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Sample records for nanotech linda young

  1. Linda Vu

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

    Linda Vu Linda Vu Lvu.jpg Linda Vu Public Affairs, Computing Sciences lvu@lbl.gov Phone: (510) 495 2402 1 Cyclotron Rd 50B4230 Berkeley, CA 94720 Last edited: 2016-02-01 08:06:58

  2. Linda Sugiyama

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

    Linda Sugiyama Linda Sugiyama FES Requirements Worksheet 1.1. Project Information - Title Document Prepared By Linda Sugiyama Project Title Title Principal Investigator Linda Sugiyama Participating Organizations test data Funding Agencies DOE SC DOE NSA NSF NOAA NIH Other: 2. Project Summary & Scientific Objectives for the Next 5 Years Please give a brief description of your project - highlighting its computational aspect - and outline its scientific objectives for the next 3-5 years. Please

  3. Linda Vu | Department of Energy

    Office of Environmental Management (EM)

    Linda Vu About Us Linda Vu Linda Vu is a writer in the Berkeley Lab's Computing Sciences Communications Group. Most Recent How to See the Supernova Berkeley Lab Just Discovered September 1 It's In The Hopper: 4,000 Scientific Users Now Working With Supercomputer June 3 Supercomputers Crack Sixty-Trillionth Binary Digit of Pi-Squared April 28

  4. Cima NanoTech | Open Energy Information

    Open Energy Info (EERE)

    including nanoparticle conductive inks and transparent conductive coatings for solar cells. References: Cima NanoTech1 This article is a stub. You can help OpenEI by...

  5. Linda Cohn SWEIS Manager

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

    Linda Cohn SWEIS Manager U.S. Department of Energy (DOE) Nevada Site Office (NSO) Transportation Working Group Meeting November 16, 2012 Nevada National Security Site (NNSS) Final Site-Wide Environmental Impact Statement (SWEIS) Update Page 2 Page 2Title ID 385 - 11/16/2012 - Page 2 Log No. 2012-267 Overview of NSO Activities * Historic nuclear weapons testing conducted from 1951 to 1992 - 100 atmospheric tests - 828 underground tests - Nuclear reactor/rocket development * Current major mission

  6. Linda Silverman | Department of Energy

    Office of Environmental Management (EM)

    Linda Silverman About Us Linda Silverman - Senior Advisor, Tech-to-Market Office Linda Silverman serves as Senior Advisor to the Office of Energy Efficiency and Renewable Energy's Tech-to-Market initiative. Most Recent Running the Race for Clean Energy September 16 Roaming Mars and Space: 3D Technology Exploration from Home November 5 America's Home Energy Education Challenge: Teaching Kids to Save Energy and Money October 22

  7. Linda Stuntz | Department of Energy

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

    Linda Stuntz About Us Linda Stuntz - Founding Partner, Stuntz, Davis & Staffier, P.C. Linda Stuntz Linda Stuntz is a founding partner of the law firm of Stuntz, Davis & Staffier, P.C. in Washington, D.C. Her law practice includes energy and environmental regulation, as well as matters relating to government support of technology development and transfer. Ms. Stuntz served as Deputy Secretary of the United States Department of Energy under President George H.W. Bush. In that position, and

  8. Linda Gaines | Argonne National Laboratory

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

    Linda Gaines Transportation System Analyst E-mail lgaines@anl.gov Publications View Publications Projects Idle Reduction Publications Idle Reduction Research Idle Reduction Tools and Outreach Materials Lithium-Ion Battery Recycling Publications Lithium-Ion Battery Recycling and Life Cycle Analysis Reducing Vehicle Idling

  9. Linda Fellers | Y-12 National Security Complex

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (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 Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Linda Fellers

  10. Women @ Energy: Linda Silverman | Department of Energy

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

    Linda Silverman Women @ Energy: Linda Silverman October 8, 2015 - 3:09pm Addthis Linda Silverman is a senior adviser in the Office of Energy Efficiency and Renewable Energy at DOE headquarters in Washington, D.C. Her hometown is Miami Beach, Florida, and she attended the University of Colorado and Johns Hopkins University. She has a bachelor of science degree in finance and international business and a master of arts in international relations. Linda Silverman is a senior adviser in the Office

  11. From: Alle-Murphy, Linda

    Office of Environmental Management (EM)

    From: 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

  12. Ask a scientist: Nanotech in our lives | Argonne National Laboratory

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

    spring 2014 issue of Argonne Now, the laboratory science magazine. Ask a scientist: Nanotech in our lives June 1, 2014 Tweet EmailPrint Is there nanotechnology already in my consumer products? Carrado Gregar: I just saw a report that named 1,628 products using nanotechnology...so I'd say yes, definitely! When you say nanotech, a lot of people are thinking of tiny machines or robots. There is a long way to go before that becomes reality. But simpler nanomaterials are very much in common use.

  13. 2013 Federal Energy and Water Management Award Winners Linda...

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

    Linda L. Collins, Luke McAuliffe, Chris McCall, and Daniel Morrison 2013 Federal Energy and Water Management Award Winners Linda L. Collins, Luke McAuliffe, Chris McCall, and ...

  14. Linda Lee | Savannah River Ecology Laboratory

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

    Lee Faculty & Scientists SREL Home Linda Lee Savannah River Ecology Laboratory P O Drawer E, Aiken, SC 29802 (803) 725-5883 office (803) 725-3309 fax lee(at)srel.uga.edu I have a broad range of interests including wetland ecology, habitat management and restoration, and plant conservation. One of my current projects is evaluating the erosion control potential of native grassland vegetation against two commonly-used turf grasses. I am also working with Audubon South Carolina on a new

  15. Women @ Energy: Linda Valerio | Department of Energy

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

    ... enjoying those careers seems to really awaken the underlying interest in young students. ... It seems to be a common perception that young women will not be allowed to have high-level ...

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

    Broader source: Energy.gov [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...

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

    Broader source: Energy.gov [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...

  18. Linda Nazar > University of Waterloo > Scientific Advisory Board > The

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

    Energy Materials Center at Cornell Linda Nazar University of Waterloo

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

    Office of Science (SC) Website

    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)...

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

    Office of Science (SC) Website

    Ms. Linda Cerrone Scientific User Facilities (SUF) Division SUF Home About Staff Dr. James B. Murphy What's New User Facilities Projects Accelerator & Detector Research Science Highlights Principal Investigators' Meetings BES Home Staff Ms. Linda Cerrone Print Text Size: A A A 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,

  1. 2013 Federal Energy and Water Management Award Winners Linda L. Collins,

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

    Luke McAuliffe, Chris McCall, and Daniel Morrison | Department of Energy Linda L. Collins, Luke McAuliffe, Chris McCall, and Daniel Morrison 2013 Federal Energy and Water Management Award Winners Linda L. Collins, Luke McAuliffe, Chris McCall, and Daniel Morrison PDF icon fewm13_pbs_dc_highres.pdf PDF icon fewm13_pbs_dc.pdf More Documents & Publications Federal Utility Partnership Working Group Meeting Notes FUPWG Spring 2014 Agenda and Presentations FUPWG Spring 2013 Report and

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

    Office of Science (SC) Website

    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: Email Us U.S. Department of Energy SC-2/Germantown Building 1000 Independence

  3. Linda Sugiyama

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

    MHD turbulencein existing plasmass (toroidal harmonics up to at least n40, poloidal harmonics at least 4X higher, radial grid on the order of half the thermal ion gyroradius). ...

  4. Young, Jupiter-like planet discovered

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

    Young, Jupiter-like planet discovered Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Young, Jupiter-like planet discovered A team of researchers has discovered a Jupiter-like planet within a young system that could provide a new understanding of how planets formed around our sun. September 1, 2015 Jupiter-like planet Jupiter-like planet Contact Linda Anderman Email A team of researchers has discovered a Jupiter-like

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

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

    100 Best Communities for Young People Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos County is among 100 Best Communities for Young People The recognition is given to locations that make youth a priority through caring adults, safe places, a healthy start, effective education, and opportunities to help others. October 1, 2012 dummy image Read our archives Contacts Editor Linda

  6. Women @ Energy: Linda Gaines

    Broader source: Energy.gov [DOE]

    "Don’t succumb to Superwoman syndrome: You can’t do everything perfectly! There are only 24 hours in a day; don’t buy into the macho work week. Identify tasks that you can ignore, skimp on, really want to do right, delegate — then DO IT!"

  7. Young's modulus

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

    Young's modulus - Sandia Energy Energy Search Icon Sandia Home Locations Contact Us Employee Locator Energy & Climate Secure & Sustainable Energy Future Stationary Power Energy Conversion Efficiency Solar Energy Wind Energy Water Power Supercritical CO2 Geothermal Natural Gas Safety, Security & Resilience of the Energy Infrastructure Energy Storage Nuclear Power & Engineering Grid Modernization Battery Testing Nuclear Fuel Cycle Defense Waste Management Programs Advanced Nuclear

  8. From: Linda To: Congestion Study Comments Subject:

    Office of Environmental Management (EM)

    request Date: Wednesday, October 01, 2014 10:15:31 AM I am opposed to the establishment of National Interest Energy Transmission Corridors (NIETC's) for the following reasons. First, the easements place an undo burden on landowners on and near the transmission lines. The compensation cannot begin to cover the all of the losses, tangible and intangible that landowners would suffer. Second, I believe that condemning private property for transmission lines in one state to transport electricity to

  9. From: Linda To: Congestion Study Comments Subject:

    Office of Environmental Management (EM)

    Please consider Date: Wednesday, October 01, 2014 10:14:34 AM I am opposed to the establishment of National Interest Energy Transmission Corridors (NIETC's) for the following reasons. First, the easements place an un do burden on landowners on and near the transmission lines. The compensation cannot begin to cover the all of the losses, tangible and intangible that landowners would suffer. Second, I believe that condemning private property for transmission lines in one state to transport

  10. New nanotech invention improves effectiveness of the 'penicillin...

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

    effects of chemotherapy." "This technique could potentially allow us to increase the proportion of cisplatin in cancer cells by a hundredfold, making it that much more effective a...

  11. Fensin receives Young Leaders Award

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

    Fensin receives Young Leaders Award Fensin receives Young Leaders Award Saryu Fensin has been selected to receive the 2015 TMS Young Leaders International Scholar-Japanese Institute of Metals (JIM) Award. March 3, 2016 Saryu Fensin Saryu Fensin Communications Office (505) 667-7000 The award provides young professionals the opportunity to present research at international meetings and network with researchers at laboratories and industrial facilities abroad. Saryu Fensin of LANL's Materials

  12. NREL: Energy Analysis - Katherine Young

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

    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 exploration analysis Regulatory and permitting Resource reporting Geothermal direct use (thermal applications) Water rights and resources engineering Database planning and

  13. Young Brothers Ltd.

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

    Young Brothers Ltd. - Sandia Energy Energy Search Icon Sandia Home Locations Contact Us Employee Locator Energy & Climate Secure & Sustainable Energy Future Stationary Power Energy Conversion Efficiency Solar Energy Wind Energy Water Power Supercritical CO2 Geothermal Natural Gas Safety, Security & Resilience of the Energy Infrastructure Energy Storage Nuclear Power & Engineering Grid Modernization Battery Testing Nuclear Fuel Cycle Defense Waste Management Programs Advanced

  14. Fensin receives Young Leaders Award

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

    Fensin receives Young Leaders Award March 3, 2016 Saryu Fensin of LANL's Materials Science in Radiation and Dynamics Extremes group has been selected to receive the 2015 TMS Young Leaders International Scholar- Japanese Institute of Metals (JIM) Award. She will represent the Minerals, Metals & Materials Society (TMS) at the JIM Spring Annual Meeting at the Tokyo University of Science in Japan and present her research. The award is part of the TMS Young Leaders International Scholar Program,

  15. Young, Jupiter-like planet discovered

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

    Young, Jupiter-like planet discovered Young, Jupiter-like planet discovered A team of researchers has discovered a Jupiter-like planet within a young system that could provide a...

  16. YoungHo Shin | Argonne National Laboratory

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

    YoungHo Shin YoungHo Shin Principal Process Development Engineer Telephone (630) 252-4861 E-mail yshin@anl.gov

  17. Young Women's Conference in Science, Technology, Engineering...

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

    Programs Young Women's Conference in Science, Technology, Engineering & Mathematics **Due to an overwhelming response, THE 2016 YOUNG WOMEN'S CONFERENCE IN STEM IS NOW FULL AND...

  18. CHRISTIE PABARUE MORTENSEN AND YOUNG

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

    - -, CHRISTIE PABARUE MORTENSEN AND YOUNG .--- ,.. PROf'ESSIONAl. CORPORATION 1880 JOHN F. KENNEDY BOULEVARD 10TH FLOOR PHIlADeLPHIA, PA 19103 Tel: 215.587.1600 * FAX:...

  19. QER- Comment of Allen Young

    Broader source: Energy.gov [DOE]

    There is much that I can say about energy policy, but most important to me is the have no new infrastructure for fossil fuels, especially a proposed Kinder Morgan "northeast extension" pipeline through beautiful countryside in Massachusetts. There needs to be focus on renewables, plus conservation and efficiency. Allen Young

  20. Young, Jupiter-like planet discovered

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

    Young, Jupiter-like planet discovered Young, Jupiter-like planet discovered A team of researchers has discovered a Jupiter-like planet within a young system that could provide a new understanding of how planets formed around our sun. August 13, 2015 A team of researchers has discovered a Jupiter-like planet within a young system that could provide a new understanding of how planets formed around our sun. Jupiter-like planet Contact Los Alamos National Laboratory Nancy Ambrosiano Communications

  1. Youngs modulus of [111] germanium nanowires

    SciTech Connect (OSTI)

    Maksud, M.; Yoo, J.; Harris, C. T.; Palapati, N. K. R.; Subramanian, A.

    2015-11-02

    Our paper reports a diameter-independent Youngs modulus of 91.9 8.2 GPa for [111] Germanium nanowires (Ge NWs). When the surface oxide layer is accounted for using a core-shell NW approximation, the YM of the Ge core approaches a near theoretical value of 147.6 23.4 GPa. The ultimate strength of a NW device was measured at 10.9 GPa, which represents a very high experimental-to-theoretical strength ratio of ~75%. Furthermore, with increasing interest in this material system as a high-capacity lithium-ion battery anode, the presented data provide inputs that are essential in predicting its lithiation-induced stress fields and fracture behavior.

  2. 2013 Federal Energy and Water Management Award Winners Linda...

    Energy Savers [EERE]

    Washington, DC In January 2012, the GSA Energy Division ran the first forward auction for demand response services by a Federal agency, resulting in awarded contracts expected to...

  3. CHRISTIE PABARUE MORTENSEN AND YOUNG

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

    CHRISTIE PABARUE MORTENSEN AND YOUNG **......---------- A PROFESSIONAL CORPORATION Susan B. Thaucr 215-587-1633 sbthauer@cpmy.com 1880 JOHN F. KENNEDY BOULEVARD 10TH FLOOR PHILADELPHIA, PA 19103 TE.l: 215.587,1600. FAX: 215.587,1699. WWW.CPMY.COM January \5.2010 FOIA OFFICER U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 iY'):'W,'F"~-', ",: " . -* . '-" . ;.. Re: Freedom of Information Act (FOIA) Request Our File Number: 100-2127 Dear Sir or

  4. Microsoft Word - young_abstract

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

    May 13th, at 1:30 pm "Measurements of Beta-Decay in the Neutron and 19Ne: Some Recent Progress" Professor A. R. Young Dept. of Physics, North Carlina State Univ., Raleigh, NC We present recent measurements of the beta-decay of the neutron and 19Ne. Both systems have spin 1/2, and are characterized by isobaric analog decays involving, in leading order, two form factors. Precise characterization of these decays requires two independent measurements, one of which is typically the lifetime

  5. Adam Young | Argonne Leadership Computing Facility

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

    Young Guest Researcher Argonne National Laboratory 9700 S. Cass Avenue Building 240 Wkstn. 4D15 Argonne, IL 60439 younga@anl...

  6. Young Womens Conference attracts more attendees in 2014! | Princeton...

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

    Young Womens Conference attracts more attendees in 2014 June 9, 2014 Gallery: The 2014 Young Women's Conference is Science, Engineering, Technology, and Mathematics attracted...

  7. One Young World Summit |GE Global Research

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

    a young leader from Arjowiggins; I got to know some of the most crucial issues facing Kurdistan by talking with their delegation; I debated about innovation and sustainability with...

  8. Young Inventor Award | GE Global Research

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

    Young Inventor Shares His Award-Winning Invention Click to email this to a friend (Opens in new window) Share on Facebook (Opens in new window) Click to share (Opens in new window)...

  9. Young Energy, LLC | Open Energy Information

    Open Energy Info (EERE)

    Energy, LLC Jump to: navigation, search Name: Young Energy, LLC Place: Texas Phone Number: 888-963-9363 Website: www.puc.texas.govindustryele Outage Hotline: 888-963-9363...

  10. Microsoft PowerPoint - NatureNanotech_748_2013.pptx

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

    Epitaxial growth of SrTiO 3 on Si by molecular beam epitaxy has opened up the route to the integration of functional complex oxides on a Si platform. Chief among them is ferroelectric functionality using perovskite oxides such as BaTiO 3 . However, it has remained a challenge to achieve ferroelectricity in epitaxial BaTiO 3 films with a polarization pointing perpendicular to the Si substrate without a conducting bottom electrode. Here, we demonstrate ferroelectricity in such stacks. Synchrotron

  11. NREL: Photovoltaics Research - David L. Young, Ph.D.

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

    p. 073502. Young, D.L., B. Egaas, S. Pinegar, and P. Stradins. A new real-time quantum efficiency measurement system. in 33rd IEEE PVSC 2008. San Diego, CA: IEEE. Young, D.L.,...

  12. Peter (Jun Young) Ko > Project Scientist - CHESS > Researchers...

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

    (Jun Young) Ko Project Scientist - CHESS jpk96@cornell.edu While he has never taken any formal courses in "synchrotron beamline science", Jun Young Peter Ko has worked on projects...

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

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

    William E. and Diane M. Spicer Young Investigator Award William E. and Diane M. Spicer Young Investigator Award William E. Spicer (1929-2004) was an esteemed member of the...

  14. Registration for the 2015 Conference for Young Women in STEM...

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

    Registration for the 2015 Conference for Young Women in STEM is OPEN October 15, 2014 The 2015 Young Women's Conference in STEM will be held on Thursday, March 19, 2015 at...

  15. Jefferson Lab Activities Group Invites Young and Not-So-Young...

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

    Holiday Events Holiday Party on Dec. 12 for Jefferson Lab Children and the Young at Heart The JAG Holiday Party is scheduled for Saturday, Dec. 12, 10 a.m.-1 p.m. in the CEBAF...

  16. Sponsoring, Mentoring and Guiding Cultural Diverse Young Scientists...

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

    Sponsoring, Mentoring and Guiding Cultural Diverse Young Scientists and Engineers Presentation on successful mentoring. PDF icon Partnership meeting presentation 020711...

  17. Young Women's Conference cheers on girls interested in STEM | Princeton

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

    Plasma Physics Lab Young Women's Conference cheers on girls interested in STEM By Jeanne Jackson DeVoe March 27, 2014 Tweet Widget Google Plus One Share on Facebook PPPL engineer Han Zhang shows off a plasma ball to a few of the 400 young women who attended PPPL's Young Women's Conference on March 21 at Princeton University. (Photo by Elle Starkman/ PPPL Office of Communications) PPPL engineer Han Zhang shows off a plasma ball to a few of the 400 young women who attended PPPL's Young Women's

  18. Young Women's Conference cheers on girls interested in STEM | Princeton

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

    Plasma Physics Lab Young Women's Conference cheers on girls interested in STEM By Jeanne Jackson DeVoe March 28, 2014 Tweet Widget Google Plus One Share on Facebook PPPL engineer Han Zhang shows off a plasma ball to a few of the 400 young women who attended PPPL's Young Women's Conference on March 21. (Photo by Elle Starkman/ PPPL Office of Communications) PPPL engineer Han Zhang shows off a plasma ball to a few of the 400 young women who attended PPPL's Young Women's Conference on March 21.

  19. NEW YOUNG STAR CANDIDATES IN CG4 AND Sa101

    SciTech Connect (OSTI)

    Rebull, L. M.; Laine, S.; Laher, R.; Legassie, M.; Hoette, V.; Kim, J. S.; Foster, M.; Mallory, C. R.; McCarron, K.; Sherry, W. H.

    2011-07-15

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

  20. SEARCHING FOR YOUNG M DWARFS WITH GALEX

    SciTech Connect (OSTI)

    Shkolnik, Evgenya L.; Weinberger, Alycia J.; Liu, Michael C.; Dupuy, Trent; Reid, I. Neill E-mail: alycia@dtm.ciw.edu E-mail: tdupuy@ifa.hawaii.edu

    2011-01-20

    The census of young moving groups in the solar neighborhood is significantly incomplete in the low-mass regime. We have developed a new selection process to find these missing members based on the Galaxy Evolution Explorer (GALEX) All-Sky Imaging Survey (AIS). For stars with spectral types {approx}>K5 (R - J {approx}> 1.5) and younger than {approx}300 Myr, we show that near-UV (NUV) and far-UV (FUV) emission is greatly enhanced above the quiescent photosphere, analogous to the enhanced X-ray emission of young low-mass stars seen by ROSAT but detectable to much larger distances with GALEX. By combining GALEX data with optical (HST Guide Star Catalog) and near-IR (2MASS) photometry, we identified an initial sample of 34 young M dwarf candidates in a 1000 deg{sup 2} region around the {approx}10 Myr TW Hydra Association (TWA). Low-resolution spectroscopy of 30 of these found 16 which had H{alpha} in emission, which were then followed up at high resolution to search for spectroscopic evidence of youth and to measure their radial velocities. Four objects have low surface gravities, photometric distances and space motions consistent with TWA, but the non-detection of Li indicates that they may be too old to belong to this moving group. One object (M3.5, 93 {+-} 19 pc) appears to be the first known accreting low-mass member of the {approx}15 Myr Lower Centaurus Crux OB association. Two objects exhibit all the characteristics of the known TWA members, and thus we designate them as TWA 31 (M4.2, 110 {+-} 11 pc) and TWA 32 (M6.3, 53 {+-} 5 pc). TWA 31 shows extremely broad (447 km s{sup -1}) H{alpha} emission, making it the sixth member of TWA found to have ongoing accretion. TWA 32 is resolved into a 0.''6 binary in Keck laser guide star adaptive optics imaging. Our search should be sensitive down to spectral types of at least M4-M5 in TWA and thus the small numbers of new member is puzzling. This might indicate TWA has an atypical mass function or that the presence of lithium absorption may be too restrictive a criteria for selecting young low-mass stars.

