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1

VELA_COMP_OUT  

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

Years of Treaty Verification from Space Operational Satellite Systems During the 50 years since the first Vela satellites, the United States developed and maintained an evolving...

2

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

3

Grady County, Oklahoma: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady County,

4

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

5

Il comfortometro al CLE Sistemi sociotecnici e risparmio energetico  

E-Print Network [OSTI]

e docenti. · Per funzionare richiede una grande quantità di energia, sia diretta che indiretta. · Qui ci occuperemo essenzialmente di energia diretta #12;Alcuni dati sul CLE · Circa 45mila mq di interazione tra final users e sistema edificio. #12;Anno 2013 1. Consumo Energia Termica 529.129 m3 metano 4

Sproston, Jeremy

6

THE HELICAL JET OF THE VELA PULSAR  

SciTech Connect (OSTI)

We have studied the fascinating dynamics of the nearby Vela pulsar's nebula in a campaign comprising 11 40 ks observations with the Chandra X-Ray Observatory. The deepest images yet revealed the shape, structure, and motion of the 2 arcmin long pulsar jet. We find that the jet's shape and dynamics are remarkably consistent with those of a steadily turning helix projected on the sky. We discuss possible implications of our results, including free precession of the neutron star and MHD instability scenarios.

Durant, Martin; Kargaltsev, Oleg [University of Florida, 211 Bryant Space Science Center, Gainesville, FL (United States)] [University of Florida, 211 Bryant Space Science Center, Gainesville, FL (United States); Pavlov, George G. [Pennsylvania State University, 525 Davey Lab, University Park, PA (United States)] [Pennsylvania State University, 525 Davey Lab, University Park, PA (United States); Kropotina, Julia; Levenfish, Kseniya, E-mail: mdurant@sri.utoronto.ca [St.-Petersburg State Polytechnical University, Polytekhnicheskaya ul. 29, St.-Petersburg, 195251 (Russian Federation)] [St.-Petersburg State Polytechnical University, Polytekhnicheskaya ul. 29, St.-Petersburg, 195251 (Russian Federation)

2013-02-15T23:59:59.000Z

7

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"

8

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

9

VERY HIGH ENERGY GAMMA RAYS FROM THE VELA PULSAR DIRECTION  

E-Print Network [OSTI]

VERY HIGH ENERGY GAMMA RAYS FROM THE VELA PULSAR DIRECTION T. Yoshikoshi1;2, T. Kifune2, S and Mathematical Physics, University of Adelaide, Adelaide, South Australia 5005, Australia 4Institute of SpaceDepartment of Physics, Kyoto University, Kyoto, Kyoto 606, Japan 8Solar-Terrestrial Environment Laboratory

Enomoto, Ryoji

10

ANGULAR MOMENTUM TRANSFER IN VELA-LIKE PULSAR GLITCHES  

SciTech Connect (OSTI)

The angular momentum transfer associated with Vela-like glitches has never been calculated directly within a realistic scenario for the storage and release of superfluid vorticity; therefore, the explanation of giant glitches in terms of vortices has not yet been tested against observations. We present the first physically reasonable model, both at the microscopic and macroscopic level (spherical geometry, n = 1 polytropic density profile, density-dependent pinning forces compatible with vortex rigidity), to determine where in the star the vorticity is pinned, how much of it is pinned, and for how long. For standard neutron star parameters (M = 1.4 M{sub Sun }, R{sub s} = 10 km, {Omega}-dot = {Omega}-dot{sub Vela} = -10{sup -10} Hz s{sup -1}), we find that maximum pinning forces of order f{sub m} Almost-Equal-To 10{sup 15} dyn cm{sup -1} can accumulate {Delta}L{sub gl} Almost-Equal-To 10{sup 40} erg s of superfluid angular momentum, and release it to the crust at intervals {Delta}t{sub gl} Almost-Equal-To 3 years. This estimate of {Delta}L{sub gl} is one order of magnitude smaller than that implied indirectly by current models for post-glitch recovery, where the core and inner-crust vortices are taken as physically disconnected; yet, it successfully yields the magnitudes observed in recent Vela glitches for both jump parameters, {Delta}{Omega}{sub gl} and {Delta}{Omega}-dot{sub gl}, provided one assumes that only a small fraction (<10%) of the total star vorticity is coupled to the crust on the short timescale of a glitch. This is reasonable in our approach, where no layer of normal matter exists between the core and the inner-crust, as indicated by existing microscopic calculation. The new scenario presented here is nonetheless compatible with current post-glitch models.

Pizzochero, Pierre M., E-mail: pierre.pizzochero@mi.infn.it [Dipartimento di Fisica, Universita degli Studi di Milano, and Istituto Nazionale di Fisica Nucleare, sezione di Milano, Via Celoria 16, 20133 Milano (Italy)

2011-12-10T23:59:59.000Z

11

Evaluation of water resources for enhanced oil recovery operations, Cement Field, Caddo and Grady Counties, Oklahoma  

SciTech Connect (OSTI)

This report is based on the results of an investigation of the water resources local to the Cement Oil Field in Caddo and Grady Counties, southwestern, Oklahoma. The intent of the report is to present at least a semi-quantitative estimate of the volume, deliverability, and chemistry of the water potentially available for enhanced oil recovery in one or more Oklahoma oil fields. Subsequent to a review of several oil fields, the Cement Field was chosen for study because of its large size (25,000 acres), its extensive subsurface control (over 1850 wells), and its long history of production (since 1952) from several producing formations, some of which are already undergoing extensive waterflood operations. A preliminary review of the available data for this study suggested a threefold categorization of water resources, since the data for each category are distinctly different in nature, and, to some extent, different in source. The three categories are: surface water, ground water, and subsurface water. Flow, volume, and chemical analyses of each source are estimated.

Preston, D.A.; Harrison, W.E.; Luza, K.V.; Prater, L.; Reddy, R.J.

1982-02-01T23:59:59.000Z

12

VERY HIGH ENERGY GAMMA RAYS FROM THE VELA PULSAR/NEBULA  

E-Print Network [OSTI]

OG 4.1.19 VERY HIGH ENERGY GAMMA RAYS FROM THE VELA PULSAR/NEBULA T. Yoshikoshi 1 , T. Kifune 1 , S Department of Physics and Mathematical Physics, University of Adelaide, South Australia 5005, Australia 3, Kobe University, Hyogo 637, Japan 8 Department of Physics, Kyoto University, Kyoto 606, Japan 9 Solar

Enomoto, Ryoji

13

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

E-Print Network [OSTI]

IMPACT Vol. 5 No. 1 | Spring 2010 CLeAn eneRGy DeMAnDS: SCienCe, innovATion, PUBLiC PoLiCy Maryland on foreign oil and become the world leader in tomorrow's clean-energy economy," says Steve Fetter, a former researchers shape the new energy economy #12;impact overview impact overview EnErgy rEsEarcH EnErgy r

Hill, Wendell T.

14

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

15

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

16

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

17

Physical and chemical inhomogeneities inside the Vela SNR shell. Indications of ejecta shrapnels  

E-Print Network [OSTI]

We present the results of the combined analysis of three XMM-Newton EPIC observations of the northern rim of the Vela SNR. The three pointings cover an area of ~10 pc^2 (at 250 pc) behind the main shock front and we aim at studying with high resolution the spatial distribution of the physical and chemical properties of the X-ray emitting plasma on this large scale. We produce count-rate images and equivalent width maps of the Ne IX and Mg XI emission blends. We also perform a spatially resolved spectral analysis of a set of physically homogeneous regions. We reveal physical and chemical inhomogeneities in the X-ray emitting plasma. In particular, we find large variations of the O, Ne, Mg, and Fe abundances. In some bright knots we also find unexpectedly enhanced Ne and Mg abundances, with values significantly larger than solar. Our results support a possible association of a few X-ray emitting knots with previously undetected residuals of stellar fragments (i. e. shrapnels) observed, in projection, inside the Vela shell.

M. Miceli; F. Bocchino; F. Reale

2007-12-18T23:59:59.000Z

18

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

19

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.

20

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

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

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

22

A 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 quasi-normal mode oscillations in their parent neutron star that couple to gravitational wave emission. In August 2006, a timing glitch was observed in the radio emission of PSR B0833-45, the Vela pulsar. At the time of the glitch, the two co-located Hanford gravitational wave detectors of the Laser Interferometer Gravitational-wave observatory (LIGO) were operational and taking data as part of the fifth LIGO science run (S5). We present the first direct search for the gravitational wave emission associated with oscillations of the fundamental quadrupole mode excited by a pulsar timing glitch. No gravitational wave detection candidate was found. We place Bayesian 90% confidence upper limits of 6.3e-21 to 1.4e-20 on the peak intrinsic strain amplitude of gravitational wave ring-down signals, depending on which spherical harmonic mode is excited. The corresponding range of energy upper limits is 5.0e44 to 1.3e45 erg.

The LIGO Scientific Collaboration; J. Abadie; B. P. Abbott; R. Abbott; R. Adhikari; P. Ajith; B. Allen; G. Allen; E. Amador Ceron; R. S. Amin; S. B. Anderson; W. G. Anderson; M. A. Arain; M. Araya; Y. Aso; S. Aston; P. Aufmuth; C. Aulbert; S. Babak; P. Baker; S. Ballmer; D. Barker; B. Barr; P. Barriga; L. Barsotti; M. A. Barton; I. Bartos; R. Bassiri; M. Bastarrika; B. Behnke; M. Benacquista; M. F. Bennett; J. Betzwieser; P. T. Beyersdorf; I. A. Bilenko; G. Billingsley; R. Biswas; E. Black; J. K. Blackburn; L. Blackburn; D. Blair; B. Bland; O. Bock; T. P. Bodiya; R. Bondarescu; R. Bork; M. Born; S. Bose; P. R. Brady; V. B. Braginsky; J. E. Brau; J. Breyer; D. O. Bridges; M. Brinkmann; M. Britzger; A. F. Brooks; D. A. Brown; S. Buchner; A. Bullington; A. Buonanno; O. Burmeister; R. L. Byer; L. Cadonati; J. Cain; J. B. Camp; J. Cannizzo; K. C. Cannon; J. Cao; C. Capano; L. Cardenas; S. Caudill; M. Cavagli; C. Cepeda; T. Chalermsongsak; E. Chalkley; P. Charlton; S. Chatterji; S. Chelkowski; Y. Chen; N. Christensen; S. S. Y. Chua; C. T. Y. Chung; D. Clark; J. Clark; J. H. Clayton; R. Conte; D. Cook; T. R. C. Corbitt; N. Cornish; D. Coward; D. C. Coyne; J. D. E. Creighton; T. D. Creighton; A. M. Cruise; R. M. Culter; A. Cumming; L. Cunningham; K. Dahl; S. L. Danilishin; K. Danzmann; B. Daudert; G. Davies; E. J. Daw; T. Dayanga; D. DeBra; J. Degallaix; V. Dergachev; R. DeSalvo; S. Dhurandhar; M. Daz; F. Donovan; K. L. Dooley; E. E. Doomes; R. W. P. Drever; J. Driggers; J. Dueck; I. Duke; J. -C. Dumas; M. Edgar; M. Edwards; A. Effler; P. Ehrens; T. Etzel; M. Evans; T. Evans; S. Fairhurst; Y. Faltas; Y. Fan; D. Fazi; H. Fehrmann; L. S. Finn; K. Flasch; S. Foley; C. Forrest; N. Fotopoulos; M. Frede; M. Frei; Z. Frei; A. Freise; R. Frey; T. T. Fricke; D. Friedrich; P. Fritschel; V. V. Frolov; P. Fulda; M. Fyffe; J. A. Garofoli; S. Ghosh; J. A. Giaime; S. Giampanis; K. D. Giardina; E. Goetz; L. M. Goggin; G. Gonzlez; S. Goler; A. Grant; S. Gras; C. Gray; R. J. S. Greenhalgh; A. M. Gretarsson; R. Grosso; H. Grote; S. Grunewald; E. K. Gustafson; R. Gustafson; B. Hage; J. M. Hallam; D. Hammer; G. D. Hammond; C. Hanna; J. Hanson; J. Harms; G. M. Harry; I. W. Harry; E. D. Harstad; K. Haughian; K. Hayama; T. Hayler; J. Heefner; I. S. Heng; A. Heptonstall; M. Hewitson; S. Hild; E. Hirose; D. Hoak; K. A. Hodge; K. Holt; D. J. Hosken; J. Hough; E. Howell; D. Hoyland; B. Hughey; S. Husa; S. H. Huttner; D. R. Ingram; T. Isogai; A. Ivanov; W. W. Johnson; D. I. Jones; G. Jones; R. Jones; L. Ju; P. Kalmus; V. Kalogera; S. Kandhasamy; J. Kanner; E. Katsavounidis; K. Kawabe; S. Kawamura; F. Kawazoe; W. Kells; D. G. Keppel; A. Khalaidovski; F. Y. Khalili; R. Khan; E. Khazanov; H. Kim; P. J. King; J. S. Kissel; S. Klimenko; K. Kokeyama; V. Kondrashov; R. Kopparapu; S. Koranda; D. Kozak; V. Kringel; B. Krishnan; G. Kuehn; J. Kullman; R. Kumar; P. Kwee; P. K. Lam; M. Landry; M. Lang; B. Lantz; N. Lastzka; A. Lazzarini; P. Leaci; M. Lei; N. Leindecker; I. Leonor; H. Lin; P. E. Lindquist; T. B. Littenberg; N. A. Lockerbie; D. Lodhia; M. Lormand; P. Lu; M. Lubinski; A. Lucianetti; H. Lck; A. Lundgren; B. Machenschalk; M. MacInnis; M. Mageswaran; K. Mailand; C. Mak; I. Mandel; V. Mandic; S. Mrka; Z. Mrka; A. Markosyan; J. Markowitz; E. Maros; I. W. Martin; R. M. Martin; J. N. Marx; K. Mason; F. Matichard; L. Matone; R. A. Matzner; N. Mavalvala; R. McCarthy; D. E. McClelland; S. C. McGuire; G. McIntyre; D. J. A. McKechan; M. Mehmet; A. Melatos; A. C. Melissinos; G. Mendell; D. F. Menndez; R. A. Mercer; L. Merrill; S. Meshkov; C. Messenger; M. S. Meyer; H. Miao; J. Miller; Y. Mino; S. Mitra; V. P. Mitrofanov; G. Mitselmakher; R. Mittleman; O. Miyakawa; B. Moe; S. D. Mohanty; S. R. P. Mohapatra; G. Moreno; K. Mors; K. Mossavi; C. MowLowry; G. Mueller; H. Mller-Ebhardt; S. Mukherjee; A. Mullavey; J. Munch; P. G. Murray; T. Nash; R. Nawrodt; J. Nelson; G. Newton; E. Nishida; A. Nishizawa; J. O'Dell; B. O'Reilly; R. O'Shaughnessy; E. Ochsner; G. H. Ogin; R. Oldenburg; D. J. Ottaway; R. S. Ottens; H. Overmier; B. J. Owen; A. Page; Y. Pan; C. Pankow; M. A. Papa; P. Patel; D. Pathak; M. Pedraza; L. Pekowsky; S. Penn; C. Peralta; A. Perreca; M. Pickenpack; I. M. Pinto; M. Pitkin; H. J. Pletsch; M. V. Plissi; F. Postiglione; M. Principe; R. Prix; L. Prokhorov; O. Puncken; V. Quetschke; F. J. Raab; D. S. Rabeling; H. Radkins; P. Raffai; Z. Raics; M. Rakhmanov; V. Raymond; C. M. Reed; T. Reed; H. Rehbein; S. Reid; D. H. Reitze; R. Riesen; K. Riles; P. Roberts; N. A. Robertson; C. Robinson; E. L. Robinson; S. Roddy; C. Rver; J. Rollins; J. D. Romano; J. H. Romie; S. Rowan; A. Rdiger; K. Ryan; S. Sakata; L. Sammut; L. Sancho de la Jordana; V. Sandberg; V. Sannibale; L. Santamara; G. Santostasi; S. Saraf; P. Sarin; B. S. Sathyaprakash; S. Sato; M. Satterthwaite; P. R. Saulson; R. Savage; R. Schilling

