National Library of Energy BETA

Sample records for aurora wal mart

  1. Reviewers required major changes, including rearranging the two articles, so the new title of the first paper is: HVAC and Refrigeration Experiments at Wal-Mart Experimental Supercenters in Texas and Colorado --- original title: ASHRAE Journal DRAFT article McKinney and Aurora Wal-Mart Stores, Part 1

    SciTech Connect (OSTI)

    MacDonald, J Michael; Deru, Michael

    2007-01-01

    In 2005, Wal-Mart opened experimental stores in McKinney, Texas (hot climate), and Aurora, Colo. (cold climate). With these projects Wal-Mart can: * Learn how to achieve sustainability improvements; * Gain experience with the design, design process, and operations for some specific advanced technologies; * Understand energy use patterns in their stores more clearly; * Lay groundwork for better understanding of how to achieve major carbon footprint reductions; and * Measure the potential benefits of specific technologies tested.

  2. McKinney Wal-Mart Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    Type Small Scale Wind Facility Status In Service Owner Wal-Mart Developer Bergey Windpower Energy Purchaser Wal-Mart Location McKinney TX Coordinates 33.220625, -96.630571...

  3. Aurora Wal Mart Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    GW Number of Units 1 Commercial Online Date 2005 Wind Turbine Manufacturer Bergey Windpower References WENDI1 Loading map... "minzoom":false,"mappingservice":"googlemaps3","...

  4. Cam Wal Electric Coop, Inc | Open Energy Information

    Open Energy Info (EERE)

    Cam Wal Electric Coop, Inc Jump to: navigation, search Name: Cam Wal Electric Coop, Inc Place: South Dakota Phone Number: 605.649.7676 Website: www.cam-walnet.com Facebook:...

  5. Aurora final report

    SciTech Connect (OSTI)

    Robert, Dross; Amedeo, Conti

    2013-12-06

    Final Technical report detailing the work done by Nuvera and its partners to fulfill the goals of the program "Transport Studies Enabling Efficiency Optimization of Cost-Competitive Fuel Cell Stacks" (a.k.a. AURORA)

  6. Aurora Cooperative | Open Energy Information

    Open Energy Info (EERE)

    to: navigation, search Name: Aurora Cooperative Place: Nebraska Zip: 68818 Product: Agricultural cooperative focused on providing service and expertise in grain, agronomy, feed and...

  7. Aurora Geothermal Area | Open Energy Information

    Open Energy Info (EERE)

    Aurora Geothermal Area Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Aurora Geothermal Area Contents 1 Area Overview 2 History and Infrastructure 3 Regulatory and...

  8. OLED Lighting in the Offices of Aurora Lighting Design, Inc.

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

    the Offices of Aurora Lighting Design, Inc. DOE Booth Pacific Northwest National Laboratory Leslie North, DesignerPrincipal Aurora Lighting Design, Inc. 2 OLED Lighting at Aurora ...

  9. Aurora Supercomputer Press Conference | Argonne National Laboratory

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

    Contact Us For more information, contact Brian Grabowski at media@anl.gov or (630) 252-1232. Aurora Supercomputer Press Conference Aurora Supercomputer Press Conference 1 of 19 Aurora Supercomputer Press Conference On April 9, 2015, the Department of Energy held a press conference along with Argonne, Intel & Cray to announce a $200 million investment to deliver a next-generation supercomputer, known as Aurora, to the Argonne Leadership Computing Facility. When commissioned in 2018, this

  10. Structure and mechanism of the essential two-component signal-transduction system WalKR in Staphylococcus aureus

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

    Ji, Quanjiang; Chen, Peter J.; Qin, Guangrong; Deng, Xin; Hao, Ziyang; Wawrzak, Zdzislaw; Yeo, Won -Sik; Quang, Jenny Winjing; Cho, Hoonsik; Luo, Guan -Zheng; et al

    2016-03-18

    Most low GC Gram-positive bacteria possess an essential walKR two-component system (TCS) for signal transduction involved in regulating cell wall homoeostasis. Despite the well-established intracellular regulatory mechanism, the role of this TCS in extracellular signal recognition and factors that modulate the activity of this TCS remain largely unknown. Here we identify the extracellular receptor of the kinase ‘WalK’ (erWalK) as a key hub for bridging extracellular signal input and intracellular kinase activity modulation in Staphylococcus aureus. Characterization of the crystal structure of erWalK revealed a canonical Per-Arnt-Sim (PAS) domain for signal sensing. Single amino-acid mutation of potential signal-transduction residues resultedmore » in severely impaired function of WalKR. A small molecule derived from structure-based virtual screening against erWalK is capable of selectively activating the walKR TCS. Lastly, the molecular level characterization of erWalK will not only facilitate exploration of natural signal(s) but also provide a template for rational design of erWalK inhibitors.« less

  11. Introducing Aurora | Argonne Leadership Computing Facility

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

    Aurora Announcement Press Conference: DOE announces next-gen supercomputer Aurora to be built at Argonne Introducing Aurora Author: ALCF staff April 9, 2015 Facebook Twitter LinkedIn Google E-mail Printer-friendly version Today, U.S. Department of Energy Under Secretary for Science and Energy Lynn Orr announced two new High Performance Computing (HPC) awards that continue to advance U.S. leadership in developing exascale computing. The announcement was made alongside leaders from Argonne

  12. Aurora Photovoltaics Manufacturing | Open Energy Information

    Open Energy Info (EERE)

    Photovoltaics Manufacturing Jump to: navigation, search Name: Aurora Photovoltaics Manufacturing Place: Lawrenceville, New Jersey Zip: 8648 Sector: Solar Product: A subsidiary of...

  13. Aurora Early Science Program: Call for Proposals opens today...

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

    Aurora Early Science Program: Call for Proposals opens today Author: ALCF staff July 6, ... accepting proposals for its Aurora Early Science Program (ESP) through September 2, 2016. ...

  14. Aurora Early Science Program Proposal Instructions | Argonne Leadership

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

    Computing Facility Early Science Program Aurora ESP Call for Proposals Aurora ESP Proposal Instructions INCITE Program ALCC Program Director's Discretionary (DD) Program ALCF Data Science Program INCITE 2016 Projects ALCC 2015 Projects ESP Projects View All Projects Publications ALCF Tech Reports Industry Collaborations Aurora Early Science Program Proposal Instructions Aurora ESP General Information and Submission Instructions Our intent is for Aurora Early Science Program (ESP) proposals

  15. Aurora ESP Call for Proposals | Argonne Leadership Computing Facility

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

    Early Science Program Aurora ESP Call for Proposals Aurora ESP Proposal Instructions INCITE Program ALCC Program Director's Discretionary (DD) Program ALCF Data Science Program INCITE 2016 Projects ALCC 2015 Projects ESP Projects View All Projects Publications ALCF Tech Reports Industry Collaborations Aurora ESP Call for Proposals Aurora ESP In late 2018, the Argonne Leadership Computing Facility (ALCF) will deploy Aurora, a new Intel-Cray system based on the third-generation Intel® Xeon

  16. Aurora

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

    that benefit humanity the most. From finding alternative energy sources to treating diseases to developing high-tech materials-the research done on leadership-class machines...

  17. Carbon Sequestration Documentary Wins Coveted Aurora Award

    Broader source: Energy.gov [DOE]

    A film about carbon sequestration produced with support from the U.S. Department of Energy has received a 2009 Gold Aurora Award in the documentary category for nature/environment.

  18. Aurora Energy Co Ltd | Open Energy Information

    Open Energy Info (EERE)

    (Republic) Sector: Solar, Wind energy Product: Manufacturer of 1-225kW micro wind turbines and solar modules. References: Aurora Energy Co Ltd1 This article is a stub. You...

  19. Aurora, Colorado: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Hide Map This article is a stub. You can help OpenEI by expanding it. Aurora is a city in Adams County and Arapahoe County and Douglas County, Colorado. It falls under Colorado's...

  20. Aurora, Colorado: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Map This article is a stub. You can help OpenEI by expanding it. Aurora is a city in Adams County and Arapahoe County and Douglas County, Colorado. It falls under Colorado's 7th...

  1. Evaluation of the Aurora Application Shade Measurement Accuracy

    SciTech Connect (OSTI)

    2015-12-01

    Aurora is an integrated, Web-based application that helps solar installers perform sales, engineering design, and financial analysis. One of Aurora's key features is its high-resolution remote shading analysis.

  2. GATEWAY Demonstrations: OLED Lighting in the Offices of Aurora...

    Energy Savers [EERE]

    in the Offices of Aurora Lighting Design, Inc. March 2016 Prepared for: Solid-State Lighting Program Building Technologies Office Office of Energy Efficiency and Renewable Energy ...

  3. Aurora BioFuels Inc | Open Energy Information

    Open Energy Info (EERE)

    BioFuels Inc Jump to: navigation, search Name: Aurora BioFuels Inc. Place: Alameda, California Zip: 94502 Sector: Biofuels, Renewable Energy Product: California-based renewable...

  4. Analysis of Aurora's Performance Simulation Engine for Three Systems

    SciTech Connect (OSTI)

    Freeman, Janine; Simon, Joseph

    2015-07-07

    Aurora Solar Inc. is building a cloud-based optimization platform to automate the design, engineering, and permit generation process of solar photovoltaic (PV) installations. They requested that the National Renewable Energy Laboratory (NREL) validate the performance of the PV system performance simulation engine of Aurora Solar’s solar design platform, Aurora. In previous work, NREL performed a validation of multiple other PV modeling tools 1, so this study builds upon that work by examining all of the same fixed-tilt systems with available module datasheets that NREL selected and used in the aforementioned study. Aurora Solar set up these three operating PV systems in their modeling platform using NREL-provided system specifications and concurrent weather data. NREL then verified the setup of these systems, ran the simulations, and compared the Aurora-predicted performance data to measured performance data for those three systems, as well as to performance data predicted by other PV modeling tools.

  5. OLED Lighting in the Offices of Aurora Lighting Design, Inc. | Department

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

    of Energy in the Offices of Aurora Lighting Design, Inc. OLED Lighting in the Offices of Aurora Lighting Design, Inc. Aurora OLED Report (March 2016) (1.71 MB) Aurora OLED Report Brief (May 2016) (1.21 MB) More Documents & Publications OLED Lighting Products: Capabilities, Challenges, Potential May 2016 Postings OLED Lighting Products Webinar Presentation Slides

  6. Press Conference: DOE announces next-gen supercomputer Aurora...

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

    Brian Grabowski at media@anl.gov or (630) 252-1232. Press Conference: DOE announces next-gen supercomputer Aurora to be built at Argonne Share Topic Programs Mathematics,...

  7. SSL EVALUATION: OLED Lighting in the Offices of Aurora Lighting...

    Energy Savers [EERE]

    EVALUATION: OLED Lighting in the Offices of Aurora Lighting Design, Inc. The first GATEWAY demonstra- tion involving OLEDs is also the first office test site for the use of OLEDs ...

  8. PROJECT PROFILE: Aurora Solar Inc. (Incubator 10) | Department...

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

    As part of the Department of Energy's SunShot Incubator program, Aurora will be developing a web-based application that quickly and precisely calculates the solar potential of a ...

  9. Regional Partnership Documentary Wins "Best of Show" Aurora Award

    Broader source: Energy.gov [DOE]

    A documentary co-produced by Prairie Public Broadcasting and the Plains CO2 Reduction (PCOR) Partnership with support from the U.S. Department of Energy has received a 2012 Platinum Best of Show Aurora Award—the highest honor awarded—in the nature/environment documentary category.

  10. Students from Aurora Triumph in Denver Regional Science Bowl

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

    Denver Regional Science Bowl For more information contact: e:mail: Public Affairs Golden, Colo., Feb. 27, 1999 — Students from Aurora's Smoky Hill High School won top honors at the 1999 Denver Regional Science Bowl today at the Colorado School of Mines in Golden. In the final round of rapid-fire questions about physics, math, biology, astronomy, chemistry, computers and the earth sciences, students from Smoky Hill High School were victorious over Highlands Ranch High School. Twenty-one student

  11. Aurora Early Science Program: Call for Proposals is now open | Argonne

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

    Leadership Computing Facility Aurora Early Science Program: Call for Proposals is now open Author: ALCF staff July 6, 2016 Facebook Twitter LinkedIn Google E-mail Printer-friendly version The Argonne Leadership Computing Facility (ALCF) is now accepting proposals for its Aurora Early Science Program (ESP) through September 2, 2016. Aurora is a pre-exascale supercomputer expected to arrive at Argonne National Laboratory in 2018. The ALCF is a U.S. Department of Energy (DOE) Office of Science

  12. ITER Diagnostic First Wal

    SciTech Connect (OSTI)

    G. Douglas Loesser, et. al.

    2012-09-21

    The ITER Diagnostic Division is responsible for designing and procuring the First Wall Blankets that are mounted on the vacuum vessel port plugs at both the upper and equatorial levels This paper will discuss the effects of the diagnostic aperture shape and configuration on the coolant circuit design. The DFW design is driven in large part by the need to conform the coolant arrangement to a wide variety of diagnostic apertures combined with the more severe heating conditions at the surface facing the plasma, the first wall. At the first wall, a radiant heat flux of 35W/cm2 combines with approximate peak volumetric heating rates of 8W/cm3 (equatorial ports) and 5W/cm3 (upper ports). Here at the FW, a fast thermal response is desirable and leads to a thin element between the heat flux and coolant. This requirement is opposed by the wish for a thicker FW element to accommodate surface erosion and other off-normal plasma events.

  13. Kim Saylors-Laster | Department of Energy

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

    Kim Saylors-Laster About Us Kim Saylors-Laster - Vice President of Energy, Wal-Mart Stores Most Recent Advancing Women in Clean Energy July 24...

  14. June 11 & 12, 2012 Meeting of the Electricity Advisory Committee...

    Energy Savers [EERE]

    Tuesday, June 12, 2012 Microgrids Panel - Ralph Masiello, EAC Storage Subcommittee Chair Jeff Marqusee, DODOSD Will Agate, Philadelphia Navy Yard Angie Beehler, WalMart ...

  15. Possible anticorrelation of polar mesospheric (noctilucent) clouds and aurorae. Master's thesis

    SciTech Connect (OSTI)

    Carr, S.S.

    1986-08-01

    The study of noctilucent clouds (NLC) is one century old, yet the origin and nature of these clouds is still uncertain. It is known that these clouds form in the cold, high latitude summer mesopause region where temperatures can approach 110K. Their association with the very cold air in this region supports the theory that they consist of water ice particles. It has been suggested that NLC are anticorrelated with aurorae since aurorally induced effects at or near the mesopause may lead to processes which retard or altogether inhibit NLC formation. This study reviews some general characteristics of NLC, polar mesospheric clouds (PMC) and aurorae and then discusses several ways in which aurorae may interact with these clouds.

