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Sample records for grady cle vela

  1. Transfer Student Information Grady College of Journalism and Mass Communication

    E-Print Network [OSTI]

    Arnold, Jonathan

    Fall 2013 Transfer Student Information Grady College of Journalism and Mass Communication 1. You 25%. 4. When you transfer to UGA, you will begin as a pre-journalism major in Franklin College and will be advised by a Franklin pre-journalism advisor. If you have met Grady's admission requirements you can apply

  2. Journalism Concentration: Grady College MA Thesis Program Planning Form

    E-Print Network [OSTI]

    Arnold, Jonathan

    Journalism Concentration: Grady College MA Thesis Program Planning Form Student and Directed Readings in Mass Communication JRMC 8350 ( ) Special Topics in Journalism JRMC 8025 ( ) Mass Media Law JRMC 8365 ( ) Media Economics JRMC 7355 ( ) Health and Medical Journalism JRMC 7356 ( ) Advanced

  3. THE CLE-2000 TOOL-BOX Institut de genie nucleaire

    E-Print Network [OSTI]

    Meunier, Michel

    THE CLE-2000 TOOL-BOX Robert ROY Institut de g´enie nucl´eaire ´Ecole Polytechnique de Montr´eal e all over the world. Assuming a basic definition for the free-format procedure, an efficient CLE- 2000 codes, without recoding or defining new modules. The CLE-2000 tool-box is described in this report

  4. In 2005, convicted child-rapist Grady Nelson brutally murdered his wife Angelina. After

    E-Print Network [OSTI]

    Wagner, Anthony

    In 2005, convicted child-rapist Grady Nelson brutally murdered his wife Angelina. After stabbing as the Florida jury that convicted him of murder next had to decide whether he would be executed or spend his

  5. The Optical Spectrum of the Vela Pulsar

    E-Print Network [OSTI]

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

    2007-07-13

    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.

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

    E-Print Network [OSTI]

    Lisboa, Universidade Técnica de

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

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

    E-Print Network [OSTI]

    Lisboa, Universidade Técnica de

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

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

    E-Print Network [OSTI]

    Beex, A. A. "Louis"

    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

  9. Journalism Concentration: Grady College MA Non-Thesis Program Planning Form

    E-Print Network [OSTI]

    Arnold, Jonathan

    Journalism Concentration: Grady College MA Non-Thesis Program Planning Form Student: Advisor Readings in Mass Communication JRMC 8350 ( ) Special Topics in Journalism JRMC 8025 ( ) Mass Media Law JRMC 8365 ( ) Media Economics JRMC 7355 ( ) Health and Medical Journalism JRMC 7356 ( ) Advanced Health

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

    E-Print Network [OSTI]

    Arnold, Jonathan

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

  11. INTEGRAL Observations of the Vela Region Focusing on Vela X-1

    E-Print Network [OSTI]

    Stephane Schanne; Diego Gotz; Lucie Gerard; Patrick Sizun; Maurizio Falanga; Clarisse Hamadache; Bertand Cordier; Andreas von Kienlin

    2007-01-23

    The Vela region has been observed for 1.7 Ms in November 2005 by the INTEGRAL satellite. We present preliminary spectral and temporal results of Vela X-1, an eclipsing neutron star hosted in a wind-accreting high-mass X-ray binary system. Using data from ISGRI, SPI and JEM-X, we firmly confirm the existence of cyclotron resonant scattering features (CRSF) at ~27 keV and ~54 keV, implying a neutron-star magnetic field of ~3 10^12 Gauss, and the presence of an iron emission line at ~6.5 keV. During two strong flares those parameters remained unchanged. Furthermore we measure the neutron-star spin period of 283.6 s, indicating a still constant trend.

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

    E-Print Network [OSTI]

    Ripperda, Katrina Ann

    2013-02-22

    -1 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'S THF. RORDFR...

  13. Multicolor Photometry of the Vela Pulsar

    E-Print Network [OSTI]

    R. P. Mignani; P. A. Caraveo

    2001-07-02

    Multicolor photometry of the Vela pulsar (PSR B0833-45), updated by recent HST/WFPC2 observations obtained in the 555W, 675W and 814W filters, is presented. The available data provide the best characterization so far of the pulsar spectral shape, which is dominated by a flat power law continuum with spectral index \\alpha = -0.2 +/- 0.2, consistent with the extrapolation in the optical domain of the power law component of the X-ray spectrum detected by Chandra. In addition, a marginally significant dip (~ 3 sigma) seems to be present at about 6500 AA. Spectroscopic observations with the VLT, now in progress, will undoubtly provide a much better assessment of the reality and characteristics of this feature.

  14. The jets of the Vela pulsar

    E-Print Network [OSTI]

    O. Kargaltsev; G. G. Pavlov; M. A. Teter; D. Sanwal

    2003-06-09

    Chandra observations of the Vela pulsar-wind nebula (PWN) have revealed a jet in the direction of the pulsar's proper motion, and a counter-jet in the opposite direction, embedded in diffuse nebular emission. The jet consists of a bright, 8''-long inner jet, between the pulsar and the outer arc, and a dim, curved outer jet that extends up to 100'' in approximately the same direction. From the analysis of thirteen Chandra observations spread over about 2.5 years we found that this outer jet shows particularly strong variability, changing its shape and brightness. We observed bright blobs in the outer jet moving away from the pulsar with apparent speeds (0.3-0.6)c and fading on time-scales of days to weeks. The spectrum of the outer jet fits a power-law model with a photon index of 1.3\\pm0.1. The X-ray emission of the outer jet can be interpreted as synchrotron radiation of ultrarelativistic electrons/positrons. This interpretation allows one to estimate the magnetic field, ~100 microGauss, maximum energy of X-ray emitting electrons, ~2\\times 10^{14} eV, and energy injection rate, ~8\\times 10^{33} erg/s, for the outer jet. In the summed PWN image we see a dim, 2'-long outer counter-jet, which also shows a power-law spectrum with photon ined of 1.2-1.5. Southwest of the jet/counter-jet an extended region of diffuse emission is seen. Relativistic particles responsible for this radiation are apparently supplied by the outer jet.

  15. The Vela pulsar with an active fallback disk

    SciTech Connect (OSTI)

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

    2014-11-20

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

  16. Two relations that generalize the $q$-Serre relations and the Dolan-Grady relations

    E-Print Network [OSTI]

    Paul Terwilliger

    2003-07-01

    We define an algebra on two generators which we call the Tridiagonal algebra, and we consider its irreducible modules. The algebra is defined as follows. Let K denote a field, and let $\\beta, \\gamma, \\gamma^*, \\varrho, \\varrho^*$ denote a sequence of scalars taken from K. The corresponding Tridiagonal algebra $T$ is the associative K-algebra with 1 generated by two symbols $A$, $A^*$ subject to the relations (i) \\lbrack A,A^2A^*-\\beta AA^*A + A^*A^2 -\\gamma (AA^*+A^*A)- \\varrho A^*\\rbrack = 0, (ii) \\lbrack A^*,A^{*2}A-\\beta A^*AA^* + AA^{*2} -\\gamma^* (A^*A+AA^*)- \\varrho^* A\\rbrack = 0, where $\\lbrack r,s\\rbrack $ means $rs-sr$. We call these relations the Tridiagonal relations. For $\\beta = q+q^{-1}$, $\\gamma = \\gamma^*=0$, $\\varrho=\\varrho^*=0$, the Tridiagonal relations are the $q$-Serre relations. For $\\beta = 2$, $\\gamma = \\gamma^*=0$, $\\varrho=b^2$, $\\varrho^*=b^{*2}$, the Tridiagonal relations are the Dolan-Grady relations. In the first part of this paper, we survey what is known about irreducible finite dimensional $T$-modules. We focus on how these modules are related to the Leonard pairs recently introduced by the present author, and the more general Tridiagonal pairs recently introduced by Ito, Tanabe, and the present author. In the second part of the paper, we construct an infinite dimensional irreducible $T$-module based on the Askey-Wilson polynomials.

  17. The BLAST Survey of the Vela Molecular Cloud: Physical Properties of the Dense Cores in Vela-D

    E-Print Network [OSTI]

    Olmi, Luca; Angles-Alcazar, Daniel; Bock, James J; Chapin, Edward L; De Luca, Massimo; Devlin, Mark J; Dicker, Simon; Elia, Davide; Fazio, Giovanni G; Giannini, Teresa; Griffin, Matthew; Gundersen, Joshua O; Halpern, Mark; Hargrave, Peter C; Hughes, David H; Klein, Jeff; Lorenzetti, Dario; Marengo, Massimo; Marsden, Gaelen; Martin, Peter G; Massi, Fabrizio; Mauskopf, Philip; Netterfield, Calvin B; Patanchon, Guillaume; Rex, Marie; Salama, Alberto; Scott, Douglas; Semisch, Christopher; Smith, Howard A; Strafella, Francesco; Thomas, Nicholas; Truch, Matthew D P; Tucker, Carole; Tucker, Gregory S; Viero, Marco P; Wiebe, Donald V

    2009-01-01

    The Balloon-borne Large-Aperture Submillimeter Telescope (BLAST) carried out a 250, 350 and 500 micron survey of the galactic plane encompassing the Vela Molecular Ridge, with the primary goal of identifying the coldest, dense cores possibly associated with the earliest stages of star formation. Here we present the results from observations of the Vela-D region, covering about 4 square degrees, in which we find 141 BLAST cores. We exploit existing data taken with the Spitzer MIPS, IRAC and SEST-SIMBA instruments to constrain their (single-temperature) spectral energy distributions, assuming a dust emissivity index beta = 2.0. This combination of data allows us to determine the temperature, luminosity and mass of each BLAST core, and also enables us to separate starless from proto-stellar sources. We also analyze the effects that the uncertainties on the derived physical parameters of the individual sources have on the overall physical properties of starless and proto-stellar cores, and we find that there appe...

  18. An expression of Philippine Sea plate rotation: the Parece Vela and Shikoku Basins

    E-Print Network [OSTI]

    Müller, Dietmar

    An expression of Philippine Sea plate rotation: the Parece Vela and Shikoku Basins Maria Sdroliasa October 2003; accepted 27 July 2004 Available online 27 October 2004 Abstract The Philippine Sea plate. The motion of the Philippine Sea plate through time is poorly understood as it is almost entirely surrounded

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

    SciTech Connect (OSTI)

    Cle Elum Supplementation and Research Facility

    2008-12-09

    FISH PRODUCTION: Final shocking of eggs was finished in the incubation. Egg enumeration for the 2008 brood was completed and the eggs are being incubated in 38 degree Fahrenheit chilled water. Don Larsen of NOAA made a request of eggs for research purposes and was able to acquire supplemental line eggs 10,555. Estimated density at the time of ponding in Mid-March of 2009 is approximately 43,869 fry per raceway after calculating an average fry loss of 2%. The end of the month totals for the 2007 brood reports 773,807 juveniles on hand with an overall average of 31.4 fish per pound. Tagging continues on the 2007 brood and is on pace to wrap up in early December. FISH CULTURE: Ponds are cleaned as needed and due to the colder water temperatures, the feeding frequency has been changed to three days a week. All ponds are sampled at the end of the month. Growth for production fish are adjusted accordingly as temperature dictates feeding levels. Torrential rain on the 12th turned the Yakima River extremely turbid. Fish tagging operations were halted and the ensuing conditions at the facility intake screens became a concern. Water flow to the wet well became restricted so the decision was made to shut the surface water (river) pumps down and turn on well pumps No.1, No.4 and No.6 to run water to the facility head box. This operation continued for twenty-four hours at which point normal operations were optimal and fish tagging resumed, although the river didn't clear up enough to feed the fish until the 17th. WATER PRODUCTION: The current combined well and river water supply to the complex is 14,822 gallons/minute. Well No.2 is pumping water at a rate of 530 gallons per minute. All four river pumps are in operation and pumping 14,292 gallons/minute. ACCLIMATION SITES: Cle Elum staff has been working to prep the acclimation sites for the upcoming fish transfer before the snow falls. Thermographs at each site are changed weekly. AMB Tools performed routine maintenance on the compressor and Brown and Jackson pumped out the septic tank at the Jack Creek acclimation site. VEHICLE MAINTENANCE: Snow tires are now on all vehicles and snow blowers were installed on the John Deere tractor and lawn tractor. The snowplow was also installed on the Ford one ton. The four Snowmobiles were serviced by Yamaha Jacks of Ellensburg. MAINTENANCE BUILDING MAINTENANCE: Clean up occurs on Fridays of each week. HATCHERY BUILDING MAINTENANCE: Water has been turned on to vertical incubator islands one and two. After eggs were transferred to vertical stacks cleaning of troughs began. WDFW crew inventoried eggs from isolettes and then transferred them to the vertical incubators. RIVER PUMP STATION MAINTENANCE: All four pumps are in operation and supplying the facility with 14,292 gallons/minute of water to rearing ponds. WELL FIELD MAINTENANCE: Well pumps No.1, No.4 and No.6 were turned on to supplement water flow to the facility as mentioned previously. Well No.5 was powered up but a winterizing valve malfunction wouldn't allow operation, we are currently working on it at this time. Well No.2 is pumping 530 gallons per minute and supplies well water to incubation and chiller. The pumps meter is recorded weekly. Test holes are monitored weekly and results are faxed to CH2MHILL afterward. SAFETY AND TRAINING: Ice melt and sand bags are popular items at the facility this month as freezing temperatures cause ground to become slippery and hazardous. GROUNDS: Van Alden's Plumbing installed a new commode in resident house No.411 and also inspected a plumbing problem at resident No.1131. Cle Elum staff along with WDFW staff worked to locate the spawning channel building back to the position it was at to have Greg Wallace of Wallace Electric hook electricity back up to the spawning shed. MEETINGS AND TOURS: Charlie attended a policy meeting at Cle Elum on the 18th. The Internal projects annual review took place at Cle Elum on the 19th and 20th. Bill Bosch continues to visit monthly to incorporate data into the YKFP data base. PERSONNEL: IHS employees traveled to Cle

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

    E-Print Network [OSTI]

    Hill, Wendell T.

    and development are vital if America is to decrease greenhouse gas emissions at lower cost, reduce dependenceIMPACT Vol. 5 No. 1 | Spring 2010 CLeAn eneRGy DeMAnDS: SCienCe, innovATion, PUBLiC PoLiCy Maryland the science to develop it, the innovation to manu- facture it, the public policy to regulate it and the social

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

    SciTech Connect (OSTI)

    Cle Elum Supplementation and Research Facility

    2008-12-11

    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

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

    SciTech Connect (OSTI)

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

    2011-12-10

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

  3. Clemson University Preservation master Plan appendix a cleMson university plant list FeBruary 2009 JMa, inc. a-1

    E-Print Network [OSTI]

    Stuart, Steven J.

    Clemson University Preservation master Plan appendix a · cleMson university plant list · FeBruary 2009 · JMa, inc. · a-1 appendix a: Clemson University CampUs plant list ~ 2009 Abelia grandifloraMson university plant list · FeBruary 2009 · JMa, inc. · a-2 Eriobotrya japonica Japanese loquat Erythronium

  4. A Comparison of Measured Crab and Vela Glitch Healing Parameters with Predictions of Neutron Star Models

    E-Print Network [OSTI]

    Fronefield Crawford; Marek Demianski

    2003-06-11

    There are currently two well-accepted models that explain how pulsars exhibit glitches, sudden changes in their regular rotational spin-down. According to the starquake model, the glitch healing parameter, Q, which is measurable in some cases from pulsar timing, should be equal to the ratio of the moment of inertia of the superfluid core of a neutron star (NS) to its total moment of inertia. Measured values of the healing parameter from pulsar glitches can therefore be used in combination with realistic NS structure models as one test of the feasibility of the starquake model as a glitch mechanism. We have constructed NS models using seven representative equations of state of superdense matter to test whether starquakes can account for glitches observed in the Crab and Vela pulsars, for which the most extensive and accurate glitch data are available. We also present a compilation of all measured values of Q for Crab and Vela glitches to date which have been separately published in the literature. We have computed the fractional core moment of inertia for stellar models covering a range of NS masses and find that for stable NSs in the realistic mass range 1.4 +/- 0.2 solar masses, the fraction is greater than 0.55 in all cases. This range is not consistent with the observational restriction Q 0.7) are consistent with the starquake model predictions and support previous conclusions that starquakes can be the cause of Crab glitches.

