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1

City of West Liberty, Iowa (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Liberty Liberty Place Iowa Utility Id 20380 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes Operates Generating Plant Yes Activity Generation Yes Activity Transmission Yes Activity Buying Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Commercial Consumers Commercial Large Industrial Customers Industrial Power Consumers Commercial Residential Customers Residential Security Lights Lighting Telephone Booths (Unmetered) Commercial Average Rates Residential: $0.0927/kWh Commercial: $0.0810/kWh Industrial: $0.0769/kWh

2

Solar Liberty | Open Energy Information  

Open Energy Info (EERE)

You can help OpenEI by expanding it. Solar Liberty is a company located in Buffalo, New York . References "Solar Liberty" Retrieved from "http:en.openei.orgw...

3

Liberty Utilities (Electric) - Commercial New Construction Rebate...  

Open Energy Info (EERE)

Service Department Liberty Utilities Address PO Box 960 Place Northborough, Massachusetts ZipPostal Code 1532-0960 Phone (800) 375-7413 Website http:liberty-utilities.comeast...

4

Liberty Utilities (Electric) Commercial New Construction Rebate Program (New Hampshire)  

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

'''Liberty Utilities has assumed National Grid's customers base in the state of New Hampshire. Customers should contact Liberty Utilities for questions regarding incentive availability.'''

5

Federal Energy Management Program: Case Study - Statue of Liberty...  

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

Statue of Liberty National Monument to someone by E-mail Share Federal Energy Management Program: Case Study - Statue of Liberty National Monument on Facebook Tweet about Federal...

6

Liberty Utilities (Gas) - Commercial Energy Efficiency Programs |  

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

Liberty Utilities (Gas) - Commercial Energy Efficiency Programs Liberty Utilities (Gas) - Commercial Energy Efficiency Programs Liberty Utilities (Gas) - Commercial Energy Efficiency Programs < Back Eligibility Commercial Industrial Institutional Local Government Schools State Government Savings Category Heating & Cooling Commercial Heating & Cooling Heating Home Weatherization Commercial Weatherization Other Construction Manufacturing Appliances & Electronics Water Heating Windows, Doors, & Skylights Maximum Rebate Custom Projects: $100,000 (existing facilities); $250,000 (new construction) Energy Efficiency Engineering Study: $10,000 Steam Traps: $2500 Programmable Thermostats: up to five units Boiler Reset Controls: up to two units Program Info State New Hampshire Program Type Utility Rebate Program Rebate Amount

7

Liberty Utilities (Electric) - Residential Energy Efficiency Rebate  

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

Liberty Utilities (Electric) - Residential Energy Efficiency Rebate Liberty Utilities (Electric) - Residential Energy Efficiency Rebate Programs Liberty Utilities (Electric) - Residential Energy Efficiency Rebate Programs < Back Eligibility Construction Low-Income Residential Residential Savings Category Home Weatherization Commercial Weatherization Appliances & Electronics Heating & Cooling Construction Commercial Heating & Cooling Design & Remodeling Other Sealing Your Home Ventilation Commercial Lighting Lighting Maximum Rebate Home Performance with ENERGY STAR®: $4000 Program Info Funding Source NH Saves State New Hampshire Program Type Utility Rebate Program Rebate Amount Home Performance with ENERGY STAR®: up to $4,000 for improvements ENERGY STAR® Homes Qualification: custom incentives and technical support

8

Liberty Utilities (Electric) - Commercial Energy Efficiency Incentive  

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

Liberty Utilities (Electric) - Commercial Energy Efficiency Liberty Utilities (Electric) - Commercial Energy Efficiency Incentive Programs Liberty Utilities (Electric) - Commercial Energy Efficiency Incentive Programs < Back Eligibility Commercial Industrial Local Government Schools Savings Category Heating & Cooling Commercial Heating & Cooling Heating Cooling Manufacturing Other Construction Heat Pumps Appliances & Electronics Commercial Lighting Lighting Maximum Rebate Custom Incentives: amount that buys down the cost of the project to a 1 year simple payback Program Info State New Hampshire Program Type Utility Rebate Program Rebate Amount Custom Retrofits and Engineering Studies: 50% of project cost Fluorescent Lighting: $10-$50 High Bay: $70 or $100 (retrofit) Metal Halide: $50 or $70 LED Exit Signs: $12 LED Traffic Signals: $50

9

Liberty Power Corp. (New York) | Open Energy Information  

Open Energy Info (EERE)

Liberty Power Corp. (New York) Jump to: navigation, search Name Liberty Power Corp. Place New York Utility Id 55781 References EIA Form EIA-861 Final Data File for 2010 -...

10

Liberty Power Corp. | Open Energy Information  

Open Energy Info (EERE)

Corp. Corp. (Redirected from Liberty Power) Jump to: navigation, search Name Liberty Power Corp. Place Florida Utility Id 55781 Utility Location Yes Ownership R ISO CA Yes ISO Ercot Yes RTO PJM Yes ISO NY Yes ISO MISO Yes ISO NE Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates No Rates Available References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=Liberty_Power_Corp.&oldid=410985" Categories: EIA Utility Companies and Aliases

11

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

Office of Legacy Management (LM)

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

12

Case Study - Statue of Liberty National Monument | Department of Energy  

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

Statue of Liberty National Monument Statue of Liberty National Monument Case Study - Statue of Liberty National Monument October 7, 2013 - 1:58pm Addthis Overview This energy savings performance contract (ESPC) focuses on improvements to the infrastructure, with the addition of energy-efficient lighting, variable-speed drives, and installation of energy management control systems. The contractor, CES/Way, is investing $1 million, and the utility, Public Service Electric & Gas Company, will provide a rebate of $1.3 million. The potential energy savings resulting from this project are about 4 Billion Btu per year, about 75 percent of which will come from Ellis Island. Background Ellis Island and the nearby Liberty Island, site of the venerable Statue of Liberty, together form the Statue of Liberty National Monument. Ellis

13

Liberty Green Renewables LLC | Open Energy Information  

Open Energy Info (EERE)

Renewables LLC Renewables LLC Jump to: navigation, search Name Liberty Green Renewables, LLC Place Georgetown, Indiana Zip 47122 Sector Biomass Product Biomass power plant developer with offices in southern Indiana and Houston, Texas. Coordinates 6.80461°, -58.154831° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":6.80461,"lon":-58.154831,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

14

Type Ia Supernovae Project at NERSC  

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

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

15

UMore Ph IA CR Report 7-8-10.pdf  

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

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

16

City of Liberty, Texas (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Liberty Liberty Place Texas Utility Id 10982 Utility Location Yes Ownership M NERC Location SERC NERC SERC Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Commercial Service Rates Commercial Large Commercial Commercial Residential service Residential Average Rates Residential: $0.1070/kWh Commercial: $0.1120/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=City_of_Liberty,_Texas_(Utility_Company)&oldid=409862" Categories: EIA Utility Companies and Aliases

17

Category:Mason, IA | Open Energy Information  

Open Energy Info (EERE)

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

18

North Liberty, Indiana: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Liberty, Indiana: Energy Resources Liberty, Indiana: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.5342125°, -86.427234° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.5342125,"lon":-86.427234,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

19

Liberty County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Liberty County, Texas: Energy Resources Liberty County, Texas: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 30.1633593°, -94.8105955° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.1633593,"lon":-94.8105955,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

20

Liberty Turbine Test Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Turbine Test Wind Farm Turbine Test Wind Farm Jump to: navigation, search Name Liberty Turbine Test Wind Farm Facility Liberty Turbine Test Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Developer Clipper Windpower Energy Purchaser Platte River Power Authority Location Near Medicine Bow WY Coordinates 41.96251°, -106.415918° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.96251,"lon":-106.415918,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

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


21

McCullough to Liberty fiber optics project  

SciTech Connect

The US Department of Energy, Western Area Power Administration (Western) proposes to replace an existing overhead static wire with a shield wire that contains optical fibers (OPGW) on transmission lines from McCullough Substation, south of Las Vegas, Nevada, to Liberty Substation near Phoenix, Arizona. The replacement will occur on the McCullough-Davis, Davis-Parker No. 2, and Parker-Liberty No. 1 230-kV transmission lines. Western is responsible for the operation and maintenance of the lines. Western prepared an Environmental Assessment (EA) entitled ``McCullough to Liberty Fiber Optics Project`` (DOE/EA-1202). The EA contains the analysis of the proposed construction, operation, and maintenance of the OPGW. Based on the analysis in the EA, Western finds that the proposed action is not a major Federal action significantly affecting the quality of the human environment, within the meaning of the National Environmental Policy Act (NEPA) of 1969. The preparation of an environmental impact statement (EIS) is not required, and therefore, Western is issuing this Findings of No Significant Impact (FONSI).

NONE

1997-05-01T23:59:59.000Z

22

Liberty Utilities (Electric) - Commercial New Construction Rebate Program  

Open Energy Info (EERE)

Utilities (Electric) - Commercial New Construction Rebate Program Utilities (Electric) - Commercial New Construction Rebate Program (New Hampshire) No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Summary Last modified on March 13, 2013. Financial Incentive Program Place New Hampshire Name Liberty Utilities (Electric) - Commercial New Construction Rebate Program (New Hampshire) Incentive Type Utility Rebate Program Applicable Sector Commercial, Industrial, Local Government, Schools Eligible Technologies Central Air conditioners, Chillers, Compressed air, Custom/Others pending approval, Energy Mgmt. Systems/Building Controls, Heat pumps, Lighting, Lighting Controls/Sensors, Motor VFDs, Motors, Geothermal Heat Pumps, Control Sensors, Economizers

23

Prospective Type Ia supernova surveys from Dome A  

E-Print Network (OSTI)

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

Kim, A.

2010-01-01T23:59:59.000Z

24

Impact of Heavy Aircraft Operations on Airport Capacity at Newark Liberty International Airport  

E-Print Network (OSTI)

Aviation System Performance Metrics (ASPM) departure and arrival rate data is collected for four common airport confi gurations at Newark Liberty International Airport (EWR) under Visual Meteorological Conditions (VMC) for ...

Simaiakis, Ioannis

25

Turbulent Combustion in Type Ia Supernova Models  

E-Print Network (OSTI)

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

F. K. Roepke; W. Hillebrandt

2006-09-15T23:59:59.000Z

26

New approaches for modeling type Ia supernovae  

SciTech Connect

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

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

2007-06-25T23:59:59.000Z

27

Theoretical cosmic Type Ia supernova rates  

E-Print Network (OSTI)

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

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

2008-07-15T23:59:59.000Z

28

Steamboat IA Geothermal Facility | Open Energy Information  

Open Energy Info (EERE)

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

29

PCCM's partnership with Liberty Science Center (LSC) has grown to improve awareness of materials science engineering among new audiences. In collaboration  

E-Print Network (OSTI)

and Liberty Science Center Expand Partnership (DMR0819860) D. Steinberg, C. Arnold, M. McAlpine, R. RegisterPCCM's partnership with Liberty Science Center (LSC) has grown to improve awareness of materials science engineering among new audiences. In collaboration with Liberty Science Center, PCCM members

Petta, Jason

30

The progenitors of subluminous type Ia supernovae  

DOE Green Energy (OSTI)

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

Howell, D. Andrew

2001-02-01T23:59:59.000Z

31

Project Liberty: Cooperative Research and Development Final Report, CRADA Number CRD-07-00245  

Science Conference Proceedings (OSTI)

NREL hosted two teams of POET Project Liberty analysts for week-long biomass compositional analysis (wet chemical analysis) classes (one in 2008, one in 2009). NREL also performed biomass compositional on over 70 samples of corn stover feedstock and pretreated corn stover provided by POET.

Wolfrum, E. J.

2010-08-01T23:59:59.000Z

32

Impact of Heavy Aircraft Operations on Airport Capacity at Newark Liberty International Airport  

E-Print Network (OSTI)

Impact of Heavy Aircraft Operations on Airport Capacity at Newark Liberty International Airport Meteorological Conditions (VMC) for the period 2007-2008. The ef- fect of the number of Heavy (including Boeing that Heavy departures and arrivals negatively impact overall airport capacity. Mechanisms by which

33

Phil West  

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

Phil West is the director of communications for the Department of Energys Office of Energy Efficiency and Renewable Energy.

34

Rates and progenitors of type Ia supernovae  

SciTech Connect

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

Wood-Vasey, William Michael

2004-08-16T23:59:59.000Z

35

Freedom and order : how democratic governments abridge civil liberties after terrorist attacks -- and why sometimes they don't  

E-Print Network (OSTI)

This dissertation is driven by the following question: "What explains the variation in governments' civil liberty-abridging responses to terrorist attacks?" In the United States, it was not until a year after the 1995 ...

Rubin, Gabriel, Ph. D. Massachusetts Institute of Technology

2008-01-01T23:59:59.000Z

36

Rolling Hills (IA) | Open Energy Information  

Open Energy Info (EERE)

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

37

On the Brightness of Supernova Ia  

E-Print Network (OSTI)

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

Yijia Zheng

2013-10-01T23:59:59.000Z

38

Spectral diversity of Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2006-05-05T23:59:59.000Z

39

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

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

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

40

LINKING TYPE Ia SUPERNOVA PROGENITORS AND THEIR RESULTING EXPLOSIONS  

Science Conference Proceedings (OSTI)

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

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

2012-06-20T23:59:59.000Z

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


41

Category:Des Moines, IA | Open Energy Information  

Open Energy Info (EERE)

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

42

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

Office of Legacy Management (LM)

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

43

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2008-01-01T23:59:59.000Z

44

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

Office of Legacy Management (LM)

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

45

Conformal cosmological model and SNe Ia data  

SciTech Connect

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

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

2012-11-15T23:59:59.000Z

46

The Distant Type Ia Supernova Rate  

DOE R&D Accomplishments (OSTI)

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

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

2002-05-28T23:59:59.000Z

47

West Valley  

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

Nuclear Facility Nuclear Facility Coalition on West Valley Nuclear Wastes PO Box 603 Springville NY 14141 WV-DigItUp@roadrunner.com Joanne Hameister CFMT (Concentrator Feed Make-up Tank) Packaged 13'x14'x19' 177.5 tons MFHT (Melter Feed Hold Tank) Packaged 13'x14'x16' 152.5 tons WIR Shipments pending to LLW facility MELTER 10'x10'x10' Packaged: 14'x13'x13' 159 tons 4,570 Curies Waste Categories High-Level Waste Based on source * Nuclear Fuel * Reprocessing * TRU Low-Level Waste Not Low Risk Complex classification based on * Nuclide inventory * Half-life(s) * Quantity * Decay products Background Radiation 1978 - average was 100 mRem per person 2011 - BRC* estimate 620 mRem per person Naturally occurring radioactive elements Additions accumulate - from fall-out,

48

West Valley  

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

Nuclear Facility Nuclear Facility Coalition on West Valley Nuclear Wastes PO Box 603 Springville NY 14141 WV-DigItUp@roadrunner.com Joanne Hameister CFMT (Concentrator Feed Make-up Tank) Packaged 13'x14'x19' 177.5 tons MFHT (Melter Feed Hold Tank) Packaged 13'x14'x16' 152.5 tons WIR Shipments pending to LLW facility MELTER 10'x10'x10' Packaged: 14'x13'x13' 159 tons 4,570 Curies Waste Categories High-Level Waste Based on source * Nuclear Fuel * Reprocessing * TRU Low-Level Waste Not Low Risk Complex classification based on * Nuclide inventory * Half-life(s) * Quantity * Decay products Background Radiation 1978 - average was 100 mRem per person 2011 - BRC* estimate 620 mRem per person Naturally occurring radioactive elements Additions accumulate - from fall-out,

49

West Virginia Direct Loan Program (West Virginia)  

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

The West Virginia Direct Loan Program, provides up to 45 percent in financing fixed assets through low-interest, direct loans to businesses expanding or locating in West Virginia. Proceeds from the...

50

Liberty and British identity: printed reactions to the Quebec Act 1774-1775  

E-Print Network (OSTI)

This thesis explores reactions to the Quebec Act of 1774 in pamphlets and newspapers within Britain and the American colonies. The Quebec Act was signed by George III in June of 1774, the bill instituted French Civil Law, put in place a military governor and a executive council, all of whom served at the will of the Crown, and effectively established Roman Catholicism in Canada under the Crowns control. The rhetoric analyzed for this thesis came from a number of contemporary pamphlets and newspaper commentaries on the Quebec Act specifically,or on colonial policy, which included the Quebec Act, more generally. The pamphlets were written by ministers, politicians, public figures and anonymous individuals. The concepts, ideals, and words used by these various commentators suggest underlying concerns and ideals which they all share and which their audience would understand and identify with. In using the rhetoric employed in these sources this study hopes to show that in their reactions to the incorporation of French Catholics, under their own laws and religious traditions, British contemporaries revealed their conception of what it meant to be British.There is a strong sense that British Protestantism was not so unified that it would serve as an effective foundation to build an identity. Therefore, rather than simply being formed as a reaction against the French and Catholic Other, this identity seems to be rooted in a positive sense of the nature of English liberty, which was then extended to the British people. The rhetoric in the American colonies is used to show how an identity centered on the ideal of liberty functions on the periphery. This thesis hopes to also address the fact that the Quebec Act has been overlooked by many who address the issue of British identity. Such an event, even if overshadowed in popular history by the other Coercive Acts, is a valuable episode in the creation and expression of a British Identity.

Willis, Aaron Lukefahr

2007-08-01T23:59:59.000Z

51

Burning Thermals in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

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

Bell, John B.

52

Visualizing Type Ia Supernova Explosions at NERSC  

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

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

53

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

Gasoline and Diesel Fuel Update (EIA)

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

54

DOE/EA-1628: Environmental Assessment for Construction and Operation of a Proposed Lignocellulosic Biorefinery, POET Project LIBERTY, LLC. (September 2008)  

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

and Notice of Wetlands and Notice of Wetlands Involvement Construction and Operation of a Proposed Lignocellulosic Biorefinery, POET Project LIBERTY, LLC. Emmetsburg, Iowa Prepared for U.S. Department of Energy by September 2008 September 2008 i POET Project LIBERTY - Final EA 9-26-08.doc Contents Executive Summary ............................................................................................................................................i Acronyms, Abbreviations, and Terms............................................................................................................iv 1.0 Introduction ............................................................................................................................................ 1-1 1.1 Background......................................................................................................................................

55

Late Light Curves of Normally-Luminous Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2006-01-05T23:59:59.000Z

56

West Virginia Venture Capital (West Virginia)  

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

The West Virginia Venture Capital provides investment funds to eligible businesses stimulating economic growth and providing or retaining jobs within the state through qualified venture capital...

57

TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM  

SciTech Connect

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

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

2013-07-01T23:59:59.000Z

58

VELOCITY EVOLUTION AND THE INTRINSIC COLOR OF TYPE Ia SUPERNOVAE  

SciTech Connect

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

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

2011-12-01T23:59:59.000Z

59

The Rate of Type Ia Supernovae at High Redshift  

E-Print Network (OSTI)

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

Brian J. Barris; John L. Tonry

2005-09-22T23:59:59.000Z

60

The diversity of Type Ia Supernovae: evidence for systematics?  

E-Print Network (OSTI)

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

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

2004-11-02T23:59:59.000Z

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


61

DISTRIBUTED FLAMES IN TYPE Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

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

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

2010-02-20T23:59:59.000Z

62

Redshift-Independent Distances to Type Ia Supernovae  

E-Print Network (OSTI)

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

Brian J. Barris; John L. Tonry

2004-08-04T23:59:59.000Z

63

West Virginia Loan Insurance Program (West Virginia)  

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

The West Virginia Loan Insurance Program, provides a loan insurance program in cooperation with third party lenders to assist firms that cannot obtain conventional bank financing. Up to 80% of the...

64

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

E-Print Network (OSTI)

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

2008-01-01T23:59:59.000Z

65

Nucleosynthesis in type Ia supernovae driven by asymmetric thermonuclear ignition  

Science Conference Proceedings (OSTI)

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

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

2012-11-12T23:59:59.000Z

66

West Biofuels | Open Energy Information  

Open Energy Info (EERE)

West Biofuels Jump to: navigation, search Name West Biofuels Place California Sector Biofuels Product West Biofuels LLC is a 2007 start-up company based in California with funding...

67

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

E-Print Network (OSTI)

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

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

2000-01-01T23:59:59.000Z

68

Progenitors of type Ia supernovae in elliptical galaxies  

Science Conference Proceedings (OSTI)

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

Gilfanov, M.; Bogdan, A.

2011-09-21T23:59:59.000Z

69

Learning from the scatter in type ia supernovae  

SciTech Connect

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

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

2005-11-01T23:59:59.000Z

70

Type Ia Supernova Spectral Line Ratios as LuminosityIndicators  

SciTech Connect

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

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

2005-12-07T23:59:59.000Z

71

West Nile Virus  

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

NILE VIRUS (WNS) NILE VIRUS (WNS) DEFINITION West Nile virus is an infection transmitted by mosquitoes. If you become infected with West Nile virus, you may not experience any signs or symptoms or you may experience only minor ones, such as fever and mild headache. However, some people who become infected with West Nile virus develop a life-threatening illness that includes inflammation of the brain. MODES OF TRANSMISSION The main route of human infection with West Nile virus is through the bite of an infected mosquito. Mosquitoes become infected when they feed on infected birds, which may circulate the virus in their blood for a few days. The virus eventually gets into the mosquito's salivary

72

West | OpenEI  

Open Energy Info (EERE)

West West Dataset Summary Description This dataset comes from the Energy Information Administration (EIA), and is part of the 2011 Annual Energy Outlook Report (AEO2011). This dataset is table 108, and contains only the reference case. The dataset uses gigawatts, billion kilowatthours and quadrillion Btu. The data is broken down into generating capacity, electricity generation and energy consumption. Source EIA Date Released April 26th, 2011 (3 years ago) Date Updated Unknown Keywords 2011 AEO EIA Reliability First Corporation Renewable Energy Generation West Data application/vnd.ms-excel icon AEO2011: Renewable Energy Generation by Fuel - Reliability First Corporation / West- Reference Case (xls, 119 KiB) Quality Metrics Level of Review Peer Reviewed Comment

73

Investigating the Flame Microstructure in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2002-04-02T23:59:59.000Z

74

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

E-Print Network (OSTI)

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

Patat, F

2004-01-01T23:59:59.000Z

75

Could There Be A Hole In Type Ia Supernovae?  

E-Print Network (OSTI)

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

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

2003-11-01T23:59:59.000Z

76

Steven Westly | Department of Energy  

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

Westly Westly About Us Steven Westly - Managing Partner, Westly Group Photo of Steven Westly Steve Westly has built one of the larger clean tech venture capital firms in the U.S. Prior to founding The Westly Group, Steve Westly served as the Controller and Chief Fiscal Officer of the state of California - the world's sixth largest economy. As Controller, he chaired the State Lands Commission and served on 63 other boards and commissions, including CalPERS and CalSTRS, the nation's two largest public pension funds, which together invest more than $350 billion. Mr. Westly led an effort to commit more than $1 billion to clean technology investments. Before running for office, Mr. Westly helped guide the online auction company eBay through its period of most rapid growth, serving as the Senior

77

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

Science Conference Proceedings (OSTI)

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

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

2012-08-10T23:59:59.000Z

78

Cooperation Reliability Testing of the Clipper Windpower Liberty 2.5 MW Turbine: Cooperative Research and Development Final Report, CRADA Number CRD-07-210  

DOE Green Energy (OSTI)

Clipper Windpower (CWP) has developed the Liberty 2.5 MW wind turbine. The development, manufacturing, and certification process depends heavily on being able to validate the full-scale system design and performance under load in both an accredited structural test facility and through accredited field testing. CWP requested that DOE/ NREL upgrade blade test capabilities to perform a scope of work including structural testing of the C-96 blade used on the CWP Liberty turbine. This funds-in CRADA was developed to upgrade NREL blade test capability, while enabling certification testing of the C-96 blade through the facility and equipment upgrades. NREL shared resource funds were used to develop hardware necessary to structurally attach a large wind turbine to the test stand at the NWTC. Participant funds-in monies were used for developing the test program.

Hughes, S.

2012-05-01T23:59:59.000Z

79

West Enfield Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

Sign Up Search Page Edit with form History Facebook icon Twitter icon West Enfield Biomass Facility Jump to: navigation, search Name West Enfield Biomass Facility Facility West...