  16. OSTIblog Articles in the auroras Topic | OSTI, US Dept of Energy Office of

    Office of Scientific and Technical Information (OSTI)

    Scientific and Technical Information auroras Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers often call it the

  17. Energetic electron precipitation associated with pulsating aurora: EISCAT and Van Allen Probe observations

    SciTech Connect (OSTI)

    Miyoshi, Y.; Oyama, S.; Saito, S.; Kurita, S.; Fujiwara, H.; Kataoka, R.; Ebihara, Y.; Kletzing, C.; Reeves, G.; Santolik, O.; Clilverd, M.; Rodger, C. J.; Turunen, E.; Tsuchiya, F.

    2015-04-21

    Pulsating auroras show quasi-periodic intensity modulations caused by the precipitation of energetic electrons of the order of tens of keV. It is expected theoretically that not only these electrons but also subrelativistic/relativistic electrons precipitate simultaneously into the ionosphere owing to whistler mode wave-particle interactions. The height-resolved electron density profile was observed with the European Incoherent Scatter (EISCAT) Tromsø VHF radar on 17 November 2012. Electron density enhancements were clearly identified at altitudes >68 km in association with the pulsating aurora, suggesting precipitation of electrons with a broadband energy range from ~10 keV up to at least 200 keV. The riometer and network of subionospheric radio wave observations also showed the energetic electron precipitations during this period. During this period, the footprint of the Van Allen Probe-A satellite was very close to Tromsø and the satellite observed rising tone emissions of the lower band chorus (LBC) waves near the equatorial plane. Considering the observed LBC waves and electrons, we conducted a computer simulation of the wave-particle interactions. This showed simultaneous precipitation of electrons at both tens of keV and a few hundred keV, which is consistent with the energy spectrum estimated by the inversion method using the EISCAT observations. This result revealed that electrons with a wide energy range simultaneously precipitate into the ionosphere in association with the pulsating aurora, providing the evidence that pulsating auroras are caused by whistler chorus waves. We suggest that scattering by propagating whistler simultaneously causes both the precipitations of subrelativistic electrons and the pulsating aurora.

  18. Energetic electron precipitation associated with pulsating aurora: EISCAT and Van Allen Probe observations

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

    Miyoshi, Y.; Oyama, S.; Saito, S.; Kurita, S.; Fujiwara, H.; Kataoka, R.; Ebihara, Y.; Kletzing, C.; Reeves, G.; Santolik, O.; et al

    2015-04-21

    Pulsating auroras show quasi-periodic intensity modulations caused by the precipitation of energetic electrons of the order of tens of keV. It is expected theoretically that not only these electrons but also subrelativistic/relativistic electrons precipitate simultaneously into the ionosphere owing to whistler mode wave-particle interactions. The height-resolved electron density profile was observed with the European Incoherent Scatter (EISCAT) Tromsø VHF radar on 17 November 2012. Electron density enhancements were clearly identified at altitudes >68 km in association with the pulsating aurora, suggesting precipitation of electrons with a broadband energy range from ~10 keV up to at least 200 keV. The riometermore » and network of subionospheric radio wave observations also showed the energetic electron precipitations during this period. During this period, the footprint of the Van Allen Probe-A satellite was very close to Tromsø and the satellite observed rising tone emissions of the lower band chorus (LBC) waves near the equatorial plane. Considering the observed LBC waves and electrons, we conducted a computer simulation of the wave-particle interactions. This showed simultaneous precipitation of electrons at both tens of keV and a few hundred keV, which is consistent with the energy spectrum estimated by the inversion method using the EISCAT observations. This result revealed that electrons with a wide energy range simultaneously precipitate into the ionosphere in association with the pulsating aurora, providing the evidence that pulsating auroras are caused by whistler chorus waves. We suggest that scattering by propagating whistler simultaneously causes both the precipitations of subrelativistic electrons and the pulsating aurora.« less

  19. Characteristics of optical emissions and particle precipitation in mid/low-latitude aurorae

    SciTech Connect (OSTI)

    Rassoul K., H.R.

    1987-01-01

    Ground-based optical observations have been made at low/mid latitudes to study the auroral effects of particle precipitation. The measured optical emissions include (OI) 5577 {Angstrom}, (OI) 6300 {Angstrom}, and (OI) 7774 {Angstrom} of atomic oxygen, the Balmer-{beta} line of Hydrogen at 4861 {Angstrom}; and the emission bands from the first negative nitrogen system at 3914 {Angstrom} and 4278 {Angstrom}. Spectral characteristics of low-latitude aurorae, the correlation of optical data with geomagnetic field variations, and the nature of the precipitating particles were established. The observed auroral emissions have characteristics appropriate to the precipitation into the thermosphere of heavy energetic (keV energy) particles and/or electrons of energy of the order of eV rather than the keV electron precipitation as in the high-latitude auroral zone. The latitude variation of optical emissions shows a strong increase from low to mid latitudes, and the strongest emissions occur in the evening to midnight local time period. The particle precipitation enhances at times when there is a populated and/or energized ring current and there exists a strong magnetic perturbation near the local meridian of the precipitation.

  20. AURORA: A FORTRAN program for modeling well stirred plasma and thermal reactors with gas and surface reactions

    SciTech Connect (OSTI)

    Meeks, E.; Grcar, J.F.; Kee, R.J.; Moffat, H.K.

    1996-02-01

    The AURORA Software is a FORTRAN computer program that predicts the steady-state or time-averaged properties of a well mixed or perfectly stirred reactor for plasma or thermal chemistry systems. The software was based on the previously released software, SURFACE PSR which was written for application to thermal CVD reactor systems. AURORA allows modeling of non-thermal, plasma reactors with the determination of ion and electron concentrations and the electron temperature, in addition to the neutral radical species concentrations. Well stirred reactors are characterized by a reactor volume, residence time or mass flow rate, heat loss or gas temperature, surface area, surface temperature, the incoming temperature and mixture composition, as well as the power deposited into the plasma for non-thermal systems. The model described here accounts for finite-rate elementary chemical reactions both in the gas phase and on the surface. The governing equations are a system of nonlinear algebraic relations. The program solves these equations using a hybrid Newton/time-integration method embodied by the software package TWOPNT. The program runs in conjunction with the new CHEMKIN-III and SURFACE CHEMKIN-III packages, which handle the chemical reaction mechanisms for thermal and non-thermal systems. CHEMKIN-III allows for specification of electron-impact reactions, excitation losses, and elastic-collision losses for electrons.

  1. Correlated Pc4-5 ULF waves, whistler-mode chorus, and pulsating aurora observed by the Van Allen Probes and ground-based systems

    SciTech Connect (OSTI)

    Jaynes, A. N.; Lessard, M. R.; Takahashi, K.; Ali, A. F.; Malaspina, D. M.; Michell, R. G.; Spanswick, E. L.; Baker, D. N.; Blake, J. B.; Cully, C.; Donovan, E. F.; Kletzing, C. A.; Reeves, G. D.; Samara, M.; Spence, H. E.; Wygant, J. R.

    2015-10-28

    Theory and observations have linked equatorial VLF waves with pulsating aurora for decades, invoking the process of pitch angle scattering of tens of keV electrons in the equatorial magnetosphere. Recently published satellite studies have strengthened this argument, by showing strong correlation between pulsating auroral patches and both lower-band chorus and tens of keV electron modulation in the vicinity of geosynchronous orbit. Additionally, a previous link has been made between Pc4–5 compressional pulsations and modulation of whistler-mode chorus using Time History of Events and Macroscale Interactions during Substorms. In the current study, we present simultaneous in situ observations of structured chorus waves and an apparent field line resonance (in the Pc4–5 range) as a result of a substorm injection, observed by Van Allen Probes, along with ground-based observations of pulsating aurora. We demonstrate the likely scenario being one of substorm-driven Pc4–5 ULF pulsations modulating chorus waves, and thus providing the driver for pulsating particle precipitation into the Earth's atmosphere. Interestingly, the modulated chorus wave and ULF wave periods are well correlated, with chorus occurring at half the periodicity of the ULF waves. We also show, for the first time, a particular few-Hz modulation of individual chorus elements that coincides with the same modulation in a nearby pulsating aurora patch. As a result, such modulation has been noticed as a high-frequency component in ground-based camera data of pulsating aurora for decades and may be a result of nonlinear chorus wave interactions in the equatorial region.

  2. Correlated Pc4-5 ULF waves, whistler-mode chorus, and pulsating aurora observed by the Van Allen Probes and ground-based systems

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

    Jaynes, A. N.; Lessard, M. R.; Takahashi, K.; Ali, A. F.; Malaspina, D. M.; Michell, R. G.; Spanswick, E. L.; Baker, D. N.; Blake, J. B.; Cully, C.; et al

    2015-10-28

    Theory and observations have linked equatorial VLF waves with pulsating aurora for decades, invoking the process of pitch angle scattering of tens of keV electrons in the equatorial magnetosphere. Recently published satellite studies have strengthened this argument, by showing strong correlation between pulsating auroral patches and both lower-band chorus and tens of keV electron modulation in the vicinity of geosynchronous orbit. Additionally, a previous link has been made between Pc4–5 compressional pulsations and modulation of whistler-mode chorus using Time History of Events and Macroscale Interactions during Substorms. In the current study, we present simultaneous in situ observations of structured chorusmore » waves and an apparent field line resonance (in the Pc4–5 range) as a result of a substorm injection, observed by Van Allen Probes, along with ground-based observations of pulsating aurora. We demonstrate the likely scenario being one of substorm-driven Pc4–5 ULF pulsations modulating chorus waves, and thus providing the driver for pulsating particle precipitation into the Earth's atmosphere. Interestingly, the modulated chorus wave and ULF wave periods are well correlated, with chorus occurring at half the periodicity of the ULF waves. We also show, for the first time, a particular few-Hz modulation of individual chorus elements that coincides with the same modulation in a nearby pulsating aurora patch. As a result, such modulation has been noticed as a high-frequency component in ground-based camera data of pulsating aurora for decades and may be a result of nonlinear chorus wave interactions in the equatorial region.« less

  3. LRD-22, a novel dual dithiocarbamatic acid ester, inhibits Aurora-A kinase and induces apoptosis and cell cycle arrest in HepG2 cells

    SciTech Connect (OSTI)

    Wang, Huiling; Li, Ridong; Li, Li; Ge, Zemei; Zhou, Rouli; Li, Runtao

    2015-02-27

    In this study we investigated the antitumor activity of the novel dual dithiocarbamatic acid ester LRD-22 in vitro and in vivo. Several cancer cell lines were employed to determine the effect of LRD-22 on cell growth, and the MTT assay showed there was a significant decrease in viable tumor cell numbers in the presence of LRD-22, especially in the HepG2 cell line. Colony formation assay also showed LRD-22 strongly inhibits HepG2 cell growth. Evaluation of the mechanism involved showed that inhibitory effects of LRD-22 on cell growth are due to induction of apoptosis and G2/M arrest. LRD-22 inhibited Aurora-A phosphorylation at Thr{sub 288} and subsequently impaired p53 phosphorylation at Ser{sub 315} which was associated with the proteasome degradation pathway. Tumor suppressor protein p53 is stabilized by this mechanism and accumulates through inhibition of Aurora-A kinase activity via treatment with LRD-22. In vivo study of HepG2 xenograft in nude mice also shows LRD-22 suppresses tumor growth at a concentration of 5 mg/kg without animals suffering loss of body weight. In conclusion, our results demonstrate LRD-22 acts as an Aurora-A kinase inhibitor to induce apoptosis and inhibit proliferation in HepG2 cells, and should be considered as a promising targeting agent for HCC therapy. - Highlights: • LRD-22 significantly inhibits cancer cell growth, especially in the HepG2 cell line. • The inhibitory effect of LRD-22 is due to induction of apoptosis and cell cycle arrest. • LRD-22 inhibits Aurora-A phosphorylation which results in subsequent impairment of the p53 pathway. • LRD-22 suppresses tumor growth in xenograft mice without body weight loss.

  4. A direct link between chorus emissions and pulsating aurora on timescales from milliseconds to minutes: A case study at subauroral latitudes

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

    Ozaki, Mitsunori; Yagitani, Satoshi; Sawai, Kaoru; Shiokawa, Kazuo; Miyoshi, Yoshizumi; Kataoka, Ryuho; Ieda, Akimasa; Ebihara, Yusuke; Connors, Martin; Schofield, Ian; et al

    2015-11-27

    A correlation was observed between chorus emissions and pulsating aurora (PA) from observations at Athabasca (L ≈ 4.3) in Canada at 9:00–9:20 UT on 7 February 2013, using an electron multiplying charge-coupled device camera and a VLF loop antenna with sampling rates of 110 Hz and 100 kHz, respectively. Pulsating aurora having a quasiperiodic variation in luminosity and a few hertz modulation was observed together with chorus emissions consisting of a group of successive rising-tone elements. The repetition period and modulation frequency of the PA are in good agreement with those of the modulated chorus. After 9:11 UT, the temporalmore » features of the aurora became aperiodic PA of indistinct modulation. Simultaneously, the rising-tone chorus turned into chorus emissions consisting of numerous rising-tone elements. The equatorial geomagnetic field inhomogeneity calculated using the Tsyganenko 2002 model shows a decreasing trend during the period. This result is consistent with nonlinear wave growth theory having a small geomagnetic field inhomogeneity, which contributes to a decrease in the threshold amplitude to trigger discrete chorus elements. As a result, these observations show a close connection between chorus emissions and PA on timescales from milliseconds for generation of discrete chorus elements on the microphysics of wave-particle interaction to minutes for the variations of the geomagnetic field inhomogeneity related with the substorm activity.« less

  5. A direct link between chorus emissions and pulsating aurora on timescales from milliseconds to minutes: A case study at subauroral latitudes

    SciTech Connect (OSTI)

    Ozaki, Mitsunori; Yagitani, Satoshi; Sawai, Kaoru; Shiokawa, Kazuo; Miyoshi, Yoshizumi; Kataoka, Ryuho; Ieda, Akimasa; Ebihara, Yusuke; Connors, Martin; Schofield, Ian; Katoh, Yuto; Otsuka, Yuichi; Sunagawa, Naoki; Jordanova, Vania K.

    2015-11-27

    A correlation was observed between chorus emissions and pulsating aurora (PA) from observations at Athabasca (L ≈ 4.3) in Canada at 9:00–9:20 UT on 7 February 2013, using an electron multiplying charge-coupled device camera and a VLF loop antenna with sampling rates of 110 Hz and 100 kHz, respectively. Pulsating aurora having a quasiperiodic variation in luminosity and a few hertz modulation was observed together with chorus emissions consisting of a group of successive rising-tone elements. The repetition period and modulation frequency of the PA are in good agreement with those of the modulated chorus. After 9:11 UT, the temporal features of the aurora became aperiodic PA of indistinct modulation. Simultaneously, the rising-tone chorus turned into chorus emissions consisting of numerous rising-tone elements. The equatorial geomagnetic field inhomogeneity calculated using the Tsyganenko 2002 model shows a decreasing trend during the period. This result is consistent with nonlinear wave growth theory having a small geomagnetic field inhomogeneity, which contributes to a decrease in the threshold amplitude to trigger discrete chorus elements. As a result, these observations show a close connection between chorus emissions and PA on timescales from milliseconds for generation of discrete chorus elements on the microphysics of wave-particle interaction to minutes for the variations of the geomagnetic field inhomogeneity related with the substorm activity.