  1. NETL Researcher Selected to Receive Nation's Highest Award for Young

    Energy Savers [EERE]

    Scientists | Department of Energy Researcher Selected to Receive Nation's Highest Award for Young Scientists NETL Researcher Selected to Receive Nation's Highest Award for Young Scientists February 26, 2016 - 10:13am Addthis NETL Researcher Selected to Receive Nation’s Highest Award for Young Scientists Dr. Paul R. Ohodnicki, a materials scientist at the National Energy Technology Laboratory (NETL), has been named by President Obama as a recipient of the Presidential Early Career Award

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

    Office of Environmental Management (EM)

    Oregon | Department of Energy 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

  3. Catching the entrepreneurial spirit at a young age

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

    Mockingbird Books. "Our mission is to create a comfortable, welcoming and inclusive environment for people who want and love to read," the young team wrote. "We will have...

  4. Young Physicist from Syracuse University Receives Jefferson Lab...

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

    Physicist from Syracuse University Receives Jefferson Lab's 2014 Thesis Prize Beminiwattha Rakitha Beminiwattha NEWPORT NEWS, VA, June 6, 2014 - A young researcher, who worked on...

  5. Three Young Scientists Earn DOE Graduate Research Grants at Jefferson...

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

    accomplishments have earned three young scientists funds to conduct part of their thesis research at the U.S. Department of Energy's Thomas Jefferson National Accelerator...

  6. Sponsoring, Mentoring and Guiding Cultural Diverse Young Scientists and

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

    Engineers | Argonne National Laboratory Sponsoring, Mentoring and Guiding Cultural Diverse Young Scientists and Engineers Presentation on successful mentoring. PDF icon Partnership meeting presentation 020711

  7. Young County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Young County, Texas: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 33.2200087, -98.7481167 Show Map Loading map... "minzoom":false,"mappingse...

  8. 2013 Young Women's Conference | Princeton Plasma Physics Lab

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

    400 students and chaperones attended the 2013 Young Women's Conference in Science, Mathematics, Technology, and Engineering - the largest YWC ever View larger image View larger...

  9. Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners...

    Office of Scientific and Technical Information (OSTI)

    Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners. Citation Details In-Document Search Title: Tunable Young's Modulus in Carbon MEMS using Graphene-based...

  10. Anglers needed - Save young salmon and reel in cash

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

    young salmon need your help. Today marks the start of a new Northern Pikeminnow Sport Reward Fishery Program that pays anglers for catching one of the biggest predators of...

  11. Sandia Energy - Sandian Selected for Outstanding Young Engineer...

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

    Award The Albuquerque Section of the Institute of Electrical and Electronics Engineers (IEEE) has selected Dr. Jose Luis Cruz-Campa as the recipient of the 2014 Outstanding Young...

  12. ARM - Field Campaign - MPL Measurements, Norwegian Young sea...

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

    would love to hear from you Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : MPL Measurements, Norwegian Young sea ICE cruise 2014.10.01 - 2015.07.09 Lead...

  13. Young PhDs in Physics | Jefferson Lab

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

    Ph.D.s in physics Young PhDs (left to right) William Luo, Jasmine Ellis, Shaun Lightfoot and Prakriti Verma made Oobleck with mechanical designer Joyce Miller during their visit to JLab. Young PhDs in Physics August 29, 2003 Jefferson Lab welcomes youngsters participating in summer science camp. Educating and exciting today's youth about science and technology is an important adjunct to Jefferson Lab's scientific mission. On July 16, the Department of Energy laboratory, located in Newport News,

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

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

    Physics Lab Young Womens Conference attracts more attendees in 2014! June 9, 2014 Gallery: The 2014 Young Women's Conference is Science, Engineering, Technology, and Mathematics attracted students from all over New Jersey! With almost 400 students, 50, chaperones and almost 100 volunteers from PPPL and Princeton University, it was our largest event to date! Over 65 exhibitors showcased the various sciences in their field and our breakout speakers, Crystal Bailey, of the American Physical

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

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

    Synchrotron Radiation Lightsource William E. and Diane M. Spicer Young Investigator Award William E. and Diane M. Spicer Young Investigator Award William E. Spicer (1929-2004) was an 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 years as a professor at Stanford where he pioneered the technique ofultraviolet photoemission spectroscopy and its subsequent expansion

  16. Progress in Understanding Iron Peak Elements in Young Supernova Remnants

    Office of Scientific and Technical Information (OSTI)

    (Conference) | SciTech Connect Progress in Understanding Iron Peak Elements in Young Supernova Remnants Citation Details In-Document Search Title: Progress in Understanding Iron Peak Elements in Young Supernova Remnants Authors: Eriksen, Kristoffer A. [1] ; Hughes, Jack [2] ; Fontes, Christopher J. [1] ; Colgan, James P. [1] ; Hungerford, Aimee L. [1] ; Fryer, Christopher L. [1] ; Zhang, Honglin [1] ; Badenes, Carles [3] ; Slane, Patrick [4] + Show Author Affiliations Los Alamos National

  17. Hanford Grows Young Minds Through Site Tours | Department of Energy

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

    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

  18. Environmental Contractor Mentors Young Students | Department of Energy

    Energy Savers [EERE]

    Contractor Mentors Young Students Environmental Contractor Mentors Young Students November 26, 2014 - 12:00pm Addthis Jeff Boulton of LATA Kentucky works with middle school students to demonstrate and test the acidity and basicity levels of groundwater. Jeff Boulton of LATA Kentucky works with middle school students to demonstrate and test the acidity and basicity levels of groundwater. Middle school students use water bottles and powdered drink mix to learn how contamination interacts with

  19. Catching the entrepreneurial spirit at a young age

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

    Catching the entrepreneurial spirit at a young age Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Catching the entrepreneurial spirit at a young age Teen Challenge allows students to test and develop business ideas July 1, 2014 Teen Challenge winners, (l to r) Dakota Waterson, Lucie Goodhart, Ezra Tredwin and Lily Sanborn. Teen Challenge winners, (l to r) Dakota Waterson, Lucie Goodhart, Ezra

  20. Calling all Young Entrepreneurs: Deadline for Energy Department Business

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

    Plan Competition Approaching | Department of Energy 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

  1. CANDIDATES FOR THE YOUNG STELLAR OUTFLOWS: WATER AND METHANOL MASERS FROM YOUNG STELLAR OBJECTS

    SciTech Connect (OSTI)

    Lim, Wanggi; Lyo, A-Ran; Kim, Kee-Tae; Byun, Do-Young

    2012-11-01

    We conducted simultaneous 22 GHz water maser and 44 GHz class I methanol maser surveys of newly identified 282 H{sub 2} emission features from the 2.122 {mu}m H{sub 2} narrowband image survey in the Galactic plane (UWISH2 project) using Korean VLBI Network 21 m radio telescopes. We detected 16 and 13 new water and methanol maser sources, respectively. This result indicates that at least {approx}5% of the H{sub 2} emission features originate from young stellar objects (YSOs) that are in the right physical condition to produce the water and methanol masers. The masers are closely related to the current outflow activities in the Galactic plane. The power sources of these 23 diffused/collimated H{sub 2} emission features (six sources are detected for both masers) are likely to be intermediate- to high-mass YSOs, based on a comparison with the maser luminosities of other well-studied YSOs. Both maser velocities are mostly close to their own systemic velocities within {approx}<5 km s{sup -1}, even though water masers generally show larger variabilities in the intensity, velocity, and shape than methanol masers. We also discovered three new water maser sources with high-velocity components: {approx}25 km s{sup -1} redshifted CMHO 019, {approx}50 km s{sup -1} blueshifted CMHO 132, and {approx}120 km s{sup -1} blueshifted CMHO 182. In particular, we propose that the dominant blueshifted water maser of CHMO 182 can be a unique laboratory for the study of the high-mass young stellar jet and its acceleration.

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

    Office of Scientific and Technical Information (OSTI)

    who at age 15 created a novel paper sensor that detects pancreatic, ovarian, and lung cancer in 5 minutes for as little as 3 cents; Jack has a huge Twitter following and is a ...

  3. Young scientist discovers magnetic material unnecessary to create spin

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

    current | Argonne National Laboratory Young scientist discovers magnetic material unnecessary to create spin current By Carla Reiter * July 23, 2015 Tweet EmailPrint It doesn't happen often that a young scientist makes a significant and unexpected discovery, but postdoctoral researcher Stephen Wu of the U.S. Department of Energy's Argonne National Laboratory just did exactly that. What he found-that you don't need a magnetic material to create spin current from insulators-has important

  4. The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane...

    Office of Scientific and Technical Information (OSTI)

    Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane-poor atmosphere Citation Details In-Document Search Title: The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and...

  5. EVIDENCE FOR A WEAK WIND FROM THE YOUNG SUN

    SciTech Connect (OSTI)

    Wood, Brian E.; Mller, Hans-Reinhard; Redfield, Seth; Edelman, Eric

    2014-02-01

    The early history of the solar wind has remained largely a mystery due to the difficulty of detecting winds around young stars that can serve as analogs for the young Sun. Here we report on the detection of a wind from the 500Myr old solar analog ?{sup 1} UMa (G1.5V), using spectroscopic observations from the Hubble Space Telescope. We detect H I Ly? absorption from the interaction region between the stellar wind and interstellar medium, i.e., the stellar astrosphere. With the assistance of hydrodynamic models of the ?{sup 1} UMa astrosphere, we infer a wind only half as strong as the solar wind for this star. This suggests that the Sun and solar-like stars do not have particularly strong coronal winds in their youth.

  6. Young Physicist from Syracuse University Receives Jefferson Lab's 2014

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

    Thesis Prize | Jefferson Lab Physicist from Syracuse University Receives Jefferson Lab's 2014 Thesis Prize Beminiwattha Rakitha Beminiwattha NEWPORT NEWS, VA, June 6, 2014 - A young researcher, who worked on software development and data analysis for a major physics experiment conducted at the Thomas Jefferson National Accelerator Facility, has received an award for the thesis he wrote about his efforts. Rakitha Beminiwattha, now a post-doctoral research associate with the Department of

  7. 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; ~~~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

  8. STEM Mentoring Café- Engaging Young Women in an Authentic Mentoring

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

    Experience | Department of Energy Mentoring Café- Engaging Young Women in an Authentic Mentoring Experience STEM Mentoring Café- Engaging Young Women in an Authentic Mentoring Experience May 30, 2014 - 1:34pm Addthis STEM Mentoring Café- Engaging Young Women in an Authentic Mentoring Experience Melinda Higgins Albert Einstein Distinguished Educator Fellow, NASA Office of Education, Headquarters and Goddard Space Flight Center It is a well-known fact: The percentage of women in science,

  9. Registration for the 2015 Conference for Young Women in STEM is OPEN! |

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

    Princeton Plasma Physics Lab Registration for the 2015 Conference for Young Women in STEM is OPEN! October 15, 2014 The 2015 Young Women's Conference in STEM will be held on Thursday, March 19, 2015 at Princeton University's Frick Chemistry building and registration is now OPEN! Please visit our Young Women's Conference program page to find out more about this great event and to register your group here! Remember, young women must be in grades 7-10 there is a 10 student and 1 chaperone limit

  10. NEW YOUNG STAR CANDIDATES IN BRC 27 AND BRC 34

    SciTech Connect (OSTI)

    Rebull, L. M.; Laher, R.; Legassie, M.; Gibbs, J. C.; Aryal, S.; Canakapalli, T. S.; Linahan, M.; Ezyk, N.; Fagan, J.; Sartore, D.; Badura, K. S.; Armstrong, J. D.; Allen, L. E.; McGehee, P.; and others

    2013-01-01

    We used archival Spitzer Space Telescope mid-infrared data to search for young stellar objects (YSOs) in the immediate vicinity of two bright-rimmed clouds, BRC 27 (part of CMa R1) and BRC 34 (part of the IC 1396 complex). These regions both appear to be actively forming young stars, perhaps triggered by the proximate OB stars. In BRC 27, we find clear infrared excesses around 22 of the 26 YSOs or YSO candidates identified in the literature, and identify 16 new YSO candidates that appear to have IR excesses. In BRC 34, the one literature-identified YSO has an IR excess, and we suggest 13 new YSO candidates in this region, including a new Class I object. Considering the entire ensemble, both BRCs are likely of comparable ages, within the uncertainties of small number statistics and without spectroscopy to confirm or refute the YSO candidates. Similarly, no clear conclusions can yet be drawn about any possible age gradients that may be present across the BRCs.

  11. DIRECT DETECTIONS OF YOUNG STARS IN NEARBY ELLIPTICAL GALAXIES

    SciTech Connect (OSTI)

    Ford, H. Alyson; Bregman, Joel N.

    2013-06-20

    Small amounts of star formation in elliptical galaxies are suggested by several results: surprisingly young ages from optical line indices, cooling X-ray gas, and mid-infrared dust emission. Such star formation has previously been difficult to directly detect, but using ultraviolet Hubble Space Telescope Wide Field Camera 3 imaging, we have identified individual young stars and star clusters in four nearby ellipticals. Ongoing star formation is detected in all galaxies, including three ellipticals that have previously exhibited potential signposts of star-forming conditions (NGC 4636, NGC 4697, and NGC 4374), as well as the typical ''red and dead'' NGC 3379. The current star formation in our closest targets, where we are most complete, is between 2.0 and 9.8 Multiplication-Sign 10{sup -5} M{sub Sun} yr{sup -1}. The star formation history was roughly constant from 0.5 to 1.5 Gyr (at (3-5) Multiplication-Sign 10{sup -4} M{sub Sun} yr{sup -1}), but decreased by a factor of several in the past 0.3 Gyr. Most star clusters have a mass between 10{sup 2} and 10{sup 4} M{sub Sun }. The specific star formation rates of {approx}10{sup -16} yr{sup -1} (at the present day) or {approx}10{sup -14} yr{sup -1} (when averaging over the past Gyr) imply that a fraction 10{sup -8} of the stellar mass is younger than 100 Myr and 10{sup -5} is younger than 1 Gyr, quantifying the level of frosting of recent star formation over the otherwise passive stellar population. There is no obvious correlation between either the presence or spatial distribution of postulated star formation indicators and the star formation we detect.

  12. Possible contribution of low shear modulus C?? to the low Youngs modulus of Ti-36Nb-5Zr alloy

    SciTech Connect (OSTI)

    Meng, Qingkun; Guo, Shun; Ren, Xiaobing; Xu, Huibin; Zhao, Xinqing

    2014-09-29

    Despite the importance of single-crystal elastic constants of ?-phase titanium alloys in understanding their low Young's modulusa property crucial for many applications, such data are often difficult to obtain when the alloy composition is close to the instability limit of the ? phase, where the presence of ?" martensite precludes the fabrication of ?-phase single crystal. In the present study, we extracted the single-crystal elastic constants of such a ?-phase titanium alloy with low Young's modulus, Ti-36Nb-5Zr (wt. %), from polycrystalline specimens by using an in-situ synchrotron X-ray diffraction technique. It is indicated that the low Young's modulus of the alloy originates from the anomalously low shear modulus C?? as well as the low shear modulus C', which is different from a common viewpoint that the Young's modulus of ?-phase titanium alloys is dominantly controlled by the C'. This suggests that low C?? is an important contributor to low Young's modulus for instable ?-phase titanium alloys.

  13. The 2015 Conference for Young Women in STEM is a smashing succes! |

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

    Princeton Plasma Physics Lab The 2015 Conference for Young Women in STEM is a smashing succes! April 2, 2015 A beautiful Thursday morning at the usually quiet and peaceful Frick Chemistry building at Princeton University, turned into a bustling hub of science and technology for a day on March 19, 2015. Over 450 young women, in grades 7-10, and their chaperones came from all over NJ, PA and even MD, to attend PPPL's 14th Annual young Women's Conference in STEM. With over 25 exhibits, the

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

    Energy Savers [EERE]

    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

  15. The evolutionary tracks of young massive star clusters

    SciTech Connect (OSTI)

    Pfalzner, S.; Steinhausen, M.; Vincke, K.; Menten, K.; Parmentier, G.

    2014-10-20

    Stars mostly form in groups consisting of a few dozen to several ten thousand members. For 30 years, theoretical models have provided a basic concept of how such star clusters form and develop: they originate from the gas and dust of collapsing molecular clouds. The conversion from gas to stars being incomplete, the leftover gas is expelled, leading to cluster expansion and stars becoming unbound. Observationally, a direct confirmation of this process has proved elusive, which is attributed to the diversity of the properties of forming clusters. Here we take into account that the true cluster masses and sizes are masked, initially by the surface density of the background and later by the still present unbound stars. Based on the recent observational finding that in a given star-forming region the star formation efficiency depends on the local density of the gas, we use an analytical approach combined with N-body simulations to reveal evolutionary tracks for young massive clusters covering the first 10 Myr. Just like the Hertzsprung-Russell diagram is a measure for the evolution of stars, these tracks provide equivalent information for clusters. Like stars, massive clusters form and develop faster than their lower-mass counterparts, explaining why so few massive cluster progenitors are found.

  16. Young Professionals in Nuclear Industry Group Forms at Savannah River Site

    Broader source: Energy.gov [DOE]

    AIKEN, S.C. – Supporting the development of young nuclear professionals in the Central Savannah River Area (CSRA) is the purpose behind a new group forming at the Savannah River Site (SRS).

  17. Optical Third-Harmonic Generation in Graphene Hong, Sung-Young...

    Office of Scientific and Technical Information (OSTI)

    Third-Harmonic Generation in Graphene Hong, Sung-Young; Dadap, Jerry I.; Petrone, Nicholas; Yeh, Po-Chun; Hone, James; Osgood, Richard M. American Physical Society None USDOE...

  18. Rsdometty C.M.R. Platt, J. W. Bennett, S. A. Young, M. D. Fenwick...

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

    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,...

  19. Three Young Scientists Earn DOE Graduate Research Grants at Jefferson Lab |

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

    Jefferson Lab Three Young Scientists Earn DOE Graduate Research Grants at Jefferson Lab NEWPORT NEWS, Va., Feb. 10, 2015 -- Outstanding academic accomplishments have earned three young scientists funds to conduct part of their thesis research at the U.S. Department of Energy's Thomas Jefferson National Accelerator Facility. In December, the Department of Energy's Office of Workforce Development for Teachers and Scientists sent letters to 65 graduate students - from 50 universities -

  20. Over 150 Young Women to Learn About Careers, Research Opportunities in

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

    Physics at Jefferson Lab on Jan. 16 | Jefferson Lab Over 150 Young Women to Learn About Careers, Research Opportunities in Physics at Jefferson Lab on Jan. 16 NEWPORT NEWS, VA, Jan. 11, 2016 -- Several hundred young women - from across the country - will gather Jan. 15-17 to learn about many career and research opportunities available in fields associated with physics. They will be attending one of nine regional events, dubbed the Conferences for Undergraduate Women in Physics (CUWiP),

  1. LANL gets young women involved in math and science at 31st Expanding Your

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

    Horizons Conference April 6 31st Expanding Your Horizons Conference LANL gets young women involved in math and science at 31st Expanding Your Horizons Conference April 6 The young women will participate in hands-on activities in such fields as astronomy, robotics, forensics, chemistry, and earth science. March 4, 2010 Los Alamos National Laboratory sits on top of a once-remote mesa in northern New Mexico with the Jemez mountains as a backdrop to research and innovation covering

  2. Young Investigator Program > Research > The Energy Materials Center at

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

    Cornell Young Investigator Program In This Section YIA1 - Chen YIA2 - Rodríguez-Calero YIA3 - Rodriguez-López YIA4 - Hernández-Burgos YIA5 - Khurana YIA6 - Potash Young Investigator Program This program is designed to encourage Center postdocs and students to submit collaborative proposals for new research projects that advance the Center's overall programmatic goal of advancing the science of energy conversion and storage by understanding and exploiting fundamental properties of active

  3. Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners.

    Office of Scientific and Technical Information (OSTI)

    (Conference) | SciTech Connect Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners. Citation Details In-Document Search Title: Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners. Authors: Washburn, Cody M. ; Blecke, Jill ; Lambert, Timothy N. ; Hance, Bradley G. ; Finnegan, Patrick Sean ; Davis, Danae Jacquelyne ; Wheeler, David R. ; Strong, Jennifer M. Publication Date: 2012-08-01 OSTI Identifier: 1073476 Report Number(s): SAND2012-6972C DOE Contract

  4. Uranium and thorium decay series disequilibria in young volcanic rocks

    SciTech Connect (OSTI)

    Williams, R.W.