2010-11-05T23:59:59.000Z

23

Modeling of the $\\gamma$-ray pulsed spectra of Geminga, Crab, and Vela with synchro-curvature radiation  

E-Print Network [OSTI]

$\\gamma$-ray spectra of pulsars have been mostly studied in a phenomenological way, by fitting them to a cut-off power-law function. Here, we analyze a model where pulsed emission comes from synchro-curvature processes in a gap. We calculate the variation of kinetic energy of magnetospheric particles along the gap and the associated radiated spectra, considering an effective particle distribution. We fit the phase-averaged and phase-resolved {\\em Fermi}-LAT spectra of the three brightest $\\gamma$-ray pulsars: Geminga, Crab, and Vela, and constrain the three free parameters we leave free in the model. Our best-fit models well reproduce the observed data, apart from residuals above a few GeV in some cases, range for which the inverse Compton scattering likely becomes the dominant mechanism. In any case, the flat slope at low-energy ($\\lesssim$ GeV) seen by {\\it Fermi}-LAT both in the phase-averaged and phase-resolved spectra of most pulsars, including the ones we studied, requires that most of the detected radi...

Vigan, Daniele

2015-01-01T23:59:59.000Z

24

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

25

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

26

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

SciTech Connect (OSTI)

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

27

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

28

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

29

Intrinsic Variability and Field Statistics for the Vela Pulsar: 3. Two-Component Fits and Detailed Assessment of Stochastic Growth Theory  

E-Print Network [OSTI]

The variability of the Vela pulsar (PSR B0833-45) corresponds to well-defined field statistics that vary with pulsar phase, ranging from Gaussian intensity statistics off-pulse to approximately power-law statistics in a transition region and then lognormal statistics on-pulse, excluding giant micropulses. These data are analyzed here in terms of two superposed wave populations, using a new calculation for the amplitude statistics of two vectorially-combined transverse fields. Detailed analyses show that the approximately power-law and lognormal distributions observed are fitted well at essentially all on-pulse phases by Gaussian-lognormal and double-lognormal combinations, respectively. These good fits, plus the smooth but significant variations in fit parameters across the source, provide strong evidence that the approximately power-law statistics observed in the transition region are not intrinsic. Instead, the data are consistent with normal pulsar emission having lognormal statistics at all phases. This is consistent with generation in an inhomogeneous source obeying stochastic growth theory (SGT) and with the emission mechanism being purely linear (either direct or indirect). A nonlinear mechanism is viable only if it produces lognormal statistics when suitably ensemble-averaged. Variations in the SGT fit parameters with phase imply that the radiation is relatively more variable near the pulse edges than near the center, as found in earlier work. In contrast, Vela's giant micropulses come from a very restricted phase range and have power-law statistics with indices ($6.7 \\pm 0.6$) not inconsistent with nonlinear wave collapse. These results imply that normal pulses have a different source and generation mechanism than giant micropulses, as suggested previously on other grounds.

Iver H. Cairns; P. Das; P. A. Robinson; S. Johnston

2003-04-24T23:59:59.000Z

30

VELA_COMP_OUT  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched Ferromagnetism inS-4500II Field EmissionFunctionalPortalV > 1114Pajarito Years

31

Vela | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300 South Place: Salt Lake City, Utah Zip:ScaleVegetation Jump to:Vehizero

32

Grady Electric Membership Corp | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Power BasicsGermany: Energy Resources JumpEnergyGoltry Public

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

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

E-Print Network [OSTI]

N, at ~ sate af $. g re/a1 at d1atjllel. war ly yqasee-~ ba11 vaeriie starnkl 48 hood prior ta txeataeet. 1 4, 08a 2 6, 49' 6, 8~ 3 7, 639 8, 488 4, 8' 8, 048 8, 47k 11 041 12, 368 . 8 'able 4. Rate of uptake of P3 fe&l at a cate cf l. pf uc/ml cf a 10...33. veevils starved 48 bangs prior to txeatmsnt ~ t ~ ~ ~ ~ s ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ R3 Bats of uptabs af P32 Psd at a gate of l. gf cc/ml af a lD psr cent hammy~ter solution by sCpxsxe xeaxed bail essvils nat stsrvslL prior...

Mayer, Marion Sidney

1961-01-01T23:59:59.000Z

35

Grady College Student Organizations www.uga.edu/adclub  

E-Print Network [OSTI]

from music reviews to student health to travel in Cambodia. #12;InfUSion INFUSION MAGAZINE www.uga.edu/infusion InfUSion is a quarterly, student-produced news magazine with a multicultural focus that covers topics including sports, politics, fashion, style, opinion and entertainment. InfUSion was founded by the Office

Arnold, Jonathan

36

Grady County, Georgia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,

37

THE CLE-2000 TOOL-BOX Institut de genie nucleaire  

E-Print Network [OSTI]

-mail: roy@meca.polymtl.ca December 1999 #12;Abstract In reactor physics, modern computer codes use a free to call a sequential calculation but with added flexibilities such as putting data wherever they want of the Bessel function J0(x) . . . . . . . . . . . . . . . . . . . . . . . . . . 36 4.3 Calculations based

Meunier, Michel

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

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

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41

OFF VUF-2700 FINAL REPORT VELA UNIFORM PROJECT SPONSORED BY  

Office of Legacy Management (LM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment ofDepartment ofof EnergyYou$0.C. 20545*.MSE Cores" _ ,' ,:.'' , pir.94

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

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

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces andMappingENVIRONMENTAL IMPACTApproved: 5-16-14Figure 1Carlsbad Draft08

48

CLE (CLAVATA3/ESR-like) Peptides: Roles in Cell Signaling and Stem cell Homeostasis in Arabidopsis  

E-Print Network [OSTI]

Molecular Technologies; Canberra; Australia. Fletcher J.C. (using pCAMBIA1305.2 (CAMBIA, Canberra, Australia) as the DNAusing pCAMBIA1305.2 (CAMBIA, Canberra, Australia) as the DNA

Meng, Ling

2010-01-01T23:59:59.000Z

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

Javier Vela Receives Midwest ACS Stanley Israel Award | The Ames Laboratory  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc DocumentationP-SeriesFlickrinformation forTechnologies | Blandine JeromeJason Hick

51

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

Office of Legacy Management (LM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment ofDepartment ofof EnergyYou$0.C. 20545*. . : '* FEB1f\l p :.; . I,F8 Rev.112,VUF

52

Commercial Building Indoor Environmental Quality Evaluation: Methods and Tools  

E-Print Network [OSTI]

Lorsch, H. G. , & Abdou, O. A. (1994). The impact of theBordass, 2007; Lorsch & Abdou, 1994; Singh, Syal, Grady, &

Heinzerling, David

2012-01-01T23:59:59.000Z

53

EIS-0169-SA-02: Supplement Analysis  

Broader source: Energy.gov [DOE]

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

54

Bonacum, J., R. DeSalle, P. O'Grady, D. Olivera, J. Wintermute, and M. Zilversmit. 2001. New nuclear and mitochondrial primers for systematics and comparative genomics in Drosophilidae. Dros. Inf. Serv. 84: 201-204.  

E-Print Network [OSTI]

nuclear and mitochondrial primers for systematics and comparative genomics in Drosophilidae. Dros. Inf. Serv. 84: 201-204. New nuclear and mitochondrial primers for systematics and comparative genomics of both mitochondrial (Simon et al., 1994) and nuclear (Brower and DeSalle, 1994) primers useful

O'Grady, Patrick M.

55

The MUSE-4 Experiment: Prompt Reactivity and Delayed Neutron Measurements A.Billebaud, J.Vollaire, R.Brissot, D.Heuer, C.Le Brun, E.Liatard,  

E-Print Network [OSTI]

The MUSE-4 Experiment: Prompt Reactivity and Delayed Neutron Measurements A.Billebaud, J the prompt multiplication factor kp and the delayed neutron fraction eff . kp values are obtained from time to experimental rates, the determination of the prompt multiplication factor is done. The delayed neutron fraction

Boyer, Edmond

56

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,...

57

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

58

4 Science Service Feature Released upon receipt  

E-Print Network [OSTI]

lightning was supposed to be the weapon of the go6.s. I t s cle- structive effects naturallzr suggested

59

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

60

Nuclear Physics A559 (1993) l-41 ~ortb-~ojland  

E-Print Network [OSTI]

Institute for Nucleur Research, Dubna, Head Post Cl&e, P.U. Box 79, Moscow, Russian Federation Received

Ponomarev, Vladimir

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.


61

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

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

UNIVERSIT DI BRESCIA FACOLT DI INGEGNERIA  

E-Print Network [OSTI]

a permettere la localizzazione a 360 gradi del robot da parte delle videocamere, anche di risparmiare energia studiato appositamente per essere immune alle interferenze dovute alla luce solare in spazi aperti. Al

Cassinis, Riccardo

64

LifeMapper: Open Source Geospatial Tools for the Biological Community  

E-Print Network [OSTI]

Lifemapper 2.0 Using and Creating Geospatial Data and Open Source Tools for the Biological Community Aimee Stewart, CJ Grady, Dave Vieglais, Jim Beach Natural History Museum and Biodiversity Institute University of Kansas Overview Overall Goals...

Stewart, Aimee

2007-11-14T23:59:59.000Z

65

Changing Places: How Communities Will Improve the Health of Boys of Color  

E-Print Network [OSTI]

Robert J. Blatchley, Terry Bennett-Sears, Kevin E. OGrady,Inclusion_7-28-09.pdf. Bennett, William J. , John Dilulio,Ibid. , 7. 71. Dilulio, Bennett, and Walters, Body Count.

Edley, Christopher; Ruiz de Velasco, Jorge

2010-01-01T23:59:59.000Z

66

Origins, Diversity, and Diversification of the Native Hawaiian Leafhoppers (Hemiptera: Cicadellidae: Nesophrosyne) and Their Obligate Endosymbionts  

E-Print Network [OSTI]

sp. nov. Nesophrosyne heopoko Bennett sp. nov. (Fig. 4ag)Broussaisia arguta. Coll. G.M. Bennett, P.M. OGrady, K.M.arguta. Coll. G.M. Bennett. Deposited in the BPBM, Honolulu,

Bennett IV, Gordon M.

