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1

Archer Daniels Midland | Open Energy Information  

Open Energy Info (EERE)

Daniels Midland Daniels Midland Jump to: navigation, search Name Archer Daniels Midland Address 4666 Faries Parkway Place Decatur, IL Zip 62526 Sector Biofuels Product turn crops into renewable products Stock Symbol ADM Phone number 800-637-5843 Website http://www.adm.com/en-US/Pages Coordinates 39.867522°, -88.887033° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.867522,"lon":-88.887033,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

2

NETL: ICCS Area 1 - Archer Daniels Midland Company  

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

Archer Daniels Midland Company - Industrial Carbon Capture and Sequestration Archer Daniels Midland Company - Industrial Carbon Capture and Sequestration Archer Daniels Midland Company: CO2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone Decatur, Illinois PROJECT FACT SHEET Archer Daniels Midland Company: CO2 Capture from Biofuels Production and Storage into the Mt. Simon Sandstone [PDF-1.07MB] (Oct 2013) ENVIRONMENTAL REPORTS Archer Daniels Midland Company - Final Environmental Assessment Archer Daniels Midland Company - Finding of No Significant Impact CONSTRUCTION PHOTOS [PDF-1.5MB] PROGRAM PUBLICATIONS Information to come. PAPERS AND PRESENTATIONS Sai Gollakota, Highlights of the DOE-Sponsored Major Carbon Sequestration Projects, Presented at the Association of Rural Electric Generating Cooperatives (AREGC) Annual Conference, Salt Lake City, June 6-7, 2011. [PDF-1.12MB]

3

STATEMENT OF CONSIDERATIONS REQUEST BY ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN  

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

ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER ITS SUBCONTRACT WITH THE NATIONAL CORN GROWERS ASSOCIATION; DOE COOPERATIVE AGREEMENT NO. DE-FC36- 03G013147; W(A)04-024; CH1193 The Petitioner, Archer-Daniels-Midland Company (ADM), is a subcontractor of the National Corn Growers Association (NCGA), a nonprofit organization, under DOE Cooperative Agreement No. DE-FC36-03G013147 entitled "Separation of Corn Fiber and Subsequent Conversion of Fuels and Chemicals, Phase II: Pilot-scale Operation." The initial phase of this work was undertaken under DOE Contract No. DE-FC36-00GO10596 for which an advance waiver of patent rights was approved on May 1, 2001 (W(A)-00-029, CH-1045). This agreement

4

STATEMENT OF CONSIDERATIONS REQUEST BY ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN  

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

ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN ARCHER-DANIELS-MIDLAND COMPANY (ADM) FOR AN ADVANCED WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER ITS SUBCONTRACT WITH THE NATIONAL CORN GROWERS ASSOCIATION; DOE COOPERATIVE AGREEMENT NO. DE-FC36- 00GO10596; W(A)-00-029; CH-1045 The Petitioner, Archer-Daniels-Midland Company (ADM), is a subcontractor of the National Corn Growers Association (NCGA), a nonprofit organization, under DOE Cooperative Agreement No. DE-FC36-00GO10596 entitled "Separation of Corn Fiber and Subsequent Conversion of Fuels and Chemicals". The agreement is essentially a teaming arrangement between ADM, NCGA and the Pacific Northwest National Laboratory (PNNL). ADM has requested an advanced waiver of domestic and foreign patent rights for all subject inventions of its employees arising from its work under its subcontract.

5

Daniel Olsen  

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

Olsen Daniel Olsen High Tech and Industrial Systems Group Demand Response Research Center (DRRC) Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 90R3111 Berkeley CA 94720...

6

Daniel Arnold  

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

Arnold Arnold Mechanical Engineering Department University of California, Berkeley This speaker was a visiting speaker who delivered a talk or talks on the date(s) shown at the links below. This speaker is not otherwise associated with Lawrence Berkeley National Laboratory, unless specifically identified as a Berkeley Lab staff member. Daniel Arnold graduated with a BS in mechanical engineering from the University of California San Diego in 2005. He received his Masters the following year in the same department. His research focused on autonomous vehicle navigation with minimal sensory input. Since receiving his master's in 2006, Daniel has been employed by the Space and Naval Warfare Center in San Diego, Ca. where he worked as a test and evaluation engineer

7

Daniel Favrat  

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

Favrat Favrat Prof. & Director Swiss Federal Institute of Technology of Lausanne (EPFL) This speaker was a visiting speaker who delivered a talk or talks on the date(s) shown at the links below. This speaker is not otherwise associated with Lawrence Berkeley National Laboratory, unless specifically identified as a Berkeley Lab staff member. Professor Daniel Favrat obtained his Master and PhD in Mechanical Engineering from the Swiss Federal Institute of Technology of Lausanne (EPFL). He then worked in several industrial research centers in Canada and in Europe before becoming professor of thermodynamics and director of the Laboratory for Industrial Energy Systems of EPFL in 1988. He is a member of the Swiss academy of engineering sciences, of the Swiss advisory committee

8

Daniel W. Greb  

Science Conference Proceedings (OSTI)

Daniel W. Greb. Daniel W. Greb is an engineering technician in the Indoor Air Quality and Ventilation Group of the Energy ...

2012-07-06T23:59:59.000Z

9

STATEMENT OF CONSIDERATIONS REQUEST BY ARCHER-DANIELS-MIDLAND...  

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

WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER ITS SUBCONTRACT WITH THE NATIONAL CORN GROWERS ASSOCIATION; DOE COOPERATIVE AGREEMENT NO. DE-FC36- 03G013147; W(A)04-024;...

10

STATEMENT OF CONSIDERATIONS REQUEST BY ARCHER-DANIELS-MIDLAND...  

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

an economically viable separation and recovery process that allows the conversion of corn fiber into its major components. Each of those components can then be employed as a...

11

Archer Daniels Midland Company: CO2 Capture from Biofuels Production...  

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

Company: CO 2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone Background Carbon dioxide (CO 2 ) emissions from industrial processes, among other...

12

Daniel A. Hitchcock  

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

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

13

Daniel W. Bearden  

Science Conference Proceedings (OSTI)

Daniel W. Bearden. Dan's research has focused on nuclear magnetic resonance (NMR) since he started graduate school ...

2012-11-14T23:59:59.000Z

14

NREL: Energy Analysis - Daniel Steinberg  

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

Steinberg Photo of Daniel Steinberg Daniel Steinberg is a member of the Energy Forecasting and Modeling Group in the Strategic Energy Analysis Center. Energy and Environmental...

15

Daniel Shechtman and Quasicrystals  

Office of Scientific and Technical Information (OSTI)

Daniel Shechtman and Quasicrystals Daniel Shechtman and Quasicrystals Resources with Additional Information · Quasicrystals Saul Perlmutter Photo Courtesy of Ames Laboratory Daniel (Danny) Shechtman has won the 2011 Nobel Prize in Chemistry "for the discovery of quasicrystals". Shechtman was on 'sabbatical from the Technion [with] a two-year stint in the United States at what's now known as the National Institute of Standards and Technology'1 when he made his discovery. 'That 1982 discovery of crystalline materials whose atoms didn't line up periodically like every crystal studied during 70 years of modern crystallography is regarded as a revolutionary find that changed ideas about matter and its atomic arrangement. ... Shechtman was studying rapidly solidified aluminum alloys with a toolbox that included transmission electron microscopy, X-ray diffraction and neutron diffraction. The transmission electron microscopy revealed a structure that science said was impossible: a pattern that when rotated a full circle repeats itself 10 times.

16

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...

17

By Daniel Poneman  

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

'Perfect storm' sank Solyndra 'Perfect storm' sank Solyndra By Daniel Poneman The International Energy Agency projects that solar power will grow steadily, producing nearly a quarter of the world's electricity within four decades. Conservatively, that means more than $3 trillion worth of solar panels will need to be manufactured - a vast economic and employment opportunity to be seized by companies that succeed in this sector. Our competitors know this, and are playing to win. Winning will require substantial investments. Last year, for example, the China Development Bank offered more than $30 billion in financing to Chinese solar manufacturers, about 20 times more than U.S.- backed loans to solar manufacturers. Unfortunately, expanding production has coincided with short-term softening demand, a

18

Daniel Wood | Department of Energy  

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

Wood Wood About Us Daniel Wood - Data Integration Specialist Daniel Wood 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 Department's vast array of data. You can check out some of his work here. Prior to joining the Energy.gov team, Daniel worked at a large PR firm in Washington, D.C, doing web development and technical project management. Daniel is a graduate of Boston University but a true Philadelphian at heart. On his off days you are likely to find him exploring new neighborhoods on his bike or hanging out with the awesome kids over at Little Lights Urban Ministries. Most Recent The History of the Light Bulb November 22

19

Daniel Yergin | Department of Energy  

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

Daniel Yergin Daniel Yergin About Us Daniel Yergin - Chairman, IHS Cambridge Energy Research Associates Photo of Daniel Yergin Daniel Yergin is a highly respected authority on energy, international politics and economics. Dr. Yergin is a Pulitzer Prize winner and recipient of the United States Energy Award for "lifelong achievements in energy and the promotion of international understanding." He is both a world-recognized author and a business leader, as chairman of IHS Cambridge Energy Research Associates (CERA), one of the world's leading consulting and research firms in its field. He is also executive vice president of IHS, the parent company of CERA. Dr. Yergin received the Pulitzer Prize for his work The Prize: The Epic Quest for Oil, Money and Power, which became a number one best seller and

20

Midland, South Dakota geothermal district heating  

SciTech Connect

This article describes historical aspects and present usage of geothermal district heating systems in the town of Midland, South Dakota. The use of geothermal resources exists due to a joint venture between the school district and the city back in the early 1960`s. A total of approximately 30,000 square feet (2800 square meters) of floor space is heated using geothermal energy in Midland. This provides an estimated annual saving in propane cost of $15,000 to the community.

Lund, J.W.

1997-12-01T23:59:59.000Z

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


21

University of California, DavisDaniel Zinn 1 University of California, DavisDaniel Zinn 1 Daniel Zinn  

E-Print Network (OSTI)

University of California, DavisDaniel Zinn 1 University of California, DavisDaniel Zinn 1 Map of California, DavisDaniel Zinn 2 Outline Motivation Programing Model of MapReduce Hadoop ­ Free Java-based MR-Software Pig Latin ­ On top of MapReduce Beyond MapReduce #12;University of California, DavisDaniel Zinn 3

Ferrara, Katherine W.

22

Midland, Michigan: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Midland, Michigan: Energy Resources Midland, Michigan: Energy Resources (Redirected from Midland, MI) Jump to: navigation, search Equivalent URI DBpedia Coordinates 43.6155825°, -84.2472116° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.6155825,"lon":-84.2472116,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

23

Repowering of the Midland Nuclear Station  

E-Print Network (OSTI)

The conversion of the Midland Nuclear Station to a combined cycle power facility is the first of its kind. The existing nuclear steam turbine, combined with new, natural-gas-fired gas turbines, will create the largest cogeneration facility in the United States. The paper describes the project and the converted facility.

Gatlin, C. E. Jr.; Vellender, G. C.; Mooney, J. A.

1988-09-01T23:59:59.000Z

24

DLMF: ProfileDaniel W. Lozier  

Science Conference Proceedings (OSTI)

... Profile Daniel W. Lozier. ... version (See MathML) . A Printed Companion is available. Frank W. J. OlverRonald F. Boisvert.

2013-05-03T23:59:59.000Z

25

Midland District Heating District Heating Low Temperature Geothermal  

Open Energy Info (EERE)

Midland District Heating District Heating Low Temperature Geothermal Midland District Heating District Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Midland District Heating District Heating Low Temperature Geothermal Facility Facility Midland District Heating Sector Geothermal energy Type District Heating Location Midland, South Dakota Coordinates 44.0716539°, -101.1554178° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[]}

26

NREL: Energy Sciences - Daniel Ruddy  

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

Ruddy Ruddy Scientist III Photo of Daniel Ruddy Phone: (303) 384-6322 Email: dan.ruddy@nrel.gov At NREL Since: 2010 Dan Ruddy received a Ph.D. degree in Inorganic Chemistry from the University of California, Berkeley in 2008. His research combined synthetic molecular and materials chemistry with detailed characterization to study novel heterogeneous catalysts. He then worked on a variety of catalyst development projects at the Dow Chemical Company in the Renewable Feedstocks & Process Catalysis Group before joining the Chemical and Nanoscale Science Group at NREL in 2010. Dr. Ruddy's research at NREL integrates the synthesis and characterization of functional molecules and materials for advanced energy technologies including solar fuels production, biomass conversion catalysis, and next-generation PV materials.

27

Daniel M. Weeber | Department of Energy  

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

Daniel M. Weeber Daniel M. Weeber About Us Daniel M. Weeber - Assistant Inspector General for Audits and Administration Daniel M. Weeber was appointed Assistant Inspector General for Audits and Administration in July 2012. He directs the planning, execution and reporting of all audits for the Eastern Audits Division, which include the annual financial statement audit, information technology audits, special reviews, and performance reviews of the Department's major programs. Mr. Weeber also directs the activities of the Inspector General's Office of Planning, Administration, and Quality Assurance, overseeing the annual risk assessment and audit planning process, policy and guidance, staffing, and audit quality control. In this capacity, he leads a professional staff located in five geographical locations. Prior to his current

28

NREL: Biomass Research - Daniel J. Schell  

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

Daniel J. Schell Daniel J. Schell Photo of Daniel Schell Daniel Schell is a senior biochemical engineer and supervisor of the Bioprocess Integration R&D section of the National Bioenergy Center at NREL. Mr. Schell has more than 25 years of research experience in bio-based conversion of lignocellulosic biomass and has expertise in integrated operations at the bench and pilot scales. He also manages numerous projects for industrial clients investigating various aspects of lignocellulosic biomass conversion and currently leads a multi-disciplinary team of engineers, microbiologists, and chemists. Research Interests Integrated biomass processing High solids biomass conversion Fermentation development Separation processes Technoeconomic analysis Measurement uncertainty Pilot plant operation and process scale up

29

Daniel B. Poneman | Department of Energy  

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

Daniel B. Poneman Daniel B. Poneman About Us Daniel B. Poneman - Deputy Secretary of Energy Daniel B. Poneman Previously, he 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 leadership of Secretary of Energy Steven Chu, Mr. Poneman also served as Chief Operating Officer of the Department. Between April 23, 2013, and May 21, 2013, Mr. Poneman served as Acting Secretary of Energy. Mr. Poneman first joined the Department of Energy in 1989 as a White House Fellow. The next year he joined the National Security Council staff as Director of Defense Policy and Arms Control. From 1993 through 1996, Mr. Poneman served as Special Assistant to the President and Senior Director for Nonproliferation and Export Controls at

30

Isaac M. Daniel Walter P. Murphy Professor  

E-Print Network (OSTI)

and R. Byron Pipes, Society for Experimental Mechanics, Monograph No. 4, SEM, Bethel, CT, 1982; Second in Fracture Mechanics and Methods of Testing, Vol. ed. by G. C. Sih and A. M. Skudra in Series Handbook," in Handbook on Experimental Mechanics, 2nd ed., VCH Publishers, New York, 1993. I. M. Daniel and E. E. Gdoutos

Ottino, Julio M.

31

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

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

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...

32

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

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

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

33

Daniel, Utah: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Daniel, Utah: Energy Resources Daniel, Utah: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.4707885°, -111.4146275° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.4707885,"lon":-111.4146275,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

34

Midland County, Michigan: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Midland County, Michigan: Energy Resources Midland County, Michigan: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 43.5750978°, -84.3542049° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.5750978,"lon":-84.3542049,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

35

Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel...  

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

Daniel B. Poneman recently issued a joint Memorandum, entitled Personal Commitment to Health and Safety through Leadership, Employee Engagement, and Organizational Learning....

36

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

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

Midland - MI 06 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: Thorium MI.06-1 Radiological Survey(s): None Indicated Site Status: Eliminated from further consideration under FUSRAP Also see Documents Related to Dow Chemical Co. - Midland MI.06-1 - NRC Letter; R. G. Page to William E. Mott; Subject: List of contaminated or potentially contaminated sites; January 22, 1982;

37

Preliminary Notice of Violation, Fluor Daniel Fernald Corporation -  

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

Fernald Corporation - Fernald Corporation - EA-97-05 Preliminary Notice of Violation, Fluor Daniel Fernald Corporation - EA-97-05 July 29, 1997 Preliminary Notice of Violation issued to Fluor Daniel Fernald Corporation related to Corrective Actions Implementation Deficiencies at the Fernald Environmental Management Project, (EA-97-05) This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances surrounding the failure of the Fluor Daniel Fernald Corporation (FDF) to effectively complete corrective actions for the referenced noncompliance, although it informed the DOE Fernald Project Office that such work had been completed. Preliminary Notice of Violation, Fluor Daniel Fernald Corporation - EA-97-05 More Documents & Publications Preliminary Notice of Violation, Fluor Fernald, Inc. - EA-2005-05

38

Senate Confirms DOE Nominees Daniel Poneman, David Sandalow, Kristina  

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

Senate Confirms DOE Nominees Daniel Poneman, David Sandalow, Senate 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 Johnson, and Under Secretary for Science Steven Koonin. Also confirmed this week were Scott Blake Harris, General Counsel; David Sandalow, Assistant Secretary for Policy and International Affairs; and Ines Triay, Assistant Secretary for Environmental Management. Secretary Chu said, "We are fortunate to have such talented and dedicated

39

VBZ-0005- In the Matter of Fluor Daniel Fernald  

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

40

Type Ia Supernovae Project at NERSC  

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

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

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


41

Daniel Bugaris - Argonne National Laboratories, Materials Sicence Division  

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

EM > Daniel Bugaris EM > Daniel Bugaris Daniel E. Bugaris Daniel E. Bugaris Postdoctoral Appointee Bldg. 223, A-125 Phone: 630-252-5525 This e-mail address is being protected from spambots. You need JavaScript enabled to view it. Biography Daniel joined the Materials Science Division at Argonne National Laboratory in March 2012. His research focuses on the exploration of superconducting behavior in pnictide and intermetallic systems exhibiting competing interactions, as well as in narrow gap semiconductors. The aim of this program is to rationally design a homologous series of phases with tunable building blocks to enable the generation of specific compositions with predictable structures. Materials of interest will possess a high degree of structural and compositional freedom and chemical/electronic complexity with which to investigate (i) density-wave instabilities (spin and charge), and their suppression through chemical doping in order to generate superconductivity that may emerge from phase competition, and (ii) how narrow energy band gaps and facile doping properties could lead to a superconducting state. Daniel received his BS in Chemistry from the University of Notre Dame in 2005 and his PhD in Chemistry from Northwestern University in 2009, advised by Prof. James A. Ibers. His thesis research involved the solid-state chemistry of uranium halides and chalcogenides, with an emphasis on their crystal growth, structures, and physical properties. Daniel joined the research group of Prof. Hans-Conrad zur Loye at the University of South Carolina in October 2009 as a post-doctoral fellow, where he worked on the structural characterization of perovskite oxides via neutron diffraction in order to better understand their potential application as electrode materials in solid oxide fuel cells.

42

STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy Leaders  

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

STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy Leaders Headline 3-Day ARPA-E Summit STARTING TODAY: Bloomberg, Daniels, Musk, Pickens, Chu and Energy Leaders Headline 3-Day ARPA-E Summit February 25, 2013 - 1:59pm Addthis NEWS MEDIA CONTACT (202) 586-4940 Follow @energy on Twitter for live coverage of the ARPA-E Summit. Check the energy.gov blog for daily wrapups and photo galleries. WASHINGTON - 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 next week to discuss cutting-edge energy issues at the Advanced Research Projects Agency - Energy's (ARPA-E) fourth annual Energy Innovation

43

Daniel Cohen Assistant General Counsel for Legislation and Regulatory Law  

Energy.gov (U.S. Department of Energy (DOE)) 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 consensus agreement, 1 and the parties discussed legal questions relating to the Department of Energy's ability to adopt the consensus

44

More than words : a biography of Daniel Francis Burns  

E-Print Network (OSTI)

Daniel Francis Burns was born in Ireland in 1888 and immigrated to the United States in 1912. He married Mary O'Neill in 1923 and had a family of seven children. He worked as a police officer in the Boston Police Department ...

