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


1

Accretion-ejection connection in the young brown dwarf candidate ISO-Cha1 217  

E-Print Network [OSTI]

As the number of observed brown dwarf outflows is growing it is important to investigate how these outflows compare to the well studied jets from young stellar objects. A key point of comparison is the relationship between outflow and accretion activity and in particular the ratio between the mass outflow and accretion rates ($\\dot{M}_{out}$/$\\dot{M}_{acc}$). The brown dwarf candidate ISO-ChaI 217 was discovered by our group, as part of a spectro-astrometric study of brown dwarfs, to be driving an asymmetric outflow with the blue-shifted lobe having a position angle of $\\sim$ 20$^{\\circ}$. The aim here is to further investigate the properties of ISO-ChaI 217, the morphology and kinematics of its outflow, and to better constrain ($\\dot{M}_{out}$/$\\dot{M}_{acc}$). The outflow is spatially resolved in the $[SII]\\lambda \\lambda 6716,6731$ lines and is detected out to $\\sim$ 1\\farcs6 in the blue-shifted lobe and ~ 1" in the red-shifted lobe. The asymmetry between the two lobes is confirmed although the velocity as...

Whelan, E T; Bacciotti, F; Nisini, B; Bonito, R; Antoniucci, S; Stelzer, B; Biazzo, K; D'Elia, V; Ray, T P

2014-01-01T23:59:59.000Z

2

Spectroscopy of New Substellar Candidates in the Pleiades: Towards a Spectral Sequence for Young Brown Dwarfs  

E-Print Network [OSTI]

We present optical and near-IR spectroscopy (600--1000 nm) of 8 faint (I$>$18) very red (R--I$>$2.2) objects discovered in a deep CCD survey of the Pleiades (Zapatero-Osorio et al. 1996). We compare them with reliable cluster members like PPl 15 and Teide 1, and with several field very late-type dwarfs (M4--M9.5), which were observed with similar instrumental configurations. Using pseudocontinuum ratios we classify the new substellar candidates in a spectal sequence defined with reference to field stars of known spectral types. We also reclassify PPl 15 and Teide 1 in a self-consistent way. The likelihood of membership for the new candidates is assesed via the study of their photospheric features, Ha emission, radial velocity, and consistency of their spectral types and I magnitudes with known cluster members. Four of the new substellar candidates are as late or later than PPl~15 (M6.5), but only one, Calar 3 (M8), clearly meets all our membership criteria. It is indeed an object very similar to the brown dwarf Teide 1. Calar 3, together with Teide 1, allows one to compare the spectroscopic characteristics of Pleiades brown dwarfs with those of old very cool dwarfs. The overall spectral properties are similar, but there are slight differences in the NaI doublet (818.3 nm, 819.5 nm), VO molecular band (740 nm), and some spectral ratios, which are probably related to lower surface gravity in the young Pleiades brown dwarfs than in field stars. Finally, we propose a way of improving future CCD-based brown dwarf surveys by using narrow-band near-IR pseudocontinuum filters.

E. L. Martin; R. Rebolo; M. R. Zapatero Osorio

1996-04-15T23:59:59.000Z

3

SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). V. NEW BROWN DWARFS IN {rho} OPHIUCHI  

SciTech Connect (OSTI)

SONYC-Substellar Objects in Nearby Young Clusters-is a survey program to investigate the frequency and properties of substellar objects with masses down to a few times that of Jupiter in nearby star-forming regions. For the {approx}1 Myr old {rho} Ophiuchi cluster, in our earlier paper we reported deep, wide-field optical and near-infrared imaging using Subaru, combined with Two Micron All Sky Survey and Spitzer photometry, as well as follow-up spectroscopy confirming three likely cluster members, including a new brown dwarf with a mass close to the deuterium-burning limit. Here we present the results of extensive new spectroscopy targeting a total of {approx}100 candidates in {rho} Oph, with Fiber Multi Object Spectrograph at the Subaru Telescope and SINFONI at the ESO's Very Large Telescope. We identify 19 objects with effective temperatures at or below 3200 K, eight of which are newly identified very low mass probable members of {rho} Oph. Among these eight, six objects have T{sub eff} {<=} 3000 K, confirming their likely substellar nature. These six new brown dwarfs comprise one-fifth of the known substellar population in {rho} Oph. We estimate that the number of missing substellar objects in our survey area is {approx}15, down to 0.003-0.03 M{sub Sun} and for A{sub V} = 0-15. The upper limit on the low-mass star to brown dwarf ratio in {rho} Oph is 5.1 {+-} 1.4, while the disk fractions are {approx}40% and {approx}60% for stars and brown dwarfs, respectively. Both results are in line with those for other nearby star-forming regions.

Muzic, Koraljka; Jayawardhana, Ray [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Scholz, Alexander [School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2 (Ireland); Geers, Vincent [Institut fuer Astronomie, ETH, Wolfgang-Pauli-Strasse 27, 8093 Zuerich (Switzerland); Tamura, Motohide, E-mail: muzic@astro.utoronto.ca [National Astronomical Observatory, Osawa 2-21-2, Mitaka, Tokyo 181 (Japan)

2012-01-10T23:59:59.000Z

4

Published Work Brown, M. J., Tandy, R. D., Wulf, G., & Young, J. C. (2013). The effect of acute exercise on  

E-Print Network [OSTI]

Dec. 2013 Published Work Brown, M. J., Tandy, R. D., Wulf, G., & Young, J. C. (2013). The effect. A., Vieira, D. C., . . . Navalta, J. W., Campbell, C. S., Cavaglieri, C. R., & Prestes, J. (2013 patients. Gait and Posture, 39, 308-313. Funghetto, S. S., Prestes, J., Silva, A. D. O., Farias, D. L

Hemmers, Oliver

5

Frazier Courts, Dallas  

E-Print Network [OSTI]

to green building First homes utilized geo-thermal air systems & energy efficient SIP (Structural Insulated Panel) construction Dallas Habitat began building all homes Energy Star Certified in 2004 2008 -DSSI; effort to link green building... are hired who are also energy conscious & utilize green building methods Ex: HVAC installer tapes duct work so does not get contaminated during construction Dallas Habitat relies heavily on the cooperation & collaboration of paid vendors...

Hall, B.

2011-01-01T23:59:59.000Z

6

Ozone induces glucose intolerance and systemic metabolic effects in young and aged brown Norway rats  

SciTech Connect (OSTI)

Air pollutants have been associated with increased diabetes in humans. We hypothesized that ozone would impair glucose homeostasis by altering insulin signaling and/or endoplasmic reticular (ER) stress in young and aged rats. One, 4, 12, and 24 month old Brown Norway (BN) rats were exposed to air or ozone, 0.25 or 1.0 ppm, 6 h/day for 2 days (acute) or 2 d/week for 13 weeks (subchronic). Additionally, 4 month old rats were exposed to air or 1.0 ppm ozone, 6 h/day for 1 or 2 days (time-course). Glucose tolerance tests (GTT) were performed immediately after exposure. Serum and tissue biomarkers were analyzed 18 h after final ozone for acute and subchronic studies, and immediately after each day of exposure in the time-course study. Age-related glucose intolerance and increases in metabolic biomarkers were apparent at baseline. Acute ozone caused hyperglycemia and glucose intolerance in rats of all ages. Ozone-induced glucose intolerance was reduced in rats exposed for 13 weeks. Acute, but not subchronic ozone increased ?{sub 2}-macroglobulin, adiponectin and osteopontin. Time-course analysis indicated glucose intolerance at days 1 and 2 (2 > 1), and a recovery 18 h post ozone. Leptin increased day 1 and epinephrine at all times after ozone. Ozone tended to decrease phosphorylated insulin receptor substrate-1 in liver and adipose tissues. ER stress appeared to be the consequence of ozone induced acute metabolic impairment since transcriptional markers of ER stress increased only after 2 days of ozone. In conclusion, acute ozone exposure induces marked systemic metabolic impairments in BN rats of all ages, likely through sympathetic stimulation. - Highlights: • Air pollutants have been associated with increased diabetes in humans. • Acute ozone exposure produces profound metabolic alterations in rats. • Age influences metabolic risk factors in aging BN rats. • Acute metabolic effects are reversible and repeated exposure reduces these effects. • Ozone metabolic effects are only slightly exacerbated in geriatric rats.

Bass, V. [Environmental Public Health Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Gordon, C.J.; Jarema, K.A.; MacPhail, R.C. [Toxicity Assessment Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Cascio, W.E. [Environmental Public Health Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Phillips, P.M. [Toxicity Assessment Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Ledbetter, A.D.; Schladweiler, M.C. [Environmental Public Health Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Andrews, D. [Research Cores Unit, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Miller, D. [Curriculum in Toxicology, University of North Carolina, Chapel Hill, NC (United States); Doerfler, D.L. [Research Cores Unit, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States); Kodavanti, U.P., E-mail: kodavanti.urmila@epa.gov [Environmental Public Health Division, National Health and Environmental Effects Research Laboratory, U.S. Environmental Protection Agency, Research Triangle Park, NC (United States)

2013-12-15T23:59:59.000Z

7

2MASS J035523.37+113343.7: A YOUNG, DUSTY, NEARBY, ISOLATED BROWN DWARF RESEMBLING A GIANT EXOPLANET  

SciTech Connect (OSTI)

We present parallax and proper motion measurements, near-infrared spectra, and Wide-field Infrared Survey Explorer photometry for the low surface gravity L5{gamma} dwarf 2MASS J035523.37+113343.7 (2M0355). We use these data to evaluate photometric, spectral, and kinematic signatures of youth as 2M0355 is the reddest isolated L dwarf yet classified. We confirm its low-gravity spectral morphology and find a strong resemblance to the sharp triangular shaped H-band spectrum of the {approx}10 Myr planetary-mass object 2M1207b. We find that 2M0355 is underluminous compared to a normal field L5 dwarf in the optical and Mauna Kea Observatory J, H, and K bands and transitions to being overluminous from 3 to 12 {mu}m, indicating that enhanced photospheric dust shifts flux to longer wavelengths for young, low-gravity objects, creating a red spectral energy distribution. Investigating the near-infrared color-magnitude diagram for brown dwarfs confirms that 2M0355 is redder and underluminous compared to the known brown dwarf population, similar to the peculiarities of directly imaged exoplanets 2M1207b and HR8799bcd. We calculate UVW space velocities and find that the motion of 2M0355 is consistent with young disk objects (<2-3 Gyr) and it shows a high likelihood of membership in the AB Doradus association.

Faherty, Jacqueline K. [Department of Astronomy, Universidad de Chile Cerro Calan, Las Condes (Chile); Rice, Emily L.; Cruz, Kelle L.; Nunez, Alejandro [Department of Astrophysics , American Museum of Natural History, Central Park West at 79th Street, New York, NY 10034 (United States); Mamajek, Eric E., E-mail: jfaherty17@gmail.com, E-mail: jfaherty@amnh.org [Cerro Tololo Inter-American Observatory, Casilla 603, La Serena (Chile)

2013-01-01T23:59:59.000Z

8

A Population of very young Brown Dwarfs and free-floating Planets in Orion  

E-Print Network [OSTI]

We describe the results of a very deep imaging survey of the Trapezium Cluster in the IJH bands, using the UKIRT high resolution camera UFTI. Approximately 32% of the 515 point sources detected are brown dwarf candidates, including several free floating objects with masses below the Deuterium burning (planetary) threshold at 0.013 solar masses, which are detectable because of their extreme youth. We have confidence that almost all the sources detected are cluster members, since foreground contamination is minimal in the 33 arcmin^2 area surveyed and the dense backdrop of OMC-1 obscures all background stars at these wavelengths. Extinction is calculated from the (J-H)colours, permitting accurate luminosity estimates and temperatures are derived from the dereddened (I-J) colours. There is some evidence for a cut-off in the luminosity function below the level corresponding to several Jupiter masses, which may represent the bottom end of the IMF. Since star formation is complete in the Trapezium this limit could have wide significance, if confirmed. However, it could well be an effect of the dispersal of the molecular cloud by the central O-type stars, a process whose timescale will vary between star formation regions.

P. W. Lucas; P. F. Roche

2000-03-07T23:59:59.000Z

9

Investigation of Trinity River paleochannels in the central business district, Dallas, Texas  

E-Print Network [OSTI]

) Allan Brown Brillinger, Jr. , B. S. Cleveland State University Chairman of Advisory Committee: Dr. Christopher C . Mathewson Downtown Dallas is built on ancient fluvial deposits of the Trinity River. Excavations in the area have encountered... significant flows of gasoline and ground-water from the fluvial sands. Organization and analysis of over 1, 000 geotechnical logs from the central business district allowed interpretation of the fluvial deposits to determine the sources of hazardous fluids...

Brillinger, Allan Brown

1985-01-01T23:59:59.000Z

10

City of Dallas- Green Energy Purchasing  

Broader source: Energy.gov [DOE]

In September 2007, the City of Dallas finalized purchase contracts for more than 333 million kilowatt-hours (kWh) of green electricity for city facilities during 2008. The city has elected to...

11

Prairie Creek Branch Public Library, Dallas  

E-Print Network [OSTI]

? intelligent landscaping ? efficient MEP systems ? 53 well geothermal / heat pump system ? greywater recapture and reuse ? 7.7 kw photovoltaic array key sustainability overview - energy and water ? compliance with City of Dallas iSWM program ? raised...

Meckfessel, R.

2011-01-01T23:59:59.000Z

12

City of Dallas- Green Buildling Ordinance (Texas)  

Broader source: Energy.gov [DOE]

In April 2008, Dallas passed a Green Building Ordinance, which requires all new buildings to meet higher efficiency standards than current building energy codes. Phase 1 runs from October 1, 2009...

13

Dallas, Texas: 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 Office of Inspector GeneralDepartmentAUDIT REPORT Americium/CuriumSunways JVGroupChoiceCoronationDaelim SolarDallas,

14

City of Dallas- Green Building Expedited Plan Review  

Broader source: Energy.gov [DOE]

The Dallas Green Building Program establishes expedited permitting for green buildings. During Phase 1 of the program (October 1, 2009 - September 30, 2011), applicants must provide a checklist...

15

Timothy E John Dallas Department of Electrical and Computer Engineering  

E-Print Network [OSTI]

Hendriske, Daniel Buscarello, Immanuel Purushothaman, and Tim Dallas, J. of Microelectromechanical Systems-Axis Stage," ­ G. Sivakumar, J. Matthews, and T. Dallas, J. of Microelectromechanical Systems 19, pp. 451. of Microelectromechanical Systems 19, pp. 632-639 (2010). 9. "Design and Analysis of a Dual-Mode MEMS Micromirror," X. Xiong

Zhuang, Yu

16

City of Dallas- Green Building Requirements for Municipal Buildings  

Broader source: Energy.gov [DOE]

In 2003 the Dallas City Council passed a resolution requiring that all new municipal buildings larger than 10,000 square feet be constructed to meet LEED Silver Certification standards. In 2006...

17

Dallas-Fort Worth, TX Clean Taxi Replacement Incentive  

Broader source: Energy.gov [DOE]

The North Central Texas Council of Governments has partnered with the U.S. Environmental Protection Agency and the City of Dallas to develop the North Texas Green & Go Clean Taxi Partnership as...

18

E-Print Network 3.0 - accreting brown dwarfs Sample Search Results  

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

<< < 1 2 3 4 5 > >> 1 The University of Western Ontario DEPARTMENT OF PHYSICS AND ASTRONOMY Summary: : Accretion and dusty disks" ABSTRACT Young brown dwarfs appear to share...

19

SOME EFFECTS OF DDT ON THE GUPPY AND THE BROWN TROUT  

E-Print Network [OSTI]

399 SOME EFFECTS OF DDT ON THE GUPPY AND THE BROWN TROUT SPECIAL SCIENTIFIC REPORT-FISHERIES Na 399, Daniel H . Janzen, Director SOME EFFECTS OF DDT ON THE GUPPY AND THE BROWN TROUT By Susan Frances King following exposure to DDT .... 6 Results 6 Bioassays with the guppy 6 Bioassays with young brown trout 8 Hi

20

Lamb customer satisfaction in two Texas cities - - Dallas and Houston  

E-Print Network [OSTI]

An in-home lamb study evaluated consumer ratings from users of lamb (at least once per month) as influenced by cut (blade chop, rib chop, loin chop, and leg steak), demographics, preparation method, and degree of doneness. Consumers in Dallas...

Maddock, Travis David

2012-06-07T23:59:59.000Z

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


21

Energy Savings Report For Dallas County, July 2000 – June 2001  

E-Print Network [OSTI]

This report presents the energy and dollar savings for the period July 2000 - June 2001 for 12 Dallas County facilities that have been retrofit by Enershop. The savings for this period total $745,046, which represent 73.2% of the audit estimated...

Claridge, D. E.; Baltazar-Cervantes, J. C.; Zhu, Y.

2001-01-01T23:59:59.000Z

22

Sterling A. Brown  

E-Print Network [OSTI]

13 STERLING A. BROWN We sincerely appreciate Charles Rowell's asking us to write this in- troductory note to Callaloo's special section on Sterling Brown. Several recent studies, symposia, and awards are testaments to a revi- val of critical... interest in Sterling Brown, poet, literary critic, teacher, anthologist, and raconteur. The Collected Poems of Sterling A. Brown (Harper & Row), for example, received the Lenore Marshall Poetry Prize for 1980 from Saturday Review. The Modern Language...

Tidwell, John E.

1982-01-01T23:59:59.000Z

23

Town of Dallas, North Carolina (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty LtdSteen,Ltd JumpOperations JumpTooele County,BelmontBostic,ClaytonDallas Town

24

3-D CURVILINEAR MODELLING OF WIND-INDUCED FLOWS THROUGH THE NORTH CHANNEL OF THE IRISH SEA by E.F. Young, J.N. Aldridge and J. Brown  

E-Print Network [OSTI]

(of the order of 1 km) to resolve the complex local bathymetry and current structure of the North Charts supplied by the U.K. Hydrographic Office (Brown et al., 1999).The numerical method used to solve) illustrate the large differences in the magnitude and cross channel variability. 55.20 55.10 55.00 54.90 54

25

Numerical Results on Low Mass Star and Brown Dwarf Multiplicity  

E-Print Network [OSTI]

We have undertaken a series of hydrodynamic + N-body simulations in order to explore the properties of young stars. Our results suggest that the IMF may be sensitive to environment in its substellar region, with more brown dwarfs being formed where clusters are denser or more compact. We find that multiple stars are a natural outcome of collapsing turbulent flows, with a high incidence of N > 2 multiples. We find a positive correlation of multiplicity with primary mass but a companion frequency that decreases with age. Binary brown dwarfs are rarely formed, in conflict with observations. Brown dwarfs as companions are predominantly found orbiting binaries or triples at large separations.

Eduardo Delgado-Donate; Cathie Clarke

2004-12-17T23:59:59.000Z

26

California’s 2012–2013 Budget: Brown’s Budget Gamble  

E-Print Network [OSTI]

Gov. Jerry Brown’s new budget plan targets schools. 24Gov. Jerry Brown’s new budget plan targets schools. 25Gov. Jerry Brown’s new budget plan targets schools. 26

DiSarro, Brian; Hussey, Wesley

2013-01-01T23:59:59.000Z

27

Geochemical study of lead in soils from West Dallas, Texas  

SciTech Connect (OSTI)

Soil samples from West Dallas near the RSR smelter were collected and tested to see the content, source, and mobility of lead. 30 cm and 90 cm long cores were cut into 1 cm long pieces and each piece analyzed separately. The results showed that 90%--95% of the lead is readily extractable in cold dilute nitric acid. The lateral distribution of lead in West Dallas indicates an exponential-like decrease with distance from the RSR smelter. Concentrations greater than 500 ppm occur in soils below 10 cm within 1,000 feet of the smelter. In the vicinity of the smelter (300 feet radius), soil cores with total lead content as high as 18,000 ppm in the top 15 cm were obtained. At a distance of 2,400 feet of the smelter the lead in the soil amounts to 400 ppm and drops to 270 ppm at 4,000 feet. The total lead content with depth, correlates with previous clean-up and civil activities in the area: (1) where the soil is original, the lead concentration decreases exponentially with depth; (2) where the soil was cleaned up, the top 10 cm are devoid of lead but are underlain by soil whose lead content varies in response to distance from the smelter; (3) where the top soil had been disturbed (removed, replaced, mixed, etc.) as a result of civil works, the lead content is relatively lower than 1 (above). The underlying insitu soils exhibit similar lead concentration as those in 2 (above).

Ibrahim, N.M.; Carter, J.L. (Univ. of Texas, Dallas, TX (United States). Programs in Geosciences)

1993-02-01T23:59:59.000Z

28

Case Study Walnut Hill United Methodist Church - Dallas, Texas, Chiller Replacement Analysis  

E-Print Network [OSTI]

In March of 1992 Walnut Hill United Methodist Church in Dallas, Tx. decided that their existing thermal storage and electric reciprocating chiller system were both in need of replacement. After analyzing several options, they chose to install 150...

Phillips, J.

1998-01-01T23:59:59.000Z

29

BROWN ALGAE Colpomenia sinuosa  

E-Print Network [OSTI]

BROWN ALGAE Colpomenia sinuosa GREEN ALGAE Dictyosphaeria cavernosa Amphiroa fragilissima Gelidiopsis intricata Botryocladia pyriformis RED ALGAE CYANOBACTERIA Oscillitoria acuminata Schizothrix sp. "ALGAE"­ A DIVERSE ASSORTMENT OF LIFE FORMS Photosynthesis is performed by a taxonomically diverse

Sullivan, Matthew B.

30

Brandeis University Brown University  

E-Print Network [OSTI]

Institute of Technology McGill University Michigan State University New York University Northwestern University of Kansas University of Maryland, College Park University of Michigan University of MinnesotaBrandeis University Brown University California Institute of Technology Carnegie Mellon University

Jiang, Huiqiang

31

Descriptions and Uses of Soils of the Texas Agricultural Experiment Stations at Dallas and Prosper.  

E-Print Network [OSTI]

in Orillaal B'uliednl . ,- .I -, " .. I. ~ ... . ,. ~. .~ ~. Descriptions and Uses of Soils of the Texas Agricultural Experiment Stations at Dallas and Prosper by Billy W. Hipp, Tim C. Knowles, and Benny J. Simpson Professor, Research Associate..., and Research Scientist, respectively Texas A&M University Research and Extension Center at Dallas Texas Agricultural Experiment Station in cooperation with Billy R. Stringer Soil Scientist Soil Conservation Service, Terrell, TX and C. Tom Hallmark...

Hipp, Billy W.; Knowles, Tim C.; Simpson, Benny J.; Stringer, Billy R.; Hallmark, C. Tom

1992-01-01T23:59:59.000Z

32

Top 10 Considerations of 2012 IECC and IgCC in Dallas  

E-Print Network [OSTI]

Air Through Energy Efficiency Conference, San Antonio, Texas Dec. 16-18 ? Statewide energy code; adoption mandated by SECO ? Jurisdictional sustainability code ?Dallas modified and adopted as Dallas City Code Chapter 61 ? Alternate compliance...CATEE CONFERENCE SAN ANTONIO, TX December 18, 2013 ESL-KT-13-12-31 CATEE 2013: Clean Air Through Energy Efficiency Conference, San Antonio, Texas Dec. 16-18 This presentation is protected by US and International copyright laws. Reproduction...

Basora, Z.

2013-01-01T23:59:59.000Z

33

Steven Brown Oral History  

E-Print Network [OSTI]

Part 4 video platform video management video solutionsvideo player Part 5 video platform video management video solutionsvideo player Part 6 video platform video management video solutionsvideo player Part 7 video platform video... Under the Rainbow: Oral Histories of GLBTQ People in Kansas Steven Brown Oral History Part 2 video platform video management video solutionsvideo player Part 3 video platform video management video solutionsvideo player...

Brown, Steven; Albin, Tami

2010-11-24T23:59:59.000Z

34

affects browning susceptibility: Topics by E-print Network  

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

17 ECOTOXICOLOGY Exposure of Brown Recluse and Brown Widow Spiders (Araneae Renewable Energy Websites Summary: ECOTOXICOLOGY Exposure of Brown Recluse and Brown Widow Spiders...

35

acquired brown syndrome: Topics by E-print Network  

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

9 ECOTOXICOLOGY Exposure of Brown Recluse and Brown Widow Spiders (Araneae Renewable Energy Websites Summary: ECOTOXICOLOGY Exposure of Brown Recluse and Brown Widow Spiders...

36

The Relationship between Land Use and Temperature Change in Dallas County, Texas  

E-Print Network [OSTI]

to the formation of urban heat islands based on different categories of land use. Specifically, this research analyzes the elements that contribute to the urban heat island effect in Dallas County using temperature data provided by remote sensing imagery and parcel...

Kim, Hee Ju

2010-10-12T23:59:59.000Z

37

The University of Texas at Dallas 1 Bachelor of Science in Geospatial  

E-Print Network [OSTI]

The University of Texas at Dallas 1 Bachelor of Science in Geospatial Information Sciences Geospatial information sciences (GISc) harness ground- breaking technologies to analyze features of the Earth range of fields to combine efforts on leading-edge research. Careers in Geospatial Information Sciences

O'Toole, Alice J.

38

The University of Texas at Dallas Erik Jonsson School c C. D. Cantrell (06/1997)  

E-Print Network [OSTI]

The University of Texas at Dallas Erik Jonsson School PhoTEC c C. D. Cantrell (06/1997) FRESNEL. D. Cantrell (06/1997) FRESNEL-KIRCHHOFF DIFFRACTION THEORY (1) · Maxwell's equations imply. Cantrell (06/1997) FRESNEL-KIRCHHOFF DIFFRACTION THEORY (2) · The scalar wave equation, 2 - 1 v2 2 t2 U

Hart, Gus

39

Dallas, August 18-22 Volume 20, Number 4, 1986 THE RENDERING EQUATION  

E-Print Network [OSTI]

Dallas, August 18-22 Volume 20, Number 4, 1986 THE RENDERING EQUATION James T. Kajiya California variety of known rendering algorithms. In the course of discussing a monte carlo solutionwe alsopresent reduction. CR CATEGORIES: 1.3.3,1.3.5,1.3.7 1. The rendering equation The technique we present subsumes

Frey, Pascal

40

SCOPES'05 Dallas, TX, Sept., 2005 Risk-Based Quality Improvement  

E-Print Network [OSTI]

distribution of cost, usage, quality, defect, performance, etc. "80:20" rule or Pareto's principle. Units-uniform attention/effort in ­ testing UBST ­ other focused quality assurance · Usage-based statistical testingSCOPES'05 Dallas, TX, Sept., 2005 Risk-Based Quality Improvement for Embedded Systems Jeff Tian

Tian, Jeff

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


41

Alabama Nuclear Profile - Browns Ferry  

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

Browns Ferry" "Unit","Summer capacity (mw)","Net generation (thousand mwh)","Summer capacity factor (percent)","Type","Commercial operation date","License expiration date"...

42

Idaho_Brown  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation ProposedUsingFun withconfinementEtching. | EMSLtheIndustryMitch Arkoosh SiteMtn.Reta Brown

43

Modeling the per capita ecological footprint for Dallas County, Texas: Examining demographic, environmental value, land-use, and spatial influences  

E-Print Network [OSTI]

This study addresses factors driving the variation in the per capita Ecological Footprint (EF) in Dallas County, Texas. A main hypothesis was that scientifically estimated demography, environmental values, spatial attributes, and land-use patterns...

Ryu, Hyung Cheal

2005-08-29T23:59:59.000Z

44

Changing the state of fairness : redeveloping Fair Park as a catalyst for the revitalization of South Dallas  

E-Print Network [OSTI]

This thesis studies Fair Park, a 277 acre public park located in Dallas, Texas. Fair Park represents prevalent planning challenges - the repurposing of sites that have outlived their initial uses and the reintegration of ...

Di Mambro, Giuliana Siena

2013-01-01T23:59:59.000Z

45

Petrologic and petrophysical evaluation of the Dallas Center Structure, Iowa, for compressed air energy storage in the Mount Simon Sandstone.  

SciTech Connect (OSTI)

The Iowa Stored Energy Plant Agency selected a geologic structure at Dallas Center, Iowa, for evaluation of subsurface compressed air energy storage. The site was rejected due to lower-than-expected and heterogeneous permeability of the target reservoir, lower-than-desired porosity, and small reservoir volume. In an initial feasibility study, permeability and porosity distributions of flow units for the nearby Redfield gas storage field were applied as analogue values for numerical modeling of the Dallas Center Structure. These reservoir data, coupled with an optimistic reservoir volume, produced favorable results. However, it was determined that the Dallas Center Structure cannot be simplified to four zones of high, uniform permeabilities. Updated modeling using field and core data for the site provided unfavorable results for air fill-up. This report presents Sandia National Laboratories' petrologic and petrophysical analysis of the Dallas Center Structure that aids in understanding why the site was not suitable for gas storage.

Heath, Jason E.; Bauer, Stephen J.; Broome, Scott Thomas; Dewers, Thomas A.; Rodriguez, Mark Andrew

2013-03-01T23:59:59.000Z

46

Spatial Ecology of and Public Attitudes toward Monk Parakeets Nesting on Electric Utility Structures in Dallas and Tarrant Counties, Texas  

E-Print Network [OSTI]

2013, we examined the spatial ecology of and public attitudes toward monk parakeets nesting on electric utility structures in Dallas and Tarrant counties, Texas, US. As nest sites, monk parakeets selected electric switchyards and substations...

Reed, Janet Elaine

2014-07-29T23:59:59.000Z

47

Measured Cooling Performance of Two-story Homes in Dallas, Texas; Insulated Concrete Form Versus Frame Construction  

E-Print Network [OSTI]

Four occupied homes near Dallas, Texas were monitored to compare heating and cooling energy use. Two homes were built with typical wood frame construction, the other two with insulated concrete form (ICF) construction. Remote data loggers collected...

Chasar, D.; Moyer, N.; Rudd, A. F.; Parker, D.; Chandra, S.

2002-01-01T23:59:59.000Z

48

Landslide susceptibility mapping for real estate development, tested along I-35, Dallas to San Antonio, Texas  

E-Print Network [OSTI]

estate industry. In order to accomplish this objective, areas were field checked for slope instabilities within four major cities o- the Cretaceous belt: Dallas, Waco, Austin, and San Antonio. All clay formations in the study area were found...-De'I Rio Formation boundaries. Here the caprock tends to squeeze out the underlying clays; rockfalls of the overlying limestone occur. The Bergstrom, Del Rio and Eagle Ford Formations of San Antonio, and the Eagle Ford Formation of Austin have...

Gaidusek, Barbara Ursel Marie

1982-01-01T23:59:59.000Z

49

Test Access Mechanism for Core Based SystemonChip The Univ. of Texas at Dallas  

E-Print Network [OSTI]

1 Test Access Mechanism for Core Based System­on­Chip M. Nourani The Univ. of Texas at Dallas Dept of TAM for SoC's. The basic goal is to develop a global design for test methodology and tool for testing as their interactions to one another. More specifically, it al­ lows at­speed testing and multi­core interaction during

Nourani, Mehrdad

50

Brown, Lipton, and the Prospects of High-level IBE Brown's Project  

E-Print Network [OSTI]

Brown, Lipton, and the Prospects of High-level IBE Brown's Project With Brown's paper we turn question about the selection procedures which scientists use for identifying those theories which

Fitelson, Branden

51

Relationally-Parametric Polymorphic Contracts Brown University  

E-Print Network [OSTI]

Relationally-Parametric Polymorphic Contracts Arjun Guha Brown University arjun@cs.brown.edu Jacob are not made or distributed for profit or commercial advantage and that copies bear this notice and the full

Krishnamurthi, Shriram

52

Two Lost Sonnets by Sterling A. Brown  

E-Print Network [OSTI]

TWO LOST SONNETS BY STERLING A. BROWN edited and introduced by John Edgar Tidwell and Ted Genoways The emergence of Sterling A. Brown into poetic maturity resulted from a well- known dialectical engagement with the aesthetics of African...-American folk tradition. As Brown recounted so often, these experiential and imaginative encounters derived from a benevolent conspiracy between his theologian father, the Rev. Sterling Nelson Brown, and the eminent historian Carter G. Woodson to send...

Tidwell, John E.

1998-09-01T23:59:59.000Z

53

L. Frank Brown, Jr. Publications  

E-Print Network [OSTI]

, Seismic stratigraphic interpretation and petroleum potential: Tulsa, American Association of Petroleum. W., and McGowen, J. H., 1971, Resource capability units, their utility in land and water-use Association of Petroleum Geologists, AAPG Memoir 58, p. 43­69. Muntingh, A., and Brown, L. F., Jr., 1994

Yang, Zong-Liang

54

Evaluation of the Dallas Thompson Riverscreen Site on the Touchet River.  

SciTech Connect (OSTI)

Riverscreen irrigation pumps are a relatively new design in which the pump intake floats on the river surface, pulling water in only from the bottom side and surrounded by a self-cleaning screen. The Walla Walla County Conservation District recently started replacing old pump screens with the Riverscreen and was interested in whether the screens are protective of juvenile salmonids. Pacific Northwest National Laboratory evaluated approach velocities and operations at the Riverscreen installation on the Dallas Thompson property, approximately 3 mi. north of Touchet, Washington and 300 ft north of Hofer Dam, on June 18, 2007. Evaluation of this site consisted of underwater videography and water velocity measurements. The Dallas Thompson Riverscreen was pumping approximately 930 gpm during our evaluation, which is close to the maximum pumping rate for this model. Underwater videography showed only slow movement of water-borne particulates toward the pump intake, and the screen material was clean. All water velocity measurements were taken below the pump intake opening and between 3 to 6 in. from the screen face. All approach velocities (flow toward the screen and pump) were below National Marine Fisheries Service draft guidelines for juvenile fish screens.

Chamness, Mickie [Pacific Northwest National Laboratory

2007-07-25T23:59:59.000Z

55

DRAFT UT DALLAS POLICY ON FINANCIAL EXIGENCY (Rev 3 MR 2010) The enunciation of a policy in Rule 31003, Section 1, of the Regents' Rules and Regulations  

E-Print Network [OSTI]

1 DRAFT UT DALLAS POLICY ON FINANCIAL EXIGENCY (Rev 3 MR 2010) Preamble The enunciation of a policy in Rule 31003, Section 1, of the Regents' Rules and Regulations (http://www.utsystem.edu/bor/rules.htm#A4

O'Toole, Alice J.

56

To be presented at the 2007 ASHRAE Winter Meeting, January 27-31, 2007, Dallas, TX. Measured energy performance a US-China demonstration  

E-Print Network [OSTI]

efficient than ASHRAE 90.1- 1999. The utility data from the first year's operation match well the analysisLBNL-60978 To be presented at the 2007 ASHRAE Winter Meeting, January 27-31, 2007, Dallas, TX

57

Fermilab Today | Brown University Profile  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation ProposedUsing ZirconiaPolicyFeasibility ofSmall Works: 2008Submit a5,19,Brown University April

58

Brown carbon formation from ketoaldehydes of biogenic monoterpenes...  

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

Brown carbon formation from ketoaldehydes of biogenic monoterpenes. Brown carbon formation from ketoaldehydes of biogenic monoterpenes. Abstract: Sources and chemical composition...

59

Human Biology Program Brown Bag Series  

E-Print Network [OSTI]

Human Biology Program Brown Bag Series Fall 2012 12:001:00 pm Morrison Hall 103 SeptemberVisser Department of Biology & Human Biology Prog. "Good Behavior, Bad Behavior: Insights From the Microbial

Indiana University

60

L. A. Brown, M. C. Higuera  

Office of Scientific and Technical Information (OSTI)

Brown, M. C. Higuera Prepared by Sandia National Laboratories Albuquerque, New Mexico 87185 and L b SANDlA REPORT SAND974017 0 UC-700 Unlimited Release Printed February i 998...

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


61

The construction of the Browns Bay Vessel  

E-Print Network [OSTI]

INVESTIGATIVE TECHNIQUES. 10 19 The Site. National Historic Sites Service Excavation and Raising of the Vessel Vessel on Display. The Vessel in 1985. 19 20 27 28 Method of Recording III THE CONSTRUCTION OF THE VESSEL 31 36 The Keel 36 The Stem... A flat-bottomed boat being built. 17 9 Forelocked eye-bolts from the midship beam of the Browne Bay Vessel 21 10 Broad arrow stamped in an eye-bolt from the Browns Bay Vessel. . . . . . . . . . . . . . . . . . . . . . . . . . . 22 11 Pulley...

Amer, Christopher Francis

2012-06-07T23:59:59.000Z

62

Impacts of cool cities on air quality: A preliminary modeling assessment for Nashville TN, Dallas TX and Atlanta GA  

SciTech Connect (OSTI)

Previous atmospheric modeling efforts that concentrated on the Los Angeles Basin suggested beneficial and significant air quality impacts from cool cities strategies. This paper discusses an extension of similar modeling efforts to three regions, Atlanta GA, Dallas - Ft. Worth TX, and Nashville TN, that experience smog and air quality problems. According to the older ozone air quality standard (120 ppb), these regions were classified as serious, moderate, and marginal, respectively, but may be out of compliance with respect to the newer, 80-ppb/8-hours standard. Results from this exploratory modeling work suggest a range of possible impacts on meteorological and air quality conditions. For example, peak ozone concentrations during each region's respective episode could be decreased by 1-6 ppb (conservative and optimistic scenarios, respectively) in Nashville, 5-15 ppb in Dallas - Fort Worth, and 5-12 ppb in Atlanta following implementation of cool cities. The reductions are generally smaller than those obtained from simulating the Los Angeles Basin but are still significant. In all regions, the simulations suggest, the net, domain-wide effects of cool cities are reductions in ozone mass and improvements in air quality. In Atlanta, Nashville, and Dallas, urban areas benefiting from reduced smog reach up to 8460, 7350, and 12870 km{sup 2} in area, respectively. Results presented in this paper should be taken as exploratory and preliminary. These will most likely change during a more comprehensive modeling study to be started soon with the support of the US Environmental Protection Agency. The main purpose of the present project was to obtain the initial data (emission inventories) for these regions, simulate meteorological conditions, and perform preliminary sensitivity analysis. In the future, additional regions will be simulated to assess the potential of cool cities in improving urban air quality.