2012-01-01T23:59:59.000Z

67

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

68

An Examination of Work to Family Spillover, Family Meal Rituals, and Parenting Styles on Children's Outcome of Obesity  

E-Print Network [OSTI]

, Mike Cummings, Ricky Bradley, Leonard Oden, Dannielle Johnson, Stacye Montez, Sonia Grady, Maurice and Lajoyce Terrell, Mr. Terrell (RIP), Andre R. Bell Sr. (My big brother). A special thanks to Richard Kendall for being a solid and loving friend...

Roberson, Samuel

2012-07-16T23:59:59.000Z

69

Response bias and aging on a recognition memory task  

E-Print Network [OSTI]

Neuropsychology, 19, 799805. Lamar, M. , Yousem, D.M. , &1997; Grady et al. , 2003; Lamar et al. , 2004) imaging, asor recognition (Buckner, 2004; Lamar et al. , 2004; Rapp &

Huh, Terri J; Kramer, Joel H; Gazzaley, Adam; Delis, Dean C

2006-01-01T23:59:59.000Z

70

BMW v. Gore: Mitigating the Punitive Economics of Punitive Damages  

E-Print Network [OSTI]

BMW v GORE: MITIGATING THE PUNITIVE ECONOMICS OF PUNITIVEE. Calfee, Mark F. Grady In BMW v Gore, the Supreme Courtadded). 480 US 102 (1987). BMW v. Gore: Mitigating the

Grady, Mark F.; Rubin, Paul H.; Calfee, John E

1997-01-01T23:59:59.000Z

71

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

72

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

73

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

74

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

75

Hydrology, environment Four remarks on the growth of channel networks  

E-Print Network [OSTI]

Hydrology, environment Four remarks on the growth of channel networks Quatre remarques sur la online xxx Presented by Ghislain de Marsily Keywords: Geomorphology Hydrology River network Mots cle

Kudrolli, Arshad

76

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

77

THE UMBRAL TRANSFER-MATRIX METHOD. IV. Counting SELF-AVOIDING POLYGONS And WALKS  

E-Print Network [OSTI]

, based on Gian-Carlo Rota's seminal notion of the umbra. In this arti* *cle we describe the Maple. 1 #12; the present case, by Gian-Carlo Rota (see [Z1]) who invented the umbra. Then th* *e task

Zeilberger, Doron

78

Selfoptimizing control of a largescale plant: The Tennessee Eastman process  

E-Print Network [OSTI]

(minimum), reactor pressure (maximum), compressor recy­ cle valve (closed), stripper steam valve (closed A. The process has five major units; a reactor, a product condenser, a vapor­liquid separator

Skogestad, Sigurd

79

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

80

Communiqu de presse Paris, le 24 novembre 2006  

E-Print Network [OSTI]

urbaniste, Lucio Costa, et un architecte, Oscar Niemeyer, résiste au temps car, près d'un demi-siècle après

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

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...

82

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...

83

851 S.W. Sixth Avenue, Suite 1100 Steve Crow 503-222-5161 Portland, Oregon 97204-1348 Executive Director 800-452-5161  

E-Print Network [OSTI]

with the monitoring of the well field as required by the ground water permit for hatchery operations. Part of the terms and conditions of the Amended Temporary Permit for the Cle Elum Hatchery Water Permit were

84

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

85

Droit de l'Environnement marin 1. Qu'est ce que le littoral marin ?  

E-Print Network [OSTI]

1681 · Code napoléon 1804 · XIX siècle :théorie de l'antipropriétarisme · XX siècle :développement du renouvellement urbain, création des SCOT) Code de l'Environnement, révision (janvier-février 2004) Loi cadre de l Mise en Valeur de laMer) Loi ...parcs nationaux, parcs naturels marins... (14 avril 2006) Principales

Boudouresque, Charles F.

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

Diagnostico de Prenez en Ganado Vacuno.  

E-Print Network [OSTI]

beneficio econ6mico derivado de la industrla fanadera depende en lucho se ha avanzado en la industria ganadera. Al... presente, un programa grande para aumentar el peso a1 destete por meclio cle selecci6n y cru- zamiento estA en progreso. El porcentaje cle I>ecerros logrados es determi- nado de \\.arias maneras. Esta pul1licaci6n considera el porcentaje de becerros 10...

Sorensen, A. M. Jr.; Beverly, J. R.; Arias, A. A.

1975-01-01T23:59:59.000Z

89

GLOBAL DISEASES: Voices from the Vanguard  

E-Print Network [OSTI]

JAMES, UNIVERSITY OF CALIFORNIA AT IRVINE Funding provided by the Center for Tropical and Emerging inc. · February 10, 2009: Dan colley, the UniverSity of GeorGia · March 17, 2009: Barney Graham, nih vaccine center · April 14, 2009: Jennifer frieDman, Brown UniverSity www.grady.uga.edu/knighthealth · www

Arnold, Jonathan

90

Climatic Change (2011) 106:93127 DOI 10.1007/s10584-010-0002-8  

E-Print Network [OSTI]

Rosenzweig · William D. Solecki · Reginald Blake · Malcolm Bowman · Craig Faris · Vivien Gornitz · Radley'Grady · Lesley Patrick · Edna Sussman · Gary Yohe · Rae Zimmerman Received: 9 March 2010 / Accepted: 8 November, NY, USA R. Blake City University of New York, New York City College of Technology, Brooklyn, NY, USA

91

THE ASTROPHYSICAL JOURNAL, 510:408412, 1999 January 1 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(  

E-Print Network [OSTI]

to that in our solar system, but it is more massive and presumably younger. Unlike the zodiacal light 45221 CAROL A. GRADY Eureka ScientiÐc, 2452 Delmer Street, Suite 100, Oakland, CA 94602 DAVID K. LYNCH1 that resembles that of the star b Pictoris and those observed in solar system comets. The structure of the band

Sitko, Michael L.

92

Recreation and Wellness Group Exercise Schedule July 1 August 16, 2013  

E-Print Network [OSTI]

THURS FRI 6:05 a.m. Cycle Cycle Robin WOW Robin Cycle Robin 12:15 p.m. C Yoga Wanda/Grady Yoga Wanda a low impact, high-energy challenge for participants of all ages, skill and fitness levels. Jump in and make a splash with this dynamic cardiovascular workout that tones and tapers the entire body. WOW

93

26473 2nd pages / 1 of 13 Following the Neoproterozoic Pan-Afri-  

E-Print Network [OSTI]

-feldspar aliquot dis- plays diffusion behavior compatible with >560 Ma cooling later affected by a heating event an abnormally steep geothermal gradi- ent to explain the complete ZFT annealing. A basal Carboniferous ages are more likely to be accurate, set- ting 1­2 km as an upper limit (depending on the geothermal

Dov, Avigad

94

Eos, Vol. 87, No. 44, 31 October 2006 The recent warming of Earth's surface is  

E-Print Network [OSTI]

is expected to increase linearly with depth with a geothermal gradi- ent determined by the subsurface thermal, subsurface temperature will depart from the linear dis- tribution.A progressive cooling at the surface://www.geo.lsa.umich/ climate).The database has been compiled as an archive of geothermal signatures of climate change

Huang, Shaopeng

95

March 28, 1995 Vol. XLVII No. 7  

E-Print Network [OSTI]

be perceived by the younger generation. She had come home to her family--her husband, 9-year-old son and 5-year' Patricia Grady To Lead Nursing Institute (See HIB VACCINES, Page 2) (See IRON MAN, Page 6) By Carla Garnett woman delegate to the United Nations, female head of the Environmental Protection Agency and, even

Bandettini, Peter A.

96

Page 1 of 3 UNIVERSITY OF BRISTOL  

E-Print Network [OSTI]

and University Secretary Members of Council Dr Andrew Garrad Mr Andrew Poolman Mr Tony Macdonald Professor Roger Horsten Prof R L Vilain Pro J A C Sterne Prof J Memmott Prof N C Norman Prof J-M Kendall Prof N Linden Dr Elmhirst Mr Ian Flavell Mr Matthew Grady Mr Charles Gunter #12;Page 3 of 3 Mr John Robert Harmer Mr Andrew

Bristol, University of

97

Division of Agricultural Sciences and Natural Resources Oklahoma State University Case Medlin  

E-Print Network [OSTI]

feeding on bull thistle. Muskthistle(Carduusnutans)(Figure2)wasfirstdocumented in Payne County, Oklahoma from the west and is known to exist in several Oklahoma counties, including Roger Mills, Custer, Love) infestations were reported in McClain and Grady counties about 25 years ago. However, those infestations were

Balasundaram, Balabhaskar "Baski"

98

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

99

mjm@nd.edu http://www.nd.edu/~mjm http://www.nd.edu/~chegdept 1 Opportunities and Challenges  

E-Print Network [OSTI]

Benefits,Air Products and Chemicals ­ 18 years at Air Products with jobs: Product manager, University://www.nd.edu/~chegdept 4 Shawn O'Grady ChEg `86 · Currently: VP Consumer Food Sales, General Mills ­ Air Products for 2 years ­ Harvard MBA, 1990 · Chose General Mills over ICI, DuPont, Air Products and Monsanto ­ Several

McCready, Mark J.

100

INSTRUCTIONS Request for Implant, Instrument or Supply for Procedure Form MM-12  

E-Print Network [OSTI]

To: Karen Grady, Materials Management Resource Manager Materials & Logistics Management Room #: LB058 ____________________________________________________ Typed Name - Mandatory Date: OFFICE MATERIALS & LOGISTICS MANAGEMENT (MLM) Reference #: Page 1 of 2 #12;SECTION 2 (To be ccompleted by Materials Management): On Contract?: Yes No If "Yes", Contract #: Product

Oliver, Douglas L.

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

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

102

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

103

Tolerant Turf: Collaborators work to improve turfgrasses' response to drought and salinity  

E-Print Network [OSTI]

genetics at the Texas AgriLife Research and Extension Center at Dallas, and researchers from #18;ve other universities have partnered with three objectives in mind#30;to develop, improve, and commercialize drought- and salinity-tolerant turfgrass. #29... in the #18;eld,? she said. Dr. Grady Miller, North Carolina State University professor and Extension turf specialist, said, ?It is critical that we #18;nd turfgrasses that can be used that require fewer inputs (water and pesticides). To meet the demand...

Smith, Courtney

2011-01-01T23:59:59.000Z

104

Grafton Electric | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady County, Place:

105

Grafton, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady County,

106

Grafton, Massachusetts: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady County,Grafton

107

Grafton, New Hampshire: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady

108

Grafton, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation,Ohio: Energy ResourcesGordon, Alabama: EnergyGowanda,Grady725522°,

109

A comparative study of collection efficiencies using 0.80 and 1.2 micrometer pore size filters in evaluating airborne asbestos dust  

E-Print Network [OSTI]

A COMPARATIVE STUDY OF COLLECTION EFFICIENCIES USING O. RO AND 1. 2 MICROMETER PORE SIZE FILTERS IN EVALUATING AIRBORNE ASBESTOS DUST A Thesis by GRADY LYNN HOLT Submitted to the Graduate College of' Texas A&M University in partial... fulfillment of the requirement for the degree of MASTER OF SCIENCE August 1974. Major Subject: Industrial Hygiene A COMPARATIVE . TUDY OF COLLECTION EFFICIENCIES USING O. BO AND 1. 2 MICROMETER PORE SIZE FILTERS IN EVALUATING AIRBORNE ASBESTOS DUST A...

Holt, Grady Lynn

1974-01-01T23:59:59.000Z

110

A review of "De lor de Virgile aux ors de Versailles: Mtamorphoses de lpope dans la seconde moiti du XVIIe sicle en France." by Luduvine Goupillaud  

E-Print Network [OSTI]

234 SEVENTEENTH-CENTURY NEWS Luduvine Goupillaud. De l?or de Virgile aux ors de Versailles: M?tamorphoses de l??pop?e dans la seconde moiti? du XVIIe si?cle en France. Travaux du Grand Si?cle 25. Geneva: Droz, 2005. 394 pp. SF 170.00. Review..., architects and orators who defined France?s classical age. That the nation sought to define itself by an epic was less evident than its prevailing desire to be known by a founding ?heroic poem.? Goupillaud shows that a first generation of inheritors...