    1988-01-01

    Two of the central questions in igneous geochemistry that study of radioactive disequilibria can help to answer are: what are the rates of magma genesis; and what are the timescales of magma separation and transport. In addition to the temporal information that may be extracted from disequilibria data, the {sup 230}Th/{sup 232}Th of a young rock may be used as a tracer of the Th/U ratio of its source region. Measurements were made by isotope dilution alpha-spectrometry of {sup 238}U, {sup 234}U, {sup 230}Th, and {sup 232}Th in 20 subduction related, 3 oceanic intraplate, and 10 continental intraplate volcanics. {sup 210}Pb was measured in all, {sup 226}Ra was measured in about half, and {sup 228}Th was measured in 10 of the most recent samples. Disequilibrium between {sup 228}Th and {sup 232}Th was found only in the Nacarbonatite samples from Oldoinyo Lengai volcano in Tanzania, which is attributable to {sup 228}Ra/{sup 232}Th {approximately} 27 at the time of eruption. These rocks also have {sup 226}Ra/{sup 230}Th > 60. Three Ra-enrichment models are developed which constrain carbonatite magma formation at less than 20 years before eruption. The effects of different partial melting processes on the {sup 238}U decay series are investigated. If mid-ocean ridge basalts are formed by a dynamic melting process, the {sup 230}Th/{sup 232}Th of the basalts provides a minimum estimate of the Th/U ratio of the source region. The {sup 238}U enrichment in arc volcanics is probably the results of metasomatism of the source by fluids derived from the subducting slab, and the {sup 230}Th enrichment observed for other volcanics is probably due to the partial melting process in the absence of U-bearing fluids.

  5. THE ENIGMATIC YOUNG, LOW-MASS VARIABLE TWA 30

    SciTech Connect (OSTI)

    Looper, Dagny L.; Rayner, John; Pitts, Mark A.; Mohanty, Subhanjoy; Bochanski, John J.; Burgasser, Adam J.; Mamajek, Eric E.; Herczeg, Gregory J.; West, Andrew A.; Faherty, Jacqueline K.; Kirkpatrick, J. Davy

    2010-05-01

    TWA 30 is a remarkable young (7 {+-} 3 Myr), low-mass (0.12 {+-} 0.04 M{sub sun}), late-type star (M5 {+-} 1) residing 42 {+-} 2 pc away from the Sun in the TW Hydrae Association (TWA). It shows strong outflow spectral signatures such as [S II], [O I], [O II], [O III], and Mg I], while exhibiting weak H{alpha} emission (-6.8 {+-} 1.2 A). Emission lines of [S II] and [O I] are common to T Tauri stars still residing in their natal molecular clouds, while [O III] and Mg I] emission lines are incredibly rare in this same population; in the case of TWA 30, these latter lines may arise from new outflow material colliding into older outflow fronts. The weak H{alpha} emission and small radial velocity shifts of line emission relative to the stellar frame of rest (generally {approx_lt}10 km s{sup -1}) suggest that the disk is viewed close to edge-on and that the stellar axis may be inclined to the disk, similar to the AA Tau system, based on its temporal changes in emission/absorption line strengths/profiles and variable reddening (A{sub V} = 1.5-9.0). The strong Li absorption (0.61 {+-} 0.13 A) and common kinematics with members of the TWA confirm its age and membership to the association. Given the properties of this system such as its proximity, low mass, remarkable outflow signatures, variability, and edge-on configuration, this system is a unique case study at a critical time in disk evolution and planet-building processes.

  6. A first-look atmospheric modeling study of the young directly imaged

    Office of Scientific and Technical Information (OSTI)

    planet-mass companion, ROXS 42Bb (Journal Article) | SciTech Connect A first-look atmospheric modeling study of the young directly imaged planet-mass companion, ROXS 42Bb Citation Details In-Document Search Title: A first-look atmospheric modeling study of the young directly imaged planet-mass companion, ROXS 42Bb We present and analyze JK{sub s}L' photometry and our previously published H-band photometry and K-band spectroscopy for ROXs 42Bb, an object Currie et al. first reported as a

  7. BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS

    SciTech Connect (OSTI)

    Malo, Lison; Doyon, Rene; Lafreniere, David; Artigau, Etienne; Gagne, Jonathan; Baron, Frederique; Riedel, Adric E-mail: doyon@astro.umontreal.ca E-mail: artigau@astro.umontreal.ca E-mail: baron@astro.umontreal.ca

    2013-01-10

    We present a new method based on a Bayesian analysis to identify new members of nearby young kinematic groups. The analysis minimally takes into account the position, proper motion, magnitude, and color of a star, but other observables can be readily added (e.g., radial velocity, distance). We use this method to find new young low-mass stars in the {beta} Pictoris and AB Doradus moving groups and in the TW Hydrae, Tucana-Horologium, Columba, Carina, and Argus associations. Starting from a sample of 758 mid-K to mid-M (K5V-M5V) stars showing youth indicators such as H{alpha} and X-ray emission, our analysis yields 214 new highly probable low-mass members of the kinematic groups analyzed. One is in TW Hydrae, 37 in {beta} Pictoris, 17 in Tucana-Horologium, 20 in Columba, 6 in Carina, 50 in Argus, 32 in AB Doradus, and the remaining 51 candidates are likely young but have an ambiguous membership to more than one association. The false alarm rate for new candidates is estimated to be 5% for {beta} Pictoris and TW Hydrae, 10% for Tucana-Horologium, Columba, Carina, and Argus, and 14% for AB Doradus. Our analysis confirms the membership of 58 stars proposed in the literature. Firm membership confirmation of our new candidates will require measurement of their radial velocity (predicted by our analysis), parallax, and lithium 6708 A equivalent width. We have initiated these follow-up observations for a number of candidates, and we have identified two stars (2MASSJ01112542+1526214, 2MASSJ05241914-1601153) as very strong candidate members of the {beta} Pictoris moving group and one strong candidate member (2MASSJ05332558-5117131) of the Tucana-Horologium association; these three stars have radial velocity measurements confirming their membership and lithium detections consistent with young age.

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

    Office of Legacy Management (LM)

    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 *

  9. IDENTIFYING THE YOUNG LOW-MASS STARS WITHIN 25 pc. II. DISTANCES, KINEMATICS, AND GROUP MEMBERSHIP

    SciTech Connect (OSTI)

    Shkolnik, Evgenya L.; Anglada-Escude, Guillem; Liu, Michael C.; Bowler, Brendan P.; Weinberger, Alycia J.; Boss, Alan P.; Reid, I. Neill; Tamura, Motohide

    2012-10-10

    We have conducted a kinematic study of 165 young M dwarfs with ages of {approx}<300 Myr. Our sample is composed of stars and brown dwarfs with spectral types ranging from K7 to L0, detected by ROSAT and with photometric distances of {approx}<25 pc assuming that the stars are single and on the main sequence. In order to find stars kinematically linked to known young moving groups (YMGs), we measured radial velocities for the complete sample with Keck and CFHT optical spectroscopy and trigonometric parallaxes for 75 of the M dwarfs with the CAPSCam instrument on the du Pont 2.5 m Telescope. Due to their youthful overluminosity and unresolved binarity, the original photometric distances for our sample underestimated the distances by 70% on average, excluding two extremely young ({approx}<3 Myr) objects found to have distances beyond a few hundred parsecs. We searched for kinematic matches to 14 reported YMGs and identified 10 new members of the AB Dor YMG and 2 of the Ursa Majoris group. Additional possible candidates include six Castor, four Ursa Majoris, two AB Dor members, and one member each of the Her-Lyr and {beta} Pic groups. Our sample also contains 27 young low-mass stars and 4 brown dwarfs with ages {approx}<150 Myr that are not associated with any known YMG. We identified an additional 15 stars that are kinematic matches to one of the YMGs, but the ages from spectroscopic diagnostics and/or the positions on the sky do not match. These warn against grouping stars together based only on kinematics and that a confluence of evidence is required to claim that a group of stars originated from the same star-forming event.

  10. Nano tech Silicon India Ltd | Open Energy Information

    Open Energy Info (EERE)

    tech Silicon India Ltd Jump to: navigation, search Name: Nano-tech Silicon India Ltd Place: Hyderabad, Andhra Pradesh, India Product: Nano-tech Silicon is a manufacturer of PV...

  11. Radiation-driven warping of circumbinary disks around eccentric young star binaries

    SciTech Connect (OSTI)

    Hayasaki, Kimitake; Sohn, Bong Won; Jung, Taehyun; Zhao, Guangyao; Okazaki, Atsuo T.; Naito, Tsuguya

    2014-12-10

    We study a warping instability of a geometrically thin, non-self-gravitating, circumbinary disk around young binary stars on an eccentric orbit. Such a disk is subject to both the tidal torques due to a time-dependent binary potential and the radiative torques due to radiation emitted from each star. The tilt angle between the circumbinary disk plane and the binary orbital plane is assumed to be very small. We find that there is a radius within/beyond which the circumbinary disk is unstable to radiation-driven warping, depending on the disk density and temperature gradient indices. This marginally stable warping radius is very sensitive to viscosity parameters, a fiducial disk radius and the temperature measured there, the stellar luminosity, and the disk surface density at a radius where the disk changes from optically thick to thin for the irradiation from the central stars. On the other hand, it is insensitive to the orbital eccentricity and binary irradiation parameter, which is a function of the binary mass ratio and luminosity of each star. Since the tidal torques can suppress the warping in the inner part of the circumbinary disk, the disk starts to be warped in the outer part. While the circumbinary disks are most likely to be subject to the radiation-driven warping on an AU to kilo-AU scale for binaries with young massive stars more luminous than 10{sup 4} L {sub ?}, the radiation-driven warping does not work for those around young binaries with the luminosity comparable to the solar luminosity.

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

    Office of Legacy Management (LM)

    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:

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

    Office of Legacy Management (LM)

    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:

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

    Office of Legacy Management (LM)

    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

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

    Office of Legacy Management (LM)

    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

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

    Office of Legacy Management (LM)

    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

  17. Discovery of the young L dwarf wise J174102.78-464225.5

    SciTech Connect (OSTI)

    Schneider, Adam C.; Cushing, Michael C.; Kirkpatrick, J. Davy; Mace, Gregory N.; Gelino, Christopher R.; Fajardo-Acosta, Sergio; Faherty, Jacqueline K.; Sheppard, Scott S.

    2014-02-01

    We report the discovery of the L dwarf WISE J174102.78464225.5, which was discovered as part of a search for nearby L dwarfs using the Wide-field Infrared Survey Explorer (WISE). The distinct triangular peak of the H-band portion of its near-infrared spectrum and its red near-infrared colors (J K{sub S} = 2.35 0.08 mag) are indicative of a young age. Via comparison to spectral standards and other red L dwarfs, we estimate a near-infrared spectral type of L7 2 (pec). From a comparison to spectral and low-mass evolutionary models, we determine self-consistent effective temperature, log g, age, and mass values of 1450 100 K, 4.0 0.25 (cm s{sup 2}), 10-100 Myr, and 4-21 M {sub Jup}, respectively. With an estimated distance of 10-30 pc, we explore the possibility that WISE J174102.78464225.5 belongs to one of the young nearby moving groups via a kinematic analysis and we find potential membership in the ? Pictoris or AB Doradus associations. A trigonometric parallax measurement and a precise radial velocity can help to secure its membership in either of these groups.

  18. SPIN EVOLUTION OF ACCRETING YOUNG STARS. II. EFFECT OF ACCRETION-POWERED STELLAR WINDS

    SciTech Connect (OSTI)

    Matt, Sean P.; Greene, Thomas P.; Pudritz, Ralph E. E-mail: thomas.p.greene@nasa.gov E-mail: pudritz@physics.mcmaster.ca

    2012-01-20

    We present a model for the rotational evolution of a young, solar-mass star interacting magnetically with an accretion disk. As in a previous paper (Paper I), the model includes changes in the star's mass and radius as it descends the Hayashi track, a decreasing accretion rate, and a prescription for the angular momentum transfer between the star and disk. Paper I concluded that, for the relatively strong magnetic coupling expected in real systems, additional processes are necessary to explain the existence of slowly rotating pre-main-sequence stars. In the present paper, we extend the stellar spin model to include the effect of a spin-down torque that arises from an accretion-powered stellar wind (APSW). For a range of magnetic field strengths, accretion rates, initial spin rates, and mass outflow rates, the modeled stars exhibit rotation periods within the range of 1-10 days in the age range of 1-3 Myr. This range coincides with the bulk of the observed rotation periods, with the slow rotators corresponding to stars with the lowest accretion rates, strongest magnetic fields, and/or highest stellar wind mass outflow rates. We also make a direct, quantitative comparison between the APSW scenario and the two types of disk-locking models (namely, the X-wind and Ghosh and Lamb type models) and identify some remaining theoretical issues for understanding young star spins.

  19. Modeling tracers of young stellar population age in star-forming galaxies

    SciTech Connect (OSTI)

    Levesque, Emily M.; Leitherer, Claus

    2013-12-20

    The young stellar population of a star-forming galaxy is the primary engine driving its radiative properties. As a result, the age of a galaxy's youngest generation of stars is critical for a detailed understanding of its star formation history, stellar content, and evolutionary state. Here we present predicted equivalent widths for the H?, H?, and Br? recombination lines as a function of stellar population age. The equivalent widths are produced by the latest generations of stellar evolutionary tracks and the Starburst99 stellar population synthesis code, and are the first to fully account for the combined effects of both nebular emission and continuum absorption produced by the synthetic stellar population. Our grid of model stellar populations spans six metallicities (0.001 < Z < 0.04), two treatments of star formation history (a 10{sup 6} M {sub ?} instantaneous burst and a continuous star formation rate of 1 M {sub ?} yr{sup 1}), and two different treatments of initial rotation rate (v {sub rot} = 0.0v {sub crit} and 0.4v {sub crit}). We also investigate the effects of varying the initial mass function. Given constraints on galaxy metallicity, our predicted equivalent widths can be applied to observations of star-forming galaxies to approximate the age of their young stellar populations.

  20. Recollimation boundary layers as X-ray sources in young stellar jets

    SciTech Connect (OSTI)

    Gnther, Hans Moritz; Li, Zhi-Yun; Schneider, P. C.

    2014-11-01

    Young stars accrete mass from circumstellar disks and, in many cases, the accretion coincides with a phase of massive outflows, which can be highly collimated. Those jets emit predominantly in the optical and IR wavelength range. However, in several cases, X-ray and UV observations reveal a weak but highly energetic component in those jets. X-rays are observed both from stationary regions close to the star and from knots in the jet several hundred AU from the star. In this article, we show semianalytically that a fast stellar wind that is recollimated by the pressure from a slower, more massive disk wind can have the right properties to power stationary X-ray emission. The size of the shocked regions is compatible with observational constraints. Our calculations support a wind-wind interaction scenario for the high-energy emission near the base of young stellar object jets. For the specific case of DG Tau, a stellar wind with a mass-loss rate of 5 10{sup 10} M {sub ?} yr{sup 1} and a wind speed of 800 km s{sup 1} reproduces the observed X-ray spectrum. We conclude that a stellar wind recollimation shock is a viable scenario to power stationary X-ray emission close to the jet launching point.

  1. YOUNG PLANETARY NEBULAE: HUBBLE SPACE TELESCOPE IMAGING AND A NEW MORPHOLOGICAL CLASSIFICATION SYSTEM

    SciTech Connect (OSTI)

    Sahai, Raghvendra; Villar, Gregory G.; Morris, Mark R.

    2011-04-15

    Using Hubble Space Telescope images of 119 young planetary nebulae (PNs), most of which have not previously been published, we have devised a comprehensive morphological classification system for these objects. This system generalizes a recently devised system for pre-planetary nebulae, which are the immediate progenitors of PNs. Unlike previous classification studies, we have focused primarily on young PNs rather than all PNs, because the former best show the influences or symmetries imposed on them by the dominant physical processes operating at the first and primary stage of the shaping process. Older PNs develop instabilities, interact with the ambient interstellar medium, and are subject to the passage of photoionization fronts, all of which obscure the underlying symmetries and geometries imposed early on. Our classification system is designed to suffer minimal prejudice regarding the underlying physical causes of the different shapes and structures seen in our PN sample, however, in many cases, physical causes are readily suggested by the geometry, along with the kinematics that have been measured in some systems. Secondary characteristics in our system, such as ansae, indicate the impact of a jet upon a slower-moving, prior wind; a waist is the signature of a strong equatorial concentration of matter, whether it be outflowing or in a bound Keplerian disk, and point symmetry indicates a secular trend, presumably precession, in the orientation of the central driver of a rapid, collimated outflow.

  2. The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane-poor

    Office of Scientific and Technical Information (OSTI)

    atmosphere (Journal Article) | SciTech Connect Journal Article: The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane-poor atmosphere Citation Details In-Document Search Title: The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane-poor atmosphere Authors: Barman, T S ; Macintosh, B A ; Konopacky, Q M ; Marois, C Publication Date: 2011-05-31 OSTI Identifier: 1122192 Report Number(s): LLNL-JRNL-485291 DOE Contract Number: W-7405-ENG-48 Resource Type: Journal Article

  3. For your calendar

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

    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar Science talks for young and old December 1, 2013 Mars rover Curosity An upcoming Café Scientifique session focuses on the Laboratory's high-tech search for signs of life on Mars. Contacts Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email Ancient Stone Calendars of the Southwest

  4. Radon Laboratory: A Proposal for Scientific Culture Dissemination Among Young Students in Italy

    SciTech Connect (OSTI)

    Groppi, Flavia; Manenti, Simone; Gini, Luigi; Bonardi, Mauro L.; Bazzocchi, Anna

    2009-08-19

    In Italy the 'nuclear issue' was for a long time a taboo. A way to approach this theme to make the public more trusting of nuclear issues is to discuss radioactivity and ionizing radiation starting from young students. An experimental activity that involves secondary school students has been developed. The approach is to have students engaged in activities that will allow them to understand how natural radioactivity is a part of our everyday environment. This would include how radiation enters our lives in different ways, to demonstrate that natural radioactive sources found in soil, water, and air contribute to our exposure to natural ionizing radiation and how this exposure effects human health. Another objective is to develop a new technique for teaching physics which will enhance scientific interest of students in applications of nuclear physics in both environmental and physical sciences.

  5. Detection of water masers toward young stellar objects in the Large Magellanic Cloud

    SciTech Connect (OSTI)

    Johanson, A. K.; Migenes, V.; Breen, S. L.

    2014-02-01

    We present results from a search for water maser emission toward N4A, N190, and N206, three regions of massive star formation in the Large Magellanic Cloud (LMC). Four water masers were detected; two toward N4A, and two toward N190. In the latter region, no previously known maser emission has been reported. Future studies of maser proper motion to determine the galactic dynamics of the LMC will benefit from the independent data points the new masers in N190 provide. Two of these masers are associated with previously identified massive young stellar objects (YSOs), which strongly supports the authenticity of the classification. We argue that the other two masers identify previously unknown YSOs. No masers were detected toward N206, but it does host a newly discovered 22 GHz continuum source, also associated with a massive YSO. We suggest that future surveys for water maser emission in the LMC be targeted toward the more luminous, massive YSOs.

  6. MAGNETIC FIELD STRUCTURE IN THE FLATTENED ENVELOPE AND JET IN THE YOUNG PROTOSTELLAR SYSTEM HH 211

    SciTech Connect (OSTI)

    Lee, Chin-Fei; Rao, Ramprasad; Hirano, Naomi; Ho, Paul T. P.; Hwang, Hsiang-Chih; Ching, Tao-Chung; Lai, Shih-Ping

    2014-12-10

    HH 211 is a young Class 0 protostellar system with a flattened envelope, a possible rotating disk, and a collimated jet. We have mapped it with the Submillimeter Array in the 341.6 GHz continuum and SiO J = 8-7 at ∼0.''6 resolution. The continuum traces the thermal dust emission in the flattened envelope and the possible disk. Linear polarization is detected in the continuum in the flattened envelope. The field lines implied from the polarization have different orientations, but they are not incompatible with current gravitational collapse models, which predict a different orientation depending on the region/distance. Also, we might have detected for the first time polarized SiO line emission in the jet due to the Goldreich-Kylafis effect. Observations at higher sensitivity are needed to determine the field morphology in the jet.

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

    SciTech Connect (OSTI)

    Gutermuth, R. A.; Pipher, J. L.; Megeath, S. T.; Allen, T. S.; Myers, P. C.; Allen, L. E.

    2011-10-01

    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.

  8. M-dwarf rapid rotators and the detection of relatively young multiple M-star systems

    SciTech Connect (OSTI)

    Rappaport, S.; Joss, M.; Sanchis-Ojeda, R. E-mail: mattjoss@mit.edu; and others

    2014-06-20

    We have searched the Kepler light curves of ?3900 M-star targets for evidence of periodicities that indicate, by means of the effects of starspots, rapid stellar rotation. Several analysis techniques, including Fourier transforms, inspection of folded light curves, 'sonograms', and phase tracking of individual modulation cycles, were applied in order to distinguish the periodicities due to rapid rotation from those due to stellar pulsations, eclipsing binaries, or transiting planets. We find 178 Kepler M-star targets with rotation periods, P {sub rot}, of <2 days, and 110 with P {sub rot} < 1 day. Some 30 of the 178 systems exhibit two or more independent short periods within the same Kepler photometric aperture, while several have 3 or more short periods. Adaptive optics imaging and modeling of the Kepler pixel response function for a subset of our sample support the conclusion that the targets with multiple periods are highly likely to be relatively young physical binary, triple, and even quadruple M star systems. We explore in detail the one object with four incommensurate periods all less than 1.2 days, and show that two of the periods arise from one of a close pair of stars, while the other two arise from the second star, which itself is probably a visual binary. If most of these M-star systems with multiple periods turn out to be bound M stars, this could prove a valuable way discovering young hierarchical M-star systems; the same approach may also be applicable to G and K stars. The ?5% occurrence rate of rapid rotation among the ?3900 M star targets is consistent with spin evolution models that include an initial contraction phase followed by magnetic braking, wherein a typical M star can spend several hundred Myr before spinning down to periods longer than 2 days.

  9. Jet emission in young radio sources: A Fermi large area telescope gamma-ray view

    SciTech Connect (OSTI)

    Migliori, G.; Siemiginowska, A.; Kelly, B. C.; Stawarz, ?.; Celotti, A.; Begelman, M. C.