  5. Footprints in the wind of Vela X-1 traced with MAXI

    E-Print Network [OSTI]

    Doroshenko, V; Nakahira, S; Mihara, T; Sugizaki, M; Matsuoka, M; Nakajima, M; Makishima, K

    2013-01-01

    The stellar wind around the compact object in luminous wind-accreting high mass X-ray binaries is expected to be strongly ionized with the X-rays coming from the compact object. The stellar wind of hot stars is mostly driven by light absorption in lines of heavier elements, and X-ray photo-ionization significantly reduces the radiative force within the so-called Stroemgren region leading to wind stagnation around the compact object. In close binaries like Vela X-1 this effect might alter the wind structure throughout the system. Using the spectral data from Monitor of All-sky X-ray Image (MAXI), we study the observed dependence of the photoelectric absorption as function of orbital phase in Vela X-1, and find that it is inconsistent with expectations for a spherically-symmetric smooth wind. Taking into account previous investigations we develop a simple model for wind structure with a stream-like photoionization wake region of slower and denser wind trailing the neutron star responsible for the observed absor...

  6. FERMI-LAT DETECTION OF PULSED GAMMA-RAYS ABOVE 50 GeV FROM THE VELA PULSAR

    SciTech Connect (OSTI)

    Leung, Gene C. K.; Takata, J.; Ng, C. W.; Cheng, K. S. [Department of Physics, The University of Hong Kong, Pokfulam Road (Hong Kong); Kong, A. K. H.; Tam, P. H. T. [Institute of Astronomy and Department of Physics, National Tsing Hua University, Hsinchu, Taiwan (China); Hui, C. Y., E-mail: gene930@connect.hku.hk, E-mail: takata@hku.hk [Department of Astronomy and Space Science, Chungnam National University, Daejeon (Korea, Republic of)

    2014-12-20

    The first Fermi-Large Area Telescope (LAT) catalog of sources above 10 GeV reported evidence of pulsed emission above 25 GeV from 12 pulsars, including the Vela pulsar, which showed evidence of pulsation at >37 GeV energy bands. Using 62 months of Fermi-LAT data, we analyzed the gamma-ray emission from the Vela pulsar and searched for pulsed emission above 50 GeV. Having confirmed the significance of the pulsation in 30-50 GeV with the H test (p-value ?10{sup –77}), we extracted its pulse profile using the Bayesian block algorithm and compared it with the distribution of the five observed photons above 50 GeV using the likelihood ratio test. Pulsation was significantly detected for photons above 50 GeV with a p-value of =3 × 10{sup –5} (4.2?). The detection of pulsation is significant above 4? at >79 GeV and above 3? at >90 GeV energy bands, making this the highest energy pulsation significantly detected by the LAT. We explore the non-stationary outer gap scenario of the very high-energy emissions from the Vela pulsar.

  7. Interstellar Seeing. II. The Case of the Vela Pulsar: Source Unresolved

    E-Print Network [OSTI]

    J. M. Cordes

    2000-07-17

    I use a method based on interstellar scintillations for discerning information about source sizes on scales less than one micro-arc sec. I use a comprehensive model for a pulsar signal, scintillated amplitude modulated noise, that includes source fluctuations and noise statistics. The method takes into account time-frequency averaging in the signal processing as well as effects due to source structure. The method is applied to interferometric visibility data on the Vela pulsar which show slightly less scintillation modulation than expected for a point source in the strong scattering regime. The decreased scintillation modulation is likely to be due exclusively to time-frequency averaging rather than from any source size effects. The implied upper limit on source extent, derived through Bayesian inference, is compared to predictions that take into account beaming from the relativistic plasma flow in neutron star magnetospheres. The upper limit for the transverse source size ($\\lesssim 400$ km at 95% confidence for a pulsar distance of 0.5 kpc) is easily consistent with conventional models for radio emission regions in pulsar magnetospheres that place them well inside the light cylinder at only a few neutron-star radii from the star's surface.

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

    E-Print Network [OSTI]

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

    2014-01-01

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

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

    E-Print Network [OSTI]

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

    2014-10-30

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

  10. NAME GRADiNG- KEy

    E-Print Network [OSTI]

    Fow- Pmsz 7(Qj,7(_b) wind 7(c): (8) (a) Z: 3—1: 1-430" {"qu 01 {'Qth“ ... (16) 8. Find the interval of convergence of the power series 2 2:". Don't forget to n=l\\/'r_t 2

  11. Pulsar Wind Nebulae as a source of the observed electron and positron excess at high energy: the case of Vela-X

    E-Print Network [OSTI]

    Della Torre, S; Rancoita, P G; Rozza, D; Treves, A

    2015-01-01

    We investigate, in terms of production from pulsars and their nebulae, the cosmic ray positron and electron fluxes above $\\sim10$ GeV, observed by the AMS-02 experiment up to 1 TeV. We concentrate on the Vela-X case. Starting from the gamma-ray photon spectrum of the source, generated via synchrotron and inverse Compton processes, we estimated the electron and positron injection spectra. Several features are fixed from observations of Vela-X and unknown parameters are borrowed from the Crab nebula. The particle spectra produced in the pulsar wind nebula are then propagated up to the Solar System, using a diffusion model. Differently from previous works, the omnidirectional intensity excess for electrons and positrons is obtained as a difference between the AMS-02 data and the corresponding local interstellar spectrum. An equal amount of electron and positron excess is observed and we interpreted this excess (above $\\sim$100 GeV in the AMS-02 data) as a supply coming from Vela-X. The particle contribution is c...

  12. Chemical evolution of the HC3N and N2H+ molecules in dense cores of the Vela C giant molecular cloud complex

    E-Print Network [OSTI]

    Ohashi, Satoshi; Fujii, Kosuke; Sanhueza, Patricio; Luong, Quang Nguyen; Choi, Minho; Hirota, Tomoya; Mizuno, Norikazu

    2015-01-01

    We have observed the HC3N (J=10-9) and N2H+ (J=1-0) lines toward the Vela C molecular clouds with the Mopra 22 m telescope to study chemical characteristics of dense cores. The intensity distributions of these molecules are similar to each other at an angular resolution of 53", corresponding to 0.19 pc suggesting that these molecules trace the same dense cores. We identified 25 local peaks in the velocity-integrated intensity maps of the HC3N and/or N2H+ emission. Assuming LTE conditions, we calculated the column densities of these molecules and found a tendency that N2H+/HC3N abundance ratio seems to be low in starless regions while it seems to be high in star-forming regions, similar to the tendencies in the NH3/CCS, NH3/HC3N, and N2H+/CCS abundance ratios found in previous studies of dark clouds and the Orion A GMC. We suggest that carbon chain molecules, including HC3N, may trace chemically young molecular gas and N-bearing molecules, such as N2H+, may trace later stages of chemical evolution in the Vela ...

  13. Filaments and ridges in Vela C revealed by Herschel: from low-mass to high-mass star-forming sites

    E-Print Network [OSTI]

    Hill, Tracey; Didelon, Pierre; Bontemps, Sylvain; Minier, Vincent; Hennemann, Martin; Schneider, Nicola; Andre, Philippe; Men'shchikov, Alexander; Anderson, Loren D; Arzoumanian, Doris; Bernard, Jean-Philippe; di Francesco, James; Elia, Davide; Giannini, Teresa; Griffin, Matt J; Kirk, Jason; Konyves, Vera; Marston, Anthony P; Martin, Peter; Molinari, Sergio; Luong, Quang Nguyen; Peretto, Nicolas; Pezzuto, Stefano; Roussel, Helene; Sauvage, Marc; Sousbie, Thierry; Testi, Leonardo; Ward-Thompson, Derek; White, Glenn J; Wilson, Christine D; Zavagno, Annie

    2011-01-01

    We present the first Herschel PACS and SPIRE results of the Vela C molecular complex in the far-infrared and submillimetre regimes at 70, 160, 250, 350, and 500 um, spanning the peak of emission of cold prestellar or protostellar cores. Column density and multi-resolution analysis (MRA) differentiates the Vela C complex into five distinct sub-regions. Each sub-region displays differences in their column density and temperature probability distribution functions (PDFs), in particular, the PDFs of the `Centre-Ridge' and `South-Nest' sub-regions appear in stark contrast to each other. The Centre-Ridge displays a bimodal temperature PDF representative of hot gas surrounding the HII region RCW 36 and the cold neighbouring filaments, whilst the South-Nest is dominated by cold filamentary structure. The column density PDF of the Centre-Ridge is flatter than the South-Nest, with a high column density tail, consistent with formation through large-scale flows, and regulation by self-gravity. At small to intermediate sc...

  14. Measurement of Plasma Dynamics in the TCSU RMF Current Drive Experiment K.M. Velas, C.L. Deards, P.A. Melnik, J.A Grossnickle, A.L. Hoffman, K.E. Miller, R.D. Milroy

    E-Print Network [OSTI]

    Washington at Seattle, University of

    Measurement of Plasma Dynamics in the TCSU RMF Current Drive Experiment K.M. Velas, C.L. Deards, P.A. Melnik, J.A Grossnickle, A.L. Hoffman, K.E. Miller, R.D. Milroy Redmond Plasma Physics Laboratory, University of Washington Detailed magnetic measurements of Field-Reversed Configurations (FRC) from

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

    SciTech Connect (OSTI)

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

    2011-09-01

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

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

    SciTech Connect (OSTI)

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

    2011-09-01

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

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

    SciTech Connect (OSTI)

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

    2011-09-01

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

  18. VELA_COMP_OUT

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

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

  19. 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 Home Page on QA:QA J-E-1 SECTION JEnvironmental Jump to:EA EISTJThin FilmUnitedVairex Corporation JumpVaron LightingVehizero

  20. 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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorking WithTelecentric viewing system forPortal. 1.1 I3:Pajarito Corridor

  1. 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 QA:QA J-E-1 SECTION J APPENDIX E LISTStar2-0057-EA Jump to:ofEniaElectricHydro Electric Co P Ltd Jump to:

  2. A CR-hydro-NEI Model of Multi-wavelength Emission from the Vela Jr. Supernova Remnant (SNR RX J0852.0-4622)

    E-Print Network [OSTI]

    Lee, Shiu-Hang; Ellison, Donald C; Nagataki, Shigehiro; Patnaude, Daniel J

    2013-01-01

    Based largely on energy budget considerations and the observed cosmic-ray (CR) ionic composition, supernova remnant (SNR) blast waves are the most likely sources of CR ions with energies at least up to the "knee" near 3 PeV. Shocks in young shell-type TeV-bright SNRs are surely producing TeV particles, but the emission could be dominated by ions producing neutral pion-decay emission or electrons producing inverse-Compton gamma-rays. Unambiguously identifying the GeV-TeV emission process in a particular SNR will not only help pin down the origin of CRs, it will add significantly to our understanding of the diffusive shock acceleration (DSA) mechanism and improve our understanding of supernovae and the impact SNRs have on the circumstellar medium. In this study, we investigate the Vela Jr. SNR, an example of TeV-bright non-thermal SNRs. We perform hydrodynamic simulations coupled with non-linear DSA and non-equilibrium ionization near the forward shock (FS) to confront currently available multi-wavelength data....

  3. Balloon-Borne Submillimeter Polarimetry of the Vela C Molecular Cloud: Systematic Dependence of Polarization Fraction on Column Density and Local Polarization-Angle Dispersion

    E-Print Network [OSTI]

    Fissel, Laura M; Angilè, Francesco E; Ashton, Peter; Benton, Steven; Devlin, Mark J; Dober, Bradley; Fukui, Yasuo; Galitzki, Nicholas; Gandilo, Natalie N; Klein, J R; Li, Zhi-Yun; Korotkov, Andrei L; Martin, Peter G; Matthews, Tristan G; Moncelsi, Lorenzo; Nakamura, Fumitaka; Netterfield, C Barth; Novak, Giles; Pascale, Enzo; Poidevin, Frédérick; Santos, Fabio P; Savini, Giorgio; Scott, Douglas; Shariff, Jamil A; Soler, Juan D; Thomas, Nicholas E; Tucker, Carole E; Tucker, Gregory S; Ward-Thompson, Derek

    2015-01-01

    We present results for Vela C obtained during the 2012 flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol). We mapped polarized intensity across almost the entire extent of this giant molecular cloud, in bands centered at 250, 350, and 500 {\\mu}m. In this initial paper, we show our 500 {\\mu}m data smoothed to a resolution of 2.5 arcminutes (approximately 0.5 pc). We show that the mean level of the fractional polarization p and most of its spatial variations can be accounted for using an empirical three-parameter power-law fit, p = p_0 N^(-0.4) S^(-0.6), where N is the hydrogen column density and S is the polarization-angle dispersion on 0.5 pc scales. The decrease of p with increasing S is expected because changes in the magnetic field direction within the cloud volume sampled by each measurement will lead to cancellation of polarization signals. The decrease of p with increasing N might be caused by the same effect, if magnetic field disorder increases for high colum...

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

    SciTech Connect (OSTI)

    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..

    2012-03-29

    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.

  5. Grady Roberts, PhD Director and Associate Professor

    E-Print Network [OSTI]

    Ma, Lena

    will develop a research idea connected to teaching and learning, solidify the research project, and move focused on a variety of topics for teaching enhancement and pro- grammatic development. The keynote Teaching Scholars were also recognized. #12;Scholarship of Teaching and Learning Brown Bag Seminar Series

  6. Tagging the boll weevil (Anthonomus gradis Boh.) with P³² 

    E-Print Network [OSTI]

    Mayer, Marion Sidney

    1961-01-01

    of qptahs of PIL feil at ~ xate of 1D ac/al af a R5 Psx asst bags~ter so3utian by media?reaxed boll weeviis AMN6 ~l8 bacxe prior ta treatment ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ 28 Bats af nptabs cf P3 f46 at a gate of 25 Qc/ml cl' a 25 per- cent bagmCjt~ter sot...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...

  7. 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 Center Home Page on QA:QAsource History View New PagesSustainableGlynn County, Georgia: EnergyGorlitz AG JumpGeorgia: Energy Resources Jump

  8. 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 Center Home Page on QA:QAsource History View New PagesSustainableGlynn County, Georgia: EnergyGorlitz AG JumpGeorgia: Energy Resources

  9. German Club for Rural Electrification CLE | 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 QA:QA J-E-1 SECTION J APPENDIX E LISTStar2-0057-EA Jump to:ofEniaElectric Jump to:Ger te undAssociation

  10. Expression analysis of the CLE signaling gene family in Arabidopsis thaliana and functional characterization of CLE8 in seed development

    E-Print Network [OSTI]

    Fiume, Elisa

    2010-01-01

    that 0.5 mM potassium ferrocyanide and 2.5 mM potassiumthat 1mM potassium ferrocyanide and 1mM potassium

  11. Design and Fabrication of a High Aspect Ratio Cable for a High Gradie nt Quadrupole Magnet

    E-Print Network [OSTI]

    Scanlan, R.M.

    2011-01-01

    0 25 mm Illick x 9.5 mm wide polyimide, followed with a .05mm x 9.5 mm wide polyimide film wound with a 2JllOl gap (

  12. Design and Fabrication of a High Aspect Ratio Cable for a High Gradie nt Quadrupole Magnet

    E-Print Network [OSTI]

    Scanlan, R.M.

