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  1. Nova Scotia: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    by expanding it. Nova Scotia is a province in Canada. Energy Incentives for Nova Scotia Air Quality (Nova Scotia, Canada) Capital Investment Incentive (Nova Scotia, Canada)...

  2. Efficiency Nova Scotia Releases Energy Efficiency Mobile App...

    Energy Savers [EERE]

    Better Buildings Residential Network member Efficiency Nova Scotia recently released Spot it-an energy efficiency game app for mobile devices. The app features 13 levels where ...

  3. Efficiency Nova Scotia Releases Energy Efficiency Mobile App

    Broader source: Energy.gov [DOE]

    Better Buildings Residential Network member Efficiency Nova Scotia recently released Spot it!—an energy efficiency game app for mobile devices. The app features 13 levels where players are...

  4. MHK Projects/OpenHydro Bay of Fundy Nova Scotia CA | Open Energy...

    Open Energy Info (EERE)

    Phase Phase 1 Project Details OpenHydro is working with Canadian utility Nova Scotia Power to create a tidal demonstration project in the Bay of Fundy. Following successful...

  5. EA-355 Scotia Capital Energy, Inc. | Department of Energy

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

    5 Scotia Capital Energy, Inc. EA-355 Scotia Capital Energy, Inc. Order authorizing Scotia Capital Energy, Inc. to export electric energy to Canada EA-355 Scotia Capital Energy, ...

  6. Chedabucto Bay 1992 shoreline oil conditions survey: Long-term fate of bunker C oil from the arrow spill in Chedabucto Bay, Nova Scotia

    SciTech Connect (OSTI)

    Owens, E.H.; McGuire, B.E.; Humphrey, B.

    1994-03-01

    The report presents a description of the activities related to and a summary of the information generated by a field survey carried out in Chedabucto Bay, Nova Scotia, for Environment Canada from June to September 1992. The objective of the survey was to locate and document any residual oil on the shores of Chedabucto Bay. The grounding of the tanker Arrow in February 1970 resulted in the release of more than 11 million liters of Bunker C fuel oil. This oil was stranded over an estimated 305 km of shoreline in the Chedabucto Bay area.

  7. Reasons for decision in the matter of Sable Offshore Energy Inc., application dated 9 June 1998 for approval of the plan, profile and book of reference respecting the detailed route of a subsea pipeline from the Thebaud platform to a landfall near Goldboro, Nova Scotia, and an onshore pipeline from the landfall point to the inlet of the gas processing plant located east of Goldboro, Nova Scotia: MH-4-98

    SciTech Connect (OSTI)

    1998-12-31

    The National Energy Board approved a natural gas pipeline to be built by the proponents of the Sable Offshore Energy Project within a specified 500-meter-wide corridor. The pipeline will run from an offshore platform near Sable Island to a gas plant on the Nova Scotia mainland. This report summarizes proceedings of hearings held to determine the detailed route of the pipeline within the specified corridor and to consider the most appropriate methods and timing of constructing the pipeline. Specific objections to the detailed route from holders of mineral rights licenses are noted and a Board decision on the detailed route is presented.

  8. Application to Export Electric Energy OE Docket No. EA-355 Scotia Capital

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

    Energy | Department of Energy 5 Scotia Capital Energy Application to Export Electric Energy OE Docket No. EA-355 Scotia Capital Energy Application from Scotia Capital Energyto export electric energy to Canada Application to Export Electric Energy OE Docket No EA-355 Scotia Capital Energy (209.34 KB) More Documents & Publications EA-355 Scotia Capital Energy, Inc. Application to Export Electric Energy OE Docket No. EA-407 Vitol Inc.: Federal Register Notice, Volume 80, No. 42 - March 4,

  9. EIS-0339: Presidential Permit Application, GenPower 500 kV Submarine Electric Transmission Cable from Nova Scotia to New York

    Broader source: Energy.gov [DOE]

    The Department of Energy (DOE) announced its intent to prepare an Environmental Impact Statement (EIS) in accordance with the National Environmental Policy Act of 1969 (NEPA) for GenPower New York, L.L.C.’s (GenPower) request for a Presidential permit for a proposed international electric transmission line.

  10. Radiological Scoping Survey of the Scotia Depot, Scotia, NY

    SciTech Connect (OSTI)

    Bailey, E. N.

    2008-02-25

    The objectives of the radiological scoping survey were to collect adequate field data for use in evaluating the radiological condition of Scotia Depot land areas, warehouses, and support buildings.

  11. Scotia Wind Ltd | Open Energy Information

    Open Energy Info (EERE)

    Wind Ltd Jump to: navigation, search Name: Scotia Wind Ltd Place: Stirling, Scotland, United Kingdom Zip: FK9 7AJ Sector: Wind energy Product: Scotia Wind is an independent...

  12. Clean Stuff: the Latest from NOVA's "Making Stuff" Mini-Series | Department

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

    of Energy Stuff: the Latest from NOVA's "Making Stuff" Mini-Series Clean Stuff: the Latest from NOVA's "Making Stuff" Mini-Series February 4, 2011 - 3:27pm Addthis Charles Rousseaux Charles Rousseaux Senior Communications Specialist (detailee) What are the key facts? Materials Science technology of transforming plastics - say from grocery bags - into carbon nanotubes and spheres, which can then be used in lithium-ion batteries, can be used for an array of other

  13. Application to Export Electric Energy OE Docket No. EA-355 Scotia...

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

    5 Scotia Capital Energy Application to Export Electric Energy OE Docket No. EA-355 Scotia Capital Energy Application from Scotia Capital Energyto export electric energy to Canada ...

  14. Final Scientific/Technical Report to the U.S. Department of Energy on NOVA's Einstein's Big Idea (Project title: E-mc2, A Two-Hour Television Program on NOVA)

    SciTech Connect (OSTI)

    Susanne Simpson

    2007-05-07

    Executive Summary A woman in the early 1700s who became one of Europe’s leading interpreters of mathematics and a poor bookbinder who became one of the giants of nineteenth-century science are just two of the pioneers whose stories NOVA explored in Einstein’s Big Idea. This two-hour documentary premiered on PBS in October 2005 and is based on the best-selling book by David Bodanis, E=mc2: A Biography of the World’s Most Famous Equation. The film and book chronicle the scientific challenges and discoveries leading up to Einstein’s startling conclusion that mass and energy are one, related by the formula E = mc2.

  15. Nova Produtiva | Open Energy Information

    Open Energy Info (EERE)

    search Name: Nova Produtiva Place: Astorga, Parana, Brazil Product: Brazil based ethanol producer, located in the state of Parana. References: Nova Produtiva1 This article...

  16. AT Cnc: A SECOND DWARF NOVA WITH A CLASSICAL NOVA SHELL Shara...

    Office of Scientific and Technical Information (OSTI)

    and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts, in accord with the hibernation scenario of cataclysmic binaries. Here...

  17. Nova Biosource Fuels formerly Nova Energy Holding Inc | Open...

    Open Energy Info (EERE)

    Nova Energy Holding Inc) Place: Colbert, Washington State Zip: 99005 Product: Former oil company which has shifted its focus to biodiesel production. Coordinates: 47.831021,...

  18. NovaTorque | Open Energy Information

    Open Energy Info (EERE)

    NovaTorque Jump to: navigation, search Logo: NovaTorque Name: NovaTorque Address: 145 N. Wolfe Road Place: Sunnyvale, California Zip: 94086 Region: Bay Area Sector: Efficiency...

  19. RECURRENT NOVAE IN M31

    SciTech Connect (OSTI)

    Shafter, A. W.; Henze, M.; Rector, T. A.; Schweizer, F.; Hornoch, K.; Orio, M.; Pietsch, W.; Darnley, M. J.; Williams, S. C.; Bode, M. F.; Bryan, J.

    2015-02-01

    The reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova (RN) candidates. To pass the initial screen and qualify as a RN candidate, two or more eruptions were required to be coincident within 0.′1, although this criterion was relaxed to 0.′15 for novae discovered on early photographic patrols. A total of 118 eruptions from 51 potential RN systems satisfied the screening criterion. To determine what fraction of these novae are indeed recurrent, the original plates and published images of the relevant eruptions have been carefully compared. This procedure has resulted in the elimination of 27 of the 51 progenitor candidates (61 eruptions) from further consideration as RNe, with another 8 systems (17 eruptions) deemed unlikely to be recurrent. Of the remaining 16 systems, 12 candidates (32 eruptions) were judged to be RNe, with an additional 4 systems (8 eruptions) being possibly recurrent. It is estimated that ∼4% of the nova eruptions seen in M31 over the past century are associated with RNe. A Monte Carlo analysis shows that the discovery efficiency for RNe may be as low as 10% that for novae in general, suggesting that as many as one in three nova eruptions observed in M31 arise from progenitor systems having recurrence times ≲100 yr. For plausible system parameters, it appears unlikely that RNe can provide a significant channel for the production of Type Ia supernovae.

  20. Argonne's Vilas Pol on NOVA!

    SciTech Connect (OSTI)

    2011-01-01

    Can innovations in materials science help clean up our world? Argonne's material scientist Vilas Pol guest starred on NOVA's "Making Stuff: Cleaner," where David Pogue explored the rapidly-developing science and business of clean energy.

  1. Argonne's Vilas Pol on NOVA!

    ScienceCinema (OSTI)

    None

    2013-04-19

    Can innovations in materials science help clean up our world? Argonne's material scientist Vilas Pol guest starred on NOVA's "Making Stuff: Cleaner," where David Pogue explored the rapidly-developing science and business of clean energy.

  2. NOvA Experiment - The Local Community

    ScienceCinema (OSTI)

    Deb Wieber

    2010-01-08

    Local proprietors Steve and Deb Wieber discuss the impact of the NOvA experiment on their community.

  3. Dept. of Energy/NOVA announce re-airing on Oct. 16 of special program:

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

    Einstein's Big Idea | Jefferson Lab Dept. of Energy/NOVA announce re-airing on Oct. 16 of special program: Einstein's Big Idea Dept. of Energy/NOVA announce re-airing on Oct. 16 of special program: Einstein's Big Idea October 13, 2005 For those who missed the NOVA special "Einstein's Big Idea", the two-hour show will air again Sunday, Oct. 16, at 6 p.m. on WHRO. The show is based on David Bodanis' book, E=mc2, and is a biography of the famous equation. The Department of Energy's

  4. Jefferson Lab News -Dept. of Energy co-sponsors Oct. 11th NOVA program:

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

    Einstein's Big Idea | Jefferson Lab Dept. of Energy co-sponsors Oct. 11th NOVA program: Einstein's Big Idea Dept. of Energy co-sponsors Oct. 11th NOVA program: Einstein's Big Idea October 4, 2005 On Tuesday, Oct. 11, PBS stations nationwide will air a new NOVA program, "Einstein's Big Idea." The two-hour show is based on David Bodanis' book, E=mc2, and is a biography of the famous equation. The Department of Energy's Office of Science is co-sponsoring "Einstein's Big

  5. Mapping quadrupole collectivity in the Cd isotopes: The breakdown...

    Office of Scientific and Technical Information (OSTI)

    Department of Physics, University of Guelph, Guelph, Ontario, N1G2W1 (Canada) (Canada) Department of Astronomy and Physics, Saint Mary's University, Halifax, Nova Scotia, B3H3C3 ...

  6. NOvA Detector Construction Timelapse

    SciTech Connect (OSTI)

    2014-10-06

    More than 7 cameras recorded the two year long process of constructing the world's largest self-supporting plastic structure, the NOvA experiment's far detector.

  7. Api Nova Energia Srl | Open Energy Information

    Open Energy Info (EERE)

    search Name: Api Nova Energia Srl Place: Roma, Italy Zip: 198 Sector: Renewable Energy Product: Develops, builds, finances, acquires, owns and operates energy production...

  8. NOVA Portal: Submit VASP Jobs to Carver via the Web

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

    NOVA Portal: Submit VASP Jobs to Carver via the Web NOVA Portal: Submit VASP Jobs to Carver via the Web May 11, 2012 by Francesca Verdier NOVA is an experimental web application ...

  9. Geradora de Energia Nova Fatima | Open Energy Information

    Open Energy Info (EERE)

    Nova Fatima Jump to: navigation, search Name: Geradora de Energia Nova Fatima Place: Braco do Norte, Santa Catarina, Brazil Zip: 88750-000 Sector: Hydro Product: Santa...

  10. Sandia Energy - Mark Boslough Featured in NOVA Special about...

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

    in NOVA Special about the Chelyabinsk Meteor Scientist Mark Boslough (Discrete Mathematics and Complex Systems Dept.) was featured in NOVA's special program "Meteor Strike,"...

  11. Nova Chemicals Reliance Industries JV | Open Energy Information

    Open Energy Info (EERE)

    Product: Nova Chemicals has signed an agreement with Reliance Industries to construct energy efficient buildings in India. References: Nova Chemicals & Reliance Industries...

  12. Cataventos Novas Energias Brasil Ltda | Open Energy Information

    Open Energy Info (EERE)

    Cataventos Novas Energias Brasil Ltda Jump to: navigation, search Name: Cataventos Novas Energias Brasil Ltda Place: Fortaleza, Ceara, Brazil Sector: Wind energy Product: Wind farm...

  13. CX-200004: Categorical Exclusion Determination | Department of Energy

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

    4: Categorical Exclusion Determination CX-200004: Categorical Exclusion Determination Pieridae Energy (USA) LTD CX(s) Applied: B5.7 Date: 1/28/2016 Location(s): Other Offices(s): Fossil Energy, Natural Gas Regulation Pieridae US proposes to export the LNG from the proposed Goldboro LNG Project (Project) located in Nova Scotia, Canada. The Application requests authority to export the LNG from the Project to any country (i) with which the United States does not have a free trade agreement (FTA)

  14. The NOvA Technical Design Report

    SciTech Connect (OSTI)

    Ayres, D.S.; Drake, G.R.; Goodman, M.C.; Grudzinski, J.J.; Guarino, V.J.; Talaga, R.L.; Zhao, A.; Stamoulis, P.; Stiliaris, E.; Tzanakos, G.; Zois, M.; /Athens U. /Caltech /UCLA /Fermilab /College de France /Harvard U. /Indiana U. /Lebedev Inst. /Michigan State U. /Minnesota U., Duluth /Minnesota U.

    2007-10-08

    Technical Design Report (TDR) describes the preliminary design of the NOvA accelerator upgrades, NOvA detectors, detector halls and detector sites. Compared to the March 2006 and November 2006 NOvA Conceptual Design Reports (CDR), critical value engineering studies have been completed and the alternatives still active in the CDR have been narrowed to achieve a preliminary technical design ready for a Critical Decision 2 review. Many aspects of NOvA described this TDR are complete to a level far beyond a preliminary design. In particular, the access road to the NOvA Far Detector site in Minnesota has an advanced technical design at a level appropriate for a Critical Decision 3a review. Several components of the accelerator upgrade and new neutrino detectors also have advanced technical designs appropriate for a Critical Decision 3a review. Chapter 1 is an Executive Summary with a short description of the NOvA project. Chapter 2 describes how the Fermilab NuMI beam will provide a narrow band beam of neutrinos for NOvA. Chapter 3 gives an updated overview of the scientific basis for the NOvA experiment, focusing on the primary goal to extend the search for {nu}{sub {mu}} {yields} {nu}{sub e} oscillations and measure the sin{sup 2}(2{theta}{sub 13}) parameter. This parameter has not been measured in any previous experiment and NOvA would extend the search by about an order of magnitude beyond the current limit. A secondary goal is to measure the dominant mode oscillation parameters, sin{sup 2}(2{theta}{sub 23}) and {Delta}m{sub 32}{sup 2} to a more precise level than previous experiments. Additional physics goals for NOvA are also discussed. Chapter 4 describes the Scientific Design Criteria which the Fermilab accelerator complex, NOvA detectors and NOvA detector sites must satisfy to meet the physics goals discussed in Chapter 3. Chapter 5 is an overview of the NOvA project. The changes in the design relative to the NOvA CDR are discussed. Chapter 6 summarizes the NOvA

  15. Shortest recurrence periods of novae

    SciTech Connect (OSTI)

    Kato, Mariko [Department of Astronomy, Keio University, Hiyoshi, Yokohama 223-8521 (Japan); Saio, Hideyuki [Astronomical Institute, Graduate School of Science, Tohoku University, Sendai 980-8578 (Japan); Hachisu, Izumi [Department of Earth Science and Astronomy, College of Arts and Sciences, The University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902 (Japan); Nomoto, Ken'ichi, E-mail: mariko@educ.cc.keio.ac.jp [Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

    2014-10-01

    Stimulated by the recent discovery of the 1 yr recurrence period nova M31N 2008-12a, we examined the shortest recurrence periods of hydrogen shell flashes on mass-accreting white dwarfs (WDs). We discuss the mechanism that yields a finite minimum recurrence period for a given WD mass. Calculating the unstable flashes for various WD masses and mass accretion rates, we identified a shortest recurrence period of about two months for a non-rotating 1.38 M {sub ?} WD with a mass accretion rate of 3.6 10{sup 7} M {sub ?} yr{sup 1}. A 1 yr recurrence period is realized for very massive (? 1.3 M {sub ?}) WDs with very high accretion rates (? 1.5 10{sup 7} M {sub ?} yr{sup 1}). We revised our stability limit of hydrogen shell burning, which will be useful for binary evolution calculations toward Type Ia supernovae.

