and Technology, Faculty of Energy and Fuels (Poland); Gazi, S.; Huran, J. [Institute of Electrical Engineering SAS (Slovakia); Kobzev, A. P. [Joint Institute for Nuclear Research (Russian Federation); Mesyats, G. A. [Lebedev Physical Institute of the Russian Academy of Sciences (Russian Federation); Nechaev, B. A.; Padalko, V. N. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Parzhitskii, S. S. [Joint Institute for Nuclear Research (Russian Federation); Pen'kov, F. M. [Institute of Nuclear Physics NNC (Kazakhstan); Philippov, A. V. [Joint Institute for Nuclear Research (Russian Federation); Kaminskii, V. L. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Tuleushev, Yu. Zh. [Institute of Nuclear Physics NNC (Kazakhstan); Wozniak, J. [AGH, University of Science and Technology, Faculty of Physics and Applied Computer Sciences (Poland)

2012-08-15T23:59:59.000Z

239

Self-consistent QM/MM methodologies for structural refinement of photosystem II and other macromolecules of biological interest  

SciTech Connect (OSTI)

The combination of quantum mechanics and molecular mechanics (QM/MM) is one of the most promising approaches to study the structure, function, and properties of proteins and nucleic acids. However, there some instances in which the limitations of either the MM (lack of a proper electronic description) or QM (limited to a few number of atoms) methods prevent a proper description of the system. To address this issue, we review here our approach to fine-tune the structure of biological systems using post-QM/MM refinements. These protocols are based on spectroscopy data, and/or partitioning of the system to extend the QM description to a larger region of a protein. We illustrate these methodologies through applications to several biomolecules, which were pre-optimized at the QM/MM level and then further refined using postQM/MM refinement methodologies: mod(QM/MM), which refines the atomic charges of the residues included in the MM region accounting for polarization effects; mod(QM/MM)-opt that partition the MM region in smaller parts and optimizes each part in an iterative. self-consistent way, and the Polarized-Extended X-Ray Absorption Fine Structure (P-EXAFS) fitting procedure, which fine-tune the atomic coordinates to reproduce experimental polarized EXAFS spectra. The first two techniques were applied to the guanine quadruplex. while the P-EXAFS refinement was applied to the oxygen evolving complex of photosystem II.

Batista, Enrique R [Los Alamos National Laboratory; Sproviero, Eduardo M [YALE UNIV; Newcomer, Michael [YALE UNIV; Gascon, Jose A [YALE UNIV; Batista, Victor S [YALE UNIV

2008-01-01T23:59:59.000Z

240

Design development for the 50mm Superconducting Super Collider dipole cryostat  

SciTech Connect (OSTI)

The cryostat of a Superconducting Super Collider (SSC) dipole magnet consists of all magnet components except the magnet assembly itself. It serves to support the magnet accurately and reliably within the vacuum vessel, provide all required cryogenic piping, and to insulate the cold mass from heat radiated and conducted from the environment. It must function reliably during storage, shipping and handling, normal magnet operation, quenches, and seismic excitations, and must be manufacturable at low cost. The major components of the cryostat are the vacuum vessel, thermal shields, multilayer insulation system, cryogenic piping, interconnections, and suspension system. The overall design of a cryostat for superconducting accelerator magnets requires consideration of fluid flow, proper selection of materials for their thermal and structural performance at both ambient and operating temperature, and knowledge of the environment to which the magnets will be subjected over the course their expected operating life. This paper describes the design of the current 50mm SSC collider dipole cryostat and includes discussions on the structural and thermal considerations involved in the development of each of the major systems. Where appropriate, comparisons will be made with the 40mm cryostat. 7 refs., 5 figs., 4 tabs.

Nicol, T.H.

1991-03-01T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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

A 16 mm3 autonomous solar-powered sensor node with bi-directional optical communication for distributed sensor net-  

E-Print Network [OSTI]

Abstract A 16 mm3 autonomous solar-powered sensor node with bi- directional optical communication for distributed sensor net- works has been demonstrated. The device digitizes inte- grated sensor signals, a 2.6 mm2 SOI solar cell array, and a micromachined four-quadrant corner-cube retroreflector (CCR

Kahn, Joseph M.

242

The CR 2.0mm (.079") insulation displacement connector features a mounting height as low as  

E-Print Network [OSTI]

7 The CR 2.0mm (.079") insulation displacement connector features a mounting height as low as 6.9mm") pitch insulation displacement connector allows automatic harness production for connection of UL1007 of misinsertion without being permanently distorted. Twin U-slot insulation displacement section The insulation

Wedeward, Kevin

243

Spray drift collector efficiency: Assessment of deposition on 2 mm diameter PVC line in a wind tunnel  

E-Print Network [OSTI]

Spray drift collector efficiency: Assessment of deposition on 2 mm diameter PVC line in a wind and Miller and Hadfield, 1989) and to trap it on passive collectors. This method is cheap and easy to set-up but the efficiency of the collectors has to be evaluated. The cylindrical collectors with a diameter of 2 mm

Paris-Sud XI, Universit de

244

Data:Eab18dd4-f972-4058-93a1-20f8cbef15b3 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1cc No revision hasa3e396ee3eb No revision hasa749-1d1f78c6b844 NoEab18dd4-f972-4058-93a1-20f8cbef15b3

245

Data:54b5fc48-9fe6-4638-8079-56aa3e128dd4 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b3da-78f7ef0b79f6 No revision has2fea1047f348 No revision has beenb9c0fd2f8fb Noaa3e128dd4

246

Data:Cdd1388f-c999-4f06-83dd-1c353bb566ad | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742e80b26cc4 No revision5d06fb2b0ba No revisionCdd1388f-c999-4f06-83dd-1c353bb566ad No

247

Evolution of complex organic molecules in hot molecular cores: Synthetic spectra at (sub-)mm wavebands  

E-Print Network [OSTI]

Hot molecular cores (HMCs) are intermediate stages of high-mass star formation and are also known for their rich emission line spectra at (sub-)mm wavebands. The observed spectral feature of HMCs such as total number of emission lines and associated line intensities are also found to vary with evolutionary stages. We developed various 3D models for HMCs guided by the evolutionary scenarios proposed by recent empirical and modeling studies. We then investigated the spatio-temporal variation of temperature and molecular abundances in HMCs by consistently coupling gas-grain chemical evolution with radiative transfer calculations. We explored the effects of varying physical conditions on molecular abundances including density distribution and luminosity evolution of the central protostar(s). The time-dependent temperature structure of the hot core models provides a realistic framework for investigating the spatial variation of ice mantle evaporation as a function of evolutionary timescales. With increasing protos...

Choudhury, Rumpa; Stphan, Gwendoline; Bergin, Edwin A; Mller, Thomas; Schmiedeke, Anika; Zernickel, Alexander

2015-01-01T23:59:59.000Z

248

DESIGN AND CONSTRUCTION OF A 15 T, 120 MM BORE IR QUADRUPOLE MAGNET FOR LARP  

SciTech Connect (OSTI)

Pushing accelerator magnets beyond 10 T holds a promise of future upgrades to machines like the Large Hadron Collider (LHC) at CERN. Nb{sub 3}Sn conductor is at the present time the only practical superconductor capable of generating fields beyond 10 T. In support of the LHC Phase-II upgrade, the US LHC Accelerator Research Program (LARP) is developing a large bore (120 mm) IR quadrupole (HQ) capable of reaching 15 T at its conductor peak field and a peak gradient of 219 T/m at 1.9 K. While exploring the magnet performance limits in terms of gradient, forces and stresses the 1 m long two-layer coil will demonstrate additional features such as alignment and accelerator field quality. In this paper we summarize the design and report on the magnet construction progress.

Caspi, S.; Cheng, D.; Dietderich, D.; Felice, H.; Ferracin, P.; Hafalia, R.; Hannaford, R.; Sabbi, G. S.; Anerella, M.; Ghosh, A.; Schmalzle, J.; Wanderer, P.; Ambrosio, G.; Bossert, R.; Kashikhin, V.; Pasholk, D.; Zlobin, A.

2009-05-04T23:59:59.000Z

249

Fluorescence of PRODAN in Water: a Computational QM/MM MD Study  

SciTech Connect (OSTI)

Fluorescent properties of PRODAN (6-propionyl-2-dimethylaminonaphthalene) in water were studied by means of excited state molecular dynamics simulations employing a combined quantum mechanical and molecular mechanical approach with the time-dependent density functional theory (TD-DFT QM/MM MD). The state of the art coupled cluster method was used to benchmark density functional theory calculations. The influence of the water environment on PRODAN emission was investigated by employing several computational schemes with varying description of the solvent. The issue of the molecular geometry of the excited state PRODAN molecule in water was addressed. The experimental emission spectrum was reproduced for the planar excited state conformer of PRODAN in the extended environment of 300 explicit water molecules. The planar conformer was shown to be predominantly responsible for fluorescence. The twisted isomer is strongly stabilized in water, but rapidly evolve towards a conical intersection, and hence the twisted conformer is fluorescently inactive.

Pederzoli, Marek; Sobek, Lukas; Brabec, Jiri; Kowalski, Karol; Cwiklik, Lukasz; Pittner, Jiri

2014-03-28T23:59:59.000Z

250

Operating the LCLS Gas Attenuator and Gas Detector System with Apertures of 6mm Diameter  

SciTech Connect (OSTI)

The possibility of increasing the apertures of the LCLS gas attenuator/gas detector system is considered. It is shown that increase of the apertures from 3 to 6 mm, together with 4-fold reduction of the operation pressure does not adversely affect the vacuum conditions upstream or downstream. No change of the pump speed and the lengths of the differential pumping cells is required. One minor modification is the use of 1.5 cm long tubular apertures in the end cells of the differential pumping system. Reduction of the pressure does not affect performance of the gas attenuator/gas detector system at the FEL energies below, roughly, 2 keV. Some minor performance degradation occurs at higher energies.

Ryutov, D.D.; Bionta, R.M.; Hau-Riege, S.P.; Kishiyama, K.I.; Roeben, M.D.; Shen, S.; /LLNL, Livermore; Stefan, P.M.; /SLAC; ,

2010-11-17T23:59:59.000Z

251

Structure for an LHC 90mm Nb3Sn Quadrupole Magnet  

SciTech Connect (OSTI)

A full-scale mechanical model of the LHC Nb{sub 3}Sn quadrupole magnet structure has been designed, built and tested. The structure will support a 90mm bore, 1m long magnet prototype as part of the US LHC Accelerator Research Program (LARP). The structure utilizes Bladder and Key Technology to control and transfer pre-stress from an outer aluminum shell to an inner coil. Axial aluminum rods take care of pre-stress at the ends--ensuring that the coil is fully constrained along all three axes. The outer aluminum shell and an inner ''dummy coil'' (aluminum tube) were extensively instrumented with strain gauges. The gauges were used to monitor and map the effectiveness of the stress relation between the loading structure and a ''dummy'' coil through varying mechanical load conditions --from bladder and key pre-stress at room temperature through cool-down. Test results of the stress distribution in the structure and the in dummy coil is reported and compared with expected results calculated with the structural analysis program ANSYS.

Hafalia, A.R.; Caspi, S.; Bartlett, S.E.; Dietderich, D.R.; Ferracin, P.; Gourlay, S.A.; Hannaford, C.R.; Higley, H.; Lietzke, A.F.; Lau, B.; Liggins, N.; Mattafirri, S.; McInturff, A.D.; Nyman, M.; Sabbi,G.L.; Scanlan, R.M.; Swanson, J.

2005-04-16T23:59:59.000Z

252

The (anti)correlation of the sub-mm and X-ray background sources  

E-Print Network [OSTI]

The connection between the sub-mm and the hard X-ray backgrounds is studied by comparing data at 2-10 keV and at 850um for a sample of 34 sources at fluxes (or limiting fluxes) which resolve most of the background in the two bands. These data were obtained with new SCUBA observations and by correlating data sets available from the literature. None of the 11 hard X-ray (2-10 keV) sources has a counterpart at 850um, with the exception of a faint Chandra source, which is a candidate type 2 QSO at high redshift. These data indicate that 2-10 keV sources brighter than 10^-15 erg s-1 cm-2, which make at least 75% of the background in this band, contribute for less than 7% to the submillimetric background. Out of the 24 SCUBA sources 23 are undetected by Chandra. These data indicate that most of these SCUBA sources must be powered either by starburst activity, or by an AGN which is obscured by a column Nh > 10^25 cm-2, with a reflection efficiency in the hard X-rays significantly lower than 1% in most cases.

P. Severgnini

2000-05-22T23:59:59.000Z

253

Discrimination Report: A Multisensor system for detection andcharacterization of UXO, ESTCP Project MM-0437,  

SciTech Connect (OSTI)

The Berkeley UXO Discriminator (BUD) is an optimally designed active electromagnetic system that not only detects but also characterizes UXO. The performance of the system is governed by a target size-depth curve. BUD was designed to detect UXO in the 20 mm to 155 mm size range for depths between 0 and 1.5 m, and to characterize them in a depth range from 0 to 1.1 m. The system incorporates three orthogonal transmitters and eight pairs of differenced receivers. Eight receiver coils are placed horizontally along the two diagonals of the upper and lower planes of the two horizontal transmitter loops. These receiver coil pairs are located on symmetry lines through the center of the system and each pair sees identical fields during the on-time of the pulse in all of the transmitter coils. They are wired in opposition to produce zero output during the on-time of the pulses in three orthogonal transmitters. Moreover, this configuration dramatically reduces noise in the measurements by canceling the background electromagnetic fields (these fields are uniform over the scale of the receiver array and are consequently nulled by the differencing operation), and by canceling the noise contributed by the tilt motion of the receivers in the Earth's magnetic field, and greatly enhances receiver sensitivity to the gradients of the target response. BUD is mounted on a small cart to assure system mobility. System positioning is provided by a Real Time Kinematic (RTK) GPS receiver. The system has two modes of operation: (1) the search mode, in which BUD moves along a profile and exclusively detects targets in its vicinity providing target depth and horizontal location, and (2) the discrimination mode, in which BUD is stationary above a target, and determines three discriminating polarizability responses together with the object location and orientation from a single position of the system. The detection performance of the system is governed by a size-depth curve shown in Figure 2. This curve was calculated for BUD assuming that the receiver plane is 0.2 m above the ground. Figure 2 shows that, for example, BUD can detect an object with 0.1 m diameter down to the depth of 0.9 m with a depth uncertainty of 10%. Any objects buried at a depth of more than 1.3 m will have a low probability of detection. The discrimination performance of the system is governed by a size-depth curve shown in Figure 3. Again, this curve was calculated for BUD assuming that the receiver plane is 0.2 m above the ground. Figure 3 shows that, for example, BUD can determine the polarizability of an object with 0.1 m diameter down to the depth of 0.63 m with polarizability uncertainty of 10%. Any objects buried at the depth more than 0.9 m will have a low discrimination probability. Object orientation estimates and equivalent dipole polarizability estimates used for large and shallow UXO/scrap discrimination are more problematic as they are affected by higher order (non-dipole) terms induced in objects due to source field gradients along the length of the objects. For example, a vertical 0.4 m object directly below the system needs to be about 0.90 m deep for perturbations due to gradients along the length of the object to be of the order of 20% of the uniform field object response. Similarly, vertical objects 0.5 m, and 0.6 m long need to be 1.15 m, and 1.42 m, respectively, below the system. For horizontal objects the effect of gradients across the object diameter are much smaller. For example, 155 mm and 105 mm projectiles need to be only 0.30 m, and 0.19 m, respectively, below the system. A polarizability index (in cm{sup 3}), which is an average value of the product of time (in seconds) and polarizability rate (in m{sup 3}/s) over the 34 sample times logarithmically spaced from 143 to 1300 {micro}s, and three polarizabilities, can be calculated for any object. We used this polarizability index to decide when the object is in a uniform source field. Objects with the polarizability index smaller than 600 cm{sup 3} and deeper than 1.8 m below BUD, or smaller than 200

Gasperikova, Erika; Smith, J. Torquil; Morrison, H.Frank; Becker,Alex

2008-01-14T23:59:59.000Z

254

The orifice expansion correction for a 50 mm line size at various diameter ratios  

SciTech Connect (OSTI)

The expansion coefficient or factor for a compressible flowmeter corrects for the change in pressure and density as the fluid is accelerated through the flowmeter. The expansion correction currently in use in the United States and also in other countries was developed over fifty years ago by Buckingham and Bean. More recent work reported by Kinghorn shows the equation currently in use to be in error. This paper describes the results of a test program to determine the expansion factors for flange-tapped sharp-edged orifices with diameter ratios between 0.242 and 0.726 in a nominal 50 mm (2 inch) line. Critical flow Venturis are used as the reference standards and dry air as the flowing fluid. The ratio of differential pressure to inlet static pressure is varied over a range of zero to about 0.2 at a constant Reynolds number. The expansion factor is determined form the apparent change in discharge coefficient at a constant Reynolds number.

