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1

Vela | Open Energy Information  

Open Energy Info (EERE)

Vela Vela Jump 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 1984 Phone number +971 4 3123100 Website http://www.vela.ae/-History-Ve Coordinates 25.2269166031°, 55.2832889557° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":25.2269166031,"lon":55.2832889557,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

2

Grady Electric Membership Corp | Open Energy Information  

Open Energy Info (EERE)

Grady Electric Membership Corp Grady Electric Membership Corp Jump to: navigation, search Name Grady Electric Membership Corp Place Georgia Utility Id 7450 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Net Metering Outdoor Lighting Service - High Pressure Sodium 100w Lighting Outdoor Lighting Service - High Pressure Sodium 100w decorative Lighting Outdoor Lighting Service - High Pressure Sodium 250w Lighting Outdoor Lighting Service - High Pressure Sodium 400w Lighting Outdoor Lighting Service - Mercury Vapor 175w Lighting

3

Escape from Vela X  

SciTech Connect (OSTI)

While the Vela pulsar and its associated nebula are often considered as the archetype of a system powered by a {approx} 10{sup 4} year old isolated neutron star, many features of the spectral energy distribution of this pulsar wind nebula are both puzzling and unusual. Here we develop a model that for the first time relates the main structures in the system, the extended radio nebula (ERN) and the X-ray cocoon through continuous injection of particles with a fixed spectral shape. We argue that diffusive escape of particles from the ERN can explain the steep Fermi-LAT spectrum. In this scenario Vela X should produce a distinct feature in the locally-measured cosmic ray electron spectrum at very high energies. This prediction can be tested in the future using the Cherenkov Telescope Array (CTA). If particles are indeed released early in the evolution of PWNe and can avoid severe adiabatic losses, PWN provide a natural explanation for the rising positron fraction in the local CR spectrum.

Hinton, J.; /Leicester U.; Funk, S.; /KIPAC, Menlo Park; Parsons, R.D.; /Leeds U.; Ohm, S.; /Leicester U. /Leeds U.

2012-02-15T23:59:59.000Z

4

Telecommunications Concentration: Grady College MA Thesis Program Planning Form  

E-Print Network [OSTI]

Telecommunications Concentration: Grady College MA Thesis Program Planning Form Student: Advisor ( ) Telecommunication Policy JRMC 8220 ( ) Telecommunications Programming and Criticism JRMC 8230 ( ) Emerging Telecommunication Technologies JRMC 8240 ( ) Special Topics in Telecommunications JRMC 8365 ( ) Media Economics JRMC

Arnold, Jonathan

5

Automatic Synthesis of Fault Detection Modules for Mobile Robots Anders Lyhne Christensen Rehan O'Grady Mauro Birattari Marco Dorigo  

E-Print Network [OSTI]

'Grady Mauro Birattari Marco Dorigo IRIDIA-CoDE, Universit´e Libre de Bruxelles 50, Avenue Franklin Roosevelt

Birattari, Mauro

6

Telecommunications Concentration: Grady College MA Non-Thesis Program Planning Form  

E-Print Network [OSTI]

Telecommunications Concentration: Grady College MA Non-Thesis Program Planning Form Student Methodology in Mass Communication 3. JRMC 8025 ( ) Mass Media Law OR JRMC 8120 ( ) Telecommunications Policy in Media Industries JRMC 8200 ( ) Media Management JRMC 8210 ( ) Telecommunications Policy JRMC 8220

Arnold, Jonathan

7

Telecommunications Concentration: Grady College MA Non-Thesis Program Planning Form  

E-Print Network [OSTI]

Telecommunications Concentration: Grady College MA Non-Thesis Program Planning Form Student JRMC 8210 ( ) Telecommunications Policy JRMC 8220 ( ) Telecommunications Programming and Criticism JRMC 8230 ( ) Emerging Telecommunications Technologies JRMC 8240 ( ) Special Topics in Telecommunications

Arnold, Jonathan

8

The Optical Spectrum of the Vela Pulsar  

E-Print Network [OSTI]

Our knowledge of the optical spectra of Isolated Neutron Stars (INSs) is limited by their intrinsic faintness. Among the fourteen optically identified INSs, medium resolution spectra have been obtained only for a handful of objects. No spectrum has been published yet for the Vela pulsar (PSR B0833-45), the third brightest (V=23.6) INS with an optical counterpart. Optical multi-band photometry underlines a flat continuum.In this work we present the first optical spectroscopy observations of the Vela pulsar, performed in the 4000-11000 A spectral range.Our observations have been performed at the ESO VLT using the FORS2 instrument. The spectrum of the Vela pulsar is characterized by a flat power-law (alpha = -0.04 +/- 0.04), which compares well with the values obtained from broad-band photometry. This confirms, once more, that the optical emission of Vela is entirely of magnetospheric origin. The comparison between the optical spectral indeces of rotation-powered INSs does not show evidence for a spectral evolution suggesting that, as in the X-rays, the INS aging does not affect the spectral properties of the magnetospheric emission. At the same time, the optical spectral indeces are found to be nearly always flatter then the X-rays ones, clearly suggesting a general spectral turnover at lower energies.

R. P. Mignani; S. Zharikov; P. A. Caraveo

2007-07-13T23:59:59.000Z

9

A Taxonomy of C-systems WALTER A. CARNIELLI CLE and IFCH, Unicamp, Brazil  

E-Print Network [OSTI]

15 A Taxonomy of C-systems · WALTER A. CARNIELLI CLE and IFCH, Unicamp, Brazil carniell@cle.unicamp.br JO?O MARCOS RUG, Ghent, Belgium, and IFCH, Unicamp, Brazil vegetal@cle.unicamp.br Abstract The logics from CNPq / Brazil and from the A. von Humboldt Foundation, and thanks colleagues from the Advanced

Lisboa, Universidade Técnica de

10

A Taxonomy of C-systems WALTER A. CARNIELLI CLE and IFCH, Unicamp, Brazil  

E-Print Network [OSTI]

1 A Taxonomy of C-systems ···· WALTER A. CARNIELLI CLE and IFCH, Unicamp, Brazil carniell@cle.unicamp.br JO?O MARCOS RUG, Ghent, Belgium, and IFCH, Unicamp, Brazil vegetal@cle.unicamp.br Abstract The logics from CNPq / Brazil and from the A. von Humboldt Foundation, and thanks colleagues from the Advanced

Lisboa, Universidade Técnica de

11

Health & Medical Journalism Concentration: Grady College MA Non-Thesis Program Planning Form  

E-Print Network [OSTI]

Health & Medical Journalism Concentration: Grady College MA Non-Thesis Program Planning Form Methodology in Mass Communication 3. JRMC 7355 ( ) Health and Medical Journalism 4. JRMC 7356 ( ) Advanced Health and Medical Journalism Co-requisite for Concentration ­ for students with limited undergraduate

Arnold, Jonathan

12

Water Use and Sustainability in La Altagracia, Dominican Republic Caitlin Grady  

E-Print Network [OSTI]

Water Use and Sustainability in La Altagracia, Dominican Republic By Caitlin Grady Tamim Younos Research Experiences for Undergraduates (NSF REU) program Grant No.0649070, the Virginia Water Resources as necessarily representing the official policies, either expressed or implied, of the Virginia Water Resources

Beex, A. A. "Louis"

13

Differences in cultural perception: a comparison of John Grady Cole & Billy Parham in Cormac McCarthy's The Border Trilogy  

E-Print Network [OSTI]

DIFFERENCES IN CULTURAL PERCEPTION: A COMPARISON OF JOHN GRADY COLE & BILLY PARHAM IN CORMAC MCCARTHY' S THE BORDER TRILOGY A Senior Honors Thesis by KATRINA ANN RIPPERDA Submitted to the Office of Honors Programs & Academic Scholarships... Texas ARM University in partial fulfillment of the requirements of the UNIVERSITY UNDERGRADUATE RESFARCH FELLOWS April 2001 Group: Humanilies DIFFERENCES IN CULTURAL PERCEPTION: A COMPARISON OF JOHN GRADY COLE 4 BILLY PARHAM IN CORMAC MCCARTHY...

Ripperda, Katrina Ann

2013-02-22T23:59:59.000Z

14

GRADY GRADUATION CHECKLIST Retrieve and review the Advising Plan-of-Study Form you received during your last  

E-Print Network [OSTI]

GRADY GRADUATION CHECKLIST Retrieve and review the Advising Plan-of-Study Form you received during in to DegreeWorks (degreeworks.uga.edu) to review your degree audit. Review your "Expected Graduation Term for that minor on your degree audit. Review all sections and each individual requirement on the audit. All

Arnold, Jonathan

15

Spatially Resolved X-ray Spectroscopy of Vela Shrapnel A  

E-Print Network [OSTI]

We present the detailed X-ray spectroscopy of Vela shrapnel A with the XMM-Newton satellite. Vela shrapnel A is one of several protrusions identified as bullets from Vela supernova explosion. The XMM-Newton image shows that shrapnel A consists of a bright knot and a faint trailing wake. We extracted spectra from various regions, finding a prominent Si Ly$_\\alpha$ emission line in all the spectra. All the spectra are well represented by the non-equilibrium ionization (NEI) model. The abundances are estimated to be O$\\sim$0.3, Ne$\\sim$0.9, Mg$\\sim$0.8, Si$\\sim$3, Fe$\\sim$0.8 times their solar values. The non-solar abundance ratio between O and Si indicates that shrapnel A originates from a deep layer of a progenitor star. We found that the relative abundances between heavy elements are almost uniform in shrapnel A, which suggests that the ejecta from supernova explosion are well mixed with swept-up interstellar medium.

S. Katsuda; H. Tsunemi

2006-03-17T23:59:59.000Z

16

NNSA Commemorates 50th Anniversary of First Vela Launch | National Nuclear  

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

Commemorates 50th Anniversary of First Vela Launch | National Nuclear Commemorates 50th Anniversary of First Vela Launch | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Press Releases > NNSA Commemorates 50th Anniversary of First Vela Launch Press Release NNSA Commemorates 50th Anniversary of First Vela Launch Oct 28, 2013 Vela Launch WASHINGTON, D.C. - The National Nuclear Security

17

OFF VUF-2700 FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY  

Office of Legacy Management (LM)

09 09 OFF VUF-2700 FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY THE ADVANCED RESEARCH PROJECTS AGENCY OF THE DEPARTMENT OF DEFENSE AND THE U.S. ATOMIC ENERGY COMMISSION FALLON, NEVADA OCTOBER 26, 1963 Project 9.1 U.s. Army Engineer Waterways Experiment Station James M. Polatty / James E. McDonald Issuance Dates May 1j 1965 IT lAS VEGAS llBiU\Rl LEG A L NOTICE '. ':" This report was prepared as an account or Government eponecred work. Neither the United States, nor the commtseton, nor any pereon acting oabahal! of the Commission: A.Makesany warranty or representation. e.xpressedor implied, with reepect to the accu- racy, completeness,orusefulnes8o! tbeinformaUoncontalned in this report, cr tbst the use of any tntormeucn, appa-ratua, method, or prcceee disclosed in this report may not infringe privately owned rights; or B. Assumes any lIabUitlea wIth respect to the use of.

18

Cle Elum and Supplementation Research Facility : Monthly Progress Report October 2008.  

SciTech Connect (OSTI)

FISH PRODUCTION: On October 7th the 2008 spawning season was completed. 823 adults were transferred to the facility for the 2008 season. The overall adult mortality was 6.9% (1.3% pre-spawning mortality and 5.6% encountered after sorting). Wild/natural salmon collected included 278 females, 173 males, and 29 jacks for a total 480 fish for the 2008 brood. Supplemented brood stock collected included 149 adults (85 females, 35 males and 29 jacks). Hatchery control brood collected for research included 194 adults (91 females, 68 males and 35 jacks). Eggs will be inventoried in November with an actual summary of eggs numbers to be submitted for the November report. The estimated egg takes (production) for the 2008 season was 1,375,146 eggs with 1,006,063 comprising of W x W crosses and 250,755 eggs of H x H crosses with 118,328 supplement crosses. Total fish on hand for the 2007 brood is 768,751 with an average fish per pound of 30.6 f/lb. FISH CULTURE: The marking and pit-tagging operation started on October 13th. The pit-tagging portion was completed on October 23rd. A total 40,000 juveniles were pit-tagged (2,000 from each of the production ponds and 4,000 each for the hatchery juvenile ponds 9 & 10). Cle Elum staff began shocking, sorting, counting and splitting eggs in incubation. Shocking eggs will separate live eggs from dead eggs. Eggs are treated with formalin three times a week to control fungus. The focus for the culturists during the month of October entail completing the final spawn (egg take) on the 7th, pond cleaning, keeping the marking trailers supplied with fish and end of month sampling. The adult holding ponds were power washed and winterized for the shut down period. Facility crew members Greg Strom and Mike Whitefoot assisted Joe Blodgett and his crew with fish brood collection on the 22nd of October. Fall Chinook and Coho salmon were seined up and put in tanker trucks from Chandler canal and transported to holding ponds for later spawning. Charlie, Simon and Vernon assisted with sorting and spawning Summer Chinook at the Wells hatchery for the Summer Chinook reintroduction program on the lower Yakima River. WATER PRODUCTION: The current combined well and river water supply to the complex is 12,909 gallons/min. Four river pumps (12,400gpm) and one well pump No.2 (509gpm) are supplying water to the facility main head box and the egg incubation building. ACCLIMATION SITES: Easton had much activity in October, the electrical power panel that's switches commercial power operation to generator power (transfer switch) malfunctioned. Charlie called Wallace Electric as well as ASCO Services to trouble shoot the problem which has yet to be determined. Heaters have been turned on in all service buildings at the acclimation sites. Pacific States Marine Fisheries Commission traveled to Easton to install a pole to mount a satellite and a new ups backup system with new monitors and computers for pit tag data recording and transmitting. Brown and Jackson pumped out the septic tanks at Easton and Clark Flat. AMB Tools performed maintenance on the compressors at the acclimation sites as well as Cle Elum (5 total). VEHICLE MAINTENANCE: Day Wireless performed maintenance on all handheld and vehicle radios. Day Wireless repaired radio communications (static noise) on the 6th also. All vehicles mileages and conditions are reported monthly to Toppenish. Cle Elum staff continues to clean and maintain all facility vehicles weekly. MAINTENANCE BUILDING MAINTENANCE: Kevin of Raincountry was called in response to repairs needed to the water chiller system. Cle Elum staff winterized all irrigation as well as shop grounds. Brown and Jackson pumped out the septic tank at the hatchery on the 22nd. HATCHERY BUILDING MAINTENANCE: The incubation room has been set up for transfer of eggs from isolation buckets to vertical stacks, temperature units are recorded daily. RESENTDENTIAL HOUSING: Residents irrigation has been winterized and fall fertilizer was applied to all grass on facility. Four Seasons performed maintenance on all heating sy

Cle Elum Supplementation and Research Facility

2008-12-11T23:59:59.000Z

19

Probing large-scale wind structures in Vela X-1 using off-states with INTEGRAL  

E-Print Network [OSTI]

Vela X-1 is the prototype of the class of wind-fed accreting pulsars in high mass X-ray binaries hosting a supergiant donor. We have analyzed in a systematic way ten years of INTEGRAL data of Vela X-1 (22-50 keV) and we found that when outside the X-ray eclipse, the source undergoes several luminosity drops where the hard X-rays luminosity goes below 5x10^34 erg/s, becoming undetected by INTEGRAL. These drops in the X-ray flux are usually referred to as "off-states" in the literature. We have investigated the distribution of these off-states along the Vela X-1 ~8.9 day orbit, finding that their orbital occurrence displays an asymmetric distribution, with a higher probability to observe an off-state near the pre-eclipse than during the post-eclipse. This asymmetry can be explained by scattering of hard X-rays in a region of ionized wind, able to reduce the source hard X-ray brightness preferentially near eclipse ingress. We associate this ionized large-scale wind structure with the photo-ionization wake produc...

Sidoli, L; Fuerst, F; Torrejon, J M; Kretschmar, P; Bozzo, E; Pottschmidt, K

2014-01-01T23:59:59.000Z

20

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

SciTech Connect (OSTI)

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.

Mattana, F.; Terrier, R.; Zurita Heras, J. A. [Francois Arago Centre, APC (UMR 7164 Universite Paris Diderot, CNRS/IN2P3, CEA/DSM, Observatoire de Paris), 13 rue Watt, F-75205 Paris Cedex 13 (France); Goetz, D.; Caballero, I.; Soldi, S.; Schanne, S. [AIM (UMR 7158 CEA/DSM-CNRS-Universite Paris Diderot) Irfu/Service d'Astrophysique, F-91191 Gif-sur-Yvette (France); Bouchet, L. [Universite de Toulouse, UPS-OMP, IRAP, Toulouse (France); Ponti, G. [Faculty of Physical and Applied Science, University of Southampton, Southampton, SO17 1BJ (United Kingdom); Falanga, M. [International Space Science Institute (ISSI), Hallerstrasse 6, CH-3012 Bern (Switzerland); Renaud, M., E-mail: fabio.mattana@apc.univ-paris7.fr [Laboratoire Univers et Particules de Montpellier (LUPM), Universite Montpellier II, CNRS/IN2P3 UMR 5299, F-34095 Montpellier (France)

2011-12-10T23:59:59.000Z

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


21

A search for optical counterparts of the complex Vela X system  

E-Print Network [OSTI]

The pulsar wind nebula (PWN) associated with the Vela pulsar is a bright source in the radio, X-ray and gamma-ray bands, but not in the optical. This source is very near, lying at a distance of 290 pc, as inferred from the radio and optical parallax measurements of the pulsar. Knowledge of the brightness and structure of the Vela PWN in optical is important in order to constrain the underlying particle spectrum (and possibly the B-field properties and particle losses) associated with this extended source. We use results from the Digital Sky Survey, as well as results obtained using the SAAO 1.0 m telescope equipped with an imaging CCD (STE4) and BV filters, in an attempt to measure optical radiation from Vela X. To enlarge our field of view, we constructed a mosaic consisting of 3 x 3 frames around the pulsar position. We present spectral measurements from the High Energy Stereoscopic System (H.E.S.S.), Fermi Large Area Telescope (LAT), ASCA, Hubble Space Telescope (HST), Very Large Telescope (VLT), New Techn...

Marubini, T E; Venter, C; de Jager, O C

2015-01-01T23:59:59.000Z

22

Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data  

E-Print Network [OSTI]

In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small ...

Aasi, J.

23

The Cabo de la Vela MaficUltramafic Complex, Northeastern Colombian Caribbean region: a record of Multistage evolution  

E-Print Network [OSTI]

The Cabo de la Vela Mafic­Ultramafic Complex, Northeastern Colombian Caribbean region: a record-related rocks have been described from the Colombian Caribbean (MacDonald 1964; Lockwood 1965; Alvarez 1967. Geological setting The Meso-Cenozoic history of the Colombian Andes in the Caribbean region is characterized

Bermingham, Eldredge

24

FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY THE ADVANCED RESEARCH PROJECTS AGENCY OF THE  

Office of Legacy Management (LM)

VUF -1009 VUF -1009 FINAL REPORT - VELA UNIFORM PROJECT SPONSORED BY THE ADVANCED RESEARCH PROJECTS AGENCY OF THE DEPARTMENT OF DEFENSE AND THE U. S. ATOMIC ENERGY COMMl SSlON FALLON, NEVADA OCTOBER 26,1963 FINAL REPORT OF OFF-SITE SURVEILLANCE Southwestern Radiological Health Laboratory September 1, 1964 Issuance Date: November 27, 1964 L E G A L N O T I C E This report war preprred a r an account of Government rponrored work. Neither the Unlted Strtor, nor the Commlerlon, nor m y perron acting on behalf of the Commlrslon: A. Maker any warranty o r reprerentition, exprerred o r Implied, wlth respect to the accu- racy, completanerr, o r urefulners of the lnfornutlon contrlned in thls report, o r that the u r e of any lnformnti~n. apparatur, method, o r procerr dlrclored in thlr report may not infringe

25

The accretion environment in Vela X-1 during a flaring period using XMM-Newton  

E-Print Network [OSTI]

We present analysis of 100 ks contiguous XMM-Newton data of the prototypical wind accretor Vela X-1. The observation covered eclipse egress between orbital phases 0.134 and 0.265, during which a giant flare took place, enabling us to study the spectral properties both outside and during the flare. This giant flare with a peak luminosity of $3.92^{+0.42}_{-0.09} \\times 10^{37}$ erg s$^{-1}$ cm$^{-2}$ allows estimates of the physical parameters of the accreted structure with a mass of $\\sim$ $10^{21}$ g. We have been able to model several contributions to the observed spectrum with a phenomenological model formed by three absorbed power laws plus three emission lines. After analysing the variations with orbital phase of the column density of each component, as well as those in the Fe and Ni fluorescence lines, we provide a physical interpretation for each spectral component. Meanwhile, the first two components are two aspects of the principal accretion component from the surface of the neutron star, and the thi...

Martnez-Nez, Silvia; Khnel, Matthias; Kretschmar, Peter; Stuhlinger, Martin; Rodes-Roca, Jos Joaqun; Frst, Feliz; Kreykenbohm, Ingo; Martin-Carrillo, Antonio; Pollock, Andy M T; Wilms, Joern

2014-01-01T23:59:59.000Z

26

THE VELA PULSAR AND ITS LIKELY COUNTER-JET IN THE K{sub s} BAND  

SciTech Connect (OSTI)

We report the first high spatial resolution near-infrared (near-IR) imaging of the Vela pulsar in the K{sub s} band obtained with the new adaptive optics system recently mounted on the Gemini-South telescope. For the first time, we have firmly detected the pulsar in this band with K{sub s} ? 21.8 mag, and have resolved in detail an extended feature barely detected previously in the immediate vicinity of the pulsar in the J{sub s}H bands. The pulsar K{sub s} flux is fully consistent with the extension of the flat optical spectrum of the pulsar toward the IR and does not confirm the strong IR flux excess in the pulsar emission suggested earlier by the low spatial resolution data. The extended feature is about two times brighter than the pulsar and is likely associated with its X-ray counter-jet. It extends ?2'' southward of the pulsar along the X-ray counter-jet and shows knot-like structures and a red spectrum.

Zyuzin, D.; Shibanov, Yu.; Danilenko, A. [Ioffe Physical Technical Institute, Politekhnicheskaya 26, St. Petersburg 194021 (Russian Federation); Mennickent, R. E. [Department of Astronomy, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile); Zharikov, S. [Observatorio Astronmico Nacional SPM, Instituto de Astronoma, UNAM, Ensenada, BC (Mexico)

2013-10-01T23:59:59.000Z

27

Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data  

E-Print Network [OSTI]

In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a signal has been found and 95$\\%$ confidence level upper limits have been computed both assuming polarization parameters are completely unknown and that they are known with some uncertainty, as derived from X-ray observations of the pulsar wind torii. For Vela the upper limits are comparable to the spin-down limit, computed assuming that all the observed spin-down is due to the emission of gravitational waves. For Crab the upper limits are about a factor of two below the spin-down limit, and represent a significant improvement with respect to past analysis. This is the first time the spin-down limit is significantly overcome in a narrow-band search.