Conley, Tom

2006-01-01T23:59:59.000Z

111

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

112

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

113

Acceleration of Energetic Particles Through Self-Generated Waves in a Decelerating Coronal Shock  

E-Print Network [OSTI]

, Finland Department of Physics, University of Helsinki, Finland Abstract. We have developed a simulation- ered the primary source of large solar energetic parti- cle (SEP) intensities. Injected particles repeatedly cross the shock front, scattering from the plasma waves, and gain energy on each crossing

Sanahuja, Blai

114

i\\ccurate and Efficient Curve Detection in Images: The Importance Sarnpling Hough Transform *  

E-Print Network [OSTI]

i\\ccurate and Efficient Curve Detection in Images: The Importance Sarnpling Hough TransformCleIJltlty UlllHlV'C curves in an image. \\Ve also use probabilistic to develop stopping conditions for the algorithm. The is called the Importance Sam- Hough Transform (ISHT). We apply our method to both simulated

Washington at Seattle, University of

115

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

116

The erosion of ductile metals by solid particles  

E-Print Network [OSTI]

results - the angular particles cause appreciably more erosion than the sl~herical, and the angle of maximum erosion is rather lower with angular parti cle s than with round shot. As mentioned above, erosive particles are nearly always harder t...

Hutchings, Ian Michael

1975-02-04T23:59:59.000Z

117

Les groupes financiers et industriels au service du roi -Espagne Fin XVIIe -dbut XVIIIe sicle  

E-Print Network [OSTI]

'une part de la puissance publique y avaient massivement recours, les évêques, les seigneurs, les villes importance au XVIIIe siècle. Voir, entre autres: Torres Sánchez (Rafael), "El gran negocio de la época, la

Paris-Sud XI, Université de

118

LES PIRATES DU CYBERART, INCONFORT TECHNIQUE ET CONTAMINATION  

E-Print Network [OSTI]

), Les oeuvres noires de l'art et de la Littérature , L'Harmattan, Paris, pp. 31-50. #12;2 LES OEUVRES-Caroline Vanbremeersch L'Harmattan, Logiques sociales - Sociologie de la connaissance L'art du noir a traversé le siècle

Paris-Sud XI, Université de

119

Les facteurs d'mergence de la mesure scientifique de l'encombrement des mnages parisiens  

E-Print Network [OSTI]

'urbanisme Français. Regards croisés de scientifiques et de professionnels 19-20ème siècle, L'Harmattan 2 Si l'on ne-1891 » Genèses, 5 ; FIJALKOW Y. (1998) La construction des îlots insalubres, Paris 1850-1945, l'Harmattan 4

Boyer, Edmond

120

Paru dans la Revue pour l'histoire du CNRS, No. 18, Automne 2007, p. 38-43 Les sciences morales et politiques : de la gloire l'oubli ?  

E-Print Network [OSTI]

.-S. Leterrier, L'institution des sciences morales, L'Harmattan, 1995 ; C. Delmas, Instituer des savoirs d'?tat : l'Académie des sciences morales au XIXe siècle, L'Harmattan, 2006 ; D. Palfrey, The Moral Science

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.


121

25Gochronique n115, 2010 Regards sur...  

E-Print Network [OSTI]

'île d'Hispaniola, plusieurs failles absor- bent le déplacement relatif oblique, de 2 cm/an, entre ces- ments destructeurs qui a affecté le sud d'Hispaniola au 18e siècle (1751a, 1751b, 1770). En janvier 2010

Lacassin, Robin

122

2006 Nature Publishing Group Controlled multiple reversals of a ratchet effect  

E-Print Network [OSTI]

2006 Nature Publishing Group Controlled multiple reversals of a ratchet effect Clecio C. de confined in an asymmetric potential demon- strates an anticipated ratchet effect by drifting along the `easy' ratchet direction when subjected to non-equilibrium fluctu- ations13 . This well-known effect

Moshchalkov, Victor V.

123

1. QMM. Sputmsc. Radial. Transfer Vol. 23, pp. 545-573 Pergmon Press Ltd., 1980. Prinkd in Great Britain  

E-Print Network [OSTI]

+ &+#J(v, CL)e+ dv + &(T, CL). (3) -I tpermanent address: Instituto de Energia AtGmica,Cidade Universitaria, Sgo Paulo, Brasil. 565 #12;566 Here C. E. SIEWERT etal. `h(x)= $4x.XL and the polynomials g

Siewert, Charles E.

124

Accuracy of Memory Reference Traces of Parallel Computations  

E-Print Network [OSTI]

, the trace-driven simulator uses the intrinsic traces and the sequence of loads and stores before the current cy- cle, to determine the next address. The mapping between load and store sequences and next addresses to issue, sometimes, requires partial program reexecution. Programs that do not require partial

Holliday, Mark A.

125

Mass and spin content of a free relativistic particle of arbitrary spins and the group  

E-Print Network [OSTI]

of particles with several spins and masses which can exist in positive as well as negative energy states Postal 20-364, 01000 Mexico D. F., Mexico 2 Instituto de Ciencias Nucleares, UNAM, Apdo. Postal 70 approach to the free parti- cle of arbitrary spins whose relativistic equation can be obtained from

Nikitin, Anatoly

126

Please cite this article in press as: A.P. Hitchcock, et al., J. Electron Spectrosc. Relat. Phenom. (2009), doi:10.1016/j.elspec.2009.12.002 ARTICLE IN PRESS  

E-Print Network [OSTI]

beam energy exhibits multiple peaks at positions which depend on the nuclear mass of the elementsV incident energy, 20 a.u.). The peak positions agree completely with those predicted by classical of energy and momentum in binary collisions of the incident parti- cle within the assumption

Hitchcock, Adam P.

2009-01-01T23:59:59.000Z

127

Journal of Electron Spectroscopy and Related Phenomena 181 (2010) 135139 Contents lists available at ScienceDirect  

E-Print Network [OSTI]

beam energy exhibits multiple peaks at positions which depend on the nuclear mass of the elements, 2.25 keV incident energy, 20 a.u.). The peak positions agree completely with those predicted of energy and momentum in binary collisions of the incident parti- cle within the assumption

Hitchcock, Adam P.

2010-01-01T23:59:59.000Z

128

Observation of intermittency in gene expression on cDNA microarrays  

E-Print Network [OSTI]

, Texas 77030 2 Department of Physics, University of Houston, Texas 77204 May 14, 2002 Abstract We used Scaled factorial moments have found widespread use in high-energy physics for detecting intermittency in parti- cle production [1-10]. The presence of jet-like structures and perhaps quark-gluon plasma phase

129

Very preliminary H4 Beamtest Summary  

E-Print Network [OSTI]

acceptance angle: c = 2U0 pv Poten8al well depth Par8cle energy Deflec8on angle is the bending angle 8000 10000 Energy (ADC values) Log (Entries) Muons Hadrons Beam energy ~ 150 GeV Horizontal beam

130

851 S.W. Sixth Avenue, Suite 1100 Steve Crow 503-222-5161 Portland, Oregon 97204-1348 Executive Director 800-452-5161  

E-Print Network [OSTI]

of the four natural lakes that produced them was dammed for irrigation water storage. The summer Chinook, and sockeye salmon into the Yakima Basin. Historically there were six stocks of Pacific salmon produced implemented for each of these species. Sockeye salmon adults that were naturally produced in the Cle Elum

131

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

132

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

133

Error Estimation And Accurate Mapping Based ALE Formulation For 3D Simulation Of Friction Stir Welding  

E-Print Network [OSTI]

Welding Simon Guerdoux, Lionel Fourment* CEMEF, Mines cle Paris, BP 207, 06 904 Sophia Antipolis Ceclex) formulation is developed to simulate the different stages of the Friction Stir Welding (FSW) process standard approaches. The proposed ALE formulation is applied to FSW simulation. Steady state welding

Paris-Sud XI, Université de

134

Journal of Power Sources xxx (2005) xxxxxx Vehicle-to-grid power implementation: From stabilizing the  

E-Print Network [OSTI]

December 2004 Abstract Vehicle-to-grid power (V2G) uses electric-drive vehicles (battery, fuel cell fleet with the electric power system. The vehicle fleet has 20 times the power capacity, less than one for electric-drive vehicles used to provide power for several power markets. This arti- cle quantitatively

Firestone, Jeremy

135

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

136

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

137

JOINT ACOUSTIC-VIDEO FINGERPRINTING OF VEHICLES, PART II , F. Guo, A. C. Sankaranarayanan, and R. Chellappa  

E-Print Network [OSTI]

JOINT ACOUSTIC-VIDEO FINGERPRINTING OF VEHICLES, PART II V. Cevher , F. Guo, A. C. Sankaranarayanan, and R. Chellappa Center for Automation Research, University of Maryland, College Park, MD 20742 {volkan the wheelbase length of a vehicle using line metrology in video. We then address the vehi- cle fingerprinting

Cevher, Volkan

138

Transportation S e m i n a r S e r i e s  

E-Print Network [OSTI]

of the history of bicycling policy in Davis; a behavioral study of factors contributing to high levels of Davis as a bicy community. ll cle Susan Handy is a professor in the Department of Environmental Science for her work on the impact of neighborhood design on travel behavior. She serves on three committees

Bertini, Robert L.

139

OneBusAway: Results from Providing Real-Time Arrival Information for Public Transit  

E-Print Network [OSTI]

]. Use of public transportation reduced U.S. CO2 emissions by 6.9 million metric tons in 2005 [18]. While hybrid and electric vehi- cle technologies can reduce the carbon-footprint of single- occupancy vehicles@cs.washington.edu ABSTRACT Public transit systems play an important role in combating traffic congestion, reducing carbon

Anderson, Richard

140

MAGIC A YEAR-LONG INVESTIGATION OF MARINE CLOUDS IN THE PACIFIC  

E-Print Network [OSTI]

of Washington, Seattle, WA For presentation at the SOLAS Open Science Conference, Cle Elum, WA May 7-10, 2012 of Energy Office of Science Managed by Brookhaven Science Associates, LLC for the United States Department of Energy under Contract No. DE-AC02-98CH10886 ABSTRACT The MAGIC project will deploy the Second ARM

Homes, Christopher C.

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

Communiqu de presse 15 novembre 2013 L'Herbier du Musum  

E-Print Network [OSTI]

, que le chantier de rénovation tout juste achevé fait entrer de plain- pied dans le XXI e siècle. Les classification, l'introduction et la disparition des espèces. Il présente les portraits des grands botanistes qui

142

UNITED STATES DEPARTMENT OF THE INTERIOR FISH AND WILDLIFE SERVICE  

E-Print Network [OSTI]

Biochemical indices of quality. . . . . . . . . . . 6 Engineering studies on freezing and cold storage systems . · · . . . . . . . · . . . . . . . . . . . . 4 Storage of fish in refrigerated sea water . . . 5 Time-temperature tolerance of frozen seafoods 5 to meet the needs of industry. Funda- ment al research has been continued in the field of fish - mus cle

143

China's Space Robotic Arms Programs  

E-Print Network [OSTI]

innovation-and-technology-in-china/sitc-publications/. 34Andrea Shalal-Esa, U.S. Sees China Launch as Test of Anti-arti- cle/2013/05/15/us-china-launch-idUSBRE94E07D20130515.

POLLPETER, Kevin

2013-01-01T23:59:59.000Z

144

A quantitative analysis of benthic polychaetous annelids from the northwestern Gulf of Mexico  

E-Print Network [OSTI]

area / / 'y 2o L 1 Figure 1 '. 'p shomi. n, loca Gn of stat ons ' -. sos ar . I sir, lti "1e J r s to s' c illevt t1': gioclp 8 polyc lad. e-a-sr-'. Slaps-proup: Gr up A, cle/ ?-sard', :, roun ll loha are ri sf@hated ' ? a trier ';. . Stole 3 lc...

