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Sample records for daniels midland ia

  1. Archer Daniels Midland Company | Department of Energy

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

    Archer Daniels Midland Company Archer Daniels Midland Company Inter‐stage Piping in Compressor facility (Courtesy of Archer Daniels Midland Company) Inter-stage Piping in Compressor facility (Courtesy of Archer Daniels Midland Company) ARCHER DANIELS MIDLAND ILLINOIS ICCS PROJECT In October 2009, DOE selected the Archer Daniels Midland Company (ADM) team to conduct one of 12 projects in Phase 1 of its Industrial Carbon Capture and Storage (ICCS) program. DOE again selected the project in

  2. Biomass IBR Fact Sheet: Archer Daniels Midland

    Office of Energy Efficiency and Renewable Energy (EERE)

    Archer Daniels Midland will develop a pilot plant to demonstrate the continuous production of cellulosic ethanol and butyl acrylate from densified corn stover.

  3. Archer Daniels Midland | Open Energy Information

    Open Energy Info (EERE)

    Daniels Midland Address: 4666 Faries Parkway Place: Decatur, IL Zip: 62526 Sector: Biofuels Product: turn crops into renewable products Phone Number: 800-637-5843 Website:...

  4. Midland Power Coop | Open Energy Information

    Open Energy Info (EERE)

    search Name: Midland Power Coop Address: 1005 E. Lincoln Way Place: Jefferson, IA Zip: 50129 Phone Number: 1-515-386-4111 Facebook: https:www.facebook.commidlandpower...

  5. Daniel Wood

    Broader source: Energy.gov [DOE]

    Daniel Wood is the Data Visualization and Cartographic Specialist in the Office of Public Affairs at the Department of Energy. He develops creative and interactive ways of viewing the Energy...

  6. Daniel Haskel

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

    Daniel Haskel Argonne National Laboratory 9700 S. Cass Ave 431E008 Argonne, Il 60439 Phone: 252-7758 Fax: 252-7392 E-Mail: haskel@aps.anl.gov EducationExperience: University of...

  7. Midland County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Zone Subtype B. Registered Energy Companies in Midland County, Texas Hilliard Energy Renovar Energy Corp Skyward Energy LLC Places in Midland County, Texas Midland, Texas Odessa,...

  8. NREL: Energy Analysis - Daniel Getman

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

    Daniel Getman Photo of Daniel Getman. Daniel Getman is a member of the Data Analysis and Visualization Group in the Strategic Energy Analysis Center. Geospatial Data Science Team...

  9. Sandia Energy - Daniel Laird

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

    Sandia National Laboratories' Water Power Technologies department which includes Marine Hydrokinetic, Conventional Hydro, and Offshore Wind technologies. Daniel joined...

  10. Daniel A. Hitchcock

    Broader source: Energy.gov [DOE]

    Dr. Daniel A. Hitchcock is the acting Associate Director for Advanced Scientific Computing in the Office of Science.

  11. Daniel Oblinsky | Photosynthetic Antenna Research Center

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

    Daniel Oblinsky Daniel Oblinsky Daniel Oblinsky Graduate Student E-mail: doblinsky@gmail.com Website: Princeton University Graduate Students...

  12. Daniel Carpenter | Bioenergy | NREL

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

    Daniel.Carpenter@nrel.gov | 303-384-6709 Research Interests Impact of feedstocks on thermochemical conversion performance (pyrolysis, catalytic pyrolysis, gasification), especially ...

  13. Daniel Shechtman and Quasicrystals

    Office of Scientific and Technical Information (OSTI)

    Daniel (Danny) Shechtman has won the 2011 Nobel Prize in Chemistry "for the discovery of ... Technion Scientist Wins Nobel Prize in Chemistry Resources with Additional Information ...

  14. Daniel Adams | Department of Energy

    Energy Savers [EERE]

    Daniel Adams About Us Daniel Adams - Research Analyst, Bioenergy Technologies Office Most Recent Energy Department Harvesting Technology Goes Commercial October 1 Cornstalks Aren't ...

  15. DOE Zero Energy Ready Home Case Study: Cobblestone Homes, Midland...

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

    Cobblestone Homes, Midland, MI DOE Zero Energy Ready Home Case Study: Cobblestone Homes, Midland, MI Case study of a DOE Zero Energy Ready home in Midland, MI, that scored HERS 49 ...

  16. Midland, Michigan: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    1st congressional district and Michigan's 4th congressional district.12 Registered Energy Companies in Midland, Michigan Dow Chemical Co Dow Kokam References US Census...

  17. Midland, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    district.12 Registered Energy Companies in Midland, Texas Hilliard Energy Renovar Energy Corp Skyward Energy LLC References US Census Bureau Incorporated place and...

  18. Midland District Heating District Heating Low Temperature Geothermal...

    Open Energy Info (EERE)

    Midland District Heating District Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Midland District Heating District Heating Low Temperature Geothermal...

  19. Daniel B. Poneman

    Office of Energy Efficiency and Renewable Energy (EERE)

    Former Deputy Secretary Daniel Poneman was nominated by President Obama to be Deputy Secretary of Energy on April 20, 2009, and was confirmed by the United States Senate on May 18, 2009. Under the...

  20. Daniel B. Poneman | Department of Energy

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

    Daniel B. Poneman - Former Deputy Secretary of Energy Daniel B. Poneman Former Deputy Secretary Daniel Poneman was nominated by President Obama to be Deputy Secretary of Energy on...

  1. Daniel Molzahn | Argonne National Laboratory

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

    Photo of Daniel Molzahn Daniel Molzahn Computational Engineer, Energy Systems Modeling & Simulation News Research projects will help optimize grid E-mail dmolzahn@anl.gov Projects Distribution Automation

  2. Dr. Daniel Bullen- Biography

    Broader source: Energy.gov [DOE]

    Dr. Daniel Bullen is the Defense Nuclear Facilities Board Lead of their Nuclear Programs & Analysis Group. He has been on the nuclear engineering faculty of several universities, consulting engineer for a number of technology firms, and an engineer with DOE's Lawrence Livermore National Laboratory.

  3. Daniel Wildcat | Department of Energy

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

    Daniel Wildcat About Us Daniel Wildcat, Ph.D. - Professor at Haskell Indian Nations University Daniel Wildcat Daniel Wildcat, Ph.D., is a professor at Haskell Indian Nations University in Lawrence, Kansas, and an accomplished scholar who writes on indigenous knowledge, technology, environment, and education. He is also co-director of the Haskell Environmental Research Studies Center, which he founded with colleagues from the Center for Hazardous Substance Research at Kansas State University. A

  4. NREL: Energy Sciences - Daniel A. Beaton

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

    Daniel A. Beaton Daniel A. Beaton Postdoctoral Researcher Photo of Daniel A. Beaton Phone: (303) 384-7201 Email: Daniel.Beaton@nrel.gov Growing up in Cape Breton eastern Canada,...

  5. Daniel Holz | Department of Energy

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

    Holz About Us Daniel Holz - University of Chicago Daniel Holz writes for Symmetry, an online magazine about particle physics jointly published by Fermilab and SLAC, two of the Department of Energy's 17 National Laboratories. Daniel is a Senior Member of the Kavli Institute for Cosmological Physics at the University of Chicago. Most Recent What are Gravitational Waves? June 27

  6. Daniel Weisz | Photosynthetic Antenna Research Center

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

    Weisz Daniel Weisz Daniel Weisz Graduate Student E-mail: daweisz@wustl.edu Website: Washington University in St. Louis

  7. From: Cohen, Daniel

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

    Cohen, Daniel Sent: Tuesday, March 10, 2015 12:13 PM To: 'Miller, William' Cc: Cymbalsky, John; rmurphy@aga.org; Schryver, David Subject: RE: AGA/APGA Questions re Pre-publication Furnace NOPR Bud, Thank you very much for your questions. We are currently reviewing the questions. As you know, DOE can't answer questions provided by one party concerning a proposed rule outside the public docket for the rulemaking. As such, we will include these questions in our public docket and post to our ex

  8. NREL: Energy Analysis - Daniel Steinberg

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

    Daniel Steinberg is a section supervisor of the Energy Forecasting and Modeling Group in ... from lease and power-purchase agreement contract structures and costs in California." ...

  9. Dr. Daniel Giammar | Photosynthetic Antenna Research Center

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

    Daniel Giammar November 25, 2014 Dr. Daniel Giammar The Chemistry and Engineering for Producing and Supplying Clean Drinking Water An error occurred. Try watching this video on...

  10. Daniel B. Fishman | Department of Energy

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

    B. Fishman About Us Daniel B. Fishman - Technology Manager Daniel B. Fishman is a Technology Manager for the Bioenergy Technologies Office

  11. Daniel Boff | Department of Energy

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

    Daniel Boff About Us Daniel Boff - Analyst, SunShot Initiative Daniel Boff joined the SunShot team in 2014 as analyst for the soft cost program, providing on-the-spot market analysis to support Department of Energy decision makers. Dan also helps manage the soft costs team's diverse portfolio, working on projects related to solar's environmental and avian impacts, real estate, the commercial market, and data standardization. Prior to joining SunShot, Dan worked as an intern at the Solar Energy

  12. Edward J. Daniels | Argonne National Laboratory

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

    Edward J. Daniels Sr. Energy Systems Scientist Telephone (630) 252-5279 E-mail edaniels

  13. Daniel Schabacker | Argonne National Laboratory

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

    Daniel Schabacker Biochemist; Bio-Detection Technologies Team Leader - Energy Systems Daniel Schabacker holds the position of Team Leader, Bio-Detection Technologies, where he is the lead scientist for the development of Argonne's biochip portfolio. In this role, he is leading the development of nucleic acid and protein array applications. Current projects include the development of a high-resolution biomolecular characterization platform, a bovine mastitis diagnostic, cancer biomarker

  14. Daniel J. Schell | Bioenergy | NREL

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

    J. Schell Daniel J. Schell Manager, BioProcess Integration R&D Dan.Schell@nrel.gov | 303-384-6869 Research Interests Daniel J. Schell is manager of the BioProcess Integration R&D section of the National Bioenergy Center at the National Renewable Energy Laboratory (NREL) and currently leads a multidisciplinary team of engineers and pilot plant technicians. Schell has more than 30 years of research experience in bio-based conversion of lignocellulosic biomass and has extensive expertise in

  15. Midland reactor pressure vessel flaw distribution

    SciTech Connect (OSTI)

    Foulds, J.R.; Kennedy, E.L.; Rosinski, S.T.

    1993-12-01

    The results of laboratory nondestructive examination (NDE), and destructive cross-sectioning of selected weldment sections of the Midland reactor pressure vessel were analyzed per a previously developed methodology in order to develop a flaw distribution. The flaw distributions developed from the NDE results obtained by two different ultrasonic test (UT) inspections (Electric Power Research Institute NDE Center and Pacific Northwest Laboratories) were not statistically significantly different. However, the distribution developed from the NDE Center`s (destructive) cross-sectioning-based data was found to be significantly different than those obtained through the UT inspections. A fracture mechanics-based comparison of the flaw distributions showed that the cross-sectioning-based data, conservatively interpreted (all defects considered as flaws), gave a significantly lower vessel failure probability when compared with the failure probability values obtained using the UT-based distributions. Given that the cross-sectioning data were reportedly biased toward larger, more significant-appearing (by UT) indications, it is concluded that the nondestructive examinations produced definitively conservative results. In addition to the Midland vessel inspection-related analyses, a set of twenty-seven numerical simulations, designed to provide a preliminary quantitative assessment of the accuracy of the flaw distribution method used here, were conducted. The calculations showed that, in more than half the cases, the analysis produced reasonably accurate predictions.

  16. Midland County, Michigan: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    is classified as ASHRAE 169-2006 Climate Zone Number 5 Climate Zone Subtype A. Registered Energy Companies in Midland County, Michigan Dow Chemical Co Dow Kokam LXE Places in...

  17. TO: Daniel Cohen Cc: John Cymbalsky

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

    4/2014 TO: Daniel Cohen Cc: John Cymbalsky RE: Ex Parte discussion of commercial fan and blower rulemaking On November 3rd, Jordan Doria, Manager of Stakeholder Engagement, Ingersoll Rand, convened a teleconference with John Cymbalsky and Daniel Cohen of DOE. The purpose of the discussion was to address issues pertaining to the ongoing commercial and industrial fan and blower rulemaking as they impact Ingersoll Rand's Trane products. Jordan updated John and Daniel on the impacts of the rule on

  18. Daniel Yates Advisor: Dr. Rogachev Texas...

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

    gas mixtures for active target detector application Daniel Yates Advisor: Dr. Rogachev Texas Active Target (TexAT) New active target detector under development by Rogachev...

  19. Daniel, Utah: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Daniel, Utah: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.4707885, -111.4146275 Show Map Loading map... "minzoom":false,"mappingservice"...

  20. Daniel Lee Cloyd named Counterintelligence Office

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

    FBI officer accepts LANL counterintelligence post November 10, 2010 Daniel Lee Cloyd named ... Cloyd brings to Los Alamos 25 years of FBI experience in counterintelligence (including ...

  1. Gamesa and Daniel Alonso Group JV | Open Energy Information

    Open Energy Info (EERE)

    and Daniel Alonso Group JV Jump to: navigation, search Name: Gamesa and Daniel Alonso Group JV Place: Spain Sector: Wind energy Product: A JV between Gamesa and Daniel Alonso Group...

  2. QER- Comment of Daniel Dibble

    Broader source: Energy.gov [DOE]

    Happy Earth Day! 40 + years and the best our leaders (?) can come up with is MORE PIPELINES?! Come on, this is the same "forward thinking" that lost Detroit the race for the new car market. We, in New England are not yet heavily invested in gas infrastructure, so we can be positioned for the new forms of renewable, sustainable energy. It is so sad to think that government agencies are so heavily invested in (or is it that they are so heavily invested in by) old forms of energy that there is NO innovation and we are going to once again have to play catch up, to say nothing of the harm we are doing to the earth we will pass on to our children and grandchildren. Rev Daniel Dibble

  3. Daniel Beat Mller, Norwegian University of Science and Technology...

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

    Daniel Beat Mller, Norwegian University of Science and Technology, Material Flow Analysis Daniel Beat Mller, Norwegian University of Science and Technology, Material Flow...

  4. Memorandum from Daniel B. Poneman dated August 27, 2010, Strategic...

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

    Daniel B. Poneman dated August 27, 2010, Strategic Business Initiatives Memorandum from Daniel B. Poneman dated August 27, 2010, Strategic Business Initiatives Dep Sec Memo ...

  5. Daniel Lee Cloyd named Counterintelligence Office

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

    FBI officer accepts LANL counterintelligence post November 10, 2010 Daniel Lee Cloyd named Counterintelligence Office leader LOS ALAMOS, New Mexico, November 10, 2010-Daniel Lee Cloyd has been named as leader of the Laboratory's Office of Counterintelligence starting January 2011. Cloyd has most recently served as assistant director of the Counterintelligence Division of the Federal Bureau of Investigation headquarters. Cloyd brings to Los Alamos 25 years of FBI experience in counterintelligence

  6. DOE - Office of Legacy Management -- Dow Chemical Co - Midland - MI 06

    Office of Legacy Management (LM)

    Midland - MI 06 FUSRAP Considered Sites Site: Dow Chemical Co. - Midland (MI.06 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Midland , Michigan MI.06-1 Evaluation Year: Circa 1987 MI.06-2 Site Operations: Conducted development work for production of magnesium-thorium alloys. MI.06-1 Site Disposition: Eliminated - AEC licensed site MI.06-1 MI.06-2 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled:

  7. Science in St. Louis featuring Dr. Daniel Giammar | Photosynthetic...

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

    Daniel Giammar Science in St. Louis featuring Dr. Daniel Giammar The Chemistry and Engineering for Producing and Supplying Clean Drinking Water November 22, 2014 - 10:30am Brauer...

  8. Preliminary Notice of Violation, Fluor Daniel Fernald Corporation...

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

    Fernald Corporation - EA-97-05 Preliminary Notice of Violation, Fluor Daniel Fernald Corporation - EA-97-05 July 29, 1997 Issued to Fluor Daniel Fernald Corporation related to...

  9. NREL: Photovoltaics Research - Daniel J. Friedman, Ph.D.

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

    303-384-6472 daniel.friedman@nrel.gov Dr. Daniel Friedman is the manager of the High Efficiency Crystalline Photovoltaics Group. He received his doctorate in applied physics...

  10. Daniel Hoag Named Y-12 Site Office Deputy Manager | National...

    National Nuclear Security Administration (NNSA)

    Home Field Offices Welcome to the NNSA Production Office NPO News Releases Daniel Hoag Named Y-12 Site Office Deputy Manager Daniel Hoag Named Y-12 Site Office Deputy...

  11. Daniel Mieritz | Center for Bio-Inspired Solar Fuel Production

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

    Daniel Mieritz Graduate student Subtask 5 project: "Transparent, Mesoporous Zr(1-x)Ti(x)O2 Thin Films

  12. Enforcement Letter, Fluor Daniel Hanford, Inc- July 31, 1998

    Broader source: Energy.gov [DOE]

    Issued to Fluor Daniel Hanford, Inc., related to Incomplete Corrective Actions at the Hanford Site, July 31, 1998

  13. Enforcement Letter, Fluor Daniel Hanford, Inc.- July 7, 1997

    Broader source: Energy.gov [DOE]

    Issued to Fluor Daniel Hanford, Inc., related to Potential Quality Assurance Rule Violations at the Hanford Site

  14. Secretary Moniz Hosts Energy Security Symposium, Honors Dr. Daniel Yergin

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

    with First James R. Schlesinger Medal for Energy Security | Department of Energy Hosts Energy Security Symposium, Honors Dr. Daniel Yergin with First James R. Schlesinger Medal for Energy Security Secretary Moniz Hosts Energy Security Symposium, Honors Dr. Daniel Yergin with First James R. Schlesinger Medal for Energy Security October 1, 2014 - 11:00am Addthis News Media Contact 202-586-4940 Secretary Moniz Hosts Energy Security Symposium, Honors Dr. Daniel Yergin with First James R.

  15. Senate Confirms DOE Nominees Daniel Poneman, David Sandalow, Kristina

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

    Johnson, Steve Koonin, Scott Harris, and Ines Triay | Department of Energy Confirms DOE Nominees Daniel Poneman, David Sandalow, Kristina Johnson, Steve Koonin, Scott Harris, and Ines Triay Senate Confirms DOE Nominees Daniel Poneman, David Sandalow, Kristina Johnson, Steve Koonin, Scott Harris, and Ines Triay May 21, 2009 - 12:00am Addthis WASHINGTON, D.C. -- This week, the Senate confirmed six DOE nominees, including Deputy Secretary Daniel Poneman, Under Secretary for Energy Kristina

  16. The Honorable Harold Rogers The Honorable Daniel K. Inouye

    Office of Environmental Management (EM)

    Washington, DC 20585 (enter date here, centered) The Honorable Harold Rogers The Honorable Daniel K. Inouye Chairman, Committee on Appropriations Chairman, Committee on...

  17. Daniels County, Montana: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Daniels County, Montana: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 48.7744137, -105.7248763 Show Map Loading map... "minzoom":false,"mapp...

  18. 10 Questions with Author and Energy Expert Daniel Yergin | Department...

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

    Addthis Secretary Moniz presents the first ever James Schlesinger Medal for Energy Security to Dr. Daniel Yergin. | Photo Courtesy of the Energy Department. Secretary Moniz ...

  19. Daniel Cohen Assistant General Counsel for Legislation and Regulatory...

    Energy Savers [EERE]

    2, 2014 Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law Office of the General Counsel Department of Energy 1000 Independence Avenue, SW Washington, DC ...

  20. Daniel Cohen Assistant General Counsel for Legislation and Regulatory...

    Energy Savers [EERE]

    Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law Office of the General Counsel Department of Energy 1000 Independence Avenue, SW Washington, DC 20585-0121 ...

  1. Employment Impacts of Geothermal Electric Projects Entingh, Daniel...

    Office of Scientific and Technical Information (OSTI)

    Employment Impacts of Geothermal Electric Projects Entingh, Daniel J. 15 GEOTHERMAL ENERGY; 24 POWER TRANSMISSION AND DISTRIBUTION; CAPITAL; CONSTRUCTION; EMPLOYMENT; EXPLORATION;...

  2. WIPP transportation exercise to test emergency response capablities for Midland-Odessa

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

    Transportation Exercise to Test Emergency Response Capabilities for Midland-Odessa CARLSBAD, N.M., January 10, 2000 - Emergency response agencies from Midland and Odessa, Texas, will take part in a 1 p.m. (CST) training exercise Jan. 12 at the Ector County Coliseum. The graded exercise will help agencies determine whether emergency personnel are prepared to respond to a possible accident involving a shipment of transuranic radioactive waste headed for the U.S. Department of Energy's (DOE) Waste

  3. Microsoft Word - DOE-ID-11-016 Midlands EC.doc

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

    6 SECTION A. Project Title: Nuclear Infrastructure Upgrade to Enhance Teaching Capabilities in the Nuclear Systems Technology Program at Midlands Technical College SECTION B. Project Description Midlands Technical College will purchase a metallographic microscope and imaging workstation to allow students to perform structural defect analysis is simulated radiation-damaged, thermal shocked, and stress and corrosion damaged materials, as well as evaluate other surface properties of materials.

  4. Pre-Leonardian geology of Midland Farms field area, Andrews County, Texas

    SciTech Connect (OSTI)

    Mear, C.E.; Dufurrena, C.K.

    1984-01-01

    The Midland Farms (Ellenburger) oil field was discovered on September 16, 1952, with the completion of Anderson-Pritchard's 1 Fasken-24 well, drilled on an indicated single-fold seismic structure. The field produces from vuggy, fractured Ellenburger dolomite with up to 310 ft (94 m) of gross and net pay. The Midland Farms (Ellenburger) field is part of a larger structure which incorporates not only Midland Farms field, but Midland Farms, West (Devonian), Inez (Ellenburger), and parts of the Fasken (Penn) and Block 41 (Wolfcamp) fields. The structure is a complex, uplifted block composed of two doubly plunging, asymmetric anticlines bisected by at least one wrench-type fault and several normal faults. Penecontemporaneous leaching produced oomoldic porosity in the limestones. Ellenburger oil production was established in the Midland Farms area in September 1952, and has amounted to 61.6 million bbl oil and 28.5 bcf of gas from 91 wells to January 1983. Major Fusselman and Wolfcamp oil accumulations were discovered during development of the Ellenburger field. Fusselman oil was first produced in June 1953, and has totaled 10.1 million bbl of oil and 5 bcf of gas from 33 wells to January 1983. Wolfcamp production was established in January 1954 and totals 10.7 million bbl of oil and 1 bcf of gas from 39 wells. Total production from all zones including post-Leonard beds in the Midland Farms field area to date has been 210 million bbl of oil and 84 bcf of gas.

  5. Hamiltonian model Gamel, Omar; James, Daniel F. V. [Department...

    Office of Scientific and Technical Information (OSTI)

    of the effective Hamiltonian model Gamel, Omar; James, Daniel F. V. Department of Physics, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 1A7 (Canada) 71...

  6. Daniel Wright Junior High School Wins First Place In Hydrogen...

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

    Daniel Wright Junior High School Wins First Place In Hydrogen Fuel Cell Car Contest National "Battle of the Brains" continues June 23-24 at the University of Denver June 23, 2006 ...

  7. VWC-0001- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This case involves a complaint filed by Daniel Holsinger (Holsinger) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The matter comes before me...

  8. VWC-0002- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This case involves a complaint filed by Daniel Holsinger (Holsinger) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. The matter comes before me...

  9. Fluor Daniel Hanford contract standards/requirements identification document

    SciTech Connect (OSTI)

    Bennett, G.L.

    1997-04-24

    This document, the Standards/Requirements Identification Document (S/RID) for the Fluor Daniel Hanford Contract, represents the necessary and sufficient requirements to provide an adequate level of protection of the worker, public health and safety, and the environment.

  10. VWA-0005- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This Decision involves a complaint filed by Daniel L. Holsinger (Holsinger) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. In his complaint,...

  11. Saluting Daniel Poneman's Service to the Department of Energy

    Broader source: Energy.gov [DOE]

    On October 2, 2014, the Energy Department honored Daniel Poneman, the longest-serving Deputy Secretary of Energy in American history. Check out our photo gallery to see highlights from Poneman's tenure.

  12. Saluting Daniel Poneman's Service to the Department of Energy

    Broader source: Energy.gov [DOE]

    The Energy Department is saying farewell to Daniel Poneman, the longest-serving Deputy Secretary of Energy in American history. Check out a photo gallery to see highlights from Poneman's tenure.

  13. VBZ-0005- In the Matter of Fluor Daniel Fernald

    Broader source: Energy.gov [DOE]

    This decision will consider a Motion to Dismiss Fluor Daniel Fernald (FDF) filed on September 7, 1999. FDF moves to dismiss a Complaint filed by Thomas W. Dwyer under the Department of Energy's ...

  14. Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law

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

    Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law Office of the General Counsel Department of Energy 1000 Independence Avenue, SW Washington, DC 20585-0121 Re: Ex Parte Memorandum Dear Mr. Cohen: On Tuesday, May 4, 2010, Kit Kennedy and Kate Houren of the Natural Resources Defense Council (NRDC) initiated a telephone call with Daniel Cohen and Bryan Miller of the Department of Energy's Office of the General Council. During the call, NRDC advocated for the adoption of the

  15. IA Experts Listing 2014 | Department of Energy

    Energy Savers [EERE]

    IA Experts Listing 2014 IA Experts Listing 2014 PDF icon IA Experts Listing January 2014 More Documents & Publications Office of International Affairs Organization Chart PI...

  16. Rolling Hills (IA) | Open Energy Information

    Open Energy Info (EERE)

    Rolling Hills (IA) Jump to: navigation, search Name Rolling Hills (IA) Facility Rolling Hills (IA) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service...

  17. Steamboat IA Geothermal Facility | Open Energy Information

    Open Energy Info (EERE)

    IA Geothermal Facility Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Steamboat IA Geothermal Facility General Information Name Steamboat IA Geothermal Facility...

  18. DOE Zero Energy Ready Home Case Study: Cobblestone Homes, Midland, MI

    Broader source: Energy.gov [DOE]

    Case study of a DOE Zero Energy Ready home in Midland, MI, that scored HERS 49 without PV or HERS 44 with 1.4 kW of PV. The custom home served as a prototype and energy efficiency demonstration...

  19. Deputy Secretary Daniel Poneman's Remarks to the Washington Institute for

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

    Near East Policy | Department of Energy to the Washington Institute for Near East Policy Deputy Secretary Daniel Poneman's Remarks to the Washington Institute for Near East Policy March 17, 2010 - 1:04pm Addthis U.S. Deputy Secretary of Energy Daniel Poneman Remarks as Prepared for Delivery Washington Institute for Near East Policy Washington, D.C. March 17, 2010 Good afternoon. I would like to thank Rob Satloff and the Washington Institute for inviting me to speak with you today. For 25

  20. Deputy Secretary Daniel Poneman USA Today Op-Ed September 13...

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

    Deputy Secretary Daniel Poneman USA Today Op-Ed September 13, 2011 Deputy Secretary Daniel Poneman USA Today Op-Ed September 13, 2011 PDF icon 091411Poneman USA Today op-ed.pdf...

  1. Daniel Hoag Named NNSA Production Office Deputy Manager | National Nuclear

    National Nuclear Security Administration (NNSA)

    Security Administration | (NNSA) NNSA Production Office Deputy Manager July 20, 2012 OAK RIDGE, Tenn. - Daniel Hoag has been named deputy manager for the National Nuclear Security Administration's Production Office (NPO) that was established in June to provide federal oversight of nuclear production missions at the Pantex Plant in Amarillo, Texas, and the Y-12 National Security Complex in Oak Ridge, Tennessee. File 2012-07-20 Hoag NPO Deputy Manager.docx

  2. Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law

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

    2, 2014 Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law Office of the General Counsel Department of Energy 1000 Independence Avenue, SW Washington, DC 20585-0121 Re: Ex Parte Communication following meeting between DOE and the National Marine Manufacturers Association At 2 p.m. ET on Wednesday, May 7 2014 the National Marine Manufacturers Association (NMMA) along with representatives from three of its member organizations met with Jeremy Dommu of the Department of

  3. From: CELIA DANIELS To: Congestion Study Comments Subject:

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

    CELIA DANIELS To: Congestion Study Comments Subject: NIETC comment Date: Friday, September 19, 2014 2:25:17 PM Greetings: I would like to express my opposition to the establishment of National Interest Energy Transmission Corridors (NIETC's) for the following reasons. First and foremost, the same landowners should not have to endure the problems and hazards of the construction of transmission lines on their land again and again. We have suffered through the building of three pipelines on our

  4. Daniel A. Ruddy, Ph.D. | Bioenergy | NREL

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

    A. Ruddy Daniel A. Ruddy, Ph.D. Inorganic and Materials Chemist, Senior Scientist Dan.Ruddy@nrel.gov | 303-384-6322 Research Interests Inorganic chemistry and catalysis New synthetic pathways to functional materials Renewable fuels production and processes Biomass conversion catalysis Areas of Expertise Dan received a Ph.D. degree in Inorganic Chemistry from the University of California, Berkeley in 2008. His doctoral research combined synthetic molecular and materials chemistry with detailed

  5. Deputy Secretary Daniel Poneman's Remarks at IFNEC Meeting in Warsaw,

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

    Poland - As Prepared for Delivery | Department of Energy IFNEC Meeting in Warsaw, Poland - As Prepared for Delivery Deputy Secretary Daniel Poneman's Remarks at IFNEC Meeting in Warsaw, Poland - As Prepared for Delivery September 29, 2011 - 12:00pm Addthis Thank you, Madame Chairwoman Trojanowska. On behalf of the United States government, I would like to extend my sincere appreciation to the Government of Poland for hosting and chairing the 2011 International Framework for Nuclear Energy

  6. Evolution of Permian carbonate shelf and foreshelf detrital systems, Midland basin, Texas

    SciTech Connect (OSTI)

    Mazzullo, S.J.; Reid, A.M. II; Reid, S.T.

    1986-03-01

    A major phase of shelf progradation and consequent filling of the Midland basin began in the Early Permian. Prior to this time, shelf carbonate systems were mostly ineffective in generating coarse detritus in quantities sufficient to infill adjoining basins. Beginning in the Early Permian (Wolfcampian), however, the character of shelf and basin deposition was abruptly modified, in part because of faunal changes - proliferation of rock-forming biotic communities and the consequent potential for rapid shelf-marginal oversteepening - and the effects of sea level fluctuations and periods of shale influx. Shelf systems in the northern Midland basin and Eastern shelf evolved from ramps in the lowermost Wolfcamp to steep rimmed platforms by the lower Leonard. Shelf progradation into the Midland basin was cyclic, with extensive carbonate shelves having developed during sea level highstands and massive shale wedges deposited during alternate lowstands. Coarse megabreccia with markedly little sand dominates in the lower to middle Wolfcamp systems, despite the occurrence of ramps in this section. Such an anomaly can be explained by invoking widespread shelf wastage caused by the inherent instability and failure of the shale slopes on which these ramps were deposited. In certain middle Wolfcamp zones, thin shelf-ramp sections may be recognized only because any thick shelf-marginal buildups that may have been present have been displaced into adjoining basinal tracts. The evolution to rimmed-platform shelves by the lower Leonard strata, foreshelf debris occurs mostly as complexes of megabreccia wedges and aprons, anastomosing megabreccia, and sand-channel and lobe deposits derived from adjoining rimmed-platforms. Major variations exist in the gross geometries of foreshelf units and component reservoirs even laterally within rocks of the same age.