  6. Fast modulations of pulsating proton aurora related to subpacket structures of Pc1 geomagnetic pulsations at subauroral latitudes

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

    Ozaki, M.; Shiokawa, K.; Miyoshi, Y.; Kataoka, R.; Yagitani, S.; Inoue, T.; Ebihara, Y.; Jun, C. -W; Nomura, R.; Sakaguchi, K.; et al

    2016-08-14

    To understand the role of electromagnetic ion cyclotron (EMIC) waves in determining the temporal features of pulsating proton aurora (PPA) via wave-particle interactions at subauroral latitudes, high-time-resolution (1/8 s) images of proton-induced N2>+ emissions were recorded using a new electron multiplying charge-coupled device camera, along with related Pc1 pulsations on the ground. The observed Pc1 pulsations consisted of successive rising-tone elements with a spacing for each element of 100 s and subpacket structures, which manifest as amplitude modulations with a period of a few tens of seconds. In accordance with the temporal features of the Pc1 pulsations, the auroral intensitymore » showed a similar repetition period of 100 s and an unpredicted fast modulation of a few tens of seconds. Furthermore, these results indicate that PPA is generated by pitch angle scattering, nonlinearly interacting with Pc1/EMIC waves at the magnetic equator.« less

  7. SciTech Connect: auroras

    Office of Scientific and Technical Information (OSTI)

    Renewable Energy Laboratory (NREL), Golden, CO (United States) Naval Petroleum and Oil Shale Reserves (United States) Navarro Navarro Nevada Environmental Services Nevada Field...

  8. Energy Efficiency for the Nunamiut People of Anaktuvuk Pass, Alaska

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

    November 16, 2011 Dave Messier Yukon River Inter-Tribal Watershed Council Energy Department } Established in 1997 } Treaty Based } 70 Tribes and First Nations } Directive - Clean Water Needs Clean Energy } Efficiency First } RE and Energy Efficiency Trainings and Capacity Building } Nunamiut People- Inland Eskimo of Alaska } Anaktuvuk - place of caribou droppings } Corp = The Local Wal-Mart Hardware Store, Bank, Grocery Store, Restaurant, Hotel, Gas Station, radio station } Electric Rate:

  9. Powering Business in Ohio with Cellex Fuel Cells

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

    Powering Business in Ohio with Cellex Fuel Cells Cellex powered twelve class 3 electric pallet trucks with its fuel cell power units at two Ohio based Wal-Mart distribution centers for four months to demonstrate the commercial viability of hydrogen fuel cells. This project was funded by the Ohio Department of Development's Third Frontier Fuel Cell Program, which provides grants to support the growth of Ohio's fuel cell industry through collaborations between research organizations, businesses

  10. Feasibility Study of Economics and Performance of Solar Photovoltaics at the Tower Road Site in Aurora, Colorado. A Study Prepared in Partnership with the Environmental Protection Agency for the RE-Powering America's Land Initiative: Siting Renewable Energy on Potentially Contaminated Land and Mine Sites

    SciTech Connect (OSTI)

    Van Geet, O.; Mosey, G.

    2013-03-01

    The U.S. Environmental Protection Agency (EPA), in accordance with the RE-Powering America's Land initiative, selected the Tower Road site in Aurora, Colorado, for a feasibility study of renewable energy production. The National Renewable Energy Laboratory (NREL) provided technical assistance for this project. The purpose of this report is to assess the site for a possible photovoltaic (PV) system installation and estimate the cost, performance, and site impacts of different PV options. In addition, the report recommends financing options that could assist in the implementation of a PV system at the site. This study did not assess environmental conditions at the site.

  11. Aurora Geothermal Project | Open Energy Information

    Open Energy Info (EERE)

    EFAULT","autoinfowindows":false,"kml":,"gkml":,"fusiontables":,"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":,"markercluster":false,"searchmarkers...

  12. Aurora, Ohio: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    lse,"poi":true,"imageoverlays":,"markercluster":false,"searchmarkers":"","locations":"text":"","title":"","link":null,"lat":41.3175549,"lon":-81.3453858,"alt":0,"address":"","i...

  13. Buildings Energy Data Book: 3.7 Retail Markets and Companies

    Buildings Energy Data Book [EERE]

    3 2010 Top Supermarkets, by Sales 2010 All Commodity Supermarket Wal-Mart Stores 3,001 Kroger Co. 2,460 Safeway, Inc. 1,461 Supervalu, Inc. 1,504 Ahold USA, Inc. (Stop and Shop, Giant) 746 Publix Super Markets, Inc. 1,035 Delhaize America, Inc. (Food Lion) 1,641 H.E. Butt Grocery Co. (HEB) 291 Meijer Inc. 195 Great Atlantic & Pacific Tea Co. (Pathmark) 373 Note(s): Source(s): All commodity volume in this example represents the "annualized range of the estimated retail sales volume of

  14. Rocky Flats Overview Aurora History Museum October 16, 2013

    Office of Environmental Management (EM)

    5 Nuclear Weapons Complex Nuclear Weapons Production Processes Step Process Major Sites 1 Uranium Mining, Milling, and Refining Uranium Mill Tailing Remedial Action Project sites,...

  15. Molecular mechanism of Aurora A kinase autophosphorylation and...

    Office of Scientific and Technical Information (OSTI)

    Publication Date: 2014-05-27 OSTI Identifier: 1197669 GrantContract Number: The Office of Basic Energy Sciences, Catalyst Science Program, DE-FG02-05ER15699 Type: Published ...

  16. Students from Aurora Triumph in Competition of the Mind

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

    Security Administration | (NNSA) flock to Science on Saturday, 22 years running Friday, March 25, 2016 - 9:51am Scores of teenagers can be found waiting outside the Bankhead Theater in Livermore, Calif., early on Saturday mornings throughout the month of February, hoping for a seat to one of the city's longest running feature presentations, Science on Saturday. The crowd gathers for stars, light and chemistry on stage - all part of science presentations given by leading researchers from

  17. OSTIblog Articles in the auroras Topic | OSTI, US Dept of Energy...

    Office of Scientific and Technical Information (OSTI)

    ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson ... physics, chemistry, energy security, advanced space propulsion, and material science. ...

  18. Solar Technology Acceleration Center (SolarTAC): Solar Resource & Meteorological Assessment Project (SOLRMAP); Aurora, Colorado (Data)

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

    Wilcox, S.; Andreas, A.

    Located in Colorado, near Denver International Airport, SolarTAC is a private, member-based, 74-acre outdoor facility where the solar industry tests, validates, and demonstrates advanced solar technologies. SolarTAC was launched in 2008 by a public-private consortium, including Midwest Research Institute (MRI). As a supporting member of SolarTAC, the U.S. Department of Energy's National Renewable Energy Laboratory (NREL) has established a high quality solar and meteorological measurement station at this location. This Solar Resource and Meteorological Assessment Project (SOLRMAP) provides high quality measurements to support deployment of power projects in the United States. The no-funds-exchanged collaboration brings NREL solar resource assessment expertise together with industry needs for measurements. The end result is high quality data sets to support the financing, design, and monitoring of large scale solar power projects for industry in addition to research-quality data for NREL model development. NREL provides consultation for instrumentation and station deployment, along with instrument calibrations, data acquisition, quality assessment, data distribution, and summary reports. Industry participants provide equipment, infrastructure, and station maintenance.

  19. Solar Technology Acceleration Center (SolarTAC): Solar Resource & Meteorological Assessment Project (SOLRMAP); Aurora, Colorado (Data)

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

    Wilcox, S.; Andreas, A.

    2011-02-11

    Located in Colorado, near Denver International Airport, SolarTAC is a private, member-based, 74-acre outdoor facility where the solar industry tests, validates, and demonstrates advanced solar technologies. SolarTAC was launched in 2008 by a public-private consortium, including Midwest Research Institute (MRI). As a supporting member of SolarTAC, the U.S. Department of Energy's National Renewable Energy Laboratory (NREL) has established a high quality solar and meteorological measurement station at this location. This Solar Resource and Meteorological Assessment Project (SOLRMAP) provides high quality measurements to support deployment of power projects in the United States. The no-funds-exchanged collaboration brings NREL solar resource assessment expertise together with industry needs for measurements. The end result is high quality data sets to support the financing, design, and monitoring of large scale solar power projects for industry in addition to research-quality data for NREL model development. NREL provides consultation for instrumentation and station deployment, along with instrument calibrations, data acquisition, quality assessment, data distribution, and summary reports. Industry participants provide equipment, infrastructure, and station maintenance.

  20. Midwest Energy (Gas and Electric)- How$mart Energy Efficiency Finance Program

    Broader source: Energy.gov [DOE]

    Midwest Energy offers its residential and small commercial electricity and natural gas customers in good standing a way to finance energy efficiency improvements on eligible properties. Under the...

  1. Buildings Energy Data Book: 3.7 Retail Markets and Companies

    Buildings Energy Data Book [EERE]

    1 2010 Top Retail Companies, by Sales # Stores % Change over Chain ($billion) 2009 Revenues 2010 2009 Stores Wal-Mart Stores, Inc. 419.0 3.4% 8,970 6.0% The Kroger Co. 82.2 7.1% 3,605 -0.4% Costco 76.3 9.1% 572 1.1% The Home Depot 68.0 2.8% 2,248 0.2% Walgreen Co. 67.4 6.4% 8,046 7.3% Target Corp. 67.4 3.1% 1,750 0.6% CVS Caremark 57.3 3.6% 7,182 2.2% Best Buy 50.3 1.2% 4,172 3.7% Lowes Cos. 48.8 3.4% 1,749 2.3% Sears Holdings 43.3 -1.6% 4,038 2.2% Source(s): 2010 Revenues % Change over Chain

  2. Relative brightness of the O{sup +}({sup 2} D-{sup 2} P) doublets in low-energy aurorae

    SciTech Connect (OSTI)

    Whiter, D. K.; Lanchester, B. S.; Gustavsson, B.; Jallo, N. I. B.; Jokiaho, O.; Dahlgren, H.; Ivchenko, N.

    2014-12-10

    The ratio of the emission line doublets from O{sup +} at 732.0 nm (I {sub 732}) and 733.0 nm (I {sub 733}) has been measured in auroral conditions of low-energy electron precipitation from Svalbard (78.°20 north, 15.°83 east). Accurate determination of R = I {sub 732}/I {sub 733} provides a powerful method for separating the density of the O{sup +} {sup 2} P{sub 1} {sub /2,3} {sub /2}{sup o} levels in modeling of the emissions from the doublets. A total of 383 spectra were included from the winter of 2003-2004. The value obtained is R = I {sub 732}/I {sub 733} = 1.38 ± 0.02, which is higher than theoretical values for thermal equilibrium in fully ionized plasma, but is lower than reported measurements by other authors in similar auroral conditions. The continuity equations for the densities of the two levels are solved for different conditions, in order to estimate the possible variations of R. The results suggest that the production of ions in the two levels from O ({sup 3} P {sub 1}) and O ({sup 3} P {sub 2}) does not follow the statistical weights, unlike astrophysical calculations for plasmas in nebulae. The physics of auroral impact ionization may account for this difference, and therefore for the raised value of R. In addition, the auroral solution of the densities of the ions, and thus of the value of R, is sensitive to the temperature of the neutral atmosphere. Although the present work is a statistical study, it shows that it is necessary to determine whether there are significant variations in the ratio resulting from non-equilibrium conditions, from auroral energy deposition, large electric fields, and changes in temperature and composition.

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

    Office of Energy Efficiency and Renewable Energy (EERE)

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

  4. Sandia National Laboratories: Research: High Consequence, Automation...

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

    Weight and Leak Check System (WALS) The Nuclear Weapons Complex stores radioactive nuclear ... A redundant computer to independently monitor forces on the pit during robot motion. ...

  5. NREL: Energy Analysis - Chris Webber

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

    Prior work experience Deployment Engineer, SAIC Corporation, Aurora, CO (2009-2011) System Engineer, Scitor Corporation, Aurora, CO (2006-2009) System Administrator, BCER ...

  6. Browse by Discipline -- E-print Network Subject Pathways: Environmenta...

    Office of Scientific and Technical Information (OSTI)

    N O P Q R S T U V W X Y Z Mahat, Pukar (Pukar Mahat) - Department of Energy Technology, Aalborg University Mart, Jos R. (Jos R. Mart) - Department of Electrical and ...

  7. Correlated Pc4-5 ULF waves, whistler-mode chorus, and pulsating...

    Office of Scientific and Technical Information (OSTI)

    and pulsating aurora observed by the Van Allen Probes and ground-based systems Citation ... and pulsating aurora observed by the Van Allen Probes and ground-based systems Theory and ...

  8. Quasar-Lyman α forest cross-correlation from BOSS DR11: Baryon...

    Office of Scientific and Technical Information (OSTI)

    de Cincies del Cosmos (IEECUB), Mart i Franqus 1, Barcelona, 08028 Catalonia (Spain) Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA (United States) ...

  9. TITLE AUTHORS SUBJECT SUBJECT RELATED DESCRIPTION PUBLISHER AVAILABILI...

    Office of Scientific and Technical Information (OSTI)

    Training and Research on Probabilistic Hydro Thermo Mechanical Modeling of Carbon Dioxide Geological Sequestration in Fractured Porous Rocks Gutierrez Marte ENVIRONMENTAL SCIENCES...

  10. Carbon Dioxide Geological Sequestration in Fractured Porous Rocks

    Office of Scientific and Technical Information (OSTI)

    Training and Research on Probabilistic Hydro-Thermo-Mechanical Modeling of Carbon Dioxide Geological Sequestration in Fractured Porous Rocks Gutierrez, Marte 54 ENVIRONMENTAL...

  11. McLennan County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Lorena, Texas Mart, Texas McGregor, Texas Moody, Texas Riesel, Texas Robinson, Texas Ross, Texas Valley Mills, Texas Waco, Texas West, Texas Woodway, Texas Retrieved from...

  12. --No Title--

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

    ... Global Companies Global Petroleum Go-Mart Goodway Refining GP&W Great Island Energy Green Valley Oil Griffith Energy Services Growmark Gulf Oil Gulf Oil Limited Partnership ...

  13. Portage County, Ohio: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Rotek Incorporated Sadoun Solar Sales Places in Portage County, Ohio Aurora, Ohio Brady Lake, Ohio Brimfield, Ohio Garrettsville, Ohio Hiram, Ohio Kent, Ohio Mantua, Ohio...