Seidl, W. [Colorado Engineering Experiment Station, Inc., Nunn, CO (United States)

1995-12-31T23:59:59.000Z

255

Comparison of QM-Only and QM/MM Models for the Mechanism of Tungsten-Dependent Acetylene Hydratase  

E-Print Network [OSTI]

Comparison of QM-Only and QM/MM Models for the Mechanism of Tungsten-Dependent Acetylene Hydratase study on the formation of vinyl alcohol in the catalytic cycle of tungsten-dependent acetylene hydratase

Liao, Rongzhen

256

Fabrication and characterization of a 0.5-mm lutetium oxyorthosilicate detector array for high-resolution PET applications  

E-Print Network [OSTI]

for a high resolution PET detector using position sensitive51:21312142. 0.5- MM LSO A RRAY FOR PET Stickel et al.Instrumentation aspects of animal PET. Annu Rev Biomed Eng.

Stickel, Jennifer R; Qi, Jinyi; Cherry, Simon R

2007-01-01T23:59:59.000Z

257

Detection of significant cm to sub-mm band radio and gamma-ray correlated variability in Fermi bright blazars  

E-Print Network [OSTI]

The exact location of the gamma-ray emitting region in blazars is still controversial. In order to attack this problem we present first results of a cross-correlation analysis between radio (11 cm to 0.8 mm wavelength, F-GAMMA program) and gamma-ray (0.1-300 GeV) ~ 3.5 year light curves of 54 Fermi-bright blazars. We perform a source stacking analysis and estimate significances and chance correlations using mixed source correlations. Our results reveal: (i) the first highly significant multi-band radio and gamma-ray correlations (radio lagging gamma rays) when averaging over the whole sample, (ii) average time delays (source frame: 76+/-23 to 7+/-9 days), systematically decreasing from cm to mm/sub-mm bands with a frequency dependence tau_r,gamma (nu) ~ nu^-1, in good agreement with jet opacity dominated by synchrotron self-absorption, (iii) a bulk gamma-ray production region typically located within/upstream of the 3 mm core region (tau_3mm,gamma=12+/-8 days), (iv) mean distances between the region of gamma-...

Fuhrmann, L; Chiang, J; Angelakis, E; Zensus, J A; Nestoras, I; Krichbaum, T P; Ungerechts, H; Sievers, A; Pavlidou, V; Readhead, A C S; Max-Moerbeck, W; Pearson, T J

2014-01-01T23:59:59.000Z

258

System Description for the K-25/K-27 D&D Project Polyurethane Foam Delivery System, East Tennessee Technology Park, Oak Ridge, Tennessee  

SciTech Connect (OSTI)

The Foam Delivery System used in the decontamination and decommissioning (D&D) project for the K-25/K-27 Buildings at the East Tennessee Technology Park (ETTP) is comprised of a trailer-mounted Gusmer{reg_sign} H20/35 Pro-TEC Proportioning Unit and the associated equipment to convey electrical power, air, and foam component material to the unit. This high-pressure, plural-component polyurethane foam pouring system will be used to fill process gas and non-process equipment/piping (PGE/P) within the K-25/K-27 Buildings with polyurethane foam to immobilize contaminants prior to removal. The system creates foam by mixing isocyanate and polyol resin (Resin) component materials. Currently, the project plans to utilize up to six foaming units simultaneously during peak foaming activities. Also included in this system description are the foam component material storage containers that will be used for storage of the component material drums in a staging area outside of the K-25/K-27 Buildings. The Foam Delivery System and foam component material storage enclosures (i.e., Foaming Component Protective Enclosures) used to store polymeric methylene diphenyl diisocyanate (PMDI) component material are identified as Safety Significant (SS) Structures, Systems and Components (SSC) in the Documented Safety Analysis (DSA) for the project, Documented Safety Analysis for the K-25 and K-27 Facilities at the East Tennessee Technology Park, Oak Ridge, Tennessee, DSA-ET-K-25/K-27-0001.

Boris, G.

2008-02-21T23:59:59.000Z

259

The south central Texas heavy rain event of October 1998: an MM5 simulation and diagnosis of convective initiation  

E-Print Network [OSTI]

During the weekend of 17-18 October 1998, extremely heavy rainfall over south central Texas resulted in widespread flash flooding and numerous river floods. Southern Hays County received 760 mm of rainfall, and an area of 18,000 km recorded over...

Scott, Richard Kevin

2001-01-01T23:59:59.000Z

260

FINE-SCALE STRUCTURE OF THE QUASAR 3C 279 MEASURED WITH 1.3 mm VERY LONG BASELINE INTERFEROMETRY  

SciTech Connect (OSTI)

We report results from five day very long baseline interferometry observations of the well-known quasar 3C 279 at 1.3 mm (230 GHz) in 2011. The measured nonzero closure phases on triangles including stations in Arizona, California, and Hawaii indicate that the source structure is spatially resolved. We find an unusual inner jet direction at scales of {approx}1 pc extending along the northwest-southeast direction (P.A. = 127 Degree-Sign {+-} 3 Degree-Sign ), as opposed to other (previously) reported measurements on scales of a few parsecs showing inner jet direction extending to the southwest. The 1.3 mm structure corresponds closely with that observed in the central region of quasi-simultaneous super-resolution Very Long Baseline Array images at 7 mm. The closure phase changed significantly on the last day when compared with the rest of observations, indicating that the inner jet structure may be variable on daily timescales. The observed new direction of the inner jet shows inconsistency with the prediction of a class of jet precession models. Our observations indicate a brightness temperature of {approx}8 Multiplication-Sign 10{sup 10} K in the 1.3 mm core, much lower than that at centimeter wavelengths. Observations with better uv coverage and sensitivity in the coming years will allow the discrimination between different structure models and will provide direct images of the inner regions of the jet with 20-30 {mu}as (5-7 light months) resolution.

Lu Rusen; Fish, Vincent L.; Doeleman, Sheperd S.; Crew, Geoffrey; Cappallo, Roger J. [Massachusetts Institute of Technology, Haystack Observatory, Route 40, Westford, MA 01886 (United States); Akiyama, Kazunori; Honma, Mareki [National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 181-8588 (Japan); Algaba, Juan C.; Ho, Paul T. P.; Inoue, Makoto [Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan, R.O.C. (China); Bower, Geoffrey C.; Dexter, Matt [Department of Astronomy, Radio Astronomy Laboratory, University of California Berkeley, 601 Campbell, Berkeley, CA 94720-3411 (United States); Brinkerink, Christiaan [Department of Astrophysics, IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500-GL Nijmegen (Netherlands); Chamberlin, Richard [Caltech Submillimeter Observatory, 111 Nowelo Street, Hilo, HI 96720 (United States); Freund, Robert [Arizona Radio Observatory, Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065 (United States); Friberg, Per [James Clerk Maxwell Telescope, Joint Astronomy Centre, 660 North A'ohoku Place, University Park, Hilo, HI 96720 (United States); Gurwell, Mark A. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Jorstad, Svetlana G. [Institute for Astrophysical Research, Boston University, Boston, MA 02215 (United States); Krichbaum, Thomas P. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); Loinard, Laurent, E-mail: rslu@haystack.mit.edu [Centro de Radiostronomia y Astrofisica, Universidad Nacional Autonoma de Mexico, 58089 Morelia, Michoacan (Mexico); and others

2013-07-20T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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.


261

A Note on the M/M/ Queue in Random Environment and Uri Yechiali 1,2  

E-Print Network [OSTI]

environment, the joint prob- ability distribution function (pdf) of the two variables: random phase and number random environment and show that the joint probability distribution function (pdf) of the environment. 2 The model and balance equations Consider an M/M/ type queue operating in 'random environment

Yechiali, Uri

262

NIST Mobility and Manipulation Project Needs and Plans The NIST Mobility and Manipulation (MM) Project is seeking government, industry  

E-Print Network [OSTI]

. The project testbed includes an industrial robot mounted on a linear rail. The MM Project also plans characterizing components of the new NIST robot testbed, which includes a six-axis industrial robot arm under that are of concern to industry. Real world applications are also highly beneficial for developing and evaluating

Perkins, Richard A.

263

A mineralogy of extrasolar silicate dust from 10-mm spectra J. E. Bowey1,2P  

E-Print Network [OSTI]

A mineralogy of extrasolar silicate dust from 10-mm spectra J. E. Bowey1,2P and A. J. Adamson1,3 1 in amorphous silicates, since the spectra of crystalline silicates are narrow and highly structured. The standard approach to the interpretation of astronomical spectra is to assume that the silicates

Bowey, Janet

264

Progresses in Ab Initio QM/MM Free Energy Simulations of Electrostatic Energies in Proteins: Accelerated QM/MM Studies of pKa, Redox Reactions and Solvation Free Energies  

SciTech Connect (OSTI)

Hybrid quantum mechanical / molecular mechanical (QM/MM) approaches have been used to provide a general scheme for chemical reactions in proteins. However, such approaches still present a major challenge to computational chemists, not only because of the need for very large computer time in order to evaluate the QM energy but also because of the need for propercomputational sampling. This review focuses on the sampling issue in QM/MM evaluations of electrostatic energies in proteins. We chose this example since electrostatic energies play a major role in controlling the function of proteins and are key to the structure-function correlation of biological molecules. Thus, the correct treatment of electrostatics is essential for the accurate simulation of biological systems. Although we will be presenting here different types of QM/MM calculations of electrostatic energies (and related properties), our focus will be on pKa calculations. This reflects the fact that pKa of ionizable groups in proteins provide one of the most direct benchmarks for the accuracy of electrostatic models of macromolecules. While pKa calculations by semimacroscopic models have given reasonable results in many cases, existing attempts to perform pKa calculations using QM/MM-FEP have led to large discrepancies between calculated and experimental values. In this work, we accelerate our QM/MM calculations using an updated mean charge distribution and a classical reference potential. We examine both a surface residue (Asp3) of the bovine pancreatic trypsin inhibitor, as well as a residue buried in a hydrophobic pocket (Lys102) of the T4-lysozyme mutant. We demonstrate that by using this approach, we are able to reproduce the relevant sidechain pKas with an accuracy of 3 kcal/mol. This is well within the 7 kcal/mol energy difference observed in studies of enzymatic catalysis, and is thus sufficient accuracy to determine the main contributions to the catalytic energies of enzymes. We also provide an overall perspective of the potential of QM/MM calculations in general evaluations of electrostatic free energies, pointing out that our approach should provide a very powerful and accurate tool to predict the electrostatics of not only solution but also enzymatic reactions, as well as the solvation free energies of even larger systems, such as nucleic acid bases incorporated into DNA.

Kamerlin, Shina C. L.; Haranczyk, Maciej; Warshel, Arieh

2009-03-01T23:59:59.000Z

265

Accelerator Quality HTS Dipole Magnet Demonstrator Designs for the EuCARD-2, 5 Tesla 40 mm Clear Aperture Magnet  

E-Print Network [OSTI]

Future high-energy accelerators will need very high magnetic fields in the range of 20 T. The EuCARD-2 work-package-10 is a collaborative push to take HTS materials into an accelerator quality demonstrator magnet. The demonstrator will produce 5 T standalone and between 17 T and 20 T, when inserted into the 100 mm aperture of Fresca-2 high field out-sert magnet. The HTS magnet will demonstrate the field strength and field quality that can be achieved. An effective quench detection and protection system will have to be developed to operate with the HTS superconducting materials. This paper presents a ReBCO magnet design using multi strand Roebel cable that develops a stand-alone field of 5 T in a 40 mm clear aperture and discusses the challenges associated with good field quality using this type of material. A selection of magnet designs is presented as result of a first phase of development.

Kirby, GA; Ballarino, A; Bottura, L; Chouika, N; Clement, S; Datskov, V; Fajardo, L; Fleiter, J; Gauthier, R; Gentini, L; Lambert, L; Lopes, M; Perez, JC; de Rijk, G; Rijllart, A; Rossi, L; ten Kate, H; Durante, M; Fazilleau, P; Lorin, C; Hr, E; Stenvall, A; Caspi, S; Marchevsky, M; Goldacker, W; Kario, A

2015-01-01T23:59:59.000Z

266

Accelerator Quality HTS Dipole Magnet Demonstrator designs for the EuCARD-2, 5 Tesla 40 mm Clear Aperture Magnet  

E-Print Network [OSTI]

Future high-energy accelerators will need very high magnetic fields in the range of 20 T. The EuCARD-2 work-package-10 is a collaborative push to take HTS materials into an accelerator quality demonstrator magnet. The demonstrator will produce 5 T standalone and between 17 T and 20 T, when inserted into the 100 mm aperture of Fresca-2 high field out-sert magnet. The HTS magnet will demonstrate the field strength and field quality that can be achieved. An effective quench detection and protection system will have to be developed to operate with the HTS superconducting materials. This paper presents a ReBCO magnet design using multi strand Roebel cable that develops a stand-alone field of 5 T in a 40 mm clear aperture and discusses the challenges associated with good field quality using this type of material. A selection of magnet designs is presented as result of a first phase of development.

Kirby, G; Ballarino, A; Bottura, L; Chouika, N; Clement, S; Datskov, V; Fajardo, L; Fleiter, J; Gauthier, R; Lambert, L; Lopes, M; Perez, J; DeRijk, G; Rijllart, A; Rossi, L; Ten Kate, H; Durante, M; Fazilleau, P; Lorin, C; Haro, E; Stenvall, A; Caspi, S; Marchevsky, M; Goldacker, W; Kario, A

2014-01-01T23:59:59.000Z

267

mm-WAVE Op-Amps FOR LOW DISTORTION AMPLIFICATION WITH HIGH OIP3/PDC RATIO > 100 AT 2 GHz  

E-Print Network [OSTI]

mm-WAVE Op-Amps FOR LOW DISTORTION AMPLIFICATION WITH HIGH OIP3/PDC RATIO > 100 AT 2 GHz Zach in bandwidth for an op-amp of any kind, as well as 3? betterment in OIP3/PDC ratio at fs = 2-3 GHz, when dissipation PDC. This very high ratio of third-order-intercept power to DC power consumption POIP 3/PDC > 100

Rodwell, Mark J. W.

269

Data:E7e6a9ec-c429-42d6-90c9-64f337dd0502 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1cc No revision has beenace4-3e58210a501f Noc9-64f337dd0502 No revision has been approved for this

270

Data:Ed4d5a2f-32a1-4b80-8c8a-2dd694c0ff57 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1cc NoEce78e10-0967-4d20-a270-53a70a3b054f No revision has been approved2dd694c0ff57 No revision has

271

Data:B0f82e5f-2590-48f3-aa42-0f179f7dd0b1 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2 No revision has38865d08 No revision has been approved for thisc607ec833c8 Nodc1-ec5083dd1c49 No

272

Data:02c3db94-dc82-47c7-8f9d-d4c57e9fc8ae | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable Solutions LLC JumpCrowd6-a5ed76e6de80bed2-4ca0-824f-0bc1544dd749 Noc57e9fc8ae

273

Data:4b21a8f6-4cb3-498b-a3b2-f5c98dd29320 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revisione66e17fc7f7d25b394 Noc98dd29320 No revision has been approved for this page.

274

Data:0ac97b38-3dd4-4ac6-94a0-1b3ab8d36bb0 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable-1a29da98863b No revision has beencde-a5ba-d1dd41e15527f402edce27

275

Data:A1da55ee-dd49-412a-bdd8-1d6e6a86b70d | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 Nod2db5b31cb44 No revision-b209-069dd1fd7c05 No revision has been6-d6a01778f46a No revision

276

Data:Ad926f1e-cbd4-4dd6-a809-80e47b5e3b75 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2 No revision has been approved forcbd4-4dd6-a809-80e47b5e3b75 No revision has been approved for this

277

Data:D88af676-8c67-4b0c-90f6-9dd3d910ac75 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 No revision has beenadf9-4884-b0c1-529b3bb19f9c No revision has been approved for thiscdc53116dd3d910ac75 No

278

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279

Magnetic Materials (MM)  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces and InterfacesAdministration -Lowell L.FallU . S .ofFieldMagnetic Materials

280

Fabrication and Test of 90-mm Nb3Sn Quadrupole Model Based on Dipole-type Collar  

SciTech Connect (OSTI)

A series of 90-mm TQC quadrupole models with a collar-based mechanical structure has been fabricated and tested within the framework of the US-LHC Accelerator Research Program (LARP) using quadrupole-symmetric stainless steel collar laminations. This paper describes the design features, construction and test of TQC02Eb, the first TQC made with dipole-type collar and collaring techniques. Magnet test includes quench performance and field quality measurements at 4.5 and 1.9 K. Results of model performance for TQC quadrupoles based on dipole-type and quadrupole-type collars are compared and discussed.