  16. Spectra Nova Technologies Inc | Open Energy Information

    Open Energy Info (EERE)

    to: navigation, search Name: Spectra Nova Technologies Inc. Place: Ottawa, Ontario, Canada Zip: K2E 7J5 Sector: Solar Product: A Canadian based technology company, active in...

  17. Department

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

    This requirements review is organized by the Department of Energy's Office of Advanced Scientific Computing Research (ASCR) and the National Energy Research Scientific Computing ...

  18. Department

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

    . , Department of Energy Washington, DC 20585 FEB 102014 Dear Colleague: We would like to invite you to participate in a Pro'gram Requirements Review entitled "Large Scale...

  19. NOVA Portal: Submit VASP Jobs to Carver via the Web

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

    NOVA Portal: Submit VASP Jobs to Carver via the Web NOVA Portal: Submit VASP Jobs to Carver via the Web May 11, 2012 by Francesca Verdier NOVA is an experimental web application that enables users to submit VASP jobs to NERSC resources. You must be a licensed VASP user in order to submit jobs through NOVA. This initial version of NOVA runs only on Carver. Most input files can be prepared either by manipulating graphical controls, or by copying and pasting text and editing in the browser. NOVA

  20. Department

    Office of Legacy Management (LM)

    u.s. Department of the Interior U.S. Geological Survey Analysis of Borehole-Radar Reflection Logs from Selected HC Boreholes at the Project Shoal Area, Churchill County, Nevada By John W. Lane, Jr., Peter K. Joesten, Greg Pohll, and Todd Mihevic Water-Resources Investigations Report 01-4014 Prepared in cooperation with the U.S. Department of Energy Storrs, Connecticut 2001 U.S. DEPARTMENT OF THE INTERIOR GALE A. NORTON, Secretary U.S. GEOLOGICAL SURVEY Charles G. Groat, Director The use of firm,

  1. Department

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

    Director, Office of Hearings and Appeals (HG-1), U.S. Department of Energy, L'Enfant Plaza Building, 1000 Independence Avenue SW, Washington, D.C. 20585-1615, and shall be filed...

  2. Department

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

    be made in writing to the Director, Office of Hearings and Appeals (HG-1), L'Enfant Plaza Building, US. Department of Energy, 1000 Independence Avenue SW, Washington, D.C....

  3. Department

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

    for High Energy Physics" on November 12-13,2009, in the Washington, DC, area. This workshop is organized by the Department of Energy's Offices of High Energy Physics (HEP) and ...

  4. Fermilab | Newsroom | Press Releases | March 2013: NOvA Photos

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

    NOvA collaboration. Med Res | Hi Res The NOvA detector, currently under construction in Ash River, Minn., stands about 50 feet tall and 50 feet wide. The completed detector will...

  5. Fermilab | Newsroom | Press Releases | February 2014: NOvA Images

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

    NOvA collaboration Med Res | Hi Res The NOvA detector, currently under construction in Ash River, Minn., stands about 50 feet tall and 50 feet wide. The completed detector will...

  6. Vis Nova Trading GmbH | Open Energy Information

    Open Energy Info (EERE)

    Nova Trading GmbH Jump to: navigation, search Name: Vis Nova Trading GmbH Place: Bremen, Germany Zip: 28217 Product: Germany-based producer and trader of wood pellets....

  7. HelioNova S L | Open Energy Information

    Open Energy Info (EERE)

    HelioNova S L Jump to: navigation, search Name: HelioNova S.L. Place: Santiago de Compostela, Spain Zip: 15890 Sector: Renewable Energy Product: HELIONOVA develops and...

  8. Department

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

    Richland Operations Office . P.O. Box 550 Richland, Washington 99352 May 17,2010 Certified Mail Mr. Glenn Draper Bergman Draper & Frockt 614 First Avenue, Third Floor Seattle, Washington 98 I 04 Dear Mr. Draper: FREEDOM OF INFORMATION ACT REQUEST (FOI 2010-01224) You requested, pursuant to the Freedom of Information Act (FOIA), "copies of contracts entered into between Burns & Roe Industrial Services, Burns & Roe Pacific Incorporated and the Department of Energy-Hanford Nuclear

  9. Department

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

    Nuclear Physics," on May 26-27,2011, in Bethesda, MD (Washington, DC area). This workshop is organized by the Department of Energy's Offices of Nuclear Physics (NP) and Advanced Scientific Computing Research (ASCR). The workshop's goal is to characterize NP production computing requirements over the next 3 - 5 years at NERSC,the National Energy Research Scientific Computing Center. NERSCis the principal provider of production High Performance Computing (HPC) facilities and services for the

  10. NOvA: Exploring Neutrino Mysteries

    ScienceCinema (OSTI)

    Vahle, Tricia; Messier, Mark

    2014-08-12

    Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers.

  11. The NOvA simulation chain

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

    Aurisano, A.; Backhouse, C.; Hatcher, R.; Mayer, N.; Musser, J.; Patterson, R.; Schroeter, R.; Sousa, A.

    2015-12-23

    The NOvA experiment is a two-detector, long-baseline neutrino experiment operating in the recently upgraded NuMI muon neutrino beam. Simulating neutrino interactions and backgrounds requires many steps including: the simulation of the neutrino beam flux using FLUKA and the FLUGG interface, cosmic ray generation using CRY, neutrino interaction modeling using GENIE, and a simulation of the energy deposited in the detector using GEANT4. To shorten generation time, the modeling of detector-specific aspects, such as photon transport, detector and electronics noise, and readout electronics, employs custom, parameterized simulation applications. We will describe the NOvA simulation chain, and present details on the techniquesmore » used in modeling photon transport near the ends of cells, and in developing a novel data-driven noise simulation. Due to the high intensity of the NuMI beam, the Near Detector samples a high rate of muons originating in the surrounding rock. In addition, due to its location on the surface at Ash River, MN, the Far Detector collects a large rate ((˜) 140 kHz) of cosmic muons. Furthermore, we will discuss the methods used in NOvA for overlaying rock muons and cosmic ray muons with simulated neutrino interactions and show how realistically the final simulation reproduces the preliminary NOvA data.« less

  12. THE DWARF NOVA OUTBURSTS OF NOVA HER 1960 (=V446 HER)

    SciTech Connect (OSTI)

    Honeycutt, R. K.; Robertson, J. W.; Kafka, S. E-mail: jrobertson@atu.edu

    2011-04-15

    V446 Her is the best example of an old nova which has developed dwarf nova (DN) eruptions in the post-nova state. We report on observed properties of the long-term light curve of V446 Her, using photometry over 19 years. Yearly averages of the outburst (OB) magnitudes show a decline of {approx}0.013 mag yr{sup -1}, consistent with the decline of other post-novae that do not have DN OBs. Previous suggestions of bimodal distributions of the amplitudes and widths of the OBs are confirmed. The OBs occur at a mean spacing of 18 days but the range of spacings is large (13-30 days). From simulations of DN OBs, it has been predicted that the OB spacing in V446 Her will increase as M-dot from the red dwarf companion slowly falls following the nova; however, the large intrinsic scatter in the spacings serves to hide any evidence of this effect. We do find a systematic change in the OB pattern in which the brighter, wider type of OBs disappeared after late 2003, and this phenomenon is suggested to be due to falling M-dot following the nova.

  13. NOVA Making Stuff Season 2

    SciTech Connect (OSTI)

    Leombruni, Lisa; Paulsen, Christine Andrews

    2014-12-12

    Over the course of four weeks in fall 2013, 11.7 million Americans tuned in to PBS to follow host David Pogue as he led them in search of engineering and scientific breakthroughs poised to change our world. Levitating trains, quantum computers, robotic bees, and bomb-detecting plants—these were just a few of the cutting-edge innovations brought into the living rooms of families across the country in NOVA’s four-part series, Making Stuff: Faster, Wilder, Colder, and Safer. Each of the four one-hour programs gave viewers a behind-the-scenes look at novel technologies poised to change our world—showing them how basic research and scientific discovery can hold the keys to transforming how we live. Making Stuff Season 2 (MS2) combined true entertainment with educational value, creating a popular and engaging series that brought accessible science into the homes of millions. NOVA’s goal to engage the public with such technological innovation and basic research extended beyond the broadcast series, including a variety of online, educational, and promotional activities: original online science reporting, web-only short-form videos, a new online quiz-game, social media engagement and promotion, an educational outreach “toolkit” for science educators to create their own “makerspaces,” an online community of practice, a series of nationwide Innovation Cafés, educator professional development, a suite of teacher resources, an “Idealab,” participation in national conferences, and specialized station relation and marketing. A summative evaluation of the MS2 project indicates that overall, these activities helped make a significant impact on the viewers, users, and participants that NOVA reached. The final evaluation conducted by Concord Evaluation Group (CEG) confidently concluded that the broadcast, website, and outreach activities were successful at achieving the project’s intended impacts. CEG reported that the MS2 series and website content were

  14. Department

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

    Ener9Y Richland Operations Office P.O. Box 550 Richland, Washington 99352 May 11,2010 Certified Mail Ms. Linda Lammendola Christie Pabarue Mortensen and Young 1880 John F. Kennedy Boulevard 10 th Floor Philadelphia, Pennsylvania 19103 Dear Ms. Larnmendola: FREEDOM OF INFORMATION ACT REQUEST (FOI 2010-01394) Your Freedom of Information Act (FOIA) request dated Apri121, 2010, addressed to the U.S. Department of Energy, Headquarters FOIA Office has been forwarded to this office for response and was

  15. Improved optical diagnostics for the NOVA laser

    SciTech Connect (OSTI)

    Fernandez, J.C.; Berggren, R.R.; Bradley, K.S.; Hsing, W.W.; Gomez, C.C.; Cobble, J.A.

    1994-07-01

    This paper describes three diagnostics for detecting optical scatter from NOVA laser targets. Detecting such scatter can help not only the authors` understanding of plasma instabilities in laser plasmas, but also their efforts at plasma characterization, particularly hohlraum plasmas. These diagnostics are: the Full Aperture Backscatter Station (FABS), presently being built; the Oblique Scatter Array (OSA), just starting operation; and the Axial Imager, also just starting operation. FABS will allow imaging at high resolution of Brillouin and Raman backscatter. The OSA allows a quantitative measurement of Brillouin and Raman scatter in many directions (assuming the target allows the scatter to escape). The axial imager allows high-resolution imaging of Brillouin, Two-Plasmon Decay and Raman scatter emitted towards the East direction, which is along the symmetry axis of the NOVA laser beams.

  16. Improved optical diagnostics for the NOVA laser

    SciTech Connect (OSTI)

    Fernandez, J.C.; Berggren, R.R.; Bradley, K.S.; Hsing, W.W.; Gomez, C.C.; Cobble, J.A.; Wilke, M.D. )

    1995-01-01

    This paper describes three diagnostics detecting optical scatter from NOVA laser targets. Detecting such scatter can help to understand instabilities in laser plasmas and to characterize such plasmas, particularly hohlraum plasmas. These diagnostics are the full aperture backscatter station (FABS), presently being built; the oblique scatter array (OSA), just starting operation; and the axial imager, also just starting operation. FABS will allow imaging at high resolution of Brillouin and Raman backscatter. The OSA provides a quantitative measurement of Brillouin and Raman scatter in many directions. The axial imager allows high-resolution imaging of Brillouin, two-plasmon decay and Raman scatter emitted toward the direction of the symmetry axis of the NOVA laser beams.

  17. Integration of the Super Nova early warning system with the NOvA Trigger

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

    Habig, Alec; Zirnstein, Jan

    2015-01-01

    The NOvA experiment, with a baseline of 810km, samples Fermilab’s upgraded NuMI beam with a Near Detector on-site and a Far Detector (FD) at Ash River, MN, to observe oscillations of muon neutrinos. The 344,064 liquid scintillator-filled cells of the 14 kton FD provide high granularity of a large detector mass and enable us to also study non-accelerator based neutrinos with our Data Driven Trigger framework. This paper will focus on the real time integration of the SNEWS with the NOvA Trigger where we have set up an XML-RPC based messaging system to inject the SNEWS signal directly into ourmore » trigger. In conclusion, this presents a departure from the E-Mail based notification mechanism used by SNEWS in the past and allows NOvA more control over propagation and transmission timing.« less

  18. Petra Nova - W.A. Parish Project | Department of Energy

    Office of Environmental Management (EM)

    The project will demonstrate Mitsubishi Heavy Industries' (MHI) CO2 capture technology at an existing coal-fired power plant. The project will demonstrate Mitsubishi Heavy ...

  19. Liquid Scintillator Production for the NOvA Experiment

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

    Mufson, S.; Baugh, B.; Bower, C.; Coan, T.; Cooper, J.; Corwin, L.; Karty, J.; Mason, P.; Messier, M. D.; Pla-Dalmau, A.; et al

    2015-04-15

    The NOvA collaboration blended and delivered 8.8 kt (2.72M gal) of liquid scintillator as the active detector medium to its near and far detectors. The composition of this scintillator was speci#12;cally developed to satisfy NOvA's performance requirements. A rigorous set of quality control procedures was put in place to verify that the incoming components and the blended scintillator met these requirements. The scintillator was blended commercially in Hammond, IN. The scintillator was shipped to the NOvA detectors using dedicated stainless steel tanker trailers cleaned to food grade.

  20. Liquid Scintillator Production for the NOvA Experiment

    SciTech Connect (OSTI)

    Mufson, S.; Baugh, B.; Bower, C.; Coan, T.; Cooper, J.; Corwin, L.; Karty, J.; Mason, P.; Messier, M. D.; Pla-Dalmau, A.; Proudfoot, M.

    2015-04-15

    The NOvA collaboration blended and delivered 8.8 kt (2.72M gal) of liquid scintillator as the active detector medium to its near and far detectors. The composition of this scintillator was specifically developed to satisfy NOvA's performance requirements. A rigorous set of quality control procedures was put in place to verify that the incoming components and the blended scintillator met these requirements. The scintillator was blended commercially in Hammond, IN. The scintillator was shipped to the NOvA detectors using dedicated stainless steel tanker trailers cleaned to food grade.

  1. Fermilab | Newsroom | Press Releases | October 6, 2014: NOvA...

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

    courtesy of Fermilab Med Res | Hi Res A view across the top of the NOvA far detector in Ash River, Minnesota. Electronics that make up part of the data acquisition system are...

  2. Nova Bio Fuels Pvt Ltd | Open Energy Information

    Open Energy Info (EERE)

    Pvt Ltd Jump to: navigation, search Name: Nova Bio Fuels Pvt. Ltd. Place: New Delhi, Delhi (NCT), India Zip: 110048 Product: New Delhi-based biofuel project developer. References:...

  3. Nova Alinca Agricola e Comercial | Open Energy Information

    Open Energy Info (EERE)

    Alinca Agricola e Comercial Jump to: navigation, search Name: Nova Alinca Agricola e Comercial Place: So Joaquim da Barra, Sao Paulo, Brazil Zip: 14.600-000 Product: Sao...

  4. Multi-Dimensional Modeling of Nova with Realistic Nuclear Physics

    SciTech Connect (OSTI)

    Zingale, M; Hoffman, R D

    2011-01-27

    This contract covered the period from 03/09/2010 to 09/30/2010. Over this period, we adapted the low Mach number hydrodynamics code MAESTRO to perform simulations of novae. A nova is the thermonuclear runaway of an accreted hydrogen layer on the surface of a white dwarf. As the accreted layer grows in mass, the temperature and density at the base increase to the point where hydrogen fusion can begin by the CNO cycle - a burning process that uses carbon, nitrogen, and oxygen to complete the fusion of four hydrogen nuclei into one helium-4 nucleus. At this point, we are running initial models of nova, exploring the details of the convection. In the follow-on contract to this one, we will continue this investigation.

  5. PW Vulpeculae - A nova with nearly solar abundances

    SciTech Connect (OSTI)

    Saizar, P.; Ferland, G.J.; Wagner, R.M.; Starrfield, S.; Truran, J.W. Arizona State Univ., Tempe Illinois Univ., Urbana )

    1991-01-01

    Optical spectrophotometry of PW Vulpeculae is combined with ultraviolet data to estimate electron temperatures, densities, and abundances in the ejecta of this slow classical nova. The reddening, the distance, and the evolution of the ultraviolet spectrum are discussed. Abundances are nearly solar, with the exception of nitrogen, which is substantially higher. Although neon has been reported to be enhanced in several novae, it does not seem to be the case for PW Vul. Photoionization model calculations of the ejecta that give a reasonable match of the observed emission spectrum are presented. A strong featureless continuum shows that very hot, presumably shock-heated, gas plays a major role in determining the energetics of this nova. Emission from this hot gas is responsible for the ionization of the nebular gas. A calculation of the masses of both the hot coronal gas and the cooler nebular gas shows that the former may account for most of the mass of the ejecta. 32 refs.

  6. NOvA: Building a Next Generation Neutrino Experiment

    ScienceCinema (OSTI)

    Perko, John; Williams, Ron; Miller, Bill;

    2014-05-30

    The NOvA neutrino experiment is searching for the answers to some of the most fundamental questions of the universe. This video documents how collaboration between government research institutions like Fermilab, academia and industry can create one of the largest neutrino detectors in the world.