80

THE DIFFUSE GAMMA-RAY BACKGROUND FROM TYPE Ia SUPERNOVAE  

SciTech Connect

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

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

2012-03-10T23:59:59.000Z

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81

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

E-Print Network (OSTI)

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

F. Patat

2004-09-28T23:59:59.000Z

82

Turbulence-Flame Interactions in Type Ia Supernovae  

SciTech Connect

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

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

2008-05-27T23:59:59.000Z

83

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2008-11-17T23:59:59.000Z

84

Circleville, West Virginia 26804  

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

P.O. Box 194 P.O. Box 194 Circleville, West Virginia 26804 March 28, 2012 Lamont Jackson Office of Electricity Delivery and Energy Reliability U.S. Department of Energy 1000 Independence Ave. SW Washington, DC 20585 Via email to lamont.jackson@hq.doe.gov Re: OE Docket No. RRTT-IR-001 (Rapid Response Team for Transmission); Office of Electricity Delivery and Energy Reliability, Department of Energy Dear Mr. Jackson: Please accept the following comments submitted on behalf of the Allegheny Highlands Alliance, Inc. ("AHA"), an organization comprised of residents of the states of West Virginia, Pennsylvania, Maryland, Virginia and North Carolina. AHA is presently awaiting a decision

85

West Virginia Higher Education Graduate  

E-Print Network (OSTI)

1. Work Participation And Annualized Wages Of West Virginia Public Higher Education Graduates From This report analyzes the West Virginia industry of employment (and wages) of graduates from state public .................................................................................................1 Results By Industry And Summary Degree

Mohaghegh, Shahab

86

West Texas A&M  

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

West Texas A&M ffiUNIVERSITY Division of Nursing MEMORANDUM OF UNDERSTANDING AND AFFILIATION AGREEMENT BWXT PANTEX, Amarillo, Texas and WEST TEXASA&M UNIVERSITY DEPARTMENT OF...

87

WestConnect Transmission Product  

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

WestConnect Transmission Product Federal Register Notices Customer Notifications Customer Comments Approved Rate Order FERC Confirmation...

88

Independent Oversight Review, West Valley Demonstration Project...  

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

Independent Oversight Review, West Valley Demonstration Project Transportation - September 2000 Independent Oversight Review, West Valley Demonstration Project Transportation -...

89

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

Gasoline and Diesel Fuel Update (EIA)

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

90

West Virginia | Department of Energy  

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

United States » West Virginia United States » West Virginia West Virginia October 22, 2013 Data Safer than Ever with FM-200 Installation The consolidated data center at the Legacy Management Business Center (LMBC) in Morgantown, West Virginia, is now guarded by a state-of-the-art FM-200® Fire Suppression System. Installation of the new system began on June 11, 2013, and the system became operational on July 18. October 16, 2013 West Virginia Venture Capital (West Virginia) The West Virginia Venture Capital provides investment funds to eligible businesses stimulating economic growth and providing or retaining jobs within the state through qualified venture capital companies. Terms and conditions for funding eligibility are dependent on the varying terms of participating venture capital funds.

91

West Virginia.indd  

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

West Virginia West Virginia www.effi cientwindows.org March 2013 1. Meet the Energy Code and Look for the ENERGY STAR ® Windows must comply with your local energy code. Windows that are ENERGY STAR qualifi ed typically meet or exceed energy code requirements. To verify if specific window energy properties comply with the local code requirements, go to Step 2. 2. Look for Effi cient Properties on the NFRC Label The National Fenestration Rating Council (NFRC) label is needed for verifi cation of energy code compliance (www.nfrc. org). The NFRC label displays whole- window energy properties and appears on all fenestration products which are part of the ENERGY STAR program.

92

Enforcement Letter - Argonne West  

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

9, 1999 9, 1999 Mr. John I. Sackett [ ] Argonne National Laboratory-West P.O. Box 2528 Idaho Falls, Idaho 83403-6000 Subject: Enforcement Letter (NTS-CH-AA-ANLW-ANLW-1998-0001) Dear Mr. Sackett: This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances concerning two incidents occurring in June and August 1998 at Argonne National Laboratory - West's (ANLW) Fuel Conditioning Facility (FCF): dropping a fuel basket assembly containing chopped fuel elements and repair of a manipulator seal tube. During November 2-3, 1998, DOE conducted an investigation to determine what, if any, noncompliances with applicable nuclear safety regulations may have been associated with these incidents. A copy of the investigation summary report is

93

Microsoft PowerPoint - IEEE IAS PES 102313.pptx  

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

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

94

Type Ia Supernova: Burning and Detonation in the Distributed Regime  

E-Print Network (OSTI)

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

S. E. Woosley

2007-09-26T23:59:59.000Z

95

Alternative Fuels Data Center: West Virginia Information  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

West Virginia West Virginia Information to someone by E-mail Share Alternative Fuels Data Center: West Virginia Information on Facebook Tweet about Alternative Fuels Data Center: West Virginia Information on Twitter Bookmark Alternative Fuels Data Center: West Virginia Information on Google Bookmark Alternative Fuels Data Center: West Virginia Information on Delicious Rank Alternative Fuels Data Center: West Virginia Information on Digg Find More places to share Alternative Fuels Data Center: West Virginia Information on AddThis.com... West Virginia Information This state page compiles information related to alternative fuels and advanced vehicles in West Virginia and includes new incentives and laws, alternative fueling station locations, truck stop electrification sites,

96

West Virginia | Department of Energy  

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

Groundwater Protection Rules Coal Mining Operations (West Virginia) Groundwater Protection Rules Coal Mining Operations (West Virginia) These rules establish a series of practices for the protection of groundwater which are to be followed by any person who conducts coal mining operations subject to the provisions of West Virginia Groundwater Protection Act and subject to regulation under the West Virginia Coal Mining and Reclamation Act and/or under West Virginia Water Pollution Control Act as it relates to coal mining operations. October 16, 2013 Groundwater Protection Plan (West Virginia) Groundwater Protection Plans (GPPs) are required for all facilities having the potential to impact groundwater. They are "preventive maintenance" documents that cover all processes and materials at a facility that "may

97

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

E-Print Network (OSTI)

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

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

2008-01-31T23:59:59.000Z

98

,"West Virginia Natural Gas Prices"  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Natural Gas Prices",11,"Annual",2012,"6301967" ,"Release Date:","10312013" ,"Next Release...

99

West Valley Site History, Cleanup Status, and Role of the West...  

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

West Valley Site History, Cleanup Status, and Role of the West Valley Citizen Task Force West Valley Site History, Cleanup Status, and Role of the West Valley Citizen Task Force...

100

Fitting Type Ia supernovae with coupled dark energy  

E-Print Network (OSTI)

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

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

2004-01-01T23:59:59.000Z

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


101

,"West Virginia Natural Gas Summary"  

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

1: Prices" "Sourcekey","N3050WV3","N3010WV3","N3020WV3","N3035WV3","N3045WV3" "Date","Natural Gas Citygate Price in West Virginia (Dollars per Thousand Cubic Feet)","West Virginia...

102

Gulf of Mexico -West Florida  

E-Print Network (OSTI)

Gulf of Mexico - Alabama - West Florida - Louisiana - Mississippi - Texas #12;Regional Summary Gulf of Mexico Region Management Context The Gulf of Mexico Region includes Alabama, Louisiana, Mississippi, Texas, and West Florida. Federal fisheries in this region are managed by the Gulf of Mexico Fishery

103

Gulf of Mexico -West Florida  

E-Print Network (OSTI)

Gulf of Mexico - Alabama - West Florida - Louisiana - Mississippi - Texas #12;Regional Summary Gulf of Mexico Management Context The Gulf Region is comprised of Texas, Louisiana, Mississippi, Alabama and West Florida. Federal fisheries in this region are managed by the Gulf of Mexico Fishery Management Council

104

CO2 Emissions - East and West Pakistan  

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

Far East East and West Pakistan CO2 Emissions from East and West Pakistan Data graphic Data CO2 Emissions from East and West Pakistan image Per capita CO2 Emission Estimates for...

105

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

E-Print Network (OSTI)

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

Juramy, Claire

2006-01-01T23:59:59.000Z

106

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

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

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

107

West Virginia | Department of Energy  

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

January 12, 2010 January 12, 2010 Training Changing Face of West Virginia's Workforce West Virginia's stimulus funding is expected to spur green jobs and build skills for the future in a state that relies on a nonrenewable energy source -- coal - to employ 35,000 members of its workforce. October 19, 2009 CX-000162: Categorical Exclusion Determination West Virginia State Energy Office CX(s) Applied: A9, A11 Date: 10/19/2009 Location(s): West Virginia Office(s): Energy Efficiency and Renewable Energy, Golden Field Office June 26, 2009 Obama Administration Awards More than $96 Million for State Energy Programs in Ohio, Oregon, Virginia and West Virginia Funding Will Speed Adoption of Efficiency and Renewable Energy Technologies March 26, 2009 Obama Administration Announces Additional $14,003,800 for Local Energy

108

Geothermal investigations in West Virginia  

DOE Green Energy (OSTI)

Deep sedimentary basins and warm-spring systems in West Virginia are potential geothermal resources. A temperature gradient map based on 800 bottom-hole temperatures for West Virginia shows that variations of temperature gradient trend northeasterly, parallel to regional structure. Highest temperature gradient values of about 28/sup 0/C/km occur in east-central West Virginia, and the lowest gradients (18/sup 0/C/km) are found over the Rome Trough. Results from ground-water geochemistry indicate that the warm waters circulate in very shallow aquifers and are subject to seasonal temperature fluctuations. Silica heat-flow data in West Virginia vary from about 0.89 to 1.4 HFU and generally increase towards the west. Bouguer, magnetic, and temperature gradient profiles suggest that an ancient rift transects the state and is the site of several deep sedimentary basins.

Hendry, R.; Hilfiker, K.; Hodge, D.; Morgan, P.; Swanberg, C.; Shannon, S.S. Jr.

1982-11-01T23:59:59.000Z

109

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

E-Print Network (OSTI)

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

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

2008-09-18T23:59:59.000Z

110

West Virginia Shale Production (Billion Cubic Feet)  

Annual Energy Outlook 2012 (EIA)

View History: Annual Download Data (XLS File) West Virginia Shale Production (Billion Cubic Feet) West Virginia Shale Production (Billion Cubic Feet) Decade Year-0 Year-1 Year-2...

111

NETL: Science Bowl Information - West Virginia  

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

Home > Educational Initiatives > Science Bowl Information > Science Bowl Information - West Virginia Educational Initiatives Science Bowl Information - West Virginia Welcome to the...

112

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

SciTech Connect

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

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

2008-02-28T23:59:59.000Z

113

Precipitation Patterns in West Africa  

Science Conference Proceedings (OSTI)

A regional precipitation analysis from a total of 813 recording stations in 11 West African countries for the drought period 196875 is presented. Results illustrate the severity and extent of meteorological drought which prevailed throughout the ...

Raymond P. Motha; Sharon K. Leduc; Louis T. Steyaert; Clarence M. Sakamoto; Norton D. Strommen

1980-10-01T23:59:59.000Z

114

West Virginia | Department of Energy  

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

Qualifying RPS State Export Markets (West Virginia) Qualifying RPS State Export Markets (West Virginia) This entry lists the states with Renewable Portfolio Standard (RPS) policies that accept generation located in West Virginia as eligible sources towards their RPS targets or goals. For specific information with regard to eligible technologies or other restrictions which may vary by state, see the RPS policy entries for the individual states, shown below in the Authority listings. Typically energy must be delivered to an in-state utility or Load Serving Entity, and often only a portion of compliance targets may be met by out-of-state generation. October 16, 2013 Proof of Proper Solid Waste Disposal (West Virginia) This rule provides guidance to persons occupying a residence or operating a business establishment in this state regarding the approved method of

115

West Virginia | Department of Energy  

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

June 17, 2010 June 17, 2010 CX-002740: Categorical Exclusion Determination Coal Use By-Product Characterization Lab Decommissioning CX(s) Applied: B3.6 Date: 06/17/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory June 9, 2010 CX-002635: Categorical Exclusion Determination Energy Conservation Measure (ECM) #2: MERC Well Upgrade, National Energy Technology Laboratory Morgantown, West Virginia CX(s) Applied: B5.12 Date: 06/09/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory June 7, 2010 EIS-0445: Notice of Intent to Prepare an Environmental Impact Statement Mountaineer Commercial Scale Carbon Capture and Storage Project, Mason County, West Virginia June 4, 2010

116

West Virginia | Department of Energy  

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

Underground Injection Control (West Virginia) Underground Injection Control (West Virginia) This rule set forth criteria and standards for the requirements which apply to the State Underground Injection Control Program (U.I.C.). The UIC permit program regulates underground injections by 5 classes of wells. All owners or operators of these injection wells must be authorized either by permit or rule by the Director. October 16, 2013 Underground Gas Storage Reservoirs (West Virginia) Lays out guidelines for the conditions under which coal mining operations must notify state authorities of intentions to mine where underground gas is stored as well as map and data requirements, inspection of facilities and penalties. October 16, 2013 Tax Exemption for Wind Energy Generation In March 2007, West Virginia enacted legislation

117

GeoPowering the West  

DOE Green Energy (OSTI)

Summary brochure of GeoPowering the West (GPW) activities, and areas of technology transfer and market transformation. It also provides current contact information for key DOE and national laboratory staff representing the GPW program.

Not Available

2007-02-01T23:59:59.000Z

118

,"West Virginia Natural Gas Summary"  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet)","West Virginia Dry Natural Gas Reserves Estimated Production (Billion Cubic Feet)" 28306,1567,1,76,63,,,97,5,17,124...

119

West Virginia Gasoline Price Data  

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

West Virginia Exit Fueleconomy.gov The links below are to pages that are not part of the fueleconomy.gov. We offer these external links for your convenience in accessing additional...

120

China Marches West: Jacket cover  

E-Print Network (OSTI)

The China we know today is the product of vast frontier conquests of the seventeenth and eighteenth centuries by the expanding Qing empire. China Marches West tells the story of this unprecedented expansion and explores ...

Perdue, Peter C.

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


121

West Virginia 1995 Vintage Gas Well History  

U.S. Energy Information Administration (EIA)

West Virginia 1995 Vintage Gas Well History. Energy Information Administration (U.S. Dept. of Energy)

122

West Virginia 1995 Vintage Oil Well History  

U.S. Energy Information Administration (EIA)

West Virginia 1995 Vintage Oil Well History. Energy Information Administration (U.S. Dept. of Energy)

123

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

Science Conference Proceedings (OSTI)

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

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

2012-07-01T23:59:59.000Z

124

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

E-Print Network (OSTI)

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

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

2006-03-03T23:59:59.000Z

125

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

SciTech Connect

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

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

2012-06-01T23:59:59.000Z

126

EARLY PHASE OBSERVATIONS OF EXTREMELY LUMINOUS TYPE Ia SUPERNOVA 2009dc  

Science Conference Proceedings (OSTI)

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

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

2009-12-20T23:59:59.000Z

127

West Virginia/Incentives | Open Energy Information  

Open Energy Info (EERE)

source source History View New Pages Recent Changes All Special Pages Semantic Search/Querying Get Involved Help Apps Datasets Community Login | Sign Up Search Page Edit History Facebook icon Twitter icon » West Virginia/Incentives < West Virginia Jump to: navigation, search Contents 1 Financial Incentive Programs for West Virginia 2 Rules, Regulations and Policies for West Virginia Download All Financial Incentives and Policies for West Virginia CSV (rows 1 - 62) Financial Incentive Programs for West Virginia Download Financial Incentives for West Virginia CSV (rows 1 - 12) Incentive Incentive Type Active AEP Appalachian Power - Commercial and Industrial Rebate Programs (West Virginia) Utility Rebate Program Yes AEP Appalachian Power - Residential Energy Efficiency Rebate Program (West Virginia) Utility Rebate Program Yes

128

West Virginia | Department of Energy  

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

May 13, 2010 May 13, 2010 CX-002246: Categorical Exclusion Determination Decommission of B4, 112, Atmospheric Cold Flow Laboratory CX(s) Applied: B1.24, B1.27, B1.31 Date: 05/13/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory May 13, 2010 CX-002573: Categorical Exclusion Determination Millsop Community Center Energy Reduction Renovations CX(s) Applied: B2.5, B1.4, B5.1 Date: 05/13/2010 Location(s): Weirton, West Virginia Office(s): Energy Efficiency and Renewable Energy May 10, 2010 CX-002372: Categorical Exclusion Determination Building 17 and 19 Utility Meter Install CX(s) Applied: B1.15, B2.2 Date: 05/10/2010 Location(s): Morgantown, West Virginia Office(s): National Energy Technology Laboratory April 23, 2010 Recycling Energy Yields Super Savings

129

West Virginia | Department of Energy  

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

April 29, 2011 April 29, 2011 CX-005662: Categorical Exclusion Determination The Use of Scrap Tires for Oil Well Stimulation CX(s) Applied: B3.7 Date: 04/29/2011 Location(s): Upper Falls, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 13, 2011 CX-005614: Categorical Exclusion Determination Building 33 Chemical Resistant Flooring Project CX(s) Applied: B1.3 Date: 04/13/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 13, 2011 CX-005613: Categorical Exclusion Determination Site-Wide Roadway Replacement CX(s) Applied: B1.3 Date: 04/13/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 12, 2011 CX-005607: Categorical Exclusion Determination

130

West Virginia | Department of Energy  

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

April 7, 2010 April 7, 2010 CX-001435: Categorical Exclusion Determination Building 33 Chemical Resistant Flooring Project CX(s) Applied: B1.3 Date: 04/07/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 7, 2010 CX-001434: Categorical Exclusion Determination Building 7 Roof Replacement Project CX(s) Applied: B1.3 Date: 04/07/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 7, 2010 CX-001433: Categorical Exclusion Determination Site Perimeter Fencing Project CX(s) Applied: B1.3 Date: 04/07/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory April 2, 2010 W.Va. Mom Sees Benefits of Weatherization

131

West Virginia | Department of Energy  

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

September 8, 2011 September 8, 2011 CX-006741: Categorical Exclusion Determination Information Technology Hub Relocation CX(s) Applied: B1.31 Date: 09/08/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory August 22, 2011 CX-006543: Categorical Exclusion Determination Building 40 New Video Surveillance CX(s) Applied: A11, B1.15, B2.3 Date: 08/22/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory August 12, 2011 CX-006480: Categorical Exclusion Determination Materials Research Laboratory (MRL) CX(s) Applied: B3.6 Date: 08/12/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory August 8, 2011 CX-006464: Categorical Exclusion Determination

132

West Virginia | Department of Energy  

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

1, 2011 1, 2011 EIS-0445: DOE Notice of Availability of the Draft Environmental Impact Statement Mountaineer Commercial Scale Carbon Capture and Storage Project, Mason County, West Virginia March 4, 2011 EIS-0445: EPA Notice of Availability of the Draft Environmental Impact Statement Mountaineer Commercial Scale Carbon Capture and Storage Project, Mason County, West Virginia March 1, 2011 CX-005336: Categorical Exclusion Determination Materials Synthesis Laboratory Modifications/Additions CX(s) Applied: B3.6 Date: 03/01/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory March 1, 2011 CX-005335: Categorical Exclusion Determination National Energy Technology Laboratory Reciprocating Laboratory Decommissioning CX(s) Applied: B3.6

133

West Virginia | Department of Energy  

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

June 28, 2011 June 28, 2011 CX-006117: Categorical Exclusion Determination Flooring Improvements CX(s) Applied: B2.1, B2.5 Date: 06/28/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory June 23, 2011 CX-006129: Categorical Exclusion Determination Optical Sensors Laboratory CX(s) Applied: B3.6 Date: 06/23/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory June 21, 2011 CX-006132: Categorical Exclusion Determination Replacement of Sidewalk Along Collins Ferry Road CX(s) Applied: B1.3 Date: 06/21/2011 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory June 15, 2011 CX-006137: Categorical Exclusion Determination B39 Cellular Repeater Installation

134

West Virginia | Department of Energy  

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

November 30, 2010 November 30, 2010 CX-004582: Categorical Exclusion Determination Re-Utilization of Industrial Carbon Dioxide for Algae Production Using a Phase Change Material CX(s) Applied: A9, A11, B3.6 Date: 11/30/2010 Location(s): Triadelphia, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory November 18, 2010 CX-004477: Categorical Exclusion Determination Extreme Drilling Laboratory (XDL) CX(s) Applied: B3.6 Date: 11/18/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory November 18, 2010 CX-004470: Categorical Exclusion Determination Relocation of Laboratory on Morgantown Site from B25/102 to B4/112 CX(s) Applied: B3.6 Date: 11/18/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory

135

West Virginia | Department of Energy  

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

March 19, 2010 March 19, 2010 CX-001303: Categorical Exclusion Determination Morgantown B39, Room B73: New Multi-Media Room Construction CX(s) Applied: B1.15 Date: 03/19/2010 Location(s): Morgantown, West Virginia Office(s): National Energy Technology Laboratory March 19, 2010 CX-001305: Categorical Exclusion Determination Site Wide Upgrade to Metering Software CX(s) Applied: A8 Date: 03/19/2010 Location(s): Morgantown, West Virginia Office(s): National Energy Technology Laboratory March 19, 2010 CX-001304: Categorical Exclusion Determination B3 Hot and Chilled Water Pump Upgrades CX(s) Applied: B1.5 Date: 03/19/2010 Location(s): Morgantown, West Virginia Office(s): National Energy Technology Laboratory March 17, 2010 CX-001327: Categorical Exclusion Determination Design/Construction/Installation of Appliance Technology Evaluation Center

136

West Virginia | Department of Energy  

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

Carbon Dioxide Sequestration (West Virginia) Carbon Dioxide Sequestration (West Virginia) The purpose of this law is to: October 16, 2013 Building Energy Code ''Much of the information presented in this summary is drawn from the U.S. Department of Energy's (DOE) Building Energy Codes Program and the Building Codes Assistance Project (BCAP). For more detailed information about building energy codes, visit the [http://www.energycodes.gov/states/ DOE] and [http://bcap-ocean.org/ BCAP] websites.'' October 16, 2013 Alternative and Renewable Energy Portfolio Standard In June 2009, West Virginia enacted an ''Alternative and Renewable Energy Portfolio Standard'' that requires investor-owned utilities (IOUs)* with more than 30,000 residential customers to supply 25% of retail electric sales from eligible alternative and renewable energy resources by 2025.

137

State Energy Program Assurances - West Virginia Governor Manchin...  

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

State Energy Program Assurances - West Virginia Governor Manchin State Energy Program Assurances - West Virginia Governor Manchin Letter from West Virginia Governor Manchin...

138

West Virginia Business & Economic Review, Spring 2010 1 West Virginia  

E-Print Network (OSTI)

in West Virginia during the past year have been widely distributed across industries. Indeed, losses were for energy and steel that results in less demand for coal and natural gas. Within the natural resources of con- struction and hotel accommodations, mostly in Las Vegas. Losses in the financial industry greatly

Mohaghegh, Shahab

139

20120328 WEST Comments on RRTT RFI Response Request  

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

March March 2 8, 2 012 Mr. L amont J ackson Office o f E lectricity D elivery a nd E nergy R eliability ( OE---20) U.S. D epartment o f E nergy 1000 I ndependence A venue, S W Washington, D C 2 0585 Submitted e lectronically v ia d ocket ( Document I D D OE_FRDOC_0001---1840) a nd e mail t o: Lamont.Jackson@hq.doe.gov Re: Department o f E nergy --- R apid R esponse T eam f or T ransmission R equest for I nformation, R RTT---IR---01, 7 7 F ed. R eg. 1 1517 ( Feb. 2 7, 2 012) 1 Dear M r. J ackson: I. INTRODUCTION The W estern E nergy S upply a nd T ransmission A ssociates ( "WEST") 2 respectfully s ubmits t hese r esponses t o t he s pecific q uestions r aised i n t he Department o f E nergy's ( DOE) a bove---referenced R equest f or I nformation ( RFI) regarding F ederal e fforts t o r esolve t he i ssue o f i ncongruent

140

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

Science Conference Proceedings (OSTI)

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

Saurabh W. Jha

2012-10-03T23:59:59.000Z

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


141

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

E-Print Network (OSTI)

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

Miko?ajewska, J

2011-01-01T23:59:59.000Z

142

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

SciTech Connect

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

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

2011-09-01T23:59:59.000Z

143

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

E-Print Network (OSTI)

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

144

West Virginia/Geothermal | Open Energy Information  

Open Energy Info (EERE)

West Virginia/Geothermal West Virginia/Geothermal < West Virginia Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Print PDF West Virginia Geothermal General Regulatory Roadmap Geothermal Power Projects Under Development in West Virginia No geothermal projects listed. Add a geothermal project. Operational Geothermal Power Plants in West Virginia No geothermal power plants listed. Add a geothermal energy generation facility. Geothermal Areas in West Virginia No areas listed. GRR-logo.png Geothermal Regulatory Roadmap for West Virginia Overview Flowchart The flowcharts listed below were developed as part of the Geothermal Regulatory Roadmap project. The flowcharts cover the major requirements for developing geothermal energy, including, land access, exploration and drilling, plant construction and operation, transmission siting, water

145

Gulf of Mexico -West Florida  

E-Print Network (OSTI)

Gulf of Mexico - Alabama - West Florida - Louisiana - Mississippi - Texas 119 #12;Regional Summary Gulf of Mexico Key Gulf of Mexico Commercial Species · Blue crab · Mullets · Stone crab · Oyster are managed by the Gulf of Mexico Fishery Management Council (GMFMC) and NOAA Fisheries (NMFS) under seven

146

Why Is West Coast Gasoline So Expensive?  