The LIGO Scientific Collaboration; the Virgo Collaboration; J. Aasi; B. P. Abbott; R. Abbott; T. Abbott; M. R. Abernathy; F. Acernese; K. Ackley; C. Adams; T. Adams; T. Adams; P. Addesso; R. X. Adhikari; V. Adya; C. Affeldt; M. Agathos; K. Agatsuma; N. Aggarwal; O. D. Aguiar; A. Ain; P. Ajith; A. Alemic; B. Allen; A. Allocca; D. Amariutei; S. B. Anderson; W. G. Anderson; K. Arai; M. C. Araya; C. Arceneaux; J. S. Areeda; G. Ashton; S. Ast; S. M. Aston; P. Astone; P. Aufmuth; C. Aulbert; B. E. Aylott; S. Babak; P. T. Baker; F. Baldaccini; G. Ballardin; S. W. Ballmer; J. C. Barayoga; M. Barbet; S. Barclay; B. C. Barish; D. Barker; F. Barone; B. Barr; L. Barsotti; M. Barsuglia; J. Bartlett; M. A. Barton; I. Bartos; R. Bassiri; A. Basti; J. C. Batch; Th. S. Bauer; C. Baune; V. Bavigadda; B. Behnke; M. Bejger; C. Belczynski; A. S. Bell; C. Bell; M. Benacquista; J. Bergman; G. Bergmann; C. P. L. Berry; D. Bersanetti; A. Bertolini; J. Betzwieser; S. Bhagwat; R. Bhandare; I. A. Bilenko; G. Billingsley; J. Birch; S. Biscans; M. Bitossi; C. Biwer; M. A. Bizouard; J. K. Blackburn; L. Blackburn; C. D. Blair; D. Blair; S. Bloemen; O. Bock; T. P. Bodiya; M. Boer; G. Bogaert; P. Bojtos; C. Bond; F. Bondu; L. Bonelli; R. Bonnand; R. Bork; M. Born; V. Boschi; Sukanta Bose; C. Bradaschia; P. R. Brady; V. B. Braginsky; M. Branchesi; J. E. Brau; T. Briant; D. O. Bridges; A. Brillet; M. Brinkmann; V. Brisson; A. F. Brooks; D. A. Brown; D. D. Brown; N. M. Brown; S. Buchman; A. Buikema; T. Bulik; H. J. Bulten; A. Buonanno; D. Buskulic; C. Buy; L. Cadonati; G. Cagnoli; J. Caldern Bustillo; E. Calloni; J. B. Camp; K. C. Cannon; J. Cao; C. D. Capano; F. Carbognani; S. Caride; S. Caudill; M. Cavagli; F. Cavalier; R. Cavalieri; G. Cella; C. Cepeda; E. Cesarini; R. Chakraborty; T. Chalermsongsak; S. J. Chamberlin; S. Chao; P. Charlton; E. Chassande-Mottin; Y. Chen; A. Chincarini; A. Chiummo; H. S. Cho; M. Cho; J. H. Chow; N. Christensen; Q. Chu; S. Chua; S. Chung; G. Ciani; F. Clara; J. A. Clark; F. Cleva; E. Coccia; P. -F. Cohadon; A. Colla; C. Collette; M. Colombini; L. Cominsky; M. Constancio, Jr.; A. Conte; D. Cook; T. R. Corbitt; N. Cornish; A. Corsi; C. A. Costa; M. W. Coughlin; J. -P. Coulon; S. Countryman; P. Couvares; D. M. Coward; M. J. Cowart; D. C. Coyne; R. Coyne; K. Craig; J. D. E. Creighton; T. D. Creighton; J. Cripe; S. G. Crowder; A. Cumming; L. Cunningham; E. Cuoco; C. Cutler; K. Dahl; T. Dal Canton; M. Damjanic; S. L. Danilishin; S. D'Antonio; K. Danzmann; L. Dartez; V. Dattilo; I. Dave; H. Daveloza; M. Davier; G. S. Davies; E. J. Daw; R. Day; D. DeBra; G. Debreczeni; J. Degallaix; M. De Laurentis; S. Delglise; W. Del Pozzo; T. Denker; T. Dent; H. Dereli; V. Dergachev; R. De Rosa; R. T. DeRosa; R. DeSalvo; S. Dhurandhar; M. Daz; L. Di Fiore; A. Di Lieto; I. Di Palma; A. Di Virgilio; G. Dojcinoski; V. Dolique; E. Dominguez; F. Donovan; K. L. Dooley; S. Doravari; R. Douglas; T. P. Downes; M. Drago; J. C. Driggers; Z. Du; M. Ducrot; S. Dwyer; T. Eberle; T. Edo; M. Edwards; M. Edwards; A. Effler; H. -B. Eggenstein; P. Ehrens; J. Eichholz; S. S. Eikenberry; R. Essick; T. Etzel; M. Evans; T. Evans; M. Factourovich; V. Fafone; S. Fairhurst; X. Fan; Q. Fang; S. Farinon; B. Farr; W. M. Farr; M. Favata; M. Fays; H. Fehrmann; M. M. Fejer; D. Feldbaum; I. Ferrante; E. C. Ferreira; F. Ferrini; F. Fidecaro; I. Fiori; R. P. Fisher; R. Flaminio; J. -D. Fournier; S. Franco; S. Frasca; F. Frasconi; Z. Frei; A. Freise; R. Frey; T. T. Fricke; P. Fritschel; V. V. Frolov; S. Fuentes-Tapia; P. Fulda; M. Fyffe; J. R. Gair; L. Gammaitoni; S. Gaonkar; F. Garufi; A. Gatto; N. Gehrels; G. Gemme; B. Gendre; E. Genin; A. Gennai; L. . Gergely; S. Ghosh; J. A. Giaime; K. D. Giardina; A. Giazotto; J. Gleason; E. Goetz; R. Goetz; L. Gondan; G. Gonzlez; N. Gordon; M. L. Gorodetsky; S. Gossan; S. Goler; R. Gouaty; C. Grf; P. B. Graff; M. Granata; A. Grant; S. Gras; C. Gray; G. Greco; R. J. S. Greenhalgh; A. M. Gretarsson; P. Groot; H. Grote; S. Grunewald; G. M. Guidi; C. J. Guido; X. Guo; K. Gushwa; E. K. Gustafson; R. Gustafson; J. Hacker; E. D. Hall; G. Hammond; M. Hanke; J. Hanks; C. Hanna; M. D. Hannam; J. Hanson; T. Hardwick; J. Harms; G. M. Harry; I. W. Harry; M. Hart; M. T. Hartman; C. -J. Haster; K. Haughian; S. Hee; A. Heidmann; M. Heintze; G. Heinzel; H. Heitmann; P. Hello; G. Hemming; M. Hendry; I. S. Heng; A. W. Heptonstall; M. Heurs; M. Hewitson; S. Hild; D. Hoak; K. A. Hodge; D. Hofman; S. E. Hollitt; K. Holt; P. Hopkins; D. J. Hosken; J. Hough; E. Houston; E. J. Howell; Y. M. Hu; E. Huerta; B. Hughey; S. Husa; S. H. Huttner; M. Huynh; T. Huynh-Dinh; A. Idrisy; N. Indik; D. R. Ingram; R. Inta; G. Islas; J. C. Isler; T. Isogai; B. R. Iyer; K. Izumi; M. Jacobson; H. Jang; P. Jaranowski; S. Jawahar; Y. Ji; F. Jimnez-Forteza; W. W. Johnson; D. I. Jones; R. Jones; R. J. G. Jonker; L. Ju; Haris K

2014-10-30T23:59:59.000Z

28

On the Expansion Rate, Age, and Distance of the Supernova Remnant G266.2-1.2 (Vela Jr.)  

E-Print Network [OSTI]

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 or 13.6 +/- 4.2%/kyr) 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, Katsuda et al. 2008a). 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...

Allen, G E; DeLaney, T; Filipovic, M D; Houck, J C; Pannuti, T G; Stage, M D

2014-01-01T23:59:59.000Z

29

The Gaia-ESO Survey: Discovery of a spatially extended low-mass population in the Vela OB2 association  

E-Print Network [OSTI]

The nearby (distance~350-400 pc), rich Vela OB2 association, includes $\\gamma^2$ Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for investigating the formation and early evolution of young clusters. Recent Gaia-ESO survey observations have led to the discovery of two kinematically distinct populations in the young (10-15 Myr) cluster immediately surrounding $\\gamma^2$ Velorum. Here we analyse the results of Gaia-ESO survey observations of NGC 2547, a 35 Myr cluster located two degrees south of $\\gamma^2$ Velorum. The radial velocity distribution of lithium-rich pre-main sequence stars shows a secondary population that is kinematically distinct from and younger than NGC 2547. The radial velocities, lithium absorption lines, and the positions in a colour-magnitude diagram of this secondary population are consistent with those of one of the components discovered around $\\gamma^2$ Velorum. This result shows that there is a young, low-mass stellar population spread...

Sacco, G G; Randich, S; Franciosini, E; Jackson, R J; Cottaar, M; Spina, L; Palla, F; Mapelli, M; Alfaro, E J; Bonito, R; Damiani, F; Frasca, A; Klutsch, A; Lanzafame, A; Bayo, A; Barrado, D; Jimenez-Esteban, F; Gilmore, G; Micela, G; Vallenari, A; Prieto, C Allende; Flaccomio, E; Carraro, G; Costado, M T; Jofre, P; Lardo, C; Magrini, L; Morbidelli, L; Prisinzano, L; Sbordone, L

2015-01-01T23:59:59.000Z

30

SHORT-TERM VARIABILITY OF X-RAYS FROM ACCRETING NEUTRON STAR VELA X-1. I. SUZAKU OBSERVATIONS  

SciTech Connect (OSTI)

We have analyzed the time variability of the wide-band X-ray spectrum of Vela X-1, the brightest wind-fed accreting neutron star, on a short timescale of 2 ks by using Suzaku observations with an exposure of 100 ks. During the observation, the object showed strong variability, including several flares and so-called 'low states', in which the X-ray luminosity decreases by an order of magnitude. Although the spectral hardness increases with the X-ray luminosity, the majority of the recorded flares do not show any significant changes in circumstellar absorption. However, a sign of heavy absorption was registered immediately before one short flare that showed a significant spectral hardening. In the low states, the flux level is modulated with the pulsar spin period, indicating that even at this state the accretion flow reaches the close proximity of the neutron star. Phenomenologically, the broadband X-ray spectra, which are integrated over the entire spin phase, are well represented by the 'NPEX' function (a combination of negative and positive power laws with an exponential cutoff by a common folding energy) with a cyclotron resonance scattering feature at 50 keV. Fitting of the data allowed us to infer a correlation between the photon index and X-ray luminosity. Finally, the circumstellar absorption shows a gradual increase in the orbital phase interval 0.25-0.3, which can be interpreted as an impact of a bow shock imposed by the motion of the compact object in the supersonic stellar wind.

Odaka, Hirokazu; Khangulyan, Dmitry; Watanabe, Shin; Takahashi, Tadayuki [Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa 252-5210 (Japan)] [Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa 252-5210 (Japan); Tanaka, Yasuyuki T. [Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)] [Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Makishima, Kazuo [Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan)] [Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033 (Japan)

2013-04-10T23:59:59.000Z

31

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)

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.

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

2011-09-01T23:59:59.000Z

32

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)

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.

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

2011-09-01T23:59:59.000Z

33

Fermi LAT Detection of Pulsed Gamma-Rays From the Vela-Like Pulsars PSR J1048-5832 and PSR J2229+6114  

SciTech Connect (OSTI)

We report the detection of {gamma}-ray pulsations ({ge}0.1 GeV) from PSR J2229+6114 and PSR J1048-5832, the latter having been detected as a low-significance pulsar by EGRET. Data in the {gamma}-ray band were acquired by the Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope, while the radio rotational ephemerides used to fold the {gamma}-ray light curves were obtained using the Green Bank Telescope, the Lovell telescope at Jodrell Bank, and the Parkes Telescope. The two young radio pulsars, located within the error circles of the previously unidentified EGRET sources 3EG J1048-5840 and 3EG J2227+6122, present spin-down characteristics similar to the Vela pulsar. PSR J1048-5832 shows two sharp peaks at phases 0.15 {+-} 0.01 and 0.57 {+-} 0.01 relative to the radio pulse confirming the EGRET light curve, while PSR J2229+6114 presents a very broad peak at phase 0.49 {+-} 0.01. The {gamma}-ray spectra above 0.1 GeV of both pulsars are fit with power laws having exponential cutoffs near 3 GeV, leading to integral photon fluxes of (2.19 {+-} 0.22 {+-} 0.32) x 10{sup -7} cm{sup -2} s{sup -1} for PSR J1048-5832 and (3.77 {+-} 0.22 {+-} 0.44) x 10{sup -7} cm{sup -2} s{sup -1} for PSR J2229+6114. The first uncertainty is statistical and the second is systematic. PSR J1048-5832 is one of the two LAT sources which were entangled together as 3EG J1048-5840. These detections add to the growing number of young {gamma}-ray pulsars that make up the dominant population of GeV {gamma}-ray sources in the Galactic plane.

Abdo, A.A.; /Naval Research Lab, Wash., D.C. /Federal City Coll.; Ackermann, M.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Ajello, M.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Atwood, W.B.; /UC, Santa Cruz; Axelsson, M.; /Stockholm U. /Stockholm U., OKC; Baldini, L.; /INFN, Pisa; Ballet, J.; /DAPNIA, Saclay; Barbiellini, G.; /INFN, Trieste /Trieste U.; Baring, M.G.; /Rice U.; Bastieri, D.; /INFN, Padua /Padua U.; Baughman, B.M.; /Ohio State U.; Bechtol, K.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Bellazzini, R.; /INFN, Pisa; Berenji, B.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Bloom, E.D.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Bonamente, E.; /INFN, Perugia /Perugia U.; Borgland, A.W.; /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept.; Bregeon, J.; /INFN, Pisa; Brez, A.; /INFN, Pisa; Brigida, M.; /Bari U. /INFN, Bari; Bruel, P.; /Ecole Polytechnique /Bari U. /INFN, Bari /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Columbia U. /IASF, Milan /Milan Polytechnic /DAPNIA, Saclay /INFN, Perugia /Perugia U. /Naval Research Lab, Wash., D.C. /George Mason U. /NASA, Goddard /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /INFN, Perugia /Perugia U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /LPCE, Orleans /Montpellier U. /Stockholm U. /Stockholm U., OKC /INFN, Trieste /Bari U. /INFN, Bari /UC, Santa Cruz /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /CENBG, Gradignan /CENBG, Gradignan /Montpellier U. /Bari U. /INFN, Bari /INFN, Trieste /Arecibo Observ. /Hiroshima U. /Stanford U., HEPL /KIPAC, Menlo Park /Stanford U., Phys. Dept. /Bari U. /INFN, Bari /INFN, Bari /NASA, Goddard /Maryland U. /INFN, Perugia /Perugia U.; /more authors..

2012-03-29T23:59:59.000Z

34

Grady County, Georgia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

County, Georgia: Energy Resources County, Georgia: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 30.9050079°, -84.2278796° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.9050079,"lon":-84.2278796,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

35

Grady County, Oklahoma: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

2°, -97.87216° 2°, -97.87216° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":35.0472662,"lon":-97.87216,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

36

Tagging the boll weevil (Anthonomus gradis Boh.) with P  

E-Print Network [OSTI]

moue than ths f~. The next experiment was designed to detexmLns the xate of qptaLcs males and fsua1m during a six dsy feeding period on P+. The P3 was fcd in a 2$ percent solutice of honey snd watex at, a does of 0. 62 uc/ml of soluticux. There weze...JxLrts? The next experiment was exec~ with a dose cf g. 37 uc cf P32 per mi11Giter cf soluticn. The test consisted of two replicaticne of five Ghhl@ 2. Rht@ ot lgtf4RO of p3 flkL at a rate of' 86, 4 lR/0Ll of 4ietiUA04 mter bg aquare reared, boll ?erNUs etanre4...

Mayer, Marion Sidney

2012-06-07T23:59:59.000Z

37

Scientists Fail to Solve Vela Mystery  

Science Journals Connector (OSTI)

...nuclear powers had conducted a surreptitious bomb test. Now, lacking firm...would escape detection. Other monitoring systems apparently turned up no...points out that the traditional monitoring device at Arecibo-ionosonde-did...

ELIOT MARSHALL

1980-02-01T23:59:59.000Z

38

2013-14 Alphabetical Listing of CLE Courses CLE2013-14.xlsx 1 6/27/13  

E-Print Network [OSTI]

Agricultural Development and Trade (Pre: AAEC 1005, 1006) 7 AAEC 3314 Environmental Law 2 AFST 1714 Black History of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 2 ART 2385 Survey of the History of Western Art

Buehrer, R. Michael

39

2014-15 Alphabetical Listing of CLE Courses CLE 2014-15.xlsx 1 7/29/14  

E-Print Network [OSTI]

Agricultural Development and Trade (Pre: AAEC 1005, 1006) 7 AAEC 3314 Environmental Law 2 AFST 1714 Black History of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 2 ART 2385 Survey of the History of Western Art

Buehrer, R. Michael

40

Maxwell Grady, a Ph.D. student in Physics, received a Leitzel Center  

E-Print Network [OSTI]

: 109 students presented posters, and 76 students gave oral presentations. The conference is devoted-17, was the Joan and James Leitzel Award of excellence in Science, Technology, engineering, and Mathematics education Outreach. Two graduate students were presented with cash awards--one to the student with the best

New Hampshire, University of

Note: This page contains sample records for the topic "grady cle vela" from the National Library of EnergyBeta (NLEBeta).
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they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Solving the Vela pulsar infrared excess problem Dima Zyuzin1  

E-Print Network [OSTI]

are marked using notations from Shibanov et al. (2003), except of o4 which is detected only with Gemini by about 2 along the X-ray counter-jet direction with PA 130 (Helfand et al. (2001)) marked by the dashed projected onto the counter-jet origin of its PWN (Hester et al. (1995)). The putative near-IR jet feature

42

2011 -12 Alphabetical Listing of CLE Courses Area 2011 Course Information  

E-Print Network [OSTI]

Arts and Architecture (Pre: ART 2385) 6 ART 3184 Roman Art and Architecture (3 cr.) (Pre: ART 2385) 2 ART 3184 Roman Art and Architecture (Pre: ART 2385) 6 ART 3284 Medieval Art and Architecture (3 cr Economics of the Food & Fiber System I 3 AAEC 1006 Economics of the Food & Fiber System II (Pre: AAEC 1005

Buehrer, R. Michael

43

2009 -10 Alphabetical Listing of CLE Courses Area 2009 Course Information  

E-Print Network [OSTI]

) 7 AAEC 3314 Environmental Law 2 AFST 1714 Black Studies 7 AFST 1814 Introduction to African Studies.) (for ARCH majors only) 2 ARCH 3115 History of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 6 ART 1004

Buehrer, R. Michael

44

2008-9 Alphabetical Listing of CLE Courses Area 2008 Course Information  

E-Print Network [OSTI]

Environmental Law 2 AFST 1714 Black Studies 7 AFST 1814 Introduction to African Studies (cross-listed with IDST only) 2 ARCH 3115 History of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 6 ART 1004 Experiencing

Buehrer, R. Michael

45

2007-8 Alphabetical Listing of CLE Courses Area Course Information  

E-Print Network [OSTI]

Environmental Law 2 AFST 1714 Black Studies 2 AFST 1814 Introduction to African Studies (cross-listed with IDST.) (for ARCH majors only) 2 ARCH 3115 History of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 6 ART 1004

Buehrer, R. Michael

46

2010 -11 Alphabetical Listing of CLE Courses Area 2010 Course Information  

E-Print Network [OSTI]

) 7 AAEC 3314 Environmental Law 2 AFST 1714 Black Studies 7 AFST 1814 Introduction to African Studies of Architecture I 6 ARCH 3115 History of Architecture I (3 cr.) 2 ARCH 3116 History of Architecture II 6 ARCH 3116 History of Architecture II (3 cr.) 6 ART 1004 Experiencing the Visual Arts (1 cr.) 6 ART 1114 Living

Buehrer, R. Michael

47

Helping new students navigate McGill Brought to you by Campus Life & Engagement (CL&E) THE HOME STRETCH  

E-Print Network [OSTI]

: A Charlie Brown Christmas (1965) and Dr. Seuss' How the Grinch Stole Christmas (1966). WHEN: Sunday December at home. - Exam locations can be noisy (lights "hum", people cough, etc.), so you may want earplugs

Barthelat, Francois

48

IMPACT Vol. 5 No. 1 | Spring 2010 CLeAn eneRGy DeMAnDS  

E-Print Network [OSTI]

and development are vital if America is to decrease greenhouse gas emissions at lower cost, reduce dependence and reduce environ- mental risks. The University of Maryland Energy Research Center, or UMERC, coordinates of Science and Technology Policy. Many of the major federal grants related to energy research, including

Hill, Wendell T.

49

Search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar  

E-Print Network [OSTI]

The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mode oscillations in their parent neutron star that couple to gravitational-wave emission. In August 2006, a timing glitch ...

Barsotti, Lisa

50

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

51

EIS-0169-SA-08: Supplement Analysis  

Broader source: Energy.gov [DOE]

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

52

Sommersemester 2006 -Veranstaltungen Studieneinheit  

E-Print Network [OSTI]

113 Bonachera Rom/Hisp ?bung CLE I 4 6 36 114 Álvarez Rom/Hisp ?bung CLE I 4 6 36 115 Verdugo-Raab Rom/Hisp ?bung CLE I 4 6 36 121 Álvarez Rom/Hisp ?bung CLE II 4 6 36 122 Verdugo-Raab Rom/Hisp ?bung CLE II 4 6

Schubart, Christoph

53

CoverSheet  

Office of Scientific and Technical Information (OSTI)

is unlimited. Title: Response of High-Tc Superconductor Metamaterials to High Intensity THz Radiation Author(s): Grady, Nathaniel Perkins Jr., Bradford G. Hwang, Harold...

54

E-Print Network 3.0 - ae stars driving Sample Search Results  

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

Herbig Ae stars HD 104237 (Grady et al. 2004) and HD 163296 (Devine et... degrees inclination from pole-on) for both ... Source: Schneider, Glenn - Department of Astronomy,...

