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1

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

2

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

3

MidAmerican Energy (Electric) - Residential Energy Efficiency...  

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

Electric) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings...

4

MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate  

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

MidAmerican Energy (Electric) - Residential Energy Efficiency MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Heat Pumps Program Info Start Date 1/1/2011 Expiration Date 12/31/2012 State Illinois Program Type Utility Rebate Program Rebate Amount Room Air Conditioners: $25 Central Air Conditioners: $100-$200 Heat Pumps: $100-$400 Ground-source Heat Pumps: $1000-$2000 Desuperheaters: $100 Programmable Thermostat: $20 Provider MidAmerican Energy Company MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of participating homes. Electric customers of MidAmerican Energy qualify for rebates on programmable thermostats, air

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MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs |  

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

Gas) - Residential Energy Efficiency Rebate Gas) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Heating Appliances & Electronics Water Heating Program Info State Illinois Program Type Utility Rebate Program Rebate Amount Furnaces: $250 - $400 Boilers: $150 - $400 Water Heaters: $50 - $300 Provider MidAmerican Energy Company '''The availability of rebates through this program is unclear. Contact MidAmerican regarding the availability of gas incentives for residential customers.''' MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of eligible homes. The Residential Equipment Brochure on the program web site above provides specific rebate

6

MidAmerican Energy (Electric) - Municipal Solid-State Lighting...  

Open Energy Info (EERE)

must be an Iowa electric governmental customer of MidAmerican Energy Company. Light-emitting diode and induction types of solid state lighting (SSL) qualify under this program....

7

MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate  

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

MidAmerican Energy (Electric) - Residential Energy Efficiency MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Appliances & Electronics Heat Pumps Commercial Lighting Lighting Water Heating Other Program Info Expiration Date 12/31/2013 State Iowa Program Type Utility Rebate Program Rebate Amount Room Air Conditioners: $25 Central Air Conditioners: $100-$200 Heat Pumps: $100-$400 Ground-source Heat Pumps: $1000-$2000 Desuperheaters: $100 Heat Pump Water Heaters: $100 Water Heaters: $50 Washer/Dryer: $50/unit Hard-Wired Light Fixture: $20/fixture Refrigerator: $50 Freezer: $25 Dishwasher: $20 Appliance Recycling: $25-$50/unit

8

MidAmerican Energy (Gas and Electric) - Commercial New Construction  

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

MidAmerican Energy (Gas and Electric) - Commercial New Construction MidAmerican Energy (Gas and Electric) - Commercial New Construction Energy-Efficiency Program MidAmerican Energy (Gas and Electric) - Commercial New Construction Energy-Efficiency Program < Back Eligibility Commercial Fed. Government Industrial Local Government Nonprofit State Government Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Commercial Heating & Cooling Cooling Construction Design & Remodeling Other Sealing Your Home Ventilation Heat Pumps Heating Appliances & Electronics Commercial Lighting Lighting Manufacturing Windows, Doors, & Skylights Solar Program Info State Iowa Program Type Utility Rebate Program Rebate Amount Construction rebates: $0.06-$0.19/kWh saved; $0.60-$1.90/therm saved based on % savings from Iowa Energy Code

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MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs |  

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

Appliances & Electronics Appliances & Electronics Water Heating Program Info Expiration Date 12/31/2013 State Iowa Program Type Utility Rebate Program Rebate Amount Natural Gas Furnace: $250 - $400 Efficient Furnace Fan Motor: $50 Natural Gas Boiler: $150 - $400 Natural Gas Water Heater: $50 - $300 Programmable thermostat: $20 Provider MidAmerican Energy MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of eligible homes. The Residential Equipment Brochure on the program web site above provides specific rebate amounts, efficiency requirements and further details. After installing qualifying equipment, customers should submit a completed Equipment Rebate Application and a detailed invoice to MidAmerican. Heating and cooling

10

MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate  

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

Electric) - Residential Energy Efficiency Electric) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Electric) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Heat Pumps Appliances & Electronics Water Heating Program Info Expiration Date 12/31/2013 State South Dakota Program Type Utility Rebate Program Rebate Amount Electric Water Heaters: $50 Room Air Conditioning Unit: $40 Central Air Conditioning: $150 - $1625 Air-to-Air Heat Pumps: $150 - $1700 Add-on Heat Pumps: $150 - $1700 Provider MidAmerican Energy Company MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of their homes. Eligible customers are eligible for rebates on water heaters, air conditioners, air-source heat

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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":""}]}

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MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs |  

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

Home Weatherization Home Weatherization Commercial Weatherization Manufacturing Appliances & Electronics Water Heating Program Info Start Date 1/1/2011 Expiration Date 12/31/2012 State South Dakota Program Type Utility Rebate Program Rebate Amount Furnaces: $250-$400 Furnace Fan Motors: $50 Boilers: $150-$400 Water Heaters: $50-$100 Energy Audit: Free including water heater/pipe insulation Building Insulation: 70% or $750 Provider MidAmerican Energy Company MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of homes. Eligible customers are eligible for rebates on furnaces, furnace fan motors, boilers, water heaters, air conditioners, air-source heat pumps, geothermal heat pumps and insulation. Customers should see the equipment brochure for more rebate information and

13

MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs |  

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

Gas) - Residential Energy Efficiency Rebate Gas) - Residential Energy Efficiency Rebate Programs MidAmerican Energy (Gas) - Residential Energy Efficiency Rebate Programs < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Heating Commercial Weatherization Manufacturing Appliances & Electronics Water Heating Program Info Expiration Date 12/31/2013 State Nebraska Program Type Utility Rebate Program Rebate Amount Energy Audit: Free Furnaces: $250-$400 Boilers: $150 or $400 Water Heaters: $50 or $100 Provider Remittance MidAmerican Energy offers basic energy efficiency incentives for residential customers in Nebraska to improve the comfort and savings in participating homes. These incentives include gas heating equipment such as boilers, furnaces, and water heaters. Free energy audits are also available

14

Thom Mason | ornl.gov  

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

Find People Find People General Contacts Leadership Team Media Contacts User Facility Contacts Internal Users Home | Our People | Leadership Team SHARE Thom Mason Laboratory Director Thom Mason Dr. Mason, who became Laboratory Director July 1, 2007, is an experimental condensed matter physicist whose primary research tool has been neutron scattering, supplemented by the use of X rays and transport and thermodynamic measurements. As Laboratory Director he is responsible for a diverse portfolio of science and energy R&D spanning fundamental research in physics, biology, and chemistry through climate change; energy generation, distribution, and end use; and national security programs. Operating responsibilities include a nuclear reactor, a high-power proton accelerator, classified activities, and a complex array of research

15

MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant  

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

MidAmerican Energy (Electric) - Municipal Solid-State Lighting MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant Program MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant Program < Back Eligibility Local Government Savings Category Appliances & Electronics Commercial Lighting Lighting Maximum Rebate Minimum project size for the full $5,000 grant is 20 fixtures; smaller projects will receive a $250 per-fixture grant. Program Info State Iowa Program Type Utility Grant Program Rebate Amount Up to $5,000 Provider MidAmerican Energy Company MidAmerican Energy offers grants to munipalities which implement solid-state roadway street lighting upgrades. Grants of up to $5,000 are available to participating entities who install eligible roadway lighting fixtures. Participants must be an Iowa electric governmental customer of

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MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program |  

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

MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Agricultural Commercial Construction Industrial Institutional Nonprofit Schools Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Commercial Heating & Cooling Cooling Other Construction Manufacturing Heat Pumps Appliances & Electronics Commercial Lighting Lighting Water Heating Maximum Rebate Insulation: 70% of cost; ebates exceeding $10,000 require preapproval Variable-Speed Drives: 70% of cost Custom: All project installations with rebates exceeding $20,000 require on-site verification Program Info State Illinois Program Type Utility Rebate Program Rebate Amount

17

Microsoft Word - CX_Memo_Mason.docx  

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

5, 2012 5, 2012 REPLY TO ATTN OF: KEC-4 SUBJECT: Environmental Clearance Memorandum Robert Trismen Project Manager - TEP-CSB-1 Proposed Action: Mason Substation Metering Replacement Project Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B1.7 Electronic equipment. Location: Mason County, Washington Proposed by: Bonneville Power Administration (BPA) Description of the Proposed Action: BPA is proposing to remove existing equipment and install new revenue metering equipment in the existing Mason Substation. Mason County Public Utility District No. 3 (the District), a customer of BPA, owns and operates Mason Substation and plans to rebuild it as a 115/12.5 kV, 24 MVA facility. Mason Substation is a BPA Point of

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MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant  

Open Energy Info (EERE)

MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant Program (Iowa) 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 November 9, 2012. Financial Incentive Program Place Iowa Additional Place applies to MidAmerican Energy Name MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant Program Incentive Type Utility Grant Program Applicable Sector Local Government Eligible Technologies Lighting, Lighting Controls/Sensors, Induction Lighitng, LED Lighting Active Incentive Yes Implementing Sector Utility Energy Category Energy Efficiency Incentive Programs Amount Up to $5,000 Equipment Requirements Fixtures must have an efficiency rating equal to or greater than 66 lumens per watt as tested under Illuminating Engineering Society of North America LM-79-08 testing to qualify for a grant.

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Mason, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Login | Sign Up Search Page Edit with form History Facebook icon Twitter icon Mason, Ohio: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates...

20

MidAmerican Energy Co (South Dakota) | Open Energy Information  

Open Energy Info (EERE)

South Dakota South Dakota Utility Id 12341 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 Residential, Base Use - Price Schedule RBD Residential Average Rates Residential: $0.0701/kWh Commercial: $0.0670/kWh Industrial: $0.0403/kWh The following table contains monthly sales and revenue data for MidAmerican Energy Co (South Dakota). Month RES REV (THOUSAND $) RES SALES (MWH) RES CONS COM REV (THOUSAND $) COM SALES (MWH) COM CONS IND_REV (THOUSAND $) IND SALES (MWH) IND CONS OTH REV (THOUSAND $) OTH SALES (MWH) OTH CONS TOT REV (THOUSAND $) TOT SALES (MWH) TOT CONS 2009-03 194.993 2,939.31 3,394 175.381 2,708.24 769 322.555 8,514.71 22 692.929 14,162.26 4,185

Note: This page contains sample records for the topic "mason ia midamerican" 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

MidAmerican Energy Co (Illinois) | Open Energy Information  

Open Energy Info (EERE)

Illinois Illinois Utility Id 12341 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 Rate NO. 10 Residence Electric Service Residential Rate NO. 10 Residence Electric Service Residential Average Rates Commercial: $0.0135/kWh The following table contains monthly sales and revenue data for MidAmerican Energy Co (Illinois). Month RES REV (THOUSAND $) RES SALES (MWH) RES CONS COM REV (THOUSAND $) COM SALES (MWH) COM CONS IND_REV (THOUSAND $) IND SALES (MWH) IND CONS OTH REV (THOUSAND $) OTH SALES (MWH) OTH CONS TOT REV (THOUSAND $) TOT SALES (MWH) TOT CONS 2009-03 3,715.539 48,604.05 75,610 3,009.136 52,899.71 9,170 2,446.37 74,307.41 90 9,171.045 175,811.17 84,870

22

Mr. James R. Mason, Chief  

Office of Legacy Management (LM)

0 High Street - 0 High Street - May 6,' 1952 Mr. James R. Mason, Chief Radioisotopes Branch 6 Isotopes Division Oak Ridge Opertions Oak Ridge, Tennessee I Dear Mr. Hason: The purpose af this letter is to learn what steps this laboratory must'take in order to secure, on shqrt notice and at intermittent intervals, a one-week irradiation of normal U3OS, either at Oak Ridge or in the thermal column at Brookhavetii. During the past two years, Tracerlab has received about 25 such irradiations, for work on a secret contract with the Air Force. On last January 24, we placed an order similar to all previous orders. At the same time, someone in the N. Y. Operations Office decided to change our accountability status. The ensuing confusion and delay was the subject of numerous telephone calls

23

MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program |  

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

MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Agricultural Commercial Construction Industrial Institutional Nonprofit Schools Savings Category Heating & Cooling Commercial Heating & Cooling Heating Home Weatherization Commercial Weatherization Cooling Other Construction Manufacturing Appliances & Electronics Water Heating Maximum Rebate Insulation: 70% of cost Program Info State Illinois Program Type Utility Rebate Program Rebate Amount Furnaces: $250-$350 Boilers: $100-$400 Water Heaters: $50 Programmable Thermostats: $20 Cooking Equipment: Varies widely Attic/Roof/Ceiling Insulation: $0.015/R-value increase per sq. ft. Sidewall Insulation: $0.01/R-value increase per sq. ft.

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MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program |  

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

MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Commercial Fed. Government Local Government Nonprofit State Government Savings Category Heating & Cooling Commercial Heating & Cooling Heating Home Weatherization Commercial Weatherization Sealing Your Home Design & Remodeling Windows, Doors, & Skylights Appliances & Electronics Commercial Lighting Lighting Water Heating Program Info State Iowa Program Type Utility Rebate Program Rebate Amount Furnaces: $250-$400 Fan Motors for Natural Gas Furnaces: $50 Boilers: $150-$400 or $0.80/MBtuh x $0.20/TE over 82 Water Heaters/Tankless Water Heaters: $50-$300 or $0.80/MBtuh x $0.20/TE over 85 Programmable Thermostats: $20

25

MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program |  

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

MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Commercial Fed. Government Local Government Nonprofit State Government Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Commercial Heating & Cooling Cooling Sealing Your Home Design & Remodeling Windows, Doors, & Skylights Heat Pumps Appliances & Electronics Commercial Lighting Lighting Manufacturing Water Heating Maximum Rebate See applicable program brochure on program website for maximum rebate levels Program Info State Iowa Program Type Utility Rebate Program Rebate Amount CFL Lamp: up to $2/lamp CFL Fixture (Hardwired): $20/fixture T5/T8 Fluorescent Lighting: $6-$42/fixture

26

MidAmerican Energy (Gas and Electric) - Residential EnergyAdvantage Loan  

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

Gas and Electric) - Residential EnergyAdvantage Gas and Electric) - Residential EnergyAdvantage Loan Program MidAmerican Energy (Gas and Electric) - Residential EnergyAdvantage Loan Program < Back Eligibility Installer/Contractor Residential Savings Category Heating & Cooling Commercial Heating & Cooling Heating Cooling Other Home Weatherization Commercial Weatherization Sealing Your Home Ventilation Heat Pumps Appliances & Electronics Water Heating Windows, Doors, & Skylights Maximum Rebate not specified Program Info Start Date 1/1/2011 State Iowa Program Type Utility Loan Program Rebate Amount Joint check payable to customer and dealer Provider MidAmerican Energy MidAmerican Energy's EnergyAdvantage Financing Program, in partnership with First American Bank, offers Iowa residential energy customers below-prime

27

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

28

Mason County PUD 3 - Commercial and Industrial Energy Rebates | Department  

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

Commercial and Industrial Energy Rebates Commercial and Industrial Energy Rebates Mason County PUD 3 - Commercial and Industrial Energy Rebates < Back Eligibility Agricultural Commercial Construction Fed. Government Industrial Local Government Nonprofit State Government Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Construction Commercial Heating & Cooling Design & Remodeling Other Appliances & Electronics Commercial Lighting Lighting Manufacturing Program Info State District of Columbia Program Type Utility Rebate Program Rebate Amount Lighting Rebates: Up to 70% of project cost Prescriptive Rebates: Varies widely, contact Mason County PUD 3 Custom Rebates: Varies widely, contact Mason County PUD 3 Provider Mason County PUD 3 Mason County PUD 3 offers rebates to its non-residential customers for

29

Mason, Michigan: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Mason, Michigan: Energy Resources Mason, Michigan: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.5792027°, -84.4435845° 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":42.5792027,"lon":-84.4435845,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

30

MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program |  

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

Commercial EnergyAdvantage Rebate Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Electric) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Agricultural Commercial Construction Industrial Institutional Nonprofit Schools Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Commercial Heating & Cooling Cooling Other Construction Manufacturing Heat Pumps Appliances & Electronics Commercial Lighting Lighting Water Heating Program Info Expiration Date 12/31/2012 State South Dakota Program Type Utility Rebate Program Rebate Amount Variable-Speed Drives: $30/HP Clothes Washer: $100 Dishwasher: $20 Vending Machine Controller: $50 Fluorescent Lighting: $6-$42/fixture Lighting Occupancy Sensors: $20/sensor Pulse Start Metal Halide Lighting: $25 or $50/fixture

31

Mason Energy + Management | Open Energy Information  

Open Energy Info (EERE)

+ Management + Management Jump to: navigation, search Logo: Mason Energy + Management Name Mason Energy + Management Address 790 Racquet Lane Place Boulder, Colorado Zip 80303 Sector Buildings, Efficiency, Services Product Energy Efficiency for Commercial Buildings Year founded 2009 Number of employees 1-10 Phone number 720 242-7088 Website http://www.masoneam.com Coordinates 40.002049°, -105.222508° 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":40.002049,"lon":-105.222508,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

32

MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program |  

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

Commercial EnergyAdvantage Rebate Commercial EnergyAdvantage Rebate Program MidAmerican Energy (Gas) - Commercial EnergyAdvantage Rebate Program < Back Eligibility Agricultural Commercial Construction Industrial Institutional Nonprofit Schools Savings Category Heating & Cooling Commercial Heating & Cooling Heating Home Weatherization Commercial Weatherization Cooling Other Construction Manufacturing Appliances & Electronics Water Heating Program Info State South Dakota Program Type Utility Rebate Program Rebate Amount Attic/Roof/Ceiling Insulation: $0.015 x R-value increase x sq. ft. Wall Insulation: $0.01 x R-value increase x sq. ft. Furnaces: $250-$400 Fan Motors for Furnaces: $50 Boilers: $150-$400 or ($0.80+($0.20 x TE) x MBtuh Water Heaters: $75 or ($0.80+($0.20 x TE) x MBtuh Programmable Thermostats: $25

33

DOE/EIS-0456 CUSHMAN HYDROELECTRIC PROJECT MASON COUNTY, WASHINGTON  

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

6 6 CUSHMAN HYDROELECTRIC PROJECT MASON COUNTY, WASHINGTON (FERC PROJECT NO. 460) FINAL ENVIRONMENTAL IMPACT STATEMENT (FERC/EIS-0095F, ADOPTED AS DOE/EIS-0456) US Department of Energy OCTOBER 2010 Lead Agency: U.S. Department of Energy (DOE) Title: Final Environmental Impact Statement (FEIS) for the Cushman Hydroelectric Project, Mason County, Washington (Adopted) Contact: For additional copies or more information on this final environmental impact statement (EIS), please

34

Fleming-Mason Energy Coop Inc | Open Energy Information  

Open Energy Info (EERE)

Fleming-Mason Energy Coop Inc Fleming-Mason Energy Coop Inc Jump to: navigation, search Name Fleming-Mason Energy Coop Inc Place Kentucky Utility Id 6442 Utility Location Yes Ownership C NERC Location RFC NERC RFC 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 All Electric School High Pressure Sodium - 22000 Lumen Directional Lighting High Pressure Sodium - 22000 Lumen Ornamental Lighting High Pressure Sodium - 22000 Lumen Standard Lighting High Pressure Sodium - 50000 Lumen Directional Lighting High Pressure Sodium - 50000 Lumen Ornamental Lighting High Pressure Sodium - 50000 Lumen Standard Lighting

35

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

Open Energy Info (EERE)

Mason Mason Place Texas Utility Id 11793 Utility Location Yes Ownership M NERC Location TRE NERC ERCOT Yes Activity Distribution 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 Commercial Service Rates Commercial Residential service Residential Street Lights(Rental) Lighting Average Rates Residential: $0.1150/kWh Commercial: $0.1160/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_Mason,_Texas_(Utility_Company)&oldid=409926"

36

Mason County PUD 3 - Residential Energy Rebates | Department of Energy  

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

Mason County PUD 3 - Residential Energy Rebates Mason County PUD 3 - Residential Energy Rebates Mason County PUD 3 - Residential Energy Rebates < Back Eligibility Construction Residential Savings Category Home Weatherization Commercial Weatherization Sealing Your Home Ventilation Heating & Cooling Commercial Heating & Cooling Heat Pumps Appliances & Electronics Water Heating Program Info State District of Columbia Program Type Utility Rebate Program Rebate Amount Energy Audit: Free Clothes Washer: $30 - $70 Refrigerator/Freezer: $15 Decommissioned Refrigerator/Freezer: $30 Storage Water Heater: $25 Heat Pump Water Heater: $300 - $500 PTSC Duct Sealing: $400 - $500 Insulation: Varies based on R-Value increase and location Air Source Heat Pump (conversion): $1,400 - $1,900 Ductless Heat Pump System: $1,500

37

PUD No 3 of Mason County | Open Energy Information  

Open Energy Info (EERE)

3 of Mason County 3 of Mason County Jump to: navigation, search Name PUD No 3 of Mason County Place Washington Utility Id 15419 Utility Location Yes Ownership P NERC WECC Yes ISO Other Yes Activity Transmission Yes Activity Buying Transmission Yes Activity Distribution Yes Activity Wholesale Marketing Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 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 1,000 Watt Commercial 200 WATT Commercial 300 WATT Commercial 400 WATT Commercial 500 WATT Commercial 600 WATT Commercial 700 WATT Commercial 800 WATT Commercial 900 WATT Commercial LOW INCOME AND SENIOR DISABILITY ACCOUNT Residential

38

Consent Order, Mason & Hanger Corporation - EA-2000-07 | Department of  

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

Mason & Hanger Corporation - EA-2000-07 Mason & Hanger Corporation - EA-2000-07 Consent Order, Mason & Hanger Corporation - EA-2000-07 June 21, 2000 Price-Anderson Enforcement Consent Order issued to Mason & Hanger Corporation related to Fire Suppression System Issues at the Pantex Plant, (EA-2000-07) 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. Consent Order, Mason & Hanger Corporation - EA-2000-07 More Documents & Publications Preliminary Notice of Violation, Argonne National Laboratory-West - EA-2001-01 Preliminary Notice of Violation, Mason & Hanger Corporation - EA-1999-05

39

The hymn tunes of Lowell Mason: a performance edition of five settings for brass quintet.  

E-Print Network (OSTI)

??Lowell Mason (1792-1872) was an influential figure in the development of American music in the nineteenth century. In addition to being one of the first (more)

McIvor, Christian Clinton

2011-01-01T23:59:59.000Z

40

Renewable Resources: a national catalog of model projects. Volume 2. Mid-American Solar Energy Complex Region  

DOE Green Energy (OSTI)

This compilation of diverse conservation and renewable energy projects across the United States was prepared through the enthusiastic participation of solar and alternate energy groups from every state and region. Compiled and edited by the Center for Renewable Resources, these projects reflect many levels of innovation and technical expertise. In many cases, a critique analysis is presented of how projects performed and of the institutional conditions associated with their success or failure. Some 2000 projects are included in this compilation; most have worked, some have not. Information about all is presented to aid learning from these experiences. The four volumes in this set are arranged in state sections by geographic region, coinciding with the four Regional Solar Energy Centers. The table of contents is organized by project category so that maximum cross-referencing may be obtained. This volume includes information on the Mid-American Solar Energy Complex Region. (WHK)

None

1980-07-01T23:59:59.000Z

Note: This page contains sample records for the topic "mason ia midamerican" 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

PUD No 1 of Mason County | Open Energy Information  

Open Energy Info (EERE)

County County Place Washington Utility Id 22355 Utility Location Yes Ownership P NERC Location WECC 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 General Service Three Phase Commercial General Service-Single Phase Commercial Residential Service Residential Security Lights 100 watt high pressure sodium Lighting Average Rates Residential: $0.0872/kWh Commercial: $0.0837/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=PUD_No_1_of_Mason_County&oldid=411313

42

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...

