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1

Linda Young of APS Elected Vice Chair of DAMOP  

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

Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award Argonne's Fenter Wins Warren Award for X-ray Diffraction Studies Lahsen Assoufid Elected a Fellow of SPIE 2011 Arthur H. Compton Award Announced by APSUO X-Ray Focusing: Techniques and Applications APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Linda Young of APS Elected Vice Chair of DAMOP JULY 14, 2011 Bookmark and Share Linda Young Argonne Distinguished Fellow and Argonne National Laboratory X-ray Science Division (XSD) Director Linda Young has been elected vice chair of the Division of Atomic, Molecular, and Optical Physics of the American Physical Society (DAMOP). The position became official at the 2011 DAMOP Meeting

2

Art Scene Investigation: Picasso goes Nanotech  

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

Linda Young of APS Elected Vice Chair of DAMOP Linda Young of APS Elected Vice Chair of DAMOP Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award Argonne's Fenter Wins Warren Award for X-ray Diffraction Studies Lahsen Assoufid Elected a Fellow of SPIE 2011 Arthur H. Compton Award Announced by APSUO APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Art Scene Investigation: Picasso goes Nanotech AUGUST 8, 2011 Bookmark and Share Beamline scientist Volker Rose (Argonne National Laboratory) inside the control room [of the nanoprobe x-ray beamline at the APS]. At right, tools of the trade, and our Picasso sample (try to spot the almost invisible white paint chip hanging in the circular hole!) From the Art Institute of Chicago ARTicle blog entry by Francesca Casadio,

3

Clean Cities: Linda Bluestein  

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

Clean Cities: Linda Bluestein on Twitter Bookmark Clean Cities: Linda Bluestein on Google Bookmark Clean Cities: Linda Bluestein on Delicious Rank Clean Cities: Linda Bluestein...

4

Linda Nazar  

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

Nazar Canada Research Chair Department of Chemistry University of Waterloo Linda Nazar is a Professor of Chemistry and Electrical Engineering at the University of Waterloo,...

5

Nanotech/Environment, Health & Safety Portal  

Science Conference Proceedings (OSTI)

NIST Home > Nanotech/Environment, Health & Safety Portal. Nanotech/Environment, Health & Safety Portal. Programs and ...

2013-05-16T23:59:59.000Z

6

Linda Fellers | Y-12 National Security Complex  

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

Linda Fellers Linda Fellers Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake...

7

Linda Snider | Department of Energy  

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

Linda Snider Linda Snider About Us Linda Snider - Deputy Inspector General for Management and Administration Career Highlights Assistant Inspector General for Audit Planning and Administration Senior Auditor, U.S. Army Audit Agency Director for the East/West Regions Team Leader, Washington and Federal Energy Regulatory Commission Audit Groups Linda J. Snider was appointed the Deputy Inspector General for Management and Administration in December 2010. Prior to this she was the Assistant Inspector General for Resource Management. Ms. Snider manages all the administrative and management responsibilities of the Office of Inspector General. She provides oversight, policy direction and implementation of the Office's budget and financial resources, human resources management, space, facilities and equipment

8

From: Alle-Murphy, Linda  

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

Alle-Murphy, Linda Alle-Murphy, Linda Sent: Wednesday, December 28, 2005 9:05 AM To: Mansueti, Lawrence Subject: Re: Order No. 202-05-3 Dear Mr. Mansueti, I am an associate at Schnader Harrison Segal and Lewis, working together with John Britton, who represents the City of Alexandria in the Mirant Power Plant matter. I have a few procedural questions regarding the application for rehearing. According to Section VI.H. of Order No. 202-05-3, applications for rehearing in this matter should be addressed to you. Section VI.H. cites to 16 U.S.C. Section 825(l), which refers to the "Commission" (FERC). I am just seeking to confirm that Section 825(l) also applies to this DOE proceeding. Also, are 10 CFR Section 1003.1 et seq., Office of Hearings and Appeals

9

Women @ Energy: Linda Valerio | Department of Energy  

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

Linda Valerio Linda Valerio Women @ Energy: Linda Valerio March 14, 2013 - 11:04am Addthis Mrs. Linda Valerio is a Mechanical Engineer here at Fermi National Accelerator Laboratory. She specializes in planning, design, and installation of particle accelerator beam line and vacuum systems. Mrs. Linda Valerio is a Mechanical Engineer here at Fermi National Accelerator Laboratory. She specializes in planning, design, and installation of particle accelerator beam line and vacuum systems. Check out other profiles in the Women @ Energy series and share your favorites on Pinterest. Linda Valerio is a Mechanical Engineer at Fermi National Accelerator Laboratory. She specializes in planning, design, and installation of particle accelerator beam line and vacuum systems. She began her employment

10

Google Search Web www.nanotech-now.com  

E-Print Network (OSTI)

Google Search Web www.nanotech-now.com Our NanoNews Digest Sponsors www.pcb123.com Feedback - Ads by Google Home > Press > Researchers bend light through waveguides in colloidal crystals Abstract news from around the world, FREE Full Name Email Address Subscribe Ads by Google Nano News MEMS News

Braun, Paul

11

NREL Melds Nature with Nanotech for Solar-Powered Hydrogen Production...  

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

Melds Nature with Nanotech for Solar-Powered Hydrogen Production NREL researchers are finding ways to mimic photosynthesis by combining enzymes with nanoparticles-particles on the...

12

NWX-NOAA USEC & ADMIN OFFICES Moderator: Linda Belton  

E-Print Network (OSTI)

NWX-NOAA USEC & ADMIN OFFICES Moderator: Linda Belton 08-13-13/2:00 pm CT Confirmation # 1496113-NOAA USEC & ADMIN OFFICES Moderator: Linda Belton August 13, 2013 2:00 pm CT Coordinator: Welcome and thank with the Department of Commerce. Administrative NOAA has assigned NOAA's Office of Legislative #12;NWX-NOAA USEC

13

VWD-0007- In the Matter of Linda D. Gass  

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

This determination will consider a Motion for Discovery filed with the Office of Hearings and Appeals (OHA) by Linda D. Gass. This Motion, dated August 10, 1999, concerns the hearing requested by...

14

VWR-0003- In the Matter of Linda D. Gass  

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

This decision will consider a “Motion to Revive Disclosures Dismissed Prior to the Enactment of Revisions to Part 708” Linda D. Gass filed on March 8, 1999. In her Motion, Ms. Gass requests that I...

15

Linda Young Named to Head X-ray Science Division  

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

to the APS Hard X-ray Nanoprobe Earns an R&D 100 Award Winans of XSD Elected to ACS Fellowship Gluskin of Photon Sciences named Argonne Distinguished Fellow UChicago...

16

NWX-NOAA-USEC & ADMIN OFFICES Moderator: Linda Belton  

E-Print Network (OSTI)

NWX-NOAA-USEC & ADMIN OFFICES Moderator: Linda Belton 07-17-13/2:00 pm CT Confirmation #1496093 for Government-to-Government Consultation with Federally Recognized Indian Tribes and Alaska Natives." NWX-NOAA-USEC and Intergovernmental Affairs, and most recently I've been appointed NOAA's Tribal Liaison. #12;NWX-NOAA-USEC & ADMIN

17

Rio Linda, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Linda, California: Energy Resources Linda, California: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 38.6910138°, -121.4485654° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.6910138,"lon":-121.4485654,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

18

Yorba Linda, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Yorba Linda, California: Energy Resources Yorba Linda, California: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 33.8886259°, -117.8131125° 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":33.8886259,"lon":-117.8131125,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

19

Martin, Mary From: Sent: To: Cc: Subject: Cohn, Linda  

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

Mary Mary From: Sent: To: Cc: Subject: Cohn, Linda Thursday, January 20,201 1 9:00 PM Martin, Mary Ginyard, Irma; Tauber, Alicia ANNUAL NEPA SUMMARY - NEVADA SITE OFFICE Attached is the Annual NEPA Summary for the Nevada Site Office. Please give me a call if you have any questions or need fkther information. Linda M. Cohn, NEPA Compliance Officer National Nuciear Security Administration Nevada Site Office P.O. Box 98518 Las Vegas, NV 89193-8518 702-295-0077 ! Annual NEPA Planning Summary - . - - - - . - - - - - -. - . - . - I Environmental Assessments Ongoing or Expected to be Prepared in the Next 12 Months . - - - -- - - - . -- - ~ .. National Nuclear Security - - Administrafion - Nevada Site Office - . - I -- I Estimated Schedule I Title, Location, Document Number , Estimated Cost

20

Dr Linda Horton | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Information » Dr. Linda Horton Information » Dr. Linda Horton Materials Sciences and Engineering (MSE) Division MSE Home About Staff Listings/Contact Information What's New Research Areas Scientific Highlights Reports and Activities Principal Investigators' Meetings BES Home Staff Listings/Contact Information Dr. Linda Horton Print Text Size: A A A RSS Feeds FeedbackShare Page Dr. Linda Horton Director Materials Sciences and Engineering Division Office of Basic Energy Sciences SC-22.2/Germantown Building, Rm F-411 U.S. Department of Energy 1000 Independence Avenue, SW Washington, D.C. 20585-1290 E-Mail: Linda.Horton@science.doe.gov Phone: (301) 903-7506 Fax: (301) 903-9513 Prior to joining the Department of Energy, Dr. Linda Horton was the Director for the Center for Nanophase Materials Sciences (CNMS) at Oak

Note: This page contains sample records for the topic "nanotech linda young" 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

Dr. Linda G. Blevins | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Linda G. Blevins Linda G. Blevins Deputy Director for Science Programs Deputy Director Home Mission & Functions Deputy Director Biography Organization Staff Presentations & Testimony Federal Advisory Committees Committees of Visitors Contact Information Deputy Director for Science Programs U.S. Department of Energy SC-2/Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 F: (202) 586-4120 E: sc.science@science.doe.gov U.S. Department of Energy SC-2/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-5316 F: (301) 903-7780 E: sc.science@science.doe.gov Staff Dr. Linda G. Blevins Print Text Size: A A A RSS Feeds FeedbackShare Page Dr. Linda G. Blevins Dr. Linda G. Blevins Senior Technical Advisor Office of the Deputy Director for Science Programs

22

Linda Sargent Wood. A More Perfect Union: Holistic Worldviews and the Transformation of American Culture after World War II.  

E-Print Network (OSTI)

23 No. 1 Linda Sargent Wood. A More Perfect Union: HolisticCold War era, Linda Sargent Wood argues that the equallyWorld War II period. For Wood, this cultural perspective

Promnitz, Sarah

2012-01-01T23:59:59.000Z

23

Ms Linda Cerrone | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ms. Linda Cerrone Ms. Linda Cerrone Scientific User Facilities (SUF) Division SUF Home About Staff Listings/Contact Information What's New User Facilities Accelerator & Detector Research & Development Principal Investigators' Meetings Scientific Highlights Construction Projects BES Home Staff Listings/Contact Information Ms. Linda Cerrone Print Text Size: A A A RSS Feeds FeedbackShare Page Cerrone Program Support Specialist Scientific User Facilities Division Office of Basic Energy Sciences SC-22.3/Germantown Building U.S. Department of Energy 1000 Independence Avenue, SW Washington, D.C. 20585-1290 E-Mail: Linda.Cerrone@science.doe.gov Phone: (301) 903-0064 or (301) 903-0065 Fax: (301) 903-1690 Ms. Cerrone worked as administrative support specialist/office manager within the Department of Energy's (DOE's) Office of Independent

24

OSTIblog Posts by Linda McBrearty | OSTI, US Dept of Energy, Office of  

Office of Scientific and Technical Information (OSTI)

Linda McBrearty Linda McBrearty Linda McBrearty's picture Communications and Public Affairs Specialist Communications lead specializing in social media, outreach, promotions, events and fresh collaborations. Experienced professional having worked many years directly with senior level agency management, Congressional staff and corporate industry leaders. 100th DOE R&D Accomplishments Feature Page Celebration DOE R&D Accomplishments 100th Feature Page Published on Jul 08, 2013 DOE R&D Accomplishments is a unique website and database in the OSTI collection. For over 14 years, special Feature pages have been methodically researched and useful information collected on scientists, discoveries, and historical events to include in this searchable resource. It is a rich source of DOE trivia unto itself.

25

Bibliography [1] Linda Allen, Stochastic Processes with Applications to Biology, Pearson, New  

E-Print Network (OSTI)

, Multi-level Monte Carlo for stochas- tically modeled chemical kinetic systems, accepted for publicationBibliography [1] Linda Allen, Stochastic Processes with Applications to Biology, Pearson, New. Kurtz, Continuous time markov chain models for chemical reaction networks, Design and Analysis

Anderson, David F.

26

Linda Milburn  

Science Conference Proceedings (OSTI)

... Employment History: 1988-present: Group Office Assistant, Ceramics Division, NIST 1985-1988: Group Secretary, Metallurgy Division, NIST. ...

2012-10-01T23:59:59.000Z

27

Linda D. Cameron 1 LINDA D. CAMERON  

E-Print Network (OSTI)

, 37-47. Leventhal, E., Easterling, D., Leventhal, H., & Cameron, L. (1995). Conservation of energy of Internal Medicine, 151, 1842- 1847. Love, R., Wiebe, D., Newcomb, P., Cameron, L., Leventhal, H., Jordan, C

Chiao, Raymond

28

Linda L. Gaines resume  

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

L. Gaines L. Gaines Systems Analyst Center for Transportation Research Energy Systems Division Argonne National Laboratory 9700 South Cass Avenue, Bldg. 362 Argonne, IL 60439 phone: 630/252-4919 e-mail: lgaines@anl.gov Professional Experience * Lead analyst for U.S. Department of Energy's heavy vehicle idling studies. * Study costs and impacts on energy use and environment of production and recycling of advanced- design automobiles, trucks, trains, and batteries. * Primary interest is problem solving, which has been applied to efficient use of resources. * Since joining Argonne in 1976, have written handbooks of energy and material flows in petroleum refining, organic chemicals, and copper industries that provided background for reports and papers on technical and institutional issues involved in recycling discarded tires, packaging,

29

YOUNG RESEARCHER SYMPOSIUM  

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

2 BROOKHAVEN NATIONAL LABORATORY CALL FOR PAPERS YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG...

30

YOUNG RESEARCHER SYMPOSIUM  

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

3 BROOKHAVEN NATIONAL LABORATORY CALL FOR PAPERS YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG...

31

Argonne Breaks Ground on $34.5M MX Research Facility  

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

Stephenson Appointed ALD for Photon Sciences Stephenson Appointed ALD for Photon Sciences APS, Other DOE Labs Help Develop New Cancer Fighting Drug Paper on Fast Pharmaceuticals by APS Authors Featured in New Journal Art Scene Investigation: Picasso goes Nanotech Linda Young of APS Elected Vice Chair of DAMOP APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Argonne Breaks Ground on $34.5M MX Research Facility SEPTEMBER 15, 2011 Bookmark and Share Artist's rendering of the Advanced Protein Crystallization Facility (left in drawing). The Advanced Photon Source experiment hall is at right. The U.S. Department of Energy's (DOE's) Argonne National Laboratory broke ground on August 30, 2011, for a $34.5 million Advanced Protein

32

Stephenson Appointed ALD for Photon Sciences  

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

APS, Other DOE Labs Help Develop New Cancer Fighting Drug APS, Other DOE Labs Help Develop New Cancer Fighting Drug Paper on Fast Pharmaceuticals by APS Authors Featured in New Journal Art Scene Investigation: Picasso goes Nanotech Linda Young of APS Elected Vice Chair of DAMOP Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Stephenson Appointed ALD for Photon Sciences SEPTEMBER 7, 2011 Bookmark and Share Brian Stephenson Argonne National Laboratory Director Eric D. Isaacs announced today that Brian Stephenson has been appointed Associate Laboratory Director (ALD) for Photon Sciences, effective September 1, 2011. The directorate comprises three research and support divisions centered on Argonne's

33

Young Leaders Professional Development Award  

Science Conference Proceedings (OSTI)

YOUNG PROFESSIONAL LINKS. YOUNG PROFESSIONALS HOME [MORE]; YL INTERNATIONAL SCHOLAR AWARD Learn about the international scholar ...

34

Nanotech/Environment, Health & Safety News  

Science Conference Proceedings (OSTI)

... for numerous applications—small as a ... in the Home: More and Smaller Than Previously ... nanoparticles emitted by common household appliances. ...

2010-08-19T23:59:59.000Z

35

NIST, UM Program To Support Nanotech Development  

Science Conference Proceedings (OSTI)

... National Institute of Standards and Technology (NIST) and the University of Maryland (UM) have joined in a $1.5 million cooperative program that ...

2013-08-13T23:59:59.000Z

36

Young Researcher Symposium 2013  

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

Brookhaven National Laboratory Young Researcher Symposium 2013 Homepage Registration Talks Program Abstract Submission Sponsors Feedback Contact Us Symposium Information pulldown...

37

Controlling the Inner Electron Dance  

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

2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Controlling the Inner Electron Dance JANUARY 9, 2012 Bookmark and Share Linda Young Linda Young, Director of the...

38

Linda Collins Director Lynelle Gehrke Associate Director  

E-Print Network (OSTI)

the correct Sponsor, please call the main line X43330 Please enter the correct Sponsor Deadline date if known) working days prior to the sponsor's published deadline 8am five (5) working with University and sponsor requirements #12;Checklists and Helpful Tools (live links) http

Tsien, Roger Y.

39

M. Paul Scott Linda M. Pollak  

E-Print Network (OSTI)

dam- age, but this tool would be lost if insects develop resis- tance to the Bt toxin. Thus far be carried by gravity and wind to the silk. A consequence of this process is that it is difficult to ensure

Scott, Paul

40

Young Scientist Research Award  

Science Conference Proceedings (OSTI)

Recognizing substantial research contributions by someone 36 years of age or younger. Young Scientist Research Award Divisions achievement agricultural analytical application award awards biotechnology detergents distinguished division Divisions

Note: This page contains sample records for the topic "nanotech linda young" 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

2013 Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM  

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

Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM 2013 BROOKHAVEN NATIONAL LABORATORY NOVEMBER 15, 2013 YRS LETTER FROM THE ORGANIZERS 2013 Dear Guest, Welcome...

42

Steve Young | Data.gov  

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

Steve Young Primary tabs View(active tab) Track Communities: Energy Display Name: Steve Young History Member for 1 year 1 week...

43

SSA Young Aspen Site  

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

Site (SSA-YA) The pole-tower at the YA site Closer look at the pole-tower at the YA site Solar panels powering the site, mounted on a folding ladder The young aspen canopy...

44

Jun-Young Choi  

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

Jun-Young Choi Korea Testing Laboratory NOTICE Due to the current lapse of federal funding, Berkeley Lab websites are accessible, but may not be updated until Congress approves...

45

Young Leaders Committee Bylaws  

Science Conference Proceedings (OSTI)

The vice chair is to be selected by the current chair/vice chair from Young Professionals who wish to serve in this capacity who have indicated a willingness to do ...

46

Won Young Park  

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

Won Park Won Park Won Young Park International Energy Studies Group Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 90R2002 Berkeley CA 94720 Office Location: 90-2144 (510) 495-2252 WYPark@lbl.gov Won Young Park is a senior research associate at Lawrence Berkeley National Laboratory (LBNL). He is working on technical analysis for televisions, computer monitors, and lighting for the Super-efficient Equipment and Appliance Deployment (SEAD) Initiative. In the studies, he assesses energy savings potential in efficiency improvement options, evaluates cost effectiveness of key technologies, and provides technical information and recommendations for policies and programs designed to accelerate the adoption of efficient technologies. He also supports a Korea project that

47

NREL: Energy Analysis - Katherine Young  

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

Katherine Young, P.E. Katherine Young, P.E. Photo of Katherine Young Katherine Young is a member of the Technology Systems and Sustainability Analysis Group in the Strategic Energy Analysis Center. Geothermal Energy Engineer On staff since June 2008 Phone number: 303-384-7402 E-mail: katherine.young@nrel.gov Areas of expertise Geothermal planning and opportunities Database planning and development Primary research interests Geothermal and hydroelectric energy opportunities U.S. DOE Geothermal Program Information Education and background training Continuing Education at University of Colorado in Boulder and Denver Groundwater modeling Quantitative methods in water resource engineering Water resource engineering and management Independent study in groundwater hydrology M.S. in geochemistry and isotope geology, 2002, University of

48

Young Americans | Department of Energy  

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

Young Americans Young Americans Young Americans Competitions 2013 EcoCar2 Challenge Primary Ed DOE 2013 National Science Bowl Primary Ed DOE Challenge Home Student Design University EERE 2013 National Clean Energy Business Plan University EERE 2013 Solar Decathlon University EERE/DOE 2013 National Collegiate Wind University DOE Better Buildings University DOE Energy Challenge University DOE Georgetown University Energy Prize University Georgetown Univ. P3: People, Prosperitym and the Planet University EPA National Clean Energy Business Plan University DOE National Geothermal Student University ORISE Hydrogen and Fuel Cell Competitions University NREL H2U Student Contest University HEF American Solar Challenge University ASC

49

NERSC/DOE FES Requirements Workshop Worksheet - Linda Sugiyama  

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

at least 4X higher, radial grid on the order of half the thermal ion gyroradius). Extension of the physics of the MHD plasma model will become a major focus over the next 3-5...

50

SHOP SMART Linda Dai & Wilfred Dang WHAT DO YOU BUY?  

E-Print Network (OSTI)

expensive and usually high in fat and salt. Vegetables and Fruit 7 - 10 Best Buys: apples, bananas, eggs, hamburger, blade or rump roast, canned tuna and or frozen fish. Chicken legs and thighs rather than breasts Ground turkey and chicken. Trail Mix Try meals that don't have meat a few times each week

Thompson, Michael

51

MIKE TURNER ON SPOTTING YOUNG  

E-Print Network (OSTI)

BAE SYSTEMS MIKE TURNER ON SPOTTING YOUNG TALENT AND THE GROWTH OF HIS BUSINESS Success stories? Surely, it is about making lots of money, gaining power, status and prestige, and then using this wealth, the extinction of many animal and plant species, and global warming demonstrated that the raw materials

52

Feeding Young Horses For Sound Development  

E-Print Network (OSTI)

Horse owners must decide whether their young horses will be fed for moderate or rapid growth. One concern is the occurrence of bone and joint disorders in young horses that develop rapidly. Research has shown that this and other problems can be decreased by ensuring that young horses receive proper nutrition. Specific recommendations are included for creep feeding foals and for feeding weanlings and yearlings. Nutritional levels are discussed in relation to the amount of exercise young horses receive.

Gibbs, Pete G.; Potter, Gary D.

2005-05-25T23:59:59.000Z

53

The Newsletter of the TMS Young Leaders Committee RESEARCH ...  

Science Conference Proceedings (OSTI)

Volume 3, Number 1. The Newsletter of the TMS Young Leaders Committee. RESEARCH, EXCHANGE, AND EXPLORATION: THE YOUNG LEADER ...

54

October The Young Leader.indd  

Science Conference Proceedings (OSTI)

The award includes a $500 stipend from the Ford Motor Company and is open exclusively ... for young professionals in the oil and gas industry. In May, Csontos.

55

2013 Young Leader Meet the Candidate Poster Session  

Science Conference Proceedings (OSTI)

Jan 15, 2013... Young Leader Meet the Candidate Poster Session. Sponsorship, TMS: Young Leaders Committee. Organizer(s), Kinga A. Unocic, ORNL

56

Young Energy, LLC | Open Energy Information  

Open Energy Info (EERE)

Young Energy, LLC Place Texas Utility Id 56248 Utility Location Yes Ownership R NERC ERCOT Yes ISO Ercot Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data...

57

Hopf Structures on Standard Young Tableaux  

SciTech Connect

We review the Poirier-Reutenauer Hopf structure on Standard Young Tableaux and show that it is a distinguished member of a family of Hopf structures. The family in question is related to deformed parastatistics.

Loday, Jean-Louis [IRMA, CNRS and Univ. Strasbourg, 7 rue Descartes, 67084 Strasbourg (France); Popov, Todor [INRNE, BAS, 72 Tsarigradsko Chaussee, 1784 Sofia (Bulgaria)

2010-06-17T23:59:59.000Z

58

2008 Rosalind Franklin Young Investigator Award  

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

The 2008 3-Way Meeting The 2008 3-Way Meeting In R&D, Super X-rays Mark Many Spots A New Gas Loading System for Diamond Anvil Cells at GSECARS Sidorowicz Named "Supervisor of the Year" SESS 2007: The School for Environmental Sciences with Synchrotrons APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed 2008 Rosalind Franklin Young Investigator Award APRIL 24, 2008 Bookmark and Share Oleg Shpyrko The Advanced Photon Source (APS) Users Organization has named Oleg G. Shpyrko of the University of California, San Diego, as the recipient of the 2008 Rosalind Franklin Young Investigator Award. The award recognizes an important technical or scientific accomplishment by a young investigator that depended on, or is beneficial to, the APS. Shpyrko will receive the

59

APSUO Announces Rosalind Franklin Young Investigator Award  

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

APSUO Announces Rosalind Franklin Young Investigator Award APSUO Announces Rosalind Franklin Young Investigator Award In conjunction with the Advanced Photon Source (APS), the APS Users Organization (APSUO) has established the APSUO Rosalind Franklin Young Investigator Award. The nomination deadline for this award is March 15, 2004. The award will be presented at the 2004 Users Meeting for the Advanced Photon Source, held at Argonne on May 3-6, 2004. Rosalind Franklin Born in 1920, Rosalind Franklin graduated from Cambridge University in 1941 in time to focus on a wartime problem: the composition of coal and charcoal and how to use them most efficiently. She published five papers on the subject before she was 26 years old, work that is still quoted today, and helped launch the field of high-strength carbon fibers. When Franklin had

60

Neural processes supporting young and older adults' emotional memories  

Science Conference Proceedings (OSTI)

Young and older adults are more likely to remember emotional information than neutral information. The present functional magnetic resonance imaging study examined the neural processes supporting young (ages 18--35) and older (ages 62--79) adults' successful ...

Elizabeth A. Kensinger; Daniel L. Schacter

2008-07-01T23:59:59.000Z

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61

Mi-Young Kim - Research Staff - FEERC  

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

Mi-Young Kim Mi-Young Kim Post Doctoral Research Associate (F) 865-946-1354 kimm@ornl.gov Professional Highlights Education Ph.D., Applied Chemical Engineering, Chonnam National University, 2008 Miyoung joined the Oak Ridge National Laboratory (ORNL) as a post-doctoral researcher in 2010. She has worked at the Center for Development of Fine Chemicals and the Research Institute for Catalysis in Chonnam National University prior to joining the ORNL. Her research background is in heterogeneous catalysis and highly dispersed noble metal catalysts. She has extensive experience in characterizing catalysts using EXAFS, XPS, XRD, solid NMR and ESR. She is currently involved in automotive catalysis research with an emphasis on monolithic catalysts & materials relevant to lean NOx and cold start emissions controls

62

Women @ Energy: Young-Kee Kim | Department of Energy  

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

Young-Kee Kim Young-Kee Kim Women @ Energy: Young-Kee Kim March 19, 2013 - 3:37pm Addthis Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago Check out other profiles in the Women @ Energy series and share your favorites on Pinterest. Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago. As an experimental particle physicist, Young-Kee's research focuses on understanding the origin of mass for fundamental particles. Since July 2006, she has served as Deputy Director of Fermi National

63

NREL Melds Nature with Nanotech for Solar-Powered Hydrogen Production (Fact Sheet)  

SciTech Connect

NREL researchers are finding ways to mimic photosynthesis by combining enzymes with nanoparticles - particles on the scale of a billionth of a meter - to produce hydrogen directly from water and sunlight. This breakthrough project began in 2008 with scientists and researchers asking how they might learn from nature and develop a synthetic process that is more efficient than plants at converting sunlight to hydrogen. The goal was to find a new way to produce hydrogen that could then be commercialized inexpensively for fuel cells and other uses. Among the various approaches to making hydrogen, the NREL researchers wondered about a hybrid molecular assembly that might pair the best natural molecule with a synthesized nanoparticle. Researchers looked at using hydrogenase enzymes as one part of the equation. These biological catalysts can convert electrons and protons into hydrogen gas, or convert hydrogen into electrons and protons. The choice seemed worthwhile because the hydrogenase enzyme has some intriguing properties: a high substrate selectivity, meaning a very high preference for catalyzing reactions with protons rather than with other atoms and molecules; and fast turnover, which enables it to produce a hydrogen molecule in milliseconds.

Not Available

2011-09-01T23:59:59.000Z

64

TMS Young Leaders Committee Materials Week '97 Meeting Minutes  

Science Conference Proceedings (OSTI)

Sep 14, 1997 ... Each attendee participated in one of the focus groups established to focus on directives and goals of the Young Leaders Committee.

65

Combinatorics of Arc Diagrams, Ferrers Fillings, Young ... - CECM  

E-Print Network (OSTI)

Jul 22, 2009 ... I Generalization of permutation matrices: fill each row & column of a Ferrers shape ... Standard Young Tableaux. Arc Diagrams,. Nesting and.

66

New Directions in Gender and Sexuality Studies: Gayatri Chakravorty Spivak, Rebecca Jordan-Young, and Alondra Nelson Will Be Featured in Winter Quarter  

E-Print Network (OSTI)

Chakravorty Spivak, Rebecca Jordan-Young, and Alondra NelsonUniversity, Rebecca Jordan-Young, Associate Professor ofan embarrassment. Rebecca Jordan-Young Rebecca Jordan-Young

McLean, Lindsey; Johnson, Jane’a

2011-01-01T23:59:59.000Z

67

Computer game design and the imaginative play of young children  

Science Conference Proceedings (OSTI)

This paper discusses preliminary findings of the study of computer game design in relation to current understanding of imaginative play and its developmental value for young children. The crucial role of children's play in their development is well documented. ... Keywords: child development, computer games, design criteria, imaginative play, young children

Irina Verenikina; Jan Herrington

2009-06-01T23:59:59.000Z

68

HOW TO FIND YOUNG MASSIVE CLUSTER PROGENITORS  

SciTech Connect

We propose that bound, young massive stellar clusters form from dense clouds that have escape speeds greater than the sound speed in photo-ionized gas. In these clumps, radiative feedback in the form of gas ionization is bottled up, enabling star formation to proceed to sufficiently high efficiency so that the resulting star cluster remains bound even after gas removal. We estimate the observable properties of the massive proto-clusters (MPCs) for existing Galactic plane surveys and suggest how they may be sought in recent and upcoming extragalactic observations. These surveys will potentially provide a significant sample of MPC candidates that will allow us to better understand extreme star-formation and massive cluster formation in the Local Universe.

Bressert, E.; Longmore, S.; Testi, L. [European Southern Observatory, Karl Schwarzschild Str. 2, D-85748 Garching bei Muenchen (Germany); Ginsburg, A.; Bally, J.; Battersby, C. [Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309 (United States)

2012-10-20T23:59:59.000Z

69

EA-1974: Wallooskee-Youngs Confluence Restoration Project, Clatsop County,  

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

4: Wallooskee-Youngs Confluence Restoration Project, Clatsop 4: Wallooskee-Youngs Confluence Restoration Project, Clatsop County, Oregon EA-1974: Wallooskee-Youngs Confluence Restoration Project, Clatsop County, Oregon Summary Bonneville Power Administration is preparing an EA to assess the potential environmental impacts of the proposed restoration of a tidal marsh in the Columbia River Estuary, near Astoria in Clatsop County, Oregon. The project website is https://www.bpa.gov/goto/WallooskeeYoungs. Public Comment Opportunities Comments on the scope of the EA should be marked "Wallooskee-Youngs Confluence Restoration Project" and submitted by January 27, 2014, by one of the methods listed below. Comments will be posted in their entirety on BPA's website at www.bpa.gov/comments. Toll-free phone: 800-622-4519

70

Brigham Young University, Brigham Young University--Hawaii, BYU--Idaho, and LDS Business College exist to provide an  

E-Print Network (OSTI)

Brigham Young University, Brigham Young University--Hawaii, BYU--Idaho, and LDS Business College, and student body at BYU, BYU-- Hawaii, BYU--Idaho, and LDSBC are selected and retained from among those who represent BYU, BYU--Hawaii, BYU--Idaho, and LDSBC are to maintain the highest standards of honor, integrity

Hart, Gus

71

Nonproliferation Graduate Fellowship Program Attracts High Caliber Young  

National Nuclear Security Administration (NNSA)

Graduate Fellowship Program Attracts High Caliber Young Graduate Fellowship Program Attracts High Caliber Young Professionals to Careers in Nonproliferation and National Security | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > NNSA Blog > Nonproliferation Graduate Fellowship Program Attracts High Caliber ... Nonproliferation Graduate Fellowship Program Attracts High Caliber Young

72

Development of Convective Systems over Baja California during Tropical Cyclone Linda (2003)  

Science Conference Proceedings (OSTI)

Characteristics of the life cycle and motion of convective systems that occurred over the Baja California Peninsula were determined from a case study in September of 2003. This note applies data from satellite imagery, regular observations from ...

Luis M. Farfán

2005-10-01T23:59:59.000Z

73

Computational Science and EngineeringComputational Science and Engineering Linda Petzold  

E-Print Network (OSTI)

-Scale Computer Simulation Methods Ã? Practical High-Performance Computing Internship: Our industry (McMeeking, Fredrickson) Ã? Ferroelectric ceramics Ã? Ceramic Composites Computational Systems Biology

Bigelow, Stephen

74

Prioritizing Burn-Injured Patients During a Disaster Carri W. Chan, Linda V. Green, Yina Lu  

E-Print Network (OSTI)

York City, this corresponds to 400 patients. There are currently 140 burn beds in the region which can on September 11, 2001, the US government initiated the development of disaster plans for resource allocation, Bravata et al. 2006). In the event of a nuclear attack, guidance is needed on whether people should

Chan, Carri W.

75

Bioconversion and Biorefineries of the Future Linda L. Lasure, Pacific Northwest National Laboratory  

E-Print Network (OSTI)

of corn stover as a sustainable feedstock for bioethanol production" Bioresource Technology 88, p15-25 Lal

76

Linda York, M.S.R.D. MAINTAINING NUTRITIONAL STATUS IN PATIENTS  

E-Print Network (OSTI)

for no salt adobo, jerk seasoning and other spices. (www.penzeys.com) Instead of salt, pair chicken: Nausea and Anorexia Small low fat frequent meals with Enlive. Depression Meds, yoga, socialization

Oliver, Douglas L.

77

10/17/2005 10:02 AM LINDA HOWELL HARDESTY  

E-Print Network (OSTI)

and Fisheries Management, University of Idaho. 1974. PROFESSIONAL EXPERIENCE Associate Professor, Range affiliate faculty in Department of Range Resources, University of Idaho 1990 appointed as adjunct faculty, Idaho Department of Lands, Boise and Gooding, Idaho. 1977-1980. Administered leasing of state lands

78

Start-up Optimization of a Combined Cycle Power Plant A. Linda, E. Sllberga,  

E-Print Network (OSTI)

bModelon AB, Lund, Sweden cSiemens AG, Energy Sector, Erlangen, Germany Abstract In the electricity market of today, with increasing de- mand for electricity production on short notice, the combined cycle to opti- mize are explored. Results are encouraging and show that energy production during start-up can

79

Application for Presidential Permit OE Docket No. PP-371 Northern Pass Transmission: Comments from Linda Upham  

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

Application from Northern Pass Transmission to construct, operate and maintain electric transmission facilities at the U.S. - Canada Border.

80

Research drilling in young silicic volcanoes  

DOE Green Energy (OSTI)

Magmatic activity, and particularly silicic magmatic activity, is the fundamental process by which continental crust forms and evolves. The transport of magma from deep crustal reservoirs to the surface is a neglected but important aspect of magmatic phenomena. It encompasses problems of eruptive behavior, hydrothermal circulation, and ore deposition, and must be understood in order to properly interpret deeper processes. Drilling provides a means for determining the relationship of shallow intrusive processes to eruption processes at young volcanoes where eruptions are best understood. Drilling also provides a means for directly observing the processes of heat and mass transfer by which recently emplaced intrusions approach equilibrium with their new environment. Drilling in the Inyo Chain, a 600-year-old chain of volcanic vents in California, has shown the close relationship of silicic eruption to shallow dike emplacement, the control of eruptive style by shallow porous-flow degassing, the origin of obsidian by welding, the development of igneous zonation by viscosity segregation, and the character and size of conduits in relation to well-understood magmatic and phreatic eruptions. 36 refs., 9 figs.

Eichelberger, J.C.

1989-06-30T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" from the National Library of EnergyBeta (NLEBeta).
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they are not comprehensive nor are they the most current set.
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to obtain the most current and comprehensive results.


