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1

Blue Star Memorial By-Way Dedication: Weldon Spring Interpretive Center |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Blue Star Memorial By-Way Dedication: Weldon Spring Interpretive Blue Star Memorial By-Way Dedication: Weldon Spring Interpretive Center Blue Star Memorial By-Way Dedication: Weldon Spring Interpretive Center July 12, 2013 - 1:04pm Addthis Since 2003, the Lewis and Clark Garden Club (LCGC) of St. Charles County, Missouri, has held their monthly meetings in the Weldon Spring Interpretive Center (WSIC). The LCGC has 22 active members and takes care of 2 garden beds at the WSIC Native Plant Educational Garden under the site's Adopt-A-Garden program. In 2010 the LCGC contacted the U.S. Department of Energy (DOE), seeking approval to install a Blue Star Memorial By-Way Marker as a tribute to the nation's armed forces (see bottom of page for a history of the Blue Star Memorials). A 2,300-pound pink mica memorial marker was placed

2

Blue Star Energy Services | Open Energy Information  

Open Energy Info (EERE)

BlueStar) BlueStar) Jump to: navigation, search Name Blue Star Energy Services Place Illinois Utility Id 55722 Utility Location Yes Ownership R NERC Location RFC NERC RFC Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates Residential: $0.1180/kWh Commercial: $0.0687/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Star_Energy_Services&oldid=409064" Categories: EIA Utility Companies and Aliases

3

Blue Star Energy Services | Open Energy Information  

Open Energy Info (EERE)

Blue Star Energy Services Place Illinois Utility Id 55722 Utility Location Yes Ownership R NERC Location RFC NERC RFC Yes Activity Retail Marketing Yes References EIA Form EIA-861...

4

Blue Star Energy Services (Maryland) | Open Energy Information  

Open Energy Info (EERE)

Maryland) Maryland) Jump to: navigation, search Name Blue Star Energy Services Place Maryland Utility Id 55722 References EIA Form EIA-861 Final Data File for 2010 - File2_2010[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates Commercial: $0.0994/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File2_2010" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Star_Energy_Services_(Maryland)&oldid=412437" Categories: EIA Utility Companies and Aliases Utility Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link

5

IDENTIFYING BLUE HORIZONTAL BRANCH STARS USING THE z FILTER  

SciTech Connect

In this paper we present a new method for selecting blue horizontal branch (BHB) candidates based on color-color photometry. We make use of the Sloan Digital Sky Survey z band as a surface gravity indicator and show its value for selecting BHB stars from quasars, white dwarfs, and main-sequence A-type stars. Using the g, r, i, and z bands, we demonstrate that extraction accuracies on a par with more traditional u, g, and r photometric selection methods may be achieved. We also show that the completeness necessary to probe major Galactic structure may be maintained. Our new method allows us to efficiently select BHB stars from photometric sky surveys that do not include a u-band filter such as the Panoramic Survey Telescope and Rapid Response System.

Vickers, John J.; Grebel, Eva K.; Huxor, Avon P., E-mail: jvickers@ari.uni-heidelberg.de [Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Moenchhofstr. 12-14, 69120 Heidelberg (Germany)

2012-04-15T23:59:59.000Z

6

Performance and scalability evaluation of "Big Memory" on Blue Gene Linux.  

Science Conference Proceedings (OSTI)

We address memory performance issues observed in Blue Gene Linux and discuss the design and implementation of 'Big Memory' - an alternative, transparent memory space introduced to eliminate the memory performance issues. We evaluate the performance of Big Memory using custom memory benchmarks, NAS Parallel Benchmarks, and the Parallel Ocean Program, at a scale of up to 4,096 nodes. We find that Big Memory successfully resolves the performance issues normally encountered in Blue Gene Linux. For the ocean simulation program, we even find that Linux with Big Memory provides better scalability than does the lightweight compute node kernel designed solely for high-performance applications. Originally intended exclusively for compute node tasks, our new memory subsystem dramatically improves the performance of certain I/O node applications as well. We demonstrate this performance using the central processor of the LOw Frequency ARray radio telescope as an example.

Yoshii, K.; Iskra, K.; Naik, H.; Beckman, P.; Broekema, P. C. (LCF); ( MCS); (Netherlands Inst. for Radio Astronomy)

2011-05-01T23:59:59.000Z

7

Dust-to-gas ratio and star formation history of blue compact dwarf galaxies  

E-Print Network (OSTI)

This paper investigates the origin of the observed large variety in dust-to-gas ratio among blue compact dwarf galaxies (BCDs). By applying our chemical evolution model, we find that the dust destruction can largely suppress the dust-to-gas ratio when the metallicity of a BCD reaches $12+\\log{\\rm (O/H)}\\sim 8$, i.e., a typical metallicity level of BCDs. We also show that dust-to-gas ratio is largely varied owing to the change of dust destruction efficiency that has two effects: (i) a significant contribution of Type Ia supernovae to total supernova rate; (ii) variation of gas mass contained in a star-forming region. While mass loss from BCDs was previously thought to be the major cause for the variance of dust-to-gas ratio, we suggest that the other two effects are also important. We finally discuss the intermittent star formation history, which naturally explains the large dispersion of dust-to-gas ratio among BCDs.

H. Hirashita; Y. Y. Tajiri; H. Kamaya

2002-04-18T23:59:59.000Z

8

Bending of Light Near a Star and Gravitational Red/Blue Shift : Alternative Explanation Based on Refraction of Light  

E-Print Network (OSTI)

Many of the general-relativity-tests such as bending of light near a star and gravitational red/blue shift are explained without general-relativity and without Newtonian-approach. The author first casts doubts on both, the Newtonian and the relativistic approach; and proposes a novel alternative-explanation. The new alternative-explanation is based on refraction-phenomenon of optics. It predicts that as the ray passes through/near the stars atmospheric-medium, it bends due to refraction-phenomenon towards star-core, like a ray bends while passing through a prism or water-drop. A semi-empirical estimation of the atmospheric-height and its refractive-index are made to find the refraction-results. The refraction-based theory also suggests new explanation for gravitational red/blue shift; it tells that frequency remains constant (as it is so in refraction-phenomenon) and the red/blue shift is due to change in wavelength due to change in velocity of light in the medium . Estimated results for bending of light and the red/blue shift etc. with the new approach though agree well with known values, but important thing is that the physics is quite different. The proposed refraction-based theory proposes a new-look on black-hole, suggesting that black-hole formation is critically due to total-internal-reflection within atmosphere and subsequent absorption into the star-core. Gravitational-lensing is explained as real refraction-lensing. The present paper also suggests a possible-alternative and meaning to the curved geometry of space-time, and indicates that the fabric of space-time which warps(curves) around the mass is not the empty-vacuum but the atmospheric-medium.

Dr. R. C. Gupta

2004-09-24T23:59:59.000Z

9

THE EFFECT OF THE {sup 14}N(p, {gamma}){sup 15}O REACTION ON THE BLUE LOOPS IN INTERMEDIATE-MASS STARS  

SciTech Connect

We present stellar evolutionary sequences of stars in the mass range 5-12 M{sub Sun }, having solar-like initial composition. The stellar models are obtained using updated input physics, including recent rates of thermonuclear reactions. We investigate the effects of a modification of the {sup 14}N(p, {gamma}){sup 15}O reaction rate, as suggested by recent evaluations, on the formation and extension of the blue loops encountered during the evolution of the stars in the above mass range. We find that a reduced {sup 14}N(p, {gamma}){sup 15}O rate, as described in the text, has a striking impact on the physical conditions of burning and mixing during shell hydrogen burning when the blue loops are formed. In particular, we find that the efficiency of shell hydrogen burning is crucial for the formation of an extended blue loop. We show that a significantly reduced {sup 14}N(p, {gamma}){sup 15}O rate affects severely the extension of the blue loops and the time spent by the star in the blue part of the Hertzsprung-Russell diagram in the mass range 5-7 M{sub Sun} if the treatment of convection is based on the Schwarzschild criterion only. In this case, envelope overshooting helps to restore well-extended blue loops as supported by the observations of the Cepheid stars. If core overshooting is included during the core hydrogen and core helium burning phases, the loop formation and its properties depend on how this overshooting is treated for a given stellar mass range, as well as on its efficiency.

Halabi, Ghina M.; El Eid, Mounib F. [Department of Physics, American University of Beirut, Beirut (Lebanon); Champagne, Arthur [Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC (United States)

2012-12-10T23:59:59.000Z

10

THE RISE AND FALL OF THE STAR FORMATION HISTORIES OF BLUE GALAXIES AT REDSHIFTS 0.2 < z < 1.4  

Science Conference Proceedings (OSTI)

Popular cosmological scenarios predict that galaxies form hierarchically from the merger of many progenitors, each with their own unique star formation history (SFH). We use a sophisticated approach to constrain the SFHs of 4517 blue (presumably star-forming) galaxies with spectroscopic redshifts in the range 0.2 < z < 1.4 from the All-Wavelength Extended Groth Strip International Survey. This consists in the Bayesian analysis of the observed galaxy spectral energy distributions with a comprehensive library of synthetic spectra assembled using realistic, hierarchical star formation, and chemical enrichment histories from cosmological simulations. We constrain the SFH of each galaxy in our sample by comparing the observed fluxes in the B, R, I, and K{sub s} bands and rest-frame optical emission-line luminosities with those of one million model spectral energy distributions. We explore the dependence of the resulting SFHs on galaxy stellar mass and redshift. We find that the average SFHs of high-mass galaxies rise and fall in a roughly symmetric bell-shaped manner, while those of low-mass galaxies rise progressively in time, consistent with the typically stronger activity of star formation in low-mass compared to high-mass galaxies. For galaxies of all masses, the star formation activity rises more rapidly at high than at low redshift. These findings imply that the standard approximation of exponentially declining SFHs widely used to interpret observed galaxy spectral energy distributions may not be appropriate to constrain the physical parameters of star-forming galaxies at intermediate redshifts.

Pacifici, Camilla [Yonsei University Observatory, Yonsei University, Seoul 120-749 (Korea, Republic of); Kassin, Susan A.; Gardner, Jonathan P. [Astrophysics Science Division, Goddard Space Flight Center, Code 665, Greenbelt, MD 20771 (United States); Weiner, Benjamin [Steward Observatory, 933 North Cherry Street, University of Arizona, Tucson, AZ 85721 (United States); Charlot, Stephane [UPMC-CNRS, UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris (France)

2013-01-01T23:59:59.000Z

11

DIRECT N-BODY MODELING OF THE OLD OPEN CLUSTER NGC 188: A DETAILED COMPARISON OF THEORETICAL AND OBSERVED BINARY STAR AND BLUE STRAGGLER POPULATIONS  

SciTech Connect

Following on from a recently completed radial-velocity survey of the old (7 Gyr) open cluster NGC 188 in which we studied in detail the solar-type hard binaries and blue stragglers of the cluster, here we investigate the dynamical evolution of NGC 188 through a sophisticated N-body model. Importantly, we employ the observed binary properties of the young (180 Myr) open cluster M35, where possible, to guide our choices for parameters of the initial binary population. We apply pre-main-sequence tidal circularization and a substantial increase to the main-sequence tidal circularization rate, both of which are necessary to match the observed tidal circularization periods in the literature, including that of NGC 188. At 7 Gyr the main-sequence solar-type hard-binary population in the model matches that of NGC 188 in both binary frequency and distributions of orbital parameters. This agreement between the model and observations is in a large part due to the similarities between the NGC 188 and M35 solar-type binaries. Indeed, among the 7 Gyr main-sequence binaries in the model, only those with P {approx}> 1000 days begin to show potentially observable evidence for modifications by dynamical encounters, even after 7 Gyr of evolution within the star cluster. This emphasizes the importance of defining accurate initial conditions for star cluster models, which we propose is best accomplished through comparisons with observations of young open clusters like M35. Furthermore, this finding suggests that observations of the present-day binaries in even old open clusters can provide valuable information on their primordial binary populations. However, despite the model's success at matching the observed solar-type main-sequence population, the model underproduces blue stragglers and produces an overabundance of long-period circular main-sequence-white-dwarf binaries as compared with the true cluster. We explore several potential solutions to the paucity of blue stragglers and conclude that the model dramatically underproduces blue stragglers through mass-transfer processes. We suggest that common-envelope evolution may have been incorrectly imposed on the progenitors of the spurious long-period circular main-sequence-white-dwarf binaries, which perhaps instead should have gone through stable mass transfer to create blue stragglers, thereby bringing both the number and binary frequency of the blue straggler population in the model into agreement with the true blue stragglers in NGC 188. Thus, improvements in the physics of mass transfer and common-envelope evolution employed in the model may in fact solve both discrepancies with the observations. This project highlights the unique accessibility of open clusters to both comprehensive observational surveys and full-scale N-body simulations, both of which have only recently matured sufficiently to enable such a project, and underscores the importance of open clusters to the study of star cluster dynamics.

Geller, Aaron M. [Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 (United States); Hurley, Jarrod R. [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122 (Australia); Mathieu, Robert D., E-mail: a-geller@northwestern.edu, E-mail: mathieu@astro.wisc.edu, E-mail: jhurley@astro.swin.edu.au [Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53706 (United States)

2013-01-01T23:59:59.000Z

12

BONA FIDE, STRONG-VARIABLE GALACTIC LUMINOUS BLUE VARIABLE STARS ARE FAST ROTATORS: DETECTION OF A HIGH ROTATIONAL VELOCITY IN HR CARINAE  

Science Conference Proceedings (OSTI)

We report optical observations of the luminous blue variable (LBV) HR Carinae which show that the star has reached a visual minimum phase in 2009. More importantly, we detected absorptions due to Si IV lambdalambda4088-4116. To match their observed line profiles from 2009 May, a high rotational velocity of v{sub rot} approx = 150 +- 20 km s{sup -1} is needed (assuming an inclination angle of 30 deg.), implying that HR Car rotates at approx =0.88 +- 0.2 of its critical velocity for breakup (v{sub crit}). Our results suggest that fast rotation is typical in all strong-variable, bona fide galactic LBVs, which present S-Dor-type variability. Strong-variable LBVs are located in a well-defined region of the HR diagram during visual minimum (the 'LBV minimum instability strip'). We suggest this region corresponds to where v{sub crit} is reached. To the left of this strip, a forbidden zone with v{sub rot}/v{sub crit}>1 is present, explaining why no LBVs are detected in this zone. Since dormant/ex LBVs like P Cygni and HD 168625 have low v{sub rot}, we propose that LBVs can be separated into two groups: fast-rotating, strong-variable stars showing S-Dor cycles (such as AG Car and HR Car) and slow-rotating stars with much less variability (such as P Cygni and HD 168625). We speculate that supernova (SN) progenitors which had S-Dor cycles before exploding (such as in SN 2001ig, SN 2003bg, and SN 2005gj) could have been fast rotators. We suggest that the potential difficulty of fast-rotating Galactic LBVs to lose angular momentum is additional evidence that such stars could explode during the LBV phase.

Groh, J. H. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); Damineli, A.; Moises, A. P.; Teodoro, M. [Instituto de Astronomia, Geofisica e Ciencias Atmosfericas, Universidade de Sao Paulo, Rua do Matao 1226, Cidade Universitaria, 05508-090, Sao Paulo, SP (Brazil); Hillier, D. J. [Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States); Barba, R. [Departamento de fisica, Universidad de La Serena, Benavente 980, La Serena (Chile); Fernandez-Lajus, E.; Gamen, R. C.; Solivella, G., E-mail: jgroh@mpifr-bonn.mpg.d [Facultad de Ciencias Astronomicas y Geofisicas, Universidad Nacional de La Plata, and Instituto de Astrofisica de La Plata (CCT La Plata-CONICET), Paseo del Bosque S/N, B1900FWA, La Plata (Argentina)

2009-11-01T23:59:59.000Z

13

ENERGY STAR Certified New Homes : ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

little label with a big message. Better is better. The blue ENERGY STAR label on a new home means: Peace of Mind Enduring Quality Wall-to-Wall Comfort Proven Value ENERGY STAR...

14

ON THE NATURE OF THE PROTOTYPE LUMINOUS BLUE VARIABLE AG CARINAE. II. WITNESSING A MASSIVE STAR EVOLVING CLOSE TO THE EDDINGTON AND BISTABILITY LIMITS  

Science Conference Proceedings (OSTI)

We show that the significantly different effective temperatures (T{sub eff}) achieved by the luminous blue variable AG Carinae during the consecutive visual minima of 1985-1990 (T{sub eff} {approx_equal} 22,800 K) and 2000-2001 (T{sub eff} {approx_equal} 17,000 K) place the star on different sides of the bistability limit, which occurs in line-driven stellar winds around T{sub eff} {approx} 21,000 K. Decisive evidence is provided by huge changes in the optical depth of the Lyman continuum in the inner wind as T{sub eff} changes during the S Dor cycle. These changes cause different Fe ionization structures in the inner wind. The bistability mechanism is also related to the different wind parameters during visual minima: the wind terminal velocity was 2-3 times higher and the mass-loss rate roughly two times smaller in 1985-1990 than in 2000-2003. We obtain a projected rotational velocity of 220 {+-} 50 km s{sup -1} during 1985-1990 which, combined with the high luminosity (L{sub *} = 1.5 x 10{sup 6} L{sub sun}), puts AG Car extremely close to the Eddington limit modified by rotation ({Omega}{Gamma} limit): for an inclination angle of 90{sup 0}, {Gamma}{sub {Omega}} {approx}> 1.0 for M{sub sun} {approx}Car. Therefore, AG Car is close to, if not at, the {Omega}{Gamma} limit during visual minimum. Assuming M = 70 M{sub sun}, we find that {Gamma}{sub {Omega}} decreases from 0.93 to 0.72 as AG Car expands toward visual maximum, suggesting that the star is not above the Eddington limit during maximum phases.

Groh, J. H. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); Hillier, D. J. [Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States); Damineli, A., E-mail: jgroh@mpifr.de [Instituto de Astronomia, Geofisica e Ciencias Atmosfericas, Universidade de Sao Paulo, Rua do Matao 1226, Cidade Universitaria, 05508-900, Sao Paulo, SP (Brazil)

2011-07-20T23:59:59.000Z

15

Behind Blue Eyes: A Memoir of Childhood Who Am I?: A Collection of Essays.  

E-Print Network (OSTI)

??How should one approach childhood memories for the writing of literary memoir? Behind Blue Eyes is my childhood revisited. I have fashioned my earliest memories (more)

Parry, Glyn

2006-01-01T23:59:59.000Z

16

Automated Nonlinear Stellar Pulsation Calculations: Applications to RR Lyrae stars. The Slope of the Fundamental Blue Edge and the First RRd Model Survey  

E-Print Network (OSTI)

We describe a methodology that allows us to follow the pulsational behavior of an RR Lyrae model consistently and automatically along its evolutionary track throughout the whole instability strip. It is based on the powerful amplitude equation formalism, and resorts to a judicious combination of numerical hydrodynamical simulations, the analytical signal time-series analysis, and amplitude equations. A large-scale survey of the nonlinear pulsations in RR Lyr instability strip is then presented, and the mode selection mechanism is delineated throughout the relevant regions of parameter space. We obtain and examine two regions with hysteresis, where the pulsational state depends on the direction of the evolutionary tracks, namely a region with either fundamental (RRab) or first overtone (RRc) pulsations and a region with either fundamental (RRab) or double-mode (RRd) pulsations. The regions where stable double-mode (DM, or RRd) pulsations occur are very narrow and hard to find in astrophysical parameter (L, M, T_eff, X, Z) space with hydrodynamic simulations, but our systematic and efficient methodology allows us to investigate them with unprecedented detail. It is shown that by simultaneously considering the effects of mode selection and of horizontal branch evolution we can naturally solve one of the extant puzzles involving the topologies of the theoretical and observed instability strips, namely the slope of the fundamental blue edge. The importance of the interplay between mode selection and stellar evolutionary effects is also demonstrated for the properties of double-mode RR Lyr. Finally, the Petersen diagram of double-mode RR Lyr models is discussed for the first time.

R. Szabo; Z. Kollath; J. R. Buchler

2004-06-16T23:59:59.000Z

17

Parallel volume rendering on the IBM Blue Gene/P  

Science Conference Proceedings (OSTI)

Parallel volume rendering is implemented and tested on an IBM Blue Gene distributed-memory parallel architecture. The goal of studying the cost of parallel rendering on a new class of supercomputers such as the Blue Gene/P is not necessarily to achieve ...

Tom Peterka; Hongfeng Yu; Robert Ross; Kwan-Liu Ma

2008-04-01T23:59:59.000Z

18

Detroit blues women.  

E-Print Network (OSTI)

??ABSTRACT DETROIT BLUES WOMEN by Michael Duggan Murphy August 2011 Advisor: Dr. John J. Bukowczyk Major: History Degree: Doctor of Philosophy "Detroit Blues Women" explores (more)

Murphy, Michael Duggan

2011-01-01T23:59:59.000Z

19

Blue-green algae  

NLE Websites -- All DOE Office Websites (Extended Search)

green algae Name: Renee Location: NA Country: NA Date: NA Question: How much oxygen does green-blue algae produce, and how big are they? Replies: Blue-green algae...

20

Blue-eyed Babies  

NLE Websites -- All DOE Office Websites (Extended Search)

Blue-eyed Babies Blue-eyed Babies Name: Jill Location: N/A Country: N/A Date: N/A Question: One of my students asked me the other day why all babies are born with blue eyes, even though they are truly brown-eyed, once their eyes change colour. What causes this phenomenon? Exposure to air, maybe? Replies: Hi, First of all not all babies are born with blue eyes. This is especially evident in the Asian/ Indian continents. The cause for the delay is nothing more than a delay in the enzymes that bring on the darker color proteins. You are probably aware that eye color is determined by more than one gene. The darker colors have blue coloration as part of their make-up and that may be the only protein of the color exposed at birth for many individuals. The proteins that give the darker colors usually turn on within a year of birth and this timing varies with individuals.

Note: This page contains sample records for the topic "blue star memorial" 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

Free stars  

E-Print Network (OSTI)

Free stars are certain subsets of a poset, first defined by me in [1]. Free stars are closely related with filters, namely free stars on a boolean lattice bijectively correspond to filters on this lattice. This article introduces consideration of free stars. Some questions are raised. Free stars are useful in my further (yet unpublished) research (in general topology).

Victor Porton; Shay Agnon

2012-01-01T23:59:59.000Z

22

Blue Ridge Biofuels LLC | Open Energy Information  

Open Energy Info (EERE)

Blue Ridge Biofuels LLC Jump to: navigation, search Name Blue Ridge Biofuels LLC Place Asheville, North Carolina Zip 28801 Sector Biofuels Product Blue Ridge Biofuels is a worker...

23

STAR Search STAR Search5 30  

E-Print Network (OSTI)

STAR Search "" STAR STAR Search5 30 Tokyo Tech STAR STAR Search Tech OCW T2R2 Google Web T2R2 Tokyo Tech OCW Web #12; STAR STAR Search DB DB T2R2 Tokyo Tech OCW T2R2 Tokyo Tech OCW STAR Search STAR Search T2R2 Tokyo Tech OCW STAR

24

Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain...  

Open Energy Info (EERE)

DOI: Unavailable Core Holes At Blue Mountain Area (Fairbank & Neggemann, 2004) Thermal Gradient Holes At Blue Mountain Area (Fairbank & Neggemann, 2004) Blue Mountain Geothermal...

25

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

26

ENERGY STAR Snapshot | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

27

Massachusetts Institute of Technology StarT-X: A One-Man-Year Exercise in  

E-Print Network (OSTI)

with StarT-X, a processor can send and receive a 64-byte message in less than 0.4 and 3.5 usec respectively and incur less than 5.6 usec user-to-user latency. StarT-X's remote memory-to-memory DMA mechanism can

28

BRANCHED ALKANES FROM BLUE-GREEN ALGAE  

E-Print Network (OSTI)

ALKANES FROM BLUE-GREEN ALGAE RECEIV r - LAWREW RADIATIONAlkanes From Blue-Green Algae by Jerry Han and Oep~rtment l~alkanes from blue-green algae were separated on a The

Han, Jerry; Calvin, Melvin.

2008-01-01T23:59:59.000Z

29

Kurucz model energy distributions: a comparison with real stars. II. Metal-deficient stars  

E-Print Network (OSTI)

Energy distributions of synthetic spectra for Kurucz model atmospheres are compared with observed energy distributions of metal-deficient stars of the blue horizontal-branch (BHB), F-G-K subdwarf (SD) and G-K giant (MDG) types. The best coincidence of the synthetic and observed energy curves is found for BHB stars. The largest differences are found in the ultraviolet wavelengths for subdwarfs and cool MDGs. The influence of errors of effective temperatures, gravities and metallicities is estimated.

V. Straizys; R. Lazauskaite; G. Valiauga

2002-12-04T23:59:59.000Z

30

ENERGY STAR in action | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Benchmark energy use ENERGY STAR in action Programs and policies using ENERGY STAR Green buildings and ENERGY STAR Communicate and educate Find out who's partnered with...

31

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

and Other and Other Climate Protection Partnerships 2011 Annual Report CONTENTS Letter from the Administrator ............................................................................................................................................................................. 1 Executive Summary .............................................................................................................................................................................................. 2 Highlights of 2011 ......................................................................................................................................................................................... 4 ENERGY STAR Overview ......................................................................................................................................................................................

32

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

the measurement and tracking of electricity, gas, and water data, through the use of the ENERGY STAR Portfolio Manager tool. Goals included completion rates for critical and...

33

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

such as: Choosing ENERGY STAR certified appliances and electronics. Maintaining home heating and cooling systems to improve efficiency. Ensuring homes are well sealed...

34

NIST Stars  

Science Conference Proceedings (OSTI)

... Weather and climate research satellites could use SI Stars for on orbit calibration of their spectroradiometers and astronomers ... Facilities/Tools Used ...

2012-11-16T23:59:59.000Z

35

MPI-StarT: Delivering Network Performance to Numerical Applications  

E-Print Network (OSTI)

T-X, a processor can send and receive a 64-byte message in less than 0.4 and 3.5 usec respectively and incur less than 5.6 usec user-to-user one-way latency. StarT-X's remote memory-to-memory DMA mechanism can

36

Blue Ng | Open Energy Information  

Open Energy Info (EERE)

Ng Jump to: navigation, search Name Blue-Ng Place Bath, United Kingdom Zip BA1 1SR Sector Biomass Product UK-based company that constructs and operates combined heat and...

37

Active memory operations  

Science Conference Proceedings (OSTI)

The performance of modern microprocessors is increasingly limited by their inability to hide main memory latency. The problem is worse in large-scale shared memory systems, where remote memory latencies are hundreds, and soon thousands, of processor ... Keywords: DRAM, cache coherence, distributed shared memory, memory performance, stream processing, thread synchronization

Zhen Fang; Lixin Zhang; John B. Carter; Ali Ibrahim; Michael A. Parker

2007-06-01T23:59:59.000Z

38

Shape Memory Alloys  

Science Conference Proceedings (OSTI)

Scope, Shape memory alloys (SMA) have received widespread attention from ... The symposium focuses on shape memory and superelastic materials and their...

39

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

STAR certified buildings > photo of a room in the W Hotel, San Francisco, CA W HOTEL, San Francisco, Calif. In 2007, hotel employees submitted a petition asking management to...

40

Memory Considerations for Carver  

NLE Websites -- All DOE Office Websites (Extended Search)

Memory Considerations Memory Considerations Memory Considerations Overview Carver login nodes each have 48GB of physical memory. Most compute nodes have 24GB; however, 80 compute nodes have 48GB. Not all of this memory is available to user processes. Some memory is reserved for the Linux kernel. Furthermore, since Carver nodes have no disk, the "root" file system (including /tmp) is kept in memory ("ramdisk"). The kernel and root file system combined occupy about 4GB of memory. Therefore users should try to use no more than 20GB on most compute nodes, or 44GB on the large-memory compute nodes. There are also two "extra-large" memory nodes; each node has four 8-core Intel X7550 ("Nehalem EX") 2.0 GHz processors (32 cores total) and 1TB memory. These nodes are available through the queue "reg_xlmem". Please

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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

Blue-green upconversion laser  

DOE Patents (OSTI)

A blue-green laser (450--550 nm) uses a host crystal doped with Tm[sup 3+]. The Tm[sup 3+] is excited through upconversion by a red pumping laser and an IR pumping laser to a state which transitions to a relatively lower energy level through emissions in the blue-green band, e.g., 450.20 nm at 75 K. The exciting laser may be tunable dye lasers or may be solid-state semiconductor laser, e.g., GaAlAs and InGaAlP. 3 figs.

Nguyen, D.C.; Faulkner, G.E.

1990-08-14T23:59:59.000Z

42

Blue-green upconversion laser  

DOE Patents (OSTI)

A blue-green laser (450-550 nm) uses a host crystal doped with Tm{sup 3+}. The Tm{sup 3+} is excited through upconversion by a red pumping laser and an IR pumping laser to a state which transitions to a relatively lower energy level through emissions in the blue-green band, e.g., 450.20 nm at 75 K. The exciting laser may be tunable dye lasers or may be solid-state semiconducting laser, e.g., GaAlAs and InGaAlP.

Nguyen, Dinh C.; Faulkner, G.E.

1989-08-25T23:59:59.000Z

43

Blue-green upconversion laser  

DOE Patents (OSTI)

A blue-green laser (450-550 nm) uses a host crystal doped with Tm.sup.3+. The Tm.sup.+ is excited through upconversion by a red pumping laser and an IR pumping laser to a state which transitions to a relatively lower energy level through emissions in the blue-green band, e.g., 450.20 nm at 75 K. The exciting laser may be tunable dye lasers or may be solid-state semiconductor laser, e.g., GaAlAs and InGaAlP.

Nguyen, Dinh C. (Los Alamos, NM); Faulkner, George E. (Los Alamos, NM)

1990-01-01T23:59:59.000Z

44

Blue light emitting thiogallate phosphor  

DOE Patents (OSTI)

A crystalline blue emitting thiogallate phosphor of the formula RGa.sub.2 S.sub.4 :Ce.sub.x where R is selected from the group consisting of calcium, strontium, barium and zinc, and x is from about 1 to 10 atomic percent, the phosphor characterized as having a crystalline microstructure on the size order of from about 100 .ANG. to about 10,000 .ANG. is provided together with a process of preparing a crystalline blue emitting thiogallate phosphor by depositing on a substrate by CVD and resultant thin film electroluminescent devices including a layer of such deposited phosphor on an ordinary glass substrate.

Dye, Robert C. (Los Alamos, NM); Smith, David C. (Los Alamos, NM); King, Christopher N. (Portland, OR); Tuenge, Richard T. (Hillsboro, OR)

1998-01-01T23:59:59.000Z

45

Optical memory  

DOE Patents (OSTI)

Optical memory comprising: a semiconductor wire, a first electrode, a second electrode, a light source, a means for producing a first voltage at the first electrode, a means for producing a second voltage at the second electrode, and a means for determining the presence of an electrical voltage across the first electrode and the second electrode exceeding a predefined voltage. The first voltage, preferably less than 0 volts, different from said second voltage. The semiconductor wire is optically transparent and has a bandgap less than the energy produced by the light source. The light source is optically connected to the semiconductor wire. The first electrode and the second electrode are electrically insulated from each other and said semiconductor wire.

Mao, Samuel S; Zhang, Yanfeng

2013-07-02T23:59:59.000Z

46

Earn recognition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Partner of the Year Award ENERGY STAR plant certification ENERGY STAR Challenge for Industry Success stories: Industrial energy management Market impacts: Improvements...

47

On the Evolution of Helium in Blue Compact Galaxies  

E-Print Network (OSTI)

We discuss the chemical evolution of dwarf irregular and blue compact galaxies in light of recent data, new stellar yields and chemical evolution models. We examine the abundance data for evidence of HII region self-enrichment effects, which would lead to correlations in the scatter of helium, nitrogen, and oxygen abundances around their mean trends. The observed helium abundance trends show no such correlations, though the nitrogen--oxygen trend does show strong evidence for real scatter beyond observational error. We construct simple models for the chemical evolution of these galaxies, using the most recent yields of \\he4, C, N and O in intermediate- and high-mass stars. The effects of galactic outflows, which can arise both from bulk heating and evaporation of the ISM, and from the partial escape of enriched supernova ejecta are included. In agreement with other studies, we find that supernova-enriched outflows can roughly reproduce the observed He, C, N, and O trends; however, in models that fit N versus O, the slopes $\\Delta Y/\\Delta$O and $\\Delta Y/\\Delta$N consistently fall more than $2\\sigma$ below the fit to observations. We discuss the role of the models and their uncertainties in the extrapolation of primordial helium from the data. We also explore the model dependence arising nucleosynthesis uncertainties associated with nitrogen yields in intermediate mass stars, the fate of $8-11 \\msol$ stars, and massive star winds.

Brian D. Fields; Keith A. Olive

1998-03-25T23:59:59.000Z

48

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Protection Agency program helping businesses and individuals fight global warming through superior energy efficiency. Bring Your Green to Work with ENERGY STAR ® 1 Give It a rest Use the ENERGY STAR power management settings on your computer and monitor so they go into power save mode when not in use. Also use a power strip as a central "turn off" point when you are using equipment to completely disconnect the power supply. 2 Unplug It Unplug electronics such as cell phones and laptops once they are charged. Adapters plugged into outlets use energy even if they are not charging. 3 Light Up Your Work Life Replace the light bulb in your desk lamp with an ENERGY STAR qualified bulb. It will last up to 10 times longer and use about 75 percent less energy. Turn off the lights when

49

Chameleon stars  

Science Conference Proceedings (OSTI)

We consider a gravitating spherically symmetric configuration consisting of a scalar field nonminimally coupled to ordinary matter in the form of a perfect fluid. For this system we find static, regular, asymptotically flat solutions for both relativistic and nonrelativistic cases. It is shown that the presence of the nonminimal interaction leads to substantial changes both in the radial matter distribution of the star and in the star's total mass. A simple stability test indicates that, for the choice of parameters used in the paper, the solutions are unstable.