55

Gamma-Ray Bursts Nuclear Test Ban Treaty, 1963  

E-Print Network [OSTI]

Lecture 18 Gamma-Ray Bursts #12;Nuclear Test Ban Treaty, 1963 First Vela satellite pair launched and their predecessors, Vela 4, discovered the first gamma-ray bursts. The discovery was announced by Klebesadel, Strong, and Olson (ApJ, 182, 85) in 1973. #12;First Gamma-Ray Burst The Vela 5 satellites functioned from July, 1969

Harrison, Thomas

56

TECHNICAL REPORT THE GANLIB5 KERNEL GUIDE  

E-Print Network [OSTI]

The ANSI C CLE-2000 API . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3 2.1 The main . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16 3 The ANSI C LCM API . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18

Meunier, Michel

57

Formation of the Great LakesFormation of the Great Lakes Part 1Part 1  

E-Print Network [OSTI]

Precambrian Geology History Channel VideoHistory Channel Video Chapter 2 in GradyChapter 2 in Grady Chapter 2, releasing particles and energy. High energy particles may damage living cells or DNA. #12;3 Radioactive Processes involved shifting bedrock sedimentation movements of ice, water, and wind (erosion) Cambrian #12

Cochran-Stafira, D. Liane

58

Studieneinheit Nordamerika-Studien I  

E-Print Network [OSTI]

114 Bonachera Álvarez Rom/Hisp ?bung CLE I 4 6 36 115 Alvarez Olañeta Rom/Hisp ?bung CLE I 4 6 36 116 Verdugo-Raab Rom/Hisp ?bung CLE I 4 6 36 121 Álvarez Olañeta Rom/Hisp ?bung CLE II 4 6 36 122 Verdugo-Raab Rom/Hisp ?bung CLE II 4 6 Wahlbereich siehe Modul- beschreibung und VV Basismodul Sprach- und

Schubart, Christoph

59

Studieneinheit Nordamerika-Studien I  

E-Print Network [OSTI]

Faure Romanistik ?bung CLF II 4 6 36 112 Bonachera Rom/Hisp ?bung CLE I 4 6 36 113 Álvarez Rom/Hisp ?bung CLE I 4 6 36 114 Verdugo-Raab Rom/Hisp ?bung CLE I 4 6 36 121 Álvarez Rom/Hisp ?bung CLE II 4 6 36 121 Verdugo-Raab Rom/Hisp ?bung CLE II 4 6 Wahlbereich siehe Modul- beschreibung und VV Basismodul

Schubart, Christoph

60

Astronomy by microscope  

Science Journals Connector (OSTI)

......August 2009 research-article Features Astronomy by microscope Monica M Grady reviews the astronomy revealed in samples of solar system material...of the Natural History Museum, London. Astronomy is the study of stars (and galaxies......

Monica M Grady

2009-08-01T23:59:59.000Z

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61

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

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

erie.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,...

62

DEAN'S LIST Spring Semester 2014  

E-Print Network [OSTI]

Andrews, Eric Scott Armstrong, Ian Patrick Arreaga, Kevin Joel Arroyo-Williams, Noe Isaac Arth, Adeline Gotlieb, Isaac Benjamin Gotobed, Phillip Tulio Grady, Ryan P. Grainger, Alexis V. Grainger, Katerina Shae

Wong, Pak Kin

63

Senescence Can Explain Microbial Persistence I. Klappera,b  

E-Print Network [OSTI]

@math.montana.edu. Running Title: Senescence Can Explain Microbial Persistence Contents Category: Theoretical Microbiology 1 been observed (Balaban et al., 2004; Bigger, 1944; Gilbert et al., 1990; Green- wood & O'Grady, 1970

Klapper, Isaac

64

ENCLOSURE A (D.R. n. 903 del 11.10.2010) SUBJECT GROUP: INDUSTRIAL ENGINEERING  

E-Print Network [OSTI]

meccanica applicata e robotica Subjects of interview metodi di analisi e sintesi di meccanismi, meccanismi per la robotica, gradi di libertà e criteri di distribuzione fra robot cooperanti, knowledge

Genova, Università degli Studi di

65

HELIOS Helical Orbit Spectrometer HELIOS  

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

locations of the Si detector array for outgoing charged parti- cle detection, an elastic scattering monitor, and a detector for recoil identification. www.phy.anl.govatlashelios...

66

LES KARATES UNE COMMUNAUTE CAIROTE A L'HEURE DE L'TAT-NATION  

E-Print Network [OSTI]

ensuite en Palestine au Xe siècle, et arriva en Egypte. Un certain nombre de familles persanes, dont les

Paris-Sud XI, Université de

67

Compte rendu de : Jack FEUILLET -Introduction la typologie linguistique. Honor Champion, Paris  

E-Print Network [OSTI]

'analyse par exemple Sibawayhi, le grammairien persan de l'arabe, VIII siècle). Dans le chapitre sur la

Paris-Sud XI, Université de

68

La porcelaine de Chine Byzance et dans l'Orient chrtien  

E-Print Network [OSTI]

arabes, persans et turcs relatifs à l'Extrême-Orient du 8e au 13e siècle, Paris, 1913, p. 31 ; P. KAHLE

Paris-Sud XI, Université de

69

Numro d'ordre : 2009-ISAL-0083 Anne 2009 prsente devant  

E-Print Network [OSTI]

te procure des souliers. Avicenne, philosophe et médecin persan, IXème siècle. A Anaïs, A mes parents

Paris-Sud XI, Université de

70

The Smartest Living Nanomachine Silent Sentries  

E-Print Network [OSTI]

weapons programs. In the late 1950s the United States launched Project Vela to monitor nuclear testing for detecting atmospheric tests, and Vela Hotel for detecting nuclear tests from space. Between 1960 and 1963 stations that could detect all but the smallest underground nuclear tests. Within a few short years

71

NERSC-ScienceHighlightsMarch2014.pptx  

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

s imula5ons o f nanopar5cle a ssembly d uring controlled l iquid e vapora5on s how that quality of the nanopar5cle crystal forma5on i s a f unc5on o f e vapora5on rate....

72

ERCOT Wind Scraper | Open Energy Information  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » ERCOT Wind Scraper Jump to: navigation, search Tool Summary Name: ERCOT Wind Scraper Agency/Company /Organization: Prof. Mack Grady, Baylor University Sector: Energy Focus Area: Wind Resource Type: Software/modeling tools User Interface: Desktop Application Website: web.ecs.baylor.edu/faculty/grady/ OpenEI Keyword(s): Community Generated ERCOT Wind Scraper Screenshot References: W. Mack Grady[1] ERCOT Wind Scraper retrieves, displays, and logs minute-by-minute system generation, load, and wind generation from ERCOT's public web site. ERCOT Wind Scraper retrieves, displays, and logs minute-by-minute system generation, load, and wind generation from ERCOT's public web site. Instructions are included in a zipped file along with the program.

73

50 Years of Space  

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

energy to propel an aircraft or rocket. First nuclear reactor-rocket x x 1963 GAMMA-RAY BURSTS Designed and built to warn of banned nuclear tests, our Vela satellite...

74

shoal.cdr  

Office of Legacy Management (LM)

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...

75

Le vendredi 7 juin 2013 Friday, June 7, 2013 20 h 8:00 p.m.  

E-Print Network [OSTI]

La France profane au XXe siècle / XXth Century secular France Pilons l'orge FRANCIS POULENC Deux dans des écoles à vocation musicale et des camps musicaux, dont notamment le Camp musical St

Volesky, Bohumil

76

E-Print Network 3.0 - aupres du futur Sample Search Results  

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

futur Search Powered by Explorit Topic List Advanced Search Sample search results for: aupres du futur Page: << < 1 2 3 4 5 > >> 1 Mise en accord de cle de session authentifiee par...

77

UNIVERSIT PARIS 7 DENIS DIDEROT UFR SCIENCES PHYSIQUES DE LA TERRE  

E-Print Network [OSTI]

mathématiques de Omar Khayyam, sage persan, poète, et astronome du onzième siècle. A une époque où règne une

Paris-Sud XI, Université de

78

E-Print Network 3.0 - atlas aupres du Sample Search Results  

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

du Search Powered by Explorit Topic List Advanced Search Sample search results for: atlas aupres du Page: << < 1 2 3 4 5 > >> 1 Mise en accord de cle de session authentifiee...

79

Mercury speciation in Galveston Bay, Texas: the importance of complexation by natural organic ligands.  

E-Print Network [OSTI]

??The major goal of this research is the development of a competitive ligand equilibration-solvent solvent extraction (CLE-SSE) method to determine organically complexed mercury species in (more)

Han, Seunghee

2005-01-01T23:59:59.000Z

80

La vitesse de rarfaction n'est donc pas, et on devait s'y attendre a priori, comparable celle que ralise la pompe mcanique de  

E-Print Network [OSTI]

'acide oxalique en pré- sence de nitrate d'uranyle. Contrairement à la théorie de Bodens- (1) J. cle 5e série, t

Boyer, Edmond

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


81

GeT Move: An Efficient and Unifying Spatio-Temporal Pattern Mining System for  

E-Print Network [OSTI]

been applied in many real world applications, e.g., in ecological study, vehi- cle control, mobile and vehicle control. Despite the growing demands for diverse applications, there have been few scalable tools

Paris-Sud XI, Université de

82

131st AAAS Annual Meeting  

Science Journals Connector (OSTI)

...spectrum as an unex-plored natural resource for economic...develop-ment of museums of natural history and anthropology...G. E. L. Owen (Corpus Christi College, Oxford, England...Brunswick). Man's natural mus-cle system, G...

1964-12-04T23:59:59.000Z

83

Pense, langage et communaut Automne 2014  

E-Print Network [OSTI]

, apparue au d�but du 20e si�cle, qui affirme le caract�re central de la philosophie du langage au sein de l'ensemble des disciplines philosophiques et qui fait intervenir l'analyse du langage comme m�thode de d�couverte philosophique. Il s'agit de l'un des plus importants courants de pens�e du vingti�me si�cle, d�velopp� surtout

Parrott, Lael

84

Alleaume, Denis, 1998, L'Egypte l'aube du XXe sicle : Pays, bourgs, cits en des temporalits divergentes,  

E-Print Network [OSTI]

Alleaume, Denis, 1998, « L'Egypte à l'aube du XXe siècle : Pays, bourgs, cités en des temporalités L'Egypte à l'aube du XXe siècle : Pays, bourgs, cités en des temporalités divergentes Ghislaine), SEDET, université Paris 7, 2009 Dans les travaux sur l'histoire récente des villes d'Egypte, l

Boyer, Edmond

85

Transparent Slippery Surfaces Made with Sustainable Porous Cellulose Lauroyl Ester Films  

Science Journals Connector (OSTI)

(c) Transparency of various nanoporous CLE films (dotted lines) and corresponding slippery CLE films (solid lines). ... The critical magnetic field required to start the drop in motion was 0.06 T (measured at a 20 mm dropmagnet distance by a Teslameter, Projekt Elektronik GmbH, Berlin). ... (c) Magnetic glycerol drop (60 ?L) divided into two droplets by two magnets applied beside the drop. ...

Longquan Chen; Andreas Geissler; Elmar Bonaccurso; Kai Zhang

2014-04-22T23:59:59.000Z

86

Rseaux marchands et comptabilit au XVIIIe Cheryl S. Mc  

E-Print Network [OSTI]

Réseaux marchands et comptabilité au XVIIIe siècle Cheryl S. Mc Watters, University of Alberta intéressante de franchir les clivages disciplinaires. Nous nous intéressons en priorité aux réseaux marchands processus de croissance du capitalisme marchand au XVIIIe siècle. Dans ces travaux, les réseaux constituent

Paris-Sud XI, Université de

87

The conformal loop ensemble nesting field  

E-Print Network [OSTI]

The conformal loop ensemble CLE$_\\kappa$ with parameter $8/3 nesting field. We generalize this result by assigning i.i.d. weights to the loops, and we treat an alternate notion of convergence to the nesting field in the case where the weight distribution has mean zero. We also establish estimates for moments of the number of CLE loops surrounding two given points.

Jason Miller; Samuel S. Watson; David B. Wilson

2014-12-21T23:59:59.000Z

88

SPECOLA Computer Enquiry Language for the Non-Programmer  

Science Journals Connector (OSTI)

......though this would be at some cost in efficiency, to use the language...wants to find the two words Nuclear and Reactor (a) next to each...JOHN OUTPUT H 641005 BA BULL BS EA1 EA2 O'GRADY SEAN ES IRISH...SUBJ AND GIST OUTPUT 630615 NUCLEAR PHYSICS CA JAMES P PARKINGTON......

Bernard Smith

1968-08-01T23:59:59.000Z

89

Genotype determining low catechol-O-methyltransferase activity as a risk factor for obsessive-compulsive?disorder  

Science Journals Connector (OSTI)

...6 Murphy D L Greenberg B Altemus M Benjamin J Grady T Pigott T ( 1995 ) in Advances in the Neurobiology...Gogos, J. A, Galke, B. L., Jeffery, J. A., Nestadt, G., Wolyniec, P. S, Antonarakis...Psychiatry, in press. We thank Dr. Benjamin Greenberg for his help with the collection...

Maria Karayiorgou; Margaret Altemus; Brandi L. Galke; David Goldman; Dennis L. Murphy; Jurg Ott; Joseph A. Gogos

1997-01-01T23:59:59.000Z

90

A Multivariate Baltic Sea Environmental Index Joachim W. Dippner, Georgs Kornilovs,  

E-Print Network [OSTI]

, and pronounced heterogeneity in ecosystem variables. The horizontal salinity gradient is responsible: the Arctic Oscillation index, the salinity between 120 and 200 m in the Gotland Sea, the integrated river by a closed basin circulation (Voss et al. 2005) strong horizontal as well as vertical salinity gradi- ents

Dippner, Joachim W.

91

Model Systems for Cervical Cancer  

Science Journals Connector (OSTI)

...Josey, W. E., Murphy, F. A., and Luce, C. F. Sarcomas after Inoculation of Newborn Hamsters with Herpesvirus Hom- inis Type 2 Strains. Proc. Soc. Exptl. Biol. Med., 134: 1065-1069,1970. 14. O'Grady, W. P. and McDiritt, R. W...

Nubia Muoz

1976-02-01T23:59:59.000Z

92

Power Fluctuation Minimization During Behavioral Synthesis using ILP-Based Datapath Scheduling  

E-Print Network [OSTI]

Power Fluctuation Minimization During Behavioral Synthesis using ILP-Based Datapath Scheduling, FL 33620 smohanty,ranganat,chappidi¡ @csee.usf.edu Abstract-- We model the power fluctuation as cycle-to-cycle power gradi- ent and minimize the mean of the power gradients using ILP. We propose

Mohanty, Saraju P.

93

Materials for Advanced Energy Technologies  

Science Journals Connector (OSTI)

...made to the national energy balance. At a later...reactors may be added as converters of uranium, and...any of the solar energy methods-photovoltaic, wind, ocean thermal gradi-ent, space...way to convert the energy in coal to electricity...

Richard S. Claassen

1976-02-20T23:59:59.000Z

94

The key role of the western boundary in linking the AMOC1 strength to the north-south pressure gradient.2  

E-Print Network [OSTI]

. The simple analytical model also26 shows how available potential energy is converted into kinetic energy gradi-18 ent locally from the density distribution in numerical ocean models to test such19 an idea, has been lacking however. Recently, studies of ocean energetics have20 suggested that the AMOC is driven

Sijp, Willem

95

DE DOCTORAT *Pour davantage de dtails, ajouter le n de la thse la suite de l'adresse: http://archive-ouverte.unige.ch/unige  

E-Print Network [OSTI]

Dir. Kaufmann-Kohler, Gabrielle; Thévenoz, Luc Th. UNIGE 2013, D. 861 | Web*: 28623 CHATTON, GREGOR, Giorgio; Hottelier, Michel Th. UNIGE 2013, D. 866 | Web*: 28622 FOUOMENE, ERNEST Les protections, Paul-Gérard Th. UNIGE 2013, D. 865 | Web*: 28342 JOHANNOT GRADIS, CHRISTIANE Le patrimoine culturel

Rochaix, Jean-David

96

Hydrodynamic and Spectral Simulations of HMXB Winds  

E-Print Network [OSTI]

We describe preliminary results of a global model of the radiatively-driven photoionized wind and accretion flow of the high-mass X-ray binary Vela X-1. The full model combines FLASH hydrodynamic calculations, XSTAR photoionization calculations, HULLAC atomic data, and Monte Carlo radiation transport. We present maps of the density, temperature, velocity, and ionization parameter from a FLASH two-dimensional time-dependent simulation of Vela X-1, as well as maps of the emissivity distributions of the X-ray emission lines.

Christopher W. Mauche; Duane A. Liedahl; Shizuka Akiyama; Tomasz Plewa

2007-04-02T23:59:59.000Z

97

EIS-0169-SA-02: Supplement Analysis | Department of Energy  

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

EIS-0169-SA-02: Supplement Analysis EIS-0169-SA-02: Supplement Analysis EIS-0169-SA-02: Supplement Analysis 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 The Yakima Fisheries Project is co-managed by the Yakama Nation (YN) and the Washington Department of Fish and Wildlife (WDFW). The project consists of the collection of salmonid broodstock, incubation of eggs and rearing of fry in hatcheries, the acclimation and release of smolts, and related ecological studies in the study of natural production. DOE/EIS-0169-SA-02: Supplement Analysis for Yakima Fisheries Project-Natural Spawning Channels, Increased On-site Housing, and Upgrades to the Prosser Hatchery. Cle Elum Supplementation and Research Facility,

98

CX-006312: Categorical Exclusion Determination | Department of Energy  

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

2: Categorical Exclusion Determination 2: Categorical Exclusion Determination CX-006312: Categorical Exclusion Determination Small-Scale Spring Chinook and Coho Reintroduction CX(s) Applied: B1.20 Date: 07/21/2011 Location(s): Cle Elum, Washington Office(s): Bonneville Power Administration Bonneville Power Administration (BPA) proposes to allow the use of excess Cle Elum Hatchery supplementation line (S-line) spring Chinook adults and coho adults in a reintroduction program in habitat above Cle Elum Dam. BPA currently funds the propagation of these spring Chinook and coho salmon. BPA?s Yakima Fisheries Project Environmental Impact Statement (EIS) (DOE/EIS-0169, January 1996) anticipated that excess returning hatchery adults would be culled and landfilled or used as fertilizer. Instead, the returning adult hatchery-origin spring Chinook and coho salmon would be

99

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

Office of Scientific and Technical Information (OSTI)

P Q R S P Q R S T U V W X Y Z O'Connor, Mary (Mary O'Connor) - Department of Zoology, University of British Columbia O'Donnell, Sean (Sean O'Donnell) - Department of Biology, Drexel University O'Driscoll, Michael. A. -Department of Geological Sciences, East Carolina Universit('Driscoll, Michael. A. -Department of Geological Sciences, East Carolina Universi)ty O'Driscoll, Nelson (Nelson O'Driscoll) - Department of Earth and Environmental Sciences, Acadia University O'Gorman, Paul (Paul O'Gorman) - Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology (MIT) O'Grady, Patrick M. (Patrick M. O'Grady) - Department of Environmental Science Policy and Management, University of California at Berkeley O'Laughlin, Jay (Jay O'Laughlin) - Department of Forest Resources,

100

Browse by Discipline -- E-print Network Subject Pathways: Computer  

Office of Scientific and Technical Information (OSTI)

P Q R S P Q R S T U V W X Y Z O'Brien, Eamonn (Eamonn O'Brien) - Department of Mathematics, University of Auckland O'Brien, Timothy E. (Timothy E. O'Brien) - Department of Mathematics and Statistics, Loyola University Chicago O'Bryant, Kevin (Kevin O'Bryant) - Department of Mathematics, College of Staten Island, City University of New York O'Connell, Neil (Neil O'Connell) - Mathematics Institute, University of Warwick O'Grady, Kieran G. (Kieran G. O'Grady) - Dipartimento di Matematica, Università di Roma "La Sapienza" O'Hagan, Tony (Tony O'Hagan) - Centre for Bayesian Statistics in Health Economics & Department of Probability and Statistics, University of Sheffield O'Leary, Michael (Michael O'Leary) - Department of Mathematics, Towson University

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


101

Effects of directional epistasis on molecular evolution  

E-Print Network [OSTI]

frequency of deleterious alleles Nu cle oti de po lym orp his mm 2N? = 0.2 2Nr = 0 2Nr = 1 0 0.02 0.04 0.06 0.08 0.1 0.12 0.14 0.16 0 0.1 0.2 0.3 0.4 0.5 0.6 Average equilibrium frequency of deleterious alleles Nu cle oti de po lym orp his m m Figure 4...

Gong, Qin Qin

2009-04-24T23:59:59.000Z

102

Stabilit montaire dans l'Egypte ottomane du XVIe sicle et commerce de l'or en poudre  

E-Print Network [OSTI]

Stabilité monétaire dans l'Egypte ottomane du XVIe siècle et commerce de l'or en poudre à partir du Bilâd al-Takrûr Durant le XVIe siècle, l'évolution monétaire de l'Egypte était notablement différente de au niveau économique et commercial. L'Egypte se trouvait toujours au coeur d'un vaste réseau

Paris-Sud XI, Université de

103

A study and investigation of human error in time study observations  

E-Print Network [OSTI]

. . d, t'o st& dy a iMrute ele'ident; . third? to study a so . crrhat Ion{;er oiearent? the ~ Du +i*nate. cle:, . crit?T'or. t. ', o atua'. I of . ti?e ~ 02 mirurte cle?aerit? the follovh!: cc' binntionc !rare c:caen to deter. . ". inc the effect... Deviation fax each pattern ~ ~, vs'? ths last elsxaent in each pattern for the ?02; ?08? Seriea ? ? ? ? ?, ? ? ? ?'? 13 Ths standax'd Deviation for each pattern. va ths liat. . element in each patte'rn fox' 'ths ?03, . ?08? aex...

Case, Richard Blanch

2012-06-07T23:59:59.000Z

104

DOI: 10.1126/science.1142204 , 1412 (2007);318Science  

E-Print Network [OSTI]

. Mislow, M. S. Kim, D. B. Davis, E. M. McNally, J. Cell Sci. 115, 61 (2002). 93. J. M. Mislow et al., FEBS.sciencemag.orgDownloadedfrom #12;91. E. D. Apel, R. M. Lewis, R. M. Grady, J. R. Sanes, J. Biol. Chem. 275, 31986 (2000). 92. J. M. Cell Biol. 178, 785 (2007). 102. R. Goldman et al., Ann. N. Y. Acad. Sci. 455, 1 (1985). 103. A. J

Bedwell, David M.

105

Numerical analysis of laminar fluid flow and heat transfer in a parallel plate channel with normally in-line positioned plates  

E-Print Network [OSTI]

NUMERICAL ANALYSIS OF LAMINAR FLUID FLOW AND HEAT TRANSFER IN A PARALLEL PLATE CHANNEL WITH NORMALLY IN-LINE POSITIONED PLATES A Thesis by JOHN GRADY iVICMATH Submitted to the Office of Graduate Studies of Texas AkM University in partial... fulfillment of the requirements for the degree of MASTER OF SCIENCE December 1991 Major Subject: Mechanical Engineering NUMERICAL ANALYSIS OF LAMINAR FLUID FLOW AND HEAT TRANSFER IN A PARALLEL PLATE CHANNEI WITH NORMALLY IN-LINE POSITIONED PLATES A...