  7. SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

    SciTech Connect (OSTI)

    Schwarz, Greg J.; Ness, Jan-Uwe; Osborne, J. P.; Page, K. L.; Evans, P. A.; Beardmore, A. P.; Walter, Frederick M.; Andrew Helton, L.; Woodward, Charles E.; Bode, Mike; Starrfield, Sumner; Drake, Jeremy J.

    2011-12-01

    The Swift gamma-ray burst satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the X-Ray Telescope (0.3-10 keV) instrument count rates and the UltraViolet and Optical Telescope (1700-8000 A) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with Super Soft X-ray emission, 19 from Swift observations. The data set shows that the faster novae have an early hard X-ray phase that is usually missing in slower novae. The Super Soft X-ray phase occurs earlier and does not last as long in fast novae compared to slower novae. All the Swift novae with sufficient observations show that novae are highly variable with rapid variability and different periodicities. In the majority of cases, nuclear burning ceases less than three years after the outburst begins. Previous relationships, such as the nuclear burning duration versus t{sub 2} or the expansion velocity of the eject and nuclear burning duration versus the orbital period, are shown to be poorly correlated with the full sample indicating that additional factors beyond the white dwarf mass and binary separation play important roles in the evolution of a nova outburst. Finally, we confirm two optical phenomena that are correlated with strong, soft X-ray emission which can be used to further increase the efficiency of X-ray campaigns.

  8. AT Cnc: A SECOND DWARF NOVA WITH A CLASSICAL NOVA SHELL (Journal...

    Office of Scientific and Technical Information (OSTI)

    Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, ... Country of Publication: United States Language: English Subject: 79 ...

  9. NOVA NERSC's Online VASP Application Annette Greiner Shreyas Cholia

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

    NOVA NERSC's Online VASP Application Annette Greiner Shreyas Cholia 0 10 20 30 40 50 60 70 80 90 VASP Gaussian Quantum Espresso NWChem LAMMPS NAMD NIMROD WRF CPMD Codes Used by the Most Projects at NERSC Number of Projects as of Sep 2010 Why VASP? Why run VASP in a browser? Making interacting with HPC more efficient * Error checking * Organizing and retrieving jobs * Real-time job monitoring * Integrated analysis tools * Integration with other online tools * Meaningful UI controls VASP with a

  10. Intial performance from the NOvA surface prototype detector

    SciTech Connect (OSTI)

    Muether, M.; ,

    2011-09-01

    NOvA, the NuMI Off-Axis {nu}{sub e} Appearance experiment, will study {nu}{sub {mu}} {yields} {nu}{sub e} oscillations characterized by the mixing angle {Theta}{sub 13}. Provided {Theta}{sub 13} is large enough, NOvA may ultimately determine the ordering of the neutrino masses and measure CP violation in neutrino oscillations. A complementary pair of detectors will be constructed {approx}14 mrad off beam axis to optimize the energy profile of the neutrinos. This system consists of a surface based 14 kTon liquid scintillator tracking volume located 810 km from the main injector source (NuMI) in Ash River, Minnesota and a smaller underground 222 Ton near detector at the Fermilab. The first neutrino signals at the Ash River Site are expected prior to the 2012 accelerator shutdown. In the meantime, a near detector surface prototype has been completed and neutrinos from two Fermilab sources have been observed using the same highly segmented PVC and liquid scintillator detector system that will be deployed in the full scale experiment. Design and initial performance characteristics of this prototype system are being fed back into the design for the full NOvA program.

  11. THE DUSTY NOVA V1065 CENTAURI (NOVA CEN 2007): A SPECTROSCOPIC ANALYSIS OF ABUNDANCES AND DUST PROPERTIES

    SciTech Connect (OSTI)

    Helton, L. Andrew; Woodward, Charles E.; Gehrz, Robert D.; Walter, Frederick M.; Vanlandingham, Karen; Schwarz, Greg J.; Evans, Aneurin; Ness, Jan-Uwe; Geballe, Thomas R.; Greenhouse, Matthew; Krautter, Joachim; Liller, William; Lynch, David K.; Rudy, Richard J.; Shore, Steven N.; Starrfield, Sumner; Truran, Jim

    2010-11-15

    We examine the ejecta evolution of the classical nova V1065 Centauri, constructing a detailed picture of the system based on spectrophotometric observations obtained from 9 to approximately 900 days post-outburst with extensive coverage from optical to mid-infrared wavelengths. We estimate a reddening toward the system of E(B-V) = 0.5 {+-} 0.1, based upon the B - V color and analysis of the Balmer decrement, and derive a distance estimate of 8.7{sup +2.8}{sub -2.1} kpc. The optical spectral evolution is classified as P {sup o}{sub fe} N{sub ne} A{sub o} according to the CTIO Nova Classification system of Williams et al. Photoionization modeling yields absolute abundance values by number, relative to solar of He/H = 1.6 {+-} 0.3, N/H = 144 {+-} 34, O/H = 58 {+-} 18, and Ne/H = 316 {+-} 58 for the ejecta. We derive an ejected gas mass of M{sub g} = (1.6 {+-} 0.2) x 10{sup -4} M{sub sun}. The infrared excess at late epochs in the evolution of the nova arises from dust condensed in the ejecta composed primarily of silicate grains. We estimate a total dust mass, M{sub d} , of order (0.2-3.7) x 10{sup -7} M{sub sun}, inferred from modeling the spectral energy distribution observed with the Spitzer IRS and Gemini-South GNIRS spectrometers. Based on the speed class, neon abundance, and the predominance of silicate dust, we classify V1065 Cen as an ONe-type classical nova.

  12. ON THE PROGENITORS OF LOCAL GROUP NOVAE. I. THE M31 CATALOG

    SciTech Connect (OSTI)

    Williams, S. C.; Darnley, M. J.; Bode, M. F.; Keen, A.; Shafter, A. W.

    2014-07-01

    We report the results of a survey of M31 novae in quiescence. This is the first catalog of extragalactic systems in quiescence to be published, and contains data for 38 spectroscopically confirmed novae from 2006 to 2012. We used Liverpool Telescope images of each nova during eruption to define an accurate position for each system. These positions were then matched to archival Hubble Space Telescope (HST) images and we performed photometry on any resolved objects that were coincident with the eruption positions. The survey aimed to detect quiescent systems with red giant secondaries, as only these, along with a few systems with bright sub-giant secondaries, will be resolvable in the HST images. There are only a few confirmed examples of such red giant novae in our Galaxy, the majority of which are recurrent novae. However, we find that a relatively high percentage of the nova eruptions in M31 may occur in systems containing red giant secondaries. Of the 38 systems in this catalog, 11 have a progenitor candidate whose probability of being a coincidental alignment is less than 5%. We show that at the 3? limit, up to only 2 of these 11 systems may be due to chance alignments, leading to an estimate of the M31 nova population with evolved secondaries of up to 24%, compared to the ?3% seen Galactically. Such an elevated proportion of nova systems with evolved secondaries may imply the presence of a much larger population of recurrent novae than previously thought. This would have considerable impact, particularly with regards to their potential as Type Ia supernova progenitors. Additionally, for several novae, serendipitous HST images had been taken when the nova was still fading; this allowed us to produce light curves that go fainter than is usually achievable for most extragalactic systems. Finally, as this survey is astrometric in nature, we also update the position of each nova in the catalog.

  13. Detecting Neutrinos with the NOvA Detectors (Other) | SciTech...

    Office of Scientific and Technical Information (OSTI)

    PARTICLES AND FIELDS NOVA; NEUTRINO; NEUTRINO DETECTOR; DETECTOR; COSMIC RAY; NEUTRINO INTERACTION Word Cloud More Like This Multimedia File size NAView Multimedia View Multimedia...

  14. A LIGHT CURVE ANALYSIS OF CLASSICAL NOVAE: FREE-FREE EMISSION VERSUS PHOTOSPHERIC EMISSION

    SciTech Connect (OSTI)

    Hachisu, Izumi; Kato, Mariko E-mail: mariko@educ.cc.keio.ac.jp

    2015-01-10

    We analyzed light curves of seven relatively slower novae, PW Vul, V705 Cas, GQ Mus, RR Pic, V5558 Sgr, HR Del, and V723 Cas, based on an optically thick wind theory of nova outbursts. For fast novae, free-free emission dominates the spectrum in optical bands rather than photospheric emission, and nova optical light curves follow the universal decline law. Faster novae blow stronger winds with larger mass-loss rates. Because the brightness of free-free emission depends directly on the wind mass-loss rate, faster novae show brighter optical maxima. In slower novae, however, we must take into account photospheric emission because of their lower wind mass-loss rates. We calculated three model light curves of free-free emission, photospheric emission, and their sum for various white dwarf (WD) masses with various chemical compositions of their envelopes and fitted reasonably with observational data of optical, near-IR (NIR), and UV bands. From light curve fittings of the seven novae, we estimated their absolute magnitudes, distances, and WD masses. In PW Vul and V705 Cas, free-free emission still dominates the spectrum in the optical and NIR bands. In the very slow novae, RR Pic, V5558 Sgr, HR Del, and V723 Cas, photospheric emission dominates the spectrum rather than free-free emission, which makes a deviation from the universal decline law. We have confirmed that the absolute brightnesses of our model light curves are consistent with the distance moduli of four classical novae with known distances (GK Per, V603 Aql, RR Pic, and DQ Her). We also discussed the reason why the very slow novae are about ∼1 mag brighter than the proposed maximum magnitude versus rate of decline relation.

  15. Equation of State measurements of hydrogen isotopes on Nova

    SciTech Connect (OSTI)

    Collins, G. W., LLNL

    1997-11-01

    High intensity lasers can be used to perform measurements of materials at extremely high pressures if certain experimental issues can be overcome. We have addressed those issues and used the Nova laser to shock-compress liquid deuterium and obtain measurements of density and pressure on the principal Hugoniot at pressures from 300 kbar to more than 2 Mbar. The data are compared with a number of equation of state models. The data indicate that the effect of molecular dissociation of the deuterium into a monatomic phase may have a significant impact on the equation of state near 1 Mbar.

  16. NOvA (Fermilab E929) Official Plots and Figures

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    The NOvA collaboration, consisting of 180 researchers across 28 institutions and managed by the Fermi National Accelerator Laboratory (FNAL), is developing instruments for a neutrino-focused experiment that will attempt to answer three fundamental questions in neutrino physics: 1) Can we observe the oscillation of muon neutrinos to electron neutrinos; 2) What is the ordering of the neutrino masses; and 3) What is the symmetry between matter and antimatter? The collaboration makes various data plots and figures available. These are grouped under five headings, with brief descriptions included for each individual figure: Neutrino Spectra, Detector Overview, Theta12 Mass Hierarchy CP phase, Theta 23 Delta Msqr23, and NuSterile.

  17. NOVA-NREL Optimal Vehicle Acquisition Analysis (Brochure)

    SciTech Connect (OSTI)

    Blakley, H.

    2011-03-01

    Federal fleet managers face unique challenges in accomplishing their mission - meeting agency transportation needs while complying with Federal goals and mandates. Included in these challenges are a variety of statutory requirements, executive orders, and internal goals and objectives that typically focus on petroleum consumption and greenhouse gas (GHG) emissions reductions, alternative fuel vehicle (AFV) acquisitions, and alternative fuel use increases. Given the large number of mandates affecting Federal fleets and the challenges faced by all fleet managers in executing day-to-day operations, a primary challenge for agencies and other organizations is ensuring that they are as efficient as possible in using constrained fleet budgets. An NREL Optimal Vehicle Acquisition (NOVA) analysis makes use of a mathematical model with a variety of fleet-related data to create an optimal vehicle acquisition strategy for a given goal, such as petroleum or GHG reduction. The analysis can helps fleets develop a vehicle acquisition strategy that maximizes petroleum and greenhouse gas reductions.

  18. 1

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

    Cirrus Horizontal Inhomogeneity and OLR Bias Q. Fu and B. Carlin Department of Oceanography Dalhousie University Halifax, Nova Scotia Canada G. G. Mace Department of Meteorology University of Utah Salt Lake City, Utah Introduction Clouds exhibit dramatic variabilities at spatial scales smaller than typical grid cells of large-scale models used to study climate and weather. These unresolved cloud fluctuations are potentially important for parameterizations of both cloud radiative effects and

  19. Fermilab | Newsroom | Press Releases | August 7, 2015: NOvA Images

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

    Fermilab Med Res | Hi Res A view across the top of the NOvA far detector in Ash River, Minnesota. Electronics that make up part of the data acquisition system are...

  20. Dept. of Energy/NOVA announce re-airing on Oct. 16 of special...

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

    Dept. of EnergyNOVA announce re-airing on Oct. 16 of special program: Einstein's Big Idea Dept. of Energy... the nation and its communities through education and public outreach. ...

  1. Jefferson Lab News -Dept. of Energy co-sponsors Oct. 11th NOVA...

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

    Dept. of Energy co-sponsors Oct. 11th NOVA program: Einstein's Big Idea Dept. of Energy ... to serve the nation and its communities through education and public outreach. ...

  2. Usina Nova Uni o S A A car e lcool | Open Energy Information

    Open Energy Info (EERE)

    o S A A car e lcool Jump to: navigation, search Name: Usina Nova Unio SA Acar e lcool Place: Serrana, Sao Paulo, Brazil Zip: 14150-000 Product: Brazil based...

  3. Petra Nova Project Breaks Ground on World’s Largest Post-Combustion Carbon Capture Project

    Office of Energy Efficiency and Renewable Energy (EERE)

    The Houston-area Petra Nova project is designed to capture 1.4 million tons of CO2 per year -- making it the world's largest post-combustion carbon capture facility.

  4. Natural Gas Weekly Update, Printer-Friendly Version

    Gasoline and Diesel Fuel Update (EIA)

    Database. Row and column sums may not equal totals due to independent rounding. Other Market Trends: Report on Nova Scotia Natural Gas Reserves: According to a report...

  5. Property:Incentive/ContFax | Open Energy Information

    Open Energy Info (EERE)

    Regulations: No.27 - Control of Nitrogen Oxide Emissions (Rhode Island) + 401-222-2017 + Air Quality (Nova Scotia, Canada) + (902) 424-0503 + Air Quality Approvals and Permits...

  6. Better Buildings Residential Network Peer Exchange Call Series...

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

    Call Slides and Discussion Summary Call Participants Residential Network Members District of Columbia Sustainable Energy Utility Efficiency Nova Scotia Elevate Energy ...

  7. Pulsed power supply for Nova Upgrade. Final report, August 1, 1991 to March 31, 1992

    SciTech Connect (OSTI)

    Bacon, J.L.; Kajs, J.P.; Walls, A.; Weldon, W.F.; Zowarka, R.C.

    1992-12-31

    This report describes work carried out at the Center for Electromechanics at The University of Texas at Austin (CEM-UT). A baseline design of the Nova Upgrade has been completed by Lawrence Livermore National Laboratory. The Nova Upgrade is an 18 beamline Nd: glass laser design utilizing fully relayed 4x4 30 cm aperture segmented optical components. The laser thus consists of 288 independent beamlets nominally producing 1.5 to 2.0 MJ of 0.35 {mu}m light in a 3 to 5 ns pulse. The laser design is extremely flexible and will allow a wide range of pulses to irradiate ICF targets. This facility will demonstrate ignition/gain and the scientific feasibility of ICF for energy and defense applications. The pulsed power requirements for the Nova Upgrade are given. CEM-UT was contracted to study and develop a design for a homopolar generator/inductor (HPG/inductor) opening switch system which would satisfy the pulsed power supply requirements of the Nova Upgrade. The Nd:glass laser amplifiers used in the Nova Upgrade will be powered by light from xenon flashlamps. The pulsed power supply for the Nova Upgrade powers the xenon flashlamps. This design and study was for a power supply to drive flashlamps.

  8. Modeling of Nova indirect drive Rayleigh--Taylor experiments

    SciTech Connect (OSTI)

    Weber, S.V.; Remington, B.A.; Haan, S.W.; Wilson, B.G.; Nash, J.K. )

    1994-11-01

    The growth due to the Rayleigh--Taylor (RT) instability of single-wavelength surface perturbations on planar foils of brominated CH [CH(Br)] and fluorosilicone (FS) was measured. The foils were accelerated by x-ray ablation with temporally shaped drive pulses. A range of initial amplitudes ([ital a][sub 0]) and wavelengths ([lambda]) have been used. This paper focuses upon foils with small [ital a][sub 0]/[lambda], which exhibit substantial growth in the linear regime, and are most sensitive to the calculated growth rate. The CH(Br) foils exhibit slower RT perturbation growth because opacity differences result in a larger ablation velocity and a longer density scale length than for FS. Tabulated opacities from detailed atomic models, OPAL [Astrophys. J. [bold 397], 717 (1992)] and super transition array (STA) [Phys. Rev. A [bold 40], 3183 (1989)] were employed. Unlike previous simulations which employed the average atom (XSN) opacity treatment, parameter adjustments to fit experimental data no longer appear necessary. Nonlocal thermodynamic equilibrium (NLTE) effects do not appear to be important. Other variables which may affect the modeling, such as changes of the equation of state and radiation drive spectrum, were also examined. The current calculational model, which incorporates physically justified choices for these calculational ingredients, agrees with the Nova single wavelength RT perturbation growth data.

  9. Nova-like cataclysmic variables in the infrared

    SciTech Connect (OSTI)

    Hoard, D. W.; Long, Knox S.; Howell, Steve B.; Wachter, Stefanie; Brinkworth, Carolyn S.; Knigge, Christian; Drew, J. E.; Szkody, Paula; Kafka, S.; Belle, Kunegunda; Ciardi, David R.; Froning, Cynthia S.; Van Belle, Gerard T.; Pretorius, M. L.