Dzhunushaliev, Vladimir [Institute for Basic Research, Eurasian National University, Astana, 010008 (Kazakhstan); Institute of Physicotechnical Problems and Material Science of the NAS of the Kyrgyz Republic, 265 a, Chui Street, Bishkek, 720071 (Kyrgyzstan); Folomeev, Vladimir [Institute of Physicotechnical Problems and Material Science of the NAS of the Kyrgyz Republic, 265 a, Chui Street, Bishkek, 720071 (Kyrgyzstan); Singleton, Douglas [Institute for Basic Research, Eurasian National University, Astana, 010008 (Kazakhstan); Physics Department, CSU Fresno, Fresno, California 93740-8031 (United States)

2011-10-15T23:59:59.000Z

50

`blue-sky' science Spending review  

E-Print Network (OSTI)

. Cooling Towers Fiddlers Ferry #12;What are the benefits of `blue-sky' science? At a time where every penny

51

ENERGY STAR Challenge for Industry | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR plant certification ENERGY STAR Challenge for Industry See who has taken the Challenge See who has achieved the Challenge See who is promoting the Challenge ENERGY...

52

AN ECLIPSING BLUE STRAGGLER IN THE GLOBULAR CLUSTER {omega} CENTAURI  

Science Conference Proceedings (OSTI)

{omega} Centauri is the largest globular cluster in the Milky Way and hence contains the largest number of variable stars within a single cluster. The results of photometric solutions are presented for the EA-type binary V239 in this cluster. According to our analysis, V239 is a typical Algol-type binary. We obtain M = 1.20 {+-} 0.10 M{sub Sun }, R = 1.21 {+-} 0.03 R{sub Sun }, and L = 13.68 {+-} 0.63 L{sub Sun} for the primary component. The secondary component has M = 0.07 {+-} 0.02 M{sub Sun }, R = 0.90 {+-} 0.03 R{sub Sun }, and L = 2.17 {+-} 0.14 L{sub Sun }. The binary system is located in the blue straggler region on the color-magnitude diagram of {omega} Centauri and the mass of the primary component exceeds the mass of a turnoff star. Therefore, we think that V239 is a blue straggler and that V239 was formed by mass transfer from the present secondary component to the present primary.

Li Kai; Qian Shengbang, E-mail: likai@ynao.ac.cn [National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming (China)

2012-12-01T23:59:59.000Z

53

PDSF Memory Considerations  

NLE Websites -- All DOE Office Websites (Extended Search)

Memory Considerations Memory Considerations Memory Considerations Interactive Nodes The amount of memory available on the interactive nodes is described on the Interactive (login) Nodes page. The interactive nodes are shared among all users and running high memory jobs on the interactive nodes slows them down for everyone. If you think your work might be disruptive you should either run it in batch or run it interactively on a batch node as described here. Batch Nodes The batch system knows how much memory each node has and how much memory each job requires. By default each job is given 1.1GB, but you can request more or less memory by following the instructions in Submitting Jobs. However, it should be noted that the more memory you require, the harder it will be for the batch system to schedule your job, especially when the

54

Blue Summit | Open Energy Information  

Open Energy Info (EERE)

Summit Summit Jump to: navigation, search Name Blue Summit Facility Blue Summit Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner NextEra Energy Resources Developer NextEra Energy Resources Energy Purchaser Undisclosed PPA Location Vernon TX Coordinates 34.304837°, -99.376873° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.304837,"lon":-99.376873,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

55

Status of Blue Ridge Reservoir  

DOE Green Energy (OSTI)

This is one in a series of reports prepared by the Tennessee Valley Authority (TVA) for those interested in the conditions of TVA reservoirs. This overview of Blue Ridge Reservoir summarizes reservoir and watershed characteristics, reservoir uses and use impairments, water quality and aquatic biological conditions, and activities of reservoir management agencies. This information was extracted from the most current reports and data available, as well as interview with water resource professionals in various federal, state, and local agencies. Blue Ridge Reservoir is a single-purpose hydropower generating project. When consistent with this primary objective, the reservoir is also operated to benefit secondary objectives including water quality, recreation, fish and aquatic habitat, development of shoreline, aesthetic quality, and other public and private uses that support overall regional economic growth and development. 8 refs., 1 fig.

Not Available

1990-09-01T23:59:59.000Z

56

NIST Blue Ribbon Commission on Management and Safety ? ...  

Science Conference Proceedings (OSTI)

NIST Blue Ribbon Commission on Management and Safety II. The NIST Blue Ribbon Commission on Management and ...

2012-08-27T23:59:59.000Z

57

NIST Blue Ribbon Commission on Management and Safety ...  

Science Conference Proceedings (OSTI)

... See NIST Blue Ribbon Commission on Management and Safety II. NIST Blue Ribbon Commission on Management and Safety. ...

2010-10-05T23:59:59.000Z

58

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

of Air and Radiation * For more information www.energystar.gov or call 1.888.STAR.YES (1.888.782.7937) * (6202J) EPA 430-H-08-002 * December 2008 * Recycled/Recyclable - Printed with Vegetable Oil Based Inks on Recycled Paper (Minimum 50% Post-consumer Content) of Air and Radiation * For more information www.energystar.gov or call 1.888.STAR.YES (1.888.782.7937) * (6202J) EPA 430-H-08-002 * December 2008 * Recycled/Recyclable - Printed with Vegetable Oil Based Inks on Recycled Paper (Minimum 50% Post-consumer Content) Enable power management settings so they automatically enter a low-power mode when not in use. monitor/computer Use a power strip as a central "turn off" point when you are done using office equipment to completely disconnect the power supply. power strip Unplug electronics

59

Silicon nanocrystal memories  

Science Conference Proceedings (OSTI)

In this paper, we present an overview of memory structures fabricated by our group by using silicon nanocrystals as storage nodes. These devices show promising characteristics as candidates for future deep-submicron non-volatile memories.

S. Lombardo; B. De Salvo; C. Gerardi; T. Baron

2004-05-01T23:59:59.000Z

60

Drifting absence :: drafting memory  

E-Print Network (OSTI)

The emotive power of a memorial derives from its ability to engage the viewer in active remembrance. The project considers the limitations of a monumentality which embraces a distinct division between viewer and memorial. ...

Kuhn, Marlene Eva

2006-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

Samuel Rosen Memorial Award  

Science Conference Proceedings (OSTI)

Recognizing accomplishments in surfactant chemistry. The Samuel Rosen Memorial Award is sponsored by Milton J. Rosen. Samuel Rosen Memorial Award Membership Information achievement application award Awards distinguished division Divisions fats job

62

Deep Blue No. 2-A Resource in the Making at Blue Mountain | Open Energy  

Open Energy Info (EERE)

Deep Blue No. 2-A Resource in the Making at Blue Mountain Deep Blue No. 2-A Resource in the Making at Blue Mountain Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Deep Blue No. 2-A Resource in the Making at Blue Mountain Abstract This paper provides a summary of the drilling operations, flow and injection testing and downhole measurements obtained during the drilling and testing of Deep Blue No.2. This well was sited as a step out to Deep Blue No.1 which measured 145°C at a depth of 645 meters. The maximum temperature recorded in Deep Blue No.2 while drilling was 167.5°C at a depth of 585 meters. Preliminary geothermometry from the short rigon flow test conducted last April 2004 indicated a parent reservoir temperature of 240°C. The results from the November 2004 flow and injection testing

63

Tolerating memory leaks  

Science Conference Proceedings (OSTI)

Type safety and garbage collection in managed languages eliminate memory errors such as dangling pointers, double frees, and leaks of unreachable objects. Unfortunately, a program still leaks memory if it maintains references to objects it will never ... Keywords: bug tolerance, managed languages, memory leaks

Michael D. Bond; Kathryn S. McKinley

2008-10-01T23:59:59.000Z

64

External Memory Algorithms  

Science Conference Proceedings (OSTI)

Data sets in large applications are often too massive to fit completely inside the computer's internal memory. The resulting input/ output communication (or I/O) between fast internal memory and slower external memory (such as disks) can be a major performance ...

Jeffrey Scott Vitter

1998-08-01T23:59:59.000Z

65

Xenon in Mercury-Manganese Stars  

E-Print Network (OSTI)

Previous studies of elemental abundances in Mercury-Manganese (HgMn) stars have occasionally reported the presence of lines of the ionized rare noble gas Xe II, especially in a few of the hottest stars with Teff ~ 13000--15000 K. A new study of this element has been undertaken using observations from Lick Observatory's Hamilton Echelle Spectrograph. In this work, the spectrum synthesis program UCLSYN has been used to undertake abundance analysis assuming LTE. We find that in the Smith & Dworetsky sample of HgMn stars, Xe is vastly over-abundant in 21 of 22 HgMn stars studied, by factors of 3.1--4.8 dex. There does not appear to be a significant correlation of Xe abundance with Teff. A comparison sample of normal late B stars shows no sign of Xe II lines that could be detected, consistent with the expected weakness of lines at normal abundance. The main reason for the previous lack of widespread detection in HgMn stars is probably due to the strongest lines being at longer wavelengths than the photographic blue. The lines used in this work were 4603.03A, 4844.33A and 5292.22A.

M. M. Dworetsky; J. L. Persaud; K. Patel

2008-01-16T23:59:59.000Z

66

Tight LMC massive star clusters R 127 and R 128  

E-Print Network (OSTI)

We study the Large Magellanic Cloud (LMC) star clusters R 127 and R 128 using imaging and spectroscopy obtained at the ESO NTT telescope. An advanced image restoration technique allows us to resolve these two clusters into at least 14 and 33 stars respectively and obtain their photometry. In particular, we show that the core of R 127 is composed of at least four stars and identify the Luminous Blue Variable (LBV) component. The closest neighbor of the LBV (star #8) is 1".5 away. Moreover, from medium dispersion spectroscopy we determine the spectral types for 19 stars in and near both clusters, and in particular present the first spatially resolved observation of the second brightest component of the R 127 cluster (star #3) situated 3".3 from the LBV. By comparing with evolutionary models we also look into the stellar ages. The oldest stars of the cluster are ~ 6-8 Myr old, whereas the most massive star of the region (#7), formed ~ 3 Myr ago as an 80 solar mass star, has turned into an LBV, the ``R 127'' star.

M. Heydari-Malayeri; F. Meynadier; Nolan R. Walborn

2003-01-15T23:59:59.000Z

67

RHIC | STAR Detector  

NLE Websites -- All DOE Office Websites (Extended Search)

The STAR Detector The STAR detector specializes in tracking the thousands of particles produced by each ion collision at RHIC. Weighing 1,200 tons and as large as a house, STAR is...

68

Blue Green Capital | Open Energy Information  

Open Energy Info (EERE)

Capital Jump to: navigation, search Name Blue Green Capital Place Spain Zip 8860 Sector Renewable Energy, Solar Product String representation "Spanish develop ... their projects."...

69

Blue Planet Solar | Open Energy Information  

Open Energy Info (EERE)

Solar Product Belgium-based firm that offers installation, operating, developing and investment services for solar projects. References Blue Planet Solar1 LinkedIn Connections...

70

Blue C Ltd | Open Energy Information  

Open Energy Info (EERE)

Zip 98104 Sector Renewable Energy Product An advisory firm providing project and investment advice to renewable energy projects. References Blue C, Ltd.1 LinkedIn Connections...

71

Blue Sun Biodiesel | Open Energy Information  

Open Energy Info (EERE)

held Blue Sun Biodiesel is a breakthrough agriculture energy company, developing oilseed energy crops and production and distribution networks to bring high-performance biodiesel...

72

THE SIZE SCALE OF STAR CLUSTERS  

SciTech Connect

Direct N-body simulations of star clusters in a realistic Milky-Way-like potential are carried out using the code NBODY6. Based on these simulations, a new relationship between scale size and galactocentric distance is derived: the scale size of star clusters is proportional to the hyperbolic tangent of the galactocentric distance. The half-mass radius of star clusters increases systematically with galactocentric distance but levels off when star clusters orbit the galaxy beyond {approx}40 kpc. These simulations show that the half-mass radius of individual star clusters varies significantly as they evolve over a Hubble time, more so for clusters with shorter relaxation times, and remains constant through several relaxation times only in certain situations when expansion driven by the internal dynamics of the star cluster and the influence of the host galaxy tidal field balance each other. Indeed, the radius of a star cluster evolving within the inner 20 kpc of a realistic galactic gravitational potential is severely truncated by tidal interactions and does not remain constant over a Hubble time. Furthermore, the half-mass radius of star clusters measured with present-day observations bears no memory of the original cluster size. Stellar evolution and tidal stripping are the two competing physical mechanisms that determine the present-day size of globular clusters. These simulations also show that extended star clusters can form at large galactocentric distances while remaining fully bound to the host galaxy. There is thus no need to invoke accretion from an external galaxy to explain the presence of extended clusters at large galactocentric distances in a Milky-Way-type galaxy.

Madrid, Juan P.; Hurley, Jarrod R.; Sippel, Anna C. [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122 (Australia)

2012-09-10T23:59:59.000Z

73

Home : ENERGY STAR  

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STAR logo Skip directly to page content Energy Efficient Products Energy Efficient Products ENERGY STAR products are independently certified to save energy without sacrificing...

74

ENERGY STAR Challenge  

NLE Websites -- All DOE Office Websites (Extended Search)

STAR Challenge for Industry Participant Handbook June 2013 ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change...

75

Participation Form | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

application. Select the ENERGY STAR program you intend to participate in, and choose your primary contacts. Return this form to ENERGY STAR for consideration as a partner....

76

ENERGY STAR plant certification | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

77

ENERGY STAR industrial partnership | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

78

ENERGY STAR communications toolkit | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

79

ENERGY STAR Congregations Handout | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

handout to learn a summary of ENERGY STAR offerings for congregations, quick tips for saving energy in religious worship facilities, and how to sign up for the ENERGY STAR...

80

The value of ENERGY STAR | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

Note: This page contains sample records for the topic "blue star memorial" 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

ENERGY STAR Challenge for Industry | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

82

ENERGY STAR for existing buildings | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

83

Blue LED for RS Monitor  

E-Print Network (OSTI)

Abstract We report on a design of RS gain monitor system based on blue LED. Gain of each RS PMT is monitored by a LED, which is mounted in front of the PMT window in its _-metal shield. The blue LED well simulates scintillation light with its short pulse and wavelength. The LED is as small as 3 mmOE. The light yield is stable and has small temperature dependence. These are nice properties to install in present RS system with small modification and to operate without air conditioning. In this note we will present outline of our design and test results which demonstrate its desirable properties. 1 Introduction RS gain monitor has been carried out with K_2 events at E787. They are sat- isfactory to monitor long and medium term stability but it is not satisfactory to monitor short term stability and to check PMT and related electronics quickly and frequently. These capabilities are important to reduce setup time and loss time in long E949 run. For these purpose triggerable and stable light source is required at RS system. We consider two types of monitoring system. One is the system which consists of one light source and its light distribution network, such as a Xe lamp with a optical fiber network. It has the advantage that light intensity of the source itself can be monitored and be corrected. But, practically, it is not easy to estimate light output of individual fiber correctly by checking light source and to handle optical fibers, and we have to think out a solution how we introduce lights to RS or its PMT. Also the system is rather expensive and it will take long time to

unknown authors

2000-01-01T23:59:59.000Z

84

EarlyExperienceOnBlueGeneQ.pptx  

NLE Websites -- All DOE Office Websites (Extended Search)

and Performance Engineering Team Early Experience on the Blue Gene/Q Supercomputing System Mira P erformance B oot C amp Argonne, M ay 2 1, 2 013 Argonne L eadership C ompuDng F acility Argonne N aDonal L aboratory, A rgonne, I L 2 Outline  Introduc+on - Argonne L eadership C ompu+ng F acility - From B G/P t o B G/Q  BG/Q S ystem C haracteris+cs - Memory S ubsystem - Computa+on C apabili+es - Interconnect a nd C ommunica+on P roper+es - Power C onsump+on a nd E fficiency  BG/Q S pecific F eatures - QPX --- 4 ---way S IMD V ector U nit - Prefetching U nit a nd L ist P refetching  Applica+on S tudies - GTC, G FMC, D NS3D ALCF @ Argonne 3 Produc'on S ystems: Mira - B G/Q s ystem - 49,152 nodes / 786,432 cores - 786 TB of memory - Peak fl op r ate: 1 0 P F - Linpack fl op r ate: 8 .1 P F Intrepid

85

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

New Energy Technology 2754 Compass Drive, Grand Junction, CO 81506 Business: Energy Management Services/Consulting Sarah Faverman Phone: 970-243-0255 / Fax: 970-245-4268 Email: sarah@newenergytech.net Customer JCPenney Company, Inc. 6501 Legacy Drive, Plano, TX 75024 Business: Retail Rob Keller, P.E., Energy Management & Engineering Services Director Phone: 972-431-1788 / Fax: 972-531-1788 Email: rkeller@jcpenney.com New Energy Technology helped JCPenney earn the first ENERGY STAR labels for retail buildings and Partner of the Year Award. Project Scope New Energy Technology (NET) supports JCPenney's (JCP) energy conservation culture through three programs focused on high-quality energy data and energy management. Through its automated benchmarking

86

ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Green Team Checklist Green Team Checklist One person cannot do it all! So when it comes to making your workplace greener and more energy efficient, nothing beats a team. The Environmental Protection Agency (EPA) has learned from ENERGY STAR partners that forming a green team with coworkers is a great way to help increase energy efficiency and reduce office waste. Consider the following checklist of creative ideas from EPA to help your green team get started. Once you've formed your team, start by planting the seeds for success with small changes in individual workspaces. Then move through the list and help success bloom with bigger changes that can affect the whole organization. Together, these actions can help your green team build a better world! Start Off Right-Meet with management to get approval and buy-in for the idea of forming a green team. Not only does support

87

Multi-class blue noise sampling  

Science Conference Proceedings (OSTI)

Sampling is a core process for a variety of graphics applications. Among existing sampling methods, blue noise sampling remains popular thanks to its spatial uniformity and absence of aliasing artifacts. However, research so far has been mainly focused ... Keywords: blue noise, dart throwing, multi-class, poisson hard/soft disk, relaxation, sampling

Li-Yi Wei

2010-07-01T23:59:59.000Z

88

Scalable Time Warp on Blue Gene Supercomputers  

Science Conference Proceedings (OSTI)

n this paper we illustrate scalable parallel performance for the TimeWarp synchronization protocol on the L and P variants of the IBM BlueGene supercomputer. Scalable Time Warp performance for models that communicate a large percentage of the event population ... Keywords: Time Warp, Blue Gene Supercomputer

David W. Bauer Jr.; Christopher D. Carothers; Akintayo Holder

2009-06-01T23:59:59.000Z

89

Evolution of massive stars losing mass and angular momentum supergiants  

SciTech Connect

Evolutionary sequences have been computed to central helium exhaustion for massive Population I star models with initial masses of 40, 60, 80, and 100 M/sub sun/. Mass loss occurs through radiatively driven winds and through the effects of nonthermal winds generated both by rotational shear turbulence during the mainsequence (MS) phase and by the acoustic energy flux from the convective envelope during the red supergiant phase. The size of the convective envelope in the red supergiant phase is found to depend on the mass loss history of the star, through the effect of mass loss on the position of the hydrogen shell source (HSS) and on the opacity of the envelope above the HSS. Previous evolutionary calculations have shown that, for low mass loss rates, a blue loop forms when the HSS contacts the discontinuity at the base of the convective envelope. In contrast, the higher mass loss rates considered here produce a blue loop only if sufficient mass loss occurs during the red supergiant phase to eliminate the convective envelope entirely. On the other hand, sufficiently high mass loss rates during the MS phase can remove most of the hydrogen-rich envelope, and then the red supergiant phase does not occur. In these models the mass loss and evolutionary patterns for a star depend on its initial rotational speed, which in actual stars is expected to vary from star to star. The observed blue-to-red supergiant ratios are then interpreted as weighted means of different evolutionary patterns resulting from a spread of initial rotational speeds. The same interpretation may extend to Wolf-Rayet stars.

Sreenivasan, S.R.; Wilson, W.J.F.

1985-03-15T23:59:59.000Z

90

Blue Flint Ethanol | Open Energy Information  

Open Energy Info (EERE)

Flint Ethanol Flint Ethanol Jump to: navigation, search Name Blue Flint Ethanol Place Underwood, North Dakota Zip ND 58576 Product Joint Venture bentween Great River Energy and Headwaters Incorporated, was established to build and operate a 50 million gallon per year dry mill ethanol plant in Underwood, North Dakota. References Blue Flint Ethanol[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Blue Flint Ethanol is a company located in Underwood, North Dakota . References ↑ "Blue Flint Ethanol" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Flint_Ethanol&oldid=342914" Categories: Clean Energy Organizations Companies Organizations Stubs What links here

91

Blue Marble Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

Energy Corporation Energy Corporation Jump to: navigation, search Name Blue Marble Energy Corporation Place Seattle, Washington Zip 98108 Sector Bioenergy Product Washington State-based firm developing technology to convert biowaste into bioenergy and biochemicals. References Blue Marble Energy Corporation[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Blue Marble Energy Corporation is a company located in Seattle, Washington . References ↑ "Blue Marble Energy Corporation" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Marble_Energy_Corporation&oldid=380764" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes

92

Big Blue Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Big Blue Wind Farm Big Blue Wind Farm Jump to: navigation, search Name Big Blue Wind Farm Facility Big Blue Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Exergy Developer Exergy Energy Purchaser Xcel Energy Location Blue Earth MN Coordinates 43.64324946°, -94.22179699° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.64324946,"lon":-94.22179699,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

93

Exposing Memory Access Regularities Using Object-Relative Memory Profiling  

Science Conference Proceedings (OSTI)

Memory profiling is the process of characterizing a program's memorybehavior by observing and recording its response to specific inputsets. Relevant aspects of the program's memory behavior maythen be used to guide memory optimizations in an aggressively ...

Qiang Wu; Artem Pyatakov; Alexey Spiridonov; Easwaran Raman; Douglas W. Clark; David I. August

2004-03-01T23:59:59.000Z

94

Using Cyclic Memory Allocation to Eliminate Memory Leaks  

E-Print Network (OSTI)

We present and evaluate a new memory management technique for eliminating memory leaks in programs with dynamic memory allocation. This technique observes the execution of the program on a sequence of training inputs to ...

Nguyen, Huu Hai

95

2014 ENERGY STAR Awards : ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Partner Resources Partner Resources Manufacturers Retailers New Home Industry Utilities/EEPS Residential & Commercial Products Programs Service & Product Providers Buildings & Plants Small Businesses Congregations For Contractors For Federal Agencies Join ENERGY STAR Home > Partner Resources > ENERGY STAR Awards 2014 ENERGY STAR Awards The application submission period for the 2014 ENERGY STAR Awards has closed. Each year, the ENERGY STAR program honors organizations that have made outstanding contributions to protecting the environment through energy efficiency. Please save the date for our awards ceremony on April 29, 2014. Ceremony registration information will be available on this website in January 2014. If you have any questions, please contact Rebecca Hudson, at

96

Deep Blue No 2- A Resource In The Making At Blue Mountain | Open Energy  

Open Energy Info (EERE)

2- A Resource In The Making At Blue Mountain 2- A Resource In The Making At Blue Mountain Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Deep Blue No 2- A Resource In The Making At Blue Mountain Details Activities (1) Areas (1) Regions (0) Abstract: This paper provides a summary of the drilling operations, flow and injection testing and downhole measurements obtained during the drilling and testing of Deep Blue No.2. This well was sited as a step out to Deep Blue No.1 which measured 145°C at a depth of 645 meters. The maximum temperature recorded in Deep Blue No.2 while drilling was 167.5°C at a depth of 585 meters. Preliminary geothermometry from the short rigon flow test conducted last April 2004 indicated a parent reservoir temperature of 240°C. The results from the November 2004 flow and

97

THE NATURE OF STARBURSTS. III. THE SPATIAL DISTRIBUTION OF STAR FORMATION  

SciTech Connect

We map the spatial distribution of recent star formation over a few Multiplication-Sign 100 Myr timescales in 15 starburst dwarf galaxies using the location of young blue helium burning stars identified from optically resolved stellar populations in archival Hubble Space Telescope observations. By comparing the star formation histories from both the high surface brightness central regions and the diffuse outer regions, we measure the degree to which the star formation has been centrally concentrated during the galaxies' starbursts, using three different metrics for the spatial concentration. We find that the galaxies span a full range in spatial concentration, from highly centralized to broadly distributed star formation. Since most starbursts have historically been identified by relatively short timescale star formation tracers (e.g., H{alpha} emission), there could be a strong bias toward classifying only those galaxies with recent, centralized star formation as starbursts, while missing starbursts that are spatially distributed.

McQuinn, Kristen B. W.; Skillman, Evan D. [Minnesota Institute for Astrophysics, School of Physics and Astronomy, 116 Church Street, S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Dalcanton, Julianne J.; Weisz, Daniel R.; Williams, Benjamin F. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Cannon, John M. [Department of Physics and Astronomy, Macalester College, 1600 Grand Avenue, Saint Paul, MN 55105 (United States); Dolphin, Andrew E. [Raytheon Company, 1151 E. Hermans Road, Tucson, AZ 85756 (United States); Holtzman, Jon, E-mail: kmcquinn@astro.umn.edu [Department of Astronomy, New Mexico State University, Box 30001-Department 4500, 1320 Frenger Street, Las Cruces, NM 88003 (United States)

2012-11-01T23:59:59.000Z

98

Science at LLNL with IBM Blue Gene/Q  

Science Conference Proceedings (OSTI)

Lawrence Livermore National Laboratory (LLNL) has a long history of working with IBM on Blue Gene supercomputers. Beginning in November 2001 with the joint announcement of a partnership to expand the Blue Gene research project (including Blue Gene/L ...

B. Carnes, B. Chan, E. W. Draeger, J.-L. Fattebert, L. Fried, J. Glosli, W. D. Krauss, S. H. Langer, R. McCallen, A. A. Mirin, F. Najjar, A. L. Nichols, T. Oppelstrup, J. A. Rathkopf, D. Richards, F. Streitz, P. M. Vranas, J. J. Rice, J. A. Gunnels, V. Gurev, C. Kim, J. Magerlein, M. Reumann, H.-F. Wen

2013-01-01T23:59:59.000Z

99

BlueFire Ethanol, Inc. | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

BlueFire Ethanol, Inc. BlueFire Ethanol, Inc. A proposal issued by BlueFire Ethanol Inc,describing a project that will give DOE understanding of a new biological fermentation...

100

Memory Usage Considerations on Hopper  

NLE Websites -- All DOE Office Websites (Extended Search)

Memory Considerations Memory Considerations Memory Considerations Memory Usage Considerations on Hopper Most Hopper compute nodes have 32 GB of physical memory, but, not all that memory is available to user programs. Compute Node Linux (the kernel), the Lustre file system software, and message passing library buffers all consume memory, as does loading the executable into memory. Thus the precise memory available to an application varies. Approximately 31 GB of memory can be allocated from within an MPI program using all 24 cores per node, i.e., 1.29 GB per MPI task on average. If an application uses 12 MPI tasks per node, then each MPI task could use about 2.58 GB of memory. You may see an error message such as "OOM killer terminated this process." "OOM" means Out of Memory and it means that your code has exhausted the

Note: This page contains sample records for the topic "blue star memorial" 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

Shape memory alloys  

SciTech Connect

A shape memory alloy is disclosed consisting essentially of, by weight ratio, 2 to 15% aluminium, 0.01 to 3% beryllium and the balance being substantially copper, with impurities being inevitably present in the process of preparation, and a shape memory alloy further including 0.05 to 15% zinc, both including composition ranges which allows cold work.

Suzuki, K.

1983-10-04T23:59:59.000Z

102

The Java memory model  

Science Conference Proceedings (OSTI)

This paper describes the new Java memory model, which has been revised as part of Java 5.0. The model specifies the legal behaviors for a multithreaded program; it defines the semantics of multithreaded Java programs and partially determines legal implementations ... Keywords: Java, concurrency, memory model, multithreading

Jeremy Manson; William Pugh; Sarita V. Adve

2005-01-01T23:59:59.000Z

103

Hysteresis, Reversibility, and Shape Memory  

Science Conference Proceedings (OSTI)

Basic Properties of Shape Memory Materials from First-Principles ... Control Loops of Shape Memory Actuators by Detection of the Electrical Resistance.

104

Update on Blue Ribbon Commission for America's Nuclear Future...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Nuclear Future Update on Blue Ribbon Commission for America's Nuclear Future BRC-SEAB-October-12%202011.pdf More Documents & Publications Blue Ribbon Commission on America's...

105

Changes related to "Blue Spark Technologies formerly Thin Battery...  

Open Energy Info (EERE)

icon Twitter icon Changes related to "Blue Spark Technologies formerly Thin Battery Technologies Inc" Blue Spark Technologies formerly Thin Battery Technologies Inc...

106

Pages that link to "Blue Spark Technologies formerly Thin Battery...  

Open Energy Info (EERE)

icon Twitter icon Pages that link to "Blue Spark Technologies formerly Thin Battery Technologies Inc" Blue Spark Technologies formerly Thin Battery Technologies Inc...

107

Computer memory management system  

DOE Patents (OSTI)

A computer memory management system utilizing a memory structure system of "intelligent" pointers in which information related to the use status of the memory structure is designed into the pointer. Through this pointer system, The present invention provides essentially automatic memory management (often referred to as garbage collection) by allowing relationships between objects to have definite memory management behavior by use of coding protocol which describes when relationships should be maintained and when the relationships should be broken. In one aspect, the present invention system allows automatic breaking of strong links to facilitate object garbage collection, coupled with relationship adjectives which define deletion of associated objects. In another aspect, The present invention includes simple-to-use infinite undo/redo functionality in that it has the capability, through a simple function call, to undo all of the changes made to a data model since the previous `valid state` was noted.

Kirk, III, Whitson John (Greenwood, MO)

2002-01-01T23:59:59.000Z

108

Chemical Abundances of RR Lyrae Type C Star AS162158  

E-Print Network (OSTI)

We report the first extensive model atmosphere and detailed chemical abundance study of eight RR Lyrae variable stars of c subclass throughout their pulsation cycles. Atmospheric parameters effective temperature, surface gravity, microturbulent velocity, and metallicity have been derived. Spectra for this abundace analysis have been obtained with the echelle spectrograph of 100-inch du Pont telescope at Las Campanas Observatory. We have found metallicities and element abundance ratios to be constant within observational uncertainties at all phases of all stars. Moreover, the $\\alpha$-element and Fe-group abundance ratios with respect to iron are consistent with other horizontal-branch members (RRab, blue and red non-variables). The [Fe/H] values of these eight RRc stars have been used to anchor the metallicity scale of a much larger sample of RRc stars obtained with low S/N "snapshot" spectra.

Govea, Jose; Preston, George W; Sneden, Christopher

2013-01-01T23:59:59.000Z

109

Technology strategy for the semiconductor memory market  

E-Print Network (OSTI)

Solid state memories are used in a variety of applications as data and code storages. A non-volatile memory is a memory that retains information when its power supply is off. Flash memory is a type of nonvolatile memory ...

Nakamura, Tomohiko

2012-01-01T23:59:59.000Z

110

Building Technologies Program: ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR on Twitter Bookmark Building Technologies Program: ENERGY STAR on Google Bookmark Building Technologies Program: ENERGY STAR on Delicious Rank Building...

111

Building Technologies Office: ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR on Twitter Bookmark Building Technologies Office: ENERGY STAR on Google Bookmark Building Technologies Office: ENERGY STAR on Delicious Rank Building...

112

STAR Test Environment  

NLE Websites -- All DOE Office Websites (Extended Search)

STAR Test Environment STAR Test Environment STAR Test Environment These instructions describe how to set up the STAR environment independent of the production environment in order to test different installations in $OPTSTAR and $GROUP_DIR. If you want to modify those installations you will need access to the starofl account. Bypass STAR envionment login Edit your ~/.pdsf_setup file changing the STAR_LINUX_SETUP to "use_none" and start a new session. You should not see all the STAR environmental variables defined when you do this (and it will probably be much quicker than usual, too). Do a manual STAR login If you want to modify what test environment you use copy the test login scripts to your own working area: cp -r /common/star/startest /path/to/myworkdir/. If you don't want to modify these files you can source them directly from

113

CA-TRIBE-BLUE LAKE RANCHERIA  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

CA-TRIBE-BLUE LAKE RANCHERIA CA-TRIBE-BLUE LAKE RANCHERIA Location: Tribe CA-TRIBE-BLUE CA LAKE RANCHERIA American Recovery and Reinvestment Act: Proposed Action or Project Description The Blue Lake Rancheria Tribe of California proposes to hire a technical consultant to gather additional information and make recommendations as to the best energy efficiency and conservation project or projects to utilize energy efficiency and conservation block grant funds. Following these recommendations, a decision will be made on building retrofits, and the specific retrofits will be identified and submitted for NEPA review. Conditions: None Categorical Exclusion(s) Applied: A9, A11 *-For the complete DOE National Environmental Policy Act regulations regarding categorical exclusions, see Subpart D of 10 CFR10 21

114

The California Economy: Singing the Housing Blues  

E-Print Network (OSTI)

THECALIFORNIAECONOMY:SINGINGTHEHOUSING BLUESMany parts of the economy are doing better thantowards2007theentireeconomyisbeingthreatenedbythe

Thornberg, Christopher

2007-01-01T23:59:59.000Z

115

Become an ENERGY STAR partner | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Become an ENERGY STAR partner Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

116

Green buildings and ENERGY STAR | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Green buildings and ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

117

Earn ENERGY STAR certification | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Earn ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

118

Sample ENERGY STAR performance documents | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Verify and document your savings Sample ENERGY STAR performance documents Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers...

119

ENERGY STAR for small business | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

STAR, you can improve your small business's financial performance by reducing energy waste and energy costs, while protecting the environment. Join the network When you join...