McMath, John Grady

2012-06-07T23:59:59.000Z

106

CLNS 95/1352 Observation of a Narrow State Decaying into \\Xi +  

E-Print Network [OSTI]

'Grady, 18 J. Urheim, 18 A.J. Weinstein, 18 F. W¨urthwein, 18 D.M. Asner, 19 M. Athanas, 19 D.W. Bliss, 19 W.S. Cinabro, 2 T. Liu, 2 M. Saulnier, 2 R. Wilson, 2 H. Yamamoto, 2 T. Bergfeld, 3 B.I. Eisenstein, 3 J. Ernst S.L. Jones, 22 J. Kandaswamy, 22 N. Katayama, 22 P.C. Kim, 22 D.L. Kreinick, 22 T. Lee, 22 Y. Liu

107

Size distribution functions for rock fragments  

Science Journals Connector (OSTI)

Abstract The capacity of 17 functions to represent the size distribution of fragmented rock is assessed on 1234 data sets of screened fragments from blasted and crushed rock of different origins, of sizes ranging from 0.002 to 2000mm. The functions evaluated are Weibull, Grady, log-normal, log-logistic and Gilvarry, in their plain, re-scaled and bi-component forms, and also the Swebrec distribution and its bi-component extension. In terms of determination coefficient, the Weibull is the best two-parameter function for describing rock fragments, with a median R2 of 0.9886. Among re-scaled, three-parameter distributions, Swebrec and Weibull lead with median R2 values of 0.9976 and 0.9975, respectively. Weibull and Swebrec distributions tie again as best bi-component, with median R2 of 0.9993. Re-scaling generally reduces the unexplained variance by a factor of about four with respect to the plain function; bi-components further reduce this unexplained variance by a factor of about two to three. Size-prediction errors are calculated in four zones: coarse, central, fines and very fines. Expected and maximum errors in the different ranges are discussed. The extended Swebrec is the best fitting function across the whole passing range for most types of data. Bimodal Weibull and Grady distributions follow, except for the coarse range, where re-scaled forms are preferable. Considering the extra difficulty in fitting a five-parameter function with respect to a three-parameter one, re-scaled functions are the best choice if data do not extend far below 20% passing. If the focus is on the fine range, some re-scaled distributions may still do (Weibull, Swebrec and Grady, with maximum errors of 1520% at 8% passing), but serious consideration should be given to bi-component distributions, especially extended Swebrec, bimodal Weibull and bimodal Grady.

Jos A. Sanchidrin; Finn Ouchterlony; Pablo Segarra; Peter Moser

2014-01-01T23:59:59.000Z

108

Seismic Travel-Time Residuals and Plates  

Science Journals Connector (OSTI)

......United States, Canada and Greenland under the auspices of Project Vela Uniform (Long Range Seismic Measurements 1966). Arrival...1 that if we plot residuals on the focal sphere, we are at liberty to ascribe these residuals to source effects, receiver effects......

D. Davies; D. P. McKenzie

1969-09-01T23:59:59.000Z

109

Gamma Ray Bursts Sudden, intense flashes of gamma rays  

E-Print Network [OSTI]

Gamma Ray Bursts #12;The Case Sudden, intense flashes of gamma rays come from nowhere and disappear with out a trace. Incredibly powerful: A single gamma ray burst is hundreds of times brighter a supernova #12;Who Vela (1960's) Looking for arms testing, found gamma ray bursts Compton Gamma Ray Observatory

Washington at Seattle, University of - Department of Physics, Electroweak Interaction Research Group

110

The dynamics of pulsar glitches: contrasting phenomenology with numerical evolutions  

Science Journals Connector (OSTI)

......rotation axis, R is the radius of the star and c is the speed of light. As I pI nI (typically), we can use where M is the mass...sudden. The best resolved event to date is the so-called Christmas glitch in the Vela pulsar, where the glitch rise time was......

T. Sidery; A. Passamonti; N. Andersson

2010-06-21T23:59:59.000Z

111

Magnetohydrodynamics in superconducting-superfluid neutron stars  

Science Journals Connector (OSTI)

......2) the phase velocities are small compared to the speed of light. Alfve n waves are the characteristic MHD waves that travel...1996) have shown that the rapid spin-up time for the 1988 `Christmas' glitch in the Vela pulsar implies a crustcore coupling time......

Gregory Mendell

1998-06-01T23:59:59.000Z

112

College of Science Bachelor of Science, Psychology  

E-Print Network [OSTI]

College of Science Bachelor of Science, Psychology Major Checksheet for Students Graduating Education (CLE) courses and the foreign language requirement, psychology majors are required to take 28 OF PSYCHOLOGY (6 hrs.): PSYC 2004-rntroductory Psychology (Prereq. for all other courses) PSYC 2094-Principles

Virginia Tech

113

From the Editor A six-week cyclotron shutdown to address necessary mainte-  

E-Print Network [OSTI]

out projects that will improve the performance and reliability of the Coupled Cyclotron Facility ended. Cyclotron Operations Recent Upgrades A beam of 160 MeV/nucleon 58Ni at an intensity of 5 parti- cle n array. Based on the nuclei selected from charged reaction products of 8Li breaking up in a carbon target

114

Annales Geophysicae (2003) 21: 13031313 c European Geosciences Union 2003 Geophysicae  

E-Print Network [OSTI]

Breathing of heliospheric structures triggered by the solar-cycle activity K. Scherer and H. J. Fahr Abstract. Solar wind ram pressure variations occuring within the solar activity cycle are communicated period of about 11 years. At outer heliospheric regions, the main surviving solar cy- cle feature

Boyer, Edmond

115

Presents the EENR Speaker Series for Spring 2014 "Allocating Energy Governance"  

E-Print Network [OSTI]

(2nd Floor) 1 Hour CLE Credit (no ethics) As the United States produces more of its own energy resources, land use and nuisance-based issues associated with energy development have heightened conflicts and renewable energy development. She currently teaches at Florida State University College of Law. Please RSVP

Azevedo, Ricardo

116

Different Properties of the Native and Reconstituted Heterotrimeric G Protein Thomas E. Angel,  

E-Print Network [OSTI]

Ve UniVersity, CleVeland, Ohio 44106-4970 ABSTRACT: Visual signal transduction serves as one of the best rhodopsin (Rho) causing a conformational change leading to productive interaction of this G protein-coupled receptor with the heterotrimeric G protein, transducin (Gt). Here we describe a new method for Gt

Palczewski, Krzysztof

117

Annales Geophysicae, 23, 853865, 2005 SRef-ID: 1432-0576/ag/2005-23-853  

E-Print Network [OSTI]

wind electrons and the interplanetary magnetic field (IMF) direction in the wake formation; Electrostatic structures; Spacecraft sheaths, wakes, charging) 1 Introduction The properties and dynamics that fluctuations develop in the wake behind the obsta- cle, but that they can take the form of long

Paris-Sud XI, Université de

118

Thank YouPrESIDENT'S Alfred P Sloan Foundation  

E-Print Network [OSTI]

Thank YouPrESIDENT'S CIrCLE $100,000+ Alfred P Sloan Foundation ConocoPhillips Canada ASSINIBo Industries Inc. · Alzheimer Society of Canada · Andy Liu · Branch Out Neurological Foundation · Canadian of Violet Lesia Starck · George Castles · Google Inc. · Heart & Stroke Foundation of Alberta, NWT & Nunavut

Machel, Hans

119

3D model-based tracking for UAV position control Celine Teuli`ere, Laurent Eck, Eric Marchand, Nicolas Guenard  

E-Print Network [OSTI]

3D model-based tracking for UAV position control C´eline Teuli`ere, Laurent Eck, Eric Marchand control of an unmanned aerial vehi- cle (UAV). Given a 3D model of the edges of its environment, the UAV approach. I. INTRODUCTION Unmanned aerial vehicles (UAVs) have a large range of in- door or outdoor

Paris-Sud XI, Université de

120

CoViCAD: Comprehensive Visualization of Coronary Artery Disease  

E-Print Network [OSTI]

, the patient suffers a my- ocardial infarction, also known as heart attack. Part of the heart mus- cle tissue viability information in a detailed anatomical context. We combine multiple MRI scans (whole heart anatomical data, late enhancement data) and multiple segmentations (polygonal heart model, late enhancement

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


121

4 Science Service Feature Released upon receipt  

E-Print Network [OSTI]

the idea that a solid object of some sort vas hurled to the ground vith the lightning flash, and hence lightning was supposed to be the weapon of the go6.s. I t s cle- structive effects naturallzr suggested the homes of the peasants as chams against lightning, as ne11 as other harmful agencies, real and imaginary

122

Slide 1  

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

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 ...

123

Plant Hormones and Regulators  

Science Journals Connector (OSTI)

...in-hibits a-amylase activity (44...dormin inhibits a-amylase activity induced...tubes to grow down the style toward...digestion of the starch-filled storage...radi-cle) to break through, and...now called a-amylase) responsible...liqui-fying the reserve starch. The pres-ence...

J. van Overbeek

1966-05-06T23:59:59.000Z

124

Patterns of Aging  

Science Journals Connector (OSTI)

...maintains that the impending exhaustion of the pool of grow-ing ovarian follicles triggers...size of the initial primordial folli-cle pool. In mammals, during early fetal development...that the rate of loss of the follicular pool during postnatal life is deter-mined...

Katrina L. Kelner; Jean Marx

1996-07-05T23:59:59.000Z

125

The fl Subunit of the Signal Recognition Particle Receptor Is a Transmembrane GTPase that Anchors the a Subunit, a Peripheral  

E-Print Network [OSTI]

recognition parti- cle (SRP) which is bound to the signal sequence of the nascent protein chain. This interaction catalyzes the GTP-dependent transfer of the nascent chain from SRP to the protein translocationD subunit of SRP (SRP54) each contain related GTPase domains which are required for SR and SRP function

Walter, Peter

126

Les marchands orientaux et les langues occidentales au XVIIe sicle : l'exemple des Choffelins de Marseille  

E-Print Network [OSTI]

1 Les marchands orientaux et les langues occidentales au XVIIe siècle : l'exemple des « Choffelins » de Marseille La question des marchands et des langues à l'époque moderne est loin d'être un domaine la question des marchands et des langues dans le commerce de moyenne et longue distances. Le but de

Paris-Sud XI, Université de

127

Calendar of Events Spring 2011 Wallace Stegner Center -S. J. Quinney College of Law 332 S. 1400 E. Room 101 Salt Lake City, UT 84112 801.585.3440  

E-Print Network [OSTI]

, University of Utah Director, Yellowstone Seismic Network Resources 12:15 pm � 1:15 pm, Room 106 S.J. Quinney of Law 1 hour CLE. Lunch Provided. Wallace Stegner Lecture Classic Lessons from a Little Fish in a Pork

Capecchi, Mario R.

128

Tillman Creek Mitigation Site As-Build Report.  

SciTech Connect (OSTI)

This as-built report describes site conditions at the Tillman Creek mitigation site in South Cle Elum, Washington. This mitigation site was constructed in 2006-2007 to compensate for wetland impacts from the Yakama Nation hatchery. This as-built report provides information on the construction sequence, as-built survey, and establishment of baseline monitoring stations.

Gresham, Doug [Otak, Inc.

2009-05-29T23:59:59.000Z

129

SCIENTIFIC NEWS IN WASHINGTON  

Science Journals Connector (OSTI)

...different parts of the world, and are injurious to agriculture or horticulture, he cle-voted his paper chiefly to a consideration of their...the same causes. There are two items of cost in electric lighting, the cost of the current supplied to the lamp, and the cost...

1888-04-20T23:59:59.000Z

130

Advanced High Energy and High Power Battery Systems for Automotive Applications Khalil Amine  

E-Print Network [OSTI]

Geothermal 2.5 Wind 0.22 Solar 0.02 Coal 110 Natural Gas 107 Residential 50 Vehicle 39 Freight 40 Air 129.30am Advanced High Energy and High Power Battery Systems for Automotive Applications Khalil Amine electric drive Plug in Hybrid Electric Vehicle (P-HEVs), long range electric vehi cle (EV) and sm art grid

Levi, Anthony F. J.

131

APPL: A Probability Programming Language Maj. Andrew G. GLEN, Diane L. EVANS, and Lawrence M. LEEMIS  

E-Print Network [OSTI]

APPL: A Probability Programming Language Maj. Andrew G. GLEN, Diane L. EVANS, and Lawrence M having arbitrary distributions. This arti- cle presents a prototype probability package named APPL (A probability software package, referred to as "A Prob- ability Programming Language" (APPL), that fills

Leemis, Larry

132

The nested simple conformal loop ensembles in the Riemann sphere  

E-Print Network [OSTI]

Simple conformal loop ensembles (CLE) are a class of random collection of simple non-intersecting loops that are of particular interest in the study of conformally invariant systems. Among other things related to these CLEs, we prove the invariance in distribution of their nested "full-plane" versions under the inversion $z \\mapsto 1/z$.

Antti Kemppainen; Wendelin Werner

2014-05-23T23:59:59.000Z

133

Annales Geophysicae (2003) 21: 11211140 c European Geosciences Union 2003 Geophysicae  

E-Print Network [OSTI]

, Norway 3University of Washington, Geophysics Program, Seattle, Washington, USA 4The Johns Hopkins "closed terrestrial" magnetic flux and "open" flux interconnected with the solar wind, allows of magnetic energy within the magnetosphere during the substorm cy- cle. We show the magnetosphere

Paris-Sud XI, Université de

134

CLNS 95/1347 Measurements of the decays \\Gamma ! h \\Gamma h + h \\Gamma  

E-Print Network [OSTI]

'Grady, 20 J. Urheim, 20 A.J. Weinstein, 20 F. W¨urthwein, 20 D.M. Asner, 21 M. Athanas, 21 D.W. Bliss, 21 W.S. Katayama, 2 P.C. Kim, 2 D.L. Kreinick, 2 T. Lee, 2 Y. Liu, 2 G.S. Ludwig, 2 J. Masui, 2 J. Mevissen, 2 N, 4 D. Cinabro, 4 T. Liu, 4 M. Saulnier, 4 R. Wilson, 4 H. Yamamoto, 4 T. Bergfeld, 5 B.I. Eisenstein

135

Collecting Texas: constructing regional stories among the deconstructionists  

E-Print Network [OSTI]

uniquely, and I am glad or grateful for their dissimilarities. The minutes within my stories, like those of contemporary writers, are intense, full of discovery, and always dynamic. They often come as a series of close-up photographs like those scenes... the screen door slapped shut behind us, I heard Mom ask Grady to mow the lawn. "Give you ten dollars. " "I would. Sure. But I promised to take Grandmother to the cemetery. " I knew he was looking away, avoiding the tall grass which waved across the next...

Patterson, Leslie Jill

2012-06-07T23:59:59.000Z

136

Very high energy emission as a probe of relativistic magnetic reconnection in pulsar winds  

E-Print Network [OSTI]

The population of gamma-ray pulsars, including Crab observed in the TeV range, and Vela detected above 50 GeV, challenges existing models of pulsed high-energy emission. Such models should be universally applicable, yet they should account for spectral differences among the pulsars. We show that the gamma-ray emission of Crab and Vela can be explained by synchrotron radiation from the current sheet of a striped wind, expanding with a modest Lorentz factor $\\Gamma\\lesssim100$ in the Crab case, and $\\Gamma\\lesssim50$ in the Vela case. In the Crab spectrum a new synchrotron self-Compton component is expected to be detected by the upcoming experiment CTA. We suggest that the gamma-ray spectrum directly probes the physics of relativistic magnetic reconnection in the striped wind. In the most energetic pulsars, like Crab, with $\\dot{E}_{38}^{3/2}/P_{-2}\\gtrsim0.002$ (where $\\dot{E}$ is the spin down power, $P$ is the pulsar period, and $X=X_i\\times10^i$ in CGS units), reconnection proceeds in the radiative cooling ...

Mochol, Iwona

2015-01-01T23:59:59.000Z

137

DOE/EIS-0169-SA-02: Supplement Analysis for Yakima Fisheries Project --Natural Spawning Channels, Increased On-site Housing and Upgrades to the Prosser Hatchery (8/16/99)  

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

August 16, 1999 August 16, 1999 REPLY TO ATTN OF: KEWI-4 SUBJECT: Supplement Analysis for Yakima Fisheries Project, DOE/EIS-0169-SA-02 David Byrnes Project Manager - KEWN-4 Proposed Action: Yakima Fisheries Project - Natural Spawning Channels, Increased On-site Housing, and Upgrades to the Prosser Hatchery PL-6: F3204 Location: Cle Elum Supplementation and Research Facility, Cle Elum, Washington (CESRF) and Prosser Juvenile Research Facility, Prosser, Washington Proposed by: Bonneville Power Administration (BPA) and Co-Managed by the Yakama Nation (YN) and the Washington Department of Fish and Wildlife (WDFW). 1. Introduction The Bonneville Power Administration (BPA) is funding ongoing studies, research, and artificial production of several salmonid species in the Yakima and Klickitat river basins. BPA analyzed

138

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)

Mortem of the NERSC Franklin XT 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 Introduction NERSC * NERSC is a Production Computing Facility for DOE Office of Science * NERSC serves a large scientific population * Approximately 3,000 users, * 400 projects, * 500 code instances * Focus is high end computing services CUG 2008 page 3 NERSC-5 Systems

139

Geddes_ LPAv3.pptx  

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

P 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 ! Tajima & Dawson PRL 1979; Esarey et al. RMP 2009 λ p ~100µm at 10 17 /cc Laser or beam Trapped particles Simulation reviews :ScDAC Review 2009, Huang J. Phys C.S. 2009 FD solve Maxwell ! Weight current to grid ! Move particles ! Weight Force to particles !  Electromagne0cs + p ar0cle

140

Microsoft Word - SA-07-EIS-0169-biocontrol.doc  

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

14, 2003 14, 2003 REPLY TO ATTN OF: KEC-4 SUBJECT: Supplement Analysis for Yakima/Klickitat Fisheries Project, Noxious Weed Control at Cle Elum and Jack Creek (DOE/EIS-0169-SA-07) David Byrnes - KEWL-4 Fish & Wildlife Project Manager Proposed Action: Under the Yakima/Klickitat Fisheries Project (YKFP), the Cle Elum Supplementation and Research Facility (CESRF) Management Plan calls for noxious weed control at the hatchery and acclimation sites. Biological control agents are being proposed for use at the hatchery and Jack Creek acclimation sites to reduce weeds along BPA-owned property, hatchery structures, roads, and wildlife preserve lands. The Kittitas County Noxious Weed Control Board has targeted the management of diffuse knapweed (Centaurea diffusa) and Dalmatian toadflax (Linaria genistifolia ssp. Dalmatica) as

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


141

Washington | Department of Energy  

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

January 16, 2004 January 16, 2004 EIS-0246-SA-37: Supplement Analysis Wildlife Mitigation Program, On the Spokane Indian Reservation, near Wellpinit, Stevens County, Washington November 10, 2003 EIS-0349: Record of Decision Electrical Interconnection of the BP Cherry Point Cogeneration Project October 2, 2003 EA-0307-SA-01: Supplement Analysis Colville Resident Trout Hatchery Project Supplement Analysis September 5, 2003 EIS-0349: Draft Environmental Impact Statement BP Cherry Point Cogeneration Project July 21, 2003 EIS-0317: Record of Decision Kangley-Echo Lake Transmission Line Project July 14, 2003 EIS-1069-SA-07: Supplement Analysis Yakima/Kilickitat Fisheries Project, Noxious Weed Control at Cle Elum and Jack Creek, Cle Elum Supplementation and Research Facility and Jack Creek

142

WASH-  

Office of Legacy Management (LM)

rcc.p,anc. 01 thts arf~cle. tha rcc.p,anc. 01 thts arf~cle. tha yubl~rhe, "r ~u~~iunl riknouu~adqnS the U.S. C;ov.rnmmnf' s rayhr (0 retam l nOn*aClulive.roy~ltV (r-0 ltconso In ma IO Dny Copvrlqhl WASH- covrrm~ the wtvdo. ISADIOLOGICAL SURVEY OF THE SEAWAY INDUSTRIAL PARK W . D. Cottrell, R. W . Leggett and H. W . Dickson Health Physics Division, Oak Ridge National Laboratory Oak Ridge, Tennessee 37830 December 1976 CONTENTS l&t of Tab1 es - . . . List of Illustrations . . Abstract . . . . . . Introduction . . . . ............ ............ ............ ............ Radiological Survey Techniques . . . . . . 1 . . Measurement of External Gamma and Beta-Gamma Radiation Levels . . . . . . . . . . . . Measurement of Radium in the Soil . . . . . . Measurement of Radioactivity in Surface Water

143

Supplement Analysis for Yakima/Klickitat Fisheries Project, Boone Pond Acclimation Site (DOE/EIS-0169-SA-08)  

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

April 7, 2004 April 7, 2004 REPLY TO ATTN OF: KEC-4 SUBJECT: Supplement Analysis for Yakima/Klickitat Fisheries Project, Boone Pond Acclimation Site (DOE/EIS-0169-SA-08) memorandum David Byrnes Project Manager - KEWL-4 TO: Proposed Action: Yakima/Klickitat Fisheries Project - Under the Monitoring and Evaluation Program (M&E), the coho acclimation research task would be modified to include a new site located in the upper Yakima south of Cle Elum, WA. Project No.: F3204 Location: Cle Elum, Kittitas County, Washington. Proposed by: Bonneville Power Administration (BPA) and Co-Managed by the Yakama Nation (YN) and the Washington Department of Fish and Wildlife (WDFW). 1. Introduction The Yakima Fisheries Project Final Environmental Impact Statement (YFP EIS)

144

Cray XT Documentation  

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

Cray XT Documentation Cray XT Documentation Cray XT Documentation & Cray XT Documentation Search Preferences | Advanced Search Home Browse Books Man Pages Glossary Platforms Cray XC30 Cray XE and Cray XK Cray XT Cray Sonexion Cray X2 Cray X1 Knowledge Base by Category by Date by Platform by Title by User Release Announcements @Twitter Cray XT System Documentation Getting Started Cray XT System Overview Cray Linux Environment (CLE) Software Release Overview Cray Linux Environment (CLE) Software Release Overview Supplement Glossary of Terms Programming Environment Cray Application Developer's Environment User's Guide Cray Compiling Environment (CCE) Cray Fortran Reference Manual crayftn man page Cray C and C++ Reference Manual craycc man page crayCC man page Intrinsic function man pages Assign environment man pages

145

Supplement Analyses (SA) | Department of Energy  

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

October 2, 2003 October 2, 2003 EA-0307-SA-01: Supplement Analysis Colville Resident Trout Hatchery Project Supplement Analysis August 27, 2003 EIS-0246-SA-35: Supplement Analysis Wildlife Mitigation Program, seven miles east of Juntura, Oregon, Malheur County August 22, 2003 EIS-0246-SA-34: Supplement Analysis Wildlife Mitigation Program, Flathead County, Montana July 14, 2003 EIS-1069-SA-07: Supplement Analysis 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 May 21, 2003 EIS-0246-SA-33: Supplement Analysis Wildlife Mitigation Program, Flathead County, Montana May 20, 2003 EIS-0246-SA-32: Supplement Analysis Wildlife Mitigation Program

146

Microsoft Word - Spring-Chinook_CX_6.28.11.doc  

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

July 21, 2011 July 21, 2011 REPLY TO ATTN OF: KEC-4 SUBJECT: Environmental Clearance Memorandum Patricia Smith Project Manager - KEWL-4 Proposed Action: Small-scale spring Chinook and coho reintroduction Fish and Wildlife Project No.: 1995-063-25 Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B1.20 Small-scale activities undertaken to protect, restore, or improve fish and wildlife habitat, fish passage facilities (such as fish ladders or minor diversion channels), or fisheries. Location: Cle Elum, Yakima County, Washington Proposed by: Bonneville Power Administration (BPA) Description of the Proposed Action: BPA proposes to allow the use of excess Cle Elum Hatchery supplementation line (S-line) spring Chinook adults and coho adults in a reintroduction

147

Goals:  

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

CUG 2009 Proceedings 1 of 8 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 user issues etc from these upgrades. The performance impacts on the kernel benchmarks and selected application benchmarks will also be presented. KEYWORDS: Cray XT4, Franklin, NERSC, Quad Core, CLE 2.1, Application Performance, IO Performance, User Impacts.