  7. DOE Zero Ready Home Case Study: Cobblestone Homes, 2014 Model Home, Midland, MI

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

    Cobblestone Homes 2014 Model Home Midland, MI DOE ZERO ENERGY READY HOME(tm) The U.S. Department of Energy invites home builders across the country to meet the extraordinary levels of excellence and quality specified in DOE's Zero Energy Ready Home program (formerly known as Challenge Home). Every DOE Zero Energy Ready Home starts with ENERGY STAR Certified Homes Version 3.0 for an energy-efficient home built on a solid foundation of building science research. Advanced technologies are designed

  8. Dark Energy and Cosmic Sound Daniel Eisenstein Harvard University

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

    Dark Energy and Cosmic Sound Daniel Eisenstein Harvard University May 27, 2015 4:00 p.m. (coffee @ 3:30) Discuss how the acoustic oscillations that propagate in the photon- baryon fluid during the first million years of the Universe provide a robust method for measuring the cosmological distance scale. The distance that the sound can travel can be computed to high precision and creates a signature in the late-time clustering of matter that serves as a standard ruler. Galaxy clustering results

  9. Clifton Truman Daniel's visit to Oak Ridge and Y-12, part 2

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

    2 President Harry S. Truman's grandson, Clifton Truman Daniel, after visiting Japan to attend an anniversary of the bombing of Hiroshima and Nagasaki, recently visited Oak Ridge to...

  10. Preliminary Notice of Violation, Fluor Daniel Fernald Corporation- EA-97-05

    Broader source: Energy.gov [DOE]

    Issued to Fluor Daniel Fernald Corporation related to Corrective Actions Implementation Deficiencies at the Fernald Environmental Management Project, (EA-97-05)

  11. Daniel Hoag Named Y-12 Site Office Deputy Manager | National Nuclear

    National Nuclear Security Administration (NNSA)

    Security Administration | (NNSA) Y-12 Site Office Deputy Manager March 23, 2011 Daniel hoag named y-12 site office deputy manager. OAK RIDGE, Tenn. -- Daniel K. Hoag has been named Deputy Manager for the National Nuclear Security Administration's Y-12 Site Office (YSO). Microsoft Office document icon NR-03-23.doc

  12. Characterization of bedded salt for storage caverns -- A case study from the Midland Basin, Texas

    SciTech Connect (OSTI)

    Hovorka, Susan D.; Nava, Robin

    2000-06-13

    The geometry of Permian bedding salt in the Midland Basin is a product of interaction between depositional facies and postdepositional modification by salt dissolution. Mapping high-frequency cycle patterns in cross section and map view using wireline logs documents the salt geometry. Geologically based interpretation of depositional and dissolution processes provides a powerful tool for mapping and geometry of salt to assess the suitability of sites for development of solution-mined storage caverns. In addition, this process-based description of salt geometry complements existing data about the evolution of one of the best-known sedimentary basins in the world, and can serve as a genetic model to assist in interpreting other salts.

  13. Category:Mason, IA | Open Energy Information

    Open Energy Info (EERE)

    Mason, IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Mason, IA" The following 16 files are in this category, out of 16 total....

  14. Defining photometric peculiar type Ia supernovae

    SciTech Connect (OSTI)

    González-Gaitán, S.; Pignata, G.; Förster, F.; Gutiérrez, C. P.; Bufano, F.; Galbany, L.; Hamuy, M.; De Jaeger, T.; Hsiao, E. Y.; Phillips, M. M.; Folatelli, G.; Anderson, J. P.

    2014-11-10

    We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e., objects with light curve characteristics such as later primary maxima and the absence of a secondary peak in redder filters. This method is capable of selecting this sub-group from the normal type Ia population. Furthermore, we find that recently identified peculiar sub-types such as SNe Iax and super-Chandrasekhar SNe Ia have photometric characteristics similar to 91bg-like SNe Ia, namely, the absence of secondary maxima and shoulders at longer wavelengths, and can also be classified with our technique. The similarity of these different SN Ia sub-groups perhaps suggests common physical conditions. This typing methodology permits the photometric identification of peculiar SNe Ia in large upcoming wide-field surveys either to study them further or to obtain a pure sample of normal SNe Ia for cosmological studies.

  15. IA News Archive | Department of Energy

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

    17, 2012 Deputy Secretary Poneman Statement on Second Meeting of the U.S. - South Africa Bilateral Energy Dialogue U.S. Deputy Secretary of Energy Daniel Poneman and South...

  16. Remarks from Congressional Leaders: Congressman Daniel Lipinski (2011 EFRC Summit)

    ScienceCinema (OSTI)

    Lipinski, Daniel (Congressman, Illinois)

    2012-03-14

    Congressman Daniel Lipinski (D-Illinois) spoke during the opening session of the EFRC Summit. The 2011 EFRC Summit and Forum brought together the EFRC community and science and policy leaders from universities, national laboratories, industry and government to discuss "Science for our Nation's Energy Future." In August 2009, the Office of Science established 46 Energy Frontier Research Centers. The EFRCs are collaborative research efforts intended to accelerate high-risk, high-reward fundamental research, the scientific basis for transformative energy technologies of the future. These Centers involve universities, national laboratories, nonprofit organizations, and for-profit firms, singly or in partnerships, selected by scientific peer review. They are funded at $2 to $5 million per year for a total planned DOE commitment of $777 million over the initial five-year award period, pending Congressional appropriations. These integrated, multi-investigator Centers are conducting fundamental research focusing on one or more of several ?grand challenges? and use-inspired ?basic research needs? recently identified in major strategic planning efforts by the scientific community. The purpose of the EFRCs is to integrate the talents and expertise of leading scientists in a setting designed to accelerate research that transforms the future of energy and the environment.

  17. transport Lau, Hoi-Kwan; James, Daniel F. V. [Department of Physics...

    Office of Scientific and Technical Information (OSTI)

    Stark effect in rapid ion transport Lau, Hoi-Kwan; James, Daniel F. V. Department of Physics, University of Toronto, 60 Saint George Street, Toronto, M5S 1A7 Ontario (Canada) 71...

  18. FIA-13-0075- In the Matter of Daniel W. McKeel, Jr.

    Broader source: Energy.gov [DOE]

    On December 23, 2013, the Department of Energy’s (DOE) Office of Hearings and Appeals (OHA) denied a Freedom of Information Act (FOIA) Appeal filed by Daniel W. McKeel, Jr., (Appellant) of a...

  19. Microsoft PowerPoint - Fukushima_perspectives from FRMAC_Daniel...

    National Nuclear Security Administration (NNSA)

    Response to Radiological Releases from the Fukushima Dai-ichi Nuclear Power Plant Daniel Blumenthal, PhD, CHP Manager, Consequence Management Program U.S. Department of Energy ...

  20. Preliminary Notice of Violation, Fluor Daniel Hanford Company- EA-98-02

    Broader source: Energy.gov [DOE]

    Issued to Fluor Daniel Hanford Company, related to Criticality Safety Infractions, Radiological Control Violations, and an Explosion at the Plutonium Finishing Plant at the Hanford Site, (EA-98-02)

  1. Memorandum from Daniel B. Poneman dated August 27, 2010, Strategic Business

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

    Initiatives | Department of Energy Daniel B. Poneman dated August 27, 2010, Strategic Business Initiatives Memorandum from Daniel B. Poneman dated August 27, 2010, Strategic Business Initiatives Dep Sec Memo 082710.pdf (45.83 KB) More Documents & Publications Policy Flash 2015-10 Improving Capital Assets Project Documentation Letter from Deputy Secretary Poneman to Clean Line Energy Regarding the Plains & Eastern Clean Line Project Under Section 1222 of EPAct 2005 (April 5, 2012

  2. Establish and Operate a Geologic Core and Sample Repository in Midland, Texas

    SciTech Connect (OSTI)

    Tyler, Noel

    2000-08-14

    Shell Oil Company donated its proprietary core and sample repository to the Bureau of Economic Geology, The University of Texas at Austin, in 1994. This collection of geologic materials is composed of 325,000 boxes of rocks and samples housed in a 32,700-ft{sup 2} warehouse in Midland, Texas. The material includes cores from more than 3,000 wells (75,000 boxes) and cuttings from more than 90,000 wells (260,000 boxes). In addition to the warehouse space, the repository consists of layout rooms, a processing room, and office space. The U.S. Department of Energy provided $375,000 under Grant Number DE-FG22-94BC14854 for organizing the collection, staffing the facility, and making the material available to the public for the first 5 years of operation. Shell Oil Company provided an endowment of $1.3 million to cover the cost of operating the facility after the fifth year of operation.

  3. IA Blog Archive | Department of Energy

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

    Blog Archive IA Blog Archive RSS May 31, 2016 IA Blog Archive Global Energy Leaders Gather in California to Drive Clean Energy Development and Deployment Goal of meetings will be to expand international collaboration in clean energy research, development, demonstration and deployment to combat climate change. May 18, 2016 IA Blog Archive 10 Ways the Clean Energy Ministerial Is Speeding Up the World's Clean Energy Revolution The world needs a lot more clean energy, and fast. Here are 10 ways the

  4. The Spraberry trend, Midland basin, Texas: Development, innovation, and reserve growth potential in a mature giant

    SciTech Connect (OSTI)

    Guevara, E.H. ); Tyler, N. )

    1991-03-01

    The Spraberry trend area field is a stratigraphic trap about 60 mi long (N-S) and 40 mi wide (E-W) on a west-dipping monocline in the central Midland basin, west Texas. It contained 9,500 MMbls of in-place oil at discovery in 1949; recovery efficiency in these solution-gas-drive, originally underpressured reservoirs is projected to be 8%. There are more than 10,000 wells in the field, which, in the 1980s, was among the most intensely drilled areas in the nation. Wells are mostly at 160-ac and locally at 40-ac centers. Rapid production declines prompted local waterflooding. The Spraberry trend has been the experimental site of significant technological innovations, among them imbibition flooding, drilling using air, horizontal wells, and development of naturally fractured reservoirs. Main reservoirs occur in the Spraberry, Dean, and upper Wolfcamp formations (Lower Permian) at depths ranging from about 6,000 to 9,000 ft. They are naturally fractured, very fine-grained sandstones and siltstones in beds up to 14 ft thick, forming part of mid- to outer-fan, channel-fill and associated submarine-fan facies. Permeabilities average less than 1 md, and porosities are mostly less than 10%. Geochemical data suggest indigenous oils and short migration paths. Oils are paraffinic-naphthenic, light (36-40 API), and low in sulfur (0.17%). Entrapment is a product of reservoir pinch-out into slope and base-of-slope mud facies. Internal reservoir compartments result from channel-to-interchannel facies changes causing intrareservoir stratigraphic traps.

  5. Facies architecture of Spraberry submarine fan reservoirs (Permian), Midland basin, Texas

    SciTech Connect (OSTI)

    Guevara, E.H.; Tyler, N.

    1989-03-01

    Facies of mud-rich submarine fans of the Spraberry formation (Permian, Leonardian) form oil reservoirs in the central part of the Midland basin, west Texas. The principal reservoirs are submarine-channel and associated facies in the upper parts of generally upward-coarsening and upward-thickening sequences of the Jo Mill (lower Spraberry) and Driver and overlying Floyd (upper Spraberry) fans. They are naturally fractured, massive and laminated, very fine-grained, calcareous sandstones and siltstones usually occurring in beds 2 to approximately 12 ft thick. Two main subdivisions, inner and middle to outer fan, are recognized using isoliths, log motifs, and cores of predominantly terrigenous clastic, mostly basin-wide genetic intervals. The boundary between the subdivisions approximately coincides with the location of the subjacent Horseshoe atoll (Pennsylvanian). The narrow range in grain size of the fans results in limited basinward variations in texture and sedimentary structures and paucity of Bouma sequences. Facies architecture strongly influences hydrocarbon distribution and recovery. Wells having the best cumulative productions generally occur in sandstone depositional axes. Most accumulations in inner fan facies are scattered structural traps having relatively high recovery efficiencies (24%, Jo Mill field). The largest accumulations in mid to outer fan facies are stratigraphic traps in meandering to anastomosing channel sandstone belts 1-3 mi wide occurring in a widespread area. Recovery efficiencies range from 5% (Spraberry trend, stratigraphic trap) to 15% (Benedum field, combined stratigraphic-structural trap). Additional reserves can be recovered from partly drained and untapped reservoir compartments, especially in layered and compartmentalized middle to outer fan facies.

  6. Dolomitization of coeval shelf and fore-shelf carbonates, Lower Permian, Midland basin, Texas

    SciTech Connect (OSTI)

    Mazzullo, S.J.; Qiuchang, Ye )

    1991-03-01

    Coeval shelf and fore-shelf carbonates in Lower Permian (Leonardian) rocks in the Midland basin are pervasively dolomitized. Shelf strata consist of a regional mosaic of shelf margin reef, lagoon, and peritidal facies associated with contemporaneous evaporite deposition; fore-shelf facies consist of resedimented shelf margin deposits. Numerous relative sea-level fluctuations that resulted in the formation of Type 1 and 2 unconformities are recognized throughout this section. Mean stable oxygen and carbon isotopic compositions of the shelf strate suggest that dolomitization occurred essentially syndepositionally, likely by interaction with normal marine( ) and hypersaline fluids. In fore-shelf strata petrographic evidence, in combination with paleotemperature estimates from isotopic data and the burial depth-temperature history of these rocks, suggest relatively early (late Permian) dolomitization in rock-dominated systems. Three possible modes of dolomitization could have affected these fore-shelf beds: (1) dolomitization by reflux of normal-marine and/or hypersaline fluids during sea level highstands or lowstands; (2) dolomitization by mixed meteoric-marine fluids during lowstands; and (3) replacement by calcic dolomites via reaction with circulating marine fluids during deposition and early, shallow burial without organic matter influences. The latter mode of origin, however, is favored for most of the rocks examined on the basis of the slightly positive carbon isotopic compositions, Sr versus MgCO{sub 3} compositions (mean Sr 61 ppm, mean MgCO{sub 3} 49.5), and low Mn contents (mean 61 ppm) of the dolomites, although later burial recrystallization is indicated by their relatively depleted isotopic compositions.

  7. Deputy Secretary Daniel Poneman’s Remarks to the International Forum for a Nuclear Weapons-Free World

    Office of Energy Efficiency and Renewable Energy (EERE)

    Please find below Deputy Secretary Daniel Poneman’s remarks, as prepared for delivery, to the International Forum for a Nuclear Weapons-Free World in Astana, Kazakhstan.

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

    Office of Legacy Management (LM)

    Titus Metals - IA 04 FUSRAP Considered Sites Site: TITUS METALS ( IA.04 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Waterloo , Iowa IA.04-1 Evaluation Year: 1987 IA.04-2 Site Operations: Extruded uranium billets to produce fuel plates for the Argonaut reactor in June, 1956. IA.04-1 IA.04-2 Site Disposition: Eliminated - Potential for contamination considered remote based on the limited scope of activities at the site and results of

  9. New approaches for modeling type Ia supernovae (Conference) ...

    Office of Scientific and Technical Information (OSTI)

    Type Ia supernovae (SNe Ia) are the largest thermonuclearexplosions in the Universe. Their light output can be seen across greatstances and has led to the discovery that the ...

  10. ASTRONOMY AND ASTROPHYSICS Dark Energy, Type Ia supernovae, radiative

    Office of Scientific and Technical Information (OSTI)

    of Oklahoma Univ. of Oklahoma 79 ASTRONOMY AND ASTROPHYSICS Dark Energy, Type Ia supernovae, radiative transfer, Dark Energy, Type Ia supernovae, radiative transfer, The...

  11. Constraining Cosmic Evolution of Type Ia Supernovae (Journal...

    Office of Scientific and Technical Information (OSTI)

    Constraining Cosmic Evolution of Type Ia Supernovae Citation Details In-Document Search Title: Constraining Cosmic Evolution of Type Ia Supernovae We present the first large-scale...

  12. Geological characterization of permian submarine fan reservoirs of the driver waterflood unit, Spraberry Trend, Midland Basin, Texas

    SciTech Connect (OSTI)

    Guevara, E.H.

    1989-01-01

    This book discusses the geological characterization and assessment of the relationship between reservoir stratigraphy and oil recovery of the Driver waterflood unit of the Spraberry Trend, Midland Basin, West Texas. In this study , the author focuses on the Driver waterflood unit, which is located in Midland, Glasscock, Upton, and Reagan Counties and is part of the giant Spraberry Trend currently being studied by the Bureau. Gamma-ray logs and scout cards from more than 350 wells and slabbed cores from 2 wells, along with core analyses and production data, provided the main sources of information for the study. Fifteen log-defined genetic-stratigraphic operational units were delineated in the Spraberry Formation and were correlated throughout the study area to define the stratigraphic framework. The text presents net sandstone and siltstone maps, cross sections, depth plots of core analyses, and maps of production data. The author describes the depositional systems and hydrocarbon distribution in the Driver unit (currently operated by Standard Oil), details the influence of reservoir stratigraphy on oil recovery, and outlines opportunities for additional recovery. He notes that reservoir management strategies must take into account the stratigraphic heterogeneities of accumulations in the unit. He concludes that a program of selective recompletions and infill drilling based on knowledge of both reservoir stratigraphy and natural fractures is the key to improving oil recovery from the Driver unit in particular and from the Spraberry Trend in general.

  13. OSTIblog Posts by Cathey Daniels | OSTI, US Dept of Energy Office of

    Office of Scientific and Technical Information (OSTI)

    Scientific and Technical Information Cathey Daniels Cathey Daniels's picture Program Manager, Information International Associates, Inc. It's been a big summer for sharing science info--and it's still only June! 1535 OSTINewsIcon.jpg It's been a big summer for sharing science info--and it's still only June! Read more about 1535 Products and Content Published on Jun 30, 2009 Did you know: That now you can find research from China when you search within WorldWideScience.org? OSTI was in Ottawa

  14. Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel Poneman

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

    Announce Results of Pilot Project on Home Energy Use | Department of Energy Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel Poneman Announce Results of Pilot Project on Home Energy Use Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel Poneman Announce Results of Pilot Project on Home Energy Use July 26, 2011 - 3:10pm Addthis Houston, TX - CenterPoint Energy, Inc.'s (NYSE:CNP) electric transmission and distribution subsidiary, CenterPoint Energy Houston Electric, LLC

  15. Type Ia Supernovae Project at NERSC

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

    of star called a white dwarf. The majority of SN Ia explosions occur far away from our galaxy; yet, due to their enormous intrinsic brightness, outshining billions of stars, we can...

  16. IA Blog Archive | Department of Energy

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

    "always be five years away." For four key clean energy technologies, that clean energy future has already arrived. August 21, 2013 IA Blog Archive ActOnClimate: Secretary...

  17. Sequence stratigraphic framework and exploration potential of lower Permian (Wolfcampian) gravity-flow deposits, eastern Midland Basin, Texas

    SciTech Connect (OSTI)

    Morgan, W.A.; Clopine, W.W. ); Kokkoros, G.F.; Wiley, B.H. )

    1996-01-01

    Eight major Wolfcampian sequences (W1-W8) have been identified on seismic data and well logs in a 1500 square mile study area along the Eastern Shelf of the Midland Basin. These sequences compose two lower frequency sequences (W1-W5 W6-W8) which are separated by a major erosional surface associated with a sea-level fall near the time of the early-middle Wolfcampian boundary. Sea-level falls associated with sequences W5 and W6 resulted in significant erosion of platform-margin deposits, incision of a submarine canyon several miles into the Eastern Shelf, and deposition of carbonate gravity flows in the Midland Basin. Gravity flows entered the basin via the submarine canyon and fed basin-floor fan systems which extend up to 25 miles basinward of the toe-of-slope. Within the study area, production from carbonate gravity-flow deposits is mostly from three submarine fan systems within sequences W5 and W6 - the Credo (10 MMBOER) fan (oldest) , the Triple M (5 MMBOER)-Howard Glasscock (7 MMBOER) fan, and the Hutto (5 MMBOER) fan (youngest). The maximum gross thickness of the fans ranges from 100 to 200 feet. Regional isolith and seismic amplitude data were used to high-grade a 70 square mile area in the vicinity of Triple M and Howard Glasscock fields. Model-based velocity inversions, constrained by sonic and density data from 52 wells, were performed utilizing a grid of 2-D seismic data and a 3-D survey. Both Triple M and Howard Glasscock fields are clearly defined by high-velocity anomalies within the productive basin-floor fan interval of sequence W6. An untested high-velocity anomaly with a velocity signature and stratal geometry similar to the two fields, and estimated reserves of 5 MMBOER, is scheduled to be drilled in 1995.

  18. Sequence stratigraphic framework and exploration potential of lower Permian (Wolfcampian) gravity-flow deposits, eastern Midland Basin, Texas

    SciTech Connect (OSTI)

    Morgan, W.A.; Clopine, W.W.; Kokkoros, G.F.; Wiley, B.H.

    1996-12-31

    Eight major Wolfcampian sequences (W1-W8) have been identified on seismic data and well logs in a 1500 square mile study area along the Eastern Shelf of the Midland Basin. These sequences compose two lower frequency sequences (W1-W5 & W6-W8) which are separated by a major erosional surface associated with a sea-level fall near the time of the early-middle Wolfcampian boundary. Sea-level falls associated with sequences W5 and W6 resulted in significant erosion of platform-margin deposits, incision of a submarine canyon several miles into the Eastern Shelf, and deposition of carbonate gravity flows in the Midland Basin. Gravity flows entered the basin via the submarine canyon and fed basin-floor fan systems which extend up to 25 miles basinward of the toe-of-slope. Within the study area, production from carbonate gravity-flow deposits is mostly from three submarine fan systems within sequences W5 and W6 - the Credo (10 MMBOER) fan (oldest) , the Triple M (5 MMBOER)-Howard Glasscock (7 MMBOER) fan, and the Hutto (5 MMBOER) fan (youngest). The maximum gross thickness of the fans ranges from 100 to 200 feet. Regional isolith and seismic amplitude data were used to high-grade a 70 square mile area in the vicinity of Triple M and Howard Glasscock fields. Model-based velocity inversions, constrained by sonic and density data from 52 wells, were performed utilizing a grid of 2-D seismic data and a 3-D survey. Both Triple M and Howard Glasscock fields are clearly defined by high-velocity anomalies within the productive basin-floor fan interval of sequence W6. An untested high-velocity anomaly with a velocity signature and stratal geometry similar to the two fields, and estimated reserves of 5 MMBOER, is scheduled to be drilled in 1995.

  19. To: Daniel Cohen, Assistant General Counsel for Legislation, Regulation, and Energy

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

    February 19, 2015 To: Daniel Cohen, Assistant General Counsel for Legislation, Regulation, and Energy Efficiency, DOE From: Amy Shepherd, General Counsel, AHRI Re: Ex Parte Communication On Friday, February 13, 2015, AHRI staff met telephonically with the Department of Energy to discuss issues pertaining to the ongoing efficiency standards rulemaking for single package vertical air-conditioning and single package vertical heat pump (collectively, SPVU) equipment. The purpose of the conversation

  20. By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency

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

    August 1, 2011 By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency U.S. Department of Energy Office of the General Counsel 1000 Independence Ave., SW Room 6A245 Washington, D.C. 20585 Regulatory.Review@hq.doe.gov Re: EO 13563 Preliminary Plan Dear Mr. Cohen: The Association of Home Appliance Manufacturers (AHAM) respectfully submits the following comments to the Department of Energy (DOE) on preliminary plan for retrospective analysis of existing

  1. By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency

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

    June 19, 2012 By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency U.S. Department of Energy Office of the General Counsel 1000 Independence Ave., SW Washington, D.C. 20585 Regulatory.Review@hq.doe.gov Re: Regulatory Burden RFI Dear Mr. Cohen: The Association of Home Appliance Manufacturers (AHAM) respectfully submits the following comments to the Department of Energy (DOE) on its Regulatory Burden RFI, 77 Fed. Reg. 28518 (May 15, 2012). AHAM

  2. By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency

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

    21, 2011 By E-Mail Daniel Cohen Assistant General Counsel for Legislation, Regulation, and Energy Efficiency U.S. Department of Energy Office of the General Counsel 1000 Independence Ave., SW Room 6A245 Washington, D.C. 20585 Regulatory.Review@hq.doe.gov Re: Regulatory Burden RFI Dear Mr. Cohen: The Association of Home Appliance Manufacturers (AHAM) respectfully submits the following comments to the Department of Energy (DOE) on its Request for Information on reducing regulatory burden, 76 Fed.

  3. Microsoft PowerPoint - Fukushima_perspectives from FRMAC_Daniel Blumenthal

    National Nuclear Security Administration (NNSA)

    Response to Radiological Releases from the Fukushima Dai-ichi Nuclear Power Plant Daniel Blumenthal, PhD, CHP Manager, Consequence Management Program U.S. Department of Energy National Nuclear Security Administration 2 2 Office of Emergency Response  Expert technical advice from the DOE/NNSA National Laboratories in response to:  Nuclear weapon accidents and incidents  Possible acts of nuclear terrorism  Lost or stolen radioactive materials  Radiological accidents  Expertise in

  4. Improved Distances to Type Ia Supernovae withMulticolor Light...

    Office of Scientific and Technical Information (OSTI)

    We present an updated version of the Multicolor Light Curve Shape method to measure distances to type Ia supernovae (SN Ia), incorporating new procedures for K-correction and ...

  5. Ideal bandpasses for type Ia supernova cosmology

    SciTech Connect (OSTI)

    Davis, Tamara M.; Schmidt, Brian P.; Kim, Alex G.

    2005-10-24

    To use type Ia supernovae as standard candles for cosmologywe need accurate broadband magnitudes. In practice the observed magnitudemay differ from the ideal magnitude-redshift relationship either throughintrinsic inhomogeneities in the type Ia supernova population or throughobservational error. Here we investigate how we can choose filterbandpasses to reduce the error caused by both these effects. We find thatbandpasses with large integral fluxes and sloping wings are best able tominimise several sources of observational error, and are also leastsensitive to intrinsic differences in type Ia supernovae. The mostimportant feature of a complete filter set for type Ia supernovacosmology is that each bandpass be a redshifted copy of the first. Wedesign practical sets of redshifted bandpasses that are matched totypical high resistivity CCD and HgCdTe infra-red detector sensitivities.These are designed to minimise systematic error in well observedsupernovae, final designs for specific missions should also considersignal-to-noise requirements and observing strategy. In addition wecalculate how accurately filters need to be calibrated in order toachieve the required photometric accuracy of future supernova cosmologyexperiments such as the SuperNova-Acceleration-Probe (SNAP), which is onepossible realisation of the Joint Dark-Energy mission (JDEM). We considerthe effect of possible periodic miscalibrations that may arise from theconstruction of an interference filter.

  6. A threat-based definition of IA- and IA-enabled products.

    SciTech Connect (OSTI)

    Shakamuri, Mayuri; Schaefer, Mark A.; Campbell, Philip LaRoche

    2010-07-01

    This paper proposes a definition of 'IA and IA-enabled products' based on threat, as opposed to 'security services' (i.e., 'confidentiality, authentication, integrity, access control or non-repudiation of data'), as provided by Department of Defense (DoD) Instruction 8500.2, 'Information Assurance (IA) Implementation.' The DoDI 8500.2 definition is too broad, making it difficult to distinguish products that need higher protection from those that do not. As a consequence the products that need higher protection do not receive it, increasing risk. The threat-based definition proposed in this paper solves those problems by focusing attention on threats, thereby moving beyond compliance to risk management. (DoDI 8500.2 provides the definitions and controls that form the basis for IA across the DoD.) Familiarity with 8500.2 is assumed.

  7. A threat-based definition of IA and IA-enabled products.

    SciTech Connect (OSTI)

    Shakamuri, Mayuri; Schaefer, Mark A.; Campbell, Philip LaRoche

    2010-09-01

    This paper proposes a definition of 'IA and IA-enabled products' based on threat, as opposed to 'security services' (i.e., 'confidentiality, authentication, integrity, access control or non-repudiation of data'), as provided by Department of Defense (DoD) Instruction 8500.2, 'Information Assurance (IA) Implementation.' The DoDI 8500.2 definition is too broad, making it difficult to distinguish products that need higher protection from those that do not. As a consequence the products that need higher protection do not receive it, increasing risk. The threat-based definition proposed in this paper solves those problems by focusing attention on threats, thereby moving beyond compliance to risk management. (DoDI 8500.2 provides the definitions and controls that form the basis for IA across the DoD.) Familiarity with 8500.2 is assumed.

  8. Ecological effects of pipeline construction through deciduous forested wetlands, Midland County, Michigan. Topical report, October 1990--August 1992

    SciTech Connect (OSTI)

    Rastorfer, J.R.; Van Dyke, G.D.; Zellmer, S.D.; Wilkey, P.L.

    1995-04-01

    This study is designed to record vegetational changes induced by the construction of a large-diameter gas pipeline through deciduous forested wetlands. Two second-growth wetland sites mapped Lenawee soils were selected in Midland County, Michigan: Site 1, a younger stand subjected to recent selective logging, and Site 2, a more mature stand. The collection of ecological data to analyze plant succession on the right-of-way (ROW) and the effects of the developing ROW plant communities on adjacent forest communities was initiated in 1989. Cover class estimates were made for understory and ROW plant species on the basis of 1 {times} 1{minus}m quadrats. Individual stem diameters and species counts were recorded for overstory plants in 10{minus}m quadrats. Although long-term studies have not been completed, firm baseline data were established for comparative analyses with future sampling. Current data indicate that vegetation became well-established on the ROW within one year and subsequently increased in coverage. About 65% of the species were wetland indicators, and the dominants included seeded and natural invading species; nevertheless, some elements of the original flora regenerated and persist. The plants of the ecotone understories of both sites changed from their original composition as a result of the installation of the gas pipeline. Although some forest species persist at both sites, the ecotone of Site I was influenced more by the seeded species, whereas the natural invaders were more important at Site 2.

  9. Depositional environments, sequence stratigraphy, and trap configuration of lower Wolfcampian clastics along eastern edge of Midland basin, west Texas

    SciTech Connect (OSTI)

    Stewart, N.R.; Reuter, S.G.