    2011-01-01

    0.8 mill diam wire and a keystone a ng le of 0 . 99 deg. Theexample, the maximum safe keystone angle and compaction fortype cables Strand Suand Keystone Cable Aspect Ratio (

  13. 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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouthReport for the Weldon Spring,7=cr5rnP 7694 i+lJNew York,' ,9229409

  14. Isoprene Suppression of New Par1cle Forma1on on Long Island

    E-Print Network [OSTI]

    (University of Illinois, Urbana, IL 61801) Ernie Lewis (Brookhaven Na1onal Laboratory, Upton, NY 11973) Figure 2 · New particle formation (NPF) occurs in the atmosphere in the formation of sulfuric acid. · It s hypothesized that the frequency of NPF will be positively correlated

  15. of glucose on insulin responsiveness in mus-cle and on insulin secretion from pancreas are

    E-Print Network [OSTI]

    Shneiderman, Ben

    and gluconeogenesis (6). CRTC2 enhances the transcription of genes encoding proteins critical to gluconeogenesis

  16. 108 / CLE0'97 / TUESDAY MORNING CTuN4 11:15am

    E-Print Network [OSTI]

    Sipe,J. E.

    ,**Department of Electrical and ComputerEngineering, University of Toronto, 10King's CollegeRoad, Toronto, Ontario, Canada M5S-based devices and applications typically involve optical pulses or other types of narrowband sources whose

  17. 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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on77 PAGE OF PAGESpersonal March 3, 2015 -Far-redCarlsbad.1,08

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

    E-Print Network [OSTI]

    Meng, Ling

    2010-01-01

    into a 2 ml Eppendorf tube. • Vortex vigorously for 5 min,tube, and add 1/2 volume of chloroform (~500 ?l), vortex for

  19. Cell Cycle 13:15, 23222322; August 1, 2014; 2014 Landes Bioscience CeLL CyCLe News & Views

    E-Print Network [OSTI]

    Calvi, Brian R.

    , and it has been linked to oncogenesis.1 HBO1 is a member of a protein complex that includes the plant

  20. A Single Parti cleApproach to Cy clotron Heating in a Non-Unifonn Magneti c Field

    E-Print Network [OSTI]

    Sprott, Julien Clinton

    to estimate the heating rate. The approach 1 is similar to that of Kuckes in a recent paper. We begin (10) of Kuckes paper (where w c '= aw c ). Now consider a group of non-interacting particles, all

  1. Enhancing the Expressiveness of the CleanJava Language Melisa Vela and Yoonsik Cheon

    E-Print Network [OSTI]

    Cheon, Yoonsik

    for Java to support Cleanroom-style functional program verification that views a program as a mathematical function, CleanJava. I. INTRODUCTION In Cleanroom-style functional program verification, a pro- gram

  2. A Tutorial on Functional Program Verification Yoonsik Cheon and Melisa Vela

    E-Print Network [OSTI]

    Cheon, Yoonsik

    ; Cleanroom; 1998 CR Categories: D.2.4 [Software Engineering] Software/Program Verification -- Correctness at IBM developed an approach to software development called Cleanroom Software Engineering [1] [2]. Its specification. Cleanroom is a lightweight, or semi-formal, method and tries to verify the correctness

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

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 OutreachProductswsicloudwsiclouddenDVA N C E D B L O OLaura|Bilayer Graphene Gets aVehicles and Fuels

  4. 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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouth DakotaRobbins and700, 1.Reports1E~ S·D3 WeldonY.B.

  5. This report was funded by the Illinois Department of Commerce and Economic Opportunity. Special thanks to Jonathan Feipel and Alyson Grady

    E-Print Network [OSTI]

    Branoff, Theodore J.

    and outreach materials about utility-scale development and small wind electric systems to utilities, rural

  6. Arithmetic Coding for Data Compression

    E-Print Network [OSTI]

    Howard, Paul G.; Vitter, Jeffrey Scott

    1994-01-01

    of the particular sequence of events in the #0Cle. The #0Cnal step uses at most b,log 2 pc + 2 bits to distinguish the #0Cle fromall other possible #0Cles. We need some mechanism to indicate the end ofthe #0Cle, either a special end- of-#0Cle event coded just once... of the particular sequence of events in the #0Cle. The #0Cnal step uses at most b,log 2 pc + 2 bits to distinguish the #0Cle fromall other possible #0Cles. We need some mechanism to indicate the end ofthe #0Cle, either a special end- of-#0Cle event coded just once...

  7. 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

  8. SAPIENZA UNIVERSIT DI ROMA DIPARTIMENTO DI INGEGNERIA INFORMATICA AUTOMATICA E

    E-Print Network [OSTI]

    Di Pillo, Gianni

    , prototipazione e installazione dispositivo d'attuazione controllo vela fotovoltaica e varie COMPETENZE DEL

  9. Decreto N. 91/2013 APPROVAZIONE ATTI

    E-Print Network [OSTI]

    Di Pillo, Gianni

    progettazione, prototipazione e installazione dispositivo d'attuazione controllo vela fotovoltaica e varie" Art

  10. 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]

    O'Grady, Patrick M.

    positive results with include fkh, glass, amylase (amy), esc, mago nashi (mago), ntid, boss, snf, and sia

  11. Please cite this article in press as: Vargas-Mendoza, C. F., et al. Genetic diversity, outcrossing rate, and demographic history along a climatic gradi-ent in the ruderal plant Ruellia nudiflora (Acanthaceae). Revista Mexicana de Biodiversidad (2015), htt

    E-Print Network [OSTI]

    Herrera, Carlos M.

    2015-01-01

    (Acanthaceae). Revista Mexicana de Biodiversidad (2015), http://dx.doi.org/10.1016/j.rmb.2015.04.034 ARTICLE Biodiversidad www.ib.unam.mx/revista/ Revista Mexicana de Biodiversidad xxx (2015) xxx­xxx Evolution Genetic

  12. OBSERVATIONAL CONSTRAINTS ON THE INTERNAL STRUCTURE AND DYNAMICS OF THE VELA PULSAR MARK ABNEY,1, 2 RICHARD I. EPSTEIN,1 AND ANGELA V. OLINTO1, 2

    E-Print Network [OSTI]

    Abney, Mark

    with a magnitude that exceeds 1013 G for a normal interior and 1011 G for a superconducting interior. These lower

  13. BLAST: The Mass Function, Lifetimes, and Properties of Intermediate Mass Cores from a 50 Square Degree Submillimeter Galactic Survey in Vela (l = ~265)

    E-Print Network [OSTI]

    Netterfield, Calvin B; Bock, James J; Chapin, Edward L; Devlin, Mark J; Griffin, Matthew; Gundersen, Joshua O; Halpern, Mark; Hargrave, Peter C; Hughes, David H; Klein, Jeff; Marsden, Gaelen; Martin, Peter G; Mauskopf, Phillip; Olmi, Luca; Pascale, Enzo; Patanchon, Guillaume; Rex, Marie; Roy, Arabindo; Scott, Douglas; Semisch, Christopher; Thomas, Nicholas; Truch, Matthew D P; Tucker, Carole; Tucker, Gregory S; Viero, Marco P; Wiebe, Donald V

    2009-01-01

    We present first results from an unbiased, 50 square degree submillimeter Galactic survey at 250, 350, and 500 microns from the 2006 flight of the Balloon-borne Large Aperture Submillimeter Telescope (BLAST). The map has resolution ranging from 36" to 60" in the three submillimeter bands spanning the thermal emission peak of cold starless cores. We determine the temperature, luminosity, and mass of more than a thousand compact sources in a range of evolutionary stages and an unbiased statistical characterization of the population. From comparison with C^18 O data, we find the dust opacity per gas mass, kappa/R = 0.16 cm^2/g at 250 microns, for cold clumps. We find that 2% of the mass of the molecular gas over this diverse region is in cores colder than 14 K, and that the mass function for these cold cores is consistent with a power law with index alpha = -3.22 +/- 0.14 over the mass range 14 M_sun < M < 80 M_sun, steeper than the Salpeter alpha = -2.35 initial massfunction for stars. Additionally, we in...

  14. Chicane simula-on update Pavel Snopok

    E-Print Network [OSTI]

    McDonald, Kirk

    Chicane simula-on update Pavel Snopok Front end phone mee-ng April 22 energy ref par-cle loses 0.2 MeV/m, low energy ref par-cle gains 5.1 Me

  15. Search for: All records | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    for a way to improve these results? Response of High-Tc Superconductor Metamaterials to High Intensity THz Radiation Grady, Nathaniel ; Perkins Jr., Bradford G. ;...

  16. SciTech Connect:

    Office of Scientific and Technical Information (OSTI)

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

  17. Nuclear and Particle Physics, Astrophysics, and Cosmology

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

    Administrator Kay Grady Email Find Expertise header Search our employee skills database Dark sky Simulation of the cosmic web of the dark matter mass distribution. This region...

  18. SAPIENZA UNIVERSIT DI ROMA DIPARTIMENTO DI INGEGNERIA INFORMATICA, AUTOMATICA E

    E-Print Network [OSTI]

    Di Pillo, Gianni

    installazione dispositivo d'attuazione controllo vela fotovoltaica e varie" a favore del Dipartimento di installazione dispositivo d'attuazione controllo vela fotovoltaica e varie Articolo 2 L'attività oggetto della

  19. Gamma-Ray Bursts Nuclear Test Ban Treaty, 1963

    E-Print Network [OSTI]

    Harrison, Thomas

    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

  20. ENVIRONMENTAL VARIABLES AFFECTING ANT (FORMICIDAE) COMMUNITY COMPOSITION IN MISSISSIPPI'S BLACK BELT

    E-Print Network [OSTI]

    Ray, David

    BELT AND FLATWOODS REGIONS By JoVonn Grady Hill A Thesis Submitted to the Faculty of Mississippi State COMPOSITION IN MISSISSIPPI'S BLACK BELT AND FLATWOODS REGIONS. By JoVonn Grady Hill Approved: Richard L. Brown (FORMICIDAE) COMMUNITY COMPOSITION IN MISSISSIPPI'S BLACK BELT AND FLATWOODS REGIONS Pages in Study: 72

  1. DISCOVERY OF AN 86 AU RADIUS DEBRIS RING AROUND HD 181327 Glenn Schneider,1

    E-Print Network [OSTI]

    Schneider, Glenn

    Clampin,5 Carol Grady,6 David Golimowski,7 David Ardila,8 Thomas Henning,9 Sebastian Wolf,9 and Jens itsconstituent grains(HR 4796A; Schneider et al. 1999). Advances in space- and ground-based high-contrast imaging

  2. Atmos. Chem. Phys., 10, 919929, 2010 www.atmos-chem-phys.net/10/919/2010/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    of acetaldehyde in snow and its processes of physical and chemical exchanges requires the knowledge of its in a manipulated snowpack where temperature gradi- ents were suppressed. Snow crystals there transformed much more

  3. Integrating Multiple Geographic Information Systems to Create a Versatile Land Evaluation Site Assessment Model

    E-Print Network [OSTI]

    Morrison, Grady

    2008-11-19

    GIS in Urban Planning Integrating Multiple Geographic Information Systems to Create a Versatile Land Suitability Analysis Model Grady Morrison Undergraduate Department of Geography University of Kansas gmorrisn@ku.edu Impervious Surface...

  4. Optimizac~ao e Algoritmos (2004/2005) Instituto Superior Tecnico Engenharia Electrotecnica e de Computadores

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    Optimiza¸c~ao e Algoritmos (2004/2005) Instituto Superior T´ecnico ­ Engenharia Electrot´ecnica e um mini- mizante global. Problema 6.[Algoritmos: coordenadas c´iclicas, descida de gradi- ente e

  5. UNIVERSIT DI BRESCIA FACOLT DI INGEGNERIA

    E-Print Network [OSTI]

    Cassinis, Riccardo

    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

  6. Subterranean Termites 

    E-Print Network [OSTI]

    Gold, Roger E.; Howell Jr., Harry N.; Glenn, Grady J.; Engler, Kimberly

    2005-12-05

    /05 Roger E. Gold, Harry N. Howell Jr., Grady J. Glenn and Kimberly M. Engler* *Professor and Extension Specialist in Urban Entomology; Associate Research Scientist; Research Associate; and Program Specialist?Urban IPM; The Texas A&M University System...

  7. How to Select a Termite Control Service 

    E-Print Network [OSTI]

    Gold, Roger E.; Merchant, Michael E.; Howell Jr., Harry N.; Glenn, Grady J.

    2005-12-05

    Service E-369 12/05 Roger E. Gold, Michael E. Merchant, Harry N. Howell, Jr., and Grady J. Glenn* *Professor and Extension Specialist in Urban Entomology; Professor and Extension Urban Entomologist; Associate Research Scientist, Research Associate, Center...

  8. Curriculum for Liberal Education A Guide for Students, Advisors & Faculty

    E-Print Network [OSTI]

    Curriculum for Liberal Education A Guide for Students, Advisors & Faculty 2009 - 2010 Updated: June 2009 Note: As of October 2006, the University Core Curriculum was renamed the Curriculum for Liberal Education #12;2 The Curriculum for Liberal Education (CLE) at Virginia Tech Welcome to the CLE Guide

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

    E-Print Network [OSTI]

    Capecchi, Mario R.

    CLE. Lunch Provided. March 10 Green Bag Lessons from Disasters: What We Are Learning from the BP Deepwater Blowout in the Gulf of Mexico That We Should Have Learned 21 Years Ago in Alaska Zygmunt Jan Broël of Law 1 hour CLE. Lunch Provided. Wallace Stegner Lecture Classic Lessons from a Little Fish in a Pork

  10. 50 Years of Treaty Verification from Space Operational Satellite

    E-Print Network [OSTI]

    of the universe. The Vela satellites discovered bursts of gamma- ray energy emanating from beyond the solar system gamma-ray burst measured with Vela (Credit: R. Klebesadel, I. Strong & R. Olson (LANL) NASA Swift Spacecraft devoted to the study of cosmic gamma-ray bursts (Credit: NASA/GSFC) The U.S. Nuclear Detonation

  11. Particulate matter and atherosclerosis: role of particle size, composition and oxidative stress

    E-Print Network [OSTI]

    Araujo, Jesus A; Nel, Andre E

    2009-01-01

    California Particle Center (SCPC) are consistent with theParti- cle Center space (SCPC) and the University ofOne limitation of the SCPC study is that the concentrator

  12. If your codes run much slower than before the maintenance on...

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

    or run much slower than before after recompilation. We believe this is due to some regression introduced in the new CLE version, and have filed a bug with Cray. If you find your...

  13. U.S. NAVAL ACADEMY COMPUTER SCIENCE DEPARTMENT

    E-Print Network [OSTI]

    Crabbe, Frederick

    of a Military RC project would be the Predator UAV (Unmanned Areal Vehi- cle). The Predator1 is flown from UAV and similar programs can be found at: http://en.wikipedia.org/wiki/Unmanned_ aerial

  14. How Things Get Stuck: Kinetics, Elastohydrodynamics, and Soft Adhesion Madhav Mani,1,* Arvind Gopinath,2

    E-Print Network [OSTI]

    Mahadevan, L.

    the colloid and the substrate, the viscous drag on the sphere is dominated by lubrication forces assume that the reaction is diffusion limited), exerting an elastic force on the parti- cle. If binding

  15. Insects of the Garden, With a Chapter on the Melon Louse and Other Aphids. 

    E-Print Network [OSTI]

    Conradi, Albert F. (Albert Frederick); Sanborn, C. E.

    1906-01-01

    Cle MISS M. H. WATKINS ........................................ 1 . Stenograp? tor :or rol ~t-k ,A ier STATE SUB-STATIONS S. A. WASCHKA, superintendent ........... .................. Trou p Smith County W. S. HOTCHKISS, Superintendent... .......... ........ ... ............................................................................................................ 18 Squash .............................................................................................................................. .......................... 18 Onion...