  14. EECBG Success Story: Illinois Town Launches Toilet Rebate Program

    Broader source: Energy.gov [DOE]

    The city of Aurora, Illinois, has launched a rebate program that aims to help residents avoid flushing money and energy down the toilet. Learn more.

  15. SREL Reprint #3332

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

    Smithfield, Queensland 4878, Australia 5Department of Biochemistry and Molecular Genetics, University of Colorado School of Medicine, Aurora, Colorado 80045 USA Premise of...

  16. SREL Reprint #3262

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

    of Georgia, Aiken, South Carolina, USA 2Department of Biochemistry and Molecular Genetics, University of Colorado School of Medicine, Aurora, Colorado, USA Abstract:...

  17. SREL Reprint #3318

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

    Regents University, Augusta, GA 30904, USA 3Department of Biochemistry and Molecular Genetics, University of Colorado School of Medicine, Aurora, CO 80045, USA Abstract: We...

  18. SREL Reprint #3254

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

    University of Georgia, Aiken, SC 29802, USA 2Department of Biochemistry and Molecular Genetics, School of Medicine, University of Colorado, Aurora, CO 80045, USA 3Department of...

  19. SREL Reprint #3271

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

    University of Georgia, Aiken, SC 29802, USA 3Department of Biochemistry and Molecular Genetics, University of Colorado School of Medicine, Aurora, CO 80045, USA 4Laboratorio de...

  20. ECOsponsible | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search Name: ECOsponsible Address: 120 Mitchell Road Suite 100 Place: East Aurora Zip: 14052-9710 Sector: Marine and Hydrokinetic This company is...

  1. B O N N E V I L L E ...

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

    incremental transmission, and ancillary services costs were computed under 3,200 AURORA games which tested different load and resource conditions for each month. Incremental...

  2. Lawrenceville, New Jersey: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Energy Companies in Lawrenceville, New Jersey Aurora Photovoltaics Manufacturing Hydrocarbon Technologies References US Census Bureau 2005 Place to 2006 CBSA Retrieved from...

  3. Ennovate Corporation | Open Energy Information

    Open Energy Info (EERE)

    Aurora, Colorado Zip: 80014 Region: Rockies Area Sector: Efficiency Product: Energy Service Company specializing in providing energy savings projects for institutional...

  4. ProLogis | Open Energy Information

    Open Energy Info (EERE)

    Name: ProLogis Place: Aurora, Colorado Zip: 80011 Sector: Services Product: Provider of distribution facilities and services. Coordinates: 39.325162, -79.54975 Show Map...

  5. Western Turbine | Open Energy Information

    Open Energy Info (EERE)

    Turbine Jump to: navigation, search Name: Western Turbine Place: Aurora, Colorado Zip: 80011 Sector: Wind energy Product: Wind Turbine Installation and Maintainance. Coordinates:...

  6. Property:Purchasers | Open Energy Information

    Open Energy Info (EERE)

    Pass Geothermal Area Augusta Mountains Geothermal Area Aurora Geothermal Area B Bac-Man Laguna Geothermal Area Bailey Bay Hot Springs Geothermal Area Baker Hot Spring...

  7. Property:OtherUses | Open Energy Information

    Open Energy Info (EERE)

    Pass Geothermal Area Augusta Mountains Geothermal Area Aurora Geothermal Area B Bac-Man Laguna Geothermal Area Bad Blumau Geothermal Area Bailey Bay Hot Springs Geothermal...

  8. Property:CaseStudyPriority | Open Energy Information

    Open Energy Info (EERE)

    Geothermal Area + 4 - Not Assigned + Aurora Geothermal Area + 4 - Not Assigned + B Bac-Man Laguna Geothermal Area + 4 - Not Assigned + Bad Blumau Geothermal Area + 4 - Not...

  9. Property:BoundingCoordinatesSW | Open Energy Information

    Open Energy Info (EERE)

    -98.55 + Aurora Geothermal Area + 38.301488855308, -119.02164916992 + B Bac-Man Laguna Geothermal Area + 13.016892384898, 123.91971130371 + Bad Blumau Geothermal...

  10. Category:Available for Case Study | Open Energy Information

    Open Energy Info (EERE)

    Pass Geothermal Area Augusta Mountains Geothermal Area Aurora Geothermal Area B Bac-Man Laguna Geothermal Area Bad Blumau Geothermal Area Bailey Bay Hot Springs Geothermal...

  11. Property:FirstWellFlowRate | Open Energy Information

    Open Energy Info (EERE)

    Pass Geothermal Area Augusta Mountains Geothermal Area Aurora Geothermal Area B Bac-Man Laguna Geothermal Area Bad Blumau Geothermal Area Bailey Bay Hot Springs Geothermal...

  12. Property:TectonicSetting | Open Energy Information

    Open Energy Info (EERE)

    Area + Extensional Tectonics + Aurora Geothermal Area + Extensional Tectonics + B Bac-Man Laguna Geothermal Area + Subduction Zone + Beowawe Hot Springs Geothermal Area +...

  13. Alameda, California: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    in Alameda, California Aurora BioFuels Inc Makani Power Makani Power Inc Primus Power Solo Energy References US Census Bureau Incorporated place and minor civil division...

  14. NREL: Solar Research - News Release Archives

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

    09 October 21, 2009 Solar Technology Acceleration Center is Powering Up Members of the Solar Technology Acceleration Center (SolarTAC) and supporters convened in Aurora, Colo., ...

  15. Press Materials for Argonne CORAL announcement | Argonne National...

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

    Livermore (CORAL) initiative, the U.S. Department of Energy announced a 200 million investment to deliver a next-generation supercomputer, known as Aurora, to the Argonne...

  16. U.S. Department of Energy awards $200 million for next-generation...

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

    (CORAL) initiative, the U.S. Department of Energy (DOE) announced a 200 million investment to deliver a next-generation supercomputer, known as Aurora, to the Argonne...

  17. Solar Roofing Systems Inc | Open Energy Information

    Open Energy Info (EERE)

    Inc Place: Aurora, Ontario, Canada Zip: L4G 3S8 Product: Manufactures and develops photovoltaic roofing and portable products. References: Solar Roofing Systems Inc1 This...

  18. Other Participants 2006 | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Academy , Pelahatchie , MS Edwin O. Smith High School , Mansfield , CT Fergus High ... Aurora, CO Southside High School , Fort Smith , AR Star Lane Center , Casper , WY State ...

  19. Other Participants 2004 | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    ... School , Washington , DC Skyline High School , Idaho Falls, ID Skyview High School , Billings , MT Smoky Hill High School, Aurora, CO Southside High School , Fort Smith , AR St. ...

  20. Other Participants 2002 | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    ... Skyline High School , Idaho Falls, ID Skyview High School , Billings , MT Smoky Hill High School, Aurora, CO South Aiken High School , Aiken , SC Southside High School , Fort Smith ...

  1. "Title","Creator/Author","Publication Date","OSTI Identifier...

    Office of Scientific and Technical Information (OSTI)

    Training and Research on Probabilistic Hydro-Thermo-Mechanical Modeling of Carbon Dioxide Geological Sequestration in Fractured Porous Rocks","Gutierrez, Marte","2013-05-31T04:00:0...

  2. Nebraska Appliance Rebate Program opens

    Broader source: Energy.gov [DOE]

    Nearly 500 people lined up outside of Omaha's Nebraska Furniture Mart on July 6, waiting to get ENERGY STAR washing machines, dishwashers and refrigerators on the first day of Nebraska's Appliance Rebate Program.

  3. VeraSun Energy Corp | Open Energy Information

    Open Energy Info (EERE)

    VeraSun Energy Corp Place: Aurora, South Dakota Zip: 57002 Product: VeraSun uses biotechnology to convert corn to fuel-grade ethanol, which is blended with gasoline and results...

  4. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Grbel, Gerhard (1) Guo, Hongyu (1) Hernndez, Rebeca (1) Hernndez, Rebeca, E-mail: rhernandez@ictp.csic.es, E-mail: aurora.nogales@csic.es (1) Hwang, Ho-Ling (1) Ishikawa, ...

  5. Usibelli Coal Mine - Cleaner Energy, Brighter Future

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

    * Operated by Aurora Energy Services, LLC 14 Historical Coal Export Markets * South Korea - 15 million tons since 1984 * Chile - 3.3 million tons since 2003 * Japan - 840,000 ...

  6. CX-002241: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Maximizing Alternative Fuel Use and Distribution in ColoradoCX(s) Applied: B5.1Date: 05/13/2010Location(s): Aurora, ColoradoOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  7. Merrick and Co | Open Energy Information

    Open Energy Info (EERE)

    Year 1999 Link to project description http:www.nrel.govnewspress1999899corn.html Merrick and Co is a company located in Aurora, CO. References Retrieved from "http:...

  8. Property:BoundingCoordinatesNE | Open Energy Information

    Open Energy Info (EERE)

    + 39.7, -98.15 + Aurora Geothermal Area + 38.468856230108, -118.71640625 + B Bac-Man Laguna Geothermal Area + 13.112513717997, 124.00935153418 + Bad Blumau Geothermal...

  9. Microsoft Word - Alcoa Extension EBT ROD Attachments - 2010-10...

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

    load forecast used in AURORA xmp , the WECC 10-Year Coordinated Plan Summary (2006-2015) was used in WP-10. That load forecast has since been discontinued. In its place, the...

  10. DOI-BLM-NV-W010-2009-0018-CX | Open Energy Information

    Open Energy Info (EERE)

    18-CX Jump to: navigation, search NEPA Document Collection for: DOI-BLM-NV-W010-2009-0018-CX CX at Aurora Geothermal Area for GeothermalExploration CX for Geophysical Survey at...

  11. DOI-BLM-NV-030-06-025-EA | Open Energy Information

    Open Energy Info (EERE)

    30-06-025-EA Jump to: navigation, search NEPA Document Collection for: DOI-BLM-NV-030-06-025-EA EA at Aurora Geothermal Area for GeothermalLeasing, GeothermalExploration,...

  12. http://www.fs.usda.gov/wps/portal/fsinternet/!ut/p/c5/04_SB8K8x

    National Nuclear Security Administration (NNSA)

    "Don't Trash Nevada" Pledge? Recent News Subscribe to this feed Correction to Aurora Geothermal Release Dated May 4, 20M VEB6FWOPOOW6 2011 Bridgeport and Carson Ranger Districts...

  13. Chena Geothermal Area | Open Energy Information

    Open Energy Info (EERE)

    the winter, and is maintained using a 15 ton (53 kW) absorption chiller designed by Energy Concepts Co., which utilizes geothermal fluids.6 Forbes magazine voted the Aurora...

  14. World-Class Test Facility Increases Efficiency of Solar Products

    Broader source: Energy.gov [DOE]

    This photograph features PV arrays at the SunEdison Facility at the Solar Technology Acceleration Center (SolarTAC) in Aurora, Colorado. SolarTAC is an integrated, world-class test facility where...

  15. Exact and approximate Kohn-Sham potentials in ensemble density...

    Office of Scientific and Technical Information (OSTI)

    Title: Exact and approximate Kohn-Sham potentials in ensemble density-functional theory Authors: Yang, Zeng-hui ; Trail, John R. ; Pribram-Jones, Aurora ; Burke, Kieron ; Needs, ...

  16. Hot electron dynamics in graphene (Thesis/Dissertation) | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Thesis/Dissertation: Hot electron dynamics in graphene Citation Details In-Document Search Title: Hot electron dynamics in graphene Graphene, a two-dimensional (2D) honeycomb structure allotrope of carbon atoms, has a long history since the invention of the pencil [Petroski (1989)] and the linear dispersion band structure proposed by Wallace [Wal]; however, only after Novoselov et al. successively isolated graphene from graphite [Novoselov et al. (2004)], it has been studied intensively during

  17. PowerPoint Presentation

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

    WORKERS' COMPENSATION CLAIM PROCESS FOR HANFORD SITE EMPLOYEES PENSER'S CLAIM PROCESS PENSER and WAL&I *Requests a Physicians Initial Report (PIR) if not already provided *Investigates claim to determine validity *Contacts worker for statement *Verifies employment data and interviews witnesses, if any *Obtains information from contractor's WCR, if appropriate *Requests additional medical documentation if needed *Ensures claim details satisfy requirements of the law *If an investigation does

  18. CX-003477: Categorical Exclusion Determination | Department of Energy

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

    77: Categorical Exclusion Determination CX-003477: Categorical Exclusion Determination National Institute of Advanced Industrial Science and Technology (AIST) - National Renewable Energy Laboratory (NREL) Concentrator Photovoltaic (CPV) Demonstration (Solar Technology Acceleration Center, Aurora, Colorado); NREL Tracking Number 10-035 CX(s) Applied: A9, A11, B1.3 Date: 08/20/2010 Location(s): Aurora, Colorado Office(s): Energy Efficiency and Renewable Energy, Golden Field Office The proposed

  19. 2007 Wholesale Power Rate Case Final Proposal : Market Price Forecast Study.

    SciTech Connect (OSTI)

    United States. Bonneville Power Administration.

    2006-07-01

    This study presents BPA's market price forecasts for the Final Proposal, which are based on AURORA modeling. AURORA calculates the variable cost of the marginal resource in a competitively priced energy market. In competitive market pricing, the marginal cost of production is equivalent to the market-clearing price. Market-clearing prices are important factors for informing BPA's power rates. AURORA was used as the primary tool for (a) estimating the forward price for the IOU REP Settlement benefits calculation for fiscal years (FY) 2008 and 2009, (b) estimating the uncertainty surrounding DSI payments and IOU REP Settlements benefits, (c) informing the secondary revenue forecast and (d) providing a price input used for the risk analysis. For information about the calculation of the secondary revenues, uncertainty regarding the IOU REP Settlement benefits and DSI payment uncertainty, and the risk run, see Risk Analysis Study WP-07-FS-BPA-04.

  20. To: H: Bauer M: Kahal

    Office of Legacy Management (LM)

    I-T: c;:y::: DhTo: 19 Ma!ch 1985 7117-01.85.aw.17 To: H: Bauer M: Kahal C. Young - B. Fritz &?, \' ,',l --- s"mJ~cI: Elimination of ARF, Chica~go, IL ROY: A. Wal.lo BLDq woe ROOM: m-r: 6320 The enclosed summary wa's prepared on the basis of a review of NRC files. This site was fully licensed. Based on DRAP policy, no additional FUSRAP investigations are warranted. AWfsb Enclosure .: . . > . . . . . ELIMINATION SUMMARY FOR THE ARMOUR RESEARCH FOUNDATION SUMMARY: ji,i7 Records searches

  1. IO6490

    Office of Legacy Management (LM)

    1 ' f. (5 4 . . i/ IO6490 ~-~~ -Landfill, ' cleanup plan' is. expected by August peruneat OfEnergy tiy they hope mlxa~~amfari~cclcanupplan for four radioactive oitcs m the puwn of Tonawanda by early e- naidE.%rk,DOEsitcman- ~a,saidalltkrexarchandtech- fucd data cdkted at ctkc four 6ilc5 ha3 been forwarded ti his suptx.iors In WashingronJC. ' when it still awaits We' re still wal r .f$, co* liar iEP-+-* 6adMr. Wehmdaiinourd0cum8nu in February .bur unfommuely them' s a group in Wnshington we.