81

The Young Open Cluster NGC 2129  

E-Print Network (OSTI)

The first CCD UBV(RI) photometric study in the area of the doubtful open cluster NGC 2129 is presented. Photometry of a field offset 15 arcmin northward is also provided, to probe the Galactic disk population toward the cluster. Using star counts, proper motions from the UCAC2 catalog, colour-magnitude and colour-colour diagrams we demonstrate that NGC 2129 is a young open cluster. The cluster radius is 2.5 arcmin, and across this region we find evidence of significant differential reddening, although the reddening law seems to be normal toward its direction. Updated estimates of the cluster fundamental parameters are provided. The mean reddening is found to be E(B-V)=0.80$\\pm$0.08 and the distance modulus is $(m-M)_o$= 11.70$\\pm0.30$. Hence, NGC 2129 is located at 2.2$\\pm$0.2 kpc from the Sun inside the Local spiral arm. The age derived from 37 photometrically selected members is estimated to be approximately 10 million years. These stars are used to provide new estimates of the cluster absolute proper motion components.

Giovanni Carraro; Brian Chaboyer; James Perencevich

2005-10-19T23:59:59.000Z

82

Young Scientist Research Award – The award recognizes a scienti  

Science Conference Proceedings (OSTI)

Young Scientist Research Award The award recognizes a scientist who has made a significant and substantial research contribution in one of the areas represented by the Divisions of AOCS.

83

Hanford Grows Young Minds Through Site Tours | Department of Energy  

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

Hanford Grows Young Minds Through Site Tours Hanford Grows Young Minds Through Site Tours Hanford Grows Young Minds Through Site Tours June 3, 2013 - 12:00pm Addthis John Britton, with Office of River Protection contractor Washington River Protection Solutions, explains the Hanford tank waste program to Western Washington University students in a recent tour of the Hanford site. John Britton, with Office of River Protection contractor Washington River Protection Solutions, explains the Hanford tank waste program to Western Washington University students in a recent tour of the Hanford site. RICHLAND, Wash. - It is harvest season for cherries, raspberries and rhubarb in Washington state. But employees at the Hanford site are helping grow the young minds of the nation's future science, technology,

84

Using computer-based testing with young children  

Science Conference Proceedings (OSTI)

In this era of increased accountability in education, there is a need for tools to use in assessing the abilities and instructional levels of young children. Computers have been used successfully to assess older children and adults. However, ...

Susan Kubic Barnes / J. Christine Harmes

2010-01-01T23:59:59.000Z

85

Trends in the Health of Young Children in California  

E-Print Network (OSTI)

Research Brief October 2008 Trends in the Health of YoungThis brief examines trends in key health indicators forpoints (Exhibit 2). This trend has kept the overall health

Grant, David; Kurosky, Samantha

2008-01-01T23:59:59.000Z

86

Wave Breaking Dissipation in a Young Wind Sea  

Science Conference Proceedings (OSTI)

Coupled in situ and remote sensing measurements of young, strongly-forced, wind waves are applied to assess the role of breaking in an evolving wavefield. In situ measurements of turbulent energy dissipation from wave-following “SWIFT” drifters ...

Michael Schwendeman; Jim Thomson; Johannes R. Gemmrich

87

The Martin Boundary Of The Young-Fibonacci Lattice  

E-Print Network (OSTI)

In this paper we find the Martin boundary for the Young-Fibonacci lattice YF. Along with the lattice of Young diagrams, this is the most interesting example of a differential partially ordered set. The Martin boundary construction provides an explicit Poisson-type integral representation of non-negative harmonic functions on YF. The latter are in a canonical correspondence with a set of traces on Okada locally semisimple algebra.

Frederick M. Goodman; Sergei V. Kerov

1997-01-01T23:59:59.000Z

88

Lithium: Measurement of Young's Modulus and Yield Strength  

Science Conference Proceedings (OSTI)

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

Ryan P Schultz

2002-11-07T23:59:59.000Z

89

Calling all Young Entrepreneurs: Deadline for Energy Department Business  

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

Calling all Young Entrepreneurs: Deadline for Energy Department Calling all Young Entrepreneurs: Deadline for Energy Department Business Plan Competition Approaching Calling all Young Entrepreneurs: Deadline for Energy Department Business Plan Competition Approaching December 1, 2011 - 12:08pm Addthis If you’re a university student interested in low-carbon technologies and entrepreneurship, then this is the premier opportunity for you to pitch your idea. The Regional Clean Energy Business Plan Competition is accepting business plan submissions from today until March 2, 2012. If you're a university student interested in low-carbon technologies and entrepreneurship, then this is the premier opportunity for you to pitch your idea. The Regional Clean Energy Business Plan Competition is accepting business plan submissions from today until March 2, 2012.

90

Why Has Home Ownership Fallen Among the Young? ?  

E-Print Network (OSTI)

We document that home ownership of households with “heads ” aged 25– 44 years fell substantially between 1980 and 2000 and recovered only partially during the 2001–2005 housing boom. The 1980–2000 decline in young home ownership occurred as improvements in mortgage opportunities made it easier to purchase a home. This paper uses an equilibrium life-cycle model calibrated to micro and macro evidence to understand why young home ownership fell over a period when it became easier to own a home. Our findings indicate that a trend toward marrying later and the increase in household earnings risk that occurred after 1980 account for 3/5 to 4/5 of the decline in young home ownership.

Jonas D. M. Fisher; Martin Gervais

2009-01-01T23:59:59.000Z

91

Duck Young Chung - Argonne National Laboratories, Materials Sicence  

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

EM > Duck Young Chung EM > Duck Young Chung Duck Young Chung Principal Materials Engineer Bldg. 223, C-233 Phone: 630-252-4907 This e-mail address is being protected from spambots. You need JavaScript enabled to view it. Biography Duck Young Chung is a staff scientist in the Emerging Materials Group. After receiving his B.A. from DanKook University in 1984, M.S. and Ph.D from Kyungpook National University in 1991, he joined the group of Prof. Kanatzidis as a postdoc at Michigan State University in 1992 where later he became a research faculty, then moved to Argonne in 2006. His expertise includes exploratory synthesis, crystal growth, and characterization of a wide variety of bulk materials as well as development of synthesis techniques and methods in the areas of chalcogenides, pnictides, and intermetallic alloys for thermoelectrics, superconductivity, topological insulators, and semiconducting materials with interesting electronic or magnetic properties. He is the author of 80 peer-reviewed articles and patents published. Notable achievements include discovery of high performance thermoelectric semiconductor, CsBi4Te6, which holds the record of figure of merit for low temperature cooling applications (Science, 2000) and synthesis of an unconventional superconductors Ba1-xKxFe2As2 characterized by inelastic neutron scattering (Nature, 2008).

92

THE FORMATION OF YOUNG DENSE STAR CLUSTERS THROUGH MERGERS  

SciTech Connect

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

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

2012-07-01T23:59:59.000Z

93

Young children's ability to use a computer mouse  

Science Conference Proceedings (OSTI)

Because there is little empirical data available on how well young children are able to use a computer mouse, the present study examined their proficiency in clicking on small objects at various positions on the screen and their skill in moving objects ... Keywords: Elementary education, Human-computer interaction, Interface, Media in education, Navigation

Afke Donker; Pieter Reitsma

2007-05-01T23:59:59.000Z

94

Young modulus dependence of nanoscopic friction coefficient in hard coatings  

E-Print Network (OSTI)

with miniature moving parts, such as micro- electromechanical systems and hard-disk drives.1,2 A betterYoung modulus dependence of nanoscopic friction coefficient in hard coatings Elisa Riedoa with varying hardness obtained by different growth temperatures. For the CrN films, we show that the changes

Brune, Harald

95

Young children's computer skills development from kindergarten to third grade  

Science Conference Proceedings (OSTI)

This investigation explores young children's computer skills development from kindergarten to third grade using the Early Childhood Longitudinal Study-Kindergarten (ECLS-K) dataset. The sample size of the study was 8642 children. Latent growth curve ... Keywords: Computer skills, Kindergarten, Latent growth curve modeling

Mesut Saçkes; Kathy Cabe Trundle; Randy L. Bell

2011-09-01T23:59:59.000Z

96

Binary populations and stellar dynamics in young clusters  

E-Print Network (OSTI)

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (unconventionally formed objects) like intermediate mass black holes, Eta Carinae, Zeta Puppis, Gamma Velorum and WR 140.

D. Vanbeveren; H. Belkus; J. Van Bever; N. Mennekens

2008-01-17T23:59:59.000Z

97

Binary populations and stellar dynamics in young clusters  

E-Print Network (OSTI)

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (unconventionally formed objects) like intermediate mass black holes, Eta Carinae, Zeta Puppis, Gamma Velorum and WR 140.

Vanbeveren, D; Van Bever, J; Mennekens, N

2008-01-01T23:59:59.000Z

98

The Paleo Project - Fossil, Oregon by Jenny Young, Rowell Brokaw Architects [EDRA/Places Awards 2006 -- Planning  

E-Print Network (OSTI)

courtesy of Rowell Brokaw Architects. Top: Construction ofYoung, Rowell Brokaw Architects In an economically bypassedYoung and Rowell Brokaw Architects / Paleo Project 2006

Moffat, David

2006-01-01T23:59:59.000Z

99

Proceedings Fourth European Young Researchers Workshop on Service Oriented Computing  

E-Print Network (OSTI)

Service-Oriented Computing (SOC) is an emerging new paradigm for distributed and object-oriented computing by allowing autonomous, platform-independent computational entities (called services) to be built (described, discovered, composed, orchestrated) within and across organizational boundaries. Like no other computing paradigm before, SOC is destined to exert a lasting influence on the business domain, among others (e-commerce, e-government, e-business, e-learning, e-health, etc.). The Young Researchers workshop series on Service-Oriented Computing is meant to be a platform for junior researchers from industry and academics alike. Its core objectives are to exchange information regarding advancements in the state of the art and practice of SOC, as well as to identify emerging research topics and the future trends in this domain. Following the success of the previous three workshops, the 4th European Young Researchers Workshop on Service-Oriented Computing (YR-SOC 2009) introduced two novelties: it was organ...

ter Beek, Maurice H

2009-01-01T23:59:59.000Z

100

No evidence for mass segregation in young clusters  

E-Print Network (OSTI)

Aims. We investigate the validity of mass segregation indicators commonly used in the analysis of young stellar clusters. Methods. We simulate observations by constructing synthetic seeing limited images of a 1000 massive clusters (10^4 Msun) with a standard IMF and a King density distribution function. Results. We find that commonly used indicators are highly sensitive to sample incompleteness in observational data, and that radial completeness determinations do not provide satisfactory corrections, rendering the studies of radial properties highly uncertain. On the other hand, we find that under certain conditions, the global completeness can be estimated accurately, allowing for the correction of the global luminosity and mass functions of the cluster. Conclusions. We argue that there is currently no observational evidence for mass segregation in young compact clusters since there is not a robust way to differentiate between true mass segregation and sample incompleteness effects. Caution should then be ex...

Ascenso, J; Lago, M T V T

2008-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" 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

Young Professionals in Nuclear Industry Group Forms at Savannah River Site  

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

Young Professionals in Nuclear Industry Group Forms at Savannah Young Professionals in Nuclear Industry Group Forms at Savannah River Site Young Professionals in Nuclear Industry Group Forms at Savannah River Site January 1, 2012 - 12:00pm Addthis The Savannah River Chapter of North American – Young Generation in Nuclear is a new group forming at the Savannah River Site. The Savannah River Chapter of North American - Young Generation in Nuclear is a new group forming at the Savannah River Site. AIKEN, S.C. - Supporting the development of young nuclear professionals in the Central Savannah River Area (CSRA) is the purpose behind a new group forming at the Savannah River Site (SRS). The Savannah River Chapter of North American - Young Generation in Nuclear (SR-YGN) will hold a kick-off meeting Jan. 26 in Aiken and all

102

Warming mineralises young and old soil carbon equally  

E-Print Network (OSTI)

Abstract. The temperature sensitivity of soil organic carbon decomposition is critical for predicting future climate change because soils store 2-3 times the amount of atmospheric carbon. Of particular controversy is the question, whether temperature sensitivity differs between young or labile and old or more stable carbon pools. Ambiguities in experimental methodology have so far limited corroboration of any particular hypothesis. Here, we show in a clear-cut approach that differences in temperature sensitivity between young and old carbon are negligible. Using the change in stable isotope composition in transitional systems from C3 to C4 vegetation, we were able to directly distinguish the temperature sensitivity of carbon differing several decades in age. This method had several advantages over previously followed approaches. It allowed to identify release of much older carbon, avoided un-natural conditions of long-term incubations and did not require arguable curve-fitting. Our results demonstrate that feedbacks of the carbon cycle on climate change are driven equally by young and old soil organic carbon. 1

F. Conen; J. Leifeld; B. Seth; C. Alewell

2006-01-01T23:59:59.000Z

103

Mission of ITER and Challenges for the Young  

Science Conference Proceedings (OSTI)

It is recognized that the ongoing effort to provide sufficient energy for the wellbeing of the globe's population and to power the world economy is of the greatest importance. ITER is a joint international research and development project that aims to demonstrate the scientific and technical feasibility of fusion power. It represents the responsible actions of governments whose countries comprise over half the world's population, to create fusion power as a source of clean, economic, carbon dioxide-free energy. This is the most important science initiative of our time.The partners in the Project--the ITER Parties--are the European Union, Japan, the People's Republic of China, India, the Republic of Korea, the Russian Federation and the USA. ITER will be constructed in Europe, at Cadarache in the South of France. The talk will illustrate the genesis of the ITER Organization, the ongoing work at the Cadarache site and the planned schedule for construction. There will also be an explanation of the unique aspects of international collaboration that have been developed for ITER.Although the present focus of the project is construction activities, ITER is also a major scientific and technological research program, for which the best of the world's intellectual resources is needed. Challenges for the young, imperative for fulfillment of the objective of ITER will be identified. It is important that young students and researchers worldwide recognize the rapid development of the project, and the fundamental issues that must be overcome in ITER.The talk will also cover the exciting career and fellowship opportunities for young people at the ITER Organization.

Ikeda, Kaname [Director General, ITER Organization Cadarache Centre, 13108 St Paul lez Durance (France)

2009-02-19T23:59:59.000Z

104

Microsoft Word - SNOPUD_Youngs_Cr_Hydro_CX_+_Checklist.doc  

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

18, 2010 18, 2010 REPLY TO ATTN OF: KEC-4 SUBJECT: Environmental Clearance Memorandum James Hall Customer Service Engineer - TPC-TPP-4 Proposed Action: Interconnection of Snohomish County Public Utility District No.1 (SNOPUD) Young's Creek Hydro Small Generation Budget Information: WO# 00231295, Task 01 Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B4.6 Additions or modifications to electric power transmission facilities that would not affect the environment beyond the previously developed facility area including, but not limited to, switchyard rock grounding upgrades, secondary containment projects, paving projects, seismic upgrading, tower modifications, changing insulators, and replacement of poles, circuit breakers, conductors,

105

Snowmass 2013 Young Physicists Science and Career Survey Report  

E-Print Network (OSTI)

From April to July 2013 the Snowmass Young Physicists (SYP) administered an online survey collecting the opinions and concerns of the High Energy Physics (HEP) community. The aim of this survey is to provide input into the long term planning meeting known as the Community Summer Study (CSS), or Snowmass on the Mississippi. In total, 1112 respondents took part in the survey including 74 people who had received their training within HEP and have since left for non-academic jobs. This paper presents a summary of the survey results including demographic, career outlook, planned experiments and non-academic career path information collected.

J. Anderson; J. Asaadi; B. Carls; R. Cotta; R. Guenette; B. Kiburg; A. Kobach; H. Lippincott; B. Littlejohn; J. Love; B. Penning; M. Soares Santos; T. Strauss; A. Szelc; E. Worcester; F. Yu

2013-07-30T23:59:59.000Z

106

11/14/12 Could Climate Change Drive Giant Pandas to Extinction? | TIME.com 1/3newsfeed.time.com/2012/11/13/climate-change-threatens-pandas-diet/  

E-Print Network (OSTI)

Machine (Journey) 3 Things To Remember About Fracking (Energy From Shale) New Nanotech Batteries Might Get

107

Physiological responses of young thoroughbred horses to intermittent high-intensity treadmill training  

E-Print Network (OSTI)

age or extent of previous training in young horses or theirat the outset of the training. Endnotes a Mustang 2200,References 1. Evans DL: Training thoroughbred racehorses. In

Ohmura, Hajime; Matsui, Akira; Hada, Tetsuro; Jones, James H

2013-01-01T23:59:59.000Z

108

Relationships among the personal fable, drug use and parental monitoring in adolescents and young adults.  

E-Print Network (OSTI)

??Relationships among the personal fable, drug use and parental monitoring in adolescents and young adults were tested in this study. Participants were 56 students, with… (more)

Liu, Xin, 1986 Feb. 2-

2011-01-01T23:59:59.000Z

109

SENAI and the insertion of the young apprentice in the formal labor market.  

E-Print Network (OSTI)

??This study investigates the impact on the contribution of industrial learning for employability among young learners. The Government, through the Law of the Apprentice (10,097… (more)

SÃlon Nogueira de Lima

2009-01-01T23:59:59.000Z

110

A Real Reflection of How I Write: Young Adult Female Authors Seizing Agency Through Fan Fiction.  

E-Print Network (OSTI)

??This research project examines ""fan fiction"" (stories based upon existing texts such as movies, books, and video games) written by a young adult female and… (more)

Coleman, Susanna

2008-01-01T23:59:59.000Z

111

book on theory and applications of MDS by Young and Hamer, [21 ...  

E-Print Network (OSTI)

book on theory and applications of MDS by Young and Hamer, [21] presents applications of MDS in such diverse fields as marketing.. sociology, physics, ...

112

K-Ar dating of young volcanic rocks  

DOE Green Energy (OSTI)

Potassium-Argon (K-Ar) age dates were determined for forty-two young geologic samples by the Laboratory of Isotope Geochemistry, Department of Geosciences, in the period February 1, 1986 to June 30, 1989. Under the terms of Department of Energy Grant No. FG07-86ID12622, The University of Arizona was to provide state-of-the-art K-Ar age dating services, including sample preparation, analytical procedures, and computations, for forty-two young geologic samples submitted by DOE geothermal researchers. We billed only for forty samples. Age dates were determined for geologic samples from five regions with geothermal potential: the Cascade Mountains (Oregon); the Cascade Mountains (Washington); Ascension Island, South Atlantic Ocean; Cerro Prieto, Mexico; and Las Azufres, Mexico. The ages determined varied from 5.92 m.a. to 0.62 m.a. The integration of K-Ar dates with geologic data and the interpretation in terms of geologic and geothermal significance has been reported separately by the various DOE geothermal researchers. Table 1 presents a detailed listing of all samples dated, general sample location, researcher, researcher's organization, rock type, age, and probable error (1 standard deviation). Additional details regarding the geologic samples may be obtained from the respective geothermal researcher. 1 tab.

Damon, P.E.; Shafiqullah, M.

1991-01-31T23:59:59.000Z

113

Climate Change and Forest VIRGINIA H. DALE, LINDA A. JOYCE, STEVE McNULTY, RONALD P NEILSON, MATTHEW P AYRES,  

E-Print Network (OSTI)

).For- est disturbances influence how much carbon is stored in trees or dead wood. All these natural in maturevegetation (Lugoand Scatena 1995).Hurricanescan also resultin buriedvegetation and carbon sinks. Windstorms. This understanding, however, is complicated by the diverse goals of forest man- agement (e.g.,fiber products

114

Adopt, adapt, abandon: Understanding why some young adults start, and then stop, using instant messaging  

Science Conference Proceedings (OSTI)

Instant messaging (IM) has become a popular and important mode of staying in touch for teens and young adults. It allows for easy, frequent and lightweight interaction that contributes to building and sustaining friendships, as well as coordinating social ... Keywords: Adoption, Computer-mediated communication (CMC), Dropouts, Instant messaging, Young adults

Jeremy Birnholtz

2010-11-01T23:59:59.000Z

115

Young's modulus evaluation by SAWs for porous silica low-k film with cesium doping  

Science Conference Proceedings (OSTI)

Young's moduli of porous silica low-k films with cesium (Cs) doping are determined by surface acoustic waves (SAWs) in this study. Four low-k samples doped with 0-30ppmwt% Cs in the precursor solution are investigated to check the mechanical promotion ... Keywords: Cesium doping, Low-k film, Porous silica, Surface acoustic waves, Young's modulus

X. Xiao; X. M. Shan; Y. Kayaba; K. Kohmura; H. Tanaka; T. Kikkawa

2011-05-01T23:59:59.000Z

116

Aiming and clicking in young children's use of the computer mouse  

Science Conference Proceedings (OSTI)

The present study investigated the abilities of young children to aim and click with a computer mouse. Young children have not yet fully developed their motor skills and they are therefore more likely than adults to click next to targets on the computer ... Keywords: Elementary education, Human-computer interaction, Input device, Interface, Media in education, Navigation

Afke Donker; Pieter Reitsma

2007-11-01T23:59:59.000Z

117

Technology policy for the knowledge economy: Public support to young ICT service firms  

Science Conference Proceedings (OSTI)

Public intervention in high-tech sectors is often advocated to resolve market imperfections that may possibly limit the viability of young high-tech enterprises. Although some European countries have adopted national government support policies that ... Keywords: Horizontal direct public subsidies, Italy, Young ICT service firms

Massimo G. Colombo; Luca Grilli

2007-11-01T23:59:59.000Z

118

Charles D. Young Project Engineer Government Support Directorate  

Office of Legacy Management (LM)

Please call if you have questions regarding the attached recommendation. i?&,o-o; Please call if you have questions regarding the attached recommendation. i?&,o-o; ~~~pApv $l$I Charles D. Young Project Engineer Government Support Directorate Architecture Planning and Technology Division CDY/smb Attachment cc: J. Fiore ;;,ewis (w/o) TH' E AEROSPACE CORPORATION i ' 0 A Suite 7900, 955 L' Enfam Plaza. S. W., Woshingron. D.C. 20024-2174. Tekphonc (202) 488-6000 7117-03.87.cdy.43 23 September 1987 CA Mr. Andrew Wallo, III, NE-23 Division of Facility & Site Decosunissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear Mr. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES The attached elimination reconnnendation was prepared in accordance PC.o= with your suggestion during our meeting on 22 September. The recommendation flD.o-02

119

Baby Brutes: Simulations Help Solve the Mysteries of Massive Young  

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

Baby Brutes Baby Brutes Baby Brutes Simulations Help Solve the Mysteries of Massive Young Star-Forming Galaxies March 31, 2010 | Tags: Astrophysics Contact: Margie Wylie, mwylie@lbl.gov, +1 510 486 7421 Primack-fig1a.png Figure 1. In this model galactic plane (seen in cross section), the energy input of stellar superclusters causes gases to shoot out at speeds up to 1000 kilometers per second at temperatures reaching 100 million Kelvin. These appear as plumes or "chimneys," visible in the top three frames (showing density, temperature, and velocity; the bottom frame shows gas column density). Small bubbles of hot gas in the field (visible in the top two frames) are the result of stellar feedback from runaway stars. Astronomers have in recent years been surprised to find hulking brutes

120

The Very Young Radio Pulsar J1357-6429  

E-Print Network (OSTI)

We report the discovery of a radio pulsar with a characteristic age of 7300 years, making it one of the 10 apparently youngest Galactic pulsars known. PSR J1357-6429, with a spin period of P = 166 ms and spin-down luminosity of 3.1e36 ergs/s, was detected during the Parkes multibeam survey of the Galactic plane. We have measured a large rotational glitch in this pulsar, with Delta P/P = -2.4e-6, similar in magnitude to those experienced occasionally by the Vela pulsar. At a nominal distance of only ~ 2.5 kpc, based on the measured free electron column density of 127 pc/cc and the electron distribution model of Cordes & Lazio, this may be, after the Crab, the nearest very young pulsar known. The pulsar is located near the radio supernova remnant candidate G309.8-2.6.

F. Camilo; R. N. Manchester; A. G. Lyne; B. M. Gaensler; A. Possenti; N. D'Amico; I. H. Stairs; A. J. Faulkner; M. Kramer; D. R. Lorimer; M. A. McLaughlin; G. Hobbs

2004-06-23T23:59:59.000Z

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121

HUNTING FOR YOUNG DISPERSING STAR CLUSTERS IN IC 2574  

SciTech Connect

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

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

2012-12-01T23:59:59.000Z

122

MASS AND LUMINOSITY EVOLUTION OF YOUNG STELLAR OBJECTS  

SciTech Connect

A model of protostar mass and luminosity evolution in clusters gives new estimates of cluster age, protostar birthrate, accretion rate, and mean accretion time. The model assumes constant protostar birthrate, core-clump accretion, and equally likely accretion stopping. Its parameters are set to reproduce the initial mass function and to match protostar luminosity distributions in nearby star-forming regions. It obtains cluster ages and birthrates from the observed numbers of protostars and pre-main sequence (PMS) stars, and from the modal value of the protostar luminosity. In 31 embedded clusters and complexes, the global cluster age is 1-3 Myr, matching available estimates based on optical spectroscopy (OS) and evolutionary tracks. This method of age estimation is simpler than OS and is more useful for young embedded clusters where optical spectroscopy is not possible. In the youngest clusters, the protostar fraction decreases outward from the densest gas, indicating that the local star-forming age increases outward from a few 0.1 Myr in small protostar-dominated zones to a few Myr in large PMS-dominated zones.

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

2012-06-10T23:59:59.000Z

123

Linear spectropolarimetry of young and other emission line stars  

E-Print Network (OSTI)

The aim of this article is to demonstrate the useful role that can be played by spectropolarimetric observations of young and evolved emission line stars that analyse the linearly polarized component in their spectra. At the time of writing, this demonstration has to be made on the basis of optical data since there is no common-user infrared facility, in operation, that offers the desired combination of spectral resolution and sensitivity. Here we focus on what can be learned from linear spectropolarimetry alone at reasonably high spectral resolution and at $10^3 < $S/N$ < 10^4$. And we remind that the near infrared (1--2 micron) has the potential to out-perform the optical as a domain to work in because of the greatly reduced interstellar obscuration at these wavelengths. This point has been reached at a time when theory, exploiting flexible Monte Carlo methods, is fast becoming a powerful tool. In short we have the complex phenomena, and the rise of the modelling capability to match -- good data are the missing link.

Janet Drew; Jorick Vink; Tim Harries; Ryuichi Kurosawa; Rene Oudmaijer

2004-03-30T23:59:59.000Z

124

AFDC Benefits and Nonmarital Births to Young Women  

E-Print Network (OSTI)

Building on recent work by Rosenzweig (1999), this paper re-examines the effect of AFDC benefits on early non-marital childbearing. Unlike most previous work in this area, Rosenzweig finds a statistically significant and quantitatively large positive effect of AFDC benefits. Using data from the Panel Study of Income Dynamics, we replicate Rosenzweig’s analysis and explore the reasons his findings differ from earlier research findings. We are able to reproduce his main finding that AFDC generosity influences non-marital childbearing when state and cohort fixed-effects are included. However, we find that model specification matters a great deal. An alternative specification of state fixed-effects yields no evidence of an AFDC effect, and when we focus on fertility only through age 19 (as in prior work), we also find no AFDC effect. This latter finding implies that the behavior of women in their early 20s may be far more sensitive to welfare In this paper, we replicate and extend recent research by Mark Rosenzweig (1999) on the relationship between AFDC benefits and non-marital childbearing by young women. Most previous work on the effects of AFDC benefit levels on a wide range of demographic behaviors, including non-marital childbearing, has found a relatively weak relationship. In some papers, benefits do have a statistically significant effect that is

Saul D. Hoffman; E. Michael Foster; David Neumark; Robert Moffitt; Rebecca Blank; Greg Duncan

2000-01-01T23:59:59.000Z

125

Evaluation of 1991-1992 Brood Overwinter-Reared Coho Released from Net Pens in Youngs Bay, Oregon : Final Completion Report Youngs Bay Terminal Fishery Project.  

DOE Green Energy (OSTI)

Funding from Bonneville Power Administration was provided to the Oregon Department of Fish and Wildlife and the Clatsop County Economic Development Council`s Fisheries Project to identify and develop terminal fishing opportunities. The 1991 and 1992 brood fingerling coho from Oregon Department of Fish and Wildlife hatcheries were successfully reared during the winter period to smolt stage in Youngs Bay utilizing floating net pens. Based on coded-wire-tag recoveries during 1991--93 from 2-week net-pen acclimation releases, total accountability of coho adults averaged 40,540 fish, with the Youngs Bay commercial harvest accounting for 39%. With reduced ocean harvest impacts during 1994 and 1995, 92% of 51,640 coho in 1994 and 68% of 23,599 coho in 1995 (based on coded-wire-tag recoveries) were accounted for in the Youngs Bay commercial fishery for combined 2-week and overwinter acclimation net-pen releases. Overwinter net-pen acclimation coho accounted for 35,063 and 15,775 coho adults in 1994 and 1995 with 93% and 68% accountable in the Youngs Bay commercial harvest. Based on coded-wire-tag recoveries, less than 1% of the adults resulting from releases at Youngs Bay net pens strayed to hatcheries, while none were recovered on spawning ground surveys during 1991--95. The highest survival rates were observed for 1991 and 1992 brood overwinter coho released in early May. Time of release, not rearing strategy, appears to be the determining factor affecting survival in Youngs Bay.

Hirose, Paul S.

1997-01-01T23:59:59.000Z

126

238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc  

Open Energy Info (EERE)

238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc 238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: 238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc Details Activities (0) Areas (0) Regions (0) Abstract: Activities of 238U decay series radioisotopes have been determined for both postcaldera basalts erupted between 1849 and 1974 and genetically related young precaldera dacites from Batur volcano, Bali, Sunda arc. All rocks possess (230Th/238U) = 1 within 2 sigma error indicating that little, if any, fractionation between Th and U occurred during their genesis, or in their source regions, within approximately the last 350 ka. Both the basaltic and the dacitic rocks possess (230Th/232U) ~

127

Bright Young Minds for a Clean Energy Future | Department of Energy  

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

Bright Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future August 16, 2011 - 12:11pm Addthis Bright Young Minds for a Clean Energy Future Sarah Jane Maxted Special Assistant, Office of Energy Efficiency & Renewable Energy How can I participate? Registration begins August 15 and ends on October 7, 2011. Students are encouraged to register with their teachers by September 30, 2011 to take advantage of the full energy savings period. It's that time again: Back to school season is officially here! Time for students to prepare for the new experiences and challenges that they will encounter throughout the upcoming school year. One such challenge-from the Energy Department in partnership with the National Science Teachers Association (NSTA)-aims to tap into the

128

Bright Young Minds for a Clean Energy Future | Department of Energy  

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

Young Minds for a Clean Energy Future Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future August 16, 2011 - 12:11pm Addthis Bright Young Minds for a Clean Energy Future Sarah Jane Maxted Special Assistant, Office of Energy Efficiency & Renewable Energy How can I participate? Registration begins August 15 and ends on October 7, 2011. Students are encouraged to register with their teachers by September 30, 2011 to take advantage of the full energy savings period. It's that time again: Back to school season is officially here! Time for students to prepare for the new experiences and challenges that they will encounter throughout the upcoming school year. One such challenge-from the Energy Department in partnership with the National Science Teachers Association (NSTA)-aims to tap into the

129

Hands to Work: The Practical Artistry of David DeYoung  

Science Conference Proceedings (OSTI)

Jun 4, 2009 ... Based on advice given to him by an architect at Children's Hospital of Pittsburgh, DeYoung devised an open floor plan in the living area that ...

130

Effects of acidic water on young-of-the-year smallmouth bass ...  

Science Conference Proceedings (OSTI)

Environmental Biology of Fishes Vol. 21, No. 3, pp. 223-229,1988. 0 Dr W. Junk Publishers, Dordrecht. Effects of acidic water on young-of-the-year smallmouth ...

131

Molecular and Stellar Disks Galaxies Lisa Young (New Mexico Tech) and Martin Bureau (Oxford)  

E-Print Network (OSTI)

Molecular and Stellar Disks Galaxies Lisa Young (New Mexico Tech) and Martin Bureau (Oxford galaxies contain molecular disks. These internal structures evolution galaxies. to place observational constraints on the formation in early galaxies studying the relationships between embedded disks, molecular

Bureau, Martin

132

Bounded rationality and satisficing in young people's Web-based decision making  

Science Conference Proceedings (OSTI)

This study investigated Simon's behavioral decision-making theories of bounded rationality and satisficing in relation to young people's decision making in the World Wide Web, and considered the role of personal preferences in Web-based decisions. It ...

Denise E. Agosto

2002-01-01T23:59:59.000Z

133

What causes the density effect in young forest plantations?  

DOE Green Energy (OSTI)

In young forest plantations, trees planted at high densities frequently show more rapid height and diameter growth than those plants at lower densities. This positive growth response to density (the ''density effect'') often manifests long before seedlings are tall enough to shade one another, so it is not a simple response to shade. The mechanism(s) which trigger and sustain this growth enhancement are unknown. Our objectives were to document the temporal dynamics of positive growth response to increasing density in Douglas-fir plantations and to test two hypotheses as potential mechanisms for this response. The hypotheses are (1) a canopy boundary layer effect, and (2) alterations in the quality of light reflected from neighboring trees. The ''boundary layer'' hypotheses proposes that changes in atmospheric mixing occur in high-density plantations, promoting increased concentrations of CO{sub 2} and H{sub 2}O vapor during early morning hours, which in turn would enhance carbon assimilation. The ''light quality'' hypothesis proposes that the presence of neighbors alters the ratio of red to far red light in the canopy environment. Plant sensors detect this change in light quality, and growth and development is altered in response. We found that boundary layer conductance was higher, as we predicted, in low-density Douglas-fir stands than in high-density stands five years after planting. The changes in boundary conductance were accompanied by higher CO{sub 2} and H{sub 2}O vapor during early morning hours. However, we also found that the primary manifestation of the density effect in Douglas-fir occurs two to four years after planting, and we were not able to measure differences in boundary conductance in different densities at that time. Also, we found no difference in carbon isotope composition of wood cellulose formed in high- vs. low-density stands two to three years after planting. We conclude that although stand density may have a significant impact on boundary layer conductance in young stands, it does not account for the ''density effect''. Our tests of the light quality hypothesis were slowed due to poor plantation establishment in the early phase of this study. In a variable density experiment we detected significant changes in R:FR related to density. Also in that study we measured a significant enhancement of tree height at high density. However, after three years of growth, the study trees did not show significant differences in stem diameter related to density. Experimenters at Weyerhaeuser therefore decided not to harvest the trees at the end of the 3rd growth year, as originally planned. In a 1-year study of seedlings planted in raised beds subjected to different light quality treatments using transparent plastic film, we found that tree height but not diameter increased in response to decreased R:FR. At this point, we conclude that R:FR remains a viable hypothesis for the ''density effect'', but evidence is not conclusive. We expect that continued measurements in the variable density test plot at Weyerhaeuser will add more evidence in the future.

Barbara J. Bond; Gary A. Ritchie

2002-07-21T23:59:59.000Z

134

X-ray chemistry in envelopes around young stellar objects  

E-Print Network (OSTI)

We present chemical models of the envelope of a young stellar object (YSO) exposed to a central X-ray source. The models are applied to the massive star-forming region AFGL 2591 for different X-ray fluxes. The total X-ray ionization rate is dominated by the `secondary' ionization rate of H2 resulting from fast electrons. The carbon, sulphur and nitrogen chemistries are discussed. It is found that He+ and H3+ are enhanced and trigger a peculiar chemistry. Several molecular X-ray tracers are found and compared to tracers of the far ultraviolet (FUV) field. Like ultraviolet radiation fields, X-rays enhance simple hydrides, ions and radicals. In contrast to ultraviolet photons, X-rays can penetrate deep into the envelope and affect the chemistry even at large distances from the source. Whereas the FUV enhanced species cover a region of 200-300 AU, the region enhanced by X-rays is >1000 AU. Best-fit models for AFGL 2591 predict an X-ray luminosity LX > 1e+31 ergs/s with a hard X-ray spectrum TX > 3e+07 K. Furthermore, we find LX/Lbol ~ 1e-6. The chemistry of the bulk of the envelope mass is dominated by cosmic-ray induced reactions rather than by X-ray induced ionization for X-ray luminosities LX < 1e+33 ergs/s. The calculated line intensities of HCO+ and HCS+ show that high-J lines are more affected than lower J lines by the presence of X-rays due to their higher critical densities, and that such differences are detectable even with large aperture single-dish telescopes. Future instruments such as Herschel-HIFI or SOFIA will be able to observe X-ray enhanced hydrides whereas the sensitivity and spatial resolution of ALMA is well-suited to measure the size and geometry of the region affected by X-rays.