    2014-05-01

    Nova-like (NL) cataclysmic variables have persistently high mass transfer rates and prominent steady state accretion disks. We present an analysis of infrared observations of 12 NLs obtained from the Two Micron All Sky Survey, the Spitzer Space Telescope, and the Wide-field Infrared Survey Explorer All Sky Survey. The presence of an infrared excess at ? ? 3-5 ?m over the expectation of a theoretical steady state accretion disk is ubiquitous in our sample. The strength of the infrared excess is not correlated with orbital period, but shows a statistically significant correlation (but shallow trend) with system inclination that might be partially (but not completely) linked to the increasing view of the cooler outer accretion disk and disk rim at higher inclinations. We discuss the possible origin of the infrared excess in terms of emission from bremsstrahlung or circumbinary dust, with either mechanism facilitated by the mass outflows (e.g., disk wind/corona, accretion stream overflow, and so on) present in NLs. Our comparison of the relative advantages and disadvantages of either mechanism for explaining the observations suggests that the situation is rather ambiguous, largely circumstantial, and in need of stricter observational constraints.

  10. SWIFT X-RAY AND ULTRAVIOLET MONITORING OF THE CLASSICAL NOVA V458 VUL (NOVA VUL 2007)

    SciTech Connect (OSTI)

    Ness, J.-U. [European Space Astronomy Centre, P.O. Box 78, 28691 Villanueva de la Canada, Madrid (Spain); Drake, J. J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Beardmore, A. P.; Evans, P. A.; Osborne, J. P.; Page, K. L. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Boyd, D. [BAA VSS, 5 Silver Lane, West Challow, Wantage, OX12 9TX (United Kingdom); Bode, M. F. [Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD (United Kingdom); Brady, S. [AAVSO, 5 Melba Drive, Hudson, NH 03051 (United States); Gaensicke, B. T.; Steeghs, D. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Kitamoto, S.; Takei, D. [Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501 (Japan); Knigge, C. [School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom); Miller, I. [BAA VSS, Furzehill House, Ilston, Swansea SA2 7LE (United Kingdom); Rodriguez-Gil, P. [Isaac Newton Group, PO Ap. de Correos 321, 38700 Sta. Cruz de la Palma (Spain); Schwarz, G. [Department of Geology and Astronomy, West Chester University, West Chester, PA 19383 (United States); Staels, B. [CBA Flanders, Alan Guth Observatory, Koningshofbaan 51, Hofstade, Aalst (Belgium); Tsujimoto, M. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Wesson, R. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom)], E-mail: juness@sciops.esa.int (and others)

    2009-05-15

    We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vul became a variable hard X-ray source due to optically thin thermal emission at kT = 0.64 keV with an X-ray band unabsorbed luminosity of 2.3 x 10{sup 34} erg s{sup -1} during days 71-140. The X-ray spectrum at this time requires a low Fe abundance (0.2{sup +0.3} {sub -0.1} solar), consistent with a Suzaku measurement around the same time. On day 315 we find a new X-ray spectral component which can be described by a blackbody with temperature of kT = 23{sup +9} {sub -5} eV, while the previous hard X-ray component has declined by a factor of 3.8. The spectrum of this soft X-ray component resembles those typically seen in the class of supersoft sources (SSS) which suggests that the nova ejecta were starting to clear and/or that the white dwarf photosphere is shrinking to the point at which its thermal emission reaches into the X-ray band. We find a high degree of variability in the soft component with a flare rising by an order of magnitude in count rate in 0.2 days. In the following observations on days 342.4-383.6, the soft component was not seen, only to emerge again on day 397. The hard component continued to evolve, and we found an anticorrelation between the hard X-ray emission and the UV emission, yielding a Spearman rank probability of 97%. After day 397, the hard component was still present, was variable, and continued to fade at an extremely slow rate but could not be analyzed owing to pile-up contamination from the bright SSS component.

  11. chin-98.pdf

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

    5 A Diagnostic Study on Retrieving Bulk Microphysical Properties of Low-Level Stratiform Clouds and Its Implication on Climate Research H.-N. S. Chin, D. J. Rodriguez, R. T. Cederwall, C. C. Chuang, A. S. Grossman, and J. J. Yio Atmospheric Science Division Lawrence Livermore National Laboratory Livermore, California Q. Fu Departments of Oceanography and Physics Dalhousie University Halifax, Nova Scotia, Canada M. A. Miller Division of Applied Science Brookhaven National Laboratory Upton, New

  12. 1

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

    Light Scattering and Absorption by Spherical Particles in an Absorbing Medium Q. Fu and W. B. Sun Department of Oceanography Dalhousie University Halifax, Nova Scotia Canada Introduction Light scattering and absorption by spherical particles in an absorbing medium occur in the earth- atmosphere system. Some examples are light scattering by cloud particles surrounded by the water vapor in the atmosphere, by biological particles in the ocean, and by air bubbles in the ocean and sea ice. It is

  13. 1

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

    Five Years of Clear-Sky Solar Radiation Measurements and Aerosol Forcing at the SGP ARM Site G. Lesins and Q. Fu Department of Oceanography Dalhousie University Halifax, Nova Scotia Canada Introduction The Atmospheric Radiation Measurement (ARM) Program Southern Great Plains (SGP) Cloud and Radiation Testbed (CART) site has been collecting high-quality surface radiative flux measurements for over five years. The array of radiometers and other atmospheric instrumentation provides an excellent

  14. THE INTER-ERUPTION TIMESCALE OF CLASSICAL NOVAE FROM EXPANSION...

    Office of Scientific and Technical Information (OSTI)

    Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, ... Country of Publication: United States Language: English Subject: 79 ...

  15. Using near detector(s) to predict the far detector events in NOvA experiment

    SciTech Connect (OSTI)

    Djurcic, Zelimir; /Argonne

    2011-01-01

    The NOvA experiment is designed to search for a non-vanishing mixing angle {theta}{sub 13} with unprecedented sensitivity and has the potential to resolve the neutrino mass hierarchy and constrain CP-violation phase. NOvA will use two functionally identical detectors at near and far locations to eliminate sensitivity to modeling of neutrino flux and cross-sections. The near detector will measure neutrino rate to constrain backgrounds expected in the far detector which will search for appearance of electron neutrinos and/or anti-neutrinos using Fermilab NuMI neutrino beam. This report describes initial thoughts on how the available beams and detectors may be used to reach the NOvA goals.

  16. Construction of AC Motor Controllers for NOvA Experiment Upgrades

    SciTech Connect (OSTI)

    Cooley, Patrick; ,

    2011-08-04

    I have been constructing Alternating Current (AC) motor controllers for manipulation of particle beam detectors. The capability and reliability of these motor controllers are essential to the Laboratory's mission of accurate analysis of the particle beam's position. The device is moved in and out of the beam's path by the motor controller followed by the Neutrinos at the Main Injector Off-Axis {nu}{sub e} Appearance (NOvA) Experiment further down the beam pipe. In total, I built and tested ten ac motor controllers for new beam operations in the NOvA experiment. These units will prove to be durable and provide extremely accurate beam placement for NOvA Experiment far into the future.

  17. Integration of the Super Nova Early Warning System with the NO$\

    SciTech Connect (OSTI)

    Habig, Alec; Zirnstein, Jan

    2015-12-23

    The NOvA experiment, with a baseline of 810km, samples Fermilab’s upgraded NuMI beam with a Near Detector on-site and a Far Detector (FD) at Ash River, MN, to observe oscillations of muon neutrinos. The 344,064 liquid scintillator-filled cells of the 14 kton FD provide high granularity of a large detector mass and enable us to also study non-accelerator based neutrinos with our Data Driven Trigger framework. This paper will focus on the real time integration of the SNEWS with the NOvA Trigger where we have set up an XML-RPC based messaging system to inject the SNEWS signal directly into our trigger. This presents a departure from the E-Mail based notification mechanism used by SNEWS in the past and allows NOvA more control over propagation and transmission timing.

  18. RAPID DUST FORMATION IN NOVAE: THE SPEED CLASSFORMATION TIMESCALE CORRELATION EXPLAINED

    SciTech Connect (OSTI)

    Williams, S. C.; Bode, M. F.; Darnley, M. J.; Evans, A.; Zubko, V.; Shafter, A. W.

    2013-11-10

    Observations show that the time of onset of dust formation in classical novae depends strongly on their speed class, with dust typically taking longer to form in slower novae. Using empirical relationships between speed class, luminosity and ejection velocity, it can be shown that dust formation timescale is expected to be essentially independent of speed class. However, following a nova outburst the spectrum of the central hot source evolves, with an increasing proportion of the radiation being emitted short-ward of the Lyman limit. The rate at which the spectrum evolves also depends on the speed class. We have therefore refined the simple model by assuming photons at energies higher than the Lyman limit are absorbed by neutral hydrogen gas internal to the dust formation sites, therefore preventing these photons reaching the nucleation sites. With this refinement the dust formation timescale is theoretically dependent on speed class and the results of our theoretical modification agree well with the observational data. We consider two types of carbon-based dust, graphite and amorphous carbon, with both types producing similar relationships. Our results can be used to predict when dust will form in a nova of a given speed class and hence when observations should optimally be taken to detect the onset of dust formation.

  19. Isospin mixing reveals 30P(p, γ)31S resonance influencing nova nucleosynthesis

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

    Bennett, M. B.; Wrede, C.; Brown, B. A.; Liddick, S. N.; Perez-Loureiro, D.; Bardayan, D. W.; Chen, A. A.; Chipps, K. A.; Fry, C.; Glassman, B. E.; et al

    2016-03-08

    Here, the thermonuclear 30P(p, γ)31S reaction rate is critical for modeling the final elemental and isotopic abundances of ONe nova nucleosynthesis, which affect the calibration of proposed nova thermometers and the identification of presolar nova grains, respectively. Unfortunately, the rate of this reaction is essentially unconstrained experimentally, because the strengths of key 31S proton capture resonance states are not known, largely due to uncertainties in their spins and parities. Using the β decay of 31Cl, we have observed the β-delayed γ decay of a 31S state at Ex = 6390.2(7) keV, with a 30P(p, γ)31S resonance energy of Er =more » 259.3(8) keV, in the middle of the 30P(p, γ)31S Gamow window for peak nova temperatures. This state exhibits isospin mixing with the nearby isobaric analog state at Ex = 6279.0(6) keV, giving it an unambiguous spin and parity of 3/2+ and making it an important l = 0 resonance for proton capture on 30P.« less

  20. Serendipitous discovery of a dwarf Nova in the Kepler field near the G dwarf KIC 5438845

    SciTech Connect (OSTI)

    Brown, Alexander; Ayres, Thomas R.; Neff, James E.; Wells, Mark A.; Kowalski, Adam; Berdyugina, Svetlana; Harper, Graham M.; Korhonen, Heidi; Piskunov, Nikolai; Saar, Steven; Walkowicz, Lucianne

    2015-02-01

    The Kepler satellite provides a unique window into stellar temporal variability by observing a wide variety of stars with multi-year, near-continuous, high precision, optical photometric time series. While most Kepler targets are faint stars with poorly known physical properties, many unexpected discoveries should result from a long photometric survey of such a large area of sky. During our Kepler Guest Observer programs that monitored late-type stars for starspot and flaring variability, we discovered a previously unknown dwarf nova that lies within a few arcseconds of the mid-G dwarf star KIC 5438845. This dwarf nova underwent nine outbursts over a 4 year time span. The two largest outbursts lasted ?1718 days and show strong modulations with a 110.8 minute period and a declining amplitude during the outburst decay phase. These properties are characteristic of an SU UMa-type cataclysmic variable. By analogy with other dwarf nova light curves, we associate the 110.8 minute (1.847 hr) period with the superhump period, close to but slightly longer than the orbital period of the binary. No precursor outbursts are seen before the super-outbursts and the overall super-outburst morphology corresponds to Osaki and Meyer Case B outbursts, which are initiated when the outer edge of the disk reaches the tidal truncation radius. Case B outbursts are rare within the Kepler light curves of dwarf novae. The dwarf nova is undergoing relatively slow mass transfer, as evidenced by the long intervals between outbursts, but the mass transfer rate appears to be steady, because the smaller normal outbursts show a strong correlation between the integrated outburst energy and the elapsed time since the previous outburst. At super-outburst maximum the system was at V ? 18, but in quiescence it is fainter than V ? 22, which will make any detailed quiescent follow-up of this system difficult.

  1. DAQ Software Contributions, Absolute Scale Energy Calibration and Background Evaluation for the NOvA Experiment at Fermilab

    SciTech Connect (OSTI)

    Flumerfelt, Eric Lewis

    2015-08-01

    The NOvA (NuMI Off-axis ve [nu_e] Appearance) Experiment is a long-baseline accelerator neutrino experiment currently in its second year of operations. NOvA uses the Neutrinos from the Main Injector (NuMI) beam at Fermilab, and there are two main off-axis detectors: a Near Detector at Fermilab and a Far Detector 810 km away at Ash River, MN. The work reported herein is in support of the NOvA Experiment, through contributions to the development of data acquisition software, providing an accurate, absolute-scale energy calibration for electromagnetic showers in NOvA detector elements, crucial to the primary electron neutrino search, and through an initial evaluation of the cosmic background rate in the NOvA Far Detector, which is situated on the surface without significant overburden. Additional support work for the NOvA Experiment is also detailed, including DAQ Server Administration duties and a study of NOvA’s sensitivity to neutrino oscillations into a “sterile” state.

  2. ELEMENTAL ABUNDANCES IN THE EJECTA OF OLD CLASSICAL NOVAE FROM LATE-EPOCH SPITZER SPECTRA

    SciTech Connect (OSTI)

    Helton, L. Andrew; Vacca, William D.; Gehrz, Robert D.; Woodward, Charles E.; Shenoy, Dinesh P.; Wagner, R. Mark; Evans, Aneurin; Krautter, Joachim; Schwarz, Greg J.; Starrfield, Sumner

    2012-08-10

    We present Spitzer Space Telescope mid-infrared IRS spectra, supplemented by ground-based optical observations, of the classical novae V1974 Cyg, V382 Vel, and V1494 Aql more than 11, 8, and 4 years after outburst, respectively. The spectra are dominated by forbidden emission from neon and oxygen, though in some cases, there are weak signatures of magnesium, sulfur, and argon. We investigate the geometry and distribution of the late time ejecta by examination of the emission line profiles. Using nebular analysis in the low-density regime, we estimate lower limits on the abundances in these novae. In V1974 Cyg and V382 Vel, our observations confirm the abundance estimates presented by other authors and support the claims that these eruptions occurred on ONe white dwarfs (WDs). We report the first detection of neon emission in V1494 Aql and show that the system most likely contains a CO WD.

  3. NOVA: a nonvariational code for solving MHD stability of axisymmetric toroidal plasmas

    SciTech Connect (OSTI)

    Cheng, C.Z.; Chance, M.S.

    1986-04-01

    A nonvariational approach for determining the ideal MHD stability of axisymmetric toroidal confinement systems is presented. The code (NOVA) employs cubic B-spline finite elements and Fourier expansion in a general flux coordinate (psi, theta, zeta) system. Better accuracy and faster convergence were obtained in comparison with the variational PEST and ERATO codes. The nonvariational approach can be extended to problems having non-Hermitian eigenmode equations where variational energy principles cannot be obtained.

  4. Data handling with SAM and art at the NOvA experiment

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

    Aurisano, A.; Backhouse, C.; Davies, G. S.; Illingworth, R.; Mayer, N.; Mengel, M.; Norman, A.; Rocco, D.; Zirnstein, J.

    2015-12-23

    During operations, NOvA produces between 5,000 and 7,000 raw files per day with peaks in excess of 12,000. These files must be processed in several stages to produce fully calibrated and reconstructed analysis files. In addition, many simulated neutrino interactions must be produced and processed through the same stages as data. To accommodate the large volume of data and Monte Carlo, production must be possible both on the Fermilab grid and on off-site farms, such as the ones accessible through the Open Science Grid. To handle the challenge of cataloging these files and to facilitate their off-line processing, we havemore » adopted the SAM system developed at Fermilab. SAM indexes files according to metadata, keeps track of each file's physical locations, provides dataset management facilities, and facilitates data transfer to off-site grids. To integrate SAM with Fermilab's art software framework and the NOvA production workflow, we have developed methods to embed metadata into our configuration files, art files, and standalone ROOT files. A module in the art framework propagates the embedded information from configuration files into art files, and from input art files to output art files, allowing us to maintain a complete processing history within our files. Embedding metadata in configuration files also allows configuration files indexed in SAM to be used as inputs to Monte Carlo production jobs. Further, SAM keeps track of the input files used to create each output file. Parentage information enables the construction of self-draining datasets which have become the primary production paradigm used at NOvA. In this study we will present an overview of SAM at NOvA and how it has transformed the file production framework used by the experiment.« less

  5. THE 2001-2003 LOW STATE OF NOVA LACERTAE 1950 (DK LAC)

    SciTech Connect (OSTI)

    Honeycutt, R. K.; Jacobson, H.; Hoffman, D.; Maxwell, T.; Croxall, K.; Kafka, S.; Henden, A. A.; Robertson, J. W. E-mail: jacob189@msu.edu E-mail: tmaxwell@astro.indiana.edu E-mail: skafka@dtm.ciw.edu E-mail: Jeff.Robertson@atu.edu

    2011-04-15

    We report on extensive photometry of DK Lac obtained during the interval 1990-2009, which includes a 2 mag low state during 2001-2003. Much of the photometry consists of exposures obtained with a typical spacing of several days, but also includes 26 sequences of continuous photometry each lasting 2-7 hr. We find no evidence for periodicities in our data. We do find that the random variations in the low state are approximately twice those in the high state, when expressed in magnitudes. The lack of orbital-timescale variations is attributed to the nearly face-on presentation of the disk. There is a 0.2 mag decline in the high-state brightness of the system over 19 years, which is consistent with the behavior of other old novae in the decades following outburst. High-state spectra are also presented and discussed. We find that the equivalent width of H{alpha} falls by about double from 1991 to 2008. The photometric properties are discussed in the context of the hibernation scenario for the behavior of novae between outbursts, in which we conclude that low states in old novae are probably unrelated to their possible entrance into hibernation.