  2. Market Evolution: Wholesale Electricity Market Design for 21st Century Power Systems

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

    1stCenturyPower.org Technical Report NREL/TP-6A20-57477 October 2013 Contract No. DE-AC36-08GO28308 Market Evolution: Wholesale Electricity Market Design for 21 st Century Power Systems Jaquelin Cochran, Mackay Miller, Michael Milligan, Erik Ela, Douglas Arent, and Aaron Bloom National Renewable Energy Laboratory Matthew Futch IBM Juha Kiviluoma and Hannele Holtinnen VTT Technical Research Centre of Finland Antje Orths Energinet.dk Emilio Gómez-Lázaro and Sergio Martín-Martínez Universidad

  3. Plasma 101 | Princeton Plasma Physics Lab

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

    Plasma 101 10 Facts You Should Know About Plasma By Larry Bernard February 22, 2016 Tweet Widget Google Plus One Share on Facebook The Aurora Borealis (Northern Lights) (Photo by Philippe Moussette for Nasa.gov) The Aurora Borealis (Northern Lights) Gallery: NSTX interior NSTX interior W7-X plasma W7-X plasma The sun (Photo by nasa.gov) The sun It's the fourth state of matter: Solid, liquid, gas, and plasma. Plasma is a super-heated gas, so hot that its electrons get out of the atom's orbit and

  4. Chemistry, Reservoir, and Integrated Models | Department of Energy

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

    Chemistry, Reservoir, and Integrated Models Chemistry, Reservoir, and Integrated Models Below are the project presentations and respective peer review results for Chemistry, Reservoir and Integrated Models. Development and Validation of an Advanced Stimulation Prediction Model for Enhanced Geothermal Systems (EGS), Marte Gutierrez and Masami Nakagawa, Colorado School of Mines Development of Advanced Thermal-Hydrological-Mechanical-Chemical (THMC) Modeling Capabilities for Enhanced Geothermal

  5. Solar Energy Research and Education Foundation. Final reports by task

    SciTech Connect (OSTI)

    von Reis, K.; Waegel, A.S.; Totten, M.

    1997-12-10

    This document contains final reports for the following tasks: kiosk for the children`s museum renewable energy exhibit and display, internet promotional and educational material, Aurora renewable energy science and engineering, CD-ROM training materials, presentations and traveling display, radio show `Energy Matters`, and newspaper articles and weekly news column.

  6. CX-002538: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Tangent Grant Application for American Recovery and Reinvestment Act Business Development ProgramCX(s) Applied: B5.1Date: 05/27/2010Location(s): Aurora, IllinoisOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  7. CX-007120: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Full-Scale Mercury Control Demonstrations: Information Collection Request Sampling with Mercury ControlCX(s) Applied: A9, B3.1Date: 10/04/2011Location(s): Aurora, Saint Louis County, MissouriOffice(s): Fossil Energy, National Energy Technology Laboratory

  8. News | Princeton Plasma Physics Lab

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

    Plasma 101 10 Facts You Should Know About Plasma Click on an image below to view the high resolution image. Then right click on the image and select "Save Image" or "Save Image As..." The Aurora Borealis (Northern Lights) NSTX interior W7-X plasma The sun

  9. A comparison of the performance of digital mammography systems

    SciTech Connect (OSTI)

    Monnin, P.; Gutierrez, D.; Bulling, S.; Guntern, D.; Verdun, F. R.

    2007-03-15

    An objective analysis of image quality parameters was performed for six digital mammography systems. The presampled modulation transfer function (MTF), normalized noise power spectrum (NNPS), and detective quantum efficiency (DQE) for the systems were determined at different doses, for 28 kVp with a Mo/Mo or W/Al target/filter combination and 2 mm of additional aluminium filtration. The flat-panel units have higher MTF and DQE in the mid to high frequency range than standard CR systems. The highest DQE, over the whole dose range, is for the slit-scanning direct photon counting system. Dual-side read CR can overcome the inherent x-ray absorption and signal collection limitations of standard CR mammography, improving the low-frequency DQE by 40%, to the same level as full-field systems, but it does not improve the poor spatial resolution of phosphor.

  10. A mirror for lab-based quasi-monochromatic parallel x-rays

    SciTech Connect (OSTI)

    Nguyen, Thanhhai; Lu, Xun; Lee, Chang Jun; Jeon, Insu; Jung, Jin-Ho; Jin, Gye-Hwan; Kim, Sung Youb

    2014-09-15

    A multilayered parabolic mirror with six W/Al bilayers was designed and fabricated to generate monochromatic parallel x-rays using a lab-based x-ray source. Using this mirror, curved bright bands were obtained in x-ray images as reflected x-rays. The parallelism of the reflected x-rays was investigated using the shape of the bands. The intensity and monochromatic characteristics of the reflected x-rays were evaluated through measurements of the x-ray spectra in the band. High intensity, nearly monochromatic, and parallel x-rays, which can be used for high resolution x-ray microscopes and local radiation therapy systems, were obtained.

  11. ORIGIN OF ELECTRON CYCLOTRON MASER INDUCED RADIO EMISSIONS AT ULTRACOOL DWARFS: MAGNETOSPHERE-IONOSPHERE COUPLING CURRENTS

    SciTech Connect (OSTI)

    Nichols, J. D.; Burleigh, M. R.; Casewell, S. L.; Cowley, S. W. H.; Wynn, G. A.; Clarke, J. T.; West, A. A.

    2012-11-20

    A number of ultracool dwarfs emit circularly polarized radio waves generated by the electron cyclotron maser instability. In the solar system such radio is emitted from regions of strong auroral magnetic-field-aligned currents. We thus apply ideas developed for Jupiter's magnetosphere, being a well-studied rotationally dominated analog in our solar system, to the case of fast-rotating UCDs. We explain the properties of the radio emission from UCDs by showing that it would arise from the electric currents resulting from an angular velocity shear in the fast-rotating magnetic field and plasma, i.e., by an extremely powerful analog of the process that causes Jupiter's auroras. Such a velocity gradient indicates that these bodies interact significantly with their space environment, resulting in intense auroral emissions. These results strongly suggest that auroras occur on bodies outside our solar system.

  12. Chena Hot Springs Resort - Electric Power Generation Using Geothermal Fluid Coproduced from Oil and/or Gas Wells

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

    Below are the project presentations and respective peer review results for Chemistry, Reservoir and Integrated Models. Development and Validation of an Advanced Stimulation Prediction Model for Enhanced Geothermal Systems (EGS), Marte Gutierrez and Masami Nakagawa, Colorado School of Mines Development of Advanced Thermal-Hydrological-Mechanical-Chemical (THMC) Modeling Capabilities for Enhanced Geothermal Systems, Yu-Shu Wu, Colorado School of Mines Enhanced Geothermal Systems (EGS) with CO2 as

  13. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    Gutierrez, Marte" Name Name ORCID Product Type: All Book/Monograph Conference/Event Journal Article Miscellaneous Patent Program Document Software Manual Technical Report Thesis/Dissertation Subject: Identifier Numbers: Site: All Alaska Power Administration, Juneau, Alaska (United States) Albany Research Center (ARC), Albany, OR (United States) Albuquerque Complex - NNSA Albuquerque Operations Office, Albuquerque, NM (United States) Amarillo National Resource Center for Plutonium, Amarillo,

  14. Investigation of waste rag generation at Naval Station Mayport. Project report, May 1990-July 1993

    SciTech Connect (OSTI)

    1995-08-01

    The report presents the results of an investigation examining pollution prevention alternatives for reducing the volume of waste rags generated at Naval Station Mayport, located near Jacksonville Beach, Florida. The report recommends five specific pollution prevention alternatives: better operating practices, installation of equipment cleaning stations to remove contaminants normally removed with rags; replacement of SERVE MART rags with disposable wipers; use of recyclable rats for oil and great removal; and confirmation that used rags are fully contaminated prior to disposal.

  15. Automatic Fault Classification

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

    Automatic Fault Classification of Photovoltaic Strings Based on an In Situ IV Characterization System and a Gaussian Process Algorithm. C. Birk Jones ∗ , Manel Mart´ ınez-Ram´ on ‡ , § Ryan Smith † , Craig K. Carmignani ∗ , Olga Lavrova ∗ , Charles Robinson ∗ , and Joshua S. Stein ∗ ∗ Sandia National Laboratories Solar PV & Grid Integration, Albuquerque, NM, USA. ‡ Department of Electrical and Computer Engineering, University of New Mexico, Albuquerque, NM, USA, §

  16. Independent Activity Report, Sandia National Laboratory - February 2011 |

    Energy Savers [EERE]

    Illinois Town Launches Toilet Rebate Program Illinois Town Launches Toilet Rebate Program June 11, 2010 - 4:23pm Addthis Paul Lester Paul Lester Digital Content Specialist, Office of Public Affairs What are the key facts? The EPA estimates toilets account for about 30 percent of an average home's indoor water use. Replacing inefficient toilets with new WaterSense toilets could save almost 2 billion gallons of water per day throughout the country, according to the EPA. The city of Aurora,

  17. Plasma Astrophysics | Princeton Plasma Physics Lab

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

    Plasma Astrophysics One of the most common but least understood phenomena in the universe is an explosive process called magnetic reconnection. PPPL's Magnetic Reconnection Experiment (MRX) studies this process, which gives rise to astrophysical events that include auroras, solar flares and geomagnetic storms. The process occurs when the magnetic field lines in plasmas break and violently reconnect. Generating and studying reconnection under controlled laboratory conditions can yield insights

  18. OSTIblog Articles in the OSTI collections Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information collections Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers often

  19. OSTIblog Articles in the William Watson Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information William Watson Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers

  20. Geothermal systems of the Mono Basin-Long Valley region, eastern California and western Nevada

    SciTech Connect (OSTI)

    Higgins, C.T.; Flynn, T.; Chapman, R.H.; Trexler, D.T.; Chase, G.R.; Bacon, C.F.; Ghusn, G. Jr.

    1985-01-01

    The region that includes Mono Basin, Long Valley, the Bridgeport-Bodie Hills area, and Aurora, in eastern California and western Nevada was studied to determine the possible causes and interactions of the geothermal anomalies in the Mono Basin-Long Valley region as a whole. A special goal of the study was to locate possible shallow bodies of magma and to determine their influence on the hydrothermal systems in the region. (ACR)

  1. Susan Martindale

    Office of Environmental Management (EM)

    WINTER 2008 MEETING SAN ANTONIO, TEXAS FEBRUARY 6-7, 2008 Mark Abkowitz Nuclear Waste Technical Review Board Box 1831, Station B Nashville, Tennessee 37235 mark.abkowitz@vanderbilt.edu Aurora Aboite Director, Environmental Program Wells Band Te-Moak Western Shoshone Tribe P.O. Box 809 Wells, Nevada 89835 wbcepa@yahoo.com Michael Aguilar, Tribal Councilman Governor's Office Pueblo de San Ildefonso Route 5, Box 315-A Santa Fe, New Mexico 87506 abaca@sanipueblo.org Martin Aguilar, Governor

  2. DOE Publishes GATEWAY Report on OLED Lighting in an Office Setting |

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

    Department of Energy OLED Lighting in an Office Setting DOE Publishes GATEWAY Report on OLED Lighting in an Office Setting April 26, 2016 - 11:50am Addthis The U.S. Department of Energy has released a report on the first GATEWAY demonstration involving OLED lighting. Aurora Lighting Design, Inc., in Grayslake, IL, installed Acuity Brands' Trilia(tm) OLED lighting system in September 2014. The new report recounts the experiences of this pioneering project and provides valuable feedback to

  3. OSTIblog Articles in the geomagnetic storms Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information geomagnetic storms Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset.

  4. OSTIblog Articles in the microwave thrusters Topic | OSTI, US Dept of

    Office of Scientific and Technical Information (OSTI)

    Energy Office of Scientific and Technical Information microwave thrusters Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset.

  5. OSTIblog Articles in the nanomaterials Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information nanomaterials Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers

  6. OSTIblog Articles in the spaceship propulsion Topic | OSTI, US Dept of

    Office of Scientific and Technical Information (OSTI)

    Energy Office of Scientific and Technical Information spaceship propulsion Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset.

  7. Solar Technology Acceleration Center is Powering Up - News Releases | NREL

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

    Solar Technology Acceleration Center is Powering Up October 21, 2009 Members of the Solar Technology Acceleration Center (SolarTAC) and supporters convened in Aurora, Colo., today, to mark a milestone in "Powering Up" one of the world's largest solar test and demonstration facilities. Since announcing the initial launch of SolarTAC one year ago, the site infrastructure development has progressed to the point where members can now break ground for their planned solar technology

  8. CX-004249: Categorical Exclusion Determination | Department of Energy

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

    249: Categorical Exclusion Determination CX-004249: Categorical Exclusion Determination Low Cost High Concentration Photovoltaic Power Systems for Utility Power Generation CX(s) Applied: B5.1 Date: 10/14/2010 Location(s): Aurora, California Office(s): Energy Efficiency and Renewable Energy, Golden Field Office Amonix, Inc. proposes to use federal funding to install, and ultimately remove 7 to 9 power modules (Amonix 7700 High Concentration Photovoltaic systems) for field testing at SolarTac

  9. 2009 News | Concentrating Solar Power | NREL

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

    9 News Below are news stories related to Concentrating Solar Power. RSS Learn about RSS. October 21, 2009 Solar Technology Acceleration Center is Powering Up Members of the Solar Technology Acceleration Center (SolarTAC) and supporters convened in Aurora, Colo., today, to mark a milestone in "Powering Up" one of the world's largest solar test and demonstration facilities. Since announcing the initial launch of SolarTAC one year ago, the site infrastructure development has progressed to

  10. Illinois Town Launches Toilet Rebate Program | Department of Energy

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

    Illinois Town Launches Toilet Rebate Program Illinois Town Launches Toilet Rebate Program June 11, 2010 - 4:23pm Addthis Paul Lester Paul Lester Digital Content Specialist, Office of Public Affairs What are the key facts? The EPA estimates toilets account for about 30 percent of an average home's indoor water use. Replacing inefficient toilets with new WaterSense toilets could save almost 2 billion gallons of water per day throughout the country, according to the EPA. The city of Aurora,

  11. Colorado Students Head to National Science Competition

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

    Head to National Science Competition For more information contact: e:mail: Public Affairs Golden, Colo., April 9, 1999 — Two teams of Colorado high school students will head to our nation's capital to compete in the U.S. Department of Energy's (DOE) National Science Bowl April 30 - May 3. Students from Smoky Hill High School in Aurora and Fairview High School in Boulder placed first in regional Science Bowl competitions earlier this year and will represent Colorado at the national competition.