    2014-01-10

    We investigate the contribution of the beamed jet component to the high-energy emission in young and compact extragalactic radio sources, focusing for the first time on the ?-ray band. We derive predictions on the ?-ray luminosities associated with the relativistic jet assuming a leptonic radiative model. The high-energy emission is produced via Compton scattering by the relativistic electrons in a spherical region at the considered scales (?10 kpc). Simulations show a wide range of ?-ray luminosities, with intensities up to ?10{sup 46}-10{sup 48} erg s{sup 1} depending on the assumed jet parameters. We find a highly linear relation between the simulated X-ray and ?-ray luminosities that can be used to select candidates for ?-ray detection. We compare the simulated luminosity distributions in the radio, X-ray, and ?-ray regimes with observations for the largest sample of X-ray-detected young radio quasars. Our analysis of ?4-yr Fermi Large Area Telescope (LAT) data does not yield any statistically significant detections. However, the majority of the model-predicted ?-ray fluxes for the sample are near or below the current Fermi-LAT flux threshold and compatible with the derived upper limits. Our study gives constraints on the minimum jet power (L {sub jet,} {sub kin}/L {sub disk} > 0.01) of a potential jet contribution to the X-ray emission in the most compact sources (? 1 kpc) and on the particle-to-magnetic field energy density ratio that are in broad agreement with equipartition assumptions.

  10. CSI 2264: characterizing accretion-burst dominated light curves for young stars in NGC 2264

    SciTech Connect (OSTI)

    Stauffer, John; Cody, Ann Marie; Rebull, Luisa; Carey, Sean; Baglin, Annie; Alencar, Silvia; Hillenbrand, Lynne A.; Carpenter, John; Findeisen, Krzysztof; Venuti, Laura; Bouvier, Jerome; Plavchan, Peter; Terebey, Susan; Morales-Caldern, Mara; Micela, Giusi; Flaccomio, Ettore; Song, Inseok; Gutermuth, Rob; Hartmann, Lee; and others

    2014-04-01

    Based on more than four weeks of continuous high-cadence photometric monitoring of several hundred members of the young cluster NGC 2264 with two space telescopes, NASA's Spitzer and the CNES CoRoT (Convection, Rotation, and planetary Transits), we provide high-quality, multi-wavelength light curves for young stellar objects whose optical variability is dominated by short-duration flux bursts, which we infer are due to enhanced mass accretion rates. These light curves show many briefseveral hours to one daybrightenings at optical and near-infrared wavelengths with amplitudes generally in the range of 5%-50% of the quiescent value. Typically, a dozen or more of these bursts occur in a 30 day period. We demonstrate that stars exhibiting this type of variability have large ultraviolet (UV) excesses and dominate the portion of the u g versus g r color-color diagram with the largest UV excesses. These stars also have large H? equivalent widths, and either centrally peaked, lumpy H? emission profiles or profiles with blueshifted absorption dips associated with disk or stellar winds. Light curves of this type have been predicted for stars whose accretion is dominated by Rayleigh-Taylor instabilities at the boundary between their magnetosphere and inner circumstellar disk, or where magneto-rotational instabilities modulate the accretion rate from the inner disk. Among the stars with the largest UV excesses or largest H? equivalent widths, light curves with this type of variability greatly outnumber light curves with relatively smooth sinusoidal variations associated with long-lived hot spots. We provide quantitative statistics for the average duration and strength of the accretion bursts and for the fraction of the accretion luminosity associated with these bursts.

  11. Effects of turbulence on cosmic ray propagation in protostars and young star/disk systems

    SciTech Connect (OSTI)

    Fatuzzo, Marco; Adams, Fred C. E-mail: fca@umich.edu

    2014-05-20

    The magnetic fields associated with young stellar objects are expected to have an hour-glass geometry, i.e., the magnetic field lines are pinched as they thread the equatorial plane surrounding the forming star but merge smoothly onto a background field at large distances. With this field configuration, incoming cosmic rays experience both a funneling effect that acts to enhance the flux impinging on the circumstellar disk and a magnetic mirroring effect that acts to reduce that flux. To leading order, these effects nearly cancel out for simple underlying magnetic field structures. However, the environments surrounding young stellar objects are expected to be highly turbulent. This paper shows how the presence of magnetic field fluctuations affects the process of magnetic mirroring, and thereby changes the flux of cosmic rays striking circumstellar disks. Turbulence has two principle effects: (1) the (single) location of the magnetic mirror point found in the absence of turbulence is replaced with a wide distribution of values. (2) The median of the mirror point distribution moves outward for sufficiently large fluctuation amplitudes (roughly when ?B/B {sub 0} > 0.2 at the location of the turbulence-free mirror point); the distribution becomes significantly non-Gaussian in this regime as well. These results may have significant consequences for the ionization fraction of the disk, which in turn dictates the efficiency with which disk material can accrete onto the central object. A similar reduction in cosmic ray flux can occur during the earlier protostellar stages; the decrease in ionization can help alleviate the magnetic braking problem that inhibits disk formation.

  12. ORIGIN OF THE UNUSUALLY LOW NITROGEN ABUNDANCES IN YOUNG POPULATIONS OF THE LARGE MAGELLANIC CLOUD

    SciTech Connect (OSTI)

    Bekki, Kenji [ICRAR, M468, University of Western Australia, 35 Stirling Highway, Crawley Western Australia 6009 (Australia); Tsujimoto, Takuji [National Astronomical Observatory, Mitaka-shi, Tokyo 181-8588 (Japan)

    2010-10-01

    It is a longstanding problem that H II regions and very young stellar populations in the Large Magellanic Cloud (LMC) have nitrogen abundances ([N/H]) that are a factor of {approx}7 lower than the solar value. We here discuss a new scenario in which the observed unusually low nitrogen abundances can be closely associated with recent collisions and subsequent accretion of H I high velocity clouds (HVCs) that surround the Galaxy and have low nitrogen abundances. We show that if the observed low [N/H] is limited to very young stars with ages less than {approx}10{sup 7} yr, then the collision/accretion rate of the HVCs onto the LMC needs to be {approx}0.2 M{sub sun} yr{sup -1} (corresponding to the total HVC mass of 10{sup 6}-10{sup 7} M{sub sun}) to dilute the original interstellar medium (ISM) before star formation. The required accretion rate means that even if the typical mass of HVCs accreted onto the LMC is {approx}10{sup 7} M{sub sun}, the Galaxy needs to have {approx}2500 massive HVCs within the LMC's orbital radius with respect to the Galactic center. The rather large number of required massive HVCs drives us to suggest that the HVCs are not likely to efficiently dilute the ISM of the LMC and consequently lower the [N/H]. We thus suggest the transfer of gas with low [N/H] from the Small Magellanic Cloud to the LMC as a promising scenario that can explain the observed low [N/H].

  13. TENTATIVE EVIDENCE FOR RELATIVISTIC ELECTRONS GENERATED BY THE JET OF THE YOUNG SUN-LIKE STAR DG Tau

    SciTech Connect (OSTI)

    Ainsworth, Rachael E.; Ray, Tom P.; Taylor, Andrew M.; Scaife, Anna M. M.; Green, David A.; Buckle, Jane V.

    2014-09-01

    Synchrotron emission has recently been detected in the jet of a massive protostar, providing further evidence that certain jet formation characteristics for young stars are similar to those found for highly relativistic jets from active galactic nuclei. We present data at 325 and 610MHz taken with the Giant Metrewave Radio Telescope of the young, low-mass star DG Tau, an analog of the Sun soon after its birth. This is the first investigation of a low-mass young stellar object at such low frequencies. We detect emission with a synchrotron spectral index in the proximity of the DG Tau jet and interpret this emission as a prominent bow shock associated with this outflow. This result provides tentative evidence for the acceleration of particles to relativistic energies due to the shock impact of this otherwise very low-power jet against the ambient medium. We calculate the equipartition magnetic field strength B {sub min} ? 0.11mG and particle energy E {sub min} ? 4 10{sup 40}erg, which are the minimum requirements to account for the synchrotron emission of the DG Tau bow shock. These results suggest the possibility of low energy cosmic rays being generated by young Sun-like stars.

  14. A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFS

    SciTech Connect (OSTI)

    Allers, K. N.; Liu, Michael C.

    2013-08-01

    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.

  15. MAIN-SEQUENCE STARS MASQUERADING AS YOUNG STELLAR OBJECTS IN THE CENTRAL MOLECULAR ZONE

    SciTech Connect (OSTI)

    Koepferl, Christine M.; Robitaille, Thomas P.; Morales, Esteban F. E.; Johnston, Katharine G.

    2015-01-20

    In contrast to most other galaxies, star formation rates in the Milky Way can be estimated directly from young stellar objects (YSOs). In the central molecular zone the star formation rate calculated from the number of YSOs with 24?m emission is up to an order of magnitude higher than the value estimated from methods based on diffuse emission (such as free-free emission). Whether this effect is real or whether it indicates problems with either or both star formation rate measures is not currently known. In this paper, we investigate whether estimates based on YSOs could be heavily contaminated by more evolved objects such as main-sequence stars. We present radiative transfer models of YSOs and of main-sequence stars in a constant ambient medium which show that the main-sequence objects can indeed mimic YSOs at 24?m. However, we show that in some cases the main-sequence models can be marginally resolved at 24?m, whereas the YSO models are always unresolved. Based on the fraction of resolved MIPS 24?m sources in the sample of YSOs previously used to compute the star formation rate, we estimate the fraction of misclassified ''YSOs'' to be at least 63%, which suggests that the star formation rate previously determined from YSOs is likely to be at least a factor of three too high.

  16. Measurement of the temperature dependence of Young's modulus of cartilage by phase-sensitive optical coherence elastography

    SciTech Connect (OSTI)

    Liu, C H; Li, J; Singh, M; Larin, K V; Skryabina, M N; Sobol, E N

    2014-08-31

    The development of an effective system to monitor the changes in the elastic properties of cartilage tissue with increasing temperature in laser reconstruction is an urgent practical task. In this paper, the use of phase-sensitive optical coherence elastography for detection of elastic waves in the sample has allowed Young's modulus of cartilage tissue to be measured directly during heating. Young's modulus was calculated from the group velocity of propagation of elastic waves excited by means of a system supplying focused air pulses. The measurement results are in agreement with the results of measurements of the modulus of elasticity under mechanical compression. The technique developed allows for noninvasive measurements; its development is promising for the use in vivo. (laser biophotonics)

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

    SciTech Connect (OSTI)

    Bass, V.; Gordon, C.J.; Jarema, K.A.; MacPhail, R.C.; Cascio, W.E.; Phillips, P.M.; Ledbetter, A.D.; Schladweiler, M.C.; Andrews, D.; Miller, D.; Doerfler, D.L.; Kodavanti, U.P.

    2013-12-15

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

  18. Nonthermal radiation of young supernova remnants: The case of Cas A

    SciTech Connect (OSTI)

    Zirakashvili, V. N.; Aharonian, F. A.; Yang, R.; Oa-Wilhelmi, E.; Tuffs, R. J.

    2014-04-20

    The processes responsible for the broadband radiation of the young supernova remnant Cas A are explored by using a new code that is designed for a detailed treatment of the diffusive shock acceleration of particles in the nonlinear regime. The model is based on spherically symmetric hydrodynamic equations complemented with transport equations for relativistic particles. Electrons, protons, and the oxygen ions accelerated by forward and reverse shocks are included in the numerical calculations. We show that the available multi-wavelength observations in the radio, X-ray, and gamma-ray bands can be best explained by invoking particle acceleration by both forward and reversed shocks. Although the TeV gamma-ray observations can be interpreted by interactions of both accelerated electrons and protons/ions, the measurements by Fermi Large Area Telescope at energies below 1 GeV give a tentative preference to the hadronic origin of gamma-rays. Then, the acceleration efficiency in this source, despite the previous claims, should be very high; 25% of the explosion energy (or approximately 3 10{sup 50} erg) should already be converted to cosmic rays, mainly by the forward shock. At the same time, the model calculations do not provide extension of the maximum energy of accelerated protons beyond 100 TeV. In this model, the acceleration of electrons is dominated by the reverse shock; the required 10{sup 48} erg can be achieved under the assumption that the injection of electrons (positrons) is supported by the radioactive decay of {sup 44}Ti.

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

    SciTech Connect (OSTI)

    Aller, Kimberly M.; Kraus, Adam L.; Liu, Michael C.; Burgett, William S.; Chambers, Kenneth C.; Hodapp, Klaus W.; Kaiser, Nick; Magnier, Eugene A.; Price, Paul A.

    2013-08-10

    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.

  20. The Gemini NICI planet-finding campaign: the orbit of the young exoplanet ? Pictoris b

    SciTech Connect (OSTI)

    Nielsen, Eric L.; Liu, Michael C.; Chun, Mark; Ftaclas, Christ; Wahhaj, Zahed; Biller, Beth A.; Hayward, Thomas L.; Kuchner, Marc J.; Rodigas, Timothy J.; Toomey, Douglas W.

    2014-10-20

    We present new astrometry for the young (12-21 Myr) exoplanet ? Pictoris b taken with the Gemini/NICI and Magellan/MagAO instruments between 2009 and 2012. The high dynamic range of our observations allows us to measure the relative position of ? Pic b with respect to its primary star with greater accuracy than previous observations. Based on a Markov Chain Monte Carlo analysis, we find the planet has an orbital semi-major axis of 9.1{sub ?0.5}{sup +5.3} AU and orbital eccentricity <0.15 at 68% confidence (with 95% confidence intervals of 8.2-48 AU and 0.00-0.82 for semi-major axis and eccentricity, respectively, due to a long narrow degenerate tail between the two). We find that the planet has reached its maximum projected elongation, enabling higher precision determination of the orbital parameters than previously possible, and that the planet's projected separation is currently decreasing. With unsaturated data of the entire ? Pic system (primary star, planet, and disk) obtained thanks to NICI's semi-transparent focal plane mask, we are able to tightly constrain the relative orientation of the circumstellar components. We find the orbital plane of the planet lies between the inner and outer disks: the position angle (P.A.) of nodes for the planet's orbit (211.8 0.3) is 7.4? greater than the P.A. of the spine of the outer disk and 3.2? less than the warped inner disk P.A., indicating the disk is not collisionally relaxed. Finally, for the first time we are able to dynamically constrain the mass of the primary star ? Pic to 1.76{sub ?0.17}{sup +0.18} M {sub ?}.

  1. SPIN EVOLUTION OF ACCRETING YOUNG STARS. I. EFFECT OF MAGNETIC STAR-DISK COUPLING

    SciTech Connect (OSTI)

    Matt, Sean P.; Greene, Thomas P.; Pinzon, Giovanni; De la Reza, Ramiro E-mail: thomas.p.greene@nasa.go E-mail: delareza@on.b

    2010-05-10

    We present a model for the rotational evolution of a young, solar mass star interacting with an accretion disk. The model incorporates a description of the angular momentum transfer between the star and the disk due to a magnetic connection, and includes changes in the star's mass and radius and a decreasing accretion rate. The model also includes, for the first time in a spin evolution model, the opening of the stellar magnetic field lines, as expected to arise from twisting via star-disk differential rotation. In order to isolate the effect that this has on the star-disk interaction torques, we neglect the influence of torques that may arise from open field regions connected to the star or disk. For a range of magnetic field strengths, accretion rates, and initial spin rates, we compute the stellar spin rates of pre-main-sequence stars as they evolve on the Hayashi track to an age of 3 Myr. How much the field opening affects the spin depends on the strength of the coupling of the magnetic field to the disk. For the relatively strong coupling (i.e., high magnetic Reynolds number) expected in real systems, all models predict spin periods of less than {approx}3 days, in the age range of 1-3 Myr. Furthermore, these systems typically do not reach an equilibrium spin rate within 3 Myr, so that the spin at any given time depends upon the choice of initial spin rate. This corroborates earlier suggestions that, in order to explain the full range of observed rotation periods of approximately 1-10 days, additional processes, such as the angular momentum loss from powerful stellar winds, are necessary.

  2. SEARCH FOR IONIZED JETS TOWARD HIGH-MASS YOUNG STELLAR OBJECTS

    SciTech Connect (OSTI)

    Guzman, Andres E.; Garay, Guido; Brooks, Kate J.; Voronkov, Maxim A.

    2012-07-01

    We are carrying out multi-frequency radio continuum observations, using the Australia Telescope Compact Array, to systematically search for collimated ionized jets toward high-mass young stellar objects (HMYSOs). Here we report observations at 1.4, 2.4, 4.8, and 8.6 GHz, made with angular resolutions of about 7'', 4'', 2'', and 1'', respectively, toward six objects of a sample of 33 southern HMYSOs thought to be in very early stages of evolution. The objects in the sample were selected from radio and infrared catalogs by having positive radio spectral indices and being luminous (L{sub bol} > 2 Multiplication-Sign 10{sup 4} L{sub Sun }), but underluminous in radio emission compared with that expected from its bolometric luminosity. This criterion makes the radio sources good candidates for being ionized jets. As part of this systematic search, two ionized jets have been discovered: one previously published and the other reported here. The rest of the observed candidates correspond to three hypercompact H II regions and two ultracompact H II regions. The two jets discovered are associated with two of the most luminous (7 Multiplication-Sign 10{sup 4} and 1.0 Multiplication-Sign 10{sup 5} L{sub Sun }) HMYSOs known to harbor this type of object, showing that the phenomena of collimated ionized winds appear in the formation process of stars at least up to masses of {approx}20 M{sub Sun} and provide strong evidence for a disk-mediated accretion scenario for the formation of high-mass stars. From the incidence of jets in our sample, we estimate that the jet phase in high-mass protostars lasts for {approx}4 Multiplication-Sign 10{sup 4} yr.

  3. PHOTOELECTRIC CHARGING OF DUST GRAINS IN THE ENVIRONMENT OF YOUNG STELLAR OBJECTS

    SciTech Connect (OSTI)

    Pedersen, Andreas; Gomez de Castro, Ana I.

    2011-10-20

    The evolution of disks around young stellar objects (YSOs) is deeply affected by the YSOs' ultraviolet (UV) radiation field especially in the 500-1100 A spectral range. The two dominant processes are: the photodissociation of H{sub 2} molecules in the Werner and Lyman bands, and the emission of photoelectrons from dust grains when high energy photons are absorbed. Photoelectrons are an important source of gas heating. In this paper, dust grain charging when exposed to various possible UV fields in the YSOs' environment is investigated. Numerical simulations of the evolution of photoelectrons in the electric field created by the charged dust grains are carried out to obtain the charging profile of dust grains. From the simulations it appears that the different spectra produce significant quantitative and qualitative differences in the charging processes. Both the UV background and the Ae-Herbig star radiation field produce a relatively slow charging of dust grains due to the low fraction of sufficiently energetic photons. The radiation field of T Tauri stars (TTSs) is harder due to the release of magnetic energy in the dense magnetospheric environment. These numerical results have been used to propose a new simple analytical model for grain charging in the atmosphere of protostellar disks around TTSs susceptible to be used in any disk modeling. It has been found that the yield decreases exponentially with the dust charge and that two populations of photoelectrons are produced: a low energy population with mean kinetic energy E = 2.5 eV and a high energy population with E = 5.5-6 eV; the energy dispersion within the populations is {approx}1.3 eV (T {approx} 1.5 x 10{sup 4} K). The high energy population is susceptible of dissociating the H{sub 2} and ionizing some low ionization potential species, such as the Mg. These results add an additional role to dust on the chemistry of the layers just below the H{sub 2} photoionization front. This photoelectic yield has been applied to a simple evaluation of the dust charge in the atmospheres of accretion disks ({alpha}-disks).

  4. Young stellar object variability (YSOVAR): Long timescale variations in the mid-infrared

    SciTech Connect (OSTI)

    Rebull, L. M.; Cody, A. M.; Stauffer, J. R.; Morales-Caldern, M.; Carey, S. J.; Covey, K. R.; Gnther, H. M.; Poppenhaeger, K.; Wolk, S. J.; Hora, J. L.; Hillenbrand, L. A.; Plavchan, P.; Gutermuth, R.; Song, I.; Barrado, D.; Bayo, A.; James, D.; Vrba, F. J.; Alves de Oliveira, C.; Bouvier, J.; and others

    2014-11-01

    The YSOVAR (Young Stellar Object VARiability) Spitzer Space Telescope observing program obtained the first extensive mid-infrared (3.6 and 4.5 ?m) time series photometry of the Orion Nebula Cluster plus smaller footprints in 11 other star-forming cores (AFGL 490, NGC 1333, Mon R2, GGD 12-15, NGC 2264, L1688, Serpens Main, Serpens South, IRAS 20050+2720, IC 1396A, and Ceph C). There are ?29,000 unique objects with light curves in either or both IRAC channels in the YSOVAR data set. We present the data collection and reduction for the Spitzer and ancillary data, and define the 'standard sample' on which we calculate statistics, consisting of fast cadence data, with epochs roughly twice per day for ?40 days. We also define a 'standard sample of members' consisting of all the IR-selected members and X-ray-selected members. We characterize the standard sample in terms of other properties, such as spectral energy distribution shape. We use three mechanisms to identify variables in the fast cadence datathe Stetson index, a ?{sup 2} fit to a flat light curve, and significant periodicity. We also identified variables on the longest timescales possible of six to seven years by comparing measurements taken early in the Spitzer mission with the mean from our YSOVAR campaign. The fraction of members in each cluster that are variable on these longest timescales is a function of the ratio of Class I/total members in each cluster, such that clusters with a higher fraction of Class I objects also have a higher fraction of long-term variables. For objects with a YSOVAR-determined period and a [3.6]-[8] color, we find that a star with a longer period is more likely than those with shorter periods to have an IR excess. We do not find any evidence for variability that causes [3.6]-[4.5] excesses to appear or vanish within our data set; out of members and field objects combined, at most 0.02% may have transient IR excesses.