Hubbard, Guinn Fain

1977-01-01T23:59:59.000Z

145

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

146

Towards a Conceptual Model of a Bio-Robotic AUV: Pectoral Fin Hydrodynamics  

E-Print Network [OSTI]

of these technological problems whereas the FY03 ONR MURI program (Integrated Artificial Mus- cle, High-Lift Bio of marine mammals systems (MMS), specifically dolphins. The key technological advances required in order to reach this goal are: 1) An engineered sonar system that matches the perfor- mance of MMS. 2) An AUV

Mittal, Rajat

147

Towards DRAGON Version4 Institut de genie nucleaire  

E-Print Network [OSTI]

Version4 is a new distribution of the reactor physics computer codes at GAN. Its components are: DRAGR module in NJOY and Python script PyNjoy.py Ganlib tools (CLE-2000, LCM/XSM API) Modules (calculation operators) of the following codes: Dragon: lattice code Trivac: reactor (full core) code Donjon: simulation

Meunier, Michel

148

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

149

Atmos. Chem. Phys., 10, 947959, 2010 www.atmos-chem-phys.net/10/947/2010/  

E-Print Network [OSTI]

-cloud or aerosol droplet process (PKU 80%, Yufa 70%) and gas condensation process (PKU 14%, Yufa 22%). According accounted for more than 50% in fine par- ticles. PMF model analysis was used to resolve the parti- cle modes. Three modes were resolved at Yufa, represent- ing condensation, droplet and coarse mode. However, one

Meskhidze, Nicholas

150

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

151

Larry Cox, ljcox@lanl.gov, (505) 665-7344 One important applica.on domain is Monte  

E-Print Network [OSTI]

.on shielding, radiography, medical physics, cri.cality safety, nuclear oil well logging, isotope produc.on, accelerator target design, fission and fusion reactor design, and decontamina.on and decommissioning of nuclear facili.es. The goal of this effort is to define a neutralpar.cle (n, ) MC package tailored

152

An H minority heating regime in Tore Supra showing improved L mode confinement  

E-Print Network [OSTI]

on the plasma facing components, parti- cle control through pumping and thermalization of fast particles for the next tokamak generation. High energy confinement will also be required for fusion reactor operation to the magnetic axis. The working gas is either deuterium or helium. The density is raised by gas puffing

Budny, Robert

153

LASER & PHOTONICS www.lpr-journal.org  

E-Print Network [OSTI]

, electronic warfare, and medical diagnostics systems. Continually extending the bandwidth of digitizers has hence become a central challenge in electronics. Fortunately, it has been shown that photonic pre-processing of wideband signals can boost the performance of electronic digitizers. In this arti- cle, the underlying

Jalali. Bahram

154

Fig. 6. Plots of temperature increase at the center of nanoparticle lattice as a function of particle spacing. These fit shown in the figure is a power law,  

E-Print Network [OSTI]

of particles. Simula'ons of Nanopar'cle Hea'ng for Remote S'mula'on of Cells Katherine: kspoth@buffalo.edu, apralle@buffalo.edu Abstract Nanoparticles heated in alternating magnetic field for more efficient heating on cell surfaces. To better understand particle heating in this configuration

Pralle, Arnd

155

A review of biomass integrated-gasifier/gas turbine combined cycle technology and its  

E-Print Network [OSTI]

A review of biomass integrated-gasifier/gas turbine combined cycle technology and its application Copersucar, CP 162, Piracicaba, SP ­ Brazil ­ 13400-970 Biomass integrated-gasifier/gas turbine combined-from-sugarcane program. 1. Introduction The biomass integrated-gasifier/gas turbine combined cy- cle (BIG

156

Marges linguistiques -Numro 10, Novembre 2005 -M.L.M.S. diteur http://www.marges-linguistiques.com -13250 Saint-Chamas (France)  

E-Print Network [OSTI]

commun guyanais découpe en effet la population présente sur le département en différents groupes aux Marrons, descendants d'esclaves ayant fui les plantations du Surinam voisin au XVIIIe siècle, perçus

Paris-Sud XI, Université de

157

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

158

LANL: AOT & LANSCE The Pulse November 2010  

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

titAnium voltAge bArs 5 los AlAmos lenDs its exPertise to cleAn energy AnD cArbon sequestrAtion Projects 6 electric-FielD moDiFicA- tion oF mAgnetism in A thin Film...

159

seari.mit.edu SEAri Working Paper Series  

E-Print Network [OSTI]

- cle (MAV) is a less-than-one-pound unmanned air system equipped with a visual sensor. Con- ceptual and of high energy density power supplies. Based on these uncertainties, several change scenar- ios were. A change in the endurance require- ment to allow entry into a new market (CS#3) #12;Systems Engineering

de Weck, Olivier L.

160

2014Staff Learning & DeveLopment reSource guiDe for acaDemic & paSS Staff  

E-Print Network [OSTI]

CREATINgTHELEADINgEDgE(CLE):REgIONAL MANAGEMENT DEVELOPMENT PROGRAM: CHEC 34 LEADERSHIP PART 1: PERSONAL: MANAGING SUBSTANCE ABUSE 41 PPS FOR MANAGERS OF PASS STAFF 42 personal leadership skills 43 ASSERTIVENESS RESEARCH CONTRACTS & INTELLECTUAL PROPERTY INDUCTION 54 resoUrce managemenT 55 UNDERSTANDING BASIC

Jarrett, Thomas H.

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

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

162

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

163

Thaisa Storchi Bergmann Instituto de Fsica UFRGS  

E-Print Network [OSTI]

, 2011 #12;Unidades e métodos de determinação de distâncias Tamanhos no Sistema Solar Tamanho das Olbers O Conteúdo do Universo A matéria e energia escuras Questões O tamanho, idade e conteúdo do Astronômicas · Sistema Solar próximo: radar · Estrelas próximas: paralaxe #12;· Estrelas e galáxias: velas

dos Santos, C.A.

164

arXiv:0711.2528v2[astro-ph]23Jan2008 Production of Neutrinos and Secondary Electrons in Cosmic  

E-Print Network [OSTI]

of secondary electrons in a young shell-type SNR, RX J1713.7-3946, which is a measure of the age, the spectral-mG fields recently invoked to explain the X-ray flux variations are unlikely to extend over a large fractionCube-like detector that are induced by muon neutrinos from high-energy -ray sources such as RX J1713.7-3946, Vela Jr

165

Safe Handling of Fresh Fruits and Vegetables (Spanish)  

E-Print Network [OSTI]

temperatura ambiental por m?s de dos horas, des?chelos. Recuerde: Para prevenir enfermedades alimenticias, compre frutas y verduras de buena calidad, almac?nelas adecuadamente y l?velas completamente. Producido por AgriLife Communications, El Sistema...*Especialista de Programa, El Sistema Texas A&M Las frutas y verduras frescas son una parte importante de una dieta saludable. ?stas proveen vitaminas, minerales y fibras para ayudar a mantener su cuerpo saludable. A veces, las frutas y...

Scott, Amanda

2008-09-05T23:59:59.000Z

166

X-rays from Supernova Remnants  

E-Print Network [OSTI]

A summary of X-ray observations of supernova remnants is presented including the explosion fragment A of the Vela SNR, Tycho, N132D, RX J0852-4622, the Crab Nebula and the 'bulls eye', and SN 1987A, high-lighting the progress made with Chandra and XMM-Newton and touching upon the questions which arise from these observations and which might inspire future research.

B. Aschenbach

2002-08-28T23:59:59.000Z

167

Effects of directional epistasis on molecular evolution  

E-Print Network [OSTI]

N? = 0.04 2Nr = 0 2Nr = 1 0 0.01 0.02 0.03 0.04 0.05 0 0.1 0.2 0.3 0.4 0.5 0.6 Average equilibrium frequency of deleterious alleles Nu cle oti de di ver sit y y 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 di ve ris ty y Figure 3. Nucleotide diversity under different selection scenarios. In each graph, the two groups of plots are for the cases with no recombination and with 2Nr...

Gong, Qin Qin

2009-04-24T23:59:59.000Z

168

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

169

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

E-Print Network [OSTI]

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... Detection of Shock Waves Page 38 Sensitivity of Occupancy Measurements 38 Occupancy Differential Concept Determination of' Occupancy D"' fzerence Parameters Det, ection of Shock Waves 41 RESULTS Critical Occupancy Concept Determination of Critical...

Friebele, John Duncan

1972-01-01T23:59:59.000Z

170

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

171

Appel contributions L'Universit Euro-Mditerranenne de Fs et l'Institut  

E-Print Network [OSTI]

tendances. L'atelier Au cours de la seconde moitié du siècle dernier, le Maroc est devenu l'un des concerne les migrations qualifiées. Depuis 1995, le Maroc a ainsi devancé la Turquie comme principale source de main-d'oeuvre immigrée en Europe. Cependant, le rôle du Maroc dans le système migratoire euro

Oxford, University of

172

Valence hroque : premiers pomes piques espagnols de la fin du rgne de Charles-Quint (Nicols Espinosa et Francisco Garrido de Villena, 1555)  

E-Print Network [OSTI]

XVIè siècle (1504-1517), consacra à la ville qui l'accueillait un poème panégyrique, d'abord en latin Romance heroico en loor de la ciudad de Valencia, il dégage cinq caractéristiques glorieuses de la ville, Andrés Sánchez Robayna (ed.), Las Palmas de Gran Canaria : Academia Canaria de la Historia, 2010, p. 189

Paris-Sud XI, Université de

173

De Tolde Zamora, l'errance des reliques de saint Ildephonse au Moyen ge  

E-Print Network [OSTI]

reliques de saint Ildephonse dans la ville de Zamora. Mais que pouvait bien faire à cet endroit reculé la hispánicos más ilustres en un rincón tan olvidado? Lo cierto es que el descubrimiento causó una gran la ville de León, l'urbs regia du xie siècle, et à la transformer en un

Boyer, Edmond

174

Site Battelle, Bt. A -7 route de Drize -CH-1227 Carouge Tl. 022 379 07 70 -Fax 022 379 07 71 -http://www.unige.ch/environnement/index.html  

E-Print Network [OSTI]

/ Alain Cluzet. ­ Paris : L'Harmattan, 2010. ­ 189 p. ­ ISBN 978­229­611­6481. vtls005474111 GE ISE : rez'équipe de l'encyclopédie du développement durable. ­ Paris : Ed. L'Harmattan : Récollets, 2010. ­ 192 p XXIe siècle ? / Mathieu Baudin. ­ Paris : L'Harmattan, 2009. ­ 102 p. : ill. ­ (Prospective). ­ ISBN

Laemmli, Ulrich

175

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

176

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

177

Marginalit biogographique et rsilience Le territoire forestier insulaire du Fleuve Uruguay, 1800-2000.  

E-Print Network [OSTI]

1 Marginalité biogéographique et résilience Le territoire forestier insulaire du Fleuve Uruguay Uruguay, 1800-2000. Colloque « La nature a-t-elle encore une place dans les milieux géographiques territoires forestiers. Dans les îles de l'Uruguay, exploitées dès le XVIIè siècle pour leur bois, si rare

Paris-Sud XI, Université de

178

02 Hoffmann 1 Hoffmann, Odile, 2000, "Jeux de parole et de mmoire autour des mobilisations identitaires dans  

E-Print Network [OSTI]

lieux, de rivières qu'ils habitent depuis plus d'un siècle sans titres fonciers, le "deviennent" pour s titres fonciers collectifs aux "communautés noires riveraines du Pacifique". Pour des raisons du même au contraire après une profonde mutation de leurs valeurs racistes (la côte nord du Nariño). Des

Paris-Sud XI, Université de

179

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

180

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

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

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

182

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

183

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...

184

Design criteria for centripeter aerosol samplers  

E-Print Network [OSTI]

, the model centripeter consists of seven parts: the acceleration nozzle, the collection nozzle, the large parti- cle conveyance tube, the small particle transport chamber, the main hou- sing, the 47 mm diameter large particle collection filter holder... of model centripeter sampler 13 matter was increased. It then flowed into the separation zone which is essentially the gap between the acceleration nozzle discharge plane and the intake of the collection nozzle. The large particles which, due to high...

King, Connie Hazel

1977-01-01T23:59:59.000Z

185

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

186

Version finale avant publication. Publie in Weller Jean-Marc, Comment ranger son bureau ? Le fonctionnaire, l'agriculteur, le droit et l'argent , Rseaux, 2012/1 n 171, p. 67-101. DOI  

E-Print Network [OSTI]

, croulant sous d'improbables piles de papiers mais jurant qu'il ne faut rien toucher à ce désordre, sous prétexte qu'il dissimulerait, en vérité, un ordonnancement délicat ? La question du rangement peut paraître incroyable phénomène qu'est l'invention du « bureau moderne ». Né au tournant du siècle dernier, il s

Boyer, Edmond

187

.LE TERRITOIRE DANS LES STRATGIES DE GESTION DE L'EAU De l'intgration sectorielle l'intgration des territoires au Maroc  

E-Print Network [OSTI]

, ils ont été limités à l'analyse du territoire structuré par le réseau hydraulique sans questionner les structuration de territoires distincts : la ville, la plaine et la montagne1 . Dès le XIIème siècle, l'établissement du pouvoir central dans la plaine, à travers le captage et la distribution de l'eau, a profondément

Boyer, Edmond

188

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

189

ROLE OF FUSION ENERGY FOR THE 21 CENTURY ENERGY MARKET AND DEVELOPMENT STRATEGY WITH INTERNATIONAL THERMONUCLEAR EXPERIMENTAL  

E-Print Network [OSTI]

THERMONUCLEAR EXPERIMENTAL REACTOR Rôle de l'énergie de fusion dans la production énergétique du 21 e siècle etROLE OF FUSION ENERGY FOR THE 21 CENTURY ENERGY MARKET AND DEVELOPMENT STRATEGY WITH INTERNATIONAL be improved to contribute to this issue. Fusion is an energy source of the Sun and the Star. It is a quite

190

Exclusive hadronic B decays to charm and charmonium final states  

E-Print Network [OSTI]

. Ogg, D.I. Britton, E.R.F. Hyatt, D.B. MacFarlane, P.M. Patel, D.S. Akerib, B. Barjsh M. Chadha S. Chan D.F. Cowen G. Ejgen J.S. Mjller C. O' Grady J. Urhejm A.J. Weinstein, D. Acosta, M. Athanas, G. Masek, H.P. Paar, J. Gronberg, R. Kutschke, S. Menary... resolution. De- pending on the B decay mode, o~E, the rms resolution on the energy di8'erence AE = Ebeam Emeas from 8 to 46 MeV. The modes considered and the cor- responding o~E values are given in Tables IIIVII and Tables IXX. VA divide the B candidates...

Ammar, Raymond G.; Ball, S.; Baringer, Philip S.; Bean, Alice; Besson, David Zeke; Coppage, Don; Copty, N.; Davis, Robin E. P.; Hancock, N.; Kelly, M.; Kwak, Nowhan; Lam, H.