120

ENERGY STAR Building Upgrade Manual | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Building Upgrade Manual Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

Note: This page contains sample records for the topic "blue star memorial" 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

THE STAR FORMATION MASS SEQUENCE OUT TO z = 2.5  

SciTech Connect

We study the star formation rate (SFR)-stellar mass (M{sub *}) relation in a self-consistent manner from 0 < z < 2.5 with 22,816 star-forming galaxies selected from the NEWFIRM Medium-Band Survey. We find a significant nonlinear slope of the relation, SFR{proportional_to}M {sup 0.6}{sub *}, and a constant observed scatter of 0.34 dex, independent of redshift and M{sub *}. However, if we select only blue galaxies we find a linear relation SFR{proportional_to}M{sub *}, similar to previous results at z = 0 by Peng et al. This selection excludes red, dusty, star-forming galaxies with higher masses, which brings down the slope. By selecting on L{sub IR}/L{sub UV} (a proxy for dust obscuration) and the rest-frame U - V colors, we show that star-forming galaxies fall in three distinct regions of the log(SFR)-log(M{sub *}) plane: (1) actively star-forming galaxies with 'normal' dust obscuration and associated colors (54% for log (M{sub *}) > 10 at 1 < z < 1.5), (2) red star-forming galaxies with low levels of dust obscuration and low-specific SFRs (11%), and (3) dusty, blue star-forming galaxies with high-specific SFRs (7%). The remaining 28% comprises quiescent galaxies. Galaxies on the 'normal' star formation sequence show strong trends of increasing dust attenuation with stellar mass and a decreasing specific SFR, with an observed scatter of 0.25 dex. The dusty, blue galaxies reside in the upper envelope of the star formation sequence with remarkably similar spectral shapes at all masses, suggesting that the same physical process is dominating the stellar light. The red, low-dust star-forming galaxies may be in the process of shutting off and migrating to the quiescent population.

Whitaker, Katherine E.; Van Dokkum, Pieter G. [Department of Astronomy, Yale University, New Haven, CT 06511 (United States); Brammer, Gabriel [European Southern Observatory, Alonso de Cordova 3107, Casilla 19001, Vitacura, Santiago (Chile); Franx, Marijn, E-mail: katherine.whitaker@yale.edu [Sterrewacht Leiden, Leiden University, NL-2300 RA Leiden (Netherlands)

2012-08-01T23:59:59.000Z

122

Reconsidering custom memory allocation  

Science Conference Proceedings (OSTI)

Programmers hoping to achieve performance improvements often use custom memory allocators. This in-depth study examines eight applications that use custom allocators. Surprisingly, for six of these applications, a state-of-the-art general-purpose allocator ...

Emery D. Berger; Benjamin G. Zorn; Kathryn S. McKinley

2002-11-01T23:59:59.000Z

123

Warship : memorial in antithesis  

E-Print Network (OSTI)

This thesis is divided into three distinct yet related parts. The first consists of observations and reflections on some of New York City's many war memorials, ranging from one commemorating the Revolutionary War to one ...

Tchelistcheff, Andre Victor

1992-01-01T23:59:59.000Z

124

Mondriaan memory protection  

E-Print Network (OSTI)

Reliability and security are quickly becoming users' biggest concern due to the increasing reliance on computers in all areas of society. Hardware-enforced, fine-grained memory protection can increase the reliability and ...

Witchel, Emmett Jethro, 1970-

2004-01-01T23:59:59.000Z

125

NVLAP Recognized by ENERGY STAR  

Science Conference Proceedings (OSTI)

NVLAP Recognized by ENERGY STAR. For ... criteria. Details of the program can be found on the ENERGY STAR website. ...

2012-05-08T23:59:59.000Z

126

Competitor resources | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

127

Federal agencies | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

128

ENERGY STAR Challenge  

NLE Websites -- All DOE Office Websites (Extended Search)

STAR Challenge STAR Challenge for Industry Participant Handbook June 2013 ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change through superior energy efficiency. Learn more at energystar.gov/buildings. 2 Contents Overview ............................................................................................................................. 3 Participation Eligibility .......................................................................................................... 4 How to Participate ............................................................................................................... 5 Step 1: Establish an energy intensity metric ................................................................ 5

129

Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt  

Open Energy Info (EERE)

1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt County, Nevada Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt County, Nevada Details Activities (2) Areas (1) Regions (0) Abstract: The purpose of this paper is to provide a summary of the geology, drilling operations, and down-hole measurements obtained during the drilling of Deep Blue No.1. This well was sited on the basis of proximity to numerous gold exploration holes that indicated thermal water, high temperature gradients recorded in the 12 shallow gradient holes, and low resistivity values associated with certain interpreted major faults. The well was targeted to intersect fracture zones associated with the West and

130

Deep Blue No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt  

Open Energy Info (EERE)

No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt County, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Deep Blue No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt County, Nevada Abstract The purpose of this paper is to provide a summary of the geology, drilling operations, and down-hole measurements obtained during the drilling of Deep Blue No.1. This well was sited on the basis of proximity to numerous gold exploration holes that indicated thermal water, high temperature gradients recorded in the 12 shallow gradient holes, and low resistivity values associated with certain interpreted major faults. The well was targeted to intersect fracture zones associated with the West and Central Faults, two

131

Blue Valley Energy | Open Energy Information  

Open Energy Info (EERE)

Blue Valley Energy Blue Valley Energy Name Blue Valley Energy Address 3075 75th Street Place Boulder, Colorado Zip 80301 Sector Efficiency Product Geothermal heating and cooling systems Website http://www.bluevalleyenergy.co Coordinates 40.030298°, -105.179643° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.030298,"lon":-105.179643,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

132

BlueFire Ethanol | Open Energy Information  

Open Energy Info (EERE)

BlueFire Ethanol BlueFire Ethanol Jump to: navigation, search Name BlueFire Ethanol Place Irvine, California Zip 92618 Sector Hydro Product US biofuel producer that utilises a patented concentrated acid hydrolysis technology to process various cellulosic waste materials into ethanol. Coordinates 41.837752°, -79.268594° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.837752,"lon":-79.268594,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

133

Chemical Evolution of Dwarf Spheroidal and Blue Compact Galaxies  

E-Print Network (OSTI)

We studied the chemical evolution of Dwarf Spheroidal (dSph) and Blue Compact Galaxies (BCGs) by means of comparison between the predictions of chemical evolution models and several observed abundance ratios. Detailed models with up to date nucleosynthesis taking into account the role played by supernovae of different types (II, Ia) were developed for both types of galaxies allowing us to follow the evolution of several chemical elements. The models are specified by the prescriptions of the star formation (SF) and galactic wind efficiencies chosen to reproduce the main features of these galaxies. We also investigated a possible connection in the evolution of dSph and BCGs and compared the predictions of the models to the abundance ratios observed in Damped Lyman alpha Systems (DLAs). The main conclusions are: i) the observed distribution of [alpha/Fe] vs. [Fe/H] in dSph is mainly a result of the SF rate coupled with the wind efficiency; ii) a low SF efficiency and a high wind efficiency are required to reproduce the observational data for dSph; iii) the low gas content of these galaxies is the result of the combined action of gas consumption by SF and gas removal by galactic winds; iv) the BCGs abundance ratios are reproduced by models with 2 to 7 bursts of SF with low efficiencies ; v) the low values of N/O observed in BCGs are the natural result of a bursting SF; vi) a connection between dSph and BCGs in an unified evolutionary scenario is unlikely; vii) the models for the dSph and BCGs imply different formation scenarios for the DLAs; viii) a suitable amount of primary N produced in massive stars can be perhaps an explanation for the low plateau in the [N/$\\alpha$] distribution observed in DLAs, if real.

Gustavo A. Lanfranchi; Francesca Matteucci

2003-06-23T23:59:59.000Z

134

Using Cyclic Memory Allocation to Eliminate Memory Leaks  

E-Print Network (OSTI)

We present and evaluate a new memory management technique foreliminating memory leaks in programs with dynamic memoryallocation. This technique observes the execution of the program on asequence of training inputsto find ...

Nguyen, Huu Hai

2005-10-26T23:59:59.000Z

135

ENERGY STAR Challenge for Architects | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Race to Denver 2012 Race to DC 2011 Race to New Orleans 2010 Race to Miami 2009 Race to San Francisco 2008 Race to Boston 2007 Race to San Antonio ENERGY STAR Challenge for...

136

The rope memory: a permanent storage device  

Science Conference Proceedings (OSTI)

A powerful way of increasing the capability and flexibility of digital computing systems is through the use of permanent storage memories. Such memories are also known as readonly memories or NDRO electrically unalterable memories. As an example of the ...

P. Kuttner

1963-11-01T23:59:59.000Z

137

THE FORMATION OF YOUNG DENSE STAR CLUSTERS THROUGH MERGERS  

SciTech Connect

Young star clusters such as NGC 3603 and Westerlund 1 and 2 in the Milky Way and R136 in the Large Magellanic Cloud are dynamically more evolved than expected based on their current relaxation times. In particular, the combination of a high degree of mass segregation, a relatively low central density, and the large number of massive runaway stars in their vicinity are hard to explain with the monolithic formation of these clusters. Young star clusters can achieve such a mature dynamical state if they formed through the mergers of a number of less massive clusters. The shorter relaxation times of less massive clusters cause them to dynamically evolve further by the time they merge, and the merger product preserves the memory of the dynamical evolution of its constituent clusters. With a series of N-body simulations, we study the dynamical evolution of single massive clusters and those that are assembled through merging smaller clusters together. We find that the formation of massive star clusters through the mergers of smaller clusters can reproduce the currently observed spatial distribution of massive stars, the density, and the characteristics (number and mass distribution) of the stars ejected as runaways from young dense clusters. We therefore conclude that these clusters and possibly other young massive star clusters formed through the mergers of smaller clusters.

Fujii, M. S.; Portegies Zwart, S. F. [Leiden Observatory, Leiden University, NL-2300RA Leiden (Netherlands); Saitoh, T. R. [Interactive Research Center of Science, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551 (Japan)

2012-07-01T23:59:59.000Z

138

Dynamically replicated memory: building reliable systems from nanoscale resistive memories  

Science Conference Proceedings (OSTI)

DRAM is facing severe scalability challenges in sub-45nm tech- nology nodes due to precise charge placement and sensing hur- dles in deep-submicron geometries. Resistive memories, such as phase-change memory (PCM), already scale well beyond DRAM and ... Keywords: phase-change memory, write endurance

Engin Ipek; Jeremy Condit; Edmund B. Nightingale; Doug Burger; Thomas Moscibroda

2010-03-01T23:59:59.000Z

139

Cushman & Wakefield Environmental Challenge | ENERGY STAR  

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STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR Motivate with a competition ENERGY STAR National Building...

140

High Temperature Shape Memory Alloys  

Science Conference Proceedings (OSTI)

Mar 5, 2013 ... Shape Memory Response of NiTiHfPd High Strength and High Hysteresis Shape Memory Alloys: Emre Acar1; Haluk Karaca1; Hirobumi Tobe1;...

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141

Thomas H. Smouse Memorial Fellowship  

Science Conference Proceedings (OSTI)

Awarded to a graduate student doing research in areas of interest to AOCS. Thomas H. Smouse Memorial Fellowship Thomas H. Smouse Memorial Fellowship graduate research scholastically outstanding Smouse Award Student Award Student Awards achievemen

142

Unifluxor: a permanent memory element  

Science Conference Proceedings (OSTI)

The Unifluxor is a new binary permanent memory element which appears to have the advantages of high-speed operation, easy fabrication, and low cost. Unlike cores, twistors, capacitors, and other commonly used memory devices, the Unifluxor does not depend ...

A. M. Renard; W. J. Neumann

1960-05-01T23:59:59.000Z

143

Memory Usage Considerations on Franklin  

NLE Websites -- All DOE Office Websites (Extended Search)

the memory requirement vvia internal checking in their codes or by some tools. Craypat could track heap usage. And IPM also tracks memory usage. Last edited: 2013-06-30 08:33:51...

144

BRANCHED ALKANES FROM BLUE-GREEN ALGAE  

DOE Green Energy (OSTI)

Branched alkanes from blue-green algae were separated on a 750 feet high resolution capillary gas chromatographic column. The mixture was found to be 90% of 1:1 ratio 7-methyl, and 8-methyl-heptadecane, and 10% of 6-methylheptadecane. An optical rotation of +2.5 {+-} 0.5 was obtained on a 5 mg of mixture.

Han, Jerry; Calvin, Melvin.

1970-08-01T23:59:59.000Z

145

Blue Mountain Geothermal Area | Open Energy Information  

Open Energy Info (EERE)

Blue Mountain Geothermal Area Blue Mountain Geothermal Area (Redirected from Blue Mountain Area) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermal Resource Area: Blue Mountain Geothermal Area Contents 1 Area Overview 2 History and Infrastructure 3 Regulatory and Environmental Issues 4 Exploration History 5 Well Field Description 6 Geology of the Area 7 Geofluid Geochemistry 8 NEPA-Related Analyses (2) 9 Exploration Activities (15) 10 References Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":6,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"500px","height":"300px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41,"lon":-118.13,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

146

Blue Sun Biodiesel LLC | Open Energy Information  

Open Energy Info (EERE)

Blue Sun Biodiesel LLC Blue Sun Biodiesel LLC Jump to: navigation, search Logo: Blue Sun Energy, Inc. Name Blue Sun Energy, Inc. Address 14143 Denver West Parkway Place Golden, Colorado Zip 80401 Sector Biofuels Product Biofuels marketer and distributor Year founded 2001 Number of employees 11-50 Phone number 303-865-7700 Website http://www.gobluesun.com/ Coordinates 39.7438336°, -105.1614242° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.7438336,"lon":-105.1614242,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

147

Preparing Red-Green-Blue (RGB) Images from CCD Data  

E-Print Network (OSTI)

We present a new, and we believe arguably correct, algorithm for producing Red-Green-Blue (RBG) composites from 3-band astronomical images. Our method ensures that an object with a specified astronomical color (e.g. g-r and r-i) has a unique color in the RGB image, as opposed to the burnt-out white stars to which we are accustomed. A natural consequence of this is that we can use the same colors to code color-magnitude diagrams, providing a natural `index' to our images. We also introduce the use of an asinh stretch, which allows us to show faint objects while simultaneously preserving the structure of brighter objects in the field, such as the spiral arms of large galaxies. We believe that, in addition to their aesthetic value, our images convey far more information than do the traditional ones, and provide examples from Sloan Digital Sky Survey (SDSS) imaging, the Hubble Deep Field (HDF), and Chandra to support our claims. More examples are available at http://www.astro.princeton.edu/~rhl/PrettyPictures

Robert Lupton; Michael R. Blanton; George Fekete; David W. Hogg; Wil O'Mullane; Alex Szalay; N. Wherry

2003-12-18T23:59:59.000Z

148

Shape memory polymer medical device  

SciTech Connect

A system for removing matter from a conduit. The system includes the steps of passing a transport vehicle and a shape memory polymer material through the conduit, transmitting energy to the shape memory polymer material for moving the shape memory polymer material from a first shape to a second and different shape, and withdrawing the transport vehicle and the shape memory polymer material through the conduit carrying the matter.

Maitland, Duncan (Pleasant Hill, CA); Benett, William J. (Livermore, CA); Bearinger, Jane P. (Livermore, CA); Wilson, Thomas S. (San Leandro, CA); Small, IV, Ward (Livermore, CA); Schumann, Daniel L. (Concord, CA); Jensen, Wayne A. (Livermore, CA); Ortega, Jason M. (Pacifica, CA); Marion, III, John E. (Livermore, CA); Loge, Jeffrey M. (Stockton, CA)

2010-06-29T23:59:59.000Z

149

Transparently consistent asynchronous shared memory  

Science Conference Proceedings (OSTI)

The advent of many-core processors is imposing many changes on the operating system. The resources that are under contention have changed; previously, CPU cycles were the resource in demand and required fair and precise sharing. Now compute cycles are ... Keywords: copy on write, memory management, memory sharing, virtual memory

Hakan Akkan, Latchesar Ionkov, Michael Lang

2013-06-01T23:59:59.000Z

150

Blue Cross and Blue Shield of Illinois, a Division of Health Care Service Corporation,  

E-Print Network (OSTI)

Intelligence and Counterintelligence Operations, April 2002. #12; FM 2 COUNTERINTELLIGENCE INTENT Degrade Red's Visualization of Blue TARGET · Adversary Intelligence Activities FUNCTIONSFM 2-22.3 (FM 34-52) HUMAN INTELLIGENCE COLLECTOR OPERATIONS HEADQUARTERS, DEPARTMENT OF THE ARMY

Shull, Kenneth R.

151

star-shaped polygon  

Science Conference Proceedings (OSTI)

NIST. star-shaped polygon. (definition). Definition: A polygon P in which there exists an interior point p such that all the boundary ...

2013-05-08T23:59:59.000Z

152

Energy Star Portfolio Manager  

NLE Websites -- All DOE Office Websites (Extended Search)

May 2013 What's New in Portfolio Manager ? EPA's ENERGY STAR Portfolio Manager tool helps you measure and track energy use, water use, and greenhouse gas emissions of your...

153

Energy guides | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

154

A Star on Earth  

Science Conference Proceedings (OSTI)

Jun 2, 2009 ... The world's highest-energy laser system, capable of creating temperatures and pressures that now only exist in the cores of stars, was unveiled...

155

Press room | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

improve their efficiency, and earn recognition. Learn more about the program Facts and statistics See who's partnered with ENERGY STAR Find certified buildings and plants...

156

IBM Blue Gene Parallel Supercomputer, Brookhaven National Laboratory, (BNL)  

NLE Websites -- All DOE Office Websites (Extended Search)

How to Login How to Login Please note, New York Blue/L has been decommissioned and these web pages have not yet been updated to reflect its removal from service. The New York Blue/P is now one rack and remains in service. The BNL Blue Gene/Q also remains in service. Introduction Accessing the Blue Gene SSH Gateways Accessing the Blue Gene Front-End Nodes Accessing the Visualization Cluster Accessing the CSC GPU Cluster SSH Tunneling Introduction The only way to access Blue Gene computing resources remotely (outside the Blue Gene network enclave) is through the Blue Gene ssh gateways. Even users connecting from inside the BNL campus network need to go through the gateways. Outside the BNL campus the gateways are known as: ssh.bluegene.bnl.gov Inside the BNL campus they are known as: ssh.bluegene.bnl.local

157

Account Request Form | IBM Blue Gene Parallel Supercomputer,...  

NLE Websites -- All DOE Office Websites (Extended Search)

(check all that apply) Please make at least one selection Brookhaven Blue GeneQ Argonne Leadership Computing Facility (based on Blue GeneQ) What is the name of the code? Do you...

158

BlueSol Solar Energy | Open Energy Information  

Open Energy Info (EERE)

BlueSol Solar Energy Jump to: navigation, search Name BlueSol - Solar Energy Place Sao Paulo, Sao Paulo, Brazil Zip 04551-060 Sector Solar Product Sao Paulo-based sole distributor...

159

The memory book  

Science Conference Proceedings (OSTI)

In this paper we present an Augmented Reality book for remembering past events and to plan future ones. We have developed this system using Brainstorm eStudio. We have incorporated Augmented Reality options into Brainstorm eStudio using a plugin of ARToolKit. ... Keywords: augmented reality, memory book, storytelling

M. C. Juan; B. Rey; D. Perez; D. Tomas; M. Alcaiz

2005-06-01T23:59:59.000Z

160

Library Book Memorial and  

E-Print Network (OSTI)

Library Book Memorial and Honorary Gift Program A university library provides the information or event. We will inform the individual or family of your gift and the book(s) we add to the library Enclosed is my $___________ contribution for gift books. K $20 or more -- Bookplate(s) K Under $20

VanDieren, Monica

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161

THE STAR FORMATION HISTORY OF M32  

SciTech Connect

We use deep Hubble Space Telescope Advanced Camera for Surveys/High Resolution Channel observations of a field within M32 (F1) and an M31 background field (F2) to determine the star formation history (SFH) of M32 from its resolved stellar population. We find that 2-5 Gyr old stars contribute {approx}40% {+-} 17% of M32's mass, while {approx}55% {+-} 21% of M32's mass comes from stars older than 5 Gyr. The mass-weighted mean age and metallicity of M32 at F1 are (Age) = 6.8 {+-} 1.5 Gyr and ([M/H]) = -0.01 {+-} 0.08 dex. The SFH additionally indicates the presence of young (<2 Gyr old), metal-poor ([M/H] {approx} -0.7) stars, suggesting that blue straggler stars contribute {approx}2% of the mass at F1; the remaining {approx}3% of the mass is in young metal-rich stars. Line-strength indices computed from the SFH imply a light-weighted mean age and metallicity of 4.9 Gyr and [M/H] = -0.12 dex, and single stellar population-equivalent parameters of 2.9 {+-} 0.2 Gyr and [M/H] = 0.02 {+-} 0.01 dex at F1 ({approx}2.7 r{sub e} ). This contradicts spectroscopic studies that show a steep age gradient from M32's center to 1 r{sub e} . The inferred SFH of the M31 background field F2 reveals that the majority of its stars are old, with {approx}95% of its mass already acquired 5-14 Gyr ago. It is composed of two dominant populations; {approx}30% {+-} 7.5% of its mass is in a 5-8 Gyr old population, and {approx}65% {+-} 9% of the mass is in an 8-14 Gyr old population. The mass-weighted mean age and metallicity of F2 are (Age) = 9.2 {+-} 1.2 Gyr and ([M/H]) = -0.10 {+-} 0.10 dex, respectively. Our results suggest that the inner disk and spheroid populations of M31 are indistinguishable from those of the outer disk and spheroid. Assuming the mean age of M31's disk at F2 ({approx}1 disk scale length) to be {approx}5-9 Gyr, our results agree with an inside-out disk formation scenario for M31's disk.

Monachesi, Antonela; Trager, Scott C. [Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen (Netherlands); Lauer, Tod R.; Mighell, Kenneth J. [National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726 (United States); Hidalgo, Sebastian L. [Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38200 La Laguna, Tenerife (Spain); Freedman, Wendy; Dressler, Alan [The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Grillmair, Carl, E-mail: antonela@umich.edu [Spitzer Science Center, 1200 East California Boulevard, Pasadena, CA 91125 (United States)

2012-01-20T23:59:59.000Z

162

Thermal Gradient Holes At Blue Mountain Area (Fairbank & Neggemann...  

Open Energy Info (EERE)

Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Thermal Gradient Holes At Blue Mountain Area (Fairbank & Neggemann, 2004) Exploration...

163

Ground Gravity Survey At Blue Mountain Area (Fairbank Engineering...  

Open Energy Info (EERE)

to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Ground Gravity Survey At Blue Mountain Area (Fairbank Engineering, 2006) Exploration Activity...

164

Video - Microbial Bebop - Blues for Elle | Argonne National Laboratory  

NLE Websites -- All DOE Office Websites (Extended Search)

Blues for Elle Share Topic Environment Biology Computational biology Environmental biology Metagenomics Molecular biology Environmental science & technology Ecology This musical...

165

Ten reasons to pursue ENERGY STAR certification | ENERGY STAR...  

NLE Websites -- All DOE Office Websites (Extended Search)

substantial. For example, ENERGY STAR certified office buildings cost 0.50 less per square foot to operate than their peers. Currently, ENERGY STAR certified buildings are...

166

ENERGY STAR Homes in the News : ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR products are...

167

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR communications toolkit Motivate with a competition EPA's ENERGY STAR National Building Competition Secondary menu About us Press room Contact Us Portfolio...

168

ENERGY STAR Partner of the Year Award | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Partner of the Year profiles in leadership ENERGY STAR plant certification ENERGY STAR Challenge for Industry Success stories: Industrial energy management Market impacts:...

169

Join ENERGY STAR as a partner | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and...

170

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

How can we help you? Communicate and educate ENERGY STAR communications toolkit Motivate with a competition EPA's ENERGY STAR National Building Competition...

171

The value of ENERGY STAR certification | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

building as ENERGY STAR. Below is a summary of several studies that evaluated the added market value of ENERGY STAR certified buildings. Chart showing price advantages of ENERGY...

172

ENERGY STAR certification | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR certification ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Facts and stats Climate change and buildings ENERGY STAR certification

173

STAR METRICS | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

STAR METRICS STAR METRICS May 4, 2011 - 4:47pm Addthis Energy continues to define Phase II of the STAR METRICS program, a collaborative initiative to track Research and Development...

174

ENERGY STAR Score for Offices  

NLE Websites -- All DOE Office Websites (Extended Search)

July 2013 ENERGY STAR Score for Offices in the United States Page 1 ENERGY STAR Score for Offices in the United States Technical Reference OVERVIEW The ENERGY STAR Score for...

175

Laboratory Shuttle Bus Routes: Blue Route  

NLE Websites -- All DOE Office Websites (Extended Search)

Blue Route Map (On-Site/Off-Site) Blue Route Map (On-Site/Off-Site) Scroll down or click here for schedule ↓ Printable Map Blue Route map Blue Route Schedule Effective May 3, 2013 Text Box: BLUE SHUTTLE SCHEDULE BLUE Route # 65 DOWNHILL BART 65 UPHILL 62/66 1 6:20 AM 6:30 AM 6:40 AM 6:52 AM 2 6:30 AM 6:40 AM 6:50 AM 7:02 AM 3 6:40 AM 6:50 AM 7:00 AM 7:12 AM 4 6:50 AM 7:00 AM 7:10 AM 7:22 AM 1 7:04 AM 7:16 AM 7:28 AM 7:40 AM 2 7:16 AM 7:28 AM 7:40 AM 7:52 AM 3 7:28 AM 7:40 AM 7:52 AM 8:04 AM 4 7:40 AM 7:52 AM 8:04 AM 8:16 AM 1 7:52 AM 8:04 AM 8:16 AM 8:28 AM 2 8:04 AM 8:16 AM 8:28 AM 8:40 AM 3 8:16 AM 8:28 AM 8:40 AM 8:52 AM 4 8:28 AM 8:40 AM 8:52 AM 9:04 AM 1 8:40 AM 8:52 AM 9:04 AM 9:16 AM 2 8:52 AM 9:04 AM 9:16 AM 9:28 AM 3 9:04 AM 9:16 AM 9:28 AM 9:40 AM 4 9:16 AM 9:28 AM 9:40 AM 9:52 AM 1 9:28 AM 9:40 AM 9:52 AM 10:04 AM 2 9:40 AM 9:52 AM 10:04 AM 10:16 AM 3 9:52 AM 10:04 AM

176

Commercial new construction | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

6: Complete the ENERGY STAR lifecycle See projects that have been Designed to Earn the ENERGY STAR 1 World Green Building Trends: Business Benefits Driving New and Retrofit...

177

Star Biomass | Open Energy Information  

Open Energy Info (EERE)

Biomass Jump to: navigation, search Name Star Biomass Place India Sector Biomass Product Plans to set up biomass projects in Rajasthan. References Star Biomass1 LinkedIn...

178

ENERGY STAR Score for Hospitals  

NLE Websites -- All DOE Office Websites (Extended Search)

Hospitals in the United States Page 1 ENERGY STAR Score for Hospitals in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Hospitals applies to general...

179

Home : ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Who dared imagine? Who dared imagine? Our newest video celebrates 20 years of success with our innovative ENERGY STAR partners. See the Video EPA Logo ENERGY STAR is a U.S. Environmental Protection Agency voluntary program that helps businesses and individuals save money and protect our climate through superior energy efficiency. Learn more about ENERGY STAR. A comprehensive review of ENERGY STAR and other EPA climate protection partnerships. See 2011 Annual Report. Basic information on climate change, greenhouse gas emissions, and climate change science. See Climate Change. With help from ENERGY STAR, by 2012, Americans had cumulatively prevented more than 1.8 billion metric tons of GHG emissions. See 2012 Achievements. Energy Efficiency For Your Home

180

Protoneutron Star Winds  

E-Print Network (OSTI)

Neutrino-driven winds are thought to accompany the Kelvin-Helmholtz cooling phase of nascent protoneutron stars in the first seconds after a core-collapse supernova. These outflows are a likely candidate as the astrophysical site for rapid neutron-capture nucleosynthesis (the r-process). In this chapter we review the physics of protoneutron star winds and assess their potential as a site for the production of the heavy r-process nuclides. We show that spherical transonic protoneutron star winds do not produce robust $r$-process nucleosynthesis for `canonical' neutron stars with gravitational masses of 1.4 M_sun and coordinate radii of 10 km. We further speculate on and review some aspects of neutrino-driven winds from protoneutron stars with strong magnetic fields.

Todd A. Thompson

2003-09-03T23:59:59.000Z

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181

Electrically charged compact stars  

E-Print Network (OSTI)

We review here the classical argument used to justify the electrical neutrality of stars and show that if the pressure and density of the matter and gravitational field inside the star are large, then a charge and a strong electric field can be present. For a neutron star with high pressure (~ 10^{33} to 10^{35} dynes /cm^2) and strong gravitational field (~ 10^{14} cm/s^2), these conditions are satisfied. The hydrostatic equation which arises from general relativity, is modified considerably to meet the requirements of the inclusion of the charge. In order to see any appreciable effect on the phenomenology of the neutron stars, the charge and the electrical fields have to be huge (~ 10^{21} Volts/cm). These stars are not however stable from the viewpoint that each charged particle is unbound to the uncharged particles, and thus the system collapses one step further to a charged black hole

Subharthi Ray; Manuel Malheiro; Jose' P. S. Lemos; Vilson T. Zanchin

2006-04-17T23:59:59.000Z

182

Blue Ribbon Commission on America's Nuclear Future  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Blue Ribbon Commission on America's Nuclear Future Blue Ribbon Commission on America's Nuclear Future Agenda March 25 - 26, 2010 Willard Intercontinental Hotel, Washington, DC Thursday, March 25, 2010 Open Meeting - Grand Ballroom 11:00 a.m. Open meeting/review agenda Tim Frazier 11:10 a.m. Opening comments from Secretary Chu 11:25 a.m. Opening discussion - Co-chairs Honorable Lee Hamilton General Brent Scowcroft 11:35 a.m. Opening discussion - members Honorable Pete Domenici Honorable Chuck Hagel Honorable Phil Sharp Mr. Mark H. Ayers Honorable Vicky Bailey Dr. Albert Carnesale Ms. Susan Eisenhower Mr. Jonathan Lash Dr. Allison Macfarlane Dr. Richard A. Meserve Dr. Ernie Moniz Mr. John Rowe Dr. Per F. Peterson 12:30 p.m. Lunch

183

Blue Canyon VI | Open Energy Information  

Open Energy Info (EERE)

VI VI Jump to: navigation, search Name Blue Canyon VI Facility Blue Canyon VI Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner EDP Renewables North America LLC Developer EDP Renewables North America LLC Energy Purchaser Merchant Location Lawton OK Coordinates 34.8582°, -98.54752° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.8582,"lon":-98.54752,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

184

Blue Creek Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Farm Farm Jump to: navigation, search Name Blue Creek Wind Farm Facility Blue Creek Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Iberdrola Renewables Developer Iberdrola Renewables Energy Purchaser First Energy Solutions Location Van Wert County OH Coordinates 41.018286°, -84.615355° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.018286,"lon":-84.615355,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

185

Blue Sky Optimum Energy | Open Energy Information  

Open Energy Info (EERE)

Optimum Energy Optimum Energy Jump to: navigation, search Name Blue Sky Optimum Energy Place Buffalo, New York Product Blue Sky offers a processing system to produce biodiesel at a cheaper price. Coordinates 42.88544°, -78.878464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.88544,"lon":-78.878464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

186

Summit Blue Consulting | Open Energy Information  

Open Energy Info (EERE)

Summit Blue Consulting Summit Blue Consulting Place Boulder, Colorado Zip 80302 Sector Efficiency, Renewable Energy Product String representation "Consulting firm ... egy development" is too long. Coordinates 42.74962°, -109.714163° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.74962,"lon":-109.714163,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

187

Blue Sky Bio Fuels | Open Energy Information  

Open Energy Info (EERE)

Bio Fuels Bio Fuels Jump to: navigation, search Name Blue Sky Bio-Fuels Place Oakland, California Zip 94602 Product Blue Sky owns and operates a biodiesel plant in Idaho with a capacity of 37.9mLpa (10m gallons annually). Coordinates 37.805065°, -122.273024° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.805065,"lon":-122.273024,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

188

Genepool Memory Heatmaps  

NLE Websites -- All DOE Office Websites (Extended Search)

Genepool Memory Heatmaps Genepool Memory Heatmaps Heatmap of Memory and Slots Requested vs Time Waited (in hours) | Queue: All | Last 7 Days Memory Requested Slots <5GB 5-10GB 10-20GB 20-30GB 30-40GB 40-50GB 50-100GB 100-150GB 150-200GB 200-256GB 256-512GB 512+GB Job Count Longest Wait 1 2.26 (2693) 10.5 (201167) 3.2 (11650) 0 1.75 (282) 1.49 (1627) 0.03 (1) 0 0 0 0 0 217420 538.96 2 0.26 (103) 1.02 (2817) 0 0 0 0 0 0 0 0 0 0 2920 9.1 4 1.55 (198) 1.48 (104) 0.34 (8) 0 0 0 1.86 (3) 0 0 0 0 0 313 20.48 6 0.01 (1) 0.09 (34) 0 0 0 0 0 0 0 0 0 0 35 1.22 8 0.34 (37) 6.15 (12376) 1.01 (17) 24.7 (1) 0.03 (3) 0 0.02 (6) 0 0 0 0 0 12440 46.16 10 0 8.56 (1) 0 0 0 0 0 0 0 0 0 0 1 8.56 16 0 0.03 (1) 0 0 0 0 0 0 0 0 0 0 1 0.03 24 0 0 0.01 (1) 0 0 0 0 0 0 0 0 0 1 0.01 32 0 0.01 (4) 0.05 (9) 0 0.01 (6) 0 0.0 (1) 0 0 0 0 0 20 0.26

189

Shape memory alloy actuator  

DOE Patents (OSTI)

An actuator for cycling between first and second positions includes a first shaped memory alloy (SMA) leg, a second SMA leg. At least one heating/cooling device is thermally connected to at least one of the legs, each heating/cooling device capable of simultaneously heating one leg while cooling the other leg. The heating/cooling devices can include thermoelectric and/or thermoionic elements.

