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


1

Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site  

Office of Legacy Management (LM)

3-TAC 3-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project January through March 2003 Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site April 2003 Grand Junction Office U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy DE-AC13-02GJ79491 Approved for public release; distribution is unlimited. N0060800 GJO-2003-433-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project Quarterly Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site January through March 2003 April 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107

2

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

Young - Rainey Star Center Young - Rainey Star Center 110406202 Accutest Job Number: F30886 Sampling Date: 04/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

3

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

Young - Rainey Star Center Young - Rainey Star Center 110406202 Accutest Job Number: F35489 Sampling Date: 10/05/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

4

S M Stoller Pinellas Environmental Restoration Project - Young- Rainey Star Center  

Office of Legacy Management (LM)

Pinellas Environmental Restoration Project - Young- Rainey Star Center Pinellas Environmental Restoration Project - Young- Rainey Star Center 7030-226 Accutest Job Number: F29125 Sampling Date: 01/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

5

S M Stoller Pinellas Environmental Restoration Project - Young- Rainey Star Center  

Office of Legacy Management (LM)

Pinellas Environmental Restoration Project - Young- Rainey Star Center Pinellas Environmental Restoration Project - Young- Rainey Star Center 110406202 Accutest Job Number: F33039 Sampling Date: 07/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

6

Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site  

Office of Legacy Management (LM)

600 600 GJO-2003-410-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project Quarterly Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site October through December 2002 January 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0057600 Contents DOE/Grand Junction Office 4.5 Acre Site Quarterly Progress Report January 2003 Page iii Contents Acronyms and Abbreviations ..........................................................................................................v 1.0 Introduction ............................................................................................................................1

7

Economic Development Activities at the Young - Rainey Science, Technology, & Research (STAR) Center  

SciTech Connect

Project mission was to mitigate the adverse economic effects of closing the U.S. Department of Energy's Pinellas Plant in Largo, Florida. This project was to facilitate the physical renovation of the plant and to help maintain and create jobs for the employees that worked at the plant when DOE terminated its operations. It also included finding and attracting high technology, industrial manufacturing and related firms to utilize the space and high tech equipment to remain at the plant. Stakeholders included the affected plant employees, local government and related public organizations, and businesses and universities in the Tampa Bay Florida area. The $17.6 million funded for this project helped produce 2,780 jobs at the Young - Rainey STAR Center at an average cost of $6,328. Rental income from STAR Center tenants and third party cash input amounted to approximately $66 million over the project period of 13.3 years.

Paul S. Sacco; Carl Smeigh; John Caponiti, Jr.

2008-06-30T23:59:59.000Z

8

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

6/06 6/06 Technical Report for S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center 110406202 Accutest Job Number: F43553 Sampling Date: 09/07/06 Report to: U.S. Dept of Energy, Grand Jct Office 2597 B 3/4 Road Grand Juction, CO 81503 ATTN: Contracts Department, PO# 24231 x Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference

9

Successful Field-Scale In Situ Thermal NAPL Remediation at the Young-Rainey Star Center  

SciTech Connect

The U.S. Department of Energy (DOE) successfully completed a fieldscale remediation to remove non-aqueous phase liquids (NAPLs) from the subsurface at a site on the Young-Rainey Science, Technology, and Research (STAR) Center, Largo, Florida. The STAR Center is a former DOE facility. The remediation project covered an area of 930 m2 (10,000 ft2) and depths extending to 10.5 m (35 ft) below ground surface. In July 2001, DOEs contractor awarded a subcontract to SteamTech Environmental Services for removal of NAPLs from a portion of the Northeast Site. The technologies used for remediation were steam-enhanced extraction and Electro-Thermal Dynamic Stripping Process, an electrical resistive heating technology. McMillan-McGee Corporation implemented the process. Construction of the remediation system was completed in September 2002. Operations began immediately after construction, and active heating ended in February 2003. After operations were completed, confirmatory sampling was conducted over a 6-month period to verify the level of cleanup achieved. Results of the sampling showed that NAPL concentrations were reduced significantly below the required cleanup goals and, in most cases, below the regulatory maximum contaminant levels. Lessons learned relative to the design, construction, operation, confirmatory sampling approach, and subcontracting could benefit managers of similar remediation projects

Gavaskar, A.R. [ed.; Chen, A.S.C. [ed.; none,

2004-05-04T23:59:59.000Z

10

Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center, October through December 2002  

Office of Legacy Management (LM)

7500 7500 GJO-2003-409-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center October through December 2002 January 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0057500 Contents DOE/Grand Junction Office Pinellas Environmental Restoration Project January 2003 Page iii Contents Page Acronyms and Abbreviations ..........................................................................................................v 1.0 Introduction ............................................................................................................................1

11

Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainy STAR Center  

Office of Legacy Management (LM)

2-TAC 2-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project January through March 2003 Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center April 2003 Grand Junction Office Grand Junction Office Grand Junction Office U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy DE-AC13-02GJ79491 Approved for public release; distribution is unlimited. N0060700 GJO-2003-432-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center January through March 2003 April 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491

12

Successful Field-Scale In Situ Thermal NAPL Remediation at the Young- Rainey STAR Center  

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

Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds.May 2004, Monterey, California.Randall Juhlin, Michael Butherus, Joseph Daniel, David S....

13

ENERGY STAR Score for Data Centers  

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

Data Centers in the United States Page 1 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 spaces specifically designed and equipped to meet the needs of high density computing equipment such as server racks, used for data storage and processing. 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

14

ENERGY STAR Success Story: San Diego Convention Center | ENERGY STAR  

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

San Diego Convention Center San Diego Convention Center 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

15

ENERGY STAR Success Story: The Virginia Beach Convention Center | ENERGY  

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

ENERGY STAR Success Story: The Virginia Beach Convention Center ENERGY STAR Success Story: The Virginia Beach Convention Center 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

16

ENERGY STAR Success Story San Diego Convention Center  

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

ENERGY STAR Success Story ENERGY STAR Success Story San Diego Convention Center Since opening 20 years ago, San Diego's bayside convention facility has been a green industry leader and continues to receive accolades for environmental stewardship. The San Diego Convention Center Corporation (SDCCC) joined the Environmental Protection Agency's (EPA) ENERGY STAR program as a partner in 2008. Using the EPA's online energy management and tracking tool, Portfolio Manager, the SDCCC tracked its energy consumption and has improved the facility's overall performance. Since then, the San Diego Convention Center has become a model for other convention and meeting facilities demonstrating the value of benchmarking to improve efficiency and to save money. . The Convention Center is managed and marketed by the SDCCC, a non-profit public

17

Discovery of hot supergiant stars near the Galactic center  

E-Print Network (OSTI)

We report new results of a campaign to find Wolf-Rayet and O (WR/O) stars and high-mass X-ray binaries (HMXBs) in the Galactic center. We searched for candidates by cross-correlating the 2MASS catalog with a deep Chandra catalog of X-ray point sources in the Radio Arches region. Following up with K-band spectroscopy, we found two massive stellar counterparts to CXOGC J174555.3-285126 and CXOGC J174617.0-285131, which we classify as a broad-lined WR star of sub-type WN6b and an O Ia supergiant, respectively. Their X-ray properties are most consistent with those of known colliding-wind binaries in the Galaxy and the Large Magellanic Cloud, although a scenario involving low-rate accretion onto a compact object is also possible. The O Ia star lies 4.4 pc in projection from the Quintuplet cluster, and has a radial velocity consistent with that of the Quintuplet, suggesting that this star might have escaped from the cluster. We also present the discovery of a B2 Ia supergiant, which we identified as a candidate massive star using 8 micron Spitzer maps of the Galactic center in a region near the known massive X-ray-emitting star CXOGC J174516.1-290315. We discuss the origin of these stars in the context of evolving stellar clusters in the Galactic center.

Jon C. Mauerhan; Michael P. Muno; Mark Morris

2007-03-08T23:59:59.000Z

18

Industrial energy management information center | ENERGY STAR Buildings &  

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

energy management information center energy management information center 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 Market impacts: Improvements in the industrial sector

19

ENERGY STAR Success Story VA Beach Convention Center  

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

STAR Success Story: STAR Success Story: The Virginia Beach Convention Center Located in Virginia's most populous city, the Virginia Beach Convention Center (VBCC) comprises more than 516,000 square feet and typically hosts 400 events a year. Fully opened in 2007, the VBCC has served as the anchor for the successful revitalization of Virginia Beach's old beach district. With historical references and maritime themes integrated into the structure's modern design, the Center features many technological advances that make it a prime location for meetings, conferences, and trade shows. However, even with a newly constructed building, the VBCC has demonstrated an important energy management principle: all buildings, regardless of their age and building systems they employ, can reduce energy consumption, save money, and offset greenhouse gas

20

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

Quarterly Sampling, STAR Center, Largo, FL Quarterly Sampling, STAR Center, Largo, FL 110406202 Accutest Job Number: F33211 Sampling Dates: 07/13/05 - 07/14/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

Note: This page contains sample records for the topic "rainey star center" 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

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

Quarterly Sampling, STAR Center, Largo, FL Quarterly Sampling, STAR Center, Largo, FL 7030-226 Accutest Job Number: F27229 Sampling Date: 10/07/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

22

pinellas  

Office of Legacy Management (LM)

use. The County currently owns the facility, which is now called the Young - Rainey Science, Technology, and Research (STAR) Center. The STAR Center houses more than 20...

23

ENERGY STAR Success Story Fleet Science Center Dec 2009  

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

ENERGY STAR Success Story: Reuben H. Fleet Science Center The Reuben H. Fleet Science Center (the Fleet) is one of twenty-four arts, science, and cultural institutions that are part of San Diego's Balboa Park Cultural Partnership. The Partnership launched a sustainability initiative in 2008 along with the City of San Diego and San Diego Gas & Electric ® (SDG&E) with the goal of improving energy efficiency and reducing resource consumption at the Park's cultural institutions. To date, Balboa Park venues have decreased electricity usage by more than 3.5 million kWh and 87,000 therms of natural gas, realizing savings of $530,000. Built in 1973, the Fleet serves as a leader and a model in environmental sustainability to venues of Balboa Park and other entertainment facilities across the country. For over a decade, the Fleet has

24

A DISTENSIBLETUBE WAVE ENERGY CONVERTER WITH A DISTRIBUTED POWERTAKEOFF R.C.T.Rainey, Atkins Ltd., Woodcote Grove, Epsom KT18 5BW, U.K. rod.rainey@atkinsglobal.com  

E-Print Network (OSTI)

1 A DISTENSIBLETUBE WAVE ENERGY CONVERTER WITH A DISTRIBUTED POWERTAKEOFF R.C.T.Rainey, Atkins A distensibletube Wave Energy Converter (WEC) operates by converting the wave energy into "bulge waves interaction then occurs, and large bulge waves are generated, concentrating the wave energy

25

S M Stoller Star Center-B100  

Office of Legacy Management (LM)

/19/06 /19/06 Technical Report for S M Stoller Star Center-B100 110406202 7031-877 Accutest Job Number: F41217 Sampling Date: 06/02/06 Report to: US Dept of Energy, Grand Jct Office 2597 B3/4 Road Grand Junction, CO 81503 ATTN: Contracts Department, PO# 24231 x Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference

26

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

2/04 2/04 Technical Report for S M Stoller Quarterly Sampling, STAR Center, Largo, FL 110406202 Accutest Job Number: F25409 Sampling Dates: 07/13/04 - 07/14/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

27

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

0/06 0/06 Technical Report for S M Stoller Quarterly Sampling, STAR Center, Largo, FL 110406202 Accutest Job Number: F39137 Sampling Dates: 03/08/06 - 03/09/06 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

28

PROJECT SCIENTIST II NOAA NESDIS Center for Satellite Applications and Research (STAR)  

E-Print Network (OSTI)

PROJECT SCIENTIST II NOAA NESDIS Center for Satellite Applications and Research (STAR) College Park Visiting Scientist Programs is seeking a Project Scientist II to work at the NOAA NESDIS Center design and implementation and the development of common tools and procedures for STAR researchers

Droegemeier, Kelvin K.

29

Microsoft Word - N01765_4_5 Acre semiannual june-nov 2012.doc  

Office of Legacy Management (LM)

SEEPro Site Environmental Evaluation for Projects STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPCs total contaminants of...

30

Microsoft Word - DOE_RM_DM-#99942-v1-4_5_Acre_Quarterly_October...  

Office of Legacy Management (LM)

Turbidity Units RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPC total contaminants of...

31

Microsoft Word - DOE_RM_DM-#345141-v1-4_5_Quarterly_Oct_Dec_2005...  

Office of Legacy Management (LM)

Turbidity Units RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPC total contaminants of...

32

Microsoft Word - N01687_4_5Acre June - Nov 2011  

Office of Legacy Management (LM)

Corrective Action RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPCs total contaminants of...

33

Microsoft Word - DOE_RM_DM-#101993-v1-4_5_Acre_Quarterly_Jan...  

Office of Legacy Management (LM)

Turbidity Units RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPC total contaminants of...

34

Microsoft Word - DOE_RM_DM-#103356-v1-4_5_Acre_Quarterly_Apr...  

Office of Legacy Management (LM)

Turbidity Units RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPC total contaminants of...

35

Microsoft Word - N01440_4 5Acre Jun-Nov09.doc  

Office of Legacy Management (LM)

Corrective Action RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPC total contaminants of...

36

Quarterly Progress Report, 4.5 Acre Site April through June 2003  

Office of Legacy Management (LM)

RAP Remedial Action Plan RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center STL Severn Trent Laboratories TCE trichloroethene...

37

Pinellas County, Florida, Site Environmental Restoration Project  

Office of Legacy Management (LM)

mgL milligrams per liter RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPCs total contaminants of...

38

Microsoft Word - N01629_4_5Acre_Dec-May 2011  

Office of Legacy Management (LM)

Corrective Action RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPCs total contaminants of...

39

Microsoft Word - N01844_4_5Acre Semiannual june_nov13.docx  

Office of Legacy Management (LM)

mgL milligrams per liter RPD relative percent difference STAR Center Young - Rainey Science, Technology, and Research Center TCE trichloroethene TCOPCs total contaminants of...

40

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

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


41

1STAR Seminar, NOAA Science Center, 8 Jan 2008 Impact of GOES Spacecraft Stabilization  

E-Print Network (OSTI)

Programs, NSOF, 30 Oct 2007 Lessons learned during a major transition are useful to both MTG and GOES-R #12 at the Earth #12;6STAR Seminar, NOAA Science Center, 8 Jan 2008 The process of quantitatively defining

Kuligowski, Bob

42

S M Stoller Star Center-B100 Monthly/Effluent; Largo, FL  

Office of Legacy Management (LM)

Water Date Received: 010506 Percent Solids: na Project: Star Center-B100 General Chemistry Analyte Result RL Units DF Analyzed By Method Hardness, Total as CaCO3 372 4.0 mgl...

43

Ejection of hypervelocity stars by the (binary) black hole(s) in the Galactic center  

E-Print Network (OSTI)

We study three processes that eject hypervelocity (>10^3 km/s) stars from the Galactic center: (i) close encounters of two single stars; (ii) tidal breakup of binary stars by the central black hole, as originally proposed by Hills; and (iii) three-body interactions between a star and a binary black hole (BBH). Mechanism (i) expels hypervelocity stars to the solar radius at a negligible rate, ~10^{-11}/yr. Mechanism (ii) expels hypervelocity stars at a rate ~ 10^{-5}(\\eta/0.1)/yr, where \\eta is the fraction of stars in binaries with semimajor axis a_b<~0.3 AU. For solar-mass stars, the corresponding number of hypervelocity stars within the solar radius R_0=8 kpc is ~60(\\eta/0.1)(a_b/0.1 AU)^{1/2}. For mechanism (iii), Sgr A^* is assumed to be one component of a BBH. We constrain the allowed parameter space (semimajor axis, mass ratio) of the BBH. In the allowed region (for example, semimajor axis of 0.5x10^{-3} pc and mass ratio of 0.01), the rate of ejecting hypervelocity stars can be as large as ~10^{-4}/yr and the expected number of hypervelocity stars within the solar radius can be as large as ~10^3. Hypervelocity stars may be detectable by the next generation of large-scale optical surveys.

Qingjuan Yu; Scott Tremaine

2003-09-03T23:59:59.000Z

44

DOE - Office of Legacy Management -- Pinellas  

Office of Legacy Management (LM)

Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2013 Through May 2014 LMSPINN01883 June 2014 Semiannual Progress Report for the 4.5 Acre...

45

Microsoft Word - DOE_RM_DM-#98960-v1-Sitewide_July_-_September...  

Office of Legacy Management (LM)

2004 - - GJ749 U.S. Department of Energy Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center...

46

S M Stoller STAR Center- 4.5 Acre Site, Largo, FL  

Office of Legacy Management (LM)

STAR Center- 4.5 Acre Site, Largo, FL STAR Center- 4.5 Acre Site, Largo, FL 110406202 Accutest Job Number: F25243 Sampling Date: 07/06/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

47

S M Stoller STAR Center- 4.5 Acre Site, Largo, FL  

Office of Legacy Management (LM)

STAR Center- 4.5 Acre Site, Largo, FL STAR Center- 4.5 Acre Site, Largo, FL 7030-226/Monthly Accutest Job Number: F27168 Sampling Date: 10/05/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

48

S M Stoller STAR Center- 4.5 Acre Site, Largo, FL  

Office of Legacy Management (LM)

STAR Center- 4.5 Acre Site, Largo, FL STAR Center- 4.5 Acre Site, Largo, FL 110406202 Accutest Job Number: F23552 Sampling Date: 04/20/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

49

Best Practices Guide for Energy-Efficient Data Center Design | ENERGY STAR  

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

Guide for Energy-Efficient Data Center Design Guide for Energy-Efficient Data Center Design 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

50

Trane and The American Center: SPP Success Story | ENERGY STAR Buildings &  

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

Trane and The American Center: SPP Success Story Trane and The American Center: SPP Success Story 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

51

SPP marketing flyer for data centers | ENERGY STAR Buildings & Plants  

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

data centers data centers 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

52

Energy Loss of Neutrinos in 20M{center_dot} Star  

SciTech Connect

Current ideas on neutrino oscillation plus confirmation from neutrino experiments make possible the changing of neutrino flavor due to interactions with the electrons in medium. When neutrinos pass through a medium and interact with the electrons, an effective potential energy is produced due to coherent forward scattering that occurred in the medium. This potential engenders significant changes in the neutrino masses and their mixing in the medium. Thus electron neutrinos would oscillate into different mass eigenstate and this is dependent on the energy of the neutrinos. Some of the energy will be lost in the coherent scattering with the electrons by the charged current interaction. We have calculated the energy loss of the neutrinos by using a stopping power equation for a 20M{center_dot} star.

Ahmad, Nor Sofiah; Yusof, Norhasliza; Kassim, Hasan Abu [Department of Physics, University of Malaya, 50603, Kuala Lumpur (Malaysia)

2010-08-12T23:59:59.000Z

53

KECK OBSERVATIONS OF THE GALACTIC CENTER SOURCE G2: GAS CLOUD OR STAR?  

SciTech Connect

We present new observations and analysis of G2-the intriguing red emission-line object which is quickly approaching the Galaxy's central black hole. The observations were obtained with the laser guide star adaptive optics systems on the W. M. Keck I and II telescopes (2006-2012) and include spectroscopy (R {approx} 3600) centered on the hydrogen Br{gamma} line as well as K' (2.1 {mu}m) and L' (3.8 {mu}m) imaging. Analysis of these observations shows the Br{gamma} line emission has a positional offset from the L' continuum. This offset is likely due to background source confusion at L'. We therefore present the first orbital solution derived from Br{gamma} line astrometry, which, when coupled with radial velocity measurements, results in a later time of closest approach (2014.21 {+-} 0.14), closer periastron (130 AU, 1600 R{sub s}), and higher eccentricity (0.9814 {+-} 0.0060) compared to a solution using L' astrometry. It is shown that G2 has no K' counterpart down to K' {approx} 20 mag. G2's L' continuum and the Br{gamma} line emission appears unresolved in almost all epochs, which implies that the bulk of the emission resides in a compact region. The observations altogether suggest that while G2 has a gaseous component that is tidally interacting with the central black hole, there is likely a central star providing the self-gravity necessary to sustain the compact nature of this object.

Phifer, K.; Meyer, L.; Ghez, A. M.; Witzel, G.; Yelda, S.; Boehle, A.; Morris, M. R.; Becklin, E. E. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Do, T. [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H4 (Canada); Lu, J. R. [Institute for Astronomy, University of Hawaii, Hilo, HI 96720 (United States); Matthews, K., E-mail: ghez@astro.ucla.edu [Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States)

2013-08-10T23:59:59.000Z

54

Microsoft Word - N01307_Sitewide semiannual June-Nov08.doc  

Office of Legacy Management (LM)

Young - Rainey STAR Center Young - Rainey STAR Center June through November 2008 December 2008 LMS/PIN/N01307 LMS/PIN/N01307 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center June through November 2008 December 2008 U.S. Department of Energy Sitewide Semiannual Progress Report for June through November 2008 December 2008 Doc. No. N0130700 Page i Contents Acronyms and Abbreviations ........................................................................................................ iii 1.0 Introduction.............................................................................................................................1 1.1 Building 100 Area.........................................................................................................2

55

Microsoft Word - N01308_4 5Acre June-Nov08_psd.doc  

Office of Legacy Management (LM)

Young - Rainey STAR Center's Young - Rainey STAR Center's 4.5 Acre Site June through November 2008 December 2008 LMS/PIN/N01308 LMS/PIN/N01308 Pinellas Environmental Restoration Project Semiannual Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site June through November 2008 December 2008 U.S. Department of Energy 4.5 Acre Site Semiannual Progress Report for June through November 2008 December 2008 Doc. No. N0130800 Page i Contents Acronyms and Abbreviations ......................................................................................................... ii 1.0 Introduction ............................................................................................................................1 1.1 Site Activities................................................................................................................2

56

RADIO DETECTION OF A CANDIDATE NEUTRON STAR ASSOCIATED WITH GALACTIC CENTER SUPERNOVA REMNANT SAGITTARIUS A EAST  

SciTech Connect

We report the Very Large Array (VLA) detection of the radio counterpart of the X-ray object referred to as the 'Cannonball', which has been proposed to be the remnant neutron star resulting from the creation of the Galactic center supernova remnant, Sagittarius A East. The radio object was detected both in our new VLA image from observations in 2012 at 5.5 GHz and in archival VLA images from observations in 1987 at 4.75 GHz and in the period from 1990 to 2002 at 8.31 GHz. The radio morphology of this object is characterized as a compact, partially resolved point source located at the northern tip of a radio 'tongue' similar to the X-ray structure observed by Chandra. Behind the Cannonball, a radio counterpart to the X-ray plume is observed. This object consists of a broad radio plume with a size of 30''15'', followed by a linear tail having a length of 30''. The compact head and broad plume sources appear to have relatively flat spectra (??{sup ?}) with mean values of ? = 0.44 0.08 and 0.10 0.02, respectively, and the linear tail shows a steep spectrum with the mean value of 1.94 0.05. The total radio luminosity integrated from these components is ?8 10{sup 33} erg s{sup 1}, while the emission from the head and tongue amounts for only ?1.5 10{sup 31} erg s{sup 1}. Based on the images obtained from the two epochs' observations at 5 GHz, we infer the proper motion of the object: ?{sub ?} = 0.001 0.003 arcsec yr{sup 1} and ?{sub ?} = 0.013 0.003 arcsec yr{sup 1}. With an implied velocity of 500 km s{sup 1}, a plausible model can be constructed in which a runaway neutron star surrounded by a pulsar wind nebula was created in the event that produced Sgr A East. The inferred age of this object, assuming that its origin coincides with the center of Sgr A East, is approximately 9000 yr.

Zhao, Jun-Hui [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 78, Cambridge, MA 02138 (United States); Morris, Mark R. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Goss, W. M., E-mail: jzhao@cfa.harvard.edu, E-mail: morris@astro.ucla.edu, E-mail: mgoss@aoc.nrao.edu [NRAO, P.O. Box O, Socorro, NM 87801 (United States)

2013-11-10T23:59:59.000Z

57

Energy Loss of Neutrinos in 20 M{sub {center_dot}} and 40 M{sub {center_dot}} Massive Stars  

SciTech Connect

The progress from the theoretical and experimental aspects in neutrino physics shines light into neutrino physics as well as in astrophysics. It is known that when neutrinos pass through a medium, the neutrinos interact with electrons before emerging from the stars with an effective potential energy produced due to coherent forward scatterings that occurred in the medium. This potential engenders significant changes in the neutrino masses and their mixing in the medium. Thus electron neutrinos would oscillate into different mass eigenstate and this is dependent on the energy of the neutrinos. Some of the energy will be lost in the coherent scattering with the electrons by the charged current interaction. We have calculated the energy loss of the neutrinos by using a stopping power equation for both rotating and non-rotating 20 M{sub {center_dot}} and 40 M{sub {center_dot}} stars. The total energy loss of neutrinos depends on the electron density in the stars and on the survival probability of the electron neutrino. For high electron density profile and the survival probability, the energy loss will be significant.

Sofiah Ahmad, Nor; Yusof, Norhasliza; Abu Kassim, Hasan [Department of Physics, University of Malaya, 50603 Kuala Lumpur (Malaysia)

2011-03-30T23:59:59.000Z

58

Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site  

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

Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young - Rainey STAR Center Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young - Rainey STAR Center Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds. May 2004, Monterey, California. Gorm Heron, Steven Carroll, Hank Sowers, Bruce McGee, Randall Juhlin, Joe Daniel, David S. Ingle Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young - Rainey STAR Center More Documents & Publications Successful Field-Scale In Situ Thermal NAPL Remediation at the Young - Rainey STAR Center Project Overview: Successful Field-Scale In Situ Thermal NAPL Remediation Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification

59

Microsoft Word - N01549_Sitewide semiannual Jun-Nov 2010 final draft  

Office of Legacy Management (LM)

Young - Rainey STAR Center June Through November 2010 December 2010 LMS/PIN/N01549 LMS/PIN/N01549 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center June Through November 2010 December 2010 U.S. Department of Energy Sitewide Semiannual Progress Report for June Through November 2010 December 2010 Doc. No. N01549 Page i Contents Abbreviations ................................................................................................................................. iii 1.0 Introduction .............................................................................................................................1 1.1 Building 100 Area .........................................................................................................2

60

EARLY-STAGE MASSIVE STAR FORMATION NEAR THE GALACTIC CENTER: Sgr C  

SciTech Connect

We present near-infrared spectroscopy and 1 mm line and continuum observations of a recently identified site of high mass star formation likely to be located in the Central Molecular Zone (CMZ) near Sgr C. Located on the outskirts of the massive evolved H II region associated with Sgr C, the area is characterized by an Extended Green Object (EGO) measuring ?10'' in size (0.4 pc), whose observational characteristics suggest the presence of an embedded massive protostar driving an outflow. Our data confirm that early-stage star formation is taking place on the periphery of the Sgr C H II region, with detections of two protostellar cores and several knots of H{sub 2} and Brackett ? emission alongside a previously detected compact radio source. We calculate the cores' joint mass to be ?10{sup 3} M {sub ?}, with column densities of 1-2 10{sup 24} cm{sup 2}. We show the host molecular cloud to hold ?10{sup 5} M {sub ?} of gas and dust with temperatures and column densities favorable for massive star formation to occur, however, there is no evidence of star formation outside of the EGO, indicating that the cloud is predominantly quiescent. Given its mass, density, and temperature, the cloud is comparable to other remarkable non-star-forming clouds such as G0.253 in the eastern CMZ.

Kendrew, S.; Johnston, K.; Beuther, H. [Max-Planck-Institut fr Astronomie, Knigstuhl 17, D-69117 Heidelberg (Germany)] [Max-Planck-Institut fr Astronomie, Knigstuhl 17, D-69117 Heidelberg (Germany); Ginsburg, A.; Bally, J.; Battersby, C. [CASA, University of Colorado at Boulder, UCB 389, Boulder, CO 80309 (United States)] [CASA, University of Colorado at Boulder, UCB 389, Boulder, CO 80309 (United States); Cyganowski, C. J., E-mail: kendrew@mpia.de [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)

2013-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "rainey star center" from the National Library of EnergyBeta (NLEBeta).
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61

THE GALACTIC CENTER CLOUD G0.253+0.016: A MASSIVE DENSE CLOUD WITH LOW STAR FORMATION POTENTIAL  

SciTech Connect

We present the first interferometric molecular line and dust emission maps for the Galactic Center (GC) cloud G0.253+0.016, observed using CARMA and the SMA. This cloud is very dense, and concentrates a mass exceeding the Orion Molecular Cloud Complex (2 Multiplication-Sign 10{sup 5} M{sub Sun }) into a radius of only 3 pc, but it is essentially starless. G0.253+0.016 therefore violates ''star formation laws'' presently used to explain trends in galactic and extragalactic star formation by a factor {approx}45. Our observations show a lack of dense cores of significant mass and density, thus explaining the low star formation activity. Instead, cores with low densities and line widths {approx}< 1 km s{sup -1}-probably the narrowest lines reported for the GC region to date-are found. Evolution over several 10{sup 5} yr is needed before more massive cores, and possibly an Arches-like stellar cluster, could form. Given the disruptive dynamics of the GC region, and the potentially unbound nature of G0.253+0.016, it is not clear that this evolution will happen.

Kauffmann, Jens; Pillai, Thushara [Astronomy Department, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Zhang Qizhou, E-mail: jens.kauffmann@astro.caltech.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS78, Cambridge, MA 02138 (United States)

2013-03-10T23:59:59.000Z

62

doe-lm-1419-2007.cdr  

Office of Legacy Management (LM)

Young Rainey STAR Center Young Rainey STAR Center Wastewater Neutralization Area No Further Action With Controls Proposal March 2007 Office of Legacy Management DOE M/1419 2007 - -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy This page intentionally left blank DOE-LM/1419-2007 Pinellas Environmental Restoration Project Young - Rainey STAR Center Wastewater Neutralization Area No Further Action With Controls Proposal March 2007 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491

63

A STAR DISRUPTED BY A STELLAR BLACK HOLE AS THE ORIGIN OF THE CLOUD FALLING TOWARD THE GALACTIC CENTER  

SciTech Connect

We propose that the cloud moving on a highly eccentric orbit near the central black hole in our Galaxy, reported by Gillessen et al., is formed by a photoevaporation wind originating in a disk around a star that is tidally perturbed and shocked at every peribothron passage. The disk is proposed to have formed when a stellar black hole flew by the star, tidally disrupted its envelope, and placed the star on its present orbit with some of the tidal debris forming a disk. A disrupting encounter at the location of the observed cloud is most likely to be caused by a stellar black hole because of the expected dynamical mass segregation; the rate of these disk-forming encounters may be as high as {approx}10{sup -6} per year. The star should also be spun up by the encounter, so the disk may subsequently expand by absorbing angular momentum from the star. Once the disk expands up to the tidal truncation radius, the tidal perturbation of the outer disk edge at every peribothron may place gas streams on larger orbits, which can give rise to a photoevaporation wind that forms the cloud at every orbit. This model predicts that, after the cloud is disrupted at the next peribothron passage in 2013, a smaller unresolved cloud will gradually grow around the star on the same present orbit. An increased infrared luminosity from the disk may also be detectable when the peribothron is reached. We also note that this model revives the encounter theory for planet formation.