P. Staeuber; S. D. Doty; E. F. van Dishoeck; A. O. Benz

2005-06-14T23:59:59.000Z

135

Water destruction by X-rays in young stellar objects  

E-Print Network (OSTI)

We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemistry is modeled as a function of time, hydrogen density and X-ray flux. To cover a wide range of physical environments, densities between n_H = 10^4-10^9 cm^-3 and temperatures between T = 10-1000 K are studied. Three different regimes are found: For T water abundance is of order 10^-7-10^-6 and can be somewhat enhanced or reduced due to X-rays, depending on time and density. For 100 K 10^-3 ergs s-1 cm^-2 (t = 10^4 yrs) and for F_X > 10^-4 ergs s^-1 cm^-2 (t = 10^5 yrs). At higher temperatures (T > 250 K) and hydrogen densities, water can persist with x(H2O) ~ 10^-4 even for high X-ray fluxes. The X-ray and FUV models are applied to envelopes around low-mass Class 0 and I young stellar objects (YSOs). Water is destroyed in both Class 0 and I envelopes on relatively short timescales (t ~ 5000 yrs) for realistic X-ray fluxes, although the effect is less prominent in Class 0 envelopes due to the higher X-ray absorbing densities there. FUV photons from the central source are not effective in destroying water. The average water abundance in Class I sources for L_X > 10^27 ergs s^-1 is predicted to be x(H2O) < 10^-6.

P. Stauber; J. K. Jorgensen; E. F. van Dishoeck; S. D. Doty; A. O. Benz

2006-02-06T23:59:59.000Z

136

A Survey for Young Spectroscopic Binary K7-M4 Stars in Ophiuchus  

E-Print Network (OSTI)

This paper describes a high-resolution, infrared spectroscopic survey of young, low-mass stars designed to identify and characterize pre-main-sequence spectroscopic binaries. This is the first large infrared radial velocity survey of very young stars to date. The frequency and mass ratio distribution of the closest, low-mass binaries bear directly on models of stellar, brown dwarf, and planetary mass companion formation. Furthermore, spectroscopic binaries can provide mass ratios and ultimately masses, independent of assumptions, needed to calibrate models of young star evolution. I present the initial results from observations of a uniform sample of 33 T Tauri M stars in the Ophiuchus molecular cloud. The average mass of this sample is less than that of other young star radial velocity surveys of similar scope by a factor of ~2. Almost every star was observed at 3-4 epochs over 3 years with the 10 meter Keck II telescope and the facility infrared spectrometer NIRSPEC. An internal precision of 0.43 km/s was obtained with standard cross-correlation calibration techniques. Four of the targets are newly discovered spectroscopic binaries, one of which is located in a sub-arcsecond, hierarchical quadruple system. Three other sub-arcsecond visual binaries were also serendipitously identified during target acquisition. The spectroscopic multiplicity of the sample is comparable to that of earlier type, pre-main-sequence objects. Therefore, there is no dearth of young, low-mass spectroscopic binary stars, at least in the Ophiuchus region.

L. Prato

2006-11-20T23:59:59.000Z

137

AGE AND MASS STUDIES FOR YOUNG STAR CLUSTERS IN M31 FROM SEDS-FIT  

SciTech Connect

In this paper, we present photometry for young star clusters in M31, which are selected from Caldwell et al. These star clusters have been observed as part of the Beijing-Arizona-Taiwan-Connecticut (BATC) Multicolor Sky Survey from 1995 February to 2008 March. The BATC images including these star clusters are taken with 15 intermediate-band filters covering 3000-10000 A. Combined with photometry in the GALEX far- and near-ultraviolet, broadband UBV RI, SDSS ugriz, and infrared JHK{sub s} of Two Micron All Sky Survey, we obtain their accurate spectral energy distributions (SEDs) from 1538 to 20000 A. We derive these star clusters' ages and masses by comparing their SEDs with stellar population synthesis models. Our results are in good agreement with previous determinations. The mean value of age and mass of young clusters (<2 Gyr) is about 385 Myr and 2 Multiplication-Sign 10{sup 4} M{sub Sun }, respectively. There are two distinct peaks in the age distribution, a highest peak at age {approx}60 Myr and a secondary peak around 250 Myr, while the mass distribution shows a single peak around 10{sup 4} M{sub Sun }. A few young star clusters have two-body relaxation times greater than their ages, indicating that those clusters have not been well dynamically relaxed and therefore have not established the thermal equilibrium. There are several regions showing aggregations of young star clusters around the 10 kpc ring and the outer ring, indicating that the distribution of the young star clusters is well correlated with M31's star-forming regions. The young massive star clusters (age {<=}100 Myr and mass {>=}10{sup 4} M{sub Sun }) show apparent concentration around the ring splitting region, suggesting a recent passage of a satellite galaxy (M32) through M31 disk.

Wang Song; Ma Jun; Fan Zhou; Wu Zhenyu; Zhang Tianmeng; Zou Hu; Zhou Xu, E-mail: majun@nao.cas.cn [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)

2012-12-01T23:59:59.000Z

138

Click Here to Subscribe! Previous Page | Cover | Contents | Full Screen | Print | Search | Next Page Nanotech BriefsTM June 2006 Vol.3 / No.6  

E-Print Network (OSTI)

.90 V Pt L3 PtCu/Vulcan In situ EXAFS at Brookhaven NL synchrotron (NSLS), using GM beamtime 25 #12;GM

Azad, Abdul-Majeed

139

Measuring Liquid Volumes in Sub-nanoliter Wells Ian T. Young*1  

E-Print Network (OSTI)

Measuring Liquid Volumes in Sub-nanoliter Wells Ian T. Young*1 , Kari T. Hjelt2 , Richard van den. These wells can serve as bioreactors for studying a variety of biochemical reactions such as the enzymatic of liquid that has been deposited in a given well and/or to monitor the evaporation of the liquid. Using

van Vliet, Lucas J.

140

Belowground and aboveground biomass in young postfire lodgepole pine forests of contrasting tree  

E-Print Network (OSTI)

Belowground and aboveground biomass in young postfire lodgepole pine forests of contrasting tree as 40% of live biomass in coniferous forests is located belowground, yet the effect of tree density on biomass allocation is poorly understood. We developed allometric equations using traditional harvesting

Turner, Monica G.

Note: This page contains sample records for the topic "nanotech linda young" 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

Homeless young people's experiences with information systems: life and work in a community technology center  

Science Conference Proceedings (OSTI)

This paper explores how homeless young people, aged 13-25, make use of information systems in daily life. Observed in a community technology center, four different examples of uses are described: i) Using digital tools to find employment, ii) Telling ... Keywords: digital media, homelessness, identity, youth

Jill Palzkill Woelfer; David G. Hendry

2010-04-01T23:59:59.000Z

142

Texas Tech at TMEA 2013 Clinicians: Janice Killian & John Wayman, Young Harris College  

E-Print Network (OSTI)

Texas Tech at TMEA 2013 ,k9ki9o Clinicians: Janice Killian & John Wayman, Young Harris College Wood The Yin and Yang of Teaching Music Thurs. Feb 14 th 11:00 am ­ Noon / CC 212 Texas Tech Consortium Thurs. Feb 14 th 5:00-6:00 pm / CC 212 Concert: Texas Tech University Symphonic Wind Ensemble Conductor

Rock, Chris

143

Water harvesting for young trees using Peltier modules powered by photovoltaic solar energy  

Science Conference Proceedings (OSTI)

Young trees transplanted from nursery into open field require a minimum amount of soil moisture to successfully root in their new location, especially in dry-climate areas. One possibility is to obtain the required water from air moisture. This can be ... Keywords: DAQB, Dew condenser, EMF, ETc, Hr, Irrigation, SPV, SPVM, Solar photovoltaic energy, TD, Ta, Tdp, Thermoelectric effect, Ts, Water harvesting

M. A. MuñOz-GarcíA; G. P. Moreda; M. P. Raga-Arroyo; O. MaríN-GonzáLez

2013-04-01T23:59:59.000Z

144

Probing the close environment of massive young stars with spectro-astrometry  

E-Print Network (OSTI)

Aims: We test the technique of spectro-astrometry as a potential method to investigate the close environment of massive young stars. Method: Archival VLT near infrared K band spectra (R=8900) of three massive young stellar objects and one Wolf-Rayet star are examined for spectro-astrometric signatures. The young stellar objects display emission lines such as Brackett gamma, CO 2-0 and CO 3-1 that are characteristic of ionised regions and molecular disks respectively. Two of the sample sources also display emission lines such as NIII and MgII that are characteristic of high temperatures. Results: Most of the emission lines show spectro-astrometric signal at various levels resulting in different positional displacements. The shapes and magnitudes of the positional displacements imply the presence of large disk/envelopes in emission and expanding shells of ionised gas. The results obtained for the source 18006-2422nr766 in particular provide larger estimates (> 300AU) on CO emitting regions indicating that in MYSOs CO may arise from inner regions of extended dense envelopes as well. Conclusions: The overall results from this study demonstrate the utility of spectro-astrometry as a potential method to constrain the sizes of various physical entities such as disks/envelopes, UCHII regions and/or ionised shells in the close environment of a massive young star.

J. M. C. Grave; M. S. N. Kumar

2006-12-05T23:59:59.000Z

145

We often think about energy in personal terms. People comment on the energy young children  

E-Print Network (OSTI)

Overview We often think about energy in personal terms. People comment on the energy young children seem to possess. Others mention that they don't feel they have enough energy to make it through the day. We've heard that the world is running out of certain types of energy. In spite of all of our everyday

Hardy, Darel

146

Modeling the Young Sun's Solar Wind and its Interaction with Earth's Paleomagnetosphere  

E-Print Network (OSTI)

We present a focused parameter study of solar wind - magnetosphere interaction for the young Sun and Earth, $~3.5$ Ga ago, that relies on magnetohydrodynamic (MHD) simulations for both the solar wind and the magnetosphere. By simulating the quiescent young Sun and its wind we are able to propagate the MHD simulations up to Earth's magnetosphere and obtain a physically realistic solar forcing of it. We assess how sensitive the young solar wind is to changes in the coronal base density, sunspot placement and magnetic field strength, dipole magnetic field strength and the Sun's rotation period. From this analysis we obtain a range of plausible solar wind conditions the paleomagnetosphere may have been subject to. Scaling relationships from the literature suggest that a young Sun would have had a mass flux different from the present Sun. We evaluate how the mass flux changes with the aforementioned factors and determine the importance of this and several other key solar and magnetospheric variables with respect t...

Sterenborg, M Glenn; Drake, Jeremy J; Gombosi, Tamas I; 10.1029/2010JA016036

2011-01-01T23:59:59.000Z

147

eter Agre is a medical doc-tor, professor and molecu-  

E-Print Network (OSTI)

Solazyme [SZYM]. PXN: The PowerShares Lux Nanotech edged almost 1% higher. PBW: The PowerShares Wilder

Wechsler, Risa H.

148

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.

149

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

150

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.

151

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.

152

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.

153

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

154

First principles study of the Young's modulus of Si <001> nanowires  

DOE Green Energy (OSTI)

We report the results of first-principles calculations of the Young's modulus and other mechanical properties of hydrogen-passivated Si <001> nanowires. The nanowires are taken to have predominantly {l_brace}100{r_brace} surfaces, with small {l_brace}110{r_brace} facets according to the Wulff shape. The Young's modulus, the equilibrium length and the constrained residual stress of a series of prismatic beams of differing sizes is found to have a size dependence that scales like the surface area to volume ratio for all but the smallest beam. The results are compared with two different models (and the results of classical atomistic calculations based on an empirical potential). We discuss the physics of the hydrogen interactions on the surface and the charge density variations within the beam that may account for the discrepancies of the models and the first principles results.

Lee, B; Rudd, R E

2006-07-03T23:59:59.000Z

155

Cooper minima and Young-type interferences in the photoionization of H{sub 2}{sup +}  

SciTech Connect

We present a detailed study of the partial and total cross sections for photon-induced electron emission from H{sub 2}{sup +}. By comparing the results employing exact and approximate, bounded and continuum wave functions, for one- and two-center basis functions, we find the origin and position of the Cooper-like minima in the partial cross sections and their relationship with the Young-type interference pattern.

Della Picca, R. [CONICET and Centro Atomico Bariloche, Comision Nacional de Energia Atomica, Avda E. Bustillo 9500, 8400 Bariloche (Argentina); UPMC Univ. Paris 6, UMR 7614, Laboratoire de Chimie Physique-Matiere et Rayonnement, 11 rue Pierre et Marie Curie, F-75231 Paris Cedex 05 (France); Fainstein, P. D. [CONICET and Centro Atomico Bariloche, Comision Nacional de Energia Atomica, Avda E. Bustillo 9500, 8400 Bariloche (Argentina); Dubois, A. [UPMC Univ. Paris 6, UMR 7614, Laboratoire de Chimie Physique-Matiere et Rayonnement, 11 rue Pierre et Marie Curie, F-75231 Paris Cedex 05 (France); CNRS UMR 7614, LCPMR, F-75005 Paris (France)

2011-09-15T23:59:59.000Z

156

Hubble Space Telescope Imaging of the Young Planetary Nebula GL 618  

E-Print Network (OSTI)

We present narrow-band Hubble Space Telescope images of the young planetary nebula GL 618. These images have allowed us to study the detailed morphology of shock-excited emission present in the bipolar lobes of this object. These images reveal the presence of three highly collimated outflows emanating from the central regions of GL 618. We discuss the significance of the detection of these outflows and the possible origins of these features.

Susan R. Trammell

2000-01-10T23:59:59.000Z

157

Age distribution of young clusters and field stars in the SMC  

E-Print Network (OSTI)

In this paper we discuss the cluster and field star formation in the central part of the Small Magellanic Cloud. The main goal is to study the correlation between young objects and their interstellar environment. The ages of about 164 associations and 311 clusters younger than 1 Gyr are determined using isochrone fitting. The spatial distribution of the clusters is compared with the HI maps, with the HI velocity dispersion field, with the location of the CO clouds and with the distribution of young field stars. The cluster age distribution supports the idea that clusters formed in the last 1 Gyr of the SMC history in a roughly continuous way with periods of enhancements. The two super-shells 37A and 304A detected in the HI distribution are clearly visible in the age distribution of the clusters: an enhancement in the cluster formation rate has taken place from the epoch of the shell formation. A tight correlation between young clusters and the HI intensity is found. The degree of correlation is decreasing with the age of the clusters. Clusters older than 300 Myr are located away from the HI peaks. Clusters and associations younger than 10 Myr are related to the CO clouds in the SW region of the SMC disk. A positive correlation between the location of the young clusters and the velocity dispersion field of the atomic gas is derived only for the shell 304A, suggesting that the cloud-cloud collision is probably not the most important mechanism of cluster formation. Evidence of gravitational triggered episode due to the most recent close interaction between SMC and LMC is found both in the cluster and field star distribution.

E. Chiosi; A. Vallenari; E. V. Held; L. Rizzi; A. Moretti

2006-04-07T23:59:59.000Z

158

Bayesian analysis to identify very low-mass members of nearby young stellar kinematic groups  

E-Print Network (OSTI)

We describe our all-sky survey for >M4 candidate members to nearby, young associations from the 2MASS and WISE catalogs using bayesian inference. We report the first results, including 38 highly probable candidates showing spectroscopic signs of low-gravity (and thus youth). The latest of these objects would correspond to a 11 - 13 MJup object, around the limit of the planetary regime.

Gagné, Jonathan; Doyon, René; Malo, Lison; Faherty, Jacqueline; Artigau, Étienne

2013-01-01T23:59:59.000Z

159

Probing the close environment of massive young stars with spectro-astrometry  

E-Print Network (OSTI)

Aims: We test the technique of spectro-astrometry as a potential method to investigate the close environment of massive young stars. Method: Archival VLT near infrared K band spectra (R=8900) of three massive young stellar objects and one Wolf-Rayet star are examined for spectro-astrometric signatures. The young stellar objects display emission lines such as Brackett gamma, CO 2-0 and CO 3-1 that are characteristic of ionised regions and molecular disks respectively. Two of the sample sources also display emission lines such as NIII and MgII that are characteristic of high temperatures. Results: Most of the emission lines show spectro-astrometric signal at various levels resulting in different positional displacements. The shapes and magnitudes of the positional displacements imply the presence of large disk/envelopes in emission and expanding shells of ionised gas. The results obtained for the source 18006-2422nr766 in particular provide larger estimates (> 300AU) on CO emitting regions indicating that in MY...

Grave, J M C

2006-01-01T23:59:59.000Z

160

Moving the Goalposts: The Impact of Soccer on the Lives and Prospects of Girls and Young Women Rural Kenya  

E-Print Network (OSTI)

2004). Seventh lowest out of 69 districts in Kenya UNDP (2005) Fourth Kenya Human Development Report 2 MTGK (2005) '·Girls and Young Women in Rural Kenya Sarah Forde and Andrea

Forde, Sarah; Kendall-Taylor, Andrea

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" 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

Modulatory effects of levodopa on cognitive control in young but not in older subjects: A pharmacological fmri study  

Science Conference Proceedings (OSTI)

Older individuals show decline of prefrontal cortex (PFC) functions which may be related to altered dopaminergic neurotransmission. We investigated the effects of aging and dopaminergic stimulation in 15 young and 13 older healthy subjects on the neural ...

Özgür A. Onur; Martina Piefke; Chuh-Hyoun Lie; Christiane M. Thiel; Gereon R. Fink

2011-10-01T23:59:59.000Z

162

"Young Town" growing up : four decades later : self-help housing and upgrading lessons from a squatter neighborhood in Lima  

E-Print Network (OSTI)

This thesis examines self-help housing policies in Peru by revisiting Independencia, one of Lima's young towns (squatter settlements), forty-five years after its founding. The study was designed to better understand how ...

Williams, Susana M. (Susana Maria)

2005-01-01T23:59:59.000Z

163

Young Scientist  

Science Conference Proceedings (OSTI)

Mar 14, 2012... Schmidt1; Mathis Ruppert1; Patrick Knödler1; Heinz Werner Höppel1; Mathias Göken1; 1Friedrich-Alexander-Universität Erlangen-Nürnberg

164

Scott Young  

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

Engineering, University of Toronto 2003, M.Sc. Biosystems Engineering, University of Manitoba 2000, B.Sc. Biosystems Engineering, University of Manitoba Vision & Mission...

165

Young Scientist  

Science Conference Proceedings (OSTI)

Feb 17, 2010 ... Unconventional ECAE Processing of Magnesium Alloys: David Foley1; Majid ... An examination of conventional and unconventional ECAE ...

166

(290), ra75. [DOI: 10.1126/scisignal.2004097]6Science Signaling Linda C. Hsieh-Wilson and David Baltimore (27 August 2013)  

E-Print Network (OSTI)

Function of the NF-kB Protein c-Rel by O-GlcNAc Glycosylation Parameswaran Ramakrishnan,1 * Peter M. Clark factor nuclear factor kB (NF-kB) rapidly reprograms gene expression in response to various stimuli stress. We report that the NF-kB subunit c-Rel is modified and acti- vated by O-GlcNAcylation. We

Gleeson, Joseph G.

167

Detection of steam in the circumstellar disk around a massive Young Stellar Object  

E-Print Network (OSTI)

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the infrared spectrometer ISAAC mounted on the VLT-ANTU. The water vapor is at a mean temperature of 1565+/-510 K, cooler than the hot CO found in the same object, which is at 1660K and the column density is N(H2O)=(2.5 +/- 0.4)x1E18 cm-2. The profile of both H2O and CO lines is best reproduced by the emission from a Keplerian disk. To interpret the data, we also investigate the formation of molecules and especially CO and water vapor in the inner hot and dense part of disks around young high mass stars using a pseudo time-dependent gas-phase chemical model. Molecules are rapidly photodissociated but this destruction is compensated by an efficient formation due to fast neutral-neutral reactions. The ability of CO molecules to self-shield significantly enhances its abundance. Water molecules are sufficiently abundant to be detectable. The observed H2O/CO ratio is reproduced by gas at 1600K and an enhanced UV field over gas density ratio I_UV/nH=1E(-4)- 1E(-6). The simulations support the presence of CO and H2O molecules in the inner disks around young massive stars despite the strong UV radiation and show that the OH radical plays an essential role in hot gas chemistry.

W. -F. Thi; A. Bik

2005-03-24T23:59:59.000Z

168

Passive solar water heating: breadbox design for the Fred Young Farm Labor Center in Indio  

SciTech Connect

An appropriate passive solar preheater for multifamily housing units in the Fred Young Farm Labor Center in Indio, California, was designed and analyzed. A brief summary of passive preheater systems and the key design features used in current designs is presented. The design features necessary for the site requirements are described. The eight preliminary preheater designs reviewed for the project are presented. The results of thermal performance simulation for the eight prototype systems are discussed. Alternative monitoring systems for the installation are described and evaluated. The consultants' recommendations, working drawings, and performance estimates of the system selected are presented. (MHR)

Melzer, B; Maeda, B

1979-10-01T23:59:59.000Z

169

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

170

The effects of stellar dynamics on the evolution of young dense stellar systems  

E-Print Network (OSTI)

In the present paper we report on first results of a project in Brussels where we study the effects of stellar dynamics on the evolution of young dense stellar systems using the 3 decades expertise in massive star evolution and our population (number and spectral) synthesis code. We highlight an unconventionally formed object scenario (UFO-scenario) for Wolf Rayet binaries and study the effects of a luminous blue variable-type instability wind mass loss formalism on the formation of intermediate mass black holes.

Belkus, H; Vanbeveren, D

2004-01-01T23:59:59.000Z

171

The effects of stellar dynamics on the evolution of young dense stellar systems  

E-Print Network (OSTI)

In the present paper we report on first results of a project in Brussels where we study the effects of stellar dynamics on the evolution of young dense stellar systems using the 3 decades expertise in massive star evolution and our population (number and spectral) synthesis code. We highlight an unconventionally formed object scenario (UFO-scenario) for Wolf Rayet binaries and study the effects of a luminous blue variable-type instability wind mass loss formalism on the formation of intermediate mass black holes.

H. Belkus; J. Van Bever; D. Vanbeveren

2004-10-21T23:59:59.000Z

172

A COMPREHENSIVE GALEX ULTRAVIOLET CATALOG OF STAR CLUSTERS IN M31 AND A STUDY OF THE YOUNG CLUSTERS  

Science Conference Proceedings (OSTI)

We present a comprehensive catalog of 700 confirmed star clusters in the field of M31 compiled from three major existing catalogs. We detect 418 and 257 star clusters in Galaxy Evolution Explorer near-ultraviolet and far-ultraviolet (FUV) imaging, respectively. Our final catalog includes photometry of star clusters in up to 16 passbands ranging from FUV to NIR as well as ancillary information such as reddening, metallicity, and radial velocities. In particular, this is the most extensive and updated catalog of UV-integrated photometry for M31 star clusters. Ages and masses of star clusters are derived by fitting the multi-band photometry with model spectral energy distribution (SED); UV photometry enables more accurate age estimation of young clusters. Our catalog includes 182 young clusters with ages less than 1 Gyr. Our estimated ages and masses of young clusters are in good agreement with previously determined values in the literature. The mean age and mass of young clusters are about 300 Myr and 10{sup 4} M{sub Sun }, respectively. We found that the compiled [Fe/H] values of young clusters included in our catalog are systematically lower (by more than 1 dex) than those from recent high-quality spectroscopic data and our SED-fitting result. We confirm that most of the young clusters' kinematics shows systematic rotation around the minor axis and association with the thin disk of M31. The young cluster distribution exhibits a distinct peak in the M31 disk around 10-12 kpc from the center and follows a spatial distributions similar to other tracers of disk structure such as OB stars, UV star-forming regions, and dust. Some young clusters also show concentration around the ring splitting regions found in the southern part of the M31 disk and most of them have systematically younger (star formation ring structure in the M31 disk. Consequently, we suggest that various properties of young clusters in M31 might be in line with the scenarios that a satellite galaxy had passed through the disk of M31 less than few hundred million years ago.

Kang, Yongbeom; Rey, Soo-Chang; Lee, Kyungsook; Kim, YoungKwang [Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764 (Korea, Republic of); Bianchi, Luciana [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Sohn, Sangmo Tony, E-mail: ybkang@cnu.ac.kr, E-mail: screy@cnu.ac.kr [Space Telescope Science Institute, Baltimore, MD 21218 (United States)

2012-04-01T23:59:59.000Z

173

ORIGINAL ARTICLE Low Motor Assessment: A Comparative Pilot Study with Young Children With and Without Motor  

E-Print Network (OSTI)

# The Author(s) 2009. This article is published with open access at Springerlink.com Abstract Most of the developmental instruments that measure cognitive development in children rely heavily on fine motor skills, especially for young children whose language skills are not yet well developed. This is problematic when evaluating the cognitive development of young children with motor impairment. The purpose of this study is to assess the need for a Low Motor adapation of a standardized instrument when testing children with motor impairment. To accomplish this, we have adapted the procedures, item instructions and play material of a widely used and standardized instrument, the Bayley Scales of Infant Development-Second Edition (BSID-II, Bayley 1993). The Original and the Low Motor versions were administered to 20 children experiencing typical development and 19 children with motor impairment within a period of two weeks. Results showed that children with motor impairments scored significantly higher on the Low Motor version of the Bayley Mental Scale than on the Original version: a difference of between 5 and 10 points when the score is expressed in terms of a developmental index score. Results from children with typical development support the assumption that item content and difficulty remain unchanged in the Low Motor version.

J Dev Phys Disabil; Selma Anne; José Ruiter; Han Nakken; Bieuwe F. Van Der Meulen; Carolien B. Lunenborg

2009-01-01T23:59:59.000Z

174

Warm Gas in the Inner Disks around Young Intermediate Mass Stars  

E-Print Network (OSTI)

The characterization of gas in the inner disks around young stars is of particular interest because of its connection to planet formation. In order to study the gas in inner disks, we have obtained high-resolution K-band and M-band spectroscopy of 14 intermediate mass young stars. In sources that have optically thick inner disks, i.e. E(K-L)>1, our detection rate of the ro-vibrational CO transitions is 100% and the gas is thermally excited. Of the five sources that do not have optically thick inner disks, we only detect the ro-vibrational CO transitions from HD 141569. In this case, we show that the gas is excited by UV fluorescence and that the inner disk is devoid of gas and dust. We discuss the plausibility of the various scenarios for forming this inner hole. Our modeling of the UV fluoresced gas suggests an additional method by which to search for and/or place stringent limits on gas in dust depleted regions in disks around Herbig Ae/Be stars.

Sean Brittain; Theodore Simon; Joan Najita; Terrence Rettig

2006-12-08T23:59:59.000Z

175

Detection of steam in the circumstellar disk around a massive Young Stellar Object  

E-Print Network (OSTI)

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the infrared spectrometer ISAAC mounted on the VLT-ANTU. The water vapor is at a mean temperature of 1565+/-510 K, cooler than the hot CO found in the same object, which is at 1660K and the column density is N(H2O)=(2.5 +/- 0.4)x1E18 cm-2. The profile of both H2O and CO lines is best reproduced by the emission from a Keplerian disk. To interpret the data, we also investigate the formation of molecules and especially CO and water vapor in the inner hot and dense part of disks around young high mass stars using a pseudo time-dependent gas-phase chemical model. Molecules are rapidly photodissociated but this destruction is compensated by an efficient formation due to fast neutral-neutral reactions. The ability of CO molecules to self-shield significantly enhances its abundance. Wa...

Thi, W F

2005-01-01T23:59:59.000Z

176

RADIO DETECTION OF GREEN PEAS: IMPLICATIONS FOR MAGNETIC FIELDS IN YOUNG GALAXIES  

Science Conference Proceedings (OSTI)

Green Peas are a new class of young, emission line galaxies that were discovered by citizen volunteers in the Galaxy Zoo project. Their low stellar mass, low metallicity, and very high star formation rates make Green Peas the nearby (z {approx} 0.2) analogs of the Lyman break galaxies which account for the bulk of the star formation in the early universe (z {approx} 2-5). They thus provide accessible laboratories in the nearby universe for understanding star formation, supernova feedback, particle acceleration, and magnetic field amplification in early galaxies. We report the first direct radio detection of Green Peas with low frequency Giant Metrewave Radio Telescope observations and our stacking detection with archival Very Large Array FIRST data. We show that the radio emission implies that these extremely young galaxies already have magnetic fields ({approx}> 30 {mu}G) even larger than that of the Milky Way. This is at odds with the present understanding of magnetic field growth based on amplification of seed fields by dynamo action over a galaxy's lifetime. Our observations strongly favor models with pregalactic magnetic fields at {mu}G levels.

Chakraborti, Sayan; Yadav, Naveen; Ray, Alak [Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai 400005 (India); Cardamone, Carolin, E-mail: sayan@tifr.res.in [Massachusetts Institute of Technology, 77 Massachusetts Avenue, Bldg. 26-331, Cambridge, MA 02139 (United States)

2012-02-10T23:59:59.000Z

177

A PAN-CARINA YOUNG STELLAR OBJECT CATALOG: INTERMEDIATE-MASS YOUNG STELLAR OBJECTS IN THE CARINA NEBULA IDENTIFIED VIA MID-INFRARED EXCESS EMISSION  

Science Conference Proceedings (OSTI)

We present a catalog of 1439 young stellar objects (YSOs) spanning the 1.42 deg{sup 2} field surveyed by the Chandra Carina Complex Project (CCCP), which includes the major ionizing clusters and the most active sites of ongoing star formation within the Great Nebula in Carina. Candidate YSOs were identified via infrared (IR) excess emission from dusty circumstellar disks and envelopes, using data from the Spitzer Space Telescope (the Vela-Carina survey) and the Two-Micron All Sky Survey. We model the 1-24 {mu}m IR spectral energy distributions of the YSOs to constrain physical properties. Our Pan-Carina YSO Catalog (PCYC) is dominated by intermediate-mass (2 M{sub sun} 2 x 10{sup 4} YSOs and a present-day star formation rate (SFR) of >0.008 M{sub sun} yr{sup -1}. The global SFR in the Carina Nebula, averaged over the past {approx}5 Myr, has been approximately constant.

Povich, Matthew S.; Getman, Konstantin V.; Townsley, Leisa K.; Broos, Patrick S. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Smith, Nathan [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Majewski, Steven R.; Indebetouw, Remy [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325 (United States); Babler, Brian L.; Meade, Marilyn R.; Whitney, Barbara A. [Department of Astronomy, University of Wisconsin, 475 N. Charter Street, Madison, WI 53706 (United States); Robitaille, Thomas P. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Stassun, Keivan G. [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Yonekura, Yoshinori [Department of Physical Science, Osaka Prefecture University, 1-1 Gakuen-cho, Sakai, Osaka 599-8531 (Japan); Fukui, Yasuo, E-mail: povich@astro.psu.edu [Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 (Japan)

2011-05-01T23:59:59.000Z

178

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

179

X-ray Chemistry in the Envelopes around Young Stellar Objects  

E-Print Network (OSTI)

We have studied the influence of X-rays from a massive young stellar object (YSO) on the chemistry of its own envelope by extending the models of Doty et al. (2002) and Staeuber et al. (2004). The models are applied to the massive star-forming region AFGL 2591 for different X-ray luminosities and plasma temperatures. Enhanced column densities for several species are predicted. In addition we present first detections of CO+ and SO+ toward AFGL 2591. These molecular ions are believed to be high-energy tracers. Herschel-HIFI will be able to observe other tracers like CH and CH+ whereas ALMA is well suited to measure the size and geometry of the emitting region.

P. Staeuber; A. O. Benz; S. D. Doty; E. F. van Dishoeck

2004-12-13T23:59:59.000Z

180

"I'm not perfect": an analysis of the narratives of young women's body image  

E-Print Network (OSTI)

Previous research has explored the influence of media on the development of feminine body image. Additional research has examined the influence of interpersonal relationships such as family and friends on body image. No research has yet examine the ways in which these factors are related and the effect they have on one another. This thesis examines the ways in which young women who are all members of the same sorority discuss their body image with one another, the stories that they tell about developing their own body image, and the factors that they find most influential to their body image. The girls speak about their body image in relation to mediated images; food, exercise, and diet; and clothing. The stories that they tell about developing body image either include the influence of friends and family or the influence of a particular activity that changes their body image. Finally, the girls' body image is most influenced by external situations such as interactions with others.

Dummer, Susan Ilene

2002-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" from the National Library of EnergyBeta (NLEBeta).
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181

HST/NICMOS Imaging of Disks and Envelopes Around Very Young Stars  

E-Print Network (OSTI)

We present HST/NICMOS observations with 0.1" (15 AU) resolution of six young stellar objects in the Taurus star-formation region. The targets of our survey are three Class I IRAS sources (IRAS 04016+2610, IRAS 04248+2612, and IRAS 04302+2247) and three low-luminosity stars (DG Tau B, Haro 6-5B, and CoKu Tau/1) associated with Herbig Haro jets. The broad-band images show that the near-infrared radiation from these sources is dominated by light scattered from dusty circumstellar material distributed in a region 10 - 15 times the size of our solar system. Although the detailed morphologies of the individual objects are unique, the observed young stellar objects share common features. All of the circumstellar reflection nebulae are crossed by dark lanes from 500 - 900 AU in extent and from less than 50 to 350 AU in apparent thickness. The absorption lanes extend perpendicular to known optical and millimeter outflows in these sources. We interpret the dark lanes as optically thick circumstellar disks seen in silhouette against bright reflection nebulosity. The bipolar reflection nebulae extending perpendicular to the dust lanes appear to be produced by scattering from the upper and lower surfaces of the disks and from dusty material within or on the walls of the outflow cavities. Out of five objects in which the central source is directly detected, two are found to be subarcsecond binaries. This mini-survey is the highest resolution near-infrared study to date of circumstellar environments around solar-type stars with age <= 1 Myr.

Deborah L. Padgett; Wolfgang Brandner; Karl R. Stapelfeldt; Stephen E. Strom; Susan Terebey; David Koerner

1999-02-06T23:59:59.000Z

182

A CORRELATION BETWEEN SURFACE DENSITIES OF YOUNG STELLAR OBJECTS AND GAS IN EIGHT NEARBY MOLECULAR CLOUDS  

SciTech Connect

We report the discovery and characterization of a power-law correlation between the local surface densities of Spitzer-identified, dusty young stellar objects (YSOs) and the column density of gas (as traced by near-IR extinction) in eight molecular clouds within 1 kpc and with 100 or more known YSOs. This correlation, which appears in data smoothed over size scales of {approx}1 pc, varies in quality from cloud to cloud; those clouds with tight correlations, MonR2 and Ophiuchus, are fit with power laws of slope 2.67 and 1.87, respectively. The spread in the correlation is attributed primarily to local gas disruption by stars that formed there or to the presence of very young subregions at the onset of star formation. We explore the ratio of the number of Class II to Class I sources, a proxy for the star formation age of a region, as a function of gas column density; this analysis reveals a declining Class II to Class I ratio with increasing column density. We show that the observed star-gas correlation is consistent with a star formation law where the star formation rate per area varies with the gas column density squared. We also propose a simple picture of thermal fragmentation of dense gas in an isothermal, self-gravitating layer as an explanation for the power law. Finally, we briefly compare the star-gas correlation and its implied star formation law with other recent proposed of star formation laws at similar and larger size scales from nearby star-forming regions.

Gutermuth, R. A. [Five College Astronomy Department, Smith College, Northampton, MA 01063 (United States); Pipher, J. L. [Department of Physics and Astronomy, University of Rochester, Rochester, NY (United States); Megeath, S. T.; Allen, T. S. [Department of Physics and Astronomy, University of Toledo, Toledo, OH (United States); Myers, P. C. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Allen, L. E. [National Optical Astronomy Observatories, Tucson, AZ (United States)

2011-10-01T23:59:59.000Z

183

CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters  

E-Print Network (OSTI)

We present CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters namely NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2006, SL 538, NGC 2011, NGC 2098 and NGC 2136. The BVRI data reaching down to V ~ 21 mag, are collected from 3.5-meter NTT/EFOSC2 in sub-arcsec seeing conditions. For NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2011 and NGC 2136, broad band photometric CCD data are presented for the first time. Seven of the 9 clusters have ages between 16 to 25 Myr while remaining two clusters have ages $32\\pm4$ Myr (NGC 2098) and $90\\pm10$ Myr (NGC 2136). For 7 younger clusters, the age estimates based on a recent model and the integrated spectra are found to be systematically lower ($\\sim$ 10 Myr) from the present estimate. In the mass range of $\\sim 2 - 12$ $M_{\\odot}$, the MF slopes for 8 out of nine clusters were found to be similar with the value of $\\gamma$ ranging from $-1.90\\pm0.16$ to $-2.28\\pm0.21$. For NGC 1767 it is flatter with $\\gamma = -1.23\\pm0.27$. Mass segregation effects are observed for NGC 2002, NGC 2006, NGC 2136 and NGC 2098. This is consistent with the findings of Kontizas et al. for NGC 2098. Presence of mass segregation in these clusters could be an imprint of star formation process as their ages are significantly smaller than their dynamical evolution time. Mean MF slope of $\\gamma = -2.22\\pm0.16$ derived for a sample of 25 young ($\\le 100$ Myr) dynamically unevolved LMC stellar systems provide support for the universality of IMF in the intermediate mass range $\\sim 2-12 M_{\\odot}$.