Bossert, R.; Andreev, N.; Chlachidze, G.; Kashikhin, V.S.; Kashikhin, V.V.; Lamm, M.J.; Nobrega, F.; Novitski, I.; Tartaglia, M.; Velev, G.; Zlobin, A.V.; /Fermilab

2010-07-29T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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

Vapor-liquid equilibria of coal-derived liquids; 3: Binary systems with tetralin at 200 mmHg  

SciTech Connect (OSTI)

Isobaric vapor-liquid equilibrium data are reported for binary systems of tetralin with p-xylene, [gamma]-picoline, piperidine, and pyridine; all systems were measured at 26.66 kPa (200 mmHg) with a recirculation still. Liquid-phase activity coefficients were correlated using the Van Laar, Wilson, NRTL, and UNIQUAC equations. Vapor-phase nonidealities were found negligible under the experimental conditions of this work, and deviations of the liquid phase from the ideal behavior, as described by Raoult's law, were found to be slightly positive for all the systems.

Blanco, B.; Beltran, S.; Cabezas, J.L. (University Coll., Burgos (Spain). Dept. of Chemical Engineering); Coca, J. (Univ. of Oviedo (Spain). Dept. of Chemical Engineering)

1994-01-01T23:59:59.000Z

282

Proposal for the award of a contract for the supply of 5 mm depleted-uranium plates for the UA1 calorimeter upgrading  

E-Print Network [OSTI]

Proposal for the award of a contract for the supply of 5 mm depleted-uranium plates for the UA1 calorimeter upgrading

1986-01-01T23:59:59.000Z

283

Proposal for the award of a contract for the supply of 5 mm depleted-uranium plates for the UA1 experiment  

E-Print Network [OSTI]

Proposal for the award of a contract for the supply of 5 mm depleted-uranium plates for the UA1 experiment

1986-01-01T23:59:59.000Z

284

The Ability of MM5 to Simulate Ice Clouds: Systematic Comparison between Simulated and Measured Fluxes and Lidar/Radar Profiles at the  

E-Print Network [OSTI]

to produce too much solid water (ice and snow) and not enough liquid water. 1. Introduction Ice clouds playThe Ability of MM5 to Simulate Ice Clouds: Systematic Comparison between Simulated and Measured­NCAR Mesoscale Model (MM5) to simulate midlatitude ice clouds is evaluated. Model outputs are compared to long

Protat, Alain

285

Simultaneous Radio to (Sub-) Mm-Monitoring of Variability and Spectral Shape Evolution of Potential GLAST Blazars  

SciTech Connect (OSTI)

The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11 cm to 7mm wavelength). Here, we present a short overview of these activities which will complement the multi-wavelengths activities of the GLAST/LAT collaboration towards the 'low-energy' radio bands. Further we will give a brief outlook including the extension of this coordinated campaign towards higher frequencies and future scientific aims.

Fuhrmann, L.; Zensus, J.A.; Krichbaum, T.P.; Angelakis, E.; /Bonn, Max Planck Inst., Radioastron.; Readhead, A.C.S.; /Caltech

2011-11-29T23:59:59.000Z

286

ASSEMBLY AND TEST OF A 120 MM BORE 15 T NB3SN QUADRUPOLE FOR THE LHC UPGRADE  

SciTech Connect (OSTI)

In support of the Large Hadron Collider (LHC) luminosity upgrade, the US LHC Accelerator Research Program (LARP) has been developing a 1-meter long, 120 mm bore Nb{sub 3}Sn IR quadrupole magnet (HQ). With a design short sample gradient of 219 T/m at 1.9 K and a peak field approaching 15 T, one of the main challenges of this magnet is to provide appropriate mechanical support to the coils. Compared to the previous LARP Technology Quadrupole and Long Quadrupole magnets, the purpose of HQ is also to demonstrate accelerator quality features such as alignment and cooling. So far, 8 HQ coils have been fabricated and 4 of them have been assembled and tested in HQ01a. This paper presents the mechanical assembly and test results of HQ01a.

Felice, H.; Caspi, S.; Cheng, D.; Dietderich, D.; Ferracin, P.; Hafalia, R.; Joseph, J.; Lizarazo, J.; Sabbi, G. L.; Wang, X.; Anerella, M.; Ghosh, A. K.; Schmalzle, J.; Wanderer, P.; Ambrosio, G.; Bossert, R.; Zlobin, A. V.

2010-05-23T23:59:59.000Z

287

Test Results of HD2, A High Field Nb3Sn Dipole with A 36 MM Bore  

SciTech Connect (OSTI)

The Superconducting Magnet Program at Lawrence Berkeley National Laboratory (LBNL) has developed the 1 m long Nb{sub 3}Sn dipole magnet HD2. With tilted (flared) ends to avoid obstructing a 36 mm clear bore, HD2 represents a step towards the use of block-type coils in high-field accelerator magnets. The coil design has been optimized to minimize geometric harmonics and reduce the conductor peak field in the end region, resulting in an expected short sample dipole field of 15 T. The support structure is composed by an external aluminum shell pre-tensioned with pressurized bladders and interference keys, and by two stainless steel end plates compressing the coil ends through four aluminum axial rods. We report on magnet design, assembly, and test results, including training performance, quench locations, and strain gauge measurements.

Ferracin, Paolo

2008-05-19T23:59:59.000Z

288

Description and commissioning of NEXT-MM prototype: first results from operation in a Xenon-Trimethylamine gas mixture  

E-Print Network [OSTI]

A technical description of NEXT-MM and its commissioning and first performance is reported. Having an active volume of ~35 cm drift $\\times$ 28 cm diameter, it constitutes the largest Micromegas-read TPC operated in Xenon ever constructed, made by a sectorial arrangement of the 4 largest single wafers manufactured with the Microbulk technique to date. It is equipped with a suitably pixelized readout and with a sufficiently large sensitive volume (~23 l) so as to contain long (~20 cm) electron tracks. First results obtained at 1 bar for Xenon and trimethylamine (Xe-(2 %)TMA) mixture are presented. The TPC can accurately reconstruct extended background tracks. An encouraging full-width half-maximum of 11.6 % was obtained for ~29 keV gammas without resorting to any data post-processing.

lvarez, V; Borges, F I G M; Calvet, D; Crcel, S; Castel, J; Cebrin, S; Cervera, A; Conde, C A N; Dafni, T; Dias, T H V T; Daz, J; Druillole, F; Egorov, M; Esteve, R; Evtoukhovitch, P; Fernandes, L M P; Ferrario, P; Ferreira, A L; Ferrer-Ribas, E; Freitas, E D C; Gehman, V M; Gil, A; Giomataris, I; Goldschmidt, A; Gmez, H; Gmez-Cadenas, J J; Gonzlez-Daz, D; Gutirrez, R M; Hauptman, J; Morata, J A Hernando; Herrera, D C; Iguaz, F J; Irastorza, I G; Jinete, M A; Labarga, L; Laing, A; Coguie, A Le; Liubarsky, I; Lopes, J A M; Lorca, D; Losada, M; Luzn, G; Mar, A; Martn-Albo, J; Martnez, A; Martnez-Lema, G; Miller, T; Moiseenko, A; Mols, J P; Monrabal, F; Monteiro, C M B; Mora, F J; Moutinho, L M; Vidal, J Muoz; da Luz, H Natal; Navarro, G; Nebot-Guinot, M; Nygren, D; Oliveira, C A B; Palma, R; Prez, J; Aparicio, J L Prez; Renner, J; Ripoll, L; Rodrguez, A; Rodrguez, J; Santos, P; Santos, J M F dos; Segui, L; Serra, L; Shuman, D; Simn, A; Sofka, C; Sorel, M; Toledo, J F; Toms, A; Torrent, J; Tsamalaidze, Z; Veloso, J F C A; Villar, J A; Webb, R C; White, J T; Yahlali, N

2013-01-01T23:59:59.000Z

289

Electron dynamics in complex environments with real-time time dependent density functional theory in a QM-MM framework  

SciTech Connect (OSTI)

This article presents a time dependent density functional theory (TDDFT) implementation to propagate the Kohn-Sham equations in real time, including the effects of a molecular environment through a Quantum-Mechanics Molecular-Mechanics (QM-MM) hamiltonian. The code delivers an all-electron description employing Gaussian basis functions, and incorporates the Amber force-field in the QM-MM treatment. The most expensive parts of the computation, comprising the commutators between the hamiltonian and the density matrixrequired to propagate the electron dynamics, and the evaluation of the exchange-correlation energy, were migrated to the CUDA platform to run on graphics processing units, which remarkably accelerates the performance of the code. The method was validated by reproducing linear-response TDDFT results for the absorption spectra of several molecular species. Two different schemes were tested to propagate the quantum dynamics: (i) a leap-frog Verlet algorithm, and (ii) the Magnus expansion to first-order. These two approaches were confronted, to find that the Magnus scheme is more efficient by a factor of six in small molecules. Interestingly, the presence of iron was found to seriously limitate the length of the integration time step, due to the high frequencies associated with the core-electrons. This highlights the importance of pseudopotentials to alleviate the cost of the propagation of the inner states when heavy nuclei are present. Finally, the methodology was applied to investigate the shifts induced by the chemical environment on the most intense UV absorption bands of two model systems of general relevance: the formamide molecule in water solution, and the carboxy-heme group in Flavohemoglobin. In both cases, shifts of several nanometers are observed, consistently with the available experimental data.

Morzan, Uriel N.; Ramrez, Francisco F.; Scherlis, Damin A., E-mail: damian@qi.fcen.uba.ar, E-mail: mcgl@qb.ffyb.uba.ar [Departamento de Qumica Inorgnica, Analtica y Qumica Fsica/INQUIMAE, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, Pab. II, Buenos Aires (C1428EHA) (Argentina); Oviedo, M. Beln; Snchez, Cristin G. [Departamento de Matemtica y Fsica, Facultad de Ciencias Qumicas, INFIQC, Universidad Nacional de Crdoba, Ciudad Universitaria, X5000HUA Crdoba (Argentina)] [Departamento de Matemtica y Fsica, Facultad de Ciencias Qumicas, INFIQC, Universidad Nacional de Crdoba, Ciudad Universitaria, X5000HUA Crdoba (Argentina); Lebrero, Mariano C. Gonzlez, E-mail: damian@qi.fcen.uba.ar, E-mail: mcgl@qb.ffyb.uba.ar [Instituto de Qumica y Fisicoqumica Biolgicas, IQUIFIB, CONICET (Argentina)] [Instituto de Qumica y Fisicoqumica Biolgicas, IQUIFIB, CONICET (Argentina)

2014-04-28T23:59:59.000Z

290

Data:Ec6b2c66-7eaf-4334-8f4d-d1f81a4e3535 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1cc No revisionEc01d6d9-0b5c-46e0-8010-da811753d74a No revisionb36b06409 No revision-8f4d-d1f81a4e3535

291

Data:Dd421e92-b3b3-44d5-8e6a-5db40d2fe654 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744 NoDce066cd-9c07-4949-aa43-5e5007829464 No revision has been approved forDd421e92-b3b3-44d5-8e6a-5db40d2fe654

292

Auditory Processing Disorders Pre-Screening Form Child's Name:____________________________ Date of Birth:_________________  

E-Print Network [OSTI]

Static Encephalopathy Syndrome (i.e. Down Syndrome, Velocardiofacial Syndrome, Pierre Robin Sequence: Diagnosis Date (mm/dd/yyyy) Diagnosis Date (mm/dd/yyyy) ADD/ADHD Anxiety Asperger's Syndrome Autism Behavior

O'Toole, Alice J.

293

Comparative Theoretical Study of the Ring-Opening Polymerization of Caprolactam vs Caprolactone Using QM/MM Methods  

SciTech Connect (OSTI)

Candida antarctica lipase B (CALB) efficiently catalyzes the ring-opening polymerization of lactones to high molecular weight products in good yield. In contrast, an efficient enzymatic synthesis of polyamides has so far not been described in the literature. This obvious difference in enzyme catalysis is the subject of our comparative study of the initial steps of a CALB catalyzed ring-opening polymerization of ?- caprolactone and ?-caprolactam. We have applied docking tools to generate the reactant state complex and performed quantum mechanical/molecular mechanical (QM/MM) calculations at the density functional theory (DFT) PBE0 level of theory to simulate the acylation of Ser105 by the lactone and the lactam, respectively, via the corresponding first tetrahedral intermediates. We could identify a decisive difference in the accessibility of the two substrates in the ring-opening to the respective acyl enzyme complex as the attack of ?-caprolactam is hindered because of an energetically disfavored proton transfer during this part of the catalytic reaction while ?-caprolactone is perfectly processed along the widely accepted pathway using the catalytic triade of Ser105, His224, and Asp187. Since the generation of an acylated Ser105 species is the crucial step of the polymerization procedure, our results give an explanation for the unsatisfactory enzymatic polyamide formation and opens up new possibilities for targeted rational catalyst redesign in hope of an experimentally useful CALB catalyzed polyamide synthesis.

Elsasser, Brigitta M.; Schoenen, Iris; Fels, Gregor

2013-06-07T23:59:59.000Z

294

A 0.042 mm^2 programmable biphasic stimulator for cochlear implants suitable for a large number of channels  

E-Print Network [OSTI]

This paper presents a compact programmable biphasic stimulator for cochlear implants. By employing double-loop negative feedback, the output impedance of the current generator is increased, while maximizing the voltage compliance of the output transistor. To make the stimulator circuit compact, the stimulation current is set by scaling a reference current using a two stage binary-weighted transistor DAC (comprising a 3 bit high-voltage transistor DAC and a 4 bit low-voltage transistor DAC). With this structure the power consumption and the area of the circuit can be minimized. The proposed circuit has been implemented in AMS 0.18um high-voltage CMOS IC technology, using an active chip area of about 0.042mm^2. Measurement results show that proper charge balance of the anodic and cathodic stimulation phases is achieved and a dc blocking capacitor can be omitted. The resulting reduction in the required area makes the proposed system suitable for a large number of channels.

Ngamkham, W; Serdijn, W A; Bes, C J; Briaire, J J; Frijns, J H M

2015-01-01T23:59:59.000Z

295

Of Horseshoes and Heliotropes: Dynamics of Dust in the Encke Gap M.M. Hedmana,, J.A. Burnsb, D.P. Hamiltonc, M.R. Showalterd  

E-Print Network [OSTI]

Of Horseshoes and Heliotropes: Dynamics of Dust in the Encke Gap M.M. Hedmana,, J.A. Burnsb, D demonstrates "heliotropic" behavior: its geometric center is displaced away from Saturn's center towards

Hamilton, Douglas P.

296

IEEE JOURNAL OF SOLID-STATE CIRCUITS, VOL. 48, NO. 1, JANUARY 2013 229 A Modular 1 mm Die-Stacked Sensing Platform  

E-Print Network [OSTI]

IEEE JOURNAL OF SOLID-STATE CIRCUITS, VOL. 48, NO. 1, JANUARY 2013 229 A Modular 1 mm Die with compatibility to commercial C protocols. A self-adapting power management unit is proposed for efficient battery voltage down conversion for wide range of battery voltages and load current. The power man- agement unit

Dutta, Prabal

297

570 2008 IEEE International Solid-State Circuits Conference ISSCC 2008 / SESSION 31 / RF & mm-WAVE POWER AMPLIFIERS / 31.7  

E-Print Network [OSTI]

570 · 2008 IEEE International Solid-State Circuits Conference ISSCC 2008 / SESSION 31 / RF & mm supply voltages that is very useful for a low-battery-voltage solution. However, it is not compatible with the higher voltages presented by the Li-ion batteries which under charging situations can present supply

Hajimiri, Ali

298

12A.4 VERTICAL VELOCITY AND BUOYANCY CHARACTERISTICS OF ECHO PLUMES DETECTED BY AN AIRBORNE MM-WAVE RADAR IN THE CONVECTIVE  

E-Print Network [OSTI]

12A.4 VERTICAL VELOCITY AND BUOYANCY CHARACTERISTICS OF ECHO PLUMES DETECTED BY AN AIRBORNE MM-WAVE, is the availability of in situ thermodynamic and kinematic observations, and the direct observation of horizontal, as part of IHOP_02 (The International Water Vapor Project, Weckwerth et al 2003). The key radar

Geerts, Bart

299

MM 7/2011 (rev from JB) When writing a paper or conducting academic research, you'll often come across many different  

E-Print Network [OSTI]

MM 7/2011 (rev from JB) When writing a paper or conducting academic research, you'll often come across many different types of sources. Most of the time, these sources will include periodical articles. Periodical articles can be comprised of news accounts, opinion, commentary, scholarly analysis, and

300

To obtain representative temperatures, sensors were made with a length of 35 cm. The stainless steel needles have a diameter of 3 mm. Inside are five  

E-Print Network [OSTI]

To obtain representative temperatures, sensors were made with a length of 35 cm. The stainless steel needles have a diameter of 3 mm. Inside are five Platinum Pt-100 sensors, that are cascaded in series to obtain a Pt-500 sensor. The sensors are calibrated to retrieve individual calibration

Haak, Hein

Note: This page contains sample records for the topic "mm dd yy" 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

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 1.76mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 1.76 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

302

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.22mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.22 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

303

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 1.76mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 1.76 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

304

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 4.4mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 4.4 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions. The experiments...