Miralda-Escude, Jordi [Institucio Catalana de Recerca i Estudis Avancats, Barcelona, Catalonia (Spain)

2012-09-01T23:59:59.000Z

64

Microsoft Word - N01347_Sitewide semiannual Dec-May09.doc  

Office of Legacy Management (LM)

for the for the Young - Rainey STAR Center December 2008 through May 2009 June 2009 LMS/PIN/N01347 LMS/PIN/N01347 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2008 through May 2009 June 2009 U.S. Department of Energy Sitewide Semiannual Progress Report for December 2008 through May 2009 June 2009 Doc. No. N01347 Page i Contents Abbreviations................................................................................................................................. iii 1.0 Introduction.............................................................................................................................1 1.1 Building 100 Area.........................................................................................................2

65

VVV SURVEY NEAR-INFRARED PHOTOMETRY OF KNOWN BULGE RR LYRAE STARS: THE DISTANCE TO THE GALACTIC CENTER AND ABSENCE OF A BARRED DISTRIBUTION OF THE METAL-POOR POPULATION  

SciTech Connect

We have combined optical and near-infrared data of known RR Lyrae (RRL) stars in the bulge in order to study the spatial distribution of its metal-poor component by measuring precise reddening values and distances of 7663 fundamental-mode RRL stars with high-quality photometry. We obtain a distance to the Galactic center of R {sub 0} = 8.33 0.05 0.14 kpc. We find that the spatial distribution of the RRL stars differs from the structures traced by the predominantly metal-rich red clump (RC) stars. Unlike the RC stars, the RRL stars do not trace a strong bar, but have a more spheroidal, centrally concentrated distribution, showing only a slight elongation in its very center. We find a hint of bimodality in the density distribution at high southern latitudes (b < 5), which needs to be confirmed by extending the areal coverage of the current census. The different spatial distributions of the metal-rich and metal-poor stellar populations suggest that the Milky Way has a composite bulge.

Dkny, I.; Minniti, D.; Catelan, M.; Zoccali, M.; Hempel, M. [Instituto de Astrofsica, Facultad de Fsica, Pontificia Universidad Catlica de Chile, Av. Vicua Mackenna 4860, 782-0436 Macul, Santiago (Chile)] [Instituto de Astrofsica, Facultad de Fsica, Pontificia Universidad Catlica de Chile, Av. Vicua Mackenna 4860, 782-0436 Macul, Santiago (Chile); Saito, R. K. [Departamento de Fsica, Universidade Federal de Sergipe, Av. Marechal Rondon s/n, 49100-000, So Cristvo, SE (Brazil)] [Departamento de Fsica, Universidade Federal de Sergipe, Av. Marechal Rondon s/n, 49100-000, So Cristvo, SE (Brazil); Gonzalez, O. A., E-mail: idekany@astro.puc.cl [European Southern Observatory, Alonso de Crdova 3170, Vitacura, Santiago (Chile)

2013-10-20T23:59:59.000Z

66

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

67

Meredith Rainey BIO515 Fall 2009  

E-Print Network (OSTI)

; a single route's total resistance is equivalent to its cost-weighted distance (McRae et al. 2008). Circuit landscapes have emerged. These methods first quantify resistance to movement across the landscape for a focal.g., cover type, slope). This resistance surface is then used to identify likely movement routes between core

Hansen, Andrew J.

68

2B-01.doc  

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

1, in: A.R. Gavaskar and A.S.C. Chen (Eds.), Remediation of Chlorinated and Recalcitrant Compounds 1, in: A.R. Gavaskar and A.S.C. Chen (Eds.), Remediation of Chlorinated and Recalcitrant Compounds -2004. Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds (Monterey, CA; May 2004). ISBN 1-57477-145-0, published by Battelle Press, Columbus, OH, www.battelle.org/bookstore. SUCCESSFUL FIELD-SCALE IN SITU THERMAL NAPL REMEDIATION AT THE YOUNG-RAINEY STAR CENTER ABSTRACT: The U.S. Department of Energy (DOE) successfully completed a field- scale remediation to remove non-aqueous phase liquids (NAPLs) from the subsurface at a site on the Young-Rainey Science, Technology, and Research (STAR) Center, Largo, Florida. The STAR Center is a former DOE facility. The remediation project covered an

69

Microsoft Word - San Diego 2004 ORT Conference paper_1.doc  

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

presented at the Third International Conference on Oxidation and Reduction Technologies for Soil and presented at the Third International Conference on Oxidation and Reduction Technologies for Soil and Groundwater in San Diego, CA, on October 24-28, 2004 PROJECT OVERVIEW: SUCCESSFUL FIELD-SCALE IN SITU THERMAL NAPL REMEDIATION ABSTRACT: The U.S. Department of Energy (DOE) successfully completed a field-scale remediation to remove non-aqueous phase liquids (NAPLs) from the subsurface at the Northeast Site on the Young-Rainey Science, Technology, and Research (STAR) Center, Largo, Florida. The Young-Rainey STAR Center is a former DOE facility that was previously known as the Pinellas Plant and the Pinellas STAR Center. The remediation project encompassed an area of 10,000 ft 2 and depths extending to 35 ft below ground surface. Prior to the remediation, DOE evaluated technologies that had the potential to remove

70

Covered Product Category: Data Center Storage  

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

The Federal Energy Management Program (FEMP) provides acquisition guidance for data center storage, which is a product category covered by the ENERGY STAR program. Federal laws and requirements...

71

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

72

Dark Stars: A Review  

E-Print Network (OSTI)

Dark Stars (DS) are stellar objects made (almost entirely) of ordinary atomic material but powered by the heat from Dark Matter (DM) annihilation (rather than by fusion). Weakly Interacting Massive Particles (WIMPs), among the best candidates for DM, can be their own antimatter and can accumulate inside the star, with their annihilation products thermalizing with and heating the DS. The resulting DSs are in hydrostatic and thermal equilibrium. The first phase of stellar evolution in the history of the Universe may have been dark stars. Though DM constituted only $power the star for millions to billions of years. Depending on their DM environment, early DSs can become very massive ($>10^6 M_\\odot$), very bright ($>10^9 L_\\odot$), and potentially detectable with the James Webb Space Telescope (JWST). Once the DM runs out and the dark star dies, it may collapse to a black hole; thus DSs can provide seeds for the supermassive black holes observed throughout the Universe and at early times. Other sites for dark star formation exist in the Universe today in regions of high dark matter density such as the centers of galaxies. The current review briefly discusses DSs existing today but focuses on the early generation of dark stars.

Katherine Freese; Tanja Rindler-Daller; Douglas Spolyar; Monica Valluri

2015-01-10T23:59:59.000Z

73

STAR METRICS  

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

Energy continues to define Phase II of the STAR METRICS program, a collaborative initiative to track Research and Development expenditures and their outcomes. Visit the STAR METRICS website for...

74

Microsoft Word - N0075600-sitewide April to June 2004.doc  

Office of Legacy Management (LM)

2004 - - GJ 95 U.S. Department of Energy Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center April Through June 2004 July 2004 Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management Office of Legacy Management N00075600 DOE-LM/GJ695-2004 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center April through June 2004 July 2004 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491

75

Pinellas Environmental Restoration Project Quarterly Progress Report, Sitewide, January through March 2004  

Office of Legacy Management (LM)

44 44 2004 GJ - - U.S. Department of Energy Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center January Through March 2004 April 2004 Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management Office of Legacy Management N00074400 DOE-LM/GJ644-2004 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center January through March 2004 April 2004 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491

76

Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification  

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

Nonaqueous-Phase Liquid Characterization and Post-Remediation Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds. May 2004, Monterey, California. Charles Tabor, Randall Juhlin, Paul Darr, Julian Caballero, Joseph Daniel, David Ingle Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling More Documents & Publications Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young - Rainey STAR Center Project Overview: Successful Field-Scale In Situ Thermal NAPL Remediation Successful Field-Scale In Situ Thermal NAPL Remediation at the Young - Rainey STAR Center

77

Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification  

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

Nonaqueous-Phase Liquid Characterization and Post-Remediation Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds. May 2004, Monterey, California. Charles Tabor, Randall Juhlin, Paul Darr, Julian Caballero, Joseph Daniel, David Ingle Nonaqueous-Phase Liquid Characterization and Post-Remediation Verification Sampling More Documents & Publications Project Overview: Successful Field-Scale In Situ Thermal NAPL Remediation Successful Field-Scale In Situ Thermal NAPL Remediation at the Young - Rainey STAR Center Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young - Rainey STAR Center

78

Final Report Northeast Site Area B NAPL Remediation Project  

Office of Legacy Management (LM)

Northeast Site Area B Northeast Site Area B NAPL Remediation Project at the Young - Rainey STAR Center Largo, Pinellas County, Florida April 2007 Office of Legacy Management DOE M/1457 2007 - -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy This page intentionally left blank DOE-LM/1457-2007 Final Report Northeast Site Area B NAPL Remediation Project at the Young - Rainey STAR Center Largo, Pinellas County, Florida April 2007 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado

79

2B-05.doc  

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

5, in: A.R. Gavaskar and A.S.C. Chen (Eds.), Remediation of Chlorinated and Recalcitrant Compounds 5, in: A.R. Gavaskar and A.S.C. Chen (Eds.), Remediation of Chlorinated and Recalcitrant Compounds -2004. Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds (Monterey, CA; May 2004). ISBN 1-57477-145-0, published by Battelle Press, Columbus, OH, www.battelle.org/bookstore. STEAM AND ET-DSP COMBINED FOR DNAPL REMEDIATION: FULL-SCALE SITE RESTORATION AT YOUNG-RAINEY STAR CENTER ABSTRACT: In March of 2003, the United States Department of Energy (DOE) com- pleted a full-scale nonaqueous-phase liquid (NAPL) remediation of Area A of the North- east Site at the Young-Rainey STAR Center, Largo, Florida. The site was contaminated with approximately 2,300 kg (5,000 lbs) of NAPL constituents such as TCE, cis-1,2-

80

Microsoft Word - N01715_Sitewide semiannual Dec - May 2012 FINAL DRAFT.doc  

Office of Legacy Management (LM)

Sitewide Environmental Monitoring Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2011 Through May 2012 June 2012 LMS/PIN/N01715 U.S. Department of Energy Sitewide Semiannual Progress Report for December 2011 Through May 2012 June 2012 Doc. No. N01715 Page i Contents Abbreviations ................................................................................................................................. iii 1.0 Introduction ............................................................................................................................1 1.1 Building 100 Area .........................................................................................................2 1.2 Northeast Site ................................................................................................................5

Note: This page contains sample records for the topic "rainey star center" 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

Microsoft Word - N01439_Sitewide semiannual Jun-Nov09.doc  

Office of Legacy Management (LM)

June through November 2009 June through November 2009 December 2009 LMS/PIN/N01439 LMS/PIN/N01439 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center June through November 2009 December 2009 U.S. Department of Energy Sitewide Semiannual Progress Report for June through November 2009 December 2009 Doc. No. N01439 Page i Contents Abbreviations................................................................................................................................. iii 1.0 Introduction.............................................................................................................................1 1.1 Building 100 Area.........................................................................................................2

82

Discovery of new Milky Way star cluster candidates in the 2MASS point source catalog III. Follow-up observations of cluster candidates in the Galactic Center region  

E-Print Network (OSTI)

This paper is part of a project to search the inner Milky Way for hidden massive clusters and to address the question of whether our Galaxy still forms clusters similar to the progenitors of the present-day globular clusters. We report high angular resolution deep near-infrared imaging of 21 cluster candidates selected from the catalogues of Bica et al. (2003) and Dutra et al.(2003) in a region around the Galactic Center. These catalogues were created from visual inspection of the 2MASS images. Seven objects appear to be genuine clusters, and for these objects we present estimates of extinction, distance and in some cases age and mass. Our estimated masses range from 1200 to 5500 solar masses. These clusters are thus significantly smaller than any Galactic globular cluster, and indicate that the formation of massive young clusters such as Arches and Quintuplet is not common in the present-day Milky Way. The remaining 14 objects are either not clusters or cannot be classified based on our data.

J. Borissova; V. D. Ivanov; D. Minniti; D. Geisler; A. W. Stephens

2005-02-01T23:59:59.000Z

83

Dark Stars: A Review  

E-Print Network (OSTI)

Dark Stars (DS) are stellar objects made (almost entirely) of ordinary atomic material but powered by the heat from Dark Matter (DM) annihilation (rather than by fusion). Weakly Interacting Massive Particles (WIMPs), among the best candidates for DM, can be their own antimatter and can accumulate inside the star, with their annihilation products thermalizing with and heating the DS. The resulting DSs are in hydrostatic and thermal equilibrium. The first phase of stellar evolution in the history of the Universe may have been dark stars. Though DM constituted only $10^6 M_\\odot$), very bright ($>10^9 L_\\odot$), and potentially detectable with the James Webb Space Telescope (JWST). Once the DM runs out and the dark star dies, it may collapse to a black hole; thus DSs can provide seeds for the supermassive black holes observed throughout the Universe and at early times. Other sites for dark star formation exist in the Universe today in regions of high dark matter density such as the centers of galaxies. The curre...

Freese, Katherine; Spolyar, Douglas; Valluri, Monica

2015-01-01T23:59:59.000Z

84

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 ......................................................................................................................................................................................

85

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

86

Hypervelocity binary stars: smoking gun of massive binary black holes  

E-Print Network (OSTI)

The hypervelocity stars recently found in the Galactic halo are expelled from the Galactic center through interactions between binary stars and the central massive black hole or between single stars and a hypothetical massive binary black hole. In this paper, we demonstrate that binary stars can be ejected out of the Galactic center with velocities up to 10^3 km/s, while preserving their integrity, through interactions with a massive binary black hole. Binary stars are unlikely to attain such high velocities via scattering by a single massive black hole or through any other mechanisms. Based on the above theoretical prediction, we propose a search for binary systems among the hypervelocity stars. Discovery of hypervelocity binary stars, even one, is a definitive evidence of the existence of a massive binary black hole in the Galactic center.

Youjun Lu; Qingjuan Yu; D. N. C. Lin

2007-07-12T23:59:59.000Z

87

Establishing Regional Resource Centers  

Wind Powering America (EERE)

Establishing Regional Resource Centers Establishing Regional Resource Centers July 25, 2013 Coordinator: Welcome and thank you for standing by. At this time all participants are in a listen only mode. To ask a question later during the question and answer session please press star then 1 on your touchtone phone. Today's conference is being recorded. If you have any objections you may disconnect. And I would like to turn it over to Mr. Jonathan Bartlett. Sir, you may begin. Jonathan Bartlett: Thank you very much. This is Jonathan Bartlett from the Department of Energy's Wind and Water Power Technologies Office. Today's WPA Webinar will be on the subject of establishing regional resource centers. I will be joined by Ian Baring-Gould at the National Renewable Energy Laboratory and the

88

Neutron star interiors and topology change  

E-Print Network (OSTI)

Quark matter is believed to exist in the center of neutron stars. A combined model consisting of quark matter and ordinary matter is used to show that the extreme conditions existing in the center could result in a topology change, that is, in the formation of wormholes.

Peter K. F. Kuhfittig

2012-07-27T23:59:59.000Z

89

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

90

Star Power  

SciTech Connect

The U.S. Department of Energy's Princeton Plasma Physics Laboratory has released ''Star Power,'' a new informational video that uses dramatic and beautiful images and thought-provoking interviews to highlight the importance of the Laboratory's research into magnetic fusion.

None

2014-10-17T23:59:59.000Z

91

Star Power  

ScienceCinema (OSTI)

The U.S. Department of Energy's Princeton Plasma Physics Laboratory has released ''Star Power,'' a new informational video that uses dramatic and beautiful images and thought-provoking interviews to highlight the importance of the Laboratory's research into magnetic fusion.

None

2014-11-18T23:59:59.000Z

92

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

93

operations center  

National Nuclear Security Administration (NNSA)

1%2A en Operations Center http:nnsa.energy.govaboutusourprogramsemergencyoperationscounterterrorismoperationscenter

...

94

Voluntary Protection Program Onsite Review, Volpentest HAMMER Training Center January 2011  

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

Evaluation to determine whether Volpentest Hazardous Materials Management and Emergency Response Training Center is continuing to perform at a level deserving DOE-VPP Star recognition.

95

Voluntary Protection Program Onsite Review, Transuranic Waste Processing Center- September 2012  

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

Evaluation to determine whether Transuranic Waste Processing Center is continuing to perform at a level deserving DOE-VPP Star recognition.

96

Data Centers: Looking for Energy Solutions  

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

operating costs, benchmark energy performance, and demonstrate environmental stewardship. Turn to an ENERGY STAR ® Service and Product Provider Partner ENERGY STAR Service and Product Providers (SPPs) have the experience and tools to implement energy-efficient strategies that are right for you. Following the U.S. Environmental Protection Agency's (EPA) Guidelines for Energy Management, a proven strategy developed from ENERGY STAR partner successes, SPPs can help your organization gain control of energy consumption and costs. ENERGY STAR SPPs can help data center owners and operators reap the financial and environmental benefits of superior energy efficiency. In its 2007 Report to Congress on Server and Data Center Energy Efficiency Opportunities, EPA estimated that the nation's servers and data

97

Energy Star  

E-Print Network (OSTI)

ENERGY STAR ENERGY TARGETS ESL-KT-12-10-08 CATEE 2012: Clean Air Through Energy Efficiency Conference, Galveston, TX, October 9-11, 2012 POP QUIZ!!!! What is EUI?? Energy Use Intensity Do you know the EUI and any of the buildings you designed... this past year? Do you know what a good EUI is for an Office building? K-12 School? ESL-KT-12-10-08 CATEE 2012: Clean Air Through Energy Efficiency Conference, Galveston, TX, October 9-11, 2012 POP QUIZ!!!! ESL-KT-12-10-08 CATEE 2012: Clean Air...

Reihl, K.; Tullos, A.

2012-01-01T23:59:59.000Z

98

Help Center  

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

Los Alamos National Laboratory Advanced Simulation and Computing Los Alamos National Laboratory Advanced Simulation and Computing Menu Events Partnerships Help Center Events Partnerships Help Center Videos Advanced Simulation and Computing Program » Help Center Computing Help Center Help hotlines, hours of operation, training, technical assistance, general information Los Alamos National Laboratory Hours: Monday through Friday, 8:00 a.m. - noon, 1:00-5:00 p.m. Mountain time Telephone: (505) 665-4444 option 3 Fax: (505) 665-6333 E-mail: consult@lanl.gov 24 hours a day, 7 days a week Operations (to report a system or network problem: (505) 667-2919 Lawrence Livermore National Laboratory Hours: Monday through Friday, 8:00 a.m. - noon, 1:00-4:45 p.m. Pacific time High Performance Hotline (technical consulting) Telephone: (925) 422-4532

99

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

100

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

Note: This page contains sample records for the topic "rainey star center" 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

Directed search for continuous gravitational waves from the Galactic center  

E-Print Network (OSTI)

We present the results of a directed search for continuous gravitational waves from unknown, isolated neutron stars in the Galactic center region, performed on two years of data from LIGOs fifth science run from two LIGO ...

Aggarwal, Nancy

102

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

103

ASU EFRC - Center researchers  

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

Principal Investigators Postdoctoral Fellows Center researchers Graduate Students Undergraduate Students All Bisfuel Center Personnel Center researchers Chad Simmons Academic...

104

Centers | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Centers Centers Energy Frontier Research Centers (EFRCs) EFRCs Home Centers Research Science Highlights News & Events Publications Contact BES Home Centers Print Text Size: A A A RSS Feeds FeedbackShare Page Energy Frontier Research Centers To learn more about each of the 46 EFRC centers, click on the stars in the map or the html links below. Interactive Map of Energy Frontier Research Centers CETM PHaSE CES RPEMSC NECCES CEFRC EMC2 CCEI CLSF Efree NEES CCHF UNC HeteroFoaM CSTEC RMSSEC MSA C3Bio CABS PARC CALCD SSLS CISSEM BISfuel LMI CEN MEEM CEEM CNEEC CGS NCGC CID CMSNF CME CE S3TEC FIRST CDP CEES IACT ANSER NERC CST CFSES CMIME CASP Centers ordered alphabetically by state and then by center name Arizona Center for Bio-Inspired Solar Fuel Production (BISfuel) Devens Gust, Arizona State University

105

Center Resources  

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

Resources for Planning Center Activities Resources for Planning Center Activities       QuarkNet at Work - Resources Home QuarkNet is a teacher professional development effort funded by the National Science Foundation and the US Department of Energy. Teachers work on particle physics experiments during a summer and join a cadre of scientists and teachers working to introduce some aspects of their research into their classrooms. This allows tomorrow's particle physicists to peek over the shoulder of today's experimenters. These resources are available for lead teachers and mentors at Quartnet Centers as they design activities for associate teacher workshops and follow-on activities. Important Findings from Previous Years Mentor Tips Associate Teacher Institute Toolkit

106

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

107

n0052300-4_5 acre.doc  

Office of Legacy Management (LM)

2300 2300 MAC-PIN 25.5.1 Pinellas Environmental Restoration Project Interim Remedial Action Quarterly Progress Report for the Young-Rainey Star Center's 4.5-Acre Site January through March 2002 April 2002 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-96GJ87335 Task Order Number MAC02-10 Document Number N0052300 Contents DOE/Grand Junction Office 4.5 Acre Site Interim Remedial Action April 2002 Page iii Contents Acronyms and Abbreviations ........................................................................................................... v 1.0 Introduction ............................................................................................................................1

108

Microsoft Word - N01513_Sitewide semiannual Dec09-May10.doc  

Office of Legacy Management (LM)

December 2009 through May 2010 December 2009 through May 2010 June 2010 LMS/PIN/N01513 LMS/PIN/N01513 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2009 through May 2010 June 2010 U.S. Department of Energy Sitewide Semiannual Progress Report for December 2009 through May 2010 June 2010 Doc. No. N01513 Page i Contents Abbreviations................................................................................................................................. iii 1.0 Introduction.............................................................................................................................1 1.1 Building 100 Area.........................................................................................................2

109

Microsoft Word - Bldg 100 Pilot Test.doc  

Office of Legacy Management (LM)

DOE-LM/GJ791-2005 DOE-LM/GJ791-2005 Pinellas Environmental Restoration Project Young - Rainey STAR Center Building 100 Area Enhanced Bioremediation Pilot Test Final Report January 2005 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Building 100 Area Enhanced Bioremediation Pilot Test Final Report January 2005 Page ii Contents 1.0 Introduction......................................................................................................................... 1 2.0 Results from the May 2004 (P8) Sampling Event .............................................................. 1 3.0 Microorganism Data

110

n0055800-4_5 acre.doc  

Office of Legacy Management (LM)

5800 5800 GJO- 2002-379- TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project Quarterly Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site July through September 2002 October 2002 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0055800 Contents DOE/Grand Junction Office 4.5 Acre Site Quarterly Progress Report October 2002 Page iii Contents Acronyms and Abbreviations ........................................................................................................... v 1.0 Introduction ............................................................................................................................1

111

Microsoft Word - N0064700-April 2004 version.doc  

Office of Legacy Management (LM)

64700 64700 DOE-LM-GJ/628-2004 Pinellas Environmental Restoration Project Young - Rainey STAR Center Reactive Transport Modeling of Enhanced Bioremediation in the Building 100 Area April 2004 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado This page intentionally left blank Document Number N0064700 Contents U.S. Department of Energy Reactive Transport Modeling of Enhanced Bioremediation in the Building 100 Area April 2004 Page iii Contents 1.0 Introduction ............................................................................................................................1 2.0 Background

112

N0055700-sitewideJuly to September.doc  

Office of Legacy Management (LM)

5700 5700 GJO- 2002-378- TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center July through September 2002 October 2002 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0055700 Contents DOE/Grand Junction Office Pinellas Environmental Restoration Project October 2002 Page iii Contents Page Acronyms and Abbreviations .........................................................................................................vii 1.0 Introduc tion ............................................................................................................................1

113

Microsoft Word - N01628_Sitewide semiannual Dec-May 2011  

Office of Legacy Management (LM)

0 Through May 2011 0 Through May 2011 June 2011 LMS/PIN/N01628 LMS/PIN/N01628 Pinellas County, Florida, Site Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2010 Through May 2011 June 2011 U.S. Department of Energy Sitewide Semiannual Progress Report for December 2010 Through May 2011 June 2011 Doc. No. N01628 Page i Contents Abbreviations ................................................................................................................................. iii 1.0 Introduction ............................................................................................................................1 1.1 Building 100 Area .........................................................................................................2

114

Microsoft Word - N00647-Enhanced Bioremediation-October 2003.doc  

Office of Legacy Management (LM)

N0064700 N0064700 GJO-2003-495-TAC PIN 700.20.10 Pinellas Environmental Restoration Project Young - Rainey STAR Center Simulation of Enhanced Bioremediation at the Building 100 Area October 2003 Prepared by U.S. Department of Energy Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Document Number N0064700 Contents U.S. Department of Energy at Grand Junction Simulation of Enhanced Bioremediation at the Building 100 Area October 2003 Page ii Contents 1.0 Introduction ............................................................................................................................1 2.0 Assessment of HRC Penetration ............................................................................................1

115

Microsoft Word - PINReuseAward20030723.doc  

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

3, 2003 3, 2003 Energy Department Awards $260,000 Grant to the Pinellas Plant Community Reuse Organization WASHINGTON, DC - The Department of Energy (DOE) announced today that it will award $260,000 to the Pinellas Plant Community Reuse Organization (CRO) located at the department's former Pinellas Plant near Tampa, Fla. The grant will be used for the transition's latest project, titled Suncoast Technology Enterprise Accelerator Project, a program to provide startup enterprises with the necessary specialized business mentoring, technology development and manufacturing planning assistance, and access to all required professional services vital to a successful enterprise. The Suncoast Technology Enterprise Accelerator Project will be located at the Young - Rainey STAR Center.

116

Microsoft Word - N0049800.doc  

Office of Legacy Management (LM)

49800 49800 GJO-2002-306-TAR MAC-PIN 14.5.2 Pinellas Environmental Restoration Project at the Young-Rainey STAR Center Building 100 Area Plume Control Technology Selection Report February 2002 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-96GJ87335 Task Order Number MAC02-10 This page intentionally left blank Document Number N0049800 Contents DOE/Grand Junction Office Building 100 Area Plume Control Technology Selection Report February 2002 Page iii Contents Acronyms and Abbreviations ....................................................................................................... vii Executive Summary .......................................................................................................................

117

n0053200-sitewide.doc  

Office of Legacy Management (LM)

3200 3200 GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center April through June 2002 July 2002 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST02-107 Document Number N0053200 Contents DOE/Grand Junction Office Pinellas Environmental Restoration Project July 2002 Page iii Contents Page Acronyms and Abbreviations .........................................................................................................vii 1.0 Introduction ............................................................................................................................1

118

Better Buildings Residential Program Solution Center Demonstration Webinar Transcript  

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

The Better Buildings Residential Program Solution Center is a robust online collection of nearly 1,000 examples, strategies, and resources from Better Buildings Neighborhood Program partners, Home Performance with ENERGY STAR Sponsors, and others. This webinar presented on November 19, 2014 gives more information on the Solution Center.

119

Supermassive Stars: Fact or Fiction?  

E-Print Network (OSTI)

Supermassive black holes are now realized to exist in the centers of most galaxies. The recent discoveries of luminous quasars at redshifts higher than 6 require that these black holes were assembled already when the Universe was less than a billion years old. They might originate from the collapse of supermassive stars, a scenario which could ensure a sufficiently rapid formation. Supermassive stars are dominated by photon pressure and radiate at their Eddington limit, which drives their quasi-static evolution to a final relativistic instability. Above some critical value of the metallicity, their collapse can lead to a gigantic explosion, powered by the energy release due to hydrogen burning, but below this critical metallicity their collapse inevitably ends in the formation of a black hole, accompanied by the emission of huge amounts of energy in the form of neutrinos. Although collapsing supermassive stars are the most powerful known burst sources of neutrinos, the associated conditions do not appear favorable for producing highly relativistic outflows that can explain cosmic gamma-ray bursts.

H. -Th. Janka

2002-02-01T23:59:59.000Z

120

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

Note: This page contains sample records for the topic "rainey star center" 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

Upsilon Productions at STAR  

E-Print Network (OSTI)

The $\\Upsilon(1S+2S+3S)\\to e^{+}e^{-}$ cross section is measured at mid-rapidity ($y$) in $p+p$ collisions and in d$+Au$ collisions at center-of-mass energy $\\sqrt{s}$ = 200 GeV with the STAR detector at RHIC. In $p+p$, the measured cross section is found to be consistent with the world data trend as a function of $\\sqrt{s}$, in agreement with the Color Evaportaion Model (CEM), and underestimated by the Color Singlet Model (CSM) up to the Next-to-Leading-Order Quantum Chromodynamics (NLO QCD) calculations. In d+$Au$, the measured cross section is in agreement with the CEM prediction with anti-shadowing effects, and the nuclear modification factor indicates that $\\Upsilon(1S+2S+3S)$ production follows binary scaling within the current uncertainties. These measurements provide a benchmark for the future measurements of $\\Upsilon$ production in $Au+Au$ collisions.

A. M. Hamed

2010-05-22T23:59:59.000Z

122

APS Conference Center  

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

Advanced Photon Source Conference Center The APS Conference Center at Argonne National Laboratory is the ideal location for scientific and professional meetings. The Center can...

123

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Fuels Promotion and Information The Center for Alternative Fuels (Center) promotes alternative fuels as viable energy sources in the state. The Center must assess the...

124

Center Research  

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

5 5 Center Research ... Supports Electric Utility Restructuring Winds of change in the U.S. power sector: factors listed in the left column have created a gap between the prices utilities must charge to recover their embedded costs and the lower rates they would have to charge in a competitive environment. Possible responses to these pressures are listed to the right. The electricity industry in the U.S. is being dramatically restructured by state regulatory commissions and the Federal Energy Regulatory Commission. Efforts are underway to create a wholesale market for electricity, with wholesale prices to distributing utility companies no longer being regulated. Discussions in several states and at the FERC are aimed at revising the regulation of the structure, operation, and pricing of the

125

KILLGORE CENTER  

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

LEASE AGREEMENT NO. DE-AC04-89-AL42 1 10 LEASE AGREEMENT NO. DE-AC04-89-AL42 1 10 KILLGORE CENTER AMENDMENT NO. 6 Lease Agreement No. DE-AC04-89-AL-42110, between the U.S. Department of Energy and Texas Tech University, dated October 1, 1989, as amended (amendments one, two, three, four, and five), is hereby further amended as follows: Article I1 of the base lease entitled, "TERM AND RENT," paragraph A., is hereby deleted and revised to read: A. The term of this Lease is extended for five years beginning October 1, 2009, and ending September 30, 2014. The annual rental for this term shall be as indicated in the following rate schedule determined as follows: 1. Approximately 6,680 square feet of office space. $ 58,280.00 2. Approximately 380 square feet of space in the foyer. $ 3,314.00

126

ENERGY STAR Success Story: Staples, Inc.  