  12. Computational Physics and Methods

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

    2 Computational Physics and Methods Performing innovative simulations of physics phenomena on tomorrow's scientific computing platforms Growth and emissivity of young galaxy hosting a supermassive black hole as calculated in cosmological code ENZO and post-processed with radiative transfer code AURORA. image showing detailed turbulence simulation, Rayleigh-Taylor Turbulence imaging: the largest turbulence simulations to date Advanced multi-scale modeling Turbulence datasets Density iso-surfaces

  13. Upper atmospheric effects of the hf active auroral research program ionospheric research instrument (HAARP IRI)

    SciTech Connect (OSTI)

    Eccles, V.; Armstrong, R.

    1993-05-01

    The earth's ozone layer occurs in the stratosphere, primarily between 10 and 30 miles altitude. The amount of ozone, O3, present is the result of a balance between production and destruction processes. Experiments have shown that natural processes such as auroras create molecules that destroy O. One family of such molecules is called odd nitrogen of which nitric oxide (NO) is an example. Because the HAARP (HF Active Auroral Research Program) facility is designed to mimic and investigate certain natural processes, a study of possible effects of HAARP on the ozone layer was conducted. The study used a detailed model of the thermal and chemical effects of the high power HF beam, which interacts with free electrons in the upper atmosphere above 50 miles altitude. It was found only a small fraction of the beam energy goes into the production of odd nitrogen molecules, whereas odd nitrogen is efficiently produced by auroras. Since the total energy emitted by HAARP in the year is some 200,000 times less than the energy deposited in the upper atmosphere by auroras, the study demonstrates that HAARP HF beam experiments will cause no measurable depletion of the earth's ozone layer.... Ozone, Ozone depletion, Ozone layer, Odd nitrogen, Nitric oxide, HAARP Emitter characteristics.

  14. 2007 Wholesale Power Rate Case Initial Proposal : Risk Analysis Study Documentation.

    SciTech Connect (OSTI)

    United States. Bonneville Power Administration.

    2005-11-01

    The RiskMod Model is comprised of a set of risk simulation models, collectively referred to as RiskSim; a set of computer programs that manages data referred to as Data Management Procedures; and RevSim, a model that calculates net revenues. RiskMod interacts with the AURORA Model, the RAM2007, and the ToolKit Model during the process of performing the Risk Analysis Study. AURORA is the computer model being used to perform the Market Price Forecast Study (see Market Price Forecast Study, WP-07-E-BPA-03); the RAM2007 is the computer model being used to calculate rates (see Wholesale Power Rate Development Study, WP-07-E-BPA-05); and the ToolKit is the computer model being used to develop the risk mitigation package that achieves BPA's 92.6 percent TPP standard (see Section 3 in the Risk Analysis Study, WP-07-E-BPA-04). Variations in monthly loads, resources, natural gas prices, forward market electricity prices, transmission expenses, and aluminum smelter benefit payments are simulated in RiskSim. Monthly spot market electricity prices for the simulated loads, resources, and natural gas prices are estimated by the AURORA Model. Data Management Procedures facilitate the format and movement of data that flow to and/or from RiskSim, AURORA, and RevSim. RevSim estimates net revenues using risk data from RiskSim, spot market electricity prices from AURORA, loads and resources data from the Load Resource Study, WP-07-E-BPA-01, various revenues from the Revenue Forecast component of the Wholesale Power Rate Development Study, WP-07-E-BPA-05, and rates and expenses from the RAM2007. Annual average surplus energy revenues, purchased power expenses, and section 4(h)(10)(C) credits calculated by RevSim are used in the Revenue Forecast and the RAM2007. Heavy Load Hour (HLH) and Light Load Hour (LLH) surplus and deficit energy values from RevSim are used in the Transmission Expense Risk Model. Net revenues estimated for each simulation by RevSim are input into the ToolKit Model

  15. 2007 Wholesale Power Rate Case Final Proposal : Risk Analysis Study Documentation.

    SciTech Connect (OSTI)

    United States. Bonneville Power Administration.

    2006-07-01

    The RiskMod Model is comprised of a set of risk simulation models, collectively referred to as RiskSim; a set of computer programs that manages data referred to as Data Management Procedures; and RevSim, a model that calculates net revenues. RiskMod interacts with the AURORA Model, the RAM2007, and the ToolKit Model during the process of performing the Risk Analysis Study. AURORA is the computer model being used to perform the Market Price Forecast Study (see Market Price Forecast Study, WP-07-FS-BPA-03); the RAM2007 is the computer model being used to calculate rates (see Wholesale Power Rate Development Study, WP-07-FS-BPA-05); and the ToolKit is the computer model being used to develop the risk mitigation package that achieves BPA's 92.6 percent TPP standard (see Section 3 in the Risk Analysis Study, WP-07-FS-BPA-04). Variations in monthly loads, resources, natural gas prices, forward market electricity prices, transmission expenses, and aluminum smelter benefit payments are simulated in RiskSim. Monthly spot market electricity prices for the simulated loads, resources, and natural gas prices are estimated by the AURORA Model. Data Management Procedures facilitate the format and movement of data that flow to and/or from RiskSim, AURORA, and RevSim. RevSim estimates net revenues using risk data from RiskSim, spot market electricity prices from AURORA, loads and resources data from the Load Resource Study, WP-07-FS-BPA-01, various revenues from the Revenue Forecast component of the Wholesale Power Rate Development Study, WP-07-FSBPA-05, and rates and expenses from the RAM2007. Annual average surplus energy revenues, purchased power expenses, and section 4(h)(10)(C) credits calculated by RevSim are used in the Revenue Forecast and the RAM2007. Heavy Load Hour (HLH) and Light Load Hour (LLH) surplus and deficit energy values from RevSim are used in the Transmission Expense Risk Model. Net revenues estimated for each simulation by RevSim are input into the Tool

  16. Microsoft Word - Submittal Letter for Recommendation 2016-01 Campaign Approach

    Office of Environmental Management (EM)

    Northern New Mexico Citizens' Advisory Board 94 Cities of Gold Road Santa Fe, NM 87506 Phone: 505-989-1662 Fax: 505-989-1752 1-800-218-5942 www.energy.gov/em/nnmcab NNMCAB Members Douglas Sayre, Chair Santa Fe, NM Gerard Martínez y Valencia, Vice-Chair Santa Fe, NM Carla Abeyta Chimayo, NM Max Baca Las Vegas, NM Diahann Cordova Alcalde, NM Mary Friday Taos, NM Nona Girardi Los Alamos, NM Angelica Gurulé Española, NM Joshua Madalena Pueblo of Jemez, NM Tessa Mascareñas Española, NM Daniel

  17. Albany, OR * Anchorage, AK * Morgantown, WV * Pittsburgh, PA * Sugar Land, TX

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

    CONTACTS Traci Rodosta Carbon Storage Technology Manager National Energy Technology Laboratory 3610 Collins Ferry Road P.O. Box 880 Morgantown, WV 26507-0880 304-285-1345 traci.rodosta@netl.doe.gov Andrea Dunn Project Manager National Energy Technology Laboratory 626 Cochrans Mill Road P.O. Box 10940 Pittsburgh, PA 15236 412-386-7594 andrea.dunn@netl.doe.gov Marte Gutierrez Principal Investigator Colorado School of Mines 1600 Illinois Street Golden, CO 80401 303-273-3468 Fax: 303-273-3602

  18. SLIDESHOW: Solar Industry At Work | Department of Energy

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

    Solar Industry At Work SLIDESHOW: Solar Industry At Work June 4, 2012 - 9:37am Addthis 1 of 11 Vice President Joe Biden talks with staff at the National Renewable Energy Lab's Process Development and Integration Laboratory (PDIL). The PDIL brings together technical experts from NREL, the solar industry, and universities for collaborative research. Image: Dennis Schroeder (NREL) 2 of 11 Steven Bohn, an engineer at SunEdison oversees SunEdison's testing facility at SolarTAC in Aurora, CO. The

  19. SREL Reprint #3202

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

    2 Rapid Microsatellite Identification from Illumina Paired-End Genomic Sequencing in Two Birds and a Snake Todd A. Castoe1, Alexander W. Poole1, A. P. Jason de Koning1, Kenneth L. Jones1, Diana F. Tomback2, Sara J. Oyler-McCance3, Jennifer A. Fike3, Stacey L. Lance4, Jeffrey W. Streicher5, Eric N. Smith5, and David D. Pollock1 1Department of Biochemistry and Molecular Genetics, University of Colorado School of Medicine, Aurora, Colorado, USA 2Department of Integrative Biology, University of

  20. OSTIblog Articles in the ambient-gas Topic | OSTI, US Dept of Energy Office

    Office of Scientific and Technical Information (OSTI)

    of Scientific and Technical Information ambient-gas Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers often call

  1. Golden - Local Information | NREL

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

    Golden-Local Information This page provides travel information for visitors to the Golden offices and laboratories of the National Renewable Energy Laboratory. Transportation NREL is accessible via bus on the RTD route 20 from Aurora and Denver. Route 20 travels along 20th Avenue and ends at the NREL Education Center. Visit the RTD Web site or call 303-299-6000 to plan your trip or for more information. Visit the Denver International Airport site to find: Car rental agencies Shuttle services,

  2. Students from Smoky Hill High School Triumph in Colorado High School

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

    Science Bowl - News Releases | NREL Students from Smoky Hill High School Triumph in Colorado High School Science Bowl February 11, 2006 Golden, Colo. - For the fifth year in a row, students from Smoky Hill High School won top honors at the Colorado High School Science Bowl. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, Smoky Hill High School from Aurora was victorious over D'Evelyn High School from

  3. Students from Smoky Hill High School Triumph in Colorado Science Bowl -

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

    News Releases | NREL Students from Smoky Hill High School Triumph in Colorado Science Bowl February 12, 2005 Golden, Colo. - Students from Smoky Hill High School won top honors at the Colorado Science Bowl today for the fourth year in a row. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, Smoky Hill High School team #2 from Aurora was victorious over Smoky Hill High School team #1. Thirty-six student

  4. OSTIblog Articles in the plasma Topic | OSTI, US Dept of Energy Office of

    Office of Scientific and Technical Information (OSTI)

    Scientific and Technical Information plasma Topic Plasmas - The Greatest Show on Earth by Kathy Chambers 24 Jun, 2013 in Products and Content Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers often call it the

  5. ALCF Theta Early Science Program: Call for Proposals | Argonne Leadership

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

    Computing Facility ALCF Theta Early Science Program: Call for Proposals Theta ESP CFP is Closed Aurora ESP CFP coming in Early July 2016! Introduction In late 2016, the Argonne Leadership Computing Facility (ALCF) will deploy Theta, a next-generation Cray/Intel system based on the 2nd Generation Intel® Xeon Phi(tm) processor (code name: Knights Landing (KNL)). The system will have over 2500 nodes, each with a KNL 60-or-more-core processor having up to 16 GB of high-bandwidth in-package

  6. OSTI, US Dept of Energy Office of Scientific and Technical Information |

    Office of Scientific and Technical Information (OSTI)

    Speeding access to science information from DOE and Beyond Plasmas - The Greatest Show on Earth by Kathy Chambers on Mon, June 24, 2013 Perhaps the most beautiful and eerie displays of light in our sky are a phenomenon known as the auroras. This natural glow of light in the sky in high latitude regions usually displays ribbons of colors from a fluorescent green to brilliant purple to a vivid crimson somewhat like an unexpected beautiful sunrise or sunset. Observers often call it the greatest

  7. Study of mid-latitude 5577A CI dayglow emissions. Doctoral thesis

    SciTech Connect (OSTI)

    Hume, E.E.

    1992-01-01

    Summary of thesis: The green line (5577angstroms) is a bright, persistent component of the visible airglow. It is produced by an electric quadruple transition from the metastable second excited state (1So) to the first excited state (1D2) of atomic oxygen. These two excited states all lie in the same electron shell of the atom and have the same electron configuration as the ground state of 1s22s22p4, which is the 3P2,1,0. This emission is present in both the daytime and night airglow and in the aurora, and despite a long history of study it is still not fully understood. The emission in the dayglow and the nightglow is relatively homogeneous spatially and global in coverage. In the aurora, the emission is much brighter than the airglow, high structured and very localized being restricted to higher latitudes. The structure of the 5577angstroms emission with altitude and the chemistry responsible for the production of the emission are complex. The vertical structure for the emission has two distinct layers in the airglow each with its own set of production and loss mechanisms. the chemistry for either of these layers is not completely known. The auroral emission is not understood either since it overlaps the upper and lower layer altitudes and it tends to contain some parts of the chemistry of both layers as sources and losses.

  8. Investigations of low-temperature geothermal potential in New York State

    SciTech Connect (OSTI)

    Hodge, D.S.; De Rito, R.; Hifiker, K.; Morgan, P.; Swanberg, C.A.

    1981-09-01

    Temperature gradient map and published heat flow data indicate a possible potential for a geothermal resource in western and central New York State. A new analysis of bottom-hole temperature data for New York State confirms the existence of three positive gradient anomalies: the East Aurora, Cayuga, and Elmira anomalies, with gradients as high as 32/sup 0/C/km, 36/sup 0/C/km, and 36/sup 0/C/km, respectively. Ground waters from two of these anomalies are enriched in silica relative to surrounding areas. Heat flows based on silica geothermometry are 50 to 70 mWm/sup -2/ for the anomalies and 41.4 mWm/sup -2/ for bordering regional flux. A correlation between Bouguer gravity anomalies and the temperature gradient map suggests that the geothermal anomalies may occur above radioactive granites in the basement.