Hassell, David

2008-09-05T23:59:59.000Z

305

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 1.32mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 1.32 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

306

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.88mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.88 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

307

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 2.2mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 2.2 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions. The experiments...

Hassell, David

2008-09-05T23:59:59.000Z

308

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.088mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.088 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

309

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.44mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.44 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

310

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.088mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.088 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

311

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.044mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.044 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

312

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 2.2mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 2.2 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions. The experiments...

Hassell, David

2008-09-05T23:59:59.000Z

313

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 2.64mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 2.64 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

314

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 1.32mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 1.32 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

315

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.88mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.88 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-05T23:59:59.000Z

316

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.044mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.044 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

317

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.44mm/s, 155C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.44 mm/s at 155C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

318

HDPE (CM1) optical birefringence pattern in cross-slot flow, piston speed 0.22mm/s, 175C  

E-Print Network [OSTI]

Rheometer (MPR4) at a piston speed of 0.22 mm/s at 175C. The geometry generates a flow field with an extensional component at the centreline. If the no slip condition at a solid surface is satisfied, the side walls are high shear rate regions...

Hassell, David

2008-09-04T23:59:59.000Z

319

July 1, 1997 / Vol. 22, No. 13 / OPTICS LETTERS 991 Passively Q-switched 1.34-mm Nd:YVO4 microchip laser with  

E-Print Network [OSTI]

-pumped 1.34-mm Nd:YVO4 microchip laser. We achieved single- frequency, 230-ps pulses by using an InGaAsP Nd:YVO4 microchip laser that uses InGaAsP semiconductor saturable- absorber mirrors (SESAM's).1 ­ 3 mode spacing exceeds the gain bandwidth. In addition, a short absorption length is needed for efficient

Keller, Ursula

320

Mon. Not. R. Astron. Soc. 320, 131138 (2001) Discs and the 10-mm silicate spectra of young stellar objects with non-  

E-Print Network [OSTI]

Mon. Not. R. Astron. Soc. 320, 131±138 (2001) Discs and the 10-mm silicate spectra of young stellar and Taurus-Elias 7 (Haro6-10, GV Tau) is distinguished from foreground silicate absorption using a simple that of Elias 7 is optically thick. We suggest that HL Tau's optically thin component arises from silicate dust

Bowey, Janet

Note: This page contains sample records for the topic "mm dd yy" 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.


321

IUPILLiadTNz427447"mum""nmm'mm"mm  

E-Print Network [OSTI]

measured, and measured spectra were compared with those predicted by the seismic displacement discontinuity theory. Results are compared with those...

322

Coupling MM5 with ISOLSM:  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation Proposed Newcatalyst phases on &gamma;-Al2O3. |ID#: 19834Costsincludingincludinga Yun

323

a. Lngsamt & adiabatiskt reversibel, dvs en isentropisk process V1 = nRT1 / p1 = (m/M) RT1/p1 , massa m = 1 kg  

E-Print Network [OSTI]

Svar 1303: a. Långsamt & adiabatiskt reversibel, dvs en isentropisk process V1 = n·R·T1 / p1 = (m/M) ·R·T1/p1 , massa m = 1 kg H2 : M = 0.002 kg/mol; CO : M = 0.028 kg/mol; CO2 : M = 0.044 kg/mol p1 = z bar V1 = (R/M) · (300 + 50·a) / z m3 . t.ex. 30066 : p = 3 bar, gas = CO, T1 = 450 K V1 = 0.445 m3

Zevenhoven, Ron

324

US graphite reactor D&D experience  

SciTech Connect (OSTI)

This report describes the results of the U.S. Graphite Reactor Experience Task for the Decommissioning Strategy Plan for the Leningrad Nuclear Power Plant (NPP) Unit 1 Study. The work described in this report was performed by the Pacific Northwest National Laboratory (PNNL) for the Department of Energy (DOE).

Garrett, S.M.K.; Williams, N.C.

1997-02-01T23:59:59.000Z

325

DD-R-15(EN) Clearance Laboratory  

E-Print Network [OSTI]

-active materials, which will originate from the decommissioning of all the nuclear facilities at the Risø originating from decommissioning the nuclear facilities at the site: the research reactors DR 1, DR 2 and DR 3 Lauridsen, João Silva, Jens Søgaard-Hansen, Lisbeth Warming Danish Decommissioning, Roskilde September 2005

326

Microsoft Word - turner-dd2.doc  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment SurfacesResource Program PreliminaryA TrimodalRECENTMicrophysical Properties

327

Microsoft Word - turner-dd3.doc  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment SurfacesResource Program PreliminaryA TrimodalRECENTMicrophysical PropertiesImproved

328

Director's Discretionary (DD) Program | Argonne Leadership Computing  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc DocumentationP-Series to UserProduct:Directives Templates by WebsiteFacility Science at ALCF

329

D&D and Risk Assessment Tools  

Office of Environmental Management (EM)

compares radionuclides of concern and survey media to detector capabilities. With input data on radionuclides of concern, the tool recommends radiation detectors that have the...

330

Two-Dimensional Thin Layer Chromatography (2D-TLC) 1. Resuspend RNA pellet in 5 l ddH2O. Place at room temperature for 5-15 minutes. Use pipette tip  

E-Print Network [OSTI]

not damage surface of plate at origin. · Use Merck plates, 20 X 20 cm, pre-coated with cellulose, 0.1 mm, no indicator (from VWR). 5. Spot sample on chromatography plate at origin. Do 0.1 - 0.2 µl at a time. Dry with a gentle stream of filtered air across origin. Wait until spot is completely dry between applications

Aris, John P.

331

Deposition of TiN and HfO{sub 2} in a commercial 200 mm remote plasma atomic layer deposition reactor  

SciTech Connect (OSTI)

The authors describe a remote plasma atomic layer deposition reactor (Oxford Instruments FlexAL trade mark sign ) that includes an inductively coupled plasma source and a load lock capable of handling substrates up to 200 mm in diameter. The deposition of titanium nitride (TiN) and hafnium oxide (HfO{sub 2}) is described for the combination of the metal-halide precursor TiCl{sub 4} and H{sub 2}-N{sub 2} plasma and the combination of the metallorganic precursor Hf[N(CH{sub 3})(C{sub 2}H{sub 5})]{sub 4} and O{sub 2} plasma, respectively. The influence of the plasma exposure time and substrate temperature has been studied and compositional, structural, and electrical properties are reported. TiN films with a low Cl impurity content were obtained at 350 deg. C at a growth rate of 0.35 A /cycle with an electrical resistivity as low as 150 {mu}{omega} cm. Carbon-free (detection limit <2 at. %) HfO{sub 2} films were obtained at a growth rate of 1.0 A /cycle at 290 deg. C. The thickness and resisitivity nonuniformity was <5% for the TiN and the thickness uniformality was <2% for the HfO{sub 2} films as determined over 200 mm wafers.

Heil, S. B. S.; Hemmen, J. L. van; Hodson, C. J.; Singh, N.; Klootwijk, J. H.; Roozeboom, F.; Sanden, M. C. M. van de; Kessels, W. M. M. [Department of Applied Physics, Eindhoven University of Technology, P.O. Box 513, 5600 MB Eindhoven (Netherlands); Oxford Instruments Plasma Technology, North End, Yatton BS49 4AP (United Kingdom); Philips Research Laboratories, High Tech Campus 4, 5656 AE Eindhoven (Netherlands); NXP Semiconductors Research, High Tech Campus 4, 5656 AE Eindhoven (Netherlands); Department of Applied Physics, Eindhoven University of Technology, P.O. Box 513, 5600 MB Eindhoven (Netherlands)

2007-09-15T23:59:59.000Z

332

Measurement of astrophysical S factors and electron screening potentials for d(d, n){sup 3}He reaction In ZrD{sub 2}, TiD{sub 2}, D{sub 2}O, and CD{sub 2} targets in the ultralow energy region using plasma accelerators  

SciTech Connect (OSTI)

The paper is devoted to study electron screening effect influence on the rate of d(d, n){sup 3}He reaction in the ultralow deuteron collision energy range in the deuterated polyethylene (CD{sub 2}), frozen heavy water (D{sub 2}O) and deuterated metals (ZrD{sub 2} and TiD{sub 2}). The ZrD{sub 2} and TiD{sub 2} targets were fabricated via magnetron sputtering of titanium and zirconium in gas (deuterium) environment. The experiments have been carried out using high-current plasma pulsed accelerator with forming of inverse Z pinch (HCEIRAS, Russia) and pulsed Hall plasma accelerator (NPI at TPU, Russia). The detection of neutrons with energy of 2.5MeV from dd reaction was done with plastic scintillation spectrometers. As a result of the experiments the energy dependences of astrophysical S factor for the dd reaction in the deuteron collision energy range of 2-7 keV and the values of the electron screening potential U{sub e} of interacting deuterons have been measured for the indicated above target: U{sub e}(CD{sub 2}) Less-Than-Or-Slanted-Equal-To 40 eV; U{sub e}(D{sub 2}O) Less-Than-Or-Slanted-Equal-To 26 eV; U{sub e}(ZrD{sub 2}) = 157 {+-} 43 eV; U{sub e}(TiD{sub 2}) = 125{+-}34 eV. The value of astrophysical S factor, corresponding to the deuteron collision energy equal to zero, in the experiments with D{sub 2}O target is found: S{sub b}(0) = 58.6 {+-} 3.6 keV b. The paper compares our results with other available published experimental and calculated data.

Bystritsky, V. M. [Joint Institute for Nuclear Research (Russian Federation); Bystritskii, Vit. M. [University of California, Department of Physics and Astronomy (United States); Dudkin, G. N. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Filipowicz, M. [University of Science and Technology, Faculty of Fuels and Energy, AGH (Poland); Gazi, S.; Huran, J. [Institute of Electrical Engineering SAS (Slovakia); Kobzev, A. P. [Joint Institute for Nuclear Research (Russian Federation); Mesyats, G. A. [Lebedev Physical Institute of the Russian Academy of Sciences (Russian Federation); Nechaev, B. A.; Padalko, V. N. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Parzhitskii, S. S. [Joint Institute for Nuclear Research (Russian Federation); Pen'kov, F. M. [Institute of Nuclear Physics NNC (Kazakhstan); Philippov, A. V. [Joint Institute for Nuclear Research (Russian Federation); Kaminskii, V. L. [National Scientific Research Tomsk Polytechnical University (Russian Federation); Tuleushev, Yu. Zh. [Institute of Nuclear Physics NNC (Kazakhstan); Wozniak, J. [University of Science and Technology, Faculty of Physics and Applied Computer Sciences, AGH (Poland)

2012-01-15T23:59:59.000Z

333

Testing Results for Nb-Ti, 120-mm-Aperture, Low-B Quadrupole Models for the LHC High-Luminosity Insertion  

E-Print Network [OSTI]

The design and construction of a 120 mm wide-aperture, Nb-Ti superconducting quadrupole magnet for the LHC insertion region is part of a study towards a luminosity upgrade of the LHC at CERN, envisaged for 2020-22. The main challenges for this accelerator quality magnet are to operate reliably with the high heat and radiation loads that are predicted in the insertion magnet regions. Calculations give approximately 500 Watts over the 30-m-long string of insertion magnets, while today LHC is operating for a nominal heat load of 12 Watts. To extract this heat, the model magnets incorporate new features: Open cable insulation, open ground insulation, open magnet structure, and a quench heater that has open channels to help extract the steady state heat load. This paper presents results from tests at room temperature and 1.8 K for the initial model magnet. We report magnet training, transfer function and field quality measurements, quench heater performance, and heat extraction studies using imbedded heaters to si...

Kirby, G A; Bajko, M; Charrondiere, M; Bourcey, N; Datskov, V I; Fessia, P; Feuvrier, J; Galbraith, P; Garcia Tabares, A; Garcia-Perez, J; Granieri, P; Hagen, P; Lorin, C; Perez, J C; Russenschuck, S; Sahner, T; Segreti, M; Todesco, E; Willering, G

2013-01-01T23:59:59.000Z

334

The Ability of MM5 to Simulate Ice Clouds: Systematic Comparison between Simulated and Measured Fluxes and Lidar/Radar Profiles at SIRTA Atmospheric Observatory  

SciTech Connect (OSTI)

Ice clouds play a major role in the radiative energy budget of the Earth-atmosphere system (Liou 1986). Their radiative effect is governed primarily by the equilibrium between their albedo and greenhouse effects. Both macrophysical and microphysical properties of ice clouds regulate this equilibrium. For quantifying the effect of these clouds onto climate and weather systems, they must be properly characterized in atmospheric models. In this paper we use remote-sensing measurements from the SIRTA ground based atmospheric observatory (Site Instrumental de Recherche par Teledetection Atmospherique, http://sirta.lmd.polytechnique.fr). Lidar and radar observations taken over 18 months are used, in order to gain statistical confidence in the model evaluation. Along this period of time, 62 days are selected for study because they contain parts of ice clouds. We use the ''model to observations'' approach by simulating lidar and radar signals from MM5 outputs. Other more classical variables such as shortwave and longwave radiative fluxes are also used. Four microphysical schemes, among which that proposed by Reisner et al. (1998) with original or modified parameterizations of particle terminal fall velocities (Zurovac-Jevtic and Zhang 2003, Heymsfield and Donner 1990), and the simplified Dudhia (1989) scheme are evaluated in this study.

Chiriaco, M.; Vautard, R.; Chepfer, H.; Haeffelin, M.; Wanherdrick, Y.; Morille, Y.; Protat, A.; Dudhia, J.

2005-03-18T23:59:59.000Z

335

Friction Factor Measurement, Analysis, and Modeling for Flat-Plates with 12.15 mm Diameter Hole-Pattern, Tested with Air at Different Clearances, Inlet Pressures, and Pressure Ratios  

E-Print Network [OSTI]

of 800, 1000, and 1200 psi respectively). These nine combinations of clearance and inlet pressure will give a range of friction factor. The following objectives are considered. 17 Figure 10. Detailed view of a 3.175 mm diameter hole...

Deva Asirvatham, Thanesh

2011-02-22T23:59:59.000Z

336

mm-Wave Op-Amps employing simple-Miller compensation, with OIP3/PDC ratios of 211 (10 dB NF) and 144 (6.0 dB NF) at 2 GHz  

E-Print Network [OSTI]

mm-Wave Op-Amps employing simple-Miller compensation, with OIP3/PDC ratios of 211 (10 dB NF/PDC ratio at fs = 2-3 GHz, compared to state-of-the-art. We address considerations important 1000 mW power dissipation PDC . This very high ratio of output-referred third-order-intercept power

Rodwell, Mark J. W.

337

Computation of the free energy due to electron density fluctuation of a solute in solution: A QM/MM method with perturbation approach combined with a theory of solutions  

SciTech Connect (OSTI)

We developed a perturbation approach to compute solvation free energy ?? within the framework of QM (quantum mechanical)/MM (molecular mechanical) method combined with a theory of energy representation (QM/MM-ER). The energy shift ? of the whole system due to the electronic polarization of the solute is evaluated using the second-order perturbation theory (PT2), where the electric field formed by surrounding solvent molecules is treated as the perturbation to the electronic Hamiltonian of the isolated solute. The point of our approach is that the energy shift ?, thus obtained, is to be adopted for a novel energy coordinate of the distribution functions which serve as fundamental variables in the free energy functional developed in our previous work. The most time-consuming part in the QM/MM-ER simulation can be, thus, avoided without serious loss of accuracy. For our benchmark set of molecules, it is demonstrated that the PT2 approach coupled with QM/MM-ER gives hydration free energies in excellent agreements with those given by the conventional method utilizing the Kohn-Sham SCF procedure except for a few molecules in the benchmark set. A variant of the approach is also proposed to deal with such difficulties associated with the problematic systems. The present approach is also advantageous to parallel implementations. We examined the parallel efficiency of our PT2 code on multi-core processors and found that the speedup increases almost linearly with respect to the number of cores. Thus, it was demonstrated that QM/MM-ER coupled with PT2 deserves practical applications to systems of interest.

Suzuoka, Daiki; Takahashi, Hideaki, E-mail: hideaki@m.tohoku.ac.jp; Morita, Akihiro [Department of Chemistry, Graduate School of Science, Tohoku University, Sendai Miyagi 980-8578 (Japan)] [Department of Chemistry, Graduate School of Science, Tohoku University, Sendai Miyagi 980-8578 (Japan)

2014-04-07T23:59:59.000Z

338

ELSEVIER Surface Science 303 (lYY4) 206-230 ;,,.;_:_.y y .../. .' ..`,. :> .,  

E-Print Network [OSTI]

by means of the Fischer- Tropsch technique, and the steam reforming of natural gas to form so-called syngas. Representative examples are the ammonia synthesis via Haber-Bosch, the synthesis of alco- hols and hydrocarbons of products, and (7) diffusion of products from the surface. One typically treats these elementary reactions

Miller, William H.

