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Sample records for grady cle vela

  1. abstract-grady

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

    Building An Integrated Activity-Based and Dynamic Network Assignment Model For Sacramento Area Council of Governments (SACOG) Brian Grady (RSG) and/or Joe Castiglione (RSG) List of Authors ================ Joe Castiglione, Resource Systems Group, Inc. 29 Belmont Street, Somerville, MA 02143 This email address is being protected from spambots. You need JavaScript enabled to view it. Brian Grady, Resource Systems Group, Inc. 55 Railroad Row, White River Junction, VT 05001 802-295-4999 This email

  2. Sheila Grady-McBride | Bioenergy | NREL

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

    Sheila Grady-McBride Sheila Grady-McBride Business Support II, Administrative Associate Sheila.Grady-Mcbride@nrel.gov | 303-384-6220 Areas of Expertise Sheila Grady-McBride joined the National Bioenergy Center at the end of June 2012 as a research support assistant supporting the Thermochemical Group. Prior to joining the National Renewable Energy Laboratory (NREL), Grady-McBride most recently worked at The Beck Group as a project assistant. Before that she worked for 12 years at GE Access as an

  3. Vela | Open Energy Information

    Open Energy Info (EERE)

    to: navigation, search Logo: Vela Name: Vela Place: Dubai, United Arab Emirates Sector: Oil and Gas Product: marine transportation for refined products and crude oi Year Founded:...

  4. Grady County, Oklahoma: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Zone Subtype A. Places in Grady County, Oklahoma Alex, Oklahoma Amber, Oklahoma Blanchard, Oklahoma Bradley, Oklahoma Bridge Creek, Oklahoma Chickasha, Oklahoma Minco,...

  5. German Club for Rural Electrification CLE | Open Energy Information

    Open Energy Info (EERE)

    Electrification CLE Jump to: navigation, search Name: German Club for Rural Electrification (CLE) Place: Freiburg, Germany Zip: 79114 Sector: Renewable Energy Product: German...

  6. The Vela pulsar with an active fallback disk

    SciTech Connect (OSTI)

    Özsükan, Gökçe; Ek?i, K. Yavuz [Faculty of Science and Letters, Department of Physics, ?stanbul Technical University, Maslak 34469, ?stanbul (Turkey); Hambaryan, Valeri; Neuhäuser, Ralph; Hohle, Markus M.; Ginski, Christian [Astrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, Schillergäßchen 2-3, 07745 Jena (Germany); Werner, Klaus, E-mail: eksi@itu.edu.tr [Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, D-72076 Tübingen (Germany)

    2014-11-20

    Fallback disks are expected to form around young neutron stars. The presence of these disks can be revealed by their blackbody spectrum in the infrared, optical, and UV bands. We present a re-reduction of the archival optical and infrared data of the Vela pulsar, together with the existing infrared and UV spectrum of Vela, and model their unpulsed components with the blackbody spectrum of a supernova debris disk. We invoke the quiescent disk solution of Sunyaev and Shakura for the description of the disk in the propeller stage and find the inner radius of the disk to be inside the light cylinder radius. We perform a high-resolution X-ray analysis with XMM-Newton and find a narrow absorption feature at 0.57 keV that can be interpreted as the K {sub ?} line of He-like oxygen (O VII). The strength of the line indicates an element over-abundance in our line of sight exceeding the amounts that would be expected from interstellar medium. The spectral feature may originate from the pulsar wind nebula and may be partly caused by the reprocessed X-ray radiation by the fallback disk. We discuss the lower-than-three braking index of Vela as partially due to the contribution of the propeller torques. Our results suggest that the pulsar mechanism can work simultaneously with the propeller processes and that the debris disks can survive the radiation pressure for at least ?10{sup 4} yr. As Vela is a relatively close object, and a prototypical pulsar, the presence of a disk, if confirmed, may indicate the ubiquity of debris disks around young neutron stars.

  7. Bio Sciences: Ryan Agh Haide Vela-Alvarez Chemistry: Morgan Kelley

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

    Symposium Winners Bio Sciences: Ryan Agh Haide Vela-Alvarez Chemistry: Morgan Kelley Belinda Pacheco Computing: Nicholas Lewis Colin Redman and Gerald Collom Earth and Space Sciences: Sean Dolan Lois Smith Engineering: Babatunde Adigun Lexey Sbriglia Health and Safety: Micaela Christensen Information Technology: Michael Salazar Mathematics: William Casper Material Sciences: Matthew Herman Sergio Pino-Gellardo, Matthew Kroonblawd Purnima Ghale, Georg Hahn, Vivek Sardeshmuckh and Jerry Shi

  8. First light from the Vela pulsar with the Fermi Gamma-ray Space Telescope

    SciTech Connect (OSTI)

    Razzano, M.

    2009-04-08

    The Fermi Gamma-ray Space Telescope, launched in June 2008, is an international space mission entirely devoted to the study of the high-energy gamma rays from the Universe. The main instrument aboard Fermi is the Large Area Telescope (LAT), a pair conversion telescope equipped with the state-of-the art in gamma-ray detectors technology. Thanks to its large field of view and effective area, combined with its excellent timing capability, Fermi-LAT is a perfect instrument for probing physics of gamma-ray emission in pulsars. LAT is expected to discover tens of new pulsars, both radio-loud and radio-quiet (Geminga-like). Moreover, LAT will observe with unprecedented statistics the brightest pulsars, investigating the details of magnetospheric emission. The first two months of the mission have been focused on the commissioning and first light, during which the LAT firmly detected the six previously known EGRET gamma-ray pulsars. One of the main sources of interest during our first light observations has been the Vela pulsar, the brightest persistent source in the whole gamma-ray sky. Thanks to its brightness, the Vela pulsar is an ideal candidate for calibrating the LAT and testing its performance. In addition, observations of Vela will help answer many questions related to the physics of pulsar emission processes. We present here some recent results obtained by the LAT on the Vela pulsar, using high-quality timing solutions provided by radio observations carried out within the Fermi pulsar radio timing campaign.

  9. EXTENDED HARD X-RAY EMISSION FROM THE VELA PULSAR WIND NEBULA

    SciTech Connect (OSTI)

    Mattana, F.; Terrier, R.; Zurita Heras, J. A.; Goetz, D.; Caballero, I.; Soldi, S.; Schanne, S.; Ponti, G.; Falanga, M.; Renaud, M.

    2011-12-10

    The nebula powered by the Vela pulsar is one of the best examples of an evolved pulsar wind nebula, allowing access to the particle injection history and the interaction with the supernova ejecta. We report on the INTEGRAL discovery of extended emission above 18 keV from the Vela nebula. The northern side has no known counterparts and it appears larger and more significant than the southern one, which is in turn partially coincident with the cocoon, the soft X-ray, and TeV filament toward the center of the remnant. We also present the spectrum of the Vela nebula in the 18-400 keV energy range as measured by IBIS/ISGRI and SPI on board the INTEGRAL satellite. The apparent discrepancy between IBIS/ISGRI, SPI, and previous measurements is understood in terms of the point-spread function, supporting the hypothesis of a nebula more diffuse than previously thought. A break at {approx}25 keV is found in the spectrum within 6' from the pulsar after including the Suzaku XIS data. Interpreted as a cooling break, this points out that the inner nebula is composed of electrons injected in the last {approx}2000 years. Broadband modeling also implies a magnetic field higher than 10 {mu}G in this region. Finally, we discuss the nature of the northern emission, which might be due to fresh particles injected after the passage of the reverse shock.

  10. VELA program. A twenty-five year review of basic research

    SciTech Connect (OSTI)

    Kerr, A.U.

    1985-01-01

    Partial Contents: A Review of Test Ban Research; Underground Nuclear Weapons Testing and Seismology - A Cooperative Effort; Forensic Seismology; Technical Issues Related to Nuclear Test Ban Treaties; VELA Overview: The Early Years of the Seismic Research Program; Explosion/Earthquake Source Theory; Linear Elastic Waveform Modeling in the Inelastic Region of Underground Nuclear Explosions; Seismic Wave Propagation Effects; Development of Theory and Numerical Modeling; In-Situ Paths Strain and Stress Bounds with Application to Desert Alluvium; Seismic Scattering and Lithospheric Heterogeneity; Body Wave Propagation in three-Dimensional Source and Receiver Structure; Instrumentation and Signal Analysis; Regional Seismic Array Program and High Frequency Instrumentation; Signal Analysis: Explosion Seismology; Earthquake or Explosion: Where are We Now; Teleseismic Methods; Regional Methods; and Tools for Seismic Data Analysis and Management for Research and International Data Exchange.

  11. Microsoft Word - CLE_2.1_Post-Mortem_2009-v9-Accepted.doc

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

    08 Proceedings 1 of 8 Post-Mortem of the NERSC Franklin XT Upgrade to CLE 2.1 James M. Craw, Nicholas P. Cardo, Yun (Helen) He Lawrence Berkeley National Laboratory National Energy Research Scientific Computing Center Berkeley, CA 94720 craw@nersc.gov, cardo@nersc.gov, yhe@lbl.gov And Janet M. Lebens Cray, Inc. jml@cray.com ABSTRACT: This paper will discuss the lessons learned of the events leading up to the production deployment of CLE 2.1 and the post install issues experienced in upgrading

  12. THE YOUNG STELLAR OBJECT POPULATION IN THE VELA-D MOLECULAR CLOUD

    SciTech Connect (OSTI)

    Strafella, F.; Maruccia, Y.; Maiolo, B.; Lorenzetti, D.; Giannini, T.; Elia, D.; Molinari, S.; Pezzuto, S.; Massi, F.; Olmi, L.

    2015-01-10

    We investigate the young stellar population in the Vela Molecular Ridge, Cloud-D, a star-forming region observed by both the Spitzer/NASA and Herschel/ESA space telescopes. The point-source, band-merged, Spitzer-IRAC catalog complemented with MIPS photometry previously obtained is used to search for candidate young stellar objects (YSOs), also including sources detected in less than four IRAC bands. Bona fide YSOs are selected by using appropriate color-color and color-magnitude criteria aimed at excluding both Galactic and extragalactic contaminants. The derived star formation rate and efficiency are compared with the same quantities characterizing other star-forming clouds. Additional photometric data, spanning from the near-IR to the submillimeter, are used to evaluate both bolometric luminosity and temperature for 33 YSOs located in a region of the cloud observed by both Spitzer and Herschel. The luminosity-temperature diagram suggests that some of these sources are representative of Class 0 objects with bolometric temperatures below 70 K and luminosities of the order of the solar luminosity. Far-IR observations from the Herschel/Hi-GAL key project for a survey of the Galactic plane are also used to obtain a band-merged photometric catalog of Herschel sources intended to independently search for protostars. We find 122 Herschel cores located on the molecular cloud, 30 of which are protostellar and 92 of which are starless. The global protostellar luminosity function is obtained by merging the Spitzer and Herschel protostars. Considering that 10 protostars are found in both the Spitzer and Herschel lists, it follows that in the investigated region we find 53 protostars and that the Spitzer-selected protostars account for approximately two-thirds of the total.