148

The Global Atmospheric Environment for the Next Generation  

SciTech Connect (OSTI)

Air quality, ecosystem exposure to nitrogen deposition, and climate change are intimately coupled problems: we assess changes in the global atmospheric environment between 2000 and 2030 using twenty-five state-of-the-art global atmospheric chemistry models and three different emissions scenarios. The first (CLE) scenario reflects implementation of current air quality legislation around the world, whilst the second (MFR) represents a more optimistic case in which all currently feasible technologies are applied to achieve maximum emission reductions. We contrast these scenarios with the more pessimistic IPCC SRES A2 scenario. Ensemble simulations for the year 2000 are consistent among models, and show a reasonable agreement with surface ozone, wet deposition and NO{sub 2} satellite observations. Large parts of the world are currently exposed to high ozone concentrations, and high depositions of nitrogen to ecosystems. By 2030, global surface ozone is calculated to increase globally by 1.5 {+-} 1.2 ppbv (CLE), and 4.3 {+-} 2.2 ppbv (A2). Only the progressive MFR scenario will reduce ozone by -2.3 {+-} 1.1 ppbv. The CLE and A2 scenarios project further increases in nitrogen critical loads, with particularly large impacts in Asia where nitrogen emissions and deposition are forecast to increase by a factor of 1.4 (CLE) to 2 (A2). Climate change may modify surface ozone by -0.8 {+-} 0.6 ppbv, with larger decreases over sea than over land. This study shows the importance of enforcing current worldwide air quality legislation, and the major benefits of going further. Non-attainment of these air quality policy objectives, such as expressed by the SRES-A2 scenario, would further degrade the global atmospheric environment.

Dentener, F; Stevenson, D; Ellingsen, K; van Joije, T; Schultz, M; Amann, M; Atherton, C; Bell, N; Bergmann, D; Bey, I; Bouwman, L; Butler, T; Cofala, J; Collins, B; Drevet, J; Doherty, R; Eickhout, B; Eskes, H; Fiore, A; Gauss, M; Hauglustaine, D; Horowitz, L; Isaksen, I A; Josse, B; Lawrence, M; Krol, M; Lamarque, J F; Montanaro, V; Muller, J F; Peuch, V H; Pitari, G; Pyle, J; Rast, S; Rodriguez, J; Sanderson, M; Savage, N H; Shindell, D; Strahan, S; Szopa, S; Sudo, K; Van Dingenen, R; Wild, O; Zeng, G

2005-12-07T23:59:59.000Z

149

Investigation of lane occupancy as a freeway control parameter for use during incident conditions  

E-Print Network [OSTI]

parameters were used in the automatic control of' a freeway safety warning device. Two concepts, usir g measured lane occupancy foz the detection of' freeway incidents, were developed, . The f'irst concept was ter. . . cd critical occupancy... freeway safety warning device, using critical occupancy parameters, was developed and simulated in real-time. Evaluation of the simulated operation of the device revealed. that relia'cle detection of shock waves generated by freeway incidents...

Friebele, John Duncan

1972-01-01T23:59:59.000Z

150

User and Performance Impacts from Franklin Upgrades  

SciTech Connect (OSTI)

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.

He, Yun (Helen)

2009-05-10T23:59:59.000Z

151

LANL: AOT & LANSCE The Pulse April 2011  

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

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...

152

La lecture au dfi du virtuel Christian Vandendorpe  

E-Print Network [OSTI]

autotélique, qui trouve en soi sa pro- pre finalité. Ce faisant, le roman nous a aussi appris comment lire les fait que, historiquement, le roman a été notre maître de lecture et a fait de celle-ci une activité. C'est la diffusion massive du roman à la fin du XVIe siècle, suivant de peu l'essor de l

Boyer, Edmond

153

Introduction L'Encyclopdie des Carabes ou Encyclopdie des Kali'na du Suriname  

E-Print Network [OSTI]

Introduction « L'Encyclopédie des Caraïbes » ou Encyclopédie des Kali'na du Suriname Odile Renault Suriname, jusqu'à la deuxième moitié du 20ème siècle5, pour désigner les peuples et langues de famille étude comparée des langues de la famille caribe du Suriname, ainsi que des descriptions grammaticales et

Boyer, Edmond

154

TRAVAUX DU COMIT FRANAIS D'HISTOIRE DE LA GOLOGIE (COFRHIGO)  

E-Print Network [OSTI]

Lincei (1603-1651) Résumé. Le Romain Federico Cesi fonda en 1603 l'Accademia dei Lincei, première e siècle. Abstract. The Roman Federico Cesi founded in 1603 the Accademia dei Lincei, the first ­ fossil woods ­ Vesuvius ­ Galileo ­ Peiresc ­ Barberini ­ 17 th century. Introduction Le 17 août 1603

Boyer, Edmond

155

Facult Warocqu d'Economie et de Gestion  

E-Print Network [OSTI]

certification ISO 9001-2008. Par ailleurs, Warocqué se distingue également par un attachement indéfectible à sa certifiée ISO depuis 2003 #12;P3 La Faculté Warocqué a accumulé depuis plus d'un siècle une expérience une politique de qualité exclusive et volontariste, marquée par la certification IS0 9001-2000 dont

Dupont, Stéphane

156

LA DISTILLATION a t introduite en Occident avec l'alchimie au cours du XIIe sicle. Par convention, on  

E-Print Network [OSTI]

LA DISTILLATION a été introduite en Occident avec l'alchimie au cours du XIIe siècle. Par Pseudo-Geber, distingue plusieurs façons de distiller et propose même une classi- fication de ces distillat (per descensum). La distillation par élévation des vapeurs, ou per ascensum, nécessite l

Paris-Sud XI, Université de

157

RM (1207-1273), POTE ET MYSTIQUE Quelques notes prliminaires  

E-Print Network [OSTI]

Turquie que lorsque l'on dit Mowlavi (prononciation persane) ou Mevlânâ (prononciation turque) sans plus, le soufisme et la littérature persane. ? la fin du XIIe siècle, la Transoxiane et l'Iran presque entier appartenaient aux Turcs musulmans du Khwarazm, de culture arabo-persane. Derrière eux, le reste de

Paris-Sud XI, Université de

158

Agns LENEPVEU-HOTZ doctorante l'Ecole Pratique des Hautes Etudes  

E-Print Network [OSTI]

morphèmes ham, - et bi- à l'aune d'un texte persan du XIe siècle de notre ère, le Trx-i Sstn RESUME Les morphèmes grammaticaux ham, - et bi- du persan archaïque sont traditionnellement analysés comme suit. ham rhématicité, et non d'une action semelfactive et ponctuelle. Mots clés : persan archaïque ; ham ; - ; bi

Paris-Sud XI, Université de

159

Claire Judde de Larivire, Procdures, enjeux et fonctions du testament Venise aux confins du Moyen ge et des Temps modernes. Le cas du patriciat marchand , Le Moyen  

E-Print Network [OSTI]

Moyen ?ge et des Temps modernes. Le cas du patriciat marchand », Le Moyen ?ge, t. 108, fasc. 3-4, 2002 testaments de patriciens marchands vénitiens vivant au début du seizième siècle, puisque ce travail s étaient consignées les listes des sociétaires participant à la gestion des galères marchandes4 . Ainsi l

Paris-Sud XI, Université de

160

Les communauts marchandes de l'Europe du Nord dans les ports bretons au XVIIIe  

E-Print Network [OSTI]

Les communautés marchandes de l'Europe du Nord dans les ports bretons au XVIIIe siècle Pierrick Peter Voss, «Les communautés marchandes étrangères dans l'espace urbain bordelais (62075)», dans J ou moins grande fréquentation par les communautés marchandes des différents pays européens. Cet

Paris-Sud XI, Université de

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


161

Gene rearrangement in cells with natural killer activity and expression of the ?-chain of the T-cell antigen receptor  

Science Journals Connector (OSTI)

... of Thomas19. Hybridization was to nick-translated ClE (a), ClV (b) or C2U (c) labelled with 32P-dCTP according to the procedure of Rigby et al25. ... 3'-untranslated region of Cl, isolated from RBL-5, a murine cDNA clone27. C2U is a 2.5-kb Sstl/Sstl fragment from the cosmid clone 2.3W718 which ...

Y. Yanagi; N. Caccia; M. Kronenberg; B. Chin; J. Roder; D. Rohel; T. Kiyohara; R. Lauzon; B. Toyonaga; K. Rosenthal; G. Dennert; H. Acha-Orbea; H. Hengartner; L. Hood; T. W. Mak

1985-04-18T23:59:59.000Z

162

Les rseaux judiciaires en Iraq l'poque abbasside Mathieu Tillier  

E-Print Network [OSTI]

1 Les réseaux judiciaires en Iraq à l'époque abbasside par Mathieu Tillier Parmi les institutions nature et sur leur mode de fonctionnement en Iraq entre le II e /VIII e et le IV e /X e siècle. La ville (Bagdad fut divisée en trois 1 M. Tillier, Les cadis d'Iraq à l'époque abbside : organisation

Paris-Sud XI, Université de

163

L'IDENTIT AU MIROIR DU DROIT LE STATUT DES PERSONNES EN EGYPTE,  

E-Print Network [OSTI]

L'IDENTIT? AU MIROIR DU DROIT LE STATUT DES PERSONNES EN EGYPTE, FIN DU XIXe - MILIEU DU XXe SI?CLE sur les statuts et les identités en Egypte, à l'époque où l'ordre ottoman, fondé sur l'abolition des capitulations (1937), privilèges conférés aux étrangers et devenus insupportables à l'Egypte

Paris-Sud XI, Université de

164

CARBON7510.pdf  

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

Author's personal copy Author's personal copy NMR a critical tool to study the production of carbon fiber from lignin Marcus Foston a , Grady A. Nunnery b , Xianzhi Meng a , Qining Sun a , Frederick S. Baker b , Arthur Ragauskas a, * a BioEnergy Science Center, School of Chemistry and Biochemistry, Institute of Paper Science and Technology, Georgia Institute of Technology, 500 10th St., Atlanta, GA 30332, United States b Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831-6087, United States A R T I C L E I N F O Article history: Received 7 April 2012 Accepted 6 September 2012 Available online 14 September 2012 A B S T R A C T The structural changes occurring to hardwood Alcell TM lignin as a result of fiber devolatiliza- tion/extrusion, oxidative thermo-stabilization and carbonization are investigated in this study by solid-state and solution nuclear magnetic resonance

165

Invariance of the Dissipative Action at Ultrahigh Strain Rates Above the Strong Shock Threshold  

Science Journals Connector (OSTI)

We have directly resolved shock structures in pure aluminum in the first few hundred picoseconds subsequent to a dynamic load at peak stresses up to 43GPa and strain rates in excess of 1010??s-1. For strong shocks we obtain peak stresses, strain rates, and rise times. From these data, we directly validate the invariance of the dissipative action in the strong shock regime, and by comparing with data obtained at much lower strain rates show that this invariance is observed over at least 5 orders of magnitude in the strain rate. Over the same range, we similarly validate the fourth-power scaling of the strain rate with the peak stress (the Swegle-Grady relation).

Jonathan C. Crowhurst; Michael R. Armstrong; Kimberly B. Knight; Joseph M. Zaug; Elaine M. Behymer

2011-09-30T23:59:59.000Z

166

Journal of Undergraduate Research, Spring 2012  

E-Print Network [OSTI]

the use of DNA Sequences for Species Identification in Medusozoans (Phylum Cnidaria) 72 Rhea Richardson (Faculty Advisor: Paulyn Cartwright, Ecology and Evolutionary Biology] A New Stabilization Approach to Cadaveric Shoulder Joint Testing 84 Cole... : s of the G l o b a l i z a t i o : of C l i : i c a l Research ." New England Journal of Medicine 36O.8 (2OO9): 8 1 6 - 2 3 . 2 Ezekiel E = a : u e l ; D a v i d W e : d l e r ; a : d C h r i s t i : e Grady. " W h a t M a k e s C l i : i c a l R e s e a...

2012-04-01T23:59:59.000Z

167

A review of "The Ends of Life: Roads to Fulfilment in Early Modern England" by Keith Thomas  

E-Print Network [OSTI]

reviews 59 future of the humanities in general and seventeenth-century studies in particular, H?fer?s study reaffirms the centrality of the grand si?cle through a timely return to a larger concept of the humanities, before that other... of Life: Roads to Fulfilment in Early Modern England. Oxford and New York: Oxford University Press, 2009. xvi + 393 pp. + 14 illus. $60.00. Review by catherine patterson, university of houston In this wide-ranging and engaging book, Keith Thomas brings...

Patterson, Catherine

2010-01-01T23:59:59.000Z

168

A flexible location management scheme for mobile computing  

E-Print Network [OSTI]

&rib?ted Database Manage- ment. System (DDBMS) is the clevelopirient, p)atlo& m, and we are using Proc"'C with el&lbeddi (I SQL. Though t, he two Viv&IX workstation& are accessing thi. san&e ORA- CLE server at SparcServer l000, they are using indcpen&leut dat, a..., objects. In fact, , these data objects can he distributed among s&vcral network hosts usiug OKACLE SQL NET ivithoiit any modihcation of the codes foi thc location operations. The Chent (UltraSparc: dasher) Client (UltraSparc: dancer) ORACLE Server...

Zhang, Ying

1996-01-01T23:59:59.000Z

169

The Sherman Anti-Trust Law: in its Relation to the Economic Welfare of The United Stats  

E-Print Network [OSTI]

the Ameri can Sugar Refining Co., a trust controlling most of the sugar refineries in the Uni te d' state B, whi ch purchased stock in four Phila- (a) In re Greene, 52 Fed . 104. (b') . 156 U. s. 1. -6- delphia refineries and attained a practical... commodi ties whi ch are produced under competi ti ve condi tions. (a) The 1 i st 8 of t he arti cle s whi ch he has se Ie cte d a re as :fo llow s: (b) TRUST .6..n thrac i te co al Ame rican cement Refined petroleum Cot'tlon-seed oil Gluco se...

Schnake, Francis Dean

1912-05-15T23:59:59.000Z

170

A LA CROISEE DES VOIES CELESTES FAXR AL-DIN `ERAQI  

E-Print Network [OSTI]

, métaphysicien et maître spirituel, ,,Erâqi est un auteur mystique persan du XIIIe siècle à la pensée riche en exemplaires, et représentatives de toute la poésie classique persane. Peu détudes analytiques ont été jusquici consacrées à loeuvre et à la pensée des poètes mystiques persans. Le soufisme classique et le soufisme

Paris-Sud XI, Université de

171

A review of "Mastering Memory: Salons, History, and the Creation of Seventeenth-Century France." by Faith E. Beasley  

E-Print Network [OSTI]

as arbiters of taste, such as the women Corneille unashamedly sought to please in Le Cid, but also as writers, as Madame de Lafayette famously did with La Princesse de Cl?ves. Beasley also offers intriguing readings of Lafayette?s Za?de and Villedieu?s D... the salons, and in which only two exceptional women writers (Lafayette and S?vign?) can be found to have existed in seventeenth-century France. The fourth chapter, ?Disseminating a National Past: Teaching Le Grand Si?cle,? illustrates the depressing extent...

OHara, Stephanie

2007-01-01T23:59:59.000Z

172

Sundry Brief Articles, Compiled from Press Notes Published During the Years 1894 and 1895. Index.  

E-Print Network [OSTI]

to force horse stock to eat cotton seed meal in any form or combination. Should you not be able to bring your colts to eat tile cotton seed meal here suggested, it will be necessary to increase the amonnt of bran or ship stuff to 20 pounds. A good grain... mentioned. "Nu tritive ratio" i a measure of tile total fattening or lean producing tend- ney of the foo 1. If tlle figures read 1 to 7 or 8, this is fattening, while if th y r ad from 1 to 2 or 3, tlle general tendency of the food is to Ue. ?ll (mu cle...

Connell, J. H.; Harrington, H. H.; Francsis, M.; Price, R. H.; Clayton, James

1895-01-01T23:59:59.000Z

173

Thtres de Perse et d'Iran : aperu gnral ve FEUILLEBOIS-PIERUNEK  

E-Print Network [OSTI]

1 Théâtres de Perse et d'Iran : aperçu général ?ve FEUILLEBOIS-PIERUNEK Sorbonne Nouvelle ­ Paris 3, UMR 7528 « Mondes iranien et indien » L'Iran possède à la fois un théâtre rituel encore très vivace siècle, ne doit rien à l'Occident. La question de l'existence d'un théâtre indigène en Iran s

Paris-Sud XI, Université de

174

Making Use of Low-Level Heat  

E-Print Network [OSTI]

to discuss today ~s This method is based on the organic Rankine c~cle power, either electrical or mechanical power. using a suitable working fluid in a closed loop. . 11 t pressure, adds heat ito To refresh your memory, the Rankine cycle pumps liquid... electric power, by the organic Rankine cycle mechanism. A~I I Energy Systems is a company set up by Allied Chemical and Ishikawajima-Harima Heavy Industri~s i Co. of Japan to design and sell the IHI System, operating mainly with freon fluids. i i f I...

Plaster, W. E.

1979-01-01T23:59:59.000Z

175

The crystalliquid interface of a body?centered?cubic?forming substance: Computer simulations of the r ? 6 potential  

E-Print Network [OSTI]

(the bulk density change).27 For the (100) interface this 10--90 width is measured to be about 5.7a (just over 8 lattice planes). The variation of the diffusion constant through the in terface was calculated by dividing the z direction into 30 bins..., and were found not to differ measurably. The limiting liquid value of D (0.011 59 0.000 01) was obtained in a separate 686 parti cle simulation of the bulk liquid. Note that bulk liquid diffu sion constants are known to be somewhat system size depen...

Laird, Brian Bostian; Haymet, A. D. J.

1989-09-01T23:59:59.000Z

176

Rings and Jets around PSR J2021+3651: the `Dragonfly Nebula'  

E-Print Network [OSTI]

We describe recent Chandra ACIS observations of the Vela-like pulsar PSR J2021+3651 and its pulsar wind nebula (PWN). This `Dragonfly Nebula' displays an axisymmetric morphology, with bright inner jets, a double-ridged inner nebula, and a ~30" polar jet. The PWN is embedded in faint diffuse emission: a bow shock-like structure with standoff ~1' brackets the pulsar to the east and emission trails off westward for 3-4'. Thermal (kT=0.16 +/-0.02 keV) and power law emission are detected from the pulsar. The nebular X-rays show spectral steepening from Gamma=1.5 in the equatorial torus to Gamma=1.9 in the outer nebula, suggesting synchrotron burn-off. A fit to the `Dragonfly' structure suggests a large (86 +/-1 degree) inclination with a double equatorial torus. Vela is currently the only other PWN showing such double structure. The >12 kpc distance implied by the pulsar dispersion measure is not supported by the X-ray data; spectral, scale and efficiency arguments suggest a more modest 3-4 kpc.

Adam Van Etten; Roger W. Romani; C. -Y. Ng

2008-02-25T23:59:59.000Z

177

The electronic structure and positron annihilation characteristics of positronium halides, [X?; e +]. I. HartreeFock calculations and stability  

Science Journals Connector (OSTI)

The electronic structure of the atom/positron systems [F?;e +] [Cl?;e +] [Br?;e +] and [I?;e +] are examined by means of restricted HartreeFock calculations on the ...n s 2 n p 6(n l)+ 2 L and...n s 2 n p 5 (n+1) s l s + 2 P 4 P states. A modified version of the numerical MCHF72 program of FroeseFischer was used in these calculations. Our theoretical investigations suggest that...n s 2 n p 61s + 2 S is the ground state of the system. It is shown that X? ions have a substantial positron affinity (e.g. ?5 eV for F? to 3.3 eV for I?) and arguments based on pair?correlation and many?electron perturbation theory are used to obtain hard lower limit estimates of the binding energy of Ps to the X atom. We thus find that the ground state of [X?:e +] is stable with respect to dissociation into X and Ps with binding energies of at l e a s t 1.66 0.80 0.19 and ?0.45 eV for [F?:e +] [Cl?:e +] [Br?:e +] and [I?:e +] respectively. The details of the positronic orbitals are presented and discussed.

Paul E. Cade; Abbas Farazdel

1977-01-01T23:59:59.000Z

178

Issuance Date:: February  

Office of Legacy Management (LM)

Issuance Issuance Date:: February 11, 1966 POST-SHOT HYDROLOGI C SAFETY 68296 VUF-1014 FINAL REPORT FALLON, NEVADA OCTOBER 26, 1963 Hazleton-Nuclear Science Corporation October 30, 1965 SPONSORED BY THE ADVANCED RESEARCH PROJECTS AGENCY OF THE DEPARTMENT OF DEFENSE AND THE U. S.ATOMIC ENERGY COMMISSION VELA UNIFORM PROJECT LEG A L NOTICE This report was prepared as an account of Government sponsored work. Neither the United States, nor the Commission, nor any person acting on behalf of the Commission: A. Makes any warranty or representation, expressed or implied, with respect to the accu- racy, completeness, or usefulness of the information contained in this report, or that the use of any information. apparatus, method, or process disclosed in this report may not infringe privately owned rights; or B. Assumes any liabilities with respect to the use of, or for damages resulting from the

179

shoal.cdr  

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

Shoal, Shoal, Nevada, Site F A C T S H E E T This fact sheet provides information about the Shoal, Nevada, Site. This site is managed by the U.S. Department of Energy Office of Legacy Management. Shoal, Nevada, Site Site Description and History 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

180

Broad-band Spectral Properties of Accreting X-ray Binary Pulsars  

E-Print Network [OSTI]

Broad-band spectra of accreting X-ray binary pulsars can be fit by a phenomenological model composed by a power law with a high energy rollover above 10 keV, plus a blackbody component with a temperature of few hundred eV. While, at least qualitatively, the hard tail can be explained in terms of (inverse) Compton scattering, the origin of the soft component cannot find a unique explanation. Recently a qualitative picture able to explain the overall broad band-spectrum of luminous X-ray pulsars was carried out by taking into account the effect of bulk Comptonization in the accretion column. After a review on these recent theoretical developments, I will present a case study of how different modelization of the continuum affect broad features, in particular the cyclotron resonance features in Vela X-1.