Burns, Matthew R. (Matthew Robert)

2005-01-01T23:59:59.000Z

45

Enforcement Letter, Fluor Daniel Hanford, Inc., H5-20- July 7, 1997  

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

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

46

Category:Mason, IA | Open Energy Information  

Open Energy Info (EERE)

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

47

5_5_09_Daniel_Poneman_Nomination.pdf  

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

Daniel B. Poneman Daniel B. Poneman Before the Committee on Energy and Natural Resources United States Senate May 5, 2009 Chairman Bingaman, Ranking Member Murkowski, and distinguished Members of the Committee, it is an honor and a privilege to appear before you today as President Obama's nominee to be Deputy Secretary of Energy. I would like to introduce my wife of nearly 25 years, Susan, and our sons, Michael and William. Our daughter, Claire, is away at college. I am grateful and humbled by the confidence that President Obama and Secretary Chu have expressed in me through this nomination. President Obama has articulated a clear and compelling vision of America's energy future - one that will transform our economy, protect our security, and save our planet from the worst impacts of climate change.

48

Deputy Secretary Daniel Poneman's Remarks to the International Forum for  

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

to the International to the International Forum for a Nuclear Weapons-Free World Deputy Secretary Daniel Poneman's Remarks to the International Forum for a Nuclear Weapons-Free World October 12, 2011 - 12:48pm Addthis 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. A fact sheet describing the broad scope of U.S.-Kazakh nuclear security cooperation is available here: http://nnsa.energy.gov/mediaroom/factsheets/uskazakhcooperation-0 Remarks: Good morning, ladies and gentlemen. It is an honor to have the opportunity to represent the United States today and to address such a distinguished group of dignitaries, leaders, and experts from around the world. President Obama could not be here today, but wanted to address this forum

49

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

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

to the Washington 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 years, the Washington Institute has provided valuable insight on Middle East issues and fostered dialogue that is critical to increasing awareness and understanding of the region. I'm honored to be a part of the conversation today. The United States has deep ties throughout the Middle East. Our interests in the region are fundamental to America's national, energy and economic

50

The Honorable Harold Rogers The Honorable Daniel K. Inouye  

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

Washington, DC 20585 (enter date here, centered) The Honorable Harold Rogers The Honorable Daniel K. Inouye Chairman, Committee on Appropriations Chairman, Committee on Appropriations U.S. House of Representatives U.S. Senate Washington, DC 20515 Washington, DC 20510 The Honorable Rodney P. Frelinghuysen The Honorable Dianne Feinstein Chairman, Subcommittee on Energy Chairman, Subcommittee on Energy and Water Development and Water Development Committee on Appropriations Committee on Appropriations U.S. House of Representatives U.S. Senate Washington, DC 20515 Washington, DC 20510 Subject: Notification of Pending Contract Award, or Public Announcement of Selected Applications for Negotiation of Financial Assistance Awards, or Pending Financial

51

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

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

Transportation Exercise to Test 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 Isolation Pilot Plant (WIPP). "This is an excellent opportunity for emergency responders to test the skills they've learned," said Dale Childers, assistant chief of the Odessa Fire Department and emergency management coordinator for Ector County. "It will also help us determine what improvements,

52

Prospective Type Ia supernova surveys from Dome A  

E-Print Network (OSTI)

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

Kim, A.

2010-01-01T23:59:59.000Z

53

Mr. Daniel Cohen U.S. Department of Energy  

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

March 21, 2011 March 21, 2011 Mr. Daniel Cohen U.S. Department of Energy Office of the General Council 1000 Independence Avenue, SW., Room 6A245 Washington, DC 20585-0121 Docket ID: DOE-HQ-2011-0014 Dear Mr. Cohen: This letter comprises the comments of the Pacific Gas and Electric Company (PG&E), Southern California Gas Company (SCGC), San Diego Gas and Electric (SDG&E), and Southern California Edison (SCE) in response to the U.S. Department of Energy's (DOE) Request for Information on Regulatory Burden. The signatories of this letter, collectively referred to herein as the California Investor Owned Utilities (CA IOUs) represent some of the largest utility companies in the Western United States, serving over 35 million customers. We support the development of efficiency standards by DOE's Appliances and Commercial Equipment

54

Deputy Secretary Daniel Poneman's Remarks at the Council on Competitiveness  

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

Council on Council on Competitiveness 25th Anniversary Summit -- As Prepared for Delivery Deputy Secretary Daniel Poneman's Remarks at the Council on Competitiveness 25th Anniversary Summit -- As Prepared for Delivery December 8, 2011 - 2:34pm Addthis Thank you, Sam, for the introduction. And thank you to the Council on Competitiveness for giving me the opportunity to speak here today. Congratulations on your 25th anniversary. For a quarter of a century, you have fostered dialogue and promoted ideas that have helped keep America competitive in the global economy. I applaud your focus on strengthening U.S. manufacturing and I appreciate the collaborative effort your members have undertaken to produce the report that the Council is releasing today. To say that its publication is timely would be an understatement.

55

Deputy Secretary Daniel Poneman's Remarks at the Tokyo American Center --  

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

the Tokyo American the Tokyo American Center -- As Prepared for Delivery Deputy Secretary Daniel Poneman's Remarks at the Tokyo American Center -- As Prepared for Delivery December 15, 2011 - 12:00pm Addthis 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 helped to support Japan across a broad range of energy issues. I also want to thank our hosts here at the Tokyo American Center for graciously providing me with the opportunity to speak with you this evening. And thank you to our many Japanese friends here tonight, for the warm welcome and bright hospitality. It is great to be back in Japan. Over the years I have visited Japan many times, but this is my first visit

56

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

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

IFNEC Meeting in 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 Cooperation Executive Committee meeting. Nuclear energy provides the world with hundreds of thousands of megawatts of clean, reliable, low-carbon power, and it has an important role to play as we work to achieve our global objectives to strengthen energy security, to spur economic growth and job creation, and to protect the environment.

57

Giangiacorno, SPE, Fluor Daniel (NPOSR), Inc.; D. Michael Dennis, Geo  

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

1 1 Field Testing of the Biocompetitive Exclusion Process for Control of Iron and Hydrogen Sulfides Leo A. Giangiacorno, SPE, Fluor Daniel (NPOSR), Inc.; D. Michael Dennis, Geo - Microbial Technologies, Inc. This paper was prepared for presentation at the 1997 SPE Rocky Mountain Regional Meeting held in Casper, Wyoming, 18 - 21 May 1997. This paper was selected for presentation by an SPE Program Committee following review of information contained in an abstract submitted by the author(s) Contents of the paper, as presented, have not been reviewed by the Society of Petroleum Engineers and are subject to co rrection by the author(s). The material, as presented, does not necessarily reflect any position of the Society of Petroleum Engineers, its officers, or members. Papers

58

Seismic attribute analyses of lower Permian (Wolfcampian-Leonardian) carbonate buildups, SW Midland, Texas  

E-Print Network (OSTI)

A trend of Wolfcampian-Leonardian carbonate buildups is located in the southwestern Midland Basin, Upton County, Texas. The buildup trend is located east of the eastern faulted margin of the Central Basin Platform and north of the Ozona Arch. Carbonate deposition began during lowstand times, within or just below wave base. In the Southwestern Midland Basin, the Wolfcampian-Leonardian carbonate interval is lithologically heterogeneous due to the presence of abundant lithoclastic debris that was shed from the uplifted Central Basin Platform. The lithologic heterogeneity makes it difficult to identify the buildups on seismic profiles. Several inferred buildups have been drilled in the past, but many boreholes only penetrated lithoclastic facies, not true buildup facies. Analyses of various seismic attributes were conducted for the Wolfcampian-Leonardian interval in the SW Midland Basin in an attempt to improve the recognition and imaging of the carbonate buildups. The objective was to identify a set of attributes that directly indicate the buildup locations. After extensive trial of various attributes, the variance attribute was selected as the optimum seismic attribute. The resultant 3D variance volume was used to detect the buildup locations, and some aspects of their internal stratigraphy, and to establish the fault framework in the Amacker survey. The instantaneous frequency attribute, combined with the variance attribute was also marginally useful for imaging the buildups. The variance attribute and instantaneous frequency were compared. Images generated from the variance attribute are better than those generated using the instantaneous frequency because on these images, it is possible to localize the buildups. The instantaneous frequency attribute combined with the variance attribute allows recognition of lithologic heterogeneities inside the buildup interval.

Decalf, Carole Christiane

2001-01-01T23:59:59.000Z

59

Depositional history of Lower Permian (Wolfcampian-Leonardian) carbonate buildups, Midland Basin, Upton County, Texas  

E-Print Network (OSTI)

A north-south oriented trend of Wolfcampian-Leonardian carbonate buildups is located in the southwestern Midland Basin, Upton County, Texas. The buildup trend is located west of the eastern faulted margin of the Central Basin Platform and north of the Ozona Arch. This trend was deposited during late Paleozoic time, just after major uplift of the Central Basin Platform and as the Midland Basin subsided. Chevron U.S.A. Production Company has actively explored for petroleum in the buildup trend since the early 1980s and loaned their data set to Texas A&M University for this study. The carbonate buildups lie stratigraphically within the Eddleman and Amacker formations. The Eddleman (middle Wolfcampian (PW-2)-late Wolfcampian (PW-3)) and smacker (early Leonardian (PL-1)-early middle Leonardian (PL-2-A)) formations are composed of varying amounts of shallow-water skeletal limestones, matrix-supported limestones, lithoclastic facies, and minor boundstone facies. Dominant grain types include dasycladacean green algae, Tubiphytes, phylloid algae, crinoids, fusulinids, foraminifera, and coated grains. Carbonate deposition begins during lowstand times within or just below wave base in a low energy environment. Separating the two carbonate units is a basibal dark-colored calcareous shale known informally as the Twenty-one formation (late Wolfcampian) that was deposited during a rapid relative sea-level rise. The Tippett shale overlies the Amacker formation and consists of transgressive, basibal, dark-colored calcareous shale that terminated carbonate deposition in the southwestern Midland Basin during early middle Leonardian time. Two basic types of carbonate buildups, skeletal-sand and carbonate-debris, have been identified in this interval. The buildups formed on a ramp-like depositional profile with subtle paleobathymetric highs and lows that were created by mostly post-strewn (middle Pennsylvanian) deformation. The importance of the paleohighs and lows is that the cleaner skeletal-sand buildups initiated growth within the paleolows, and the carbonate-debris buildups (largely sediment gravity-flow deposits) were deposited on paleohighs. The skeletal-sand buildups created synoptic relief during Leonardian time that forced sediment gravity-flows to move between the buildups. This resulted in the abrupt lateral facies transitions within the Eddleman-Amacker interval. Understanding the depositional history of this carbonate buildup trend is important for establishing models for carbonate deposition in the southwestern Midland Basin, where active deformation, rapid subsidence, and major sea-level fluctuations influenced sedimentation.

Merriam, Catherine O'Hara

1999-01-01T23:59:59.000Z

60

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

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

Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel 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 and U.S. Deputy Secretary of Energy Daniel B. Poneman today released survey results from a 500 participant smart meter In-Home Display pilot program begun last fall. Based on surveys, 71 percent of customers reported that they have changed their electricity consumption behavior as a result of the energy use data they accessed on their in-home displays.

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61

VWC-0002 - In the Matter of Daniel L. Holsinger | Department of Energy  

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

2 - In the Matter of Daniel L. Holsinger 2 - In the Matter of Daniel L. Holsinger VWC-0002 - In the Matter of Daniel L. Holsinger 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 pursuant to a decision by the Deputy Secretary of Energy. In a December 17, 1996 Decision Reversing and Remanding Initial Agency Decision, the Deputy Secretary instructed the Office of Hearings and Appeals (OHA) to conduct a full assessment of the equities involved concerning the reinstatement of Holsinger to a position of security guard at the DOE Federal Energy Technology Center (FETC), located in Morgantown, West Virginia. (1) Following that directive, I have held a hearing to take evidence and have considered the issues raised by

62

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

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

Centerpoint Energy and U.S. Deputy Secretary of Energy Daniel 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 August 2, 2011 - 7:08pm Addthis Poneman visits Houston to review progress of CenterPoint Energy's Smart Meter/Intelligent Grid Deployment Houston, TX - CenterPoint Energy, Inc.'s (NYSE:CNP) electric transmission and distribution subsidiary, CenterPoint Energy Houston Electric, LLC and U.S. Deputy Secretary of Energy Daniel B. Poneman today released survey results from a 500 participant smart meter In-Home Display pilot program begun last fall. Based on surveys, 71 percent of customers reported that they have changed their electricity consumption behavior as a result of the

63

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

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

10 Questions for a Batteries Expert: Daniel Abraham 10 Questions for a Batteries Expert: Daniel Abraham 10 Questions for a Batteries Expert: Daniel Abraham August 11, 2011 - 3:56pm Addthis Dan Abraham | Image Courtesy of Argonne National Laboratory Dan Abraham | Image Courtesy of Argonne National Laboratory Angela Hardin Media Specialist at Argonne National Laboratory "Almost every cell phone contains a lithium-ion battery; they are also in our cameras, camcorders, and computers. Our goal is to get the batteries into our cars - into the next generation of plug-in hybrid and electric vehicles." Dan Abraham, Batteries Expert Ed. note: This is a cross-post from Argonne National Laboratory. In the latest 10 Questions, Daniel Abraham, a leading scientist at Argonne National Laboratory, shares his work on lithium-ion batteries and why he

64

From TUNA Attribute Sets to Portuguese Text: a First Report Daniel Bastos Pereira Ivandr Paraboni  

E-Print Network (OSTI)

From TUNA Attribute Sets to Portuguese Text: a First Report Daniel Bastos Pereira Ivandré Paraboni" or even as "a boy") ­ will be discussed elsewhere. Given a TUNA attribute set as an input, we compute all

65

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

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

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...

66

Paradigm or pariah? : an architectural intervention into Daniel Burnham's timeless plan of Chicago  

E-Print Network (OSTI)

This thesis is not a eulogy to but an analysis of and contemporary intervention into Daniel Hudson Burnham's 1909 Plan of Chicago. It presses the boundary of what is known, and concentrates on dissecting and analyzing ...

Pettigrew, Paul Stephen

1988-01-01T23:59:59.000Z

67

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

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

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

68

Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Poneman  

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

Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Poneman issue Personal Commitment to Health and Safety of DOE employees Secretary of Energy Ernest J. Moniz and Deputy Secretary Daniel B. Poneman issue Personal Commitment to Health and Safety of DOE employees September 27, 2013 - 9:32am Addthis Photo courtesy of Oak Ridge Photo courtesy of Oak Ridge 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. "The Department's thousands of Federal, laboratory, and contractor employees work hard every day in pursuit of energy independence, global scientific leadership, national security, and environmental stewardship,"

69

Turbulent Combustion in Type Ia Supernova Models  

E-Print Network (OSTI)

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

F. K. Roepke; W. Hillebrandt

2006-09-15T23:59:59.000Z

70

New approaches for modeling type Ia supernovae  

SciTech Connect

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

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

2007-06-25T23:59:59.000Z

71

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

SciTech Connect

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.

Hovorka, Susan D.; Nava, Robin

2000-06-13T23:59:59.000Z

72

Theoretical cosmic Type Ia supernova rates  

E-Print Network (OSTI)

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

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

2008-07-15T23:59:59.000Z

73

Steamboat IA Geothermal Facility | Open Energy Information  

Open Energy Info (EERE)

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

74

The Perils of Consumption and the Gift Economy as the Solution Daniel Millers Consumption and Its Consequences  

E-Print Network (OSTI)

Press. Miller, D. (2012). Consumption and its consequences.The Perils of Consumption and the Gift Economy asSolution Daniel Millers Consumption and Its Consequences

Leahy, Terry

2013-01-01T23:59:59.000Z

75

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

Office of Scientific and Technical Information (OSTI)

Cathey Daniels 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! 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 June 10 helping formalize the addition of China to the WorldWideScience Alliance? In addition, now you can quickly narrow your WorldWideScience.org results list to the research you need, share them on social networking sites, bookmark your search, and set up alerts. 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 Published on Dec 05, 2007

76

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

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

Deputy Secretary Decision - In the Matter of Daniel L. Deputy Secretary Decision - In the Matter of Daniel L. Holsinger VWA-0005 - Deputy Secretary Decision - In the Matter of Daniel L. Holsinger 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 is a necessary and appropriate action to effect full relief for a retaliatory termination made by the previous security contractor, Watkins Security Agency, Inc., ("WSA"). Based upon my review of the regulatory language, the relevant case law, and the entire record, I conclude that OHA's decision is incorrect. Mr. Holsinger filed a complaint with the Office of Contractor Employee Protection ("OCEP") on October 7, 1994. R. 103-106. He alleged that he had

77

The progenitors of subluminous type Ia supernovae  

DOE Green Energy (OSTI)

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

Howell, D. Andrew

2001-02-01T23:59:59.000Z

78

Multi-Agent Simulation of Disaster Response Daniel Massaguer, Vidhya Balasubramanian, Sharad Mehrotra, and Nalini Venkatasubramanian  

E-Print Network (OSTI)

Multi-Agent Simulation of Disaster Response Daniel Massaguer, Vidhya Balasubramanian, Sharad on the context of disaster response. The ar- chitecture of DrillSim is based on a multi-agent simulation. The simulation of the disaster response activity is achieved by modeling each person involved as an agent

Venkatasubramanian, Nalini

79

Daniel E. Archer Ph.D., Experimental Nuclear Structure Physics, Florida State University, 1996  

E-Print Network (OSTI)

in radiation detectors for Homeland Security, the NMIS ­ Nuclear materials Identification System, and CMTB Highway Patrol in an effort to secure California borders against the nuclear threat; and acting as LeadDaniel E. Archer Ph.D., Experimental Nuclear Structure Physics, Florida State University, 1996 M

80

Recovering latent information in treebanks David Chiang and Daniel M. Bikel  

E-Print Network (OSTI)

Recovering latent information in treebanks David Chiang and Daniel M. Bikel University lexicalized TAG models in (Chiang, 2000; Sarkar, 2001; Chen and Vijay­ Shanker, 2000). Inducing a lexicalized­ searchers investigated this type of extraction to con­ struct stochastic TAG parsers (Chiang, 2000; Chen

Chiang, David

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


81

Transition events in butane simulations: Similarities across models Daniel M. Zuckermana)  

E-Print Network (OSTI)

Transition events in butane simulations: Similarities across models Daniel M. Zuckermana of long simulations of all-atom butane using both stochastic and fully solved molecular dynamics, we have behavior in molecular simulations has long been a topic of interest, and butane has been an important test

Zuckerman, Daniel M.