  16. FESAC Mee)ng Monday 16 June 2014

    E-Print Network [OSTI]

    >vi>es of the FESAC Strategic Planning (SP) panel, refer to hUps://www.burningplasma.org/ac)vi)es/?ar)cle=2014%20FESAC%20Strategic%20Planning%20Panel Adjourn #12;Presenta

  17. A

    Office of Environmental Management (EM)

    Board 6. Make sure that your car is in good operating condi- tion. Be prepared for an emergency, it's a good idea to carry the following items in your vehi- cle. 1. Jumper...

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

    E-Print Network [OSTI]

    Han, Seunghee

    2005-02-17

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

  19. CX-006312: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

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

  20. Languages of the World Kevin Duh

    E-Print Network [OSTI]

    Duh, Kevin

    is a dialect with an army and navy" ­ Max Weinreich ­E.g. Chinese "dialects Sprachbund: Albanian, Greek, Romanian, Bulgarian, Macedonian à verb-Not-verb, post-ar?cle,

  1. Prospects and alterna.ves for development of US stellarator program

    E-Print Network [OSTI]

    equilibrium and stability -Energy, par^cle, and impurity transport -Alpha par.1-0.4% (reduced neoclassical xport) Quasi-axisymmetry (RS tokamak) Compact system size 5 W% Helical ripple 1% (reduced neoclassical xport) Isodynamic (Shafranov shiq ~ 0

  2. Major_Projects_Quick_Starts_Jobs_Creation_Office_Clean_Coal.pdf...

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

    MajorProjectsQuickStartsJobsCreationOfficeCleanCoal.pdf MajorProjectsQuickStartsJobsCreationOfficeCleanCoal.pdf MajorProjectsQuickStartsJobsCreationOfficeCle...

  3. The NC1/Endostatin Domain of Caenorhabditis elegans Type XVIII Collagen Affects Cell Migration and Axon Guidance

    E-Print Network [OSTI]

    Ackley, Brian D.; Crew, Jennifer R.; Elamaa, Harri; Pihlajaniemi, Tania; Kuo, Calvin J.; Kramer, James M.

    2001-03-19

    Type XVIII collagen is a homotrimeric basement membrane molecule of unknown function, whose COOH-terminal NC1 domain contains endostatin (ES), a potent antiangiogenic agent. The Caenorhabditis elegans collagen XVIII homologue, cle-1, encodes three...

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

    E-Print Network [OSTI]

    Siewert, Charles E.

    . SIEWERT,J. R. MAIORINO~,and M. N. ~ZISIK Departments of Nuclear and Mechanical Engineering, North Carolina + &+#J(v, CL)e+ dv + &(T, CL). (3) -I tpermanent address: Instituto de Energia At

  5. Influence of rainfall on the retention of sludge trace metals by the leaves of forage crops 

    E-Print Network [OSTI]

    Jones, Stephen Grady

    1977-01-01

    INFLUENCE OF RAINFALL ON THE RETENTION OF SLUDGE TRACE METALS BY THE LEAVES OF FORAGE CROPS A Thesis STEPHEN GRADY JONES Submitted to the Graduate College of Texas A&M University in partial fulfillment of the requirement for the degree... of MASTER OF SCIENCE December 1977 Major Subject: Soil Science INFLUENCE OF RAINFALL ON THE RETENTION OF SLUDGE TRACE MFTALS BY THE LEAVES OF FORAGE CROPS A Thesis by STEPHEN GRADY JONES Approved a to style and content by: 1 (Chairman of Committee...

  6. The Eyes of Texas Are Upon You

    E-Print Network [OSTI]

    Trimble, V

    2013-01-01

    Nemiroff, A century of gamma ray burst models. Comments onwere important. 4 The Gamma Ray Burst Saga The Vela andstreams were the first gamma ray bursts (from 1967 onward),

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

    Office of Science (SC) Website

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

  8. Operated by Los Alamos National Security, LLC for the U.S. Department...

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

    and Our Evolving Universe Slide 8 Touched by a supernova: * Discovery by Vela of gamma ray bursts (Klebesadel et al., 1973) Exploding stars, a window into the early universe and...

  9. Pre-Service Teachers' and Students' (Mis)Conceptions About the Equal Sign 

    E-Print Network [OSTI]

    Vela, Katherine

    2012-02-14

    -SERVICE TEACHERS? AND STUDENTS? (MIS)CONCEPTIONS ABOUT THE EQUAL SIGN A Thesis by KATHERINE NICOLE VELA Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER... OF SCIENCE December 2011 Major Subject: Curriculum and Instruction Pre-Service Teachers? and Students? (Mis)Conceptions About the Equal Sign Copyright 2011 Katherine Nicole Vela PRE...

  10. Barbara DeHaven Executive Director

    E-Print Network [OSTI]

    Yang, Eui-Hyeok

    Jessica Grady Postaward Specialist Steve Berhang Director ­ Sponsored Contracts and Export Controls Office and resolution Review and negotiate research contracts Negotiate and issue all subcontracts Provide expertise FCOI; ITAR, IRB, IACUC and IBSC; Small Business Subcontracting Plans; OSP-specific section

  11. MA Thesis Degree Program Checklist By End of Second Term

    E-Print Network [OSTI]

    Arnold, Jonathan

    MA Thesis Degree Program Checklist By End of Second Term ( ) Select major professor and other two Advisory Committee members. ( ) Submit Program of Study. ( ) Submit thesis proposal to Advisory Committee for approval. ( ) Submit copy of approved thesis proposal to Grady Graduate Studies Office. ( ) Pick up thesis

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

    E-Print Network [OSTI]

    Mohanty, Saraju P.

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

  13. Corn Variety Experiments, Substation no. 3, Angleton, Texas. 

    E-Print Network [OSTI]

    Reynolds, E. B. (Elbert Brunner)

    1921-01-01

    1777 1330 1983 1712 Mosby's Prolific. Munson. Oklahoma Yellow Dent. Rockdale. St. Charles White. Sllrcropper. Surcropper. . Surcropper. Surcropper. Tankersley. Thomas. Virginia White Dent. ' Ferguson Yellow Dent. Given's Red Cob.... Golden Dent. . Gorham's Yellow Dent. Hastings' Prolific. Henry Grady. Improved Indian Squaw. Improved Indian +.Squaw. Improved Learning. Mosby's Prolific. Munson. Oklahoma White Wonder. 2444 1713 2425 2435 2424 2445 1777 2420 327...

  14. PUBLISHED ONLINE: 20 JUNE 2010 | DOI: 10.1038/NPHYS1686 Propulsion generated by diffusion-driven flow

    E-Print Network [OSTI]

    Loss, Daniel

    processes, including mineral transport in rocks2 , the melting of icebergs3 and the migration of tectonic = 0.40 m, width W = 0.20 m and length L=0.40 m, filled with salt-stratified water with density gradi

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

    E-Print Network [OSTI]

    Huang, Shaopeng

    including the continental landmasses. Based on world- wide meteorological and borehole tempera- ture records is expected to increase linearly with depth with a geothermal gradi- ent determined by the subsurface thermal readings while lowering a thermometer into a borehole. There are thousands of boreholes drilled origi

  16. doi:10.1152/ajpgi.00073.2012 303:G894-G903, 2012. First published 16 August 2012;Am J Physiol Gastrointest Liver Physiol

    E-Print Network [OSTI]

    Bogyo, Matthew

    Austin W. Walker,1 Margot Paulick,2 Daniel Cox,1 Jordan Cloyd,1 James Buxbaum,3 James Ostroff,3 Matthew Cox, Jordan Cloyd, James Buxbaum, James Ostroff, Matthew Victoria Lyo, Fiore Cattaruzza, Tyson N. Kim Gastrointest Liver Physiol Bogyo, Eileen F. Grady, Nigel W. Bunnett and Kimberly S. Kirkwood Paulick, Daniel

  17. Weierstra-Institut fr Angewandte Analysis und Stochastik

    E-Print Network [OSTI]

    Mielke, Alexander

    -rule, energy-dissipation balance, integrated evolutionary variational estimate, energetic solutions, energy functional, dissipation potential, dissipation distance, gradi- ent flows, Gamma convergence-303 E-Mail: preprint@wias-berlin.de World Wide Web: http://www.wias-berlin.de/ #12;Abstract

  18. Research Article An Age-Related Deficit in

    E-Print Network [OSTI]

    Scholl, Brian

    ) with age (Grady, 2000; Gunning-Dixon & Raz, 2000; O'Sullivan et al., 2001; Raz, 2000; West, 1996), strongly; Logan, Sanders, Snyder, Morris, & Buckner, 2002; Park, Polk, Mikels, Taylor, & Mar- shuetz, 2001; Reuter-Lorenz, 2002; Reuter-Lorenz, Marshuetz, Jonides, & Smith, 2001; Stebbins et al., 2002): Sometimes older adults

  19. FeaFiner: Biomarker Identification from Medical Data through Feature Generalization and Selection

    E-Print Network [OSTI]

    Lu, Zhaosong

    .J. Watson Research Center, Yorktown Heights, NY ABSTRACT Traditionally, feature construction and feature-convexity objective and non-smoothness penal- ties. We apply a recently developed augmented Lagrangian method to solve this formulation in which each subprob- lem is solved by a non-monotone spectral projected gradi- ent method. Our

  20. The Mobile Web Comes of Age

    E-Print Network [OSTI]

    Chen, Yuanzhu Peter

    The Mobile Web Comes of Age Steven J. Vaughan-Nichols T he mobile Web has changed dramatically can do on the Web, said Stephen O'Grady, cofounder of and analyst with Red- Monk, a market research, such as phones, now have larger screens with better resolution, making Web browsing more worthwhile, noted

  1. IEEE TRANSACTIONS ON COMPUTERS 1 Optimizing Hardware Function Evaluation

    E-Print Network [OSTI]

    Mencer, Oskar

    present a methodology and an automated system for function evaluation unit generation. Our system selects(x) and x accurate to one unit in the last place using MATLAB and ASC, A Stream Compiler for Field on function evaluation operations in a simulation of a jet engine reported by O'Grady and Wang [1

  2. Improved repeat identification and masking in Dipterans Christopher D. Smith1,2,,*, Robert C. Edgar3,, Mark D. Yandell4, Douglas R. Smith5, Susan

    E-Print Network [OSTI]

    Yandell, Mark

    Heterochromatin Genome Project, Lawrence Berkeley National Laboratory, Berkeley, CA. 3Tiburon, CA., bob@drive5.com, such as Drosophila melanogaster and Anopheles gambiae, are estimated to be 30-60% repetitive. Mammalian genomes in genome architecture and inheritance, including centromere function (Grady et al., 1992), generation

  3. 1A-01 C JOG System Engineering, IncA-1 SHIPBOARD SYSTEM INTERFACE

    E-Print Network [OSTI]

    SPACE-TIME MATTER-ENERGY MILKY WAY GALAXY OTHER GALACTIC MATTER SPIRITUAL ENTITY SOLAR SYSTEM EARTH1A-01 C JOG System Engineering, IncA-1 SHIPBOARD SYSTEM INTERFACE DEVELOPMENT Presented at the Naval Post Graduate School August 12, 2004 Jeffrey O. Grady President, JOG System Engineering, Inc. 6015

  4. University of Virginia Housing Areas

    E-Print Network [OSTI]

    Huang, Wei

    University of Virginia Housing Areas Copeley Hill Faulkner Copeley III & IV Piedmont Hereford Gardens Lile-Maupin House 2372 Tuttle - Dunnington House 2373 Shannon House 2374 Gibbons House 2375 IvyGardensWay Tree House Drive Grady Avenue University Court Farrish Circle W estview Road Engineer'sWay Gildersleve

  5. Departamento de Matematica do IST, Secc~ao de Algebra e Analise Analise Matematica III

    E-Print Network [OSTI]

    Nunes, João Pimentel

    por arcos. Teorema fundamental do c´alculo para inte- grais de linha. Conserva¸c~ao de energia mec^anica vectorial seja gradi- ante. C´alculo de fun¸c~oes potenciais. 12. Homotopia. Invari^ancia de integrais de conjuntos em estrela em R3 . Exemplo de campo solenoidal sem potencial vectorial: campo gravitacional de uma

  6. JUST-IN-TIME SCHEDULES FOR THE SMALL MAKE-TO-ORDER SHOP

    E-Print Network [OSTI]

    Sinnamon, Gordon J.

    The University of Western Ontario and Fraser Valley College October 15, 1996 Abstract. In order to use Just, Hewlett-Packard and Harley Davidson [O'Grady 1988], to General Electric, RCA, the Pontiac division of GM to correct bottlenecks, sources of defects, under-utilized stations, and even poor shop layouts. The ability

  7. Moore, J. C, Mascle, A., et al., 1990 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 110

    E-Print Network [OSTI]

    scales of tens to tens of thousands of years. High heat flow in the vicinity of 15°30'N and not elsewhere. Surface heat-flow values from Leg110(calculated from geothermal gradients forced through the bottom forearc and trench sediments. Geothermal gradi ents in the upper kilometer of sediment that extrapolate

  8. Drywood Termites 

    E-Print Network [OSTI]

    Gold, Roger E.; Glenn, Grady J.; Howell Jr., Harry N.; Brown, Elizabeth

    2005-12-05

    or reproductives, winged male and female Youngest nymph Older nymph Reproductive nymph Reproductives after loss of wings King Queen Eggs Figure 2. Termite life cycle. Figure 1. Distribution of drywood termites in Texas. I Roger E. Gold, Grady J. Glenn, Harry N...

  9. Formosan Subterranean Termites 

    E-Print Network [OSTI]

    Gold, Roger E.; Glenn, Grady J.; Howell Jr., Harry N.; Keck, Molly

    2005-12-05

    are also a honey- brown color and are about the same size as Roger E. Gold, Grady J. Glenn, Harry N. Howell, Jr. and Molly Keck* F 2 the wings and characteristics of the head (Fig. 3). If identification is in doubt, the termites should be submitted...

  10. Phylogeography and Meta-Community Analysis in QGIS

    E-Print Network [OSTI]

    Cavner, Jeff; Beach, James H.; Stewart, Aimee M.; Grady, C.J.

    2014-11-19

    Lifemapper Jeff Cavner, Jim Beach, Aimee Stewart, CJ Grady Informatics, Biodiversity Institute, KU P h y l o g e o g r a p h y a n d M e t a Co m m u n i t y A n a l y s i s i n Q g i s Lifemapper Species Occurrence Data Potential Habitat...Lifemapper Jeff Cavner, Jim Beach, Aimee Stewart, CJ Grady Informatics, Biodiversity Institute, KU P h y l o g e o g r a p h y a n d M e t a Co m m u n i t y A n a l y s i s i n Q g i s Lifemapper Species Occurrence Data Potential Habitat...

  11. Effect of grain on silage characteristics for ruminants 

    E-Print Network [OSTI]

    Groves, William Grady

    1977-01-01

    F 'C'1' QZ GRAI!i OU SILAG" CHA~ACZ ';. ISTIC', ~OR RU1'IliuA1TS A ihesis by '. vl' 1. IA11 GRADY GROV~ S Sub. ~i ted to the Graduate Colle'e of Texas A~~", Univsrsity in partial fulfill:nant of the re", .ui anent for the de~res of , EST...:. . . OZ SCI=11C=- ilay " '&77 i. ajor' Su'ojac: Ani:nal 1ut rition =FFECI' OF GRAIN ON SILAG ~ CNARACT 'RIG TICS FOR PUIIINANTS A Thesis by ". /ILLIAi'I GRADY GROVES Approved as to style and content by: airman of Coi-. . sittee H a ~ Dep rti...

  12. Generation Y in the Workplace 

    E-Print Network [OSTI]

    Brown, Sky; Carter, Britt; Collins, Michael; Gallerson, Christopher; Giffin, Grady; Greer, Jon; Griffith, Ray; Johnson, Emily; Richardson, Kate

    2009-01-01

    stream_source_info 2009GenerationYintheWorkplace.pdf.txt stream_content_type text/plain stream_size 155407 Content-Encoding ISO-8859-1 stream_name 2009GenerationYintheWorkplace.pdf.txt Content-Type text/plain; charset=ISO-8859...-1 Generation Y in the Workplace Sky Brown Britt Carter Michael Collins Christopher Gallerson Grady Giffin Jon Greer Ray Griffith Emily Johnson Kate Richardson Faculty Advisor: Dr. Domonic Bearfield i Executive Summary...