    1989-03-01

    The Lower Permian (lower Wolfcampian) along the eastern edge of the Midland basin, west Texas, is characterized by ramp-type shelf margins. During eustatic lowstand, nearshore sedimentation shifted drastically to the west into a basinal setting below the Pennsylvanian (Canyon) shelf margin. Core descriptions demonstrate that lowstand systems tract (LST) and transgressive systems tract (TST) siliciclastics were deposited in deltaic and coastal-plain environments. Prodelta, delta-front, and stream-mouth bar facies are associated with the LST. Coastal-plain and distributary channels are preserved in the TST. The sequence stratigraphic framework indicates type 1 sequence boundaries at 287 Ma, 282 Ma, and 280 Ma in the lower Wolfcampian clastics. This lower Wolfcampian package of sedimentary rocks overlies the Pennsylvanian and is capped by the 279-Ma middle Wolfcampian unconformity. All three sequence boundaries and associated systems tract deposits exhibit a prograding stacking pattern within the sequence stratigraphic framework. Basinally restricted prograding LST deltaic rocks are overlain by backstepping TST deltaics and highstand systems tract (HST) outer marine shales. Production in lower Wolfcampian clastic fields is associated with fine-grained quartzarenites up to 45 ft thick which were deposited in stream-mouth bars. Delta-front and prodelta low-permeability shales encase the reservoir facies, forming lateral permeability barriers. HST outer marine shales deposited over the stream-mouth-bar sandstones act as a top seal, creating a stratigraphic trap and providing source for the high-BTU gas and oil produced from these basinally restricted LST deltaics.

  10. Daniel Udwary

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

    biology, and taught medicinal chemistry and bioinformatics. He later moved to Cambridge to work as a Senior Scientist with Warp Drive Bio's Computational Biology group....

  11. Daniel Woomer

    Broader source: Energy.gov [DOE]

    Mr. Woomer, or "Dan" to his friends and colleagues, joined the Office of Technology Transitions (OTT) in May 2015. Dan oversees the business operation side of the office, which includes...

  12. Daniel Boff

    Broader source: Energy.gov [DOE]

    Dan Boff, the Office of Energy Efficiency and Renewable Energy’s current intern for Education and Workforce Development, is a senior at the George Washington University, majoring in...

  13. Daniel White

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

    Opportunities ESnet Staff & Org Chart Administration Advanced Network Technologies Cybersecurity Infrastructure, Identity & Collaboration Network Engineering Office of the CTO...

  14. Deputy Secretary Daniel Poneman's Remarks at demosEUROPA Event in Warsaw,

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

    Poland - As Prepared for Delivery | Department of Energy demosEUROPA Event in Warsaw, Poland - As Prepared for Delivery Deputy Secretary Daniel Poneman's Remarks at demosEUROPA Event in Warsaw, Poland - As Prepared for Delivery September 28, 2011 - 12:00pm Addthis Thank you, Ambassador Feinstein, for the introduction. And thank you to demosEUROPA and President Pawel Swieboda for hosting today's event. We are here today to talk about the future - our collective future - and how we can work

  15. IA News Archive | Department of Energy

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

    News Archive IA News Archive RSS July 22, 2016 Energy Department Selects Argonne National Laboratory to Lead U.S. Consortium for New CERC Medium- and Heavy-Duty Truck Technical Track The New Consortium of University, Private Sector and National Laboratory Partners will Advance Collaboration between the U.S. and China on Truck Efficiency Technologies June 10, 2016 Energy Department Invests More than $10 Million in Efficient Lighting Research and Development New projects designed to save consumers

  16. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties...

    Office of Scientific and Technical Information (OSTI)

    SciTech Connect Search Results Journal Article: Type Ia Supernova Hubble Residuals and ... as distinguished from previous works that use magnitude corrections as a ...

  17. CEPHEID CALIBRATIONS OF MODERN TYPE Ia SUPERNOVAE: IMPLICATIONS...

    Office of Scientific and Technical Information (OSTI)

    CEPHEID CALIBRATIONS OF MODERN TYPE Ia SUPERNOVAE: IMPLICATIONS FOR THE HUBBLE CONSTANT ... Country of Publication: United States Language: English Subject: 79 ASTROPHYSICS, ...

  18. Constraining Cosmic Evolution of Type Ia Supernovae

    SciTech Connect (OSTI)

    Foley, Ryan J.; Filippenko, Alexei V.; Aguilera, C.; Becker, A.C.; Blondin, S.; Challis, P.; Clocchiatti, A.; Covarrubias, R.; Davis, T.M.; Garnavich, P.M.; Jha, S.; Kirshner, R.P.; Krisciunas, K.; Leibundgut, B.; Li, W.; Matheson, T.; Miceli, A.; Miknaitis, G.; Pignata, G.; Rest, A.; Riess, A.G.; /UC, Berkeley, Astron. Dept. /Cerro-Tololo InterAmerican Obs. /Washington U., Seattle, Astron. Dept. /Harvard-Smithsonian Ctr. Astrophys. /Chile U., Catolica /Bohr Inst. /Notre Dame U. /KIPAC, Menlo Park /Texas A-M /European Southern Observ. /NOAO, Tucson /Fermilab /Chile U., Santiago /Harvard U., Phys. Dept. /Baltimore, Space Telescope Sci. /Johns Hopkins U. /Res. Sch. Astron. Astrophys., Weston Creek /Stockholm U. /Hawaii U. /Illinois U., Urbana, Astron. Dept.

    2008-02-13

    We present the first large-scale effort of creating composite spectra of high-redshift type Ia supernovae (SNe Ia) and comparing them to low-redshift counterparts. Through the ESSENCE project, we have obtained 107 spectra of 88 high-redshift SNe Ia with excellent light-curve information. In addition, we have obtained 397 spectra of low-redshift SNe through a multiple-decade effort at Lick and Keck Observatories, and we have used 45 ultraviolet spectra obtained by HST/IUE. The low-redshift spectra act as a control sample when comparing to the ESSENCE spectra. In all instances, the ESSENCE and Lick composite spectra appear very similar. The addition of galaxy light to the Lick composite spectra allows a nearly perfect match of the overall spectral-energy distribution with the ESSENCE composite spectra, indicating that the high-redshift SNe are more contaminated with host-galaxy light than their low-redshift counterparts. This is caused by observing objects at all redshifts with similar slit widths, which corresponds to different projected distances. After correcting for the galaxy-light contamination, subtle differences in the spectra remain. We have estimated the systematic errors when using current spectral templates for K-corrections to be {approx}0.02 mag. The variance in the composite spectra give an estimate of the intrinsic variance in low-redshift maximum-light SN spectra of {approx}3% in the optical and growing toward the ultraviolet. The difference between the maximum-light low and high-redshift spectra constrain SN evolution between our samples to be < 10% in the rest-frame optical.

  19. Search for surviving companions in type Ia supernova remnants

    SciTech Connect (OSTI)

    Pan, Kuo-Chuan; Ricker, Paul M.; Taam, Ronald E. E-mail: pmricker@illinois.edu E-mail: taam@asiaa.sinica.edu.tw

    2014-09-01

    The nature of the progenitor systems of type Ia supernovae (SNe Ia) is still unclear. One way to distinguish between the single-degenerate scenario and double-degenerate scenario for their progenitors is to search for the surviving companions (SCs). Using a technique that couples the results from multi-dimensional hydrodynamics simulations with calculations of the structure and evolution of main-sequence- (MS-) and helium-rich SCs, the color and magnitude of MS- and helium-rich SCs are predicted as functions of time. The SC candidates in Galactic type Ia supernova remnants (Ia SNR) and nearby extragalactic Ia SNRs are discussed. We find that the maximum detectable distance of MS SCs (helium-rich SCs) is 0.6-4 Mpc (0.4-16 Mpc), if the apparent magnitude limit is 27 in the absence of extinction, suggesting that the Large and Small Magellanic Clouds and the Andromeda Galaxy are excellent environments in which to search for SCs. However, only five Ia SNRs have been searched for SCs, showing little support for the standard channels in the singe-degenerate scenario. To better understand the progenitors of SNe Ia, we encourage the search for SCs in other nearby Ia SNRs.

  20. THE ULTRAVIOLET BRIGHTEST TYPE Ia SUPERNOVA 2011de

    SciTech Connect (OSTI)

    Brown, Peter J., E-mail: pbrown@physics.tamu.edu [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A and M University, Department of Physics and Astronomy, 4242 TAMU, College Station, TX 77843 (United States)

    2014-11-20

    We present and discuss the ultraviolet (UV)/optical photometric light curves and absolute magnitudes of the TypeIa supernova (SN Ia) 2011de from the Swift Ultraviolet/Optical Telescope. We find it to be the UV brightest SN Ia yet observedmore than a factor of 10 brighter than normal SNe Ia in the mid-ultraviolet. We find that the UV/optical brightness and broad light curve evolution can be modeled with additional flux from the shock of the ejecta hitting a relatively large red giant companion separated by 6 10{sup 13} cm. However, the post-maximum behavior of other UV-bright SNe Ia can also be modeled in a similar manner, including objects with UV spectroscopy or pre-maximum photometry which is inconsistent with this model. This suggests that similar UV luminosities can be intrinsic or caused by other forms of shock interaction. The high velocities reported for SN 2011de make it distinct from the UV-bright ''super-Chandrasekhar'' SNe Ia and the NUV-blue group of normal SNe Ia. SN 2011de is an extreme example of the UV variations in SNe Ia.

  1. DIVERSITY OF TYPE Ia SUPERNOVAE IMPRINTED IN CHEMICAL ABUNDANCES

    SciTech Connect (OSTI)

    Tsujimoto, Takuji [National Astronomical Observatory of Japan, Mitaka-shi, Tokyo 181-8588 (Japan); Shigeyama, Toshikazu, E-mail: taku.tsujimoto@nao.ac.jp [Research Center for the Early Universe, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)

    2012-12-01

    A time delay of Type Ia supernova (SN Ia) explosions hinders the imprint of their nucleosynthesis on stellar abundances. However, some occasional cases give birth to stars that avoid enrichment of their chemical compositions by massive stars and thereby exhibit an SN-Ia-like elemental feature including a very low [Mg/Fe] ( Almost-Equal-To - 1). We highlight the elemental feature of Fe-group elements for two low-Mg/Fe objects detected in nearby galaxies, and propose the presence of a class of SNe Ia that yield the low abundance ratios of [Cr, Mn, Ni/Fe]. Our novel models of chemical evolution reveal that our proposed class of SNe Ia (slow SNe Ia) is associated with ones exploding on a long timescale after their stellar birth and give a significant impact on the chemical enrichment in the Large Magellanic Cloud (LMC). In the Galaxy, on the other hand, this effect is unseen due to the overwhelming enrichment by the major class of SNe Ia that explode promptly (prompt SNe Ia) and eject a large amount of Fe-group elements. This nicely explains the different [Cr, Mn, Ni/Fe] features between the two galaxies as well as the puzzling feature seen in the LMC stars exhibiting very low Ca but normal Mg abundances. Furthermore, the corresponding channel of slow SN Ia is exemplified by performing detailed nucleosynthesis calculations in the scheme of SNe Ia resulting from a 0.8 + 0.6 M{sub Sun} white dwarf merger.

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

    Office of Legacy Management (LM)

    05 Corp Pioneer Div - IA 05 FUSRAP Considered Sites Site: BENDIX AVIATION CORP., PIONEER DIV. (IA.05 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Pioneer Division, Bendix Aviation Corporation Bendix Aviation Corporation Bendix Pioneer Division IA.05-1 IA.05-2 IA.05-3 Location: Davenport , Iowa IA.05-1 Evaluation Year: 1990 IA.05-2 IA.05-4 Site Operations: Conducted studies to investigate the feasibility of using sonic cleaning equipment to

  3. Color dispersion and Milky-Way-like reddening among type Ia supernovae...

    Office of Scientific and Technical Information (OSTI)

    Authors: Scolnic, Daniel M. ; Riess, Adam G. ; Rodney, Steven A. ; Brout, Dillon J. ; Jones, David O. 1 ; Foley, Ryan J. 2 ; Rest, Armin 3 + Show Author Affiliations ...

  4. ADM Cabrera JV | Open Energy Information

    Open Energy Info (EERE)

    Jose do Rio Preto, Sao Paulo, Brazil Product: Archer Daniels Midland Company (ADM) and Grupo Cabrera have formed a partnership to develop two ethanol plants in Brazil. References:...

  5. EA-1828: Final Environmental Assessment

    Office of Energy Efficiency and Renewable Energy (EERE)

    Industrial Carbon Capture and Sequestration (ICCS) Area 1 Project : CO2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone, Archer Daniels Midland Company Decatur, Illinois

  6. FE Press Releases and Techlines | Department of Energy

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

    large-scale industrial carbon capture and storage demonstration project. The Archer Daniels Midland Company (ADM) marked the progress made on construction on the project's...

  7. Environmental Assessments (EA) | Department of Energy

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

    from Biofuels Production and Sequestration into the Mt. Simon Sandstone, Archer Daniels Midland Company Decatur, Illinois April 1, 2011 EA-1795: Final Environmental...

  8. FE Carbon Capture and Storage News | Department of Energy

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

    large-scale industrial carbon capture and storage demonstration project. The Archer Daniels Midland Company (ADM) marked the progress made on construction on the project's...

  9. FE Clean Coal News | Department of Energy

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

    large-scale industrial carbon capture and storage demonstration project. The Archer Daniels Midland Company (ADM) marked the progress made on construction on the project's...

  10. Energy News | Department of Energy

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

    Founder and Managing Partner Nancy Pfund, SolarCity CEO Lyndon Rive and Archer Daniels Midland Company Chairman and CEO Patricia Woertz. Additional speakers will be...

  11. Illinois' 18th congressional district: Energy Resources | Open...

    Open Energy Info (EERE)

    Daniels Midland Aventine Renewable Energy Holdings Aventine Renewable Energy Inc Firefly Energy Inc Illinois Commerce Commission Marquis Energy LLC Tate & Lyle Energy...

  12. Macon County, Illinois: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    5 Climate Zone Subtype A. Registered Energy Companies in Macon County, Illinois Archer Daniels Midland Tate & Lyle Energy Generation Facilities in Macon County, Illinois KMS Macon...

  13. Illinois' 17th congressional district: Energy Resources | Open...

    Open Energy Info (EERE)

    Illinois. Registered Energy Companies in Illinois' 17th congressional district Archer Daniels Midland EPower Synergies Inc Illinois Commerce Commission Illinois Institute for...

  14. Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Poneman issue Personal Commitment to Health and Safety of DOE employees

    Office of Energy Efficiency and Renewable Energy (EERE)

    Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Poneman recently issued a joint Memorandum, entitled Personal Commitment to Health and Safety through Leadership, Employee Engagement, and Organizational Learning.

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

    Office of Legacy Management (LM)

    Army Ammunition Plant - IA 02 FUSRAP Considered Sites Iowa Army Ammunition Plant, IA Alternate Name(s): Burlington Ordnance Plant Iowa Ordnance Plant Silas Mason Company IA.02-3 Location: Located in Township 70 North, Range 3 West, Section 32, 5th Principal Meridian, Des Moines County, Burlington, Iowa IA.02-1 IA.02-5 Historical Operations: Assembled nuclear weapons, primarily high explosive components and conducted explosives testing using the high explosive components and depleted uranium. AEC

  16. U.S. Energy Information Administration | Annual Coal Report 2014

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

    5. Coal Consumers in the Manufacturing and Coke Sectors, 2014 Company Name Plant Location Top Ten Manufacturers American Crystal Sugar Co MN, ND Archer Daniels Midland IA, IL, MN, NE Carmeuse Lime Stone Inc AL, IN, KY, MI, OH, PA, TN, WI Cemex Inc AL, CA, CO, FL, GA, KY, OH, TN, TX Dakota Gasification Company ND Eastman Chemical Company TN Georgia-Pacific Consumer Products LP AL, GA, OK, VA, WI Holcim (US) Inc AL, CO, MD, MO, MT, OK, SC, TX, UT NewPage Corporation MD, MI, WI U S Steel

  17. SAS Output

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

    5. Coal Consumers in the Manufacturing and Coke Sectors, 2014" "Company Name","Plant Location" "Top Ten Manufacturers" "American Crystal Sugar Co","MN, ND" "Archer Daniels Midland","IA, IL, MN, NE" "Carmeuse Lime Stone Inc","AL, IN, KY, MI, OH, PA, TN, WI" "Cemex Inc","AL, CA, CO, FL, GA, KY, OH, TN, TX" "Dakota Gasification Company","ND" "Eastman Chemical

  18. A STUDY OF CARBON FEATURES IN TYPE Ia SUPERNOVA SPECTRA (Journal...

    Office of Scientific and Technical Information (OSTI)

    A STUDY OF CARBON FEATURES IN TYPE Ia SUPERNOVA SPECTRA Citation Details In-Document Search Title: A STUDY OF CARBON FEATURES IN TYPE Ia SUPERNOVA SPECTRA One of the major ...

  19. An Analysis of Department of Defense Instruction 8500.2 'Information Assurance (IA) Implementation.'

    SciTech Connect (OSTI)

    Campbell, Philip LaRoche

    2012-01-01

    The Department of Defense (DoD) provides its standard for information assurance in its Instruction 8500.2, dated February 6, 2003. This Instruction lists 157 'IA Controls' for nine 'baseline IA levels.' Aside from distinguishing IA Controls that call for elevated levels of 'robustness' and grouping the IA Controls into eight 'subject areas' 8500.2 does not examine the nature of this set of controls, determining, for example, which controls do not vary in robustness, how this set of controls compares with other such sets, or even which controls are required for all nine baseline IA levels. This report analyzes (1) the IA Controls, (2) the subject areas, and (3) the Baseline IA levels. For example, this report notes that there are only 109 core IA Controls (which this report refers to as 'ICGs'), that 43 of these core IA Controls apply without variation to all nine baseline IA levels and that an additional 31 apply with variations. This report maps the IA Controls of 8500.2 to the controls in NIST 800-53 and ITGI's CoBIT. The result of this analysis and mapping, as shown in this report, serves as a companion to 8500.2. (An electronic spreadsheet accompanies this report.)

  20. Type Ia Supernova Spectral Line Ratios as LuminosityIndicators

    SciTech Connect (OSTI)

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

    2005-12-07

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

  1. Next-Generation Petascale Simulations of Type Ia Supernovae | Argonne

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

    Leadership Computing Facility deflagration to detonation transition model Deflagration to detonation transition model. Min lOng, Dan van Rossum, Sean Couch, George Jordan, Brad Gallagher, Don Lamb, University of Chicago; Michael E. Papka, Argonne National Laboratory/University of Chicago Next-Generation Petascale Simulations of Type Ia Supernovae PI Name: Don Lamb PI Email: lamb@oddjob.uchicago.edu Institution: The University of Chicago Allocation Program: INCITE Allocation Hours at ALCF:

  2. Microsoft PowerPoint - IEEE IAS PES 102313.pptx

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

    DOE's ARRA Smart Grid Program Steve Bossart, Senior Energy Analyst IEEE IAS/PES Pittsburgh Section October 23, 2013 # Topics * OE ARRA Smart Grid Program * OE ARRA Smart Grid Progress * Results and Case Studies * Life After ARRA Smart Grid # DOE OE ARRA Smart Grid Program # American Recovery and Reinvestment Act ($4.5B) * Smart Grid Investment Grants (99 projects) - $3.4 billion Federal; $4.7 billion private sector - > 800 PMUs covering almost 100% of transmission - ~ 8000 distribution

  3. Power-law cosmology, SN Ia, and BAO

    SciTech Connect (OSTI)

    Dolgov, Aleksander; Halenka, Vitali; Tkachev, Igor E-mail: vithal@umich.edu

    2014-10-01

    We revise observational constraints on the class of models of modified gravity which at low redshifts lead to a power-law cosmology. To this end we use available public data on Supernova Ia and on baryon acoustic oscillations. We show that the expansion regime a(t)?t{sup ?} with ? close to 3/2 in a spatially flat universe is a good fit to these data.

  4. Signatures of a companion star in type Ia supernovae

    SciTech Connect (OSTI)

    Maeda, Keiichi; Kutsuna, Masamichi; Shigeyama, Toshikazu

    2014-10-10

    Although type Ia supernovae (SNe Ia) have been used as precise cosmological distance indicators, their progenitor systems remain unresolved. One of the key questions is whether there is a nondegenerate companion star at the time of a thermonuclear explosion of a white dwarf. In this paper, we investigate whether an interaction between the SN ejecta and the companion star may result in observable footprints around the maximum brightness and thereafter, by performing multidimensional radiation transfer simulations based on hydrodynamic simulations of the interaction. We find that such systems result in variations in various observational characteristics due to different viewing directions, and the predicted behaviors (redder and fainter for the companion direction) are the opposite of what were suggested by the previous study. The variations are generally modest and within observed scatters. However, the model predicts trends between some observables different from those observationally derived, so a large sample of SNe Ia with small calibration errors may be used to constrain the existence of such a companion star. The variations in different colors in optical band passes can be mimicked by external extinctions, so such an effect could be a source of scatter in the peak luminosity and derived distance. After the peak, hydrogen-rich materials expelled from the companion will manifest themselves in hydrogen lines, but Hα is extremely difficult to identify. Alternatively, we find that P{sub β} in postmaximum near-infrared spectra can potentially provide a powerful diagnostic.

  5. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties (Journal

    Office of Scientific and Technical Information (OSTI)

    Article) | SciTech Connect Journal Article: Type Ia Supernova Hubble Residuals and Host-Galaxy Properties Citation Details In-Document Search Title: Type Ia Supernova Hubble Residuals and Host-Galaxy Properties Kim et al. (2013) [K13] introduced a new methodology for determining peak- brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized

  6. THE HYBRID CONe WD + He STAR SCENARIO FOR THE PROGENITORS OF TYPE Ia SUPERNOVAE

    SciTech Connect (OSTI)

    Wang, B.; Meng, X.; Liu, D.-D.; Han, Z.; Liu, Z.-W.

    2014-10-20

    Hybrid CONe white dwarfs (WDs) have been suggested to be possible progenitors of type Ia supernovae (SNe Ia). In this Letter, we systematically studied the hybrid CONe WD + He star scenario for the progenitors of SNe Ia, in which a hybrid CONe WD increases its mass to the Chandrasekhar mass limit by accreting He-rich material from a non-degenerate He star. We obtained the SN Ia birthrates and delay times for this scenario using to a series of detailed binary population synthesis simulations. The SN Ia birthrates for this scenario are ∼0.033-0.539 × 10{sup –3} yr{sup –1}, which roughly accounts for 1%-18% of all SNe Ia. The estimated delay times are ∼28 Myr-178 Myr, which makes these the youngest SNe Ia predicted by any progenitor model so far. We suggest that SNe Ia from this scenario may provide an alternative explanation for type Iax SNe. We also presented some properties of the donors at the point when the WDs reach the Chandrasekhar mass. These properties may be a good starting point for investigating the surviving companions of SNe Ia and for constraining the progenitor scenario studied in this work.

  7. Improved Dark Energy Constraints From ~ 100 New CfA Supernova Type Ia Light

    Office of Scientific and Technical Information (OSTI)

    Curves (Journal Article) | SciTech Connect Improved Dark Energy Constraints From ~ 100 New CfA Supernova Type Ia Light Curves Citation Details In-Document Search Title: Improved Dark Energy Constraints From ~ 100 New CfA Supernova Type Ia Light Curves We combine the CfA3 supernovae Type Ia (SN Ia) sample with samples from the literature to calculate improved constraints on the dark energy equation of state parameter, w. The CfA3 sample is added to the Union set of Kowalski et al. to form the

  8. The Carnegie Supernova Project: Intrinsic colors of type Ia supernovae

    SciTech Connect (OSTI)

    Burns, Christopher R.; Persson, S. E.; Freedman, Wendy L.; Madore, Barry F. [Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Stritzinger, Maximilian; Contreras, Carlos [Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C (Denmark); Phillips, M. M.; Hsiao, E. Y.; Boldt, Luis; Campillay, Abdo; Castelln, Sergio; Morrell, Nidia; Salgado, Francisco [Carnegie Institution of Washington, Las Campanas Observatory, Colina El Pino, Casilla 601 (Chile); Folatelli, Gaston [Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, the University of Tokyo, 277-8583 Kashiwa (Japan); Suntzeff, Nicholas B. [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A and M University, Department of Physics and Astronomy, College Station, TX 77843 (United States)

    2014-07-01

    We present an updated analysis of the intrinsic colors of Type Ia supernova (SNe Ia) using the latest data release of the Carnegie Supernova Project. We introduce a new light-curve parameter very similar to stretch that is better suited for fast-declining events, and find that these peculiar types can be seen as extensions to the population of 'normal' SNe Ia. With a larger number of objects, an updated fit to the Lira relation is presented along with evidence for a dependence on the late-time slope of the B V light-curves with stretch and color. Using the full wavelength range from u to H band, we place constraints on the reddening law for the sample as a whole and also for individual events/hosts based solely on the observed colors. The photometric data continue to favor low values of R{sub V} , though with large variations from event to event, indicating an intrinsic distribution. We confirm the findings of other groups that there appears to be a correlation between the derived reddening law, R{sub V} , and the color excess, E(B V), such that larger E(B V) tends to favor lower R{sub V} . The intrinsic u-band colors show a relatively large scatter that cannot be explained by variations in R{sub V} or by the Goobar power-law for circumstellar dust, but rather is correlated with spectroscopic features of the supernova and is therefore likely due to metallicity effects.

  9. MaRIE 1.0: A briefing to Katherine Richardson-McDaniel, Staff Member for U. S. Senator Martin Heinrich (D-NM)

    SciTech Connect (OSTI)

    Barnes, Cris William

    2015-02-24

    At the request of Katherine Richardson-McDaniel, Staff Member to U.S. Senator Martin Heinrich (D-NM), a high-level briefing was requested about MaRIE 1.0, the Matter-Radiation Interactions in Extremes effort at Los Alamos National Laboratory. What it would be, the mission need motivation, the scientific challenge, and the current favorable impact on both programs and people are shown in viewgraph form.

  10. Grouping normal type Ia supernovae by UV to optical color differences

    SciTech Connect (OSTI)

    Milne, Peter A.; Brown, Peter J.; Roming, Peter W. A.; Bufano, Filomena; Gehrels, Neil

    2013-12-10

    Observations of many Type Ia supernovae (SNe Ia) for multiple epochs per object with the Swift Ultraviolet Optical Telescope instrument have revealed that there exists order to the differences in the UV-optical colors of optically normal supernovae (SNe). We examine UV-optical color curves for 23 SNe Ia, dividing the SNe into four groups, and find that roughly one-third of 'NUV-blue' SNe Ia have bluer UV-optical colors than the larger 'NUV-red' group. Two minor groups are recognized, 'MUV-blue' and 'irregular' SNe Ia. While we conclude that the latter group is a subset of the NUV-red group, containing the SNe with the broadest optical peaks, we conclude that the 'MUV-blue' group is a distinct group. Separating into the groups and accounting for the time evolution of the UV-optical colors lowers the scatter in two NUV-optical colors (e.g., u v and uvw1 v) to the level of the scatter in b v. This finding is promising for extending the cosmological utilization of SNe Ia into the NUV. We generate spectrophotometry of 33 SNe Ia and determine the correct grouping for each. We argue that there is a fundamental spectral difference in the 2900-3500 wavelength range, a region suggested to be dominated by absorption from iron-peak elements. The NUV-blue SNe Ia feature less absorption than the NUV-red SNe Ia. We show that all NUV-blue SNe Ia in this sample also show evidence of unburned carbon in optical spectra, whereas only one NUV-red SN Ia features that absorption line. Every NUV-blue event also exhibits a low gradient of the Si II ?6355 absorption feature. Many NUV-red events also exhibit a low gradient, perhaps suggestive that NUV-blue events are a subset of the larger low-velocity gradient group.

  11. THE BIRTH RATE OF SNe Ia FROM HYBRID CONe WHITE DWARFS

    SciTech Connect (OSTI)

    Meng, Xiangcun [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Podsiadlowski, Philipp, E-mail: xiangcunmeng@ynao.ac.cn [Department of Astronomy, Oxford University, Oxford OX1 3RH (United Kingdom)

    2014-07-10

    Considering the uncertainties of the C-burning rate (CBR) and the treatment of convective boundaries, Chen et al. found that there is a regime where it is possible to form hybrid CONe white dwarfs (WDs), i.e., ONe WDs with carbon-rich cores. As these hybrid WDs can be as massive as 1.30 M {sub ?}, not much mass needs to be accreted for these objects to reach the Chandrasekhar limit and to explode as Type Ia supernovae (SNe Ia). We have investigated their contribution to the overall SN Ia birth rate and found that such SNe Ia tend to be relatively young with typical time delays between 0.1 and 1 Gyr, where some may be as young as 30 Myr. SNe Ia from hybrid CONe WDs may contribute several percent to all SNe Ia, depending on the common-envelope ejection efficiency and the CBR. We suggest that these SNe Ia may produce part of the 2002cx-like SN Ia class.

  12. Type Ia supernova rate studies from the SDSS-II Supernova Study

    SciTech Connect (OSTI)

    Dilday, Benjamin

    2008-08-01

    The author presents new measurements of the type Ia SN rate from the SDSS-II Supernova Survey. The SDSS-II Supernova Survey was carried out during the Fall months (Sept.-Nov.) of 2005-2007 and discovered ~ 500 spectroscopically confirmed SNe Ia with densely sampled (once every ~ 4 days), multi-color light curves. Additionally, the SDSS-II Supernova Survey has discovered several hundred SNe Ia candidates with well-measured light curves, but without spectroscopic confirmation of type. This total, achieved in 9 months of observing, represents ~ 15-20% of the total SNe Ia discovered worldwide since 1885. The author describes some technical details of the SN Survey observations and SN search algorithms that contributed to the extremely high-yield of discovered SNe and that are important as context for the SDSS-II Supernova Survey SN Ia rate measurements.

  13. On silicon group elements ejected by supernovae type IA

    SciTech Connect (OSTI)

    De, Soma; Timmes, F. X. [School of Earth and Space Exploration, Arizona State University, Tempe, AZ (United States); Brown, Edward F. [Joint Institute for Nuclear Astrophysics, University of Notre Dame, IN 46556 (United States); Calder, Alan C. [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY (United States); Townsley, Dean M. [Department of Physics and Astronomy, The University of Alabama, Tuscaloosa, AL (United States); Athanassiadou, Themis [Swiss National Supercomputing Centre, Via Trevano 131, 6900 Lugano (Switzerland); Chamulak, David A. [Physics Division, Argonne National Laboratory, Argonne, IL (United States); Hawley, Wendy [Laboratoire d'Astrophysique de Marseille, Marseille cedex 13 F-13388 (France); Jack, Dennis, E-mail: somad@asu.edu [Departamento de Astronoma, Universidad de Guanajuato, Apartado Postal 144, 36000 Guanajuato (Mexico)

    2014-06-01

    There is evidence that the peak brightness of a Type Ia supernova is affected by the electron fraction Y {sub e} at the time of the explosion. The electron fraction is set by the aboriginal composition of the white dwarf and the reactions that occur during the pre-explosive convective burning. To date, determining the makeup of the white dwarf progenitor has relied on indirect proxies, such as the average metallicity of the host stellar population. In this paper, we present analytical calculations supporting the idea that the electron fraction of the progenitor systematically influences the nucleosynthesis of silicon group ejecta in Type Ia supernovae. In particular, we suggest the abundances generated in quasi-nuclear statistical equilibrium are preserved during the subsequent freeze-out. This allows potential recovery of Y {sub e} at explosion from the abundances recovered from an observed spectra. We show that measurement of {sup 28}Si, {sup 32}S, {sup 40}Ca, and {sup 54}Fe abundances can be used to construct Y {sub e} in the silicon-rich regions of the supernovae. If these four abundances are determined exactly, they are sufficient to recover Y {sub e} to 6%. This is because these isotopes dominate the composition of silicon-rich material and iron-rich material in quasi-nuclear statistical equilibrium. Analytical analysis shows the {sup 28}Si abundance is insensitive to Y {sub e}, the {sup 32}S abundance has a nearly linear trend with Y {sub e}, and the {sup 40}Ca abundance has a nearly quadratic trend with Y {sub e}. We verify these trends with post-processing of one-dimensional models and show that these trends are reflected in the model's synthetic spectra.