339

TRANS. INF. THEORY, VOL. XX, NO. YY, THEMONTH YEAR 1 Information-Theoretic Analysis  

E-Print Network [OSTI]

by the Swiss National Science Foundation (SNF) under grant No. 200021-100025/1. D. S. Baum was with ETH Zurich.baum@ieee.org). H. B¨olcskei is with ETH Zurich, 8092 Zurich, Switzerland (e-mail: boelcskei, 8092 Zurich, Switzerland. He is now with Baum Consulting GmbH, 8003 Zurich, Switzerland (e-mail: daniel

Bölcskei, Helmut

340

Kronos 6.2 Project Charter OEPM101 Kronos Project Charter Page 1 of 11  

E-Print Network [OSTI]

Kronos 6.2 Project Charter OEPM101 Kronos Project Charter Page 1 of 11 Project Name: Campus Wide Implementation of a Standardized Timekeeping System ­ Kronos 6.2 Prepared by: Steven McCabe - Project Manager Date (MM/DD/YYYY): June 30, 2011 Project Charter Version History: Version Date (MM/DD/YYYY) Comments

Doudna, Jennifer A.

Note: This page contains sample records for the topic "mm dd yy" 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.


341

PROJECT REQUEST FORM PROJECT HOLDER INFORMATION  

E-Print Network [OSTI]

PROJECT REQUEST FORM Last Name: Email: PROJECT HOLDER INFORMATION UCID:Last Name: Email: Institute if different than Project Holder) First Name: Project Short Name: (50 characters max) (for eFIN view only) Project Title: PROJECT INFORMATION Start Date (MM/DD/YYYY): End Date (MM/DD/YYYY): For Questions or HELP

de Leon, Alex R.

342

Mme B. Cunot MM. N. Bertier  

E-Print Network [OSTI]

combustion de turbine a gaz Luc-Henry DOREY Dpartement d'nergtique Fondamentale et Applique Thse de de combustion de turbine gaz Soutenue le 1 juin 2012 Composition du jury : Mme Cunot B. Rapporteur

Paris-Sud XI, Universit de

343

Mineralogic Model (MM3.0) Report  

SciTech Connect (OSTI)

The purpose of this report is to provide a three-dimensional (3-D) representation of the mineral abundance within the geologic framework model domain. The mineralogic model enables project personnel to estimate mineral abundances at any position, within the model region, and within any stratigraphic unit in the model area. The model provides the abundance and distribution of 10 minerals and mineral groups within 22 stratigraphic sequences or model layers in the Yucca Mountain area. The uncertainties and limitations associated with this model are discussed in Section 6.4. Model validation accomplished by corroboration with data not cited as direct input is discussed in Section 7.

A. Sanchez

2004-09-07T23:59:59.000Z

344

mm-Wave Phase Shifters and Switches  

E-Print Network [OSTI]

media players and other personal devices while enhancing thein Personal Digital Assistant (PDA) devices to automotive

Adabi Firouzjaei, Ehsan

2010-01-01T23:59:59.000Z

345

INSTRUCTIONS Annual Supply Inventory Certificate MM-5  

E-Print Network [OSTI]

, University Director & Operations Manager Materials & Logistics Management Room #: FB058 MC 2012 Telephone - Mandatory _______ _________________________________________________ 3. Materials Management Supervisor for Materials & Logistics Management _______________________________________________ Typed Name - Mandatory

Oliver, Douglas L.

346

Physical Consequences of a Momenta-Transfering Particle Theory of Induced Gravity and New Measurements Indicating Variation from Inverse Square Law at Length Scale of .1 mm: Statistical Time Properties of Gravitational Interaction and Analysis Thereof  

E-Print Network [OSTI]

This work presents physical consequences of our theory of induced gravity (Ref.1) regarding: 1) the requirement to consider shape and materials properties when calculating graviton cross section collision area; 2) use of Special Relativity; 3) implications regarding the shape of cosmos; 4) comparison to explanations using General Relativity; 5) properties of black holes; 6) relationship to the strong force and the theorized Higgs boson; 7) the possible origin of magnetic attraction; 8) new measurements showing variation from gravitational inverse square behavior at length scales of 0.1 mm and relationship to the Cosmological constant, and proof of the statistical time properties of the gravitational interaction.

Gary Christopher Vezzoli

2001-04-04T23:59:59.000Z

347

DD2431 Machine Learning Lab 2: Bayes Classifier & Boosting  

E-Print Network [OSTI]

be expressed as: t = - R + QQQ (1) R = uuu (2) QQQ = 1 We (2 1 ddd - ) + LLL + LLLT , (3) #12;where

Kjellstrm, Hedvig

348

W&> Dd/ K ^ , > ^ d & MANAGEMENT OF TECHNOLOGY & ENTREPRENEURSHIP INSTITUTE  

E-Print Network [OSTI]

is perhaps the most uncomfortable infliction (...) But being paid, --what will compare with it? The urbane of value, which includes the trade of goods and services between different economic agents. A puzzling question addressed by price theory is, for example: why is water so cheap and diamonds are so expensive

349

The Office of Environmental Management Uranium Enrichment D&D...  

Energy Savers [EERE]

and Staffing Plan Report - Portsmouth Paducah Project Office Above on the left is K-25, at Oak Ridge before and after the 844,000 sq-ft demolition. In addition, on the...

350

SIMULATION OF CARGO CONTAINER INTERROGATION BY D-D NEUTRONS  

E-Print Network [OSTI]

of Energys National Nuclear Security Administration underof Homeland Security, Domestic Nuclear Detection Office,nuclear material hidden in cargo containers has become an important research topic for homeland security.

Lou, Tak Pui; Antolak, Arlyn

2007-01-01T23:59:59.000Z

351

Microsoft Word - 25788WDC_DOE DD FS.docx  

Energy Savers [EERE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector General Office0-72.pdfGeorgeDoesn't32 Master EM ManagementWe at NAPAWM2012 Conference,SANDIAMayJune

352

Crew-Served Machine Guns 5.56-mm and 7.62-mm  

E-Print Network [OSTI]

....................................................................................................1-19 CLEANING AND LUBRICATING PROCEDURES AND PREVENTIVE MAINTENANCE .........................................................................1-8 Section II. MAINTENANCE..........................................................................................1-28 MAINTENANCE PROCEDURES .....................................................................1

US Army Corps of Engineers

353

Coupling MM5 with LSM1: Development, Testing, and Application - MM5_workshop  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation Proposed Newcatalyst phases on &gamma;-Al2O3. |ID#: 19834Costsincludingincludinga

354

EELL DDEERREECCHHOO AALL SSEERRVVIICCIIOO DDEE LLAASS PPRROOBBLLEEMMTTIICCAASS AALLIIMMEENNTTAARRIIAASS DDEE LLAA EEXXPPLLOOTTAACCIINN YY DDEELL CCOOMMEERRCCIIOO DDEE LLOOSS RREECCUURRSSOOSS NNAATTUURRAALLEESS ((**))  

E-Print Network [OSTI]

230400. 1 Ver OMC, Informe sobre el Comercio Mundial 2010, p. 46. halshs-01060946,version1-4Sep2014 #12 problemticas alimentarias del comercio de los recursos naturales resultan igualmente evidentes. Lo que que adoptan la explotacin y el comercio de los recursos naturales, por una parte, y las consecuencias

Boyer, Edmond

355

E-Print Network 3.0 - atpae certification program Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Last First Middle Other names under which records might... be listed: RedID: Date of Birth: MM DD YYYY Name of Certificate Program: Code: Date Completed: Date... were...

356

UU NN II VV EE RR SS II DD AA DD EE FF EE DD EE RR AA LL DD OO RR II OO DD EE JJ AA NN EE II RR OO --UU FF RR JJ Sistema de Bibliotecas e Informao -SiBI  

E-Print Network [OSTI]

para a entrada de dados de monografias na Base Minerva Maria Luiza Cavalcanti Jardim (Organizadora/Biblioteca Suely Alves Ano Bom MN/Biblioteca M294 Manual de entrada de dados de monografias na Base Minerva / Maria INFORMA??O Paula Maria Abrantes Cotta de Mello COMIT? T?CNICO DE PADRONIZA??O DA BASE MINERVA (Monografias

Liu, I-Shih

357

UU NN II VV EE RR SS II DD AA DD EE FF EE DD EE RR AA LL DD OO RR II OO DD EE JJ AA NN EE II RR OO --UU FF RR JJ Sistema de Bibliotecas e Informao -SiBI  

E-Print Network [OSTI]

para a entrada de dados de periódicos na Base Minerva Maria Luiza Cavalcanti Jardim (Organizadoram Jardim, Maria Luiza Cavalcanti. Manual de entrada de dados de periódicos na Base Minerva / Maria PADRONIZA??O DA BASE MINERVA (Periódicos): Maria Luiza Cavalcanti Jardim (Organizadora) IPPUR/Biblioteca Elisa

Liu, I-Shih

358

DSU Research Foundation Profile of Activities  

E-Print Network [OSTI]

Margarita Ecological Reserve additional acreage acquired 2004 yy Dede Alpert Center for Community of Peres Center & dedication of Peres Peace House in Israel 2009 yy Immunologists join BioScience Center yy

Ponce, V. Miguel

359

Microsoft Word - WH-MM-809 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

on three offsite 36" crude oil pipeline valves running from WH to the Lake Charles Meter Station (3-PL00-MOV2, 3-PL00-MOV3, and 3-PL00-MOV4). Tasks include excavation of the...

360

MEASUREMENTS OF THE 1MM RECEIVER OPTICS Dick Plambeck  

E-Print Network [OSTI]

defective rods of extruded Teflon (PTFE). These rods were slightly porous along their central axes, leading roughness, gaps between panels, and scattering by panel #12; -- 2 -- adjusting screws) are summarized

Note: This page contains sample records for the topic "mm dd yy" 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

Microsoft Word - BM-MM-821A.docx  

Broader source: Energy.gov (indexed) [DOE]

carbon dioxide, geothermal system fluids, hydrogen gas, natural gas, nitrogen gas, oil, produced water, steam, and water). Covered modifications would not have the potential to...

362

Microsoft Word - BM-MM-762 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

tools, equipment, and supervision required to replace the existing brine disposal piping to the BM brine tank with new carbon steel pipe and concrete lined carbon steel pipe....

363

Microsoft Word - BM-MM-1026 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

026 Title: Replace Sparge Piping at BM RWIS Description: Subcontractor shall shall provide all labor, materials, tools, equipment, and supervision required to replace sparge piping...

364

Microsoft Word - VP-MM-820 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

recovery, or treatment facilities, but the proposal may include categorically excluded waste storage, disposal, recovery, or treatment actions. 3. Disturb hazardous substances,...

365

Microsoft Word - BH-MM-746B NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

of water, soil, rock, or contaminants; and sampling and characterization of water effluents, air emissions, or solid waste streams. Electronic approval via NEPA Workflow 92313 ....

366

800mm luxury : pencil tower phenomenon in Hong Kong, China  

E-Print Network [OSTI]

150m2 - 40m2 - 60m3. Pencil Towers are slender pencil-like apartment buildings. They are commonly found in high-dense Asian cities such as Hong Kong, Tokyo and Singapore. Focusing on Hong Kong as the context of research, ...

Yam, Hiu Lan

2012-01-01T23:59:59.000Z

367

In-vehicle mm-Wave Channel Model and Measurement  

E-Print Network [OSTI]

and costly cable bundles with wireless links. The current upswing of electrically-propelled vehicles, Ales Prokes The Faculty of Electrical Engineering and Communication Brno University of Technology Brno kilometers of wires weighing easily up to 50 kg [1], while vehicle manufacturers appreciate weight savings

Zemen, Thomas

368

Dimensions are shown in inch (mm ) Dimensions subject to change  

E-Print Network [OSTI]

pole 1 BCD code 2 BCD complement code 3 Gray code 4 Hexadecimal code Contact Material 3 (STD), Gold 1 SPDT, SP3T, SP4T functions · Rotary binary-decimal and hexadecimal coding Typical Applications · Timers RTE1010N13 10 BCD 65 RTE1000N33 RTE1010N33 10 GRAY 65 RTE1600N43 RTE1610N43 10 HEXADECIMAL 65 PC Mount

Berns, Hans-Gerd

369

Microsoft Word - BM-MM-762A,GFE.docx  

Broader source: Energy.gov (indexed) [DOE]

A Title: Replace Brine Disposal System Header to BM Brine Tank, GFE Description: Manufacturer shall provide the piping and fittings associated with the replacement of the brine...

370

A mm-scale aeroelastic oscillation-based anemometer  

E-Print Network [OSTI]

The flutter of a thin filament can provide a good indication of fluid velocity at small scales. By combining a 'fishtail'-shaped filament's aeroelastic and vortex-forced flutter modes, its oscillation frequency can be ...

McKay, Ian Salmon

2012-01-01T23:59:59.000Z

371

Microsoft Word - WH-MM-780 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

to replace the seven obsolete WH raw water injection pump vibration transmitters at pumps WHP-526 though WHP-532. Tasks include replacing the existing GE Bentley Nevada 1800...

372

Microsoft Word - BM-MM-1152 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

equipment, and supervision required to replace the existing Bryan Mound brine disposal pumps, BMP- 115 and BMP-116 with two new pumps (supplied as Government Furnished Equipment)....

373

40 MM Grenade Launcher Qualification Requirements at Department of Energy  

Energy Savers [EERE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankCombustionImprovement3 Beryllium-Associated Worker2014Department of Energy 3Keene -EXECUTIVE.5

374

Posters Surface Flux Intercomparison Between the MM5 Model  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the1 - September 2006PhotovoltaicSeptember 22, 2014SocietyJ. Dudhia51 Posters755177331

375

Microsoft Word - WH-MM-767B NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

67B Title: Replace WH Brine Disposal System Header from MOV-51's to WHT-1415 Brine Tanks with HDPE Pipe Description: Subcontractor shall provide all labor, tools, materials,...

376

Microsoft Word - BC-MM-815 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

resources. Categorical Exclusion to be applied: B1.4 Installation or modification of air conditioning systems required for temperature control for operation of existing...

377

Microsoft Word - MM5_LSM_JGR.doc  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces andMappingENVIRONMENTALHYDROPOWERFebruarySave the October 30,74Impact of

378

Microsoft Word - BH-MM-1038 NEPA.docx  

Broader source: Energy.gov (indexed) [DOE]

38 Title: Recondition and Repair BHTX-14 Transformer Description: Subcontractor shall provide all labor, supervision, tools, equipment, and transportation required to remanufacture...

379

ANNUAL REPORT U.S. DEPARlMm OF COMMERCE  

E-Print Network [OSTI]

, or to this publication furnished by the NOAA Environmental Research Laboratories, in any advertising or sales an intent to cause directly or indirectly the advertised product to be used or purchased because and an understanding of the transport and dispersion of pollutants; surface waves and oscillations-critical to lake

380

Data:65aed576-0dd2-4878-ae9d-dd07d4589b76 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved fore6e8eee4495-afb210887c9b

Note: This page contains sample records for the topic "mm dd yy" 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.


381

Data:6c1ba52d-d942-40cb-b589-c25844dd9573 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approvedea02758d3f49fa2694 No revision hasd4ce025baf7c No72b65ec3 Nob0127d90

382

Data:761dd206-b302-48e5-84dd-4e1808070e4c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision has6dcc3af95b5a09e36f Nob9d5-01febf45da66

383

Data:1e1dba06-f5bd-4860-b42a-dd3781dd577e | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision5af6d400c2d No revisionb-80ce915ef62f No revision has

384

Data:B6dd2dd6-e825-4f99-ac5a-aa825ef1867c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2 No revision has38865d08 No revisionb6dbbdc091c4061e2fe19b No revision has been approved for this

385

Data:Ba8d22e9-7084-435c-a5dd-22b446a766dd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2 No revision has38865d08d442d74d244 No revision has been53122027 No revision hasaf671e4b7c No

386

Data:12cdff13-e018-4faa-bfe0-df0dd9cd82dd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 No revision has been approved for

387

Data:16179df3-1f99-4dd3-836a-dd8eeb2b9441 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 Nob97eb4d202d0 No revision has been approved for

388

HCFC1 is a common component of active human CpG-island promoters and coincides with ZNF143, THAP11, YY1, and GABP transcription factor occupancy  

E-Print Network [OSTI]

In human transcriptional regulation, DNA-sequence-specific factors can associate with intermediaries that orchestrate interactions with a diverse set of chromatin-modifying enzymes. One such intermediary is HCFC1 (also ...

JnBaptiste, Courtney Kenneil

389

Lochon Catalyzed D-D Fusion in Deuterated Palladium in the Solid State  

E-Print Network [OSTI]

Lochons (local charged bosons or local electron pairs) can form on D+ to give D- (bosonic ions) in Palladium Deuteride in the solid state. Such entities will occur at special sites or in linear channel owing to strong electron-phonon interaction or due to potential inversion on metallic electrodes. These lochons can catalyze D- - D+ fusion as a consequence of internal conversion leading to the formation of He-4 plus production of energy (Q=23.8 MeV) which is carried by the alpha particle and the ejected electron-pair. The reaction rate for this fusion process is calculated.