  13. 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]

    Holt, Grady Lynn

    1974-01-01

    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...

  14. An AVO method toward direct detection of lithologies combining P-P and P-S reflection data 

    E-Print Network [OSTI]

    Carcuz Jerez, Juan Ramon de Jesus

    2004-09-30

    of the intercepts and gradients [APP : RPP in- tercept; BPP : RPP gradient; APS: R0PS intercept; and BPS: R0PS gradient]. : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : 18 2.3 Estimated and actual values of ¢VP =VP ;¢VS=VS;¢½=½, and VP =VS... chapter II [VP : P¡wave velocity; VS : S¡wave veloc- ity; and ½ : density]. : : : : : : : : : : : : : : : : : : : : : : : : : : : 37 3.2 Intercepts and gradients [APP : RPP intercept; BPP : RPP gradi- ent; APS: R0PS intercept; and BPS: R0PS gradient...

  15. Curriculum for Liberal Education A Guide for Students, Advisors & Faculty

    E-Print Network [OSTI]

    Curriculum for Liberal Education A Guide for Students, Advisors & Faculty 2008 - 2009 Updated: June 2008 Note: As of October 2006, the University Core Curriculum was renamed the Curriculum for Liberal Education #12;2 The Curriculum for Liberal Education (CLE) at Virginia Tech This guide will assist students

  16. Curriculum for Liberal Education A Guide for Students, Advisors & Faculty

    E-Print Network [OSTI]

    Curriculum for Liberal Education A Guide for Students, Advisors & Faculty 2007 - 2008 Updated: July 2007 Note: As of October 2006, the University Core Curriculum was renamed the Curriculum for Liberal Education #12;2 The Curriculum for Liberal Education (CLE) at Virginia Tech This guide will assist students

  17. COLLEGE OF NATURAL RESOURCES AND ENVIRONMENT Bachelor of Science in Environmental Resources Management

    E-Print Network [OSTI]

    Virginia Tech

    Resources Management For Students Graduating in Calendar Year 2013 Environmental Resource Management Option and Water Res. Management 3 FOR 2314 Forest Biology and Dendrology 2 FOR 2554 Nature and Amer. Values(CLE2. Policy 3 UAP 4384 Pollution Control Plan/Policy 3 Aquatic Life Restricted Electivec 3 or 4 Geospatial

  18. Graham Greene's use of the christian concept of descent 

    E-Print Network [OSTI]

    Love, Frances Ann C

    1969-01-01

    '" ( p. 126). Pinkie does suffer and. descend, but it is a cle cent accoc!panied by faith in the devil: " Credo in unum Satanum, ' the 33oy said" (p. 165). Following the precepts of St. John of the Cross, Greene implies that a 'oelief in God must...

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

    E-Print Network [OSTI]

    Leemis, Larry

    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

  20. Tillman Creek Mitigation Site As-Build Report.

    SciTech Connect (OSTI)

    Gresham, Doug [Otak, Inc.

    2009-05-29

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

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

    E-Print Network [OSTI]

    Boyer, Edmond

    2003-01-01

    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

  2. Combustion in a Transonic Flow with Large Axial and Transverse Pressure Gradients

    E-Print Network [OSTI]

    Liu, Feng

    that we have named "turbine burners." References 1­7 present the progress to date on this emerging for bypass flows (turbofans), afterburners, and turbine burners. A simplified thermodynamic cy- cle portrayed for the turbine burner is given in Figure 2. Turbine burners are shown with continuous com- bustion through

  3. Atmos. Chem. Phys., 6, 211223, 2006 www.atmos-chem-phys.org/acp/6/211/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    metal source, ferrous metal source, gasoline vehi- cle, diesel vehicle, copper smelter and volcanic). The diesel vehicle source contributed the most in the ultra-fine size range (0.070.56 µm) and was responsible of the westerly wind latitude region of northeast Asia, many studies on the influence of long-range transport (LRT

  4. EUROGRAPHICS Workshop on Sketch-Based Interfaces and Modeling (2007), pp. 18 M. van de Panne, E. Saund (Editors)

    E-Print Network [OSTI]

    Vetter, Thomas

    2007-01-01

    in the automotive industry is a time-consuming process. Iterations between concept sketches created with traditional representations 1. Introduction In the automotive industry, most steps of the design cy- cle have been digitized in the automotive industry. Even small changes to the concept model can be cumbersome and could require start- ing

  5. LASER & PHOTONICS www.lpr-journal.org

    E-Print Network [OSTI]

    Jalali. Bahram

    -processing of wideband signals can boost the performance of electronic digitizers. In this arti- cle, the underlying principle of the time-stretch analog-to-digital converter (TSADC) that addresses the demands on resolution of information. However, most physical- world signals are analog in nature and analog-to-digital converters (ADCs

  6. STRATEGIC REPORT 2007 COVER: EARTH AND SUNRISE. PHOTO ILLUSTRATION BY RISTESKI GOCE

    E-Print Network [OSTI]

    de Weck, Olivier L.

    AERO-ASTRO STRATEGIC REPORT 2007 #12;COVER: EARTH AND SUNRISE. PHOTO ILLUSTRATION BY RISTESKI GOCE and excellence in these three areas are critical for producing scientific, industrial, and societal advances of the technologies critical to aerospace vehi- cle and information engineering, and to the architecture

  7. Generalized Streak Lines: Analysis and Visualization of Boundary Induced Vortices

    E-Print Network [OSTI]

    Tricoche, Xavier

    fluid flow datasets from computational fluid dynamics simulations. Index Terms--Skin friction INTRODUCTION Simulation and visualization of fluid flows plays an important role dur- ing the design process on the drag coefficient, which affects fuel efficiency and overall vehi- cle performance. In turbines

  8. Mechanobiology of the Aortic Heart Valve Jonathan T. Butcher1

    E-Print Network [OSTI]

    Simmons, Craig A.

    Review: Mechanobiology of the Aortic Heart Valve Jonathan T. Butcher1 , Craig A. Simmons2 , James N valve, positioned between the left ventri- cle and aortic root, prevents retrograde flow of blood into the ventricle during diastole. Opening and closing of the valve occurs passively in response to inertial forces

  9. MouStress: Detecting Stress from Mouse Motion David Sun1,2

    E-Print Network [OSTI]

    Canny, John

    -hand dynamics that captures mus- cle stiffness during mouse movement. We show that the within-subject mouse interfaces, mouse interaction ACM Classification Keywords H.5.2 User Interfaces (H.1.2, I.3.6): Theory and methods, Input devices and strategies INTRODUCTION Stress has a profound impact on the emotional

  10. College of Science Bachelor of Science, Psychology

    E-Print Network [OSTI]

    Zallen, Richard

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

  11. Econometrics: A Bird's Eye View

    E-Print Network [OSTI]

    Geweke, John; Horowitz, Joel; Pesaran, M Hashem

    cycle of about 7—11 years duration, commonly known as the Juglar cycle. Other economists such as Kitchin, Kuznets and Kondratieff followed Juglar’s lead and discovered the inventory cycle (3—5 years duration), the building cy- cle (15—25 years duration...

  12. Transportation Research Record: Journal of the Transportation Research Board, No. 2247, Transportation Research Board of the National Academies, Washington,

    E-Print Network [OSTI]

    Bertini, Robert L.

    24 Transportation Research Record: Journal of the Transportation Research Board, No. 2247, Transportation Research Board of the National Academies, Washington, D.C., 2011, pp. 24­32. DOI: 10 for different types of vehi- cle and bicycle infrastructure is needed to understand how to lower exposures

  13. LANL: AOT & LANSCE The Pulse November 2010

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

    Phys- ics in leAD-zirconium- titAnium voltAge bArs 5 los AlAmos lenDs its exPertise to cleAn energy AnD cArbon sequestrAtion Projects 6 electric-FielD moDiFicA- tion oF mAgnetism...

  14. Conserving Energy in Real-Time Storage Systems with I/O Burstiness

    E-Print Network [OSTI]

    Qin, Xiao

    20 Conserving Energy in Real-Time Storage Systems with I/O Burstiness ADAM MANZANARES, XIAOJUN RUAN of Southern Mississippi Energy conservation has become a critical problem for real-time embedded storage, energy conservation for real-time embedded storage systems is still an open problem. In this arti- cle

  15. An important recenttechnologicaldevelopmentin commercialF-T conversionis "liquid-phase" synthesis. In a liquid phasereactor,the feedgasis bubbled througha heavyoil (e.g.,the waxy

    E-Print Network [OSTI]

    the F-T synthesisreactions. 2.3. F-T conversion of biomass Theprocessfor converting biomassinto F gasificationto maximize conversionto Gasification F-T liquids. Biomassis &Gas morereactive thancoal, Bianass-T synthesis Gasification GasTurbine&Gas F-T Combined8edJ1d!yreactor. Unconvertedgas,ratherthan Bicxnas Cle

  16. A dynamic grouping strategy for implementation of the particle filter on a massively parallel computer

    E-Print Network [OSTI]

    Nakano, Shin'ya

    computer Shin'ya Nakano The Institute of Statistical Mathematics Tachikawa, Tokyo, Japan. shiny@ism.ac.jp Abstract ­ A practical way to implement the parti- cle filter (PF) on a massively parallel computer is dis to be computation- ally expensive in applying to high-dimensional problems because a enormous number of particles

  17. 10.1177/0270467603256089ARTICLEBULLETIN OF SCIENCE, TECHNOLOGY & SOCIETY / August 2003Yamaguchi / WHOSE SUSTAINABLE DEVELOP-MENT? Whose Sustainable Development?

    E-Print Network [OSTI]

    Delaware, University of

    Policy and Funding for Energy Sector Projects Hideka Yamaguchi Center for Energy and Environmental Policy. As an alternative, this arti- cle suggests a policy of promoting small and decen- tralized renewable energy technology. Keywords: Japanese foreign aid policy, energy sector, sustainable development, ODA, development

  18. Proceedings of the ASME 2013 International Design Engineering Technical Conferences & Computers and Information in Engineering Conference

    E-Print Network [OSTI]

    Papalambros, Panos

    a systematic way to identify the optimal architecture for a given vehicle drive cycle, rather than-optimal pair of modes for a given driving cycle and vehi- cle specification. In a study this process identifies architecture over a standard drive cycle. 1 Introduction A variety of hybrid-electric vehicle (HEV

  19. An inventory of invasive alien species in China 1 An inventory of invasive alien species in China

    E-Print Network [OSTI]

    Kratochvíl, Lukas

    An inventory of invasive alien species in China 1 An inventory of invasive alien species in China of invasive alien species in China. NeoBiota 15: 1­26. doi: 10.3897/neobiota.15.3575 Abstract Invasive alien: 10.3897/neobiota.15.3575 www.pensoft.net/journals/neobiota review ArtiCle Advancing research on alien

  20. Atmos. Chem. Phys., 10, 32613272, 2010 www.atmos-chem-phys.net/10/3261/2010/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    and Physics Parametric studies of contrail ice particle formation in jet regime using microphysical parcel (contrails) formed from water vapor emissions behind aircraft engines are the most uncer- tain components cloud formation, understanding of contrail ice parti- cle formation immediately after aircraft engines

  1. Lifecycle Knowledge Management: Getting the Semantics Across in X-Media

    E-Print Network [OSTI]

    Staab, Steffen

    of product lifecy- cle knowledge for complex industrial products (such as cars or jet engines) by targeting. What happens, when maintenance tech- nicians or pilots perceive unusual sound or vibration of a jet engine? Usually, the relevant pieces of problem-related information are scattered across several systems

  2. Atmos. Chem. Phys., 13, 91419158, 2013 www.atmos-chem-phys.net/13/9141/2013/

    E-Print Network [OSTI]

    Meskhidze, Nicholas

    ) of emissions from a modern (Euro 5) gasoline car operated during a driving cy- cle (New European Driving Cycle vehicle emissions in a new mobile environmental reaction chamber S. M. Platt1, I. El Haddad1, A. A, 5232, Switzerland 2Institute for Energy and Transport, Sustainable Transport Unit, European Commission

  3. This Week in The Journal F Cellular/Molecular

    E-Print Network [OSTI]

    - tionhasbeenlinkedtomentalretardationin humans. OE Development/Plasticity/Repair VTA Projections to Motor Cortex Are Required for Motor and are involved in reward, emotion, and cognition. Dopami- nergic terminals are also found in the pri- mary motor in the PRF. Neurobiology of Disease Molecular Tolerance to Ethanol Depends on Exposure Duration Cristina Vela

  4. Premio Perini Navi S.p.A. IL COMITATO LEONARDO ITALIAN QUALIT COMMITTE HA

    E-Print Network [OSTI]

    Segatti, Antonio

    1 Premio Perini Navi S.p.A. IL COMITATO LEONARDO ­ ITALIAN QUALITÀ COMMITTE ­ HA DELIBERATO DI DELEGATO DI PERINI NAVI SPA. - ANNO 2011 - "Progetto di un natante ad uso tender per un'imbarcazione a vela dalla direzione della Perini Navi S.p.A. FINALITÀ: Premiare i due migliori progetti relativi ad un

  5. Proceedings of the 2002 IEEE International Conference on Robotics and Automation, pp. 756-762 Trajectory Stabilization

    E-Print Network [OSTI]

    -762 Trajectory Stabilization for a Planar Carangiform Robot Fish Kristi A. Morgansen , Patricio A. Vela , Joel W: This paper considers the task of trajectory sta- bilization for a fish-like robot by means of feedback. We present a specific model of a planar carangiform fish, and verify the stabilization results

  6. Two types of glitches in a solid quark star model

    E-Print Network [OSTI]

    Zhou, Enping

    2015-01-01

    Glitch (sudden spinup) is a common phenomenon in pulsar observations. However, the physical mechanism of glitch is still a matter of debate because it depends on the puzzle of pulsar's inner structure, i.e., the equation of state of dense matter. Some pulsars (e.g., Vela-like) show large glitches ({\\Delta}{\

  7. Imagen de esfera parcialmente sumergidaImagen de esfera pa rcialmente sumergida

    E-Print Network [OSTI]

    Vela-Arevalo, Luz V.

    Teorema Pi y la modelaci´on P´ag. 29 Luis Quintanar Medina La trayectoria del cometa Oterma P´ag. 35 Luz Morales Comit´e Editorial: Dr. Jorge Eduardo Mac´ias D´iaz, jmacias@correo.uaa.mx Dra. Luz Vianey Vela Ar

  8. Imagen de esfera parcialmente sumergidaImagen de esfera pa rcialmente sumergida

    E-Print Network [OSTI]

    Vela-Arevalo, Luz V.

    y la modelaci´on P´ag. 29 Luis Quintanar Medina La trayectoria del cometa Oterma P´ag. 35 Luz Vianey´e Editorial: Dr. Jorge Eduardo Mac´ias D´iaz, jmacias@correo.uaa.mx Dra. Luz Vianey Vela Ar´evalo, lvela

  9. Gamma Ray Bursts Sudden, intense flashes of gamma rays

    E-Print Network [OSTI]

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

    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

  10. HAPPENING THIS WEEK NEWSLETTER FOR OCTOBER 14th -OCTOBER 21st

    E-Print Network [OSTI]

    Lawrence, Rick L.