  13. THE SPITZER-IRAC POINT-SOURCE CATALOG OF THE VELA-D CLOUD

    SciTech Connect (OSTI)

    Strafella, F.; Elia, D.; Campeggio, L. E-mail: loretta.campeggio@le.infn.i

    2010-08-10

    This paper presents the observations of Cloud D in the Vela Molecular Ridge, obtained with the Infrared Array Camera (IRAC) camera on board the Spitzer Space Telescope at the wavelengths {lambda} = 3.6, 4.5, 5.8, and 8.0 {mu}m. A photometric catalog of point sources, covering a field of approximately 1.2 deg{sup 2}, has been extracted and complemented with additional available observational data in the millimeter region. Previous observations of the same region, obtained with the Spitzer MIPS camera in the photometric bands at 24 {mu}m and 70 {mu}m, have also been reconsidered to allow an estimate of the spectral slope of the sources in a wider spectral range. A total of 170,299 point sources, detected at the 5{sigma} sensitivity level in at least one of the IRAC bands, have been reported in the catalog. There were 8796 sources for which good quality photometry was obtained in all four IRAC bands. For this sample, a preliminary characterization of the young stellar population based on the determination of spectral slope is discussed; combining this with diagnostics in the color-magnitude and color-color diagrams, the relative population of young stellar objects (YSOs) in different evolutionary classes has been estimated and a total of 637 candidate YSOs have been selected. The main differences in their relative abundances have been highlighted and a brief account for their spatial distribution is given. The star formation rate has also been estimated and compared with the values derived for other star-forming regions. Finally, an analysis of the spatial distribution of the sources by means of the two-point correlation function shows that the younger population, constituted by the Class I and flat-spectrum sources, is significantly more clustered than the Class II and III sources.

  14. SPITZER-IRAC SURVEY OF MOLECULAR JETS IN VELA-D

    SciTech Connect (OSTI)

    Giannini, T.; Lorenzetti, D.; Nisini, B.; Salama, A.; De Luca, M.; Strafella, F.; Maiolo, B.; Maruccia, Y.; Elia, D.; Marengo, M.; Massi, F.; Olmi, L.; Smith, H. A.

    2013-04-20

    We present a survey of H{sub 2} jets from young protostars in the Vela-D molecular cloud (VMR-D), based on Spitzer-IRAC data between 3.6 {mu}m and 8.0 {mu}m. Our search has led to the identification of 15 jets (two new discoveries) and about 70 well-aligned knots within 1.2 deg{sup 2}. We compare the Infrared Array Camera (IRAC) maps with observations of the H{sub 2} 1-0 S(1) line at 2.12 {mu}m, with a Spitzer-MIPS map at 24 {mu}m and 70 {mu}m, and with a map of the dust continuum emission at 1.2 mm. From such a comparison, we find a tight association between molecular jets and dust peaks. The jet candidate exciting sources have been searched for in the published catalog of the young stellar objects of VMR-D. In particular, we searched for all the sources of Class II or (preferentially) earlier which are located close to the jet center and aligned with it. Furthermore, the association between jet and exciting source was validated by estimating the differential extinction between the jet opposite lobes. We are able to find a best-candidate exciting source in all but two jets, for which two alternative candidates are given. Four exciting sources are not (or very barely) observed at wavelengths shorter than 24 {mu}m, suggesting that they are very young protostars. Three of them are also associated with the most compact jets (projected length {approx}<0.1 pc). The exciting source spectral energy distributions (SEDs) have been constructed and modeled by means of all the available photometric data between 1.2 {mu}m and 1.2 mm. From SEDs fits, we derive the main source parameters, which indicate that most of them are low-mass protostars. A significant correlation is found between the projected jet length and the [24]-[70] color, which is consistent with an evolutionary scenario according to which shorter jets are associated with younger sources. A rough correlation is found between IRAC line cooling and exciting source bolometric luminosity, in agreement with the previous

  15. Grady Electric Membership Corp | Open Energy Information

    Open Energy Info (EERE)

    2010 - File1a1 EIA Form 861 Data Utility Id 7450 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes Activity Retail Marketing Yes This article is a stub. You can...

  16. The Off-Site Plowshare and Vela Uniform Programs: Assessing Potential Environmental Liabilities through an Examination of Proposed Nuclear Projects,High Explosive Experiments, and High Explosive Construction Activities Volume 3 of 3

    SciTech Connect (OSTI)

    Beck Colleen M.,Edwards Susan R.,King Maureen L.

    2011-09-01

    This document presents the results of nearly six years (2002-2008) of historical research and field studies concerned with evaluating potential environmental liabilities associated with U.S. Atomic Energy Commission projects from the Plowshare and Vela Uniform Programs. The Plowshare Program's primary purpose was to develop peaceful uses for nuclear explosives. The Vela Uniform Program focused on improving the capability of detecting, monitoring and identifying underground nuclear detonations. As a result of the Project Chariot site restoration efforts in the early 1990s, there were concerns that there might be other project locations with potential environmental liabilities. The Desert Research Institute conducted archival research to identify projects, an analysis of project field activities, and completed field studies at locations where substantial fieldwork had been undertaken for the projects. Although the Plowshare and Vela Uniform nuclear projects are well known, the projects that are included in this research are relatively unknown. They are proposed nuclear projects that were not executed, proposed and executed high explosive experiments, and proposed and executed high explosive construction activities off the Nevada Test Site. The research identified 170 Plowshare and Vela Uniform off-site projects and many of these had little or no field activity associated with them. However, there were 27 projects that merited further investigation and field studies were conducted at 15 locations.

  17. The Off-Site Plowshare and Vela Uniform Programs: Assessing Potential Environmental Liabilities through an Examination of Proposed Nuclear Projects,High Explosive Experiments, and High Explosive Construction Activities Volume 2 of 3

    SciTech Connect (OSTI)

    Beck Colleen M.,Edwards Susan R.,King Maureen L.

    2011-09-01

    This document presents the results of nearly six years (2002-2008) of historical research and field studies concerned with evaluating potential environmental liabilities associated with U.S. Atomic Energy Commission projects from the Plowshare and Vela Uniform Programs. The Plowshare Program's primary purpose was to develop peaceful uses for nuclear explosives. The Vela Uniform Program focused on improving the capability of detecting, monitoring and identifying underground nuclear detonations. As a result of the Project Chariot site restoration efforts in the early 1990s, there were concerns that there might be other project locations with potential environmental liabilities. The Desert Research Institute conducted archival research to identify projects, an analysis of project field activities, and completed field studies at locations where substantial fieldwork had been undertaken for the projects. Although the Plowshare and Vela Uniform nuclear projects are well known, the projects that are included in this research are relatively unknown. They are proposed nuclear projects that were not executed, proposed and executed high explosive experiments, and proposed and executed high explosive construction activities off the Nevada Test Site. The research identified 170 Plowshare and Vela Uniform off-site projects and many of these had little or no field activity associated with them. However, there were 27 projects that merited further investigation and field studies were conducted at 15 locations.

  18. The Off-Site Plowshare and Vela Uniform Programs: Assessing Potential Environmental Liabilities through an Examination of Proposed Nuclear Projects,High Explosive Experiments, and High Explosive Construction Activities Volume 1 of 3

    SciTech Connect (OSTI)

    Beck Colleen M,Edwards Susan R.,King Maureen L.

    2011-09-01

    This document presents the results of nearly six years (2002-2008) of historical research and field studies concerned with evaluating potential environmental liabilities associated with U.S. Atomic Energy Commission projects from the Plowshare and Vela Uniform Programs. The Plowshare Program's primary purpose was to develop peaceful uses for nuclear explosives. The Vela Uniform Program focused on improving the capability of detecting, monitoring and identifying underground nuclear detonations. As a result of the Project Chariot site restoration efforts in the early 1990s, there were concerns that there might be other project locations with potential environmental liabilities. The Desert Research Institute conducted archival research to identify projects, an analysis of project field activities, and completed field studies at locations where substantial fieldwork had been undertaken for the projects. Although the Plowshare and Vela Uniform nuclear projects are well known, the projects that are included in this research are relatively unknown. They are proposed nuclear projects that were not executed, proposed and executed high explosive experiments, and proposed and executed high explosive construction activities off the Nevada Test Site. The research identified 170 Plowshare and Vela Uniform off-site projects and many of these had little or no field activity associated with them. However, there were 27 projects that merited further investigation and field studies were conducted at 15 locations.

  19. VELA_COMP_OUT

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

    I. Strong & R. Olson (LANL) NASA Swift Spacecraft devoted to the study of cosmic gamma-ray bursts (Credit: NASAGSFC) The U.S. Nuclear Detonation Detection System is managed as a...

  20. VELA_COMP_OUT

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

    as experimental payloads on the Space Shuttle, the Space Station, and other spacecraft. ... December 1960 USAF, NASA, and AEC representatives meet to define satellite system to ...

  1. ON THE EXPANSION RATE, AGE, AND DISTANCE OF THE SUPERNOVA REMNANT G266.2–1.2 (Vela Jr.)

    SciTech Connect (OSTI)

    Allen, G. E.; Chow, K.; DeLaney, T.; Filipović, M. D.; Houck, J. C.; Pannuti, T. G.; Stage, M. D. E-mail: kc71135@gmail.com E-mail: m.filipovic@uws.edu.au E-mail: t.pannuti@moreheadstate.edu

    2015-01-10

    An analysis of Chandra ACIS data for two relatively bright and narrow portions of the northwestern rim of G266.2–1.2 (a.k.a. RX J0852.0-4622 or Vela Jr.) reveal evidence of a radial displacement of 2.40 ± 0.56 arcsec between 2003 and 2008. The corresponding expansion rate (0.42 ± 0.10 arcsec yr{sup –1} or 13.6% ± 4.2% kyr{sup –1}) is about half the rate reported for an analysis of XMM-Newton data from a similar, but not identical, portion of the rim over a similar, but not identical, time interval (0.84 ± 0.23 arcsec yr{sup –1}). If the Chandra rate is representative of the remnant as a whole, then the results of a hydrodynamic analysis suggest that G266.2–1.2 is between 2.4 and 5.1 kyr old if it is expanding into a uniform ambient medium (whether or not it was produced by a Type Ia or Type II event). If the remnant is expanding into the material shed by a steady stellar wind, then the age could be as much as 50% higher. The Chandra expansion rate and a requirement that the shock speed be greater than or equal to 1000 km s{sup –1} yields a lower limit on the distance of 0.5 kpc. An analysis of previously published distance estimates and constraints suggests G266.2–1.2 is no further than 1.0 kpc. This range of distances is consistent with the distance to the nearer of two groups of material in the Vela Molecular Ridge (0.7 ± 0.2 kpc) and to the Vel OB1 association (0.8 kpc)

  2. OFF VUF-2700 FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY

    Office of Legacy Management (LM)

    AND THE U.S. ATOMIC ENERGY COMMISSION FALLON, NEVADA OCTOBER 26, 1963 Project 9.1 U.s. ... The major constituents, as determined by X-ray tests and thin-section examination, were ...