  14. CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA

    SciTech Connect (OSTI)

    Hicken, Malcolm; Challis, Peter; Kirshner, Robert P.; Bakos, Gaspar; Berlind, Perry; Brown, Warren R.; Caldwell, Nelson; Calkins, Mike; Cho, Richard; Contreras, Maria; Jha, Saurabh; Matheson, Tom; Modjaz, Maryam; Rest, Armin; Michael Wood-Vasey, W.; Barton, Elizabeth J.; Bragg, Ann; Briceno, Cesar; Ciupik, Larry; Dendy, Kristi-Concannon E-mail: kirshner@cfa.harvard.edu

    2009-07-20

    We present multiband photometry of 185 type-Ia supernovae (SNe Ia), with over 11,500 observations. These were acquired between 2001 and 2008 at the F. L. Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics (CfA). This sample contains the largest number of homogeneously observed and reduced nearby SNe Ia (z {approx}< 0.08) published to date. It more than doubles the nearby sample, bringing SN Ia cosmology to the point where systematic uncertainties dominate. Our natural system photometry has a precision of {approx}<0.02 mag in BVRIr'i' and {approx}<0.04 mag in U for points brighter than 17.5 mag. We also estimate a systematic uncertainty of 0.03 mag in our SN Ia standard system BVRIr'i' photometry and 0.07 mag for U. Comparisons of our standard system photometry with published SN Ia light curves and comparison stars, where available for the same SN, reveal agreement at the level of a few hundredths mag in most cases. We find that 1991bg-like SNe Ia are sufficiently distinct from other SNe Ia in their color and light-curve-shape/luminosity relation that they should be treated separately in light-curve/distance fitter training samples. The CfA3 sample will contribute to the development of better light-curve/distance fitters, particularly in the few dozen cases where near-infrared photometry has been obtained and, together, can help disentangle host-galaxy reddening from intrinsic supernova color, reducing the systematic uncertainty in SN Ia distances due to dust.

  15. From: Cohen, Daniel

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

    William T. Miller | Partner McCARTER & ENGLISH, LLP 1015 15th Street, NW, 12th Floor | ... message from the law firm of McCarter & English, LLP is for the sole use of the intended ...

  16. From: Cohen, Daniel

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

    Bud William T. Miller | Partner McCARTER & ENGLISH, LLP 1015 15th Street, NW, 12th Floor | Washington DC, 20005 T: 202-753-3420 F: 202-354-4658 wmiller@mccarter.com | ...

  17. From: Cohen, Daniel

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

    ... whether DOE intends to heed this request. Bud William T. Miller | Partner McCARTER & ENGLISH, LLP 1015 15th Street, NW, 12th Floor | Washington DC, 20005 T: 202-753-3420 F: ...

  18. Daniel C. Tobin

    Broader source: Energy.gov [DOE]

    [[{"type":"media","view_mode":"media_large","fid":"885651","attributes":{"alt":"Dan Tobin Portrait.jpg","class":"media-image caption","style":"font-size: 12px; width: 360px; height: 450px; float:...

  19. Daniel J. Miller - JCAP

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

    Membranes are useful in a wide variety of separations, including water purification and desalination, removal of greenhouse gases from industrial emissions, and prevention of ...

  20. Daniel Shechtman and Quasicrystals

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

    science and engineering, and the Philip Tobias Professor of Materials Science at the Technion - Israel Institute of Technology. He is currently at the Technion in Haifa, Israel. ...

  1. From: Cohen, Daniel

    Energy Savers [EERE]

    This includes the approach to: * Incorporating the 1994 through 2009 state-level AHRI condensing and non-condensing furnace shipment data available only to LBNL as confidential ...

  2. Daniel (Todd) Griffith

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

    Lab Photovoltaic Systems Evaluation Laboratory PV Regional ... Facility Geomechanics and Drilling Labs National ... He is the Technical Lead for Sandia's Offshore Wind Energy ...

  3. Type Ia supernovae yielding distances with 3-4% precision (Journal...

    Office of Scientific and Technical Information (OSTI)

    A paper copy of this document is also available for sale to the public from the National Technical Information Service, Springfield, VA at www.ntis.gov. The luminosities of Type Ia ...

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

    Open Energy Info (EERE)

    IA.pdf Jump to: navigation, search File File history File usage Iowa Ethanol Plant Locations Size of this preview: 776 600 pixels. Full resolution (1,650 1,275 pixels,...

  5. Low Mach Number Modeling of Type Ia Supernovae

    SciTech Connect (OSTI)

    Almgren, Ann S.; Bell, John B.; Rendleman, Charles A.; Zingale,Michael

    2005-08-05

    We introduce a low Mach number equation set for the large-scale numerical simulation of carbon-oxygen white dwarfs experiencing a thermonuclear deflagration. Since most of the interesting physics in a Type Ia supernova transpires at Mach numbers from 0.01 to 0.1, such an approach enables both a considerable increase in accuracy and savings in computer time compared with frequently used compressible codes. Our equation set is derived from the fully compressible equations using low Mach number asymptotics, but without any restriction on the size of perturbations in density or temperature. Comparisons with simulations that use the fully compressible equations validate the low Mach number model in regimes where both are applicable. Comparisons to simulations based on the more traditional an elastic approximation also demonstrate the agreement of these models in the regime for which the anelastic approximation is valid. For low Mach number flows with potentially finite amplitude variations in density and temperature, the low Mach number model overcomes the limitations of each of the more traditional models and can serve as the basis for an accurate and efficient simulation tool.

  6. Cosmological parameter uncertainties from SALT-II type Ia supernova light curve models

    SciTech Connect (OSTI)

    Mosher, J.; Sako, M. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Guy, J.; Astier, P.; Betoule, M.; El-Hage, P.; Pain, R.; Regnault, N. [LPNHE, CNRS/IN2P3, Universit Pierre et Marie Curie Paris 6, Universi Denis Diderot Paris 7, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Kessler, R.; Frieman, J. A. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Marriner, J. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Biswas, R.; Kuhlmann, S. [Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439 (United States); Schneider, D. P., E-mail: kessler@kicp.chicago.edu [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States)

    2014-09-20

    We use simulated type Ia supernova (SN Ia) samples, including both photometry and spectra, to perform the first direct validation of cosmology analysis using the SALT-II light curve model. This validation includes residuals from the light curve training process, systematic biases in SN Ia distance measurements, and a bias on the dark energy equation of state parameter w. Using the SN-analysis package SNANA, we simulate and analyze realistic samples corresponding to the data samples used in the SNLS3 analysis: ?120 low-redshift (z < 0.1) SNe Ia, ?255 Sloan Digital Sky Survey SNe Ia (z < 0.4), and ?290 SNLS SNe Ia (z ? 1). To probe systematic uncertainties in detail, we vary the input spectral model, the model of intrinsic scatter, and the smoothing (i.e., regularization) parameters used during the SALT-II model training. Using realistic intrinsic scatter models results in a slight bias in the ultraviolet portion of the trained SALT-II model, and w biases (w {sub input} w {sub recovered}) ranging from 0.005 0.012 to 0.024 0.010. These biases are indistinguishable from each other within the uncertainty; the average bias on w is 0.014 0.007.

  7. EA-1626: Final Environmental Assessment | Department of Energy

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

    DOE proposes to co-fund an 84,274,927 project located on property of the MGSC partner Archer Daniels Midland Company (ADM). The overall objective of this project would be to ...

  8. CO2 Capture and Storage Project, Education and Training Center...

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

    It's the process of capturing and storing or re-using carbon dioxide (CO2) from coal-fired ... from Archer Daniels Midland's ethanol plant in Decatur, transported via a mile-long ...

  9. Conversion of Lignocellulosic Biomass to Ethanol Butyl Acrylate

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

    Conversion of Lignocellulosic Biomass to Ethanol and Butyl Acrylate March 25, 2015 Principal Investigator Thomas P. Binder ARCHER DANIELS MIDLAND COMPANY 2 Where does ADM fit with the IBR? * Ensuring a supply of technology for future growth is a priority for ADM Research * Corn stover utilization may enable continued growth in starch supply while starting a new industry around a currently underutilized material James R Randall Research Center Decatur, IL ARCHER DANIELS MIDLAND COMPANY 3 Quad

  10. fe0001547 | netl.doe.gov

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

    1547 Recovery Act: CO2 Capture From Biofuels Production and Sequestration into the Mt. Simon Sandstone Reservoir Email Page email Print This Page print Performer: Archer Daniels Midland Corporation (ADM) fe0001547 ADM's Agricultural Processing and Biofuels Plant, Decatur, IL. Website: Archer Daniels Midland Corporation (ADM) Award Number: FE0001547 Project Duration: 11/16/2009 - 09/30/2017 Total Award Value: $207,942,199.00 DOE Share: $141,405,945.00 Performer Share: $66,536,254.00 Technology

  11. Type Ia supernovae from merging white dwarfs. II. Post-merger detonations

    SciTech Connect (OSTI)

    Raskin, Cody; Kasen, Daniel; Moll, Rainer; Woosley, Stan; Schwab, Josiah

    2014-06-10

    Merging carbon-oxygen (CO) white dwarfs are a promising progenitor system for Type Ia supernovae (SNe Ia), but the underlying physics and timing of the detonation are still debated. If an explosion occurs after the secondary star is fully disrupted, the exploding primary will expand into a dense CO medium that may still have a disk-like structure. This interaction will decelerate and distort the ejecta. Here we carry out multidimensional simulations of 'tamped' SN Ia models, using both particle and grid-based codes to study the merger and explosion dynamics and a radiative transfer code to calculate synthetic spectra and light curves. We find that post-merger explosions exhibit an hourglass-shaped asymmetry, leading to strong variations in the light curves with viewing angle. The two most important factors affecting the outcome are the scale height of the disk, which depends sensitively on the binary mass ratio, and the total {sup 56}Ni yield, which is governed by the central density of the remnant core. The synthetic broadband light curves rise and decline very slowly, and the spectra generally look peculiar, with weak features from intermediate mass elements but relatively strong carbon absorption. We also consider the effects of the viscous evolution of the remnant and show that a longer time delay between merger and explosion probably leads to larger {sup 56}Ni yields and more symmetrical remnants. We discuss the relevance of this class of aspherical 'tamped' SN Ia for explaining the class of 'super-Chandrasekhar' SN Ia.

  12. Ultraviolet observations of Super-Chandrasekhar mass type Ia supernova candidates with swift UVOT

    SciTech Connect (OSTI)

    Brown, Peter J.; Smitka, Michael T.; Krisciunas, Kevin; Wang, Lifan; Kuin, Paul; De Pasquale, Massimiliano; Scalzo, Richard; Holland, Stephen; Milne, Peter

    2014-05-20

    Among Type Ia supernovae (SNe Ia), a class of overluminous objects exist whose ejecta mass is inferred to be larger than the canonical Chandrasekhar mass. We present and discuss the UV/optical photometric light curves, colors, absolute magnitudes, and spectra of three candidate Super-Chandrasekhar mass SNe—2009dc, 2011aa, and 2012dn—observed with the Swift Ultraviolet/Optical Telescope. The light curves are at the broad end for SNe Ia, with the light curves of SN 2011aa being among the broadest ever observed. We find all three to have very blue colors which may provide a means of excluding these overluminous SNe from cosmological analysis, though there is some overlap with the bluest of 'normal' SNe Ia. All three are overluminous in their UV absolute magnitudes compared to normal and broad SNe Ia, but SNe 2011aa and 2012dn are not optically overluminous compared to normal SNe Ia. The integrated luminosity curves of SNe 2011aa and 2012dn in the UVOT range (1600-6000 Å) are only half as bright as SN 2009dc, implying a smaller {sup 56}Ni yield. While it is not enough to strongly affect the bolometric flux, the early time mid-UV flux makes a significant contribution at early times. The strong spectral features in the mid-UV spectra of SNe 2009dc and 2012dn suggest a higher temperature and lower opacity to be the cause of the UV excess rather than a hot, smooth blackbody from shock interaction. Further work is needed to determine the ejecta and {sup 56}Ni masses of SNe 2011aa and 2012dn and to fully explain their high UV luminosities.

  13. Strong near-infrared carbon in the Type Ia supernova iPTF13ebh

    SciTech Connect (OSTI)

    Hsiao, E. Y.; Burns, C. R.; Contreras, C.; Höflich, P.; Sand, D.; Marion, G. H.; Phillips, M. M.; Stritzinger, M.; González-Gaitán, S.; Mason, R. E.; Folatelli, G.; Parent, E.; Gall, C.; Amanullah, R.; Anupama, G. C.; Arcavi, I.; Banerjee, D. P. K.; Beletsky, Y.; Blanc, G. A.; Bloom, J. S.; Brown, P. J.; Campillay, A.; Cao, Y.; De Cia, A.; Diamond, T.; Freedman, W. L.; Gonzalez, C.; Goobar, A.; Holmbo, S.; Howell, D. A.; Johansson, J.; Kasliwal, M. M.; Kirshner, R. P.; Krisciunas, K.; Kulkarni, S. R.; Maguire, K.; Milne, P. A.; Morrell, N.; Nugent, P. E.; Ofek, E. O.; Osip, D.; Palunas, P.; Perley, D. A.; Persson, S. E.; Piro, A. L.; Rabus, M.; Roth, M.; Schiefelbein, J. M.; Srivastav, S.; Sullivan, M.; Suntzeff, N. B.; Surace, J.; Woźniak, P. R.; Yaron, O.

    2015-05-22

    We present near-infrared (NIR) time-series spectroscopy, as well as complementary ultraviolet (UV), optical, and NIR data, of the Type Ia supernova (SN Ia) iPTF13ebh, which was discovered within two days from the estimated time of explosion. The first NIR spectrum was taken merely 2.3 days after explosion and may be the earliest NIR spectrum yet obtained of a SN Ia. The most striking features in the spectrum are several NIR C I lines, and the C Iλ1.0693 μm line is the strongest ever observed in a SN Ia. Interestingly, no strong optical C II counterparts were found, even though the optical spectroscopic time series began early and is densely cadenced. Except at the very early epochs, within a few days from the time of explosion, we show that the strong NIR C I compared to the weaker optical C II appears to be general in SNe Ia. iPTF13ebh is a fast decliner with Δm15(B) = 1.79 ± 0.01, and its absolute magnitude obeys the linear part of the width-luminosity relation. It is therefore categorized as a “transitional” event, on the fast-declining end of normal SNe Ia as opposed to subluminous/91bg-like objects. iPTF13ebh shows NIR spectroscopic properties that are distinct from both the normal and subluminous/91bg-like classes, bridging the observed characteristics of the two classes. These NIR observations suggest that composition and density of the inner core are similar to that of 91bg-like events, and that it has a deep-reaching carbon burning layer that is not observed in more slowly declining SNe Ia. Furthermore, there is also a substantial difference between the explosion times inferred from the early-time light curve and the velocity evolution of the Si II λ0.6355 μm line, implying a long dark phase of ~4 days.

  14. Strong near-infrared carbon in the Type Ia supernova iPTF13ebh

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

    Hsiao, E. Y.; Burns, C. R.; Contreras, C.; Höflich, P.; Sand, D.; Marion, G. H.; Phillips, M. M.; Stritzinger, M.; González-Gaitán, S.; Mason, R. E.; et al

    2015-05-22

    We present near-infrared (NIR) time-series spectroscopy, as well as complementary ultraviolet (UV), optical, and NIR data, of the Type Ia supernova (SN Ia) iPTF13ebh, which was discovered within two days from the estimated time of explosion. The first NIR spectrum was taken merely 2.3 days after explosion and may be the earliest NIR spectrum yet obtained of a SN Ia. The most striking features in the spectrum are several NIR C I lines, and the C Iλ1.0693 μm line is the strongest ever observed in a SN Ia. Interestingly, no strong optical C II counterparts were found, even though themore » optical spectroscopic time series began early and is densely cadenced. Except at the very early epochs, within a few days from the time of explosion, we show that the strong NIR C I compared to the weaker optical C II appears to be general in SNe Ia. iPTF13ebh is a fast decliner with Δm15(B) = 1.79 ± 0.01, and its absolute magnitude obeys the linear part of the width-luminosity relation. It is therefore categorized as a “transitional” event, on the fast-declining end of normal SNe Ia as opposed to subluminous/91bg-like objects. iPTF13ebh shows NIR spectroscopic properties that are distinct from both the normal and subluminous/91bg-like classes, bridging the observed characteristics of the two classes. These NIR observations suggest that composition and density of the inner core are similar to that of 91bg-like events, and that it has a deep-reaching carbon burning layer that is not observed in more slowly declining SNe Ia. Furthermore, there is also a substantial difference between the explosion times inferred from the early-time light curve and the velocity evolution of the Si II λ0.6355 μm line, implying a long dark phase of ~4 days.« less

  15. Strong near-infrared carbon in the Type Ia supernova iPTF13ebh

    SciTech Connect (OSTI)

    Hsiao, E. Y.; Burns, C. R.; Contreras, C.; Hflich, P.; Sand, D.; Marion, G. H.; Phillips, M. M.; Stritzinger, M.; Gonzlez-Gaitn, S.; Mason, R. E.; Folatelli, G.; Parent, E.; Gall, C.; Amanullah, R.; Anupama, G. C.; Arcavi, I.; Banerjee, D. P. K.; Beletsky, Y.; Blanc, G. A.; Bloom, J. S.; Brown, P. J.; Campillay, A.; Cao, Y.; De Cia, A.; Diamond, T.; Freedman, W. L.; Gonzalez, C.; Goobar, A.; Holmbo, S.; Howell, D. A.; Johansson, J.; Kasliwal, M. M.; Kirshner, R. P.; Krisciunas, K.; Kulkarni, S. R.; Maguire, K.; Milne, P. A.; Morrell, N.; Nugent, P. E.; Ofek, E. O.; Osip, D.; Palunas, P.; Perley, D. A.; Persson, S. E.; Piro, A. L.; Rabus, M.; Roth, M.; Schiefelbein, J. M.; Srivastav, S.; Sullivan, M.; Suntzeff, N. B.; Surace, J.; Wo?niak, P. R.; Yaron, O.

    2015-05-22

    We present near-infrared (NIR) time-series spectroscopy, as well as complementary ultraviolet (UV), optical, and NIR data, of the Type Ia supernova (SN Ia) iPTF13ebh, which was discovered within two days from the estimated time of explosion. The first NIR spectrum was taken merely 2.3 days after explosion and may be the earliest NIR spectrum yet obtained of a SN Ia. The most striking features in the spectrum are several NIR C I lines, and the C I?1.0693 ?m line is the strongest ever observed in a SN Ia. Interestingly, no strong optical C II counterparts were found, even though the optical spectroscopic time series began early and is densely cadenced. Except at the very early epochs, within a few days from the time of explosion, we show that the strong NIR C I compared to the weaker optical C II appears to be general in SNe Ia. iPTF13ebh is a fast decliner with ?m15(B) = 1.79 0.01, and its absolute magnitude obeys the linear part of the width-luminosity relation. It is therefore categorized as a transitional event, on the fast-declining end of normal SNe Ia as opposed to subluminous/91bg-like objects. iPTF13ebh shows NIR spectroscopic properties that are distinct from both the normal and subluminous/91bg-like classes, bridging the observed characteristics of the two classes. These NIR observations suggest that composition and density of the inner core are similar to that of 91bg-like events, and that it has a deep-reaching carbon burning layer that is not observed in more slowly declining SNe Ia. Furthermore, there is also a substantial difference between the explosion times inferred from the early-time light curve and the velocity evolution of the Si II ?0.6355 ?m line, implying a long dark phase of ~4 days.

  16. TYPE Ia SUPERNOVA COLORS AND EJECTA VELOCITIES: HIERARCHICAL BAYESIAN REGRESSION WITH NON-GAUSSIAN DISTRIBUTIONS

    SciTech Connect (OSTI)

    Mandel, Kaisey S.; Kirshner, Robert P. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Foley, Ryan J., E-mail: kmandel@cfa.harvard.edu [Astronomy Department, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States)

    2014-12-20

    We investigate the statistical dependence of the peak intrinsic colors of Type Ia supernovae (SNe Ia) on their expansion velocities at maximum light, measured from the Si II ?6355 spectral feature. We construct a new hierarchical Bayesian regression model, accounting for the random effects of intrinsic scatter, measurement error, and reddening by host galaxy dust, and implement a Gibbs sampler and deviance information criteria to estimate the correlation. The method is applied to the apparent colors from BVRI light curves and Si II velocity data for 79 nearby SNe Ia. The apparent color distributions of high-velocity (HV) and normal velocity (NV) supernovae exhibit significant discrepancies for B V and B R, but not other colors. Hence, they are likely due to intrinsic color differences originating in the B band, rather than dust reddening. The mean intrinsic B V and B R color differences between HV and NV groups are 0.06 0.02 and 0.09 0.02 mag, respectively. A linear model finds significant slopes of 0.021 0.006 and 0.030 0.009 mag (10{sup 3} km s{sup 1}){sup 1} for intrinsic B V and B R colors versus velocity, respectively. Because the ejecta velocity distribution is skewed toward high velocities, these effects imply non-Gaussian intrinsic color distributions with skewness up to +0.3. Accounting for the intrinsic-color-velocity correlation results in corrections to A{sub V} extinction estimates as large as 0.12 mag for HV SNe Ia and +0.06 mag for NV events. Velocity measurements from SN Ia spectra have the potential to diminish systematic errors from the confounding of intrinsic colors and dust reddening affecting supernova distances.

  17. 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.

  18. 2:30 PM TODAY: On-the-Record Conference Call with Deputy Assistant to the President for Energy and Climate Change Heather Zichal and Deputy Energy Secretary Daniel Poneman to Discuss the President’s Trip to Holland, Michigan to Tour the Johnson Controls I

    Broader source: Energy.gov [DOE]

    WASHINGTON, D.C. –  Today, Deputy Assistant to the President for Energy and Climate Change Heather Zichal and Deputy Energy Secretary Daniel Poneman will hold an on-the-record conference call to...

  19. SNe Ia tests of quintessence tracker cosmology in an anisotropic background

    SciTech Connect (OSTI)

    Miranda, W.; Carneiro, S.; Pigozzo, C. E-mail: saulo.carneiro@pq.cnpq.br

    2014-07-01

    We investigate the observational effects of a quintessence model in an anisotropic spacetime. The anisotropic metric is a non-rotating particular case of a generalized Gödel's metric and is classified as Bianchi III. This metric is an exact solution of the Einstein-Klein-Gordon field equations with an anisotropic scalar field ψ, which is responsible for the anisotropy of the spacetime geometry. We test the model against observations of type Ia supernovae, analyzing the SDSS dataset calibrated with the MLCS2k2 fitter, and the results are compared to standard quintessence models with Ratra-Peebles potentials. We obtain a good agreement with observations, with best values for the matter and curvature density parameters Ω{sub M} = 0.29 and Ω{sub k}= 0.01 respectively. We conclude that present SNe Ia observations cannot, alone, distinguish a possible anisotropic axis in the cosmos.

  20. THE EARLIEST NEAR-INFRARED TIME-SERIES SPECTROSCOPY OF A TYPE Ia SUPERNOVA

    SciTech Connect (OSTI)

    Hsiao, E. Y.; Phillips, M. M.; Morrell, N.; Contreras, C.; Roth, M.; Marion, G. H.; Kirshner, R. P.; Burns, C. R.; Freedman, W. L.; Persson, S. E.; Winge, C.; Gerardy, C. L.; Hoeflich, P.; Im, M.; Jeon, Y.; Pignata, G.; Stanishev, V.; and others

    2013-04-01

    We present ten medium-resolution, high signal-to-noise ratio near-infrared (NIR) spectra of SN 2011fe from SpeX on the NASA Infrared Telescope Facility (IRTF) and Gemini Near-Infrared Spectrograph (GNIRS) on Gemini North, obtained as part of the Carnegie Supernova Project. This data set constitutes the earliest time-series NIR spectroscopy of a Type Ia supernova (SN Ia), with the first spectrum obtained at 2.58 days past the explosion and covering -14.6 to +17.3 days relative to B-band maximum. C I {lambda}1.0693 {mu}m is detected in SN 2011fe with increasing strength up to maximum light. The delay in the onset of the NIR C I line demonstrates its potential to be an effective tracer of unprocessed material. For the first time in a SN Ia, the early rapid decline of the Mg II {lambda}1.0927 {mu}m velocity was observed, and the subsequent velocity is remarkably constant. The Mg II velocity during this constant phase locates the inner edge of carbon burning and probes the conditions under which the transition from deflagration to detonation occurs. We show that the Mg II velocity does not correlate with the optical light-curve decline rate {Delta}m{sub 15}(B). The prominent break at {approx}1.5 {mu}m is the main source of concern for NIR k-correction calculations. We demonstrate here that the feature has a uniform time evolution among SNe Ia, with the flux ratio across the break strongly correlated with {Delta}m{sub 15}(B). The predictability of the strength and the onset of this feature suggests that the associated k-correction uncertainties can be minimized with improved spectral templates.

  1. Comparing the host galaxies of type Ia, type II, and type Ibc supernovae

    SciTech Connect (OSTI)

    Shao, X.; Liang, Y. C.; Chen, X. Y.; Zhong, G. H.; Deng, L. C.; Zhang, B.; Shi, W. B.; Zhou, L.; Dennefeld, M.; Hammer, F.; Flores, H. E-mail: ycliang@bao.ac.cn

    2014-08-10

    We compare the host galaxies of 902 supernovae (SNe), including SNe Ia, SNe II, and SNe Ibc, which are selected by cross-matching the Asiago Supernova Catalog with the Sloan Digital Sky Survey (SDSS) Data Release 7. We selected an additional 213 galaxies by requiring the light fraction of spectral observations to be >15%, which could represent well the global properties of the galaxies. Among these 213 galaxies, 135 appear on the Baldwin-Phillips-Terlevich diagram, which allows us to compare the hosts in terms of whether they are star-forming (SF) galaxies, active galactic nuclei (AGNs; including composites, LINERs, and Seyfert 2s) or absorption-line galaxies (Absorps; i.e., their related emission lines are weak or non-existent). The diagrams related to the parameters D{sub n}(4000), H?{sub A}, stellar masses, star formation rates (SFRs), and specific SFRs for the SNe hosts show that almost all SNe II and most of the SNe Ibc occur in SF galaxies, which have a wide range of stellar masses and low D{sub n}(4000). The SNe Ia hosts as SF galaxies following similar trends. A significant fraction of SNe Ia occurs in AGNs and absorption-line galaxies, which are massive and have high D{sub n}(4000). The stellar population analysis from spectral synthesis fitting shows that the hosts of SNe II have a younger stellar population than hosts of SNe Ia. These results are compared with those of the 689 comparison galaxies where the SDSS fiber captures less than 15% of the total light. These comparison galaxies appear biased toward higher 12+log(O/H) (?0.1 dex) at a given stellar mass. Therefore, we believe the aperture effect should be kept in mind when the properties of the hosts for different types of SNe are discussed.

  2. Optical and ultraviolet observations of the narrow-lined type Ia SN 2012fr in NGC 1365

    SciTech Connect (OSTI)

    Zhang, Ju-Jia; Bai, Jin-Ming; Wang, Bo; Liu, Zheng-Wei [Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650011 (China); Wang, Xiao-Feng; Zhao, Xu-Lin; Chen, Jun-Cheng [Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing 100084 (China); Zhang, Tian-Meng, E-mail: jujia@ynao.ac.cn, E-mail: baijinming@ynao.ac.cn, E-mail: wang_xf@mail.tsinghua.edu.cn [National Astronomical Observatories of China (NAOC), Chinese Academy of Sciences, Beijing 100012 (China)

    2014-07-01

    Extensive optical and ultraviolet (UV) observations of the type Ia supernova (SN Ia) 2012fr are presented in this paper. It has a relatively high luminosity, with an absolute B-band peak magnitude of about 19.5 mag and a smaller post-maximum decline rate than normal SNe Ia (e.g., ?m {sub 15}(B) =0.85 0.05 mag). Based on the UV and optical light curves, we derived that a {sup 56}Ni mass of about 0.88 M {sub ?} was synthesized in the explosion. The earlier spectra are characterized by noticeable high-velocity features of Si II ?6355 and Ca II with velocities in the range of ?22, 000-25, 000 km s{sup 1}. At around the maximum light, these spectral features are dominated by the photospheric components which are noticeably narrower than normal SNe Ia. The post-maximum velocity of the photosphere remains almost constant at ?12,000 km s{sup 1} for about one month, reminiscent of the behavior of some luminous SNe Ia like SN 1991T. We propose that SN 2012fr may represent a subset of the SN 1991T-like SNe Ia viewed in a direction with a clumpy or shell-like structure of ejecta, in terms of a significant level of polarization reported in Maund et al. in 2013.

  3. NREL: Energy Analysis - Daniel Inman

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

    Systems and Sustainability Analysis Group in the Strategic Energy Analysis Center. ... Primary research interests Sustainability analysis Biomass Scenario Model Education and ...

  4. Daniel Lopez | Argonne National Laboratory

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

    Lopez Group Leader, Nanofabrication & Devices Ph.D., Instituto Balseiro, Bariloche, Argentina Nano and micro electro mechanical systems (NEMS/MEMS) for high-impact applications in science and technology, spatial light modulators for use in medical instrumentation, X-ray manipulation nanomanufacturing and optical communications; nonlinear dynamics of nanoscale devices News Manipulating X-rays with Tiny Mirrors Scientists tune X-rays with tiny mirrors Nano-mechanical plasmonic phase modulator

  5. Daniel Rosenmann | Argonne National Laboratory

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

    Rosenmann Principal Engineering Specialist Synthesis of high-quality superconducting, metallic, and dielectric films as well as metamaterials structures for plasmonic and nanophotonics applications. Focus on the development of novel "smart probes" which act as detectors for synchrotron x-ray scanning tunneling microscopy (SX-STM) applications. News Dialing in the Properties of Dual Metallic-Insulating Materials Fast Times and Hot Spots in Plasmonic Nanostructures Combining Elemental

  6. Daniel Yergin | Department of Energy

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

    ... Yergin co-founded IHS Cambridge Energy Research Associates. Its offices are in Cambridge, Massachusetts, Beijing, Calgary, Dubai, Mexico City, Moscow, Oslo, Paris, San Francisco, ...