Taha, Haider

1998-06-15T23:59:59.000Z

63

E-Print Network 3.0 - asian brown cloud Sample Search Results  

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

brown cloud Search Powered by Explorit Topic List Advanced Search Sample search results for: asian brown cloud Page: << < 1 2 3 4 5 > >> 1 ANNOUNCEMENT Project Atmospheric Brown...

64

17 Years of Lithium Brown Dwarfs 10/21/12Ringberg Brown Dwarfs 1  

E-Print Network [OSTI]

, Graham, ApJ, 428, L57, June. 1994 #12;The First (correct and public) Brown Dwarf: PPl 15 10/21/12Ringberg Dwarf: PPl 15 10/21/12Ringberg Brown Dwarfs 4 We found that the only plausible way to reconcile "lithium dating". This adjustment in age meant that the inferred mass of PPl 15 rose to near the substellar

Joergens, Viki

65

Hermitian Young operators  

SciTech Connect (OSTI)

Starting from conventional Young operators, we construct Hermitian operators which project orthogonally onto irreducible representations of the (special) unitary group.

Keppeler, Stefan, E-mail: stefan.keppeler@uni-tuebingen.de [Mathematisches Institut, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen (Germany)] [Mathematisches Institut, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen (Germany); Sjödahl, Malin, E-mail: malin.sjodahl@thep.lu.se [Department of Astronomy and Theoretical Physics, Lund University, Sölvegatan 14A, 223 62 Lund (Sweden)] [Department of Astronomy and Theoretical Physics, Lund University, Sölvegatan 14A, 223 62 Lund (Sweden)

2014-02-15T23:59:59.000Z

66

acute brown adipose: Topics by E-print Network  

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

into the brown "lithium dating". This adjustment in age meant that the inferred mass of PPl 15 rose to near the substellar Joergens, Viki 62 Orbital migration and the brown dwarf...

67

author browne niall: Topics by E-print Network  

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

into the brown "lithium dating". This adjustment in age meant that the inferred mass of PPl 15 rose to near the substellar Joergens, Viki 63 Orbital migration and the brown dwarf...

68

FIA-12-0009- In the Matter of Cynthia Brown  

Broader source: Energy.gov [DOE]

Cynthia Brown filed an Appeal regarding a request she filed under the Freedom of Information Act. In December 2011, Ms. Brown filed a request for records regarding her late mother.

69

FIA-12-0044- In the Matter of Cynthia Brown  

Broader source: Energy.gov [DOE]

Cynthia Brown filed an Appeal regarding a request filed under the Freedom of Information Act. In March 2012, Ms. Brown filed a request for records regarding her late mother.

70

Publications of Richard E. Brown Refereed Journal Articles  

E-Print Network [OSTI]

-2838. Brown, Richard E., and Jonathan G. Koomey. 2003. "Electricity Use in California: Past Trends and Present-Haggerty, H.Y. Iris Cheung, Jay Taneja, David Culler, and Richard Brown. 2013. "Methods for detailed energy E. Brown, and Brett C. Singer. 2013. "Evaluation of miscellaneous and electronic device energy use

71

Title Position Holder Increased GPA Student Affairs Dr. Charles Brown  

E-Print Network [OSTI]

Dr. Charles Brown Associate Vice President & Dean of Students Dr. Corey King 3 6 15 $4000-10,000 per Dr. Charles Brown Associate Vice President & Dean of Students Dr. Corey King Develop a program. Charles Brown Associate Vice President & Dean of Students Dr. Corey King identify student needs, location

Fernandez, Eduardo

72

Caribbean House Patrick Brown, Faculty Director  

E-Print Network [OSTI]

1 Caribbean House Patrick Brown, Faculty Director Jerry Aviles, Student Director Sonia Nelson, Student Director OVERVIEW The Caribbean House will be a phenomenal experience for everyone, not just the Caribbean culture and demonstrate the beautiful lifestyle that we try to live everyday. There is already

Hayden, Nancy J.

73

Molecular Selectivity of Brown Carbon Chromophores  

SciTech Connect (OSTI)

Complementary methods of high-resolution mass spectrometry and micro-spectroscopy were utilized for molecular analysis of secondary organic aerosol (SOA) generated from ozonolysis of two structural monoterpene isomers: D-limonene (LSOA) and a-pinene (PSOA). Laboratory simulated aging of LSOA and PSOA, through conversion of carbonyls into imines mediated by NH3 vapors in humid air, resulted in selective browning of the LSOA sample, while the PSOA sample remained white. Comparative analysis of the reaction products in the aged LSOA and PSOA samples provided insights into chemistry relevant to formation of brown carbon chromophores. A significant fraction of carbonyl-imine conversion products with identical molecular formulas were detected in both samples. This reflects the high level of similarity in the molecular composition of these two closely related SOA materials. Several highly conjugated products were detected exclusively in the brown LSOA sample and were identified as potential chromophores responsible for the observed color change. The majority of the unique products in the aged LSOA sample with the highest number of double bonds contain two nitrogen atoms. We conclude that chromophores characteristic of the carbonyl- imine chemistry in LSOA are highly conjugated oligomers of secondary imines (Schiff bases) present at relatively low concentrations. Formation of this type of conjugated compounds in PSOA is hindered by the structural rigidity of the a-pinene oxidation products. Our results suggest that the overall light-absorbing properties of SOA may be determined by trace amounts of strong brown carbon chromophores.

Laskin, Julia; Laskin, Alexander; Nizkorodov, Sergey; Roach, Patrick J.; Eckert, Peter A.; Gilles, Mary K.; Wang, Bingbing; Lee, Hyun Ji; Hu, Qichi

2014-09-18T23:59:59.000Z

74

February 1, 2006 Emmett Brown, Executive Director  

E-Print Network [OSTI]

February 1, 2006 Emmett Brown, Executive Director National Fresh Water Fishing Hall of Fame P deduce the length of the fish by assuming a height of the angler of 72" and using direct scaling. Even between the distance of the camera to the angler and to the fish. Discounting that distance leads

Arnold, Douglas N.

75

David K Brown Geriatrics Scholar Program  

E-Print Network [OSTI]

David K Brown Geriatrics Scholar Program Sponsored By: This project is supported by a grant from the Health Resources and Services Administration (HRSA), under grant number UB4HP19050 West Virginia, DHHR, or U. S. government. #12;Background and Introduction The WVGEC is funded by the U. S. Department

Mohaghegh, Shahab

76

ROBERT BROWN DEPUTY MANAGER, OAK RIDGE OFFICE  

E-Print Network [OSTI]

ROBERT BROWN DEPUTY MANAGER, OAK RIDGE OFFICE AUGUST 24, 2010 OVERVIEW OF THE UNITED STATES DEPARTMENT OF ENERGY OAK RIDGE OFFICE #12;( 2 ) KEY OAK RIDGE MISSIONS Oak Ridge Office · Science CONTRACTORS Oak Ridge National Laboratory Oak Ridge Institute for Science and Education Office of Scientific

77

2006 BEEKEEPING Young Harris College  

E-Print Network [OSTI]

2006 BEEKEEPING INSTITUTE May 18-20 Young Harris College Young Harris, Georgia #12;Young Harris in honey, the Honey Show includes classes in photography, art, candles, section comb honey, mead

Delaplane, Keith S.

78

BEEKEEPING INSTITUTE Young Harris College  

E-Print Network [OSTI]

2008 BEEKEEPING INSTITUTE May 15-17 Young Harris College Young Harris, Georgia #12;Young Harris, section comb honey, mead, and beekeeping gadgets. We urge students to participate in the Institute Honey

Delaplane, Keith S.

79

Home sweet home: Texas A&M AgriLife opens the first WaterSense-labeled house in Dallas-Fort Worth  

E-Print Network [OSTI]

, Woodson said. O#14;en, rebates and incentives are also available for irrigation e#16;ciency upgrades, rainwater collection systems and smart irrigation controllers. According to the experts at the Dallas center, taking advantage of such incentives.... ?Blackfoot daisies will bloom all summer long.? ?#29;e plants we selected are so dependable and hardy #20; you never have to worry about them, unless you overwater them,? Dickinson said. #29;e #27;,#30;#30;#30;-gallon rainwater tank at the rear...

Lee, Leslie

2013-01-01T23:59:59.000Z

80

Organizational Chart Michelle H. Brown-Nevers, Ed.D.  

E-Print Network [OSTI]

Organizational Chart Michelle H. Brown-Nevers, Ed.D. Associate Vice President Marlene Bruno Manager Assistant Director Mainframe Systems Kate Micklow Assistant Director Administrative Support Stuart Campbell

Plotkin, Joshua B.

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


81

The Formation of Brown Dwarfs as Ejected Stellar Embryos  

E-Print Network [OSTI]

We conjecture that brown dwarfs are substellar objects because they have been ejected from small newborn multiple systems which have decayed in dynamical interactions. In this view, brown dwarfs are stellar embryos for which the star formation process was aborted before the hydrostatic cores could build up enough mass to eventually start hydrogen burning. The disintegration of a small multiple system is a stochastic process, which can be described only in terms of the half-life of the decay. A stellar embryo competes with its siblings in order to accrete infalling matter, and the one that grows slowest is most likely to be ejected. With better luck, a brown dwarf would therefore have become a normal star. This interpretation of brown dwarfs readily explains the rarity of brown dwarfs as companions to normal stars (aka the ``brown dwarf desert''), the absence of wide brown dwarf binaries, and the flattening of the low mass end of the initial mass function. Possible observational tests of this scenario include statistics of brown dwarfs near Class 0 sources, and the kinematics of brown dwarfs in star forming regions while they still retain a kinematic signature of their expulsion. Because the ejection process limits the amount of gas brought along in a disk, it is predicted that substellar equivalents to the classical T Tauri stars should be very rare.

Bo Reipurth; Cathie Clarke

2001-03-01T23:59:59.000Z

82

ORIGINAL RESEARCH Introgression of Brown Norway Chromosome 1 onto the Fawn  

E-Print Network [OSTI]

ORIGINAL RESEARCH Introgression of Brown Norway Chromosome 1 onto the Fawn Hooded Hypertensive (FHH) and Brown Norway (BN) parent strains with a Brown Norway chromosome 1 substitution on the FHH

Helmstetter, Fred J.

83

Light brown apple moth’s arrival in California worries commodity groups  

E-Print Network [OSTI]

control of light brown apple moth, Epi- phyas postvittana (2007a. Light brown apple moth host list. www.cdfa.ca.gov/p. CDFA. 2007b. Light brown apple moth project: Advisories.

Varela, Lucia G.; Johnson, Marshall W; Strand, Larry; Wilen, Cheryl A; Pickel, Carolyn

2008-01-01T23:59:59.000Z

84

Solar heating and hot water system installed at office building, One Solar Place, Dallas, Texas. Final report  

SciTech Connect (OSTI)

This document is the Final Report of the Solar Energy System Installed at the First Solar Heated Office Building, One Solar Place, Dallas, Texas. The Solar System was designed to provide 87 percent of the space heating needs, 100 percent of the potable hot water needs and is sized for future absorption cooling. The collection subsystem consists of 28 Solargenics, series 76, flat plate collectors with a total area of 1596 square feet. The solar loop circulates an ethylene glycol-water solution through the collectors into a hot water system heat exchanger. The hot water storage subsystem consists of a heat exchanger, two 2300 gallon concrete hot water storage tanks with built in heat exchangers and a back-up electric boiler. The domestic hot water subsystem sends hot water to the 10,200 square feet floor area office building hot water fixtures. The building cold water system provides make-up to the solar loop, the heating loop, and the hot water concrete storage tanks. The design, construction, cost analysis, operation and maintenance of the solar system are described. The system became operational July 11, 1979.

Not Available

1980-06-01T23:59:59.000Z

85

Abiotic and biotic factors affecting light brown apple moth, Epiphyas postvittana, in California  

E-Print Network [OSTI]

mortality of lightbrown apple moth. In: O’Callaghan, M. (tryoni and the light brown apple moth Epiphyas postvittanaof the light brown apple moth, Epiphyas postvittana (

Buergi, Linda Patricia

2012-01-01T23:59:59.000Z

86

Biosorption of Trivalent Chromium on the Brown Seaweed Biomass  

E-Print Network [OSTI]

Biosorption of Trivalent Chromium on the Brown Seaweed Biomass Y E O U N G - S A N G Y U N , D O N brown alga Ecklonia biomass as a model system. Titration of the biomass revealed that it contains that various biosorbents are able to effectively remove chromium (4-11). Some of the biomass types have

Volesky, Bohumil

87

Boiler Gold Rush Prof. Johnny Brown (MATH 700)  

E-Print Network [OSTI]

Boiler Gold Rush Prof. Johnny Brown (MATH 700) jeb@math.purdue.edu #12;#12;#12;David McCullough, Jr help Always be prepared #12;Boiler Gold Rush Prof. Johnny Brown (MATH 700) jeb@math.purdue.edu #12;

Brown, Johnny E.

88

Project-Based Engineering Education at Brown University  

E-Print Network [OSTI]

in calculation-based, creative design projects, start- ing in their first semester engineering courseProject-Based Engineering Education at Brown University The School of Engineering at Brown. At the same time, students develop strong theoretical foundations in different areas of engineering before

89

BROWN Y FERNNDEZ, Heliconiini de Venezuela Los Heliconiini (Lepidoptera, Nymphalidae)  

E-Print Network [OSTI]

BROWN Y FERNÁNDEZ, Heliconiini de Venezuela 29 Los Heliconiini (Lepidoptera, Nymphalidae) de Venezuela KEITH S. BROWN, JR.* Y F. FERNÁNDEZ Y�PEZ** RESUMEN Se ilustran y presentan datos sobre variación, distribución y biología de las 42 especies y 88 subespecies de Heliconiini conocidas de Venezuela, con

Mallet, James

90

December 2013 EA Report Brown Bagger 1 Train the Trainer,  

E-Print Network [OSTI]

December 2013 EA Report Brown Bagger 1 Brown Bagger Train the Trainer, before Training Others. In truth, the secret to successful training is to train the trainers FIRST...before they train others. There is an entire skill set that needs to belong to a person conducting a given training, which includes knowing

Kim, Duck O.

91

Russell Brown: Department of Mathematics, University of Kentucky, Lexington, Kentucky 40506--0027, brown@ms.uky.edu  

E-Print Network [OSTI]

Russell Brown: Department of Mathematics, University of Kentucky, Lexington, Kentucky 40506--0027, brown@ms.uky.edu Zhongwei Shen: Department of Mathematics, University of Kentucky, Lexington, Kentucky 40506--0027, shenz@ms.uky.edu Peter Perry: Department of Mathematics, University of Kentucky, Lexington

Kentucky, University of

92

Planets of young stars  

E-Print Network [OSTI]

Since the first massive planet in a short period orbit was discovered, the question arised how such an object could have formed. There are basically two formation scenarios: migration due to planet-disk or planet-planet interaction. Which of the two scenarios is more realistic can be found out by observing short-period planets of stars with an age between 10E7 and 10E8 yrs. The second aim of the survey is to find out how many planets originally formed, and how many of these are destroyed in the first Gyrs: Do most young, close-in planets evaporate, or spiral into the host stars? In here we report on the first results of a radial-velocity search program for planets of young stars which we began in 2004. Using HARPS, we currently monitor 85 stars with ages between 10E7 and 10E8 yrs. We show that the detection of planets of young stars is possible. Up to now, we have identified 3 planet-candidates. Taking this result together with the results of other surveys, we conclude that the frequency of massive-short period planets of young stars is not dramatically higher than that of old stars.

E. W. Guenther; E. Esposito

2007-01-10T23:59:59.000Z

93

Correlated spectral variability in brown dwarfs  

E-Print Network [OSTI]

Models of brown dwarf atmospheres suggest they exhibit complex physical behaviour. Observations have shown that they are indeed dynamic, displaying small photometric variations over timescales of hours. Here I report results of infrared (0.95-1.64 micron) spectrophotometric monitoring of four field L and T dwarfs spanning timescales of 0.1-5.5 hrs, the goal being to learn more about the physical nature of this variability. Spectra are analysed differentially with respect to a simultaneously observed reference source in order to remove Earth-atmospheric variations. The variability amplitude detected is typically 2-10%, depending on the source and wavelength. I analyse the data for correlated variations between spectral indices. This approach is more robust than single band or chisq analyses, because it does not assume an amplitude for the (often uncertain) noise level (although the significance test still assumes a shape for the noise power spectrum). Three of the four targets show significant evidence for cor...

Bailer-Jones, C A L

2007-01-01T23:59:59.000Z

94

Toxins not neutralized by brown snake antivenom  

SciTech Connect (OSTI)

The Australian snakes of the genus Pseudonaja (dugite, gwardar and common brown) account for the majority of snake bite related deaths in Australia. Without antivenom treatment, the risk of mortality is significant. There is an accumulating body of evidence to suggest that the efficacy of the antivenom is limited. The current study investigates the protein constituents recognized by the antivenom using 2-DE, immuno-blot techniques and rat tracheal organ bath assays. The 2-DE profiles for all three snake venoms were similar, with major species visualized at 78-132 kDa, 32-45 kDa and 6-15 kDa. Proteins characterized by LC-MS/MS revealed a coagulant toxin ({approx}42 kDa) and coagulant peptide ({approx}6 kDa), as well as two PLA{sub 2} ({approx}14 kDa). Peptides isolated from {approx}78 kDa and 15-32 kDa protein components showed no similarity to known protein sequences. Protein recognition by the antivenom occurred predominantly for the higher molecular weight components with little recognition of 6-32 kDa MW species. The ability of antivenom to neutralize venom activity was also investigated using rat tracheal organ bath assays. The venoms of Pseudonaja affinis affinis and Pseudonaja nuchalis incited a sustained, significant contraction of the trachea. These contractions were attributed to PLA{sub 2} enzymatic activity as pre-treatment with the PLA{sub 2} inhibitor 4-BPB attenuated the venom-induced contractions. The venom of Pseudonaja textilis incited tracheal contractility through a non-PLA{sub 2} enzymatic activity. Neither activity was attenuated by the antivenom treatment. These results represent the first proteomic investigation of the venoms from the snakes of the genus Pseudonaja, revealing a possible limitation of the brown snake antivenom in binding to the low MW protein components.

Judge, Roopwant K. [Molecular Genetics and Evolution Group, Research School of Biological Sciences, Australian National University, Canberra 2601, ACT (Australia); Henry, Peter J. [School of Medicine and Pharmacology, University of Western Australia, Crawley 6009, Western Australia (Australia); Mirtschin, Peter [Venom Supplies, Tanunda 5352, South Australia (Australia); Jelinek, George [School of Primary, Aboriginal and Rural Health Care, QEII Medical Centre, Western Australia (Australia); Wilce, Jacqueline A. [Department of Biochemistry and Molecular Biology, Monash University, Clayton 3800, VIC Victoria (Australia)]. E-mail: Jackie.Wilce@med.monash.edu.au

2006-06-01T23:59:59.000Z

95

BEEKEEPING INSTITUTE Young Harris College  

E-Print Network [OSTI]

2007 BEEKEEPING INSTITUTE May 17-19 Young Harris College Young Harris, Georgia #12;Young Harris in photography, art, candles, cut- comb honey, mead, and beekeeping gadgets. We urge students to participate for Observation Hives, Tom Webster 10:00 BREAK 10:30 Spring and Summer Management, One Perspective, Dan Harris

Delaplane, Keith S.

96

Kinematics of stars and brown dwarfs at birth  

E-Print Network [OSTI]

We use numerical N-body simulations in order to test whether the kinematics of stars and brown dwarfs at birth depend on mass. In particular we examine how initial variations in velocity dispersion can affect the spatial distribution of stellar and substellar objects in clusters. We use 'toy' N-body models of a Pleiades-like cluster in which brown dwarfs have their own velocity dispersion sigma_(V_BD) which is k times larger than the stellar one. We find that in order to match the broad agreement between the brown dwarf fraction in the field and in the Pleiades, the velocity dispersion of brown dwarfs at birth has to be less than twice the stellar velocity dispersion, i.e. cannot exceed a few km/s in the Pleiades cluster. In order to discern more subtle differences between the kinematics of brown dwarfs and stars at birth, our simulations show that we need to look at clusters that are much less dynamically evolved than the Pleiades. One might especially seek evidence of high velocity brown dwarfs at birth by examining spatial distribution of stars and brown darfs in clusters that are about a crossing timescale old.

E. Moraux C. Clarke

2004-10-01T23:59:59.000Z

97

Energy Input, Carbon Intensity, and Cost for Ethanol Produced from Brown Seaweed  

E-Print Network [OSTI]

Energy Input, Carbon Intensity, and Cost for Ethanol Produced from Brown Seaweed by Aaron, Carbon Intensity, and Cost for Ethanol Produced from Brown Seaweed by Aaron Philippsen B.Eng, University of Mechanical Engineering) Co-Supervisor Brown macroalgae or brown seaweed is a promising source of ethanol

Victoria, University of

98

Discovery of a Young Substellar Companion in Chamaeleon  

E-Print Network [OSTI]

During an imaging survey of the Chamaeleon I star-forming region with the ACS aboard HST, we have discovered a candidate substellar companion to the young low-mass star CHXR 73 (~2 Myr, M=0.35 Msun). We measure a projected separation of 1.3+/-0.03" for the companion, CHXR 73 B, which corresponds to 210 AU at the distance of the cluster. A near-infrared spectrum of this source obtained with CorMASS at the Magellan II telescope exhibits strong steam absorption that confirms its late-type nature (>=M9.5). In addition, the gravity-sensitive shapes of the H- and K-band continua demonstrate that CHXR 73 B is a young, pre-main-sequence object rather than a field star. The probability that CHXR 73A and B are unrelated members of Chamaeleon I is ~0.001. We estimate the masses of CHXR 73 B and other known substellar companions in young clusters with a method that is consistent with the dynamical measurements of the eclipsing binary brown dwarf 2M 0535-0546, which consists of a comparison of the bolometric luminosities ...

Luhman, K L; Brandner, W; Skrutskie, M F; Nelson, M J; Smith, J D; Peterson, D E; Cushing, M C; Young, E

2006-01-01T23:59:59.000Z

99

Edmund G. Brown Jr. LIFE HISTORY PARAMETERS OF  

E-Print Network [OSTI]

History Parameters of Common Marine Fish Subject to Entrainment. California Energy Commission, PIER · Renewable Energy Technologies · Transportation Life History Parameters of Common Southern California MEdmund G. Brown Jr. Governor LIFE HISTORY PARAMETERS OF COMMON SOUTHERN CALIFORNIA MARINE FISHES

100

Molecular insights into the niche of harmful brown tides  

E-Print Network [OSTI]

Recurrent brown tide blooms caused by the harmful alga Alureococcus anophagefferens have decimated coastal ecosystems and shellfisheries along the Eastern U.S and South Africa. The exact mechanisms controlling bloom ...

Wurch, Louie L. (Louie Lorne)

2011-01-01T23:59:59.000Z

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


101

Chemical Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

environments. Courses in mathematics, chemistry, physics, and computational engineering provide the background120 Chemical Engineering The George R. Brown School of Engineering Chair Kyriacos Zygourakis to create a focus area in one of the following four disciplines: bioengineering, environmental engineering

Richards-Kortum, Rebecca

102

Genome sequence of the Brown Norway rat yields insights into  

E-Print Network [OSTI]

Genome sequence of the Brown Norway rat yields insights into mammalian evolution Rat Genome Norway (BN) rat strain. The sequence represents a high-quality `draft' covering over 90% of the genome

Pachter, Lior

103

Quiescent X-ray emission from an evolved brown dwarf ?  

E-Print Network [OSTI]

I report on the X-ray detection of Gl569Bab. During a 25ksec Chandra observation the binary brown dwarf is for the first time spatially separated in X-rays from the flare star primary Gl569A. Companionship to Gl569A constrains the age of the brown dwarf pair to ~300-800 Myr. The observation presented here is only the second X-ray detection of an evolved brown dwarf. About half of the observing time is dominated by a large flare on Gl569Bab, the remainder is characterized by weak and non-variable emission just above the detection limit. This emission -- if not related to the afterglow of the flare -- represents the first detection of a quiescent corona on a brown dwarf, representing an important piece in the puzzle of dynamos in the sub-stellar regime.

B. Stelzer

2004-09-27T23:59:59.000Z

104

Edmund G. Brown, Jr. PIER INDUSTRIAL, AGRICULTURAL, AND  

E-Print Network [OSTI]

, petroleum refining, natural gas, beverage industry, water and wastewater, energy efficiency, industrial natural gas efficiency, electronics, Public Interest Energy R Edmund G. Brown, Jr. Governor PIER INDUSTRIAL, AGRICULTURAL, AND WATER ENERGY EFFICIENCY

105

Intern experience at Brown & Root, Inc.: an internship report  

E-Print Network [OSTI]

. The internship report outlines the process by which Brown & Root carries out the design and construction of offshore oil and gas production facilities ... A supplementary presentation of the author's previous experience at an oil company permits...

Kibbee, Stephen Edward, 1951-

2013-03-13T23:59:59.000Z

106

atmospheric brown cloud: Topics by E-print Network  

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

I.; Burrows, Adam 2003-01-01 3 II. Black Carbon, Atmospheric Brown Clouds and Greenhouse Effect: Background CiteSeer Summary: satellite. The optical depth is a good index for...

107

atmospheric brown clouds: Topics by E-print Network  

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

I.; Burrows, Adam 2003-01-01 3 II. Black Carbon, Atmospheric Brown Clouds and Greenhouse Effect: Background CiteSeer Summary: satellite. The optical depth is a good index for...

108

Correlated spectral variability in brown dwarfs  

E-Print Network [OSTI]

Models of brown dwarf atmospheres suggest they exhibit complex physical behaviour. Observations have shown that they are indeed dynamic, displaying small photometric variations over timescales of hours. Here I report results of infrared (0.95-1.64 micron) spectrophotometric monitoring of four field L and T dwarfs spanning timescales of 0.1-5.5 hrs, the goal being to learn more about the physical nature of this variability. Spectra are analysed differentially with respect to a simultaneously observed reference source in order to remove Earth-atmospheric variations. The variability amplitude detected is typically 2-10%, depending on the source and wavelength. I analyse the data for correlated variations between spectral indices. This approach is more robust than single band or chisq analyses, because it does not assume an amplitude for the (often uncertain) noise level (although the significance test still assumes a shape for the noise power spectrum). Three of the four targets show significant evidence for correlated variability. Some of this can be associated with specific features including Fe, FeH, VO and KI, and there is good evidence for intrinsic variability in water and possibly also methan. Yet some of this variability covers a broader spectral range which would be consistent with dust opacity variations. The underlying common cause is plausibly localized temperature or composition fluctuations caused by convection. Looking at the high signal-to-noise ratio stacked spectra we see many previously identified spectral features of L and T dwarfs, such as KI, NaI, FeH, water and methane. In particular we may have detected methane absorption at 1.3-1.4 micron in the L5 dwarf SDSS 0539-0059.

C. A. L. Bailer-Jones

2007-11-28T23:59:59.000Z

109

FIRE Diagnostics Kenneth M. Young  

E-Print Network [OSTI]

FIRE Diagnostics Kenneth M. Young Princeton Plasma Physics Laboratory Workshop on Physics Issues. Young 5/2/00 #12;FIRE: Diagnostics Schedule 1 2YEAR 3 4 5 6 7 8 9 10 11 12 16151413 First Plasma Vac for FIRE PPPL May 1 - 3, 2000 #12;Role for the Plasma Measurements · 1) Provide data for physics studies

110

COOL YOUNG STARS IN THE NORTHERN HEMISPHERE: {beta} PICTORIS AND AB DORADUS MOVING GROUP CANDIDATES  

SciTech Connect (OSTI)

As part of our continuing effort to identify new, low-mass members of nearby, young moving groups (NYMGs), we present a list of young, low-mass candidates in the northern hemisphere. We used our proven proper-motion selection procedure and ROSAT X-ray and GALEX-UV activity indicators to identify 204 young stars as candidate members of the {beta} Pictoris and AB Doradus NYMGs. Definitive membership assignment of a given candidate will require a measurement of its radial velocity and distance. We present a simple system of indices to characterize the young candidates and help prioritize follow-up observations. New group members identified in this candidate list will be high priority targets for (1) exoplanet direct imaging searches, (2) the study of post-T-Tauri astrophysics, (3) understanding recent local star formation, and (4) the study of local galactic kinematics. Information available now allows us to identify eight likely new members in the list. Two of these, a late-K and an early-M dwarf, we find to be likely members of the {beta} Pic group. The other six stars are likely members of the AB Dor moving group. These include an M dwarf triple system, and three very cool objects that may be young brown dwarfs, making them the lowest-mass, isolated objects proposed in the AB Dor moving group to date.

Schlieder, Joshua E.; Simon, Michal [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (United States); Lepine, Sebastien, E-mail: michal.simon@stonybrook.edu, E-mail: schlieder@mpia-hd.mpg.de, E-mail: lepine@amnh.org [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States)

2012-04-15T23:59:59.000Z

111

Batch sorption of divalent metal ions onto brown coal  

SciTech Connect (OSTI)

Brown coal, a relatively abundant and inexpensive material is currently being investigated as an adsorbent to remove some contaminants from aqueous solution. The adsorption of some heavy metals from aqueous solutions on the brown coals was studied as a function of pH, contact time, adsorbent dosage and concentration of metal solutions. A carboxyl, phenolic hydroxyl, and metoxyl functional group present on the coal surface was the adsorption site to remove metal ions from solution by means of ion exchange and hydrogen bonding. Effective removal of heavy metals was achieved at pH values of 4.0-5.0. The experimental data have been analyzed using the Langmuir isotherm models. Under optimized conditions, the percentage of metal removal by brown coal adsorption was over 80%.

Pehlivan, E.; Gode, F. [University of Selcuk, Konya (Turkey). Faculty of Engineering & Architecture

2006-12-15T23:59:59.000Z

112

2001 7: 1566-1577RNA J. T. Brown and A. W. Johnson  

E-Print Network [OSTI]

2001 7: 1566-1577RNA J. T. Brown and A. W. Johnson and phenocopies a ski mutant cellsenhances cells and phenocopies a ski mutant JUSTIN T. BROWN and ARLEN W. JOHNSON Department of Molecular Genetics

Johnson, Arlen

113

Toward Systems Biology in Brown Algae to Explore Acclimation and Adaptation to the Shore Environment  

E-Print Network [OSTI]

Toward Systems Biology in Brown Algae to Explore Acclimation and Adaptation to the Shore,2 Catherine Boyen,1,2 and Anne Siegel4,5 Abstract Brown algae belong to a phylogenetic lineage distantly siliculosus as a model organism for brown algae has represented a framework in which several omics techniques

Paris-Sud XI, Université de

114

Red ribbon and brown boots: becoming an agrarian girl.  

E-Print Network [OSTI]

??The essays and poems in this collection come together to create a portrait of place, the upper Midwest of my childhood and young adult years.… (more)

Romkema, Erica Joy

2009-01-01T23:59:59.000Z

115

Edmund G. Brown, Jr. ENERGY-EFFICIENT COMMUNITY  

E-Print Network [OSTI]

's provided structure-specific building plans. The alternative energy efficiency approaches are; "EE Package" design approach incorporating advanced energy efficiency measures including alternative grades of wall andEdmund G. Brown, Jr. Governor ENERGY-EFFICIENT COMMUNITY DEVELOPMENT IN CALIFORNIA: CHULA VISTA

116

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

145 Computer Science The George R. Brown School of Engineering Chair Keith Cooper Professors Robert Tour researCh Professor Peter Druschel #12;146 Departments/ Computer Science Eight courses for a total Intermediate Programming COMP 280 Mathematics of Computer Science COMP 314 Applied Algorithms and Data

Richards-Kortum, Rebecca

117

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

139 Computer Science The George R. Brown School of Engineering Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science is concerned with the study of computers and computing, focusingonalgorithms to real-world computational problems. Computer science is the intellectual discipline underlying

Richards-Kortum, Rebecca

118

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

145 Computer Science The George R. Brown School of Engineering Chair Keith Cooper Professors Robert Chemistry) Professor James Tour #12;146 DEPARTMENTS / Computer Science Computer science is concerned to produce solutions to real-world computational problems. Computer science is the intellectual discipline

Richards-Kortum, Rebecca

119

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

141 Computer Science The George R. Brown School of Engineering Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science is concerned with the study of computers and computing, focusingonalgorithmsTour #12;142 DEPARTMENTS/ Computer Science body of knowledge can be used to produce solutions to real

Richards-Kortum, Rebecca

120

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

153 Computer Science The George R. Brown School of Engineering Chair Joe Warren Professors Robert S'Malley with Chemistry Professor James Tour researCh Professor Peter Druschel #12;154 Departments/ Computer Science Six Matrix Analysis Math and Science Courses Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science

Richards-Kortum, Rebecca

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


121

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

Computer Science The George R. Brown School of Engineering Chair Joe D. Warren Professors Robert S researCh Professor Peter Druschel #12;2 Departments/ Computer Science Six courses for a total of 18 hours Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science is concerned with the study of computers

Richards-Kortum, Rebecca

122

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

1 Computer Science The George R. Brown School of Engineering Chair Joe Warren Professors Robert S #12;2 Departments/ Computer Science Six courses for a total of 18 hours, required for all majors, MS, and PhD Computer science is concerned with the study of computers and computing

Richards-Kortum, Rebecca

123

Computer Science The George R. Brown School of Engineering  

E-Print Network [OSTI]

135 Computer Science The George R. Brown School of Engineering Chair Moshe Y. Vardi Professors Science Computer science is concerned with the study of computers and computing, focusing on algorithms. Computer science is the intellectual discipline underlying information technology, which is widely accepted

Richards-Kortum, Rebecca

124

Air Traffic Control Using Virtual Stationary Automata Matthew D. Brown  

E-Print Network [OSTI]

Air Traffic Control Using Virtual Stationary Automata by Matthew D. Brown B.S., Massachusetts by . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Arthur C. Smith Chairman, Department Committee on Graduate Students #12;Air Traffic Control Using Virtual of Engineering Abstract As air travel has become an essential part of modern life, the air traffic control system

Lynch, Nancy

125

Novel Dipole Trapped Spheromak Configuration M. R. Brown,1,  

E-Print Network [OSTI]

Novel Dipole Trapped Spheromak Configuration M. R. Brown,1, * C. D. Cothran,1 J. Fung,1 M. J. Schaffer,2 and E. Belova3 We report the observation and characterization of a spheromak formed in the Swarthmore Spheromak Experiment (SSX) and trapped in a simple dipole magnetic field. The spheromak is studied

Brown, Michael R.

126

SSX Spheromak Merging Experiment Michael Brown, Swarthmore, PI  

E-Print Network [OSTI]

SSX Spheromak Merging Experiment Michael Brown, Swarthmore, PI Scientific Goals: We have three main gun technique to form single spheromaks and merged pairs of spheromaks to study novel magnetic configurations. A single spheromak can be injected into a flux conserver and stabilized with a simple dipole

Brown, Michael R.

127

Join us for this"bonus" brown bag seminar,  

E-Print Network [OSTI]

policy. He also is the founding director of the Renewable and Appropriate Energy Laboratory (RAELJoin us for this"bonus" brown bag seminar, sponsored by the National Renewable Energy Laboratory link to Golden,Colorado. Topics focus on new and innovative renewable energy and energy analysis

Kammen, Daniel M.

128

Chemical Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

environments. Courses in mathematics, chemistry, physics, and computational engineering provide the background/312 Physical Chemistry Any 2 of CHEM 212, CHEM 311, or CHEM 312 Chemical Engineering CENG 301 Chemical110 Chemical Engineering The George R. Brown School of Engineering Chair Kyriacos Zygourakis

Richards-Kortum, Rebecca

129

Software Reuse in High Performance Computing Shirley Browne  

E-Print Network [OSTI]

Software Reuse in High Performance Computing Shirley Browne University of Tennessee 107 Ayres Hall high performance computing architectures in the form of distributed memorymul- tiprocessors have become of programming applications to run on these machines. Economical use of high performance computing and subsequent

Hawick, Ken

130

Software Reuse in High Performance Computing Shirley Browne  

E-Print Network [OSTI]

Software Reuse in High Performance Computing Shirley Browne University of Tennessee 107 Ayres Hall high performance computing architectures in the form of distributed memory mul­ tiprocessors have and cost of programming applications to run on these machines. Economical use of high performance computing

Dongarra, Jack

131

PLEASE JOIN US! NANOSCIENCE and TECHNOLOGY BROWN BAG  

E-Print Network [OSTI]

PLEASE JOIN US! NANOSCIENCE and TECHNOLOGY BROWN BAG Friday, 7 November 2008 Noon - 1 pm Columbia Meyyappan Chief Scientist for Exploration Technology, NASA Ames Research Center & IEEE Electron Devices Society Distinguished Lecturer presenting Nanotechnology in Chemical and Bio Sensor Systems Abstract

132

INDIUM--1997 37.1 By Robert D. Brown, Jr.  