43

Preliminary Notice of Violation, Mason & Hanger Corporation - EA-1999-05 |  

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

& Hanger Corporation - & Hanger Corporation - EA-1999-05 Preliminary Notice of Violation, Mason & Hanger Corporation - EA-1999-05 July 30, 1999 Preliminary Notice of Violation issued to Mason & Hanger Corporation, related to a Chemical Fire at the Pantex Plant, (EA-1999-05 This letter refers to the Department of Energy's (DOE) evaluation of an [chemical] fire in Building 12-044, Cell 3, on December 29, 1998, during cleaning operations on a weapon component. Inadequate controls to mitigate the fire hazard posed by the [chemical] were determined to be the root cause of the event. However, the failure to adhere to existing procedural controls was determined to be a significant contributing cause. Preliminary Notice of Violation, Mason & Hanger Corporation - EA-1999-05

44

Preliminary Notice of Violation, Mason and Hanger Corporation - EA-97-02 |  

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

and Hanger Corporation - and Hanger Corporation - EA-97-02 Preliminary Notice of Violation, Mason and Hanger Corporation - EA-97-02 June 5, 1997 Preliminary Notice of Violation issued to Mason and Hanger Corporation related to Inaccurate Training and Certification Records at the Pantex Plant, (EA-97-02) This letter refers to the Department of Energy's (DOE) evaluation of alleged irregularities associated with training requirements for Production Technicians who performed work in the W55 nuclear weapons dismantlement program in [building]. The DOE Office of Enforcement and Investigation initiated its inquiry on December 4, 1996, after several workers communicated concerns to the DOE Amarillo Area Office regarding the accuracy of weapon work proficiency records. The DOE's Investigation

45

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

46

A Quick Guide for Applying at Mason Applying online is as easy as 1-2-3!  

E-Print Network (OSTI)

Jobs" from the quick links.. You can search jobs in the following ways: · Keywords - enter your own search terms · Posted Within - a drop-down list will appear ­ select from day, week, or month Innovation Is Tradition Page 1 of 6 11/15/2012 #12;A Quick Guide for Applying at Mason Step 1: Search

47

Thomas Mason Oak Ridge National Lab July 10 2012 SB Summit  

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

National Laboratory Presented to the DOE/NNSA Regional Small Business Summit Thomas E. Mason Director, Oak Ridge National Laboratory Knoxville, Tennessee July 10, 2012 2 Managed by UT-Battelle for the U.S. Department of Energy RegionalSummit_1207 ORNL is DOE's largest science and energy laboratory 2 Managed by UT-Battelle for the U.S. Department of Energy $1.65B budget World's most intense neutron source 4,400 employees World-class research reactor 3,000 research guests annually $500M modernization investment Nation's largest materials research portfolio Most powerful open scientific computing facility Nation's most diverse energy portfolio Managing billion-dollar U.S. ITER project 3 Managed by UT-Battelle for the U.S. Department of Energy RegionalSummit_1207

48

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

49

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

50

GREEN PURCHASING GUIDE THE FOLLOWING PRODUCTS CAN BE FOUND ON W.B. MASON'S GREEN PRODUCTS PAGE AND HAVE BEEN SELECTED BY THE CAMPUS  

E-Print Network (OSTI)

COMPOSTABLE COMPOSTABLE COMPOSTABLE HYPERLINK LIGHT BULBS **ALL COMPACT FLUORESCENT (CFL) AND LED LIGHT BULBS OF BULBS PROPERLY. THE LED BULBS FROM WB MASON ARE SIGNIFICANTLY (5-6X) MORE EXPENSIVE THAN THOSE FOUND

Massachusetts at Amherst, University of

51

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

52

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":""}]}

53

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

54

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

55

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

56

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

57

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...

58

Evolution of suprathermal seed particle and solar energetic particle R. A. Mewaldt, G. M. Mason, C. M. S. Cohen, R. Gmez-Herrero, D. K. Haggerty et al.  

E-Print Network (OSTI)

). 25. R. Müller-Mellin et al., Solar Physics 162, 483 (1995). 26. G. M. Mason et al., Space Sci. RevEvolution of suprathermal seed particle and solar energetic particle abundances R. A. Mewaldt, G. M incidence x-ray fluorescence technique to discriminate and quantify implanted solar wind J. Appl. Phys. 105

Jensen, Grant J.

59

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

60

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,...

Note: This page contains sample records for the topic "mason ia midamerican" 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

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

62

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

63

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

64

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

65

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.

66

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,

67

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...

68

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

69

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

70

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

71

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

72

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

73

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

74

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

75

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

76

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

77

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

78

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

79

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

80

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

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81

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

82

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

83

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

84

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

85

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

86

Category:SecondarySchool | Open Energy Information  

Open Energy Info (EERE)

IA MidAmerican Energy Co (Iowa).png SVSecondarySchool Des ... 68 KB SVSecondarySchool Detroit MI Detroit Edison Co.png SVSecondarySchool Detr... 66 KB SVSecondarySchool El Paso TX...

87

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

88

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

89

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

90

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

91

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

92

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

93

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

94

Nicole Darnall George Mason University  

E-Print Network (OSTI)

tetrachloride, denitrification 1. Introduction Groundwater contamination originates from a variety of sources, including synthetic organic chemicals, metal ions, petroleum products, volatile organic compounds

Darnall, Nicole

95

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

96

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

97

MidAmerican Energy Co (Ohio) | Open Energy Information  

Open Energy Info (EERE)

Retrieved from "http:en.openei.orgwindex.php?titleMidAmericanEnergyCo(Ohio)&oldid412693" Categories: EIA Utility Companies and Aliases Utility Companies...

98

MidAmerican Energy (Electric) - Residential Energy Efficiency...  

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

Air Conditioners: 25 Central Air Conditioners: 100-200 Heat Pumps: 100-400 Ground-source Heat Pumps: 1000-2000 Desuperheaters: 100 Heat Pump Water Heaters: 100 Water...

99

MidAmerican Energy (Gas and Electric) - Commercial New Construction...  

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

Iowa Program Type Utility Rebate Program Rebate Amount Construction rebates: 0.06-0.19kWh saved; 0.60-1.90therm saved based on % savings from Iowa Energy Code Design rebates:...

100

MidAmerican Energy Co | Open Energy Information  

Open Energy Info (EERE)

Iowa Iowa Utility Id 12341 Utility Location Yes Ownership I NERC MRO Yes NERC RFC Yes ISO MISO Yes Operates Generating Plant Yes Activity Generation Yes Activity Transmission Yes Activity Buying Transmission Yes Activity Distribution Yes Activity Buying Distribution Yes Activity Wholesale Marketing Yes Activity Retail Marketing Yes Activity Bundled Services Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] Energy Information Administration Form 826[2] 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 Contract Power - Price Schedule LJD - (John Deere Waterloo Works)

Note: This page contains sample records for the topic "mason ia midamerican" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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101

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

102

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...

103

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

104

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

105

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

106

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

107

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

108

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

109

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

110

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

111

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

112

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

113

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

114

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

115

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

116

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

117

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

118

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

119

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

120

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 "mason ia midamerican" 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

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

122

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

123

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

124

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

125

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

126

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

127

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

128

GEORGE MASON UNIVERSITY TAX DEFERRED SAVINGS PLAN  

E-Print Network (OSTI)

­Tax $_______________ or ______________% TIAA-CREF Pre-Tax $_______________ or ______________% TIAA-CREF Roth Post­Tax $_______________ or ______________% Effective Pay Date (mm/dd/year) ______________ *Only salaried employee contributions to TIAA-CREF & Fidelity

129

GEORGE MASON UNIVERSITY TAX DEFERRED SAVINGS PLAN  

E-Print Network (OSTI)

­Tax $_______________ or ______________% TIAA-CREF Pre-Tax $_______________ or ______________% TIAA-CREF Roth Post

130

George Mason University 2012 College of Science ...  

Science Conference Proceedings (OSTI)

... reality is far from Hollywood's projection of instant ... up when I initially failed with some projects. ... Oppenheimer, who led the Manhattan Project to build ...

2012-05-17T23:59:59.000Z

131

George Mason University Laboratory Safety Manual  

E-Print Network (OSTI)

.4.3 Chemical/Biological or Chemical/Radioactive Waste Disposal .... 11-3 11.4.4 Cylinder Disposal corrective actions as necessary. · Manage radioactive waste generated in instructional and research.3.11 Director of MRI Safety and Operations...................................1-8 1.3.12 Waste Management

132

Mason-0124123 - Argonne National Laboratories, Materials Sicence...  

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

measured work function. Materials to be considered in the talk include pure and tin-doped indium oxide (In2O3, ITO), pure and Al-doped zinc oxide (ZnO, AZO), pure and...

133

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

134

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

135

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

136

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

137

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

138

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

139

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

140

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

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to obtain the most current and comprehensive results.


141

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

142

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

143

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

144

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

145

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

146

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

147

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

148

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

149

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

150

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

151

LAX XXlCfl jX?iK, Idd+?KYLViG?IA  

Office of Legacy Management (LM)

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152

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

153

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

154

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

155

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

156

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

157

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

158

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

159

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

160

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

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to obtain the most current and comprehensive results.


161

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

162

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

163

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

164

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

165

Adair Wind Farm II | Open Energy Information  

Open Energy Info (EERE)

II II Jump to: navigation, search Name Adair Wind Farm II Facility Adair Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location IA Coordinates 41.499234°, -94.692628° 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":41.499234,"lon":-94.692628,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

166

Pomeroy III Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Pomeroy III Wind Farm Pomeroy III Wind Farm Facility Pomeroy III Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Pocahontas County IA Coordinates 42.570484°, -94.702506° 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":42.570484,"lon":-94.702506,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

167

Pomeroy IV Wind Farm | Open Energy Information  

Open Energy Info (EERE)

IV Wind Farm IV Wind Farm Facility Pomeroy IV Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Pomeroy IA Coordinates 42.570484°, -94.702506° 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":42.570484,"lon":-94.702506,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

168

Charles City (2Q08) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

2Q08) Wind Farm 2Q08) Wind Farm Facility Charles City (2Q08) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Charles City IA Coordinates 43.004101°, -92.722392° 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":43.004101,"lon":-92.722392,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

169

Carroll Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Carroll Wind Farm Carroll Wind Farm Jump to: navigation, search Name Carroll Wind Farm Facility Carroll Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Carroll County IA Coordinates 42.112208°, -94.910631° 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":42.112208,"lon":-94.910631,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

170

Century Expansion (4Q07) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Century Expansion (4Q07) Wind Farm Century Expansion (4Q07) Wind Farm Facility Century Expansion (4Q07) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location IA Coordinates 42.495789°, -93.652368° 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":42.495789,"lon":-93.652368,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

171

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

172

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

173

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

174

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

175

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

176

MidAmerican Energy (Gas and Electric) - Residential EnergyAdvantage...  

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

Energy's EnergyAdvantage Financing Program, in partnership with First American Bank, offers Iowa residential energy customers below-prime financing on installation of...

177

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

178

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

179

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

180

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

Note: This page contains sample records for the topic "mason ia midamerican" 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

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

182

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

183

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

184

A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae  

E-Print Network (OSTI)

The dynamics of the explosive burning process is highly sensitive to the flame speed model in numerical simulations of type Ia supernovae. Based upon the hypothesis that the effective flame speed is determined by the unresolved turbulent velocity fluctuations, we employ a new subgrid scale model which includes a localised treatment of the energy transfer through the turbulence cascade in combination with semi-statistical closures for the dissipation and non-local transport of turbulence energy. In addition, subgrid scale buoyancy effects are included. In the limit of negligible energy transfer and transport, the dynamical model reduces to the Sharp-Wheeler relation. According to our findings, the Sharp-Wheeler relation is insuffcient to account for the complicated turbulent dynamics of flames in thermonuclear supernovae. The application of a co-moving grid technique enables us to achieve very high spatial resolution in the burning region. Turbulence is produced mostly at the flame surface and in the interior ash regions. Consequently, there is a pronounced anisotropy in the vicinity of the flame fronts. The localised subgrid scale model predicts significantly enhanced energy generation and less unburnt carbon and oxygen at low velocities compared to earlier simulations.

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

2006-01-23T23:59:59.000Z

185

Early and late time VLT spectroscopy of SN 2001el - progenitor constraints for a type Ia supernova  

E-Print Network (OSTI)

We present early time high-resolution (VLT/UVES) and late time low-resolution (VLT/FORS) optical spectra of the normal type Ia supernova, SN 2001el. The high-resolution spectra were obtained 9 and 2 days before (B-band) maximum light in order to detect narrow hydrogen and/or helium emission lines from the SN CSM. No such lines were detected in our data. We therefore use photoionisation models to derive upper limits of 1x10^-5 and 6x10^-5 Msol/yr, assuming wind velocities of 10 and 50 km/s, respectively, for the mass loss rate from the progenitor system of SN 2001el. This excludes a symbiotic star in the upper mass loss rate regime from being the progenitor of SN 2001el. The low-resolution spectrum was obtained in the nebular phase of the supernova, \\~400 days after the maximum light, to search for any hydrogen rich gas originating from the SN progenitor system. However, we see no signs of Balmer lines in our spectrum. Therefore, we model the late time spectra to derive an upper limit of ~0.03 Msol for solar a...

Mattila, S; Sollerman, J; Kozma, C; Baron, E; Fransson, C; Leibundgut, B; Nomoto, K

2005-01-01T23:59:59.000Z

186

Mason County, Kentucky: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

8897057° 8897057° 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":38.6194103,"lon":-83.8897057,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

187

Mason, New Hampshire: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

436984°, -71.768963° 436984°, -71.768963° 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":42.7436984,"lon":-71.768963,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

188

Mason County, West Virginia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

°, -81.9971108° °, -81.9971108° 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":38.7553693,"lon":-81.9971108,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

189

Mason City, Nebraska: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

City, Nebraska: Energy Resources City, Nebraska: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.222477°, -99.297977° 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":41.222477,"lon":-99.297977,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

190

Mason County, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

3°, -89.9253233° 3°, -89.9253233° 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":40.2271003,"lon":-89.9253233,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

191

Mason County, Washington: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

6°, -123.1951376° 6°, -123.1951376° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":47.4251146,"lon":-123.1951376,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

192

Mason County, Michigan: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

6.4996546° 6.4996546° 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":43.9664537,"lon":-86.4996546,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

193

Medieval Islamic and Gothic architectural drawings : masons, craftsmen and architects  

E-Print Network (OSTI)

As medieval designers and craftsmen have left us with no textual evidence of their thinking processes, their drawings offer valuable sources through which their approach to design and construction can be investigated. ...

Etemad Yousefi, Arash

2005-01-01T23:59:59.000Z

194

Statement of Thomas E. Mason Director, Oak Ridge National Laboratory  

E-Print Network (OSTI)

, and national security benefits. The main cost lies in the intellectual content and high-end manufacturing, both of which are hallmarks of American industrial strength, so in addition to providing an attractive solution creates opportunities for U.S. industry to manufacture the high-technology components that make up roughly

195

Mason County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

°, -99.2785583° °, -99.2785583° 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":30.6556091,"lon":-99.2785583,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

196

Role of GPS in Smart Grid George Mason University  

E-Print Network (OSTI)

A White Book on Smart Grid Faculty of Information Technology, Mathematics and Electrical............................................................................................................................4 2. Definition of Smart Grid........................................................................................................5 3. Smart Grid Structure

197

EVOLUTION OF POST-IMPACT COMPANION STARS IN SN Ia REMNANTS WITHIN THE SINGLE-DEGENERATE SCENARIO  

Science Conference Proceedings (OSTI)

The nature of the progenitor systems of Type Ia supernovae is still uncertain. One way to distinguish between the single-degenerate scenario and double-degenerate scenario is to search for the post-impact remnant star. To examine the characteristics of the post-impact remnant star, we have carried out three-dimensional hydrodynamic simulations of supernova impacts on main-sequence-like stars. We explore the evolution of the post-impact remnants using the stellar evolution code MESA. We find that the luminosity and radius of the remnant star dramatically increase just after the impact. After the explosion, post-impact companions continue to expand on a progenitor-dependent timescale of {approx}10{sup 2.5}-10{sup 3} years before contracting. It is found that the time evolution of the remnant star is dependent not only on the amount of energy absorbed but also on the depth of the energy deposition. We examine the viability of the candidate star Tycho G as the possible remnant companion in Tycho's supernova by comparing it to the evolved post-impact remnant stars in our simulations. The closest model in our simulations has a similar effective temperature, but the luminosity and radius are twice as large. By examining the angular momentum distribution in our simulations, we find that the surface rotational speed could drop to {approx}10 km s{sup -1} if the specific angular momentum is conserved during the post-impact evolution, implying that Tycho G cannot be completely ruled out because of its low surface rotation speed.

Pan, Kuo-Chuan; Ricker, Paul M. [Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States); Taam, Ronald E., E-mail: kpan2@illinois.edu, E-mail: pmricker@illinois.edu, E-mail: taam@northwestern.edu [Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 (United States)

2012-11-20T23:59:59.000Z

198

Gorchakova-IA  

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

(3D) Radiation Codes (Cahalan 2000). In the present work, the broadband fluxes of solar radiation are calculated using two different approaches. The purpose is * to compare...

199

Neutron Diffraction Residual Strain Tensor Measurements Within The Phase IA Weld Mock-up Plate P-5  

SciTech Connect

Oak Ridge National Laboratory (ORNL) has worked with NRC and EPRI to apply neutron and X-ray diffraction methods to characterize the residual stresses in a number of dissimilar metal weld mockups and samples. The design of the Phase IA specimens aimed to enable stress measurements by several methods and computational modeling of the weld residual stresses. The partial groove in the 304L stainless steel plate was filled with weld beads of Alloy 82. A summary of the weld conditions for each plate is provided in Table 1. The plates were constrained along the long edges during and after welding by bolts with spring-loaded washers attached to the 1-inch thick Al backing plate. The purpose was to avoid stress relief due to bending of the welded stainless steel plate. The neutron diffraction method was one of the methods selected by EPRI for non-destructive through thickness strain and stress measurement. Four different plates (P-3 to P-6) were studied by neutron diffraction strain mapping, representing four different welding conditions. Through thickness neutron diffraction strain mappings at NRSF2 for the four plates and associated strain-free d-zero specimens involved measurement along seven lines across the weld and at six to seven depths. The mountings of each plate for neutron diffraction measurements were such that the diffraction vector was parallel to each of the three primary orthogonal directions of the plate: two in-plane directions, longitudinal and transverse, and the direction normal to the plate (shown in left figure within Table 1). From the three orthogonal strains for each location, the residual stresses along the three plate directions were calculated. The principal axes of the strain and stress tensors, however, need not necessarily align with the plate coordinate system. To explore this, plate P-5 was selected for examination of the possibility that the principal axes of strain are not along the sample coordinate system axes. If adequate data could be collected the goal would be to determine the strain tensor's orientation and magnitude of strain along each principle axis direction.

Hubbard, Camden R [ORNL

2011-09-01T23:59:59.000Z

200

Early and late time VLT spectroscopy of SN 2001el - progenitor constraints for a type Ia supernova  

E-Print Network (OSTI)

We present early time high-resolution (VLT/UVES) and late time low-resolution (VLT/FORS) optical spectra of the normal type Ia supernova, SN 2001el. The high-resolution spectra were obtained at -9 and -2 days to allow the detection of narrow hydrogen and/or helium emission lines from the circumstellar medium of the SN. No such lines were detected, and we therefore use photoionisation models to derive upper limits of 9x10^-6 Msun/yr and 5x10^-5 Msun/yr for the mass loss rate from the progenitor system assuming velocities of 10 km/s and 50 km/s, respectively, for a wind extending to outside at least a few x 10^15 cm away from the SN explosion site. These limits exclude a symbiotic star in the upper mass loss rate regime from being the progenitor of SN 2001el. The low resolution spectrum was obtained in the nebular phase of the SN, 400 days after the maximum light, to search for any hydrogen rich gas originating from the SN progenitor system. However, we see no signs of Balmer lines in our spectrum. Therefore, we model the late time spectra to derive an upper limit of ~0.03 Msun for solar abundance material present at velocities lower than 1000 km/s within the SN explosion site. According to simulations of Marietta et al. (2000) this is less than the expected mass lost by a subgiant, red giant or main sequence secondary star at a small binary separation as a result of the SN explosion. Finally, we discuss the origin of high velocity Ca II lines. We see both the CaII IR triplet and the H&K lines in the -9 days spectrum at a very high velocity of up to 34000 km/s. The spectrum also shows a flat-bottomed Si II `6150 A' feature similar to the one previously observed in SN 1990N at -14 days. We compare these spectral features to those observed in SNe 1984A and 1990N at even higher velocities.

S. Mattila; P. Lundqvist; J. Sollerman; C. Kozma; E. Baron; C. Fransson; B. Leibundgut; K. Nomoto

2005-01-20T23:59:59.000Z

Note: This page contains sample records for the topic "mason ia midamerican" 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

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 rate, $r_V \\propto (1+z)^{\\beta}$, we obtain a value of $\\beta = 1.5 \\pm 0.6$, i.e. the SN Ia rate is determined to be an increasing function of redshift at the $\\sim 2.5 \\sigma$ level. Fitting the results to a model in which the volumetric SN rate, $r_V=A\\rho(t)+B\\dot \\rho(t)$, where $\\rho(t)$ is the stellar mass density and $\\dot \\rho(t)$ is the star formation rate, we find $A = (2.8 \\pm 1.2) \\times 10^{-14} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1} \\mathrm{year}^{-1}$, $B = (9.3^{+3.4}_{-3.1})\\times 10^{-4} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1}$.