  3. NNSA Commemorates 50th Anniversary of First Vela Launch | National...

    National Nuclear Security Administration (NNSA)

    significant scientific data. Examples include the first measurements that lead to the discovery of naturally occurring gamma ray bursts, data on trapped radiation within ...

  4. FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY THE ADVANCED RESEARCH...

    Office of Legacy Management (LM)

    ... U S A r m y Raymond Moore, MD Donald Smith, DVM USPHS, Medical Officer USPHS, V e t e ... Ranch 2 1 Schur z 0709 - - - 2 1 3 4 2 Seyler R e s e r v o i r 1 1 Smith C r e e k Ranch ...

  5. Bio Sciences: Ryan Agh Haide Vela-Alvarez Chemistry: Morgan Kelley

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

    Winners Morgan Kelley Belinda Pacheco Threat Identification and Response Science and Engineering Andrew Hollis Babatunde Adigun Jordan Fonseca Christopher McGahee Logan Ott

  6. Cle Elum Lake Anadromous Salmon Restoration Feasibility Study: Summary of Research, 1986-1999 Progress Report.

    SciTech Connect (OSTI)

    Dey, Douglas

    2000-04-01

    The focus of this research was to study the feasibility for anadromous salmonids to recolonize the habitat above reservoirs in the Yakima River without disruption to irrigation withdrawals. A primary concern was whether anadromous fish could successfully exit reservoirs and survive downstream passage through the Yakima and Columbia Rivers to the ocean.

  7. p

    Gasoline and Diesel Fuel Update (EIA)

    ... Armstrong Hutchinson Childress Dallam Collingsworth Hartley Harmon Oldham Cotton Canadian Deaf Smith Kingfisher Grant Hardeman Hale Floyd Lamb Motley Cottle Wilbarger Grady ...

  8. SciTech Connect:

    Office of Scientific and Technical Information (OSTI)

    Grady, Nathaniel" Name Name ORCID Search Authors Type: All BookMonograph ConferenceEvent Journal Article Miscellaneous Patent Program Document Software Manual Technical Report...

  9. EIS-0169-SA-02: Supplement Analysis

    Broader source: Energy.gov [DOE]

    Yakima Fisheries Project-Natural Spawning Channels, Increased On-site Housing, and Upgrades to the Prosser Hatchery. Cle Elum Supplementation and Research Facility, Cle Elum, Washington

  10. EIS-1069-SA-07: Supplement Analysis

    Broader source: Energy.gov [DOE]

    Yakima/Kilickitat Fisheries Project, Noxious Weed Control at Cle Elum and Jack Creek, Cle Elum Supplementation and Research Facility and Jack Creek Acclimation Site, Kittitas County, Washington

  11. EIS-0169-SA-08: Supplement Analysis

    Broader source: Energy.gov [DOE]

    Yakima/Klickitat Fisheries Project, Boone Pond Acclimation Site, Cle Elum, Kittitas County, Washington

  12. Manipulation of Electromagnetic Fields with Plasmonic Nanostructures...

    Office of Scientific and Technical Information (OSTI)

    A paper copy of this document is also available for sale to the public from the National Technical Information Service, Springfield, VA at www.ntis.gov. Authors: Grady, Nathaniel ...

  13. Energy Efficiency in New Mexico Frees Money in Local Coffers...

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

    By saving energy, municipalities can save money on their energy bills - money which can then be used for other public services. Grady, New Mexico, population 98, received 431,908 ...

  14. Nanostructured Organometal Halide Perovskites | The Ames Laboratory

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

    them in the construction of new porous and nanostructured solar cell architectures. Research area: Materials Sciences Program mentor: Javier Vela, Assistant Professor of Chemistry...

  15. VFP Research Projects | The Ames Laboratory

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

    into the cell (Marit Nilsen-Hamilton) Nanostructured Organometal Halide Perovskites (Javier Vela) Nanocasting for a new generation of smart nanodevices (Igor Slowing) Exploration...

  16. Near-Unity Quantum Yields of Biexciton Emission from CdSe=CdS...

    Office of Scientific and Technical Information (OSTI)

    Authors: Park, Young-Shin 1 ; Malko, Anton V. 2 ; Vela, Javier 1 ; Chen, Yongfen 1 ; Ghosh, Yagnaseni 1 ; Garcia-Santamaria, Florencio 1 ; Hollingsworth, Jennifer A. ...

  17. Past VFP research projects | The Ames Laboratory

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

    Past VFP research projects Nanostructured Organometal Halide Perovskites (Javier Vela) Nanocasting for a new generation of smart nanodevices (Igor Slowing) Exploration of ...

  18. European Wind Atlas: France | Open Energy Information

    Open Energy Info (EERE)

    URI: cleanenergysolutions.orgcontenteuropean-wind-atlas-france,http:cle Language: English Policies: Deployment Programs DeploymentPrograms: Technical Assistance This...

  19. A golden anniversary for space-based treaty verification

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

    A golden anniversary for space-based treaty verification A golden anniversary for space-based treaty verification Fifty years ago this month, LANL sensor technology lifted off into space to help verify that world Superpowers were abiding by the newly signed Limited Test Ban Treaty. October 22, 2013 Los Alamos National Laboratory researcher Richard Belian performs a final check of the Vela V-B satellite prior to its launch in April 1970. Vela V-B was the last of the Vela twin satellites launched

  20. All-Star Nanocrystals | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    ... Publications F. Zhu, L. Men, Y. Guo, Q. Zhu, U. Bhattacharjee, P.M. Goodwin, J.W. Petrich, E.A. Smith, J. Vela, "Shape evolution and single particle luminescence of organometal ...

  1. Department

    Office of Legacy Management (LM)

    ... was estimated for each reflector using a straight-ray reflection path approximation. ... County, Nevada: U.S. Atomic Energy Commission, Vela Uniform Rep011, v. 1001,369 p. ...

  2. PSA_Well_Completion_Report.book

    Office of Legacy Management (LM)

    ... B.1-4 Geophysical Data Project Shoal Area MV-3 Spontaneous Potential and Gamma Ray . . . . ... The Vela Uniform Program was a joint effort conducted by the U.S. Atomic Energy Commission ...

  3. 1997 Annual Facility Representative Workshop Attendees

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

    (925) 423-7567 henry.rio@oak.doe.gov Rose Grady AL AAO (505) 477-3162 grose@pantex.com Ross Bill AL AAO (806) 477-7239 wross@pantex.com Seaborg Don RL PFP (509) 372-2889 ...

  4. Slide 1

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

    ... Totalview, DDT) PGIGNUIntel Compilers GNUIntel Compilers Cray Linux Environment MOABLSFPBS Pro ALPS LustreDVSNFS CLE SuSE components Intel Processors Components Gemini ...

  5. EIS-0169-SA-05: Supplement Analysis | Department of Energy

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

    to include a hatchery control line, maintained entirely by spawning hatchery-origin fish. DOEEIS-0169-SA-05, Supplement Analysis for YakimaKlickitat Fisheries Project, Cle...

  6. Compute Nodes

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

    low-overhead operating system optimized for high performance computing called "Cray Linux Environment" (CLE). This OS supports only a limited number of system calls and UNIX...

  7. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    ... If the C-cost for ecosystem management is taken into ... the effects of climate change. less January 2012 ... The first (CLE) scenario reflects implementation of current ...

  8. Supplement Analyses (SA) | Department of Energy

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

    Accelerators September 2, 2002 EIS-0169-SA-05: Supplement Analysis YakimaKlickitat Fisheries Project, Cle Elum, Kittitas County, Washington September 2, 2002...

  9. Hawaii Department of Health Clean Air Branch Webpage | Open Energy...

    Open Energy Info (EERE)

    Branch Webpage Internet. cited 20141013. Available from: http:health.hawaii.govcab Retrieved from "http:en.openei.orgwindex.php?titleHawaiiDepartmentofHealthCle...

  10. Links

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

    Links: CAMD's SAXS beamline sister page By Derek Dorman General Reference: Glatter and Kratky Small Angle X-ray Scattering Book (subject to the permission letter and terms of use) SAXS Presentation by Jianhua Li SAXS Presentation by John Pople Dr. Brian Grady's Polymer Characterization Group SAXS page Jun, Y., Waychunas, G. "Molecular-Level Investigations of Nucleation Mechanisms and Kinetics of Formation of Environmental Nanoparticles" Poster SAXS Analysis/Simulation: Paul Scherrer

  11. Contacts for the Office of Administrative Operations | Department of Energy

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

    Administrative Operations Contacts for the Office of Administrative Operations John D. (Dan) Bullington, Director of Administrative Operations 202-586-7364 dan.bullington@hq.doe.gov Valerie Mills, Management and Program Analysis Officer 202-586-8533 Valerie.mills@hq.doe.gov Claude Barnes, Management Analyst 202-586-2957 Dorothy Cofield, Computer Technician 202-586-9525 Robert Grady, Computer Technician 202-586-9525 Diane Himes, Administrative Officer 202-586-2941 Laura Ryan, Clerk 202-586-1634

  12. Los Alamos honors computer code team with Feynman Innovation Prize

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

    Team honored with Feynman Innovation Prize Los Alamos honors computer code team with Feynman Innovation Prize This year's honorees for the Richard P. Feynman Innovation Prize at Los Alamos National Laboratory are the Monte Carlo Radiation Transport Team members. July 22, 2015 Winners of the 2015 Richard P. Feynman Innovation Prize at Los Alamos National Laboratory, from left, are Larry J. Cox, Forrest B. Brown, Avneet Sood, Gregg W. McKinney, Jeffrey S. Bull and H. Grady Hughes. Also on the

  13. Response of High-Tc Superconductor Metamaterials to High Intensity THz

    Office of Scientific and Technical Information (OSTI)

    Radiation (Conference) | SciTech Connect Response of High-Tc Superconductor Metamaterials to High Intensity THz Radiation Citation Details In-Document Search Title: Response of High-Tc Superconductor Metamaterials to High Intensity THz Radiation Authors: Grady, Nathaniel [1] ; Perkins Jr., Bradford G. [2] ; Hwang, Harold Y. [2] ; Brandt, Nate [2] ; Torchinsky, Darius [2] ; Singh, Ranjan [1] ; Yan, Li [3] ; Jia, Quanxi [1] ; Trugman, Stuart A. [1] ; Taylor, Antoinette J. [1] ; Nelson, Keith

  14. CX-006312: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Small-Scale Spring Chinook and Coho ReintroductionCX(s) Applied: B1.20Date: 07/21/2011Location(s): Cle Elum, WashingtonOffice(s): Bonneville Power Administration

  15. Category:Cleveland, OH | Open Energy Information

    Open Energy Info (EERE)

    Cle... 69 KB SVOutPatient Cleveland OH Ohio Power Co.png SVOutPatient Cleveland... 68 KB SVPrimarySchool Cleveland OH Ohio Power Co.png SVPrimarySchool Clevel... 68 KB...