  5. Greenhouse gas emissions from landfill leachate treatment plants: A comparison of young and aged landfill

    SciTech Connect (OSTI)

    Wang, Xiaojun; Jia, Mingsheng; Chen, Xiaohai; Xu, Ying; Lin, Xiangyu; Kao, Chih Ming; Chen, Shaohua

    2014-07-15

    Highlights: • Young and aged leachate works accounted for 89.1% and 10.9% of 33.35 Gg CO{sub 2} yr{sup −1}. • Fresh leachate owned extremely low ORP and high organic matter content. • Strong CH{sub 4} emissions occurred in the fresh leachate ponds, but small in the aged. • N{sub 2}O emissions became dominant in the treatment units of both systems. • 8.45–11.9% of nitrogen was removed as the form of N{sub 2}O under steady-state. - Abstract: With limited assessment, leachate treatment of a specified landfill is considered to be a significant source of greenhouse gas (GHG) emissions. In our study, the cumulative GHG emitted from the storage ponds and process configurations that manage fresh or aged landfill leachate were investigated. Our results showed that strong CH{sub 4} emissions were observed from the fresh leachate storage pond, with the fluxes values (2219–26,489 mg C m{sup −2} h{sup −1}) extremely higher than those of N{sub 2}O (0.028–0.41 mg N m{sup −2} h{sup −1}). In contrast, the emission values for both CH{sub 4} and N{sub 2}O were low for the aged leachate tank. N{sub 2}O emissions became dominant once the leachate entered the treatment plants of both systems, accounting for 8–12% of the removal of N-species gases. Per capita, the N{sub 2}O emission based on both leachate treatment systems was estimated to be 7.99 g N{sub 2}O–N capita{sup −1} yr{sup −1}. An increase of 80% in N{sub 2}O emissions was observed when the bioreactor pH decreased by approximately 1 pH unit. The vast majority of carbon was removed in the form of CO{sub 2}, with a small portion as CH{sub 4} (<0.3%) during both treatment processes. The cumulative GHG emissions for fresh leachate storage ponds, fresh leachate treatment system and aged leachate treatment system were 19.10, 10.62 and 3.63 Gg CO{sub 2} eq yr{sup −1}, respectively, for a total that could be transformed to 9.09 kg CO{sub 2} eq capita{sup −1} yr{sup −1}.

  6. PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT ,

    SciTech Connect (OSTI)

    Bowler, Brendan P.; Liu, Michael C.; Shkolnik, Evgenya L.; Dupuy, Trent J.

    2013-09-01

    We report the discovery of an L-type companion to the young M3.5V star 2MASS J01225093-2439505 at a projected separation of 1.''45 ( Almost-Equal-To 52 AU) as part of our adaptive optics imaging search for extrasolar giant planets around young low-mass stars. 2MASS 0122-2439 B has very red near-infrared colors similar to the HR 8799 planets and the reddest known young/dusty L dwarfs in the field. Moderate-resolution (R Almost-Equal-To 3800) 1.5-2.4 {mu}m spectroscopy reveals a near-infrared spectral type of L4-L6 and an angular H-band shape, confirming its cool temperature and young age. The kinematics of 2MASS 0122-2439 AB are marginally consistent with members of the {approx}120 Myr AB Dor young moving group based on the photometric distance to the primary (36 {+-} 4 pc) and our radial velocity measurement of 2MASS 0122-2439 A from Keck/HIRES. We adopt the AB Dor group age for the system, but the high energy emission, lack of Li I {lambda}6707 absorption, and spectral shape of 2MASS 0122-2439 B suggest a range of {approx}10-120 Myr is possible. The age and luminosity of 2MASS 0122-2439 B fall in a strip where ''hot-start'' evolutionary model mass tracks overlap as a result of deuterium burning. Several known substellar companions also fall in this region (2MASS J0103-5515 ABb, AB Pic b, {kappa} And b, G196-3 B, SDSS 2249+0044 B, LP 261-75 B, HD 203030 B, and HN Peg B), but their dual-valued mass predictions have largely been unrecognized. The implied mass of 2MASS 0122-2439 B is Almost-Equal-To 12-13 M{sub Jup} or Almost-Equal-To 22-27 M{sub Jup} if it is an AB Dor member, or possibly as low as 11 M{sub Jup} if the wider age range is adopted. Evolutionary models predict an effective temperature for 2MASS 0122-2439 B that corresponds to spectral types near the L/T transition ( Almost-Equal-To 1300-1500 K) for field objects. However, we find a mid-L near-infrared spectral type, indicating that 2MASS 0122-2439 B represents another case of photospheric dust being retained to cooler temperatures at low surface gravities, as seen in the spectra of young (8-30 Myr) planetary companions. Altogether, the low mass, low temperature, and red colors of 2MASS 0122-2439 B make it a bridge between warm planets like {beta} Pic b and cool, very dusty ones like HR 8799 bcde.

  7. BANYAN. II. Very low mass and substellar candidate members to nearby, young kinematic groups with previously known signs of youth

    SciTech Connect (OSTI)

    Gagn, Jonathan; Lafrenire, David; Doyon, Ren; Malo, Lison; Artigau, tienne

    2014-03-10

    We present Bayesian Analysis for Nearby Young AssociatioNs II (BANYAN II), a modified Bayesian analysis for assessing the membership of later-than-M5 objects to any of several Nearby Young Associations (NYAs). In addition to using kinematic information (from sky position and proper motion), this analysis exploits 2MASS-WISE color-magnitude diagrams in which old and young objects follow distinct sequences. As an improvement over our earlier work, the spatial and kinematic distributions for each association are now modeled as ellipsoids whose axes need not be aligned with the Galactic coordinate axes, and we use prior probabilities matching the expected populations of the NYAs considered versus field stars. We present an extensive contamination analysis to characterize the performance of our new method. We find that Bayesian probabilities are generally representative of contamination rates, except when a parallax measurement is considered. In this case contamination rates become significantly smaller and hence Bayesian probabilities for NYA memberships are pessimistic. We apply this new algorithm to a sample of 158 objects from the literature that are either known to display spectroscopic signs of youth or have unusually red near-infrared colors for their spectral type. Based on our analysis, we identify 25 objects as new highly probable candidates to NYAs, including a new M7.5 bona fide member to Tucana-Horologium, making it the latest-type member. In addition, we reveal that a known L2? dwarf is co-moving with a bright M5 dwarf, and we show for the first time that two of the currently known ultra red L dwarfs are strong candidates to the AB Doradus moving group. Several objects identified here as highly probable members to NYAs could be free-floating planetary-mass objects if their membership is confirmed.

  8. HERSCHEL FINDS EVIDENCE FOR STELLAR WIND PARTICLES IN A PROTOSTELLAR ENVELOPE: IS THIS WHAT HAPPENED TO THE YOUNG SUN?

    SciTech Connect (OSTI)

    Ceccarelli, C.; Lpez-Sepulcre, A.; Dominik, C.; Kama, M.; Padovani, M.; Caux, E.; Caselli, P.

    2014-07-20

    There is evidence that the young Sun emitted a high flux of energetic (?10MeV) particles. The collisions of these particles with the material at the inner edge of the Protosolar Nebula disk induced spallation reactions that formed short-lived radionuclei, like {sup 10}Be, whose trace is now visible in some meteorites. However, it is poorly known exactly when this happened, and whether and how it affected the solar system. Here, we present indirect evidence for an ejection of energetic particles in the young protostar, OMC-2 FIR 4, similar to that experienced by the young solar system. In this case, the energetic particles collide with the material in the protostellar envelope, enhancing the abundance of two molecular ions, HCO{sup +} and N{sub 2}H{sup +}, whose presence is detected via Herschel observations. The flux of energetic particles at a distance of 1AU from the emitting source, estimated from the measured abundance ratio of HCO{sup +} and N{sub 2}H{sup +}, can easily account for the irradiation required by meteoritic observations. These new observations demonstrate that the ejection of ?10MeV particles is a phenomenon occurring very early in the life of a protostar, before the disappearance of the envelope from which the future star accretes. The whole envelope is affected by the event, which sets constraints on the magnetic field geometry in the source and opens up the possibility that the spallation reactions are not limited to the inner edge of the Protosolar Nebula disk.

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

    Office of Legacy Management (LM)

    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

  10. Possible contribution of low shear modulus C{sub 44} to the low Young's modulus of Ti-36Nb-5Zr alloy

    SciTech Connect (OSTI)

    Meng, Qingkun; Xu, Huibin; Zhao, Xinqing; Guo, Shun; Ren, Xiaobing

    2014-09-29

    Despite the importance of single-crystal elastic constants of ?-phase titanium alloys in understanding their low Young's modulusa property crucial for many applications, such data are often difficult to obtain when the alloy composition is close to the instability limit of the ? phase, where the presence of ?' martensite precludes the fabrication of ?-phase single crystal. In the present study, we extracted the single-crystal elastic constants of such a ?-phase titanium alloy with low Young's modulus, Ti-36Nb-5Zr (wt.?%), from polycrystalline specimens by using an in-situ synchrotron X-ray diffraction technique. It is indicated that the low Young's modulus of the alloy originates from the anomalously low shear modulus C{sub 44} as well as the low shear modulus C?, which is different from a common viewpoint that the Young's modulus of ?-phase titanium alloys is dominantly controlled by the C?. This suggests that low C{sub 44} is an important contributor to low Young's modulus for instable ?-phase titanium alloys.

  11. Geologic Characterization of Young Alluvial Basin-Fill Deposits from Drill Hole Data in Yucca Flat, Nye County, Nevada.

    SciTech Connect (OSTI)

    Donald S. Sweetkind; Ronald M. Drake II

    2007-01-22

    Yucca Flat is a topographic and structural basin in the northeastern part of the Nevada Test Site (NTS) in Nye County, Nevada, that has been the site of numerous underground nuclear tests; many of these tests occurred within the young alluvial basin-fill deposits. The migration of radionuclides to the Paleozoic carbonate aquifer involves passage through this thick, heterogeneous section of Tertiary and Quaternary rock. An understanding of the lateral and vertical changes in the material properties of young alluvial basin-fill deposits will aid in the further development of the hydrogeologic framework and the delineation of hydrostratigraphic units and hydraulic properties required for simulating ground-water flow in the Yucca Flat area. This report by the U.S. Geological Survey, in cooperation with the U.S. Department of Energy, presents data and interpretation regarding the three-dimensional variability of the shallow alluvial aquifers in areas of testing at Yucca Flat, data that are potentially useful in the understanding of the subsurface flow system. This report includes a summary and interpretation of alluvial basin-fill stratigraphy in the Yucca Flat area based on drill hole data from 285 selected drill holes. Spatial variations in lithology and grain size of the Neogene basin-fill sediments can be established when data from numerous drill holes are considered together. Lithologic variations are related to different depositional environments within the basin including alluvial fan, channel, basin axis, and playa deposits.

  12. KEPLER-63b: A GIANT PLANET IN A POLAR ORBIT AROUND A YOUNG SUN-LIKE STAR

    SciTech Connect (OSTI)

    Sanchis-Ojeda, Roberto; Winn, Joshua N.; Albrecht, Simon; Marcy, Geoffrey W.; Isaacson, Howard; Howard, Andrew W.; Johnson, John Asher; Torres, Guillermo; Carter, Joshua A.; Dawson, Rebekah I.; Geary, John C.; Campante, Tiago L.; Chaplin, William J.; Davies, Guy R.; Lund, Mikkel N.; Buchhave, Lars A.; Everett, Mark E.; Fischer, Debra A.; Gilliland, Ronald L.; Horch, Elliott P.; and others

    2013-09-20

    We present the discovery and characterization of a giant planet orbiting the young Sun-like star Kepler-63 (KOI-63, m{sub Kp} = 11.6, T{sub eff} = 5576 K, M{sub *} = 0.98 M{sub ?}). The planet transits every 9.43 days, with apparent depth variations and brightening anomalies caused by large starspots. The planet's radius is 6.1 0.2 R{sub ?}, based on the transit light curve and the estimated stellar parameters. The planet's mass could not be measured with the existing radial-velocity data, due to the high level of stellar activity, but if we assume a circular orbit, then we can place a rough upper bound of 120 M{sub ?} (3?). The host star has a high obliquity (? = 104), based on the Rossiter-McLaughlin effect and an analysis of starspot-crossing events. This result is valuable because almost all previous obliquity measurements are for stars with more massive planets and shorter-period orbits. In addition, the polar orbit of the planet combined with an analysis of spot-crossing events reveals a large and persistent polar starspot. Such spots have previously been inferred using Doppler tomography, and predicted in simulations of magnetic activity of young Sun-like stars.

  13. THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A MULTIPLE SYSTEM ORBITING THE YOUNG A STAR HD 1160

    SciTech Connect (OSTI)

    Nielsen, Eric L.; Liu, Michael C.; Wahhaj, Zahed; Bowler, Brendan; Kraus, Adam; Chun, Mark; Ftaclas, Christ; Biller, Beth A.; Hayward, Thomas L.; Shkolnik, Evgenya L.; Tecza, Matthias; Clarke, Fraser; Close, Laird M.; Hartung, Markus; Males, Jared R.; Skemer, Andrew J.; Reid, I. Neill; Alencar, Silvia H. P.; Burrows, Adam; and others

    2012-05-01

    We report the discovery of two low-mass companions to the young A0V star HD 1160 at projected separations of 81 {+-} 5 AU (HD 1160 B) and 533 {+-} 25 AU (HD 1160 C) by the Gemini NICI Planet-Finding Campaign. Very Large Telescope images of the system taken over a decade for the purpose of using HD 1160 A as a photometric calibrator confirm that both companions are physically associated. By comparing the system to members of young moving groups and open clusters with well-established ages, we estimate an age of 50{sup +50}{sub -40} Myr for HD 1160 ABC. While the UVW motion of the system does not match any known moving group, the small magnitude of the space velocity is consistent with youth. Near-IR spectroscopy shows HD 1160 C to be an M3.5 {+-} 0.5 star with an estimated mass of 0.22{sup +0.03}{sub -0.04} M{sub Sun }, while NIR photometry of HD 1160 B suggests a brown dwarf with a mass of 33{sup +12}{sub -9} M{sub Jup}. The very small mass ratio (0.014) between the A and B components of the system is rare for A star binaries, and would represent a planetary-mass companion were HD 1160 A to be slightly less massive than the Sun.

  14. THE EXTREMELY RED, YOUNG L DWARF PSO J318.533822.8603: A FREE-FLOATING PLANETARY-MASS ANALOG TO DIRECTLY IMAGED YOUNG GAS-GIANT PLANETS

    SciTech Connect (OSTI)

    Liu, Michael C.; Magnier, Eugene A.; Kotson, Michael C.; Aller, Kimberly M.; Burgett, W. S.; Chambers, K. C.; Hodapp, K. W.; Jedicke, R.; Kaiser, N.; Kudritzki, R.-P.; Morgan, J. S.; Tonry, J. L.; Wainscoat, R. J.; Deacon, Niall R.; Allers, Katelyn N.; Dupuy, Trent J.; Draper, P. W.; Price, P. A.; Metcalfe, N.

    2013-11-10

    We have discovered using Pan-STARRS1 an extremely red late-L dwarf, which has (J K){sub MKO} = 2.78 and (J K){sub 2MASS} = 2.84, making it the reddest known field dwarf and second only to 2MASS J120739b among substellar companions. Near-IR spectroscopy shows a spectral type of L7 1 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 J318.522 point to membership in the ? Pic moving group. Evolutionary models give a temperature of 1160{sup +30}{sub -40} K and a mass of 6.5{sup +1.3}{sub -1.0} M {sub Jup}, making PSO J318.522 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 suggests that young L dwarfs with similar ages and temperatures can have different spectral signatures of youth. For the two objects with well constrained ages (PSO J318.522 and 2MASS J0355+11), we find their temperatures are ?400 K cooler than field objects of similar spectral type but their luminosities are similar, i.e., these young L dwarfs are very red and unusually cool but not 'underluminous'. Altogether, PSO J318.522 is the first free-floating object with the colors, magnitudes, spectrum, luminosity, and mass that overlap the young dusty planets around HR 8799 and 2MASS J120739.

  15. CHARACTERIZATION OF THE YOUNG OPEN CLUSTER G144.9+0.4 IN THE CAMELOPARDALIS OB1 ASSOCIATION

    SciTech Connect (OSTI)

    Lin, Chien-Cheng; Chen, W. P.; Panwar, Neelam

    2013-10-01

    Our star-count analysis of the Two Micron All Sky Survey point sources resulted in an identification of the star cluster G144.9+0.4. The cluster was found, but not characterized, by Glushkova et al. We show that the cluster is physically associated with the Cam OB1 association at a distance of about 1 kpc and with an age of 1-2 Myr. Pre-main sequence stars are identified on the basis of photometric and proper motion data. A total of 91 additional OB star candidates was found in subgroups 1A and 1B, a significant increase from the currently known 43 OB stars. The OB members show an age spread that indicates a sustained star formation for at least the last 10-15 Myr. The young cluster G144.9+0.4 represents the latest episode of sequential star formation in this cloud complex.

  16. Using ISMS Principles and Functions in Developing an ARRA Readiness Review Process

    Broader source: Energy.gov [DOE]

    Presenter: Linda K. Rogers, Assessments & Readiness Programs Manager, Bechtel Jacobs Company, LLC Track 8-8

  17. A123 Systems | Open Energy Information

    Open Energy Info (EERE)

    Zip: 02472 Region: Greater Boston Area Sector: Efficiency Product: Nanotech batteries Website: www.a123systems.com Coordinates: 42.3637762, -71.1662161 Show Map...

  18. 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 This article...

  19. News | Argonne National Laboratory

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

    launches Nano Design Works to support materials commercialization and accelerate the translation of research into products TMR Blog New Argonne centers focus on nanotech, EV energy...

  20. Materials for Energy | Argonne National Laboratory

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

    launches Nano Design Works to support materials commercialization and accelerate the translation of research into products TMR Blog New Argonne centers focus on nanotech, EV energy...

  1. Luminescent single-walled carbon nanotube/silica composite materials...

    Office of Scientific and Technical Information (OSTI)

    Type: Conference Resource Relation: Conference: Nanotech 2011 ; June 16, 2011 ; Boston, MA, USA Research Org: Los Alamos National Laboratory (LANL) Sponsoring Org: DOE Country of...

  2. Fermi-LAT Discovery of GeV Gamma-ray Emission from the Young Supernova Remnant Cassiopeia A

    SciTech Connect (OSTI)

    Abdo, A.A.

    2011-08-19

    We report on the first detection of GeV high-energy gamma-ray emission from a young supernova remnant with the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope. These observations reveal a source with no discernible spatial extension detected at a significance level of 12.2{sigma} above 500 MeV at a location that is consistent with the position of the remnant of the supernova explosion that occurred around 1680 in the Cassiopeia constellation - Cassiopeia A. The gamma-ray flux and spectral shape of the source are consistent with a scenario in which the gamma-ray emission originates from relativistic particles accelerated in the shell of this remnant. The total content of cosmic rays (electrons and protons) accelerated in Cas A can be estimated as W{sub CR} {approx_equal} (1-4) x 10{sup 49} erg thanks to the well-known density in the remnant assuming that the observed gamma-ray originates in the SNR shell(s). The magnetic field in the radio-emitting plasma can be robustly constrained as B {ge} 0.1 mG, providing new evidence of the magnetic field amplification at the forward shock and the strong field in the shocked ejecta.

  3. DYNAMICAL EVIDENCE FOR A MAGNETOCENTRIFUGAL WIND FROM A 20 M{sub Sun} BINARY YOUNG STELLAR OBJECT

    SciTech Connect (OSTI)

    Greenhill, L. J.; Goddi, C.; Humphreys, E. M. L.; Chandler, C. J.; Matthews, L. D.

    2013-06-20

    In Orion BN/KL, proper motions of {lambda}7 mm vibrationally excited SiO masers trace the rotation of a nearly edge-on disk and a bipolar wide-angle outflow 10-100 AU from radio source I, a binary young stellar object of {approx}20 M{sub Sun }. Here we map ground-state {lambda}7 mm SiO emission with the Very Large Array and track proper motions over 9 yr. The innermost and strongest emission lies in two extended arcs bracketing Source I. The proper motions trace a northeast-southwest bipolar outflow 100-1000 AU from Source I with a median three-dimensional motion of {approx}18 km s{sup -1}. An overlying distribution of {lambda}1.3 cm H{sub 2}O masers betrays similar flow characteristics. Gas dynamics and emission morphology traced by the masers suggest the presence of a magnetocentrifugal disk wind. Reinforcing evidence lies in the colinearity of the flow, apparent rotation across the flow parallel to the disk rotation, and recollimation that narrows the flow opening angle {approx}120 AU downstream. The arcs of ground-state SiO emission may mark the transition point to a shocked super-Alfvenic outflow.

  4. Prevalence of persistent cough and phlegm in young adults in relation to long-term ambient sulfur oxide exposure

    SciTech Connect (OSTI)

    Chapman, R.S.; Calafiore, D.C.; Hasselblad, V.

    1985-01-01

    In early 1976, a survey of persistent co gh and plegma (PCP) prevalence was conducted in 5623 young adults in four Utah communities. Over the previous five years, community specific mean sulfur dioxide levels had been 11, 18, 36, and 115 ug/mT. Corresponding mean suspended sulfate levels had been 5, 7, 8, and 14 g/mT No intercommunity exposure gradient of total suspended particulates or suspended nitrates was observed. In mothers, PCP prevalence among non-smokers was 4.2% in the high-exposure community and about 2.0% in all other communities. In smoking mothers, PCP prevalence was 21.8% in the high-exposure community and about 15.0% elsewhere. In fathers, PCP prevalence among non-smokers was about 8.0% in the high-exposure community and averaged about 3.0% elsewhere. In smoking fathers, PCP prevalence was less strongly associated with sulfur oxide exposure. PCP prevalence rates estimated in a categorical logistic regression model were qualitatively consistent with the prevalences presented above.