82

ADM, Cargill lose bid to end suit over corn-syrup price-fixing WASHINGTON, D.C. --Archer Daniels Midland Co., Cargill Inc. and another maker of corn sweeteners must face a trial  

E-Print Network (OSTI)

, an animal feed additive. ADM and closely held Cargill are the two biggest rivals in the $3 billion U. The justices, without comment Monday, declined to hear arguments by ADM, Cargill and A.E. Staley Manufacturing

Manga, Michael

83

Slide 1  

Science Conference Proceedings (OSTI)

Mark W. Collison, Ph. D., Director, Analytical Chemistry Research Division Archer Daniels Midland Company Current status of MCPD and Glycidol Analysis in Oils ARCHER DANIELS MIDLAND COMPANY 2 2012 -2013 AOCS Indirect Methods Collaborative M

84

Rates and progenitors of type Ia supernovae  

SciTech Connect

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

Wood-Vasey, William Michael

2004-08-16T23:59:59.000Z

86

Rolling Hills (IA) | Open Energy Information  

Open Energy Info (EERE)

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

87

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

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

Hon. Daniel B. Poneman Hon. Daniel B. Poneman Deputy Secretary U.S. Department of Energy Before the Subcommittee on Strategic Forces Committee on Armed Services U.S. House of Representatives February 28, 2013 Chairman Rogers, Ranking Member Cooper, and members of the Subcommittee, thank you for the invitation to appear before you today to provide the subcommittee details on the actions the Department has taken or will take to strengthen the security of the nuclear weapons complex in the wake of the July 2012 Y-12 incident. We appreciate the interest and engagement of this Committee and recognize the important oversight role that you fulfill. We also share the Committee's commitment to assure that all of our offices and operations are delivering on our mission safely and securely- from Washington, DC, to California, from every

88

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

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

Hanford Company - Hanford Company - EA-98-02 Preliminary Notice of Violation, Fluor Daniel Hanford Company - EA-98-02 March 26, 1998 Preliminary Notice of Violation 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) This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances surrounding criticality safety infractions and a violation of radiological controls which occurred between November 1996 and June 1997 at the Plutonium Finishing Plant (PFP), and an explosion that occurred in May 1997 at [a facility] of the PFP. The Office of Enforcement and Investigation, in coordination with the DOE Richland Operations Office

89

VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter of Daniel  

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

VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter of 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. 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 Appeals ("OHA") on remand from the Deputy Secretary adhering, after an additional evidentiary hearing and an assessment of the equities, to its earlier finding that reinstatement of Complainant Holsinger as a security guard is a necessary and appropriate action to effect full relief, even though it was the prior security contractor, Watkins Security Agency, Inc.,

90

VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter of Daniel  

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

VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter VWC-0001 and VWC-0002 - Deputy Secretary Decision - In the Matter of 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. 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 Appeals ("OHA") on remand from the Deputy Secretary adhering, after an additional evidentiary hearing and an assessment of the equities, to its earlier finding that reinstatement of Complainant Holsinger as a security guard is a necessary and appropriate action to effect full relief, even though it was the prior security contractor, Watkins Security Agency, Inc.,

91

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

Office of Science (SC) Website

Dr. Dr. Daniel A. Hitchcock Advanced Scientific Computing Research (ASCR) ASCR Home About Research Facilities Science Highlights Benefits of ASCR Funding Opportunities Advanced Scientific Computing Advisory Committee (ASCAC) News & Resources ASCR Discovery Monthly News Roundup News Archives ASCR Program Documents ASCR Workshops and Conferences ASCR Presentations 100Gbps Science Network Related Links Contact Information Advanced Scientific Computing Research U.S. Department of Energy SC-21/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-7486 F: (301) 903-4846 E: sc.ascr@science.doe.gov More Information » News & Resources Dr. Daniel A. Hitchcock Print Text Size: A A A RSS Feeds FeedbackShare Page Dr. Hitchcock came to DOE in 1983 to manage the Fusion Energy Theory

92

On the Brightness of Supernova Ia  

E-Print Network (OSTI)

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

Yijia Zheng

2013-10-01T23:59:59.000Z

93

Spectral diversity of Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2006-05-05T23:59:59.000Z

94

FIA-13-0075 - In the Matter of Daniel W. McKeel, Jr. | Department of Energy  

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

5 - In the Matter of Daniel W. McKeel, Jr. 5 - In the Matter of Daniel W. McKeel, Jr. FIA-13-0075 - In the Matter of Daniel W. McKeel, Jr. 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 determination issued by the National Nuclear Security Administration (NNSA). In his request, the Appellant asked for a copy of "any and all documents related to shipments by truck or rail, in the 1951-2000 time fram, of magnesium-thorium alloy metal plates, . . ., from Dow Madison, Illinois, Atomic Weapons Employer . . . [energy Employees Occupational Illness Compensation Program Act (EEOICPA)] site to the Rocky Flats (DOE) EEOICPA site in Golden, Colorado." NNSA found no responsive documents in the documents stored

95

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

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

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

96

Daniel Haskel  

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

"XAFS study of the low-temperature tetragonal phase of La2-xBaxCuO4: Disorder, stripes and Tc suppression at x0.125", D. Haskel, E. A. Stern, F. Dogan and A. Moodenbaugh,...

97

Daniel Fischer  

Science Conference Proceedings (OSTI)

... Leader, Synchrotron Methods, Ceramics Division, NIST 1991-2003: Physicist, Ceramics Division, NIST 1984-1991: Physicist, Exxon Research and ...

2013-04-17T23:59:59.000Z

98

Daniel Olsen  

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

and Aimee T. McKane. Opportunities for Automated Demand Response in Wastewater Treatment Facilities in California - Southeast Water Pollution Control Plant Case Study. CEC...

99

Daniel Boff  

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

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

100

Daniel Favrat  

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

industrial research centers in Canada and in Europe before becoming professor of thermodynamics and director of the Laboratory for Industrial Energy Systems of EPFL in 1988. He...

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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101

Daniel Arnold  

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

the mechanical engineering department. His research is focused on the implementation of residential demand side management via the introduction of communications infrastructure...

102

Daniel Josell  

Science Conference Proceedings (OSTI)

... has focused on advanced interconnects for ... Experimental and computational studies of solder joint ... Philosophy in Materials Science from Harvard's ...

2013-01-09T23:59:59.000Z

103

LINKING TYPE Ia SUPERNOVA PROGENITORS AND THEIR RESULTING EXPLOSIONS  

Science Conference Proceedings (OSTI)

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

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

2012-06-20T23:59:59.000Z

104

Fluor Daniel Hanford Inc. integrated safety management system phase 1 verification final report  

SciTech Connect

The purpose of this review is to verify the adequacy of documentation as submitted to the Approval Authority by Fluor Daniel Hanford, Inc. (FDH). This review is not only a review of the Integrated Safety Management System (ISMS) System Description documentation, but is also a review of the procedures, policies, and manuals of practice used to implement safety management in an environment of organizational restructuring. The FDH ISMS should support the Hanford Strategic Plan (DOE-RL 1996) to safely clean up and manage the site's legacy waste; deploy science and technology while incorporating the ISMS theme to ''Do work safely''; and protect human health and the environment.

PARSONS, J.E.

1999-10-28T23:59:59.000Z

105

Category:Des Moines, IA | Open Energy Information  

Open Energy Info (EERE)

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

106

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

Office of Legacy Management (LM)

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

107

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2008-01-01T23:59:59.000Z

108

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

Office of Legacy Management (LM)

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

109

Prepared Statement The Honorable Daniel B. Poneman Deputy Secretary of Energy  

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

Prepared Statement Prepared Statement The Honorable Daniel B. Poneman Deputy Secretary of Energy Before the Subcommittee of Oversight and Investigations Committee on Energy and Commerce U.S. House of Representatives July 24, 2013 Chairman Murphy, Ranking Member DeGette and Members of the Subcommittee: Thank you for the opportunity to discuss with you today the Department of Energy's ongoing efforts to improve its management and performance. These efforts are more important than ever, in light of the increasing responsibilities the President has entrusted to the Department. Let me explain. In the past month, the President has given two major policy speeches, and the work that we do at the Department of Energy lies at the heart of both of these issues.

110

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

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

demosEUROPA Event in 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 together to achieve our shared energy goals. I am reminded of the dramatic moments when the whole world was watching the Gdańsk shipyards. Now, we can look back at those events with the patina of historical inevitability, but at the time, the outcome was much less evident. As a global community, we watched this battle for freedom unfold

111

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

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

June 19, 2012 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 represents manufacturers of major, portable and floor care home appliances, and suppliers to the industry. AHAM's more than 150 members employ tens of thousands of people in the U.S. and produce more than 95% of the household appliances shipped for sale within the

112

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

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

2011 U.S.-China 2011 U.S.-China Relations Conference - As Prepared for Delivery Deputy Secretary Daniel Poneman's Remarks at the 2011 U.S.-China Relations Conference - As Prepared for Delivery October 24, 2011 - 12:00pm Addthis 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 experts convened by Secretary Chu to offer recommendations on how to improve the safety and environmental performance of shale gas drilling. I am honored to be here today with my distinguished colleagues Cao Jianlin, China's Vice Minister of Science and Technology, and Zhu Weilin with the China National Offshore Oil Corporation. Over the past decade, the U.S.-China Relations Conference, championed by

113

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

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

1, 2011 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: 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. Reg. 6123 (Feb. 3, 2011). AHAM represents manufacturers of major, portable and floor care home appliances, and suppliers to the industry. AHAM's more than 150 members employ tens of thousands of people in the U.S. and produce more than 95% of the household appliances shipped for sale within the

114

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

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

August 1, 2011 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 rules, 76 Fed. Reg. 40646 (July 11, 2011). AHAM represents manufacturers of major, portable and floor care home appliances, and suppliers to the industry. AHAM's more than 150 members employ tens of thousands of people in the U.S. and produce more than 95% of the household appliances shipped for sale within the

115

Conformal cosmological model and SNe Ia data  

SciTech Connect

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

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

2012-11-15T23:59:59.000Z

116

The Distant Type Ia Supernova Rate  

DOE R&D Accomplishments (OSTI)

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

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

2002-05-28T23:59:59.000Z

117

AN ABSTRACT OF THE THESIS OF Daniel Alan Peterson for the degree of Master of Science in  

E-Print Network (OSTI)

Methane-Steam Reformer Abstract approved: Sourabh V. Apte Numerical modeling of methane-steam reforming numerical framework. Methane-steam reforming is modeled by three reduced-order reactions occurring Simulation of Micro/Mini-Channel based Methane-Steam Reformer by Daniel Alan Peterson A THESIS submitted

Apte, Sourabh V.

118

Burning Thermals in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

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

Bell, John B.

119

Visualizing Type Ia Supernova Explosions at NERSC  

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

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

120

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

Gasoline and Diesel Fuel Update (EIA)

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

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


121

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

Office of Legacy Management (LM)

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

122

Late Light Curves of Normally-Luminous Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2006-01-05T23:59:59.000Z

123

UMore Ph IA CR Report 7-8-10.pdf  

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

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

124

TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM  

SciTech Connect

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

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

2013-07-01T23:59:59.000Z

125

VELOCITY EVOLUTION AND THE INTRINSIC COLOR OF TYPE Ia SUPERNOVAE  

SciTech Connect

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

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

2011-12-01T23:59:59.000Z

126

The Rate of Type Ia Supernovae at High Redshift  

E-Print Network (OSTI)

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

Brian J. Barris; John L. Tonry

2005-09-22T23:59:59.000Z

127

The diversity of Type Ia Supernovae: evidence for systematics?  

E-Print Network (OSTI)

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

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

2004-11-02T23:59:59.000Z

128

DISTRIBUTED FLAMES IN TYPE Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

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

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

2010-02-20T23:59:59.000Z

129

Redshift-Independent Distances to Type Ia Supernovae  

E-Print Network (OSTI)

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

Brian J. Barris; John L. Tonry

2004-08-04T23:59:59.000Z

130

NETL: Major Demonstrations Reference Shelf  

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

Shelf Previous Next Recovery Act: Re-utilization of Industrial Carbon Dioxide for Algae Production Using a Phase Change Material Archer Daniels Midland Company: CO2 Capture...

131

 

Science Conference Proceedings (OSTI)

THOMAS H. SMOUSE MEMORIAL FELLOWSHIP MAJOR CONTRIBUTORS: American Oil Chemists Society American Oil Chemists Society Foundation Archer Daniels Midland Company PROGRAM DESCRIPTION and APPLICATION INSTRU

132

This Week at NETL  

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

and is now operating four surface seismic sensors at the Archer Daniels Midland corn processing complex in Decatur, Ill. The sensors, which surround the injection well of...

133

Albany, OR * Anchorage, AK * Morgantown, WV * Pittsburgh, PA...  

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

Archer Daniels Midland Company: CO 2 Capture from Biofuels Production and Storage into the Mt. Simon Sandstone Background Carbon dioxide (CO 2 ) emissions from industrial...

134

ADM Cabrera JV | Open Energy Information  

Open Energy Info (EERE)

to: navigation, search Name ADM Cabrera JV Place Sao Jose do Rio Preto, Sao Paulo, Brazil Product Archer Daniels Midland Company (ADM) and Grupo Cabrera have formed a...

135

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

Open Energy Info (EERE)

Illinois. Registered Energy Companies in Illinois' 18th congressional district Archer Daniels Midland Aventine Renewable Energy Holdings Aventine Renewable Energy Inc Caterpillar...

136

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

E-Print Network (OSTI)

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

2008-01-01T23:59:59.000Z

137

Nucleosynthesis in type Ia supernovae driven by asymmetric thermonuclear ignition  

Science Conference Proceedings (OSTI)

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

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

2012-11-12T23:59:59.000Z

138

High-Speed Internet Access via HVAC Ducts: A New Approach Daniel D. Stancil, Ozan K. Tonguz, Ariton Xhafa, Ahmet Cepni, and Pavel Nikitin  

E-Print Network (OSTI)

High-Speed Internet Access via HVAC Ducts: A New Approach Daniel D. Stancil, Ozan K. Tonguz, Ariton conditioning (HVAC) ducts for indoor wireless transmission systems and networks. Mea- surements and system to 100 Mbps should be possible, when HVAC system is used in con- junction with OFDM technology. Keywords

Stancil, Daniel D.

139

Organic-vapor-liquid-solid deposition with an impinging gas jet Daniel W. Shaw, Kevin Bufkin, Alexandr A. Baronov, Brad L. Johnson, and David L. Patrick  

E-Print Network (OSTI)

Organic-vapor-liquid-solid deposition with an impinging gas jet Daniel W. Shaw, Kevin Bufkin gas jet to a substrate coated by a thin liquid solvent layer. Films of the organic semiconductor, and the results compared to experiment. The combination of gas jet delivery with an organic-vapor-liquid

Patrick, David L.

140

Design Procedure for a Very High Speed Slotless Permanent Magnet Motor Pierre-Daniel Pfister, Student Member, IEEE and Yves Perriard, Senior Member, IEEE  

E-Print Network (OSTI)

Design Procedure for a Very High Speed Slotless Permanent Magnet Motor Pierre-Daniel Pfister speed slotless permanent magnet motor design procedure using an analyti- cal model. The multiphysics magnet (PM) motors are increasingly demanded on the market [1]. In a VHS motor, the different parts

Psaltis, Demetri

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141

A 200 000 rpm, 2 kW Slotless Permanent Magnet Pierre-Daniel Pfister, Student Member IEEE and Yves Perriard, Senior Member IEEE  

E-Print Network (OSTI)

A 200 000 rpm, 2 kW Slotless Permanent Magnet Motor Pierre-Daniel Pfister, Student Member IEEE high speed (200 krpm, 2 kW) slotless permanent magnet motor, using an analytical model that reached 200 krpm. Index Terms--Very high speed, Slotless permanent magnet motor, Multiphysics analytical

Psaltis, Demetri

142

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

E-Print Network (OSTI)

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

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

2000-01-01T23:59:59.000Z

143

Progenitors of type Ia supernovae in elliptical galaxies  

Science Conference Proceedings (OSTI)

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

Gilfanov, M.; Bogdan, A.

2011-09-21T23:59:59.000Z

144

Learning from the scatter in type ia supernovae  

SciTech Connect

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

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

2005-11-01T23:59:59.000Z

145

Type Ia Supernova Spectral Line Ratios as LuminosityIndicators  

SciTech Connect

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

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

2005-12-07T23:59:59.000Z

146

Investigating the Flame Microstructure in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2002-04-02T23:59:59.000Z

147

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

E-Print Network (OSTI)

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

Patat, F

2004-01-01T23:59:59.000Z

148

Could There Be A Hole In Type Ia Supernovae?  

E-Print Network (OSTI)

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

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

2003-11-01T23:59:59.000Z

149

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

Science Conference Proceedings (OSTI)

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

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

2012-08-10T23:59:59.000Z

150

THE DIFFUSE GAMMA-RAY BACKGROUND FROM TYPE Ia SUPERNOVAE  

SciTech Connect

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

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

2012-03-10T23:59:59.000Z

151

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

E-Print Network (OSTI)

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

F. Patat

2004-09-28T23:59:59.000Z

152

Turbulence-Flame Interactions in Type Ia Supernovae  

SciTech Connect

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

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

2008-05-27T23:59:59.000Z

153

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

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

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

2008-11-17T23:59:59.000Z

154

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

Gasoline and Diesel Fuel Update (EIA)

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

155

Microsoft PowerPoint - IEEE IAS PES 102313.pptx  

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

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

156

Type Ia Supernova: Burning and Detonation in the Distributed Regime  

E-Print Network (OSTI)

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

S. E. Woosley

2007-09-26T23:59:59.000Z

157

Daniel R. Flynn  

Science Conference Proceedings (OSTI)

... up to 1300 K, design of an improved apparatus for determination of the thermal conductivity of refractory materials using a steam calorimeter, and ...

2012-07-06T23:59:59.000Z

158

Dr. Daniel A. Veronica  

Science Conference Proceedings (OSTI)

... to NIST, Dan managed the Karl Larson Building Energy Systems Laboratory at ... engineering and deck officer on US Navy nuclear submarines, and ...

2012-07-06T23:59:59.000Z

159

Abstract for Daniel Phillips  

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

Phillips ohio University, Athens Using chiral perturbation theory to extract the neutron-neutron scattering length from pi- d->gamma nn The up and down quarks do not have equal...

160

Daniel N. Madrzykowski  

Science Conference Proceedings (OSTI)

... has conducted a study with 20 MW gas/oil well fires to determine the radiation reduction effects of small quantities of water spray entrained near the ...

2010-11-05T23:59:59.000Z

Note: This page contains sample records for the topic "daniels midland ia" from the National Library of EnergyBeta (NLEBeta).
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161

Dr. Daniel Siderius  

Science Conference Proceedings (OSTI)

... Adsorbent materials have a wide range of actual and potential application, including gas storage, carbon capture, mitigation of environmental ...

2013-02-14T23:59:59.000Z

162

Female community leaders in Houston, Texas: a study of the education of Ima Hogg and Christia Daniels Adair  

E-Print Network (OSTI)

Houston, Texas, the fourth largest metropolitan area in the United States, has several structures named after historically male leaders of the city?George R. Brown Convention Center, Mickey Leland Federal Building, William P. Hobby Airport, and Jesse H. Jones Hall. However, Houston women have also had a history that included positions of leadership in the community. Not only were women instrumental in creating the citys cultural institutions such as the Houston Symphony, Alley Theater, and Houston Public Library, but female community leaders were also responsible for social and political reforms including the integration of public facilities in Houston and the campaign for womens suffrage. These women leaders have not been recognized, and there are no public buildings in Houston that bear the names of women. This study seeks, in part, to make known the achievements of two women?one white, one black?who played an integral part in the political and cultural fabric of twentieth century Houston. The purpose of this dissertation was to analyze the relationship between educational experience and community leadership in the lives of two female community leaders in Houston, Texas, Ima Hogg and Christia Daniels Adair. Utilizing published interviews, government records, and manuscript collections, I detail the beliefs and values taught and modeled by parents and reinforced by church, school, and community, as well as the knowledge and skills developed through organizational work and self-directed study. Upon initial observation, the lives of Ima Hogg and Christia Adair seemed quite different, separated by issues of race and class. However, by examining both the formal and informal educational experiences of these two women, common patterns or themes emerged. The themes were identified as service to community, expectations of success and leadership, a belief in the value of education and lifelong learning, and the development of leadership skills. The informal educational experience, in particular, proved to be especially significant in the development of leadership skills for these women and in their eventual roles as community leaders. Using these themes, this study analyzes the education of two female community leaders as a way of understanding the relationship between womens education and womens achievement.

Black, Linda L.

2008-12-01T23:59:59.000Z

163

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

E-Print Network (OSTI)

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

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

2008-01-31T23:59:59.000Z

164

Lithologic characteristics, depositional environments and geometries of reservoir and nonreservoir facies in the Queen Formation (Guadalupian, Permian) of Moose and Virey Fields, Midland County, Texas  

E-Print Network (OSTI)

The Queen Formation is a member of the Artesia Group, which is a sequence of intermingling carbonates, classics and evaporates that were deposited during Guadalupian (Permian) time across the Northwest Shelf, Central Basin Platform, and Midland Basin of the Permian Basin, west Texas and southeastern New Mexico. In Moose and Virey Fields, the Queen is the main producing formation and consists entirely of intercepted back-reef shelf elastics and evaporates which were deposited in a variety of continental desert and marginal marine settings. The Queen desert was a broad and generally low-relief surface transected by warm temperatures, semi-arid climate, scarce vegetation, and alternating periods of dryness and intense storm-induced flashflooding. Sedimentation within the Queen desert took place in six separate depositional environments. The elastics of Moose and Virey Fields were deposited in proximal fluvial sandflat and fluvial-dominated sabra environments, and along the edge of a shallow hypersaline lagoon. The anhydrides (formerly gypsum) were precipitated subaqueously on the floor of and in the subsurface beneath a broad and shallow, hypersaline lagoon which was characterized by poor circulation and restriction from the normal marine environment. Some halides formed subaqueously in a large, but very shallow, isolated inland saliva situated in the topographic lows of the desert sabkha. Other halides formed in an ephemeral and sometimes desiccated salt-pan environment which was subjected to alternating 'wet' and 'dry' conditions. It is believed that the progression of depositional environments across the study area was in part controlled by fourth- and fifth-order relative sea level fluctuations during a major third-order marine regression. Two large subsurface structural collapse features with at least 200 feet of vertical relief are located in the central portions of Moose and Virey Fields. The collapse of the Queen Formation in these areas was induced by the post-depositional and post-burial dissolution of the halides primarily of the underlying Grayburg Formation, and to a lesser extent of the Queen Formation. It apparently occurred as a series of minor collapse events which first began in Post-oueen Guadalupian time, during deposition of the lower Seven Rivers Formation, and finally ended in the Ochoan during deposition of the Rustler Anhydrite.