B. Kumar; R. Sagar; J. Melnick

2008-01-07T23:59:59.000Z

184

TAYouKi: A Sketch-Based Tutoring System for Young Kids  

E-Print Network (OSTI)

Intelligent tutoring systems (ITS) have proven to be effective tools for aiding in the instruction of new skills for young kids; however, interaction methods that employ traditional input devices such as the keyboard and mouse may present barriers to children who have yet learned how to write. Existing applications which utilize pen-input devices better mimic the physical act of writing, but few provide useful feedback to the users. This thesis presents a system specifically designed to serve as a useful tool in teaching children how to draw basic shapes, and helping them develop basic drawing and writing skills. The system uses a combination of sketch recognition techniques to interpret the handwritten strokes from sketches of the children, and then provides intelligent feedback based on what they draw. Our approach provides a virtual coach to assist teachers teaching the critical skills of drawing and handwriting. We do so by guiding children through a set of exercises of increasing complexity according to their progress, and at the same time keeping track of students' performance and engagement, giving them differentiated instruction and feedback. Our system would be like a virtual Teaching Assistant for Young Kids, hence we call it TAYouKi. We collected over five hundred hand-drawn shapes from grownups that had a clear understanding of what a particular geometric shape should look like. We used this data to test the recognition of our system. Following, we conducted a series of case studies with children in age group three to six to test the interactivity efficacy of the system. The studies served to gain important insights regarding the research challenges in different domains. Results suggest that our approach is appealable and engaging to children and can help in more effectively teach them how to draw and write.

Vides Ceron, Francisco

2012-08-01T23:59:59.000Z

185

Effect of synthetic ANP on renal and loop of Henle functions in the young rat  

SciTech Connect

The present studies were undertaken to determine, by recollection micropuncture, the effect of a synthetic atrial natriuretic peptide (ANP) on the absolute and fractional deliveries of water and sodium to the juxtamedullary end-descending limb. Two groups of young female Munich-Wistar rats were studied: 1) control received the vehicle only; and 2) ANP received a prime followed by the constant infusion of a synthetic rat atrial peptide (28 amino acids). With the infusion of ANP, clearance of p-( UC)aminohippurate (( UC(PAH) and glomerular filtration rate (GFR) fell significantly. Despite this fall in GFR and renal plasma flow, ANP produced a 2-fold increase in urine volume and a 10-fold increase in sodium excretion. Absolute and fractional sodium deliveries to the end-descending limb increased by approx.30% in the ANP group, whereas mean juxtamedullary single-nephron glomerular filtration rate (SNGFR) remained stable. In three additional rats prepared for micropuncture of the superficial end-accessible proximal tubule, ANP reduced cortical SNGFR by approx.15%. By contrast, GFR did not decline in response to ANP in larger rats, when treated identically. The authors conclude that 1) in young rats ANP can produce a natriuresis in the absence of a rise in GFR; 2) the fall in GFR observed following ANP is due presumably to the immaturity of the animals used in these studies; and 3) ANP produces a rise in absolute and fractional water and sodium deliveries to the end-descending limb that cannot be attributed to a change in SNGFR. The relatively small rise in fractional sodium delivery to the end-descending limb, most probably due to inhibition of sodium and water reabsorption in the juxtamedullary proximal tubule and/or thin descending limb, accounts for only a smallproportion of sodium excretion in the final urine.

Roy, D.R.

1986-08-01T23:59:59.000Z

186

Comprehensive tables giving physical data and thermal energy estimates for young igneous systems of the United States  

DOE Green Energy (OSTI)

Two tables are presented. The first is a comprehensive table of 157 young igneous systems in the western United States, giving locations, physical data, and thermal energy estimates, where appropriate for each system. The second table is a list of basaltic fields probably less than 10,000 years old in the western United States.

Smith, R.L.; Shaw, H.R.; Leudke, R.G.; Russell, S.L.

1978-01-01T23:59:59.000Z

187

COMPARISON OF CONVECTIVE OVERSHOOTING MODELS AND THEIR IMPACT ON ABUNDANCES FROM INTEGRATED LIGHT SPECTROSCOPY OF YOUNG (<3 Gyr) STAR CLUSTERS  

Science Conference Proceedings (OSTI)

As part of an ongoing program to measure detailed chemical abundances in nearby galaxies, we use a sample of young- to intermediate-age clusters in the Large Magellanic Cloud with ages of 10 Myr-2 Gyr to evaluate the effect of isochrone parameters, specifically core convective overshooting, on Fe abundance results from high-resolution, integrated light spectroscopy. In this work we also obtain fiducial Fe abundances from high-resolution spectroscopy of the cluster individual member stars. We compare the Fe abundance results for the individual stars to the results from isochrones and integrated light spectroscopy to determine whether isochrones with convective overshooting should be used in our integrated light analysis of young- to intermediate-age (10 Myr-3 Gyr) star clusters. We find that when using the isochrones from the Teramo group, we obtain more accurate results for young- and intermediate-age clusters over the entire age range when using isochrones without convective overshooting. While convective overshooting is not the only uncertain aspect of stellar evolution, it is one of the most readily parameterized ingredients in stellar evolution models, and thus important to evaluate for the specific models used in our integrated light analysis. This work demonstrates that our method for integrated light spectroscopy of star clusters can provide unique tests for future constraints on stellar evolution models of young- and intermediate-age clusters.

Colucci, Janet E.; Bernstein, Rebecca A., E-mail: jcolucci@ucolick.org, E-mail: rab@ucolick.org [Department of Astronomy and Astrophysics, 1156 High Street, UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States)

2012-04-20T23:59:59.000Z

188

An Underwater Communication and Sensing Testbed in Marina del Rey Andrew Goodney, Young H. Cho, John Heidemann, John Wroclawski  

E-Print Network (OSTI)

An Underwater Communication and Sensing Testbed in Marina del Rey Andrew Goodney, Young H. Cho, and communication underwater is increasingly important to scientists who study the oceans, rivers, and lakes, as government and industry seek to observe, protect, exploit, and control resources underwater. With growing

Heidemann, John

189

Nonlinear Dynamics in an OLG Growth Model with Young and Old Age Labour Supply: The Role of Public Health Expenditure  

Science Conference Proceedings (OSTI)

This study analyses the dynamics of a two-dimensional overlapping generations economy with young and old age labour supply. We show that the public provision of investments in health, which, in turn, affects the demand for material consumption of the ... Keywords: C62, C68, Chaos, I18, J22, Labour supply, O41, OLG model, Public health expenditure

Luca Gori; Mauro Sodini

2011-10-01T23:59:59.000Z

190

Laser Extinction in Laminar Inverse Diffusion Flames  

E-Print Network (OSTI)

Berkeley Linda G. Blevins † Sandia National Laboratories,Berkeley Linda G. Blevins Sandia National Laboratories,invaluable assistance. Sandia is a multiprogram laboratory

Macko, Kevin; Mikofski, Mark A; Fernandez-Pello, Carlos; Blevins, Linda G; Davis, Ronald W.

2005-01-01T23:59:59.000Z

191

Study of Four Young TeV Pulsar Wind Nebulae with a Spectral Evolution Model  

E-Print Network (OSTI)

We study four young Pulsar Wind Nebulae (PWNe) detected in TeV gamma-rays, G21.5-0.9, G54.1+0.3, Kes 75, and G0.9+0.1, using the spectral evolution model developed and applied to the Crab Nebula in our previous work. We model the evolution of magnetic field and particle distribution function inside a uniformly expanding PWN considering a time-dependent injection from the pulsar and radiative and adiabatic losses. Considering uncertainties in the interstellar radiation field (ISRF) and their distance, we study two cases for each PWN. Because TeV PWNe have a large TeV gamma-rays to X-rays flux ratio, the magnetic energy of the PWNe accounts for only a small fraction of the total energy injected (typically a few x 10^{-3}). The gamma-ray emission is dominated by inverse Compton scattering off the infrared photons of the ISRF. A broken power-law distribution function for the injected particles reproduces the observed spectrum well, except for G0.9+0.1. For G0.9+0.1, we do not need a low energy counterpart because...

Tanaka, Shuta J

2011-01-01T23:59:59.000Z

192

The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos  

E-Print Network (OSTI)

The energetic balance of the Standard Solar Model (SSM) results from an equilibrium between nuclear energy production, energy transfer, and photospheric emission. In this letter, we derive an order of magnitude of several % for the loss of energy in kinetic energy, magnetic energy, and X or UV radiation during the whole solar lifetime from the observations of the present Sun. We also estimate the mass loss from the observations of young solar analogs which could reach up to 30% of the current mass. We deduce new models of the present Sun, their associated neutrino fluxes, and their internal sound-speed profile. This approach sheds quantitative lights on the disagreement between the sound speed obtained by helioseismology and the sound speed derived from the SSM including the updated photospheric CNO abundances, based on recent observations. We conclude that about 20% of the present discrepancy could come from the incorrect description of the early phases of the Sun, its activity, its initial mass and mass-loss history. This study has obvious consequences on the solar system formation and the early evolution of the closest planets.

Sylvaine Turck-Chieze; Laurent Piau; Sébastien Couvidat

2011-03-14T23:59:59.000Z

193

CLOSE STELLAR ENCOUNTERS IN YOUNG, SUBSTRUCTURED, DISSOLVING STAR CLUSTERS: STATISTICS AND EFFECTS ON PLANETARY SYSTEMS  

SciTech Connect

Both simulations and observations indicate that stars form in filamentary, hierarchically clustered associations, most of which disperse into their galactic field once feedback destroys their parent clouds. However, during their early evolution in these substructured environments, stars can undergo close encounters with one another that might have significant impacts on their protoplanetary disks or young planetary systems. We perform N-body simulations of the early evolution of dissolving, substructured clusters with a wide range of properties, with the aim of quantifying the expected number and orbital element distributions of encounters as a function of cluster properties. We show that the presence of substructure both boosts the encounter rate and modifies the distribution of encounter velocities compared to what would be expected for a dynamically relaxed cluster. However, the boost only lasts for a dynamical time, and as a result the overall number of encounters expected remains low enough that gravitational stripping is unlikely to be a significant effect for the vast majority of star-forming environments in the Galaxy. We briefly discuss the implications of this result for models of the origin of the solar system, and of free-floating planets. We also provide tabulated encounter rates and orbital element distributions suitable for inclusion in population synthesis models of planet formation in a clustered environment.

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

2013-06-01T23:59:59.000Z

194

A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFS  

SciTech Connect

We present a near-infrared (0.9-2.4 {mu}m) spectroscopic study of 73 field ultracool dwarfs having spectroscopic and/or kinematic evidence of youth ( Almost-Equal-To 10-300 Myr). Our sample is composed of 48 low-resolution (R Almost-Equal-To 100) spectra and 41 moderate-resolution spectra (R {approx}> 750-2000). First, we establish a method for spectral typing M5-L7 dwarfs at near-IR wavelengths that is independent of gravity. We find that both visual and index-based classification in the near-IR provides consistent spectral types with optical spectral types, though with a small systematic offset in the case of visual classification at J and K band. Second, we examine features in the spectra of {approx}10 Myr ultracool dwarfs to define a set of gravity-sensitive indices based on FeH, VO, K I, Na I, and H-band continuum shape. We then create an index-based method for classifying the gravities of M6-L5 dwarfs that provides consistent results with gravity classifications from optical spectroscopy. Our index-based classification can distinguish between young and dusty objects. Guided by the resulting classifications, we propose a set of low-gravity spectral standards for the near-IR. Finally, we estimate the ages corresponding to our gravity classifications.

Allers, K. N. [Department of Physics and Astronomy, Bucknell University, Lewisburg, PA 17837 (United States); Liu, Michael C., E-mail: k.allers@bucknell.edu [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

2013-08-01T23:59:59.000Z

195

Can gas in young debris disks be constrained by their radial brightness profiles?  

E-Print Network (OSTI)

Disks around young stars are known to evolve from optically thick, gas-dominated protoplanetary disks to optically thin, almost gas-free debris disks. It is thought that the primordial gas is largely removed at ages of ~10 Myr, but it is difficult to discern the true gas densities from gas observations. This suggests using observations of dust: it has been argued that gas, if present with higher densities, would lead to flatter radial profiles of the dust density and surface brightness than those actually observed. However, here we show that these profiles are surprisingly insensitive to variation of the parameters of a central star, location of the dust-producing planetesimal belt, dustiness of the disk and - most importantly - the parameters of the ambient gas. This result holds for a wide range of gas densities (three orders of magnitude), for different radial distributions of the gas temperature, and different gas compositions. The brightness profile slopes of -3...-4 we find are the same that were theore...

Krivov, Alexander V; Brandeker, Alexis; Thébault, Philippe

2009-01-01T23:59:59.000Z

196

High-resolution spectropolarimetric of k Cet: A proxy for the young Sun  

E-Print Network (OSTI)

Among the solar proxies studied in the Sun in Time k Cet (HD 20630) stands out as potentially having a mass very close to solar and a young age. On this study, we monitored the magnetic field and the chromospheric activity from the Ca II H & K lines of k Cet. We used the Least-Square-Deconvolution (LSD, Donati et al. 1997) by simultaneously extracting the information contained in all 8,000 photospheric lines of the echelogram (K1 type star). To reconstruct a reliable magnetic map and characterize the surface differential rotation of k Cet we used 14 exposures spread over 2 months, in order to cover at least two rotational cycles (Prot ~ 9.2 days). The LSD technique was applied to detect the Zeeman signature of the magnetic field in each of our 14 observations and to measure its longitudinal component. In order to reconstruct the magnetic field geometry of k Cet, we applied the Zeeman Doppler Imaging (ZDI) inversion method. ZDI revealed a structure in the radial magnetic field consisting of a polar magneti...

Nascimento, J D do; Marsden, S; de Mello, G F Porto; Ribas, I; Jeffers, S; Castro, M; Guinan, E

2013-01-01T23:59:59.000Z

197

NEW BROWN DWARF COMPANIONS TO YOUNG STARS IN SCORPIUS-CENTAURUS  

Science Conference Proceedings (OSTI)

We present the discoveries of three faint companions to young stars in the Scorpius-Centaurus region, imaged with the NICI instrument on Gemini South. We have confirmed all three companions through common proper motion tests. Follow-up spectroscopy has confirmed two of them, HIP 65423 B and HIP 65517 B, to be brown dwarfs, while the third, HIP 72099 B, is more likely a very low mass star just above the hydrogen burning limit. The detection of wide companions in the mass range of {approx}40-100 M{sub jup} complements previous work in the same region, reporting detections of similarly wide companions with lower masses, in the range of {approx}10-30 M{sub jup}. Such low masses near the deuterium burning limit have raised the question of whether those objects formed like planets or stars. The existence of intermediate objects as reported here could represent a bridge between lower-mass companions and stellar companions, but in any case demonstrate that mass alone may not provide a clear-cut distinction for the formation of low-mass companions to stars.

Janson, Markus [Department of Astrophysical Sciences, Princeton University, Princeton, NJ (United States); Jayawardhana, Ray; Bonavita, Mariangela [Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON (Canada); Girard, Julien H. [European Southern Observatory, Santiago (Chile); Lafreniere, David [Department of Physics, University of Montreal, Montreal, QC (Canada); Gizis, John [Department of Physics and Astronomy, University of Delaware, Newark, DE (United States); Brandeker, Alexis, E-mail: janson@astro.princeton.edu [Department of Astronomy, Stockholm University, Stockholm (Sweden)

2012-10-10T23:59:59.000Z

198

Difficulty Accessing Syringes Mediates the Relationship Between Methamphetamine Use and Syringe Sharing Among Young Injection Drug Users  

E-Print Network (OSTI)

Ó The Author(s) 2010. This article is published with open access at Springerlink.com Abstract Injection drug users (IDU) who use methamphetamine (MA) are at an increased risk of HIV infection due to engagement in injection-related risk behavior including syringe sharing. In this cohort study of young IDU aged 18-30, we investigated the relationship between injection MA use and syringe sharing, and whether difficulty accessing sterile syringes mediated this association. Behavioral questionnaires were completed by 384 IDU in Vancouver, Canada between October 2005 and May 2008. Generalized estimating equations were used to estimate direct and indirect effects. The median age of participants was 24 (IQR: 22–27) and 214 (55.7%) were male. Injecting MA was independently associated with syringe sharing. Mediation analyses revealed that difficulty accessing sterile syringes partially mediated the association between injecting MA and syringe sharing. Interventions to reduce syringe sharing among young methamphetamine injectors

Evan Wood; Thomas L. Patterson; Thomas Kerr; E. Wood; T. Kerr; T. L. Patterson

2011-01-01T23:59:59.000Z

199

Overcoming Obstacles to Mobility for Apprentices and Other Young People in Vocational Education and Training Final Report  

E-Print Network (OSTI)

This document acts as the final report of the ‘Study on the obstacles to transnational mobility faced apprentices and other young people in initial vocational training and on ways of overcoming them ’ also referred to as the MoVE-iT project. The report was financed and prepared for the use of the European Commission, Directorate-General for Education and Culture under contract nr 2005-4579/001 PIL-PILOTP.

unknown authors

2007-01-01T23:59:59.000Z

200

The Meaning of Success: Young Women and High Academic Achievement in Rapidly Developed Areas. A Comparative Study of Contemporary Rural Vermont, USA and Leinster, Ireland.  

E-Print Network (OSTI)

??This thesis is an in-depth, comparative international study on young women’s high academic achievement in rural Leinster (Ireland) and Vermont (USA). The research analyses how… (more)

Fuller, Wendy Irene

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" 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

Peluchi : product development of a programmable robotic toy to stimulate interest in the fields of science and technology amongst young girls  

E-Print Network (OSTI)

Statistically speaking, science, technology, and engineering are male dominated fields. Peluchi is a second-generation prototype of a programmable robotic toy targeted towards young girls in hope of promoting more interest ...

Vu, My (My H.)

2011-01-01T23:59:59.000Z

202

A PAN-STARRS + UKIDSS SEARCH FOR YOUNG, WIDE PLANETARY-MASS COMPANIONS IN UPPER SCORPIUS  

SciTech Connect

We have combined optical and NIR photometry from Pan-STARRS 1 and UKIDSS to search the young (5-10 Myr) star-forming region of Upper Scorpius for wide ( Almost-Equal-To 400-4000 AU) substellar companions down to {approx}5 M{sub Jup}. Our search is Almost-Equal-To 4 mag deeper than previous work based on the Two Micron All Sky Survey. We identified several candidates around known stellar members using a combination of color selection and spectral energy distribution fitting. Our follow-up spectroscopy has identified two new companions as well as confirmed two companions previously identified from photometry, with spectral types of M7.5-M9 and masses of {approx}15-60 M{sub Jup}, indicating a frequency for such wide substellar companions of {approx}0.6% {+-} 0.3%. Both USco 1610-1913B and USco 1612-1800B are more luminous than expected for their spectral type compared with known members of Upper Sco. HIP 77900B has an extreme mass ratio (M{sub 2}/M{sub 1} Almost-Equal-To 0.005) and an extreme separation of 3200 AU. USco 1602-2401B also has a very large separation of 1000 AU. We have also confirmed a low-mass stellar companion, USco 1610-2502B (730 AU, M5.5). Our substellar companions appear both non-coeval with their primary stars according to evolutionary models and, as a group, are systematically more luminous than the Upper Sco cluster sequence. One possible reason for these luminosity discrepancies could be different formation processes or accretion histories for these objects.

Aller, Kimberly M.; Kraus, Adam L.; Liu, Michael C.; Burgett, William S.; Chambers, Kenneth C.; Hodapp, Klaus W.; Kaiser, Nick; Magnier, Eugene A. [Institute of Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Price, Paul A. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)

2013-08-10T23:59:59.000Z

203

Shaking things up: young infants' use of sound information for object individuation  

E-Print Network (OSTI)

Object individuation, the capacity to determine whether two perceptual encounters belong to the same object or two different objects, is one of the most basic cognitive abilities and provides a foundation for infants’ understanding of the physical world. Yet very little work has been done to explore infants’ use of auditory information to individuate objects. The first research to investigate infants’ use of sound information to individuate objects was reported by Wilcox et al. (2006), who used a violation-ofexpectation task to examine the extent to which 4.5-month-olds use differences in sound to individuate objects. The results suggested that 4.5-month-olds use property-rich sounds (sounds intimately related to an objects’ physical, amodal properties) but not property-poor sounds (sounds that are more contrived) to distinguish the identity of objects involved in occlusion events. The current study investigated infants’ sensitivity to these two types of sounds within the context of a search task. Three experiments were conducted with infants aged 5 to 7 months. The outcome of these experiments builds and extends on the findings of Wilcox et al. in three ways. First, converging evidence was obtained, using a search task, that young infants are more sensitive to property-rich than property-poor sounds. Second, more detailed information was obtained on infants’ interpretation of samesounds events (two identical, rather than two different, sounds). Finally, possible explanations for infants’ greater sensitivity to property-rich sounds were assessed. The outcome of these studies, collectively, provides insight into the types of sounds that infants use to identify objects and the reasons why some sounds are more salient to infants than others.

Smith, Tracy Rebecca

2007-12-01T23:59:59.000Z

204

OPTICAL PHOTOMETRIC GTC/OSIRIS OBSERVATIONS OF THE YOUNG MASSIVE ASSOCIATION CYGNUS OB2  

Science Conference Proceedings (OSTI)

In order to fully understand the gravitational collapse of molecular clouds, the star formation process, and the evolution of circumstellar disks, these phenomena must be studied in different Galactic environments with a range of stellar contents and positions in the Galaxy. The young massive association Cygnus OB2, in the Cygnus-X region, is a unique target to study how star formation and the evolution of circumstellar disks proceed in the presence of a large number of massive stars. We present a catalog obtained with recent optical observations in the r, i, z filters with OSIRIS, mounted on the 10.4 m Gran Telescopio CANARIAS telescope, which is the deepest optical catalog of Cyg OB2 to date. The catalog consists of 64,157 sources down to M = 0.15 M{sub Sun} at the adopted distance and age of Cyg OB2. A total of 38,300 sources have good photometry in all three bands. We combined the optical catalog with existing X-ray data of this region, in order to define the cluster locus in the optical diagrams. The cluster locus in the r - i versus i - z diagram is compatible with an extinction of the optically selected cluster members in the 2.64{sup m} < A{sub V} < 5.57{sup m} range. We derive an extinction map of the region, finding a median value of A{sub V} = 4.33{sup m} in the center of the association, decreasing toward the northwest. In the color-magnitude diagrams, the shape of the distribution of main-sequence stars is compatible with the presence of an obscuring cloud in the foreground {approx}850 {+-} 25 pc from the Sun.

Guarcello, M. G.; Wright, N. J.; Drake, J. J.; Aldcroft, T.; Kashyap, V. L. [Smithsonian Astrophysical Observatory, MS-67, 60 Garden Street, Cambridge, MA 02138 (United States); Garcia-Alvarez, D. [Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife (Spain); Drew, J. E. [CAR/STRI, University of Hertfordshire, College Lane, Hatfield, AL10 9AB (United Kingdom)

2012-10-15T23:59:59.000Z

205

Application of composted pulp and paper mill sludge to a young pine plantation  

SciTech Connect

Disposing of sludge recovered from the effluent stream of pulp and paper mills has traditionally involved landfilling. Shortages in landfill space and increasingly stringent environmental regulations in many countries have forced the industry to seek alternative disposal options. The authors assessed the feasibility of compost-recycling a primary pulp and paper mill sludge (PMS) for use as a nutrient-releasing mulch in plantation forestry. The effects of the composted PMS on the growth, nutrition, water relations, and week suppression in a 3-yr-old plantation of radiata pine (Pinus radiata D.Don) on an infertile sandy soil in southern Tasmania were assessed. Compost was applied to the surface without incorporation in 0.5-m wide bands in tree rows at rates of 0, 20, 40, and 60 metric t ha{sup {minus}1} (dry matter). One year after application of compost, the percentage increase in stem diameter was 40 to 66% greater than that achieved in untreated plots, with better growth at the highest compost application rate. Improved growth of radiata pine after application of compost was primarily attributable to a 17 to 37% increase in the concentration of foliar N and to decreased water stress in amended plots. Nitrogen released from the compost was mostly absorbed by plant roots within the first 20 cm of the soil profile, with no significant movement beyond this depth range. Application of compost prepared from PMS to young stands of radiata pine was found to be acceptable recycling alternative for this material, capable of improving plantation productivity.

Jackson, M.J.; Line, M.A.; Wilson, S.; Hetherington, S.J.

2000-04-01T23:59:59.000Z

206

Report on enhancing young scholars in science and technology the Center for Excellence in Education  

Science Conference Proceedings (OSTI)

The present stock and flow of highly talented young persons engaged in the global discovery and application of science and technology are critical to the future pace of innovation. Historically, the world`s largest reservoirs of scientists and engineers have been in the Western economies. Overtime, however, Asia has begun to build equivalent pools of scientists and engineers among their university graduates. According to 1993 data from the National Science Foundation and the UNESCO World Science Report, Germany leads all economies with a 67% ratio of science and engineering degrees to total first university degrees compared to the United States with a distant fifth place at 32% behind Italy, Mexico and Poland. If the nation is to keep its scientific and technological prowess, it must capture its very best talent in the science and technology fields. The question is then raised as to the source within the United States of the science and technology talent pool. While between 1978 and 1991 there was an overall decline in male participation in undergraduate (-9%) and graduate degrees (-12%), the number of women receiving undergraduate (+8%) and graduate degrees (+34%) rose dramatically. These numbers are encouraging for women`s participation overall, however, women earn only a small percentage of physical science and engineering degrees. Why are there so few women in mathematics, engineering, and the physical sciences? The answers are complex and begin early in a woman`s exposure to science and mathematics. This report presents results on a study of careers of alumni from the Research Science Institute. Investigations were concerned with the timing of decision processes concerned with the sciences and math and factors that influenced people to turn away from or proceed with careers in science and math.

NONE

1996-09-30T23:59:59.000Z

207

A Sample of Very Young Field L Dwarfs and Implications for the Brown Dwarf "Lithium Test" at Early Ages  

E-Print Network (OSTI)

Using a large sample of optical spectra of late-type dwarfs, we identify a subset of late-M through L field dwarfs that, because of the presence of low-gravity features in their spectra, are believed to be unusually young. From a combined sample of 303 field L dwarfs, we find observationally that 7.6+/-1.6% are younger than 100 Myr. This percentage is in agreement with theoretical predictions once observing biases are taken into account. We find that these young L dwarfs tend to fall in the southern hemisphere (Dec < 0 deg) and may be previously unrecognized, low-mass members of nearby, young associations like Tucana-Horologium, TW Hydrae, beta Pictoris, and AB Doradus. We use a homogeneously observed sample of roughly one hundred and fifty 6300-10000 Angstrom spectra of L and T dwarfs taken with the Low-Resolution Imaging Spectrometer at the W. M. Keck Observatory to examine the strength of the 6708-A Li I line as a function of spectral type and further corroborate the trends noted by Kirkpatrick et al. (2000). We use our low-gravity spectra to investigate the strength of the Li I line as a function of age. The data weakly suggest that for early- to mid-L dwarfs the line strength reaches a maximum for a few 100 Myr, whereas for much older (few Gyr) and much younger (<100 Myr) L dwarfs the line is weaker or undetectable. We show that a weakening of lithium at lower gravities is predicted by model atmosphere calculations, an effect partially corroborated by existing observational data. Larger samples containing L dwarfs of well determined ages are needed to further test this empirically. If verified, this result would reinforce the caveat first cited in Kirkpatrick et al. (2006) that the lithium test should be used with caution when attempting to confirm the substellar nature of the youngest brown dwarfs.

J. Davy Kirkpatrick; Kelle L. Cruz; Travis S. Barman; Adam J. Burgasser; Dagny L. Looper; C. G. Tinney; Christopher R. Gelino; Patrick J. Lowrance; James Liebert; John M. Carpenter; Lynne A. Hillenbrand; John R. Stauffer

2008-08-22T23:59:59.000Z

208

NIST Reference Materials Are 'Gold Standard' for Bio ...  

Science Conference Proceedings (OSTI)

NIST Reference Materials Are 'Gold Standard' for Bio-Nanotech Research. ... The National Institute of Standards and Technology (NIST) has issued its ...

2013-03-15T23:59:59.000Z

209

Argonne CNM: 2013 Seminar Series  

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

(i.e., multiferroicity). April 10, 2013 "Scanning probe characterization of energy nanomaterials and devices," by Liwei Chen, Suzhou Institute of Nanotech and Nanobionics,...

210

Special Topics: Nanomaterials: Web resources  

Science Conference Proceedings (OSTI)

WEB: Material Innovations: from Nanotech to Biotech and Beyond! Presentations from the 2007 ACS Presidential Session, 0, 759, Todd Osman, 1/9/2008 7:45 ...

211

DOE Hydrogen and Fuel Cells Program: SBIR/STTR Phase I Release...  

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

as hydrogen and fuel cells that could improve manufacturing processes, reduce reliance on foreign oil, and generate electricity from renewable sources. Applied Nanotech, Inc. of...

212

Small Business Innovation Research (SBIR) Hydrogen Program New...  

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

city, State XIII.5 Ultra-Lightweight High Pressure Hydrogen Fuel Tanks Reinforced with Carbon Nanotubes (Phase II Project) Applied Nanotech, Inc. Austin, TX XIII.6 New High...

213

Mentarix Pte Ltd | Open Energy Information  

Open Energy Info (EERE)

producing efficiency enhancement components for use on all type of solar cells, using quantum dot technology and nanotech structuring. References Mentarix Pte Ltd1 LinkedIn...

214

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

215

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

SciTech Connect

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

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

2013-01-01T23:59:59.000Z

216

Workshop Advisory Committee Gabe Aeppli (LCN London)  

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

Workshop Advisory Committee Gabe Aeppli (LCN London) Massimo Altarelli (Euro-XFEL ) Andrea Cavalleri (Oxford/DESY) Lin Chen (Argonne/Northwestern) George Crabtree (Argonne) Helmut Dosch (DESY) Janos Hajdu (Uppsala) Sol Gruner (Cornell) Jerry Hastings (SLAC) Rus Hemley (Carnegie Institute) Eric Isaacs (Argonne) Ben Larson (Oak Ridge) Richard Lee (Livermore) Ingolf Lindau (SLAC) Denny Mills (Argonne) Keith Moffat (Univ. Chicago) David Moncton (MIT) Harald Reichert (ESRF) Jo Stöhr (SLAC) Lou Terminello (PNNL) Linda Young (Argonne) Soichi Wakatsuki (KEK) Workshop Coordinator Anne Owens Workshop Chairs Uwe Bergmann, SLAC National Accelerator Laboratory Gopal Shenoy, Argonne National Laboratory Edgar Weckert, Deutsches Elektronen-Synchrotron, DES

217

Weight-related Beliefs, Behaviors, and Social Networks of Obese, Young Adult African- American Women: Implications for Healthy Weight Interventions  

E-Print Network (OSTI)

Obesity is a public health concern that affects over 30% of Americans. Approximately 78% of African-American women are overweight/obese, as compared to 46% of Caucasian women. Obese African-American women are at higher risk for associated morbidities (e.g., hypertension, type II diabetes, select cancers, and early mortality) as compared to non-Hispanic whites. Weight gain after young adulthood (ages 20-35) is associated with an increased risk of cardiovascular disease and other health problems later in life. Research that seeks to explain, predict, or control obesity among African-American women has focused on individual behavior change. Few studies have addressed the social contexts within which these behaviors occur. The purpose of this exploratory study was to examine the weight-related beliefs, behaviors, and social network characteristics of obese, young adult African-American women. A conceptual framework based on social support and social network theory guided the design of the study. Ten African-American women between the ages of 20 and 35, self-described as “plus-size” or “full-figured,” completed initial informal conversations about weight-related issues and concerns and semi-structured, in-depth face-to-face interviews. Five participants were randomly selected to complete social network profiles to identify potential social influences on weight-related beliefs and behaviors. Results of the initial conversations revealed approximately half of the participants were class III obesity (BMI > 40), reported overall good health, and 70% participated in physical activity at least one day a week. Semi-structured interviews results disclosed two primary reasons for unsuccessful long-term weight loss: (a) inconsistent weight loss behaviors and (b) lack of accountability. Weight-related beliefs and behaviors of study participants were similar to those reported for older adult African-American women. Similarities included (a) mixed levels of body satisfaction; (b) the belief that health is not determined by weight; (c) sedentary lifestyles and; (d) social support from family and friends impacts long-term weight loss success. The five social network profiles indicated participants’ networks are small, comprised of at least two overweight/obese females, and exhibited positive social support behaviors. Social networks included positive, negative, and non-positive relationships. Social support for weight loss is shared among network members through face-to-face interactions, phone conversations, and use of social media tools such as Facebook, Twitter, and text messaging. Future healthy weight studies would benefit from comprehensive analyses of the social networks of obese, young adult African-American women, inclusive of interviews with social network members. Culture-based healthier weight interventions that organize social support networks through social media tools are promising strategies for promoting healthy weight management among obese, young adult African-American women.

Rollins, Brandy 1982-

2012-12-01T23:59:59.000Z

218

H2 carrier gas dependence of Young's modulus and hardness of chemical vapor deposited polycrystalline 3C-SiC thin films  

Science Conference Proceedings (OSTI)

This paper presents the mechanical properties of poly (polycrystalline) 3C-SiC thin films according to 0%, 7%, and 10% carrier gas (H"2) concentrations using nano-indentation. When H"2 concentration was 10%, it has been proved that the mechanical properties, ... Keywords: AFM, Hardness, Nano-indentation, Poly 3C-SiC, Young's modulus

Gwiy-Sang Chung; Ki-Bong Han

2008-12-01T23:59:59.000Z

219

Internationalization of a Talking Head Ouni, S. Massaro, D.W., Cohen, M.M., Young, K. & Jesse, A.(2003). Internationalization  

E-Print Network (OSTI)

Internationalization of a Talking Head Ouni, S. Massaro, D.W., Cohen, M.M., Young, K. & Jesse, A and providing the test facilities. REFERENCES [1] D.W. Massaro, Perceiving Talking Faces, From Speech Perception to a Behavioral Principle, MIT Press, 1998. [2] A. Bosseler and D.W. Massaro, "Development and Evaluation

Cohen, Michael M.

220

Similar Survival With Breast Conservation Therapy or Mastectomy in the Management of Young Women With Early-Stage Breast Cancer  

Science Conference Proceedings (OSTI)

Purpose: To evaluate survival outcomes of young women with early-stage breast cancer treated with breast conservation therapy (BCT) or mastectomy, using a large, population-based database. Methods and Materials: Using the Surveillance, Epidemiology, and End Results (SEER) database, information was obtained for all female patients, ages 20 to 39 years old, diagnosed with T1-2 N0-1 M0 breast cancer between 1990 and 2007, who underwent either BCT (lumpectomy and radiation treatment) or mastectomy. Multivariable and matched pair analyses were performed to compare overall survival (OS) and cause-specific survival (CSS) of patients undergoing BCT and mastectomy. Results: A total of 14,764 women were identified, of whom 45% received BCT and 55% received mastectomy. Median follow-up was 5.7 years (range, 0.5-17.9 years). After we accounted for all patient and tumor characteristics, multivariable analysis found that BCT resulted in OS (hazard ratio [HR], 0.93; 95% confidence interval [CI], 0.83-1.04; p = 0.16) and CSS (HR, 0.93; CI, 0.83-1.05; p = 0.26) similar to that of mastectomy. Matched pair analysis, including 4,644 BCT and mastectomy patients, confirmed no difference in OS or CSS: the 5-, 10-, and15-year OS rates for BCT and mastectomy were 92.5%, 83.5%, and 77.0% and 91.9%, 83.6%, and 79.1%, respectively (p = 0.99), and the 5-, 10-, and 15-year CSS rates for BCT and mastectomy were 93.3%, 85.5%, and 79.9% and 92.5%, 85.5%, and 81.9%, respectively (p = 0.88). Conclusions: Our analysis of this population-based database suggests that young women with early-stage breast cancer have similar survival rates whether treated with BCT or mastectomy. These patients should be counseled appropriately regarding their treatment options and should not choose a mastectomy based on the assumption of improved survival.