Benjamin Dilday; R. Kessler; J. A. Frieman; J. Holtzman; J. Marriner; G. Miknaitis; R. C. Nichol; R. Romani; M. Sako; B. Bassett; A. Becker; D. Cinabro; F. DeJongh; D. L. Depoy; M. Doi; P. M. Garnavich; C. J. Hogan; S. Jha; K. Konishi; H. Lampeitl; J. L. Marshall; D. McGinnis; J. L. Prieto; A. G. Riess; M. W. Richmond; D. P. Schneider; M. Smith; N. Takanashi; K. Tokita; K. van der Heyden; N. Yasuda; C. Zheng; J. Barentine; H. Brewington; C. Choi; A. Crotts; J. Dembicky; M. Harvanek; M. Im; W. Ketzeback; S. J. Kleinman; J. Krzesi?ski; D. C. Long; E. Malanushenko; V. Malanushenko; R. J. McMillan; A. Nitta; K. Pan; G. Saurage; S. A. Snedden; S. Watters; J. C. Wheeler; D. York

2008-01-22T23:59:59.000Z

202

Victory Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Farm Wind Farm Facility Victory Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Invenergy Energy Purchaser MidAmerican Energy Location Carroll and Crawford Counties IA Coordinates 42.144715°, -95.138183° 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":42.144715,"lon":-95.138183,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

203

Laurel | Open Energy Information  

Open Energy Info (EERE)

Laurel Laurel Jump to: navigation, search Name Laurel Facility Laurel Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer RPM Access Wind Development Energy Purchaser MidAmerican Energy Location Haverhill IA Coordinates 41.89096884°, -92.97214508° 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":41.89096884,"lon":-92.97214508,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

204

Pomeroy II (08) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Pomeroy II (08) Wind Farm Pomeroy II (08) Wind Farm Facility Pomeroy II (08) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Pocahontas County IA Coordinates 42.570484°, -94.702506° 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":42.570484,"lon":-94.702506,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

205

Pomeroy Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Pomeroy Wind Farm Pomeroy Wind Farm Jump to: navigation, search Name Pomeroy Wind Farm Facility Pomeroy Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Pocahontas County IA Coordinates 42.570484°, -94.702506° 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":42.570484,"lon":-94.702506,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

206

Eclipse | Open Energy Information  

Open Energy Info (EERE)

Eclipse Eclipse Jump to: navigation, search Name Eclipse Facility Eclipse Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Clipper Windpower Development Company Energy Purchaser MidAmerican Energy Location Adair IA Coordinates 41.53604897°, -94.65567112° 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":41.53604897,"lon":-94.65567112,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

207

Vienna | Open Energy Information  

Open Energy Info (EERE)

Vienna Vienna Jump to: navigation, search Name Vienna Facility Vienna Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer RPM Access Wind Development Energy Purchaser MidAmerican Energy Location Marshalltown IA Coordinates 42.159909°, -92.779639° 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":42.159909,"lon":-92.779639,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

208

Pomeroy II (4Q07) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Pomeroy II (4Q07) Wind Farm Pomeroy II (4Q07) Wind Farm Facility Pomeroy II (4Q07) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Pocahontas County IA Coordinates 42.570484°, -94.702506° 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":42.570484,"lon":-94.702506,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

209

Century Wind Project Expansion | Open Energy Information  

Open Energy Info (EERE)

Project Expansion Project Expansion Jump to: navigation, search Name Century Wind Project Expansion Facility Century Wind Project Expansion Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Wright and Hamilton Counties IA Coordinates 42.509141°, -93.682151° 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":42.509141,"lon":-93.682151,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

210

Century Wind Project | Open Energy Information  

Open Energy Info (EERE)

Project Project Jump to: navigation, search Name Century Wind Project Facility Century Wind Project Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Wright and Hamilton Counties IA Coordinates 42.504259°, -93.646524° 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":42.504259,"lon":-93.646524,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

211

Intrepid Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Farm Wind Farm Jump to: navigation, search Name Intrepid Wind Farm Facility Intrepid Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Clipper Windpower Energy Purchaser MidAmerican Energy Location Buena Vista Sac Counties IA Coordinates 42.537923°, -95.289502° 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":42.537923,"lon":-95.289502,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

212

Morning Light | Open Energy Information  

Open Energy Info (EERE)

Morning Light Morning Light Jump to: navigation, search Name Morning Light Facility Morning Light Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Clipper Windpower Development Company Energy Purchaser MidAmerican Energy Location Casey IA Coordinates 41.44819506°, -94.58280087° 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":41.44819506,"lon":-94.58280087,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

213

RELATIVISTIC SHOCK BREAKOUTS-A VARIETY OF GAMMA-RAY FLARES: FROM LOW-LUMINOSITY GAMMA-RAY BURSTS TO TYPE Ia SUPERNOVAE  

SciTech Connect

The light from a shock breakout of stellar explosions, which carries a wealth of information, strongly depends on the shock velocity at the time of the breakout. The emission from Newtonian breakouts, typical in regular core-collapse supernovae (SNe), has been explored extensively. However, a large variety of explosions result in mildly or ultrarelativistic breakouts, where the observed signature is unknown. Here we calculate the luminosity and spectrum produced by relativistic breakouts. In order to do so, we improve the analytic description of relativistic radiation-mediated shocks and follow the system from the breakout itself, through the planar phase and into the spherical phase. We limit our calculation to cases where the post-breakout acceleration of the gas ends during the planar phase (i.e., the final gas Lorentz factor {approx}< 30). We find that spherical relativistic breakouts produce a flash of gamma rays with energy, E{sub bo}, temperature, T{sub bo}, and duration, t{sup obs} b{sub o}, that provide the breakout radius ( Almost-Equal-To 5 R{sub Sun }(t{sup obs}{sub bo}/10 s)(T{sub bo}/50 keV){sup 2}) and the Lorentz factor ( Almost-Equal-To T{sub bo}/50 keV). They also always satisfy a relativistic breakout relation (t{sup obs}{sub bo}/20 s) {approx} (E{sub bo}/10{sup 46} erg){sup 1/2}(T{sub bo}/50 keV){sup -2.68}. The breakout flare is typically followed, on longer timescales, by X-rays that carry a comparable energy. We apply our model to a variety of explosions, including Type Ia and .Ia SNe, accretion-induced collapse, energetic SNe, and gamma-ray bursts (GRBs). We find that all these events produce detectable gamma-ray signals, some of which may have already been seen. Some particular examples are: (1) relativistic shock breakouts provide a natural explanation to the energy, temperature, and timescales of low-luminosity GRBs. Indeed, all observed low-luminosity GRBs satisfy the relativistic breakout relation. (2) Nearby broad-line Type Ib/c (like SN 2002ap) may produce a detectable {gamma}-ray signal. (3) Galactic Type Ia SNe may produce detectable {gamma}-ray flares. We conclude that relativistic shock breakouts provide a generic process for the production of gamma-ray flares.

Nakar, Ehud [Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978 (Israel); Sari, Re'em [Racah Institute for Physics, Hebrew University, Jerusalem 91904 (Israel)

2012-03-10T23:59:59.000Z

214

Solar Wind: Manifestations of Solar Activity E N CYC LO PE D IA O F AS T R O N O MY AN D AS T R O PHYS I C S Solar Wind: Manifestations of Solar  

E-Print Network (OSTI)

Solar Wind: Manifestations of Solar Activity E N CYC LO PE D IA O F AS T R O N O MY AN D AS T R O PHYS I C S Solar Wind: Manifestations of Solar Activity The Sun's outer atmosphere, the corona, is continually heated and expands to create the solar wind. Solar activity waxes and wanes with the 11 yr cycle

Webb, David F.

215

Century Expansion (08) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Century Expansion (08) Wind Farm Century Expansion (08) Wind Farm Jump to: navigation, search Name Century Expansion (08) Wind Farm Facility Century Expansion (08) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location IA Coordinates 42.504142°, -93.656316° 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":42.504142,"lon":-93.656316,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

216

Charles City (1Q08) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Charles City (1Q08) Wind Farm Charles City (1Q08) Wind Farm Facility Charles City (1Q08) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Charles City IA Coordinates 43.049152°, -92.734151° 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":43.049152,"lon":-92.734151,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

217

Intrepid Expansion Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Intrepid Expansion Wind Farm Intrepid Expansion Wind Farm Jump to: navigation, search Name Intrepid Expansion Wind Farm Facility Intrepid Expansion Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser MidAmerican Energy Location Buena Vista & Sac Counties IA Coordinates 42.483311°, -95.308807° 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":42.483311,"lon":-95.308807,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

218

Multi-Megawatt Organic Rankine Engine power plant (MORE). Phase IA final report: system design of MORE power plant for industrial energy conservation emphasizing the cement industry  

SciTech Connect

The Multi-Megawatt Organic Rankine Engine (MORE) program is directed towards the development of a large, organic Rankine power plant for energy conservation from moderate temperature industrial heat streams. Organic Rankine power plants are ideally suited for use with heat sources in the temperature range below 1100/sup 0/F. Cement manufacture was selected as the prototype industry for the MORE system because of the range of parameters which can be tested in a cement application. This includes process exit temperatures of 650/sup 0/F to 1110/sup 0/F for suspension preheater and long dry kilns, severe dust loading, multi-megawatt power generation potential, and boiler exhaust gas acid dew point variations. The work performed during the Phase IA System Design contract period is described. The System Design task defines the complete MORE system and its installation to the level necessary to obtain detailed performance maps, equipment specifications, planning of supporting experiments, and credible construction and hardware cost estimates. The MORE power plant design is based upon installation in the Black Mountain Quarry Cement Plant near Victorville, California.

Bair, E.K.; Breindel, B.; Collamore, F.N.; Hodgson, J.N.; Olson, G.K.

1980-01-31T23:59:59.000Z

219

THE POST-MERGER MAGNETIZED EVOLUTION OF WHITE DWARF BINARIES: THE DOUBLE-DEGENERATE CHANNEL OF SUB-CHANDRASEKHAR TYPE Ia SUPERNOVAE AND THE FORMATION OF MAGNETIZED WHITE DWARFS  

SciTech Connect

Type Ia supernovae (SNe Ia) play a crucial role as standardizable cosmological candles, though the nature of their progenitors is a subject of active investigation. Recent observational and theoretical work has pointed to merging white dwarf binaries, referred to as the double-degenerate channel, as the possible progenitor systems for some SNe Ia. Additionally, recent theoretical work suggests that mergers which fail to detonate may produce magnetized, rapidly rotating white dwarfs. In this paper, we present the first multidimensional simulations of the post-merger evolution of white dwarf binaries to include the effect of the magnetic field. In these systems, the two white dwarfs complete a final merger on a dynamical timescale, and are tidally disrupted, producing a rapidly rotating white dwarf merger surrounded by a hot corona and a thick, differentially rotating disk. The disk is strongly susceptible to the magnetorotational instability (MRI), and we demonstrate that this leads to the rapid growth of an initially dynamically weak magnetic field in the disk, the spin-down of the white dwarf merger, and to the subsequent central ignition of the white dwarf merger. Additionally, these magnetized models exhibit new features not present in prior hydrodynamic studies of white dwarf mergers, including the development of MRI turbulence in the hot disk, magnetized outflows carrying a significant fraction of the disk mass, and the magnetization of the white dwarf merger to field strengths {approx}2 Multiplication-Sign 10{sup 8} G. We discuss the impact of our findings on the origins, circumstellar media, and observed properties of SNe Ia and magnetized white dwarfs.

Ji Suoqing; Fisher, Robert T. [University of Massachusetts Dartmouth, Department of Physics, 285 Old Westport Road, North Dartmouth, MA 02740 (United States); Garcia-Berro, Enrique [Departament de Fisica Aplicada, Universitat Politecnica de Catalunya, c/Esteve Terrades, 5, E-08860 Castelldefels (Spain); Tzeferacos, Petros; Jordan, George; Lee, Dongwook [Center for Astrophysical Thermonuclear Flashes, The University of Chicago, Chicago, IL 60637 (United States); Loren-Aguilar, Pablo [School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL (United Kingdom); Cremer, Pascal [Bethe Center for Theoretical Physics, Universitaet Bonn, Nussallee 12, D-53115 Bonn (Germany); Behrends, Jan [Fachbereich Physik, Freie Universitaet Berlin, Arnimallee 14, D-14195 Berlin (Germany)

2013-08-20T23:59:59.000Z

220

Mason Faculty/ Staff Book Scholarship Application George Mason University, in a nationwide competition, submitted the most ideas in TIAA-CREF's Raise  

E-Print Network (OSTI)

, in a nationwide competition, submitted the most ideas in TIAA-CREF's Raise the Rate contest and received a $25

Note: This page contains sample records for the topic "mason ia midamerican" 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

IA_50m_Wind  

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

ISDataTechnologySpecificUnitedStatesWindHighResolutionIowaWindHighResolution.zip> Description: Abstract: Annual average wind resource potential for the state of Iowa at...

222

Consolidative Involved-Node Proton Therapy for Stage IA-IIIB Mediastinal Hodgkin Lymphoma: Preliminary Dosimetric Outcomes From a Phase II Study  

SciTech Connect

Purpose: To compare the dose reduction to organs at risk (OARs) with proton therapy (PT) versus three-dimensional conformal radiotherapy (3D-CRT) and intensity-modulated radiotherapy (IMRT) in patients with mediastinal Hodgkin lymphoma (HL) enrolled on a Phase II study of involved-node radiotherapy (INRT). Methods and Materials: Between June 2009 and October 2010, 10 patients were enrolled on a University of Florida institutional review board-approved protocol for de novo 'classical' Stage IA-IIIB HL with mediastinal (bulky or nonbulky) involvement after chemotherapy. INRT was planned per European Organization for Research and Treatment of Cancer guidelines. Three separate optimized plans were developed for each patient: 3D-CRT, IMRT, and PT. The primary end point was a 50% reduction in the body V4 with PT compared with 3D-CRT or IMRT. Results: The median relative reduction with PT in the primary end point, body V4, was 51% compared with 3D-CRT (p = 0.0098) and 59% compared with IMRT (p = 0.0020), thus all patients were offered treatment with PT. PT provided the lowest mean dose to the heart, lungs, and breasts for all 10 patients compared with either 3D-CRT or IMRT. The median difference in the OAR mean dose reduction with PT compared with 3D-CRT were 10.4 Gy/CGE for heart; 5.5 Gy/CGE for lung; 0.9 Gy/CGE for breast; 8.3 Gy/CGE for esophagus; and 4.1 Gy/CGE for thyroid. The median differences for mean OAR dose reduction for PT compared with IMRT were 4.3 Gy/CGE for heart, 3.1 Gy/CGE for lung, 1.4 Gy/CGE for breast, 2.8 Gy/CGE for esophagus, and 2.7 Gy/CGE for thyroid. Conclusions: All 10 patients benefitted from dose reductions to OARs with PT compared with either 3D-CRT or IMRT. It is anticipated that these reductions in dose to OAR will translate into lower rates of late complications, but long-term follow-up on this Phase II INRT study is needed.

Hoppe, Bradford S., E-mail: bhoppe@floridaproton.org [University of Florida Proton Therapy Institute, Jacksonville, FL (United States); Flampouri, Stella; Su Zhong; Morris, Christopher G. [University of Florida Proton Therapy Institute, Jacksonville, FL (United States); Latif, Naeem [University of Florida Hematology/Oncology, Jacksonville, FL (United States); Dang, Nam H.; Lynch, James [University of Florida Hematology/Oncology, Gainesville, FL (United States); Li Zuofeng; Mendenhall, Nancy P. [University of Florida Proton Therapy Institute, Jacksonville, FL (United States)

2012-05-01T23:59:59.000Z

223

State Fair Wind Energy Education Center Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Energy Education Center Wind Farm Wind Energy Education Center Wind Farm Jump to: navigation, search Name State Fair Wind Energy Education Center Wind Farm Facility Wind Energy Education Center Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer MidAmerican Energy Energy Purchaser Iowa State Fair Location IA State Fairgrounds IA Coordinates 41.595052°, -93.548779° 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":41.595052,"lon":-93.548779,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

224

"Report Date","U.S.",,,"PADD I",,,"PADD IA",,,"PADD IB",,,"PADD IC",,,"PADD II"  

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

Residential Heating Oil Prices (Before and After Change in Aggregation Methodology)" Residential Heating Oil Prices (Before and After Change in Aggregation Methodology)" "Report Date","U.S.",,,"PADD I",,,"PADD IA",,,"PADD IB",,,"PADD IC",,,"PADD II" ,"Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference"

225

Propagation of Innovations in Networked Groups Winter A. Mason (wimason@indiana.edu)  

E-Print Network (OSTI)

of information transmission (Nowak, Szamrej, & Latané, 1990; Axelrod, 1997; Kennedy, Eberhart, & Shi, 2001-409. Nowak, A., Szamrej, J., & Latané, B. (1990). From private attitude to public opinion: A dynamic theory

Goldstone, Robert

226

Microsoft PowerPoint - 1-07 Mason DOE EM Waste Processing Technology...  

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

plants: Studsvik Processing Facility: Ion exchange resins (45" diameter FBSR) DOE Idaho Integrated Waste Treatment Unit: SBW treatment (48" diameter FBSR) DOE...

227

PLEASE SCROLL DOWN FOR ARTICLE This article was downloaded by: [George Mason University  

E-Print Network (OSTI)

Assemblages, NUREG/CR-6708, U. S. Nuclear Regulatory Commission, Washington, D.C., 214 pp. Davis, J.A., Hess, Colorado, Report NUREG CR-6820, U. S. Nuclear Regulatory Commission, Rockville, MD, 223 pp. Fuller, C. C Facilities, Report NUREG CR-6870, U. S. Nuclear Regulatory Commission, Rockville, MD, 111 pp. T. E. Payne, J

Parasuraman, Raja

228

Thomas Mason Oak Ridge National Lab July 10 2012 SB Summit  

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

by UT-Battelle for the U.S. Department of Energy RegionalSummit1207 Computational science and engineering Materials science and engineering Neutron science and technology...

229

Walnut Wind Project Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Walnut Wind Project Wind Farm Walnut Wind Project Wind Farm Jump to: navigation, search Name Walnut Wind Project Wind Farm Facility Walnut Wind Project Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer EnXco Energy Purchaser MidAmerican Energy Location Pottawattamie County IA Coordinates 41.484094°, -95.185339° 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":41.484094,"lon":-95.185339,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

230

2008 WIND TECHNOLOGIES MARKET REPORT  

E-Print Network (OSTI)

MidAmerican Energy Public Service New Mexico LuminantNew Mexico MSR Public Power Agency Reliant Energy Minnkota

Bolinger, Mark

2010-01-01T23:59:59.000Z

231

Data:C786e656-9210-43d5-8029-7a4ba672dfae | Open Energy Information  

Open Energy Info (EERE)

56-9210-43d5-8029-7a4ba672dfae 56-9210-43d5-8029-7a4ba672dfae No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Separately Metered Electric Space Heating Price Schedule GSN Sector: Commercial Description: Available In the Company's Iowa electric service area (North System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh):

232

Data:499e824e-7f63-4baa-96c1-6b8411553a06 | Open Energy Information  

Open Energy Info (EERE)

e-7f63-4baa-96c1-6b8411553a06 e-7f63-4baa-96c1-6b8411553a06 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Base - Energy Only Metering - Price Schedule GBN Sector: Commercial Description: Available In the Company's Iowa electric service area (North System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh):

233

Data:C397a4c8-9425-4984-98d3-49da244a4e1e | Open Energy Information  

Open Energy Info (EERE)

c8-9425-4984-98d3-49da244a4e1e c8-9425-4984-98d3-49da244a4e1e No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Separately Metered Electric Water Heating Price Schedule GWN Sector: Commercial Description: Available In the Company's Iowa electric service area (North System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh):

234

Data:50da35ec-f510-4633-8c08-d9b7075e274f | Open Energy Information  

Open Energy Info (EERE)

ec-f510-4633-8c08-d9b7075e274f ec-f510-4633-8c08-d9b7075e274f No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Electric Heat - Energy Only Metering Price Schedule GES Sector: Commercial Description: Available In the Company's Iowa electric service area (South System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh):

235

Data:35c710b0-2043-4cc1-84be-7a25c3fd666b | Open Energy Information  

Open Energy Info (EERE)

0b0-2043-4cc1-84be-7a25c3fd666b 0b0-2043-4cc1-84be-7a25c3fd666b No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Base - Energy Only Metering - Price Schedule GBS Sector: Commercial Description: Available In the Company's Iowa electric service area (South System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh):

236

Adair Wind Farm I | Open Energy Information  

Open Energy Info (EERE)

I I Jump to: navigation, search Name Adair Wind Farm I Facility Adair Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Shafer Systems Developer MidAmerican Energy Energy Purchaser Alliant/IES Utilities Location IA Coordinates 41.499234°, -94.692628° 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":41.499234,"lon":-94.692628,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

237

Rates and progenitors of type Ia supernovae  

E-Print Network (OSTI)

Propulsion Laboratory, operated under contract NAS7-030001 with the National Aeronautics and SpacePropulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

Wood-Vasey, William Michael

2004-01-01T23:59:59.000Z

238

Visualizing Type Ia Supernova Explosions at NERSC  

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

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,...

239

Distributed Flames in Type Ia Supernovae  

E-Print Network (OSTI)

In the distributed burning 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 depends on the turbulent Damkohler number (Da), which steadily declines from much greater than one to less that one as the density decreases to a few 10^6 g/cc. Scaling arguments predict that the turbulent flame speed s, normalized by the turbulent intensity u, follows s/u=Da^1/2 for Da1, and that localized excursions to as much as five times u can occur. The lambda-flame speed and width can be predicted based on the turbulence in the star and the turbulent nuclear burning time scale of the fuel. We propose a practical method for measuring these 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 supernovae flames.

Aspden, A J; Woosley, S E; 10.1088/0004-637X/710/2/1654

2011-01-01T23:59:59.000Z

240

Variable CcainAdaptiveControlSystemfor Turning Oren Mason/, TexasA&M University, CollegeStation, Texas  

E-Print Network (OSTI)

. 6, pp. 856­862, June 1995. [30] A. Tonazzini, L. Bedini, and E. Salerno, "A Markov model for blind

Michigan, University of

Note: This page contains sample records for the topic "mason ia midamerican" 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

Collective Search in Concrete and Abstract Robert L. Goldstone, Michael E. Roberts, Winter Mason, and Todd Gureckis  

E-Print Network (OSTI)

0022-3514/11/$12.00 DOI: 10.1037/a0022982 967 #12;& Eberhart, 2001; Nowak, Szamrej, & Latane´, 1990

Goldstone, Robert

242

Mason and Enterprise Development under the Biogas Program in Vietnam: An Impact Study of the Effects of the Biogas Program.  

E-Print Network (OSTI)

??The research proposed to analyze the impact of a renewable energy project entitled The Biogas Project Program for the department of Animal Husbandry and livestock (more)

Schaart, I.G.

2010-01-01T23:59:59.000Z

243

High-resolution stratigraphic and structural characterization of the fault-partitioned Hickory Sandstone aquifer system, Mason County, central Texas  

E-Print Network (OSTI)

The Hickory Sandstone is an important aquifer in central Texas and is partitioned by faults that impede cross-fault fluid flow. This study provides a detailed stratigraphic and structural model in the vicinity of a normal, oblique-slip fault with 60' (18.3 m) of stratigraphic throw. The model is developed using 3500' (1050 m) of continuous core and geophysical logs from eleven closely spaced boreholes. The local stratigraphy is studied in detail and environments of deposition inferred. A model of fault evolution is inferred using the observed fault structure and throw distributions. Locally, the Hickory Sandstone consists of 450' (137 m) of Cambrian-aged, quartzose and arkosic sandstone with localized mudstone and siltstone interbeds and overlies Precambrian Town Mountain Granite. Within the study area, the Hickory Sandstone is subdivided into four facies: the cross-bedded facies, the mudstone facies, the interbedded sandstone facies and the hematite facies. These facies form a stacked sequence representing an initial braided-stream fluvial environment that grades into a high energy, open marine environment that closely matches the tide-dominated, high microtidal estuarine model of Reinson (1992). Lateral correlation of strata packages in the cross-bedded facies was very difficult and complicated development of the fault model. The study fault is a linked fault system consisting of several major segments. Two segments overlap and locally hard link along both strike and dip. The major fault segments also consist of several linked subsegments. Net stratigraphic throw decreases slightly upward from a maximum of 60' (18.3 m) near the granite basement. Where the major segments overlap, the throw exhibits systematic variations consistent with displacement transfer between the neighboring segments. The linked fault system is inferred to have formed by interaction and linkage of two, early, en echelon basement faults. Ultimately these faults propagated upward and laterally into the overlying Hickory Sandstone, interacted and partially hard-linked, producing a large linkage structure that affected subsequent, neighboring hanging wall deformation. Subsidiary small faults are common but do not exhibit simple spatial relations with the large fault segments. There is only a weak correlation between a fault's shear zone thickness and stratigraphic throw for faults with 1' to 60' (0.3 to 18.3 m) of throw.

