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Sample records for mun elec sys

  1. Virginia Mun Elec Assn No 1 | Open Energy Information

    Open Energy Info (EERE)

    Elec Assn No 1 Jump to: navigation, search Name: Virginia Mun Elec Assn No 1 Place: Virginia Website: www.mepav.org References: EIA Form EIA-861 Final Data File for 2010 -...

  2. Utah Associated Mun Power Sys | Open Energy Information

    Open Energy Info (EERE)

    Generation Yes Activity Transmission Yes Activity Buying Transmission Yes Activity Wholesale Marketing Yes This article is a stub. You can help OpenEI by expanding it. Utility...

  3. Massachusetts Mun Wholes Electric Co | Open Energy Information

    Open Energy Info (EERE)

    Massachusetts Mun Wholes Electric Co Jump to: navigation, search Name: Massachusetts Mun Wholes Electric Co Place: Massachusetts Phone Number: (413) 589-0141 Website:...

  4. Choctawhatche Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Choctawhatche Elec Coop, Inc Jump to: navigation, search Name: Choctawhatche Elec Coop, Inc Place: Florida Phone Number: (850) 892-2111 Website: www.chelco.com Twitter: https:...

  5. Withlacoochee River Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Withlacoochee River Elec Coop Jump to: navigation, search Name: Withlacoochee River Elec Coop Place: Florida Phone Number: 352-567-5133 Website: www.wrec.net Twitter: https:...

  6. Weatherford Mun Utility System | Open Energy Information

    Open Energy Info (EERE)

    Weatherford Mun Utility System Place: Texas Phone Number: 817-598-4257 Website: www.ci.weatherford.tx.usindex Outage Hotline: 817-598-4257 References: EIA Form EIA-861 Final...

  7. Washington Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    Washington Elec Member Corp Jump to: navigation, search Name: Washington Elec Member Corp Place: Georgia Phone Number: 478-552-2577; 1-800-552-2577 Website: washingtonemc.com...

  8. Intermountain Rural Elec Assn | Open Energy Information

    Open Energy Info (EERE)

    Rural Elec Assn Place: Colorado Website: www.irea.coop Twitter: @IREAColorado Facebook: https:www.facebook.comIntermountainREA Outage Hotline: 1-800-332-9540 References:...

  9. Public Service Elec & Gas Co | Open Energy Information

    Open Energy Info (EERE)

    Elec & Gas Co (Redirected from PSEG) Jump to: navigation, search Name: Public Service Elec & Gas Co Abbreviation: PSEG Place: New Jersey Year Founded: 1903 Phone Number:...

  10. Mountrail-Williams Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Mountrail-Williams Elec Coop Jump to: navigation, search Name: Mountrail-Williams Elec Coop Place: North Dakota Phone Number: Williston Office- 701-577-3765 -- Stanley Office-...

  11. Hess Retail Natural Gas and Elec. Acctg. (Delaware) | Open Energy...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. (Delaware) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Delaware References: EIA Form EIA-861 Final...

  12. Hess Retail Natural Gas and Elec. Acctg. (Connecticut) | Open...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. (Connecticut) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Connecticut Phone Number: 212-997-8500...

  13. Hess Retail Natural Gas and Elec. Acctg. (District of Columbia...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. (District of Columbia) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: District of Columbia References:...

  14. Clinton Combined Utility Sys | Open Energy Information

    Open Energy Info (EERE)

    Clinton Combined Utility Sys Jump to: navigation, search Name: Clinton Combined Utility Sys Place: South Carolina Phone Number: 864-833-7524 Website: www.cityofclintonsc.com...

  15. Northern Virginia Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    NOVEC) Jump to: navigation, search Name: Northern Virginia Elec Coop Place: Manassas, Virginia References: EIA Form EIA-861 Final Data File for 2010 - File1a1 SGIC2 EIA Form...

  16. Northern Virginia Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Northern Virginia Elec Coop Place: Manassas, Virginia References: EIA Form EIA-861 Final Data File for 2010 - File1a1 SGIC2 EIA Form 861 Data Utility Id 13640 Utility Location...

  17. Upson Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    Name: Upson Elec Member Corp Place: Georgia Website: www.upsonemc.comUpson%20EMC%2 Facebook: https:www.facebook.comupson.emc Outage Hotline: 706-647-5475 References: EIA...

  18. Copper Valley Elec Assn, Inc | Open Energy Information

    Open Energy Info (EERE)

    Valley Elec Assn, Inc Jump to: navigation, search Name: Copper Valley Elec Assn, Inc Place: Alaska Phone Number: Copper Basin: 907-822-3211 or Valdez: 907-835-4301 Website:...

  19. Public Service Elec & Gas Co | Open Energy Information

    Open Energy Info (EERE)

    Elec & Gas Co Jump to: navigation, search Name: Public Service Elec & Gas Co Abbreviation: PSEG Place: New Jersey Year Founded: 1903 Phone Number: 1-800-436-7734 Website:...

  20. Central Hudson Gas & Elec Corp | Open Energy Information

    Open Energy Info (EERE)

    Gas & Elec Corp Jump to: navigation, search Name: Central Hudson Gas & Elec Corp Place: New York Phone Number: 845-452-2700 or 1-800-527-2714 Website: www.centralhudson.com...

  1. New England Hydro-Tran Elec Co | Open Energy Information

    Open Energy Info (EERE)

    New England Hydro-Tran Elec Co Jump to: navigation, search Name: New England Hydro-Tran Elec Co Place: Massachusetts Phone Number: 860 729 9767 Website: www.nehydropower.com...

  2. Big Horn County Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    County Elec Coop, Inc Jump to: navigation, search Name: Big Horn County Elec Coop, Inc Place: Montana Phone Number: (406) 665-2830 Website: www.bhcec.com Outage Hotline: (406)...

  3. Wayne-White Counties Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Wayne-White Counties Elec Coop Jump to: navigation, search Name: Wayne-White Counties Elec Coop Place: Illinois Phone Number: (618) 842-2196 Website: waynewhitecoop.com Facebook:...

  4. Deep East Texas Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Deep East Texas Elec Coop Inc Jump to: navigation, search Name: Deep East Texas Elec Coop Inc Place: Texas Phone Number: 1-800-392-5986 Website: www.deepeast.com Facebook: https:...

  5. Joe Wheeler Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    Joe Wheeler Elec Member Corp Jump to: navigation, search Name: Joe Wheeler Elec Member Corp Place: Alabama Phone Number: (256) 552-2300 Website: www.jwemc.org Twitter: @jwemc...

  6. Mora-San Miguel Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Mora-San Miguel Elec Coop, Inc Jump to: navigation, search Name: Mora-San Miguel Elec Coop, Inc Place: New Mexico Phone Number: 575-387-2205 (Mora) -- 505-757-6490 (Pecos) Website:...

  7. HHH FEC Cooperation Mach Elec Co Ltd | Open Energy Information

    Open Energy Info (EERE)

    HHH FEC Cooperation Mach Elec Co Ltd Jump to: navigation, search Name: HHH-FEC Cooperation Mach.&Elec. Co., Ltd Place: Weihai, Shanghai Municipality, China Zip: 264209 Sector:...

  8. Brown County Rural Elec Assn | Open Energy Information

    Open Energy Info (EERE)

    Rural Elec Assn Jump to: navigation, search Name: Brown County Rural Elec Assn Place: Minnesota Phone Number: 1-800-658-2368 Website: www.browncountyrea.coop Outage Hotline:...

  9. East End Mutual Elec Co Ltd | Open Energy Information

    Open Energy Info (EERE)

    End Mutual Elec Co Ltd Jump to: navigation, search Name: East End Mutual Elec Co Ltd Place: Idaho Phone Number: (208) 436-9357 Website: www.electricunion.orgcompany- Outage...

  10. Harrison County Rrl Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Harrison County Rrl Elec Coop Jump to: navigation, search Name: Harrison County Rrl Elec Coop Place: Iowa Phone Number: 712-647-2727 Website: www.hcrec.coop Outage Hotline:...

  11. Harrison Rural Elec Assn, Inc | Open Energy Information

    Open Energy Info (EERE)

    Harrison Rural Elec Assn, Inc Jump to: navigation, search Name: Harrison Rural Elec Assn, Inc Place: West Virginia Phone Number: 304.624.6365 Website: www.harrisonrea.com...

  12. Panola-Harrison Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Panola-Harrison Elec Coop, Inc Jump to: navigation, search Name: Panola-Harrison Elec Coop, Inc Place: Texas Phone Number: (903) 935-7936 Website: www.phec.us Facebook: https:...

  13. Clearwater-Polk Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Clearwater-Polk Elec Coop Inc Jump to: navigation, search Name: Clearwater-Polk Elec Coop Inc Place: Minnesota Phone Number: 218-694-6241 Website: www.clearwater-polk.com Outage...

  14. Barrow Utils & Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Utils & Elec Coop, Inc Jump to: navigation, search Name: Barrow Utils & Elec Coop, Inc Place: Alaska Phone Number: 907-852-6166 Website: www.bueci.org Outage Hotline: After Hours:...

  15. Nelson Lagoon Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Lagoon Elec Coop Inc Jump to: navigation, search Name: Nelson Lagoon Elec Coop Inc Place: Alaska Phone Number: (907) 989-2204 Website: www.swamc.orghtmlsouthwest-a Outage...

  16. Red River Valley Rrl Elec Assn | Open Energy Information

    Open Energy Info (EERE)

    Elec Assn Jump to: navigation, search Name: Red River Valley Rrl Elec Assn Place: Oklahoma Phone Number: 1-800-749-3364 or 580-564-1800 Website: www.rrvrea.com Twitter:...

  17. South River Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    River Elec Member Corp Jump to: navigation, search Name: South River Elec Member Corp Place: North Carolina Phone Number: (910) 892-8071 Website: www.sremc.com Twitter: https:...

  18. Cavalier Rural Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Rural Elec Coop, Inc Jump to: navigation, search Name: Cavalier Rural Elec Coop, Inc Place: North Dakota Phone Number: 701-256-5511 Facebook: https:www.facebook.compages...

  19. Hess Retail Natural Gas and Elec. Acctg. (Maine) | Open Energy...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. (Maine) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Maine Phone Number: 1-800-437-7645 Website:...

  20. Sioux Valley SW Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    SW Elec Coop Jump to: navigation, search Name: Sioux Valley SW Elec Coop Place: Colman, South Dakota References: EIA Form EIA-861 Final Data File for 2010 - File1a1 SGIC2 EIA...

  1. Rich Mountain Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Rich Mountain Elec Coop, Inc Jump to: navigation, search Name: Rich Mountain Elec Coop, Inc Place: Arkansas Phone Number: 1-877-828-4074 Website: www.rmec.com Outage Hotline:...

  2. Tipmont Rural Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    search Name: Tipmont Rural Elec Member Corp Abbreviation: Tipmont REMC Address: 403 S Main St Place: Linden, Indiana Zip: 47955 Phone Number: 800-726-3953 Website:...

  3. Denton County Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    County Elec Coop, Inc Place: Texas Service Territory: Texas Website: www.coserv.com Outage Hotline: (800) 274-4014 Outage Map: outagemap.coserv.comexternal References: EIA...

  4. Hess Retail Natural Gas and Elec. Acctg. (Pennsylvania) | Open...

    Open Energy Info (EERE)

    Pennsylvania) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Pennsylvania References: EIA Form EIA-861 Final Data File for 2010 - File220101...

  5. AeroSys: Order (2011-SCE-1624)

    Office of Energy Efficiency and Renewable Energy (EERE)

    DOE ordered AeroSys, Inc. (AeroSys) to pay a $100,000 civil penalty after finding AeroSys had (1) failed to certify that certain models of space-constrained central air conditioners and air conditioning heat pumps comply with the applicable energy conservation standards; and (2) manufactured and distributed in commerce in the U.S. units of noncompliant models of space-constrained central air conditioners and air conditioning heat pumps.

  6. Southern Pine Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    search Name: Southern Pine Elec Coop, Inc Place: Alabama Phone Number: Atmore Office: 251.368.4842; Brewton Office: 251.867.5415; Evergreen Office: 251.578.3460; Frisco...

  7. East Mississippi Elec Pwr Assn | Open Energy Information

    Open Energy Info (EERE)

    search Name: East Mississippi Elec Pwr Assn Place: Mississippi Phone Number: Meridian Office: 601-581-8600 -- Quitman Office: 601-776-6271 -- DeKalb Office: 601-743-2641 --...

  8. South Louisiana Elec Coop Assn | Open Energy Information

    Open Energy Info (EERE)

    search Name: South Louisiana Elec Coop Assn Place: Louisiana Phone Number: Houma Office: (985) 876-6880 or Amelia Office: (985) 631-3605 Website: www.sleca.com Facebook:...

  9. New England Elec Transm'n Corp | Open Energy Information

    Open Energy Info (EERE)

    Transm'n Corp Jump to: navigation, search Name: New England Elec Transm'n Corp Place: New Hampshire References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form 861...

  10. North Central Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Central Elec Coop, Inc Place: Ohio Website: www.ncelec.org Twitter: @NorthCentralEC Facebook: https:www.facebook.comNorthCentralElectric Outage Hotline: 419-426-3072 ...

  11. Buckeye Rural Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Buckeye Rural Elec Coop, Inc Place: Ohio Website: www.buckeyerec.commain Facebook: https:www.facebook.combuckeyerec Outage Hotline: 1-800-282-7204 References: EIA Form EIA-861...

  12. Bailey County Elec Coop Assn | Open Energy Information

    Open Energy Info (EERE)

    Elec Coop Assn Place: Texas Phone Number: (806) 272-4504 Website: www.bcecoop.com Facebook: https:www.facebook.combcecoop Outage Hotline: (806) 272-4504 References: EIA Form...

  13. Comanche County Elec Coop Assn | Open Energy Information

    Open Energy Info (EERE)

    Comanche County Elec Coop Assn Place: Texas Website: www.ceca.coophome.aspx Facebook: https:www.facebook.comCECA.coop Outage Hotline: 1-800-915-2533 References: EIA Form...

  14. Delaware County Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Delaware County Elec Coop Inc Place: New York Phone Number: (607) 746-9283 or Toll Free at (866) 436-1223 Website: www.dce.coop Facebook: https:www.facebook.compages...

  15. Elec District No. 5 Maricopa C | Open Energy Information

    Open Energy Info (EERE)

    District No. 5 Maricopa C Jump to: navigation, search Name: Elec District No. 5 Maricopa C Place: Arizona Phone Number: (480) 610-8741 Outage Hotline: (480) 610-8741 References:...

  16. Raft River Rural Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Raft River Rural Elec Coop Inc Place: Idaho Service Territory: Idaho, Utah, Nevada Phone Number: 208-645-2211 Website: rrelectric.com Facebook: https:www.facebook.compages...

  17. Panola-Harrison Elec Coop, Inc (Louisiana) | Open Energy Information

    Open Energy Info (EERE)

    Louisiana) Jump to: navigation, search Name: Panola-Harrison Elec Coop, Inc Place: Louisiana Phone Number: (318) 933-5096 Outage Hotline: (318) 933-5096 References: EIA Form...

  18. Morgan County Rural Elec Assn | Open Energy Information

    Open Energy Info (EERE)

    search Name: Morgan County Rural Elec Assn Place: Colorado Website: www.mcrea.org Twitter: @MorganCountyREA Facebook: https:www.facebook.compagesMorgan-County-Rural-Ele...

  19. Heartland Rural Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Elec Coop, Inc Place: Kansas Phone Number: (800) 835-9586 Website: www.heartland-rec.com Twitter: @HeartlandREC Facebook: https:www.facebook.comHeartlandREC Outage Hotline:...

  20. Blue Ridge Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    Blue Ridge Elec Member Corp Place: North Carolina Phone Number: 1-800-448-2383 Website: www.blueridgeemc.com Twitter: @blueridgeemc Facebook: https:www.facebook.comBlueRidgeEMC...

  1. French Broad Elec Member Corp (Tennessee) | Open Energy Information

    Open Energy Info (EERE)

    French Broad Elec Member Corp Place: Tennessee Phone Number: (828)649-2051 or (828)688-4815 or (800)222-6190 or (828)682-6121 Website: www.frenchbroademc.com Twitter:...

  2. French Broad Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    French Broad Elec Member Corp Place: North Carolina Phone Number: (828)649-2051 or (828)688-4815 or (800)222-6190 or (828)682-6121 Website: www.frenchbroademc.com Twitter:...

  3. Central Valley Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Coop, Inc Jump to: navigation, search Name: Central Valley Elec Coop, Inc Place: New Mexico Phone Number: (575) 746-3571 Website: cvecoop.org Outage Hotline: (575) 746-3571...

  4. North Georgia Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    navigation, search Name: North Georgia Elec Member Corp Place: Georgia Phone Number: Dalton: (706) 259-9441; Fort Oglethorpe: (706) 866-2231; Calhoun: (706) 629-3160; Trion:...

  5. Oliver-Mercer Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Oliver-Mercer Elec Coop Inc Place: North Dakota References: Energy Information Administration.1 EIA Form 861 Data Utility Id 14088 This article is a stub. You can help OpenEI...

  6. Grundy County Rural Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Elec Coop Place: Iowa Phone Number: 319-824-5251 Website: www.grundycountyrecia.com Outage Hotline: 1-800-390-7605 Outage Map: www.iowarec.orgoutages References: EIA Form...

  7. Hess Retail Natural Gas and Elec. Acctg. (Maryland) | Open Energy...

    Open Energy Info (EERE)

    Maryland) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Maryland References: EIA Form EIA-861 Final Data File for 2010 - File220101 EIA Form...

  8. Hess Retail Natural Gas and Elec. Acctg. (Massachusetts) | Open...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. Place: Massachusetts Phone Number: 212-997-8500 Website: www.hess.com Twitter: @HessCorporation Facebook: https:www.facebook.com...

  9. Hess Retail Natural Gas and Elec. Acctg. (Rhode Island) | Open...

    Open Energy Info (EERE)

    Rhode Island) Jump to: navigation, search Name: Hess Retail Natural Gas and Elec. Acctg. Place: Rhode Island References: EIA Form EIA-861 Final Data File for 2010 - File220101...

  10. Hess Retail Natural Gas and Elec. Acctg. (New Hampshire) | Open...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. Place: New Hampshire Phone Number: 1-800-437-7645 Website: www.hess.com Twitter: @HessCorporation Facebook: https:www.facebook.com...

  11. Paulding-Putman Elec Coop, Inc (Indiana) | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search Name: Paulding-Putman Elec Coop, Inc Address: 401 McDonald Pike Place: Paulding, Ohio Zip: 45879-9270 Service Territory: Indiana, Ohio Phone Number:...

  12. Rich Mountain Elec Coop, Inc (Oklahoma) | Open Energy Information

    Open Energy Info (EERE)

    Inc (Oklahoma) Jump to: navigation, search Name: Rich Mountain Elec Coop, Inc Place: Oklahoma Phone Number: 1-877-828-4074 Website: www.rmec.com Outage Hotline: 1-877-828-4074...

  13. A Resource assessment protocol for GEO-ELEC | Open Energy Information

    Open Energy Info (EERE)

    Resource assessment protocol for GEO-ELEC Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: A Resource assessment protocol for GEO-ELEC Authors...

  14. Sam Rayburn G&T Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Sam Rayburn G&T Elec Coop Inc Jump to: navigation, search Name: Sam Rayburn G&T Elec Coop Inc Place: Texas Phone Number: (936) 560-9532 Outage Hotline: (936) 560-9532 References:...

  15. AeroSys: Test Notice (2009)

    Broader source: Energy.gov [DOE]

    DOE issued a test notice to AeroSys, Inc., requiring the company to provide sample units for laboratory testing to determine the compliance of various models of central air conditioners and air conditioning heat pumps with the applicable energy conservation standards.

  16. Bath Electric Gas & Water Sys | Open Energy Information

    Open Energy Info (EERE)

    Electric Gas & Water Sys Jump to: navigation, search Name: Bath Electric Gas & Water Sys Place: New York Phone Number: (607) 776-3072 Website: www.villageofbath.orgBEGWS.ht Outage...

  17. Steuben Rural Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Steuben Rural Elec Coop, Inc Place: New York Phone Number: 607-776-4161 or 800-843-3414 or 716-296-5651 or 800-883-8236 Website: www.steubenrec.coop Outage Hotline: 1-866-430-4293...

  18. AeroSysNNC_3-25.pdf | Department of Energy

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

    AeroSysNNC_3-25.pdf AeroSysNNC_3-25.pdf PDF icon AeroSysNNC_3-25.pdf More Documents & Publications AeroSys: Noncompliance Determination (2010-SE-0302) AeroSys: Test Notice (2009) AeroSys: Order (2010-CE-01/0201 and 2010-SE-0302)

  19. MHK Projects/Homeowner Tidal Power Elec Gen | Open Energy Information

    Open Energy Info (EERE)

    Homeowner Tidal Power Elec Gen < MHK Projects Jump to: navigation, search << Return to the MHK database homepage Loading map... "minzoom":false,"mappingservice":"googlemaps3","typ...

  20. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    Germany) Jump to: navigation, search Project Name AFTER A Framework for electrical power sysTems vulnerability identification, dEfense and Restoration Country Germany Coordinates...

  1. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    France) Jump to: navigation, search Project Name AFTER A Framework for electrical power sysTems vulnerability identification, dEfense and Restoration Country France Coordinates...

  2. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    United Kingdom) Jump to: navigation, search Project Name AFTER A Framework for electrical power sysTems vulnerability identification, dEfense and Restoration Country United Kingdom...

  3. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    Ireland) Jump to: navigation, search Project Name AFTER A Framework for electrical power sysTems vulnerability identification, dEfense and Restoration Country Ireland Coordinates...

  4. Department of Energy Announces Testing for AeroSys, Inc. Products...

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

    Testing for AeroSys, Inc. Products to Ensure Compliance with Appliance Standards Department of Energy Announces Testing for AeroSys, Inc. Products to Ensure Compliance with ...

  5. AeroSys: Noncompliance Determination (2010-SE-0302)

    Broader source: Energy.gov [DOE]

    DOE issued a Notice of Noncompliance Determination to AeroSys, Inc. finding that basic models THHP-24T* and THDC-30T* do not comport with the energy conservation standards.

  6. Department of Energy Subpoenas Compliance Data from AeroSys,...

    Office of Environmental Management (EM)

    country. "We are not prejudging the merits of this particular case, and we certainly hope that the response to this subpoena will reveal that the relevant AeroSys products fully...

  7. EnerSys GmbH | Open Energy Information

    Open Energy Info (EERE)

    GmbH Jump to: navigation, search Name: EnerSys GmbH Place: Bietigheim-Bissingen, Germany Zip: D-74321 Sector: Wind energy Product: Provides turnkey windfarm planning in...

  8. AeroSys: Proposed Penalty (2010-CE-01/0201)

    Broader source: Energy.gov [DOE]

    DOE alleged in a Notice of Proposed Civil Penalty that AeroSys, Inc. failed to certify residential central air conditioners and air conditioning heat pumps as compliant with the applicable energy conservation standards.

  9. Hess Retail Natural Gas and Elec. Acctg. (New York) | Open Energy...

    Open Energy Info (EERE)

    Hess Retail Natural Gas and Elec. Acctg. Place: New York References: EIA Form EIA-861 Final Data File for 2010 - File220101 EIA Form 861 Data Utility Id 22509 This article is a...

  10. GenSys Blue: Fuel Cell Heating Appliance | Department of Energy

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

    GenSys Blue: Fuel Cell Heating Appliance GenSys Blue: Fuel Cell Heating Appliance Presented at the High Temperature Membrane Working Group Meetng, Nov. 16, 2009. PDF icon ...

  11. DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner...

    Energy Savers [EERE]

    Orders AeroSys to Halt Distribution of Inefficient Air Conditioner and Heat Pump Models DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner and Heat Pump Models ...

  12. AeroSys: Noncompliance Determination (2010-SE-0302) | Department of Energy

    Energy Savers [EERE]

    Noncompliance Determination (2010-SE-0302) AeroSys: Noncompliance Determination (2010-SE-0302) April 13, 2010 DOE issued a Notice of Noncompliance Determination to AeroSys, Inc. finding that basic model THDC-24SG does not comport with the energy conservation standards. DOE determined the product was noncompliant based on DOE testing. AeroSys must immediately notify each person (or company) to whom AeroSys distributed the noncompliant product that the product does not meet Federal standards. In

  13. AeroSys: Order (2010-CE-01/0201 and 2010-SE-0302)

    Office of Energy Efficiency and Renewable Energy (EERE)

    DOE ordered AeroSys, Inc. to pay a $25,000 civil penalty after finding AeroSys had manufactured and distributed in commerce in the U.S. various models of air conditioners and air conditioning heat pumps that did not comport with the applicable energy conservation standards. In addition, AeroSys had distributed air conditioners and air conditioning heat pumps without submitting the required certification reports.

  14. AeroSys: Proposed Penalty (2011-SCE-1624) | Department of Energy

    Energy Savers [EERE]

    Proposed Penalty (2011-SCE-1624) AeroSys: Proposed Penalty (2011-SCE-1624) September 30, 2013 DOE alleged in an Amended Notice of Proposed Civil Penalty (NPCP) that AeroSys, Inc. failed to certify various basic models of space-constrained central air conditioners and air conditioning heat pumps as compliant with the applicable energy conservation standards. DOE also alleged in the NPCP that AeroSys, Inc. manufactured and distributed in the U.S. noncompliant space-constrained central air

  15. DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner and

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

    Heat Pump Models Shown to Violate Minimum Efficiency Standards | Department of Energy AeroSys to Halt Distribution of Inefficient Air Conditioner and Heat Pump Models Shown to Violate Minimum Efficiency Standards DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner and Heat Pump Models Shown to Violate Minimum Efficiency Standards March 30, 2010 - 12:00am Addthis WASHINGTON, DC - Today, the Department of Energy announced that it is requiring AeroSys, Inc. to stop

  16. Department of Energy Announces Testing for AeroSys, Inc. Products to Ensure

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

    Compliance with Appliance Standards | Department of Energy Testing for AeroSys, Inc. Products to Ensure Compliance with Appliance Standards Department of Energy Announces Testing for AeroSys, Inc. Products to Ensure Compliance with Appliance Standards September 24, 2009 - 12:00am Addthis Washington, DC - As part of its renewed efforts to ensure compliance with national energy efficiency appliance standards, the U.S. Department of Energy today issued a test notice requiring AeroSys, Inc. to

  17. EnerSys Motive Power Hawker formerly Energy Storage Group ESG...

    Open Energy Info (EERE)

    Motive Power Hawker formerly Energy Storage Group ESG Jump to: navigation, search Name: EnerSys Motive Power (Hawker), formerly Energy Storage Group (ESG) Place: United Kingdom...

  18. NuCellSys GmbH formerly Ballard AG formerly XCellsis | Open Energy...

    Open Energy Info (EERE)

    Germany Product: Focused on developing and manufacturing fuel cell systems for automotive applications. References: NuCellSys GmbH (formerly Ballard AG, formerly XCellsis)1...

  19. The RenewElec Project: Variable Renewable Energy and the Power System

    SciTech Connect (OSTI)

    Apt, Jay

    2014-02-14

    Variable energy resources, such as wind power, now produce about 4% of U.S. electricity. They can play a significantly expanded role if the U.S. adopts a systems approach that considers affordability, security and reliability. Reaching a 20-30% renewable portfolio standard goal is possible, but not without changes in the management and regulation of the power system, including accurately assessing and preparing for the operational effects of renewable generation. The RenewElec project will help the nation make the transition to the use of significant amounts of electric generation from variable and intermittent sources of renewable power.

  20. DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner and Heat Pump Models

    Broader source: Energy.gov [DOE]

    Today, the Department of Energy announced that it is requiring AeroSys, Inc. to stop distributing two product models - one air conditioner and one heat pump - that DOE testing found to consume more...

  1. AeroSys: Noncompliance Determination (2010-CE-01/0201 and 2010-SE-0302)

    Broader source: Energy.gov [DOE]

    DOE issued a Notice of Noncompliance Determination to AeroSys, Inc. finding that basic models THDC-18S, THDC-18T, THDC-24S, and THDC-24T do not comport with the energy conservation standards.

  2. DOE Institutes Enforcement Action Against AeroSys, Inc. for Failure...

    Office of Environmental Management (EM)

    to Certify Air Conditioners and Heat Pumps DOE Institutes Enforcement Action Against AeroSys, Inc. for Failure to Certify Air Conditioners and Heat Pumps February 4, 2010 - 1:58pm ...

  3. DOE Orders AeroSys to Halt Distribution of Inefficient Air Conditioner...

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

    ... Enforcement Action Against AeroSys, Inc. for Failure to Certify Air Conditioners and Heat Pumps Aerosys Agrees to Pay Civil Penalty and Submit Test Data in Settlement with DOE

  4. Process for selecting engineering tools : applied to selecting a SysML tool.

    SciTech Connect (OSTI)

    De Spain, Mark J.; Post, Debra S.; Taylor, Jeffrey L.; De Jong, Kent

    2011-02-01

    Process for Selecting Engineering Tools outlines the process and tools used to select a SysML (Systems Modeling Language) tool. The process is general in nature and users could use the process to select most engineering tools and software applications.

  5. DOE Institutes Enforcement Action Against AeroSys, Inc. for Failure to Certify Air Conditioners and Heat Pumps

    Broader source: Energy.gov [DOE]

    Washington, DC - The Department of Energy’s Office of General Counsel has issued a Notice of Proposed Civil Penalty to AeroSys, Inc. for failing to file certification reports or filing data that...

  6. Lakes_Elec_You

    Office of Environmental Management (EM)

    ... Florida Jim Woodruff Preference Customers 115 Lincoln Drive Chattahoochee, FL 32324 850663-4475 Georgia Municipal Electric Authority of Georgia Atlanta, GA 30328-4640 770952-5445 ...

  7. FileSys.pptx

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

    Navigating NERSC File Systems May 3, 2011 David Turner NERSC User Services Group * Focus on user-writable file systems * Global file systems * Local file systems * Policies * Performance * Data movement * Data sharing * Platform summary * Hopper, Franklin, Carver/Magellan, Euclid, Datatrans (dtn01/dtn02) Overview * Some file systems are backed up for disaster recovery (of entire file system). * Some file systems are not backed up at all. * Restoration of individual files/directories is not

  8. American Mun Power-Ohio, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 40577 Utility Location Yes Ownership A NERC Location RFC NERC RFC Yes RTO PJM Yes ISO MISO Yes Operates Generating Plant Yes Activity Generation Yes Activity...

  9. New York Mun Power Agency | Open Energy Information

    Open Energy Info (EERE)

    Id 13539 Utility Location Yes Ownership A NERC Location NPCC NERC NPCC Yes Activity Wholesale Marketing Yes This article is a stub. You can help OpenEI by expanding it. Utility...

  10. North Carolina Mun Power Agny | Open Energy Information

    Open Energy Info (EERE)

    Plant Yes Activity Generation Yes Activity Buying Transmission Yes Activity Wholesale Marketing Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes This article is a stub. You...

  11. Southern Minnesota Mun P Agny | Open Energy Information

    Open Energy Info (EERE)

    Address: 500 First Avenue SW Place: Rochester, Minnesota Zip: 55902-3303 Year Founded: 1977 Website: www.smmpa.com References: EIA Form EIA-861 Final Data File for 2010 -...

  12. Grundy Center Mun Light & Power | Open Energy Information

    Open Energy Info (EERE)

    www.gcmuni.nettextcontactus. Facebook: https:www.facebook.compagesCity-of-Grundy-Center169381736410558 Outage Hotline: (319)-825-5207 References: EIA Form EIA-861 Final...

  13. Northern Virginia Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 13640 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes RTO PJM Yes Activity Distribution Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes This...

  14. Central Wisconsin Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    https:www.facebook.compagesCentral-Wisconsin-Electric-Cooperative268841143249085?refaymthomepagepanel Outage Hotline: 800-377-2932 References: EIA Form EIA-861 Final...

  15. 2005 Elec. Safety-rev1.pmd

    Energy Savers [EERE]

    Department of Energy 5 Diesel Engine Emissions Reduction (DEER) Conference Presentations 2005 Diesel Engine Emissions Reduction (DEER) Conference Presentations August 21-25, 2005 Chicago, Illinois The following documents are available as Adobe Acrobat PDFs. Download Adobe Reader. Plenary Session: A View from the Bridge Technical Session 4: Emission Control Technologies, Part 1 Technical Session 1: Advanced Combustion Technologies Part 1 Poster Session 2: Light-Duty Diesels and Emission

  16. Northwestern Wisconsin Elec Co | Open Energy Information

    Open Energy Info (EERE)

    Yes Activity Distribution Yes Activity Wholesale Marketing Yes Activity Retail Marketing Yes This article is a stub. You can help OpenEI by expanding it. Utility Rate...

  17. Western Massachusetts Elec Co | Open Energy Information

    Open Energy Info (EERE)

    Green Button Access: Implemented Green Button Landing Page: www.wmeco.comResidential Green Button Reference Page: www.wmeco.comResidential References: EIA Form EIA-861 Final...

  18. Illinois Municipal Elec Agency | Open Energy Information

    Open Energy Info (EERE)

    Yes Activity Buying Transmission Yes Activity Buying Distribution Yes Activity Wholesale Marketing Yes This article is a stub. You can help OpenEI by expanding it. Utility...

  19. Cumberland Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    EIA Form EIA-861 Final Data File for 2010 - File1a1 Energy Information Administration Form 8262 EIA Form 861 Data Utility Id 4624 Utility Location Yes Ownership C...

  20. Cumberland Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    Schedules Grid-background.png Average Rates Residential: 0.1060kWh Commercial: 0.1120kWh Industrial: 0.0733kWh The following table contains monthly sales and revenue data...

  1. 2005 Elec. Safety-rev1.pmd

    Energy Savers [EERE]

    Positioning System KCP Kansas City Plant LLNL Lawrence Livermore National ... Equipment SC Office of Science SRS Savannah River Site FOREWORD Since 1984, the Office of ...

  2. Rutherford Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    1-800-521-0920 or 1-800-228-9756 or 1-800-228-5331 Outage Map: www.remc.comstorm-centerouta References: EIA Form EIA-861 Final Data File for 2010 - File1a1 Energy...

  3. EnerSys | Open Energy Information

    Open Energy Info (EERE)

    2366 Bernville Road Place: Reading, Pennsylvania Zip: 19605 Region: Northeast - NY NJ CT PA Area Sector: Efficiency Product: Stored energy solutions for industrial applications...

  4. U. 5. COLUMBIA RIVER POWER SYS1

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

    Bonneville Power Administration deposited 12,800,000 to the reclamation fund in the United States Treasury for the account of Columbia Basin Project, Yakima Project...

  5. Paulding-Putman Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 14599 Utility Location Yes Ownership C NERC Location RFC NERC RFC Yes RTO PJM Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  6. Northeast Texas Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 13670 Utility Location Yes Ownership C NERC Location SPP NERC SPP Yes RTO SPP Yes Operates Generating Plant Yes Activity Generation Yes Activity Buying...

  7. Pioneer Rural Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 15054 Utility Location Yes Ownership C NERC Location RFC NERC RFC Yes RTO PJM Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  8. Northern Neck Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 13762 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes RTO PJM Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  9. Cookson Hills Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    861 Data Utility Id 4296 Utility Location Yes Ownership C NERC Location SPP NERC SPP Yes RTO SPP Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  10. Western Farmers Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 20447 Utility Location Yes Ownership C NERC Location SPP NERC SPP Yes RTO SPP Yes Operates Generating Plant Yes Activity Generation Yes Activity Transmission Yes...

  11. Upshur Rural Elec Coop Corp | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 19579 Utility Location Yes Ownership C NERC Location SPP NERC SPP Yes RTO SPP Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  12. Jefferson Davis Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Data Utility Id 9682 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes RTO SPP Yes Activity Distribution Yes This article is a stub. You can help OpenEI by...

  13. East River Elec Pwr Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Facebook: https:www.facebook.compagesEd-the-Energy-Expert431620883566287?refts&frefts Outage Hotline: (605) 256-8057 or (605) 256-8056 or (605) 256-8059...

  14. Central Texas Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    https:www.facebook.compagesCentral-Texas-Electric-Cooperative520773011297941?reftntnmn Outage Hotline: 1-800-900-2832 References: EIA Form EIA-861 Final Data File for...

  15. Southwest Iowa Rural Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    888-220-4869 Website: www.swiarec.coop Facebook: https:www.facebook.comswiarec?refhl Outage Hotline: (888) 220-4869 Outage Map: www.iowarec.orgoutages References: EIA...

  16. Four County Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    www.facebook.compagesFour-County-Electric-Membership-Corporation188316197857616?reftntnmn Outage Hotline: (888)368-7289 Outage Map: gis.fourcty.orgpubmap.html...

  17. Wright-Hennepin Coop Elec Assn | Open Energy Information

    Open Energy Info (EERE)

    3,398.952 34,434.725 40,549 1,975.209 23,239.907 4,920 388.083 5,035.346 51 5,762.244 62,709.978 45,520 2008-04 3,544.862 38,665.009 40,564 1,688.916 21,647.519 4,965 376.604...

  18. Arkansas Valley Elec Coop Corp | Open Energy Information

    Open Energy Info (EERE)

    3,460 776 15,071 13 7,532 101,140 52,031 2009-01 5,376 71,871 48,524 794 11,779 3,462 709 14,853 13 6,879 98,503 51,999 2008-12 4,441 59,651 48,487 736 11,437 3,460 541 15,069...

  19. Big Sandy Rural Elec Coop Corp | Open Energy Information

    Open Energy Info (EERE)

    www.bigsandyrecc.com Twitter: @bigsandycoop Facebook: https:www.facebook.compagesBig-Sandy-RECC142216049157162 Outage Hotline: 888-789-7322 Outage Map:...

  20. Osage Valley Elec Coop Assn | Open Energy Information

    Open Energy Info (EERE)

    Outage Hotline: 660-679-3131 or 800-889-6832 Outage Map: ebill.osagevalley.comomsouta References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form 861...

  1. Canadian Valley Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    anadianValleyElectric Outage Hotline: (855)875-7166 Outage Map: ebill.canadianvalley.orgomso References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form 861 Data...

  2. Claverack Rural Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Outage Hotline: 1-800-326-9799 or 570-265-2167 Outage Map: ebill.claverack.comomsoutage References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form 861...

  3. Monroe County Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Hours (618) 939-7171 or (800) 757-7433 or (866) 567-2759 Outage Map: ebill.mcec.orgomsoutageMap References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form...

  4. Maquoketa Valley Rrl Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Place: Iowa Phone Number: 319-462-3542 or 800-927-6068 Website: mvec.com Twitter: @mvecia Facebook: https:www.facebook.comMaquoketaValleyElectricCooperative Outage Hotline:...

  5. RegIntlElecTrade_Eng_final.PDF

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

    ... and at CRE's web site: www.cre.gob.mxEnglishpublicationsbookletsfollet o%207... and at CRE's web site: www.cre.gob.mxEnglishpublicationsbookletsfolle to%207...

  6. Golden Valley Elec Assn Inc | Open Energy Information

    Open Energy Info (EERE)

    36,891 1,877.823 13,175.914 6,327 8,171.591 69,159.555 448 14,556.482 111,832.096 43,666 2009-01 5,677.62 38,170.143 36,902 2,140.742 15,217.149 6,337 8,864.82 76,857.948 449...

  7. New York State Elec & Gas Corp | Open Energy Information

    Open Energy Info (EERE)

    76,528 8,823 123,751 1,276 219 2,550 4 97,366 787,691 737,183 2008-01 71,181 538,900 666,439 24,517 211,875 77,744 4,058 66,989 1,321 204 2,341 4 99,960 820,105 745,508...

  8. Calhoun County Elec Coop Assn | Open Energy Information

    Open Energy Info (EERE)

    Facebook: https:www.facebook.compagesCalhoun-County-REC173498466069004?skwall Outage Hotline: 800-821-4879 Outage Map: www.iowarec.orgoutages References: EIA Form...

  9. Plumas-Sierra Rural Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    PlumasSierraREC Outage Hotline: (800) 555-2207 Outage Map: www.psrec.coopservice-area.ph References: EIA Form EIA-861 Final Data File for 2010 - File1a1 EIA Form 861 Data...

  10. Dakota Valley Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    1,101.081 16,334.085 5,106 390.564 6,162.524 588 1,168.972 25,110.935 332 2,660.617 47,607.544 6,026 2008-12 1,130.851 17,821.033 5,108 429.98 6,905.622 589 861.853 26,018.826...

  11. Verdigris Valley Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    ) TOT SALES (MWH) TOT CONS 2009-03 3,334 39,732 29,287 620 6,280 4,308 487 5,668 607 4,441 51,680 34,202 2009-02 3,065 36,726 29,285 456 4,469 4,299 405 4,606 607 3,926...

  12. Southern Indiana Gas & Elec Co | Open Energy Information

    Open Energy Info (EERE)

    104,006.182 18,545 11,514.897 200,402.234 101 33,244.465 421,608.6 146,543 2008-02 12,607.003 129,571.861 128,066 9,445.235 104,704.602 18,561 11,374.157 198,519.29 100...

  13. Jones-Onslow Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    56,736 2,076 24,111 4,679 10,879 107,097 61,415 2008-07 8,471 79,614 56,654 1,971 22,607 4,668 10,442 102,221 61,322 2008-06 6,356 61,755 56,244 1,774 20,036 4,651 8,130 81,791...

  14. Southern Indiana Gas & Elec Co | Open Energy Information

    Open Energy Info (EERE)

    EIA Form EIA-861 Final Data File for 2010 - File1a1 Energy Information Administration Form 8262 EIA Form 861 Data Utility Id 17633 Utility Location Yes Ownership I...

  15. Roosevelt County Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    3,749 3,650 146 1,178 965 1,478 13,978 1,594 2,017 18,905 6,209 2008-06 357 3,560 3,638 132 1,092 961 1,347 13,188 1,579 1,836 17,840 6,178 2008-05 292 2,856 3,639 128 1,070 964...