Mahmood, Usama, E-mail: usama.mahmood@gmail.com [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States); Morris, Christopher; Neuner, Geoffrey [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States); Koshy, Matthew [Department of Cellular and Radiation Oncology, University of Chicago, Chicago, Illinois (United States)] [Department of Cellular and Radiation Oncology, University of Chicago, Chicago, Illinois (United States); Kesmodel, Susan; Buras, Robert [Department of Surgery, University of Maryland, Baltimore, Maryland (United States)] [Department of Surgery, University of Maryland, Baltimore, Maryland (United States); Chumsri, Saranya; Bao Ting; Tkaczuk, Katherine [Department of Medicine, University of Maryland, Baltimore, Maryland (United States)] [Department of Medicine, University of Maryland, Baltimore, Maryland (United States); Feigenberg, Steven [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)

2012-08-01T23:59:59.000Z

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221

NEWS FROM WASHINGTON STATE UNIVERSITY'S OFFICE OF EQUITY AND DIVERSITY MARCH 3, 2006November 30, 2007 News from Washington State University Extension http://cahnrsnews.wsu.edu/extensiontoday Linda Kirk Fox  

E-Print Network (OSTI)

Soil Scientist NMSU's Extension Plant Sciences Lupe Garcia Owner Garcia Farms Ed Hughs Research Leader in Chile Peppers Report 20: Using a Color Sorter to Remove Sticks from Mechanically Harvested Red Chile of a Prototype Mechanical Gap Sorter for Mechanically Harvested Red Chile Report 26: Good Agricultural Practices

Collins, Gary S.

222

Localization of shallow gas deposits and uncontrolled gas flows in young and unconsolidated sediments by geophysical methods  

SciTech Connect

The great mass of Neogene sediments in the Hungarian basin, where several hydrocarbon accumulations are known, is affected by Pliocene strike-slip movements, resulting in many [open quotes]flower structures.[close quotes] The gas may migrate from the reservoirs upward to the surface along the faults. Thus, shallow gas deposits can be located in the young, unconsolidated sands. There are also several shallow gas deposits derived from uncontrolled gas flows. In Hungary, the shallow gas reservoirs, which are small but increasingly important, have not yet been explored properly. However, the depleting gas may pollute the water in the soil as well as cause explosions. Our purpose is to develop inexpensive, complete, and highly sophisticated field- and data-processing techniques and an integrated complex of geophysical methods in order to define the limits of shallow gas deposits. To avoid anomalous behavior on seismic sections of the depleting gas, we started from uncontrolled gas flows which require special velocity and amplitude vs. offset analyses. In addition, natural and controlled source electromagnetic/electric surveys with various parameters were applied. An industrial-scale seismic section over an uncontrolled gas flow, special sections over flower structures and geoelectric sections, and a magnetic map are presented. The integrated complex of geophysical methods outlined above is being developed in order to establish the conditions for the exploration of gas reservoirs which have been used close to their locality and which could be recovered inexpensively.

Csoergei, J.; Kummer, I.; Papa, A.; Sipos, J.; Solyom, I.; Takacs, E.; Timar, Z. (Eotvos Lorand Geophysical Institute of Hungary, Budapest (Hungary)); Keresztes, T. (MOL RT, Budapest (Hungary))

1993-09-01T23:59:59.000Z

223

Herschel/PACS observations of young sources in Taurus: the far-infrared counterpart of optical jets  

E-Print Network (OSTI)

Observations of the atomic and molecular line emission associated with jets and outflows emitted by young stellar objects can be used to trace the various evolutionary stages they pass through as they evolve to become main sequence stars. To understand the relevance of atomic and molecular cooling in shocks, and how accretion and ejection efficiency evolves with the source evolutionary state, we will study the far-infrared counterparts of bright optical jets associated with Class I and II sources in Taurus (T Tau, DG Tau A, DG Tau B, FS Tau A+B, and RW Aur). We have analysed Herschel/PACS observations of a number of atomic ([OI]63um, 145um, [CII]158um) and molecular (high-J CO, H2O, OH) lines, collected within the OTKP GASPS. To constrain the origin of the detected lines we have compared the FIR emission maps with the emission from optical-jets and millimetre-outflows, and the line fluxes and ratios with predictions from shock and disk models. All of the targets are associated with extended emission in the at...

Podio, L; Flower, D; Howard, C; Sandell, G; Mora, A; Aresu, G; Brittain, S; Dent, W F R; Pinte, C; White, G J

2012-01-01T23:59:59.000Z

224

The near-IR Surface Brightness Method applied to six Cepheids in the young LMC cluster NGC1866  

E-Print Network (OSTI)

We present new near-IR light curves for six Cepheids in the young blue LMC cluster NGC1866 as well as high precision radial velocity curves for ten Cepheids in NGC1866 and two in NGC2031. For the six Cepheids in NGC1866 with new J and K light curves we determine distances and absolute magnitudes by applying the near-IR surface brightness method. We find that the formal error estimates on the derived distances are underestimated by about a factor of two. We find excellent agreement between the absolute magnitudes for the low metallicity LMC Cepheids with the Period-Luminosity (P-L) relation determined by the near-IR surface brightness (ISB) method for Galactic Cepheids suggesting that the slope of the P-L relations for low metallicity and solar metallicity samples could be very similar in contrast to other recent findings. Still there appears to be significant disagreement between the observed slopes of the OGLE based apparent P-L relations in the LMC and the slopes derived from ISB analysis of Galactic Cepheids, and by inference for Magellanic Cloud Cepheids, indicating a possible intrinsic problem with the ISB method itself. Resolving this problem could reaffirm the P-L relation as the prime distance indicator applicable as well to metallicities significantly different from the LMC value.

Jesper Storm; Wolfgang P. Gieren; Pascal Fouque; Thomas G. Barnes III; Matias Gomez

2005-06-06T23:59:59.000Z

225

Estimation of Young's modulus and of hardness by ultra-low load hardness tests with a Vickers indenter  

SciTech Connect

The evaluation of the elastic-plastic properties of a material by using an ultra-low load hardness test requires a geometrical calibration that must take into account the imperfect form of the diamond indenter. In the present work, the Vickers indenter offset of the microindentation equipment was estimated using differently heat-treated steel samples. To this end, the dimensions of the indentations have been evaluated by two different methods: optical measurement of the diagonals and direct measurement of the penetration depth during the test. The elastic-plastic properties are then calculated from the analysis of the penetration depth/indentation load curves. The Young's modulus values determined for the different high-speed steel samples were very similar and close to the literature value for steel if the appropriate corrections are performed. The hardness values decrease when the determination procedure includes the geometrical correction of the indenter offset, and still further when using the total correction obtained by means of optical measurements of the indenter diagonal. Variation of the hardness values with the applied load is much less when the corrections are carried out.

Trindade, A.C. (Instituto Politecnico de Viseu (Portugal). Escola Superior de Tecnologia); Cavaleiro, A.; Fernandes, J.V. (Univ. de Coimbra (Portugal). Dept. de Engenharia Mecanica)

1994-07-01T23:59:59.000Z

226

Clumpy stellar winds and high-energy emission in high-mass binaries hosting a young pulsar  

E-Print Network (OSTI)

High-mass binaries hosting young pulsars can be powerful gamma-ray emitters. The stellar wind of the massive star in the system is expected to be clumpy. Since the high-energy emission comes from the pulsar-star wind interaction, the presence of clumps can affect the spectrum and variability of this radiation. We look for the main effects of the clumps on the two-wind interaction region and on the non-thermal radiation. A simple analytical model for the two-wind interaction dynamics was developed accounting for the lifetime of clumps under the pulsar-wind impact. This time plays a very important role with regard to the evolution of the clump, the magnetic field in the clump-pulsar wind interaction region, and the non-radiative and radiative cooling of the non-thermal particles. We also computed the high-energy emission produced at the interaction of long-living clumps with the pulsar wind. For reasonable parameters, the clumps will induce small variability on the X-ray and gamma-ray radiation. Sporadically, l...

Bosch-Ramon, V

2013-01-01T23:59:59.000Z

227

The young's modulus of 1018 steel and 67061-T6 aluminum measured from quasi-static to elastic precursor strain-rates  

Science Conference Proceedings (OSTI)

The assumption that Young's modulus is strain-rate invariant is tested for 6061-T6 aluminium alloy and 1018 steel over 10 decades of strain-rate. For the same billets of material, 3 quasi-static strain-rates are investigated with foil strain gauges at room temperature. The ultrasonic sound speeds are measured and used to calculate the moduli at approximately 10{sup 4} s{sup -1}. Finally, ID plate impact is used to generate an elastic pre-cursor in the alloys at a strain-rate of approximately 10{sup 6} s{sup -1} from which the longitudinal sound speed may be obtained. It is found that indeed the Young's modulus is strain-rate independent within the experimental accuracy.

Rae, Philip J [Los Alamos National Laboratory; Trujillo, Carl [Los Alamos National Laboratory; Lovato, Manuel [Los Alamos National Laboratory

2009-01-01T23:59:59.000Z

228

Anomalies in the Young modulus at structural phase transitions in rare-earth cobaltites RBaCo{sub 4}O{sub 7} (R = Y, Tm-Lu)  

SciTech Connect

The elastic properties of rare-earth cobaltites RBaCo{sub 4}O{sub 7} (R = Y, Tm-Lu) have been experimentally studied in the temperature range of 80-300 K. The strong softening of the Young modulus {Delta}E(T)/E{sub 0} Almost-Equal-To -(0.1-0.2) of cobaltites with Lu and Yb ions has been revealed, which is due to the instability of the crystal structure upon cooling and is accompanied by an inverse jump at the second-order structural phase transition. The softening of the Young modulus and the jump at the phase transition decrease by an order of magnitude and the transition temperature T{sub s} and hysteresis {Delta}T{sub s} increase from a compound with Lu to that with Tm. A large softening of the Young modulus at the structural transition in Lu- and Yb cobaltites indicates that the corresponding elastic constant goes to zero, whereas this constant in Tm cobaltite is not a 'soft' mode of the phase transition. It has been found that the structural phase transition in Lu- and Yb cobaltites is accompanied by a large absorption maximum at the phase transition point and an additional maximum in the low-temperature phase and absorption anomalies in Tm cobaltite is an order of magnitude smaller.

Kazei, Z. A., E-mail: kazei@plms.phys.msu.ru; Snegirev, V. V.; Andreenko, A. S. [Moscow State University (Russian Federation); Kozeeva, L. P. [Russian Academy of Sciences, Nikolaev Institute of Inorganic Chemistry, Siberian Branch (Russian Federation)

2011-08-15T23:59:59.000Z

229

Abstract for Ross Young  

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

Model has proven an extremely successful theory in describing the behaviour of nuclear and particle physics. The theoretical desire to restore simplicity in the fundamental...

230

YOUNG LEADER the - TMS  

Science Conference Proceedings (OSTI)

responsibility and ethics; multicultural, gender, and generational communication; and conflict resolution. Before and after the workshop, participants will have ...

231

Young Leaders Tutorial Lecture  

Science Conference Proceedings (OSTI)

Presented by: Dr. F.H. (Sam) Froes, University of Idaho Location: 230C, Orange County Convention Center When: Monday, February 10, 12:00 noon-1:30 p.m..

232

Young Jong Lee  

Science Conference Proceedings (OSTI)

... used to provide 3D chemical and orientational information for other ... Entropy and Time-Domain Kramers-Kronig Phase Retrieval Approaches are ...

2013-11-26T23:59:59.000Z

233

Young Professionals Program  

Science Conference Proceedings (OSTI)

Vice Chair Kinga Unocic, Past Chair Oak Ridge National Lab UnocicKA@ornl. gov, Saryu Fensin, Secretary Los Alamos National Lab saryuj@lanl.gov ...

234

Young Jack Pine Site  

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

NSA-YJP) The hut, tent, and dirt road from the flux tower The sun photometer on top of the hut The bottom of the YJP flux tower NSA-YJP taken at a low sun angle to show the subtle...

235

Won Young Park  

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

designed to accelerate the adoption of efficient technologies. He also supports a Korea project that is to demonstrate economic potential for energy efficiency improvement in...

236

Distribution of toenail selenium levels in young adult Caucasians and African Americans in the United States: The CARDIA Trace Element Study  

SciTech Connect

Background: Data on selenium (Se) levels in American young adults, especially in African Americans, are lacking. Objective: This study presented toenail Se distributions in American young adults of both genders, including both Caucasians and African Americans; and explored potential predictors of toenail Se levels. Data and methods: Data from the Coronary Artery Risk Development in Young Adults study among 4252 American young adults, aged 20-32 in 1987 was used to examine toenail Se levels by instrumental neutron-activation analysis. The distribution of Se levels was described and multivariable linear regression was used to examine potential modifiers of toenail Se concentration within ethnicity-gender subgroups. Results: The geometric mean of toenail Se in this cohort was 0.844 {mu}g/g (95% CI, 0.840-0.849 {mu}g/g) and the median was 0.837 {mu}g/g (95% CI, 0.833-0.844 {mu}g/g). Median levels from lowest to highest quintile were 0.691, 0.774, 0.838, 0.913 and 1.037 {mu}g/g. Se levels varied geographically, and were generally in accordance with its concentrations in local soil. Males, African Americans, current smokers, heavy drinkers and less educated participants were more likely to have low Se levels. Conclusion: This study suggests that toenail Se levels vary geographically depending on soil Se concentrations. In addition to gender, ethnicity and education level, smoking status and alcohol consumption are two important indicators of Se status since they are modifiable lifestyle factors. Findings from this study might aid public health professionals in identifying people at relatively high or low Se levels, so that chronic disease prevention efforts can be directed toward these subgroups. - Research highlights: {yields} Average of toenail Se levels in this cohort was 0.844 {mu}g/g (95% CI, 0.840-0.849 {mu}g/g). {yields} Toenail Se levels vary geographically depending on soil Se concentrations. {yields} Males, African Americans and less educated participants have low Se levels. {yields} Smoking status and alcohol consumption are two important indicators of Se status.

Xun, Pengcheng; Bujnowski, Deborah [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States) [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); Department of Epidemiology, Gillings School of Global Public Health, University of North Carolina at Chapel Hill, Chapel Hill, NC (United States); Liu, Kiang [Department of Preventive Medicine, Feinberg School of Medicine, Northwestern University, Chicago, IL (United States)] [Department of Preventive Medicine, Feinberg School of Medicine, Northwestern University, Chicago, IL (United States); Steve Morris, J. [Research Reactor Center, University of Missouri-Columbia, Columbia, MO (United States)] [Research Reactor Center, University of Missouri-Columbia, Columbia, MO (United States); Guo, Zhongqin [Department of Epidemiology and Biostatistics, School of Public Health, Ningxia Medical University, Ningxia (China) [Department of Epidemiology and Biostatistics, School of Public Health, Ningxia Medical University, Ningxia (China); Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); He, Ka, E-mail: kahe@unc.edu [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States) [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); Department of Epidemiology, Gillings School of Global Public Health, University of North Carolina at Chapel Hill, Chapel Hill, NC (United States)

2011-05-15T23:59:59.000Z

237

The long term dynamics of the solar radiative zone associated to new results from SoHO and young solar analogs  

E-Print Network (OSTI)

The Standard Solar Model (SSM) is no more sufficient to interpret all the observations of the radiative zone obtained with the SoHO satellite. We recall our present knowledge of this internal region and compare the recent results to models beyond the SSM assumptions. Then we discuss the missing processes and quantify some of them in using young analog observations to build a more realistic view of our star. This progress will be useful for solar-like stars observed by COROT and KEPLER.

Sylvaine Turck-Chieze; Sebastien Couvidat; Antonio Eff-Darwich; Vincent Duez; Rafael A. Garcia; Stephane Mathis; Savita Mathur; Laurent Piau; David Salabert

2011-09-19T23:59:59.000Z

238

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT PLANNING ALTERNATIVE5002013021 Prepared for: California Energy Commission Prepared by: Facet Decision Systems, Inc. #12-08-030 Prepared for: California Energy Commission Linda Spiegel Contract Manager Linda Spiegel Office Manager

239

Policy Flash 2013-54 Acquisition Certification Program Handbook 4th Edition  

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

Questions concerning this policy flash should be directed to Linda Ott of the Office Acquistion and Project Management, Professional Development DIvision, at (202) 287-5310 or at Linda.Ott@hq.doe.gov.

240

Satyriasis: The Pornographic Afterlife of Vaslav Nijinsky  

E-Print Network (OSTI)

in the Stag Film. ” Porn Studies. Ed. Linda Williams.The Autobiography of a Gay Porn Pioneer. LosAngeles : Alysonin the Stag Film,” Porn Studies, ed. Linda Williams (Durham,

Horowitz, Katie R.

2008-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" 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
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241

Self-Colonizing eEurope: The Information Society Merges onto the Information Superhighway  

E-Print Network (OSTI)

of the Pornographic Feature. ”  In Porn Studies, ed.  Linda of the Pornographic Feature,” in  Porn Studies, ed.  Linda Hit Teutonic Wall over Porn,” Christian Science Monitor, 

Schulte, Stephanie R

2009-01-01T23:59:59.000Z

242

One patient's artificial retina story  

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

Eyeing the Future, A New Kind of Vision One Patient's Story Linda M meets Mickey Mouse Linda M., a petite brunette in her early 60s (pictured at right), first realized that...

243

Argonne Chemical Sciences & Engineering - People - Fundamental Interactions  

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

Fundamental Interactions Fundamental Interactions Atomic, Molecular, and Optical Physics Linda Young, Argonne Distinguished Fellow and Group Leader phone: 630/252-8878, fax: 630/252-6210, e-mail: young@anl.gov Ph.D., Chemical Physics, University of California, Berkeley Ultrafast x-ray and laser science Strong-field control of x-ray processes Atomic and molecular behavior in strong-electromagnetic fields Precision measurements in atom traps Robert W. Dunford, Physicist phone: 630/252-4052, fax: 630/252-2864, email: dunford@anl.gov Ph.D., Physics, University of Michigan Experimental atomic physics Elliot Kanter, Physicist phone: 630/252-4050, fax: 630/252-2864, e-mail: kanter@anl.gov Bertold Krässig, Physicist phone 630/252-9230, fax 630/252-6210, e-mail kraessig@anl.gov Ph.D. / Dr. Rer. Nat., Physics, University of Freiburg, Germany

244

Universit de Caen BasseNormandie Ecole doctorale SIMEM  

E-Print Network (OSTI)

ce manuscrit), nos discussions concernant le DIY et son utilisation au sein de la recherche. ­ Linda

245

PowerPoint Presentation  

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

* Linda Cady-Hoffman - Rates Manager * Steve Sanders - Operations and Transmission Advisor * Sara Baker - Public Utilities Specialist Agenda * Meeting Purpose *...

246

Replacement solvents for use in chemical synthesis - Energy ...  

The replacement solvents may be readily recovered from the reaction train using conventional methods. Inventors: Molnar; Linda K. (Philadelphia, PA), ...

247

Performance Assessment Scoping - Hanford Example  

Performance Assessment Scoping - Hanford Example Linda Suttora Office of Environmental Compliance DOE-HQ Waste Processing Technical Exchange 2010

248

THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A CLOSE SUBSTELLAR COMPANION TO THE YOUNG DEBRIS DISK STAR PZ Tel  

SciTech Connect

We report the discovery of a tight substellar companion to the young solar analog PZ Tel, a member of the {beta} Pic moving group observed with high-contrast adaptive optics imaging as part of the Gemini Near-Infrared Coronagraphic Imager Planet-Finding Campaign. The companion was detected at a projected separation of 16.4 {+-} 1.0 AU (0.''33 {+-} 0.''01) in 2009 April. Second-epoch observations in 2010 May demonstrate that the companion is physically associated and shows significant orbital motion. Monte Carlo modeling constrains the orbit of PZ Tel B to eccentricities >0.6. The near-IR colors of PZ Tel B indicate a spectral type of M7 {+-} 2 and thus this object will be a new benchmark companion for studies of ultracool, low-gravity photospheres. Adopting an age of 12{sup +8} {sub -4} Myr for the system, we estimate a mass of 36 {+-} 6 M {sub Jup} based on the Lyon/DUSTY evolutionary models. PZ Tel B is one of the few young substellar companions directly imaged at orbital separations similar to those of giant planets in our own solar system. Additionally, the primary star PZ Tel A shows a 70 {mu}m emission excess, evidence for a significant quantity of circumstellar dust that has not been disrupted by the orbital motion of the companion.

Biller, Beth A.; Liu, Michael C.; Wahhaj, Zahed; Dupuy, Trent J.; Ftaclas, Christ [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Nielsen, Eric L.; Close, Laird M.; Males, Jared; Skemer, Andrew [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Hayward, Thomas L.; Hartung, Markus [Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena (Chile); Burrows, Adam [Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States); Chun, Mark [Institute for Astronomy, 640 North Aohoku Place, 209, Hilo, HI 96720-2700 (United States); Clarke, Fraser; Tecza, Matthias; Thatte, Niranjan [Department of Astronomy, University of Oxford, DWB, Keble Road, Oxford OX1 3RH (United Kingdom); Reid, I. Neill [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Shkolnik, Evgenya L. [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015 (United States); Alencar, Silvia H. P. [Departamento de Fisica-ICEx-Universidade Federal de Minas Gerais, Av. Antonio Carlos, 6627, 30270-901, Belo Horizonte, MG (Brazil); Artymowicz, Pawel [University of Toronto at Scarborough, 1265 Military Trail, Toronto, Ontario M1C 1A4 (Canada)

2010-09-01T23:59:59.000Z

249

INDEPENDENT TECHNICAL REVIEW OF THE BUILDING 100 PLUME, FORMER DOE PINELLAS SITE (YOUNG - RAINEY STAR CENTER), LARGO, FLORIDA  

SciTech Connect

Contaminated groundwater associated with Building 100 at the Young-Rainey Science, Technology, and Research Center, formerly the DOE Pinellas plant, is the primary remedial challenge that remains to be addressed at the site. Currently, Building 100 is an active industrial facility that is now owned and operated by the Pinellas county government. Groundwater samples collected from monitoring wells recently installed near the southern boundary of the site suggest that contaminated groundwater has migrated off the plant site. In response to the challenges presented by the Building 100 plume, the Office of Legacy Management (LM) requested assistance from the DOE Office of Groundwater and Soil Remediation (EM-32) to provide a review team to make technical recommendations so that they can efficiently and effectively address characterization and remediation of the plume. The review team was unanimous in the conclusion that a dynamic strategy that combines a phased implementation of direct push samplers, sensors, and tools can be used to better delineate the extent of contamination, control plume migration, and rapidly remediate the contaminated groundwater at the site. The initial efforts of the team focused on reviewing the site history and data, organizing the information into a conceptual model, identifying appropriate technologies, and recommending an integrated strategy. The current groundwater data from the site indicate a two-lobed plume extending to the east and south. To the east vinyl chloride is the primary contaminant of concern, to the south, vinyl chloride and cis1, 2-DCE are the primary contaminants. The limited data that are available suggest that reductive dechlorination of the TCE is already occurring but is not sufficient to prevent offsite migration of low concentrations of TCE daughter products. The team recommends that DOE pursue a strategy that builds on the natural cleansing capacity of the subsurface with reductive methods including biostimulation and/or bioaugmentation to provide a sustainable remediation system within the flow path of the plume. Additional data will be required to implement this approach and will include: (1) Better delineation of the nature and extent of contamination; (2) Demonstration the plume is currently stable or shrinking; and (3) Demonstration the full reductive dechlorination is occurring. The technical team recommends that DOE use a phased approach to identify residual contamination and to provide rapid installation of remedies. Matrices of characterization and remediation sensors, technologies, and tools were developed by the team in order to match the specific conditions and requirements of the site. The team provides a specific example of remedy that includes the incorporation of a dynamic characterization strategy moving from minimally invasive to more aggressive field techniques, the consideration of multiple complementary remediation approaches based on a spatiotemporally phased approach keyed to the different demands of different parts of the plume, and the integration and sequencing of the characterization and remediation activities.

Eddy-Dilek, C.; Rossabi, J.; Amidon, M.; Riha, B.; Kaback, D.

2010-07-30T23:59:59.000Z

250

Influence of an Intra-articular Lipopolysaccharide Challenge on Markers of Inflammation and Cartilage Metabolism and the Ability of Oral Glucosamine to Mitigate these Alterations in Young Horses  

E-Print Network (OSTI)

This project established an in vivo method to identify and manipulate expression of markers of osteoarthritis (OA). Specifically, strategies that predictably induce joint inflammation to evaluate dietary methods of OA prevention in young horses have yet to be accomplished. Therefore, the 3 studies described herein were conducted to determine effectiveness of an intra-articular lipopolysaccharide (LPS) challenge on markers of inflammation and cartilage metabolism in young horses and potential of dietary glucosamine hydrochloride (HCl) to mitigate these alterations. In the first study, horses were challenged with 0.25 ng or 0.50 ng of intra-articular LPS solution or lactated ringer’s solution (control). Injection of LPS increased inflammation based on synovial prostaglandin E2 (PGE2) concentrations. Carboxypeptide of type II collagen (CPII), a maker of type II collagen synthesis, also increased in a dose-dependent manner. However, clinical parameters of health were not influenced and remained within normal ranges. Carpal circumference increased in response to repeated arthrocentesis. Lameness scores increased with LPS injection when compared to controls. This model of joint inflammation (0.5 ng LPS) was used in the second study to evaluate potential chondroprotective effects of oral glucosamine HCl supplementation in yearling horses. Specifically, the oral absorption of glucosamine HCl versus saline was determined by nasogastric dosing and incorporation of dietary glucosamine HCl into plasma and synovial fluid over time. Plasma and synovial fluid concentrations of glucosamine tended to increase over the 98-d period. In the third study, yearlings were challenged with intra-articular LPS to determine the potential of glucosamine HCl to mitigate inflammation when compared to contralateral joints. Injection of LPS increased synovial PGE2 and cartilage biomarkers CPII and collagenase cleavage neopeptide (C2C), a marker of type II collagen degradation. Oral glucosamine HCl decreased PGE2 and C2C concentrations, but increased levels of CPII. Results of these 3 studies provide a clearer understanding of joint inflammation and cartilage turnover in young horses and demonstrated a potential role of oral glucosamine to mitigate these effects and possibly prevent OA in horses.

Lucia, Jessica Lauren

2013-05-01T23:59:59.000Z

251

Rsdometty C.M.R. Platt, J. W. Bennett, S. A. Young, M. D. Fenwick, P. J. Manson, G. R. Patterson, and B. Petraitis  

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

Rsdometty Rsdometty C.M.R. Platt, J. W. Bennett, S. A. Young, M. D. Fenwick, P. J. Manson, G. R. Patterson, and B. Petraitis CSIRO Division of Atmospheric Research Station Street Aspendale, Victoria, Australia Introduction a suitable detector, such a radiometer can yield a response time of about one second, which will follow most cl6ud fluctuations with minimum lag. The LIRAD Method The use of narrow beam filter radiometers with lidars goes back some considerable time. The CSIRO Marl< I radiometer was designed and constructed in 1970 (Platt 1971). Since then, improved versions (Marl< II and Marl< 111) have been constructed (Platt et al. 1987). Using the URAD method, much information has been obtained on the optical properties of cirrus (e.g., Platt et al. 1987, Platt and

252

GAS SURFACE DENSITY, STAR FORMATION RATE SURFACE DENSITY, AND THE MAXIMUM MASS OF YOUNG STAR CLUSTERS IN A DISK GALAXY. I. THE FLOCCULENT GALAXY M 33  

Science Conference Proceedings (OSTI)

We analyze the relationship between maximum cluster mass M{sub max} and surface densities of total gas ({Sigma}{sub gas}), molecular gas ({Sigma}{sub H{sub 2}}), and star formation rate ({Sigma}{sub SFR}) in the flocculent galaxy M 33, using published gas data and a catalog of more than 600 young star clusters in its disk. By comparing the radial distributions of gas and most massive cluster masses, we find that M{sub max}{proportional_to}{Sigma}{sup 4.7{+-}0.4}{sub gas}, M{sub max}{proportional_to}{Sigma}{sup 1.3{+-}0.1}{sub H{sub 2}}, and M{sub max}{proportional_to}{Sigma}{sup 1.0{+-}0.1}{sub SFR}. We rule out that these correlations result from the size of the sample; hence, the change of the maximum cluster mass must be due to physical causes.

Gonzalez-Lopezlira, Rosa A.; Pflamm-Altenburg, Jan; Kroupa, Pavel, E-mail: r.gonzalez@crya.unam.mx [Argelander Institut fuer Astronomie, Universitaet Bonn, Auf dem Huegel 71, D-53121 Bonn (Germany)

2012-12-20T23:59:59.000Z

253

Louisville, KY Led by Debbie Grusenmeyer (Extension Associate/ PRO-DAIRY Youth Specialist) and Matt Young (Cornell Animal Science '02) a team of New York 4-H youth recently won the National 4-H  

E-Print Network (OSTI)

) and Matt Young (Cornell Animal Science '02) a team of New York 4-H youth recently won the National 4-H Dairy Quiz Bowl Championship title for the 10th time. The 33rd annual North American Invitational 4-H Dairy Quiz Bowl Contest was held at the North American International Livestock Exposition in Louisville

Keinan, Alon

254

Microsoft PowerPoint - 2008-07-08-ArgonneKulinowski.ppt  

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

Planning Team Crowell & Moring, LLP NIOSH U Wisc NSEC U Mass Amherst NSEC ILO IOM (UK) RTI Evonik DeGussa Nanotech Industries Assoc (UK) Boeing ... http:icon.rice.edu...

255

SunShot Initiative: SunShot Prize Resources  

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

hosted the event on April 10, 2013. It was held at CNSE's Albany Nanotech Complex in Albany, New York. Learn more about the speakers and presentations. July 2013 SunShot Prize...

256

Engineering Emergence  

Science Conference Proceedings (OSTI)

We explore various definitions and characteristics of emergence, how we might recognise and measure emergence, and how we might engineer emergent systems. We discuss the TUNA ("Theory Underpinning Nanotech Assemblers") project, which is investigating ...

Susan Stepney; Fiona A. C. Polack; Heather R. Turner

2006-08-01T23:59:59.000Z

257

final program ( 4.4 mb pdf download) - TMS  

Science Conference Proceedings (OSTI)

Nov 11, 2007 ... Scott Livingston, Managing Director, Axiom Capital Management Inc. ... Environmental, Health and Safety Panel Discussion ... Thomas Armstrong, Nanotech Program Manager, Pennsylvania Department of Community & ..... si of more than an order magnitude in nanoscale specimens by restructuring.

258

News Item  

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

Seeing in Color at the Nanoscale: Foundry Scientists Develop a New Nanotech Tool to Probe Solar Energy Conversion If nanoscience were television, we'd be in the 1950s. Although...

259

Radiation for Hodgkin's Lymphoma in Young Female Patients: A New Technique to Avoid the Breasts and Decrease the Dose to the Heart  

SciTech Connect

Purpose: To demonstrate how, in young female patients with Hodgkin's lymphoma, using an inclined board technique can further decrease the volume of breasts and heart in the treatment field. Methods and Materials: An inclined board was constructed with the ability to mount an Aquaplast face mask, a Vacu-Lock, and a hip stopper. Eight female patients with early-stage Hodgkin's lymphoma were planned and compared using the conventional flat position and the inclined board position. All patients on the inclined board were planned with 90{sup o} degree table position and 15{sup o} gantry angle rotation to compensate for the beam divergence resulting from the patient's position on the inclined board. Dose-volume histograms were generated, as well as the mean V30 and V5 of both breasts and heart using both treatment positions. Results: The mean value of V30 of the right breast, left breast, and heart decreased from 3%, 3%, and 13%, respectively, using the flat position to 0, 0.4%, and 5%, respectively, using the inclined board. The mean value of V5 of the right breast, left breast, and heart decreased from 6%, 13%, and 36%, respectively, using the flat position to 2%, 8%, and 29%, respectively, using the inclined board. Conclusions: Compared with conventional flat positioning, this simple device and technique allows better sparing of the breasts and the heart while maintaining comparable target coverage and total lung dose.

Dabaja, Bouthaina S., E-mail: bdabaja@mdanderson.or [Department of Radiation Oncology, University of Texas M. D. Anderson Cancer Center, Houston, TX (United States); Rebueno, Neal C.S.; Mazloom, Ali; Thorne, Scott; Perrin, Kelly J.; Tolani, Naresh; Das, Pragnan; Delclos, Marc E.; Iyengar, Puneeth; Reed, Valerie K.; Horace, Patrecia; Salehpour, Mohammad R. [Department of Radiation Oncology, University of Texas M. D. Anderson Cancer Center, Houston, TX (United States)

2011-02-01T23:59:59.000Z

260

Sowing the seeds of massive black holes in small galaxies: Young clusters as the building blocks of Ultra-Compact-Dwarf Galaxies  

E-Print Network (OSTI)

Interacting galaxies often have complexes of hundreds of young stellar clusters of individual masses ~ 10^{4-6} Msun in regions that are a few hundred parsecs across. These cluster complexes interact dynamically, and their coalescence is a candidate for the origin of some ultracompact dwarf galaxies (UCDs). Individual clusters with short relaxation times are candidates for the production of intermediate-mass black holes of a few hundred solar masses, via runaway stellar collisions prior to the first supernovae in a cluster. It is therefore possible that a cluster complex hosts multiple intermediate-mass black holes that may be ejected from their individual clusters due to mergers or binary processes, but bound to the complex as a whole. Here we explore the dynamical interaction between initially free-flying massive black holes and clusters in an evolving cluster complex. We find that, after hitting some clusters, it is plausible that the massive black hole will be captured in an ultracompact dwarf forming near the center of the complex. In the process, the hole typically triggers electromagnetic flares via stellar disruptions, and is also likely to be a prominent source of gravitational radiation for the advanced ground-based detectors LIGO and VIRGO. We also discuss other implications of this scenario, notably that the central black hole could be considerably larger than expected in other formation scenarios for ultracompact dwarfs.

Pau Amaro-Seoane; Symeon Konstantinidis; Marc Dewi Freitag; M. Coleman Miller; Frederic A. Rasio

2012-11-28T23:59:59.000Z

Note: This page contains sample records for the topic "nanotech linda young" 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

SPECTRAL TYPING OF LATE-TYPE STELLAR COMPANIONS TO YOUNG STARS FROM LOW-DISPERSION NEAR-INFRARED INTEGRAL FIELD UNIT DATA  

Science Conference Proceedings (OSTI)

We used the Project 1640 near-infrared coronagraph and integral field spectrograph to observe 19 young solar-type stars. Five of these stars are known binary stars and we detected the late-type secondaries and were able to measure their JH spectra with a resolution of R {approx} 30. The reduced, extracted, and calibrated spectra were compared to template spectra from the IRTF spectral library. With this comparison, we test the accuracy and consistency of spectral-type determination with the low-resolution near-infrared spectra from P1640. Additionally, we determine effective temperature and surface gravity of the companions by fitting synthetic spectra calculated with the PHOENIX model atmosphere code. We also present several new epochs of astrometry of each of the systems. Together, these data increase our knowledge and understanding of the stellar make up of these systems. In addition to the astronomical results, the analysis presented helps validate the Project 1640 data reduction and spectral extraction processes and the utility of low-resolution, near-infrared spectra for characterizing late-type companions in multiple systems.

Roberts, Lewis C.; Beichman, Charles A.; Burruss, Rick; Ligon, E. Robert; Lockhart, Thomas G.; Roberts, Jennifer E.; Shao, Michael [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Rice, Emily L.; Brenner, Douglas; Oppenheimer, Ben R. [American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); Crepp, Justin R.; Dekany, Richard G.; Hillenbrand, Lynne A.; Hinkley, Sasha [California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); King, David; Parry, Ian R. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA (United Kingdom); Metchev, Stanimir [Department of Physics and Astronomy, State University of New York, Stony Brook, NY 11794-3800 (United States); Pueyo, Laurent; Sivaramakrishnan, Anand; Soummer, Remi, E-mail: lewis.c.roberts@jpl.nasa.gov [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); and others

2012-07-15T23:59:59.000Z

262

A Catalog of Extended Green Objects (EGOs) in the GLIMPSE Survey: A new sample of massive young stellar object outflow candidates  

E-Print Network (OSTI)

Using images from the Spitzer GLIMPSE Legacy survey, we have identified more than 300 extended 4.5 micron sources (abbreviated EGO, Extended Green Object, for the common coding of the [4.5] band as green in 3-color composite IRAC images). We present a catalog of these EGOs, including integrated flux density measurements at 3.6, 4.5, 5.8, 8.0, and 24 microns from the GLIMPSE and MIPSGAL surveys. The average angular separation between a source in our sample and the nearest IRAS point source is >1 arcminute. The majority of EGOs are associated with infrared dark clouds (IRDCs), and where high-resolution 6.7 GHz methanol maser surveys overlap the GLIMPSE coverage, EGOs and 6.7 GHz methanol masers are strongly correlated. Extended 4.5 micron emission is thought to trace shocked molecular gas in protostellar outflows; the association of EGOs with IRDCs and 6.7 GHz methanol masers suggests that extended 4.5 micron emission may pinpoint outflows specifically from massive protostars. The mid-infrared colors of EGOs lie in regions of color-color space occupied by young protostars still embedded in infalling envelopes.