Mauro Orlandini

2005-10-10T23:59:59.000Z

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


181

Modified Finch and Skea stellar model compatible with observational data  

E-Print Network [OSTI]

We present a new class of solutions to the Einstein's field equations corresponding to a static spherically symmetric anisotropic system by generalizing the ansatz of Finch and Skea [Class. Quantum Grav. 6 (1989) 467] for the gravitational potential $g_{rr}$. The anisotropic stellar model previously studied by Sharma and Ratanpal (2013) [Int. J. Mod. Phy. D 13 (2013) 1350074] is a sub-class of the solutions provided here. Based on physical requirements, regularity conditions and stability, we prescribe bounds on the model parameters. By systematically fixing values of the model parameters within the prescribed bound, we demonstrate that our model is compatible with the observed masses and radii of a wide variety of compact stars like 4U 1820-30, PSR J1903+327, 4U 1608-52, Vela X-1, PSR J1614-2230, SAX J1808.4-3658 and Her X-1.

Pandya, D M; Sharma, R

2014-01-01T23:59:59.000Z

182

Category:Cleveland, OH | Open Energy Information  

Open Energy Info (EERE)

Cleveland, OH Cleveland, OH Jump to: navigation, search Go Back to PV Economics By Location Media in category "Cleveland, OH" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Cleveland OH Ohio Power Co.png SVFullServiceRestauran... 69 KB SVHospital Cleveland OH Ohio Power Co.png SVHospital Cleveland O... 60 KB SVLargeHotel Cleveland OH Ohio Power Co.png SVLargeHotel Cleveland... 61 KB SVLargeOffice Cleveland OH Ohio Power Co.png SVLargeOffice Clevelan... 59 KB SVMediumOffice Cleveland OH Ohio Power Co.png SVMediumOffice Clevela... 67 KB SVMidriseApartment Cleveland OH Ohio Power Co.png SVMidriseApartment Cle... 69 KB SVOutPatient Cleveland OH Ohio Power Co.png SVOutPatient Cleveland... 68 KB SVPrimarySchool Cleveland OH Ohio Power Co.png

183

European Wind Atlas: France | Open Energy Information  

Open Energy Info (EERE)

European Wind Atlas: France European Wind Atlas: France Jump to: navigation, search Tool Summary LAUNCH TOOL Name: European Wind Atlas: France Focus Area: Renewable Energy Topics: Potentials & Scenarios Website: 130.226.17.201/extra/web_docs/windmaps/france.jpg Equivalent URI: cleanenergysolutions.org/content/european-wind-atlas-france,http://cle Language: English Policies: Deployment Programs DeploymentPrograms: Technical Assistance This wind resource map shows resources at 50 meters above ground level for four different topographic conditions, including sheltered terrain, open plain, coastal and hills and ridges. The greatest resources appear to be near the Mediterranean Sea coast, and the second greatest resources are near the English Channel and northern Atlantic coast.

184

BETWEEN RANDALL COUNTY, TEXAS AND 'I'HE UNITED STATES DEPARTMENT OF ENEKGY  

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

BETWEEN BETWEEN RANDALL COUNTY, TEXAS AND - 'I'HE UNITED STATES DEPARTMENT OF ENEKGY This Memorandum of Understanding (hereinslfier callcd "MOU") is between Randall County. Texas, (hereinaner callcd "Cnunty") and thc Uni~ed States Department of Energy: (hcrcinafter called "I3ClE'' or b'l'an?ex"). 1. INTRODUCTION A. BACKGKOUN L) Both prties havc a mutual interest and responsibility for fire fighting activities tu protect penplc, propxty. and the cnvimnmcnt. B. fl RPOSE 'Ihe purpose of this Mot' is to recognize the need Tor coopemtion on certain fire lighting responsibilities of mutuaI conccrn and to provide for the mutual assistance of parties in accordance \hi tith thc Standard Opemting Pmedures (SOP) contained in Appendix A of this

185

 

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

ftn ftn [-A module_name[, module_name] ...] [-b bin_obj_file] [-c] [-d disable] [-D identifier[=value]] [-e enable] [-f source_form] [-F] [-g] [-G debug_lvl] [-h arg] [-I incldir] [-J dir_name] [-K trap=opt[, opt] ...] [-l libname] [-L ldir] [-m msg_lvl] [-M msgs] [-N col] [-o out_file] [-O opt[, opt] ...] [-p module_site [,module_site ...]] [-Q path] [-r list_opt] [-R runchk] [-s size] [-S] [-T] [-U identifier[, identifier] ...] [-v] [-V] [-Wphase,"opt...",] [-x dirlist] [-X npes] [-Yphase,dirname] [--] sourcefile [sourcefile ...] IMPLEMENTATION Cray Linux Environment (CLE) DESCRIPTION The ftn command invokes the Cray Fortran Compiler. Typically, the command processes the input files named on the command line and generates a binary object file, and then loads the binary object file

186

Cray XC30 User Documentation  

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

Cray XC30 Cray XC30 Documentation Cray XC30 User Documentation L Cray XC30 Documentation Search Preferences | Advanced Search Home Browse Books Man Pages Glossary Platforms Cray XC30 Cray XE and Cray XK Cray XT Cray Sonexion Cray X2 Cray X1 Knowledge Base by Category by Date by Platform by Title by User Release Announcements @Twitter Cray XC30 System Documentation This site map also contains legacy documentation. Always consult the latest version of documentation for your site-specific configuration and ask your Cray Customer Service representative for additional guidance on the latest software documents. Getting Started Cray Linux Environment (CLE) Software Release Overview Programming Environment Cray Programming Environments User Guide Cray Compiling Environment (CCE) Cray Fortran Reference Manual

187

Appendix B: CArBon dioxide CApture teChnology SheetS  

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

sorbents sorbents B-14 Pre-Combustion sorbents u.s. DePartment of energy aDvanCeD Carbon DioxiDe CaPture r&D Program: teChnology uPDate, may 2013 aDvanCeD Carbon DioxiDe CaPture teChnology for low-rank Coal integrateD gasifiCation CombineD CyCle (igCC) systems primary project goals TDA will investigate the technical and economic advantages of using an integrated carbon dioxide (CO 2 ) sorbent and water-gas shift (WGS) catalyst system in an integrated gasifi- cation combined cycle (IGCC) power plant, fueled with low-rank coal, and designed to capture more than 90% of the CO 2 emissions. technical goals * TDA will evaluate the physical mix of the sorbent and catalyst pellets within the same

188

Improved  

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

Improved Improved cache performance in Monte Carlo transport calculations using energy banding A. Siegel a , K. Smith b , K. Felker c,∗ , P . Romano b , B. Forget b , P . Beckman c a Argonne National Laboratory, Theory and Computing Sciences and Nuclear Engineering Division b Massachusetts Institute of Technology, Department of Nuclear Science and Engineering c Argonne National Laboratory, Theory and Computing Sciences Abstract We present an energy banding algorithm for Monte Carlo (MC) neutral parti- cle transport simulations which depend on large cross section lookup tables. In MC codes, read-only cross section data tables are accessed frequently, ex- hibit poor locality, and are typically much too large to fit in fast memory. Thus, performance is often limited by long latencies to RAM, or by off-node communication latencies when the data footprint is very large and must be decomposed on

189

C:\ANNUAL\VENTCHAP.V8\NewNGA02.vp  

Gasoline and Diesel Fuel Update (EIA)

1 1 Glossary Aquifer Storage Field: A sub-surface facility for storing nat- ural gas consisting of water-bearing sands topped by an imper- meable cap rock. Balancing Item: Represents differences between the sum of the components of natural gas supply and the sum of the com- ponents of natural gas disposition. These differences may be due to quantities lost or to the effects of data-reporting prob- lems. Reporting problems include differences due to the net result of conversions of flow data metered at varying tempera- ture and pressure bases and converted to a standard tempera- ture and pressure base; the effect of variations in company ac- counting and billing practices; differences between billing cy- cle and calendar period time frames; and imbalances resulting from the merger of data-reporting systems that vary in scope, format, definitions, and type of respondents. Biomass

190

 

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

cc 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 9899:1999 and to the American National Standards Institute (ANSI) X3.159-1989 standards. Typically, the cc command processes the source files named on the command line, generates a binary object file (sourcefile.o), links the binary object file, and generates an executable file (named a.out by default). Other files used and created by the C compiler are discussed under the FILES section.

191

Supplement Analysis for Yakima/Klickitat Fisheries Project, (DOE/EIS-0169-SA-05) 9/20/02  

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

September 20, 2002 September 20, 2002 REPLY TO ATTN OF: KEC-4 SUBJECT: Supplement Analysis for Yakima/Klickitat Fisheries Project, (DOE/EIS-0169-SA-05) memorandum David Byrnes Project Manager - KEWL-4 TO: Proposed Action: Yakima/Klickitat Fisheries Project - Under the Monitoring and Evaluation Program (M&E), the domestication selection research task would be modified to include a hatchery control line, maintained entirely by spawning hatchery-origin fish. Project No.: F3204 Location: Cle Elum, Kittitas County, Washington. Proposed by: Bonneville Power Administration (BPA) and Co-Managed by the Yakama Nation (YN) and the Washington Department of Fish and Wildlife (WDFW). 1. Introduction The Bonneville Power Administration is funding ongoing studies, research, and artificial production of

192

Cray XC30 User Documentation  

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

Documentation Documentation Cray XC30 User Documentation L Cray XC30 Documentation Search Preferences | Advanced Search Home Browse Books Man Pages Glossary Platforms Cray XC30 Cray XE and Cray XK Cray XT Cray Sonexion Cray X2 Cray X1 Knowledge Base by Category by Date by Platform by Title by User Release Announcements @Twitter Cray XC30 System Documentation This site map also contains legacy documentation. Always consult the latest version of documentation for your site-specific configuration and ask your Cray Customer Service representative for additional guidance on the latest software documents. Getting Started Cray Linux Environment (CLE) Software Release Overview Programming Environment Cray Programming Environments User Guide Cray Compiling Environment (CCE) Cray Fortran Reference Manual

193

Page not found | Department of Energy  

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

81 - 19890 of 28,905 results. 81 - 19890 of 28,905 results. Download CX-006586: Categorical Exclusion Determination Integration of G0387 Energetics Solar Integration Project CX(s) Applied: B1.7, B4.6 Date: 09/01/2011 Location(s): Lake County, Oregon Office(s): Bonneville Power Administration http://energy.gov/nepa/downloads/cx-006586-categorical-exclusion-determination Download CX-006312: Categorical Exclusion Determination Small-Scale Spring Chinook and Coho Reintroduction CX(s) Applied: B1.20 Date: 07/21/2011 Location(s): Cle Elum, Washington Office(s): Bonneville Power Administration http://energy.gov/nepa/downloads/cx-006312-categorical-exclusion-determination Download CX-000007: Categorical Exclusion Determination Spirit Tap to Colville-Boundary #1 Landings and Access Roads Construction

194

C:\Annual\VENTCHAP.V8\NGA02.vp  

Gasoline and Diesel Fuel Update (EIA)

0 0 Energy Information Administration / Natural Gas Annual 2002 Glossary Aquifer Storage Field: A sub-surface facility for storing nat- ural gas consisting of water-bearing sands topped by an imper- meable cap rock. Balancing Item: Represents differences between the sum of the components of natural gas supply and the sum of the com- ponents of natural gas disposition. These differences may be due to quantities lost or to the effects of data-reporting prob- lems. Reporting problems include differences due to the net result of conversions of flow data metered at varying tempera- ture and pressure bases and converted to a standard tempera- ture and pressure base; the effect of variations in company ac- counting and billing practices; differences between billing cy- cle and calendar period time frames; and imbalances resulting from the merger of data-reporting systems that vary in scope,

195

A Comparison  

Gasoline and Diesel Fuel Update (EIA)

Theresa Theresa E. Hallquist Introduction The Petroleum Division (PD) of the Energy Informa- tion Administration (EIA) collects information relating to petroleum market prices and volumes on the EIA-782 survey. One way PD assesses the quality of these data is to compare the data with other sources. Large, irreconcilable differences among data series could indicate the need for improvement in survey de- sign or implementation, or may be due to conceptual differences. For more detailed information on the EIA-782 survey, refer to the notes at the end of this arti- cle. PD compares its EIA-782 series of petroleum market prices and volumes with both internal and external data sources on an ongoing basis. The sources include: * The Bureau of Labor Statistics (BLS) Consumer Price Index (CPI) data for retail prices of motor gasoline and No. 2 fuel oil * Form EIA-821, "Annual Fuel Oil and Kerosene

196

Washington | Department of Energy  

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

August 2, 2004 August 2, 2004 EIS-0349: Final Environmental Impact Statement, Volume 2 BP Cherry Point Cogeneration Project Volume 2 August 2, 2004 EIS-0349: Final Environmental Impact Statement, Figures BP Cherry Point Cogeneration Project August 2, 2004 EIS-0349: Final Environmental Impact Statement, Appendices BP Cherry Point Cogeneration Project June 23, 2004 EIS-0026-SA-02: Supplement Analysis Disposal of Polychlorinated Biphenyl-Commingled Transuranic Waste at the Waste Isolation Pilot Plant April 7, 2004 EIS-0169-SA-08: Supplement Analysis Yakima/Klickitat Fisheries Project, Boone Pond Acclimation Site, Cle Elum, Kittitas County, Washington March 12, 2004 EA-1486: Final Environmental Assessment East and West Diversion Screening Proposal Methow Valley Irrigation District Project

197

Wind Resource Atlas of Oaxaca | Open Energy Information  

Open Energy Info (EERE)

Resource Atlas of Oaxaca Resource Atlas of Oaxaca Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Wind Resource Atlas of Oaxaca Focus Area: Renewable Energy Topics: Potentials & Scenarios Website: www.nrel.gov/wind/pdfs/34519.pdf Equivalent URI: cleanenergysolutions.org/content/wind-resource-atlas-oaxaca,http://cle Language: English Policies: Deployment Programs DeploymentPrograms: Technical Assistance This wind resource atlas identifies wind characteristics and distribution of wind resources in Oaxaca, Mexico, at a wind power density of 50 meters above ground. The detailed wind resource maps contained in the atlas facilitate the identification of prospective areas for use of wind energy technologies for utility-scale power generation, village power, and off-grid wind energy applications. The wind maps were created using a

198

PowerPoint Presentation  

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

and Performance Impacts from 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 most NERSC users from modest to extreme concurrencies. * Expects significant percentage of time to be used for capability jobs on Franklin. 3 Kernel Benchmarks * Processor: NAS Parallel Benchmarks (NPB) - Serial: NPB 2.3 Class B * best understood code base - Parallel: NPB 2.4 Class D at 64 and 256 ways

199

Page not found | Department of Energy  

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

61 - 8870 of 26,764 results. 61 - 8870 of 26,764 results. Download Electricity Advisory Committee Meeting, March 5-6, 2012- Meeting Minutes and Transcripts Meeting minutes and transcripts for the March 5-6, 2012 meeting of the Electricity Advisory Committee. http://energy.gov/oe/downloads/electricity-advisory-committee-meeting-march-5-6-2012-meeting-minutes-and-transcripts Download Transmission Planning: Institutional Issues in the West http://energy.gov/oe/downloads/transmission-planning-institutional-issues-west Download EIS-0169-SA-05: Supplement Analysis Yakima/Klickitat Fisheries Project, Cle Elum, Kittitas County, Washington http://energy.gov/nepa/downloads/eis-0169-sa-05-supplement-analysis Download Hydride Rim Formation in Unirradiated Zircaloy The purpose of this work is to develop the means of pre-hydriding

200

Aprun MAN Page  

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

aprun » Aprun MAN Page 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 Application Level Placement Scheduler (ALPS) aprun command. The aprun command specifies application resource requirements, requests application placement, and initiates application launch. The aprun utility provides user identity and environment information as part of the application launch so that your login node session can

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201

Karl Haushofer and his impact on the German-Japanese Alliance  

E-Print Network [OSTI]

&del'au&rents in Jr&pan and Germany ol' impeniili?tic expan?ion, anti-communism, riibid nation;ilism, and the drive toward technological ?upcnority formed the bii?i? I'or thi? coalition. The?ecd? ol thi? Geiman-Japanese alliance began hesitantly;is carly;is 1880... and lasted ?& the finiil days of ?Vorld &Vi&r Il. It is cle;&r thai Hausholcr ?;&s in?trumental in developing Germany's alliance ?&th hi? heli&&ed J;ip;in. ?hich hc sa&v as Germany'? brothe&' n i&i&in. Ih? interest evolved into a lil'elong p;ission. He...

Hayes, Tracey Michelle

2004-01-01T23:59:59.000Z

202

1995 Reformulated Gasoline Market Affected Refiners Differently  

Gasoline and Diesel Fuel Update (EIA)

5 Reformulated Gasoline Market Affected 5 Reformulated Gasoline Market Affected Refiners Differently by John Zyren, Charles Dale and Charles Riner Introduction The United States has completed its first summer driving season using reformulated gasoline (RFG). Motorists noticed price increases at the retail level, resulting from the increased cost to produce and deliver the product, as well as from the tight sup- ply/demand balance during the summer. This arti- cle focuses on the costs of producing RFG as experienced by different types of refiners and on how these refiners fared this past summer, given the prices for RFG at the refinery gate. RFG Regulatory Requirements The use of RFG is a result of the Clean Air Act Amendments of 1990 (CAAA). The CAAA cover a wide range of programs aimed at improving air qual-

203

CX-003628: Categorical Exclusion Determination | Department of Energy  

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

628: Categorical Exclusion Determination 628: Categorical Exclusion Determination CX-003628: Categorical Exclusion Determination Kittitas County Conservation Easement Acquisition CX(s) Applied: B1.25 Date: 07/12/2010 Location(s): Kittitas County, Washington Office(s): Bonneville Power Administration Bonneville Power Administration (BPA) proposes to fund Washington Department of Fish and Wildlife (WDFW?s) acquisition of a conservation easement on 5 parcels of the Hundley property totaling 432.3 acres near Cle Elum, Washington. The property has outstanding riparian and floodplain natural resource values, which provide an opportunity to enhance, restore, and manage high quality spawning and rearing habitat for Endangered Species Act-listed Mid-Columbia River steelhead (threatened) and Columbia River

204

Microsoft Word - CX-Rocky Reach-Maple Valley No1_WEB.doc  

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

3, 2010 3, 2010 REPLY TO ATTN OF: KEP-4 SUBJECT: Environmental Clearance Memorandum Darin Bowman Project Manager - TELF-TPP-3 Proposed Action: Rocky Reach-Maple Valley No. 1 mile 47 bridge replacement project Budget Information: Work Order # 219783 PP&A Project No.: 955 Proposed by: Bonneville Power Administration (BPA) Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B1.3, Routine maintenance activities for structures, rights-of-way, and infrastructures such as roads that are required to maintain infrastructures in a condition suitable for a facility to be used for its designed purpose. Location: BPA, in coordination with the Cle Elum Ranger District of the Okanogan-Wenatchee National Forest, is proposing to construct a bridge across Cold Creek. The proposed project is

205

Washington | Department of Energy  

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

September 5, 2002 September 5, 2002 EIS-0285-SA-107: Supplement Analysis Transmission System Vegetation Management Program September 2, 2002 EIS-0169-SA-05: Supplement Analysis Yakima/Klickitat Fisheries Project, Cle Elum, Kittitas County, Washington August 30, 2002 EIS-0332: Final Environmental Impact Statement McNary-John Day Transmission Line Project August 29, 2002 EIS-0285-SA-99: Supplement Analysis Transmission System Vegetation Management Program Final Environmental Impact Statement - Olympia-Grand Coulee No.1 August 22, 2002 EIS-0285-SA-105: Supplement Analysis Transmission System Vegetation Management Program August 21, 2002 EIS-0285-SA-104: Supplement Analysis Transmission System Vegetation Management Program August 1, 2002 EIS-0344: Draft Envrionmental Impact Statement

206

Citation: D.E. Groom  

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

± ± I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. B ± MASS B ± MASS B ± MASS B ± MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.4 ±0.4 526 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5279.1±1.7 ±1.4 147 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. * * * 5278.8±0.54 ±2.0 362 ALAM 94 CLE2 e + e - → Υ(4S) 5278.3±0.4 ±2.0 BORTOLETTO92 CLEO e + e - → Υ(4S) 5280.5±1.0 ±2.0 2 ALBRECHT 90J ARG e + e - → Υ(4S) 5275.8±1.3 ±3.0 32 ALBRECHT 87C ARG e + e - → Υ(4S) 5278.2±1.8

207

s041.dvi  

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

± ± I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. B ± MASS B ± MASS B ± MASS B ± MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.13± 0.31 OUR FIT 5279.13± 0.31 OUR FIT 5279.13± 0.31 OUR FIT 5279.13± 0.31 OUR FIT 5279.1 ± 0.4 OUR AVERAGE 5279.1 ± 0.4 OUR AVERAGE 5279.1 ± 0.4 OUR AVERAGE 5279.1 ± 0.4 OUR AVERAGE 5279.10± 0.41 ± 0.36 1 ACOSTA 06 CDF p p at 1.96 TeV 5279.1 ± 0.4 ± 0.4 526 2 CSORNA 00 CLE2 e + e - → Υ(4S) 5279.1 ± 1.7 ± 1.4 147 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. * * * 5278.8 ± 0.54± 2.0 362 ALAM 94 CLE2 e + e - → Υ(4S) 5278.3 ± 0.4 ± 2.0 BORTOLETTO92 CLEO e + e - → Υ(4S) 5280.5 ± 1.0 ± 2.0 3 ALBRECHT 90J ARG e + e - → Υ(4S)

208

s041.dvi  

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

± ± I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. B ± MASS B ± MASS B ± MASS B ± MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.0±0.5 OUR FIT 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.5 OUR AVERAGE 5279.1±0.4 ±0.4 526 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5279.1±1.7 ±1.4 147 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. * * * 5278.8±0.54 ±2.0 362 ALAM 94 CLE2 e + e - → Υ(4S) 5278.3±0.4 ±2.0 BORTOLETTO92 CLEO e + e - → Υ(4S) 5280.5±1.0 ±2.0 2 ALBRECHT 90J ARG e + e - → Υ(4S) 5275.8±1.3 ±3.0 32 ALBRECHT 87C ARG e + e - → Υ(4S) 5278.2±1.8

209

The behaviour of niobium and molybdenum during uni-axial strain loading  

SciTech Connect (OSTI)

The mechanical response of niobium and molybdenum during one dimensional shock loading in the weak shock regime is investigated in terms of the Hugoniot elastic limit (dynamic yield) and spall (tensile) strengths. Results indicate that although both metals have high elastic limits of ca. 2?GPa, their responses are very different. Deformation in the weak shock regime in niobium is controlled by both the motion and generation of dislocations, resulting in high spall (dynamic tensile) strengths and ductility. In contrast, molybdenum has low spall strength and ductility, which suggests lower dislocation mobility in this metal. We have also shown that the strain-rate in the rising part of the shock front is related to the stress amplitude by the fourth power, as first shown by Swegle and Grady. Although we have not been able to elucidate further on the power relation, we believe that the scaling factor A is related to a materials ability to accommodate shock imposed plasticity via slip and dislocation generation. Overall, we have used arguments about the Peierls stress in body centred cubic metals to explain these results, with niobium (low Peierls stress) having a high dislocation mobility, resulting in behaviour showing some similarities to face centred cubic metals. Molybdenum, with its much higher Peierls stress has a much lower dislocation mobility, and hence lower spall strengths and ductility.