  16. Southern Pine Elec Power Assn | Open Energy Information

    Open Energy Info (EERE)

    87,734 60,157 3,222 30,360 4,536 5,087 63,820 24 18,195 181,914 64,717 2008-05 6,897 62,132 60,058 2,887 27,862 4,522 4,430 56,228 24 14,214 146,222 64,604 2008-04 6,581 59,423...

  17. Singing River Elec Pwr Assn (Mississippi) | Open Energy Information

    Open Energy Info (EERE)

    9,647.445 93,322.028 60,225 3,117.42 30,825.248 8,207 692.763 8,259.846 11 13,457.628 132,407.122 68,443 2008-06 9,059.584 86,892.462 60,106 3,046.146 30,089.083 8,193 709.428...

  18. Duck River Elec Member Corp | Open Energy Information

    Open Energy Info (EERE)

    10,355 1,290 21,368 18 13,312 170,739 70,025 2008-01 8,728 110,789 59,691 2,848 31,132 10,373 1,150 18,079 18 12,726 160,000 70,082 References "EIA Form EIA-861 Final...

  19. Navasota Valley Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Website: www.navasotavalley.com Facebook: https:www.facebook.comnavasotavalley Outage Hotline: 1-800-443-9462 Outage Map: outages.navasotavalley.com:85 References: EIA...

  20. Central Florida Elec Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Inc Place: Florida Phone Number: 1-800-227-1302 or 352-493-2511 Website: www.cfec.com Outage Hotline: 1-800-227-1302 or 352-493-2511 Outage Map: www.cfec.comoutage-mapsite...

  1. Fall River Rural Elec Coop Inc (Wyoming) | Open Energy Information

    Open Energy Info (EERE)

    Website: www.fallriverelectric.com Facebook: https:www.facebook.comFallRiverREC Outage Hotline: 1.866.887.8442 (After Hours) Outage Map: outage.fallriverelectric.como...

  2. Mountain View Elec Assn, Inc | Open Energy Information

    Open Energy Info (EERE)

    Inc Place: Colorado Website: www.mvea.coop Facebook: https:www.facebook.comMVEAInc Outage Hotline: (800) 388-9881 Outage Map: outage.mvea.org References: EIA Form EIA-861...

  3. Columbia Basin Elec Cooperative, Inc | Open Energy Information

    Open Energy Info (EERE)

    EIA-861 Final Data File for 2010 - File1a1 EIA Form 861 Data Utility Id 4005 Utility Location Yes Ownership C NERC Location WECC NERC WECC Yes Activity Transmission Yes...

  4. Guadalupe Valley Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    2010 - File1a1 EIA Form 861 Data Utility Id 7752 Utility Location Yes Ownership C NERC Location TRE NERC ERCOT Yes Activity Transmission Yes Activity Buying Transmission Yes...

  5. Houston County Elec Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    2010 - File1a1 EIA Form 861 Data Utility Id 8898 Utility Location Yes Ownership C NERC Location TRE NERC ERCOT Yes Activity Transmission Yes Activity Distribution Yes Activity...

  6. Butler County Rural Elec Coop | Open Energy Information

    Open Energy Info (EERE)

    Iowa Phone Number: 888-267-2726 Website: www.butlerrec.coop Twitter: @ButlerCountyREC Facebook: https:www.facebook.combcrec Outage Hotline: 888-267-2726 Outage Map:...

  7. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    and contingency planning of the energy grids and energy plants considering also the ICT systems used in protection and control. Main addressed problems concern high impact,...

  8. Regenerative Energie Systeme RegEnSys | Open Energy Information

    Open Energy Info (EERE)

    Zip: 67227 Sector: Solar Product: Sale and installation of solar (thermal and PV) and ventilation systems. Coordinates: 51.131202, 14.106809 Show Map Loading map......

  9. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    Retrieved from "http:en.openei.orgwindex.php?titleAFTERAFrameworkforelectricalpowersysTemsvulnerabilityidentification,dEfenseandRestoration(SmartGridProject)(...

  10. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    Retrieved from "http:en.openei.orgwindex.php?titleAFTERAFrameworkforelectricalpowersysTemsvulnerabilityidentification,dEfenseandRestoration(SmartGridProject)&o...

  11. Property:Incentive/EligSysSize | Open Energy Information

    Open Energy Info (EERE)

    minimum
    Recycled Energy: 15 Megawatt maximum Alameda Municipal Power - Solar Photovoltaics Rebate Program (California) + Maximum size is 1 MW or 110% of customer's...

  12. EnSys Energy Report on Keystone XL Pipeline

    Broader source: Energy.gov [DOE]

    As part of ongoing analysis, the Department of Energy's Office of Policy and International Affairs commissioned a report on the proposed Keystone XL pipeline project.

  13. AFTER A Framework for electrical power sysTems vulnerability...

    Open Energy Info (EERE)

    :"","inlineLabel":"","visitedicon":"" Display map Period 2011-2014 References EU Smart Grid Projects Map1 Overview AFTER addresses vulnerability evaluation and contingency...

  14. U-045: Windows Win32k.sys Keyboard Layout Bug Lets Local Users...

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

    ID: SA46919 IMPACT ASSESSMENT: Low Discussion: A vulnerability has been discovered in Microsoft Windows, which can be exploited by malicious, local users to cause a DoS (Denial...

  15. Predicts the Long Term Performance and Economic Feasibility of Hybrid Power Sys

    Energy Science and Technology Software Center (OSTI)

    1996-12-01

    HYBRID2 is a combined probalistic/time series model designed to study a wide variety of hybrid power systems. Hybrid power systems combine a number of sources of power generation and, usually, a form of energy storage to supply an electrical load. Hybrid power systems are mainly used in areas such as islands or remote communities that are removed from a power distribution network. These power systems can range from large, multi-megawatt systems to those supplying singlemore » family dwellings. HYBRID2 simulates systems that include diesel generators, wind turbines, battery storage, different power conversion devices and a photovoltaic array. Systems can be modeled with components on the AC, DC or multiple buses. A variety of different operating strategies have been allowed as well as an economic analysis tool. The HYBRID2 code has a user-friendly Graphical User Interface (GUI) as well as a glossary of terms commonly associated with hybrid power systems. HYBRID2 is also packaged with an extensive library of equipment to assist the user in designing hybrid power systems. Each piece of equipment is commercially available and uses manufacturer''s specifications. In addition the library includes resource data and some sample power systems and projects that can be used as templates. Two levels of output are provided, a summary as well as a detailed time step by time step description of power flows. A Graphical Results Interface (GRI) allows for easy and in-depth review of the detailed simulation results.« less

  16. T-601: Windows Kernel win32k.sys Lets Local Users Gain Elevated Privileges

    Broader source: Energy.gov [DOE]

    Multiple vulnerabilities were reported in the Windows Kernel. A local user can obtain elevated privileges on the target system. A local user can trigger a use-after free or null pointer dereference to execute arbitrary commands on the target system with kernel level privileges.

  17. U-028: Microsoft Windows win32k.sys TrueType Font Parsing Vulnerability

    Broader source: Energy.gov [DOE]

    A vulnerability has been reported in Microsoft Windows, which can be exploited by malicious people to compromise a user's system.

  18. Microsoft Word - NG_ResQrySys_UsersGuide_Sept2015-FINAL.docx

    Gasoline and Diesel Fuel Update (EIA)

    ... the Query System is a web-based system, no download or installation is necessary. All that is needed to run the Query System is a PC with up-to-date web-browsing software (such ...

  19. Released: June 2006

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

    ,,,"Elec- tricity","Natural Gas","District Chilled Water",,,"Elec- tricity","Natural Gas","District Chilled Water" "All Buildings* ......",4645,3625,3589,17,33,6478...

  20. Kotzebue Wind Project I | Open Energy Information

    Open Energy Info (EERE)

    Status In Service Owner Kotzebue Elec. Assoc. Developer Kotzebue Electric Association Energy Purchaser Kotzebue Elec. Assoc. Location Kotzebue AK Coordinates 66.836485,...

  1. Alaska Village Cooperative Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    In Service Owner Alaska Village Elec Coop Developer Kotzebue Electric Association Energy Purchaser Alaska Village Elec Coop Location Toksook Bay AK Coordinates 60.5315,...

  2. --No Title--

    Gasoline and Diesel Fuel Update (EIA)

    Energy Sources (more than one may apply) Elec- tricity Natural Gas District Chilled Water Elec- tricity Natural Gas District Chilled Water All Buildings* ......

  3. United States

    Office of Legacy Management (LM)

    ... ---- Sobtotalr Policy and aanaderent......,..... ---... TOTAL, ENERGY SUFPLY RESEARCH AND ... III...... 83-N-401 Ref. of elec, circuit breaker Gas dif. ...

  4. Conceptual Design Report Cask Loadout Sys and Cask Drop Redesign for the Immersion Pail Support Structure and Operator Interface Platform at 105 K West

    SciTech Connect (OSTI)

    LANGEVIN, A.S.

    1999-07-12

    This conceptual design report documents the redesign of the IPSS and the OIP in the 105 KW Basin south loadout pit due to a postulated cask drop accident, as part of Project A.5/A.6, Canister Transfer Facility Modifications. Project A.5/A.6 involves facility modifications needed to transfer fuel from the basin into the cask-MCO. The function of the IPSS is to suspend, guide, and position the immersion pail. The immersion pail protects the cask-MCO from contamination by basin water and acts as a lifting device for the cask-MCO. The OIP provides operator access to the south loadout pit. Previous analyses studied the effects of a cask-MCO drop on the south loadout pit concrete structure and on the IPSS. The most recent analysis considered the resulting loads at the pit slab/wall joint (Kanjilal, 1999). This area had not been modeled previously, and the analysis results indicate that the demand capacity exceeds the allowable at the slab/wall joint. The energy induced on the south loadout pit must be limited such that the safety class function of the basin is maintained. The solution presented in this CDR redesigns the IPSS and the OIP to include impact-absorbing features that will reduce the induced energy. The impact absorbing features of the new design include: Impact-absorbing material at the IPSS base and at the upper portion of the IPSS legs. A sleeve which provides a hydraulic means of absorbing energy. Designing the OIP to act as an impact absorber. The existing IPSS structure in 105 KW will be removed. This conceptual design considers only loads resulting from drops directly over the IPSS and south loadout pit area. Drops in other areas of the basin are not considered, and will be covered as part of a future revision to this CDR.

  5. In-Situ observation of wet oxidation kinetics on Si (100) via...

    Office of Scientific and Technical Information (OSTI)

    Authors: Hussain, Zahid ; Rossi, Massimiliano ; Mun, Bongjin S. ; Enta, Yoshiharu ; Fadley, Charles S. ; Lee, Ki-Suk ; Kim, Sang-Koog ; Shin, Hyun-Joon ; Hussain, Zahid ; Ross, ...

  6. A photoemission study of Pd ultrathin films on Pt(111) (Journal...

    Office of Scientific and Technical Information (OSTI)

    Authors: Mun, Bongjin Simon ; Lee, Choongman ; Stamenkovic, Vojislav ; Markovic, Nenad M. ; Ross Jr., Philip N. Publication Date: 2005-05-11 OSTI Identifier: 860351 Report ...

  7. PSERC Webinar March 20, 2012

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

    of renewable generation technologies coupled to the grid through power elec- tronic interfaces, and the potential for future growth of electrical storage similarly coupled through ...

  8. Cimarron Electric Coop | Open Energy Information

    Open Energy Info (EERE)

    Twitter: @CimarronElec Facebook: https:www.facebook.comprofile.php?refname&id100000678310273 Outage Hotline: (800) 375-4121 References: EIA Form EIA-861...

  9. Word Pro - S12

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

    Coal Coke Net Imports Natural Gas b Petroleum Retail Elec- tricity g Total h Distillate ... and miscellaneous petroleum products. g Emissions from energy consumption (for ...

  10. Effects of Feedback on Residential Electricity Consumption: A...

    Office of Scientific and Technical Information (OSTI)

    none of which were elec- trically heated; each had an electric stove, dryer, dishwasher, and water heater. The researchers installed 24-h chart recorders in each residence...

  11. Property:EIA/861/NercMro | Open Energy Information

    Open Energy Info (EERE)

    + true + Brainerd Public Utilities + true + Brodhead Water & Lighting Comm + true + Brown County Rural Elec Assn + true + Burke-Divide Electric Coop Inc + true + Butler County...

  12. Awardee AwardeeHeadquarters RecoveryFunding TotalValue Tech Inc...

    Open Energy Info (EERE)

    City South Dakota Black Hills Colorado Elec Utility Co LP Pueblo Colorado City of Burbank Water and Power California Utility Company Burbank California Center for the...

  13. Callaway Electric Cooperative | Open Energy Information

    Open Energy Info (EERE)

    Place: Missouri Phone Number: (573) 642-3326 Website: www.callawayelectric.com Twitter: @CallawayElec Facebook: http:www.facebook.comCallawayElectric Outage Hotline:...

  14. District of Columbia: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    (District of Columbia) Glacial Energy Holdings (District of Columbia) Hess Retail Natural Gas and Elec. Acctg. (District of Columbia) Integrys Energy Services, Inc. (District...

  15. Document

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

    Limit Values for Chemical Substances and Physical Agents and Biological Exposure Indices'' ... National Fire Protection Association (NFPA) 70, ''National Elec- trical Codes''. ...

  16. Kotzebue Wind Project III | Open Energy Information

    Open Energy Info (EERE)

    Kotzebue Wind Project III Facility Kotzebue Wind Project Sector Wind energy Facility Type Small Scale Wind Facility Status In Service Owner Kotzebue Elec. Assoc. Developer Kotzebue...

  17. Colman, South Dakota: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Inc. Smart Grid Project Utility Companies in Colman, South Dakota Sioux Valley SW Elec Coop References US Census Bureau Incorporated place and minor civil division...

  18. Alternative Fuels Data Center

    Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

    (B20 and above) CNG Compressed Natural Gas E85 Ethanol (E85) ELEC Electric HY Hydrogen LNG Liquefied Natural Gas LPG Liquefied Petroleum Gas (Propane) stationname Type:...

  19. 11,23,1,3,2,19,30,"BANGOR HYDRO ELECTRIC CO","MEDWAY",0,"LIGHT...

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

    ...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...17,1,07977,"FO2","ST" 31,39,5,2,6,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"BIT ...

  20. 11,23,1,3,2,19,30,"BANGOR HYDRO ELECTRIC CO","MEDWAY",0,"LIGHT...

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

    ... 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT OIL",51225,0,"M",1299,,,2000,74,155,1e+15,2917,1,07977,"FO2","ST" 31,39,5,2,6,605,1,"HAMILTON (CITY OF)","HAM MUN ...

  1. U-233: Oracle Database INDEXTYPE CTXSYS.CONTEXT Bug Lets Remote Authenticated Users Gain Elevated Privileges

    Broader source: Energy.gov [DOE]

    A remote authenticated user with 'Create Table' privileges can gain 'SYS' privileges on the target system.

  2. Aerogel Impregnated Polyurethane Piping and Duct Insulation

    Energy Savers [EERE]

    AeroSysNNC_3-25.pdf AeroSysNNC_3-25.pdf PDF icon AeroSysNNC_3-25.pdf More Documents & Publications AeroSys: Noncompliance Determination (2010-SE-0302) AeroSys: Test Notice (2009) AeroSys: Order (2010-CE-01/0201 and 2010-SE-0302)

    Aerogel Impregnated Polyurethane Piping and Duct Insulation David M. Hess InnoSense LLC david.hess@innosense.us, 310-530-2011 April 4, 2013 2 | Building Technologies Office eere.energy.gov Purpose & Objectives Problem Statement: Develop an efficient insulation

  3. Magnetic field effects on transport properties of PtSn4 (Journal...

    Office of Scientific and Technical Information (OSTI)

    field effects on transport properties of PtSn4 Prev Next Title: Magnetic field effects on transport properties of PtSn4 Authors: Mun, Eundeok ; Ko, Hyunjin ; Miller, Gordon ...

  4. Looking at Transistor Gate Oxide Formation in Real Time

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

    University, Japan); B.S. Mun (Hanyang University, Korea, and ALS); M. Rossi, and Z. Hussain (ALS); P.N. Ross Jr. (Berkeley Lab); C.S. Fadley (University of California at...

  5. CENSUS","FIPST","OWNER","PMOVER","FUELTYP","COCODE","PLTCODE...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",5400,,52224,0,0,1285,,,86,2601400,0,...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",128000,"LIGHT ...

  6. 63,01,1,1,,10,1,"ALABAMA POWER CO","BANKHEAD DM",0,,50022,0,0...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",0,,52224,0,0,1287,,,88,953200,0,0,11...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  7. CENSUS","FIPST","OWNER","PMOVER","FUELTYP","COCODE","PLTCODE...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",5390,,14328,0,0,1283,,,84,3696700,0,...14,1,50806,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",127991,"LIGHT ...

  8. 63,01,1,1,,10,1,"ALABAMA POWER CO","BANKHEAD DM",0,,19500,1293...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",0,,1432800,1293,,,94,1962,0,0,1168,0...14,1,50806,"FO2","IC" 31,39,5,2,6,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"BIT ...

  9. CENSUS","FIPST","OWNER","PMOVER","FUELTYP","COCODE","PLTCODE...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",0,,52224,0,0,1286,,,87,1321000,0,0,1...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  10. 63,01,1,1,,10,1,"ALABAMA POWER CO","BANKHEAD DM",0,,50022,0,0...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",0,,52224,0,0,1288,,,89,633000,0,0,58...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  11. 63,01,1,1,,10,1,"ALABAMA POWER CO","BANKHEAD DM",0,,50022,0,0...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",0,,52224,0,0,1289,,,90,1884,0,0,791,...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  12. CENSUS","FIPST","OWNER","PMOVER","FUELTYP","COCODE","PLTCODE...

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

    ... GAS & ELECTRIC CO","HAMILTON BR",5390,,52224,0,0,1284,,,85,1431000,0,...14,1,05336,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",127991,"LIGHT ...

  13. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Effect in Ni 3 TeO 6 Kim, Jae Wook ; Artyukhin, S. ; Mun, E. D. ; Jaime, M. ; Harrison, N. ; Hansen, A. ; Yang, J. J. ; Oh, Y. S. ; Vanderbilt, D. ; Zapf, V. S. ; et al...

  14. A sub-GeV charged-current quasi-elastic $\

    SciTech Connect (OSTI)

    Walding, Joseph James; /Imperial Coll., London

    2010-04-01

    Neutrino-nucleus charged-current quasi-elastic scattering is the signal interaction used by many neutrino oscillation experiments. For muon disappearance studies the signal mode is {nu}{sub {mu}}n {yields} {mu}p. Modern oscillation experiments, such as T2K, produce neutrino beams with peak beam energies of order a few-GeV. It is therefore vitally important to have accurate measurements of the charged-current quasi-elastic cross-section for future neutrino oscillation experiments. Neutrino-nucleus cross-sections in the few-GeV region are not well understood, with the main uncertainties coming from understanding of the neutrino beam flux and the final state interactions within nuclei. SciBooNE is a sub-GeV neutrino-nucleus cross-section experiment based at Fermilab, Batavia, USA, with the goal to measure neutrino cross-sections with precision of order 5%. SciBooNE took data from June 2007 until August 2008, in total 0.99 x 10{sup 20} and 1.53 x 10{sup 20} protons on target were collected in neutrino and anti-neutrino mode, respectively. In this thesis a {nu}{sub {mu}} charged-current quasi-elastic (CCQE) cross-section contained within the SciBar sub-detector is presented. A method to tag muons in SciBar was developed and three samples were isolated. An excess in backwards tracks in the one-track sample is observed. A Poisson maximum likelihood is used to extract the CCQE cross-section. The fit was applied using a basic fit parameter model, successfully used to obtain the cross-section in the SciBar-MRD matched CCQE analysis. This method was found to be insufficient in describing the data for the SciBar-contained CCQE analysis. By adding two migration parameters the cross-section was calculated to be 1.004 {+-} 0.031 (stat){sub -0.150}{sup +0.101}(sys) x 10{sup -38} cm{sup 2}/neutron, excluding backwards tracks with a {chi}{sup 2} = 203.8/76 d.o.f. and 1.083 {+-} 0.030(stat){sub -0.177}{sup +0.115}(sys) x 10{sup -38} cm{sup 2}/neutron, including backwards tracks with a {chi}{sup 2} = 659.8/133 d.o.f. Only neutrino beam and detector systematics have been considered. Further study of the SciBar-contained sample is suggested, introducing additional fit parameters and considering the remaining systematics. The end goal is to extract a SciBooNE CCQE cross-section using the SciBar-contained and SciBar-MRD matched samples.

  15. Four Central Air Conditioners Determined Noncompliant With Energy Efficiency Standard

    Broader source: Energy.gov [DOE]

    The U.S. Department of Energy’s Office of Enforcement issued a Notice of Noncompliance Determination (Notice) on September 27, 2011, to AeroSys, Inc. (AeroSys) regarding four models of central ...

  16. Four Central Air Conditioners Determined Noncompliant With Energy...

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

    (Notice) on September 27, 2011, to AeroSys, Inc. (AeroSys) regarding four models of central (through-the-wall) air conditioners that fail to meet Federal energy...

  17. Chapter 39 - Acquisition of Information Technology | Department...

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

    9 - Acquisition of Information Technology Chapter 39 - Acquisition of Information Technology PDF icon 39.1AcquisitionofInformationResources0.pdf PDF icon 39.2GuidanceonElec...

  18. CX-000958: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    RenewElec ProjectCX(s) Applied: A9, A11Date: 02/26/2010Location(s): Pittsburgh, PennsylvaniaOffice(s): Fossil Energy, National Energy Technology Laboratory

  19. Category:Atlantic City, NJ | Open Energy Information

    Open Energy Info (EERE)

    16 files are in this category, out of 16 total. SVFullServiceRestaurant Atlantic City NJ Public Service Elec & Gas Co.png SVFullServiceRestauran... 63 KB SVMidriseApartment...

  20. Word Pro - S2

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

    Petroleum Other Mobility Fuels f Elec- tricity Purchased Steam and Other g Total Aviation ... B100 (100% biodiesel); hydrogen; and methanol. g Other types of energy used in facilities. ...

  1. John Bistline, Project Manager EIA Energy Conference

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

    U.S. Sectors, GHG Emissions, and Mitigation Goals 26% below 2005 2025 30% below 2005 Elec Sec 2050 80% below 2005 Source: E PA I nventory o f U .S. G reenhouse G as E missions a nd ...

  2. Waste Heat Utilization System Income Tax Deduction (Personal)

    Office of Energy Efficiency and Renewable Energy (EERE)

    Waste heat utilization system means facilities and equipment for the recovery of waste heat generated in the process of generating electricity and the use of such heat to generate additional elec...

  3. Waste Heat Utilization System Income Tax Deduction (Corporate)

    Office of Energy Efficiency and Renewable Energy (EERE)

    Waste heat utilization system means facilities and equipment for the recovery of waste heat generated in the process of generating electricity and the use of such heat to generate additional elec...

  4. "2014 Utility Bundled Retail Sales- Residential"

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

    ...ipal",5758,49078,4553,9.2770692 "City of Hamilton - (OH)","OH","Municipal",26127,267514,28...operative",19241,368809,42042,11.399396 "Hamilton County Elec Coop Assn","TX","Cooperative...

  5. "2014 Utility Bundled Retail Sales- Total"

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

    ...ipal",5990,105389,8856,8.403154 "City of Hamilton - (OH)","OH","Municipal",29042,578972,61...operative",24868,502493,56758,11.295282 "Hamilton County Elec Coop Assn","TX","Cooperative...

  6. "2014 Utility Bundled Retail Sales- Commercial"

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

    ...nicipal",162,8706,777,8.9248794 "City of Hamilton - (OH)","OH","Municipal",2861,136480,163...ooperative",5626,130607,14559,11.147182 "Hamilton County Elec Coop Assn","TX","Cooperative...

  7. National Electric Transmission Congestion Study 2009 Executive...

    Energy Savers [EERE]

    (DOE) to conduct a study every three years on elec- tric transmission congestion and ... built in the region in the past three years, al- though many new backbone and ...

  8. CarBen_Operators_Manual_-_9-27-10_Final_Draft

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

    Source Data o ER: Emissions Reduction Case o Ref: Reference Case o Res: Residential Module o Com: Commercial Module o Ind: Industrial Module o Elec: Electricity Module o Trans:...

  9. Impact of Extended Daylight Saving Time on National Energy Consumption...

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

    Energy Consumption Report to Congress Energy Policy Act of 2005, Section 110 October 2008 ... Error Indianapolis Power & Light 2.4% 0.9% -3.8% 1.3% Louisville Gas & Elec 1.7% 1.0% ...

  10. Property:Awardee | Open Energy Information

    Open Energy Info (EERE)

    Utility Co. Smart Grid Project + Black HillsColorado Elec.Utility Co. LP + Burbank Water and Power Smart Grid Project + City of Burbank Water and Power, California (Utility...

  11. Category:Elkins, WV | Open Energy Information

    Open Energy Info (EERE)

    16 files are in this category, out of 16 total. SVFullServiceRestaurant Elkins WV Harrison Rural Elec Assn Inc.png SVFullServiceRestauran... 59 KB SVQuickServiceRestaurant...

  12. Oklahoma Electric Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Electric Coop Inc Place: Oklahoma Phone Number: 1-405-321-2024 Website: www.okcoop.org Twitter: @okcoop Facebook: https:www.facebook.comOklaElec Outage Hotline: 405-321-2024...

  13. Buying an Energy-Efficient Electric Motor

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

    ... of Electrical and Elec- tronics Engineers (IEEE ) 112 Method B, which uses a dynamometer ... uses bands of efficiency values based on IEEE 112 testing. 4. When should I consider ...

  14. b30.xls

    Gasoline and Diesel Fuel Update (EIA)

    District Chilled Water Elec- tricity Natural Gas District Chilled Water All Buildings* ...... 4,645 3,625 3,589 17 33 64,783 56,940 54,321 1,018 2,853 ...

  15. Word Pro - S2

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

    Renewable Energy b Elec- tricity Net Imports e Total Primary Coal Natural Gas c Petro- leum Total Hydro- electric Power d Geo- thermal Solar PV Wind Bio- mass Total 1950 Total ...

  16. Cass County Electric Coop Inc | Open Energy Information

    Open Energy Info (EERE)

    Twitter: @CassCountyElec Facebook: https:www.facebook.comCassCountyElectric Outage Hotline: 701-356-4499 or 1-888-277-4424 Outage Map: outage.kwh.com References: EIA...

  17. --No Title--

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

    123 YESNO. PHOTVL8 Photovoltaic cells used to generate elec 125- 125 YESNO. FUELCL8 Fuel cells used to generate electricity 127- 127 YESNO. MCROTB8 Microturbines used to...

  18. --No Title--

    Gasoline and Diesel Fuel Update (EIA)

    than one may apply) Elec- tricity Natural Gas Fuel Oil District Heat District Chilled Water Propane Other a All Buildings* ... 4,645 4,414 4,404 2,391...

  19. --No Title--

    Gasoline and Diesel Fuel Update (EIA)

    than one may apply) Elec- tricity Natural Gas Fuel Oil District Heat District Chilled Water Propane Other a All Buildings* ... 64,783 63,343 63,307...

  20. NRELs Energy-Saving Technology for Air Conditioning Cuts Peak...

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

    (DEVAP) air-condi- tioning will provide superior comfort for commercial buildings in any climate at a small fraction of the elec- tricity costs of conventional air-conditioning ...

  1. The Ames Laboratory

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

    Directory: Information Systems Name Title Office Email Phone Number Mark Clarridge Sys Sup Spec IV 334 TASF clarridge@ameslab.gov 515-294-6396 Karla Concannon Sys Analyst II 334 TASF kconcann@ameslab.gov 515-294-8334 Klarida Cubacub Sys Sup Spec III 334 TASF cubacub@ameslab.gov 515-294-5325 Diane Denadel Mgr Ames Lab Info Sys 334 TASF ddenadel@ameslab.gov 515-294-1061 Fang Fang 334 TASF ffang@iastate.edu 515-294-8348 Christopher Farrington Sys Sup Spec III 334 TASF farrington@ameslab.gov

  2. gharper | The Ames Laboratory

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

    gharper Ames Laboratory Profile Gregory Harper Sys Control Tech Facilities Services Maintenance Shop Phone Number: 515-294-1746 Email Address: gharper

  3. Microsoft PowerPoint - 12_BRIAN_HORN_NRC and DOE recognition...

    National Nuclear Security Administration (NNSA)

    20 days after starting, and reconciled the same day as received at NMMSS Global Laser enrichment and Paducah (SYS) -each submitted inventory less than 52 days after ...

  4. Process Heating: A Special Supplement to Energy Matters

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

    The Components of Process Heating Sys- tems Process heating systems are made up of five ... heat source, or indirectly through the The Big Picture on Process Heating Materials ...

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

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

    Fincham Hydrate Modeling & Flow Loop Experiments for Water Continuous and Dispersed Sys. Design and machine fiber optic seismic sensors. Wind sensors in the Paulsson clean room....

  6. mhend | The Ames Laboratory

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

    mhend Ames Laboratory Profile Matthew Henderson Sys Analyst I Chemical & Biological Sciences 327 Wilhelm Phone Number: 515-294-1293 Email Address: mhend@ameslab.gov

  7. rberrett | The Ames Laboratory

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

    rberrett Ames Laboratory Profile Ronald Berrett Sys Control Tech Facilities Services Maintenance Shop Phone Number: 515-294-1746 Email Address: rberrett

  8. Bioenergy Technologies Office Fiscal Year 2014 Annual Report

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

    ... state of the science, research needs, tools, and methodologies for implementing landscape designs for bioenergy sys- tems across the supply chain and across sustainability metrics. ...

  9. Tax Credits, Rebates & Savings | Department of Energy

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

    to the utility for an impact study, including a request for an estimate of the cost of interconnecting the proposed sys... Eligibility: Commercial, Industrial, Local...

  10. Civil Penalties for Energy Conservation Standards Program Violations...

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

    More Documents & Publications Air-Con International: Noncompliance Determination and Proposed Penalty (2010-SE-0301) AeroSys: Proposed Penalty (2011-SCE-1624) Goodman ...

  11. Aerodynamic Lightweight Cab Structure Components | Department of Energy

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

    PDF icon AeroSysNNC_3-25.pdf More Documents & Publications AeroSys: Noncompliance Determination (2010-SE-0302) AeroSys: Test Notice (2009) AeroSys: Order (2010-CE-01/0201 and 2010-SE-0302)

    2012 DOE Hydrogen and Fuel Cells Program and Vehicle Technologies Program Annual Merit Review and Peer Evaluation Meeting PDF icon lm060_smith_2012_o.pdf More Documents & Publications Aerodynamic Lightweight Cab Structure Components Vehicle Technologies Office Merit Review 2014: Aerodynamic

  12. Table 2.5 Household Energy Consumption and Expenditures by End Use, Selected Years, 1978-2005

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

    5 Household 1 Energy Consumption and Expenditures by End Use, Selected Years, 1978-2005 Year Space Heating Air Conditioning Water Heating Appliances, 2 Electronics, and Lighting Natural Gas Elec- tricity 3 Fuel Oil 4 LPG 5 Total Electricity 3 Natural Gas Elec- tricity 3 Fuel Oil 4 LPG 5 Total Natural Gas Elec- tricity 3 LPG 5 Total Consumption (quadrillion Btu)<//td> 1978 4.26 0.40 2.05 0.23 6.94 0.31 1.04 0.29 0.14 0.06 1.53 0.28 1.46 0.03 1.77 1980 3.41 .27 1.30 .23 5.21 .36 1.15 .30 .22

  13. Word Pro - Untitled1

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

    3 Table 2.5 Household 1 Energy Consumption and Expenditures by End Use, Selected Years, 1978-2005 Year Space Heating Air Conditioning Water Heating Appliances, 2 Electronics, and Lighting Natural Gas Elec- tricity 3 Fuel Oil 4 LPG 5 Total Electricity 3 Natural Gas Elec- tricity 3 Fuel Oil 4 LPG 5 Total Natural Gas Elec- tricity 3 LPG 5 Total Consumption (quadrillion Btu) 1978 4.26 0.40 2.05 0.23 6.94 0.31 1.04 0.29 0.14 0.06 1.53 0.28 1.46 0.03 1.77 1980 3.41 .27 1.30 .23 5.21 .36 1.15 .30 .22

  14. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1295,,,96,606...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  15. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ...2,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",54020,0,"M",1199,"N",,199...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  16. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1297,,,1998,6...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  17. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,0...

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

    ...2,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",0,1292,,,93,36,93,3861,72...914,1,50806,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  18. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,0...

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

    ...2,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",0,1290,,,91,21,66,4481,33...14,1,50806,"FO2","IC" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  19. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,0...

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

    ...2,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",0,1291,,,92,54,141,4036,0...914,1,50806,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  20. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1296,,,97,268...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  1. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1297,,,98,73,...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  2. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1295,,,96,291...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  3. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,50159...

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

    ... 23,42,1,4,2,114,24,"GPU SERVICE CORP","HAMILTON",0,"LIGHT OIL",54020,0,"M",1296,,,97,0,7...914,1,05336,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  4. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,1179...

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

    ...2,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",12390,"0M",1294,,,95,0,44...914,1,50806,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT ...

  5. 2014 Utility Bundled Retail Sales- Commercial

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

    ... Municipal 162 8,706 777.0 8.92 City of Hamilton - (OH) OH Municipal 2,861 136,480 ... TX Cooperative 5,626 130,607 14,559.0 11.15 Hamilton County Elec Coop Assn TX Cooperative ...

  6. 2014 Utility Bundled Retail Sales- Total

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

    ... 5,990 105,389 8,856.0 8.40 City of Hamilton - (OH) OH Municipal 29,042 578,972 ... TX Cooperative 24,868 502,493 56,758.0 11.30 Hamilton County Elec Coop Assn TX Cooperative ...

  7. 2014 Utility Bundled Retail Sales- Residential

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

    ... 5,758 49,078 4,553.0 9.28 City of Hamilton - (OH) OH Municipal 26,127 267,514 ... TX Cooperative 19,241 368,809 42,042.0 11.40 Hamilton County Elec Coop Assn TX Cooperative ...

  8. NUG Teleconference

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

    o n P hase I i n F eb. 2 013 - Phase I I p lanned f or s ummer 2 013 --- 5 --- NUGEX Elections * 22 candidates for 11 posi?ons * Elec?on dates: ? * Candidate s tatements n eeded....

  9. Interconnection Guidelines

    Broader source: Energy.gov [DOE]

    Under this process, an interconnection applicant must submit an application to the utility for an impact study, including a request for an estimate of the cost of interconnecting the proposed sys...

  10. Hydrogen Home Refueling: Status, Key Issues, and Challenges

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

    Journal of The Electrochem ical Society, 159(6) K165-K176 (2012) 3 Home Refueling Issues: Cost 0.2 kghr Sys tem 5000 ps i with no further com pres sion High utilization and energy ...

  11. WE2 | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search Name: WE2 Place: Bietigheim-Bissingen, Baden-Wrttemberg, Germany Zip: 74321 Sector: Wind energy Product: JV between WPD AG and EnerSys GmbH for...

  12. Remote sensing of fugitive methane emissions from oil and gas...

    Energy Savers [EERE]

    ... sys- tems corresponds to 0.7% of the U.S. crude oil production (0.5%-1.7% at the 95% ... (e.g., enteric fermentation in live- stock), were temporally constant to a ...

  13. California Energy Commissioner Carla Peterman and James

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

    California Energy Commissioner Carla Peterman and James Bartridge (CEC) discuss electric vehicle technologies with Fraser Murison Smith (right) of i-GATE NEST client, Elec- traDrive. The partnership with i-GATE has made it easier for businesses and the state of California to engage with Sandia and its assets, helping to push our economic goals forward. Louis Stewart Deputy Director Innovation and Entrepreneurship Governor's Office of Business & Economic Development Innovation Hub Connects

  14. Table 3. Top five retailers of electricity, with end use sectors, 2014

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

    Colorado" "megawatthours" ,"Entity","Type of provider","All sectors","Residential","Commercial","Industrial","Transportation" 1,"Public Service Co of Colorado","Investor-owned",28671219,9008526,12886370,6712282,64041 2,"City of Colorado Springs - (CO)","Public",4477715,1425423,1097160,1955132,0 3,"Intermountain Rural Elec

  15. Buildings*","Buildings Using Any Energy

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

    3. Energy Sources, Floorspace for Non-Mall Buildings, 2003" ,"Total Floorspace (million square feet)" ,"All Buildings*","Buildings Using Any Energy Source","Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","District Chilled Water","Propane","Other a " "All Buildings*

  16. Tools_Equipment under 10K RO 23_120213.xlsx

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

    Other Government Furnished Property (GFP) / Equipment 1 RO BARCODE DESCRIPTION MANUF. MODEL SN COST BLDG ROOM INVT_DATE 23 0000032497 THERMAL LABELING SYS BRADY WORLDWIDE TLS2200 BPTLS901644924 $0.00 28 119 24-Sep-13 23 F13412 PWR SUPPLY & READ BR BROOKS 5878 881OHC025872 $0.00 94 01 24-Sep-13 23 0000032498 THERMAL LABELING SYS BRADY WORLDWIDE TLS2200 BPTLS902745018 $0.00 17 106 24-Sep-13 23 0000106857 RECIRCULATOR POLYSCI POLY SCIENCE N0691883 G52197 $0.00 83 242 4-Oct-13 23 0000021812

  17. Table 10.5 Estimated Number of Alternative-Fueled Vehicles in Use and Fuel Consumption, 1992-2010

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

    Estimated Number of Alternative-Fueled Vehicles in Use and Fuel Consumption, 1992-2010 Year Alternative and Replacement Fuels 1 Liquefied Petroleum Gases Compressed Natural Gas Liquefied Natural Gas Methanol, 85 Percent (M85) 3 Methanol, Neat (M100) 4 Ethanol, 85 Percent (E85) 3,5 Ethanol, 95 Percent (E95) 3 Elec- tricity 6 Hydro- gen Other Fuels 7 Subtotal Oxygenates 2 Bio- diesel 10 Total Methyl Tertiary Butyl Ether 8 Ethanol in Gasohol 9 Total Alternative-Fueled Vehicles in Use 11

  18. Table 11.2c Carbon Dioxide Emissions From Energy Consumption: Industrial Sector, 1949-2011 (Million Metric Tons of Carbon Dioxide )

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

    c Carbon Dioxide Emissions From Energy Consumption: Industrial Sector, 1949-2011 (Million Metric Tons of Carbon Dioxide 1) Year Coal Coal Coke Net Imports Natural Gas 3 Petroleum Retail Elec- tricity 8 Total 2 Biomass 2 Distillate Fuel Oil 4 Kero- sene LPG 5 Lubri- cants Motor Gasoline 6 Petroleum Coke Residual Fuel Oil Other 7 Total Wood 9 Waste 10 Fuel Ethanol 11 Total 1949 500 -1 166 41 18 3 3 16 8 95 25 209 120 995 44 NA NA 44 1950 531 (s) 184 51 20 4 3 18 8 110 26 239 140 1,095 50 NA NA 50

  19. Table 11.2d Carbon Dioxide Emissions From Energy Consumption: Transportation Sector, 1949-2011 (Million Metric Tons of Carbon Dioxide )

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

    d Carbon Dioxide Emissions From Energy Consumption: Transportation Sector, 1949-2011 (Million Metric Tons of Carbon Dioxide 1) Year Coal Natural Gas 3 Petroleum Retail Elec- tricity 7 Total 2 Biomass 2 Aviation Gasoline Distillate Fuel Oil 4 Jet Fuel LPG 5 Lubricants Motor Gasoline 6 Residual Fuel Oil Total Fuel Ethanol 8 Biodiesel Total 1949 161 NA 12 30 NA (s) 4 306 91 443 6 611 NA NA NA 1950 146 7 14 35 NA (s) 5 332 95 481 6 640 NA NA NA 1951 129 11 18 42 NA (s) 6 360 102 529 7 675 NA NA NA

  20. Word Pro - Untitled1

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

    1 Table 10.5 Estimated Number of Alternative-Fueled Vehicles in Use and Fuel Consumption, 1992-2010 Year Alternative and Replacement Fuels 1 Liquefied Petroleum Gases Compressed Natural Gas Liquefied Natural Gas Methanol, 85 Percent (M85) 3 Methanol, Neat (M100) 4 Ethanol, 85 Percent (E85) 3,5 Ethanol, 95 Percent (E95) 3 Elec- tricity 6 Hydro- gen Other Fuels 7 Subtotal Oxygenates 2 Bio- diesel 10 Total Methyl Tertiary Butyl Ether 8 Ethanol in Gasohol 9 Total Alternative-Fueled Vehicles in Use

  1. Word Pro - Untitled1

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

    7 Table 11.2c Carbon Dioxide Emissions From Energy Consumption: Industrial Sector, Selected Years, 1949-2011 (Million Metric Tons of Carbon Dioxide 1 ) Year Coal Coal Coke Net Imports Natural Gas 3 Petroleum Retail Elec- tricity 8 Total 2 Biomass 2 Distillate Fuel Oil 4 Kero- sene LPG 5 Lubri- cants Motor Gasoline 6 Petroleum Coke Residual Fuel Oil Other 7 Total Wood 9 Waste 10 Fuel Ethanol 11 Total 1949 500 -1 166 41 18 3 3 16 8 95 25 209 120 995 44 NA NA 44 1950 531 (s) 184 51 20 4 3 18 8 110

  2. Word Pro - Untitled1

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

    8 U.S. Energy Information Administration / Annual Energy Review 2011 Table 11.2d Carbon Dioxide Emissions From Energy Consumption: Transportation Sector, Selected Years, 1949-2011 (Million Metric Tons of Carbon Dioxide 1 ) Year Coal Natural Gas 3 Petroleum Retail Elec- tricity 7 Total 2 Biomass 2 Aviation Gasoline Distillate Fuel Oil 4 Jet Fuel LPG 5 Lubricants Motor Gasoline 6 Residual Fuel Oil Total Fuel Ethanol 8 Biodiesel Total 1949 161 NA 12 30 NA (s) 4 306 91 443 6 611 NA NA NA 1950 146 7

  3. Richard Gerber Helen He, Zhengji Zhao, Chris Daley NUG Monthly

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

    Helen He, Zhengji Zhao, Chris Daley NUG Monthly Meeting --- 1 --- NUG M onthly M ee-ng October 2 , 2 014 Agenda * Hopper and Edison Status Updates * ERCAP ( Alloca-ons) U pdate * Queue C ommiIee T opics * NUGEX Elec-ons * NUG 2 015 M ee-ng P lanning * Mini---Seminar: S teps t o i mprove t he p erformance o f a h ydrodynamics a pplica-on o n t he I ntel M IC architecture --- 2 --- Edison Update" Zhengji Zhao, User Services --- 3 --- Edison Updates * 9/25 7 :30 P DT --- 9 /28 1 :30 P DT D IMM

  4. Released: June 2006

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

    3. Cooking Energy Sources, Number of Buildings and Floorspace for Non-Mall Buildings, 2003" ,"Number of Buildings (thousand)",,,,,"Total Floorspace (million square feet)" ,"All Build- ings*","Build- ings with Cooking","Cooking Energy Sources (more than one may apply)",,,"All Build- ings*","Build- ings with Cooking","Cooking Energy Sources (more than one may apply)" ,,,"Elec- tricity","Natural

  5. Table 3. Top Five Retailers of Electricity, with End Use Sectors, 2014

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

    Five Retailers of Electricity, with End Use Sectors, 2014" "Alaska" "megawatthours" ,"Entity","Type of Provider","All Sectors","Residential","Commercial","Industrial","Transportation" 1,"Golden Valley Elec Assn Inc","Cooperative",1219363,276627,129773,812963,0 2,"Chugach Electric Assn Inc","Cooperative",1134527,513748,563581,57198,0 3,"Anchorage Municipal

  6. Recent Development of SOFC Metallic Interconnect

    SciTech Connect (OSTI)

    Wu JW, Liu XB

    2010-04-01

    Interest in solid oxide fuel cells (SOFC) stems from their higher eciencies and lower levels of emitted pollu- tants, compared to traditional power production methods. Interconnects are a critical part in SOFC stacks, which connect cells in series electrically, and also separate air or oxygen at the cathode side from fuel at the anode side. Therefore, the requirements of interconnects are the most demanding, i:e:, to maintain high elec- trical conductivity, good stability in both reducing and oxidizing atmospheres, and close coecient of thermal expansion (CTE) match and good compatibility with other SOFC ceramic components. The paper reviewed the interconnect materials, and coatings for metallic interconnect materials.