Wilson, Jason Steven

2001-01-01T23:59:59.000Z

244

Agreement between the Cement Masons, Local 580 and the City and County of San Francisco, 2001-2003  

E-Print Network (OSTI)

a journey-level worker or an apprentice; and The entrysalary step of the apprentice program shall be at leastnegotiated otherwise, apprentices in the service of the City

Cement Masons, Local 580

2001-01-01T23:59:59.000Z

245

Habitat-Mediated Predator-Prey Interactions in the Eastern Gulf of Primary Investigator: Doran Mason -NOAA /GLERL  

E-Print Network (OSTI)

. Our project simply asks why? Is it a supply-demand issue (e.g., per capita prey availability) mediated) that either decrease consumption rates (i.e., decrease foraging efficiency) or increase metabolic costs consumed; and f) calculation of daily gross energy intake for gag using an appropriate consumption model

246

1 | EqIA Summary| Diversity Team| 08/12/08 EqIA Summary  

E-Print Network (OSTI)

) Summary of Impact There are no direct or significant adverse impacts on Race, Gender, Disability, Sexual, in particular benefits relating to age as there will be a strong focus on bio energy, which will support fuel

247

Retail Unbundling - South Dakota  

U.S. Energy Information Administration (EIA)

Number of Customers (All Sectors) Number of Transportation Customers (All Sectors) MidAmerican Energy Company. 82,236. 213. Montana-Dakota Utilities Company . 52,046 ...

248

Retail Unbundling - South Dakota  

U.S. Energy Information Administration (EIA)

Number of Transportation Customers (All Sectors) MidAmerican Energy Company. 72,731. 141. Montana-Dakota Utilities. 46,346. 39. NorthWestern Public Service.

249

Work Management Improvement at Louisa Generating Station  

Science Conference Proceedings (OSTI)

This report describes results of a Work Management Improvement project at the Louisa Generating Station, MidAmerican Energy Company, Muscatine, Iowa.

2001-11-19T23:59:59.000Z

250

Category:Utility Rate Impacts on PV Economics By Location | Open Energy  

Open Energy Info (EERE)

Utility Rate Impacts on PV Economics By Location Utility Rate Impacts on PV Economics By Location Jump to: navigation, search Impact of Utility Rates on PV Economics Montgomery, AL Little Rock, AR Flagstaff, AZ Phoenix, AZ Tucson, AZ Arcata, CA LA, CA San Francisco, CA Boulder, CO Eagle County, CO Pueblo, CO Bridgeport, CT Wilmington, DE Miami, FL Tampa, FL Atlanta, GA Savannah, GA Des Moines, IA Mason, IA Boise, ID Chicago, IL Springfield, IL Indianapolis, IN Goodland, KS Wichita, KS Lexington, KY New Orleans, LA Shreveport, LA Boston, MA Baltimore, MD Caribou, ME Portland, ME Detroit, MI Houghton-Lake, MI Traverse City, MI International Falls, MN Minneapolis, MN Kansas City, MO Jackson, MS Billings, MT Greensboro, NC Wilmington, NC Bismarck, ND Minot, ND Omaha, NE Concord, NH Atlantic City, NJ Albuquerque, NM Las Vegas, NV Reno, NV New York, NY

251

Part I--A Rational Aerodynamic Design Procedure  

E-Print Network (OSTI)

'The design of a turbine stage is described in which all leading parameters (stage loading, flow coefficient, pitch/chord ratio, blade profile shape and aspect ratio) have been selected conservatively to accord with current ideas for ensuring a reasonably high level of aerodynamic efficiency. From consideration of the influence of stage loading KpAT V~ U,2, flow coefficient ~ and rotor exit swirl angle c ~ 3, the stage design was selected such that these parameters were 1.15, 0.65 and 10 degrees respectively. At the design speed of U ~ = 34 the resulting stage pressure ratio is approximately 1.65. Such a stage duty is 'light ' by aero engine standards but very comparable to much industrial gas turbine design practice. Blade spacing and profile shapes are 'finally selected in such a way as to preclude severe opposing pressure gradients on the suction surface which might result in local separation of the boundary layer from the blade surfaces. The methods applied and described for predicting blade surface velocities are simple and approximate only, and might readily be imitated by designers not wishing or able to exploit more elaborate and complex digital techniques.

M. No; D. J. L. Smith; I. H. Johnston; D. J. L. Smith; D. J. Fullbrook; D. J. L. Smith; I. H. Johnston

1967-01-01T23:59:59.000Z

252

K-corrections and spectral templates of Type Ia supernovae  

E-Print Network (OSTI)

Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

Hsiao, E. Y.

2008-01-01T23:59:59.000Z

253

The complete mitochondrial genome of Articulate Brachiopod Terebratal ia transversa  

SciTech Connect

We have sequenced the complete mitochondrial DNA (mtDNA) of the articulate brachiopod Terebratalia transversa. The circular genome is 14,291 bp in size, relatively small compared to other published metazoan mtDNAs. The 37 genes commonly found in animal mtDNA are present; the size decrease is due to the truncation of several tRNA, rRNA, and protein genes, to some nucleotide overlaps, and to a paucity of non-coding nucleotides. Although the gene arrangement differs radically from those reported for other metazoans, some gene junctions are shared with two other articulate brachiopods, Laqueus rubellus and Terebratulina retusa. All genes in the T. transversa mtDNA, unlike those in most metazoan mtDNAs reported, are encoded by the same strand. The A+T content (59.1 percent) is low for a metazoan mtDNA, and there is a high propensity for homopolymer runs and a strong base-compositional strand bias. The coding strand is quite G+T-rich, a skew that is shared by the confamilial (laqueid) specie s L. rubellus, but opposite to that found in T. retusa, a cancellothyridid. These compositional skews are strongly reflected in the codon usage patterns and the amino acid compositions of the mitochondrial proteins, with markedly different usage observed between T. retusa and the two laqueids. This observation, plus the similarity of the laqueid non-coding regions to the reverse complement of the non-coding region of the cancellothyridid, suggest that an inversion that resulted in a reversal in the direction of first-strand replication has occurred in one of the two lineages. In addition to the presence of one non-coding region in T. transversa that is comparable to those in the other brachiopod mtDNAs, there are two others with the potential to form secondary structures; one or both of these may be involved in the process of transcript cleavage.

Helfenbein, Kevin G.; Brown, Wesley M.; Boore, Jeffrey L.

2001-07-01T23:59:59.000Z

254

IA/Cyber Defense Brief for USAREUR Land EXPO  

Science Conference Proceedings (OSTI)

... Duty, Honor, Country. The Unholy Alliances. Spam Entrepreneurs; Adware / Spyware Providers; File Sharers; Phishers; Porn Purveyors; Hackers. ...

2007-11-15T23:59:59.000Z

255

www.ias.edu/rise Science Initiative Group  

E-Print Network (OSTI)

funds. He has an ally in Heneri Dzinotyiweyi, the Minister for Science and Technology Development as a regional research facility and as the coordinating hub of a regional network. The 60 computer users ­ staff

256

The SN Ia Rate in High-Redshift Galaxy Clusters  

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

Lin, Y.-T. & Mohr, J. J. 2004, ApJ, 617, 879 Livio, M. 2001, in Supernovae and Gamma-Ray Bursts: the Greatest Explosions since the Big Bang, ed. M. Livio, N. Panagia, & K....

257

UMore Ph IA CR Report 7-8-10.pdf  

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

associated with construction of the wind turbine, 34.5 kV interconnect line, meteorologic tower, and associated roads and laydown areas, which encompasses approximately 33.25 acres...

258

Next-Generation Petascale Simulations of Type Ia Supernovae ...  

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

deflagration to detonation transition model Deflagration to detonation transition model. Min lOng, Dan van Rossum, Sean Couch, George Jordan, Brad Gallagher, Don Lamb, University...

259

Closest Type Ia Supernova in Decades Solves a Cosmic Mystery  

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

use to measure cosmic growth, a technique that in 1998 led to the discovery of dark energy - and 13 years later to a Nobel Prize, "for the discovery of the accelerating...

260

UNU-IAS Policy Report Biofuels in Africa  

E-Print Network (OSTI)

. Currently, liquid biofuels (e.g. bioethanol and biodiesel) produced from edible plants or animal fats/power generation (FAO, 2009; IEA, 2004). Currently, liquid biofuels (e.g. bioethanol and biodiesel) are by far) and conversion technology used, biofuels can be distinguished as first- and second-generation biofuels.2 First

Note: This page contains sample records for the topic "mason ia midamerican" 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

Distributed Flames in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

generator trip controller AEC Canada, Ont. Hydro Nuclear reactor controller Argonne Token­based ACS of axioms of the logical theory. Part 2, 32.1.6 In summary, the practical options for Formal Arguments Case Studies: Verification Software Domain SACEM (Paris metro) GEC Alsthom, RATP Darlington nuclear

262

A High-Yield Hydrothermal Preparation of CuAlO2 Dean Y. Shahriari, Antoine Barnabe`,,, Thomas O. Mason, and Kenneth R. Poeppelmeier*,  

E-Print Network (OSTI)

unreacted Ag2O through treatment of the two-phase product with dilute nitric acid. Later, R. D. Shannon et varied based on x in accordance with Scheme 1. For x ) 0, the reaction is simply a dissolution increases from 0 to 1. The balance of the aluminum species was found * Corresponding author. E-mail: krp

Poeppelmeier, Kenneth R.

263

We are very pleased that you have chosen to live at Mason and we hope that you settle in quickly and enjoy your stay.  

E-Print Network (OSTI)

with the Chartered Institute of Building Service Engineers (CIBSE) recommendations. If you have any queries regarding

Birmingham, University of

264

We are very pleased that you have chosen to live at Mason and we hope that you settle in quickly and enjoy your stay.  

E-Print Network (OSTI)

is provided in accordance with the Chartered Institute of Building Service Engineers (CIBSE) recommendations

Birmingham, University of

265

In Proceedings of the Conference "Ontology for the Intelligence Community: Towards Effective Exploitation and Integration of Intelligence Resources," George Mason University, Fairfax, Virginia Campus, 3 -4 December 2008.  

E-Print Network (OSTI)

This Is Espionage Today................................................................ 14 Foreign Intelligence we have. Insiders--Clandestine intelligence gathering is a reality. Also, some workers are willing know that New Mexico is a hot spot for spies? Counterintelligence expert Bruce Held says: "For many

Tecuci, Gheorghe

266

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

Gasoline and Diesel Fuel Update (EIA)

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

267

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

Annual Energy Outlook 2012 (EIA)

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

268

The Large Synoptic Survey Telescope  

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

night sky. Below: The telescope depicted at its future site atop Cerro Pachn in Chile. (Top image by Todd Mason, Mason Productions Inc. LSST Corporation. Bottom image...

269

Sorption studies of subsurface pantex soils.  

E-Print Network (OSTI)

??The Pantex Plant is a Department of Energy facility that is jointly managed by Mason and Hanger-Silas Mason Company, Inc., and Battelle Memorial Institute (BMI). (more)

Givens, Dennis R.

1997-01-01T23:59:59.000Z

270

Data:D48b8f09-d5f3-48b6-998f-cd47d6f26c4e | Open Energy Information  

Open Energy Info (EERE)

f09-d5f3-48b6-998f-cd47d6f26c4e f09-d5f3-48b6-998f-cd47d6f26c4e No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 1999/03/01 End date if known: Rate name: General Service, Base - Demand Metered - Price Schedules GDN and ADN Sector: Industrial Description: Available In the Company's Iowa electric service area (North System only). Demand Charge: Summer: $6.51 per kW, less a discount per kWh of 1.10 cents. Winter: $4.75 per kW, less a discount per kWh of 0.60 cents. Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf

271

Data:E645ef6d-4655-4c9e-965a-2ea2ebfb01a1 | Open Energy Information  

Open Energy Info (EERE)

ef6d-4655-4c9e-965a-2ea2ebfb01a1 ef6d-4655-4c9e-965a-2ea2ebfb01a1 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/03/01 End date if known: Rate name: General Service, Electric Heat - Demand Metered - Price Schedule GHN Sector: Industrial Description: Available In the Company's Iowa electric service area (North System only). Demand Charge: Summer: $6.51 per kW, less a discount per kWh of 1.10 cents. Winter: $3.50 per kW, less a discount per kWh of 0.20 cents. Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf

272

Data:Ddb84f72-e1ac-4a6e-9042-f1c8b15d31d8 | Open Energy Information  

Open Energy Info (EERE)

Ddb84f72-e1ac-4a6e-9042-f1c8b15d31d8 Ddb84f72-e1ac-4a6e-9042-f1c8b15d31d8 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2010/10/01 End date if known: Rate name: General Service, Electric Heat - Energy Only Metering - Price Schedule GEN Sector: Commercial Description: Available In the Company's Iowa electric service area (North System only). Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh):

273

Storm Lake I Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Storm Lake I Wind Farm Storm Lake I Wind Farm Jump to: navigation, search Name Storm Lake I Wind Farm Facility Storm Lake I Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Edison Mission Group Developer GE Energy Energy Purchaser MidAmerican Energy Location Buena Vista and Cherokee Counties IA Coordinates 42.57215°, -95.340693° 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":42.57215,"lon":-95.340693,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

274

Data:55d4472a-592a-4e97-b786-a296b6d4f5df | Open Energy Information  

Open Energy Info (EERE)

592a-4e97-b786-a296b6d4f5df 592a-4e97-b786-a296b6d4f5df No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 1999/03/01 End date if known: Rate name: General Service, Base - Primary Metered - Price Schedules GPN and ARN Sector: Industrial Description: Available In the Company's Iowa electric service area (North System only). Demand Charge: Summer: $6.36 per kW, less a discount per kWh of 1.07 cents. Winter: $4.64 per kW, less a discount per kWh of 0.58 cents. Source or reference: http://www.midamericanenergy.com/include/pdf/rates/elecrates/iaelectric/ia-elec.pdf

275

SANDIA REPORT SAND99-1941  

E-Print Network (OSTI)

-Silas Mason Company at Pantex for providing clarification of the 1945 military regulations governing

Fuerschbach, Phillip

276

Alternative Energy Law (AEL)  

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

Iowa requires its two investor-owned utilities (MidAmerican Energy and Alliant Energy Interstate Power and Light) to own or to contract for a combined total of 105 megawatts (MW) of renewable...

277

Solar | Department of Energy  

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

end of 2005. The city reached this goal in 2008, the city with a purchase of 215 million kWh of wind and biomass energy from MidAmerican Energy. July 12, 2013 City of Chicago -...

278

City of Chicago - Green Power Purchasing | Department of Energy  

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

end of 2005. The city reached this goal in 2008, the city with a purchase of 215 million kWh of wind and biomass energy from MidAmerican Energy. The http:www.chicagoclimateactio...

279

QCL IA 2009-2012 Proposed Research The QCL IA has several major themes around which our individual research projects are organized.  

E-Print Network (OSTI)

)a 1970 2 015 424 ­ Cemet factory expansion (1972­1973)d ; sugar cane mill (1974); PEMEX oil refinery (1978) 1980 2 369 076 Miguel de la Madrid (1988) PEMEX oil refinery expansion (1981, 1983)e ; PEMEX

Texas at Austin, University of

280

STATEMENT OF CONSIDERATIONS CLASS WAIVER OF THE GOVERNMENT'S...  

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

PANTEX PLANT PURSUANT TO THE DEPARTMENT OF ENERGYMASON AND HANGER-SILAS MASON CO., INC., PERFORMANCE-BASED MANAGEMENT CONTRACT NO. DE-AC04-91AL65030 - W(C)95-002 MASON AND...

Note: This page contains sample records for the topic "mason ia midamerican" 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

Automated Combinatorial Testing for Software (ACTS)  

Science Conference Proceedings (OSTI)

... than 170 organizations; Collaborators active collaboration with faculty from five universities (U. Texas, NC State, George Mason, UMBC, Utah State ...

2013-01-15T23:59:59.000Z

282

NIST CNR SANS NG7 30 Meter SANS Instrument  

Science Conference Proceedings (OSTI)

... nanoparticle aggregation in mixtures of incompatible crude oils, TG Mason ... nanoparticle aggregation kinetics in incompatible crude oil mixtures, TG ...

283

SANS Publications - 2003  

Science Conference Proceedings (OSTI)

... nanoparticle aggregation in mixtures of incompatible crude oils, TG Mason ... nanoparticle aggregation kinetics in incompatible crude oil mixtures, TG ...

284

NNSA employees selected for Nuclear Scholars Initiative program...  

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

Biodefense at George Mason University, and specializes in national security technology policy, international security, counterproliferation, and intelligence studies. His research...

285

Text REtrieval Conference (TREC) TREC-4 Proceedings  

Science Conference Proceedings (OSTI)

... of Information Technology), DO Holmes (AT&T Global Information Solutions, O. Frieder (George Mason University), MD Nguyen (Coherent Design ...

286

Agenda_27Jul2010 Agenda for the 2010 NIST Workshop on ...  

Science Conference Proceedings (OSTI)

... storage Julius Ojwang, CIW Yuri Mishin, George Mason U. Mike Baskes, LANL Jincheng Du, U. North Texas Yue Qi, GM ...

2010-08-05T23:59:59.000Z

287

Welcome to the NIST Workshop on Atomistic Simulations for ...  

Science Conference Proceedings (OSTI)

... storage Julius Ojwang, CIW Yuri Mishin, George Mason U. Mike Baskes, LANL Jincheng Du, U. North Texas Yue Qi, GM ...

2010-08-05T23:59:59.000Z

288

Agenda_final_11.06.16 Agenda (final) for the 2011 NIST ...  

Science Conference Proceedings (OSTI)

... system Mike Baskes, LANL Zachary Trautt and Yuri Mishin, George Mason Univ. Scott Oppenheimer, ATI Allvac Overview ...

2011-06-20T23:59:59.000Z

289

Download PDF  

Science Conference Proceedings (OSTI)

Surya Kalidindi (Georgia Institute of Technology). Paul Mason (Thermocalc). Farrokh Mistree (U. of Oklahoma). Greg Olson (QuesTek Innovations/

290

Sensitivity analysis of world oil prices. Analysis report AR/IA/79-47  

SciTech Connect

An analysis of the impact of the political disruption in Iran on the world oil market is presented. During the first quarter of 1979, this disruption caused a loss of approximately 5 million barrels per day (MMBD) of oil production available for export from Iran to the rest of the world. This loss of production and the political climate in Iran have caused much speculation concerning future Iranian oil production and total Organization of Petroleum Exporting Countries (OPEC) oil production in the nearterm and midterm. The analysis describes these issues in terms of two critical factors: the world oil price and the level of OPEC oil production in the nearterm and midterm. A detailed comparison of the Central Intelligence Agency (CIA) and Energy Information Agency (EIA) forecasting models of world oil prices is presented. This comparison consists of examining reasons for differences in the price forecasts of the CIA model by using CIA assumptions within the EIA model. The CIA and EIA model structures and major parameters are also compared. It is important to note that this analysis is not all encompassing. In particular, the analysis does not provide data on crude oil prices in the spot market, but does provide information on the average crude oil price; and does not permit rationing of oil, since the market is forced to clear only through changes in oil prices. Throughout this paper, world oil prices are defined in terms of real 1978 dollars per barrel of crude oil delivered to the East Coast of the United States net of any import fees.

Rodekohr, M.; Cato, D.

1979-09-01T23:59:59.000Z

291

The A2iA Arabic Handwritten Text Recognition System at the ...  

Science Conference Proceedings (OSTI)

... This two- step training schedule greatly helped to reduce convergence times ... This pro- cedure requires the construction of a decoding graph that ...

2013-08-19T23:59:59.000Z

292

Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study  

E-Print Network (OSTI)

Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

Garavini, G.; Supernova Cosmology Project

2008-01-01T23:59:59.000Z

293

Improving Type Ia Supernova Standard Candle Cosmology Measurements Using Observations of Early-Type Host Galaxies  

E-Print Network (OSTI)

Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

Meyers, Joshua Evan

2012-01-01T23:59:59.000Z

294

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg130  

E-Print Network (OSTI)

. Journal of "Solar Energy Materials and Solar Cells". Proceedings of IEEE Photovoltaic Specialist Conferences. Proceedings of European Photovoltaic Solar Energy Conferences. #12;Module 2/Photovoltaics, Wiley, 1995. R.H.Bube, Photovoltaic Materials, Imperial College Press, 1998. Journal of "Solar Energy

295

_ _i_i Association for ,nformation and Image Management i; _ J , IA Spring, Maryland 20310  

E-Print Network (OSTI)

the maximum pressure needed to lift the overburden (``the fracture pressure''), and new CO2 injection wells (MMscf) of natural gas burned to generate elec- tricity (n3045us2a.xls). All these data are posted generation has been calculated from the DOE EIA files epmxlfile4_1.xls (Report DOE/EIA-0226) for coal, and n

Hazen, Terry

296

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 estim...

Gmez-Gomar, J; Jean, P; Gomez-Gomar, Jordi; Isern, Jordi; Jean, Pierre

1997-01-01T23:59:59.000Z

297

OS and compiler considerations in the design of the IA-64 architecture  

Science Conference Proceedings (OSTI)

Increasing demands for processor performance have outstripped the pace of process and frequency improvements, pushing designers to find ways of increasing the amount of work that can be processed in parallel. Traditional RISC architectures use hardware ...

Rumi Zahir; Jonathan Ross; Dale Morris; Drew Hess

2000-12-01T23:59:59.000Z

298

Pacific Northwest National Laboratory: INstItute for INterfacIaL cataLysIs  

E-Print Network (OSTI)

shell (biomass) cellulosa type of reaction flash pyrolysis pyrolysis flash pyrolysis slow pyrolysis. Scott, J. Piskorz, D. Radlein; Liquid Products from the Continuous Flash Pyrolysis of Biomass, Ind. Eng; The Continous Flash Pyrolysis of Biomass, The Canadian Journal of Chemical Engineering, 1984, 62, 404-412 #12

299

Regional Initiative in Science and Education www.ias.edu/rise  

E-Print Network (OSTI)

funds. He has an ally in Heneri Dzinotyiweyi, the Minister for Science and Technology Development as a regional research facility and as the coordinating hub of a regional network. The 60 computer users ­ staff

300

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg102  

E-Print Network (OSTI)

when carbon dioxide is introduced into thermal conversion processes such as the gasification of coal to syngas, leaving behind only a carbonless char. Castaldi estimates that if the biomass were used

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


301

Pacific Northwest National Laboratory: INstItute for INterfacIaL cataLysIs  

E-Print Network (OSTI)

of Chemistry University of Calgary,Alberta, Canada T2N 1N4 New Orleans National Meeting Modeling the Fischer-Tropsch study Fischer-Tropsch synthesis: An Introduction First discovered by Sabatier and Sanderens in 1902: CO + H2 CH4 Ni,Fe,Co Fischer and Tropsch reported in 1923 the synthesis of liquid hydrocarbons with high

302

Targeted Energy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

303

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg 141  

E-Print Network (OSTI)

- onry is also crucial to their safe storage. Plutonium, an active ingredient in nuclear weap- ons, has to determine how the electrons within these materials will behave. "The plutonium in the weapons ages, and we have to be able to predict the proper- ties of plutonium under a variety of conditions," Chris

304

From Convection to Explosion: End-to-End Simulation of Type Ia Supernovae  

E-Print Network (OSTI)

INCITE award at the Oak Ridge Leadership Computational Facility (OLCF) at Oak Ridge National Laboratory

Bell, John B.