  16. BPA offering grants in science and energy education

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

    offering grants in science and energy education 462015 12:00 AM Tweet Page Content Students from East Valley Central School in Yakima, Washington took a field trip to the Cle...

  17. January 2013 Most Viewed Documents for National Defense | OSTI, US Dept of

    Office of Scientific and Technical Information (OSTI)

    Energy Office of Scientific and Technical Information January 2013 Most Viewed Documents for National Defense Dynamic equation of state and strength properties of unreacted PBXW-128 explosive Chhabildas, L.C.; Grady, D.E.; Reinhart, W.D.; Wilson, L.T. From separations to reconstitution - a short history of Plutonium in the U.S. and Russia Gray, L W Condensation induced water hammer safety Gintner, M.A. Direct calibration of the yield of nuclear explosion Nakanishi, K.; Nikolayev, A. [SYNAPSE

  18. Shoal, Nevada Site Fact Sheet

    SciTech Connect (OSTI)

    2009-04-01

    The Shoal Site is situated on 2,560 acres of withdrawn federal lands located within the north-central portion of the Sand Springs Range in Churchill County, Nevada. The town of Fallon is the largest populated area in the region and is about 30 miles northwest of the site. The region around the Shoal Site is sparsely populated; military installations, recreation, ranching, and mining provide the dominant commercial interests. The Project Shoal underground nuclear test was part of the Vela Uniform program sponsored jointly by the U.S Department of Defense and U.S. Atomic Energy Commission (AEC), a predecessor agency of the U.S. Department of Energy (DOE). Vela Uniform was a research and development program directed toward locating, detecting, and identifying underground detonations. The objective of Project Shoal was to detonate a nuclear device underground in an active seismic area to improve the United States' ability to detect, identify, and locate underground nuclear detonations.

  19. Chemical Analysis of Nanodomains | The Ames Laboratory

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

    Analysis of Nanodomains FWP/Project Description: Project Leader(s): Emily Smith Principal Investigators: Jacob Petrich, Emily Smith, Javier Vela We seek to understand the basic principles that underlie energy-relevant chemical separations; develop analytical methods to improve the sensitivity, reliability, and productivity of analytical determinations; and to develop new approaches to analysis. Our research emphasizes instrumentation and technique development highly relevant to the main focus

  20. AVRAM user's manual

    SciTech Connect (OSTI)

    McGrady, P.W.

    1988-02-01

    This document details the use of the reliability code for the Atomic Vapor Laser Isotope Separation (AVLIS) project. This code was designed by Tom Anklam and John Harris. In late 1984 Patrick McGrady and Elena Koontz of C and TD/TA were assigned the task of improving the code and converting it for use on the DEC-10 system. In early 1986, Patric McGrady converted it to the CRAY. The AVRAM code is divided into distinct parts (often referred to as programs in this document). There is a COSMOS file that controls the execution of the FORTRAN code and controls the naming of output datasets and the deletion of temporary datasets created by the code. The FORTRAN code consists of a main program as a driver and of three main subroutines: EDIT, PARAM, and AVRAM. The EDIT program allows the user to create a new user defined system or add to an existing system or to change certain parameters. The PARAM program allows the user to alter system parameters and to select options such as economics run, criticality analysis or sensitivity studies. The AVRAM program does a reliability analysis of the system.

  1. X:\ARM_19~1\P397-400.WPD

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

    P( ) N x P lay ( ) (1 N) x P cle ( ) " " P cle P lay , , S S A s , P St ( ), P Cu ( ) 80 , Session Papers 397 (1) Absorption of Solar Radiation in Broken Clouds V. E. Zuev, G. A. Titov, and T. B. Zhuravleva Institute of Atmospheric Optics Russian Academy of Sciences Tomsk, Russia Introduction It is recognized now that the plane-parallel model unsatisfactorily describes the transfer of radiation through broken clouds and that, consequently, the radiation codes of general circulation

  2. James M. Craw, Nicholas P. Cardo, Yun (Helen) He Lawrence Berkeley National Laboratory

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

    Post-Mortem of the NERSC Franklin XT Upgrade to CLE 2.1 James M. Craw, Nicholas P. Cardo, Yun (Helen) He Lawrence Berkeley National Laboratory Berkeley, CA craw@nersc.gov, cardo@nersc.gov, yhe@lbl.gov And Janet M. Lebens Cray, Inc. jml@cray.com May 4, 2009 Atlanta CUG This presentation will discuss the lessons learned of the events leading up to the production deployment of CLE 2.1 and the post install issues experienced in upgrading NERSC's XT4(tm) system called Franklin CUG 2008 page 2

  3. H

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

    Innova've u se o f H igh P erformance C ompu'ng through t he M odeling o f P ar'cle A ... J.---L. V ay, I . H aber & B . B . Godfrey, J. Comput. P hys. 2 43, 260---268 (2013) ...

  4. An efficient method for unfolding kinetic pressure driven VISAR data

    SciTech Connect (OSTI)

    Mark Harry Hess; Peterson, Kyle; Harvey-Thompson, Adam James

    2015-08-18

    Velocity Interferometer System for Any Reflector (VISAR) [Barker and Hollenbach, J. Appl. Phys. 43, 4669 (1972)] is a well-known diagnostic that is employed on many shock physics and pulsed-power experiments. With the VISAR diagnostic, the velocity on the surface of any metal flyer can be found. For most experiments employing VISAR, either a kinetic pressure [Grady, Mech. Mater. 29, 181 (1998)] or a magnetic pressure [Lemke et al., Intl J. Impact Eng. 38, 480 (2011)] drives the motion of the flyer. Moreover, reliable prediction of the time-dependent pressure is often a critical component to understanding the physics of these experiments. Although VISAR can provide a precise measurement of a flyer’s surface velocity, the real challenge of this diagnostic implementation is using this velocity to unfold the time-dependent pressure. The purpose of this study is to elucidate a new method for quickly and reliably unfolding VISAR data.

  5. Rear surface spallation on single-crystal silicon in nanosecond laser micromachining

    SciTech Connect (OSTI)

    Ren, Jun; Orlov, Sergei S.; Hesselink, Lambertus

    2005-05-15

    Rear surface spallation of single-crystal silicon under 5-ns laser pulse ablation at intensities of 0.6-60 GW/cm{sup 2} is studied through postablation examination of the ablated samples. The spallation threshold energy and the spallation depth's dependences on the energy and target thickness are measured. From the linear relation between the spallation threshold energy and the target thickness, an estimation of the material spall strength around 1.4 GPa is obtained, in reasonable agreement with the spall strength estimation of 0.8-1.2 GPa at a strain rate of 10{sup 7} s{sup -1} using Grady's model for brittle materials. The experiment reveals the internal fracturing process over an extended zone in silicon, which is controlled by the competition between the shock pressure load and the laser ablation rate. The qualities of the laser microstructuring and micromachining results are greatly improved by using an acoustic impedance matching approach.

  6. Towards assessing the violence of reaction during cookoff of confined energetic materials

    SciTech Connect (OSTI)

    Baer, M.R.; Kipp, M.E.; Schmitt, R.G.; Hobbs, M.L.

    1996-11-01

    An analysis of post-ignition events in a variable confinement cookoff test (VCCT) geometry is presented aimed toward predicting the level of violence during cookoff of confined thermally-degraded energetic materials. This study focuses on the dynamic events following thermal initiation whereby accelerated combustion interacts with confinement. Numerical simulations, based on a model of reactive multiphase mixtures, indicate that the response of energetic material is highly dependent upon thermal/mechanical damage states prior to ignition. These damaged states affect the rate of pressurization, dynamic compaction behavior and subsequent growth to detonation. Variations of the specific surface area and porosity produced by decomposition of the energetic material causes different responses ranging from pressure burst to detonation. Calculated stress histories are used in estimating breakup of the VCCT confinement based on Grady-Kipp fragmentation theory.

  7. Fifty-one years of Los Alamos Spacecraft

    SciTech Connect (OSTI)

    Fenimore, Edward E.

    2014-09-04

    From 1963 to 2014, the Los Alamos National Laboratory was involved in at least 233 spacecraft. There are probably only one or two institutions in the world that have been involved in so many spacecraft. Los Alamos space exploration started with the Vela satellites for nuclear test detection, but soon expanded to ionospheric research (mostly barium releases), radioisotope thermoelectric generators, solar physics, solar wind, magnetospheres, astrophysics, national security, planetary physics, earth resources, radio propagation in the ionosphere, and cubesats. Here, we present a list of the spacecraft, their purpose, and their launch dates for use during RocketFest

  8. Physically consistent simulation of mesoscale chemical kinetics: The non-negative FIS-{alpha} method

    SciTech Connect (OSTI)

    Dana, Saswati, E-mail: saswatid@rishi.serc.iisc.ernet.in [Supercomputer Education and Research Centre, Indian Institute of Science, Bangalore 560012 (India); Raha, Soumyendu, E-mail: raha@serc.iisc.ernet.in [Supercomputer Education and Research Centre, Indian Institute of Science, Bangalore 560012 (India)

    2011-10-01

    Biochemical pathways involving chemical kinetics in medium concentrations (i.e., at mesoscale) of the reacting molecules can be approximated as chemical Langevin equations (CLE) systems. We address the physically consistent non-negative simulation of the CLE sample paths as well as the issue of non-Lipschitz diffusion coefficients when a species approaches depletion and any stiffness due to faster reactions. The non-negative Fully Implicit Stochastic {alpha} (FIS {alpha}) method in which stopped reaction channels due to depleted reactants are deleted until a reactant concentration rises again, for non-negativity preservation and in which a positive definite Jacobian is maintained to deal with possible stiffness, is proposed and analysed. The method is illustrated with the computation of active Protein Kinase C response in the Protein Kinase C pathway.

  9. Holistic Evaluation of Lightweight Operating Systems using the PERCU Method

    SciTech Connect (OSTI)

    Kramer, William T.C.; He, Yun; Carter, Jonathan; Glenski, Joseph; Rippe, Lynn; Cardo, Nicholas

    2008-05-01

    The scale of Leadership Class Systems presents unique challenges to the features and performance of operating system services. This paper reports results of comprehensive evaluations of two Light Weight Operating Systems (LWOS), Cray's Catamount Virtual Node (CVN) and Linux Environment (CLE) operating systems, on the exact same large-scale hardware. The evaluation was carried out over a 5-month period on NERSC's 19,480 core Cray XT-4, Franklin, using a comprehensive evaluation method that spans Performance, Effectiveness, Reliability, Consistency and Usability criteria for all major subsystems and features. The paper presents the results of the comparison between CVN and CLE, evaluates their relative strengths, and reports observations regarding the world's largest Cray XT-4 as well.