Aller, Gregory Shane

1999-01-01T23:59:59.000Z

165

Fitting Type Ia supernovae with coupled dark energy  

E-Print Network (OSTI)

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

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

2004-01-01T23:59:59.000Z

166

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

E-Print Network (OSTI)

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

Juramy, Claire

2006-01-01T23:59:59.000Z

167

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

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

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

168

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

E-Print Network (OSTI)

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

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

2008-09-18T23:59:59.000Z

169

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

SciTech Connect

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

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

2008-02-28T23:59:59.000Z

170

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

Science Conference Proceedings (OSTI)

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

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

2012-07-01T23:59:59.000Z

171

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

E-Print Network (OSTI)

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

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

2006-03-03T23:59:59.000Z

172

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

SciTech Connect

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

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

2012-06-01T23:59:59.000Z

173

EARLY PHASE OBSERVATIONS OF EXTREMELY LUMINOUS TYPE Ia SUPERNOVA 2009dc  

Science Conference Proceedings (OSTI)

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

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

2009-12-20T23:59:59.000Z

174

Energy Department Applauds Nation's First Large-Scale Industrial...  

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

one million tons of carbon dioxide (CO2) per year produced as the result of processing corn into fuel-grade ethanol from the nearby Archer Daniels Midland biofuels plant. Since...

175

designed to store approximately ...  

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

each year in the Illinois Basin region. The injected CO 2 is a byproduct from processing corn into fuel-grade ethanol at Archer Daniels Midland Company's (ADM) biofuels plant near...

176

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

Science Conference Proceedings (OSTI)

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

Saurabh W. Jha

2012-10-03T23:59:59.000Z

177

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

E-Print Network (OSTI)

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

Miko?ajewska, J

2011-01-01T23:59:59.000Z

178

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

SciTech Connect

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

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

2011-09-01T23:59:59.000Z

179

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

E-Print Network (OSTI)

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

180

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

E-Print Network (OSTI)

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

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

2000-08-21T23:59:59.000Z

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181

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

SciTech Connect

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

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

2012-10-20T23:59:59.000Z

182

SAS Output  

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

Coal Consumers in the Manufacturing and Coke Sectors, 2012" Coal Consumers in the Manufacturing and Coke Sectors, 2012" "Company Name","Plant Location" "Top Ten Manufacturers" "American Crystal Sugar Co","MN, ND" "Archer Daniels Midland","IA, IL, MN, ND, NE" "Carmeuse Lime Stone Inc","AL, IL, IN, KY, MI, OH, PA, TN, VA, WI" "Cemex Inc","AL, CA, CO, FL, GA, KY, OH, TN, TX" "Dakota Gasification Company","ND" "Eastman Chemical Company","TN" "Georgia-Pacific LLC","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 Corporation","AL, IN, MI, MN"

183

U.S. Energy Information Administration | Annual Coal Report 2012  

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

Coal Consumers in the Manufacturing and Coke Sectors, 2012 Coal Consumers in the Manufacturing and Coke Sectors, 2012 U.S. Energy Information Administration | Annual Coal Report 2012 Table 25. Coal Consumers in the Manufacturing and Coke Sectors, 2012 U.S. Energy Information Administration | Annual Coal Report 2012 Company Name Plant Location Top Ten Manufacturers American Crystal Sugar Co MN, ND Archer Daniels Midland IA, IL, MN, ND, NE Carmeuse Lime Stone Inc AL, IL, IN, KY, MI, OH, PA, TN, VA, WI Cemex Inc AL, CA, CO, FL, GA, KY, OH, TN, TX Dakota Gasification Company ND Eastman Chemical Company TN Georgia-Pacific LLC 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 Corporation AL, IN, MI, MN Other Major Manufacturers Ash Grove Cement Co

184

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

Open Energy Info (EERE)

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

185

IA REP0 SAND85-2809 Unlimited Release UC-92A  

Office of Scientific and Technical Information (OSTI)

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

186

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

E-Print Network (OSTI)

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

Meng, Xiangcun

2013-01-01T23:59:59.000Z

187

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

Science Conference Proceedings (OSTI)

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

Munroe J.; Wilkins K.; Gruber M.

2000-05-01T23:59:59.000Z

188

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

E-Print Network (OSTI)

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

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

2009-01-01T23:59:59.000Z

189

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

E-Print Network (OSTI)

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

Minnihan, Ellen Catherine

190

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

SciTech Connect

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

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

2013-01-10T23:59:59.000Z

191

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

SciTech Connect

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

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

2005-04-01T23:59:59.000Z

192

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

E-Print Network (OSTI)

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

Nora Bretn; Ariadna Montiel

2013-03-06T23:59:59.000Z

193

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

E-Print Network (OSTI)

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

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

2003-12-03T23:59:59.000Z

194

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

E-Print Network (OSTI)

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

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

2010-01-01T23:59:59.000Z

195

Keynote Address Daniel B. Poneman  

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

Expert Laura Turner Seydel is a nationally recognized environmental advocate and eco-living expert committed to the education, conservation and efforts working to continuously...

196

Prepared by: Tosin Daniel Oyetoyan  

E-Print Network (OSTI)

in Smartgrid Some Available Open Source Smartgrid Software Repositories http://code.google.com http://sourceforge.net/ http://www.codeplex.com/ http://www.ohloh.net Search terms "Smart grid", "Smartgrid", "smart meter

197

NREL: Energy Analysis - Daniel Getman  

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

of the Data Analysis and Visualization Group in the Strategic Energy Analysis Center. GIS Scientist IV - Geospatial Section Supervisor On staff since March 2010 Phone number:...

198

NREL: Biomass Research - Daniel Inman  

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

us to examine the feasibility of alternative process configurations. Learn more about Biomass Technology Analysis at NREL. System Dynamics I am also interested in dynamic modeling...

199

Daniel Sperling Professor and Director  

E-Print Network (OSTI)

and wasteful for everyone · 30 years ago ­ Synfuels (oil shale, coal) · 22 years ago ­ Methanol (and CNG) · 18 Produced WEO required Cumulative 2030 Arctic Deep Water Super Deep EOR Heavy oil Bitumen Oil Shale Other Already Produced WEO required Cumulative 2030 Arctic Deep Water Super Deep EOR Heavy oil Bitumen Oil Shale

California at Davis, University of

200

"1. Victor J Daniel Jr","Gas","Mississippi Power Co",1992 "2. Grand Gulf","Nuclear","System Energy Resources, Inc",1251  

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

Mississippi" Mississippi" "1. Victor J Daniel Jr","Gas","Mississippi Power Co",1992 "2. Grand Gulf","Nuclear","System Energy Resources, Inc",1251 "3. Baxter Wilson","Gas","Entergy Mississippi Inc",1176 "4. Jack Watson","Coal","Mississippi Power Co",998 "5. Magnolia Power Plant","Gas","Magnolia Energy LP",863 "6. Batesville Generation Facility","Gas","LSP Energy Ltd Partnership",858 "7. Reliant Energy Choctaw County","Gas","RRI Energy Wholesale Generation LLC",848 "8. TVA Southaven Combined Cycle","Gas","Tennessee Valley Authority",774

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


201

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

E-Print Network (OSTI)

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

Shojai, F

2013-01-01T23:59:59.000Z

202

On the hydrogen emission from the type Ia supernova 2002ic  

DOE Green Energy (OSTI)

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

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

2003-12-10T23:59:59.000Z

203

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

E-Print Network (OSTI)

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

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

2004-01-01T23:59:59.000Z

204

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

E-Print Network (OSTI)

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

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

2003-12-08T23:59:59.000Z

205

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

E-Print Network (OSTI)

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

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

2007-06-07T23:59:59.000Z

206

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

E-Print Network (OSTI)

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

F. K. Roepke

2007-09-26T23:59:59.000Z

207

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  

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

14%20-%20Daniel%20Cohen%20-%20GC/Comments%20from%20FDMS/Dan%20Manole%20DRAFT-0004.html[3/23/2011 2:21:55 PM] 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: 2700 Crestridge Court N/A Suwanee, GA, 30024 Email: dan_manole@irco.com Phone: 770-291-2378 Submitter's Representative: Dan Manole Organization: Hussmann General Comment See attached file(s) Attachments DOE-HQ-2011-0014-DRAFT-0004.1: Comment on FR Doc # 2011-02368 From: Dan Manole, Regulatory Compliance Manager, Hussmann Corporation

208

O:\IM-20\E-Government Program Office\FDMS\FDMS database\DOE\2011\DOE-HQ-2011-0014 - Daniel Cohen - GC\Comments from FDMS\Charles W Adams DRAFT-0005.html  

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

%20Daniel%20Cohen%20-%20GC/Comments%20from%20FDMS/Charles%20W%20Adams%20DRAFT-0005.html[3/23/2011 2:17:13 PM] %20Daniel%20Cohen%20-%20GC/Comments%20from%20FDMS/Charles%20W%20Adams%20DRAFT-0005.html[3/23/2011 2:17:13 PM] PUBLIC SUBMISSION As of: March 23, 2011 Received: March 21, 2011 Status: Pending_Post Tracking No. 80c0d05f 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-0005 Comment on FR Doc # 2011-02368 Submitter Information Name: Charles W Adams Address: A.O. Smith Corporation 11270 W. PARK PLACE MILWAUKEE, WI, 53224 Email: cadams@aosmith.com Phone: 414-359-4274 Organization: A.O. Smith Corporation General Comment I am commenting on behalf of A.O. Smith Water Products Company, the largest manufacturer of residential and commercial water heaters in the USA. We are members of the Air-conditioning,

209

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

SciTech Connect

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

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

2007-11-02T23:59:59.000Z

210

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

SciTech Connect

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

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

2013-08-01T23:59:59.000Z

211

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

Science Conference Proceedings (OSTI)

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

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

2012-06-01T23:59:59.000Z

212

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

SciTech Connect

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

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

2012-07-15T23:59:59.000Z

213

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

E-Print Network (OSTI)

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

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

2012-01-01T23:59:59.000Z

214

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

E-Print Network (OSTI)

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

Zhiglo, Andrey V

2009-01-01T23:59:59.000Z

215

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

E-Print Network (OSTI)

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

unknown authors

2010-01-01T23:59:59.000Z

216

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

SciTech Connect

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

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

2012-02-10T23:59:59.000Z

217

Midland, Michigan: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Michigan: Energy Resources Michigan: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 43.6155825°, -84.2472116° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.6155825,"lon":-84.2472116,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

218

Midland, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

73456°, -102.0779146° 73456°, -102.0779146° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":31.9973456,"lon":-102.0779146,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

219

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

E-Print Network (OSTI)

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

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

2004-08-12T23:59:59.000Z

220

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

E-Print Network (OSTI)

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

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

2004-01-15T23:59:59.000Z

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221

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

SciTech Connect

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

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

2010-03-20T23:59:59.000Z

222

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

Science Conference Proceedings (OSTI)

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

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

2010-01-01T23:59:59.000Z

223

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

E-Print Network (OSTI)

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

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

2006-01-19T23:59:59.000Z

224

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

Science Conference Proceedings (OSTI)

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

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

2010-03-01T23:59:59.000Z

225

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Office of Legacy Management (LM)

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226

Prospects for Type Ia Supernova explosion mechanism identification with gamma rays  

E-Print Network (OSTI)

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

Jordi Gomez-Gomar; Jordi Isern; Pierre Jean

1997-09-05T23:59:59.000Z

227

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

SciTech Connect

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

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

2012-10-01T23:59:59.000Z

228

Phenomenology for Supernova Ia Data Based on a New Cosmic Time  

E-Print Network (OSTI)

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

Charles B. Leffert

2007-07-26T23:59:59.000Z

229

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

E-Print Network (OSTI)

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

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

2012-01-01T23:59:59.000Z

230

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

Science Conference Proceedings (OSTI)

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

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

2004-01-12T23:59:59.000Z

231

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

E-Print Network (OSTI)

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

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

2006-01-01T23:59:59.000Z

232

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

SciTech Connect

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

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

2003-11-24T23:59:59.000Z

233

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

Science Conference Proceedings (OSTI)

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

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

2011-06-10T23:59:59.000Z

234

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

SciTech Connect

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

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

2009-10-10T23:59:59.000Z

235

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

SciTech Connect

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

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

2012-04-20T23:59:59.000Z

236

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

E-Print Network (OSTI)

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

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

2006-11-01T23:59:59.000Z

237

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

E-Print Network (OSTI)

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

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

2006-06-28T23:59:59.000Z

238

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

E-Print Network (OSTI)

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

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

2010-01-01T23:59:59.000Z

239

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

Science Conference Proceedings (OSTI)

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

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

2010-01-01T23:59:59.000Z

240

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

Science Conference Proceedings (OSTI)

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

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

2012-11-01T23:59:59.000Z

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241

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

SciTech Connect

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

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

2005-01-28T23:59:59.000Z

242

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

E-Print Network (OSTI)

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

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

2006-09-15T23:59:59.000Z

243

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

E-Print Network (OSTI)

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

Shunsaku Horiuchi; John F. Beacom

2010-06-30T23:59:59.000Z

244

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

E-Print Network (OSTI)

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

Ferrero, Alejandro

2010-01-01T23:59:59.000Z

245

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

E-Print Network (OSTI)

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

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

2012-01-01T23:59:59.000Z

246

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

SciTech Connect

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosions of carbon-oxygen (C-O) white dwarfs (WDs). The single-degenerate scenario is a well-explored model of SNe Ia where unstable thermonuclear burning initiates in an accreting, Chandrasekhar-mass WD and forms an advancing flame. By several proposed physical processes, the rising, burning material triggers a detonation, which subsequently consumes and unbinds the WD. However, if a detonation is not triggered and the deflagration is too weak to unbind the star, a completely different scenario unfolds. We explore the failure of the gravitationally confined detonation mechanism of SNe Ia, and demonstrate through two-dimensional and three-dimensional simulations the properties of failed-detonation SNe. We show that failed-detonation SNe expel a few 0.1 M{sub Sun} of burned and partially burned material and that a fraction of the material falls back onto the WD, polluting the remnant WD with intermediate-mass and iron-group elements that likely segregate to the core forming a WD whose core is iron rich. The remaining material is asymmetrically ejected at velocities comparable to the escape velocity from the WD, and in response, the WD is kicked to velocities of a few hundred km s{sup -1}. These kicks may unbind the binary and eject a runaway/hypervelocity WD. Although the energy and ejected mass of the failed-detonation SN are a fraction of typical thermonuclear SNe, they are likely to appear as subluminous low-velocity SNe Ia. Such failed detonations might therefore explain or are related to the observed branch of peculiar SNe Ia, such as the family of low-velocity subluminous SNe (SN 2002cx/SN 2008ha-like SNe).

Jordan, George C. IV; Van Rossum, Daniel R. [Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637 (United States); Perets, Hagai B. [Physics Department, Technion, Israel Institute of Technology, Haifa 32000 (Israel); Fisher, Robert T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States)

2012-12-20T23:59:59.000Z

247

TYPE Ia SUPERNOVA PROPERTIES AS A FUNCTION OF THE DISTANCE TO THE HOST GALAXY IN THE SDSS-II SN SURVEY  

Science Conference Proceedings (OSTI)

We use Type Ia supernovae (SNe Ia) discovered by the Sloan Digital Sky Survey-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host-galaxy center, using the distance as a proxy for local galaxy properties (local star formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light curves using both MLCS2K2 and SALT2, and determine color (A{sub V} , c) and light-curve shape ({Delta}, x{sub 1}) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4{sigma} level) finding is that the average fitted A{sub V} from MLCS2K2 and c from SALT2 decrease with the projected distance for SNe Ia in spiral galaxies. We also find indications that supernovae (SNe) in elliptical galaxies tend to have narrower light curves if they explode at larger distances, although this may be due to selection effects in our sample. We do not find strong correlations between the residuals of the distance moduli with respect to the Hubble flow and the galactocentric distances, which indicates a limited correlation between SN magnitudes after standardization and local host metallicity.

Galbany, Lluis; Miquel, Ramon; Oestman, Linda [Institut de Fisica d'Altes Energies, Universitat Autonoma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Brown, Peter J.; Olmstead, Matthew D. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); D'Andrea, Chris B.; Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX (United Kingdom); Frieman, Joshua [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellise Avenue, Chicago, IL 60637 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, John [Center for Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Nordin, Jakob [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720 (United States); Sako, Masao [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7535, Cape Town (South Africa); Sollerman, Jesper [Oskar Klein Centre, Department of Astronomy, AlbaNova, SE-106 91 Stockholm (Sweden); Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard, E-mail: lluis.galbany@ist.utl.pt [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); and others

2012-08-20T23:59:59.000Z

248

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rat...

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

2008-01-01T23:59:59.000Z

249

NREL: Energy Sciences - Daniel A. Beaton  

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

was on hole transport in this material system, where it was found that the hole mobility was not so dramatically reduced as in the analogous case of the dilute nitride...

250

Daniel Bouchez Buddhism and Neo-Confucianism  

E-Print Network (OSTI)

, embora se destaquem os naturais da respectiva vila. Depois Sapardos, Sopo e Lovelhe, pela mesma ordem

Paris-Sud XI, Université de

251

Dr. Daniel G. Friend, Technical Program Director  

Science Conference Proceedings (OSTI)

... He has recently served in consultative capacities on energy research strategies ... on Understanding the Impact of Selling the Helium Reserve, 2008; ...

2012-10-01T23:59:59.000Z

252

Daniel Myers dsm@csail.mit.edu  

E-Print Network (OSTI)

. Shrira. HQ Replication: a Hybrid Quorum Protocol for Byzantine Fault Tolerance. In Proc. OSDI `06 2004. #12;other activities Commodore, MIT Nautical Association October 2007- Managed organization for students in lower-division courses Organized a weekend student-faculty retreat and a series of program

253

Daniel P. Abraham Argonne National Laboratory  

E-Print Network (OSTI)

innovati nNREL Enhances the Performance of a Lithium-Ion Battery Cathode Scientists from NREL to significantly enhance the performance of lithium iron phosphate (LiFePO4) cathodes for lithium-ion batteries. In the most common commercial design for lithium-ion (Li-ion) batteries, the positive electrode or cathode

Ginzel, Matthew

254

Daniel Murphy-Olson | Argonne National Laboratory  

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

over ten years' experience managing enterprise systems. Research Interests Fault-tolerant systems Big data and storage Scalable and elastic systems, cloud computing E-mail dolson...

255

Bibliographies By Author - Russel, Daniel, M.  

Science Conference Proceedings (OSTI)

... of Personal & Communal Large Information Scale Appliances. ... introduce LISA (large information scale appliance). ... to be used by small work groups ...

256

Daniel Abraham, Ph.D. resume  

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

graduate students and postdoctoral associates from the U.S., Sweden, Germany, Poland, Spain, Japan, India and China Past member of ASM International, NACE...

257

EDWIN DANIEL HIRLEMAN JR. Birthplace: Wichita, Kansas  

E-Print Network (OSTI)

of the dose factor Fd for every radioactive isotope is based on evaluation given by International Commission generators, turbines and generators produces electrical energy which is more than sufficient to operate

Chiao, Raymond

258

Sequence Signals for Protein Benjamin Daniel Hyer  

E-Print Network (OSTI)

­ Carinthia Tech Institute ­ Carter Holt Harvey Pulp and Paper ­ Celulose Nipo-Brasileira ­ Cesaroni ­ Clyde

259

Curriculum Vitae DANIEL J. INMAN, Chair  

E-Print Network (OSTI)

Berichte Nr. 689, 243 ­ 260, 2008. [46] von Wagner, U.: Nonlinear Dynamic Behaviour of a Railway Wheelset squeal with piezoelectric actuators. Proceedings of Braking 2009 York, 159 ­ 168, 2009 #12;[50] von.: Minimal Models for Squealing of Railway Block Brakes. Archive of Applied Mechanics 81, 503-511, 2011. [65

Eustice, Ryan

260

Making the Standard Candle: A study of how the progenitor white dwarf modulates the peak luminosity of type Ia supernovae  

SciTech Connect

The goals of the proposed research as stated in the proposal were to: Build a suite of one-dimensional initial models of different metallicities and central densities. Using the improved flame capturing scheme, simulate the explosion of a white dwarf with embedded Lagrangian tracer particles, and post-process the thermal histories of the tracers to reconstruct the nucleosynthesis of the explosion. Survey the effects of a changing progenitor metallicity on the isotopic yields. Of particular interest is 1) whether the linear relation between the mass of 56Ni synthesized and the pro- genitor metallicity is moderated by the effect of electron captures in the core; and 2) how a varying central density alters the relation between metallicity and 56Ni mass. Using these results, examine how the observed metallicity distribution would affect the brightness distribution of SNe Ia and the isotopic ratios about the Fe-peak.