  6. The 1991-2012 light curve of the old nova HR Lyrae

    SciTech Connect (OSTI)

    Honeycutt, R. K.; Shears, J.; Kafka, S.; Robertson, J. W.; Henden, A. A. E-mail: bunburyobservatory@hotmail.com E-mail: Jeff.Robertson@atu.edu

    2014-05-01

    The 22 yr light curve of HR Lyr, acquired with a typical cadence of 2-6 days, is examined for periodic and quasi-periodic variations. No persistent periodicities are revealed. Rather, the light curve variations often take the form of nearly linear rises and falls having typical e-folding times of about 100 days. Occasional ?0.6 mag outbursts are also seen, with properties similar to those of small outbursts found in some nova-like cataclysmic variables. When the photometry is formed into yearly averages, a decline of 0.012 0.005 mag yr{sup 1} is apparent, consistent with the fading of irradiation-induced M-dot following the nova. The equivalent width of H? is tabulated at three epochs over the interval 1986-2008 in order to compare with a recent result for DK Lac in which H? was found to be fading 50 yr after the nova. However, our results for such a fading in HR Lyr are inconclusive.

  7. NOvA detector technology with intial performance from the surface prototype

    SciTech Connect (OSTI)

    Muether, M.; /Fermilab

    2011-09-01

    NOvA, the NuMI Off-Axis {nu}{sub e} Appearance experiment, will study {nu}{sub {mu}} {yields} {nu}{sub e} oscillations characterized by the mixing angle {Theta}{sub 13}. Provided {Theta}{sub 13} is large enough, NOvA may ultimately determine the ordering of the neutrino masses and measure CP violation in neutrino oscillations. A complementary pair of detectors will be constructed {approx}14 mrad off beam axis to optimize the energy profile of the neutrinos. This system consists of a surface based 14 kTon liquid scintillator tracking volume located 810 km from the main injector source (NuMI) in Ash River, Minnesota and a smaller underground 222 Ton near detector at the Fermilab. The first neutrino signals at the Ash River Site are expected prior to the 2012 accelerator shutdown. In the meantime, a near detector surface prototype has been completed and neutrinos from two Fermilab sources have been observed using the same highly segmented PVC and liquid scintillator detector system that will be deployed in the full scale experiment. Design and initial performance characteristics of this prototype system are being fed back into the design for the full NOvA program.

  8. Recent evolution of the offline computing model of the NOvA experiment

    SciTech Connect (OSTI)

    Habig, Alec; Norman, A.; Group, Craig

    2015-12-23

    The NOvA experiment at Fermilab is a long-baseline neutrino experiment designed to study νe appearance in a νμ beam. Over the last few years there has been intense work to streamline the computing infrastructure in preparation for data, which started to flow in from the far detector in Fall 2013. Major accomplishments for this effort include migration to the use of off-site resources through the use of the Open Science Grid and upgrading the file-handling framework from simple disk storage to a tiered system using a comprehensive data management and delivery system to find and access files on either disk or tape storage. NOvA has already produced more than 6.5 million files and more than 1 PB of raw data and Monte Carlo simulation files which are managed under this model. In addition, the current system has demonstrated sustained rates of up to 1 TB/hour of file transfer by the data handling system. NOvA pioneered the use of new tools and this paved the way for their use by other Intensity Frontier experiments at Fermilab. Most importantly, the new framework places the experiment's infrastructure on a firm foundation, and is ready to produce the files needed for first physics.

  9. Recent evolution of the offline computing model of the NOvA experiment

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

    Habig, Alec; Norman, A.; Group, Craig

    2015-12-23

    The NOvA experiment at Fermilab is a long-baseline neutrino experiment designed to study νe appearance in a νμ beam. Over the last few years there has been intense work to streamline the computing infrastructure in preparation for data, which started to flow in from the far detector in Fall 2013. Major accomplishments for this effort include migration to the use of off-site resources through the use of the Open Science Grid and upgrading the file-handling framework from simple disk storage to a tiered system using a comprehensive data management and delivery system to find and access files on either diskmore » or tape storage. NOvA has already produced more than 6.5 million files and more than 1 PB of raw data and Monte Carlo simulation files which are managed under this model. In addition, the current system has demonstrated sustained rates of up to 1 TB/hour of file transfer by the data handling system. NOvA pioneered the use of new tools and this paved the way for their use by other Intensity Frontier experiments at Fermilab. Most importantly, the new framework places the experiment's infrastructure on a firm foundation, and is ready to produce the files needed for first physics.« less

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  12. Radio frequency models of novae in eruption. I. The free-free process in bipolar morphologies

    SciTech Connect (OSTI)

    Ribeiro, V. A. R. M.; Simon, T.; Woudt, P. A.; Chomiuk, L.; Munari, U.; Steffen, W.; Koning, N.; O'Brien, T. J.; Bode, M. F.

    2014-09-01

    Observations of novae at radio frequencies provide us with a measure of the total ejected mass, density profile, and kinetic energy of a nova eruption. The radio emission is typically well characterized by the free-free emission process. Most models to date have assumed spherical symmetry for the eruption, although for as long as there have been radio observations of these systems, it has been known that spherical eruptions are too simplistic a geometry. In this paper, we build bipolar models of the nova eruption, assuming the free-free process, and show the effects of varying different parameters on the radio light curves. The parameters considered include the ratio of the minor- to major-axis, the inclination angle, and shell thickness. We also show the uncertainty introduced when fitting spherical-model synthetic light curves to bipolar-model synthetic light curves. We find that the optically thick phase rises with the same power law (S {sub ?}?t {sup 2}) for both the spherical and bipolar models. In the bipolar case, there is a 'plateau' phasedepending on the thickness of the shell as well as the ratio of the minor- to major-axisbefore the final decline, which follows the same power law (S {sub ?}?t {sup 3}) as in the spherical case. Finally, fitting spherical models to the bipolar-model synthetic light curves requires, in the worst-case scenario, doubling the ejected mass, more than halving the electron temperature, and reducing the shell thickness by nearly a factor of 10. This implies that in some systems we have been over-predicting the ejected masses and under-predicting the electron temperature of the ejecta.

  13. HUBBLE SPACE TELESCOPE FAR ULTRAVIOLET SPECTROSCOPY OF THE RECURRENT NOVA T PYXIDIS

    SciTech Connect (OSTI)

    Godon, Patrick; Sion, Edward M. [Astronomy and Astrophysics, Villanova University, Villanova, PA 19085 (United States); Starrfield, Sumner [School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287 (United States); Livio, Mario; Williams, Robert E. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Woodward, Charles E. [Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, MN 55455 (United States); Kuin, Paul [Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT (United Kingdom); Page, Kim L., E-mail: patrick.godon@villanova.edu, E-mail: edward.sion@villanova.edu, E-mail: sumner.starrfield@asu.edu, E-mail: mlivio@stsci.edu, E-mail: wms@stsci.edu, E-mail: chelsea@astro.umn.edu, E-mail: n.kuin@ucl.ac.uk, E-mail: klp5@leicester.ac.uk [Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH (United Kingdom)

    2014-04-01

    With six recorded nova outbursts, the prototypical recurrent nova T Pyxidis (T Pyx) is the ideal cataclysmic variable system to assess the net change of the white dwarf mass within a nova cycle. Recent estimates of the mass ejected in the 2011 outburst ranged from a few ?10{sup 5} M {sub ?} to 3.3 10{sup 4} M {sub ?}, and assuming a mass accretion rate of 10{sup 8}-10{sup 7} M {sub ?}yr{sup 1} for 44yr, it has been concluded that the white dwarf in T Pyx is actually losing mass. Using NLTE disk modeling spectra to fit our recently obtained Hubble Space Telescope COS and STIS spectra, we find a mass accretion rate of up to two orders of magnitude larger than previously estimated. Our larger mass accretion rate is due mainly to the newly derived distance of T Pyx (4.8kpc, larger than the previous 3.5kpc estimate), our derived reddening of E(B V) = 0.35 (based on combined IUE and GALEX spectra), and NLTE disk modeling (compared to blackbody and raw flux estimates in earlier works). We find that for most values of the reddening (0.25 ? E(B V) ? 0.50) and white dwarf mass (0.70 M {sub ?} ? M {sub wd} ? 1.35 M {sub ?}) the accreted mass is larger than the ejected mass. Only for a low reddening (?0.25 and smaller) combined with a large white dwarf mass (0.9 M {sub ?} and larger) is the ejected mass larger than the accreted one. However, the best results are obtained for a larger value of reddening.

  14. MULTIWAVELENGTH PHOTOMETRY AND HUBBLE SPACE TELESCOPE SPECTROSCOPY OF THE OLD NOVA V842 CENTAURUS

    SciTech Connect (OSTI)

    Sion, Edward M. [Department of Astronomy and Astrophysics, Villanova University, 800 Lancaster Avenue, Villanova, PA 19085 (United States); Szkody, Paula; Mukadam, Anjum [Department of Astronomy, University of Washington, Seattle, WA 98195 (United States); Warner, Brian; Woudt, Patrick [Astrophysics, Cosmology and Gravity Centre, Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701 (South Africa); Walter, Frederic [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (United States); Henden, Arne [AAVSO 49 Bay State Road, Cambridge, MA 02138 (United States); Godon, Patrick, E-mail: edward.sion@villanova.edu, E-mail: szkody@astro.washington.edu, E-mail: anjum@astro.washington.edu, E-mail: brian.warner@uct.ac.za, E-mail: pwoudt@ast.uct.ac.za, E-mail: frederick.walter@stonybrook.edu, E-mail: arne@aavso.edu [Department of Astronomy and Astrophysics, Villanova University, Villanova, PA 19085 (United States)

    2013-08-01

    We present ground-based optical and near infrared photometric observations and Hubble Space Telescope (HST) COS spectroscopic observations of the old nova V842 Cen (Nova Cen 1986). Analysis of the optical light curves reveals a peak at 56.5 {+-} 0.3 s with an amplitude of 8.9 {+-} 4.2 mma, which is consistent with the rotation of a magnetic white dwarf primary in V842 Cen that was detected earlier by Woudt et al., and led to its classification as an intermediate polar. However, our UV lightcurve created from the COS time-tag spectra does not show this periodicity. Our synthetic spectral analysis of an HST COS spectrum rules out a hot white dwarf photosphere as the source of the FUV flux. The best-fitting model to the COS spectrum is a full optically thick accretion disk with no magnetic truncation, a low disk inclination angle, low accretion rate and a distance less than half the published distance that was determined on the basis of interstellar sodium D line strengths. Truncated accretion disks with truncation radii of 3 R{sub wd} and 5 R{sub wd} yielded unsatisfactory agreement with the COS data. The accretion rate is unexpectedly low for a classical nova only 24 yr after the explosion when the accretion rate is expected to be high and the white dwarf should still be very hot, especially if irradiation of the donor star took place. Our low accretion rate is consistent with those derived from X-ray and ground-based optical data.

  15. Neutrino Oscillations with the MINOS, MINOS+, T2K, and NOvA Experiments

    SciTech Connect (OSTI)

    Nakaya, Tsuyoshi; Plunkett, Robert K.

    2015-07-29

    Our paper discusses results and near-term prospects of the long-baseline neutrino experiments MINOS, MONOS+, T2K and NOvA. The non-zero value of the third neutrino mixing angle θ13 allows experimental analysis in a manner which explicitly exhibits appearance and disappearance dependencies on additional parameters associated with mass-hierarchy, CP violation, and any non-maximal θ23. Our current and near-future experiments begin the era of precision accelerator long-baseline measurements and lay the framework within which future experimental results will be interpreted.

  16. US Department

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

    ... fraud, waste, and abuse, and protect public health and safety. The OIG Whistleblower Ombudsman educates Department employees about prohibitions on retaliation for whistleblowing, ...

  17. Fabrication and testing of gas-filled targets for large-scale plasma experiments on nova

    SciTech Connect (OSTI)

    Stone, G.F.; Rivers, C.J.; Spragge, M.R.; Wallace, R.J.

    1996-06-01

    The proposed next-generation ICF facility, the National Ignition Facility (NIF) is designed to produce energy gain from x-ray heated {open_quotes}indirect-drive{close_quotes} fuel capsules. For indirect-drive targets, laser light heats the inside of the Au hohlraum wall and produces x rays which in turn heat and implode the capsule to produce fusion conditions in the fuel. Unlike Nova targets, in NIF-scale targets laser light will propagate through several millimeters of gas, producing a plasma, before impinging upon the Au hohlraum wall. The purpose of the gas-produced plasma is to provide sufficient pressure to keep the radiating Au surface from expanding excessively into the hohlraum cavity. Excessive expansion of the Au wall interacts with the laser pulse and degrades the drive symmetry of the capsule implosion. The authors have begun an experimental campaign on the Nova laser to study the effect of hohlraum gas on both laser-plasma interaction and implosion symmetry. In their current NIF target design, the calculated plasma electron temperature is T{sub e} {approx} 3 keV and the electron density is N{sub e} {approx} 10{sup 21}cm{sup {minus}3}.

  18. MULTIPLICITY OF NOVA ENVELOPE SOLUTIONS AND OCCURRENCE OF OPTICALLY THICK WINDS

    SciTech Connect (OSTI)

    Kato, Mariko; Hachisu, Izumi E-mail: hachisu@ea.c.u-tokyo.ac.jp

    2009-07-10

    We revisit the occurrence condition of optically thick winds reported by Kato in 1985 and Kato and Hachisu in 1989 who mathematically examined nova envelope solutions with an old opacity and found that optically thick winds are accelerated only in massive white dwarfs (WDs) of {approx}>0.9 M{sub sun}. With the OPAL opacity we find that the optically thick wind occurs for {approx}>0.6 M{sub sun} WDs and that the occurrence of winds depends not only on the WD mass but also on the ignition mass. When the ignition mass is larger than a critical value, winds are suppressed by a density-inversion layer. Such a static solution can be realized in WDs of mass {approx}0.6-0.7 M{sub sun}. We propose that sequences consisting only of static solutions correspond to slow evolutions in symbiotic novae like PU Vul because PU Vul shows no indication of strong winds in a long-lasted flat peak followed by a very slow decline in its light curve.

  19. Surface studies and implanted helium measurements following NOVA high-yield DT experiments

    SciTech Connect (OSTI)

    Stoyer, M.A.; Hudson, G.B.

    1997-02-18

    This paper presents the results of three March 6, 1996 direct-drive high-yield DT NOVA experiments and provides `proof-of-principal` results for the quantitative measurement of energetic He ions. Semiconductor quality Si wafers and an amorphous carbon wafer were exposed to NOVA high-yield implosions. Surface damage was sub-micron in general, although the surface ablation was slightly greater for the carbon wafer than for the Si wafers. Melting of a thin ({approx} 0.1{mu}) layer of Si was evident from microscopic investigation. Electron microscopy indicated melted blobs of many different metals (e.g. Al, Au, Ta, Fe alloys, Cu and even Cd) on the surfaces. The yield measured by determining the numbers of atoms of implanted {sup 4}He and {sup 3}He indicate the number of DT fusions to be 9.1({plus_minus}2.3) X 10{sup 12} and DD fusions to be 4.8({plus_minus}1.0) x 10{sup 10}, respectively. The helium DT fusion yield is slightly lower than that of the Cu activation measurement, which was 1.3({plus_minus}0.l) x 10{sup 13} DT fusions.

  20. US Department

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

    US Department of Energy Office of Inspector General FY 2014 Annual Performance Report FYs 2015 & 2016 Performance Plan U.S. Department of Energy, Office of Inspector General Annual Performance Report FY 2014 Annual Performance Plan FYs 2015 & 2016 Page i Table of Contents Page Message from the Inspector General ii At a Glance: Performance Results for FY 2014 iii Overview 1 Our Organization 2 External Factors Challenging Our Organization 4 Our Management Challenges 4 Measuring Our

  1. The 2011 outburst of recurrent nova T PYX: Radio observations reveal the ejecta mass and hint at complex mass loss

    SciTech Connect (OSTI)

    Nelson, Thomas; Chomiuk, Laura; Roy, Nirupam; Krauss, Miriam I.; Mioduszewski, Amy J.; Rupen, Michael P.; Sokoloski, J. L.; Weston, Jennifer; Mukai, Koji

    2014-04-10

    Despite being the prototype of its class, T Pyx is arguably the most unusual and poorly understood recurrent nova. Here, we use radio observations from the Karl G. Jansky Very Large Array to trace the evolution of the ejecta over the course of the 2011 outburst of T Pyx. The radio emission is broadly consistent with thermal emission from the nova ejecta. However, the radio flux began rising surprisingly late in the outburst, indicating that the bulk of the radio-emitting material was either very cold, or expanding very slowly, for the first ∼50 days of the outburst. Considering a plausible range of volume filling factors and geometries for the ejecta, we find that the high peak flux densities of the radio emission require a massive ejection of (1-30) × 10{sup –5} M {sub ☉}. This ejecta mass is much higher than the values normally associated with recurrent novae, and is more consistent with a nova on a white dwarf well below the Chandrasekhar limit.