K. P. Sinha; A. Meulenberg

2007-05-04T23:59:59.000Z

390

DOE Presents Proposed D&D and Waste Disposition Plans for EM...  

Office of Environmental Management (EM)

community leaders, and workers attended a public meeting in November 2014 at a high school near the plant. Many of the attendees voiced their opinions on the preferred...

391

Public Can Comment on Proposed D&D and Waste Disposition Plans...  

Energy Savers [EERE]

community leaders, and workers attended the public meeting this month at a high school near the plant. Many of the attendees voiced their opinions on the preferred...

392

Initiating the D&D Project for the EBR-II  

SciTech Connect (OSTI)

A novel decommissioning project is underway to close the Experimental Breeder Reactor-II (EBR-II) fast reactor at the Idaho National Laboratory (INL), Materials and Fuels Complex (MFC) facility near Idaho Falls, ID. The facility was placed in cold shutdown in 1994 and work began on the removal of the metallic sodium coolant. The bulk of the sodium was drained and treated beginning in 2001. The residual sodium heel was chemically passivated to render it less reactive in 2005 using a novel carbon dioxide treatment. Approximately 700 kg of metallic sodium and 3500 kg of sodium bicarbonate remain in the facility. A RCRA Waste Treatment Permit, issued in 2002 by the State of Idaho Department of Environmental Quality, requires annual progress toward closure of the facility, and that all regulated materials be removed or deactivated, and the waste products removed by 2022. The baseline sodium removal technology would result in about 100,000 gallons of low-level waste solution requiring treatment along with separate handling of the large components (intermediate heat exchanger, rotating plug, etc) outside of the primary tank.

Rick Demmer

2010-08-01T23:59:59.000Z

393

Remote Manipulation of D&D Exhibiting Tele-Autonomy and Tele-Collaboration  

SciTech Connect (OSTI)

Teleoperation has found much application in today's society. While its benefits make it advantageous in many situations, teleoperation also introduces new challenges. In this paper, we present techniques to improve teleoperation performance by making better use of the human's inherent skills.

J. Edward Colgate; Thomas F. Ewing; Young S. Park; Michael A. Peshkin

2006-12-05T23:59:59.000Z

394

Demonstration of Fixatives to Control Contamination and Accelerate D&D  

Broader source: Energy.gov [DOE]

The 2000 Complex at the Oak Ridge National Laboratory (ORNL) has been identified as a high risk facility. The 50-year-old series of connected metal buildings has deteriorated to the point that it...

395

DDaanniieell BB.. SShhoorrtt,, PPhh..DD.. Email: short@rmu.edu  

E-Print Network [OSTI]

history of industrial pollution in the English Lake District was presented. Atmospheric fluxes were investigated using naturally occurring archives of pollution (lake sediments and peat bogs). Radioactive decay Environmental Science BS/BA advisor. Designed teaching and research laboratories for new building construction

Short, Daniel

396

Novel perfluoroalkylated derivatives of DD-galactopyranose and xylitol for biomedical uses. Hemocompatibility and effect on  

E-Print Network [OSTI]

of Chemistry of Natural Compounds, Institute of Chemical Technology Prague, Technicka 5, 166 28 Prague, Czech as biocompatible surfactants in the medical area1,2 displaying unique properties for the formulation of colloidal-galactose were synthesized by the one-step nucleophilic addition of protected carbohy- drates to perfluorinated

Cirkva, Vladimir

397

Report on D&D of Large Components with Valuable EM Contributions is Available on Powerpedia  

Broader source: Energy.gov [DOE]

WASHINGTON, D.C. EMs Office of Deactivation and Decommissioning/Facility Engineering (D&D/FE), representing DOE on the Nuclear Energy Agencys (NEA) Working Party on Decommissioning and Dismantling (WPDD) of the Radioactive Waste Management Committee, provided significant contributions to the recently published report titled, The Management of Large Components from Decommissioning to Storage and Disposal.

398

Table 3: Results of the Probability Based Heuristic Method for DD Reordering  

E-Print Network [OSTI]

1908:isc 13934 8762 78 c3540:isc 72858 43564 727 5xp1:pla 74 42 ! 1 9sym:pla 25 25 ! 1 alu4:pla 1197 567 3 bw:pla 108 101 ! 1 con1:pla 18 16 ! 1 duke2:pla 973 361 1 misex1:pla 41 37 ! 1 misex2:pla 136 96 ! 1 misex3:pla 1301 504 3 symmetry detection and decision diagram variable re­ ordering. Although some

Thornton, Mitchell

399

ALLEGATO 2 AL D.D. N. 481 DEL 20.06.2011 BANDO DI CONCORSO  

E-Print Network [OSTI]

INNOVATIVE PER L'INGEGNERIA DELL'INFORMAZIONE E COMUNICAZIONE E PER LA ROBOTICA Settore di Ingegneria in Tecnologie Innovative per l'Ingegneria dell'Informazione e Comunicazione e la Robotica- Settore di Ingegneria ai temi della microingegneria biomedica, della robotica biomimetica, delle tecnologie per la

Lipari, Giuseppe

400

A compact stilbene crystal neutron spectrometer for EAST D-D plasma neutron diagnostics  

SciTech Connect (OSTI)

A new compact stilbene crystal neutron spectrometer has been investigated and applied in the neutron emission spectroscopy on the EAST tokamak. A new components analysis method is presented to study the anisotropic light output in the stilbene crystal detector. A Geant4 code was developed to simulate the neutron responses in the spectrometer. Based on both the optimal light output function and the fitted pulse height resolution function, a reliable neutron response matrix was obtained by Geant4 simulations and validated by 2.5 MeV and 14 MeV neutron measurements at a 4.5 MV Van de Graaff accelerator. The spectrometer was used to diagnose the ion temperature in plasma discharges with lower hybrid wave injection and ion cyclotron resonance heating on the EAST tokamak.

Zhang Xing; Yuan Xi; Xie Xufei; Chen Zhongjing; Peng Xingyu; Chen Jinxiang; Zhang Guohui; Li Xiangqing; Fan Tieshuan [School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Chengfu Road 201, 100871 Beijing (China); Zhong Guoqiang; Hu Liqun; Wan Baonian [Institute of Plasma Physics, Chinese Academy of Sciences, PO Box 1126, 230031 Hefei, Anhui (China)

2013-03-15T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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

Public Comment Period for Portsmouth Site D&D and Waste Disposition...  

Office of Environmental Management (EM)

2014 8:00AM EST to March 11, 2015 5:00PM EDT Public Comment Period for the Process Buildings and Complex Facilities Decontamination and Decommissioning and Site-Wide Waste...

402

CLEARANCE OF BULK MATERIALS FROM D&D - LIFE AFTER THE NAS REPORT  

SciTech Connect (OSTI)

Lack of consistent free release standards for solid materials has been an issue that has been around for several decades. The Nuclear Regulatory Commission (NRC) has had specific and dose-based standards for the release of liquids and gases for several decades, but no regulatory mechanisms for the release of solid materials from a nuclear power plant. Even though free releases of small quantities of solid materials continue under existing guidelines from operating plants, the regulatory void creates major difficulties for the bulk materials that result from decommissioning projects. For the nation's fleet of nuclear reactors the cost of this regulatory void could be as high as $10 billion. The NRC has recently resumed the enhanced rulemaking process that was originally initiated in 1999 but was deferred pending a study by the National Academy of Sciences (NAS)/National Research Council. The NAS report and recommendations were issued in March 2002 and the NRC decided in October 2002 to resume the rulemaking process. This paper provides an overview of the developments in this area. It specifically discusses the applicability of ANSI N13.12 as a consensus standard that should be seriously considered for adoption as a regulatory standard.

Devgun, Jas S., Ph.D.

2003-02-27T23:59:59.000Z

403

Risk D&D Rapid Prototype: Scenario Documentation and Analysis Tool  

SciTech Connect (OSTI)

Report describes process and methodology associated with a rapid prototype tool for integrating project risk analysis and health & safety risk analysis for decontamination and decommissioning projects.

Unwin, Stephen D.; Seiple, Timothy E.

2009-05-28T23:59:59.000Z

404

PPrreeppaarreedd bbyy LLaarrrryy PP.. WWaallkkeerr,, PPhh..DD.. PPrrooffeessssoorr,, DDeeppaarrttmmeenntt ooff BBiioollooggiiccaall aanndd EEnnvviirroonnmmeennttaall EEnnggiinneeeerriinngg  

E-Print Network [OSTI]

, such the Renewable Fuels Standard that mandates the production of 16 billion gallons for cellulosic biofuel use by 2022. Such a rapid expansion in biofuels production will require large increases in feedstock a participant in a Regional Herbaceous Feedstock Production Trial, sponsored by the Sun Grant Initiative

Walter, M.Todd

405

E-Print Network 3.0 - anisotropic d-d fusion Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

F. Leipold1 Summary: and Fusion Center, Cambridge, MA 02139, USA Introduction Plasmas for thermonuclear fusion contain a highly... in the deuterium-tritium fusion reaction which is...

406

Data:3f661084-6107-4522-9923-7dd335dc7787 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has beend26-1acc36863a1d No revision has been approved for this page.

407

MODEL FOR AN ASSESSOR BIOGRAPHICAL SKETCH* Title + First Name + Middle Name + Last Name (printed by NIS)  

E-Print Network [OSTI]

Communications, Inc. centers. She has been the team leader at two facilities for implementation of ISO 9001 and professional development accomplishments. Rev. yyyy-mm-dd (use ISO standard calendar date format) * Use and ISO 14001 management systems and a team member for implementation at two other plants. The size

408

HealthPoint Employee Assistance Program Non-Employee Client Information  

E-Print Network [OSTI]

of birth (MM/DD/YYYY) Gender Male Female Home phone Work phone Cell phone E-mail Preferred methods to contact you Work phone Home phone Cell phone E-mail Ethnicity (optional) - check all that apply African 101 E. 27th Street, STOP A9200 Austin, TX 78712-1540 phone 512-471-3366 fax 512-475-8558 www

Yang, Zong-Liang

409

HealthPoint Employee Assistance Program Client Information  

E-Print Network [OSTI]

EID Date of birth (MM/DD/YYYY) Gender Male Female Home phone Work phone Cell phone E-mail Preferred methods to contact you Work phone Home phone Cell phone E-mail Ethnicity (optional) - check all that apply time. HealthPoint EAP Mail Code A9200 101 E. 27th Street, STOP A9200 Austin, TX 78712-1540 phone 512

Yang, Zong-Liang

410

HealthPoint Employee Assistance Program Manager Information  

E-Print Network [OSTI]

of birth (MM/DD/YYYY) Gender Male Female Home phone Work phone Cell phone E-mail Preferred methods to contact you Work phone Home phone Cell phone E-mail Ethnicity (optional) - check all that apply African Austin, TX 78712-1540 phone 512-471-3366 fax 512-475-8558 www.utexas.edu/hr/current/services/ Revised 5

Yang, Zong-Liang

411

NIF NOI 2009_E Page 1 of 6 Notice of Intent to Submit an Application  

E-Print Network [OSTI]

NIF NOI 2009_E Page 1 of 6 Notice of Intent to Submit an Application New Initiatives Fund (NIF Foundation for Innovation NIF NOI 2009_E Page 2 of 6 Date printed (dd/mm/yyyy): 27/06/2008 Canadian

Martin, Jeff

412

Single Atom Electron and Ion Sources and Their Applications  

E-Print Network [OSTI]

- energy electron point projection microscope, PPM) (37, 38) 1. (shadow microscopy) (shadow image-walled carbon nanotubes, SWNTs) (111) (pizeo-scanner) X- Y-Z (scanning tunneling microscope) 3. (a on the screen (mm) Intensity(Arb.Units) (c) (a) (b) Q FWHM P (a) (b)Dd sample holder detector-MCP #12;13 98

413

H-1B, O-1 & PR Beneficiary Information for all H-1B, O-1 & PR applications  

E-Print Network [OSTI]

diploma, transcripts, publications, marriage or birth certificates or letters of recommendation, Middle) 2. Other names used, including maiden names and any Anglicized names. 3. Date of birth (mm/dd/yyyy) 4. Gender 5. U.S. Social Security Number 6. Country of birth 7. Province of birth 8. Country

Scharer, John E.

414

Revised June 2013 This form can be used if you are: (Please check the appropriate box)  

E-Print Network [OSTI]

a certificate or diploma Changing to a new certificate or diploma Dropping a certificate or diploma * If you are declaring more than one certificate/diploma, please check all that apply on this form. CERTIFICATES Completed: Transfer Credit Hours: Staff Name: Staff Signature: Date: Student # Date of Birth DD/MM/YYYY Last

Northern British Columbia, University of

415

CSIR-CENTRE FOR CELLULAR AND MOLECULAR BIOLOGY Uppal Road, Habsiguda, Hyderabad 500 007 (India)  

E-Print Network [OSTI]

ii) Experience certificate, if any iii) All the original certificates/documents in support) Father Name: 3. Date of Birth: Age (dd/mm/yyyy): Place of birth: 4. Gender: 5. Marital Status: 6. Category: GENERAL/SC/ST/OBC (tick appropriate one) 7. Are you citizen of India by birth or domicle?: 8

Udgaonkar, Jayant B.

416

Registrar's Office 303-273-3200  

E-Print Network [OSTI]

: ___ ___ ___ -- ___ ___ -- ___ ___ ___ ___ Correct Date of Birth ­ If filling out this section: ORIGINAL OR NOTARIZED COPY OF BIRTH CERTIFICATE ­ If filling out this section: ORIGINAL OR NOTARIZED COPY OF BIRTH CERTIFICATE OR MEDICAL DOCUMENTATION OR PASSPORT Correct Date of Birth: __ __ / __ __ / __ __ __ __ (mm/dd/yyyy) Change or Correct Gender

417

1000 Asp Avenue, Room 127 OFFICE OF ADMISSIONS AND RECORDS  

E-Print Network [OSTI]

with marriage and birth certificates, as applicable, to verify your family relationship. If you are currently INFORMATION Last Name (Family or Surname) First Name Middle Name Birth Date MM/DD/YYYY Sooner ID# (if available) Country of Citizenship Country of Birth City of Birth Country of Legal Permanent Residence SEVIS

Oklahoma, University of

418

An Advanced Reader in Chinese Sociology-Anthropology  

E-Print Network [OSTI]

- ( # ) 3. 22.lt ^ M o mm 2b ? % %.- cm) $tmm?m&mm.? 33 3. 26. T y (# ) US i' ( ft ) j& * ( 1$ ) 4. 3. 3X $ ( fC ) 3^ ?N c m ) 4.5. mi- m ? 4. ll.ffi?L ^I*JittR? '^fe o 4. i2A... m ft -5L^ m '^^ sr P/M& a0r^ &?-tk$ 13*SSy0 ^ 4yy|^^0?rn xn A B%.%)&!?&&&&&, ss?i^^^(i &m^m&nPo ^^gi^m^, ^iTifcttiw 3 Eft, 5E5#*^O JiM^^ftffl, ^flMHi^^T ti?ft*@AKift?^&8i?#lfi?r&f Sia-^ Ifr %%&*:$ fi*:fc7&:#iftfrBA%fl?;feg, ^ Mm?&&, mijn...

Johnson, Wallace

1978-01-01T23:59:59.000Z

419

THE CM-, MM-, AND SUB-MM-WAVE SPECTRUM OF ALLYL ISOCYANIDE AND RADIOASTRONOMICAL OBSERVATIONS IN ORION KL AND THE SgrB2 LINE SURVEYS  

SciTech Connect (OSTI)

Organic isocyanides have an interesting astrochemistry and some of these molecules have been detected in the interstellar medium (ISM). However, rotational spectral data for this class of compounds are still scarce. We provide laboratory spectra of the four-carbon allyl isocyanide covering the full microwave region, thus allowing a potential astrophysical identification in the ISM. We assigned the rotational spectrum of the two cis (synperiplanar) and gauche (anticlinal) conformations of allyl isocyanide in the centimeter-wave region (4-18 GHz), resolved its {sup 14}N nuclear quadrupole coupling (NQC) hyperfine structure, and extended the measurements into the millimeter and submillimeter-wave (150-900 GHz) ranges for the title compound. Rotational constants for all the monosubstituted {sup 13}C and {sup 15}N isotopologues are additionally provided. Laboratory observations are supplemented with initial radioastronomical observations. Following analysis of an extensive dataset (>11000 rotational transitions), accurate ground-state molecular parameters are reported for the cis and gauche conformations of the molecule, including rotational constants, NQC parameters, and centrifugal distortion terms up to octic contributions. Molecular parameters have also been obtained for the two first excited states of the cis conformation, with a dataset of more than 3300 lines. The isotopic data allowed determining substitution and effective structures for the title compound. We did not detect allyl isocyanide either in the IRAM 30 m line survey of Orion KL or in the PRIMOS survey toward SgrB2. Nevertheless, we provided an upper limit to its column density in Orion KL.