  10. Sensitivity improvement of Cerenkov luminescence endoscope with terbium doped Gd{sub 2}O{sub 2}S nanoparticles

    SciTech Connect (OSTI)

    Cao, Xin; Chen, Xueli E-mail: jimleung@mail.xidian.edu.cn; Cao, Xu; Zhan, Yonghua; Liang, Jimin E-mail: jimleung@mail.xidian.edu.cn; Kang, Fei; Wang, Jing; Wu, Kaichun

    2015-05-25

    Our previous study showed a great attenuation for the Cerenkov luminescence endoscope (CLE), resulting in relatively low detection sensitivity of radiotracers. Here, a kind of radioluminescence nanoparticles (RLNPs), terbium doped Gd{sub 2}O{sub 2}S was mixed with the radionuclide {sup 68}Ga to enhance the intensity of emitted luminescence, which finally improved the detection sensitivity of the CLE by using the radioluminescence imaging technique. With the in vitro and in vivo pseudotumor experiments, we showed that the use of RLNPs mixed with the radionuclide {sup 68}Ga enabled superior sensitivity compared with the radionuclide {sup 68}Ga only, with 50-fold improvement on detection sensitivity, which guaranteed meeting the demands of the clinical diagnosis of gastrointestinal tract tumors.

  11. Slide 1

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

    Dana Bryson River Corridor Division Director and DDFO to the Hanford Advisory Board S a fe a n d E ff e c ti v e C le a n u p th a t P ro te c ts th e C o lu m b ia R iv e r  Re du ce s the Ac tiv e Sit e Fo otp rin t of Cle an up to 75 Sq ua re Mi les (58 6 to 75 )  Sig nif ica ntl y Re du ce s Lo ng -Te rm Mo rtg ag e Co sts  At Co mp let ion , Sh ifts Em ph as is an d Re so urc es to Fu ll Sc ale Cle an up of the Ce ntr al Pla tea u (75 sq ua re mi les )  Re du ce s Co sts by

  12. Slide 1

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

    Jonathan A. Dowell DOE-RL Assistant Manager for River and Plateau S a fe a n d E ff e c ti v e C le a n u p th a t P ro te c ts th e C o lu m b ia R iv e r  Re du ce s the Ac tiv e Sit e Fo otp rin t of Cle an up to 75 Sq ua re Mi les (58 6 to 75 )  Sig nif ica ntl y Re du ce s Lo ng -Te rm Mo rtg ag e Co sts  At Co mp let ion , Sh ifts Em ph as is an d Re so urc es to Fu ll Sc ale Cle an up of the Ce ntr al Pla tea u (75 sq ua re mi les )  Re du ce s Co sts by "R igh t Siz ing

  13. Goals:

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

    CUG 2009 Proceedings 1 of 8 User and Performance Impacts from Franklin Upgrades Yun (Helen) He National Energy Research Supercomputing Center Lawrence Berkeley National Laboratory Berkeley, CA 94720 ABSTRACT: The NERSC flagship computer Cray XT4 system "Franklin" has gone through three major upgrades: quad core upgrade, CLE 2.1 upgrade, and IO upgrade, during the past year. In this paper, we will discuss the various aspects of the user impacts such as user access, user environment, and

  14. User and Performance Impacts from Franklin Upgrades

    SciTech Connect (OSTI)

    He, Yun

    2009-05-10

    The NERSC flagship computer Cray XT4 system"Franklin" has gone through three major upgrades: quad core upgrade, CLE 2.1 upgrade, and IO upgrade, during the past year. In this paper, we will discuss the various aspects of the user impacts such as user access, user environment, and user issues etc from these upgrades. The performance impacts on the kernel benchmarks and selected application benchmarks will also be presented.

  15. PowerPoint Presentation

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

    and Performance Impacts from Franklin Upgrades Yun (Helen) He National Energy Research Supercomputing Center Cray User Group Meeting May 4-7, 2009 1 Outline * Franklin Introduction * Benchmarks * Quad Core Upgrade * CLE 2.1 Upgrade * IO Upgrade * Summary 2 Franklin's Role at NERSC * NERSC is the US DOE's keystone high performance computing center. * Franklin is the "flagship" system at NERSC serving ~3,100 scientific users in different application disciplines. * Serves the needs for

  16. Search for Pulsed TeV Gamma-Ray Emission from Young Pulsars with H.E.S.S

    SciTech Connect (OSTI)

    Schmidt, P.; Breitling, F.; Lohse, T.; Schlenker, S.; Schwanke, U.; Stegmann, C.; Gillessen, S.; Konopelko, A.

    2005-02-21

    The H.E.S.S. experiment is a next-generation imaging atmospheric Cherenkov detector with a {approx}1% Crab flux sensitivity for gamma-rays above 100 GeV. The full 4-telescope array has been operational since December 2003. The three young pulsars, Crab, Vela, and PSR B1706-44, are among the six pulsars whose pulsed emission has been detected up to energies of several GeV by EGRET. These pulsars have been selected for H.E.S.S. observations on grounds of their high rank in apparent spin-down luminosity Esd/d2 and observability for the H.E.S.S. array. No pulsed emission was found and flux upper limits are given.

  17. An efficient method for unfolding kinetic pressure driven VISAR data

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

    Mark Harry Hess; Peterson, Kyle; Harvey-Thompson, Adam James

    2015-08-18

    Velocity Interferometer System for Any Reflector (VISAR) [Barker and Hollenbach, J. Appl. Phys. 43, 4669 (1972)] is a well-known diagnostic that is employed on many shock physics and pulsed-power experiments. With the VISAR diagnostic, the velocity on the surface of any metal flyer can be found. For most experiments employing VISAR, either a kinetic pressure [Grady, Mech. Mater. 29, 181 (1998)] or a magnetic pressure [Lemke et al., Intl J. Impact Eng. 38, 480 (2011)] drives the motion of the flyer. Moreover, reliable prediction of the time-dependent pressure is often a critical component to understanding the physics of these experiments.more » Although VISAR can provide a precise measurement of a flyer’s surface velocity, the real challenge of this diagnostic implementation is using this velocity to unfold the time-dependent pressure. The purpose of this study is to elucidate a new method for quickly and reliably unfolding VISAR data.« less

  18. NERSC Data Efforts Update

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

    Data Efforts Update --- 1 --- Prabhat Data and Analytics Group Lead February 23, 2015 A little bit about myself * Computer S cien.st - Brown, I IT D elhi * Real---3me G raphics, V irtual R eality, H CI - Computa3onal R esearch D ivision * Scien3fic V isualiza3on, H PC * Data M anagement, P arallel I /O * Sta3s3cs, M achine L earning, B ig D ata * Climate S cien.st - Pursuing P hD i n U C B erkeley w / B ill C ollins * Broadly i nterested i n: - Physics ( Par3cle P hysics, A stronomy) - Chemistry

  19. Geddes_ LPAv3.pptx

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

    P lasma A ccelerator S imula0on U sing L aser a nd Par0cle B eam D rivers C.G.R. G eddes, L BNL F.S. T sung, U CLA 27 November 2012 Office of Science Office of Science SciDAC-2&3 Compass Approach: plasma wave accelerator structure, laser & particle beam evolution excited by laser or particle beam ! λ p ~100µm at 10 17 /cc Laser or beam Trapped particles L plasma ~ mm-m Approach: plasma wave accelerator structure, laser & particle beam evolution excited by laser or particle beam !

  20. Tracking tumor boundary in MV-EPID images without implanted markers: A feasibility study

    SciTech Connect (OSTI)

    Zhang, Xiaoyong Homma, Noriyasu; Ichiji, Kei; Takai, Yoshihiro; Yoshizawa, Makoto

    2015-05-15

    Purpose: To develop a markerless tracking algorithm to track the tumor boundary in megavoltage (MV)-electronic portal imaging device (EPID) images for image-guided radiation therapy. Methods: A level set method (LSM)-based algorithm is developed to track tumor boundary in EPID image sequences. Given an EPID image sequence, an initial curve is manually specified in the first frame. Driven by a region-scalable energy fitting function, the initial curve automatically evolves toward the tumor boundary and stops on the desired boundary while the energy function reaches its minimum. For the subsequent frames, the tracking algorithm updates the initial curve by using the tracking result in the previous frame and reuses the LSM to detect the tumor boundary in the subsequent frame so that the tracking processing can be continued without user intervention. The tracking algorithm is tested on three image datasets, including a 4-D phantom EPID image sequence, four digitally deformable phantom image sequences with different noise levels, and four clinical EPID image sequences acquired in lung cancer treatment. The tracking accuracy is evaluated based on two metrics: centroid localization error (CLE) and volume overlap index (VOI) between the tracking result and the ground truth. Results: For the 4-D phantom image sequence, the CLE is 0.23 ± 0.20 mm, and VOI is 95.6% ± 0.2%. For the digital phantom image sequences, the total CLE and VOI are 0.11 ± 0.08 mm and 96.7% ± 0.7%, respectively. In addition, for the clinical EPID image sequences, the proposed algorithm achieves 0.32 ± 0.77 mm in the CLE and 72.1% ± 5.5% in the VOI. These results demonstrate the effectiveness of the authors’ proposed method both in tumor localization and boundary tracking in EPID images. In addition, compared with two existing tracking algorithms, the proposed method achieves a higher accuracy in tumor localization. Conclusions: In this paper, the authors presented a feasibility study of tracking tumor

  1. Open Issues

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

    March 2011 Resolved: some OpenMP flags ignored in PGI C/C++ compiler March 29, 2011 by Helen He Description: OpenMP flags other than -mp=nonuma are ignored with the PGI C and C++ wrapper on Hopper. The PGI Fortran wrapper behaves correctly. Read the full post "gni_pub.h" not found in compilation March 29, 2011 by Helen He Description: After the OS upgrade to CLE3.1UP03, codes using "gni_pub.h" are getting the "gni_pub.h not found" error at compile time. The

  2. Open Issues

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

    June 2015 runtime error message: "readControlMsg: System returned error Connection timed out on TCP socket fd" June 30, 2015 Symptom User jobs with sinlge or multiple apruns in a batch script may get this run time error: "readControlMsg: System returned error Connection timed out on TCP socket fd". This problem is intermittent, sometimes resubmit works. This error message started to appear after the Hopper OS upgrade to CLE52UP02 on March 11, 2015.