E-Print Network [OSTI]

INDIUM--1997 37.1 INDIUM By Robert D. Brown, Jr. There was no known production of indium at domestic mines, and none was recovered from ores in the United States in 1997. Domestic indium production and Rhode Island, were the major producers of indium metal and indium products in 1997. Several smaller

133

Brown Dwarfs as Ejected Stellar Embryos: Observational Perspectives  

E-Print Network [OSTI]

We discuss a scenario in which brown dwarfs are formed like stars, except that their full collapse phases are interrupted through dynamical interactions in small multiple systems, leading to the ejection of the lightest member. This disintegration is a stochastic process, often resulting in the expulsion of newborn low mass stars, but when it occurs early enough the ejected stellar embryo will be a substellar object. This process may be so common at early ages that a large fraction of the ubiquitous brown dwarfs could have formed in this manner. Detailed gas dynamical simulations are required in order to better understand the details of the decay of small newborn multiple systems. We discuss the observational consequences of the ejection hypothesis, noting especially the importance of binaries with brown dwarf components as an observational test. Finally, we note that brown dwarfs that have recently been ejected may be so disturbed, by infall from the collapsing core and also by heavy accretion from perturbed circumstellar disks, that traditional spectral and luminosity criteria may fail to identify their substellar nature.

Bo Reipurth; Cathie Clarke

2002-08-31T23:59:59.000Z

134

Edmund G. Brown, Jr. ENERGY-EFFICIENT COMMUNITY  

E-Print Network [OSTI]

Commission Elaine Hebert Project Manager Chris Scruton Program Area Lead Buildings Energy End-Use Efficiency Remp ­ City of Chula Vista, California · Larisa Dobriansky ­ National Energy Center for SustainableEdmund G. Brown, Jr. Governor ENERGY-EFFICIENT COMMUNITY DEVELOPMENT IN CALIFORNIA: CHULA VISTA

135

Edmund G. Brown, Jr. FUEL CELL AND DISTRIBUTED  

E-Print Network [OSTI]

Edmund G. Brown, Jr. Governor FUEL CELL AND DISTRIBUTED GENERATION RESEARCH, DEVELOPMENT Research Program Prepared By: National Fuel Cell Research Center August 2011 CEC-500-2011-042 #12; Prepared By: National Fuel Cell Research Center Project Manager: G. Scott Samuelsen, Ph.D. Authors: Josh

136

Astronomy Advisory Panel Richard Bower, Michael Brown, Anthony  

E-Print Network [OSTI]

Astronomy Advisory Panel Richard Bower, Michael Brown, Anthony Challinor, Chris Evans, Paul O to provide large contracts for UK industry. · High Performance Computing access ­ fund hardware upgrades via over 10 years Many UK science areas: dark energy/matter, galactic structure, transients, solar system

Crowther, Paul

137

SHORT COMMUNICATION Behaviour of brown bears killing wild ungulates  

E-Print Network [OSTI]

SHORT COMMUNICATION Behaviour of brown bears killing wild ungulates in the Cantabrian Mountains documentation regarding bear predation on wild ungulates in Southern Europe. We describe search, detection wild boar by a female bear with cubs surprised by a sudden encounter. They did not eat the boar after

Boyer, Edmond

138

Molecular Selectivity of Brown Carbon Chromophores Julia Laskin,*,  

E-Print Network [OSTI]

, Irvine, California 92697, United States Chemical Sciences Division, Lawrence Berkeley National into imines mediated by NH3 vapors in humid air, resulted in selective browning of the LSOA sample, while the PSOA sample remained white. Comparative analysis of the reaction products in the aged LSOA and PSOA

Nizkorodov, Sergey

139

Hydroliquefaction of Big Brown lignite in supercritical fluids  

E-Print Network [OSTI]

Big Brown lignite was liquefied in a fixed bed tube reactor. Three solvents were used in the liquefaction studies, toluene, cyclohexane and methanol. Two co-solvents, tetralin and water were used with toluene. The effects of the solvents and co...

Chen, Hui

1996-01-01T23:59:59.000Z

140

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES  

E-Print Network [OSTI]

#12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 33, Part 1 CONTENTS Tertiary Geologic History Geology of the Deadman Canyon 7112-Minute Quadrangle, Carbon County, Utah, Utah. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .James Douglas Smith 135 Geology

Seamons, Kent E.

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


141

AA Dor - An Eclipsing sdOB - Brown Dwarf Binary  

E-Print Network [OSTI]

AA Dor is an eclipsing, close, post common-envelope binary consisting of a sdOB primary star and an unseen secondary with an extraordinary small mass - formally a brown dwarf. The brown dwarf may have been a former planet which survived a common envelope phase and has even gained mass. A recent determination of the components' masses from results of NLTE spectral analysis and subsequent comparison to evolutionary tracks shows a discrepancy to masses derived from radial-velocity and the eclipse curves. Phase-resolved high-resolution and high-SN spectroscopy was carried out in order to investigate on this problem. We present results of a NLTE spectral analysis of the primary, an analysis of its orbital parameters, and discuss possible evolutionary scenarios.

Thomas Rauch

2003-11-25T23:59:59.000Z

142

Intern experience at Teledyne Brown Engineering: an internship report  

E-Print Network [OSTI]

-Value Attack and Defense Effectiveness Model MX Missile X NASA National Aeronautics and Space Agency OPUS Optimal Preferential Utilities and Strategies Program OR Operations Research O&S Operations and Support PBV Post Boost Vehicle P.E. Professional... under decentralized management and strong local autonomy. In addition to its main facilities in Huntsville's Cummings Research Park, Teledyne Brown Engineering has branch operations at the Huntsville-Madison County Airport and in California, Colorado...

Hammond, Walter Edward, 1947-

2013-03-13T23:59:59.000Z

143

Engineering internship at Brown & Root, Incorporated: a report  

E-Print Network [OSTI]

A Report by RANDALL JOE GANNAWAY Submitted to the College of Engineering Texas A&M University in partial fulfillment of the requirement for the degree DOCTOR OF ENGINEERING December 1977 Major Subjects Industrial Engineering A Report... e of Engineering) W. Smith (Member) December 1977 A Report on an Engineering Internship at Brown & Root, Incorporated. (December 1977) Randall Joe Gannaway, B.S., Texas A&M University; M.E., Texas A&M University Co-Chairmen of Advisory...

Gannaway, Randall Joe, 1952-

2013-03-13T23:59:59.000Z

144

ATMOSPHERIC DYNAMICS OF BROWN DWARFS AND DIRECTLY IMAGED GIANT PLANETS  

SciTech Connect (OSTI)

A variety of observations provide evidence for vigorous motion in the atmospheres of brown dwarfs and directly imaged giant planets. Motivated by these observations, we examine the dynamical regime of the circulation in the atmospheres and interiors of these objects. Brown dwarfs rotate rapidly, and for plausible wind speeds, the flow at large scales will be rotationally dominated. We present three-dimensional, global, numerical simulations of convection in the interior, which demonstrate that at large scales, the convection aligns in the direction parallel to the rotation axis. Convection occurs more efficiently at high latitudes than low latitudes, leading to systematic equator-to-pole temperature differences that may reach ?1 K near the top of the convection zone. The interaction of convection with the overlying, stably stratified atmosphere will generate a wealth of atmospheric waves, and we argue that, as in the stratospheres of planets in the solar system, the interaction of these waves with the mean flow will cause a significant atmospheric circulation at regional to global scales. At large scales, this should consist of stratified turbulence (possibly organizing into coherent structures such as vortices and jets) and an accompanying overturning circulation. We present an approximate analytic theory of this circulation, which predicts characteristic horizontal temperature variations of several to ?50 K, horizontal wind speeds of ?10-300 m s{sup –1}, and vertical velocities that advect air over a scale height in ?10{sup 5}-10{sup 6} s. This vertical mixing may help to explain the chemical disequilibrium observed on some brown dwarfs. Moreover, the implied large-scale organization of temperature perturbations and vertical velocities suggests that near the L/T transition, patchy clouds can form near the photosphere, helping to explain recent observations of brown-dwarf variability in the near-IR.

Showman, Adam P. [Department of Planetary Sciences and Lunar and Planetary Laboratory, The University of Arizona, 1629 University Boulevard, Tucson, AZ 85721 (United States); Kaspi, Yohai, E-mail: showman@lpl.arizona.edu [Center for Planetary Science, Weizmann Institute of Science, Rehovot (Israel)

2013-10-20T23:59:59.000Z

145

A review of "Thomas Browne" edited by Kevin Killeen  

E-Print Network [OSTI]

marks an important contribution to the revival of interest in a writer whose work, while long admired, had been largely relegated by the academy to the category of literary curiosity (according to the editors of Sir Thomas Browne: The World Proposed... unto me at nights till she read them all out” (in Keynes (ed.), Miscellaneous Writings (1931), 295–96). Recent work on book and reading history has made such documents far more interesting than they were once considered, and this (rather dauntingly...

Black, Joseph L.

2015-01-01T23:59:59.000Z

146

YOUNG GEOLOGY GEOLOGY OF THE  

E-Print Network [OSTI]

YOUNG GEOLOGY UNIVERSITY May, 1962 GEOLOGY OF THE SOUTHERN WASATCH MOUNTAINS AND VICIN~IM,UTAH C O ....................J. Keith Rigby 80 Economic Geology of North-Central Utah ...,............... Kcnneth C.Bdodc 85 Rod Log ........................Lehi F. Hintze, J. Ka# Ri&, & ClydeT. Hardy 95 Geologic Map of Southern

Seamons, Kent E.

147

SCOPE-Zhongyu Young Scientist  

E-Print Network [OSTI]

and research on best management practices. The Scientific Committee on Problems of the Environment (SCOPESCOPE-Zhongyu Young Scientist Environmental Awards 2011 The SCOPE-Zhongyu Environmental Awards were to the improvement of the world environment through promotion of environmental sciences, technological advances

Wang, Wei Hua

148

Young Supernova Remnants: Issues and Prospects  

E-Print Network [OSTI]

After reviewing recent work on the dynamics of young supernova remnants (YSNRs) and discussing how YSNRs can be used as physics laboratories, I discuss several challenges: Where are the very young SNRs in the Galaxy? Can very young SNRs produce gamma ray bursts? The Connections Challenge: Can one infer the nature of the supernova and its progenitor star from observations of the YSNR?

Christopher F. McKee

2001-01-03T23:59:59.000Z

149

E-Print Network 3.0 - arctic endemic brown Sample Search Results  

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

results for: arctic endemic brown Page: << < 1 2 3 4 5 > >> 1 Southeast Alaska Conservation Assessment -Chapter 6.7 Page 1 Endemic Mammals of the Alexander Archipelago...

150

THE BROWN DWARF KINEMATICS PROJECT (BDKP). III. PARALLAXES FOR 70 ULTRACOOL DWARFS  

SciTech Connect (OSTI)

We report parallax measurements for 70 ultracool dwarfs (UCDs) including 11 late-M, 32 L, and 27 T dwarfs. In this sample, 14 M and L dwarfs exhibit low surface gravity features, 6 are close binary systems, and 2 are metal-poor subdwarfs. We combined our new measurements with 114 previously published UCD parallaxes and optical-mid-IR photometry to examine trends in spectral-type/absolute magnitude, and color-color diagrams. We report new polynomial relations between spectral type and M{sub JHK}. Including resolved L/T transition binaries in the relations, we find no reason to differentiate between a 'bright' (unresolved binary) and a 'faint' (single source) sample across the L/T boundary. Isolating early T dwarfs, we find that the brightening of T0-T4 sources is prominent in M{sub J} where there is a [1.2-1.4] mag difference. A similar yet dampened brightening of [0.3-0.5] mag happens at M{sub H} and a plateau or dimming of [-0.2 to -0.3] mag is seen in M{sub K} . Comparison with evolutionary models that vary gravity, metallicity, and cloud thickness verifies that for L into T dwarfs, decreasing cloud thickness reproduces brown dwarf near-IR color-magnitude diagrams. However we find that a near constant temperature of 1200 {+-}100 K along a narrow spectral subtype of T0-T4 is required to account for the brightening and color-magnitude diagram of the L-dwarf/T-dwarf transition. There is a significant population of both L and T dwarfs which are red or potentially 'ultra-cloudy' compared to the models, many of which are known to be young indicating a correlation between enhanced photospheric dust and youth. For the low surface gravity or young companion L dwarfs we find that 8 out of 10 are at least [0.2-1.0] mag underluminous in M{sub JH} and/or M{sub K} compared to equivalent spectral type objects. We speculate that this is a consequence of increased dust opacity and conclude that low surface gravity L dwarfs require a completely new spectral-type/absolute magnitude polynomial for analysis.

Faherty, Jacqueline K.; Shara, Michael M.; Cruz, Kelle L. [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10034 (United States); Burgasser, Adam J. [Center of Astrophysics and Space Sciences, Department of Physics, University of California, San Diego, CA 92093 (United States); Walter, Frederick M. [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800 (United States); Van der Bliek, Nicole [CTIO/National Optical Astronomy Observatory (Chile); West, Andrew A. [Department of Astronomy, Boston University, 725 Commonwealth Ave Boston, MA 02215 (United States); Vrba, Frederick J. [US Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002 (United States); Anglada-Escude, Guillem, E-mail: jfaherty@amnh.org [Department of Terrestrial Magnetism, Carnegie Institution of Washington 5241 Broad Branch Road, NW, Washington, DC 20015 (United States)

2012-06-10T23:59:59.000Z

151

Controlling Brown Stomach Worms in Cattle by Management  

E-Print Network [OSTI]

environment in the stomach for worms. Overcrowding and overgrazing pasture lead to poor nutrition of cattle and to poor sanita- tion. Excess manure and worm larvae contami- nate the pasture. Rain is needed to wash the larvae from the manure onto pasture where.... eggs passed in their manure become a con- tinual source of pasture contamination during the spring if weekly rains occur to wash the larvae from manure. To ensure cattle maintain noneconomic, low levels of brown stomach worms, feed a protein supplement...

Faries Jr., Floron C.

2002-02-05T23:59:59.000Z

152

Time resolved spectroscopy of the variable brown dwarf Kelu-1  

E-Print Network [OSTI]

We report the results of observations designed to investigate the spectroscopic signatures of dust clouds on the L2 brown dwarf Kelu-1. Time resolved medium resolution spectra show no significant evidence of variability in the dust sensitive TiO, CrH and FeH bandheads on the timescale of 1--24 hours. We do however report periodic variability in the psuedo-equivelent width of H-alpha consistent with the 1.8 hour rotation period previously reported for this object Clarke, Tinney & Tolley (2002). Near-contemporaneous I-band photometry shows evidence for non-periodic variability at the level of 2%.

F. J. Clarke; C. G. Tinney; S. T. Hodgkin

2003-01-09T23:59:59.000Z

153

Observations on the biology of the smoky brown cockroach  

E-Print Network [OSTI]

. Of these, fresh apple, brown sugar, wet dehydrated potato, and wet powdered milk were most preferred. Seven types of materials were tested for preference by the roach as resting surface sites. In descending order of preference, these were concrete... cockroach had not been reported before 1940 (Gould and Deay 1940a). This study was very scanty in that only a small number of roaches were used. Thus the need existed for an extensive investigation of the:life history of this species. A number of food...

Clark, Jerry Lee

1970-01-01T23:59:59.000Z

154

Brown County, Texas: 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 Home5b9fcbce19 NoPublic Utilities Address: 160Benin: EnergyBoston Areais a village in CookEnergyBrookwood,Illinois.Brown County,

155

Brown County, Wisconsin: 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 Home5b9fcbce19 NoPublic Utilities Address: 160Benin: EnergyBoston Areais a village in CookEnergyBrookwood,Illinois.Brown

156

The Tropical Brown Alga Lobophora variegata (Lamouroux) Womersley: A Prospective Bioindicator for Ag Contamination in Tropical Coastal Waters  

E-Print Network [OSTI]

The Tropical Brown Alga Lobophora variegata (Lamouroux) Womersley: A Prospective Bioindicator determined in the brown alga Lobophora variegata, using radiotracer techniques. Results indicate that this widely distributed alga could be a useful bioindicator species for surveying silver contamination

Paris-Sud XI, Université de

157

Optical Flow Estimation using Laplacian Mesh Energy Wenbin Li Darren Cosker Matthew Brown Rui Tang  

E-Print Network [OSTI]

Optical Flow Estimation using Laplacian Mesh Energy Wenbin Li Darren Cosker Matthew Brown Rui Tang.p.cosker,m.brown,r.tang}@bath.ac.uk Abstract In this paper we present a novel non-rigid optical flow algorithm for dense image correspondence and non-rigid registration. The algorithm uses a unique Laplacian Mesh Energy term to encourage local

Martin, Ralph R.

158

Pollution-induced behavioural effects in the brown bullhead (Ameiurus nebulosus)  

E-Print Network [OSTI]

Pollution-induced behavioural effects in the brown bullhead (Ameiurus nebulosus) Ross D. Breckels on biodiversity. Thus, it is important to understand the nature of pollution- induced change in aquatic ecosystems. We show that brown bullheads (Ameiurus nebulosus) may have evolved in response to chronic pollution

Neff, Bryan D.

159

Anaerobic Co-digestion of Brown Water and Food Waste for Energy Recovery  

E-Print Network [OSTI]

waste. Keywords Anaerobic digestion; food waste; brown water; biogas; co-digestion INTRODUCTION-cal/m3 , biogas has been widely used in heating digesters and gas engines (Wang et al., 2007LIM J.W. Anaerobic Co-digestion of Brown Water and Food Waste for Energy Recovery Jun Wei LIM

Paris-Sud XI, Université de

160

Capping the Brown Energy Consumption of Internet Services at Low Cost  

E-Print Network [OSTI]

Capping the Brown Energy Consumption of Internet Services at Low Cost Kien T. Le Ricardo Bianchini Consumption of Data Centers 0 20 40 60 80 100 120 140 2000 2006 2011 Electricity consumption of US DCs Billion Energy Consumption · Improving efficiency does not promote green energy or guarantee limits on brown

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


161

Capping the Brown Energy Consumption of Internet Services at Low Cost  

E-Print Network [OSTI]

energy" (produced via carbon-intensive means) relative to renewable or "green" energy. This paper their brown energy consumption and lever- age green energy, while respecting their SLAs and minimizing energy-intensive energy as "brown" energy, in contrast with "green" or renewable energy.) We argue that placing caps

162

A review of "Sir Thomas Browne: A Life" by Reid Barbour  

E-Print Network [OSTI]

26) cites recent scholarship (1998-99) that refutes this early nineteenth-century orthodoxy. Right from the start Barbour enters Browne’s world of words in portraying that life as a “miracle,” a “fable” or “peece of Poetry.” From 1637, after...

Todd, Richard

2014-01-01T23:59:59.000Z

163

PPl 15: The First Brown Dwarf Spectroscopic Binary  

E-Print Network [OSTI]

PPl 15 is the first object to have been confirmed as a brown dwarf by the lithium test (in 1995), though its inferred mass was very close to the substellar limit. It is a member of the Pleiades open cluster. Its position in a cluster color-magnitude diagram suggested that it might be binary, and preliminary indications that it is a double-lined spectroscopic binary were reported by us in 1997. Here we report on the results of a consecutive week of Keck HIRES observations of this system, which yield its orbit. It has a period of about 5.8 days, and an eccentricity of 0.4+/-0.05. The rotation of the stars is slow for this class of objects. Because the system luminosity is divided between 2 objects with a mass ratio of 0.85, this renders each of them an incontrovertible brown dwarf, with masses between 60-70 jupiters. We show that component B is a little redder than A by studying their wavelength-dependent line ratios, and that this variation is compatible with the mass ratio. We confirm that the system has lithium, but cannot support the original conclusion that it is depleted (which would be surprising, given the new masses). This is a system of very close objects which, if they had combined, would have produced a low mass star. We discuss the implications of this discovery for the theories of binary formation and formation of very low mass objects.

Gibor Basri; Eduardo Martin

1999-08-02T23:59:59.000Z

164

PPl 15 The First Brown Dwarf Spectroscopic Binary  

E-Print Network [OSTI]

PPl 15 is the first object to have been confirmed as a brown dwarf by the lithium test (in 1995), though its inferred mass was very close to the substellar limit. It is a member of the Pleiades open cluster. Its position in a cluster color-magnitude diagram suggested that it might be binary, and preliminary indications that it is a double-lined spectroscopic binary were reported by us in 1997. Here we report on the results of a consecutive week of Keck HIRES observations of this system, which yield its orbit. It has a period of about 5.8 days, and an eccentricity of 0.4+/-0.05. The rotation of the stars is slow for this class of objects. Because the system luminosity is divided between 2 objects with a mass ratio of 0.85, this renders each of them an incontrovertible brown dwarf, with masses between 60-70 jupiters. We show that component B is a little redder than A by studying their wavelength-dependent line ratios, and that this variation is compatible with the mass ratio. We confirm that the system has lith...

Basri, G S; Basri, Gibor; Martin, Eduardo

1999-01-01T23:59:59.000Z

165

Rheological properties of water-coal slurries based on brown coal in the presence of sodium lignosulfonates and alkali  

SciTech Connect (OSTI)

The effect of the oxidized surface of brown coal on the structural and rheological properties of water-coal slurries was found. The kinetics of structure formation processes in water-coal slurries based on as-received and oxidized brown coal was studied. The effect of lignosulfonate and alkali additives on the samples of brown coal was considered.

D.P. Savitskii; A.S. Makarov; V.A. Zavgorodnii [National Academy of Sciences of Ukraine, Kiev (Ukraine). Dumanskii Institute of Colloid and Water Chemistry

2009-07-01T23:59:59.000Z

166

The Brown-dwarf Atmosphere Monitoring (BAM) Project II: Multi-epoch monitoring of extremely cool brown dwarfs  

E-Print Network [OSTI]

With the discovery of Y dwarfs by the WISE mission, the population of field brown dwarfs now extends to objects with temperatures comparable to those of Solar System planets. To investigate the atmospheres of these newly identified brown dwarfs, we have conducted a pilot study monitoring an initial sample of three late T-dwarfs (T6.5, T8 and T8.5) and one Y-dwarf (Y0) for infrared photometric variability at multiple epochs. With J-band imaging, each target was observed for a period of 1.0h to 4.5h per epoch, which covers a significant fraction of the expected rotational period. These measurements represent the first photometric monitoring for these targets. For three of the four targets (2M1047, Ross 458C and WISE0458), multi-epoch monitoring was performed, with the time span between epochs ranging from a few hours to ~2 years. During the first epoch, the T8.5 target WISE0458 exhibited variations with a remarkable min-to-max amplitude of 13%, while the second epoch light curve taken ~2 years later did not not...

Rajan, A; Wilson, P A; Bulger, J; De Rosa, R J; Ward-Duong, K; Morley, C; Pont, F; Windhorst, R

2015-01-01T23:59:59.000Z

167

THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF GIANT PLANETS AROUND YOUNG B AND A STARS  

SciTech Connect (OSTI)

We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (?1.5-2.5 M{sub ?}) conducted to date and includes the planet hosts ? Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58{sup +21}{sub -20} M{sub Jup} and 55{sup +20}{sub -19} M{sub Jup}, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M{sub ?} stars can have giant planets greater than 4 M{sub Jup} between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M{sub Jup} between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M{sub Jup}, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.

Nielsen, Eric L.; Liu, Michael C.; Chun, Mark; Ftaclas, Christ [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Wahhaj, Zahed [European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago (Chile); Biller, Beth A. [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg (Germany); Hayward, Thomas L.; Hartung, Markus [Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena (Chile); Close, Laird M.; Males, Jared R.; Skemer, Andrew J. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Alencar, Silvia H. P. [Departamento de Fisica, ICEx, Universidade Federal de Minas Gerais, Av. Antonio Carlos 6627, 30270-901 Belo Horizonte, MG (Brazil); Artymowicz, Pawel [University of Toronto at Scarborough, 1265 Military Trail, Toronto, Ontario M1C 1A4 (Canada); Boss, Alan [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, DC 20015 (United States); Clarke, Fraser [Department of Astronomy, University of Oxford, DWB, Keble Road, Oxford OX1 3RH (United Kingdom); De Gouveia Dal Pino, Elisabete; Gregorio-Hetem, Jane [Departamento de Astronomia, Universidade de Sao Paulo, IAG/USP, Rua do Matao 1226, 05508-900 Sao Paulo, SP (Brazil); Ida, Shigeru [Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8550 (Japan); Kuchner, Marc [NASA Goddard Space Flight Center, Exoplanets and Stellar Astrophysics Laboratory, Greenbelt, MD 20771 (United States); Lin, Douglas N. C. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA (United States); and others

2013-10-10T23:59:59.000Z

168

NREL: Energy Analysis - Katherine Young  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the Contributions and Achievements of WomenEventsToolsFranciscoJayJoshKatherine Young,

169

Periodic photometric variability of the brown dwarf Kelu-1  

E-Print Network [OSTI]

We have detected a strong periodicity of 1.80+/-0.05 hours in photometric observations of the brown dwarf Kelu-1. The peak-to-peak amplitude of the variation is ~1.1% (11.9+/-0.8 mmag) in a 41nm wide filter centred on 857nm and including the dust/temperature sensitive TiO & CrH bands. We have identified two plausible causes of variability: surface features rotating into- and out-of-view and so modulating the light curve at the rotation period; or, elliposidal variability caused by an orbiting companion. In the first scenario, we combine the observed vsin(i) of Kelu-1 and standard model radius to determine that the axis of rotation is inclined at 65+/-12 degrees to the line of sight.

F. J. Clarke; C. G. Tinney; K. R. Covey

2002-01-10T23:59:59.000Z

170

Hanbury-Brown-Twiss analysis and dynamical correlations  

SciTech Connect (OSTI)

We test the applicability of the Hanbury-Brown-Twiss theory of bosonic enhancement for the analysis of heavy ion reactions. The correlation function is calculated in a solvable model. We find that the analysis in terms of the ratio of like-sign to unlike-sign pairs is more reliable and more stable than in terms of the ratio of pairs to single mesons. We also compare our exact results with the predictions obtained in a classical treatment of the source function, like the one that is used to extract correlation functions from cascade type simulations. In spite of agreement for extreme choices of the parameters of our model, the results of the approximation deviate strongly from the exact correlation function for Physical Noticed choices. We thus call into question the use of classical approximations for the analysis of reactions in which the final state is produced by a cascade of resonance decays.

Herrmann, M.; Bertsch, G.F.; Danielewicz, P.

1993-10-01T23:59:59.000Z

171

Hanbury-Brown--Twiss analysis in a solvable model  

SciTech Connect (OSTI)

The analysis of meson correlations by Hanbury-Brown--Twiss interferometry is tested with a simple model of meson production by resonance decay. We derive conditions which should be satisfied in order to relate the measured momentum correlation to the classical source size. The Bose correlation effects are apparent in both the ratio of meson pairs to singles and in the ratio of like to unlike pairs. With our parameter values, we find that the single particle distribution is too distorted by the correlation to allow a straightforward analysis using pair correlation normalized by the singles rates. An analysis comparing symmetrized to unsymmetrized pairs is more robust, but nonclassical off-shell effects are important at realistic temperatures.

Bertsch, G.F.; Danielewicz, P.; Herrmann, M. (Institute for Nuclear Theory, HN-12, University of Washington, Seattle, Washington 98195 (United States) Physics Department, FM-15, University of Washington, Seattle, Washington 98195 (United States) Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 (United States))

1994-01-01T23:59:59.000Z

172

The theory of globulettes: candidate precursors of brown dwarfs and free floating planets in H II regions  

E-Print Network [OSTI]

Large numbers of small opaque dust clouds - termed 'globulettes' by Gahm et al - have been observed in the H II regions surrounding young stellar clusters. With masses typically in the planetary (or low mass brown dwarf) regime, these objects are so numerous in some regions (e.g. the Rosette) that, if only a small fraction of them could ultimately collapse, then they would be a very significant source of free floating planets. Here we review the properties of globulettes and present a theoretical framework for their structure and evolution. We demonstrate that their interior structure is well described by a pressure confined isothermal Bonnor-Ebert sphere and that the observed mass-radius relation (mass approximately proportional to the radius squared) is a systematic consequence of a column density threshold below which components of the globulette are not identified. We also find that globulettes with this interior structure are very stable against collapse within H II regions. We follow Gahm et al in assum...

Haworth, Thomas J; Clarke, Cathie J

2014-01-01T23:59:59.000Z

173

May 14-16, 2009 Young Harris College, Young Harris, Georgia  

E-Print Network [OSTI]

May 14-16, 2009 Young Harris College, Young Harris, Georgia Master Beekeeper levels: · Certified · Journeyman · Master · Master Craftsman Young Harris College and the University of Georgia are offering, candles, section comb honey, mead, and beekeeping gadgets. We urge students to participate

Delaplane, Keith S.

174

Lean color characteristics of beef from steers and young bulls  

E-Print Network [OSTI]

, appropriate di iutions on pr epoured plates of trypcic soy agar (TSA, Difco). Plates were incuoated 11 TABLE 1. SCORING SYSTEM FOR MUSCLE COLOR Description Bri ght cherry red Moderately bright cherry red Slightly light cherry red Cherry red Slightly... dark red Moderately dark cherry red Dark red or brown Very dark red or brown Extreme1y dark red or brown Score TABLE 2. SCORING SYSTEM FOR SURFACE DISCOLORATION Descri tion Score No surface discoloration Less than 10% surface discoloration 10...

Purser, David Elbert

1982-01-01T23:59:59.000Z

175

THE YOUNG ACADEMY MOVEMENT CTHB MEMBER PLAYS A LEADING ROLE IN THE GLOBAL YOUNG ACADEMY AND THE  

E-Print Network [OSTI]

THE YOUNG ACADEMY MOVEMENT CTHB MEMBER PLAYS A LEADING ROLE IN THE GLOBAL YOUNG ACADEMY AND THE SOUTH AFRICAN YOUNG ACADEMY OF SCIENCE (SAYAS) In tracing the development and establishment of the Global Young Academy (GYA) and South African Young Academy of Science (SAYAS), it is necessary to sketch

176

MICHIGAN STATE UNIVERSITY YOUNG ALUMNI AWARD  

E-Print Network [OSTI]

MICHIGAN STATE UNIVERSITY YOUNG ALUMNI AWARD The MSU Alumni Association annually seeks and accepts nominations for the Michigan State University YOUNG ALUMNI AWARD. The selection is made from candidates who State University. These individuals demonstrate a commitment to Michigan State University by continuing

177

Palatability of beef from young bulls  

E-Print Network [OSTI]

beef; hower et, previous research (Adams and Arthaud, 1963; Aitken er al. , 1963; Reagan et al. , 1971; Gortsema et al. , 1974) has shown that meat from young bulls is not as tender as that from steers and that the palatability of young bull beef...

Riley, Ray Renfrow

1981-01-01T23:59:59.000Z

178

Federal Reserve Bank of Dallas  

E-Print Network [OSTI]

The effect of oil price shocks on U.S. economic activity seems to have changed since the mid-1990s. A variety of explanations have been offered for the seeming change — including better luck, the reduced energy intensity of the U.S. economy, a more flexible economy, more experience with oil price shocks and better monetary policy. These explanations point to a weakening of the relationship between oil prices shocks and economic activity rather than the fundamentally different response that may be evident since the mid-1990s. Using a dynamic stochastic general equilibrium model of world economic activity, we employ Bayesian methods to assess how economic activity responds to oil price shocks arising from supply shocks and demand shocks originating in the United States or elsewhere in the world. We find that both oil supply and oil demand shocks have contributed significantly to oil

Nathan S. Balke; Stephen P. A. Brown; Mine K. Yücel; Jel Codes F

2008-01-01T23:59:59.000Z

179

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

Recommendation 6 Redwood Coast Energy Authority Northwest California Alternative Fuels Readiness Project $300 Alternative Fuel Readiness Proposed Awards California Energy Commission Alternative and Renewable FuelSTATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

180

E-Print Network 3.0 - anadromous brown trout Sample Search Results  

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

Search Sample search results for: anadromous brown trout Page: << < 1 2 3 4 5 > >> 1 J. Fish Biol. (1987)31, 143-146 Mating of anadromousAtlanticsalmon, Salmo salar L., with...

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


181

Brown Bag Lunch Tuesday, October 23, 12:15-1:15  

E-Print Network [OSTI]

Brown Bag Lunch Tuesday, October 23, 12:15-1:15 Open Access: How does it impact teaching Campbell, Kathleen MacKenzie, Glenna Quinn Open Access has been both hailed as the answer to unrestricted

182

LETTER doi:10.1038/nature12771 Efficient ethanol production from brown macroalgae  

E-Print Network [OSTI]

Asteromyces cruciatus4 . The genomic integration and overexpression of the gene encodingthis transporter not contain lignin, simple biorefinery processes such as milling, leaching and extraction can separate sustainable food production13 (see Supplementary Discussion for a brown macroalgae biorefinery description

Cai, Long

183

New Zealand lessons may aid efforts to control light brown apple moth in California  

E-Print Network [OSTI]

1975. Integrated control of apple pests in New Zealand. 1.of the light brown apple moth Epiphyas postvittana (Walker),685–92. Dumbleton L J. 1932. The apple leaf-roller (Tortrix

Varela, Lucia G.; Walker, James T.S.; Lo, Peter L; Rogers, David J

2010-01-01T23:59:59.000Z

184

The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD  

E-Print Network [OSTI]

Introduction to Engineering Computation · STAT 310 Probability and Statistics · STAT 410 Introduction246 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

Richards-Kortum, Rebecca

185

The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD  

E-Print Network [OSTI]

Introduction to Engineering Computation · STAT 310 Probability and Statistics · STAT 410 Introduction253 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

Richards-Kortum, Rebecca

186

Variability and change in the Canadian cryosphere C. Derksen & S. L. Smith & M. Sharp & L. Brown &  

E-Print Network [OSTI]

Variability and change in the Canadian cryosphere C. Derksen & S. L. Smith & M. Sharp & L. Brown-mail: Chris.Derksen@ec.gc.ca S. L. Smith :J. Bourgeois Geological Survey of Canada, Natural Resources Canada

187

Two Writers Sharing: Sterling A. Brown, Robert Frost, and In "Dives's Dive"  

E-Print Network [OSTI]

Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Two writers sharing: Sterling A. Brown, Robert Frost, and "in dives' dive Tidwell, John Edgar African American Review; Fall 1997; 31, 3; Pro...

Tidwell, John E.

1997-09-01T23:59:59.000Z

188

Civil and Environmental Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

) environmental engineering (air and water quality, transport theory, modeling, and energy) (2) hydrology) urbaninfrastructureandmanagement(transportationsystems,complex urban systems, soil mechanics, engineering economics, management1 Civil and Environmental Engineering The George R. Brown School of Engineering Chair Pedro J. J

Richards-Kortum, Rebecca

189

Anglers needed - Save young salmon and reel in cash  

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

Power Administration funds the program. Pikeminnow represent about 80 percent of all fish that kill young salmon. So these young salmon need your help. Each angler counts. The...

190

Brown is the color of many things: a collection of short stories  

E-Print Network [OSTI]

BROWN IS THE COLOR OF MANY THINGS: A COLLECTION OF SHORT STORIES A Thesis by CHANDRALEKHA GUPTA Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF ARTS... May 2000 Major Subject: English BROWN IS THE COLOR OF MANY THINGS: A COLLECTION OF SHORT STORIES A Thesis by CHANDRALEKHA GUPTA Submitted to Texas ARM University in partial fulfillment of the requirements for the degree of MASTER OF ARTS...

Gupta, Chandralekha

2000-01-01T23:59:59.000Z

191

Honeywell Young Innovator Award 2012 Team of Criti Mahajan and Ritubhan Gautam from IIT Delhi won the Honeywell Young  

E-Print Network [OSTI]

the Honeywell Young Innovator Challenge for their entry titled "Blue Energy" (reverse electrodialysis

Kumar, M. Jagadesh

192

CHARACTERIZATION OF THE NEARBY L/T BINARY BROWN DWARF WISE J104915.57-531906.1 AT 2 pc FROM THE SUN  

SciTech Connect (OSTI)

WISE J104915.57-531906.1 is a L/T brown dwarf binary located 2 pc from the Sun. The pair contains the closest known brown dwarfs and is the third closest known system, stellar or sub-stellar. We report comprehensive follow-up observations of this newly uncovered system. We have determined the spectral types of both components (L8 {+-} 1, for the primary, agreeing with the discovery paper; T1.5 {+-} 2 for the secondary, which was lacking spectroscopic type determination in the discovery paper) and, for the first time, their radial velocities (V{sub rad} {approx} 23.1, 19.5 km s{sup -1}) using optical spectra obtained at the Southern African Large Telescope and other facilities located at the South African Astronomical Observatory (SAAO). The relative radial velocity of the two components is smaller than the range of orbital velocities for theoretically predicted masses, implying that they form a gravitationally bound system. We report resolved near-infrared JHK{sub S} photometry from the Infrared Survey Facility telescope at the SAAO which yields colors consistent with the spectroscopically derived spectral types. The available kinematic and photometric information excludes the possibility that the object belongs to any of the known nearby young moving groups or associations. Simultaneous optical polarimetry observations taken at the SAAO 1.9 m give a non-detection with an upper limit of 0.07%. For the given spectral types and absolute magnitudes, 1 Gyr theoretical models predict masses of 0.04-0.05 M{sub Sun} for the primary, and 0.03-0.05 M{sub Sun} for the secondary.