C. J. Cyganowski; B. A. Whitney; E. Holden; E. Braden; C. L. Brogan; E. Churchwell; R. Indebetouw; D. F. Watson; B. L. Babler; R. Benjamin; M. Gomez; M. R. Meade; M. S. Povich; T. P. Robitaille; C. Watson

2008-10-02T23:59:59.000Z

263

X-ray flares observed from six young stars located in the region of star clusters NGC 869 and IC 2602  

E-Print Network (OSTI)

We present an analysis of seven intense X-ray flares observed from six stars (LAV 796, LAV 1174, SHM2002 3734, 2MASS 02191082+5707324, V553 Car, V557 Car) for the first time. These stars are located in the region of young open star clusters NGC 869 and IC 2602. These flares detected in the XMM-Newton data show a rapid rise (10-40 minutes) and a slow decay (20-90 minutes). The X-ray luminosities during the flares in the energy band 0.3-7.5 keV are in the range of $10^{29.9}$ to $10^{31.7}$ erg s$^{-1}$. The strongest flare was observed with the ratio $\\sim 13$ for count rates at peak of the flare to the quiescent intensity. The maximum temperature during the flares has been found to be $\\sim$100 MK. The semi loop lengths for the flaring loops are estimated to be of the order of $\\rm{10^{10}}$ cm. The physical parameters of the flaring structure, the peak density, pressure, and minimum magnetic field required to confine the plasma have been derived and found to be consistent with flares from pre-main sequence s...

Bhatt, Himali; Singh, K P; Sagar, Ram; Kumar, Brijesh

2013-01-01T23:59:59.000Z

264

PLANETS AROUND LOW-MASS STARS (PALMS). II. A LOW-MASS COMPANION TO THE YOUNG M DWARF GJ 3629 SEPARATED BY 0.''2  

SciTech Connect

We present the discovery of a 0.''2 companion to the young M dwarf GJ 3629 as part of our high-contrast adaptive optics imaging search for giant planets around low-mass stars with the Keck-II and Subaru telescopes. Two epochs of imaging confirm that the pair is comoving and reveal signs of orbital motion. The primary exhibits saturated X-ray emission which, together with its UV photometry from GALEX, points to an age younger than {approx}300 Myr. At these ages the companion lies below the hydrogen burning limit with a model-dependent mass of 46 {+-} 16 M{sub Jup} based on the system's photometric distance of 22 {+-} 3 pc. Resolved YJHK photometry of the pair indicates a spectral type of M7 {+-} 2 for GJ 3629 B. With a projected separation of 4.4 {+-} 0.6 AU and an estimated orbital period of 21 {+-} 5 yr, GJ 3629 AB is likely to yield a dynamical mass in the next several years, making it one of only a handful of brown dwarfs to have a measured mass and an age constrained from the stellar primary.

Bowler, Brendan P.; Liu, Michael C. [Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Shkolnik, Evgenya L. [Lowell Observatory, 1400 W. Mars Hill Road, Flagstaff, AZ 86001 (United States); Tamura, Motohide, E-mail: bpbowler@ifa.hawaii.edu [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

2012-09-01T23:59:59.000Z

265

Bringing Fruit Flies in from the Cold  

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

DOE Environmental Sustainability Award to Three from APS DOE Environmental Sustainability Award to Three from APS 2009 Chemistry Nobel to APS Users The First Experiment at the LCLS Linda Young Named to Head X-ray Science Division $7.9 M in ARRA Funding Brings New Instrumentation to the APS APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Bringing Fruit Flies in from the Cold DECEMBER 21, 2009 Bookmark and Share See the video of synchrotron x-ray visualization of ice formation in insects during lethal and non-lethal freezing at http://www.youtube.com/watch?v=m07CKU1XGdk Based on the University of Western Ontario press release Using a microscope the size of a football field, researchers from The University of Western Ontario, the University of Nevada-Las Vegas, Argonne

266

2011 Arthur H. Compton Award Announced by APSUO  

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X-Ray Focusing: Techniques and Applications X-Ray Focusing: Techniques and Applications Linda Young of the APS "On the Record at the APS March Meeting" John "Jack" Carpenter of AES Named a Fellow of AAAS APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed 2011 Arthur H. Compton Award Announced by APSUO APRIL 21, 2011 Bookmark and Share The 2011 Compton Award winners. Clockwise from top left: Farrel Lytle, John Rehr, Edward Stern, and Dale Sayers. The U.S. Department of Energy's Advanced Photon Source (APS) and the APS Users Organization (APSUO) announce that the 2011 Arthur H. Compton Award will be presented jointly to Edward Stern, Farrel Lytle, Dale Sayers (posthumously), and John Rehr for their development of the technique of

267

2009 Chemistry Nobel to APS Users  

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The First Experiment at the LCLS The First Experiment at the LCLS Linda Young Named to Head X-ray Science Division $7.9 M in ARRA Funding Brings New Instrumentation to the APS Hard X-ray Nanoprobe Earns an R&D 100 Award Winans of XSD Elected to ACS Fellowship APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed 2009 Chemistry Nobel to APS Users OCTOBER 7, 2009 Bookmark and Share Clockwise from top left: Ada Yonath, Venkatraman Ramakrishnan, and Thomas Steitz. All three recipients of the 2009 Nobel Prize in Chemistry published papers on their award-winning work based on data collected at the U.S. Department of Energy's (DOE) Advanced Photon Source (APS) at Argonne National Laboratory. Between them, biochemists Thomas Steitz of Yale University, Ada Yonath of

268

In Other News  

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In Other News In Other News Community Connections: Our link to Northern New Mexico Communities Latest Issue:Dec. 2013 - Jan. 2014 All Issues » submit In Other News LANL employee chosen for "Frontiers of Engineering" Symposium; 16th Annual Hazmat Challenge strengthens response skills. September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email LANL Employee Chosen for "Frontiers of Engineering" Symposium Only 78 of the nation's brightest young engineers were selected to participate in the 18th Annual U.S. Frontiers in Engineering symposium, and Nathan Moody, who works for the Lab's High Power Electrodynamics group in the Accelerator Operations and Technology Division, will be one of them.

269

Short Pulse X-rays at the APS  

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Short Pulse X-rays at the APS Workshop Summary Friday, May 9, 2008 Building 401, Room A5000 Organizers: Jin Wang (Argonne National Laboratory), Lin Chen (Argonne National Laboratory), David Reis ( University of Michigan ), Paul Evans ( University of Wisconsin ), Ali Nassiri (Argonne National Laboratory), and Linda Young ( Argonne National Laboratory) Agenda Registration - complete the visitor registration form. For "purpose of visit," please enter "APS SPX Workshop" https://www.aps.anl.gov/About/Visiting/visitor_registration.php On-site lodging is at the Argonne Guest House http://www.anlgh.org/ Travel to Argonne National Laboratory http://www.aps.anl.gov/About/Visiting/Directions/ Fees There is no charge for this workshop. Since the 2004 Lake Geneva Workshop, the APS has performed three years of

270

APS User News, Issue 71  

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1, August 18, 2011 1, August 18, 2011 CONTENTS 1. DIRECTOR'S CORNER USER MATTERS 2. How to Wow! "Secrets" for a Successful Proposal 3. Sweet Dreams Mean Safer Work 4. XSD's Linda Young Elected DAMOP Vice Chair 5. Successful 2011 APS/IIT Summer XAFS School BRIEFLY NOTED -- John Quintana Appointed Argonne's Deputy COO -- 2011 X-Ray Spectroscopy of Magnetic Solids Workshop Set for October 22-23 -- Workshops on Hard X-ray Instrumentation at the SwissFEL -- Next GUP Deadline is October 28, 2011 ===================================================== Instructions for subscribing, unsubscribing, and submitting info http://www.aps.anl.gov/Users/Communications/User_News/ ===================================================== DIRECTOR'S CORNER During the last week of July, we had the annual review of APS organized by

271

Workshop on Time Domain Science Using X-ray Techniques  

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Time-Resolved Beamlines Time-Resolved Beamlines Advisory Committee Workshop Home Workshop Chairs: Lin Chen (Argonne National Laboratory) Steve Milton (Advanced Photon Source) David Reis (University of Michigan) Linda Young (Argonne National Laboratory) Workshop on Time Domain Science Using X-ray Techniques August 29 September 1, 2004, The Abbey, Fontana, Lake Geneva Area, Wisconsin A workshop on "Time Domain Science Using X-ray Techniques" was held from August 29 September 1, 2004 , welcoming both experts and beginners in the field. This is one of the concurrently held workshops in the series on "Future Scientific Directions for the Advanced Photon Source." The goal of the workshop was to identify future directions in scientific research using time resolved x-ray techniques and to address possiblities to produce ps

272

Expanding Your Horizons scheduled for March 2  

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Expanding Your Horizons Expanding Your Horizons Community Connections: Our link to Northern New Mexico Communities Latest Issue:Dec. 2013 - Jan. 2014 All Issues » submit Expanding Your Horizons scheduled for March 2 The conference offers fifth- to 12th-grade girls opportunities to participate in hands-on workshops about science, technology, engineering, math and related fields. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Up to 250 young women are expected to participate in the workshops that will include subjects such as computers and robots, veterinary medicine, cryptography and ocean science. This year the Santa Fe and Los Alamos Expanding Your Horizons (EYH) conferences are combined into one, all-day session to be held on March 2 at

273

Lahsen Assoufid Elected a Fellow of SPIE  

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

2011 Arthur H. Compton Award Announced by APSUO 2011 Arthur H. Compton Award Announced by APSUO X-Ray Focusing: Techniques and Applications Linda Young of the APS "On the Record at the APS March Meeting" John "Jack" Carpenter of AES Named a Fellow of AAAS APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Lahsen Assoufid Elected a Fellow of SPIE APRIL 21, 2011 Bookmark and Share Lahsen Assoufid Lahsen Assoufid has been elected a Fellow of SPIE, the international society for optics and photonics. He is Section Leader for Mirror Multilayer and Metrology in the X-ray Science Division (XSD) Optics and Detectors Group of the Advanced Photon Source at Argonne National Laboratory. Assoufid is acknowledged for his "achievements in metrology and x-ray

274

High-Energy Processes in Young Stars: Chandra X-ray Spectroscopy of HDE 283572, RY Tau, and LkCa 21  

E-Print Network (OSTI)

Weak-lined T Tauri stars (WTTS) represent the important stage of stellar evolution between the accretion phase and the zero-age main sequence. At this stage, the star decouples from its accretion disk, and spins up to a higher rotation rate than in the preceding classical T Tauri phase. Consequently, dynamo processes can be expected to become even stronger at this stage. High energy processes can have effects on the remaining circumstellar material, possibly including protoplanets and planetesimals, and these effects may account for certain observable properties of asteroids in the current solar system. Chandra observed for 100 ks the WTTS HDE 283572 which probes the PMS stage of massive A-type stars. We present first results of the analysis of its high-resolution X-ray spectrum obtained with the High-Energy Transmission Grating Spectrometer. A wide range of Fe lines of high ionization states are observed, indicating a continuous emission measure distribution. No significant signal is detected longward of the O \\textsc{viii} Ly$\\alpha$ line because of the high photoelectric absorption. We also report on the preliminary analysis of the zeroth order spectra of RY Tau and LkCa21. In particular, we show evidence of an emission line in RY Tau at 6.4 keV that we identify as fluorescent emission by neutral Fe caused by a strong X-ray flare which illuminated some structure in (or surrounding) the CTTS. A comparison of X-ray spectra of classical T Tau stars, other WTTS, and young main-sequence stars is made.

Marc Audard; Stephen L. Skinner; Kester W. Smith; Manuel Guedel; Roberto Pallavicini

2004-09-13T23:59:59.000Z

275

DEEP X-RAY OBSERVATIONS OF THE YOUNG HIGH-MAGNETIC-FIELD RADIO PULSAR J1119-6127 AND SUPERNOVA REMNANT G292.2-0.5  

SciTech Connect

High-magnetic-field radio pulsars are important transition objects for understanding the connection between magnetars and conventional radio pulsars. We present a detailed study of the young radio pulsar J1119-6127, which has a characteristic age of 1900 yr and a spin-down-inferred magnetic field of 4.1 Multiplication-Sign 10{sup 13} G, and its associated supernova remnant G292.2-0.5, using deep XMM-Newton and Chandra X-ray Observatory exposures of over 120 ks from each telescope. The pulsar emission shows strong modulation below 2.5 keV with a single-peaked profile and a large pulsed fraction of 0.48 {+-} 0.12. Employing a magnetic, partially ionized hydrogen atmosphere model, we find that the observed pulse profile can be produced by a single hot spot of temperature 0.13 keV covering about one-third of the stellar surface, and we place an upper limit of 0.08 keV for an antipodal hot spot with the same area. The non-uniform surface temperature distribution could be the result of anisotropic heat conduction under a strong magnetic field, and a single-peaked profile seems common among high-B radio pulsars. For the associated remnant G292.2-0.5, its large diameter could be attributed to fast expansion in a low-density wind cavity, likely formed by a Wolf-Rayet progenitor, similar to two other high-B radio pulsars.

Ng, C.-Y.; Kaspi, V. M. [Department of Physics, McGill University, Montreal, QC H3A 2T8 (Canada); Ho, W. C. G. [School of Mathematics, University of Southampton, Southampton SO17 1BJ (United Kingdom); Weltevrede, P. [Jodrell Bank Centre for Astrophysics, University of Manchester, Alan Turing Building, Manchester M13 9PL (United Kingdom); Bogdanov, S. [Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027 (United States); Shannon, R. [CSIRO Astronomy and Space Sciences, Australia Telescope National Facility, Marsfield, NSW 2210 (Australia); Gonzalez, M. E., E-mail: ncy@physics.mcgill.ca [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1 (Canada)

2012-12-10T23:59:59.000Z

276

2012 Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM  

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

of Cost-Effective and Environmentally-Benign Biogas Purification Technology Using Biochar Saurabh Patel, D. Mahajan YRS POSTERS 2012 10 36. Synthesis and...

277

Young Leaders Award Winner Summaries  

Science Conference Proceedings (OSTI)

... to participate in a wide variety of social function events, including Yong Leaders Tutorial Luncheon, EMPMD council meeting, and TMS-AIME Awards Banquet.

278

SSA Young Jack Pine Site  

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

View an aerial photo-map of the SSA-YJP site. Beginning of the "flagged path" to the tower, from the road The "new trail" to the YJP site, looking towards the site The hut and...

279

Young Leader International Scholar Program  

Science Conference Proceedings (OSTI)

TMS ESSENTIALS. MEMBERS ... The chosen International Scholars also spend a few days visiting select industrial facilities, research labs, or universities.

280

Diagnostics for Kenneth M. Young  

E-Print Network (OSTI)

remote handled waste activities and $23 million for the central characterization project. The bill million for the LANL CMR Wing 9 hot cells, and $5 million for LANSCE materials test station at LANL

Note: This page contains sample records for the topic "nanotech linda young" 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

FIRE Diagnostics Kenneth M. Young  

E-Print Network (OSTI)

Facility h ardware integration, mock-ups & in stallation Shielding/Remote Handling Integration Physics, ­ Effective change in numerical aperture. · Running fibers hot only affects the long-term absorption. · Great° Vacuum Vessel Test Cell Floor Quartz coherent fiber optic bundles Radiation Shielding Enclosure Detector

282

LS-65  

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

5 5 July 17, 1986 Comparison of LINDA and POISSON of a Dipole Field Calculation S. H. Kim 7/17/86 LS-65 Comparison of LINDA and POISSON of a Dipole Field Calculation S. H. Kim Two-dimensional magnetic field computations of a dipole magnet using LINDA and POISSON are compared. The purpose is not to distinguish the basic differences between the two codes, but to compare the results for different mesh sizes in a given problem region. The magnet geometry chosen for the calculation is the 6-GeV injector synchrotron H-type dipole magnet. Figure 1 is the geometry used for LINDA runs. The outside air region is required to satisfy the geometrical constraints of the input parameters in LINDA. LINDA divides the problem space into uniform rectangular meshes. The

283

Final Credentialing Standards for Issuing Personal Identity Verificati...  

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

AND AGENCIES FROM: LINDA M. SPRINGER DIRECTOR SUBJECT: Final Credentialing Standards for Issuing Personal Identity Verification Cards under HSPD-12 This memorandum...

284

Fermilab Today  

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Jack Anderson, Karen Seifrid, Kappy Sherman, Linda Diepholz, Jamie Grado, Karen Karlix-Smith, Gayle Millman, Rosa Foote, Anita Menz-Cwilik, Marie Herman. Photo: Reidar Hahn...

285

Energy Education and Workforce Development: Text-Alternative...  

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

their hand raised. Oh wait. Linda Silverman: Are there opportunities for compressed biogas for federal fleet use? Pam Frugoli: We did not cover any transportation in this model,...

286

07 AnRepcvr fnl.indd  

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

Sloan James and Linda Smedinghoff Ken and Paula Spengler Marion and Mollie Stoerker Dennis and Lee Theriot Michael Turner and Barbara Ahlberg Kay Van Vreede William and...

287

Welcome to the Cultural Resources Newsletter  

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

Officer: Terrence R. Fehner, Ph.D. Environment, Safety and Health Coordinator: Lois Thompson Executive Committee: Linda Cohn, DOE, NNSA, Nevada Site Office Gary Hartman, DOE,...

288

Scientists Studying Photosynthesis to Generate Electricity  

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

supercomputers to investigate photosynthetic materials May 15, 2012 | Tags: Carver, Energy Technologies, HPSS, Magellan NERSC Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402...

289

Electricity Advisory Committee  

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

3:30 - 3:40 pm Welcome and Opening Comments Kevin Kolevar, Assistant Secretary for Electricity Delivery and Energy Reliability Linda Stuntz, Chair, Electricity Advisory Committee...

290

Powerchoice Residential Customer Response to TOU Rates  

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

Woods, Linda Dethman, and Rick Kunkle Institution Research Into Action Keywords behavior, demand response and distributed energy resources center, demand response research center...

291

Atlanta TEC Meeting -- Tribal Group Summary 3-6-07  

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

of Acoma), Bob Lupton (DOE Yucca Mountain Project), Corinne Macaluso (OCRWM), Kevin Mariano (Pueblo of Acoma), Linda Minton (Emergency Nurses Association), James Montague...

292

Asian/American Bodies in Extremis: Gendering Power, Pleasure, and Nation through "Spectacular" Excess  

E-Print Network (OSTI)

Erika Lust is Occupying Feminist Porn. ” Vice http://is-occupying-feminist-porn. (22 July 2012). Stud Hunters.Television. Williams, Linda. Porn Studies. Durham: Duke UP,

Knoll, Melissa Garcia

2012-01-01T23:59:59.000Z

293

PowerPoint Presentation  

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

Linda Holmes, Educational Outreach Katy Waldrop, HR Manager Tim Guilliams, Information Technology Media Relations Ron Walli Employee Communications Bill Cabage ORNL Review Jim...

294

Contribution of Tissue Level Organization to Genomic Stability...  

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

of Tissue Level Organization to Genomic Stability Following Low Dose Gamma Irradiation Cheryl Burrell Loma Linda University Abstract Our study proposes that the level of...

295

Pulsed laser microbeams for cellular manipulation : applications in cell biology and microfluidics  

E-Print Network (OSTI)

Applications in Cell Biology and Microfluidics AMicrobeams in Biology and Biotechnology..3for her expertise in cell biology and biochemistry, Linda Li

Hellman, Amy Noel Stacy

2008-01-01T23:59:59.000Z

296

Effect of Varied Air Flow on Flame Structure of Laminar Inverse Diffusion Flames  

E-Print Network (OSTI)

provided invaluable assistance. Sandia is a multiprogramlaboratory operated by Sandia Corporation, a Lockheed MartinShaddix, and Linda G. Blevins Sandia National Laboratories,

Mikofski, Mark A; Williams, Timothy C; Shaddix, Christopher R; Blevins, Linda G

2004-01-01T23:59:59.000Z

297

A C S  

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

Thomas and Edna Groves Margery Hanson Drasko and Stanka Jovanovic Mike and Linda Knapp Peter Koehler David and Joanna Livengood Gordon and Cynthia Marler Spencer and Eileen...

298

HROM_Org Chart_July2013  

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

& Occupational Medicine Division and Guest, User, Visitor (GUV) Center Approved by Robert Lincoln July 2013 Lizette Domenech Kelly Guiffreda Teri Lazar Erika Reyes Linda Rundlett...

299

Lab sustainability efforts move toward solar energy: DOE issues...  

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110112solar 11012012 Lab sustainability efforts move toward solar energy: DOE issues call for proposals Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov...

300

Bioenergy Technologies Office: Bioenergy Technologies Office...  

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

Goss Eng, Program Operations Supervisor Administrative Linda Malloy Analysis & Sustainability Zia Haq Kristen Johnson Alicia Lindauer Budget Moon Lao Natalie Roberts...

Note: This page contains sample records for the topic "nanotech linda young" 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

Site Map: Artificial Retina Project  

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Site Index Home About the Project Overview How the Artificial Retina Works Implant Patient Stories Terry Byland Linda M. Kathy B. How to Participate Project Collaborators CRADA...

302

Female Gubernatorial Candidates: Strategies for Overcoming Gendered Perceptions of Viability  

E-Print Network (OSTI)

2002. Television Zanobini 67 Fowler, Linda L. , and Jenniferseeking political office (Fowler and Lawless 2009, 521). TheSenate and the White House (Fowler and Lawless 2009, 519).

Zanobini, Annie

2011-01-01T23:59:59.000Z

303

A Comparison of Li-Ion Battery Recycling Options  

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

1 A Comparison of Li-Ion Battery Recycling Options Linda Gaines and Jennifer Dunn Center for Transportation Research Argonne National Laboratory SAE World Congress April 2012 PAPER...

304

Lithium-Ion Batteries: Examining Material Demand and Recycling...  

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

ISSUES Linda Gaines and Paul Nelson Argonne National Laboratory, Argonne, IL Keywords: battery materials, lithium, recycling Abstract Use of vehicles with electric drive, which...

305

Lithium-Ion Battery Issues  

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Lithium-Ion Battery Issues IEA Workshop on Battery Recycling Hoboken, Belgium September 26-27, 2011 Linda Gaines Center for Transportation Research Argonne National Laboratory...

306

Trip to China  

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

to China By row boat or by plane... 16 hours later Linda Field Patent Counsel Department of Energy Destination: Wuhan, China Purpose: Innovation Promotion in CERC - IP Clarity &...

307

Lab suppliers receive Department of Energy awards  

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Department of Energy awards LANL's Small Business Program Office nominated the companies for the awards. August 1, 2012 dummy image Read our archives Contacts Editor Linda...

308

Microsoft PowerPoint - 7-03 Suttora Tech Exchange - Hanford Scoping...  

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

- Hanford Example Linda Suttora Office of Environmental Compliance DOE-HQ Waste Processing Technical Exchange 2010 Print Close Scoping of the Hanford PA * Reason for new Hanford C...

309

Sacramento en El Movimiento : Chicano politics in the civil rights era  

E-Print Network (OSTI)

Avella, Steven M. Sacramento, CA. Charleston, SC: Arcadiafourth from right), Sacramento, CA. (Courtesy of Linda M.Sacramento Region,” Sacramento, CA: Community Service

Márquez, Lorena Valdivia

2010-01-01T23:59:59.000Z

310

BLACK HISTORY @ Your Education Library  

E-Print Network (OSTI)

BLACK HISTORY @ Your Education Library Focus on Canadian Resources: Songs Granfield, Linda. Illus, Rella. Solme Black Women: Profiles of Black Women in Canada. Sister Vision, 1993. FC106.B6B73 1993 Bramble, Linda. Black Fugitive Slaves in Early Canada. Vanwell, 1987. Juv E450.B73 1987 Carter, Velma

Ellis, Randy

311

High-level networking with mobile code and first order AND-continuations  

Science Conference Proceedings (OSTI)

We describe a scheme for moving living code between a set of distributed processes coordinated with unification based Linda operations, and its application to building a comprehensive Logic programming based Internet programming framework. Mobile ... Keywords: Internet programming, Linda coordination, blackboard-based logic programming, code migration, dynamic recompilation, first order continuations, mobile agents, mobile computations, networking, remote execution

Paul Tarau; Veronica Dahl

2001-05-01T23:59:59.000Z

312

A Survey on ATM Security Donglin Liang, dliang@cis.ohio-state.edu  

E-Print Network (OSTI)

and an alternate algorithms are available to select for each security service. Hebda, Shields and Kubic point out, Linda Shields, and Chris Kubic, Selection and Negotiation of Multiple Algorithms to Support Security. [SKH97] Linda Shields, Chris Kubic, and Kim Hebda, Control Panel Authentication, ATM FORUM/97

Jain, Raj

313

Visiting Brookhaven National Laboratory | Young Researcher Symposium...  

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

looks like a giant fish, with a forked tail on the "East End" -- the North Fork is rural, and the South Fork has many famous "Hamptons" resort towns. The Peconic Bay and...

314

General Information, Young Researcher Symposium 2012  

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

looks like a giant fish, with a forked tail on the "East End" -- the North Fork is rural, and the South Fork has many famous "Hamptons" resort towns. The Peconic Bay and...

315

Holmberg Ix: The Nearest Young Galaxy  

E-Print Network (OSTI)

Deep images taken with the Wide Field Channel of the Advanced Camera for Surveys on board the Hubble Space Telescope provide the basis for study the resolved stellar population of the M81 companion dwarf irregular galaxy Holmberg IX. Based on color-magnitude diagrams the stellar population toward Holmberg IX contains numerous stars with ages of <~200 Myr as well as older red giant stars. By charting the spatial distribution of the red giant stars and considering their inferred metallicities, we concluded that most of these older stars are associated with M81 or its tidal debris. At least 20% of the stellar mass in Holmberg IX was produced in the last ~200 Myr, giving it the youngest stellar populations if any nearby galaxy. The location of Holmberg IX, its high gas content, and its youthful stellar population suggests that it is a tidal dwarf galaxy, perhaps formed during the last close passage of M82 around M81.

Sabbi, E; Smith, L J; De Mello, D F; Mountain, M

2008-01-01T23:59:59.000Z

316

Celebrating 20 Years of Outstanding Young Leaders  

E-Print Network (OSTI)

Beesley 2001 Brent Heber Olson 2001 Kara Turner 2000 Richard Gurgel 2000 John Patrick Torgenson 1999 Eryn MaryLou Leyba 1991 Paula Quenemoen Bowman #12;NEENA PACK (2012) is a junior studying political science in 2008. He served as Campaign Finance Counsel for McCain-Palin 2008, Senator John McCain's presidential

Provancher, William

317

TMS Young Leaders Committee Meeting Minutes  

Science Conference Proceedings (OSTI)

Feb 4, 1996... are certain questions and answers that would be sensitive and should not be placed on the general bulletin board; i.e., a salary question.

318

LEARNING FAITH YOUNG CHRISTIANS AND CATECHISM  

E-Print Network (OSTI)

Christians. The catechism handbooks were presented in a dialogue form borrowed from the first catechisms it fundamentally is. In other words, it is a relational involvement between different beings. According to him to the divergent theologies of the Lord's Supper. For the Catholics, the Eucharist holds a central and fundamental

Paris-Sud XI, Université de

319

Lithium Depletion of Nearby Young Stellar Associations  

E-Print Network (OSTI)

We estimate cluster ages from lithium depletion in five pre-main-sequence groups found within 100 pc of the Sun: TW Hydrae Association, Eta Chamaeleontis Cluster, Beta Pictoris Moving Group, Tucanae-Horologium Association and AB Doradus Moving Group. We determine surface gravities, effective temperatures and lithium abundances for over 900 spectra through least squares fitting to model-atmosphere spectra. For each group, we compare the dependence of lithium abundance on temperature with isochrones from pre-main-sequence evolutionary tracks to obtain model dependent ages. We find that the Eta Chamaelontis Cluster and the TW Hydrae Association are the youngest, with ages of 12+/-6 Myr and 12+/-8 Myr, respectively, followed by the Beta Pictoris Moving Group at 21+/-9 Myr, the Tucanae-Horologium Association at 27+/-11 Myr, and the AB Doradus Moving Group at an age of at least 45 Myr (where we can only set a lower limit since the models -- unlike real stars -- do not show much lithium depletion beyond this age). Here, the ordering is robust, but the precise ages depend on our choice of both atmospheric and evolutionary models. As a result, while our ages are consistent with estimates based on Hertzsprung-Russell isochrone fitting and dynamical expansion, they are not yet more precise. Our observations do show that with improved models, much stronger constraints should be feasible: the intrinsic uncertainties, as measured from the scatter between measurements from different spectra of the same star, are very low: around 10 K in effective temperature, 0.05 dex in surface gravity, and 0.03 dex in lithium abundance.

Erin Mentuch; Alexis Brandeker; Marten H. van Kerkwijk; Ray Jayawardhana; Peter H. Hauschildt

2008-08-26T23:59:59.000Z

320

TMS Young Leaders Professional Development Award Application  

Science Conference Proceedings (OSTI)

leadership positions in the society in the future. Funding ... $500 travel allowance toward airfare and round-trip transportation from airport to hotel. •. Tickets to ...

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321

TMS Young Leaders International Scholar Application Form  

Science Conference Proceedings (OSTI)

Zip: Country: Birth Date: Telephone Number: E-mail: Supervisor's Name: 2. EDUCATIONAL BACKGROUND (most recent). College or University: City: State:

322

The Young Leader August 09.indd  

Science Conference Proceedings (OSTI)

als Science and Toyota Central R&D Labs. Travel expenses were paid for by the TMS Foundation. Applications for the 2010 International Scholar Award must in ...

323

The Young Leader February 09.indd  

Science Conference Proceedings (OSTI)

Srikanth Bontha is a milling systems engineer at Kennametal Inc. in Latrobe, Pennsylvania, where he leads product development projects in the area of cutting ...

324

EMPMD 2014 Technical Division Young Professional Poster ...  

Science Conference Proceedings (OSTI)

InGaN light-emitting diode (LED) epitaxial layer was separated from undoped GaN/sapphire structures through a chemical lift-off process. A 0.2 µm-thick ...

325

TMS Young Leaders Committee 1998 Meeting Minutes  

Science Conference Proceedings (OSTI)

Feb 5, 1998 ... Thoughts included advanced refractories (including NASA work), nuclear fuels ( including burning weapons grade plutonium--swords into ...

326

References - Hydrate dissolution influence on the Young's ...  

Science Conference Proceedings (OSTI)

... LMT-ENS de Cachan, France, PhD Thesis. Lide, DR 1997. CRC Handbook of Chemistry and Physics. 78 th Edition. CRC ...

2004-07-27T23:59:59.000Z

327

February The Young Leader 269 5783.indd  

Science Conference Proceedings (OSTI)

p.m. as part of the 2006 TMS Annual Meeting in San Antonio, Texas. Professional and student members alike are welcome to attend the tutorial free of charge.

328

Young's Modulus Measurements in Standard IC CMOS ...  

Science Conference Proceedings (OSTI)

... 3, pp. 689–699, Mar. 1987. [3] D. Zeng et al., “Residual stress and strain in CdZnTe wafer examined by X-ray diffraction methods,” Appl. Phys. ...

2013-05-03T23:59:59.000Z

329

February 2010 Young Leader Revised 3.indd  

Science Conference Proceedings (OSTI)

University of Kentucky. Rachel DeLucas. Extraction & Processing Division. Rachel DeLucas is a process engineer in the melting operations and SGQ plant at ...

330

Diagnostics for FIRE Kenneth M. Young  

E-Print Network (OSTI)

&D and Integration Facility h ardware integration, mock-ups & in stallation Shielding/Remote Handling Integration. · Running fibers hot only affects the long-term absorption. · Great disparity in radiation effects in an -diagnostic Plasma 90° 60° 45° 20° Vacuum Vessel Test Cell Floor Quartz coherent fiber optic bundles Radiation

331

44 IAEA BULLETIN 48/2 March 2007 Science and scientists play a vital role in society. The  

E-Print Network (OSTI)

are evaluated and bal- anced, in the nuclear reactor arena, as well as in the nuclear waste arena. Science abound. From nanotech- nology, to bioengineering, to terahertz imaging, to string theory, to space movement of terrorists and illicit activity. The efforts of the IAEA to uncover the nuclear weapons

Salama, Khaled

332

B R I G H A M YOUNG UNIVERSITY BRIGHAM YOUNG UNIVERSITY  

E-Print Network (OSTI)

borings in brachiopod shells from the Caradoc Oil Shale of Estonia. Olev VINN 1 Abstract: Abundant worm (Caradoc) oil shale in North Estonia. 9 of 21 brachiopod genera (43 %) have been bored. Excluding the size. Key Words: Ordovician; Estonia; oil shale; Brachiopoda; Trypanites; palaeoecology Citation: VINN O

Seamons, Kent E.

333

Young´s Modulus of Al/Sicp/Mgal2o4 Composites with Different ...  

Science Conference Proceedings (OSTI)

Results show that with increase in particles size distribution, residual .... Using the Computational Modelling to Improve Durability of Diesel Engine Elements.

334

Assessing the massive young Sun hypothesis to solve the warm young Earth puzzle  

E-Print Network (OSTI)

A moderately massive early Sun has been proposed to resolve the so-called faint early Sun paradox. We calculate the time-evolution of the solar mass that would be required by this hypothesis, using a simple parametrized energy-balance model for Earth's climate. Our calculations show that the solar mass loss rate would need to have been 2-3 orders of magnitude higher than present for a time on the order of ~2 Gy. Such a mass loss history is significantly at variance (both in timescale and in the magnitude of the mass loss rates) with that inferred from astronomical observations of mass loss in younger solar analogues. While suggestive, the astronomical data cannot completely rule out the possibility that the Sun had the required mass loss history; therefore, we also examine the effects of the hypothetical historical solar mass loss on orbital dynamics in the solar system, with a view to identifying additional tests of the hypothesis. Planetary and satellite orbits provide a few tests, but these are weak or non-unique.

David A. Minton; Renu Malhotra

2006-12-12T23:59:59.000Z

335

'Fun with Science' travels north to Alaska  

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

312science 12132012 'Fun with Science' travels north to Alaska Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly Students in Noorvik, Alaska...

336

Why do persimmons pucker your mouth?  

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

Why do persimmons pucker your mouth? Name: Linda Martin Status: NA Age: NA Location: NA Country: NA Date: Around 1993 Question: What exactly is the astringent that is found in...

337

Clean Cities: San Joaquin Valley Clean Cities coalition  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Joaquin Valley Clean Cities Coalition Joaquin Valley Clean Cities Coalition The San Joaquin Valley Clean Cities coalition works with vehicle fleets, fuel providers, community leaders, and other stakeholders to reduce petroleum use in transportation. San Joaquin Valley Clean Cities coalition Contact Information Linda Urata 661-342-8262 iwantcleanair@aim.com Spencer Schluter 661-599-9454 scschluter@gmail.com Coalition Website Clean Cities Coordinators Coord Linda Urata Coord Coord Spencer Schluter Coord Photo of Linda Urata In 2000, Linda Urata became the coordinator of the San Joaquin Valley Clean Cities coalition. Urata works at Kern Council of Governments in Bakersfield, California. There, she coordinates the Kern Energy Watch program, which is a local government and utility company partnership effort

338

Contacts  

Gasoline and Diesel Fuel Update (EIA)

Contacts Contacts The International Energy Outlook 2011 was prepared under the general direction of John Conti, Assistant Administrator for Energy Analysis (john.conti@eia.gov, 202-586-2222), and Paul Holtberg, Team Leader, Analysis Integration Team (paul.holtberg@eia. gov, 202-586-1284). General questions concerning the content of this report may be directed to the Office of Communications (202-586-8800). Specific questions about the report should be referred to Linda E. Doman (linda.doman@eia.gov, 202-586-1041) or the following analysts: World energy demand and economic outlook ..................................... Linda E. Doman (linda.doman@eia.gov, 202-586-1041) Macroeconomic assumptions .............. Kay A. Smith (kay.smith@eia.gov, 202-586-1132)

339

International Energy Outlook 1999  

Gasoline and Diesel Fuel Update (EIA)

contacts.gif (2957 bytes) contacts.gif (2957 bytes) The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to Mary J. Hutzler (202/586-2222), Director, Office of Integrated Analysis and Forecasting, or Arthur T. Andersen, Director, International, Economic, and Greenhouse Gases Division. Specific questions about the report should be referred to Linda E. Doman (202/586-1041) or the following analysts: Report Contact World Energy Consumption Linda E. Doman - 202/586-1041 linda.doman@eia.doe.gov World Oil Markets G. Daniel Butler - 202/586-9503 gbutler@eia.doe.gov Stacy MacIntyre - 202/586-9795- (Consumption) stacy.macintyre@eia.doe.gov Natural Gas Linda E. Doman - 202/586-1041

340

Lab partners with Navajo Nation on uranium mine project  

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

> Around the Lab > atl043013navajo 04302013 Lab partners with Navajo Nation on uranium mine project Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov...