  3. Aprun MAN Page

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

    aprun » Aprun MAN Page Aprun MAN Page aprun [-a arch ] [-b ] [-B] [-cc cpu_list | keyword ] [-cp cpu_placement_file_name ] [-d depth ] [-D value ] [-L node_list ] [-m size[h|hs] ] [-n pes ] [-N pes_per_node ][-F access mode ] [-q ] [-r cores][-S pes_per_numa_node ] [-sl list_of_numa_nodes ] [-sn numa_nodes_per_node ] [-ss ] [-T ] [-t sec ] executable [ arguments_for_executable ] IMPLEMENTATION Cray Linux Environment (CLE) DESCRIPTION To run an application on CNL compute nodes, use the

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

    CC [-c] [-C] [-D macro[=def]] [-E] [-g] [-G level] [-h arg] [-I incldir] [-K trap=opt[,opt]...] [-l libfile] [-L ldir] [-M] [-nostdinc] [-o outfile] [-O level] [-P] [-S] [-U macro] [-V] [-W phase,"opt..."] [-X npes] [-Y phase,dirname] [-#] [-##] [-###] files ... IMPLEMENTATION Cray Linux Environment (CLE) DESCRIPTION The CC command invokes the Cray C++ compiler. The compiler conforms to the ISO/IEC 14882:2003 standard, with some exceptions. The exceptions are noted in the Cray C and

  5. Open Issues

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

    Open Issues Open Issues runtime error message: "readControlMsg: System returned error Connection timed out on TCP socket fd" June 30, 2015 Symptom User jobs with sinlge or multiple apruns in a batch script may get this run time error: "readControlMsg: System returned error Connection timed out on TCP socket fd". This problem is intermittent, sometimes resubmit works. This error message started to appear after the Hopper OS upgrade to CLE52UP02 on March 11, 2015. Read the full

  6. Untitled

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

    Professor R. S. Markiewicz Northeastern University, Boston Excitonic Insulators in Correlated Materials Thursday, May 19, 2016 2:00 - 3:00 pm Wijiji Conference Room - MPA-CINT (TA-03 - Bldg 1420 - Room 2101) Abstract: Shining light on a semiconductor can create excitons - bound states of electron-hole pairs, which lower the single par9cle gap E G by the excitonic binding energy E X . Four years a@er BCS theory, MoD showed that as E G is decreased, there can be an instability when E G <E X,

  7. Scientific Achievement

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

    Discovered the reactive Leidenfrost' effect in cellulose & transition temperature (750 °C). Structured materials with engineered macropores (e.g. catalysts) allow for its tunable control. Controlling Biomass Leidenfrost Liftoff and Heat Transfer Work w as p erformed a t t he U niversity o f M innesota b y t he g roup o f Dauenhauer Research Details --- Cellulose par=cles levitate above 750 o C from generated v apor fl ow --- Onset o f p ar=cle l evita=on d rama=cally l owers heat t ransfer

  8. I

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

    jects the remainder of the fuel early in the cy- cle during the compression stroke. This pro- vides equivalence ratio stratification in the combustion chamber and it is thought that by varying the level of stratification, the combus- tion process can be controlled. Dual-fuel RCCI is similar in that it premixes a high oc- tane number fuel like gasoline, but the direct injected fuel has a low octane number, like diesel fuel, which is direct injected during the compression stroke. Thus, in addition

  9. QBR1024-07-30-ZZ.pptx

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

    ! ! NERSC ! Cray QBR Meeting! July 30, 2014, Oakland, CA Quality and testing of PE release NERSC PE bugs opened in last three months (4/24/2014 - 7/29/2014) --- 2 --- ID Type Product Component Severity Resolution Summary Created Changed 815222 BUG Perftools Other major Vtune8installation8issues 7/29/14812:12 7/29/14812:13 815130 BUG PE8libs hdf5 major crayFhdf5Fparallel8gives8bad8result8for8integers8for8version81.8.13 7/25/14815:31 7/25/14817:39 814838 BUG CLE IAA major FIXED

  10. 2014 Well Completion Report for Corrective Action Unit 447 Project Shoal Area Churchill County, Nevada October 2015

    SciTech Connect (OSTI)

    Findlay, Rick

    2015-11-01

    This report summarizes the drilling program conducted by the U.S. Department of Energy (DOE) Office of Legacy Management at the Project Shoal Area (Shoal) Subsurface Corrective Action Unit 447 in Churchill County, Nevada. Shoal was the location of an underground nuclear test conducted on October 26, 1963, as part of the Vela Uniform program sponsored jointly by the U.S. Department of Defense and the U.S. Atomic Energy Commission (a predecessor to DOE). The test consisted of detonating a 12-kiloton nuclear device in granitic rock at a depth of approximately 1,211 feet (ft) below ground surface (bgs) (AEC 1964). The corrective action strategy for the site is focused on revising the site conceptual model and evaluating the adequacy of the monitoring well network at the site. Field activities associated with the project were conducted in accordance with the Federal Facility Agreement and Consent Order (FFACO 1996, as amended) and applicable Nevada Division of Environmental Protection (NDEP) policies and regulations.

  11. Spatially resolving the very high energy emission from MGRO J2019+37 with VERITAS

    SciTech Connect (OSTI)

    Aliu, E.; Errando, M. [Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States); Aune, T. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Behera, B.; Chen, X.; Federici, S. [DESY, Platanenallee 6, D-15738 Zeuthen (Germany); Beilicke, M.; Buckley, J. H.; Bugaev, V. [Department of Physics, Washington University, St. Louis, MO 63130 (United States); Benbow, W.; Cerruti, M. [Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645 (United States); Berger, K. [Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716 (United States); Bird, R. [School of Physics, University College Dublin, Belfield, Dublin 4 (Ireland); Bouvier, A. [Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064 (United States); Ciupik, L. [Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States); Connolly, M. P. [School of Physics, National University of Ireland Galway, University Road, Galway (Ireland); Cui, W. [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Dumm, J. [School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 (United States); Dwarkadas, V. V. [Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States); Falcone, A., E-mail: ealiu@astro.columbia.edu, E-mail: nahee@uchicago.edu [Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802 (United States); and others

    2014-06-10

    We present very high energy (VHE) imaging of MGRO J2019+37 obtained with the VERITAS observatory. The bright extended (?2°) unidentified Milagro source is located toward the rich star formation region Cygnus-X. MGRO J2019+37 is resolved into two VERITAS sources. The faint, point-like source VER J2016+371 overlaps CTB 87, a filled-center remnant (SNR) with no evidence of a supernova remnant shell at the present time. Its spectrum is well fit in the 0.65-10 TeV energy range by a power-law model with photon index 2.3 ± 0.4. VER J2019+378 is a bright extended (?1°) source that likely accounts for the bulk of the Milagro emission and is notably coincident with PSR J2021+3651 and the star formation region Sh 2–104. Its spectrum in the range 1-30 TeV is well fit with a power-law model of photon index 1.75 ± 0.3, among the hardest values measured in the VHE band, comparable to that observed near Vela-X. We explore the unusual spectrum and morphology in the radio and X-ray bands to constrain possible emission mechanisms for this source.

  12. MAGNETIC END CLOSURES FOR PLASMA CONFINING AND HEATING DEVICES

    DOE Patents [OSTI]

    Post, R.F.

    1963-08-20

    More effective magnetic closure field regions for various open-ended containment magnetic fields used in fusion reactor devices are provided by several spaced, coaxially-aligned solenoids utilized to produce a series of nodal field regions of uniform or, preferably, of incrementally increasing intensity separated by lower intensity regions outwardly from the ends of said containment zone. Plasma sources may also be provided to inject plasma into said lower intensity areas to increase plasma density therein. Plasma may then be transported, by plasma diffusion mechanisms provided by the nodal fields, into the containment field. With correlated plasma densities and nodal field spacings approximating the mean free partl cle collision path length in the zones between the nodal fields, optimum closure effectiveness is obtained. (AEC)

  13. LANL: AOT & LANSCE The Pulse April 2011

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

    1 Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 2 From Alex's Desk 3 lANsCe Former stuDeNt seleCteD to AtteND 61st liNDAu Nobel lAureAtes meetiNg iN germANy experimeNts At the NuCleAr sCieNCe leAD slowiNg-DowN speCtrometer 4 NeutroN sCAtteriNg exAmiNes DyNAmiC properties oF biomembrANes 5 NeutroN sChool will FoCus oN the eNviroNmeNt 6 heADsup! meetiNg plANNiNg serviCes

  14. LANL: AOT & LANSCE The Pulse May 2010

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

    0 Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 2 A nAno look At AmmoniA borAne And hydrogen storAge lujAn Center studies struCturAl mAteriAls for nuCleAr AppliCAtions And highly irrAdiAted steels 3 lAnsCe-ns hosts nAtionAl lAborAtories At fission meAsure- ment meeting 4 unrAveling the mysteries of lipid domAins in bio-membrAnes 5 heAds up! James Rhyne selected to be a

  15. LANL: AOT & LANSCE The Pulse November 2010

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

    10 Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 2 From Alex's Desk 3 First beAm tests with the time Projection chAmber 4 Discovery oF new Phys- ics in leAD-zirconium- titAnium voltAge bArs 5 los AlAmos lenDs its exPertise to cleAn energy AnD cArbon sequestrAtion Projects 6 electric-FielD moDiFicA- tion oF mAgnetism in A thin Film 7 Aot & lAnsce Division stAFF AwArDeD

  16. 20140115ColellaASCRNERSC.ppt

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

    Defining R equirements, M ee1ng R equirements Phillip C olella Applied N umerical A lgorithms G roup Computa1onal R esearch D ivision, L BNL NERSC ASCR Requirements for 2017 January 15, 2014 LBNL Research p rojects * Base p rogram r esearch i n n umerical m ethods f or par1al d ifferen1al e qua1ons. * Par1cipa1on S ciDAC F ASTMath I ns1tute a c1vi1es i n structured g rid a nd p ar1cle m ethods. * "Exascale" r esearch: p ar1cipa1on i n ExReDi p roject (RXSolver p rogram) a nd D ---TEC a

  17. Including the temporal change in PM{sub 2.5} concentration in the assessment of human health impact: Illustration with renewable energy scenarios to 2050

    SciTech Connect (OSTI)

    Gschwind, Benoit; Lefevre, Mireille; Blanc, Isabelle; Ranchin, Thierry; Wyrwa, Artur; Drebszok, Kamila; Cofala, Janusz; Fuss, Sabine

    2015-04-15

    This article proposes a new method to assess the health impact of populations exposed to fine particles (PM{sub 2.5}) during their whole lifetime, which is suitable for comparative analysis of energy scenarios. The method takes into account the variation of particle concentrations over time as well as the evolution of population cohorts. Its capabilities are demonstrated for two pathways of European energy system development up to 2050: the Baseline (BL) and the Low Carbon, Maximum Renewable Power (LC-MRP). These pathways were combined with three sets of assumptions about emission control measures: Current Legislation (CLE), Fixed Emission Factors (FEFs), and the Maximum Technically Feasible Reductions (MTFRs). Analysis was carried out for 45 European countries. Average PM{sub 2.5} concentration over Europe in the LC-MRP/CLE scenario is reduced by 58% compared with the BL/FEF case. Health impacts (expressed in days of loss of life expectancy) decrease by 21%. For the LC-MRP/MTFR scenario the average PM{sub 2.5} concentration is reduced by 85% and the health impact by 34%. The methodology was developed within the framework of the EU's FP7 EnerGEO project and was implemented in the Platform of Integrated Assessment (PIA). The Platform enables performing health impact assessments for various energy scenarios. - Highlights: • A new method to assess health impact of PM{sub 2.5} for energy scenarios is proposed. • An algorithm to compute Loss of Life Expectancy attributable to exposure to PM{sub 2.5} is depicted. • Its capabilities are demonstrated for two pathways of European energy system development up to 2050. • Integrating the temporal evolution of PM{sub 2.5} is of great interest for assessing the potential impacts of energy scenarios.