  7. 1,"Victor J Daniel Jr","Coal","Mississippi Power Co",1992 2,"Grand Gulf","Nuclear","System Energy Resources, Inc",1408.5

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

    Mississippi" ,"Plant","Primary energy source","Operating company","Net summer capacity (MW)" 1,"Victor J Daniel Jr","Coal","Mississippi Power Co",1992 2,"Grand Gulf","Nuclear","System Energy Resources, Inc",1408.5 3,"Baxter Wilson","Natural gas","Entergy Mississippi Inc",1143.2 4,"Jack Watson","Coal","Mississippi Power Co",998

  8. O:\IM-20\E-Government Program Office\FDMS\FDMS database\DOE\2011\DOE-HQ-2011-0014 - Daniel Cohen - GC\Comments from FDMS\Dan Manole DRAFT-0004.html

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

    14%20-%20Daniel%20Cohen%20-%20GC/Comments%20from%20FDMS/Dan%20Manole%20DRAFT-0004.html[3/23/2011 2:21:55 PM] PUBLIC SUBMISSION As of: March 23, 2011 Received: March 21, 2011 Status: Pending_Post Tracking No. 80c0d039 Comments Due: April 04, 2011 Submission Type: Web Docket: DOE-HQ-2011-0014 Reducing Regulatory Burden Comment On: DOE-HQ-2011-0014-0001 Reducing Regulatory Burden Document: DOE-HQ-2011-0014-DRAFT-0004 Comment on FR Doc # 2011-02368 Submitter Information Name: Dan Manole Address:

  9. A SUPER-EDDINGTON WIND SCENARIO FOR THE PROGENITORS OF TYPE Ia SUPERNOVAE

    SciTech Connect (OSTI)

    Ma, Xin; Chen, Xuefei; Chen, Hai-liang; Han, Zhanwen; Denissenkov, Pavel A. E-mail: cxf@ynao.ac.cn

    2013-12-01

    The accretion of hydrogen-rich material on to carbon-oxygen white dwarfs (CO WDs) is crucial for understanding Type Ia supernova (SN Ia) from the single-degenerate model, but this process has not been well understood due to the numerical difficulties in treating H and He flashes during the accretion. For CO WD masses from 0.5 to 1.378 M {sub ?} and accretion rates in the range from 10{sup 8} to 10{sup 5} M {sub ?} yr{sup 1}, we simulated the accretion of solar-composition material on to CO WDs using the state-of-the-art stellar evolution code of MESA. For comparison with steady-state models, we first ignored the contribution from nuclear burning to the luminosity when determining the Eddington accretion rate, and found that the properties of H burning in our accreting CO WD models are similar to those from the steady-state models, except that the critical accretion rates at which the WDs turn into red giants or H-shell flashes occur on their surfaces are slightly higher than those from the steady-state models. However, the super-Eddington wind is triggered at much lower accretion rates than previously thought, when the contribution of nuclear burning to the total luminosity is included. This super-Eddington wind naturally prevents the CO WDs with high accretion rates from becoming red giants, thus presenting an alternative to the optically thick wind proposed by Hachisu etal. Furthermore, the super-Eddington wind works in low-metallicity environments, which may explain SNe Ia observed at high redshifts.

  10. SPECTROPOLARIMETRY OF THE TYPE Ia SN 2007sr TWO MONTHS AFTER MAXIMUM LIGHT

    SciTech Connect (OSTI)

    Zelaya, P.; Quinn, J. R.; Clocchiatti, A.; Baade, D.; Patat, F.; Hoeflich, P.; Maund, J.; Wang, L.; Wheeler, J. C.

    2013-02-01

    We present late-time spectropolarimetric observations of SN 2007sr, obtained with the Very Large Telescope at the ESO Paranal Observatory when the object was 63 days after maximum light. The late-time spectrum displays strong line polarization in the Ca II absorption features. SN 2007sr adds to the case of some normal Type Ia supernovae that show high line polarization or repolarization at late times, a fact that might be connected with the presence of high-velocity features at early times.

  11. Spectroscopic Determination of the Low Redshift Type Ia Supernova Rate from the Sloan Digital Sky Survey

    SciTech Connect (OSTI)

    Krughoff, K. S.; Connolly, Andrew J.; Frieman, Joshua; SubbaRao, Mark; Kilper, Gary; Schneider, Donald P.

    2011-04-10

    Supernova rates are directly coupled to high mass stellar birth and evolution. As such, they are one of the few direct measures of the history of cosmic stellar evolution. In this paper we describe an probabilistic technique for identifying supernovae within spectroscopic samples of galaxies. We present a study of 52 type Ia supernovae ranging in age from -14 days to +40 days extracted from a parent sample of \\simeq 50,000 spectra from the SDSS DR5. We find a Supernova Rate (SNR) of 0.472^{+0.048}_{-0.039}(Systematic)^{+0.081}_{-0.071}(Statistical)SNu at a redshift of = 0.1. This value is higher than other values at low redshift at the 1{\\sigma}, but is consistent at the 3{\\sigma} level. The 52 supernova candidates used in this study comprise the third largest sample of supernovae used in a type Ia rate determination to date. In this paper we demonstrate the potential for the described approach for detecting supernovae in future spectroscopic surveys.

  12. TYCHO SN 1572: A NAKED Ia SUPERNOVA REMNANT WITHOUT AN ASSOCIATED AMBIENT MOLECULAR CLOUD

    SciTech Connect (OSTI)

    Tian, W. W.; Leahy, D. A.

    2011-03-10

    The historical supernova remnant (SNR) Tycho SN 1572 originates from the explosion of a normal Type Ia supernova that is believed to have originated from a carbon-oxygen white dwarf in a binary system. We analyze the 21 cm continuum, H I, and {sup 12}CO-line data from the Canadian Galactic Plane Survey in the direction of SN 1572 and the surrounding region. We construct H I absorption spectra to SN 1572 and three nearby compact sources. We conclude that SN 1572 has no molecular cloud interaction, which argues against previous claims that a molecular cloud is interacting with the SNR. This new result does not support a recent claim that dust, newly detected by AKARI, originates from such an SNR-cloud interaction. We suggest that the SNR has a kinematic distance of 2.5-3.0 kpc based on a nonlinear rotational curve model. Very high energy {gamma}-ray emission from the remnant has been detected by the VERITAS telescope, so our result shows that its origin should not be an SNR-cloud interaction. Both radio and X-ray observations support that SN 1572 is an isolated Type Ia SNR.

  13. Spectroscopic Observations and Analysis of the Unusual Type Ia SN1999ac

    SciTech Connect (OSTI)

    Garavini, G.; Aldering, G.; Amadon, A.; Amanullah, R.; Astier,P.; Balland, C.; Blanc, G.; Conley, A.; Dahlen, T.; Deustua, S.E.; Ellis,R.; Fabbro, S.; Fadeyev, V.; Fan, X.; Folatelli, G.; Frye, B.; Gates,E.L.; Gibbons, R.; Goldhaber, G.; Goldman, B.; Goobar, A.; Groom, D.E.; Haissinski, J.; Hardin, D.; Hook, I.; Howell, D.A.; Kent, S.; Kim, A.G.; Knop, R.A.; Kowalski, M.; Kuznetsova, N.; Lee, B.C.; Lidman, C.; Mendez,J.; Miller, G.J.; Moniez, M.; Mouchet, M.; Mourao, A.; Newberg, H.; Nobili, S.; Nugent, P.E.; Pain, R.; Perdereau, O.; Perlmutter, S.; Quimby, R.; Regnault, N.; Rich, J.; Richards, G.T.; Ruiz-Lapuente, P.; Schaefer, B.E.; Schahmaneche, K.; Smith, E.; Spadafora, A.L.; Stanishev,V.; Thomas, R.C.; Walton, N.A.; Wang, L.; Wood-Vasey, W.M.

    2005-07-12

    The authors present optical spectra of the peculiar Type Ia supernova (SN Ia) 1999ac. The data extend from -15 to +42 days with respect to B-band maximum and reveal an event that is unusual in several respects. prior to B-band maximum, the spectra resemble those of SN 1999aa, a slowly declining event, but possess stronger Si II and Ca II signatures (more characteristic of a spectroscopically normal SN). Spectra after B-band maximum appear more normal. The expansion velocities inferred from the Iron lines appear to be lower than average; whereas, the expansion velocity inferred from Calcium H and K are higher than average. The expansion velocities inferred from the Iron lines appear to be lower than average; whereas, the expansion velocity inferred from Calcium H and K are higher than average. The expansion velocities inferred from Si II are among the slowest ever observed, though SN 1999ac is not particularly dim. The analysis of the parameters v{sub 10}(Si II), R(Si II), v, and {Delta}m{sub 15} further underlines the unique characteristics of SN 1999ac. They find convincing evidence of C II {lambda}6580 in the day -15 spectrum with ejection velocity v > 16,000 km s{sup -1}, but this signature disappears by day -9. This rapid evolution at early times highlights the importance of extremely early-time spectroscopy.

  14. Consistent use of type Ia supernovae highly magnified by galaxy clusters to constrain the cosmological parameters

    SciTech Connect (OSTI)

    Zitrin, Adi [Cahill Center for Astronomy and Astrophysics, California Institute of Technology, MS 249-17, Pasadena, CA 91125 (United States); Redlich, Matthias [Universitt Heidelberg, Zentrum fr Astronomie, Institut fr Theoretische Astrophysik, Philosophenweg 12, D-69120 Heidelberg (Germany); Broadhurst, Tom, E-mail: adizitrin@gmail.com [Department of Theoretical Physics, University of Basque Country UPV/EHU, Bilbao (Spain)

    2014-07-01

    We discuss how Type Ia supernovae (SNe) strongly magnified by foreground galaxy clusters should be self-consistently treated when used in samples fitted for the cosmological parameters. While the cluster lens magnification of a SN can be well constrained from sets of multiple images of various background galaxies with measured redshifts, its value is typically dependent on the fiducial set of cosmological parameters used to construct the mass model. In such cases, one should not naively demagnify the observed SN luminosity by the model magnification into the expected Hubble diagram, which would create a bias, but instead take into account the cosmological parameters a priori chosen to construct the mass model. We quantify the effect and find that a systematic error of typically a few percent, up to a few dozen percent per magnified SN may be propagated onto a cosmological parameter fit unless the cosmology assumed for the mass model is taken into account (the bias can be even larger if the SN is lying very near the critical curves). We also simulate how such a bias propagates onto the cosmological parameter fit using the Union2.1 sample supplemented with strongly magnified SNe. The resulting bias on the deduced cosmological parameters is generally at the few percent level, if only few biased SNe are included, and increases with the number of lensed SNe and their redshift. Samples containing magnified Type Ia SNe, e.g., from ongoing cluster surveys, should readily account for this possible bias.

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

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

    Models | Argonne Leadership Computing Facility Toward Exascale Computing of Type Ia and Ib,c Supernovae: V&V of Current Models PI Name: Don Lamb PI Email: lamb@oddjob.uchicago.edu Institution: University Of Chicago Allocation Program: INCITE Allocation Hours at ALCF: 40,000,000 Year: 2012 Research Domain: Physics This project continues a program of verification and validation of Type Ia supernova models. More 3-D simulations of the explosion phase will be performed, along with 2-D

  16. Near-infrared line identification in type Ia supernovae during the transitional phase

    SciTech Connect (OSTI)

    Friesen, Brian; Baron, E.; Wisniewski, John P.; Miller, Timothy R.; Parrent, Jerod T.; Thomas, R. C.; Marion, G. H.

    2014-09-10

    We present near-infrared synthetic spectra of a delayed-detonation hydrodynamical model and compare them to observed spectra of four normal Type Ia supernovae ranging from day +56.5 to day +85. This is the epoch during which supernovae are believed to be undergoing the transition from the photospheric phase, where spectra are characterized by line scattering above an optically thick photosphere, to the nebular phase, where spectra consist of optically thin emission from forbidden lines. We find that most spectral features in the near-infrared can be accounted for by permitted lines of Fe II and Co II. In addition, we find that [Ni II] fits the emission feature near 1.98 μm, suggesting that a substantial mass of {sup 58}Ni exists near the center of the ejecta in these objects, arising from nuclear burning at high density.

  17. LAX XXlCfl jX?iK, Idd+?KYLViG?IA

    Office of Legacy Management (LM)

    f , : I~&l, samtier cipwati8Aa CffUm - . Jiux.lCJ d,# 1754 - - _- - .- t :; . Jesse e. ahizmn*~*ter -2.' -------- - _ &tV' hi@A l f izau Bkteriala ;' . . 1 -7 I _' i' . Fpr&G& r&Q Q,&& fu &fI& L;&& -l&d 2;,i' iI,;/Qi' rIGN CQ&GgJy p;E& p;~p>gyf LAX XXlCfl jX?iK, Idd+?KYLViG?IA i-icfer~~o is &o ta yaw rwarandu3;: l P iimwmbec L?, 1953, reque&in~ a d&q.&ti of khority tA A&sister prog= for th+zz developmrrrl,

  18. EARLY OBSERVATIONS AND ANALYSIS OF THE TYPE Ia SN 2014J IN M82

    SciTech Connect (OSTI)

    Marion, G. H.; Vinkó, J.; Sand, D. J.; Hsiao, E. Y.; Banerjee, D. P. K.; Joshi, V.; Venkataraman, V.; Ashok, N. M.; Valenti, S.; Howell, D. A.; Stritzinger, M. D.; Amanullah, R.; Johansson, J.; Binzel, R. P.; Bochanski, J. J.; Bryngelson, G. L.; Burns, C. R.; Drozdov, D.; Fieber-Beyer, S. K.; Graham, M. L.; and others

    2015-01-01

    We present optical and near infrared (NIR) observations of the nearby Type Ia SN 2014J. Seventeen optical and 23 NIR spectra were obtained from 10 days before (–10d) to 10 days after (+10d) the time of maximum B-band brightness. The relative strengths of absorption features and their patterns of development can be compared at one day intervals throughout most of this period. Carbon is not detected in the optical spectra, but we identify C I λ1.0693 in the NIR spectra. Mg II lines with high oscillator strengths have higher initial velocities than other Mg II lines. We show that the velocity differences can be explained by differences in optical depths due to oscillator strengths. The spectra of SN 2014J show that it is a normal SN Ia, but many parameters are near the boundaries between normal and high-velocity subclasses. The velocities for O I, Mg II, Si II, S II, Ca II, and Fe II suggest that SN 2014J has a layered structure with little or no mixing. That result is consistent with the delayed detonation explosion models. We also report photometric observations, obtained from –10d to +29d, in the UBVRIJH and K{sub s} bands. The template fitting package SNooPy is used to interpret the light curves and to derive photometric parameters. Using R{sub V} = 1.46, which is consistent with previous studies, SNooPy finds that A{sub V} = 1.80 for E(B – V){sub host} = 1.23 ± 0.06 mag. The maximum B-band brightness of –19.19 ± 0.10 mag was reached on February 1.74 UT ± 0.13 days and the supernova has a decline parameter, Δm {sub 15}, of 1.12 ± 0.02 mag.

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

    SciTech Connect (OSTI)

    Dilday, Benjamin; Smith, Mathew; Bassett, Bruce; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Filippenko, Alexei V.; Frieman, Joshua A.; Galbany, Lluis; Garnavich, Peter M.; /Notre Dame U. /Stockholm U., OKC /Stockholm U.

    2010-01-01

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

  20. EVOLUTION OF POST-IMPACT REMNANT HELIUM STARS IN TYPE Ia SUPERNOVA REMNANTS WITHIN THE SINGLE-DEGENERATE SCENARIO

    SciTech Connect (OSTI)

    Pan, Kuo-Chuan; Ricker, Paul M.; Taam, Ronald E. E-mail: pmricker@illinois.edu

    2013-08-10

    The progenitor systems of Type Ia supernovae (SNe Ia) are still under debate. Based on recent hydrodynamics simulations, non-degenerate companions in the single-degenerate scenario (SDS) should survive the supernova (SN) impact. One way to distinguish between the SDS and the double-degenerate scenario is to search for the post-impact remnant stars (PIRSs) in SN Ia remnants. Using a technique that combines multi-dimensional hydrodynamics simulations with one-dimensional stellar evolution simulations, we have examined the post-impact evolution of helium-rich binary companions in the SDS. It is found that these helium-rich PIRSs (He PIRSs) dramatically expand and evolve to a luminous phase (L {approx} 10{sup 4} L{sub Sun }) about 10 yr after an SN explosion. Subsequently, they contract and evolve to become hot blue-subdwarf-like (sdO-like) stars by releasing gravitational energy, persisting as sdO-like stars for several million years before evolving to the helium red-giant phase. We therefore predict that a luminous OB-like star should be detectable within {approx}30 yr after the SN explosion. Thereafter, it will shrink and become an sdO-like star in the central regions of SN Ia remnants within star-forming regions for SN Ia progenitors evolved via the helium-star channel in the SDS. These He PIRSs are predicted to be rapidly rotating (v{sub rot} {approx}> 50 km s{sup -1}) and to have high spatial velocities (v{sub linear} {approx}> 500 km s{sup -1}). Furthermore, if SN remnants have diffused away and are not recognizable at a later stage, He PIRSs could be an additional source of single sdO stars and/or hypervelocity stars.

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

    SciTech Connect (OSTI)

    Dilday, Benjamin; Bassett, Bruce; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Frieman, Joshua A.; Galbany, Lluis; Garnavich, Peter; Goobar, Ariel; Hopp, Ulrich; /Munich, Tech. U. /Munich U. Observ. /Tokyo U.

    2010-03-01

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

  2. PRODUCTION OF THE p-PROCESS NUCLEI IN THE CARBON-DEFLAGRATION MODEL FOR TYPE Ia SUPERNOVAE

    SciTech Connect (OSTI)

    Kusakabe, Motohiko; Iwamoto, Nobuyuki; Nomoto, Ken'ichi E-mail: iwamoto.nobuyuki@jaea.go.jp

    2011-01-01

    We calculate the nucleosynthesis of proton-rich isotopes in the carbon-deflagration model for Type Ia supernovae (SNe Ia). The seed abundances are obtained by calculating the s-process nucleosynthesis that is expected to occur in the repeating helium shell flashes on the carbon-oxygen (CO) white dwarf (WD) during mass accretion from a binary companion. When the deflagration wave passes through the outer layer of the CO WD, p-nuclei are produced by photodisintegration reactions on s-nuclei in a region where the peak temperature ranges from 1.9 to 3.6 x 10{sup 9} K. We confirm the sensitivity of the p-process on the initial distribution of s-nuclei. We show that the initial C/O ratio in the WD does not affect much the yield of p-nuclei. On the other hand, the abundance of {sup 22}Ne left after s-processing has a large influence on the p-process via the {sup 22}Ne({alpha},n) reaction. We find that about 50% of p-nuclides are co-produced when normalized to their solar abundances in all adopted cases of seed distribution. Mo and Ru, which are largely underproduced in Type II supernovae (SNe II), are produced more than in SNe II although they are underproduced with respect to the yield levels of other p-nuclides. The ratios between p-nuclei and iron in the ejecta are larger than the solar ratios by a factor of 1.2. We also compare the yields of oxygen, iron, and p-nuclides in SNe Ia and SNe II and suggest that SNe Ia could make a larger contribution than SNe II to the solar system content of p-nuclei.

  3. The crossing statistic: dealing with unknown errors in the dispersion of Type Ia supernovae

    SciTech Connect (OSTI)

    Shafieloo, Arman; Clifton, Timothy; Ferreira, Pedro E-mail: tclifton@astro.ox.ac.uk

    2011-08-01

    We propose a new statistic that has been designed to be used in situations where the intrinsic dispersion of a data set is not well known: The Crossing Statistic. This statistic is in general less sensitive than χ{sup 2} to the intrinsic dispersion of the data, and hence allows us to make progress in distinguishing between different models using goodness of fit to the data even when the errors involved are poorly understood. The proposed statistic makes use of the shape and trends of a model's predictions in a quantifiable manner. It is applicable to a variety of circumstances, although we consider it to be especially well suited to the task of distinguishing between different cosmological models using type Ia supernovae. We show that this statistic can easily distinguish between different models in cases where the χ{sup 2} statistic fails. We also show that the last mode of the Crossing Statistic is identical to χ{sup 2}, so that it can be considered as a generalization of χ{sup 2}.

  4. FIRST EVIDENCE OF GLOBULAR CLUSTER FORMATION FROM THE EJECTA OF PROMPT TYPE Ia SUPERNOVAE

    SciTech Connect (OSTI)

    Tsujimoto, Takuji [National Astronomical Observatory of Japan, Mitaka-shi, Tokyo 181-8588 (Japan); Bekki, Kenji, E-mail: taku.tsujimoto@nao.ac.jp [ICRAR, M468, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009 (Australia)

    2012-06-01

    Recent spectroscopic observations of globular clusters (GCs) in the Large Magellanic Cloud (LMC) have discovered that one of the intermediate-age GCs, NGC 1718, with [Fe/H] = -0.7 has an extremely low [Mg/Fe] ratio of {approx}-0.9. We propose that NGC 1718 was formed from the ejecta of Type Ia supernovae mixed with very metal-poor ([Fe/H] <-1.3) gas about {approx}2 Gyr ago. The proposed scenario is shown to be consistent with the observed abundances of Fe-group elements such as Cr, Mn, and Ni. In addition, compelling evidence for asymptotic giant branch stars playing a role in chemical enrichment during this GC formation is found. We suggest that the origin of the metal-poor gas is closely associated with efficient gas transfer from the outer gas disk of the Small Magellanic Cloud to the LMC disk. We anticipate that the outer part of the LMC disk contains field stars exhibiting significantly low [Mg/Fe] ratios, formed through the same process as NGC 1718.

  5. Constraints on the progenitor system of the type Ia supernova 2014J from pre-explosion Hubble space telescope imaging

    SciTech Connect (OSTI)

    Kelly, Patrick L.; Fox, Ori D.; Filippenko, Alexei V.; Shen, Ken J.; Zheng, WeiKang; Graham, Melissa L.; Tucker, Brad E.; Cenko, S. Bradley; Schaefer, Gail

    2014-07-20

    We constrain the properties of the progenitor system of the highly reddened Type Ia supernova (SN Ia) 2014J in Messier 82 (M82; d ? 3.5 Mpc). We determine the supernova (SN) location using Keck-II K-band adaptive optics images, and we find no evidence for flux from a progenitor system in pre-explosion near-ultraviolet through near-infrared Hubble Space Telescope (HST) images. Our upper limits exclude systems having a bright red giant companion, including symbiotic novae with luminosities comparable to that of RS Ophiuchi. While the flux constraints are also inconsistent with predictions for comparatively cool He-donor systems (T ? 35,000 K), we cannot preclude a system similar to V445 Puppis. The progenitor constraints are robust across a wide range of R{sub V} and A{sub V} values, but significantly greater values than those inferred from the SN light curve and spectrum would yield proportionally brighter luminosity limits. The comparatively faint flux expected from a binary progenitor system consisting of white dwarf stars would not have been detected in the pre-explosion HST imaging. Infrared HST exposures yield more stringent constraints on the luminosities of very cool (T < 3000 K) companion stars than was possible in the case of SN Ia 2011fe.

  6. Metabolomic profiling of the nectars of Aquilegia pubescens and <i>A. Canadensis

    SciTech Connect (OSTI)

    Noutsos, Christos; Perera, Ann M.; Nikolau, Basil J.; Seaver, Samuel M. D.; Ware, Doreen H.; Motta, Andrea

    2015-05-01

    To date, variation in nectar chemistry of flowering plants has not been studied in detail. Such variation exerts considerable influence on pollinator–plant interactions, as well as on flower traits that play important roles in the selection of a plant for visitation by specific pollinators. Over the past 60 years the Aquilegia genus has been used as a key model for speciation studies. In this study, we defined the metabolomic profiles of flower samples of two Aquilegia species, <i>A. Canadensis and <i>A. pubescens. We identified a total of 75 metabolites that were classified into six main categories: organic acids, fatty acids, amino acids, esters, sugars, and unknowns. The mean abundances of 25 of these metabolites were significantly different between the two species, providing insights into interspecies variation in floral chemistry. Using the PlantSEED biochemistry database, we found that the majority of these metabolites are involved in biosynthetic pathways. Finally, we explored the annotated genome of <i>A. coerulea, using the PlantSEED pipeline and reconstructed the metabolic network of Aquilegia. This network, which contains the metabolic pathways involved in generating the observed chemical variation, is now publicly available from the DOE Systems Biology Knowledge Base (KBase; http://kbase.us).

  7. Spectroscopic Properties of Star-Forming Host Galaxies and Type Ia Supernova Hubble Residuals in a Nearly Unbiased Sample

    SciTech Connect (OSTI)

    D'Andrea, Chris B.; et al.

    2011-12-20

    We examine the correlation between supernova host galaxy properties and their residuals on the Hubble diagram. We use supernovae discovered during the Sloan Digital Sky Survey II - Supernova Survey, and focus on objects at a redshift of z < 0.15, where the selection effects of the survey are known to yield a complete Type Ia supernova sample. To minimize the bias in our analysis with respect to measured host-galaxy properties, spectra were obtained for nearly all hosts, spanning a range in magnitude of -23 < M_r < -17. In contrast to previous works that use photometric estimates of host mass as a proxy for global metallicity, we analyze host-galaxy spectra to obtain gas-phase metallicities and star-formation rates from host galaxies with active star formation. From a final sample of ~ 40 emission-line galaxies, we find that light-curve corrected Type Ia supernovae are ~ 0.1 magnitudes brighter in high-metallicity hosts than in low-metallicity hosts. We also find a significant (> 3{\\sigma}) correlation between the Hubble residuals of Type Ia supernovae and the specific star-formation rate of the host galaxy. We comment on the importance of supernova/host-galaxy correlations as a source of systematic bias in future deep supernova surveys.

  8. A POSSIBLE EVOLUTIONARY SCENARIO OF HIGHLY MAGNETIZED SUPER-CHANDRASEKHAR WHITE DWARFS: PROGENITORS OF PECULIAR TYPE Ia SUPERNOVAE

    SciTech Connect (OSTI)

    Das, Upasana; Mukhopadhyay, Banibrata; Rao, A. R. E-mail: bm@physics.iisc.ernet.in

    2013-04-10

    Several recently discovered peculiar Type Ia supernovae seem to demand an altogether new formation theory that might help explain the puzzling dissimilarities between them and the standard Type Ia supernovae. The most striking aspect of the observational analysis is the necessity of invoking super-Chandrasekhar white dwarfs having masses {approx}2.1-2.8 M{sub Sun }, M{sub Sun} being the mass of Sun, as their most probable progenitors. Strongly magnetized white dwarfs having super-Chandrasekhar masses have already been established as potential candidates for the progenitors of peculiar Type Ia supernovae. Owing to the Landau quantization of the underlying electron degenerate gas, theoretical results yielded the observationally inferred mass range. Here, we sketch a possible evolutionary scenario by which super-Chandrasekhar white dwarfs could be formed by accretion on to a commonly observed magnetized white dwarf, invoking the phenomenon of flux freezing. This opens multiple possible evolution scenarios ending in supernova explosions of super-Chandrasekhar white dwarfs having masses within the range stated above. We point out that our proposal has observational support, such as the recent discovery of a large number of magnetized white dwarfs by the Sloan Digital Sky Survey.

  9. Radiogenic p-isotopes from type Ia supernova, nuclear physics uncertainties, and galactic chemical evolution compared with values in primitive meteorites

    SciTech Connect (OSTI)

    Travaglio, C.; Gallino, R.; Rauscher, T.; Dauphas, N.; Rpke, F. K.; Hillebrandt, W. E-mail: claudia.travaglio@b2fh.org

    2014-11-10

    The nucleosynthesis of proton-rich isotopes is calculated for multi-dimensional Chandrasekhar-mass models of Type Ia supernovae (SNe Ia) with different metallicities. The predicted abundances of the short-lived radioactive isotopes {sup 92}Nb, {sup 97,} {sup 98}Tc, and {sup 146}Sm are given in this framework. The abundance seeds are obtained by calculating s-process nucleosynthesis in the material accreted onto a carbon-oxygen white dwarf from a binary companion. A fine grid of s-seeds at different metallicities and {sup 13}C-pocket efficiencies is considered. A galactic chemical evolution model is used to predict the contribution of SN Ia to the solar system p-nuclei composition measured in meteorites. Nuclear physics uncertainties are critical to determine the role of SNe Ia in the production of {sup 92}Nb and {sup 146}Sm. We find that, if standard Chandrasekhar-mass SNe Ia are at least 50% of all SN Ia, they are strong candidates for reproducing the radiogenic p-process signature observed in meteorites.

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

    SciTech Connect (OSTI)

    Jordan, G. C. IV; Graziani, C.; Weide, K.; Norris, J.; Hudson, R.; Lamb, D. Q.; Fisher, R. T.; Townsley, D. M.; Meakin, C.; Reid, L. B.

    2012-11-01

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

  11. Persistent C II absorption in the normal type Ia supernova 2002fk

    SciTech Connect (OSTI)

    Cartier, Rgis; Zelaya, Paula [Millennium Institute of Astrophysics, Casilla 36-D, Santiago (Chile); Hamuy, Mario; Maza, Jos; Gonzlez, Luis; Huerta, Leonor [Departamento de Astronoma, Universidad de Chile, Casilla 36-D, Santiago (Chile); Pignata, Giuliano [Departamento Ciencias Fisicas, Universidad Andres Bello, Av. Repblica 252, Santiago (Chile); Frster, Francisco [Center for Mathematical Modelling, Universidad de Chile, Avenida Blanco Encalada 2120, Piso 7, Santiago (Chile); Folatelli, Gaston [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Phillips, Mark M.; Morrell, Nidia; Contreras, Carlos; Roth, Miguel; Gonzlez, Sergio [Carnegie Institution of Washington, Las Campanas Observatory, Colina el Pino s/n, Casilla 601 (Chile); Krisciunas, Kevin; Suntzeff, Nicholas B. [Department of Physics and Astronomy, Texas A and M University, 4242 TAMU, College Station, TX 77843 (United States); Clocchiatti, Alejandro [Departamento de Astronoma y Astrofsica, Pontificia Universidad Catlica de Chile, Casilla 306, Santiago (Chile); Coppi, Paolo [Department of Astronomy, Yale University, New Haven, CT 06520-8101 (United States); Koviak, Kathleen, E-mail: rcartier@das.uchile.cl [Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 911901 (United States)

    2014-07-01

    We present well-sampled UBVRIJHK photometry of SN 2002fk starting 12 days before maximum light through 122 days after peak brightness, along with a series of 15 optical spectra from 4 to +95 days since maximum. Our observations show the presence of C II lines in the early-time spectra of SN 2002fk, expanding at 11,000 km s{sup 1} and persisting until 8 days past maximum light with a velocity of ?9000 km s{sup 1}. SN 2002fk is characterized by a small velocity gradient of v-dot {sub Si} {sub II}=26 km s{sup 1} day{sup 1}, possibly caused by an off-center explosion with the ignition region oriented toward the observer. The connection between the viewing angle of an off-center explosion and the presence of C II in the early-time spectrum suggests that the observation of C II could be also due to a viewing angle effect. Adopting the Cepheid distance to NGC 1309 we provide the first H {sub 0} value based on near-infrared (near-IR) measurements of a Type Ia supernova (SN) between 63.0 0.8 (3.4 systematic) and 66.7 1.0 (3.5 systematic) km s{sup 1} Mpc{sup 1}, depending on the absolute magnitude/decline rate relationship adopted. It appears that the near-IR yields somewhat lower (6%-9%) H {sub 0} values than the optical. It is essential to further examine this issue by (1) expanding the sample of high-quality near-IR light curves of SNe in the Hubble flow, and (2) increasing the number of nearby SNe with near-IR SN light curves and precise Cepheid distances, which affords the promise to deliver a more precise determination of H {sub 0}.