  9. Project Award Spreadsheets 2010 12 21 1232.xlsx

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

    City HQ State Congressional District(s) Population Recovery Act Funding* Asheville ** NC NC-011 500,000 $209,940 Aspen CO CO-003 5,902 $59,193 Aurora CO CO-007 319,057 $151,800 Baltimore MD MD-002 636,919 $200,000 Baton Rouge LA LA-6 223,689 $200,000 Boston MA MA-009 609,023 $300,000 Casper WY WY-001 54,047 $130,000 Chicago IL IL-005 2,853,114 $300,000 Chula Vista CA CA-051 219,318 $200,000 City and County of Denver CO CO-001 598,707 $210,040 Columbia MO MO-009 100,733 $200,000 Davenport IA

  10. INTERSTELLAR NEUTRAL ATOMS AT 1 AU OBSERVED BY THE IMAGE/LENA IMAGER

    SciTech Connect (OSTI)

    Fuselier, S. A.; Ghielmetti, A. G.; Wurz, P. E-mail: gmetti@mail.spasci.com

    2009-06-20

    Observations from the Imager for Magnetopause to Aurora: Global Exploration (IMAGE) Low Energy Neutral Atom (LENA) imager from 2005 are used to investigate characteristics of interstellar neutrals in the inner solar system. The LENA imager detected an interstellar neutral signal starting in 2004 December and extending to early 2005 April. Using the orientation of the field of view of the imager and the date of the loss of the interstellar neutral signal, it is concluded that the signal is consistent with a relatively compact (several degrees wide in ecliptic latitude and longitude) source of neutral helium and/or energetic (>150 eV) hydrogen originating from the solar apex direction. Observations later in 2005 are used to distinguish the composition and conclude that the relatively compact source likely contains some energetic hydrogen (in addition to the helium)

  11. InterMine Webservices for Phytozome (Rev2)

    SciTech Connect (OSTI)

    Carlson, Joseph; Goodstein, David; Rokhsar, Dan

    2014-07-10

    A datawarehousing framework for information provides a useful infrastructure for providers and users of genomic data. For providers, the infrastructure give them a consistent mechanism for extracting raw data. While for the users, the web services supported by the software allows them to make complex, and often unique, queries of the data. Previously, phytozome.net used BioMart to provide the infrastructure. As the complexity, scale and diversity of the dataset as grown, we decided to implement an InterMine web service on our servers. This change was largely motivated by the ability to have a more complex table structure and richer web reporting mechanism than BioMart. For InterMine to achieve its more complex database schema it requires an XML description of the data and an appropriate loader. Unlimited one-to-many and many-to-many relationship between the tables can be enabled in the schema. We have implemented support for:1.) Genomes and annotations for the data in Phytozome. This set is the 48 organisms currently stored in a back end CHADO datastore. The data loaders are modified versions of the CHADO data adapters from FlyMine. 2.) Interproscan results from all proteins in the Phytozome database. 3.) Clusters of proteins into a grouped heirarchically by similarity. 4.) Cufflinks results from tissue-specific RNA-Seq data of Phytozome organisms. 5.) Diversity data (GATK and SnpEFF results) from a set of individual organism. The last two datatypes are new in this implementation of our web services. We anticipate that the scale of these data will increase considerably in the near future.

  12. WE-A-17A-10: Fast, Automatic and Accurate Catheter Reconstruction in HDR Brachytherapy Using An Electromagnetic 3D Tracking System

    SciTech Connect (OSTI)

    Poulin, E; Racine, E; Beaulieu, L; Binnekamp, D

    2014-06-15

    Purpose: In high dose rate brachytherapy (HDR-B), actual catheter reconstruction protocols are slow and errors prompt. The purpose of this study was to evaluate the accuracy and robustness of an electromagnetic (EM) tracking system for improved catheter reconstruction in HDR-B protocols. Methods: For this proof-of-principle, a total of 10 catheters were inserted in gelatin phantoms with different trajectories. Catheters were reconstructed using a Philips-design 18G biopsy needle (used as an EM stylet) and the second generation Aurora Planar Field Generator from Northern Digital Inc. The Aurora EM system exploits alternating current technology and generates 3D points at 40 Hz. Phantoms were also scanned using a ?CT (GE Healthcare) and Philips Big Bore clinical CT system with a resolution of 0.089 mm and 2 mm, respectively. Reconstructions using the EM stylet were compared to ?CT and CT. To assess the robustness of the EM reconstruction, 5 catheters were reconstructed twice and compared. Results: Reconstruction time for one catheter was 10 seconds or less. This would imply that for a typical clinical implant of 17 catheters, the total reconstruction time would be less than 3 minutes. When compared to the ?CT, the mean EM tip identification error was 0.69 0.29 mm while the CT error was 1.08 0.67 mm. The mean 3D distance error was found to be 0.92 0.37 mm and 1.74 1.39 mm for the EM and CT, respectively. EM 3D catheter trajectories were found to be significantly more accurate (unpaired t-test, p < 0.05). A mean difference of less than 0.5 mm was found between successive EM reconstructions. Conclusion: The EM reconstruction was found to be faster, more accurate and more robust than the conventional methods used for catheter reconstruction in HDR-B. This approach can be applied to any type of catheters and applicators. We would like to disclose that the equipments, used in this study, is coming from a collaboration with Philips Medical.

  13. Fast, automatic, and accurate catheter reconstruction in HDR brachytherapy using an electromagnetic 3D tracking system

    SciTech Connect (OSTI)

    Poulin, Eric; Racine, Emmanuel; Beaulieu, Luc; Binnekamp, Dirk

    2015-03-15

    Purpose: In high dose rate brachytherapy (HDR-B), current catheter reconstruction protocols are relatively slow and error prone. The purpose of this technical note is to evaluate the accuracy and the robustness of an electromagnetic (EM) tracking system for automated and real-time catheter reconstruction. Methods: For this preclinical study, a total of ten catheters were inserted in gelatin phantoms with different trajectories. Catheters were reconstructed using a 18G biopsy needle, used as an EM stylet and equipped with a miniaturized sensor, and the second generation Aurora{sup ®} Planar Field Generator from Northern Digital Inc. The Aurora EM system provides position and orientation value with precisions of 0.7 mm and 0.2°, respectively. Phantoms were also scanned using a μCT (GE Healthcare) and Philips Big Bore clinical computed tomography (CT) system with a spatial resolution of 89 μm and 2 mm, respectively. Reconstructions using the EM stylet were compared to μCT and CT. To assess the robustness of the EM reconstruction, five catheters were reconstructed twice and compared. Results: Reconstruction time for one catheter was 10 s, leading to a total reconstruction time inferior to 3 min for a typical 17-catheter implant. When compared to the μCT, the mean EM tip identification error was 0.69 ± 0.29 mm while the CT error was 1.08 ± 0.67 mm. The mean 3D distance error was found to be 0.66 ± 0.33 mm and 1.08 ± 0.72 mm for the EM and CT, respectively. EM 3D catheter trajectories were found to be more accurate. A maximum difference of less than 0.6 mm was found between successive EM reconstructions. Conclusions: The EM reconstruction was found to be more accurate and precise than the conventional methods used for catheter reconstruction in HDR-B. This approach can be applied to any type of catheters and applicators.

  14. Bio-Inspired Cyber Security for Smart Grid Deployments

    SciTech Connect (OSTI)

    McKinnon, Archibald D.; Thompson, Seth R.; Doroshchuk, Ruslan A.; Fink, Glenn A.; Fulp, Errin W.

    2013-05-01

    mart grid technologies are transforming the electric power grid into a grid with bi-directional flows of both power and information. Operating millions of new smart meters and smart appliances will significantly impact electric distribution systems resulting in greater efficiency. However, the scale of the grid and the new types of information transmitted will potentially introduce several security risks that cannot be addressed by traditional, centralized security techniques. We propose a new bio-inspired cyber security approach. Social insects, such as ants and bees, have developed complex-adaptive systems that emerge from the collective application of simple, light-weight behaviors. The Digital Ants framework is a bio-inspired framework that uses mobile light-weight agents. Sensors within the framework use digital pheromones to communicate with each other and to alert each other of possible cyber security issues. All communication and coordination is both localized and decentralized thereby allowing the framework to scale across the large numbers of devices that will exist in the smart grid. Furthermore, the sensors are light-weight and therefore suitable for implementation on devices with limited computational resources. This paper will provide a brief overview of the Digital Ants framework and then present results from test bed-based demonstrations that show that Digital Ants can identify a cyber attack scenario against smart meter deployments.

  15. DataFoundry: Warehousing techniques for dynamic environments

    SciTech Connect (OSTI)

    Critchlow, T.; Fidelis, K.; Ganesh, M.; Musick, R.; Slezak, T., LLNL

    1998-01-29

    Data warehouses and data marts have been successfully applied to a multitude of commercial business applications as tools for integrating and providing access to data located across an enterprise. Although the need for this capability is as vital in the scientific world as in the business domain, working warehouses in our community are scarce. A primary technical reason for this is that our understanding of the concepts being explored in an evolving scientific domain change constantly, leading to rapid changes in the data representation. When any database providing information to a warehouse changes its format, the warehouse must be updated to reflect these changes, or it will not function properly. The cost of maintaining a warehouse using traditional techniques in this environment is prohibitive. This paper describes ideas for dramatically reducing the amount of work that must be done to keep a warehouse up to date in a dynamic, scientific environment. The ideas are being applied in a prototype warehouse called DataFoundry. DataFoundry, currently in use by structural biologists at LLNL, will eventually support scientists at the Department of Energy`s Joint Genome Institute.

  16. Earth's mysterious atmosphere. ATLAS 1: Teachers guide with activities

    SciTech Connect (OSTI)

    Not Available

    1991-11-01

    One of our mission's primary goals is to better understand the physics and chemistry of our atmosphere, the thin envelope of air that provides for human life and shields us from the harshness of space. The Space Shuttle Atlantis will carry the ATLAS 1 science instruments 296 km above Earth, so that they can look down into and through the various layers of the atmosphere. Five solar radiometers will precisely measure the amount of energy the Sun injects into Earth's environment. The chemistry at different altitudes will be measured very accurately by five other instruments called spectrometers. Much of our time in the cockpit of Atlantis will be devoted to two very exciting instruments that measure the auroras and the atmosphere's electrical characteristics. Finally, our ultraviolet telescope will probe the secrets of fascinating celestial objects. This Teacher's Guide is designed as a detective story to help you appreciate some of the many questions currently studied by scientists around the world. Many complex factors affect our atmosphere today, possibly even changing the course of global climate. All who live on Earth must recognize that they play an ever-growing role in causing some of these changes. People must solve this great atmospheric mystery if they are to understand all these changes and know what to do about them.

  17. The flavonoid eupatorin inactivates the mitotic checkpoint leading to polyploidy and apoptosis

    SciTech Connect (OSTI)

    Salmela, Anna-Leena; Turku Graduate School of Biomedical Sciences, Turku; Turku Centre for Biotechnology, P.O. Box 123, University of Turku ; Pouwels, Jeroen; Kukkonen-Macchi, Anu; Waris, Sinikka; Toivonen, Pauliina; Jaakkola, Kimmo; Maeki-Jouppila, Jenni; Turku Centre for Biotechnology, P.O. Box 123, University of Turku; Drug Discovery Graduate School, University of Turku ; Kallio, Lila; Kallio, Marko J.; Turku Centre for Biotechnology, P.O. Box 123, University of Turku; Centre of Excellence for Translational Genome-Scale Biology, P.O. Box 106, Academy of Finland

    2012-03-10

    The spindle assembly checkpoint (SAC) is a conserved mechanism that ensures the fidelity of chromosome distribution in mitosis by preventing anaphase onset until the correct bipolar microtubule-kinetochore attachments are formed. Errors in SAC function may contribute to tumorigenesis by inducing numerical chromosome anomalies (aneuploidy). On the other hand, total disruption of SAC can lead to massive genomic imbalance followed by cell death, a phenomena that has therapeutic potency. We performed a cell-based high-throughput screen with a compound library of 2000 bioactives for novel SAC inhibitors and discovered a plant-derived phenolic compound eupatorin (3 Prime ,5-dihydroxy-4 Prime ,6,7-trimethoxyflavone) as an anti-mitotic flavonoid. The premature override of the microtubule drug-imposed mitotic arrest by eupatorin is dependent on microtubule-kinetochore attachments but not interkinetochore tension. Aurora B kinase activity, which is essential for maintenance of normal SAC signaling, is diminished by eupatorin in cells and in vitro providing a mechanistic explanation for the observed forced mitotic exit. Eupatorin likely has additional targets since eupatorin treatment of pre-mitotic cells causes spindle anomalies triggering a transient M phase delay followed by impaired cytokinesis and polyploidy. Finally, eupatorin potently induces apoptosis in multiple cancer cell lines and suppresses cancer cell proliferation in organotypic 3D cell culture model.

  18. STELLAR WIND INDUCED SOFT X-RAY EMISSION FROM CLOSE-IN EXOPLANETS

    SciTech Connect (OSTI)

    Kislyakova, K. G.; Lammer, H.; Fossati, L.; Johnstone, C. P.; Holmström, M.; Zaitsev, V. V.

    2015-01-30

    In this Letter, we estimate the X-ray emission from close-in exoplanets. We show that the Solar/Stellar Wind Charge Exchange Mechanism (SWCX), which produces soft X-ray emission, is very effective for hot Jupiters. In this mechanism, X-ray photons are emitted as a result of the charge exchange between heavy ions in the solar wind and the atmospheric neutral particles. In the solar system, comets produce X-rays mostly through the SWCX mechanism, but it has also been shown to operate in the heliosphere, in the terrestrial magnetosheath, and on Mars, Venus, and the Moon. Since the number of emitted photons is proportional to the solar wind mass flux, this mechanism is not very effective for the solar system giants. Here we present a simple estimate of the X-ray emission intensity that can be produced by close-in extrasolar giant planets due to charge exchange with the heavy ions of the stellar wind. Using the example of HD 209458b, we show that this mechanism alone can be responsible for an X-ray emission of ≈10{sup 22} erg s{sup –1}, which is 10{sup 6} times stronger than the emission from the Jovian aurora. We discuss also the possibility of observing the predicted soft X-ray flux of hot Jupiters and show that despite high emission intensities they are unobservable with current facilities.

  19. Solid-state dosimeters: A new approach for mammography measurements

    SciTech Connect (OSTI)

    Brateman, Libby F.; Heintz, Philip H.

    2015-02-15

    Purpose: To compare responses of modern commercially available solid-state dosimeters (SStDs) used in mammography medical physics surveys for two major vendors of current digital mammography units. To compare differences in dose estimates among SStD responses with ionization chamber (IC) measurements for several target/filter (TF) combinations and report their characteristics. To review scientific bases for measurements of quantities required for mammography for traditional measurement procedures and SStDs. Methods: SStDs designed for use with modern digital mammography units were acquired for evaluation from four manufacturers. Each instrument was evaluated under similar conditions with the available mammography beams provided by two modern full-field digital mammography units in clinical use: a GE Healthcare Senographe Essential (Essential) and a Hologic Selenia Dimensions 5000 (Dimensions), with TFs of Mo/Mo, Mo/Rh; and Rh/Rh and W/Rh, W/Ag, and W/Al, respectively. Measurements were compared among the instruments for the TFs over their respective clinical ranges of peak tube potentials for kVp and half-value layer (HVL) measurements. Comparisons for air kerma (AK) and their associated relative calculated average glandular doses (AGDs), i.e., using fixed mAs, were evaluated over the limited range of 2830 kVp. Measurements were compared with reference IC measurements for AK, reference HVLs and calculated AGD, for two compression paddle heights for AK, to evaluate scatter effects from compression paddles. SStDs may require different positioning from current mammography measurement protocols. Results: Measurements of kVp were accurate in general for the SStDs (within ?1.2 and +1.1 kVp) for all instruments over a wide range of set kVps and TFs and most accurate for Mo/Mo and W/Rh. Discrepancies between measurements and reference values were greater for HVL and AK. Measured HVL values differed from reference values by ?6.5% to +3.5% depending on the SStD and TF. AK

  20. An improved catalog of halo wide binary candidates

    SciTech Connect (OSTI)

    Allen, Christine; Monroy-Rodríguez, Miguel A.