305

Teor'ia de Grupos y Mec'anica Qu'antica Luis A. Seco  

E-Print Network (OSTI)

armonicos desacoplados. 7. El ' atomo de hidr'ogeno. 8. El helio y los otros 'atomos. 9. Mol'eculas. 10

Seco, Luis A.

306

INFORMATION EXCELLENTIA CoLumbIA ENgINEErINg238  

E-Print Network (OSTI)

that bends and twists. "Computers, geometry, and physics are my ingredients. I mix them up in a bowl and what science as well. B.A.Sc., University of Toronto (Canada), 1997; M.S., California Institute of TechnologySPUn Associate Professor of Computer Science #12;

Hone, James

307

Targeted Eneregy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

308

REPORT OF THE PRESIDENT,~ -01 OF THE UNIVERSITY OF BRITISH COLm~IA~ -  

E-Print Network (OSTI)

38 R~port of the Instructor in Physical Education for Women 39 g~portof the Office!: Co Second Yearoo.....eoQ....oo........... Third Year.....OOO..OO..O.............Fourth Ye~.O..O.O.OIO; Engineer 134; Farmer 75; Inspector 21; Insurance 34; Lawyer 39; Lumberman 33; Manager 54; Merchant 97

Pulfrey, David L.

309

Just What is a Supernova?  

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

Matter transfer in a binary system Distances to Type Ia Supernovae Slide 8 Supernova "CAT Scan" Type Ia Supernova lightcurves Type Ia Supernovae and Cosmology Type Ia Supernovae...

310

Page not found | Department of Energy  

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

91 - 25200 of 28,904 results. 91 - 25200 of 28,904 results. Rebate MidAmerican Energy (Electric)- Residential Energy Efficiency Rebate Programs MidAmerican Energy offers a variety of incentives for residential customers to improve the energy efficiency of eligible homes. The Residential Equipment Brochure on the program web site above... http://energy.gov/savings/midamerican-energy-electric-residential-energy-efficiency-rebate-programs-0 Rebate National Grid (Gas)- Residential Energy Efficiency Rebate Programs (Upstate New York) National Grid's High Efficiency Heating Rebates are offered to gas heating customers in the Upstate New York counties of Albany, Columbia, Fulton, Herkimer, Jefferson, Madison, Montgomery, Oneida,... http://energy.gov/savings/national-grid-gas-residential-energy-efficiency-rebate-programs-upstate-new-york-0

311

Closed Sessions Program The closed session program plan is given in detail in Appendix I-A. The program started  

E-Print Network (OSTI)

for enhancing renewable energy usage · Assist in education and research in renewable energy · Changing behavior on "Energy for Sustainable Development: Perspectives from the Arab Region", followed by 20-minute presentations by participating Middle East Universities on their country specific energy profiles, with emphasis

312

Automotive Stirling Engine Market and Industrial Readiness Program (MIRP). Final report for Phase IA, September 15, 1982-July 31, 1984  

SciTech Connect

A brief history of the project is presented. Included in appendices are the scope of work, management and cost plans, major milestones, and the digital engine control spare parts' list. (MHR)

Not Available

1984-08-01T23:59:59.000Z

313

Analysis of the Thermal Performance of Tierra I--A Low-Energy High-Mass Residence  

DOE Green Energy (OSTI)

A low-energy concrete house was designed using passive solar strategies to consume 70% less heating and cooling energy than a base case that conformed to the 1996 Home Energy Rating System (HERS) and the 1995 Model Energy Code (MEC). The performance of this house was then evaluated using computer simulations and measured data. The house, Tierra I, was monitored from July 22, 1996, through October 14, 1997. A Short Term Energy Monitoring (STEM) test was done November 19 to December 10, 1996. Computer simulations of the house were done using SUNREL, an updated version of the hourly data simulation package SERI-RES. The SUNREL model of the house was calibrated using both short- and long-term data. The house achieved energy savings of 56%, below the goal of 70%. The lower than expected savings resulted from problems with the window modeling. As a result, during the design phase the solar gains were overestimated causing an underestimate in the level of insulation necessary to achieve the savings goal. For very low-energy passive solar buildings, it is apparent that very accurate window modeling is required. It also became apparent that accurate ground models are required as well because ground-heat loss accounts for a significant portion of the total heat loss in low-energy buildings.

Smith, M. W.

2001-05-31T23:59:59.000Z

314

IA-SDSS: A GIS-based land use decision support system with consideration of carbon sequestration  

Science Conference Proceedings (OSTI)

Land use, land use change and forestry (LULUCF) can play a positive role in mitigating global warming by sequestering carbon from the atmosphere into vegetation and soils. Local entities (e.g. local government, community, stockholders) have been making ... Keywords: Carbon models, Carbon sequestration, GIS, Integrated assessment, Land-use planning, RS, SDSS

Jun Wang; Jingming Chen; Weimin Ju; Manchun Li

2010-04-01T23:59:59.000Z

315

On October 15, 2010, the University of Memphis Center for Information Assurance (CfIA) hosted the 3rd  

E-Print Network (OSTI)

digital devices, and we encourage you to read the excellent summary from the National Counter-Intelligence for an unspecified period of time. This policy applies to anyone entering the country, including US citizens

Memphis, University of

316

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

E-Print Network (OSTI)

A. 1999, ApJ, 525, 583 Balbi, A. , Ade, P. , Bock, J. etJa?e, A.H. , Ade, P.A. , Balbi, A. et al. , 2001, Phys. Rev.

2005-01-01T23:59:59.000Z

317

Ab initio formation energies of FeCr alloys P. Olsson a,*, I.A. Abrikosov b  

E-Print Network (OSTI)

University, Box 534, SE-75121 Uppsala, Sweden c Department of Nuclear and Reactor Physics, Royal Institute Uppsala, Sweden b Condensed Matter Theory Group, Physics Department, AAngstroom Laboratory, Uppsala reactors, face centered cubic (fcc) and hexagonal close packed (hcp) phases were considered in order

318

Phenotypic Data Collection and Sample Preparation for Genomics of Wood Formation and Cellulosic Biomass Traits in Sunflower: Ames, IA location.  

Science Conference Proceedings (OSTI)

Three fields were planted in Ames in 2010, two association mapping fields, N3 and A, and a recombinant inbred line field, N13. Phenotype data and images were transferred to UGA to support genetic and genomic analyses of woody biomass-related traits.

Marek, Laura F.

2011-06-17T23:59:59.000Z

319

EIS-0456: Record of Decision and Floodplain Statement of Findings...  

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

456: Record of Decision and Floodplain Statement of Findings EIS-0456: Record of Decision and Floodplain Statement of Findings Cushman Hydroelectric Project, Mason County,...

320

Seagate Crystal Reports - Meeti  

Science Conference Proceedings (OSTI)

William T. Martin, III. Technical Director. King Fifth Wheel. Paul Mason. UES Software Inc. Wendy Matthews. Capstone Turbine Corp. Gernant E. Maurer.

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


321

Generalized Pattern Search in a Parallel Environment - CECM  

E-Print Network (OSTI)

Nov 2, 2002 ... 1. Generalized Pattern Search in a Parallel. Environment. Mason Macklem. Mathematics and Statistics. Simon Fraser University. November 2...

322

SSATTM CFP - SAMATE  

Science Conference Proceedings (OSTI)

... PROGRAM COMMITTEE: Freeland Abbott Georgia Tech Jim Alves-Foss U. Idaho Paul Ammann George Mason U. Paul E. Black NIST Elizabeth ...

2013-05-22T23:59:59.000Z

323

Desert Hedgehog/Patched 1 signaling specifies fetal Leydig cell fate in  

E-Print Network (OSTI)

precursor. Dev. Biol. 240: 92­107. Ariyaratne, S.H.B., Mendis-Handagama, C.S., Hales, B.D., and Mason, I

Richardson, David

324

A History of ?Direct Search? Methods - CECM - Simon Fraser University  

E-Print Network (OSTI)

1. A History of ?Direct Search? Methods. Mason Macklem. Department of Mathematics. Simon Fraser University. May 1, 2003 msmackle@cecm.sfu.ca.

325

NETL F 451.1/1-1, Categorical Exclusion Designation Form  

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

EE0002213 National Biodiesel Foundation EE Renewable Energy Group OEPMPVTD FY10-14 1012009 - 9302014 Nicholas D'Amico Mason City, Cerro Gordo, Iowa 2009 National Biodiesel...

326

--No Title--  

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

manager for Science, DOE Oak Ridge Operations; ORNL Director Thom Mason; Joe Zimmerman, XCEL Engineering; Corey Martin, MartinFederal; Randall McGinnis, Echota Technologies;...

327

CX-008691: Categorical Exclusion Determination  

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

Mason Substation Metering Replacement Project CX(s) Applied: B1.7 Date: 06/25/2012 Location(s): Washington Offices(s): Bonneville Power Administration

328

Tungsten Oxide and Heteropoly Acid Based System for Ultra-High...  

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

for the Oxygen Reduction Reaction", K. Mason, M. Kuo, K. Horning, K. Neyerlin, and A. Herring, Journal of the Electrochemical Society (Submitted June 2012). 5. "Durability...

329

Microsoft PowerPoint - IPRC  

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

* Depleted uranium (III) chloride additions studied at INL Crushed salt in mason jar Desiccators 5 Electrochemistry Equipment - UW Electrochemistry glovebox Heater O 2...

330

The Prospects for Social Business in Peri-Urban Water Supply: Employment and Household Welfare Impacts of the Grameen Veolia Venture  

E-Print Network (OSTI)

such as pipes, spigots and jars. Masons are essential toselling water delivered in jars. These alterations to thethe program launched a jar business in peri-urban centers

Pierce, Gregory

2013-01-01T23:59:59.000Z

331

The use of benchmarking at the U.S. Department of Energy`s Pantex Plant  

SciTech Connect

The U.S. Department of Energy`s (DOE`s) Pantex Plant, located in Amarillo, Texas, is responsible for the assembly, stockpile maintenance, and disassembly of nuclear weapons. Pantex is operated by the Mason and Hanger-Silas Mason Co., Inc. The following summarizes the pilot study that was designed to establish Pantex as a leader in using the continuous improvement tool of benchmarking within the DOE`s Nuclear Weapon Complex (NWC). The pilot study was conducted with Mason and Hanger-Silas Mason Co. and Pacific Northwest Laboratory (PNL) personnel during 1992.

Anderson, F.G.; Burling, J.; Moncivais, G.C.; Skelton, R. [Mason and Hanger-Silas Mason Co., Inc., Amarillo, TX (United States); Fulton, J.T.; Hostick, C.J.; Tuttle, T. [Pacific Northwest Lab., Richland, WA (United States)

1993-09-01T23:59:59.000Z

332

EIS-0445: American Electric Power Service Corporation's Mountaineer...  

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

5: American Electric Power Service Corporation's Mountaineer Commercial Scale Carbon Capture and Storage Demonstration, New Haven, Mason County, West Virginia EIS-0445: American...

333

Current Trends in Image Quality Perception - CECM - Simon Fraser ...  

E-Print Network (OSTI)

Current Trends in Image Quality Perception. Mason Macklem. Simon Fraser University. http://www.cecm.sfu.ca/~msmackle. General Outline. Examine model of...

334

"Genetic Factors Affecting Susceptibility to Low-Dose Radiation...  

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

Laboratory, University of Maryland, Baltimore, MD 2 Virginia Mason Cancer Center, Seattle, WA 3 Memorial Sloan Kettering Cancer Center, New York, NY Rationale: Risk estimates...

335

Microsoft Word - DOE-Morgan-1.doc  

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

Laboratory, University of Maryland, Baltimore, MD 2 Virginia Mason Cancer Center, Seattle, WA 3 Memorial Sloan Kettering Cancer Center, New York, NY Rationale: Risk estimates...

336

Calibrating Artificial Neural Networks by Global Optimization  

E-Print Network (OSTI)

integrated oil and gas production systems (Mason et al., 2007), vehicle component design. (Goossens et al., 2007), various packing problems with industrial...

337

Microsoft PowerPoint - NERC Reliability Standards and Mandatory...  

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

NERC Reliability Standards and Standards and Mandatory Compliance Mandatory Compliance Hydro Hydro - - Power Conference Power Conference June 13, 2007 June 13, 2007 Stan Mason...

338

NIST Provides Octagonal Window of Opportunity for Carbon ...  

Science Conference Proceedings (OSTI)

... MR Hudson, WL Queen, JA Mason, DW Fickel, RF Lobo and CM Brown. Unconventional, highly selective CO 2 adsorption in zeolite SSZ-13. ...

2012-02-07T23:59:59.000Z

339

--No Title--  

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

constructed for Aid to Distressed Families of Appalachian Counties by volunteers from Oak Ridge National Laboratory's Team UT-Battelle. Looking on are Lab Director Thom Mason,...

340

SITE CHARACTERIZATION FOR CO  

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

Mason Tomson University of Alabama at Birmingham Pete Walsh Southern Company, Alabama Power Richard Esposito Schlumberger Carbon Services Micro-g Lacoste SECARB OUTLINE *...

Note: This page contains sample records for the topic "mason ia midamerican" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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341

EIS-0445: Draft Environmental Impact Statement | Department of...  

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

Statement EIS-0445: Draft Environmental Impact Statement Mountaineer Commercial Scale Carbon Capture and Storage Project, Mason County, West Virginia This EIS evaluates the...

342

NCNR NG7-SANS Instrument Schedule P. Butler Tel: (301) ...  

Science Conference Proceedings (OSTI)

... White + M. Copolyesters and Lin Surfactant Mixtures Aug 1 3 T. Mason 2827 Crude Oil in Mixed 10CB Lin Solvents Aug 4 3 G. Schmidt 2834 ...

343

American Conference on Neutron Scattering 2010 - ORNL Neutron...  

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

Update on Sample Environment Plenary Session: Thom Mason: Neutron Scattering and Energy ACNS website with Program Back to Top an error occurred while processing this directive...

344

Occult Americans: Invisible Culture and the Literary Imagination  

E-Print Network (OSTI)

England and the Bavarian Illuminati. Diss. Columbia U, 1918.Meetings of Free Masons, Illuminati, and Reading Societies.Bryan. The Bavarian Illuminati, the Early American Novel,

Finley, Lana Louise

2012-01-01T23:59:59.000Z

345

Pb-Free Sn-Ag-Cu-Mn Solder - Energy Innovation Portal  

Anderson, Iver E. (Ames, IA), Harringa, Joel (Ames, IA), Walleser, Jason K. (Idaho Falls, IA) Assignee: Iowa State University Research Foundation, ...

346

The SOFL Approach: An Improved Principle for Requirements Analysis 3  

E-Print Network (OSTI)

, Mitsuru Ohbay , Keijiro Araki? y Hiroshima City University, Japan z George Mason University, USA ? KyushuMinistryofEducationofJapanunderJointResearchGrant-in-AidforInternational Scienti#12;c Research FM-ISEE (08044167) and by Hiroshima City University under Hiroshima City University among Hiroshima City University and Kyushu University of Japan, George Mason University of 1 #12;be

347

 

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

Media Relations Media Relations Communications 865.576.1946 Mason elected AAAS fellow OAK RIDGE, Tenn., Nov. 19, 2001 - Thomas Mason, associate laboratory director of the Spallation Neutron Source at Oak Ridge National Laboratory, has been elected a fellow of the American Association for the Advancement of Science. Mason was cited for "distinguished contributions to condensed matter physics using neutron scattering and for leadership in the development of neutron scattering sources and instrumentation." Before being named associate laboratory director in February, Mason had worked with the SNS project since 1998 as director of its Experimental Facilities Division. Mason, a native of Canada, received a bachelor of science degree in physics from Dalhousie University, Halifax, Nova Scotia, and a doctorate in

348

Page not found | Department of Energy  

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

81 - 22490 of 28,905 results. 81 - 22490 of 28,905 results. Rebate Energy Revolving Loan Fund- Clean Energy Advanced Manufacturing '''''Note: This program is not currently accepting applications. Check the program web site for information regarding future solicitations.'''''... http://energy.gov/savings/energy-revolving-loan-fund-clean-energy-advanced-manufacturing Rebate Grant County PUD- Residential Loan Program Grant County PUD assists residential customers who wish to increase the efficiency of homes by providing financing for a variety of improvements. 10-year loans with an interest rate of 4% are... http://energy.gov/savings/grant-county-pud-residential-loan-program Rebate MidAmerican Energy (Electric) - Municipal Solid-State Lighting Grant Program MidAmerican Energy offers grants to munipalities which implement

349

PRE-STUDY COMMENTS OF IOWA UTILITIES BOARD ON DOE 2012 ELECTRIC TRANSMISSION CONGESTION STUDY  

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

PRE-STUDY COMMENTS OF IOWA UTILITIES BOARD ON PRE-STUDY COMMENTS OF IOWA UTILITIES BOARD ON DOE 2012 ELECTRIC TRANSMISSION CONGESTION STUDY JANUARY 2012 The Iowa Utilities Board (Board) is pleased to provide these comments as the Department of Energy (DOE) commences its next transmission congestion study (2012). These comments are organized to give DOE a perspective on electric transmission issues in Iowa - transmission planning, congestion, and siting. Iowa has been a leader in wind generation installation as well as manufacturing of wind turbines. Iowa has the second most installed wind capacity of any state. Since the DOE 2009 congestion study, Iowa added 884 MW of wind generation in 2009 -2010. MidAmerican Energy Company (MidAmerican), an Iowa investor owned utility added 593.5 MW in 2011 and plans to

350

National plan for the accelerated commercialization of solar energy. Final report  

SciTech Connect

After a brief profile of the Mid-American region and characterization of the residential and commercial markets and the industry of the region, a short description is given of a regional planning meeting held for the purpose of preparing input for the Mid-American section of the National Program for the Accelerated Commercialization of Solar Energy (NPAC) Implementation plans. For each of thirty-eight programs, the objective, rationale, task statement/description, evaluation measures, and implementor are given. The programs are in these areas: public education/awareness; education/training; legislative/regulatory; performance/analysis; design/planning;demonstrations; state interface; technology; information dissemination; legal and regulatory; analysis and assessment; and regional coordination. Two policy statements are included - one on cratering a solar society and the other recommending the expansion of the commercialization to encompass and include the concepts of utilization and popularization in the plan for the advancement of solar energy. (LEW)

1979-09-01T23:59:59.000Z

351

NETL: Mercury Emissions Control Technologies - Low-Cost Options for  

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

Low-Cost Options for Moderate Levels of Mercury Control Low-Cost Options for Moderate Levels of Mercury Control ADA- Environmental Solutions will test two new technologies for mercury control. The TOXECON II(tm) technology injects activated carbon directly into the downstream collecting fields of an electrostatic precipitator. The benefit of this technology is that the majority of the fly ash is collected in the upstream collecting fields which results in only a small portion of carbon-contaminated ash. Additionally, the TOXECON II(tm) technology requires minimal capital investment as only minor retrofits to the electrostatic precipitator are needed. The second technology is injection of novel sorbents for mercury removal on units with hot-side electrostatic precipitators (ESPs). Mercury removal from hot-side electrostatic precipitators is difficult as their high operating temperature range keeps the mercury in the vapor phase and prevents the mercury from adsorbing onto sorbents. The TOXECON II(tm) technology will be tested at Entergy's Independence Station which burns PRB coal. The novel sorbents for hot-side ESPs technology will be tested at MidAmerican's Council Bluffs Energy Center and MidAmerican's Louisa Station, both of which burn PRB coal. Additional project partners include EPRI, MidAmerican, Entergy, Alliant, ATCO Power, DTE Energy, Oglethorpe Power, Norit Americas Inc., Xcel Energy, Southern Company, Arch Coal, and EPCOR.

352

Measurement of Omega_m, Omega_Lambda from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe  

E-Print Network (OSTI)

Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

2006-01-01T23:59:59.000Z

353

OES-IA Annex IV: Environmental Effects of Marine and Hydrokinetic Devices - Report from the Experts Workshop September 27th 28th 2010 Clontarf Castle, Dublin Ireland  

SciTech Connect

An experts' workshop was convened in Dublin Ireland September 27th 28th 2010 in support of IEA Ocean Energy Systems Implementing Agreement Annex IV. PNNL was responsible for organizing the content of the workshop, overseeing the contractors (Irish Marine Institute) hosting the event, presenting material on Annex IV and materials applicable to the workshop intent. PNNL is also overseeing a contractor (Wave Energy Center/University of Plymouth WEC/UP) in the collection and analysis of the Annex IV data. Fifty-eight experts from 8 countries attended the workshop by invitation, spending two days discussing the needs of Annex IV. Presentations by DOE (background on Annex IV), PNNL (process for developing Annex IV; presentation of the draft database for PNNL project, plans for incorporating Annex IV data), WEC/UP on the environmental effect matrix, and four MHK developers (two from the UK, one from Ireland and one from Sweden; each discussing their own projects and lessons learned for measuring and mitigating environmental effects, as well as interactions with consenting [permitting] processes) helped provide background. The workshop participants worked part of the time in the large group and most of the time in four smaller breakout groups. Participants engaged in the process and provided a wealth of examples of MHK environmental work, particularly in the European nations. They provided practical and actionable advice on the following: Developing the Annex IV database, with specific uses and audiences Strong consensus that we should collect detailed metadata on available data sets, rather than attempting to draw in copious datasets. The participants felt there would then be an opportunity to then ask for specific set of data as needed, with specific uses and ownership of the data specified. This is particularly important as many data collected, particularly in Europe but also in Canada, are proprietary; developers were not comfortable with the idea of handing over all their environmental effects data, but all said they would entertain the request if they specifics were clear. The recommendation was to collect metadata via an online interactive form, taking no more than one hour to complete. Although the idea of cases representing the best practices was recognized as useful, the participants pointed out that there are currently so few MHK projects in the water, that any and all projects were appropriate to highlight as cases. There was also discomfort at the implication that best practices implied lesser practices; this being unhelpful to a new and emerging industry. Workshop participants were asked if they were willing to continue to engage in the Annex IV process; all expressed willingness. The workshop was successful in adequately addressing its objectives and through participation and interaction in the breakout sessions around the various topics. As a result of the workshop, many delegates are now better informed and have a greater understanding of the potential environmental effects of MHK devices on the marine environment. There is now a greater sense of understanding of the issues involved and consensus by those regulators, developers and scientists who attended the workshop. A strong network has also been built over the two days between European and US/Canadian technical experts in wave and tidal energy.

Copping, Andrea E.; O'Toole, Michael J.

2010-12-02T23:59:59.000Z

354

??eia e e et ??? oa0 to 3i5ontinBoB5 PieeFi5e Hinea tiTiUation ...  