  12. MID-IR SPECTRA OF TYPE Ia SN 2014J IN M82 SPANNING THE FIRST 4 MONTHS

    SciTech Connect (OSTI)

    Telesco, Charles M.; Li, Dan; Barnes, Peter J.; Mariñas, Naibí; Zhang, Han; Höflich, Peter; Álvarez, Carlos; Fernández, Sergio; Rebolo, Rafael; Hough, James H.; Levenson, N. A.; Pantin, Eric; Roche, Patrick E-mail: phoeflich77@gmail.com

    2015-01-10

    We present a time series of 8-13 μm spectra and photometry for SN 2014J obtained 57, 81, 108, and 137 days after the explosion using CanariCam on the Gran Telescopio Canarias. This is the first mid-IR time series ever obtained for a Type Ia supernova (SN Ia). These observations can be understood within the framework of the delayed detonation model and the production of ∼0.6 M {sub ☉} of {sup 56}Ni, consistent with the observed brightness, the brightness decline relation, and the γ-ray fluxes. The [Co III] line at 11.888 μm is particularly useful for evaluating the time evolution of the photosphere and measuring the amount of {sup 56}Ni and thus the mass of the ejecta. Late-time line profiles of SN 2014J are rather symmetric and not shifted in the rest frame. We see argon emission, which provides a unique probe of mixing in the transition layer between incomplete burning and nuclear statistical equilibrium. We may see [Fe III] and [Ni IV] emission, both of which are observed to be substantially stronger than indicated by our models. If the latter identification is correct, then we are likely observing stable Ni, which might imply central mixing. In addition, electron capture, also required for stable Ni, requires densities larger than ∼1 × 10{sup 9} g cm{sup –3}, which are expected to be present only in white dwarfs close to the Chandrasekhar limit. This study demonstrates that mid-IR studies of SNe Ia are feasible from the ground and provide unique information, but it also indicates the need for better atomic data.

  13. 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}.

  14. Nearby Supernova Factory Observations of SN 2005gj: Another TypeIa Supernova in a Massive Circumstellar Envelope

    SciTech Connect (OSTI)

    Aldering, G.; Antilogus, P.; Bailey, S.; Baltay, C.; Bauer, A.; Blanc, N.; Bongard, S.; Copin, Y.; Gangler, E.; Gilles, S.; Kessler, R.; Kocevski, D.; Lee, B.C.; Loken, S.; Nugent, P.; Pain, R.; Pecontal, E.; Pereira, R.; Perlmutter, S.; Rabinowitz, D.; Rigaudier, G.; Scalzo, R.; Smadja, G.; Thomas, R.C.; Wang, L.; Weaver, B.A.; Rabinowitz, D.; Bauer, A.

    2006-06-01

    We report the independent discovery and follow-up observations of supernova 2005gj by the Nearby Supernova Factory. This is the second confirmed case of a ''hybrid'' Type Ia/IIn supernova, which like the prototype SN 2002ic, we interpret as the explosion of a white dwarf interacting with a circumstellar medium. Our early-phase photometry of SN 2005gj shows that the strength of the interaction between the supernova ejecta and circumstellar material is much stronger than for SN 2002ic. Our .rst spectrum shows a hot continuum with broad and narrow H{alpha} emission. Later spectra, spanning over 4 months from outburst, show clear Type Ia features combined with broad and narrow H{gamma}, H{beta},H{alpha} and He I {lambda}{lambda}5876,7065 in emission. At higher resolution, P Cygni profiles are apparent. Surprisingly, we also observe an inverted P Cygni profile for [O III] {lambda}5007. We find that the lightcurve and measured velocity of the unshocked circumstellar material imply mass loss as recently as 8 years ago. This is in contrast to SN 2002ic, for which an inner cavity in the circumstellar material was inferred. Within the context of the thin-shell approximation, the early lightcurve is well-described by a flat radial density profile for the circumstellar material. However, our decomposition of the spectra into Type Ia and shock emission components allows for little obscuration of the supernova, suggesting an aspherical or clumpy distribution for the circumstellar material. We suggest that the emission line velocity profiles arise from electron scattering rather than the kinematics of the shock. This is supported by the inferred high densities, and the lack of evidence for evolution in the line widths. Ground- and space-based photometry, and Keck spectroscopy, of the host galaxy are used to ascertain that the host galaxy has low metallicity (Z/Z{sub {circle_dot}} < 0.3; 95% confidence) and that this galaxy is undergoing a significant star formation event that

  15. DISPLAYING THE HETEROGENEITY OF THE SN 2002cx-LIKE SUBCLASS OF TYPE Ia SUPERNOVAE WITH OBSERVATIONS OF THE Pan-STARRS-1 DISCOVERED SN 2009ku

    SciTech Connect (OSTI)

    Narayan, G.; Foley, R. J.; Berger, E.; Chornock, R.; Rest, A.; Soderberg, A. M.; Kirshner, R. P.; Botticella, M. T.; Smartt, S.; Valenti, S.; Huber, M. E.; Scolnic, D.; Grav, T.; Burgett, W. S.; Chambers, K. C.; Flewelling, H. A.; Gates, G.; Kaiser, N.; Magnier, E. A.; Morgan, J. S. E-mail: rfoley@cfa.harvard.edu

    2011-04-10

    SN 2009ku, discovered by Pan-STARRS-1, is a Type Ia supernova (SN Ia), and a member of the distinct SN 2002cx-like class of SNe Ia. Its light curves are similar to the prototypical SN 2002cx, but are slightly broader and have a later rise to maximum in g. SN 2009ku is brighter ({approx}0.6 mag) than other SN 2002cx-like objects, peaking at M{sub V} = -18.4 mag, which is still significantly fainter than typical SNe Ia. SN 2009ku, which had an ejecta velocity of {approx}2000 km s{sup -1} at 18 days after maximum brightness, is spectroscopically most similar to SN 2008ha, which also had extremely low-velocity ejecta. However, SN 2008ha had an exceedingly low luminosity, peaking at M{sub V} = -14.2 mag, {approx}4 mag fainter than SN 2009ku. The contrast of high luminosity and low ejecta velocity for SN 2009ku is contrary to an emerging trend seen for the SN 2002cx class. SN 2009ku is a counterexample of a previously held belief that the class was more homogeneous than typical SNe Ia, indicating that the class has a diverse progenitor population and/or complicated explosion physics. As the first example of a member of this class of objects from the new generation of transient surveys, SN 2009ku is an indication of the potential for these surveys to find rare and interesting objects.

  16. A Chandrasekhar mass progenitor for the Type Ia supernova remnant 3C 397 from the enhanced abundances of nickel and manganese

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

    Yamaguchi, Hiroya; Badenes, Carles; Foster, Adam R.; Bravo, Eduardo; Williams, Brian J.; Maeda, Keiichi; Nobukawa, Masayoshi; Eriksen, Kristoffer A.; Brickhouse, Nancy S.; Petre, Robert; et al

    2015-03-12

    Despite decades of intense efforts, many fundamental aspects of Type Ia supernovae (SNe Ia) remain elusive. One of the major open questions is whether the mass of an exploding white dwarf (WD) is close to the Chandrasekhar limit. Here, we report the detection of strong K-shell emission from stable Fe-peak elements in the Suzaku X-ray spectrum of the Type Ia supernova remnant (SNR) 3C 397. The high Ni/Fe and Mn/Fe mass ratios (0.11–0.24 and 0.018–0.033, respectively) in the hot plasma component that dominates the K-shell emission lines indicate a degree of neutronization in the supernova ejecta that can only bemore » achieved by electron capture in the dense cores of exploding WDs with a near-Chandrasekhar mass. This suggests a single-degenerate origin for 3C 397, since Chandrasekhar mass progenitors are expected naturally if the WD accretes mass slowly from a companion. Altogether with other results supporting the double-degenerate scenario, our work adds to the mounting evidence that both progenitor channels make a significant contribution to the SN Ia rate in star-forming galaxies.« less

  17. A Chandrasekhar mass progenitor for the Type Ia supernova remnant 3C 397 from the enhanced abundances of nickel and manganese

    SciTech Connect (OSTI)

    Yamaguchi, Hiroya; Badenes, Carles; Foster, Adam R.; Bravo, Eduardo; Williams, Brian J.; Maeda, Keiichi; Nobukawa, Masayoshi; Eriksen, Kristoffer A.; Brickhouse, Nancy S.; Petre, Robert; Koyama, Katsuji

    2015-03-12

    Despite decades of intense efforts, many fundamental aspects of Type Ia supernovae (SNe Ia) remain elusive. One of the major open questions is whether the mass of an exploding white dwarf (WD) is close to the Chandrasekhar limit. Here, we report the detection of strong K-shell emission from stable Fe-peak elements in the Suzaku X-ray spectrum of the Type Ia supernova remnant (SNR) 3C 397. The high Ni/Fe and Mn/Fe mass ratios (0.11–0.24 and 0.018–0.033, respectively) in the hot plasma component that dominates the K-shell emission lines indicate a degree of neutronization in the supernova ejecta that can only be achieved by electron capture in the dense cores of exploding WDs with a near-Chandrasekhar mass. This suggests a single-degenerate origin for 3C 397, since Chandrasekhar mass progenitors are expected naturally if the WD accretes mass slowly from a companion. Altogether with other results supporting the double-degenerate scenario, our work adds to the mounting evidence that both progenitor channels make a significant contribution to the SN Ia rate in star-forming galaxies.

  18. Daniel Udwary NERSC Data Science Engagement Group"

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

    23% 20% 6% 3% 1% 1% 1% 0% 10% Genepool Usage By Process (past 6 mo.) usearch* blast* java hmmer* crossmatch R bwa blasr mono other BLAST makes up a very significant portion of...

  19. Daniel Udwary NERSC Data Science Engagement Group"

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

    Feb 8 Mendel+ Legacy Computes Feb 22? Mendel Outage @CRT @OSF Filesystems Scheduler Down6me for power work and networking maintenance ? SeqFS Key Differences Between CoriEdison ...

  20. Daniel M. Weeber | Department of Energy

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

    From 1991 to 1999, he worked for the Internal Revenue Service as the Information Systems Division Chief for the Pittsburgh, Newark, and Buffalo District Offices. Mr. Weeber holds a ...

  1. NREL: Biomass Research - Daniel J. Schell

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

    of the Bioprocess Integration R&D section of the ... Research Interests Integrated biomass processing High solids ... CO, 2005-2013 Senior Biochemical Engineer, NREL, Golden, ...

  2. Telecommunications Environment Daniel M. Fleetwood Abstract

    Office of Scientific and Technical Information (OSTI)

    ... Microprocessors, linear ICs, combinational logic, and even flash memories can present ... R. S c h w a D. K Nichols, and A. H. Johnston, "SEU in Flash Memories," IEEE Trans. Nucl. ...

  3. Korea Midland Power Co Ltd KOMIPO | Open Energy Information

    Open Energy Info (EERE)

    Seoul, Korea (Republic) Zip: 135 791 Sector: Renewable Energy Product: Korea-based on-grid power generator that is active in investing into renewable energy. Coordinates:...

  4. Platform, Delaware Basin, and Midland Basin, West Texas and New...

    Office of Scientific and Technical Information (OSTI)

    The two primary emphases were on: (1) delineating the temporal and spatial evolution of the regional stress state; and (2) calculating the amount of regional shortening...

  5. Midland, North Carolina: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    North Carolina: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 35.2273656, -80.5006219 Show Map Loading map... "minzoom":false,"mappingservice...

  6. DOE Zero Energy Ready Home Case Study: Cobblestone Homes, Midland...

    Energy Savers [EERE]

    heel trusses, closed-cell spray foam over the top plates, and 15 inches of blown cellulose; a basement insulated with1-inch of rigid XPS foam on the inside and the outside of...

  7. Midland Park, New Jersey: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Park, New Jersey: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.9892643, -74.1406988 Show Map Loading map... "minzoom":false,"mappingservi...

  8. 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.

  9. No X-rays from the very nearby type Ia SN 2014J: Constraints on its environment

    SciTech Connect (OSTI)

    Margutti, R.; Parrent, J.; Kamble, A.; Soderberg, A. M.; Milisavljevic, D.; Drout, M. R.; Kirshner, R. [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States); Foley, R. J. [Astronomy Department, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801 (United States)

    2014-07-20

    Deep X-ray observations of the post-explosion environment around the very nearby Type Ia SN 2014J (d{sub L} = 3.5 Mpc) reveal no X-ray emission down to a luminosity L{sub x} < 7 10{sup 36} erg s{sup 1} (0.3-10 keV) at ?t ? 20 days after the explosion. We interpret this limit in the context of inverse Compton emission from upscattered optical photons by the supernova shock and constrain the pre-explosion mass-loss rate of the stellar progenitor system to be M-dot <10{sup ?9} M{sub ?} yr{sup ?1} (for wind velocity v{sub w} = 100 km s{sup 1}). Alternatively, the SN shock might be expanding into a uniform medium with density n{sub CSM} < 3 cm{sup 3}. These results rule out single-degenerate (SD) systems with steady mass loss until the terminal explosion and constrain the fraction of transferred material lost at the outer Lagrangian point to be ?1%. The allowed progenitors are (1) white dwarf-white dwarf progenitors, (2) SD systems with unstable hydrogen burning experiencing recurrent nova eruptions with recurrence time t < 300 yr, and (3) stars where the mass loss ceases before the explosion.

  10. ASYMMETRY IN THE OBSERVED METAL-RICH EJECTA OF THE GALACTIC TYPE IA SUPERNOVA REMNANT G299.22.9

    SciTech Connect (OSTI)

    Post, Seth; Park, Sangwook [Department of Physics, University of Texas at Arlington, Arlington, Box 19059, TX 76019 (United States); Badenes, Carles [Department of Physics and Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT-PACC), University of Pittsburgh, 3941 OHara Street, Pittsburgh, PA 15260 (United States); Burrows, David N. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Hughes, John P. [Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854-8019 (United States); Lee, Jae-Joon [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of); Mori, Koji [Department of Applied Physics, University of Miyazaki, 1-1 Gakuen Kibana-dai Nishi, Miyazaki 889-2192 (Japan); Slane, Patrick O., E-mail: seth.post@mavs.uta.edu, E-mail: badenes@pitt.edu, E-mail: burrows@astro.psu.edu, E-mail: jph@physics.rutgers.edu, E-mail: mori@astro.miyazaki-u.ac.jp, E-mail: slane@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

    2014-09-01

    We have performed a deep Chandra observation of the Galactic TypeIa supernova remnant G299.22.9. Here we report the initial results from our imaging and spectral analysis. The observed abundance ratios of the central ejecta are in good agreement with those predicted by delayed-detonation TypeIa supernovae models. We reveal inhomogeneous spatial and spectral structures of metal-rich ejecta in G299.22.9. The Fe/Si abundance ratio in the northern part of the central ejecta region is higher than that in the southern part. A significant continuous elongation of ejecta material extends out to the western outermost boundary of the remnant. In this western elongation, both the Si and Fe are enriched with a similar abundance ratio to that in the southern part of the central ejecta region. These structured distributions of metal-rich ejecta material suggest that this TypeIa supernova might have undergone a significantly asymmetric explosion and/or has been expanding into a structured medium.

  11. Expectations for the hard x-ray continuum and gamma-ray line fluxes from the typE IA supernova SN 2014J in M82

    SciTech Connect (OSTI)

    The, Lih-Sin [Department of Physics and Astronomy, Clemson University, SC 29634 (United States); Burrows, Adam, E-mail: tlihsin@clemson.edu, E-mail: burrows@astro.princeton.edu [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)

    2014-05-10

    The hard X-ray continuum and gamma-ray lines from a Type Ia supernova dominate its integrated photon emissions and can provide unique diagnostics of the mass of the ejecta, the {sup 56}Ni yield and spatial distribution, its kinetic energy and expansion speed, and the mechanism of explosion. Such signatures and their time behavior 'X-ray' the bulk debris field in direct fashion, and do not depend on the ofttimes problematic and elaborate UV, optical, and near-infrared spectroscopy and radiative transfer that have informed the study of these events for decades. However, to date no hard photons have ever been detected from a Type Ia supernova in explosion. With the advent of the supernova SN 2014J in M82, at a distance of ?3.5 Mpc, this situation may soon change. Both NuSTAR and INTEGRAL have the potential to detect SN 2014J, and, if spectra and light curves can be measured, would usefully constrain the various explosion models published during the last ?30 yr. In support of these observational campaigns, we provide predictions for the hard X-ray continuum and gamma-line emissions for 15 Type Ia explosion models gleaned from the literature. The model set, containing as it does deflagration, delayed detonation, merger detonation, pulsational delayed detonation, and sub-Chandrasekhar helium detonation models, collectively spans a wide range of properties, and hence signatures. We provide a brief discussion of various diagnostics (with examples), but importantly make the spectral and line results available electronically to aid in the interpretation of the anticipated data.

  12. THE EFFECT OF THE PRE-DETONATION STELLAR INTERNAL VELOCITY PROFILE ON THE NUCLEOSYNTHETIC YIELDS IN TYPE Ia SUPERNOVA

    SciTech Connect (OSTI)

    Kim, Yeunjin; Jordan, G. C. IV; Graziani, Carlo; Lamb, D. Q.; Truran, J. W.; Meyer, B. S.

    2013-07-01

    A common model of the explosion mechanism of Type Ia supernovae is based on a delayed detonation of a white dwarf. A variety of models differ primarily in the method by which the deflagration leads to a detonation. A common feature of the models, however, is that all of them involve the propagation of the detonation through a white dwarf that is either expanding or contracting, where the stellar internal velocity profile depends on both time and space. In this work, we investigate the effects of the pre-detonation stellar internal velocity profile and the post-detonation velocity of expansion on the production of {alpha}-particle nuclei, including {sup 56}Ni, which are the primary nuclei produced by the detonation wave. We perform one-dimensional hydrodynamic simulations of the explosion phase of the white dwarf for center and off-center detonations with five different stellar velocity profiles at the onset of the detonation. In order to follow the complex flows and to calculate the nucleosynthetic yields, approximately 10,000 tracer particles were added to every simulation. We observe two distinct post-detonation expansion phases: rarefaction and bulk expansion. Almost all the burning to {sup 56}Ni occurs only in the rarefaction phase, and its expansion timescale is influenced by pre-existing flow structure in the star, in particular by the pre-detonation stellar velocity profile. We find that the mass fractions of the {alpha}-particle nuclei, including {sup 56}Ni, are tight functions of the empirical physical parameter {rho}{sub up}/v{sub down}, where {rho}{sub up} is the mass density immediately upstream of the detonation wave front and v{sub down} is the velocity of the flow immediately downstream of the detonation wave front. We also find that v{sub down} depends on the pre-detonation flow velocity. We conclude that the properties of the pre-existing flow, in particular the internal stellar velocity profile, influence the final isotopic composition of burned

  13. Gorchakova-IA

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

    Atl anta, Georgia, March 19-23, 2001 1 Estimate of Horizontal Cloud Inhomogeneity Effect on Solar Radiative Fluxes for Conditions of Winter Zvenigorod Experiment I. A. Gorchakova, G. S. Golitsyn, and I. I. Mokhov Oboukhov Institute of Atmospheric Physics Russian Academy of Sciences Moscow, Russia T. B. Zhuravleva Institute of Atmospheric Optics Tomsk, Russia Introduction Study of physical phenomena determining large-scale dynamical and energetic processes in the atmosphere requires quite full

  14. Type Ia Supernovae

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

    that the universe is undergoing an accelerated expansion - a result which fits the General Relativity if a yet unknown form of "dark" energy is assumed to dominate the...

  15. IA Blog Archive

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

    2014 21:03:00 +0000 921386 at http:energy.gov Ministers Meet in Addis Ababa for U.S.-Africa Energy Ministerial http:energy.goviaarticlesministers-meet-addis-ababa-us-africa-...

  16. IA News Archive

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

    Dilma Rousseff of Brazil and he announced the creation of a Strategic Energy Dialogue (SED) to support the two countries' common goals of developing safe, secure and affordable...

  17. EASI HOUSE | Department of Energy

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

    Saginaw, MI | Department of Energy 0 EA-1827: Final Environmental Assessment Suniva Solar Project Site Community Development Block Grant in Thomas Township, Saginaw County, Michigan October 5, 2010 EA-1827: Finding of No Significant Impact Suniva Inc's Artisun Project in Thomas Township, Saginaw, Michigan

    Industrial Carbon Capture and Sequestration (ICCS) Area 1 Project : CO2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone, Archer Daniels Midland Company

  18. Microsoft Word - Final EA- ADM.doc

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

    28 Final Environmental Assessment Industrial Carbon Capture and Sequestration (ICCS) Area 1 Project "CO 2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone" Archer Daniels Midland Company Decatur, Illinois For U.S. Department of Energy National Energy Technology Laboratory DE-FE0001547 April 2011 ACKNOWLEDGEMENT This report was prepared with the support of the U.S. Department of Energy (DOE) under Award No. DE-FE0001547 (Recovery Act - Industrial Carbon

  19. OPTICAL AND NEAR-INFRARED POLARIMETRY OF HIGHLY REDDENED Type Ia SUPERNOVA 2014J: PECULIAR PROPERTIES OF DUST IN M82

    SciTech Connect (OSTI)

    Kawabata, K. S.; Akitaya, H.; Itoh, R.; Moritani, Y. [Hiroshima Astrophysical Science Center, Hiroshima University, Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Yamanaka, M. [Department of Physics, Faculty of Science and Engineering, Konan University, Okamoto, Kobe, Hyogo 658-8501 (Japan); Maeda, K.; Nogami, D. [Department of Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502 (Japan); Ui, T.; Kawabata, M.; Mori, K.; Takaki, K.; Ueno, I.; Chiyonobu, S.; Harao, T.; Matsui, R.; Miyamoto, H.; Nagae, O. [Department of Physical Science, Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526 (Japan); Nomoto, K.; Suzuki, N. [Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Kashiwa, Chiba 277-8583 (Japan); Tanaka, M., E-mail: kawabtkj@hiroshima-u.ac.jp [National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588 (Japan); and others

    2014-11-01

    We present optical and near-infrared multi-band linear polarimetry of the highly reddened Type Ia supernova (SN) 2014J that appeared in M82. SN 2014J exhibits large polarization at shorter wavelengths, e.g., 4.8% in the B band, which decreases rapidly at longer wavelengths, while the position angle of the polarization remains at approximately 40 over the observed wavelength range. These polarimetric properties suggest that the observed polarization is likely predominantly caused by the interstellar dust within M82. Further analysis shows that the polarization peaks at a wavelengths much shorter than those obtained for the Galactic dust. The wavelength dependence of the polarization can be better described by an inverse power law rather than by the Serkowski law for Galactic interstellar polarization. These points suggest that the nature of the dust in M82 may be different from that in our Galaxy, with polarizing dust grains having a mean radius of <0.1 ?m.

  20. Deputy Secretary Daniel Poneman's Remarks to the International...

    Energy Savers [EERE]

    ... or remove every nuclear warhead inherited by Kazakhstan after the dissolution of the Soviet Union, and has led to the removal of hundreds of additional missiles and bombers. ...

  1. Deputy Secretary Daniel Poneman's Remarks to the International...

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

    uranium from the Kazakh Institute of Nuclear Physics in Almaty. The resulting low-enriched uranium cannot be redirected for use in nuclear weapons. Instead, it will be returned...

  2. Deputy Secretary Daniel Poneman's Remarks at demosEUROPA Event...

    Energy Savers [EERE]

    ... - of recoverable natural gas resources, ... to explore for shale gas in Poland. And we expect this kind of foreign investment to ... Clean Energy Investments While these ...

  3. Daniel Cohen Assistant General Counsel for Legislation and Regulatory...

    Office of Environmental Management (EM)

    Heating, and Refrigeration Institute; John Mandyck of Carrier Corporation; Jeffrey Harris of the Alliance to Save Energy; Jim VerShaw of Trane International, Incorporated; two ...

  4. Deputy Secretary Daniel Poneman's Remarks at the Council on Competitiv...

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

    as difficult and, indeed, just as consequential for our future, as those we faced in the dark days of World War II and the Cold War. Once again, we must gear up the great machine...

  5. Carbon Dioxide Sequestering Using Microalgal Systems Daniel J...

    Office of Scientific and Technical Information (OSTI)

    the preliminary economic viability of a COsub 2-sequestering system integrated with a coal-fired power plant based on microalgae biofixation. A review of relevant literature was...

  6. Deputy Secretary Daniel Poneman's Remarks at IFNEC Meeting in...

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

    ... enrichment and reprocessing facilities beyond the needs of the commercial marketplace. In so doing, CFS can enhance the economic viability of nuclear power by reducing the ...

  7. Deputy Secretary Daniel Poneman's Remarks to the Washington Institute...

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

    ... to rely on international markets for nuclear fuel rather than to rely on the costly and difficult steps of uranium enrichment and plutonium reprocessing on their territories. ...

  8. Theresa M. Christian, Daniel A. Beaton, Kunal Mukherjee, Kirstin...

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

    (LEDs), direct color-mixed architectures for SSL retain a high level of technological appeal due to their potential advantages in increased energy savings and flexible tuning of ...

  9. STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy...

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

    Bank Regulatory Affairs Blythe Masters Tesla Motors CEO Elon Musk Entrepreneur T. Boone ... Addthis Related Articles Elon Musk, CEO of Tesla Motors, and Secretary Chu during a ...

  10. Deputy Secretary Daniel Poneman's Remarks at the Tokyo American...

    Energy Savers [EERE]

    ... As soon as we learned about the problems at Fukushima ... plants, including new emergency safety measures and ... them, and those that are planning them - are now in the ...

  11. Prepared Statement The Honorable Daniel B. Poneman Deputy Secretary...

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

    President Obama's nuclear security objectives, including the prevention of nuclear terrorism and the grave and urgent threat it presents to our nation and the world. As long as...

  12. Deputy Secretary Daniel Poneman's Remarks at the Council on Competitiv...

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

    businesses to discover and deliver new technologies. The national labs came into the world out of necessity. In the 1940s, our Nation was at war, confronting imperialist Japan...

  13. Saluting Daniel Poneman's Service to the Department of Energy...

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

    ... and response capabilities, leading the Department's efforts in the wake of the Fukushima Daiichi disaster in 2011, as well as during and after Hurricane Sandy in 2012. In ...

  14. Senate Confirms DOE Nominees Daniel Poneman, David Sandalow,...

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

    Prior to that, Johnson served as the Dean of Duke University's Pratt School of Engineering from 1999-2007 where she helped to set up interdisciplinary efforts in photonics, ...

  15. Secretary Moniz Hosts Energy Security Symposium, Honors Dr. Daniel...

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

    News Media Contact 202-586-4940 Secretary Moniz Hosts Energy Security Symposium, Honors ... Action Month, Energy Secretary Ernest Moniz today hosted the first Schlesinger Medal ...

  16. capture quantum correlations Qasimi, Asma Al-; James, Daniel...

    Office of Scientific and Technical Information (OSTI)

    University of Toronto, Toronto, Ontario M5S 1A7 (Canada) 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; ALGORITHMS; CAPTURE; ENTROPY; MIXED STATES; PURE STATES; QUANTUM...

  17. Daniel Hoag Named NNSA Production Office Deputy Manager | National...

    National Nuclear Security Administration (NNSA)

    (NPO) that was established in June to provide federal oversight of nuclear production missions at the Pantex Plant in Amarillo, Texas, and the Y-12 National Security Complex in Oak ...

  18. Mr. Daniel Cohen U.S. Department of Energy

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

    ... with models not applicable to the established test procedures (due to product innovation) to petition for a test procedure waiver in order to certify, rate, and sell such models. ...

  19. TYPE Ia SUPERNOVA REMNANT SHELL AT z = 3.5 SEEN IN THE THREE SIGHTLINES TOWARD THE GRAVITATIONALLY LENSED QSO B1422+231

    SciTech Connect (OSTI)

    Hamano, Satoshi; Kobayashi, Naoto [Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Kondo, Sohei [Koyama Astronomical Observatory, Kyoto-Sangyo University, Motoyama, Kamigamo, Kita-Ku, Kyoto 603-8555 (Japan); Tsujimoto, Takuji [National Astronomical Observatory of Japan and Department of Astronomical Science, Graduate University for Advanced Studies, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Okoshi, Katsuya [Faculty of Industrial Science and Technology, Tokyo University of Science, 102-1 Tomino, Oshamanbe, Hokkaido 049-3514 (Japan); Shigeyama, Toshikazu, E-mail: hamano@ioa.s.u-tokyo.ac.jp [Research Center for the Early Universe, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan)

    2012-08-01

    Using the Subaru 8.2 m Telescope with the IRCS Echelle spectrograph, we obtained high-resolution (R = 10,000) near-infrared (1.01-1.38 {mu}m) spectra of images A and B of the gravitationally lensed QSO B1422+231 (z = 3.628) consisting of four known lensed images. We detected Mg II absorption lines at z = 3.54, which show a large variance of column densities ({approx}0.3 dex) and velocities ({approx}10 km s{sup -1}) between sightlines A and B with a projected separation of only 8.4h{sup -1}{sub 70} pc at that redshift. This is the smallest spatial structure of the high-z gas clouds ever detected after Rauch et al. found a 20 pc scale structure for the same z = 3.54 absorption system using optical spectra of images A and C. The observed systematic variances imply that the system is an expanding shell as originally suggested by Rauch et al. By combining the data for three sightlines, we managed to constrain the radius and expansion velocity of the shell ({approx}50-100 pc, 130 km s{sup -1}), concluding that the shell is truly a supernova remnant (SNR) rather than other types of shell objects, such as a giant H II region. We also detected strong Fe II absorption lines for this system, but with much broader Doppler width than that of {alpha}-element lines. We suggest that this Fe II absorption line originates in a localized Fe II-rich gas cloud that is not completely mixed with plowed ambient interstellar gas clouds showing other {alpha}-element low-ion absorption lines. Along with the Fe richness, we conclude that the SNR is produced by an SN Ia explosion.