Kniazev, A. Y.; Vaisanen, P.; Potter, S. B.; Crawford, S.; Gulbis, A. A. S. [South African Astronomical Observatory, P.O. Box 9, 7935 Observatory, Cape Town (South Africa); Muzic, K.; Mehner, A.; Boffin, H. M. J.; Melo, C.; Ivanov, V. D.; Girard, J.; Mawet, D.; Schmidtobreick, L. [European Southern Observatory, Ave. Alonso de Cordova 3107, Casilla 19001, Santiago 19 (Chile); Kurtev, R.; Borissova, J. [Departamento de Fisica y Astronomia, Universidad de Valparaiso, Av. Gran Bretana 1111, Playa Ancha, 5030 Casilla (Chile); Huelamo, N. [CAB (INTA-CSIC), LAEFF, P.O. Box 78, E-28691 Villanueva de la Canada, Madrid (Spain); Minniti, D. [Departamento Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile, Av. Vicuna Mackenna 4860, Santiago (Chile); Ishibashi, K. [Nagoya University, Nagoya (Japan); Beletsky, Y. [Las Campanas Observatory, Carnegie Institution of Washington, Colina el Pino, Casilla 601 La Serena (Chile); Buckley, D. A. H. [Southern African Large Telescope Foundation, P.O. Box 9, 7935 Observatory, Cape Town (South Africa); and others

2013-06-20T23:59:59.000Z

193

The Decay of Accreting Triple Systems as Brown Dwarf Formation Scenario  

E-Print Network [OSTI]

We investigate the dynamical decay of non-hierarchical accreting triple systems and its implications on the ejection model as Brown Dwarf formation scenario. A modified chain-regularization scheme is used to integrate the equations of motion, that also allows for mass changes over time as well as for momentum transfer from the accreted gas mass onto the bodies. We integrate an ensemble of triple systems within a certain volume with different accretion rates, assuming several prescriptions of how momentum is transferred onto the bodies. We follow their evolution until the systems have decayed. We analyze the end states and decay times of these systems and determine the fraction of Brown Dwarfs formed, their escape speeds as well as the semi-major axis distribution of the formed Brown Dwarf binaries. We find that the formation probability of Brown Dwarfs depends strongly on the assumed momentum transfer which is related to the motion of the gas. Due to ongoing accretion and consequent shrinkage of the systems, the median escape velocity is increased by a factor of 2 and the binary separations are decreased by a factor of 5 compared with non-accreting systems. Furthermore, the obtained semi-major axis distribution drops off sharply to either side of the median, which is also supported by observations. We conclude that accretion and momentum transfer of accreted gas during the dynamical decay of triple systems is able to produce the observed distribution of close binary Brown Dwarfs, making the ejection model a viable option as Brown Dwarf formation scenario.

Stefan Umbreit; Andreas Burkert; Thomas Henning; Seppo Mikkola; Rainer Spurzem

2005-01-05T23:59:59.000Z

194

HST SPECTRAL MAPPING OF L/T TRANSITION BROWN DWARFS REVEALS CLOUD THICKNESS VARIATIONS  

SciTech Connect (OSTI)

Most directly imaged giant exoplanets are fainter than brown dwarfs with similar spectra. To explain their relative underluminosity, unusually cloudy atmospheres have been proposed. However, with multiple parameters varying between any two objects, it remained difficult to observationally test this idea. We present a new method, sensitive time-resolved Hubble Space Telescope near-infrared spectroscopy, to study two rotating L/T transition brown dwarfs (2M2139 and SIMP0136). The observations provide spatially and spectrally resolved mapping of the cloud decks of the brown dwarfs. The data allow the study of cloud structure variations while other parameters are unchanged. We find that both brown dwarfs display variations of identical nature: J- and H-band brightness variations with minimal color and spectral changes. Our light curve models show that even the simplest surface brightness distributions require at least three elliptical spots. We show that for each source the spectral changes can be reproduced with a linear combination of only two different spectra, i.e., the entire surface is covered by two distinct types of regions. Modeling the color changes and spectral variations together reveal patchy cloud covers consisting of a spatially heterogeneous mix of low-brightness, low-temperature thick clouds and brighter, thin, and warm clouds. We show that the same thick cloud patches seen in our varying brown dwarf targets, if extended to the entire photosphere, predict near-infrared colors/magnitudes matching the range occupied by the directly imaged exoplanets that are cooler and less luminous than brown dwarfs with similar spectral types. This supports the models in which thick clouds are responsible for the near-infrared properties of these ''underluminous'' exoplanets.

Apai, Daniel [Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721 (United States); Radigan, Jacqueline; Jayawardhana, Ray [Department of Astronomy, University of Toronto, 50 St. George Street, Toronto M5S 3H4 (Canada); Buenzli, Esther [Department of Astronomy and Steward Observatory, 933 N. Cherry Avenue, University of Arizona, Tucson, AZ 85721 (United States); Burrows, Adam [Department of Astrophysical Sciences, 105 Peyton Hall, Princeton University, Princeton, NJ 08544 (United States); Reid, Iain Neill, E-mail: apai@as.arizona.edu [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21212 (United States)

2013-05-10T23:59:59.000Z

195

Limits to the potential distribution of light brown apple moth in Arizona–California based on climate suitability and host plant availability  

E-Print Network [OSTI]

503–531 Dumbleton LJ (1932) The apple leaf roller (TortrixJW (1937) The light-brown apple moth (Tortrix post- vittana,distribution of light brown apple moth in Arizona–California

Gutierrez, Andrew Paul; Mills, Nicholas J.; Ponti, Luigi

2010-01-01T23:59:59.000Z

196

Deterministic Time Classes Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. p.1  

E-Print Network [OSTI]

Lecture 11 Deterministic Time Classes Slides modified by Benny Chor, based on original slides on Model Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. ­ p Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. ­ p.1 #12

Beimel, Amos

197

Reduction Involving Controlled Execution Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. p.1  

E-Print Network [OSTI]

Lecture 10 Reduction Involving Controlled Execution Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. ­ p.1 #12;Lecture 10 Reduction Involving Controlled Execution Rice Theorem Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown

Beimel, Amos

198

2010 USDA Research Forum on Invasive Species GTR-NRS-P-75 87 ECONOMIC ANALYSIS OF LIGHT BROWN APPLE MOTH  

E-Print Network [OSTI]

2010 USDA Research Forum on Invasive Species GTR-NRS-P-75 87 ECONOMIC ANALYSIS OF LIGHT BROWN APPLE. Our analyses indicated that LBAM could cause substantial economic losses to U.S. apple, grape, orange an economic analysis of the light brown apple moth (LBAM), (Epiphyas postvittana (Walker)), whose presence

199

Ionization in atmospheres of Brown Dwarfs and extrasolar planets IV. The Effect of Cosmic Rays  

E-Print Network [OSTI]

Cosmic rays provide an important source for free electrons in the Earth's atmosphere and also in dense interstellar regions where they produce a prevailing background ionization. We utilize a Monte Carlo cosmic ray transport model for particle energies of 1 MeV model for particle energies of 1 GeV model atmospheres of an example brown dwarf with effective temperature Teff = 1500 K, and two example giant gas planets (Teff = 1000 K, 1500 K). For the model brown dwarf atmosphere, the electron fraction is enhanced significantly by cosmic rays when the pressure pgas model atmosphere of the examp...

Rimmer, Paul

2013-01-01T23:59:59.000Z

200

A model for the management of the Texas brown shrimp fishery  

E-Print Network [OSTI]

1979 Major Subject: Agricultural Economics A MODEL FOR THE MANAGEMENT OF THE TEXAS BROWN SHRIMP FISHERY A Thesis by GLENN CHARLES TYDLACKA Approved as to style and content by: (Chairman oE Commi e) pg w~ (Member) (M j) Augvst 1979 ABSTRACT... A Model for the Management of the Texas Brown Shrimp Fishery. (August 1979) Glenn Charles Tydlacka, B. S. , Texas A&M University Chairman of Advi" ory Committee: Dr. Wade L. Griffin The management of the shrimp fi-hery in Texas is an important...

Tydlacka, Glenn Charles

1979-01-01T23:59:59.000Z

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


201

In vitro kinetics of hepatic glutathione s-transferase conjugation in largemouth bass and brown bullheads  

SciTech Connect (OSTI)

The kinetics of glutathione 5-transferase (GST) catalysis were investigated in largemouth bass (Micropterus salmoides) and brown bullheads (Amerius nebulosus), two freshwater fish species found in a variety of polluted waterways in the eastern US. The initial rates of hepatic GST activity toward four GST substrates, including 1-chloro-2,4-dinitrobenzene, ethacrynic acid, {Delta}5-androstene-17-dione, and nitrobutyl chloride, were significantly higher in brown bullheads than in largemouth bass. Hepatic GST activity toward 1,2-dichloro-4-nitrobenzene, a {mu}-class GST substrate in rodents, was not detectable in either species. Liver cytosolic GSTs were more efficient in bullheads than in bass at catalyzing 1-chloro-2,4-dinitrobenzene-reduced glutathione (CDNB-GSH) conjugation over a broad range of electrophile (CDNB) concentrations, including those representative of environmental exposure. In contrast, largemouth bass maintained higher ambient concentrations of GSH, the nucleophilic cofactor for GST-mediated conjugation, than brown bullheads. Biphasic kinetics for GST-CDNB conjugation under conditions of variable GSH concentration were apparent in Eadie-Hofstee plots of the kinetic data, suggesting the presence of at least two hepatic GST isozymes with markedly different K{sub m} values for GSH in both species. The GST-CDNB reaction rate data obtained under conditions of variable GSH were well fitted (R{sup 2} = 0.999) by the two-enzyme Michaelis-Menten equation. In addition, Western blotting experiments confirmed the presence of two different hepatic GST-like proteins in both largemouth bass and brown bullhead liver. Collectively, these findings indicate that largemouth bass and brown bullhead GSTs catalyze the conjugation of structurally diverse, class-specific GST substrates, and that brown bullheads exhibit higher initial rates of GST activity than largemouth bass. The relatively higher rates of in vitro liver GST activity at the low substrate concentrations relevant to environmental exposure is expected to protect brown bullheads from the toxic effects of sediment-associated electrophilic chemicals. The somewhat lower rates of GST activity in largemouth bass liver compared with brown bullhead liver, however, may be offset by maintenance of higher ambient hepatic GSH concentrations in largemouth bass.

Gallagher, E.P.; Sheehy, K.M.; Lame, M.W.; Segall, H.J.

2000-02-01T23:59:59.000Z

202

Double Conscious Brother in the Veil Toward an Intellectual Biography of Sterling A. Brown  

E-Print Network [OSTI]

DOUBLE CONSCIOUS BROTHER IN THE VEIL Toward an Intellectual Biography of Sterling A. Brown by John Edgar Tidwell Our home was graced with six children, five girls arid one boy. . . . The youngest of the family is a boy now 22 years of age. He... to that proffered in the High Schools of Washington. —Rev. Dr. Sterling Nelson Brown, My Own Life Story (37) "I kin be a good bishop, I got de looks, An' I ain't spoiled myself By readin' books. "Don't know so much 'Bout de Holy Ghost, But I likes de long...

Tidwell, John E.

1998-09-01T23:59:59.000Z

203

Young and Older Adults’ Reading of Distracters  

E-Print Network [OSTI]

. Psychology and Aging, 21, 448-465. Shipley, W. C. (1940). A self-administered scale for measuring intellectual impairment and deterioration. Journal of Psychology, 9, 371-377. Kemper, S., McDowd, J., Metcalf, K., & Liu, C.-J. (2008). Young and older...Kemper, S., McDowd, J., Metcalf, K., & Liu, C.-J. (2008). Young and older adults’ reading of distracters. Educational Gerontology, 34, 489-502. PM#2396579. Publisher’s official version: http://dx.doi.org/10.1080/03601270701835858. Open Access...

Kemper, Susan; McDowd, Joan; Metcalf, Kim; Liu, Chiung-Ju

2008-05-01T23:59:59.000Z

204

NATIONAL PRESS RELEASE I PARIS I 30 AUGUST 2013 Brown algae contain phlorotannins, aromatic (phenolic) compounds that are unique in the plant  

E-Print Network [OSTI]

NATIONAL PRESS RELEASE I PARIS I 30 AUGUST 2013 Brown algae contain phlorotannins, aromatic elucidated the key step in the production of these compounds in Ectocarpus siliculosus, a small brown alga phlorotannins from brown algae for use in industry was a complex process, and the biosynthesis pathways

Canet, LĂ©onie

205

, UNIVERSITY Brigham Young University Geology Studies  

E-Print Network [OSTI]

, UNIVERSITY #12;Brigham Young University Geology Studies Volume 1 5 - 1968 Part 2 Studies for Students No. 1 Guide to the Geology of the Wasatch Mountain Front, Between Provo Canyon and Y Mountain, Northeast of Provo, Utah by J. Keith Rigby and Lehi F. Hintze #12;A publication of the Department of Geology

Seamons, Kent E.

206

Distinguished Engineering Graduate Outstanding Young Engineering Graduate  

E-Print Network [OSTI]

, or service delivery through the application of engineering principles; or · Contributed truly exceptional2013 Distinguished Engineering Graduate and Outstanding Young Engineering Graduate Award Nomination Form Print Form #12;The highest honor the Cockrell School of Engineering can bestow on one of its own

Lightsey, Glenn

207

Diagnostics for FIRE Kenneth M. Young  

E-Print Network [OSTI]

Diagnostics for FIRE Kenneth M. Young Princeton Plasma Physics Laboratory Burning Plasma Workshop May 1 - 3, 2001 General Atomics San Diego, CA #12;Aspects of Plasma Diagnostics to achieve Burning Plasma Physics Goals in FIRE · The diagnostic set should provide the same quality of data as in best

208

Diagnostics for FIRE Kenneth M. Young  

E-Print Network [OSTI]

Diagnostics for FIRE Kenneth M. Young Princeton Plasma Physics Laboratory NSO PAC 2 Meeting January 17, 2001 MIT Plasma Fusion Center Cambridge, MA #12;Aspects of Plasma Diagnostics to achieve Burning Plasma Physics Goals in FIRE · The diagnostic set should provide the same quality of data as in best

209

EFFECTS OF SOUND WAVES ON YOUNG SALMON  

E-Print Network [OSTI]

EFFECTS OF SOUND WAVES ON YOUNG SALMON Marine Biological Laboratory X. 1 33 R A. RTT ir.':; WOODS instantaneously to sounds. It was con- were tested in an experimental tank and in eluded that sound waves were, Wash . sound studies conducted under the above contract are terminated. #12;EFFECTS OF SOUND WAVES

210

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

on the results of the Renewable Energy Program's activities and status of funding. The 2011 Annual Report and funding awards. The Appendix contains detailed project descriptions, statistics, and financial dataSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

211

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

annually on the results of the Renewable Energy Program's activities and status of funding. The 2011 Annual and funding awards. The Appendix contains detailed project descriptions, statistics, and financial dataSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

212

Short communication Control of brown rot of stone fruits by brief heated water immersion treatments  

E-Print Network [OSTI]

Short communication Control of brown rot of stone fruits by brief heated water immersion treatments. Several studies have shown that hot water treatments by themselves or in combination with other treatments they require are an issue that has hindered the commercial adoption of hot water treatments. While higher water

Crisosto, Carlos H.

213

DYNAMIC TRACKING PHASED ARRAY DATA LINKS K. D. Brown Dr. Chris Allen  

E-Print Network [OSTI]

DYNAMIC TRACKING PHASED ARRAY DATA LINKS K. D. Brown Dr. Chris Allen NNSA-KCP University of Kansas link developed by National Nuclear Safety Administration's Kansas City Plant (NNSA-KCP) and the University of Kansas (KU) in support of NNSA's Remote Sensing Laboratory (NNSA-RSL) located at the Nevada

Kansas, University of

214

Nutrition and Cancer Brown Kelp Modulates Endocrine Hormones in Female Sprague-Dawley  

E-Print Network [OSTI]

Nutrition and Cancer Brown Kelp Modulates Endocrine Hormones in Female Sprague-Dawley Rats Asians. However, studies from our laboratory suggest that the anti-estrogenic effects of dietary kelp modulation related to kelp ingestion in a pilot study of premenopausal women, we investigated the endocrine

California at Berkeley, University of

215

Policy Based Storage System For Heterogeneous Environment Dai Qin, Ashvin Goel, Angela Demke Brown,  

E-Print Network [OSTI]

Policy Based Storage System For Heterogeneous Environment Dai Qin, Ashvin Goel, Angela Demke Brown storage sys- tems to the needs of specific applications and hardware. Most storage systems are not aware of this issue: file systems or other applications talk to the storage system using a simple block layer

Goel, Ashvin

216

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

of the California Solar Initiative, a comprehensive statewide solar program. The NSHP provides rebates to encourage of the NSHP is to install 400 MW of solar electric capacity on new homes and residential buildings by the endSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

217

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

Award Score Score Status 1 CaliSolar, Inc. Manufacturing Capacity Expansion from 60 MW to 155 MW $5 SV Green Tech Corp. Expansion of Solar Panel Manufacturing in California $4,948,000 $0 61 Finalist 12STATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

218

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

STATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY a containment structure that would be located between the solar fields of SEGS VIII and SEGS IX, for the storage STAFF REVIEW AND DETERMINATION Pursuant to section 1769(a)(2), Title 20, California Code of Regulations

219

Dipole trapped spheromak in a prolate flux conserver M. R. Brown,a  

E-Print Network [OSTI]

Dipole trapped spheromak in a prolate flux conserver M. R. Brown,a C. D. Cothran, J. Fung, M. Chang reports the observation and characterization of a spheromak formed in the Swarthmore Spheromak Experiment. The spheromak is studied in a prolate tilt unstable 0.4 m diameter, 0.6 m length copper flux conserver in SSX

Brown, Michael R.

220

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

-2013-007 The Distributed Generation Integration Cost Study: Analytical Framework is available free from the Energy level of confidence. This study uses the framework to highlight potential impacts, least-cost solutionsSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

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


221

Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs  

E-Print Network [OSTI]

The fundamental properties of brown dwarfs evolve with age. Models describing the evolution of luminosities and effective temperatures, among other physical parameters, can be empirically constrained using brown dwarfs of various masses in star clusters of well determined age and metallicity. We aim to carry out a spectroscopic and photometric characterization of low-mass brown dwarfs of the ~120 Myr old Pleiades open cluster. We obtained low-resolution near-infrared spectra of the J=17.4-18.8 mag candidate L-type brown dwarfs PLIZ 28 and 35, BRB 17, 21, 23, and 29, which are Pleiades members by photometry and proper motion. We also obtained spectra of the well-known J=15.4-16.1 mag late M-type cluster members PPl 1, Teide 1, and Calar 3. We find that the former six objects have early- to mid-L spectral types and confirm previously reported M-types for the other three objects. The spectra of the L0-type BRB 17 and PLIZ 28 present a triangular H-band continuum shape and remarkable VO absorption, indicating tha...

Bihain, G; Osorio, M R Zapatero; Béjar, V J S; Caballero, J A

2010-01-01T23:59:59.000Z

222

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

(RNS), and is based on the amount of current electric generation from renewable resources) that is generated from renewable generation resources instead of the capacity (megawatt ­ MW) of these facilitiesSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

223

A Review of "Sir Thomas Browne: The World Proposed" edited by Reid Barbour and Claire Preston  

E-Print Network [OSTI]

passage into what is surely one of the most important topics for readers of Milton. Reid Barbour and Claire Preston, eds. Sir Thomas Browne: The World Proposed. Oxford: Oxford University Press, 2008. xii + 368 pp. + 3 illus. $120.00. Review by joseph...

Black, Joseph

2011-01-01T23:59:59.000Z

224

Energy Efficient Digital Networks Bruce Nordman, Steven Lanzisera and Richard Brown  

E-Print Network [OSTI]

LBNL-6254E Energy Efficient Digital Networks Bruce Nordman, Steven Lanzisera and Richard Brown, product, or process disclosed, or represents that its use would not infringe on privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark

225

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

examines a range of issues facing the state's electricity, natural gas, and transportation fuel sectorsSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY reliability, enhance the #12;2 state's economy, and protect public health and safety." (Public Resources Code

226

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

of major energy trends and issues facing California's electricity, natural gas, and transportation fuelSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY reliable, secure, and diverse energy supplies; enhance California's economy; and protect public health

227

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G BROWN, JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G BROWN, JR., Governor CALIFORNIA ENERGY and Reinvestment Act of 2009 (ARRA) funding to California's transition to a clean energy economy. ARRA dedicated, and greenhouse gas emission reductions as well as the contribution to California's energy and environmental

228

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

, natural gas, and transportation fuels to meet the needs of the state's economy and growing population proceeding on a range of issues facing California's electricity, natural gas, and transportation fuel sectorsSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

229

From Nash and Brown to Maynard Smith: Equilibria, Dynamics and ESS* J. HOFBAUER  

E-Print Network [OSTI]

From Nash and Brown to Maynard Smith: Equilibria, Dynamics and ESS* J. HOFBAUER Institut fĂŒr that in more sophisticated models, an equilibrium satisfying the ESS conditions often re- mains stable in some sense. For example, in the stan- dard dynamic model for haploids, the replicator dy- namics, an ESS

Hofbauer, Josef

230

From Nash and Brown to Maynard Smith: Equilibria, Dynamics, and ESS  

E-Print Network [OSTI]

From Nash and Brown to Maynard Smith: Equilibria, Dynamics, and ESS Josef Hofbauer Institut f sophisticated models, an equilibrium satisfying the ESS conditions often remains stable in some sense. For example, in the standard dynamic model for haploids, the replicator dynamics, an ESS is asymptotically

Hofbauer, Josef

231

STATE OF CALIFORNIA -NATURAL RESOURCES AGENCY EDMUND G. BROWN JR.. Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

in June 2012. · Two reports on trends in natural gas markets that were published in 2012. · An assessment: · Forecasts of electricity and natural gas demand for 2012-2022 that were adopted by the Energy CommissionSTATE OF CALIFORNIA - NATURAL RESOURCES AGENCY EDMUND G. BROWN JR.. Governor CALIFORNIA ENERGY

232

Hot Dry Rock Geothermal Energy Development in the USA David Duchane and Donald Brown  

E-Print Network [OSTI]

1 Hot Dry Rock Geothermal Energy Development in the USA by David Duchane and Donald Brown Los of the world's store of geothermal energy. The real potential for growth in the use of geothermal energy lies system. Water is circulated around a closed loop to extract thermal energy from an engineered geothermal

233

EARLY DEVELOPMENTAL STAGES OF THE BROWN SHRIMP, Penaeus aztecus IVES, REARED IN THE LABORATORY 1  

E-Print Network [OSTI]

. :Manuscript received September 1970. FISHERY BULLETIN: VOL. 69, NO. I, 1971. cies, accurate identification and white shrimps. METHODS AND MATERIALS Larvae of the brown shrimp were first suc- cessfully cultured on these figures are intended to in- dicate only relative size and position, not to show details of setation

234

Friction in Mid-latitude Bob Plant, Stephen Belcher, Bob Beare, Andy Brown  

E-Print Network [OSTI]

Friction in Mid-latitude Cyclones Ian Boutle Bob Plant, Stephen Belcher, Bob Beare, Andy Brown #12;Motivation · Many studies have shown the significance of friction in formation and dissipation of cyclones Dt = + � . F . Diabatic Term: · Surface heat fluxes · Latent heat fluxes Frictional Term

Plant, Robert

235

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY that must be replaced to satisfy local capacity area requirements. · A status report on the several studies, protect the environment, ensure energy reliability, enhance the state's economy, and protect public health

236

Electrical and Computer Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

160 Electrical and Computer Engineering The George R. Brown School of Engineering CHAIR Behnaam Offered: BA, BSEE, MEE, MS, PhD The electrical and computer engineering department strives to provide high for roles of leadership in their chosen careers. In support of this goal, the electrical and computer

Richards-Kortum, Rebecca

237

SPECTRA OF TUKEY TYPES OF ULTRAFILTERS ON BOOLEAN JENNIFER A. BROWN AND NATASHA DOBRINEN  

E-Print Network [OSTI]

SPECTRA OF TUKEY TYPES OF ULTRAFILTERS ON BOOLEAN ALGEBRAS JENNIFER A. BROWN AND NATASHA DOBRINEN Abstract. Extending recent investigations on the structure of Tukey types of ultrafilters on P() to Boolean algebras in general, we classify the spectra of Tukey types of ultrafilters for several classes of Boolean

Dobrinen, Natasha

238

Spectra of Tukey types of ultrafilters on Boolean algebras Jennifer A. Brown and Natasha Dobrinen  

E-Print Network [OSTI]

Spectra of Tukey types of ultrafilters on Boolean algebras Jennifer A. Brown and Natasha Dobrinen Abstract. Extending recent investigations on the structure of Tukey types of ul- trafilters on P() to Boolean algebras in general, we classify the spectra of Tukey types of ultrafilters for several classes

Dobrinen, Natasha

239

SPECTRA OF TUKEY TYPES OF ULTRAFILTERS ON BOOLEAN JENNIFER BROWN AND NATASHA DOBRINEN  

E-Print Network [OSTI]

SPECTRA OF TUKEY TYPES OF ULTRAFILTERS ON BOOLEAN ALGEBRAS JENNIFER BROWN AND NATASHA DOBRINEN Abstract. Extending recent investigations on the structure of Tukey types of ultrafilters on P() to Boolean algebras in general, we classify the spectra of Tukey types of ultrafilters for several classes of Boolean

Dobrinen, Natasha

240

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

, a reasonable assumption must be made about how much energy is lost due to electrical resistanceSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Notice

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


241

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor NOTICE OF RECEIPT  

E-Print Network [OSTI]

STATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor NOTICE OF RECEIPT PETITION TO AMEND the CALIFORNIA ENERGY COMMISSION DECISION for the SACRAMENTO POWER AUTHORITY CAMPBELL with the California Energy Commission requesting to amend Condition of Certification EFF-1 for the Campbell

242

HIST 462: The French Revolution and Napoleonic Era Gregory Brown; gbrown@unlv.nevada.edu; 8954181  

E-Print Network [OSTI]

and Society a. Popkin 8 14 /Doyle 66 85 b. Campbell 239 ­ 265 c. Tackett 19 ­ 47 d. Dubois, 30 72. Campbell, 139 ­ 218 c. Tackett, 48 ­ 76 d. Dubois, 73 84 5. Sept 20, 22 Coming of the FrenchHIST 462: The French Revolution and Napoleonic Era Gregory Brown; gbrown@unlv.nevada.edu; 8954181

Ahmad, Sajjad

243

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

Foresight Renewable Solutions Integrated Solar PV, Advanced Compressed Air Energy Storage, and MicrogridSTATE OF CALIFORNIA ­NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 NINTH STREET SACRAMENTO, CA 95814-5512 www.energy.ca.gov NOTICE OF PROPOSED AWARDS Community

244

Letter from Shirley Maiewski to Diana Brown re: Alternative Universe Four  

E-Print Network [OSTI]

niv/e 481 Main Street Hatfield, MA 01038 April 22, 1977 Diana G. Brown PO Box 187 Henderson, NV 89015 Dear Diana: Thank you for taking the time to write us about AU4. We are delighted that you have enjoyed our efforts. We had such fun...

Maiewski, Shirley

1977-01-01T23:59:59.000Z

245

EIS-0435: Modification of the Groton Generation Station Interconnection Agreement, Brown County, South Dakota  

Broader source: Energy.gov [DOE]

This EIS evaluates the environmental impacts of a proposal for DOE's Western Area Power Administration to modify its Large Generator Connection Agreement for the Groton Generation Station in Brown County, South Dakota. The modification would allow Basin Electric Power Cooperative, which operates the generation station, to produce power above the current operating limit of 50 average megawatts.

246

Nematode faunal analysis in an aquic brown soil fertilised with slow-release urea, Northeast China  

E-Print Network [OSTI]

Nematode faunal analysis in an aquic brown soil fertilised with slow-release urea, Northeast China, Institute of Applied Ecology, Chinese Academy of Sciences, Shenyang 110016, PR China b Department of Earth of the Chinese Academy of Sciences, Beijing 100039, PR China Received 14 May 2004; received in revised form 15

Neher, Deborah A.

247

STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

/or under- utilized technologies to increase natural gas end-use efficiency in California's industrial* Benz Air Engineering, Co., Inc. High Efficiency Natural Gas Reciprocating Engine Boiler $2STATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

248

Browne, CB, Research Proposal, March 2009 Activation of the Inflammasome in Gout  

E-Print Network [OSTI]

Browne, CB, Research Proposal, March 2009 1 Activation of the Inflammasome in Gout Background Gout. The overall prevalence of gout in the U.S. was determined to be 41 in 1000 (1). Men are at a higher risk than women for gout, and the risk increases with age for both males and females (1). The initiation

Gleeson, Joseph G.

249

THE NEAR-INFRARED SPECTRUM OF THE BROWN DWARF GLIESE 229B T. R. GEBALLE  

E-Print Network [OSTI]

THE NEAR-INFRARED SPECTRUM OF THE BROWN DWARF GLIESE 229B T. R. GEBALLE Joint Astronomy Centre, 660 vapor. Water and methane are both shown to be strong absorbers in the near-infrared spectrum. (1995) obtained a low-resolution ( / 2 150) near-infrared (1­2.5 m) spectrum of Gl 229B and found

Sloan, Gregory C.

250

Reassessing U.S. nuclear weapons policy Harold Brown[1] and John Deutch[2  

E-Print Network [OSTI]

is the belief that the possession of nuclear weapons will improve its security. Nothing that the United States1 Reassessing U.S. nuclear weapons policy Harold Brown[1] and John Deutch[2] The end of the Cold War changed "the balance of nuclear terror" and with it the centrality of nuclear forces in U

Deutch, John

251

METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1  

E-Print Network [OSTI]

METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1 K. M. Barkume,1 G. A regime and by absorption due to methane in the near-infrared. The solid methane absorption lines through the methane. These long path lengths can be parameterized as a methane grain size of approximately

Brown, Michael E.

252

Methane oxidation associated with submerged brown mosses reduces methane emissions from Siberian  

E-Print Network [OSTI]

Methane oxidation associated with submerged brown mosses reduces methane emissions from Siberian, University of Hamburg, Allende-Platz 2, 20146 Hamburg, Germany Summary 1. Methane (CH4) oxidation to Sphagnum species and low-pH peatlands. 2. Moss-associated methane oxidation (MAMO) can be an effective

Wehrli, Bernhard

253

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

/strikeout. Background The NSHP is part of a comprehensive statewide solar program known as the California Solar scheduled Energy Commission Business Meeting. The minimum guidelines for implementing California's solarSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

254

STATE OF CALIFORNIA THE RESOURCES AGENCY EDMUND G. BROWN, JR. , Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

having been shown, the California Energy Commission hereby grants the request by AES Solar to terminateSTATE OF CALIFORNIA THE RESOURCES AGENCY EDMUND G. BROWN, JR. , Governor CALIFORNIA ENERGY COMMISSION 1516 NINTH STREET SACRAMENTO, CA 95814-5112 STATE OF CALIFORNIA ENERGY RESOURCES CONSERVATION

255

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN Jr., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Presentation on the U.S. Department of Defense Study: Solar Energy Development on Department of Defense Installations

256

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

to Proposed Revisions to the New Solar Homes Partnership Guidebook The California Energy Commission will hold1 STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov In the matter

257

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

known as the California Solar Initiative. The NSHP provides financial incentives to encourageSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov In the matter

258

The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD  

E-Print Network [OSTI]

211Introduction to Engineering Computation · STAT310Probability and Statistics · STAT410Introduction263 Statistics The George R. Brown School of Engineering Degrees Offered: BA, MStat, MA, PhD Course engineering, computational and applied mathematics, managerial studies, mathematics, political science

Richards-Kortum, Rebecca

259

PHENOLOGY AND BROWN-HEADED COWBIRD PARASITISM B.A., University of Colorado, 2003  

E-Print Network [OSTI]

PHENOLOGY AND BROWN-HEADED COWBIRD PARASITISM by TY TUFF B.A., University of Colorado, 2003 A thesis submitted to the Faculty of the Graduate School of the University of Colorado in partial, to evaluate the impact of parasitism on two local hosts in the Colorado Front Range: the primary host

Hammerton, James

260

A Navigation System for Robot Soccer Brett Browning, Gordon Wyeth and Ashley Tews  

E-Print Network [OSTI]

A Navigation System for Robot Soccer Brett Browning, Gordon Wyeth and Ashley Tews Computer Science describes the navigation system used for the UQ RoboRoos robot soccer team, runner up in the 1998 world RoboCup championships. The navigation system has been developed to cope with the dynamic environment of robot soccer

Browning, Brett

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


261

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

: SERVICE ON THE CHIEF COUNSEL INSTRUCTIONS: Service of complaints/documents on the Chief Counsel EnergySTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Form CEC-108

262

STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN Jr., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

Startups, and more clean energy jobs. The Forum will: 1) Showcase companies that have developed new cuttingSTATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Venture Capital

263

STATE OF CALIFORNIA -NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION  

E-Print Network [OSTI]

the CALIFORNIA ENERGY COMMISSION DECISION for the SEGS VIII SOLAR FACILITY (88-AFC-1C) On June 11, 2013, Next, and standards (Title 20, California Code of Regulations, section 1769). Energy Commission staff is currentlySTATE OF CALIFORNIA - NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY

264

Light brown apple moth Epiphyas postvittana Michigan State University's invasive species factsheets  

E-Print Network [OSTI]

shelters. Older larvae may create nests by folding or webbing leaves, buds and fruits together where-11 mm long; pale to dark brown; can be found in leaves that are spun together. Eggs : About 1 mm (folded leaves or leaves, buds and fruits webbed together). Superficial fruit damage; point-like holes

265

Civil and Environmental Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

infrastructure and management (transportation systems, urban systems, soil mechanics, engineering economics129 Civil and Environmental Engineering The George R. Brown School of Engineering Chair Pedro. Wiesner adjunCt assistant Professor Karen Duston Professor in the PraCtiCe in Civil engineering management

Richards-Kortum, Rebecca

266

Civil and Environmental Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

infrastructure and management (transportation systems, urban systems, soil mechanics, engineering economics engineering management Joseph Cibor Ed Segner, III Professor in the PraCtiCe of environmental law James B137 Civil and Environmental Engineering The George R. Brown School of Engineering Chair Pedro

Richards-Kortum, Rebecca

267

Civil and Environmental Engineering The George R. Brown School of Engineering  

E-Print Network [OSTI]

: · structural engineering · environmental engineering · engineering management Associate Professors Panos and Watershed Analysis CIVI 451 Introduction to Transportation CIVI 470 Basic Soil Mechanics CIVI 480 Senior119 Civil and Environmental Engineering The George R. Brown School of Engineering Chair Joseph B

Richards-Kortum, Rebecca

268

SPECTRAL PICTURES OF AB AND BA Robin Harte, Young Ok Kim and Woo Young Lee  

E-Print Network [OSTI]

;2 ROBIN HARTE, YOUNG OK KIM AND WOO YOUNG LEE If A B(X), write (A), left (A), right (A), ess(A), left ess (A), and right ess (A) for the spectrum, the left spectrum, the right spectrum, the essential(X), a hole in ess(A) is a bounded component of C \\ ess(A) and a pseudohole in ess(A) is a component of ess

Lee, Woo Young

269

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4  

E-Print Network [OSTI]

#12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4 The Fossil Vertebrates of Utah Salt Lake Gty, Utah 84102 W .E. Miller Deparlment~of Geology and Zoology Bngham Young Unrwerrrly Provo of Geology Brigham Young University Provo, Utah 84602 Editors W. Kenneth Hamblln Cynthia M. Gardner Issue

Seamons, Kent E.

270

Lifestyle, identity and young people's experiences of mountain biking  

E-Print Network [OSTI]

Lifestyle, identity and young people's experiences of mountain biking It has been widely recognised emphasis on young people as a key target group. Mountain biking, as a popular youth sport that often occurs biking and to investigate the resulting relation- ships young people developed with countryside spaces

271

Designing for Homeless Young People: Precaution in Ubiquitous Computing  

E-Print Network [OSTI]

, academics, and many others. Less obviously, homeless young people, unlike these other people, actually liveDesigning for Homeless Young People: Precaution in Ubiquitous Computing Abstract How should ubiquitous access to information through computing be shaped to improve the lives of homeless young people

Anderson, Richard

272

YOUNG RADIO PULSARS IN GALACTIC GLOBULAR CLUSTERS  

SciTech Connect (OSTI)

Currently three isolated radio pulsars and one binary radio pulsar with no evidence of any previous recycling are known in 97 surveyed Galactic globular clusters (GCs). As pointed out by Lyne et al., the presence of these pulsars cannot be explained by core-collapse supernovae, as commonly assumed for their counterparts in the Galactic disk. We apply a Bayesian analysis to the results from surveys for radio pulsars in GCs and find the number of potentially observable non-recycled radio pulsars present in all clusters to be <3600. Accounting for beaming and retention considerations, the implied birthrate for any formation scenario for all 97 clusters is <0.25 pulsars century{sup -1} assuming a Maxwellian distribution of velocities with a dispersion of 10 km s{sup -1}. The implied birthrates for higher velocity dispersions are substantially higher than inferred for such pulsars in the Galactic disk. This suggests that the velocity dispersion of young pulsars in GCs is significantly lower than those of disk pulsars. These numbers may be substantial overestimates due to the fact that the currently known sample of young pulsars is observed only in metal-rich clusters. We propose that young pulsars may only be formed in GCs with metallicities with log[Fe/H] > - 0.6. In this case, the potentially observable population of such young pulsars is 447{sup +1420}{sub -399} (the error bars give a 95% confidence interval) and their birthrate is 0.012{sup +0.037}{sub -0.010} pulsars century{sup -1}. The most likely creation scenario to explain these pulsars is the electron capture supernova of an OMgNe white dwarf.

Boyles, J.; Lorimer, D. R. [Department of Physics, 210 Hodges Hall, West Virginia University, Morgantown, WV 26506 (United States); Turk, P. J.; Mnatsakanov, R. [Department of Statistics, 423 Hodges Hall, West Virginia University, Morgantown, WV 26506 (United States); Lynch, R. S. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Ransom, S. M. [National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA (United States); Freire, P. C. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel D-53121, Bonn (Germany); Belczynski, K. [Astronomical Observatory, University of Warsaw, AL Ujazdowskie 4,00-478, Warsaw (Poland)

2011-11-20T23:59:59.000Z

273

Feeding Young Horses For Sound Development  

E-Print Network [OSTI]

futurity contenders and for foals entering race training as yearlings, and while size itself is not a marketing factor for some disciplines such as cutting and reining, rigors of early training place great demands on young skeletal systems. Horse owners... and joint problems known as developmental orthopedic diseases (DOD) are a major concern of horse owners. 29 DOD appears to be heritable. 22 Horses with genetic predispositions for large mature size often develop skeletal problems regardless of how...