Reports and Publications (EIA)

Testimony on current gasoline prices as well as the unique situations on the West Coast with regard to prices.

Information Center

2001-04-25T23:59:59.000Z

147

West Valley Demonstration Project Transportation Emergency Management...  

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

West Valley Demonstration Project Transportation Emergency Management Program Independent Oversight Review of the Office of Independent Oversight and Performance Assurance...

148

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

E-Print Network (OSTI)

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

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

2000-08-21T23:59:59.000Z

149

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

SciTech Connect

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

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

2012-10-20T23:59:59.000Z

150

The West Virginia Coal Economy February 2010  

E-Print Network (OSTI)

The West Virginia Coal Economy 2008 February 2010 Prepared By: Bureau of Business and Economic Partial funding for this research was provided by the West Virginia Coal Association. The opinions herein are those of the authors and do not necessarily reflect those of the West Virginia Coal Association, Higher

Mohaghegh, Shahab

151

Independent Oversight Review, West Valley Demonstration Project  

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

Independent Oversight Review, West Valley Demonstration Project Independent Oversight Review, West Valley Demonstration Project Transportation - September 2000 Independent Oversight Review, West Valley Demonstration Project Transportation - September 2000 September 2000 Transportation Emergency Management Review of the West Valley Demonstration Project (WVDP) and National Transportation Program (NTP)/Transportation Compliance Evaluation/Assistance Program (TCEAP) The U.S. Department of Energy (DOE) Office of Emergency Management Oversight, within the Secretary of Energy's Office of Independent Oversight and Performance Assurance, conducted a transportation emergency management review of the West Valley Demonstration Project (WVDP) and National Transportation Program (NTP)/Transportation Compliance Evaluation/Assistance Program (TCEAP) in September 2000.

152

Forestry Policies (West Virginia) | Department of Energy  

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

Forestry Policies (West Virginia) Forestry Policies (West Virginia) Forestry Policies (West Virginia) < Back Eligibility Agricultural Commercial Program Info State West Virginia Program Type Environmental Regulations Provider Department of Commerce West Virginia's Forests are managed by the State Division of Forestry. In 2010 the State issues its Forest Resource Assessment: http://www.wvforestry.com/DOF100Assessment_Revised_091310_Part1.pdf The report summarizes available woody biomass resources, citing harvesting cost as a limiting factor due to complex terrain. In 2010 the Forestry Division issued the document "Strategic Plan for the sustainability of West Virginia Forests", which included a section summarizing the State Forester's Report to FMRC on the use of wood biomass from West Virginia forests:

153

West Virginia | Department of Energy  

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

September 8, 2010 September 8, 2010 Today: Live from the Carbon Capture and Storage Forum Want to know more about carbon capture and sequestration? Here'e how. August 25, 2010 CX-003556: Categorical Exclusion Determination Morgantown Site Metering Installation CX(s) Applied: B2.2 Date: 08/25/2010 Location(s): Morgantown, West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory August 23, 2010 CX-003462: Categorical Exclusion Determination Visitor's Center Conference Room CX(s) Applied: B1.7, B1.15 Date: 08/23/2010 Location(s): Morgantown,West Virginia Office(s): Fossil Energy, National Energy Technology Laboratory August 17, 2010 CX-003427: Categorical Exclusion Determination Research Ridge 4 and 6 Data and Communication Cabling CX(s) Applied: B1.7 Date: 08/17/2010

154

West Virginia | Department of Energy  

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

April 18, 2013 April 18, 2013 LM Discusses Management of LTS&M Records The U.S. Department of Energy Office of Legacy Management's (LM) efforts to maintain long-term surveillance and maintenance (LTS&M) records were highlighted during the 2013 Waste Management Symposia held February 24 through 28, in Phoenix, Arizona. April 18, 2013 Legacy Management Business Center January 25, 2013 AVESTAR provides high-quality, hands-on, simulator-based workforce training delivered by an experienced team of power industry training professionals for West Virginia students. | Photo courtesy of the Office of Fossil Energy. National Lab Helping to Train Operators for Next Generation of Power Plants Students in West Virginia are receiving hands-on experience for careers at cleaner-burning coal-fired power plants.

155

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

Open Energy Info (EERE)

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

156

IA REP0 SAND85-2809 Unlimited Release UC-92A  

Office of Scientific and Technical Information (OSTI)

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

157

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

E-Print Network (OSTI)

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

Meng, Xiangcun

2013-01-01T23:59:59.000Z

158

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

Science Conference Proceedings (OSTI)

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

Munroe J.; Wilkins K.; Gruber M.

2000-05-01T23:59:59.000Z

159

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

E-Print Network (OSTI)

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

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

2009-01-01T23:59:59.000Z

160

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

E-Print Network (OSTI)

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

Minnihan, Ellen Catherine

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


161

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

SciTech Connect

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

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

2013-01-10T23:59:59.000Z

162

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

SciTech Connect

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

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

2005-04-01T23:59:59.000Z

163

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

E-Print Network (OSTI)

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

Nora Bretn; Ariadna Montiel

2013-03-06T23:59:59.000Z

164

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

E-Print Network (OSTI)

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

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

2003-12-03T23:59:59.000Z

165

DOE Solar Decathlon: West Virginia University  

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

West Virginia University West Virginia University Team website: solar.wvu.edu Photo of members of the West Virginia University Solar Decathlon 2013 team in front of a building on campus. Enlarge image The West Virginia University Solar Decathlon 2013 team (Courtesy of the West Virginia University Solar Decathlon 2013 team) he West Virginia University audiovisual presentation Jury Feedback Architecture Contest Market Appeal Contest Engineering Contest Communications Contest Team Deliverables Project Manual Construction Drawings Menu and Recipes Neither the United States, nor the Department of Energy, nor the Alliance for Sustainable Energy LLC, nor any of their contractors, subcontractors, or their employees make any warranty, express or implied, or assume any legal liability or responsibility for the accuracy, completeness, or

166

West Virginia | Building Energy Codes Program  

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

West Virginia West Virginia Last updated on 2013-08-02 Commercial Residential Code Change Current Code ASHRAE Standard 90.1-2007 Approved Compliance Tools Can use COMcheck State Specific Research Impacts of ASHRAE 90.1-2007 for Commercial Buildings in the State of West Virginia (BECP Report, Sept. 2009) Approximate Energy Efficiency Equivalent to ASHRAE 90.1-2007 Effective Date 09/01/2013 Adoption Date 07/18/2012 Code Enforcement Mandatory DOE Determination Standard 90.1-2007: Yes Standard 90.1-2010: No West Virginia DOE Determination Letter, May 31, 2013 West Virginia State Certification of Commercial and Residential Building Energy Codes Current Code 2009 IECC Approved Compliance Tools Can use REScheck State Specific Research Impacts of the 2009 IECC for Residential Buildings in the State of West Virginia (BECP Report, Sept. 2009)

167

K-25 West Wing Demolition Completed  

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

Thirteen months after demolition began, the final unit of K-25's 844,000 square foot west wing was taken down.

168

New infrastructure boosts West Virginia, southern Pennsylvania ...  

U.S. Energy Information Administration (EIA)

September 2012: Equitrans placed into service its newly built 0.20 Bcf/d Blacksville Compressor Station in Monongalia County, West Virginia.

169

The Black Shale Basin of West Texas.  

E-Print Network (OSTI)

??The Black Shale Basin of West Texas covers an area in excess of 21,000 square miles and includes the region from Terrell and Pecos Counties (more)

Cole, Charles Taylor, 1913-

2012-01-01T23:59:59.000Z

170

Retail Unbundling - West Virginia - Energy Information Administration  

U.S. Energy Information Administration (EIA)

Energy Information Administration (U.S ... Unbundled service has been on the books to all ... West Virginia had 374,301 residential customers who consumed 30 ...

171

New infrastructure boosts West Virginia, southern Pennsylvania ...  

U.S. Energy Information Administration (EIA)

A notable increase since early 2012 in natural gas production in West Virginia and nearby counties in southern Pennsylvania continued through July 2013.

172

,"West Virginia Underground Natural Gas Storage Capacity"  

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

Capacity" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Underground Natural...

173

Independent Activity Report, West Valley Demonstration Project...  

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

West Valley Demonstration Project - July 2012 Independent Activity Report, New Brunswick Laboratory - November 2011 Orientation Visit to the Paducah Gaseous Diffusion Plant,...

174

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

E-Print Network (OSTI)

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

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

2010-01-01T23:59:59.000Z

175

Design and safety basis sludge characterization from exposure-adjusted radioisotopic source terms for N reactor fuel stored at K-East and K-West basins  

Science Conference Proceedings (OSTI)

The Safeguards and Accountability database was used as the primary source document for exposure data for spent N Reactor fuel stored at the K-East and K-West basins. This database is a listing of all keys (ie., groups of fuel discharged from the reactor at the same time), and the exposure for that key, mass of uranium in the key, fuel type (whether Mark IV or Mark IA), and several other parameters. There are nearly five hundred records (keys) in this database. Figure 1 illustrates an N Reactor Mark IV fuel assembly. The axial length of the endcap is approximately 0.19 inch. Mark IA and Mark IV fuel are low enriched zircalloy-2 clad metallic uranium tube-in-tube assemblies held together with spacers and clips. Unexposed Mark IV fuel assemblies have an enrichment of 0.947 wt% {sup 235}U in both inner and outer tubes. Unexposed Mark IA assemblies have an enrichment of 1.25 wt% {sup 235}U in the outer tube and 0.947 wt% {sup 235}U in the inner tube.

SCHWINKENDORF, K.N.

2001-10-23T23:59:59.000Z

176

Dynamics of the West African Westerly Jet  

Science Conference Proceedings (OSTI)

The West African westerly jet (WAWJ) is a low-level westerly jet located at 811N over the eastern Atlantic and the West African coast. It is clearly distinguished from the monsoon westerly flow by its structure and dynamics, and plays an ...

Bing Pu; Kerry H. Cook

2010-12-01T23:59:59.000Z

177

2010 Annual Report Greater West Texas  

E-Print Network (OSTI)

2010 Annual Report Greater West Texas State Employee Charitable Campaign You will find, as you look- rized workplace campaign for state agency and higher education em- ployees throughout Texas. In 2010,717 and West Central Texas SECC raised $131,797 for a combined total of $957,514! · 4,608 state employees gave

Rock, Chris

178

Book Review Sex Allocation. Stuart West.  

E-Print Network (OSTI)

Book Review Sex Allocation. Stuart West. Princeton, NJ: Princeton University Press, 2009. xii þ 466 offspring. This vast literature is now elegantly sum- marized and synthesized in Stuart West's book entitled, as evident in this book, has a commanding grasp of the large body of theoretical and empirical work

West, Stuart

179

West Virginia | Department of Energy  

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

December 1, 2006 December 1, 2006 EIS-0361: EPA Notice of Availability of Environmental Impact Statement Western Greenbrier Co-Production Demonstration Project, Rainelle, WV December 1, 2006 EIS-0361: Draft Environmental Impact Statement Western Greenbrier Co-Production Demonstration Project June 3, 2003 EIS-0361: Notice of Intent to Prepare an Environmental Impact Statement and Notice of Floodplain/Wetlands Involvement Western Greenbrier Co-Production Demonstration Project, Rainelle, West Virginia September 16, 2002 EA-1444: Finding of No Significant Impact Construction of a New Office Building, Childcare Facility, Parking Garage, and Storm water Retention Pond September 2, 2002 EA-1444: Final Environmental Assessment Construction of New Office Building, Child-Care Facility, Parking Garage,

180
Note: This page contains sample records for the topic "west liberty ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

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

E-Print Network (OSTI)

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

Shojai, F

2013-01-01T23:59:59.000Z

182

On the hydrogen emission from the type Ia supernova 2002ic  

DOE Green Energy (OSTI)

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

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

2003-12-10T23:59:59.000Z

183

Transmission Planning: Institutional Issues in the West | Department...  

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

Planning: Institutional Issues in the West Transmission Planning: Institutional Issues in the West Prepared for The CREPC Transmission Planning and Expansion Work Group by the...

184

EA-1843: Imperial Solar Energy Center West, California | Department...  

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

43: Imperial Solar Energy Center West, California EA-1843: Imperial Solar Energy Center West, California Summary This Environmental Impact Report Environmental Assessment (EIR...

185

BLM West Desert District Office | Open Energy Information  

Open Energy Info (EERE)

West Desert District Office Jump to: navigation, search Name BLM West Desert District Office Parent Organization BLM Place Salt Lake City, Utah Phone number (801) 977-4300...

186

FirstEnergy (West Penn Power) - Residential Solar Water Heating...  

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

FirstEnergy (West Penn Power) - Residential Solar Water Heating Program (Pennsylvania) FirstEnergy (West Penn Power) - Residential Solar Water Heating Program (Pennsylvania)...

187

Barbour County, West Virginia ASHRAE 169-2006 Climate Zone |...  

Open Energy Info (EERE)

Barbour County, West Virginia ASHRAE 169-2006 Climate Zone Jump to: navigation, search County Climate Zone Place Barbour County, West Virginia ASHRAE Standard ASHRAE 169-2006...

188

Demand Response National Trends: Implications for the West? ...  

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

Demand Response National Trends: Implications for the West? Demand Response National Trends: Implications for the West? Committee on Regional Electric Power Cooperation. San...

189

Merle West Medical Center Space Heating Low Temperature Geothermal...  

Open Energy Info (EERE)

Merle West Medical Center Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Merle West Medical Center Space Heating Low Temperature Geothermal...

190

West Virginia/EZ Policies | Open Energy Information  

Open Energy Info (EERE)

http:www.wvcommerce.orgAppMediaassetsdocenergy11WVWoodByproduct.pdf Gas Pipeline Safety (West Virginia) West Virginia Safety and Operational Guidelines Yes State...

191

West Virginia Shale Proved Reserves (Billion Cubic Feet)  

Annual Energy Outlook 2012 (EIA)

View History: Annual Download Data (XLS File) West Virginia Shale Proved Reserves (Billion Cubic Feet) West Virginia Shale Proved Reserves (Billion Cubic Feet) Decade Year-0...

192

West Virginia Natural Gas Gross Withdrawals from Shale Gas (Million...  

Annual Energy Outlook 2012 (EIA)

Annual Download Data (XLS File) West Virginia Natural Gas Gross Withdrawals from Shale Gas (Million Cubic Feet) West Virginia Natural Gas Gross Withdrawals from Shale Gas...

193

Water Pollution Control Act (West Virginia) | Department of Energy  

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

Water Pollution Control Act (West Virginia) Water Pollution Control Act (West Virginia) Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State...

194

Water Resources Protection and Management Act (West Virginia...  

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

Resources Protection and Management Act (West Virginia) Water Resources Protection and Management Act (West Virginia) Eligibility Utility Fed. Government Commercial Agricultural...

195

Geothermal Literature Review At U.S. West Region (Blackwell,...  

Open Energy Info (EERE)

GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Geothermal Literature Review At U.S. West Region (Blackwell, Et Al., 2010) Exploration Activity Details Location U.S. West...

196

Redefining Agrarian Power: Resurgent Agrarian Movements in West Java, Indonesia  

E-Print Network (OSTI)

Agrarian Movements in West Java, Indonesia Suraya Afiff Noeron agrarian change in Java in the 1970s and has, moreand agrarian change in Java, West Kalimantan, and other

Afiff, Suraya; Fauzi, Noer; Hart, Gillian; Ntsebeza, Lungisile; Peluso, Nancy

2005-01-01T23:59:59.000Z

197

New Solar Farms in West Tennessee Signal Growth - EERE ...  

New Solar Farms in West Tennessee Signal Growth. April 13, 2012. Two new solar energy farms are generating a small but growing supply of electricity in West Tennessee ...

198

,"West Virginia Natural Gas Gross Withdrawals from Shale Gas...  

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

PM" "Back to Contents","Data 1: West Virginia Natural Gas Gross Withdrawals from Shale Gas (Million Cubic Feet)" "Sourcekey","NGMEPG0FGSSWVMMCF" "Date","West Virginia...

199

Technical Services Contract Awarded for West Valley Demonstration...  

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

Technical Services Contract Awarded for West Valley Demonstration Project Support Services Technical Services Contract Awarded for West Valley Demonstration Project Support...

200

West Virginia Dry Natural Gas Reserves Sales (Billion Cubic Feet...  

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

View History: Annual Download Data (XLS File) West Virginia Dry Natural Gas Reserves Sales (Billion Cubic Feet) West Virginia Dry Natural Gas Reserves Sales (Billion Cubic Feet)...

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


201

West Virginia Natural Gas % of Total Residential - Sales (Percent...  

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

View History: Monthly Annual Download Data (XLS File) West Virginia Natural Gas % of Total Residential - Sales (Percent) West Virginia Natural Gas % of Total Residential - Sales...

202

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

E-Print Network (OSTI)

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

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

2004-01-01T23:59:59.000Z

203

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

E-Print Network (OSTI)

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

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

2003-12-08T23:59:59.000Z

204

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

E-Print Network (OSTI)

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

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

2007-06-07T23:59:59.000Z

205

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

E-Print Network (OSTI)

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

F. K. Roepke

2007-09-26T23:59:59.000Z

206

West Virginia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

West Virginia: Energy Resources West Virginia: Energy Resources Jump to: navigation, search Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":6,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"500px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.5976262,"lon":-80.4549026,"alt":0,"address":"West

207

Spent fuel treatment at ANL-West  

SciTech Connect

At Argonne National Laboratory-West (ANL-West) there are several thousand kilograms of metallic spent nuclear fuel containing bond sodium. This fuel will be treated in the Fuel Cycle Facility at ANL-West to produce stable waste forms for storage and disposal. The treatment operations will employ a pyrochemical process that also has applications for treating most of the fuel types within the Department of Energy complex. The treatment equipment is in its last stage of readiness, and operations will begin in the Fall of 1994.

Goff, K.M.; Benedict, R.W.; Levinskas, D.

1994-12-31T23:59:59.000Z

208

OPEC versus the west: a robust equilibrium  

Science Conference Proceedings (OSTI)

Suppose that both OPEC and the West possess stocks of oil which can be extracted at constant and identical cost. Consumption takes place only in the West. Suppose, hypothetically, that the West behaves as a single agent and, more realistically, that OPEC does also. Each agent makes a strategic choice of the pattern of exploitation over time of its own reserve. The Nash equilibrium obtained is ''robust'' in that it is also a ''Stakelberg equilibrium'' in which each agent is ''right for the right reason.'' Further, the equilibrium obtained is equivalent to that obtained when Western oil companies constitute a competitive fringe to the OPEC monopoly. 4 figures, 12 references

Robson, A.J.

1983-03-01T23:59:59.000Z

209

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

SciTech Connect

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

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

2007-11-02T23:59:59.000Z

210

Intercomparison and analyses of the climatology of the West African Monsoon in the West African Monsoon Modeling and Evaluation project (WAMME) first model intercomparison experiment  

E-Print Network (OSTI)

of the climatology of the West African Monsoon in theWest African Monsoon Modeling and Evaluation project (the West African Monsoon (WAM) Modeling and Evaluation

2010-01-01T23:59:59.000Z

211

West Texas Intermediate Spot Average ............................  

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

Crude Oil (dollars per barrel) Crude Oil (dollars per barrel) West Texas Intermediate Spot Average ............................ 102.88 93.42 92.24 87.96 94.34 94.10 105.84 96.30 95.67 95.33 95.67 93.33 94.12 97.64 95.00 Brent Spot Average ........................................................... 118.49 108.42 109.61 110.09 112.49 102.58 110.27 108.29 106.33 105.00 103.00 102.00 111.65 108.41 104.08 Imported Average .............................................................. 108.14 101.18 97.18 97.64 98.71 97.39 103.07 100.03 99.64 99.33 99.69 97.35 101.09 99.85 99.04 Refiner Average Acquisition Cost ...................................... 107.61 101.44 97.38 97.27 101.14 99.45 105.24 100.44 100.15 99.82 100.18 97.83 100.83 101.61 99.50 Liquid Fuels (cents per gallon) Refiner Prices for Resale Gasoline .........................................................................