Haykal, I.; Marguls, L.; Huet, T. R.; Motyienko, R. A. [Laboratoire de Physique des Lasers, Atomes, et Molcules, UMR CNRS 8523, Universit de Lille 1, F-59655 Villeneuve d'Ascq Cdex (France); cija, P.; Cocinero, E. J.; Basterretxea, F.; Fernndez, J. A.; Castao, F. [Departamento de Qumica Fsica, Facultad de Ciencia y Tecnologa, Universidad del Pas Vasco, Barrio Sarriena s/n, E-48940 Leioa (Spain); Lesarri, A. [Departamento de Qumica Fsica y Qumica Inorgnica, Facultad de Ciencias, Universidad de Valladolid, E-47011 Valladolid (Spain); Guillemin, J. C. [Institut des Sciences Chimiques de Rennes, Ecole Nationale Suprieure de Chimie de Rennes, CNRS, UMR 6226, Alle de Beaulieu, CS 50837, F-35708 Rennes Cedex 7 (France); Tercero, B.; Cernicharo, J., E-mail: laurent.margules@univ-lille1.fr [Centro de Astrobiologa (CSIC-INTA), Laboratory of Molecular Astrophysics, Department of Astrophysics, Ctra. De Ajalvir, km 4, E-28850 Torrejn de Ardoz, Madrid (Spain)

2013-11-10T23:59:59.000Z

420

MMPerformance MM JAZZ MM Conducting MA/MS Apply to the Department and to the University. See the Yellow "Notice to Graduate Applicants" Sheet for required materials.  

E-Print Network [OSTI]

and Oral Form All students must complete the Degree Audit Reporting System (DARS) and submit it the term before taking the Exit Exam. Submit DARS to the Music Graduate Studies Coordinator, Dr. Joel Bluestone

Note: This page contains sample records for the topic "mm dd yy" 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.


421

A MOLECULAR LINE SURVEY OF THE CARBON-RICH PROTOPLANETARY NEBULA AFGL 2688 IN THE 3 mm AND 1.3 mm WINDOWS  

SciTech Connect (OSTI)

We present a spectral line survey of the protoplanetary nebula (PPN) AFGL 2688 in the frequency ranges of 71-111 GHz, 157-160 GHz, and 218-267 GHz using the Arizona Radio Observatory 12 m telescope and the Heinrich Hertz Submillimeter Telescope. A total of 143 individual spectral features associated with 32 different molecular species and isotopologues were identified. The molecules C{sub 3}H, CH{sub 3}CN, H{sub 2}CO, H{sub 2}CS, and HCO{sup +} were detected for the first time in this object. By comparing the integrated line strengths of different transitions, we are able to determine the rotation temperatures, column densities, and fractional abundances of the detected molecules. The C, O, and N isotopic ratios in AFGL 2688 are compared with those in IRC+10216 and the Sun, and were found to be consistent with stellar nucleosynthesis theory. Through comparisons of molecular line strengths in asymptotic giant branch stars, PPNs, and planetary nebulae, we discuss the evolution in circumstellar chemistry in the late stages of evolution.

Zhang Yong; Kwok, Sun; Nakashima, Jun-ichi; Chau, Wayne [Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong (Hong Kong); Dinh-V-Trung, E-mail: zhangy96@hku.hk, E-mail: sunkwok@hku.hk, E-mail: junichi@hku.hk, E-mail: dvtrung@iop.vast.ac.vn [Institute of Physics, Vietnam Academy of Science and Technology, 10 DaoTan Street, BaDinh, Hanoi (Viet Nam)

2013-08-10T23:59:59.000Z

422

NdI dyLf da. 8005, df.df. Tddd AdySdj, dya>ddjT -560 080, ddTd ddTdfSd edddd AIdQdf  

E-Print Network [OSTI]

fy, vfHknku uohdj.k Hkkjrh; foKku vdkneh dh LFkkiuk lj lh oh jkeu }kjk 1934 esa gqbZ vkSj rHkh ls oV lkbal vlksfl,'ku }kjk izdkf'kr fd;k tkrk gS] Hkh vdkneh }kjk izcaf/kr dh tkrh gSA fiNys dbZ n'kdksa ls"Bk izkIr dj pqdh gSaA bl ekU;rk dh le;-le; ij dbZ ckj varjkZ"Vªh; vfHkdrkZvksa }kjk cuk, x, ekun.Mksa t

Dhingra, Narender K.

423

A U T R E R E G A R DD O S S I E R 11 septembre 1973.  

E-Print Network [OSTI]

% des suffrages exprims devant le candidat conservateur, Jorge Alessandri, et le reprsentant de la

Paris-Sud XI, Universit de

424

Automation of System Safety Analysis: Possibilities and Pitfalls Andrew Galloway, University of York, Heslington, York YO10 5DD UK  

E-Print Network [OSTI]

evolved to support safety analysis work (in this paper, we use the term "safety analysis" to encompass all, safety engineers may only achieve closure at the end of a system's working life, when it is possibleAutomation of System Safety Analysis: Possibilities and Pitfalls Andrew Galloway, University

Pumfrey, David

425

Measurement of the Time-Dependent CP Asymmetry of Partially Reconstructed B0 to D*+D*- Decays  

SciTech Connect (OSTI)

We present a new measurement of the time-dependent CP asymmetry of B{sup 0} {yields}D*{sup +}D*{sup -} decays using (471 {+-} 5) million B{bar B} pairs collected with the BABAR detector at the PEP-II B Factory at the SLAC National Accelerator Laboratory. Using the technique of partial reconstruction, we measure the time-dependent CP asymmetry parameters S = -0.34 {+-} 0.12 {+-} 0.05 and C = +0:15 {+-} 0.09 {+-} 0.04. Using the value for the CP-odd fraction R{perpendicular} = 0.158 {+-} 0.028 {+-} 0.006, previously measured by BABAR with fully reconstructed B{sup 0} {yields} D{sup *+}D{sup *-} events, we extract the CP-even components S{sub +} = -0.49 {+-} 0.18 {+-} 0.07 {+-} 0.04 and C{sub +} = +0.15 {+-} 0.09 {+-} 0.04. In each case, the first uncertainty is statistical and the second is systematic; the third uncertainty on S{sub +} is the contribution from the uncertainty on R{perpendicular}. The measured value of the CP-even component S{sub +} is consistent with the value of sin 2{beta} measured in b {yields} (c{bar c})s transitions, and with the Standard Model expectation of small penguin contributions.

Lees, J. P.

2012-08-13T23:59:59.000Z

426

"! #%$&'$)(1032465786)$9A@CB$DAE FHGPI Q'6@@3$D($D5RRS  

E-Print Network [OSTI]

~{'HEw|w'~¡Huti~uwd¥Q? ru|wti{wv¨`~ {uu~|`h¡w§w`iw±{i|`?i¢w¬iwRwwE¢b`'uH`¤Di¢Ei{miw{w¨u}¢w~E~}uD ¡ui

Nestorov, Svetlozar

427

UFC/UFR Sciences et Techniques Dpartement d'lectronique -2007/08 Point d'avancement Projet DD  

E-Print Network [OSTI]

mettre en oeuvre un système d'éclairage « grand public » (pouvant servir à l'installation luminaire de l par rapport au planning · Eclairage type spot « Dot It » (marque OSRAM). Disponible en grande surface

Jeanjean, Louis

428

The Chemical Hazards Assessments Prior to D&D of the Plutonium Finishing Plant Hanford Nuclear Reservation  

SciTech Connect (OSTI)

All Hanford facilities, including the Plutonium Finishing Plant (PFP) were evaluated for chemical hazards in 1997, 1998 and 2000. The hazard evaluation, known as the PFP Facility Vulnerability Assessment (FVA), was prompted when chemicals in Tank A-109 in the Plutonium Reclamation Facility (PRF) exploded in May 1997. Actions were undertaken to eliminate or reduce what were thought to be the worst hazards following that evaluation. In 2001, a new PFP team was organized to review the progress to date in reducing hazards and to reassess hazards that might still remain within the facility. This reassessment continued into 2002 and is referred to as the 2002 PFP Residual Chemical Hazards Reassessment (RCHR). This report explains the results of the 2001/2002 reassessment of the chemical hazards at PFP. This reassessment effort forms the basis of the RCHR. The RCHR relied on previous assessments as the starting point for the 2001/2002 evaluation and used ranking criteria very similar to previous efforts. The RCHR team was composed of professionals representing Industrial Hygiene, Chemical Engineering, Mechanical Engineering, Hazardous Materials Handling Specialists, Solid Waste Management Specialists and Environmental Specialists. All areas of concern that could be accessed were physically examined and photographed where possible. Information from processing records, facility drawings and documents, design engineers, process engineers and work packages were compiled. The PFP vessel inventory was examined and expanded where required. New items listed in the vessel inventory were investigated. All items investigated were ranked using the hazard ranking criteria developed. This information was put on data sheets and compiled in a database.

FITCH, L.R.; HOPKINS, A.M.

2003-01-01T23:59:59.000Z

429

Inverse relationship between salinity and n-alkane dD values in the mangrove Avicennia marina  

E-Print Network [OSTI]

ratios in lipids derived from mangroves have the potential to be used for paleohydrologic reconstructions incorporated in leaf waxes, and/or (iii) increased secretion of salty brine by leaves at high salinity ratios of mangrove lipid biomarkers can be developed as a paleosalinity indicator. They also imply

Sachs, Julian P.

430

SSuuppppoorrtt aa PPhhDD aatt oonnee ooff SSccoottllaanndd''ss lleeaaddiinngg UUnniivveerrssiittiieess The Energy Technology Partnership (ETP)  

E-Print Network [OSTI]

and a further 25 are available in 2011. These are across a range of areas, including; wind; marine; solar; bio-energy and a further 25 are available in 2011. These are across a range of areas, including; wind; marine; solar; bio-energy UUnniivveerrssiittiieess The Energy Technology Partnership (ETP) is an alliance of Scottish Universities engaged in world

Strathclyde, University of

431

Pulsed DD Neutron Generator Measurements for HEU Oxide Fuel Pins Using Liquid Scintillators with Pulse Shape Discrimination  

E-Print Network [OSTI]

measurements have been performed on high-enriched uranium (HEU) oxide fuel pins and depleted uranium metal

Pennycook, Steve

432

Data:Ef303637-53dd-4066-a4bc-3bc9294274b7 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1ccEeae2669-ec94-4cc4-bbae-0108084310cc Nobeedba3b42c No revision has been approved for this

433

Data:F741842e-8820-4383-9865-11dd3bc7012d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved for this page.b4-a4ba-cd54152b8724 No revisione3fc05525fd2 No7ecf396c026b No

434

Data:F8229eec-f0ec-483a-9091-dd160a194dfc | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has been approved for this page.b4-a4ba-cd54152b8724 Noc6b7edf0a23ae9774adcb-ab7e-cc59b1d3a531

435

Data:663995dd-d34d-4335-b8bd-538564d23ea0 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved fore6e8eee4495-afb210887c9bf3ac6ed3cc6f836fd42ce63791b259cf

436

Data:6fbb7966-0826-4faf-8ac7-dc957086dd38 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has beenb-ff986065de63 No revision9-abd1-c3e1b33869bc8645d3b33ee No revision

437

Data:7160826e-dd5f-4852-9597-710ef492b817 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has beenb-ff986065de63cfd4f0-e47e-4d0c-bf46-09878b282c9064de77e8a1a1c75a8f13657eef492b817

438

Data:728dd673-63f7-4836-86b5-9499adad5931 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision has been approved for-e7599dcd5a17 No revision

439

Data:76a13e5d-6dd4-4662-8216-dc66b8761472 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision8390-f3c1d17c852d No revision has been approved for this

440

Data:7718928a-741b-4dd6-b746-154f0ac11312 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision8390-f3c1d17c852d Nof0ac11312 No revision has been approved for

Note: This page contains sample records for the topic "mm dd yy" 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.


441

Data:77dd6abf-99cf-415b-9cea-4541ea1bccf5 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has6a0216321b No revision8390-f3c1d17c852df4287f69e308 No revision

442

Data:1d2012db-460c-406a-9dd1-ac121fa0965c | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision5af6d400c2d No revision has been-9b29bec4d26e No revision has been1fa0965c No revision

443

Data:24137d13-52ca-4344-9879-9aed569dd62d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision5af6d400c2d4-4797-b850-d42be48a30cf No revisionf-e4d20400b3b9687d635a8 No revision

444

Data:26d218aa-3411-4513-8e61-dd945f8a9791 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 Noc7e1a8ffe No revision has been approved fordec-411fce1605ac Nodd945f8a9791 No revision has been

445

Data:2a37681e-f5dd-4fcc-8752-abc9b912fbac | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 Noc7e1a8ffe No revision has beena2ac591a5e3 Nobcf-1b589b1c9a42 Noa9c4572a Noabc9b912fbac No

446

Data:C251fa67-9544-43dd-8774-478976beffc5 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742 No revision has beena032db6d83 No revisionf87c65d6be13a3e1faa No revision

447

Data:5ddafa23-377a-4dd5-a8cf-2e8851449029 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved for this page. It1f847bdc66 No

448

Data:5ea371f2-7571-40f3-94ea-dd3497056727 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved for this page.f9b87a5 No revision has been approved

449

Data:64870dd2-bf18-4934-b2fe-04311ededd14 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revision has been approved fore6e8eee44 Nobfa2-747e1ee9f93d No revision3-834441124f9c

450

Data:040d6974-0fca-4caa-88ef-1a570dd45919 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable Solutions LLCd32fc5a84 Noade9-f289aea29999 No revision

451

Data:04763027-dea5-434f-aea0-ced2aa932dd4 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable Solutions LLCd32fc5a8420a0c118b388 No revision has been

452

Data:422bd1dd-77bc-4623-9720-85294b12010d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has beend26-1acc36863a1df4498ed9aae No revision has2010d No revision has

453

Data:42e7a416-d7ef-49c0-8052-172981434dd3 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has beend26-1acc36863a1df4498ed9aae Nobbe81d2e60ba829f4e Noe69edb6a695f

454

Data:433362fc-dd42-4420-83ad-3612a28b99eb | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revision has beend26-1acc36863a1df4498ed9aae6b1ccc67 No49487c85d Nof69b4ddaf8b9515

455

Data:4821e8dd-e044-4eab-9936-f2dfd1698153 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revisione66e17fc7f7 Nofa3d068c3333 No revision has6-f2dfd1698153 No revision has been

456

Data:491c73f1-ddce-4570-83dd-0e85759011b8 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3a87dcc95b No revisione66e17fc7f7 Nofa3d068c3333 No78eaa3f7

457

Data:0b88faa8-7bcc-4654-baf2-69691d0454dd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable-1a29da98863b No revision hasd22b56e08c283c4ccd9d8074c6af6600fd5a3e7

458

Data:0d33d6a5-5339-46dd-96cb-139092549af0 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable-1a29da98863bcec555c-6237-4cd1-931a-4d87b7a8618b3a12 No revision

459

Data:114520d4-26dd-4665-b70a-5a5841caea01 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has been approved for720c8ec90dba Noc8-52ffe80cce2e Noc4899237d23dc2437f4 No

460

Data:12161c8c-37ac-4aef-9801-dfbb928dd419 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has been approvedffcd81-3241-484a-b7b3-bac27985d9fd No revision has been

Note: This page contains sample records for the topic "mm dd yy" 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

Data:1494dd51-0213-4adb-9027-e475207b66b7 | Open Energy Information  

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371 No revision78ced93e0 No revision has beenef136e5ab03e475207b66b7 No

462

Data:19d06049-dd1b-4b49-8bed-232300791a06 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of48d9ff47edf3 No revision has beenba5b1d371fdc-b6c0-9cd6b0d70ef9b4eb15e81c7a49c4c690071 No300791a06 No revision

463

Data:Aaedcabd-e823-469d-8442-2de2dd396b69 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186Aade79ec-8628-4e5e-a921-24d1b399e432 No revision has been approved for this page. It

464

Data:9242fe81-bdec-4dd5-9817-d38bacc7f59d | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No revision has been040c1bfd8d

465

Data:938d4865-feda-4683-809f-cd56b41dd597 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No revision hascbfc79d6989fbb28142c454 No revision

466

Data:9576c0dd-6d4a-40af-8560-125902234c79 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf35248292f1 No789501c8a3b5 No revisione3c83837b69 No4ddca7bc8c20d2d327b2b2d04d

467

Data:Ccb31222-37dd-4600-909c-976cea30c527 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onb5-dcc1fcffd1f2bb71-d4159a938742e80b26cc4 No revision has been930896a NoCcac6ff8-58ed-4e49-bca6-b71c70a960ec Nocea30c527

468

Data:Cce77243-dd33-4763-aeb7-be03857267a6 | Open Energy Information  

Open Energy Info (EERE)

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469

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470

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Pagec-01b596aa1744b55997c1cc No revision has been approvedfcfd-fe97-4342-8248-2959f3ac61fa9a-a9ec6b91021dce483dfd0

471

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472

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AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office695810186 No revisione0a2d50bdf No revision has been approved for this page. It ise23ca5646aadc-727d8479d452 No

473

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475

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480

Measurement of CP Content and Time-Dependent CP Violation in B0 --> D*+D*- Decays  

SciTech Connect (OSTI)

This dissertation presents the measurement of the Cp-odd fraction and time-dependent CP violation parameters for the B{sup 0} {yields} D*{sup +} D*{sup -} decay. These results are based on the full BABAR dataset of (467 {+-} 5) x 10{sup 6} B{bar B} pairs collected at the PEP-II B Factory at the Stanford Linear Accelerator Center. An angular analysis finds that the CP-odd fraction of the B{sup 0} {yields} D*{sup +} D*{sup -} decay is R{sub {perpendicular}} = 0.158 {+-} 0.028 {+-} 0.006, where the first uncertainty is statistical, and the second is systematic. A fit to the flavor-tagged, time-dependent, angular decay rate yields C{sub +} = 0.02 {+-} 0.12 {+-} 0.02; C{sub {perpendicular}} = 0.41 {+-} 0.50 {+-} 0.08; S{sub +} = -0.76 {+-} 0.16 {+-} 0.04; S{sub {perpendicular}} = -1.81 {+-} 0.71 {+-} 0.16, for the CP-odd ({perpendicular}) and CP-even (+) contributions. Constraining these two contributions to be the same results in C = 0.047 {+-} 0.091 {+-} 0.019; S = -0.71 {+-} 0.16 {+-} 0.03. These measurements are consistent with the Standard Model and with measurements of sin2{beta} from B{sup 0} {yields} (c{bar c})K{sup 0} decays.