E-Print Network (OSTI)

Analysis and Simplicial Subdivision,?l k ?????? ? ransactions onvd ircuits ... Ordered Sets: A Polyhedral Approach,%q h atC? ematicalG? ro?? ram-.

355

Gene F. Parkin, P.E. B.S.C.E. University of Iowa, Iowa City, IA; 1970 (with High Distinction)  

E-Print Network (OSTI)

Stimulation of Anaerobic Digestion," Water Research, 17, 677 (1983). 11. Hergenroeder, R. and Parkin, G of Anaerobic Toxicity by Batch and Semi-Continuous Assays," Jour. Water Pollution Control Fed., 52, 720 (1980 Anaerobic Reactors: Response to Toxic Substances," Water Science and Tech., 15, 261 (1983). #12;2 13.

Stanier, Charlie

356

50,000-Watt AM Stations IA | MB | MI | MN | NE | ND | ON | SD | WI | Station News | Owners | TV Captures | Links  

E-Print Network (OSTI)

2) and the concentration of 65Cu2+ estimated by the speciation model WHAM (1.0 (28)), we could]e^ equals zero and that [65 Cu2+ ] was constant (i.e., nominal [65 Cu2+ ] ) 5.2-µg L-1). That is, WHAM the speciation model WHAM (28) assuming that the lake water has a pH near 8 (30), a dissolved organic carbon

Allen, Gale

357

IEEE IAS Annual Meeting, Oct. 6-10, 1996, San Diego, CA, pp. 2333-2339 Survey of Harmonics Measurements in Electrical Distribution Systems  

E-Print Network (OSTI)

be 1.0 [7]. Form Factor I I RMS _ = 1 (5) Symmetrical components is a mathematical tool used to analyze of several buildings in the three Department of Energy (DOE) Oak Ridge plants in Tennessee has yielded), variable frequency drives, switch mode power supplies, and uninterruptible power supplies. A discussion

Tolbert, Leon M.

358

Bell L a b s , NE C Re s e ar ch I n stit u t e a nd Telco r d ia ... - CECM  

E-Print Network (OSTI)

i nfo r m ation doe s no t t ell u s t he loc ation of t he co rr e sp ond i ng f ra gmen t on t he tar ge t D N A , only s ome t h i ng a bou t t he r el ative o r de r of t he...

359

Targeted Energy Efficiency Expert Evaluation (E4) Report: Iowa City Federal Building and U.S. Post Office, Iowa City, IA  

SciTech Connect

Final report summarizing Targeted E4 measures and energy savings analysis for the Iowa City Federal Building and Post Office.

Goddard, James K.; Fernandez, Nicholas; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

360

Contribution of Iron-Reducing Bacteria to Mercury Methylation in Marine Sediments  

E-Print Network (OSTI)

AND R. P. MASON. 2006. Mercury methylation by dissimilatoryPRUCHA, AND G. MIERLE. 1991. Mercury methylation by sulfate-AND J. M. SIEBURTH. 1993. Mercury biogeochemical cycling in

Fleming, Emily J.; Nelson, D C

2006-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "mason ia midamerican" 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

Control of mercury methylation in wetlands through iron addition  

E-Print Network (OSTI)

Mason, R. P. ; Flegal, A. R. , Mercury speciation in the SanP. ; Flegal, A. R. , Decadal mercury trends in San FranciscoP. G. ; Nelson, D. C. , Mercury methylation from unexpected

Sedlak, David L; Ulrich, Patrick D

2009-01-01T23:59:59.000Z

362

STATEMENT OF CONSIDERATIONS CLASS WAIVER OF THE GOVERNMENT'S U.S. AND FOREIGN  

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

PANTEX PLANT PANTEX PLANT PURSUANT TO THE DEPARTMENT OF ENERGY/MASON AND HANGER-SILAS MASON CO., INC., PERFORMANCE-BASED MANAGEMENT CONTRACT NO. DE-AC04-91AL65030 - W(C)95-002 MASON AND HANGER-SILAS MASON CO., INC., (Contractor), manages and operates the Pantex Plant for the Department of Energy (DOE) under Prime Contract No. DE-AC04-91AL65030. Contractor is organized as a large, for-profit corporation. The Pantex Plant is a Government-owned, Contractor-operated facility located near Amarillo, Texas and is a part of the DOE nuclear weapons complex. The recent modification of Section 91 of the Atomic Energy Act, coupled with the National Competitiveness Technology Transfer Act of 1989 (NCTTA)(P.L. 101-189), clarified that technology transfer is a mission of Defense Programs consistent with the national security

363

Putting Science to Work BUILDING NANOTECHNOLOGY DEVELOPMENT  

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

BUILDING BUILDING NANOTECHNOLOGY DEVELOPMENT THOM MAsON NAMED ORNL DiRECTOR Accompanying Congressman Wamp (at lectern) during the grant announcement are, from left, Oak Ridge City Councilwoman Lou Dunlap; Tom Ballard, ORNL director of Economic Development and Partnerships; and Gerald Boyd, manager, DOE Oak Ridge Office. THOM MAsON NAMED ORNL DiRECTOR T hom Mason has been named ORNL's new direc- tor, effective July 1. The choice was announced in late May by UT-Battelle Board of Governors Chair Carl Kohrt and Vice Chair John Petersen. Mason's most recent role has been associate labora- tory director for Neutron Sciences. As head of the Spallation Neutron Source project, he led a consortium of six DOE labs in the design and construction of the $1.4 billion neutron accelerator. Completed on time,

364

Mountain Association for Community Economic Development- How$martKY On Bill Financing Energy Efficiency Program  

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

Four rural utility cooperatives in Eastern Kentucky (Big Sandy RECC, Fleming-Mason RECC, Grayson RECC, and Jackson Energy) work with MACED to provide energy retrofits as part of utility service...

365

NCNR NG7-SANS Instrument Schedule P. Butler Tel: (301) ...  

Science Conference Proceedings (OSTI)

... Oct 20 2 Reactor Shutdown Oct 22 3 T. Mason + E. 1596 Asphaltene Aggregation in 10CB Lin Sirota + M. Lin Crude Oil Oct 25 1 D. Peiffer + M ...

366

ABAA - 6th International Conference on Advanced Lithium Batteries...  

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

06:15 Mason Harrup Scientist, Idaho National Laboratory, USA 6:15 Close 07:00 - 09:30 Banquet Conference Schedule on Sep. 11, 2013 Time Event SESSION ONE: BEYOND LI-ION BATTERY...

367

Development of Extraction Techniques for the Detection of Signature Lipids from Oil  

E-Print Network (OSTI)

hasbeenshownpreviouslyinoilsamples (Hallman,2008)ofsignaturelipidsfromoil SharonBorglin,OliviaMason,were combined with model oil samples and oil/diesel mixtures

Borglin, Sharon

2011-01-01T23:59:59.000Z

368

Supertidal Frequency Internal Waves on the Continental Shelf South of New England  

Science Conference Proceedings (OSTI)

Large-amplitude internal waves of supertidal frequency are commonly observed on continental shelves during the stratified mason. We present a series of intensive observations of such waves at an anchor station south of New England using two CTD ...

Derek M. Burrage; Richard W. Garvine

1987-06-01T23:59:59.000Z

369

Gene Expression by Microbial Communities in Response to Soil Wet-Up: Microbial Resuscitation Strategies, Nitrifier Response Dynamics, and N2O Pulses  

E-Print Network (OSTI)

field, and sealed in mason jars prior to returning to thehumidity in Berkeley, CA. Jars were kept in the dark at roomperformed in 8-oz. glass jars. For each soil, 5 jars were

Placella, Sarah Anne

2011-01-01T23:59:59.000Z

370

The School Terrarium  

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

germinating seeds hard to grow. Almost any clear glass container, from an ordinary mason jar up to a large show case, can be used. A rectangular aquarium, even a leaky one, makes a...

371

Evaluation of Fitness and Genetic Variation in Aphytis melinus DeBach, an Important Biological Control Agent of Aonidiella aurantii (Maskell) in California  

E-Print Network (OSTI)

mouth, pint size Kerr Mason jars (Jarden Corporation, Rye,NY). Jars were covered with a fine mesh cloth that wasthe Petri dish and into the jar for 20 minutes. Individuals

Vasquez, Casandra Jean

2010-01-01T23:59:59.000Z

372

VBA-0060 - In the Matter of Robert Burd | Department of Energy  

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

of Robert Burd VBA-0060 - In the Matter of Robert Burd On November 16, 2001, BWXT Pantex, as successor to Mason & Hanger Corporation (M&H) (collectively referred to as "the...

373

VBX-0060 - In the Matter of Robert Burd | Department of Energy  

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

of Robert Burd VBX-0060 - In the Matter of Robert Burd On November 16, 2001, BWXT Pantex, as successor to Mason & Hanger Corporation (M&H) (collectively referred to as "the...

374

PARTITIONING OF MAJOR, MINOR, AND TRACE ELEMENTS DURING SIMULATED IN SITU OIL SHALE RETORTING IN A CONTROLLED-STATE RETORT  

E-Print Network (OSTI)

v. 18, p. Hadeishi, T. and McLaughlin, R. D. , 1975, IsotopeAugust. Hadeishi, T. and McLaughlin, R. D. , 1978, ZeemanJ. J. , Mason, K. K. , McLaughlin, R, E. , Bartke, T. C. ,

Fox, J. P.

2011-01-01T23:59:59.000Z

375

Grain Core Dielectric Constants of Acceptor-doped Oxide Electrolytes  

Science Conference Proceedings (OSTI)

Author(s), Nicola H. Perry, Ted C. Yeh, Thomas O. Mason. On-Site Speaker ... Water Uptake and Conduction Property of Nano-grained Fluorite-type Oxides.

376

Commonwealth of Virginia 457 Deferred Compensation Plan Payroll Authorization Form --Instructions for State Agencies  

E-Print Network (OSTI)

for State Agencies Without Online Functionality Action Requested: Check the box that describes the action Compensation Plan Payroll Authorization Form -- State Agencies Without Online Functionality Currently, three State agencies (George Mason University, Virginia Commonwealth University and the University of Virginia

Brodie III, Edmund D.

377

Argonne PowerPoint Presentation  

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

School on Neutron and X-ray Scattering Oak Ridge 12-26 June 2010 John M. Carpenter IPNS, SNS 23 June 2010 I acknowledge the assistance of Thom Mason, Kent Crawford and Ron Cooper...

378

Copyright 2005 by the Genetics Society of America DOI: 10.1534/genetics.104.027607  

E-Print Network (OSTI)

of Subfunctions and Modular Gene Regulation Allan Force,*,1 William A. Cresko,, F. Bryan Pickett,§ Steven R. Proulx, Chris Amemiya* and Michael Lynch** *Benaroya Research Institute at Virginia Mason, Seattle

Lynch, Michael

379

NCNR NG7-SANS Instrument Schedule P. Butler Tel: (301) ...  

Science Conference Proceedings (OSTI)

... S. 3160 Structure of Ion- 9P Kline Young Substituted Nafion Mar 20 2 T. Mason 3208 Crude Oil in Mixed 10CB Lin Solvents Mar 22 3 D. Ho + M ...

380

NCNR NG7-SANS Instrument Schedule P. Butler Tel: (301) ...  

Science Conference Proceedings (OSTI)

... May 9 2 B. Chapman 2725 Polyolefin Blends 7H Lin May 11 3 T. Mason + Z. Cheng 2706 Crude Oil Mixtures 10CB Lin + B. Silbernagel May 14 3 J ...

Note: This page contains sample records for the topic "mason ia midamerican" 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

Two dimensional NMR Investigations of the dynamic conformations of Phospholipids and liquid crystals  

E-Print Network (OSTI)

I. H. In Phosphorous-31 NMR: Principles and Applications; I.L. B. ; Kalabin, G. A. Prog. in NMR Spect. 1989,21, 293. , IJ Jameson, C. J. In Multinuclear NMR; J. Mason, Ed. ; Plenum

Hong, Mei

2010-01-01T23:59:59.000Z

382

District of Columbia | Department of Energy  

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

Mason County PUD 3 - Commercial and Industrial Energy Rebates Mason County PUD 3 - Commercial and Industrial Energy Rebates Mason County PUD 3 offers rebates to its non-residential customers for implementing energy efficient lighting, motor rewinds, refrigeration, commercial cooking equipment, and custom projects. Prescriptive rebates vary by type and the efficiency of purchased equipment. Information on some of these programs is available on the program web site. For more details on all rebate programs, contact the Energy Conservation Department at Mason County PUD 3. October 16, 2013 Mandatory Utility Green Power Option In May 2001, Washington enacted legislation (EHB 2247) that requires all electric utilities serving more than 25,000 customers to offer customers the option of purchasing renewable energy. Eligible renewables include

383

DOE - Office of Legacy Management -- Iowa State University Ames Laboratory  

Office of Legacy Management (LM)

Iowa State University Ames Iowa State University Ames Laboratory - IA 01 FUSRAP Considered Sites Site: Iowa State University Ames Laboratory (IA.01 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Wallace Road , Ames , Iowa IA.01-1 IA.01-2 Evaluation Year: Circa 1985 IA.01-3 Site Operations: Produced uranium and thorium metal, recovered uranium scrap, and conducted studies and experimental investigations in connection with chemistry and metallurgy of natural uranium and its allied forms. IA.01-1 IA.01-4 IA.01-5 IA.01-6 IA.01-7 Site Disposition: Eliminated - Referred to Chicago Operations Office for appropriate action IA.01-6 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium, Thorium IA.01-1

384

--No Title--  

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

Diversity of Type Ia Supernovae in the Near-Infrared Eric Hsiao University of Victoria ABSTRACT The photometric studies of Type Ia supernovae (SNe Ia) in the optical have...

385

DOE - Office of Legacy Management -- Ames Laboratory Research...  

Office of Legacy Management (LM)

Ames Laboratory Research Reactor Facility - IA 03 FUSRAP Considered Sites Site: Ames Laboratory Research Reactor Facility (IA.03) Designated Name: Alternate Name: Location:...

386

Interconnection Standards | Department of Energy  

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

You are here You are here Home » Interconnection Standards Interconnection Standards < Back Eligibility Agricultural Commercial Fed. Government Industrial Institutional Local Government Nonprofit Residential Schools State Government Savings Category Bioenergy Commercial Heating & Cooling Manufacturing Buying & Making Electricity Water Solar Wind Program Info State Iowa Program Type Interconnection Provider Iowa Utilities Board Different rules govern the interconnection of distributed generation facilities in Iowa, depending on whether or not the interconnection is with a utility whose rates are regulated by the Iowa Utilities Board (IUB). Rate regulated utilities include only the state's two investor-owned utilities -- MidAmerican Energy and Interstate Power and Light (IPL) -- and Linn

387

Residential conservation service program support. Final report  

SciTech Connect

Five tasks conducted by the Mid-American Solar Energy Center to research and prepare information for various constituents of the Residential Conservation Program are described. The tasks are: preparing cost data on renewable program (specifically solar) measure; designing and publishing a consumer agency guide to advise consumers of preventive and corrective actions to take when contracting for home improvements; providing a report on financing residential energy improvements; designing solar industry information releases, specifically on solar water heaters; and preparing a brochure, Your Place in the Sun - Solar Options Available to Homeowners. (MCW)

Not Available

1981-09-01T23:59:59.000Z

388

EIS-0456: Record of Decision and Floodplain Statement of Findings |  

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

Record of Decision and Floodplain Statement of Findings Record of Decision and Floodplain Statement of Findings EIS-0456: Record of Decision and Floodplain Statement of Findings Cushman Hydroelectric Project, Mason County, Washington DOE announces its decision to provide approximately $4.6 million appropriated under the American Recovery and Reinvestment Act to the city of Tacoma, Washington for the design and construction of certain components of the Cushman Hydroelectric Project in Mason County, Washington. Record of Decision and Floodplain Statement of Findings for the Cushman Hydroelectric Project, Mason County, Washington, Environmental Impact Statement, DOE/EIS-0456 (November 2010) 75 FR 73059 More Documents & Publications EIS-0456: Final Environmental Impact Statement EIS-0456: EPA Notice of Availability of the Final Environmental Impact

389

Page not found | Department of Energy  

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

21 - 16830 of 28,560 results. 21 - 16830 of 28,560 results. Download Puerto Rico Recovery Act State Memo http://energy.gov/downloads/puerto-rico-recovery-act-state-memo Download Preliminary Notice of Violation, Mason & Hanger Corporation- EA-1999-05 Preliminary Notice of Violation issued to Mason & Hanger Corporation, related to a Chemical Fire at the Pantex Plant, (EA-1999-05 http://energy.gov/hss/downloads/preliminary-notice-violation-mason-hanger-corporation-ea-1999-05 Download Preliminary Notice of Violation, Fluor Fernald, Inc.- EA-2004-07 Preliminary Notice of Violation issued to Fluor Fernald, Inc., related to Respiratory Protection Issues at the Fernald Environmental Management Project http://energy.gov/hss/downloads/preliminary-notice-violation-fluor-fernald-inc-ea-2004-07

390

Page not found | Department of Energy  

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

11 - 23120 of 28,560 results. 11 - 23120 of 28,560 results. Rebate Mason County PUD 3- Residential Energy Rebates Mason County PUD 3 encourages customers to use energy efficient products and home equipment by offering incentives for the purchase of qualifying products. The utility offers residential customers... http://energy.gov/savings/mason-county-pud-3-residential-energy-rebates Rebate Missouri Gas Energy (MGE)- Residential and Small Business Efficiency Rebates Missouri Gas Energy (MGE) offers its residential and small business customers rebates for the purchase and installation of efficient natural gas water heating and space heating equipment within its... http://energy.gov/savings/missouri-gas-energy-mge-residential-and-small-business-efficiency-rebates Rebate Montana-Dakota Utilities (Gas)- Residential Energy Efficiency Rebate

391

Page not found | Department of Energy  

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

31 - 24040 of 28,905 results. 31 - 24040 of 28,905 results. Rebate Liquefied Natural Gas (Iowa) This document adopts the standards promulgated by the National Fire Protection Association as rules for the transportation, storage, handling, and use of liquefied natural gas. The NFPA standards... http://energy.gov/savings/liquefied-natural-gas-iowa Rebate Mason County PUD 3- Commercial and Industrial Energy Rebates Mason County PUD 3 offers rebates to its non-residential customers for implementing energy efficient lighting, motor rewinds, refrigeration, commercial cooking equipment, and custom projects.... http://energy.gov/savings/mason-county-pud-3-commercial-and-industrial-energy-rebates Rebate Michigan Saves- Business Energy Financing Michigan Saves is a non-profit that offers financing options for energy

392

 

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

Bill Cabage Bill Cabage Communications 865.574.4399 Mason, Rykaczewski, Budai honored by American Physical Society OAK RIDGE, Tenn., Dec. 10, 2007 - Three scientists at the Department of Energy's Oak Ridge National Laboratory--including the laboratory's director--have been elected fellows of the American Physical Society (APS). The new APS fellows are ORNL Director Thom Mason, nuclear physicist Krzysztof Piotr Rykaczewski and materials scientist John Budai. Election to fellowship in the APS is limited to no more than one half of one percent of the annual APS membership and is in recognition of outstanding contributions to physics. Mason was cited by the APS's Division of Condensed Matter Physics for his career in condensed matter physics with a focus on neutron scattering

393

HANGER\MH  

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

MASON & HANGER CORPORATION MASON & HANGER CORPORATION February 10, 1998 U. S. Department of Energy Office of General Counsel, GC-52 1000 Independence Ave. SW. Washington, DC 20585 Subject: Reply comments to notice of inquiry concerning preparation of report to Congress on the Price-Anderson Act Dear Sir or Madam: Mason & Hanger Corporation has reviewed the Federal Register Notice published December 31, 1997. It is our intent to offer the attached replies to the listed questions contained in the Notice. Thank you for the opportunity to provide input to the report preparation process. Please contact myself or Alan G. Wagner, Esq. at (806) 477-7233 if you have any questions. Very truly yours,

394

Page not found | Department of Energy  

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

41 - 24250 of 29,416 results. 41 - 24250 of 29,416 results. Rebate Intercounty Electric Cooperative- Energy Efficiency Rebate Program Intercounty Electric Cooperative provides rebates to its customers for the purchase of a variety of energy efficient equipment and appliances. Eligible technologies include: geothermal, air source,... http://energy.gov/savings/intercounty-electric-cooperative-energy-efficiency-rebate-program Rebate Mason County PUD 3- Commercial and Industrial Energy Rebates Mason County PUD 3 offers rebates to its non-residential customers for implementing energy efficient lighting, motor rewinds, refrigeration, commercial cooking equipment, and custom projects.... http://energy.gov/savings/mason-county-pud-3-commercial-and-industrial-energy-rebates Rebate Michigan Saves- Business Energy Financing

395

Consent Order EA-2000-07  

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

1, 2000 1, 2000 Dr. Benjamin Pellegrini [ ] Mason & Hanger Corporation P.O. Box 30020 Amarillo, TX 79120-0020 EA 2000-07 Subject: Consent Order Incorporating Agreement between U.S. Department of Energy and Mason & Hanger Corporation Dear Dr. Pellegrini: 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. In January 1998, the contractor identified a systemic problem at the site in Building 12-98 when it was determined that certain high-pressure fire suppression valves were left in the closed position, which would have prevented their activation in

396

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

397

Corona driven air propulsion for cooling of electronics F. Yang, N.E. Jewell-Larsen, D.L. Brown, K. Pendergrass, D.A. Parker, I.A. Krichtafovitch*, A.V. Mamishev  

E-Print Network (OSTI)

generation with low noise, static filtration [5], air sterilization [6], and no moving parts. These ideal Abstract: The possibility of building a high voltage electrostatic air pump for cooling of microelectronics is investigated. Existing cooling technology no longer provides adequate heat dissipation due to excessive heat

Mamishev, Alexander

398

HIGH VOLTAGE TERMINAL IN COSY ELECTRON COOLER V.A. Chekavinskiy, E.A. Bekhtenev, I.A. Gusev, M.N. Kondaurov, V.R. Kozak, E.A. Kuper, V.R.  

E-Print Network (OSTI)

, and powered by multistage transformer, capable of 15 kW power at 26 kHz. Wireless control is passed through high voltage circumstances. Powering of HVT electronics is provided by cascade transformer acceleration system ­ high voltage terminal. All power and control electronics were placed in a single isolated

Kozak, Victor R.

399

BIG IDEAS FOR JOB CREATIOn A PROJECT OF ThE UnIvERSITy OF CALIFORnIA, BERKELEy AnD ThE AnnIE E. CASEy FOUnDATIOn  

E-Print Network (OSTI)

businesses generate more jobs. · Developing new jobs in emerging or resurgent sectors, such as clean energy-skilled workers. We sought to avoid gimmicks (such as one-time budget transfers), as well as wasteful incentive

California at Berkeley, University of

400

Annotated bibliography of research carried out from 1993 to 1999 under DoE Award No. DE-IA02-94ER14411: Spectroscopic investigation of the vibrational quasi-continuum arising from internal rotation of a methyl group  

DOE Green Energy (OSTI)

This report covers work carried out during a six year period under a DoE interagency grant. Because all results have been published as full papers in appropriate refereed journals that are openly available in most scientific libraries, the report takes the form of an annotated bibliography. In the interests of scientific continuity and bibliographic usefulness, however, work carried out on this same project from 1990-1992 under an earlier DoE award, as well as related work currently (2000-2002) in progress, will also be discussed. It should be stressed, however, that only work directly connected to the grantee is cited explicitly in this final grant report. The many important papers by other workers in the field during the last decade must be obtained from reference citations in the 21 publications mentioned.