Millett, J. C. F.; Cotton, M.; Bourne, N. K.; Park, N. T.; Whiteman, G. [AWE, Aldermaston, Reading RG7 4PR (United Kingdom)

2014-02-21T23:59:59.000Z

210

Simulations of pulsar wind formation  

E-Print Network [OSTI]

We present initial results of the first self-consistent numerical model of the outer magnetosphere of a pulsar. By using the relativistic ``particle-in-cell'' method with special boundary conditions to represent plasma dynamics in 3D, we are able to follow magnetospheric plasma through the light cylinder into the wind zone for arbitrary magnetic inclination angles. For aligned rotators we confirm the ``disk-dome'' charge-separated structure of the magnetosphere and find that this configuration is unstable to a 3D nonaxisymmetric diocotron instability. This instability allows plasma to move across the field lines and approach the corotating Goldreich-Julian solution within several rotation periods. For oblique rotators formation of the spiral ``striped wind'' in the equatorial direction is demonstrated and the acceleration of the wind and its magnetization is discussed. We find that the wind properties vary with stellar latitude; however, whether injection conditions at the pulsar are responsible for the observed jet-equator geometry of Crab and Vela is currently under investigation. We also comment on the electrodynamics of the simulated magnetospheres, their current closure, and future simulations.

Anatoly Spitkovsky; Jonathan Arons

2002-01-22T23:59:59.000Z

211

VHE gamma-ray Emitting Pulsar Wind Nebulae Discovered by H.E.S.S.  

SciTech Connect (OSTI)

Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window on the physics of pulsars. The high sensitivity of current imaging atmospheric Cherenkov telescopes, and in particular of the H.E.S.S. array, has already led to the discovery of about a dozen VHE-emitting pulsar wind nebulae (PWNe) and PWN candidates. These include the plerions in the composite supernova remnants MSH 15-52, G21.5-0.9, Kes 75, and Vela, two sources in the Kookaburra, and the nebula of PSR B1823-13. This VHE emission is generally interpreted as inverse Compton emission from the relativistic electrons and positrons accelerated by the pulsar and its wind; as such, it can yield a more direct spatial and spectral view of the accelerated particles than can be inferred from observations of their synchrotron emission. The VHE-emitting PWNe detected by the H.E.S.S. telescopes are reviewed and the implications for pulsar physics discussed.

Gallant, Y.A.; /Montpellier U.; Carrigan, S.; /Heidelberg, Max Planck Inst.; Djannati-Atai, A.; /APC, Paris; Funk, S.; /KIPAC, Menlo Park; Hinton, J.A.; /Leeds U.; Hoppe, S.; /Heidelberg, Max Planck Inst.; de Jager, O.C.; /Potchefstroom U.; Khelifi, B.; /Ecole Polytechnique; Komin, Nu.; /Montpellier U.; Kosack, K.; /Heidelberg, Max Planck Inst.; Lemiere, A. /APC, Paris; Masterson, C.; /Dublin Inst.

2008-06-05T23:59:59.000Z

212

Pulsar Wind Nebulae with Thick Toroidal Structure  

Science Journals Connector (OSTI)

We investigate a class of pulsar wind nebulae that show synchrotron emission from a thick toroidal structure. The best studied such object is the small radio and X-ray nebula around the Vela pulsar, which can be interpreted as the result of interaction of a mildly supersonic inward flow with the recent pulsar wind. Such a flow near the center of a supernova remnant can be produced in a transient phase when the reverse shock reaches the center of the remnant. Other nebulae with a thick toroidal structure are G106.6+2.9 and G76.9+1.0. Their structure contrasts with young pulsar nebulae like the Crab Nebula and 3C 38, which show a more chaotic, filamentary structure in the synchrotron emission. In both situations, a torus-jet structure is present where the pulsar wind passes through a termination shock, indicating the flow is initially toroidal. We suggest that the difference is due to the Rayleigh-Taylor instability that operates when the outer boundary of the nebula is accelerating into freely expanding supernova ejecta. The instability gives rise to mixing in the Crab and related objects, but is not present in the nebulae with thick toroidal regions.

Roger A. Chevalier; Stephen P. Reynolds

2011-01-01T23:59:59.000Z

213

The Physics of Wind-Fed Accretion  

E-Print Network [OSTI]

We provide a brief review of the physical processes behind the radiative driving of the winds of OB stars and the Bondi-Hoyle-Lyttleton capture and accretion of a fraction of the stellar wind by a compact object, typically a neutron star, in detached high-mass X-ray binaries (HMXBs). In addition, we describe a program to develop global models of the radiatively-driven photoionized winds and accretion flows of HMXBs, with particular attention to the prototypical system Vela X-1. The models combine XSTAR photoionization calculations, HULLAC emission models appropriate to X-ray photoionized plasmas, improved models of the radiative driving of photoionized winds, FLASH time-dependent adaptive-mesh hydrodynamics calculations, and Monte Carlo radiation transport. We present two- and three-dimensional maps of the density, temperature, velocity, ionization parameter, and emissivity distributions of representative X-ray emission lines, as well as synthetic global Monte Carlo X-ray spectra. Such models help to better constrain the properties of the winds of HMXBs, which bear on such fundamental questions as the long-term evolution of these binaries and the chemical enrichment of the interstellar medium.

Christopher W. Mauche; Duane A. Liedahl; Shizuka Akiyama; Tomasz Plewa

2008-06-05T23:59:59.000Z

214

The Most Likely Sources of High Energy Cosmic-Ray Electrons in Supernova Remnants  

E-Print Network [OSTI]

Evidences of non-thermal X-ray emission and TeV gamma-rays from the supernova remnants (SNRs) has strengthened the hypothesis that primary Galactic cosmic-ray electrons are accelerated in SNRs. High energy electrons lose energy via synchrotron and inverse Compton processes during propagation in the Galaxy. Due to these radiative losses, TeV electrons liberated from SNRs at distances larger than ~1 kpc, or times older than ~10^5 yr, cannot reach the solar system. We investigated the cosmic-ray electron spectrum observed in the solar system using an analytical method, and considered several candidate sources among nearby SNRs which may contribute to the high energy electron flux. Especially, we discuss the effects for the release time from SNRs after the explosion, as well as the deviation of a source spectrum from a simple power-law. From this calculation, we found that some nearby sources such as the Vela, Cygnus Loop, or Monogem could leave unique signatures in the form of identifiable structure in the energ...

Kobayashi, T; Yoshida, K; Nishimura, J

2004-01-01T23:59:59.000Z

215

High-energy emission from the stellar wind collisions in gamma-2 Velorum  

E-Print Network [OSTI]

The binary system gamma-2 Velorum (WC8+O7.5) contains the nearest known Wolf-Rayet star to the Sun, at a distance of 258$_{-31}^{+41}$ pc. Its strong radio emission shows evidence for a partially absorbed nonthermal component, which has been interpreted as synchrotron emission from electrons accelerated in the colliding wind region. Inverse Compton cooling of these electrons in the intense UV radiation field from the O-type companion star could produce a significant hard X-ray and gamma-ray emission, whose flux depends on the ratio of the energy densities of magnetic to seed photon fields. The Vela region was observed with the INTEGRAL satellite in 2003, as part of the Core Programme. No signals from gamma-2 Vel are detected in the images obtained with the IBIS/ISGRI coded aperture instrument in the energy ranges 20-40 and 40-80 keV. From the derived 3$\\sigma$ upper limits, we show that the average magnetic field near the region of stellar wind collision should be relatively high, greater than about 1 G. The ...

Tatischeff, V; Lebrun, F

2004-01-01T23:59:59.000Z

216

Implications of the X-Ray Properties of Pulsar Nebulae  

E-Print Network [OSTI]

A plausible model for the Crab Nebula is one in which a particle dominated, highly relativistic wind from the pulsar passes through a shock front in which the particles attain a power law energy distribution. The electrons and positrons lose energy radiating synchrotron emission. Here, a one zone version of the model is developed and applied to observations of X-ray pulsar nebulae. Efficient conversion of pulsar spin-down power to X-ray luminosity is expected if the observed electrons are in the synchrotron cooling regime and their energy spectrum is similar to that in the Crab Nebula. In this case, the relation between X-ray luminosity and pulsar spin-down power depends only weakly on the model parameters. The dependence is stronger for a steeper particle spectrum, as appears to be present in N157B, and the efficiency of X-ray production can be lower. If the electrons are not in the cooling regime, the X-ray luminosity can be low, as appears to be the case for the compact nebula around the Vela pulsar. Slow cooling is likely to be caused by a sub-equipartition magnetic field in the radiating region. Observations can place constraints on the uncertain physics of relativistic MHD shocks. The model is related to those developed for gamma-ray burst afterglows.

Roger A. Chevalier

2000-06-01T23:59:59.000Z

217

Workshop2011Final.pptx  

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

Challenges Challenges a nd A pplica/on G ems on t he P ath t o Exascale Alice K oniges, N ERSC, B erkeley L ab ASCR P rogramming C hallenges W orkshop July 2 011 Path to E xascale: some examples, their discovered "gems," and implica/ons for programming models * GTS - m agne+c f usion p ar+cle---in---cell ( PIC) c ode - Already o p+mized a nd h ybrid ( MPI + O penMP) - Consider a dvanced h ybrid t echniques a nd P GAS * GPU S creening o f C arbon C apture M aterials - Op+miza+on f or G PU * PIR3D T hree---dimensional F low S olver - Hybridiza+on v ia e xpert + a pplica+on s cien+st * NBP's N AS P arallel B enchmarks i n v arious l anguages - Comparison o f M PI, H ybrid, a nd U PC * fvCAM C limate B enchmark - Hybrid f or r educing m emory * S3D - T urbulent C ombus+on - Hybridiza+on f or h eterogeneous p rocessors

218

Citation: W.-M. Yao  

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

(1450) (1450) I G (J PC ) = 1 + (1 - - ) See our mini-review under the ρ(1700). ρ(1450) MASS ρ(1450) MASS ρ(1450) MASS ρ(1450) MASS VALUE (MeV) DOCUMENT ID 1459 ± 11 OUR AVERAGE 1459 ± 11 OUR AVERAGE 1459 ± 11 OUR AVERAGE 1459 ± 11 OUR AVERAGE Includes data from the 3 datablocks that follow this one. Er- ror includes scale factor of 3.4. See the ideogram below. WEIGHTED AVERAGE 1459±11 (Error scaled by 3.4) FUKUI 88 SPEC 1.7 ANTONELLI 88 DM2 0.3 AKHMETSHIN 00D CMD2 6.5 AKHMETSHIN 01B CMD2 7.3 CLEGG 94 RVUE 0.0 EDWARDS 00A CLE2 40.7 AKHMETSHIN 03B CMD2 16.5 ARMSTRONG 89E OMEG 6.5 ACHASOV 97 RVUE 4.8 ABELE 01B CBAR 0.4 χ 2 84.7 (Confidence Level 0.001) 1350 1400 1450 1500 1550 1600 1650 1700 ρ(1450) mass (MeV) η ρ 0 MODE η ρ 0 MODE η ρ 0 MODE η ρ 0 MODE VALUE (MeV) DOCUMENT ID TECN COMMENT The data in this block is included in the average printed for a previous datablock. 1497 ± 14 1 AKHMETSHIN

219

Complexation of mercury by dissolved organic matter in surface waters of Galveston Bay, Texas  

Science Journals Connector (OSTI)

The chemical speciation of dissolved mercury in surface waters of Galveston Bay was determined using the concentrations of mercury-complexing ligands and conditional stability constants of mercury-ligand complexes. Two classes of natural ligands associated with dissolved organic matter were determined by a competitive ligand exchange-solvent solvent extraction (CLE-SSE) method: a strong class (Ls), ranging from 19 to 93 pM with an average conditional stability constant (KHgLs) of 1028, and a weak class (Lw) ranging from 1.4 to 9.8 nM with an average \\{KHgLs\\} of 1023. The range of conditional stability constants between mercury and natural ligands suggested that sulfides and thiolates are important binding sites for dissolved mercury in estuarine waters. A positive correlation between the estuarine distribution of dissolved glutathione and that of mercury-complexing ligands supported this suggestion. Thermodynamic equilibrium modeling using stability constants for HgL, HgClx, Hg(OH)x, and HgCl(OH) and concentrations of each ligand demonstrated that almost all of the dissolved mercury (>99%) in Galveston Bay was complexed by natural ligands associated with dissolved organic matter. The importance of low concentrations of high-affinity ligands that may originate in the biological system (i.e., glutathione and phytochelatin) suggests that the greater portion of bulk dissolved organic matter may not be important for mercury complexation in estuarine surface waters.

Seunghee Han; Gary A. Gill; Ronald D. Lehman; Key-Young Choe

2006-01-01T23:59:59.000Z

220

Comparing the Reproductive Success of Yakima River Hatchery-and Wild-Origin Spring Chinook; Yakima/Klickitat Fisheries Project Monitoring and Evaluation, 2000-2001 Annual Report.  

SciTech Connect (OSTI)

In the Yakima Spring Chinook supplementation program, wild fish are brought into the Cle Elum Hatchery, artificially crossed, reared, transferred to acclimation sites, and released into the upper Yakima River as smolts. When these fish mature and return to the Yakima River most of them will be allowed to spawn naturally; a few, however, will be brought back to the hatchery and used for research purposes. In order for this supplementation approach to be successful, hatchery-origin fish must be able to spawn and produce offspring under natural conditions. Recent investigations on salmonid fishes have indicated that exposure to hatchery environments during juvenile life may cause significant behavioral, physiological, and morphological changes in adult fish. These changes appear to reduce the reproductive competence of hatchery fish. In general, males are more affected than females; species with prolonged freshwater rearing periods are more strongly impacted than those with shorter rearing periods; and stocks that have been exposed to artificial culture for multiple generations are more impaired than those with a relatively short exposure history to hatchery conditions.

Schroder, S.L. (Washington Department of Fish and Wildlife, Olympia, WA); Knudsen, C.M. (Oncorh Consulting, Olympia, WA); Rau, J.A. (Cle Elum Supplementation Research, Cle Elum, WA)

2003-01-01T23:59:59.000Z

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221

LIFTING THE DUSTY VEIL WITH NEAR- AND MID-INFRARED PHOTOMETRY. III. TWO-DIMENSIONAL EXTINCTION MAPS OF THE GALACTIC MIDPLANE USING THE RAYLEIGH-JEANS COLOR EXCESS METHOD  

SciTech Connect (OSTI)

We provide new, high-resolution A(K{sub s} ) extinction maps of the heavily reddened Galactic midplane based on the Rayleigh-Jeans Color Excess ({sup R}JCE{sup )} method. RJCE determines star-by-star reddening based on a combination of near- and mid-infrared photometry. The new RJCE-generated maps have 2' Multiplication-Sign 2' pixels and span some of the most severely extinguished regions of the Galaxy-those covered with Spitzer/IRAC imaging by the GLIMPSE-I, -II, -3D, and Vela-Carina surveys, from 256 Degree-Sign < l < 65 Degree-Sign and, in general, for |b| {<=} 1 Degree-Sign -1.{sup 0}5 (extending up to |b| {<=} 4 Degree-Sign in the bulge). Using RJCE extinction measurements, we generate dereddened color-magnitude diagrams and, in turn, create maps based on main sequence, red clump, and red giant star tracers, each probing different distances and thereby providing coarse three-dimensional information on the relative placement of dust cloud structures. The maps generated from red giant stars, which reach to {approx}18-20 kpc, probe beyond most of the Milky Way extinction in most directions and provide close to a 'total Galactic extinction' map-at minimum they provide high angular resolution maps of lower limits on A(K{sub s} ). Because these maps are generated directly from measurements of reddening by the very dust being mapped, rather than inferred on the basis of some less direct means, they are likely the most accurate to date for charting in detail the highly patchy differential extinction in the Galactic midplane. We provide downloadable FITS files and an IDL tool for retrieving extinction values for any line of sight within our mapped regions.

Nidever, David L.; Zasowski, Gail; Majewski, Steven R., E-mail: dln5q@virginia.edu, E-mail: gz2n@virginia.edu, E-mail: srm4n@virginia.edu [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States)

2012-08-01T23:59:59.000Z

222

Geophysical investigation, Salmon Site, Lamar County, Mississippi  

SciTech Connect (OSTI)

Geophysical surveys were conducted in 1992 and 1993 on 21 sites at the Salmon Site (SS) located in Lamar County, Mississippi. The studies are part of the Remedial Investigation/Feasibility Study (RI/FS) being conducted by IT Corporation for the U.S. Department of Energy (DOE). During the 1960s, two nuclear devices and two chemical tests were detonated 826 meters (in) (2710 feet [ft]) below the ground surface in the salt dome underlying the SS. These tests were part of the Vela Uniform Program conducted to improve the United States capability to detect, identify, and locate underground nuclear detonations. The RI/FS is being conducted to determine if any contamination is migrating from the underground shot cavity in the salt dome and if there is any residual contamination in the near surface mud and debris disposal pits used during the testing activities. The objective of the surface geophysical surveys was to locate buried debris, disposal pits, and abandoned mud pits that may be present at the site. This information will then be used to identify the locations for test pits, cone penetrometer tests, and drill hole/monitor well installation. The disposal pits were used during the operation of the test site in the 1960s. Vertical magnetic gradient (magnetic gradient), electromagnetic (EM) conductivity, and ground-penetrating radar (GPR) surveys were used to accomplish these objectives. A description of the equipment used and a theoretical discussion of the geophysical methods are presented Appendix A. Because of the large number of figures relative to the number of pages of text, the geophysical grid-location maps, the contour maps of the magnetic-gradient data, the contour maps of the EM conductivity data, and the GPR traverse location maps are located in Appendix B, Tabs I through 22. In addition, selected GPR records are located in Appendix C.

NONE

1995-02-01T23:59:59.000Z

223

On the absence of wind bow-shocks around OB-runaway stars: probing the physical conditions of the interstellar medium  

E-Print Network [OSTI]

High-resolution IRAS maps are used to search for the presence of stellar-wind bow-shocks around high-mass X-ray binaries (HMXBs). Their high space velocities, recently confirmed with Hipparcos observations, combined with their strong stellar winds should result in the formation of wind bow-shocks. Except for the already known bow-shock around Vela X-1 (Kaper et al. 1997), we do not find convincing evidence for a bow-shock around any of the other HMXBs. Also in the case of (supposedly single) OB-runaway stars, only a minority appears to be associated with a bow-shock (Van Buren et al. 1995). We investigate why wind bow-shocks are not detected for the majority of these OB-runaway systems: is this due to the IRAS sensitivity, the system's space velocity, the stellar-wind properties, or the height above the galactic plane? It turns out that none of these suggested causes can explain the low detection rate (~40%). We propose that the conditions of the interstellar medium mainly determine whether a wind bow-shock is formed or not. In hot, tenuous media (like inside galactic superbubbles) the sound speed is high (~100 km/s), such that many runaways move at subsonic velocity through a low-density medium, thus preventing the formation of an observable bow-shock. Superbubbles are expected (and observed) around OB associations, where the OB-runaway stars were once born. Turning the argument around, we use the absence (or presence) of wind bow-shocks around OB runaways to probe the physical conditions of the interstellar medium in the solar neighbourhood.

Fredrik Huthoff; Lex Kaper

2001-12-18T23:59:59.000Z

224

COOLING OF COMPACT STARS WITH COLOR SUPERCONDUCTING PHASE IN QUARK-HADRON MIXED PHASE  

SciTech Connect (OSTI)

We present a new scenario for the cooling of compact stars considering the central source of Cassiopeia A (Cas A). The Cas A observation shows that the central source is a compact star that has high effective temperature, and it is consistent with the cooling without exotic phases. The observation also gives the mass range of M {>=} 1.5 M {sub Sun }, which may conflict with the current plausible cooling scenario of compact stars. There are some cooled compact stars such as Vela or 3C58, which can barely be explained by the minimal cooling scenario, which includes the neutrino emission by nucleon superfluidity (PBF). Therefore, we invoke the exotic cooling processes, where a heavier star cools faster than lighter one. However, the scenario seems to be inconsistent with the observation of Cas A. Therefore, we present a new cooling scenario to explain the observation of Cas A by constructing models that include a quark color superconducting (CSC) phase with a large energy gap; this phase appears at ultrahigh density regions and reduces neutrino emissivity. In our model, a compact star has a CSC quark core with a low neutrino emissivity surrounded by high emissivity region made by normal quarks. We present cooling curves obtained from the evolutionary calculations of compact stars: while heavier stars cool slowly, and lighter ones indicate the opposite tendency without considering nucleon superfluidity. Furthermore, we show that our scenario is consistent with the recent observations of the effective temperature of Cas A during the last 10 years, including nucleon superfluidity.