Gibbs, Pete G.; Potter, Gary D.

2005-05-25T23:59:59.000Z

274

Brown University is an Ivy League school that competes for today's brightest students and faculty. Biomedical Engineering at Brown creates new knowledge and improves human health through cross-disciplinary research  

E-Print Network [OSTI]

. Biomedical Engineering at Brown creates new knowledge and improves human health through cross, Biomechanics/Motion Sciences, Biosensing and Biomolecular Engineering, Biomaterials, and Biomedical device, mentoring the new generation of leaders in biomedical engineering, strong interest in undergraduate

Adams, Mark

275

Irish Astr. J., 27(1), XXXX, (2000) M. D. SMITH EVOLUTIONARY SCHEMES FOR PROTOSTARS, PROTO BROWN DWARFS  

E-Print Network [OSTI]

Irish Astr. J., 27(1), XXXX, (2000) M. D. SMITH EVOLUTIONARY SCHEMES FOR PROTOSTARS, PROTO BROWN DWARFS AND THEIR ENVIRONMENTS M. D. SMITH Armagh Observatory, College Hill, Armagh, N. Ireland, BT61 9DG

276

A T8.5 BROWN DWARF MEMBER OF THE {xi} URSAE MAJORIS SYSTEM  

SciTech Connect (OSTI)

The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper motion with a solar-neighborhood (8 pc) quadruple star system-{xi} Ursae Majoris. The angular separation is 8.'5, and the projected physical separation is Almost-Equal-To 4000 AU. The sub-solar metallicity and low chromospheric activity of {xi} UMa A argue that the system has an age of at least 2 Gyr. The infrared luminosity and color of the brown dwarf suggests the mass of this companion ranges between 14 and 38 M{sub J} for system ages of 2 and 8 Gyr, respectively.

Wright, Edward L.; Mace, Gregory; McLean, Ian S. [UCLA Astronomy, P.O. Box 951547, Los Angeles, CA 90095-1547 (United States); Skrutskie, M. F.; Nelson, M. J.; Borish, H. J. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States); Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L.; Jarrett, Tom [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Marsh, Kenneth A. [School of Physics and Astronomy, Cardiff University, Cardiff CF243AA (United Kingdom); Mainzer, Amanda K.; Eisenhardt, Peter R. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8001 (United States); Tobin, John J. [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Cushing, Michael C., E-mail: wright@astro.ucla.edu [Department of Physics and Astronomy, MS 111, University of Toledo, 2801 W. Bancroft St., Toledo, OH 43606-3328 (United States)

2013-03-15T23:59:59.000Z

277

NEW YOUNG STAR CANDIDATES IN CG4 AND Sa101  

SciTech Connect (OSTI)

The CG4 and Sa101 regions together cover a region of {approx}0.5 deg{sup 2} in the vicinity of a 'cometary globule' that is part of the Gum Nebula. There are seven previously identified young stars in this region; we have searched for new young stars using mid- and far-infrared data (3.6-70 {mu}m) from the Spitzer Space Telescope, combined with ground-based optical data and near-infrared data from the Two Micron All Sky Survey. We find infrared excesses in all six of the previously identified young stars in our maps and identify 16 more candidate young stars based on apparent infrared excesses. Most (73%) of the new young stars are Class II objects. There is a tighter grouping of young stars and young star candidates in the Sa101 region, in contrast to the CG4 region, where there are fewer young stars and young star candidates, and they are more dispersed. Few likely young objects are found in the 'fingers' of the dust being disturbed by the ionization front from the heart of the Gum Nebula.

Rebull, L. M.; Laine, S.; Laher, R.; Legassie, M. [Spitzer Science Center/Caltech, M/S 220-6, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Johnson, C. H. [Breck School Science Department, 123 Ottawa Ave., N., Golden Valley, MN 55422 (United States); Hoette, V. [The University of Chicago Department of Astronomy and Astrophysics, Yerkes Observatory Education and Outreach, 373 W. Geneva St., Williams Bay, WI 53191 (United States); Kim, J. S.; Foster, M. [Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721 (United States); Mallory, C. R. [Department of Astronomy, Pierce College, 6201 Winnetka Ave., Woodland Hills, CA 91371 (United States); McCarron, K. [Science Division, Oak Park and River Forest High School, 201 N. Scoville Ave., Oak Park, IL 60302 (United States); Sherry, W. H., E-mail: luisa.rebull@jpl.nasa.gov [NOAO/NSO, 950 N. Cherry Ave., Tucson, AZ 85719 (United States)

2011-07-15T23:59:59.000Z

278

THE DEPENDENCE OF BROWN DWARF RADII ON ATMOSPHERIC METALLICITY AND CLOUDS: THEORY AND COMPARISON WITH OBSERVATIONS  

SciTech Connect (OSTI)

Employing realistic and consistent atmosphere boundary conditions, we have generated evolutionary models for brown dwarfs and very low mass stars (VLMs) for different atmospheric metallicities ([Fe/H]), with and without clouds. We find that the spread in radius at a given mass and age can be as large as {approx}10% to {approx}25%, with higher-metallicity, higher-cloud-thickness atmospheres resulting quite naturally in larger radii. For each 0.1 dex increase in [Fe/H], radii increase by {approx}1% to {approx}2.5%, depending upon the age and mass. We also find that, while for smaller masses and older ages brown dwarf radii decrease with increasing helium fraction (Y, as expected), for more massive brown dwarfs and a wide range of ages they increase with helium fraction. The increase in radius in going from Y = 0.25 to Y = 0.28 can be as large as {approx}0.025 R{sub J} ({approx}2.5%). Furthermore, we find that for VLMs an increase in atmospheric metallicity from 0.0 to 0.5 dex, increases radii by {approx}4%, and from -0.5 to 0.5 dex by {approx}10%. Therefore, we suggest that opacity due to higher metallicity might naturally account for the apparent radius anomalies in some eclipsing VLM systems. Ten to twenty-five percent variations in radius exceed errors stemming from uncertainties in the equation of state alone. This serves to emphasize that transit and eclipse measurements of brown dwarf radii constrain numerous effects collectively, importantly including the atmosphere and condensate cloud models, and not just the equation of state. At all times, one is testing a multi-parameter theory, and not a universal radius-mass relation.

Burrows, Adam; Nampaisarn, Thane [Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States); Heng, Kevin, E-mail: burrows@astro.princeton.edu, E-mail: tnampais@astro.princeton.edu, E-mail: kheng@phys.ethz.ch [Institute for Advanced Study, School of Natural Sciences, 1 Einstein Drive, Princeton, NJ 08540 (United States)

2011-07-20T23:59:59.000Z

279

A comparison of selected quality and compositional characteristics of brown and white shell eggs  

E-Print Network [OSTI]

for the degree of MASTER OF SCIENCE December 1982 Major Subject: Food Science and Tecnnology A COMPARISON OF SELECTED QUALITI AND COMPOSITIONAL CHARACTERISITICS OF HROWN AND WHITE SHELL EGGS A Thesis by PATRICIA ANN CURTIS Approved as to style... and cortent by: (Chairman of Committee) (Department ead) (Member) -'(, ( ember) ip (Member) December 1982 ABSTRACT A Comparison of Selected Quality and Compositional Characteristics of Brown and White Shell Eggs (December 1982) Patricia Ann Curtis...

Curtis, Patricia Ann

1982-01-01T23:59:59.000Z

280

Productivity and Quality of Brown Midrib (bmr) Sorghum Varieties to Producers in Central America  

E-Print Network [OSTI]

PRODUCTIVITY AND QUALITY OF BROWN MIDRIB (BMR) SORGHUM VARIETIES TO PRODUCERS IN CENTRAL AMERICA A Thesis by OSTILIO ROLANDO PORTILLO RODRIGUEZ Submitted to the Office of Graduate Studies of Texas A&M University in the partial... for Honduras, Guatemala and Nicaragua across several environments. iii ACKNOWLEDGEMENTS I would like to thank God Almighty for his blessings which made this cultural and academic experience at Texas A&M University a reality. I also would like...

Portillo Rodriguez, Ostilio Rolando

2013-05-01T23:59:59.000Z

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


281

Brown snow: A long-range transport event in the Canadian Arctic  

SciTech Connect (OSTI)

The authors document the occurrence of a long-range transport event that deposited thousands of tons of fine particulates on the District of Keewatin, central Canadian Arctic, {approximately}63 N. Air mass trajectories, clay mineral composition, soot particles, and visible organic remains point to Asian sources for the brown snow material, probably western China. Semivolatile organic pollutants detected in the brown snow included polycyclic aromatic hydrocarbons ({Sigma}PAH), PCB congeners, and DDT-related compounds ({Sigma}DDT), polychlorinated camphenes (PCCs), as well as the herbicide trifuluralin and insecticides methoxychlor, endosulfan, and hexachlorocyclohexane (HCH). {Sigma}PAH, PCB, and PCC concentrations were within the range reported in other studies of Arctic snow but {Sigma}DDT levels were 2-10 times higher than previous reports. High molecular weight PAH may have been associated with soot particles in the brown snow but evidence for Asian sources of the pesticides was not strong because of unknown source signal strengths and possible atmospheric transformations of the compounds. Fluxes of these pollutants were also determined by analyzing sediment cores from two small headwater lakes near the sampling site. The quantities of pollutants deposited in this single event may have comprised a significant fraction (>10%) of total annual input {Sigma}PAH and {Sigma}DDT, as determined from lake sedimentation records.

Welch, H.E.; Muir, D.C.G.; Billeck, B.N.; Lockhart, W.L.; Brunskill, G.J.; Kling, H.J. (Freshwater Inst., Winnipeg (Canada)); Olson, M.P. (Atmospheric Environment Service, Downsview, Ontario (Canada)); Lemoine, R.M. (Hardy BBT Ltd., Winnipeg, Manitoba (Canada))

1991-02-01T23:59:59.000Z

282

Humic substances and nitrogen-containing compounds from low rank brown coals  

SciTech Connect (OSTI)

Coal is one of the sources of nitrogen-containing compounds (NCCs). Recovery of NCCs from brown coals in high yield was carried out from tars of stepwise semicoking of brown coals. Humic acids have been shown to contain many types of nitrogen compounds. Humic acids are thought to be complex aromatic macromolecules with amino acids, amino sugars, peptides, and aliphatic compounds that are involved in the linkages between the aromatic groups. Humic acids extracted from peats, brown coals, and lignites, are characterized using different techniques. Humic substances (HSs) have several known benefits to agriculture. The properties of humic substances vary from source to source, because they are heterogeneous mixtures of biochemical degradation products from plant and animal residues, and synthesis activities of microorganisms. HSs have been considered to be a significant floculant in surface water filtration plants for the production of drinking water as well as the processing of water. HSs are produced from chemical and biological degradation of plant and animal residues and from synthetic activities of microorganisms.

Demirbas, A.; Kar, Y.; Deveci, H. [Selcuk University, Konya (Turkey). Department of Chemical Engineering

2006-03-15T23:59:59.000Z

283

Young Inventor Award | GE Global Research  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLasDelivered energy consumption byAbout SRNL HomeYoung Inventor Shares His Award-Winning

284

I'm Too Young for This: Adolescent and Young Adult Cancer Survivorship  

E-Print Network [OSTI]

As of January 1, 2012, an estimated 13.7 million cancer survivors were alive in the United States. The number of cancer survivors is expected to reach 18 million by the year 2022. Adolescent and Young Adult (AYA) cancer survivors, ages 15-39, are a...

Vollmer Dahlke, Deborah

2014-07-25T23:59:59.000Z

285

Stroke in young women: an interpretive phenomenological analysis.  

E-Print Network [OSTI]

??A comprehensive picture of the psychosocial consequences of stroke in young adults, that is grounded in the experience and perspective of stroke survivors, is currently… (more)

Leahy, Dorothy Maria

2010-01-01T23:59:59.000Z

286

active young females: Topics by E-print Network  

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

Consumer Vulnerability in the Web Physics Websites Summary: Vulnerability in the Web 2.0 Society Abstract The young consumers constitute one of the fastest growing Internet:...

287

asymptomatic young adults: Topics by E-print Network  

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

Consumer Vulnerability in the Web Physics Websites Summary: Vulnerability in the Web 2.0 Society Abstract The young consumers constitute one of the fastest growing Internet:...

288

Microsoft Word - SNOPUD_Youngs_Cr_Hydro_CX_+_Checklist.doc  

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

Interconnection of Snohomish County Public Utility District No.1 (SNOPUD) Young's Creek Hydro Small Generation Budget Information: WO 00231295, Task 01 Categorical Exclusion...

289

australian young adults: Topics by E-print Network  

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

theatre to construct a participatory creative space for Indigenous Australian young people . Open Access Theses and Dissertations Summary: ??This thesis investigates the use of...

290

Identification of a mutation in the tyrosinase related protein 1 (TRP1) gene associated with brown oculocutaneous albinism (OCA3)  

SciTech Connect (OSTI)

The genes responsible for the two most common types of human oculocutaneous albinism (OCA) have been identified. Mutations of the tyrosinase gene (chromosome 11q14-21) produce OCA1, and mutations of the P gene (chromosome 15q11.2-13) produce OCA2. Another type of OCA known as brown OCA or OCA3 is found commonly in the African and African-American population. OCA3 is characterized by light brown skin and hair with the ocular features of albinism and represents the third most frequent type of OCA. We previously identified dizygotic African-American twin boys who were discordant for OCA3. Melanocytes from the affected twin produced brown melanin and contained no detectable TRP1 protein. We have now characterized the TRP1 gene from the affected twin. The human TRP1 gene, homologous to the murine brown locus, contains 8 exons and maps to chromosome 9p23. Using PCR amplification of each exon coupled with SSCP analysis and direct DNA sequencing, we found the affected twin to homozygous for a single bp deletion in exon 6. The deletion removes a G in codon 368 leading to a premature stop at codon 384. We also identified a Tsp509 polymorphism in the 3{prime} UTR. We conclude that mutations of the TRP1 gene are responsible for brown OCA or OCA3, making this the third major OCA gene identified in humans.

Wildenberg, S.C.; Oetting, W.S.; Fryer, J.P. [Univ. of Minnesota, Minneapolis, MN (United States)] [and others

1994-09-01T23:59:59.000Z

291

A Herschel PACS survey of brown dwarfs in IC 2391: Limits on primordial and debris disk fractions  

E-Print Network [OSTI]

We present results from a Herschel PACS survey of 8 brown dwarfs in the IC 2391 cluster. Our aim was to determine the brown dwarf disk fraction at ages of ~40-50 Myr. None of the 8 brown dwarfs observed were detected in the PACS 70 or 160mu bands. We have determined the detection limits of our survey using the 1-sigma flux upper limits in the PACS far-infrared and the WISE mid-infrared bands. The sensitivity of our observations would only allow for the detection of debris disks with exceptionally large fractional luminosities (>1%). Considering that only the most extreme and rare debris disks have such high fractional luminosities, it can be hypothesized that Vega-like debris disks, as observed around ~30% of low-mass stars at similar ages, could exist around the targeted IC 2391 brown dwarfs. Most primordial disks similar to the ones observed for the younger 1-10 Myr brown dwarfs would be within the detection sensitivities of our survey, and could have been detected. The non-detection for all targets then su...

Riaz, B

2014-01-01T23:59:59.000Z

292

Brigham Young University Geology Studies Volume 26, Part I  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 26, Part I Papers presented at the 31st annual meeting, Rocky Mountain Section, Geological Society of America, April 28-29, 1978, at Brig- ham Young ............................................................................................................................Publications and Maps of the Geology Department 91 Cover The Great Basrn seen from a htgh

Seamons, Kent E.

293

Brigham Young University Geology Studies Volume 25, Part 3  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 25, Part 3 CONTENTS Remains of Ornithopod ...........................................................................................................................................................ames M. Stolle Publications and Maps of the Geology Department Index to volumes 21-25 of Brigham Young University Geology Studies ........................................Carol T . Smith and Nathan M. Smith Cwec

Seamons, Kent E.

294

Brigham Young University Geology Studies Volume 26, Part 2  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 26, Part 2 CONTENTS A New Large Theropod................................................................................................................................................................ Danny J. Wyatt Publications and Maps of the Geology Department Cover: Cretaceouscoals near Castle Gate, Utab. #12;A publication of the Department of Geology Brigham Young University Provo, Utah 84602 Editors

Seamons, Kent E.

295

Brigham Young University Geology Studies Volume 26, Part 3  

E-Print Network [OSTI]

#12;P I - #12;Brigham Young University Geology Studies Volume 26, Part 3 Conodont Biostratigraphy-meeting field trip held in conjunction with the Rocky Mountain section, Geological Society of America of the Department of Geology Brigham Young University Provo, Utah 84602 Editors W. Kenneth Hamblin Cynthia M

Seamons, Kent E.

296

RESIDUAL STRESS AND YOUNG'S MODULUS MEASUREMENT OF CAPACITIVE MICROMACHINED ULTRASONIC  

E-Print Network [OSTI]

deposition technique yields residual stress of around 100 MPa and Young's modulus of around 300 GPa. Keywords's modulus, Poisson's ratio, and residual stress of the deposited thin films. In this paper, we propose a newRESIDUAL STRESS AND YOUNG'S MODULUS MEASUREMENT OF CAPACITIVE MICROMACHINED ULTRASONIC TRANSDUCER

Khuri-Yakub, Butrus T. "Pierre"

297

SED modeling of Young Massive Stars  

E-Print Network [OSTI]

In this contribution, I review the applications and potential limitations of the spectral energy distribution fitting tool that I have developed, with a strong emphasis on the limits to which this tool can be used to improve our understanding of massive star formation. I discuss why our current grid of models cannot be used to distinguish between the several competing theories of massive star formation. I also discuss stellar mass determinations, artificial correlations between parameters in the grid of models, multiplicity, confusion, dust assumptions, and unique fits. I briefly review the improvements we intend to carry out for our next grid of models, which will eliminate many of these limitations. Finally, I show examples of applications of this tool to massive young stars.

Thomas P. Robitaille

2007-11-27T23:59:59.000Z

298

Extended emission associated with young HII regions  

E-Print Network [OSTI]

We have used the Australia Telescope Compact Array (ATCA) to make observations of a sample of eight young ultra-compact HII regions, selected on the basis that they have associated class II methanol maser emission. We have made observations sensitive to both compact and extended structures and find both to be present in most sources. The scale of the extended emission in our sample is in general less than that observed towards samples based on IRAS properties, or large single-dish flux densities. Our observations are consistent with a scenario where extended and compact radio continuum emission coexists within HII regions for a significant period of time. We suggest that these observations are consistent with a model where HII evolution takes place within hierarchically structured molecular clouds. This model is the subject of a companion paper (Shabala et al. 2005) and addresses both the association between compact and extended emission and UCHII region lifetime problem.

S. P. Ellingsen; S. S. Shabala; S. E. Kurtz

2004-12-06T23:59:59.000Z

299

Composition of the wax fraction of bitumen from methylated brown coals  

SciTech Connect (OSTI)

Changes in the group and individual compositions of the wax fractions of bitumen in the course of brown coal methylation were studied. With the use of IR and NMR spectroscopy and chromatography-mass spectrometry, it was found that the esters of methylated coal waxes consisted of the native esters of fatty acids and the methyl esters of these acids formed as a result of an alkylation treatment. Esterification and transesterification were predominant among the reactions of aliphatic fraction components. A positive effect of methanol alkylation on an increase in the yield of the aliphatic fractions was found.

S.I. Zherebtsov; A.I. Moiseev [Russian Academy of Sciences, Kemerovo (Russian Federation). Institute of Coal and Coal Chemistry

2009-04-15T23:59:59.000Z

300

SciTech Connect: Brown Grease to Biodiesel Demonstration Project Report  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administrationcontroller systems controllerAdditiveBetatron Radiation from aBrown Grease to

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


301

Induction of micronuclei and nuclear abnormalities in the erythrocytes of mudminnows (Umbra limi) and brown bullheads (Ictalurus nebulosus)  

SciTech Connect (OSTI)

The authors are interested in determining whether the MN technique can be developed as an in situ assay for genotoxicity in fish species; and in particular, the brown bullhead (Ictalurus nebulosus). In this study, central mudminnows (Umbra limi) and brown bullheads were exposed to EMS and benzo(a)pyrene (BaP) by intraperitoneal injection. The various experiments were designed to: i) compare the sensitivity of the MN and SCE assays using the mudminnow model; ii) determine whether MN are induced in the erythrocytes of the brown bullhead by exposure to genotoxic chemicals (EMS and BaP); iii) determine whether erythrocytes harvested from the erythropoietic tissues of fish (pronephros) have a greater incidence of MN than peripheral erythrocytes; iv) examine the association between the induction of MN and the induction of nuclear abnormalities in erythrocytes after exposure of genotoxic agents.

Metcalfe, C.D.

1988-04-01T23:59:59.000Z

302

Antagonist effect between violaxanthin and de-epoxidated pigments in nonphotochemical quenching induction in the qE deficient brown alga  

E-Print Network [OSTI]

induction in the qE deficient brown alga Macrocystis pyrifera HĂ©ctor Ocampo-Alvarez a , Ernesto GarcĂ­aZ) De-epoxidation rate control Brown alga Macrocystis pyrifera Nonphotochemical quenching (NPQ quenching (qE), is not present in this alga. In contrast to higher plants, NPQ in this organism is much more

Govindjee

303

Miller, K.G., Sugarman, P.J., Browning, J.V., et al., 1998 Proceedings of the Ocean Drilling Program, Initial Reports, Vol. 174AX  

E-Print Network [OSTI]

,4 James V. Browning,2 Richard K. Olsson,2 Stephen F. Pekar,2 Timothy J. Reilly,2 Benjamin S. Cramer,2 Uptegrove,4 David Bukry,8 Lloyd H. Burckle,3 James D. Wright,9 Mark D. Feigenson,2 Gilbert J. Brenner,10, Olsson, Pekar, Reilly, Stewart, Uptegrove Biostratigraphy: Foraminifers: Browning, Olsson, Pekar

304

The vibrationally mediated photodissociation of Cl2 E. K. Campbell, A. B. Alekseyev, G. G. Balint-Kurti, M. Brouard, Alex Brown et al.  

E-Print Network [OSTI]

of Cl2 E. K. Campbell,1 A. B. Alekseyev,2 G. G. Balint-Kurti,3 M. Brouard,1,a) Alex Brown,4 R. JThe vibrationally mediated photodissociation of Cl2 E. K. Campbell, A. B. Alekseyev, G. G. Balint-Kurti, M. Brouard, Alex Brown et al. Citation: J. Chem. Phys. 137, 124310 (2012); doi: 10

Brown, Alex

305

The First Science Results from SPHERE: Disproving the Predicted Brown Dwarf around V471 Tau  

E-Print Network [OSTI]

Variations of eclipse arrival times have recently been detected in several post common envelope binaries consisting of a white dwarf and a main sequence companion star. The generally favoured explanation for these timing variations is the gravitational pull of one or more circumbinary substellar objects periodically moving the center of mass of the host binary. Using the new extreme-AO instrument SPHERE, we image the prototype eclipsing post-common envelope binary V471 Tau in search of the brown dwarf that is believed to be responsible for variations in its eclipse arrival times. We report that an unprecedented contrast of 12.1 magnitudes in the H band at a separation of 260 mas was achieved, but resulted in a non-detection. This implies that there is no brown dwarf present in the system unless it is three magnitudes fainter than predicted by evolutionary track models, and provides damaging evidence against the circumbinary interpretation of eclipse timing variations. In the case of V471 Tau, a more consisten...

Hardy, A; Parsons, S G; Caceres, C; Retamales, G; Wahhaj, Z; Mawet, D; Canovas, H; Cieza, L; Marsh, T R; Bours, M C P; Dhillon, V S; Bayo, A

2015-01-01T23:59:59.000Z

306

A HYBRID SCENARIO FOR THE FORMATION OF BROWN DWARFS AND VERY LOW MASS STARS  

SciTech Connect (OSTI)

We present a calculation of protostellar disk formation and evolution in which gaseous clumps (essentially, the first Larson cores formed via disk fragmentation) are ejected from the disk during the early stage of evolution. This is a universal process related to the phenomenon of ejection in multiple systems of point masses. However, it occurs in our model entirely due to the interaction of compact, gravitationally bound gaseous clumps and is free from the smoothing-length uncertainty that is characteristic of models using sink particles. Clumps that survive ejection span a mass range of 0.08-0.35 M{sub Sun }, and have ejection velocities 0.8 {+-} 0.35 km s{sup -1}, which are several times greater than the escape speed. We suggest that, upon contraction, these clumps can form substellar or low-mass stellar objects with notable disks, or even close-separation very low mass binaries. In this hybrid scenario, allowing for ejection of clumps rather than finished protostars/proto-brown-dwarfs, disk formation and the low velocity dispersion of low-mass objects are naturally explained, while it is also consistent with the observation of isolated low-mass clumps that are ejection products. We conclude that clump ejection and the formation of isolated low-mass stellar and substellar objects is a common occurrence, with important implications for understanding the initial mass function, the brown dwarf desert, and the formation of stars in all environments and epochs.

Basu, Shantanu [Department of Physics and Astronomy, University of Western Ontario, London, Ontario, N6A 3K7 (Canada); Vorobyov, Eduard I., E-mail: basu@uwo.ca, E-mail: eduard.vorobiev@univie.ac.at [Institute of Astrophysics, The University of Vienna, Vienna, 1180 (Austria)

2012-05-01T23:59:59.000Z

307

Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer  

E-Print Network [OSTI]

We present a sample of brown dwarfs identified with the {\\it Wide-field Infrared Survey Explorer} (WISE) for which we have obtained {\\it Hubble Space Telescope} ({\\it HST}) Wide Field Camera 3 (WFC3) near-infrared grism spectroscopy. The sample (twenty-two in total) was observed with the G141 grism covering 1.10$-$1.70 $\\mu$m, while fifteen were also observed with the G102 grism, which covers 0.90$-$1.10 $\\mu$m. The additional wavelength coverage provided by the G102 grism allows us to 1) search for spectroscopic features predicted to emerge at low effective temperatures (e.g.\\ ammonia bands) and 2) construct a smooth spectral sequence across the T/Y boundary. We find no evidence of absorption due to ammonia in the G102 spectra. Six of these brown dwarfs are new discoveries, three of which are found to have spectral types of T8 or T9. The remaining three, WISE J082507.35$+$280548.5 (Y0.5), WISE J120604.38$+$840110.6 (Y0), and WISE J235402.77$+$024015.0 (Y1) are the nineteenth, twentieth, and twenty-first spec...

Schneider, Adam C; Kirkpatrick, J Davy; Gelino, Christopher R; Mace, Gregory N; Wright, Edward L; Eisenhardt, Peter R; Skrutskie, M F; Griffith, Roger L; Marsh, Kenneth A

2015-01-01T23:59:59.000Z

308

Brown - leaves  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAboutScienceCareers ApplyResistant:NOAA-EPA UV BrewerandAaSymposiumSector

309

Brown - leaves  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAboutScienceCareers ApplyResistant:NOAA-EPA UV

310

City of Dallas Green Building Case Study  

E-Print Network [OSTI]

of the city?s green building and energy management policies ?Update of green building policy in 2006 to require a minimum compliance of LEED Gold and incorporation of carbon neutrality goals ? Implementation of training programs on sustainability for city... Roofs for slopes 2:12 or less to meet EPA ENERGY STAR, or ? Install a green/vegetated roof that covers at least 50% of the roof area with the remainder following the Cool Roof requirement for slopes 2:12 or less ?Outdoor Lighting restriction 14...

Basora, Z.

2012-01-01T23:59:59.000Z

311

Dallas, Texas: 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 Office of InspectorConcentratingRenewable Solutions LLC JumpCrow Lake Wind107 CX at North BrawleyDNADTETexas:

312

Jefferson Lab Leadership Council - Michael Dallas  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation ProposedUsingFunInfraredJefferson Lab Click onLaser Twinkles in RareMichaelChief Operating

313

Jefferson Lab Leadership Council - Michael Dallas  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation ProposedUsingFunInfraredJefferson Lab Click onLaser Twinkles in RareMichaelChief

314

Brigham Young University Geology Studies Volume 28, Part 3  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 28, Part 3 CONTENTS Three Creeks Caldera ................................................................................................................................... Scott Dean Geology of the Antelope Peak Area of the Southern .................................................................................................................. Craig D. Hall Geology of the Longlick and White Mountain Area, Southern San Francisco Mountains

Seamons, Kent E.

315

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I  

E-Print Network [OSTI]

#12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I Preble Formation, a Cambrian Outer ..........................................................................J. Roger Olsen Geology of the Sterling Quadrangle, Sanpete County, Utah ..............................................................................James Michael Taylor Publications and Maps of the Geology Department Cover: Aertalphorograph rhowing

Seamons, Kent E.

316

Young children selectively seek and offer help when solving problems  

E-Print Network [OSTI]

and other-oriented help-providers. Current Psychology, 17(2-M. (2008). Sex-differences in help-seeking appear in early1995). Young children’s help-seeking in mastery oriented

Cluver, Annette Lynne

2010-01-01T23:59:59.000Z

317

Acceleration of wound healing in young and aged rats  

E-Print Network [OSTI]

in senescence, and that macrophage activation or supplementation may yield an acceleration in wound closure. This thesis focuses on the ability of Acemannan (ACM), a complex plant carbohydrate and macrophage stimulator, to accelerate wound healing in both young...

Maxwell, Bryan Douglas

1996-01-01T23:59:59.000Z

318

BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL  

E-Print Network [OSTI]

-6) ...........................................................13 C. Credit for Co-Curricular (Law 793R §§1BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL Policies and Procedures March 2013 #12;Table ................................................................................1 C. Speakers

Seamons, Kent E.

319

BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL  

E-Print Network [OSTI]

-6) ...........................................................13 C. Credit for Co-Curricular (Law 793R §§1BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL Policies and Procedures November 2012 #12;Table ................................................................................1 C. Speakers

Seamons, Kent E.

320

BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL  

E-Print Network [OSTI]

-6) ...........................................................13 C. Credit for Co-Curricular (Law 793R §§1BRIGHAM YOUNG UNIVERSITY J. REUBEN CLARK LAW SCHOOL Policies and Procedures September 2011 (Revised ................................................................................1 C. Speakers

Seamons, Kent E.

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


321

Arsenic Modulates Cell Proliferation Pathways in MCF-7 Breast Cancer Cells Krystle Brown, Somaly Neang, Dorrelyn Patacsil, and Deepak Kumar  

E-Print Network [OSTI]

Viability Assay: The cell viability and proliferation of MCF-7 breast cancer cell lines were determined (SDS-PAGE) and Western Blotting. Figure 2. MCF-7 breast cancer cell lines were treated with variousArsenic Modulates Cell Proliferation Pathways in MCF-7 Breast Cancer Cells Krystle Brown, Somaly

District of Columbia, University of the

322

STATE OF CALIFORNIA --THE RESOURCES AGENCY Edmund G. Brown Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814  

E-Print Network [OSTI]

, on paper, and orally at Energy Commission hearings. A. A Brief History of the Energy Commission's BuildingSTATE OF CALIFORNIA -- THE RESOURCES AGENCY Edmund G. Brown Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov INITIAL STATEMENT

323

STATE OF CALIFORNIA --THE RESOURCES PROVIDER Edmund G. Brown Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814  

E-Print Network [OSTI]

electronically, on paper, and orally at Energy Commission hearings. A. A Brief History of the Energy Commission1 STATE OF CALIFORNIA -- THE RESOURCES PROVIDER Edmund G. Brown Jr., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov INITIAL STATEMENT

324

DISTINCT PATTERNS OF NITRATE REDUCTASE ACTIVITY IN BROWN ALGAE: LIGHT AND AMMONIUM SENSITIVITY IN LAMINARIA DIGITATA IS ABSENT IN  

E-Print Network [OSTI]

DISTINCT PATTERNS OF NITRATE REDUCTASE ACTIVITY IN BROWN ALGAE: LIGHT AND AMMONIUM SENSITIVITY and lowest in summer. This is the first report of NR activity in any alga that is not strongly regulated the regulation of NR by light that has been observed in other algae and higher plants. Key index words: ammonium

Berges, John A.

325

Safety Meeting Minutes, July 2, 2008 Members Present: Randy Walker, Hollis Lundeen, Devin Brakob, Rick Brown, Ann  

E-Print Network [OSTI]

Safety Meeting Minutes, July 2, 2008 Members Present: Randy Walker, Hollis Lundeen, Devin Brakob, Rick Brown, Ann Byer, Steve Hammond, Michelle Ottmar and Vlada Gertseva Ann Byer, Safety Compliance officer from National Marine Fisheries Services came to the meeting and outlined the safety review

326

Is the Extended Red Emission due to CO? Philip D. Bennett, Graham M. Harper, and Alexander Brown  

E-Print Network [OSTI]

Is the Extended Red Emission due to CO? Philip D. Bennett, Graham M. Harper, and Alexander Brown. The Extended Red Emission (ERE) is a broad emission feature ob­ served between 5000 and 8000 ƥ A in a large to be correct. The strongest known source of the ERE is the bipolar nebula (the ``Red Rect­ angle'') associated

Harper, Graham

327

A Textile Information Resource for Extension Agents and 4-H Leaders Pamela J. Brown, Ph.D.  

E-Print Network [OSTI]

FIBERS A Textile Information Resource for Extension Agents and 4-H Leaders 1999 Pamela J. Brown, Ph cotton tree -lightweight, soft fiber -with use, has a tendency to break down into a powder -used Abaca -obtained from a member of the banana tree family; sometimes referred to as Manila hemp -produced

328

Probing Structural Dynamics with High Spatial and Temporal Resolution Research Team: Nigel Browning, James Evans, Patricia Abellan, Russell Tonkyn  

E-Print Network [OSTI]

Probing Structural Dynamics with High Spatial and Temporal Resolution Research Team: Nigel Browning of the structural dynamics that occur on the ”s-ns timescale We will make use of a unique aberration-corrected dynamic TEM (DTEM), where a photoemission source will enable these time-resolved images to be obtained at

329

Lithium: Measurement of Young's Modulus and Yield Strength  

SciTech Connect (OSTI)

The Lithium Collection Lens is used for anti-proton collection. In analyzing the structural behavior during operation, various material properties of lithium are often needed. properties such as density, coefficient of thermal expansion, thermal conductivity, specific heat, compressability, etc.; are well known. However, to the authors knowledge there is only one published source for Young's Modulus. This paper reviews the results from the testing of Young's Modulus and the yield strength of lithium at room temperature.

Ryan P Schultz

2002-11-07T23:59:59.000Z

330

X-ray Detection from Bona-fide and Candidate Brown Dwarfs in the Rho Ophiuchi Cloud with Chandra  

E-Print Network [OSTI]

We present results of an X-ray search from bona-fide and candidate brown dwarfs in the Rho Ophiuchi cloud cores with the Chandra X-ray Observatory. The selected areas are two fields near the cloud center and are observed with the ACIS-I array of a 17'x17' size and a ~100 ks exposure. Among 18 bona-fide and candidate brown dwarfs listed by the infrared spectroscopy, we find X-ray emission from 7 sources above 99.9% confidence level. Therefore ~40% of the infrared-selected brown dwarfs in this cloud emit X-rays. For the brightest 4 sources, the X-ray spectra are made and are fitted with a thin-thermal plasma model of a temperature 1-2.5 keV. The X-rays are also time variable with rapid flares from 2 of the brown dwarfs. Assuming 2 keV temperature and using the empirical relation of Av vs. NH, we estimate the X-ray luminosity or its upper limit of the other faint or non-X-ray sources. The X-ray luminosity (Lx) of the X-ray-detected sources is in the range of 0.3-90x10^28 ergs s^-1, while the luminosity ratio of X-ray to bolometric (Lx/Lbol) is 10^-3 - 10^-5, similar to those of low-mass pre-main-sequence and dMe stars. All these results suggest that the X-ray origin of brown dwarfs is the same as low-mass stars; strong magnetic activity at the stellar surface.

Kensuke Imanishi; Masahiro Tsujimoto; Katsuji Koyama

2001-08-06T23:59:59.000Z

331

A Possible Brown Dwarf Companion to the White Dwarf GD1400  

E-Print Network [OSTI]

An unresolved, likely L dwarf companion to the DA white dwarf GD1400 is reported. This would be only the second such system known, discovered 17 years after the prototype L dwarf, GD165B, was determined to be a companion to a white dwarf. Photometric observations and model predicted stellar parameters of the well studied white dwarf primary indicate that GD1400B has $J-K\\ga2.0$ and $M_K=12.13$ mag. If correct, this would place GD1400B at spectral type L6, and it would be the lowest luminosity unevolved companion known to a white dwarf, and thus a definite brown dwarf. However, a low resolution Keck NIRSPEC $2.1-2.4\\mu$m spectrum may not be consistent with known L dwarfs. Uncertainties in classification remain until the binary is resolved or a trigonometric parallax is measured.

J. Farihi; M. Christopher

2004-07-01T23:59:59.000Z

332

Active reagents from brown coal and hydrolysis lignin and their interaction with calcium phosphates  

SciTech Connect (OSTI)

A method has been developed for producing active reagents from brown coal and hydrolysis lignin by their oxidation with dilute nitric acid. The products obtained contain up to 30 and 46% respectively of humic acids with active functional groups. Reactions of oxidized and ammoniated coal with mono,- di-, and tricalcium phosphate have also been studied. The variation of the composition and yield of the reaction products with the ratio of the substances taken have been investigated. It has been found that the addition of oxidized coal to mono-, di-, and tricalcium phosphate raised the quantity of the water-soluble P/sub 2/O/sub 5/ froms, i.e., this hinders phosphorous fixation in the soil.