Varma, Venugopal K. (Knoxville, TN)

2001-01-01T23:59:59.000Z

190

What is Energy Star? ENERGY STAR  

E-Print Network (OSTI)

What is Energy Star? ENERGY STAR® qualified products and practices help you save money and reduce greenhouse gas emissions by meeting strict energy efficiency guidelines set by the U.S. Environmental Protection Agency (EPA) and the U.S. Department of Energy. You can help reduce electricity usage and its

van Tiggelen, Bart

191

HUNTING FOR YOUNG DISPERSING STAR CLUSTERS IN IC 2574  

SciTech Connect

Dissolving stellar groups are very difficult to detect using traditional surface photometry techniques. We have developed a method to find and characterize non-compact stellar systems in galaxies where the young stellar population can be spatially resolved. By carrying out photometry on individual stars, we are able to separate the luminous blue stellar population from the star field background. The locations of these stars are used to identify groups by applying the HOP algorithm, which are then characterized using color-magnitude and stellar density radial profiles to estimate age, size, density, and shape. We test the method on Hubble Space Telescope Advanced Camera for Surveys archival images of IC 2574 and find 75 dispersed stellar groups. Of these, 20 highly dispersed groups are good candidates for dissolving systems. We find few compact systems with evidence of dissolution, potentially indicating that star formation in this galaxy occurs mostly in unbound clusters or groups. These systems indicate that the dispersion rate of groups and clusters in IC 2574 is at most 0.45 pc Myr{sup -1}. The location of the groups found with HOP correlate well with H I contour map features. However, they do not coincide with H I holes, suggesting that those holes were not created by star-forming regions.

Pellerin, Anne [Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843-4242 (United States); Meyer, Martin M. [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, CRAWLEY WA 6009 (Australia); Calzetti, Daniella [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Harris, Jason, E-mail: apellerin@mta.ca, E-mail: martin.meyer@uwa.edu.au, E-mail: calzetti@astro.umass.edu, E-mail: jharris@30doradus.org [Illumina, Inc., 25861 Industrial Blvd, Hayward, CA 94545 (United States)

2012-12-01T23:59:59.000Z

192

Leading organizations choose ENERGY STAR | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Leading organizations choose ENERGY STAR Leading organizations choose ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why design to earn ENERGY STAR Leading organizations choose ENERGY STAR Sell others on the idea of ENERGY STAR An overview of the ENERGY STAR lifecycle Design to earn ENERGY STAR Leading organizations choose ENERGY STAR Facebook's data center achieved Designed to Earn the ENERGY STAR More than

193

Page placement in hybrid memory systems  

Science Conference Proceedings (OSTI)

Phase-Change Memory (PCM) technology has received substantial attention recently. Because PCM is byte-addressable and exhibits access times in the nanosecond range, it can be used in main memory designs. In fact, PCM has higher density and lower idle ... Keywords: hybrid memory, memory controller, phase-change memory

Luiz E. Ramos; Eugene Gorbatov; Ricardo Bianchini

2011-05-01T23:59:59.000Z

194

APC: a performance metric of memory systems  

Science Conference Proceedings (OSTI)

Due to the infamous "memory wall" problem and a drastic increase in the number of data intensive applications, memory rather than processor has become the leading performance bottleneck of modern computing systems. Evaluating and understanding memory ... Keywords: measurement methodology, memory metric, memory performance measurement

Xian-He Sun; Dawei Wang

2012-10-01T23:59:59.000Z

195

Hypernuclear Physics for Neutron Stars  

E-Print Network (OSTI)

The role of hypernuclear physics for the physics of neutron stars is delineated. Hypernuclear potentials in dense matter control the hyperon composition of dense neutron star matter. The three-body interactions of nucleons and hyperons determine the stiffness of the neutron star equation of state and thereby the maximum neutron star mass. Two-body hyperon-nucleon and hyperon-hyperon interactions give rise to hyperon pairing which exponentially suppresses cooling of neutron stars via the direct hyperon URCA processes. Non-mesonic weak reactions with hyperons in dense neutron star matter govern the gravitational wave emissions due to the r-mode instability of rotating neutron stars.

Jurgen Schaffner-Bielich

2008-01-24T23:59:59.000Z

196

Applications of Shape Memory Alloys  

Science Conference Proceedings (OSTI)

Mar 3, 2011 ... More than 50 years after the discovery of shape memory alloys, and after investments of millions of dollars, there are very few successful...

197

Using Hardware Memory Protection to Build a High-Performance, Strongly-Atomic Hybrid Transactional Memory  

Science Conference Proceedings (OSTI)

We demonstrate how fine-grained memory protection can be used in support of transactional memory systems: first showing how a software transactional memory system (STM) can be made strongly atomic by using memory protection on transactionally-held state, ... Keywords: Transactional Memory, Hybrid, Memory Protection, Primitives, Abort Handler, Strong Atomicity

Lee Baugh; Naveen Neelakantam; Craig Zilles

2008-06-01T23:59:59.000Z

198

Service providers | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

buildings and industrial plants. Photo of a man with a clipboard. Verify applications for ENERGY STAR certification Find how-to guides and training for individuals who sign off on...

199

Blue, green, orange, and red upconversion laser  

DOE Patents (OSTI)

A laser for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr.sup.3+ ions and Yb.sup.3+ ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output.

Xie, Ping (San Jose, CA); Gosnell, Timothy R. (Sante Fe, NM)

1998-01-01T23:59:59.000Z

200

Blue, green, orange, and red upconversion laser  

DOE Patents (OSTI)

A laser is disclosed for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr{sup 3+} ions and Yb{sup 3+} ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output. 11 figs.

Xie, P.; Gosnell, T.R.

1998-09-08T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

An analysis of MRAM based memory technologies  

E-Print Network (OSTI)

MRAM is a memory (RAM) technology that uses electron spin to store information. Often been called "the ideal memory", it can potentially combine the density of DRAM with the speed of SRAM and non-volatility of FLASH memory ...

Vijayaraghavan, Rangarajan, M. Eng. Massachusetts Institute of Technology

2006-01-01T23:59:59.000Z

202

Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars  

E-Print Network (OSTI)

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in two additional cases. The mean pulsation period of Blazhko stars is 0.04 d shorter than the mean period of the entire RRab sample in M5. Among the RRab stars with period shorter than 0.55 d the incidence rate of the modulation is as high as 60 per cent. The mean $B-V$ colours of Blazhko stars overlap with the colours of first overtone RRc (RR1) pulsators. The mean $V$ magnitudes of Blazhko stars are on the average 0.05-mag fainter than those of the RRab stars with stable light curves. Blazhko stars tend to be situated close to the zero-age horizontal branch at the blue edge of the fundamental-mode instability strip in M5. We speculate that this specific location hints that the Blazhko effect may have an evolutionary connection with the mode switch from the fundamental to the overtone-mode pulsation.

Jurcsik, J; Clement, C; Hurta, Zs; Lovas, M

2010-01-01T23:59:59.000Z

203

IBM Blue Gene Parallel Supercomputer, Brookhaven National Laboratory, (BNL)  

NLE Websites -- All DOE Office Websites (Extended Search)

L L Overview Simple Example: Compile, Link, Run Compiler Invocation Compile and Link Tips Batch Job Submission Applications Support Math Libraries MPI Version IBM Fortran Blue Gene & Linux Manuals (IBM Redbooks) Much of the info you need will be in the Linux manual, but there is also some Blue Gene-specific info in the Blue Gene manual. Current Fortran compiler version number can be determined on fen by typing: ls /opt/ibmcmp/xlf/bg, will be highest number listed. IBM C/C++ Blue Gene & Linux Manuals (IBM Redbooks) Much of the info you need will be in the Linux manual, but there is also some Blue Gene-specific info in the Blue Gene manual. Linux Manual: Go to XL C/C++ for Linux, choose the Product Library link, then select current version number in tab at page top. (Current C/C++

204

A Preliminary Structural Model for the Blue Mountain Geothermal Field,  

Open Energy Info (EERE)

Structural Model for the Blue Mountain Geothermal Field, Structural Model for the Blue Mountain Geothermal Field, Humboldt County, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: A Preliminary Structural Model for the Blue Mountain Geothermal Field, Humboldt County, Nevada Abstract The Blue Mountain geothermal field is a blind geothermalprospect (i.e., no surface hot springs) along the west flank of BlueMountain in southern Humboldt County, Nevada. Developmentwells in the system have high flow rates and temperatures above190°C at depths of ~600 to 1,070 m. Blue Mountain is a small~8-km-long east-tilted fault block situated between the EugeneMountains and Slumbering Hills. The geothermal field occupiesthe intersection between a regional NNE- to ENE-striking,west-dipping

205

DISCOVERY OF A WOLF-RAYET STAR THROUGH DETECTION OF ITS PHOTOMETRIC VARIABILITY  

SciTech Connect

We report the serendipitous discovery of a heavily reddened Wolf-Rayet star that we name WR 142b. While photometrically monitoring a cataclysmic variable, we detected weak variability in a nearby field star. Low-resolution spectroscopy revealed a strong emission line at 7100 A, suggesting an unusual object and prompting further study. A spectrum taken with the Hobby-Eberly Telescope confirms strong He II emission and an N IV 7112 A line consistent with a nitrogen-rich Wolf-Rayet star of spectral class WN6. Analysis of the He II line strengths reveals no detectable hydrogen in WR 142b. A blue-sensitive spectrum obtained with the Large Binocular Telescope shows no evidence for a hot companion star. The continuum shape and emission line ratios imply a reddening of E(B - V) = 2.2-2.6 mag. We estimate that the distance to WR 142b is 1.4 {+-} 0.3 kpc.

Littlefield, Colin [Law School, University of Notre Dame, Notre Dame, IN 46556 (United States); Garnavich, Peter; McClelland, Colin; Rettig, Terrence [Physics Department, University of Notre Dame, Notre Dame, IN 46556 (United States); Marion, G. H. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Vinko, Jozsef [Department of Optics, University of Szeged (Hungary); Wheeler, J. Craig [Astronomy Department, University of Texas, Austin, TX 78712 (United States)

2012-06-15T23:59:59.000Z

206

Blue Oak Energy | Open Energy Information  

Open Energy Info (EERE)

Energy Energy Jump to: navigation, search Logo: Blue Oak Energy Name Blue Oak Energy Address 4614 Second Street Place Davis, California Zip 95618 Sector Solar Product photovoltaics, design and engineering, feasibility studies, turn-key installation, system maintenance, PV products Year founded 2003 Number of employees 11-50 Phone number (530) 747-2026 Website http://www.blueoakenergy.com Coordinates 38.5509256°, -121.7069073° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.5509256,"lon":-121.7069073,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

207

Blue Mountain Geothermal Area | Open Energy Information  

Open Energy Info (EERE)

form form View source History View New Pages Recent Changes All Special Pages Semantic Search/Querying Get Involved Help Apps Datasets Community Login | Sign Up Search Page Edit with form History Facebook icon Twitter icon » Blue Mountain Geothermal Area Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermal Resource Area: Blue Mountain Geothermal Area Contents 1 Area Overview 2 History and Infrastructure 3 Regulatory and Environmental Issues 4 Exploration History 5 Well Field Description 6 Geology of the Area 7 Geofluid Geochemistry 8 NEPA-Related Analyses (2) 9 Exploration Activities (15) 10 References Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":6,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"500px","height":"300px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41,"lon":-118.13,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

208

Blue Hill Partners LLC | Open Energy Information  

Open Energy Info (EERE)

Logo: Blue Hill Partners LLC Name Blue Hill Partners LLC Address 40 W. Evergreen Ave. Place Philadelphia, Pennsylvania Zip 19118 Region Northeast - NY NJ CT PA Area Product Invests equity capital in venture-stage companies in the advanced industrial technology sector Phone number (215) 247-2400 Website http://www.bluehillpartners.co Coordinates 40.075493°, -75.208266° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.075493,"lon":-75.208266,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

209

ENERGY STAR industrial partnership | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR industrial partnership ENERGY STAR industrial partnership Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Improve energy performance ENERGY STAR industrial partnership New ENERGY STAR industrial partners Energy guides Energy efficiency and air regulation

210

Use ENERGY STAR benchmarking tools | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Use ENERGY STAR benchmarking tools Use ENERGY STAR benchmarking tools Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use Learn about benchmarking Use ENERGY STAR benchmarking tools ENERGY STAR in action Communicate and educate

211

Shape memory alloy thaw sensors  

DOE Patents (OSTI)

A sensor permanently indicates that it has been exposed to temperatures exceeding a critical temperature for a predetermined time period. An element of the sensor made from shape memory alloy changes shape when exposed, even temporarily, to temperatures above the Austenitic temperature of the shape memory alloy. The shape change of the SMA element causes the sensor to change between two readily distinguishable states.

Shahinpoor, Mohsen (Albuquerque, NM); Martinez, David R. (Albuquerque, NM)

1998-01-01T23:59:59.000Z

212

Memory exploration for low power, embedded systems  

Science Conference Proceedings (OSTI)

Keywords: cache simulator, design automation, low power design, low power embedded systems, memory exploration and optimization, memory hierarchy, off-chip data assignment

Wen-Tsong Shiue; Chaitali Chakrabarti

1999-06-01T23:59:59.000Z

213

Self Potential At Blue Mountain Area (Fairbank Engineering, 2008) | Open  

Open Energy Info (EERE)

Page Page Edit History Facebook icon Twitter icon » Self Potential At Blue Mountain Area (Fairbank Engineering, 2008) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Self Potential At Blue Mountain Area (Fairbank Engineering, 2008) Exploration Activity Details Location Blue Mountain Area Exploration Technique Self Potential Activity Date Usefulness not indicated DOE-funding Unknown Notes Geophysical surveys that have been conducted specifically for the geothermal program at Blue Mountain include a self-potential (SP) survey, and additional IP/electrical resistivity traversing. These surveys were conducted under a cooperative program between Noramex Corporation and the Energy and Geosciences Institute (EGI), University of Utah, with funding

214

Observation Wells At Blue Mountain Area (Warpinski, Et Al., 2004...  

Open Energy Info (EERE)

navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Observation Wells At Blue Mountain Area (Warpinski, Et Al., 2004) Exploration Activity Details Location...

215

Update on Blue Ribbon Commission for America's Nuclear Future...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

More Documents & Publications Summary Minutes of the Secretary of Energy Advisory Board Public Meeting on October 12, 2011 Blue Ribbon Commission on...

216

Epithermal Gold Mineralization and a Geothermal Resource at Blue...  

Open Energy Info (EERE)

1991 DOI Not Provided Check for DOI availability: http:crossref.org Online Internet link for Epithermal Gold Mineralization and a Geothermal Resource at Blue Mountain,...

217

Energy Materials Blue Ribbon Panel Releases Vision Report  

Science Conference Proceedings (OSTI)

Jun 22, 2010 ... Said Blue Ribbon Panel member Michael J. Dolan, senior vice ... Solar technology, while being designated as a moderately important MSE...

218

Pages that link to "Aeromagnetic Survey At Blue Mountain Area...  

Open Energy Info (EERE)

wikiSpecial:WhatLinksHereAeromagneticSurveyAtBlueMountainArea(FairbankEngineering,2004)" Special pages About us Disclaimers Energy blogs Developer services...

219

Pages that link to "Aeromagnetic Survey At Blue Mountain Area...  

Open Energy Info (EERE)

wikiSpecial:WhatLinksHereAeromagneticSurveyAtBlueMountainArea(FairbankEngineering,2003)" Special pages About us Disclaimers Energy blogs Developer services...

220

Jazz and Blues Legends Rock the Northeast, Help Save Louisiana ...  

U.S. Energy Information Administration (EIA)

Jazz and Blues Legends Rock the Northeast, Help Save Louisiana's Coastal Wetlands. 6.8.2006 Neville Brothers, Dr. John and Mavis Staples Highlight the ...

Note: This page contains sample records for the topic "blue star memorial" 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

Energy Materials Blue Ribbon Panel Report June 2010 - TMS  

Science Conference Proceedings (OSTI)

Jun 22, 2010 ... The Energy Materials Blue Ribbon Panel convened by TMS has released Linking Transformational Materials and Processing for an Energy-...

222

Blue Hill Investment Partners LLC | Open Energy Information  

Open Energy Info (EERE)

Investment Partners LLC Jump to: navigation, search Name Blue Hill Investment Partners LLC Place Philadelphia, Pennsylvania Zip PA 19118 Sector Renewable Energy Product A...

223

Improved Performance of a Fluorescent Blue Organic Light Emitting ...  

Science Conference Proceedings (OSTI)

Presentation Title, Improved Performance of a Fluorescent Blue Organic Light Emitting Diode with Hole Blocking Materials as Dopants for Transport Layers.

224

Blue Crane Holdings Pvt Ltd | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Name Blue Crane Holdings Pvt. Ltd. Place Mumbai, Maharashtra, India Zip 400023 Sector Efficiency, Solar, Wind energy Product Mumbai-based firm involved...

225

ENERGY STAR | Open Energy Information  

Open Energy Info (EERE)

ENERGY STAR ENERGY STAR Jump to: navigation, search Logo: ENERGY STAR Name ENERGY STAR Year founded 1992 Notes Partnered with more than 20,000 public sector organizations. Website https://www.energystar.gov/ind References About ENERGY STAR[1] LinkedIn Connections Contents 1 About ENERGY STAR 1.1 For the Home 1.2 For Business 1.3 References About ENERGY STAR ENERGY STAR is a joint program of the U.S. Environmental Protection Agency and the U.S. Department of Energy helping us all save money and protect the environment through energy efficient products and practices. Results are already adding up. Americans, with the help of ENERGY STAR, saved enough energy in 2010 alone to avoid greenhouse gas emissions equivalent to those from 33 million cars - all while saving nearly $18 billion on their

226

ENERGY STAR Focus on Energy Efficiency in Printing | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

227

ENERGY STAR certification for your building | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

that your building can earn ENERGY STAR certification just like a refrigerator or light bulb? The mark of efficiency No matter where you see it, the ENERGY STAR label means the...

228

ENERGY STAR Small Business Network List | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

229

Comment submitted by Traulsen regarding the Energy Star Verification Testing Program  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4401 Blue Mound Rd. www.traulsen.com 817 740-6733 4401 Blue Mound Rd. www.traulsen.com 817 740-6733 Fort Worth, Texas 76106 cboryca@traulsen.com 800 825-8220 Date: May 9, 2011 To: Ms. Ashley Armstrong, Ms. Brenda Edwards From: Mr. Chris Boryca, Engineer II Cc: John Davis, Walt Boryca, Gary Hoying, Mike Lynch, Joe Sanders, Jennifer Baker Reid Subject: DOE Verification in Support of Energy Star These comments are in response to the document released on April 22, 2011 related to verification testing in support of Energy Star. As a general statement Traulsen is pleased to hear that the DOE and EPA are working together. We do have several concerns, some of which the DOE has seen before and will be quickly restated. 6.3 Manufacturer Notification Traulsen believes that barring manufacturers who operate qualified "Client Test Data Program" test labs from

230

Making Carbon in Stars  

E-Print Network (OSTI)

The triple alpha process plays an important role in the production of 12C in stars. Its rate is known with an accuracy of about 12%. We examine the corresponding uncertainties introduced in the description of pre-supernova stars, of nucleosynthesis in a core-collapse SN explosion, and of the production of 12C during the third dredge-up in asymptotic giant branch (AGB) stars. For the AGB case we consider also the effects of uncertainties in the 14N(p,gamma)15O rate. We conclude that the present accuracy of the triplr alpha rate is inadequate and describe new experiments that will lead to a more accurate value.

Sam M. Austin

2004-11-30T23:59:59.000Z

231

ENERGY STAR Commercial Buildings College Course | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program...

232

ENERGY STAR Guidelines for Energy Management | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

233

ENERGY STAR Partner of the Year Awards | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

234

Earn the ENERGY STAR and other recognition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

235

ENERGY STAR portfolio-wide recognition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

236

ELECTROSTATIC MEMORY SYSTEM  

DOE Patents (OSTI)

An improved electrostatic memory system is de scribed fer a digital computer wherein a plarality of storage tubes are adapted to operate in either of two possible modes. According to the present irvention, duplicate storage tubes are provided fur each denominational order of the several binary digits. A single discriminator system is provided between corresponding duplicate tubes to determine the character of the infurmation stored in each. If either tube produces the selected type signal, corresponding to binazy "1" in the preferred embodiment, a "1" is regenerated in both tubes. In one mode of operation each bit of information is stored in two corresponding tubes, while in the other mode of operation each bit is stored in only one tube in the conventional manner.

Chu, J.C.

1958-09-23T23:59:59.000Z

237

Pacific Blue Energy | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Name Pacific Blue Energy Place Flagstaff, Arizona Zip 86001 Sector Solar Product Arizona-based solar project developer. Coordinates 45.238793°, -70.330276° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":45.238793,"lon":-70.330276,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

238

Blue Canyon Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Wind Farm Wind Farm Facility Blue Canyon Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Babcock & Brown/Horizon Developer Zilkha Renewable/Kirmart Corp. Energy Purchaser Western Farmers' Electric Cooperative Location North of Lawton OK Coordinates 34.852678°, -98.551807° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.852678,"lon":-98.551807,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

239

Blue Marble Energy | Open Energy Information  

Open Energy Info (EERE)

Energy Energy Jump to: navigation, search Name Blue Marble Energy Address P.O. Box 9190 Place Seattle, Washington Zip 98109 Sector Biomass Product Aims to turn algae and other cellulosic biomass into natural gas Website http://www.bluemarbleenergy.ne Coordinates 47.6163159°, -122.3463563° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":47.6163159,"lon":-122.3463563,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

240

Statistical thermodynamics of supercapacitors and blue engines  

E-Print Network (OSTI)

We study the thermodynamics of electrode-electrolyte systems, for instance supercapacitors filled with an ionic liquid or blue-energy devices filled with river- or sea water. By a suitable mapping of thermodynamic variables, we identify a strong analogy with classical heat engines. We introduce several Legendre transformations and Maxwell relations. We argue that one should distinguish between the differential capacity at constant ion number and at constant ion chemical potential, and derive a relation between them that resembles the standard relation between heat capacity at constant volume and constant pressure. Finally, we consider the probability distribution of the electrode charge at a given electrode potential, the standard deviation of which is given by the differential capacity.

Ren van Roij

2012-11-06T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

Blue Grass Energy - Residential Energy Efficiency Rebate Program...  

Open Energy Info (EERE)

certify it with the EPA as an Energy Star home. The Energy Star label increases the value and efficiency of a home as well as the resale value. This program is available to...

242

BlueTorrent: Cooperative content sharing for Bluetooth users  

Science Conference Proceedings (OSTI)

People wish to enjoy their everyday lives in various ways, among which entertainment plays a major role. In order to improve lifestyle with more ready access to entertainment content, we propose BlueTorrent, a P2P file sharing application based on ubiquitous ... Keywords: BlueTorrent, Bluetooth, P2P

Sewook Jung; Uichin Lee; Alexander Chang; Dae-Ki Cho; Mario Gerla

2007-12-01T23:59:59.000Z

243

Early Experience on the Blue Gene/Q Supercomputing System  

Science Conference Proceedings (OSTI)

The Argonne Leadership Computing Facility (ALCF) is home to Mira, a10 PF Blue Gene/Q (BG/Q) system. The BG/Q system is the third generation in Blue Gene architecture from IBM and like its predecessors combines system-on-chip technology with a proprietary ... Keywords: supercomputing, performance, multi-core, scalability, applications

Vitali Morozov, Kalyan Kumaran, Venkatram Vishwanath, Jiayuan Meng, Michael E. Papka

2013-05-01T23:59:59.000Z

244

Petascale Debugging via Allinea DDT for IBM Blue Gene /P  

E-Print Network (OSTI)

@allinea.com> Senior Systems Engineer, Allinea Software Inc. ALCF L2P Workshop, May 23, 2012 #12;Outline ExperienceArchitecture #12;Current Status IBM Blue Gene /P Acceptance testing at ALCF (Allinea DDT 3.1) ­ Scale (Allinea DDT 3.2) ­ Early access for IBM Blue Gene /Q expected July 2012 ALCF requirement ­ Scale for Mira

Kemner, Ken

245

EnsemBlue: integrating distributed storage and consumer electronics  

Science Conference Proceedings (OSTI)

EnsemBlue is a distributed file system for personal multimedia that incorporates both general-purpose computers and consumer electronic devices (CEDs). Ensem-Blue leverages the capabilities of a few general-purpose computers to make CEDs first class ...

Daniel Peek; Jason Flinn

2006-11-01T23:59:59.000Z

246

BlueGene/L applications: Parallelism On a Massive Scale  

Science Conference Proceedings (OSTI)

BlueGene/L (BG/L), developed through a partnership between IBM and Lawrence Livermore National Laboratory (LLNL), is currently the world's largest system both in terms of scale, with 131,072 processors, and absolute performance, with a peak rate of ... Keywords: BlueGene/L, application scalability, massively parallel architectures, performance study and optimization

Bronis R. De Supinski; Martin Schulz; Vasily V. Bulatov; William Cabot; Bor Chan; Andrew W. Cook; Erik W. Draeger; James N. Glosli; Jeffrey A. Greenough; Keith Henderson; Alison Kubota; Steve Louis; Brian J. Miller; Mehul V. Patel; Thomas E. Spelce; Frederick H. Streitz; Peter L. Williams; Robert K. Yates; Andy Yoo; George Almasi; Gyan Bhanot; Alan Gara; John A. Gunnels; Manish Gupta; Jose Moreira; James Sexton; Bob Walkup; Charles Archer; Francois Gygi; Timothy C. Germann; Kai Kadau; Peter S. Lomdahl; Charles Rendleman; Michael L. Welcome; William Mclendon; Bruce Hendrickson; Franz Franchetti; Stefan Kral; Jrgen Lorenz; Christoph W. berhuber; Edmond Chow; mit atalyrek

2008-02-01T23:59:59.000Z

247

ENERGY STAR Score for Hotels  

NLE Websites -- All DOE Office Websites (Extended Search)

Hotels in the United States Page 1 ENERGY STAR Score for Hotels in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Hotels applies to properties renting...

248

Shape memory metals. Final report  

SciTech Connect

The ability to define a manufacturing process to form, heat-treat, and join parts made of nickel-titanium and/or copper-zinc-aluminum shape memory alloys was investigated. The specific emphasis was to define a process that would produce shape memory alloy parts in the configuration of helical coils emulating the appearance of compression springs. In addition, the mechanical strength of the finished parts along with the development of a electrical lead attachment method using shape memory alloy wire was investigated.

Dworak, T.D.

1993-09-01T23:59:59.000Z

249

Barron Electric Cooperative - Energy Star Appliance & Energy...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Barron Electric Cooperative - Energy Star Appliance & Energy Efficient Lighting Rebate Program Barron Electric Cooperative - Energy Star Appliance & Energy Efficient Lighting...

250

Learn the benefits | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

251

About the battle | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

252

Direct-Current Resistivity At Blue Mountain Area (Fairbank Engineering,  

Open Energy Info (EERE)

Direct-Current Resistivity At Blue Mountain Area (Fairbank Engineering, Direct-Current Resistivity At Blue Mountain Area (Fairbank Engineering, 2005) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Direct-Current Resistivity At Blue Mountain Area (Fairbank Engineering, 2005) Exploration Activity Details Location Blue Mountain Area Exploration Technique Direct-Current Resistivity Survey Activity Date Usefulness not indicated DOE-funding Unknown Notes Geophysical surveys that have been conducted specifically for the geothermal program at Blue Mountain include a self-potential (SP) survey, and additional IP/electrical resistivity traversing. These surveys were conducted under a cooperative program between Noramex Corporation and the Energy and Geosciences Institute (EGI), University of Utah, with funding

253

Static Temperature Survey At Blue Mountain Area (Fairbank Engineering,  

Open Energy Info (EERE)

Static Temperature Survey At Blue Mountain Area (Fairbank Engineering, Static Temperature Survey At Blue Mountain Area (Fairbank Engineering, 2010) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Static Temperature Survey At Blue Mountain Area (Fairbank Engineering, 2010) Exploration Activity Details Location Blue Mountain Area Exploration Technique Static Temperature Survey Activity Date Usefulness useful DOE-funding Unknown Notes Using a precision thermistor probe, EGI, University of Utah, obtained detailed temperature logs of eleven new mineral exploration holes drilled at Blue Mountain. The holes, ranging in depth from 99 to 244 meters (325 to 800 feet), were drilled in areas to the northeast, northwest and southwest of, and up to distances of two kilometers from, the earlier mineral exploration drill holes that encountered hot artesian flows. Unfortunately,

254

The Blue Ribbon Commission Offers Strong Step Forward | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

The Blue Ribbon Commission Offers Strong Step Forward The Blue Ribbon Commission Offers Strong Step Forward The Blue Ribbon Commission Offers Strong Step Forward July 29, 2011 - 12:27pm Addthis Damien LaVera Damien LaVera Deputy Director, Office of Public Affairs Today, the Blue Ribbon Commission on America's Nuclear Future issued a draft of its recommendations. The Obama Administration continues to believe that nuclear energy has an important role to play as America moves to a clean energy future. As part of our commitment to restarting the American nuclear industry and creating thousands of new jobs and export opportunities in the process, we are committed to finding a sustainable approach to assuring safe, secure long-term disposal of used nuclear fuel and nuclear waste. Secretary Chu appreciates the hard work done by the members of the Blue

255

Geophysical Studies in the Vicinity of Blue Mountain and Pumpernickel  

Open Energy Info (EERE)

the Vicinity of Blue Mountain and Pumpernickel the Vicinity of Blue Mountain and Pumpernickel Valley near Winnemucca, North-Central Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: Geophysical Studies in the Vicinity of Blue Mountain and Pumpernickel Valley near Winnemucca, North-Central Nevada Abstract From May 2008 to September 2009, the U.S. Geological Survey (USGS) collected data from more than 660 gravity stations, 100 line-km of truck-towed magnetometer traverses, and 260 physical-property sites in the vicinity of Blue Mountain and Pumpernickel Valley, northern Nevada (fig. 1). Gravity, magnetic, and physical-property data were collected to study regional crustal structures as an aid to understanding the geologic framework of the Blue Mountain and Pumpernickel Valley areas, which in

256

Blue Lake Plant Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

Blue Lake Plant Biomass Facility Blue Lake Plant Biomass Facility Jump to: navigation, search Name Blue Lake Plant Biomass Facility Facility Blue Lake Plant Sector Biomass Location Blue Lake, California Coordinates 40.8829072°, -123.9839488° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.8829072,"lon":-123.9839488,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

257

Building Energy Software Tools Directory: BlueSol  

NLE Websites -- All DOE Office Websites (Extended Search)

BlueSol BlueSol tool_bluesol BlueSol is a software for the design of photovoltaic systems in every country in the world. It allows you to perform the entire process of designing a PV system, from the preliminary assessment of producibility to the realization of the project documentation. Screen Shots Keywords PV system sizing, PV system simulation, grid-connected PV systems, electrical components, shading, economic analysis. Validation/Testing N/A Expertise Required No special expertise or training needed. Users BlueSol runs in English language and has been released in may 2013. BlueSol originates from his Italian version: over 2100 copies of Italian version dowloaded since it was first release in november 2009. Audience PV specialists, energy and electrical engineers, system installers, energy

258

A durable and energy efficient main memory using phase change memory technology  

Science Conference Proceedings (OSTI)

Using nonvolatile memories in memory hierarchy has been investigated to reduce its energy consumption because nonvolatile memories consume zero leakage power in memory cells. One of the difficulties is, however, that the endurance of most nonvolatile ... Keywords: endurance, low power, phase change memory

Ping Zhou; Bo Zhao; Jun Yang; Youtao Zhang

2009-06-01T23:59:59.000Z

259

Spectral signatures of photosynthesis II: coevolution with other stars and the atmosphere on extrasolar worlds  

E-Print Network (OSTI)

As photosynthesis on Earth produces the primary signatures of life that can be detected astronomically at the global scale, a strong focus of the search for extrasolar life will be photosynthesis, particularly photosynthesis that has evolved with a different parent star. We take planetary atmospheric compositions simulated by Segura, et al. (2003, 2005) for Earth-like planets around observed F2V and K2V stars, modeled M1V and M5V stars, and around the active M4.5V star AD Leo; our scenarios use Earth's atmospheric composition as well as very low O2 content in case anoxygenic photosynthesis dominates. We calculate the incident spectral photon flux densities at the surface of the planet and under water. We identify bands of available photosynthetically relevant radiation and find that photosynthetic pigments on planets around F2V stars may peak in absorbance in the blue, K2V in the red-orange, and M stars in the NIR, in bands at 0.93-1.1 microns, 1.1-1.4 microns, 1.5-1.8 microns, and 1.8-2.5 microns. In addition, we calculate wavelength restrictions for underwater organisms and depths of water at which they would be protected from UV flares in the early life of M stars. We estimate the potential productivity for both surface and underwater photosynthesis, for both oxygenic and anoxygenic photosynthesis, and for hypothetical photosynthesis in which longer wavelength, multi-photosystem series are used.

Nancy Y. Kiang; Antigona Segura; Giovanna Tinetti; Govindjee; Robert E. Blankenship; Martin Cohen; Janet Siefert; David Crisp; Victoria S. Meadows

2007-01-12T23:59:59.000Z

260

High-gravity central stars  

E-Print Network (OSTI)

NLTE spectral analyses of high-gravity central stars by means of state-of-the-art model atmosphere techniques provide information about the precursor AGB stars. The hydrogen-deficient post-AGB stars allow investigations on the intershell matter which is apparently exhibited at the stellar surface. We summarize recent results from imaging, spectroscopy, and spectropolarimetry.