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

STAR Success Story: STAR Success Story: Staples, Inc. Staples, the world's largest office products company, has been an energy management and environmental leader in the retail industry for several years. Staples first partnered with the U.S. Environmental Protection Agency's (EPA) Green Lights Program, the predecessor to ENERGY STAR, and in 1999, won the Green Lights Partner of the Year recognition. Staples also has the distinction of being one of the first retailers to benchmark its entire portfolio of over 1,500 retail stores and 200 distribution centers. Even as the company's building portfolio has grown, with total square footage increasing by over 6 percent in just the past three years, Staples has reduced its building portfolio-wide energy usage by more than 11.4%, and recently became the first retailer

127

TRAN-STAR EXECUTIVE LIMOUSINE COMPANY  

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

TRAN-STAR EXECUTIVE LIMOUSINE COMPANY TRAN-STAR EXECUTIVE LIMOUSINE COMPANY http://www.tranexec.com 20% off published rates for BNL Our reservation center is open 24 hours a day, 365 days a year, so you will always talk to a live agent who has direct contact with our chauffeurs. You can make reservations via phone, website or a simple e-mail to customerservice@tranexec.com once a profile has been established. Our advanced reservation system will track any flight and you can rest assured someone will always be there to meet the arriving passenger, no matter what time the flight arrives. http://www.tranexec.com/TranStarSalesBrochure.pdf These rates are inclusive rates, meaning they include gratuity, taxes....everything. They do not include parking or tolls

128

COMMITTEE OF CENTERS AND  

E-Print Network (OSTI)

...................................................................................................... 75 9. CENTER FOR ELECTRIC CAR AND ENERGY CONVERSION............................................... 89

Massachusetts at Lowell, University of

129

2013 Bisfuel Center Retreat at Camp Tontozona | Center for Bio...  

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

Center News Research Highlights Center Research News Media about Center Center Video Library Bisfuel Picture Gallery 2013 Bisfuel Center Retreat at Camp Tontozona 28 Oct 2013 The...

130

STAR Teaching Program Application Period | Department of Energy  

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

STAR Teaching Program Application Period STAR Teaching Program Application Period STAR Teaching Program Application Period December 28, 2012 2:30PM EST to January 31, 2013 5:30PM EST Cal Poly The Science Teacher and Researcher (STAR) Researcher program, a collaborative project of California State University, provides pre-service and early career science teachers with eight week long paid mentor and research opportunities at a national research center. Applicants must have the following: A demonstrated interest in becoming a science or mathematics teacher at the secondary level (grades 6-12) Either a California State University (CSU) student OR NSF Noyce Scholar in the United States OR a STAR Alum with two or fewer years of participation AND two or fewer years of teaching experience (first time participants must be pre-service teachers, i.e., not yet teaching full-time

131

Data Center Report to Congress -FINAL 7-25-07.doc  

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

Server and Data Center Energy Efficiency Server and Data Center Energy Efficiency Public Law 109-431 U.S. Environmental Protection Agency ENERGY STAR Program August 2, 2007 Table of Contents Table of Contents............................................................................................................................. i Executive Summary ........................................................................................................................ 4 Background ................................................................................................................................. 4 Energy Use in Data Centers Through 2011 ................................................................................ 7 Incentives and Voluntary Programs to Promote Energy Efficiency ......................................... 11

132

The role of magnetic fields in hyperon stars  

SciTech Connect

We investigate the effects of strong magnetic fields (SMF) on the properties of neutron stars that have hyperons in their composition. The matter is described by a hadronic model in which a parameterized and derivative coupling between hadrons and mesons is considered. We study the magnetic effects on the equation of state (EoS) from Landau quantization, assuming a density dependent static magnetic field that reaches 10{sup 19} G in the center of the star. The Tolman- Oppenheimer-Volkoff (TOV) equations are solved in order to show the dependence of the massradius relation and population of hyperon stars on the central magnetic field and on different hyperon coupling schemes.

Gomes, R. O.; Vasconcellos, C. A. Z. [Instituto de Fsica - Universidade Federal do Rio Grande do Sul, Porto Alegre, RS 91501-970 (Brazil); Dexheimer, V. [Department of Physics - Kent State University, Kent, OH 44242 (United States)

2014-05-09T23:59:59.000Z

133

Stars and statistical physics: A teaching experience  

Science Journals Connector (OSTI)

The physics of stars their workings and their evolution is a goldmine of problems in statistical mechanics and thermodynamics. We discuss many examples that illustrate the possibility of deepening students knowledge of statistical mechanics by an introductory study of stars. The matter constituting the various stellar objects provides examples of equations of state for classical or quantal and relativistic or non-relativistic gases. Maximum entropy can be used to characterize thermodynamic and gravitational equilibrium which determines the structure of stars and predicts their instability above a certain mass. Contraction accompanying radiation induces either heating or cooling which explains the formation of stars above a minimum mass. The characteristics of the emitted light are understood from blackbody radiation and more precisely from the BoltzmannLorentz kinetic equation for photons. The luminosity is governed by the transport of heat by photons from the center to the surface. Heat production by thermonuclear fusion is determined by microscopic balance equations. The stability of the steady state of stars is controlled by the interplay of thermodynamics and gravitation.

Roger Balian; Jean-Paul Blaizot

1999-01-01T23:59:59.000Z

134

Maintaining STAR - Hanford Site  

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

VPP Hanford Site Champions Committee Getting Started Maintaining STAR VPP CampaignPosters VPP Tools VPP Presentations VPP Awareness VPP Communications VPP Conferences...

135

Star-ND (Multi-Dimensional Star-Identification)  

E-Print Network (OSTI)

In order to perform star-identification with lower processing requirements, multi-dimensional techniques are implemented in this research as a database search as well as to create star pattern parameters. New star pattern parameters are presented...

Spratling, Benjamin

2012-07-16T23:59:59.000Z

136

ATOMIC HYDROGEN IN A GALACTIC CENTER OUTFLOW  

SciTech Connect

We describe a population of small, high-velocity, atomic hydrogen clouds, loops, and filaments found above and below the disk near the Galactic center. The objects have a mean radius of 15 pc, velocity widths of {approx}14 km s{sup -1}, and are observed at |z| heights up to 700 pc. The velocity distribution of the clouds shows no signature of Galactic rotation. We propose a scenario where the clouds are associated with an outflow from a central star-forming region at the Galactic center. We discuss the clouds as entrained material traveling at {approx}200 km s{sup -1} in a Galactic wind.

McClure-Griffiths, N. M.; Green, J. A.; Hill, A. S. [Australia Telescope National Facility, CSIRO Astronomy and Space Science, Marsfield, NSW 2122 (Australia); Lockman, F. J. [National Radio Astronomy Observatory, Green Bank, WV 24944 (United States); Dickey, J. M. [School of Physics and Mathematics, University of Tasmania, TAS 7001 (Australia); Gaensler, B. M.; Green, A. J., E-mail: naomi.mcclure-griffiths@csiro.au [Sydney Institute for Astronomy, School of Physics, The University of Sydney, NSW 2006 (Australia)

2013-06-10T23:59:59.000Z

137

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

138

Microsoft Word - N01628_Sitewide semiannual Dec-May 2011  

Office of Legacy Management (LM)

Bryan Dairy Road immediately south of the Building 100 Area at the Young - Rainey Science Technology and Research Center. A direct-push drill rig was used to collect...

139

Video Center Administrator Guide  

E-Print Network (OSTI)

LifeSize® Video Center Administrator Guide March 2011 LifeSize Video Center 2200 #12;LifeSize Video Center Adminstrator Guide 2 Administering LifeSize Video Center LifeSize Video Center is a network server that stores and streams video sent by LifeSize video communications systems enabled for recording. It can also

Eisen, Michael

140

Neutron Stars and Fractal Dimensionality  

E-Print Network (OSTI)

We argue that the material inside Neutron stars behaves anomalously with fractal statistics and that in principle, we could induce mini Neutron stars, with the release of energy.

Burra G. Sidharth

2008-05-06T23:59:59.000Z

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


141

Carbon Stars | Open Energy Information  

Open Energy Info (EERE)

Stars Jump to: navigation, search Name: Carbon Stars Place: Netherlands Sector: Services Product: General Financial & Legal Services ( Private family-controlled ) References:...

142

Energy Center Center for Coal Technology Research  

E-Print Network (OSTI)

Energy Center Center for Coal Technology Research http://www.purdue.edu/dp/energy/CCTR/ Consumption Production Gasification Power Plants Coking Liquid Fuels Environment Oxyfuels Byproducts Legislation, 500 Central Drive West Lafayette, IN 47907-2022 #12;INDIANA COAL REPORT 2009 Center for Coal

Fernández-Juricic, Esteban

143

Chemical Hydrogen Storage Center Center of Excellence  

E-Print Network (OSTI)

alternatives and assess economics and life cycle analysis of borohydride/water to hydrogen · Millennium CellChemical Hydrogen Storage Center Center of Excellence for Chemical Hydrogen Storage William Tumas proprietary or confidential information #12;2 Chemical Hydrogen Storage Center Overview Project Start Date: FY

Carver, Jeffrey C.

144

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

145

PNNL: News Center - Search  

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

Newsroom Search the News Center Keywords Search News Center News Center Home News Releases Social Media Directory PNNL Leadership Our Experts Subscribe to E-Mail News Service RSS...

146

Centers | ornl.gov  

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

Centers Centers SHARE Centers BioEnergy Science Center (BESC) The BioEnergy Science Center (BESC) is a multi-institutional (17 partners), multidisciplinary research (biological, chemical, physical and computational sciences, mathematics and engineering) organization focused on the fundamental understanding and elimination of biomass recalcitrance. DOE Energy Frontier Research Centers The Energy Frontier Research Centers program aims to accelerate such transformative discovery, combining the talents and creativity of our national scientific workforce with a powerful new generation of tools for penetrating, understanding, and manipulating matter on the atomic and molecular scales. ORNL is also home to two DOE Energy Frontier Research Centers, the Fluid Interface, Reactions, Structures and Transport (FIRST)

147

Benchmarking Help Center Guide  

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

Benchmarking Help Center Guide provides recommendations for establishing a benchmarking help center based on experiences and lessons learned in New York City and Seattle.

148

Energy Efficient Data Centers  

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

Presentationgiven at the Federal Utility Partnership Working Group (FUPWG) Fall 2008 meetingcovers energy efficiency improvement opportunities for data centers, including data center design.

149

S M Stoller Star Center-B100  

Office of Legacy Management (LM)

B100 B100 7030-226/Monthly Accutest Job Number: F27169 Sampling Date: 10/05/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director

150

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

7170 7170 Sampling Date: 10/05/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director e-Hardcopy 2.0 Automated Report 12 1 of 12

151

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

227 227 Sampling Dates: 03/31/04 - 04/01/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director e-Hardcopy 2.0 Automated Report

152

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

WWNA Monthly; Largo, FL WWNA Monthly; Largo, FL 7031-226 Accutest Job Number: F36361 Sampling Date: 11/03/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

153

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

124 124 Sampling Date: 01/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director e-Hardcopy 2.0 Automated Report 18 1 of 18

154

S M Stoller Quarterly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

531 531 Sampling Date: 04/16/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director e-Hardcopy 2.0 Automated Report 21 1 of 21

155

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

8014 8014 Sampling Date: 11/09/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director e-Hardcopy 2.0 Automated Report 12 1 of 12

156

S M Stoller Star Center-B100  

Office of Legacy Management (LM)

B100 B100 110406202 Accutest Job Number: F33040 Sampling Date: 07/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D. Laboratory Director

157

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

WWNA Monthly; Largo, FL WWNA Monthly; Largo, FL 110406202 Accutest Job Number: F25982 Sampling Date: 08/10/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

158

S M Stoller Star Center-B100  

Office of Legacy Management (LM)

B100 B100 Monthly Sampling, 110406202 Accutest Job Number: F25245 Sampling Date: 07/06/04 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

159

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

WWNA Monthly; Largo, FL WWNA Monthly; Largo, FL 7030-226 Accutest Job Number: F33038 Sampling Date: 07/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

160

S M Stoller Monthly Sampling (Pinellas Co), STAR Center, Largo...  

Office of Legacy Management (LM)

* Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http:www.accutest.com Test results contained within this data package meet the requirements of the National...

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


161

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

623 Sampling Date: 020205 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ...

162

S M Stoller Star Center-WWNA Monthly; Largo, FL  

Office of Legacy Management (LM)

Chloroform ND 1.0 0.50 ugl 110-75-8 2-Chloroethyl vinyl ether ND 5.0 2.5 ugl 56-23-5 Carbon tetrachloride ND 1.0 0.50 ugl 75-34-3 1,1-Dichloroethane ND 1.0 0.50 ugl 75-35-4...

163

S M Stoller Monthly Sampling, STAR Center, Largo, FL  

Office of Legacy Management (LM)

Chloroform ND 1.0 0.50 ugl 110-75-8 2-Chloroethyl vinyl ether ND 5.0 2.5 ugl 56-23-5 Carbon tetrachloride ND 1.0 0.50 ugl 75-34-3 1,1-Dichloroethane ND 1.0 0.50 ugl 75-35-4...

164

Hyperons in neutron stars  

E-Print Network (OSTI)

Using the Dirac-Brueckner-Hartree-Fock approach, the properties of neutron-star matter including hyperons are investigated. In the calculation, we consider both time and space components of the vector self-energies of baryons as well as the scalar ones. Furthermore, the effect of negative-energy states of baryons is partly taken into account. We obtain the maximum neutron-star mass of $2.08\\,M_{\\odot}$, which is consistent with the recently observed, massive neutron stars. We discuss a universal, repulsive three-body force for hyperons in matter.

Katayama, Tetsuya

2015-01-01T23:59:59.000Z

165

On the conversion of neutron stars into quark stars  

E-Print Network (OSTI)

The possible existence of two families of compact stars, neutron stars and quark stars, naturally leads to a scenario in which a conversion process between the two stellar objects occurs with a consequent release of energy of the order of $10^{53}$ erg. We discuss recent hydrodynamical simulations of the burning process and neutrino diffusion simulations of cooling of a newly formed strange star. We also briefly discuss this scenario in connection with recent measurements of masses and radii of compact stars.

Giuseppe Pagliara

2013-12-04T23:59:59.000Z

166

Designing for Sustainability: Houston DOW Center LEED Gold  

E-Print Network (OSTI)

materials ? Plastic moving crates in place of cardboard boxes ? Energy Star rated appliances ? Secondary Goals ? Building operating cost savings ? Community outreach Driving Energy Efficiency at Dow Designing for Sustainability Houston Dow Center... capable of housing 1,200 employees ? Energy efficient ? Sustainable ? Good location close to employees ? Cost effective ? Project to be started in 2007 and completed by November 2008 Designing for Sustainability Houston Dow Center Search for a LEED...

McCall, H.; McVey, K.; Rash, A.

167

Reliability-Centered Maintenance  

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

Reliability-centered maintenance leverages the same practices and technologies of predictive maintenance.

168

Nuclear Reactions in Stars  

Science Journals Connector (OSTI)

21 February 1961 research-article Nuclear Reactions in Stars T. G. Cowling Thermonuclear reactions important for the generation of stellar energy during different phases of stellar evolution are discussed. The Royal...

1961-01-01T23:59:59.000Z

169

Neutron stars - thermal emitters  

E-Print Network (OSTI)

Confronting theoretical models with observations of thermal radiation emitted by neutron stars is one of the most important ways to understand the properties of both, superdense matter in the interiors of the neutron stars and dense magnetized plasmas in their outer layers. Here we review the theory of thermal emission from the surface layers of strongly magnetized neutron stars, and the main properties of the observational data. In particular, we focus on the nearby sources for which a clear thermal component has been detected, without being contaminated by other emission processes (magnetosphere, accretion, nebulae). We also discuss the applications of the modern theoretical models of the formation of spectra of strongly magnetized neutron stars to the observed thermally emitting objects.

Potekhin, A Y; Pons, J A

2014-01-01T23:59:59.000Z

170

Masers and star formation  

E-Print Network (OSTI)

Recent observational and theoretical advances concerning astronomical masers in star forming regions are reviewed. Major masing species are considered individually and in combination. Key results are summarized with emphasis on present science and future prospects.

Vincent L. Fish

2007-04-02T23:59:59.000Z

171

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

AFDC AFDC Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Alternative Fuels Data Center: Page Not Found Skip to Content Eere_header_logo U.S. Department of Energy Energy Efficiency and Renewable Energy EERE Home | Programs & Offices | Consumer Information Alternative Fuels Data Center Search Search Help Alternative Fuels Data Center Fuels & Vehicles Biodiesel | Diesel Vehicles

172

Holographic Neutron Stars  

E-Print Network (OSTI)

We construct in the context of the AdS/CFT correspondence degenerate composite operators in the conformal field theory that are holographically dual to degenerate stars in anti de Sitter space. We calculate the effect of the gravitational back-reaction using the Tolman-Oppenheimer-Volkoff equations, and determine the "Chandrasekhar limit" beyond which the star undergoes gravitational collapse towards a black hole.

Jan de Boer; Kyriakos Papadodimas; Erik Verlinde

2009-07-16T23:59:59.000Z

173

Guidance for Preparing ENERGY STAR Challenge for Industry Plant Profile  

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

Long Beach Douglas Center Long Beach Douglas Center The Boeing Company 4000 Lakewood Blvd. Long Beach, CA 90808 The Boeing Long Beach Douglas Center campus hosts a wide array of activities supporting the development of commercial airplanes including: Airplane Programs Engineering, Product Support Engineering, Modification Services, Spares, and Continental Data Graphics. This site achieved the Challenge for Industry in 2010, 2011 and 2012. Achieving the ENERGY STAR Challenge for Industry has been a key factor in Boeing's 'four walls' strategy to reduce energy usage and waste along with reducing the environmental footprint of its operations. The energy savings was achieved by upgrading air-conditioning, lighting and energy-management systems,

174

A star cluster at the edge of the Galaxy  

E-Print Network (OSTI)

We study stars and molecular gas in the direction of IRAS06145+1455 (WB89-789) through NIR (JHK), molecular line-, and dust continuum observations. The kinematic distance of the associated molecular cloud is 11.9 kpc. With a galactocentric distance of about 20.2 kpc, this object is at the edge of the (molecular) disk of the Galaxy. The near-IR data show the presence of an (embedded) cluster of about 60 stars, with a radius ca. 1.3 pc and an average stellar surface density of ca. 12 pc^{-2}. We find at least 14 stars with NIR-excess, 3 of which are possibly Class I objects. The cluster is embedded in a 1000 Mo molecular/dust core, from which a molecular outflow originates. The temperature of most of the outflowing gas is < 40 K, and the total mass of the swept-up material is < 10 Mo. Near the center of the flow, indications of much higher temperatures are found, probably due to shocks. A spectrum of one of the probable cluster members shows a tentative likeness to that of a K3III-star (with an age of at least 20 Myr). If correct, this would confirm the kinematic distance. This cluster is the furthest one from the Galactic center yet detected. The combination of old and recent activity implies that star formation has been going on for at least 20 Myr, which is difficult to understand considering the location of this object, where external triggers are either absent or weak, compared to the inner Galaxy. This suggests that once star formation is occurring, later generations of stars may form through the effect of the first generation of stars on the (remnants of) the original molecular cloud.

J. Brand; J. G. A. Wouterloot

2007-02-20T23:59:59.000Z

175

The Era of Star Formation in Galaxy Clusters  

E-Print Network (OSTI)

We analyze the star formation properties of 16 infrared-selected, spectroscopically confirmed galaxy clusters at $1 1.35$. Using infrared luminosities measured with deep Spitzer/MIPS observations at 24 $\\mu$m, along with robust optical+IRAC photometric redshifts and SED-fitted stellar masses, we present the dust-obscured star-forming fractions, star formation rates and specific star formation rates in these clusters as functions of redshift and projected clustercentric radius. We find that $z\\sim 1.4$ represents a transition redshift for the ISCS sample, with clear evidence of an unquenched era of cluster star formation at earlier times. Beyond this redshift the fraction of star-forming cluster members increases monotonically toward the cluster centers. Indeed, the specific star formation rate in the cores of these distant clusters is consistent with field values at similar redshifts, indicating that at $z>1.4$ environment-dependent quenching had not yet been established in ISCS clusters. Combining these obse...

Brodwin, M; Gonzalez, Anthony H; Zeimann, G R; Snyder, G F; Mancone, C L; Pope, A; Eisenhardt, P R; Stern, D; Alberts, S; Ashby, M L N; Brown, M J I; Chary, R -R; Dey, Arjun; Galametz, A; Gettings, D P; Jannuzi, B T; Miller, E D; Moustakas, J; Moustakas, L A

2013-01-01T23:59:59.000Z

176

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

177

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

178

Star Power | Princeton Plasma Physics Lab  

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

Star Power Star Power The U.S. Department of Energy's Princeton Plasma Physics Laboratory has released "Star Power," a new informational video that uses dramatic and beautiful...

179

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

180

Compact boson stars in K field theories  

E-Print Network (OSTI)

We study a scalar field theory with a non-standard kinetic term minimally coupled to gravity. We establish the existence of compact boson stars, that is, static solutions with compact support of the full system with self-gravitation taken into account. Concretely, there exist two types of solutions, namely compact balls on the one hand, and compact shells on the other hand. The compact balls have a naked singularity at the center. The inner boundary of the compact shells is singular, as well, but it is, at the same time, a Killing horizon. These singular, compact shells therefore resemble black holes.

C. Adam; N. Grandi; P. Klimas; J. Sanchez-Guillen; A. Wereszczynski

2009-09-16T23:59:59.000Z

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


181

Compact boson stars in K field theories  

E-Print Network (OSTI)

We study a scalar field theory with a non-standard kinetic term minimally coupled to gravity. We establish the existence of compact boson stars, that is, static solutions with compact support of the full system with self-gravitation taken into account. Concretely, there exist two types of solutions, namely compact balls on the one hand, and compact shells on the other hand. The compact balls have a naked singularity at the center. The inner boundary of the compact shells is singular, as well, but it is, at the same time, a Killing horizon. These singular, compact shells therefore resemble black holes.

Adam, C; Klimas, P; Snchez-Guilln, J; Wereszczynski, A

2009-01-01T23:59:59.000Z

182

Star Formation in the Local Universe  

E-Print Network (OSTI)

We present preliminary results of a long-term study aimed at answering a number of open questions on the evolution of starbursts in local galaxies. The project employes mainly HST data from the ultraviolet to the red of the stellar continuum and of the nebular emission from the galaxies. Here we concentrate on NGC5253 and NGC5236 (M83), that form a dwarf--massive galaxy pair at about 4 Mpc distance. The recent star formation history of the centers of the two galaxies is investigated in order to identify similarities and differences in the evolution of their central starbursts.

Daniela Calzetti; Jason Harris

2001-11-28T23:59:59.000Z

183

Variable Star Network: World Center for Transient Object Astronomy and Variable Stars  

Science Journals Connector (OSTI)

......from the Ministry of Education, Culture, Sports, Science and Technology. Part...for the Promotion of Science for Young Scientists...GCVS. Appendix 1. Poster Presented at the 23rd...for the Promotion of Science for Young Scientists......

Taichi Kato; Makoto Uemura; Ryoko Ishioka; Daisaku Nogami; Chatief Kunjaya; Hajime Baba; Hitoshi Yamaoka

2004-03-25T23:59:59.000Z

184

Variable Star Network: World Center for Transient Object Astronomy and Variable Stars  

Science Journals Connector (OSTI)

......2001; Duerbeck 2002; Clayton 2002; Jeffery, Pollacco 2002; Kamath, Ashok 2002...Frank J. 1982b, Nature, 300, 152. Jeffery C. S. , Pollacco D. 2002, ApSS, 279...7253. Swartz D. A. , Clocchiatti A., Benjamin R., Lester D. F., Wheeler J. C......

Taichi Kato; Makoto Uemura; Ryoko Ishioka; Daisaku Nogami; Chatief Kunjaya; Hajime Baba; Hitoshi Yamaoka

2004-03-25T23:59:59.000Z

185

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Center to someone by E-mail Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Local Laws and Incentives There are a variety of local laws and incentives that support reducing U.S. petroleum consumption by encouraging or requiring individuals and/or public and private organizations to use alternative fuels, advanced vehicles, and strategies to decrease fuel use or increase fuel economy. Local city and county governments create such laws and incentives to ensure people use

186

About Cost Center  

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

from the university, fee-for-service contracts, as well as establishing CAMD as a cost center. We know that our users are reluctant to see CAMD become a cost center, however...

187

NREL: Education Center - Events  

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

phone number is 303-384-6565. November 2014 Education Center Holiday Hours November 26 - December 1, 2014 Golden, CO Contact: NREL Education Center 303-384-6565 The NREL...

188

ARM - News Center Archive  

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

3 1 BAECC 1 BBOP 4 ENA 1 GOAMAZON 6 MAGIC 15 MC3E 17 SGP 3 STORMVEX 29 TCAP 3 Search News Search Blog News Center All Categories What's this? Social Media Guidance News Center...

189

LANSCE | Lujan Center | Publications  

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

use of add here name of specific Lujan instruments at the Lujan Center at Los Alamos Neutron Science Center. Los Alamos National Laboratory is operated by Los Alamos National...

190

ENERGY CENTER OF WISCONSIN  

E-Print Network (OSTI)

ENERGY CENTER OF WISCONSIN report report report report report report report report report report energy center Report 193-1 Fuel Cells for Distributed Generation A Technology and Marketing Summary March

Wisconsin at Madison, University of

191

INTERNATIONAL PACIFIC RESEARCH CENTER  

E-Print Network (OSTI)

INTERNATIONAL PACIFIC RESEARCH CENTER APRIL 2004­MARCH 2005 REPORT SCHOOL OF OCEAN AND EARTH RESEARCH HIGHLIGHTS Indo-Pacific Ocean Climate Pacific Research Center Design by: Susan Yamamoto Printed by: Hagadone Printing Company Photo: Waikiki

Wang, Yuqing

192

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Center to someone by E-mail Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Recent Federal Actions This list includes recent federal actions, such as Federal Register notices and rulemaking actions, agency directives or agency communications, that are all publicly available. These actions relate to alternative fuels and vehicles, fuel blends, hybrid vehicles, and idle reduction and fuel economy measures. When rulemakings are finalized, they will move to the list of

193

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Center to someone by E-mail Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Expired, Repealed, and Archived Federal Incentives and Laws The following is a list of expired, repealed, and archived incentives, laws, regulations, funding opportunities, or other initiatives related to alternative fuels and vehicles, advanced technologies, or air quality. Value-Added Producer Grants (VAPG) Archived: 12/31/2012

194

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Tools Tools Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... Truckstop Electrification Truck Stop Electrification Locator Locate truck stops with electrification sites. Click on a location on the map for site details. A U.S. Department of Energy Energy Efficiency and Renewable Energy Source: Alternative Fuels Data Center dditional Resources View list of electrification sites in the U.S. by state. Learn more about idle reduction techniques.

195

Cooling of neutron stars  

Science Journals Connector (OSTI)

On the basis of current physical understanding, it is impossible to predict with confidence the interior constitution of neutron stars. Cooling of neutron stars provides a possible way of discriminating among possible states of matter within them. In the standard picture of cooling by neutrino emission developed over the past quarter of a century, neutron stars are expected to cool relatively slowly if their cores are made up of nucleons, and to cool faster if matter is in an exotic state, such as a pion condensate, a kaon condensate, or quark matter. This view has recently been called into question by the discovery of a number of other processes that could lead to copious neutrino emission and rapid cooling.

C. J. Pethick

1992-10-01T23:59:59.000Z

196

Microsoft Word - N01180_4.5Acre Dec-May08Edited  

Office of Legacy Management (LM)

Center's Center's 4.5 Acre Site December 2007 through May 2008 June 2008 Office of Legacy Management LMS/PIN/N01180 Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AM01-07LM00060 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy LMS/PIN/N01180 Pinellas Environmental Restoration Project Semiannual Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site December 2007 Through May 2008 June 2008 U.S. Department of Energy 4.5 Acre Site Semiannual Progress Report for December 2007 through May 2008 June 2008 Doc. No. N0118000 Page ii Contents Acronyms and Abbreviations ........................................................................................................

197

On the efficiency of field star capture by star clusters  

E-Print Network (OSTI)

An exciting recent finding regarding scaling relations among globular clusters is the so-called 'blue tilt': clusters of the blue sub-population follow a trend of redder colour with increasing luminosity. In this paper we evaluate to which extent field star capture over a Hubble time may explain the 'blue tilt'. We perform collisional N-body simulations to quantify the amount of field star capture occuring over a Hubble time to star clusters with 10^3 to 10^6 stars. In the simulations we follow the orbits of field stars passing through a star cluster and calculate the energy change that the field stars experience due to gravitational interaction with cluster stars during one passage through the cluster. The capture condition is that their total energy after the passage is smaller than the gravitational potential at the cluster's tidal radius. By folding this with the fly-by rates of field stars with an assumed space density as in the solar neighbourhood and a range of velocity dispersions, we derive estimates on the mass fraction of captured field stars as a function of environment. We find that integrated over a Hubble time, the ratio between captured field stars and total number of clusters stars is very low (capture is not a probable mechanism for creating the colour-magnitude trend of metal-poor globular clusters.

Steffen Mieske; Holger Baumgardt

2007-09-10T23:59:59.000Z

198

Energy Technology Engineering Center  

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

Technology Engineering Center Technology Engineering Center 41 00 Guardian Street, Suite # 160 Simi Valley, CA 93063 Memorandum for: Gregory H. Woods General Council January 30, 2013 FROM: John Jones EL\= Federal Proje� irector Energy Technology Engineering Center (ETEC) Project Office SUBJECT: Annual National Environmental Policy Act {NEPA) Planning Summary Attached is the 2013 Annual NEPA Planning Summary for the ETEC Project Office.

199

Louisiana Transportation Research Center  

E-Print Network (OSTI)

Louisiana Transportation Research Center LTRC www.ltrc.lsu.edu 2012-13 ANNUALREPORT #12;The Louisiana Transportation Research Center (LTRC) is a research, technology transfer, and training center administered jointly by the Louisiana Department of Transportation and Development (DOTD) and Louisiana State

Harms, Kyle E.

200

A Star on Earth  

ScienceCinema (OSTI)

At the Energy Department's Princeton Plasma Physics Lab, scientists are trying to accomplish what was once considered the realm of science fiction: create a star on Earth. The National Spherical Torus Experiment (NSTX) is a magnetic fusion device that is used to study the physics principles of spherically shaped plasmas -- hot ionized gases in which, under the right conditions, nuclear fusion will occur. Fusion is the energy source of the sun and all of the stars. Not just limited to theoretical work, the NSTX is enabling cutting-edge research to develop fusion as a future energy source.

Prager, Stewart; Zwicker, Andrew; Hammet, Greg; Tresemer, Kelsey; Diallo, Ahmed

2014-06-06T23:59:59.000Z

Note: This page contains sample records for the topic "rainey star center" 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

A Star on Earth  

SciTech Connect

At the Energy Department's Princeton Plasma Physics Lab, scientists are trying to accomplish what was once considered the realm of science fiction: create a star on Earth. The National Spherical Torus Experiment (NSTX) is a magnetic fusion device that is used to study the physics principles of spherically shaped plasmas -- hot ionized gases in which, under the right conditions, nuclear fusion will occur. Fusion is the energy source of the sun and all of the stars. Not just limited to theoretical work, the NSTX is enabling cutting-edge research to develop fusion as a future energy source.