Brown, Edward F [Michigan State University

2010-01-21T23:59:59.000Z

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261

Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae  

E-Print Network (OSTI)

We estimate the solar system motion relative to the cosmic microwave background using type Ia supernovae (SNe) measurements. We take into account the correlations in the error bars of the SNe measurements arising from correlated peculiar velocities. Without accounting for correlations in the peculiar velocities, the SNe data we use appear to detect the peculiar velocity of the solar system at about the 3.5 sigma level. However, when the correlations are correctly accounted for, the SNe data only detects the solar system peculiar velocity at about the 2.5 sigma level. We forecast that the solar system peculiar velocity will be detected at the 9 sigma level by GAIA and the 11 sigma level by the LSST. For these surveys we find the correlations are much less important as most of the signal comes from higher redshifts where the number density of SNe is insufficient for the correlations to be important.

Christopher Gordon; Kate Land; Anze Slosar

2007-11-27T23:59:59.000Z

262

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

E-Print Network (OSTI)

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

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

2006-01-23T23:59:59.000Z

263

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

E-Print Network (OSTI)

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

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

2005-01-01T23:59:59.000Z

264

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

Science Conference Proceedings (OSTI)

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

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

2012-11-20T23:59:59.000Z

265

Midland, North Carolina: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

North Carolina: Energy Resources North Carolina: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 35.2273656°, -80.5006219° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":35.2273656,"lon":-80.5006219,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

266

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

Open Energy Info (EERE)

892643°, -74.1406988° 892643°, -74.1406988° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.9892643,"lon":-74.1406988,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

267

Midland County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Texas: Energy Resources Texas: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 31.8781368°, -101.9804613° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":31.8781368,"lon":-101.9804613,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

268

New PDC system making hole in Midland - And fast  

SciTech Connect

A new PDC drilling system being field tested in West Texas is penetrating hard rock at unheard of rates, controlling bit balling and slowing bit body erosion, thanks to an ingenious bit stabilization system and an unusual bit nozzle design. The new system also uses lower drill string weight and less mud pump pressure, while running at lower rpms than is common in the area. In one recent shallow-well test in the McElroy Ranch field near Crane, Tex., the Sta-bit system (short for stabilized bit), drilled from 660 ft to 2403 ft (1743 ft total) through shale, siltstone, sands and anhydrite stringers at nearly 70 ft/hr-some two to four times above typical West Texas penetration rates. At the same time, the bit required a drill string weight of only 16,000 lb, and 800-psi mud pump pressure and ran at 70 rpm. The patented Sta-bit system consists of two parts - a spiral-patterned PDC bit and a separate, pressure-actuated stabilizer. But the stabilizer is both the heart of the system and the source of most of its problems. It's designed to eliminate vibrational and rotational whip, which it is believed destroys PDC cutters in hard formations.

Not Available

1988-07-01T23:59:59.000Z

269

Gorchakova-IA  

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

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

270

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

SciTech Connect

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

Hubbard, Camden R [ORNL

2011-09-01T23:59:59.000Z

271

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

E-Print Network (OSTI)

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

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

2005-01-20T23:59:59.000Z

272

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rate, $r_V \\propto (1+z)^{\\beta}$, we obtain a value of $\\beta = 1.5 \\pm 0.6$, i.e. the SN Ia rate is determined to be an increasing function of redshift at the $\\sim 2.5 \\sigma$ level. Fitting the results to a model in which the volumetric SN rate, $r_V=A\\rho(t)+B\\dot \\rho(t)$, where $\\rho(t)$ is the stellar mass density and $\\dot \\rho(t)$ is the star formation rate, we find $A = (2.8 \\pm 1.2) \\times 10^{-14} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1} \\mathrm{year}^{-1}$, $B = (9.3^{+3.4}_{-3.1})\\times 10^{-4} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1}$.

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

2008-01-22T23:59:59.000Z

273

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

SciTech Connect

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

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

2012-03-10T23:59:59.000Z

274

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

E-Print Network (OSTI)

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

Webb, David F.

275

PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs |  

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

PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs October 17, 2011 - 2:50pm Addthis A highly efficient catalyst to convert renewable crops into the product propylene glycol was discovered by scientists at the Pacific Northwest National Laboratory (PNNL) and commercialized by the Archer Daniels Midland Company. | Image courtesy of PNNL. A highly efficient catalyst to convert renewable crops into the product propylene glycol was discovered by scientists at the Pacific Northwest National Laboratory (PNNL) and commercialized by the Archer Daniels Midland Company. | Image courtesy of PNNL. Ginny Simmons Ginny Simmons Former Managing Editor for Energy.gov, Office of Public Affairs

276

EA-1828: Final Environmental Assessment | Department of Energy  

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

Final Environmental Assessment Final Environmental Assessment EA-1828: Final Environmental Assessment 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 DOE prepared this EA to evaluate the potential environmental consequences of providing a financial assistance grant under the American Recovery and Reinvestment Act of 2009 (ARRA) in a cooperative agreement with Archer Daniels Midland Company (ADM). If ADM received the funding, the company would demonstrate an integrated system of carbon dioxide (CO2) capture in an industrial setting and geologic sequestration in a sandstone reservoir. The CO2 that would be sequestered is currently a by-product of ADM's

277

EA-1828: Finding of No Significant Impact | Department of Energy  

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

Finding of No Significant Impact Finding of No Significant Impact EA-1828: Finding of No Significant Impact Carbon Dioxide Capture from Biofuels Production and Sequestration into the Mount Simon Sandstone Phase II Project in Decatur, Illinois Based on the analyses in the environmental assessment DOE determined that its proposed action-awarding a grant to Archer Daniels Midland Company (ADM) to demonstrate an integrated system of carbon dioxide capture in an industrial setting and geologic sequestration in a sandstone reservoir-would result in no significant adverse impacts. Finding of No Significant Impact for Archer Daniels Midland Company's "CO2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone, Decatur, Illinois, DOE/EA-1828 (May 2011) More Documents & Publications

278

PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs |  

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

Breakthrough Leads to Less Foreign Oil, More American Jobs Breakthrough Leads to Less Foreign Oil, More American Jobs PNNL Breakthrough Leads to Less Foreign Oil, More American Jobs October 17, 2011 - 2:50pm Addthis A highly efficient catalyst to convert renewable crops into the product propylene glycol was discovered by scientists at the Pacific Northwest National Laboratory (PNNL) and commercialized by the Archer Daniels Midland Company. | Image courtesy of PNNL. A highly efficient catalyst to convert renewable crops into the product propylene glycol was discovered by scientists at the Pacific Northwest National Laboratory (PNNL) and commercialized by the Archer Daniels Midland Company. | Image courtesy of PNNL. Ginny Simmons Ginny Simmons Former Managing Editor for Energy.gov, Office of Public Affairs "Not only can we reduce our use of petroleum, but we can make better use

279

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

SciTech Connect

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

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

1980-01-31T23:59:59.000Z

280

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

SciTech Connect

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

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

2013-08-20T23:59:59.000Z

Note: This page contains sample records for the topic "daniels midland ia" from the National Library of EnergyBeta (NLEBeta).
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281

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

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

produced new technologies such as radar, the computer, the proximity fuze, and the atomic bomb, which proved decisive for the Allied victory. But he knew that brilliance alone...

282

The Evolutionary Origins of Glia DANIEL K. HARTLINE*  

E-Print Network (OSTI)

and connec- tives, and thus resembling the nerve nets of cnidarians and ctenophores (Bedini and Lanfranchi, 1991; Rama- chandra et al., 2002). An electron microscopic study by Bedini and Lanfranchi (1991

Hartline, Daniel K.

283

Models for managing the impact of an epidemic Daniel Bienstock ...  

E-Print Network (OSTI)

However, even a much milder epidemic would have vast social impact as services such as health care, police and utilities became severely hampered by staff.

284

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

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

Polish companies. For example, a number of major U.S. oil and gas companies, including Exxon Mobil, Chevron, and ConocoPhillips have been granted licenses to explore for shale gas...

285

Daniels County, Montana: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

County, Montana: Energy Resources County, Montana: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 48.7744137°, -105.7248763° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":48.7744137,"lon":-105.7248763,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

286

Daniel van der Lelie, Safiyh Taghavi - Brookhaven National Laboratory  

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

and specifically address the microbial communities involved in the decay of poplar biomass, and the rhizosphere of poplar. BNL Press Release of December 19, 2007...

287

GSLIS, UIUC; 501 East Daniel Street; Champaign; IL; 61820 ...  

Science Conference Proceedings (OSTI)

... N - 1 eigenvalues (for a real symmetric matrix ... complexity of the principal components analysis, coupled ... are suitable for visualization and navigation ...

1997-09-23T23:59:59.000Z

288

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

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

energy and climate legislation this year that will create incentives to invest in clean energy by setting a price on carbon. The President also continues to work...

289

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

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

risks. And though the Fukushima accident has heightened awareness about the risks of nuclear energy, we must recognize that the larger energy challenges we faced before the...

290

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

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

Blake Harris, General Counsel; David Sandalow, Assistant Secretary for Policy and International Affairs; and Ines Triay, Assistant Secretary for Environmental Management....

291

Seckin Gokaltun, Dwayne McDaniel and David Roelant Florida ...  

R pulse from the plate center. ----Sketch of bubble-growth during Pulsed-air mixing Sketch showing mixing pattern induced by the rising bubble.

292

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

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

- about 45 percent - from coal-fired power plants. We, like Poland, have tremendous shale gas reserves that we are in the process of developing. We, like Poland, are looking...

293

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

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

the framework for nuclear safety worldwide. Over the past year since we met in Jordan, IFNEC has played an important role in the international arena, bringing together...

294

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

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

and Limits to Recycling of Critical Materials for Clean Energies Peter Dent, Electron Energy Corporation, Strategies for More Effective Critical Materials Use Steve...

295

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

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

two nations partnered with the International Atomic Energy Agency to blend down 33 kilograms of highly enriched uranium from the Kazakh Institute of Nuclear Physics in Almaty....

296

2007 Botany and Plant Pathology Publications Arp, Daniel  

E-Print Network (OSTI)

-subunit of butane monooxygenase. J. Bacteriol. 189: 5068-5074 (2007). Gvakharia, B.O., E.A. Permina, M.A. Sayavedra-Soto, D.J. Arp. Butane monooxygenase of Pseudomonas butanovora: purification and biochemical of butane monooxygenase activity in Pseudomonas butanovora; Biochemical and physiological implications

Grünwald, Niklaus J.

297

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

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

before March 11th - when the earthquake and then the tsunami struck and crippled the Fukushima Daiichi nuclear power plant - the tradition of cooperation between our two countries...

298

Getting the carbon out Alex Farrell, Daniel Sperling  

E-Print Network (OSTI)

Schwarzenegger's new policy to reduce global warming emissions from our cars and trucks. This new policy, the low, or buying credits from providers of other low-carbon fuels (such as low-carbon electricity or natural gas and for their customers. At first, fuel providers will most likely offer liquid fuels that work in today's cars

299

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

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

Steve Nadel of the American Council for an Energy-Efficient Economy; Karen Meyers of Rheem Manufacturing Company; Karim Amrane, Joseph Mattingly and David Calabrese of the...

300

Victor J. Daniel Jr. CO2 Injection Test Site Plan  

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

Mississippi Test Site JAF02664.PPT 1 1.1 SITE BACKGROUND 1.2 GENERAL IDENTIFICATION DATA 1.3 REGULATORY CLASSIFICATION 1.4 WELL DATA - INJECTION WELL NO. 1 1.5 WELL DATA -...

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


301

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

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

Caffarey, UMICORE, "Opportunities and Limits to Recycling of Critical Materials for Clean Energies EIS-0250-S2: Draft Supplemental Environmental Impact Statement...

302

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

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

Affairs Blythe Masters Tesla Motors CEO Elon Musk Entrepreneur T. Boone Pickens DARPA Director Arati Prabhakar Michael Jones, Chief Technology Advocate, Google Ventures...

303

Second completely revised edition Daniel Desbruyres, Michel Segonzac & Monika Bright  

E-Print Network (OSTI)

the increased computational load. Since all of these transactions are stored in the VAMPIRE database, no dataVAMPIRE microarray suite: a web-based platform for the interpretation of gene expression data of analysis, collectively known as variance-modeled posterior inference with regional exponentials (VAMPIRE

Oppo, Delia W.

304

IA_50m_Wind  

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

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

305

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

SciTech Connect

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

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

2012-05-01T23:59:59.000Z

306

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

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

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

307

How to Get the Snowball Rolling and Extend the Franchise: Voting on the Great Reform Act of 1832  

E-Print Network (OSTI)

in the Midlands and the North, such as Birmingham, Leeds and Manchester, did not elect any MP. The politics of the Unreformed Parliament was very different from that of modern parliamentary democracies. Firstly, the franchise rules, which governed who could... to Manchester, Birmingham and Leeds was defeated by 188 to 140 votes and in May, Daniel OConnells radical bill demanding manhood suffrage only received 13 votes in support. At the opening of the Parliament on 2 November 1830, Wellington declared that he...

Aidt, Toke S; Franck, R

308

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

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

radiation counters, nuclear science lab trainers, and Geiger counters for instructor-led demonstrations and basic laboratory exercises. SECTION C. Environmental Aspects ...

309

Integrated Analysis and Application of Reservoir Models to Early Permian Detrital Carbonate Deposits, Midland Basin, Texas  

E-Print Network (OSTI)

A 3-D seismic volume, wireline logs and core data were integrated to determine the spatial distribution of porous reservoirs within the Wolfcampian-Leonardian detrital carbonate slope and basin strata in Glasscock County, Texas. A 3-D seismic amplitude volume was used to construct a seismic facies analysis of the detrital carbonate section, and generated attribute volumes helped identify detrital carbonate depositional trends, as well as establish a potential correlation between thick detrital carbonate intervals and associated amplitude response. Eight lithofacies were identified in core and were subsequently classified into three main facies: debris flow, grain flow/turbidite, and basinal shale. A facies type log was then created, which was used to supervise the creation of facies logs within other wells to ultimately use in the creation of a 3-D facies model. Cross sections through the study area show an increase in bathymetric relief beginning in Wolfcampian time and continuing through the Leonardian. Detrital carbonate deposition increases dramatically during the Leonardian, consisting of large gravity flows deposited basinward in a northwest-southeast linear trend, rapidly thinning basinward. Individual flows are discontinuous and bounded by basinal shale facies. Four seismic facies were identified within the interval of interest using a structurally smoothed attribute volume, while an RMS amplitude attribute volume provided a correlation between high RMS amplitude values and detrital carbonate thickness. A high RMS amplitude value corresponding to the debris flow facies was extracted from the RMS attribute volume in the form of a seismic geobody. Two facies models and one porosity model were generated by using upscaled values from the gamma ray, total porosity, and lithofacies logs, which were applied over areas with the densest well control. Although the facies model populated from upscaled GR values was useful in stratigraphic interpretation, it is determined that the models should be applied over areas with denser well spacing in order to provide a more accurate and geologically viable subsurface model.

Johnston, Travis 1987-

2012-12-01T23:59:59.000Z

310

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

SciTech Connect

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.

Montgomery, S.L. [Petroleum Consultant, Seattle, WA (United States)

1996-09-01T23:59:59.000Z

311

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

SciTech Connect

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.

Mazzullo, S.J. [Wichita State Univ., KS (United States)

1997-10-01T23:59:59.000Z

312

Page not found | Department of Energy  

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

71 - 180 of 31,917 results. 71 - 180 of 31,917 results. Download WA_1993_024_ABB_AIR_PREHEATER_INC_Waiver_of_Domestic_and_For.pdf http://energy.gov/gc/downloads/wa1993024abbairpreheaterincwaiverofdomesticandforpdf Download WA_04_024_ARCHER-DANIELS-MIDLAND_CO_Waiver_of_Domestic_and_F.pdf http://energy.gov/gc/downloads/wa04024archer-daniels-midlandcowaiverofdomesticandfpdf Download WA_04_066_GENERAL_ELECTRIC_CO_Waiver_of_Domestic_and_Foreign.pdf http://energy.gov/gc/downloads/wa04066generalelectriccowaiverofdomesticandforeignpdf Download WA_98_014_ALUMINUM_COMPANY_OF_AMERICA_(ALCOA)_Waiver_of_Dome.pdf http://energy.gov/gc/downloads/wa98014aluminumcompanyofamericaalcoawaiverofdomepdf Download WA_03_012_SIEMENS_WESTINGHOUSE_Waiver_of_Domestic_and_Foreig.pdf http://energy.gov/gc/downloads/wa03012siemenswestinghousewaiverofdomesticandforeigpdf

313

Michigan - State Energy Profile Data - U.S. Energy ...  

U.S. Energy Information Administration (EIA)

Monroe (Detroit Edison Co) ; Ludington (Consumers Energy Co) ; Dan E Karn (Consumers Energy Co) ; Midland Cogeneration Venture (Midland Cogeneration ...

314

Michigan Profile - Energy Information Administration  

U.S. Energy Information Administration (EIA)

Monroe (Detroit Edison Co) ; Ludington (Consumers Energy Co) ; Dan E Karn (Consumers Energy Co) ; Midland Cogeneration Venture (Midland Cogeneration ...

315

Notices  

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

15 Federal Register 15 Federal Register / Vol. 78, No. 48 / Tuesday, March 12, 2013 / Notices Complainant's wind turbine located at 3065 220th Street, Williams, IA 50271- 7518 before drawing power from Midland, (2) require Midland to install a mechanical meter without any blockers or detents to allow parallel operation, and (3) use this mechanical meter for registering and keeping track of the KWH consumed or generated for the billing month. Any person desiring to intervene or to protest this filing must file in accordance with Rules 211 and 214 of the Commission's Rules of Practice and Procedure (18 CFR 385.211, 385.214). Protests will be considered by the Commission in determining the appropriate action to be taken, but will not serve to make protestants parties to

316

Rates and progenitors of type Ia supernovae  

E-Print Network (OSTI)

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

Wood-Vasey, William Michael

2004-01-01T23:59:59.000Z

317

Visualizing Type Ia Supernova Explosions at NERSC  

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

Childs1a-Supernovasm.png Deep inside a dying star in a galaxy far, far away, a carbon fusion flame ignites. Ignition may happen in the middle or displaced slightly to one side,...

318

Distributed Flames in Type Ia Supernovae  

E-Print Network (OSTI)

In the distributed burning regime, turbulence disrupts the internal structure of the flame, and so the idea of laminar burning propagated by conduction is no longer valid. The nature of the burning depends on the turbulent Damkohler number (Da), which steadily declines from much greater than one to less that one as the density decreases to a few 10^6 g/cc. Scaling arguments predict that the turbulent flame speed s, normalized by the turbulent intensity u, follows s/u=Da^1/2 for Da1, and that localized excursions to as much as five times u can occur. The lambda-flame speed and width can be predicted based on the turbulence in the star and the turbulent nuclear burning time scale of the fuel. We propose a practical method for measuring these based on the scaling relations and small-scale computationally-inexpensive simulations. This suggests that a simple turbulent flame model can be easily constructed suitable for large-scale distributed supernovae flames.