    VaNCE FOR $500. #12;SAvE THE DATE CELEBRaTE aLTERNaTiVE ENERgy RESOURCES ORga- NizaTiON'S 40Th aNNiVERSaRy iN REd WiTh aN EVENiNg dEVOTEd TO ELECTRiC VEhiCLES aNd BiOdiESEL. ThE EVENT WiLL CONSiST OF a paNEL OF ExpERTS ON EVSRk, idahO NaTiONaL LaBORaTORy, adVaNCEd VEhiCLE TEChNOLOgy RON gOmpERTz, BOzEmaN ELECTRiC VEhiCLE ExpERT Ca

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

    SciTech Connect (OSTI)

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

    2011-10-01

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

  12. Measurement of the ?(0)(b) Lifetime Using Semileptonic Decays

    E-Print Network [OSTI]

    Baringer, Philip S.; Bean, Alice; Hensel, Carsten; Moulik, Tania; Wilson, Graham Wallace; Abazov, V. M.; Abbott, B.; Abolins, M.; Acharya, B. S.; Adams, M.

    2007-10-30

    . Chan,5 A. Chandra,48 F. Charles,18 E. Cheu,45 F. Chevallier,13 D.K. Cho,62 S. Choi,31 B. Choudhary,27 L. Christofek,77 T. Christoudias,43 S. Cihangir,50 D. Claes,67 C. Cle´ment,40 B. Cle´ment,18 Y. Coadou,5 M. Cooke,80 W. E. Cooper,50 M. Corcoran,80 F.... The expected number of signal events in each bin, nei , is given by nei #6; Ntot R i f#4; M#5;d M, where Ntot is the total number of #1;#1;#2;c events, and f#4; M#5; is the probability density function (PDF) for M. The integration is done within the range of a...

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

    SciTech Connect (OSTI)

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

    2008-05-01

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

  14. An investigation of the oil from the seed of Citrullus vulgaris 

    E-Print Network [OSTI]

    Tsao, Chung Min

    1951-01-01

    - ~ && rW~~ TABLE II FRACTICSATI08 CF ~~ ESTEBS QF THE SOLID ACIDS Fraction Mt. , g. B. P. , C, Sap. Eq. I. V. Eaters af S t. Acids @ 2 m Hg ~C 016 ~C OLeate Sl 4'23 130-150 269. 2 5. 88 0. 35 3. 59 ? 0. 29 S2 7. 63 150-164 285. 0 23. 90 ? 3. 33 2... 3. 1 TABLE III fRACTI(NATION OF HTBTL ESTERS OF THE LIQUID ACIDS Fraction Wt. , g. B. P. , W, Sap. Eq. I. V. Saturated I4oncothenoic Diethenoic e 2 HE 014 016 014 016 Cle Cle 1. 86 132-155 255. 3 34. 8 0. 36 0, 85 0. 29 0. 36 Lz 20. 14 155 165...

  15. (Human Papillomavirus: HPV) HPV 8kb DNA

    E-Print Network [OSTI]

    Zhang, Byoung-Tak

    , 35 . cluster 1 2 3 4 5 6 9 10 3-mer seq. TLE RFH KRR DLC TTL SVY VYR PAE RRF IRC IRC LCD KPL FAF EVL WTG VEE CCK AFR RCC RRL KPL GLH IRC WRG LLC PYG ISG LRL CLL RPR EEK VYR RFH PRT IRC EKQ WTG HNI SKI LCH QLC AST VFC CVF VEK PLC CLE AAC IRC EKL RTV IRC VRN KLL AEK DLV LCR SLC LEF TAT FLD WKG

  16. Appel%%Projets% Formations%pluridisciplinaires%en%master%

    E-Print Network [OSTI]

    Bordenave, Charles

    %du%projet% Couleur!et!Design!Thinking! Nom%du%porteur% Delphine!Talbot!et!Céline!Caumon! Contact%% (mail!et!téléphone)% Delphine.talbot@univ;tlse2.fr! 06!63!04!08!11! Etablissement/Ecole% IUP!Arts!Appliqués!Couleur!Image!Design!Lemercier!(MCF!HDR,!CLE!LTC,!UT2)! Céline!Poisson!(PR,!UQAM,!Québec)! Marc!Boyer!(MCF,!IUT!GEAR,!INSERM,!UT3)! Georges

  17. 000075 /Bonnet, Rpke, Scarpi 20.07.06 11:55 Du nom des images d'Isis polymorphe

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    000075 /Bonnet, Rpke, Scarpi 20.07.06 11:55 Du nom des images d'Isis polymorphe Laurent Bricault 1 Anciens et Modernes face aux images d'Isis L'e´volution la plus imme´diatement perceptible d'Isis dans l´e des sources grecques d'E´gypte ­ et d'ailleurs ­ jusqu'au milieu du IVe sie`cle av. J.-C., Isis

  18. Laredo 2010-2035 Metropolitan Transportation Plan 

    E-Print Network [OSTI]

    Laredo Urban Transportation Study

    2009-12-11

    ?Rivera,?PE? Linda?Vela The?preparation?and?publication?of?this?report?was?financed?in?part?through?grants?from?the? Federal?Highway?Administration,?the?Federal?Transit?Administration,?and?the?Texas? Department?of?Transportation.?All?opinions,?findings,?and...?conclusions?presented?in?this?report? reflect?the?view?of?the?Plan?authors?and?do?not?necessarily?reflect?the?official?views?or?policy? of?the?Federal?Highway?Administration,?the?Federal?Transit?Administration,?or?the?Texas? Department?of?Transportation.? ? ? ? ? ? ? ? ? ? ? THIS...

  19. Design Studies and Commissioning Plans for PARS Experimental Program

    E-Print Network [OSTI]

    Mete, O; Xia, G; Dover, M; Wigram, M; Wright, J; Zhang, J; Smith, J

    2015-01-01

    PARS (Plasma Acceleration Research Station) is an electron beam driven plasma wakefield acceleration test stand proposed for VELA/CLARA facility in Daresbury Laboratory. In order to optimise various operational configurations, 2D numerical studies were performed by using VSIM for a range of parameters such as bunch length, radius, plasma density and positioning of the bunches with respect to each other for the two-beam acceleration scheme. In this paper, some of these numerical studies and considered measurement methods are presented.

  20. X-rays from Supernova Remnants

    E-Print Network [OSTI]

    B. Aschenbach

    2002-08-28

    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.

  1. The stellar wind velocity field of HD 77581

    E-Print Network [OSTI]

    Manousakis, A

    2015-01-01

    The early acceleration of stellar winds in massive stars is poorly constrained. The scattering of hard X-ray photons emitted by the pulsar in the high-mass X-ray binary Vela X-1 can be used to probe the stellar wind velocity and density profile close to the surface of its supergiant companion HD 77581. We built a high signal-to-noise and high resolution hard X-ray lightcurve of Vela X-1 measured by Swift/BAT over 300 orbital periods of the system and compared it with the predictions of a grid of hydrodynamic simulations. We obtain a very good agreement between observations and simulations for a narrow set of parameters, implying that the wind velocity close to the stellar surface is twice larger than usually assumed with the standard beta law. Locally a velocity gradient of $\\beta\\sim0.5$ is favoured. Even if still incomplete, hydrodynamic simulations are successfully reproducing several observational properties of Vela X-1.

  2. AVRAM user's manual

    SciTech Connect (OSTI)

    McGrady, P.W.

    1988-02-01

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

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

    SciTech Connect (OSTI)

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

    2015-05-15

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

  4. Contributions to the bioassay of Gymnodinium breve toxin(s) with mosquito fish (Gambusia affinis 

    E-Print Network [OSTI]

    Russell, Melvin Curtis

    1972-01-01

    solvents. See Figures 6-10 for dose response data 36 Mean death times of fish exposed to two con- t t' f d G~dt ' d t ' \\ 0. 06%%d polysorbate 80 (tween 80) solution to pro- vide reference points for tests with five solvent- toxin concentrations... solvents on bases of various 44 viii LIST OF FIGURES ~Fi ure P ~cle Dose-response curve for Gambusia affinis in poly- sorbate 80 (tween 80). Mean death time for each test group indicated by value to right of "X". Actual values of upper and lower...

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

    E-Print Network [OSTI]

    Patterson, Catherine

    2010-01-01

    science and art. This book highlights the important role of early modern thought in how we understand and express our psychic selves today. In a nearly transparent transla- tion by Jane Marie Todd... Keith Thomas. The Ends of Life: Roads to Fulfilment... future of the humanities in general and seventeenth-century studies in particular, H?fer?s study reaffirms the centrality of the grand si?cle through a timely return to a larger concept of the humanities, before that other dualistic split: between...

  6. Ambulatory infusion suite: pre- and post-occupancy evaluation 

    E-Print Network [OSTI]

    Shepley, Mardelle McCuskey; Rybkowski, Zofia; Aliber, Jennifer; Lange, Cathleen

    2015-02-08

    dans ce contexte. Mots cle´s: e´tablissement de lutte contre le cancer, e´valuation d’e´tablissement, soins de sante´, centre de perfusion, occupation, vie prive´e, interaction sociale Introduction This study focuses on an evaluation of infusion suites... facility, facility evaluation, healthcare, infusion suite, post-occupancy, privacy, social interaction Il est pre´sente´ une e´valuation de l’expe´rience ve´cue par les patients, les familles et les employe´s dans deux centres de perfusion. L’un des centres...

  7. An empirical parametric determination for a simulation model 

    E-Print Network [OSTI]

    Russell, Kenneth Ernest

    1967-01-01

    to that for the Sophomore Class ij j ii ) j-1 ilj-1 ij where the variables are now C j = the jth academic level in the ith year i, Ci 1 = freshman academic classification Ci 2 sophomore Ci S = junior t C. , = senior 1 ?4 Ci 5 = first year masters degree candidates... Class men Sophomore Class Junior Class Senior Class Rec cle Rec cl Drop Out~s X Drop)ilats ~ Drop Outs Graduates & Drop Outs Teaching Staff Transfers ~ansfers ~Tndfers Transfers& From Senior Class 1st Year Masters 2nd Year Meters-/ 1...

  8. Questioning the HIV-AIDS hypothesis: 30 years of dissent 

    E-Print Network [OSTI]

    Goodson, Patricia

    2014-09-23

    PUBLIC HEALTH OPINION ARTICLE published: 23 September 2014 doi: 10.3389/fpubh.2014.00154 Questioning the HIV-AIDS hypothesis: 30 years of dissent Patricia Goodson* Department of Health & Kinesiology, Texas A&M University, College Station, TX, USA... it is important to remember: over 60 conditions can yield a false-positive ELISA) (13, 18). Critics of the orthodox view decry the lack of standardized criteria for a positive result in a WB, across countries, world- wide (19). Bauer (Table 1), in a 2010 arti- cle...

  9. Experimental Results on Advanced Rotary Desiccant Dehumidifiers 

    E-Print Network [OSTI]

    Barathan, D.; Parsons, J. M.; MaClaine-Cross, I.

    1986-01-01

    and mass exchange, respectively. A mean Nusselt number Nu was derived as where and The results are plotted as the measured Nusselt number Nu versus a Craetz number Cr defined as in Figure 8. The Eigure indicates effective Nusselt number values oE Nul... = 4.5 (for test arti- cle I) and NuZ = 4.9 (for test article 2). The earlier data on presure drop indicate that given the assumed probability distributions for passage gap nonuniformity, the experimentally measured val- ues of Nul and Nu2...

  10. TREKiSM Issue 41/42 

    E-Print Network [OSTI]

    1985-01-01

    \\4220 CONVENTION LOG COORDINATOR: Teri Hecken~ueller, 547 Cle •• er Ave, Cincinnati OH 45219 TREKisM back issues ($]@): Louise Langberg. 2021 Sheridan, St. Paul HN 55116 ~:\\·r '] rl ~ II Press Release: Paramount Pictures Corporation P... (George Tekel) and Communications Officer Uhure (Nlchelle Nichols). Further I n9 the popu I ar I ty fo the c I ass i c "Star Trek'~ television serles, ParGmount's past three "Star Trek" fil~St: have earned 8 combined total of more than $250 mJ 1 l...

  11. Marketing Practices and Costs of Texas Egg Producer-Wholesalers. 

    E-Print Network [OSTI]

    Shafer, Carl E.

    1964-01-01

    -wholesalers. It was not cafes and but they not be to a random sample of the producer-who~esaler compete for the large retailer outlets. The small population, of Texas. producers generally have higher costs per cue and insufficient volume to adequately service Labor... efficiency. Size Number Tt: Whole- On group SalerS consumer stores At cafes other1 Labor Efficiency and Costs routes farm Differences in costs per case for egg cle- - - - - - Number - - - - livery were mainly associated with variatiolli 1 A 1s 4 9 3...

  12. Los

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL AMOS

  13. Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL AMOS1

  14. Los Alamos ChamberFest

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL

  15. Los Alamos County is among 100 Best Communities for Young People

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL100

  16. Los Alamos Dynamics Application

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL100Los

  17. Los Alamos Dynamics Summer School-Past Programs

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL100Los

  18. Los Alamos Dynamics Summer School-Past Programs

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS AL100Los

  19. Los Alamos Employees' Scholarship

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOS

  20. Los Alamos Employees' Scholarship

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOSfive New

  1. Los Alamos Employees' Scholarship Fund raises record amount

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle LOSfive

  2. Los Alamos Field Office Emergency Public Information | National Nuclear

    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: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverseIMPACTThousand CubicResourcelogo and-E CChinaC LLos t!darnos cle

  3. Inclusive ?(2P) production in ?(3S) decay

    E-Print Network [OSTI]

    Baringer, Philip S.

    1991-09-23

    . Lewis, G. S. Ludwig, J. Masui, J. Mevissen, N. B. Mistry, S. Nandi, C. R. Ng, E. Nordberg, C. O' Grady, " J. R. Patterson, D. Peterson, M. Pisharody, D. Riley, M. Sapper, M. Selen, H. Worden, M. Norris, P. Avery, A. Freyberger, J. Rodriguez, J. Yelton, K....o( 1.17 0.73 1.04 0.90 1.12 0.86 1.08 0.80 1.14 0.85 tion, and b as the tensor contribution, the masses are given by [9] M(gq) =M+a ——', b, M(gl) =M —a+2b, and M(go) =M —2a 4b—He. re a and b are computed as the configuration-space expectation values: &v...

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

    SciTech Connect (OSTI)

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

    1996-11-01

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

  5. Guide for Citrus Production in the Lower Rio Grande Valley. 

    E-Print Network [OSTI]

    Maxwell, Norman P. (Norman Paul); Bailey, Morris A.

    1963-01-01

    Norman Maxwell, Ralph Petersen, Robert Orton and Donald Haddock* The earliest record of citrus planted in the Valley is a planting of seedling orange trees, made by Don JIaceclona Vela in the early 1880's, on the Laguna 5eca Ranch, north of Edinburg..., Morris Bailey, Norman Maxwell, V. C. Cooper and Bruce Lime" GRAPF,%R UIT VA R6ETI.S The Valley's reputation as a citrus area is based primarily upon the high interior quality of its grape- fruit. Valley grapefruit is sweeter than that raised...

  6. News: El grupo de Teatro Esquina Latina cumple quince años

    E-Print Network [OSTI]

    1988-10-01

    FAIJL 108ft 37 El grupo de Teatro Esquina Latina cumple quince años "A vosotros los audaces buscadores e indagadores y a quien quiera que alguna vez se haya lanzado con astutas velas a mares terribles subid a nuestra nave de sueños, venid a... se va visualizando a través de metas y objetivos en un principio planteados, tratando de expresar el contexto que destruye y constituye nuestro mundo. Nos interesa la expresión abierta y amplia de las imágenes de la vida que develan el concepto...

  7. Fifty-one years of Los Alamos Spacecraft

    SciTech Connect (OSTI)

    Fenimore, Edward E.