1994-07-01T23:59:59.000Z

191

Pulsar Braking Index and Mass Accretion  

E-Print Network [OSTI]

I show that the braking index, $N$, a fundamental pulsar experimental quantity, naturally differs from the canonical value of 3 by terms which involve mass accretion. Using the measured values of $N$ for PSR1509-58 and PSR0531+21, I determine that for constant density neutron stars their present mass accretion rates are $(3.10\\pm.51)\\times10^{-5}$ M year$^{-1}$ and $(9.946\\pm.089)\\times10^{-5}$ M year$^{-1}$ respectively, where M is the mass of each pulsar. Finally, I demonstrate that mass accretion removes the outstanding problem of the origin of the big glitches of the Vela Pulsar.

P. D. Morley

1993-11-15T23:59:59.000Z

192

Langues et Mdia au Maroc dans la premire dcennie du XXIme sicle : la monte irrsistible de la drija ?  

E-Print Network [OSTI]

Langues et Média au Maroc dans la première décennie du XXIème siècle : la montée irrésistible de la séries télévisuelles en arabe marocain est une nouveauté au Maroc, initié par TV2M en Mai 2009 avec le certains milieux intellectuels ou politiques défendant la place de larabe standard au Maroc. Pourtant

Paris-Sud XI, Université de

193

Areal distribution of clay minerals and their relationship to physical properties, Gulf of Mexico  

E-Print Network [OSTI]

of the first major works examining physical properties of Gulf of Mexico sediments was by Fisk and McCle lland (1959). They dis- cussed the influence of the geology of the Louisiana continental shelf on offshore foundation design, They showed that foundation... of the variation in shear strength can be attributed to either depth in core or to a change in water content. Bouma et a!. (1972) showed the importance of geo- technical investigation through their comparison of geological and engineering parameters of marine...

Hottman, William Edward

1975-01-01T23:59:59.000Z

194

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

195

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

196

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

197

Farm records: a study of their relationship to farm management and federal income taxation.  

E-Print Network [OSTI]

charges incurred in acquirin' the 6o . ds vill m ice up the inventory value. In ce. . e of products produced on the f- rm th~ co. t b. si. will include co. t of raw m=. teri-l;, dir~ct labor =nd indirect expenses. l For ex mple, the co. t of . e..., to ~irect 1-)or for the entire farm ~nd pplying thi. ratio to the di- rect 1;, tor cost for the 10 acre plot, Indirect expense. m. , y be lioc. :t~d by any m thod which will conform to -cce. ted accountin~ pr ctice an& cle rly reflect. income, ' 1 Feder...

Warren, Steve Pearce

1949-01-01T23:59:59.000Z

198

Impurity-induced local density of states in a d-wave superconductor carrying a supercurrent  

E-Print Network [OSTI]

2sqs,ivnd ? asqs,ivndbsqs,ivnd . s5d Obviously, when a supercurrent is applied, the quasiparti- cle energy has a momentum-dependent shift 1 /2sek+qs ?e ?k+qsd fsee the bare Green?s function Gkn0 sqs , ivnd in Eq.s5dg, which leads to different... of the bias energies and the strength of Js, and it has the strongest intensity at the sites next to the defect when the quasiparticle energy sor the bias voltage times ed v=0 meV fsee Fig. 2scd s0dg. Near the impurity, the LDOS has a pattern of fourfold...

Zhang, DG; Ting, CS; Hu, Chia-Ren.

2005-01-01T23:59:59.000Z

199

The effects of source, levels and method of feeding calcium on the performance of commercial layers  

E-Print Network [OSTI]

, 75 and 3. bO noucent). '. ~a~ac dj ets co?uIraj n, . d calcium fnom lie&os tone at the basic lovel "; three diets contained cajc j um f corn oyster shell at the basic levels; and three diets contained lime- stone at the basic levels plus... the calcium level in th diets was in- creased. The ser um calcium level was also increased with increased dietar y calcj. um levels. Thor e ~;, cl'e fee dif for er ces in pr oduc tioir f rc t or s ?hon t:-os tsrent ane cosrpai'od, but ogg quality rras j...

Walker, Jerry Charles

2012-06-07T23:59:59.000Z

200

Mining Users' Significant Driving Routes with Low-power Sensors  

E-Print Network [OSTI]

sensing [38] from low power sensors, the energy cost of location sensing is high when location sensors are active. It is also possible for the phone to be plugged in a charging port in the vehi- cle during journeys but this places an extra constraint... on the user to remember to plug the phone in during each journey for energy intensive location sensing. Significantly lower- ing the energy consumption of sensing these journeys will relieve the user of this requirement and thus make it more likely...

Nawaz, Sarfraz; Mascolo, Cecilia

2014-01-01T23:59:59.000Z

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.


201

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

202

Evaluation of a reduced mechanism for turbulent premixed combustion  

E-Print Network [OSTI]

as alternative fuels for power generation using indus- trial gas-turbines [1]. These are typically multi-component fuels, involving CO; H2; H2O; CH4; CO2; O2 and N2, with their composi- reaction set usually involves more than hundreds of reactions and tens... ]. The supplementary material of this arti- cle provides a CHEMKIN compatible subroutine to calculate these reaction rates. 2.3. Flow configuration and boundary conditions A sketch of the computational domain is given in Fig. 1. The computational domain is discretized...

Nikolaou, Zacharias M.; Swaminathan, Nedunchezhian; Chen, Jyh-Yuan

2014-07-21T23:59:59.000Z

203

Development and application of a high speed digital data acquisition technique to study steam bubble collapse using particle image velocimetry  

E-Print Network [OSTI]

John Poston ( Head of Department ) ABSTRACT Development anil Appl&cat&on of a. H&vh Speed D&g&tal Data A?qu&s&t&on Techn&que to Study Steam Bubble & 'ollapse us&ng Part&cle Image L'elo imetry I August 1090) K&)liam Dan&el Schr&n Jl. B S . 1&nited... vnth the practical applicatloils of the hardware used in this prelect. TABLE OF CONTENTS CHAPTER Page I INTRODUCTION I 1 Background I 9 Background for Pulsed Laser Velocimetry I 3 tlethodnlogy for Particle Image Velocimetry 14 Background...

Schmidl, William Daniel

1992-01-01T23:59:59.000Z

204

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

205

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

206

Thermal structure and cooling of neutron stars with magnetized envelopes  

E-Print Network [OSTI]

The thermal structure of neutron stars with magnetized envelopes is studied using modern physics input. The relation between the internal (T_i) and local surface temperatures is calculated and fitted by analytic expressions for magnetic field strengths B from 0 to 10^{16} G and arbitrary inclination of the field lines to the surface. The luminosity of a neutron star with dipole magnetic field is calculated and fitted as a function of B, T_i, stellar mass and radius. In addition, we simulate cooling of neutron stars with magnetized envelopes. In particular, we analyse ultramagnetized envelopes of magnetars and also the effects of the magnetic field of the Vela pulsar on the determination of critical temperatures of neutron and proton superfluids in its core.

A. Y. Potekhin; D. G. Yakovlev

2001-06-19T23:59:59.000Z

207

Improving the Angular Resolution of EGRET and New Limits on Supersymmetric Dark Matter Near the Galactic Center  

E-Print Network [OSTI]

Using the EGRET data and an improved point source analysis, including an energy dependent point spread function and an unbinned maximum likelihood technique, we have been able to place considerably lower limits on the gamma ray flux from the galactic center region. We also test this method on known sources, the Crab and Vela pulsars. In both cases, we find that our method improves the angular precision of EGRET data over the 3EG catalog. This new limit on gamma rays from the galactic center can be used to test models of annihilating supersymmetric dark matter and galactic halo profiles. We find that the present EGRET data can limit many supersymmetric models if the density of the galactic dark matter halo is cuspy or spiked toward the galactic center. We also discuss the ability of GLAST to test these models.

Hooper, D; Hooper, Dan; Dingus, Brenda

2002-01-01T23:59:59.000Z

208

Improving the Angular Resolution of EGRET and New Limits on Supersymmetric Dark Matter Near the Galactic Center  

E-Print Network [OSTI]

Using the EGRET data and an improved point source analysis, including an energy dependent point spread function and an unbinned maximum likelihood technique, we have been able to place considerably lower limits on the gamma ray flux from the galactic center region. We also test this method on known sources, the Crab and Vela pulsars. In both cases, we find that our method improves the angular precision of EGRET data over the 3EG catalog. This new limit on gamma rays from the galactic center can be used to test models of annihilating supersymmetric dark matter and galactic halo profiles. We find that the present EGRET data can limit many supersymmetric models if the density of the galactic dark matter halo is cuspy or spiked toward the galactic center. We also discuss the ability of GLAST to test these models.

Dan Hooper; Brenda Dingus

2002-12-20T23:59:59.000Z

209

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.

D. M. Pandya; V. O. Thomas; R. Sharma

2014-11-20T23:59:59.000Z

210

Analysis of Arithmetic Coding for Data Compression  

E-Print Network [OSTI]

appears in the analysis of enumerative codes by Cleary and Witten #5B7#5D. The resulting code length for a semi-adaptive decrementing code is L SD = ,lg #20#20 k Y i=1 c i ! ! #1E t! ! : #281#29 It is straightforward to show that for all input #0Cles... then the overhead will increase the code length by only about #28k=B#29lg#28B=k#29 bits per input symbol, less than 0.1 bit per symbol for a typical #0Cle. We conclude that the bene#0Cts of scaling usually outweigh the minor ine#0Eciencies it sometimes introduces. 2.2...

Howard, Paul G.; Vitter, Jeffrey Scott

1992-01-01T23:59:59.000Z

211

Regmi Research Series ,Year 4, January 1, 1972  

E-Print Network [OSTI]

"ion : in thcleAr thet ~l1bN Dh.."lukal 51ngh had been' !!PP')intcd 3S an IjaradJr, or r~)venuc farmer, ntthoueh e copy ot t .bt: lctk:r ot appointment is not av .... llabl~ . It c...

Regmi, Mahesh C

1972-01-01T23:59:59.000Z

212

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

213

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

214

LINEAR RELATION FOR WIND-BLOWN BUBBLE SIZES OF MAIN-SEQUENCE OB STARS IN A MOLECULAR ENVIRONMENT AND IMPLICATION FOR SUPERNOVA PROGENITORS  

SciTech Connect (OSTI)

We find a linear relationship between the size of a massive star's main-sequence bubble in a molecular environment and the star's initial mass: R{sub b} Almost-Equal-To 1.22 M/M{sub Sun} - 9.16 pc, assuming a constant interclump pressure. Since stars in the mass range of 8 to 25-30 M{sub Sun} will end their evolution in the red supergiant phase without launching a Wolf-Rayet wind, the main-sequence wind-blown bubbles are mainly responsible for the extent of molecular gas cavities, while the effect of the photoionization is comparatively small. This linear relation can thus be used to infer the masses of the massive star progenitors of supernova remnants (SNRs) that are discovered to evolve in molecular cavities, while few other means are available for inferring the properties of SNR progenitors. We have used this method to estimate the initial masses of the progenitors of eight SNRs: Kes 69, Kes 75, Kes 78, 3C 396, 3C 397, HC 40, Vela, and RX J1713-3946.

Chen Yang; Zhou Ping [Department of Astronomy, Nanjing University, Nanjing 210093 (China); Chu Youhua [Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States)

2013-05-20T23:59:59.000Z

215

Gravitational waves from known pulsars: results from the initial detector era  

E-Print Network [OSTI]

We present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo. We do not see evidence for gravitational wave emission from any of the targeted sources but produce upper limits on the emission amplitude. We highlight the results from seven young pulsars with large spin-down luminosities. We reach within a factor of five of the canonical spin-down limit for all seven of these, whilst for the Crab and Vela pulsars we further surpass their spin-down limits. We present new or updated limits for 172 other pulsars (including both young and millisecond pulsars). Now that the detectors are undergoing major upgrades, and, for completeness, we bring together all of the most up-to-date results from all pulsars searched for during the operations of the first-generation LIGO, Virgo and GEO600 detectors. This gives a total of 195 pulsars including the most recent results described in this paper.