  5. Department

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

    Ener9Y Richland Operations Office P.O. Box 550 Richland, Washington 99352 May 11,2010 Certified Mail Ms. Linda Lammendola Christie Pabarue Mortensen and Young 1880 John F. Kennedy Boulevard 10 th Floor Philadelphia, Pennsylvania 19103 Dear Ms. Larnmendola: FREEDOM OF INFORMATION ACT REQUEST (FOI 2010-01394) Your Freedom of Information Act (FOIA) request dated Apri121, 2010, addressed to the U.S. Department of Energy, Headquarters FOIA Office has been forwarded to this office for response and was

  6. BANYAN. V. A SYSTEMATIC ALL-SKY SURVEY FOR NEW VERY LATE-TYPE LOW-MASS STARS AND BROWN DWARFS IN NEARBY YOUNG MOVING GROUPS

    SciTech Connect (OSTI)

    Gagn, Jonathan; Lafrenire, David; Doyon, Ren; Malo, Lison; Artigau, tienne

    2015-01-10

    We present the BANYAN All-Sky Survey (BASS) catalog, consisting of 228 new late-type (M4-L6) candidate members of nearby young moving groups (YMGs) with an expected false-positive rate of ?13%. This sample includes 79 new candidate young brown dwarfs and 22 planetary-mass objects. These candidates were identified through the first systematic all-sky survey for late-type low-mass stars and brown dwarfs in YMGs. We cross-matched the Two Micron All Sky Survey and AllWISE catalogs outside of the galactic plane to build a sample of 98,970 potential ?M5 dwarfs in the solar neighborhood and calculated their proper motions with typical precisions of 5-15 mas yr{sup 1}. We selected highly probable candidate members of several YMGs from this sample using the Bayesian Analysis for Nearby Young AssociatioNsII tool (BANYANII). We used the most probable statistical distances inferred from BANYANII to estimate the spectral type and mass of these candidate YMG members. We used this unique sample to show tentative signs of mass segregation in the AB Doradus moving group and the Tucana-Horologium and Columba associations. The BASS sample has already been successful in identifying several new young brown dwarfs in earlier publications, and will be of great interest in studying the initial mass function of YMGs and for the search of exoplanets by direct imaging; the input sample of potential close-by ?M5 dwarfs will be useful to study the kinematics of low-mass stars and brown dwarfs and search for new proper motion pairs.

  7. PLANETS AROUND LOW-MASS STARS (PALMS). I. A SUBSTELLAR COMPANION TO THE YOUNG M DWARF 1RXS J235133.3+312720

    SciTech Connect (OSTI)

    Bowler, Brendan P.; Liu, Michael C.; Cieza, Lucas A.; Kraus, Adam L.; Shkolnik, Evgenya L.; Dupuy, Trent J.; Tamura, Motohide

    2012-07-10

    We report the discovery of a brown dwarf companion to the young M dwarf 1RXS J235133.3+312720 as part of a high contrast imaging search for planets around nearby young low-mass stars with Keck-II/NIRC2 and Subaru/HiCIAO. The 2.''4 ({approx}120 AU) pair is confirmed to be comoving from two epochs of high-resolution imaging. Follow-up low- and moderate-resolution near-infrared spectroscopy of 1RXS J2351+3127 B with IRTF/SpeX and Keck-II/OSIRIS reveals a spectral type of L0{sup +2}{sub -1}. The M2 primary star 1RXS J2351+3127 A exhibits X-ray and UV activity levels comparable to young moving group members with ages of {approx}10-100 Myr. UVW kinematics based the measured radial velocity of the primary and the system's photometric distance (50 {+-} 10 pc) indicate it is likely a member of the {approx}50-150 Myr AB Dor moving group. The near-infrared spectrum of 1RXS J2351+3127 B does not exhibit obvious signs of youth, but its H-band morphology shows subtle hints of intermediate surface gravity. The spectrum is also an excellent match to the {approx}200 Myr M9 brown dwarf LP 944-20. Assuming an age of 50-150 Myr, evolutionary models imply a mass of 32 {+-} 6 M{sub Jup} for the companion, making 1RXS J2351+3127 B the second lowest-mass member of the AB Dor moving group after the L4 companion CD-35 2722 B and one of the few benchmark brown dwarfs known at young ages.

  8. The slow ionized wind and rotating disklike system that are associated with the high-mass young stellar object G345.4938+01.4677

    SciTech Connect (OSTI)

    Guzmn, Andrs E.; Garay, Guido; Bronfman, Leonardo; Mardones, Diego; Rodrguez, Luis F.; Moran, James; Brooks, Kate J.; Nyman, Lars-ke; Sanhueza, Patricio

    2014-12-01

    We report the detection, made using ALMA, of the 92 GHz continuum and hydrogen recombination lines (HRLs) H40?, H42?, and H50? emission toward the ionized wind associated with the high-mass young stellar object G345.4938+01.4677. This is the luminous central dominating source located in the massive and dense molecular clump associated with IRAS 165623959. The HRLs exhibit Voigt profiles, which is a strong signature of Stark broadening. We successfully reproduce the observed continuum and HRLs simultaneously using a simple model of a slow ionized wind in local thermodynamic equilibrium, with no need for a high-velocity component. The Lorentzian line wings imply electron densities of 5 10{sup 7} cm{sup 3} on average. In addition, we detect SO and SO{sub 2} emission arising from a compact (?3000 AU) molecular core associated with the central young star. The molecular core exhibits a velocity gradient that is perpendicular to the jet-axis, which we interpret as evidence of rotation. The set of observations toward G345.4938+01.4677 are consistent with it being a young high-mass star associated with a slow photo-ionized wind.

  9. 2MASS 22344161+4041387AB: A WIDE, YOUNG, ACCRETING, LOW-MASS BINARY IN THE LkH{alpha}233 GROUP

    SciTech Connect (OSTI)

    Allers, K. N.; Liu, Michael C.; Cushing, Michael C.; Dupuy, Trent J.; Mathews, Geoffrey S.; Shkolnik, Evgenya; Reid, I. Neill; Cruz, Kelle L.; Vacca, W. D.

    2009-05-20

    We report the discovery of a young, 0.''16 binary, 2M2234+4041AB, found as the result of a Keck laser guide star adaptive optics imaging survey of young field ultracool dwarfs. Spatially resolved near-infrared photometry and spectroscopy indicate that the luminosity and temperature ratios of the system are near unity. From optical and near-infrared spectroscopy, we determine a composite spectral type of M6 for the system. Gravity-sensitive spectral features in the spectra of 2M2234+4041AB are best matched to those of young objects ({approx}1 Myr old). A comparison of the T {sub eff} and age of 2M2234+4041AB to evolutionary models indicates that the mass of each component is 0.10{sup +0.075} {sub -0.04} M {sub sun}. Emission lines of H{alpha} in the composite optical spectrum of the system and Br{gamma} in spatially resolved near-IR spectra of the two components indicate that the system is actively accreting. Both components of the system have IR excesses, indicating that they both harbor circumstellar disks. Though 2M2234+4041AB was originally identified as a young field dwarf, it lies 1.'5 from the well-studied Herbig Ae/Be star, LkH{alpha}233. The distance to LkH{alpha}233 is typically assumed to be 880 pc. It is unlikely that 2M2234+4041AB could be this distant, as it would then be more luminous than any known Taurus objects of similar spectral type. We re-evaluate the distance to the LkH{alpha}233 group and find a value of 325{sup +72} {sub -50} pc, based on the Hipparcos distance to a nearby B3-type group member (HD 213976). 2M2234+4041AB is the first low-mass star to be potentially associated with the LkH{alpha}233 group. At a distance of 325 pc, its projected physical separation is 51 AU, making it one of the growing number of wide, low-mass binaries found in young star-forming regions.

  10. MULTIDIMENSIONAL CHEMICAL MODELING OF YOUNG STELLAR OBJECTS. III. THE INFLUENCE OF GEOMETRY ON THE ABUNDANCE AND EXCITATION OF DIATOMIC HYDRIDES

    SciTech Connect (OSTI)

    Bruderer, S.; Benz, A. O.; Staeuber, P.; Doty, S. D.

    2010-09-10

    The Herschel Space Observatory enables observations in the far-infrared at high spectral and spatial resolution. A particular class of molecules will be directly observable: light diatomic hydrides and their ions (CH, OH, SH, NH, CH{sup +}, OH{sup +}, SH{sup +}, NH{sup +}). These simple constituents are important both for the chemical evolution of the region and as tracers of high-energy radiation. If outflows of a forming star erode cavities in the envelope, protostellar far-UV (FUV; 6 < E{sub {gamma}} < 13.6 eV) radiation may escape through such low-density regions. Depending on the shape of the cavity, the FUV radiation then irradiates the quiescent envelope in the walls along the outflow. The chemical composition in these outflow walls is altered by photoreactions and heating via FUV photons in a manner similar to photo-dominated regions. In this work, we study the effect of cavity shapes, outflow density, and of a disk with the two-dimensional chemical model of a high-mass young stellar object introduced in the second paper in this series. The model has been extended with a self-consistent calculation of the dust temperature and a multi-zone escape probability method for the calculation of the molecular excitation and the prediction of line fluxes. We find that the shape of the cavity is particularly important in the innermost part of the envelope, where the dust temperatures are high enough ({approx}>100 K) for water ice to evaporate. If the cavity shape allows FUV radiation to penetrate this hot-core region, the abundance of FUV-destroyed species (e.g., water) is decreased. On larger scales, the shape of the cavity is less important for the chemistry in the outflow wall. In particular, diatomic hydrides and their ions CH{sup +}, OH{sup +}, and NH{sup +} are enhanced by many orders of magnitude in the outflow walls due to the combination of high gas temperatures and rapid photodissociation of more saturated species. The enhancement of these diatomic hydrides is sufficient for a detection using the HIFI and PACS instruments on board Herschel. The effect of X-ray ionization on the chemistry is found to be small, due to the much larger luminosity in FUV bands compared to X-rays.

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

    SciTech Connect (OSTI)

    Biller, Beth A.; Ftaclas, Christ; Liu, Michael C.; Wahhaj, Zahed; Nielsen, Eric L.; Hayward, Thomas L.; Hartung, Markus; Chun, Mark; Clarke, Fraser; Thatte, Niranjan; Shkolnik, Evgenya L.; Reid, I. Neill; Boss, Alan; Lin, Douglas; Alencar, Silvia H. P.; De Gouveia Dal Pino, Elisabete; Gregorio-Hetem, Jane [Universidade de Sao Paulo, IAG and others

    2013-11-10

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

  12. Mobile Technology and Social Media in the Clinical Practice of Young Radiation Oncologists: Results of a Comprehensive Nationwide Cross-sectional Study

    SciTech Connect (OSTI)

    Bibault, Jean-Emmanuel; Leroy, Thomas; Blanchard, Pierre; Biau, Julian; Cervellera, Mathilde; Diaz, Olivia; Faivre, Jean Christophe; and others

    2014-09-01

    Purpose: Social media and mobile technology are transforming the way in which young physicians are learning and practicing medicine. The true impact of such technologies has yet to be evaluated. Methods and Materials: We performed a nationwide cross-sectional survey to better assess how young radiation oncologists used these technologies. An online survey was sent out between April 24, 2013, and June 1, 2013. All residents attending the 2013 radiation oncology French summer course were invited to complete the survey. Logistic regressions were performed to assess predictors of use of these tools in the hospital on various clinical endpoints. Results: In all, 131 of 140 (93.6%) French young radiation oncologists answered the survey. Of these individuals, 93% owned a smartphone and 32.8% owned a tablet. The majority (78.6%) of the residents owning a smartphone used it to work in their department. A total of 33.5% had more than 5 medical applications installed. Only 60.3% of the residents verified the validity of the apps that they used. In all, 82.9% of the residents had a social network account. Conclusions: Most of the residents in radiation oncology use their smartphone to work in their department for a wide variety of tasks. However, the residents do not consistently check the validity of the apps that they use. Residents also use social networks, with only a limited impact on their relationship with their patients. Overall, this study highlights the irruption and the risks of new technologies in the clinical practice and raises the question of a possible regulation of their use in the hospital.

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

    SciTech Connect (OSTI)

    Biller, Beth A.; Liu, Michael C.; Wahhaj, Zahed; Dupuy, Trent J.; Ftaclas, Christ; Nielsen, Eric L.; Close, Laird M.; Males, Jared; Skemer, Andrew; Hayward, Thomas L.; Hartung, Markus; Chun, Mark; Clarke, Fraser; Tecza, Matthias; Thatte, Niranjan; Reid, I. Neill; Shkolnik, Evgenya L.; Alencar, Silvia H. P.; Artymowicz, Pawel

    2010-09-01

    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.

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

    SciTech Connect (OSTI)

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

    2010-07-30

    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.

  15. ORISE: Beryllium Laboratory Accredited by College of American...

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

    proliferation test FOR IMMEDIATE RELEASE: Aug. 12, 2011 FY11-41 Linda Nichols performs blood test in ORISE Beryllium Lab Linda Nichols, MS, MT(ASCP) and Beryllium Lab manager,...

  16. Text-Alternative Version: Solid-State Lighting Early Lessons Learned Webinar

    Broader source: Energy.gov [DOE]

    Linda Sandahl: Welcome, ladies and gentlemen. I'm Linda Sandahl with the Pacific Northwest National Laboratory, and I'd like to welcome you to today's webcast, Solid-State Lighting: Early Lessons...

  17. Tentative Agreement.doc

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

    Keith A. Klein, Manager Linda Hoffman, Acting Director U. S. Department of Energy, Richland State of Washington, Department...

  18. Application for Presidential Permit OE Docket No. PP-371 Northern Pass

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

    Transmission: Comments from Linda Upham | Department of Energy Linda Upham Application for Presidential Permit OE Docket No. PP-371 Northern Pass Transmission: Comments from Linda Upham Application from Northern Pass Transmission to construct, operate and maintain electric transmission facilities at the U.S. - Canada Border. PDF icon LindaUpham_Pp-371 Comments.pdf More Documents & Publications Application for Presidential Permit OE Docket No. PP-371 Northern Pass Transmission: Comments

  19. Jefferson Lab Builds First Single Crystal Single Cell Accelerating...

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

    superconducting accelerator cavities, visit: http:www.jlab.orgexpprogtechtransfernewtech.htmlcavities. For more information, or to schedule an interview, contact: Linda...

  20. A SURVEY OF H{sub 2}O, CO{sub 2}, AND CO ICE FEATURES TOWARD BACKGROUND STARS AND LOW-MASS YOUNG STELLAR OBJECTS USING AKARI

    SciTech Connect (OSTI)

    Noble, J. A.; Fraser, H. J.; Aikawa, Y.; Pontoppidan, K. M.; Sakon, I.

    2013-10-01

    We present near-infrared spectroscopic observations of 19 molecular clouds made using the AKARI satellite, and the data reduction pipeline written to analyze those observations. The 2.5-5 ?m spectra of 30 objects22 field stars behind quiescent molecular clouds and 8 low-mass young stellar objects in coreswere successfully extracted using the pipeline. Those spectra are further analyzed to calculate the column densities of key solid phase molecular species, including H{sub 2}O, CO{sub 2}, CO, and OCN{sup }. The profile of the H{sub 2}O ice band is seen to vary across the objects observed and we suggest that the extended red wing may be an evolutionary indicator of both dust and ice mantle properties. The observation of 22 spectra with fluxes as low as < 5 mJy toward background stars, including 15 where the column densities of H{sub 2}O, CO, and CO{sub 2} were calculated, provides valuable data that could help to benchmark the initial conditions in star-forming regions prior to the onset of star formation.

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

    SciTech Connect (OSTI)

    Bowler, Brendan P.; Liu, Michael C.; Shkolnik, Evgenya L.; Tamura, Motohide

    2012-09-01

    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.

  2. LOW-VELOCITY SHOCKS TRACED BY EXTENDED SiO EMISSION ALONG THE W43 RIDGES: WITNESSING THE FORMATION OF YOUNG MASSIVE CLUSTERS

    SciTech Connect (OSTI)

    Nguyen-Luong, Q.; Martin, P. G.; Motte, F.; Louvet, F.; Hill, T.; Hennemann, M.; Didelon, P.; Lesaffre, P.; Gusdorf, A.; Menten, K. M.; Wyrowski, F.; Bendo, G.; Roussel, H.; Bernard, J.-P.; Bronfman, L.; and others

    2013-10-01

    The formation of high-mass stars is tightly linked to that of their parental clouds. Here, we focus on the high-density parts of W43, a molecular cloud undergoing an efficient event of star formation. Using a column density image derived from Herschel continuum maps, we identify two high-density filamentary clouds, called the W43-MM1 and W43-MM2 ridges. Both have gas masses of 2.1 10{sup 4} M{sub ?} and 3.5 10{sup 4} M{sub ?} above >10{sup 23} cm{sup -2} and within areas of ?6 and ?14 pc{sup 2}, respectively. The W43-MM1 and W43-MM2 ridges are structures that are coherent in velocity and gravitationally bound, despite their large velocity dispersion measured by the N{sub 2}H{sup +} (1-0) lines of the W43-HERO IRAM large program. Another intriguing result is that these ridges harbor widespread (?10 pc{sup 2}) bright SiO (2-1) emission, which we interpret to be the result of low-velocity shocks (?10 km s{sup 1}). We measure a significant relationship between the SiO (2-1) luminosity and velocity extent and show that it distinguishes our observations from the high-velocity shocks associated with outflows. We use state-of-the-art shock models to demonstrate that a small percentage (10%) of Si atoms in low-velocity shocks, observed initially in gas phase or in grain mantles, can explain the observed SiO column density in the W43 ridges. The spatial and velocity overlaps between the ridges of high-density gas and the shocked SiO gas suggest that ridges could be forming via colliding flows driven by gravity and accompanied by low-velocity shocks. This mechanism may be the initial conditions for the formation of young massive clusters.

  3. News Item

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

    Develop a New Nanotech Tool to Probe Solar Energy Conversion If nanoscience were television, we'd be in the 1950s. Although scientists can make and manipulate nanoscale objects...

  4. National Innovation Summit

    Broader source: Energy.gov [DOE]

    The TechConnect World Innovation Conference, in Washington, D.C.,co-locates with the largest global innovation program in physical and life sciences. The joint programs include the Nanotech 2016...

  5. CSI 2264: simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzerevidence for multiple origins of variability

    SciTech Connect (OSTI)

    Cody, Ann Marie; Stauffer, John; Rebull, Luisa M.; Carey, Sean; Baglin, Annie; Micela, Giuseppina; Flaccomio, Ettore; Morales-Caldern, Mara; Aigrain, Suzanne; Bouvier, Jrme; Gutermuth, Robert; Song, Inseok; Turner, Neal; Alencar, Silvia H. P.; Zwintz, Konstanze; Plavchan, Peter; Terebey, Susan; and others

    2014-04-01

    We present the Coordinated Synoptic Investigation of NGC 2264, a continuous 30 day multi-wavelength photometric monitoring campaign on more than 1000 young cluster members using 16 telescopes. The unprecedented combination of multi-wavelength, high-precision, high-cadence, and long-duration data opens a new window into the time domain behavior of young stellar objects. Here we provide an overview of the observations, focusing on results from Spitzer and CoRoT. The highlight of this work is detailed analysis of 162 classical T Tauri stars for which we can probe optical and mid-infrared flux variations to 1% amplitudes and sub-hour timescales. We present a morphological variability census and then use metrics of periodicity, stochasticity, and symmetry to statistically separate the light curves into seven distinct classes, which we suggest represent different physical processes and geometric effects. We provide distributions of the characteristic timescales and amplitudes and assess the fractional representation within each class. The largest category (>20%) are optical 'dippers' with discrete fading events lasting ?1-5 days. The degree of correlation between the optical and infrared light curves is positive but weak; notably, the independently assigned optical and infrared morphology classes tend to be different for the same object. Assessment of flux variation behavior with respect to (circum)stellar properties reveals correlations of variability parameters with H? emission and with effective temperature. Overall, our results point to multiple origins of young star variability, including circumstellar obscuration events, hot spots on the star and/or disk, accretion bursts, and rapid structural changes in the inner disk.

  6. Newton County, Missouri: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Acres, Missouri Diamond, Missouri Fairview, Missouri Granby, Missouri Grand Falls Plaza, Missouri Joplin, Missouri Leawood, Missouri Loma Linda, Missouri Neosho, Missouri...

  7. Federal Utility Partnership Working Group (FUPWG) Meeting Report...

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

    13 Fall 2008 Report Robert Charles National Aeronautics and Space Administration Linda Collins General Services Administration Anne Crawley Department of Energy Doug Culbreth...

  8. UEC Members attending: Nina Balke, Nazanin Bassiri-Gharb, Milan...

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

    Prabhu, Megan Robertson, Ichiro Takeuchi, Rafael Verduzco CNMS representatives: Sean Smith, Tony Haynes, Vivane Schwartz DOE Guest: Linda Horton Meeting convened approximately...

  9. Fermilab Art Gallery

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

    Linda Conlee-Johnson I have evolved from a basketry artist who wove sculptural art-vessels using traditional basketry materials to an artist experimenting with the weaving...

  10. Pre-decisional - For Discussion Purposes Only

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

    on the phone: Larry Blaufus (Clark) Van Ashton (Idaho) Brian Fawcett (Clatskanie) Jim Russell (Tacoma) Kathy Moore (Umatilla) John Walkowiak (Tacoma) Peter Meyer (Tacoma) Linda...

  11. --No Title--

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

    downloadsacq uisition-certifications-program-handbook Questions concerning this policy flash should be directed to Linda Ott of the Office of Acquisition and Project Management,...

  12. Clot Busting Simulations Test Potential Stroke Treatment

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

    Clot Busting Simulations Test Potential Stroke Treatment Clot Busting Simulations Test Potential Stroke Treatment September 24, 2013 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov ...

  13. David Skinner Named NERSC Strategic Partnerships Lead

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

    David Skinner Named NERSC Strategic Partnerships Lead David Skinner Named NERSC Strategic Partnerships Lead January 24, 2014 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov...

  14. September2015News

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

    that our visitors want to use their smart phones and tablets to share spontaneously on social media about their visit," said Linda Deck, the Bradbury's director. Omar Juveland,...