    2014-09-04

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

  8. The Parkes multibeam pulsar survey III. Young pulsars & the discovery and timing of 200 pulsars

    E-Print Network [OSTI]

    Krämer, M; Manchester, R N; Lyne, A G; Camilo, F; Stairs, I H; D'Amico, N; Kaspi, V M; Hobbs, G; Morris, D J; Crawford, F; Possenti, A; Joshi, B C; McLaughlin, M A; Lorimer, D R; Faulkner, A J

    2003-01-01

    The Parkes multibeam pulsar survey has unlocked vast areas of the Galactic plane which were previously invisible to earlier low-frequency and less-sensitive surveys. The survey has discovered more than 600 new pulsars so far, including many that are young and exotic. In this paper we report the discovery of 200 pulsars for which we present positional and spin-down parameters, dispersion measures, flux densities and pulse profiles. A large number of these new pulsars are young and energetic, and we review possible associations of $\\gamma$-ray sources with the sample of about 1300 pulsars for which timing solutions are known. Based on a statistical analysis, we estimate that about $19\\pm6$ associations are genuine. The survey has also discovered 12 pulsars with spin properties similar to those of the Vela pulsar, nearly doubling the known population of such neutron stars. Studying the properties of all known `Vela-like' pulsars, we find their radio luminosities to be similar to normal pulsars, implying that the...

  9. COMPTEL limits on 26Al 1.809 MeV line emission from gamma^2 Velorum

    E-Print Network [OSTI]

    U. Oberlack; U. Wessolowski; R. Diehl; K. Bennett; H. Bloemen; W. Hermsen; J. Knödlseder; D. Morris; V. Schönfelder; P. von Ballmoos

    1999-10-29

    The Wolf-Rayet binary system gamma^2 Vel (WR 11} is the closest known Wolf-Rayet (WR) star. Recently, its distance has been redetermined by parallax measurements with the HIPPARCOS astrometric satellite yielding 258^{+41}_{-31} pc, significantly lower than previous estimates (300 -- 450 pc). Wolf-Rayet stars have been proposed as a major source of the Galactic 26Al observed at 1.809 MeV. The gamma-ray telescope COMPTEL has previously reported 1.8 MeV emission from the Vela region, yet located closer to the Galactic plane than the position of gamma^2 Vel. We derive an upper 1.8 MeV flux limit of 1.1 10^{-5} ph cm^{-2} s^{-1} (2 \\sigma) for the WR star. With the new distance estimate, COMPTEL measurements place a limit of (6.3^{+2.1}_{-1.4}) 10^{-5} M_\\odot the 26Al yield of gamma^2 Vel, thus constrains theories of nucleosynthesis in Wolf-Rayet stars. We discuss the implications in the context of the binary nature of gamma^2 Vel and present a new interpretation of the IRAS Vela shell.

  10. The ephemeris, orbital decay, and masses of 10 eclipsing HMXBs

    E-Print Network [OSTI]

    Falanga, M; Lutovinov, A; Bonnet-Bidaud, J M; Fetisova, Y; Puls, J

    2015-01-01

    We take advantage of more than 10 years of monitoring of the eclipsing HMXB systems LMC X-4, Cen X-3, 4U 1700-377, 4U 1538-522, SMC X-1, IGR J18027-2016, Vela X-1, IGR J17252-3616, XTE J1855-026, and OAO 1657-415 with the ASM on-board RXTE and ISGRI on-board INTEGRAL to update their ephemeris. These results are used to refine previous measurements of the orbital period decay of all sources (where available) and provide the first accurate values of the apsidal advance in Vela X-1 and 4U 1538-522. Updated values for the masses of the neutron stars hosted in the ten HMXBs are also provided, as well as the long-term lightcurves folded on the sources best determined orbital parameters. These lightcurves reveal complex eclipse ingresses and egresses, that are understood mostly as being due to the presence of accretion wakes. The results reported in this paper constitute a database to be used for population and evolutionary studies of HMXBs, as well as theoretical modelling of long-term accretion in wind-fed X-ray b...

  11. Simulations of Atomic Processes at Semiconductor Surfaces - General-Method and Chemisorption on Gaas(110) 

    E-Print Network [OSTI]

    MENON, M.; Allen, Roland E.

    1988-01-01

    ,??1 EF ?E' 1. Also, one can see in Fig. 1 that cl a i 1Im ln cl ~ ??m' 26 ?EC ! BE", F, =?Im g lnTT; BX Fq ?g FJ, clE ?E.a i E ?E,clC (2.41) (2.42a) as R ?+00, so 1F 2; Bx (2.49} The expression for the electronic force thus simplifies....63,3.45,0) before they are al- lowed to relax. Figure 2 also schematically shows a top view of six possible chemisorption sites on the surface, 0.0. GaAs(110) ?0.5. ?1.0 1.0 0.5 0.0. ?0 5. ?1.0. ?1.5 0 100 200 300 400 500 600 700 800 t GaAs FIG. 2...

  12. The investigation of the electrodeposition of iron from fluoborate solutions 

    E-Print Network [OSTI]

    Mosier, Benjamin

    1952-01-01

    gA ~ useeeah@ Ae %ho ~ et yM@ale~ S8a ~ Leal. ~ hag ~ Qsa ot'4he'"~ 4k', eg ~ ylang~~ ms ysdea%4@R ee 4gNg: ~ Scca Oe ecch et Ng&yke @5) e eeeeelee4a4 ~ )eeeahe ~ ?elba' eymrhe4 a4 eh@4 'lf ~~ ~ ~ e ~Acne cg ahe4 SA 8a weeeaeeN~ Ske ea4ahhN yea4...aa ~a %e eyeaeM ~we XX' M ~ IeiaaLe W %aaeloL IMt ge ~easy yei~y ~ Le, Ne oalxNca awk awLIeee yL4Qaag %o e; e~g~ eehek wither ~mvgag vQh. the leAQj+ ot the 4eaa ~W. QIgeeee Re ee4 XI@ TeQe VXXIi R~eeia XP eCLe~ ykttkwg to ~ ~ east deaewesoe ~ oaa...

  13. Something Lost 

    E-Print Network [OSTI]

    Clark, Sheila

    1983-01-01

    D, giving the closest the spoken 'words 0 ;; If you ":JOuld come this 1tlay, [{entlemen 9 II "'food said.. Kirk \\'IA,tohed thc,m go, slightly disturhed hy the Hay that the last lTI,-"nhe2' of the p'p,:cty to leave carried his tail bet\\Kirk's tempcT. L?t~. Pro}-:'C1sko. came OVer to him. ~;I'm sorrY9 sirs there's notbinrs? to inclicate ':[here tb['.t fJl"l1ell migrlt be coming from. J~ncl we CEi,n I t cle?a1.' it until H0 find tho source...

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

    E-Print Network [OSTI]

    Schmidl, William Daniel

    1992-01-01

    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... '2 Description of the i'omponents IV THE EXPERIiXIE'XTAL PRO('EDI RE 4i IV 1 Introduction IV 3 Seed Selection IV 3 Expentnental Apparatus IV. 4 Experimental Setup IV 6 Taking data . IV 6 Fhpping, Looking, and Appraising the Data IV 7 Enhancing...

  15. BEAM DYNAMICS IN NS-FFAG EMMAWITH DYNAMICAL MAPS

    E-Print Network [OSTI]

    Giboudot, Y; Edgecock, R; Wolski, A

    2010-01-01

    The Non Scal­ing Fixed Field Al­ter­nat­ing Gra­di­ent EMMA has a com­pact lin­ear lat­tice. Ef­fect of Fringe Field on the beam has to be stud­ied care­ful­ly. A nu­mer­i­cal mag­net­ic field map is gen­er­at­ed by mag­net mea­sure­ments or mag­net de­sign soft­wares. We de­vel­oped a tech­nique that pro­duces from the nu­mer­i­cal field map, a dy­nam­i­cal map for a par­ti­cle trav­el­ling in the en­tire EMMA cell for a ref­er­ence en­er­gy with­out ac­cel­er­a­tion. Since the beam dy­nam­ics change with en­er­gy, a set of maps have been pro­duce with dif­fer­ent ref­er­ence en­er­gies be­tween 10 and 20MeV. For each ref­er­ence en­er­gy, sim­u­lat­ed tune and time of flight (TOF) have been com­pared with re­sults in Zgoubi - track­ing di­rect­ly through nu­mer­i­cal field map. The range of va­lid­i­ty of a sin­gle map has been in­ves­ti­gat­ed by track­ing par­ti­cle with large en­er­gy de­vi­a­tion. From that, a ...

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

    E-Print Network [OSTI]

    Dan Hooper; Brenda Dingus

    2002-12-20

    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.

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

    E-Print Network [OSTI]

    Hooper, D; Hooper, Dan; Dingus, Brenda

    2002-01-01

    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.

  18. Neutron Stars : A Comparative Study

    E-Print Network [OSTI]

    Mehedi Kalam; Sk. Monowar Hossein; Sajahan Molla

    2015-10-23

    The inner structure of neutron star is considered from theoretical point of view and is compared with the observed data. We have proposed a form of an equation of state relating pressure with matter density which indicates the stiff equation of state of neutron stars. From our study we have calculated mass(M), compactness(u) and surface red-shift(Zs ) for the neutron stars namely PSR J1614-2230, PSR J1903+327, Cen X-3, SMC X-1, Vela X-1, Her X-1 and compared with the recent observational data. We have also indicated the possible radii of the different stars which needs further study. Finally we have examined the stability for such type of theoretical structure.

  19. Searching for Very High Energy Emission from Pulsars Using the High Altitude Water Cherenkov (HAWC) Observatory

    E-Print Network [OSTI]

    C. Alvarez Ochoa; P. M. Saz Parkinson; A. Belfiore; A. Carramiñana; C. Rivière; E. Moreno Barbosa; for the HAWC collaboration

    2015-08-20

    There are currently over 160 known gamma-ray pulsars. While most of them are detected only from space, at least two are now seen also from the ground. MAGIC and VERITAS have measured the gamma ray pulsed emission of the Crab pulsar up to hundreds of GeV and more recently MAGIC has reported emission at $\\sim2$ TeV. Furthermore, in the Southern Hemisphere, H.E.S.S. has detected the Vela pulsar above 30 GeV. In addition, non-pulsed TeV emission coincident with pulsars has been detected by many groups, including the Milagro Collaboration. These GeV-TeV observations open the possibility of searching for very-high-energy (VHE, > 100GeV) pulsations from gamma-rays pulsars in the HAWC field of view.

  20. Pinning down the superfluid and measuring masses using pulsar glitches

    E-Print Network [OSTI]

    Ho, Wynn C G; Antonopoulou, Danai; Andersson, Nils

    2015-01-01

    Pulsars are known for their superb timing precision, although glitches can interrupt the regular timing behavior when the stars are young. These glitches are thought to be caused by interactions between normal and superfluid matter in the crust of the star. However, glitching pulsars such as Vela have been shown to require a superfluid reservoir that greatly exceeds that available in the crust. We examine a model in which glitches tap the superfluid in the core. We test a variety of theoretical superfluid models against the most recent glitch data and find that only one model can successfully explain up to 45 years of observational data. We develop a new technique for combining radio and X-ray data to measure pulsar masses, thereby demonstrating how current and future telescopes can probe fundamental physics such as superfluidity near nuclear saturation.

  1. Pinning down the superfluid and measuring masses using pulsar glitches

    E-Print Network [OSTI]

    Wynn C. G. Ho; Cristobal M. Espinoza; Danai Antonopoulou; Nils Andersson

    2015-10-01

    Pulsars are known for their superb timing precision, although glitches can interrupt the regular timing behavior when the stars are young. These glitches are thought to be caused by interactions between normal and superfluid matter in the crust of the star. However, glitching pulsars such as Vela have been shown to require a superfluid reservoir that greatly exceeds that available in the crust. We examine a model in which glitches tap the superfluid in the core. We test a variety of theoretical superfluid models against the most recent glitch data and find that only one model can successfully explain up to 45 years of observational data. We develop a new technique for combining radio and X-ray data to measure pulsar masses, thereby demonstrating how current and future telescopes can probe fundamental physics such as superfluidity near nuclear saturation.

  2. Searching for Very High Energy Emission from Pulsars Using the High Altitude Water Cherenkov (HAWC) Observatory

    E-Print Network [OSTI]

    Ochoa, C Alvarez; Belfiore, A; Carramiñana, A; Rivière, C; Barbosa, E Moreno

    2015-01-01

    There are currently over 160 known gamma-ray pulsars. While most of them are detected only from space, at least two are now seen also from the ground. MAGIC and VERITAS have measured the gamma ray pulsed emission of the Crab pulsar up to hundreds of GeV and more recently MAGIC has reported emission at $\\sim2$ TeV. Furthermore, in the Southern Hemisphere, H.E.S.S. has detected the Vela pulsar above 30 GeV. In addition, non-pulsed TeV emission coincident with pulsars has been detected by many groups, including the Milagro Collaboration. These GeV-TeV observations open the possibility of searching for very-high-energy (VHE, > 100GeV) pulsations from gamma-rays pulsars in the HAWC field of view.

  3. Constitutive Model for Material Comminuting at High Shear Rate

    E-Print Network [OSTI]

    Zdenek P. Bazant; Ferhun C. Caner

    2013-06-04

    The modeling of high velocity impact into brittle or quasibrittle solids is hampered by the unavailability of a constitutive model capturing the effects of material comminution into very fine particles. The present objective is to develop such a model, usable in finite element programs. The comminution at very high strain rates can dissipate a large portion of the kinetic energy of an impacting missile. The spatial derivative of the energy dissipated by comminution gives a force resisting the penetration, which is superposed on the nodal forces obtained from the static constitutive model in a finite element program. The present theory is inspired partly by Grady's model for comminution due to explosion inside a hollow sphere, and partly by analogy with turbulence. In high velocity turbulent flow, the energy dissipation rate is enhanced by the formation of micro-vortices (eddies) which dissipate energy by viscous shear stress. Similarly, here it is assumed that the energy dissipation at fast deformation of a confined solid gets enhanced by the release of kinetic energy of the motion associated with a high-rate shear strain of forming particles. For simplicity, the shape of these particles in the plane of maximum shear rate is considered to be regular hexagons. The rate of release of free energy density consisting of the sum of this energy and the fracture energy of the interface between the forming particle is minimized. The particle sizes are assumed to be distributed according to Schuhmann's power law. It is concluded that the minimum particle size is inversely proportional to the (2/3)-power of the shear strain rate, that the kinetic energy release is to proportional to the (2/3)-power, and that the dynamic comminution creates an apparent material viscosity inversely proportional to the (1/3)-power of the shear strain rate.

  4. Evaluating operating system vulnerability to memory errors.

    SciTech Connect (OSTI)

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

    2012-05-01

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

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

    E-Print Network [OSTI]

    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. Brückner; T. Bulik; H. J. Bulten; A. Buonanno; D. Buskulic; C. Buy; R. L. Byer; L. Cadonati; G. Cagnoli; J. Calderón 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. Cavaglià; 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. Deléglise; 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. Díaz; 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. González; N. Gordon; M. L. Gorodetsky; S. Gossan; S. Goßler; 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. Jiménez-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

    2014-04-24

    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.

  6. Gravitational-waves from known pulsars: results from the initial detector era

    E-Print Network [OSTI]

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

    2013-01-01

    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 G...

  7. Gravitational waves from known pulsars: Results from the initial detector era

    SciTech Connect (OSTI)

    Aasi, J.; Abadie, J.; Abbott, B. P.; Abbott, R.; Abernathy, M. R.; Adhikari, R. X.; Ajith, P. [LIGO - California Institute of Technology, Pasadena, CA 91125 (United States); Abbott, T. [Louisiana State University, Baton Rouge, LA 70803 (United States); Accadia, T. [Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux (France); Acernese, F. [INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli (Italy); Adams, C. [LIGO - Livingston Observatory, Livingston, LA 70754 (United States); Adams, T. [Cardiff University, Cardiff, CF24 3AA (United Kingdom); Affeldt, C.; Allen, B. [Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover (Germany); Agathos, M. [Nikhef, Science Park, 1098 XG Amsterdam (Netherlands); Aggarwal, N. [LIGO - Massachusetts Institute of Technology, Cambridge, MA 02139 (United States); Aguiar, O. D. [Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, SP (Brazil); Allocca, A. [INFN, Sezione di Pisa, I-56127 Pisa (Italy); Ceron, E. Amador [University of Wisconsin-Milwaukee, Milwaukee, WI 53201 (United States); Amariutei, D. [University of Florida, Gainesville, FL 32611 (United States); Collaboration: LIGO Scientific Collaboration and The Virgo Collaboration; and others

    2014-04-20

    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.