  2. Observation of Electron Neutrino Appearance in the NuMI Beam with the NOvA Experiment

    SciTech Connect (OSTI)

    Niner, Evan David

    2015-01-01

    NOvA is a long-baseline neutrino oscillation experiment that uses two functionally identical detectors separated by 810 kilometers at locations 14 milliradians off-axis from the NuMI muon neutrino beam at Fermilab. At these locations the beam energy peaks at 2 GeV. This baseline is the longest in the world for an accelerator-based neutrino oscillation experiment, which enhances the sensitivity to the neutrino mass ordering. The experiment studies oscillations of the muon neutrino and anti-neutrino beam that is produced. Both detectors completed commissioning in the summer of 2014 and continue to collect data. One of the primary physics goals of the experiment is the measurement of electron neutrino appearance in the muon neutrino beam which yields measurements of the oscillation parameters sin213, δ , and the neutrino mass ordering within the standard model of neutrino oscillations. This thesis presents the analysis of data collected between February 2014 and May 2015, corresponding to 3.52 X 1020 protons-on-target. In this first analysis NOvA recorded 6 electron neutrino candidates, which is a 3.3σ observation of electron neutrino appearance. The T2K experiment performs the same measurement on a baseline of 295 kilometers and has a 1 σ preference for the normal mass ordering over the inverted ordering over the phase space of the CP violating parameter δ, which is also weakly seen in the NOvA result. By the summer of 2016 NOvA will triple its statistics due to increased beam power and a completed detector. If electron neutrinos continue to be observed at the current rate NOvA will be able to establish a mass ordering preference at a similar confidence level to T2K.

  3. Procedures for Departing Employees | Department of Energy

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    Procedures for Departing Employees Procedures for Departing Employees RM Exit Procedures (2)3.12.12.pdf (39.89 KB) More Documents & Publications Procedures for Departing Employees ...

  4. Procedures for Departing Employees | Department of Energy

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    Procedures for Departing Employees Procedures for Departing Employees RM Exit Procedures.doc (337 KB) More Documents & Publications Procedures for Departing Employees Records ...

  5. Green Power Labs Inc | Open Energy Information

    Open Energy Info (EERE)

    Labs Inc Jump to: navigation, search Name: Green Power Labs Inc. Place: Dartmouth, Nova Scotia, Canada Zip: B2Y4M9 Sector: Services, Solar Product: Provides solar energy assessment...

  6. Full aperture backscatter station imager diagnostics system for far-field imaging of laser plasma instabilities on Nova

    SciTech Connect (OSTI)

    Wilke, M.D.; Fernandez, J.C.; Berggren, R.R.; Horton, R.F.; Montgomery, D.S.; Faulkner, J.A.; Looney, L.D.; Jimerson, J.R.

    1997-01-01

    In ICF, the understanding of laser plasma scattering processes is essential for laser target coupling and for controlling the symmetry of indirect drive implosions. The existing Nova full aperture backscatter station has been useful in understanding laser plasma instabilities occurring in hohlraums by measuring the quantity, spectral distribution, and near-field spatial distributions of Brillouin and more recently Raman backscatter. Equally important is an understanding of the far-field spatial intensity distribution which could help in understanding filamentation, threshold and saturation processes. This article describes a broadband, color-corrected far-field imager and associated diagnostics capable of imaging the source of scattered light to better than 25 {mu}m resolution. Brillouin and Raman backscatter can be imaged through the Nova beam-7 focusing lens or the imager can be used like a microscope to image side scatter from other beams. {copyright} {ital 1997 American Institute of Physics.}

  7. THE SUPERSOFT X-RAY PHASE OF NOVA RS OPHIUCHI 2006

    SciTech Connect (OSTI)

    Osborne, J. P.; Page, K. L.; Beardmore, A. P.; Goad, M. R.; Bode, M. F.; O'Brien, T. J.; Starrfield, S.; Rauch, T.; Ness, J.-U.; Krautter, J.; Schwarz, G.; Burrows, D. N.; Gehrels, N.; Drake, J. J.; Evans, A.; Eyres, S. P. S.

    2011-02-01

    Swift X-ray observations of the {approx}60 day supersoft phase of the recurrent nova RS Ophiuchi (RS Oph) 2006 show the progress of nuclear burning on the white dwarf (WD) in exquisite detail. First seen 26 days after the optical outburst, this phase started with extreme variability likely due to variable absorption, although intrinsic WD variations are not excluded. About 32 days later, a steady decline in count rate set in. NLTE model atmosphere spectral fits during the supersoft phase show that the effective temperature of the WD increases from {approx}65 eV to {approx}90 eV during the extreme variability phase, falling slowly after about day 60 and more rapidly after day 80. The bolometric luminosity is seen to be approximately constant and close to Eddington from day 45 up to day 60, the subsequent decline possibly signaling the end of extensive nuclear burning. Before the decline, a multiply-periodic {approx}35 s modulation of the soft X-rays was present and may be the signature of a nuclear fusion driven instability. Our measurements are consistent with a WD mass near the Chandrasekhar limit; combined with a deduced accumulation of mass transferred from its binary companion, this leads us to suggest that RS Oph is a strong candidate for a future supernova explosion. The main uncertainty now is whether the WD is the CO type necessary for a Type Ia supernova. This may be confirmed by detailed abundance analyses of spectroscopic data from the outbursts.

  8. I Department

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    Department of Energy RdII_ 0pir1tl0llS O'"et po. lox &10 Ibchllll1f. WahHlltOn 88382 , 0801071:1 S' * , . JUL 15- Mr. R. H. Gibbons 1Juor Tecbnoloat, lne. Advanced Technilogy Dtvlston 3333 H'chelson DrIve Irvine. CA 92730 Dear Mr. Gtbbofts: CONTRACT NO. DE**ACO&-86RLl0838. HANFORDUASTE YIlRlFlCAnOH plAm,. RE~EST fOR APPROVALOF TRAVEL POLICY The travel pol1c1 sublllttted for r.view and approval ~r your 'auer of " June 17. 1988. does Dot meet the requ'rements of FAR 31.205-46,

  9. The 2011 outburst of recurrent nova T Pyx: X-ray observations expose the white dwarf mass and ejection dynamics

    SciTech Connect (OSTI)

    Chomiuk, Laura; Nelson, Thomas; Mukai, Koji; Rupen, Michael P.; Mioduszewski, Amy J.; Krauss, Miriam I.; Page, Kim L.; Osborne, Julian P.; Kuulkers, Erik; Roy, Nirupam

    2014-06-20

    The recurrent nova T Pyx underwent its sixth historical outburst in 2011, and became the subject of an intensive multi-wavelength observational campaign. We analyze data from the Swift and Suzaku satellites to produce a detailed X-ray light curve augmented by epochs of spectral information. X-ray observations yield mostly non-detections in the first four months of outburst, but both a super-soft and hard X-ray component rise rapidly after Day 115. The super-soft X-ray component, attributable to the photosphere of the nuclear-burning white dwarf, is relatively cool (∼45 eV) and implies that the white dwarf in T Pyx is significantly below the Chandrasekhar mass (∼1 M {sub ☉}). The late turn-on time of the super-soft component yields a large nova ejecta mass (≳ 10{sup –5} M {sub ☉}), consistent with estimates at other wavelengths. The hard X-ray component is well fit by a ∼1 keV thermal plasma, and is attributed to shocks internal to the 2011 nova ejecta. The presence of a strong oxygen line in this thermal plasma on Day 194 requires a significantly super-solar abundance of oxygen and implies that the ejecta are polluted by white dwarf material. The X-ray light curve can be explained by a dual-phase ejection, with a significant delay between the first and second ejection phases, and the second ejection finally released two months after outburst. A delayed ejection is consistent with optical and radio observations of T Pyx, but the physical mechanism producing such a delay remains a mystery.

  10. EA-355_Scotia_Capital_CN.pdf

    Office of Environmental Management (EM)

    4 Endure Energy, L.L.C. EA-354 Endure Energy, L.L.C. Order authorizing Endure Energy, L.L.C. to export electric energy to Canada EA-354 Endure Energy, L.L.C. (380.51 KB) More Documents & Publications Application to Export Electric Energy OE Docket No. EA-354 Endure Energy, L.L.C. EA-357 Hunt Electric Power Marketing, L.L.C. Application to Export Electric Energy OE Docket No. EA-354 Endure Energy, L.L.C.: Federal Register Notice Volume 74, No. 105 - Jun. 3, 2009

  11. Full aperture backscatter station imager (FABSI) diagnostics system for far-field imaging of laser plasma instabilities on Nova

    SciTech Connect (OSTI)

    Wilke, M.D.; Fernandez, J.C.; Berggren, R.R.; Montgomery, D.; Faulkner, J.; Looney, L.; Jimerson, J.; Horton, R.F.

    1996-06-01

    In ICF, the understanding of laser plasma scattering processes is essential for laser target coupling and in controlling the symmetry of indirect drive implosions. The existing Nova Full Aperture Backscatter Station (FABS) has been useful in understanding laser plasma instabilities occurring in hohlraums by measuring the quantity, spectral distribution and near-field spatial distributions of Brillouin and more recently Raman backscatter. Equally important is an understanding of the farfield spatial intensity distribution which provides information on density, temperature and velocity gradient distributions, and which affect capsule implosion symmetry in hohlraums. Such information could potentially help in understanding processes such as filamentation and saturation mechanism. This paper describes a broad-band, color-corrected far-field imager and associated diagnostics capable of imaging the source of scattered light to better than 25 {micro}m resolution. The imager can either image Brillouin or Raman backscatter through the Nova beam 7 focusing lens or be used like a microscope to image side scatter from other beams.

  12. Calendar Year 2010 | Department of Energy

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    Laboratory's NOvA Project April 9, 2010 Audit Report: OAS-RA-10-07 Management Alert on Environmental Management's Select Strategy for Disposition of Savannah River Site Depleted...

  13. Modernization | Department of Energy

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    the Departments missions in science, energy efficiency, and national security. ... conduct the Department's missions in science, energy efficiency, and national security. ...

  14. Department of Energy

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    most important and technically advanced missions, the Department of Energy faces an array ... To accomplish its vital missions, the Department employs approximately 115,000 Federal and ...

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    Department of Energy No. AL 2016-02 Acquisition Regulation Date 021716 Department of ... covered by the Federal Acquisition Regulation; (C) issue a letter of intent to make ...

  16. Grants | Department of Energy

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    October 20, 2004 Energy Department Provides 250,000 to Idaho's Regional Development ... July 29, 2003 Energy Department Awards 300,000 Grant to the Regional Development ...

  17. Department of Energy Accomplishments | Department of Energy

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    Accomplishments Department of Energy Accomplishments Topic: DOE provided the members with an overview of its accomplishments on the 2005 Consent Order. DOE Accomp - November 12, ...

  18. Department of Energy | Department of Energy

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    Energy Department of Energy More Documents & Publications Policy Flash Search Listing (2001-2014) Acquisition Letter Archive listing Impacts of IPv6 on Infrastructure Control ...

  19. FAR-ULTRAVIOLET SPECTROSCOPY OF THE NOVA-LIKE VARIABLE KQ MONOCEROTIS: A NEW SW SEXTANTIS STAR?

    SciTech Connect (OSTI)

    Wolfe, Aaron; Sion, Edward M.; Bond, Howard E. E-mail: edward.sion@villanova.edu

    2013-06-01

    New optical spectra obtained with the SMARTS 1.5 m telescope and archival International Ultraviolet Explorer (IUE) far-ultraviolet (FUV) spectra of the nova-like variable KQ Mon are discussed. The optical spectra reveal Balmer lines in absorption as well as He I absorption superposed on a blue continuum. The 2011 optical spectrum is similar to the KPNO 2.1 m IIDS spectrum we obtained 33 years earlier except that the Balmer and He I absorption is stronger in 2011. Far-ultraviolet IUE spectra reveal deep absorption lines due to C II, Si III, Si IV, C IV, and He II, but no P Cygni profiles indicative of wind outflow. We present the results of the first synthetic spectral analysis of the IUE archival spectra of KQ Mon with realistic optically thick, steady-state, viscous accretion-disk models with vertical structure and high-gravity photosphere models. We find that the photosphere of the white dwarf (WD) contributes very little FUV flux to the spectrum and is overwhelmed by the accretion light of a steady disk. Disk models corresponding to a WD mass of {approx}0.6 M {sub Sun }, with an accretion rate of order 10{sup -9} M {sub Sun} yr{sup -1} and disk inclinations between 60 Degree-Sign and 75 Degree-Sign , yield distances from the normalization in the range of 144-165 pc. KQ Mon is discussed with respect to other nova-like variables. Its spectroscopic similarity to the FUV spectra of three definite SW Sex stars suggests that it is likely a member of the SW Sex class and lends support to the possibility that the WD is magnetic.

  20. XMM-NEWTON X-RAY AND ULTRAVIOLET OBSERVATIONS OF THE FAST NOVA V2491 Cyg DURING THE SUPERSOFT SOURCE PHASE

    SciTech Connect (OSTI)

    Ness, J.-U.; Osborne, J. P.; Page, K. L.; Beardmore, A. P.; Dobrotka, A.; Drake, J. J.; Pinto, C.; Detmers, R. G.; Schwarz, G.; Bode, M. F.; Starrfield, S.; Hernanz, M.; Sala, G.; Krautter, J.; Woodward, C. E.

    2011-05-20

    Two XMM-Newton observations of the fast classical nova V2491 Cyg were carried out in short succession on days 39.93 and 49.62 after discovery, during the supersoft source (SSS) phase, yielding simultaneous X-ray and UV light curves and high-resolution X-ray spectra. The first X-ray light curve is highly variable, showing oscillations with a period of 37.2 minutes after an extended factor of three decline lasting {approx}3 hr, while the second X-ray light curve is less variable. The cause of the dip is currently unexplained and has most likely the same origin as similar events in the early SSS light curves of the novae V4743 Sgr and RS Oph, as it occurred on the same timescale. The oscillations are not present during the dip minimum and also not in the second observation. The UV light curves are variable but contain no dips and no period. High-resolution X-ray spectra are presented for four intervals of differing intensity. All spectra are atmospheric continua with deep absorption lines and absorption edges. Two interstellar lines of O I and N I are clearly seen at their rest wavelengths, while a large number of high-ionization absorption lines are found at blueshifts indicating an expansion velocity of 3000-3400 km s{sup -1}, which does not change significantly during the epochs of observation. Comparisons with the slower nova V4743 Sgr and the symbiotic recurrent nova RS Oph are presented. The SSS spectrum of V4743 Sgr is much softer with broader and more complex photospheric absorption lines. The ejecta are extended, allowing us to view a larger range of the radial velocity profile. Meanwhile, the absorption lines in RS Oph are as narrow as in V2491 Cyg, but they are less blueshifted. A remarkable similarity in the continua of V2491 Cyg and RS Oph is found. The only differences are smaller line shifts and additional emission lines in RS Oph that are related to the presence of a dense stellar wind from the evolved companion. Three unidentified absorption lines are

  1. | Department of Energy

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    SmallScaleBiorefineriesMatrix.pdf More Documents & Publications U.S. Department of Energy Small-Scale Biorefineries: Project Overview U.S. Department of Energy Small-Scale...

  2. Careers | Department of Energy

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    Careers Careers Come Join the Best The Office of Inspector General (OIG) identifies opportunities to improve the performance of the Department of Energy's (Department) programs and operations. Given the Department's mission, we are directly involved in current efforts to move energy and environment to the forefront of our national agenda. The American Recovery and Reinvestment Act of 2009 has infused more than $60 billion into clean energy investments. The Department plays an important role in

  3. Services | Department of Energy

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    EHSS provides technical assistance, coordination, and integration throughout the complex ... with Department operations and supports international health studies and programs. ...

  4. Department of Energy | Department of Energy

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    ... The purpose of DOE Policy 141.1 is to ensure that Department of Energy (DOE) programs and field elements integrate cultural resources management into their missions and activities ...