Rubinchik, G.F.; Adylkhodzhaeva, T.A.; Tadzhiev, A.T.

1985-09-01T23:59:59.000Z

333

Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945  

E-Print Network [OSTI]

We present evolutionary models for cool brown dwarfs and extra-solar giant planets. The models reproduce the main trends of observed methane dwarfs in near-IR color-magnitude diagrams. We also present evolutionary models for irradiated planets, coupling for the first time irradiated atmosphere profiles and inner structures. We focus on HD 209458-like systems and show that irradiation effects can substantially affect the radius of sub-jovian mass giant planets. Irradiation effects, however, cannot alone explain the large observed radius of HD 209458b. Adopting assumptions which optimise irradiation effects and taking into account the extension of the outer atmospheric layers, we still find $\\sim$ 20% discrepancy between observed and theoretical radii. An extra source of energy seems to be required to explain the observed value of the first transit planet.

I. Baraffe; G. Chabrier; T. Barman; F. Allard; P. H. Hauschildt

2003-02-14T23:59:59.000Z

334

IONIZATION IN ATMOSPHERES OF BROWN DWARFS AND EXTRASOLAR PLANETS. III. BREAKDOWN CONDITIONS FOR MINERAL CLOUDS  

SciTech Connect (OSTI)

Electric discharges were detected directly in the cloudy atmospheres of Earth, Jupiter, and Saturn, are debatable for Venus, and indirectly inferred for Neptune and Uranus in our solar system. Sprites (and other types of transient luminous events) have been detected only on Earth, and are theoretically predicted for Jupiter, Saturn, and Venus. Cloud formation is a common phenomenon in ultra-cool atmospheres such as in brown dwarf and extrasolar planetary atmospheres. Cloud particles can be expected to carry considerable charges which may trigger discharge events via small-scale processes between individual cloud particles (intra-cloud discharges) or large-scale processes between clouds (inter-cloud discharges). We investigate electrostatic breakdown characteristics, like critical field strengths and critical charge densities per surface, to demonstrate under which conditions mineral clouds undergo electric discharge events which may trigger or be responsible for sporadic X-ray emission. We apply results from our kinetic dust cloud formation model that is part of the DRIFT-PHOENIX model atmosphere simulations. We present a first investigation of the dependence of the breakdown conditions in brown dwarf and giant gas exoplanets on the local gas-phase chemistry, the effective temperature, and primordial gas-phase metallicity. Our results suggest that different intra-cloud discharge processes dominate at different heights inside mineral clouds: local coronal (point discharges) and small-scale sparks at the bottom region of the cloud where the gas density is high, and flow discharges and large-scale sparks near, and maybe above, the cloud top. The comparison of the thermal degree of ionization and the number density of cloud particles allows us to suggest the efficiency with which discharges will occur in planetary atmospheres.

Helling, Ch.; Jardine, M.; Stark, C. [SUPA, School of Physics and Astronomy, University of St. Andrews, St. Andrews KY16 9SS (United Kingdom); Diver, D., E-mail: ch@leap2010.eu [SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ (United Kingdom)

2013-04-20T23:59:59.000Z

335

Are red 2MASS QSOs young?  

E-Print Network [OSTI]

We use photometric data from Spitzer to explore the mid- and far-IR properties of 10 red QSOs (J-K>2, R-K>5) selected by combining the 2MASS in the NIR with the SDSS at optical wavelengths. Optical and/or near-infrared spectra are available for 8/10 sources. Modeling the SED from UV to far-IR shows that moderate dust reddening (A_V=1.3-3.2) can explain the red optical and near-IR colours of the sources in the sample. There is also evidence that red QSOs have 60/12micron luminosity ratio higher than PG QSOs (97% significance). This can be interpreted as a higher level of star-formation in these systems (measured by the 60micron luminosity) for a given AGN power (approximated by the 12micron luminosity). This is consistent with a picture where red QSOs represent an early phase of AGN evolution, when the supermassive black hole is enshrouded in dust and gas clouds, which will eventually be blown out (possibly by AGN driven outflows) and the system will appear as typical optically luminous QSO. There is also tentative evidence significant at the 96% level that red 2MASS QSOs are more often associated with radio emission than optically selected SDSS QSOs. This may indicate outflows, also consistent with the young AGN interpretation. We also estimate the space density of red QSOs relative to optically selected SDSS QSOs, taking into account the effect of dust extinction and the intrinsic luminosity of the sources. We estimate that the fraction of red QSOs in the overall population increases from 3% at M_K=-27.5mag to 12% at M_K=-29.5mag. This suggests that reddened QSOs become more important at the bright end of the Luminosity Function. If red QSOs are transition objects on the way to becoming typical optically luminous QSOs, the low fractions above suggest that these systems spent <12% of their lifetime at the "reddened" stage.

A. Georgakakis; D. L. Clements; G. Bendo; M. Rowan-Robinson; K. Nandra; M. S. Brotherton

2008-12-10T23:59:59.000Z

336

510 Plant Disease / Vol. 97 No. 4 Etiology of Moldy Core, Core Browning, and Core Rot of Fuji Apple in China  

E-Print Network [OSTI]

Province, 712000, P. R. China; and Alan R. Biggs, Kearneysville Tree Fruit Research and Education Center., Zhang, R., Sun, G. Y., Zha, Y. L., and Biggs, A. R. 2013. Etiology of moldy core, core browning

Biggs, Alan R.

337

Field Testing of Activated Carbon Injection Options for Mercury Control at TXU's Big Brown Station  

SciTech Connect (OSTI)

The primary objective of the project was to evaluate the long-term feasibility of using activated carbon injection (ACI) options to effectively reduce mercury emissions from Texas electric generation plants in which a blend of lignite and subbituminous coal is fired. Field testing of ACI options was performed on one-quarter of Unit 2 at TXU's Big Brown Steam Electric Station. Unit 2 has a design output of 600 MW and burns a blend of 70% Texas Gulf Coast lignite and 30% subbituminous Powder River Basin coal. Big Brown employs a COHPAC configuration, i.e., high air-to-cloth baghouses following cold-side electrostatic precipitators (ESPs), for particulate control. When sorbent injection is added between the ESP and the baghouse, the combined technology is referred to as TOXECON{trademark} and is patented by the Electric Power Research Institute in the United States. Key benefits of the TOXECON configuration include better mass transfer characteristics of a fabric filter compared to an ESP for mercury capture and contamination of only a small percentage of the fly ash with AC. The field testing consisted of a baseline sampling period, a parametric screening of three sorbent injection options, and a month long test with a single mercury control technology. During the baseline sampling, native mercury removal was observed to be less than 10%. Parametric testing was conducted for three sorbent injection options: injection of standard AC alone; injection of an EERC sorbent enhancement additive, SEA4, with ACI; and injection of an EERC enhanced AC. Injection rates were determined for all of the options to achieve the minimum target of 55% mercury removal as well as for higher removals approaching 90%. Some of the higher injection rates were not sustainable because of increased differential pressure across the test baghouse module. After completion of the parametric testing, a month long test was conducted using the enhanced AC at a nominal rate of 1.5 lb/Macf. During the time that enhanced AC was injected, the average mercury removal for the month long test was approximately 74% across the test baghouse module. ACI was interrupted frequently during the month long test because the test baghouse module was bypassed frequently to relieve differential pressure. The high air-to-cloth ratio of operations at this unit results in significant differential pressure, and thus there was little operating margin before encountering differential pressure limits, especially at high loads. This limited the use of sorbent injection as the added material contributes to the overall differential pressure. This finding limits sustainable injection of AC without appropriate modifications to the plant or its operations. Handling and storage issues were observed for the TOXECON ash-AC mixture. Malfunctioning equipment led to baghouse dust hopper plugging, and storage of the stagnant material at flue gas temperatures resulted in self-heating and ignition of the AC in the ash. In the hoppers that worked properly, no such problems were reported. Economics of mercury control at Big Brown were estimated for as-tested scenarios and scenarios incorporating changes to allow sustainable operation. This project was funded under the U.S. Department of Energy National Energy Technology Laboratory project entitled 'Large-Scale Mercury Control Technology Field Testing Program--Phase II'.

John Pavlish; Jeffrey Thompson; Christopher Martin; Mark Musich; Lucinda Hamre

2009-01-07T23:59:59.000Z

338

A review of "The Sale of the Century: Artistic Relations between Spain and Great Britain, 1604-1655." by Jonathan Brown and John Elliott, eds.  

E-Print Network [OSTI]

. Jonathan Brown and John Elliott, eds. The Sale of the Century: Ar- tistic Relations between Spain and Great Britain, 1604?1655. Madrid: Yale University Press and Museo Nacional del Prado, 2002. 315 pp. $65 hardback. Review by ELIZABETH R. WRIGHT..., UNIVERSITY OF GEORGIA. Art historian Jonathan Brown and historian John Elliott have joined forces to provide an indispensable guide to the political and artistic relationship between Spain and England in the first half of the seventeenth century. Though...

Elizabeth R. Wright

2003-01-01T23:59:59.000Z

339

On the limiting behavior of the Brown-York quasi-local mass in asymptotically hyperbolic manifolds  

E-Print Network [OSTI]

We show that the limit at infinity of the vector-valued Brown-York-type quasi-local mass along any coordinate exhaustion of an asymptotically hyperbolic $3$-manifold satisfying the relevant energy condition on the scalar curvature has the conjectured causal character. Our proof uses spinors and relies on a Witten-type formula expressing the asymptotic limit of this quasi-local mass as a bulk integral which manifestly has the right sign under the above assumptions. In the spirit of recent work by Hijazi, Montiel and Raulot, we also provide another proof of this result which uses the theory of boundary value problems for Dirac operators on compact domains to show that a certain quasi-local mass, which converges to the Brown-York mass in the asymptotic limit, has the expected causal character under suitable geometric assumptions.

Ezequiel Barbosa; Levi Lopes de Lima; Frederico Girăo

2014-07-02T23:59:59.000Z

340

A simulation model of brown shrimp (Penaeus aztecus Ives) growth, movement, and survival in Galveston Bay, Texas  

E-Print Network [OSTI]

. Factors likely affecting recruitment of postlarval brown shrimp from the Gulf to the estuaries and bays include seasonality, water movement, and water temperature. In the model, recruitment is represented explicitly by wind conditions and water... of shrimp emigrating from the bays to the Gulf of Mexico. Environmental Submodels Three environmental conditons, water temperature, wind direction, and wind velocity were found to be significant in describing recruitment, growth, and natural mortality...

George, Leroy Conrad

1981-01-01T23:59:59.000Z

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341

Azimuthally sensitive hanbury brown-twiss interferometry in Au + Au collisions sqrt S sub NN = 200 GeV  

SciTech Connect (OSTI)

We present the results of a systematic study of the shape of the pion distribution in coordinate space at freeze-out in Au+Au collisions at RHIC using two-pion Hanbury Brown-Twiss (HBT) interferometry. Oscillations of the extracted HBT radii vs. emission angle indicate sources elongated perpendicular to the reaction plane. The results indicate that the pressure and expansion time of the collision system are not sufficient to completely quench its initial shape.

Adams, J.; Adler, C.; Aggarwal, M.M.; Ahammed, Z.; Amonett, J.; Anderson, B.D.; Arkhipkin, D.; Averichev, G.S.; Badyal, S.K.; Balewski, J.; Barannikova, O.; Barnby, L.S.; Baudot, J.; Bekele, S.; Belaga, V.V.; Bellwied, R.; Berger, J.; Bezverkhny, B.I.; Bhardwaj, S.; Bhati, A.K.; Bichsel, H.; Billmeier, A.; Bland, L.C.; Blyth, C.O.; Bonner, B.E.; Botje, M.; Boucham, A.; Brandin, A.; Bravar, A.; Cadman, R.V.; Cai, X.Z.; Caines, H.; Calderon de la Barca Sanchez, M.; Carroll, J.; Castillo, J.; Cebra, D.; Chaloupka, P.; Chattopadhyay, S.; Chen, H.F.; Chen, Y.; Chernenko, S.P.; Cherney, M.; Chikanian, A.; Christie, W.; Coffin, J.P.; Cormier, T.M.; Cramer, J.G.; Crawford, H.J.; Das, D.; Das, S.; Derevschikov, A.A.; Didenko, L.; Dietel, T.; Dong, W.J.; Dong, X.; Draper, J.E.; Du, F.; Dubey, A.K.; Dunin, V.B.; Dunlop, J.C.; Dutta Majumdar, M.R.; Eckardt, V.; Efimov, L.G.; Emelianov, V.; Engelage, J.; Eppley, G.; Erazmus, B.; Estienne, M.; Fachini, P.; Faine, V.; Faivre, J.; Fatemi, R.; Filimonov, K.; Filip, P.; Finch, E.; Fisyak, Y.; Flierl, D.; Foley, K.J.; Fu, J.; Gagliardi, C.A.; Gagunashvili, N.; Gans, J.; Gaudichet, L.; Geurts, F.; Ghazikhanian, V.; Ghosh, P.; Gonzalez, J.E.; Grachov, O.; Grebenyuk, O.; Gronstal, S.; Grosnick, D.; Guertin, S.M.; Gupta, A.; Gutierrez, T.D.; Hallman, T.J.; Hamed, A.; Hardtke, D.; Harris, J.W.; Heinz, M.; Henry, T.W.; Heppelmann, S.; Hippolyte, B.; Hirsch, A.; Hjort, E.; Hoffmann, G.W.; Horsley, M.; Huang, H.Z.; Huang, L.S.; Hughes, E.; Humanic, T.J.; Igo, G.; Ishihara, A.; Jacobs, P.; Jacobs, W.W.; Janik, M.; Jiang, H.; Johnson, I.; Jones, P.G.; Judd, E.G.; Kabana, S.; Kaplan, M.; Keane, D.; Khodyrev, V.Yu.; Kiryluk, J.; Kisiel, A.; Klay, J.; Klein, S.R.; Klyachko, A.; Koetke, D.D.; Kollegger, T.; Kopytine, M.; Kotchenda, L.; Kovalenko, A.D.; Kramer, M.; Kravtsov, V.I.; Kravtsov, P.; Krueger, K.; Kuhn, C.; Kulikov, A.I.; Kumar, A.; Kunde, G.J.; Kunz, C.L.; Kutuev, R.Kh.; Kuznetsov, A.A.; Lamont, M.A.C.; et al.

2004-06-30T23:59:59.000Z

342

An individual-based instream flow model for coexisting populations of brown and rainbow trout  

SciTech Connect (OSTI)

This report describes an individual-based model for sympatric populations of brown and rainbow trout in a stream habitat. Hatchery rainbow trout are included as a third species. The model provides a tool for predicting flow effects on trout populations by linking the hydraulic component of the Physical Habitat Simulation (PHABSIM) methodology and an individual-based population modeling approach. PHABSIM simulates the spatial distribution of depth and velocity at different flows. The individual-based model simulates the reproduction, foraging, consumption, energetic costs, growth, habitat utilization, movement, and mortality of individual fish, and enables population attributes to be determined from relevant attributes of individual fish. The spatially explicit nature of the model permits evaluation of behavioral responses used by fish to mitigate temporary setbacks in habitat quality. This linked mechanistic modeling approach readily lends itself to the iterative process of making predictions, testing against field data, improving the model, and making more predictions. The model has been applied to a stream segment in the Tule River, California. Physical and biological data from this site are used as input to the model. Calibrating the model to abundance data was relatively easy because values for mortality parameters were not strongly constrained by empirical data. Calibrating the model to observed growth rates and habitat use was more challenging. The primary reason for developing this model has been to provide a new and complementary tool to PHABSIM that can be used in instream-flow assessments.

Van Winkle, W.; Jager, H.I.; Holcomb, B.D.

1996-03-01T23:59:59.000Z

343

A Brown Dwarf Microlens Candidate in the OGLE-II Database  

E-Print Network [OSTI]

We describe a unique mass determination for a microlensing event from the second phase of the Optical Gravitational Microlensing Experiment (OGLE-II). The event, sc26_2218, which is very bright (baseline magnitude I=15.10), appears to exhibit both parallax and finite source effects. The parallax effect allows us to determine the projected Einstein radius on the observer plane (approx. 3.8 AU), while the finite source effect allows us to determine the ratio of the angular source size and the angular Einstein radius. As the angular size of the star can be estimated using its color and magnitude, we can hence determine the angular Einstein radius (approx. 0.1 mas). By combining both the projected and angular Einstein radius we can determine the lens mass M = 0.050^{+0.016}_{-0.011} solar masses, independent of the source distance. The lens is therefore a brown dwarf candidate. However, the `parallax' signature is weak and so we cannot completely discount the possibility that these signatures originate from binary rotation of the source (which would prevent any estimate of the lens mass), rather than parallax. However, this can be tested by future spectroscopic observations. This event highlights the scientific returns for intense monitoring of bright microlensing events, since the parallax and finite source effects can be more easily identified due to their high signal-to-noise ratios.

M. C. Smith; S. Mao; P. R. Wozniak

2003-01-16T23:59:59.000Z

344

Brown oculocutaneous albinism is allelic to tyrosinase-positive oculocutaneous albinism in southern African Negroids  

SciTech Connect (OSTI)

Brown oculocutaneous albinism (BOCA) is an autosomal recessive disorder involving a decrease in pigment of the skin, hair and eyes as well as decreased visual acuity. Evidence from two families who have co-existent BOCA and tyrosinase-positive oculocutaneous albinism (ty-pos OCA), suggests that the two conditions are allelic. Ty-pos OCA has been mapped to chromosome 15q11-q12 and the gene has been confirmed to be the human homologue (P) of the mouse pink-eyed dilute gene (p). Seven markers known to be linked to the P gene, D15S11, D15S10, MS14, GABA3, GABA5, IR10 and pCMW-1, were used to construct haplotypes in 5 families with BOCA. The haplotype data was subjected to linkage analysis and a maximum lod score of 2.85 ({theta} 0.0) was obtained. It has been reported previously that BOCA, in an Afro-American, was due to the lack of tyrosinase-protein 1 (Trp-1) in melanocytes. Trp-1 has been excluded as the disease-causing locus in the southern African families by linkage analysis with D9S43. A lod score of -2.02 was obtained at {theta} = 0.02.

Manga, P.; Ramsay, M.; Kromberg, J.; Jenkins, T. [Univ. of the Witwatersrand, Johannesburg (South Africa)

1994-09-01T23:59:59.000Z

345

PARALLAXES AND PROPER MOTIONS OF ULTRACOOL BROWN DWARFS OF SPECTRAL TYPES Y AND LATE T  

SciTech Connect (OSTI)

We present astrometric measurements of 11 nearby ultracool brown dwarfs of spectral types Y and late-T, based on imaging observations from a variety of space-based and ground-based telescopes. These measurements have been used to estimate relative parallaxes and proper motions via maximum likelihood fitting of geometric model curves. To compensate for the modest statistical significance ({approx}< 7) of our parallax measurements we have employed a novel Bayesian procedure for distance estimation which makes use of an a priori distribution of tangential velocities, V {sub tan}, assumed similar to that implied by previous observations of T dwarfs. Our estimated distances are therefore somewhat dependent on that assumption. Nevertheless, the results have yielded distances for five of our eight Y dwarfs and all three T dwarfs. Estimated distances in all cases are {approx}> 3 pc. In addition, we have obtained significant estimates of V {sub tan} for two of the Y dwarfs; both are <100 km s{sup -1}, consistent with membership in the thin disk population. Comparison of absolute magnitudes with model predictions as a function of color shows that the Y dwarfs are significantly redder in J - H than predicted by a cloud-free model.

Marsh, Kenneth A.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L. [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States)] [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Wright, Edward L. [Department of Physics and Astronomy, UCLA, P.O. Box 951547, Los Angeles, CA 90095 (United States)] [Department of Physics and Astronomy, UCLA, P.O. Box 951547, Los Angeles, CA 90095 (United States); Cushing, Michael C. [Department of Physics and Astronomy, The University of Toledo, 2801 West Bancroft Street, Toledo, OH 43606 (United States)] [Department of Physics and Astronomy, The University of Toledo, 2801 West Bancroft Street, Toledo, OH 43606 (United States); Skrutskie, Michael F. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States)] [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States); Eisenhardt, Peter R., E-mail: ken.marsh@astro.cf.ac.uk [NASA Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States)

2013-01-10T23:59:59.000Z

346

ON THE SURVIVAL OF BROWN DWARFS AND PLANETS ENGULFED BY THEIR GIANT HOST STAR  

SciTech Connect (OSTI)

The recent discovery of two Earth-mass planets in close orbits around an evolved star has raised questions as to whether substellar companions can survive encounters with their host stars. We consider whether these companions could have been stripped of significant amounts of mass during the phase when they orbited through the dense inner envelopes of the giant. We apply the criterion derived by Murray et al. for disruption of gravitationally bound objects by ram pressure to determine whether mass loss may have played a role in the histories of these and other recently discovered low-mass companions to evolved stars. We find that the brown dwarf and Jovian-mass objects circling WD 0137-349, SDSS J08205+0008, and HIP 13044 are most unlikely to have lost significant mass during the common envelope phase. However, the Earth-mass planets found around KIC 05807616 could well be the remnants of one or two Jovian-mass planets that lost extensive mass during the common envelope phase.

Passy, Jean-Claude; Mac Low, Mordecai-Mark [Department of Astrophysics, American Museum of Natural History, New York, NY (United States); De Marco, Orsola [Department of Physics and Astronomy, Macquarie University, Sydney, NSW (Australia)

2012-11-10T23:59:59.000Z

347

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3  

E-Print Network [OSTI]

#12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3 CONTENTS Studies for Students #lo, Geologic Guide to Provo Canyon and Weber Canyon, Central Wasatch Mountains, Utah ............................................................................................................................. Randy L. Chamberlain The Geology of the Drum Mountains, Millard and Juab Counties, Utah

Seamons, Kent E.

348

Brigham Young University Geology Studies Volume 27, Part 2  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 27, Part 2 CONTENTS The Kinnikinic Quartzite ........................................................Robert Q. Oaks,Jr., and W . Calvin James Geology of the Sage Valley 7 W'Quadrangle, Caribou County, Idaho, and Lincoln County, Wyoming ....................J ohn L. Conner Geology of the Elk Valley Quadrangle, Bear

Seamons, Kent E.

349

Brigham Young University Geology Studies Volume 24, Part 2  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 24, Part 2 CONTENTS Studies for Students ............................................................................................................................... Robert C. Ahlborn Publications and Maps of the Geology Department Cover: Sahara dune sand, X130. Photo, Univer~ityof Cincinnati, Cincinnati, Ohio 45221. #12;A publication of the Department of Geology Brigham

Seamons, Kent E.

350

Brigham Young University Geology Studies Volume 29, Part 2  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 29, Part 2 CONTENTS Stratigraphy ...................................................................................................... Terry C. Gosney 27 Geology of the Champlin Peak Quadrangle,Juab and Millard Counties, Utah ..................................................................................................................................... David R. Keller 103 Publications and Maps of the Department of Geology 117 Cover: Rafted orjoreign

Seamons, Kent E.

351

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 25,Part 1  

E-Print Network [OSTI]

#12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 25,Part 1 Papers reviewing geology of field trip areas, 31st annual meeting, Rocky Mountain Section, Geological Society of America, April 28 ....................................................................................................................................................... Geology of Volcanic Rocks and Mineral Deposits in the Southern Thomas Range, Utah: A Brief Summary

Seamons, Kent E.

352

Brigham Young University Geology Studies Volume 30, Part 1  

E-Print Network [OSTI]

#12;Brigham Young University Geology Studies Volume 30, Part 1 CONTENTS Diagenetic Aspects ................................................................................................... Steven G. Driese Geology of the Dog Valley-Red Ridge Area, Southern Pavant Mountains, Millard County .................................................................................................. Lynn C Meibos Geology of the Southwestern Quarter of the Scipio North (15-Minute) Quadrangle, Millard

Seamons, Kent E.

353

VOLUMF -31, PART 1 BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES  

E-Print Network [OSTI]

Y O U N G VOLUMF -31, PART 1 #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES VOLUME 31.PART 1 CONTENTS .................................................................. Ralph E.Lambert Geology of the Mount Ellen Quadrangle. Henry Mountains. Garfield County. Utah near White Horse Pass. Elko County. Nevada ............Stephen M Smith Geology of the Steele Butte

Seamons, Kent E.

354

Carbon Storage in Young Growth Coast Redwood Stands  

E-Print Network [OSTI]

515 Carbon Storage in Young Growth Coast Redwood Stands Dryw A. Jones1 and Kevin L. O'Hara1 Abstract Carbon sequestration is an emerging forest management objective within California and around the dynamics of carbon sequestration and to accurately measure carbon storage is essential to insure successful

Standiford, Richard B.

355

Press Releases and News BT-Citibank Young Investors' Forum  

E-Print Network [OSTI]

Researcher, Prof. Joseph Cherian Business Time, Singapore 20 June 2011 Several factors make this investment of the major investment asset classes out there. For young retail investors, pumping money direct into corn or oil, or buying shares in a far-off land can be daunting. So over the next few Mondays, we'll look

Chaudhuri, Sanjay

356

Building Knowledge about Buildings Matthew T. Young and Eyal Amir  

E-Print Network [OSTI]

Building Knowledge about Buildings Matthew T. Young and Eyal Amir University of Illinois, Urbana The ability to encode information about the structure of buildings is essential for the development of applications which are able to reason about buildings and answer queries concerning their design and function

Amir, Eyal

357

Observation of large continuous-wave two-photon optical amplification Hope M. Concannon, William J. Brown, Jeff R. Gardner, and Daniel J. Gauthier  

E-Print Network [OSTI]

(DAMTP; now ENS Lyon) · Megan Davies Wykes (DAMTP) · David Youngs (AWE) · Robin Williams (AWE) · Jeff

Gauthier, Daniel

358

E-Print Network 3.0 - at-risk young men Sample Search Results  

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

at-risk young men Page: << < 1 2 3 4 5 > >> 1 The Annals of the American Academy of Political and Social Science Young Disadvantaged Men: Fathers, Families, Poverty, and Policy...

359

The Effects of Varying Task Priorities on Language Production by Young and Older Adults  

E-Print Network [OSTI]

The present study compared how varying task priorities affected young and older adults' language production. Both young and older adults responded to monetary incentives to vary their performance when simultaneously talking ...

Kemper, Susan; Schmalzried, RaLynn Cheri; Herman, Ruth; Mohankumar, Deepthi

2011-02-01T23:59:59.000Z

360

A Systematic Study of X-Ray Flares from Low-Mass Young Stellar Objects in the Rho Ophiuchi Star-Forming Region with Chandra  

E-Print Network [OSTI]

We report on the results of a systematic study of X-ray flares from low-mass young stellar objects, using Chandra observations of the main region of the Rho Oph. From 195 X-ray sources, including class I-III sources and some young brown dwarfs, we detected a total of 71 X-ray flares. Most of the flares have the typical profile of solar and stellar flares, fast rise and slow decay. We derived the time-averaged temperature (kT), luminosity (L_X), rise and decay timescales (tau_r and tau_d) of the flares, finding that (1) class I-II sources tend to have a high kT, (2) the distribution of L_X during flares is nearly the same for all classes, and (3) positive and negative log-linear correlations are found between tau_r and tau_d, and kT and tau_r. In order to explain these relations, we used the framework of magnetic reconnection model to formulate the observational parameters as a function of the half-length of the reconnected magnetic loop (L) and magnetic field strength (B). The estimated L is comparable to the typical stellar radius of these objects (10^{10-11} cm), which indicates that the observed flares are triggered by solar-type loops, rather than larger ones (10^{12} cm) connecting the star with its inner accretion disk. The higher kT observed for class I sources may be explained by a higher magnetic field strength (about 500 G) than for class II-III sources (200-300 G).

K. Imanishi; H. Nakajima; M. Tsujimoto; K. Koyama; Y. Tsuboi

2003-05-10T23:59:59.000Z

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


361

THE BIMODALITY OF ACCRETION IN T TAURI STARS AND BROWN DWARFS  

SciTech Connect (OSTI)

We present numerical solutions of the collapse of prestellar cores that lead to the formation and evolution of circumstellar disks. The disk evolution is then followed for up to three million years. A variety of models of different initial masses and rotation rates allow us to study disk accretion around brown dwarfs and low-mass T Tauri stars (TTSs), with central object mass M{sub *} < 0.2 M{sub sun}, as well as intermediate- and upper-mass TTSs (0.2 M{sub sun} < M{sub *} < 3.0 M{sub sun}). Our models include self-gravity and allow for nonaxisymmetric motions. In addition to the self-consistently generated gravitational torques, we introduce an effective turbulent alpha-viscosity with alpha = 0.01, which allows us particularly to model accretion in the low-mass regime where disk self-gravity is diminishing. A range of models with observationally motivated values of the initial ratio of rotational-to-gravitational energy yield a correlation between mass accretion rate M-dot and M{sub *} that is relatively steep, as observed. Additionally, our modeling reveals evidence for a bimodality in the M-dot - M{sub *} correlation, with a steeper slope at lower masses and a shallower slope at intermediate and upper masses, as also implied by observations. Furthermore, we show that the neglect of disk self-gravity leads to a much steeper M-dot - M{sub *} relation for intermediate- and upper-mass TTSs. This demonstrates that an accurate treatment of global self-gravity is essential to understanding observations of circumstellar disks.

Vorobyov, E. I. [Institute for Computational Astrophysics, Saint Mary's University, Halifax, B3H 3C3 (Canada); Basu, Shantanu, E-mail: vorobyov@ap.smu.c, E-mail: basu@astro.uwo.c [Department of Physics and Astronomy, University of Western Ontario, London, Ontario, N6A 3K7 (Canada)

2009-09-20T23:59:59.000Z

362

On the polar cap cascade pair multiplicity of young pulsars  

E-Print Network [OSTI]

We study the efficiency of pair production in polar caps of young pulsars under a variety of conditions to estimate the maximum possible multiplicity of pair plasma in pulsar magnetospheres. We develop a semi-analytic model for calculation of cascade multiplicity which allows efficient exploration of the parameter space and corroborate it with direct numerical simulations. Pair creation processes are considered separately from particle acceleration in order to assess different factors affecting cascade efficiency, with acceleration of primary particles described by recent self-consistent non-stationary model of pair cascades. We argue that the most efficient cascades operate in the curvature radiation/synchrotron regime, the maximum multiplicity of pair plasma in pulsar magnetospheres is ~few x 10^5. The multiplicity of pair plasma in magnetospheres of young energetic pulsars weakly depends on the strength of the magnetic field and the radius of curvature of magnetic field lines and has a stronger dependence ...

Timokhin, A N

2015-01-01T23:59:59.000Z

363

Rhizoctonia spp. associated with brown patch of St. Augustinegrass: isolate characterization, host range, and screening for resistance  

E-Print Network [OSTI]

Resistance CONCLUSION LITERATURE CITED 13 13 18 18 25 27 34 41 45 VITA 50 LIST OF TABLES Page TABLE 1. Dates St. Augustinegrsss displaying brown patch symptoms was collected, location of the collection sites, and type of host tissue from..., drained, and placed under a laminar- flow hood on paper towels for 10 min to remove excess water. The cut end of each tip was dipped in molten Paraplast (Lancer Co. , St. Louis, NO. , 63103) to seal the wound. One tip was placed in each of the WA...

Hurd, Bernadette Murphy

1982-01-01T23:59:59.000Z

364

Report on the culture of brown shrimp, Penaeus aztecus, in ponds receiving thermal effluent from a power plant  

E-Print Network [OSTI]

. (December 1974) Donald Martin Quarberg, B. S. , University of Wisconsin--Stevens Point Chairman of Advisory Committee: Dr. David V. Aldrich During 1973 brown shrimp, Penaeus aztecus, were cultured in 0. 1 ha ponds designed to receive a constant supply... pond study in early August and the other was terminated in mid- September. Survival was under 0. 5%, growth less than 0. 6 mm/day, and production only 0. 53 and 1. 59 kg/ha. In September two ponds were each stocked with 50, two ponds with 500...

Quarberg, Donald Martin

1974-01-01T23:59:59.000Z

365

Optoelectronic Mixers for Fiber-fed 60-GHz Wireless Systems Woo-Young Choi, Jae-Young Kim and Myung-Jae Lee  

E-Print Network [OSTI]

#12;Optoelectronic Mixers for Fiber-fed 60-GHz Wireless Systems Woo-Young Choi, Jae-Young Kim investigated millimeter-wave fiber-fed wireless systems using optoelectronic mixers based on hetero-effective optoelectronic (O/E) mixer, which performs photo- detection and frequency conversion functions simultaneously. We

Choi, Woo-Young

366

MARVELS-1b: A Short-Period, Brown Dwarf Desert Candidate from the SDSS-III MARVELS Planet Search  

E-Print Network [OSTI]

We present a new short-period brown dwarf candidate around the star TYC 1240-00945-1. This candidate was discovered in the first year of the Multi-object APO Radial Velocity Exoplanets Large-area Survey (MARVELS), which is part of the third phase of the Sloan Digital Sky Survey (SDSS-III), and we designate the brown dwarf as MARVELS-1b. MARVELS uses the technique of dispersed fixed-delay interferometery to simultaneously obtain radial velocity measurements for 60 objects per field using a single, custom-built instrument that is fiber fed from the SDSS 2.5-m telescope. From our 20 radial velocity measurements spread over a ~370 d time baseline, we derive a Keplerian orbital fit with semi-amplitude K=2.533+/-0.025 km/s, period P=5.8953+/-0.0004 d, and eccentricity consistent with circular. Independent follow-up radial velocity data confirm the orbit. Adopting a mass of 1.37+/-0.11 M_Sun for the slightly evolved F9 host star, we infer that the companion has a minimum mass of 28.0+/-1.5 M_Jup, a semimajor axis 0....

Lee, Brian L; Fleming, Scott W; Stassun, Keivan G; Gaudi, B Scott; Barnes, Rory; Mahadevan, Suvrath; Eastman, Jason D; Wright, Jason; Siverd, Robert J; Gary, Bruce; Ghezzi, Luan; Laws, Chris; Wisniewski, John P; de Mello, G F Porto; Ogando, Ricardo L C; Maia, Marcio A G; da Costa, Luiz Nicolaci; Sivarani, Thirupathi; Pepper, Joshua; Nguyen, Duy Cuong; Hebb, Leslie; De Lee, Nathan; Wang, Ji; Wan, Xiaoke; Zhao, Bo; Chang, Liang; Groot, John; Varosi, Frank; Hearty, Fred; Hanna, Kevin; van Eyken, J C; Kane, Stephen R; Agol, Eric; Bizyaev, Dmitry; Bochanski, John J; Brewington, Howard; Chen, Zhiping; Costello, Erin; Dou, Liming; Eisenstein, Daniel J; Fletcher, Adam; Ford, Eric B; Guo, Pengcheng; Holtzman, Jon A; Jiang, Peng; Leger, R French; Liu, Jian; Long, Daniel C; Malanushenko, Elena; Malanushenko, Viktor; Malik, Mohit; Oravetz, Daniel; Pan, Kaike; Rohan, Pais; Schneider, Donald P; Shelden, Alaina; Snedden, Stephanie A; Simmons, Audrey; Weaver, B A; Weinberg, David H; Xie, Ji-Wei

2010-01-01T23:59:59.000Z

367

Eye movements of young and older adults during reading  

E-Print Network [OSTI]

Kemper, S., & Liu, C. – J. (2007). Eye movements of young and older adults during reading. Psychology and Aging, 22, 84-94. PMID: 17385986. Publisher’s official version: http://psycnet.apa.org/doi/10.1037/0882-7974.22.1.84. Open Access version... n is a va ila b le o n it s si te . [This document contains the author’s accepted manuscript. For the publisher’s version, see the link in the header of this document.] Paper citation: Kemper, S., & Liu, C. – J. (2007). Eye...

Kemper, Susan; Liu, Chiung-Ju

2007-03-01T23:59:59.000Z

368

Particle acceleration at supernova shocks in young stellar clusters  

E-Print Network [OSTI]

We briefly discuss models of energetic particle acceleration by supernova shock in active starforming regions at different stages of their evolution. Strong shocks may strongly amplify magnetic fields due to cosmic ray driven instabilities. We discuss the magnetic field amplification emphasizing the role of the long-wavelength instabilities. Supernova shock propagating in the vicinity of a powerful stellar wind in a young stellar cluster is argued to increase the maximal CR energies at a given evolution stage of supernova remnant (SNR) and can convert a sizeable fraction of the kinetic energy release into energetic particles.

Bykov, A M; Osipov, S M

2011-01-01T23:59:59.000Z

369

Young Women's Conference in Science, Technology, Engineering & Mathematics  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLasDelivered energy consumption byAbout SRNL HomeYoung Inventor Shares His Award-Winning|

370

Young County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:SeadovCooperative JumpWilliamsonWoodsonCounty is aYoakum County,Springs,Yorktown, NewYoung

371

Young Womens Conference attracts more attendees in 2014! | Princeton Plasma  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWaste andAnniversary, part 2 ContinuingYan MeiPhysics Lab Young

372

Different effects of dual task demands on the speech of young and older adults  

E-Print Network [OSTI]

Kemper, S., Herman, R. E., Nartowicz, J.(2005). Different Effects of Dual Task Demands on the Speech of Young and Older Adults. Aging, Neuropsychology, and Cognition, 12, 340-358. PM#1410812. Publisher’s official version: http://dx.doi.org/10...., Nartowicz, J.(2005). Different Effects of Dual Task Demands on the Speech of Young and Older Adults. Aging, Neuropsychology, and Cognition, 12, 340-358. PM#1410812 Abstract: Young and older adults provided language samples in response to elicitation...