  8. Core-crust transition and crustal fraction of moment of inertia in neutron stars

    E-Print Network [OSTI]

    Debasis Atta; Somnath Mukhopadhyay; D. N. Basu

    2015-09-29

    The crustal fraction of moment of inertia in neutron stars is calculated using $\\beta$-equilibrated nuclear matter obtained from density dependent M3Y effective interaction. The transition density, pressure and proton fraction at the inner edge separating the liquid core from the solid crust of the neutron stars determined from the thermodynamic stability conditions are found to be $\\rho_t=$ 0.0938 fm$^{-3}$, P$_t=$ 0.5006 MeV fm$^{-3}$ and $x_{p(t)}=$ 0.0308, respectively. The crustal fraction of the moment of inertia can be extracted from studying pulsar glitches and is most sensitive to the pressure as well as density at the transition from the crust to the core. These results for pressure and density at core-crust transition together with the observed minimum crustal fraction of the total moment of inertia provide a new limit for the radius of the Vela pulsar: $R \\geq 4.10 + 3.36 M/M_\\odot$ kms.

  9. INTEGRAL observations of TeV plerions

    E-Print Network [OSTI]

    A. I. D. Hoffmann; D. Horns; A. Santangelo

    2006-09-14

    Amongst the sources seen in very high gamma-rays several are associated with Pulsar Wind Nebulae (``TeV plerions''). The study of hard X-ray/soft gamma-ray emission is providing an important insight into the energetic particle population present in these objects. The unpulsed emission from pulsar/pulsar wind nebula systems in the energy range accessible to the INTEGRAL satellite is mainly synchrotron emission from energetic and fast cooling electrons close to their acceleration site. Our analyses of public INTEGRAL data of known TeV plerions detected by ground based Cherenkov telescopes indicate a deeper link between these TeV plerions and INTEGRAL detected pulsar wind nebulae. The newly discovered TeV plerion in the northern wing of the Kookaburra region (G313.3+0.6 powered by the middle aged PSR J1420-6048) is found to have a previously unknown INTEGRAL counterpart which is besides the Vela pulsar the only middle aged pulsar detected with INTEGRAL. We do not find an INTEGRAL counterpart of the TeV plerion associated with the X-ray PWN ``Rabbit'' G313.3+0.1 which is possibly powered by a young pulsar.

  10. GAMMA-400 gamma-ray observatory

    E-Print Network [OSTI]

    Topchiev, N P; Bonvicini, V; Adriani, O; Aptekar, R L; Arkhangelskaja, I V; Arkhangelskiy, A I; Bakaldin, A V; Bergstrom, L; Berti, E; Bigongiari, G; Bobkov, S G; Boezio, M; Bogomolov, E A; Bonechi, L; Bongi, M; Bottai, S; Castellini, G; Cattaneo, P W; Cumani, P; Dalkarov, O D; Dedenko, G L; De Donato, C; Dogiel, V A; Finetti, N; Gascon, D; Gorbunov, M S; Gusakov, Yu V; Hnatyk, B I; Kadilin, V V; Kaplin, V A; Kaplun, A A; Kheymits, M D; Korepanov, V E; Larsson, J; Leonov, A A; Loginov, V A; Longo, F; Maestro, P; Marrocchesi, P S; Martinez, M; Menshenin, A L; Mikhailov, V V; Mocchiutti, E; Moiseev, A A; Mori, N; Moskalenko, I V; Naumov, P Yu; Papini, P; Paredes, J M; Pearce, M; Picozza, P; Rappoldi, A; Ricciarini, S; Runtso, M F; Ryde, F; Serdin, O V; Sparvoli, R; Spillantini, P; Stozhkov, Yu I; Suchkov, S I; Taraskin, A A; Tavani, M; Tiberio, A; Tyurin, E M; Ulanov, M V; Vacchi, A; Vannuccini, E; Vasilyev, G I; Ward, J E; Yurkin, Yu T; Zampa, N; Zirakashvili, V N; Zverev, V G

    2015-01-01

    The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Galactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well as diffuse gamma-ray emission, along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will study gamma-ray bursts and gamma-ray emission from the Sun during periods of solar activity. The energy range of GAMMA-400 is expected to be from ~20 MeV up to TeV energies for gamma rays, up to 20 TeV for electrons + positrons, and up to 10E15 eV for cosmic-ray nuclei. For high-energy gamma rays with energy from 10 to 100 GeV, the GAMMA-400 angular resolution improves from 0.1{\\deg} to ~0.01{\\deg} and energy resolution from 3% to ~1%; the proton rejection factor is ~5x10E5. GAMMA-400 will be installed onboard the Russian space observatory.

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

    SciTech Connect (OSTI)

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

    2014-06-10

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

  12. Evidence for Environmental Changes in the Submillimeter Dust Opacity

    E-Print Network [OSTI]

    Martin, Peter G; Bontemps, Sylvain; Miville-Deschênes, Marc-Antoine; Ade, Peter A R; Bock, James J; Chapin, Edward L; Devlin, Mark J; Dicker, Simon R; Griffin, Matthew; Gundersen, Joshua O; Halpern, Mark; Hargrave, Peter C; Hughes, David H; Klein, Jeff; Marsden, Gaelen; Mauskopf, Philip; Netterfield, Calvin B; Olmi, Luca; Patanchon, Guillaume; Rex, Marie; Scott, Douglas; Semisch, Christopher; Truch, Matthew D P; Tucker, Carole; Tucker, Gregory S; Viero, Marco P; Wiebe, Donald V

    2011-01-01

    The submillimeter opacity of dust in the diffuse Galactic interstellar medium (ISM) has been quantified using a pixel-by-pixel correlation of images of continuum emission with a proxy for column density. We used three BLAST bands at 250, 350, and 500 \\mu m and one IRAS at 100 \\mu m. The proxy is the near-infrared color excess, E(J-Ks), obtained from 2MASS. Based on observations of stars, we show how well this color excess is correlated with the total hydrogen column density for regions of moderate extinction. The ratio of emission to column density, the emissivity, is then known from the correlations, as a function of frequency. The spectral distribution of this emissivity can be fit by a modified blackbody, whence the characteristic dust temperature T and the desired opacity \\sigma_e(1200) at 1200 GHz can be obtained. We have analyzed 14 regions near the Galactic plane toward the Vela molecular cloud, mostly selected to avoid regions of high column density (N_H > 10^{22} cm^-2) and small enough to ensure a u...

  13. Chandra Observations of the Northeastern Rim of the Cygnus Loop

    E-Print Network [OSTI]

    Katsuda, Satoru; Kimura, Masashi; Mori, Koji

    2008-01-01

    We present results from spatially resolved spectral analyses of the northeastern (NE) rim of the Cygnus Loop supernova remnant (SNR) based on two Chandra observations. One pointing includes northern outermost abundance-enhanced regions discovered by recent Suzaku observations, while the other pointing is located on regions with "normal" abundances in the NE rim of the Cygnus Loop. The superior spatial resolving power of Chandra allows us to reveal that the abundance-enhanced region is concentrated in an about 200"-thickness region behind the shock front. We confirm absolute metal abundances (i.e., relative to H) as well as abundance ratios between metals are consistent with those of the solar values within a factor of about 2. Also, we find that the emission measure in the region gradually decreases toward the shock front. These features are in contrast with those of the ejecta fragments around the Vela SNR, which leads us to believe that the abundance enhancements are not likely due to metal-rich ejecta. We ...

  14. Chandra Observations of the Northeastern Rim of the Cygnus Loop

    E-Print Network [OSTI]

    Satoru Katsuda; Hiroshi Tsunemi; Masashi Kimura; Koji Mori

    2008-06-25

    We present results from spatially resolved spectral analyses of the northeastern (NE) rim of the Cygnus Loop supernova remnant (SNR) based on two Chandra observations. One pointing includes northern outermost abundance-enhanced regions discovered by recent Suzaku observations, while the other pointing is located on regions with "normal" abundances in the NE rim of the Cygnus Loop. The superior spatial resolving power of Chandra allows us to reveal that the abundance-enhanced region is concentrated in an about 200"-thickness region behind the shock front. We confirm absolute metal abundances (i.e., relative to H) as well as abundance ratios between metals are consistent with those of the solar values within a factor of about 2. Also, we find that the emission measure in the region gradually decreases toward the shock front. These features are in contrast with those of the ejecta fragments around the Vela SNR, which leads us to believe that the abundance enhancements are not likely due to metal-rich ejecta. We suggest that the origin of the plasma in this region is the interstellar medium (ISM). In the "normal" abundance regions, we confirm that abundances are depleted to the solar values by a factor of about 5 that is not expected in the ISM around the Cygnus Loop. Introduction of non-thermal emission in our model fitting can not naturally resolve the abundance-depletion problem. The origin of the depletion still remains as an open question.

  15. The soft gamma-ray pulsar population: an high-energy overview

    E-Print Network [OSTI]

    Kuiper, L

    2015-01-01

    At high-energy gamma-rays (>100 MeV) the Large Area Telescope (LAT) on the Fermi satellite already detected more than 145 rotation-powered pulsars (RPPs), while the number of pulsars seen at soft gamma-rays (20 keV - 30 MeV) remained small. We present a catalogue of 18 non-recycled RPPs from which presently non-thermal pulsed emission has been securely detected at soft gamma-rays above 20 keV, and characterize their pulse profiles and energy spectra. For 14 of them we report new results, (re)analysing mainly data from RXTE, INTEGRAL, XMM-Newton and Chandra. The soft gamma-pulsars are all fast rotators and on average ~9.3x younger and ~ 43x more energetic than the Fermi LAT sample. The majority (11 members) exhibits broad, structured single pulse profiles, and only 6 have double (or even multiple, Vela) pulses. Fifteen soft gamma-ray pulsar show hard power-law spectra in the hard X-ray band and reach maximum luminosities typically in the MeV range. For only 7 of the 18 soft gamma-ray pulsars pulsed emission ha...

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

    SciTech Connect (OSTI)

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

    2014-06-01

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

  17. Constraints on the symmetry energy from observational probes of the neutron star crust

    E-Print Network [OSTI]

    William G. Newton; Joshua Hooker; Michael Gearheart; Kyleah Murphy; De-Hua Wen; Farrukh Fattoyev; Bao-An Li

    2015-06-07

    A number of observed phenomena associated with individual neutron star systems or neutron star populations find explanations in models in which the neutron star crust plays an important role. We review recent work examining the sensitivity to the slope of the symmetry energy $L$ of such models, and constraints extracted on $L$ from confronting them with observations. We focus on six sets of observations and proposed explanations: (i) The cooling rate of the neutron star in Cassiopeia A, confronting cooling models which include enhanced cooling in the nuclear pasta regions of the inner crust, (ii) the upper limit of the observed periods of young X-ray pulsars, confronting models of magnetic field decay in the crust caused by the high resistivity of the nuclear pasta layer, (iii) glitches from the Vela pulsar, confronting the paradigm that they arise due to a sudden re-coupling of the crustal neutron superfluid to the crustal lattice after a period during which they were decoupled due to vortex pinning, (iv) The frequencies of quasi-periodic oscillations in the X-ray tail of light curves from giant flares from soft gamma-ray repeaters, confronting models of torsional crust oscillations, (v) the upper limit on the frequency to which millisecond pulsars can be spun-up due to accretion from a binary companion, confronting models of the r-mode instability arising above a threshold frequency determined in part by the viscous dissipation timescale at the crust-core boundary, and (vi) the observations of precursor electromagnetic flares a few seconds before short gamma-ray bursts, confronting a model of crust shattering caused by resonant excitation of a crustal oscillation mode by the tidal gravitational field of a companion neutron star just before merger.

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

    E-Print Network [OSTI]

    B. B. Jones

    2002-02-04

    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.

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

    SciTech Connect (OSTI)

    Firestone, R. B., E-mail: rbfirestone@lbl.gov [Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States)

    2014-07-01

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

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

    E-Print Network [OSTI]

    Myron A. Smith

    2001-07-10

    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.

  1. Observations of Accreting Pulsars

    E-Print Network [OSTI]

    Lars Bildsten; Deepto Chakrabarty; John Chiu; Mark H. Finger; Danny T. Koh; Robert W. Nelson; Thomas A. Prince; Bradley C. Rubin; D. Matthew Scott; Mark Stollberg; Brian A. Vaughan; Colleen A. Wilson; Robert B. Wilson

    1997-07-22

    We summarize five years of continuous monitoring of accretion-powered pulsars with the Burst and Transient Source Experiment (BATSE) on the Compton Gamma Ray Observatory. Our 20-70 keV observations have determined or refined the orbital parameters of 13 binaries, discovered 5 new transient accreting pulsars, measured the pulsed flux history during outbursts of 12 transients (GRO J1744-28, 4U 0115+634, GRO J1750-27, GS 0834-430, 2S 1417-624, GRO J1948+32, EXO 2030+375, GRO J1008-57, A 0535+26, GRO J2058+42, 4U 1145-619 and A 1118-616), and also measured the accretion torque history of during outbursts of 6 of those transients whose orbital parameters were also known. We have also continuously measured the pulsed flux and spin frequency for eight persistently accreting pulsars (Her X-1, Cen X-3, Vela X-1, OAO 1657-415, GX 301-2, 4U 1626-67, 4U 1538-52, and GX 1+4). Because of their continuity and uniformity over a long baseline, BATSE observations have provided new insights into the long-term behavior of accreting magnetic stars. We have found that all accreting pulsars show stochastic variations in their spin frequencies and luminosities, including those displaying secular spin-up or spin-down on long time scales, blurring the conventional distinction between disk-fed and wind-fed binaries. Pulsed flux and accretion torque are strongly correlated in outbursts of transient accreting pulsars, but uncorrelated, or even anticorrelated, in persistent sources.

  2. Point X-ray sources in the SNR G 315.4-2.30 (MSH 14-63, RCW 86)

    E-Print Network [OSTI]

    V. V. Gvaramadze; A. A. Vikhlinin

    2002-12-25

    We report the results of a search for a point X-ray source (stellar remnant) in the southwest protrusion of the supernova remnant G 315.4-2.30 (MSH 14-63, RCW 86) using the archival data of the Chandra X-ray Observatory. The search was motivated by a hypothesis that G 315.4-2.30 is the result of an off-centered cavity supernova explosion of a moving massive star, which ended its evolution just near the edge of the main-sequence wind-driven bubble. This hypothesis implies that the southwest protrusion in G 315.4-2.30 is the remainder of a pre-existing bow shock-like structure created by the interaction of the supernova progenitor's wind with the interstellar medium and that the actual location of the supernova blast center is near the center of this hemispherical structure. We have discovered two point X-ray sources in the "proper" place. One of the sources has an optical counterpart with the photographic magnitude $13.38\\pm0.40$, while the spectrum of the source can be fitted with an optically thin plasma model. We interpret this source as a foreground active star of late spectral type. The second source has no optical counterpart to a limiting magnitude $\\sim 21$. The spectrum of this source can be fitted almost equally well with several simple models (power law: photon index $=1.87$; two-temperature blackbody: $kT_1 =0.11$ keV, $R_1 =2.34 $ km and $kT_2 =0.71$ keV, $R_2 =0.06$ km; blackbody plus power law: $kT =0.07$ keV, photon index $=2.3$). We interpret this source as a candidate stellar remnant (neutron star), while the photon index and non-thermal luminosity of the source (almost the same as those of the Vela pulsar and the recently discovered pulsar PSR J 0205+6449 in the supernova remnant 3C 58) suggest that it can be a young "ordinary" pulsar.

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

    SciTech Connect (OSTI)

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

    2013-09-01

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