  5. XMM-NEWTON OBSERVATIONS OF THE DWARF NOVA RU Peg IN QUIESCENCE: PROBE OF THE BOUNDARY LAYER

    SciTech Connect (OSTI)

    Balman, Soelen; Godon, Patrick; Sion, Edward M.; Ness, Jan-Uwe; Schlegel, Eric; Barrett, Paul E.; Szkody, Paula E-mail: patrick.godon@villanova.edu E-mail: juness@sciops.esa.int E-mail: barrett.paul@usno.navy.mil

    2011-11-10

    We present an analysis of X-ray and UV data obtained with the XMM-Newton Observatory of the long-period dwarf nova RU Peg. RU Peg contains a massive white dwarf (WD), possibly the hottest WD in a dwarf nova (DN), it has a low inclination, thus optimally exposing its X-ray emitting boundary layer (BL), and has an excellent trigonometric parallax distance. We modeled the X-ray data using XSPEC assuming a multi-temperature plasma emission model built from the MEKAL code (i.e., CEVMKL). We obtained a maximum temperature of 31.7 keV, based on the European Photon Imaging Camera MOS1, 2 and pn data, indicating that RU Peg has an X-ray spectrum harder than most DNe, except U Gem. This result is consistent with and indirectly confirms the large mass of the WD in RU Peg. The X-ray luminosity we computed corresponds to a BL luminosity for a mass accretion rate of 2 Multiplication-Sign 10{sup -11} M{sub sun} yr{sup -1} (assuming M{sub wd} = 1.3 M{sub sun}), in agreement with the expected quiescent accretion rate. The modeling of the O VIII emission line at 19 A as observed by the Reflection Grating Spectrometer implies a projected stellar rotational velocity v{sub rot}sin i = 695 km s{sup -1}, i.e., the line is emitted from material rotating at {approx}936-1245 km s{sup -1} (i {approx} 34 Degree-Sign -48 Degree-Sign) or about 1/6 of the Keplerian speed; this velocity is much larger than the rotation speed of the WD inferred from the Far Ultraviolet Spectroscopic Explorer spectrum. Cross-correletion analysis yielded an undelayed (time lag {approx} 0) component and a delayed component of 116 {+-} 17 s where the X-ray variations/fluctuations lagged the UV variations. This indicates that the UV fluctuations in the inner disk are propagated into the X-ray emitting region in about 116 s. The undelayed component may be related to irradiation effects.

  6. 2012 Department of Energy Project Management Workshop | Department...

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    2 Department of Energy Project Management Workshop 2012 Department of Energy Project Management Workshop 2012 Department of Energy Project Management Workshop ***...

  7. Department of Energy Asset Management Plan | Department of Energy

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    Department of Energy Asset Management Plan Department of Energy Asset Management Plan The Department of Energy Asset Management Plan (2015) provides an integrating strategy for ...

  8. Energy Department Small Business Partner Success Stories | Department of

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    Energy Energy Department Small Business Partner Success Stories Energy Department Small Business Partner Success Stories Energy Department Small Business Partner Success Stories

  9. Energy Department to Sign MOU with Interior Department to Assist...

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    to Sign MOU with Interior Department to Assist Indian Tribes to Develop Energy Resources Energy Department to Sign MOU with Interior Department to Assist Indian Tribes to Develop ...

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    FACT SHEET: Department of Energy's Jobs Strategy Council FACT SHEET: Department of Energy's Jobs Strategy Council PDF icon FACT SHEET: Department of Energy's Jobs Strategy Council...

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    Texas Department of State Health Services - WIPP Program Texas Department of State Health Services - WIPP Program PDF icon Texas Department of State Health Services - WIPP Program ...

  12. X-RAY ECLIPSE DIAGNOSIS OF THE EVOLVING MASS LOSS IN THE RECURRENT NOVA U SCORPII 2010

    SciTech Connect (OSTI)

    Takei, D.; Drake, J. J.; Tsujimoto, M.; Ness, J.-U.; Osborne, J. P.; Starrfield, S.; Kitamoto, S.

    2013-05-20

    We report the Suzaku detection of the earliest X-ray eclipse seen in the recurrent nova U Scorpii 2010. A target-of-opportunity observation 15 days after the outburst found a 27% {+-} 5% dimming in the 0.2-1.0 keV energy band at the predicted center of an eclipse. In comparison with the X-ray eclipse depths seen at two later epochs by XMM-Newton, the source region shrank by about 10%-20% between days 15 and 35 after the outburst. The X-ray eclipses appear to be deeper than or similar to contemporaneous optical eclipses, suggesting the X-ray and optical source region extents are comparable on day 15. We raise the possibility of the energy dependency in the photon escape regions, and that this would be a result of the supersoft X-ray opacity being higher than the Thomson scattering opacity at the photosphere due to bound-free transitions in abundant metals that are not fully ionized. Assuming a spherically symmetric model, we constrain the mass-loss rate as a function of time. For a ratio of actual to Thomson opacity of 10-100 in supersoft X-rays, we find an ejecta mass of about 10{sup -7}-10{sup -6} M{sub Sun }.

  13. Innovation | Department of Energy

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    Innovation Innovation For America's next generation of clean energy innovators, getting started can be the hardest part. That's why the Department of Energy is testing a new model for clean energy research and development (R&D) through a program called Cyclotron Road. As a science agency, the Energy Department plays an important role in the innovation economy. The Department catalyzes the transformative growth of basic applied scientific research, the discovery and development of new clean

  14. Publications | Department of Energy

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    UNITED STATES OF AMERICA OFFICE OF ENERGY EFFICIENCY AND RENEWABLE ENERGY PUBLIC MEETING SUSTAINABLE DESIGN STANDARDS FOR FEDERAL BUILDINGS U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 Room 8E-089 Wednesday July 28, 2010 Chair: Cyrus Nasseri Department of Energy (FEMP) Facilitator: Jim Raba Department of Energy Executive Court Reporters (301) 565-0064 2 Participants Identified: Mark Ames American Society of Heating, Refrigerating and Air- Conditioning Engineers

  15. Leadership | Department of Energy

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    Leadership Leadership Leadership Joseph Hezir Chief Financial Officer (CFO) Joseph Hezir was confirmed by the Senate on December 4, 2014 as the Department of Energy's Chief Financial Officer. As Chief Financial Officer, Mr. Hezir will work to assure the effective management and financial integrity of Department of Energy. He will help to implement and monitor Department-wide policies and systems in the areas of budget administration, program analysis and evaluation, finance and accounting,

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    DEPARTMENT OF ENERGY Invitation for Public Comment to Inform the Design of a Consent-Based Siting Process for Nuclear Waste Storage and Disposal Facilities AGENCY: Fuel Cycle Technologies, Office of Nuclear Energy, Department of Energy. ACTION: Notice of Invitation for Public Comment (IPC) SUMMARY: The U.S Department of Energy (DOE) is implementing a consent-based siting process to establish an integrated waste management system to transport, store, and dispose of commercial spent nuclear fuel

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    DEPARTMENT OF ENERGY 10 CFR Part 900 RIN 1901-AB18 Coordination of Federal Authorizations for Electric Transmission Facilities AGENCY: Office of Electricity Delivery and Energy Reliability, Department of Energy. ACTION: Notice of proposed rulemaking. SUMMARY: The Department of Energy (DOE) proposes to amend its regulations for the timely coordination of Federal authorizations for proposed interstate electric transmission facilities pursuant to section 216(h) of the Federal Power Act (FPA). The

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    U.S. Department of Energy Office of Inspector General Office of Audits and Inspections Audit Report Department of Energy's Uranium Enrichment Decontamination and Decommissioning Fund's Fiscal Year 2012 Financial Statement Audit OAS-FS-14-07 March 2014 Department of Energy Washington, DC 20585 March 20, 2014 MEMORANDUM FOR THE SENIOR ADVISOR FOR ENVIRONMENTAL MANAGEMENT FROM: Rickey R. Hass Deputy Inspector General for Audits and Inspections Office of Inspector General SUBJECT: INFORMATION:

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    Management of Selected Department of Energy Contractors' Health and Post-Retirement Benefits OAI-M-16-15 August 2016 U.S. Department of Energy Office of Inspector General Office of Audits and Inspections Department of Energy Washington, DC 20585 August 4, 2016 MEMORANDUM FOR THE HEAD OF CONTRACTING ACTIVITY, OFFICE OF SCIENCE ASSOCIATE ADMINISTRATOR FOR ACQUISITION AND PROJECT MANAGEMENT, NATIONAL NUCLEAR SECURITY ADMINISTRATION FROM: Michelle Anderson Assistant Inspector General for Audits and

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    Funding Funding Federal agencies, including the U.S. Department of Energy Office of Indian Energy, provide grant, loan, and technical assistance programs to support tribal energy projects. Find information about past funding opportunities. Current Funding Opportunities Ongoing Opportunities Current Funding Opportunities Close Date Organization Opportunity 8/5/2016 U.S. Department of Agriculture Rural Energy Savings Program The U.S. Department of Agriculture is accepting applications for the

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    Mission Mission To strengthen the integrity, economy, and efficiency of the Department's programs and operations. Vision Statement To be a highly effective organization that promotes positive change.

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    Phonebook Phonebook Search the Energy Department Phonebook Enter your search request * Search Mission Leadership Organization Chart Staff and Contractors News & Blog

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    DEPARTMENT OF ENERGY NATIONAL NUCLEAR SECURITY ADMINISTRATION Draft Site-Wide Environmental Impact Statement for ... The Draft SVEIS for the continued management and operation of ...

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    themselves to Department resources using: digital Identities digital Signatures two-factor authentication tokens For additional information, see the links under "Learn More." ...

  5. Nanotechnology | Department of Energy

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    Nanotechnology Nanotechnology The Department of Energy's Nanotechnology Safety provides a forum for the exchange of best practices, lessons learned, and guidance in the area of ...

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    09 MEMORANDUM FOR THE SECRETARY FROM: Gregory H. Friedman Inspector General SUBJECT: INFORMATION: Report on "The Department of Energy's Fiscal Year 2009 Consolidated Financial...

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    2000-05-26

    Establishes requirements for Department of Energy (DOE) badges. DOE N 251.40, dated 5/3/01, extends this directive until 12/31/01.

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    in the production of clean energy technologies like electric vehicles, LED bulbs and solar panels. The Department is also working with manufacturers to increase their energy...

  9. Fossil | Department of Energy

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    by Daniel Wood, Energy Department. Fossil energy sources, including oil, coal and natural gas, are non-renewable resources that formed when prehistoric plants and animals died...

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    Investments in Carbon Capture Technologies 2011 Department of Energy Investments in Carbon Capture Technologies 2010 Smart Meter Installations 2010 Smart Meter Installations...

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    Wilkins, Energy Department INFOGRAPHIC: How Appliance Standards Help Consumers Save Big Consumers are saving more than 62 billion a year as a result of Appliance and...

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    Melanie A. Kenderdine Director of the Office of Energy Policy and Systems Analysis Melanie A. ... Carol joined the Department of Energy, Energy Efficiency and Renewable Energy (EERE) ...

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    Carolina and Washington, D.C. We analyzed large volumes of documents, including over 150,000 emails, and we identified and reviewed applicable Federal and Department regulations. ...

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    These experts also provide oversight of the Department's Indian Policy implementation, and monitor state, local and tribal energy trends and legislative developments which could ...

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    of the Department's 2010 Agency Financial Report is presented for purposes of additional analysis of the consolidated financial statements rather than to present the financial...

  16. Department of Energy

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

    No. AL 2013-05 Acquisition Regulation Date 050213 Department of Energy No. FAL 2013-03 ... covered by the Federal Acquisition Regulation, unless the Secretary of Energy ...

  17. News | Department of Energy

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

    that will help businesses and communities save money, create jobs, and reduce pollution. May 4, 2015 Energy Department Awards Nearly 10 Million for Efficient Lighting...

  18. Department of Energy

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

    of Energy Order 580.1, Department of Energy Personal Property Management including Policy Flash 2006-21 (Outdated) 2007-01 12152006 Implementation of Functional...

  19. Notices DEPARTMENT OF EDUCATION

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

    Director of the Information Collection Clearance Division, U.S. Department of Education, ... Dated: May 6, 2016. Kate Mullan, Acting Director, Information Collection Clearance ...

  20. Telework | Department of Energy

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

    Telework Telework The Department's telework program is referred to as DOE-Flex. Telework is also referred to as flexiplace and telecommuting. This page includes guidance on ...

  1. Speakers | Department of Energy

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

    Dr. Dan Arvizu Director, National Renewable Energy Laboratory Dr. Dan Arvizu is the Director of the National Renewable Energy Laboratory, the U.S. Department of Energy's primary ...

  2. Blog | Department of Energy

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

    reflective coatings on windows, exterior walls, and roofs to provide comfort during the cooling season. | Photo courtesy of Jason Flakes, U.S. Department of Energy Using Passive...

  3. DEPARTMENT OF ENERGY

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

    Comprehensive Land-Use Plan Environmental Impact Statement AGENCY: Department of Energy ... policies, and (iv) implementing procedures that apply to the review and ...

  4. Mission | Department of Energy

    Office of Environmental Management (EM)

    Mission Mission OSDBU is building sustainable small businesses to enable the Department of Energy to achieve its mission, through innovation and creativity. Sections 8 and 15 of ...

  5. DEPARTMENT OF ENERGY

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

    DEPARTMENT OF ENERGY 10 CFR Part 1021 National Environmental ... room 1E-190, Forrestal Building, 1000 Independence ... that may in any way reveal the identity of offerors. ...

  6. Department of Energy

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

    at Sandia National Laboratories - New Mexico INS-L-11-04 September 2011 Department of ... at Sandia National Laboratories - New Mexico" BACKGROUND Sandia National ...

  7. Vehicles | Department of Energy

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

    To help you save money by saving energy, our experts are answering your home cooling questions. | Photo courtesy of iStockphotoJaniceRichard Energy Department experts answer ...

  8. Activities | Department of Energy

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

    Once member organizations submit their results, the Residential Network will be able to recognize them through a variety of U.S. Department of Energy (DOE) publications, reports, ...

  9. Resources | Department of Energy

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

    The following tools and resources have been useful to Department of Energy (DOE) programs and partners as they build and maintain their residential energy efficiency programs. ...

  10. Mission | Department of Energy

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

    Department including NNSA, the Power Marketing Administrations, and the National Labs); ... efforts, designing effective marketing and branding efforts to attract the ...

  11. STATEOFNEWMEXICO ENVIRONMENT DEPARTMENT ENVIRONMENTAL HEALTH...

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

    STATEOFNEWMEXICO ENVIRONMENT DEPARTMENT ENVIRONMENTAL HEALTH DIVISION, HAZARDOUS WASTE ... OF NEW MEXICO BEFORE THE SECRETARY OF ENVIRONMENT NEW MEXICO ENVIRONMENT DEPARTMENT, ...

  12. Slide 1 | Department of Energy

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

    Capstone Workshop Portfolio Department of Energy Quadrennial Technology Review Clean Electricity Workshop Department of Energy Quadrennial Technology Review Grid Modernization ...

  13. Presentations | Department of Energy

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

    Information Resources » Presentations Presentations Energy Department presentations allow stakeholders to learn and engage around innovative technology development. Source: Geothermal Resources Council Energy Department presentations allow stakeholders to learn and engage around innovative technology development. Source: Geothermal Resources Council Douglas Hollett, former office director for the Geothermal Technologies Office, addresses over 1,000 during his keynote address at the annual

  14. Public Affairs Department

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

    Public Affairs Department Public Affairs Communications Community Public Affairs Org Chart Education Creative Services ⇒ Navigate Section Public Affairs Communications Community Public Affairs Org Chart Education Creative Services The Public Affairs Department serves Berkeley Lab's scientific and educational missions by: Providing timely information and perspective about scientific discoveries to all of the Lab's internal and external audiences, ranging from potential scientific collaborators

  15. Piercing 'The Illusion of Time' | Department of Energy

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

    Piercing 'The Illusion of Time' Piercing 'The Illusion of Time' November 8, 2011 - 5:43pm Addthis <a href="http://www.pbs.org/wgbh/nova/physics/fabric-of-cosmos.html#fabric-time"> "The Illusion of Time"</a> is the second installment in the PBS Nova series, "The Fabric of the Cosmos." | Image courtesy of PBS "The Illusion of Time" is the second installment in the PBS Nova series, "The Fabric of the Cosmos." | Image courtesy of PBS

  16. Contact Hanford Fire Department - Hanford Site

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

    Department Contact Hanford Fire Department Hanford Fire Department Hanford Fire Department Home About Hanford Fire Department Fire and Life Safety Information Hot Links to Cool...

  17. 2006 Department of Energy Strategic Plan | Department of Energy

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

    Plan 2006 Department of Energy Strategic Plan Major DOE Laboratories & Field Facilities, Table of Contents, and Operating Principals 2006 Department of Energy Strategic Plan (2.35 MB) More Documents & Publications U.S Department of Energy Strategic Plan 2006 Department of Energy Strategic Plan - Scientific Discovery and Innovation 2006 Department of Energy Strategic Plan - Linking Strategic Goals to Annual Performance Goals

  18. Electricity | Department of Energy

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

    Department and our partners. June 16, 2014 Ministers Meet in Addis Ababa for U.S.-Africa Energy Ministerial Learn more about the U.S.-Africa Energy Ministerial, held June 3-4,...

  19. Notices DEPARTMENT OF DEFENSE

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

    Surplus Land at a Military Installation Designated for Disposal: Ernest Veuve Hall USARC AMSA 75, T-25, Fort Missoula, Montana AGENCY: Department of the Army, DoD. ACTION: Notice. ...

  20. The Department of Energy

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

    S. Department of ENERGY Draft Workforce Restructuring Plan for the [Name Site] DATE: [Insert Date] WORKFORCE RESTRUCTURING PLAN For the [NAME SITE] Table of Contents I. INTRODUCTION ...................................................................................................................................................... 1 Executive Summary ................................................................................................................................................ 1

  1. Picture | Department of Energy

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

    Picture Picture Picture of a fireplace Picture (62.15 KB) More Documents & Publications Re: Regulatory Burden RFI Regulatory Burden RFI from HPBA Department of Energy Request for Information: Reducing Regulatory Burden (Reply Comments)

  2. Blog | Department of Energy

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

    million gasoline-powered cars off the road. December 17, 2015 Small Business Award to Sage Energy Trading The Department of Energy (DOE) today announced the award of a Firm-Fixed...