Prager, Stewart; Zwicker, Andrew; Hammet, Greg; Tresemer, Kelsey; Diallo, Ahmed

2014-03-05T23:59:59.000Z

202

Aircraft Integration and Flight Testing of 4STAR  

SciTech Connect

Under funding from the U.S. Dept. of Energy, in conjunction with a funded NASA 2008 ROSES proposal, with internal support from Battelle Pacific Northwest Division (PNWD), and in collaboration with NASA Ames Research Center, we successfully integrated the Spectrometer for Sky-Scanning, Sun-Tracking Atmospheric Research (4STAR-Air) instrument for flight operation aboard Battelles G-1 aircraft and conducted a series of airborne and ground-based intensive measurement campaigns (hereafter referred to as intensives) for the purpose of maturing the initial 4STAR-Ground prototype to a flight-ready science-ready configuration.

Flynn, CJ; Kassianov, E; Russell, P; Redemann, J; Dunagan, S; Holben, B

2012-10-12T23:59:59.000Z

203

Star Biomass | Open Energy Information  

Open Energy Info (EERE)

India Sector: Biomass Product: Plans to set up biomass projects in Rajasthan. References: Star Biomass1 This article is a stub. You can help OpenEI by expanding it. Star Biomass...

204

Center for Bio-inspired Solar Fuel Production Personnel | Center...  

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

Center for Bio-inspired Solar Fuel Production Personnel Principal Investigators Postdoctoral Fellows Center researchers Graduate Students Undergraduate Students All Bisfuel Center...

205

Star clusters as diaries of galaxies  

E-Print Network (OSTI)

Most if not all stars form in star clusters. Thus the distribution of star clusters preserves the information on the star formation history of a galaxy. Massive clusters form only during episodes of high star formation activity whereas periods of low star formation activity cannot produce them. We present here the method of Maschberger & Kroupa (2007) to derive the star formation history of a galaxy from its star-cluster content.

Th. Maschberger; P. Kroupa

2007-06-11T23:59:59.000Z

206

ADVANCED BURNING STAGES AND FATE OF 8-10 M{sub Sun} STARS  

SciTech Connect

The stellar mass range 8 {approx}< M/M{sub Sun} {approx}< 12 corresponds to the most massive asymptotic giant branch (AGB) stars and the most numerous massive stars. It is host to a variety of supernova (SN) progenitors and is therefore very important for galactic chemical evolution and stellar population studies. In this paper, we study the transition from super-AGB (SAGB) star to massive star and find that a propagating neon-oxygen-burning shell is common to both the most massive electron capture supernova (EC-SN) progenitors and the lowest mass iron-core-collapse supernova (FeCCSN) progenitors. Of the models that ignite neon-burning off-center, the 9.5 M{sub Sun} star would evolve to an FeCCSN after the neon-burning shell propagates to the center, as in previous studies. The neon-burning shell in the 8.8 M{sub Sun} model, however, fails to reach the center as the URCA process and an extended (0.6 M{sub Sun }) region of low Y{sub e} (0.48) in the outer part of the core begin to dominate the late evolution; the model evolves to an EC-SN. This is the first study to follow the most massive EC-SN progenitors to collapse, representing an evolutionary path to EC-SN in addition to that from SAGB stars undergoing thermal pulses (TPs). We also present models of an 8.75 M{sub Sun} SAGB star through its entire TP phase until electron captures on {sup 20}Ne begin at its center and of a 12 M{sub Sun} star up to the iron core collapse. We discuss key uncertainties and how the different pathways to collapse affect the pre-SN structure. Finally, we compare our results to the observed neutron star mass distribution.

Jones, S.; Hirschi, R. [Astrophysics Group, Lennard Jones Building, Keele University, Staffordshire ST5 5BG (United Kingdom); Nomoto, K. [Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583 (Japan); Fischer, T.; Martinez-Pinedo, G. [GSI Helmholtzzentrum fuer Schwerionenforschung GmbH, Planckstrasse 1, D-64291 Darmstadt (Germany); Timmes, F. X. [School of Earth and Space Exploration, University of Arizona, Tempe, AZ 85287 (United States); Herwig, F. [Joint Institute for Nuclear Astrophysics, University of Notre Dame, IN 46556 (United States); Paxton, B. [KITP and Department of Physics, University of California, Santa Barbara, CA 93106 (United States); Toki, H. [Research Center for Nuclear Physics (RCNP), Osaka University, Osaka 567-0047 (Japan); Suzuki, T. [Department of Physics, College of Humanities and Sciences, Nihon University Sakurajosui 3-25-40, Setagaya-ku, Tokyo 156-8550 (Japan); Lam, Y. H. [Institut fuer Kernphysik, Technische Universitaet Darmstadt, Schlossgartenstrasse 2, D-64289 Darmstadt (Germany); Bertolli, M. G., E-mail: s.w.jones@keele.ac.uk [Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545 (United States)

2013-08-01T23:59:59.000Z

207

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

208

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

209

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

210

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Tools Tools Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... Fuel Properties Search Fuel Properties Comparison Create a custom chart comparing fuel properties and characteristics for multiple fuels. Select the fuel and properties of interest. Select Fuels Clear all All Fuels Gasoline Diesel (No. 2) Biodiesel Compressed Natural Gas (CNG) Electricity Ethanol Hydrogen Liquefied Natural Gas (LNG) Propane (LPG)

211

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Electricity » Laws & Incentives Electricity » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Electricity Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for EVs The list below contains summaries of all Federal laws and incentives related to EVs. Incentives Alternative Fuel Infrastructure Tax Credit Fueling equipment for natural gas, liquefied petroleum gas (propane),

212

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Propane » Laws & Incentives Propane » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Propane Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for Propane (LPG) The list below contains summaries of all Federal laws and incentives related to Propane (LPG). Incentives Alternative Fuel Infrastructure Tax Credit Fueling equipment for natural gas, liquefied petroleum gas (propane),

213

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Biodiesel » Laws & Incentives Biodiesel » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Biodiesel Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for Biodiesel The list below contains summaries of all Federal laws and incentives related to Biodiesel. Incentives Alternative Fuel Infrastructure Tax Credit Fueling equipment for natural gas, liquefied petroleum gas (propane),

214

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Ethanol » Laws & Incentives Ethanol » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Ethanol Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for Ethanol The list below contains summaries of all Federal laws and incentives related to Ethanol. Incentives Alternative Fuel Infrastructure Tax Credit Fueling equipment for natural gas, liquefied petroleum gas (propane),

215

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Hydrogen » Laws & Incentives Hydrogen » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Hydrogen Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for Hydrogen Fuel Cells The list below contains summaries of all Federal laws and incentives related to Hydrogen Fuel Cells. Incentives Alternative Fuel Tax Exemption Alternative fuels used in a manner that the Internal Revenue Service (IRS)

216

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Tools Tools Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... Data Included in the Alternative Fuel Stations Download The following data fields are provided in the downloadable files for alternative fuel stations. Field Value Description fuel_type_code Type: string The type of alternative fuel the station provides. Fuel types are given as code values as described below: Value Description BD Biodiesel (B20 and above)

217

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Conserve Fuel » Laws & Incentives Conserve Fuel » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Biodiesel Electricity Ethanol Hydrogen Natural Gas Propane Emerging Fuels Fuel Prices Federal Laws and Incentives for Idle Reduction The list below contains summaries of all Federal laws and incentives related to Idle Reduction. Incentives Idle Reduction Technology Excise Tax Exemption Qualified on-board idle reduction devices and advanced insulation are

218

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Natural Gas » Laws & Incentives Natural Gas » Laws & Incentives Printable Version Share this resource Send a link to Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center on AddThis.com... More in this section... Natural Gas Basics Benefits & Considerations Stations Vehicles Laws & Incentives Federal Laws and Incentives for Natural Gas The list below contains summaries of all Federal laws and incentives related to Natural Gas. Incentives Alternative Fuel Infrastructure Tax Credit Fueling equipment for natural gas, liquefied petroleum gas (propane),

219

Massive Star Outflows  

E-Print Network (OSTI)

Molecular outflows in the form of wide-angle winds and/or well-collimated jets are associated with young stellar objects of all luminosities. Independent studies have established that the mass outflow rate is proportional to L_bol^0.6 for L_bol = 0.3 to 10^5 L_sun, suggesting that there is a strong link between accretion and outflow for a wide range of source luminosity and there is reasonable evidence that accretion-related processes are responsible for generating massive molecular flows from protostars up to spectral type B0. Beyond L_bol ~ 10^4 L_sun, O stars generate powerful wide-angle, ionized winds that can dramatically affect outflow morphology and even call into question the relationship between outflow and accretion. Recently Beuther & Shepherd (2005) proposed an evolutionary scenario in which massive protostellar flows (up to early B spectral type) begin collimated. Once the star reaches the Main Sequence, ionizing radiation may affect the balance between magnetic and plasma pressure, inducing changes in the flow morphology and energetics. Here I review the properties of outflows from young OB stars, discuss implications and observational tests of this proposed evolutionary scenario, and examine differences between low-mass and massive star formation.

D. S. Shepherd

2005-06-01T23:59:59.000Z

220

Physical Processes in Stars  

Science Journals Connector (OSTI)

... : Structure and Evolution of the Stars (Princeton University Press, 1958), by M. Schwarzschild, and Physical Processes in Stellar Interiors (Israel Program for Scientific Translations, 1962), ... the years 1954-57 and there are only a few references of later date than Schwarzschild's book.

R. J. TAYLER

1964-12-05T23:59:59.000Z

Note: This page contains sample records for the topic "rainey star center" 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

Explosive Nucleosynthesis in Stars  

Science Journals Connector (OSTI)

... in hydrostatic equilibrium, with considerable effect on the abundances of the ejected matter. The overheating may result either from the fact that the fuels first ignite in a degenerate electron ... pressure wave propagates outward from an exploding core. In either case, large amounts of thermal energy are liberated in a time short compared with the star's ability to compensate ...

W. DAVID ARNETT; DONALD D. CLAYTON

1970-08-22T23:59:59.000Z

222

Young stars with discs  

Science Journals Connector (OSTI)

...central star. The ultraviolet excess was originally proposed to...in terms of modelling the UV excess as a contribution from a boundary...spectral features caused by lithium, calcium and iron. They report...hotspots with temperatures in excess of 5000 K, compared with the...

2000-01-01T23:59:59.000Z

223

LANSCE | Lujan Neutron Scattering Center  

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

Lujan Center Data Management Lujan Neutron Scattering Center Logo The Lujan Center within LANSCE utilizes a pulsed source and has a complement of 15 instruments. It maintains a...

224

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

225

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

226

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

227

Center for Energy Nanoscience at USC  

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

People Click HERE for the complete Center Directory. Center Leadership Center Advisory Board Members...

228

Energy Efficient Data Centers  

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

Energy Efficient Data Centers Energy Efficient Data Centers Title Energy Efficient Data Centers Publication Type Report LBNL Report Number LBNL-54163 Year of Publication 2004 Authors Tschudi, William F., Tengfang T. Xu, Dale A. Sartor, Jonathan G. Koomey, Bruce Nordman, and Osman Sezgen Call Number LBNL-54163 Abstract Data Center facilities, prevalent in many industries and institutions are essential to Californias economy. Energy intensive data centers are crucial to Californias industries, and many other institutions (such as universities) in the state, and they play an important role in the constantly evolving communications industry. To better understand the impact of the energy requirements and energy efficiency improvement potential in these facilities, the California Energy Commissions PIER Industrial Program initiated this project with two primary focus areas: First, to characterize current data center electricity use; and secondly, to develop a research roadmap defining and prioritizing possible future public interest research and deployment efforts that would improve energy efficiency.

229

DOE Information Center  

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

DOE Information Center DOE Information Center The U.S. Department of Energy (DOE) Information Center provides citizens a consolidated facility to obtain information and records related to the DOE's various programs in Oak Ridge and abroad. Employees at the DOE Information Center are available to assist with your requests and searches from 8:00 a.m. to 5:00 p.m. (EST), Monday through Friday, except for federal holidays. Requests Documents can be requested in person or by telephone, email, or fax. Reproduction Please allow DOE Information Center staff adequate time to reproduce documents. Some material requires special handling, security reviews, etc. Delivery Unless special arrangements have been made with DOE Information Center staff, documents should be picked up during normal business hours.

230

Harnessing the Energy of the Stars | Department of Energy  

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

Harnessing the Energy of the Stars Harnessing the Energy of the Stars Harnessing the Energy of the Stars September 12, 2011 - 5:52pm Addthis A view of a cryogenically cooled National Ignition Facility (NIF) target as "seen" by the laser through the hohlraum's laser entrance hole. | Photo courtesy of Lawrence Livermore National Laboratory. A view of a cryogenically cooled National Ignition Facility (NIF) target as "seen" by the laser through the hohlraum's laser entrance hole. | Photo courtesy of Lawrence Livermore National Laboratory. Former Under Secretary Koonin Former Under Secretary Koonin Director - NYU's Center for Urban Science & Progress and Former Under Secretary for Science These are exciting times for fusion energy. Today I'm sharing that excitement with several hundred scientists at a conference on Inertial

231

Harnessing the Energy of the Stars | Department of Energy  

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

Harnessing the Energy of the Stars Harnessing the Energy of the Stars Harnessing the Energy of the Stars September 12, 2011 - 5:52pm Addthis A view of a cryogenically cooled National Ignition Facility (NIF) target as "seen" by the laser through the hohlraum's laser entrance hole. | Photo courtesy of Lawrence Livermore National Laboratory. A view of a cryogenically cooled National Ignition Facility (NIF) target as "seen" by the laser through the hohlraum's laser entrance hole. | Photo courtesy of Lawrence Livermore National Laboratory. Former Under Secretary Koonin Former Under Secretary Koonin Director - NYU's Center for Urban Science & Progress and Former Under Secretary for Science These are exciting times for fusion energy. Today I'm sharing that excitement with several hundred scientists at a conference on Inertial

232

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

conduct business in Missouri. New propane commercial mowers are eligible for 15% of the cost of the equipment. Dedicated propane mower conversions are eligible for 750. New center...

233

Call center construction underway  

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

Government Services Group are making significant progress on getting the Valor Telecommunications call center ready for occupancy. After only two weeks on the job, "design and...

234

The Center for Nanoscale  

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

for Nanoscale Materials (CNM) at Argonne for interdisciplinary nanoscience and nanotechnology researchers can apply to use CNM for both nonproprietary The Center's goal is to...

235

NREL: Education Center - Programs  

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

the work of NREL. Monthly tours are also offered to give visitors an overview of our sustainable campus and featured buildings. Printable Version Education Center Home Hours,...

236

Project Overview: Successful Field-Scale in SITU Thermal NAPL Remediation  

SciTech Connect

The U.S. Department of Energy (DOE) successfully completed a field-scale remediation to remove non-aqueous phase liquids (NAPLs) from the subsurface at the Northeast Site on the Young-Rainey Science, Technology, and Research (STAR) Center, Largo, Florida. The Young-Rainey STAR Center is a former DOE facility that was previously known as the Pinellas Plant and the Pinellas STAR Center. The remediation project encompassed an area of 10,000 ft2 and depths extending to 35 ft below ground surface. Prior to the remediation, DOE evaluated technologies that had the potential to remove NAPLs from the subsurface at the site. Because of site conditions (clay lenses and an underlying clay layer that were thought to be contaminated), steam injection and electrical heating were considered to be the only technologies that had the potential to remove these NAPLs. In July 2001, DOEs contractor awarded a subcontract for removal of NAPLs from a portion of the Northeast Site. The technologies used for remediation were a combination of steam-enhanced extraction and Electro-Thermal Dynamic Stripping Process, an electrical resistive heating technology. Construction of the remediation system was completed in September 2002. Remedial operations began immediately after construction, and active heating ended in February 2003. After operations were completed, confirmatory sampling was conducted during a 6-month period to verify the level of cleanup achieved. Additional confirmatory sampling was conducted 18 months after operations ended. Analytical results of the confirmatory sampling showed that NAPL concentrations were reduced significantly below the required cleanup goals and, in most cases, below the regulatory maximum contaminant levels. Lessons learned relative to the design, construction, operation, confirmatory sampling approach, and subcontracting could benefit managers of similar remediation projects.

Butherus, Michael [S.M. Stoller Corporation; Ingle, David S. [S.M. Stoller Corporation; Juhlin, Randall [S.M. Stoller Corporation; Daniel, Joseph [S.M. Stoller Corporation; none,

2004-10-24T23:59:59.000Z

237

CENTER REPORT Center for Environmental Policy  

E-Print Network (OSTI)

such as phosphate ores and water. Certificate in Environmental Policy and Management The Center for Environmental Policy oversees the administrative aspects of the Certificate in Environmental Policy and Management in Environmental Policy and Management Eliana Bardi, Biological Scientist Matt Cohen, Post Doctoral Associate Clay

Slatton, Clint

238

Alternative Fuels Data Center: About the Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

About About Printable Version Share this resource Send a link to Alternative Fuels Data Center: About the Alternative Fuels Data Center to someone by E-mail Share Alternative Fuels Data Center: About the Alternative Fuels Data Center on Facebook Tweet about Alternative Fuels Data Center: About the Alternative Fuels Data Center on Twitter Bookmark Alternative Fuels Data Center: About the Alternative Fuels Data Center on Google Bookmark Alternative Fuels Data Center: About the Alternative Fuels Data Center on Delicious Rank Alternative Fuels Data Center: About the Alternative Fuels Data Center on Digg Find More places to share Alternative Fuels Data Center: About the Alternative Fuels Data Center on AddThis.com... More in this section... Project Assistance News & Features

239

Northwestern University Transportation Center  

E-Print Network (OSTI)

Northwestern University Transportation Center 2011 Business Advisory Committee NUTC #12;#12;I have the pleasure of presenting our Business Advisory Committee members--a distinguished group of transportation industry lead- ers who have partnered with the Transportation Center in advancing the state of knowledge

Bustamante, Fabián E.

240

University Center Breakfast Menu  

E-Print Network (OSTI)

Includes iced water and your choice of iced tea or lemonade Choice of two salads: Tossed Green, CaliforniaUniversity Center Breakfast Menu Buffets Includes coffee, decaf, hot tea service, iced water Center Deli Buffet Includes iced water and your choice of iced tea or lemonade Choice of two salads

Lee, Herbie

Note: This page contains sample records for the topic "rainey star center" 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

ENERGY CENTER OF WISCONSIN  

E-Print Network (OSTI)

ENERGY CENTER OF WISCONSIN Report Summary 210-1 Life-Cycle Energy Costs and Greenhouse Gas report energy center Net energy balance and greenhouse gas emissions from renewable energy storage systems June 2003 223-1 #12;ECW Report Number 223-1 Net energy balance and greenhouse gas emissions from

242

& Education CenterOregon  

E-Print Network (OSTI)

Center 3. Bike Hub 4. Electric Avenue 5. Montgomery Green Street GEOTHERMAL & DISTRICT ENERGY Parking Structure 3 Ho man Hall West Heating Plant Blackstone Montgomery Research Greenhouses Simon Benson EFFICIENT HEATING AND COOLING LOOP #12;Academic and Student Recreation Center (ASRC) SW 6TH AND SW

Caughman, John

243

INTERNATIONAL PACIFIC RESEARCH CENTER  

E-Print Network (OSTI)

INTERNATIONAL PACIFIC RESEARCH CENTER APRIL 2005­MARCH 2006 REPORT SCHOOL OF OCEAN AND EARTH Center 1 The Year's Highlights 3 Indo-Pacific Ocean Climate 4 Regional-Ocean Influences 10 Asian Ocean Climate: To understand climate variations in the Pacific and Indian oceans on interannual

Wang, Yuqing

244

International Pacific Research Center  

E-Print Network (OSTI)

International Pacific Research Center APRIL 2007­MARCH 2008 REPORT School of Ocean and Earth Center i Foreword ii iv Indo-Pacific Ocean Climate 1 Regional-Ocean Influences 13 Asian by the following broad research themes and goals of the IPRC Science Plan. Indo-Pacific Ocean Climate

Wang, Yuqing

245

INTERNATIONAL PACIFIC RESEARCH CENTER  

E-Print Network (OSTI)

INTERNATIONAL PACIFIC RESEARCH CENTER Annual Report April 2006 ­ March 2007 School of Ocean Research Center 1 2 The Year's Highlights 3 Research Accomplishments Indo-Pacific Ocean Climate 4 Regional-Ocean Ocean Climate: To understand climate variations in the Pacific and Indian oceans on inter- annual

Wang, Yuqing

246

Northwestern University Transportation Center  

E-Print Network (OSTI)

and challenges for our society. Energy and sustainability, economic growth and development, quality of life in the world to recognize transportation as an interdisciplinary field, the Transportation Center was founded, as the tradition lives on, and the Center continues to renew itself and engage faculty and students with new

MacIver, Malcolm A.

247

ENERGY STAR Webinar: Financing Energy Efficient Upgrades with ENERGY STAR  

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

Hosted by ENERGY STAR, this webinar will show how public sector organizations are improving energy efficiency with innovative solutions to financial barriers.

248

Detection of intergalactic red-giant-branch stars in the Virgo cluster  

E-Print Network (OSTI)

It has been suspected for nearly 50 years that clusters of galaxies contain a population of intergalactic stars, ripped from galaxies during cluster formation or when the galaxies' orbits take them through the cluster center. Support for the existence of such a population of free-floating stars comes from measurements of the diffuse light in clusters, and from recent detections of planetary nebulae with positions and/or velocities far removed from any observed cluster galaxy. But estimates for the mass of the diffuse population and its distribution relative to the galaxies are still highly uncertain. Here we report the direct detection of intergalactic stars in deep images of a blank field in the Virgo Cluster. The data suggest that approximately 10% of the stellar mass of the cluster is in intergalactic stars. We observe a relatively homogeneous distribution of stars, with evidence of a slight gradient toward M87.

Henry C. Ferguson; Nial R. Tanvir; Ted von Hippel

1998-01-23T23:59:59.000Z

249

Energy Efficient Data Centers  

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

Federal Utility Partnership Working Group Federal Utility Partnership Working Group Will Lintner November 20, 2008 Williamsburg, VA 2 Why Data Centers? * Data centers are highly energy intensive and growing at a rapid rate - Consume 10 to 100 times more energy per square foot than typical office building * Data centers consumed about 45 billion kWh in 2005 and 61 billion kWh in 2006 - This accounts for nearly 1.2% and 1.5% of all U.S. electricity respectively * At current rate, power requirements for data centers could double in 5 years 3 Typical Data Center Energy Use Server Load /Computing Operations Cooling Equipment Power Conversions & Distribution 100 Units 33 Units Delivered 35 Units 4 4 Server Load/ Computing Operations Cooling Equipment Power Conversion & Distribution Alternative Power Generation * High voltage distribution

250

LANL: Superconductivity Technology Center  

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

Sitemap | Lab Home | Phone Sitemap | Lab Home | Phone ABOUT LANL ContactsPhonebookPolicy CenterOrganizationMapsJobs Emergency NEWS LIBRARY JOBS Search Materials Physics & Applications: STC STC Home OUR FOCUS HTS Physics HTS Materials Development HTS Materials Processing Power Applications Electronic Materials FUTURE APPLICATIONS Biomedical Developments Magnetic Levitation Train MHD Ship CONTACTS Center Leader Ken Marken Program Administrator Brenda Espinoza Center Office Location: TA-03, Bdg. 0032, Rm. 141 Exploring technology at STC Superconductivity Technology Center (STC) The Superconductivity Technology Center (STC) coordinates a multidisciplinary program for research, development, and technology transfer in the area of high-temperature superconductivity. Our focus is on effective collaborations with American industry, universities, and other national laboratories to develop electric power and electronic device applications of high-temperature superconductors (HTS).

251

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

252

Crazy heart: kinematics of the "star pile" in Abell 545  

E-Print Network (OSTI)

We study the structure and internal kinematics of the "star pile" in Abell 545 - a low surface brightness structure lying in the center of the cluster.We have obtained deep long-slit spectroscopy of the star pile using VLT/FORS2 and Gemini/GMOS, which is analyzed in conjunction with deep multiband CFHT/MEGACAM imaging. As presented in a previous study the star pile has a flat luminosity profile and its color is consistent with the outer parts of elliptical galaxies. Its velocity map is irregular, with parts being seemingly associated with an embedded nucleus, and others which have significant velocity offsets to the cluster systemic velocity with no clear kinematical connection to any of the surrounding galaxies. This would make the star pile a dynamically defined stellar intra-cluster component. The complicated pattern in velocity and velocity dispersions casts doubts on the adequacy of using the whole star pile as a dynamical test for the innermost dark matter profile of the cluster. This status is fulfille...

Salinas, Ricardo; West, Michael J; Romanowsky, Aaron J; Lloyd-Davies, Ed; Schuberth, Ylva

2011-01-01T23:59:59.000Z

253

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

254

Anisotropic charged dark energy star  

E-Print Network (OSTI)

As the stars carry electrical charges, we present in this paper a model for charged dark energy star which is singularity free. We take Krori-Barua space time. We assume that the radial pressure exerted on the system due to the presence of dark energy is proportional to the isotropic perfect fluid matter density and the difference between tangential and radial pressure is proportional to the square of the electric field intensity. The solution satisfies the physical conditions inside the star

Kanika Das; Nawsad Ali

2014-02-02T23:59:59.000Z

255

Creating a Star on Earth  

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

At the Energy Department's Princeton Plasma Physics Lab, scientists are trying to accomplish what was once considered the realm of science fiction: creating a star on Earth.

256

Harmonizing Global Metrics for Data Center Energy Efficiency, February 2,  

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

Harmonizing Global Metrics for Data Center Energy Efficiency, Harmonizing Global Metrics for Data Center Energy Efficiency, February 2, 2010 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

257

Upsilon measurement in STAR  

E-Print Network (OSTI)

We present preliminary results of Upsilon production in p+p collisions at sqrt(s)=200 GeV at central rapidity. This measurement was performed at the STAR experiment through the Upsilon->e^+e^- decay channel. In this manuscript we describe the experimental details, from the development of a specially designed trigger setup to the analysis methods used to discriminate electrons from hadrons. The production cross-section obtained B*{(dsigma/dy)|(y=0)}=91(28)(22) pb is compatible with our expectations based on pQCD calculations.

Mauro R. Cosentino

2007-06-06T23:59:59.000Z

258

On Magnetized Neutron Stars  

E-Print Network (OSTI)

In this work we review the formalism normally used in the literature about the effects of density-dependent magnetic fields on the properties of neutron stars, expose some ambiguities that arise and propose a way to solve the related problem. Our approach uses a different prescription for the calculation of the pressure based on the chaotic field formalism for the stress tensor and also a different way of introducing a variable magnetic field, which depends on the energy density rather than on the baryonic density.

Lopes, Luiz L

2014-01-01T23:59:59.000Z

259

Star Canticle Issue 2  

E-Print Network (OSTI)

StA ft CANtJClt 2 * 1 1 STAR CANTICLE 2 DOTTY BARRY PRICE: P.O. BOX 921 $5.50 1st class CLAREMONT, CA 91711 4.50 book rate CON TEN TS 2 Prelude 3 Poetry ?Untitled Dotty Barry k Fiction ?"Scotty? s Decision" Joy Mancinelli 6.... .Poetry..." Rayelle Roe m Poetry ?"Shouldn't You Ask Me First?" .Susan Meek k>2 Poetry ?"Storm Haven" Ellen Kobrin ^3 Poetry ?"Fire and Ice" ? ? .Gerry Downes kk Fiction ?"Viewpoint" Kay McElvain ty Poetry ?"Threads" Susan Burr 48 Poetry ?"The Starless Sky" Liz...

Multiple Contributors

1979-01-01T23:59:59.000Z

260

Teacher Resource Center  

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

Teacher Resource Center: Putting It All Together Teacher Resource Center: Putting It All Together TRC Home TRC Fact Sheet Library Curricular Resources Science Fair Resources Bibliographies sciencelines The Best of sciencelines Archives Annotated List of URLs Catalog Teacher's Lounge Full Workshop Catalog Customized Workshops Scheduled Workshops Special Opportunities Teacher Networks Science Lab Fermilab Science Materials Samplers Order Form Science Safety Issues Tech Room Fermilab Web Resources The Teacher Resource Center provides a preview collection of K-12 instructional materials. TRC services include professional development workshops, consultation assistance, bibliographies and reference assistance. Educators have access to curriculum materials, books, multimedia, educational supply catalogs, periodicals and newsletters. The collection

Note: This page contains sample records for the topic "rainey star center" 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

Cost Update, STAR-TOFp Implementation STAR-TOFp Group  

E-Print Network (OSTI)

Cost Update, STAR-TOFp Implementation STAR-TOFp Group November 22, 1999 Abstract This document updates the cost sections of the TOFp Implementation Plan. In this update1 to the TOFp Implementation plan of Oct. 5, 1999,2 the cost estimates based on the latest quotes and the nal design are discussed

Llope, William J.

262

Data Center Optimization Plan Federal Data Center Consolidation Initiative  

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

Data Center Optimization Plan Data Center Optimization Plan Federal Data Center Consolidation Initiative Public Release 9.30.11 U.S. Department of Energy | Office of the Chief Information Officer 2 Federal Data Center Consolidation Initiative Department of Energy Data Center Optimization Plan Public Release - 09.30.11 1. Introduction ..................................................................................................................................... 3 2. Agency Goals for Data Center Optimization .................................................................................... 5 3. Implementing Shared Services/Multi-tenancy ................................................................................. 5 4. Agency Approach, Rationale and Timeline ...................................................................................... 6

263

Neutron Science Center  

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

to have rare opportunity to tour Neutron Science Center May 10, 2011 LANL Rosenfest will celebrate life of LANSCE founder Louis Rosen and offer tour LOS ALAMOS, New Mexico, May 10,...

264

Energy efficient data centers  

E-Print Network (OSTI)

Center 6.2 utilized fan coil units, rather than computerEfficiency kW/ton Fan Coil Unit Design Efficiency CFM/kWCenter 6.2 utilized fan coil units, rather than computer

Tschudi, William; Xu, Tengfang; Sartor, Dale; Koomey, Jon; Nordman, Bruce; Sezgen, Osman

2004-01-01T23:59:59.000Z

265

ELIAS Towe, Center Director  

E-Print Network (OSTI)

the generation of hydrogen as a fuel for fuel cells, novel fuel cell technologies, and spectrally broadband photovoltaic cells for solar energy conversion. The secondary focus of the Center is on nano

Goldstein, Seth Copen

266

Data Center Power Consumption  

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

Center Power Consumption Center Power Consumption A new look at a growing problem Fact - Data center power density up 10x in the last 10 years 2.1 kW/rack (1992); 14 kW/rack (2007) Racks are not fully populated due to power/cooling constraints Fact - Increasing processor power Moore's law Fact - Energy cost going up 3 yr. energy cost equivalent to acquisition cost Fact - Iterative power life cycle Takes as much energy to cool computers as it takes to power them. Fact - Over-provisioning Most data centers are over-provisioned with cooling and still have hot spots November 2007 SubZero Engineering An Industry at the Crossroads Conflict between scaling IT demands and energy efficiency Server Efficiency is improving year after year Performance/Watt doubles every 2 years Power Density is Going Up

267

Stars and gas in the Medusa merger  

E-Print Network (OSTI)

The Medusa (NGC 4194) is a well-studied nearby galaxy with the disturbed appearance of a merger and evidence for ongoing star formation. In order to test whether it could be the result of an interaction between a gas-rich disk-like galaxy and a larger elliptical, we have carried out optical and radio observations of the stars and the gas in the Medusa, and performed $N$-body numerical simulations of the evolution of such a system. We used the Nordic Optical Telescope to obtain a deep V-band image and the Westerbork Radio Synthesis Telescope to map the large-scale distribution and kinematics of atomic hydrogen. A single HI tail was found to the South of the Medusa with a projected length of 56 kpc (5') and a gas mass of 7* 10^8 M_sun, thus harbouring about one third of the total HI mass of the system. HI was also detected in absorption toward the continuum in the center. HI was detected in a small nearby galaxy to the North-West of the Medusa at a projected distance of 91 kpc. It is, however, unlikely that this galaxy has had a significant influence on the evolution of the Medusa. The simulations of the slightly prograde infall of a gas-rich disk galaxy on an larger, four time more massive elliptical (spherical) galaxy reproduce most of the observed features of the Medusa.Thus, the Medusa is an ideal object to study the merger-induced star formation contribution from the small galaxy of a minor merger.