212

WestStart CALSTART | Open Energy Information  

Open Energy Info (EERE)

WestStart CALSTART WestStart CALSTART Jump to: navigation, search Name WestStart-CALSTART Place Pasadena, California Zip 91106 Product String representation "WestStart-CALST ... nd create jobs." is too long. Coordinates 29.690847°, -95.196308° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.690847,"lon":-95.196308,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

213

West Virginia University | Department of Energy  

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

West Virginia University West Virginia University West Virginia University July 7, 2005 - 2:04pm Addthis Remarks by Energy Secretary Samuel Bodman Thank you, President Hardesty. I visited West Virginia last year when I was with the Treasury Department, and I am glad to be back today. President Hardesty has had a pretty busy week hosting visitors from Washington. President Bush was here on Monday, and I imagine many of you were in the audience for that. So I thank you for showing up for another speech a few days later. It is my pleasure to announce today that the Department of Energy is awarding almost $3 million in research funding, as part of our University Coal Research Program, to 19 universities in 15 states. Now in its 26th year, the University Coal Research Program brings science students and

214

West Virginia University | Department of Energy  

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

West Virginia University West Virginia University West Virginia University July 7, 2005 - 2:04pm Addthis Remarks by Energy Secretary Samuel Bodman Thank you, President Hardesty. I visited West Virginia last year when I was with the Treasury Department, and I am glad to be back today. President Hardesty has had a pretty busy week hosting visitors from Washington. President Bush was here on Monday, and I imagine many of you were in the audience for that. So I thank you for showing up for another speech a few days later. It is my pleasure to announce today that the Department of Energy is awarding almost $3 million in research funding, as part of our University Coal Research Program, to 19 universities in 15 states. Now in its 26th year, the University Coal Research Program brings science students and

215

West South Central | OpenEI  

Open Energy Info (EERE)

West South Central West South Central Dataset Summary Description This dataset comes from the Energy Information Administration (EIA), and is part of the 2011 Annual Energy Outlook Report (AEO2011). This dataset is table 7, and contains only the reference case. The dataset uses quadrillion btu. The data is broken down into residential, commercial, industrial, transportation, electric power and total energy consumption. Source EIA Date Released April 26th, 2011 (3 years ago) Date Updated Unknown Keywords 2011 AEO EIA Energy Consumption West South Central Data application/vnd.ms-excel icon AEO2011: Energy Consumption by Sector and Source - West South Central- Reference Case (xls, 297.7 KiB) Quality Metrics Level of Review Peer Reviewed Comment Temporal and Spatial Coverage Frequency Annually

216

West Stevens Wind | Open Energy Information  

Open Energy Info (EERE)

West Stevens Wind West Stevens Wind Facility West Stevens Wind Sector Wind energy Facility Type Commercial Scale Wind Facility Status Under Construction Developer West Stevens Wind Location 3 miles northwest of Chokio MN Coordinates 45.606472°, -96.238174° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":45.606472,"lon":-96.238174,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

217

west north central | OpenEI  

Open Energy Info (EERE)

west north central west north central Dataset Summary Description This dataset comes from the Energy Information Administration (EIA), and is part of the 2011 Annual Energy Outlook Report (AEO2011). This dataset is table 24, and contains only the reference case. The dataset uses million metric tons carbon dioxide equivalent. The data is broken down into residential, commercial, industrial, transportation, electric power, and total by fuel. Source EIA Date Released April 26th, 2011 (3 years ago) Date Updated Unknown Keywords 2011 AEO carbon dioxide emissions EIA west north central Data application/vnd.ms-excel icon AEO2011: Carbon Dioxide Emissions by Sector and Source - West North Central- Reference Case (xls, 74.3 KiB) Quality Metrics Level of Review Peer Reviewed Comment

218

TransWest Old | Open Energy Information  

Open Energy Info (EERE)

TransWest Old TransWest Old Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home NEPA Document Collection for: TransWest Old EIS at {{{GeothermalArea}}} for {{{GeothermalDevelopmentPhases}}} {{{NEPA_Name}}} General NEPA Document Info Environmental Analysis Type EIS Applicant Geothermal Area {{{GeothermalArea}}}"{{{GeothermalArea}}}" cannot be used as a page name in this wiki. Project Location Project Phase Techniques Time Frame (days) Participating Agencies Lead Agency none provided Funding Agency none provided Managing District Office none provided Managing Field Office none provided Funding Agencies none provided Surface Manager none provided Mineral Manager none provided Selected Dates Relevant Numbers Lead Agency Doc Number Retrieved from "http://en.openei.org/w/index.php?title=TransWest_Old&oldid=686707"

219

AMF Deployment, Niamey, Niger, West Africa  

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

West Africa West Africa Niamey Deployment AMF Home Niamey Home Data Plots and Baseline Instruments RADAGAST Website Rainfall Record (PDF) Publications List, (PDF) Experiment Planning RADAGAST Proposal Outreach Fact Sheets RADAGAST (PDF) Annual Climate Cycle in Niger, Africa (PDF) Posters AMF Poster, French Version We're Going to Sample the Sky in Africa! News Campaign Images AMMA International News AMF Deployment, Niamey, Niger, West Africa In 2006, the ARM Mobile Facility is collecting cloud and atmospheric property measurements from a location near the airport in Niamey, Niger, West Africa. Main Site: 13° 28' 39.15" N, 2° 10' 27.62" E Altitude: 205 meters Ancillary Site: 13° 31' 19.14" N, 2° 37' 56.46" E Altitude: 228.29 meters In January 2006, the second deployment of the ARM Mobile Facility (AMF)

220

Categorical Exclusion Determinations: West Valley Demonstration Project |  

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

Valley Demonstration Valley Demonstration Project Categorical Exclusion Determinations: West Valley Demonstration Project Categorical Exclusion Determinations issued by West Valley Demonstration Project. DOCUMENTS AVAILABLE FOR DOWNLOAD July 11, 2013 CX-010718: Categorical Exclusion Determination Replacement Ventilation System for the Main Plant Process Building CX(s) Applied: B6.3 Date: 07/11/2013 Location(s): New York Offices(s): West Valley Demonstration Project December 20, 2012 CX-009527: Categorical Exclusion Determination WVDP-2012-02 Routine Maintenance CX(s) Applied: B1.3 Date: 12/20/2012 Location(s): New York Offices(s): West Valley Demonstration Project August 2, 2012 CX-009528: Categorical Exclusion Determination WVDP-2012-01 WVDP Reservoir Interconnecting Canal Maintenance Activities

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


221

Environmental Justice Activities: Community Leaders' Institute, West  

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

Environmental Justice Activities: Community Leaders' Institute, Environmental Justice Activities: Community Leaders' Institute, West Columbia, South Carolina Environmental Justice Activities: Community Leaders' Institute, West Columbia, South Carolina July 13, 2012 - 3:06pm Addthis Environmental Justice Activities: Community Leaders' Institute, West Columbia, South Carolina What does this project do? Goal 1. Protect human health and the environment The Midlands Community Leaders' Institute (CLI), sponsored by the Medical University of South Carolina, the U.S. Department of Energy, U.S. Department of Defense, South Carolina State University, and Brookland Baptist Church was held in West Columbia, South Carolina, on July 13 and 14, 2012. The CLI continued to build on the theme Building and Sustaining Healthy Communities. A critical factor in the success of community development

222

West Winds Wind Farm | Open Energy Information  

Open Energy Info (EERE)

West Winds Wind Farm West Winds Wind Farm Facility West Winds Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Caithness Developer SeaWest Energy Purchaser Southern California Edison/PacifiCorp Location San Gorgonio CA Coordinates 33.9095°, -116.734° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.9095,"lon":-116.734,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

223

Mid-West Electric Consumers Association  

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

Mid-West Electric Consumers Association Mid-West Electric Consumers Association 4350 Wadsworth Blvd., Suite 330, Wheat Ridge, CO 80033 Tel: (303) 463-4979 Fax: (303) 463-8876 April 1, 2009 Transmission Infrastructure Program Western Area Power Administration P.O. Box 281213 Lakewood, CO 80228-8213 Comments on the Proposed Adoption of a Transmission Infrastructure Program The Mid-West Electric Consumers Association appreciates the opportunity to comment on the Western Area Power Administration's ("Western" or "WAPA") two Federal Register notices: Notice of Proposed Program and Request for Public Comments, and Notice of Availability of Request for Interest (FRN), published March 4, 2009 (pp. 9392-9393). The Mid-West Electric Consumers Association was founded in 1958 as the regional

224

From Higher Education To Work In West  

E-Print Network (OSTI)

1. Work Participation And Average Annualized Wages Of Graduates From West Virginia Public Higher .................................................................................................1 Results By Year And Residency ........................................................................................22 Appendix I: Detailed Description Of Employment Data .........................................29

Mohaghegh, Shahab

225

From Higher Education To Work In West  

E-Print Network (OSTI)

1. Work Participation And Average Annualized Wages In 2010 Of Graduates From West Virginia Public .................................................................................................1 Results By Year, Experience, Residency, And Degree............................................5.....................................................34 Appendix I: Detailed Description Of Employment Data .........................................35

Mohaghegh, Shahab

226

Dynamics of the West African Monsoon Jump  

Science Conference Proceedings (OSTI)

The observed abrupt latitudinal shift of maximum precipitation from the Guinean coast into the Sahel region in June, known as the West African monsoon jump, is studied using a regional climate model. Moisture, momentum, and energy budget analyses ...

Samson M. Hagos; Kerry H. Cook

2007-11-01T23:59:59.000Z

227

Corporate Headquarters Tax Credit (West Virginia)  

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

The Corporate Headquarters Tax Credit is available to companies who relocate their corporate headquarters to West Virginia and create 15 new jobs. The credit can offset up to 100% of the tax...

228

Qualifying RPS State Export Markets (West Virginia)  

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

This entry lists the states with Renewable Portfolio Standard (RPS) policies that accept generation located in West Virginia as eligible sources towards their RPS targets or goals. For specific...

229

The West Texas Mesonet: A Technical Overview  

Science Conference Proceedings (OSTI)

The West Texas Mesonet originated in 1999 as a project of Texas Tech University. The mesonet consists of 40 automated surface meteorological stations, two atmospheric profilers, and one upper-air sounding system. Each surface station measures up ...

J. L. Schroeder; W. S. Burgett; K. B. Haynie; I. Sonmez; G. D. Skwira; A. L. Doggett; J. W. Lipe

2005-02-01T23:59:59.000Z

230

Greater West Texas State Employee Charitable Campaign  

E-Print Network (OSTI)

together we changed lives Greater West Texas State Employee Charitable Campaign 2011 Annual Report campaign information 2011 Local Employee Committee Darcy Pollock (chair), Texas Tech University Health Sciences Center David Abercia, Texas Tech University Dianah Ascencio, Texas Department of Transportation

Rock, Chris

231

Effects of Cloud Seeding in West Texas  

Science Conference Proceedings (OSTI)

The effect of randomized seeding with droppable silver iodide (AgI) flares in West Texas during the Southwest Cooperative Program is addressed. Attention is focused on individual convective cells and on the small mesoscale convective clusters ...

Daniel Rosenfeld; William L. Woodley

1989-10-01T23:59:59.000Z

232

Linked Deposit Loan Program (West Virginia)  

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

The Linked Deposit Loan Program is targeted at small, private firms with 50 or fewer employees and gross annual revenues of $5 million or less comes. This loan offered through the West Virginia...

233

J WEST CIIIC.~G~,~LLINOIS  

Office of Legacy Management (LM)

---- "------' - J WEST CIIIC.G,LLINOIS 19th May, 1947 Mr. Frederick 1.1. Belmore U. S. Atomic Energy Commission Madison Square Area Post Office Box 42 l . Murray Hill Station...

234

NATIONAL AND GLOBAL FORECASTS WEST VIRGINIA PROFILES AND FORECASTS  

E-Print Network (OSTI)

· NATIONAL AND GLOBAL FORECASTS · WEST VIRGINIA PROFILES AND FORECASTS · ENERGY · HEALTHCARE Industry Insight: West Virginia Fiscal Forecast 34 CHAPTER 4: WEST ViRGiNiA'S 35 COUNTiES AND MSAs West Forecast Summary 2 CHAPTER 1: THE UNiTED STATES ECONOMY Figure 1.1: United States Real GDP Growth 3 Figure

Mohaghegh, Shahab

235

Weekly West Coast (PADD 5) Operable Crude Oil Distillation ...  

U.S. Energy Information Administration (EIA)

Weekly West Coast (PADD 5) Operable Crude Oil Distillation Capacity (Thousand Barrels per Calendar Day)

236

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

SciTech Connect

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

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

2013-08-01T23:59:59.000Z

237

Alternative Fuels Data Center: West Virginia Points of Contact  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

West Virginia Points West Virginia Points of Contact to someone by E-mail Share Alternative Fuels Data Center: West Virginia Points of Contact on Facebook Tweet about Alternative Fuels Data Center: West Virginia Points of Contact on Twitter Bookmark Alternative Fuels Data Center: West Virginia Points of Contact on Google Bookmark Alternative Fuels Data Center: West Virginia Points of Contact on Delicious Rank Alternative Fuels Data Center: West Virginia Points of Contact on Digg Find More places to share Alternative Fuels Data Center: West Virginia Points of Contact on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Points of Contact The following people or agencies can help you find more information about West Virginia's clean transportation laws, incentives, and funding

238

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

Science Conference Proceedings (OSTI)

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

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

2012-06-01T23:59:59.000Z

239

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

SciTech Connect

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

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

2012-07-15T23:59:59.000Z

240

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

E-Print Network (OSTI)

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

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

2012-01-01T23:59:59.000Z

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


241

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

E-Print Network (OSTI)

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

Zhiglo, Andrey V

2009-01-01T23:59:59.000Z

242

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

E-Print Network (OSTI)

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

unknown authors

2010-01-01T23:59:59.000Z

243

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

SciTech Connect

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

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

2012-02-10T23:59:59.000Z

244

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

E-Print Network (OSTI)

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

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

2004-08-12T23:59:59.000Z

245

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

E-Print Network (OSTI)

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

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

2004-01-15T23:59:59.000Z

246

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

SciTech Connect

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

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

2010-03-20T23:59:59.000Z

247

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

Science Conference Proceedings (OSTI)

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

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

2010-01-01T23:59:59.000Z

248

Alternative Fuels Data Center: West Virginia Laws and Incentives  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

West Virginia Laws and West Virginia Laws and Incentives to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives Listed below are incentives, laws, and regulations related to alternative

249

Far West Rice | Open Energy Information  

Open Energy Info (EERE)

West Rice West Rice Jump to: navigation, search Name Far West Rice Place Nelson, California Zip 95958 Sector Solar Product California-based family-owned rice mill. Owns a solar farm used mostly for the electricity needs of their factory. Coordinates 44.422864°, -92.009187° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.422864,"lon":-92.009187,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

250

West Central School Corp | Open Energy Information  

Open Energy Info (EERE)

School Corp School Corp Jump to: navigation, search Name West Central School Corp Facility West Central School Corp Sector Wind energy Facility Type Community Wind Facility Status In Service Owner West Central School Corp Developer Performance Services Energy Purchaser Net-metered Location Francesville IN Coordinates 41.02886641°, -86.89028978° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.02886641,"lon":-86.89028978,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

251

NETL: West Virginia Science Bowl Archive  

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

West Virginia Science Bowl Archive West Virginia Science Bowl Archive More media can be found on the National Science Bowl Website 2013 WVSB winner Morgantown HS places 4th at National Science Bowl Congratulations to Morgantown High School, champions of the 2012 WV Regional Science Bowl! We've got two news releases. A preview of our new buzzer system and an interview with WV Regional Science Bowl Coordinator Steve Woodruff, who passed the reins to Kirk Gerdes for 2012. 2012 2012 WV Regional Science Bowl Pictures [ZIP-21MB] 2012 WV Regional Science Bowl Team Pictures [ZIP-42MB] Two news items about planning the 2012 competition. 2011 2011 West Virginia Regional Science Bowl Results Press Release 2011 WV Regional Science Bowl Pictures [ZIP-8MB] 2011 WV Regional Science Bowl Team Pictures [ZIP-8MB]

252

NETL: Science Bowl Information - West Virginia - Overview  

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

Overview Overview CLICK ON IMAGE TO SEE LARGER VIEW Morgantown High, winners of the 2012 West Virginia Regional Science Bowl. From left, Nima Ronaghi, Samet Demircan, Dev Someshwar, Shiv Sunil, Andrew Maloney, and Joe Melia (coach). The U.S. Department of Energy National Science Bowl® is a nationwide competition held annually to promote science and technology in education. High school students compete as teams in an action-packed quiz bowl format to answer questions on science, math, and engineering. The West Virginia Regional Science Bowl® is one of many regional competitions held for high school teams across the country to select participants for the National Science Bowl held in Washington D.C. West Virginia students have represented the state admirably at the national

253

"Table HC14.13 Lighting Usage Indicators by West Census Region...  

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

3 Lighting Usage Indicators by West Census Region, 2005" " Million U.S. Housing Units" ,,"West Census Region" ,"U.S. Housing Units (millions)" ,,,"Census Division" ,,"Total West"...

254

GeoPowering the West: Geothermal Energy--The Bountiful, Clean Energy Source for the West  

DOE Green Energy (OSTI)

General fact sheet describing U.S. Department of Energy's GeoPowering the West program. Geothermal energy represents a major economic opportunity for the American West, an area characterized by a steadily increasing population that requires reliable sources of heat and power. GeoPowering the West is pursuing this opportunity by: (1) Bringing together national, state and local stakeholders for state-sponsored geothermal development workshops; (2) Working with public power companies and rural electric cooperatives to promote use of geothermal power; (3) Promoting increased federal use of geothermal energy; (4) Helping American Indians identify and develop geothermal resources on tribal lands; and (5) Sponsoring non-technical educational workshops.

Not Available

2002-04-01T23:59:59.000Z

255

West Virginia Recovery Act State Memo | Department of Energy  

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

West Virginia Recovery Act State Memo West Virginia Recovery Act State Memo West Virginia Recovery Act State Memo West Virginia has substantial natural resources, including coal and hydroelectric power. The American Recovery & Reinvestment Act (ARRA) is making a meaningful down payment on the nation's energy and environmental future. The Recovery Act investments in West Virginia are supporting a broad range of clean energy projects, from energy efficiency and the smart grid, to carbon capture and storage, transportation electrification, and the National Energy Technology Laboratory in Morgantown. Through these investments, West Virginia's businesses, West Virginia University, the National Energy Technology Laboratory, non-profits, and local governments are creating quality jobs today and positioning West Virginia to play an

256

Alternative Fuels Data Center: West Virginia Laws and Incentives  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

to someone by E-mail to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives Listed below are the summaries of all current West Virginia laws, incentives, regulations, funding opportunities, and other initiatives

257

West Valley Demonstration Project Waste Management Final Environmental Impact Statement  

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

WEST VALLEY DEMONSTRATION PROJECT WEST VALLEY DEMONSTRATION PROJECT WASTE MANAGEMENT ENVIRONMENTAL IMPACT STATEMENT FINAL SUMMARY December 2003 Prepared by: U.S. Department of Energy West Valley Area Office West Valley, NY DOE/EIS - 0337F For general questions or to request a copy of this EIS, please contact: DANIEL W. SULLIVAN, DOCUMENT MANAGER DOE WEST VALLEY AREA OFFICE 10282 Rock Springs Road WEST VALLEY, NY 14171-0191 1-800-633-5280 COVER SHEET Lead Agency: U.S. Department of Energy Title: Final West Valley Demonstration Project Waste Management Environmental Impact Statement, Cattaraugus County, West Valley, New York. Contact: For further information about this Environmental Impact Statement, contact: For general information on the Department of Energy's process for implementing the National

258

West Virginia/EZFeed Policies | Open Energy Information  

Open Energy Info (EERE)

Control Act (West Virginia) West Virginia Environmental Regulations Yes BiomassBiogas Coal with CCS Natural Gas StateProvince The purpose of this law is to provide for a...

259

The West Coast Thermal Trough: Climatology and Synoptic Evolution  

Science Conference Proceedings (OSTI)

Although the West Coast thermal trough (WCTT) is the most important mesoscale feature over the U.S. west coast during the warm season, its initiation, evolution, and structure are not well understood. Originating in the southwest United States, ...

Matthew C. Brewer; Clifford F. Mass; Brian E. Potter

2012-12-01T23:59:59.000Z

260

Climate of West Antarctica and Influence of Marine Air Intrusions  

Science Conference Proceedings (OSTI)

High-resolution numerical weather forecasts from the Antarctic Mesoscale Prediction System (AMPS) archive are used to investigate the climate of West Antarctica (WA) during 200607. A comparison with observations from West Antarctic automatic ...

Julien P. Nicolas; David H. Bromwich

2011-01-01T23:59:59.000Z

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


261

New Mexico--West Shale Proved Reserves (Billion Cubic Feet)  

Gasoline and Diesel Fuel Update (EIA)

View History: Annual Download Data (XLS File) New Mexico--West Shale Proved Reserves (Billion Cubic Feet) New Mexico--West Shale Proved Reserves (Billion Cubic Feet) Decade Year-0...

262

New Mexico--West Shale Production (Billion Cubic Feet)  

Gasoline and Diesel Fuel Update (EIA)

View History: Annual Download Data (XLS File) New Mexico--West Shale Production (Billion Cubic Feet) New Mexico--West Shale Production (Billion Cubic Feet) Decade Year-0 Year-1...

263

Exploring the context : a small hotel in Key West  

E-Print Network (OSTI)

This thesis develops a personal method and approach for designing in a delicate context such as the Key West Historic District. This thesis is composed of two parts. The first part presents observations of Key West, focusing ...

VanBeuzekom, Edrick

1984-01-01T23:59:59.000Z

264

West Virginia Datos del Precio de la Gasolina  

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

VirginiaGasPrices.com (Busqueda por Ciudad o Cdigo Postal) - GasBuddy.com West Virginia Gas Prices (Ciudades Selectas) - GasBuddy.com West Virginia Gas Prices (Organizado por...

265

oil and Gas Resources of the West Siberian Basin, Russia  

U.S. Energy Information Administration (EIA)

Energy Information Administration Oil and Gas Resources of the West Siberian Basin, Russia 139 Appendix D Field Summaries Tables 1D and 2D lists the fields of the West

266

PacifiCorp-West California ISO  

E-Print Network (OSTI)

PacifiCorp-West BANC SPP BANC BANC TID LADWP LADWP IID WALC California ISO Nevada Power Co. Nevada Power Co. BPA Balancing Authority Areas California Energy Commission 12/19/2011 Siting, Transmission Administration (BPA) California Independent System Operator (CAISO) Balancing Authority of Northern California

267

PacifiCorp-West California ISO  

E-Print Network (OSTI)

PacifiCorp-West BANC SPP BANC BANC TID LADWP LADWP IID WALC California ISO NV Energy NV Energy Balancing Authority Areas California Energy Commission 10/08/2012 Siting, Transmission and Environmental_A.mxd California Independent System Operator (CAISO) Balancing Authority of Northern California (BANC) Sierra

268

West Virginia University 1 Freshman Program  

E-Print Network (OSTI)

West Virginia University 1 Freshman Program Freshman Engineering Program The Benjamin M. Statler College of Engineering and Mineral Resources Freshman Engineering Program (FEP) is designed to support such as Microsoft Word ® , Excel ® , and Power Point ® , and MATLAB ® --to analyze, report, and present data; · Work

Mohaghegh, Shahab

269

Campus Security 1951 East-West Road  

E-Print Network (OSTI)

Campus Security 1951 East-West Road Honolulu, Hawai`i 96822 Telephone: (808) 956-9293 Fax: (808 First Female Campus Security Captain Alberta J.K. Pukahi Brings Unique Perspectives to the Position (HONOLULU, HI, December 10, 2012) University of Hawai`i at Mnoa's Campus Security and Emergency Management

270

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

E-Print Network (OSTI)

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

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

2006-01-19T23:59:59.000Z

271

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

Science Conference Proceedings (OSTI)

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

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

2010-03-01T23:59:59.000Z

272

West Virginia Percent of Historical Gas Wells by Production Rate ...  

U.S. Energy Information Administration (EIA)

West Virginia Percent of Historical Gas Wells by Production Rate Bracket. Energy Information Administration (U.S. Dept. of Energy)

273

West Virginia Percent of Historical Oil Wells by Production Rate ...  

U.S. Energy Information Administration (EIA)

West Virginia Percent of Historical Oil Wells by Production Rate Bracket. Energy Information Administration (U.S. Dept. of Energy)

274

West Texas Intermediate - U.S. Energy Information Administration (EIA)  

U.S. Energy Information Administration (EIA)

West Texas Intermediate Crude Oil Prices. Sources: History: EIA; Projections: Short-Term Energy Outlook, November 2000.

275

High-temperature hydrothermal systems in West Yunnan Province, China  

SciTech Connect

There are more than 660 thermal springs in West Yunnan Province, 30 of which are high-temperature hydrothermal systems with reservoir temperatures above 150/sup 0/C. All thermal springs in West Yunnan are under the control of tectonics, most of them distributed at anticlinoria of metamorphic rocks and granites. This paper discusses the relationship between thermal areas and tectonics, the correlation between thermal springs in West Yunnan and North Thailand, and the geothermal prospects in West Yunnan.

Laio, Z.; Tong, W.; Liu, S.; Zhao, F.

1986-01-01T23:59:59.000Z

276

West Coast (PADD 5) Refinery Operable Atmospheric Crude Oil ...  

U.S. Energy Information Administration (EIA)

West Coast (PADD 5) Refinery Operable Atmospheric Crude Oil Distillation Capacity as of January 1 (Barrels per Calendar Day)

277

LAX XXlCfl jX?iK, Idd+?KYLViG?IA  

Office of Legacy Management (LM)

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

278

Prospects for Type Ia Supernova explosion mechanism identification with gamma rays  

E-Print Network (OSTI)

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

Jordi Gomez-Gomar; Jordi Isern; Pierre Jean

1997-09-05T23:59:59.000Z

279

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

SciTech Connect

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

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

2012-10-01T23:59:59.000Z

280

Phenomenology for Supernova Ia Data Based on a New Cosmic Time  

E-Print Network (OSTI)

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

Charles B. Leffert

2007-07-26T23:59:59.000Z

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


281

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

E-Print Network (OSTI)

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

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

2012-01-01T23:59:59.000Z

282

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

Science Conference Proceedings (OSTI)

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

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

2004-01-12T23:59:59.000Z

283

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

E-Print Network (OSTI)

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

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

2006-01-01T23:59:59.000Z

284

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

SciTech Connect

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

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

2003-11-24T23:59:59.000Z

285

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

Science Conference Proceedings (OSTI)

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

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

2011-06-10T23:59:59.000Z

286

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

SciTech Connect

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

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

2009-10-10T23:59:59.000Z

287

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

SciTech Connect

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

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

2012-04-20T23:59:59.000Z

288

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

E-Print Network (OSTI)

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

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

2006-11-01T23:59:59.000Z

289

GeoPowering the West: Geothermal Energy--The West's Clean Energy Source  

DOE Green Energy (OSTI)

This ''calling card'' type brochure describes the GeoPowering the West (GPW) Initiative and activities, and lists critical contact information. This brochure serves as an introductory piece for anyone inquiring about the GPW initiative.