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

2011-01-01T23:59:59.000Z

319

Functional Role of NMDA Autoreceptors in Olfactory Mitral Cells DANIEL FRIEDMAN AND BEN W. STROWBRIDGE  

E-Print Network (OSTI)

V (Depol), and the reduction in both responses in APV (50 M at 70 mV). Responses from the same mitral cell

Strowbridge, Ben

320

Stationary state volume fluctuations granular medium Matthias Schrter,* Daniel Goldman, Harry Swinney  

E-Print Network (OSTI)

#; Donev, Torquato, F. H. Stillinger, ibid. 011105 #2005#. #15# Srebro Levine, 061301 #2003#. SCHR?TER

Texas at Austin. University of

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321

Selfish Multi-User Task Scheduling Thomas E. Carroll and Daniel Grosu  

E-Print Network (OSTI)

R -- = +-+++ = 3 2.0 0 0.4 33 )/](][2[][ CppMOFkR 5.3 0 _ 3 _ 3 )/](2][1[ - = ppIIkR 444 ]1[ CIkR =

Grosu, Daniel

322

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

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

Energy and Commerce Committee Energy and Commerce Committee U.S. House of Representatives March 13, 2013 Chairman Murphy, Ranking Member DeGette, and members of the Subcommittee, thank you for the invitation to appear before you today to provide the subcommittee details on the actions the Department has taken or will take to strengthen management, oversight, and security of the nuclear weapons complex in the wake of the July 2012 Y-12 incident. We appreciate the interest and engagement of this Committee and recognize the important oversight role that you fulfill. We also share the Committee's commitment to assure that all of our offices and operations are delivering on our mission safely and securely- from Washington, DC, to California, from every naval reactor to every warhead, from production to

323

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

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

Strategic Forces Strategic Forces Armed Services Committee U.S. House of Representatives September 13, 2012 Chairman Turner, Ranking Member Sanchez, and members of the Subcommittee, thank you for the invitation to appear before you today to discuss the Department of Energy's oversight of the nuclear weapons complex and the recent security incident at the Y-12 National Security Complex (Y-12). We appreciate the interest and engagement of this Committee and recognize the important oversight role that you fulfill. We also share the Committee's commitment to assure that all of our offices and operations are delivering on our mission safely, securely, and in a fiscally responsible manner - from Washington, DC, to California, from every naval reactor

324

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

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

Committee on Energy and Commerce 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 invitation to appear before you today to discuss the Department of Energy's oversight of the nuclear weapons complex and the recent security incident at the Y-12 National Security Complex (Y-12). We appreciate the interest and engagement of this Committee and recognize the important oversight role that you fulfill. We also share the Committee's commitment to assure that all of our offices and operations are delivering on our mission safely, securely, and in a fiscally responsible manner - from Washington, DC, to California, from every naval reactor to every warhead, from production to clean-up, from deterrence to nonproliferation.

325

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

Energy.gov (U.S. Department of Energy (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,...

326

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

Energy.gov (U.S. Department of Energy (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,...

327

Mr. J. Daniel Mahoney '66, President Mr. Bob Hardin '68, President-Elect  

E-Print Network (OSTI)

photo courtesy of Glen Rose / Joe's Garage p. 4 Kenny Chesney photo courtesy of Melanie Dunea / Joe Worthys. Photo Courtesy: Melanie Dunea/Joe's Garage #12;Governor Phil Bredesen confirmed his support

Karsai, Istvan

328

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

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

329

A Database and Evaluation Methodology for Optical Flow Simon Baker Daniel Scharstein J.P. Lewis  

E-Print Network (OSTI)

algorithms by Barron et al. led to significant advances in the performance of optical flow methods benefited greatly from this study, which led to rapid and measurable progress. When the Barron et al. [2. The dense ground-truth flow for this nonrigid scene was ob- tained using hidden fluorescent texture. See

Black, Michael J.

330

Daniel Huson, Oliver Kohlbacher, Andrei Lupas, Kay Nieselt and Andreas Zell (eds.)  

E-Print Network (OSTI)

(Hrsg.), Identitäten, Frankfurt a. M. 1998, S. 73-504, hier S. 87. 7 Ebenda, S. 503. 8 Ebenda, S.97. 9, hrsg. von Michael Schröter, Frankfurt a. M. 1989, S. 67 ff. #12;Männlichkeit als Studienziel I: ders./James Walvin (Hrsg.), Manliness and Morality. Middle-class Masculinity in Britain and America

Spang, Rainer

331

SNOUT: One-Handed use of Capacitive Touch Devices Adam Zarek, Daniel Wigdor, Karan Singh  

E-Print Network (OSTI)

- rameters and speech-to-text for text entry. An evaluation of SNOUT shows it to effectively render handheld and accuracy issues that make it similar to but distinctly different from fat-finger problem [28]. Second

Toronto, University of

332

A quantum mechanical look at time travel and free will Daniel Greenberger  

E-Print Network (OSTI)

, City College of the City University of New York, New York, NY 10031, USA Karl Svozil Institute://tph.tuwien.ac.at/~svozil 1 #12;I. CLASSICAL PART 1. Principle of self-consistency An irreducible, atomic physical phenomenon

Svozil, Karl

333

Mr. J. Daniel Mahoney '66, President Mr. Bob Hardin '68, President-Elect  

E-Print Network (OSTI)

1970-1977: John Weaver, president3 1964-1967: Robben Fleming, chancellor2 1967-1968: William Sewell;1891 Edward A. Birge is named first dean of the College of Letters and Science. William Arnon Henry is named

Karsai, Istvan

334

Book review: Artificial Intelligence in Perspective by Daniel G. Bobrow (Ed.) (The MIT Press 1993)  

Science Conference Proceedings (OSTI)

The past and present of Artificial Intelligence have been nicely presented in the book, "Artificial Intelligence in Perspective". This book is dedicated to Allen Newell, one of the founders of artificial intelligence (AI). The book looks at the achievements ...

Rajkumar Roy; Raju S. Bapi

1996-01-01T23:59:59.000Z

335

Secure Systems Editors: Patrick McDaniel, mcdaniel@cse.psu.edu  

E-Print Network (OSTI)

the smartgrid technology. His research interests include network and systems security, telecommunications

McDaniel, Patrick Drew

336

Structured Security Testing in the Smartgrid Patrick McDaniel and Stephan McLaughlin  

E-Print Network (OSTI)

.B. in SmartGrids als Sicherheits- schicht, die die Einhaltung der Randbedingungen ga- rantiert, oder als Hilfe

McDaniel, Patrick Drew

337

Controlling Widgets with One Power-up Button Daniel Spelmezan1,2  

E-Print Network (OSTI)

-up Button can recog- nize six different mid-air gestures performed on the side of a mobile device. Author Keywords Mobile device; Proximity input; Pressure input ACM Classification Keywords H.5 with One Power-up Button. In UIST '13: Proceedings of the 26th ACM Symposium on User Interface Software

Recanati, Catherine

338

Firebot: Design of an Autonomous Fire Fighting Robot Lynette Miller Daniel Rodriguez Kristen Allen Maksim Makeev  

E-Print Network (OSTI)

that is designed to find a small fire represented by a light emitting diode in a model home and extinguish it by a cylindrical red object with six red light emitting diodes (LED). The candle can be found in any of the four

Schwartz, Eric M.

339

A Low-Cost Quantitative Absorption Spectrophotometer Daniel R. Albert, Michael A. Todt, H. Floyd Davis*  

E-Print Network (OSTI)

is constructed using Lego® blocks, a light emitting diode, and optical elements including a lens, slide

Davis, H. Floyd

340

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

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

that knowledge for granted, many in the rest of the world are just like Clifton. The light bulb comes on when they see the real thing. This "seeing the real thing" is one of the...

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


341

Sustainable Cities Joel E. Cohen, Daniel L. Doctoroff, and Martin Filler  

E-Print Network (OSTI)

be achieved by taking 174 cars off the street. Addition- ally, we collect rainwater on the roof, which besides enter and exit rooms. So all over the building, we are controlling the output of electricity, which

Cohen, Joel E.

342

NASA Air Quality Applied Sciences Team (AQAST) Daniel J. Jacob, Harvard University  

E-Print Network (OSTI)

Crystal River ECDs implemented June 2009 Crystal River facility, Florida x1015 molec/cm2 OMI NO2 shows

Jacob, Daniel J.

343

Space Series: simultaneous display of spatial and temporal data Daniel C. Glaser Marti A. Hearst  

E-Print Network (OSTI)

time such as daylighting or airflow in buildings. Advanced simulation programs represent this data Department of Architecture School of Information Management and Systems University of California at Berkeley daylighting. Keywords: focus + context, information visualization, daylighting, architectural simulation

Hearst, Marti

344

USING VIDEO FOR ANALYZING DAYLIGHT SIMULATION TOOLS Daniel C. Glaser1  

E-Print Network (OSTI)

of the daylighting system in The New York Times Headquarters.3 DALI continues to mature as a technology. Thus, there is a need for an advanced daylight sensor that can reap the benefits and flexibility for a given amount of time, the system goes to standby mode where daylight dimming is not operational. Normal

Salama, Khaled

345

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

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

Management Principles, which provide that: * We will treat our people as our greatest asset; * We will pursue our mission in a manner that is safe, secure, legally and ethically...

346

Semi-Autonomous Car Control Using Brain Computer Daniel Gohring, David Latotzky, Miao Wang, Raul Rojas  

E-Print Network (OSTI)

to the introduction of various driver assistance systems for street cars. One key aspect for driver assistance systems. Recently, BCI-systems have become relatively affordable and allow people to interact directly-violations and accidents by reclaiming control before they happen. The second application implements a semi-autonomous path

Göhring, Daniel

347

Requirements for Maintaining Web Access for Hearing-Impaired Individuals1 Daniel M. Berry  

E-Print Network (OSTI)

gotten even more difficult to use. The equipment available today is of mark- edly lower quality than/~dberry/FTP_SITE/reprints.journals.conferences/WSE_paper.txt 2 It's hard to believe that there are any left these days! from Western Electric, and there is more the non-HI population. 4 To avoid heavy usage of "he or she" as a third person singular personal pronoun

Berry, Daniel M.

348

An Unsupervised Approach to Recognizing Discourse Relations Daniel Marcu and Abdessamad Echihabi  

E-Print Network (OSTI)

still be able to legally buy arms. (1) a. South Africa can afford to forgo sales of guns and grenades b, the sentence/clause pairs below. a. Such standards would preclude arms sales to states like Libya, which. because it actually makes most of its profits from the sale of expensive, high-technology systems like

349

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

E-Print Network (OSTI)

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

350

The composition and diagenesis of the Queen Formation (Guadalupian, Permian) at Virey and Moose Queen fields, Midland County, Texas  

E-Print Network (OSTI)

The Permian Basin of West Texas and Eastern New Mexico has been a center of oil and gas exploration since the early 1940s. Hydrocarbon profusion is focused in the shelfal areas of the Permian Basil with one of the most prolific clastic reservoirs being the Queen Formation. The Queen Formation is part of the Artesia Group, a sequence of interbedded shelf carbonates. evaporates, and classics. The first purpose of this thesis is to characterize the facies and petrography of the Queen Formation and its sandstone reservoirs at the Moose and Virey Queen fields. The second purpose is to investigate the depositional and diagenetic processes that control the formation, size and quality of the sandstone reservoirs and non-reservoirs. The Queen Formation at the Moose and Virey Queen Gelds generally consist of feldspathic litharenites to litharenites in a complex sequence of interbreed very fine-grained sandstones, coarse grained milestones, anhydritic very fine-grained sandstones, halitic very fine-grained sandstones. Based upon grain size measurements and petrographic analyses, these sandstones can be classified as well sorted sandflat, saline sandflat, and intertidal sandstones from a fluvial depositional system represented by a sequence of coarsening and finning upward cycles.The primary porosity of all of the sandstones of the Queen Formation was reduced by the precipitation of authigenic clay, the infiltration of mud and the formation of soil structures, and the precipitation of authigenic cements such as halite and anhydrite. Reservoirs were formed in the sandflat facies by the dissolution of cements and labile grains, creating enhanced secondary porosity. This project is just one part of a regional study of the Queen Formation in the Permian Basil which can be added to the extensive database on the Queen sandstones in order to obtain a more accurate delineation of the processes responsible for the deposition of the Queen Formation.

Voncannon, Jennifer Catherine

1999-01-01T23:59:59.000Z

351

Energy Department Applauds Nation's First Large-Scale Industrial Carbon  

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

Nation's First Large-Scale Industrial Nation's First Large-Scale Industrial Carbon Capture and Storage Facility Energy Department Applauds Nation's First Large-Scale Industrial Carbon Capture and Storage Facility August 24, 2011 - 6:23pm Addthis Washington, D.C. - The U.S. Department of Energy issued the following statement in support of today's groundbreaking for construction of the nation's first large-scale industrial carbon capture and storage (ICCS) facility in Decatur, Illinois. Supported by the 2009 economic stimulus legislation - the American Recovery and Reinvestment Act - the ambitious project will capture and store one million tons of carbon dioxide (CO2) per year produced as the result of processing corn into fuel-grade ethanol from the nearby Archer Daniels Midland biofuels plant. Since all of

352

STATEMENT OF CONSIDERATIONS. REQUEST BY ROHM AND HAAS COMPANY FOR AN ADVANCE WAIVER OF  

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

CONSIDERATIONS. CONSIDERATIONS. REQUEST BY ROHM AND HAAS COMPANY FOR AN ADVANCE WAIVER OF PATENT RIGHTS UNDER DOE COOPERATIVE AGREEMENT NO. DE-FC36- 04G0014158 ENTITLED "NEW SUSTAINABLE CHEMISTRIES FOR LOW VOC COATINGS"; W(A)-04-031; CH-1199 The Petitioner, Rohm and Haas Company (Rohm and Haas), has requested an advance waiver of domestic and foreign patent rights for all subject inventions made under the above- identified contract by its employees and its subcontractors' employees, regardless of tier, except inventions made by subcontractors eligible to retain title to inventions, pursuant to P.L. 96-517, as amended, or National Laboratories. Rohm and Haas is leading ; teaming arrangement including Archer-Daniels-Midland Company (ADM) as its primEary subcontractor to

353

Page not found | Department of Energy  

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

41 - 12350 of 26,764 results. 41 - 12350 of 26,764 results. Download EA-1828: Final Environmental Assessment 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 http://energy.gov/nepa/downloads/ea-1828-final-environmental-assessment Download Audit Report: OAS-L-05-07 The Department of Energy's Annual Report to Congress on Management and Operating Contractor Employees in the Washington, D.C. Area http://energy.gov/ig/downloads/audit-report-oas-l-05-07 Download Records Management Handbook http://energy.gov/cio/downloads/records-management-handbook-0 Download Technical Standards Newsletter- March 2006 The Standards Forum and Standards Actions - March 2006

354

Energy Department Applauds Nation's First Large-Scale Industrial Carbon  

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

Energy Department Applauds Nation's First Large-Scale Industrial Energy Department Applauds Nation's First Large-Scale Industrial Carbon Capture and Storage Facility Energy Department Applauds Nation's First Large-Scale Industrial Carbon Capture and Storage Facility August 24, 2011 - 6:23pm Addthis Washington, D.C. - The U.S. Department of Energy issued the following statement in support of today's groundbreaking for construction of the nation's first large-scale industrial carbon capture and storage (ICCS) facility in Decatur, Illinois. Supported by the 2009 economic stimulus legislation - the American Recovery and Reinvestment Act - the ambitious project will capture and store one million tons of carbon dioxide (CO2) per year produced as the result of processing corn into fuel-grade ethanol from the nearby Archer Daniels Midland biofuels plant. Since all of

355

Energy Department Announces Major Milestones for Decatur, Ill. Clean Coal  

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

Announces Major Milestones for Decatur, Ill. Announces Major Milestones for Decatur, Ill. Clean Coal Project Energy Department Announces Major Milestones for Decatur, Ill. Clean Coal Project September 19, 2012 - 1:00pm Addthis Washington, DC - Today, the U.S. Energy Department marked two important milestones in the Illinois Industrial Carbon Capture and Storage (ICCS) project in Decatur, Illinois, a major clean coal project and the Department's first 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 storage facility, as well as the public opening of the National Sequestration Education Center. The Center was funded in partnership with the Richland Community College and will contain classrooms, training, and laboratory facilities, offering

356

Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction |  

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

Large-Scale Industrial Carbon Capture, Storage Plant Begins Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction August 24, 2011 - 1:00pm Addthis Washington, DC - Construction activities have begun at an Illinois ethanol plant that will demonstrate carbon capture and storage. The project, sponsored by the U.S. Department of Energy's Office of Fossil Energy, is the first large-scale integrated carbon capture and storage (CCS) demonstration project funded by the American Recovery and Reinvestment Act (ARRA) to move into the construction phase. Led by the Archer Daniels Midland Company (ADM), a member of DOE's Midwest Geological Sequestration Consortium, the Illinois-ICCS project is designed to sequester approximately 2,500 metric tons of carbon dioxide

357

All General Counsel Reports | Department of Energy  

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

96_027_MOTOROLA_MANUFACTURING_SYSTEMS_Waiver_of_Domestic_.pdf 96_027_MOTOROLA_MANUFACTURING_SYSTEMS_Waiver_of_Domestic_.pdf July 27, 2011 WA_03_048_AMERICAN_SUPERCONDUCTOR_CORP_Waiver_of_Patent_Righ.pdf July 27, 2011 WA_05_055_SIEMENS_WESTINGHOUSE_POWER_CORPORATION_FORAN_Waive.pdf July 27, 2011 WA_00_029_ARCHER_DANIELS_MIDLAND_CO_Waiver_of_Domestic_and_F.pdf July 27, 2011 WC_1995_008_CLASS_WAIVER_of_Governments_Patent_Rights_In_In.pdf July 27, 2011 Comments from Nevada to Notice of Inquiry Concerning Preparation of a Report to Congress on the Price-Anderson Act Comments from the State of Nevada on the December 31, 1997 Federal Register "Notice of Inquiry Concerning Preparation of a Report to Congress on the Price-Anderson Act." July 27, 2011 WA1995_008_ALLIED_SIGNAL_INC_Waiver_of_Domestic_and_Foreign_.pdf July 27, 2011

358

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

Office of Legacy Management (LM)

Staten Island Warehouse - NY 22 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 Engineers. USACE Website Long-term Care Requirements: To be determined upon completion. Also see Documents Related to Staten Island Warehouse, NY NY.22-1 - MED Trip Report Summary; Authors: Ruhoff (Corps of Engineers) and Geddes (Stone & Webster); Subject: Trip to New York;

359

First U.S. Large-Scale CO2 Storage Project Advances | Department of Energy  

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

First U.S. Large-Scale CO2 Storage Project Advances First U.S. Large-Scale CO2 Storage Project Advances First U.S. Large-Scale CO2 Storage Project Advances April 6, 2009 - 1:00pm Addthis Washington, DC - Drilling nears completion for the first large-scale carbon dioxide (CO2) injection well in the United States for CO2 sequestration. This project will be used to demonstrate that CO2 emitted from industrial sources - such as coal-fired power plants - can be stored in deep geologic formations to mitigate large quantities of greenhouse gas emissions. The Archer Daniels Midland Company (ADM) hosted an event April 6 for a CO2 injection test at their Decatur, Ill. ethanol facility. The injection well is being drilled into the Mount Simon Sandstone to a depth more than a mile beneath the surface. This is the first drilling into the sandstone geology

360

NETL: News Release - First U.S. Large-Scale CO2 Storage Project Advances  

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

April 6, 2009 April 6, 2009 First U.S. Large-Scale CO2 Storage Project Advances One Million Metric Tons of Carbon to be Injected at Illinois Site Washington, DC -Drilling nears completion for the first large-scale carbon dioxide (CO2) injection well in the United States for CO2 sequestration. This project will be used to demonstrate that CO2 emitted from industrial sources - such as coal-fired power plants - can be stored in deep geologic formations to mitigate large quantities of greenhouse gas emissions. MORE INFO Link to the Midwest Geological Sequestration Consortium web site The Archer Daniels Midland Company (ADM) hosted an event April 6 for a CO2 injection test at their Decatur, Ill. ethanol facility. The injection well is being drilled into the Mount Simon Sandstone to a depth more than a mile

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


361

Property:StockSymbol | Open Energy Information  

Open Energy Info (EERE)

StockSymbol StockSymbol Jump to: navigation, search This is a property of type String. Pages using the property "StockSymbol" Showing 25 pages using this property. (previous 25) (next 25) A A.O. Smith + AOS + AAON + AAON + Alterra Power + MGMXF + Ameresco, Inc. + AMRC + Applied Materials + AMAT + Archer Daniels Midland + ADM + Autodesk + ADSK + C China Integrated Energy + CBEH + E EEMAP, Inc. + N/A + EnerNOC + ENOC + Evergreen Solar, Inc. + ESLR + ExxonMobil + XOM + G General Electric + GE + Geothermal Resources Council + Geothermal Resources Council + Goodwill Instrument + TPE 2423 + GreenShift Corporation + GERS.OB + Gulfsands Petroleum + AIM:GPX + H Helix Wind Corp. + HLXW + I ICF International + NASDAQ:ICFI + J Johnson Controls + JCI + M Molycorp Inc. + MCP +

362

Carbon Storage Partner Completes First Year of CO2 Injection Operations in  

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

Storage Partner Completes First Year of CO2 Injection Storage Partner Completes First Year of CO2 Injection Operations in Illinois Carbon Storage Partner Completes First Year of CO2 Injection Operations in Illinois November 19, 2012 - 12:00pm Addthis Washington, DC - A project important to demonstrating the commercial viability of carbon capture, utilization and storage (CCUS) technology has completed the first year of injecting carbon dioxide (CO2) from an industrial plant at a large-scale test site in Illinois. Led by the Illinois State Geological Survey, the Illinois Basin-Decatur Project is the first demonstration-scale project in the United States to use CO2 from an industrial source and inject it into a saline reservoir. The CO2 is being captured from an ethanol production facility operated by the Archer Daniels Midland Company in Decatur, Ill., and is being injected