  15. MyPay Donation Information For Employees In the National Capital...

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

    4192700 Tony Carter LP Loan Programs 4193700 Linda Vawter MA Management 4191700 Ferrin Moore NA National Nuclear Security Administration 4191800 Mark Roman NE Nuclear Energy...

  16. A 200 kyr Pleistocene Lacustrine Record from the Valles Caldera...

    Open Energy Info (EERE)

    Magnetism and Paleomagnetism Authors Linda Donohoo-Hurley, John W. Geissman, Peter J. Fawcett, Tim Wawrzyniec and Fraser E. Goff Conference New Mexico Geological Society...

  17. Lighting Energy Efficiency in Parking Campaign

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

    Lighting Energy Efficiency in Parking (LEEP) Campaign Linda Sandahl Pacific Northwest ... Objectives: Problem Statement While new lighting technologies such as LEDs have the ...

  18. Bill Wilcox, part 3 | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  19. Patrick Case | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  20. Alice Piercey | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  1. Bill Wilcox, part 1 | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  2. Bill Wilcox, part 2 | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  3. Oral History Videos | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  4. Blake Case | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  5. Wilma Brooks | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  6. Beverly Woods | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  7. Willard Brock | Y-12 National Security Complex

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

    Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice...

  8. lenyeart | The Ames Laboratory

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

    lenyeart Ames Laboratory Profile Linda Enyeart Chemical & Biological Sciences 144 Spedding Phone Number: 515-294-6063 Email Address: lenyeart@ameslab.gov

  9. Martin Karplus Wins Nobel Prize in Chemistry

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

    Home News & Publications NERSC News Center News Martin Karplus Wins Nobel Prize in Chemistry Martin Karplus Wins Nobel Prize in Chemistry October 9, 2013 Contact: Linda...

  10. Policy Flash 2013-54 Acquisition Certification Program Handbook...

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

    Acquisition Certifications Program Handbook 4th Edition Questions concerning this policy flash should be directed to Linda Ott of the Office Acquistion and Project Management,...

  11. HAZMAT Challenge gives regional emergency responders safe, realistic...

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

    improve their skills Simulated disasters give responders an opportunity to improve their skills Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda...

  12. New research, publications and videos

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

    Linda Anderman Email News stories Medical and biofuel advances possible with new gene ... RNA molecule that could have value for medical and even biofuel production purposes. ...

  13. Taming Plasma Fusion Snakes

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

    Image credit: Linda Sugiyama Controlled nuclear fusion has held the promise of a safe, clean, sustainable energy resource for decades. Now, with concerns over global climate change ...

  14. PowerPoint Presentation

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

    Organized by Education Program: J. Michael Doster, Sherry Bailey, Rose Montgomery, John Turner, and Linda Weltman 27 graduate students representing 9 universities 11...

  15. ORISE: College of American Pathologists renews accreditation...

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

    skilled team, led by our lab manager Linda Nichols, delivers the highest level of quality and meticulous attention that our customers have come to expect from this facility."...

  16. Energy Literacy

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

    Biomass 2014 Conference Energy Literacy Linda Silverman Education and Workforce Development Department of Energy July 30, 2014 2 | Energy Education and Workforce Development ...

  17. America's Home Energy Education Challenge: Teaching Kids to Save...

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

    The deadline to register for the Home Energy Education Challenge is November 15. Linda Silverman Senior Advisor, Tech-to-Market Office Daniel Boff Intern, Office of Energy ...

  18. Slide 1

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

    (NE) Michael Worley Office of Energy Efficiency & Renewable Energy (EERE) Linda Silverman Office of Fossil Energy (FE) Bob Wright National Nuclear Security Administration ...

  19. --No Title--

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

    Wednesday, November 4, 2009 2:00 pm Conference Center, 5200 (202-B) "Discrete Stochastic Simulation of Spatially Inhomogeneous Biochemical Systems" Linda Petzold University of...

  20. Text-Alternative Version: Better than CFL? Dimmable LED Downlights in Hospitality Facilities Webinar

    Broader source: Energy.gov [DOE]

    Linda Sandahl: First, I’m very happy to welcome our speakers: Bob Davis of Pacific Northwest National Laboratory and Ardra Zinkon of Tec Studio.

  1. A classification scheme for young stellar objects using the wide-field infrared survey explorer AllWISE catalog: revealing low-density star formation in the outer galaxy

    SciTech Connect (OSTI)

    Koenig, X. P.; Leisawitz, D. T.

    2014-08-20

    We present an assessment of the performance of WISE and the AllWISE data release for a section of the Galactic Plane. We lay out an approach to increasing the reliability of point-source photometry extracted from the AllWISE catalog in Galactic Plane regions using parameters provided in the catalog. We use the resulting catalog to construct a new, revised young star detection and classification scheme combining WISE and 2MASS near- and mid-infrared colors and magnitudes and test it in a section of the outer Milky Way. The clustering properties of the candidate Class I and II stars using a nearest neighbor density calculation and the two-point correlation function suggest that the majority of stars do form in massive star-forming regions, and any isolated mode of star formation is at most a small fraction of the total star forming output of the Galaxy. We also show that the isolated component may be very small and could represent the tail end of a single mechanism of star formation in line with models of molecular cloud collapse with supersonic turbulence and not a separate mode all to itself.

  2. QER- Comment of Allen Young 2

    Broader source: Energy.gov [DOE]

    Here is a comment from me on the issue of energy infrastructure in Massachusetts. I will address only one issue: the proposed Kinder Morgan pipelines from Albany to Dracut. I am absolutely opposed to the construction of this pipeline and here are my reasons

  3. Nurturing young children's curiosity about the universe

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

    ... For Ortega, early literacy, including early STEM literacy, is a logical place to start in attempting to reverse New Mexico's poverty statistics and educational challenges. Citing ...

  4. Light-Material Interactions in Energy Conversion - Energy Frontier Research

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

    Center (LMI-EFRC) Cambridge Nanotech Atomic Layer Deposition A Cambridge Nanotech (USA) Savannah S200 atomic layer deposition (ALD) system was purchased for conformal growth of metal oxide films. ALD is the growth of films by sequential, self-limiting, surface chemical reactions and thus allows for precise thickness control. This system is capable of depositing nearly any metal oxide (e.g., TiO2, Al2O3) and is upgradable for metal sulfide deposition. This tool is housed in N. Lewis

  5. PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS

    SciTech Connect (OSTI)

    Mamajek, Eric E.; Quillen, Alice C.; Pecaut, Mark J.; Moolekamp, Fred; Scott, Erin L.; Kenworthy, Matthew A.; Cameron, Andrew Collier; Parley, Neil R.

    2012-03-15

    The large relative sizes of circumstellar and circumplanetary disks imply that they might be seen in eclipse in stellar light curves. We estimate that a survey of {approx}10{sup 4} young ({approx}10 million year old) post-accretion pre-main-sequence stars monitored for {approx}10 years should yield at least a few deep eclipses from circumplanetary disks and disks surrounding low-mass companion stars. We present photometric and spectroscopic data for a pre-main-sequence K5 star (1SWASP J140747.93-394542.6 = ASAS J140748-3945.7), a newly discovered {approx}0.9 M{sub Sun} member of the {approx}16 Myr old Upper Centaurus-Lupus subgroup of Sco-Cen at a kinematic distance of 128 {+-} 13 pc. This star exhibited a remarkably long, deep, and complex eclipse event centered on 2007 April 29 (as discovered in Super Wide Angle Search for Planets (SuperWASP) photometry, and with portions of the dimming confirmed by All Sky Automated Survey (ASAS) data). At least five multi-day dimming events of >0.5 mag are identified, with a >3.3 mag deep eclipse bracketed by two pairs of {approx}1 mag eclipses symmetrically occurring {+-}12 days and {+-}26 days before and after. Hence, significant dimming of the star was taking place on and off over at least a {approx}54 day period in 2007, and a strong >1 mag dimming event occurring over a {approx}12 day span. We place a firm lower limit on the period of 850 days (i.e., the orbital radius of the eclipser must be >1.7 AU and orbital velocity must be <22 km s{sup -1}). The shape of the light curve is similar to the lopsided eclipses of the Be star EE Cep. We suspect that this new star is being eclipsed by a low-mass object orbited by a dense inner disk, further girded by at least three dusty rings of optical depths near unity. Between these rings are at least two annuli of near-zero optical depth (i.e., gaps), possibly cleared out by planets or moons, depending on the nature of the secondary. For possible periods in the range 2.33-200 yr, the estimated total ring mass is {approx}8-0.4 M{sub Moon} (if the rings have optical opacity similar to Saturn's rings), and the edge of the outermost detected ring has orbital radius {approx}0.4-0.09 AU. In the new era of time-domain astronomy opened by surveys like SuperWASP, ASAS, etc., and soon to be revolutionized by Large Synoptic Survey Telescope, discovering and characterizing eclipses by circumplanetary and circumsecondary disks will provide us with observational constraints on the conditions that spawn satellite systems around gas giant planets and planetary systems around stars.

  6. Predicting the future could win a $1,000 California or Illinois...

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

    to post the answer to this question on their blog or website: "Where do you see the Internet in 10 years?" September 1, 2012 dummy image Read our archives Contacts Editor Linda...

  7. Disordered Materials Hold Promise for Better Batteries

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

    Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov disorderedMAT.jpg Conventional layered lithium and transition metal cathode material (top) and the new disordered material studied...

  8. New Computer Codes Unlock the Secrets of Cleaner Burning Coal

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

    New Computer Codes Unlock the Secrets of Cleaner Burning Coal New Computer Codes Unlock the Secrets of Cleaner Burning Coal March 29, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 ...

  9. Energy Efficiency Post-2011 Review Workgroup 1 Meeting Notes

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

    P Linda Esparza, Franklin PUD, P Tom Schumacher, Benton PUD, P Jim Russell, Tacoma, P John Walkowiak, Tacoma, P Tom Karier, NWPCC, P Mike Little, SCL, P Ryan Neal, WAPAG, P...

  10. Technical Meeting on the Software Framework for Transactive Energy...

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

    ... Linda has authored papers for technical journals, is a senior member of IEEE, and holds ... is intended to be used by researchers to explore and refine transactive control concepts. ...

  11. Manhattan Project National Historical Park Open House Event

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

    National Historical Park Open House Event WHEN: Jun 02, 2015 5:00 PM - 7:00 PM WHERE: Fuller Lodge 2132 Central Avenue, Los Alamos, New Mexico, 87544 USA CONTACT: Linda Deck 505...

  12. Text-Alternative Version: Webcast of the Renewable Energy Competency Model: An Aid to Build a Renewable Energy Skilled Workforce

    Broader source: Energy.gov [DOE]

    This is the Webcast of Renewable Energy and Competency model. Led by Linda Silverman an economist at Energy Efficiency and Renewable Energy and Pam Frugoli Department of Labor. This webcast was on...

  13. Funding: Future Clean Cities Solicitation and EISA Section 244

    Broader source: Energy.gov [DOE]

    At the November 6, 2008 joint Web conference of DOE's Biomass and Clean Cities programs, Linda Bluestein (U.S. Department of Energy, Clean Cities Program) described EISA 2007, Section 244 Renewable Fuel Infrastructure Grants.

  14. The Path a Proton Takes Through a Fuel Cell Membrane

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

    The Path a Proton Takes Through a Fuel Cell Membrane The Path a Proton Takes Through a Fuel Cell Membrane October 11, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Ram.jpg The cover...

  15. Welcome to the First Issue of AlumniLink

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

    Welcome to the First Issue of AlumniLink A personal message from Lab Director Charlie McMillan June 20, 2014 First Issue of AlumniLink First Issue of AlumniLink Contact Linda...

  16. OpenMSI: A Science Gateway to Sort Through Bio-Imaging's Big...

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

    OpenMSI: A Science Gateway to Sort Through Bio-Imaging's Big Datasets OpenMSI: A Science Gateway to Sort Through Bio-Imaging's Big Datasets August 27, 2013 Contact: Linda Vu, +1...

  17. Graded Interface Models for more accurate Determination of van...

    Office of Scientific and Technical Information (OSTI)

    length scale property variations. Authors: van Benthem, Klaus 1 ; Tan, Guolong 2 ; French, Roger H 3 ; DeNoyer, Linda K 4 ; Podgornik, Rudolf 5 ; Parsegian, V Adrian 5...

  18. Y-12 donates DVDs, teddy bears to Children's Hospital | Y-12...

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    Y-12 donates DVDs, teddy ... Y-12 donates DVDs, teddy bears to Children's Hospital Posted: January 24, 2014 - 3:33pm Pictured from left to right: Y-12ers Karen Dixon, Linda...

  19. Protecting Lab land and the creatures that inhabit it

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    April 1, 2013 View of Sangre de Christo mauntains from overlook on NM502 Mexican Spotted Owls live on Lab property. Contact Editor Linda Anderman Email Community Programs Office...

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    Dr. Doug Kothe, Dr. paul Turinsky, Dr. John Turner, and Mrs. Linda Weltman. Dr. John Turner gave a brief overview about the goals of VERA. He discussed VERA informing the...

  1. CX-008895: Categorical Exclusion Determination

    Office of Energy Efficiency and Renewable Energy (EERE)

    California-City-Yorba Linda CX(s) Applied: B2.5, B5.1 Date: 08/14/2012 Location(s): California Offices(s): Energy Efficiency and Renewable Energy

  2. Researchers Discover a New Kind of Neutrino Transformation

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    March 8, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Daya Bay Neutrino Facility in China. Photo by: Roy Kaltschmidt, Lawrence Berkeley National Laboratory. Neutrinos, the...

  3. San Patricio County, Texas: Energy Resources | Open Energy Information

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    A. Places in San Patricio County, Texas Aransas Pass, Texas Corpus Christi, Texas Del Sol-Loma Linda, Texas Doyle, Texas Edgewater-Paisano, Texas Edroy, Texas Falman-County...

  4. Discovery of a ternary pseudobrookite phase in the earth-abundant...

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    Title: Discovery of a ternary pseudobrookite phase in the earth-abundant TiZnO system Authors: Perry, Nicola H. ; Stevanovic, Vladan ; Lime, Linda Y. ; Mason, Thomas O. 1 ; CSM) ...

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    Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy O P Q R S T U V W X Y Z Narevicius, Edvardas (Edvardas Narevicius) - Department of Chemical Physics, Weizmann Institute of Science Nazar, Linda F. (Linda F. Nazar) - Department of Chemistry, University of Waterloo Nazarenko, Alexander (Alexander Nazarenko) - Department of Chemistry, Buffalo State College Nelson, Peter Hugo (Peter Hugo Nelson) -

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    Procurement | Department of Energy Technology Transfer and Procurement Contacts for the Assistant General Counsel for Technology Transfer and Procurement Subject Matter/Functional Area Lead Backup Technology Transfer John T. Lucas 202-586-2939 Linda Field 202-586-3440 IP Policy John T. Lucas 202-586-2939 Linda Field 202-586-3440 Litigation Administrative Claims Copyrights/Software Nathaniel Sloan 202-586-4792 Marianne Lynch 202-586-3815 Acquisition/Assistance IP Rights International

  7. Volttron (TM) Transactive Control Node: Case Study

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    TM Transactive Control Node: Case Study Linda Rankin (linda.j.rankin@gmail.com) Node Contributors: Chris Freeman (chris.freeman.pdx@gmail.com) Glen Cooper (gcooper@qualitylogic.com) VOLLTRON Technical Meeting, July 2015 Transactive Control (TC) * A unique distributed control and communication system demonstrated by the Pacific Northwest Smart Grid Demonstration Project (PNW-SGDP) - www.pnwsmartgrid.org * Localized power generation/load decisions enabled by - Distribution of predicted cost and

  8. Citizen Potawatomi Nation - Fire Lake Geothermal Heat Pump Project

    Office of Environmental Management (EM)

    John A. Barrett - Chairman Linda Capps - Vice Chairman D. Wayne Trousdale - Secretary/Treasurer Tribal Leadership John A. Barrett Chairman Linda Capps Vice Chairman D. Wayne Trousdale Secretary/Treasurer Located in Shawnee, Oklahoma * Citizen Potawatomi purchased allotment lands consisting of a small 900 square mile parcel * The largest part of the Potawatomi made their way to the new reservation in the 1880s. Humble Beginnings CPN Headquarters The Tribal Administration Building houses: The

  9. STICKY FINGERS: How One Researcher is Improving the Science of Fingerprints

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

    | Department of Energy STICKY FINGERS: How One Researcher is Improving the Science of Fingerprints STICKY FINGERS: How One Researcher is Improving the Science of Fingerprints May 1, 2015 - 3:42pm Addthis Linda Lewis takes a materials science approach to forensics research at Oak Ridge National Laboratory. | Photo courtesy of Oak Ridge National Laboratory. Linda Lewis takes a materials science approach to forensics research at Oak Ridge National Laboratory. | Photo courtesy of Oak Ridge

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  8. National Laboratory]; Kim, Young Jin [Los Alamos National Laboratory...

    Office of Scientific and Technical Information (OSTI)

    EDM Abstract Not Provided Los Alamos National Laboratory (LANL) DOELANL United States 2014-11-05 English Conference Conference: Challenges of the worldwide experimental search...

  9. A young person's view of the Superconducting Super Collider

    SciTech Connect (OSTI)

    Moya, A.

    1990-08-01

    This report gives a simple description of the Superconducting Super Collider, how it works, and what it is used for. (LSP)

  10. Thomas Edison's Legacy for Young Engineers | GE Global Research

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

    Thomas Edison's Legacy: In the Eyes of an Edison Engineer Click to email this to a friend (Opens in new window) Share on Facebook (Opens in new window) Click to share (Opens in new window) Click to share on LinkedIn (Opens in new window) Click to share on Tumblr (Opens in new window) Thomas Edison's Legacy: In the Eyes of an Edison Engineer Kimberly Hammer 2016.02.12 Yesterday would have been Thomas Edison's 169th Birthday. In honor of his birthday, February 11 is also known as National

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

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

    in science, and in particular, my interest in physics, came only when I was in middle school. I had a fantastic science teacher who handpicked me to participate in a science...

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

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

    ... She attended Instituto Tecnologico Buenos Aires, Buenos Aires, Argentina, and the Instituto Balseiro, earning a diploma in physics; as well as San Carlos de Bariloche, Argentina, ...

  13. Progress in Understanding Iron Peak Elements in Young Supernova...

    Office of Scientific and Technical Information (OSTI)

    Relation: Conference: AtomDB Work Week and Workshop 2013 ; 2013-08-19 - 2013-08-23 ; Cambridge, Massachusetts, United States Research Org: Los Alamos National Laboratory (LANL)...

  14. Calling all Young Entrepreneurs: Deadline for Energy Department...

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

    ... NORTHEAST REGION: Massachusetts Institute of Technology's MIT Clean Energy Prize (Cambridge, MA); Deadline: March 2, 2012 WESTERN REGION: California Institute of Technology's ...

  15. Progress in Understanding Iron Peak Elements in Young Supernova...

    Office of Scientific and Technical Information (OSTI)

    Los Alamos National Laboratory Rutgers Univeristy University of Pittspurgh Harvard-Smithsonian Center for Astrophysics Publication Date: 2013-09-13 OSTI Identifier: 1093345 Report ...

  16. STEM Mentoring Caf- Engaging Young Women in an Authentic Mentoring...

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

    role in choosing a career path. In addition, the more students identify with same-sex experts the more likely they will be to pursue a STEM career. So not only did the STEM...

  17. Structure and Stratigraphy Beneath a Young Phreatic Vent: South...

    Open Energy Info (EERE)

    deformation. Authors John C. Eichelberger, Thomas A. Vogel, Leland W. Younker, C. Dan Miller, Grant H. Heiken and Kenneth H. Wohletz Published Journal Journal of Geophysical...

  18. W. C. Young and D. J. Den Hartog

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    only a single time. FIG. 1. An overview of the laser components (disregarding additional mir- rors). The first amplifier uses a double pass via a quarterwave plate and polarization...

  19. Penetration equations Young, C.W. [Applied Research Associates...

    Office of Scientific and Technical Information (OSTI)

    45 MILITARY TECHNOLOGY, WEAPONRY, AND NATIONAL DEFENSE; EARTH PENETRATORS; EQUATIONS; NUCLEAR WEAPONS; SOILS; ICE; ROCKS; CONCRETES; PERMAFROST; SCALING LAWS In 1967, Sandia...

  20. EA-1974: Wallooskee-Youngs Confluence Restoration Project; Clatsop...

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

    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 ...

  1. Young scientist discovers magnetic material unnecessary to create...

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    implications for the field of spintronics and the development of high-speed, ... spin based computing (spintronics), and is also an area of great fundamental interest. ...

  2. Conference for young women aims to encourage pursuit of science...

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    Angela Hardin at (630) 252-5501 or media@anl.gov. Connect Find an Argonne expert by subject. Follow Argonne on Twitter, Facebook, Google+ and LinkedIn. For inquiries on...

  3. Quarterly Progress Report for the Young-Rainey STAR Center's...

    Office of Legacy Management (LM)

    ... The STAR Center, while owned by DOE, primarily manufactured neutron generators for nuclear weapons. Other products manufactured at the STAR Center have included ...