Not Available

2005-01-01T23:59:59.000Z

290

Title Pinnacle West Annual Board Meeting  

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

Tribal Energy Summit Tribal Energy Summit December 20, 2011 APS Renewable Energy Overall Commitment and Distributive Energy Program Arvin Trujillo 4CPP-Government Relations  APS has the 5 th Largest Service Territory in US & over 1M customers  Arizona is one of the fastest growing states in the nation  Energy demand will increase almost 50% in 20 yrs  Our customer growth has been 3 times U.S. Average  5,039 miles of transmission lines in APS territory About Arizona Public Service Co. "APS" APS Retail Service Territory Renewable Energy Standards in the U.S. State Goal ☼ PA: 18%¹ by 2020 ☼ NJ: 22.5% by 2021 CT: 23% by 2020 MA: 4% by 2009 + 1% annual increase WI: requirement varies by utility; 10% by 2015 goal IA: 105 MW MN: 25% by 2025

291

Spatio-temporal metamodeling for West African monsoon Anestis Antoniadisa  

E-Print Network (OSTI)

Spatio-temporal metamodeling for West African monsoon Anestis Antoniadisa , Céline Helberta in Western Africa : West African Monsoon. We are particularly interested in studying the influence of sea-temporal modeling, filtering, multivariate penalized regression 1. Introduction West African monsoon is the major

Paris-Sud XI, Université de

292

Spatio-temporal prediction for West African monsoon Anestis Antoniadisa  

E-Print Network (OSTI)

Spatio-temporal prediction for West African monsoon Anestis Antoniadisa , Céline Helberta in Western Africa : West African Monsoon. We are particularly interested in studying the influence of sea-temporal modeling, filtering, multivariate penalized regression 1. Introduction West African monsoon is the major

293

West Coast Aerial Sardine Survey Application for Exempted Fishing Permit  

E-Print Network (OSTI)

West Coast Aerial Sardine Survey 2011 Application for Exempted Fishing Permit Applicant Scientific Field Leader: Ryan Howe May 9, 2011 1 #12;West Coast Aerial Sardine Survey Application Requirements ................... 51 2 #12;West Coast Aerial Sardine Survey Application for Exempted Fishing

294

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

E-Print Network (OSTI)

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

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

2006-06-28T23:59:59.000Z

295

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

E-Print Network (OSTI)

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

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

2010-01-01T23:59:59.000Z

296

Intercomparison and analyses of the climatology of the West African Monsoon in the West African Monsoon Modeling and Evaluation  

E-Print Network (OSTI)

Intercomparison and analyses of the climatology of the West African Monsoon in the West African Monsoon Modeling and Evaluation project (WAMME) first model intercomparison experiment Yongkang Xue This paper briefly presents the West African Monsoon (WAM) Modeling and Evaluation Project (WAMME

Xue, Yongkang

297

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

Science Conference Proceedings (OSTI)

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

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

2010-01-01T23:59:59.000Z

298

Site Programs & Cooperative Agreements: West Valley Demonstration Project |  

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

West Valley Demonstration West Valley Demonstration Project Site Programs & Cooperative Agreements: West Valley Demonstration Project West Valley Demonstration Project The Seneca Nation of Indians has interests and concerns regarding the West Valley Demonstration Project Site. Like at Hanford, DOE environmental cleanup activities have the potential to impact natural and cultural resources and to interfere with American Indian religious practices. Through a cooperative agreement, tribal staff is engaged on a frequent basis with DOE and its contractors. The principle activities engaged by tribes include reviewing and commenting on plans and documents, participating in meetings at the request of DOE, monitoring cultural resource sites, participating in site surveys, and identifying issues that

299

Kyoto Protocol: Enforcement Prohibitions (West Virginia) | Department of  

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

Kyoto Protocol: Enforcement Prohibitions (West Virginia) Kyoto Protocol: Enforcement Prohibitions (West Virginia) Kyoto Protocol: Enforcement Prohibitions (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Climate Policies The West Virginia division of environmental protection shall refrain from proposing or promulgating any new rule intended, in whole or in part, to reduce emissions of greenhouse gases from the residential, commercial,

300

West Valley Demonstration Project Phase I Decommissioning - Facility  

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

Project Phase I Decommissioning - Project Phase I Decommissioning - Facility Disposition Partnering Performance Agreement West Valley Demonstration Project Phase I Decommissioning - Facility Disposition Partnering Performance Agreement The Department of Energy, West Valley Demonstration Project (DOE-WVDP) and CH2M Hill B&W West Valley (CHBWV) are committed to continuous improvement and will utilize principles of the DOE Environmental Management (DOE-EM) Partnering Policy to create and foster a team environment to successfully complete the West Valley Demonstration Project (WVDP) Phase I Decommissioning - Faciltiy Disposition. West Valley Demonstration Project Phase I Decommissioning - Facility Disposition Partnering Performance Agreement More Documents & Publications CX-009527: Categorical Exclusion Determination

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301

Underground Gas Storage Reservoirs (West Virginia) | Department of Energy  

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

Gas Storage Reservoirs (West Virginia) Gas Storage Reservoirs (West Virginia) Underground Gas Storage Reservoirs (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Safety and Operational Guidelines Provider West Virginia Department of Commerce Lays out guidelines for the conditions under which coal mining operations must notify state authorities of intentions to mine where underground gas

302

West Valley Demonstration Project Waste Management Environmental Impact Statement  

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

April 2003 Prepared by: U.S. Department of Energy West Valley Area Office West Valley, NY For general questions or to request a copy of this EIS, please contact: DANIEL W. SULLIVAN, DOCUMENT MANAGER DOE-WEST VALLEY AREA OFFICE P.O. BOX 191 WEST VALLEY, NY 14171-0191 1-800-633-5280 COVER SHEET Lead Agency: U.S. Department of Energy Title: Draft West Valley Demonstration Project Waste Management Environmental Impact Statement, Cattaraugus County, West Valley, New York. Contact: For further information about this Environmental Impact Statement, contact: For general information on the Department of Energy's process for implementing the National Environmental Policy Act, contact: Daniel W. Sullivan Document Manager DOE-West Valley Area Office

303

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Ethanol to someone by E-mail Ethanol to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Ethanol on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives for Ethanol

304

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Rebates to someone by E-mail Rebates to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Rebates on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives for Rebates

305

West Valley Demonstration Project Waste Management Environmental Impact Statement  

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

SUMMARY April 2003 Prepared by: U.S. Department of Energy West Valley Area Office West Valley, NY For general questions or to request a copy of this EIS, please contact: DANIEL W. SULLIVAN, DOCUMENT MANAGER DOE WEST VALLEY AREA OFFICE P.O. BOX 191 WEST VALLEY, NY 14171-0191 1-800-633-5280 COVER SHEET Lead Agency: U.S. Department of Energy Title: Draft West Valley Demonstration Project Waste Management Environmental Impact Statement, Cattaraugus County, West Valley, New York. Contact: For further information about this Environmental Impact Statement, contact: For general information on the Department of Energy's process for implementing the National Environmental Policy Act, contact: Daniel W. Sullivan Document Manager DOE West Valley Area Office

306

Wind Energy Systems Technologies LLC WEST | Open Energy Information  

Open Energy Info (EERE)

LLC WEST LLC WEST Jump to: navigation, search Name Wind Energy Systems Technologies LLC (WEST) Place New Iberia, Louisiana Sector Wind energy Product Wants to install wind turbines on abandoned Gulf of Mexico oil and natural gas platforms to generate electric power for both homes and secondary recovery efforts. References Wind Energy Systems Technologies LLC (WEST)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Wind Energy Systems Technologies LLC (WEST) is a company located in New Iberia, Louisiana . References ↑ "Wind Energy Systems Technologies LLC (WEST)" Retrieved from "http://en.openei.org/w/index.php?title=Wind_Energy_Systems_Technologies_LLC_WEST&oldid=353071

307

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Natural Gas to someone by E-mail Natural Gas to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Natural Gas on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives for Natural Gas

308

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Biodiesel to someone by E-mail Biodiesel to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Biodiesel on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives for Biodiesel

309

Clean Cities: State of West Virginia Clean Cities coalition  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

State of West Virginia Clean Cities Coalition State of West Virginia Clean Cities Coalition The State of West Virginia Clean Cities coalition works with vehicle fleets, fuel providers, community leaders, and other stakeholders to reduce petroleum use in transportation. State of West Virginia Clean Cities coalition Contact Information Kelly Bragg 800-982-3386 x2004 or 304-558-2234 x2004 kelly.a.bragg@wv.gov Casey Randolph 800-982-3386 casey.e.randolph@wv.gov Coalition Website Clean Cities Coordinators Coord Kelly Bragg Coord Coord Casey Randolph Coord Photo of Kelly Bragg Kelly Bragg has been the coordinator of the State of West Virginia Clean Cities coalition and an energy development specialist for the West Virginia Division of Energy since 2006. She works to improve energy efficiency and the use of renewable energy technologies in West Virginia. Her recent focus

310

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Propane (LPG) to someone by E-mail Propane (LPG) to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Propane (LPG) on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type West Virginia Laws and Incentives for Propane (LPG)

311

Groundwater Protection Rules Coal Mining Operations (West Virginia) |  

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

Protection Rules Coal Mining Operations (West Virginia) Protection Rules Coal Mining Operations (West Virginia) Groundwater Protection Rules Coal Mining Operations (West Virginia) < Back Eligibility Utility Commercial Investor-Owned Utility Industrial Municipal/Public Utility Local Government Rural Electric Cooperative Tribal Government Institutional Nonprofit Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection These rules establish a series of practices for the protection of groundwater which are to be followed by any person who conducts coal mining operations subject to the provisions of West Virginia Groundwater Protection Act and subject to regulation under the West Virginia Coal Mining and Reclamation Act and/or under West Virginia Water Pollution

312

THE DETONATION MECHANISM OF THE PULSATIONALLY ASSISTED GRAVITATIONALLY CONFINED DETONATION MODEL OF Type Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

We describe the detonation mechanism composing the 'pulsationally assisted' gravitationally confined detonation (GCD) model of Type Ia supernovae. This model is analogous to the previous GCD model reported in Jordan et al.; however, the chosen initial conditions produce a substantively different detonation mechanism, resulting from a larger energy release during the deflagration phase. The resulting final kinetic energy and {sup 56}Ni yields conform better to observational values than is the case for the 'classical' GCD models. In the present class of models, the ignition of a deflagration phase leads to a rising, burning plume of ash. The ash breaks out of the surface of the white dwarf, flows laterally around the star, and converges on the collision region at the antipodal point from where it broke out. The amount of energy released during the deflagration phase is enough to cause the star to rapidly expand, so that when the ash reaches the antipodal point, the surface density is too low to initiate a detonation. Instead, as the ash flows into the collision region (while mixing with surface fuel), the star reaches its maximally expanded state and then contracts. The stellar contraction acts to increase the density of the star, including the density in the collision region. This both raises the temperature and density of the fuel-ash mixture in the collision region and ultimately leads to thermodynamic conditions that are necessary for the Zel'dovich gradient mechanism to produce a detonation. We demonstrate feasibility of this scenario with three three-dimensional (3D), full star simulations of this model using the FLASH code. We characterized the simulations by the energy released during the deflagration phase, which ranged from 38% to 78% of the white dwarf's binding energy. We show that the necessary conditions for detonation are achieved in all three of the models.

Jordan, G. C. IV; Graziani, C.; Weide, K.; Norris, J.; Hudson, R.; Lamb, D. Q. [Flash Center for Computational Science, University of Chicago, Chicago, IL 60637 (United States); Fisher, R. T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States); Townsley, D. M. [Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487 (United States); Meakin, C. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Reid, L. B. [NTEC Environmental Technology, Subiaco WA 6008 (Australia)

2012-11-01T23:59:59.000Z

313

Three-dimensional numerical simulations of Rayleigh-Taylorunstable flames in type Ia supernovae  

SciTech Connect

Flame instabilities play a dominant role in accelerating the burning front to a large fraction of the speed of sound in a Type Ia supernova. We present a three-dimensional numerical simulation of a Rayleigh-Taylor unstable carbon flame, following its evolution through the transition to turbulence. A low Mach number hydrodynamics method is used, freeing us from the harsh time step restrictions imposed by sound waves. We fully resolve the thermal structure of the flame and its reaction zone, eliminating the need for a flame model. A single density is considered, 1.5x107 gm/cc, and half carbon/half oxygen fuel--conditions under which the flame propagated in the flamelet regime in our related two-dimensional study. We compare to a corresponding two-dimensional simulation, and show that while fire-polishing keeps the small features suppressed in two dimensions, turbulence wrinkles the flame on far smaller scales in the three-dimensional case, suggesting that the transition to the distributed burning regime occurs at higher densities in three dimensions. Detailed turbulence diagnostics are provided. We show that the turbulence follows a Kolmogorov spectrum and is highly anisotropic on the large scales, with a much larger integral scale in the direction of gravity. Furthermore, we demonstrate that it becomes more isotropic as it cascades down to small scales. Based on the turbulent statistics and the flame properties of our simulation, we compute the Gibson scale. We show the progress of the turbulent flame through a classic combustion regime diagram, indicating that the flame just enters the distributed burning regime near the end of our simulation.

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

2005-01-28T23:59:59.000Z

314

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

E-Print Network (OSTI)

The physical structure of a nuclear flame is a basic ingredient of the theory of Type Ia supernovae (SNIa). Assuming an exponential density reduction with several characteristic times we have followed the evolution of a planar nuclear flame in an expanding background from an initial density 6.6 10^7 g/cm3 down to 2 10^6 g/cm3. The total amount of synthesized intermediate-mass elements (IME), from silicon to calcium, was monitored during the calculation. We have made use of the computed mass fractions, X_IME, of these elements to give an estimation of the total amount of IME synthesized during the deflagration of a massive white dwarf. Using X_IME and adopting the usual hypothesis that turbulence decouples the effective burning velocity from the laminar flame speed, so that the relevant flame speed is actually the turbulent speed on the integral length-scale, we have built a simple geometrical approach to model the region where IME are thought to be produced. It turns out that a healthy production of IME involves the combination of not too short expansion times, t_c > 0.2 s, and high turbulent intensities. According to our results it could be difficult to produce much more than 0.2 solar masses of intermediate-mass elements within the deflagrative paradigma. The calculations also suggest that the mass of IME scales with the mass of Fe-peak elements, making it difficult to conciliate energetic explosions with low ejected nickel masses, as in the well observed SN1991bg or in SN1998de. Thus a large production of Si-peak elements, especially in combination with a low or a moderate production of iron, could be better addressed by either the delayed detonation route in standard Chandrasekhar-mass models or, perhaps, by the off-center helium detonation in the sub Chandrasekhar-mass scenario.

D. Garcia-Senz; E. Bravo; R. M. Cabezon; S. E. Woosley

2006-09-15T23:59:59.000Z

315

Revealing Type Ia supernova physics with cosmic rates and nuclear gamma rays  

E-Print Network (OSTI)

Type Ia supernovae (SNIa) remain mysterious despite their central importance in cosmology and their rapidly increasing discovery rate. The progenitors of SNIa can be probed by the delay time between progenitor birth and explosion as SNIa. The explosions and progenitors of SNIa can be probed by MeV nuclear gamma rays emitted in the decays of radioactive nickel and cobalt into iron. We compare the cosmic star formation and SNIa rates, finding that their different redshift evolution requires a large fraction of SNIa to have large delay times. A delay time distribution of the form t^{-1.0 +/- 0.3} provides a good fit, implying 50% of SNIa explode more than ~ 1 Gyr after progenitor birth. The extrapolation of the cosmic SNIa rate to z = 0 agrees with the rate we deduce from catalogs of local SNIa. We investigate prospects for gamma-ray telescopes to exploit the facts that escaping gamma rays directly reveal the power source of SNIa and uniquely provide tomography of the expanding ejecta. We find large improvements relative to earlier studies by Gehrels et al. in 1987 and Timmes & Woosley in 1997 due to larger and more certain SNIa rates and advances in gamma-ray detectors. The proposed Advanced Compton Telescope, with a narrow-line sensitivity ~ 60 times better than that of current satellites, would, on an annual basis, detect up to ~ 100 SNIa (3 sigma) and provide revolutionary model discrimination for SNIa within 20 Mpc, with gamma-ray light curves measured with ~ 10 sigma significance daily for ~ 100 days. Even more modest improvements in detector sensitivity would open a new and invaluable astronomy with frequent SNIa gamma-ray detections.

Shunsaku Horiuchi; John F. Beacom

2010-06-30T23:59:59.000Z

316

Mid West Energy | Open Energy Information  

Open Energy Info (EERE)

Energy Energy Jump to: navigation, search Name Mid West Energy Place Perth, Western Australia, Australia Zip WA 6005 Sector Solar Product Western Australian-based Mid West Energy is proposing to build a 200MW solar thermal plant near Perenjori. Coordinates -31.95302°, 115.857239° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":-31.95302,"lon":115.857239,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

317

Asia West LLC | Open Energy Information  

Open Energy Info (EERE)

LLC LLC Jump to: navigation, search Logo: Asia West LLC Name Asia West LLC Address One East Weaver Street Place Greenwich, Connecticut Zip 06831 Region Northeast - NY NJ CT PA Area Product Strategic investor in environmental technologies. Phone number (203) 983-6300 Website http://www.asiawestfunds.com/ Coordinates 41.017605°, -73.649147° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.017605,"lon":-73.649147,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

318

West Virginia Underground Natural Gas Storage Capacity  

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

Alaska Lower 48 States Alabama Arkansas California Colorado Illinois Indiana Iowa Kansas Kentucky Louisiana Maryland Michigan Minnesota Mississippi Missouri Montana Nebraska New Mexico New York Ohio Oklahoma Oregon Pennsylvania Tennessee Texas Utah Virginia Washington West Virginia Wyoming AGA Producing Region AGA Eastern Consuming Region AGA Western Consuming Region Period: Monthly Annual Alaska Lower 48 States Alabama Arkansas California Colorado Illinois Indiana Iowa Kansas Kentucky Louisiana Maryland Michigan Minnesota Mississippi Missouri Montana Nebraska New Mexico New York Ohio Oklahoma Oregon Pennsylvania Tennessee Texas Utah Virginia Washington West Virginia Wyoming AGA Producing Region AGA Eastern Consuming Region AGA Western Consuming Region Period: Monthly Annual Download Series History Download Series History Definitions, Sources & Notes Definitions, Sources & Notes Show Data By: Data Series Area Apr-13 May-13 Jun-13 Jul-13 Aug-13 Sep-13 View

319

West Central Cooperative | Open Energy Information  

Open Energy Info (EERE)

West Central Cooperative West Central Cooperative Place Ralston, Iowa Zip 51459 Product Iowa-based agri-business with operations across the United States. Involved in the production of biodiesel. Coordinates 44.71762°, -108.864694° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.71762,"lon":-108.864694,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

320

West Penn Power Co | Open Energy Information  

Open Energy Info (EERE)

West Penn Power Co West Penn Power Co Place Pennsylvania Utility Id 20387 Utility Location Yes Ownership I NERC Location RFC NERC RFC Yes RTO PJM Yes Activity Transmission Yes Activity Distribution Yes Activity Wholesale Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png 10 (Residential Service) Residential 20 (General Service) Commercial 30 (General Power Service >500kW) Commercial 30 (General Power Service 100kW-500kW) Commercial Average Rates Residential: $0.0291/kWh Commercial: $0.0110/kWh Industrial: $0.0058/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a"

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321

West Holt Wind Project | Open Energy Information  

Open Energy Info (EERE)

Holt Wind Project Holt Wind Project Jump to: navigation, search Name West Holt Wind Project Facility West Holt Sector Wind energy Facility Type Community Wind Location NE Coordinates 42.540997°, -98.978706° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.540997,"lon":-98.978706,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

322

Benchmark West Texas Intermediate crude assayed  

Science Conference Proceedings (OSTI)

The paper gives an assay of West Texas Intermediate, one of the world's market crudes. The price of this crude, known as WTI, is followed by market analysts, investors, traders, and industry managers around the world. WTI price is used as a benchmark for pricing all other US crude oils. The 41[degree] API WTI posted prices is the price paid for the crude at the wellhead in West Texas and is the true benchmark on which other US crudes are priced. The spot price is the negotiated price for short-term trades of the crude. And the New York Mercantile Exchange, or Nymex, price is a futures price for barrels delivered at Cushing.

Rhodes, A.K.

1994-08-15T23:59:59.000Z

323

Dylan Jones, President & CEO Canada West Foundation  

E-Print Network (OSTI)

's Crude Oil and North American Demand in 2011 Source: CAPP, EIA, Statistics Canada #12;US oil production and overseas crude oil prices. Sources: US EIA, CERI, Canada West Foundation. 0 20 40 60 80 100 120 140 160 Jul-07 Jan-08 Jul-08 Jan-09 Jul-09 Jan-10 Jul-10 Jan-11 Jul-11 Jan-12 Jul-12 US$/b Crude Oil Benchmark

Peak, Derek

324

Some Lizards of the Middle West  

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

Lizards of the Middle West Lizards of the Middle West Nature Bulletin No. 344-A May 10, 1969 Forest Preserve District of Cook County George W. Dunne, President Roland F. Eisenbeis, Supt. of Conservation SOME LIZARDS OF THE MIDDLE WEST More than 2,500 kinds of lizards are now known in the world, and they vary more widely in size, shape, color and habit than any of the other three groups of reptiles -- the snakes, the turtles and the alligators. Three kinds of lizards are known to live within 50 miles of Chicago but they are so scarce, and so wary or secretive, that the total number found by all the reptile enthusiasts is often only one or two a year. Farther south they become more common and farm boys know them well. Lizards, having dry scaly skins that they shed from time to time, should not be confused with the salamanders which, altho also four- legged and cold-blooded, are amphibians -- not reptiles -- and have moist smooth skins. The only live lizards that most of us ever see are in the zoos, notably the sluggish Gila Monster which is one of the only two poisonous species; or a friendly little Horned "Toad" which someone may have brought back from the Southwest; or one of those little American chameleons sometimes sold at carnivals or county fairs in states where that is still permitted.

325

Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations  

E-Print Network (OSTI)

The light curve of a type Ia supernova decays at a rate set by the beta-decay lifetimes of the Ni-56 and Co-56 produced in the explosion. This makes such a light curve sensitive to the value of the Fermi constant G_F at the time of the supernova. Using data from the CfA Supernova Archive, we measure the dependence of the light curve decay rate on redshift and place a bound on the time variation of G_F of |(dG_F/dt)/G_F| < 10^(-9) / y.