Kemper, Susan; Herman, Ruth; Nartowicz, Jennifer

2005-12-01T23:59:59.000Z

373

A CAUTIONARY TALE: MARVELS BROWN DWARF CANDIDATE REVEALS ITSELF TO BE A VERY LONG PERIOD, HIGHLY ECCENTRIC SPECTROSCOPIC STELLAR BINARY  

SciTech Connect (OSTI)

We report the discovery of a highly eccentric, double-lined spectroscopic binary star system (TYC 3010-1494-1), comprising two solar-type stars that we had initially identified as a single star with a brown dwarf companion. At the moderate resolving power of the MARVELS spectrograph and the spectrographs used for subsequent radial-velocity (RV) measurements (R {approx}< 30, 000), this particular stellar binary mimics a single-lined binary with an RV signal that would be induced by a brown dwarf companion (Msin i {approx} 50 M{sub Jup}) to a solar-type primary. At least three properties of this system allow it to masquerade as a single star with a very-low-mass companion: its large eccentricity (e {approx} 0.8), its relatively long period (P {approx} 238 days), and the approximately perpendicular orientation of the semi-major axis with respect to the line of sight ({omega} {approx} 189 Degree-Sign ). As a result of these properties, for {approx}95% of the orbit the two sets of stellar spectral lines are completely blended, and the RV measurements based on centroiding on the apparently single-lined spectrum is very well fit by an orbit solution indicative of a brown dwarf companion on a more circular orbit (e {approx} 0.3). Only during the {approx}5% of the orbit near periastron passage does the true, double-lined nature and large RV amplitude of {approx}15 km s{sup -1} reveal itself. The discovery of this binary system is an important lesson for RV surveys searching for substellar companions; at a given resolution and observing cadence, a survey will be susceptible to these kinds of astrophysical false positives for a range of orbital parameters. Finally, for surveys like MARVELS that lack the resolution for a useful line bisector analysis, it is imperative to monitor the peak of the cross-correlation function for suspicious changes in width or shape, so that such false positives can be flagged during the candidate vetting process.

Mack, Claude E. III; Stassun, Keivan G.; De Lee, Nathan [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Ge, Jian; Fleming, Scott W. [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL, 32611-2055 (United States); Deshpande, Rohit; Mahadevan, Suvrath [Department of Astronomy and Astrophysics, The Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Wisniewski, John P. [Homer L Dodge Department of Physics and Astronomy, University of Oklahoma, 440 W Brooks St, Norman, OK 73019 (United States); Gaudi, B. Scott; Eastman, Jason; Beatty, Thomas G. [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Ghezzi, Luan [Observatorio Nacional, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ 20921-400 (Brazil); Gonzalez Hernandez, Jonay I.; Femenia, Bruno; Mata Sanchez, Daniel [Instituto de Astrofisica de Canarias (IAC), E-38205 La Laguna, Tenerife (Spain); Ferreira, Leticia; Porto de Mello, Gustavo [Laboratorio Interinstitucional de e-Astronomia-LIneA, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ 20921-400 (Brazil); Crepp, Justin R. [Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Agol, Eric [Astronomy Department, University of Washington, Box 351580, Seattle, WA 98195 (United States); Bizyaev, Dmitry, E-mail: claude.e.mack@vanderbilt.edu [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349-0059 (United States); and others

2013-05-15T23:59:59.000Z

374

E-Print Network 3.0 - american young adults Sample Search Results  

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

2, when... as well as did young ... Source: Corkin, Suzanne - Department of Brain and Cognitive Science, Massachusetts Institute of Technology (MIT) Collection: Biology and...

375

Alcohol Mixed with Caffeinated Energy Drinks: Consumption Patterns and Trends Among Canadian Youth & Young Adults.  

E-Print Network [OSTI]

??Use of caffeinated energy drinks (CEDs) and alcohol mixed with energy drinks (AmEDs) is a growing trend worldwide, and in Canada, youth and young adults… (more)

McCrory, Cassondra

2015-01-01T23:59:59.000Z

376

E-Print Network 3.0 - anaemic young children Sample Search Results  

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

Medicine 4 UCL CENTRE FOR INTERNATIONAL HEALTH & DEVELOPMENT Summary: : Nayarit State, Mexico PARTNER: University of Nayarit, Mexico THE CHALLENgE: Young children and adults... is...

377

Hydraulic Drivetrain and Regenerative Braking Team 13: Andrew Brown, Karan Desai, Andrew McGrath, Hurst Nuckols, Grant Wilson Adviser: Dr. Andrew Jackson  

E-Print Network [OSTI]

Hydraulic Drivetrain and Regenerative Braking Team 13: Andrew Brown, Karan Desai, Andrew Mc Pressure Reservior Filter Variable Vane Pump Motor/Pump Hydraulic Accumulators Solenoid Valve Relief Valve Suction Line Since their development in 2006, hydraulic drivetrain systems have gained considerable

Carpick, Robert W.

378

Three-dimensional reconnection and relaxation of merging spheromak plasmas T. Gray, V. S. Lukin, M. R. Brown, and C. D. Cothran  

E-Print Network [OSTI]

Three-dimensional reconnection and relaxation of merging spheromak plasmas T. Gray, V. S. Lukin, M-dimensional reconnection and relaxation of merging spheromak plasmas" [Phys. Plasmas17, 102106 (2010)] Phys. Plasmas 17 and relaxation of merging spheromak plasmas T. Gray,1,a V. S. Lukin,2 M. R. Brown,1 and C. D. Cothran1,b 1

Brown, Michael R.

379

Motion and equilibrium of a spheromak in a toroidal flux conserver M. R. Brown,a) D. M. Cutrer, and P. M. Beilan  

E-Print Network [OSTI]

Motion and equilibrium of a spheromak in a toroidal flux conserver M. R. Brown,a) D. M. Cutrer field). First, a fit of the in situ magnetic data of the spheromak in the tokamak vesselto a simple of the spheromakin the dc toroidal field of the tokamak are relevant to theories of spheromak/tokamak interaction.3

Brown, Michael R.

380

Flow Dynamics of Spheromaks in SSX Mike Brown1, Chris Cothran1,2, David Cohen1, Jason Horwitz1,and Vernon Chaplin1  

E-Print Network [OSTI]

Flow Dynamics of Spheromaks in SSX Mike Brown1, Chris Cothran1,2, David Cohen1, Jason Horwitz1,and aspects of the computer models. Introduction -The Swarthmore Spheromak Experiment (SSX) is designed to study both basic plasma physics (reconnection) and fusion-related science (spheromaks and FRCs). Plasma

Cohen, David

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


381

The tropical brown alga Lobophora variegata as a bioindicator of mining1 contamination in the New Caledonia lagoon: a field transplantation study2  

E-Print Network [OSTI]

1 The tropical brown alga Lobophora variegata as a bioindicator of mining1 contamination in the New field and laboratory studies have identified the alga Lobophora variegata as a good21 candidate key contaminants, i.e. Ag, As, Cd, Co, Cr,25 Cu, Mn, Ni and Zn. Algae from clean and contaminated

Paris-Sud XI, Université de

382

Finding Forrester (2000) The film opens with 16-year-old Jamal Wallace (Rob Brown) sleeping in his bedroom, which is  

E-Print Network [OSTI]

Finding Forrester (2000) The film opens with 16-year-old Jamal Wallace (Rob Brown) sleeping in his Jamal and his friends play basketball. They regularly notice him watching them from his window, although they never see his face, and they refer to him simply as 'The Window'. One day after school, one of the boys

Schenato, Luca

383

NTIME and the classes NP. Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. p.1  

E-Print Network [OSTI]

Lecture 12 NTIME and the classes NP. Slides modified by Benny Chor, based on original slides in NP. Slides modified by Benny Chor, based on original slides by Maurice Herlihy, Brown University. ­ p.1 #12;Lecture 12 NTIME and the classes NP. Examples of Problems in NP. Verifiability. Slides

Beimel, Amos

384

Fracture Testing of a Self-Healing Polymer Composite by E.N. Brown, N.R. Sottos and S.R. White  

E-Print Network [OSTI]

Fracture Testing of a Self-Healing Polymer Composite by E.N. Brown, N.R. Sottos and S.R. White with an embedded catalyst. The effects of size and concentration of the catalyst and mi- crocapsules on fracture as much as 90 percent of its virgin fracture toughness. KEY WORDS--Self-healing, autonomic healing

Sottos, Nancy R.

385

The Analysis of Interference Effects in the Sum Frequency Spectra of Water Interfaces Mac G. Brown, Elizabeth A. Raymond, Heather C. Allen, Lawrence F. Scatena, and  

E-Print Network [OSTI]

The Analysis of Interference Effects in the Sum Frequency Spectra of Water Interfaces Mac G. Brown, Elizabeth A. Raymond, Heather C. Allen, Lawrence F. Scatena, and Geraldine L. Richmond* Department involve the surface of liquid water. Unfortunately, obtaining spectral fits to vibrational spectra

Richmond, Geraldine L.

386

On-site field tests for study of low-rank western coal fly ash. Technical summary report, field test No. 3. Big Brown Station electrostatic precipitator  

SciTech Connect (OSTI)

This report describes the results of field and laboratory studies of combined NH/sub 3/ and SO/sub 3/ conditioning at the Big Brown Station of Texas Utilities Generating Company. This unusual combination of conditioning agents is used routinely at the Big Brown Station in order to improve the performance of the cold-side electrostatic precipitators. The primary objectives of this field study were to evaluate the performance of one of the Big Brown precipitators, and to obtain data on the concentration, composition, and size distribution of the fly ash, as well as the composition of the flue gas and the overall and fractional collection efficiencies of the precipitator. The laboratory studies of the Big Brown fly ash were intended to further characterize the ash both physically and chemically, and to study the attenuation of the electrical resistivity of the ash associated with the surface film produced by the dual conditioning process and by the use of SO/sub 3/ conditioning alone. 6 references, 22 figures, 9 tables.

Dahlin, R. S.; Bickelhaupt, R. E.; Marchant, Jr., G. H.; Gooch, J. P.

1984-02-01T23:59:59.000Z

387

Biomass-Derived Hydrogen from a Thermally Ballasted Gasifier Robert C. Brown, Glenn Norton, Andy Suby, Jerod Smeenk, Keith Cummer, and Josh Nunez  

E-Print Network [OSTI]

Biomass-Derived Hydrogen from a Thermally Ballasted Gasifier Robert C. Brown, Glenn Norton, Andy fuel cells. We have developed a thermally ballasted gasifier that uses a single reactor for both compared to conventional gasifiers. The carbon monoxide, along with steam used to fluidize the reactor, can

388

836 J. GUIDANCE, VOL. 20, NO. 4: ENGINEERING NOTES 1Brown, R., "Fuzzy Logic Application for Modeling Man-in-the-Loop  

E-Print Network [OSTI]

-2800,Aug. 1991. 5Lea, R., and Jani, Y., "Fuzzy Logic Applications to Expert Systems and Control,"2nd., "A Fuzzy Logic Controller for Aircraft Flight Control," In- dustrial Applications of Fuzzy Control836 J. GUIDANCE, VOL. 20, NO. 4: ENGINEERING NOTES References 1Brown, R., "Fuzzy Logic Application

Hall, Christopher D.

389

J.D. Brown, J. Rosen, M. N. Sinanan, B. Hannaford, In-Vivo and Postmortem Compressive Properties of Porcine Abdominal Organs  

E-Print Network [OSTI]

Compressive Properties of Porcine Abdominal Organs Jeffrey D. Brown1 , Jacob Rosen1 , Mika N. Sinanan2 , Blake The biomechanics of soft tissues that are load-bearing during physiological activities (muscles, tendons, intervertebral discs, cartilage, blood vessels) have been well stud- ied. The soft abdominal organs do not bear

390

A Search for Fallback Disks in Four Young Supernova Remnants  

E-Print Network [OSTI]

We report on our search for the optical/infrared counterparts to the central compact objects in four young supernova remnants: Puppis A, PKS 1209-52, RCW 103, and Cassiopeia A. The X-ray point sources in these supernova remnants, likely members of a new class (or classes) of young neutron stars, are attractive targets for probing the existence of supernova ``fallback'' disks. Such disks, which are a general prediction of many supernova models, can form from supernova ejecta that fails to reach escape velocity during the initial explosion. Irradiation of the disk by a central X-ray source may lead to detectable optical/infrared emission from such a disk. We used imaging observations from ground-based telescopes in the optical and near-infrared regimes and from the Spitzer Space Telescope at 4.5 and 8.0 micron, to search for optical/infrared counterparts at the X-ray point source positions measured in these supernova remnants by the Chandra X-Ray Observatory. We did not detect any counterparts, and hence find n...

Wang, Z; Chakraborty, D; Wang, Zhongxiang; Kaplan, David L.; Chakrabarty, Deepto

2006-01-01T23:59:59.000Z

391

Circumbinary Molecular Rings Around Young Stars in Orion  

E-Print Network [OSTI]

We present high angular resolution 1.3 mm continuum, methyl cyanide molecular line, and 7 mm continuum observations made with the Submillimeter Array and the Very Large Array, toward the most highly obscured and southern part of the massive star forming region OMC1S located behind the Orion Nebula. We find two flattened and rotating molecular structures with sizes of a few hundred astronomical units suggestive of circumbinary molecular rings produced by the presence of two stars with very compact circumstellar disks with sizes and separations of about 50 AU, associated with the young stellar objects 139-409 and 134-411. Furthermore, these two circumbinary rotating rings are related to two compact and bright {\\it hot molecular cores}. The dynamic mass of the binary systems obtained from our data are $\\geq$ 4 M$_\\odot$ for 139-409 and $\\geq$ 0.5 M$_\\odot$ for 134-411. This result supports the idea that intermediate-mass stars will form through {\\it circumstellar disks} and jets/outflows, as the low mass stars do. Furthermore, when intermediate-mass stars are in multiple systems they seem to form a circumbinary ring similar to those seen in young, multiple low-mass systems (e.g., GG Tau and UY Aur).

Luis A. Zapata; Paul T. P. Ho; Luis F. Rodriguez; Peter Schilke; Stan Kurtz

2007-07-09T23:59:59.000Z

392

THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS  

SciTech Connect (OSTI)

We report results of a direct imaging survey for giant planets around 80 members of the ? Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of ?H = 13.9 mag at 1'' in combined CH{sub 4} narrowband ADI+SDI mode and median contrasts of ?H = 15.1 mag at 2'' in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with Near-Infrared Coronagraphic Imager (NICI) all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI Campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36 ± 6 M{sub Jup}, 16.4 ± 1.0 AU), CD–35 2722B (31 ± 8 M{sub Jup}, 67 ± 4 AU), HD 12894B (0.46 ± 0.08 M{sub ?}, 15.7 ± 1.0 AU), and BD+07 1919C (0.20 ± 0.03 M{sub ?}, 12.5 ± 1.4 AU). From a Bayesian analysis of the achieved H band ADI and ASDI contrasts, using power-law models of planet distributions and hot-start evolutionary models, we restrict the frequency of 1-20 M{sub Jup} companions at semi-major axes from 10-150 AU to <18% at a 95.4% confidence level using DUSTY models and to <6% at a 95.4% using COND models. Our results strongly constrain the frequency of planets within semi-major axes of 50 AU as well. We restrict the frequency of 1-20 M{sub Jup} companions at semi-major axes from 10-50 AU to <21% at a 95.4% confidence level using DUSTY models and to <7% at a 95.4% using COND models. This survey is the deepest search to date for giant planets around young moving group stars.

Biller, Beth A.; Ftaclas, Christ [Max-Planck-Institut für Astronomie, Königstuhl 17, D-69115 Heidelberg (Germany); Liu, Michael C.; Wahhaj, Zahed; Nielsen, Eric L. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Hayward, Thomas L.; Hartung, Markus [Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena (Chile); Males, Jared R.; Skemer, Andrew; Close, Laird M. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Chun, Mark [Institute for Astronomy, 640 North Aohoku Place, 209, Hilo, HI 96720-2700 (United States); Clarke, Fraser; Thatte, Niranjan [Department of Astronomy, University of Oxford, DWB, Keble Road, Oxford OX1 3RH (United Kingdom); Shkolnik, Evgenya L. [Lowell Observatory, 1400 West Mars Hill Road Flagstaff, AZ 86001 (United States); Reid, I. Neill [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Boss, Alan [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015 (United States); Lin, Douglas [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Alencar, Silvia H. P. [Departamento de Fisica-ICEx-Universidade Federal de Minas Gerais, Av. Antonio Carlos 6627, 30270-901 Belo Horizonte, MG (Brazil); De Gouveia Dal Pino, Elisabete; Gregorio-Hetem, Jane [Universidade de Sao Paulo, IAG/USP, Departamento de Astronomia, Rua do Matao 1226, 05508-900 Sao Paulo, SP (Brazil); and others

2013-11-10T23:59:59.000Z

393

Ionisation in atmospheres of brown dwarfs and extrasolar planets VI: Properties of large-scale discharge events  

E-Print Network [OSTI]

Mineral clouds in substellar atmospheres play a special role as a catalyst for a variety of charge processes. If clouds are charged, the surrounding environment becomes electrically activated, and ensembles of charged grains are electrically discharging (e.g. by lightning), which significantly infuences the local chemistry creating conditions similar to those thought responsible for life in early planetary atmospheres. We note that such lightning discharges contribute also to the ionisation state of the atmosphere. We apply scaling laws for electrical discharge processes from laboratory measurements and numerical experiments to Drift-Phoenix model atmosphere results to model the discharge's propagation downwards (as lightning) and upwards (as sprites) through the atmospheric clouds. We evaluate the spatial extent and energetics of lightning discharges. The atmospheric volume affected (e.g. by increase of temperature or electron number) is larger in a brown dwarf atmosphere ($10^8 -~10^{10}$m$^3$) than in a gi...

Bailey, R L; Hodos, G; Bilger, C; Stark, C R

2013-01-01T23:59:59.000Z

394

Structure and physical properties of the noncentrosymmetric superconductor Mo3Al2C A. B. Karki, Y. M. Xiong, I. Vekhter, D. Browne, P. W. Adams, and D. P. Young  

E-Print Network [OSTI]

. INTRODUCTION Metal carbide and nitride intermetallic superconductors have both fairly high transition temperatures and large criti- cal magnetic field values. Some of the metal carbides, for example, MgCNi3, La2C3, and computed its band structure. Experimental results indicate a bulk superconducting transition at Tc 9.2 K

Adams, Philip W.

395

PII S0016-7037(98)00211-7 The young age of Earth  

E-Print Network [OSTI]

PII S0016-7037(98)00211-7 The young age of Earth YOUXUE ZHANG* Department of Geological Sciences form June 8, 1998) Abstract--Patterson (1956) established that the age of Earth is close, disagreement is abundant, and the young age of Earth has not been widely accepted. In this work, I examine all

Zhang, Youxue

396

Associate Professors Limb, Gordon E. (2005) BS, Brigham Young U., 1994; MSW, U. of  

E-Print Network [OSTI]

Associate Professors Limb, Gordon E. (2005) BS, Brigham Young U., 1994; MSW, U. of Utah, 1997; PhD, U. of California, Berkeley, 2000. Marett, Kevin M. (1992) BS, Brigham Young U., 1982; MSW, U State U., 1972; MSW, DSW, U. of Utah, 1978, 1990. Panos, Patrick T. (1999) BS, U. of Utah, 1985; MS, MSW

Hart, Gus

397

Computer Usage by Young Individuals with Down Syndrome: An Exploratory Study  

E-Print Network [OSTI]

Computer Usage by Young Individuals with Down Syndrome: An Exploratory Study Jinjuan Feng, Jonathan that investigates how children and young adults with Down syndrome use computers and computer-related devices. The survey responses cover 561 individuals with Down syndrome between the age of four to 21. The survey

Lazar, Jonathan

398

August 2014 Subject: Research in Germany-Information Seminar for Young Researchers  

E-Print Network [OSTI]

26th August 2014 Subject: Research in Germany- Information Seminar for Young Researchers Warm-doctoral candidates as well as young academics interested in a research stay in Germany, towards initiating & strengthening research co operations with Germany. Date: 20th September 2014 Venue: IC & SR Auditorium, IIT

Krishnapura, Nagendra

399

Imaging Young Giant Planets From Ground and Space CHARLES A. BEICHMAN  

E-Print Network [OSTI]

of the James Webb Space Telescope (JWST). Monte Carlo modeling reveals that JWST can detect planets with masses of a dust disk. What is needed to anchor the models of young planets are objects of known ageImaging Young Giant Planets From Ground and Space CHARLES A. BEICHMAN NASA Exoplanet Science

400

Thomas Young's research on fluid transients: 200 years on Arris S Tijsseling Alexander Anderson  

E-Print Network [OSTI]

and waterhammer. Young's 1808 paper is "translated" into modern terminology. Young's discoveries, though difficult subsequently be combined into the pressure rise equation of Joukowsky. Keywords waterhammer, fluid transients of the 19th century, the three key elements for the development of modern waterhammer theory were in place

Eindhoven, Technische Universiteit

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


401

YOUNG ENTREPRENEUR PROGRAM The Indiana Economic Development Corporation (IEDC) is promoting  

E-Print Network [OSTI]

YOUNG ENTREPRENEUR PROGRAM The Indiana Economic Development Corporation (IEDC) is promoting a reality in Indiana. The IEDC will work with local and regional communities to offer incentives to the Young Entrepreneurs with the best business plans. These incentives can include and are not limited to

402

BRIEF REPORT Young Children Help Others to Achieve Their Social Goals  

E-Print Network [OSTI]

BRIEF REPORT Young Children Help Others to Achieve Their Social Goals Jonathan S. Beier University research has documented young children's propensity to help others achieve their unfulfilled goals toward. Here we demonstrate that children are also inclined, and able, to help others achieve their social

Carpenter, M.alinda

403

Skin Cancer: A Young Person's Disease By Lauren Duffy (B.S. Communication, Journalism '14)  

E-Print Network [OSTI]

Skin Cancer: A Young Person's Disease By Lauren Duffy (B.S. Communication, Journalism '14 is that this behavior is extremely unhealthy and risky for their bodies, specifically their skin. Skin cancer is the most common form of cancer found in young adults and second most common cancer found in adolescents

Massachusetts at Amherst, University of

404

Predicting Young’s Modulus of Glass/Ceramic Sealant for Solid Oxide Fuel Cell Considering the Combined Effects of Aging, Micro-Voids and Self-Healing  

SciTech Connect (OSTI)

We study the temperature dependent Young’s modulus for the glass/ceramic seal material used in Solid Oxide Fuel Cells (SOFCs). With longer heat treatment or aging time during operation, further devitrification may reduce the residual glass content in the seal material while boosting the ceramic crystalline content. In the meantime, micro-voids induced by the cooling process from the high operating temperature to room temperature can potentially degrade the mechanical properties of the glass/ceramic sealant. Upon reheating to the SOFC operating temperature, possible self-healing phenomenon may occur in the glass/ceramic sealant which can potentially restore some of its mechanical properties. A phenomenological model is developed to model the temperature dependent Young’s modulus of glass/ceramic seal considering the combined effects of aging, micro-voids, and possible self-healing. An aging-time-dependent crystalline content model is first developed to describe the increase of the crystalline content due to the continuing devitrification under high operating temperature. A continuum damage mechanics (CDM) model is then adapted to model the effects of both cooling induced micro-voids and reheating induced self-healing. This model is applied to model the glass-ceramic G18, a candidate SOFC seal material previously developed at PNNL. Experimentally determined temperature dependent Young’s modulus is used to validate the model predictions

Liu, Wenning N.; Sun, Xin; Khaleel, Mohammad A.

2008-12-01T23:59:59.000Z

405

Which young clusters/associations are we missing today?  

E-Print Network [OSTI]

Currently clusters/associations of stars are mainly detected as surface density enhancements relative to the background field. While clusters form, their surface density increases. It likely decreases again at the end of the star formation process when the system expands as a consequence of gas expulsion. Therefore the surface density of a single cluster can change considerably in young clusters/associations during the first 20 Myr of their development. We investigate the effect of the gas expulsion on the detectability of clusters/associations typical for the solar neighborhood, where the star formation efficiency is 4 Myr only the most massive clusters are identified, while systems with initially M_c < 3 000 M(sun) are missing. The temporal development of stellar properties is usually determined by observing clusters of different ages. The potentially strong inhomogeneity of the cluster sample makes this methods highly questionable. However, GAIA could provide the means to rectify this situation as it w...

Pfalzner, Susanne; Xiang, Mai

2015-01-01T23:59:59.000Z

406

Statistical fractal analysis of 25 young star clusters  

E-Print Network [OSTI]

A large sample of young stellar groups is analysed aiming to investigate their clustering properties and dynamical evolution. A comparison of the Q statistical parameter, measured for the clusters, with the fractal dimension estimated for the projected clouds shows that 52% of the sample has substructures and tends to follow the theoretically expected relation between clusters and clouds, according to calculations for artificial distribution of points. The fractal statistics was also compared to structural parameters revealing that clusters having radial density profile show a trend of parameter s increasing with mean surface stellar density. The core radius of the sample, as a function of age, follows a distribution similar to that observed in stellar groups of Milky Way and other galaxies. They also have dynamical age, indicated by their crossing time that is similar to unbound associations. The statistical analysis allowed us to separate the sample into two groups showing different clustering characteristi...

Gregorio-Hetem, J; Santos-Silva, T; Fernandes, B

2015-01-01T23:59:59.000Z

407

C32, A Young Star Cluster in IC 1613  

E-Print Network [OSTI]

The Local Group irregular galaxy IC 1613 has remained an enigma for many years because of its apparent lack of star clusters. We report the successful search for clusters among several of the candidate objects identified many years ago on photographic plates. We have used a single HST WFPC2 pointing and a series of images obtained with the WIYN telescope under exceptional seeing conditions, examining a total of 23 of the previously published candidates. All but six of these objects were found to be either asterisms or background galaxies. Five of the six remaining candidates possibly are small, sparse clusters and the sixth, C32, is an obvious cluster. It is a compact, young object, with an age of less than 10 million years and a total absolute magnitude of M_V = -5.78+/-0.16 within a radius of 13 pc.

Ted K. Wyder; Paul W. Hodge; Andrew Cole

2000-02-23T23:59:59.000Z

408

Building dwarf galaxies out of merged young star clusters  

E-Print Network [OSTI]

Young star clusters in interacting galaxies are often found in groups or clusters of star clusters containing up to 100 single clusters. In our project we study the future fate of these clusters of star clusters. We find that the star clusters merge on time scales of a few dynamical crossing times of the super-cluster. The resulting merger object has similarities with observed dwarf ellipticals (dE). Furthermore, if destructive processes like tidal heating, dynamical friction or interaction with disc or bulge of the parent galaxy are taken into account our merger objects may evolve into objects resembling dwarf spheroidal galaxies (dSph), without the need of a high dark matter content.

M. Fellhauer

2001-06-22T23:59:59.000Z

409

MID-INFRARED SPECTRAL VARIABILITY ATLAS OF YOUNG STELLAR OBJECTS  

SciTech Connect (OSTI)

Optical and near-infrared variability is a well-known property of young stellar objects. However, a growing number of recent studies claim that a considerable fraction of them also exhibit mid-infrared flux changes. With the aim of studying and interpreting variability on a decadal timescale, here we present a mid-infrared spectral atlas containing observations of 68 low- and intermediate-mass young stellar objects. The atlas consists of 2.5-11.6 {mu}m low-resolution spectra obtained with the ISOPHOT-S instrument on board the Infrared Space Observatory (ISO) between 1996 and 1998, as well as 5.2-14.5 {mu}m low-resolution spectra obtained with the Infrared Spectrograph instrument on board the Spitzer Space Telescope between 2004 and 2007. The observations were retrieved from the ISO and Spitzer archives and were post-processed interactively by our own routines. For those 47 objects where multi-epoch spectra were available, we analyze mid-infrared spectral variability on annual and/or decadal timescales. We identify 37 variable candidate sources. Many stars show wavelength-independent flux changes, possibly due to variable accretion rates. In several systems, all exhibiting 10 {mu}m silicate emission, the variability of the 6-8 {mu}m continuum, and the silicate feature exhibit different amplitudes. A possible explanation is variable shadowing of the silicate-emitting region by an inner disk structure of changing height or extra silicate emission from dust clouds in the disk atmosphere. Our results suggest that mid-infrared variability, in particular, the wavelength-dependent changes, is more ubiquitous than was known before. Interpreting this variability is a new possibility for exploring the structure of the disk and its dynamical processes.

Kospal, A. [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA, Leiden (Netherlands); Abraham, P.; Kun, M.; Moor, A. [Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, P.O. Box 67, 1525 Budapest (Hungary); Acosta-Pulido, J. A. [Instituto de Astrofisica de Canarias, Via Lactea s/n, 38200 La Laguna, Tenerife (Spain); Dullemond, C. P. [Institut fuer Theoretische Astrophysik, Zentrum fuer Astronomie der Universitaet Heidelberg, Albert-Ueberle-Str. 2, 69120 Heidelberg (Germany); Henning, Th.; Leinert, Ch. [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, 69117 Heidelberg (Germany); Turner, N. J., E-mail: akospal@rssd.esa.int [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States)

2012-08-01T23:59:59.000Z

410

Wayne State University Forensics. Director of Forensics: Kelly M. Young (313) 577-2953; email: Kelly.Young@wayne.edu. Director of Debate: Ronald Stevenson (313) 577-2951 email  

E-Print Network [OSTI]

Wayne State University Forensics. Director of Forensics: Kelly M. Young (313) 577-2953; email: Kelly.Young@wayne.edu. Director of Debate: Ronald Stevenson (313) 577-2951 email: Waynedebate Pasquinelli. Back Row: Bruce Najor, Donny Peters, Neil Butt and Kelly Young. Ron Stevenson and David Rancilio

Cinabro, David

411

1D lanthanide halide crystals inserted into single-walled carbon nanotubes Cigang Xu,a Jeremy Sloan,ab Gareth Brown,ab Sam Bailey,a V. Clifford Williams,a Steffi Friedrichs,a Karl S.  

E-Print Network [OSTI]

,ab Gareth Brown,ab Sam Bailey,a V. Clifford Williams,a Steffi Friedrichs,a Karl S. Coleman,a Emmanuel). Images were acquired digitally on a Gatan model 794 (1 k 3

Dunin-Borkowski, Rafal E.

412

Computing with living hardware K.A. Haynes, M.L. Broderick, A.D. Brown, T.L. Butner, L. Harden, L. Heard, E. Jessen, K. Malloy, B. Ogden,  

E-Print Network [OSTI]

Computing with living hardware K.A. Haynes, M.L. Broderick, A.D. Brown, T.L. Butner, L. Harden, L. Heard, E. Jessen, K. Malloy, B. Ogden, S. Rosemond, S. Simpson, E. Zwack, A. Malcolm Campbell, T

Campbell, A. Malcolm

413

The Old Brown Coat Brown Coat Family  

E-Print Network [OSTI]

medicine, pediatrics, pediatric surgery, pediatric radiology and the Sudden Infant Death Services of Illinois. Topics include "Pearls of Pediatric Radiology" by Dr. Schey, The Medically Complex Pediatric Alumni News October 2007 #12;Pediatric Emergency Medicine Conference, Nov 9-10, 2007 UIC proudly

Alford, Simon

414

Description of three ecology studies on brown shrimp Penaeus aztecus and white shrimp P. setiferus conducted by the National Marine Fisheries Service, Galveston, Texas  

E-Print Network [OSTI]

Description of three ecology studies on brown shrimp Penaeus aztecus and white shrimp'P; setiferus conducted by the Mational Marine Fisheries Service, Galveston, Texas. A professional paper by Maria Eugenia de Diego Submitted to the College... shrimp Penaeus aztecus and white shrimp P, set1ferus conducted by the Nat1onal Marine F1sheries Ser- v1ce, Galveston, Texas. (December, 19843 Maria Eugenia de Diego, B. S. , Universidad de Panama Chairman of Adv1sory Committee: Dr. Addison L...

Diego, Maria Eugenia de

1984-01-01T23:59:59.000Z

415

A k-NN METHOD TO CLASSIFY RARE ASTRONOMICAL SOURCES: PHOTOMETRIC SEARCH OF BROWN DWARFS WITH SPITZER/IRAC  

SciTech Connect (OSTI)

We present a statistical method for the photometric search of rare astronomical sources based on the weighted k-Nearest Neighbors method. A metric is defined in a multidimensional color-magnitude space based only on the photometric properties of template sources and the photometric uncertainties of both templates and data, without the need to define ad hoc color and magnitude cuts which could bias the search. The metric is defined as a function of two parameters, the number of neighbors k and a threshold distance D {sub th} that can be optimized for maximum selection efficiency and completeness. We apply the method to the search of L and T dwarfs in the Spitzer Extragalactic First Look Survey and the Booetes field of the Spitzer Shallow Survey, as well as to the search of substellar mass companions around nearby stars. With high level of completeness, we confirm the absence of late-T dwarfs detected in at least two bands in the First Look Survey, and only one in the Shallow Survey (previously discovered by Stern et al.). This result is in agreement with the expected statistics for late-T dwarfs. One L/early-T candidate is found in the First Look Survey, and three in the Shallow Surveys, currently undergoing follow-up spectroscopic verification. Finally, we discuss the potential for brown dwarf searches with this method in the Spitzer warm mission Exploration Science programs.

Marengo, Massimo [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Sanchez, Mayly C. [Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 (United States)], E-mail: mmarengo@cfa.harvard.edu, E-mail: mayly.sanchez@anl.gov

2009-07-15T23:59:59.000Z

416

Biosynthesis and intracellular movement of the melanosomal membrane glycoprotein gp75, the human b (brown) locus product  

SciTech Connect (OSTI)

A 75-kDa melanosomal glycoprotein (gp75) is the product of a gene that maps to the b (brown) locus, a genetic locus that determines coat color in the mouse. The b locus is conserved (88% identity) between mouse and human. The mouse monoclonal antibody TA99 was used to study the biosynthesis and processing of gp75. gp75 was synthesized as a 55-kDa polypeptide, glycosylated by addition and processing of five or more Asn-linked carbohydrate chains through the cis and trans Golgi, and transported to melanosomes as a mature 75-kDa form. Synthesis and processing of gp75 was rapid (T{sub 1/2} < 30 min), and early steps in processing were required for efficient export of gp75 was quite stable in the melanosome. Studies with inhibitors of steps in oligosaccharide processing showed that alternative forms of gp75 were generated during trimming reactions by mannosidase IA/IB and that further maturation resulted in the two mature forms of gp75. The authors purpose that the kinetics of biosynthesis and processing reflect events in the biogenesis and maturation of melanosomes.

Vijayasaradhi, S.; Doskoch, P.M.; Houghton, A.N. (Memorial Sloan-Kettering Cancer Center, New York, NY (United States) Cornell Univ., New York, NY (United States))

1991-10-01T23:59:59.000Z

417

Low-momentum interactions with Brown-Rho-Ericson scalings, and the density dependence of the nuclear symmetry energy  

SciTech Connect (OSTI)

We have calculated the nuclear symmetry energy E{sub sym}({rho}) up to densities of 4-5{rho}{sub 0} with the effects from the Brown-Rho (BR) and Ericson scalings with the in-medium mesons included. Using the V{sub lowk} low-momentum interaction with and without such scalings, the equations of state (EOSs) of symmetric and asymmetric nuclear matter have been calculated using a ring-diagram formalism where the particle-particle-hole-hole ring diagrams are included to all orders. The EOSs for symmetric nuclear matter and neutron matter obtained with linear BR scaling are both overly stiff compared with the empirical constraints of Danielewicz et al. [Science 298, 1592 (2002)]. In contrast, satisfactory results are obtained by either using the nonlinear Ericson scaling or by adding a Skyrme-type three-nucleon force (TNF) to the unscaled V{sub lowk} interaction. Our results for E{sub sym}({rho}) obtained with the nonlinear Ericson scaling are in good agreement with the empirical values of Tsang et al. [Phys. Rev. Lett. 102, 122701 (2009)] and Li et al. [Phys. Rev. C 72, 064611 (2005)], while those with the TNF are slightly below these values. For densities below the nuclear saturation density {rho}{sub 0}, the results of the above calculations are nearly equivalent to each other and all are in satisfactory agreement with the empirical values.

Dong Huan; Kuo, T. T. S.; Machleidt, R. [Department of Physics and Astronomy, Stony Brook University, New York 11794-3800 (United States); Department of Physics, University of Idaho, Moscow, Idaho 83844 (United States)

2011-05-15T23:59:59.000Z

418

Low-momentum interactions with Brown-Rho-Ericson scalings and the density dependence of the nuclear symmetry energy  

E-Print Network [OSTI]

We have calculated the nuclear symmetry energy $E_{sym}(\\rho)$ up to densities of $4 \\sim 5 \\rho_0$ with the effects from the Brown-Rho (BR) and Ericson scalings for the in-medium mesons included. Using the $V_{low-k}$ low-momentum interaction with and without such scalings, the equations of state (EOS) of symmetric and asymmetric nuclear matter have been calculated using a ring-diagarm formalism where the particle-particle-hole-hole ring diagrams are included to all orders. The EOS for symmetric nuclear matter and neutron matter obtained with linear BR scaling are both overly stiff compared with the empirical constraints of Danielewicz {\\it et al.} \\cite{daniel02}. In contrast, satisfactory results are obtained by either using the nonlinear Ericson scaling or by adding a Skyrme-type three-nucleon force (TNF) to the unscaled $V_{low-k}$ interaction. Our results for $E_{sym}(\\rho)$ obtained with the nonlinear Ericson scaling are in good agreement with the empirical values of Tsang {\\it et al.} \\cite{tsang09} a...