  7. "Table B27. Space Heating Energy Sources, Floorspace for Non-Mall Buildings, 2003"

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

    7. Space Heating Energy Sources, Floorspace for Non-Mall Buildings, 2003" ,"Total Floorspace (million square feet)" ,"All Buildings*","Buildings with Space Heating","Space-Heating Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","Propane","Other a" "All Buildings* ...............",64783,60028,28600,36959,5988,5198,3204,842

  8. "Table B32. Water-Heating Energy Sources, Floorspace for Non-Mall Buildings, 2003"

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

    2. Water-Heating Energy Sources, Floorspace for Non-Mall Buildings, 2003" ,"Total Floorspace (million square feet)" ,"All Buildings*","Buildings with Water Heating","Water-Heating Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","Propane" "All Buildings* ...............",64783,56478,27490,28820,1880,3088,1422 "Building

  9. Buildings*","Buildings

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

    6. Space Heating Energy Sources, Number of Buildings for Non-Mall Buildings, 2003" ,"Number of Buildings (thousand)" ,"All Buildings*","Buildings with Space Heating","Space-Heating Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","Propane","Other a" "All Buildings* ...............",4645,3982,1766,2165,360,65,372,113

  10. Buildings*","Buildings

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

    1. Water-Heating Energy Sources, Number of Buildings for Non-Mall Buildings, 2003" ,"Number of Buildings (thousand)" ,"All Buildings*","Buildings with Water Heating","Water-Heating Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","Propane" "All Buildings* ...............",4645,3472,1910,1445,94,27,128 "Building Floorspace"

  11. Buildings*","Buildings Using Any Energy

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

    2. Energy Sources, Number of Buildings for Non-Mall Buildings, 2003" ,"Number of Buildings (thousand)" ,"All Buildings*","Buildings Using Any Energy Source","Energy Sources Used (more than one may apply)" ,,,"Elec- tricity","Natural Gas","Fuel Oil","District Heat","District Chilled Water","Propane","Other a " "All Buildings*

  12. EC Publications

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

    China Lake Naval Air Stationadmin2016-04-18T20:58:24+00:00 Popular Downloads Solar Energy ... China Lake, CA was a chosen site for one Plug Power GenSysTM 5CS-5kW PEM fuel cell. The ...

  13. Auto-Versioning Systems Image Manager

    Energy Science and Technology Software Center (OSTI)

    2013-08-01

    The av_sys_image_mgr utility provides an interface for the creation, manipulation, and analysis of system boot images for computer systems. It is primarily intended to provide a convenient method for managing the introduction of changes to boot images for long-lived production HPC systems.

  14. Cyber Securing Control Systems

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

    ... WorkPlace Tech 5.7.2 TAC 4.1 TAC Signal, XPSI & ZPSIPC Teletrol eBuilding Telvent OaSys DNA 7.4.* Trane Tracer SC Tracer 3.5 Trane Tracer Summit Tracer 11 Trane Tracer Summit ...

  15. Lean Gasoline System Development for Fuel Efficient Small Car

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

    ... SCR-4 Passive Sys GM SCR-5 Supplier Data SCR-5 Modified SCR 1 Cone SCR-6 "Torpedo" SCR eta SCR-4 NH3 slip Post SCR1 SCR-5 NH3 slip Post SCR1 SCR-6 "Torpedo" Slip ; NOx conversion ...

  16. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    of w -1.07sub -0.09sup +0.09 (stat 1sigma) +- 0.13 (sys), Omegasub M 0.267sub -0.018sup +0.028 (stat 1sigma) with a best-fit chisup 2DoF of 0.91. The...

  17. COMPNAME","COMPID","YEAR","PLANTNAME","KIND","CONSTRUC","INSTALLED","MAXCAP","NE

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

    EQUIP","TOTCOST","COSTCAP","GROSSEXP","OPERENG","FUEL","COOLANTS","STEXP","STOTH","STTRANS","ELECEXP","MISCST","RENTS","MAINSUP","MAINSTRUC","MAINBOIL","MAINELEC","MAINMISC","TOTPROD","EXPKWH","UNITCL","QUANTCL","AVGHEATCL","ACDELCL","ACBURNCL","ACBTUCL","ACNETGENCL","ABTUNETGCL","UNITGAS","QUANTGAS","AVGHEATGAS","ACDELGAS","ACBURNGAS","ACBTUGAS","ACNETGNGAS","ABTUNETGAS","UNITOIL","QUANTOIL","AVGHEATOIL","ACDELOIL","ACBURNOIL","ACBTUOIL","ACNETGNOIL","ABTUNETOIL" "Tennessee Valley Authority",18642,1999,"Sequoyah","Nuclear","01/01/81",,2441160,2303000,8760,1008,1.8570502e+10,3184031,533636867,2488511062,3025331960,1239,33187938,21080862,86166618,4316783,11925073,0,0,13329621,28360769,0,16330987,1528775,8295886,3650336,7012139,201997849,11,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"MillionBTU",189924066,0,0,0,0.43,0.04,10230 "Tennessee Valley Authority",18642,1999,"Watts Bar","Nuclear","01/01/96","1/1/1996",1269000,1200000,8208,728,8230350000,1953589,2108999339,4827648621,6938601549,5468,30551823,12179502,38261150,3963151,7056493,0,0,10400580,24553068,0,14243155,2328791,9244870,870737,990214,124091711,15,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"MillionBTU",84467683,0,0,0,0.43,0.04,10260 "Tennessee Valley Authority",18642,1999,"Johnsonville","Gas Turbine","01/01/75","1/1/1975",1088000,1407000,8760,14,256798000,0,6064116,119609619,125673735,116,112893140,2747882,9870790,0,0,0,0,0,477926,0,2274,1326,0,475339,7436,13582973,53,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"Gallons",24224936,139600,0,0.41,0.03,0,13170 "Tennessee Valley Authority",18642,1999,"Gallatin","Gas Turbine","01/01/75","1/1/1975",325200,431000,8760,8,176258000,0,3324533,63486109,66810642,205,80539157,665541,6810251,0,0,0,0,0,151587,0,1339166,1553,0,3922,4338,8976358,51,,0,0,0,0,0,0,0,"Mcf",2252179,1024,0,2.67,2.61,0,0,"Gallons",2063233,139100,0,0.37,0,0.03,14710 "Tennessee Valley Authority",18642,1999,"Browns Ferry","Nuclear","01/01/74","1/1/1977",3456000,2529000,8760,1085,1.771301e+10,890631,909522117,3830292072,4740704820,1372,47061477,58344025,102890781,3642332,11672365,0,0,16130309,26099224,0,5560106,0,25822517,1921329,0,252082988,14,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"MillionBTU",186421503,0,0,0,0.53,0,10520 "Tennessee Valley Authority",18642,1999,"Cumberland","Steam","01/01/73","1/1/1973",2600000,2591000,8760,323,1.6530325e+10,1829568,103903145,1638681020,1744413733,671,63827428,5077791,197194700,0,86656,0,0,3945,13987241,0,1210473,1306476,16946838,4232440,841362,240887922,15,"Tons",6868849,10459,26.16,27.86,1.2,0.01,9746,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Thomas H. Allen","Gas Turbine","01/01/71","1/1/1972",820300,622000,8760,9,264695000,0,3063638,102977658,106041296,129,1709273,879771,11709062,0,0,0,0,0,72128,0,301000,0,0,150309,2816,13115086,50,,0,0,0,0,0,0,0,"Mcf",3589538,1024,0,3.06,3.03,0,0,"Gallons",1173222,139500,0,0.55,0,0.03,14460 "Tennessee Valley Authority",18642,1999,"Colbert","Gas Turbine","01/01/72","1/1/1972",476000,420000,8760,7,326221000,0,2826177,64911682,67737859,142,3078759,1248563,12167389,0,0,0,0,0,69117,0,27275,0,0,74,2699,13515117,41,,0,0,0,0,0,0,0,"Mcf",3866688,1024,0,2.8,2.71,0,0,"Gallons",3619161,138400,0,0.35,0,0.03,13670 "Tennessee Valley Authority",18642,1999,"Bull Run","Steam","01/01/67","1/1/1967",950000,912000,8760,87,4389788000,2220883,35786684,300943172,338950739,357,21987402,2324904,50419615,0,2286709,0,0,1742,6906593,0,754423,481980,8505768,2788903,314448,74785085,17,"Tons",1593346,11895,28.85,30.74,1.24,0.01,9257,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Thomas H. Allen","Steam","01/01/59","1/1/1959",990000,858000,8760,122,4102572000,142024,73025058,451231229,524398311,530,20254094,1206283,60294160,0,16,0,0,0,9854407,0,392524,824748,8011764,5402527,184253,86170682,21,"Tons",2039487,9680,25.5,29.45,1.39,0.01,10585,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Watts Bar","Steam","01/01/42","1/1/1945",240000,0,8760,0,-1381000,11997,4933530,18578656,23524183,98,-6629,177,0,0,0,0,0,0,109802,0,908,5,0,0,0,110892,-80,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Paradise","Steam","01/01/63","1/1/1970",2558200,2286000,8760,296,1.4181992e+10,8519495,115906466,1287447341,1411873302,552,57696636,6093708,168293657,0,752026,0,0,536,10779025,0,3529172,4127133,18094770,3094627,676700,215441354,15,"Tons",6332104,10413,21.43,26.2,1.14,0.01,10280,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Gallatin","Steam","01/01/56","1/1/1959",1255200,992000,8760,131,7002818000,690082,44703289,427469961,472863332,377,5073325,1612720,80238724,0,1258244,0,0,73323,7350012,0,1803476,714460,6039653,3054984,792751,102938347,15,"Tons",3266195,9540,22.99,24.49,1.19,0.01,9651,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"John Sevier","Steam","01/01/55","1/1/1957",800000,748000,8760,129,5522165000,1570328,37309270,253176616,292056214,365,2993416,946133,70531483,0,3286201,0,0,0,4864155,0,569877,953882,3537596,666934,559907,85916168,16,"Tons",2120222,11710,32.44,33.21,1.3,0.01,9802,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Kingston","Steam","01/01/54","1/1/1955",1700000,1583000,8760,275,1.0147089e+10,3475653,55125946,433125237,491726836,289,31839874,1201130,133624099,0,732904,0,0,671,15993919,0,2888077,697638,10886872,3114678,359796,169499784,17,"Tons",4038449,11134,31.75,32.96,1.34,0.01,9845,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Colbert","Steam","01/01/55","1/1/1965",1350000,1283000,8760,222,6557785000,279029,50717782,608908796,659905607,489,12808186,3684548,92134159,0,115314,0,0,3096,11894009,0,1552144,1216679,16776178,4392373,150021,131918521,20,"Tons",2890398,10787,27.4,31.47,1.38,0.01,10066,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Shawnee","Steam","01/01/53","1/1/1956",1750000,1368000,8760,264,8060005000,504507,64076435,534941906,599522848,343,20760203,5379072,113531307,0,6565666,0,0,278,7470171,0,2988378,2163530,11022440,5415043,396055,154931940,19,"Tons",3766896,10234,28.54,29.83,1.34,0.01,10474,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Johnsonville","Steam","01/01/51","1/1/1959",1485200,1213000,8760,269,6638234000,87967,76839994,522564850,599492811,404,5328716,12443723,83697340,0,-481100,0,0,6321,6501533,0,2973740,1891947,6444598,2867797,430252,116776151,18,"Tons",2922958,11389,26.49,28.52,1.16,0.01,10912,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Tennessee Valley Authority",18642,1999,"Widows Creek","Steam","01/01/52","1/1/1965",1968760,1652000,8760,332,8498846000,855691,74795817,748521437,824172945,419,22653730,3695032,119092329,0,6555644,0,0,1697,9854746,0,1449646,2594983,13869309,4635675,4932791,166681852,20,"Tons",3858785,10808,28.8,30.16,1.27,0.01,10896,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"PALO VERDE 17.49%","n","01/01/86","01/01/88",666364,659000,8760,0,5317709000,1244457,281584974,735793972,1018623403,1529,6013000,4282694,25651422,2986065,4032493,0,0,2276671,26939892,0,5837013,1933729,6303817,3749209,2418208,86411213,16,,0,0,0,0,0,0,0,"BBTU",57406,0,0,440.13,0.44,0.01,10795,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"San Tan","Combined Cy","01/01/74","01/01/75",414000,292000,4112,43,714062000,149179,2773141,65463525,68385845,165,-5000,380221,14107193,0,1594474,0,0,0,845877,0,332730,170816,0,7389209,249749,25070269,35,,0,0,0,0,0,0,0,"MCF",6579686,1017,2.12,2.12,2.08,0.02,9372,"BBL",291,485968,0,24.61,4.22,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"SOLAR PV1 & PV2","So1ar","01/01/98","01/01/98",216,100,3000,0,119493,0,0,1676818,1676818,7763,1852000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"KYRENE","Steam","01/01/52","01/01/54",108000,106000,736,12,50072000,313326,2433283,15283485,18030094,167,726000,180057,1483303,0,338591,0,0,169009,304652,0,157896,27729,608781,344347,214929,3829294,76,,0,0,0,0,0,0,0,"MCF",651225,1016,2.16,2.16,2.12,0.03,13215,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"KYRENE","Gas Turbine","01/01/71","01/01/73",226850,149000,290,0,18990000,0,0,16888448,16888448,74,0,114913,724438,0,85074,0,0,0,40298,0,64493,11249,0,291038,96634,1428137,75,,0,0,0,0,0,0,0,"MCF",281631,1017,2.09,2.09,2.06,0.04,15094,"BBL",60,488889,0,24.61,4.19,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"MOHAVE 10%","Steam","01/01/71","01/01/71",163620,158000,8715,0,996913000,42812,5046928,50920964,56010704,342,1221000,250561,13703464,0,389195,0,0,245787,1776796,-12611,497248,178489,1673455,685271,112185,19499840,20,"Tons",457815,10939,28.47,29.64,1.35,0.01,10093,"MCF",45107,1028,0,2.94,2.86,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"CORONADO","Steam","01/01/79","01/01/80",821880,760000,8760,213,5039392000,8300198,158523884,696108809,862932891,1050,7523000,1228492,96325127,0,4607490,0,0,403466,4002498,10446,1754276,1703703,12035645,3902862,1238765,127212770,25,"Tons",2632698,9886,34.53,35.42,1.79,0.02,10357,,0,0,0,0,0,0,0,"BBL",24155,137315,24.21,26.79,4.65,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"CRAIG 29%","Steam","01/01/79","01/01/81",259414,248000,8760,0,2050747000,83589,52424794,181936864,234445247,904,680000,368849,22362014,0,1036824,0,0,425951,1689040,12271,323682,251566,1760910,701820,370069,29302996,14,"Coal",1040589,10060,22.56,21.42,1.06,0.01,10223,"MCF",28100,1000,0,2.49,2.49,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"CROSS CUT","Steam","01/01/42","01/01/49",30000,3000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"MCF",0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"NAVAJO 21.7%","Steam","01/01/74","01/01/76",522857,488000,8760,539,3676183000,42866,27115117,246304509,273462492,523,5605000,1396220,45545213,0,1123640,0,0,257918,3750053,132023,667722,165042,7069421,2110905,434407,62652564,17,"Tons",1685726,10956,23.51,26.74,1.22,0.01,10061,,0,0,0,0,0,0,0,"BBL",8625,139078,22.75,28.63,4.9,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"NAVAJO 100%","Steam","01/01/74","01/01/76",2409480,2250000,8760,539,1.6020912e+10,197537,124954457,1135043822,1260195816,523,25829493,6236459,196347455,0,5554459,0,0,1293757,8406791,0,3306198,769371,29759456,10024854,2263428,263962228,16,"Tons",7339290,10979,23.5,26.63,1.21,0.01,10074,,0,0,0,0,0,0,0,"BBL",39756,139079,22.75,22.47,3.85,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"FOUR CORNERS 10%","Steam","01/01/69","01/01/70",163620,148000,8760,0,1176172000,11573,7334703,91939839,99286115,607,37000,105696,11684589,0,978340,0,0,90099,1040379,83795,135949,61864,1112429,291525,340786,15925451,14,"Tons",644302,8885,17.41,17.97,1.01,0.01,9757,"MCF",26430,1008,0,4.13,4.1,0,0,,0,0,0,0,0,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"HAYDEN 50%","Steam","01/01/76","01/01/76",137700,131000,6809,0,812423000,482702,13855905,64632670,78971277,574,16419000,157050,8427442,0,469402,0,0,101091,1360780,0,245277,92834,431566,123971,241674,11651087,14,"Tons",413486,10561,22.49,20.28,0.96,0.01,10759,,0,0,0,0,0,0,0,"BBL",1248,138870,26.63,32.67,5.6,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"AGUA FRIA","Steam","01/01/57","01/01/61",390472,407000,4062,62,888092000,139014,5833721,51714773,57687508,148,23000,345003,21091146,0,1032200,0,0,1186582,715713,0,741888,530777,2232219,897096,413430,29186054,33,,0,0,0,0,0,0,0,"MCF",9553025,1009,2.14,2.14,2.12,0.02,10859,"BBL",3,500000,0,24.61,4.1,0,0 "Salt River Proj Ag I & P Dist",16572,1999,"AGUA FRIA","Gas Turbine","01/01/74","01/01/75",222950,197000,451,0,42223000,0,299904,22692012,22991916,103,0,108584,1469697,0,233742,0,0,0,36481,0,284381,9332,0,296342,34359,2472918,59,,0,0,0,0,0,0,0,"MCF",617372,1007,2.12,0,2.1,0.03,14371,,0,0,0,0,0,0,0 "Alexandria City",298,1999,,"STEAM","01/01/56","01/01/74",171000,170000,5326,20,194429,0,0,0,0,0,0,708998,0,0,0,0,0,0,0,0,199997,14994,0,404462,0,1328451,6833,,0,0,0,0,0,0,0,"MCF",2346281,10,2.24,2.24,2.14,0.03,12.45,,0,0,0,0,0,0,0 "Ames City of",554,1999,,"STEAM","01/01/50",,102500,103000,8760,45,381623000,0,0,0,0,0,0,4120850,6152121,0,0,0,0,0,0,0,0,0,0,0,0,10272971,27,,239196,8800,25.72,25.72,1.46,0.02,11031,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Ames City of",554,1999,,"GAS TURBINE","01/01/72","1/1/1972",22000,18000,95,0,1007000,0,0,0,0,0,0,9422,53460,0,0,0,0,0,0,0,0,0,0,0,0,62882,62,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,99000,137300,0.54,0.54,3.93,0.05,13498 "Anaheim City of",590,1999,,"GAS TRUBINE","01/01/90","01/01/91",49270,45998,638,6,27719000,0,9226000,27237000,36463000,740,0,280835,699954,0,0,0,0,0,0,0,187223,0,0,0,1146979,2314991,84,,0,0,0,0,0,0,0,"MCF",258683,1009,2.76,2.76,2.74,25.7,9394,,0,0,0,0,0,0,0 "Anchorage City of",599,1999,"#1","4 Gas 2 Int","01/01/62","01/01/72",85000,33000,1010,14,9983618,80839,3457655,22418738,25957232,305,380194,55796,353989,0,0,0,0,809120,0,3922,67280,67353,0,442853,0,1800313,180,,0,0,0,0,0,0,0,273580,0,1000,1.38,1.38,1.38,0.03,19744,778,0,133500,33.82,33.82,6.03,0,0 "Anchorage City of",599,1999,"#2","3 Gas 1 Ste","01/01/75","01/01/84",243200,151000,19516,30,759258360,11240,8928538,75136820,84076598,346,5364843,257796,10642281,0,678572,0,0,1623991,233929,0,330573,231135,303990,1190866,118352,15611485,21,,0,0,0,0,0,0,0,7701758,0,1000,1.38,1.38,1.38,0.01,10144,570,0,133500,34.71,34.71,6.19,0,0 "Austin City of",1009,1999,"Downtown","Gas Turbine","01/01/54","01/01/54",5500,5000,0,0,493000,0,0,1065016,1065016,194,0,142,36663,0,0,0,0,7532,0,0,143,0,0,142049,0,186529,378,,0,0,0,0,0,0,0,"MCF",1347,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Austin City of",1009,1999,"Northeast","Steam","01/01/71","01/01/71",31500,31300,7566,24,120607160,70498,2376720,5711293,8158511,259,0,42490,2760067,0,395223,0,0,366434,798118,0,24135,51518,290200,20129,3652,4751966,39,"TON",58175,12000,39.8,39.48,1.64,0.02,12637,"MCF",125541,1020,2.75,2.75,2.7,0.03,12648,,0,0,0,0,0,0,0 "Austin City of",1009,1999,"Downtown","Steam","01/01/35","01/01/54",27500,22500,465,11,4508000,24099,1221355,5587700,6833154,248,0,31568,193351,0,41643,0,0,12652,492890,0,23781,136549,88433,55977,1897,1078741,239,,0,0,0,0,0,0,0,"MCF",70119,1020,2.75,2.75,2.7,0.04,15874,,0,0,0,0,0,0,0 "Austin City of",1015,1999,"DECKER TURBINES","GAS TURBINE","01/01/88","01/01/88",200000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Austin City of",1015,1999,"DECKER SOLAR","SOLAR","01/01/86","01/01/86",300,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Austin City of",1015,1999,"DECKER","STEAM","01/01/70","01/01/77",726000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Austin City of",1015,1999,"HOLLY","STEAM","01/01/60","01/01/74",558000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Austin City of",1015,1999,"SEAHOLM","STEAM","01/01/51","01/01/55",120000,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Braintree Town of",2144,1999,"Potter II","Gas Turbine","01/01/77","01/01/77",97500,79500,1284,27,72929000,20271,3762859,18429374,22212504,228,132748,176565,2625145,0,1154442,0,0,0,0,0,158096,316309,488498,491410,262035,5672500,78,,0,0,0,0,0,0,0,"MCF",931167,1035,3.03,3.03,2.92,0.03,11631,"BBLS",14190,138809,15.72,15.72,2.7,0.03,10520 "Brownsville Public Utils Board",2409,1999,"SILAS RAY","STEAM GAS T","01/01/46","01/01/77",155000,197000,5256,29,206,528443,4499041,192117166,197144650,1272,0,205477,6239714,0,1311,0,0,155739,309455,0,74856,224382,203068,176038,1264465,8854505,42983034,,0,0,0,0,0,0,0,"MCF",2346974,1059,2.65,2.65,2.5,0.03,12048,,0,0,0,0,0,0,0 "Bryan City of",2439,1999,,"Gas Turbine","01/01/70","01/01/87",39,30,265,8,5177,0,0,0,0,0,0,0,311874,0,0,0,0,499578,0,0,0,0,0,216081,0,1027533,198480,,0,0,0,0,0,0,0,"Mcf",72688,1000,3.8,3.8,3.8,0.06,29839,"Bbl29839",639,128000,55.63,55.63,7.12,0.06,29839 "Bryan City of",2442,1999,"Bryan Municipal","STEAM, GAS","01/01/55","01/01/74",138000,115000,0,20,118273000,0,7590674,7546886,15137560,110,46427,76607,3529286,0,372623,0,0,606045,154868,9320,63805,20315,520977,159461,31344,5544651,47,,0,0,0,0,0,0,0,"MCF",1626575,1,2.25,2.25,2.21,0.03,14.05,,0,0,0,0,0,0,0 "Bryan City of",2442,1999,"Roland C. Dandy","STEAM","01/01/77","01/01/77",105000,106000,0,19,461142000,1183486,10201555,18752019,30137060,287,105283,76291,11510542,0,391030,0,0,512056,181517,12858,53081,31539,405327,91686,57727,13323654,29,,0,0,0,0,0,0,0,"MCF",5120070,1,2.24,2.24,2.21,0.02,11.36,,0,0,0,0,0,0,0 "Burlington City of",2548,1999,"Gas Turbine","Gas Turbine","01/01/71","01/01/71",25500,25000,106,1,2093500,13587,531143,3214616,3759346,147,17164,6073,130467,0,0,0,0,324,5442,16648,0,0,0,75762,0,234716,112,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"BBL",6016,137674,20.61,21.69,3.75,0.06,16616 "Burlington City of",2548,1999,"Joseph C McNeil GenrЬ ","Steam","01/01/84","01/01/84",50,53,4305,48,183109400,278455,18147811,50484579,68910845,1378217,571376,140467,6439721,0,788415,0,0,291816,360657,0,131396,35661,553086,1325161,20193,10086573,55,"Wood-Tons",263762,4750,23.46,23.52,2.47,0.03,13742,"MCF",66041,1012124,2.82,2.82,2.78,0.24,86785,"BBL",2260,136430,20.13,21.19,3.7,0,71.02 "Cedar Falls City of",3203,1999,"Streeter Station","Steam","01/01/63","01/01/73",51500,50000,1650,23,38111600,281328,3758281,14375110,18414719,358,699506,97410,1113417,0,230220,0,0,102634,142771,0,90418,180725,588058,55402,9122,2610177,68,"Tons",19527,12429,38.79,36.49,1.47,0.02,14033.99,"MCF",49410,1000,2.75,2.75,2.75,0.04,14033.99,,0,0,0,0,0,0,0 "Cedar Falls City of",3203,1999,"Combustion Turbine","Combustion","01/01/68","01/01/68",25000,20000,193,0,2814300,70777,134588,3497629,3702994,148,3062,4978,122537,0,0,0,0,5713,0,0,6674,9708,0,32837,0,182447,65,,0,0,0,0,0,0,0,"MCF",50599,1000,2.42,2.42,2.42,0.04,17979.25,,0,0,0,0,0,0,0 "California Dept-Wtr Resources",3255,1999,"Reid Garner #4","Steam-coal","01/01/83","01/01/83",275000,250000,0,96,1597086000,319709000,0,0,319709000,1163,0,0,22054817,0,0,0,0,0,21659183,0,0,0,0,0,0,43714000,27,"Tons",672949,11858,0,13.11,1.31,0.01,11079,,0,0,0,0,0,0,0,"Barrels",7515,133622,0,25,4.55,0.05,11570 "California Dept-Wtr Resources",3255,1999,"BottleRock & S Geysep","Steam-Geoth","01/01/85","01/01/85",55000,0,0,0,0,10000,0,0,10000,0,0,0,0,0,0,0,0,0,553000,0,0,0,0,0,0,553000,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Chanute City of",3355,1999,"Plant #3","Internal Co","01/01/85","01/01/91",31915,39975,595,8,10378156,50000,612000,15500000,16162000,506,0,369525,245371,0,0,0,0,0,0,0,166666,0,0,136912,0,918474,89,"N/A",0,0,0,0,0,0,0,"MCF",78668,1000,2.66,2.66,2.66,0.02,0.02,"Barrels",3969,138000,26.57,26.57,0.08,0.01,0.01 "PUD No 1 of Clark County",3660,1999,"River Road CCCT","Gas Turbine","01/01/97","01/01/97",248000,258504,7058,21,1711891704,1053160,141767983,13187783,156008926,629,2319343,4203148,23066109,0,0,0,0,0,0,0,0,91900,0,0,0,27361157,16,,0,0,0,0,0,0,0,"MCF",11463,1060,2042,2012,1.9,0.01,7114,,0,0,0,0,0,0,0 "Clarksdale City of",3702,1999,,"Combine Cyc","01/01/71","01/01/71",25550,24000,2149,6,43507,0,0,4581109,4581109,179,0,10000,1053091,0,0,0,0,130000,80000,0,10000,0,12009,328580,0,1623680,37320,,0,0,0,0,0,0,0,"MCF",374997,1000,2.8,2.8,2.8,0.02,8.62,"BBL",70,142.5,23.14,23.14,3.86,0.05,13.99 "Clarksdale City of",3702,1999,,"Gas Turbine","01/01/65","01/01/65",11500,11500,754,6,12158,0,0,1445133,1445133,126,0,10000,478409,0,0,0,0,100000,50000,0,20000,0,0,226974,0,885383,72823,,0,0,0,0,0,0,0,"MCF",169662,1000,2.8,2.8,2.8,0.03,13.99,"BBL",115,142.5,23.14,23.14,3.86,0.07,20.18 "Coffeyville City o",3892,1999,"COFFEYVILLE","STEAM","01/01/01","01/01/73",56985,55900,4013,23,68578900,0,0,0,0,0,0,57285,2419645,0,0,0,0,0,1146750,0,0,0,8610,0,0,3632290,53,,0,0,0,0,0,0,0,"MMBTU",938070,1000,2.25,2.58,2.58,0.03,1368,,0,0,0,0,0,0,0 "Coldwater Board of Public Util",3915,1999,,"Steam","01/01/00","01/01/64",11125,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,68864,7301,41,105,51389,127700,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Coldwater Board of Public Util",3915,1999,,"Diesel","01/01/48","01/01/78",13250,45933,1719,6,7081208,0,0,0,0,0,0,40423,214682,0,0,0,0,37863,0,0,0,12739,0,71418,0,377125,53,,0,0,0,0,0,0,0,"Mcf",65604,9530000,2.84,0,0,0,0,"Barrels",1725,126000,17.7,0,0,0,0 "Colorado Springs City of",3989,1999,"Birdsall","Steam-Gas","01/01/53","01/01/57",62500,4500,1717,4,20716000,10761,2593301,11384249,13988311,224,0,67716,1180669,0,107787,0,0,227078,88988,0,31363,89311,290603,224308,38374,2346197,113,,0,0,0,0,0,0,0,"MCF",412714,806,2.83,2.83,3.52,0.06,16212,"GALLONS",22000,137420,0.11,0.11,0.81,0.01,16212 "Colorado Springs City of",3989,1999,"Drake","Steam-Gas","01/01/25","01/01/74",257300,256000,8760,106,1484262000,2725551,23014851,80547185,106287587,413,0,1059853,25816108,0,1094453,0,0,3228406,1184954,0,462905,237248,4111443,1735831,152472,39083673,26,"TONS",769313,10914,29.13,31.49,1.44,0.01,11585,"MCF",494125,808,2.73,2.73,3.38,0.03,11585,"BARRELS",0,0,0,0,0,0,0 "Colorado Springs City of",3989,1999,"Nixon","Steam-Gas","01/01/80","01/01/80",207000,214000,6081,81,1117841000,5059222,39785705,107090082,151935009,734,0,969721,11571054,0,779121,0,0,1343687,1057607,0,489855,218501,3309067,2974204,146609,22859426,20,"TONS",538337,10432,18.31,18.84,0.9,0,10120,,0,0,0,0,0,0,0,"BARRELS",13952,136738,24.87,24.87,4.33,0.04,10120 "Colorado Springs City of",3989,1999,"CTS","Gas","01/01/99","01/01/99",71660,73000,458,0,22292000,418573,123167,32084223,32625963,455,0,0,715385,0,0,0,0,0,0,0,0,0,0,26204,0,741589,33,,0,0,0,0,0,0,0,"MCF",291394,983,2.89,2.87,2.92,0.03,12852,,0,0,0,0,0,0,0 "Columbia City of",4045,1999,,"Steam/Gas T","01/01/10","01/01/70",86000,226000,8760,46,62152000,115894,3578025,15986526,19680445,229,5320808,43503,2133251,0,531664,0,0,967929,376491,0,170114,28005,512239,452108,0,5215304,84,"Tons",37319,13265,53.83,53.69,2.02,3.22,15930,"Mcf",34179,0,3.64,3.64,0,0,0,,0,0,0,0,0,0,0 "Columbus City of",4065,1999,"O'Shaughnessy",,,,5000,5000,0,1,5860000,0,0,0,0,0,0,0,0,0,0,0,0,49898,0,0,0,0,0,2864,0,52762,9,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Concord City of",4150,1999,,,,,0,0,0,0,545243,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Connecticut Mun Elec Engy Coop",4180,1999,"Millstone Unit 3","Nuclear (e)","01/01/86","01/01/86",1253100,1164700,7329,933,8277624400,0,20415627,29930688,50346315,40,0,324496,363329,24201,162455,0,0,48209,296706,13608,313554,74201,315415,228127,1354,2165655,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Dalton City of",4744,1999,"Wansley 1 & 2","Coal fired","01/01/76","01/01/78",22220,0,0,0,149590620,0,0,9113036,9113036,410,28304,29233,2186381,0,24950,0,0,15863,81536,0,42895,19710,138435,167350,13819,2720172,18,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Dalton City of",4744,1999,"Scherer 1 & 2","Coal fired","/ /","01/01/84",22680,0,0,0,144814966,0,0,13467749,13467749,594,50818,27106,2605498,0,25617,0,0,15303,77539,0,34949,22981,256897,16076,11927,3093893,21,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Denton City of",5063,1999,"SPENCER PLANT","STEAM","01/01/55","01/01/73",179000,259100,11980,36,305539695,0,0,0,0,0,0,233373,9138796,0,348227,0,0,468112,432003,0,71604,11794,211613,467529,210327,11593378,38,,0,0,0,0,0,0,0,"Mcf",3800668,1,2.24,2.24,2.24,2.99,12.43,"BBl",0,139.68,7.82,0,0,0,0 "Eugene City of",6022,1999,"Willamette","Steam","01/01/31","01/01/50",25000,0,0,0,0,0,0,1189332,1189332,48,0,0,260,0,1204,0,0,-975,0,0,0,0,0,5095,7459,13043,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Eugene City of",6022,1999,"Energy Center","Steam","01/01/76","01/01/76",51200,41000,0,0,192829000,1280,320371,7521672,7843323,153,0,13058,1366594,0,0,0,0,261785,0,0,0,94,0,127793,0,1769324,9,,0,0,0,0,0,0,0,,321587,0,2.51,0,0,0,2495.24,,0,0,0,0,0,0,0 "Farmington City of",6204,1999,"ANIMAS","STEAM-COMBI","01/01/55","01/01/94",32180,28000,7808,14,170805000,5968,1109574,25033191,26148733,813,0,70145,3611891,0,225548,0,0,460952,226694,0,122984,0,217797,1021413,38103,5995527,35,,0,0,0,0,0,0,0,"MCF",1668856,1013,2.13,2.13,2.1,0.02,9897,,0,0,0,0,0,0,0 "Farmington City of",6204,1999,"SAN JUAN","STEAM-COAL","/ /","/ /",4300042200,43000,7919,10,293222700,0,5471749,62874731,68346480,0,0,71242,5641682,0,114021,0,0,120758,93838,131,62021,34762,382623,77158,65298,6663534,23,"TONS",167448,9421,32.33,32.33,1.72,0.01,10774,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Fayetteville Public Works Comm",6235,1999,"Butler-Warner Gen PtP","Gas-Turbine","01/01/76","01/01/88",303400,276500,1134,33,0,749336,5123088,100277060,106149484,350,4108529,0,-6665,0,0,0,0,0,0,0,0,0,0,292639,-141172,144802,0,,0,0,0,0,0,0,0,"Mcf",1724674,1046,2.72,2.72,2.6,0.03,12249.5,"Barrels",4,138800,27.15,27.87,4.78,0.06,13375.25 "Fort Pierce Utilities Auth",6616,1999,"Steam","Steam","01/01/21","01/01/89",120011,0,0,0,0,0,0,0,0,0,0,564929,6990,0,231196,0,0,428922,138247,0,21508,56082,204594,1437831,87424,3177723,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0 "Freeport Village of Inc",6775,1999,"Power Plant #1","Internal Co",,"01/01/64",13190,0,0,9,2066120,5022,1113459,3036221,4154702,315,51721,42612,209909,0,0,0,0,518539,0,0,0,79604,0,0,0,850664,412,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"Barrels",293755,138788,0.81,0.68,0.18,0.97,14.88 "Freeport Village of Inc",6775,1999,"Power Plant #2","Internal Co","1/1/1968","01/01/73",37390,57000,1,9,1277200,1827,3178208,8088951,11268986,301,0,52596,205053,0,0,0,0,634322,0,28573,0,101784,0,0,0,1022328,800,,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,"Barrels",319336,138788,0.86,0.64,0.13,0.16,9.2 "Fremont City of",6779,1999,"Wright","Steam","01/01/56","01/01/76",132700,83390,8760,47,336075,202231,5905920,42850719,48958870,369,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,,0,0,0,0,0,0,0,,0,0,0,0,0

  18. Measurement of the cosmic ray spectrum above 4×1018 eV using inclined events detected with the Pierre Auger Observatory

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Aab, Alexander

    2015-08-26

    A measurement of the cosmic-ray spectrum for energies exceeding 4×1018 eV is presented, which is based on the analysis of showers with zenith angles greater than 60° detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.3×1018 eV, the ``ankle'', the flux can be described by a power law E–γ with index γ=2.70 ± 0.02 (stat) ± 0.1 (sys) followed by a smooth suppression region. For the energy (Es) at which the spectral flux has fallen to one-half of its extrapolated value inmore » the absence of suppression, we find Es=(5.12±0.25 (stat)+1.0–1.2 (sys))×1019 eV.« less

  19. Measurement of the cosmic ray spectrum above 4$\\times$10$^{18}$ eV using inclined events detected with the Pierre Auger Observatory

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Aab, Alexander; et al.

    2015-08-26

    A measurement of the cosmic-ray spectrum for energies exceeding 41018 eV is presented, which is based on the analysis of showers with zenith angles greater than 60 detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.31018 eV, the ``ankle'', the flux can be described by a power law E? with index ?=2.70 0.02 (stat) 0.1 (sys) followed by a smooth suppression region. For the energy (Es) at which the spectral flux has fallen to one-half of its extrapolated value inmorethe absence of suppression, we find Es=(5.120.25 (stat)+1.01.2 (sys))1019 eV.less

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

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

    11121-5503-01 RPSEA Sugar Land, TX GE Global Research, Niskayuna, Schenectady, NY (Modified CX only applies to GE Global Research activities) FE/TDIC/Oil & Gas/Natural Gas Team Bill Fincham Intelligent BOP RAM Actuation Sensor System (Project Modifications) Eval sensing approaches for instr. BOPs (blow out preventer), design, build,and test prototype sensing sys,dev land-based rig-test ready software and electronics and perform preliminary product assesment Bill Fincham Digitally signed by

  1. Measurement of ratio R = (BR(D{sup 0}{yields}K{pi}{pi}{pi})/BR(D{sup 0}{yields}K{pi})) in {pi}{sup -}-Nucleus interactions at 500 GeV/c

    SciTech Connect (OSTI)

    Solano Salinas, C. J.; Paucarchuco, C.; Fernandez, A.; Sheaff, M.

    2007-10-26

    We report a very preliminary result on the measurement of the ratio of branching ratios, for two decays D{sup 0} meson, R = (BR(D{sup 0}{yields}K{pi}{pi}{pi})/BR(D{sup 0}{yields}K{pi})), using data from the E791 experiment. We find R = 1.96{+-}0.0286 (stat){+-}0.06 (sys). This is in agreement with and of similar precision to the current PDG average value 1.97{+-}0.09.