363

EA-1626: Final Environmental Assessment | Department of Energy  

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

626: Final Environmental Assessment 626: Final Environmental Assessment EA-1626: Final Environmental Assessment Midwest Geological Sequestration Consortium (MGSC) Phase III Large-Scale Field Test 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 demonstrate the ability of the Mt. Simon Sandstone, a major regional saline reservoir in the Illinois Basin, to accept and retain approximately 1.1 million short tons (1 million metric tons) of CO2 injected over a period of three years. DOE/EA-1626: Final Environmental Assessment for Midwest Geological Sequestration Consortium (MGSC) Phase III Large-Scale Field Test (October 2008) More Documents & Publications EA-1828: Final Environmental Assessment

364

FE Press Releases and Techlines | Department of Energy  

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

September 19, 2012 September 19, 2012 Energy Department Announces Major Milestones for Decatur, Ill. Clean Coal Project Washington, DC - Today, the U.S. Energy Department marked two important milestones in the Illinois Industrial Carbon Capture and Storage (ICCS) project in Decatur, Illinois, a major clean coal project and the Department's first 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 storage facility, as well as the public opening of the National Sequestration Education Center. September 18, 2012 First-Generation Risk Profiles Help Predict CO2 Storage Site Obstacles In support of large-scale carbon capture, utilization and storage projects, a collaboration of five U.S. Department of Energy national laboratories has

365

step toward the project's planned early 2011 startup. The project  

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

step toward the project's planned early 2011 startup. The project step toward the project's planned early 2011 startup. The project will capture CO 2 from the Archer Daniels Midland (ADM) Ethanol Production Facility and inject it into a deep saline reservoir more than one mile underground. Beginning in early 2011, up to 1 million metric tons of the captured CO 2 will be compressed into a dense, liquid-like state and injected over a three-year period. The Mt. Simon Sandstone, which is the rock formation targeted for the injection, is the thickest and most widespread saline reservoir in the Illinois Basin, with an estimated CO 2 storage capacity as high as 110 billion metric tons. Analysis of the survey data is a key component in the comprehensive monitoring program that will be implemented to ensure the injected

366

Page not found | Department of Energy  

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

91 - 12100 of 28,905 results. 91 - 12100 of 28,905 results. Download EA-1828: Final Environmental Assessment 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 http://energy.gov/nepa/downloads/ea-1828-final-environmental-assessment Download Enforcement Letter, WEL-2013-01 Issued to Los Alamos National Security, LLC, related to Worker Beryllium Exposure during Machining at the Los Alamos National Laboratory's Beryllium Technology Facility http://energy.gov/hss/downloads/enforcement-letter-wel-2013-01 Download Performance Analysis- Environmental Monitoring, Surveillance, and Control Programs Within the U.S. Department of Energy, October 2002

367

PRELIMINqRY RADIOLOGICAL SURVEY REPORT OF THE FORMER STATEN ISLAND WAREHOUSE SITE  

Office of Legacy Management (LM)

pJ y, 22/4 pJ y, 22/4 PRELIMINqRY RADIOLOGICAL SURVEY REPORT OF THE FORMER STATEN ISLAND WAREHOUSE SITE (ARCHER-DANIELS MIOLANO COMPANY) AT PORT RICHMOND, NEW YORK ./ Work performed by the Health and Safety Research Division Oak Ridge National Laboratory Oak Ridge, Tennessee 37830 . . ' October 1980 OAK RIDGE NATIONAL LABORATORY operated by UNION CARBIDE CORPORATION for the DEPARTMENT OF ENERGY as part of the Former1 y Uti 1 i ted Sites-- Remedial Action Program PRELIMINARY RADIOLOGICAL SURVEY REPORT OF THE FORMER STATEN ISLANI I WAREHOUSE SITE (ARCHER-OANIELS MIDLAND COMPANY) AT PORT RICHMOND, NEW YORK B. A. Berven and C. Clark Introduction A number of buildings located at the site of the former Staten Island Warehouse in Port Richmond, New York, were used by Union Minie're

368

Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction |  

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

Large-Scale Industrial Carbon Capture, Storage Plant Begins Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction Large-Scale Industrial Carbon Capture, Storage Plant Begins Construction August 24, 2011 - 1:00pm Addthis Washington, DC - Construction activities have begun at an Illinois ethanol plant that will demonstrate carbon capture and storage. The project, sponsored by the U.S. Department of Energy's Office of Fossil Energy, is the first large-scale integrated carbon capture and storage (CCS) demonstration project funded by the American Recovery and Reinvestment Act (ARRA) to move into the construction phase. Led by the Archer Daniels Midland Company (ADM), a member of DOE's Midwest Geological Sequestration Consortium, the Illinois-ICCS project is designed to sequester approximately 2,500 metric tons of carbon dioxide

369

Microsoft Word - Final EA- ADM.doc  

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

8 8 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 Capture and Sequestration (ICCS) Area 1 Project/National Energy Technology Laboratory/Office of Fossil Energy). INTENTIONALLY LEFT BLANK COVER SHEET Responsible Agency: U.S. Department of Energy (DOE) Title: CO 2 Capture from Biofuels Production and Sequestration into the Mt. Simon Sandstone

370

Running Line-Haul Trucks on Ethanol  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

I 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 petroleum supply, the price and supply of ethanol is not subject to the whims of potentially unstable foreign governments. And domestic production translates into domestic jobs. In addition, ethanol has the potential to reduce harmful emissions, such as particulate matter and oxides of nitrogen

371

DOE Announces $160 Million for Biorefinery Construction and Highlights New  

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

$160 Million for Biorefinery Construction and $160 Million for Biorefinery Construction and Highlights New Agricultural Program to Promote Biofuels DOE Announces $160 Million for Biorefinery Construction and Highlights New Agricultural Program to Promote Biofuels February 22, 2006 - 12:11pm Addthis Funding Paves the Way for Diversifying America's Energy Mix DECATUR, IL - Energy Secretary Samuel W. Bodman, today announced $160 million in cost-shared funding over three years to construct up to three biorefineries in the United States. The Secretary made the announcement while visiting the Archer Daniels Midland Ethanol Plant, his second of four stops to promote the Advanced Energy Initiative announced by President Bush in his State of the Union address. Secretary Bodman also highlighted the United States Department of Agriculture's announcement today of almost $188

372

Property:NrelPartnerYear | Open Energy Information  

Open Energy Info (EERE)

NrelPartnerYear NrelPartnerYear Jump to: navigation, search Property Name NrelPartnerYear Property Type String Description Year partnership was initiated or announced.. Pages using the property "NrelPartnerYear" Showing 25 pages using this property. (previous 25) (next 25) 1 1366 Technologies + 2009 + 3 3M + 2010 + A A123Systems + 2008 + AVL Powertrain Engineering + 2003 + AWS Truewind + 2008 + Abengoa Solar + 2008 + Alcoa + 2010 + Alstom Energy Systems + 2010 + Alta Devices + 2010 + Ammonix + 2010 + Ampulse + 2008 + Applied Materials + 2008 + Applied Optical Systems + 2008 + Archer Daniels Midland + 2008 + Ascent Solar + 2009 + Atlas Material Testing Solutions + 2009 + B BP Solar + 2002 + Bank of America + 2009 + Benteler Industries + 2002 + Bergey Windpower Co. + 1996 +

373

Microsoft PowerPoint - 12-02 Balogapol shekarrev2.ppt  

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

CAUSTIC RECYCLING CAUSTIC RECYCLING Shekar Balagopal Anthony Nickens November 18 th 2010 Print Close Outline * Insertion Opportunities at Site * Caustic Recycling Overview * Pilot Scale Demonstration Phase * Conclusions 2 Print Close Sodium Separation Technology Already Commercially Deployed! 3 Biodiesel Facility in Mexico, MO  NaSelect Ceramic Membrane Technology Deployed  Producing Sodium Methylate (SMO) for Archer Daniels Midland  Technology is Scalable 1500 lbs/day on a 100% basis of SMO  Equivalent to production of 71.2 kgs per hour of 10 M NaOH concentration from Actual Waste Modular revolutionary commercial technology applied to treat radioactive waste Print Close Principle of Operation: Electrolytic Ceramic Membrane Cell Electrode Reactions: Anode: 2H 2 O = O 2 + 4H

374

NETL F 451.1-1/1 Categorical Exclusion (CX) Designation Form  

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

Midland, TX Texas Propane Fleet Pilot Program Propane vehicle purchases and installation of propane refueling infrastructure Midland, TX. This CX form is for one location in this...

375

Energy Systems Division Ed Daniels, Division Director University of Chicago Review Energy Engineering and Systems Analysis November 18, 2010  

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

Technology Technology Research and Development Don Hillebrand, Energy Systems Division Director Secretary of Energy Advisory Board Meeting Energy Engineering and Systems Analysis April 2012 Argonne's Transportation Research Is Focused on DOE's Energy Resources Goal  Improving energy productivity across all sectors, including transportation, is a goal in the Energy Security Theme of the DOE Strategic Plan.  A strategy to meet that goal is to develop technologies that enable cars and trucks to be fuel efficient, while remaining cost and performance competitive. 2 Market Snapshot - Auto Sales have Recovered Efficiency reduces oil use and CO2 emissions

376

ICSI'S 2005 SPEAKER RECOGNITION SYSTEM Nikki Mirghafori, Andrew O. Hatch, Steven Stafford, Kofi Boakye, Daniel Gillick, and Barbara Peskin  

E-Print Network (OSTI)

ICSI'S 2005 SPEAKER RECOGNITION SYSTEM Nikki Mirghafori, Andrew O. Hatch, Steven Stafford, Kofi://htk.eng.cam.ac.uk/. [6] D. Gillick, S. Stafford, and B. Peskin. Speaker detection without models. In ICASSP, pages I­757

Mirghafori, N. Nikki

377

A terahertz two-wire waveguide with low bending loss Marx Mbonye, Rajind Mendis, and Daniel M. Mittlemana  

E-Print Network (OSTI)

- damental transverse-electromagnetic TEM mode of this two-conductor structure by mapping the field pattern and receiver undisturbed, indi- cating no line-of-sight transmission of freely propagating ra- diation from for improved spatial resolution is raster-scanned in an 8 6 mm2 grid in steps of 1 mm. By orienting

Mittleman, Daniel

378

Multi-Flash 3D Photography: Capturing Shape and Appearance Douglas Lanman Peter G. Sibley Daniel Crispell  

E-Print Network (OSTI)

using a calibration grid. After data capture, we rectify each image to remove any radial distortion the algorithm described in [Raskar et al. 2004], we estimate a depth edge confidence map for each viewpoint International Sympo- sium on 3D Data Processing, Visualization and Transmission. RASKAR, R., TAN, K.-H., FERIS

Taubin, Gabriel

379

The Perils of Consumption and the Gift Economy as the Solution Daniel Millers Consumption and Its Consequences  

E-Print Network (OSTI)

868. Leahy, T. (2011). The gift economy. In A. Nelson & F.fair and sustainable economies (pp. 111-135). London: Plutofair and sustainable economies. London: Pluto Press. Nelson,

Leahy, Terry

2013-01-01T23:59:59.000Z

380

A supply chain carbon footprint analysis of the University of California, Berkeley Christopher M. Jones and Daniel M. Kammen  

E-Print Network (OSTI)

April 2010. iv US EPA. eGRID2007 Version 1. Available online: http://www.epa.gov/cleanenergy/energy- resources/egrid/index.html (accessed April, 2010) #12;

Kammen, Daniel M.

Note: This page contains sample records for the topic "daniels midland ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

RENEWABLE ENERGY: A VIABLE CHOICE By Antonia V. Herzog, Timothy E. Lipman, Jennifer L. Edwards, and Daniel M. Kammen  

E-Print Network (OSTI)

the United States spent more than $600 billion on energy, with U.S. oil imports climbing to $120 billion be addressed immediately--and that U.S. policy needs to be directed toward implementing clean energy solutions for renewable energy technologies SOURCE: U.S. Department of Energy (DOE), Renewable Energy Technology

Kammen, Daniel M.

382

THE LIPID WORLD DANIEL SEGR1, DAFNA BEN-ELI1, DAVID W. DEAMER2 and DORON  

E-Print Network (OSTI)

, both the Bergius and Fisher-Tropsch synthetic fuel processes build up longer chain hydrocarbons from Fischer and Tropsch, low-temperature catalysts were used to promote hydrogen's reaction with coal gas-to-liquids" (GTL) technology based on the Fischer-Tropsch process converts natural gas to liquid fuels. Essentially

Segrè, Daniel

383

Modul: 6 Modultitel: Gesundheitspolitik und Soziale Sicherung Modulverantwortliche: Prof. Dr. Friedrich-Wilhelm Schwartz, Caroline Krugmann, MPH, Daniel Reuter  

E-Print Network (OSTI)

-Verlag, Heidelberg Kück U (Hrsg.) (2004) Praktikum der Molekulargenetik, Springer-Verlag Berlin, Heidelberg

Manstein, Dietmar J.

384

Battery Powered Electric Car, Using Photovoltaic Cells Assistance Juan Dixon, Alberto Ziga, Angel Abusleme and Daniel Soto  

E-Print Network (OSTI)

transport costs. Keywords: solar energy, battery charge, photovoltaic. 1 Introduction Although rangeBattery Powered Electric Car, Using Photovoltaic Cells Assistance Juan Dixon, Alberto Zúñiga, Angel-capacity batteries, it is still difficult to develop an economically viable and socially acceptable EV for massive

Rudnick, Hugh

385

Experience of Optimizing FFT on Intel Architectures Daniel Orozco, Liping Xue, Murat Bolat, Xiaoming Li, Guang R. Gao  

E-Print Network (OSTI)

, 9] suggests that some of the lower­level optimizations, including the usage of machine, Xiaoming Li, Guang R. Gao The Electrical and Computer Engineering Department University of Delaware. At the lower kernel level, library generators use a set of kernels that are aggressively tuned for differ­ ent

Gao, Guang R.

386

Experience of Optimizing FFT on Intel Architectures Daniel Orozco, Liping Xue, Murat Bolat, Xiaoming Li, Guang R. Gao  

E-Print Network (OSTI)

, 9] suggests that some of the lower-level optimizations, including the usage of machine, Xiaoming Li, Guang R. Gao The Electrical and Computer Engineering Department University of Delaware. At the lower kernel level, library generators use a set of kernels that are aggressively tuned for differ- ent

Gao, Guang R.

387

Part I--A Rational Aerodynamic Design Procedure  

E-Print Network (OSTI)

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

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

1967-01-01T23:59:59.000Z

388

K-corrections and spectral templates of Type Ia supernovae  

E-Print Network (OSTI)

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

Hsiao, E. Y.

2008-01-01T23:59:59.000Z

389

The complete mitochondrial genome of Articulate Brachiopod Terebratal ia transversa  

SciTech Connect

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

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

2001-07-01T23:59:59.000Z

390

IA/Cyber Defense Brief for USAREUR Land EXPO  

Science Conference Proceedings (OSTI)

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

2007-11-15T23:59:59.000Z

391

www.ias.edu/rise Science Initiative Group  

E-Print Network (OSTI)

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

392

The SN Ia Rate in High-Redshift Galaxy Clusters  

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

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

393

UMore Ph IA CR Report 7-8-10.pdf  

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

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

394

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

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

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

395

Closest Type Ia Supernova in Decades Solves a Cosmic Mystery  

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

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

396

UNU-IAS Policy Report Biofuels in Africa  

E-Print Network (OSTI)

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

397

Distributed Flames in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

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

398

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

Gasoline and Diesel Fuel Update (EIA)

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

399

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

Annual Energy Outlook 2012 (EIA)

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

400

Overview of the structural geology and tectonics of the Central Basin Platform, Delaware Basin, and Midland Basin, West Texas and New Mexico  

SciTech Connect

The structural geology and tectonics of the Permian Basin were investigated using an integrated approach incorporating satellite imagery, aeromagnetics, gravity, seismic, regional subsurface mapping and published literature. 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 or contraction. Secondary objectives included delineation of basement and shallower fault zones, identification of structural style, characterization of fractured zones, analysis of surficial linear features on satellite imagery and their correlation to deeper structures. Gandu Unit, also known as Andector Field at the Ellenburger level and Goldsmith Field at Permian and younger reservoir horizons, is the primary area of interest and lies in the northern part of Ector county. The field trends northwest across the county line into Andrews County. The field(s) are located along an Ellenburger thrust anticline trap on the eastern margin of the Central Basin Platform.

Hoak, T. [Kestrel Geoscience, Littleton, CO (United States); Sundberg, K. [Phillips Petroleum Co., Bartlesville, OK (United States); Ortoleva, P. [Indiana Univ., Bloomington, IN (United States)

1998-12-31T23:59:59.000Z

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


401

Microsoft PowerPoint - DOE_presentation OSU.pptx  

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

Ohio State University Presenter: Dr. Jeff Daniels, School of Earth Sciences 1 February 23, 2011 PI: Dr. Jeff Daniels PI: Dr. Jeff Daniels Student: Michael Murphy ...

402

Fragrant Gardens and Converging Waters: Ottoman Governance in Seventeenth-Century Damascus  

E-Print Network (OSTI)

Press, Goffman, Daniel,. Izmir and the Levantine World,concerns of Daniel Goffman, Izmir and the Levantine World,

Taylor, Malissa Anne

2011-01-01T23:59:59.000Z

403

GROUP 1 GROUP 2 GROUP 3 GROUP 4 GROUP 5 GROUP 6 CARR, DANIEL ANDERSON, JENNY BANGU, LINA ABATE BESSOMO, ANNA BEHAN, LIAM ANDERSON, ARAN  

E-Print Network (OSTI)

FLEMING, BRIAN GUZUN, VLADIMIR MILNE-TURNER, ALEXANDERGARRETT, REBECCA MADDEN, STEPHEN MULLOY, AIDAN

O'Mahony, Donal E.

404

HYDROLOGY OF SOUTHWESTERNENCINAL OAK ECOSYSTEMS:A REVIEW AND MORE Gerald J. ~ottfried,'Peter F. Ffolliott, and Daniel G. ear^^  

E-Print Network (OSTI)

. Burns, R.M., Honkala, B.H., 1990. Silvics of North America. 2. Hardwoods. US Dept. Agric. Hdbk. 654, Vol

405

Semantically Rich Application-Centric Security in Android Machigar Ongtang, Stephen McLaughlin, William Enck and Patrick McDaniel  

E-Print Network (OSTI)

and package manifest files. Each definition specifies "protection level." The protection level can be "normal by a developer key (as is the framework package containing OS defined permission labels). A signature protected the package defining the permission label. Many OS defined permissions use the signature protection level

McDaniel, Patrick Drew

406

Scale-Based Monotonicity Analysis in Qualitative Modelling with Flat Segments Martin Brooks1 and Yuhong Yan1 and Daniel Lemire2  

E-Print Network (OSTI)

qualitative models for complex real world engineering systems. Current research efforts are on automatic quantitative models in tasks such as Model-based Diagnosis (MBD), explaining system behavior, and designing novel devices from first principles. Monotonicity is an important feature to leverage when constructing

Yan, Yuhong

407

Superfluid Transition in a Rotating Fermi Gas with Resonant Interactions Martin Y. Veillette, Daniel E. Sheehy, Leo Radzihovsky, and Victor Gurarie  

E-Print Network (OSTI)

Superfluid Transition in a Rotating Fermi Gas with Resonant Interactions Martin Y. Veillette atomic Fermi gas near a narrow s-wave Feshbach resonance in a uniaxial trap with frequencies ?, z. We, the centrifugal force, the trap potential, the fixed number of atoms, and the tunable resonant pairing interaction

Baltisberger, Jay H.

408

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

E-Print Network (OSTI)

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

Texas at Austin, University of

409

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

SciTech Connect

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

Rodekohr, M.; Cato, D.