J. Aasi; J. Abadie; B. P. Abbott; R. Abbott; T. Abbott; M. R. Abernathy; T. Accadia; F. Acernese; C. Adams; T. Adams; R. X. Adhikari; C. Affeldt; M. Agathos; N. Aggarwal; O. D. Aguiar; P. Ajith; B. Allen; A. Allocca; E. Amador Ceron; D. Amariutei; R. A. Anderson; S. B. Anderson; W. G. Anderson; K. Arai; M. C. Araya; C. Arceneaux; J. Areeda; S. Ast; S. M. Aston; P. Astone; P. Aufmuth; C. Aulbert; L. Austin; B. E. Aylott; S. Babak; P. T. Baker; G. Ballardin; S. W. Ballmer; J. C. Barayoga; D. Barker; S. H. Barnum; F. Barone; B. Barr; L. Barsotti; M. Barsuglia; M. A. Barton; I. Bartos; R. Bassiri; A. Basti; J. Batch; J. Bauchrowitz; Th. S. Bauer; M. Bebronne; B. Behnke; M. Bejger; M. G. Beker; A. S. Bell; C. Bell; I. Belopolski; G. Bergmann; J. M. Berliner; D. Bersanetti; A. Bertolini; D. Bessis; J. Betzwieser; P. T. Beyersdorf; T. Bhadbhade; I. A. Bilenko; G. Billingsley; J. Birch; M. Bitossi; M. A. Bizouard; E. Black; J. K. Blackburn; L. Blackburn; D. Blair; M. Blom; O. Bock; T. P. Bodiya; M. Boer; C. Bogan; C. Bond; F. Bondu; L. Bonelli; R. Bonnand; R. Bork; M. Born; V. Boschi; S. Bose; L. Bosi; J. Bowers; C. Bradaschia; P. R. Brady; V. B. Braginsky; M. Branchesi; C. A. Brannen; J. E. Brau; J. Breyer; T. Briant; D. O. Bridges; A. Brillet; M. Brinkmann; V. Brisson; M. Britzger; A. F. Brooks; D. A. Brown; D. D. Brown; F. Brckner; T. Bulik; H. J. Bulten; A. Buonanno; D. Buskulic; C. Buy; R. L. Byer; L. Cadonati; G. Cagnoli; J. Caldern Bustillo; E. Calloni; J. B. Camp; P. Campsie; K. C. Cannon; B. Canuel; J. Cao; C. D. Capano; F. Carbognani; L. Carbone; S. Caride; A. Castiglia; S. Caudill; M. Cavagli; F. Cavalier; R. Cavalieri; G. Cella; C. Cepeda; E. Cesarini; R. Chakraborty; T. Chalermsongsak; S. Chao; P. Charlton; E. Chassande-Mottin; X. Chen; Y. Chen; A. Chincarini; A. Chiummo; H. S. Cho; J. Chow; N. Christensen; Q. Chu; S. S. Y. Chua; S. Chung; G. Ciani; F. Clara; D. E. Clark; J. A. Clark; F. Cleva; E. Coccia; P. -F. Cohadon; A. Colla; M. Colombini; M. Constancio Jr.; A. Conte; R. Conte; D. Cook; T. R. Corbitt; M. Cordier; N. Cornish; A. Corsi; C. A. Costa; M. W. Coughlin; J. -P. Coulon; S. Countryman; P. Couvares; D. M. Coward; M. Cowart; D. C. Coyne; K. Craig; J. D. E. Creighton; T. D. Creighton; S. G. Crowder; A. Cumming; L. Cunningham; E. Cuoco; K. Dahl; T. Dal Canton; M. Damjanic; S. L. Danilishin; S. D'Antonio; K. Danzmann; V. Dattilo; B. Daudert; H. Daveloza; M. Davier; G. S. Davies; E. J. Daw; R. Day; T. Dayanga; R. De Rosa; G. Debreczeni; J. Degallaix; W. Del Pozzo; E. Deleeuw; S. Delglise; T. Denker; T. Dent; H. Dereli; V. Dergachev; R. DeRosa; R. DeSalvo; S. Dhurandhar; L. Di Fiore; A. Di Lieto; I. Di Palma; A. Di Virgilio; M. Daz; A. Dietz; K. Dmitry; F. Donovan; K. L. Dooley; S. Doravari; M. Drago; R. W. P. Drever; J. C. Driggers; Z. Du; J. -C. Dumas; S. Dwyer; T. Eberle; M. Edwards; A. Effler; P. Ehrens; J. Eichholz; S. S. Eikenberry; G. Endr?czi; R. Essick; T. Etzel; K. Evans; M. Evans; T. Evans; M. Factourovich; V. Fafone; S. Fairhurst; Q. Fang; S. Farinon; B. Farr; W. Farr; M. Favata; D. Fazi; H. Fehrmann; D. Feldbaum; I. Ferrante; F. Ferrini; F. Fidecaro; L. S. Finn; I. Fiori; R. Fisher; R. Flaminio; E. Foley; S. Foley; E. Forsi; N. Fotopoulos; J. -D. Fournier; S. Franco; S. Frasca; F. Frasconi; M. Frede; M. Frei; Z. Frei; A. Freise; R. Frey; T. T. Fricke; P. Fritschel; V. V. Frolov; M. -K. Fujimoto; P. Fulda; M. Fyffe; J. Gair; L. Gammaitoni; J. Garcia; F. Garufi; N. Gehrels; G. Gemme; E. Genin; A. Gennai; L. Gergely; S. Ghosh; J. A. Giaime; S. Giampanis; K. D. Giardina; A. Giazotto; S. Gil-Casanova; C. Gill; J. Gleason; E. Goetz; R. Goetz; L. Gondan; G. Gonzlez; N. Gordon; M. L. Gorodetsky; S. Gossan; S. Goler; R. Gouaty; C. Graef; P. B. Graff; M. Granata; A. Grant; S. Gras; C. Gray; R. J. S. Greenhalgh; A. M. Gretarsson; C. Griffo; P. Groot; H. Grote; K. Grover; S. Grunewald; G. M. Guidi; C. Guido; K. E. Gushwa; E. K. Gustafson; R. Gustafson; B. Hall; E. Hall; D. Hammer; G. Hammond; M. Hanke; J. Hanks; C. Hanna; J. Hanson; J. Harms; G. M. Harry; I. W. Harry; E. D. Harstad; M. T. Hartman; K. Haughian; K. Hayama; J. Heefner; A. Heidmann; M. Heintze; H. Heitmann; P. Hello; G. Hemming; M. Hendry; I. S. Heng; A. W. Heptonstall; M. Heurs; S. Hild; D. Hoak; K. A. Hodge; K. Holt; M. Holtrop; T. Hong; S. Hooper; T. Horrom; D. J. Hosken; J. Hough; E. J. Howell; Y. Hu; Z. Hua; V. Huang; E. A. Huerta; B. Hughey; S. Husa; S. H. Huttner; M. Huynh; T. Huynh-Dinh; J. Iafrate; D. R. Ingram; R. Inta; T. Isogai; A. Ivanov; B. R. Iyer; K. Izumi; M. Jacobson; E. James; H. Jang; Y. J. Jang; P. Jaranowski; F. Jimnez-Forteza; W. W. Johnson; D. Jones; D. I. Jones; R. Jones; R. J. G. Jonker; L. Ju; Haris K; P. Kalmus; V. Kalogera; S. Kandhasamy; G. Kang; J. B. Kanner; M. Kasprzack; R. Kasturi; E. Katsavounidis; W. Katzman; H. Kaufer; K. Kaufman; K. Kawabe; S. Kawamura; F. Kawazoe

2014-04-24T23:59:59.000Z

216

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

217

Salmon, Mississippi Fact Sheet  

SciTech Connect (OSTI)

The Salmon, Mississippi, Site, also called the Tatum Dome Test Site, is a 1,470-acre tract of land in Lamar County, Mississippi, 21 miles southwest of Hattiesburg. The nearest town is Purvis, about 10 miles east of the site. The site is in a forested region known as the long-leaf pine belt of the Gulf Coastal Plain. Elevations in the area range from about 240 to 350 feet above sea level. The site overlies a salt formation called the Tatum Salt Dome. Land around the Salmon site has residential, industrial, and commercial use, although no one lives within the boundary of the site itself. The U.S. Atomic Energy Commission, a predecessor agency of the U.S. Department of Energy (DOE), and the U.S. Department of Defense conducted two underground nuclear tests at the site under the designation of Project Dribble, part of a larger program known as the Vela Uniform program. Two gas explosive tests, designated Project Miracle Play, were also conducted at the site.

None

2010-01-04T23:59:59.000Z

218

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

219

Optical observations of PSR J2021+3651 in the Dragonfly Nebula with the GTC  

E-Print Network [OSTI]

PSR J2021+3651 is a 17 kyr old rotation powered pulsar detected in the radio, X-rays, and $\\gamma$-rays. It powers a torus-like pulsar wind nebula with jets, dubbed the Dragonfly, which is very similar to that of the Vela pulsar. The Dragonfly is likely associated with the extended TeV source VER J2019+368 and extended radio emission. We conducted first deep optical observations with the GTC in the Sloan $r'$ band to search for optical counterparts of the pulsar and its nebula. No counterparts were detected down to $r'\\gtrsim27.2$ and $\\gtrsim24.8$ for the point-like pulsar and the compact X-ray nebula, respectively. We also reanalyzed Chandra archival X-ray data taking into account an interstellar extinction--distance relation, constructed by us for the Dragonfly line of sight using the red-clump stars as standard candles. This allowed us to constrain the distance to the pulsar, $D=1.8^{+1.7}_{-1.4}$ kpc at 90% confidence. It is much smaller than the dispersion measure distance of $\\sim$12 kpc but compatible...

Kirichenko, Aida; Shternin, Peter; Shibanov, Yuriy; Ryspaeva, Elizaveta; Zyuzin, Dima; Durant, Martin; Kargaltsev, Oleg; Pavlov, George; Cabrera-Lavers, Antonio

2015-01-01T23:59:59.000Z

220

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

Note: This page contains sample records for the topic "grady cle vela" from the National Library of EnergyBeta (NLEBeta).
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221

Beam Halo Measurements at UMER and the JLAB FEL Using an Adaptive Masking Method  

SciTech Connect (OSTI)

Beam halo is a challenging issue for intense beams since it can cause beam loss, emittance growth, nuclear activation and secondary electron emission. Because of the potentially low number of particles in the halo compared with beam core, traditional imaging methods may not have sufficient contrast to detect faint halos. We have developed a high dynamic range, adaptive masking method to measure halo using a digital micro-mirror array device and demonstrated its effectiveness experimentally on the University of Maryland Electron Ring (UMER). We also report on similar experiments currently in progress at the Jefferson Lab Free Electron Laser (FEL) using this method.

Zhang, H D; Fiorito, R B; Kishek, R A; O& #x27; Shea, P G; Shkvarunets, A G; Benson, S V; Douglas, D; Wilson, F G

2011-03-01T23:59:59.000Z

222

Evaluating operating system vulnerability to memory errors.  

SciTech Connect (OSTI)

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

Ferreira, Kurt Brian; Bridges, Patrick G. (University of New Mexico); Pedretti, Kevin Thomas Tauke; Mueller, Frank (North Carolina State University); Fiala, David (North Carolina State University); Brightwell, Ronald Brian

2012-05-01T23:59:59.000Z

223

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

SciTech Connect (OSTI)

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

Hager, Robert C. (Hatchery Operations Consulting); Costello, Ronald J. (Mobrand Biometrics, Inc., Vashon Island, WA)

1999-10-01T23:59:59.000Z

224

A Search for Gamma-Ray Bursts and Pulsars, and the Application of Kalman Filters to Gamma-Ray Reconstruction  

E-Print Network [OSTI]

Part I describes the analysis of periodic and transient signals in EGRET data. A method to search for the transient flux from gamma-ray bursts independent of triggers from other gamma-ray instruments is developed. Several known gamma-ray bursts were independently detected, and there is evidence for a previously unknown gamma-ray burst candidate. Statistical methods using maximum likelihood and Bayesian inference are developed and implemented to extract periodic signals from gamma-ray sources in the presence of significant astrophysical background radiation. The analysis was performed on six pulsars and three pulsar candidates. The three brightest pulsars, Crab, Vela, and Geminga, were readily identified, and would have been detected independently in the EGRET data without knowledge of the pulse period. No significant pulsation was detected in the three pulsar candidates. Eighteen X-ray binaries were examined. None showed any evidence of periodicity. In addition, methods for calculating the detection threshold of periodic flux modulation were developed. The future hopes of gamma-ray astronomy lie in the development of the Gamma-ray Large Area Space Telescope, or GLAST. Part II describes the development and results of the particle track reconstruction software for a GLAST science prototype instrument beam test. The Kalman filtering method of track reconstruction is introduced and implemented. Monte Carlo simulations, very similar to those used for the full GLAST instrument, were performed to predict the instrumental response of the prototype. The prototype was tested in a gamma-ray beam at SLAC. The reconstruction software was used to determine the incident gamma-ray direction. It was found that the simulations did an excellent job of representing the actual instrument response.