  2. NV PFA - Steptoe Valley

    SciTech Connect (OSTI)

    Jim Faulds

    2015-10-29

    All datasets and products specific to the Steptoe Valley model area. Includes a packed ArcMap project (.mpk), individually zipped shapefiles, and a file geodatabase for the northern Steptoe Valley area; a GeoSoft Oasis montaj project containing GM-SYS 2D gravity profiles along the trace of our seismic reflection lines; a 3D model in EarthVision; spreadsheet of links to published maps; and spreadsheets of well data.

  3. 2009 High Temperature Membrane Working Group Meeting Archives | Department

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

    of Energy 9 High Temperature Membrane Working Group Meeting Archives 2009 High Temperature Membrane Working Group Meeting Archives View information from meetings of the High Temperature Membrane Working Group held in 2009. November 16, 2009, Palm Springs, California This meeting was held in conjunction with the Fuel Cell Seminar. Minutes U.S. Fuel Cell Council: The Voice of the Fuel Cell Industry Membrane Requirements for Back-up Power Applications, Michael Hicks, IdaTech GenSys Blue: Fuel

  4. Improved DC Gun Insulator Assembly

    SciTech Connect (OSTI)

    Sah, R.; Dudas, A.; Neubauer, M. L.; Poelker, M.; Surles-Law, K. E.L.

    2010-05-23

    Many user facilities such as synchrotron radiation light sources and free electron lasers require accelerating structures that support electric fields of 10-100 MV/m, especially at the start of the accelerator chain where ceramic insulators are used for very high gradient DC guns. These insulators are difficult to manufacture, require long commissioning times, and often exhibit poor reliability. Two technical approaches to solving this problem will be investigated. Firstly, inverted ceramics offer solutions for reduced gradients between the electrodes and ground. An inverted design will be presented for 350 kV, with maximum gradients in the range of 5-10 MV/m. Secondly, novel ceramic manufacturing processes will be studied, in order to protect triple junction locations from emission, by applying a coating with a bulk resistivity. The processes for creating this coating will be optimized to provide protection as well as be used to coat a ceramic with an appropriate gradient in bulk resistivity from the vacuum side to the air side of an HV standoff ceramic cylinder. Example insulator designs are being computer modelled, and insulator samples are being manufactured and tested

  5. Accelerating Acceptance of Fuel Cell Backup Power Systems - Final Report

    SciTech Connect (OSTI)

    Petrecky, James; Ashley, Christopher

    2014-07-21

    Since 2001, Plug Power has installed more than 800 stationary fuel cell systems worldwide. Plug Power’s prime power systems have produced approximately 6.5 million kilowatt hours of electricity and have accumulated more than 2.5 million operating hours. Intermittent, or backup, power products have been deployed with telecommunications carriers and government and utility customers in North and South America, Europe, the United Kingdom, Japan and South Africa. Some of the largest material handling operations in North America are currently using the company’s motive power units in fuel cell-powered forklifts for their warehouses, distribution centers and manufacturing facilities. The low-temperature GenSys fuel cell system provides remote, off-grid and primary power where grid power is unreliable or nonexistent. Built reliable and designed rugged, low- temperature GenSys delivers continuous or backup power through even the most extreme conditions. Coupled with high-efficiency ratings, low-temperature GenSys reduces operating costs making it an economical solution for prime power requirements. Currently, field trials at telecommunication and industrial sites across the globe are proving the advantages of fuel cells—lower maintenance, fuel costs and emissions, as well as longer life—compared with traditional internal combustion engines.

  6. CHP Fuel Cell Durability Demonstration - Final Report

    SciTech Connect (OSTI)

    Petrecky, James; Ashley, Christopher J

    2014-07-21

    Plug Power has managed a demonstration project that has tested multiple units of its high-temperature, PEM fuel cell system in micro-combined heat and power (μ-CHP) applications in California. The specific objective of the demonstration project was to substantiate the durability of GenSys Blue, and, thereby, verify its technology and commercial readiness for the marketplace. In the demonstration project, Plug Power, in partnership with the National Fuel Cell Research Center (NFCRC) at the University of California, Irvine (UCI), and Sempra, will execute two major tasks: • Task 1: Internal durability/reliability fleet testing. Six GenSys Blue units will be built and will undergo an internal test regimen to estimate failure rates. This task was modified to include 3 GenSys Blue units installed in a lab at UCI. • Task 2: External customer testing. Combined heat and power units will be installed and tested in real-world residential and/or light commercial end user locations in California.

  7. NERSC Staff

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

    Staff Introduction to OpenMP Programming Agenda * Basic i nforma,on - An s elec(ve i ntroduc(on t o t he p rogramming m odel. - Direc(ves f or w ork p aralleliza(on a nd s ynchroniza(on. - Some h ints o n u sage * Hands---on Lab - Wri(ng c ompiling a nd e xecu(ng s imple O penMP programs. * Presenta,on a vailable a t - module load training! - cp $EXAMPLES/NUG/Presentations/ IntroToOpenMP.pptx! Agenda * New stuff - Constructs i ntroduced i n OpenMP 3 .0 * Not t asking * Hands---on Lab What is

  8. 2014 YWC Gallery | Princeton Plasma Physics Lab

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

    Commercial (Data from forms EIA-861- schedules 4A & 4D and EIA-861S) Entity State Ownership Customers (Count) Sales (Megawatthours) Revenues (Thousands Dollars) Average Price (cents/kWh) Alaska Electric Light&Power Co AK Investor Owned 2,253 125,452 12,449.0 9.92 Alaska Power and Telephone Co AK Investor Owned 2,302 38,952 10,341.0 26.55 Alaska Village Elec Coop, Inc AK Cooperative 2,960 62,209 32,334.0 51.98 Anchorage Municipal Light and Power AK Municipal 6,362 879,373 113,515.6 12.91

  9. Ground-state proton-transfer tautomer of the salicylate anion

    SciTech Connect (OSTI)

    Friedrich, D.M.; Wang, Z.; Joly, A.G.; Peterson, K.A.; Callis, P.R.

    1999-12-02

    Solutions of sodium salicylate in anhydrous polar solvents exhibit a weak, temperature-dependent absorption band ({lambda}{sub max} {approx} 325 nm) lying in the Stokes gap between the main absorption (296 nm) and the fluorescence band (396 nm, acetonitrile). This weak, longer wavelength absorption band is hardly observable in aqueous solution, but its intensity increases with temperature and increases with polarity in anhydrous organic solvents in the order of ethanol < acetonitrile < dimethyl sulfoxide at room temperature. After correction for solvent thermal contraction, the temperature-dependent absorption spectrum of salicylate in acetonitrile solutions reveals a clear isosbestic point ({epsilon}{sub 310}= 2,000 M{sup {minus}1} cm{sup {minus}1}) characteristic of an equilibrium between two salicylate species with band-maximum extinction coefficients of {epsilon}{sub 325} = 3,400 M{sup {minus}1} cm{sup {minus}1} and {epsilon}{sub 296} = 3,586 M{sup {minus}1} cm{sup {minus}1}. In acetonitrile at room temperature (298 K) the concentration equilibrium constant (minor/major) for the interconversion reaction between the two species is K{sub 298} = 0.11, with {Delta}H = 1.6 kcal mol{sup {minus}1} and {Delta}S = 0.97 cal{center{underscore}dot}mol{sup {minus}1} K{sup {minus}1}. The fluorescence lifetime (4.8 ns in acetonitrile) and the shape of the fluorescence spectrum are independent of excitation wavelength. The fluorescence quantum yield for excitation in the long-wavelength shoulder (340 nm) is approximately 60% larger than the yield for excitation in the main band at 296 nm ({phi}{sub 340} = 0.29, {phi}{sub 296} = 0.18) in acetonitrile at room temperature. These results are consistent with assignment of the shoulder band to the proton-transfer tautomer of the salicylate anion. Electronic structure calculations support assignment of the 325 nm absorption band to the ground-state tautomer (phenoxide anion form) of the salicylate anion. Absorption transition moments for both the normal and tautomer forms are parallel to the emission transition moment, are electronically allowed, and are consistent with {sup 1}L{sub b} assignment for both absorbing and emitting transitions. The static dipole moments are in the order of {mu}(N*) {ge} {mu}(N) > {mu}(T*) > {mu}(T) for the normal (N) and tautomer (T) ground and electronic excited states.

  10. White Paper on the Use of Team Calendars with the JIRA Issue Tracking System and Confluence Collaboration Tools for the xLPR Project

    SciTech Connect (OSTI)

    Klasky, Hilda B; Williams, Paul T; Bass, Bennett Richard

    2012-09-01

    ORNL was tasked by xLPR project management to propose a team calendar for use within the xLPR consortium. Among various options that were considered, the approach judged by ORNL to best fit the needs of the xLPR project is presented in this document. The Atlassian Team Calendars plug-in used with the Confluence collaboration tool was recommended for several reasons, including the advantage that it provides for a tight integration between Confluence (found at https://xlpr.ornl.gov/wiki ) and xLPR s JIRA issue tracking system (found at https://xlpr.ornl.gov/jira ). This document is divided into two parts. The first part (Sections 1-6) consists of the white paper, which highlights some of the ways that Team Calendars can improve com mun ication between xLPR project managers, group leads, and team members when JIRA is applied for both issue tracking and change-management activities. Specific points emphasized herein are as follows: The Team Calendar application greatly enhances the added value that the JIRA and Confluence tools bring to the xLPR Project. The Team Calendar can improve com mun ication between xLPR project managers, group leads, and team members when JIRA is applied for both issue tracking and change-management activities. The Team Calendar works across different email tools such as Outlook 2011, Outlook 2010, Outlook 2007, Google Calendars and Mac s iCalendar to name a few. xLPR users can now access the wiki Confluence (with embedded Team Calendars) directly from JIRA without having to re-validate their login. The second part consists of an Annex (Section 7), which describes how users can subscribe to Team Calendars from different calendar applications. Specific instructions are given in the Annex that describe how to Import xLPR Team Calendar to Outlook Version Office 2010 Import xLPR Team Calendar to Outlook Version Office 2007 Subscribe to Team Calendar from Google Calendar The reader is directed to Section 4 for instructions on adding events to the Team Calendar or accessing ORNL staff for assistance with such additions. To seek help with your questions and problems regarding the content of this document, please contact Hilda Klasky at klaskyhb@ornl.gov

  11. Open Issues

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

    April 2011 "Unable to open kgni version file /sys/class/gemini/kgni0/version" error April 13, 2011 by Helen He Symptom: Dynamic executables built with compiler wrappers running directly on the external login nodes are getting the following error message: Read the full post Resolved -- Default version not shown in "module avail module_name" command April 13, 2011 by Helen He Symptom: The default software version is not shown when "module avail module_name" is issued.

  12. gillilan | The Ames Laboratory

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

    gigaflops Two of the World's Most Powerful Computers work for NNSA Two NNSA supercomputers-Trinity and Sequoia-are among the top six systems in the world, according to the 46th edition of the twice-yearly TOP500 list of the most powerful supercomputers released this month. Sequoia has been the world's third most powerful computer since June 2013, while Trinity is

    gillilan Ames Laboratory Profile Steven Gilliland Sys Control Tech Facilities Services Maintenance Shop Phone Number: 515-294-3078

  13. Aerosys Agrees to Pay Civil Penalty and Submit Test Data in Settlement with

    Energy Savers [EERE]

    DOE | Department of Energy Aerosys Agrees to Pay Civil Penalty and Submit Test Data in Settlement with DOE Aerosys Agrees to Pay Civil Penalty and Submit Test Data in Settlement with DOE July 6, 2010 - 3:08pm Addthis WASHINGTON, DC - The Department of Energy announced today that AeroSys, Inc. has agreed to pay a civil penalty of $25,000 and take a number of other actions designed to ensure its future compliance with DOE's energy efficiency standards. Last fall, the Department subpoenaed

  14. Tank evaluation system shielded annular tank application

    SciTech Connect (OSTI)

    Freier, D.A.

    1988-10-04

    TEST (Tank Evaluation SysTem) is a research project utilizing neutron interrogation techniques to analyze the content of nuclear poisons and moderators in tank shielding. TEST experiments were performed on an experimental SAT (Shielded Annular Tank) at the Rocky Flats Plant. The purpose of these experiments was threefold: (1) to assess TEST application to SATs, (2) to determine if Nuclear Safety inspection criteria could be met, and (3) to perform a preliminary calibration of TEST for SATs. Several experiments were performed, including measurements of 11 tank shielding configurations, source-simulated holdup experiments, analysis of three detector modes, resolution studies, and TEST scanner geometry experiments. 1 ref., 21 figs., 4 tabs.

  15. Measurement of the Omega0(c) lifetime

    SciTech Connect (OSTI)

    Iori, M.; Ayan, A.S.; Akgun, U.; Alkhazov, G.; Amaro-Reyes, J.; Atamantchouk, A.G.; Balatz, M.Y.; Blanco-Covarrubias, A.; Bondar, N.F.; Cooper, P.S.; Dauwe, L.J.; /Ball State U. /Bogazici U. /Carnegie Mellon U. /Rio de Janeiro, CBPF /Fermilab /Serpukhov, IHEP /Beijing, Inst. High Energy Phys. /Moscow, ITEP /Heidelberg, Max Planck Inst. /Moscow State U. /St. Petersburg, INP

    2007-01-01

    The authors report a precise measurement of the {Omega}{sub c}{sup 0} lifetime. The data were taken by the SELEX (E781) experiment using 600 GeV/c {Sigma}{sup -}, {pi}{sup -} and p beams. The measurement has been made using 83 {+-} 19 reconstructed {Omega}{sub c}{sup 0} in the {Omega}{sup -} {pi}{sup -}{pi}{sup +}{pi}{sup +} and {Omega}{sup -} {pi}{sup +} decay modes. The lifetime of the {Omega}{sub c}{sup 0} is measured to be 65 {+-} 13(stat) {+-} 9(sys) fs.

  16. Measurement of the t anti-t Cross-Section Using the Dimuon Channel in p anti-p Collisions at s**(1/2) = 1.96-TeV

    SciTech Connect (OSTI)

    McCroskey, Robert Crampton

    2004-11-01

    The author has measured the t{bar t} production cross section at {radical}s = 1.96 TeV using data collected by the D0 experiment at Fermilab. The integrated luminosity of the data set is 140 pb{sup -1} and a total of four candidate events are seen, with an expected background of 2.61 events. The measured cross section of {sigma}{sub t{bar t}} = 11.1{sub -9.3}{sup +22.1}(stat.){sub -4.5}{sup +4.3}(sys.) pb is in agreement with a NNLO calculation of 6.77 pb.

  17. Prepa~ea.for~:

    Office of Legacy Management (LM)

    t : -. . . .~. .'. ,' ., , ;,. ~ Prepa~ea.for~: ,. .s . . :=: ., .' ,..: '. ." ECLIPSR = PIORRRR DIVILiION RENDlZ~AvIATION CORPO.WTI3N . : !. '< ..; 'TmT+ORO NW .,ERsEY This proposalis ,submittedina.ccordance'.%iith the : .' ,request from,the 'Research ,D,epartment at,'sandia'Gorporation for,.an.~er~ia.~Po~er Supply&This supply woulcp~rovido : another altetinate power supply~sys~temto.~replace~batterics in: future ~ap,plic,a~ionsO '1 '~ ~'., ". .-. ,.~ ~Thisunit is to:deliver an

  18. New Limit on Time-Reversal Violation in Beta Decay

    SciTech Connect (OSTI)

    Mumm, H. P.; Chupp, T. E.; Cooper, R. L.; Coulter, K. P.; Freedman, S. J.; Fujikawa, B. K.; Garcia, A.; Jones, G. L.; Nico, J. S.; Thompson, A. K.; Trull, C. A.; Wietfeldt, F. E.; Wilkerson, J. F.

    2011-09-02

    We report the results of an improved determination of the triple correlation DP{center_dot}(p{sub e}xp{sub v}) that can be used to limit possible time-reversal invariance in the beta decay of polarized neutrons and constrain extensions to the standard model. Our result is D=[-0.96{+-}1.89(stat){+-}1.01(sys)]x10{sup -4}. The corresponding phase between g{sub A} and g{sub V} is {phi}{sub AV}=180.013 deg. {+-}0.028 deg. (68% confidence level). This result represents the most sensitive measurement of D in nuclear {beta} decay.

  19. Summary - Savannah River Site Tank 48H Waste Treatment Project

    Office of Environmental Management (EM)

    S Wet Air Savan contain liquid w contain potent to the option tank w Bed S condu be pur The as Techn Techn as liste * W o o The Ele Site: S roject: S P Report Date: J ited States Savanna Why DOE r Oxidation Proc nnah River Tan ning approxima waste. The wa ns tetraphenylb tially flammable tank head spa s have been id waste: Wet Air O team Reformin cted to aid in d rsued for treatin What th ssessment team ology Element ology Readine ed below: Wet Air Oxidatio Reactor sys Offgas Trea To view the

  20. SchemaOnRead Manual

    SciTech Connect (OSTI)

    North, Michael J.

    2015-09-30

    SchemaOnRead provides tools for implementing schema-on-read including a single function call (e.g., schemaOnRead("filename")) that reads text (TXT), comma separated value (CSV), raster image (BMP, PNG, GIF, TIFF, and JPG), R data (RDS), HDF5, NetCDF, spreadsheet (XLS, XLSX, ODS, and DIF), Weka Attribute-Relation File Format (ARFF), Epi Info (REC), Pajek network (PAJ), R network (NET), Hypertext Markup Language (HTML), SPSS (SAV), Systat (SYS), and Stata (DTA) files. It also recursively reads folders (e.g., schemaOnRead("folder")), returning a nested list of the contained elements.

  1. The Lifetime of a beautiful and charming meson: B_c lifetime measured using the D0 detector

    SciTech Connect (OSTI)

    Welty-Rieger, Leah Christine; /Indiana U.

    2008-09-01

    Using approximately 1.3 fb{sup -1} of data collected by the D0 detector between 2002 and 2006, the lifetime of the B{sub c}{sup {+-}} meson is studied in the B{sub c}{sup {+-}} {yields} J/{psi}{mu}{sup {+-}} + X final state. Using an unbinned likelihood simultaneous fit to J/{psi} + {mu} invariant mass and lifetime distributions, a signal of 810 {+-} 80(stat.) candidates is estimated and a lifetime measurement made of: {tau}(B{sub c}{sup {+-}}) = 0.448{sub -0.036}{sup +0.038}(stat) {+-} 0.032(sys) ps.

  2. The Ames Laboratory

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

    Directory: Facilities Services Name Title Office Email Phone Number Jordan Anderson 167 Metals Development ja762@iastate.edu 515-294-5428 Teresa Ball Custodian I 241C Metals Development tdball@iastate.edu 515-294-4360 Brian Bergman Facil Mechanic III Maintenance Shop bbergman@ameslab.gov 515-294-4346 Ronald Berrett Sys Control Tech Maintenance Shop rberrett@ameslab.gov 515-294-1746 Alexander Burgher Facil Mechanic III 158B Metals Development burghera@ameslab.gov 515-294-3756 Steven Carter Engr

  3. The stability of slopes subjected to blasting vibration -- Assessment and application in Hong Kong

    SciTech Connect (OSTI)

    Law, R.; Keller, R.

    1996-12-01

    In the rush to beat the clock before the handover of Hong Kong back to China in June of 1997, an unprecedented amount of infrastructure work is being undertaken at a breakneck pace. In the middle of this construction explosion, on this island of barren granite, stands some of the most concerning and restrictive slope stability measures. So conservative, these measures impact blasting and vibration control to an extent unmatched anywhere in the world. This paper covers the application of vibration limitations and assessment of the stability of rock slopes subjected to blasting vibration in a very challenging application. The widening of the Tuen Mun highway, a project to improve a main artery to the city center to accommodate the ever increasing traffic, involves the blasting of existing slopes in cuts only a few meters wide and up to 45 meters in height, while addressing assessment limitations in a variety of geological conditions. Discussed in the paper is the application of guidelines imposed by the Geotechnical Engineering Office and the Mines Division of the Hong Kong Government and measures taken to address them, i.e., adjustment of geological factors for practical application in blast design; blasting with minimal effect; and maximum protective measures. As slope stability becomes another ever-increasing environmental concern affecting blasting, these applications may be helpful in addressing the encroachment of impending restrictions in other parts of the world on challenging projects where blast assessment of slopes is a critical factor.

  4. The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda, and w from the First Year Data Set

    DOE R&D Accomplishments [OSTI]

    Astier, P.; Guy, J.; Regnault, N.; Pain, R.; Aubourg, E.; Balam, D.; Basa, S.; Carlberg, R. G.; Fabbro, S.; Fouchez, D.; Hook, I. M.; Howell, D. A.; Lafoux, H.; Neill, J. D.; Palanque-Delabrouille, N.; Perrett, K.; Pritchet, C. J.; Rich, J.; Sullivan, M.; Taillet, R.; Aldering, G.; Antilogus, P.; Arsenijevic, V.; Balland, C.; Baumont, S.; Bronder, J.; Courtois, H.; Ellis, R. S.; Filiol, M.; Goncalves, A. C.; Goobar, A.; Guide, D.; Hardin, D.; Lusset, V.; Lidman, C.; McMahon, R.; Mouchet, M.; Mourao, A.; Perlmutter, S.; Ripoche, P.; Tao, C.; Walton, N.

    2005-10-14

    We present distance measurements to 71 high redshift type Ia supernovae discovered during the first year of the 5-year Supernova Legacy Survey (SNLS). These events were detected and their multi-color light-curves measured using the MegaPrime/MegaCam instrument at the Canada-France-Hawaii Telescope (CFHT), by repeatedly imaging four one-square degree fields in four bands. Follow-up spectroscopy was performed at the VLT, Gemini and Keck telescopes to confirm the nature of the supernovae and to measure their redshift. With this data set, we have built a Hubble diagram extending to z = 1, with all distance measurements involving at least two bands. Systematic uncertainties are evaluated making use of the multiband photometry obtained at CFHT. Cosmological fits to this first year SNLS Hubble diagram give the following results: {Omega}{sub M} = 0.263 {+-} 0.042 (stat) {+-} 0.032 (sys) for a flat {Lambda}CDM model; and w = -1.023 {+-} 0.090 (stat) {+-} 0.054 (sys) for a flat cosmology with constant equation of state w when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.

  5. A measurement of the cosmic microwave background B-mode polarization power spectrum at sub-degree scales with POLARBEAR

    SciTech Connect (OSTI)

    Ade, P. A. R.; Akiba, Y.; Hasegawa, M.; Anthony, A. E.; Halverson, N. W.; Arnold, K.; Atlas, M.; Barron, D.; Boettger, D.; Elleflot, T.; Feng, C.; Borrill, J.; Errard, J.; Chapman, S.; Chinone, Y.; Flanigan, D.; Dobbs, M.; Gilbert, A.; Fabbian, G.; Collaboration: Polarbear Collaboration; and others

    2014-10-20

    We report a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile. The faint B-mode polarization signature carries information about the universe's entire history of gravitational structure formation, and the cosmic inflation that may have occurred in the very early universe. Our measurement covers the angular multipole range 500 < ? < 2100 and is based on observations of an effective sky area of 25 deg{sup 2} with 3.'5 resolution at 150 GHz. On these angular scales, gravitational lensing of the CMB by intervening structure in the universe is expected to be the dominant source of B-mode polarization. Including both systematic and statistical uncertainties, the hypothesis of no B-mode polarization power from gravitational lensing is rejected at 97.2% confidence. The band powers are consistent with the standard cosmological model. Fitting a single lensing amplitude parameter A{sub BB} to the measured band powers, A{sub BB}=1.120.61(stat){sub ?0.12}{sup +0.04}(sys)0.07(multi), where A{sub BB} = 1 is the fiducial WMAP-9 ?CDM value. In this expression, 'stat' refers to the statistical uncertainty, 'sys' to the systematic uncertainty associated with possible biases from the instrument and astrophysical foregrounds, and 'multi' to the calibration uncertainties that have a multiplicative effect on the measured amplitude A{sub BB}.

  6. Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Aab, Alexander

    2015-03-09

    We present the first hybrid measurement of the average muon number in air showers at ultra-high energies, initiated by cosmic rays with zenith angles between 62° and 80° . Our measurement is based on 174 hybrid events recorded simultaneously with the Surface Detector array and the Fluorescence Detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019 eV shower with a zenith angle of 67°, which arrives at the Surface Detector array at anmore » altitude of 1450 m above sea level, contains on average (2.68 ± 0.04 ± 0.48 (sys.)) × 107 muons with energies larger than 0.3 GeV. Finally, the logarithmic gain d ln Nµ/d ln E of muons with increasing energy between 4 × 1018 eV and 5 × 1019 eV is measured to be (1.029 ± 0.024 ± 0.030 (sys.)).« less

  7. Measurement of the cosmic ray spectrum above 4×1018 eV using inclined events detected with the Pierre Auger Observatory

    SciTech Connect (OSTI)

    Aab, Alexander

    2015-08-26

    A measurement of the cosmic-ray spectrum for energies exceeding 4×1018 eV is presented, which is based on the analysis of showers with zenith angles greater than 60° detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.3×1018 eV, the ``ankle'', the flux can be described by a power law E–γ with index γ=2.70 ± 0.02 (stat) ± 0.1 (sys) followed by a smooth suppression region. For the energy (Es) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find Es=(5.12±0.25 (stat)+1.0–1.2 (sys))×1019 eV.

  8. Muons in air showers at the Pierre Auger Observatory: Mean number in highly inclined events

    SciTech Connect (OSTI)

    Aab, Alexander

    2015-03-09

    We present the first hybrid measurement of the average muon number in air showers at ultra-high energies, initiated by cosmic rays with zenith angles between 62° and 80° . Our measurement is based on 174 hybrid events recorded simultaneously with the Surface Detector array and the Fluorescence Detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019 eV shower with a zenith angle of 67°, which arrives at the Surface Detector array at an altitude of 1450 m above sea level, contains on average (2.68 ± 0.04 ± 0.48 (sys.)) × 107 muons with energies larger than 0.3 GeV. Finally, the logarithmic gain d ln Nµ/d ln E of muons with increasing energy between 4 × 1018 eV and 5 × 1019 eV is measured to be (1.029 ± 0.024 ± 0.030 (sys.)).

  9. Understanding and controlling low-temperature aging of nanocrystalline materials.

    SciTech Connect (OSTI)

    Battaile, Corbett Chandler; Boyce, Brad Lee; Brons, Justin G.; Foiles, Stephen Martin; Hattar, Khalid Mikhiel; Holm, Elizabeth Ann; Padilla, Henry A.,; Sharon, John Anthony; Thompson, Gregory B.

    2013-10-01

    Nanocrystalline copper lms were created by both repetitive high-energy pulsed power, to produce material without internal nanotwins; and pulsed laser deposition, to produce nan- otwins. Samples of these lms were indented at ambient (298K) and cryogenic temperatures by immersion in liquid nitrogen (77K) and helium (4K). The indented samples were sectioned through the indented regions and imaged in a scanning electron microscope. Extensive grain growth was observed in the lms that contained nanotwins and were indented cryogenically. The lms that either lacked twins, or were indented under ambient conditions, were found to exhibit no substantial grain growth by visual inspection. Precession transmission elec- tron microscopy was used to con rm these ndings quantitatively, and show that 3 and 7 boundaries proliferate during grain growth, implying that these interface types play a key role in governing the extensive grain growth observed here. Molecular dynamics sim- ulations of the motion of individual grain boundaries demonstrate that speci c classes of boundaries - notably 3 and 7 - exhibit anti- or a-thermal migration, meaning that their mobilities either increase or do not change signi cantly with decreasing temperature. An in-situ cryogenic indentation capability was developed and implemented in a transmission electron microscope. Preliminary results do not show extensive cryogenic grain growth in indented copper lms. This discrepancy could arise from the signi cant di erences in con g- uration and loading of the specimen between the two approaches, and further research and development of this capability is needed.

  10. Branching Ratio of the Electromagnetic Decay of the Σ+(1385)

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Keller, D.; Hicks, K.; Adhikari, K. P.; Adikaram, D.; Amaryan, M. J.; Anghinolfi, M.; Baghdasaryan, H.; Ball, J.; Battaglieri, M.; Bedlinskiy, I.; et al

    2012-03-01

    The CLAS detector was used to obtain the first ever measurement of the electromagnetic decay of the Σ*+(1385) from the reaction γp → K0 Σ*+(1385). A real photon beam with a maximum energy of 3.8 GeV was incident on a liquid-hydrogen target, resulting in the photoproduction of the kaon and Σ* hyperon. Kinematic fitting was used to separate the reaction channel from the background processes. The fitting algorithm exploited a new method to kinematically fit neutrons in the CLAS detector, leading to the partial width measurement of 250.0 ± 56.9(stat)-41.2+34.3(sys) keV. A U-spin symmetry test using the SU(3) flavor-multiplet representationmore » yields predictions for the Σ*+(1385) → Σ+γ and Σ*0(1385) → Λγ partial widths that agree with the experimental measurements.« less

  11. Design Principles for Effective Knowledge Discovery from Big Data

    SciTech Connect (OSTI)

    Begoli, Edmon; Horey, James L

    2012-01-01

    Big data phenomenon refers to the practice of collection and processing of very large data sets and associated systems and algorithms used to analyze these massive datasets. Architectures for big data usually range across multiple machines and clusters, and they commonly consist of multiple special purpose sub-systems. Coupled with the knowledge discovery process, big data movement offers many unique opportunities for organizations to benefit (with respect to new insights, business optimizations, etc.). However, due to the difficulty of analyzing such large datasets, big data presents unique systems engineering and architectural challenges. In this paper, we present three sys- tem design principles that can inform organizations on effective analytic and data collection processes, system organization, and data dissemination practices. The principles presented derive from our own research and development experiences with big data problems from various federal agencies, and we illustrate each principle with our own experiences and recommendations.

  12. Central exclusive production at RHIC

    SciTech Connect (OSTI)

    Adamczyk, Leszek; Guryn, W?odek; Turnau, Jacek

    2014-11-10

    The present status and future plans of the physics program of Central Exclusive Production (CEP) at RHIC are described. The measurements are based on the detection of the forward protons from the Double Pomeron Exchange (DPE) process in the Roman Pot system and of the recoil system of charged particles from the DPE process measured in the STAR experiments Time Projection Chamber (TPC). The data described here were taken using polarized proton-proton collisions at ps = 200 GeV. The preliminary spectra of two pion and four pion invariant mass reconstructed by STAR TPC in central region of pseudo-rapidity |#17;| < 1, are presented. Near future plans to take data with the current system at center-of-mass energy ps = 200 GeV and plans to upgrade the forward proton tagging sys- tem are presented. Also a possible addition of the Roman Pots to the sPHENIX detector is discussed.

  13. Measurement of the t tbar cross section at the Run II Tevatron using Support Vector Machines

    SciTech Connect (OSTI)

    Whitehouse, Benjamin Eric; /Tufts U.

    2010-08-01

    This dissertation measures the t{bar t} production cross section at the Run II CDF detector using data from early 2001 through March 2007. The Tevatron at Fermilab is a p{bar p} collider with center of mass energy {radical}s = 1.96 TeV. This data composes a sample with a time-integrated luminosity measured at 2.2 {+-} 0.1 fb{sup -1}. A system of learning machines is developed to recognize t{bar t} events in the 'lepton plus jets' decay channel. Support Vector Machines are described, and their ability to cope with a multi-class discrimination problem is provided. The t{bar t} production cross section is then measured in this framework, and found to be {sigma}{sub t{bar t}} = 7.14 {+-} 0.25 (stat){sub -0.86}{sup +0.61}(sys) pb.

  14. Re

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

    Re s pons e of a CSRM t o V arying M agnit ude s of Sh ort w av e M ont e Carl o Radiat iv e Trans f e r Nois e Jas on Col e 1 H ow ard Bark e r 2 M arat K h airout dinov 3 Dav id Randal l 3 1 Univ e rs it y of Brit is h Col um bia 2 M e t e orol ogical Se rv ice of Canada 3 Col orado St at e Univ e rs it y 1. I nt roduct ion 4. Re s ul t s (TO GA/ COARE) 2. Expe rim e nt Se t up CSRM Sys t e m f or At m os ph e ric M ode l l ing v e rs ion 6.5 (SAM v 6.5) 2D w it h axis orie nt e d w e s t -e

  15. Upper bound on parity-violating neutron spin rotation in {sup 4}He

    SciTech Connect (OSTI)

    Snow, W. M.; Luo, D.; Walbridge, S. B.; Crawford, B. E.; Gan, K.; Micherdzinska, A. M.; Opper, A. K.; Heckel, B. R.; Swanson, H. E.; Sharapov, E. I.; Zhumabekova, V.

    2011-02-15

    We report an upper bound on parity-violating neutron spin rotation in {sup 4}He. This experiment is the most sensitive search for neutron-weak optical activity yet performed and represents a significant advance in precision in comparison to past measurements in heavy nuclei. The experiment was performed at the NG-6 slow-neutron beamline at the National Institute of Standards and Technology (NIST) Center for Neutron Research. Our result for the neutron spin rotation angle per unit length in {sup 4}He is d{phi}/dz=[+1.7{+-}9.1(stat.){+-}1.4(sys.)]x10{sup -7} rad/m. The statistical uncertainty is smaller than current estimates of the range of possible values of d{phi}/dz in n+{sup 4}He.

  16. Study of (W/Z)H production and Higgs boson couplings using H→ W W * decays with the ATLAS detector

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Aad, G.

    2015-08-27

    A search for Higgs boson production in association with a W or Z boson, in the H→ W W * decay channel, is performed with a data sample collected with the ATLAS detector at the LHC in proton-proton collisions at centre-of-mass energies \\( \\sqrt{s}=7 \\) TeV and 8 TeV, corresponding to integrated luminosities of 4.5 fb-1 and 20.3 fb-1, respectively. The WH production mode is studied in two-lepton and three-lepton final states, while two- lepton and four-lepton final states are used to search for the ZH production mode. The observed significance, for the combined W H and ZH production, ismore » 2.5 standard deviations while a significance of 0.9 standard deviations is expected in the Standard Model Higgs boson hypothesis. The ratio of the combined W H and ZH signal yield to the Standard Model expectation, μV H , is found to be μ V H = 3.0-1.1+1.3 (stat.)-0.7 +1.0 (sys.) for the Higgs boson mass of 125.36 GeV. The W H and ZH production modes are also combined with the gluon fusion and vector boson fusion production modes studied in the H → W W * → ℓνℓν decay channel, resulting in an overall observed significance of 6.5 standard deviations and μggF + VBF + VH = 1.16-0.15+0.16 (stat.) -0.15+0.18 (sys.). The results are interpreted in terms of scaling factors of the Higgs boson couplings to vector bosons (κV ) and fermions (κF ); the combined results are: |κ V | = 1.06-0.10+0.10, |κ F| = 0.85-0.20+0.26.« less

  17. Study of (W/Z)H production and Higgs boson couplings using H→ W W * decays with the ATLAS detector

    SciTech Connect (OSTI)