E. Manthey; S. Huettemeister; S. Aalto; C. Horellou; P. Bjerkeli

2008-08-28T23:59:59.000Z

268

Women's Center INTERNAL COORDINATOR OREGON STATE UNIVERSITY PRIDE CENTER  

E-Print Network (OSTI)

at the Center for two or less years, in order to infuse the center with new ideas, energy and perspectives. 4

Escher, Christine

269

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

270

Wind from T Tauri Stars  

Science Journals Connector (OSTI)

......December 1998 research-article Papers 8680 Wind from T Tauri Stars Masayoshi Kiguchi Shinji...was shown by DeCampli that an isothermal wind of T Tauri stars cannot explain both the...Since the assumption of an isothermal wind does not hold in general, we recalculated......

Masayoshi Kiguchi; Shinji Narita; Chushiro Hayashi

1998-12-01T23:59:59.000Z

271

Verifying the ENERGY STAR Certification Application  

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

Do you verify commercial building applications for ENERGY STAR certification? This webinar, based on the ENERGY STAR Guide for Licensed Professionals, covers the role of the licensed professional,...

272

Christmas burst reveals neutron star collision  

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

Christmas burst reveals neutron star collision Christmas burst reveals neutron star collision Called the Christmas Burst, GRB 101225A was freakishly lengthy and it produced...

273

University of Connecticut Health Center  

E-Print Network (OSTI)

University of Connecticut Health Center UCONN Medical Group Comprehensive Spine Center (Patient: ____________________ AGE: _____ SEX: M / F Referring Physician: ___________ Primary Care Physician: _____________ 1. Where your symptoms begin? __/__/__/ *HCH2199* #12;University of Connecticut Health Center UCONN Medical

Oliver, Douglas L.

274

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:

275

PNNL: News Center - Currents Newsletter  

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

help scientists design energy storage solutions and mitigate climate change. Read more. News Center News Center Home News Releases Social Media Directory PNNL Leadership Our...

276

Karen Nunez, Procedures Center Manager  

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

Karen Nunez, Procedures Center Manager Print Procedures Center Manager Karen Nunez has been working somewhat "behind the scenes" at the ALS for the past seven years, ensuring that...

277

Information Center | Department of Energy  

Office of Environmental Management (EM)

Center Information Center The U.S. Department of Energy's (DOE) Office of Enterprise Assessments (EA) provides expert evaluations of management performance in safety, security and...

278

NREL: Education Center Home Page  

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

Photo of the NREL Education Center. Clean Energy Innovation Programs for Student and Community Groups NREL's Education Center offers a variety of program topics and experiences for...

279

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

280

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

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


281

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

282

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

283

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

284

The evolution of star clusters: The resolved-star approach  

E-Print Network (OSTI)

We present the first results of a new technique to detect, locate, and characterize young dissolving star clusters. Using HST/ACS archival images of the nearby galaxy IC2574, we performed stellar PSF photometry and selected the most massive stars as our first test sample. We used a group-finding algorithm on the selected massive stars to find cluster candidates. We then plot the color-magnitude diagrams for each group, and use stellar evolutionary models to estimate their age. So far, we found 79 groups with ages of up to about 100 Myr, displaying various sizes and densities.

Anne Pellerin; Martin J. Meyer; Jason Harris; Daniela Calzetti

2008-02-29T23:59:59.000Z

285

The Brightest AGB Stars in the Inner Bulge of M31  

E-Print Network (OSTI)

JHK images with angular resolutions approaching the diffraction limit of the 3.6 meter Canada-France-Hawaii Telescope are used to investigate the bright AGB content of the M31 bulge. The AGB-tip in a field 2.6 arcmin from the galaxy center occurs at K = 15.6, which is significantly fainter than measured in previous ground-based studies that sampled similar projected distances from the center of M31. Within 2.6 arcmin of the center of M31 the number density of bright AGB stars scales with r-band surface brightness, and the K brightness of the AGB-tip does not vary measureably with radius. It is concluded that the infrared bright AGB stars (1) belong to the bulge, and not the disk, and (2) are well mixed throughout the inner bulge, suggesting that they formed at a time when the overall structural properties of the M31 bulge were imprinted. The bolometric luminosity functions of the M31 bulge and Baade's Window are in excellent agreement, while the brightest AGB stars in the M31 bulge, the Galactic bulge, and M32 have similar M_K. These data suggest that the brightest stars in M32 and the bulges of M31 and the Milky-Way belong to an old, metal-rich population; these stars are bright not because they have a young or intermediate age, but because they have a high metallicity.

T. J. Davidge

2001-06-23T23:59:59.000Z

286

Conference Center Lecture Hall  

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

401 Library Take the elevators downstairs to the Gallery. 401 Library Take the elevators downstairs to the Gallery. Conference Center Lecture Hall The Lecture Hall is a fully-equipped site for meetings of up to 540 people. This total includes: 237 seats on the Lecture Hall main level; 161 seats in the Lecture Hall balcony; and 142 seats in the two flexible rooms under the balcony (with interior walls removed). These rooms can also be used for meetings, both individually (32 classroom-style seats) or together (72 classroom-style seats). An additional 80 people can be seated in the nearby seminar room (A1100). Photo of the Conference Center's Lecture Hall Conference Center Gallery Seminar Room (A1101) The Seminar Room is located just off the Atrium. Conference Center Lecture Hall Atrium The Conference Center Atrium provides an open, elegant space ideal for registration, informational displays, and social hours. Computers are located just off the Atruim for e-mail access.

287

ARM - News Center  

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

Center Center Media Contact Lynne Roeder lynne-dot-roeder-at-pnnl-dot-gov @armnewsteam Field Notes Blog Topics Field Notes89 AGU 3 AMIE 10 ARM Aerial Facility 2 ARM Mobile Facility 1 6 ARM Mobile Facility 2 47 BAECC 1 BBOP 4 MAGIC 12 MC3E 17 SGP 2 STORMVEX 29 TCAP 3 Search News Search Blog News Center All Categories What's this? Social Media Guidance News Center All Categories Features and Releases Facility News Field Notes Blog feed Events feed Employment Research Highlights Data Announcements Education News Archive What's this? Social Media Guidance News Center Forecast Calls for Better Models: Examining the Core Components of Arctic Clouds to Clear Their Influence on Climate Jan 07, 2014 [ Research Highlights ] Predicting how atmospheric aerosols influence cloud formation and the resulting feedback to climate is a challenge that limits the accuracy of atmospheric models. This is especially true in the Arctic, where mixed-phase (both ice- and liquid-based) clouds are frequently observed, but the processes that determine their composition are poorly understood. To obtain a closer look [...]

288

National Training Center | Department of Energy  

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

Organizational Chart National Training Center National Training Center MISSION The National Training Center (NTC), the Department's Center of Excellence for Security and Safety...

289

Laboratory Computing Resource Center  

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

Computing DOE Logo Computing DOE Logo Search BIO ... Search Argonne Home > BIO home > Laboratory Computing Resource Center BIO Home Page About BIO News Releases Research Publications People Contact Us Organization Chart Site Index Inside BIO BIO Safety About Argonne Argonne National Laboratory Logo Laboratory Computing Resource Center In 2002 Argonne National Laboratory established the Laboratory Computing Project to enable and promote the use of high-performance computing (HPC) across the Laboratory in support of its varied research missions. The Laboratory Computing Resource Center (LCRC) was established, and in April 2003 LCRC began full operations with Argonne’s first teraflops computing cluster, Jazz. In 2010 Jazz was replaced by Fusion, with a peak performance of 30 teraflops (and still growing). We just acquired Blues which will a performance of 100 teraflops.

290

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Carolina Incentives and Laws Carolina Incentives and Laws The following is a list of expired, repealed, and archived incentives, laws, regulations, funding opportunities, or other initiatives related to alternative fuels and vehicles, advanced technologies, or air quality. Biofuels Commercialization Grants Archived: 10/01/2013 The Biofuels Center of North Carolina (Center) is a private, nonprofit corporation the Legislature funds to implement the goal that by 2017, 10% of liquid fuels sold in North Carolina will come from biofuels grown and produced within the state. The Center awards funds to academic institutions, economic development organizations, nonprofit corporations, and other entities through an annual competitive awards process. Grants and contracts are designed to identify and bridge gaps in knowledge and

291

ENERGY STAR Webinar: Financing Energy Efficient Upgrades with ENERGY STAR  

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

ENERGY STAR is hosting a webinar on how public sector organizations are improving energy efficiency with innovative solutions to financial barriers on Oct. 21, 2014, from 2:00 p.m. - 3:15 p.m.

292

EPA ENERGY STAR Webinar: ENERGY STAR Portfolio Manager 201  

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

Continue to learn about EPAs ENERGY STAR Portfolio Manager tool, with a deeper dive into more advanced functionalities such as: managing and tracking changes to your property uses over time; using...

293

EPA ENERGY STAR Webcast: Value of ENERGY STAR Certification  

Office of Energy Efficiency and Renewable Energy (EERE)

For thousands of organizations, ENERGY STAR is the simple choice for saving money and demonstrating environmental leadership to the public. Lower energy costs aren't the only financial benefit of...

294

Microsoft Word - 11-0632 Better Business Forms Data Report.doc  

Office of Legacy Management (LM)

Control Number 11-0632 May 13, 2011 U.S. Department of Energy Office of Legacy Management ATTN: Scott Surovchak Pinellas Site Manager 11025 Dover Street, Suite 1000 Westminster, CO 80021 SUBJECT: Contract No. DE-AM01-07LM00060, S.M. Stoller Corporation (Stoller) Better Business Forms Data Report REFERENCE: Task Order LM00-502-06-509, Pinellas, FL, Site Dear Mr. Surovchak: This letter reports the results of the final off-site plume delineation event on property owned by Better Business Forms at 10950 Belcher Road in April 2011. The purpose of this sampling event was to complete delineation of the contaminant plume that extends from the Building 100 Area on the Young - Rainey STAR Center south across Bryan Dairy Road onto private property. The

295

Microsoft Word - DOE_RM_DM-#100066-v1-Sitewide_Quarterly_Oct-Dec_2004.DOC  

Office of Legacy Management (LM)

through December 2004 through December 2004 January 2005 Office of Legacy Management DOE M/GJ 2005 - -L 799 U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management DOE-LM/GJ799-2005 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center October through December 2004 January 2005 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Quarterly Progress Report for October through December 2004

296

Microsoft Word - sitewide dec-may07.doc  

Office of Legacy Management (LM)

December 2006 through May 2007 December 2006 through May 2007 June 2007 Office of Legacy Management DOE M/1492 2007 - -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy DOE-LM/1492-2007 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2006 through May 2007 June 2007 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Semiannual Progress Report for December 2006 through May 2007

297

Program or Field Office: Office of Legacy Management Project Title and I.D. No.: Bioremediation Injection and Related Activities at the Pinellas Site, Largo, Florida,  

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

Bioremediation Injection and Related Activities at the Pinellas Site, Largo, Florida, Bioremediation Injection and Related Activities at the Pinellas Site, Largo, Florida, LM 13-13 Location: Largo, Florida Proposed Action or Project Description: DOE proposes to use a Geoprobe to inject emulsified edible soybean oil (EEO) and anaerobic microbial solution into the surficial aquifer at the 4.5 Acre Site adjacent to the DOE Young - Rainey STAR Center (Pinellas Site) in Largo, Florida. The proposed action would enhance naturally occurring anaerobic biodegradation, thereby reducing vinyl chloride contamination along the southwest boundary of the 4.5 Acre Site. Dehalococcoides ethenogenes (DHE) is a type of microbe that occurs naturally in the aquifer. Bioaugmentation with a commercially available DHE culture used in conjunction with the EEO would maximize the efficiency of contaminant biodegradation. No genetically engineered or

298

Microsoft Word - N01179_Sitewide semiannual Dec-May08  

Office of Legacy Management (LM)

December 2007 through May 2008 December 2007 through May 2008 June 2008 Office of Legacy Management LMS/PIN/N01179 Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AM01-07LM00060 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy LMS/PIN/N01179 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center December 2007 Through May 2008 June 2008 U.S. Department of Energy Sitewide Semiannual Progress Report for December 2007 through May 2008 June 2008 Doc. No. N0117900 Page ii Contents Acronyms and Abbreviations ........................................................................................................

299

Northeast Site Area A NAPL Remediation Final Report.doc  

Office of Legacy Management (LM)

82-TAC 82-TAC U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy DE-AC13-02GJ79491 Approved for public release; distribution is unlimited. Pinellas Environmental Restoration Project Northeast Site Area A NAPL Remediation Final Report September 2003 N0065200 GJO- 2003- 482- TAC GJO- PIN 13.12.10 Pinellas Environmental Restoration Project Northeast Site Area A NAPL Remediation Final Report Young - Rainey STAR Center September 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13- 02GJ79491 Document Number N0065200 Contents DOE/Grand Junction Office Northeast Site Area A NAPL Remediation Final Report September 2003 Page iii

300

Microsoft Word - DOE_RM_DM-#101996-v1-Sitewide_jan_-_march_2005.DOC  

Office of Legacy Management (LM)

January through March 2005 January through March 2005 April 2005 Office of Legacy Management DOE M/GJ874 2005 - -L U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management DOE-LM/GJ874-2005 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center January through March 2005 April 2005 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Quarterly Progress Report for January through March 2005

Note: This page contains sample records for the topic "rainey star center" 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

Microsoft Word - DOE_RM_DM-#103356-v1-4_5_Acre_Quarterly_Apr-June_2005.DOC  

Office of Legacy Management (LM)

April Through June 2005 April Through June 2005 July 2005 Office of Legacy Management DOE M/GJ925 2005 - -L U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management DOE-LM/GJ925-2005 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center April through June 2005 July 2005 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Quarterly Progress Report for April through June 2005

302

Microsoft Word - 4_5 acrejune-nov07.doc  

Office of Legacy Management (LM)

2007 Through November 2007 2007 Through November 2007 December 2007 Office of Legacy Management DOE M/1563 2007 - -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy DOE-LM/1563-2007 Pinellas Environmental Restoration Project Semiannual Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site June 2007 Through November 2007 December 2007 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy 4.5 Acre Site Semiannual Progress Report for June 2007 through November 2007

303

Microsoft Word - DOE_RM_DM-#343505-v1-Sitewide_July_September_2005.DOC  

Office of Legacy Management (LM)

July Through September 2005 July Through September 2005 October 2005 Office of Legacy Management DOE M/GJ1009 2005 - -L U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management DOE-LM/GJ1009-2005 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center July through September 2005 October 2005 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Quarterly Progress Report for July through September 2005

304

Microsoft Word - PINReuseAward20030926.doc  

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

Friday, September 26, 2003 Friday, September 26, 2003 Department of Energy Awards $2 Million to the Pinellas Plant Community Reuse Organization WASHINGTON, DC - The Department of Energy (DOE) announced today that it will award $2 million to the Pinellas Plant Community Reuse Organization (CRO) located at the department's former Pinellas Plant near Tampa, Florida. "The department is proud to support the efforts of the Pinellas Plant Community Reuse Organization and the Young - Rainey STAR Center in bringing additional jobs to the department's former plant," Secretary of Energy Spencer Abraham said. "We will continue to work with the Pinellas Plant Community Reuse Organization and other community reuse organizations around the country to retain, expand or create jobs for workers affected by

305

Microsoft Word - PinellasPlantComReuseOrg20041021.doc  

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

202/586-5806 202/586-5806 Thursday, October 21, 2004 $1.5 Million Grant Presented to Pinellas Plant Community Reuse Organization LARGO, FL, WASHINGTON, DC - Secretary of Energy Spencer Abraham and House Appropriations Chairman Bill Young today announced an award of a $1.5 million Department of Energy grant to the Pinellas Plant Community Reuse Organization (CRO) for infrastructure upgrades and to assist in the economic development of a high-tech incubator at the Young - Rainey STAR Center in Pinellas County, Florida. "Because of Chairman Young's efforts and the efforts of this active, innovative Community Reuse Organization, more people are employed at this facility today then when it was a DOE facility in the 1990s. That's good for Largo and America," said Secretary Abraham. "Today's

306

Microsoft Word - DOE_RM_DM-#359194-v1-Sitewide_report_June-Nov_2006.DOC  

Office of Legacy Management (LM)

through November 2006 through November 2006 December 2006 Office of Legacy Management DOE M/1397 2006 - -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy DOE-LM/1397-2006 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center June through November 2006 December 2006 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Semiannual Progress Report for June through November 2006

307

Microsoft Word - DOE_RM_DM-#348497-v1-Sitewide_Semiannual_Report_January-Maƒ  

Office of Legacy Management (LM)

January through May 2006 January through May 2006 June 2006 Office of Legacy Management DOE M/GJ1229-2006 -L Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy DOE-LM/GJ1229-2006 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Semiannual Progress Report for the Young - Rainey STAR Center January through May 2006 June 2006 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Semiannual Progress Report for January through May 2006

308

Microsoft Word - DOE_RM_DM-#345149-v1-Sitewide_Oct_Dec_2005.DOC  

Office of Legacy Management (LM)

Through December 2005 Through December 2005 January 2006 Office of Legacy Management DOE M/GJ1103 2006 - -L U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AC01-02GJ79491 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management DOE-LM/GJ1103-2006 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center October through December 2005 January 2006 Work Performed by S.M. Stoller Corporation under DOE Contract No. DE-AC01-02GJ79491 for the U.S. Department of Energy Office of Legacy Management, Grand Junction, Colorado U.S. Department of Energy Sitewide Quarterly Progress Report for October through December 2005

309

Page not found | Department of Energy  

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

81 - 1090 of 28,560 results. 81 - 1090 of 28,560 results. Download Steam and ET-DSP Combined for DNAPL Remediation: Full-Scale Site Restoration at Young- Rainey STAR Center Proceedings of the Fourth International Conference on Remediation of Chlorinated and Recalcitrant Compounds.May 2004, Monterey, California.Gorm Heron, Steven Carroll, Hank Sowers, Bruce McGee,... http://energy.gov/lm/downloads/steam-and-et-dsp-combined-dnapl-remediation-full-scale-site Download Independent Activity Report, Los Alamos Site Office- April 2012 Los Alamos Site Office Nuclear Maintenance Management Program Oversight Self-Assessment [HIAR-LANL-2011-11-18] http://energy.gov/hss/downloads/independent-activity-report-los-alamos-site-office-april-2012 Download 2011 Annual Planning Summary for Argonne Site Office (Argonne)

310

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

311

Impact of Continuous Commissioning on the Energy Star Rating of Hospitals and Office Buildings  

E-Print Network (OSTI)

source EUI of an office type facility ............................................................................................ 23 Table 4: Linear regression equation for calculating the predicted source EUI of a hospital type facility... of Building Centered Variables................................................ 61 Table 10: Calculation of predicted source EUI ................................................................ 62 Table 11: Lookup table for Energy Star? Rating given...

Kulkarni, Aditya Arun

2012-02-14T23:59:59.000Z

312

PAHs and crystalline silicates in the bipolar post-AGB star IRAS 16279-4757 12  

E-Print Network (OSTI)

understood. A possibility, but implausible, is that these stars all evolved from oxygen-rich to carbon with PAHs and crystalline silicates. A two-component model and images suggest a dense oxygen-rich torus at the outflow, while the continuum emission is concentrat- ed towards the center. Our findings support

Zijlstra, Albert

313

FPL's solar stars shine at new 500-acre array By SUSAN SALISBURY  

E-Print Network (OSTI)

FPL's solar stars shine at new 500-acre array By SUSAN SALISBURY Palm Beach Post Staff Writer and water, Florida Power & Light Co. workers finished cleaning the mirrors at its new Martin County solar's dedication of the one-of-a-kind hybrid solar energy center, it's nice that the 5-by-5-foot mirrors

Belogay, Eugene A.

314

A Heavy Flavor Tracker for STAR  

SciTech Connect

We propose to construct a Heavy Flavor Tracker (HFT) for the STAR experiment at RHIC. The HFT will bring new physics capabilities to STAR and it will significantly enhance the physics capabilities of the STAR detector at central rapidities. The HFT will ensure that STAR will be able to take heavy flavor data at all luminosities attainable throughout the proposed RHIC II era.

Xu, Z.; Chen, Y.; Kleinfelder, S.; Koohi, A.; Li, S.; Huang, H.; Tai, A.; Kushpil, V.; Sumbera, M.; Colledani, C.; Dulinski, W.; Himmi,A.; Hu, C.; Shabetai, A.; Szelezniak, M.; Valin, I.; Winter, M.; Surrow,B.; Van Nieuwenhuizen, G.; Bieser, F.; Gareus, R.; Greiner, L.; Lesser,F.; Matis, H.S.; Oldenburg, M.; Ritter, H.G.; Pierpoint, L.; Retiere, F.; Rose, A.; Schweda, K.; Sichtermann, E.; Thomas, J.H.; Wieman, H.; Yamamoto, E.; Kotov, I.

2005-03-14T23:59:59.000Z

315

X-ray Emission from Massive Stars  

E-Print Network (OSTI)

X-ray Emission from Massive Stars David Cohen Department of Physics and Astronomy Swarthmore be related to the production of X-rays on massive stars. If so, massive stars' X-rays are much different than those found our own Sun and other cooler stars like the Sun that produce X-rays via magnetic activity

Cohen, David

316

Energy Frontier Research Centers | ORNL  

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

Materials Synthesis from Atoms to Systems Materials Synthesis from Atoms to Systems Materials Characterization Materials Theory and Simulation Energy Frontier Research Centers Center for Defect Physics in Structural Materials Fluid Interface Reactions, Structure and Transport Advanced Materials Home | Science & Discovery | Advanced Materials | Research Areas | Energy Frontier Research Centers SHARE Energy Frontier Research Centers Advanced Materials research at ORNL is home to two Department of Energy-Office of Basic Energy Sciences' Energy Frontier Research Centers, the Fluid Interface Reaction, Structure, and Transport Center (FIRST), which focuses on understanding interfacial processes critical to electrical energy storage and catalysis, and the Center for Defect Physics, (CDP)

317

Alternative Fuels Data Center: Publications  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Publications Publications Printable Version Share this resource Send a link to Alternative Fuels Data Center: Publications to someone by E-mail Share Alternative Fuels Data Center: Publications on Facebook Tweet about Alternative Fuels Data Center: Publications on Twitter Bookmark Alternative Fuels Data Center: Publications on Google Bookmark Alternative Fuels Data Center: Publications on Delicious Rank Alternative Fuels Data Center: Publications on Digg Find More places to share Alternative Fuels Data Center: Publications on AddThis.com... Publications Find publications about alternative transportation, including alternative fuels, advanced vehicles, and regulated fleets. Keyword Category Search more search options close × Filter by Document Category Books & Chapters Brochures & Fact Sheets Conference Papers & Proceedings

318

Alternative Fuels Data Center: Newsletters  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Publications » Newsletters Publications » Newsletters Printable Version Share this resource Send a link to Alternative Fuels Data Center: Newsletters to someone by E-mail Share Alternative Fuels Data Center: Newsletters on Facebook Tweet about Alternative Fuels Data Center: Newsletters on Twitter Bookmark Alternative Fuels Data Center: Newsletters on Google Bookmark Alternative Fuels Data Center: Newsletters on Delicious Rank Alternative Fuels Data Center: Newsletters on Digg Find More places to share Alternative Fuels Data Center: Newsletters on AddThis.com... Newsletters Read these government and industry newsletters to stay current with developments in alternative transportation technologies, including alternative fuels, advanced vehicles, and regulated fleets. Government Newsletters

319

Alternative Fuels Data Center: Publications  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Publications Publications Printable Version Share this resource Send a link to Alternative Fuels Data Center: Publications to someone by E-mail Share Alternative Fuels Data Center: Publications on Facebook Tweet about Alternative Fuels Data Center: Publications on Twitter Bookmark Alternative Fuels Data Center: Publications on Google Bookmark Alternative Fuels Data Center: Publications on Delicious Rank Alternative Fuels Data Center: Publications on Digg Find More places to share Alternative Fuels Data Center: Publications on AddThis.com... Publications Find publications about alternative transportation, including alternative fuels, advanced vehicles, and regulated fleets. Keyword Category alternative fuel price report Search more search options close × Filter by Document Category

320

Energy Efficient Data Centers  

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

Federal Utility Partnership Working Group Will Lintner November 28, 2007 San Diego, CA Why Data Centers? * Data centers are highly energy intensive and growing at a rapid rate - Consume 10 to 100 times more energy per square foot than typical office building * Data centers consumed about 45 billion kWh in 2005 and 61 billion kWh in 2006 - This accounts for nearly 1.2% and 1.5% of all U.S. electricity respectively * At current rate, power requirements for data centers could double in 5 years 2 Opportunity Potential Comparison of Projected Electricity Use - All Scenarios 2007 to 2011 140 2006 Baseline 58.7 Annual Energy Use (Billion kWh/year) 120 100 80 60 40 20 B u s i n e s s a s u s u a l C u r r e n t t r e n d s I m p r o v e d o p e r a t i o n a l m a n a g e m e n t Best practice S ta te o f th e a rt 0 2007 2008 2009 2010 2011

Note: This page contains sample records for the topic "rainey star center" 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

Arkansas Water Resources Center  

E-Print Network (OSTI)

Keywords --Algal Assay/Nutrients/Heavy Metals/Toxicity #12;TABLE OF CONTENTS Page Abstract. i ListArkansas Water Resources Center ALGAL GROWTH POTENTIALS AND HEAVY METAL CONCENTRATIONS) demonstrated the probable inhibition of algal growth potential by heavy metals in upper Beaver Lake. Upper

Soerens, Thomas

322

Patrick Scheuermann Center Director  

E-Print Network (OSTI)

propulsion test facilities; and ensured Stennis continued to serve as the systems engineering center at Stennis for NASA's Reusable Launch Vehicle program, a NASA-industry effort to develop a new generation of rockets to safely and cost-effectively send payloads to space. He also served as project manager

323

National Energy Software Center  

SciTech Connect

A short introduction is given to the services of the National Energy Software Library at the Argonne National Laboratory. The objectives, history, and software collection of the center are presented. Information on ordering from the software collection of the library is also included. 4 refs., 3 tabs. (DWL)

Eyberger, L.R.

1986-01-01T23:59:59.000Z

324

Arkansas Water Resources Center  

E-Print Network (OSTI)

. Geographical Information System (GIS) Support. The Center for Advanced Spatial Technology (CAST) and the GIS Laboratory in the Department of Crop, Soil, and Environmental Sciences provide support in developing GIS data the viability of alternate water supplies using abandoned, flooded coal mines for the City of Greenwood

Soerens, Thomas

325

HEEP CENTER Building # 1502  

E-Print Network (OSTI)

1 HEEP CENTER Building # 1502 EMERGENCY EVACUATION PLAN Prepared by: Harry Cralle and Mark Wright a building. Examples of such occasions include: smoke/fire, gas leak, bomb threat. Pre-planning and rehearsal are effective ways to ensure that building occupants recognize the evacuation alarm and know how to respond

Tomberlin, Jeff

326

Infrastructure Assurance Center  

E-Print Network (OSTI)

, the United States relied on natural gas to meet about 22% of its energy needs. Therefore, assuring efficient, natural gas processing plants, and other industrial customers, along with the changes in the utilizationInfrastructure Assurance Center NGReal-time: processing and analysis tool for natural gas delivery

327

Precision Joining Center  

SciTech Connect

A workshop to obtain input from industry on the establishment of the Precision Joining Center (PJC) was held on July 10--12, 1991. The PJC is a center for training Joining Technologists in advanced joining techniques and concepts in order to promote the competitiveness of US industry. The center will be established as part of the DOE Defense Programs Technology Commercialization Initiative, and operated by EG G Rocky Flats in cooperation with the American Welding Society and the Colorado School of Mines Center for Welding and Joining Research. The overall objectives of the workshop were to validate the need for a Joining Technologists to fill the gap between the welding operator and the welding engineer, and to assure that the PJC will train individuals to satisfy that need. The consensus of the workshop participants was that the Joining Technologist is a necessary position in industry, and is currently used, with some variation, by many companies. It was agreed that the PJC core curriculum, as presented, would produce a Joining Technologist of value to industries that use precision joining techniques. The advantage of the PJC would be to train the Joining Technologist much more quickly and more completely. The proposed emphasis of the PJC curriculum on equipment intensive and hands-on training was judged to be essential.

Powell, J.W.; Westphal, D.A.

1991-08-01T23:59:59.000Z

328

RETIREMENT CENTER MISSION STATEMENT  

E-Print Network (OSTI)

timely and informative LIR programs: "What's Happening with Health Care Reform;" "The 2012 Presidential, curiosity, and their continuing care and contributions to their families, their university Caregiver Support: See p. 3 to learn more about the Center's collaborative effort with the UCB Elder Care

Alvarez-Cohen, Lisa

329

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

330

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,

331

New subdwarf B star periods  

E-Print Network (OSTI)

Subdwarf B (sdB) stars are thought to be helium burning stars with low mass hydrogen envelopes. Several evolutionary paths have been proposed to explain the formation of these systems. One of these scenarios is the evolution of the sdB progenitor within a binary system. We have looked systematically at bright sdB stars from the PG survey. By taking spectra at several different epochs we have measured the radial velocity shifts caused by the motion of the sdB star within the binary. Our data have been taken over a long time base line (2 years) which allowed us to find longer period binaries than known before. Here we present results for 29 sdB systems.

L. Morales-Rueda; P. F. L. Maxted; T. R. Marsh; R. C. North

2002-09-26T23:59:59.000Z

332

Neutron skins and neutron stars  

Science Journals Connector (OSTI)

Background: The neutron skin of a heavy nucleus as well as many neutron-star properties are highly sensitive to the poorly constrained density dependence of the symmetry energy.Purpose: To provide for the first time meaningful theoretical errors and to assess the degree of correlation between the neutron-skin thickness of 208Pb and several neutron-star properties.Methods: A proper covariance analysis based on the predictions of an accurately calibrated relativistic functional FSUGold is used to quantify theoretical errors and correlation coefficients.Results: We find correlation coefficients of nearly 1 (or ?1) between the neutron-skin thickness of 208Pb and a host of observables of relevance to the structure, dynamics, and composition of neutron stars.Conclusions: We suggest that a follow-up Lead Radius Experiment (PREX) measurement, ideally with a 0.5% accuracy, could significantly constrain the equation of state of neutron-star matter.

F. J. Fattoyev and J. Piekarewicz

2012-07-05T23:59:59.000Z

333

ENERGY STAR Portfolio Manager 101  

Office of Energy Efficiency and Renewable Energy (EERE)

Join us as we introduce and demonstrate the core functionality of EPAs ENERGY STAR Portfolio Manager tool. Attendees will learn how to: navigate Portfolio Manager; add a property and enter details...