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341

Federal Energy Regulatory Commission Order on Plan for California...  

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

L. Massey, Linda Breathitt, Pat Wood III, and Nora Mead Brownell. San Diego Gas & Electric Company, Complainant, v. Docket No. EL00-95-031 Sellers of Energy and Ancillary...

342

California Is the Primary U.S. Stop for LHC's ALICE Data - NERSC...  

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

Is the Primary U.S. Stop for LHC's ALICE Data California Is the Primary U.S. Stop for LHC's ALICE Data July 30, 2010 | Tags: Fusion Energy Contact: Linda Vu, lvu@lbl.gov, +1 510...

343

Local high school seniors receive Edward Teller science scholarships  

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

3 For immediate release: 06052013 | NR-13-06-03 Local high school seniors receive Edward Teller science scholarships Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov...

344

Paducah DUF6 Conversion Final EIS - Volume 2: Comment and Response...  

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

Safety and Security 2-8 D0004 Howell, Linda Individual 2-13 D0005 Minter, Dan Southern Ohio Diversification Initiative 2-15 D0006 Justice, T.J. Ohio Governor's Office 2-16 D0007...

345

International Energy Outlook 2011  

U.S. Energy Information Administration (EIA)

Office of Intergrated and International Energy Analysis Last modified by: Wells, Peggy Created Date: 4/3/2010 1:03:38 PM Manager: Linda E. Doman 202-586-1041

346

International Energy Outlook 2011  

U.S. Energy Information Administration (EIA)

Office of Intergrated and International Energy Analysis Last modified by: PE7 Created Date: 4/3/2010 1:03:38 PM Manager: Linda E. Doman 202-586-1041 Company:

347

International Energy Outlook 2011  

U.S. Energy Information Administration (EIA)

Office of Intergrated and International Energy Analysis Last modified by: AM4 Created Date: 4/3/2010 1:03:38 PM Manager: Linda E. Doman 202-586-1041 Company:

348

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT ASSESSMENT OF LARVAL Coastal Boundary Layer Flow SEPTEMBER 2007 CEC5002013049 Prepared for: California Energy Commission Energy Commission Joe O'Hagan Contract Manager Linda Spiegel Office Manager Energy Generation Research

349

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT AN ASSESSMENT: California Energy Commission Prepared by: University of California, Davis #12; PREPARED BY: Primary Number: 500-01-016 Prepared for: California Energy Commission Prab Sethi Contract Manager Linda Spiegel

350

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT DEVELOPMENT OF STEAM5002013092AP Prepared for: California Energy Commission Prepared by: University of California #12 Energy Commission David Effross Contract Manager Linda Spiegel Office Manager Energy Generation Research

351

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT HYBRID SOLAR LIGHTING5002013067 Prepared for: California Energy Commission Prepared by: Oakridge National Laboratory Insert-04-034-18 Prepared for: California Energy Commission Hassan Mohammed Contract Manager Linda Speigel Office Manager

352

Llife-Cycle Analysis for Lithium-Ion Battery Production and Recycling  

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

No. 11-3891 Life-Cycle Analysis for Lithium-Ion Battery Production and Recycling By Linda Gaines (630) 252-4919 E-mail: lgaines@anl.gov John Sullivan (734) 945-1261 E-mail:...

353

Red Feminist Literary Analysis: Reading Violence and Criminality in Contemporary Native Women's Writing  

E-Print Network (OSTI)

Press, 1985. ---. Solar Storms : A Novel. New York:W.W. Norton, 1998. ---. Solar Storms : A Novel. New York:in Linda Hogan's Solar Storms." Things of the Spirit: Women

Nason, Dorothy Ann

2010-01-01T23:59:59.000Z

354

Lawrence Berkeley National Laboratory Advisory Board  

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

Charter members Craig Barrett (co-chair) Aime Dorr (co-chair) T.J. Glauthier Linda Katehi Y.T. Lee Robert Powell Charles Shank Robert Socolow George M. Whitesides Keith Yamamoto...

355

The Real (Porn) World: The Politics and Aesthetics of the New Reality Porn  

E-Print Network (OSTI)

Penley, “Crackers and Whackers: The White Trashing of Porn,”Porn Studies, Ed. Linda Williams, (Durham: Duke UniversityI refer to the sort of porn that one could find in a typical

Moorman, Jennifer

2007-01-01T23:59:59.000Z

356

International Video Pornography on the Internet: Crossing Digital Borders and the Un/disciplined Gaze.  

E-Print Network (OSTI)

Eroticized Asian in Gay Video Porn. In Ono, K. A CompanionBrandon Lee: The Making of A Gay Asian American Porn Star.in Linda Williams’ Porn Studies. Duke University Press,

Woida, Chloe

2009-01-01T23:59:59.000Z

357

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

human genome Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE R&D...

358

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

Saul Perlmutter Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE...

359

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

E.O. Lawrence Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE...

360

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

David Gross Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE R&D...

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We encourage you to perform a real-time search of NLEBeta
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361

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

Melvin Calvin Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE...

362

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

Glenn Seaborg Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D Accomplishments 100th Feature Page DOE...

363

OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...  

Office of Scientific and Technical Information (OSTI)

Research & Development (R&D) Accomplishments Topic 100th DOE R&D Accomplishments Feature Page Celebration by Linda McBrearty 08 Jul, 2013 in Products and Content DOE R&D...

364

The Intersection of Feminism and Disability Theory in Sylvia Plath’s The Bell Jar  

E-Print Network (OSTI)

Linda W. “Plath’s The Bell Jar as Female Bildungsroman. ”in Sylvia Plath’s The Bell Jar Jeni Maple One effect of thePlath’s 1963 novel The Bell Jar is not typically read from

Maple, Jeni

2009-01-01T23:59:59.000Z

365

NERSC Signs Supercomputing Agreement with Cray  

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

Signs Supercomputing Agreement with Cray NERSC Signs Supercomputing Agreement with Cray June 27, 2012 NERSC Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 Cray Media: Nick Davis...

366

NERSC Cited for HPC Innovations Excellence  

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

Honored for HPC Innovations Excellence NERSC Honored for HPC Innovations Excellence 20th Century Reanalysis Project Support Cited June 20, 2011 Linda Vu, lvu@lbl.gov, +1 510 486...

367

NERSC Now Connecting All Science at 100Gbps  

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

NERSC Now Connecting All Science at 100Gbps NERSC Now Connecting All Science at 100Gbps October 17, 2013 | Tags: Data Transfer, ESnet Contact: Linda Vu, +1 510 495 2402,...

368

Aging gene  

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

Aging gene Name: Linda S Martinez Location: NA Country: NA Date: NA Question: Have the aging gene or genes been located on the human chromosomes, and, if yes, will removing that...

369

Microsoft PowerPoint - 7-02 Thomas Suttora Tech Echange - 435...  

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

Order 435.1 Radioactive Waste Management Revision Status Linda Suttora, DOE HQ, EM-41 Steve Thomas, SRR EM Waste Processing Technical Exchange November 17, 2010 Print Close What is...

370

Credits  

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

Scott Coleman (Issue 2 only) Sam Webster Copy Editors Linda Comer Ann Kelly Circulation Ralph McLaughlin Pat McLaughlin HTML Composition Sondra Jarvis CBS Newsletter Home Page...

371

Data.gov  

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

Agency (EPA) also fit the profile. Kundra asked Sanjeev "Sonny" Bhagowalia, the CIO of the DOI, and Linda Travers, CIO at EPA, to co-lead the effort with other CIOs to...

372

Biofuels: Review of Policies and Impacts  

E-Print Network (OSTI)

Linda Nostbakken. Will biofuel mandates raise food prices?impacts of alternative biofuel and energy policies. WorkingJust. The welfare economics of a biofuel tax credit and the

Janda, Karel; Kristoufek, Ladislav; Zilberman, David

2011-01-01T23:59:59.000Z

373

Turtle Care  

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

Turtle Care Name: Linda Location: NA Country: NA Date: NA Question: A student brought me a small box turtle with a shell about 5 inches long. It has swollen "cheeks" and looks...

374

Next 'Science on Saturday' lecture: The 'bio' in biofuels  

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

sos 02212013 Next 'Science on Saturday' lecture: The 'bio' in biofuels Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly "The 'Bio' in Biofuels: New...

375

Seven graduate from Y-12 Apprentice Program | Y-12 National Security...  

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

Linda Bauer, who told the graduates, "I've worked at just about every site in the Nuclear Security Enterprise, and this program is one of the best I've seen." Pictured from...

376

Catching Carbon with Computer Simulations  

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

CRD and Material Sciences Researchers Receive 2 Million to Develop Efficient Carbon Capture Simulation Tools Contact: Linda Vu, lvu@lbl.gov , 510-495-2402 Share September 30,...

377

26th INTERNATIONAL CONGRESS OF THE AERONAUTICAL SCIENCES SECURITY OF WIRELESS SENSOR NETWORK ENABLED  

E-Print Network (OSTI)

** , Linda Bushnell* , Richard Robinson** *EE Department, University of Washington, Seattle, WA, USA **Boeing onboard wireless technolo- gies can be expected to be heavy. Safety con- cerns with these technologies

Poovendran, Radha

378

NERSC Users Find That Nanodroplets of Water Can Manipulate Graphene...  

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

Users Find That Nanodroplets of Water Can Manipulate Graphene NERSC Users Find That Nanodroplets of Water Can Manipulate Graphene April 30, 2010 Contact: Linda Vu, lvu@lbl.gov, +1...

379

International Energy Outlook 1998  

Annual Energy Outlook 2012 (EIA)

Doman, linda.doman@eia.doe.gov Phone: (202) 586-1041 Fax: (202) 586-3045 If you having technical problems with this site, please contact the EIA Webmaster at wmaster@eia.doe.gov...

380

Veterans helping veterans sharpen job search skills  

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

02102012 Veterans helping veterans sharpen job search skills Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly Bill Oliver of the Lab talks to...

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381

LLNL's Saturday lectures explore cutting edge science  

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

| NR-13-01-02 LLNL's Saturday lectures explore cutting edge science Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly Lawrence Livermore National...

382

'Sentinels' seeking opportunities for wounded veterans  

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

11302012 'Sentinels' seeking opportunities for wounded veterans Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly Roy Warner of the Lab's Veterans...

383

'Fun with Science' as seen on TV  

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

2113fws 03212013 'Fun with Science' as seen on TV Linda A Lucchetti, LLNL, (925) 422-5815, lucchetti1@llnl.gov Printer-friendly A crew from Tri-Valley Community television films...

384

NERSC's Hopper is Among World's Top 10 Fastest Computers  

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Hopper Among World's Top 10 Fastest Computers Hopper Among World's Top 10 Fastest Computers One of only 10 Petaflops Systems Worldwide June 17, 2011 | Tags: Hopper, NERSC Linda Vu,...

385

Microsoft Word - CNMS UEC Meeting 09-26-08 minutes.doc  

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

Tonya Klein, Scott Retterer, Mike Kilbey (ex-officio), Brian Holloway (by phone), Sandy Lowe, Tony Haynes and Linda Horton (on behalf of CNMS), and Tof Carim (from DOE)....

386

Accountable Property Representatives and Property Pass Authorization...  

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

IM-11 (202) 586-0194 SHARIATI, LINDA SC-41 (301) 903-7433 SHARPE, DEBORAH L. NE-21 (301) 903-4921 SHEA, JOHN ED-1 (202) 586-7898 Employee Authorized...

387

Lighting Energy Efficiency in Parking Campaign  

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

Lighting Energy Efficiency in Parking Lighting Energy Efficiency in Parking (LEEP) Campaign Linda Sandahl Pacific Northwest National Laboratory linda.sandahl@pnnl.gov (503) 417-7554 April 2, 2013 LEEP Campaign 2 | Building Technologies Office eere.energy.gov Purpose & Objectives: Problem Statement While new lighting technologies such as LEDs have the potential for energy savings of 75%, or more when paired with controls, there are both technology and market-related challenges. Technology Challenges

388

Lighting Energy Efficiency in Parking Campaign  

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

Lighting Energy Efficiency in Parking Lighting Energy Efficiency in Parking (LEEP) Campaign Linda Sandahl Pacific Northwest National Laboratory linda.sandahl@pnnl.gov (503) 417-7554 April 2, 2013 LEEP Campaign 2 | Building Technologies Office eere.energy.gov Purpose & Objectives: Problem Statement While new lighting technologies such as LEDs have the potential for energy savings of 75%, or more when paired with controls, there are both technology and market-related challenges. Technology Challenges

389

Developing research capacity in the social sciences: a professionality-based model  

E-Print Network (OSTI)

Developing research capacity in the social sciences: a professionality based model Dr Linda Evans Reader in Education School of Education University of Leeds Leeds, LS2 9JT UK E:mail: Linda.Evans@education.leeds.ac.uk Introduction With so many... , Issues in European teacher development: linking theory and practice, at the European Conference on Educational Research, University of Gothenburg, September 12th. Retrieved January 30th, 2009, from http://www.leeds.ac.uk/educol/documents/175518.pdf...

Evans, Linda

2009-01-01T23:59:59.000Z

390

SMALL BUSINESS INFORMATION RESOURCES Dec 27, 2011 -Page 1  

E-Print Network (OSTI)

Operations Office http://www.hanford.gov/ U.S. Department of Energy, Richland Operations Office. Click_Business_Advocate@rl.gov Linda Bell AdvanceMed Hanford(Occupational Health) P. O. Box 150, G3-70 Richland, WA 99352 (509) 376-2041 (509) 376-2020 fax e-mail: linda_l_bell@rl.gov Jason Sperling Washington Closure Hanford 2620 Fermi

391

Temperature-Dependent Young's modulus, shear modulus and Poisson's ratio of p-type Ce0.9Fe3.5Co0.5Sb12 and n-type Co0.95Pd0.05Te0.05Sb3 Skutterudite Thermoelectric Materials  

Science Conference Proceedings (OSTI)

Effective models of the mechanical behavior of thermoelectric materials under device conditions require knowledge of the temperature-dependent elastic properties.Between room temperature and 600 K, Resonant Ultrasound Spectroscopy (RUS) measurements of the Young s and shear moduli of three skutterudite thermoelectric materials, n-type Co0.95Pd0.05Te0.05Sb3(both with and without 0.1 atomic % cerium dopant) and p-type Ce0.9Fe3.5Co0.5Sb12, decreased linearly with temperature at a rate between -0.011 GPa/K and -0.013 GPa/K. In contrast the Poisson s ratio was approximately 0.22 for the three materials and was relatively insensitive to temperature.For temperatures > 600 K, the elastic moduli decreased more rapidly and resonance peaks broadened indicating the onset of viscoelastic behavior.The viscoelastic relaxation of the moduli was least for Ce-doped n-type material, for which grain boundary precipitates may inhibit grain boundary sliding which in turn has important implications concerning creep resistance. In addition, powder processing of the n- and p-type materials should be done cautiously since submicron-sized powders of both the n- and p-type powders were pyrophoric

Schmidt, Robert [Michigan State University, East Lansing; Case, Eldon D [Michigan State University, East Lansing; Ni, Jennifer E. [Michigan State University, East Lansing; Trejo, Rosa M [ORNL; Lara-Curzio, Edgar [ORNL

2012-01-01T23:59:59.000Z

392

Fermilab Colloquium Lectures: September 2010 through August 2011 (Videos)  

DOE Data Explorer (OSTI)

Fermilab has been making its Colloquium presentations available as online videos for ten years. Many of them are also available as PowerPoint slides or PDF documents. Abstracts are provided, along with information on the presenter and links to his or her home page when possible. Some titles for the 2010 - 2011 time period include: 1) Warped Dimensions, Raman Sundrum; 2) Fundamental Physics at Low Energies, Joerg Jaeckel; 3) Physics as Information Theory, Giacomo Mauro D’Ariano; 4) Introducing C++0x, Bjarne Stroustrup; 5) The New Era of Sub-millimeter Cosmology: First Results from Herschel Space Observatory, Asantha Cooray; 6) The Deepwater Horizon Disaster: What Happened and Why, Roland N. Horne; 7) High-resolution and Adaptive Methods for Plasma Physics, Phillip Colella; 8) First Results of the CMS Experiment at the LHC, Gigi Rolandi; 9) Frontiers in X-ray Science, Linda Young; 9) The Quest for Ultra-Short X-Ray Pulses, Anlexander Zholents; 10) The Search for Dark Matter with the Fermi Gamma Ray Space Telescope, Elliott Bloom; 11) Fossils, Genes, and the Origins of Organs, Neil Shubin; 12) The Path to Magnetic Fusion Energy, Stewart Prager; 13) High-Energy X-ray Studies of Real Materials Under Real Conditions and in Real Time, Jonathan Almer; 14) The Fukushima Nuclear Event and its Implications for Nuclear Power, Michael Golay; 15) Laser Wakefield Acceleration and Fundamental Physics, Toshiki Tajiima; 16) Accelerators for Subcritical Molten-Salt Reactors, Roland Johnson; 17) The Energy Challenge: The Current and Future Role of Solar Energy, Ewa Rondio.

393

Envirodevonomics: A Research Agenda for a Young Field  

E-Print Network (OSTI)

Environmental quality in many developing countries is poor and generates substantial health and productivity costs. However, existing measures of willingness to pay for environmental quality improvements indicate low ...

Greenstone, Michael

2013-09-03T23:59:59.000Z

394

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I  

E-Print Network (OSTI)

. Abstract- A Pliocene oil shale (Pula, Hungary), a C3 plant Triticum aestivum and a C4 plant Zea mays were-alkane, n-alkene, Pula oil shale, Botryococcus braunii, alga, plant, waxes, sediment. INTRODUCTION n-rich, Pliocene deposit from Pula (Hungary). The bulk carbon isotope ratio of this oil shale was also determined

Seamons, Kent E.

395

Combinatorics of Arc Diagrams, Ferrers Fillings, Young ... - CECM  

E-Print Network (OSTI)

partition can be reinterpreted as a cycle, as demonstrated in Figure 1.10. 1. 2. 3. 4. 5. 6. 7 ...... The two theorems can be combined to give the following corollary.

396

Framtidens lantbruk / Future Agriculture Young Researchers' Forum invites to free  

E-Print Network (OSTI)

quality and composition of the fodder it is possible to reduce greenhouse gas emissions considerably at the Swedish University of Agricul- tural Sciences that adress the sustai- nable use of natural resources

397

Young County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

0087°, -98.7481167° 0087°, -98.7481167° 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":33.2200087,"lon":-98.7481167,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

398

GRAVITATIONAL SLINGSHOT OF YOUNG MASSIVE STARS IN ORION  

SciTech Connect

The Orion Nebula Cluster (ONC) is the nearest region of massive star formation and thus a crucial testing ground for theoretical models. Of particular interest among the ONC's {approx}1000 members are: {theta}{sup 1} Ori C, the most massive binary in the cluster with stars of masses 38 and 9 M{sub Sun }; the Becklin-Neugebauer (BN) object, a 30 km s{sup -1} runaway star of {approx}8 M{sub Sun }; and the Kleinmann-Low (KL) nebula protostar, a highly obscured, {approx}15 M{sub Sun} object still accreting gas while also driving a powerful, apparently 'explosive' outflow. The unusual behavior of BN and KL is much debated: How did BN acquire its high velocity? How is this related to massive star formation in the KL nebula? Here, we report the results of a systematic survey using {approx}10{sup 7} numerical experiments of gravitational interactions of the {theta}{sup 1}C and BN stars. We show that dynamical ejection of BN from this triple system at its observed velocity leaves behind a binary with total energy and eccentricity matching those observed for {theta}{sup 1}C. Five other observed properties of {theta}{sup 1}C are also consistent with it having ejected BN and altogether we estimate that there is only a {approx}< 10{sup -5} probability that {theta}{sup 1}C has these properties by chance. We conclude that BN was dynamically ejected from the {theta}{sup 1}C system about 4500 years ago. BN then plowed through the KL massive star-forming core within the last 1000 years causing its recently enhanced accretion and outflow activity.

Chatterjee, Sourav; Tan, Jonathan C., E-mail: s.chatterjee@astro.ufl.edu, E-mail: jt@astro.ufl.edu [Department of Astronomy, University of Florida, Gainesville, FL 32611 (United States)

2012-08-01T23:59:59.000Z

399

Disk Planet Interactions and Early Evolution in Young Planetary Systems  

E-Print Network (OSTI)

We study and review disk protoplanet interactions using local shearing box simulations. These suffer the disadvantage of having potential artefacts arising from periodic boundary conditions but the advantage, when compared to global simulations, of being able to capture much of the dynamics close to the protoplanet at high resolution for low computational cost. Cases with and without self sustained MHD turbulence are considered. The conditions for gap formation and the transition from type I migration are investigated and found to depend on whether the single parameter M_p R^3/(M_* H^3), with M_p, M_*, R and H being the protoplanet mass, the central mass, the orbital radius and the disk semi-thickness respectively exceeds a number of order unity. We also investigate the coorbital torques experienced by a moving protoplanet in an inviscid disk. This is done by demonstrating the equivalence of the problem for a moving protoplanet to one where the protoplanet is in a fixed orbit which the disk material flows through radially as a result of the action of an appropriate external torque. For sustainable coorbital torques to be realized a quasi steady state must be realized in which the planet migrates through the disk without accreting significant mass. In that case although there is sensitivity to computational parameters, in agreement with earlier work by Masset & Papaloizou (2003) based on global simulations, the coorbital torques are proportional to the migration speed and result in a positive feedback on the migration, enhancing it and potentially leading to a runaway. This could lead to a fast migration for protoplanets in the Saturn mass range in massive disks and may be relevant to the mass period correlation for extrasolar planets which gives a preponderance of sub Jovian masses at short orbital period.

J. C. B. Papaloizou

2004-12-30T23:59:59.000Z

400

Brigham Young University Geology Studies Volume 30, Part 1  

E-Print Network (OSTI)

hear the Baltimore oriole saying "here, here, come right here, dear" and the yel- lowhammer saying "a

Seamons, Kent E.

Note: This page contains sample records for the topic "nanotech linda young" 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

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

. Javakhishvili Tbilisi State University 3 I. Tchavtchavadze Ave., 0179, Tbilisi, Georgia b School of Informatics, Engineering and Mathematics, University of Georgia 77a M. Kostava Str., 0175, Tbilisi, Georgia * gavalish

402

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3  

E-Print Network (OSTI)

by Spieker and Ree- side (1925, p. 443) for exposures near the Blackhawk coal mine On the eastern front Huntington Creek, just south of Little Swens Canyon. East of the mapped area, where coal is being mined fromTertiary floodplains. Nonmarine limestone and thin layen of coal occur in the lacustrine middle pan of the formation

Seamons, Kent E.

403

CNST's Kartik Srinivasan Receives Sigma Xi Young Scientist ...  

Science Conference Proceedings (OSTI)

... achievements within 10 years of obtaining an advanced degree, was presented by the NIST Chapter of Sigma Xi at their annual banquet on June ...

2013-04-10T23:59:59.000Z

404

TMS 2014: Annual Meeting & Exhibition - For Young Professionals  

Science Conference Proceedings (OSTI)

To submit a poster for the competition, click on the button below that best describes your work: - Submit a poster in the Electronic, Magnetic & Photonic Materials ...

405

Evolution of emission line activity in intermediate mass young stars  

E-Print Network (OSTI)

We present optical spectra of 45 intermediate mass Herbig Ae/Be stars. Together with the multi-epoch spectroscopic and photometric data compiled for a large sample of these stars and ages estimated for individual stars by using pre-main sequence evolutionary tracks, we have studied the evolution of emission line activity in them. We find that, on average, the H_alpha emission line strength decreases with increasing stellar age in HAeBe stars, indicating that the accretion activity gradually declines during the PMS phase. This would hint at a relatively long-lived (a few Myr) process being responsible for the cessation of accretion in Herbig Ae/Be stars. We also find that the accretion activity in these stars drops substantially by ~ 3 Myr. This is comparable to the timescale in which most intermediate mass stars are thought to lose their inner disks, suggesting that inner disks in intermediate mass stars are dissipated rapidly after the accretion activity has fallen below a certain level. We, further find a relatively tight correlation between strength of the emission line and near-infrared excess due to inner disks in HAeBe stars, indicating that the disks around Herbig Ae/Be stars cannot be entirely passive. We suggest that this correlation can be understood within the frame work of the puffed-up inner rim disk models if the radiation from the accretion shock is also responsible for the disk heating.

P. Manoj; H. C. Bhatt; G. Maheswar; S. Muneer

2006-08-25T23:59:59.000Z

406

Young, Gifted & Black: Reflections, Commentaries and Girl Talk  

E-Print Network (OSTI)

Girl Talk By Carah L. B. Herring UC Berkeley Graduate Schoolfor my household, The Herring Insider (Circulation: 4. We’ll

Herring, Carah L

2011-01-01T23:59:59.000Z

407

Improving leadership capabilities for young employers at Kirin  

E-Print Network (OSTI)

My employer, Kirin Holding Company (Kirin), turned 100 years old in 2007. At the same year, Kirin changed its company structure into a holding company from Kirin Brewery Company Limited. As the former company name indicates, ...

Onuki, Hiroshi, M.B.A. Massachusetts Institute of Technology

2008-01-01T23:59:59.000Z

408

TMS Names 2013 Young Leader Professional Development Award  

Science Conference Proceedings (OSTI)

Mar 6, 2013 ... Angela Fenwick Strategic Communications Campaign Manager The Minerals ... Guang Sheng, Scientific Forming Technology Corp. Extraction ...

409

The Young Leader August 2010 version2.indd - TMS  

Science Conference Proceedings (OSTI)

Babu is currently an associate professor at. The Ohio State University and a Distinguished. Scholar of Edison Welding Institute, both based in Columbus, Ohio.

410

The effect of young biochar on soil respiration  

Science Conference Proceedings (OSTI)

The low temperature pyrolysis of organic material produces biochar, a charcoal like substance. Biochar is being promoted as a soil amendment to enhance soil quality, it is also seen as a mechanism of lomg-term sequestration of carbon. Our experiments tested the hypothesis that biochar is inert in soil. However, we measured an increase in CO2 production from soils after biochar amendment which increased with increasing rates of biochar. The ?13C signature of the CO2 evolved in the first several days of the incubation was the same as the ?13C signature of the biochar, confirming that biochar contributed to the CO2 flux. This effect diminished by day 6 of the incubation suggesting that most of the biochar C is slowly decomposing. Thus, aside from this short term mineralization increasing soil C with biochar may indeed be a long term C storage mechanism.

Smith, Jeffery L.; Collins, Harold P.; Bailey, Vanessa L.

2010-12-01T23:59:59.000Z

411

BRIGHAM YOUNG UNIVERSITY 2BYU 20122013 Graduate Catalog  

E-Print Network (OSTI)

include: pyrolysis, gasification, anaerobic digestion, mixed waste composting, plasma arc, and chemical ..................................................................................17 4.2 Gasification.4 Mixed Waste Composting............................................................21 4.5 Plasma Arc

Crandall, Keith A.

412

William E. and Diane M. Spicer Young Investigator Award | Stanford...  

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

esteemed member of the international scientific community as a teacher and researcher in electrical engineering, applied physics and materials science. Bill spent the past 40...

413

Brigham Young University Geology Studies Volume 27, Part 2  

E-Print Network (OSTI)

along the Southern Wasatch, Fish Springs, and House Ranges Wah Wah Range, Beaver County, Utah .................. Richard F. Wheeler Publications and Maps. Ccntrdl W d h Wdh Range. R e a ~ e r('ount~.1itah Ah\\trac r Inr~odurtlon #12

Seamons, Kent E.

414

Brigham Young University Geology Studies Volume 28, Part 3  

E-Print Network (OSTI)

, Southern Pavant Range, Utah December 1981 12-81600 52593 #12;CONTENTS Three Creeks Caldera. Southern Pavant Range. Utah ..............................................Dacite of Shauntie Hills ............................................Needles Range Formation Wah Wah

Seamons, Kent E.

415

Early Childbearing among Mexican-American Young Women: Place Matters  

E-Print Network (OSTI)

County Teen Birth Rates by Zip Code. Alameda County Publicteenagers in California zip code areas. Family Planningteenagers in California zip code areas. Family Planning

Richardson, Dawn Michele

2010-01-01T23:59:59.000Z

416

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

objects such as airplanes, nuclear power plants, rotor blades of wind turbines, damage detecting Application of the integral approach and wavelet transform in simulating and analysis of guided waves and numerical results. Keywords: guided waves; Lamb wave; debonding; structural health monitoring; piezoactuator

417

Serving the Brigham Young University Community universe.byu.edu  

E-Print Network (OSTI)

, and embroidered with the words, "Florida Python Hunters." Then the hike back to their Toyota Prius, which

Seamons, Kent E.

418

NOW OPEN: Young Professional "Meet the Candidate" Poster Session  

Science Conference Proceedings (OSTI)

There will be a master board, which will indicate the name of the candidate, the title of their poster and the location and times for their oral presentations (if ...

419

Biomedical Research Mentorship: The Young Investigators' Innovative High School Program  

E-Print Network (OSTI)

Hill V, Goodchild F. (1993) Apprentice Researchers at QUEST.Santa Barbara, the Apprentice Researchers at QUEST Program (Biotechnology Program, and the Apprentice Research at QUEST

Pham, Laura; Bragg, Richard; Uchio, Ken; Husted, Cynthia A. Ph.D.

2006-01-01T23:59:59.000Z

420

Eye-In-Hand Visual Servoing Curriculum for Young Students  

E-Print Network (OSTI)

It is never too early to introduce students to robotics. Inspired by courses that use Lego Mindstorms as platform, by the huge success of the FIRST competition, and by the interest and enthusiasm of many local robotics ...

Rus, Daniela L.

Note: This page contains sample records for the topic "nanotech linda young" 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 DYNAMIC EVOLUTION OF YOUNG EXTRAGALACTIC RADIO SOURCES  

SciTech Connect

The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth stages of the radio luminosity versus size of the source. The interaction of the jet with the ambient medium results in the formation and evolution of sources with non-standard (flaring) morphology. In addition, cessation or restarting of the jet power and obstruction of the jet will also result in distinct morphological structures. The radio source population may thus be classified in morphological types that indicate the prevailing physical processes. Compact symmetric objects (CSOs) occupy the earliest evolutionary phase of symmetric radio sources and their dynamical behavior is fundamental for any further evolution. Analysis of CSO dynamics is presented for a sample of 24 CSOs with known redshift and hotspot separation velocity and with a large range of radio power. Observables such as radio power, separation between two hotspots, hotspot separation velocity, and kinematic age of the source are found to be generally consistent with the self-similar predictions for individual sources that reflect the varying density structure of the ambient interstellar medium. Individual sources behave different from the group as a whole. The age and size statistics confirm that a large fraction of CSOs does not evolve into extended doubles.

An Tao [Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai (China); Baan, Willem A., E-mail: antao@shao.ac.cn, E-mail: baan@astron.nl [ASTRON, P.O. Box 2, 7990-AA Dwingeloo (Netherlands)

2012-11-20T23:59:59.000Z

422

MPMD 2014 Technical Division Young Professional Poster Contest  

Science Conference Proceedings (OSTI)

Graphics should be simple, colorful, well labeled and clear. The title should be written in letters 2 cm (3/4") to 5 cm (2") high, and all material should be readable  ...

423

2013 Young Leader "Meet the Candidate" Poster Session  

Science Conference Proceedings (OSTI)

Mar 3, 2013 ... Materials Master Student Looks for a Full-time Engineer Job: Shuai Wan1; ... Liquid Metal Batteries for Large Scale Energy Storage Applications: ... feature of these batteries is the continuous creation and annihilation of the ...

424

2006 Young Leader International Scholar Experience By: W. Jud ...  

Science Conference Proceedings (OSTI)

May 18, 2006 ... lab visits and arranging hosts in various cities. ... times when traveling between cities. ... $25 payable to City of Atlanta can perhaps go on our.

425

Young's Modulus and Poisson's Ratio on Piezoelectric Ceramics to ...  

Science Conference Proceedings (OSTI)

... of the Localized Temperature during a Back Grinding Process for TSV Wafers ... Porosification of CaO-B2O3-SiO2 Glass Ceramics by Selective Etching for ...

426

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4  

E-Print Network (OSTI)

to )/( nmn + & . This result is in agreement with experimental data of oil shale (Grady et al., 1980, 1972, p. 129-140. Grady D.E., Kipp M.E., « Continuum Modeling of Explosive Fracture in Oil Shale », Int

Seamons, Kent E.

427

University of Florida Performing Arts Young Concert Artist  

E-Print Network (OSTI)

. Doch hast du das Mahl genossen, den Durst gestillt, Dann verlasse der lauten Genossen festfreudiges

Roy, Subrata

428

Three-Fold Increase in the Young's Modulus of Graphite ...  

Science Conference Proceedings (OSTI)

... Microstructures into Li-ion battery ... EV: Need double the energy density of presently available Li batteries ... Atomic Charges in Li-GIC Structures a3 ...

2012-10-04T23:59:59.000Z

429

Anatomy of a young giant component in the random graph  

E-Print Network (OSTI)

We provide a complete description of the giant component of the Erd\\H{o}s-R\\'enyi random graph $G(n,p)$ as soon as it emerges from the scaling window, i.e., for $p = (1+\\epsilon)/n$ where $\\epsilon^3 n \\to \\infty$ and $\\epsilon=o(1)$. Our description is particularly simple for $\\epsilon = o(n^{-1/4})$, where the giant component $C_1$ is contiguous with the following model (i.e., every graph property that holds with high probability for this model also holds w.h.p. for $C_1$). Let $Z$ be normal with mean $\\frac23 \\epsilon^3 n$ and variance $\\epsilon^3 n$, and let $K$ be a random 3-regular graph on $2\\lfloor Z\\rfloor$ vertices. Replace each edge of $K$ by a path, where the path lengths are i.i.d. geometric with mean $1/\\epsilon$. Finally, attach an independent Poisson($1-\\epsilon$)-Galton-Watson tree to each vertex. A similar picture is obtained for larger $\\epsilon=o(1)$, in which case the random 3-regular graph is replaced by a random graph with $N_k$ vertices of degree $k$ for $k\\geq 3$, where $N_k$ has mean...

Ding, Jian; Lubetzky, Eyal; Peres, Yuval

2009-01-01T23:59:59.000Z

430

What could infant and young child nutrition learn from sweatshops?  

E-Print Network (OSTI)

: accounting for ethical, social, cultural and commercialization issues. J Technol Manag Innov 2009, 4(3):24-33. Pre-publication history The pre-publication history for this paper can be accessed here: http://www.biomedcentral.com/1471-2458/11/276/prepub doi:10...

Singer, Peter A; Ansett, Sean; Sagoe-Moses, Isabella

2011-05-05T23:59:59.000Z

431

Understanding Wye Using Traditional Timber to Connect Young People  

E-Print Network (OSTI)

Biblins Youth Campsite accessible to groups from all backgrounds and abilities by improving facilities constructed. · Solar powered toilets and shower facilities will be installed before the end of 2007 and opened to follow for successful projects. · Joined-up thinking is essential between FC staff, stakeholders

432

NETL: News Release - Brigham Young University Professor Named...  

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

Fossil Fuel Combustion in Announcing 25,000 Award WASHINGTON, DC - Secretary of Energy Spencer Abraham today announced that the Department of Energy's 2002 Homer H. Lowry...

433

SMD 2013 Technical Division Young Professional Poster Contest  

Science Conference Proceedings (OSTI)

Mar 4, 2013... candidate materials for structural applications in nuclear reactors as .... Yield Point: Amit Pandey1; Robert Wheeler2; Amit Shyam1; 1ORNL; ...

434

Young: The Ute Indians of Colorado in the Twentieth Century  

E-Print Network (OSTI)

The Ute Indians of Colorado in the Twentieth Century.Bibliography of the Ute In- dians of Colorado.Beulder: University of Colorado Studies, Series in

Knack, Martha C.