Hougen, Jon T.

2002-03-04T23:59:59.000Z

Note: This page contains sample records for the topic "mason ia midamerican" 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

Regulatory Considerations for Developing Generation Projects on Federal Lands  

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

Mason Emnett Mason Emnett Office of Energy Policy and Innovation Jonathan First Office of the General Counsel February 6, 2013 NOTE: Comments herein do not represent the views of the Federal Energy Regulatory Commission or its Commissioners Regulatory Considerations for Developing Generation Projects on Federal Lands 2 Purpose of this Presentation * Describe the types of transactions that fall under FERC jurisdiction * Describe pertinent federal laws and how they apply - What does it mean to be a "public utility" or "transmitting utility" under federal law? - How does ownership and usage of a generation facility impact regulatory considerations? - When are parties required to register with NERC? 3 FERC-Related Statutes * Federal Power Act

402

Regulatory Considerations for Developing Generation Projects on Federal Lands  

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

Mason Emnett Mason Emnett Office of Energy Policy and Innovation Jonathan First Office of the General Counsel February 6, 2013 NOTE: Comments herein do not represent the views of the Federal Energy Regulatory Commission or its Commissioners Regulatory Considerations for Developing Generation Projects on Federal Lands 2 Purpose of this Presentation * Describe the types of transactions that fall under FERC jurisdiction * Describe pertinent federal laws and how they apply - What does it mean to be a "public utility" or "transmitting utility" under federal law? - How does ownership and usage of a generation facility impact regulatory considerations? - When are parties required to register with NERC? 3 FERC-Related Statutes * Federal Power Act

403

Stability Criteria for Impulsive Systems with Time Delay and Unstable System Matrices  

E-Print Network (OSTI)

the above it is su cient to prove that for any A 2 F0, the following holds : IE0 1IAN0;t = IE0 Z t 0 sds1IA0 N;Ft-intensity of fNtg it follows that IE0 N Z t 0 Zs,dNs1IA = IE0 N Z t 0 Zs,sds1IA : But since that IE0 N Z t 0 ZsdNs1IA = IE0 N Z t 0 Zssds1IA : Noting that IE0 N Z t 0 Zssds1IA = N IE0 Z t 0 sds1

Shen, Xuemin "Sherman"

404

Part B - Requirements & Funding Information PART B - Requirements...  

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

authorities) B.3. Part B Identifier If this is a new IA, then leave this blank. After STRIPES creates the IA identifier number, the number will appear in Part A Section A.3....

405

Part B - Requirements & Funding Information PART B - Requirements...  

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

authorities B.3. Part B Identifier If this is a new IA, then leave this blank. After STRIPES creates the IA identifier number, the number will appear in Part A Section A.3....

406

NERSC Users Group Meeting October 3-4, 2005 Presentations  

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

of the rate of acceleration of the universe's expansion, and of the density of "dark energy" believed to be driving it, hinge on observations of type Ia supernovae (SNe Ia). The...

407

Toyota Prius "hum"  

Science Conference Proceedings (OSTI)

Directed by Sam Mason and Pete Candeland, "Hum" is set to a catchy song that carries us on a journey through a charming miniature-style landscape to demonstrate the versatility of the Toyota Prius Hybrid and the lifestyles of various owners.

Anna Cunnington

2013-07-01T23:59:59.000Z

408

Comparing different overlay topologies and metrics in pulse-coupled multi-agent systems  

Science Conference Proceedings (OSTI)

In Multi-Agent Systems (MASs) it is of vital importance that basic network operations are performed without the interference of a central entity (i.e. agent). In this paper we will present how to use a self-organization approach to achieve time synchronization ... Keywords: MASON, firefly synchronization, pulse-coupled oscillators, self-organization

Iva Bojic; Mario Kusek

2012-06-01T23:59:59.000Z

409

R E N E W A B L E E N E R G Y  

E-Print Network (OSTI)

, and affordable nuclear energy Renewable Solar and Wind energy · Reduce the cost of solar PV technologies so for distributed (rooftop) PV systems. *From Zweibel, Mason, Fthenakis. "An Imminent Solar Solution to Climate-Reliance* PV and compressed air energy storage (CAES) for 24-hour electricity Concentrating Solar Power

410

Workshop on Virtual Reality Interaction and Physical Simulation VRIPHYS (2012) J. Bender, A. Kuijper, D. W. Fellner, and . Gurin (Editors)  

E-Print Network (OSTI)

on the challenge of establishing an Urban Atmospheric Observatory in NY Manhattan"-Tim Oke, University of British Columbia 11:30 "Overview of urban dispersion models and data sets" - Steve Hanna, George Mason University. Moderator: Tim Oke 14:45 Data collection, external data, OEM pipeline. Moderator: Rick Wagener 15:45 Coffee

Teschner, Matthias

411

Above All Men: a novel  

E-Print Network (OSTI)

a box of spaghetti. He got a jar of tomatoes from the pantryof her hand. Ill get a jar or something. She took thedown a bowl and a small mason jar. Thats alright. I havent

Shonkwiler, Eric Michael

2011-01-01T23:59:59.000Z

412

Browse by Discipline -- E-print Network Subject Pathways: Mathematics...  

Office of Scientific and Technical Information (OSTI)

Go back to Individual Researchers Collections: A B C D E F G H I J K L M N O P Q R S T U V W X Y Z George Mason University, Center for Air Transportation Systems Research...

413

Benefit/cost analysis for Transportation Infrastructure: A Practitioner's Workshop:Infrastructure: A Practitioner s Workshop  

E-Print Network (OSTI)

Benefit/cost analysis for Transportation Infrastructure: A Practitioner's Workshop for Transportation, Policy, O i d L i iOperations, and Logistics George Mason University #12;The idea of benefit fas well as the nearer future) and a wide view (in the sense of allowing for sideeffects of many

414

CCSF Topical Lunch Summary Systems Approach to Sustainable Energy  

E-Print Network (OSTI)

and the Smartgrid. Attendees mentioned other colleagues who are share these interests: Mason Peck, Steve Pope, Hsiao. Lang Tong Expertise in communication networks/IT; interested in Smartgrid and energy distributions; optimization systems, machine learning, inference and Smartgrid Tim Mount Power systems, deregulation

Angenent, Lars T.

415

401 Academy Street Monday-Friday 8 am to 5 pm  

E-Print Network (OSTI)

- NewYork.com #12;Classifieds - The New York Times' Real Estate Section Lists inexpensive hotels, hostels, and boarding houses - SpanishNewYork.com Student Housing and Hotels in Manhattan, New York City utilities included The Catholic University of America - Summer housing is available for interns George Mason

Cakoni, Fioralba

416

On Subgrid Models and Filter Operations in Large Eddy Simulations  

Science Conference Proceedings (OSTI)

Large eddy simulations use a subgrid model, which is characterized by a length scale that is often related to the scale of the computational mesh by a numerical constant, Cs. Mason and Callen argued that this subgrid model and its length scale ...

P. J. Mason; A. R. Brown

1999-07-01T23:59:59.000Z

417

Y campusmap Mead Visitor Center  

E-Print Network (OSTI)

& applied science law school graduate school Mason Lab Helen Hadley Hall Leet Oliver Watson Hall Malone left. The Visitor Center is on the left in the middle of the first block, across from the New Haven 203.432.2798 www.library.yale.edu Yale Bowl 81 Central Ave From downtown New Haven, go west on Chapel

418

New Synchronous Orbits Using the Geomagnetic Lorentz Force Brett Streetman  

E-Print Network (OSTI)

New Synchronous Orbits Using the Geomagnetic Lorentz Force Brett Streetman and Mason A. Peck the interaction between the Earth's geomagnetic field and an electrostatic charge built up on a satellite [2 causes an interaction between the geomagnetic field and the vehicle in the form of the Lorentz force

Peck, Mason A.

419

New Synchronous Orbits Using the Geomagnetic Lorentz Force  

E-Print Network (OSTI)

New Synchronous Orbits Using the Geomagnetic Lorentz Force Brett Streetman and Mason A. Peck makes use of the interaction between the Earth's geomagnetic field and an electrostatic charge built up an interaction between the geomagnetic field and the vehicle in the form of the Lorentz force. The magnitude

Peck, Mason A.

420

Supporting Information Model Selection Process. We began our analyses by determining the best general model.  

E-Print Network (OSTI)

aerial and/or ground surveys gave estimates of 0.886 (Owen-Smith & Mason 2005) and 0.915 (Nje 1983). Our occasion two in January-March 2009. Estimates based on aerial surveys in the 2001 wet season (March to compare directly because the aerial survey estimate included calves in the total count and covered

Farid, Hany

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


421

J. Fluid Mech. (2007), vol. 592, pp. 447469. c 2007 Cambridge University Press doi:10.1017/S0022112007008701 Printed in the United Kingdom  

E-Print Network (OSTI)

address: Departamento de Ingenier´ia Aeroespacial y Mec´anica de Fluidos, Universidad de Sevilla, Camino

Gelfond, Michael

422

Dr. Christina A. Hacker  

Science Conference Proceedings (OSTI)

... Clarke College, Dubuque, IA; BS, Chemistry; May 1997, Minor in mathematics. Graduated summa cum laude. Contact. Phone ...

2013-04-08T23:59:59.000Z

423

CORPORATE CAPABILITIES  

Science Conference Proceedings (OSTI)

... NSA sponsored IA programs and curriculum. ... comprehensive critical infrastructure curricula or graduate ... Nascent master's curriculums are underway ...

2013-04-09T23:59:59.000Z

424

You are now leaving Energy.gov | Department of Energy  

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

coolice.legis.state.ia.usCool-ICEdefault.asp?Categorybillinfo&ServiceBillbook&frame1&GA81&hbillHF2361...

425

National Laboratories - Energy Innovation Portal  

Name Address City, State; Ames Laboratory: Ames Laboratory: Ames, IA: Argonne National Laboratory: 9700 S. Cass Avenue: Argonne, IL: Brookhaven ...

426

Observation of a Narrow Charm-Strange Meson D A.V. Evdokimov,8  

E-Print Network (OSTI)

University of Iowa, Iowa City, IA 52242, USA 17 University of Michigan-Flint, Flint, MI 48502, USA 18

Akgun, Ugur

427

Conference on Physics with Large Gamma-Ray Detector Arrays, Volume II Proceedings  

E-Print Network (OSTI)

Laboratory, Berkeley, CA 94720 University of California, Davis, CA 95616 Iowa State University, Ames, IA 50010 Rutgers University, New Brunswick,

Lawler editor, G.

2010-01-01T23:59:59.000Z

428

Intracellular trafficking of adeno-associated viral and JF Engelhardt1,2,3  

E-Print Network (OSTI)

, Iowa City, IA, USA; 2 Department of Internal Medicine, University of Iowa School of Medicine, Iowa City, IA, USA; and 3 Center for Gene Therapy, University of Iowa School of Medicine, Iowa City, IA, USA following receptor binding and leading to nuclear uptake. These stages are broadly classified

Engelhardt, John F.

429

Grado en Ingenieria de Tecnologias Industriales --E.T.S.I. Industriales (U.P.M.) Mecanica del solido deformable  

E-Print Network (OSTI)

Grado en Ingenier´ia de Tecnolog´ias Industriales -- E.T.S.I. Industriales (U.P.M.) Mec´anica del s´ia adicional: · Zubizarreta, V. y Ros, A. Introducci´on a la mec´anica de los s´olidos. Segunda Ed

Romero, Ignacio

430

Bishop Hill II | Open Energy Information  

Open Energy Info (EERE)

II II Jump to: navigation, search Name Bishop Hill II Facility Bishop Hill II Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Ivenergy Energy Purchaser Ameren Illinois Location Cambridge IL Coordinates 41.24438513°, -90.09338379° 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":41.24438513,"lon":-90.09338379,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

431

Page not found | Department of Energy  

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

71 - 12980 of 28,560 results. 71 - 12980 of 28,560 results. Rebate Montana Electric Cooperatives- Net Metering The Montana Electric Cooperatives' Association (MECA) adopted model interconnection guidelines in 2001 and a revised net-metering policy in September 2008. Net metering is available in whole or... http://energy.gov/savings/montana-electric-cooperatives-net-metering Rebate U.S. Virgin Islands- Net Metering In February 2007, the U.S. Virgin Islands Public Services Commission approved a limited net-metering program for residential and commercial photovoltaic (PV), wind-energy or other renewable energy... http://energy.gov/savings/us-virgin-islands-net-metering Download Microsoft Word- AL2005-16.doc http://energy.gov/management/downloads/microsoft-word-al2005-16doc Rebate MidAmerican Energy (Electric)- Commercial EnergyAdvantage Rebate

432

Energy Incentive Programs, Iowa | Department of Energy  

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

Iowa Iowa Energy Incentive Programs, Iowa October 29, 2013 - 11:29am Addthis Updated September 2013 In 2012 Iowa utilities budgeted $over 180 million for energy efficiency programs in the state. What public-purpose-funded energy efficiency programs are available in my state? Iowa has no public-purpose-funded energy efficiency programs. What utility energy efficiency programs are available to me? MidAmerican Energy Company offers energy efficiency programs under the umbrella of the EnergyAdvantage initiative. A multitude of energy-efficient equipment financing opportunities and rebates are available, covering lighting, various heating and cooling equipment, motors, variable speed drives, commercial kitchen equipment, building insulation, and windows. Rebates are cash-back payments based on equipment type. For example,

433

Data:120314a7-504b-4237-a73b-9eac5bf40a17 | Open Energy Information  

Open Energy Info (EERE)

504b-4237-a73b-9eac5bf40a17 504b-4237-a73b-9eac5bf40a17 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/11/09 End date if known: Rate name: Price Schedule - LXS - Large General Service Base Use at Transmission Voltage Sector: Commercial Description: Source or reference: www.midamericanenergy.com Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous

434

Data:4ea9a256-e75c-4a2d-9108-c1cf18682044 | Open Energy Information  

Open Energy Info (EERE)

6-e75c-4a2d-9108-c1cf18682044 6-e75c-4a2d-9108-c1cf18682044 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 175W MV - Billed Use Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >>

435

Pinyon Pines II | Open Energy Information  

Open Energy Info (EERE)

Pinyon Pines II Pinyon Pines II Jump to: navigation, search Name Pinyon Pines II Facility Pinyon Pines II (Alta IX) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Terra-Gen Power Energy Purchaser Southern California Edison Co Location Tehachapi Pass CA Coordinates 35.01917213°, -118.3031845° 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":35.01917213,"lon":-118.3031845,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

436

Data:6af307a9-ffe0-4158-8b87-8be392c2fe7d | Open Energy Information  

Open Energy Info (EERE)

af307a9-ffe0-4158-8b87-8be392c2fe7d af307a9-ffe0-4158-8b87-8be392c2fe7d No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/03/02 End date if known: Rate name: Large General Service, Base Use at Primary Voltage Price Schedules LPN and APN Sector: Industrial Description: APPLICABLE: At the option of the customer, to all electric service required on premises by customer, subject to applicable terms and conditions of the Company's Electric Service Policies and Electric Rate Application. Applicable to standby or supplementary service (under written agreement only) in conjunction with applicable Company riders for such service.

437

Data:75dfaf36-ae84-4bdb-a820-c7ba5abe8686 | Open Energy Information  

Open Energy Info (EERE)

dfaf36-ae84-4bdb-a820-c7ba5abe8686 dfaf36-ae84-4bdb-a820-c7ba5abe8686 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 175W MV MP Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

438

Data:21770933-917e-4238-b47b-b5b2cec44616 | Open Energy Information  

Open Energy Info (EERE)

917e-4238-b47b-b5b2cec44616 917e-4238-b47b-b5b2cec44616 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 175W MV Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

439

State Solar Consumer Assurance Network (SOLCAN). Report, Phase I  

SciTech Connect

Existing consumer protection mechanisms and resources in each of the 12 states within the Mid-American Region are identified which may apply to solar technology or which have been designed especially to apply to solar energy systems. Consumer assurance mechanisms identified include consumer protection statues, codes/standards, licensing/certification of installers and contractors, incentives, energy audits/inspections, warranty law. A directory was prepared for each state that outlines the agencies and groups who provide energy-related services within the state and identifies the particular service which they provide, and which identifies solar-related technical training and educational resources within each state, the location of the resource, and specific course offerings. Services identified include information/technical assistance, referral, arbitration/mediation, legal redress, and legislative service. (LEW)

1981-01-01T23:59:59.000Z

440

Data:0016f771-cda9-4312-afc2-63f10c8d8bf5 | Open Energy Information  

Open Energy Info (EERE)

cda9-4312-afc2-63f10c8d8bf5 cda9-4312-afc2-63f10c8d8bf5 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 250W HPS MP Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

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


441

Data:56a3f20a-7cc2-4794-b563-9f75d355af9a | Open Energy Information  

Open Energy Info (EERE)

a-7cc2-4794-b563-9f75d355af9a a-7cc2-4794-b563-9f75d355af9a No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W MV MP - Billed Use Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >>

442

Data:F2321389-fbb2-44f7-845d-f37976dd288c | Open Energy Information  

Open Energy Info (EERE)

fbb2-44f7-845d-f37976dd288c fbb2-44f7-845d-f37976dd288c No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/11/09 End date if known: Rate name: Price Schedule - LVS Large General Service Time of Use at Primary Voltage Sector: Commercial Description: Source or reference: www.midamericanenergy.com Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous

443

Data:Ff784b14-46e2-4318-b000-f97d26a84499 | Open Energy Information  

Open Energy Info (EERE)

Ff784b14-46e2-4318-b000-f97d26a84499 Ff784b14-46e2-4318-b000-f97d26a84499 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W MV MP Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >>

444

Data:E0e8e48a-b0b7-48e6-af1f-249600fe111d | Open Energy Information  

Open Energy Info (EERE)

8a-b0b7-48e6-af1f-249600fe111d 8a-b0b7-48e6-af1f-249600fe111d No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 250W HPS Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

445

Data:F6da0f0c-3da5-4551-8ea5-2bc8c477931b | Open Energy Information  

Open Energy Info (EERE)

c-3da5-4551-8ea5-2bc8c477931b c-3da5-4551-8ea5-2bc8c477931b No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W HPS Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

446

Property:EnergyPurchaser | Open Energy Information  

Open Energy Info (EERE)

EnergyPurchaser EnergyPurchaser Jump to: navigation, search This is a property of type Page. Subproperties This property has the following 1 subproperty: G GRR/Section 4-FD-a - Exploration Permit BLM Pages using the property "EnergyPurchaser" Showing 25 pages using this property. (previous 25) (next 25) A AB Tehachapi Wind Farm + Southern California Edison Co + AFCEE MMR Turbines + Distributed generation - net metered + AG Land 1 + Alliant Energy + AG Land 2 + Alliant Energy + AG Land 3 + Alliant Energy + AG Land 4 + Alliant Energy + AG Land 5 + Alliant Energy + AG Land 6 + Alliant Energy + AVTEC + AVTEC + Adair Wind Farm I + Alliant/IES Utilities + Adair Wind Farm II + MidAmerican Energy + Aeroman Repower Wind Farm + Southern California Edison Co + Agassiz Beach Wind Farm + Xcel Energy +

447

Data:8256663a-ab3a-4a6f-b5bb-072096de823d | Open Energy Information  

Open Energy Info (EERE)

663a-ab3a-4a6f-b5bb-072096de823d 663a-ab3a-4a6f-b5bb-072096de823d No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/03/02 End date if known: Rate name: Large General Service, Base Use at Secondary Voltage Price Schedules LLN and ALN Sector: Industrial Description: APPLICABLE: At the option of the customer, to all electric service required on premises by customer, subject to applicable terms and conditions of the Company's Electric Service Policies and Electric Rate Application. Applicable to standby or supplementary service (under written agreement only) in conjunction with applicable Company riders for such service.