Noda, Tsuneo; Hashimoto, Masa-aki [Department of Physics, Kyushu University, 6-10-1 Hakozaki, Higashi-ku, Fukuoka, 812-8581 Japan (Japan)] [Department of Physics, Kyushu University, 6-10-1 Hakozaki, Higashi-ku, Fukuoka, 812-8581 Japan (Japan); Yasutake, Nobutoshi [Research Center for the Early Universe, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)] [Research Center for the Early Universe, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Maruyama, Toshiki [Advanced Science Research Center, Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195 (Japan)] [Advanced Science Research Center, Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195 (Japan); Tatsumi, Toshitaka [Department of Physics, Kyoto University, Kitashirakawa-Oiwake-cho, Kyoto 606-8502 (Japan)] [Department of Physics, Kyoto University, Kitashirakawa-Oiwake-cho, Kyoto 606-8502 (Japan); Fujimoto, Masayuki, E-mail: tsune@phys.kyushu-u.ac.jp, E-mail: hashimoto@phys.kyushu-u.ac.jp [Department of Physics, Hokkaido University, Kita-10 Nishi-8, Kita-ku, Sapporo, Hokkaido 060-0810 (Japan)] [Department of Physics, Hokkaido University, Kita-10 Nishi-8, Kita-ku, Sapporo, Hokkaido 060-0810 (Japan)

2013-03-01T23:59:59.000Z

225

Chlorine/bromine ratios in fracture-filling aqueous alteration products in Nakhla olivine  

SciTech Connect (OSTI)

The Cl/Br ratios in fracture-filling materials in veins in Nakhla olivine was determined using x-ray microprobe (Br) and EDX (Cl) techniques. The Cl/Br ratio of 55 +/- 13 shows that the secondary altered material is pristine, extraterrestrial and akin to the Martian soil. During the early Martian history, volcanic emanations contributed large excesses of volatiles including halogens, sulfur and water to the Martian crust. These chemically-reactive elements had undergone extensive redistribution over time due to a variety of surface processes on Mars. To understand the nature of the alterations due to aqueous activity in the Martian surface environment, a study of halogens, in particular Cl/Br ratios in secondary mineralization products may provide valuable insights. Dreibus and Waenke arrived at a Cl/Br ratio of {approx}110 for the Martian surface materials by studying glasses and bulk samples of several SNC meteorites using neutron activation. Nakhla probably offers the most diverse suite of aqueous precipitates to be found among the SNC meteorites. Numerous veins of hydrous clay within olivine grains are present in Nakhla. Bridges and Grady and Wentworth and McKay observed massive concentrations of halite of probable Martian evaporitic origin, in association with siderite and anhydrite in interstitial areas in Nakhla. Dreibus et al. reported Cl/Br ratios in 3 Nakhla fragments from 104 to 550 and found that 90% of the Cl and Br was readily leachable from this material. Their Nakhla leachate ratio was 580. Their analysis of an attached salt grain yielded a ratio of 5440, similar to that in table salt. Xirouchakis et al. found 20 ppm Br in glass veins in Los Angeles shergottite based on XRF measurements with the x-ray microprobe (beamline X26A) at the Brookhaven Nat. Lab. We examine in this study whether a Cl/Br ratio similar to that of Dreibus and Waenke is also present in products of secondary mineralization, generated as a result of aqueous alteration in some SNC meteorites. We have studied the Cl/Br ratios in fracture-filling materials in veins in Nakhla olivines (thin sections) by determining Br contents using the X-ray Microprobe facility at GeoSoilEnviroCARS (Advanced Photon Source/University of Chicago) and by determining Cl using SEM-based EDX measurements at the same sites in the veins.

Sutton, S.R.; Rao, M.N.; Dreibus, G.; McKay, D.S.; Wanke, H.; Wentworth, S.; Newville, M.; Trainor, T.; Flynn, G.J. (Max-Plank Inst); (SUNY Plattsburgh); (UofC); (Lockheed Martin); (NASA)

2005-04-22T23:59:59.000Z

226

s042.dvi  

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

I I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.50± 0.30 OUR FIT 5279.50± 0.30 OUR FIT 5279.50± 0.30 OUR FIT 5279.50± 0.30 OUR FIT 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.63± 0.53 ± 0.33 1 ACOSTA 06 CDF p p at 1.96 TeV 5279.1 ± 0.7 ± 0.3 135 2 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3 ± 2.2 ± 1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for

227

s042.dvi  

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

0 0 I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.50± 0.33 OUR FIT 5279.50± 0.33 OUR FIT 5279.50± 0.33 OUR FIT 5279.50± 0.33 OUR FIT 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.5 ± 0.5 OUR AVERAGE 5279.63± 0.53 ± 0.33 1 ACOSTA 06 CDF p p at 1.96 TeV 5279.1 ± 0.7 ± 0.3 135 2 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3 ± 2.2 ± 1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for

228

m057.dvi  

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

7 7 χ c2 (1P) I G (J PC ) = 0 + (2 + + ) See the Review on "ψ(2S) and χ c branching ratios" before the NODE=M057 χ c0 (1P) Listings. χ c2 (1P) MASS χ c2 (1P) MASS χ c2 (1P) MASS χ c2 (1P) MASS NODE=M057M NODE=M057M VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3555.3 ± 0.6 ± 2.2 2.5k UEHARA 08 BELL γ γ → hadrons 3555.70 ± 0.59 ± 0.39 ABLIKIM 05G BES2 ψ(2S) → γ χ c2 3556.173 ± 0.123 ± 0.020 ANDREOTTI 05A E835 p p → e + e - γ 3559.9 ± 2.9 EISENSTEIN 01 CLE2 e + e - → e + e - χ c2 3556.4 ± 0.7 BAI 99B BES ψ(2S) → γ X 3556.22 ± 0.131 ± 0.020 585 1 ARMSTRONG 92 E760 p p → e + e - γ 3556.9 ± 0.4 ± 0.5 50 BAGLIN 86B SPEC p p → e + e - X 3557.8 ± 0.2 ± 4 2 GAISER 86 CBAL ψ(2S) → γ X 3553.4 ± 2.2 66 3 LEMOIGNE 82 GOLI 185 π - Be → γ µ + µ - A 3555.9 ± 0.7 4 OREGLIA 82 CBAL e + e - → J/ψ 2γ 3557 ± 1.5

229

s041.dvi  

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

3 3 Page 1 NODE=S041 B ± I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model NODE=S041 predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. B ± MASS B ± MASS B ± MASS B ± MASS NODE=S041M The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , NODE=S041M and the mass difference. NODE=S041M VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.26 ± 0.17 OUR FIT 5279.26 ± 0.17 OUR FIT 5279.26 ± 0.17 OUR FIT 5279.26 ± 0.17 OUR FIT NEW [5279.25 ± 0.17 MeV OUR 2012 FIT] 5279.25 ± 0.26 OUR AVERAGE 5279.25 ± 0.26 OUR AVERAGE 5279.25 ± 0.26 OUR AVERAGE 5279.25 ± 0.26 OUR AVERAGE 5279.38 ± 0.11 ± 0.33 1 AAIJ 12E LHCB p p at 7 TeV 5279.10 ± 0.41 ± 0.36 2 ACOSTA 06 CDF p p at 1.96 TeV 5279.1 ± 0.4 ± 0.4 526 3 CSORNA 00 CLE2 e + e - → Υ(4S) 5279.1 ± 1.7 ± 1.4 147 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc.

230

m057.dvi  

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

c2 c2 (1P) I G (J PC ) = 0 + (2 + + ) See the Review on "ψ(2S) and χ c branching ratios" before the χ c0 (1P) Listings. χ c2 (1P) MASS χ c2 (1P) MASS χ c2 (1P) MASS χ c2 (1P) MASS VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3556.20 ± 0.09 OUR AVERAGE 3555.70 ± 0.59 ± 0.39 ABLIKIM 05G BES2 ψ(2S) → γ χ c2 3556.173± 0.123 ± 0.020 ANDREOTTI 05A E835 p p → e + e - γ 3559.9 ± 2.9 EISENSTEIN 01 CLE2 e + e - → e + e - χ c2 3556.4 ± 0.7 BAI 99B BES ψ(2S) → γ X 3556.22 ± 0.131 ± 0.020 585 1 ARMSTRONG 92 E760 p p → e + e - γ 3556.9 ± 0.4 ± 0.5 50 BAGLIN 86B SPEC p p → e + e - X 3557.8 ± 0.2 ± 4 2 GAISER 86 CBAL ψ(2S) → γ X 3553.4 ± 2.2 66 3 LEMOIGNE 82 GOLI 185 π - Be → γ µ + µ - A 3555.9 ± 0.7 4 OREGLIA 82 CBAL e + e - → J/ψ 2γ 3557 ± 1.5 69 5 HIMEL 80 MRK2 e + e - → J/ψ 2γ 3551 ± 11 15 BRANDELIK 79B DASP e + e - → J/ψ 2γ 3553 ± 4 5 BARTEL

231

s042.dvi  

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

0 0 I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing and CP Violation in B Decay" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.1±0.7 ±0.3 135 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3±2.2 ±1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. *

232

s042.dvi  

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

0 0 I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing and CP Violation in B Decay" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.4±0.5 OUR FIT 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.3±0.7 OUR AVERAGE 5279.1±0.7 ±0.3 135 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3±2.2 ±1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. *

233

Citation: W.-M. Yao  

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

c0 c0 (1P) I G (J PC ) = 0 + (0 + + ) χ c0 (1P) MASS χ c0 (1P) MASS χ c0 (1P) MASS χ c0 (1P) MASS VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 3414.76 ± 0.35 OUR AVERAGE 3414.76 ± 0.35 OUR AVERAGE 3414.76 ± 0.35 OUR AVERAGE 3414.76 ± 0.35 OUR AVERAGE Error includes scale factor of 1.2. 3414.21 ± 0.39 ± 0.27 ABLIKIM 05G BES2 ψ(2S) → γ χ c0 3414.7 + 0.7 - 0.6 ± 0.2 1 ANDREOTTI 03 E835 p p → χ c0 → π 0 π 0 3415.5 ± 0.4 ± 0.4 392 2 BAGNASCO 02 E835 p p → χ c0 → J/ψ γ 3417.4 + 1.8 - 1.9 ± 0.2 1 AMBROGIANI 99B E835 p p → e + e - γ 3414.1 ± 0.6 ± 0.8 BAI 99B BES ψ(2S) → γ X 3417.8 ± 0.4 ± 4 1 GAISER 86 CBAL ψ(2S) → γ X 3416 ± 3 ± 4 3 TANENBAUM 78 MRK1 e + e - * * * We do not use the following data for averages, fits, limits, etc. * * * 3407 ± 11 89 4 ABE 04G BELL 10.6 e + e - → J/ψ(c c) 3416.5 ± 3.0 EISENSTEIN 01 CLE2 e + e - → e + e - χ c0 3422 ± 10 3 BARTEL 78B CNTR e + e - → J/ψ 2γ 3415 ± 9 3 BIDDICK 77 CNTR e + e - → γ X 1 Using mass

234

Citation: W.-M. Yao  

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

B B 0 I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.4 ± 0.5 OUR FIT 5279.4 ± 0.5 OUR FIT 5279.4 ± 0.5 OUR FIT 5279.4 ± 0.5 OUR FIT 5279.3 ± 0.7 OUR AVERAGE 5279.3 ± 0.7 OUR AVERAGE 5279.3 ± 0.7 OUR AVERAGE 5279.3 ± 0.7 OUR AVERAGE 5279.1 ± 0.7 ± 0.3 135 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3 ± 2.2 ± 1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. * * * 5279.2 ± 0.54 ± 2.0 340

235

s042.dvi  

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

0 0 I (J P ) = 1 2 (0 - ) Quantum numbers not measured. Values shown are quark-model predictions. See also the B ± /B 0 ADMIXTURE and B ± /B 0 /B 0 s /b-baryon AD- MIXTURE sections. See the Note "Production and Decay of b-flavored Hadrons" at the beginning of the B ± Particle Listings and the Note on "B 0 -B 0 Mixing" near the end of the B 0 Particle Listings. B 0 MASS B 0 MASS B 0 MASS B 0 MASS The fit uses m B + , (m B 0 - m B + ), and m B 0 to determine m B + , m B 0 , and the mass difference. VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 5279.4± 0.5 OUR FIT 5279.4± 0.5 OUR FIT 5279.4± 0.5 OUR FIT 5279.4± 0.5 OUR FIT 5279.3± 0.7 OUR AVERAGE 5279.3± 0.7 OUR AVERAGE 5279.3± 0.7 OUR AVERAGE 5279.3± 0.7 OUR AVERAGE 5279.1± 0.7 ± 0.3 135 1 CSORNA 00 CLE2 e + e - → Υ(4S) 5281.3± 2.2 ± 1.4 51 ABE 96B CDF p p at 1.8 TeV * * * We do not use the following data for averages, fits, limits, etc. * * * 5279.2± 0.54 ± 2.0 340

236

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

SciTech Connect (OSTI)

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.

Larsen, Donald; Beckman, Brian; Cooper, Kathleen

2003-08-01T23:59:59.000Z

237

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

SciTech Connect (OSTI)

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.

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

2013-08-27T23:59:59.000Z

238

DISCOVERY OF AN ENERGETIC PULSAR ASSOCIATED WITH SNR G76.9+1.0  

SciTech Connect (OSTI)

We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray Observatory, the Robert C. Byrd Green Bank Radio Telescope, and the Rossi X-ray Timing Explorer (RXTE). The pulsar's spin-down rate implies a rotation-powered luminosity E-dot = 1.2x10{sup 38} erg s{sup -1}, a surface dipole magnetic field strength B{sub s} = 1.0 x 10{sup 12} G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly rotating young, radio-bright pulsar known. The radio pulsations are highly dispersed and broadened by interstellar scattering, and we find that a large ({delta}f/f {approx} 1.9 x 10{sup -6}) spin glitch must have occurred between our discovery and confirmation observations. The X-ray pulses are narrow (0.06 cycles FWHM) and visible up to 20 keV, consistent with magnetospheric emission from a rotation-powered pulsar. The Chandra X-ray image identifies the pulsar with a hard, unresolved source at the midpoint of the double-lobed radio morphology of G76.9+1.0 and embedded within faint, compact X-ray nebulosity. The spatial relationship of the X-ray and radio emissions is remarkably similar to the extended structure seen around the Vela pulsar. The combined Chandra and RXTE pulsar spectrum is well fitted by an absorbed power-law model with column density N{sub H} = (1.7 {+-} 0.3) x 10{sup 22} cm{sup -2} and photon index {Gamma} = 1.0 {+-} 0.2; this implies that the Chandra point-source flux is virtually 100% pulsed. For a distance of 10 kpc, the X-ray luminosity of PSR J2022+3842 is L{sub X}(2-10 keV) = 7.0 x 10{sup 33} erg s{sup -1}. Despite being extraordinarily energetic, PSR J2022+3842 lacks a bright X-ray wind nebula and has an unusually low conversion efficiency of spin-down power to X-ray luminosity, L{sub X}/ E-dot = 5.9x10{sup -5}.

Arzoumanian, Z. [Center for Research and Exploration in Space Science and Technology and X-ray Astrophysics Laboratory, NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771 (United States); Gotthelf, E. V. [Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027 (United States); Ransom, S. M. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22901 (United States); Safi-Harb, S. [Canada Research Chair, Department of Physics and Astronomy, University of Manitoba, Winnipeg, MB, R3T 2N2 (Canada); Kothes, R.; Landecker, T. L., E-mail: Zaven.Arzoumanian@nasa.gov [National Research Council of Canada, Herzberg Institute of Astrophysics, Dominion Radio Astrophysical Observatory, Box 248, Penticton, BC, V2A 6J9 (Canada)

2011-09-20T23:59:59.000Z

239

m056.dvi  

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

1P) 1P) I G (J PC ) = 0 + (0 + + ) χ c0 (1P) MASS χ c0 (1P) MASS χ c0 (1P) MASS χ c0 (1P) MASS VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 3414.75± 0.31 OUR AVERAGE 3414.75± 0.31 OUR AVERAGE 3414.75± 0.31 OUR AVERAGE 3414.75± 0.31 OUR AVERAGE 3414.2 ± 0.5 ± 2.3 5.4k UEHARA 08 BELL γ γ → χ c0 → hadrons 3406 ± 7 ± 6 230 1 ABE 07 BELL e + e - → J/ψ (c c) 3414.21± 0.39± 0.27 ABLIKIM 05G BES2 ψ(2S) → γ χ c0 3414.7 + 0.7 - 0.6 ± 0.2 2 ANDREOTTI 03 E835 p p → χ c0 → π 0 π 0 3415.5 ± 0.4 ± 0.4 392 3 BAGNASCO 02 E835 p p → χ c0 → J/ψ γ 3417.4 + 1.8 - 1.9 ± 0.2 2 AMBROGIANI 99B E835 p p → e + e - γ 3414.1 ± 0.6 ± 0.8 BAI 99B BES ψ(2S) → γ X 3417.8 ± 0.4 ± 4 2 GAISER 86 CBAL ψ(2S) → γ X 3416 ± 3 ± 4 4 TANENBAUM 78 MRK1 e + e - * * * We do not use the following data for averages, fits, limits, etc. * * * 3416.5 ± 3.0 EISENSTEIN 01 CLE2 e + e - → e + e - χ c0 3422 ± 10 4 BARTEL 78B CNTR e + e - → J/ψ 2γ 3415 ± 9 4 BIDDICK 77 CNTR e

240

The Reaches Project : Ecological and Geomorphic Dtudies Supporting Normative Flows in the Yakima River Basin, Washington, Final Report 2002.  

SciTech Connect (OSTI)

The Yakima River system historically produced robust annual runs of chinook, sockeye, chum and coho salmon and steelhead. Many different stocks or life history types existed because the physiography of the basin is diverse, ranging from very dry and hot in the high desert of the lower basin to cold and wet in the Cascade Mountains of the headwaters (Snyder and Stanford 2001). Habitat diversity and life history diversity of salmonids are closely correlated in the Yakima Basin. Moreover, habitat diversity for salmonids and many other fishes maximizes in floodplain reaches of river systems (Ward and Stanford 1995, Independent Scientific Group 2000). The flood plains of Yakima River likely were extremely important for spawning and rearing of anadromous salmonids (Snyder and Stanford 2001). However, Yakima River flood plains are substantially degraded. Primary problems are: revetments that disconnect main and side channel habitats; dewatering associated with irrigation that changes base flow conditions and degrades the shallow-water food web; chemical and thermal pollution that prevents proper maturation of eggs and juveniles; and extensive gravel mining within the floodplain reaches that has severed groundwater-channel connectivity, increased thermal loading and increased opportunities for invasions of nonnative species. The Yakima River is too altered from its natural state to allow anything close to the historical abundance and diversity of anadromous fishes. Habitat loss, overharvest and dam and reservoir passage problems in the mainstem Columbia River downstream of the Yakima, coupled with ocean productivity variation, also are implicated in the loss of Yakima fisheries. Nonetheless, in an earlier analysis, Snyder and Stanford (2001) concluded that a significant amount of physical habitat remains in the five floodplain reaches of the mainstem river because habitat-structuring floods do still occur on the remaining expanses of floodplain environment. Assuming main stem and ocean bottlenecks are not overriding, restoration of floodplain connectivity by elevating base flows throughout the corridor, removing revetments and refilling gravel pits by natural riverine transport of gravel where possible could be successful in substantially enhancing Yakima salmon and steelhead runs. Hence, the overarching purpose of this research was to determine the ecology of major floodplain reaches of the Yakima River: Cle Elum, Kittitas, Naches, Union Gap and Wapato. Specifically, the study documented groundwater-channel connectivity and flow relations; use and quality of side channel and other floodplain habitats by salmonid fishes; and classification and analysis of floodplain habitat using remote sensing and documentation of geomorphic processes, required for a robust understanding of the feasibility of revetment removal and establishment of a normative flow regime for the mainstem river.

Stanford, Jack A.; Lorang, Mark N.; Matson, Phillip L. (University of Montana, Flathead Lake Biological Station, Poison, MT)

2002-10-01T23:59:59.000Z

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241

Book Reviews: Search for Life; Health Physics; Language and Literacy in Science Education; Science Web ReaderPhysicsCorrectionGCSE Book Reviews: Physics for Higher Tier; Modular Science; Modular Science for AQA: Foundation level and Higher level; Physics for OCR A; Physics Matters, 3rd edition; Physics; Science Foundations: Physics (new edition); Target Science: Physics Foundation Tier; Target Science: Physics Foundation Tier: AQA Modular ScienceReviewersFree PostersWeb Watch: Medical physics organizations  

Science Journals Connector (OSTI)

Contents: Book Review: Search for Life Book Review: Health Physics Book Review: Language and Literacy in Science Education Book Review: Science Web ReaderPhysics Correction GCSE Book Review: Physics for Higher Tier GCSE Book Review: Modular Science GCSE Book Review: Modular Science for AQA: Foundation level and Higher level GCSE Book Review: Physics for OCR A GCSE Book Review: Physics Matters, 3rd edition GCSE Book Review: Physics GCSE Book Review: Science Foundations: Physics (new edition) GCSE Book Review: Target Science: Physics Foundation Tier GCSE Book Review: Target Science: Physics Foundation Tier: AQA Modular Science Reviewers Free Posters Web Watch: Medical physics organizations BOOK REVIEW Search for Life This slim volume begins by examining the origins and evolution of life on Earth before moving on to explore the possibility of life existing elsewhere in our solar system, or beyond. The book is organized and written in a way that makes it easy to read, whilst keeping a wealth of detailed, up-to-date information available in separate, well defined panels. Astounding photographs and excellent illustrations help to examine the evidence which leads to our current understanding of the structure of the Universe, and investigate the possibility of the existence of other lifeforms. I found the book extremely readable and highly informative on this rapidly developing, high profile area of science. With a layout that would not preclude its use as a reference book for younger (KS3) pupils, at the same time it provides enough depth of information to enthral both myself and older pupils. I will certainly be recommending that both our school and department libraries have a copy, and would unreservedly recommend it to other teachers of Astronomy, Physics or Biology. PH Search for Life Monica Grady Rating: excellent Price: 9.95 pbk Details: Published 2001, Natural History Museum, 96pp, www.nhm.ac.uk ISBN: 0 565 09157 3 BOOK REVIEW Health Physics This short introductory text forms part of a series, edited by David Sang, which specifically cover the OCR 'specification A' A-level exams. Thus Health Physics is a revised version of the 1996 book by the same authors which was written for the Cambridge-examined modular A-level. Superficially the new book is very similar to the original it is light (at 80 pages, only 10 pages longer) and easily accessible. The book follows Cambridge Advanced Sciences (CAS) house style with lots of illustrations, clear chapter objective and summaries, SAQs interspersed in the text and end-of-chapter questions. What's new? Most of the changes reflect changes in the OCR specification. The chapter on Energy Needs is replaced by Body Mechanics. Sadly the chapter is marred with sloppy language, imprecise diagrams and, worst of all, the incorrect classification of a toe raise as class 2 lever. (The author was only recently alerted to this common mistake by reading the ASE's very useful Signs, Symbols and Systematics 16-19 1.) The rest of the book is very similar to the original the chapters on the eye and the ear are almost identical. The chapters covering radiation and ultrasound have been reorganized into smaller, more logical chapters, which I think will suit my lesson-plans better, and my feeling is that there is a slight improvement in the quality and the quantity of medical images (though sadly, they are mostly still in black and white). A useful book by way of an introduction to medical physics, and vital if you teach the OCR course. KP 1 Signs, Symbols and Systematics 16-19, ASE, 2000. ISBN 0863573126, price 30.00. Health Physics Alexander Elliott and Andrew McCormick Rating: very good Price: 7.95 pbk Details: Published 2001, Cambridge University Press, 96pp, www.cambridge.org ISBN: 0 521 78726 2 BOOK REVIEW Language and Literacy in Science Education This book is a comprehensive study of the use of language in science education. It is aimed at helping teachers to become more effective communicators of their subject. The book calls upon research of the past thirty years which sugges