    Aad, G.; Abbott, B.; Abdallah, J.; Abdinov, O.; Aben, R.; Abolins, M.; AbouZeid, O. S.; Abramowicz, H.; Abreu, H.; Abreu, R.; Abulaiti, Y.; Acharya, B. S.; Adamczyk, L.; Adams, D. L.; Adelman, J.; Adomeit, S.; Adye, T.; Affolder, A. A.; Agatonovic-Jovin, T.; Aguilar-Saavedra, J. A.; Ahlen, S. P.; Ahmadov, F.; Aielli, G.; Akerstedt, H.; Åkesson, T. P. A.; Akimoto, G.; Akimov, A. V.; Alberghi, G. L.; Albert, J.; Albrand, S.; Alconada Verzini, M. J.; Aleksa, M.; Aleksandrov, I. N.; Alexa, C.; Alexander, G.; Alexopoulos, T.; Alhroob, M.; Alimonti, G.; Alio, L.; Alison, J.; Alkire, S. P.; Allbrooke, B. M. M.; Allport, P. P.; Aloisio, A.; Alonso, A.; Alonso, F.; Alpigiani, C.; Altheimer, A.; Alvarez Gonzalez, B.; Álvarez Piqueras, D.; Alviggi, M. G.; Amadio, B. T.; Amako, K.; Amaral Coutinho, Y.; Amelung, C.; Amidei, D.; Amor Dos Santos, S. P.; Amorim, A.; Amoroso, S.; Amram, N.; Amundsen, G.; Anastopoulos, C.; Ancu, L. S.; Andari, N.; Andeen, T.; Anders, C. F.; Anders, G.; Anders, J. K.; Anderson, K. J.; Andreazza, A.; Andrei, V.; Angelidakis, S.; Angelozzi, I.; Anger, P.; Angerami, A.; Anghinolfi, F.; Anisenkov, A. V.; Anjos, N.; Annovi, A.; Antonelli, M.; Antonov, A.; Antos, J.; Anulli, F.; Aoki, M.; Aperio Bella, L.; Arabidze, G.; Arai, Y.; Araque, J. P.; Arce, A. T. H.; Arduh, F. A.; Arguin, J-F.; Argyropoulos, S.; Arik, M.; Armbruster, A. J.; Arnaez, O.; Arnal, V.; Arnold, H.; Arratia, M.; Arslan, O.; Artamonov, A.; Artoni, G.; Asai, S.; Asbah, N.; Ashkenazi, A.; Åsman, B.; Asquith, L.; Assamagan, K.; Astalos, R.; Atkinson, M.; Atlay, N. B.; Auerbach, B.; Augsten, K.; Aurousseau, M.; Avolio, G.; Axen, B.; Ayoub, M. K.; Azuelos, G.; Baak, M. A.; Baas, A. E.; Bacci, C.; Bachacou, H.; Bachas, K.; Backes, M.; Backhaus, M.; Bagiacchi, P.; Bagnaia, P.; Bai, Y.; Bain, T.; Baines, J. T.; Baker, O. K.; Balek, P.; Balestri, T.; Balli, F.; Banas, E.; Banerjee, Sw.; Bannoura, A. A. E.; Bansil, H. S.; Barak, L.; Barberio, E. L.; Barberis, D.; Barbero, M.; Barillari, T.; Barisonzi, M.; Barklow, T.; Barlow, N.; Barnes, S. L.; Barnett, B. M.; Barnett, R. M.; Barnovska, Z.; Baroncelli, A.; Barone, G.; Barr, A. J.; Barreiro, F.; Barreiro Guimarães da Costa, J.; Bartoldus, R.; Barton, A. E.; Bartos, P.; Basalaev, A.; Bassalat, A.; Basye, A.; Bates, R. L.; Batista, S. J.; Batley, J. R.; Battaglia, M.; Bauce, M.; Bauer, F.; Bawa, H. S.; Beacham, J. B.; Beattie, M. D.; Beau, T.; Beauchemin, P. H.; Beccherle, R.; Bechtle, P.; Beck, H. P.; Becker, K.; Becker, M.; Becker, S.; Beckingham, M.; Becot, C.; Beddall, A. J.; Beddall, A.; Bednyakov, V. A.; Bee, C. P.; Beemster, L. J.; Beermann, T. A.; Begel, M.; Behr, J. K.; Belanger-Champagne, C.; Bell, W. H.; Bella, G.; Bellagamba, L.; Bellerive, A.; Bellomo, M.; Belotskiy, K.; Beltramello, O.; Benary, O.; Benchekroun, D.; Bender, M.; Bendtz, K.; Benekos, N.; Benhammou, Y.; Benhar Noccioli, E.; Benitez Garcia, J. A.; Benjamin, D. P.; Bensinger, J. R.; Bentvelsen, S.; Beresford, L.; Beretta, M.; Berge, D.; Bergeaas Kuutmann, E.; Berger, N.; Berghaus, F.; Beringer, J.; Bernard, C.; Bernard, N. R.; Bernius, C.; Bernlochner, F. U.; Berry, T.; Berta, P.; Bertella, C.; Bertoli, G.; Bertolucci, F.; Bertsche, C.; Bertsche, D.; Besana, M. I.; Besjes, G. J.; Bessidskaia Bylund, O.; Bessner, M.; Besson, N.; Betancourt, C.; Bethke, S.; Bevan, A. J.; Bhimji, W.; Bianchi, R. M.; Bianchini, L.; Bianco, M.; Biebel, O.; Bieniek, S. P.; Biglietti, M.; Bilbao De Mendizabal, J.; Bilokon, H.; Bindi, M.; Binet, S.; Bingul, A.; Bini, C.; Black, C. W.; Black, J. E.; Black, K. M.; Blackburn, D.; Blair, R. E.; Blanchard, J. -B.; Blanco, J. E.; Blazek, T.; Bloch, I.; Blocker, C.; Blum, W.; Blumenschein, U.; Bobbink, G. J.; Bobrovnikov, V. S.; Bocchetta, S. S.; Bocci, A.; Bock, C.; Boehler, M.; Bogaerts, J. A.; Bogdanchikov, A. G.; Bohm, C.; Boisvert, V.; Bold, T.; Boldea, V.; Boldyrev, A. S.; Bomben, M.; Bona, M.; Boonekamp, M.; Borisov, A.; Borissov, G.; Borroni, S.; Bortfeldt, J.; Bortolotto, V.; Bos, K.; Boscherini, D.; Bosman, M.; Boudreau, J.; Bouffard, J.; Bouhova-Thacker, E. V.; Boumediene, D.; Bourdarios, C.; Bousson, N.; Boveia, A.; Boyd, J.; Boyko, I. R.; Bozic, I.; Bracinik, J.; Brandt, A.; Brandt, G.; Brandt, O.; Bratzler, U.; Brau, B.; Brau, J. E.; Braun, H. M.; Brazzale, S. F.; Brendlinger, K.; Brennan, A. J.; Brenner, L.; Brenner, R.; Bressler, S.; Bristow, K.; Bristow, T. M.; Britton, D.; Britzger, D.; Brochu, F. M.; Brock, I.; Brock, R.; Bronner, J.; Brooijmans, G.; Brooks, T.; Brooks, W. K.; Brosamer, J.; Brost, E.; Brown, J.; Bruckman de Renstrom, P. A.; Bruncko, D.; Bruneliere, R.; Bruni, A.; Bruni, G.; Bruschi, M.; Bryngemark, L.; Buanes, T.; Buat, Q.; Buchholz, P.; Buckley, A. G.; Buda, S. I.; Budagov, I. A.; Buehrer, F.; Bugge, L.; Bugge, M. K.; Bulekov, O.; Bullock, D.; Burckhart, H.; Burdin, S.; Burghgrave, B.; Burke, S.; Burmeister, I.; Busato, E.; Büscher, D.; Büscher, V.; Bussey, P.; Butler, J. M.; Butt, A. I.; Buttar, C. M.; Butterworth, J. M.; Butti, P.; Buttinger, W.; Buzatu, A.; Buzykaev, A. R.; Cabrera Urbán, S.; Caforio, D.; Cairo, V. M.; Cakir, O.; Calafiura, P.; Calandri, A.; Calderini, G.; Calfayan, P.; Caloba, L. P.; Calvet, D.; Calvet, S.; Camacho Toro, R.; Camarda, S.; Camarri, P.; Cameron, D.; Caminada, L. M.; Caminal Armadans, R.; Campana, S.; Campanelli, M.; Campoverde, A.; Canale, V.; Canepa, A.; Cano Bret, M.; Cantero, J.; Cantrill, R.; Cao, T.; Capeans Garrido, M. D. M.; Caprini, I.; Caprini, M.; Capua, M.; Caputo, R.; Cardarelli, R.; Carli, T.; Carlino, G.; Carminati, L.; Caron, S.; Carquin, E.; Carrillo-Montoya, G. D.; Carter, J. R.; Carvalho, J.; Casadei, D.; Casado, M. P.; Casolino, M.; Castaneda-Miranda, E.; Castelli, A.; Castillo Gimenez, V.; Castro, N. F.; Catastini, P.; Catinaccio, A.; Catmore, J. R.; Cattai, A.; Caudron, J.; Cavaliere, V.; Cavalli, D.; Cavalli-Sforza, M.; Cavasinni, V.; Ceradini, F.; Cerio, B. C.; Cerny, K.; Cerqueira, A. S.; Cerri, A.; Cerrito, L.; Cerutti, F.; Cerv, M.; Cervelli, A.; Cetin, S. A.; Chafaq, A.; Chakraborty, D.; Chalupkova, I.; Chang, P.; Chapleau, B.; Chapman, J. D.; Charlton, D. G.; Chau, C. C.; Chavez Barajas, C. A.; Cheatham, S.; Chegwidden, A.; Chekanov, S.; Chekulaev, S. V.; Chelkov, G. A.; Chelstowska, M. A.; Chen, C.; Chen, H.; Chen, K.; Chen, L.; Chen, S.; Chen, X.; Chen, Y.; Cheng, H. C.; Cheng, Y.; Cheplakov, A.; Cheremushkina, E.; Cherkaoui El Moursli, R.; Chernyatin, V.; Cheu, E.; Chevalier, L.; Chiarella, V.; Childers, J. T.; Chiodini, G.; Chisholm, A. S.; Chislett, R. T.; Chitan, A.; Chizhov, M. V.; Choi, K.; Chouridou, S.; Chow, B. K. B.; Christodoulou, V.; Chromek-Burckhart, D.; Chu, M. L.; Chudoba, J.; Chuinard, A. J.; Chwastowski, J. J.; Chytka, L.; Ciapetti, G.; Ciftci, A. K.; Cinca, D.; Cindro, V.; Cioara, I. A.; Ciocio, A.; Citron, Z. H.; Ciubancan, M.; Clark, A.; Clark, B. L.; Clark, P. J.; Clarke, R. N.; Cleland, W.; Clement, C.; Coadou, Y.; Cobal, M.; Coccaro, A.; Cochran, J.; Coffey, L.; Cogan, J. G.; Cole, B.; Cole, S.; Colijn, A. P.; Collot, J.; Colombo, T.; Compostella, G.; Conde Muiño, P.; Coniavitis, E.; Connell, S. H.; Connelly, I. A.; Consonni, S. M.; Consorti, V.; Constantinescu, S.; Conta, C.; Conti, G.; Conventi, F.; Cooke, M.; Cooper, B. D.; Cooper-Sarkar, A. M.; Cornelissen, T.; Corradi, M.; Corriveau, F.; Corso-Radu, A.; Cortes-Gonzalez, A.; Cortiana, G.; Costa, G.; Costa, M. J.; Costanzo, D.; Côté, D.; Cottin, G.; Cowan, G.; Cox, B. E.; Cranmer, K.; Cree, G.; Crépé-Renaudin, S.; Crescioli, F.; Cribbs, W. A.; Crispin Ortuzar, M.; Cristinziani, M.; Croft, V.; Crosetti, G.; Cuhadar Donszelmann, T.; Cummings, J.; Curatolo, M.; Cuthbert, C.; Czirr, H.; Czodrowski, P.; D’Auria, S.; D’Onofrio, M.; Da Cunha Sargedas De Sousa, M. J.; Da Via, C.; Dabrowski, W.; Dafinca, A.; Dai, T.; Dale, O.; Dallaire, F.; Dallapiccola, C.; Dam, M.; Dandoy, J. R.; Dang, N. P.; Daniells, A. C.; Danninger, M.; Dano Hoffmann, M.; Dao, V.; Darbo, G.; Darmora, S.; Dassoulas, J.; Dattagupta, A.; Davey, W.; David, C.; Davidek, T.; Davies, E.; Davies, M.; Davison, P.; Davygora, Y.; Dawe, E.; Dawson, I.; Daya-Ishmukhametova, R. K.; De, K.; de Asmundis, R.; De Castro, S.; De Cecco, S.; De Groot, N.; de Jong, P.; De la Torre, H.; De Lorenzi, F.; De Nooij, L.; De Pedis, D.; De Salvo, A.; De Sanctis, U.; De Santo, A.; De Vivie De Regie, J. B.; Dearnaley, W. J.; Debbe, R.; Debenedetti, C.; Dedovich, D. V.; Deigaard, I.; Del Peso, J.; Del Prete, T.; Delgove, D.; Deliot, F.; Delitzsch, C. M.; Deliyergiyev, M.; Dell’Acqua, A.; Dell’Asta, L.; Dell’Orso, M.; Della Pietra, M.; della Volpe, D.; Delmastro, M.; Delsart, P. A.; Deluca, C.; DeMarco, D. A.; Demers, S.; Demichev, M.; Demilly, A.; Denisov, S. P.; Derendarz, D.; Derkaoui, J. E.; Derue, F.; Dervan, P.; Desch, K.; Deterre, C.; Deviveiros, P. O.; Dewhurst, A.; Dhaliwal, S.; Di Ciaccio, A.; Di Ciaccio, L.; Di Domenico, A.; Di Donato, C.; Di Girolamo, A.; Di Girolamo, B.; Di Mattia, A.; Di Micco, B.; Di Nardo, R.; Di Simone, A.; Di Sipio, R.; Di Valentino, D.; Diaconu, C.; Diamond, M.; Dias, F. A.; Diaz, M. A.; Diehl, E. B.; Dietrich, J.; Diglio, S.; Dimitrievska, A.; Dingfelder, J.; Dita, P.; Dita, S.; Dittus, F.; Djama, F.; Djobava, T.; Djuvsland, J. I.; do Vale, M. A. B.; Dobos, D.; Dobre, M.; Doglioni, C.; Dohmae, T.; Dolejsi, J.; Dolezal, Z.; Dolgoshein, B. A.; Donadelli, M.; Donati, S.; Dondero, P.; Donini, J.; Dopke, J.; Doria, A.; Dova, M. T.; Doyle, A. T.; Drechsler, E.; Dris, M.; Dubreuil, E.; Duchovni, E.; Duckeck, G.; Ducu, O. A.; Duda, D.; Dudarev, A.; Duflot, L.; Duguid, L.; Dührssen, M.; Dunford, M.; Duran Yildiz, H.; Düren, M.; Durglishvili, A.; Duschinger, D.; Dyndal, M.; Eckardt, C.; Ecker, K. M.; Edgar, R. C.; Edson, W.; Edwards, N. C.; Ehrenfeld, W.; Eifert, T.; Eigen, G.; Einsweiler, K.; Ekelof, T.; El Kacimi, M.; Ellert, M.; Elles, S.; Ellinghaus, F.; Elliot, A. A.; Ellis, N.; Elmsheuser, J.; Elsing, M.; Emeliyanov, D.; Enari, Y.; Endner, O. C.; Endo, M.; Erdmann, J.; Ereditato, A.; Ernis, G.; Ernst, J.; Ernst, M.; Errede, S.; Ertel, E.; Escalier, M.; Esch, H.; Escobar, C.; Esposito, B.; Etienvre, A. I.; Etzion, E.; Evans, H.; Ezhilov, A.; Fabbri, L.; Facini, G.; Fakhrutdinov, R. M.; Falciano, S.; Falla, R. J.; Faltova, J.; Fang, Y.; Fanti, M.; Farbin, A.; Farilla, A.; Farooque, T.; Farrell, S.; Farrington, S. M.; Farthouat, P.; Fassi, F.; Fassnacht, P.; Fassouliotis, D.; Faucci Giannelli, M.; Favareto, A.; Fayard, L.; Federic, P.; Fedin, O. L.; Fedorko, W.; Feigl, S.; Feligioni, L.; Feng, C.; Feng, E. J.; Feng, H.; Fenyuk, A. B.; Fernandez Martinez, P.; Fernandez Perez, S.; Ferrando, J.; Ferrari, A.; Ferrari, P.; Ferrari, R.; Ferreira de Lima, D. E.; Ferrer, A.; Ferrere, D.; Ferretti, C.; Ferretto Parodi, A.; Fiascaris, M.; Fiedler, F.; Filipčič, A.; Filipuzzi, M.; Filthaut, F.; Fincke-Keeler, M.; Finelli, K. D.; Fiolhais, M. C. N.; Fiorini, L.; Firan, A.; Fischer, A.; Fischer, C.; Fischer, J.; Fisher, W. C.; Fitzgerald, E. A.; Flechl, M.; Fleck, I.; Fleischmann, P.; Fleischmann, S.; Fletcher, G. T.; Fletcher, G.; Flick, T.; Floderus, A.; Flores Castillo, L. R.; Flowerdew, M. J.; Formica, A.; Forti, A.; Fournier, D.; Fox, H.; Fracchia, S.; Francavilla, P.; Franchini, M.; Francis, D.; Franconi, L.; Franklin, M.; Fraternali, M.; Freeborn, D.; French, S. T.; Friedrich, F.; Froidevaux, D.; Frost, J. A.; Fukunaga, C.; Fullana Torregrosa, E.; Fulsom, B. G.; Fuster, J.; Gabaldon, C.; Gabizon, O.; Gabrielli, A.; Gabrielli, A.; Gadatsch, S.; Gadomski, S.; Gagliardi, G.; Gagnon, P.; Galea, C.; Galhardo, B.; Gallas, E. J.; Gallop, B. J.; Gallus, P.; Galster, G.; Gan, K. K.; Gao, J.; Gao, Y.; Gao, Y. S.; Garay Walls, F. M.; Garberson, F.; García, C.; García Navarro, J. E.; Garcia-Sciveres, M.; Gardner, R. W.; Garelli, N.; Garonne, V.; Gatti, C.; Gaudiello, A.; Gaudio, G.; Gaur, B.; Gauthier, L.; Gauzzi, P.; Gavrilenko, I. L.; Gay, C.; Gaycken, G.; Gazis, E. N.; Ge, P.; Gecse, Z.; Gee, C. N. P.; Geerts, D. A. A.; Geich-Gimbel, Ch.; Geisler, M. P.; Gemme, C.; Genest, M. H.; Gentile, S.; George, M.; George, S.; Gerbaudo, D.; Gershon, A.; Ghazlane, H.; Giacobbe, B.; Giagu, S.; Giangiobbe, V.; Giannetti, P.; Gibbard, B.; Gibson, S. M.; Gilchriese, M.; Gillam, T. P. S.; Gillberg, D.; Gilles, G.; Gingrich, D. M.; Giokaris, N.; Giordani, M. P.; Giorgi, F. M.; Giorgi, F. M.; Giraud, P. F.; Giromini, P.; Giugni, D.; Giuliani, C.; Giulini, M.; Gjelsten, B. K.; Gkaitatzis, S.; Gkialas, I.; Gkougkousis, E. L.; Gladilin, L. K.; Glasman, C.; Glatzer, J.; Glaysher, P. C. F.; Glazov, A.; Goblirsch-Kolb, M.; Goddard, J. 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R.; Pauly, T.; Pearce, J.; Pearson, B.; Pedersen, L. E.; Pedersen, M.; Pedraza Lopez, S.; Pedro, R.; Peleganchuk, S. V.; Pelikan, D.; Peng, H.; Penning, B.; Penwell, J.; Perepelitsa, D. V.; Perez Codina, E.; Pérez García-Estañ, M. T.; Perini, L.; Pernegger, H.; Perrella, S.; Peschke, R.; Peshekhonov, V. D.; Peters, K.; Peters, R. F. Y.; Petersen, B. A.; Petersen, T. C.; Petit, E.; Petridis, A.; Petridou, C.; Petrolo, E.; Petrucci, F.; Pettersson, N. E.; Pezoa, R.; Phillips, P. W.; Piacquadio, G.; Pianori, E.; Picazio, A.; Piccaro, E.; Piccinini, M.; Pickering, M. A.; Piegaia, R.; Pignotti, D. T.; Pilcher, J. E.; Pilkington, A. D.; Pina, J.; Pinamonti, M.; Pinfold, J. L.; Pingel, A.; Pinto, B.; Pires, S.; Pitt, M.; Pizio, C.; Plazak, L.; Pleier, M. -A.; Pleskot, V.; Plotnikova, E.; Plucinski, P.; Pluth, D.; Poettgen, R.; Poggioli, L.; Pohl, D.; Polesello, G.; Policicchio, A.; Polifka, R.; Polini, A.; Pollard, C. S.; Polychronakos, V.; Pommès, K.; Pontecorvo, L.; Pope, B. G.; Popeneciu, G. A.; Popovic, D. S.; Poppleton, A.; Pospisil, S.; Potamianos, K.; Potrap, I. N.; Potter, C. J.; Potter, C. T.; Poulard, G.; Poveda, J.; Pozdnyakov, V.; Pralavorio, P.; Pranko, A.; Prasad, S.; Prell, S.; Price, D.; Price, L. E.; Primavera, M.; Prince, S.; Proissl, M.; Prokofiev, K.; Prokoshin, F.; Protopapadaki, E.; Protopopescu, S.; Proudfoot, J.; Przybycien, M.; Ptacek, E.; Puddu, D.; Pueschel, E.; Puldon, D.; Purohit, M.; Puzo, P.; Qian, J.; Qin, G.; Qin, Y.; Quadt, A.; Quarrie, D. R.; Quayle, W. B.; Queitsch-Maitland, M.; Quilty, D.; Raddum, S.; Radeka, V.; Radescu, V.; Radhakrishnan, S. K.; Radloff, P.; Rados, P.; Ragusa, F.; Rahal, G.; Rajagopalan, S.; Rammensee, M.; Rangel-Smith, C.; Rauscher, F.; Rave, S.; Ravenscroft, T.; Raymond, M.; Read, A. L.; Readioff, N. P.; Rebuzzi, D. M.; Redelbach, A.; Redlinger, G.; Reece, R.; Reeves, K.; Rehnisch, L.; Reisin, H.; Relich, M.; Rembser, C.; Ren, H.; Renaud, A.; Rescigno, M.; Resconi, S.; Rezanova, O. L.; Reznicek, P.; Rezvani, R.; Richter, R.; Richter, S.; Richter-Was, E.; Ricken, O.; Ridel, M.; Rieck, P.; Riegel, C. J.; Rieger, J.; Rijssenbeek, M.; Rimoldi, A.; Rinaldi, L.; Ristić, B.; Ritsch, E.; Riu, I.; Rizatdinova, F.; Rizvi, E.; Robertson, S. H.; Robichaud-Veronneau, A.; Robinson, D.; Robinson, J. E. M.; Robson, A.; Roda, C.; Roe, S.; Røhne, O.; Rolli, S.; Romaniouk, A.; Romano, M.; Romano Saez, S. M.; Romero Adam, E.; Rompotis, N.; Ronzani, M.; Roos, L.; Ros, E.; Rosati, S.; Rosbach, K.; Rose, P.; Rosendahl, P. L.; Rosenthal, O.; Rossetti, V.; Rossi, E.; Rossi, L. P.; Rosten, R.; Rotaru, M.; Roth, I.; Rothberg, J.; Rousseau, D.; Royon, C. R.; Rozanov, A.; Rozen, Y.; Ruan, X.; Rubbo, F.; Rubinskiy, I.; Rud, V. I.; Rudolph, C.; Rudolph, M. S.; Rühr, F.; Ruiz-Martinez, A.; Rurikova, Z.; Rusakovich, N. A.; Ruschke, A.; Russell, H. L.; Rutherfoord, J. P.; Ruthmann, N.; Ryabov, Y. F.; Rybar, M.; Rybkin, G.; Ryder, N. C.; Saavedra, A. F.; Sabato, G.; Sacerdoti, S.; Saddique, A.; Sadrozinski, H. F-W.; Sadykov, R.; Safai Tehrani, F.; Saimpert, M.; Sakamoto, H.; Sakurai, Y.; Salamanna, G.; Salamon, A.; Saleem, M.; Salek, D.; Sales De Bruin, P. H.; Salihagic, D.; Salnikov, A.; Salt, J.; Salvatore, D.; Salvatore, F.; Salvucci, A.; Salzburger, A.; Sampsonidis, D.; Sanchez, A.; Sánchez, J.; Sanchez Martinez, V.; Sandaker, H.; Sandbach, R. L.; Sander, H. G.; Sanders, M. P.; Sandhoff, M.; Sandoval, C.; Sandstroem, R.; Sankey, D. P. C.; Sannino, M.; Sansoni, A.; Santoni, C.; Santonico, R.; Santos, H.; Santoyo Castillo, I.; Sapp, K.; Sapronov, A.; Saraiva, J. G.; Sarrazin, B.; Sasaki, O.; Sasaki, Y.; Sato, K.; Sauvage, G.; Sauvan, E.; Savage, G.; Savard, P.; Sawyer, C.; Sawyer, L.; Saxon, J.; Sbarra, C.; Sbrizzi, A.; Scanlon, T.; Scannicchio, D. A.; Scarcella, M.; Scarfone, V.; Schaarschmidt, J.; Schacht, P.; Schaefer, D.; Schaefer, R.; Schaeffer, J.; Schaepe, S.; Schaetzel, S.; Schäfer, U.; Schaffer, A. C.; Schaile, D.; Schamberger, R. D.; Scharf, V.; Schegelsky, V. A.; Scheirich, D.; Schernau, M.; Schiavi, C.; Schillo, C.; Schioppa, M.; Schlenker, S.; Schmidt, E.; Schmieden, K.; Schmitt, C.; Schmitt, S.; Schmitt, S.; Schneider, B.; Schnellbach, Y. J.; Schnoor, U.; Schoeffel, L.; Schoening, A.; Schoenrock, B. D.; Schopf, E.; Schorlemmer, A. L. S.; Schott, M.; Schouten, D.; Schovancova, J.; Schramm, S.; Schreyer, M.; Schroeder, C.; Schuh, N.; Schultens, M. J.; Schultz-Coulon, H. -C.; Schulz, H.; Schumacher, M.; Schumm, B. A.; Schune, Ph.; Schwanenberger, C.; Schwartzman, A.; Schwarz, T. A.; Schwegler, Ph.; Schwemling, Ph.; Schwienhorst, R.; Schwindling, J.; Schwindt, T.; Schwoerer, M.; Sciacca, F. G.; Scifo, E.; Sciolla, G.; Scuri, F.; Scutti, F.; Searcy, J.; Sedov, G.; Sedykh, E.; Seema, P.; Seidel, S. C.; Seiden, A.; Seifert, F.; Seixas, J. M.; Sekhniaidze, G.; Sekhon, K.; Sekula, S. J.; Selbach, K. E.; Seliverstov, D. M.; Semprini-Cesari, N.; Serfon, C.; Serin, L.; Serkin, L.; Serre, T.; Sessa, M.; Seuster, R.; Severini, H.; Sfiligoj, T.; Sforza, F.; Sfyrla, A.; Shabalina, E.; Shamim, M.; Shan, L. Y.; Shang, R.; Shank, J. T.; Shapiro, M.; Shatalov, P. B.; Shaw, K.; Shaw, S. M.; Shcherbakova, A.; Shehu, C. Y.; Sherwood, P.; Shi, L.; Shimizu, S.; Shimmin, C. O.; Shimojima, M.; Shiyakova, M.; Shmeleva, A.; Shoaleh Saadi, D.; Shochet, M. J.; Shojaii, S.; Shrestha, S.; Shulga, E.; Shupe, M. A.; Shushkevich, S.; Sicho, P.; Sidiropoulou, O.; Sidorov, D.; Sidoti, A.; Siegert, F.; Sijacki, Dj.; Silva, J.; Silver, Y.; Silverstein, S. B.; Simak, V.; Simard, O.; Simic, Lj.; Simion, S.; Simioni, E.; Simmons, B.; Simon, D.; Simoniello, R.; Sinervo, P.; Sinev, N. B.; Siragusa, G.; Sisakyan, A. N.; Sivoklokov, S. Yu.; Sjölin, J.; Sjursen, T. B.; Skinner, M. B.; Skottowe, H. P.; Skubic, P.; Slater, M.; Slavicek, T.; Slawinska, M.; Sliwa, K.; Smakhtin, V.; Smart, B. H.; Smestad, L.; Smirnov, S. Yu.; Smirnov, Y.; Smirnova, L. N.; Smirnova, O.; Smith, M. N. K.; Smizanska, M.; Smolek, K.; Snesarev, A. A.; Snidero, G.; Snyder, S.; Sobie, R.; Socher, F.; Soffer, A.; Soh, D. A.; Solans, C. A.; Solar, M.; Solc, J.; Soldatov, E. Yu.; Soldevila, U.; Solodkov, A. A.; Soloshenko, A.; Solovyanov, O. V.; Solovyev, V.; Sommer, P.; Song, H. Y.; Soni, N.; Sood, A.; Sopczak, A.; Sopko, B.; Sopko, V.; Sorin, V.; Sosa, D.; Sosebee, M.; Sotiropoulou, C. L.; Soualah, R.; Soueid, P.; Soukharev, A. M.; South, D.; Spagnolo, S.; Spalla, M.; Spanò, F.; Spearman, W. R.; Spettel, F.; Spighi, R.; Spigo, G.; Spiller, L. A.; Spousta, M.; Spreitzer, T.; Denis, R. D. St.; Staerz, S.; Stahlman, J.; Stamen, R.; Stamm, S.; Stanecka, E.; Stanescu, C.; Stanescu-Bellu, M.; Stanitzki, M. M.; Stapnes, S.; Starchenko, E. A.; Stark, J.; Staroba, P.; Starovoitov, P.; Staszewski, R.; Stavina, P.; Steinberg, P.; Stelzer, B.; Stelzer, H. J.; Stelzer-Chilton, O.; Stenzel, H.; Stern, S.; Stewart, G. A.; Stillings, J. A.; Stockton, M. C.; Stoebe, M.; Stoicea, G.; Stolte, P.; Stonjek, S.; Stradling, A. R.; Straessner, A.; Stramaglia, M. E.; Strandberg, J.; Strandberg, S.; Strandlie, A.; Strauss, E.; Strauss, M.; Strizenec, P.; Ströhmer, R.; Strom, D. M.; Stroynowski, R.; Strubig, A.; Stucci, S. A.; Stugu, B.; Styles, N. A.; Su, D.; Su, J.; Subramaniam, R.; Succurro, A.; Sugaya, Y.; Suhr, C.; Suk, M.; Sulin, V. V.; Sultansoy, S.; Sumida, T.; Sun, S.; Sun, X.; Sundermann, J. E.; Suruliz, K.; Susinno, G.; Sutton, M. R.; Suzuki, S.; Suzuki, Y.; Svatos, M.; Swedish, S.; Swiatlowski, M.; Sykora, I.; Sykora, T.; Ta, D.; Taccini, C.; Tackmann, K.; Taenzer, J.; Taffard, A.; Tafirout, R.; Taiblum, N.; Takai, H.; Takashima, R.; Takeda, H.; Takeshita, T.; Takubo, Y.; Talby, M.; Talyshev, A. A.; Tam, J. Y. C.; Tan, K. G.; Tanaka, J.; Tanaka, R.; Tanaka, S.; Tannenwald, B. B.; Tannoury, N.; Tapprogge, S.; Tarem, S.; Tarrade, F.; Tartarelli, G. F.; Tas, P.; Tasevsky, M.; Tashiro, T.; Tassi, E.; Tavares Delgado, A.; Tayalati, Y.; Taylor, F. E.; Taylor, G. N.; Taylor, W.; Teischinger, F. A.; Teixeira Dias Castanheira, M.; Teixeira-Dias, P.; Temming, K. K.; Ten Kate, H.; Teng, P. K.; Teoh, J. J.; Tepel, F.; Terada, S.; Terashi, K.; Terron, J.; Terzo, S.; Testa, M.; Teuscher, R. J.; Therhaag, J.; Theveneaux-Pelzer, T.; Thomas, J. P.; Thomas-Wilsker, J.; Thompson, E. N.; Thompson, P. D.; Thompson, R. J.; Thompson, A. S.; Thomsen, L. A.; Thomson, E.; Thomson, M.; Thun, R. P.; Tibbetts, M. J.; Ticse Torres, R. E.; Tikhomirov, V. O.; Tikhonov, Yu. A.; Timoshenko, S.; Tiouchichine, E.; Tipton, P.; Tisserant, S.; Todorov, T.; Todorova-Nova, S.; Tojo, J.; Tokár, S.; Tokushuku, K.; Tollefson, K.; Tolley, E.; Tomlinson, L.; Tomoto, M.; Tompkins, L.; Toms, K.; Torrence, E.; Torres, H.; Torró Pastor, E.; Toth, J.; Touchard, F.; Tovey, D. R.; Trefzger, T.; Tremblet, L.; Tricoli, A.; Trigger, I. M.; Trincaz-Duvoid, S.; Tripiana, M. F.; Trischuk, W.; Trocmé, B.; Troncon, C.; Trottier-McDonald, M.; Trovatelli, M.; True, P.; Truong, L.; Trzebinski, M.; Trzupek, A.; Tsarouchas, C.; Tseng, J. C-L.; Tsiareshka, P. V.; Tsionou, D.; Tsipolitis, G.; Tsirintanis, N.; Tsiskaridze, S.; Tsiskaridze, V.; Tskhadadze, E. G.; Tsukerman, I. I.; Tsulaia, V.; Tsuno, S.; Tsybychev, D.; Tudorache, A.; Tudorache, V.; Tuna, A. N.; Tupputi, S. A.; Turchikhin, S.; Turecek, D.; Turra, R.; Turvey, A. J.; Tuts, P. M.; Tykhonov, A.; Tylmad, M.; Tyndel, M.; Ueda, I.; Ueno, R.; Ughetto, M.; Ugland, M.; Uhlenbrock, M.; Ukegawa, F.; Unal, G.; Undrus, A.; Unel, G.; Ungaro, F. C.; Unno, Y.; Unverdorben, C.; Urban, J.; Urquijo, P.; Urrejola, P.; Usai, G.; Usanova, A.; Vacavant, L.; Vacek, V.; Vachon, B.; Valderanis, C.; Valencic, N.; Valentinetti, S.; Valero, A.; Valery, L.; Valkar, S.; Valladolid Gallego, E.; Vallecorsa, S.; Valls Ferrer, J. A.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; Van Der Leeuw, R.; van Eldik, N.; van Gemmeren, P.; Van Nieuwkoop, J.; van Vulpen, I.; van Woerden, M. C.; Vanadia, M.; Vandelli, W.; Vanguri, R.; Vaniachine, A.; Vannucci, F.; Vardanyan, G.; Vari, R.; Varnes, E. W.; Varol, T.; Varouchas, D.; Vartapetian, A.; Varvell, K. E.; Vazeille, F.; Vazquez Schroeder, T.; Veatch, J.; Veloso, F.; Velz, T.; Veneziano, S.; Ventura, A.; Ventura, D.; Venturi, M.; Venturi, N.; Venturini, A.; Vercesi, V.; Verducci, M.; Verkerke, W.; Vermeulen, J. C.; Vest, A.; Vetterli, M. C.; Viazlo, O.; Vichou, I.; Vickey, T.; Vickey Boeriu, O. E.; Viehhauser, G. H. A.; Viel, S.; Vigne, R.; Villa, M.; Villaplana Perez, M.; Vilucchi, E.; Vincter, M. G.; Vinogradov, V. B.; Vivarelli, I.; Vives Vaque, F.; Vlachos, S.; Vladoiu, D.; Vlasak, M.; Vogel, M.; Vokac, P.; Volpi, G.; Volpi, M.; von der Schmitt, H.; von Radziewski, H.; von Toerne, E.; Vorobel, V.; Vorobev, K.; Vos, M.; Voss, R.; Vossebeld, J. H.; Vranjes, N.; Vranjes Milosavljevic, M.; Vrba, V.; Vreeswijk, M.; Vuillermet, R.; Vukotic, I.; Vykydal, Z.; Wagner, P.; Wagner, W.; Wahlberg, H.; Wahrmund, S.; Wakabayashi, J.; Walder, J.; Walker, R.; Walkowiak, W.; Wang, C.; Wang, F.; Wang, H.; Wang, H.; Wang, J.; Wang, J.; Wang, K.; Wang, R.; Wang, S. M.; Wang, T.; Wang, X.; Wanotayaroj, C.; Warburton, A.; Ward, C. P.; Wardrope, D. R.; Warsinsky, M.; Washbrook, A.; Wasicki, C.; Watkins, P. M.; Watson, A. T.; Watson, I. J.; Watson, M. F.; Watts, G.; Watts, S.; Waugh, B. M.; Webb, S.; Weber, M. S.; Weber, S. W.; Webster, J. S.; Weidberg, A. R.; Weinert, B.; Weingarten, J.; Weiser, C.; Weits, H.; Wells, P. S.; Wenaus, T.; Wengler, T.; Wenig, S.; Wermes, N.; Werner, M.; Werner, P.; Wessels, M.; Wetter, J.; Whalen, K.; Wharton, A. M.; White, A.; White, M. J.; White, R.; White, S.; Whiteson, D.; Wickens, F. J.; Wiedenmann, W.; Wielers, M.; Wienemann, P.; Wiglesworth, C.; Wiik-Fuchs, L. A. M.; Wildauer, A.; Wilkens, H. G.; Williams, H. H.; Williams, S.; Willis, C.; Willocq, S.; Wilson, A.; Wilson, J. A.; Wingerter-Seez, I.; Winklmeier, F.; Winter, B. T.; Wittgen, M.; Wittkowski, J.; Wollstadt, S. J.; Wolter, M. W.; Wolters, H.; Wosiek, B. K.; Wotschack, J.; Woudstra, M. J.; Wozniak, K. W.; Wu, M.; Wu, M.; Wu, S. L.; Wu, X.; Wu, Y.; Wyatt, T. R.; Wynne, B. M.; Xella, S.; Xu, D.; Xu, L.; Yabsley, B.; Yacoob, S.; Yakabe, R.; Yamada, M.; Yamaguchi, Y.; Yamamoto, A.; Yamamoto, S.; Yamanaka, T.; Yamauchi, K.; Yamazaki, Y.; Yan, Z.; Yang, H.; Yang, H.; Yang, Y.; Yao, L.; Yao, W-M.; Yasu, Y.; Yatsenko, E.; Yau Wong, K. H.; Ye, J.; Ye, S.; Yeletskikh, I.; Yen, A. L.; Yildirim, E.; Yorita, K.; Yoshida, R.; Yoshihara, K.; Young, C.; Young, C. J. S.; Youssef, S.; Yu, D. R.; Yu, J.; Yu, J. M.; Yu, J.; Yuan, L.; Yurkewicz, A.; Yusuff, I.; Zabinski, B.; Zaidan, R.; Zaitsev, A. M.; Zalieckas, J.; Zaman, A.; Zambito, S.; Zanello, L.; Zanzi, D.; Zeitnitz, C.; Zeman, M.; Zemla, A.; Zengel, K.; Zenin, O.; Ženiš, T.; Zerwas, D.; Zhang, D.; Zhang, F.; Zhang, J.; Zhang, L.; Zhang, R.; Zhang, X.; Zhang, Z.; Zhao, X.; Zhao, Y.; Zhao, Z.; Zhemchugov, A.; Zhong, J.; Zhou, B.; Zhou, C.; Zhou, L.; Zhou, L.; Zhou, N.; Zhu, C. G.; Zhu, H.; Zhu, J.; Zhu, Y.; Zhuang, X.; Zhukov, K.; Zibell, A.; Zieminska, D.; Zimine, N. I.; Zimmermann, C.; Zimmermann, S.; Zinonos, Z.; Zinser, M.; Ziolkowski, M.; Živković, L.; Zobernig, G.; Zoccoli, A.; zur Nedden, M.; Zurzolo, G.; Zwalinski, L.

    2015-08-01

    A search for Higgs boson production in association with a W or Z boson, in the H→ W W* decay channel, is performed with a data sample collected with the ATLAS detector at the LHC in proton-proton collisions at centre-of-mass energies √s=7 TeV and 8 TeV, corresponding to integrated luminosities of 4.5 fb-1 and 20.3 fb-1, respectively. The WH production mode is studied in two-lepton and three-lepton final states, while two- lepton and four-lepton final states are used to search for the ZH production mode. The observed significance, for the combined W H and ZH production, is 2.5 standard deviations while a significance of 0.9 standard deviations is expected in the Standard Model Higgs boson hypothesis. The ratio of the combined W H and ZH signal yield to the Standard Model expectation, μ V H , is found to be μ V H =3.0 -1.1 + 1.3 (stat.) -0.7 +1.0 (sys.) for the Higgs boson mass of 125.36 GeV. The W H and ZH production modes are also combined with the gluon fusion and vector boson fusion production modes studied in the H → W W * → ℓνℓν decay channel, resulting in an overall observed significance of 6.5 standard deviations and μ ggF+VBF+VH=1.16 -0.15 +0.16 (stat.) -0.15 +0.18 (sys.). The results are interpreted in terms of scaling factors of the Higgs boson couplings to vector bosons (κ V ) and fermions (κ F ); the combined results are: |κ V |=1.06 -0.10 +0.10 , |κ F |=0.85 -0.20 +0.26 .

  18. DETECTION OF A DISTINCT METAL-POOR STELLAR HALO IN THE EARLY-TYPE GALAXY NGC3115

    SciTech Connect (OSTI)

    Peacock, Mark B.; Strader, Jay; Romanowsky, Aaron J.; Brodie, Jean P.

    2015-02-10

    We present the resolved stellar populations in the inner and outer halo of the nearby lenticular galaxy NGC3115. Using deep Hubble Space Telescope observations, we analyze stars 2 mag fainter than the tip of the red giant branch (TRGB). We study three fields along the minor axis of this galaxy, 19, 37, and 54kpc from its centercorresponding to 7, 14, and 21 effective radii (r{sub e} ). Even at these large galactocentric distances, all of the fields are dominated by a relatively enriched population, with the main peak in the metallicity distribution decreasing with radius from [Z/H] ? 0.5 to 0.65. The fraction of metal-poor stars ([Z/H] < 0.95) increases from 17% at 16-37 kpc to 28% at ?54kpc. We observe a distinct low-metallicity population (peaked at [Z/H] ? 1.3 and with total mass 2 10{sup 10} M {sub ?} ? 14% of the galaxy's stellar mass) and argue that this represents the detection of an underlying low-metallicity stellar halo. Such halos are generally predicted by galaxy formation theories and have been observed in several late-type galaxies, including the Milky Way and M31. The metallicity and spatial distribution of the stellar halo of NGC3115 are consistent with the galaxy's globular cluster system, which has a similar low-metallicity population that becomes dominant at these large radii. This finding supports the use of globular clusters as bright chemodynamical tracers of galaxy halos. These data also allow us to make a precise measurement of the magnitude of the TRGB, from which we derive a distance modulus of NGC3115 of 30.05 0.05 0.10{sub sys} (10.2 0.2 0.5{sub sys}Mpc)

  19. Numerical Calculation of Neoclassical Distribution Functions and Current Profiles in Low Collisionality, Axisymmetric Plasmas

    SciTech Connect (OSTI)

    B.C. Lyons, S.C. Jardin, and J.J. Ramos

    2012-06-28

    A new code, the Neoclassical Ion-Electron Solver (NIES), has been written to solve for stationary, axisymmetric distribution functions (f ) in the conventional banana regime for both ions and elec trons using a set of drift-kinetic equations (DKEs) with linearized Fokker-Planck-Landau collision operators. Solvability conditions on the DKEs determine the relevant non-adiabatic pieces of f (called h ). We work in a 4D phase space in which ? defines a flux surface, ? is the poloidal angle, v is the total velocity referenced to the mean flow velocity, and ? is the dimensionless magnetic moment parameter. We expand h in finite elements in both v and ?#21; . The Rosenbluth potentials, ?#8; and ?, which define the integral part of the collision operator, are expanded in Legendre series in cos ? , where #31;? is the pitch angle, Fourier series in cos #18;? , and finite elements in v . At each ? , we solve a block tridiagonal system for hi (independent of fe ), then solve another block tridiagonal system for he (dependent on fi ). We demonstrate that such a formulation can be accurately and efficiently solved. NIES is coupled to the MHD equilibrium code JSOLVER [J. DeLucia, et al., J. Comput. Phys. 37 , pp 183-204 (1980).] allowing us to work with realistic magnetic geometries. The bootstrap current is calculated as a simple moment of the distribution function. Results are benchmarked against the Sauter analytic formulas and can be used as a kinetic closure for an MHD code (e.g., M3D-C1 [S.C. Jardin, et al ., Computational Science & Discovery, 4 (2012).]).

  20. Estimating the maximum potential revenue for grid connected electricity storage : arbitrage and regulation.

    SciTech Connect (OSTI)

    Byrne, Raymond Harry; Silva Monroy, Cesar Augusto.

    2012-12-01

    The valuation of an electricity storage device is based on the expected future cash ow generated by the device. Two potential sources of income for an electricity storage system are energy arbitrage and participation in the frequency regulation market. Energy arbitrage refers to purchasing (stor- ing) energy when electricity prices are low, and selling (discharging) energy when electricity prices are high. Frequency regulation is an ancillary service geared towards maintaining system frequency, and is typically procured by the independent system operator in some type of market. This paper outlines the calculations required to estimate the maximum potential revenue from participating in these two activities. First, a mathematical model is presented for the state of charge as a function of the storage device parameters and the quantities of electricity purchased/sold as well as the quantities o ered into the regulation market. Using this mathematical model, we present a linear programming optimization approach to calculating the maximum potential revenue from an elec- tricity storage device. The calculation of the maximum potential revenue is critical in developing an upper bound on the value of storage, as a benchmark for evaluating potential trading strate- gies, and a tool for capital nance risk assessment. Then, we use historical California Independent System Operator (CAISO) data from 2010-2011 to evaluate the maximum potential revenue from the Tehachapi wind energy storage project, an American Recovery and Reinvestment Act of 2009 (ARRA) energy storage demonstration project. We investigate the maximum potential revenue from two di erent scenarios: arbitrage only and arbitrage combined with the regulation market. Our analysis shows that participation in the regulation market produces four times the revenue compared to arbitrage in the CAISO market using 2010 and 2011 data. Then we evaluate several trading strategies to illustrate how they compare to the maximum potential revenue benchmark. We conclude with a sensitivity analysis with respect to key parameters.

  1. Study of (W/Z)H production and Higgs boson couplings using H→ W W * decays with the ATLAS detector

    SciTech Connect (OSTI)

    Aad, G.

    2015-08-27

    A search for Higgs boson production in association with a W or Z boson, in the H→ W W * decay channel, is performed with a data sample collected with the ATLAS detector at the LHC in proton-proton collisions at centre-of-mass energies \\( \\sqrt{s}=7 \\) TeV and 8 TeV, corresponding to integrated luminosities of 4.5 fb-1 and 20.3 fb-1, respectively. The WH production mode is studied in two-lepton and three-lepton final states, while two- lepton and four-lepton final states are used to search for the ZH production mode. The observed significance, for the combined W H and ZH production, is 2.5 standard deviations while a significance of 0.9 standard deviations is expected in the Standard Model Higgs boson hypothesis. The ratio of the combined W H and ZH signal yield to the Standard Model expectation, μV H , is found to be μ V H = 3.0-1.1+1.3 (stat.)-0.7 +1.0 (sys.) for the Higgs boson mass of 125.36 GeV. The W H and ZH production modes are also combined with the gluon fusion and vector boson fusion production modes studied in the H → W W * → ℓνℓν decay channel, resulting in an overall observed significance of 6.5 standard deviations and μggF + VBF + VH = 1.16-0.15+0.16 (stat.) -0.15+0.18 (sys.). The results are interpreted in terms of scaling factors of the Higgs boson couplings to vector bosons (κV ) and fermions (κF ); the combined results are: |κ V | = 1.06-0.10+0.10, |κ F| = 0.85-0.20+0.26.