448

Data:D8f17bd4-b6b1-4602-9ddf-65f907b8e2bf | Open Energy Information  

Open Energy Info (EERE)

b6b1-4602-9ddf-65f907b8e2bf b6b1-4602-9ddf-65f907b8e2bf No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W HPS - Billed Use Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >>

449

Pinyon Pines I | Open Energy Information  

Open Energy Info (EERE)

Pinyon Pines I Pinyon Pines I Jump to: navigation, search Name Pinyon Pines I Facility Pinyon Pines I (Alta VII) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Developer Terra-Gen Power Energy Purchaser Southern California Edison Co Location Tehachapi Pass CA Coordinates 35.01917213°, -118.3031845° 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":35.01917213,"lon":-118.3031845,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

450

Data:643b2c4b-9492-4af4-87c5-3967de1f5305 | Open Energy Information  

Open Energy Info (EERE)

c4b-9492-4af4-87c5-3967de1f5305 c4b-9492-4af4-87c5-3967de1f5305 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/11/09 End date if known: Rate name: Price Schedule - LHS Large General Service with Electric Space Heating at Primary Voltage Sector: Commercial Description: Source or reference: www.midamericanenergy.com Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring:

451

Data:869b2063-643e-4e7c-a37b-08573c6b5e1f | Open Energy Information  

Open Energy Info (EERE)

63-643e-4e7c-a37b-08573c6b5e1f 63-643e-4e7c-a37b-08573c6b5e1f No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: End date if known: Rate name: Price Schedule ATS - Other Electric Service to Public Authorities - Traffic Controls Sector: Description: To all electric service required for traffic control signals and flashers by municipal, county, state and federal governments or agencies, subject to applicable terms and conditions of the Company's Electric Service Policies and Electric Rate Application. Source or reference: www.midamericanenergy.com Source Parent:

452

Data:B3e843be-0576-476d-8412-90b0f72d5c20 | Open Energy Information  

Open Energy Info (EERE)

be-0576-476d-8412-90b0f72d5c20 be-0576-476d-8412-90b0f72d5c20 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2012/11/09 End date if known: Rate name: Price Schedule - LES Large General Service with Electric Space Heating at Secondary Voltage Sector: Commercial Description: Source or reference: www.midamericanenergy.com Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring:

453

Net Metering | Department of Energy  

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

You are here You are here Home » Net Metering Net Metering < Back Eligibility Commercial Industrial Residential Savings Category Bioenergy Water Buying & Making Electricity Solar Home Weatherization Wind Program Info State Iowa Program Type Net Metering Provider Iowa Utilities Board Iowa's statutes do not explicitly authorize the Iowa Utilities Board (IUB) to mandate net metering, but this authority is implicit through the board's enforcement of PURPA and Iowa Code § 476.41 ''et seq.'' Iowa's net-metering subrule, adopted by the IUB in July 1984, applies to customers that generate electricity using alternate energy production facilities (AEPs). Net metering is available to all customer classes of Iowa's two investor-owned utilities -- MidAmerican Energy and Interstate Power and

454

Property:Owner | Open Energy Information  

Open Energy Info (EERE)

property of type Page. property of type Page. Subproperties This property has the following 1 subproperty: G GRR/Section 4-FD-a - Exploration Permit BLM Pages using the property "Owner" Showing 25 pages using this property. (previous 25) (next 25) A AB Tehachapi Wind Farm + Coram Energy + AFCEE MMR Turbines + AFCEE + AG Land 1 + AG Land Energy LLC + AG Land 2 + AG Land Energy LLC + AG Land 3 + AG Land Energy LLC + AG Land 4 + AG Land Energy LLC + AG Land 5 + AG Land Energy LLC + AG Land 6 + AG Land Energy LLC + AVTEC + AVTEC + Aberdeen Biomass Facility + Sierra Pacific Industries + Adair Wind Farm I + Shafer Systems + Adair Wind Farm II + MidAmerican Energy + Aero Turbine + AeroTurbine Energy Company + Aeroman Repower Wind Farm + Coram Energy + Affinity Wind Farm + Affinity Wind LLC +

455

Low-Cost Options for Moderate Levels of Mercury Control  

Science Conference Proceedings (OSTI)

This is the final technical report for a three-site project that is part of an overall program funded by the U.S. Department of Energy's National Energy Technology Laboratory (DOE/NETL) and industry partners to obtain the necessary information to assess the feasibility and costs of controlling mercury from coal-fired utility plants. This report summarizes results from tests conducted at MidAmerican's Louisa Generating Station and Entergy's Independence Steam Electric Station (ISES) and sorbent screening at MidAmerican's Council Bluffs Energy Center (CBEC) (subsequently renamed Walter Scott Energy Center (WSEC)). Detailed results for Independence and Louisa are presented in the respective Topical Reports. As no full-scale testing was conducted at CBEC, screening updates were provided in the quarterly updates to DOE. ADA-ES, Inc., with support from DOE/NETL, EPRI, and other industry partners, has conducted evaluations of EPRI's TOXECON II{trademark} process and of high-temperature reagents and sorbents to determine the capabilities of sorbent/reagent injection, including activated carbon, for mercury control on different coals and air emissions control equipment configurations. An overview of each plant configuration is presented: (1) MidAmerican's Louisa Generating Station burns Powder River Basin (PRB) coal in its 700-MW Unit 1 and employs hot-side electrostatic precipitators (ESPs) with flue gas conditioning for particulate control. This part of the testing program evaluated the effect of reagents used in the existing flue gas conditioning on mercury removal. (2) MidAmerican's Council Bluffs Energy Center typically burns PRB coal in its 88-MW Unit 2. It employs a hot-side ESP for particulate control. Solid sorbents were screened for hot-side injection. (3) Entergy's Independence Steam Electric Station typically burns PRB coal in its 880-MW Unit 2. Various sorbent injection tests were conducted on 1/8 to 1/32 of the flue gas stream either within or in front of one of four ESP boxes (SCA = 542 ft{sup 2}/kacfm), specifically ESP B. Initial mercury control evaluations indicated that although significant mercury control could be achieved by using the TOXECON II{trademark} design, the sorbent concentration required was higher than expected, possibly due to poor sorbent distribution. Subsequently, the original injection grid design was modeled and the results revealed that the sorbent distribution pattern was determined by the grid design, fluctuations in flue gas flow rates, and the structure of the ESP box. To improve sorbent distribution, the injection grid and delivery system were redesigned and the effectiveness of the redesigned system was evaluated. This project was funded through the DOE/NETL Innovations for Existing Plants program. It was a Phase II project with the goal of developing mercury control technologies that can achieve 50-70% mercury capture at costs 25-50% less than baseline estimates of $50,000-$70,000/lb of mercury removed. Results from testing at Independence indicate that the DOE goal was successfully achieved. Further improvements in the process are recommended, however. Results from testing at Louisa indicate that the DOE goal was not achievable using the tested high-temperature sorbent. Sorbent screening at Council Bluffs also indicated that traditional solid sorbents may not achieve significant mercury removal in hot-side applications.

Sharon Sjostrom

2008-02-09T23:59:59.000Z

456

Data:B00a67c6-dbd5-4e91-a5de-2728c7ae9dab | Open Energy Information  

Open Energy Info (EERE)

c6-dbd5-4e91-a5de-2728c7ae9dab c6-dbd5-4e91-a5de-2728c7ae9dab No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 100W HPS MP SU2 Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

457

Data:A02a9522-30f8-46d8-8697-ba8e02daa117 | Open Energy Information  

Open Energy Info (EERE)

2-30f8-46d8-8697-ba8e02daa117 2-30f8-46d8-8697-ba8e02daa117 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 100W HPS MP Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

458

Data:B5d62fba-63cd-4400-8206-52426695fab1 | Open Energy Information  

Open Energy Info (EERE)

fba-63cd-4400-8206-52426695fab1 fba-63cd-4400-8206-52426695fab1 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W MV - Billed Use Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >>

459

Data:9d92dafb-3cc4-4457-bfb2-e76608bbe8d3 | Open Energy Information  

Open Energy Info (EERE)

dafb-3cc4-4457-bfb2-e76608bbe8d3 dafb-3cc4-4457-bfb2-e76608bbe8d3 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 100W HPS SR2 Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

460

Data:3ae481f4-b1a1-425a-bcbd-e23bc3ea577c | Open Energy Information  

Open Energy Info (EERE)

f4-b1a1-425a-bcbd-e23bc3ea577c f4-b1a1-425a-bcbd-e23bc3ea577c No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: MidAmerican Energy Co Effective date: 2006/03/06 End date if known: Rate name: Private Lighting - North - 1000W MV Sector: Lighting Description: Source or reference: www.midamericanenergy.com/include/pdf/ Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months): Energy (kWh) Minimum (kWh): Maximum (kWh): History (months): Service Voltage Minimum (V): Maximum (V): Character of Service Voltage Category: Phase Wiring: << Previous 1 2 3 Next >> << Previous

Note: This page contains sample records for the topic "mason ia midamerican" 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

 

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

Type Ia Supernovae as Distance Indicators Type Ia Supernovae as Distance Indicators Brian Hayden ND/LBNL Abstract: Type Ia supernovae are remarkable for their use as distance indicators, yet a coherent physical explosion mechanism continues to elude us. In this talk, I will discuss my dissertation, which addresses many areas of contemporary SN Ia physics. I present a new light curve fitting technique, called "2-stretch", which demonstrates the diversity in SN Ia light curve shapes. 2-stretch also has implications when estimating the amount of nickel-56 produced in the explosion, which powers the light curve through radioactive decay. I will present a direct search for SN Ia companion stars. Using the SDSS-II dataset, I am able to constrain possible progenitor models in the single degenerate channel, where a type Ia

462

Document3  

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

18, 2013 18, 2013 Center Spotlight: Hampton & George Mason Universities/College of William & Mary (Virginia Center) For ideas on how to maintain a geographically diverse center, contact lead teacher Deborah Roudebush. The Hampton University QuarkNet Center began in 2000. Now, the center incorporates two other research institutions. Teachers are spread in an arc from southeast northern Virginia. Teachers reached out to Josh Erlich at the College of William and Mary and Phil Rubin of George Mason University for assistance. Both have joined Vassilis Vassilikopoulos of Hampton as mentors. The center has 10 active teachers. Four teachers actively share leadership. They split up workshop topics creating a strong cosmic ray detector program and offering three different masterclass institutes. One was held at

463

EIS-0456: EPA Notice of Availability of the Final Environmental Impact  

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

EPA Notice of Availability of the Final Environmental EPA Notice of Availability of the Final Environmental Impact Statement EIS-0456: EPA Notice of Availability of the Final Environmental Impact Statement Cushman Hydroelectric Project (FERC No. 0456) Notice of Availability for the Final Environmental Impact Statement for the Cushman Hydroelectric Project (FERC No. 0456), Design and Construction of New 3.6-MW Powerhouse on the North Fork of the Skokomish River, Mason County, Washington. Notice of Availability for the Final Environmental Impact Statement Cushman Hydroelectric Project (FERC No. 0456), Design and Construction of New 3.6-MW Powerhouse on the North Fork of the Skokomish River, Mason County, Washington, DOE/EIS-0456 (October 2010 - 75 FR 62386) More Documents & Publications EIS-0409: EPA Notice of Availability of the Final Environmental Impact

464

EIS-0456: EPA Notice of Availability of the Final Environmental Impact  

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

456: EPA Notice of Availability of the Final Environmental 456: EPA Notice of Availability of the Final Environmental Impact Statement EIS-0456: EPA Notice of Availability of the Final Environmental Impact Statement Cushman Hydroelectric Project (FERC No. 0456) Notice of Availability for the Final Environmental Impact Statement for the Cushman Hydroelectric Project (FERC No. 0456), Design and Construction of New 3.6-MW Powerhouse on the North Fork of the Skokomish River, Mason County, Washington. Notice of Availability for the Final Environmental Impact Statement Cushman Hydroelectric Project (FERC No. 0456), Design and Construction of New 3.6-MW Powerhouse on the North Fork of the Skokomish River, Mason County, Washington, DOE/EIS-0456 (October 2010 - 75 FR 62386) More Documents & Publications EIS-0409: EPA Notice of Availability of the Final Environmental Impact

465

 

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

Media Relations Media Relations Communications 865.576.1946 Bredesen Dedicates Joint Research Facility at Oak Ridge National Laboratory An appreciative ORNL Director Thom Mason (left) and University of Tennessee Interim President Jan Simek (right) wish Gov. Phil Bredesen well at the dedication of the UT-ORNL Joint Institute for Neutron Sciences. An appreciative ORNL Director Thom Mason (left) and University of Tennessee Interim President Jan Simek (right) wish Gov. Phil Bredesen well at the dedication of the UT-ORNL Joint Institute for Neutron Sciences. (hi-res image) OAK RIDGE, Tenn., Dec. 3, 2010 - Governor Phil Bredesen today joined officials from the University of Tennessee and the Department of Energy in dedicating a new state-funded research facility at Oak Ridge National

466

Microsoft PowerPoint - NERC Reliability Standards and Mandatory Compliance Presentation to Hydro-Power Conference - June 2007.p  

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

NERC Reliability NERC Reliability NERC Reliability NERC Reliability Standards and Standards and Mandatory Compliance Mandatory Compliance Hydro Hydro - - Power Conference Power Conference June 13, 2007 June 13, 2007 Stan Mason Stan Mason 2 EPACT 2005 EPACT 2005 Congress approved the related legislation Congress approved the related legislation in August 2005 in August 2005 It required creation of an Electric It required creation of an Electric Reliability Organization (ERO) to be Reliability Organization (ERO) to be approved by the Federal Energy approved by the Federal Energy Regulatory Commission (FERC) Regulatory Commission (FERC) It mandated Standards that would be It mandated Standards that would be approved by FERC with financial sanctions approved by FERC with financial sanctions

467

Los Alamos director echoes cyber concerns  

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

Los Alamos director echoes cyber concerns Los Alamos director echoes cyber concerns Los Alamos director echoes cyber concerns Director Charlie McMillan told a gathering of energy executives that securing the electrical grid is a major concern now and it's only becoming more serious. May 21, 2013 Los Alamos National Laboratory Director Charlie McMillan (right), with, from left, Anthony Cugini of the National Energy Technology Laboratory, Thom Mason of Oak Ridge National Laboratory, and Tomas Diaz de la Rubia of Deloitte Consulting LLP. Los Alamos National Laboratory Director Charlie McMillan (right), with, from left, Anthony Cugini of the National Energy Technology Laboratory, Thom Mason of Oak Ridge National Laboratory, and Tomas Diaz de la Rubia of Deloitte Consulting LLP. Contact Fred deSousa

468

Role of nanoscale AlN and InN for the microwave characteristics of AlGaN/(Al,In)N/GaN-based HEMT  

Science Conference Proceedings (OSTI)

A new AlGaN/GaN-based high electron mobility transistor (HEMT) is proposed and its micro-wave characteristics are discussed by introducing a nanoscale AlN or InN layer to study the potential improvement in their high frequency performance. The 2DEG transport mechanism including various sub-band calculations for both (Al,In) N-based HEMTs are also discussed in the paper. Apart from direct current characteristics of the proposed HEMT, various microwave parameters such as transconductance, unit current gain (h{sub 21} = 1) cut-off frequency (f{sub t}), high power-gain frequency (f{sub max}). Masons available/stable gain and masons unilateral gain are also discussed for both devices to understand its suitable deployment in microwave frequency range.

Lenka, T. R., E-mail: trlenka@gmail.com; Panda, A. K., E-mail: akpanda62@hotmail.com [National Institute of Science and Technology (India)

2011-09-15T23:59:59.000Z

469

Enforcement Letter - Evaluation of Deficiencies Operational Emergency at Building 6000, Holifield Radioactive Ion Beam Facility, Oak Ridge National Laboratory  

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

3,2009 3,2009 Dr. Thom Mason President and CEO UT-Battelle Oak Ridge National Laboratory P.O. Box 2008 Oak Ridge, Tennessee 37831-6255 Dear Dr. Mason: The Department of Energy's Office of Enforcement within the Office of Health, Safety and Security has conducted an evaluation of the deficiencies described in Noncompliance Tracking System (NTS) report NTS-ORO--0RNL-XlOPHYSICS-2008-0001, Operational Emergency at Building 6000, Holzfield Radioactive Ion Beam Facility. Our evaluation included a review of the Oak Ridge National Laboratory (ORNL) Management Investigation Team Report dated November 19,2008, the associated corrective action plan, and discussions with site personnel. The subject NTS report described a series of deficiencies at the Holifield Radioactive Ion

470

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

471

Enforcement Documents - Pantex Plant | Department of Energy  

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

Pantex Plant Pantex Plant Enforcement Documents - Pantex Plant January 7, 2013 Enforcement Letter, NEL-2013-01 Issued to B&W Pantex, LLC related to the Conduct of Nuclear Explosive Operations at the Pantex Plant November 21, 2006 Preliminary Notice of Violation, BWXT Pantex, LLC - EA-2006-04 Issued to BWXT Pantex, LLC, related to Quality Assurance and Safety Basis Requirements Violations at the Pantex Plant May 16, 2005 Preliminary Notice of Violation, BWXT Pantex LLC - EA-2005-02 Preliminary Notice of Violation issued to BWXT Pantex LLC, related to High Explosive Cracking during Weapon Disassembly at the Pantex Plant June 21, 2000 Consent Order, Mason & Hanger Corporation - EA-2000-07 Price-Anderson Enforcement Consent Order issued to Mason & Hanger Corporation related to Fire Suppression System Issues at the Pantex Plant,

472

 

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

Parting Shots Parting Shots e-tracer 79 Bob Larsen Above, Argonne researcher Geoffrey Amann prepares the E-Tracer 79 for testing at the laboratory's APRF. In August 2010, APRF researchers provided validation testing for the finalists in Progressive Insurance's Automotive X Prize Competition to determine they met the competition's goals for performance and efficiency targets. Larger image. Above, Argonne researcher Bob Larsen explains the Green Racing Simulator to budding young drivers. Photo courtesy of American LeMans Series. Larger image. Oyelayo Ajayi (left) and Ashley Masoner Above, Argonne tribology scientist Oyelayo Ajayi (left) and research aide Ashley Masoner use a block-on-ring test machine to study a type of engine and drivetrain failure, known as scuffing or galling, which occurs under severe contact at high loads and speeds. Larger image.

473

 

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

2 2 SHARE Media Contact: Media Relations Communications 865.576.1946 Team UT-Battelle builds a home to help ADFAC mark 25 years of service Carly Gilbert cuts the ribbon on her new home in Oak Ridge, constructed for Aid to Distressed Families of Appalachian Counties by volunteers from Oak Ridge National Laboratory's Team UT-Battelle. Looking on are Lab Director Thom Mason, right, and ADFAC board member Darrell Daugherty, center. Carly Gilbert cuts the ribbon on her new home in Oak Ridge, constructed for Aid to Distressed Families of Appalachian Counties by volunteers from Oak Ridge National Laboratory's Team UT-Battelle. Looking on are Lab Director Thom Mason, right, and ADFAC board member Darrell Daugherty, center. (hi-res image) Listen to the audio OAK RIDGE, Tenn., Aug. 31, 2012 - Oak Ridge National Laboratory Director

474

News & Events | ORNL Neutron Sciences  

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

7 News 7 News SNS News Archive-2007 December November October September August July June May March February January Because some media sources archive past articles and require a subscription for access, some of the links below might not be active. If a citation listed here is no longer available, please contact the newspaper or your library directly. December ORNL could feel squeeze Knoxville News Sentinel, 12/29 The 2008 budget bill belatedly passed by Congress last week will have some negative impacts on Oak Ridge National Laboratory because of cuts in the U.S. Department of Energy's science funding. However, the lab should be OK in most research areas, according to ORNL Director Thom Mason. "We're in reasonably good shape," Mason said in a recent interview at the

475

Renewable Fuels Consulting | Open Energy Information  

Open Energy Info (EERE)

Consulting Consulting Jump to: navigation, search Name Renewable Fuels Consulting Place Mason City, Iowa Sector Renewable Energy Product RFC specializes in providing technical solutions to renewable energy production plants. References Renewable Fuels Consulting[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Renewable Fuels Consulting is a company located in Mason City, Iowa . References ↑ "Renewable Fuels Consulting" Retrieved from "http://en.openei.org/w/index.php?title=Renewable_Fuels_Consulting&oldid=350341" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link

476

EIS-0445: American Electric Power Service Corporation's Mountaineer  

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

5: American Electric Power Service Corporation's Mountaineer 5: American Electric Power Service Corporation's Mountaineer Commercial Scale Carbon Capture and Storage Demonstration, New Haven, Mason County, West Virginia EIS-0445: American Electric Power Service Corporation's Mountaineer Commercial Scale Carbon Capture and Storage Demonstration, New Haven, Mason County, West Virginia Summary This EIS evaluates the environmental impacts of a proposal to provide financial assistance for the construction and operation of a project proposed by American Electric Power Service Corporation (AEP). DOE selected tbis project for an award of financial assistance through a competitive process under the Clean Coal Power Initiative (CCPI) Program. AEP's Mountaineer Commercial Scale Carbon Capture and Storage Project (Mountaineer CCS II Project) would construct a commercial scale

477

Preliminary Notice of Violation EA 97-02  

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

5, 1997 5, 1997 W. A. Weinreich [ ] Mason and Hanger Corporation Pantex Plant P. O. Box 30020 Amarillo, Texas 79120-0020 EA 97-02 Subject: Preliminary Notice of Violation (NTS-ALO-AO-MHSM-PANTEX-1996-0008) Dear Mr. Weinreich: This letter refers to the Department of Energy's (DOE) evaluation of alleged irregularities associated with training requirements for Production Technicians who performed work in the W55 nuclear weapons dismantlement program in [building]. The DOE Office of Enforcement and Investigation initiated its inquiry on December 4, 1996, after several workers communicated concerns to the DOE Amarillo Area Office regarding the accuracy of weapon work proficiency records. The DOE's Investigation Summary Report is enclosed. After the concerns were raised to DOE, Mason and Hanger Corporation began an

478

EIS-0445: Notice of Cancellation of an Environmental Impact Statement |  

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

445: Notice of Cancellation of an Environmental Impact 445: Notice of Cancellation of an Environmental Impact Statement EIS-0445: Notice of Cancellation of an Environmental Impact Statement Mountaineer Commercial Scale Carbon Capture and Storage Project, Mason County, WV The Office of Fossil Energy is cancelling the EIS for the Mountaineer Commercial Scale Carbon Capture and Storage Project in Mason County, WV (DOE/EIS-0445). DOE selected this project proposed by American Electric Power (AEP) under the Round 3 solicitation of the Clean Coal Power Initiative. DOE's proposed action was to provide $334 million in cost-shared financial assistance to AEP to support the construction and operation of AEP's proposed project. The cooperative agreement was terminated at the end of phase 1. EIS-0445-DEIS-NoticeofCancellation-2012.pdf

479

Microsoft Word - Peninsula_Light_Co_L0308_Mod_CX_and_EnvCkLt.doc  

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

3 3 REPLY TO ATTN OF: KEC-4 SUBJECT: Environmental Clearance Memorandum Chad Hamel, Project Manager, TEP-TPP-1 Proposed Action: Peninsula Light Company Line and Load Interconnection Request L0308 (amendment to previous Categorical Exclusion issued on May 5, 2011) Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B4.12 Construction of powerlines Location: Mason County, WA Proposed by: Bonneville Power Administration (BPA) Description of the Proposed Action: BPA proposes a modification to a tap line that would interconnect Peninsula Light Company (PLC) into BPA's Shelton-Kitsap #2 115-kV transmission line in Mason County, WA. The original proposal involved constructing the tap within existing BPA right-of-way (ROW), as described in the categorical exclusion issued

480

Solid phase microextraction analysis of B83 SLTS and Core B compatibility test units  

SciTech Connect

Solid phase microextraction has permitted the efficient collection and analysis of a broad range of volatile and semivolatile compounds outgassed from materials. In 1998, we implemented a microextraction protocol at Mason and Hanger, Pantex Plant, for the analysis of weapons and compatibility test units. The chemical information that was obtained from this work is interpreted by determining the source and outgas mechanism for each compound in the weapon signature, which is a task only accomplished by analysis of material standards.

Chambers, D M; Ithaca, J; King, H A; Malcolm, S

1999-03-26T23:59:59.000Z

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481

STRIPES TEMPLATE  

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

STRIPES TEMPLATE STRIPES TEMPLATE IA Part A - Page 1 of 5 Interagency Agreement (IA) Part A - General Terms and Conditions Prescription: Part A: When DOE is the Requesting Agency for an Interagency Agreement (IA), the DOE Contracting Officer will complete IA Part A, General Terms and Conditions. It will be necessary for the Contracting Officer to coordinate with the program office and the Servicing Agency for completion of IA Part A. Part B: When the Program Office prepares and submits the requisition, the Program Office will prepare Part B with the assistance of the Servicing Agency and the Contracting Officer, as needed. Part B will be an attachment to the requisition. The DOE Contracting Officer and the DOE Budget Office will review IA Part

482

Abstract for David Chamulak  

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

Michigan State University, East Lansing, MI Michigan State University, East Lansing, MI The Effect of Ne-22 on the Thermonuclear Processes in White Dwarf Supernovae Type Ia supernovae (SNe Ia) are among the most luminous events in the universe. A single SN Ia at maximum light is as bright as its host galaxy. This property along with the ability to calibrate their light curves has made SNe Ia the premier standard candle for measuring cosmological distances. SNe Ia have recently been found to fall into two populations, a "prompt", and a "tardy" type. The "prompt" type supernovae have been observed to be on average brighter then their "tardy" relatives. It is currently unknown what causes the dispersion in the brightness of SNe Ia, but one idea could be the composition of the progenitor star. Ne-22 is the

483

STRIPES TEMPLATE  

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

STRIPES TEMPLATE STRIPES TEMPLATE IA Part A - Page 1 of 5 Interagency Agreement (IA) Part A - General Terms and Conditions Prescription: Part A: When DOE is the Requesting Agency for an Interagency Agreement (IA), the DOE Contracting Officer will complete IA Part A, General Terms and Conditions. It will be necessary for the Contracting Officer to coordinate with the program office and the Servicing Agency for completion of IA Part A. Part B: When the Program Office prepares and submits the requisition, the Program Office will prepare Part B with the assistance of the Servicing Agency and the Contracting Officer, as needed. Part B will be an attachment to the requisition. The DOE Contracting Officer and the DOE Budget Office will review IA Part