  18. Pair creation above pulsar polar caps: geometrical structure and energetics of slot caps

    SciTech Connect (OSTI)

    Arons, J.

    1983-03-01

    A theory of pair creation over the polar caps of isolated, magnetized, rotating neutron stars with magnetic axis oblique to the rotation is developed, when steady, space charge limited flow occurs within a narrow polar flux tube bounded by regions of high conductivity and negligible flow. A quantitative calculation is given of the structure of the pair formation front which divides the low altitude, charge separated region of strong acceleration from the dense pair plasma flowing outward along the polar flux tube, including the structure and energetics of the slot gap formed between the pair plasma and the closed regions of the magnetosphere. Both the electron emission and the ion emission cases are incorporated in the electrodynamical theory. In short period objects with simple magnetic structure near the star, the particle acceleration power generated is found to be on the order of a few tenths of a percent of the total spin-down energy loss, more than enough to explain all the photon emission from the Crab and Vela pulsars. Most of this energy is generated in the slot gap. In dipole geometry, the energy is concentrated into two or three ''beams'' of accelerated particles with the regions of highest energy density filling only a small fraction of the polar flux tube. In long period objects with complex surface fields, the power generated in particle acceleration is comparable to the total spin-down energy loss rate, and is mostly created in the low altitude gap region between the star and the pair plasma. Some implications of this local particle acceleration theory for the beaming morphology of pulsars' photon emission are discussed, especially the possibility of observationally distinguishing the electron emission and the ion emission cases.

  19. Evaluating operating system vulnerability to memory errors.

    SciTech Connect (OSTI)

    Ferreira, Kurt Brian; Bridges, Patrick G.; Pedretti, Kevin Thomas Tauke; Mueller, Frank; Fiala, David; Brightwell, Ronald Brian

    2012-05-01

    Reliability is of great concern to the scalability of extreme-scale systems. Of particular concern are soft errors in main memory, which are a leading cause of failures on current systems and are predicted to be the leading cause on future systems. While great effort has gone into designing algorithms and applications that can continue to make progress in the presence of these errors without restarting, the most critical software running on a node, the operating system (OS), is currently left relatively unprotected. OS resiliency is of particular importance because, though this software typically represents a small footprint of a compute node's physical memory, recent studies show more memory errors in this region of memory than the remainder of the system. In this paper, we investigate the soft error vulnerability of two operating systems used in current and future high-performance computing systems: Kitten, the lightweight kernel developed at Sandia National Laboratories, and CLE, a high-performance Linux-based operating system developed by Cray. For each of these platforms, we outline major structures and subsystems that are vulnerable to soft errors and describe methods that could be used to reconstruct damaged state. Our results show the Kitten lightweight operating system may be an easier target to harden against memory errors due to its smaller memory footprint, largely deterministic state, and simpler system structure.

  20. Optimal Conventional and Semi-Natural Treatments for the Upper Yakima Spring Chinook Salmon Supplementation Project; Treatment Definitions and Descriptions and Biological Specifications for Facility Design, 1995-1999 Final Report.

    SciTech Connect (OSTI)

    Hager, Robert C.; Costello, Ronald J.

    1999-10-01

    This report describes the Yakima Fisheries Project facilities (Cle Elum Hatchery and acclimation satellites) which provide the mechanism to conduct state-of-the-art research for addressing questions about spring chinook supplementation strategies. The definition, descriptions, and specifications for the Yakima spring chinook supplementation program permit evaluation of alternative fish culture techniques that should yield improved methods and procedures to produce wild-like fish with higher survival that can be used to rebuild depleted spring chinook stocks of the Columbia River Basin. The definition and description of three experimental treatments, Optimal Conventional (OCT), Semi-Natural (SNT), Limited Semi-Natural (LSNT), and the biological specifications for facilities have been completed for the upper Yakima spring chinook salmon stock of the Yakima Fisheries Project. The task was performed by the Biological Specifications Work Group (BSWG) represented by Yakama Indian Nation, Washington Department of Fish and Wildlife, National Marine Fisheries Service, and Bonneville Power Administration. The control and experimental variables of the experimental treatments (OCT, SNT, and LSNT) are described in sufficient detail to assure that the fish culture facilities will be designed and operated as a production scale laboratory to produce and test supplemented upper Yakima spring chinook salmon. Product specifications of the treatment groups are proposed to serve as the generic templates for developing greater specificity for measurements of product attributes. These product specifications will be used to monitor and evaluate treatment effects, with respect to the biological response variables (post release survival, long-term fitness, reproductive success and ecological interactions).

  1. X-RAY OBSERVATIONS OF THE SUPERNOVA REMNANT CTB 87 (G74.9+1.2): AN EVOLVED PULSAR WIND NEBULA

    SciTech Connect (OSTI)

    Matheson, H.; Safi-Harb, S.; Kothes, R. E-mail: samar@physics.umanitoba.ca

    2013-09-01

    Pulsar wind nebulae (PWNe) studies with the Chandra X-Ray Observatory have opened a new window to address the physics of pulsar winds, zoom on their interaction with their hosting supernova remnant (SNR) and interstellar medium, and identify their powering engines. We here present a new 70 ks, plus an archived 18 ks, Chandra ACIS observation of the SNR CTB 87 (G74.9+1.2), classified as a PWN with unusual radio properties and poorly studied in X-rays. We find that the peak of the X-ray emission is clearly offset from the peak of the radio emission by {approx}100'' and located at the southeastern edge of the radio nebula. We detect a point source-the putative pulsar-at the peak of the X-ray emission and study its spectrum separately from the PWN. This new point source, CXOU J201609.2+371110, is surrounded by a compact nebula displaying a torus-like structure and possibly a jet. A more extended diffuse nebula is offset from the radio nebula, extending from the point source to the northwest for {approx}250''. The spectra of the point source, compact nebula, and extended diffuse nebula are all well described by a power-law model with a photon index of 1.1 (0.7-1.6), 1.2 (0.9-1.4), and 1.7 (1.5-1.8), respectively, for a column density N{sub H} = 1.38 (1.21-1.57) Multiplication-Sign 10{sup 22} cm{sup -2} (90% confidence). The total X-ray luminosity of the source is {approx}1.6 Multiplication-Sign 10{sup 34} erg s{sup -1} at an assumed distance of 6.1 kpc, with {approx}2% and 6% contribution from the point source and compact nebula, respectively. The observed properties suggest that CTB 87 is an evolved ({approx}5-28 kyr) PWN, with the extended radio emission likely a ''relic'' PWN, as in Vela-X and G327.1-1.1. To date, however, there is no evidence for thermal X-ray emission from this SNR, and the SNR shell is still missing, suggesting expansion into a low-density medium (n{sub 0} < 0.2 D{sup -1/2}{sub 6.1} cm{sup -3}), likely caused by a stellar wind bubble blown by the

  2. Observation of 23 supernovae that exploded <300 pc from Earth during the past 300 kyr

    SciTech Connect (OSTI)

    Firestone, R. B.

    2014-07-01

    Four supernovae (SNe), exploding ≤300 pc from Earth, were recorded 44, 37, 32, and 22 kyr ago in the radiocarbon ({sup 14}C) record during the past 50 kyr. Each SN left a nearly identical signature in the record, beginning with an initial sudden increase in atmospheric radiocarbon, when the SN exploded, followed by a hiatus of 1500 yr, and concluding with a sustained 2000 yr increase in global radiocarbon due to γ-rays produced by diffusive shock in the SN remnant (SNR). For the past 18 kyr excess radiocarbon has decayed with the {sup 14}C half-life. SN22kyrBP, is identified as the Vela SN that exploded 250 ± 30 pc from Earth. These SN are confirmed in the {sup 10}Be, {sup 26}Al, {sup 36}Cl, and NO{sub 3}{sup −} geologic records. The rate of near-Earth SNe is consistent with the observed rate of historical SNe giving a galactic rate of 14 ± 3 kyr{sup –1} assuming the Chandra Galactic Catalog SNR distribution. The Earth has been used as a calorimeter to determine that ≈2 × 10{sup 49} erg were released as γ-rays at the time of each SN explosion and ≈10{sup 50} erg in γ-rays following each SN. The background rate of {sup 14}C production by cosmic rays has been determined as 1.61 atoms cm{sup –2} s{sup –1}. Approximately 1/3 of the cosmic ray energy produced by diffusive shock in the SNR was observed to be emitted as high-energy γ-rays. Analysis of the {sup 10}Be/{sup 9}Be ratio in marine sediment identified 19 additional near-Earth SNe that exploded 50-300 kyr ago. Comparison of the radiocarbon record with global temperature variations indicated that each SN explosion is correlated with a concurrent global warming of ≈3°C-4°C.

  3. SU-E-I-80: Beta-Minus Emitting Radiotracers Improves Molecular Endoscopy

    SciTech Connect (OSTI)

    Carpenter, C; Ma, X; Sun, C; Pratx, G; Cheng, Z; Xing, L

    2014-06-01

    Purpose: Molecular Endoscopy using Cerenkov Luminescence can be used to monitor the distribution of many clinically-available PET and SPECT probes for endoscopic applications. A main limitation of Cerenkov is its limited sensitivity to small concentrations of radiotracer when using light guides s. Herein we demonstrate that the use of a high energy beta emitting radioisotope, exemplified here with 90Y provides superior sensitivity to 18F because of its higher light output and its lack of corresponding gamma emission. Methods: A series of phantom experiments were performed to compare the sensitivity and noise of the CLE system for imaging 90Y and 18F. Three vials of known concentrations of 90Y (0.008 ?Ci, 0.08 ?Ci, 1 ?Ci) were placed in centrifuge tubes and isolated from each other. One vial of 18F (100 ?Ci) was placed in the imaging chamber and imaged over the course of decay (19 hours, 43 minutes, or ?10 half-lives). Image time-points were formed from 5-minute integrations. Results: Using an SNR of 10 to define the noise-floor, the 90Y minimum detectable activity was 0.056 ?Ci. To the contrast, the minimum detectable activity for 18F was 11.63 ?Ci. These data demonstrate a 207-fold improvement in SNR of 90Y compared to 18F, when controlled for activity. Conclusion: This study demonstrated that a pure ?- radionuclide such as 90Y be used is superior to 18F for Cerenkov Endoscopy. Further study is needed to demonstrate its utility in preclinical studies, endoscopic applications, intraoperative, and radiotherapy applications.