  2. Measurement of muon neutrino and antineutrino induced single neutral pion production cross sections

    SciTech Connect (OSTI)

    Anderson, Colin; ,

    2010-12-01

    Elucidating the nature of neutrino oscillation continues to be a goal in the vanguard of the efforts of physics experiment. As neutrino oscillation searches seek an increasingly elusive signal, a thorough understanding of the possible backgrounds becomes ever more important. Measurements of neutrino-nucleus interaction cross sections are key to this understanding. Searches for {nu}{sub {mu}} {yields} {nu}{sub e} oscillation - a channel that may yield insight into the vanishingly small mixing parameter {theta}{sub 13}, CP violation, and the neutrino mass hierarchy - are particularly susceptible to contamination from neutral current single {pi}{sup 0} (NC 1{pi}{sup 0}) production. Unfortunately, the available data concerning NC 1{pi}{sup 0} production are limited in scope and statistics. Without satisfactory constraints, theoretical models of NC 1{pi}{sup 0} production yield substantially differing predictions in the critical E{sub {nu}} {approx} 1 GeV regime. Additional investigation of this interaction can ameliorate the current deficiencies. The Mini Booster Neutrino Experiment (MiniBooNE) is a short-baseline neutrino oscillation search operating at the Fermi National Accelerator Laboratory (Fermilab). While the oscillation search is the principal charge of the MiniBooNE collaboration, the extensive data ({approx} 10{sup 6} neutrino events) offer a rich resource with which to conduct neutrino cross section measurements. This work concerns the measurement of both neutrino and antineutrino NC 1{pi}{sup 0} production cross sections at MiniBooNE. The size of the event samples used in the analysis exceeds that of all other similar experiments combined by an order of magnitude. We present the first measurements of the absolute NC 1{pi}{sup 0} cross section as well as the first differential cross sections in both neutrino and antineutrino mode. Specifically, we measure single differential cross sections with respect to pion momentum and pion angle. We find the flux-averaged, total cross sections for NC 1{pi}{sup 0} production on CH{sub 2} to be (4.76 {+-} 0.05{sub stat} {+-} 0.76{sub sys}) x 10{sup -40} cm{sup 2}/nucleon at = 808 MeV for neutrino induced production and (1.48 {+-} 0.05{sub stat} {+-} 0.23{sub sys}) x 10{sup -40} cm{sup 2}/nucleon at = 664 MeV for antineutrino induced production.

  3. Jas

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

    Sh ort w av e Radiat iv e T rans f e r in t h e M ul t is cal e M ode l l ing Fram e w ork Jas on Col e 1 H ow ard Bark e r 2 M arat K h airout dinov 3 Dav id Randal l 4 1 Univ e rs it y of Brit is h Col um bia 2 M e t e orol ogical Se rv ice of Canada 3 St ony Brook Univ e rs it y 4 Col orado St at e Univ e rs it y 1. I nt roduct ion 3. Re s ul t s 2. Expe rim e nt Se t up CSRM Sys t e m f or At m os ph e ric M ode l l ing v e rs ion 6.6.5 (SAM v 6.6.5) * 2D w it h axis orie nt e d w e s t -e

  4. The B*Bπ coupling using relativistic heavy quarks

    SciTech Connect (OSTI)

    Flynn, J. M.; Fritzsch, P.; Kawanai, T.; Lehner, C.; Samways, B.; Sachrajda, C. T.; Van de Water, R. S.; Witzel, O.

    2015-06-23

    We report on a calculation of the B*Bπ coupling in lattice QCD. The strong matrix element (Bπ|B*) is directly related to the leading order low-energy constant in heavy meson chiral perturbation theory (HMΧPT) for B mesons. We carry out our calculation directly at the b-quark mass using a non-perturbatively tuned clover action that controls discretization effects of order |pa| and (ma)n for all n. Our analysis is performed on RBC/UKQCD gauge configurations using domain-wall fermions and the Iwasaki gauge action at two lattice spacings of a–1 = 1.729(25) GeV, a–1 = 2.281 (28) GeV, and unitary pion masses down to 290 MeV. We achieve good statistical precision and control all systematic uncertainties, giving a final result for the HMΧPT coupling gb = 0.56(3)stat(7)sys in the continuum and at the physical light-quark masses. Furthermore, this is the first calculation performed directly at the physical b-quark mass and lies in the region one would expect from carrying out an interpolation between previous results at the charm mass and at the static point.

  5. Gamma-Ray Observations of the Supernova Remnant RX J0852.0-4622 with the Fermi LAT

    SciTech Connect (OSTI)

    Tanaka, T.; Allafort, A.; Ballet, J.; Funk, S.; Giordano, F.; Hewitt, J.; Lemoine-Goumard, M.; Tajima, H.; Tibolla, O.; Uchiyama, Y.; /Stanford U., HEPL /KIPAC, Menlo Park

    2011-12-13

    We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0-4622 with the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope. In the Fermi LAT data, we find a spatially extended source at the location of the SNR. The extension is consistent with the SNR size seen in other wavelengths such as X-rays and TeV gamma rays, leading to the identification of the gamma-ray source with the SNR. The spectrum is well described as a power law with a photon index of {Lambda} = 1.85 {+-} 0.06 (stat){sub -0.19}{sup +0.18} (sys), which smoothly connects to the H.E.S.S. spectrum in the TeV energy band. We discuss the gamma-ray emission mechanism based on multiwavelength data. The broadband data can be fit well by a model in which the gamma rays are of hadronic origin. We also consider a scenario with inverse Compton scattering of electrons as the emission mechanism of the gamma rays. Although the leptonic model predicts a harder spectrum in the Fermi LAT energy range, the model can fit the data considering the statistical and systematic errors.

  6. Central exclusive production at RHIC

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Adamczyk, Leszek; Guryn, Włodek; Turnau, Jacek

    2014-11-10

    The present status and future plans of the physics program of Central Exclusive Production (CEP) at RHIC are described. The measurements are based on the detection of the forward protons from the Double Pomeron Exchange (DPE) process in the Roman Pot system and of the recoil system of charged particles from the DPE process measured in the STAR experiment’s Time Projection Chamber (TPC). The data described here were taken using polarized proton-proton collisions at ps = 200 GeV. The preliminary spectra of two pion and four pion invariant mass reconstructed by STAR TPC in central region of pseudo-rapidity |#17;| sys- tem are presented. Also a possible addition of the Roman Pots to the sPHENIX detector is discussed.« less

  7. Measurement of the nue and Total 8B Solar Neutrino Fluxes with theSudbury Neutrino Observatory Phase I Data Set

    SciTech Connect (OSTI)

    Aharmim, B.; Ahmad, Q.R.; Ahmed, S.N.; Allen, R.C.; Andersen,T.C.; Anglin, J.D.; Buehler, G.; Barton, J.C.; Beier, E.W.; Bercovitch,M.; Bergevin, M.; Bigu, J.; Biller, S.D.; Black, R.A.; Blevis, I.; Boardman, R.J.; Boger, J.; Bonvin, E.; Boulay, M.G.; Bowler, M.G.; Bowles, T.J.; Brice, S.J.; Browne, M.C.; Bullard, T.V.; Burritt, T.H.; Cameron, J.; Chan, Y.D.; Chen, H.H.; Chen, M.; Chen, X.; Cleveland, B.T.; Cowan, J.H.M.; Cowen, D.F.; Cox, G.A.; Currat, C.A.; Dai, X.; Dalnoki-Veress, F.; Davidson, W.F.; Deng, H.; DiMarco, M.; Doe, P.J.; Doucas, G.; Dragowsky, M.R.; Duba, C.A.; Duncan, F.A.; Dunford, M.; Dunmore, J.A.; Earle, E.D.; Elliott, S.R.; Evans, H.C.; Ewan, G.T.; Farine, J.; Fergani, H.; Ferraris, A.P.; Fleurot, F.; Ford, R.J.; Formaggio, J.A.; Fowler, M.M.; Frame, K.; Frank, E.D.; Frati, W.; Gagnon,N.; Germani, J.V.; Gil, S.; Goldschmidt, A.; Goon, J.T.M.; Graham, K.; Grant, D.R.; Guillian, E.; Hahn, R.L.; Hallin, A.L.; Hallman, E.D.; Hamer, A.S.; Hamian, A.A.; Handler, W.B.; Haq, R.U.; Hargrove, C.K.; Harvey, P.J.; Hazama, R.; Heeger, K.M.; Heintzelman, W.J.; Heise, J.; Helmer, R.L.; Henning, R.; Hepburn, J.D.; Heron, H.; Hewett, J.; Hime,A.; Howard, C.; Howe, M.A.; Huang, M.; Hykawy, J.G.; Isaac, M.C.P.; Jagam, P.; Jamieson, B.; Jelley, N.A.; Jillings, C.; Jonkmans, G.; Kazkaz, K.; Keener, P.T.; Kirch, K.; Klein, J.R.; Knox, A.B.; Komar,R.J.; Kormos, L.L.; Kos, M.; Kouzes, R.; Krueger, A.; Kraus, C.; Krauss,C.B.; Kutter, T.; Kyba, C.C.M.; Labranche, H.; Lange, R.; Law, J.; Lawson, I.T.; Lay, M.; Lee, H.W.; Lesko, K.T.; Leslie, J.R.; Levine, I.; Loach, J.C.; Locke, W.; Luoma, S.; Lyon, J.; MacLellan, R.; Majerus, S.; Mak, H.B.; Maneira, J.; Marino, A.D.; Martin, R.; McCauley, N.; McDonald,A.B.; McDonald, D.S.; McFarlane, K.; McGee, S.; McGregor, G.; MeijerDrees, R.; Mes, H.; Mifflin, C.; Miknaitis, K.K.S.; Miller, M.L.; Milton,G.; Moffat, B.A.; Monreal, B.; Moorhead, M.; Morrissette, B.; Nally,C.W.; Neubauer, M.S.; et al.

    2007-02-01

    This article provides the complete description of resultsfrom the Phase I data set of the Sudbury Neutrino Observatory (SNO). ThePhase I data set is based on a 0.65 kt-year exposure of heavy water tothe solar 8B neutrino flux. Included here are details of the SNO physicsand detector model, evaluations of systematic uncertainties, andestimates of backgrounds. Also discussed are SNO's approach tostatistical extraction of the signals from the three neutrino reactions(charged current, neutral current, and elastic scattering) and theresults of a search for a day-night asymmetry in the ?e flux. Under theassumption that the 8B spectrum is undistorted, the measurements fromthis phase yield a solar ?e flux of ?(?e) =1.76+0.05?0.05(stat.)+0.09?0.09 (syst.) x 106 cm?2 s?1, and a non-?ecomponent ?(? mu) = 3.41+0.45?0.45(stat.)+0.48?0.45 (syst.) x 106 cm?2s?1. The sum of these components provides a total flux in excellentagreement with the predictions of Standard Solar Models. The day-nightasymmetry in the ?e flux is found to be Ae = 7.0 +- 4.9 (stat.)+1.3?1.2percent (sys.), when the asymmetry in the total flux is constrained to bezero.

  8. Measurement of the t anti-t production cross section in p anti-p collisions at s**(1/2) = 1.96-TeV

    SciTech Connect (OSTI)

    Ray, Heather Lynn

    2004-02-01

    The direct observation of the top quark was first achieved at the Tevatron proton anti-proton collider at Fermilab. This discovery completed the third generation quark sector where the top quark is expected to accompany the bottom quark in the weak isospin doublet. This dissertation discusses the experimental verification of the production cross section as predicted by the Standard Model. A measurement of the t{bar t} production cross section using 107.9 pb{sup -1} of p{bar p} collisions at {radical}s = 1.96 TeV collected with the Collider Detector at Fermilab between March of 2003 and June of 2003 is presented. The measurement focuses on the t{bar t} production in the ''lepton plus jets'' final state in which one of the W bosons from the t{bar t} decay subsequently decays leptonically to an electron or a muon, and the other decays hadronically. The B-tagging technique which utilizes the precision silicon detector tracking is used to enhance the signal for t{bar t} events relative to the background through identification of the bottom quark from its measurable lifetime. The t{bar t} production cross section is measured to be {sigma}{sub t{bar t}} = 4.5 {+-} 1.4(stat) {+-} 0.8(sys) pb.

  9. HerMES: A DEFICIT IN THE SURFACE BRIGHTNESS OF THE COSMIC INFRARED BACKGROUND DUE TO GALAXY CLUSTER GRAVITATIONAL LENSING

    SciTech Connect (OSTI)

    Zemcov, M.; Cooray, A.; Bock, J.; Dowell, C. D.; Nguyen, H. T.; Blain, A.; Bethermin, M.; Conley, A.; Glenn, J.; Conversi, L.; Farrah, D.; Oliver, S. J.; Roseboom, I. G.; Griffin, M.; Halpern, M.; Marsden, G.; Jullo, E.; Kneib, J.-P.; Richard, J.; and others

    2013-06-01

    We have observed four massive galaxy clusters with the SPIRE instrument on the Herschel Space Observatory and measure a deficit of surface brightness within their central region after removing detected sources. We simulate the effects of instrumental sensitivity and resolution, the source population, and the lensing effect of the clusters to estimate the shape and amplitude of the deficit. The amplitude of the central deficit is a strong function of the surface density and flux distribution of the background sources. We find that for the current best fitting faint end number counts, and excellent lensing models, the most likely amplitude of the central deficit is the full intensity of the cosmic infrared background (CIB). Our measurement leads to a lower limit to the integrated total intensity of the CIB of I{sub 250{mu}m}>0.69{sub -0.03}{sup +0.03}(stat.){sub -0.06}{sup +0.11}(sys.) MJy sr{sup -1}, with more CIB possible from both low-redshift sources and from sources within the target clusters. It should be possible to observe this effect in existing high angular resolution data at other wavelengths where the CIB is bright, which would allow tests of models of the faint source component of the CIB.

  10. GADRAS isotope ID users manual for analysis of gamma-ray measurements and API for Linux and Android .

    SciTech Connect (OSTI)

    Mitchell, Dean J; Harding, Lee T.

    2014-05-01

    Isotope identification algorithms that are contained in the Gamma Detector Response and Analysis Software (GADRAS) can be used for real-time stationary measurement and search applications on platforms operating under Linux or Android operating sys-tems. Since the background radiation can vary considerably due to variations in natu-rally-occurring radioactive materials (NORM), spectral algorithms can be substantial-ly more sensitive to threat materials than search algorithms based strictly on count rate. Specific isotopes or interest can be designated for the search algorithm, which permits suppression of alarms for non-threatening sources, such as such as medical radionuclides. The same isotope identification algorithms that are used for search ap-plications can also be used to process static measurements. The isotope identification algorithms follow the same protocols as those used by the Windows version of GADRAS, so files that are created under the Windows interface can be copied direct-ly to processors on fielded sensors. The analysis algorithms contain provisions for gain adjustment and energy lineariza-tion, which enables direct processing of spectra as they are recorded by multichannel analyzers. Gain compensation is performed by utilizing photopeaks in background spectra. Incorporation of this energy calibration tasks into the analysis algorithm also eliminates one of the more difficult challenges associated with development of radia-tion detection equipment.

  11. Tracking the Performance Evolution of Blue Gene Systems

    SciTech Connect (OSTI)

    Kerbyson, Darren J.; Barker, Kevin J.; Gallo, Diego S.; Chen, Dong; Brunheroto, Jose R.; Ryu, Kyung D.; Chiu, George L.; Hoisie, Adolfy

    2013-06-17

    IBMs Blue Gene supercomputer has evolved through three generations from the original Blue Gene/L to P to Q. A higher level of integration has enabled greater single-core performance, and a larger concurrency per compute node. Although these changes have brought with them a higher overall system peak-performance, no study has examined in detail the evolution of perfor-mance across system generations. In this work we make two significant contri-butions that of providing a comparative performance analysis across Blue Gene generations using a consistent set of tests, and also in providing a validat-ed performance model of the NEK-Bone proxy application. The combination of empirical analysis and the predictive performance model enable us to not only directly compare measured performance but also allow for a comparison of sys-tem configurations that cannot currently be measured. We provide insights into how the changing characteristics of Blue Gene have impacted on the application performance, as well as what future systems may be able to achieve.

  12. The Mass Distribution and Assembly of the Milky Way from the Properties of the Magellanic Clouds

    SciTech Connect (OSTI)

    Busha, Michael T.; Marshall, Philip J.; Wechsler, Risa H.; Klypin, Anatoly; Primack, Joel; /UC, Santa Cruz, Phys. Dept.

    2012-02-29

    We present a new measurement of the mass of the Milky Way (MW) based on observed properties of its largest satellite galaxies, the Magellanic Clouds (MCs), and an assumed prior of a {Lambda}CDM universe. The large, high-resolution Bolshoi cosmological simulation of this universe provides a means to statistically sample the dynamical properties of bright satellite galaxies in a large population of dark matter halos. The observed properties of the MCs, including their circular velocity, distance from the center of the MW, and velocity within the MW halo, are used to evaluate the likelihood that a given halo would have each or all of these properties; the posterior probability distribution function (PDF) for any property of the MW system can thus be constructed. This method provides a constraint on the MW virial mass, 1.2{sup +0.7} - {sub 0.4}(stat.){sup +0.3} - {sub 0.3}(sys.) x 10{sup 12} M {circle_dot} (68% confidence), which is consistent with recent determinations that involve very different assumptions. In addition, we calculate the posterior PDF for the density profile of the MW and its satellite accretion history. Although typical satellites of 10{sup 12} M {circle_dot} halos are accreted over a wide range of epochs over the last 10 Gyr, we find a {approx}72% probability that the MCs were accreted within the last Gyr, and a 50% probability that they were accreted together.

  13. Measurement of the atmospheric muon charge ratio at TeV energies with MINOS

    SciTech Connect (OSTI)

    Adamson, P.; Andreopoulos, C.; Arms, K.E.; Armstrong, R.; Auty, D.J.; Avvakumov, S.; Ayres, D.S.; Baller, B.; Barish, B.; Barnes, P.D., Jr.; Barr, G.; /Fermilab /University Coll. London /Rutherford /Minnesota U. /Indiana U. /Sussex U. /Stanford U., Phys. Dept. /Argonne /Caltech /LLNL, Livermore /Oxford U.

    2007-05-01

    The 5.4 kton MINOS far detector has been taking charge-separated cosmic ray muon data since the beginning of August, 2003 at a depth of 2070 m.w.e. in the Soudan Underground Laboratory, Minnesota, USA. The data with both forward and reversed magnetic field running configurations were combined to minimize systematic errors in the determination of the underground muon charge ratio. When averaged, two independent analyses find the charge ratio underground to be N{sub {mu}}+/N{sub {mu}}-=1.374{+-}0.004(stat)-0.010{sup +0.012}(sys). Using the map of the Soudan rock overburden, the muon momenta as measured underground were projected to the corresponding values at the surface in the energy range 1-7 TeV. Within this range of energies at the surface, the MINOS data are consistent with the charge ratio being energy independent at the 2 standard deviation level. When the MINOS results are compared with measurements at lower energies, a clear rise in the charge ratio in the energy range 0.3-1.0 TeV is apparent. A qualitative model shows that the rise is consistent with an increasing contribution of kaon decays to the muon charge ratio.

  14. High resolution spectroscopic study of BeΛ10

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Gogami, T.; Chen, C.; Kawama, D.; Achenbach, P.; Ahmidouch, A.; Albayrak, I.; Androic, D.; Asaturyan, A.; Asaturyan, R.; Ates, O.; et al

    2016-03-10

    Spectroscopy of amore » $$^{10}_{\\Lambda}$$Be hypernucleus was carried out at JLab Hall C using the $$(e,e^{\\prime}K^{+})$$ reaction. A new magnetic spectrometer system (SPL+HES+HKS), specifically designed for high resolution hypernuclear spectroscopy, was used to obtain an energy spectrum with a resolution of 0.78 MeV (FWHM). The well-calibrated spectrometer system of the present experiment using the $$p(e,e^{\\prime}K^{+})\\Lambda,\\Sigma^{0}$$ reactions allowed us to determine the energy levels, and the binding energy of the ground state peak (mixture of 1$$^{-}$$ and 2$$^{-}$$ states) was obtained to be B$$_{\\Lambda}$$=8.55$$\\pm$$0.07(stat.)$$\\pm$$0.11(sys.) MeV. Furthermore, the result indicates that the ground state energy is shallower than that of an emulsion study by about 0.5 MeV which provides valuable experimental information on charge symmetry breaking effect in the $$\\Lambda N$$ interaction.« less

  15. Symmetrical and Unsymmetrical Fault Currents of a Wind Power Plant: Preprint

    SciTech Connect (OSTI)

    Gevorgian, V.; Singh, M.; Muljadi, E.

    2011-12-01

    This paper investigates the short-circuit behavior of a wind power plant for different types of wind turbines. Both symmetrical faults and unsymmetrical faults are investigated. The size of wind power plants (WPPs) keeps getting bigger and bigger. The number of wind plants in the U.S. has increased very rapidly in the past 10 years. It is projected that in the U.S., the total wind power generation will reach 330 GW by 2030. As the importance of WPPs increases, planning engi-neers must perform impact studies used to evaluate short-circuit current (SCC) contribution of the plant into the transmission network under different fault conditions. This information is needed to size the circuit breakers, to establish the proper sys-tem protection, and to choose the transient suppressor in the circuits within the WPP. This task can be challenging to protec-tion engineers due to the topology differences between different types of wind turbine generators (WTGs) and the conventional generating units. This paper investigates the short-circuit behavior of a WPP for different types of wind turbines. Both symmetrical faults and unsymmetrical faults are investigated. Three different soft-ware packages are utilized to develop this paper. Time domain simulations and steady-state calculations are used to perform the analysis.

  16. Measurement of the Cosmic Ray and Neutrino-Induced Muon Flux at the Sudbury Neutrino Observatory

    DOE R&D Accomplishments [OSTI]

    SNO collaboration; Aharmim, B.; Ahmed, S. N.; Andersen, T. C.; Anthony, A. E.; Barros, N.; Beier, E. W.; Bellerive, A.; Beltran, B.; Bergevin, M.; Biller, S. D.; Boudjemline, K.; Boulay, M. G.; Burritt, T. H.; Cai, B.; Chan, Y. D.; Chen, M.; Chon, M. C.; Cleveland, B. T.; Cox-Mobrand, G. A.; Currat, C. A.; Dai, X.; Dalnoki-Veress, F.; Deng, H.; Detwiler, J.; Doe, P. J.; Dosanjh, R. S.; Doucas, G.; Drouin, P.-L.; Duncan, F. A.; Dunford, M.; Elliott, S. R.; Evans, H. C.; Ewan, G. T.; Farine, J.; Fergani, H.; Fleurot, F.; Ford, R. J.; Formaggio, J. A.; Gagnon, N.; Goon, J. TM.; Grant, D. R.; Guillian, E.; Habib, S.; Hahn, R. L.; Hallin, A. L.; Hallman, E. D.; Hargrove, C. K.; Harvey, P. J.; Harvey, P. J.; Heeger, K. M.; Heintzelman, W. J.; Heise, J.; Helmer, R. L.; Hemingway, R. J.; Henning, R.; Hime, A.; Howard, C.; Howe, M. A.; Huang, M.; Jamieson, B.; Jelley, N. A.; Klein, J. R.; Kos, M.; Kruger, A.; Kraus, C.; Krauss, C. B.; Kutter, T.; Kyba, C. C. M.; Lange, R.; Law, J.; Lawson, I. T.; Lesko, K. T.; Leslie, J. R.; Levine, I.; Loach, J. C.; Luoma, S.; MacLellan, R.; Majerus, S.; Mak, H. B.; Maneira, J.; Marino, A. D.; Martin, R.; McCauley, N.; McDonald, A. B.; McGee, S.; Mifflin, C.; Miller, M. L.; Monreal, B.; Monroe, J.; Noble, A. J.; Oblath, N. S.; Okada, C. E.; O'Keeffe, H. M.; Opachich, Y.; Orebi Gann, G. D.; Oser, S. M.; Ott, R. A.; Peeters, S. J. M.; Poon, A. W. P.; Prior, G.; Rielage, K.; Robertson, B. C.; Robertson, R. G. H.; Rollin, E.; Schwendener, M. H.; Secrest, J. A.; Seibert, S. R.; Simard, O.; Simpson, J. J.; Sinclair, D.; Skensved, P.; Smith, M. W. E.; Sonley, T. J.; Steiger, T. D.; Stonehill, L. C.; Tagg, N.; Tesic, G.; Tolich, N.; Tsui, T.; Van de Water, R. G.; VanDevender, B. A.; Virtue, C. J.; Waller, D.; Waltham, C. E.; Wan Chan Tseung, H.; Wark, D. L.; Watson, P.; Wendland, J.; West, N.; Wilkerson, J. F.; Wilson, J. R.; Wouters, J. M.; Wright, A.; Yeh, M.; Zhang, F.; Zuber, K.

    2009-07-10

    Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and un-oscillated portion of the neutrino flux. A total of 514 muon-like events are measured between -1 {le} cos {theta}{sub zenith} 0.4 in a total exposure of 2.30 x 10{sup 14} cm{sup 2} s. The measured flux normalization is 1.22 {+-} 0.09 times the Bartol three-dimensional flux prediction. This is the first measurement of the neutrino-induced flux where neutrino oscillations are minimized. The zenith distribution is consistent with previously measured atmospheric neutrino oscillation parameters. The cosmic ray muon flux at SNO with zenith angle cos {theta}{sub zenith} > 0.4 is measured to be (3.31 {+-} 0.01 (stat.) {+-} 0.09 (sys.)) x 10{sup -10} {micro}/s/cm{sup 2}.

  17. A High Performance Computing Network and System Simulator for the Power Grid: NGNS^2

    SciTech Connect (OSTI)

    Villa, Oreste; Tumeo, Antonino; Ciraci, Selim; Daily, Jeffrey A.; Fuller, Jason C.

    2012-11-11

    Designing and planing next generation power grid sys- tems composed of large power distribution networks, monitoring and control networks, autonomous generators and consumers of power requires advanced simulation infrastructures. The objective is to predict and analyze in time the behavior of networks of systems for unexpected events such as loss of connectivity, malicious attacks and power loss scenarios. This ultimately allows one to answer questions such as: What could happen to the power grid if .... We want to be able to answer as many questions as possible in the shortest possible time for the largest possible systems. In this paper we present a new High Performance Computing (HPC) oriented simulation infrastructure named Next Generation Network and System Simulator (NGNS2 ). NGNS2 allows for the distribution of a single simulation among multiple computing elements by using MPI and OpenMP threads. NGNS2 provides extensive configuration, fault tolerant and load balancing capabilities needed to simulate large and dynamic systems for long periods of time. We show the preliminary results of the simulator running approximately two million simulated entities both on a 64-node commodity Infiniband cluster and a 48-core SMP workstation.

  18. A Study of Charged Current Single Charged Pion Productions on Carbon in a Few-GeV Neutrino Beam

    SciTech Connect (OSTI)

    Hiraide, Katsuki; /Kyoto U.

    2009-01-01

    Understanding single charged pion production via neutrino-nucleus charged current interaction in the neutrino energy region of a few GeV is essential for future neutrino oscillation experiments since this process is a dominant background for {nu}{sub {mu}} {yields} {nu}{sub x} oscillation measurements. There are two contributions to this process: single pion production via baryonic resonance ({nu}{sub {mu}}N {yields} {mu}{sup -} N{pi}{sup +}) and coherent pion production interacting with the entire nucleus ({nu}{sub {mu}}A {yields} {mu}{sup -} A{pi}{sup +}), where N is nucleon in the nucleus and A is the nucleus. The purpose of the study presented in this thesis is a precise measurement of charged current single charged pion productions, resonant and coherent pion productions, with a good final state separation in the neutrino energy region of a few GeV. In this thesis, we focus on the study of charged current coherent pion production from muon neutrinos scattering on carbon, {nu}{sub {mu}} {sup 12}C {yields} {mu}{sup -12}C{pi}{sup +}, in the SciBooNE experiment. This is motivated by the fact that without measuring this component first, the precise determination of resonant pion production cross section can not be achieved since the contribution of coherent pion production in the region of small muon scattering angle is not small. Furthermore, the coherent process is particularly interesting because it is deeply rooted in fundamental physics via Adler's partially conserved axial-vector current theorem. We took data from June 2007 until August 2008, in both the neutrino and antineutrino beam. In total, 2.52 x 10{sup 20} protons on target were collected. We have performed a search for charged current coherent pion production by using SciBooNE's full neutrino data set, corresponding to 0.99 x 10{sup 20} protons on target. No evidence for coherent pion production is observed. We set 90% confidence level upper limits on the cross section ratio of charged current coherent pion production to the total charged current cross section at 0.67 x 10{sup -2} at mean neutrino energy 1.1 GeV and 1.36 x 10{sup -2} at mean neutrino energy 2.2 GeV. We reveal that the Rein-Sehgal model widely used in neutrino oscillation experiments breaks down at the neutrino energy region of a few GeV. This creates active controversies on the model of coherent pion production, and the understanding of coherent pion production is being progressed. In addition, future prospects of measurements of charged current single charged pion production in SciBooNE are discussed.

  19. Search for WW and WZ production in lepton, neutrino plus jets final states at CDF Run II and Silicon module production and detector control system for the ATLAS SemiConductor Tracker

    SciTech Connect (OSTI)

    Sfyrla, Anna; /Geneva U.

    2008-03-01

    In the first part of this work, we present a search for WW and WZ production in charged lepton, neutrino plus jets final states produced in p{bar p} collisions with {radical}s = 1.96 TeV at the Fermilab Tevatron, using 1.2 fb{sup -1} of data accumulated with the CDF II detector. This channel is yet to be observed in hadron colliders due to the large singleWplus jets background. However, this decay mode has a much larger branching fraction than the cleaner fully leptonic mode making it more sensitive to anomalous triple gauge couplings that manifest themselves at higher transverse W momentum. Because the final state is topologically similar to associated production of a Higgs boson with a W, the techniques developed in this analysis are also applicable in that search. An Artificial Neural Network has been used for the event selection optimization. The theoretical prediction for the cross section is {sigma}{sub WW/WZ}{sup theory} x Br(W {yields} {ell}{nu}; W/Z {yields} jj) = 2.09 {+-} 0.14 pb. They measured N{sub Signal} = 410 {+-} 212(stat) {+-} 102(sys) signal events that correspond to a cross section {sigma}{sub WW/WZ} x Br(W {yields} {ell}{nu}; W/Z {yields} jj) = 1.47 {+-} 0.77(stat) {+-} 0.38(sys) pb. The 95% CL upper limit to the cross section is estimated to be {sigma} x Br(W {yields} {ell}{nu}; W/Z {yields} jj) < 2.88 pb. The second part of the present work is technical and concerns the ATLAS SemiConductor Tracker (SCT) assembly phase. Although technical, the work in the SCT assembly phase is of prime importance for the good performance of the detector during data taking. The production at the University of Geneva of approximately one third of the silicon microstrip end-cap modules is presented. This collaborative effort of the university of Geneva group that lasted two years, resulted in 655 produced modules, 97% of which were good modules, constructed within the mechanical and electrical specifications and delivered in the SCT collaboration for assembly on the end-cap disks. The SCT end-caps and barrels consist of 4088 silicon modules, with a total of 6.3 million readout channels. The coherent and safe operation of the SCT during commissioning and subsequent operation is the essential task of the Detector Control System (DCS). The main building blocks of the DCS are the cooling system, the power supplies and the environmental system. The DCS has been initially developed for the SCT assembly phase and this system is described in the present work. Particular emphasis is given in the environmental hardware and software components, that were my major contributions. Results from the DCS testing during the assembly phase are also reported.

  20. Measurements of dielectron production in Au + Au collisions at sNN=200 GeV from the STAR experiment

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Adamczyk, L.; Adkins, J. K.; Agakishiev, G.; Aggarwal, M. M.; Ahammed, Z.; Alekseev, I.; Alford, J.; Aparin, A.; Arkhipkin, D.; Aschenauer, E. C.; et al

    2015-08-24

    We report on measurements of dielectron (e⁺e⁻) production in Au+Au collisions at a center-of-mass energy of 200 GeV per nucleon-nucleon pair using the STAR detector at RHIC. Systematic measurements of the dielectron yield as a function of transverse momentum (pT) and collision centrality show an enhancement compared to a cocktail simulation of hadronic sources in the low invariant-mass region (Mee < 1GeV/c2). This enhancement cannot be reproduced by the ρ-meson vacuum spectral function. In minimum-bias collisions, in the invariant-mass range of 0.30 – 0.76GeV/c², integrated over the full pT acceptance, the enhancement factor is 1.76±0.06(stat.)±0.26(sys.)±0.29(cocktail). The enhancement factor exhibits weakmore » centrality and pT dependence in STAR's accessible kinematic regions, while the excess yield in this invariant-mass region as a function of the number of participating nucleons follows a power-law shape with a power of 1.44±0.10. Models that assume an in-medium broadening of the ρ-meson spectral function consistently describe the observed excess in these measurements. In addition, we report on measurements of ω- and Φ-meson production through their e⁺e⁻ decay channel. These measurements show good agreement with Tsallis blast-wave model predictions, as well as, in the case of the Φ meson, results through its K⁺K⁻ decay channel. In the intermediate invariant-mass region (1.1 < Mee < 3GeV/c²), we investigate the spectral shapes from different collision centralities. Physics implications for possible in-medium modification of charmed hadron production and other physics sources are discussed.« less

  1. Demonstration of fully coupled simplified extended station black-out accident simulation with RELAP-7

    SciTech Connect (OSTI)

    Zhao, Haihua; Zhang, Hongbin; Zou, Ling; Anders, David; Martineau, Richard

    2014-10-01

    The RELAP-7 code is the next generation nuclear reactor system safety analysis code being developed at the Idaho National Laboratory (INL). The RELAP-7 code develop-ment effort started in October of 2011 and by the end of the second development year, a number of physical components with simplified two phase flow capability have been de-veloped to support the simplified boiling water reactor (BWR) extended station blackout (SBO) analyses. The demonstration case includes the major components for the primary system of a BWR, as well as the safety system components for the safety relief valve (SRV), the reactor core isolation cooling (RCIC) system, and the wet well. Three scenar-ios for the SBO simulations have been considered. Since RELAP-7 is not a severe acci-dent analysis code, the simulation stops when fuel clad temperature reaches damage point. Scenario I represents an extreme station blackout accident without any external cooling and cooling water injection. The system pressure is controlled by automatically releasing steam through SRVs. Scenario II includes the RCIC system but without SRV. The RCIC system is fully coupled with the reactor primary system and all the major components are dynamically simulated. The third scenario includes both the RCIC system and the SRV to provide a more realistic simulation. This paper will describe the major models and dis-cuss the results for the three scenarios. The RELAP-7 simulations for the three simplified SBO scenarios show the importance of dynamically simulating the SRVs, the RCIC sys-tem, and the wet well system to the reactor safety during extended SBO accidents.

  2. Systematic uncertainties associated with the cosmological analysis of the first Pan-STARRS1 type Ia supernova sample

    SciTech Connect (OSTI)

    Scolnic, D.; Riess, A.; Brout, D.; Rodney, S. [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Rest, A. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Huber, M. E.; Tonry, J. L. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Foley, R. J.; Chornock, R.; Berger, E.; Soderberg, A. M.; Stubbs, C. W.; Kirshner, R. P.; Challis, P.; Czekala, I.; Drout, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Narayan, G. [Department of Physics, Harvard University, 17 Oxford Street, Cambridge, MA 02138 (United States); Smartt, S. J.; Botticella, M. T. [Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast, Belfast BT7 1NN (United Kingdom); Schlafly, E. [Max Planck Institute for Astronomy, Konigstuhl 17, D-69117 Heidelberg (Germany); and others

    2014-11-01

    We probe the systematic uncertainties from the 113 Type Ia supernovae (SN Ia) in the Pan-STARRS1 (PS1) sample along with 197 SN Ia from a combination of low-redshift surveys. The companion paper by Rest et al. describes the photometric measurements and cosmological inferences from the PS1 sample. The largest systematic uncertainty stems from the photometric calibration of the PS1 and low-z samples. We increase the sample of observed Calspec standards from 7 to 10 used to define the PS1 calibration system. The PS1 and SDSS-II calibration systems are compared and discrepancies up to ?0.02 mag are recovered. We find uncertainties in the proper way to treat intrinsic colors and reddening produce differences in the recovered value of w up to 3%. We estimate masses of host galaxies of PS1 supernovae and detect an insignificant difference in distance residuals of the full sample of 0.037 0.031 mag for host galaxies with high and low masses. Assuming flatness and including systematic uncertainties in our analysis of only SNe measurements, we find w =?1.120{sub ?0.206}{sup +0.360}(Stat){sub ?0.291}{sup +0.269}(Sys). With additional constraints from Baryon acoustic oscillation, cosmic microwave background (CMB) (Planck) and H {sub 0} measurements, we find w=?1.166{sub ?0.069}{sup +0.072} and ?{sub m}=0.280{sub ?0.012}{sup +0.013} (statistical and systematic errors added in quadrature). The significance of the inconsistency with w = 1 depends on whether we use Planck or Wilkinson Microwave Anisotropy Probe measurements of the CMB: w{sub BAO+H0+SN+WMAP}=?1.124{sub ?0.065}{sup +0.083}.

  3. Type Ia supernova rate measurements to redshift 2.5 from CANDELS: Searching for prompt explosions in the early universe

    SciTech Connect (OSTI)

    Rodney, Steven A.; Riess, Adam G.; Graur, Or; Jones, David O. [Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218 (United States); Strolger, Louis-Gregory; Dahlen, Tomas; Casertano, Stefano; Ferguson, Henry C.; Koekemoer, Anton M. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Dickinson, Mark E. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Garnavich, Peter [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Hayden, Brian [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Jha, Saurabh W.; McCully, Curtis; Patel, Brandon [Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, NJ 08854 (United States); Kirshner, Robert P. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Weiner, Benjamin J. [Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States); Cenko, S. Bradley [Astrophysics Science Division, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771 (United States); Clubb, Kelsey I. [Department of Astronomy, University of California, Berkeley, CA 94720 (United States); and others

    2014-07-01

    The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) was a multi-cycle treasury program on the Hubble Space Telescope (HST) that surveyed a total area of ?0.25 deg{sup 2} with ?900 HST orbits spread across five fields over three years. Within these survey images we discovered 65 supernovae (SNe) of all types, out to z ? 2.5. We classify ?24 of these as Type Ia SNe (SNe Ia) based on host galaxy redshifts and SN photometry (supplemented by grism spectroscopy of six SNe). Here we present a measurement of the volumetric SN Ia rate as a function of redshift, reaching for the first time beyond z = 2 and putting new constraints on SN Ia progenitor models. Our highest redshift bin includes detections of SNe that exploded when the universe was only ?3 Gyr old and near the peak of the cosmic star formation history. This gives the CANDELS high redshift sample unique leverage for evaluating the fraction of SNe Ia that explode promptly after formation (<500 Myr). Combining the CANDELS rates with all available SN Ia rate measurements in the literature we find that this prompt SN Ia fraction is f{sub P} = 0.53{sub stat0.10}{sup 0.09}{sub sys0.26}{sup 0.10}, consistent with a delay time distribution that follows a simple t {sup 1} power law for all times t > 40 Myr. However, mild tension is apparent between ground-based low-z surveys and space-based high-z surveys. In both CANDELS and the sister HST program CLASH (Cluster Lensing And Supernova Survey with Hubble), we find a low rate of SNe Ia at z > 1. This could be a hint that prompt progenitors are in fact relatively rare, accounting for only 20% of all SN Ia explosionsthough further analysis and larger samples will be needed to examine that suggestion.

  4. Study of B̄→Xulν̄ decays in BB̄ events tagged by a fully reconstructed B-meson decay and determination of |Vub|

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Lees, J. P.; Poireau, V.; Tisserand, V.; Garra Tico, J.; Grauges, E.; Martinelli, M.; Milanes, D. A.; Palano, A.; Pappagallo, M.; Eigen, G.; et al

    2012-08-07

    We report measurements of partial branching fractions for inclusive charmless semileptonic B decays B¯¯¯→Xulν¯ and the determination of the Cabibbo–Kobayashi–Maskawa (CKM) matrix element |Vub|. The analysis is based on a sample of 467×10⁶ Υ(4S)→BB¯¯¯ decays recorded with the BABAR detector at the PEP-II e⁺e⁻ storage rings. We select events in which the decay of one of the B mesons is fully reconstructed and an electron or a muon signals the semileptonic decay of the other B meson. We measure partial branching fractions ΔB in several restricted regions of phase space and determine the CKM element |Vub| based on different QCDmore » predictions. For decays with a charged lepton momentum p*l>1.0 GeV in the B meson rest frame, we obtain ΔB=(1.80±0.13stat±0.15sys±0.02theo)×10⁻³ from a fit to the two-dimensional MX-q² distribution. Here, MX refers to the invariant mass of the final state hadron X and q² is the invariant mass squared of the charged lepton and neutrino. From this measurement we extract |Vub|=(4.33±0.24exp±0.15theo)×10⁻³ as the arithmetic average of four results obtained from four different QCD predictions of the partial rate. We separately determine partial branching fractions for B¯¯¯0 and B⁻ decays and derive a limit on the isospin breaking in B¯¯¯→Xulν¯ decays.« less

  5. Search for supersymetric particles desintegrant itself in R-parite violee (coupling lambda_121) in a final state has three leptons

    SciTech Connect (OSTI)

    Magnan, Anne-Marie

    2005-07-01

    This thesis is dedicated to the study of the first data taken by the D0 detector during the Run II of the Tevatron. Supersymmetric particles have been search for in proton-antiproton collisions, with a center of mass energy of 1.96 TeV. In the framework of supersymmetry with R-parity violation, I have studied the pair production of Gauginos, leading to a pair of LSP ({chi}{sub 1}{sup 0}), each one decaying into ee{nu}{sub {mu}} or e{mu}{nu}{sub e} with a {lambda}{sub 121} coupling. The final state contains at least two electrons: I have thus paid special attention in this work to the methods concerning identification and mis-identification of electromagnetic particles, as well as reconstruction, triggering, and correction (of the reconstructed energy). In a selection of trileptons, with at least two electrons, and some transverse missing energy, we observed 0 event in the 350 pb{sup -1} of analyzed data, for 0,4{sub -0,05}{sup +0,35}(stat) {+-} 0,16 (sys) expected from the Standard Model contributions. In the signal considered in this analysis, the selection efficiency is around 12%. Results have been studied in two models: mSUGRA and MSSM. In mSUGRA model, limits on m{sub 1/2} and lightest gauginos's masses have been obtained, with tan{beta} = 5, A{sub 0} = 0, m{sub 0} = 100 and 1000 GeV.c{sup -2} and both signs of {mu}. In MSSM, with the hypothesis of massive sfermions (1000 GeV.c{sup -2}), we can exclude, at 95% Confidence Level, the region m{sub {chi}{sub 1}}{+-} < 200 GeV.c{sup -2}, for all masses of {chi}{sub 1}{sup 0} LSP.