334

ENERGY STAR Portfolio Manager 201  

Office of Energy Efficiency and Renewable Energy (EERE)

Continue to learn about EPAs new ENERGY STAR Portfolio Manager tool, with a deeper dive into more advanced functionalities such as: managing and tracking changes to your property uses over time;...

335

Inversion of the star transform  

E-Print Network (OSTI)

We define the star transform as a generalization of the broken ray transform introduced by us in previous work. The advantages of using the star transform include the possibility to reconstruct the absorption and the scattering coefficients of the medium separately and simultaneously (from the same data) and the possibility to utilize scattered radiation which, in the case of the conventional X-ray tomography, is discarded. In this paper, we derive the star transform from physical principles, discuss its mathematical properties and analyze numerical stability of inversion. In particular, it is shown that stable inversion of the star transform can be obtained only for configurations involving odd number of rays. Several computationally-efficient inversion algorithms are derived and tested numerically.

Fan Zhao; John C. Schotland; Vadim A. Markel

2014-05-06T23:59:59.000Z

336

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":""}]}

337

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

338

Buildings Energy Data Book: 9.1 ENERGY STAR  

Buildings Energy Data Book (EERE)

3 3 ENERGY STAR Commercial and Institutional Buildings and Industrial Plants (1) Building Type 1999 Office 2000 K-12 School 2001 Retail 2002 Hospital (General and Surgical) 2003 Supermarket/Grocery 2004 Hotel 2005 Bank/Financial Institution 2006 Warehouse (Unrefrigerated) 2007 Courthouse 2008 Medical Office 2009 Residence Hall/Dormitory 2010 Senior Care Facility 2011 Data Center Total (2) Warehouse (Refrigerated) House of Worship Industrial Plants Total Note(s): Source(s): 1) Data as of February 13, 2012. Additional buildings may qualify after applications are reviewed. 2) Totals are less than sum of individual years since some buildings have multiple years listed. Totals include buildings qualified in 2012. EPA, Database of ENERGY STAR Labeled Buildings and Plants, accessed February 13, 2012

339

STAR Vertex Detector Upgrade Development  

SciTech Connect

We report on the development and prototyping efforts undertaken with the goal of producing a micro-vertex detector for the STAR experiment at the RHIC accelerator at BNL. We present the basic detector requirements and show a sensor development path, conceptual mechanical design candidates and readout architecture. Prototyping and beam test results with current generation MimoSTAR-2 sensors and a readout system featuring FPGA based on-the-fly hit finding and data sparsification are also presented.

Greiner, Leo C.; Matis, Howard S.; Stezelberger, Thorsten; Vu,Chinh Q.; Wieman, Howard; Szelezniak, Michal; Sun, Xiangming

2008-01-28T23:59:59.000Z

340

GRBs from the First Stars  

SciTech Connect

We present an estimate of the Gamma Ray Bursts which should be expected from metal-free, elusive first generation of stars known as PopulationIII (PopIII). We derive the GRB rate from these stars from the Stellar Formation Rate obtained in several Reionization scenarios available in the literature. In all of the analyzed models we find that GRBs from PopIII are subdominant with respect to the ''standard'' (PopII) ones up to z {approx} 10.

Iocco, Fabio; /Naples U. /KIPAC, Menlo Park

2007-04-16T23:59:59.000Z

Note: This page contains sample records for the topic "rainey star center" 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

Magnesium Isotopes in Halo Stars  

E-Print Network (OSTI)

We have determined Mg isotope ratios in halo field dwarfs and giants in the globular cluster M71 based on high S/N high spectral resolution (R = 10$^5$) Keck HIRES spectra. Unlike previous claims of an important contribution from intermediate-mass AGB stars to the Galactic halo, we find that our $^{26}$Mg/$^{24}$Mg ratios can be explained by massive stars.

Jorge Melendez; Judith G. Cohen

2007-08-29T23:59:59.000Z

342

Electron Microscopy Center  

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

Acknowledgment Acknowledgment EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers Acknowledgment Please acknowledge your use of the EMC in your publications and presentations with the following acknowledgment statement: The electron microscopy was accomplished at the Electron Microscopy Center at Argonne National Laboratory, a U.S. Department of Energy Office of Science Laboratory operated under Contract No. DE-AC02-06CH11357 by UChicago Argonne, LLC.

343

LHC Physics Center | (none)  

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

Physics Center Physics Center Fermilab Home Visit LPC Physics Programs LPC Guest and Visitors HATS@LPC, Workshops and CMSDAS Jet-Substructure HATS CMS Data Analysis School 2013 CMS Data Analysis School 2012 CMS Data Analysis School 2011 EJTERM (CMS Data Analysis School 2010) Confronting Theory with Experiment: November 2011 Standard Model Benchmarks at the Tevatron and LHC Standard Model Benchmarks at High-Energy Hadron Colliders GED workshop 20-22 Aug, 2012 Topic of the Week Upcoming Past Speakers Archive Program Info LPC Physics Forum LPC Snowmass Efforts The INFIERI Project Fellows LPC Fellows Program Newsletter - LPC Fellows LPC Fellows - 2014 LPC Fellows - 2013 LPC Fellows - 2012 LPC Fellows - 2011 Community Faces of the LPC LPC Fellows - Current LPC Coffee Hour Calendar LPC Conf. Room Calendar

344

Aperture center energy showcase  

SciTech Connect

Sandia and Forest City have established a Cooperative Research and Development Agreement (CRADA), and the partnership provides a unique opportunity to take technology research and development from demonstration to application in a sustainable community. A project under that CRADA, Aperture Center Energy Showcase, offers a means to develop exhibits and demonstrations that present feedback to community members, Sandia customers, and visitors. The technologies included in the showcase focus on renewable energy and its efficiency, and resilience. These technologies are generally scalable, and provide secure, efficient solutions to energy production, delivery, and usage. In addition to establishing an Energy Showcase, support offices and conference capabilities that facilitate research, collaboration, and demonstration were created. The Aperture Center project focuses on establishing a location that provides outreach, awareness, and demonstration of research findings, emerging technologies, and project developments to Sandia customers, visitors, and Mesa del Sol community members.

Torres, J. J.

2012-03-01T23:59:59.000Z

345

PIA - I-Manage STARS | Department of Energy  

Energy Savers (EERE)

STARS PIA - I-Manage STARS PIA - I-Manage STARS More Documents & Publications PIA - INL PeopleSoft - Human Resource System PIA - Human Resources - Personal Information Change...

346

Intirion: ENERGY STAR Referral (MFRA-4GF) | Department of Energy  

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

specification. Intirion: ENERGY STAR Referral (MFRA-4GF) More Documents & Publications Samsung: ENERGY STAR Referral (RF26VAB) Friedrich: ENERGY STAR Referral (CP15F10) Friedrich:...

347

DOE Verification Testing in Support of ENERGY STAR, April 22...  

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

Verification Testing in Support of ENERGY STAR, April 22, 2011 DOE Verification Testing in Support of ENERGY STAR, April 22, 2011 This document describes ENERGY STAR verificaion...

348

ENERGY STAR Test Procedures and Verification | Department of...  

Energy Savers (EERE)

Appliance & Equipment Standards ENERGY STAR ENERGY STAR Test Procedures and Verification ENERGY STAR Test Procedures and Verification The Department of Energy (DOE) is the...

349

Doyle Conservation Center (DCC)  

Leominster, MA Built on a 50-acre reservation in Leominster, the Doyle Conservation Center (DCC) houses core Trustees staff and serves as a central training facility that showcases the organization's conservation activities. The DCC's LEED Gold rating reflects the mission of the Trustees of Reservations, which is "To preserve, for public use and enjoyment, properties of exceptional scenic, historic, and ecological value in Massachusetts." The DCC is accessible to the public and is often rented out by various groups and organizations.

350

Honda Transmission Technical Center  

Russells Point, OH The Honda Transmission Technical Center is located on the Honda of America Manufacturing Plant facility site in Russells Point, Ohio. This facility is used for product engineering and market quality testing and analysis of automatic transmissions. The building contains a large workshop area for ten cars, a future dynamometer, two laboratories, an open office area, three conference rooms, a break room, restrooms, and related support areas.

351

Industrial Assessment Centers (IACs)  

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

Small- and medium-sized manufacturers may be eligible to receive a no-cost assessment provided by DOE Industrial Assessment Centers (IACs). Teams located at 24 universities around the country conduct the energy audits to identify opportunities to improve productivity, reduce waste, and save energy. Each manufacturer typically identifies about $55,000 in potential annual savings on average. Over 15,000 IAC assessments have been conducted. IACs also train the next-generation of energy savvy engineers.

352

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

353

Electron Microscopy Center  

NLE Websites -- All DOE Office Websites

Laboratory Laboratory Electron Microscopy Center Argonne Home > EMC > EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers An Office of Science User Facility The Electron Microscopy Center (EMC) at Argonne National Laboratory develops and maintains unique capabilities for electron beam characterization and applies those capabilities to solve materials problems. The EMC staff carry out research with collaborators and users from Argonne, universities, and other laboratories. The expertise and facilities of the EMC additionally serve a group of national and international researchers. The EMC emphasizes three major areas: materials research, technique and instrumentation development, and operation as a national research facility. Research by EMC personnel includes microscopy based studies in high Tc superconducting materials, irradiation effects in metals and semiconductors, phase transformations, and processing related structure and chemistry of interfaces in thin films.

354

About CRSP Management Center  

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

CRSP Act Power Projects Contact CRSP Customers Environmental Review-NEPA Financial Data Operations Planning & Projects Power Marketing Rates CRSP Act Power Projects Contact CRSP Customers Environmental Review-NEPA Financial Data Operations Planning & Projects Power Marketing Rates About Colorado River Storage Project Management Center CRSP Management Center Office The Ak-Chin Indian Community in Arizona, the city of Aspen, Colo., and Kirtland Air Force Base in New Mexico are a few of the vital customers of the Colorado River Storage Project's Management Center. We assist customers in saving their valuable electrical resources by actively promoting energy management and conservation programs and helping them determine their future energy needs. When customers want new products and services tailored to their individual needs, we explore their ideas. We are also committed to protecting the delicate balance of the Colorado River and its tributaries. Agencies that manage this river's resources must weigh its many roles: irrigation, recreation, hydropower and native and non-native endangered species habitat protection. Balancing these resources with the needs of water and electrical energy customers is a chief concern.

355

John C. Stennis Space Center History of Stennis Space Center  

E-Print Network (OSTI)

Laboratory Propulsion Test Lead Center SSME Test Resp. 5/94 Stennis Space Center Estab. (5/88) Stennis Space · Dept. of Marine Science · Major Contractors · Pratt and Whitney Rocketdyne · Jacobs Technology Inc. · A, National Data Buoy Center · NOAA National Marine Fisheries Service · NOAA National Coastal Data Development

Waliser, Duane E.

356

Rochester Prevention Research Center National Center for Deaf Health Research  

E-Print Network (OSTI)

is being overweight or obese dangerous to your health? #12;Rochester Prevention Research Center NationalRochester Prevention Research Center National Center for Deaf Health Research Obesity and Your Health: The Deaf Weight Wise Research Project Scott Smith, MD, MPH Matt Starr, MPH Deaf Health Talks

Goldman, Steven A.

357

CenterPulse Wisconsin National Primate Research Center  

E-Print Network (OSTI)

CenterPulse Wisconsin National Primate Research Center University of Wisconsin-Madison Contents Welcome to our year in review, CenterPulse. We hope you enjoy the new format. In making our news more Affiliates 3 Just Published 7 In the news 7 WIMR Opening and Board Tour 8 Reduced Diet Thwarts Aging 10 Kate

Wisconsin at Madison, University of

358

MSU EASTERN AGRICULTURAL RESEARCH CENTER NDSU WILLISTON RESEARCH EXTENSION CENTER  

E-Print Network (OSTI)

MSU EASTERN AGRICULTURAL RESEARCH CENTER NDSU WILLISTON RESEARCH EXTENSION CENTER 2006 AGRICULTURAL://www.sidney.ars.usda.gov/state/ North Dakota State University Williston Research Extension Center 14120 Hwy 2 Williston, ND 58801 (701 may have been more or less. Weather Summary Williston, nd Precipitation Temperature Month 2006 Avg

Dyer, Bill

359

MSU EASTERN AGRICULTURAL RESEARCH CENTER NDSU WILLISTON RESEARCH EXTENSION CENTER  

E-Print Network (OSTI)

MSU EASTERN AGRICULTURAL RESEARCH CENTER NDSU WILLISTON RESEARCH EXTENSION CENTER 2007 AGRICULTURAL Dakota State University Williston Research Extension Center 14120 Hwy 2 Williston, ND 58801 (701) 774-4315 Fax: (701) 774-4307 E-mail: NDSU.Williston.REC@.ndsu.edu http

Dyer, Bill

360

"Infotonics Technology Center"  

SciTech Connect

During this grant period July 15, 2002 thru September 30, 2004, the Infotonics Technology Center developed the critical infrastructure and technical expertise necessary to accelerate the development of sensors, alternative lighting and power sources, and other specific subtopics of interest to Department of Energy. Infotonics fosters collaboration among industry, universities and government and operates as a national center of excellence to drive photonics and microsystems development and commercialization. A main goal of the Center is to establish a unique, world-class research and development facility. A state-of-the-art microsystems prototype and pilot fabrication facility was established to enable rapid commercialization of new products of particular interest to DOE. The Center has three primary areas of photonics and microsystems competency: device research and engineering, packaging and assembly, and prototype and pilot-scale fabrication. Center activities focused on next generation optical communication networks, advanced imaging and information sensors and systems, micro-fluidic systems, assembly and packaging technologies, and biochemical sensors. With targeted research programs guided by the wealth of expertise of Infotonics???????????????????????????????????????????????????????????????¢???????????????????????????????????????????????????????????????????????????????????????????????????????????????????????????????? business and scientific staff, the fabrication and packaging facility supports and accelerates innovative technology development of special interest to DOE in support of its mission and strategic defense, energy, and science goals.

Fritzemeier, L., Boysel, M.B., and Smith, D.R.

2005-01-14T23:59:59.000Z

Note: This page contains sample records for the topic "rainey star center" 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

Data Center Energy Benchmarking: Part 4 - Case Study on a Computer-testing Center (No. 21)  

E-Print Network (OSTI)

data center & non-chilling Load Data Center Computer Loadpower density (W/ft2) Total Non-Data Center Load Data CenterComputer Load Data Center CRAH Units Chillers (Data Center

Xu, Tengfang; Greenberg, Steve

2007-01-01T23:59:59.000Z

362

Shear viscosity in hybrid stars  

Science Journals Connector (OSTI)

A study of the shear viscosity of hadrons and quarks in hybrid stars has been performed in the framework of the microscopic transport theory. The neutron-star structure has been determined employing the equation of state from the Brueckner theory with three-body force for the hadron phase, and the equation of state from the MIT bag model for the deconfined quark phase. The nucleon-nucleon cross sections in dense matter have been consistently calculated from the Brueckner G matrix, whereas for the quark-quark cross sections the perturbative QCD has been adopted. Despite that the quark contribution to the shear viscosity is quite small at low temperature, the transition to the deconfined phase makes the equation of state much softer with the result that the baryon viscosity turns out to be enhanced instead of reduced in hybrid stars. The damping time scale of r-modes due to the shear viscosity has been evaluated for several stable configurations of a hybrid star and compared with the neutron-star spin-down time scale induced by the emission gravitation radiation from the r-modes. The enhancement of the total viscosity makes the viscosity time scale comparable with the gravitation radiation one at low temperature.

D. Jaccarino; S. Plumari; V. Greco; U. Lombardo; A. B. Santra

2012-05-03T23:59:59.000Z

363

Evolution of the Dark Matter Distribution at the Galactic Center  

Science Journals Connector (OSTI)

Annihilation radiation from neutralino dark matter at the Galactic center (GC) would be greatly enhanced if the dark matter were strongly clustered around the supermassive black hole (SBH). The existence of a dark matter spike is made plausible by the observed, steeply rising stellar density near the GC SBH. Here the time-dependent equations describing gravitational interaction of the dark matter with the stars are solved. Scattering of dark matter particles by stars would substantially lower the dark matter density near the GC SBH over 10Gyr, due both to kinetic heating and to capture of dark matter particles by the SBH. This evolution implies a decrease by several orders of magnitude in the observable flux of annihilation products compared with models that associate a steep, dark matter spike with the SBH.

David Merritt

2004-05-20T23:59:59.000Z

364

Alternative Fuels Data Center: Disclaimer  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

AFDC AFDC Printable Version Share this resource Send a link to Alternative Fuels Data Center: Disclaimer to someone by E-mail Share Alternative Fuels Data Center: Disclaimer on Facebook Tweet about Alternative Fuels Data Center: Disclaimer on Twitter Bookmark Alternative Fuels Data Center: Disclaimer on Google Bookmark Alternative Fuels Data Center: Disclaimer on Delicious Rank Alternative Fuels Data Center: Disclaimer on Digg Find More places to share Alternative Fuels Data Center: Disclaimer on AddThis.com... Disclaimer The U.S. Department of Energy's (DOE) Alternative Fuels Data Center (AFDC) offers a wealth of information in the form of text, drawings, specifications, images, maps, and databases. This information combines research results, data analysis, descriptions of laws and incentives,

365

Alternative Fuels Data Center: Webmaster  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

About About Printable Version Share this resource Send a link to Alternative Fuels Data Center: Webmaster to someone by E-mail Share Alternative Fuels Data Center: Webmaster on Facebook Tweet about Alternative Fuels Data Center: Webmaster on Twitter Bookmark Alternative Fuels Data Center: Webmaster on Google Bookmark Alternative Fuels Data Center: Webmaster on Delicious Rank Alternative Fuels Data Center: Webmaster on Digg Find More places to share Alternative Fuels Data Center: Webmaster on AddThis.com... More in this section... Project Assistance News & Features Spanish Resources Contacts Webmaster Please use this form to send us your comments, report problems, and/or ask questions about information on the Alternative Fuels Data Center website. If your comment applies to a particular page, please provide the relevant

366

LANSCE | Lujan Neutron Scattering Center  

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

Department of Energy, National Office of Science Department of Energy, National Office of Science science.energy.gov Department of Energy, National Nuclear Security Administration nnsa.energy.gov Lujan Neutron Scattering Center Logo Lujan Center Mission The Lujan Center delivers science by exploiting the unique characteristics of intense beams of pulsed neutrons for academia, national security, and industry. Lujan Center Vision The Lujan Center will operate a world class user program in the service of the nation. Lujan Center scientists will be recognized for their leadership and innovation in neutron scattering. Lujan Center at LANSCE The Lujan Center is one of five user facilities supported by the LANSCE accelerator which is stewarded. Funding to operate 10 instruments in a national user program is provided by the Department of Energy's Office of

367

Center for Beam Physics, 1992  

SciTech Connect

This report contains the following information on the center for beam physics: Facilities; Organizational Chart; Roster; Profiles of Staff; Affiliates; Center Publications (1991--1993); and 1992 Summary of Activities.

Not Available

1993-06-01T23:59:59.000Z

368

Alternative Fuels Data Center: Contacts  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

About About Printable Version Share this resource Send a link to Alternative Fuels Data Center: Contacts to someone by E-mail Share Alternative Fuels Data Center: Contacts on Facebook Tweet about Alternative Fuels Data Center: Contacts on Twitter Bookmark Alternative Fuels Data Center: Contacts on Google Bookmark Alternative Fuels Data Center: Contacts on Delicious Rank Alternative Fuels Data Center: Contacts on Digg Find More places to share Alternative Fuels Data Center: Contacts on AddThis.com... More in this section... Project Assistance News & Features Spanish Resources Contacts Contacts Use these contacts for questions or comments about the Alternative Fuels Data Center. Website Contact Send us your comments, report problems, and/or ask questions about information on this site.

369

GEORGE WATTS HILL ALUMNI CENTER  

E-Print Network (OSTI)

BR IN KH O U S- BU LLITT CHILLER BUILDING F KENAN STADIUM GEORGE WATTS HILL ALUMNI CENTER EHRINGHAUS

North Carolina at Chapel Hill, University of

370

Drought Update Colorado Climate Center  

E-Print Network (OSTI)

Drought Update Colorado Climate Center Roger Pielke, Sr., Director Prepared by Tara Green and Odie Bliss http://climate.atmos.colostate.edu #12;© 2003 by The Colorado Climate Center. 2 http://www.ncdc.noaa.gov/oa/climate/research/2003/mar/st005dv00pcp200303.html #12;© 2003 by The Colorado Climate Center. 3 #12;© 2003

371

Ethics Center Annual Report III  

E-Print Network (OSTI)

#12;Ethics Center Annual Report III 2012-2013 TEXAS TECH UNIVERSITY #12;#12;TEXAS TECH UNIVERSITY August 31, 2013 Prepared by the TTU Ethics Center Annual Report III 2012-2013 #12;1 AnnualReportIII|8 proposed a university ethics center to provide the campus with ethics education resources. Since its

Rock, Chris

372

Pricing data center demand response  

Science Journals Connector (OSTI)

Demand response is crucial for the incorporation of renewable energy into the grid. In this paper, we focus on a particularly promising industry for demand response: data centers. We use simulations to show that, not only are data centers large loads, ... Keywords: data center, demand response, power network, prediction based pricing

Zhenhua Liu; Iris Liu; Steven Low; Adam Wierman

2014-06-01T23:59:59.000Z

373

Davison Health Center Dear Doctor,  

E-Print Network (OSTI)

5/131 Davison Health Center Dear Doctor, The Wesleyan University Davison Health Center is happy specific requirements detailed below. Our health center is equivalent to a typical outpatient community for allergy immunotherapy services within the context of our level of care, please complete the included

Royer, Dana

374

Data Center Airflow Management Retrofit  

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

Case study bulletin describes the data center airflow management retrofit. The study includes information about how the data center energy densities (measured in power-use per square foot), increase energy savings for cooling, and how it can be realized by optimizing airflow pathways within the data center.

375

University of Connecticut Health Center  

E-Print Network (OSTI)

by a designated licensed health care professional here at UCHC who did not participate in the original denialUniversity of Connecticut Health Center (Patient Identification) Request to View Record DHHS Government Center University of Connecticut Health Center J.F. Kennedy Federal Building ­ Room

Oliver, Douglas L.

376

A Walking Tour Health Center  

E-Print Network (OSTI)

and caring. #12;3. River of Ponds Tapestry Enter the Health Center, look to the left, and see the massiveHealing Pathways A Walking Tour of the UConn Health Center Public Art Collection Made possible by a generous gift from the Health Center Auxiliary #12;#12;Welcome! Everywhere you walk, whether outdoors

Oliver, Douglas L.

377

The Star Formation History of NGC 6822  

E-Print Network (OSTI)

Images of five fields in the Local Group dwarf irregular galaxy NGC 6822 obtained with the {\\it Hubble Space Telescope} in the F555W and F814W filters are presented. Photometry for the stars in these images was extracted using the Point-Spread-Function fitting program HSTPHOT/MULTIPHOT. The resulting color-magnitude diagrams reach down to $V\\approx26$, a level well below the red clump, and were used to solve quantitatively for the star formation history of NGC 6822. Assuming that stars began forming in this galaxy from low-metallicity gas and that there is little variation in the metallicity at each age, the distribution of stars along the red giant branch is best fit with star formation beginning in NGC 6822 12-15 Gyr ago. The best-fitting star formation histories for the old and intermediate age stars are similar among the five fields and show a constant or somewhat increasing star formation rate from 15 Gyr ago to the present except for a possible dip in the star formation rate from 3 to 5 Gyr ago. The main differences among the five fields are in the higher overall star formation rate per area in the bar fields as well as in the ratio of the recent star formation rate to the average past rate. These variations in the recent star formation rate imply that stars formed within the past 0.6 Gyr are not spatially very well mixed throughout the galaxy.

Ted K. Wyder

2001-07-31T23:59:59.000Z

378

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

379

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

380

National Carbon Capture Center Launches Post-Combustion Test Center |  

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

Carbon Capture Center Launches Post-Combustion Test Center Carbon Capture Center Launches Post-Combustion Test Center National Carbon Capture Center Launches Post-Combustion Test Center June 6, 2011 - 2:32pm Addthis Jenny Hakun What does this mean for me? Commercial deployment of the processes tested here could cut carbon pollution. Innovation is important to finding ways to make energy cleaner. And testing the ideas and processes that researchers come up with is critical to moving ideas from the lab to the marketplace. That's why the Department of Energy recently commissioned an Alabama testing facility that will help move research forward and speed up deployment of innovative post-combustion carbon dioxide (CO2) capture technologies for coal-based power plants. The Post-Combustion Carbon Capture Center (or PC4) facility tests new

Note: This page contains sample records for the topic "rainey star center" 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

National Carbon Capture Center Launches Post-Combustion Test Center |  

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

National Carbon Capture Center Launches Post-Combustion Test Center National Carbon Capture Center Launches Post-Combustion Test Center National Carbon Capture Center Launches Post-Combustion Test Center June 7, 2011 - 1:00pm Addthis Washington, D.C. - The recent successful commissioning of an Alabama-based test facility is another step forward in research that will speed deployment of innovative post-combustion carbon dioxide (CO2) capture technologies for coal-based power plants, according to the U.S. Department of Energy (DOE). Technologies tested at the Post-Combustion Carbon Capture Center (or PC4) are an important component of Carbon Capture and Storage, whose commercial deployment is considered by many experts as essential for helping to reduce human-generated CO2 emissions that contribute to potential climate change.

382

SciTech Connect: Energy Frontier Research Center Center for Materials...  

Office of Scientific and Technical Information (OSTI)

Technical Report: Energy Frontier Research Center Center for Materials Science of Nuclear Fuels Citation Details In-Document Search Title: Energy Frontier Research Center Center...

383

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Connecticut Incentives and Laws Connecticut Incentives and Laws The following is a list of expired, repealed, and archived incentives, laws, regulations, funding opportunities, or other initiatives related to alternative fuels and vehicles, advanced technologies, or air quality. Hydrogen and Fuel Cell Promotion Archived: 08/31/2013 The Connecticut Center for Advanced Technology (CCAT), with funding from the Department of Economic and Community Development (DECD), has established a Connecticut Hydrogen-Fuel Cell Coalition (Coalition). The Coalition works to enhance economic growth through the development, manufacture, and deployment of fuel cell and hydrogen technologies and associated fueling systems. Representatives from industry, government, academia, labor, and other stakeholders make up the Coalition. CCAT

384

Providence Newberg Medical Center  

Newberg, OR In 2002, Providence Health & Services began planning a new 188,000 square foot medical center in Newberg, Oregon to respond to the growing community's need for accessible health care. Since this was Providence's first new hospital in almost thirty years, its leaders decided to approach the project through innovative planning, design, and construction, including the achievement of lifecycle energy savings and a potential LEED certification. The hospital is comprised of 40 inpatient beds with views out to the surrounding rural landscape or into lushly planted internal courtyards.

385

Neutron skins and neutron stars  

SciTech Connect

The neutron-skin thickness of heavy nuclei provides a fundamental link to the equation of state of neutron-rich matter, and hence to the properties of neutron stars. The Lead Radius Experiment ('PREX') at Jefferson Laboratory has recently provided the first model-independence evidence on the existence of a neutron-rich skin in {sup 208}Pb. In this contribution we examine how the increased accuracy in the determination of neutron skins expected from the commissioning of intense polarized electron beams may impact the physics of neutron stars.

Piekarewicz, J. [Department of Physics, Florida State University, Tallahassee, FL 32306-4350 (United States)

2013-11-07T23:59:59.000Z

386

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

387

Towards a realistic axion star  

E-Print Network (OSTI)

In this work we estimate the radius and the mass of a self-gravitating system made of axions. The quantum axion field satisfies the Klein-Gordon equation in a curved space-time and the metric components of this space-time are solutions to the Einstein equations with a source term given by the vacuum expectation value of the energy-momentum operator constructed from the axion field. As a first step towards an axion star we consider the up to the sixth term in the axion potential expansion. We found that axion stars would have masses of the order of asteroids and radius of the order of few centimeters.

J. Barranco; A. Bernal

2008-08-01T23:59:59.000Z

388

Coalescing Neutron Stars -- a Step Towards Physical Models. I. Hydrodynamic Evolution and Gravitational-Wave Emission  

E-Print Network (OSTI)

We investigate the dynamics and evolution of coalescing neutron stars. Although the code (Piecewise Parabolic Method) is purely Newtonian, we do include the emission of gravitational waves and their backreaction on the hydrodynamic flow. The properties of neutron star matter are described by the physical equation of state of Lattimer \\& Swesty (1991). Energy loss by all types of neutrinos and changes of the electron fraction due to the emission of electron neutrinos and antineutrinos are taken into account by an elaborate ``neutrino leakage scheme''. We simulate the coalescence of two identical, cool neutron stars with a baryonic mass of $\\approx\\!1.6\\,M_\\odot$ and a radius of $\\approx\\!15$~km and with an initial center-to-center distance of 42~km. The initial distributions of density and electron concentration are given from a model of a cold neutron star in hydrostatic equilibrium (central temperature about $8\\,{\\rm MeV}$). We investigate three cases which differ by the initial velocity distribution in the neutron stars, representing different cases of the neutron star spins relative to the direction of the orbital angular momentum vector. Within about 1~ms the neutron stars merge into a rapidly spinning ($P_{\\rm spin}\\approx 1$~ms), high-density body ($\\rho\\approx 10^{14}$~g/cm$^3$) with a surrounding thick disk of material with densities $\\rho\\approx 10^{10}-10^{12}$~g/cm$^3$ and orbital velocities of~0.3--0.5~c. In this work we evaluate the models in detail with respect to the gravitational wave emission using the quadrupole approximation. In a forthcoming paper we will concentrate on the neutrino emission and implications for gamma-ray bursters. A maximum luminosity in excess of $10^{55}$~erg/s is reached for about 1~ms.

M. Ruffert; H. -Th. Janka; G. Schaefer

1995-09-01T23:59:59.000Z

389

Beryllium abundances in metal-poor stars  

Science Journals Connector (OSTI)

......standard big bang nucleosynthesis. Be cannot be produced by nuclear fusion in the interiors of stars; in contrast, Be would be...model of Allen Santillan (1991) for our sample stars. Input parameters, such as radial velocities, parallaxes and......

K. F. Tan; J. R. Shi; G. Zhao

2009-01-01T23:59:59.000Z

390

Cold quark matter in compact stars  

SciTech Connect

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

391

Haier: ENERGY STAR Referral (ESA408J)  

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

DOE referred Haier room air conditioner model ESA408J to EPA, brand manager of the ENERGY STAR program, for appropriate action after DOE testing revealed that the model does not meet ENERGY STAR requirements.

392

Haier: ENERGY STAR Referral (ESA3087)  

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

DOE referred Haier room air conditioner model ESA3087 to EPA, brand manager of the ENERGY STAR program, for appropriate action after DOE testing revealed that the model does not meet ENERGY STAR requirements.

393

Equator Appliance: ENERGY STAR Referral (EZ 3720)  

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

DOE referred Equator Appliance clothes washer EZ 3720 to EPA, brand manager of the ENERGY STAR program, for appropriate action after DOE testing revealed that the model does not meet ENERGY STAR requirements.