Ferrero, Alejandro

2010-01-01T23:59:59.000Z

326

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Vehicle Owner/Driver to someone by E-mail Vehicle Owner/Driver to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Vehicle Owner/Driver on AddThis.com... More in this section... Federal State Advanced Search

327

Governor's Guaranteed Work Force Program (West Virginia) | Department of  

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

Governor's Guaranteed Work Force Program (West Virginia) Governor's Guaranteed Work Force Program (West Virginia) Governor's Guaranteed Work Force Program (West Virginia) < Back Eligibility Commercial Savings Category Alternative Fuel Vehicles Hydrogen & Fuel Cells Buying & Making Electricity Water Home Weatherization Solar Wind Program Info State West Virginia Program Type Workforce development Small, medium and large West Virginia private-for-profit businesses, including but not limited to: Energy, Technology, Aerospace, Automotive, Business Services, Chemicals/Plastics, Metals, Tourist Destinations, Wood Products, Biometrics, Biotech, Food Products, Printing and Warehouse/Distribution are eligible to be reimbursed for expenses incurred when training new employees. Under this program, the West Virginia Development Office can pay up to 100% or $2,000 per trainee, whichever is

328

Independent Activity Report, West Valley Demonstration Project - November  

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

Activity Report, West Valley Demonstration Project - Activity Report, West Valley Demonstration Project - November 2011 Independent Activity Report, West Valley Demonstration Project - November 2011 November 2011 West Valley Demonstration Project Orientation Visit [HIAR-WVDP-2011-11-07] The U.S. Department of Energy (DOE) Office of Enforcement and Oversight, within the Office of Health, Safety and Security (HSS), conducted an orientation visit to the DOE West Valley Demonstration Project (WVDP) Office and the nuclear facility at West Valley, NY, on November 7, 2011. The purpose of the visit was to discuss the nuclear safety oversight strategy, describe the site lead program, increase HSS personnel's operational awareness of the site's activities, and identify specific activities that HSS can perform to carry out its independent oversight

329

West Valley Demonstration Project 10282 Rock Springs Road  

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

West Valley Demonstration Project West Valley Demonstration Project 10282 Rock Springs Road West Valley, NY 141 71 -9799 Mr. Daniel W. Coyne President & General Manager CH2M HILL B&W West Valley, LLC West Valley Demonstration Project 10282 Rock Springs Road West Valley, NY 141 71 -9799 ATTENTION: J. D. Rendall, Regulatory Strategy, AC-EA SUBJECT: Environmental Checklist WVDP-20 12-0 1, " WVDP Reservoir Interconnecting Canal Maintenance Activities" REFERENCE: Letter WD:2012:0409 (357953), D. W. Coyne to R. W. Reffner, "CONTRACT NO. DE-EM000 1529, Section 5-3, Item 105, NEPA Documentation (Transmittal of Environmental Checklist WVDP-20 12-0 1, WVDP Reservoir Interconnecting Canal Maintenance Activities), Revision 1 ," dated July 24, 20 12 Dear Mr. Coyne:

330

Training Changing Face of West Virginia's Workforce | Department of  

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

Training Changing Face of West Virginia's Workforce Training Changing Face of West Virginia's Workforce Training Changing Face of West Virginia's Workforce January 12, 2010 - 12:41pm Addthis Joshua DeLung West Virginia is wild and wonderful, known for its rushing whitewater, luscious valleys and John Denver's country roads. The state that powers 33 others and the District of Columbia is getting ready for the clean energy economy. New River Community and Technical College is training the workforce - and more trainers - in measures used to weatherize American homes. With 3,700 homes slated to be weatherized in West Virginia under the Recovery Act, educating enough trainers to teach the large workforce is a daunting challenge that its community colleges are eager to meet. West Virginia's stimulus funding is expected to spur green jobs and build

331

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Acquisition / Fuel Use to someone by E-mail Acquisition / Fuel Use to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Acquisition / Fuel Use on AddThis.com... More in this section... Federal

332

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Producer to someone by E-mail Producer to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Alternative Fuel Producer on AddThis.com... More in this section... Federal

333

Scott Runnels of Computational Physics to teach at West Point  

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

Scott Runnels to teach at West Point Scott Runnels to teach at West Point Scott Runnels of Computational Physics to teach at West Point Runnels has been selected for a two-year faculty post in the Department of Physics and Nuclear Engineering at West Point. March 19, 2013 Scott Runnels Scott Runnels Contact Kevin Roark Communications Office (505) 665-9202 Email I'm sure this exchange will have tremendous benefits for both West Point and the Laboratory, and it continues a relationship with the Army that began more than 70 years ago with the Manhattan Project. LOS ALAMOS, N. M., March 19, 2013- Under an agreement between Los Alamos National Laboratory and the U.S. Military Academy, Scott Runnels has been selected for a two-year faculty post in the Department of Physics and Nuclear Engineering at West Point.

334

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Driving / Idling to someone by E-mail Driving / Idling to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Driving / Idling on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type

335

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Aftermarket Conversions to someone by E-mail Aftermarket Conversions to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Aftermarket Conversions on AddThis.com... More in this section...

336

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Hydrogen Fuel Cells to someone by E-mail Hydrogen Fuel Cells to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Hydrogen Fuel Cells on AddThis.com... More in this section... Federal State Advanced Search

337

Categorical Exclusion Determinations: West Virginia | Department of Energy  

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

West Virginia West Virginia Categorical Exclusion Determinations: West Virginia Location Categorical Exclusion Determinations issued for actions in West Virginia. DOCUMENTS AVAILABLE FOR DOWNLOAD September 25, 2013 CX-010926: Categorical Exclusion Determination Development of Integrated Biomimetic Framework with Intelligent Monitoring, Cognition, and Decision... CX(s) Applied: A9 Date: 09/25/2013 Location(s): West Virginia Offices(s): National Energy Technology Laboratory September 17, 2013 CX-010953: Categorical Exclusion Determination Building 28 Demolition CX(s) Applied: B1.23 Date: 09/17/2013 Location(s): West Virginia Offices(s): National Energy Technology Laboratory September 17, 2013 CX-010950: Categorical Exclusion Determination Building 30 (B-30) Demolition CX(s) Applied: B1.16, B1.23

338

West Valley Demolition Marks Important Accomplishment for EM | Department  

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

West Valley Demolition Marks Important Accomplishment for EM West Valley Demolition Marks Important Accomplishment for EM West Valley Demolition Marks Important Accomplishment for EM June 13, 2013 - 12:00pm Addthis Workers demolish the West Valley Demonstration Project's largest and most complex ancillary facility. Workers demolish the West Valley Demonstration Project's largest and most complex ancillary facility. Demolition work is shown in February 2013. Demolition work is shown in February 2013. Demolition continues in April 2013 with removal of internal components and concrete cell walls. Demolition continues in April 2013 with removal of internal components and concrete cell walls. Debris is removed following demolition. Debris is removed following demolition. Workers demolish the West Valley Demonstration Project's largest and most complex ancillary facility.

339

Enforcement Letter, West Valley Nuclear Services - March 30, 1998 |  

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

West Valley Nuclear Services - March 30, 1998 West Valley Nuclear Services - March 30, 1998 Enforcement Letter, West Valley Nuclear Services - March 30, 1998 March 30, 1998 Issued to West Valley Nuclear Services related to Hazard Analysis, Design Review, Work Control Implementation, and a Contamination Event at the West Valley Demonstration Project This letter refers to the Department of Energy's (DOE) evaluation of West Valley Nuclear Services Company's (WVNS) report of a potential noncompliance with the requirements of 10 CFR 830.120 (Quality Assurance) and 10 CFR 835 (Occupational Radiation Protection). This potential noncompliance, which involved inadequate hazards analysis, design review, and implementation of work controls during decontamination activities for a high-level waste tank mobilization pump, was identified by WVNS on

340

Independent Activity Report, West Valley Demonstration Project - July 2012  

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

West Valley Demonstration Project - West Valley Demonstration Project - July 2012 Independent Activity Report, West Valley Demonstration Project - July 2012 July 2012 Operational Awareness Oversight of the West Valley Demonstration Project [HIAR WVDP-2012-07-30] The purpose of this Office of Health, Safety and Security (HSS) activity was for the HS-45 Site Lead to meet with Department of Energy (DOE) site personnel, tour the facilities, and obtain a status report on the upcoming activities at the West Valley Demonstration Project (WVDP). In the fall of 2011, a new contractor, CH2M Hill-B&W West Valley (CHBWV), was selected to perform site operations for Phase 1 decommissioning and facility disposition, including the Main Plant Process Building, the Low-Level Waste Treatment Facility, and other facilities.

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


341

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Climate Change / Energy Initiatives to someone by E-mail Climate Change / Energy Initiatives to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Climate Change / Energy Initiatives on

342

Alternative Fuels Data Center: West Virginia Laws and Incentives for  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Fueling / TSE Infrastructure Owner to someone by E-mail Fueling / TSE Infrastructure Owner to someone by E-mail Share Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on Facebook Tweet about Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on Twitter Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on Google Bookmark Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on Delicious Rank Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on Digg Find More places to share Alternative Fuels Data Center: West Virginia Laws and Incentives for Fueling / TSE Infrastructure Owner on

343

Training Changing Face of West Virginia's Workforce | Department of  

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

Changing Face of West Virginia's Workforce Changing Face of West Virginia's Workforce Training Changing Face of West Virginia's Workforce January 12, 2010 - 12:41pm Addthis Joshua DeLung West Virginia is wild and wonderful, known for its rushing whitewater, luscious valleys and John Denver's country roads. The state that powers 33 others and the District of Columbia is getting ready for the clean energy economy. New River Community and Technical College is training the workforce - and more trainers - in measures used to weatherize American homes. With 3,700 homes slated to be weatherized in West Virginia under the Recovery Act, educating enough trainers to teach the large workforce is a daunting challenge that its community colleges are eager to meet. West Virginia's stimulus funding is expected to spur green jobs and build

344

ARM - Field Campaign - ARM West Antarctic Radiation Experiment  

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

govCampaignsARM West Antarctic Radiation Experiment govCampaignsARM West Antarctic Radiation Experiment Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : ARM West Antarctic Radiation Experiment 2015.10.01 - 2016.03.31 Lead Scientist : Dan Lubin Description West Antarctica is one of the most rapidly warming regions on Earth, and this warming is closely connected with global sea level rise. The discovery of rapid climate change on the West Antarctic Ice Sheet (WAIS) has challenged previous explanations of Antarctic climate change that focused on strengthening of circumpolar westerlies in response to the positive polarity trend in the Southern Annular Mode. West Antarctic warming does not yet have a comprehensive explanation: dynamical mechanisms may vary

345

Gas Pipeline Safety (West Virginia) | Department of Energy  

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

Pipeline Safety (West Virginia) Pipeline Safety (West Virginia) Gas Pipeline Safety (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Safety and Operational Guidelines Provider Public Service Commission of West Virginia The Gas Pipeline Safety Section of the Engineering Division is responsible for the application and enforcement of pipeline safety regulations under Chapter 24B of the West Virginia Code and 49 U.S.C. Chapter 601,

346

Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey  

E-Print Network (OSTI)

We use type-Ia supernovae (SNe Ia) discovered by the SDSS-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host galaxy center, using the distance as a proxy for local galaxy properties (local star-formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light-curves using both MLCS2k2 and SALT2, and determine color (AV, c) and light-curve shape (delta, x1) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4-sigma level) finding is that the average fitted AV from MLCS2k2 and c from SALT2 decrease with the proj...

Galbany, Lluis; Ostman, Linda; Brown, Peter J; Cinabro, David; D'Andrea, Chris B; Frieman, Joshua; Jha, Saurabh W; Marriner, John; Nichol, Robert C; Nordin, Jakob; Olmstead, Matthew D; Sako, Masao; Schneider, Donald P; Smith, Mathew; Sollerman, Jesper; Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Simmons, Audrey; Shelden, Alaina

2012-01-01T23:59:59.000Z

347

West Valley Demonstration Project Waste Incidental to Reprocessing Evaluation  

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

West Valley Demonstration Project West Valley Demonstration Project Waste Incidental to Reprocessing Evaluation for the Concentrator Feed Makeup Tank and the Melter Feed Hold Tank February 2013 Prepared by the U.S. Department of Energy West Valley, New York This page is intentionally blank. WASTE-INCIDENTAL-TO-REPROCESSING EVALUATION FOR THE WVDP CFMT AND MFHT CONTENTS Revision 0 i NOTATION (Acronyms, Abbreviations, and Units).................................................. v 1.0 INTRODUCTION ...................................................................................................... 1 1.1 Purpose. ................................................................................................................. 2

348

Southwestern Power Administration One West Third Street  

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

Department of Energy Department of Energy Southwestern Power Administration One West Third Street Tulsa, Oklahoma 74103-3502 December 2, 2008 ENVIRONMENTAL POLICY STATEMENT The Environmental Policy is the driver for implementing and improving Southwestern Power Administration's (Southwestern) Environmental Management System so that Southwestern can maintain and improve environmental performance. The policy reflects the commitment of top management to comply with applicable legal and other requirements, to prevent pollution and to continually improve. Southwestern's Environmental Policy forms the basis upon which its Environmental Objectives and Targets are established. Southwestern's senior management has committed in writing the following Environmental Policy:

349

RING ROAD SOUTH IVERSITY ROAD WEST  

E-Print Network (OSTI)

Webb ­ Earth Sciences R5 Aston Webb ­ B Block R6 Aston Webb ­ Great Hall R7 Aston Webb ­ C Block R8P P P Barber Institute ELSROAD M R.15 R.30 24h Security R.3 RING ROAD SOUTH U N IVERSITY ROAD WEST South Car Park P R21 R17 R18 R22 Main Library R19 R20R20 R23 R24R24 R25 Munrow Sport Centre R27 R26 R28

Sloman, Aaron

350

RING ROAD SOUTH IVERSITY ROAD WEST  

E-Print Network (OSTI)

­ Earth Sciences R5 Aston Webb ­ B Block R6 Aston Webb ­ Great Hall R7 Aston Webb ­ C Block R8 PhysicsP P P Barber Institute ELSROAD M R.15 R.30 24h Security R.3 RING ROAD SOUTH U N IVERSITY ROAD WEST South Car Park P R21 R17 R18 R22 Main Library R19 R2020 R23 R2424 R25 Munrow Sport Centre R27 R26 R28 R

Yao, Xin

351

Light celebrating place, West Texas Road Trip  

E-Print Network (OSTI)

The dissertation explores the ability of light to embody and enhance the spirit of place in the Big Bend section of West Texas. A series of surveys and research investigated and then paired elements of light and place that were designed, and installed or simulated, in four experiential case studies. The case studies were evaluated by published authors of light and place and the dissertation committee and deemed mostly successful. Light installations can be embodied and enhance the spirit of place, the installations which were experienced live did this most effectively.

Mulholland, Jill Cecilia

2007-05-01T23:59:59.000Z

352

DOE - Office of Legacy Management -- Argonne National Laboratory - West -  

Office of Legacy Management (LM)

Argonne National Laboratory - West Argonne National Laboratory - West - 014 FUSRAP Considered Sites Site: Argonne National Laboratory - West (014) Designated Name: Alternate Name: Location: Evaluation Year: Site Operations: Site Disposition: Radioactive Materials Handled: Primary Radioactive Materials Handled: Radiological Survey(s): Site Status: The primary mission of the Argonne National Laboratory-West was to support liquid metal reactor research and development for the Department of Energy¿s Integral Fast Reactor Program, but the program was terminated. Activities at the Laboratory now include technology development for spent nuclear fuel and waste treatment, reactor and fuel cycle safety, and facility decommissioning. The decommissioning and other clean up is being

353

Water pollution Control Permit Fee Schedules (West Virginia) | Department  

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

pollution Control Permit Fee Schedules (West Virginia) pollution Control Permit Fee Schedules (West Virginia) Water pollution Control Permit Fee Schedules (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Fees Siting and Permitting Provider Department of Environmental Protection This rule establishes schedules of permit application fees and annual permit fees for state water pollution control permits and national

354

Alternative Fuels Data Center: West Virginia Laws and Incentives...  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

gallon equivalent, with a variable component equal to at least 5% of the average wholesale price of the fuel. (Reference Senate Bill 454, 2013, and West Virginia Code...

355

Underground Storage Tank Act (West Virginia) | Department of Energy  

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

Act (West Virginia) Act (West Virginia) Underground Storage Tank Act (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection New underground storage tank construction standards must include at least the following requirements: (1) That an underground storage tank will prevent releases of regulated substances stored therein, which may occur as

356

Requirements Governing Water Quality Standards (West Virginia) | Department  

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

Requirements Governing Water Quality Standards (West Virginia) Requirements Governing Water Quality Standards (West Virginia) Requirements Governing Water Quality Standards (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting This rule establishes the requirements governing the discharge or deposit of sewage, industrial wastes and other wastes into waters and establishes water quality standards.

357

Groundwater Protection Plan (West Virginia) | Department of Energy  

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

Groundwater Protection Plan (West Virginia) Groundwater Protection Plan (West Virginia) Groundwater Protection Plan (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection Groundwater Protection Plans (GPPs) are required for all facilities having the potential to impact groundwater. They are "preventive maintenance"

358

Dam Safety Rules (West Virginia) | Department of Energy  

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

Safety Rules (West Virginia) Safety Rules (West Virginia) Dam Safety Rules (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Savings Category Water Buying & Making Electricity Home Weatherization Program Info State West Virginia Program Type Safety and Operational Guidelines Provider Department of Environmental Protection This establishes requirements relating to the design, placement, construction, enlargement, alteration, removal, abandonment, and repair of

359

Solid Waste Management Rule (West Virginia) | Department of Energy  

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

Rule (West Virginia) Rule (West Virginia) Solid Waste Management Rule (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting This rule establishes requirements for the siting, financial assurance, installation, establishment, construction, design, groundwater monitoring, modification, operation, permitting, closure and post-closure care of any

360

Solid Waste Management Act (West Virginia) | Department of Energy  

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

Act (West Virginia) Act (West Virginia) Solid Waste Management Act (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection In addition to establishing a comprehensive program of controlling all phases of solid waste management and assigning responsibilities for solid waste management to the Secretary of Department of Environmental

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


361

Underground Storage Tanks (West Virginia) | Department of Energy  

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

Tanks (West Virginia) Tanks (West Virginia) Underground Storage Tanks (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection This rule governs the construction, installation, upgrading, use, maintenance, testing, and closure of underground storage tanks, including certification requirements for individuals who install, repair, retrofit,

362

NPDES Rule for Coal Mining Facilities (West Virginia) | Department of  

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

NPDES Rule for Coal Mining Facilities (West Virginia) NPDES Rule for Coal Mining Facilities (West Virginia) NPDES Rule for Coal Mining Facilities (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection This rule establishes requirements implementing the powers, duties, and responsibilities of State's Water Pollution Control Act with respect to all

363

Air Pollution Control Act (West Virginia) | Department of Energy  

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

Act (West Virginia) Act (West Virginia) Air Pollution Control Act (West Virginia) < Back Eligibility Agricultural Commercial Construction Developer Fed. Government Fuel Distributor General Public/Consumer Industrial Installer/Contractor Institutional Investor-Owned Utility Local Government Low-Income Residential Multi-Family Residential Municipal/Public Utility Nonprofit Residential Retail Supplier Rural Electric Cooperative Schools State/Provincial Govt Systems Integrator Transportation Tribal Government Utility Program Info State West Virginia Program Type Environmental Regulations Provider Department of Environmental Protection The purpose of this law is to provide for a coordinated statewide program of air pollution prevention, abatement and control; to facilitate cooperation across jurisdictional lines in dealing with problems of air

364

Sewage Sludge Management Rule (West Virginia) | Department of Energy  

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

Sewage Sludge Management Rule (West Virginia) Sewage Sludge Management Rule (West Virginia) Sewage Sludge Management Rule (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting This rule establishes requirements for the permitting siting, bonding, installation, establishment, construction, modification, and operation of any facility that generates, processes, recycles and/or disposes of sewage

365

,"West Virginia Shale Gas Proved Reserves, Reserves Changes,...  

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

Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Shale Gas Proved Reserves, Reserves Changes, and Production",10,"Annual",2011,"6302007"...

366

California South/West Bay Area Regional Middle School Science...  

Office of Science (SC) Website

California SouthWest Bay Area Regional Middle School Science Bowl National Science Bowl (NSB) NSB Home About High School Middle School Middle School Students Middle School...

367

,"West Virginia Crude Oil Reserves in Nonproducing Reservoirs...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Crude Oil Reserves in Nonproducing Reservoirs (Million Barrels)",1,"Annual",2011 ,"Release...

368

New Mexico--West Natural Gas Liquids Lease Condensate, Proved...  

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

Natural Gas Liquids Lease Condensate, Proved Reserves (Million Barrels) New Mexico--West Natural Gas Liquids Lease Condensate, Proved Reserves (Million Barrels) Decade Year-0...

369

West Virginia Natural Gas Plant Liquids, Proved Reserves (Million...  

Gasoline and Diesel Fuel Update (EIA)

company data. Release Date: 812013 Next Release Date: 812014 Referring Pages: Natural Gas Liquids Proved Reserves as of Dec. 31 West Virginia Natural Gas Liquids Proved...

370

West Virginia Natural Gas Liquids Lease Condensate, Proved Reserves...  

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

Liquids Lease Condensate, Proved Reserves (Million Barrels) West Virginia Natural Gas Liquids Lease Condensate, Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3...

371

West Virginia Natural Gas Plant Liquids Production, Gaseous Equivalent...  

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

Liquids Production, Gaseous Equivalent (Million Cubic Feet) West Virginia Natural Gas Plant Liquids Production, Gaseous Equivalent (Million Cubic Feet) Decade Year-0 Year-1 Year-2...

372

,"West Virginia Natural Gas Plant Liquids Production, Gaseous...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Natural Gas Plant Liquids Production, Gaseous Equivalent (MMcf)",1,"Annual",2012 ,"Release...

373

West Virginia Percent of Historical Gas Well Production (BOE) by ...  

U.S. Energy Information Administration (EIA)

West Virginia Percent of Historical Gas Well Production (BOE) by Production Rate Bracket. Energy Information Administration (U.S. Dept. of Energy)

374

Dam Safety Rules (West Virginia) | Open Energy Information  

Open Energy Info (EERE)

Manager Department Department of Environmental Protection Division Water and Waste Management -- Environmental Enforcement Address 601 57Th St. SE Place Charleston, West...

375

Dam Control and Safety Act (West Virginia) | Open Energy Information  

Open Energy Info (EERE)

Manager Department Department of Environmental Protection Division Water and Waste Management -- Environmental Enforcement Address 601 57Th St. SE Place Charleston, West...

376

West Texas Intermediate crude oil price and NYMEX 95% confidence ...  

U.S. Energy Information Administration (EIA)

West Texas Intermediate crude oil price and NYMEX 95% confidence intervals January 2007 October 2009 Short-Term Energy Outlook Note: Confidence intervals for the ...

377

Craig-Botetourt Electric Coop (West Virginia) | Open Energy Informatio...  

Open Energy Info (EERE)

"EIA Form EIA-861 Final Data File for 2010 - File22010" Retrieved from "http:en.openei.orgwindex.php?titleCraig-BotetourtElectricCoop(WestVirginia)&oldid412507...

378

New Mexico - West Crude Oil + Lease Condensate Proved Reserves...  

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

Crude Oil + Lease Condensate Proved Reserves (Million Barrels) New Mexico - West Crude Oil + Lease Condensate Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3...

379

,"West Virginia Natural Gas Gross Withdrawals and Production...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Natural Gas Gross Withdrawals and Production",11,"Annual",2012,"6301967" ,"Release Date:","1212...

380

Redefining Agrarian Power: Resurgent Agrarian Movements in West Java, Indonesia  

E-Print Network (OSTI)

Movements in West Java, Indonesia Suraya Afiff Noer Fauzienvironmental change in Indonesia since 1985. She receivedenvironmental change in Indonesia since the 1990s. In Fall

Afiff, Suraya; Fauzi, Noer; Hart, Gillian; Ntsebeza, Lungisile; Peluso, Nancy

2005-01-01T23:59:59.000Z

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


381

,"West Virginia Natural Gas Gross Withdrawals from Shale Gas...  

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

,"Workbook Contents" ,"West Virginia Natural Gas Gross Withdrawals from Shale Gas (Million Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet...

382

Geographic Information System At U.S. West Region (Williams ...  

Open Energy Info (EERE)

navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Geographic Information System At U.S. West Region (Williams & Deangelo, 2008) Exploration Activity Details...

383

Operational Awareness Oversight of the West Valley Demonstration...  

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

on the upcoming activities at the West Valley Demonstration Project (WVDP). Major decommissioning activities underway include removal of asbestos-containing materials, disassembly...

384

,"West Virginia Natural Gas Industrial Price (Dollars per Thousand...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Natural Gas Industrial Price (Dollars per Thousand Cubic Feet)",1,"Monthly","72013" ,"Release...

385

West Coast (PADD 5) Exports of Normal Butane-Butylene ...  

U.S. Energy Information Administration (EIA)

Normal Butane/Butylene Exports; Normal Butane/Butylene Supply and Disposition; West Coast (PADD 5) Exports of Crude Oil and Petroleum Products ...

386

K West integrated water treatment system subproject safety analysis document  

Science Conference Proceedings (OSTI)

This Accident Analysis evaluates unmitigated accident scenarios, and identifies Safety Significant and Safety Class structures, systems, and components for the K West Integrated Water Treatment System.

SEMMENS, L.S.

1999-02-24T23:59:59.000Z

387

Price protection options for West Virginia beef cattle producers.  

E-Print Network (OSTI)

??The purpose of this study was to determine if a price protection option would be beneficial to West Virginia's beef cattle industry. Fourteen years of (more)

Kleski, Matthew C., 1979-

2004-01-01T23:59:59.000Z

388

,"West Virginia Dry Natural Gas Production (Million Cubic Feet...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Dry Natural Gas Production (Million Cubic Feet)",1,"Monthly","122011" ,"Release Date:","7312013"...

389

Argonne National Laboratory-West, Former Production Workers Screening...  

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

Production Workers Screening Projects (now known as the Idaho National Laboratory) Argonne National Laboratory-West, Former Production Workers Screening Projects (now known as...

390

,"West Virginia Natural Gas Wellhead Price (Dollars per Thousand...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Natural Gas Wellhead Price (Dollars per Thousand Cubic Feet)",1,"Annual",2010 ,"Release Date:","9...