  6. Code System Calculate One-Dimensional Vertical Transport Unsaturated Soil Zone

    Energy Science and Technology Software Center (OSTI)

    1989-03-01

    SESOIL, as an integrated screening-level soil compartment model, is designed to simultaneously model water transport, sediment transport, and pollutant fate. SESOIL is a one-dimensional vertical transport model for the unsaturated soil zone. Only one compound at a time can be considered. The model is based on mass balance and equilibrium partitioning of the chemical between different phases (dissolved, sorbed, vapor, and pure). The SESOIL model was designed to perform long-term simulations of chemical transport andmore » transformations in the soil and uses theoretically derived equations to represent water transport, sediment transport on the land surface, pollutant transformation, and migration of the pollutant to the atmosphere and groundwater. Climatic data, compartment geometry, and soil and chemical property data are the major components used in the equations. SESOIL was developed as a screening-level model, utilizing less soil, chemical, and meteorological values as input than most other similar models. Output of SESOIL includes time-varying pollutant concentrations at various soil depths and pollutant loss from the unsaturated zone in terms of surface runoff, percolation to the groundwater, volatilization, and degradation. The February 1995 release corrects an error that caused the code to fail when average monthly air temperature was -10C and includes an improved iteration procedure for the mass balance equations in the model. PLEASE NOTE: The RISKPRO information management software (see OTHER PROG/OPER SYS INFO) was used by the developers of the New SESOIL User''s Guide in their study and revisions of SESOIL. Using RISKPRO in conjunction with SESOIL is an option, and it may provide the easiest way to use SESOIL. The other option, use of SESOIL in stand-alone mode, has been tested and used. The stand-alone option is covered in ''Instructions for Running Stand-Alone SESOIL Code'', and in ''A Seasonal Soil Compartment Model''.« less

  7. DEVELOPING THE NATIONAL GEOTHERMAL DATA SYSTEM ADOPTION OF CKAN FOR DOMESTIC & INTERNATIONAL DATA DEPLOYMENT

    SciTech Connect (OSTI)

    Clark, Ryan J.; Kuhmuench, Christoph; Richard, Stephen M.

    2013-01-01

    The National Geothermal Data System (NGDS) De- sign and Testing Team is developing NGDS software currently referred to as the “NGDS Node-In-A-Box”. The software targets organizations or individuals who wish to host at least one of the following: • an online repository containing resources for the NGDS; • an online site for creating metadata to register re- sources with the NGDS • NDGS-conformant Web APIs that enable access to NGDS data (e.g., WMS, WFS, WCS); • NDGS-conformant Web APIs that support dis- covery of NGDS resources via catalog service (e.g. CSW) • a web site that supports discovery and under- standing of NGDS resources A number of different frameworks for development of this online application were reviewed. The NGDS Design and Testing Team determined to use CKAN (http://ckan.org/), because it provides the closest match between out of the box functionality and NGDS node-in-a-box requirements. To achieve the NGDS vision and goals, this software development project has been inititated to provide NGDS data consumers with a highly functional inter- face to access the system, and to ease the burden on data providers who wish to publish data in the sys- tem. It is important to note that this software package constitutes a reference implementation. The NGDS software is based on open standards, which means other server software can make resources available, and other client applications can utilize NGDS data. A number of international organizations have ex- pressed interest in the NGDS approach to data access. The CKAN node implementation can provide a sim- ple path for deploying this technology in other set- tings.

  8. The L_X-M relation of Clusters of Galaxies

    SciTech Connect (OSTI)

    Rykoff, E.S.; Evrard, A.E.; McKay, T.A.; Becker, M.R.; Johnston, D.E.; Koester, B.P.; Nord, B.; Rozo, E.; Sheldon, E.S.; Stanek, R.; Wechsler, R.H.

    2008-05-16

    We present a new measurement of the scaling relation between X-ray luminosity and total mass for 17,000 galaxy clusters in the maxBCG cluster sample. Stacking sub-samples within fixed ranges of optical richness, N200, we measure the mean 0.1-2.4 keV X-ray luminosity, , from the ROSAT All-Sky Survey. The mean mass, , is measured from weak gravitational lensing of SDSS background galaxies (Johnston et al. 2007). For 9 {le} N{sub 200} < 200, the data are well fit by a power-law, /10{sup 42} h{sup -2} ergs{sup -1} = (12.6{sub -1.3}{sup +1.4}(stat) {+-} 1.6 (sys)) (/10{sup 14} h{sup -1} M{sub {circle_dot}}){sup 1.65{+-}0.13}. The slope agrees to within 10% with previous estimates based on X-ray selected catalogs, implying that the covariance in L{sub X} and N{sub 200} at fixed halo mass is not large. The luminosity intercept is 30%, or 2{sigma}, lower than determined from the X-ray flux-limited sample of Reiprich & Boehringer (2002), assuming hydrostatic equilibrium. This slight difference could arise from a combination of Malmquist bias and/or systematic error in hydrostatic mass estimates, both of which are expected. The intercept agrees with that derived by Stanek et al. (2006) using a model for the statistical correspondence between clusters and halos in a WMAP3 cosmology with power spectrum normalization {sigma}{sub 8} = 0.85. Similar exercises applied to future data sets will allow constraints on the covariance among optical and hot gas properties of clusters at fixed mass.

  9. Measurement of the Top Quark Mass Simultaneously in Dilepton and Lepton + Jets Decay Channels

    SciTech Connect (OSTI)

    Fedorko, Wojciech T.; /Chicago U.

    2008-09-01

    The authors present the first measurement of the top quark mass using simultaneously data from two decay channels. They use a data sample of {radical}s = 1.96 TeV collisions with integrated luminosity of 1.9 fb{sup -1} collected by the CDF II detector. They select dilepton and lepton + jets channel decays of t{bar t} pairs and reconstruct two observables in each topology. They use non-parametric techniques to derive probability density functions from simulated signal and background samples. The observables are the reconstructed top quark mass and the scalar sum of transverse energy of the event in the dilepton topology and the reconstructed top quark mass and the invariant mass of jets from the W boson decay in lepton + jets channel. They perform a simultaneous fit for the top quark mass and the jet energy scale which is constrained in situ by the hadronic W boson resonance from the lepton + jets channel. Using 144 dilepton candidate events and 332 lepton + jets candidate events they measure: M{sub top} = 171.9 {+-} 1.7 (stat. + JES) {+-} 1.1 (other sys.) GeV/c{sup 2} = 171.9 {+-} 2.0 GeV/c{sup 2}. The measurement features a robust treatment of the systematic uncertainties, correlated between the two channels and develops techniques for a future top quark mass measurement simultaneously in all decay channels. Measurements of the W boson mass and the top quark mass provide a constraint on the mass of the yet unobserved Higgs boson. The Higgs boson mass implied by measurement presented here is higher than Higgs boson mass implied by previously published, most precise CDF measurements of the top quark mass in lepton + jets and dilepton channels separately.

  10. CloudSat as a Global Radar Calibrator

    SciTech Connect (OSTI)

    Protat, Alain; Bouniol, Dominique; O'Connor, E. J.; Baltink, Henk K.; Verlinde, J.; Widener, Kevin B.

    2011-03-01

    The calibration of the CloudSat spaceborne cloud radar has been thoroughly assessed using very accurate internal link budgets before launch, comparisons with predicted ocean surface backscatter at 94 GHz, direct comparisons with airborne cloud radars, and statistical comparisons with ground-based cloud radars at different locations of the world. It is believed that the calibration of CloudSat is accurate to within 0.5 to 1 dB. In the present paper it is shown that an approach similar to that used for the statistical comparisons with ground-based radars can now be adopted the other way around to calibrate other ground-based or airborne radars against CloudSat and / or detect anomalies in long time series of ground-based radar measurements, provided that the calibration of CloudSat is followed up closely (which is the case). The power of using CloudSat as a Global Radar Calibrator is demonstrated using the Atmospheric Radiation Measurement cloud radar data taken at Barrow, Alaska, the cloud radar data from the Cabauw site, The Netherlands, and airborne Doppler cloud radar measurements taken along the CloudSat track in the Arctic by the RASTA (Radar SysTem Airborne) cloud radar installed in the French ATR-42 aircraft for the first time. It is found that the Barrow radar data in 2008 are calibrated too high by 9.8 dB, while the Cabauw radar data in 2008 are calibrated too low by 8.0 dB. The calibration of the RASTA airborne cloud radar using direct comparisons with CloudSat agrees well with the expected gains and losses due to the change in configuration which required verification of the RASTA calibration.

  11. Impact of spurious shear on cosmological parameter estimates from weak lensing observables

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Petri, Andrea; May, Morgan; Haiman, Zoltán; Kratochvil, Jan M.

    2014-12-30

    We research, residual errors in shear measurements, after corrections for instrument systematics and atmospheric effects, can impact cosmological parameters derived from weak lensing observations. Here we combine convergence maps from our suite of ray-tracing simulations with random realizations of spurious shear. This allows us to quantify the errors and biases of the triplet (Ωm,w,σ8) derived from the power spectrum (PS), as well as from three different sets of non-Gaussian statistics of the lensing convergence field: Minkowski functionals (MFs), low-order moments (LMs), and peak counts (PKs). Our main results are as follows: (i) We find an order of magnitude smaller biasesmore » from the PS than in previous work. (ii) The PS and LM yield biases much smaller than the morphological statistics (MF, PK). (iii) For strictly Gaussian spurious shear with integrated amplitude as low as its current estimate of σsys2 ≈ 10-7, biases from the PS and LM would be unimportant even for a survey with the statistical power of Large Synoptic Survey Telescope. However, we find that for surveys larger than ≈ 100 deg2, non-Gaussianity in the noise (not included in our analysis) will likely be important and must be quantified to assess the biases. (iv) The morphological statistics (MF, PK) introduce important biases even for Gaussian noise, which must be corrected in large surveys. The biases are in different directions in (Ωm,w,σ8) parameter space, allowing self-calibration by combining multiple statistics. Our results warrant follow-up studies with more extensive lensing simulations and more accurate spurious shear estimates.« less

  12. Impact of spurious shear on cosmological parameter estimates from weak lensing observables

    SciTech Connect (OSTI)

    Petri, Andrea; May, Morgan; Haiman, Zoltn; Kratochvil, Jan M.

    2014-12-30

    We research, residual errors in shear measurements, after corrections for instrument systematics and atmospheric effects, can impact cosmological parameters derived from weak lensing observations. Here we combine convergence maps from our suite of ray-tracing simulations with random realizations of spurious shear. This allows us to quantify the errors and biases of the triplet (?m,w,?8) derived from the power spectrum (PS), as well as from three different sets of non-Gaussian statistics of the lensing convergence field: Minkowski functionals (MFs), low-order moments (LMs), and peak counts (PKs). Our main results are as follows: (i) We find an order of magnitude smaller biases from the PS than in previous work. (ii) The PS and LM yield biases much smaller than the morphological statistics (MF, PK). (iii) For strictly Gaussian spurious shear with integrated amplitude as low as its current estimate of ?sys2 ? 10-7, biases from the PS and LM would be unimportant even for a survey with the statistical power of Large Synoptic Survey Telescope. However, we find that for surveys larger than ? 100 deg2, non-Gaussianity in the noise (not included in our analysis) will likely be important and must be quantified to assess the biases. (iv) The morphological statistics (MF, PK) introduce important biases even for Gaussian noise, which must be corrected in large surveys. The biases are in different directions in (?m,w,?8) parameter space, allowing self-calibration by combining multiple statistics. Our results warrant follow-up studies with more extensive lensing simulations and more accurate spurious shear estimates.

  13. Study of B??Xul?? decays in BB? events tagged by a fully reconstructed B-meson decay and determination of |Vub|

    SciTech Connect (OSTI)

    Lees, J. P.; Poireau, V.; Tisserand, V.; Garra Tico, J.; Grauges, E.; Martinelli, M.; Milanes, D. A.; Palano, A.; Pappagallo, M.; Eigen, G.; Stugu, B.; Brown, D. N.; Kerth, L. T.; Kolomensky, Yu. G.; Lynch, G.; Tackmann, K.; Koch, H.; Schroeder, T.; Asgeirsson, D. J.; Hearty, C.; Mattison, T. S.; McKenna, J. A.; Khan, A.; Blinov, V. E.; Buzykaev, A. R.; Druzhinin, V. P.; Golubev, V. B.; Kravchenko, E. A.; Onuchin, A. P.; Serednyakov, S. I.; Skovpen, Yu. I.; Solodov, E. P.; Todyshev, K. Yu.; Yushkov, A. N.; Bondioli, M.; Kirkby, D.; Lankford, A. J.; Mandelkern, M.; Stoker, D. P.; Atmacan, H.; Gary, J. W.; Liu, F.; Long, O.; Vitug, G. M.; Campagnari, C.; Hong, T. M.; Kovalskyi, D.; Richman, J. D.; West, C. A.; Eisner, A. M.; Kroseberg, J.; Lockman, W. S.; Martinez, A. J.; Schalk, T.; Schumm, B. A.; Seiden, A.; Cheng, C. H.; Doll, D. A.; Echenard, B.; Flood, K. T.; Hitlin, D. G.; Ongmongkolkul, P.; Porter, F. C.; Rakitin, A. Y.; Andreassen, R.; Dubrovin, M. S.; Huard, Z.; Meadows, B. T.; Sokoloff, M. D.; Sun, L.; Bloom, P. C.; Ford, W. T.; Gaz, A.; Nagel, M.; Nauenberg, U.; Smith, J. G.; Wagner, S. R.; Ayad, R.; Toki, W. H.; Spaan, B.; Kobel, M. J.; Schubert, K. R.; Schwierz, R.; Bernard, D.; Verderi, M.; Clark, P. J.; Playfer, S.; Bettoni, D.; Bozzi, C.; Calabrese, R.; Cibinetto, G.; Fioravanti, E.; Garzia, I.; Luppi, E.; Munerato, M.; Negrini, M.; Petrella, A.; Piemontese, L.; Santoro, V.; Baldini-Ferroli, R.; Calcaterra, A.; de Sangro, R.; Finocchiaro, G.; Nicolaci, M.; Patteri, P.; Peruzzi, I. M.; Piccolo, M.; Rama, M.; Zallo, A.; Contri, R.; Guido, E.; Lo Vetere, M.; Monge, M. R.; Passaggio, S.; Patrignani, C.; Robutti, E.; Bhuyan, B.; Prasad, V.; Lee, C. L.; Morii, M.; Edwards, A. J.; Adametz, A.; Marks, J.; Uwer, U.; Bernlochner, F. U.; Ebert, M.; Lacker, H. M.; Lueck, T.; Dauncey, P. D.; Tibbetts, M.; Behera, P. K.; Mallik, U.; Chen, C.; Cochran, J.; Meyer, W. T.; Prell, S.; Rosenberg, E. I.; Rubin, A. E.; Gritsan, A. V.; Guo, Z. J.; Arnaud, N.; Davier, M.; Grosdidier, G.; Le Diberder, F.; Lutz, A. M.; Malaescu, B.; Roudeau, P.; Schune, M. H.; Stocchi, A.; Wormser, G.; Lange, D. J.; Wright, D. M.; Bingham, I.; Chavez, C. A.; Coleman, J. P.; Fry, J. R.; Gabathuler, E.; Hutchcroft, D. E.; Payne, D. J.; Touramanis, C.; Bevan, A. J.; Di Lodovico, F.; Sacco, R.; Sigamani, M.; Cowan, G.; Brown, D. N.; Davis, C. L.; Denig, A. G.; Fritsch, M.; Gradl, W.; Hafner, A.; Prencipe, E.; Alwyn, K. E.; Bailey, D.; Barlow, R. J.; Jackson, G.; Lafferty, G. D.; Cenci, R.; Hamilton, B.; Jawahery, A.; Roberts, D. A.; Simi, G.; Dallapiccola, C.; Cowan, R.; Dujmic, D.; Sciolla, G.; Lindemann, D.; Patel, P. M.; Robertson, S. H.; Schram, M.; Biassoni, P.; Lazzaro, A.; Lombardo, V.; Neri, N.; Palombo, F.; Stracka, S.; Cremaldi, L.; Godang, R.; Kroeger, R.; Sonnek, P.; Summers, D. J.; Nguyen, X.; Taras, P.; De Nardo, G.; Monorchio, D.; Onorato, G.; Sciacca, C.; Raven, G.; Snoek, H. L.; Jessop, C. P.; Knoepfel, K. J.; LoSecco, J. M.; Wang, W. F.; Honscheid, K.; Kass, R.; Brau, J.; Frey, R.; Sinev, N. B.; Strom, D.; Torrence, E.; Feltresi, E.; Gagliardi, N.; Margoni, M.; Morandin, M.; Posocco, M.; Rotondo, M.; Simonetto, F.; Stroili, R.; Ben-Haim, E.; Bomben, M.; Bonneaud, G. R.; Briand, H.; Calderini, G.; Chauveau, J.; Hamon, O.; Leruste, Ph.; Marchiori, G.; Ocariz, J.; Sitt, S.; Biasini, M.; Manoni, E.; Pacetti, S.; Rossi, A.; Angelini, C.; Batignani, G.; Bettarini, S.; Carpinelli, M.; Casarosa, G.; Cervelli, A.; Forti, F.; Giorgi, M. A.; Lusiani, A.; Oberhof, B.; Paoloni, E.; Perez, A.; Rizzo, G.; Walsh, J. J.; Lopes Pegna, D.; Lu, C.; Olsen, J.; Smith, A. J. S.; Telnov, A. V.; Anulli, F.; Cavoto, G.; Faccini, R.; Ferrarotto, F.; Ferroni, F.; Gaspero, M.; Li Gioi, L.; Mazzoni, M. A.; Piredda, G.; Bnger, C.; Grnberg, O.; Hartmann, T.; Leddig, T.; Schrder, H.; Waldi, R.; Adye, T.; Olaiya, E. O.; Wilson, F. F.; Emery, S.; Hamel de Monchenault, G.; Vasseur, G.; Yche, Ch.; Aston, D.; Bard, D. J.; Bartoldus, R.; Cartaro, C.; Convery, M. R.; Dorfan, J.; Dubois-Felsmann, G. P.; Dunwoodie, W.; Field, R. C.; Franco Sevilla, M.; Fulsom, B. G.; Gabareen, A. M.; Graham, M. T.; Grenier, P.; Hast, C.; Innes, W. R.; Kelsey, M. H.; Kim, H.; Kim, P.; Kocian, M. L.; Leith, D. W. G. S.; Lewis, P.; Li, S.; Lindquist, B.; Luitz, S.; Luth, V.; Lynch, H. L.; MacFarlane, D. B.; Muller, D. R.; Neal, H.; Nelson, S.; Ofte, I.; Perl, M.; Pulliam, T.; Ratcliff, B. N.; Roodman, A.; Salnikov, A. A.; Schindler, R. H.; Snyder, A.; Su, D.; Sullivan, M. K.; Vavra, J.; Wagner, A. P.; Weaver, M.; Wisniewski, W. J.; Wittgen, M.; Wright, D. H.; Wulsin, H. W.; Yarritu, A. K.; Young, C. C.; Ziegler, V.; Park, W.; Purohit, M. V.; White, R. M.; Wilson, J. R.; Randle-Conde, A.; Sekula, S. J.; Bellis, M.; Benitez, J. F.; Burchat, P. R.

    2012-08-07

    We report measurements of partial branching fractions for inclusive charmless semileptonic B decays B?Xul? and the determination of the CabibboKobayashiMaskawa (CKM) matrix element |Vub|. The analysis is based on a sample of 46710? ?(4S)?BB decays recorded with the BABAR detector at the PEP-II e?e? storage rings. We select events in which the decay of one of the B mesons is fully reconstructed and an electron or a muon signals the semileptonic decay of the other B meson. We measure partial branching fractions ?B in several restricted regions of phase space and determine the CKM element |Vub| based on different QCD predictions. For decays with a charged lepton momentum p*l>1.0 GeV in the B meson rest frame, we obtain ?B=(1.800.13stat0.15sys0.02theo)10? from a fit to the two-dimensional MX-q distribution. Here, MX refers to the invariant mass of the final state hadron X and q is the invariant mass squared of the charged lepton and neutrino. From this measurement we extract |Vub|=(4.330.24exp?0.15theo)10? as the arithmetic average of four results obtained from four different QCD predictions of the partial rate. We separately determine partial branching fractions for B0 and B? decays and derive a limit on the isospin breaking in B?Xul? decays.

  14. Impact of spurious shear on cosmological parameter estimates from weak lensing observables

    SciTech Connect (OSTI)

    Petri, Andrea; May, Morgan; Haiman, Zoltán; Kratochvil, Jan M.

    2014-12-30

    We research, residual errors in shear measurements, after corrections for instrument systematics and atmospheric effects, can impact cosmological parameters derived from weak lensing observations. Here we combine convergence maps from our suite of ray-tracing simulations with random realizations of spurious shear. This allows us to quantify the errors and biases of the triplet (Ωm,w,σ8) derived from the power spectrum (PS), as well as from three different sets of non-Gaussian statistics of the lensing convergence field: Minkowski functionals (MFs), low-order moments (LMs), and peak counts (PKs). Our main results are as follows: (i) We find an order of magnitude smaller biases from the PS than in previous work. (ii) The PS and LM yield biases much smaller than the morphological statistics (MF, PK). (iii) For strictly Gaussian spurious shear with integrated amplitude as low as its current estimate of σsys2 ≈ 10-7, biases from the PS and LM would be unimportant even for a survey with the statistical power of Large Synoptic Survey Telescope. However, we find that for surveys larger than ≈ 100 deg2, non-Gaussianity in the noise (not included in our analysis) will likely be important and must be quantified to assess the biases. (iv) The morphological statistics (MF, PK) introduce important biases even for Gaussian noise, which must be corrected in large surveys. The biases are in different directions in (Ωm,w,σ8) parameter space, allowing self-calibration by combining multiple statistics. Our results warrant follow-up studies with more extensive lensing simulations and more accurate spurious shear estimates.

  15. A chemical confirmation of the faint Boötes II dwarf spheroidal galaxy

    SciTech Connect (OSTI)

    Koch, Andreas; Rich, R. Michael

    2014-10-10

    We present a chemical abundance study of the brightest confirmed member star of the ultra-faint dwarf galaxy Boötes II from Keck/HIRES high-resolution spectroscopy at moderate signal-to-noise ratios. At [Fe/H] = –2.93 ± 0.03(stat.) ± 0.17(sys.), this star chemically resembles metal-poor halo field stars and the signatures of other faint dwarf spheroidal galaxies at the same metallicities in that it shows enhanced [α/Fe] ratios, Solar Fe-peak element abundances, and low upper limits on the neutron-capture element Ba. Moreover, this star shows no chemical peculiarities in any of the eight elements we were able to measure. This implies that the chemical outliers found in other systems remain outliers pertaining to the unusual enrichment histories of the respective environments, while Boo II appears to have experienced an enrichment history typical of its very low mass. We also re-calibrated previous measurements of the galaxy's metallicity from the calcium triplet (CaT) and find a much lower value than reported before. The resulting broad metallicity spread, in excess of one dex, the very metal-poor mean, and the chemical abundance patterns of the present star imply that Boötes II is a low-mass, old, metal-poor dwarf galaxy and not an overdensity associated with the Sagittarius Stream as has been previously suggested based on its sky position and kinematics. The low, mean CaT metallicity of –2.7 dex falls right on the luminosity-metallicity relation delineated over four orders of magnitude from the more luminous to the faintest galaxies. Thus Boötes II's chemical enrichment appears representative of the galaxy's original mass, while tidal stripping and other mass loss mechanisms were probably not significant as for other low-mass satellites.

  16. A Measurement of the t anti-t Cross Section in p anti-p Collisions at s**(1/2) = 1.96-TeV using Dilepton Events with a Lepton plus Track Selection

    SciTech Connect (OSTI)

    Aaltonen, T.; Adelman, Jahred A.; Akimoto, T.; Alvarez Gonzalez, B.; Amerio, S.; Amidei, Dante E.; Anastassov, A.; Annovi, Alberto; Antos, Jaroslav; Apollinari, G.; Apresyan, A.; /Purdue U. /Waseda U.

    2009-03-01

    This paper reports a measurement of the cross section for the pair production of top quarks in p{bar p} collisions at {radical}s = 1.96 TeV at the Fermilab Tevatron. The data was collected from the CDF II detector in a set of runs with a total integrated luminosity of 1.1 fb{sup -1}. The cross section is measured in the dilepton channel, the subset of t{bar t} events in which both top quarks decay through t {yields} Wb {yields} {ell}{nu}b, where {ell} = e, {mu}, or {tau}. The lepton pair is reconstructed as one identified electron or muon and one isolated track. The use of an isolated track to identify the second lepton increases the t{bar t} acceptance, particularly for the case in which one W decays as W {yields} {tau}{nu}. The purity of the sample may be further improved at the cost of a reduction in the number of signal events, by requiring an identified b-jet. They present the results of measurements performed with and without the request of an identified b-jet. the former is the first published CDF result for which a b-jet requirement is added to the dilepton selection. In the CDF data there are 129 pretag lepton + track candidate events, of which 69 are tagged. With the tagging information, the sample is divided into tagged and untagged sub-samples, and a combined cross section is calculated by maximizing a likelihood. The result is {sigma}{sub t{bar t}} = 9.6 {+-} 1.2(stat.){sub -0.5}{sup +0.6}(sys.) {+-} 0.6(lum.) pb, assuming a branching ratio of BR(W {yields} {ell}{nu}) = 10.8% and a top mass of m{sub t} = 175 GeV/c{sup 2}.

  17. HST-COS SPECTROSCOPY OF THE COOLING FLOW IN A1795EVIDENCE FOR INEFFICIENT STAR FORMATION IN CONDENSING INTRACLUSTER GAS

    SciTech Connect (OSTI)

    McDonald, Michael; Ehlert, Steven; Roediger, Joel; Veilleux, Sylvain

    2014-08-20

    We present far-UV spectroscopy from the Cosmic Origins Spectrograph on the Hubble Space Telescope of a cool, star-forming filament in the core of A1795. These data, which span 1025 < ?{sub rest} < 1700, allow for the simultaneous modeling of the young stellar populations and the intermediate-temperature (10{sup 5.5}K) gas in this filament, which is far removed (?30kpc) from the direct influence of the central active galactic nucleus. Using a combination of UV absorption line indices and stellar population synthesis modeling, we find evidence for ongoing star formation, with the youngest stars having ages of 7.5{sub ?2.0}{sup +2.5}Myr and metallicities of 0.4{sub ?0.1}{sup +0.2} Z {sub ?}. The latter is consistent with the local metallicity of the intracluster medium. We detect the O VI?1038 line, measuring a flux of f {sub O} {sub VI,} {sub 1038} = 4.0 0.9 10{sup 17} erg s{sup 1} cm{sup 2}. The O VI?1032 line is redshifted such that it is coincident with a strong Galactic H{sub 2} absorption feature, and is not detected. The measured O VI?1038 flux corresponds to a cooling rate of 0.85 0.2 (stat) 0.15 (sys) M {sub ?} yr{sup 1} at ?10{sup 5.5}K, assuming that the cooling proceeds isochorically, which is consistent with the classical X-ray luminosity-derived cooling rate in the same region. We measure a star formation rate of 0.11 0.02 M {sub ?} yr{sup 1} from the UV continuum, suggesting that star formation is proceeding at 13{sub ?2}{sup +3}% efficiency in this filament. We propose that this inefficient star formation represents a significant contribution to the larger-scale cooling flow problem.

  18. Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters

    SciTech Connect (OSTI)

    Chiu, I.

    2015-10-06

    We present a detection of the enhancement in the number densities of background galaxies induced from lensing magnification and use it to test the Sunyaev-Zel'dovich effect (SZE) inferred masses in a sample of 19 galaxy clusters with median redshift z?0.42 selected from the South Pole Telescope SPT-SZ survey. Two background galaxy populations are selected for this study through their photometric colours; they have median redshifts zmedian?0.9 (low-z background) and zmedian?1.8 (high-z background). Stacking these populations, we detect the magnification bias effect at 3.3? and 1.3? for the low- and high-z backgrounds, respectively. We fit NFW models simultaneously to all observed magnification bias profiles to estimate the multiplicative factor ? that describes the ratio of the weak lensing mass to the mass inferred from the SZE observable-mass relation. We further quantify systematic uncertainties in ? resulting from the photometric noise and bias, the cluster galaxy contamination and the estimations of the background properties. The resulting ? for the combined background populations with 1? uncertainties is 0.830.24(stat)0.074(sys), indicating good consistency between the lensing and the SZE-inferred masses. We also use our best-fit ? to predict the weak lensing shear profiles and compare these predictions with observations, showing agreement between the magnification and shear mass constraints. Our work demonstrates the promise of using the magnification as a complementary method to estimate cluster masses in large surveys.

  19. WE-F-16A-01: Commissioning and Clinical Use of PC-ISO for Customized, 3D Printed, Gynecological Brachytherapy Applicators

    SciTech Connect (OSTI)

    Cunha, J; Sethi, R; Mellis, K; Siauw, T; Sudhyadhom, A; Hsu, I; Pouliot, J

    2014-06-15

    Purpose: (1) Evaluate the safety and radiation attenuation properties of PCISO, a bio-compatible, sterilizable 3D printing material by Stratasys, (2) establish a method for commissioning customized multi- and single-use 3D printed applicators, (3) report on use of customized vaginal cylinders used to treat a series of serous endometrial cancer patient. Methods: A custom film dosimetry apparatus was designed to hold a Gafchromic radio film segment between two blocks of PC-ISO and 3D-printed using a Fortus 400mc (StrataSys). A dose plan was computed using 13 dwell positions at 2.5 mm spacing and normalized to 1500 cGy at 1 cm. Film exposure was compared to control tests in only air and only water. The average Hounsfield Unit (HU) was computed and used to verify water equivalency. For the clinical use cases, the physician specifies the dimensions and geometry of a custom applicator from which a CAD model is designed and printed. Results: The doses measured from the PC-ISO Gafchromic film test were within 1% of the dose measured in only water between 1cm and 6cm from the channel. Doses increased 74% measured in only air. HU range was 1143. The applicators were sterilized using the Sterrad system multiple times without damage. As of submission 3 unique cylinders have been designed, printed, and used in the clinic. A standardizable workflow for commissioning custom 3D printed applicators was codified and will be reported. Conclusions: Quality assurance (QA) evaluation of the PC-ISO 3D-printing material showed that PC-ISO is a suitable material for a gynecological brachytherapy vaginal cylinder in a clinical setting. With the material commissioning completed, if the physician determines that a better treatment would Result, a customized design is fabricated with limited additional QA necessary. Although this study was specific to PC-ISO, the same setup can be used to evaluate other 3D-printing materials.

  20. Measurement of the Oscillation Frequency of B_s Mesons in the Hadronic Decay Mode B_s-> pi D_s(phi pi)X$ with the D0 Detector at the Fermilab Tevatron Collider

    SciTech Connect (OSTI)

    Weber, Gernot August; /Mainz U., Inst. Phys.

    2009-03-01

    The standard model (SM) of particle physics is a theory, describing three out of four fundamental forces. In this model the Cabibbo-Kobayashi-Maskawa (CKM) matrix describes the transformation between the mass and weak eigenstates of quarks. The matrix properties can be visualized as triangles in the complex plane. A precise measurement of all triangle parameters can be used to verify the validity of the SM. The least precisely measured parameter of the triangle is related to the CKM element |V{sub td}|, accessible through the mixing frequency (oscillation) of neutral B mesons, where mixing is the transition of a neutral meson into its anti-particle and vice versa. It is possible to calculate the CKM element |V{sub td}| and a related element |V{sub ts}| by measuring the mass differences {Delta}m{sub d} ({Delta}m{sub s}) between neutral B{sub d} and {bar B}{sub d} (B{sub s} and {bar B}{sub s}) meson mass eigenstates. This measurement is accomplished by tagging the initial and final state of decaying B mesons and determining their lifetime. Currently the Fermilab Tevatron Collider (providing p{bar p} collisions at {radical}s = 1.96 TeV) is the only place, where B{sub s} oscillations can be studied. The first selection of the 'golden', fully hadronic decay mode B{sub s} {yields} {pi}D{sub s}({phi}{pi})X at D0 is presented in this thesis. All data, taken between April 2002 and August 2007 with the D0 detector, corresponding to an integrated luminosity of {integral} Ldt = 2.8 fb{sup -1} is used. The oscillation frequency {Delta}m{sub s} and the ratio |V{sub td}|/|V{sub ts}| are determined as {Delta}m{sub s} = (16.6{sub -0.4}{sup +0.5}(stat){sub -0.3}{sup +0.4}(sys)) ps{sup -1}, |V{sub td}|/|V{sub ts}| = 0.213{sub -0.003}{sup +0.004}(exp) {+-} 0.008(theor). These results are consistent with the standard model expectations and no evidence for new physics is observable.

  1. FEMTOSECOND TIMING DISTRIBUTION AND CONTROL FOR NEXT GENERATION ACCELERATORS AND LIGHT SOURCES

    SciTech Connect (OSTI)

    Chen, Li-Jin

    2014-03-31

    Femtosecond Timing Distribution At LCLS Free-electron-lasers (FEL) have the capability of producing high photon flux from the IR to the hard x-ray wavelength range and to emit femtosecond and eventually even at-tosecond pulses. This makes them an ideal tool for fundamental as well as applied re-search. Timing precision at the Stanford Linear Coherent Light Source (LCLS) between the x-ray FEL (XFEL) and ultrafast optical lasers is currently no better than 100 fs RMS. Ideally this precision should be much better and could be limited only by the x-ray pulse duration, which can be as short as a few femtoseconds. An increasing variety of science problems involving electron and nuclear dynamics in chemical and material systems will become accessible as the timing improves to a few femtoseconds. Advanced methods of electron beam conditioning or pulse injection could allow the FEL to achieve pulse durations less than one femtosecond. The objec-tive of the work described in this proposal is to set up an optical timing distribution sys-tem based on modelocked Erbium doped fiber lasers at LCLS facility to improve the timing precision in the facility and allow time stamping with a 10 fs precision. The primary commercial applications for optical timing distributions systems are seen in the worldwide accelerator facilities and next generation light sources community. It is reasonable to expect that at least three major XFELs will be built in the next decade. In addition there will be up to 10 smaller machines, such as FERMI in Italy and Maxlab in Sweden, plus the market for upgrading already existing facilities like Jefferson Lab. The total market is estimated to be on the order of a 100 Million US Dollars. The company owns the exclusive rights to the IP covering the technology enabling sub-10 fs synchronization systems. Testing this technology, which has set records in a lab environment, at LCLS, hence in a real world scenario, is an important corner stone of bringing the technology to market.

  2. Cosmological constraints from measurements of type Ia supernovae discovered during the first 1.5 yr of the Pan-STARRS1 survey

    SciTech Connect (OSTI)

    Rest, A. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Scolnic, D.; Riess, A.; Rodney, S.; Brout, D. [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Foley, R. J.; Chornock, R.; Berger, E.; Soderberg, A. M.; Stubbs, C. W.; Kirshner, R. P.; Challis, P.; Czekala, I.; Drout, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Huber, M. E.; Tonry, J. L. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Narayan, G. [Department of Physics, Harvard University, 17 Oxford Street, Cambridge, MA 02138 (United States); Smartt, S. J. [Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast, Belfast BT71NN (United Kingdom); Schlafly, E. [Max Planck Institute for Astronomy, Knigstuhl 17, D-69117 Heidelberg (Germany); Botticella, M. T. [INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Napoli (Italy); and others

    2014-11-01

    We present griz {sub P1} light curves of 146 spectroscopically confirmed Type Ia supernovae (SNe Ia; 0.03 < z < 0.65) discovered during the first 1.5 yr of the Pan-STARRS1 Medium Deep Survey. The Pan-STARRS1 natural photometric system is determined by a combination of on-site measurements of the instrument response function and observations of spectrophotometric standard stars. We find that the systematic uncertainties in the photometric system are currently 1.2% without accounting for the uncertainty in the Hubble Space Telescope Calspec definition of the AB system. A Hubble diagram is constructed with a subset of 113 out of 146 SNe Ia that pass our light curve quality cuts. The cosmological fit to 310 SNe Ia (113 PS1 SNe Ia + 222 light curves from 197 low-z SNe Ia), using only supernovae (SNe) and assuming a constant dark energy equation of state and flatness, yields w=?1.120{sub ?0.206}{sup +0.360}(Stat){sub ?0.291}{sup +0.269}(Sys). When combined with BAO+CMB(Planck)+H {sub 0}, the analysis yields ?{sub M}=0.280{sub ?0.012}{sup +0.013} and w=?1.166{sub ?0.069}{sup +0.072} including all identified systematics. The value of w is inconsistent with the cosmological constant value of 1 at the 2.3? level. Tension endures after removing either the baryon acoustic oscillation (BAO) or the H {sub 0} constraint, though it is strongest when including the H {sub 0} constraint. If we include WMAP9 cosmic microwave background (CMB) constraints instead of those from Planck, we find w=?1.124{sub ?0.065}{sup +0.083}, which diminishes the discord to <2?. We cannot conclude whether the tension with flat ?CDM is a feature of dark energy, new physics, or a combination of chance and systematic errors. The full Pan-STARRS1 SN sample with ?three times as many SNe should provide more conclusive results.