394

Review: Magnetic fields of O stars  

E-Print Network (OSTI)

Since 2002, strong, organized magnetic fields have been firmly detected at the surfaces of about 10 Galactic O-type stars. In this paper I will review the characteristics of the inferred fields of individual stars, as well as the overall population. I will discuss the extension of the 'magnetic desert', first inferred among the A-type stars, to O stars up to 60 solar masses. I will discuss the interaction of the winds of the magnetic stars with the fields above their surfaces, generating complex 'dynamical magnetosphere' structures detected in optical and UV lines, and in X-ray lines and continuum. Finally, I will discuss the detection of a small number of variable O stars in the LMC and SMC that exhibit spectral characteristics analogous to the known Galactic magnetic stars, and that almost certainly represent the first known examples of extra-Galactic magnetic stars.

Wade, G A

2014-01-01T23:59:59.000Z

395

ENERGY STAR Webinar: Portfolio Manager 101  

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

ENERGY STAR is hosting a webinar on the U.S. Environmental Protection Agency's new ENERGY STAR Portfolio Manager tool on Oct. 28, 2014, from 1:00 p.m. - 2:30 p.m. Eastern Standard Time.

396

How to Apply for the ENERGY STAR  

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

Join us to learn about applying for ENERGY STAR Certification in Portfolio Manager. Understand the value of the ENERGY STAR certification, see the step-by-step process of applying, and gain tips to...

397

Materials Preparation Center | Ames Laboratory  

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

Materials Preparation Center Materials Preparation Center Materials Preparation Center The Materials Preparation Center (MPC) is a U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Division of Materials Sciences & Engineering specialized research center located at the Ames Laboratory. MPC operations are primarily funded by the Materials Discovery, Design, & Synthesis team's Synthesis & Processing Science core research activity. MPC is recognized throughout the worldwide research community for its unique capabilities in purification, preparation, and characterization of: Rare earth metals [learn about rare earths] Single crystal growth Metal Powders/Atomization Alkaline-earth metals [learn more, wikipedia] External Link Icon Refractory metal [learn more, wikipedia] External Link Icon

398

Electron Microscopy Center  

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

Overview Overview The mission of the Electron Microscopy Center (EMC) is to: Conduct materials research using advanced microstructural characterization methods; Maintain unique resources and facilities for scientific research for the both the Argonne National Laboratory and national scientific community. Develop and expand the frontiers of microanalysis by fostering the evolution of synergistic state-of-the-art resources in instrumentation, techniques and scientific expertise; The staff members of the EMC carry out their own research as well as participate in collaborative programs with other scientists at Argonne National Laboratory as well as researchers, educators and students worldwide. The Electron Microscopy Center (EMC) at Argonne National Laboratory develops and maintains unique capabilities for electron beam characterization and applies those capabilities to solve materials problems. The EMC staff perform collaborative research with members of other Divisions at Argonne National Laboratory and with collaborators from universities and other laboratories. The expertise and facilities of the EMC additionally serve a group of national and international researchers. The EMC emphasizes three major areas: materials research, technique and instrumentation development, and operation as a national research facility. Research by EMC personnel includes microscopy based studies in high Tc superconducting materials, irradiation effects in metals and semiconductors, phase transformations, and processing related structure and chemistry of interfaces in thin films.

399

Hubble Sees a Neutron Star Alone in Space Nearest Known Neutron Star  

E-Print Network (OSTI)

Hubble Sees a Neutron Star Alone in Space Nearest Known Neutron Star #12;Birth of a Neutron Star In the core, nuclei are smashed into protons & neutrons; the protons combine with electrons to make neutrons & neutrinos. The birth temperature of a neutron star is ~5?1011 K, but neutrino emission cools it to `only

Barnes, Joshua Edward

400

Gas & Stars Aging low-mass stars eject their outer layers.  

E-Print Network (OSTI)

Recycling Gas & Stars #12;Aging low-mass stars eject their outer layers. M57:The Ring Nebula #12;Thor's Emerald Helmet Winds from high-mass stars blow bubbles of hot gas. #12;Supernova blast waves in stars are mixed back into the gas. NGC 6992: Filaments of theVeil Nebula #12;Bubbles blown by high

Barnes, Joshua Edward

Note: This page contains sample records for the topic "rainey star center" 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

NuSTAR: Nuclear Spectroscopic Telescope Array  

SciTech Connect

Bill Craig, an astrophysicist at Lawrence Livermore National Laboratory, describes the NASA NuSTAR mission, launched June 13, 2012.

Craig, Bill

2012-06-13T23:59:59.000Z

402

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

403

ENERGY STAR Guide to Retro-Commissioning  

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

ENERGY STAR Guide to Retro-Commissioning gives an overview of RCx and provides detailed project guidance.

404

The nuclear physics of neutron stars  

SciTech Connect

We explore the unique and fascinating structure of neutron stars. Although neutron stars are of interest in many areas of Physics, our aim is to provide an intellectual bridge between Nuclear Physics and Astrophysics. We argue against the naive perception of a neutron star as a uniform assembly of neutrons packed to enormous densities. Rather, by focusing on the many exotic phases that are speculated to exist in a neutron star, we show how the reality is different and far more interesting.

Piekarewicz, J. [Department of Physics, Florida State University, Tallahassee, FL 32306-4350 (United States)

2014-05-09T23:59:59.000Z

405

Alternative Fuels Data Center: Propane  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Propane Propane Printable Version Share this resource Send a link to Alternative Fuels Data Center: Propane to someone by E-mail Share Alternative Fuels Data Center: Propane on Facebook Tweet about Alternative Fuels Data Center: Propane on Twitter Bookmark Alternative Fuels Data Center: Propane on Google Bookmark Alternative Fuels Data Center: Propane on Delicious Rank Alternative Fuels Data Center: Propane on Digg Find More places to share Alternative Fuels Data Center: Propane on AddThis.com... More in this section... Propane Basics Benefits & Considerations Stations Vehicles Laws & Incentives Propane Fuel Prices Find propane fuel prices and trends. Propane, also known as liquefied petroleum gas (LPG) or autogas, has been used worldwide as a vehicle fuel for decades. It is stored as a liquid, and

406

Alternative Fuels Data Center: Hydrogen  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Hydrogen Hydrogen Printable Version Share this resource Send a link to Alternative Fuels Data Center: Hydrogen to someone by E-mail Share Alternative Fuels Data Center: Hydrogen on Facebook Tweet about Alternative Fuels Data Center: Hydrogen on Twitter Bookmark Alternative Fuels Data Center: Hydrogen on Google Bookmark Alternative Fuels Data Center: Hydrogen on Delicious Rank Alternative Fuels Data Center: Hydrogen on Digg Find More places to share Alternative Fuels Data Center: Hydrogen on AddThis.com... More in this section... Hydrogen Basics Benefits & Considerations Stations Vehicles Laws & Incentives Hydrogen Hydrogen is a potentially emissions-free alternative fuel that can be produced from diverse domestic energy sources. Research is under way to make hydrogen vehicles practical for widespread use.

407

Alternative Fuels Data Center: Biodiesel  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Biodiesel Biodiesel Printable Version Share this resource Send a link to Alternative Fuels Data Center: Biodiesel to someone by E-mail Share Alternative Fuels Data Center: Biodiesel on Facebook Tweet about Alternative Fuels Data Center: Biodiesel on Twitter Bookmark Alternative Fuels Data Center: Biodiesel on Google Bookmark Alternative Fuels Data Center: Biodiesel on Delicious Rank Alternative Fuels Data Center: Biodiesel on Digg Find More places to share Alternative Fuels Data Center: Biodiesel on AddThis.com... More in this section... Biodiesel Basics Benefits & Considerations Stations Vehicles Laws & Incentives Biodiesel Fuel Prices Find biodiesel fuel prices and trends. Biodiesel is a domestically produced, renewable fuel that can be manufactured from vegetable oils, animal fats, or recycled restaurant

408

JGI - DOE Bioenergy Research Centers  

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

DOE Bioenergy Research Centers DOE Bioenergy Research Centers DOE JGI performs sequencing on behalf of the U.S. Department of Energy Bioenergy Research Centers. The Centers are intended to accelerate basic research in the development of cellulosic ethanol and other biofuels, advancing the federal initiative that seeks to reduce U.S. gasoline consumption by 20% within 10 years through increased efficiency and diversification of clean energy sources. The three Centers are located in geographically distinct areas and use different plants both for laboratory research and for improving feedstock crops. DOE BioEnergy Science Center led by DOE's Oak Ridge National Laboratory in Oak Ridge, Tennessee. This center will focus on the resistance of plant fiber to breakdown into sugars and is studying the potential energy crops

409

Alternative Fuels Data Center: Electricity  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Electricity Electricity Printable Version Share this resource Send a link to Alternative Fuels Data Center: Electricity to someone by E-mail Share Alternative Fuels Data Center: Electricity on Facebook Tweet about Alternative Fuels Data Center: Electricity on Twitter Bookmark Alternative Fuels Data Center: Electricity on Google Bookmark Alternative Fuels Data Center: Electricity on Delicious Rank Alternative Fuels Data Center: Electricity on Digg Find More places to share Alternative Fuels Data Center: Electricity on AddThis.com... More in this section... Electricity Basics Benefits & Considerations Stations Vehicles Laws & Incentives Electricity Fuel Prices Find electricity fuel prices and trends. Electricity can be used to power all-electric vehicles and plug-in hybrid

410

Regency Centers | Open Energy Information  

Open Energy Info (EERE)

Regency Centers Regency Centers Jump to: navigation, search Name Regency Centers Place Jacksonville, FL Zip 32202 Website http://www.regencycenters.com References Regency Centers[1] Information About Partnership with NREL Partnership with NREL Yes Partnership Type Test & Evaluation Partner Partnering Center within NREL Electricity Resources & Building Systems Integration Partnership Year 2009 Link to project description http://www.nrel.gov/features/20090619_buildings.html LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! Regency Centers is a company located in Jacksonville, FL. Recency Centers is one of 23 National Accounts Companies partnering with NREL and PNNL for testing and validation of design concepts that will reduce energy consumption in commercial buildings[2].

411

Alternative Fuels Data Center: Glossary  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

AFDC AFDC Printable Version Share this resource Send a link to Alternative Fuels Data Center: Glossary to someone by E-mail Share Alternative Fuels Data Center: Glossary on Facebook Tweet about Alternative Fuels Data Center: Glossary on Twitter Bookmark Alternative Fuels Data Center: Glossary on Google Bookmark Alternative Fuels Data Center: Glossary on Delicious Rank Alternative Fuels Data Center: Glossary on Digg Find More places to share Alternative Fuels Data Center: Glossary on AddThis.com... Glossary Use this comprehensive glossary to define terms commonly used in the alternative fuels and advanced vehicles industry. If you have questions about specific technologies or fuels, contact the Technical Response Service at 1-800-254-6735. Click on the appropriate letter. · A· B· C· D· E· F· G· H· I· J· K· L· M· N· O· P· Q· R· S· T· U· V· W· X· Y· Z·

412

Alternative Fuels Data Center: Widgets  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Widgets to someone by Widgets to someone by E-mail Share Alternative Fuels Data Center: Widgets on Facebook Tweet about Alternative Fuels Data Center: Widgets on Twitter Bookmark Alternative Fuels Data Center: Widgets on Google Bookmark Alternative Fuels Data Center: Widgets on Delicious Rank Alternative Fuels Data Center: Widgets on Digg Find More places to share Alternative Fuels Data Center: Widgets on AddThis.com... Widgets The Alternative Fuels Data Center (AFDC) offers widgets about alternative fuels and advanced technology vehicles. Get these widgets for your website, blog, or social networking site so your readers can access current information from the AFDC. Also find more widgets from the U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy. Alternative Fueling Station Locator

413

Alternative Fuels Data Center: Ethanol  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Ethanol Ethanol Printable Version Share this resource Send a link to Alternative Fuels Data Center: Ethanol to someone by E-mail Share Alternative Fuels Data Center: Ethanol on Facebook Tweet about Alternative Fuels Data Center: Ethanol on Twitter Bookmark Alternative Fuels Data Center: Ethanol on Google Bookmark Alternative Fuels Data Center: Ethanol on Delicious Rank Alternative Fuels Data Center: Ethanol on Digg Find More places to share Alternative Fuels Data Center: Ethanol on AddThis.com... More in this section... Ethanol Basics Benefits & Considerations Stations Vehicles Laws & Incentives Ethanol Fuel Prices Find ethanol fuel prices and trends. Ethanol is a renewable fuel made from corn and other plant materials. The use of ethanol is widespread-almost all gasoline in the U.S. contains

414

Alternative Fuels Data Center: Tools  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Tools to someone by Tools to someone by E-mail Share Alternative Fuels Data Center: Tools on Facebook Tweet about Alternative Fuels Data Center: Tools on Twitter Bookmark Alternative Fuels Data Center: Tools on Google Bookmark Alternative Fuels Data Center: Tools on Delicious Rank Alternative Fuels Data Center: Tools on Digg Find More places to share Alternative Fuels Data Center: Tools on AddThis.com... Tools The Alternative Fuels Data Center offers a large collection of helpful tools. These calculators, interactive maps, and data searches can assist fleets, fuel providers, and other transportation decision makers in their efforts to reduce petroleum use. Calculators Vehicle Cost Calculator Compare cost of ownership and emissions for most vehicle models. Icon_mobile_version mobile

415

Solar Energy Resource Center | Department of Energy  

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

Energy Resource Center Solar Energy Resource Center The SunShot Initiative's Solar Energy Resource Center contains work developed by DOE, national laboratories and SunShot...

416

Data Center Energy Efficiency | Department of Energy  

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

Program Areas Data Center Energy Efficiency Data Center Energy Efficiency The Federal Energy Management Program (FEMP) supports data center efficiency initiatives by encouraging...

417

Industrial Assessment Centers Quarterly Update, Spring 2014 ...  

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

Assessment Centers Quarterly Update, Spring 2014 Read the Industrial Assessment Centers (IAC) Quarterly Update -- Spring 2014 Industrial Assessment Centers (IAC) Quarterly Update...

418

The DOE Information Center | Department of Energy  

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

Community Engagement The DOE Information Center The DOE Information Center The DOE Information Center provides citizens a consolidated facility to obtain information and records...

419

Evaluating Economizer Use In Data Centers  

E-Print Network (OSTI)

Evaluating Economizer Use in Data Centers Benjamin Chu,eelet Keywords: Data centers, economizers, HVAC, indoor airfor data centers are economizers, which turn off the power

Chu, Benjamin

2009-01-01T23:59:59.000Z

420

WINDExchange: Wind Energy Regional Resource Centers  

Wind Powering America (EERE)

Bookmark and Share Regional Resource Centers About Economic Development Siting Wind Energy Regional Resource Centers The U.S. Department of Energy's Regional Resource Centers...

Note: This page contains sample records for the topic "rainey star center" 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

The Nature of the Massive Young Stars in W75 N  

E-Print Network (OSTI)

We have observed the W75 N massive star forming region in SiO(J=2-1 & J=1-0) at 3" - 5" resolution and in 6 cm, 2 cm, and 7 mm continuum emission at 1.4" - 0.2" resolution. The abundance ratio of [SiO]/[H2] is roughly 5-7 x 10^-11 which is typical for what is expected in the ambient component of molecular clouds with active star formation. The SiO morphology is diffuse and centered on the positions of the ultracompact HII regions - no collimated, neutral jet was discovered. The ionized gas surrounding the protostars have emission measures ranging from 1-15 x 10^6 pc cm^-6, densities from 0.4-5 x 10^4 cm^-3, and derived spectral types of the central ionizing stars ranging from B0.5 to B2. Most of the detected sources have spectral indicies which suggest optically thin to moderately optically thick HII regions produced by a central ionizing star. The spread in ages between the oldest and youngest early-B protostars in the W75 N cluster is 0.1-5 x 10^6 years. This evolutionary timescale for W75 N is consistent with that found for early-B stars born in clusters forming more massive stars (Mstar > 25 Msun).

D. S. Shepherd; S. E. Kurtz; L. Testi

2003-10-15T23:59:59.000Z

422

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

423

STAR Highlights on Heavy Ion Physics  

E-Print Network (OSTI)

RHIC-STAR is a mid-rapidity collider experiment for studying high energy nuclear collisions. The main physics goals of STAR experiment are 1) studying the properties of the strongly coupled Quark Gluon Plasma, 2) explore the QCD phase diagram structure. In these proceedings, we will review the recent results of heavy ion physics at STAR.

Shusu Shi

2014-09-30T23:59:59.000Z

424

Massive Stars: Their Birth Sites and Distribution  

E-Print Network (OSTI)

The stellar IMF has been found to be an invariant Salpeter power-law (alpha=2.35) above about 1 Msun, but at the same time a massive star typically has more than one companion. This constrains the possible formation scenarios of massive stars, but also implies that the true, binary-star corrected stellar IMF could be significantly steeper than Salpeter, alpha>2.7. A significant fraction of all OB stars are found relatively far from potential birth sites which is most probably a result of dynamical ejections from cores of binary-rich star clusters. Such cores form rapidly due to dynamical mass segregation, or they are primordial. Probably all OB stars thus form in stellar clusters together with low-mass stars, and they have a rather devastating effect on the embedded cluster by rapidly driving out the remaining gas leaving expanding OB associations and bound star clusters. The distributed population of OB stars has a measured IMF with alpha about 4, which however, does not necessarily constitute a different physical mode for isolated star formation. A steep field-star IMF is obtained naturally because stars form in clusters which are distributed according to a power-law cluster mass function.

Pavel Kroupa

2003-09-22T23:59:59.000Z

425

Evolution of Low-Mass Population III Stars  

E-Print Network (OSTI)

We present the evolutionary models of metal-free stars in the mass range from 0.8 to 1.2 Msun with up-to-date input physics. The evolution is followed to the onset of hydrogen mixing into a convection, driven by the helium flash at red giant or asymptotic giant branch phase. The models of mass M >= 0.9 Msun undergo the central hydrogen flash, triggered by the carbon production due to the 3-alpha reactions. We find that the border of the off-center and central ignition of helium core flash falls between 1.1 and 1.2 Msun; the models of mass M hydrogen mixing at the tip of red giant branch while the models of M = 1.2 Msun during the helium shell flashes on the asymptotic giant branch. The equation of state for the Coulomb liquid region, where electron conduction and radiation compete, is shown to be important since it affects the thermal state in the helium core and influences the red giant branch evolution. It is also found that the non-resonant term of 3-alpha reactios plays an important role, although it has negligible effect in the evolution of stars of younger populations. We compare our models with the computations by several other sets of authors, to confirm the good agreement except for one study which finds the helium ignition much closer to the center with consequences important for subsequent evolution.

Takuma Suda; Masayuki Y. Fujimoto; Naoki Itoh

2005-04-25T23:59:59.000Z

426

Toy stars in one dimension  

Science Journals Connector (OSTI)

......equilibrium position due to forces from much greater masses...toy star stayed in the fundamental mode regardless of the...suggested that maybe the fundamental was an exact solution...really a many-body force that Newton had used...Stegun I. A., 1972, Handbook of Mathematical Functions......

J. J. Monaghan; D. J. Price

2004-06-01T23:59:59.000Z

427

BPS Skyrmions as neutron stars  

E-Print Network (OSTI)

The BPS Skyrme model has been demonstrated already to provide a physically intriguing and quantitatively reliable description of nuclear matter. Indeed, the model has both the symmetries and the energy-momentum tensor of a perfect fluid, and thus represents a field theoretic realization of the "liquid droplet" model of nuclear matter. In addition, the classical soliton solutions together with some obvious corrections (spin-isospin quantization, Coulomb energy, proton-neutron mass difference) led to an accurate modeling of nuclear binding energies for heavier nuclei. These results lead to the rather obvious proposal to try to describe also neutron stars by the BPS Skyrme model coupled to gravity. We find that the resulting self-gravitating BPS Skyrmions provide an excellent description of neutron stars when the parameter values of the model are extracted from nuclear physics. Specifically, the maximum possible mass of a neutron star before black-hole formation sets in is a few solar masses, the precise value depending on the precise values of the model parameters, and the resulting neutron star radius is of the order of 10 km.

C. Adam; C. Naya; J. Sanchez-Guillen; R. Vazquez; A. Wereszczynski

2014-07-14T23:59:59.000Z

428

BPS Skyrmions as neutron stars  

E-Print Network (OSTI)

The BPS Skyrme model has been demonstrated already to provide a physically intriguing and quantitatively reliable description of nuclear matter. Indeed, the model has both the symmetries and the energy-momentum tensor of a perfect fluid, and thus represents a field theoretic realization of the "liquid droplet" model of nuclear matter. In addition, the classical soliton solutions together with some obvious corrections (spin-isospin quantization, Coulomb energy, proton-neutron mass difference) provide an accurate modeling of nuclear binding energies for heavier nuclei. These results lead to the rather natural proposal to try to describe also neutron stars by the BPS Skyrme model coupled to gravity. We find that the resulting self-gravitating BPS Skyrmions provide excellent results as well as some new perspectives for the description of bulk properties of neutron stars when the parameter values of the model are extracted from nuclear physics. Specifically, the maximum possible mass of a neutron star before black-hole formation sets in is a few solar masses, the precise value depending on the precise values of the model parameters, and the resulting neutron star radius is of the order of 10 km.

C. Adam; C. Naya; J. Sanchez-Guillen; R. Vazquez; A. Wereszczynski

2014-07-14T23:59:59.000Z

429

Dark Stars: the First Stars in the Universe may be powered by Dark Matter Heating  

E-Print Network (OSTI)

A new line of research on Dark Stars is reviewed, which suggests that the first stars to exist in the universe were powered by dark matter heating rather than by fusion. Weakly Interacting Massive Particles, which may be there own antipartmers, collect inside the first stars and annihilate to produce a heat source that can power the stars. A new stellar phase results, a Dark Star, powered by dark matter annihilation as long as there is dark matter fuel.

Katherine Freese; Peter Bodenheimer; Paolo Gondolo; Douglas Spolyar

2008-12-28T23:59:59.000Z

430

Electron Microscopy Center  

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

Submit an EMC Proposal Submit an EMC Proposal EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers Submit an EMC Proposal EMC Proposal Submission Deadline Dates for FY2014: November 1, 2013 March 7, 2014 July 11, 2014 Is your proposal a multi-facility proposal? In other words, do you intend to submit proposals to EMC and APS or CNM for your research project? If your answer is "yes," go now to the Proposal Gateway.

431

Electron Microscopy Center  

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

EMC Users Committee EMC Users Committee EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers EMC Users Committee An EMC Users Committee has been organized to enhance communication between the user community and the EMC. While the EMC relies on and encourages strong interaction among its users and between its staff and users, the Users Committee provides an additional formal mechanism for user input into EMC planning and operations to ensure that users' needs and concerns are addressed.

432

factsheet: National Prototype Center  

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

the World Safer the World Safer This enduring national asset integrates science and technology for manufacturing success that meets our customer's special manufacturability challenges. Since its establishment in 1997, more than 5,0 0 0 i ndustr ies and government agencies have capitalized on the resources of the National Prototype Center (NPC). These customers received subject -matter expertise as well as critical manufacturing resources enabling development of i n novat ive manufacturing solutions. Specializing in high-risk, complex prototype work, the NPC integrates manufacturing, engineering and science to build first-of-a-kind products. It also modifies or enhances existing products and develops new, innovative manufacturing processes to solve the toughest manufacturing problems.

433

National Fertilizer Development Center  

Office of Legacy Management (LM)

h-L h-L National Fertilizer Development Center May 15, 1980 nww Hr. William Et Mott, Director Environmental Control Technology Division Office of Environment Dcpartiaent of Energy Washington, DC 20545 Dear Mr. Mott: This is in response to your letter of May 5 requesting ccmments on a report dated Xarct; 1930 which summarizes a preliminary radiological survey of facilities used in the early 1950's for studies of recovery of uranium from leached zone ore. I have made a few suggested changes to the report, which is being returned to you. * Thaul, you for the opportunity to review this report. Sincerely, , Enclosure Development Branch . 1 -a' . I . . . PRELIMINARY SURVEY OF TENNESSEE VALLEY AUTHORITY MUSCLE SHOALS, ALA&A Work .performed by the Health and Safety Research Division

434

Alternative Fuels Data Center  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Do alternative fuel vehicles Do alternative fuel vehicles (AFVs) improve air quality? How does the use of alternative fuels affect smog formation? You may find answers to these and other questions through the U.S. Department of Energy's (DOE) Alternative Fuels Data Center (AFDC)-the nation's most com- prehensive repository of perfor- mance data and general informa- tion on AFVs. To date, more than 600 vehi- cles-including light-duty cars, trucks, vans, transit buses, and heavy-duty trucks-have been tested on various alternative and conventional fuels with the goal of identifying the potential for alter- native fuels to displace petroleum and improve our nation's air quality. Although comparing regu- lated emissions between fuels may seem straightforward, evaluating emissions is complicated by

435

EV Technical Center  

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

December 2000 December 2000 AQMD CONTRACT #00192 Project Number: TC-00-0101 Report Number: TC-00-0101-TR02 Electric Vehicle Technical Center Prepared by: Ricardo Solares Juan C. Argueta Southern California Edison December 20, 2000 Page i DISCLAIMER OF WARRANTIES AND LIMITATION OF LIABILITIES This report was prepared by the Electric Transportation Division of Southern California Edison, a subsidiary of Edison International. Neither the Electric Transportation Division of Southern California Edison, Southern California Edison, Edison International, nor any person working for or on behalf of any of them makes any warranty or representation, express or implied, (i) with respect to the use of any information, product, process or procedure discussed in this report, including

436

Electron Microscopy Center  

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

An Office of Science User Facility An Office of Science User Facility The Electron Microscopy Center (EMC) at Argonne National Laboratory develops and maintains unique capabilities for electron beam characterization and applies those capabilities to solve materials problems. The EMC staff carry out research with collaborators and users from Argonne, universities, and other laboratories. The expertise and facilities of the EMC additionally serve a group of national and international researchers. The EMC emphasizes three major areas: materials research, technique and instrumentation development, and operation as a national research facility. Research by EMC personnel includes microscopy based studies in high Tc superconducting materials, irradiation effects in metals and semiconductors, phase transformations, and processing related structure and chemistry of interfaces in thin films.

437

Electron Microscopy Center  

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

End-of-Proposal Report End-of-Proposal Report EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers End-of-Proposal Report In accordance with the User Agreement, please provide the EMC with the following information when your proposal expires (one year after its acceptance date or when the experiments end, whichever is sooner). A research summary/progress report using these two templates:

438

Valley Forge Corporate Center  

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

55 Jefferson Ave. 55 Jefferson Ave. Valley Forge Corporate Center Norristown, PA 19403-2497 Pauline Foley Assistant General Counsel 610.666.8248 | Fax - 610.666.8211 foleyp@pjm.com October 30, 2013 Via Electronic Mail: juliea.smith@hq.doe.gov Christopher.lawrence@hq.doe.gov Julie A. Smith Office of Electricity Delivery and Energy Reliability Mail Code: OE-20 U.S. Department of Energy 1000 Independence Avenue, SW Washington, D.C. 20585 Re: Department of Energy - Improving Performance of Federal Permitting and Review of Infrastructure Projects. Request for Information ("RFI") 78 Fed. Reg. 53436 (August 29, 2013) Dear Ms. Smith: Please accept the following comments submitted on behalf of PJM Interconnection, L.L.C. ("PJM") in response to the RFI issued in the above captioned matter. This letter responds

439

EV Technical Center  

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

Carrier Route Vehicles Carrier Route Vehicles Quarterly Report, June 2001 AQMD CONTRACT #00192 Project Number: TC-00-0101 Report Number: TC-00-0101-TR04 Electric Vehicle Technical Center An ISO 9001 Certified Facility Prepared by: Michel Wehrey Juan C. Argueta Julie M. Phung Southern California Edison June 15, 2001 Page i DISCLAIMER OF WARRANTIES AND LIMITATION OF LIABILITIES This report was prepared by the Electric Transportation Division of Southern California Edison, a subsidiary of Edison International. Neither the Electric Transportation Division of Southern California Edison, Southern California Edison, Edison International, nor any person working for or on behalf of any of them makes any warranty or representation, express or implied, (i) with respect to the

440

Electron Microscopy Center  

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

SAMM SAMM EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers Sub-Ångstrom Microscopy and Microanalysis Facility In order to meet the scientific challenges of the future, the EMC has built a new state-of-the-art laboratory space for advanced electron microscopy. The new building has been designed to provide next- generation science with an operating environment that cannot be attained by renovating existing facilities. The EMC staff learned as much as possible from similar efforts around the world, including the SuperSTEM building at Daresbury, the Triebenberg Special Laboratory, the AML at Oak Ridge National Laboratory, the new NIST building, and various facilities for nanoscience.

Note: This page contains sample records for the topic "rainey star center" 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

Electron Microscopy Center  

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

Becoming a User Becoming a User EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers Procedure to Become a User at the EMC 1. Summary All users have to fulfill certain requirements before access to the EMC can be granted. The following list provides short descriptions of the requirements. Details can be found on this page and via the relevant links at the left. Register for access to Argonne's scientific user facilities (or update your user registration information).

442

Lujan Center User Guide  

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

1 1 The Surface Profile Analysis Reflectometer (SPEAR), located on Flight Path 9 in the Lujan Center, is ideally suited to study thin (from 5 - 3000 Å) organic and inorganic layers in a variety of different environments. The instrument uses an unpolarized neutron beam to study a broad range of materials including polymers, nano-engineered films, and biological systems. SPEAR is a time-of-flight (TOF) reflectometer using 2 choppers to define a typical wavelength range of 4.5 Å - 16 Å. With this polychromatic beam, a range of momentum transfer vectors (Q z ) can be measured without altering the angle of the incident beam. An important feature of SPEAR's design is that the beam is inclined to the horizon at 1.0°±0.0.25 This inclination allows for reflectivity

443

LANSCE | Lujan Center | Highlights  

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

Highlights New Evidence to Aid Search for Charge 'Stripes' in Superconductors Findings identify signature that will help scientists investigate and understand materials that carry current with no resistance "The scientists ground up crystals of the test material into a fine powder and placed samples of it in line with a beam of neutrons at the Los Alamos Neutron Scattering Center at Los Alamos National Laboratory. Similar to the way light reflecting off an object enters your eyes to create an image, the neutron beams diffracted by the crystals' atoms yield information about the positions of the atoms. The scientists used that information to infer the material's electronic structure, and repeated the experiment at gradually warmer temperatures."

444

Supernova Science Center  

SciTech Connect

The Supernova Science Center (SNSC) was founded in 2001 to carry out theoretical and computational research leading to a better understanding of supernovae and related transients. The SNSC, a four-institutional collaboration, included scientists from LANL, LLNL, the University of Arizona (UA), and the University of California at Santa Cruz (UCSC). Intitially, the SNSC was funded for three years of operation, but in 2004 an opportunity was provided to submit a renewal proposal for two years. That proposal was funded and subsequently, at UCSC, a one year no-cost extension was granted. The total operational time of the SNSC was thus July 15, 2001 - July 15, 2007. This document summarizes the research and findings of the SNSC and provides a cummulative publication list.

S. E. Woosley

2008-05-05T23:59:59.000Z

445

Industrial Assessment Center  

SciTech Connect

The University of Dayton (UD) performed energy assessments, trained students and supported USDOE objectives. In particular, the UD Industrial Assessment Center (IAC) performed 96 industrial energy assessment days for mid-sized manufacturers. The average identified and implemented savings on each assessment were $261,080 per year and $54,790 per year. The assessments served as direct training in industrial energy efficiency for 16 UD IAC students. The assessments also served as a mechanism for the UD IAC to understand manufacturing energy use and improve upon the science of manufacturing energy efficiency. Specific research results were published in 16 conference proceedings and journals, disseminated in 22 additional invited lectures, and shared with the industrial energy community through the UD IAC website.