Thomas Rauch

2006-07-11T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

THE BHB STARS IN THE SURVEY FIELDS OF RODGERS ET AL. (1993): NEW OBSERVATIONS AND COMPARISONS WITH OTHER RECENT SURVEYS  

Science Conference Proceedings (OSTI)

We study blue horizontal branch (BHB) and RR Lyrae stars in the Rodgers et al. fields and compare their velocity and density distributions with other surveys in the same part of the sky. Photometric data are given for 176 early-type stars in the northern field. We identify fourteen BHB stars and four possible BHB stars, and determine the selection efficiency of the Century survey, the HK survey, and the SDSS survey for BHB stars. We give light curves and {gamma} radial velocities for three type ab RR Lyrae stars in the northern field; comparison with the nearby LONEOS survey shows that there is likely to be an equal number of lower-amplitude type ab RR Lyrae stars that we do not find. There are therefore at least twice as many BHB stars as type ab RR Lyrae stars in the northern field-similar to the ratio in the solar neighborhood. The velocity distribution of the southern field shows no evidence for an anomalous thick disk that was found by Gilmore et al.; the halo velocity peaks at a slightly prograde rotational velocity but there is also a significant retrograde halo component in this field. The velocity distribution in the northern field shows no evidence of Galactic rotation for |Z| {>=} 4 kpc and a slight prograde motion for |Z| < 4 kpc. The space densities of BHB stars in the northern field agree with an extrapolation of the power-law distribution recently derived by de Propris et al. For |Z| < 4 kpc, however, we observe an excess of BHB stars compared with this power law. We conclude that these BHB stars mostly belong to a spatially flattened, non-rotating inner halo component of the Milky Way in confirmation of the Kinman et al. analysis of Century survey BHB stars.

Kinman, T. D. [NOAO, P.O. Box 26732, Tucson, Arizona 85726 (United States); Brown, Warren R. [Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138 (United States)

2011-05-15T23:59:59.000Z

262

ENERGY STAR plant certification | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

» ENERGY STAR plant certification » ENERGY STAR plant certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Improve energy performance Industrial service and product providers Earn recognition ENERGY STAR Partner of the Year Award

263

Campaigns and incentive programs that incorporate ENERGY STAR | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Campaigns and incentive programs that incorporate ENERGY STAR Campaigns and incentive programs that incorporate ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Policies that specify the use of ENERGY STAR tools Campaigns and incentive programs that incorporate ENERGY STAR Lead by example Gather support Develop programs and policies Host a competition Use financing vehicles

264

ENERGY STAR service and product provider training series | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

service and product provider training series service and product provider training series Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can ENERGY STAR help your business? Get started Join ENERGY STAR as a partner ENERGY STAR service & product provider training series Service and product provider's marketing toolkit ENERGY STAR sales tools for service and product providers

265

Window To The Stars  

E-Print Network (OSTI)

We present Window To The Stars, a graphical user interface to the popular TWIN single/binary stellar evolution code, for novices, students and professional astrophysicists. It removes the drudgery associated with the traditional approach to running the code, while maintaining the power, output quality and flexibility a modern stellar evolutionist requires. It is currently being used for cutting edge research and interactive teaching.

Robert G. Izzard; Evert Glebbeek

2006-07-27T23:59:59.000Z

266

OMC-INTEGRAL Memory Management  

Science Conference Proceedings (OSTI)

The management of the memory restrictions imposed by the processor (1750A) was one of the major difficulties found in designing the Software (SW) controlling the Optical Monitoring Camera (OMC) payload of the International Gamma Ray Laboratory (INTEGRAL) ...

Jose Manuel Prez Lobato; Eva Martn Lobo

2002-06-01T23:59:59.000Z

267

Leading firms choose ENERGY STAR | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Leading firms choose ENERGY STAR Leading firms choose ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why you should design to earn the ENERGY STAR Leading firms choose ENERGY STAR Why new doesn't always mean efficient Follow EPA's step-by-step process ENERGY STAR Challenge for Architects Leading firms choose ENERGY STAR Facebook data center Hundreds of leading A/E firms have already partnered

268

About ENERGY STAR for commercial and industrial buildings | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR for commercial and industrial buildings ENERGY STAR for commercial and industrial buildings Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Facts and stats Climate change and buildings

269

Earn ENERGY STAR certification | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Earn ENERGY STAR certification Earn ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR

270

Anisotropic mass ejection from black hole-neutron star binaries: Diversity of electromagnetic counterparts  

E-Print Network (OSTI)

The merger of black hole-neutron star binaries can eject substantial material with the mass ~0.01-0.1M_sun when the neutron star is disrupted prior to the merger. The ejecta shows significant anisotropy, and travels in a particular direction with the bulk velocity ~0.2c. This is drastically different from the binary neutron star merger, for which ejecta is nearly isotropic. Anisotropic ejecta brings electromagnetic-counterpart diversity which is unique to black hole-neutron star binaries, such as viewing-angle dependence, polarization, and proper motion. The kick velocity of the black hole, gravitational-wave memory emission, and cosmic-ray acceleration are also discussed.

Koutarou Kyutoku; Kunihito Ioka; Masaru Shibata

2013-05-27T23:59:59.000Z

271

Halo Star Evolution  

E-Print Network (OSTI)

In this review, I will discuss a few problems which point to the need for improved stellar evolution models of halo stars. Current stellar evolution models do not match the observed $^7$Li abundance patterns, suggesting that the input physics and/or the assumptions used in constructing the models are in need of revision. It appears that all halo stars have suffered some $^7$Li depletion, implying that the primordial $^7$Li abundance is higher than that presently observed in hot halo stars. Observations of abundances of various elements in globular cluster giant branch stars have suggested for some time now that some form of deep mixing, which is not present in theoretical models, occurs in halo stars. The driving mechanism for this mixing, and its incorporation into stellar models remain one of the key problems in stellar modeling. Current theoretical isochrones are able to provide a good match to observed colour-magnitude diagrams. However, there is some evidence that the theoretical luminosity functions are in disagreement with observations. This is an area which requires further study, as it suggests that the relative main sequence/giant branch lifetimes predicted by the models are incorrect. A discussion of some of the uncertainties involved in determining the ages of globular clusters is presented. The absolute ages of globular clusters provide a lower bound to the age of the universe, and so are of great interest to cosmologists. Unfortunately, present uncertainties in stellar models lead to a rather large range in the inferred ages of globular clusters of 11 -- 18 Gyr.

Brian Chaboyer

1995-09-08T23:59:59.000Z

272

Shape memory alloy thaw sensors  

SciTech Connect

A sensor permanently indicates that it has been exposed to temperatures exceeding a critical temperature for a predetermined time period. An element of the sensor made from shape memory alloy changes shape when exposed, even temporarily, to temperatures above the austenitic temperature of the shape memory alloy. The shape change of the SMA element causes the sensor to change between two readily distinguishable states. 16 figs.

Shahinpoor, M.; Martinez, D.R.

1998-04-07T23:59:59.000Z

273

ENERGY STAR Success Story Mark Twain House Museum  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Success Story: ENERGY STAR Success Story: Mark Twain House & Museum Built in 1874, the Mark Twain House & Museum is considered one of the premier tourist attractions in the State of Connecticut. This 19-room Victorian home changed owners numerous times before the Mark Twain Memorial and Library Commission, a non-profit organization chartered by the State of Connecticut, purchased and restored the house in 1929 for historical and educational purposes. The Museum comprises the 12,298-square-foot Main House (the historic house of Mark Twain) and the 4,935-square- foot Carriage House (the location of all staff offices). The state-of-the-art 33,000-square-foot Museum Center was added in 2003, thrusting the Mark Twain House & Museum into the 21 st Century. The Main

274

The MACHO Project LMC Variable Star Inventory Classical Cepheids, AGB Variables, and the 9 Million Star Color-Magnitude Diagram  

E-Print Network (OSTI)

We measure the ratio of ~5 M_solar blue and red LMC supergiants (representative of classical Cepheids) using the MACHO Project's 9 million star color-magnitude diagram (9M CMD) of the LMC bar. We find b/r = 0.39, which favors the z=0.008, 5 M_solar theoretical model of Schaerer et al.(1993) over that of Fagatto et al. (1994). Next, we examine the low mass (old) and low metallicity LMC field population (Pop. II). Features in the 9M CMD and properties of LMC field RRab are consistent with a mean iron abundance of [Fe/H] = -1.5 dex for this population. Newly discovered post-HB/early-AGB Pop. II variables are identified in order to delineate the instability strip (IS). Good agreement with the theoretical IS of Bono et al. (1997) is found. We then compare the field RRab with newly identified RRab variables in the LMC clusters NGC 1898 and NGC 1835. We find the mean colors of these cluster RRab lie near the red and blue edges of the IS, respectively, which is similar to their respective (overall) red and blue HB mo...

Alves, D R; Cook, K H; Welch, D L; Alcock, C B; Marshall, S; Axelrod, T S; Drake, A; Freeman, K C; Peterson, B M; Allsman, R A; Becker, A; Tomaney, A B; Griest, K; Vandehei, T; Lehner, M; Bennett, D; Minniti, D; Pratt, M; Sutherland, W; Quinn, P

1998-01-01T23:59:59.000Z

275

Cerenkov radiation and scalar stars  

E-Print Network (OSTI)

We explore the possibility that a charged particle moving in the gravitational field generated by a scalar star could radiate energy via a recently proposed gravitational \\v{C}erenkov mechanism. We numerically prove that this is not possible for stable boson stars. We also show that soliton stars could have \\v{C}erenkov radiation for particular values of the boson mass, although diluteness of the star grows and actual observational possibility decreases for the more usually discussed boson masses. These conclusions diminish, although do not completely rule out, the observational possibility of actually detecting scalar stars using this mechanism, and lead us to consider other forms, like gravitational lensing.

S. Capozziello; G. Lambiase; Diego F. Torres

2000-06-23T23:59:59.000Z

276

The H II Region of a Primordial Star  

DOE Green Energy (OSTI)

The concordance model of cosmology and structure formation predicts the formation of isolated very massive stars at high redshifts in dark matter dominated halos of 10{sup 5} to 10{sup 6} Msun. These stars photo-ionize their host primordial molecular clouds, expelling all the baryons from their halos. When the stars die, a relic H II region is formed within which large amounts of molecular hydrogen form which will allow the gas to cool efficiently when gravity assembles it into larger dark matter halos. The filaments surrounding the first star hosting halo are largely shielded and provide the pathway for gas to stream into the halo when the star has died. We present the first fully three dimensional cosmological radiation hydrodynamical simulations that follow all these effects. A novel adaptive ray casting technique incorporates the time dependent radiative transfer around point sources. This approach is fast enough so that radiation transport, kinetic rate equations, and hydrodynamics are solved self-consistently. It retains the time derivative of the transfer equation and is explicitly photon conserving. This method is integrated with the cosmological adaptive mesh refinement code enzo, and runs on distributed and shared memory parallel architectures. Where applicable the three dimensional calculation not only confirm expectations from earlier one dimensional results but also illustrate the multi-fold hydrodynamic complexities of H II regions. In the absence of stellar winds the circumstellar environments of the first supernovae and putative early gamma-ray bursts will be of low density {approx}1 cm{sup -3}. Albeit marginally resolved, ionization front instabilities lead to cometary and elephant trunk like small scale structures reminiscent of nearby star forming regions.

Abel, Tom; Wise, John H.; /KIPAC, Menlo Park; Bryan, Greg L.; /Columbia U., Astron. Astrophys.

2006-06-07T23:59:59.000Z

277

Energy Star | Open Energy Information  

Open Energy Info (EERE)

Star Star Jump to: navigation, search Energystarlogo.jpg Contents 1 What's new 2 About ENERGY STAR 3 For the Home 4 For Business 5 History 6 References What's new On March 15, 2012, the EPA released a press release announcing 2012's ENERGY STAR award winners, and celebrating the 20 year anniversary of the award. Overall, the EPA estimates that American's have saved nearly $230 billion over two decades of the award. About ENERGY STAR ENERGY STAR is a joint program of the United States Environmental Protection Agency and the United States Department of Energy helping us all save money and protect the environment through energy efficient products and practices. Results are already adding up. Americans, with the help of ENERGY STAR, saved enough energy in 2009 alone to avoid greenhouse gas emissions

278

Energy efficient Phase Change Memory based main memory for future high performance systems  

Science Conference Proceedings (OSTI)

Phase Change Memory (PCM) has recently attracted a lot of attention as a scalable alternative to DRAM for main memory systems. As the need for high-density memory increases, DRAM has proven to be less attractive from the point of view of scaling and ... Keywords: DDR3 commodity DRAM memory system, energy efficient phase change memory, main memory, future high performance systems, energy consumption, latency issues, write energy, write endurance, cache, embedded DRAM

R. A. Bheda; Jason A. Poovey; J. G. Beu; T. M. Conte

2011-07-01T23:59:59.000Z

279

Effect of memory access and caching on high performance computing.  

E-Print Network (OSTI)

??High-performance computing is often limited by memory access. As speeds increase, processors are often waiting on data transfers to and from memory. Classic memory controllers (more)

Groening, James

2012-01-01T23:59:59.000Z

280

Direct-Current Resistivity Survey At Blue Mountain Area (Fairbank  

Open Energy Info (EERE)

5) 5) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Direct-Current Resistivity Survey At Blue Mountain Area (Fairbank Engineering, 2005) Exploration Activity Details Location Blue Mountain Area Exploration Technique Direct-Current Resistivity Survey Activity Date Usefulness not indicated DOE-funding Unknown Notes Geophysical surveys that have been conducted specifically for the geothermal program at Blue Mountain include a self-potential (SP) survey, and additional IP/electrical resistivity traversing. These surveys were conducted under a cooperative program between Noramex Corporation and the Energy and Geosciences Institute (EGI), University of Utah, with funding support from the DOE's Office of Geothermal Technology (DOE/OGT).

Note: This page contains sample records for the topic "blue star memorial" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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281

SeaStar Unchained: Multiplying the Performance of the Cray SeaStar Network  

SciTech Connect

The Oak Ridge Leadership Computing Facility (OLCF) supports many different systems and many differ- ent interconnects. The only common programming interfaces across these systems are BSD Sockets and MPI. Due to the design assumptions such as implicit buffering leading to extra copies, Sockets performance is almost universally lower than the native interface. Even in the cases that Sockets provides similar bandwidth as the native interface, it suffers from excessive CPU usage. MPI is the de-facto interface for intra- job communication, but is difficult to use between jobs and provides no ability to communicate with service nodes or off- system nodes (e.g. for I/O forwarding). We have developed the Common Communication Interface (CCI), a programming interface that exposes the advances in interconnect hardware, notably Remote Direct Memory Access (RDMA) and operating system (OS) bypass, while imposing as little overhead as possible. This API directly supports inter-job as well as off- system communication. CCI is a lightweight abstraction layer that provides point-to-point messaging and remote memory access. The Cray SeaStar ASIC, with its programmable embedded processor, provides an excellent platform to investigate the properties of various network protocols and programming interfaces. This paper describes our native implementation CCI on the SeaStar platform, and details how we implemented full OS bypass for common operations. We demonstrate a 30% to 50% reduction in latency, more than a six-fold increase in message injection rate, and an almost 7x improvement in bandwidth for small message sizes when compared to the generic Cray Portals implementation.

Dillow, David A [ORNL; Atchley, Scott [ORNL

2013-01-01T23:59:59.000Z

282

What Scientific Applications can Benefit from Hardware Transactional Memory?  

Science Conference Proceedings (OSTI)

Achieving efficient and correct synchronization of multiple threads is a difficult and error-prone task at small scale and, as we march towards extreme scale computing, will be even more challenging when the resulting application is supposed to utilize millions of cores efficiently. Transactional Memory (TM) is a promising technique to ease the burden on the programmer, but only recently has become available on commercial hardware in the new Blue Gene/Q system and hence the real benefit for realistic applications has not been studied, yet. This paper presents the first performance results of TM embedded into OpenMP on a prototype system of BG/Q and characterizes code properties that will likely lead to benefits when augmented with TM primitives. We first, study the influence of thread count, environment variables and memory layout on TM performance and identify code properties that will yield performance gains with TM. Second, we evaluate the combination of OpenMP with multiple synchronization primitives on top of MPI to determine suitable task to thread ratios per node. Finally, we condense our findings into a set of best practices. These are applied to a Monte Carlo Benchmark and a Smoothed Particle Hydrodynamics method. In both cases an optimized TM version, executed with 64 threads on one node, outperforms a simple TM implementation. MCB with optimized TM yields a speedup of 27.45 over baseline.

Schindewolf, M; Bihari, B; Gyllenhaal, J; Schulz, M; Wang, A; Karl, W

2012-06-04T23:59:59.000Z

283

Detector limitations, STAR  

Science Conference Proceedings (OSTI)

Every detector has limitations in terms of solid angle, particular technologies chosen, cracks due to mechanical structure, etc. If all of the presently planned parts of STAR [Solenoidal Tracker At RHIC] were in place, these factors would not seriously limit our ability to exploit the spin physics possible in RHIC. What is of greater concern at the moment is the construction schedule for components such as the Electromagnetic Calorimeters, and the limited funding for various levels of triggers.

Underwood, D. G.

1998-07-13T23:59:59.000Z

284

Stable dark energy stars  

E-Print Network (OSTI)

The gravastar picture is an alternative model to the concept of a black hole, where there is an effective phase transition at or near where the event horizon is expected to form, and the interior is replaced by a de Sitter condensate. In this work, a generalization of the gravastar picture is explored, by considering a matching of an interior solution governed by the dark energy equation of state, $\\omega\\equiv p/ \\rhosolution at a junction interface. The motivation for implementing this generalization arises from the fact that recent observations have confirmed an accelerated cosmic expansion, for which dark energy is a possible candidate. Several relativistic dark energy stellar configurations are analyzed by imposing specific choices for the mass function. The first case considered is that of a constant energy density, and the second choice, that of a monotonic decreasing energy density in the star's interior. The dynamical stability of the transition layer of these dark energy stars to linearized spherically symmetric radial perturbations about static equilibrium solutions is also explored. It is found that large stability regions exist that are sufficiently close to where the event horizon is expected to form, so that it would be difficult to distinguish the exterior geometry of the dark energy stars, analyzed in this work, from an astrophysical black hole.

Francisco S. N. Lobo

2005-08-28T23:59:59.000Z

285

Task Force for Strategic Developments to Blue Ribbon Commission  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Task Force for Strategic Developments to Blue Ribbon Commission Task Force for Strategic Developments to Blue Ribbon Commission Recommendations Task Force for Strategic Developments to Blue Ribbon Commission Recommendations Formed at the direction of the President to Secretary Chu and included leading experts. Purpose to conduct a comprehensive review of polices for managing the back end of the nuclear fuel cycle; i.e., recycle before storage and permanent disposal. Detailed analysis, with eight major recommendations; also recommended near-term actions. Task Force for Strategic Developments to Blue Ribbon Commission Recommendations More Documents & Publications Categorization of Used Nuclear Fuel Inventory in Support of a Comprehensive National Nuclear Fuel Cycle Strategy DOE Office of Nuclear Energy Transportation Planning, Route Selection, and

286

Epithermal Gold Mineralization and a Geothermal Resource at Blue Mountain,  

Open Energy Info (EERE)

Epithermal Gold Mineralization and a Geothermal Resource at Blue Mountain, Epithermal Gold Mineralization and a Geothermal Resource at Blue Mountain, Humboldt County, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Epithermal Gold Mineralization and a Geothermal Resource at Blue Mountain, Humboldt County, Nevada Abstract Shallow exploration drilling on the west flank of Blue Mountain discovered sub economic gold mineralization and a spatially associated active geothermal system. The gold mineralization is an unusual example of an acid sulfate type epithermal system developed in pre Tertiary sedimentary host rocks. The geothermal system is largely unexplored but is unusual in that surface manifestation s typically associated with active geothermal system are not present. Authors Andrew J. Parr and Timothy J. Percival

287

USD 384 Blue Valley Wind Project | Open Energy Information  

Open Energy Info (EERE)

Blue Valley Wind Project Blue Valley Wind Project Jump to: navigation, search Name USD 384 Blue Valley Wind Project Facility USD 384 Blue Valley Sector Wind energy Facility Type Community Wind Location KS Coordinates 39.433575°, -96.758011° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.433575,"lon":-96.758011,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

288

Geothermal Drilling Success at Blue Mountain, Nevada | Open Energy  

Open Energy Info (EERE)

Drilling Success at Blue Mountain, Nevada Drilling Success at Blue Mountain, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Conference Paper: Geothermal Drilling Success at Blue Mountain, Nevada Abstract Exploration in a blind prospect has led to the confirmation of a geothermal resource at Blue Mt.Nevada. The latest results include drilling of three production wells into Piedmont faults. These wells produce from a 185 to 190°C dilute benign brine reservoir. Short flow tests have shown prolific flow rates and indications of reservoir continuity.Well entries have shown that system permeability is fault-dominated. This is confirmed by the results of seismic reflection imaging. Young faulting in the area includes intersecting range front faults that strike NW, NS, and NE. Exposure of

289

Aeromagnetic Survey At Blue Mountain Area (Fairbank Engineering, 2003) |  

Open Energy Info (EERE)

Blue Mountain Area (Fairbank Blue Mountain Area (Fairbank Engineering, 2003) Exploration Activity Details Location Blue Mountain Area Exploration Technique Aeromagnetic Survey Activity Date Usefulness not indicated DOE-funding Unknown Notes The airborne magnetometer and VLF-EM surveys carried out by Aerodat Limited, in 1988, covered the western flank of Blue Mountain including most of the geothermal lease area. The interpreted data (total field magnetic contours; calculated vertical magnetic gradient) indicate parallel sets of northerly, northeasterly, and northwesterly-trending structures that correspond well with the major fault sets identified from geologic mapping and interpreted drilling sections. Also, an elongate northerly-trending area of low magnetic gradient coincides closely with the area of intense

290

MHK Technologies/Blue Motion Energy marine turbine | Open Energy  

Open Energy Info (EERE)

Motion Energy marine turbine Motion Energy marine turbine < MHK Technologies Jump to: navigation, search << Return to the MHK database homepage Blue Motion Energy marine turbine.jpg Technology Profile Primary Organization Blue Motion Energy Technology Resource Click here Current Technology Type Click here Cross Flow Turbine Technology Description The Blue Motion Energy marine turbine however uses a patented system of seawalls A placed radial around the vertically mounted rotor B this way it is possible to funnel the current and significantly increase the flow velocity independent of the direction of the current Technology Dimensions Device Testing Date Submitted 59:30.2 << Return to the MHK database homepage Retrieved from "http://en.openei.org/w/index.php?title=MHK_Technologies/Blue_Motion_Energy_marine_turbine&oldid=681547

291

Geology and Temperature Gradient Surveys Blue Mountain Geothermal  

Open Energy Info (EERE)

Geology and Temperature Gradient Surveys Blue Mountain Geothermal Geology and Temperature Gradient Surveys Blue Mountain Geothermal Discovery, Humboldt County, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Geology and Temperature Gradient Surveys Blue Mountain Geothermal Discovery, Humboldt County, Nevada Abstract Triassic argillite and sandstone of the Grass Valley Formation and phyllitic mudstone of the overlying Raspberry Formation, also of Triassic age, host a blind geothermal system under exploration by Blue Mountain Power Company Inc. with assistance from the Energy & Geoscience Institute. Geologically young, steeply dipping, open fault sets, striking N50-60°E,N50-60°W, and N-S intersect in the geothermal zone providing deep permeability over a wide area. Extensive silicification andhydro

292

Secretary Chu Announces Blue Ribbon Commission on America's Nuclear  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Blue Ribbon Commission on America's Blue Ribbon Commission on America's Nuclear Future Secretary Chu Announces Blue Ribbon Commission on America's Nuclear Future January 29, 2010 - 12:57pm Addthis As part of the Obama Administration's commitment to restarting America's nuclear industry, U.S. Secretary of Energy Steven Chu today announced the formation of a Blue Ribbon Commission on America's Nuclear Future to provide recommendations for developing a safe, long-term solution to managing the Nation's used nuclear fuel and nuclear waste. The Commission is being co-chaired by former Congressman Lee Hamilton and former National Security Advisor Brent Scowcroft. In light of the Administration's decision not to proceed with the Yucca Mountain nuclear waste repository, President Obama has directed Secretary

293

Blue Ridge Electric Cooperative - Heat Pump Loan Program | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

You are here You are here Home » Blue Ridge Electric Cooperative - Heat Pump Loan Program Blue Ridge Electric Cooperative - Heat Pump Loan Program < Back Eligibility Residential Savings Category Heating & Cooling Commercial Heating & Cooling Heat Pumps Maximum Rebate 12,000 Program Info State South Carolina Program Type Utility Loan Program Rebate Amount $500 - $12,000 Provider Blue Ridge Electric Cooperative Blue Ridge Electric Cooperative (BREC) offers low interest loans to help members finance the purchase of energy efficient heat pumps. Loans under $1,500 can be financed for up to 42 months, and loans above $1,500 can be financed for up to 60 months for houses and 48 months for mobile homes. Homeowners planning to install one heat pump, electric or geothermal can

294

Reflection Survey At Blue Mountain Area (Fairbank Engineering, 2007) | Open  

Open Energy Info (EERE)

Blue Mountain Area (Fairbank Engineering, 2007) Blue Mountain Area (Fairbank Engineering, 2007) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Reflection Survey At Blue Mountain Area (Fairbank Engineering, 2007) Exploration Activity Details Location Blue Mountain Area Exploration Technique Reflection Survey Activity Date Usefulness useful DOE-funding Unknown Notes A high-resolution seismic reflection survey was conducted by Utah Geophysical, Inc. (1990) along four widely spaced survey lines normal to range front fault sets. The survey was designed primarily to detect silicified zones or zones of argillic alteration, and faulting, to depths of about 300 meters (1000 feet), as part of the precious metals exploration program. One interpretation of the data showed discrete, high-angle faults

295

Secretary Chu Announces Blue Ribbon Commission on America's Nuclear Future  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Blue Ribbon Commission on America's Nuclear Blue Ribbon Commission on America's Nuclear Future Secretary Chu Announces Blue Ribbon Commission on America's Nuclear Future January 29, 2010 - 12:00am Addthis Washington, D.C. - As part of the Obama Administration's commitment to restarting America's nuclear industry, U.S. Secretary of Energy Steven Chu today announced the formation of a Blue Ribbon Commission on America's Nuclear Future to provide recommendations for developing a safe, long-term solution to managing the Nation's used nuclear fuel and nuclear waste. The Commission is being co-chaired by former Congressman Lee Hamilton and former National Security Advisor Brent Scowcroft. In light of the Administration's decision not to proceed with the Yucca Mountain nuclear waste repository, President Obama has directed Secretary

296

Task Force for Strategic Developments to Blue Ribbon Commission  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Task Force for Strategic Developments to Blue Ribbon Commission Task Force for Strategic Developments to Blue Ribbon Commission Recommendations Task Force for Strategic Developments to Blue Ribbon Commission Recommendations Formed at the direction of the President to Secretary Chu and included leading experts. Purpose to conduct a comprehensive review of polices for managing the back end of the nuclear fuel cycle; i.e., recycle before storage and permanent disposal. Detailed analysis, with eight major recommendations; also recommended near-term actions. Task Force for Strategic Developments to Blue Ribbon Commission Recommendations More Documents & Publications DOE Office of Nuclear Energy Transportation Planning, Route Selection, and Rail Issues Categorization of Used Nuclear Fuel Inventory in Support of a Comprehensive

297

FERN Blue Ribbon Wind Farm I | Open Energy Information  

Open Energy Info (EERE)

FERN Blue Ribbon Wind Farm I FERN Blue Ribbon Wind Farm I Jump to: navigation, search Name FERN Blue Ribbon Wind Farm I Facility FERN Blue Ribbon Wind Farm I Sector Wind energy Facility Type Offshore Wind Facility Status Proposed Developer Fishermen's Energy Location Offshore from Atlantic City NJ Coordinates 39.311°, -74.41° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.311,"lon":-74.41,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

298

IBM Blue Gene Parallel Supercomputer, Brookhaven National Laboratory...  

NLE Websites -- All DOE Office Websites (Extended Search)

SSH Tunneling One-hop logins and file transfers using ssh tunneling Please note, New York BlueL has been decommissioned and these web pages have not yet been updated to reflect...

299

Second Generation Renewable Fuels Blue-Green Seminar  

E-Print Network (OSTI)

Abstract Second Generation Renewable Fuels Blue-Green Seminar at University of Michigan by Michael Ladisch Laboratory of Renewable Resources Engineering Purdue University Potter Engineering Center 500 footprint will require commercialization of industrial processes that transform renewable lignocellulosic

Eustice, Ryan

300

A disposable biosensor with Prussian blue deposited electrode  

Science Conference Proceedings (OSTI)

We propose a novel electrochemical detector (ECD) to catalyze redox efficiently by electrodepositing Prussian blue (PB, ferric hexacyanoferrate) on the indium tin oxide (ITO) electrode. Capillary electrophoresis (CE) and amperometric methods were used. ... Keywords: Amperometric, Biosensor, Catecchol, Dopamine, ITO

In-Je Yi; Ju-Ho Kim; Y. J. Choi; C. J. Kang; Yong-Sang Kim

2006-04-01T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

NETL: News Release - NETL Receives Blue Pencil and Gold Screen...  

NLE Websites -- All DOE Office Websites (Extended Search)

The honor was awarded at the NAGC Blue Pencil and Gold Screen Awards Reception and Banquet on Monday, May 17,2010, in Bethesda, Md., during the 2010 NAGC Communications School....

302

Blue-green and green phosphors for lighting applications  

Science Conference Proceedings (OSTI)

Embodiments of the present techniques provide a related family of phosphors that may be used in lighting systems to generate blue or blue-green light. The phosphors include systems having a general formula of: ((Sr.sub.1-zM.sub.z).sub.1-(x+w)A.sub.wCe.sub.x).sub.3(Al.sub.1-ySi.s- ub.y)O.sub.4+y+3(x-w)F.sub.1-y-3(x-w) (I), wherein 0lighting systems, such as LEDs and fluorescent tubes, among others, to produce blue and blue/green light. Further, the phosphors may be used in blends with other phosphors, or in combined lighting systems, to produce white light suitable for illumination.

Setlur, Anant Achyut; Chandran, Ramachandran Gopi; Henderson, Claire Susan; Nammalwar, Pransanth Kumar; Radkov, Emil

2012-12-11T23:59:59.000Z

303

REFERENCE: The Blue Planet An Introduction to Earth System  

E-Print Network (OSTI)

REFERENCE: The Blue Planet An Introduction to Earth System Science. Brian J. Skinner and Barbara Glacier E. Piedmont Glaciers #12;A. Cirque glaciers occupies a bowl shape depression on a mountainside

Gilbes, Fernando

304

Highly efficient blue polyfluorene-based polymer light-emitting...  

NLE Websites -- All DOE Office Websites (Extended Search)

of Physics Volume 42 Pagination 5 Abstract A highly efficient blue polymer light-emitting diode based on poly(9,9-di(2-(2-(2-methoxy-ethoxy)ethoxy)ethyl)fluorenyl-2,7-diyl)...

305

Blue Peter Project Group Inc | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Name Blue Peter Project Group Inc Place Oakville, Ontario, Canada Zip L6M 2B8 Sector Solar Product Alternative energy project developer in Canada,...

306

Find an ENERGY STAR service and product provider | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Find an ENERGY STAR service and product provider Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial...

307

Bring Your Green to Work with ENERGY STAR | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Bring Your Green to Work with ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

308

Celebrating a Decade of ENERGY STAR Buildings | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Celebrating a Decade of ENERGY STAR Buildings Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

309

Win ENERGY STAR Partner of the Year | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Win ENERGY STAR Partner of the Year Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

310

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR National Building Competition Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

311

How can ENERGY STAR help your business? | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR help your business? Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

312

ENERGY STAR Success Story: HEI Hotels & Resorts | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Story: HEI Hotels & Resorts HEI Hotels & Resorts is a growing hospitality company with 30 hotel properties in 13 states. Since launching its partnership with ENERGY STAR in 2006,...

313

Verify applications for ENERGY STAR certification | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Verify applications for ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial...

314

Join the ENERGY STAR Small Business Network | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Join the ENERGY STAR Small Business Network Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

315

Spectral signatures of photosynthesis II: coevolution with other stars and the atmosphere on extrasolar worlds  

E-Print Network (OSTI)

As photosynthesis on Earth produces the primary signatures of life that can be detected astronomically at the global scale, a strong focus of the search for extrasolar life will be photosynthesis, particularly photosynthesis that has evolved with a different parent star. We take planetary atmospheric compositions simulated by Segura, et al. (2003, 2005) for Earth-like planets around observed F2V and K2V stars, modeled M1V and M5V stars, and around the active M4.5V star AD Leo; our scenarios use Earth's atmospheric composition as well as very low O2 content in case anoxygenic photosynthesis dominates. We calculate the incident spectral photon flux densities at the surface of the planet and under water. We identify bands of available photosynthetically relevant radiation and find that photosynthetic pigments on planets around F2V stars may peak in absorbance in the blue, K2V in the red-orange, and M stars in the NIR, in bands at 0.93-1.1 microns, 1.1-1.4 microns, 1.5-1.8 microns, and 1.8-2.5 microns. In additio...

Kiang, N Y; Tinetti, G; Blankenship, R E; Cohen, M; Siefert, J; Crisp, D; Meadows, V S; Kiang, Nancy Y.; Segura, Antigona; Tinetti, Giovanna; Blankenship, Robert E.; Cohen, Martin; Siefert, Janet; Crisp, David; Meadows, Victoria S.