391

Energy Crossroads: Utility Energy Efficiency Programs West Virginia...  

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

West Virginia Energy Crossroads Index Utility Energy Efficiency Programs Index Suggest a Listing American Electric Power (AEP) Information for Businesses Allegheny Power...

392

oil and Gas Resources of the West Siberian Basin, Russia  

U.S. Energy Information Administration (EIA)

Energy Information Administration Oil and Gas Resources of the West Siberian Basin, Russia 29 Appendix A Petroleum Geology The petroleum geology discussion is copied ...

393

,"West Virginia Crude Oil + Lease Condensate Proved Reserves...  

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

Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Crude Oil + Lease Condensate Proved Reserves (Million Barrels)",1,"Annual",2011 ,"Release...

394

West Virginia Percent of Historical Oil Well Production (BOE) by ...  

U.S. Energy Information Administration (EIA)

West Virginia Percent of Historical Oil Well Production (BOE) by Production Rate Bracket. Energy Information Administration (U.S. Dept. of Energy)

395

New Mexico--West Natural Gas Liquids Lease Condensate, Reserves...  

Annual Energy Outlook 2012 (EIA)

Reserves Based Production (Million Barrels) New Mexico--West Natural Gas Liquids Lease Condensate, Reserves Based Production (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3...

396

New Mexico - West Dry Natural Gas New Reservoir Discoveries in...  

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

Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic Feet) New Mexico - West Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade...

397

Project #8, Emergency Response  

Science Conference Proceedings (OSTI)

... Page 10. FDNY's Initial Size-up of WTC Conditions: A large aircraft had hit the WTC 1 building. ... Command Post at West and Liberty Streets ...

2005-12-30T23:59:59.000Z

398

High-Rise and Large/Complex Incident Communications ...  

Science Conference Proceedings (OSTI)

... After the first aircraft struck the World Trade Center One building there was an approximate factor of 5 ... WTC 1 WTC 2 Marriott Hotel West & Liberty ...

2007-03-14T23:59:59.000Z

399

Appendix 4 - Presentations  

Science Conference Proceedings (OSTI)

... WTC 1 WTC 2 Marriott Hotel West & Liberty ... 1. After the first aircraft struck WTC 1, there was an approximate factor of 5 peak increase in traffic level ...

2007-10-03T23:59:59.000Z

400

Upgrade of the Proton West secondary beamline  

SciTech Connect

As originally designed and operated, protons entering PW6 were steered by a series of EPB dipoles into a single interaction length beryllium target, some 43 feet from the enclosure wall. Ensuing secondary beams, either p{sup +}/{pi}{sup +} or p{sup -}/{pi}{sup -}, were collected by a string of quadrupoles following the target, steered westward, away from the Proton Center line, through PW6 and PW7, and ultimately focussed on experiment production targets located within the large PW8 hall. Around the Spring of 1988 it was decided to upgrade the existing Proton West secondary beamline to allow for transport of a primary proton beam, anticipated to be either 800 or 900 GeV/c, through PW8. This upgrade project, which is now nearing completion, was largely motivated by the then recent approval of E-771, a hadronic beauty production experiment located in PW8. E-771 represents the third in a series of experiments for the large-acceptance dimuon spectrometer presently located at the end of the Proton West beamline. This Technical Memo is a summary of the upgrade --- an explanation of the underlying strategy and a documentation of the final locations of the secondary beamline elements. 6 refs., 2 figs., 2 tabs.

Spiegel, L.

1989-10-10T23:59:59.000Z

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


401

The New Sundanese Peasants' Union: Peasant Movements, Changes in Land Control, and Agrarian Questions in Garut, West Java  

E-Print Network (OSTI)

of the Association of West Java Plantations; and Ir. H.Questions in Garut, West Java *) Noer Fauzi Berkeleyorganization in West Java, Indonesia, was extraordinarily

Fauzi, Noer

2005-01-01T23:59:59.000Z

402

FAILED-DETONATION SUPERNOVAE: SUBLUMINOUS LOW-VELOCITY Ia SUPERNOVAE AND THEIR KICKED REMNANT WHITE DWARFS WITH IRON-RICH CORES  

SciTech Connect

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosions of carbon-oxygen (C-O) white dwarfs (WDs). The single-degenerate scenario is a well-explored model of SNe Ia where unstable thermonuclear burning initiates in an accreting, Chandrasekhar-mass WD and forms an advancing flame. By several proposed physical processes, the rising, burning material triggers a detonation, which subsequently consumes and unbinds the WD. However, if a detonation is not triggered and the deflagration is too weak to unbind the star, a completely different scenario unfolds. We explore the failure of the gravitationally confined detonation mechanism of SNe Ia, and demonstrate through two-dimensional and three-dimensional simulations the properties of failed-detonation SNe. We show that failed-detonation SNe expel a few 0.1 M{sub Sun} of burned and partially burned material and that a fraction of the material falls back onto the WD, polluting the remnant WD with intermediate-mass and iron-group elements that likely segregate to the core forming a WD whose core is iron rich. The remaining material is asymmetrically ejected at velocities comparable to the escape velocity from the WD, and in response, the WD is kicked to velocities of a few hundred km s{sup -1}. These kicks may unbind the binary and eject a runaway/hypervelocity WD. Although the energy and ejected mass of the failed-detonation SN are a fraction of typical thermonuclear SNe, they are likely to appear as subluminous low-velocity SNe Ia. Such failed detonations might therefore explain or are related to the observed branch of peculiar SNe Ia, such as the family of low-velocity subluminous SNe (SN 2002cx/SN 2008ha-like SNe).

Jordan, George C. IV; Van Rossum, Daniel R. [Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637 (United States); Perets, Hagai B. [Physics Department, Technion, Israel Institute of Technology, Haifa 32000 (Israel); Fisher, Robert T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States)

2012-12-20T23:59:59.000Z

403

TYPE Ia SUPERNOVA PROPERTIES AS A FUNCTION OF THE DISTANCE TO THE HOST GALAXY IN THE SDSS-II SN SURVEY  

Science Conference Proceedings (OSTI)

We use Type Ia supernovae (SNe Ia) discovered by the Sloan Digital Sky Survey-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host-galaxy center, using the distance as a proxy for local galaxy properties (local star formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light curves using both MLCS2K2 and SALT2, and determine color (A{sub V} , c) and light-curve shape ({Delta}, x{sub 1}) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4{sigma} level) finding is that the average fitted A{sub V} from MLCS2K2 and c from SALT2 decrease with the projected distance for SNe Ia in spiral galaxies. We also find indications that supernovae (SNe) in elliptical galaxies tend to have narrower light curves if they explode at larger distances, although this may be due to selection effects in our sample. We do not find strong correlations between the residuals of the distance moduli with respect to the Hubble flow and the galactocentric distances, which indicates a limited correlation between SN magnitudes after standardization and local host metallicity.

Galbany, Lluis; Miquel, Ramon; Oestman, Linda [Institut de Fisica d'Altes Energies, Universitat Autonoma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Brown, Peter J.; Olmstead, Matthew D. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); D'Andrea, Chris B.; Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX (United Kingdom); Frieman, Joshua [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellise Avenue, Chicago, IL 60637 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, John [Center for Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Nordin, Jakob [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720 (United States); Sako, Masao [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7535, Cape Town (South Africa); Sollerman, Jesper [Oskar Klein Centre, Department of Astronomy, AlbaNova, SE-106 91 Stockholm (Sweden); Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard, E-mail: lluis.galbany@ist.utl.pt [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); and others

2012-08-20T23:59:59.000Z

404

West Valley Demonstration Project Transportation Emergency Management Program  

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

West West Valley Demonstration Project Transportation Emergency Management Program Independent Oversight Review of the Office of Independent Oversight and Performance Assurance September 2000 OVERSIGHT Table of Contents EXECUTIVE SUMMARY ................................................................... 1 1.0 INTRODUCTION ........................................................................... 4 2.0 RESULTS ......................................................................................... 7 Hazards Survey and Hazards Assessment .................................... 7 Program Plans and Procedures ..................................................... 8 Emergency Responder Performance .......................................... 10 Feedback and Continuous Improvement....................................

405

Economic Impact of West Virginia Higher Education Institutions  

E-Print Network (OSTI)

of Technology) The economic impacts estimated in this report are for fiscal year (FY) 2008 (July 1, 2007 ­ June West Virginia University May 2010 Funding for this report was provided by the West Virginia Higher Education Policy Commission. The report includes financial and other data provided by member HEPC

Mohaghegh, Shahab

406

Financing West Virginia's Highways: Challenges and Opportunities1  

E-Print Network (OSTI)

need for additional funding for West Virginia's highway infrastructure. The funding for West Virginia To better understand the logical basis for how federal and state governments fund public highway are insufficient for the funding of public highways. Table B5 from the Federal Highway Administration shows

Mohaghegh, Shahab

407

Enforcement Letter, Argonne National Laboratory-West - February 9, 1999 |  

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

West - February 9, West - February 9, 1999 Enforcement Letter, Argonne National Laboratory-West - February 9, 1999 February 9, 1999 Enforcement Letter issued to Argonne National Laboratory related to a Dropped Fuel Basket Assembly and Radiation Protection Program Deficiencies at Argonne National Laboratory-West This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances concerning two incidents occurring in June and August 1998 at Argonne National Laboratory - West's (ANLW) Fuel Conditioning Facility (FCF): dropping a fuel basket assembly containing chopped fuel elements and repair of a manipulator seal tube. During November 2-3, 1998, DOE conducted an investigation to determine what, if any, noncompliances with applicable nuclear safety regulations may have

408

Proposed Energy Transport Corridors: West-wide energy corridor programmatic  

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

Energy Transport Corridors: West-wide energy corridor Energy Transport Corridors: West-wide energy corridor programmatic EIS, Draft Corridors - September 2007. Proposed Energy Transport Corridors: West-wide energy corridor programmatic EIS, Draft Corridors - September 2007. Map of the area covered by a programmatic environmental impact statement (PEIS), "Designation of Energy Corridors on Federal Land in the 11 Western States" (DOE/EIS-0386) to address the environmental impacts from the proposed action and the range of reasonable alternatives. The proposed action calls for designating more than 6,000 miles of energy transport corridors across the West. Proposed Energy Transport Corridors: West-wide energy corridor programmatic EIS, Draft Corridors - September 2007. More Documents & Publications

409

Energy Incentive Programs, West Virginia | Department of Energy  

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

West Virginia West Virginia Energy Incentive Programs, West Virginia October 29, 2013 - 1:19pm Addthis Updated August 2013 West Virginia utilities budgeted $10 million in 2012 to promote energy efficiency in the state. What public-purpose-funded energy efficiency programs are available in my state? West Virginia has no public-purpose-funded energy efficiency programs. What utility energy efficiency programs are available to me? AEP Appalachian Power offers prescriptive rebates for an assortment of energy-efficient lighting and HVAC equipment, as well as variable frequency drives. The maximum amount obtainable for any one entity is $150,000 per year. Any installation with greater than $20,000 of rebates claimed will be inspected. First Energy (Potomac Edison and Mon Power) sponsors the Lighting for

410

Preliminary Notice of Violation, Argonne National Laboratory-West -  

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

West - West - EA-2001-01 Preliminary Notice of Violation, Argonne National Laboratory-West - EA-2001-01 February 28, 2001 Preliminary Notice of Violation issued to the University of Chicago related to Programmatic Management Failures at Argonne National Laboratory-West, (EA-2001-01) This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances presented to DOE by Mason & Hanger Corporation's (M&H or the contractor) internal evaluation of the Building 12-79 HPFL Valve Misposition at the Pantex Plant, which was identified on November 19, 1999. Preliminary Notice of Violation, Argonne National Laboratory-West - EA-2001-01 More Documents & Publications Consent Order, Mason & Hanger Corporation - EA-2000-07 Preliminary Notice of Violation, Mason & Hanger Corporation - EA-1999-05

411

West Clare Renewable Energy Ltd | Open Energy Information  

Open Energy Info (EERE)

Renewable Energy Ltd Renewable Energy Ltd Jump to: navigation, search Name West Clare Renewable Energy Ltd Place United Kingdom Sector Wind energy Product A wind project developer established to build the Mount Callan wind farm in County Clare Ireland. References West Clare Renewable Energy Ltd[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. West Clare Renewable Energy Ltd is a company located in United Kingdom . References ↑ "West Clare Renewable Energy Ltd" Retrieved from "http://en.openei.org/w/index.php?title=West_Clare_Renewable_Energy_Ltd&oldid=352997" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages

412

Independent Oversight Inspection, Argonne National Laboratory-West -  

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

Inspection, Argonne National Laboratory-West Inspection, Argonne National Laboratory-West - November 2004 Independent Oversight Inspection, Argonne National Laboratory-West - November 2004 November 2004 Emergency Management Inspection of the Argonne National Laboratory-West The Secretary of Energy's Office of Independent Oversight and Performance Assurance (OA), within the Office of Security and Safety Performance Assurance, conducted an inspection of the emergency management program at the U.S. Department of Energy (DOE) Argonne National Laboratory - West (ANL-W) site in October 2004. The inspection was performed by the OA Office of Emergency Management Oversight. Following the 2001 OA inspection, ANL-W completed a number of activities that improved the site emergency management program. ANL-W developed a

413

NETL: Science Bowl Information - West Virginia - RESA Coordinators  

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

Sponsors Sponsors We would like to gratefully acknowledge the support of our sponsors over the past several years. Please contact Friends of West Virginia Regional Science Bowl Foundation for more information. Friends of West Virginia Regional Science Bowl Foundation 538 Valley Road Morgantown, WV 26505 2012 Sponsors Gold ($1,000 or more) KeyLogic Systems, Inc. Leonardo Technologies, Inc. Mid-Atlantic Technology, Research and Innovation Center Performance Results Corporation Society for Analytical Chemists of Pittsburgh URS Corporation-Washington Division West Virginia University National Research Center for Coal and Energy West Virginia University Research Corporation Silver ($500 to $999) Sheetz Spectroscopy Society of Pittsburgh SRA/Platinum Solutions West Virginia High Technology Consortium Foundation

414

Thanksgiving Goodwill: West Valley Demonstration Project Food Drive  

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

Thanksgiving Goodwill: West Valley Demonstration Project Food Drive Thanksgiving Goodwill: West Valley Demonstration Project Food Drive Provides 640 Turkeys to People in Need Thanksgiving Goodwill: West Valley Demonstration Project Food Drive Provides 640 Turkeys to People in Need November 26, 2013 - 12:00pm Addthis Volunteers from West Valley Demonstration Project gather before distributing items collected in an annual food drive. Volunteers from West Valley Demonstration Project gather before distributing items collected in an annual food drive. Volunteer John Schelble helps unload a delivery truck at a food pantry. Volunteer John Schelble helps unload a delivery truck at a food pantry. John Rizzo passes canned food to John Rendall to deliver to a food pantry. John Rizzo passes canned food to John Rendall to deliver to a food pantry.

415

Technical Services Contract Awarded for West Valley Demonstration Project  

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

Technical Services Contract Awarded for West Valley Demonstration Technical Services Contract Awarded for West Valley Demonstration Project Support Services Technical Services Contract Awarded for West Valley Demonstration Project Support Services February 21, 2013 - 12:00pm Addthis Media Contact Bill Taylor, 803-952-8564 bill.taylor@srs.gov Cincinnati - The U.S. Department of Energy (DOE) today awarded a task order to Safety and Ecology Corporation of Knoxville, Tennessee, for technical services at the West Valley Demonstration Project, West Valley, New York. The task order has a three-year performance period with a $1.3 million value. The task order will be issued from the Indefinite Delivery/Indefinite Quantity (ID/IQ) master contract, firm-fixed-price and time and materials. Under the task order, Safety and Ecology Corporation will perform technical

416

Enforcement Letter, Argonne National Laboratory-West - February 9, 1999 |  

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

Argonne National Laboratory-West - February 9, Argonne National Laboratory-West - February 9, 1999 Enforcement Letter, Argonne National Laboratory-West - February 9, 1999 February 9, 1999 Enforcement Letter issued to Argonne National Laboratory related to a Dropped Fuel Basket Assembly and Radiation Protection Program Deficiencies at Argonne National Laboratory-West This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances concerning two incidents occurring in June and August 1998 at Argonne National Laboratory - West's (ANLW) Fuel Conditioning Facility (FCF): dropping a fuel basket assembly containing chopped fuel elements and repair of a manipulator seal tube. During November 2-3, 1998, DOE conducted an investigation to determine what, if any, noncompliances with applicable nuclear safety regulations may have

417

Energy Efficiency Programs in West Virginia: A Partnership Approach  

E-Print Network (OSTI)

West Virginia's successful energy efficiency program relies on the close working relationship between the West Virginia Division of Energy and West Virginia University's energy efficiency programs, Industries of the Future - West Virginia and WVU Industrial Assessment Center. These organizations work together to conduct the State's energy efficiency assistance programs that include R&D, assessments, and outreach, identify potential clients, and offer a wide range of services. The partnership has the capability to provide these services to facilities ranging in size from small commercial businesses to large manufacturing facilities. The partners have affiliations not only within industry but also with industry organizations, utilities, and national laboratories. This range of services creates a synergistic relationship that allows the WV team to obtain competitive awards that benefit the stakeholders. This paper will focus on how West Virginia has a successful industrial energy efficiency program with limited state funding and no surcharges on utility bills.

Cullen, K. A.; Crowe, E.; Gopalakrishnan, B.; Chaudhari, S.

2011-01-01T23:59:59.000Z

418

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rat...

Dilday, Benjamin; Frieman, J A; Holtzman, J; Marriner, J; Miknaitis, G; Nichol, R C; Romani, R; Sako, M; Bassett, B; Becker, A; Cinabro, D; De Jongh, F; Depoy, D L; Doi, M; Garnavich, P M; Hogan, C J; Jha, S; Konishi, K; Lampeitl, H; Marshall, J L; McGinnis, D; Prieto, J L; Riess, A G; Richmond, M W; Schneider, D P; Smith, M; Takanashi, N; Tokita, K; van der Heyden, K; Zheng, N Yasuda C; Barentine, J; Brewington, H; Choi, C; Crotts, A; Dembicky, J; Harvanek, M; Im, M; Ketzeback, W; Kleinman, S J; Krzesi?ski, J; Long, D C; Malanushenko, E; Malanushenko, V; McMillan, R J; Nitta, A; Pan, K; Saurage, G; Snedden, S A; Watters, S; Wheeler, J C; York, D

2008-01-01T23:59:59.000Z

419

West Pico Food | Open Energy Information  

Open Energy Info (EERE)

Pico Food Pico Food Jump to: navigation, search Name West Pico Food Place Vernon, California Sector Solar Product A distributor of wholesale frozen foods to supermarket chains in Southern California, which has had a solar installation built on its roof. Coordinates 42.761624°, -72.511495° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.761624,"lon":-72.511495,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

420

Golden Field Office 15013 Denver West Parkway  

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

Golden Field Office 15013 Denver West Parkway Golden, Colorado 80401 FINDING OF NO SIGNIFICANT IMPACT FLORIDA ATLANTIC UNIVERSITY SOUTHEAST NATIONAL MARINE RENEWABLE ENERGY CENTER MARINE HYDROKINETIC TECHNOLOGY TESTING PROJECT DOE/EA-1965 AGENCY: U.S. Department of Energy (DOE), Office of Energy Efficiency and Renewable Energy (EERE) ACTION: Finding of No Significant Impact (FONSI) SUMMARY: DOE is proposing to provide federal funding to Florida Atlantic University (FAU) Southeast National Marine Renewable Energy Center (SNMREC) to install a non-grid- connected offshore test berth and test a variety of small-scale research and development ocean current turbine units 1 on public lands managed by the U.S. Department of Interior, Bureau of

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421

FINAL-west-doe-rfi-comments  

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

October October 31, 2013 Mr. Christopher Lawrence Office of Electricity Delivery and Energy Reliability (OE-20) U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 Submitted electronically via email to: Christopher.Lawrence@hq.doe.gov Re: Department of Energy - Improving Performance of Federal Permitting and Review of Infrastructure Projects, Request for Information, 78 Fed. Reg. 53436 (Aug. 29, 2013) Dear Mr. Lawrence: I. INTRODUCTION Western Energy Supply and Transmission Associates ("WEST") 1 respectfully submits these comments in response to the questions raised in the above-referenced Department of Energy (DOE) Request for Information (RFI). This RFI addresses the proposed pre-application process for siting of transmission projects requiring interagency

422

Notices Safety Commission, 4330 East West  

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

0 Federal Register 0 Federal Register / Vol. 77, No. 8 / Thursday, January 12, 2012 / Notices Safety Commission, 4330 East West Highway, Bethesda, MD 20814, (301) 504-7923. Dated: January 10, 2012. Todd A Stevenson, Secretary. [FR Doc. 2012-625 Filed 1-10-12; 4:15 pm] BILLING CODE 6355-01-P CORPORATION FOR NATIONAL AND COMMUNITY SERVICE Information Collection; Submission for OMB Review, Comment Request AGENCY: Corporation for National and Community Service. ACTION: Notice. SUMMARY: The Corporation for National and Community Service (the Corporation), has submitted a public information collection request (ICR) entitled Day of Service Project Promotion Tool for review and approval in accordance with the Paperwork Reduction Act of 1995, Public Law 104- 13, (44 U.S.C. chapter 35). Copies of this

423

West Point Utility System | Open Energy Information  

Open Energy Info (EERE)

System System Jump to: navigation, search Name West Point Utility System Place Iowa Utility Id 20396 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes Activity Bundled Services Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png General Service and Municipal Institutional service Large General Service Commercial Rural Resident and Farm All-Electric Residential Rural Resident and Farm Rate Residential Security Light - 150 Watt HPS Customer Owned Pole Lighting Security Light - 150 Watt HPS Utility Owned Pole Lighting Urban All-Electric Residential Rate Residential

424

High West Energy, Inc | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Jump to: navigation, search Name High West Energy, Inc Place Colorado Utility Id 27058 References Energy Information Administration.[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png A F Industrial Commercial & Small Power Commercial Farm and Home Residential Irrigation Industrial Large Power Industrial Large Power T-O-D Industrial Large Power T-O-D V2 Industrial Large Power V2 Industrial Security Lighting-150 - 175 watt M V/ HPS Lighting Security Lighting-200 - 250 watt M V/ HPS Lighting Security Lighting-400 watt M V/ HPS Lighting Street Lighting-200 - 250 watt M V/ HPS Lighting Street Lighting-400 watt M V/ HPS Lighting Time-of-Use Commercial

425

North Slope action holds West Coast spotlight  

Science Conference Proceedings (OSTI)

The first oil from a North Slope reservoir outside Prudhoe Bay will begin flowing next year at rate of 80,000 bpd from Kuparuk field now under development by Atlantic Richfield Co. west of Prudhoe Bay. Just north of the Kuparuk development, Conoco Inc. has found a commercial reservoir in the Milne Point unit and will be drilling confirmation and delineation wells later this year and in 1982. Another area which very likely will be developed for production is located northeast of Prudhoe Bay, where Sohio Alaska Petroleum Co. has announced discoveries in 2 Sag Delta wells. In California's San Joaquin Valley, 3 Kern County fields - South Belridge, Elk Hills, and Lost Hills - are the sites of intensive drilling. Seven rigs are working in the Santa Barbara Channel, 3 of them developing known fields from permanent platforms.

Wilson, H.M.

1981-05-25T23:59:59.000Z

426

Aleutians West Census Area, Alaska ASHRAE 169-2006 Climate Zone...  

Open Energy Info (EERE)

Aleutians West Census Area, Alaska ASHRAE 169-2006 Climate Zone Jump to: navigation, search County Climate Zone Place Aleutians West Census Area, Alaska ASHRAE Standard ASHRAE...

427

West Valley Demonstration Project DOE Manual 435.1-1 Waste Incidental...  

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

West Valley Demonstration Project DOE Manual 435.1-1 Waste Incidental to Reprocessing Evaluations and Determinations West Valley Demonstration Project DOE Manual 435.1-1 Waste...

428

Table HC14.8 Water Heating Characteristics by West Census Region ...  

U.S. Energy Information Administration (EIA)

Table HC14.8 Water Heating Characteristics by West Census Region, 2005 Million U.S. Housing Units Water Heating Characteristics Mountain Pacific West Census Region

429

Geothermal Literature Review At U.S. West Region (Skokan, 1993...  