J. Kelly Kissock; Becky Blust

2007-04-17T23:59:59.000Z

446

HPC Code Center Request Form | Computatioinal Scince Center, Brookhaven  

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

HPC Code Center Request Form HPC Code Center Request Form All fields are required unless marked as optional. Full Name Institution/Company Email Address Telephone Number Department * Basic Energy Sciences Directorate (DC) Bioscience Department (BO) Business Development & Analysis Office (BU) Business Operations (DI) CEGPA Directorate (DK) Center for Functional Nanomaterials (NC) Chemistry Department (CO) Collider Accelerator Department (AD) Community, Education, Government and Public Affairs (PA) Computational Science Center (CC) Condensed Matter Physics and Materials Science Department (PM) Counterintelligence (CI) Department of Energy (AE) Deputy Director for Operations Directorate (DE) Director's Office Directorate (DO) Diversity Office (DV) Energy & Utilities Division (EU) Environment, Safety and Health

447

Center for Inverse Design: Collaboration Tool for the Center...  

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

Collaboration Tool for the Center for Inverse Design The SharePoint collaboration tool provides access to research results obtained from various theoretical and experimental...

448

THE CIRCUMNUCLEAR STAR FORMATION ENVIRONMENT OF NGC 6946: Br ? AND H{sub 2} RESULTS FROM KECK INTEGRAL FIELD SPECTROSCOPY  

SciTech Connect

We present a three-dimensional data cube of the K-band continuum and the Br ?, H{sub 2} S(0), and S(1) lines within the central 18.''5 13.''8 (520 pc 390 pc) region of NGC 6946. Data were obtained using OSIRIS, a near-infrared Integral Field Spectrograph at Keck Observatory, with Laser Guide Star Adaptive Optics. The 0.''3 resolution allows us to investigate the stellar bulge and the forming star clusters in the nuclear region on 10 pc scales. We detect giant H II regions associated with massive young star clusters in the nuclear spiral/ring (R ? 30 pc) and in the principal shocks along the nuclear bar. Comparisons of the Br ? fluxes with Pa ? line emission and radio continuum indicate A{sub K} ? 3, A{sub V} ? 25 for the nuclear star-forming regions. The most luminous H II regions are restricted to within 70 pc of the center, despite the presence of high gas columns at larger radii (R ? 200 pc). H{sub 2} emission is restricted to clouds within R ? 60 pc of the center, resembling the distribution of HCN line emission. We propose that gas-assisted migration of the young star clusters is contributing to the buildup of the nuclear bar and nuclear star cluster (R < 30 pc) in this galaxy.

Tsai, Chao-Wei [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Turner, Jean L. [Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1547 (United States); Beck, Sara C. [Department of Physics and Astronomy, Tel Aviv University, Ramat Aviv (Israel); Meier, David S. [Department of Physics, New Mexico Institute of Mining and Technology, Socorro, NM 87801 (United States); Wright, Shelley A., E-mail: Chao-Wei.Tsai@jpl.nasa.gov [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, Toronto, Ontario (Canada)

2013-10-20T23:59:59.000Z

449

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

450

International Center for Advanced Renewable Energy  

E-Print Network (OSTI)

. . . . . . . . . . . . . . . . . 08 Consortium for Clean Coal Utilization . . . . . . . . . . . . . . . 09 Tyson Research Center

Subramanian, Venkat

451

Data Centers and Servers | Department of Energy  

Office of Environmental Management (EM)

Data Centers and Servers Data Centers and Servers Photo of the Green Data Center at the Research Support Facility. Data centers are one of the most energy-intensive building types,...

452

On the capture of dark matter by neutron stars  

E-Print Network (OSTI)

We calculate the number of dark matter particles that a neutron star accumulates over its lifetime as it rotates around the center of a galaxy, when the dark matter particle is a self-interacting boson but does not self-annihilate. We take into account dark matter interactions with baryonic matter and the time evolution of the dark matter sphere as it collapses within the neutron star. We show that dark matter self-interactions play an important role in the rapid accumulation of dark matter in the core of the neutron star. We consider the possibility of determining an exclusion region of the parameter space for dark matter mass and dark matter interaction cross sections based on the observation of old neutron stars with strong dark matter self-interactions. We show that for a dark matter density of $~10^3$ GeV/cm$^3$ and dark matter mass $m_\\chi$ less than approximately 10 GeV, there is a potential exclusion region for dark matter interactions with nucleons that is three orders of magnitude more stringent than without self-interactions. The potential exclusion region for dark matter self-interaction cross sections is many orders of magnitude stronger than the current Bullet Cluster limit. For example, for high dark matter density regions, we find that for $m_\\chi\\sim 10$ GeV when the dark matter interaction cross section with the nucleons ranges from $\\sigma_{\\chi n}\\sim 10^{-52}$ cm$^2$ to $10^{-57}$ cm$^2$, the dark matter self-interaction cross section limit is $\\sigma_{\\chi\\chi}ten orders of magnitude stronger than the Bullet Cluster limit.

Tolga Guver; Arif Emre Erkoca; Mary Hall Reno; Ina Sarcevic

2014-04-09T23:59:59.000Z

453

SWP Carbon Sequestration Training Center  

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

Training Center Presentation, Training Center Presentation, October 2010 SWP Carbon Sequestration Training Center Principal Investigators: New Mexico Tech, Andrew Campbell and Peter Mozley University of Utah, Brian McPherson Texas A&M University, Tarla Peterson SWP Training Center Presentation, October 2010 Background  Funded by DOE/NETL.  Purpose is to train more scientists and engineers for work in geological sequestration.  Three year grant.  Designed to be self sustaining. SWP Training Center Presentation, October 2010 Our goal is provide education about CCS at a variety of educational levels in order to promote a pipeline of future CCS scientists and engineers.  High School  K-12 Teachers  Undergraduate  Graduate  Professionals  Outreach SWP Training Center Presentation,

454

Alternative Fuels Data Center: Biobutanol  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Biobutanol to someone Biobutanol to someone by E-mail Share Alternative Fuels Data Center: Biobutanol on Facebook Tweet about Alternative Fuels Data Center: Biobutanol on Twitter Bookmark Alternative Fuels Data Center: Biobutanol on Google Bookmark Alternative Fuels Data Center: Biobutanol on Delicious Rank Alternative Fuels Data Center: Biobutanol on Digg Find More places to share Alternative Fuels Data Center: Biobutanol on AddThis.com... More in this section... Biobutanol Drop-In Biofuels Methanol P-Series Renewable Natural Gas xTL Fuels Biobutanol Biobutanol is a 4-carbon alcohol (butyl alcohol) produced from the same feedstocks as ethanol including corn, sugar beets, and other biomass feedstocks. Butanol is generally used as an industrial solvent in products such as lacquers and enamels, but it also can be blended with other fuels

455

Alternative Fuels Data Center: Telework  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Telework to someone by Telework to someone by E-mail Share Alternative Fuels Data Center: Telework on Facebook Tweet about Alternative Fuels Data Center: Telework on Twitter Bookmark Alternative Fuels Data Center: Telework on Google Bookmark Alternative Fuels Data Center: Telework on Delicious Rank Alternative Fuels Data Center: Telework on Digg Find More places to share Alternative Fuels Data Center: Telework on AddThis.com... More in this section... Idle Reduction Parts & Equipment Maintenance Driving Behavior Fleet Rightsizing System Efficiency Ridesharing Mass Transit Active Transit Multi-Modal Transportation Telework Telework Photo of a woman working from home. Telework is a flexible work arrangement where employees work from home (telecommute) or attend conferences and meetings from their computer

456

Alternative Fuels Data Center: Biogas  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Biogas to someone by Biogas to someone by E-mail Share Alternative Fuels Data Center: Biogas on Facebook Tweet about Alternative Fuels Data Center: Biogas on Twitter Bookmark Alternative Fuels Data Center: Biogas on Google Bookmark Alternative Fuels Data Center: Biogas on Delicious Rank Alternative Fuels Data Center: Biogas on Digg Find More places to share Alternative Fuels Data Center: Biogas on AddThis.com... More in this section... Biobutanol Drop-In Biofuels Methanol P-Series Renewable Natural Gas xTL Fuels Renewable Natural Gas (Biogas) Biogas-also known as biomethane, swamp gas, landfill gas, or digester gas-is the gaseous product of anaerobic digestion (decomposition without oxygen) of organic matter. In addition to providing electricity and heat, biogas is useful as a vehicle fuel. When processed to purity standards,

457

Alternative Fuels Data Center: Methanol  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Methanol to someone by Methanol to someone by E-mail Share Alternative Fuels Data Center: Methanol on Facebook Tweet about Alternative Fuels Data Center: Methanol on Twitter Bookmark Alternative Fuels Data Center: Methanol on Google Bookmark Alternative Fuels Data Center: Methanol on Delicious Rank Alternative Fuels Data Center: Methanol on Digg Find More places to share Alternative Fuels Data Center: Methanol on AddThis.com... More in this section... Biobutanol Drop-In Biofuels Methanol P-Series Renewable Natural Gas xTL Fuels Methanol Methanol (CH3OH), also known as wood alcohol, is an alternative fuel under the Energy Policy Act of 1992. As an engine fuel, methanol has chemical and physical fuel properties similar to ethanol. Methanol use in vehicles has declined dramatically since the early 1990s, and automakers no longer

458

Alternative Fuels Data Center: Ridesharing  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Ridesharing to someone Ridesharing to someone by E-mail Share Alternative Fuels Data Center: Ridesharing on Facebook Tweet about Alternative Fuels Data Center: Ridesharing on Twitter Bookmark Alternative Fuels Data Center: Ridesharing on Google Bookmark Alternative Fuels Data Center: Ridesharing on Delicious Rank Alternative Fuels Data Center: Ridesharing on Digg Find More places to share Alternative Fuels Data Center: Ridesharing on AddThis.com... More in this section... Idle Reduction Parts & Equipment Maintenance Driving Behavior Fleet Rightsizing System Efficiency Ridesharing Mass Transit Active Transit Multi-Modal Transportation Telework Ridesharing Photo of people car pooling. Rideshare programs help people share vehicles to commute together. Also known as carpooling, ridesharing conserves fuel and reduces vehicle

459

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.

460

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

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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
to obtain the most current and comprehensive results.


461

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

462

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

463

Atmospheres and radiating surfaces of neutron stars  

E-Print Network (OSTI)

The beginning of the 21st century was marked by a breakthrough in the studies of thermal radiation of neutron stars. Observations with modern space telescopes have provided a wealth of valuable information. Being correctly interpreted, this information can elucidate physics of superdense matter in the interiors of these stars. The theory of formation of thermal spectra of neutron stars is based on the physics of plasmas and radiative processes in stellar photospheres. It provides the framework for interpretation of observational data and for extracting neutron-star parameters from these data. This paper presents a review of the current state of the theory of surface layers of neutron stars and radiative processes in these layers, with the main focus on the neutron stars that possess strong magnetic fields. In addition to the conventional deep (semi-infinite) atmospheres, radiative condensed surfaces of neutron stars and "thin" (finite) atmospheres are also considered.

Potekhin, A Y

2014-01-01T23:59:59.000Z

464

Nuclear and gravitational energies in stars  

E-Print Network (OSTI)

The force that governs the evolution of stars is gravity. Indeed this force drives star formation, imposes thermal and density gradients into stars at hydrostatic equilibrium and finally plays the key role in the last phases of their evolution. Nuclear power in stars governs their lifetimes and of course the stellar nucleosynthesis. The nuclear reactions are at the heart of the changes of composition of the baryonic matter in the Universe. This change of composition, in its turn, has profound consequences on the evolution of stars and galaxies. The energy extracted from the gravitational, respectively nuclear reservoirs during the lifetimes of stars of different masses are estimated. It is shown that low and intermediate mass stars (M 8 Msol), which explode in a supernova explosion, extract more than 5 times more energy from the gravitational reservoir than from the nuclear one. We conclude by discussing a few important nuclear reactions and their link to topical astrophysical questions.

Meynet, Georges; Ekstrm, Sylvia

2013-01-01T23:59:59.000Z

465

Funding | Photosynthetic Antenna Research Center  

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

Funding Funding Investigators who receive support from the PARC should cite the Washington University Energy Frontier Research Center (EFRC) grant in all publications and projects....

466

Los Alamos Neutron Science Center  

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

Neutron Science Center gets capacity boost December 2, 2010 Los Alamos National Security funds upgrade to key facility LOS ALAMOS, New Mexico, December 2, 2010-The National Nuclear...

467

Solar Energy Research Center (SERC)  

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

Solar Energy Research Center (SERC) Community Richmond Bay Campus Planning Tours Community Programs Friends of Berkeley Lab Navigate Section Community Richmond Bay Campus...

468

Nuclear & Radiological Activity Center (NRAC)  

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

Nuclear & Radiological Activity Center (NRAC) Where nuclear research and deployment capabilities come together to solve nuclear nonproliferation challenges. Skip Navigation Links...

469

LANSCE | Lujan Center | Industrial Users  

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

Industrial Users The Lujan Neutron Scattering Center offers a diverse set of capabilities and instruments for industrial projects. Industrial users are invited to contact the Lujan...

470

ORISE: Center for Epidemiologic Research  

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

Center for Epidemiologic Research The Oak Ridge Institute for Science and Education (ORISE) has been building its capability in epidemiology since 1978. Early ORISE studies of...

471

Center for Energy Efficient Materials  

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

Plastic Solar Solid State Lighting High-Efficiency Solar Cells Thermoelectrics Undergraduate Internship Program Overview The Center for Energy Efficient Materials (CEEM) is an...

472

Center for Advanced Photophysics | Science  

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

Science The research of this Center focuses on (1) novel physical principles for solar energy conversion, (2) charge manipulation and exploratory photovoltaic device structures,...

473

Los Alamos Neutron Science Center  

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

LINAC Outreach Affiliations Visiting LANSCE Facilities Isotope Production Facility Lujan Neutron Scattering Center MaRIE Proton Radiography Ultracold Neutrons Weapons Neutron...

474

Secure Data Center (Fact Sheet)  

SciTech Connect

This fact sheet describes the purpose, lab specifications, applications scenarios, and information on how to partner with NREL's Secure Data Center at the Energy Systems Integration Facility.

Not Available

2012-08-01T23:59:59.000Z

475

Alternative Fuels Data Center: Publications  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Argonne National Laboratory Transportation Technology Research and Development Center Web Site: http:www.transportation.anl.govttrdcpublicationspdfsesd-41.pdf Clean Cities...

476

University of Connecticut Health Center  

E-Print Network (OSTI)

University of Connecticut Health Center John Dempsey Hospital Epidemiology (Patient Identification __________________ Before the procedure, did the operator: Obtain informed consent Notify direct patient care nurse

Oliver, Douglas L.

477

WINDExchange: About Regional Resource Centers  

Wind Powering America (EERE)

Development Siting About Regional Resource Centers Significant expansion of wind energy deployment will be required to achieve the President's goal of doubling renewable...

478

Joint Center for Artificial Photosynthesis  

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

North JCAP Headquarters Joint Center for Artificial Photosynthesis California Institute of Technology Jorgensen Laboratory, Mail Code 132-80 1200 East California Boulevard...

479

Joint Center for Artificial Photosynthesis  

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

Employment JCAP offers rewarding career opportunities for research scientists, engineers, and professional and administrative staff. The center is currently accepting applications...

480

Medtronic - MECC: Award Recipient of the ENERGY STAR Challenge for Industry  

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

Award Recipient of the ENERGY STAR Challenge for Industry Award Recipient of the ENERGY STAR Challenge for Industry Medtronic - MECC 6700 Shingle Creek Pkwy Brooklyn Center, MN 55430 The Medtronic-MECC facility is part of the Cardiac Rhythm and Disease Management division and specializes in the manufacturing of batteries, capacitors and other electrical components. The site also produces a variety of other components for other divisions within the Corporation. Medtronic-MECC achieved the ENERGY STAR Challenge for Industry in 2009. This plant reached 10% reduction in energy intensity in one year of its baseline. The site achieved the Challenge through fine tuning and scheduling of HVAC units and adjusting set points in manufacturing areas. Another achievement was absorbing additional manufacturing capacity within existing operations. Overall,

Note: This page contains sample records for the topic "rainey star center" 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

The Center for Laser Applications "An accomplished Center of Excellence"  

E-Print Network (OSTI)

Modular Microfluidic Systems for Drug Discovery Laser-Induced Ignition Studies of Solid Aluminum ParticlesThe Center for Laser Applications "An accomplished Center of Excellence" University of Tennessee and Combined Recovery Factor for High-Temperature Probe, AEDC TASK 09-02 Modeling of the Micro Laser Ablation

Davis, Lloyd M.

482

Gravitational collapse of a spherical star with heat flow as a possible energy mechanism of gamma-ray bursts  

E-Print Network (OSTI)

We investigate the gravitational collapse of a spherically symmetric, inhomogeneous star, which is described by a perfect fluid with heat flow and satisfies the equation of state $p=\\rho/3$ at its center. In the process of the gravitational collapsing, the energy of the whole star is emitted into space. And the remaining spacetime is a Minkowski one without a remnant at the end of the process. For a star with a solar mass and solar radius, the total energy emitted is at the order of $10^{54}$ {\\rm erg}, and the time-scale of the process is about $8s$. These are in the typical values for a gamma-ray burst. Thus, we suggest the gravitational collapse of a spherical star with heat flow as a possible energy mechanism of gamma-ray bursts.

Zhe Chang; Cheng-Bo Guan; Chao-Guang Huang; Xin Li

2008-03-26T23:59:59.000Z

483

Electron Microscopy Center  

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

Training Training EMC Home Overview Personnel Resources Highlights Publications Visit EMC Contact Info Information for Users Becoming a User Submit a Proposal End-of-Proposal Report Acknowledgment User Training User Safety User Status Instrument Access User Committee User Meetings Data Storage Policy Visiting the EMC Instrument Calendars Info for EMC Staff SÅMM Facility TEAM Project Microscopy Links Argonne Facilities DOE/BES Facilities DOE/BES BES Electron Beam Microcharacterization Centers User Training Prior Training in Electron Microscopy: People who wish to operate TEMs must have at least one college-level course in TEM with a lab component or previous TEM experience. The college course can't be one in which TEM was just one of many topics. For researchers who lack academic training and/or practical experience in electron microscopy, we suggest the short courses in TEM at the Hooke College of Applied Sciences, and the hands-on TEM courses at Northwestern University or the University of Chicago or Northern Illinois University.

484

Electron Microscopy Center  

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

General Information for EMC Users General Information for EMC Users The Electron Microscopy Center (EMC) is an Office of Science User Facility operated for the U.S. Department of Energy Office of Science by Argonne National Laboratory. It is one of three scientific user facilities for electron beam microcharacterization and one of several National User Facilities located at Argonne National Laboratory. As a scientific user facility, the EMC supports user-accessible instruments (Resources) for high spatial resolution microanalysis, field imaging, nanoscale structural characterization, nanoscale fabrication and manipulation, and unique in situ studies of materials under the influence of ion-beam irradiation. These capabilities are used in a diverse variety of research areas to address grand challenge scientific questions encompassing, for example, energy-related studies, biology, astrophysics, archaeology, superconductivity, nanotechnology, environmental engineering, tribology, and ferroelectricity. The research is performed both by users and by EMC staff. While many users work independently, the most challenging research activities require extensive contributions from EMC staff.

485

AMO Energy Resource Center  

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

Home | Programs & Offices | Consumer Information Home | Programs & Offices | Consumer Information Sign In Dashboard Home Add to Bookmark Turn on more accessible mode Skip to main content Turn off more accessible mode HOME | Help (new window) AMO Energy Resources Center HOME Tools AMO Home Tools to Manage your Energy Use DOE eGuide for ISO 50001 DOE eGuide Lite Industrial Facilities Scorecard Plant Energy Profiler (PEP) Project Opportunities Tracker EnPI V3.0 Webinars Past Webinar Titles (*Requires Login) Software Tool Updates the contents of this div will be replaced Steam System Modeler Tool: The new Steam System Modeler allows you to create up to a 3-pressure-header basic model of your current steam system. The tool includes a series of adjustable characteristics simulating technical or input changes, thereby demonstrating how each component impacts the others and what changes may best promote overall efficiency and stability of the system. The tool can be found under the "Steam" category.

486

The ecology of star clusters and intermediate mass black holes in the Galactic bulge  

E-Print Network (OSTI)

We simulate the inner 100pc of the Milky-Way Galaxy to study the formation and evolution of the population of star clusters and intermediate mass black holes. For this study we perform extensive direct N-body simulations of the star clusters which reside in the bulge, and of the inner few tenth of parsecs of the super massive black hole in the Galactic center. In our N-body simulations the dynamical friction of the star cluster in the tidal field of the bulge are taken into account via (semi)analytic soluations. The N-body calculations are used to calibrate a (semi)analytic model of the formation and evolution of the bulge. We find that about 10% of the clusters born within 100pc of the Galactic center undergo core collapse during their inward migration and form intermediate-mass black holes (IMBHs) via runaway stellar merging. After the clusters dissolve, these IMBHs continue their inward drift, carrying a few of the most massive stars with them. We predict that region within about 10 parsec of the SMBH is populated by about 50IMBHs of some 1000Msun. Several of these are expected to be accompanied still by some of the most massive stars from the star cluster. We also find that within a few milliparsec of the SMBH there is a steady population of several IMBHs. This population drives the merger rate between IMBHs and the SMBH at a rate of about one per 10Myr, sufficient to build the accumulate majority of mass of the SMBH. Mergers of IMBHs with SMBHs throughout the universe are detectable by LISA, at a rate of about two per week.

Simon Portegies Zwart; Holger Baumgardt; Stephen L. W. McMillan; Junichiro Makino; Piet Hut; Toshi Ebisuzaki

2005-12-05T23:59:59.000Z

487

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

488

$J/?$ and $?$ measurements in STAR  

E-Print Network (OSTI)

Heavy-quarkonium states are expected to evidenciate the deconfinement of the nuclear matter into a Quark-Gluon Plasma in heavy-ion collisions. To strive conclusive information from quarkonium production modification in A+A collisions, systematic measurements of the $J/\\psi$ and $\\Upsilon$ states in p+p, d+Au and Au+Au collisions are necessary. To accomplish this mission the STAR experiment has a Quarkonium program based on the development of specific trigger setups that take advantage of the large STAR acceptance. In this work we present the preliminary results of the $J/\\psi$ and $\\Upsilon$ measurement in 200 GeV p+p and the first measurements of $\\Upsilon$ in 200 GeV heavy ion collisions.

Mauro R. Cosentino; for the Star Collaboration

2008-06-02T23:59:59.000Z

489

Massive Stars and their Supernovae  

E-Print Network (OSTI)

Massive stars and their supernovae are prominent sources of radioactive isotopes, the observations of which thus can help to improve our astrophysical models of those. Our understanding of stellar evolution and the final explosive endpoints such as supernovae or hypernovae or gamma-ray bursts relies on the combination of magneto-hydrodynamics, energy generation due to nuclear reactions accompanying composition changes, radiation transport, and thermodynamic properties (such as the equation of state of stellar matter). Nuclear energy production includes all nuclear reactions triggered during stellar evolution and explosive end stages, also among unstable isotopes produced on the way. Radiation transport covers atomic physics (e.g. opacities) for photon transport, but also nuclear physics and neutrino nucleon/nucleus interactions in late phases and core collapse. Here we want to focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis ...

Thielemann, Friedrich-Karl; Liebendrfer, Matthias; Diehl, Roland; 10.1007/978-3-642-12698-7_4

2010-01-01T23:59:59.000Z

490

The Supermassive Black Hole at the Galactic Center  

E-Print Network (OSTI)

The inner few parsecs at the Galactic Center have come under intense scrutiny in recent years, in part due to the exciting broad-band observations of this region, but also because of the growing interest from theorists motivated to study the physics of black hole accretion, magnetized gas dynamics and unusual star formation. The Galactic Center is now known to contain arguably the most compelling supermassive black hole candidate, weighing in at a little over 2.6 million suns. Its interaction with the nearby environment, comprised of clusters of evolved and young stars, a molecular dusty ring, ionized gas streamers, diffuse hot gas, and a hypernova remnant, is providing a wealth of accretion phenomenology and high-energy processes for detailed modeling. In this review, we summarize the latest observational results, and focus on the physical interpretation of the most intriguing object in this region---the compact radio source Sgr A*, thought to be the radiative manifestation of the supermassive black hole.

Fulvio Melia; Heino Falcke

2001-06-08T23:59:59.000Z

491

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

492

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

493

Neutron stars and strange stars in the chiral SU(3) quark mean field model  

E-Print Network (OSTI)

We investigate the equations of state for pure neutron matter and strange hadronic matter in $\\beta$-equilibrium, including $\\Lambda$, $\\Sigma$ and $\\Xi$ hyperons. The masses and radii of pure neutron stars and strange hadronic stars are obtained. For a pure neutron star, the maximum mass is about $1.8 M_{\\mathrm{sun}}$, while for a strange hadronic star, the maximum mass is around $1.45 M_{\\mathrm{sun}}$. The typical radii of pure neutron stars and strange hadronic stars are about 11.0-12.3 km and 10.7-11.7 km, respectively.

P. Wang; S. Lawley; D. B. Leinweber; A. W. Thomas; A. G. Williams

2005-06-06T23:59:59.000Z

494

Magnetic fields in Neutron Stars  

E-Print Network (OSTI)

Isolated neutron stars show a diversity in timing and spectral properties, which has historically led to a classification in different sub-classes. The magnetic field plays a key role in many aspects of the neutron star phenomenology: it regulates the braking torque responsible for their timing properties and, for magnetars, it provides the energy budget for the outburst activity and high quiescent luminosities (usually well above the rotational energy budget). We aim at unifying this observational variety by linking the results of the state-of-the-art 2D magneto-thermal simulations with observational data. The comparison between theory and observations allows to place two strong constraints on the physical properties of the inner crust. First, strong electrical currents must circulate in the crust, rather than in the star core. Second, the innermost part of the crust must be highly resistive, which is in principle in agreement with the presence of a novel phase of matter so-called nuclear pasta phase.

Vigan, Daniele; Miralles, Juan A; Rea, Nanda

2015-01-01T23:59:59.000Z

495

The Evolution of Low Mass Helium Stars towards Supernova Type I Explosion  

E-Print Network (OSTI)

We explore the hypothesis, that helium stars in a certain mass range can evolve to a carbon core explosion similar to what is widely accepted as an explanation for the SN I phenomenon. This should happen when their carbon-oxygen core grows thanks to the helium shell burning above the core. We found that in the mass range of about 1.7-2.2 Msun, indeed this can happen. The main new insight we believe we gained is the crucial importance of an "early" off-center ignition of carbon, which at a later stage prevents the carbon which forms below the helium burning shell and ignites, from burning the carbon all the way to the center. When helium is almost depleted in the convective envelope by the helium burning shell at its bottom, the now super-Chandrasekhar mass carbon-oxygen core contracts, and the residual degenerate carbon at the center is ignited, resulting in a runaway similar to the classical SN I scenario. Since the structure and behavior of the carbon-oxygen core of the helium stars of our interest is very similar to that of a mass accreting carbon-oxygen star, we also thoroughly examined the behavior of carbon-oxygen stars. We discovered that the models which ignite carbon off-center (in the mass range of about 1.05-1.18 Msun, depending on the carbon mass fraction) present an interesting SN I progenitor scenario of their own, since whereas in the standard scenario runaway always takes place at the same density of about 2E9 gr/cm3, in our case, due to the small amount of carbon ignited, we get a whole range of densities from 1E9 up to 6E9 gr/cm3.

Roni Waldman; Zalman Barkat

2006-11-21T23:59:59.000Z

496

Sun-as-a-Star Spectrum Variations 1974-2006  

E-Print Network (OSTI)

We have observed selected Fraunhofer lines, both integrated over the Full Disk and for a small circular region near the center of the solar disk, on 1,215 days for the past 30 years. Full Disk results: Ca II K 393 nm nicely tracks the 11 year magnetic cycle based on sunspot number with a peak amplitude in central intensity of ~37%. The wavelength of the mid-line core absorption feature, called K3, referenced to nearby photospheric Fe, displays an activity cycle variation with an amplitude of 3 milli-Angstroms. Other chromospheric lines track Ca II K intensity with lower relative amplitudes. Low photosphere: Temperature sensitive CI 5380 nm appears constant in intensity to 0.2%. High photosphere: The cores of strong Fe I lines, Na D1 and D2, and the Mg I b lines, present a puzzling signal perhaps indicating a role for the 22 y Hale cycle. Solar minimum around 1985 was clearly seen, but the following minimum in 1996 was missing. This anomalous behavior is not seen in comparison atmospheric O2. Center Disk results: Both Ca II K and C I 538 nm intensities are constant, indicating that the basal quiet atmosphere is unaffected by cycle magnetism within our observational error. A lower limit to the Ca II K central intensity atmosphere is 0.040. The wavelength of Ca II K3 varies with the cycle by 6 milli-Angstroms, a factor of 2X over the full disk value. This may indicate the predominance of radial motions at Center Disk. This is not an effect of motions in plages since they are absent at Center Disk. This 11 y variation in the center of chromospheric lines could complicate the radial velocity detection of planets around solar-type stars. An appendix provides instructions for URL access to both the raw and reduced data.

W. Livingston; L. Wallace; O. R. White; M. S. Giampapa

2006-12-19T23:59:59.000Z

497

MEASUREMENT, MATERIALS & SUSTAINABLE ENVIRONMENT CENTER  

E-Print Network (OSTI)

M2SEC MEASUREMENT, MATERIALS & SUSTAINABLE ENVIRONMENT CENTER #12;#12;M2SEC | The University 66045 MEASUREMENT, MATERIALS & SUSTAINABLE ENVIRONMENT CENTER The Measurement, Materials Sustainable initiative themes of KU's strategic plan, Bold Aspirations: · Sustaining The Planet, Powering The World

498

Council of University Transportation Centers  

E-Print Network (OSTI)

Council of University Transportation Centers 13th Anniversary CUTC Awards Banquet January 9, 2010 Omni Shoreham Hotel Washington, D.C. #12;Council of University Transportation Centers 13th Anniversary Awards Banquet Saturday, January 9, 2010 Welcome Stephen Albert, CUTCVice-President WesternTransportation

Nagurney, Anna

499

Davison Health Center Price List*  

E-Print Network (OSTI)

student account. Please see a Health Center representative for more information. Under the Affordable CareDavison Health Center Price List* Beginning Fall 2013, visits and most services to the Health Act, many of the immunizations and lab tests below are covered by insurance (sexual health testing

Royer, Dana

500

AMHERST CENTER for FUNDAMENTAL INTERACTIONS  

E-Print Network (OSTI)

to harvest solar energy. ENVIRONMENTAL BIOTECHNOLOGY CENTER Develops sustainable technologies for microbial for MASSACHUSETTS BIOFUEL RESEARCH Develops cost-effective technologies to produce ethanol and other alternative with the Massachusetts Division of Marine Fisheries. MASSACHUSETTS CENTER for RENEWABLE SCIENCE and TECHNOLOGY Researches

Schweik, Charles M.