Anderson, Jacob M.; /SLAC; ,

2009-01-05T23:59:59.000Z

Note: This page contains sample records for the topic "mm dd yy" 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.


481

Oct. 12, 2005 QM/MM: What have we learned, where are we, and where  

E-Print Network [OSTI]

and electric embedding are contrasted. We consider methods applicable to gas-phase organic chemistry, liquid to computational chemists. At the same time, there is increasing interest in nanostructured materials, condensed advances in modeling potential energy surfaces, in statistical mechanical sampling, and in dynamics

Truhlar, Donald G

482

MM@MMaking Maths at Manchester General Course Information for the 2013 event.  

E-Print Network [OSTI]

walk away from the Alan Turing (Mathematics) building. Students will have their own room, with working minutes. There is a multi-storey car park next door to the Alan Turing building. A map and detailed

Glendinning, Paul

483

Ferrite-Cored Solenoidal Induction Coil Sensor for BUD (MM-1667)  

E-Print Network [OSTI]

following observations: 1) A ferrite-cored solenoidal coilthe same order as L. 2) A ferrite-cored solenoidal coil canstable response. 4) Feedback ferrite-cored solenoidal coils

Morrison, F.

2012-01-01T23:59:59.000Z

484

Ferrite-Cored Solenoidal Induction Coil Sensor for BUD (MM-1667)  

SciTech Connect (OSTI)

We have designed and lab tested a new ferrite cored induction coil sensor for measuring the secondary fields from metallic UXO with the BUD system. The objective was to replace the 5-inch diameter air-cored coils in the BUD system with smaller sensors that would allow the placement of multiple sensors in the smaller package of the new BUD hand-held system. A ferrite-cored solenoidal coil of length L can easily be made to have sensitivity and noise level roughly the same as an air-cored coil of a diameter on the same order as L. A ferrite-cored solenoidal coil can easily have a feedback configuration to achieve critical damping. The feedback configuration leads to a very stable response. Feedback ferrite-cored solenoidal coils show very little interaction as long as they are separated by one half their length.

Morrison, F.; Becker, A.; Conti, U.; Gasperikova, E.

2011-06-15T23:59:59.000Z

485

Evaluation of 5 mm-thick CdTe Detectors from the Company Acrorad  

E-Print Network [OSTI]

Using 2.0 cm x 2.0 cm x 0.5 cm Cadmium Telluride (CdTe) substrates from the company Acrorad, we have fabricated detectors with planar cathode contacts and 8x8 anode pixels. We investigate the I-V characteristics and energy resolution of the detectors for different contact materials and surface treatments. After biasing the detectors for a certain period of time, the dark currents increase dramatically. Out studies show that the time before breakdown decreases for higher detector temperatures and higher applied bias voltages. We obtained the best results with a Pt cathode and In anode pixels when we heat the detector to 90 C for 30 minutes prior to depositing the In contacts. Flood-illuminating the detector with 662 keV X-rays, we measured the pulse length distribution and derived an electron mobility of ~860 cm^(2)/V/s. We show that the energy resolution can be improved by correcting the anode signals for the depth of the primary interaction. Operated at -40 C and cathode bias of -500 V, the best pixels of the best detector achieved full width half maximum (FWHM) energy resolutions of 8 keV (6.4%) and 23 keV (3.4%) at 122 keV and 662 keV, respectively.

A. B. Garson III; I. V. Jung; J. Perkins; H. Krawczynski

2005-11-18T23:59:59.000Z

486

Particle Image Velocimetry Measurements and Analysis of Bypass Data for a Scaled 6mm Gap  

SciTech Connect (OSTI)

The purpose of the fluid dynamics experiments in the MIR (Matched Index of-Refraction) flow system at Idaho National Laboratory (INL) is to develop benchmark databases for the assessment of Computational Fluid Dynamics (CFD) solutions of the momentum equations, scalar mixing, and turbulence models for the flow ratios between coolant channels and bypass gaps in the interstitial regions of typical prismatic standard fuel element (SFE) or upper reflector block geometries of typical Modular High-temperature Gas-cooled Reactors (MHTGR) in the limiting case of negligible buoyancy and constant fluid properties. The experiments will use optical techniques, primarily particle image velocimetry (PIV) in the INL Matched Index of Refraction (MIR) flow system.

J.R. Wolf; T.E. Conder; R.R. Schultz

2012-09-01T23:59:59.000Z

487

Universit`a degli Studi di Padova Facolt`a di Scienze MM.FF.NN.  

E-Print Network [OSTI]

Bennet [4], hanno studiato la stabilit`a lineare tramite la teoria di Floquet, Alfriend [1], ha ottenuto stessi risultati dei lavori di Danby e Bennet, ma fornisce una giustificazione pi`u chiara delle

Fassò, Francesco

488

Exploring the Multidimensional Free Energy Surface of Phosphoester Hydrolysis with Constrained QM/MM Dynamics  

E-Print Network [OSTI]

Exploring the Multidimensional Free Energy Surface of Phosphoester Hydrolysis with Constrained QM water. Detailed free energy landscapes in two-dimensional and three-dimensional space were resolved that was demonstrated to be powerful for free energy calculations along multiple coordinates. As in previous theoretical

Gerwert, Klaus

489

ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength  

E-Print Network [OSTI]

The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research. By studying stellar chromospheres one aims at identifying the relevant physical processes. Defining the permittable extent of the parameter space can also serve as a template for the Sun-as-a-star. Earlier observations with Herschel and APEX have revealed the temperature minimum of alpha Cen, but these were unable to spatially resolve the binary into individual components. With the data reported here, we aim at remedying this shortcoming. Furthermore, these earlier data were limited to the wavelength region between 100 and 870mu. In the present context, we intend to extend the spectral mapping to longer wavelengths, where the contrast between stellar photospheric and chromospheric emission becomes increasingly evident. ALMA is particularly suited to point sources, such as unresolved stars. ALMA provides the means to achieve our obj...

Liseau, R; Bayo, A; Bertone, E; Black, J H; del Burgo, C; Chavez, M; Danchi, W; De la Luz, V; Eiroa, C; Ertel, S; Fridlund, M C W; Justtanont, K; Krivov, A; Marshall, J P; Mora, A; Montesinos, B; Nyman, L -A; Olofsson, G; Sanz-Forcada, J; Thebault, P; White, G J

2014-01-01T23:59:59.000Z

490

Sub-mm and X-ray background: two unrelated phenomena?  

E-Print Network [OSTI]

Obscured AGNs are thought to contribute a large fraction of the hard X-ray background (2-10 keV), and have also been proposed as the powerhouse of a fraction of the SCUBA sources which make most of the background at 850um, thus providing a link between the two spectral windows. We have tackled this issue by comparing data at 2-10 keV and at 850um for a sample of 34 sources at fluxes (or limiting fluxes) which resolve most of the background in the two bands. We present here new SCUBA observations, and new correlations between separate data sets retrieved from the literature. Similar correlations presented by others are added for completeness. None of the 11 hard X-ray (2-10 keV) sources has a counterpart at 850um, with the exception of a Chandra source in the SSA13 field, which is a candidate type 2, heavily absorbed QSO at high redshift. The ratios F(850um)/F(5keV) (mostly upper limits) of the X-ray sources are significantly lower than the value observed for the cosmic background. In particular, we obtain that 2-10 keV sources brighter than 10^-15 erg s^-1 cm^-2, which make at least 75% of the background in this band, contribute for less than 7% to the submillimeter background. Out of the 24 SCUBA sources, 23 are undetected by Chandra. The ratios F(850um)/F(5keV) (mostly lower limits) of these SCUBA sources indicate that most of them must be powered either by starburst activity, or by an AGN which is obscured by a column Nh > 10^25 cm^-2, with a reflection efficiency in the hard X rays significantly lower than 1% in most cases. However, AGNs of this type could not contribute significantly to the 2-10 keV background.

P. Severgnini; R. Maiolino; M. Salvati; D. Axon; A. Cimatti; F. Fiore; R. Gilli; F. La Franca; A. Marconi; G. Matt; G. Risaliti; C. Vignali

2000-06-16T23:59:59.000Z

491

Sub-mm and X-ray background two unrelated phenomena?  

E-Print Network [OSTI]

Obscured AGNs are thought to contribute a large fraction of the hard X-ray background (2-10 keV), and have also been proposed as the powerhouse of a fraction of the SCUBA sources which make most of the background at 850um, thus providing a link between the two spectral windows. We have tackled this issue by comparing data at 2-10 keV and at 850um for a sample of 34 sources at fluxes (or limiting fluxes) which resolve most of the background in the two bands. We present here new SCUBA observations, and new correlations between separate data sets retrieved from the literature. Similar correlations presented by others are added for completeness. None of the 11 hard X-ray (2-10 keV) sources has a counterpart at 850um, with the exception of a Chandra source in the SSA13 field, which is a candidate type 2, heavily absorbed QSO at high redshift. The ratios F(850um)/F(5keV) (mostly upper limits) of the X-ray sources are significantly lower than the value observed for the cosmic background. In particular, we obtain tha...

Severgnini, P; Salvati, M; Axon, D J; Cimatti, A; Fiore, F; Gilli, R; La Franca, F; Marconi, A; Matt, G; Risaliti, G; Vignali, C

2000-01-01T23:59:59.000Z

492

ISOLTRAP mass measurements of exotic nuclides at m/m = 10-8 , G. Bollend  

E-Print Network [OSTI]

. ISOLTRAP has so far been used to measure the masses of close to 300 radionuclides across the chart of nuclides, which are included in the recent Atomic-Mass Evaluation (AME2003) [5], with the exception

Paris-Sud XI, Université de

493

MM-wave cyclotron auto-resonance maser for plasma heating  

SciTech Connect (OSTI)

Heating and Current Drive systems are of outstanding relevance in fusion plasmas, magnetically confined in tokamak devices, as they provide the tools to reach, sustain and control burning conditions. Heating systems based on the electron cyclotron resonance (ECRH) have been extensively exploited on past and present machines DEMO, and the future reactor will require high frequencies. Therefore, high power (?1MW) RF sources with output frequency in the 200 - 300 GHz range would be necessary. A promising source is the so called Cyclotron Auto-Resonance Maser (CARM). Preliminary results of the conceptual design of a CARM device for plasma heating, carried out at ENEA-Frascati will be presented together with the planned R and D development.

Ceccuzzi, S.; Ravera, G. L.; Tuccillo, A. A. [Associazione Euratom-ENEA sulla Fusione, C.R. Frascati, Via Enrico Fermi 45, 00044, Frascati, Roma (Italy); Dattoli, G.; Di Palma, E.; Doria, A.; Gallerano, G. P.; Giovenale, E.; Spassovsky, I.; Surrenti, V. [ENEA UTAPRAD, C.R. Frascati, Via Enrico Fermi 45, 00044, Frascati, Roma (Italy); Mirizzi, F. [Consorzio CREATE, Via Claudio 21, 80125, Napoli (Italy)

2014-02-12T23:59:59.000Z

494

Vibrational Spectra of Water Solutions of Azoles from QM/MM Calculations: Effects of Solvation  

E-Print Network [OSTI]

) and solution conditions can successfully indicate the role of the solvent in determining the structural

Guidoni, Leonardo

495

Pseudobond parameters for QM/MM studies involving nucleosides, nucleotides, and their analogs  

SciTech Connect (OSTI)

In biological systems involving nucleosides, nucleotides, or their respective analogs, the ribose sugar moiety is the most common reaction site, for example, during DNA replication and repair. How- ever, nucleic bases, which comprise a sizable portion of nucleotide molecules, are usually unreactive during such processes. In quantum mechanical/molecular simulations of nucleic acid reactivity, it may therefore be advantageous to describe specific ribosyl or ribosyl phosphate groups quantum me- chanically and their respective nucleic bases with a molecular mechanics potential function. Here, we have extended the pseudobond approach to enable quantum mechanical/molecular mechanical simulations involving nucleotides, nucleosides, and their analogs in which the interface between the two subsystems is located between the sugar and the base, namely, the C(sp3) N(sp2) bond. The pseudobond parameters were optimized on a training set of 10 molecules representing several nu- cleotide and nucleoside bases and analogs, and they were then tested on a larger test set of 20 diverse molecules. Particular emphasis was placed on providing accurate geometries and electrostatic prop- erties, including electrostatic potential, natural bond orbital (NBO) and atoms in molecules (AIM) charges and AIM first moments. We also tested the optimized parameters on five nucleotide and nu- cleoside analogues of pharmaceutical relevance and a small polypeptide (triglycine). Accuracy was maintained for these systems, which highlights the generality and transferability of the pseudobond approach. 2013 American Institute of Physics. [http://dx.doi.org/10.1063/1.4772182

Chaudret, Robin [Duke University, North Carolina] [Duke University, North Carolina; Parks, Jerry M [ORNL] [ORNL; Yang, Weitao [Duke University, North Carolina] [Duke University, North Carolina

2013-01-01T23:59:59.000Z

496

This article was downloaded by: [MM Ali] On: 04 January 2012, At: 17:55  

E-Print Network [OSTI]

, 37-41 Mortimer Street, London W1T 3JH, UK Remote Sensing Letters Publication details, including of satellite-derived tropical cyclone heat potential with in situ observations in the North Indian Ocean, National Remote Sensing Centre, ISRO, Hyderabad, Andhra Pradesh, India b Atlantic Oceanographic

497

Assessing the Performance of 5mm White LED Light Sources for Developing-Country Applications  

E-Print Network [OSTI]

performance variations. Incandescent and fluorescent lightbetter than the common incandescent lamp. Off-grid lighting

Mills, Evan

2007-01-01T23:59:59.000Z

498

Powering mm-Size Wireless Implants for Brain-Machine Interfaces  

E-Print Network [OSTI]

applica- tions include bio-fuel cells utilizing glucose frombatteries [Roundy04] Glucose bio-fuel cell utilizing glucose

Mark, Michael

2011-01-01T23:59:59.000Z

499

Injection-locked composite lasers for mm-wave modulation : LDRD 117819 final report.  

SciTech Connect (OSTI)

This report summarizes a 3-year LDRD program at Sandia National Laboratories exploring mutual injection locking of composite-cavity lasers for enhanced modulation responses. The program focused on developing a fundamental understanding of the frequency enhancement previously demonstrated for optically injection locked lasers. This was then applied to the development of a theoretical description of strongly coupled laser microsystems. This understanding was validated experimentally with a novel 'photonic lab bench on a chip'.

Wendt, Joel Robert; Vawter, Gregory Allen; Raring, James; Tauke-Pedretti, Anna; Alford, Charles Fred (Sandia Staffing Alliance, LLC, Albuquerque, NM); Skogen, Erik J.; Chow, Weng Wah; Cajas, Florante G. (LMATA Government Services, LLC, Albuquerque, NM); Overberg, Mark E.; Torres, David L. (LMATA Government Services, LLC, Albuquerque, NM); Peake, Gregory Merwin

2010-09-01T23:59:59.000Z

500

MM-ulator: Towards a Common Evaluation Platform for Mixed Mode Environments  

E-Print Network [OSTI]

; Venice, Italy, Proceedings), pp.42-52, published by Springer (LNAI 5325) Abstract. We investigate interfaces, energy resources, sensor data). The scenarios addressed within MMEs may vary from monitor- ing

Stryk, Oskar von