1979-09-01T23:59:59.000Z

410

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

Science Conference Proceedings (OSTI)

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

2013-08-19T23:59:59.000Z

411

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

E-Print Network (OSTI)

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

Garavini, G.; Supernova Cosmology Project

2008-01-01T23:59:59.000Z

412

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

E-Print Network (OSTI)

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

Meyers, Joshua Evan

2012-01-01T23:59:59.000Z

413

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg130  

E-Print Network (OSTI)

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

414

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

E-Print Network (OSTI)

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

Hazen, Terry

415

Prospects for Type Ia Supernova explosion mechanism identification with gamma rays  

E-Print Network (OSTI)

The explosion mechanism associated with thermonuclear supernovae (SNIa) is still a matter of debate. There is a wide agreement that high amounts of of radioactive nuclei are produced during these events and they are expected to be strong gamma-ray emitters. In the past, several authors have investigated the use of this gamma-ray emission as a diagnostic tool. In this paper we have done a complete study of the gamma-ray spectra associated with all the different scenarios currently proposed. This includes detonation, delayed detonation, deflagration and the off-center detonation. We have performed accurate simulations for this complete set of models in order to determine the most promising spectral features that could be used to discriminate among the different models. Our study is not limited to qualitative arguments. Instead, we have quantified the differences among the spectra and established distance limits for their detection. The calculations have been performed considering the best current response estim...

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

1997-01-01T23:59:59.000Z

416

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

Science Conference Proceedings (OSTI)

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

Rumi Zahir; Jonathan Ross; Dale Morris; Drew Hess

2000-12-01T23:59:59.000Z

417

Pacific Northwest National Laboratory: INstItute for INterfacIaL cataLysIs  

E-Print Network (OSTI)

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

418

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

E-Print Network (OSTI)

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

419

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg102  

E-Print Network (OSTI)

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

420

Pacific Northwest National Laboratory: INstItute for INterfacIaL cataLysIs  

E-Print Network (OSTI)

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

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421

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

SciTech Connect

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

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

2013-03-01T23:59:59.000Z

422

SUSTAINABILITY EXCELLENTIA CoLumbIA ENgINEErINg 141  

E-Print Network (OSTI)

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

423

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

E-Print Network (OSTI)

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

Bell, John B.

424

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

E-Print Network (OSTI)

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

Seco, Luis A.

425

INFORMATION EXCELLENTIA CoLumbIA ENgINEErINg238  

E-Print Network (OSTI)

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

Hone, James

426

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

SciTech Connect

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

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

2013-03-01T23:59:59.000Z

427

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

E-Print Network (OSTI)

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

Pulfrey, David L.

428

An asixymmetric diffusion experiment for the determination of diffusion and sorption coefficients of rock samples  

E-Print Network (OSTI)

Nuclear Waste Management, Shackelford, C.D. , Daniel, D.E. ,ASCE 117(3), 467-484. Shackelford, C.D. , Daniel, D.E. ,diffusion effects (Shackelford and Daniel, 1991a) may

Takeda, M.

2011-01-01T23:59:59.000Z

429

Just What is a Supernova?  

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

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

430

 

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

one way to blow up a white dwarf one way to blow up a white dwarf Daniel Kasen LBNL/UCB Abstract: Despite intense observational and theoretical study, the progenitors of Type Ia supernovae remain uncertain. Recent observations are challenging the commonly held view that the exploding star always has a mass near the Chandrasekhar limit. I will review the different channels leading to the thermonuclear disruption of a carbon oxygen white dwarf, focusing on how these scenarios might be discriminated using observations of supernova spectra, light curves, and polarization. I will describe some theoretical predictions which may be useful in testing both the single degenerate and double white dwarf merger scenarios, and offer some model comparisons to recent observations of so-called "super-Chandrasekhar mass" events. I

431

Introduction  

Science Conference Proceedings (OSTI)

...S. Chumbley Ames Laboratory Carl Czajkowski Brookhaven National Laboratory Daniel R. Danks Danks Tribological Services Daniel P. Dennies The Boeing Company Bill Dobson Binary Egnineering Associates,

432

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

Office of Scientific and Technical Information (OSTI)

Kammen, Daniel M. (Daniel M. Kammen) - Renewable and Appropriate Energy Laboratory, University of California at Berkeley Kr, Sren Knudsen (Sren Knudsen Kr) - Department of...

433

ACCESS Magazine Fall 1996  

E-Print Network (OSTI)

Daniel "Gearing Up for Electric Cars" UCTC 146 Sperling,Gordon J. Bringing Electric Cars to Market, DanielSperling Who Will Buy Electric Cars? , Thomas Turrentine

1996-01-01T23:59:59.000Z

434

Before the Subcommittee on Strategic Forces - House Armed Services...  

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

Daniel B. Poneman, Deputy Secretary of Energy Before the Subcommittee on Strategic Forces - House Armed Services Committee 2-28-13DanielPoneman FT HASC More Documents &...

435

NIST logo  

Science Conference Proceedings (OSTI)

... 1999 Daniel Josell (Metallurgy Division). ... 2001 Daniel W. Lozier 2002 H. Heather Chen-Mayer 2003 Robert D. Shull (Metallurgy Division, MSEL). ...

436

Page not found | Department of Energy  

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

Secretary Daniel Poneman's Remarks to the International Forum for a Nuclear Weapons-Free World Please find below Deputy Secretary Daniel Poneman's remarks, as prepared for...

437

Management of dry flue gas desulfurization by-products in underground mines. Quarterly report, August 1--October 31, 1997  

Science Conference Proceedings (OSTI)

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.

Chugh, Y.P.

1997-12-31T23:59:59.000Z

438

NETL F 451.1-1/1 Categorical Exclusion (CX) Designation Form  

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

- 07312013 Midland, MI CONTRIBUTING TO NET ZERO BUILDING: HIGH ENERGY EFFICIENT EIFS WALL SYSTEMS Enhance exterior insulation and finishing system (EIFS) envelope systems to...

439

NETL F 451.1-1/1 Categorical Exclusion (CX) Designation Form  

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

Project Management Center 2010 Gary Sames 812010 - 7312013 Midland, MI Advanced Insulation for High-Performance, Cost-Effective Wall, Roof and Foundation Systems Develop...

440

Michigan | Department of Energy  

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

Assistance to Dow Kokam Mi, LLC To Manufacture Advanced Lithium Polymer Batteries for Hybrid and Electric Vehicles At Midland, Michigan March 1, 2010 EA-1721: Final...

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While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Renovar Energy Corp | Open Energy Information  

Open Energy Info (EERE)

search Name Renovar Energy Corp Place Midland, Texas Zip 79705 Product Texas-based landfill gas project developer. References Renovar Energy Corp1 LinkedIn Connections...

442

Skyward Energy LLC | Open Energy Information  

Open Energy Info (EERE)

Energy LLC is a company located in Midland, Texas . References "Skyward Energy LLC" Retrieved from "http:en.openei.orgwindex.php?titleSkywardEnergyLLC&oldid351181...

443

WIPP News Releases - 1999  

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

Symposium -- November 12 WIPP Trainers to Provide Instruction For Midland-Odessa Emergency Response Personnel -- October 29 TRUPACT-II Shipping Containers to be Built --...

444

SIM Time and Frequency Working Group  

Science Conference Proceedings (OSTI)

... IBMETRO. Report from Canada, John Bernard, NRC. Report from Chile, Daniel Mayorga, University of Concepcion. Report ...

445

Before The Subcommittee on Oversight and Investigations- House Committee on Energy and Commerce  

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

Subject: Department of Energy Management and Performance By: Daniel Poneman, Deputy Secretary of Energy

446

Newsletter Spring 1999  

E-Print Network (OSTI)

Policy Researchers: Daniel Pinkston, Jessie Jie, Elizabeth Matthews Campus Programs: Bettina Halvorsen International Affairs

1999-01-01T23:59:59.000Z

447

Ral Gonzlez Paredes INTN, Argentina Judah Levine NIST ...  

Science Conference Proceedings (OSTI)

... Ral Gonzlez Paredes INTN, Argentina ANGEL CRISTOBAL BAYAS CASTRO CMEE, Ecuador Prez, Daniel Norberto INTI, Argentina ...

2012-10-22T23:59:59.000Z

448

DIRECTOR'S MESSAGE The Research Laboratory of Electronics (RLE), founded in  

E-Print Network (OSTI)

Kleber*, Jay Fineberg² & Daniel P. Lathrop* * Institute for Plasma Research and Department of Physics

449

West Virginia University 1 Distinguished Professors  

E-Print Network (OSTI)

Distinguished Professor and Eminent Scholar · Daniel Alkon, Toyota Chair for Neurodegenerative Disease Research

Mohaghegh, Shahab

450

LL.M. PROGRAM EARN YOUR MASTER  

E-Print Network (OSTI)

." -- Gustavo Daniel Garcia Carranco `12 Head of Consulting and Prevention Division, PEMEX LL.M. SPECIALTY

Bittner, Eric R.

451

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

E-Print Network (OSTI)

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

452

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

SciTech Connect

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

Not Available

1984-08-01T23:59:59.000Z

453

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

DOE Green Energy (OSTI)

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

Smith, M. W.

2001-05-31T23:59:59.000Z

454

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

Science Conference Proceedings (OSTI)

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

Jun Wang; Jingming Chen; Weimin Ju; Manchun Li

2010-04-01T23:59:59.000Z

455

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

E-Print Network (OSTI)

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

Memphis, University of

456

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

E-Print Network (OSTI)

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

2005-01-01T23:59:59.000Z

457

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

E-Print Network (OSTI)

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

458

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

Science Conference Proceedings (OSTI)

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

Marek, Laura F.

2011-06-17T23:59:59.000Z

459

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

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

460

Readings in Common: Assimilation and Interpretive Authority in Early Modern Spain  

E-Print Network (OSTI)

Droixhe, Daniel. La linguistique et lappel de lhistoire (paradis; Droixhe, La linguistique et lappel de lhistoire (Daniel Droixhe, La linguistique et l'appel de l'histoire,

Kimmel, Seth Ross

2010-01-01T23:59:59.000Z

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461

Gearing Up for Electric Cars  

E-Print Network (OSTI)

ff sold now,they argue, electric cars would cost too muchandGearing Up for Electric Cars Daniel Sperhng Reprint UCTC Noor Gearing Up for Electric Cars Daniel Sperling Department

Sperling, Daniel

1994-01-01T23:59:59.000Z

462

Evaluation of Traffic Data Obtained via GPS-Enabled Mobile Phones: the Mobile Century Field Experiment  

E-Print Network (OSTI)

Hoh, M. Gruteser, R. Herring, J. Ban, D. Work, J. Herrera,Daniel B. Work, Ryan Herring, Xuegang (Jeff) Ban, andDaniel B. Work 2 , Ryan Herring 3 , Xuegang (Je?) Ban 4 ,

Herrera, Juan C.; Work, Daniel B.; Herring, Ryan; Ban, Xuegang Jeff; Bayen, Alexandre M

2009-01-01T23:59:59.000Z

463

Legal | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

(EM) Daniel Park, (630) 252-2308 Golden Field Office (GFO) Brian Lally, (630) 252-2042 Idaho Operations Office Daniel Park, (630) 252-2308 Western Area Power Administration (WAPA)...

464

Geological and Geophysical Investigations of the Hydrogeology  

E-Print Network (OSTI)

: Canol Road Area Daniel E. Lawson, Jeffrey C. Strasser, Jodie D. Strasser, Steven A. Arcone, Allan J of Fort Wainwright, Alaska Part I: Canol Road Area Daniel E. Lawson, Jeffrey C. Strasser, Jodie D

465

The Bumpy Road to Hydrogen  

E-Print Network (OSTI)

It appears to us that hydrogen is a highly promising option0616 The Bumpy Road to Hydrogen Daniel Sperling Joan OgdenThe Bumpy Road to Hydrogen 1 Daniel Sperling and Joan Ogden

Sperling, Dan; Ogden, Joan M

2006-01-01T23:59:59.000Z

466

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

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

0501 NETL ORD (Daniel J. Soeder) FE ORDGES FY2013Indefinite Daniel J. Soeder NETL: Morgantown, WV (B-25, RM 212) Modification to the Petrography Laboratory This lab provides...

467

FreedomCAR Automotive Lightweighting Materials  

Science Conference Proceedings (OSTI)

Apr 1, 2007... probable peaking of conventional petroleum production capacity in the ... SOURCE: Carpenter, Joseph A., Edward Daniels, Philip Sklad,...

468

Rebuilding After Katrina: A Population-Based Study of Labor and Human Rights in New Orleans  

E-Print Network (OSTI)

and Daniel P. Brown, Tropical Cyclone Report: Hurricane1-P) d 2 Knabb et al. , Tropical Cyclone Report. Gabe, et

Fletcher, Laurel; Pham, Phuong N; Stover, Eric; Vinck, Patrick

2006-01-01T23:59:59.000Z

469

Strategic Planning October 2007  

E-Print Network (OSTI)

watchword be order and your beacon, beauty. Think big! ­ Daniel Burnham; US Architect, 19th Century "Make

Milchberg, Howard

470

This article describes how the Research Library at the ...  

Science Conference Proceedings (OSTI)

... 2 (April 1996): 161- 193. 11. Eileen G. Abels, Peter Liebscher, and Daniel W. Denman, Factors that Influence the use ...

2011-07-14T23:59:59.000Z

471

Staff Listing  

Science Conference Proceedings (OSTI)

... Golas, Daniel, Nuclear Energy Institute, 301-975-5540. ... Physical Measurement Laboratory Radiation and Biomulecular Physics Division. ...

2013-06-26T23:59:59.000Z

472

International Governance of Climate Engineering  

E-Print Network (OSTI)

Solar Radiation Management Governance Initiative conference); Daniel Bodansky, Governing Climate Engineering: Scenarios for Analysis (Harvard Project on Climate Agreements,

Parson, Edward; Ernst, Lia

2012-01-01T23:59:59.000Z

473

WCM Decisionmakers' Forum  

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

& Development Autrhority - Rutgers University (NYSERDA) - National Oilwell Varco - Weatherford Laboratories Project Management Team - Daniel Collins - PI, Sandia Technologies,...

474

Detecting and Imaging He2 Molecules in Superfluid Helium by Laser-Induced Fluorescence  

E-Print Network (OSTI)

Dissertation Director: Professor Daniel N. McKinsey September 2008 #12;Copyright c 2008 by Wade G. Rellergert

McKinsey, Daniel

475

Direct detection of dark matter with liquid argon and neon Walter Hugh Lippincott  

E-Print Network (OSTI)

Lippincott Dissertation Director: Professor Daniel McKinsey December 2010 #12;i c Copyright 2010 by Walter

McKinsey, Daniel

476

Before the Subcommittee on Strategic Forces - House Armed Services Committee  

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

Subject: Security Incident at the Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

477

Before the Subcommittee on Oversight and Investigations - House Committee on Energy and Commerce  

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

Subject: Security Incident at the Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

478

MS&T '05 Technical Program  

Science Conference Proceedings (OSTI)

Program Organizers: B. Lynn Ferguson, Deformation Control. Technology, Inc. .... Session Chairs: Julie Schoenung, University of California, Davis;. Jean-Daniel...

479

Before the Subcommittee on Strategic Forces- House Armed Services Committee  

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

Subject: Security Incident at Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

480

Appendix 56 Management of Montana's Amphibians  

E-Print Network (OSTI)

and Applications, Dortmund, Germany. New York: IEEE. McDaniel, P., and S. McLaughlin. 2009. Security and privacy

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481

VIRGINIA POLYTECHNIC INSTITUTE AND STATE UNIVERSIT Y COMMENCEMENT  

E-Print Network (OSTI)

. Bruce Berriman, Ewa Deelman, John Good, Joseph C. Jacob, Daniel S. Katz, Anastasia C. Laity, Thomas A

Virginia Tech

482

State Laboratory Contact Information AZ  

Science Conference Proceedings (OSTI)

... David Pfahler Brad Stover ... Joe Benavides Harvey Fischer Daniel Gibbons Preston Adachi Philip Wright Shauna Pereiro Lisa Corn Pat Sanders ...

2013-01-07T23:59:59.000Z

483

NIST.gov - Computer Security Division - Computer Security ...  

Science Conference Proceedings (OSTI)

... PIV Implementation, Daniel Wood, Treasury; Electricity Subsector Cybersecurity ... Basic Input/Output System (BIOS) Security - Andrew Regenscheid ...

484

NIST Demonstrates Significant Improvement in the ...  

Science Conference Proceedings (OSTI)

... "A major challenge with solar energy is dealing with solar intermittency," says NIST chemical engineer Daniel Esposito. ...

2013-05-14T23:59:59.000Z

485

NIST Tech Beat for May 14, 2013  

Science Conference Proceedings (OSTI)

... "A major challenge with solar energy is dealing with solar intermittency," says NIST chemical engineer Daniel Esposito. ...

2013-05-14T23:59:59.000Z

486

No d'ordre : 4139 ANNE 2010 THSE / UNIVERSIT DE RENNES 1  

E-Print Network (OSTI)

Hulin-Hubard and Daniel Lemoal. Finally my warmest gratitude goes to those whose presence in my life

Paris-Sud XI, Université de

487

As of August 1, 2006 Review and Discussion of Draft Results  

E-Print Network (OSTI)

LLC Email: rutherford.daniel@tiaxllc.com Craig Scott Toyota Email: craig_scott@toyota.com Tom Sheahen

488

com  

Science Conference Proceedings (OSTI)

... Magnetoelastic Coupling in Iron-based Superconductors. Daniel Parshall (University of Colorado). The cause of high-temperature ...

489

Before the Senate Energy and Natural Resources Committee  

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

Subject: FY 2014 Budget Request for the Department of Energy By: Daniel B. Poneman, Deputy Secretary of Energy

490

ENVIRONMENTAL BIOTECHNOLOGY Influence of trace erythromycin and erythromycin-H2O  

E-Print Network (OSTI)

& Bonaparte, 1989a;b; Giroud et al., 1992; Daniel, 1993); (2) better biogas control; (3) minimization

Alvarez-Cohen, Lisa

491

BIG DATA Workshop  

Science Conference Proceedings (OSTI)

... Chris White, DARPA; Daniel Starosta, NOAA - Data Processing , Product Generation and Distribution at the NWS National Centers for ...

2013-04-02T23:59:59.000Z

492

REPORT TO THE PRESIDENT ON ENSURING AMERICAN ...  

Science Conference Proceedings (OSTI)

... University, St. Louis Vice President, National Academy of Sciences Eric Schmidt Executive Chairman Google, Inc. Daniel Schrag ...

2013-07-31T23:59:59.000Z

493

Deputy Secretary Poneman Delivers Remarks on Nuclear Power at Tokyo American Center in Japan  

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

Energy Deputy Secretary Daniel Poneman spoke at the Tokyo American Center today about nuclear power after Fukushima.

494

NCNR Seminar Schedule  

Science Conference Proceedings (OSTI)

... am. Place: Building 235, Room K04B. Title: Research Challenges of Unconventional Shale Reservoirs. Speaker: Daniel ...

495

Third Century Third Century  

Science Conference Proceedings (OSTI)

... Daniel T. Ames Ames on Forgery 1900 ... This laboratory was modeled after multidisciplinary European laboratories and included a ...

2013-06-12T23:59:59.000Z

496

Detection of Magnetically Trapped Neutrons: Liquid Helium as a Scintillator  

E-Print Network (OSTI)

by Daniel Nicholas McKinsey to The Department of Physics in partial fulfillment of the requirements February 2002 #12;c 2002 - Daniel Nicholas McKinsey All rights reserved. #12;To my parents #12;Thesis advisor Author John Morrissey Doyle Daniel Nicholas McKinsey Detection of Magnetically Trapped Neutrons

McKinsey, Daniel

497

A Comparison of Objective and Subjective Means of Weather Typing: An Example from West Texas  

Science Conference Proceedings (OSTI)

An objective weather typing scheme first proposed by Christensen and Bryson (1966) was applied to surface and upper air variables for the period AprilSeptember of 197376 at Midland, Texas. Principal components analysis showed that moisture and ...

Judson W. Ladd; Dennis M. Driscoll

1980-06-01T23:59:59.000Z

498

Kinetic Wave Power | Open Energy Information  

Open Energy Info (EERE)

Kinetic Wave Power Jump to: navigation, search Name Kinetic Wave Power Address 2861 N Tupelo St Place Midland Zip 48642 Sector Marine and Hydrokinetic Phone number 989-839-9757...

499

Mr. Ken Blower, Manager Corporate Environmental Affairs Standard...  

Office of Legacy Management (LM)

ad. 3 0 II, 0 s 3 & Mr. Ken Blower, Manager Corporate Environmental Affairs Standard Oil Company of Ohio Midland Building Cleveland, Ohio 44115 qITIALSSIG Jhitman )ATE 1 86...

500

International Symposium on Site Characterization for CO2 Geological Storage  

E-Print Network (OSTI)

groundwater above two Permian Basin oil fields (SACROC Unitin New Mex- ico in the Permian basin. In the field study atPermian boundary in shelf areas of the North Plat- form of the Midland Basin,

Tsang, Chin-Fu

2006-01-01T23:59:59.000Z