2007-01-01T23:59:59.000Z

316

Blue Breezes I & II Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Blue Breezes I & II Wind Farm Blue Breezes I & II Wind Farm Jump to: navigation, search Name Blue Breezes I & II Wind Farm Facility Blue Breezes I & II Sector Wind energy Facility Type Community Wind Facility Status In Service Owner John Deere Wind Energy Developer Dan Moore/John Deere Wind Energy Energy Purchaser City of Blue Earth Location City of Blue Earth MN Coordinates 43.6352°, -94.0942° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.6352,"lon":-94.0942,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

317

ENERGY STAR SNAPSHOT - Spring 2009  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 Snapshot data runs through June 30, 2010. Summary By mid-year 2010, commercial and industrial organizations have almost exceeded activity levels reached throughout all of 2009. From January through June 30, 2010: More than 80,000 buildings have benchmarked their energy usage with ENERGY STAR, of which 63,000 buildings received an ENERGY STAR energy performance score-nearly equivalent to the amount for all of 2009. Close to 3,200 buildings earned the ENERGY STAR label-the highest amount earned through two quarters of any year, and 80% higher than mid-year 2009. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is

318

ENERGY STAR EEPS Partnership Agreement  

NLE Websites -- All DOE Office Websites (Extended Search)

Approval expires 02/29/2016 1 EPA Form No. 5900-33 ENERGY STAR Partnership Agreement Instructions for Partnering with ENERGY STAR ® As an Energy Efficiency Program Sponsor Organizations interested in partnering with ENERGY STAR as an Energy Efficiency Program Sponsor should take the following steps: 1. Review the Energy Efficiency Program Sponsors Program Definitions and Program Requirements documents. 2. Select the area(s) of interest for a new partnership on the Participation Form. Please

319

An infrared study of galactic OH/IR stars. II. The `GLMP sample' of red oxygen-rich AGB stars  

E-Print Network (OSTI)

We present optical and near-infrared finding charts taken from the DSS and 2MASS surveys of 94 IRAS sources selected from the GLMP catalogue (Garc\\'{\\i}a-Lario 1992), and accurate astrometry (~0.2") for most of them. Selection criteria were very red IRAS colours representative for OH/IR stars with optically thick circumstellar shells and the presence of variability according to the IRAS variability index (VAR>50). The main photometric properties of the stars in this `GLMP sample' are presented, discussed and compared with the correspondent properties of the `Arecibo sample' of OH/IR stars studied in Jim\\'enez-Esteban et al. (2005a). We find that 37% of the sample (N=34) have no counterpart in the 2MASS, implying extremely high optical depths of their shells. Most of the sources identified in the 2MASS are faint (K>~8) and of very red colour in the near-infrared, as expected. The brightest 2MASS counterpart (K=5.3mag) was found for IRAS 18299--1705. Its blue colour H--K=1.3 suggests that IRAS 8299--1705 is a p...

Jimnez-Esteban, F M; Engels, D; Caldern, J V P

2005-01-01T23:59:59.000Z

320

Ralph H. Potts Memorial Fellowship Award  

Science Conference Proceedings (OSTI)

Awarded to a graduate student doing research in fats and oils. Ralph H. Potts Memorial Fellowship Award Awards Program achievement aocs application award Awards baldwin distinguished division memorial nomination poster program recognizing research

Note: This page contains sample records for the topic "blue star memorial" 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

Snapshot (Fall 2009) | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

322

Snapshot (Spring 2009) | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

323

Snapshot (Fall 2008) | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

324

Snapshot (Spring 2008) | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

325

A Mosque Among the Stars  

E-Print Network (OSTI)

A Mosque Among The Stars was the first anthology that dealt with the subject of Muslim characters and/or Islamic themes and Science Fiction.

Ahmad, Muhammad Aurangzeb; Khan, Ahmad

2007-01-04T23:59:59.000Z

326

Snapshot (Spring 2012) | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

resources Small business resources State and local government resources Snapshot (Spring 2012) The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance...

327

Building Technologies Program: ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

with ENERGY STAR DOE conducts research, development, and deployment to improve the energy efficiency of existing homes using a whole-building approach, which results in the...

328

Industries in focus | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Energy Performance Indicators for plants Industries in focus Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers...

329

Plant energy auditing | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

330

Improve energy performance | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

331

ENERGY STAR Petroleum Energy Guide  

NLE Websites -- All DOE Office Websites (Extended Search)

183 ERNEST ORLANDO LAWRENCE BERKELEY NATIONAL LABORATORY Energy Efficiency Improvement and Cost Saving Opportunities For Petroleum Refineries An ENERGY STAR Guide for Energy and...

332

Energy Star Building Upgrade Manual  

NLE Websites -- All DOE Office Websites (Extended Search)

program helping businesses and individuals fight global warming through superior energy efficiency. ENERGY STAR Building Upgrade Manual United States Environmental Protection...

333

Portable Data loggers | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

short list of companies that sell the products. Download more information about Portable Data Loggers here. Energy Efficient Products Learn about ENERGY STAR Products Save Energy...

334

Chapter 5: Virtual Memory Management 1 Virtual Memory Management  

E-Print Network (OSTI)

kernel data structures. The zone package This package facilitates fast allocation of memory for kernel data structures, some of which may be in time critical pieces of code. The zone package provides, organization, data structures, interactions. The emphasis is laid on both ma- chine dependent portion

Melbourne, University of

335

Available Technologies:Collective Memory Transfers for ...  

APPLICATIONS OF TECHNOLOGY: High Performance Computing (HPC) Big Data processing and analysis; Processor manufacturers; Memory module manufacturers

336

Battelle Memorial Institute Technology Marketing Summaries ...  

... applications and industries, and development stage. Battelle Memorial ... Typical existing armor for vehicles uses rigid plates of steel.

337

NIST Demonstrates Better Memory with Quantum Computer ...  

Science Conference Proceedings (OSTI)

... to demonstrate a quantum physics version of computer memory lasting ... prospects for making practical, reliable quantum computers (which make ...

2013-01-03T23:59:59.000Z

338

Thermal Gradient Holes At Blue Mountain Area (Fairbank & Neggemann, 2004) |  

Open Energy Info (EERE)

Blue Mountain Area (Fairbank & Neggemann, 2004) Blue Mountain Area (Fairbank & Neggemann, 2004) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Thermal Gradient Holes At Blue Mountain Area (Fairbank & Neggemann, 2004) Exploration Activity Details Location Blue Mountain Area Exploration Technique Thermal Gradient Holes Activity Date Usefulness useful DOE-funding Unknown References Brian D. Fairbank, Kim V. Niggemann (2004) Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt County, Nevada Retrieved from "http://en.openei.org/w/index.php?title=Thermal_Gradient_Holes_At_Blue_Mountain_Area_(Fairbank_%26_Neggemann,_2004)&oldid=386709" Category: Exploration Activities What links here Related changes Special pages Printable version Permanent link

339

TRIGGERED STAR FORMATION SURROUNDING WOLF-RAYET STAR HD 211853  

SciTech Connect

The environment surrounding Wolf-Rayet (W-R) star HD 211853 is studied in molecular, infrared, as well as radio, and H I emission. The molecular ring consists of well-separated cores, which have a volume density of 10{sup 3} cm{sup -3} and kinematic temperature {approx}20 K. Most of the cores are under gravitational collapse due to external pressure from the surrounding ionized gas. From the spectral energy distribution modeling toward the young stellar objects, the sequential star formation is revealed on a large scale in space spreading from the W-R star to the molecular ring. A small-scale sequential star formation is revealed toward core 'A', which harbors a very young star cluster. Triggered star formations are thus suggested. The presence of the photodissociation region, the fragmentation of the molecular ring, the collapse of the cores, and the large-scale sequential star formation indicate that the 'collect and collapse' process functions in this region. The star-forming activities in core 'A' seem to be affected by the 'radiation-driven implosion' process.

Liu Tie; Wu Yuefang; Zhang Huawei [Department of Astronomy, Peking University, 100871 Beijing (China); Qin Shengli, E-mail: liutiepku@gmail.com [I. Physikalisches Institut, Universitaet zu Koeln, Zuelpicher Str. 77, 50937 Koeln (Germany)

2012-05-20T23:59:59.000Z

340

Stepout-Deepening Wells At Blue Mountain Area (Niggemann Et Al, 2005) |  

Open Energy Info (EERE)

Blue Mountain Area (Niggemann Et Al, 2005) Blue Mountain Area (Niggemann Et Al, 2005) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Step-out Well At Blue Mountain Area (Niggemann Et Al, 2005) Exploration Activity Details Location Blue Mountain Area Exploration Technique Step-out Well Activity Date Usefulness not indicated DOE-funding Unknown Notes Deep Blue No. 2 was sited as a step out t5 meters.5o Deep Blue No. 1 which measured 145oC at a depth of 645 m. Max temp recorded in Deep Blue No. 2 while drilling was 167.5oC at References Kim Niggemann, Brian Fairbank, Susan Petty (2005) Deep Blue No 2- A Resource In The Making At Blue Mountain Retrieved from "http://en.openei.org/w/index.php?title=Stepout-Deepening_Wells_At_Blue_Mountain_Area_(Niggemann_Et_Al,_2005)&oldid=687863"

Note: This page contains sample records for the topic "blue star memorial" 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.


341

Shape memory polymer foams for endovascular therapies  

DOE Patents (OSTI)

A system for occluding a physical anomaly. One embodiment comprises a shape memory material body wherein the shape memory material body fits within the physical anomaly occluding the physical anomaly. The shape memory material body has a primary shape for occluding the physical anomaly and a secondary shape for being positioned in the physical anomaly.

Wilson, Thomas S. (Castro Valley, CA); Maitland, Duncan J. (Pleasant Hill, CA)

2012-03-13T23:59:59.000Z

342

Specifying memory consistency of write buffer multiprocessors  

Science Conference Proceedings (OSTI)

Write buffering is one of many successful mechanisms that improves the performance and scalability of multiprocessors. However, it leads to more complex memory system behavior, which cannot be described using intuitive consistency models, such as Sequential ... Keywords: Memory consistency framework, alpha, coherence, partial store order, relaxed memory order, sequential consistency, sparc multiprocessors, total store order, write-buffer architectures

Lisa Higham; Lillanne Jackson; Jalal Kawash

2007-02-01T23:59:59.000Z

343

Multistable Circuits for Analog Memories Implementation  

Science Conference Proceedings (OSTI)

In this work two multistable circuits suitable for analog memories implementation will be presented. These circuits have been used to implement completely asynchronous analog memories, one type based on a flash converter and thus having a linear complexity ... Keywords: analog memories, asynchronous converters, successive approximations

Giorgio Biagetti; Massimo Conti; Simone Orcioni

2004-04-01T23:59:59.000Z

344

The Tempest approach to distributed shared memory  

Science Conference Proceedings (OSTI)

This paper summarizes how distributed shared memory (DSM) can be both efficiently and portably supported by the Tempest interface. Tempest is a collection of mechanisms for communication and synchronization in parallel programs. These mechanisms provide ... Keywords: Tempest, Tempest interface, distributed shared memory, message passing, parallel programs, shared memory

David A. Wood; Mark D. Hill; James R. Larus

1996-10-01T23:59:59.000Z

345

Algorithms and data structures for external memory  

Science Conference Proceedings (OSTI)

Data sets in large applications are often too massive to fit completely inside the computer's internal memory. The resulting input/output communication (or I/O) between fast internal memory and slower external memory (such as disks) can be a major performance ...

Jeffrey Scott Vitter

2008-01-01T23:59:59.000Z

346

Reducing memory sharing overheads in distributed JVMs  

Science Conference Proceedings (OSTI)

Distributed JVM systems by supporting Javas shared-memory model enable concurrent Java applications to run transparently on clusters of computers. Aiming to reduce the overheads associated to memory coherence enforcement mechanisms required in ... Keywords: JVM, Java, cluster computing, concurrent Java applications, distributed shared memory, high-performance computing

Marcelo Lobosco; Orlando Loques; Claudio L. de Amorim

2005-09-01T23:59:59.000Z

347

Star Products for Relativistic Quantum Mechanics  

E-Print Network (OSTI)

The star product formalism has proved to be an alternative formulation for nonrelativistic quantum mechanics. We want introduce here a covariant star product in order to extend the star product formalism to relativistic quantum mechanics in the proper time formulation.

P. Henselder

2007-05-24T23:59:59.000Z

348

ENERGY STAR Score for Medical Offices  

NLE Websites -- All DOE Office Websites (Extended Search)

July 2013 ENERGY STAR Score for Medical Offices in the United States Page 1 ENERGY STAR Score for Medical Offices in the United States Technical Reference OVERVIEW The ENERGY STAR...

349

Indiana Memorial Union Wells Library  

E-Print Network (OSTI)

Franklin Hall Bryan Hall Law Indiana Memorial Union Jordan Hall Morrison Hall Wells Library Loop (0.5 miles) IMU to Greenhouse (0.3 miles) Business to Law School (0.75 miles) Wells Library to Morrison Hall (0.5 miles) Wells Library to Muisc Library (0.4 miles) #12;

Indiana University

350

Bridging the memory access gap  

Science Conference Proceedings (OSTI)

The rapid growth of electronic data processing over the past two decades has been characterized by an almost insatiable appetite for larger and faster memories. In fact, over this period of time, on-line storage capacity has increased about three times ...

Dennis E. Speliotis

1975-05-01T23:59:59.000Z

351

Trapped-flux superconducting memory  

Science Conference Proceedings (OSTI)

A memory cell based on trapped flux in superconductors has been built and tested. The cell is constructed entirely by vacuum evaporation of thin films and can be selected by coincident current or by other techniques, with drive-current requirements less ...

J. W. Crowe

1957-10-01T23:59:59.000Z

352

Modeling the near-UV band of GK stars, Paper I: LTE models  

E-Print Network (OSTI)

We present a grid of LTE atmospheric models and synthetic spectra that cover the spectral class range from mid-G to mid-K, and luminosity classes from V to III, that is dense in Teff sampling (Delta Teff=62.5 K), for stars of solar metallicity and moderately metal poor scaled solar abundance ([A/H]=0.0 and -0.5). All models have been computed with two choices of atomic line list: a) the "big" line lists of Kurucz (1992) that best reproduce the broad-band solar blue and near UV flux level, and b) the "small" lists of Kurucz & Peytremann (1975) that provide the best fit to the high resolution solar blue and near-UV spectrum. We compare our model SEDs to a sample of stars carefully selected from the large catalog of uniformly re-calibrated spectrophotometry of Burnashev (1985) with the goal of determining how the quality of fit varies with stellar parameters, especially in the historically troublesome blue and near-UV bands. We confirm that our models computed with the "big" line list recover the derived Tef...

Short, C Ian

2010-01-01T23:59:59.000Z

353

Physics of Neutron Star Crusts  

E-Print Network (OSTI)

The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.

N. Chamel; P. Haensel

2008-12-20T23:59:59.000Z

354

Reading Municipal Light Department - Residential ENERGY STAR...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Residential ENERGY STAR Appliance Rebate Program Reading Municipal Light Department - Residential ENERGY STAR Appliance Rebate Program Eligibility Residential Savings For Heating &...

355

ENERGY STAR Score for Medical Offices  

NLE Websites -- All DOE Office Websites (Extended Search)

Medical Offices in the United States Page 1 ENERGY STAR Score for Medical Offices in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Medical Offices...

356

ENERGY STAR Snapshot Spring 2012  

NLE Websites -- All DOE Office Websites (Extended Search)

Spring 2012 Spring 2012 Snapshot data runs through December 31, 2011. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is distributed twice a year and provides: * Trends in energy benchmarking of commercial and industrial buildings. * State-by-state activity along with activity for the top Designated Market Areas. * Industrial sector participation in ENERGY STAR. * Trends in ENERGY STAR certified commercial and industrial facilities. Summary By the end of calendar year 2011, commercial and industrial organizations exceeded figures for benchmarking and certification that were achieved in 2010. Since June, 2011:

357

Quadrupole moments of rotating neutron stars and strange stars  

E-Print Network (OSTI)

We present results for models of neutron stars and strange stars constructed using the Hartle-Thorne slow-rotation method with a wide range of equations of state, focusing on the values obtained for the angular momentum $J$ and the quadrupole moment $Q$, when the gravitational mass $M$ and the rotational frequency $\\Omega$ are specified. Building on previous work, which showed surprising uniformity in the behaviour of the moment of inertia for neutron-star models constructed with widely-different equations of state, we find similar uniformity for the quadrupole moment. These two quantities, together with the mass, are fundamental for determining the vacuum space-time outside neutron stars. We study particularly the dimensionless combination of parameters $QM/J^2$ (using units for which $c=G=1$). This quantity goes to 1 in the case of a Kerr-metric black hole and deviations away from 1 then characterize the difference between neutron-star and black-hole space-times. It is found that $QM/J^2$ for both neutron stars and strange stars decreases with increasing mass, for a given equation of state, reaching a value of around 2 (or even less) for maximum-mass models, meaning that their external space-time is then rather well approximated by the Kerr metric. If $QM/J^2$ is plotter against compactness $R/2M$ (where $R$ is the radius), it is found that the relationship is nearly unique for neutron-star models, independent of the equation of state, while it is significantly different for strange stars. This gives a new way of possibly distinguishing between them.

Martin Urbanec; John C. Miller; Zdenek Stuchlik

2013-01-24T23:59:59.000Z

358

Electrical Resistivity and Self-Potential Surveys Blue Mountain Geothermal  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » Electrical Resistivity and Self-Potential Surveys Blue Mountain Geothermal Area, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Electrical Resistivity and Self-Potential Surveys Blue Mountain Geothermal Area, Nevada Abstract Self potential and electrical resistivity surveys have been completed at the Blue Mountain geothermal area to search for the source of thermal fluids discovered during drilling for mineral exploration, and to help characterize the geothermal resource. Two large SP anomalies are associated with the artesian thermal area and the area of highest temperature observed in drill holes. Two similar anomalies were mapped 1 to 3 km to the south

359

Blue Ribbon Commission on America's Nuclear Future Charter | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Blue Ribbon Commission on America's Nuclear Future Charter Blue Ribbon Commission on America's Nuclear Future Charter Blue Ribbon Commission on America's Nuclear Future Charter March 2, 2010 - 12:00am Addthis The Secretary of Energy, acting at the direction of the President, is establishing the Commission to conduct a comprehensive review of policies for managing the back end of the nuclear fuel cycle, including all alternatives for the storage, processing, and disposal of civilian and defense used nuclear fuel, high-level waste, and materials derived from nuclear activities. Specifically, the Commission will provide advice, evaluate alternatives, and make recommendations for a new plan to address these issues, including: Evaluation of existing fuel cycle technologies and R&D programs. Criteria for evaluation should include cost, safety, resource utilization

360

BlueWave Capital LLC | Open Energy Information  

Open Energy Info (EERE)

BlueWave Capital LLC BlueWave Capital LLC Jump to: navigation, search Name BlueWave Capital LLC Place Boston, Massachusetts Sector Renewable Energy Product Knowledge-based investment firm focused on early- and expansion-stage environmental and renewable energy-related operating companies. Coordinates 42.358635°, -71.056699° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.358635,"lon":-71.056699,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "blue star memorial" 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

Blue Ruthenium Dimer Catalysis for Hydrogen Generation | Advanced Photon  

NLE Websites -- All DOE Office Websites (Extended Search)

A High-Pressure Nano-imaging Breakthrough A High-Pressure Nano-imaging Breakthrough Protein Structure Could Lead to Better Treatments for HIV, Early Aging The Superpower behind Iron Oxyfluoride Battery Electrodes Watching a Protein as it Functions Shedding Light on Chemistry with a Biological Twist Science Highlights Archives: 2013 | 2012 | 2011 | 2010 2009 | 2008 | 2007 | 2006 2005 | 2004 | 2003 | 2002 2001 | 2000 | 1998 | Subscribe to APS Science Highlights rss feed Blue Ruthenium Dimer Catalysis for Hydrogen Generation APRIL 15, 2013 Bookmark and Share Key intermediates in the water oxidation catalytic cycle of the blue dimer characterized by x-ray spectroscopy. Optimization of the reactivity toward water (purple arrow) and oxidation of the resulting peroxo-intermediate (blue arrow) are needed for improved catalytic activity.

362

Why sequence Eukaryotic microbial metatranscriptome of blue grama grass  

NLE Websites -- All DOE Office Websites (Extended Search)

eukaryotic microbial metatranscriptome of blue grama grass eukaryotic microbial metatranscriptome of blue grama grass rhizosphere soils? About 50 miles south of Albuquerque, New Mexico is the Sevilleta National Wildlife Refuge managed by the U.S. Department of the Interior, Fish and Wildlife Service. The region is the intersection of several regional ecosystems, including grasslands, woodlands and riparian vegetation. The location is ideal for researchers to study how climate variability and climate change can act together to impact ecosystem dynamics and is known as the Sevilleta Long Term Ecological Research (LTER) site. This project focuses on the blue grama grass rhizosphere of the LTER site. Aridland ecosystems such as the one found in the Sevilleta represent at least a third of terrestrial biomes and are known for their nutrient-poor

363

ENERGY STAR Focus on Energy Efficiency in Metalcasting | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Metalcasting Metalcasting Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Tools for benchmarking energy management practices Tools for tracking and benchmarking facility energy performance ENERGY STAR Energy Performance Indicators for plants

364

ENERGY STAR certification for your building | ENERGY STAR Buildings &  

NLE Websites -- All DOE Office Websites (Extended Search)

certification for your building certification for your building Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager Save energy Find financing Earn recognition 20-percent recognition ENERGY STAR certification How to apply for ENERGY STAR certification Tips for low-cost verifications Submit a profile of your building

365

ENERGY STAR Building Upgrade Manual | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Building Upgrade Manual ENERGY STAR Building Upgrade Manual Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager Save energy Stamp out energy waste Find cost-effective investments Engage occupants Purchase energy-saving products Put computers to sleep Get help from an expert Take a comprehensive approach

366

Portfolio Manager Technical Reference: ENERGY STAR Score | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

ENERGY STAR Score ENERGY STAR Score Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

367

Sample ENERGY STAR performance documents | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Existing buildings Existing buildings » Use Portfolio Manager » Verify and document your savings » Sample ENERGY STAR performance documents Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager The new ENERGY STAR Portfolio Manager How Portfolio Manager helps you save The benchmarking starter kit

368

MEMORIAL RESOLUTION H. TAYLOR HOWARD  

E-Print Network (OSTI)

a distinguished Stanford career in radio engineering and space sciences that spanned 50 years, and a separate Laboratory, now called the STAR (Space, Telecommunications, and Radio Science) Laboratory. This was one research programs of SRI International of Menlo Park and Stanford University. Tay installed a very powerful

Cavalli-Sforza, Luigi

369

Blue Ridge Mountain Electric Membership Corporation - Water Heater Rebate  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

You are here You are here Home » Blue Ridge Mountain Electric Membership Corporation - Water Heater Rebate Program Blue Ridge Mountain Electric Membership Corporation - Water Heater Rebate Program < Back Eligibility Residential Savings Category Home Weatherization Commercial Weatherization Sealing Your Home Heating & Cooling Commercial Heating & Cooling Cooling Construction Design & Remodeling Ventilation Manufacturing Heat Pumps Appliances & Electronics Water Heating Program Info State Georgia Program Type Utility Rebate Program Rebate Amount In-Home Energy Evaluation Program Windows: $500 Duct Repair: $500 Rehabilitation Work: $250 HVAC Replacement: $250/unit HVAC Tune-up: $150/unit Insulation: $500 Water Heater and Pipe Insulation: $50 Air Sealing: $500 Energy Right Program

370

A blue sky catastrophe in double-diffusive convection  

E-Print Network (OSTI)

A global bifurcation of the blue sky catastrophe type has been found in a small Prandtl number binary mixture contained in a laterally heated cavity. The system has been studied numerically applying the tools of bifurcation theory. The catastrophe corresponds to the destruction of an orbit which, for a large range of Rayleigh numbers, is the only stable solution. This orbit is born in a global saddle-loop bifurcation and becomes chaotic in a period doubling cascade just before its disappearance at the blue sky catastrophe.

Esteban Meca; Isabel Mercader; Oriol Batiste; Laureano Ramirez-Piscina

2004-05-27T23:59:59.000Z

371

Variable stars in the field of the open cluster NGC 7789  

E-Print Network (OSTI)

We present the results of our search for variable stars in the intermediate-age open cluster NGC 7789. We have found 45 variable stars: 35 eclipsing binaries, five pulsating variables and five miscellaneous variables. Most of the eclipsing binaries show W UMa type of variability, with periods shorter than one day. Four systems exhibit unusual behavior: two, V4276 and V6698, are probably RS CVn stars, another, V3283, is a possible cataclysmic binary. The nature of the fourth binary, V2130, is unclear: the system exhibits assymetric maxima. Among the pulsating variables two, V3407C and V4805 are background RR Lyrae stars and one, V6736, is a delta Scuti variable which is a blue straggler belonging to the cluster. Some of the miscellaneous variables may have periods longer than the five day timespan of our observations. We also present a color-magnitude diagram for the NGC 7789 open cluster, fairly complete down to V ~ 20. The relatively large number of variables found in the comparison field (14 compared to 31 in the cluster field) implies that objects not associated physically with the cluster can account for a significant number of variables identified in the cluster field, as well as in other globular and open clusters observed on a dense background/foreground of disk stars.

B. J. Mochejska; J. Kaluzny

1999-07-20T23:59:59.000Z

372

ENERGY STAR Update: ENERGY STAR Low Carbon IT Campaign Kicks...  

NLE Websites -- All DOE Office Websites (Extended Search)

Carbon IT Campaign Kicks Off 2013 with Organizations Pledging to Power Manage 360,000 Computers The ENERGY STAR Low Carbon IT (LCIT) Campaign, a nationwide effort to assist and...

373

Who else is partnered with ENERGY STAR? | ENERGY STAR Buildings...  

NLE Websites -- All DOE Office Websites (Extended Search)

Hospital logo Increased its average ENERGY STAR score by 12 points over 2010 TIAA-CREF logo Achieved its 2012 goal of a 15% portfolio-wide energy reduction Transwestern...

374

The ENERGY STAR Guidelines for Energy Management | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

a star. Your guide to building a strategic energy management program So you want to start saving energy, but you don't know where to begin. Or perhaps you've been managing energy...

375

ENERGY STAR Challenge for Industry  

NLE Websites -- All DOE Office Websites (Extended Search)

Industrial Plant Industrial Plant Certification Professional Engineers' Guide for Validating Statements of Energy Performance Office of Air and Radiation Climate Protection Partnerships Division June 2013 ii Introduction The U.S. Environmental Protection Agency's ENERGY STAR program provides guidance, tools, and recognition to help companies improve the energy performance of their facilities and strengthen the effectiveness of their energy management program. Through ENERGY STAR, the U.S. Environmental Protection Agency (EPA) offers a number of forms of recognition, including certification for facility energy efficiency. ENERGY STAR certification for industrial plants recognizes individual manufacturing plants whose

376

Blue Mountain, Humboldt County, Nevada, U.S.A  

SciTech Connect

The report documents the drilling of well Deep Blue No.2, the second deep geothermal test hole at the Blue Mountain Geothermal Area, Humboldt County, Nevada. The well was drilled by Noramex Corp, a Nevada company, with funding support from the US Department of Energy, under the DOEs GRED II Program. Deep Blue No.2 was drilled as a step-out hole from Deep Blue No.1, to further evaluate the commercial potential of the geothermal resource. Deep Blue No.2 was designed as a vertical, slim observation test hole to a nominal target depth of 1000 meters (nominal 3400 feet). The well tests an area of projected high temperatures at depth, from temperature gradients measured in a group of shallow drill holes located approximately one kilometer to the northeast of observation hole Deep Blue No.1. The well is not intended for, or designed as, a commercial well or a production well. Deep Blue No.2 was spudded on March 25, 2004 and completed to a total depth of 1127.76m (3700 ft) on April 28, 2004. The well was drilled using conventional rotary drilling techniques to a depth of 201.17 m (660 ft), and continuously cored from 201.17m (660 ft) to 1127.76m (3700 ft). A brief rig-on flow-test was conducted at completion to determine basic reservoir parameters and obtain fluid samples. A permeable fracture zone with measured temperatures of 150 to 167C (302 to 333F) occurs between 500 to 750m (1640 to 2461ft). The well was left un-lined in anticipation of the Phase III - Flow and Injection Testing. A further Kuster temperature survey was attempted after the well had been shut in for almost 3 weeks. The well appears to have bridged off at 439m (1440ft) as the Kuster tool was unable to descend past this point. Several attempts to dislodge the obstruction using tube jars were unsuccessful. Deep Blue No.2 encountered variably fractured and veined, fine-grained rocks of the Singas Formation, and intruded by minor strongly altered fine-grained felsic dikes, and less altered fineto medium-grained felsic to intermediate dikes. Widespread open fractures and extensive of quartz veining in many intervals of the core indicate a high degree of fracturing and flow of silica-bearing fluids, almost certainly hotter than 200C (392F), at some time, but these fractures are now partially sealed. Intervals of soft shaly mudstone, common clay gouge, and rocks with generally low permeability (few veins and fractures) may also form a seal or cap above the main high temperature reservoir at Blue Mountain. The encouraging results from Deep Blue No.2 support further drilling at Blue Mountain. Higher temperature fluids can be expected where fractures providing channels for the circulation of hot water from depth have not been sealed extensively by silica deposition.

Ted Fitzpatrick, Brian D. Fairbank

2005-04-01T23:59:59.000Z

377

Discovery of > 200 RR Lyrae Variables in M62: An Oosterhoff I Globular Cluster with a Predominantly Blue HB  

E-Print Network (OSTI)

We report on the discovery of a large number of RR Lyrae variable stars in the moderately metal-rich Galactic globular cluster M62 (NGC 6266), which places it among the top three most RR Lyrae-rich globular clusters known. Likely members of the cluster in our studied field, from our preliminary number counts, include about 130 fundamental-mode (RRab) pulsators, with = 0.548 d, and about 75 first-overtone (RRc) pulsators, with = 0.300 d. The average periods and the position of the RRab variables with well-defined light curves in the Bailey diagram both suggest that the cluster is of Oosterhoff type I. However, the morphology of the cluster's horizontal branch (HB) is strikingly similar to that of the Oosterhoff type II globular cluster M15 (NGC 7078), with a dominant blue HB component and a very extended blue tail. Since M15 and M62 differ in metallicity by about one dex, we conclude that metallicity, at a fixed HB type, is a key parameter determining the Oosterhoff status of a globular cluster and the posit...

Contreras, R; Smith, H A; Pritzl, B J; Borissova, J

2005-01-01T23:59:59.000Z

378

Discovery of > 200 RR Lyrae Variables in M62: An Oosterhoff I Globular Cluster with a Predominantly Blue HB  

E-Print Network (OSTI)

We report on the discovery of a large number of RR Lyrae variable stars in the moderately metal-rich Galactic globular cluster M62 (NGC 6266), which places it among the top three most RR Lyrae-rich globular clusters known. Likely members of the cluster in our studied field, from our preliminary number counts, include about 130 fundamental-mode (RRab) pulsators, with = 0.548 d, and about 75 first-overtone (RRc) pulsators, with = 0.300 d. The average periods and the position of the RRab variables with well-defined light curves in the Bailey diagram both suggest that the cluster is of Oosterhoff type I. However, the morphology of the cluster's horizontal branch (HB) is strikingly similar to that of the Oosterhoff type II globular cluster M15 (NGC 7078), with a dominant blue HB component and a very extended blue tail. Since M15 and M62 differ in metallicity by about one dex, we conclude that metallicity, at a fixed HB type, is a key parameter determining the Oosterhoff status of a globular cluster and the position of its variables in the Bailey diagram.

R. Contreras; M. Catelan; H. A. Smith; B. J. Pritzl; J. Borissova

2005-03-11T23:59:59.000Z

379

Blue Canyon II Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Blue Canyon II Wind Farm Blue Canyon II Wind Farm Jump to: navigation, search Name Blue Canyon II Wind Farm Facility Blue Canyon II Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Wind Energy Developer Horizon Wind Energy Energy Purchaser American Electric Power Location North of Lawton OK Coordinates 34.8582°, -98.54752° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.8582,"lon":-98.54752,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

380

Blue-green and green phosphors for lighting applications  

DOE Patents (OSTI)

Embodiments of the present techniques provide a related family of phosphors that may be used in lighting systems to generate blue or blue-green light. The phosphors include systems having a general formula of: ((Sr.sub.1-zM.sub.z).sub.1-(x+w)A.sub.wCe.sub.x).sub.3(Al.sub.1-ySi.s- ub.y)O.sub.4+y+3(x-w)F.sub.1-y-3(x-w) (I), wherein 0blue and blue/green light. Further, the phosphors may be used in blends with other phosphors, or in combined lighting systems, to produce white light suitable for illumination.

Setlur, Anant Achyut; Chandran, Ramachandran Gopi; Henderson, Claire Susan; Nammalwar, Pransanth Kumar; Radkov, Emil

2012-12-11T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

Recursive Wang tiles for real-time blue noise  

Science Conference Proceedings (OSTI)

Well distributed point sets play an important role in a variety of computer graphics contexts, such as anti-aliasing, global illumination, halftoning, non-photorealistic rendering, point-based modeling and rendering, and geometry processing. In this ... Keywords: Poisson disk distribution, Wang tiles, anti-aliasing, blue noise, non-periodic tiling, object positioning, sampling, stippling, texture synthesis

Johannes Kopf; Daniel Cohen-Or; Oliver Deussen; Dani Lischinski

2006-07-01T23:59:59.000Z

382

Blue-green algae: why they become dominant  

SciTech Connect

The injection of carbon dioxide and the addition of nitrogen and phosphorus to a lake population dominated by blue-green algae results in a rapid shift to dominance by green algae. The basis for the change and its implications are discussed.

Shapiro, J.