    2014-08-01

    We present an improved catalog of halo wide binaries compiled from an extensive literature search. Most of our binaries stem from the common proper motion binary catalogs by Allen et al. and Chanamé and Gould, but we have also included binaries from the lists of Ryan and Zapatero-Osorio and Martín. All binaries were carefully checked and their distances and systemic radial velocities are included when available. Probable membership to the halo population was tested by means of reduced proper motion diagrams for 251 candidate halo binaries. After eliminating obvious disk binaries, we ended up with 211 probable halo binaries, 150 of which have radial velocities available. We compute galactic orbits for these 150 binaries and calculate the time they spend within the galactic disk. Considering the full sample of 251 candidate halo binaries as well as several subsamples, we find that the distribution of angular separations (or expected major semiaxes) follows a power law f(a) ∼ a {sup –1} (Oepik's relation) up to different limits. For the 50 most disk-like binaries, those that spend their entire lives within z = ±500 pc, this limit is found to be 19,000 AU (0.09 pc), while for the 50 most halo-like binaries, those that spend on average only 18% of their lives within z = ±500 pc, the limit is 63,000 AU (0.31 pc). In a companion paper, we employ this catalog to establish limits on the masses of the halo massive perturbers (massive compact halo objects).

  1. SciFri PM: Topics 08: The Role and Benefits of Electromagnetic Needle-Tracking Technologies in Brachytherapy

    SciTech Connect (OSTI)

    Beaulieu, L.; Racine, E.; Boutaleb, S.; Filion, O.; Poulin, E.; Hautvast, G.; Binnekamp, D.

    2014-08-15

    In modern brachytherapy, application of large doses of ionizing radiation in a limited number of fractions is frequent. Furthermore, as with any surgical procedures, brachytherapy is subject to learning curve effects. In this context, there could be advantages of integrating real-time tracking of needles/catheters to existing protocols given the recent prominent advances in tracking technologies. In this work, we review the use of an electromagnetic tracking system (EMTS) based on the second generation Aurora Planar Field Generator (Northern Digital Inc) and custom design needles (Philips Healthcare) for brachytherapy applications. The position and orientation information is obtained from 5 degrees of freedom sensors. Basic system performance characterization is performed in well-controlled conditions to establish accuracy and reproducibility as well as potential interference from standard brachytherapy equipment. The results show that sensor locations can be tracked to within 0.04mm (la) when located within 26cm of the generator. Orientation accuracy of the needle remained within 1 in the same region, but rose quickly at larger distances. The errors on position and orientation strongly dependent the sensor position in the characterization volume (500500500mm{sup 3}). The presence of an ultrasound probe was shown to have negligible effects on tracking accuracy. The use of EMTS for automatic catheter/applicator reconstruction was also explored. Reconstruction time was less than 10 sec/channel and tips identification was within 0.690.29mm of the reference values. Finally, we demonstrate that hollow needle designs with special EM adaptation also allow for real-time seed drop position estimation. In phantom experiments showed that drop positions were on average within 1.60.9mm of the reference position measured from ?CT. Altogether, EMTS offer promising benefits in a wide range of brachytherapy applications.

  2. WE-A-17A-09: Exploiting Electromagnetic Technologies for Real-Time Seed Drop Position Validation in Permanent Implant Brachytherapy

    SciTech Connect (OSTI)

    Racine, E; Hautvast, G; Binnekamp, D; Beaulieu, L

    2014-06-15

    Purpose: To report on preliminary results validating the performance of a specially designed LDR brachytherapy needle prototype possessing both electromagnetic (EM) tracking and seed drop detection abilities. Methods: An EM hollow needle prototype has been designed and constructed in collaboration with research partner Philips Healthcare. The needle possesses conventional 3D tracking capabilities, along with a novel seed drop detection mechanism exploiting local changes of electromagnetic properties generated by the passage of seeds in the needle's embedded sensor coils. These two capabilities are exploited by proprietary engineering and signal processing techniques to generate seed drop position estimates in real-time treatment delivery. The electromagnetic tracking system (EMTS) used for the experiment is the NDI Aurora Planar Field Generator. The experiment consisted of dropping a total of 35 seeds in a prismatic agarose phantom, and comparing the 3D seed drop positions of the EMTS to those obtained by an image analysis of subsequent micro-CT scans. Drop position error computations and statistical analysis were performed after a 3D registration of the two seed distributions. Results: Of the 35 seeds dropped in the phantom, 32 were properly detected by the needle prototype. Absolute drop position errors among the detected seeds ranged from 0.5 to 4.8 mm with mean and standard deviation values of 1.6 and 0.9 mm, respectively. Error measurements also include undesirable and uncontrollable effects such as seed motion upon deposition. The true accuracy performance of the needle prototype is therefore underestimated. Conclusion: This preliminary study demonstrates the potential benefits of EM technologies in detecting the passage of seeds in a hollow needle as a means of generating drop position estimates in real-time treatment delivery. Such tools could therefore represent a potentially interesting addition to existing brachytherapy protocols for rapid dosimetry

  3. Managing Floods and Resources at the Arroyo Las Positas

    SciTech Connect (OSTI)

    Sanchez, L; Van Hattem, M; Mathews, S

    2002-03-05

    Engineers and water resource professionals are challenged with protecting facilities from flood events within environmental resource protection, regulatory, and economic constraints. One case in point is the Arroyo Las Positas (ALP), an intermittent stream that traverses the Lawrence Livermore National Laboratory (LLNL) in Livermore, California. Increased runoff from post-drought rainfall, upstream development, and new perennial discharges from LLNL activities have resulted in increased dry weather flows and wetland vegetation. These new conditions have recently begun to provide improved habitat for the federally threatened California red-legged frog (Rana aurora draytonii; CRLF), but the additional vegetation diminishes the channel's drainage capacity and increases flood risk. When LLNL proposed to re-grade the channel to reestablish the 100-year flood capacity, traditional dredging practices were no longer being advocated by environmental regulatory agencies. LLNL therefore designed a desilting maintenance plan to protect LLNL facility areas from flooding, while minimizing impacts to wetland resources and habitat. The result was a combination of structural upland improvements and the ALP Five Year Maintenance Plan (Maintenance Plan), which includes phased desilting in segments so that the entire ALP is desilted after five years. A unique feature of the Maintenance Plan is the variable length of the segments designed to minimize LLNL's impact on CRLF movement. State and federal permits also added monitoring requirements and additional constraints on desilting activities. Two years into the Maintenance Plan, LLNL is examining the lessons learned on the cost-effectiveness of these maintenance measures and restrictions and reevaluating the direction of future maintenance activities.

  4. Physics Division progress report, January 1, 1984-September 30, 1986

    SciTech Connect (OSTI)

    Keller, W.E.

    1987-10-01

    This report provides brief accounts of significant progress in development activities and research results achieved by Physics Division personnel during the period January 1, 1984, through September 31, 1986. These efforts are representative of the three main areas of experimental research and development in which the Physics Division serves Los Alamos National Laboratory's and the Nation's needs in defense and basic sciences: (1) defense physics, including the development of diagnostic methods for weapons tests, weapon-related high-energy-density physics, and programs supporting the Strategic Defense Initiative; (2) laser physics and applications, especially to high-density plasmas; and (3) fundamental research in nuclear and particle physics, condensed-matter physics, and biophysics. Throughout the report, emphasis is placed on the design, construction, and application of a variety of advanced, often unique, instruments and instrument systems that maintain the Division's position at the leading edge of research and development in the specific fields germane to its mission. A sampling of experimental systems of particular interest would include the relativistic electron-beam accelerator and its applications to high-energy-density plasmas; pulsed-power facilities; directed energy weapon devices such as free-electron lasers and neutral-particle-beam accelerators; high-intensity ultraviolet and x-ray beam lines at the National Synchrotron Light Source (at Brookhaven National Laboratory); the Aurora KrF ultraviolet laser system for projected use as an inertial fusion driver; antiproton physics facility at CERN; and several beam developments at the Los Alamos Meson Physics Facility for studying nuclear, condensed-matter, and biological physics, highlighted by progress in establishing the Los Alamos Neutron Scattering Center.

  5. Fast iterative technique for the calculation of frequency dependent gain in excimer laser amplifiers

    SciTech Connect (OSTI)

    Sze, R.C.

    1991-01-01

    The motivation in initiating these calculations is to allow us to observe the frequency evolution of a laser pulse as it propagates through an amplifier and then through a sequence of amplifiers. The question we seek to answer is what pulse shape do we need to produce out of a front-end oscillator so that after it propagates through the whole Aurora KrF fusion amplifier chain will result in high energy, broad-band laser fields of a given bandwidth that can be focussed onto a fusion target. The propagation of a single frequency source through an amplifier with distributed loss was considered by Rigrod and was significantly expanded by Hunter and Hunter. The latter included amplified spontaneous emission (ASE) considerations both in the direction of and transverse to the coherent field. Analytic solutions that include forward and backward prapagating fields and ASE were derived which were transcendental in nature but allowed for fairly easy computer calculations. Transverse ASE were calculated using the unsaturated gain resulting from longitudinal fields and were used to compare this with the longitudinal field equations. Large computer programs are now available at LANL which include the influence of transverse ASE on the longitudinal fields. However, none of these considerations have worried about the changes in the frequency characteristics of the propagating field or of how each of the frequency field components contributes to the saturation of the gain. The inclusion of full frequency characteristics to the analytic solutions of Hunter and Hunter proved impossible at least for this author and a new calculational technique was developed and is the subject of this talk.

  6. EUV studies of N/sub 2/ and O/sub 2/ produced by low energy electron impact

    SciTech Connect (OSTI)

    Morgan, H.D.; Mentall, J.E.

    1983-02-15

    The emission spectrum of atomic nitrogen (NI), singly ionized atomic nitrogen (NII), atomic oxygen (OI), singly ionized atomic oxygen (OII), and molecular nitrogen (N/sub 2/) dominates the day airglow and aurora spectrum in the extreme ultraviolet. However, analysis of the excitation of these lines is not possible due to the lack of laboratory or theoretical data for the relevant processes. Absolute emission excitation cross sections resulting from low energy electron impact on N/sub 2/ and O/sub 2/ have been measured in the extreme vacuum ultraviolet (500--1200 A). Electron energies were from 0 to 300 eV. Numerous bands of N/sub 2/ were found between 800 and 1000 A. These band systems are of particular interest because their optical oscillator strengths are unusually large and should have large emission cross sections. Excitation functions were measured for the N/sub 2/ c' /sup 1/..sigma../sup +//sub u/ ..-->.. X /sup 1/..sigma../sup +//sub g/ v' = 0-v'' = 0 band emission, the NII 916 A multiplet, the OI 879 A multiplet, and the OII 834 A multiplet. In addition, cross sections were measured at 200 eV only for several of the band emissions plus the NI 1135 A, NI 1164 A, NI 1177 A, NII 776 A, NII 1084 A, OI 1152 A, OI 1041 A, OI 1027 A, OI 999 A, OI 989 A, OI 879 A, OII 834 A, OII 616 A, OII 555 A, OII 539 A, and OII 718 A multiplets.

  7. Measuring the seeds of ion outflow: auroral sounding rocket observations of low-altitude ion heating and circulation

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

    Fernandes, P. A.; Lynch, K. A.; Zettergren, M.; Hampton, D. L.; Bekkeng, T. A.; Cohen, I. J.; Conde, M.; Fisher, L. E.; Horak, P.; Lessard, M. R.; et al

    2016-01-25

    Here, we present an analysis of in situ measurements from the MICA (Magnetosphere-Ionosphere Coupling in the Alfvén Resonator) nightside auroral sounding rocket with comparisons to a multifluid ionospheric model. MICA made observations at altitudes below 325 km of the thermal ion kinetic particle distributions that are the origins of ion outflow. Late flight, in the vicinity of an auroral arc, we observe frictional processes controlling the ion temperature. Upflow of these cold ions is attributed to either the ambipolar field resulting from the heated electrons or possibly to ion-neutral collisions. We measure E→xB→ convection away from the arc (poleward) andmore » downflows of hundreds of m s-1 poleward of this arc, indicating small-scale low-altitude plasma circulation. In the early flight we observe DC electromagnetic Poynting flux and associated ELF wave activity influencing the thermal ion temperature in regions of Alfvénic aurora. We observe enhanced, anisotropic ion temperatures which we conjecture are caused by transverse heating by wave-particle interactions (WPI) even at these low altitudes. Throughout this region we observe several hundred m s-1 upflow of the bulk thermal ions colocated with WPI; however, the mirror force is negligible at these low energies; thus, the upflow is attributed to ambipolar fields (or possibly neutral upwelling drivers). Moreover, the low-altitude MICA observations serve to inform future ionospheric modeling and simulations of (a) the need to consider the effects of heating by WPI at altitudes lower than previously considered viable and (b) the occurrence of structured and localized upflows/downflows below where higher-altitude heating rocesses are expected.« less

  8. Nonlinear plasma experiments in geospace with gigawatts of RF power at HAARP

    SciTech Connect (OSTI)

    Sheerin, J. P.; Cohen, Morris B.

    2015-12-10

    The ionosphere is the ionized uppermost layer of our atmosphere (from 70 – 500 km altitude) where free electron densities yield peak critical frequencies in the HF (3 – 30 MHz) range. The ionosphere thus provides a quiescent plasma target, stable on timescales of minutes, for a whole host of active plasma experiments. High power RF experiments on ionospheric plasma conducted in the U.S. have been reported since 1970. The largest HF transmitter built to date is the HAARP phased-array HF transmitter near Gakona, Alaska which can deliver up to 3.6 Gigawatts (ERP) of CW RF power in the range of 2.8 – 10 MHz to the ionosphere with microsecond pointing, power modulation, and frequency agility. With an ionospheric background thermal energy in the range of only 0.1 eV, this amount of power gives access to the highest regimes of the nonlinearity (RF intensity to thermal pressure) ratio. HAARP’s unique features have enabled the conduct of a number of unique nonlinear plasma experiments in the interaction region of overdense ionospheric plasma including generation of artificial aurorae, artificial ionization layers, VLF wave-particle interactions in the magnetosphere, parametric instabilities, stimulated electromagnetic emissions (SEE), strong Langmuir turbulence (SLT) and suprathermal electron acceleration. Diagnostics include the Modular UHF Ionospheric Radar (MUIR) sited at HAARP, the SuperDARN-Kodiak HF radar, spacecraft radio beacons, HF receivers to record stimulated electromagnetic emissions (SEE) and telescopes and cameras for optical emissions. We report on short timescale ponderomotive overshoot effects, artificial field-aligned irregularities (AFAI), the aspect angle dependence of the intensity of the HF-enhanced plasma line, and production of suprathermal electrons. One of the primary missions of HAARP, has been the generation of ELF (300 – 3000 Hz) and VLF (3 – 30 kHz) radio waves which are guided to global distances in the Earth