  20. DOE Zero Energy Ready Home Case Study: Cobblestone Homes — 2014 Model Home, Midland, MI

    SciTech Connect (OSTI)

    none,

    2014-09-01

    This builder's first DOE Zero Energy Ready Home won a Custom Builder award in the 2014 Housing Innovation Awards, scored HERS 49 without PV or HERS 44 with 1.4 kW of PV, and served as a prototype and energy efficiency demonstration model while performance testing was conducted.

  1. Permian `Wolfcamp` limestone reservoirs: Powell ranch field, eastern Midland basin: Discussion

    SciTech Connect (OSTI)

    Mazzullo, S.J.

    1997-10-01

    The {open_quotes}E&P Notes{close_quotes} paper by S.L. Montgomery (1996) on Wolfcamp resedimented carbonates in the Permian basin concerns an exploration play with the potential for significant reserves; however, its economic importance and geological complexity, and the question of whether his model can be extended to other areas in the Permian basin warrant this discussion.

  2. Permian {open_quotes}Wolfcamp{close_quotes} limestone reservoirs: Powell Ranch field, Eastern Midland Basin

    SciTech Connect (OSTI)

    Montgomery, S.L.

    1996-09-01

    Deep-water carbonate channel reservoirs form important oil reservoirs along the toe of the Eastern Shelf of the Permian basin in west Texas. In northwestern Glasscock County, these `Wolfcamp` reservoirs are Leonardian (Early Permian) in age and define high-energy channels incised into surrounding carbonate detritus and basinal shale. Porous grain-flow material filling these channels, along with encasing detritus, was derived from the shallow shelf located six miles to the east. Reservoirs are in packstone and grainstone facies and have significant interparticle and moldic porosity. Relevant exploration began in the 1960s, but expanded slowly thereafter due to lack of success caused by complex patterns of channel occurrence. Results of a three-dimensional (3-D) seismic survey conducted in 1990 have greatly enhanced the identification and mapping of productive channels in the Powell Ranch field complex. Wells in this complex are capable of flowing 400-1200 bbl of oil per day, and have reserves ranging from 0.2 to 1.3 MBO. The new 3-D data have improved the relevant geologic model and dramatically increased rates of drilling success. Application of such data to this setting offers a potential model for other parts of the Permian basin.

  3. Running Line-Haul Trucks on Ethanol

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

    I magine driving a 55,000-pound tractor- trailer that runs on corn! If you find it difficult to imagine, you can ask the truck drivers for Archer Daniels Midland (ADM) what it's like. For the past 4 years, they have been piloting four trucks powered by ethyl alcohol, or "ethanol," derived from corn. Several advantages to operating trucks on ethanol rather than on conventional petro- leum diesel fuel present themselves. Because ethanol can be produced domestically, unlike most of our

  4. BETO-Funded Team Honored by the American Chemical Society | Department of

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

    Energy Team Honored by the American Chemical Society BETO-Funded Team Honored by the American Chemical Society April 20, 2015 - 4:34pm Addthis Two Pacific Northwest National Laboratory (PNNL) scientists were part of a team honored at the 249th American Chemical Society (ACS) National Meeting & Exposition on March 25, 2015. The team, which consisted of John Frye and Alan Zacher of PNNL and Todd Werpy of Archer Daniels Midland Company, received the ACS Award for Affordable Green Chemistry

  5. Conversion of Lignocellulosic Biomass to Ethanol and Butyl Acrylate

    SciTech Connect (OSTI)

    Binder, Thomas; Erpelding, Michael; Schmid, Josef; Chin, Andrew; Sammons, Rhea; Rockafellow, Erin

    2015-04-10

    Conversion of Lignocellulosic Biomass to Ethanol and Butyl Acrylate. The purpose of Archer Daniels Midlands Integrated Biorefinery (IBR) was to demonstrate a modified acetosolv process on corn stover. It would show the fractionation of crop residue to distinct fractions of cellulose, hemicellulose, and lignin. The cellulose and hemicellulose fractions would be further converted to ethanol as the primary product and a fraction of the sugars would be catalytically converted to acrylic acid, with butyl acrylate the final product. These primary steps have been demonstrated.

  6. Final Report - Energy Reduction and Advanced Water Removal via Membrane Solvent Extraction Technology

    SciTech Connect (OSTI)

    Reed, John; Fanselow, Dan; Abbas, Charles; Sammons, Rhea; Kinchin, Christopher

    2014-08-06

    3M and Archer Daniels Midland (ADM) collaborated with the U.S. Department of Energy (DOE) to develop and demonstrate a novel membrane solvent extraction (MSE) process that can substantially reduce energy and water consumption in ethanol production, and accelerate the fermentation process. A cross-flow membrane module was developed, using porous membrane manufactured by 3M. A pilot process was developed that integrates fermentation, MSE and vacuum distillation. Extended experiments of 48-72 hours each were conducted to develop the process, verify its performance and begin establishing commercial viability.

  7. BIA Tribal Providers Conference | Department of Energy

    Energy Savers [EERE]

    Energy BETO-Funded Team Honored by the American Chemical Society BETO-Funded Team Honored by the American Chemical Society April 20, 2015 - 4:34pm Addthis Two Pacific Northwest National Laboratory (PNNL) scientists were part of a team honored at the 249th American Chemical Society (ACS) National Meeting & Exposition on March 25, 2015. The team, which consisted of John Frye and Alan Zacher of PNNL and Todd Werpy of Archer Daniels Midland Company, received the ACS Award for Affordable

  8. DOE - Office of Legacy Management -- Staten Island Warehouse - NY 22

    Office of Legacy Management (LM)

    Staten Island Warehouse - NY 22 FUSRAP Considered Sites Staten Island Warehouse, NY Alternate Name(s): Archer-Daniels Midland Company NY.22-3 Location: 2393 Richmond Terrace, Port Richmond, New York NY.22-2 Historical Operations: Stored pitchblende (high-grade uranium ore), which was purchased by the MED for the first atomic bomb. NY.22-3 Eligibility Determination: Eligible Radiological Survey(s): Assessment Survey NY.22-5 Site Status: Referred by DOE, evaluation in progess by U.S. Army Corps of

  9. Site Development, Operations, and Closure Plan Topical Report 5 An Assessment of Geologic Carbon Sequestration Options in the Illinois Basin. Phase III

    SciTech Connect (OSTI)

    Finley, Robert; Payne, William; Kirksey, Jim

    2015-06-01

    The Midwest Geological Sequestration Consortium (MGSC) has partnered with Archer Daniels Midland Company (ADM) and Schlumberger Carbon Services to conduct a large-volume, saline reservoir storage project at ADM’s agricultural products processing complex in Decatur, Illinois. The Development Phase project, named the Illinois Basin Decatur Project (IBDP) involves the injection of 1 million tonnes of carbon dioxide (CO2) into a deep saline formation of the Illinois Basin over a three-year period. This report focuses on objectives, execution, and lessons learned/unanticipated results from the site development (relating specifically to surface equipment), operations, and the site closure plan.

  10. Supernova Hunting with Supercomputers

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

    Supernova Hunting with Supercomputers Supernova Hunting with Supercomputers Berkeley researchers provide "roadmap" and tools for finding and studying Type Ia supernovae in their natural habitat May 20, 2015 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov sn-star.jpg Simulation of the expanding debris from a supernova explosion (shown in red) running over and shredding a nearby star (shown in blue). Image credit: Daniel Kasen, Berkeley Lab/ UC Berkeley Type Ia supernovae are famous for

  11. Hon. Daniel B. Poneman Deputy Secretary U.S. Department of Energy

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

    Committee on Energy and Commerce U.S. House of Representatives September 12, 2012 Chairman Stearns, Ranking Member DeGette, and members of the Subcommittee, thank you for the...

  12. Hon. Daniel B. Poneman Deputy Secretary U.S. Department of Energy

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

    ... The intruders' movement was detected, but initially went unchallenged. The Protective ... steps to improve security: * The former head of security from Pantex moved to Y-12 to ...

  13. Microsoft Word - Oil and Gas Pipelines_Statement_Dr Daniel Fine...

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

    ... Oil and an natural gas price recovery are required indefinitely to stabilize population and job markets. Its oil production, following the infusion of technology innovation, is at ...

  14. Clifton Truman Daniel's visit to Oak Ridge and Y-12, part 1

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

    called me several weeks ago to state that he had initiated contact with President Harry S. Truman's grandson and that he was anxious to visit Oak Ridge. That was exciting...

  15. A U T H O R S Daniel R. Hitchcock U.S. Department

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

    ... Construction of a stormwater bypass (30-in. 76.2-cm pipe diameter) was completed in June 2002; this bypass was intended to divert storm- water runoff, including stormwater ...

  16. Deputy Secretary Daniel Poneman's Remarks at the 2011 U.S.-China...

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

    The United States and China have cooperated in a broad range of science and technology arenas for more than 30 years, providing an important foundation for our latest joint...

  17. VWA-0005- Deputy Secretary Decision- In the Matter of Daniel L. Holsinger

    Broader source: Energy.gov [DOE]

    This is a request for review by K-Ray Security, Inc., from the Initial Agency Decision by the Office of Hearings and Appeals ("OHA"), finding that reinstatement of Mr. Holsinger as a security guard...

  18. OSTIblog Posts by Cathey Daniels | OSTI, US Dept of Energy Office...

    Office of Scientific and Technical Information (OSTI)

    That now you can learn about OSTI tools and services on our OSTI YouTube site launched in June? Read more... Mixing Science.gov, Coffee, and a Laptop Personal Perspectives ...

  19. Dr. Daniel A. Hitchcock | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Hitchcock came to DOE in 1983 to manage the Fusion Energy Theory Program. In 1985-87, he led the effort to expand the scope of the Magnetic Fusion Energy Computing Center to ...

  20. MaRIE 1.0: A briefing to Katherine Richardson-McDaniel, Staff...

    Office of Scientific and Technical Information (OSTI)

    What it would be, the mission need motivation, the scientific challenge, and the current favorable impact on both programs and people are shown in viewgraph form. Authors: Barnes, ...

  1. Hon. Daniel B. Poneman Deputy Secretary U.S. Department of Energy

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

    in its entirety. Indeed, we have reflected our commitment through our Management Principles, which provide that: * We will treat our people as our greatest asset; * We will...

  2. Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel...

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

    ... project overview video (must have Windows Media Player) or visit CenterPoint Energy's ... natural gas sales and services, interstate pipelines and field services operations. ...

  3. Hon. Daniel B. Poneman Deputy Secretary U.S. Department of Energy

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

    trespassed onto the Y-12 National Security Complex and defaced a building at NNSA's Y-12 National Security Complex in Oak Ridge, Tennessee. This incursion and inadequate response...

  4. WBZ-13-0006- In the Matter of Vincent E. Daniel

    Broader source: Energy.gov [DOE]

    On September 18, 2013, the OHA Hearing Officer issued an Initial Agency Decision considering a Motion to Dismiss filed by the Battelle Energy Alliance, LLC (BEA) against its former employee,...

  5. WBH-13-0006- In the Matter of Vincent E. Daniel

    Broader source: Energy.gov [DOE]

    On September 18, 2013, the OHA Hearing Officer issued an Initial Agency Decision considering a Motion to Dismiss filed by the Battelle Energy Alliance, LLC (BEA) against its former employee,...

  6. 10 Questions for a Batteries Expert: Daniel Abraham | Department of Energy

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

    Summary of Test Results for the Interagency Field Test &Evaluation of Wind Turbine - Radar Interference Mitigation Technologies PUBLIC RELEASE Testing Phase: April 2012-April 2013  Report: September 2013 Distribution Statement A: Approved for Public Release (July 9, 2014). 2 Purpose of this Fact Sheet: This document includes background information and a summary of three field tests designed to measure the impact of wind turbines on current air surveillance radars and the effectiveness of

  7. OSTIblog Posts by Cathey Daniels | OSTI, US Dept of Energy, Office...

    Office of Scientific and Technical Information (OSTI)

    That now you can find research from China when you search within WorldWideScience.org? OSTI was in Ottawa June 10 helping formalize the addition of China to the WorldWideScience ...

  8. Deputy Secretary Daniel Poneman's Remarks at the Tokyo American Center-- As Prepared for Delivery

    Broader source: Energy.gov [DOE]

    Thank you, Jeff, for the introduction.  Jeff has recently returned to Japan as the Department of Energy’s attaché here.  He continues the long tradition of excellent energy officers that have...

  9. FIA-13-0001- In the matter of Daniel J. Gage

    Broader source: Energy.gov [DOE]

    On January 23, 2013, the Office of Hearings and Appeals (OHA) issued a decision remanding an appeal (Appeal) from a Freedom of Information Act (FOIA) determination issued by the Golden Field Office...

  10. Members | U.S. DOE Office of Science (SC)

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

    Members Advanced Scientific Computing Advisory Committee (ASCAC) ASCAC Home Meetings Members ASCAC Members Bio Previous ASCAC Members Charges/Reports ASCAC Charter 2015 - signed .pdf file (134KB) ASCR Committees of Visitors Federal Advisory Committees ASCR Home Members Print Text Size: A A A FeedbackShare Page Professor Daniel A. Reed, Chair Office of the Vice President for Research and Economic Development University of Iowa 2660 UCC Iowa City, IA 52242 dan-reed@uiowa.edu 319-335-2119 (phone)

  11. Final Technical Report: A Paradigm Shift in Chemical Processing: New Sustainable Chemistries for Low-VOC Coatings

    SciTech Connect (OSTI)

    Smith, Kenneth F.

    2006-07-26

    The project employed new processes to make emulsion polymers from reduced levels of petroleum-derived chemical feedstocks. Most waterborne paints contain spherical, emulsion polymer particles that serve as the film-forming binder phase. Our goal was to make emulsion polymer particles containing 30 percent feedstock that would function as effectively as commercial emulsions made from higher level feedstock. The processes developed yielded particles maintained their film formation capability and binding capacity while preserving the structural integrity of the particles after film formation. Rohm and Haas Company (ROH) and Archer Daniels Midland Company (ADM) worked together to employ novel polymer binders (ROH) and new, non-volatile, biomass-derived coalescing agents (ADM). The University of Minnesota Department of Chemical Engineering and Material Science utilized its unique microscopy capabilities to characterize films made from the New Emulsion Polymers (NEP).

  12. Deputy Secretary Daniel Poneman's Remarks at the 2011 U.S.-China Relations Conference- As Prepared for Delivery

    Office of Energy Efficiency and Renewable Energy (EERE)

    Thank you, Steve, for the introduction and for your work as one of America’s energy leaders.  In addition to his work at Texas A&M, Steve Holditch recently served as a member of a group of...

  13. Deputy Secretary Daniel Poneman's Remarks at the Council on Competitiveness 25th Anniversary Summit-- As Prepared for Delivery

    Broader source: Energy.gov [DOE]

    Thank you, Sam, for the introduction.  And thank you to the Council on Competitiveness for giving me the opportunity to speak here today.

  14. STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy Leaders Headline 3-Day ARPA-E Summit

    Broader source: Energy.gov [DOE]

    Building on the President’s call in his State of the Union address to further American energy independence through innovation, key thought leaders from academia, business, and government will come together.

  15. A Chandrasekhar mass progenitor for the Type Ia supernova remnant...

    Office of Scientific and Technical Information (OSTI)

    for Astrophysics, Cambridge, MA (United States) Univ. of Pittsburgh, Pittsburgh, PA (United States) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States) Univ. ...

  16. HUBBLE RESIDUALS OF NEARBY TYPE Ia SUPERNOVAE ARE CORRELATED...

    Office of Scientific and Technical Information (OSTI)

    ... MASS; RED SHIFT; SUPERNOVAE BINARY STARS; ERUPTIVE VARIABLE STARS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STARS; VARIABLE STARS Word Cloud More Like This Full Text Journal ...

  17. THE ABSOLUTE MAGNITUDES OF TYPE Ia SUPERNOVAE IN THE ULTRAVIOLET...

    Office of Scientific and Technical Information (OSTI)

    Authors: Brown, Peter J. ; Roming, Peter W. A. ; Ciardullo, Robin ; Gronwall, Caryl ; Hoversten, Erik A. ; Pritchard, Tyler 1 ; Milne, Peter 2 ; Bufano, Filomena ; Mazzali, ...

  18. Sweetspot: Near-infrared observations of 13 type Ia supernovae...

    Office of Scientific and Technical Information (OSTI)

    Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States) Publication Date: 2014-04-01 OSTI Identifier: 22357282 Resource ...

  19. THE ULTRAVIOLET BRIGHTEST TYPE Ia SUPERNOVA 2011de (Journal Article...

    Office of Scientific and Technical Information (OSTI)

    be modeled with additional flux from the shock of the ejecta hitting a relatively large ... similar UV luminosities can be intrinsic or caused by other forms of shock interaction. ...

  20. Turbulence-Flame Interactions in Type Ia Supernovae (Journal...

    Office of Scientific and Technical Information (OSTI)

    1 ; Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 2 ; Department of Physics and Astronomy, Stony Brook University, ...

  1. Improved Distances to Type Ia Supernovae withMulticolor Light...

    Office of Scientific and Technical Information (OSTI)

    This site is a product of DOE's Office of Scientific and Technical Information (OSTI) and ... We present an updated version of the Multicolor Light Curve Shape method to measure ...

  2. Turbulence-Flame Interactions in Type Ia Supernovae (Journal...

    Office of Scientific and Technical Information (OSTI)

    turbulent intensity and l is the integral scale. For the larger integral scales characteristic of a real supernova, the flame structure is predicted to become complex and unsteady. ...

  3. New approaches for modeling type Ia supernovae (Conference) ...

    Office of Scientific and Technical Information (OSTI)

    DOE Contract Number: DE-AC02-05CH11231 Resource Type: Conference Resource Relation: Conference: SciDAC 2006, Denver, CO, 25-29 June2006 Publisher: Institute of Physics, ...

  4. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties...

    Office of Scientific and Technical Information (OSTI)

    Tao, C.; Thomas, R. C.; Weaver, B. A. 79 ASTRONOMY AND ASTROPHYSICS distance scale, supernovae: general distance scale, supernovae: general Kim et al. (2013) K13 introduced a...

  5. Climate Action Champions: Dubuque, IA | Department of Energy

    Office of Environmental Management (EM)

    meter technologies that allow them to reduce water usage, electricity usage, and garbage. ... focused on risk reduction and resilience, and it has been restoring a major ...

  6. Flames in Type Ia Supernova: Deflagration-Detonation Transition...

    Office of Scientific and Technical Information (OSTI)

    Language: English Word Cloud More Like This Full Text Journal Articles Find in Google Scholar Find in Google Scholar Search WorldCat Search WorldCat to find libraries that may hold ...

  7. Microsoft PowerPoint - IEEE IAS PES 102313.pptx

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

    ... units Cyber security Weather forecasting Equipment health monitors Smart ... savings Reduced electricity costs to consumers Lower pollutant ...

  8. Closest Type Ia Supernova in Decades Solves a Cosmic Mystery

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

    observations of SN 2011fe were carried out at the Liverpool Telescope at La Palma in the Canary Islands, followed within hours by the Shane Telescope at Lick Observatory in...

  9. Improved Constraints on Type Ia Supernova Host Galaxy Properties...

    Office of Scientific and Technical Information (OSTI)

    Astrophys. ; Smith, Mathew ; Cape Town U. ; Bassett, Bruce ; South African Astron. Observ. Cape Town U., Dept. Math. African Inst. Math. Sci., Cape Town ; Frieman, Joshua A. ; ...

  10. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties...

    Office of Scientific and Technical Information (OSTI)

    The K13 Hubble residual step with host mass is 0.013 ? 0.031 mag for a supernova subsample with data coverage corresponding to the K13 training; at ? 1?, the step is not ...

  11. Federal Project Director of the Year for 2011 | Department of...

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

    Phillip Kraushaar; Johnny Moore; Daniel Lehman; Ingrid Kolb (from left to right) Daniel Poneman; David Arakawa; Phillip Kraushaar; Johnny Moore; Daniel Lehman; Ingrid Kolb ...

  12. SREL Reprint #3357

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

    7 Functionalized magnetic mesoporous silica nanoparticles for U removal from low and high pH groundwater Dien Li1, Shani Egodawatte2, Daniel I. Kaplan1, Sarah C. Larsen2, Steven M. Serkiz1,3, and John C. Seaman4 1Savannah River National Laboratory, Aiken, SC 29808, USA 2Department of Chemistry, University of Iowa, Iowa City, IA 52242, USA 3Department of Physics and Astronomy, Clemson University, Clemson, SC 29634, USA 4Savannah River Ecology Laboratory, University of Georgia, Aiken, SC 29802,

  13. DOE - Fossil Energy:

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

    Midland Cogeneration Venture Ltd. Partnership 1765 FE02-26-LNG 043002 Various Sources El Paso Merchant Energy, L.P. (Norway) 1780 FE02-59-NG 082902 Can Midland Cogeneration...

  14. Urban Heat Islands: Anti-Soiling Cool Roof Coatings

    Broader source: Energy.gov [DOE]

    Performers: Lawrence Berkeley National Laboratory Project Partners: -- Oak Ridge National Laboratory - Oak Ridge, TN -- Dow Chemical Company - Midland, MI

  15. VWC-0001 and VWC-0002- Deputy Secretary Decision- In the Matter of Daniel Holsinger, Complainant, v. K-Ray Security, Inc.

    Broader source: Energy.gov [DOE]

    This is a request for review by K-Ray Security, Inc., the current security operations contractor at DOE’s Federal Energy Technology Center (“FETC”), of the Decision of the Office of Hearings and...

  16. Table 33. Oxygenated Motor Gasoline Prices by Grade, Sales Type...

    Gasoline and Diesel Fuel Update (EIA)

    - - - - - - - 1997 Average ... - - - - - - - - - - - - Subdistrict IA January ... - - - - - - - - - - - - February...

  17. Federal Energy Management Program Organization Chart

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

    Timothy Unruh Sustainability Services Daniel Gore Sustainability, Legislative Affairs Nicolas Baker Large Campus Initiative Daniel Gore Fleet Tom Homan (Acting) Organization Chart ...

  18. Browse by Discipline -- E-print Network Subject Pathways: Engineering...

    Office of Scientific and Technical Information (OSTI)

    Lathrop, Daniel P. (Daniel P. Lathrop) - Institute for Research in Electronics and Applied Physics & Department of Physics, University of Maryland at College Park Learned, John ...

  19. Enforcement Letters | Department of Energy

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

    and Fire at the Los Alamos National Laboratory July 7, 1997 Enforcement Letter, Fluor Daniel Hanford, Inc. - July 7, 1997 Issued to Fluor Daniel Hanford, Inc., related to...

  20. Laws & Legal Resources | Department of Energy

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

    Library Books | Credit: GC Photographer Daniel Zazueta Library Books | Credit: GC Photographer Daniel Zazueta Looking for... Online Legal Resources Laws DOE Administers Guidance &...

  1. Energy Blog | Department of Energy

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

    RSS October 3, 2014 Saluting Daniel Poneman's Service to the Department of Energy The Energy Department is saying farewell to Daniel Poneman, the longest-serving Deputy Secretary...

  2. Before the Senate Energy and Natural Resources Committee | Department...

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

    Daniel B. Poneman, Nominee for Deputy Secretary of Energy Subject: Nomination Hearing PDF icon 5509DanielPonemanNomination.pdf More Documents & Publications Before the Senate...

  3. Microsoft PowerPoint - 16.1045_Peer Reviews Panel_Lehman Workshop...

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

    Science Peer Reviews 101 Daniel R. Lehman, Director Office of Project Assessment Office of Project Assessment Office of Science Peer Review 101 Panel Members Mr. Daniel Lehman,...

  4. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Filter Results Filter by Author Frisbie, C. Daniel (1) Goldhaber-Gordon, D. (1) Lee, ... ; Zhang, Sipei ; Frisbie, C. Daniel ; Goldhaber-Gordon, D. Full Text Available December ...

  5. Structure and dynamics of the M3 muscarinic acetylcholine receptor...

    Office of Scientific and Technical Information (OSTI)

    Authors: Kruse, Andrew C. ; Hu, Jianxin ; Pan, Albert C. ; Arlow, Daniel H. ; Rosenbaum, Daniel M. ; Rosemond, Erica ; Green, Hillary F. ; Liu, Tong ; Chae, Pil Seok ; Dror, Ron O. ...

  6. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Hampton-Marcell, Jarrad T. (1) Lax, Simon (1) Smith, Daniel (1) Save Results Excel (limit ... Sean M. ; Colares, Gergia Barguil ; Smith, Daniel ; Eisen, Jonathan A. ; Gilbert, ...

  7. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Kennedy, Suzanne (1) Martin, Gilles (1) Mills, David A. (1) Smith, Daniel (1) Taghavi, ... Sean M. ; Colares, Gergia Barguil ; Smith, Daniel ; Eisen, Jonathan A. ; Gilbert, ...

  8. Browse by Discipline -- E-print Network Subject Pathways: Fossil...

    Office of Scientific and Technical Information (OSTI)

    Finer, John J. (John J. Finer) - Department of Horticulture and Crop Science, Ohio State University Fischer, Daniel (Daniel Fischer) - Center of Excellence in Bioinformatics and ...

  9. Browse by Discipline -- E-print Network Subject Pathways: Power...

    Office of Scientific and Technical Information (OSTI)

    ... Grant, Taran (Taran Grant) - Department of Herpetology, American Museum of Natural History ... Universidad Nacional Autnoma de Mxico Grnbaum, Daniel (Daniel Grnbaum) - ...

  10. Browse by Discipline -- E-print Network Subject Pathways: Chemistry...

    Office of Scientific and Technical Information (OSTI)

    University of South Florida Olgun, Daniel (Daniel Olgun) - Departamento de Fsica, Centro de Investigacin y de Estudios Avanzados del IPN Olson, Tamara (Tamara Olson) ...

  11. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... Ballaran, Tiziana Boffa (1) Beyer, Christopher (1) Chantel, Julien (1) Frost, Daniel J. ... garnet to 24 GPa and 1300 K Chantel, Julien ; Manthilake, Geeth M. ; Frost, Daniel J. ...

  12. Browse by Discipline -- E-print Network Subject Pathways: Materials...

    Office of Scientific and Technical Information (OSTI)

    ... (Alvaro Romero Jimnez) - Departamento de Ciencias de la Computacin e Inteligencia Artificial, Universidad de Sevilla Jimnez, Daniel A. (Daniel A. Jimnez) - Department ...

  13. Browse by Discipline -- E-print Network Subject Pathways: Energy...

    Office of Scientific and Technical Information (OSTI)

    of Physics & Department of Mathematics, Harvard University Jaffe, Daniel T. (Daniel T. ... of Engineering and Applied Sciences, Harvard University Joselevich, Ernesto (Ernesto ...

  14. Member Case Studies: LED Street Lighting Programs in Algona (IA), Asheville (NC), and Boston (MA)

    Broader source: Energy.gov [DOE]

    This May 8, 2013 webcast featured presentations from DOE Municipal Solid-State Street Lighting Consortium member cities about their experiences with LED street lighting. Presenters John Bilsten of...

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

    SciTech Connect (OSTI)

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

    2013-03-01

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

  16. CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE (Journal Article...

    Office of Scientific and Technical Information (OSTI)

    Authors: Hicken, Malcolm ; Challis, Peter ; Kirshner, Robert P. ; Bakos, Gaspar ; Berlind, Perry ; Brown, Warren R. ; Caldwell, Nelson ; Calkins, Mike ; Falco, Emilio ; Fernandez, ...

  17. Hubble Residuals of Nearby SN Ia Are Correlated with Host Galaxy...

    Office of Scientific and Technical Information (OSTI)

    United States Language: English Subject: 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; CALIBRATION; COSMOLOGY; DUSTS; GALAXIES; LUMINOSITY; SKY; TESTING ...

  18. CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA (Journal...

    Office of Scientific and Technical Information (OSTI)

    Authors: Hicken, Malcolm ; Challis, Peter ; Kirshner, Robert P. ; Bakos, Gaspar ; Berlind, Perry ; Brown, Warren R. ; Caldwell, Nelson ; Calkins, Mike ; Cho, Richard ; Contreras, ...

  19. NEAR-ULTRAVIOLET PROPERTIES OF A LARGE SAMPLE OF TYPE Ia SUPERNOVAE...

    Office of Scientific and Technical Information (OSTI)

    Hicken, Malcolm ; Kirshner, Robert P. ; Challis, Peter J. 6 ; Mazzali, Paolo 7 ; Schmidt, Brian P. 8 + Show Author Affiliations Steward Observatory, University of Arizona, ...

  20. Hubble Residuals of Nearby SN Ia Are Correlated with Host Galaxy...

    Office of Scientific and Technical Information (OSTI)

    Authors: Kelly, Patrick L. ; KIPAC, Menlo Park SLAC ; Hicken, Malcolm ; Harvard-Smithsonian Ctr. Astrophys. ; Burke, David L. ; KIPAC, Menlo Park SLAC ; Mandel, Kaisey S. ; ...

  1. Rock Creek I: 48-core iA Tera Scale Prototype

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

    to make sure we don't miss any great ideas. Hence, my views are by design far "off the roadmap". Here is what I'd like to talk about * Please stop using acronyms and undefined...

  2. VARIABLE SODIUM ABSORPTION IN A LOW-EXTINCTION TYPE Ia SUPERNOVA...

    Office of Scientific and Technical Information (OSTI)

    We present the third detection of such variable absorption, based on six epochs of ... Country of Publication: United States Language: English Subject: 74 ATOMIC AND MOLECULAR ...

  3. IA REP0 SAND85-2809 Unlimited Release UC-92A

    Office of Scientific and Technical Information (OSTI)

    ... The initial research and development for HEGF was conducted ... These tests, together with modeling, produced a methodology ... experiments. -3- II. Experimental A. Experiment Design ...

  4. Type Ia supernova rate measurements to redshift 2.5 from CANDELS...

    Office of Scientific and Technical Information (OSTI)

    Authors: Rodney, Steven A. ; Riess, Adam G. ; Graur, Or ; Jones, David O. 1 ; Strolger, Louis-Gregory ; Dahlen, Tomas ; Casertano, Stefano ; Ferguson, Henry C. ; Koekemoer, Anton ...

  5. "Report Date","U.S.",,,"PADD I",,,"PADD IA",,,"PADD IB",,,"PADD...

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

    Residential Heating Oil Prices (Before and After Change in Aggregation Methodology)" ... and After Change in Aggregation Methodology)" "Report Date","U.S.",,,"PADD ...

  6. Type Ia supernovae from merging white dwarfs. II. Post-merger...

    Office of Scientific and Technical Information (OSTI)

    light curves rise and decline very slowly, and the spectra generally look peculiar, with weak features from intermediate mass elements but relatively strong carbon absorption. ...

  7. HIGH-VELOCITY LINE FORMING REGIONS IN THE TYPE Ia SUPERNOVA 2009ig...

    Office of Scientific and Technical Information (OSTI)

    TX 78712-0259 (United States) Carnegie Observatories, Las Campanas Observatory, Colina El Pino, Casilla 601 (Chile) George P. and Cynthia Woods Mitchell Institute for Fundamental ...