  3. Blog | Department of Energy

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

    in April 20, 2015 Energy Department employee Bill Vandermeer tunes a bicycle as part of Earth Day events at National Renewable Energy Laboratory last year. Biking to work can...

  4. Solar | Department of Energy

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

    The Department of Energy's SunShot Initiative funds cutting-edge science that helps dramatically reduce the cost of solar energy. Drawn from diverse inspiration in the optical and ...

  5. Blog | Department of Energy

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

    salute to the Department of Defense for their heroic efforts when it comes to saving electrons. November 10, 2015 An insulated door was an easy upgrade from the steel cellar door...

  6. Department of Energy

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

    Energy.gov Solar Decathlon 2015 Solar Decathlon 2015 The competition is heating up at U.S. Department of Energy Solar Decathlon 2015 Go to energy.govsolardecathlon for full...

  7. Department of Energy

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

    No. AL 2013-08 Acquisition Regulation Date 06192013 Department of Energy No. FAL ... of a violation of any law, rule, or regulation, or mismanagement, a gross waste of ...

  8. News | Department of Energy

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

    their invention of the blue light emitting diode, a game-changer in the history of LED lights. | Photo courtesy of Soraa. Energy-Department Supported Scientist Receives Nobel Prize...

  9. Blog | Department of Energy

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

    7, 2016 Carbon capture is an important part of the Energy Department's Fossil Energy research and development efforts, but it can be hard to understand. This infographic breaks it...

  10. DEPARTMENT OF I Office

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

    DEPARTMENT OF I Office of ENERGY Science SLAC Site Office SLAC National Accelerator Laboratory 2575 Sand Hill Road, MS-8A Menlo Park, CA 94025 DATE: January 11, 2012 MEMORANDUM ...

  11. Department of Energy

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

    ... The Department of Health and Human Services (HHS), the Office of Naval Research (ONR), and the Defense Contract Audit Agency (DCAA), may have audit cognizance for other than DOE ...

  12. MOJAVE | Department of Energy

    Energy Savers [EERE]

    MOJAVE PROJECT SUMMARY In September 2011, the Department of Energy issued a 1.2 billion loan guarantee to finance Mojave, a 250-MW parabolic trough concentrating solar power (CSP) ...

  13. Contacts | Department of Energy

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

    information to contact the State and Local Solution Center by mail or email: U.S. Department of Energy State and Local Solution Center Mail Stop EE-5W 1000 Independence Ave., SW...

  14. Department of Energy

    Energy Savers [EERE]

    Enhancement Act of 2012 2013-09 062813 Revision of Department of Energy (DOE) Order 350.1 and Special H Clause 2013-10 061913 Nondisplacement of Qualified Workers under ...

  15. Kentucky Department of Agriculture

    Broader source: Energy.gov [DOE]

    At the August 7, 2008 quarterly joint Web conference of DOE's Biomass and Clean Cities programs, Wilbur Frye (Office of Consumer & Environmental Protection, Kentucky Department of Agriculture) described Biofuel Quality Testing in Kentucky.

  16. KAHUKU | Department of Energy

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

    KAHUKU PROJECT SUMMARY In July 2010, the Department of Energy issued a 117 million loan guarantee to finance Kahuku, a 30-MW wind power generation project. Located in Kahuku, ...

  17. Contacts | Department of Energy

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

    Contacts Contacts For information about Solid-State Lighting, contact James Brodrick Lighting Program Manager Building Technologies Office U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 1-202-586-5000

  18. Leadership | Department of Energy

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

    Andre H. Sayles, Ph.D., joined the Department of Energy as the Principal Deputy Director ... More about Andre H. Sayles, Ph.D. Neil Schuldenfrei Deputy Director, Office of Civil ...

  19. Department of Energy

    Energy Savers [EERE]

    Electronic Commerce EC-Web Project Plan May 1997 U. S. DEPARTMENT OF ENERGY Assistant ... i May 1997 Title Page Document Name: EC-Web Project Plan Publication Date: May 1997 ...

  20. Biota | Department of Energy

    Energy Savers [EERE]

    Welcome to the U.S. Department of Energy's (DOE) Biota Web site There is increasing ... Purpose of the Web Site This Web site was designed to provide a central access point to ...

  1. Bioenergy | Department of Energy

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

    Sources » Renewable Energy » Bioenergy Bioenergy Biomass is an organic renewable energy source that includes materials such as agriculture and forest residues, energy crops, and algae. Scientists and engineers at the Energy Department and National Laboratories are finding new, more efficient ways to convert biomass into biofuels that can take the place of conventional fuels like gasoline, diesel, and jet fuel. Learn how the Energy Department is working to sustainably transform the nation's

  2. FOIA | Department of Energy

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

    FOIA FOIA OFFICE OF INSPECTOR GENERAL (OIG) FREEDOM OF INFORMATION ACT (FOIA) What is FOIA? FOIA is a law that gives you the right to access information from the federal government. Refer to http://www.foia.gov/ for additional information. How do I submit a FOIA request for OIG information? The FOIA process for the OIG is administered by the Department's Office of Information Resources, Office of Management. For additional information on the Department of Energy FOIA process, refer to Energy

  3. Graphics | Department of Energy

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

    Graphics Graphics The Visual Media Department consists of a team of graphic artists, photographers and visual librarians working together to provide a wide variety of visual media for the Department of Energy. Graphics Offices Forrestal: Room BH-071, (202) 586-2732 Germantown: Room E-065, (301) 903-5165 Graphics@hq.doe.gov Certificates, Plaques and Special Awards Design Presentations Enhance and Print Your Files Exhibits Posters and Banners Brochures, Pamphlets and Handouts If you have need of

  4. Leadership | Department of Energy

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

    Leadership Leadership Rickey R. Hass, CPA Acting Inspector General Rickey R. Hass was named Acting Inspector General for the U.S. Department of Energy effective October 4, 2015. As the Acting Inspector General, he is responsible for a nationwide, independent program of audits, inspections, and law enforcement efforts related to the Department of Energy's programs and operations. More about Rickey Hass Virginia Grebasch Counsel to the Inspector General Virginia Grebasch was appointed Counsel to

  5. Photography | Department of Energy

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

    Photography Photography Photographic services include the Photography Office and the Energy Technology Visuals Collection (ETVC) Visuals Library. Photography Forrestal: Room BH-071 Phone: (202) 586-1350 The Photography Office is a fully digital in-house lab that serves all of the Department of Energy's Facilities. Requesting a photographer for an assignment: The department photographers cover photographic assignments within DOE buildings and other locations. All requests for services must be

  6. Recycling | Department of Energy

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

    Recycling Recycling In support of the Department's goal of implementing environmental sustainability practices across the complex, all DOE employees and contractors should incorporate the three "R's" of wise resource use as a core principle of their daily activities: reduce, reuse, and recycle. The Department's recycling program at Headquarters earns monetary credits from the GSA which is then credited to the Sheila Jo Watkins Memorial Child Development Centers for tuition assistance

  7. Services | Department of Energy

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

    Services Services Secretary Ernest Moniz takes a holistic view to diversity, recognizing that the goal of ensuring equal access to participation in the Department's programs and policies comes through in our workforce, our partners, our research, our policies, our education efforts, and our work with the general public. We invite you to browse our website to learn more about the ways we'd like to work with you to support the mission of the Energy Department. Minority Business and Economic

  8. Terrachanics | Department of Energy

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

    Terrachanics Terrachanics Terrachanics Terrachanics is a puzzle game developed for the public by the Department of Energy. It is designed as a recruitment tool to help drive interest in careers with the department, and inspire the public to learn more about the energy technologies of tomorrow. Reroute energy networks to provide resources to key hotspots! Recover and utilize cutting-edge energy technology to prevent disaster! Command specialized Units to open new energy pathways and implement

  9. Wind | Department of Energy

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

    Wind Wind Wind The United States is home to one of the largest and fastest growing wind markets in the world. To stay competitive in this sector, the Energy Department invests in wind research and development projects, both on land and offshore, to advance technology innovations, create job opportunities and boost economic growth. Moving forward, the U.S. wind industry remains a critical part of the Energy Department's all-of-the-above energy strategy to cut carbon pollution, diversify our

  10. CSKT Department of Energy

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

    CSKT Department of Energy Brian Lipscomb, Director November 15, 2012 1 Salish, Pend' Oreille, and Kootenai * Furthest Inland Salish Speaking Tribes * Southern Most band of Kootenai * Reservation established by Hellgate Treaty of 1855 ~ Steven's Treaty November 15, 2012 2 CSKT - Our Government and Businesses * Tribal Government - Tribal Council - Sovereign Entity with Government-to- government relationship with US - CSKT - 30 Agencies/Departments, 1200 Employees * CSKT has several businesses -

  11. Department of Energy

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

    March 2, 2012 MEMORANDUM TO THE DEPARTMENT OF ENERGY ELECTRICITY ADVISORY COMMITTEE From: Patricia A. Hoffman /s/ Assistant Secretary Office of Electricity Delivery and Energy Reliability Subject: DOE Responses to EAC Work Products I want to thank all members of the Department of Energy's (DOE) Electricity Advisory Committee (EAC) for your hard work during 2011. The work products delivered by the Committee during 2011 are listed below. The purpose of this memo and its attachments is to provide

  12. Multimedia | Department of Energy

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

    Information Resources » Multimedia Multimedia The U.S. Department of Energy (DOE) Wind Program is committed to developing and deploying a portfolio of innovative technologies for renewable, domestic power generation to support an ever-growing industry. In support of the President's strategy to diversify our nation's clean energy mix, an elite team of researchers, academics, scientists, engineers, and wind industry experts revisited the findings of the Energy Department's 2008 20% Wind by 2030

  13. News | Department of Energy

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

    News News News July 13, 2016 Department of Energy Cites BWXT Conversion Services, LLC for Worker Safety and Health Program Violations The U.S. Department of Energy (DOE) today issued a Preliminary Notice of Violation (PNOV) to BWXT Conversion Services, LLC (BWCS) for violations of DOE worker safety and health requirements. DOE's enforcement program holds contractors accountable for meeting regulatory requirements and maintaining a safe and healthy workplace. September 2, 2015 Nuclear Executive

  14. Abengoa | Department of Energy

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

    Abengoa Abengoa Abengoa Abengoa's biorefinery in Hugoton, Kansas, is the third cellulosic ethanol facility co-funded by the U.S. Department of Energy (DOE) to begin production at commercial scale since July 2013. The Department provides cost-shared funding to these first-of-a-kind facilities to help drive down technical risk and foster private investment in the growing U.S. bioeconomy. Abengoa designed and built the Kansas facility around an enzymatic hydrolysis process that was evaluated for

  15. Assessments | Department of Energy

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

    Assessments Assessments The Department of Energy's (DOE) Enterprise Assessments programs provide DOE line management, Congress, and other stakeholders with an independent evaluation of the effectiveness of DOE policy and line management performance in safety and security, and other critical areas as directed by the Secretary of Energy. This information provides assurance to our stakeholders and identifies areas for improvement to our leadership to support the safe performance of the Department's

  16. DEPARTMENT OF ENERGY

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

    DEPARTMENT OF ENERGY Record of Decision in re Application of Clean Line Energy Partners LLC AGENCY: Department of Energy. ACTION: Record of Decision. SUMMARY: Section 1222 of the Energy Policy Act of 2005 (EPAct 2005) grants the Secretary of Energy the authority to design, develop, construct, operate, maintain, or own, or participate with other entities in designing, developing, constructing, operating, maintaining, and owning new electric power transmission facilities and related facilities

  17. | Department of Energy

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

    5, 2015 1. Introduction The Department of Energy (DOE) sees the implementation of the Plain Writing Act as an important initiative that helps the Department share relevant information in a way that is clear, concise, and informative. The areas referenced in this report summarize some of our successes - particularly in providing Plain Language Training to employees and contractors (Part VI) - as we continue to implement the Act. 1. Departmental Plain Writing Officials 2. Ingrid Kolb, Director of

  18. Contractors | Department of Energy

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

    Contractors Contractors The U.S. Department of Energy's Oak Ridge Office of Environmental Management uses three prime contractors to conduct its major cleanup projects at the site. These companies include URS|CH2M Oak Ridge LLC (UCOR), North Wind Solutions LLC, and Isotek Systems LLC. UCOR is the Department of Energy's primary cleanup contractor for the DOE Oak Ridge Reservation, primarily focused on cleanup of East Tennessee Technology Park (the former Oak Ridge K-25 Site). UCOR is also engaged

  19. Enforcement | Department of Energy

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

    Enforcement Enforcement The Department of Energy's (DOE) Office of Enforcement promotes overall improvement in the Department's safety and security programs through management and implementation of the DOE enforcement programs for safety and classified information security that are authorized by the Atomic Energy Act. The office is independent of the DOE offices that develop and implement policy and programs. The office conducts enforcement investigations using systematic enforcement practices

  20. Environment | Department of Energy

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

    Environment Environment Environment The U. S. Department of Energy (DOE) complies with all applicable environmental laws and regulations and establishes its own environmental requirements to ensure workers, the public, and the environment is protected from hazards associated with all Department operations. DOE provides assistance to the field to implement these policies, works in resolving environmental protection issues, and provides feedback to enhance environmental performance throughout the

  1. U.S. DEPARTMENT OF ENERGYCONTRACT AND PROJECT MANAGEMENT | Department...

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

    U.S. DEPARTMENT OF ENERGYCONTRACT AND PROJECT MANAGEMENT U.S. DEPARTMENT OF ENERGYCONTRACT AND PROJECT MANAGEMENT U.S. DEPARTMENT OF ENERGY CONTRACT AND PROJECT MANAGEMENT PDF icon...

  2. Protecting Whistleblowers at the Department of Energy | Department of

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

    Energy Protecting Whistleblowers at the Department of Energy Protecting Whistleblowers at the Department of Energy August 4, 2016 - 5:14pm Addthis Employees and contractors are at the heart of the Department of Energy's mission areas -- and the Department is committed to protecting them against retaliation for raising concerns about health, safety and management issues. | Energy Department file photo. Employees and contractors are at the heart of the Department of Energy's mission areas --

  3. Department of the Navy Bioeconomy Activity | Department of Energy

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

    Department of the Navy Bioeconomy Activity Department of the Navy Bioeconomy Activity Plenary V: Federal Activities in the Bioeconomy Department of the Navy Bioeconomy Activity Chris Tindal, Director for Operational Energy, U.S. Department of Navy tindal_biomass_2014.pdf (2.47 MB) More Documents & Publications Department of the Navy, DPA Presentation U.S. Department of the Navy: Driving Alternative Fuels Adoption US Navy Tactical Fuels From Renewable Sources Program

  4. Department of Energy Response to Hurricane Katrina | Department...

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

    PDF icon Department of Energy Response to Hurricane Katrina More Documents & Publications Fact Sheet Department of Energy Response to Hurricane Katrina PRICE GOUGING PRICE GOUGING

  5. U.S. Department of Energy Booth Education Sessions | Department...

    Energy Savers [EERE]

    U.S. Department of Energy Booth Education Sessions U.S. Department of Energy Booth Education Sessions PDF icon Detailed Agenda More Documents & Publications SSL TECHNOLOGY...

  6. Department of Energy Record of Invention Form | Department of...

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

    More Documents & Publications DEPARTMENT OF ENERGY NONEXCLUSIVE PATENT LICENSE APPLICATION DEPARTMENT OF ENERGY EXCLUSIVE OR PARTIALLY EXCLUSIVE PATENT LICENSE APPLICATION Petition ...

  7. Energy Department Helps Advance Island Clean Energy Goals | Department...

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

    Department Helps Advance Island Clean Energy Goals Energy Department Helps Advance Island Clean Energy Goals Highlights a solar power purchase agreement between the Virgin Islands ...

  8. Women @ Energy: Robyn Madrak Plant | Department of Energy

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

    Robyn Madrak Plant Women @ Energy: Robyn Madrak Plant March 12, 2013 - 9:39am Addthis Dr. Robyn Madrak Plant is an Associate Scientist at Fermilab, working at the Accelerator Physics Center on the accelerator RF upgrades for the NOVA experiment. Dr. Robyn Madrak Plant is an Associate Scientist at Fermilab, working at the Accelerator Physics Center on the accelerator RF upgrades for the NOVA experiment. Dr. Robyn Madrak Plant is an Associate Scientist at Fermilab, working at the Accelerator

  9. 'What is Space?': Full of Possibilities | Department of Energy

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

    'What is Space?': Full of Possibilities 'What is Space?': Full of Possibilities November 2, 2011 - 10:21am Addthis Host Brian Greene explores the possibilities of space in tonight's premiere episode of PBS NOVA's "The Fabric of the Cosmos." Host Brian Greene explores the possibilities of space in tonight's premiere episode of PBS NOVA's "The Fabric of the Cosmos." Charles Rousseaux Charles Rousseaux Senior Communications Specialist (detailee) How can I watch? Check your local

  10. EERE News | Department of Energy

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

    January 30, 2013 Energy Department Announces New SunShot Projects to Harness the Power of Big Data As part of the Energy Department's SunShot Initiative, the Department announced...