Open Energy Info (EERE)

GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Geothermal Literature Review At U.S. West Region (Skokan, 1993) Exploration Activity Details Location U.S. West Region...

430

Making the Standard Candle: A study of how the progenitor white dwarf modulates the peak luminosity of type Ia supernovae  

SciTech Connect

The goals of the proposed research as stated in the proposal were to: Build a suite of one-dimensional initial models of different metallicities and central densities. Using the improved flame capturing scheme, simulate the explosion of a white dwarf with embedded Lagrangian tracer particles, and post-process the thermal histories of the tracers to reconstruct the nucleosynthesis of the explosion. Survey the effects of a changing progenitor metallicity on the isotopic yields. Of particular interest is 1) whether the linear relation between the mass of 56Ni synthesized and the pro- genitor metallicity is moderated by the effect of electron captures in the core; and 2) how a varying central density alters the relation between metallicity and 56Ni mass. Using these results, examine how the observed metallicity distribution would affect the brightness distribution of SNe Ia and the isotopic ratios about the Fe-peak.

Brown, Edward F [Michigan State University

2010-01-21T23:59:59.000Z

431

Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae  

E-Print Network (OSTI)

We estimate the solar system motion relative to the cosmic microwave background using type Ia supernovae (SNe) measurements. We take into account the correlations in the error bars of the SNe measurements arising from correlated peculiar velocities. Without accounting for correlations in the peculiar velocities, the SNe data we use appear to detect the peculiar velocity of the solar system at about the 3.5 sigma level. However, when the correlations are correctly accounted for, the SNe data only detects the solar system peculiar velocity at about the 2.5 sigma level. We forecast that the solar system peculiar velocity will be detected at the 9 sigma level by GAIA and the 11 sigma level by the LSST. For these surveys we find the correlations are much less important as most of the signal comes from higher redshifts where the number density of SNe is insufficient for the correlations to be important.

Christopher Gordon; Kate Land; Anze Slosar

2007-11-27T23:59:59.000Z

432

MHK Technologies/Wave Energy Seawater Transmission WEST | Open Energy  

Open Energy Info (EERE)

Wave Energy Seawater Transmission WEST Wave Energy Seawater Transmission WEST < MHK Technologies Jump to: navigation, search << Return to the MHK database homepage Wave Energy Seawater Transmission WEST.jpg Technology Profile Primary Organization Atmocean Inc Project(s) where this technology is utilized *MHK Projects/WEST Testing Technology Resource Click here Wave Technology Type Click here Point Absorber Technology Readiness Level Click here TRL 1-3: Discovery / Concept Definition / Early Stage Development & Design & Engineering Technology Description Atmocean WEST efficiently captures wave energy by deploying many inexpensive devices across large ocean regions. By using hydraulic transmission, WEST avoids the high cost of seafloor power lines, generating electricity onshore to achieve higher reliability at lower cost. When WEST is combined with Bright Energy Storage Technologies seafloor compressed air energy storage (CAES) system, the two enable base load renewable power (eliminating the need for backup fossil-fuel power) at a projected levelized cost of electricity (LCOE) of $.08/kWh to $.12/kWh.

433

West Virginia Consumers Have Appliance Rebate 'Trifecta' | Department of  

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

Consumers Have Appliance Rebate 'Trifecta' Consumers Have Appliance Rebate 'Trifecta' West Virginia Consumers Have Appliance Rebate 'Trifecta' September 13, 2010 - 10:30am Addthis West Virginia Governor Joe Manchin announces the Energy Efficient Rebate Program in June. The state received $1.7 million in Recovery Act funding to encourage residents to purchase ENERGY STAR appliances. | Photo courtesy of WVDEP West Virginia Governor Joe Manchin announces the Energy Efficient Rebate Program in June. The state received $1.7 million in Recovery Act funding to encourage residents to purchase ENERGY STAR appliances. | Photo courtesy of WVDEP Stephen Graff Former Writer & editor for Energy Empowers, EERE What are the key facts? West Virginia residents receive up to $100 in rebates for ENERGY STAR appliances

434

Groundwater Protection Act (West Virginia) | Department of Energy  

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

Act (West Virginia) Act (West Virginia) Groundwater Protection Act (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Savings Category Buying & Making Electricity Water Home Weatherization Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection The purposes of this Act are to: Maintain and protect the state's groundwater resources consistent with this article to protect the present and future beneficial uses of the

435

West Virginia/Wind Resources | Open Energy Information  

Open Energy Info (EERE)

West Virginia/Wind Resources West Virginia/Wind Resources < West Virginia Jump to: navigation, search Print PDF Print Full Version WIND ENERGY STAKEHOLDER ENGAGEMENT & OUTREACHSmall Wind Guidebook Home OpenEI Home >> Wind >> Small Wind Guidebook >> West Virginia Wind Resources WindTurbine-icon.png Small Wind Guidebook * Introduction * First, How Can I Make My Home More Energy Efficient? * Is Wind Energy Practical for Me? * What Size Wind Turbine Do I Need? * What Are the Basic Parts of a Small Wind Electric System? * What Do Wind Systems Cost? * Where Can I Find Installation and Maintenance Support? * How Much Energy Will My System Generate? * Is There Enough Wind on My Site? * How Do I Choose the Best Site for My Wind Turbine? * Can I Connect My System to the Utility Grid?

436

Pacific West I Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Pacific West I Wind Farm Pacific West I Wind Farm Facility Pacific West I Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner PacifiCorp Developer SeaWest Energy Purchaser Southern California Edison/PacifiCorp Location San Gorgonio CA Coordinates 33.9095°, -116.734° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.9095,"lon":-116.734,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

437

Argonne National Laboratory-West, Former Production Workers Screening  

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

West, Former Production Workers West, Former Production Workers Screening Projects (now known as the Idaho National Laboratory) Argonne National Laboratory-West, Former Production Workers Screening Projects (now known as the Idaho National Laboratory) Project Name: Worker Health Protection Program Covered DOE Site: Argonne National Laboratory-West Worker Population Served: Production Workers Principal Investigator: Jim Frederick Co-Principal Investigator: Steven Markowitz, MD Toll-free Telephone: (888) 241-1199 Local Outreach Office: David Fry 1055 Austin Avenue Idaho Falls, ID 83404 Website: http://www.worker-health.org/ This project is conducted by the United Steelworkers, in partnership with Queens College of the City University of New York. Free of charge, eligible workers can receive a medical exam, including chest X-ray and breathing

438

SeaWest Energy Group Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Farm Wind Farm Jump to: navigation, search Name SeaWest Energy Group Wind Farm Facility SeaWest Energy Group Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner SeaWest Developer SeaWest Energy Purchaser Pacific Gas & Electric Co Location Altamont Pass CA Coordinates 37.7347°, -121.652° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.7347,"lon":-121.652,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

439

Emigration and the Foundation of West Germany, 1933-1963  

E-Print Network (OSTI)

University Press, 2009. Feldman, Noah. What We Owe Iraq: WarGermany, 1933-1963 By Noah Benezra Strote A dissertationof West Germany, 1933-1963 By Noah Benezra Strote Doctor of

Strote, Noah Benezra

2011-01-01T23:59:59.000Z

440

West Virginia Natural Gas Wellhead Price (Dollars per ...  

U.S. Energy Information Administration (EIA)

West Virginia Natural Gas Wellhead Price (Dollars per Thousand Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 ...

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


441

Underground Injection Control Fee Schedule (West Virginia) | Department of  

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

Injection Control Fee Schedule (West Virginia) Injection Control Fee Schedule (West Virginia) Underground Injection Control Fee Schedule (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Fees Provider Department of Environmental Protection This rule establishes schedules of permit fees for state under-ground injection control permits issued by the Chief of the Office of Water Resources. This rule applies to any person who is required to apply for and

442

Merle West Medical Center Space Heating Low Temperature Geothermal Facility  

Open Energy Info (EERE)

Merle West Medical Center Space Heating Low Temperature Geothermal Facility Merle West Medical Center Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Merle West Medical Center Space Heating Low Temperature Geothermal Facility Facility Merle West Medical Center Sector Geothermal energy Type Space Heating Location Klamath Falls, Oregon Coordinates 42.224867°, -121.7816704° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[]}

443

Solid Waste Assessment Fee Exemptions (West Virginia) | Department of  

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

Solid Waste Assessment Fee Exemptions (West Virginia) Solid Waste Assessment Fee Exemptions (West Virginia) Solid Waste Assessment Fee Exemptions (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Rebate Program A person who owns, operates, or leases an approved solid waste disposal facility is exempt from the payment of solid waste assessment fees, upon the receipt of a Certificate of Exemption from the director, if that

444

SeaWest Windfarms Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Farm Wind Farm Jump to: navigation, search Name SeaWest Windfarms Wind Farm Facility SeaWest Windfarms Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner SeaWest Developer SeaWest Energy Purchaser Pacific Gas & Electric Co Location Altamont Pass CA Coordinates 37.7347°, -121.652° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.7347,"lon":-121.652,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

445

City of West Point, Georgia (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

West Point, Georgia (Utility Company) West Point, Georgia (Utility Company) Jump to: navigation, search Name City of West Point Place Georgia Utility Id 20393 Utility Location Yes Ownership M NERC Location SERC Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Large Commercial Commercial Medium Commercial Commercial Residential Residential Small Commercial Commercial Average Rates Residential: $0.0923/kWh Commercial: $0.1080/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=City_of_West_Point,_Georgia_(Utility_Company)&oldid=410414"

446

MaxWest Environmental Systems | Open Energy Information  

Open Energy Info (EERE)

MaxWest Environmental Systems MaxWest Environmental Systems Jump to: navigation, search Name MaxWest Environmental Systems Place Houston, Texas Zip 77057 Product MaxWest Environmental Systems designs, builds, owns and operates gasification systems on a turnkey basis. Coordinates 29.76045°, -95.369784° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.76045,"lon":-95.369784,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

447

Underground Injection Control (West Virginia) | Department of Energy  

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

Injection Control (West Virginia) Injection Control (West Virginia) Underground Injection Control (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting Provider Department of Environmental Protection This rule set forth criteria and standards for the requirements which apply to the State Underground Injection Control Program (U.I.C.). The UIC permit program regulates underground injections by 5 classes of wells. All owners

448

Policy for Permitting Low-Emitting Sources (West Virginia) | Department  

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

Policy for Permitting Low-Emitting Sources (West Virginia) Policy for Permitting Low-Emitting Sources (West Virginia) Policy for Permitting Low-Emitting Sources (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Siting and Permitting While this policy alleviates some requirements on low-emitting emission sources, it does not change the policy of requiring applicants to submit reasonable information concerning all potential emission sources.

449

Event:Expanded Constituency Workshop for West Africa | Open Energy  

Open Energy Info (EERE)

Expanded Constituency Workshop for West Africa Expanded Constituency Workshop for West Africa Jump to: navigation, search Calendar.png Expanded Constituency Workshop for West Africa: on 2012/09/04 The Global Environment Facility (GEF) is holding an Expanded Constituency Workshop (ECW) for West Africa, as part of the GEF Country Support Programme, including participants from Benin, Cote D'Ivoire, Ghana, Liberia, Nigeria, Sierra leone, Guinea and Togo. The workshop will bring together representatives from civil society, the GEF Secretariat and GEF Agencies, with focal points of the biodiversity, desertification, climate change, and chemicals conventions to discuss activities with global environmental benefits. Civil society organizations are invited to register at the meeting website. Runs September 4 - 6

450

Dam Control and Safety Act (West Virginia) | Department of Energy  

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

Control and Safety Act (West Virginia) Control and Safety Act (West Virginia) Dam Control and Safety Act (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Savings Category Water Buying & Making Electricity Home Weatherization Program Info State West Virginia Program Type Safety and Operational Guidelines Provider Department of Environmental Protection This law grants authority to the secretary of the Department of Environmental Protection to control and exercise regulatory jurisdiction

451

Indeck West Enfield Energy Center Biomass Facility | Open Energy  

Open Energy Info (EERE)

West Enfield Energy Center Biomass Facility West Enfield Energy Center Biomass Facility Jump to: navigation, search Name Indeck West Enfield Energy Center Biomass Facility Facility Indeck West Enfield Energy Center Sector Biomass Location Penobscot County, Maine Coordinates 45.3230777°, -68.5806727° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":45.3230777,"lon":-68.5806727,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

452

West Virginia Smart Grid Implementation Plan (WV SGIP) Project  

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

West Virginia Smart Grid Implementation Plan (WV SGIP) Project West Virginia Smart Grid Implementation Plan (WV SGIP) Project APERC Report on Assessment of As-Is Grid by Non-Utility Stakeholders Introduction One goal of this grid modernization project is to assess the current status of the electric power grid in West Virginia in order to define the potential to implement smart grid technologies. Thus, an initial task of this project was to define the current state or "As-Is" grid in West Virginia. Financial and time constraints prohibited the development and execution of formal surveys to solicit input from the various stakeholders. However attempts were made to obtain their input through informal questionnaires and meeting with focus groups. list of stakeholders which

453

Argonne National Laboratory-West Former Workers, Construction Worker  

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

West Former Workers, Construction West Former Workers, Construction Worker Screening Projects Argonne National Laboratory-West Former Workers, Construction Worker Screening Projects Project Name: Building Trades National Medical Screening Program Covered DOE Site: Argonne National Laboratory-West Worker Population Served: Construction Workers Principal Investigator: Knut Ringen, DrPH, MHA, MPH Toll-free Telephone: 1-800-866-9663 Local Outreach Office: Dan Obray 456 N. Arthur Ave. Pocatello, ID 83204 Website: http://www.btmed.org This project is intended to provide free medical screening to former workers in the building trades (construction workers). The screening targets health problems resulting from exposures, including asbestos, beryllium, cadmium, chromium, lead, mercury, noise, radiation, silica

454

Carbon Dioxide Sequestration (West Virginia) | Department of Energy  

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

Dioxide Sequestration (West Virginia) Dioxide Sequestration (West Virginia) Carbon Dioxide Sequestration (West Virginia) < Back Eligibility Utility Fed. Government Commercial Agricultural Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Residential Installer/Contractor Rural Electric Cooperative Tribal Government Low-Income Residential Schools Retail Supplier Institutional Multi-Family Residential Systems Integrator Fuel Distributor Nonprofit General Public/Consumer Transportation Program Info State West Virginia Program Type Environmental Regulations Fees Safety and Operational Guidelines Siting and Permitting The purpose of this law is to: Establish a legal and regulatory framework for the permitting of carbon dioxide sequestration operations; Designate a state agency responsible for establishing standards and

455

A Regional Approach to Market Monitoring in the West  

E-Print Network (OSTI)

hdocs/docs/ferc/ williamsaes111502osc.pdf Schnitzer, MichaelPrice Caps to the West until FERC Overturns Change, JulyEnergy Regulatory Commission (FERC) 2001a. Docket No. IN01-

Barmack, Matthew; Kahn, Edward; Tierney, Susan; Goldman, Charles

2006-01-01T23:59:59.000Z

456

West Virginia Crude Oil + Lease Condensate Proved Reserves (Million...  

Annual Energy Outlook 2012 (EIA)

+ Lease Condensate Proved Reserves (Million Barrels) West Virginia Crude Oil + Lease Condensate Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

457

Intraseasonal Variability of the West African Monsoon and Atlantic ITCZ  

Science Conference Proceedings (OSTI)

Intraseasonal variability of boreal summer rainfall and winds in tropical West Africa and the east Atlantic is examined using daily Tropical Rainfall Measuring Mission (TRMM) precipitation and the NCEPNCAR reanalysis during 19982006. ...

Eric D. Maloney; Jeffrey Shaman

2008-06-01T23:59:59.000Z

458

West African Monsoon Intraseasonal Variability: A Precipitable Water Perspective  

Science Conference Proceedings (OSTI)

West African monsoon intraseasonal variability has important implications for food security and drought early warnings. In the present study, intraseasonal variability over the Sahel is assessed from the perspective of precipitable water, as ...

D. Emmanuel Poan; Romain Roehrig; Fleur Couvreux; Jean-Philippe Lafore

2013-04-01T23:59:59.000Z

459

New Mexico - West Natural Gas Plant Liquids, Proved Reserves...  

Gasoline and Diesel Fuel Update (EIA)

Gas Plant Liquids, Proved Reserves (Million Barrels) New Mexico - West Natural Gas Plant Liquids, Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

460

West Virginia Natural Gas Plant Liquids, Proved Reserves (Million...  

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

Liquids, Proved Reserves (Million Barrels) West Virginia Natural Gas Plant Liquids, Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

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


461

New Mexico--West Natural Gas Plant Liquids, Proved Reserves ...  

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

Plant Liquids, Proved Reserves (Million Barrels) New Mexico--West Natural Gas Plant Liquids, Proved Reserves (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

462

FirstEnergy (West Penn Power) - Commercial and Industrial Energy...  

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

Source Heat Pumps: 250unit Chillers: 12.50-25ton Custom: 0.05kWh saved annually RefrigerationFood Service Equipment: Varies Provider FirstEnergy (West Penn Power)...

463

Central-West Argentina Summer Precipitation Variability and Atmospheric Teleconnections  

Science Conference Proceedings (OSTI)

The interannual-to-multidecadal variability of central-west Argentina (CWA) summer (OctoberMarch) precipitation and associated tropospheric circulation are studied in the period 19002010. Precipitation shows significant quasi cycles with periods ...

Eduardo A. Agosta; Rosa H. Compagnucci

2012-03-01T23:59:59.000Z

464

West Virginia Natural Gas Total Consumption (Million Cubic Feet...  

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

Total Consumption (Million Cubic Feet) West Virginia Natural Gas Total Consumption (Million Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9...

465

Relative Humidity over the West Florida Continental Shelf  

Science Conference Proceedings (OSTI)

Observed relative humidity variations on the coastal ocean of the West Florida Continental Shelf (WFS) are examined over the 5-yr period 19982003. Despite considerable daily variability within seasons, the monthly mean values are nearly constant ...

J. I. Virmani; R. H. Weisberg

2005-06-01T23:59:59.000Z

466

New Mexico--West Coalbed Methane Proved Reserves (Billion Cubic...  

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

Coalbed Methane Proved Reserves (Billion Cubic Feet) New Mexico--West Coalbed Methane Proved Reserves (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

467

New Mexico--West Coalbed Methane Production (Billion Cubic Feet...  

Gasoline and Diesel Fuel Update (EIA)

Production (Billion Cubic Feet) New Mexico--West Coalbed Methane Production (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's...

468

West Virginia Coalbed Methane Proved Reserves (Billion Cubic...  

Gasoline and Diesel Fuel Update (EIA)

Proved Reserves (Billion Cubic Feet) West Virginia Coalbed Methane Proved Reserves (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9...

469

West Virginia Coalbed Methane Production (Billion Cubic Feet...  

Gasoline and Diesel Fuel Update (EIA)

Production (Billion Cubic Feet) West Virginia Coalbed Methane Production (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 30...

470

West Virginia University Solar Decathlon 2011 Project Manual  

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

File Name: WVUMANUAL2013-02-14.pdf February 14 th , 2013 U.S. DEPARTMENT OF ENERGY SOLAR DECATHLON 2013 Project Manual WVU Solar House West Virginia University...

471

West Coast (PADD 5) Imports from Spain of Gasoline Blending ...  

U.S. Energy Information Administration (EIA)

West Coast (PADD 5) Imports from Spain of Gasoline Blending Components (Thousand Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9;

472

Dynamics of Wet and Dry Years in West Africa  

Science Conference Proceedings (OSTI)

This paper proposes a theoretical framework for describing interannual climatic variability over West Africa. The dynamical theory of zonally symmetrical thermally direct circulations suggests that a meridional monsoon circulation must develop ...

Elfatih A. B. Eltahir; Cuiling Gong

1996-05-01T23:59:59.000Z

473

STUDY COMMISSIONED BY WEST LOTHIAN COUNCIL OIL-SHALE BINGS  

E-Print Network (OSTI)

#12;STUDY COMMISSIONED BY WEST LOTHIAN COUNCIL OIL-SHALE BINGS Dr Barbra Harvie School of Geo.....................................................................................................3 The birth of the oil industry ...........................................................................................................................3 The impact of oil on society

474

West Coast (PADD 5) Imports of Normal Butane-Butylene ...  

U.S. Energy Information Administration (EIA)

West Coast (PADD 5) Imports of Normal Butane-Butylene (Thousand Barrels per Day) Year Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec; 1981: 9: 18: ...

475

West Virginia Natural Gas Pipeline and Distribution Use (Million...  

Annual Energy Outlook 2012 (EIA)

(Million Cubic Feet) West Virginia Natural Gas Pipeline and Distribution Use (Million Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9...

476

An Analysis of West African Dynamics Using a Linearized GCM  

Science Conference Proceedings (OSTI)

This study utilizes a linear, primitive equation spherical model to study the development and propagation of easterly wave disturbances over West Africa. Perturbations are started from an initial disturbance consisting of a barotropic vortex and ...

S. E. Nicholson; A. I. Barcilon; M. Challa

2008-04-01T23:59:59.000Z

477

West Windsor-Plainsboro High School South wins regional Science...  

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

West Windsor-Plainsboro High School South wins regional Science Bowl at PPPL By Jeanne Jackson DeVoe February 25, 2013 Tweet Widget Facebook Like Google Plus One Next stop...

478

West Windsor-Plainsboro High School South wins regional Science...  

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

West Windsor-Plainsboro High School South wins regional Science Bowl at PPPL A dramatic ending to High School Bowl sends local team to nationals By Jeanne Jackson DeVoe February...

479

GeoPowering the West: Hawaii; Why Geothermal?  

DOE Green Energy (OSTI)

This fact sheets provides a summary of geothermal potential, issues, and current development in Hawaii. This fact sheet was developed as part of DOE's GeoPowering the West initiative, part of the Geothermal Technologies Program.

Not Available

2004-04-01T23:59:59.000Z

480

Independent Oversight Activity Report, K-West Annex Facility...  

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

Annex Facility - June 2013 June 2013 Review of the Hanford Site K-West Annex Facility Layup Program for Construction SuspensionDelay HIAR-Hanford-2013-06-10 Construction on...

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


481

A Regional Model Study of Synoptic Features over West Africa  

Science Conference Proceedings (OSTI)

Synoptic weather features over West Africa were studied in simulations by the regional simulation model (RM) at the NASA Goddard Institute for Space Studies. These pioneering simulations represent the beginning of an effort to adapt regional ...

Leonard M. Druyan; Matthew Fulakeza; Patrick Lonergan; Mahaman Saloum

2001-06-01T23:59:59.000Z

482

West Coast Aerial Sardine Survey Application for Exempted Fishing Permit  

E-Print Network (OSTI)

West Coast Aerial Sardine Survey 2010 Application for Exempted Fishing Permit Applicants ........................................................................................5 A. Coastwide Summer Aerial Sardine Survey (July-August, 2010) ....................6 I. Survey Design ­ Coastwide Summer Aerial Sardine Survey ...............................6 Stage 1: Aerial Transect

483

SeaWest WindPower Inc | Open Energy Information  

Open Energy Info (EERE)

92108-4310 Sector Services, Wind energy Product SeaWest is a turnkey developer of wind power plants. Their services include consultancy on the market viability, site and...

484

oil and Gas Resources of the West Siberian Basin, Russia  

U.S. Energy Information Administration (EIA)

IOIP 7758 (1 S w) Bo IGIP 7758 (1 Sw) B g VO IOIP A h 1,000,000 VG IGIP A h 1,000,000 Energy Information Administration Oil and Gas Resources of the West ...

485

West Virginia Crude Oil Reserves in Nonproducing Reservoirs ...  

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

Reserves in Nonproducing Reservoirs (Million Barrels) West Virginia Crude Oil Reserves in Nonproducing Reservoirs (Million Barrels) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

486

New Mexico - West Dry Natural Gas Reserves Estimated Production...  

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

Estimated Production (Billion Cubic Feet) New Mexico - West Dry Natural Gas Reserves Estimated Production (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

487

New Mexico - West Dry Natural Gas Reserves Revision Increases...  

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

Increases (Billion Cubic Feet) New Mexico - West Dry Natural Gas Reserves Revision Increases (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

488

New Mexico - West Dry Natural Gas Reserves Acquisitions (Billion...  

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

Acquisitions (Billion Cubic Feet) New Mexico - West Dry Natural Gas Reserves Acquisitions (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8...

489

New Mexico - West Dry Natural Gas Reserves New Field Discoveries...  

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

New Field Discoveries (Billion Cubic Feet) New Mexico - West Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5...

490