1973-01-01T23:59:59.000Z

383

Performance Analysis on Blue Gene Q with HPCToolkit  

E-Print Network (OSTI)

for performance analysis of OpenMP · Next steps · Using HPCToolkit on Blue Gene/Q at ALCF 3 #12;4 Rice University -- within and across nodes 18 #12;HPCToolkit at ALCF · ALCF systems -- /soft/perftools/hpctoolkit/pkgs/hpctoolkit · Man pages -- /soft/perftools/hpctoolkit/pkgs/hpctoolkit/share/man · ALCF guide to HPCToolkit -- http://www.alcf

Kemner, Ken

384

BlueSpace: personalizing workspace through awareness and adaptability  

Science Conference Proceedings (OSTI)

This paper reports on research in workplace issues encountered by knowledge workers in cubicle environments, and on BlueSpace, a prototype workspace with the goal of addressing workers' critical needs for privacy, concentration and personalization. To ... Keywords: awareness, communication, knowledge workers, personalization, privacy, workspace

Jennifer Lai; Anthony Levas; Paul Chou; Claudio Pinhanez; Marisa Viveros

2002-11-01T23:59:59.000Z

385

Overview of the Blue Gene/L system architecture  

Science Conference Proceedings (OSTI)

The Blue Gene/L computer is a massively parallel supercomputer based on IBM system-on-a-chip technology. It is designed to scale to 65,536 dual-processor nodes, with a peak performance of 360 teraflops. This paper describes the project objectives ...

A. Gara; M. A. Blumrich; D. Chen; G. L.-T. Chiu; P. Coteus; M. E. Giampapa; R. A. Haring; P. Heidelberger; D. Hoenicke; G. V. Kopcsay; T. A. Liebsch; M. Ohmacht; B. D. Steinmacher-Burow; T. Takken; P. Vranas

2005-03-01T23:59:59.000Z

386

ENERGY STAR Challenge for Industry  

NLE Websites -- All DOE Office Websites (Extended Search)

Challenge Challenge for Industry Professional Engineers' Guide for Validating Statements of Energy Improvement Office of Air and Radiation Climate Protection Partnerships Division May 2013 Revised ii Introduction The U.S. Environmental Protection Agency's (U.S. EPA) ENERGY STAR program provides guidance, tools, and recognition to help companies improve their energy performance. ENERGY STAR is a voluntary partnership program that companies choose to join. Through ENERGY STAR, U.S. EPA offers a number of forms of recognition for achievements in energy efficiency. The ENERGY STAR Challenge for Industry recognizes individual industrial sites for achieving a 10 percent reduction in energy intensity within 5 years from the conclusion of an established baseline. To be

387

Appendix 5 - STARS Architectual Overview  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Last saved by Coombs Page 1 7/27/2012 Last saved by Coombs Page 1 7/27/2012 Draft Appendix 5 - STARS Architectural Overview ARC101 - Architectural Overview for Department of Energy iManage Program - STARS Project Deliverable ID: IT0013 Version number: 1.09 Draft/Final as of: 18 Oct 2005 Printed on: 27 Jul 2012 Author: Richard Popovich, STARS System Architect Richard.Popovich@hq.doe.gov (301) 903-2223 Owner: Laura Kramer, STARS Project Manager Status of Document Draft Delivered Accepted Last saved by Coombs Page 2 7/27/2012 Draft Document information Document source This document is maintained as an online document. Contact the author for the latest version. Revision history Version number Date Summary of changes Revised By 1.01 08 Jul 03 Version 1 Richard Popovich,

388

Shooting Star | Open Energy Information  

Open Energy Info (EERE)

Shooting Star Shooting Star Jump to: navigation, search Name Shooting Star Facility Shooting Star Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Exelon Wind Developer Infinity Wind Power Energy Purchaser Sunflower Electric Power Corporation Location Greensburg KS Coordinates 37.55019151°, -99.27585125° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.55019151,"lon":-99.27585125,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

389

ENERGY STAR Newsletter: Fall 2009  

NLE Websites -- All DOE Office Websites (Extended Search)

in LOCATION> for a 40-minute brown bag session to find out how we can save energy, save money, and fight climate change when we "bring our green to work." ENERGY STAR, the U.S....

390

Make a commitment | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

391

Modelling the asymmetric wind of the luminous blue variable binary MWC 314  

E-Print Network (OSTI)

We present a spectroscopic analysis of MWC 314, a luminous blue variable (LBV) candidate with an extended bipolar nebula. The detailed spectroscopic variability is investigated to determine if MWC 314 is a massive binary system with a supersonically accelerating wind or a low-mass B[e] star. We compare the spectrum and spectral energy distribution to other LBVs (such as P Cyg) and find very similar physical wind properties, indicating strong kinship. We combined long-term high-resolution optical spectroscopic monitoring and V-band photometric observations to determine the orbital elements and stellar parameters and to investigate the spectral variability with the orbital phases. We developed an advanced model of the large-scale wind-velocity and wind-density structure with 3-D radiative transfer calculations that fit the orbitally modulated P Cyg profile of He I lam5876, showing outflow velocities above 1000 km/s. We find that MWC 314 is a massive semi-detached binary system of ~1.22 AU, observed at an inclin...

Lobel, A; Martayan, C; Frmat, Y; Dozinel, K Torres; Raskin, G; Van Winckel, H; Prins, S; Pessemier, W; Waelkens, C; Hensberge, H; Dummortier, L; Jorissen, A; Van Eck, S; Lehmann, H

2013-01-01T23:59:59.000Z

392

Disaggregated memory for expansion and sharing in blade servers  

Science Conference Proceedings (OSTI)

Analysis of technology and application trends reveals a growing imbalance in the peak compute-to-memory-capacity ratio for future servers. At the same time, the fraction contributed by memory systems to total datacenter costs and power consumption during ... Keywords: disaggregated memory, memory blades, memory capacity expansion, power and cost efficiencies

Kevin Lim; Jichuan Chang; Trevor Mudge; Parthasarathy Ranganathan; Steven K. Reinhardt; Thomas F. Wenisch

2009-06-01T23:59:59.000Z

393

Architecture extensions for efficient management of scratch-pad memory  

Science Conference Proceedings (OSTI)

Nowadays, many embedded processors include in their architecture on-chip static memories, so called scratch-pad memories (SPM). Compared to cache, these memories do not require complex control logic, thus resulting in increased efficiency both in silicon ... Keywords: embedded processors, memory architecture, scratch-pad memory

Jos V. Busquets-Mataix; Carlos Catal; Antonio Mart-Campoy

2011-09-01T23:59:59.000Z

394

Introspection-based memory de-duplication and migration  

Science Conference Proceedings (OSTI)

Memory virtualization abstracts a physical machine's memory resource and presents to the virtual machines running on it a piece of physical memory that could be shared, compressed and moved. To optimize the memory resource utilization by fully leveraging ... Keywords: introspection, memory de-duplication, vm migration

Jui-Hao Chiang; Han-Lin Li; Tzi-cker Chiueh

2013-03-01T23:59:59.000Z

395

Cooling Evolution of Hybrid Stars  

E-Print Network (OSTI)

The cooling of compact isolated objects for different values of the gravitational mass has been simulated for two alternative assumptions. One is that the interior of the star is purely hadronic and second that the star can have a rather large quark core. It has been shown that within a nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star configurations with masses below 1.3 M_sun. For a realistic choice of parameters the equation of state (EoS) allows for 2SC quark matter with a large quark gap ~ 100 MeV for u and d quarks of two colors that coexists with normal quark matter within a mixed phase in the hybrid star interior. We argue that, if in the hadronic phase the neutron pairing gap in 3P_2 channel is larger than few keV and the phases with unpaired quarks are allowed, the corresponding hybrid stars would cool too fast. Even in the case of the essentially suppressed 3P_2 neutron gap if free quarks occur for M cooling data existing by today. It is suggested to discuss a "2SC+X" phase, as a possibility to have all quarks paired in two-flavor quark matter under neutron star constraints, where the X-gap is of the order of 10 keV - 1 MeV. Density independent gaps do not allow to fit the cooling data. Only the presence of an X-gap that decreases with increase of the density could allow to appropriately fit the data in a similar compact star mass interval to that following from a purely hadronic model.

H. Grigorian

2005-02-28T23:59:59.000Z

396

Experiments with Memory-to-Memory Coupling for End-to-End Fusion Simulation Workflows  

Science Conference Proceedings (OSTI)

Scientific applications are striving to accurately simulate multiple interacting physical processes that comprise complex phenomena being modeled. Efficient and scalable parallel implementations of these coupled simulations present challenging interaction ... Keywords: coupling, memory-to-memory, rdma, workflows

Ciprian Docan; Fan Zhang; Manish Parashar; Julian Cummings; Norbert Podhorszki; Scott Klasky

2010-05-01T23:59:59.000Z

397

STAR FORMATION IN DENSE CLUSTERS  

SciTech Connect

A model of core-clump accretion with equally likely stopping describes star formation in the dense parts of clusters, where models of isolated collapsing cores may not apply. Each core accretes at a constant rate onto its protostar, while the surrounding clump gas accretes as a power of protostar mass. Short accretion flows resemble Shu accretion and make low-mass stars. Long flows resemble reduced Bondi accretion and make massive stars. Accretion stops due to environmental processes of dynamical ejection, gravitational competition, and gas dispersal by stellar feedback, independent of initial core structure. The model matches the field star initial mass function (IMF) from 0.01 to more than 10 solar masses. The core accretion rate and the mean accretion duration set the peak of the IMF, independent of the local Jeans mass. Massive protostars require the longest accretion durations, up to 0.5 Myr. The maximum protostar luminosity in a cluster indicates the mass and age of its oldest protostar. The distribution of protostar luminosities matches those in active star-forming regions if protostars have a constant birthrate but not if their births are coeval. For constant birthrate, the ratio of young stellar objects to protostars indicates the star-forming age of a cluster, typically {approx}1 Myr. The protostar accretion luminosity is typically less than its steady spherical value by a factor of {approx}2, consistent with models of episodic disk accretion.

Myers, Philip C., E-mail: pmyers@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2011-12-10T23:59:59.000Z

398

Cooling Evolution of Hybrid Stars  

E-Print Network (OSTI)

The cooling of compact isolated objects for different values of the gravitational mass has been simulated for two alternative assumptions. One is that the interior of the star is purely hadronic and second that the star can have a rather large quark core. It has been shown that within a nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star configurations with masses below 1.3 M_sun. For a realistic choice of parameters the equation of state (EoS) allows for 2SC quark matter with a large quark gap ~ 100 MeV for u and d quarks of two colors that coexists with normal quark matter within a mixed phase in the hybrid star interior. We argue that, if in the hadronic phase the neutron pairing gap in 3P_2 channel is larger than few keV and the phases with unpaired quarks are allowed, the corresponding hybrid stars would cool too fast. Even in the case of the essentially supp...

Grigorian, H

2005-01-01T23:59:59.000Z

399

Rotary actuator utilizing a shape memory alloy  

SciTech Connect

An apparatus is described comprising; (a) rotary accumulator means for accumulating a length of a shape memory alloy wire; (b) the shape memory alloy wire attached at one end to a point fixed with respect to the rotary accumulator means and attached at a second end to the rotary accumulator means; (c) biasing means for biasing the rotary accumulator means to a first position; and (d) means for heating the shape memory alloy wire to cause the shape memory alloy wire to contract, thereby rotating the rotary accumulator means from the first position to a second position.

Bloch, J.T.

1988-08-09T23:59:59.000Z

400

Characterization of Shape Memory Alloys: Deformation Behavior  

Science Conference Proceedings (OSTI)

Feb 28, 2011... expected that NiTi shape memory alloys (SMA) actuators would provide simple and light weight replacements for controlling chevron-shaped...

Note: This page contains sample records for the topic "blue star memorial" 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

ON EFFICIENTLY COMBINING LIMITED MEMORY AND TRUST ...  

E-Print Network (OSTI)

... Euclidean norm with an insignificant computational overhead compared with the cost of computing the quasi-Newton direction in line-search limited memory...

402

Determining Memory Use | Argonne Leadership Computing Facility  

NLE Websites -- All DOE Office Websites (Extended Search)

Allinea DDT Core File Settings Determining Memory Use Using VNC with a Debugger bgqstack gdb Coreprocessor TotalView on BGQ Systems Performance Tools & APIs Software & Libraries...

403

Exploiting Data Similarity to Reduce Memory Footprints  

SciTech Connect

Memory size has long limited large-scale applications on high-performance computing (HPC) systems. Since compute nodes frequently do not have swap space, physical memory often limits problem sizes. Increasing core counts per chip and power density constraints, which limit the number of DIMMs per node, have exacerbated this problem. Further, DRAM constitutes a significant portion of overall HPC system cost. Therefore, instead of adding more DRAM to the nodes, mechanisms to manage memory usage more efficiently - preferably transparently - could increase effective DRAM capacity and thus the benefit of multicore nodes for HPC systems. MPI application processes often exhibit significant data similarity. These data regions occupy multiple physical locations across the individual rank processes within a multicore node and thus offer a potential savings in memory capacity. These regions, primarily residing in heap, are dynamic, which makes them difficult to manage statically. Our novel memory allocation library, SBLLmalloc, automatically identifies identical memory blocks and merges them into a single copy. SBLLmalloc does not require application or OS changes since we implement it as a user-level library. Overall, we demonstrate that SBLLmalloc reduces the memory footprint of a range of MPI applications by 32.03% on average and up to 60.87%. Further, SBLLmalloc supports problem sizes for IRS over 21.36% larger than using standard memory management techniques, thus significantly increasing effective system size. Similarly, SBLLmalloc requires 43.75% fewer nodes than standard memory management techniques to solve an AMG problem.

Biswas, S; de Supinski, B R; Schulz, M; Franklin, D; Sherwood, T; Chong, F T

2011-01-28T23:59:59.000Z

404

Memory resource management in vmware esx server  

E-Print Network (OSTI)

VMware ESX Server is a thin software layer designed to multiplex hardware resources efficiently among virtual machines running unmodified commodity operating systems. This paper introduces several novel ESX Server mechanisms and policies for managing memory. A ballooning technique reclaims the pages considered least valuable by the operating system running in a virtual machine. An idle memory tax achieves efficient memory utilization while maintaining performance isolation guarantees. Content-based page sharing and hot I/O page remapping exploit transparent page remapping to eliminate redundancy and reduce copying overheads. These techniques are combined to efficiently support virtual machine workloads that overcommit memory. 1

Carl A. Waldspurger

2002-01-01T23:59:59.000Z

405

Memorandum Memorializing Ex Parte Communication - August 12,...  

NLE Websites -- All DOE Office Websites (Extended Search)

Memorandum Memorializing Ex Parte Communication - August 12, 2011 On August 9, 2011, the Air-Conditioning, Heating and Refrigeration Institute's (AHRI) Unitary Small Engineering...

406

Julian Szekely Memorial Symposium Rental Car Information  

Science Conference Proceedings (OSTI)

The Julian Szekely Memorial Symposium on Materials Processing will be held at the Royal Sonesta Hotel in Cambridge, Massachusetts, October 5-8, 1997.

407

T-720: Blue Coat Director HTTP Trace Processing Flaw Permits Cross-Site  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

0: Blue Coat Director HTTP Trace Processing Flaw Permits 0: Blue Coat Director HTTP Trace Processing Flaw Permits Cross-Site Scripting Attacks T-720: Blue Coat Director HTTP Trace Processing Flaw Permits Cross-Site Scripting Attacks September 19, 2011 - 8:45am Addthis PROBLEM Blue Coat Director HTTP Trace Processing Flaw Permits Cross-Site Scripting Attacks. PLATFORM: All versions of Director prior to 5.5.2.3 are vulnerable. ABSTRACT: A vulnerability was reported in Blue Coat Director. A remote user can conduct cross-site scripting attacks. reference LINKS: Blue Coat Advisories ID: SA62 SecurityTracker Alert ID: 1026061 Blue Coat Director 510 Blue Coat SGME 5 IMPACT ASSESSMENT: Medium Discussion: An attacker can use the HTTP TRACE method to echo malicious script back to the client as part of a Cross Site Scripting (XSS) attack. No

408

I Have Seen the Light and It's Green...or Pink, or Blue, or Purple...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

I Have Seen the Light and It's Green...or Pink, or Blue, or Purple. Shucks, it's LED Solid-State Lighting. I Have Seen the Light and It's Green...or Pink, or Blue, or Purple....

409

Blue fan palm distribution and seed removal patterns in three desert oases of northern Baja California, Mexico  

E-Print Network (OSTI)

DOI 10.1007/s11258-009-9682-4 Blue fan palm distribution anddistribution patterns of the blue fan palm, Brahea armata,i) the levels of blue fan palm seed removal by vertebrates

Wehncke, Elisabet V.; Lpez-Medelln, Xavier; Ezcurra, Exequiel

2010-01-01T23:59:59.000Z

410

Time Series Photometry of Variable Stars in the Globular Cluster NGC 6397  

E-Print Network (OSTI)

Time series BVI photometry is presented for 16 short-period variables located in the central region of the globular cluster NGC 6397. The sample includes 9 newly detected variables. The light curve of cataclysmic variable CV6 shows variability with a period of 0.2356 days. We confirm an earlier reported period of 0.472 days for cataclysmic variable CV1. Phased light curves of both CVs exhibit sine-like light curves, with two minima occurring during each orbital cycle. The secondary component of CV1 has a low average density of 0.83 g/cm^{3} indicating that it cannot be a normal main sequence star. Variables among the cluster blue stragglers include a likely detached eclipsing binary with orbital period of 0.787 days, three new SX Phe stars (one of which has the extremely short period of 0.0215 days), and three low amplitude variables which are possible gamma Doradus variables.

Janusz Kaluzny; Ian B. Thompson

2002-10-29T23:59:59.000Z

411

Models on Distributed Memory Architectures  

NLE Websites -- All DOE Office Websites (Extended Search)

5/2004 Y.He 1 5/2004 Y.He 1 MPH: a Library for Coupling Multi-Component Models on Distributed Memory Architectures and its Applications Yun (Helen) He and Chris Ding CRD Division Lawrence Berkeley National Laboratory 10/15/2004 Y.He 2 10/15/2004 Y.He 3 Motivation n Application problems grow in scale & complexity n Effective organization of simulation software system that is maintainable, reusable, sharable, and efficient è a major issue n Community Climate System Model (CCSM) development n Software lasts much longer than a computer! 10/15/2004 Y.He 4

412

A DSL approach for object memory management of small devices  

Science Conference Proceedings (OSTI)

Small devices have a specific hardware configuration. In particular, they usually include several types of memories (typically ROM, internal and external RAM, Flash memory) different in quantities and properties. We propose an object memory management ...

Kevin Marquet; Gilles Grimaud

2007-09-01T23:59:59.000Z

413

Distributed anemone: transparent low-latency access to remote memory  

Science Conference Proceedings (OSTI)

Performance of large memory applications degrades rapidly once the system hits the physical memory limit and starts paging to local disk. We present the design, implementation and evaluation of Distributed Anemone (Adaptive Network Memory Engine) ...

Michael R. Hines; Jian Wang; Kartik Gopalan

2006-12-01T23:59:59.000Z

414

EERE EnergyStar State Allocations | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

EERE EnergyStar State Allocations EERE EnergyStar State Allocations EEEnergyStarStateAllocations.pdf More Documents & Publications State Energy Efficient Appliance Rebate...

415

Formation of Radioactive Citrulline During Photosynthetic C14O2-Fixation by Blue-Green Algae  

E-Print Network (OSTI)

ClTRULLlNE BY BLUE-GREEN ALGAE TWO-WEEK LOAN COPY This is aC~~O~-FIXATION BLUE-GREEN ALGAE Pekka Linko, 0. Holm-Hansen,C~~O~-FIXATION BLUE-GREEN ALGAE BY Pelcka Linlc~,'~ Holm-

Linko, Pekka; Holm-Hansen, O.; Bassham, J.A.; Calvin, M.

1956-01-01T23:59:59.000Z

416

Intersecting Red and Blue Line Segments in Optimal Time and Precision  

Science Conference Proceedings (OSTI)

A common geometric problem in computer graphics and geographic information systems is to compute the arrangement of a set of n segments that can be colored red and blue so that there are no red/red or blue/blue crossings. We give a sweep algorithm ...

Andrea Mantler; Jack Snoeyink

2000-11-01T23:59:59.000Z

417

Wave Star Energy | Open Energy Information  

Open Energy Info (EERE)

Star Energy Star Energy Jump to: navigation, search Name Wave Star Energy Place Denmark Zip DK-2920 Product Denmark-based private wave device developer. References Wave Star Energy[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This company is listed in the Marine and Hydrokinetic Technology Database. This company is involved in the following MHK Projects: Wave Star Energy 1 10 Scale Model Test This company is involved in the following MHK Technologies: C5 WaveStar This article is a stub. You can help OpenEI by expanding it. Wave Star Energy is a company located in Denmark . References ↑ "Wave Star Energy" Retrieved from "http://en.openei.org/w/index.php?title=Wave_Star_Energy&oldid=678928" Categories: Clean Energy Organizations

418

How the 1-100 ENERGY STAR score is calculated | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

is calculated Using the 1 - 100 ENERGY STAR score, you can understand how your building's energy consumption measures up against similar buildings nationwide. The ENERGY STAR score...

419

Old and new neutron stars  

Science Conference Proceedings (OSTI)

The youngest known radiopulsar in the rapidly spinning magnetized neutron star which powers the Crab Nebula, the remnant of the historical supernova explosion of 1054 AD. Similar neutron stars are probably born at least every few hundred years, but are less frequent than Galactic supernova explosions. They are initially sources of extreme relativistic electron and/or positron winds (approx.10/sup 38/s/sup -1/ of 10/sup 12/ eV leptons) which greatly decrease as the neutron stars spin down to become mature pulsars. After several million years these neutron stars are no longer observed as radiopulsars, perhaps because of large magnetic field decay. However, a substantial fraction of the 10/sup 8/ old dead pulsars in the Galaxy are the most probable source for the isotropically distributed ..gamma..-ray burst detected several times per week at the earth. Some old neutron stars are spun-up by accretion from companions to be resurrected as rapidly spinning low magnetic field radiopulsars. 52 references, 6 figures, 3 tables.

Ruderman, M.

1984-09-01T23:59:59.000Z

420

STAR FORMATION IN ATOMIC GAS  

SciTech Connect

Observations of nearby galaxies have firmly established, over a broad range of galactic environments and metallicities, that star formation occurs exclusively in the molecular phase of the interstellar medium (ISM). Theoretical models show that this association results from the correlation between chemical phase, shielding, and temperature. Interstellar gas converts from atomic to molecular only in regions that are well shielded from interstellar ultraviolet (UV) photons, and since UV photons are also the dominant source of interstellar heating, only in these shielded regions does the gas become cold enough to be subject to Jeans instability. However, while the equilibrium temperature and chemical state of interstellar gas are well correlated, the timescale required to reach chemical equilibrium is much longer than that required to reach thermal equilibrium, and both timescales are metallicity-dependent. Here I show that the difference in timescales implies that, at metallicities below a few percent of the solar value, well shielded gas will reach low temperatures and proceed to star formation before the bulk of it is able to convert from atomic to molecular. As a result, at extremely low metallicities, star formation will occur in a cold atomic phase of the ISM rather than a molecular phase. I calculate the observable consequences of this result for star formation in low-metallicity galaxies, and I discuss how some current numerical models for H{sub 2}-regulated star formation may need to be modified.

Krumholz, Mark R., E-mail: krumholz@ucolick.org [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)

2012-11-01T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

Shape memory polymer actuator and catheter  

SciTech Connect

An actuator system is provided for acting upon a material in a vessel. The system includes an optical fiber and a shape memory polymer material operatively connected to the optical fiber. The shape memory polymer material is adapted to move from a first shape for moving through said vessel to a second shape where it can act upon said material.

Maitland, Duncan J. (Pleasant Hill, CA); Lee, Abraham P. (Walnut Creek, CA); Schumann, Daniel L. (Concord, CA); Matthews, Dennis L. (Moss Beach, CA); Decker, Derek E. (Byron, CA); Jungreis, Charles A. (Pittsburgh, PA)

2007-11-06T23:59:59.000Z

422

Quantifying Dynamic Stability of Genetic Memory Circuits  

Science Conference Proceedings (OSTI)

Bistability/Multistability has been found in many biological systems including genetic memory circuits. Proper characterization of system stability helps to understand biological functions and has potential applications in fields such as synthetic biology. ... Keywords: Dynamic stability, genetic memory, gene circuit, dynamic noise margin.

Yong Zhang; Peng Li; Garng Huang

2012-05-01T23:59:59.000Z

423

Memory Fault Modeling Trends: A Case Study  

Science Conference Proceedings (OSTI)

In recent years, embedded memories are the fastest growing segment of system on chip. They therefore have a major impact on the overall Defect per Million (DPM). Further, the shrinking technologies and processes introduce new defects that cause previously ... Keywords: data backgrounds, dynamic faults, fault coverage, fault models, memory tests, static faults

Said Hamdioui; Rob Wadsworth; John Delos Reyes; Ad J. Van De Goor

2004-06-01T23:59:59.000Z

424

Optimizing memory accesses for spatial computation  

Science Conference Proceedings (OSTI)

In this paper we present the internal representation and optimizations used by the CASH compiler for improving the memory parallelism of pointer-based programs. CASH uses an SSA-based representation for memory, which compactly summarizes both control-flow-and ...

Mihai Budiu; Seth C. Goldstein

2003-03-01T23:59:59.000Z

425

Optimum LDPC decoder: a memory architecture problem  

Science Conference Proceedings (OSTI)

This paper addresses a frequently overlooked problem: designing a memory architecture for an LDPC decoder. We analyze the requirements to support the codes defined in the IEEE 802.11n and 802.16e standards. We show a design methodology for a flexible ... Keywords: LDPC codes, low power architectures, memory optimization

Erick Amador; Renaud Pacalet; Vincent Rezard

2009-07-01T23:59:59.000Z

426

DOE - Office of Legacy Management -- Memorial Hospital - NY 0...  

Office of Legacy Management (LM)

Memorial Hospital - NY 0-16 FUSRAP Considered Sites Site: MEMORIAL HOSPITAL (NY.0-16 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name:...

427

Crystallographic Boundary in a Magnetic Shape Memory Material  

NLE Websites -- All DOE Office Websites (Extended Search)

Home Science Highlights Science Briefs Crystallographic Boundary in a Magnetic Shape Memory Material Crystallographic Boundary in a Magnetic Shape Memory Material Print...

428

Rebuilding it Better: Greensburg, Kansas, Kiowa County Memorial...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

it Better: Greensburg, Kansas, Kiowa County Memorial Hospital (Brochure) (Revised) Rebuilding it Better: Greensburg, Kansas, Kiowa County Memorial Hospital (Brochure) (Revised)...

429

Blue Earth-Nicollet-Faribault | Open Energy Information  

Open Energy Info (EERE)

Earth-Nicollet-Faribault Earth-Nicollet-Faribault Jump to: navigation, search Name Blue Earth-Nicollet-Faribault Place Minnesota Utility Id 1884 Utility Location Yes Ownership C NERC Location MRO NERC MRO Yes Activity Distribution Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates Residential: $0.1120/kWh Commercial: $0.0912/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Earth-Nicollet-Faribault&oldid=409059

430

Blue Canyon V Wind Farm | Open Energy Information  

Open Energy Info (EERE)

V Wind Farm V Wind Farm Jump to: navigation, search Name Blue Canyon V Wind Farm Facility Blue Canyon V Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon-EDPR Developer Horizon-EDPR Energy Purchaser Public Service of Oklahoma Location Caddo & Comanche Counties OK Coordinates 34.8582°, -98.54752° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.8582,"lon":-98.54752,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

431

Blue Ridge Elec Member Corp | Open Energy Information  

Open Energy Info (EERE)

Blue Ridge Elec Member Corp Blue Ridge Elec Member Corp Place North Carolina Utility Id 1889 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes Activity Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Cogeneration and Independent Power Porducers Industrial General Service - Single-Phase Commercial General Service - Three-Phase Commercial General Service Small Commercial - Single-Phase Commercial General Service Small Commercial - Three-Phase Commercial Growth Zone Pricing Industrial Industrial Economic Development Textile Industrial

432

Blue Spruce Farm Ana Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

Spruce Farm Ana Biomass Facility Spruce Farm Ana Biomass Facility Jump to: navigation, search Name Blue Spruce Farm Ana Biomass Facility Facility Blue Spruce Farm Ana Sector Biomass Location Vermont Coordinates 44.5588028°, -72.5778415° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.5588028,"lon":-72.5778415,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

433

Blue Ash, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Blue Ash, Ohio: Energy Resources Blue Ash, Ohio: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 39.2320029°, -84.3782734° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.2320029,"lon":-84.3782734,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

434

Aeromagnetic Survey At Blue Mountain Area (Fairbank Engineering, 2004) |  

Open Energy Info (EERE)

4) 4) Exploration Activity Details Location Blue Mountain Area Exploration Technique Aeromagnetic Survey Activity Date Usefulness not indicated DOE-funding Unknown Notes The airborne magnetometer and VLF-EM surveys carried out by Aerodat Limited, in 1988, covered the western flank of Blue Mountain including most of the geothermal lease area. The interpreted data (total field magnetic contours; calculated vertical magnetic gradient) indicate parallel sets of northerly, northeasterly, and northwesterly-trending structures that correspond well with the major fault sets identified from geologic mapping and interpreted drilling sections. Also, an elongate northerly-trending area of low magnetic gradient coincides closely with the area of intense hydrothermal alteration associated with the prominent north-south range

435

Blue Aquarius Fish Farms Aquaculture Low Temperature Geothermal Facility |  

Open Energy Info (EERE)

Aquarius Fish Farms Aquaculture Low Temperature Geothermal Facility Aquarius Fish Farms Aquaculture Low Temperature Geothermal Facility Jump to: navigation, search Name Blue Aquarius Fish Farms Aquaculture Low Temperature Geothermal Facility Facility Blue Aquarius Fish Farms Sector Geothermal energy Type Aquaculture Location Mecca, California Coordinates 33.571692°, -116.0772244° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[]}

436

FERN Blue Ribbon Wind Farm II* | Open Energy Information  

Open Energy Info (EERE)

II* II* Jump to: navigation, search Name FERN Blue Ribbon Wind Farm II* Facility FERN Blue Ribbon Wind Farm II* Sector Wind energy Facility Type Offshore Wind Facility Status Proposed Developer Fishermen's Energy Location Offshore from Atlantic City NJ Coordinates 39.183°, -74.428° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.183,"lon":-74.428,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

437

Improving Organizational Memories Through User Feedback  

E-Print Network (OSTI)

The benefits of an organizational memory are ultimately determined by the usefulness of the organizational memory as perceived by its users. Therefore, an improvement of an organizational memory should be measured in the added perceived usefulness. Unfortunately, the perceived usefulness has many impact factors (e.g., the precision of the user query, the urgency with which the user needs information, the coverage of the underlying knowledge base, the quality of the schema used to store knowledge, and the quality of the implementation). Hence, it is difficult to identify good starting points for improvement. This paper presents the goal-oriented method OMI (Organizational Memory Improvement) for improving an organizational memory incrementally from the user's point of view. It has been developed through several case studies and consists of a general usage model, a set of indicators for improvement potential, and a cause-effect model. At each step of the general usage model of OMI, pro...

Klaus-Dieter Althoff; Markus Nick; Carsten Tautz

1999-01-01T23:59:59.000Z

438

Dehydrated Prussian Blues for CO2 Storage and Separation Applications  

Science Conference Proceedings (OSTI)

Adsorption isotherms of pure gases present in flue and natural gas including CO2, N2, CH4 and water were studied using prussian blues of chemical formula M3[Co(CN)6]2 (M = Cu, Ni, Mn). These materials adsorbed 8-12 wt % of CO2 at room temperature and 1 bar of pressure with heats of adsorption ranging from 6 to 16 kcal/mol.

Motkuri, Radha K.; Thallapally, Praveen K.; McGrail, B. Peter; Ghorishi, Behrooz S.

2010-08-13T23:59:59.000Z

439

New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars  

E-Print Network (OSTI)

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B-type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three beta Cephei stars and two stars suspected to be beta Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3sigma has been diagnosed in two normal B-type stars, the nitrogen-rich early B-type star HD52089 and in the B5 IV star HD153716. Roughly one third of beta Cephei stars have detected magnetic fields: Out of 13 beta Cephei stars studied to date with FORS1, four stars possess weak magnetic fields, and out of the sample of six suspected beta Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: roughl...

Hubrig, S; De Cat, P; Schller, M; Morel, T; Ilyin, I

2009-01-01T23:59:59.000Z

440

SNAPSHOT … THE ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Fall 2008 Introduction At mid-year 2008*, commercial and industrial (C&I) leaders continued to make great progress in their efforts to improve energy efficiency and reduce greenhouse gas emissions across their buildings and facilities. In the first six months of 2008, key indicators of progress have already exceeded activity levels from 2007. More than 1,500 organizations and individuals now participate in the ENERGY STAR Challenge Close to 2 billion new square feet of commercial building floor space rated in the first half of the year bringing the total to about 9.5 billion over 71,000 buildings Labels awarded through June 2008 almost equal the 2007 total, with about 5,000 facilities now qualified as ENERGY STAR ENERGY STAR Leader activity on the rise this year; almost 60 commercial partners achieved key

Note: This page contains sample records for the topic "blue star memorial" 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

ENERGY STAR Score for Warehouses  

NLE Websites -- All DOE Office Websites (Extended Search)

Warehouses in the United States Page 1 Warehouses in the United States Page 1 ENERGY STAR Score for Warehouses in the United States Technical Reference OVERVIEW The ENERGY STAR Score for warehouses applies to unrefrigerated or refrigerated buildings that are used to store goods, manufactured products, merchandise or raw materials. The objective of the ENERGY STAR score is to provide a fair assessment of the energy performance of a property relative to its peers, taking into account the climate, weather, and business activities at the property. To identify the aspects of building activity that are significant drivers of energy use and then normalize for those factors, a statistical analysis of the peer building population is

442

Toy Stars in two dimensions  

E-Print Network (OSTI)

Toy Stars are gas masses where the compressibility is treated without approximations but gravity is replaced by a force which, for any pair of masses, is along their line of centres and proportional to their separation. They provide an invaluable resource for testing the suitability of numerical codes for astrophysical gas dynamics. In this paper we derive the equations for both small amplitude oscillations and non linear solutions for rotating and pulsating Toy Stars in two dimensions, and show that the solutions can be reduced to a small number of ordinary differential equations. We compare the accurate solutions of these equations with Smoothed Particle Hydrodynamics (SPH) simulations. The two dimensional Toy Star solutions are found to provide an excellent benchmark for SPH algorithms, highlighting many of the strengths and also some weaknesses of the method.