B. B. Jones

2002-02-04T23:59:59.000Z

225

Ultraviolet Spectrophotometry of Variable Early-Type Be and B stars Derived from High-Resolution IUE Data  

E-Print Network [OSTI]

High-dispersion IUE data encode significant information about aggregate line absorptions that cannot be conveniently extracted from individual spectra. We apply a new technique in which fluxes from each echelle order of a short wavelength IUE spectrum are binned together to construct low-resolution spectra of a rapidly varying B or Be star. The ratio of binned spectra obtained bright- star and faint-star phases contains information about the mechanism responsible for a star's variability, such as from pulsations or occultations of the star by ejected matter. We model the variations caused by these mechanism by means of model atmosphere and absorbing-slab codes. Line absorptions strength changes are sensitive to conditions in circumstellar clouds with T = 8,000--13,000K. To demonstrate proofs of concept, we construct spectral ratios for circumstellar structures associated with flux variability in various Be stars: (1) Vela X1 has bow-shock wind trailing its neutron star companion and shows signatures of gas at 13,000K or 26,000K medium in different sectors, (2) 88 Her undergoes episodic outbursts as its UV flux fades, followed a year later by a dimming in visible wavelengths, a result of a gray opacity that dominates as the shell expands and cools, and (3) zeta Tau and 60 Cyg exhibit periodic spectrum and flux changes, which match model absorptions for occulting clouds. Also, ratioed UV spectra of strongly pulsating stars show unique spectrophotometric signatures which can be simulated with models. An analysis of ratioed spectra obtained for a typical sample of 18 classical Be stars known to have rapid periodic flux variations indicates that 13 of them have ratioed spectra which are relatively featureless or have signatures of pulsation. Ratioed spectra of 3 others in the sample are consistent with the presence of co-rotating clouds.

Myron A. Smith

2001-07-10T23:59:59.000Z

226

Production of Neutrinos and Secondary Electrons in Cosmic Sources  

E-Print Network [OSTI]

We study the individual contribution to secondary lepton production in hadronic interactions of cosmic rays (CRs) including resonances and heavier secondaries. For this purpose we use the same ethodology discussed earlier \\cite{Huang07}, namely the Monte Carlo particle collision code DPMJET3.04 to determine the multiplicity spectra of various secondary particles with leptons as the final decay states, that result from inelastic collisions of cosmic-ray protons and Helium nuclei with the interstellar medium of standard composition. By combining the simulation results with parametric models for secondary particle (with resonances included) for incident cosmic-ray energies below a few GeV, where DPMJET appears unreliable, we thus derive production matrices for all stable secondary particles in cosmic-ray interactions with energies up to about 10 PeV. We apply the production matrices to calculate the radio synchrotron radiation of secondary electrons in a young shell-type SNR, RX J1713.7-3946, which is a measure of the age, the spectral index of hadronic cosmic rays, and most importantly the magnetic field strength. We find that the multi-mG fields recently invoked to explain the X-ray flux variations are unlikely to extend over a large fraction of the radio-emitting region, otherwise the spectrum of hadronic cosmic rays in the energy window 0.1-100 GeV must be unusually hard. We also use the production matrices to calculate the muon event rate in an IceCube-like detector that are induced by muon neutrinos from high-energy $\\gamma$-ray sources such as RX J1713.7-3946, Vela Jr. and MGRO J2019+37. At muon energies of a few TeV, or in other word, about 10 TeV neutrino energy, an accumulation of data over about five to ten years would allow testing the hadronic origin of TeV $\\gamma$-rays.

C. -Y. Huang; M. Pohl

2008-01-23T23:59:59.000Z

227

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

228

Technical change to the work plan for the remedial investigation of the Salmon Site, Lamar County, Mississippi: Sampling and analysis plan background soil and groundwater study  

SciTech Connect (OSTI)

The Salmon Site, formerly known as the Tatum Dome Test Site, is located in south-central Mississippi, southwest of the city of Hattiesburg, in Lamar County. Between 1964 and 1970, two nuclear and two non-nuclear gas explosions were conducted deep underground in the Tatum Salt Dome beneath the site. The tests were performed as part of the former US Atomic Energy Commission`s Vela Uniform Program which was conducted to improve the United States` capability to detect underground nuclear explosions. This document details technical changes to the existing work plan for the remedial investigation of the Salmon Site. A previously conducted Remedial Investigation for the Salmon Site involved the preparation of ecological and human health risk assessments. These risk assessments, which are incorporated into the Remedial Investigation Report, identified several constituents of potential concern (COPC) that could potentially have a negative impact on ecological and human health. These COPC are the primary risk drivers for the Salmon Site; they include arsenic and naturally occurring, gamma-emitting radionuclides. If it can be demonstrated that similar concentrations of these COPCs occur naturally in surrounding areas, they can be removed from consideration in the risk assessments. The purpose of this sampling effort is to collect enough data to prove that the COPCs are naturally occurring and are not a result of the explosives testing activities conducted at the site. This will be accomplished by collecting enough soil samples to have a statistically valid population that can be used to produce defensible comparisons that prove the concentrations identified on site are the same as the background concentrations in surrounding areas.

NONE

1998-04-01T23:59:59.000Z

229

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

230

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

231

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

232

Development of a Natural Rearing System to Improve Supplemental Fish Quality, 1999-2003 Progress Report.  

SciTech Connect (OSTI)

The National Marine Fisheries Service (NMFS) has been conducting Natural Rearing Enhancement System (NATURES) research since the early 1990s. NATURES studies have looked at a variety of mechanisms to enhance production of wild-like salmonids from hatcheries. The goal of NATURES research is to develop fish culture techniques that enable hatcheries to produce salmon with more wild-like characteristics and increased postrelease survival. The development of such techniques is called for in the Columbia Basin Fish and Wildlife Program. This document is the draft report for the Supplemental Fish Quality Contract DE-AI79-91BP20651 Over the history of the project, the effects of seminatural raceway habitats, automated underwater feeders, exercise current velocities, live food diets, and predator avoidance training have been investigated. The findings of these studies are reported in an earlier contract report (Maynard et al. 1996a). The current report focuses on research that has been conducted between 1999 and 2002. This includes studies on the effect of exercise on salmon and steelhead trout, effects of predator avoid training, integration of NATUES protocols into production hatcheries, and the study of social behavior of steelhead grown in enriched and conventional environments. Traditionally, salmon (Oncorhynchus spp.) are reared in barren concrete raceways that lack natural substrate, in-stream structure, or overhead cover. The fish are fed in an unnatural manner with artificial feeds mechanically or hand broadcast across the water surface. This traditional approach has increased the egg-to-smolt survival of hatchery-reared fish by an order of magnitude over that experienced by wild-reared salmon. However, once hatchery-reared fish are released into the wild their smolt-to-adult survival is usually much lower than wild-reared salmon. The reduced postrelease survival of hatchery-reared fish may stem from differences in their behavior and morphology compared to wild-reared salmon. After release, hatchery-reared fish are inefficient foragers and are often found with empty stomachs or stomachs filled with indigestible debris (Miller 1953, Hochachka 1961, Reimers 1963, Sosiak et al. 1979, Myers 1980, O'Grady 1983, Johnsen and Ugedal 1986). Their social behavior also differs, with hatchery-reared fish congregating at higher densities, being more aggressive, and displaying less territory fidelity than wild-reared fish (Fenderson et al. 1968, Bachman 1984, Swain and Riddell 1990). In the natural environment this results in hatchery-reared fish spending more time in high-risk aggressive behavior and less time in beneficial foraging behavior than their wild-reared counterparts. Hatchery-reared fish are also more surface oriented than wild-reared salmonids (Mason et al. 1967, Sosiak 1978). This increases their risk of being attacked by avian predators, such as kingfishers (Ceryle spp.), which search for fish near the surface. Although some of the differences between wild and hatchery-reared fish are innate (Reisenbichler and McIntyre 1977, Swain and Riddell 1990), many are conditioned and can be modified by altering the hatchery rearing environment. NATURES studies are aimed at developing a more natural salmon culture environment to prevent the development of these unnatural attributes in hatchery-reared fish. NATURES fish culture practices are already producing salmon with up to about 50% higher in-stream survival than conventionally-reared fish (Maynard et al. 1996b). When these techniques are incorporated into production releases, they should also translate into increased smolt-to-adult survival. Conservation and supplementation programs can use NATURES-reared salmonids to rebuild stocks currently listed as endangered and threatened into healthy self-sustaining runs more rapidly than traditional programs. Traditional production programs can also use high-survival NATURES-reared fish to reduce their impact on wild populations, while still meeting their adult mitigation goals.

Maynard, Desmond J.

2003-02-25T23:59:59.000Z

233

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

SciTech Connect (OSTI)

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

Matheson, H.; Safi-Harb, S. [Department of Physics and Astronomy, University of Manitoba, Winnipeg, Manitoba, R3T 2N2 (Canada); Kothes, R., E-mail: matheson@physics.umanitoba.ca, E-mail: samar@physics.umanitoba.ca, E-mail: roland.kothes@nrc-cnrc.gc.ca [Dominion Radio Astrophysical Observatory, National Research Council Herzberg, P.O. Box 248, Penticton, British Columbia, V2A 6J9 (Canada)

2013-09-01T23:59:59.000Z

234

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

235

THE 3R ANTHRACITE CLEAN COAL TECHNOLOGY Economical Conversion of Browncoal to Anthracite Type Clean Coal by Low Temperature Carbonization Pre-Treatment Process  

E-Print Network [OSTI]

The pre ven tive pre-treat ment of low grade solid fu els is safer, faster, better, and less costly vs. the end-of-the-pipe post treat ment so lu tions. The 3R (Re cy cle-Re duce-Re use) in te grated en vi ron-ment con trol tech nol ogy pro vides pre ven tive pre-treat ment of low grade solid fu els, such as brown coal and con tam i nated solid fu els to achieve high grade cleansed fu els with an thra cite and coke com-pa ra ble qual ity. The goal of the 3R tech nol ogy is to pro vide cost ef fi cient and en vi ron men tally sus-tain able so lu tions by pre ven tive pre-treat ment means for ex tended op er a tions of the solid fuel com-bus tion power plants with ca pac ity up to 300 MWe power ca pac i ties. The 3R An thra cite Clean Coal end prod uct and tech nol ogy may ad van ta geously be in te grated to the oxyfuel oxy-fir ing, Fos ter Wheeler an thra cite arc-fired util ity type boiler and Heat Pipe Re former tech nol o gies in com bi na tion with CO2 cap ture and stor age pro grams. The 3R tech nol ogy is pat ented orig i nal so lu tion. Ad van tages. Feedstock flex i bil ity: ap pli ca tion of pre-treated multi fu els from wider fuel se lec tion and avail abil ity. Im proved burn ing ef fi ciency. Tech nol ogy flex i bil ity: ef fi cient and ad van ta geous inter-link to proven boiler tech nol o gies, such as oxyfuel and arc-fired boil ers. Near zero pol lut ants for haz ard ous-air-pol lut ants: pre ven tive sep a ra tion of halo gens and heavy met als into small vol ume streams prior uti li za tion of cleansed fu els. ?97 % or ganic sul phur re moval achieved by the 3R ther-

Edward Someus

236

Yakima/Klickitat Fisheries Project: Short Project Overview of Spring Chinook Salmon Supplementation in the Upper Yakima Basin; Washington Department of Fish and Wildlife Policy/Technical Involvement and Planning, 2004-2005 Annual Report.  

SciTech Connect (OSTI)

The Yakima/Klickitat Fisheries Project (YKFP) is on schedule to ascertain whether new artificial production techniques can be used to increase harvest and natural production of spring Chinook salmon while maintaining the long-term genetic fitness of the fish population being supplemented and keeping adverse genetic and ecological interactions with non-target species or stocks within acceptable limits. The Cle Elum Supplementation and Research Facility (CESRF) collected its first spring chinook brood stock in 1997, released its first fish in 1999, and age-4 adults have been returning since 2001. In these initial years of CESRF operation, recruitment of hatchery origin fish has exceeded that of fish spawning in the natural environment, but early indications are that hatchery origin fish are not as successful at spawning in the natural environment as natural origin fish when competition is relatively high. When competition is reduced, hatchery fish produced similar numbers of progeny as their wild counterparts. Most demographic variables are similar between natural and hatchery origin fish, however hatchery origin fish were smaller-at-age than natural origin fish. Long-term fitness of the target population is being evaluated by a large-scale test of domestication. Slight changes in predation vulnerability and competitive dominance, caused by domestication, were documented. Distribution of spawners has increased as a result of acclimation site location and salmon homing fidelity. Semi-natural rearing and predator avoidance training have not resulted in significant increases in survival of hatchery fish. However, growth manipulations in the hatchery appear to be reducing the number of precocious males produced by the YKFP and consequently increasing the number of migrants. Genetic impacts to non-target populations appear to be low because of the low stray rates of YKFP fish. Ecological impacts to valued non-target taxa were within containment objectives or impacts that were outside of containment objectives were not caused by supplementation activities. Some fish and bird piscivores have been estimated to consume large numbers of salmonids in the Yakima Basin. Natural production of Chinook salmon in the upper Yakima Basin appears to be density dependent under current conditions and may constrain the benefits of supplementation. However, such constraints (if they exist) could be countered by YKFP habitat actions that have resulted in: the protection of over 900 acres of prime floodplain habitat, reconnection and screening of over 15 miles of tributary habitat, substantial water savings through irrigation improvements, and restoration of over 80 acres of floodplain and side channels. Harvest opportunities for tribal and non-tribal fishers have also been enhanced, but are variable among years. The YKFP is still in the early stages of evaluation, and as such the data and findings presented in this report should be considered preliminary until further data is collected and analyses completed. Nonetheless, the YKFP has produced significant findings, and produced methodologies that can be used to evaluate and improve supplementation. A summary table of topical area performance is presented.

Fast, David E.; Bosch, William J.

2005-09-01T23:59:59.000Z