1999-01-01T23:59:59.000Z

435

NEWS ON THE s PROCESS FROM YOUNG OPEN CLUSTERS  

SciTech Connect

Recent spectroscopic measurements in open clusters younger than the Sun with [Fe/H] {approx}> 0 showed that the abundances of neutron-rich elements have continued to increase in the Galaxy after the formation of the Sun, roughly maintaining a solar-like distribution. This growth requires neutron fluences larger than those so far assumed, as these would have too few neutrons per iron seed. We suggest that the observed enhancements can be produced by nucleosynthesis in asymptotic giant branch (AGB) stars of low mass (M < 1.5 M{sub Sun }) if they release neutrons from the {sup 13}C({alpha},n){sup 16}O reaction in reservoirs larger by a factor of four than assumed in more massive AGB stars (M > 1.5 M{sub Sun }). Adopting such a stronger neutron source as a contributor to the abundances at the time of formation of the Sun, we show that this also affects the solar s-process distribution, so that its main component is well reproduced, without the need to assume ad hoc primary sources for the synthesis of s elements up to A {approx} 130, contrary to suggestions from other works. The changes in the expected abundances that we find are primarily due to the following reasons. (1) Enhancing the neutron source increases the efficiency of the s process, so that the ensuing stellar yields now mimic the solar distribution at a metallicity higher than before ([Fe/H ] {approx}> -0.1). (2) The age-metallicity relation is rather flat for several Gyr in that metallicity regime, so that those conditions remain stable and the enhanced nuclear yields, which are necessary to maintain a solar-like abundance pattern, can dominate the composition of the interstellar medium from which subsequent stars are formed.

Maiorca, Enrico; Busso, Maurizio; Palmerini, Sara; Trippella, Oscar [Department of Physics, University of Perugia, Via Pascoli, 06122 Perugia (Italy); Magrini, Laura; Randich, Sofia, E-mail: emaiorca@gmail.com [INAF, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze (Italy)

2012-03-01T23:59:59.000Z

436

Brigham Young University Geology Studies Volume 27, Part 2  

E-Print Network (OSTI)

geological deposits, such as oil shale, to extract hydrocarbons for energy needs. The apparatus provides more. The apparatus allows the liquid metal to distribute heat evenly throughout the oil shale. This reduces by providing more even heat distribution ·· Reduces costs associated with in situ heat extraction of oil shale

Seamons, Kent E.

437

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

of weak intensity using synchrotron radiation to reduce the exposure time to 1 s. It is also noted in section 2 from an adequate choice of free energy and internal variables. The model is then validated

438

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

both among scientists and environmentalists and even among politicians. A wake behind a modern heavy planes Boeing-737. The main aim of the work was to study the influence of computational domain

439

The awarded young adult novel in Greece (1985-2004).  

E-Print Network (OSTI)

??The purpose of this study was to examine the adolescent novels that were awarded in Greece from 1985 till 2005 by four major organizations. The… (more)

Komninou, Nikolitsa

2006-01-01T23:59:59.000Z

440

TMS Foundation Focus, 1 (1): Young Leaders Program  

Science Conference Proceedings (OSTI)

Jon Kellar (not pictured)--South Dakota School of Mines, Rapid City, South Dakota; Jennifer Lewis (not pictured)--University of Illinois, Urbana, Illinois; Thomas ...

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While these samples are representative of the content of NLEBeta,
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441

Who Creates Jobs? Small vs. Large vs. Young* By John ...  

Science Conference Proceedings (OSTI)

... less rapidly with firm age than does job destruction ... Birch, David L., 1981, “Who Creates Jobs?” The ... Sue, 1984, "Find the Firm", Proceedings of the ...

2013-12-24T23:59:59.000Z

442

International Energy Outlook 1998  

Gasoline and Diesel Fuel Update (EIA)

Contacts Contacts The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to Mary J. Hutzler (202/586-2222), Director, Office of Integrated Analysis and Forecasting, or Arthur T. Andersen (202/586-1441), Director, International, Economic, and Greenhouse Gases Division. Specific questions about the report should be referred toLinda E. Doman (202/586-1041) or the following analysts: World Energy Consumption Arthur Andersen (art.andersen@eia.doe.gov, 202/586-1441) Linda E. Doman (linda.doman@eia.doe.gov, 202/586-1041) World Oil Markets G. Daniel Butler (george.butler@eia.doe.gov, 202/586-9503) Perry Lindstrom (perry.lindstrom@eia.doe.gov, 202/586-0934) Reformulated Gasoline

443

International Energy Outlook 2002 - Contacts  

Gasoline and Diesel Fuel Update (EIA)

Contacts Contacts The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to Mary J. Hutzler (202/586-2222), Director, Office of Integrated Analysis and Forecasting. Specific questions about the report should be referred to Linda E. Doman (202/586-1041) or the following analysts: World Energy Consumption Linda Doman linda.doman@eia.doe.gov, 202/586-1041 World Oil Markets G. Daniel Butler Aloulou Fawzi george.butler@eia.doe.gov aloulou.fawzi@eia.doe.gov 202/586-9503 202/586-7818 Natural Gas Phyllis Martin Bruce Bawks phyllis.martin@eia.doe.gov bruce.bawks@eia.doe.gov 202/586-9592 202/586-6579 ChinaÂ’s West-to-East Pipeline Aloulou Fawzi aloulou.fawzi@eia.doe.gov 202/586-7818

444

International Energy Outlook 2000 - Contacts  

Gasoline and Diesel Fuel Update (EIA)

The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to Mary J. Hutzler (202/586-2222), Director, Office of Integrated Analysis and Forecasting. Specific questions about the report should be referred to Linda E. Doman (202/586-1041) or the following analysts: Report Contact World Energy Consumption Linda E. Doman - 202/586-1041 linda.doman@eia.doe.gov World Oil Markets G. Daniel Butler - 202/586-9503 gbutler@eia.doe.gov Bruce Bawks - 202/586-6579 bruce.bawks@eia.doe.gov Natural Gas Phyllis Martin - 202/586-9592 phyllis.martin@eia.doe.gov Gas-to-Liquids Technology William Trapmann - 202/586-6408 william.trapmann@eia.doe.gov Coal Michael Mellish - 202/586-2136

445

EIA - Forecasts and Analysis of Energy Data  

Gasoline and Diesel Fuel Update (EIA)

Contacts Contacts The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to John J. Conti (john.conti@eia.doe.gov, 202-586-2222), Director, Office of Integrated Analysis and Forecasting. Specific questions about the report should be referred to Linda E. Doman (202/586-1041) or the following analysts: World Energy and Economic Outlook Linda Doman (linda.doman@eia.doe.gov, 202-586-1041) Macroeconomic Assumptions Nasir Khilji (nasir.khilji@eia.doe.gov, 202-586-1294) Energy Consumption by End-Use Sector Residential Energy Use John Cymbalsky (john.cymbalsky@eia.doe.gov, 202-586-4815) Commercial Energy Use Erin Boedecker (erin.boedecker@eia.doe.gov, 202-586-4791)

446

Getting Traffic Lights Talking to Improve Topeka's Traffic Tunnel |  

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

Getting Traffic Lights Talking to Improve Topeka's Traffic Tunnel Getting Traffic Lights Talking to Improve Topeka's Traffic Tunnel Getting Traffic Lights Talking to Improve Topeka's Traffic Tunnel October 8, 2010 - 11:16am Addthis Topeka is using Recovery Act funding to resynchronize 22 traffic lights. | Photo by Linda Voss Topeka is using Recovery Act funding to resynchronize 22 traffic lights. | Photo by Linda Voss Lindsay Gsell The five-lane 21st street corridor in Topeka is a hub for restaurants, shopping and entertainment. "This is where everyone in Topeka goes to shop," says Topeka resident Linda Voss. In addition to food and fun, the one-mile corridor is home to seven traffic lights-and for drivers, a potential traffic stop every 754 feet, or a little more than two football fields. "The traffic signals are a challenge to time in this area," says Voss,

447

Page not found | Department of Energy  

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

11 - 3920 of 28,905 results. 11 - 3920 of 28,905 results. Download HSS Focus Group Meeting (Topical Meeting) Safety Standards/10 CFR 851 Meeting agenda, summary and information package Meeting Date: July 17, 2008 http://energy.gov/hss/downloads/hss-focus-group-meeting-topical-meeting-2 Download VWD-0007- In the Matter of Linda D. Gass This determination will consider a Motion for Discovery filed with the Office of Hearings and Appeals (OHA) by Linda D. Gass. This Motion, dated August 10, 1999, concerns the hearing requested by... http://energy.gov/oha/downloads/vwd-0007-matter-linda-d-gass Download Application to Export Electric Energy OE Docket No. EA-327-A DC Energy LLC: Federal Register Notice, Volume 77, No. 102- May 25, 2012 Application from DC Energy to export electric energy to Canada. Federal

448

Page not found | Department of Energy  

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

11 - 11620 of 26,764 results. 11 - 11620 of 26,764 results. Download Financial and Activity Report- August 7, 2009 http://energy.gov/downloads/financial-and-activity-report-august-7-2009 Download VWR-0003- In the Matter of Linda D. Gass This decision will consider a "Motion to Revive Disclosures Dismissed Prior to the Enactment of Revisions to Part 708" Linda D. Gass filed on March 8, 1999. In her Motion, Ms. Gass requests that I... http://energy.gov/oha/downloads/vwr-0003-matter-linda-d-gass Download Rebuilding It Better; BTI-Greensburg, John Deere Dealership (Brochure) (Revised) This case study highlights the energy-saving features of the BTI-Greensburg John Deere Dealership. This metal building is expected to save close to 50% in annual energy cost. http://energy.gov/eere/downloads/rebuilding-it-better-bti-greensburg-john-deere-dealership-brochure-revised

449

International Energy Outlook 2001 - Contact  

Gasoline and Diesel Fuel Update (EIA)

Contacts Contacts Printer Friendly Version (PDF) The International Energy Outlook is prepared by the Energy Information Administration (EIA). General questions concerning the contents of the report should be referred to Mary J. Hutzler (202/586-2222), Director, Office of Integrated Analysis and Forecasting. Specific questions about the report should be referred to Linda E. Doman (202/586-1041) or the following analysts: World Energy Consumption Linda Doman (linda.doman@eia.doe.gov, 202/586-1041) World Oil Markets G. Daniel Butler (george.butler@eia.doe.gov, 202/586-9503) Bruce Bawks (bruce.bawks@eia.doe.gov, 202/586-6579) Natural Gas Sara Banaszak Phyllis Martin (phyllis.martin@eia.doe.gov, 202/586-9592) Coal Sara Banaszak

450

U.S. Department of Energy NEPA Categorical Exclusion Determination Form  

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

CA-City-Yorba Linda CA-City-Yorba Linda Location: City Yorba Linda CA American Recovery and Reinvestment Act: Proposed Action or Project Description: Retrofit of ball field lighting, irrigation system, turf reduction, lights and street lights throughout city facilities and replace the roof-top air-conditioning heating unit and associated duct work located in City Hall with a new unit. Conditions: In accordance with California Programmatic Agreement Categorical Exclusion(s) Applied: B2.5, B5.1 *-For the complete DOE National Environmental Policy Act regulations regarding categorical exclusions, see Subpart D of 10 CFR10 21 This action would not: threaten a violation of applicable statutory, regulatory, or permit requirements for environment, safety, and health,

451

LIME: A coordination model and middleware supporting mobility of hosts and agents  

Science Conference Proceedings (OSTI)

LIME (Linda in a mobile environment) is a model and middleware supporting the development of applications that exhibit the physical mobility of hosts, logical mobility of agents, or both. LIME adopts a coordination perspective inspired by work on the ... Keywords: Mobile computing, middleware, tuple spaces

Amy L. Murphy; Gian Pietro Picco; Gruia-Catalin Roman

2006-07-01T23:59:59.000Z

452

Center for the Environment at Purdue University  

E-Print Network (OSTI)

are involved in activities around the world; places like China and Azerbaijan, Panama and Alaska, and of course, Caucasus Mountains, Azerbaijan John Lee Associate Director September 1, 2008 ­Current Linda Lee Associate in Azerbaijan Center Director John Bickham has been involved in biodiversity and ecotoxicology studies

453

EAC Meeting Transcript October 15, 2012  

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

UNITED STATES DEPARTMENT OF ENERGY UNITED STATES DEPARTMENT OF ENERGY ELECTRICITY ADVISORY COMMITTEE MEETING Washington, D.C. Monday, October 15, 2012 2 1 PARTICIPANTS: 2 EAC: 3 RICHARD COWART, Chair Regulatory Assistance Project 4 WILLIAM BALL 5 Southern Company 6 LINDA BLAIR 7 RICK BOWEN 8 MERWIN BROWN California Institute for Energy and 9 Environment 10 PAUL CENTOLELLA Public Utilities Commission of Ohio

454

EAC Meeting Transcript October 16, 2012  

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

Washington, D.C. Tuesday, October 16, 2012 2 1 PARTICIPANTS: 2 EAC: 3 RICHARD COWART, Chair Regulatory Assistance Project 4 WILLIAM BALL 5 Southern Company 6 LINDA BLAIR 7 RICK BOWEN 8 MERWIN BROWN California Institute for Energy and 9 Environment 10 PAUL CENTOLELLA Public Utilities Commission of Ohio 11 ROBERT CURRY 12 New York State Public Service Commission 13 CLARK GELLINGS

455

CALIFORNIA POSTSECONDARY EDUCATION COMMISSION PRESS RELEASE  

E-Print Network (OSTI)

CALIFORNIA POSTSECONDARY EDUCATION COMMISSION PRESS RELEASE Contact: Linda White California Postsecondary Education Commission 1303 J Street, Suite 500 Sacramento, California 95814-2938 (916) 322-7984 lwhite@cpec.ca.gov Commission Awards $1,889,657 Grant to California State University Fullerton to Improve

de Lijser, Peter

456

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT LIFE-CYCLE ASSESSMENT AND URBAN SUSTAINABILITY OCTOBER 2010 CEC-500-2013-129 Prepared for: California Energy Commission Prepared by: University for: California Energy Commission Erik Stokes Contract Manager Linda Spiegel Office Manager Energy

457

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT INTEGRATING BIOENERGETICS, SPACIAL for: California Energy Commission Prepared by: University of California, Santa Barbara #12;PREPARED BY Number: UC MRA-061 Prepared for: California Energy Commission Joe O'Hagan Contract Manager Linda Spiegel

458

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT RWE SCHOTT SOLAR Energy Commission Prepared by: RWE Schott Solar, Inc #12; PREPARED BY: Primary Author(s): Miles C: California Energy Commission Hassan Mohammed Project Manager Linda Spiegel Office Manager Energy Generation

459

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT COMPENSATION CEC5002013114 Prepared for: California Energy Commission Prepared by: Stratus Consulting Inc. #12-04-025 Prepared for: California Energy Commission Joe O'Hagan Contract Manager Linda Spiegel Office Manager Energy

460

Energy Research and Development Division FINAL PROJECT REPORT  

E-Print Network (OSTI)

Energy Research and Development Division FINAL PROJECT REPORT Integrated CHP Using UltraLow NOx Supplemental Firing MARCH 2013 CEC5002013043 Prepared for: California Energy://www.gastechnology.org Contract Number: PNG-07-006 Prepared for: California Energy Commission Gail Wiggett Project Manager Linda

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


461

The SGB/NP Hydration Free Energy Model Based on the Surface Generalized Born Solvent Reaction Field and  

E-Print Network (OSTI)

The SGB/NP Hydration Free Energy Model Based on the Surface Generalized Born Solvent Reaction Field and Novel Nonpolar Hydration Free Energy Estimators EMILIO GALLICCHIO, LINDA YU ZHANG, RONALD M. LEVY Generalized Born continuum dielectric electrostatic model using explicit solvent free energy perturbation

462

United States Department of  

E-Print Network (OSTI)

. Assoc. for Law Placement Lea Souza-Rasile, JD `87 Heather M. Spencer, JD `83 Thomas R. Spencer, Jr., JD Polen Michael John Ryan Thomas R. Spencer, Jr. Joseph Teichman Linda L. Vitale Edward James Waldron. Gurland, Jr. Douglas Martin Halsey Kathleen Gaye Hoague Michael George Joyce Warren J. Kozlow Bernard

Nassauer, Joan Iverson

463

PAUL SHORT --MENS BROWN file:///Users/bkatten/Desktop/R092812AF.html[9/28/12 4:04:11 PM  

E-Print Network (OSTI)

Sarah J. Girotti '93 ++ Bernard Gitlin '62 '89P '92P ++ John H. Glanville '77 ++ William A. Glaser, Jr Richard F. Boyer '68 ++ Richard R. Bradley '61 Charles J. Brand '74 `77G++ James A. Branegan, Jr. '35 ++ D A. Broscious '55 ++ David B. Brown `12P Harry K. Brown, Jr. `66 Judith S. Brown `12P Linda K. Brown

Royer, Dana

464

PAST HAA AWARD RECIPIENTS 1990 Harriet B. Belin, R '43  

E-Print Network (OSTI)

. Spencer Jr., JD `69 Sambamurthy Subramanian, JD `98 Christine & Frederick Swerdlow Tabas, Freedman Deichmann Holly Marvin S. Maltzman Ray E. Marchman, Jr. Joseph B. Merlin Martin J. Nash Bernard Rabinowitz Frederick Steven Robbins Michael John Ryan Thomas R. Spencer, Jr. Joseph Teichman Hon. Linda L. Vitale

465

Report to Donors The University of Georgia and The Arch Foundation for The University of Georgia  

E-Print Network (OSTI)

. Assoc. for Law Placement Lea Souza-Rasile, JD `87 Heather M. Spencer, JD `83 Thomas R. Spencer, Jr., JD Polen Michael John Ryan Thomas R. Spencer, Jr. Joseph Teichman Linda L. Vitale Edward James Waldron. Gurland, Jr. Douglas Martin Halsey Kathleen Gaye Hoague Michael George Joyce Warren J. Kozlow Bernard

Scott, Robert A.

466

Alphabetical List of LSU School of Renewable Natural Resources Graduates 1926-2008 Prepared by Dr. Paul Y. Burns, Prof. Emeritus, School of RNR, Dec. 26, 2008  

E-Print Network (OSTI)

Richard T. Begley George D. Bouline, Jr. Mr. and Mrs. Bernard W. Castor Robert R. Cutler Susan and John and Bernard Gitlin Suzanne and Edwin H. Gott, Jr. Sharon and Thomas Gratto William C. Hale Linda and Wilfrid and Robert Mitchell 1875 E. H. Williams, Jr. 1876 Charles W. MacFarlane Charles L. Taylor 1878 Henry M

467

Life Members The University of Memphis Alumni Association gratefully acknowledges its esteemed life members. Life  

E-Print Network (OSTI)

. Spencer Jr., JD `69 Sambamurthy Subramanian, JD `98 Christine & Frederick Swerdlow Tabas, Freedman Deichmann Holly Marvin S. Maltzman Ray E. Marchman, Jr. Joseph B. Merlin Martin J. Nash Bernard Rabinowitz Frederick Steven Robbins Michael John Ryan Thomas R. Spencer, Jr. Joseph Teichman Hon. Linda L. Vitale

Memphis, University of

468

APPLIED AND ENVIRONMENTAL MICROBIOLOGY, 0099-2240/00/$04.00 0  

E-Print Network (OSTI)

[U(IV)] can be utilized to remove soluble uranium from groundwaters, mine waters, or secondary waste of Uranium U(VI) under Variable Sulfate Concentrations by Sulfate-Reducing Bacteria JOHN R. SPEAR,* LINDA A. FIGUEROA, AND BRUCE D. HONEYMAN Division of Environmental Science and Engineering, Colorado School of Mines

469

PhD Chemical Engineering MS Chemical Engineering  

E-Print Network (OSTI)

1 PhD Chemical Engineering MS Chemical Engineering Bylaws Gene and Linda Voiland School of ChemicalD Chemical Engineering, MS Chemical Engineering B. Discipline: Edgar, et al.1 provide a succinct description of chemical engineering: "chemical engineers seek to understand, manipulate, and control the molecular basis

Collins, Gary S.

470

LIHD biofuels: toward a sustainable future  

E-Print Network (OSTI)

LIHD biofuels: toward a sustainable future 115 Linda Wallace, Department of Botany and Microbiology of America www.frontiersinecology.org Will biofuels help to wean the US off of oil, or at least off simple. First, we need to understand what is meant by the term "biofuel". All biofuels are organic

Palmer, Michael W.

471

NATURAL GAS ADVISORY COMMITTEE Name Affiliation Sector  

E-Print Network (OSTI)

NATURAL GAS ADVISORY COMMITTEE 2011-2013 Name Affiliation Sector Dernovsek, David Bonneville Power Defenbach, Byron Intermountain Gas Distribution Dragoon, Ken NWPCC Council Friedman, Randy NW Natural Gas Distribution Gopal, Jairam Southern CA Edison Electric Utility Hamilton, Linda Shell Trading Gas & Power

472

UMassLowellM A G A Z I N E F O R A L U M N I A N D F R I E N D S WINTER 2011  

E-Print Network (OSTI)

. Danser `33* Lemoyne E. Decker `33* 1934 PRESIDENT ASSOCIATES Elinor and S. Murray Rust, Jr. `34 `61P `67P Rust `57 `82P `88P ++ SOCIETY ASSOCIATES Joan H. and Delamar T. Bell, Jr. `57 Patricia and E. Richard. Murray Rust III `61 `62 Carol A. and Paul E. Smith `61 `93P ++ Gladys E. and George C. Spill `61 ++ Linda

Massachusetts at Lowell, University of

473

in appreciation Online Annual Report of Giving  

E-Print Network (OSTI)

. Danser `33* Lemoyne E. Decker `33* 1934 PRESIDENT ASSOCIATES Elinor and S. Murray Rust, Jr. `34 `61P `67P Rust `57 `82P `88P ++ SOCIETY ASSOCIATES Joan H. and Delamar T. Bell, Jr. `57 Patricia and E. Richard. Murray Rust III `61 `62 Carol A. and Paul E. Smith `61 `93P ++ Gladys E. and George C. Spill `61 ++ Linda

Napier, Terrence

474

A Lightweight Coordination Middleware for Mobile Computing  

E-Print Network (OSTI)

, and Gregory Hackmann Department of Computer Science and Engineering Washington University in Saint Louis Saint. Limone tailors Linda-like primitives for mobile environments by eliminating remote blocking and complex, explain its key features, and explore its capabilities as a coordi- nation model. A universal remote

Roman, Gruia-Catalin

475

April 6, 2009 Submitted/Glen White  

E-Print Network (OSTI)

Meaghan C. Gragg e. John & yali C. Gregory LindaS.Griffin&RobertD.Keliher,Sr. Dustin G. Hall Whitney C remedies · Fassett, Anthony & Taylor, P.A. secured transactions · Avila Rodriguez Hernandez Mena & Ferri. Lawrence & elizabeth e. Heinkel Brett T. & Rhonda K. Hendee* eugenio Hernandez Hicks, Porter, ebenfeld

Peterson, Blake R.

476

Dean's List -Winter Term 2011 Walaa Abada  

E-Print Network (OSTI)

Meaghan C. Gragg e. John & yali C. Gregory LindaS.Griffin&RobertD.Keliher,Sr. Dustin G. Hall Whitney C remedies · Fassett, Anthony & Taylor, P.A. secured transactions · Avila Rodriguez Hernandez Mena & Ferri. Lawrence & elizabeth e. Heinkel Brett T. & Rhonda K. Hendee* eugenio Hernandez Hicks, Porter, ebenfeld

Baskaran, Mark

477

The Quality of Web Data Keynote @ ICIQ 2012  

E-Print Network (OSTI)

Meaghan C. Gragg e. John & yali C. Gregory LindaS.Griffin&RobertD.Keliher,Sr. Dustin G. Hall Whitney C remedies · Fassett, Anthony & Taylor, P.A. secured transactions · Avila Rodriguez Hernandez Mena & Ferri. Lawrence & elizabeth e. Heinkel Brett T. & Rhonda K. Hendee* eugenio Hernandez Hicks, Porter, ebenfeld

Weske, Mathias

478

rado School gifts enrich  

E-Print Network (OSTI)

to the att n be compl ulti-day, sin weekend. T n of the atte es of fundra nd R C C P R L er 2010 y 2011 Page aising even Responsib CSM Office of F CSM Foundatio Policy Con Roger A. Cuswo Linda Landrum support from

479

U.S. DOE Office of Energy Efficiency and Renewable Energy Categorical Exclusion Determination Form  

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

U.S. Department of Energy Categorical Exclusion Determination Form Program or Field Office: Office of Energy Efficiency and Renewable Energy: Phase III Xlerator Program Funding Opportunity Number DE-FOA-0000397 Applicant Name: Applied Nanotech Location: Austin, TX Project Title High Capacity Manufacturing of Non-Contact, Printable Metallic Inks for Silicon Solar Cells Proposed Action or Project Description American Recovery and Reinvestment Act: Electrical contacts are a critical part of photovoltaic technology and in particular represent a difficult and costly area for silicon solar cell production. In particular, it would be desirable to non-contact printing processes which would be much more cost effective, environmentally benign and materials efficient

480

User Facilities | ORNL  

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

USER PORTAL USER PORTAL BTRICBuilding Technologies Research Integration Center CNMSCenter for Nanophase Materials Sciences CSMBCenter for Structural Molecular Biology CFTFCarbon Fiber Technology Facility HFIRHigh Flux Isotope Reactor MDF Manufacturing Demonstration Facility NTRCNational Transportation Research Center OLCFOak Ridge Leadership Computing Facility SNSSpallation Neutron Source Keeping it fresh at the Spallation Neutron Source Nanophase material sciences' nanotech toolbox Home | User Facilities SHARE ORNL User Facilities ORNL is home to a number of highly sophisticated experimental user facilities that provide unmatched capabilities to the broader scientific community, including a growing user community from universities, industry, and other laboratories research institutions, as well as to ORNL

Note: This page contains sample records for the topic "nanotech linda young" 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

Imbibition dynamics of nano-particulate ink-jet drops on micro-porous media  

E-Print Network (OSTI)

Imbibition dynamics of nano-particulate ink-jet drops on micro-porous media Hsiao, W.-K., Hoath, S. D., Martin, G. D., Hutchings, I. M., Chilton, N. B. and Jones, S., Proc Nanotech 2011 Conference, Boston, June 2011. Imbibition dynamics... of nano-particulate ink-jet drops on micro-porous media W.-K. Hsiao*, S. D. Hoath*, G. D. Martin*, I. M. Hutchings*, N. B. Chilton** and S. Jones** *Department of Engineering, University of Cambridge Cambridge CB3 0FS, United Kingdom, wkh26@cam...

Hsiao, W.-K.; Hoath, S.D.; Martin, G.D.; Hutchings, I.M.; Chilton, N.B.; Jones, S.

482

A qualitative analysis of writing as a focus for developing policy statements on public issues in large petrochemical companies  

E-Print Network (OSTI)

Research by Linda Flower, Ann Berthoff, James Stephens, Judith Langer, Arthur Applebee, and other social scientists supports the notion that writing helps individuals shape their ideas. I believe it serves the same function in developing policy in large corporations. For the people responsible for producing speeches and brochures that relate to issues of public concern, writing is more than an exercise in stating the corporate line in acceptable prose. For them, the written word is the focal point for examining a company's position. The act of writing puts ideas on the table for everyone to see. From there, the give-and-take between management and writers often becomes the choice of one word over another, because the final version of that text will be seen by the public as the company's official position. Those speeches and articles may be used for years by reporters, lawmakers, environmentalists, and citizens seeking to comment on the company's actions. This does not mean that writers and editors direct big companies. They are, however, an important part of a process that is often misunderstood, even by those who participate in it. There is a cost for that misunderstanding. Young writers often say in frustration, "My client doesn't know what he wants!" That, however, is just the point. Clients may not know what they want to say, and it is the writer's job to help them find out. Understanding the process will assist writers and clients alike to realize that the process of writing a position helps to form it. In large corporations, company policy is often shaped in the process. This paper is a qualitative analysis of the role of speeches and publications in developing corporate policy. It suggests that writing about issues of public concern can become the focal point for shaping corporate policy. The study is based on interviews with free-lance writers, and with writers, editors, managers, and executives of several major corporations, primarily in energy-related fields. Conclusions are based on what these individuals have said about their experience.

Cunningham, Richard Lee

2002-01-01T23:59:59.000Z

483

The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets  

E-Print Network (OSTI)

We have used Pan-STARRS1 to discover an extremely red late-L dwarf, which has (J-K)_MKO = 2.84 and (J-K)_2MASS = 2.78, making it the reddest known field dwarf and second only to 2MASS J1207-39b among substellar companions. Near-IR spectroscopy shows a spectral type of L7 and reveals a triangular H-band continuum and weak alkali (K I and Na I) lines, hallmarks of low surface gravity. Near-IR astrometry from the Hawaii Infrared Parallax Program gives a distance of 24.6+/-1.4 pc and indicates a much fainter J-band absolute magnitude than field L dwarfs. The position and kinematics of PSO J318-22 point to membership in the beta Pictoris moving group. Evolutionary models give a temperature of 1160 (-40,+30) K and a mass of 6.5 (-1.0, +1.3) Mjup, making PSO J318-22 one of the lowest mass free-floating objects in the solar neighborhood. This object adds to the growing list of low-gravity field L dwarfs and is the first to be strongly deficient in methane relative to its estimated temperature. Comparing their spectra...

Liu, Michael C; Deacon, Niall R; Allers, Katelyn N; Dupuy, Trent J; Kotson, Michael C; Aller, Kimberly M; Burgett, W S; Chambers, K C; Draper, P W; Hodapp, K W; Jedicke, R; Kudritzki, R -P; Metcalfe, N; Morgan, J S; Kaiser, N; Price, P A; Tonry, J L; Wainscoat, R J

2013-01-01T23:59:59.000Z

484

Biomass and nutrient accumulation in young Prosopis Juliflora at Mombasa, Kenya  

SciTech Connect

Data are presented for 6-yr old P. juliflora, grown for quarry reclamation on: biomass of stems, large branches, small branches and leaves; height and volume of stems and large branches. All were calculated from regressions on based diameter. Volume was 209 cubic m/ha (stems), 75 cubic m/ha (large branches). Total biomass was 216 t/ha (77% in stems and large branches). Leaves plus small branches (22.6% of biomass) contained over 50% of the pool of nutrients N, P, K and Mg. Implications are discussed for site depletion as a result of total tree use for fuelwood and fodder. 25 references.

Maghembe, J.A.; Kariuki, E.M.; Haller, R.D.

1983-01-01T23:59:59.000Z

485

Coming of Age in Rural America: The Educational and Occupational Outcomes of Rural Young Adults.  

E-Print Network (OSTI)

??Many of the issues related to poverty in rural communities are unique to those communities, and do not mirror the issues associated with poverty in… (more)

Kindell, Heather

2009-01-01T23:59:59.000Z

486

Design and Deployment of the Bonne Bay Observatory (B2O) B. de Young  

E-Print Network (OSTI)

and one underwater connecting the sensors, joined by an armored 1.4 km electro-optic cable. The cable

deYoung, Brad

487

The Young and the Restless: Scientific Institutions in late 17th  

E-Print Network (OSTI)

, Tipi Sassi nelle spaderie, 1852, 8; S.A. Bedini, "Introduction: The Vatican's astronomical paintings Longardi & Galdi, op.cit. (12), 91. 39 S.A. Bedini, "Introduction: The Vatican's astronomical paintings storici e i musei dell'università di Bologna, Milano, Silvana, 1987, 60. 43 Bedini, op.cit. (39), xvii

Qian, Ning

488

Factors influencing the adoption of personalisation mobile services: empirical evidence from young Australians  

Science Conference Proceedings (OSTI)

The adoption of mobile services is often studied at a generic level and limited research has addressed personalisation mobile services. The purpose of this paper is to develop a model that attempts to predict the adoption of personalisation mobile services ... Keywords: Australia, m-services, mobile communications, mobile services, perceived ease of use, perceived usefulness, performance expectancy, personalisation, technology adoption models

Sally Rao Hill; Indrit Troshani

2010-02-01T23:59:59.000Z

489

EXPERIMENTS IN MARKING YOUNG CHINOOK SALMON ON THE COLUMBIA RIVER, 1916 TO 1927  

E-Print Network (OSTI)

of the Atlantic were included, but no special search was made for them. Certain criteria were observed self-explanatory. The no.nle and initials of each author'are given as published. Because

490

"GeZhi" Forum for Young Scientists School of Physics, Peking University  

E-Print Network (OSTI)

in metallic nanostructures, surface plasmon polaritons can be excited accompanying a strong near field. In this talk, we will first review the Green's matrix method for solving the surface plasmon resonances resonances is studied [3], and a new way to control plasmonic resonances in binary metallic nanostructures

Meng, Zhiyong

491

G272.2--3.2: A centrally filled and possibly young SNR discovered by ROSAT  

E-Print Network (OSTI)

We report the discovery of a new SNR in the \\ros All-Sky-Survey data. The SNR has a nearly circular shape with a diameter of about 15 arcmin. The surface brightness is rather uniform over the remnant. The observed interstellar absorption suggests a distance of about 1.8$^{+1.4}_{-0.8}$ kpc. The X-ray emission appears to be of thermal origin with a plasma temperature of about 10$^7$ K. The Sedov model leads to an age of only 1800 years. We find no spectral evidence of non-thermal emission in the center of the remnant. The two most likely explanations for the centrally filled structure are evaporation of shock heated clouds in the interior of the remnant or a reverse shock heating the ejecta of the SNR explosion.

J. Greiner; R. Egger; B. Aschenbach

1994-05-03T23:59:59.000Z

492

Lorin Stein and his young staff reinvigorate the Paris Review for the digital age. p.  

E-Print Network (OSTI)

. The excellence you expect. Courses offered in > Baltimore, MD > Rockville, MD > Washington, DC > Online Advanced Exploration of the various Chesapeake Bay eco-systems by kayak Baltimore Sailing Camp for boys and girls 11) by The Johns Hopkins University, 901 S. Bond Street, Suite 540, Baltimore, MD 21231. Periodicals postage paid

Niebur, Ernst

493

The apotheosis of a human ideal : the Young Hegel's conception of the absolute  

E-Print Network (OSTI)

State University of New York Press, Albany, 1985), pp. 276-State University of New York Press, Albany, 1986), pp. 61-State University of New York Press, Albany, 1977). IAW “Die

Egan, Matthew Paul

2008-01-01T23:59:59.000Z

494

Planetary influence on the young Sun's evolution: the solar neutrino probe  

E-Print Network (OSTI)

Recent observations of solar twin stars with planetary systems like the Sun, have uncovered that these present a peculiar surface chemical composition. This is believed to be related to the formation of earth-like planets. This suggests that twin stars have a radiative interior that is richer in heavy elements than their envelopes. Moreover, the current standard solar model does not fully agree with the helioseismology data and solar neutrino flux measurements. In this work, we find that this agreement can improve if the Sun has mass loss during the pre-main sequence, as was previously shown by other groups. Despite this better agreement, the internal composition of the Sun is still uncertain, especially for elements heavier than helium. With the goal of inferring the chemical abundance of the solar interior, we tested several chemical compositions. We found that heavy element abundances influence the sound speed and solar neutrinos equally. Nevertheless, the carbon-nitrogen-oxygen (CNO;13N, 15O and 17F) neut...

Lopes, Ilidio

2013-01-01T23:59:59.000Z

495

Factor analysis of attentional set-shifting performance in young and aged mice  

E-Print Network (OSTI)

Treatment with tolcapone, a catechol-O-methyltransferaseDM, Sharp T, Harrison PJ: Catechol-o- methyltransferase

Tanaka, Shoji; Young, Jared W; Gresack, Jodi E; Geyer, Mark A; Risbrough, Victoria B

2011-01-01T23:59:59.000Z

496

V O L U M E 3 4 , P A R T 7 BRIGHAM YOUNG UNIVERSITY  

E-Print Network (OSTI)

Helper up Spring Canyon to Standardville and to several abandoned coal mines beyond. Numerous unimproved. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Gregory J. Jorgensen 105 Geology, Depositional Environments, and Coal Resources of the Helper 71/zf and outside contributors is externally reviewed by at least two qualified persons. Cover: Cretaceous coal

Seamons, Kent E.

497

Extending ScratchR : challenges of deploying a scalable user generated content platform for young people  

E-Print Network (OSTI)

ScratchR, a user generated content management platform, was developed by the Lifelong Kindergarten group at the MIT Media Lab. ScratchR lets users share projects developed with the Scratch programming language. This thesis ...

Xu, Han, M. Eng. Massachusetts Institute of Technology

2008-01-01T23:59:59.000Z

498

0500 1-5 KEY VISUAL CUES: laptop, young man, swivel chair ...  

Science Conference Proceedings (OSTI)

... playing with a long orange tube, little girls is ... Lake City, mountains, round tables, flag, map 0760 ... including mountains, a ski resort, flags, maps, and ...

2012-01-11T23:59:59.000Z

499

Chapter 41921 -1945 Aerial view of Brigham Young University Upper Campus -1928  

E-Print Network (OSTI)

of IEEE International Conference on Computer Design 1989, pp. 438-442. [4] K.O.Jeppson and C. M Svesson

Seamons, Kent E.

500

Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.139) Track: Technical  

E-Print Network (OSTI)

concepts will predominate the future wind turbine market: (i) doubly-fed induction generator (DFIG) wind power converter of the DFIG can be subjected to high transient short circuit currents, special measures