J. J. Monaghan; D. J. Price

2005-10-25T23:59:59.000Z

443

Nuclear Physics of Neutron Stars  

E-Print Network (OSTI)

Understanding the equation of state (EOS) of cold nuclear matter, namely, the relation between the pressure and energy density, is a central goal of nuclear physics that cuts across a variety of disciplines. Indeed, the limits of nuclear existence, the collision of heavy ions, the structure of neutron stars, and the dynamics of core-collapse supernova, all depend critically on the equation of state of hadronic matter. In this contribution I will concentrate on the special role that nuclear physics plays in constraining the EOS of cold baryonic matter and its impact on the properties of neutron stars.

J. Piekarewicz

2009-01-28T23:59:59.000Z

444

Photos and graphics | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

guidelines Refer to the ENERGY STAR Identity Guidelines for proper usage of the ENERGY STAR and Portfolio Manager marks. Graphics Click on a graphic to bring up a larger...

445

Note on star-autonomous comonads  

E-Print Network (OSTI)

We develop an alternative approach to star-autonomous comonads via linearly distributive categories. It is shown that in the autonomous case the notions of star-autonomous comonad and Hopf comonad coincide.

Pastro, Craig

2010-01-01T23:59:59.000Z

446

Industrial energy management information center | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

447

Alliance Star Energy LLC | Open Energy Information  

Open Energy Info (EERE)

Star Energy LLC Jump to: navigation, search Name Alliance Star Energy LLC Place California Utility Id 56929 References EIA Form EIA-861 Final Data File for 2010 - File220101...

448

Solar Star NAFB LLC | Open Energy Information  

Open Energy Info (EERE)

Star NAFB LLC Jump to: navigation, search Name Solar Star NAFB LLC Place Nevada Utility Id 56203 References EIA Form EIA-861 Final Data File for 2010 - File220101 LinkedIn...

449

Cold quark matter in compact stars  

Science Conference Proceedings (OSTI)

We used an equation of state for the cold quark matter to the study of properties of quark stars. We also discuss the absolute stability of quark matter and compute the mass-radius relation for self-bound stars.

Franzon, B.; Fogaca, D. A.; Navarra, F. S. [Instituto de Fisica, Universidade de Sao Paulo Rua do Matao, Travessa R, 187, 05508-090 Sao Paulo, SP (Brazil); Horvath, J. E. [Instituto de Astronomia, Geofisica e Ciencias Atmosfericas, Universidade de Sao Paulo, Rua do Matao, 1226, 05508-090, Sao Paulo, SP (Brazil)

2013-03-25T23:59:59.000Z

450

ENERGY STAR Score for Data Centers  

NLE Websites -- All DOE Office Websites (Extended Search)

Data Centers in the United States Page 1 ENERGY STAR Score for Data Centers in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Data Centers applies to...

451

Advance your energy program | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

corporate energy directors is without parallel. Join ENERGY STAR and get connected to the learning curve. Learn about world-class energy programs. EPA has profiled key ENERGY STAR...

452

Energy strategy for the future | ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

453

ENERGY STAR Industrial Plant Certification: Professional Engineers...  

NLE Websites -- All DOE Office Websites (Extended Search)

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

454

New lambda Bootis stars with a shell  

E-Print Network (OSTI)

We publish here the second part of our spectroscopic survey at high dispersion of some known and suspected lambda Bootis stars with a view to detecting circumstellar shell features. Eight stars of our sample exhibit such features. These stars are fast rotators, a result which is in line with Holweger and Rentzsch-Holm's study (1995). The analysis of the photometric data has allowed us to confirm the exclusion of a few stars misclassified from the lambda Bootis group.

B. Hauck; D. Ballereau; J. Chauville

1997-09-02T23:59:59.000Z

455

Black Stars and Gamma Ray Bursts  

E-Print Network (OSTI)

Stars that are collapsing toward forming a black hole but are frozen near the Schwarzschild horizon are termed ``black stars''. Collisions of black stars, in contrast to black hole collisions, may be sources of gamma ray bursts, whose basic parameters are estimated quite simply and are found to be consistent with observed gamma ray bursts. Black star gamma ray bursts should be preceded by gravitational wave emission similar to that from the coalescence of black holes.

Tanmay Vachaspati

2007-06-08T23:59:59.000Z

456

Join ENERGY STAR as a partner | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Join ENERGY STAR as a partner Join ENERGY STAR as a partner Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can ENERGY STAR help your business? Get started Join ENERGY STAR as a partner Service and Product Provider associations partnering with ENERGY STAR ENERGY STAR service & product provider training series Service and product provider's marketing toolkit

457

Theory of cooling neutron stars versus observations  

E-Print Network (OSTI)

We review current state of neutron star cooling theory and discuss the prospects to constrain the equation of state, neutrino emission and superfluid properties of neutron star cores by comparing the cooling theory with observations of thermal radiation from isolated neutron stars.

Yakovlev, D G; Kaminker, A D; Potekhin, A Yu

2007-01-01T23:59:59.000Z

458

Diagnosability of star graphs with missing edges  

Science Conference Proceedings (OSTI)

In this paper, we study the system diagnosis on an n-dimensional star under the comparison model. Following the concept of local diagnosability [3], the strong local diagnosability property [7] is discussed; this property describes the equivalence of ... Keywords: Comparison diagnosis model, Extended star structure, Local diagnosability, MM* diagnosis model, Star graph, Strong local diagnosability property

Chieh-Feng Chiang; Guo-Huang Hsu; Lun-Min Shih; Jimmy J. M. Tan

2012-04-01T23:59:59.000Z

459

Asteroseismology of chemically peculiar stars  

E-Print Network (OSTI)

Pulsational variability is observed in several types of main sequence stars with anomalous chemical abundances. In this contribution I summarize the relationship between pulsations and chemical peculiarities, giving special emphasis to rapid oscillations in magnetic Ap stars. These magneto-acoustic pulsators provide unique opportunities to study the interaction of pulsations, chemical inhomogeneities, and strong magnetic fields. Time-series monitoring of rapidly oscillating Ap stars using high-resolution spectrometers at large telescopes and ultra-precise space photometry has led to a number of important breakthroughs in our understanding of these interesting objects. Interpretation of the roAp frequency spectra has allowed constraining fundamental stellar parameters and probing poorly known properties of the stellar interiors. At the same time, investigation of the pulsational wave propagation in chemically stratified atmospheres of roAp stars has been used as a novel asteroseismic tool to study pulsations as a function of atmospheric height and to map in detail the horizontal structure of the magnetically-distorted p-modes.

O. Kochukhov

2008-12-01T23:59:59.000Z

460

A Quantum Information Retrieval Approach to Memory  

E-Print Network (OSTI)

As computers approach the physical limits of information storable in memory, new methods will be needed to further improve information storage and retrieval. We propose a quantum inspired vector based approach, which offers a contextually dependent mapping from the subsymbolic to the symbolic representations of information. If implemented computationally, this approach would provide exceptionally high density of information storage, without the traditionally required physical increase in storage capacity. The approach is inspired by the structure of human memory and incorporates elements of Gardenfors' Conceptual Space approach and Humphreys et al.'s matrix model of memory.

Kirsty Kitto; Peter Bruza; Liane Gabora

2013-10-11T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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

Crystallographic attributes of a shape-memory alloy  

SciTech Connect

Shape-memory alloys are attractive for many potential applications. In an attempt to provide ideas and guidelines for the development of new shape-memory alloys, this paper reports on a series of investigations that examine the reasons in the crystallography that made (i) shape-memory alloys special amongst martensites and (ii) Nickel-Titanium special among shape-memory alloys.

Bhattacharya, K. [California Inst. of Tech., Pasadena, CA (United States). Div. of Engineering and Applied Science

1999-01-01T23:59:59.000Z

462

L6: Memory Hierarchy Optimization III, Bandwidth Optimization  

E-Print Network (OSTI)

wherever there are capacity limitations ­ Between grids if total data exceeds global memory capacity will "spill" data to local memory · Local memory ­ Deals with capacity limitations of registers and shared ­ Across thread blocks if shared data exceeds shared memory capacity (also to partition computation across

Hall, Mary W.

463

Journal of Experimental Psychology: Learning, Memory, and Cognition  

E-Print Network (OSTI)

explicit and implicit tests of memory (for reviews, see Graf & Masson, 1993; Lewandosky, Dunn, & Kirsner

Shimamura, Arthur P.

464

Persistent systems techniques in forensic acquisition of memory  

Science Conference Proceedings (OSTI)

In this paper we discuss how operating system design and implementation influence the methodology for computer forensics investigations, with the focus on forensic acquisition of memory. In theory the operating system could support such investigations ... Keywords: Computer forensics, Memory acquisition, Memory forensics, Memory persistence, Persistent operating systems

Ewa Huebner; Derek Bem; Frans Henskens; Mark Wallis

2007-09-01T23:59:59.000Z

465

Memory energy management for an enterprise decision support system  

Science Conference Proceedings (OSTI)

Energy efficiency is an important factor in designing and configuring enterprise servers. In these servers, memory may consume 40% of the total system power. Different memory configurations (sizes, numbers of ranks, speeds, etc.) can have significant ... Keywords: memory power management, power-aware memory

Karthik Kumar; Kshitij Doshi; Martin Dimitrov; Yung-Hsiang Lu

2011-08-01T23:59:59.000Z

466

Architecting phase change memory as a scalable dram alternative  

Science Conference Proceedings (OSTI)

Memory scaling is in jeopardy as charge storage and sensing mechanisms become less reliable for prevalent memory technologies, such as DRAM. In contrast, phase change memory (PCM) storage relies on scalable current and thermal mechanisms. To exploit ... Keywords: dram alternative, endurance, energy, pcm, performance, phase change memory, power, scalability

Benjamin C. Lee; Engin Ipek; Onur Mutlu; Doug Burger

2009-06-01T23:59:59.000Z

467

Cork: dynamic memory leak detection for garbage-collected languages  

Science Conference Proceedings (OSTI)

A memory leak in a garbage-collected program occurs when the program inadvertently maintains references to objects that it no longer needs. Memory leaks cause systematic heap growth, degrading performance and resulting in program crashes after ... Keywords: dynamic, garbage collection, memory leak detection, memory leaks, runtime analysis

Maria Jump; Kathryn S. McKinley

2007-01-01T23:59:59.000Z

468

Characterizing the Memory Behavior of Compiler-Parallelized Applications  

Science Conference Proceedings (OSTI)

AbstractCompiler-parallelized applications are increasing in importance as moderate-scale multiprocessors become common. This paper evaluates how features of advanced memory systems (e.g., longer cache lines) impact memory system behavior for applications ... Keywords: Parallelizing compilers, memory hierarchies, shared-memory multiprocessors, cache performance, false and true sharing, parallelism granularity.

Evan Torrie; Margaret Martonosi; Chau-Wen Tseng; Mary W. Hall

1996-12-01T23:59:59.000Z

469

Dynamic tracking of page miss ratio curve for memory management  

Science Conference Proceedings (OSTI)

Memory can be efficiently utilized if the dynamic memory demands of applications can be determined and analyzed at run-time. The page miss ratio curve(MRC), i.e. page miss rate vs. memory size curve, is a good performance-directed metric to serve this ... Keywords: memory management, power management, resource allocation

Pin Zhou; Vivek Pandey; Jagadeesan Sundaresan; Anand Raghuraman; Yuanyuan Zhou; Sanjeev Kumar

2004-12-01T23:59:59.000Z

470

Shared Memory Programming in Metacomputing Environments: The Global Array Approach  

Science Conference Proceedings (OSTI)

The performance of the Global Array shared-memory nonuniform memory-access programming model is explored in a wide-area-network (WAN) distributed supercomputer environment. The Global Array model is extended by introducing a concept of mirrored arrays ... Keywords: Metacomputing, NUMA memory architecture, distributed arrays, global arrays, shared-memory programming

Jarek Nieplocha; Robert Harrison

1997-10-01T23:59:59.000Z

471

On Working Memory: Its organization and capacity limits  

E-Print Network (OSTI)

64 iii 6.2 Working memory capacity10 1.4 Capacity limits of workingcapacity . . . . . . . . . . . . . . . . . . . . . . . . . .

Lara, Antonio Homero

2010-01-01T23:59:59.000Z

472

Building Energy Software Tools Directory: Star Perfomer  

NLE Websites -- All DOE Office Websites (Extended Search)

Star Perfomer Star Perfomer Star Perfomer logo. Outlines simple steps to help office building owners, managers and tenants improve their greenhouse and energy efficiency performance, simply by asking some straightforward questions about the size, operating hours, current performance and equipment standards of the building. Star Performer is a diagnostic tool that uses the current operational energy performance of the building measured against a national benchmark, obtained through the Australian Building Greenhouse Rating scheme (see links below), as a basis for making recommendations. The tool covers all areas of the building which affect operational energy performance, including building fabric, equipment and operational practices. Star Perfomer will point you in the right direction and give

473

NLTE wind models of hot subdwarf stars  

E-Print Network (OSTI)

We calculate NLTE models of stellar winds of hot compact stars (central stars of planetary nebulae and subdwarf stars). The studied range of subdwarf parameters is selected to cover a large part of these stars. The models predict the wind hydrodynamical structure and provide mass-loss rates for different abundances. Our models show that CNO elements are important drivers of subdwarf winds, especially for low-luminosity stars. We study the effect of X-rays and instabilities on these winds. Due to the line-driven wind instability, a significant part of the wind could be very hot.

Krticka, Jiri; 10.1007/s10509-010-0385-z

2010-01-01T23:59:59.000Z

474

Contact Manufacturing Demonstration Facility Craig Blue, Ph.D.  

NLE Websites -- All DOE Office Websites (Extended Search)

Manufacturing Demonstration Facility Craig Blue, Ph.D. Director, Manufacturing Demonstration Facility (865) 574-4351 blueca@ornl.gov INNOVATIONS IN MANUFACTURING www.ornl.gov/manufacturing Advanced Manufacturing Next-Generation Manufacturing As the nation's premier research laboratory, Oak Ridge National Laboratory is one of the world's most capable resources for transforming the next generation of scientific discovery into solutions for rebuilding and revitalizing America's manufacturing industries. These industries call upon ORNL's expertise in materials synthesis, characterization, and process technology to reduce risk and accelerate the development and deployment of innovative energy-efficient manufacturing processes and materials targeting products of the future.

475

Cavity Enhancement of Single Quantum Dot Emission in the Blue  

E-Print Network (OSTI)

in the blue and green spectral region by changing the alloy content. The access to this wavelength range may prove particularly useful for free-space cryptography. It also corresponds to the range where the commercially avail- able ultrafast single... . Christmann, D. Simeonov, R. Butte, E. Feltin, J.-F. Carlin, N. Grandjean, Appl. Phy. Lett. 89, 261101 (2006) 4. F. Semond, I.R. Sellers, F. Natali, D. Byrne, M. Leroux, J. Massies, N. Ollier, J. Leymarie, P. Disseix, A. Vasson, Appl. Phys. Lett. 87, 021102...

2009-12-27T23:59:59.000Z

476

Blue light emitting diode internal and injection efficiency  

Science Conference Proceedings (OSTI)

A simple experimental method of light emitting diode(LED) injection efficiency (IE) determination was suggested. IE and internal quantum efficiency(IQE) calculation is an actual and difficult problem in LED science. In this paper IE and IQE of blue LEDs were determined separately. The method is based on electroluminescence data fitting by the modified rate equation model. Efficiency droop caused by Auger recombination and poor injection were taken into account. Only one reasonable assumption was accepted during the calculations: IE tends to 1 at low current densities.

Ilya E. Titkov; Denis A. Sannikov; Young-Min Park; Joong-Kon Son

2012-01-01T23:59:59.000Z

477

Why Has the Land Memory Changed?  

Science Conference Proceedings (OSTI)

The land memory refers to an interseasonal predictability of the summer monsoon rainfall in the southwestern United States, describing a relationship of the summer monsoon rainfall anomaly with anomalies in the antecedent winter season snow and ...

Qi Hu; Song Feng

2004-08-01T23:59:59.000Z

478

The Neural Substrate of Orientation Working Memory  

Science Conference Proceedings (OSTI)

We have used positron emission tomography (PET) to identify the neural substrate of two major cognitive components of working memory (WM), maintenance and manipulation of a single elementary visual attribute, i.e., the orientation of a grating presented ...

L. Cornette; P. Dupont; E. Salmon; Guy A. Orban

2001-08-01T23:59:59.000Z

479

30 days to a more powerful memory  

Science Conference Proceedings (OSTI)

With phones ringing off the hook, constantly changing to-do lists, and increasingly complicated schedules, having a good memory has become more important than ever. Drawing on the latest research from cognitive experts and psychologists, 30 Days to a ...

Gini Scott

2007-04-01T23:59:59.000Z

480

Revisiting parallel rendering for shared memory machines  

Science Conference Proceedings (OSTI)

Increasing the core count of CPUs to increase computational performance has been a significant trend for the better part of a decade. This has led to an unprecedented availability of large shared memory machines. Programming paradigms and systems are ...

B. Nouanesengsy; J. Ahrens; J. Woodring; H. Shen

2011-04-01T23:59:59.000Z

Note: This page contains sample records for the topic "blue star memorial" 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.


481

Commercialization of germanium based nanocrystal memory  

E-Print Network (OSTI)

This thesis explores the commercialization of germanium-based nanocrystal memories. Demand for smaller and faster electronics and embedded systems supports the development of high-density, low-power non-volatile electronic ...

Seow, Kian Chiew

2007-01-01T23:59:59.000Z

482

A strategy of memory : Suzhou, China  

E-Print Network (OSTI)

The thesis is trying to establish a strategy of memory for the urban preservation of old cities, like Suzhou, within the context of the rapid growing economy in Southern China. The general attitude towards the problem ...

Chang, Ping Hung

1995-01-01T23:59:59.000Z

483

Supermassive black holes from supermassive stars  

NLE Websites -- All DOE Office Websites (Extended Search)

Supermassive black holes from supermassive stars Supermassive black holes from supermassive stars 1663 Los Alamos science and technology magazine Latest Issue:November 2013 All Issues » submit Supermassive black holes from supermassive stars Supermassive stars in the early universe gave supermassive black holes a head start March 25, 2013 simulations suggest that star formation conditions back then allowed the first stars to become supermassive themselves In this simulation, a black hole that was just formed by the collapse of a supermassive star is surrounded by a distribution of gas (color indicates density). Because the black hole (located at the center but too small to see) grows by consuming the available gas, simulations like this one help determine how quickly the black hole can grow. The progenitor of this black

484

ORISE: Voluntary Protection Program (VPP) Star Status  

NLE Websites -- All DOE Office Websites (Extended Search)

Voluntary Protection Program (VPP) Star Status Voluntary Protection Program (VPP) Star Status Within the U.S. Department of Energy's (DOE) Voluntary Protection Program (VPP), there are three levels of recognition: STAR, MERIT and DEMONSTRATION. Contractors' programs that meet the requirements for outstanding safety and health programs, earn VPP STAR status-the highest achievement level. In December of 2003, the Oak Ridge Institute for Science and Education (ORISE) first earned STAR distinction following a comprehensive evaluation of its application for the VPP program. At that time, ORISE was just the 21st DOE site and the first in Tennessee to earn such exemplary recognition. In 2011 ORISE received its seventh consecutive Star of Excellence award. Today, ORISE is one of more than two dozen DOE sites to achieve VPP STAR

485

Energy Star Rebate Finder | Open Energy Information  

Open Energy Info (EERE)

Energy Star Rebate Finder Energy Star Rebate Finder Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Energy Star Rebate Finder Agency/Company /Organization: United States Environmental Protection Agency Sector: Energy Focus Area: Energy Efficiency Phase: Evaluate Options, Prepare a Plan Resource Type: Online calculator User Interface: Mobile Device Website: m.epa.gov/apps/energy.html Web Application Link: m.epa.gov/apps/energy.html Cost: Free Energy Star Rebate Finder Screenshot References: EPA[1] Logo: Energy Star Rebate Finder Find special offers and rebates from Energy Star partners by entering your zip code. Overview To encourage customers to buy energy efficient products, Energy Star partners occasionally sponsor special offers, such as sales tax exemptions or credits, or rebates on qualified products. Partners also occasionally

486

Green Star Alternative Energy | Open Energy Information  

Open Energy Info (EERE)

Green Star Alternative Energy Green Star Alternative Energy Jump to: navigation, search Name Green Star Alternative Energy Place San Diego, California Zip 92108 Sector Wind energy Product A US-based wind energy project developer. References Green Star Alternative Energy[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Green Star Alternative Energy is a company located in San Diego, California . References ↑ "Green Star Alternative Energy" Retrieved from "http://en.openei.org/w/index.php?title=Green_Star_Alternative_Energy&oldid=346056" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link

487

Build Your Business with ENERGY STAR  

NLE Websites -- All DOE Office Websites (Extended Search)

Service and Product Providers: Service and Product Providers: Build Your Business with ENERGY STAR ® Let ENERGY STAR Be Your Market Advantage Look to ENERGY STAR to help you bring value to your customers and more sales to your organization. Service and Product Providers (SPPs) are integral in helping existing commercial buildings use energy more efficiently. Partnering with ENERGY STAR provides you with access to free tools and resources to help you devise and implement energy- efficient strategies that are right for your customers: > Use the ENERGY STAR Brand to Enhance Your Credibility: Use the nationally recognized ENERGY STAR partner logo on your promotional materials to symbolize your commitment to delivering energy efficiency and financial savings to customers. Help customers build their reputation as environmental and social leaders through work with an ENERGY STAR SPP partner.

488

Cultural differences on the children's memory scale  

E-Print Network (OSTI)

Memory is an essential component for learning. Deficits in verbal short-term memory (STM) and working memory (WM) are thought to hinder language learning, reading acquisition, and academic achievement. The Childrens Memory Scale (CMS) is an assessment instrument used to identify memory and learning deficits and strengths in children ages five through 16. This study investigated the impact of culture and parent educational level (PEL) on student performance on the Childrens Memory Scale using the CMS standardization data. The major question addressed was: Will CMS subtest performance differ significantly between ethnic groups or as a function of PEL? The results of this study support a relationship between STM and WM performance and culture. Culture as defined by ethnicity minimally impacted student subtest performance on the CMS when PEL was taken into account. In contrast, PEL was significantly associated with student subtest performance within each ethnic group. Student subtest performance improved with each increase in PEL regardless of ethnicity. CMS subtest performance of Hispanic and African American students was most affected by PEL; however, no difference occurred in subtest performance by ethnicity or as a function of PEL for African American and Hispanic students on the Family Pictures subtest which examines visual and auditory memory processes through recall of everyday life tasks in meaningful context. Although statistical significance was found between CMS subtest performance and cultural factors, the effect sizes were mainly in the small range and variance was not specific to any one subtest. Larger effect sizes were found on verbal subtests which in previous studies have been found to be most impacted by quality of schooling and lower PELs. Mean score differences did not exceed one standard deviation with the exception of one subtest. The results of this study provide a better understanding of the effect of culture and PEL on memory and learning.

Cash, Deborah Dyer

2007-08-01T23:59:59.000Z

489

Distributed trace using central performance counter memory  

SciTech Connect

A plurality of processing cores, are central storage unit having at least memory connected in a daisy chain manner, forming a daisy chain ring layout on an integrated chip. At least one of the plurality of processing cores places trace data on the daisy chain connection for transmitting the trace data to the central storage unit, and the central storage unit detects the trace data and stores the trace data in the memory co-located in with the central storage unit.

Satterfield, David L.; Sexton, James C.

2013-01-22T23:59:59.000Z

490

Distributed trace using central performance counter memory  

Science Conference Proceedings (OSTI)

A plurality of processing cores, are central storage unit having at least memory connected in a daisy chain manner, forming a daisy chain ring layout on an integrated chip. At least one of the plurality of processing cores places trace data on the daisy chain connection for transmitting the trace data to the central storage unit, and the central storage unit detects the trace data and stores the trace data in the memory co-located in with the central storage unit.

Satterfield, David L; Sexton, James C

2013-10-22T23:59:59.000Z

491

T-713: Blue Coat Reporter Directory Traversal Flaw | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

3: Blue Coat Reporter Directory Traversal Flaw 3: Blue Coat Reporter Directory Traversal Flaw T-713: Blue Coat Reporter Directory Traversal Flaw September 9, 2011 - 10:47am Addthis PROBLEM: A vulnerability was reported in Blue Coat Reporter. A remote user can view files on the target system and gain full control of the target application. PLATFORM: All pre-9.3 versions of Reporter installed on a Windows server are vulnerable. ABSTRACT: Blue Coat Reporter Directory Traversal Flaw Lets Remote Users Gain Full Control. reference LINKS: Blue Coat Security Advisory ID: SA60 SecurityTracker Alert ID: 1026023 About Path Traversal IMPACT ASSESSMENT: High Discussion: Reporter installed on a Windows server is vulnerable to an HTTP directory traversal attack. An unauthenticated user can browse the file system and read any file. Data from these files can be used by an attacker to gain

492

STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain  

Open Energy Info (EERE)

STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain Geothermal Power Facility Jump to: navigation, search OpenEI Reference LibraryAdd to library General: STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain Geothermal Power Facility Author BRIAN D. FAIRBANK Published Publisher Not Provided, 2012 DOI Not Provided Check for DOI availability: http://crossref.org Online Internet link for STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain Geothermal Power Facility Citation BRIAN D. FAIRBANK. 2012. STATEMENT OF BRIAN D. FAIRBANK Nevada Geothermal Power Inc.'s Blue Mountain Geothermal Power Facility. N/Ap. Retrieved from "http://en.openei.org/w/index.php?title=STATEMENT_OF_BRIAN_D._FAIRBANK_Nevada_Geothermal_Power_Inc.%27s_Blue_Mountain_Geothermal_Power_Facility&oldid=682760

493

ULAS J141623.94+134836.3: A BLUE T DWARF COMPANION TO A BLUE L DWARF  

SciTech Connect

We confirm the substellar nature of ULAS J141623.94+134836.3 (aka SDSS J1416+1348B), a common proper motion companion to the blue L dwarf SDSS J141624.08+134826.7 identified by Burningham et al. and Scholz. Low-resolution 0.8-2.4 {mu}m spectroscopy obtained with the Infrared Telescope Facility/SpeX shows strong H{sub 2}O and CH{sub 4} absorption bands, consistent with a T7.5 spectral type, and we see possible indications of NH{sub 3} absorption in the 1.0-1.3 {mu}m region. More importantly, the spectrum of SDSS J1416+1348B shows a broadened Y-band peak and highly suppressed K-band flux, both indicative of high surface gravity and/or subsolar metallicity. These traits are verified through spectral model fits, from which we derive atmospheric parameters T{sub eff} = 650 {+-} 60 K, log g = 5.2 {+-} 0.4 cgs, [M/H] {<=} -0.3, and K{sub zz} = 10{sup 4} cm{sup 2} s{sup -1}, the temperature being significantly warmer than that estimated by Burningham et al. These fits also indicate a model-dependent spectroscopic distance of 10.6{sup +3.0}{sub -2.8} pc for SDSS J1416+1348B, formally consistent with the 7.9 {+-} 1.7 pc astrometric distance for SDSS J1416+1348A from Scholz. The common peculiarities of these two co-spatial, co-moving sources suggest that their unusual blue colors-and those of other blue L and T dwarfs in general-arise from age/gravity or metallicity effects, rather than cloud properties alone.

Burgasser, Adam J. [Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093 (United States); Looper, Dagny; Rayner, John T., E-mail: aburgasser@ucsd.ed [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

2010-06-15T23:59:59.000Z

494

Blue Sky Green Field Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Green Field Wind Farm Green Field Wind Farm Jump to: navigation, search Name Blue Sky Green Field Wind Farm Facility Blue Sky Green Field Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner We Energies Developer We Energies Energy Purchaser We Energies Location Fond du Lac County WI Coordinates 43.908549°, -88.305384° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.908549,"lon":-88.305384,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

495

Magnetization of neutron star matter  

E-Print Network (OSTI)

The magnetization of neutron star matter in magnetic fields is studied by employing the FSUGold interaction. It is found that the magnetic susceptibilities of the charged particles (proton, electron and muon) can be larger than that of neutron. The effects of the anomalous magnetic moments (AMM) of each component on the magnetic susceptibility are examined in detail. It is found that the proton and electron AMM affect their respective magnetic susceptibility evidently in strong magnetic fields. In addition, they are the protons instead of the electrons that contribute most significantly to the magnetization of the neutron star matter in a relative weak magnetic field, and the induced magnetic field due to the magnetization can be appear to be very large. Finally, the effect of the density-dependent symmetry energy on the magnetization is discussed.

Dong, Jianmin; Gu, Jianzhong

2013-01-01T23:59:59.000Z

496

ENERGY STAR SNAPSHOT - Spring 2009  

NLE Websites -- All DOE Office Websites (Extended Search)

Measuring Progress in the Measuring Progress in the Commercial and Industrial Sectors Fall 2009 Summary By mid-year 2009, key commercial and industrial organizations have already surpassed their 2008 efforts to improve energy performance and reduce greenhouse gas emissions: * More buildings have been rated at mid year 2009 than in all of last year. This brings the total number of buildings with energy performance ratings to more than 97,000. * Nearly 1,850 buildings have earned the ENERGY STAR in 2009, ahead of the 2008 mid-year total. * Almost 30 organizations, mostly among our nation's public school districts, have already achieved significant portfolio-wide energy improvements or top performance. The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance indicators behind

497

DELTA SCUTI, SX PHOENICIS, AND RR LYRAE STARS IN GALAXIES AND GLOBULAR CLUSTERS  

Science Conference Proceedings (OSTI)

The distances to four galaxies and two globular clusters which are derived with the aid of period-luminosity and period-color relations of {delta} Scuti and SX Phe stars are compared to the distances derived by other methods, in particular RR Lyrae stars. We examine the luminosities of horizontal branch or RR Lyrae stars in Oosterhoff I and II globular clusters. Observational data from a variety of sources indicate a discontinuous jump of {approx}0.2 mag in the luminosities of RR Lyrae variables at [Fe/H] {approx} -1.5 as we transition from Oosterhoff I to Oosterhoff II clusters. If Oosterhoff I clusters have RR Lyrae variables with average M{sub V} values of M{sub V} = 0.53 mag at [Fe/H] = -1.5, it implies that RR Lyrae stars in Oosterhoff II clusters average M{sub V} values are {approx}0.34 mag. Unlike the Oosterhoff I clusters which show an increase in the V luminosity of RR Lyrae stars as [Fe/H] becomes smaller, little or no change in the V luminosity of RR Lyrae variables is evident in Oosterhoff II clusters in the interval of [Fe/H] from -1.5 to -2.2. We find distance moduli found with RR Lyrae variables agree to {solar-metallicity {delta} Scuti stars with ages of 150 Myr to 1 Gyr) in the Large Magellanic Cloud (LMC), Small Magellanic Cloud, and the central region of the Fornax (dSph) galaxies. We also find an older population of metal-poor {delta} Scuti variables (SX Phe stars) in the LMC and Fornax galaxies. The Carina dSph is unique in that only an old population of metal-poor {delta} Scuti variables is evident. No evidence of recent {delta} Scuti star formation is found. The minimum periods observed for the SX Phe variables (blue stragglers) in the globular clusters M55 and {omega} Cen indicate that they could have been formed in a burst of metal-poor single star formation in the last 2.9-6 Gyr. If formed by the more acceptable scenario of stellar mergers, it is likely that the merged remnant resembles a normal star in a relatively advanced stage of main-sequence evolution with an enriched He core and ordinary He envelope. We present equations to calculate intrinsic-color indices for {delta} Scuti, SX Phe, and RR Lyrae stars at mean light. Finally, we show that the fundamental-radial-pulsating stars ({delta} Sct and SX Phe variables) have larger average light amplitudes than the first-overtone pulsating variables. The fundamental metal-poor variables (SX Phe stars) have the largest average and individual amplitudes.

McNamara, D. H., E-mail: harold_mcnamara@byu.edu [Department of Physics and Astronomy, Brigham Young University, Provo, UT 84602 (United States)

2011-10-15T23:59:59.000Z

498

Home Performance with Energy Star  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

- HPwES - HPwES Home Performance with ENERGY STAR Ely Jacobsohn U.S. Department of Energy Ely.jacobsohn@ee.doe.gov, 202-287-1333 April 3, 2013 2 | Building Technologies Office eere.energy.gov Purpose and Objectives: Problem Statement Works to advance the Department's and Administration's energy-related goals in the residential sector Face challenging and often conflicting mandates to save energy, meet environmental goals, and satisfy needs of

499

Find ENERGY STAR certified buildings and plants | ENERGY STAR Buildings &  

NLE Websites -- All DOE Office Websites (Extended Search)

» Buildings & Plants » Buildings & Plants » About us » Find ENERGY STAR certified buildings and plants Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants Registry of ENERGY STAR certified buildings and plants

500

The Ocean and Coastal Conservation Guide: The Blue Movement Directory (2005-2006)  

E-Print Network (OSTI)

Magazine, California Coast & Ocean, California Wild, andReview: The Ocean and Coastal Conservation Guide: The BlueMiller San Francisco, USA The Ocean and Coastal Conservation

Miller, Ryder W.

2006-01-01T23:59:59.000Z