  8. A SEARCH FOR NEW CANDIDATE SUPER-CHANDRASEKHAR-MASS TYPE Ia SUPERNOVAE...

    Office of Scientific and Technical Information (OSTI)

    Authors: Scalzo, R. 1 ; Aldering, G. ; Aragon, C. ; Bailey, S. ; Childress, M. ; Fakhouri, H. K. ; Hsiao, E. Y. 2 ; Antilogus, P. ; Bongard, S. ; Canto, A. ; Cellier-Holzem, F. ...

  9. Type Ia supernovae yielding distances with 3-4% precision (Journal...

    Office of Scientific and Technical Information (OSTI)

    dwarf stars, vary systematically with their intrinsic color and light-curve decline rate. ... two progenitor properties account for their light-curve-widthcolorluminosity relation. ...

  10. Management of dry flue gas desulfurization by-products in underground mines. Quarterly report, August 1--October 31, 1997

    SciTech Connect (OSTI)

    Chugh, Y.P.

    1997-12-31

    The objective of this project was to develop and demonstrate two technologies for the placement of coal combustion by-products in abandoned underground coal mines, and to assess the environmental impact of these technologies for the management of CCB materials. The two technologies for the underground placement that were to be developed and demonstrated are: (1) pneumatic placement using virtually dry CCB products, and (2) hydraulic placement using a paste mixture of CCB products with about 70% solids. The period covered by this report is the second quarter of Phase 3 of the overall program. During this period over 8,000 tons of CCB mixtures was injected using the hydraulic paste technology. This amount of material virtually filled the underground opening around the injection well, and was deemed sufficient to demonstrate fully the hydraulic injection technology. By the end of this quarter about 2,000 tons of fly ash had been placed underground using the pneumatic placement technology. While the rate of injection of about 50 tons per hour met design criteria, problems were experienced in the delivery of fly ash to the pneumatic demonstration site. The source of the fly ash, the Archer Daniels Midland Company power plant at Decatur, Illinois is some distance from the demonstration site, and often sufficient tanker trucks are not available to haul enough fly ash to fully load the injection equipment. Further, on some occasions fly ash from the plant was not available. The injection well was plugged three times during the demonstration. This typically occurred due to cementation of the FBC ash in contact with water. After considerable deliberations and in consultation with the technical project officer, it was decided to stop further injection of CCB`s underground using the developed pneumatic technology.

  11. No Slide Title

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

    International Affairs (IA-1) Office of Resource Management (IA-10) . DAS for Africa, Middle East, Europe & Eurasia (IA-20) OFFICE OF INTERNATIONAL AFFAIRS (IA) Office of European and Eurasian Affairs (IA-21) Office of African and Middle Eastern Affairs (IA-22) DAS for Asia & the Americas (IA-30) Office of Asian Affairs (IA-31) Office of International Science & Technology Collaboration (IA-42) Office of American Affairs (IA-32) DAS for International Climate & Technology (IA-40)

  12. Kinetic Wave Power | Open Energy Information

    Open Energy Info (EERE)

    Wave Power Jump to: navigation, search Name: Kinetic Wave Power Address: 2861 N Tupelo St Place: Midland Zip: 48642 Region: United States Sector: Marine and Hydrokinetic Phone...

  13. Dow Building Solutions | Open Energy Information

    Open Energy Info (EERE)

    Dow Building Solutions Jump to: navigation, search Name: Dow Building Solutions Place: Midland, MI Website: www.dowbuildingsolutions.com References: Dow Building Solutions1...

  14. Mr. Ken Blower, Manager Corporate Environmental Affairs Standard...

    Office of Legacy Management (LM)

    Ken Blower, Manager Corporate Environmental Affairs Standard Oil Company of Ohio Midland ... Research Laboratory (now Standard Oil Company of Ohio) to determine whether it ...

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

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

    Light and Power Cooperative Farmers Electric Cooperative Guthrie REC Linn County REC Maquoketa Valley Electric Cooperative Midland Power Cooperative Pella Cooperative Electric...

  16. Climate Zone Number 3 | Open Energy Information

    Open Energy Info (EERE)

    California Merced County, California Meriwether County, Georgia Midland County, Texas Miller County, Arkansas Mills County, Texas Mississippi County, Arkansas Mitchell County,...

  17. Renovar Energy Corp | Open Energy Information

    Open Energy Info (EERE)

    Renovar Energy Corp Jump to: navigation, search Name: Renovar Energy Corp Place: Midland, Texas Zip: 79705 Product: Texas-based landfill gas project developer. References: Renovar...

  18. Martin County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Zone Subtype B. Registered Energy Companies in Martin County, Texas Hilliard Energy Renovar Energy Corp Skyward Energy LLC Places in Martin County, Texas Ackerly, Texas Midland,...

  19. EA-1708: Final Environmental Assessment

    Broader source: Energy.gov [DOE]

    Financial Assistance to Dow Kokam Mi, LLC To Manufacture Advanced Lithium Polymer Batteries for Hybrid and Electric Vehicles At Midland, Michigan

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

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

    REC Linn County REC Maquoketa Valley Electric Cooperative Midland Power Cooperative Pella Cooperative Electric Association Southwest Iowa REC T.I.P. REC South Iowa Municipal...

  1. Dow Chemical Co | Open Energy Information

    Open Energy Info (EERE)

    search Name: Dow Chemical Co Place: Midland, Michigan Zip: 48674 Sector: Hydro, Hydrogen Product: Michigan-based global chemical, plastic and agricultural products maker,...

  2. Clinton County, Ohio: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Clarksville, Ohio Lynchburg, Ohio Martinsville, Ohio Midland, Ohio New Vienna, Ohio Port William, Ohio Sabina, Ohio Wilmington, Ohio Retrieved from "http:en.openei.orgw...

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

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

    Iowa REC Eastern Iowa Light and Power Cooperative Farmers Electric Cooperative Guthrie REC Linn County REC Maquoketa Valley Electric Cooperative Midland Power...

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

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

    Iowa REC Eastern Iowa Light and Power Cooperative Farmers Electric Cooperative Guthrie REC Linn County REC Maquoketa Valley Electric Cooperative Midland Power Cooperative...

  5. Gila County, Arizona: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Day, Arizona Central Heights-Midland City, Arizona Claypool, Arizona Gisela, Arizona Globe, Arizona Hayden, Arizona Miami, Arizona Payson, Arizona Peridot, Arizona Pine, Arizona...

  6. EA-1708: Finding of No Significant Impact | Department of Energy

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

    MI, LLC to construct and operate the Midland Battery Park for manufacturing of advanced lithium polymer batteries for hybrid and electric vehicles: (1) a grant under Funding...

  7. FE0005889_UTPermian | netl.doe.gov

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

    Performers The University of Texas of the Permian Basin, Odessa, TX 79762-8122 Kinder Morgan Production Company, Houston, TX 77002 Melzer Consulting, Midland, TX 79701 Advanced ...

  8. Before The Subcommittee on Oversight and Investigations- House Committee on Energy and Commerce

    Broader source: Energy.gov [DOE]

    Subject: Department of Energy Management and Performance By: Daniel Poneman, Deputy Secretary of Energy

  9. No Slide Title

    Office of Environmental Management (EM)

    for International Affairs (IA-1) Office of Resource Management (IA-10) . DAS for Africa, Middle East, Europe & Eurasia (IA-20) OFFICE OF INTERNATIONAL AFFAIRS (IA) Office of European and Eurasian Affairs (IA-21) Office of African and Middle Eastern Affairs (IA-22) DAS for Asia & the Americas (IA-30) Office of Asian Affairs (IA-31) Office of International Science & Technology Collaboration (IA-42) Office of American Affairs (IA-32) DAS for International Climate & Technology

  10. No Slide Title

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

    for International Affairs (IA-1) Office of Resource Management (IA-10) . DAS for Africa, Middle East, Europe & Eurasia (IA-20) OFFICE OF INTERNATIONAL AFFAIRS (IA) Office of European and Eurasian Affairs (IA-21) Office of African and Middle Eastern Affairs (IA-22) DAS for Asia & the Americas (IA-30) Office of Asian Affairs (IA-31) Office of International Science & Technology Collaboration (IA-42) Office of American Affairs (IA-32) DAS for International Climate & Technology

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

    SciTech Connect (OSTI)

    Marek, Laura F.

    2011-06-17

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

  12. Vehicle Technologies Office Merit Review 2014: International Energy Agency (IEA IA-AMT) International Characterization Methods (Agreement ID:26462)

    Broader source: Energy.gov [DOE]

    Presentation given by Oak Ridge National Laboratory at 2014 DOE Hydrogen and Fuel Cells Program and Vehicle Technologies Office Annual Merit Review and Peer Evaluation Meeting about International...

  13. Superfund Record of Decision (EPA Region 7): Vogel Paint and Wax, Maurice, IA. (First remedial action), September 1989. Final report

    SciTech Connect (OSTI)

    Not Available

    1989-09-20

    The Vogel Paint and Wax (VPW) site is an approximately two-acre disposal area two miles southwest of the town of Maurice, in Sioux County, Iowa. Adjacent land uses are primarily agricultural; however, several private residences are within one-quarter mile of the site. A surficial sand and gravel aquifer underlies the site and supplies nearby private wells and the Southern Sioux County Rural Water System, located a mile and one half southeast of the site. Paint sludge, resins, solvents, and other paint-manufacturing wastes were disposed of at the site between 1971 and 1979. VPW records indicate that approximately 43,000 gallons of aliphatic and aromatic hydrocarbons and 6,000 pounds of metals waste were buried at the site. The primary contaminants of concern affecting the soil and ground water are VOCs including benzene, toluene, and xylenes; and metals including chromium and lead. The selected remedial action for this site includes excavation of contaminated soil and separation of solid and liquid wastes; onsite bioremediation of 3,000 cubic yards of the contaminated soil in a fully contained surface impoundment unit, or onsite thermal treatment if soil contains high metal content; and stabilization of treated soil, if necessary to prevent leaching of metals, followed by disposal in the excavated area.

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

    SciTech Connect (OSTI)

    Not Available

    1984-08-01

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

  15. --No Title--

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

    - - - - - - December... - - - - - - 1997 Average... - - - - - - Subdistrict IA January... - - - - - - February... - - - - - - March... - - - - - -...

  16. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Malliakas, Christos D. (1) Mitchell, J. F. (1) Phelan, Daniel (1) Smith, Mark D. (1) ... Daniel E. ; Stackhouse, Chavis A. ; Smith, Mark D. ; Loye, Hans-Conrad zur, E-mail: ...

  17. VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter...

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

    Daniel Holsinger, Complainant, v. K-Ray Security, Inc. VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter of Daniel Holsinger, Complainant, v. K-Ray Security, Inc. ...

  18. July 2012 | National Nuclear Security Administration

    National Nuclear Security Administration (NNSA)

    Jobs Working at NNSA Blog Home July 2012 July 2012 Y-12 Press Release Jul 20, 2012 Daniel Hoag Named NNSA Production Office Deputy Manager OAK RIDGE, Tenn. - Daniel Hoag has...

  19. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... Berry, David A (6) Haynes, Daniel J. (6) Smith, Mark W. (5) Abdelsayed, Victor (3) Campos, Andrew (3) Gardner, Todd H. (3) Haynes, Daniel (3) Lyons, K. David (3) Smith, Mark (3) ...

  20. Plasma density diagnostic for capillary-discharge based plasma...

    Office of Scientific and Technical Information (OSTI)

    Plasma density diagnostic for capillary-discharge based plasma channels Authors: Daniels, J. 1 Search SciTech Connect for author "Daniels, J." Search SciTech Connect for...

  1. Directives Points of Contact

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

    cecelia.kenney@hq.doe.gov 202-586-4399 CF John Wall John.wall@hq.doe.gov 202-586-5728 CI Daniel Woomer Daniel.woomer@hq.doe.gov 202-586-9886 CTACNS Bud Danielson...

  2. Top 5 Maps and Interactive Graphics of 2014 | Department of Energy

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

    Top 5 Maps and Interactive Graphics of 2014 Top 5 Maps and Interactive Graphics of 2014 December 22, 2014 - 12:05pm Addthis Daniel Wood Daniel Wood Data Visualization and...

  3. Search for: All records | DOE PAGES

    Office of Scientific and Technical Information (OSTI)

    Results Filter by Author Bartsch, Michael S. (1) Branda, Steven S. (1) Edwards, Harrison S. (1) Kim, Hanyoup (1) Knight, Daniel L. (1) Lee, Daniel (1) Moseley, Caroline E....

  4. Advancing our Nuclear Collaboration with the Czech Republic ...

    Office of Environmental Management (EM)

    President Obama addresses a crowd in Hradcany Square on April 5, 2009, touching on issues from green energy to nuclear treaties. Daniel B. Poneman Daniel B. Poneman Former Deputy ...

  5. Argentina: An Important All-of-the-Above Energy Partner

    Broader source: Energy.gov [DOE]

    Deputy Energy Secretary Daniel Poneman recently visited Argentina to advance the bilateral energy relationship between the two countries.

  6. MEMORANDUM FOR CHIEF ACQUISITION OFFICERS

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

    Daniel I. Gordon Administrator for Federal Procurement Policy SUBJECT: "Myth-Busting": Addressing Misconceptions to Improve Communication

  7. Before the Subcommittee on Strategic Forces- House Armed Services Committee

    Broader source: Energy.gov [DOE]

    Subject: Security Incident at Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

  8. Original Workshop Proposal and Description

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

    ... Daniel Rokhsar, LBNL (Bioinformatics) ??? (environmental mod1eling ???) ??? (nano science) ??? (chemistry) ??? (computational neuroscience) Potential DoE and university- and ...

  9. Deputy Secretary Poneman Delivers Remarks on Nuclear Power at Tokyo American Center in Japan

    Office of Energy Efficiency and Renewable Energy (EERE)

    Energy Deputy Secretary Daniel Poneman spoke at the Tokyo American Center today about nuclear power after Fukushima.

  10. MEMORANDUM FOR CHIEF ACQUISITION OFFICERS

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

    Daniel I. Gordon Administrator for Federal Procurement Policy SUBJECT: "Myth-Busting": Addressing Misconceptions to Improve Communication

  11. MEMORANDUM FOR CHIEF ACQUISITION OFFICERS

    Office of Environmental Management (EM)

    Daniel I. Gordon Administrator for Federal Procurement Policy SUBJECT: "Myth-Busting": Addressing Misconceptions to Improve Communication...

  12. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... ; Schmidt, Fabian ; Senatore, Leonardo ; Smith, Kendrick M ; Whiteson, Daniel Aspen ... (Stanford University), and Kendrick Smith (Princeton University). less Full Text ...

  13. Space-Based Solar Power | Department of Energy

    Office of Environmental Management (EM)

    Space-Based Solar Power Space-Based Solar Power Graphics by Sarah Gerrity. Interactivity by Daniel Wood

  14. Before the Subcommittee on Oversight and Investigations- House Committee on Energy and Commerce

    Broader source: Energy.gov [DOE]

    Subject: Security Incident at the Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

  15. Secretary's Achievement Award (SING) | Department of Energy

    Office of Environmental Management (EM)

    SING) Secretary's Achievement Award (SING) (from left to right) Daniel Poneman; David Arakawa; Barbara Thibadeau; Phillip Kraushaar; Daniel Lehman; Ingrid Kolb (from left to right) Daniel Poneman; David Arakawa; Barbara Thibadeau; Phillip Kraushaar; Daniel Lehman; Ingrid Kolb Presented to: The Office of Science's Spallation Neutron Source Instruments - Next Generation (SING) Project The SING team capitalized on the technical and managerial efficiency gained by combining the five instruments into

  16. Secretary's Award of Excellence | Department of Energy

    Office of Environmental Management (EM)

    Award of Excellence Secretary's Award of Excellence (from left to right) Daniel Poneman; Chad Henderson; Jeff Pitman; Marc Jones; Daniel Lehman; Ingrid Kolb (from left to right) Daniel Poneman; Chad Henderson; Jeff Pitman; Marc Jones; Daniel Lehman; Ingrid Kolb Presented to: The Office of Science's Physical Sciences Facility (PSF) Project For demonstrating exceptional results in completing this complex $224 million project. The Pacific Northwest National Laboratory (PNNL) was facing the loss of

  17. Secretary's Improvement Award | Department of Energy

    Office of Environmental Management (EM)

    Improvement Award Secretary's Improvement Award (from left to right) Johnny Moore; Daniel Poneman; Gordon Fox; Marcus Jones; Daniel Lehman; Gary Bloom; Ingrid Kolb (from left to right) Johnny Moore; Daniel Poneman; Gordon Fox; Marcus Jones; Daniel Lehman; Gary Bloom; Ingrid Kolb Presented to: The Office of Science's Modernization of Laboratory Facilities (MLF) The MLF team successfully used the "Construction Manager at Risk" acquisition strategy at Oak Ridge National Laboratory. This

  18. Fast Times and Hot Spots in Plasmonic Nanostructures | Argonne...

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

    ... Structures Quantum & Energy Materials Nanofabrication & Devices Related People Gary Wiederrecht Daniel Rosenmann Next article: Spintronics: spin current from a paramagnet

  19. Staff | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Environmental Engineer Environmental Compliance NEPA (301) ... Felecia Johnson Personnel Security Specialist Contractor ... Daniel Middleton Nuclear Engineer Nuclear Safety Oversight ...

  20. TITLE AUTHORS SUBJECT SUBJECT RELATED DESCRIPTION PUBLISHER AVAILABILI...

    Office of Scientific and Technical Information (OSTI)

    Employment Impacts of Geothermal Electric Projects Entingh Daniel J GEOTHERMAL ENERGY POWER TRANSMISSION AND DISTRIBUTION CAPITAL CONSTRUCTION EMPLOYMENT EXPLORATION GEOTHERMAL...

  1. No Slide Title

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

    Dr. Ernest J. Moniz Secretary Daniel B. Poneman, Deputy Secretary* Edward B. Held Associate Deputy Secretary 6 Jun 20

  2. Community, Events

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

    ... Jr., in this October 1998 photo taken in Midland, Texas. ... experiences as a U.S. Air Force pilot flying B-1 and B-2 ... increase their revenue base and help diversify the area ...

  3. Microsoft Word - Copyright Template

    National Nuclear Security Administration (NNSA)

    1975 Beatley, J. C., 1975, Climates and Vegetation Pattern Across the MojaveGreat Basin Desert Transition of Southern Nevada, American Midland Naturalist, Vol. 93, pp, 53-77...

  4. Dow Chemical Company | Open Energy Information

    Open Energy Info (EERE)

    Company Jump to: navigation, search Name: Dow Chemical Company Place: Midland, MI Zip: 48667 Website: www.dow.com Coordinates: 43.6039709, -84.2370999 Show Map Loading map......

  5. Haakon County, South Dakota: Energy Resources | Open Energy Informatio...

    Open Energy Info (EERE)

    6 Climate Zone Subtype A. Places in Haakon County, South Dakota Midland, South Dakota Philip, South Dakota Retrieved from "http:en.openei.orgwindex.php?titleHaakonCounty,So...

  6. CX-006762: Categorical Exclusion Determination

    Office of Energy Efficiency and Renewable Energy (EERE)

    Texas Propane Fleet Pilot ProgramCX(s) Applied: A1, A7, B5.1Date: 09/14/2011Location(s): Midland, TexasOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  7. the Central Basin Platform,

    Office of Scientific and Technical Information (OSTI)

    ... As a result. it is believed that most of the structures formed within the context of an ... order to facilitate flexure modeling of the CBP and adjacent Delaware and Midland basins. ...

  8. untitled

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

    DOE'S PROPOSED FINANCIAL ASSISTANCE TO DOW KOKAM MI, LLC TO MANUFACTURE ADVANCED LITHIUM POLYMER BATTERIES FOR HYBRID AND ELECTRIC VEHICLES AT MIDLAND, MICHIGAN U.S. Department of Energy National Energy Technology Laboratory March 2010 DOE/EA-1708 FINAL ENVIRONMENTAL ASSESSMENT DOE'S PROPOSED FINANCIAL ASSISTANCE TO DOW KOKAM MI, LLC TO MANUFACTURE ADVANCED LITHIUM POLYMER BATTERIES FOR HYBRID AND ELECTRIC VEHICLES AT MIDLAND, MICHIGAN U.S. Department of Energy National Energy Technology

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

    SciTech Connect (OSTI)

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

    2013-03-01

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

  10. Superfund Record of Decision (EPA Region 7): Des Moines TCE Site, Operable Unit 3, Des Moines, IA. (Second remedial action), September 1992. Final report

    SciTech Connect (OSTI)

    Not Available

    1992-09-18

    The Des Moines TCE site is located southwest of downtown Des Moines, Polk County, Iowa. Land use in the area is predominantly industrial and commercial, and part of the site lies within the floodplain of the Raccoon River. Water from the Des Moines Water Works north infiltration gallery was found to be contaminated with trichloroethylene (TCE), dichloroethylene (DCE), and vinyl chloride at levels above accepted drinking water standards. The ROD addresses OU3, which encompasses potential sources of ground water contamination in an area north of the Raccoon River. The selected remedial action for OU3 includes no action with periodic groundwater monitoring.

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

    SciTech Connect (OSTI)

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

    2010-12-02

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

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    - IA 01 State University Ames Laboratory - IA 01 FUSRAP Considered Sites Site: Iowa State University Ames Laboratory (IA.01 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Wallace Road , Ames , Iowa IA.01-1 IA.01-2 Evaluation Year: Circa 1985 IA.01-3 Site Operations: Produced uranium and thorium metal, recovered uranium scrap, and conducted studies and experimental investigations in connection with chemistry and metallurgy

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    Direct Current's Energy Unit Calculator Direct Current's Energy Unit Calculator June 23, 2016 - 4:40pm Addthis This interactive map is not viewable in your browser. Please view it in a modern browser. Data, Methodology and Sources can be found here. Map by Daniel Wood. Daniel Wood Daniel Wood Data Visualization and Cartographic Specialist, Office of Public Affairs Learn More Check out Direct Current, Episode 2 to learn hear our story about our newly proposed energy units. Want to learn more

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    Past Recipents Daniel Shoemaker Daniel Shoemaker Named 23rd Rosen Prize Recipient Daniel P. Shoemaker, a postdoctoral fellow at Argonne National Laboratory, is the winner of the 23rd Rosen Prize. The prize, established in honor of Louis Rosen, the Father of LANSCE, is awarded for the most outstanding Ph.D. or M.S. thesis based on experimental or theoretical research performed at LANSCE. Criteria include the originality and scientific impact of the research and the student's contribution to the

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    Deputy Secretary Daniel Poneman and Iraqi President Jalal Talabani exchanging official photographs as they conclude their meeting. | Energy Department Photo Deputy Secretary Daniel Poneman and Iraqi President Jalal Talabani exchanging official photographs as they conclude their meeting. | Energy Department Photo Jen Stutsman Press Secretary, Office of Public Affairs Last week, as part of a week-long trip to the Middle East, Deputy Secretary Daniel Poneman led a U.S. interagency delegation for a

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    8-06 Audit Report: ER-B-98-06 April 1, 1998 Fluor Daniel Fernald's Use of Temporary Service Subcontractors The Department of Energy (Department) and Fluor Daniel Fernald (Fluor Daniel) implemented two work force restructurings at the Fernald Environmental Management Project between Fiscal Years (FY) 1994 and 1996. During the restructurings, the Department's cost for temporary service subcontracts increased from $2.8 million to $9.8 million annually. The objective of this audit was to determine

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    Publications, Softwaremodeling tools User Interface: Other Website: iatools.jrc.ec.europa.eubinviewIQToolWebHome.html IPTS-IA Tools Screenshot References: IPTS-IA Tools1...

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    Wind Energy Developer Horizon Wind Energy Energy Purchaser Ameren Location Northeastern IA IA Coordinates 43.450321, -92.551074 Show Map Loading map... "minzoom":false,"mappi...

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    In Service Owner Horizon Developer Horizon Energy Purchaser Na Location Northeastern IA IA Coordinates 43.450321, -92.551074 Show Map Loading map... "minzoom":false,"mappi...

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    to date have included the reduction of the number of active Issuing Authorities (IA), providing updated IA training, and requiring a Senior Review Board review and approval...

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    Organization Organization The organizational structure of the Office of International Affairs (IA) is as follows: Office of Resource Management (IA-10) Office of the Deputy ...

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    Author Affiliations Iowa State Univ., Ames, IA (United States) Xiamen Univ., Xiamen (China) Univ. of Science and Technology of China, Hefei (China) Ames Lab., Ames, IA (United...

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    PHYSICS; ACCURACY; COLOR; COSMOLOGICAL CONSTANT; LUMINOSITY; PHOTOMETRY; SHAPE; SUPERNOVAE Astrophysics,ASTRO",,"We combine the CfA3 supernovae Type Ia (SN Ia) sample with...

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    the Natural Gas Transmission and Storage System in the United States Daniel J. Zimmerle,* , Laurie L. Williams, Timothy L. Vaughn, Casey Quinn, R. Subramanian, ...

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    Armed Services Committee Before the Subcommittee on Strategic Forces - House Armed Services Committee Testimony of Daniel B. Poneman, Deputy Secretary of Energy Before the ...

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    Major Maintenance at Philpott Lake Daniel Brown Chief, Lakes Branch, Operations Division April 2, 2015 BUILDING STRONG GovernorExciter Replacement BUILDING STRONG Switchgear ...

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    class"field-item odd">Source: Energy Information Administration Short Term Energy Outlook. Chart by Daniel Wood.<...

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    Reduction of low potential electron acceptors requires the CbcL inner membrane cytochrome of Geobacter sulfurreducens Zacharoff Lori Chan Chi Ho ORCID Bond Daniel R Elsevier None...

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    localization andor polypeptide degradation. The invention also provides research tools for the study of protein function. Authors: Church, George M. 1 ; Janse, Daniel M....

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    July 31, 2015 Daniel Cohen Assistant General Counsel for Legislation, Regulation & Energy Efficiency Office of the General Counsel Department of Energy 1000 Independence Ave SW ...

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    The attendees were as follows: Lucas Adin, DOE Abigail B. Chingos, DOE Daniel Cohen, DOE Michael Kido, DOE Hampton Newsome, FTC (phone) Jennifer Cleary, AHAM Mark Drake, Electrolux ...

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    Energy) Jeremy Dommu (DOE-Office of Energy Efficiency and Renewable Energy) Daniel Cohen (DOE-Office of General Counsel) Andrew deLaski (Appliance Standards Awareness Project) ...

  4. Memo_exparte_August 29.pdf

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    The attendees were as follows: Dr. Kathleen Hogan, DOE David Catarious, Jr., DOE Daniel Cohen, DOE John Cymbalsky, DOE Kevin Messner, AHAM Jennifer Cleary, AHAM Douglas Johnson, ...

  5. Pharmacologic Profile of the Adnectin BMS-962476, a Small Protein...

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    Daniel ; Low, Simon ; Russo, Katie ; DiBella, Rose ; Denhez, Fabienne ; Gao, Mian ; Myers, Joseph ; Duke, Gerald ; Witmer, Mark ; Miao, Bowman ; Ho, Siew P. ; Khan, Javed ; ...

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    ; Proffen, Thomas E. ; Rodriguez, George ; Schwarz, Daniel E. ; Seidler, Gerald T. ; Taylor, Antoinette J. ; Trugman, Stuart A. ; Tyson, Trevor A. ; Valdez, James A. 1 ; SLAC) ...

  7. US Crude Oil Production Surpasses Net Imports | Department of...

    Office of Environmental Management (EM)

    US Crude Oil Production Surpasses Net Imports US Crude Oil Production Surpasses Net Imports Source: Energy Information Administration Short Term Energy Outlook. Chart by Daniel...

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    US Crude Oil Production Surpasses Net Imports US Crude Oil Production Surpasses Net Imports Source: Energy Information Administration Short Term Energy Outlook. Chart by Daniel ...

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    distribution in the Western U.S. WHO Deputy Secretary of Energy Daniel Poneman WHERE Lewis & Clark College Templeton Campus Center - Stamm Dining Room Portland, OR 97219 WHEN...

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    of the Bullet Cluster: Constraints on Inverse Compton Emission Wik, Daniel R.; NASA, Goddard Johns Hopkins U.; Hornstrup, A.; Denmark, Tech. U.; Molendi, S.; IASF,...

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    of the Bullet Cluster: Constraints on Inverse Compton Emission","Wik, Daniel R.; NASA, Goddard Johns Hopkins U.; Hornstrup, A.; Denmark, Tech. U.; Molendi, S.; IASF,...

  12. Translation-Coupling Cassette for Quickly and Reliably Monitoring...

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    Translation-Coupling Cassette for Quickly and Reliably Monitoring Protein Translation in Host Cells Inventors: Brian Pfleger, Daniel Mendez Perez Great Lakes Bioenergy Research...

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    Graduate research assistants Daniel Freppon, left, and Brett Boote in Emily Smith's research group use Raman spectroscopy to study growing corn plants. The technology allows ...

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    Washington, D.C. – Energy Deputy Secretary Daniel Poneman will make an important announcement today about a new Department of Energy initiative to accelerate partnerships between innovative...

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    Bryant ; Rumpf, Arthur Norman, ; Adkins, Douglas ; Hadizadeh, Rameen ; Copic, Davor ; Porter, Daniel ; Anderson, John M Publication Date: 2011-04-01 OSTI Identifier: 1108262 ...

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  18. Anomalous Dimensions and Non-Gaussianity (Journal Article) |...

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    Transport Phenomena and Interfacial Kinetics in Planar Microfluidic Membraneless Fuel Cells Abruna Hector Daniel Cornell University DIRECT ENERGY CONVERSION Our work is focused on...

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  2. Core Lithology, Valles Caldera No. 1, New Mexico | Open Energy...

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    phenomena. Authors Jamie N. Gardner, Fraser E. Goff, Sue Goff, Larry Maassen, K. Mathews, Daniel Wachs and D. Wilson Published Los Alamos National Laboratory, NM, 1987 Report...

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    Director, Energy Accounts 14 Craig, Jack R. Savannah River Site Site Manager 15 Daniel, Anamary Inspection Experts, Inc. Vice President 16 DeSimone, Michael SCI...

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  12. dpaulc | The Ames Laboratory

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  16. Understanding the Effect of Aerosol Properties on Cloud Droplet...

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  17. Secretary of Energy Advisory Board Subcommittee (SEAB) on Shale...

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    ... Defense Fund; Kathleen McGinty, Weston Solutions; Susan Tierney, Analysis Group; Daniel Yergin, IHS-Cambridge Energy Research Associates; Mark Zoback, Stanford University. ...

  18. Developing the New Bio-economy Workforce

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    Daniel Cassidy, National Institute of Food and Agriculture, presents on developing the new bioeconomy workforce for the Biomass/Clean Cities States Webinar.

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  20. dfreppon | The Ames Laboratory

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