Dong, Huan; Machleidt, R

2011-01-01T23:59:59.000Z

419

Low-momentum interactions with Brown-Rho-Ericson scalings and the density dependence of the nuclear symmetry energy  

E-Print Network [OSTI]

We have calculated the nuclear symmetry energy $E_{sym}(\\rho)$ up to densities of $4 \\sim 5 \\rho_0$ with the effects from the Brown-Rho (BR) and Ericson scalings for the in-medium mesons included. Using the $V_{low-k}$ low-momentum interaction with and without such scalings, the equations of state (EOS) of symmetric and asymmetric nuclear matter have been calculated using a ring-diagarm formalism where the particle-particle-hole-hole ring diagrams are included to all orders. The EOS for symmetric nuclear matter and neutron matter obtained with linear BR scaling are both overly stiff compared with the empirical constraints of Danielewicz {\\it et al.} \\cite{daniel02}. In contrast, satisfactory results are obtained by either using the nonlinear Ericson scaling or by adding a Skyrme-type three-nucleon force (TNF) to the unscaled $V_{low-k}$ interaction. Our results for $E_{sym}(\\rho)$ obtained with the nonlinear Ericson scaling are in good agreement with the empirical values of Tsang {\\it et al.} \\cite{tsang09} and Li {\\it et al.} \\cite{li05}, while those with TNF are slightly below these values. For densities below the nuclear saturation density $\\rho_0$, the results of the above calculations are nearly equivalent to each other and all in satisfactory agreement with the empirical values.

Huan Dong; T. T. S. Kuo; R. Machleidt

2011-01-10T23:59:59.000Z

420

The Properties of Young Clusters in M82  

E-Print Network [OSTI]

We present a detailed study of two luminous super star clusters in the starburst galaxy M82. Spectra, covering 3250-8790 A at a resolution of 1.6 A, were obtained at the 4.2 m William Herschel Telescope (WHT) for cluster F and the highly reddened cluster L. We compare the strengths of the observed Balmer absorption lines and the Balmer jump in the blue spectrum of F with theoretical model cluster spectra using the PEGASE spectral synthesis code to derive an age of 60+/-20 Myr. For cluster L, we find that the similarities in the strength of the Ca II triplet and overall spectral appearance with cluster F suggest a similar age. The brightness and compactness of cluster F make it an ideal candidate for determining its dynamical mass by measuring the velocity dispersion. We present the results of such an investigation based on echelle spectra at a resolution of 8 km/s obtained at the WHT from 5760-9140 A. By cross-correlating various wavelength regions in the spectrum of cluster F with cool giant and supergiant template stars, we derive a velocity dispersion and, by application of the virial theorem, determine a dynamical mass of 2 million solar masses. We compare our derived mass with those determined for other young super star clusters and discuss whether our derived parameters are consistent with cluster F being able to survive to become a globular cluster.

L. J. Smith; J. S. Gallagher

2000-01-31T23:59:59.000Z

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


421

Herschel Hi-GAL imaging of massive young stellar objects  

E-Print Network [OSTI]

We used Herschel Hi-GAL survey data to determine whether massive young stellar objects (MYSOs) are resolved at 70$\\mu$m and to study their envelope density distribution. Our analysis of three relatively isolated sources in the l=30{\\deg} and l=59{\\deg} Galactic fields show that the objects are partially resolved at 70$\\mu$m. The Herschel Hi-GAL survey data have a high scan velocity which makes unresolved and partially resolved sources appear elongated in the 70$\\mu$m images. We analysed the two scan directions separately and examine the intensity profile perpendicular to the scan direction. Spherically symmetric radiative transfer models with a power law density distribution were used to study the circumstellar matter distribution. Single dish sub-mm data were also included to study how different spatial information affects the fitted density distribution. The density distribution which best fits both the 70$\\mu$m intensity profile and SED has an average index of ~0.5. This index is shallower than expected an...

Olguin, F A; Wheelwright, H E; Clay, S J; de Wit, W -J; Rafiq, I; Pezzuto, S; Molinari, S

2015-01-01T23:59:59.000Z

422

The Photoevaporation of Discs Around Young Stars in Massive Clusters  

E-Print Network [OSTI]

We present models in which the photoevaporation of discs around young stars by an external ultraviolet source (as computed by Adams et al 2004) is coupled with the internal viscous evolution of the discs. These models are applied to the case of the Orion Nebula Cluster, where the presence of a strong ultraviolet field from the central OB stars, together with a detailed census of circumstellar discs and photoevaporative flows, is well established. In particular we investigate the constraints that are placed on the initial disc properties in the ONC by the twin requirement that most stars possess a disc on a scale of a few A.U., but that only a minority ($ 0.1 M_\\odot$). The ubiquity of discs on a small scale, on the other hand, mainly constrains the timespan over which the discs have been exposed to the ultraviolet field ($< 2 $Myr). We argue that the discs that are resolved by HST represent a population of discs in which self-gravity was important at the time that the dominant central OB star switched on, but that, according to our models, self-gravity is unlikely to be important in these discs at the present time. We discuss the implications of our results for the so-called proplyd lifetime problem.

C. J. Clarke

2007-02-05T23:59:59.000Z

423

Supersonic Line Broadening within Young and Massive Super Star Clusters  

E-Print Network [OSTI]

The origin of supersonic infrared and radio recombination nebular lines often detected in young and massive superstar clusters are discussed. We suggest that these arise from a collection of repressurizing shocks (RSs), acting effectively to re-establish pressure balance within the cluster volume and from the cluster wind which leads to an even broader although much weaker component. The supersonic lines are here shown to occur in clusters that undergo a bimodal hydrodynamic solution (Tenorio-Tagle et al. 2007), that is within clusters that are above the threshold line in the mechanical luminosity or cluster mass vs the size of the cluster (Silich et al. 2004). The plethora of repressurizing shocks is due to frequent and recurrent thermal instabilities that take place within the matter reinserted by stellar winds and supernovae. We show that the maximum speed of the RSs and of the cluster wind, are both functions of the temperature reached at the stagnation radius. This temperature depends only on the cluster...

Tenorio-Tagle, G; Silich, S; Munoz-Tunon, C; Palous, J

2009-01-01T23:59:59.000Z

424

Patent Foramen Ovale and Atrial Septal Aneurysm in Young Adults with Ischemic Stroke.  

E-Print Network [OSTI]

??Ischemic stroke in young adults with patent foramen ovale (PFO) and/or atrial septal aneurysm is underinvestigated. Methods: We investigated 86 such patients (age 16-49 years)… (more)

Tolppanen, Heli

2010-01-01T23:59:59.000Z

425

Eye movements of young and older adults while reading with distraction  

E-Print Network [OSTI]

The authors used eye-tracking technology to examine young and older adults' online performance in the reading in distraction paradigm. Participants read target sentences and answered comprehension questions following each sentence. In some sentences...

Kemper, Susan; McDowd, Joan; Kramer, Arthur F.

2006-03-01T23:59:59.000Z

426

The Influence of praise on help-seeking behavior in young children  

E-Print Network [OSTI]

A. (1995). Young children's help-seeking in mastery-orientedS A. ( 1998). Strategic Help Seeking. Mahwah, NJ: LawrenceNewman, R S. (1994). Adaptive help seeking: A strategy of

Tully, Lisa Marie

2012-01-01T23:59:59.000Z

427

A Research Strategy for Studying Learning Disabled Adolescents and Young Adults  

E-Print Network [OSTI]

Unique problems related to adolescents and young adults which researchers must consider in designing interventions are discussed. These unique factors associate with the condition of learning disabilities in adolescents ...

Schumaker, Jean B.; Alley, Gordon R.; Warner, Michael M.; Deshler, Donald D.

1980-01-01T23:59:59.000Z

428

Tracking Talking: Dual Task Costs of Planning and Producing Speech for Young versus Older Adults  

E-Print Network [OSTI]

A digital pursuit rotor was used to monitor speech planning and production costs by time-locking tracking performance to the auditory wave form produced as young and older adults were describing someone they admire. The ...

Kemper, Susan; Hoffman, Lesa; Schmalzried, RaLynn Cheri; Herman, Ruth; Kieweg, Doug

2011-05-01T23:59:59.000Z

429

Assumptions and Strategies for Conducting Research with Learning Disabled Adolescents and Young Adults  

E-Print Network [OSTI]

This paper details the assumptions about learning disabled adolescents and young adults as well as assumptions about conducting research with this population held by researchers at the Kansas Institute. Strategies developed ...

Meyen, Edward L.; Schiefelbusch, Richard L.; Deshler, Donald D.; Alley, Gordon R.; Moran, Mary Ross; Clark, Frances L.

1980-01-01T23:59:59.000Z

430

A Model for Conducting Research with Learning Disabled Adolescents and Young Adults  

E-Print Network [OSTI]

Issues from the field of learning disabilities and the field of education in general which impact the learning disabled individual are discussed as they relate to research with learning disabled adolescents and young adults ...

Meyen, Edward L.; Schiefelbusch, Richard L.; Deshler, Donald D.; Alley, Gordon R.; Schumaker, Jean B.; Clark, Frances L.

1980-01-01T23:59:59.000Z

431

Young Professionals in Nuclear Industry Group Forms at Savannah River Site  

Broader source: Energy.gov [DOE]

AIKEN, S.C. – Supporting the development of young nuclear professionals in the Central Savannah River Area (CSRA) is the purpose behind a new group forming at the Savannah River Site (SRS).

432

Tracking Reading: Dual Task Costs of Oral Reading for Young Versus Older Adults  

E-Print Network [OSTI]

A digital pursuit rotor was used to monitor oral reading costs by time-locking tracking performance to the auditory wave form produced as young and older adults were reading out short paragraphs. Multilevel modeling was ...

Kemper, Susan; Bontempo, Daniel; Schmalzried, RaLynn Cheri; McKedy, Whitney; Tagliaferri, Bruno; Kieweg, Doug

2014-02-01T23:59:59.000Z

433

Quality of Life Concerns in Young Adult Survivors of Childhood Cancer: A Qualitative Research Investigation  

E-Print Network [OSTI]

Although young adult (YA) survivors of child cancer comprise a unique group from a developmental standpoint, in most treatment and research settings either child or general adult measures of quality of life (QL) are used to measure adjustment...

Puckett, Stevie

2013-06-13T23:59:59.000Z

434

Residential insecticide usage in northern California homes with young XIANGMEI (MAY) WUa  

E-Print Network [OSTI]

Residential insecticide usage in northern California homes with young children XIANGMEI (MAY) WUa of Health and Environment, Seoul National University, Seoul, South Korea Residential insecticide usage and August 2008. Structured telephone interviews were conducted collecting information on residential use

Leistikow, Bruce N.

435

Growing Up in Scotland: Use of Informal Support by Families with Young Children   

E-Print Network [OSTI]

This report, which draws on data from the first sweep of the Growing Up in Scotland study, starts from the position that in order to understand the types of formal support services that parents of young children require....

Bradshaw, Paul; Jamieson, Lynn; Wasoff, Fran

2008-03-12T23:59:59.000Z

436

Eating Attitudes and Behaviours in Young People With or Without a Diabetic Sibling   

E-Print Network [OSTI]

Objectives: Body image concerns and problematic eating attitudes and behaviours are recognised as an important concern for young people and clinicians. Identification of groups that might be at risk of developing such ...

Smith, Rachel K

2007-01-01T23:59:59.000Z

437

Shaking things up: young infants' use of sound information for object individuation  

E-Print Network [OSTI]

SHAKING THINGS UP: YOUNG INFANTS? USE OF SOUND INFORMATION FOR OBJECT INDIVIDUATION A Thesis by TRACY REBECCA SMITH 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 2007 Major Subject: Psychology SHAKING THINGS UP: YOUNG INFANTS? USE OF SOUND INFORMATION FOR OBJECT INDIVIDUATION A Thesis by TRACY REBECCA SMITH Submitted to the Office...

Smith, Tracy Rebecca

2009-05-15T23:59:59.000Z

438

The effect of a new anabolic steroid on spermatogenesis in young stallions  

E-Print Network [OSTI]

THE EFFECT OF A NEW ANABOLIC STEROID ON SPERMATOGENESIS IN YOUNG STALLIONS A Thesis by TOMMY LORAN BULLARD Submitted to the Graduate College of Texas AgiM University in partial fulfillment of the requirement for the degree of MASTER...: (Chairman of ' mrnittee) (Head of Department) (Member) (Member) (Member) May 1971 111 ABSTRACT The Effect of a New Anabolic Steroid on Spermatogenesis in Young Stallions (May 1971) Tommy Loran Bullard, B, S. , Texas AK-M University; D. V. M. , Texas...

Bullard, Tommy Loran

1971-01-01T23:59:59.000Z

439

Water destruction by X-rays in young stellar objects  

E-Print Network [OSTI]

We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemistry is modeled as a function of time, hydrogen density and X-ray flux. To cover a wide range of physical environments, densities between n_H = 10^4-10^9 cm^-3 and temperatures between T = 10-1000 K are studied. Three different regimes are found: For T water abundance is of order 10^-7-10^-6 and can be somewhat enhanced or reduced due to X-rays, depending on time and density. For 100 K 10^-3 ergs s-1 cm^-2 (t = 10^4 yrs) and for F_X > 10^-4 ergs s^-1 cm^-2 (t = 10^5 yrs). At higher temperatures (T > 250 K) and hydrogen densities, water can persist with x(H2O) ~ 10^-4 even for high X-ray fluxes. The X-ray and FUV models are applied to envelopes around low-mass Class 0 and I young stellar objects (YSOs). Water is destroyed in both Class 0 and I envelopes on relatively short timescales (t ~ 5000 yrs) for realistic X-ray fluxes, although the effect is less prominent in Class 0 envelopes due to the higher X-ray absorbing densities there. FUV photons from the central source are not effective in destroying water. The average water abundance in Class I sources for L_X > 10^27 ergs s^-1 is predicted to be x(H2O) < 10^-6.

P. Stauber; J. K. Jorgensen; E. F. van Dishoeck; S. D. Doty; A. O. Benz

2006-02-06T23:59:59.000Z

440

SMU, Dept of Electrical Engineering Dallas, Texas 75275  

E-Print Network [OSTI]

on surfing habits Hijacks Web searches and IE settings Tricks user by claiming to delete porn Bundled

Chen, Thomas M.

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


441

alcaeorrhynchus grandis dallas: Topics by E-print Network  

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

Summary: ? intelligent landscaping ? efficient MEP systems ? 53 well geothermal heat pump system ? greywater recapture and reuse ? 7.7 kw photovoltaic array key...

442

The University of Texas at Dallas FACILITIES MANAGEMENT  

E-Print Network [OSTI]

Communications Special Projects Haywood McNeill* Energy Conservation/ Sustainability Building Maintenance

O'Toole, Alice J.

443

The University of Texas at Dallas Facilities Management  

E-Print Network [OSTI]

Communications Special Projects Chase York Williams* Energy Conservation/ Sustainability Building Maintenance

O'Toole, Alice J.

444

THE UNIVERSITY OF TEXAS AT DALLAS INFORMATION SECURITY  

E-Print Network [OSTI]

. Instead, these requirements should be integrated into a comprehensive system security plan. II. Scope

O'Toole, Alice J.

445

Official Approved Minutes UT DALLAS STAFF COUNCIL MEETING MINUTES  

E-Print Network [OSTI]

. UNIVERSITY SAFETY AND SECURITY (Lynne Boyer) v. WOMEN'S CENTER (Jacqueline Long) vi. IR SECURITY, PLANNING

O'Toole, Alice J.

446

Dallas: Building a Greener City | Department of Energy  

Energy Savers [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 Delicious RankCombustion |Energy UsageAUDITVehiclesTanklessDOJ Title Standards for Acquisition DOJ Title

447

Dallas County, Alabama: 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 Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation, search GEOTHERMALDale Renewables Consulting7. It is

448

Dallas County, Arkansas: 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 Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation, search GEOTHERMALDale Renewables Consulting7. It is0346533°,

449

Dallas County, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation, search GEOTHERMALDale Renewables Consulting7. It

450

Dallas County, Missouri: 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 Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to: navigation, search GEOTHERMALDale Renewables Consulting7. It6853001°,

451

Clean Cities: Dallas-Fort Worth Clean Cities coalition  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation Proposed New SubstationClean Communities of Western New York (Buffalo)

452

Dallas County, Texas: 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 Office of InspectorConcentratingRenewable Solutions LLC JumpCrow Lake Wind107 CX at North BrawleyDNADTETexas: Energy

453

Sevin Rosen Funds (Texas - Dallas) | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty Ltd Jump to: navigation, search| Open EnergySermatecMile,Seville, Ohio:-

454

Alternative Fuels Data Center: Dallas Airport Operates With Alternative  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout theOFFICE OFFuels in Its Fleeton AlternativeEthanol Use,

455

Alternative Fuels Data Center: Dallas Police Department Reduces Vehicle  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout theOFFICE OFFuels in Its Fleeton AlternativeEthanol

456

Lake Dallas, Texas: 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 Home5b9fcbce19 No revision hasInformation Earth's Heat JumpInc Place:Keystone Clean Airjoin < LEDSGPLouisiana:Ohio. Its

457

Continuous Commissioningź of the Dallas/Fort Worth International Airport  

E-Print Network [OSTI]

and cost savings. The Energy Systems Laboratory was hired to apply the Continuous Commissioning ? (CC ? ) 1 process at the airport. Five projects have been identified to date including: 1. An energy audit and assessment of Terminal B and a lighting... on the completed projects: the Consolidated Rent-A-Car Center, the Airport Administration Building, and the major on-going projects, CC of Terminal D and Energy Plaza. 1 Both Continuous Commissioning and CC...

Yazdani, B.; Schroeder, F.; Kramer, L.; Baltazar, J. C.; Turner, W. D.; Wei, G.; Deng, S.; Henson, R.; Dennis, J. R.; T., R.

458

Radio Frequency Identification (RFID) Stakeholder Meeting Dallas, Texas  

E-Print Network [OSTI]

Discussion Points · Participants highlighted the need to establish performance criteria and business rules Associations, with assistance of EPA Region 6 and Texas Commission on Environmental Quality. · Texas of Enforcement and Compliance Assurance Davis Jones, U.S. EPA Office of Enforcement and Compliance Assurance

459

Effect of Solar Radiation on the Optical Properties and Molecular Composition of Laboratory Proxies of Atmospheric Brown Carbon  

SciTech Connect (OSTI)

Sources, optical properties, and chemical composition of atmospheric brown carbon (BrC) aerosol are uncertain, making it challenging to estimate its contribution to radiative forcing. Furthermore, optical properties of BrC may change significantly during its atmospheric aging. We examined the effect of solar photolysis on the molecular composition, mass absorption coefficient, and fluorescence of secondary organic aerosol prepared by high-NOx photooxidation of naphthalene (NAP SOA). The aqueous solutions of NAP SOA was observed to photobleach with an effective half-time of ?15 hours (with sun in its zenith) for the loss of the near-UV (300 -400 nm) absorbance. The molecular composition of NAP SOA was significantly modified by photolysis, with the average SOA formula changing from C14.1H14.5O5.1N0.08 to C11.8H14.9O4.5N0.02 after 4 hours of irradiation. The average O/C ratio did not change significantly, however, suggesting that it is not a good metric for assessing the extent of photolysis-driven aging in NAP SOA (and in BrC in general). In contrast to NAP SOA, the photolysis of BrC material produced by aqueous reaction of limonene+O3 SOA (LIM/O3 SOA) with ammonium sulfate was much faster, but it did not result in a significant change in the molecular level composition. The characteristic absorbance of the aged LIM/O3 SOA in the 450-600 nm range decayed with an effective half-time of <0.5 hour. This result emphasizes the highly variable and dynamic nature of different types of atmospheric BrC.

Lee, Hyun Ji; Aiona, Paige K.; Laskin, Alexander; Laskin, Julia; Nizkorodov, Sergey

2014-09-02T23:59:59.000Z

460

A study of the distribution and condition of brown shrimp in the primary nursery areas of the Galveston Bay System, Texas  

E-Print Network [OSTI]

A STUDY OF THE DISTRIBUTION AND CONDITION OF BROWN SHRIMP IN THE PRIMARY NURSERY AREAS OF THE GALVESTON BAY SYSTEM, TEXAS A Thesis by Jack Clark Parker Submitted to the Graduate College of the Texas A&M University in partial fulfillment... of the requirements for the degree of MASTER OF SCIENCE May 1966 Major Subject: Biological Oceanography A STUDY OF THE DISTRIBUTION AND CONDITION OF BROHN SHRIMP IN THE PRIMARY NURSERY AREAS OF THE GALVESTON BAY SYSTEM, TEXAS A Thesis Jack Clark Parker...

Parker, Jack C

1966-01-01T23:59:59.000Z

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


461

Intel / Charles E. Young Endowed Chair in Nanotechnology Director of the Nanoscience Institute for Medical and Engineering Technology  

E-Print Network [OSTI]

Intel / Charles E. Young Endowed Chair in Nanotechnology Director of the Nanoscience Institute of the Nanoscience Institute for Medical and Engineering Technology. The Intel Foundation established this endowment

Slatton, Clint

462

AGE AND MASS STUDIES FOR YOUNG STAR CLUSTERS IN M31 FROM SEDS-FIT  

SciTech Connect (OSTI)

In this paper, we present photometry for young star clusters in M31, which are selected from Caldwell et al. These star clusters have been observed as part of the Beijing-Arizona-Taiwan-Connecticut (BATC) Multicolor Sky Survey from 1995 February to 2008 March. The BATC images including these star clusters are taken with 15 intermediate-band filters covering 3000-10000 A. Combined with photometry in the GALEX far- and near-ultraviolet, broadband UBV RI, SDSS ugriz, and infrared JHK{sub s} of Two Micron All Sky Survey, we obtain their accurate spectral energy distributions (SEDs) from 1538 to 20000 A. We derive these star clusters' ages and masses by comparing their SEDs with stellar population synthesis models. Our results are in good agreement with previous determinations. The mean value of age and mass of young clusters (<2 Gyr) is about 385 Myr and 2 Multiplication-Sign 10{sup 4} M{sub Sun }, respectively. There are two distinct peaks in the age distribution, a highest peak at age {approx}60 Myr and a secondary peak around 250 Myr, while the mass distribution shows a single peak around 10{sup 4} M{sub Sun }. A few young star clusters have two-body relaxation times greater than their ages, indicating that those clusters have not been well dynamically relaxed and therefore have not established the thermal equilibrium. There are several regions showing aggregations of young star clusters around the 10 kpc ring and the outer ring, indicating that the distribution of the young star clusters is well correlated with M31's star-forming regions. The young massive star clusters (age {<=}100 Myr and mass {>=}10{sup 4} M{sub Sun }) show apparent concentration around the ring splitting region, suggesting a recent passage of a satellite galaxy (M32) through M31 disk.

Wang Song; Ma Jun; Fan Zhou; Wu Zhenyu; Zhang Tianmeng; Zou Hu; Zhou Xu, E-mail: majun@nao.cas.cn [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)

2012-12-01T23:59:59.000Z

463

Interview of Dan Brown  

E-Print Network [OSTI]

progress at school, particularly maths; mother had been a teacher for a short time and helped with English; did not have a large library of books but father did give me 'The World of Science' by Sherwood Taylor; my interest in chemistry evident when I went... of organic chemistry up to the time I was learning it at university was almost all carbon chemistry; suddenly people started looking at esters, carbonyl compounds; then when Todd started on the phosphorus chemistry, that was almost another kind of chemistry...

Brown, Dan

2008-06-09T23:59:59.000Z

464

Brown Chapter 2  

E-Print Network [OSTI]

tions, the ?rst two coverages are compulsory in that the law requires each auto ..... caused by nuclear accidents or acts of war are not covered, nor are buildings

465

Brown Chapter 2  

E-Print Network [OSTI]

settlement: In this case, the court may have to make a two- part deciswn. .... to take the vehicle to a wrecker and retain any salvage value ... For example, if a ?re causes a power outage, and as a result of ... after year (at least nothing in excess of the deductible). ..... apartment building is damaged by wind, ?re or other insured.

466

Lawrence G Brown: Publications  

E-Print Network [OSTI]

In Geometric methods in operator algebras (Kyoto, 1983), volume 123 of Pitman Res. Notes Math. Ser., pages 1-35. Longman Sci. Tech., Harlow, 1986.

467

Brown Chapter 1  

E-Print Network [OSTI]

associated with the injury of a third party in a car accident for which you are responsible. Examples of early informal insurance arrangements can be found in the ...

468

Nuclear power browning out  

SciTech Connect (OSTI)

When the sad history of nuclear power is written, April 26, 1986, will be recorded as the day the dream died. The explosion at the Chernobyl plant was a terrible human tragedy- and it delivered a stark verdict on the hope that nuclear power will one day replace fossil fuel-based energy systems. Nuclear advocates may soldier on, but a decade after Chernobyl it is clear that nuclear power is no longer a viable energy option for the twenty-first century.

Flavin, C.; Lenssen, N.

1996-05-01T23:59:59.000Z

469

David ML Brown | EMSL  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation Proposed Newcatalyst phasesData Files Data Files 1 EIA BestDavid HoytDavid Lee, DouglasM.David

470

David ML Brown | EMSL  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc DocumentationP-Series to UserProduct: CrudeOffice ofINL is aID ServiceHoytL. Greene (1999)ML

471

Shaun D Brown | EMSL  

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

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

472

brown-98.pdf  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWasteupc-unified-parallel-c/upc-bug-reports/ DeadlockbostonlogosHigh

473

brown-99.PDF  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched FerromagnetismWasteupc-unified-parallel-c/upc-bug-reports/

474

Shaun D Brown | EMSL  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administrationcontroller systemsBi (2)Sharing Smart Grid Experiences through

475

Young Pulsars and the Galactic Center GeV Gamma-ray Excess  

E-Print Network [OSTI]

Studies of Fermi data indicate an excess of GeV gamma rays around the Galactic center (GC), possibly due to dark matter. We show that young gamma-ray pulsars can yield a similar signal. First, a high concentration of GC supernovae naturally leads to a population of kicked pulsars symmetric about the GC. Second, while very-young pulsars with soft spectra reside near the Galactic plane, pulsars with spectra that have hardened with age accumulate at larger angles. This combination, including unresolved foreground pulsars, traces the morphology and spectrum of the Excess.

O'Leary, Ryan M; Kerr, Matthew; Dexter, Jason

2015-01-01T23:59:59.000Z

476

Structure and Evolution of Circumstellar Disks Around Young Stars: New Views from ISO  

E-Print Network [OSTI]

A question central to understanding the origin of our solar system is: how do planets form in circumstellar disks around young stars? Because of the complex nature of the physical processes involved, multi-wavelength observations of large samples will be required in order to obtain a complete answer to this question. Surveys undertaken with ISO have helped to solve pieces of this puzzle in addition to uncovering new mysteries. We review a variety of studies aimed at understanding; i) the physical structure and composition of circumstellar disks commonly found surrounding young stellar objects; and ii) the evolution of circumstellar disks from the active accretion phase to post-planet building debris disks.

Michael R. Meyer; Steven V. W. Beckwith

2000-01-31T23:59:59.000Z

477

Log of a young author's thinking: George W. Cable's "Drop Shot".  

E-Print Network [OSTI]

. . t 1974 Major Subject: English LOG OF A YOUNG AUTHOR'S THINKING: GEORGE W CABLE'S "DROP SHOT" A Thesis by AUTRY JAMES SINITIERE Approved as to style and content by: Chairman of Committe Hea of Department M er ember) August 1974 & s ~~. )$, gg... APSTRACT Log of a Young Author's Thinking: George W. Cable's "Drop Shot" (August 1974) Autry James Sinitiere, B. A. , College of Santa Fe Chairman of Advisory Committee: Dr Richard H. Ballinger In February 1870 George W. Cable began writing a * p p...

Sinitiere, Autry James

1974-01-01T23:59:59.000Z

478

Interspecific Variability of Biomass Production of Young Coffea: No Influence of Branch Pruning. Experimental Evidence and Theoretical Analysis  

E-Print Network [OSTI]

Interspecific Variability of Biomass Production of Young Coffea: No Influence of Branch Pruning diversity and architectural plasticity. In this study, we investigated the biomass production and allocation treatment had no influence on biomass production and allocation for these young trees. We propose

Boyer, Edmond

479

You are invited to the 8th Annual Africa Institute of South Africa's (AISA) Young Graduates and Scholars Conference  

E-Print Network [OSTI]

You are invited to the 8th Annual Africa Institute of South Africa's (AISA) Young Graduates, Botswana, Belgium, Kenya, and South Africa. The participants are from multidisciplinary backgrounds. Key Institute of South Africa's (AISA) Young Graduates and Scholars Conference (AYGS) University of Johannesburg

Wagner, Stephan

480

Conditions Under Which Young Children Can Hold Two Rules in Mind and Inhibit a Prepotent Response  

E-Print Network [OSTI]

Conditions Under Which Young Children Can Hold Two Rules in Mind and Inhibit a Prepotent Response Adele Diamond, Natasha Kirkham, and Dima Amso Eunice Kennedy Shriver Center, University of Massachusetts their performance. What helped was reducing the inhibitory demand by instructing them to say "dog" and "pig" (not

Kirkham, Natasha Z.

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


481

The impact of binge drinking on the young growing female rat skeleton  

E-Print Network [OSTI]

, on the actively growing skeleton. The objective of this study was to determine whether or not binge drinking impacts the normal growth process of the young growing female rat skeleton. Twelve, four-week-old, female rats were paired to form an ethanol group and a...

Gallagher, Sharon Lee

1997-01-01T23:59:59.000Z

482

An experience of young software engineers' employability in the Moroccan offshore industry  

E-Print Network [OSTI]

An experience of young software engineers' employability in the Moroccan offshore industry Philippe the emergence of an offshore software development industry in Morocco. A network of eight Moroccan universities and the University of Brest has set up a mobility scheme for Moroccan Master students. The OTI programme "Offshoring

Paris-Sud XI, Université de

483

Survival on the ark: life-history trends in captive parrots A. M. Young1  

E-Print Network [OSTI]

demonstrate the value of the ISIS database to estimate life-history data for an at-risk taxonSurvival on the ark: life-history trends in captive parrots A. M. Young1 , E. A. Hobson1 , L 2 International Species Information System, Eagan, MN, USA Keywords captive breeding; ISIS; life-history

Wright, Timothy F.

484

CONSIDERATION OF THREE PROPOSED MODELS OF THE MIGRATION OF YOUNG SKIPJACK TUNA (KATSUWONUS PELAMIS)  

E-Print Network [OSTI]

CONSIDERATION OF THREE PROPOSED MODELS OF THE MIGRATION OF YOUNG SKIPJACK TUNA (KATSUWONUS PELAMIS (KatsuUJonus pelamis) in in the eastern Pacific Ocean have a central racific spawning origin. Three (Katsuwonus pelamis) are widely distributed in tropical and subtropical surface waters of world oceans

485

Elephant spatial use in wet and dry savannas of southern K. D. Young1  

E-Print Network [OSTI]

Elephant spatial use in wet and dry savannas of southern Africa K. D. Young1 , S. M. Ferreira1 Keywords elephants; home range; Loxodonta africana; NDVI; spatial use intensity; vegetation productivity; accepted 16 February 2009 doi:10.1111/j.1469-7998.2009.00568.x Abstract The influence of elephants on woody

Pretoria, University of

486

SIZE COMPOSITION AND GROWTH OF YOUNG ROCK CRAB, CANCER IRRORATUS, ON A ROCKY BEACH IN MAINE!  

E-Print Network [OSTI]

. Because rock crab is a valuable commercial species as well as an important food source of lobsters (EnnisSIZE COMPOSITION AND GROWTH OF YOUNG ROCK CRAB, CANCER IRRORATUS, ON A ROCKY BEACH IN MAINE! JAY S KROUSE' ABSTRACT Monthly hand collections of small rock crab, Cancer irrorallls, were made from

487

Ontogenetic and Seasonal Variation of Young Non-Native Fish Energy Densities in Lake Michigan  

E-Print Network [OSTI]

-specific trade-offs between energy allocation to different tissue-types (low energy density, structural tissueOntogenetic and Seasonal Variation of Young Non-Native Fish Energy Densities in Lake Michigan Overview Energy content is a useful metric of physiological status of fishes and may help elucidate spatial

488

YOUNG JIN LEE, PH D 3756 Gilman, Department of chemistry, Iowa State University, Ames, IA  

E-Print Network [OSTI]

Spectrometry Imaging for the Localization of Plant Lipids in High Spatial Resolution", Young Jin Lee, Gordon, Galveston, TX. 2. "Single Cell Level, High Spatial Resolution Mass Spectrometry Imaging for Plant activated dissociation of some high mass ions; Analysis of mass-analyzed ion kinetic energy peak shapes", Y

Clemmer, David E.

489

ASTRONOMY TO INSPIRE AND EDUCATE YOUNG CHILDREN EU-UNAWE Lorentz Center Workshop  

E-Print Network [OSTI]

ASTRONOMY TO INSPIRE AND EDUCATE YOUNG CHILDREN EU-UNAWE Lorentz Center Workshop Official Opening. Mitchell, MEP, Chair, EU Parliamentary Committee on Development Astronomy Research and Education in South Committee for Education, Culture and Science Video messages (5 min) Astronomy and Space collaborations

Galis, Frietson

490

Hot stars in young massive clusters: Mapping the current Galactic metallicity  

E-Print Network [OSTI]

for Detectors, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623, USA (4) Instituto). Notice the different flux scales. ACKNOWLEDGEMENTS: This project is partially supported by the Spanish extincted regions of the Galactic disk. Also, the young ages of blue massive stars (

Figer, Donald F.

491

The Astrophysical Journal, in press A Determination of the Coronal Emission Measure Distribution in the Young  

E-Print Network [OSTI]

to this temperature regime. We argue that the DEM distribution seen in EK Dra is induced by the propertiesThe Astrophysical Journal, in press A Determination of the Coronal Emission Measure Distribution of a coronal differential emission measure (DEM) analysis of the nearby analog of the young Sun, EK Draconis

Guedel, Manuel

492

Ca RETENTION IN YOUNG PULLETS AND LAYING HENS FED A Ca47 LABELLED DIET  

E-Print Network [OSTI]

Ca RETENTION IN YOUNG PULLETS AND LAYING HENS FED A Ca47 LABELLED DIET OF DIFFERENT Ca LEVELS K levels of dietary calcium. A basal diet poor in calcium but otherwise optimal was supplemented with CaC03 and Na2HP04 as seen below : #12;CaCO, supplement of the diet was replaced by Ca&dquo; labelled Calcium

Paris-Sud XI, Université de

493

"Help! What do I do now?": interactive help for young children -a case study  

E-Print Network [OSTI]

"Help! What do I do now?": interactive help for young children - a case study Tony Nicol Department An effective help system is an essential feature of any user-centric computer application. There is a wealth of knowledge and support tools available to aid in the development of help systems for adults but relatively

494

Young Children Selectively Avoid Helping People With Harmful Intentions Amrisha Vaish, Malinda Carpenter, and Michael Tomasello  

E-Print Network [OSTI]

Young Children Selectively Avoid Helping People With Harmful Intentions Amrisha Vaish, Malinda. In Study 1 (N = 54), 3-year-olds watched 1 adult (the actor) harming or helping another adult. Children subsequently helped the harmful actor less often than a third (previously neutral) adult, but helped

Carpenter, M.alinda

495

Be production-rate calibration for the Arctic NICOLA S E. YOUNG,1,2  

E-Print Network [OSTI]

A 10 Be production-rate calibration for the Arctic NICOLAÂŽ S E. YOUNG,1,2 * JOERG M. SCHAEFER,1 2013; Accepted 18 April 2013 ABSTRACT: We present a Baffin Bay 10 Be production-rate calibration published 10 Be calibration datasets to develop an Arctic 10 Be production rate. Our calibration comprises

Briner, Jason P.

496

Unsolved problems for young and old 1 The lure of an unsolved problem  

E-Print Network [OSTI]

Norman Do Unsolved problems for young and old 1 The lure of an unsolved problem In his superb by Andrew Wiles after an incredible eight years of continuous toil spent searching for the Holy Grail on the backs of envelopes, #12;84 Norman Do and passed on by word of mouth until some very clever person can

Do, Norman

497

We often think about energy in personal terms. People comment on the energy young children  

E-Print Network [OSTI]

Overview We often think about energy in personal terms. People comment on the energy young children seem to possess. Others mention that they don't feel they have enough energy to make it through the day. We've heard that the world is running out of certain types of energy. In spite of all of our everyday

Hardy, Darel

498

The Smith Normal Form of a Matrix Associated with Young's Lattice  

E-Print Network [OSTI]

The Smith Normal Form of a Matrix Associated with Young's Lattice Tommy Wuxing Cai and Richard P. Stanley Abstract. We prove a conjecture of Miller and Reiner on the Smith normal form of the operator DU be a commutative ring with 1 and M an mĂ?m matrix over R. We say that M has a Smith normal form (SNF) over R

499

Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.202) Track: Technical  

E-Print Network [OSTI]

tower-mounted instruments. Typical turbine hub heights are now in excess of 70m. For such machinesSession: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.202) Track: Technical COMMERCIAL LIDAR PROFILERS FOR WIND ENERGY. A COMPARATIVE GUIDE. (abstract

500

Effect of the Young modulus variability on the mechanical behaviour of a nuclear containment vessel  

E-Print Network [OSTI]

Effect of the Young modulus variability on the mechanical behaviour of a nuclear containment vessel on the mechanical behaviour of a nuclear containment vessel in case of a loss of cooling agent accident and under values are observed. Preprint submitted to Nuclear Engineering and Design April 19, 2010 hal-00542640