  4. Macrophysical Properties of Tropical Cirrus Clouds from the CALIPSO Satellite and from Ground-based Micropulse and Raman Lidars

    SciTech Connect (OSTI)

    Thorsen, Tyler J.; Fu, Qiang; Comstock, Jennifer M.; Sivaraman, Chitra; Vaughan, Mark A.; Winker, D.; Turner, David D.

    2013-08-27

    Lidar observations of cirrus cloud macrophysical properties over the U.S. Department of Energy Atmospheric Radiation Measurement (ARM) program Darwin, Australia site are compared from the Cloud-Aerosol Lidar and In- frared Pathfinder Satellite Observation (CALIPSO) satellite, the ground-based ARM micropulse lidar (MPL), and the ARM Raman lidar (RL). Comparisons are made using the subset of profiles where the lidar beam is not fully attenuated. Daytime measurements using the RL are shown to be relatively unaffected by the solar background and are therefore suited for checking the validity of diurnal cycles. RL and CALIPSO cloud fraction profiles show good agreement while the MPL detects significantly less cirrus, particularly during the daytime. Both MPL and CALIPSO observations show that cirrus clouds occur less frequently during the day than at night at all altitudes. In contrast, the RL diurnal cy- cle is significantly different than zero only below about 11 km; where it is the opposite sign (i.e. more clouds during the daytime). For cirrus geomet- rical thickness, the MPL and CALIPSO observations agree well and both datasets have signficantly thinner clouds during the daytime than the RL. From the examination of hourly MPL and RL cirrus cloud thickness and through the application of daytime detection limits to all CALIPSO data we find that the decreased MPL and CALIPSO cloud thickness during the daytime is very likely a result of increased daytime noise. This study highlights the vast im- provement the RL provides (compared to the MPL) in the ARM program's ability to observe tropical cirrus clouds as well as a valuable ground-based lidar dataset for the validation of CALIPSO observations and to help im- prove our understanding of tropical cirrus clouds.

  5. Assessment of High Rates of Precocious Male Maturation in a Spring Chinook Salmon Supplementation Hatchery Program, Annual Report 2002-2003.

    SciTech Connect (OSTI)

    Larsen, Donald; Beckman, Brian; Cooper, Kathleen

    2003-08-01

    The Yakima River Spring Chinook Salmon Supplementation Project in Washington State is currently one of the most ambitious efforts to enhance a natural salmon population in the United States. Over the past five years we have conducted research to characterize the developmental physiology of naturally- and hatchery-reared wild progeny spring chinook salmon (Oncorhynchus tshawytscha) in the Yakima River basin. Fish were sampled at the main hatchery in Cle Elum, at remote acclimation sites and, during smolt migration, at downstream dams. Throughout these studies the maturational state of all fish was characterized using combinations of visual and histological analysis of testes, gonadosomatic index (GSI), and measurement of plasma 11-ketotestosterone (11-KT). We established that a plasma 11-KT threshold of 0.8 ng/ml could be used to designate male fish as either immature or precociously maturing approximately 8 months prior to final maturation (1-2 months prior to release as 'smolts'). Our analyses revealed that 37-49% of the hatchery-reared males from this program undergo precocious maturation at 2 years of age and a proportion of these fish appear to residualize in the upper Yakima River basin throughout the summer. An unnaturally high incidence of precocious male maturation may result in loss of potential returning anadromous adults, skewing of female: male sex ratios, ecological, and genetic impacts on wild populations and other native species. Precocious male maturation is significantly influenced by growth rate at specific times of year and future studies will be conducted to alter maturation rates through seasonal growth rate manipulations.

  6. Evaluation of Water Quality Conditions Near Proposed Fish Production Sites Associated with the Yakima Fisheries Project, 1991-1993 Final Report.

    SciTech Connect (OSTI)

    Dauble, Dennis D.

    1994-05-01

    In 1991, the Pacific Northwest Laboratory (PNL) began studying water quality at several sites in the Yakima River Basin for the Bonneville Power Administration. These sites were being proposed as locations for fish culture facilities as part of the Yakima Fisheries Project (YFP). Surface water quality parameters near the proposed fish culture facilities are currently suitable for fish production. Water quality conditions in the mainstream Yakima River and its tributaries are generally excellent in the upper part of the watershed (i.e., near Cle Elum), but they are only fair to poor for the river downstream of Union Gap (river mile 107). Water quality of the Naches River near Oak Flats is also suitable for fish production. Groundwater supplies near the proposed fish production facilities typically have elevated concentrations of metals and dissolved gases. These conditions can be mitigated using best engineering practices such as precipitation and degasification. Additionally, mixing with surface water may improve these conditions. Depending on the location and depth of the well, groundwater temperatures may be warmer than optimum for acclimating and holding juvenile and adult fish. Water quality parameters measured in the Yakima River and tributaries sometimes exceed the range of values described as acceptable for culture of salmonids and for the protection of other aquatic life. However, constituent concentrations are within ranges that exist in many northwest fish hatcheries. Additionally, site-specific tests conducted by PNL (i.e., live box exposures and egg incubation studies) indicate that fish can be successfully reared in surface and well water near the proposed facility sites. Thus, there appear to be no constraints to artificial production for the YFP.

  7. La supraconductivité a 100 ans !

    ScienceCinema (OSTI)

    None

    2011-10-06

    Il y a 100 ans, le 8 avril 1911, une découverte majeure était réalisée : celle de la supraconductivité. La supraconductivité est la caractéristique qu?ont certains métaux et alliages de perdre toute résistance électrique en dessous d?une température donnée. Cette renversante découverte, réalisée de manière presque fortuite par Kammerlingh Onnes de l?Université de Leyde (Pays-Bas) et son étudiant Gilles Holst, a ouvert un nouveau champ de recherche en physique et de fabuleuses perspectives d?applications technologiques. Du point de vue scientifique, la supraconductivité est en effet l?une des rares manifestations de la physique quantique à l?échelle macroscopique.  Du point de vue des retombées techniques, elle est porteuse d?applications majeures dans le domaine de la santé, des communications et de l?énergie. 100 ans après, les physiciens n?ont toujours pas fini d?explorer ce phénomène et ses applications. Le CERN abrite des applications de la supraconductivité à des échelles inédites. L?accélérateur de particules LHC, avec ses milliers d?aimants supraconducteurs répartis sur 27 kilomètres de circonférence, est en effet la plus grande application mondiale de la supraconductivité. Il ne pourrait exister sans elle.  Le CERN fête donc la découverte de la supraconductivité avec une conférence exceptionnelle donnée par Philippe Lebrun. Au cours de cette conférence, l?expérience historique de Kammerlingh Onnes sera reproduite. Philippe Lebrun racontera l?histoire de cette étonnante découverte, en la replaçant dans le contexte scientifique de l?époque. Il racontera les développements scientifiques et les applications du premier siècle de la supraconductivité. Conférence en français Merci de bien vouloir vous inscrire au : +41 22 767 76 76 ou cern.reception@cern.ch

  8. La supraconductivité a 100 ans !

    SciTech Connect (OSTI)

    2011-04-14

    Il y a 100 ans, le 8 avril 1911, une découverte majeure était réalisée : celle de la supraconductivité. La supraconductivité est la caractéristique qu’ont certains métaux et alliages de perdre toute résistance électrique en dessous d’une température donnée. Cette renversante découverte, réalisée de manière presque fortuite par Kammerlingh Onnes de l’Université de Leyde (Pays-Bas) et son étudiant Gilles Holst, a ouvert un nouveau champ de recherche en physique et de fabuleuses perspectives d’applications technologiques. Du point de vue scientifique, la supraconductivité est en effet l’une des rares manifestations de la physique quantique à l’échelle macroscopique.  Du point de vue des retombées techniques, elle est porteuse d’applications majeures dans le domaine de la santé, des communications et de l’énergie. 100 ans après, les physiciens n’ont toujours pas fini d’explorer ce phénomène et ses applications. Le CERN abrite des applications de la supraconductivité à des échelles inédites. L’accélérateur de particules LHC, avec ses milliers d’aimants supraconducteurs répartis sur 27 kilomètres de circonférence, est en effet la plus grande application mondiale de la supraconductivité. Il ne pourrait exister sans elle.  Le CERN fête donc la découverte de la supraconductivité avec une conférence exceptionnelle donnée par Philippe Lebrun. Au cours de cette conférence, l’expérience historique de Kammerlingh Onnes sera reproduite. Philippe Lebrun racontera l’histoire de cette étonnante découverte, en la replaçant dans le contexte scientifique de l’époque. Il racontera les développements scientifiques et les applications du premier siècle de la supraconductivité. Conférence en français Merci de bien vouloir vous inscrire au : +41 22 767 76 76 ou cern.reception@cern.ch

  9. How consistent are top-down hydrocarbon emissions based on formaldehyde observations from GOME-2 and OMI?

    SciTech Connect (OSTI)

    Stavrakou, T.; Muller, J. F.; Bauwens, M.; De Smedt, I.; Van Roozendael, M.; De Maziere, M.; Vigouroux, C.; Hendrick, F.; George, M.; Clerbaux, C.; Coheur, P-F; Guenther, Alex B.

    2015-10-26

    The vertical columns of formaldehyde (HCHO) retrieved from two satellite instruments, the Global Ozone Monitoring Instrument-2 (GOME-2) on Metop-A and the Ozone Monitoring Instrument (OMI) on Aura, are used to constrain global emissions of HCHO precursors from open fires, vegetation and human activities in the year 2010. To this end, the emissions are varied and optimized using the ad-joint model technique in the IMAGESv2 global CTM (chem-ical transport model) on a monthly basis and at the model res-olution. Given the different local overpass times of GOME- 2 (09:30 LT) and OMI (13:30 LT), the simulated diurnal cy-cle of HCHO columns is investigated and evaluated against ground-based optical measurements at seven sites in Europe, China and Africa. The modeled diurnal cycle exhibits large variability, reflecting competition between photochemistry and emission variations, with noon or early afternoon max-ima at remote locations (oceans) and in regions dominated by anthropogenic emissions, late afternoon or evening max-ima over fire scenes, and midday minima in isoprene-rich re-gions. The agreement between simulated and ground-based columns is generally better in summer (with a clear after-noon maximum at mid-latitude sites) than in winter, and the annually averaged ratio of afternoon to morning columns is slightly higher in the model (1.126) than in the ground-based measurements (1.043).The anthropogenic VOC (volatile organic compound) sources are found to be weakly constrained by the inversions on the global scale, mainly owing to their generally minor contribution to the HCHO columns, except over strongly pol-luted regions, like China. The OMI-based inversion yields total flux estimates over China close to the bottom-up inven-tory (24.6 vs. 25.5 TgVOC yr-1 in the a priori) with, how-ever, pronounced increases in the northeast of China and re-ductions in the south. Lower fluxes are estimated based on GOME-2 HCHO columns (20.6 TgVOC yr-1), in