  3. Measurements of dielectron production in Au + Au collisions at sNN=200 GeV from the STAR experiment

    SciTech Connect (OSTI)

    Adamczyk, L.; Adkins, J. K.; Agakishiev, G.; Aggarwal, M. M.; Ahammed, Z.; Alekseev, I.; Alford, J.; Aparin, A.; Arkhipkin, D.; Aschenauer, E. C.; Averichev, G. S.; Banerjee, A.; Bellwied, R.; Bhasin, A.; Bhati, A. K.; Bhattarai, P.; Bielcik, J.; Bielcikova, J.; Bland, L. C.; Bordyuzhin, I. G.; Bouchet, J.; Brandin, A. V.; Bunzarov, I.; Burton, T. P.; Butterworth, J.; Caines, H.; Calderón de la Barca Sánchez, M.; Campbell, J. M.; Cebra, D.; Cervantes, M. C.; Chakaberia, I.; Chaloupka, P.; Chang, Z.; Chattopadhyay, S.; Chen, J. H.; Chen, X.; Cheng, J.; Cherney, M.; Christie, W.; Contin, G.; Crawford, H. J.; Das, S.; De Silva, L. C.; Debbe, R. R.; Dedovich, T. G.; Deng, J.; Derevschikov, A. A.; di Ruzza, B.; Didenko, L.; Dilks, C.; Dong, X.; Drachenberg, J. L.; Draper, J. E.; Du, C. M.; Dunkelberger, L. E.; Dunlop, J. C.; Efimov, L. G.; Engelage, J.; Eppley, G.; Esha, R.; Evdokimov, O.; Eyser, O.; Fatemi, R.; Fazio, S.; Federic, P.; Fedorisin, J.; Feng, Z.; Filip, P.; Fisyak, Y.; Flores, C. E.; Fulek, L.; Gagliardi, C. A.; Garand, D.; Geurts, F.; Gibson, A.; Girard, M.; Greiner, L.; Grosnick, D.; Gunarathne, D. S.; Guo, Y.; Gupta, S.; Gupta, A.; Guryn, W.; Hamad, A.; Hamed, A.; Haque, R.; Harris, J. W.; He, L.; Heppelmann, S.; Heppelmann, S.; Hirsch, A.; Hoffmann, G. W.; Hofman, D. J.; Horvat, S.; Huang, B.; Huang, X.; Huang, H. Z.; Huck, P.; Humanic, T. J.; Igo, G.; Jacobs, W. W.; Jang, H.; Jiang, K.; Judd, E. G.; Jung, K.; Kabana, S.; Kalinkin, D.; Kang, K.; Kauder, K.; Ke, H. W.; Keane, D.; Kechechyan, A.; Khan, Z. H.; Kikola, D. P.; Kisel, I.; Kisiel, A.; Kochenda, L.; Koetke, D. D.; Kollegger, T.; Kosarzewski, L. K.; Kraishan, A. F.; Kravtsov, P.; Krueger, K.; Kulakov, I.; Kumar, L.; Kycia, R. A.; Lamont, M. A. C.; Landgraf, J. M.; Landry, K. D.; Lauret, J.; Lebedev, A.; Lednicky, R.; Lee, J. H.; Li, X.; Li, C.; Li, W.; Li, Z. M.; Li, Y.; Li, X.; Lisa, M. A.; Liu, F.; Ljubicic, T.; Llope, W. J.; Lomnitz, M.; Longacre, R. S.; Luo, X.; Ma, Y. G.; Ma, G. L.; Ma, L.; Ma, R.; Magdy, N.; Majka, R.; Manion, A.; Margetis, S.; Markert, C.; Masui, H.; Matis, H. S.; McDonald, D.; Meehan, K.; Minaev, N. G.; Mioduszewski, S.; Mohanty, B.; Mondal, M. M.; Morozov, D.; Mustafa, M. K.; Nandi, B. K.; Nasim, Md.; Nayak, T. K.; Nigmatkulov, G.; Nogach, L. V.; Noh, S. Y.; Novak, J.; Nurushev, S. B.; Odyniec, G.; Ogawa, A.; Oh, K.; Okorokov, V.; Olvitt, D.; Page, B. S.; Pak, R.; Pan, Y. X.; Pandit, Y.; Panebratsev, Y.; Pawlik, B.; Pei, H.; Perkins, C.; Peterson, A.; Pile, P.; Planinic, M.; Pluta, J.; Poljak, N.; Poniatowska, K.; Porter, J.; Posik, M.; Poskanzer, A. M.; Pruthi, N. K.; Putschke, J.; Qiu, H.; Quintero, A.; Ramachandran, S.; Raniwala, R.; Raniwala, S.; Ray, R. L.; Ritter, H. G.; Roberts, J. B.; Rogachevskiy, O. V.; Romero, J. L.; Roy, A.; Ruan, L.; Rusnak, J.; Rusnakova, O.; Sahoo, N. R.; Sahu, P. K.; Sakrejda, I.; Salur, S.; Sandweiss, J.; Sarkar, A.; Schambach, J.; Scharenberg, R. P.; Schmah, A. M.; Schmidke, W. B.; Schmitz, N.; Seger, J.; Seyboth, P.; Shah, N.; Shahaliev, E.; Shanmuganathan, P. V.; Shao, M.; Sharma, M. K.; Sharma, B.; Shen, W. Q.; Shi, S. S.; Shou, Q. Y.; Sichtermann, E. P.; Sikora, R.; Simko, M.; Skoby, M. J.; Smirnov, D.; Smirnov, N.; Song, L.; Sorensen, P.; Spinka, H. M.; Srivastava, B.; Stanislaus, T. D. S.; Stepanov, M.; Stock, R.; Strikhanov, M.; Stringfellow, B.; Sumbera, M.; Summa, B.; Sun, X.; Sun, Z.; Sun, X. M.; Sun, Y.; Surrow, B.; Svirida, N.; Szelezniak, M. A.; Tang, A. H.; Tang, Z.; Tarnowsky, T.; Tawfik, A. N.; Thomas, J. H.; Timmins, A. R.; Tlusty, D.; Tokarev, M.; Trentalange, S.; Tribble, R. E.; Tribedy, P.; Tripathy, S. K.; Trzeciak, B. A.; Tsai, O. D.; Ullrich, T.; Underwood, D. G.; Upsal, I.; Van Buren, G.; van Nieuwenhuizen, G.; Vandenbroucke, M.; Varma, R.; Vasiliev, A. N.; Vertesi, R.; Videbæk, F.; Viyogi, Y. P.; Vokal, S.; Voloshin, S. A.; Vossen, A.; Wang, G.; Wang, Y.; Wang, F.; Wang, Y.; Wang, H.; Wang, J. S.; Webb, J. C.; Webb, G.; Wen, L.; Westfall, G. D.; Wieman, H.; Wissink, S. W.; Witt, R.; Wu, Y. F.; Xiao, Z. G.; Xie, W.; Xin, K.; Xu, Q. H.; Xu, Z.; Xu, H.; Xu, N.; Xu, Y. F.; Yang, Q.; Yang, Y.; Yang, S.; Yang, Y.; Yang, C.; Ye, Z.; Yepes, P.; Yi, L.; Yip, K.; Yoo, I. -K.; Yu, N.; Zbroszczyk, H.; Zha, W.; Zhang, X. P.; Zhang, J.; Zhang, Y.; Zhang, J.; Zhang, J. B.; Zhang, S.; Zhang, Z.; Zhao, J.; Zhong, C.; Zhou, L.; Zhu, X.; Zoulkarneeva, Y.; Zyzak, M.

    2015-08-24

    We report on measurements of dielectron (e⁺e⁻) production in Au+Au collisions at a center-of-mass energy of 200 GeV per nucleon-nucleon pair using the STAR detector at RHIC. Systematic measurements of the dielectron yield as a function of transverse momentum (pT) and collision centrality show an enhancement compared to a cocktail simulation of hadronic sources in the low invariant-mass region (Mee < 1GeV/c2). This enhancement cannot be reproduced by the ρ-meson vacuum spectral function. In minimum-bias collisions, in the invariant-mass range of 0.30 – 0.76GeV/c², integrated over the full pT acceptance, the enhancement factor is 1.76±0.06(stat.)±0.26(sys.)±0.29(cocktail). The enhancement factor exhibits weak centrality and pT dependence in STAR's accessible kinematic regions, while the excess yield in this invariant-mass region as a function of the number of participating nucleons follows a power-law shape with a power of 1.44±0.10. Models that assume an in-medium broadening of the ρ-meson spectral function consistently describe the observed excess in these measurements. In addition, we report on measurements of ω- and Φ-meson production through their e⁺e⁻ decay channel. These measurements show good agreement with Tsallis blast-wave model predictions, as well as, in the case of the Φ meson, results through its K⁺K⁻ decay channel. In the intermediate invariant-mass region (1.1 < Mee < 3GeV/c²), we investigate the spectral shapes from different collision centralities. Physics implications for possible in-medium modification of charmed hadron production and other physics sources are discussed.

  4. Measurement of top anti-top cross section in proton - anti-proton collider at s**(1/2) = 1.96-TeV

    SciTech Connect (OSTI)

    Mal, Prolay Kumar

    2005-04-01

    Discovery of the top quark in 1995 at the Fermilab Tevatron collider concluded a long search following the 1977 discovery of bottom (b) quark [1] and represents another triumph of the Standard Model (SM) of elementary particles. Top quark is one of the fundamental fermions in the Standard Model of electroweak interactions and is the weak-isospin partner of the bottom quark. A precise measurement of top pair production cross-section would be a test of Quantum Chromodynamics (QCD) prediction. Presently, Tevatron is the world's highest energy collider where protons (p) and anti-protons ({anti p}) collide at a centre of mass energy (ps) of 1.96 TeV. At Tevatron top (t) and anti-top ({anti t}) quarks are predominantly pair produced through strong interactions--quark annihilation ({approx_equal} 85%) and gluon fusion ({approx_equal} 15%). Due to the large mass of top quark, t or {anti t} decays ({approx} 10{sup -25} sec) before hadronization and in SM framework, it decays to a W boson and a b quark with {approx} 100% branching ratio (BR). The subsequent decay of W boson determines the major signatures of t{anti t} decay. If both W bosons (coming from t and {anti t} decays) decay into leptons (viz., ev{sub e}, {mu}{nu}{sub {mu}} or {tau}{nu}{sub {tau}}) the corresponding t{bar t} decay is called dileptonic decay. Of all dileptonic decay modes of t{bar t}, the t{bar t} {yields} WWb{anti b} {yields} ev{sub e}{mu}{nu}{sub {mu}}b{anti b} (e{mu} channel) decay mode has the smallest background contamination from Z{sup 0} production or Drell-Yan process; simultaneously, it has the highest BR ({approx} 3.16%) [2] amongst all dileptonic decay modes of t{bar t}. During Run I (1992-1996) of Tevatron, three e{mu} candidate events were detected by D0 experiment, out of 80 candidate events (inclusive of all decay modes of t{bar t}). Due to the rarity of the t{bar t} events, the measured cross-section has large uncertainty in its value (viz., 5.69 {+-} 1.21(stat) {+-} 1.04(sys) pb {at} {radical}s = 1.8 TeV measured by D0 [3]). This analysis presents a cross section measurement in e{mu} channel utilizing {approx} 228 pb{sup -1} of data collected by D0 experiment during Tevatron Run II (between June 2002 and April 2004).

  5. Beam Normal Single Spin Asymmetry in Forward Angle Inelastic Electron-Proton Scattering using the Q-Weak Apparatus

    SciTech Connect (OSTI)

    Nuruzzaman, nfn

    2014-12-01

    The Q-weak experiment in Hall-C at the Thomas Jefferson National Accelerator Facility has made the first direct measurement of the weak charge of the proton through the precision measurement of the parity-violating asymmetry in elastic electron-proton scattering at low momentum transfer. There is also a parity conserving Beam Normal Single Spin Asymmetry or transverse asymmetry (B_n) on H_2 with a sin(phi)-like dependence due to two-photon exchange. If the size of elastic B_n is a few ppm, then a few percent residual transverse polarization in the beam, combined with small broken azimuthal symmetries in the detector, would require a few ppb correction to the Q-weak data. As part of a program of B_n background studies, we made the first measurement of B_n in the N-to-Delta(1232) transition using the Q-weak apparatus. The final transverse asymmetry, corrected for backgrounds and beam polarization, was found to be B_n = 42.82 ± 2.45 (stat) ± 16.07 (sys) ppm at beam energy E_beam = 1.155 GeV, scattering angle theta = 8.3 deg, and missing mass W = 1.2 GeV. B_n from electron-nucleon scattering is a unique tool to study the gamma^* Delta Delta form factors, and this measurement will help to improve the theoretical models on beam normal single spin asymmetry and thereby our understanding of the doubly virtual Compton scattering process. To help correct false asymmetries from beam noise, a beam modulation system was implemented to induce small position, angle, and energy changes at the target to characterize detector response to the beam jitter. Two air-core dipoles separated by ~10 m were pulsed at a time to produce position and angle changes at the target, for virtually any tune of the beamline. The beam energy was modulated using an SRF cavity. The hardware and associated control instrumentation will be described in this dissertation. Preliminary detector sensitivities were extracted which helped to reduce the width of the measured asymmetry. The beam modulation system has also proven valuable for tracking changes in the beamline optics, such as dispersion at the target.

  6. The calibration of the WISE W1 and W2 Tully-Fisher relation

    SciTech Connect (OSTI)

    Neill, J. D. [California Institute of Technology, 1200 East California Boulevard, MC 278-17, Pasadena, CA 91125 (United States); Seibert, Mark; Scowcroft, Victoria [The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Tully, R. Brent [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Courtois, Hlne; Sorce, Jenny G. [Institut de Physique Nucleaire, Universit Claude Bernard Lyon I, F-69100 Lyon (France); Jarrett, T. H. [University of Cape Town, Private Bag X3, Rondebosch 7701, Republic of South Africa (South Africa); Masci, Frank J. [Image Processing and Analysis Center (IPAC), California Institute of Technology, 1200 East California Boulevard, MC 100-22, Pasadena, CA 91125 (United States)

    2014-09-10

    In order to explore local large-scale structures and velocity fields, accurate galaxy distance measures are needed. We now extend the well-tested recipe for calibrating the correlation between galaxy rotation rates and luminositiescapable of providing such distance measuresto the all-sky, space-based imaging data from the Wide-field Infrared Survey Explorer (WISE) W1 (3.4 ?m) and W2 (4.6 ?m) filters. We find a correlation of line width to absolute magnitude (known as the Tully-Fisher relation, TFR) of M{sub W1}{sup b,i,k,a}=?20.35?9.56(log?W{sub mx}{sup i}?2.5) (0.54 mag rms) and M{sub W2}{sup b,i,k,a}=?19.76?9.74(log?W{sub mx}{sup i}?2.5) (0.56 mag rms) from 310 galaxies in 13 clusters. We update the I-band TFR using a sample 9% larger than in Tully and Courtois. We derive M{sub I}{sup b,i,k}=?21.34?8.95(log?W{sub mx}{sup i}?2.5) (0.46 mag rms). The WISE TFRs show evidence of curvature. Quadratic fits give M{sub W1}{sup b,i,k,a}=?20.48?8.36(log?W{sub mx}{sup i}?2.5)+3.60(log?W{sub mx}{sup i}?2.5){sup 2} (0.52 mag rms) and M{sub W2}{sup b,i,k,a}=?19.91?8.40(log?W{sub mx}{sup i}?2.5)+4.32(log?W{sub mx}{sup i}?2.5){sup 2} (0.55 mag rms). We apply an I-band WISE color correction to lower the scatter and derive M{sub C{sub W{sub 1}}}=?20.22?9.12(log?W{sub mx}{sup i}?2.5) and M{sub C{sub W{sub 2}}}=?19.63?9.11(log?W{sub mx}{sup i}?2.5) (both 0.46 mag rms). Using our three independent TFRs (W1 curved, W2 curved, and I band), we calibrate the UNION2 Type Ia supernova sample distance scale and derive H {sub 0} = 74.4 1.4(stat) 2.4(sys) km s{sup 1} Mpc{sup 1} with 4% total error.

  7. Search for r-parity violating supersymmetry in multilepton final states with the D0 detector

    SciTech Connect (OSTI)

    Kaefer, Daniela; /Aachen, Tech. Hochsch.

    2006-11-01

    Results obtained from a search for the trilepton signature {mu}{mu}{ell} (with {ell} = e, or {mu}) are combined with two complementary searches for the trilepton signatures ee{ell} and eer and interpreted in the framework of R-parity violating Supersymmetry. Pairwise, R-parity conserving production of the supersymmetric particles is assumed, followed by R-parity violating decays via an LL{bar E}-operator with one dominant coupling {lambda}{sub 122}. An LL{bar E}-operator couples two weak isospin doublet and one singlet (s)lepton fields and thus violates lepton number conservation. The data, collected with the D0 detector at the Fermilab proton-antiproton collider Tevatron, corresponds to an integrated luminosity of {integral} L dt = 360 {+-} 23 pb{sup -1}. No evident is observed, while 0.41 {+-} 0.11(stat) {+-} 0.07(sys) events are expected from Standard Model processes. The resulting 95% confidence level cross section limits on new physics producing a {mu}{mu}{ell} signature in the detector are of the order of 0.020 to 0.136 pb. They are interpreted in two different supersymmetry scenarios: the mSUGRA and the MSSM model. The corresponding lower limits on the masses of the lightest neutralino ({tilde {chi}}{sub 1}{sup 0}) and the lightest chargino ({tilde {chi}}{sub 1}{sup {+-}}) in case of the mSUGRA model are found to be in the range of: mSUGRA, {mu} > 0: M({tilde {chi}}{sub 1}{sup 0}) {approx}> 115-128 GeV and M({tilde {chi}}{sub 1}{sup {+-}}) {approx}> 215-241 GeV; mSUGRA, {mu} < 0: ({tilde {chi}}{sub 1}{sup 0}) {approx}> 101-114 GeV and M({tilde {chi}}{sub 1}{sup {+-}}) {approx}> 194-230 GeV, depending on the actual values of the model parameters: m{sub 0}, m{sub 1/2}, A{sub 0}, tan{beta}, and {mu}. The first and second parameters provide the boundary conditions for the masses of the supersymmetric spin-0 and spin-1/2 particles, respectively, while A{sub 0} gives the universal value for the trilinear couplings at the GUT scale. The parameter tan {beta} denotes the ratio of the vacuum expectation values of the two Higgs fields and {mu}, finally, represents the Higgs mixing parameter. In the MSSM scenario the lower bound on the mass of the lightest chargino (for fixed neutralino mass) is found to be in the range of: M({tilde {chi}}{sub 1}{sup {+-}}) {approx}> 205 GeV, for M({tilde {chi}}{sub 1}{sup 0}) = 30 GeV; M({tilde {chi}}{sub 1}{sup {+-}}) {approx}> 232 GeV, for M({tilde {chi}}{sub 1}{sup 0}) = 200 GeV. The parameters of the considered MSSM model are: M{sub 1}, M{sub 2}, M{sub 3}, A{sub 0}, tan {beta}, {mu}, and m{sub A}. The first three parameters define the common masses of the superpartners of the U(1){sub Y}, SU(2){sub L}, and SU(3){sub C} bosons at the electroweak scale, respectively. The following three parameters are identical to those defined in the mSUGRA model above, while m{sub A} denotes the mass of the pseudoscalar Higgs boson, present in the supersymmetric extension of the Standard Model. In addition all sfermion masses are set to 1000 GeV.

  8. The power of event-driven analytics in Large Scale Data Processing

    ScienceCinema (OSTI)

    None

    2011-04-25

    FeedZai is a software company specialized in creating high-­-throughput low-­-latency data processing solutions. FeedZai develops a product called "FeedZai Pulse" for continuous event-­-driven analytics that makes application development easier for end users. It automatically calculates key performance indicators and baselines, showing how current performance differ from previous history, creating timely business intelligence updated to the second. The tool does predictive analytics and trend analysis, displaying data on real-­-time web-­-based graphics. In 2010 FeedZai won the European EBN Smart Entrepreneurship Competition, in the Digital Models category, being considered one of the "top-­-20 smart companies in Europe". The main objective of this seminar/workshop is to explore the topic for large-­-scale data processing using Complex Event Processing and, in particular, the possible uses of Pulse in the scope of the data processing needs of CERN. Pulse is available as open-­-source and can be licensed both for non-­-commercial and commercial applications. FeedZai is interested in exploring possible synergies with CERN in high-­-volume low-­-latency data processing applications. The seminar will be structured in two sessions, the first one being aimed to expose the general scope of FeedZai's activities, and the second focused on Pulse itself: 10:00-11:00 FeedZai and Large Scale Data Processing Introduction to FeedZai FeedZai Pulse and Complex Event Processing Demonstration Use-Cases and Applications Conclusion and Q&A 11:00-11:15 Coffee break 11:15-12:30 FeedZai Pulse Under the Hood A First FeedZai Pulse Application PulseQL overview Defining KPIs and Baselines Conclusion and Q&A About the speakers Nuno Sebastião is the CEO of FeedZai. Having worked for many years for the European Space Agency (ESA), he was responsible the overall design and development of Satellite Simulation Infrastructure of the agency. Having left ESA to found FeedZai, Nuno is currently responsible for the whole operations of the company. Nuno holds an M.Eng. in Informatics Engineering for the University of Coimbra, and an MBA from the London Business School. Paulo Marques is the CTO of FeedZai, being responsible for product development. Paulo is an Assistant Professor at the University of Coimbra, in the area of Distributed Data Processing, and an Adjunct Associated Professor at Carnegie Mellon, in the US. In the past Paulo lead a large number of projects for institutions like the ESA, Microsoft Research, SciSys, Siemens, among others, being now fully dedicated to FeedZai. Paulo holds a Ph.D. in Distributed Systems from the University of Coimbra.

  9. The power of event-driven analytics in Large Scale Data Processing

    SciTech Connect (OSTI)

    2011-02-24

    FeedZai is a software company specialized in creating high-­-throughput low-­-latency data processing solutions. FeedZai develops a product called "FeedZai Pulse" for continuous event-­-driven analytics that makes application development easier for end users. It automatically calculates key performance indicators and baselines, showing how current performance differ from previous history, creating timely business intelligence updated to the second. The tool does predictive analytics and trend analysis, displaying data on real-­-time web-­-based graphics. In 2010 FeedZai won the European EBN Smart Entrepreneurship Competition, in the Digital Models category, being considered one of the "top-­-20 smart companies in Europe". The main objective of this seminar/workshop is to explore the topic for large-­-scale data processing using Complex Event Processing and, in particular, the possible uses of Pulse in the scope of the data processing needs of CERN. Pulse is available as open-­-source and can be licensed both for non-­-commercial and commercial applications. FeedZai is interested in exploring possible synergies with CERN in high-­-volume low-­-latency data processing applications. The seminar will be structured in two sessions, the first one being aimed to expose the general scope of FeedZai's activities, and the second focused on Pulse itself: 10:00-11:00 FeedZai and Large Scale Data Processing Introduction to FeedZai FeedZai Pulse and Complex Event Processing Demonstration Use-Cases and Applications Conclusion and Q&A 11:00-11:15 Coffee break 11:15-12:30 FeedZai Pulse Under the Hood A First FeedZai Pulse Application PulseQL overview Defining KPIs and Baselines Conclusion and Q&A About the speakers Nuno Sebastião is the CEO of FeedZai. Having worked for many years for the European Space Agency (ESA), he was responsible the overall design and development of Satellite Simulation Infrastructure of the agency. Having left ESA to found FeedZai, Nuno is currently responsible for the whole operations of the company. Nuno holds an M.Eng. in Informatics Engineering for the University of Coimbra, and an MBA from the London Business School. Paulo Marques is the CTO of FeedZai, being responsible for product development. Paulo is an Assistant Professor at the University of Coimbra, in the area of Distributed Data Processing, and an Adjunct Associated Professor at Carnegie Mellon, in the US. In the past Paulo lead a large number of projects for institutions like the ESA, Microsoft Research, SciSys, Siemens, among others, being now fully dedicated to FeedZai. Paulo holds a Ph.D. in Distributed Systems from the University of Coimbra.

  10. Proton form factor ratio, {mu}{sub p}G{sub E}{sup P}/G{sub M}{sup P} from double spin asymmetry

    SciTech Connect (OSTI)

    Habarakada Liyanage, Anusha Pushpakumari

    2013-08-01

    The form factors are fundamental properties of the nucleon representing the effect of its structure on its response to electromagnetic probes such as electrons. They are functions of the four-momentum transfer squared Q{sup 2} between the electron and the proton. This thesis reports the results of a new measurement of the ratio of the electric and magnetic form factors of the proton up to Q{sup 2} = 5.66 (GeV/c){sup 2} using the double spin asymmetry with a polarized beam and target. Experiment E07-003 (SANE, Spin Asymmetries of the Nucleon Experiment) was carried out in Hall C at Jefferson Lab in 2009 to study the proton spin structure functions with a dynamically polarized ammonia target and longitudinally polarized electron beam. By detecting elastically scattered protons in the High-Momentum Spectrometer (HMS) in coincidence with the electrons in the Big Electron Telescope Array (BETA), elastic measurements were carried out in parallel. The elastic double spin asymmetry allows one to extract the proton electric to magnetic form factor ratio G{sup p}{sub E}/G{sup p}{sub M} at high-momentum transfer, Q{sup 2} = 5.66 (GeV/c){sup 2}. In addition to the coincidence data, inclusively scattered electrons from the polarized ammonia target were detected by HMS, which allows to measure the beam-target asymmetry in the elastic region with the target spin nearly perpendicular to the momentum transfer, and to extract G{sup p}{sub E}/G{sup p}{sub M} at low Q{sup 2} = 2.06 (GeV/c){sup 2}. This alternative measurement of G{sup p}{sub E}/G{sup p}{sub M} has verified and confirmed the dramatic discrepancy at high Q{sup 2} between the Rosenbluth and the recoil-polarization-transfer iv method with a different measurement technique and systematic uncertainties uncorrelated to those of the recoil-polarization measurements. The measurement of the form factor ratio at Q{sup 2} = 2.06 (GeV/c){sup 2} has been determined as {mu}{sub p}G{sup p}{sub E}/G{sup p}{sub M} = 0.605{+-}0.178{sub stat}{+-}0.033{sub sys} which is in agreement with an earlier measurement with the polarized target technique at similar kinematics. The measurement of the form factor ratio at Q{sup 2} = 5.66 (GeV/c){sup 2} has been determined as {mu}{sub p}G{sup p}{sub E}/G{sup p}{sub M} = 0.672 {+-} 0.362{sub stat} which represents the highest Q{sup 2} reach with the double spin asymmetry to date.

  11. Worksheet

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

    UTILITY_ID","UTILITY_NAME","TRANSLINE_NO","TERMINAL_LOC_FROM","TERMINAL_LOC_TO","PERCENT_OWNED","LINE_LENGTH","LINE_TYPE","VOLTAGE_TYPE","VOLTAGE_OPERATING","VOLTAGE_DESIGN","CONDUCTOR_SIZE","CONDUCTOR_MAT_TYPE","CONDUCTOR_CONFIG","CIRCUIT_PERSTRUCT_PRES","CIRCUIT_PERSTRUCT_ULT","POLE_TOWER_TYPE","RATED_CAPACITY","LAND_LANDRIGHT_COSTS","POLE_TOWER_FIXTURE_COSTS","CONDUCTOR_DEVICE_COSTS","CONSTRUCTION_ETC_COSTS","TOTAL_LINE_COSTS","IN_SERVICE_DATE" 2003,1015,"Austin City of",1,"Northland","Magnesium Plant",100,4.11,"OH","AC",138,138,795,"ACSR Drake/ACSS Rail","Single",1,2,"Steel & Wood Poles",215,0,17500,8000,19500,45000,"application/vnd.ms-excel" 2003,1015,"Austin City of",2,"Grove","Met Center",100,3.1,"OH","AC",138,138,795,"ASCR Drake","Double",1,1,"Steel Pole",430,0,30000,10000,35000,75000,"application/vnd.ms-excel" 2003,1015,"Austin City of",3,"Dessau","Daffin Gin",100,6.01,"OH","AC",138,138,795,"ASCR Drake","Single",1,1,"Steel Pole",215,0,60000,15000,40000,115000,"application/vnd.ms-excel" 2003,1015,"Austin City of",4,"Burleson","AMD",100,2.2,"OH","AC",138,138,795,"ACR Drake","Double",2,2,"Steel Pole",430,0,75000,55000,120000,250000,"application/vnd.ms-excel" 2003,1015,"Austin City of",5,"Bergstrom","Kingsberry",100,4.2,"OH","AC",138,138,795,"ASCR Drake/AAAC","Single",1,2,"Steel & Wood Poles",215,0,75000,35000,340000,450000,"application/vnd.ms-excel" 2003,1015,"Austin City of",6,"Mcneil","Magnesium Plant",100,3.24,"OH","AC",138,138,795,"ACSR Drake","Double",1,2,"Steel Pole & Steel Tower",430,0,380000,76000,644000,1100000,"application/vnd.ms-excel" 2003,1015,"Austin City of",7,"Summit","Magnesium Plant",100,2.18,"OH","AC",138,138,795,"ACSR Drake","Double",1,2,"Steel Pole & Steel Tower",430,0,265000,125000,410000,800000,"application/vnd.ms-excel" 2003,1307,"Basin Electric Power Coop",1,"Rapid City","New Underwood",65,18.55,"OH","AC",230,230,1272,"ACSR","Single",1,1,"Single Pole, Steel",460,0,0,0,5300000,5300000,"application/vnd.ms-excel" 2003,1586,"Bentonville City of",1,"AEP/SWEPCO","City Substation F",100,1,"OH","AC",161,161,477,"ACSR","Single",1,1,"Wood and Steel Single Pole",199,18000,81522,28082,214516,342120,"application/vnd.ms-excel" 2003,2172,"Brazos Electric Power Coop",1,"Coppell","Lewisville",100,7.03,"OH","AC",138,138,1033,"ACSR","Double",1,1,"Concrete/Steel Single Pole",485,17577.55,2527717,537265.96,956475.39,4039035.9,"application/vnd.ms-excel" 2003,2172,"Brazos Electric Power Coop",2,"Boyd","Newark",100,1.8,"OH","AC",138,138,795,"ACSR","Single",2,2,"Concrete/Steel Single Pole",215,133929.08,538282.3,131112.75,246577.6,1049901.73,"application/vnd.ms-excel" 2003,2172,"Brazos Electric Power Coop",3,"Cedar Hill","Sardis",100,5.1,"OH","AC",138,138,795,"ACSR","Single",1,1,"Concrete Si ngle Ploe",215,24515.26,652910.22,246676.96,560582.43,1484684.87,"application/vnd.ms-excel" 2003,5580,"East Kentucky Power Coop Inc",1,"Jamestown Tap","Jamestown Tap",100,0.47,"OH","AC",161,161,556.5,"ACSR","Single",1,1,"Wood Single Pole",292,43326,160508,68789,0,272623,"application/vnd.ms-excel" 2003,5580,"East Kentucky Power Coop Inc",2,"Pulaski Co. Tap","Pulaski Co. Tap",100,5.88,"OH","AC",161,161,795,"ACSR","Single",1,1,"Wood H-Frame Structure",367,494183,1092462,468198,0,2054843,"application/vnd.ms-excel" 2003,7197,"Georgia Transmission Corp",1,"Shoal Creek","Spout Spring",100,10.83,"OH","AC",230,230,1351,"ACSR","Single",1,1,"Concrete, Single Pole & Steel",602,1277945,1685271,444690,6047603,9455509,"application/vnd.ms-excel" 2003,7197,"Georgia Transmission Corp",2,"Dresden","Yellowdirt",100,9.5,"OH","AC",230,230,795,"ACSR","Double",1,1,"Concrete, Single Pole",866,870826,772876,375515,3649376,5668593,"application/vnd.ms-excel" 2003,7197,"Georgia Transmission Corp",3,"East Moultrie","West Valdosta",100,38.46,"OH","AC",230,230,1622,"ACSR","Single",1,1,"Concrete, Single Pole",596,1191168,2829632,1476802,10279078,15776680,"application/vnd.ms-excel" 2003,7490,"Grand River Dam Authority",1,"Cowskin","Grove PSO",100,4.5,"OH","AC",138,138,795,"ACSR","Single/Twisted",1,1,"Wood Pole",223,287671,135402,156769,880890,1460732,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",1,"BASTROP","AUSTIN",100,0.32,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,9155828,155817297,37044659,47228709,249246493,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",2,"BASTROP","AUSTROP",100,0.32,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",3,"BASTROP","AUSTROP",100,0.32,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",4,"BASTROP","AUSTROP",100,0.32,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",5,"CANYON","SAN MARCOS/LOCKHART",100,0.31,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",6,"CANYON","SAN MARCOS/LOCKHART",100,0.31,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",7,"CANYON","SAN MARCOS/LOCKHART",100,0.31,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",8,"CANYON","SAN MARCOS/LOCKHART",100,0.31,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",9,"CANYON","SAN MARCOS/LOCKHART",100,0.31,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",10,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",11,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",12,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",13,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",14,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",15,"CICO","HELOTES",100,4,"OH","AC",138,138,795,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",16,"LOCKHART","DUMP HILL",100,1.6,"OH","AC",138,138,795,"ACSR","Single",1,1,"Concrete Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",17,"HILL POWER STATION","NUECES BAY",100,17.3,"OH","AC",138,138,795,"ACSR","Double",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",18,"NORTH OAK PARK","LON HILL",100,14.9,"OH","AC",138,138,795,"ACSR","Double",1,1,"Wood Pole",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",19,"STATE HIGHTWAY 80",,100,0.38,"OH","AC",138,138,211.5,"ACSR","Single",1,1,"Wood H-Frame Structure",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",20,"STATE HIGHWAY 80",,100,0.38,"OH","AC",138,138,211.5,"ACSR","Single",1,1,"Wood H-Frame Structure",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",21,"STERLING/MITCHELL LINE","TWINN BUTTES",100,135.08,"OH","AC",345,345,1590,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",22,"VERDE CREEK","KERRVILLE STADIUM",100,0.1,"OH","AC",138,138,336,"ACSR","Double",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",23,"VERDE CREEK","KERRVILLE STADIUM",100,0.1,"OH","AC",138,138,336,"ACSR","Double",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",24,"VERDE CREEK","KERRVILLE STADIUM",100,0.1,"OH","AC",138,138,336,"ACSR","Double",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",25,"VERDE CREEK","KERRVILLE STADIUM",100,0.1,"OH","AC",138,138,336,"ACSR","Double",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",26,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",27,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",28,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",29,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",30,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,11269,"Lower Colorado River Authority",31,"ZORN","MCCARTY LANE",100,4.2,"OH","AC",138,138,1433.6,"ACSR","Single",1,1,"Steel Tower",,0,0,0,0,0,"application/vnd.ms-excel" 2003,15143,"Platte River Power Authority",1,"Rawhide","Timberline West",100,31.63,"OH","AC",230,230,954,"ACSR","Single",2,2,"Steel/Tower & Pole",378,5553,1928767,2385430,251850,4571600,"application/vnd.ms-excel" 2003,15159,"Plymouth City of",1,"Mullet River Sub","Sub # 1",100,0.8,"OH","AC",138,138,336.4,"ACSR","SINGLE",1,1,"Steel Double Pole",33,0,0,0,1492139,1492139,"application/vnd.ms-excel" 2003,16534,"Sacramento Municipal Util Dist",1,"Natomas","Elverta",100,4.3,"OH","AC",230,230,954,"Aluminum","Single",1,1,"Steel Tower",316,0,0,0,0,0,"application/vnd.ms-excel" 2003,17543,"South Carolina Pub Serv Auth",1,"Rainey - Anderson (Duke) #1","Rainey - Anderson (Duke) #1",100,9.51,"OH","AC",230,230,1272,"ACSR","Double",2,2,"Steel / Tower",956,840152,1230361,1207282,22364,3300159,"application/vnd.ms-excel" 2003,17543,"South Carolina Pub Serv Auth",2,"Rainey - Anderson (Duke) #2","Rainey - Anderson (Duke) #2",100,9.51,"OH","AC",230,230,1272,"ACSR","Double",2,2,"Steel / Tower",956,840152,1230361,1207282,22364,3300159,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",1,"West Ringgold","Center Point",100,7.94,"OH","AC",115,230,954,"ASCR","Single",1,2,"Steel Tower",,2086252,5658529,1502763,3053959,12301503,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",2,"NE Johnson City--Erwin 161kV T","Jonesborough 161 kV SS",100,0.28,"OH","AC",161,161,954,"ASCR","Single",1,1,"Steel Tower",,11050,191917,894933,714987,1812887,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",3,"Elizabethton","Pandara-Shouns",100,15.12,"OH","AC",161,161,636,"ASCR","Single",1,1,"Steel Tower",,282232,1797686,537733,2057572,4675223,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",4,"Sullivan","Blountville",100,0.63,"OH","AC",161,161,1590,"ASCR","Single",2,2,"Steel Tower",,547521,1134556,788061,1224067,3694205,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",5,"Pin Hook","Structure E 104A (NES)",100,1.74,"OH","DC",161,161,2034.5,"ASCR","Single",1,2,"Steel Tower",,179775,881877,641976,270782,1974410,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",6,"Dug Gap 115 kV SS","Center Point 230 kV SS",100,4.49,"OH","AC",115,230,954,"ASCR","Single",2,2,"Steel Tower",,3939251,3451555,545558,1026021,8962385,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",7,"Chickamauga-Ridgedale","Hawthorne 161 kV SS",100,2.82,"OH","AC",161,161,1590,"ASCR","Single",2,2,"Steel Tower",,87206,533582,342640,584799,1548227,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",8,"Ft. Loudoun-Elza 161 kV TL","Spallation Neutron Source 161",100,3.92,"OH","AC",161,161,954,"ASCR","Single",1,1,"Steel Tower",,2972,639541,373150,469765,1485428,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",9,"Leake","Sebastapol SW STA 161 kV",100,0.77,"OH","AC",161,161,636,"ASCR","Single",2,2,"Steel Tower",,36158,236368,103374,167311,543211,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",10,"Sebasatpol 161 kV Switching St","Five Point 161 kV Substation",100,0.13,"OH","AC",161,230,954,"ASCR","Single",1,1,"Steel Tower",,917304,1772761,931352,1477668,5099085,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",11,"Structure 170A","Structure 174",100,0.73,"OH","AC",161,161,636,"ASCR","Single",1,1,"Steel Tower",,0,445863,79638,194574,720075,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",12,"Ramer-Hickory Valley 161 kV TL","Middleton 46 kV SS",100,6.81,"OH","AC",161,161,954,"ASCR","Single",1,1,"Steel Tower",,566805,1162854,447607,787813,2965079,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",13,"Lowndes-Miller","Valley View",100,0.46,"OH","AC",500,500,954,"ASCR","Triple",1,2,"Steel Tower",,0,688737,255237,341129,1285103,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",14,"Sweetwater 161 kV SS","Madisonville 161 kV SS",100,8.95,"OH","AC",161,161,954,"ASCR","Single",1,1,"Steel Tower",,1066219,1474937,466681,797814,3805651,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",15,"East Point 500 kV SS","Hanceville 161 kV TL",100,11.25,"OH","AC",161,161,1351.5,"ASCR","Single",1,2,"Steel Tower",,1416513,1442382,606534,1427424,4892853,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",16,"W Cookeville-Crossville 161 kV","W. Crossville SS",100,4.37,"OH","AC",161,161,954,"ASCR","Single",1,2,"Steel Tower",,267463,1112667,651963,964407,2996500,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",17,"East Shelbyville-Unionville","Deason 161 kV SS",100,5.09,"OH","AC",161,161,636,"ASCR","Single",1,1,"Steel Tower",,1071199,931797,430714,320721,2754431,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",18,"Kentucky Hydro","Barkley Hydro",100,2,"OH","AC",161,161,2034.5,"ACSR","Single",1,1,"Steel Tower",,2845,406947,90111,155401,655304,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",19,"MEC Sw Station","Trinity Substation",100,2.9,"OH","AC",161,161,954,"ACSS","Single",2,2,"Steel Tower",,0,604526,474640,608702,1687868,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",20,"Hickory Valley Selmer 161 kV T","North Selmer 161 kV SS",100,4.88,"OH","AC",161,161,636,"ASCR","Single",1,1,"Steel Tower",,357578,632244,368993,899046,2257861,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",21,"Trinity","Morgan Energy Center",100,2.98,"OH","AC",161,161,1590,"ASCR","Single",2,2,"Steel Tower",,7155,647789,386671,513831,1555446,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",22,"MEC","Finley",100,0.61,"OH","AC",161,161,954,"ASCR","Single",1,2,"Steel Tower",,9879,303540,156165,181613,651197,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",23,"Pickwick-South Jackson","Magic Valley",100,1.38,"OH","AC",161,161,954,"ASCR","Single",1,1,"Steel Pole",,78377,284367,113237,237716,713697,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",24,"Wolf Creek-Choctaw 500 kV TL","Reliant French Camp Gener Plt",100,0.11,"OH","AC",500,500,954,"ASCR","Triple",1,2,"Steel Tower",,0,863770,411493,891161,2166424,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",25,"Widows Creek Ft. Payne 161 kV","Flat Rock 161 kV SS",100,2.05,"OH","AC",161,161,397.5,"ASCR","Single",1,1,"Steel Tower",,130460,443384,182965,410228,1167037,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",26,"Volunteer-Cherokee HP 161 kV T","Oakland 161 kV SS",100,0.5,"OH","AC",161,161,1351,"ASCR","Single",1,2,"Steel Tower",,0,159020,71787,133784,364591,"application/vnd.ms-excel" 2003,18642,"Tennessee Valley Authority",27,"Cordell-Hull-Carthage 161 kV","South Carthage 161 kV SS",100,1.68,"OH","AC",161,161,636,"ASCR","Single",1,2,"Steel Tower",,0,209664,102390,256537,568591,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",1,"Arco","Sprectrum",100,5.89,"OH","AC",138,138,336.4,"ACSR","Single",1,1,"Wood Pole",91,37547.56,399750.8,416067.16,0,853365.52,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",2,"Hazel Dell Jct","Hazel Dell",100,3.12,"OH","AC",138,138,795,"ACSR","Single",1,1,"Wood Pole",158,72967.09,417464.37,285659.16,0,776090.62,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",3,"Red River","Tenaska Kiowa Sw",100,75.75,"OH","AC",345,345,795,"ACSR","Single",1,1,"Combination Pole",158,0,0,0,47569327.23,47569327.23,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",4,"Washita Sw","Blue Canyon",100,23.96,"OH","AC",138,138,1590,"ACSR","Single",1,1,"Wood Pole",239,0,0,0,5092171.22,5092171.22,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",5,"Limestone Jct","Limestone",100,0.5,"OH","AC",138,138,336.4,"ACSR","Single",1,1,"Wood Pole",91,25673.08,159253.08,77468.07,0,262394.23,"application/vnd.ms-excel" 2003,20447,"Western Farmers Elec Coop Inc",6,"OGE Sunset Jct","Sunset Corner",100,0.15,"OH","AC",161,161,336.4,"ACSR","Singel",1,1,"Wood Pole",91,0,29315.87,35224.01,0,64539.88,"application/vnd.ms-excel" 2003,27000,"Western Area Power Admin",1,"Shiprock","Four Corners",100,8.2,"OH","AC",345,345,,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",2,"Coolidge","Sundance 1 and 2",100,9.8,"OH","AC",230,230,954,"ASCR",,2,2,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",3,"Structure 96/4","O/Banion 1",100,38,"OH","AC",230,230,,"ASCR",,2,2,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",4,"Mead","Market Place",100,12.9,"OH","AC",525,525,,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",5,"Bears Ears","Craig",100,1,"OH","AC",345,345,,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",6,"Glen Canyon Pumping Plant","Glen Canyon SW Yard",100,1,"OH","AC",345,345,,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",7,"Baker","Bowman",22.96,53.96,"OH","AC",230,230,954,"ASCR",,1,1,"Wood H",,0,0,0,0,0 2003,27000,"Western Area Power Admin",8,"Basin Tap #2","Washburn",100,2.23,"OH","AC",230,230,795,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",9,"Craig","Rifle",100,96,"OH","AC",230,230,1272,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",10,"Garrison","Basin Tap #1",100,20.97,"OH","AC",230,230,795,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",11,"Everta","Roseville",100,13.3,"OH","AC",230,230,,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",12,"Griffith","McConnico",100,8,"OH","AC",230,230,1272,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",13,"McConnico","Peacock",100,29.4,"OH","AC",230,230,795,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",14,"Liberty","Buckeye",100,6.7,"OH","AC",230,230,1272,"ASCR",,2,2,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",15,"Liberty","Parker",100,118.7,"OH","AC",230,230,1272,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",16,"Liberty","Estrella",100,10.8,"OH","AC",230,230,954,"ASCR",,2,2,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",17,"Liberty","Lone Batte",100,38.2,"OH","AC",230,230,954,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",18,"Lone Butte","Sundance",100,38.4,"OH","AC",230,230,954,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",19,"New Waddell","West Wing",100,10.1,"OH","AC",230,230,954,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",20,"South Point","Topock #1",100,6.46,"OH","AC",230,230,1590,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0 2003,27000,"Western Area Power Admin",21,"South Point","Topock #2",100,6.34,"OH","AC",230,230,1590,"ASCR",,1,1,"Steel Lattice",,0,0,0,0,0