  4. CAMD Nanofabrication Links

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    Research :: Publications :: Infrastructure :: Links :: Nanofabrication Facility in News Nano 50TM Awards: The Nano 50TM Awards, presented by Nanotech Briefs magazine, recognize the top 50 technologies, products and innovators that have significantly impacted, or are expected to impact, the state of the art in nanotechnology. "The winners of the Nano 50 awards are the best of the best - the innovative people and technologies that will continue to move nanotechnology to key mainstream

  5. Contribution to Nanotechnology Manufacturing

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    shares Nano 50 award for directed assembly September 3, 2008 Contribution to Nanotechnology Manufacturing LOS ALAMOS, New Mexico, September 3, 2008-A team of scientists spanning three institutions, including Los Alamos National Laboratory, has discovered a more efficient way of fusing charge-carrying electrical contacts to tiny "nanowires" of silicon to create the nanotechnology at the heart of potential future advances in modern electronics, sensing, and energy collection. Nanotech

  6. CAMD Nanofabrication

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    Research :: Publications :: Infrastructure :: News :: Links :: The emerging fields of nanoscience and nanoengineering are leading to unprecedented understanding and control over the fundamental building blocks of all physical things. This is likely to change the way almost everything—from vaccines to computers to automobile tires to objects not yet imagined—is designed and made. It is anticipated that a new world of industrial products valued at $1trillion/yr and, at least, 2 million nanotech

  7. Light-Material Interactions in Energy Conversion - Energy Frontier Research

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    Center (LMI-EFRC) Facilities Facilities, Capabilities, and Techniques of the LMI-EFRC These are available for use by all LMI researchers At Caltech Large-area vapor-liquid-solid microwire growth Cambridge Nanotech Atomic Layer Deposition Integrating sphere Ultrafast Pump-Probe System At LBL Nanocrystal synthesis Photoelectrochemical etching At UIUC Proximity field nano-patterning Direct ink writing Malvern Nano Zetasizer AJA e-beam evaporator DOE Center facilities National Energy Research

  8. Sustainable Nanomaterials from Forest Products: Umaine Perspective

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

    from Forest Products: Umaine Perspective Douglas Gardner, PhD. Advanced Structures & Composite Center Forest Bioproducts Research Institute School of Forest Resources, University of Maine Ligno-Cellulose: Maine's Niche to Compete in Nanotech Stone Age ....... Bronze Age .......... Iron Age ................ Nano Age? "From the Sawmill to the Nanomill?" Overarching Research Focus "Establish world-class R&D capacity in the field of ligno-cellulose derived nanomaterials

  9. APS Science 2009.

    SciTech Connect (OSTI)

    Gibson, J. M; Mills, D. M.; Gerig, R.

    2010-05-01

    It is my pleasure to introduce the 2009 annual report of the Advanced Photon Source. This was a very good year for us. We operated with high reliability and availability, despite growing problems with obsolete systems, and our users produced a record output of publications. The number of user experiments increased by 14% from 2008 to more than 3600. We congratulate the recipients of the 2009 Nobel Prize in Chemistry-Venkatraman Ramakrishnan (Cambridge Institute for Medical Research), Thomas Steitz (Yale University), and Ada Yonath (Weizmann Institute) - who did a substantial amount of this work at APS beamlines. Thanks to the efforts of our users and staff, and the ongoing counsel of the APS Scientific Advisory Committee, we made major progress in advancing our planning for the upgrade of the APS (APS-U), producing a proposal that was positively reviewed. We hope to get formal approval in 2010 to begin the upgrade. With advocacy from our users and the support of our sponsor, the Office of Basic Energy Sciences in the Department of Energy (DOE) Office of Science, our operating budgets have grown to the level needed to more adequately staff our beamlines. We were also extremely fortunate to have received $7.9 M in American Recovery and Reinvestment Act ('stimulus') funding to acquire new detectors and improve several of our beamlines. The success of the new Linac Coherent Light Source at Stanford, the world's first x-ray free-electron laser, made us particularly proud since the undulators were designed and built by the APS. Among other highlights, we note that more than one-quarter of the 46 Energy Frontier Research Centers, funded competitively across the U.S. in 2009 by the DOE, included the Advanced Photon Source in their proposed work, which shows that synchrotron radiation, and the APS in particular, are central to energy research. While APS research covers everything from fundamental to applied science (reflected by the highlights in this report), the challenge of sustainable energy provides an opportunity for expanded involvement with industrial research. We were privileged to recruit several outstanding new leaders at the APS. Linda Young, from Argonne's Chemical Sciences Division, became the new Director of the X-ray Science Division (XSD). Chris Jacobsen (from Stony Brook University) has been added to Linda's team as an XSD Associate Division Director, joining George Srajer. Alexander (Sasha) Zholents (formerly of Berkeley Lab) became Director of the Accelerator Systems Division. Sasha is the inventor of the short-pulse x-ray scheme that we plan to implement in the APS-U to obtain very high average brightness, broadband, 1-ps x-ray pulses. Walter Lowe (formerly of Howard University) has taken a new position as senior advisor for outreach and development of the user community. Walter's role is to increase the diversity of the user community (with diversity read broadly to include users, institutions, and technical disciplines that are underrepresented at APS). Walter is also leading an effort to increase access for industrial users. I am confident that we have in place a great team to help our users and the APS take fullest advantage of the APS-U opportunity. In planning with users for the proposed APS-U, we focused on the need to study 'real materials under real conditions in real time' on spatial and temporal scales unavailable today. Only by studying materials as they are made-or as they perform-in difficult environments can we solve the grand challenge of higher-performance, sustainable materials for energy and health. The proposed APS-U will improve the brightness of penetrating x-rays produced by the APS over 100 times, and support our efforts in developing state-of-the-art instruments to address these challenges.

  10. 7-9-draft3.indd

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

    Administration, like: Mike Deihl Administrator Tulsa, Oklahoma Special thanks to: Ladell Butts Scott Carpenter Dallas Cooper Linda Dunham Ruben Garcia Tom Green Janet Hagar Gregg Happle William Hiller Sean Long Stan Mason Linda Mummey Beth Nielsen Fritha Ohlson George Robbins Dave Sargent Aiden Smith Jane Thomas Mistie Yost U P D AT E S O U T H W E S T E R N P O W E R A D M I N I S T R A T I O N J U LY - S E P T E M B E R 2 0 0 7 Hilltop Helps Ease Transmission Woes The electricity is flowing a

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

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

    | Department of Energy Flash 2013-54 Acquisition Certification Program Handbook 4th Edition Policy Flash 2013-54 Acquisition Certification Program Handbook 4th Edition Acquisition Certifications Program Handbook 4th Edition 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. PDF icon Policy Flash 2013-54 ACMP Handbook 4th Edition.pdf More

  12. MAY 20, 2008 MEETING OF THE ELECTRICITY ADVISORY COMMITTEE | Department of

    Energy Savers [EERE]

    Energy MAY 20, 2008 MEETING OF THE ELECTRICITY ADVISORY COMMITTEE MAY 20, 2008 MEETING OF THE ELECTRICITY ADVISORY COMMITTEE From Left to Right: The Honorable Mark Whitenton; The Honorable Kevin Kolevar, Chair; Linda Stuntz From Left to Right: The Honorable Mark Whitenton; The Honorable Kevin Kolevar, Chair; Linda Stuntz DATE Tuesday, May 20, 2008, 8:30 a.m. - 12:30 p.m. LOCATION Sheraton National Hotel 900 South Orme Street Arlington, Virginia 22204 OVERVIEW The Department of Energy's

  13. Browse by Discipline -- E-print Network Subject Pathways: Biotechnology --

    Office of Scientific and Technical Information (OSTI)

    Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy L M N O P Q R S T U V W X Y Z Kaduk, Joerg (Joerg Kaduk) - Department of Geography, University of Leicester Kah, Linda (Linda Kah) - Department of Earth and Planetary Sciences, University of Tennessee Kahl, Jonathan D. W. (Jonathan D. W. Kahl) - Department of Mathematical Sciences, University of Wisconsin-Milwaukee Kalinichev, Andrey G. (Andrey

  14. Women @ Energy: Persis Drell | Department of Energy

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

    Persis Drell Women @ Energy: Persis Drell March 12, 2013 - 10:43am Addthis Persis Drell, SLAC. Photo Credit: Linda A. Cicero Stanford News Service Persis Drell, SLAC. Photo Credit: Linda A. Cicero Stanford News Service Persis S. Drell is Professor and Director Emerita at SLAC. She received her B.A. in mathematics and physics from Wellesley College in 1977. She received her Ph.D. in atomic physics from the University of California, Berkeley, in 1983. She then switched to high-energy experimental

  15. Slide 1

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    the end of delithiation Linda Y. Lim et. al., submitted to Chem. Mater. BL 11-3: Watching Batteries In-operando 2 mm 2 mm 2 mm 2 mm 2 mm 0.4 mms 1.6 mms 2.8 mms 4 mms 8 mms...

  16. Educational Opportunities in Bioenergy - NREL

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

    Education Overview Presenter: Linda Lung Date: April 23, 2012 NREL Education Programs Education Mission: Help ensure that DOE, NREL and the Nation have a sustained pipeline of highly trained science, technology, engineering and mathematics (STEM) workers. Education Priorities: * Energizing students through programs and engineering competitions. * Developing the next generation of scientists through undergraduate research experiences * Renewing teacher skills and connecting NREL to classrooms

  17. Calendar

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    Calendar Events Calendar All events at the Museum, as well as the Museum admission are free of charge. Check our calendar for an array of informative lectures, film screenings, community events and educational programs. Select a Category Clear Selection Bradbury Community Environment Holiday Science Contact Marketing & Special Projects Linda Anderman Email Event Lists Bradbury Science Museum Community Environment Science

  18. BPA-2010-01030-FOIA Response

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    503-230-4295 Mark Hadley 208-612-3170 Bonnie Hage 503-230-5104 Brent Hagen 360-418-2189 Nancy Hagen 503-230-3990 Linda Hagensen 360-619-6795 John Hahn 360-619-6257 Mary Haight...

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

    Name Title Organization Chen-Ching Liu Professor of Electrical Engineering Washington State University Ralph Maesiello Executive Advisor DNV- GL Dmitri Kosterev Principle Engineer Bonneville Power Administration Jim Thorpe Professor Cornell University Mark McGranaghan Professor EPRI Robin Podmore President Incremental Systems Eileen Buzzelli Director, Technology Management FirstEnergy Linda Nozick Cornell University Dave Alderson Professor Naval Postgraduate School Anders Johnson Director,

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    National Nuclear Security Administration (NNSA)

    Warner, 2004, has been identified as being a copyrighted material. As a general matter, copyright infringement would occur if this copyrighted work is reproduced, distributed, publically displayed without the copyright owner's permission. To obtain specific information regarding this reference, please contact Linda Cohn, EIS Document Manager for National Nuclear Security Administratio

  1. Nanofabrication

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    Facility The emerging fields of nanoscience and nanoengineering are leading to unprecedented understanding and control over the fundamental building blocks of all physical things. This is likely to change the way almost everything-from vaccines to computers to automobile tires to objects not yet imagined-is designed and made. It is anticipated that a new world of industrial products valued at $1trillion/yr and, at least, 2 million nanotech workers would emerge in 10-15yrs. In order to be part of

  2. Variable accretion processes in the young binary-star system UY Aur

    SciTech Connect (OSTI)

    Stone, Jordan M.; Eisner, J. A.; Kulesa, Craig; McCarthy, Don; Salyk, Colette E-mail: jeisner@as.arizona.edu E-mail: dmccarthy@as.arizona.edu

    2014-09-01

    We present new K-band spectroscopy of the UY Aur binary star system. Our data are the first to show H{sub 2} emission in the spectrum of UY Aur A and the first to spectrally resolve the Br? line in the spectrum of UY Aur B. We see an increase in the strength of the Br? line in UY Aur A and a decrease in Br? and H{sub 2} line luminosity for UY Aur B compared to previous studies. Converting Br? line luminosity to accretion rate, we infer that the accretion rate onto UY Aur A has increased by 2 10{sup 9} M {sub ?} yr{sup 1} per year since a rate of zero was observed in 1994. The Br? line strength for UY Aur B has decreased by a factor of 0.54 since 1994, but the K-band flux has increased by 0.9 mag since 1998. The veiling of UY Aur B has also increased significantly. These data evince a much more luminous disk around UY Aur B. If the lower Br? luminosity observed in the spectrum of UY Aur B indicates an intrinsically smaller accretion rate onto the star, then UY Aur A now accretes at a higher rate than UY Aur B. However, extinction at small radii or mass pile-up in the circumstellar disk could explain decreased Br? emission around UY Aur B even when the disk luminosity implies an increased accretion rate. In addition to our scientific results for the UY Aur system, we discuss a dedicated pipeline we have developed for the reduction of echelle-mode data from the ARIES spectrograph.

  3. THE NEAR-ULTRAVIOLET LUMINOSITY FUNCTION OF YOUNG, EARLY M-TYPE DWARF STARS

    SciTech Connect (OSTI)

    Ansdell, Megan; Baranec, Christoph; Gaidos, Eric; Mann, Andrew W.; Lpine, Sebastien; James, David; Buccino, Andrea; Mauas, Pablo; Petrucci, Romina; Law, Nicholas M.; Riddle, Reed

    2015-01-01

    Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magnetohydrodynamic dynamos during stellar youth. Near-ultraviolet (NUV) irradiation can erode and alter the chemistry of planetary atmospheres, and a quantitative description of the evolution of NUV emission from M dwarfs is needed when modeling these effects. We investigated the NUV luminosity evolution of early M-type dwarfs by cross-correlating the Lpine and Gaidos catalog of bright M dwarfs with the Galaxy Evolution Explorer (GALEX) catalog of NUV (1771-2831 ) sources. Of the 4805 sources with GALEX counterparts, 797 have NUV emission significantly (>2.5?) in excess of an empirical basal level. We inspected these candidate active stars using visible-wavelength spectra, high-resolution adaptive optics imaging, time-series photometry, and literature searches to identify cases where the elevated NUV emission is due to unresolved background sources or stellar companions; we estimated the overall occurrence of these ''false positives'' (FPs) as ?16%. We constructed an NUV luminosity function that accounted for FPs, detection biases of the source catalogs, and GALEX upper limits. We found the NUV luminosity function to be inconsistent with predictions from a constant star-formation rate and simplified age-activity relation defined by a two-parameter power law.

  4. 238U Decay Series Systematics Of Young Lavas From Batur Volcano...

    Open Energy Info (EERE)

    or post-eruptive condensation of volatile Pb salts in vesicles. Authors K. H. Rubin, G. E. Wheller, M. O. Tanzer, J. D. MacDougall, R. Varne and R. Finkel Published...

  5. STEM Mentoring Café- Engaging Young Women in an Authentic Mentoring...

    Energy Savers [EERE]

    It is a well-known fact: The percentage of women in science, technology, engineering and math (STEM) disciplines and careers is disproportionate to the amount of men in those same ...

  6. Health status of young children with cancer following discontinuation of therapy

    SciTech Connect (OSTI)

    Pastore, G.; Zurlo, M.G.; Acquaviva, A.; Calculli, G.; Castello, M.; Ceci, A.; Di Tullio, M.L.; Gandus, S.; Macchia, P.; Di Montezemolo, L.C.

    1987-01-01

    This paper reports late effects and health status of 198 children who had cancer or leukemia diagnosed under 2 years of age and their therapies electively withdrawn. This series (92 neuroblastoma (NBL), 57 Wilms' tumor (WT), 46 acute lymphoblastic leukemia (ALL), and 3 non-Hodgkin's lymphoma) was followed for 1-12 years after discontinuation of therapy. Thirty-three children were diagnosed before 1973, 92 between 1973 and 1977, and 73 after 1977 in 16 Italian Pediatric Oncology Centers. As of December 1983, 176 children were reported to be alive and without evidence of primary cancer by physicians responsible for their care. One child died from a second primary tumor, two from late recurrences of the primary cancer, and three from other causes; eight were alive with evidence of primary cancer; and eight were lost to follow-up. Kyphoscoliosis was found in 22 children and other musculoskeletal anomalies in 8. Neurological sequelae were observed in 8 of 35 children with ALL treated with radiotherapy (RT) and intrathecal methotrexate. All but one were in continuous complete remission when they developed seizures (three cases), leukoencephalopathy (three cases), or intracerebral calcifications (two cases). One child had cardiomyopathy and subsequently died from cardiac failure: he had received doxorubicin (400 mg/m2) and mediastinal RT (13 Gy) for NBL. Growth impairments were observed in children with NBL and WT.

  7. The 2015 Conference for Young Women in STEM is a smashing succes...

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

    toured cutting edge labs around campus, while others sat-in on an awe-inspiring neurology lecture and chatted with a panel of female scientists discussing their career paths....

  8. DOSFAC2 user`s guide Young, M.L.; Chanin, D. 56 BIOLOGY AND MEDICINE...

    Office of Scientific and Technical Information (OSTI)

    and (3) a users guide. 20 refs., 5 tabs. INIS; OSTI as TI97008490 Nuclear Regulatory Commission, Washington, DC (United States). Div. of Systems Technology; Sandia...

  9. Extra-nuclear starbursts: young luminous Hinge clumps in interacting galaxies

    SciTech Connect (OSTI)

    Smith, Beverly J.; Giroux, Mark L.; Soria, Roberto; Struck, Curtis; Swartz, Douglas A.; Yukita, Mihoko E-mail: girouxm@etsu.edu E-mail: curt@iastate.edu

    2014-03-01

    Hinge clumps are luminous knots of star formation near the base of tidal features in some interacting galaxies. We use archival Hubble Space Telescope (HST) UV/optical/IR images and Chandra X-ray maps along with Galaxy Evolution Explorer UV, Spitzer IR, and ground-based optical/near-IR images to investigate the star forming properties in a sample of 12 hinge clumps in five interacting galaxies. The most extreme of these hinge clumps have star formation rates of 1-9 M {sub ?} yr{sup 1}, comparable to or larger than the 'overlap' region of intense star formation between the two disks of the colliding galaxy system the Antennae. In the HST images, we have found remarkably large and luminous sources at the centers of these hinge clumps. These objects are much larger and more luminous than typical 'super star clusters' in interacting galaxies, and are sometimes embedded in a linear ridge of fainter star clusters, consistent with star formation along a narrow caustic. These central sources have FWHM diameters of ?70 pc, compared to ?3 pc in 'ordinary' super star clusters. Their absolute I magnitudes range from M{sub I} ? 12.2 to 16.5; thus, if they are individual star clusters they would lie near the top of the 'super star cluster' luminosity function of star clusters. These sources may not be individual star clusters, but instead may be tightly packed groups of clusters that are blended together in the HST images. Comparison to population synthesis modeling indicates that the hinge clumps contain a range of stellar ages. This is consistent with expectations based on models of galaxy interactions, which suggest that star formation may be prolonged in these regions. In the Chandra images, we have found strong X-ray emission from several of these hinge clumps. In most cases, this emission is well-resolved with Chandra and has a thermal X-ray spectrum, thus it is likely due to hot gas associated with the star formation. The ratio of the extinction-corrected diffuse X-ray luminosity to the mechanical energy rate (the X-ray production efficiency) for the hinge clumps is similar to that in the Antennae galaxies, but higher than those for regions in the normal spiral galaxy NGC 2403. Two of the hinge clumps have point-like X-ray emission much brighter than expected for hot gas; these sources are likely 'ultra-luminous X-ray sources' due to accretion disks around black holes. The most extreme of these sources, in Arp 240, has a hard X-ray spectrum and an absorbed X-ray luminosity of ?2 10{sup 41} erg s{sup 1}; this is above the luminosity expected by single high mass X-ray binaries (HMXBs), thus it may be either a collection of HMXBs or an intermediate mass black hole (?80 M {sub ?}).

  10. A first-look atmospheric modeling study of the young directly...

    Office of Scientific and Technical Information (OSTI)

    For an age of 1-3 Myr and considering the lifetime of the protostar phase, ROXs 42Bb's luminosity of log(LL sub ) -3.07 0.07 implies a mass of 9submore -3sup ...

  11. YIA1 - Chen > Young Investigator Program > Research > The Energy Materials

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

    Center at Cornell Using a microfluidic device to synthesize bimetallic nanoparticle catalysts with desired phase and size: An improvement of the nanoparticle-KCl matrix method With efforts from Hao Chen (DiSalvo), Deli Wang (Abruña) and Joshua Tokuda (Pollack), this research is looking to improve the nanoparticle-KCl matrix method. A great effort at emc2 has been focused on synthesizing bimetallic nanoparticle (Np) catalysts for oxygen reduction reactions. Recently, we developed a Np-KCl

  12. YIA2 - Rodríguez-Calero > Young Investigator Program > Research > The

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

    Energy Materials Center at Cornell Three Dimensionally Integrated Architecture for Ultra-High Rate Li-Ion Batteries Gabriel Rodríguez-Calero (Abruña) and Joerg Werner (Wiesner) are taking a closer look at Li-Ion batteries. Conventional lithium ion batteries (LIBs) are built in a macroscopically layered structure consisting of an anode, an electrolyte/separator and a cathode with dimensions of the order of microns. One of the main constraints for fast charge/discharge is the diffusion

  13. YIA3 - Rodriguez-López > Young Investigator Program > Research > The

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

    Energy Materials Center at Cornell Tuning the ORR Electrocatalytic Activity via Controllably Induced Strain With Joaquin Rodriguez-López (Abruña) and Manuel Plaza (Brock), proposed is a novel approach consisting on the use of a piezoelectric platform on which thin epitaxial layers of Pt and Ru will be grown and strained in order to manipulate their electrocatalytic properties towards the Oxygen Reduction Reaction. We anticipate the applied strain will impact the electronic structure of the

  14. YIA4 - Hernández-Burgos > Young Investigator Program > Research > The

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

    Energy Materials Center at Cornell In Situ Characterization of the Electrolyte-Anode Interface in Magnesium Ion Batteries With Kenneth Hernández-Burgos (Abruña), Nicole Ritzert (Abruña) and Xin Huang (Brock) this research will look at a the rechargeable magnesium ion battery. A main limitation in the development of rechargeable magnesium ion batteries is failure due to the decomposition of the electrolyte, causing the formation of a non-conductive, passivating film on the anode. We

  15. YIA5 - Khurana > Young Investigator Program > Research > The Energy

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

    Materials Center at Cornell Single-Ion Gel Polymer Electrolytes for Lithium-Ion and Lithium Metal Secondary Batteries Rachna Khurana (Coates) and Jennifer Schaefer (Archer) hope to find new materials and design rules for creating single-ion conducting polymer membranes suitable for application in lithium-ion and lithium metal batteries with improved performance and safety. Mobile anions produced from dissociation of binary salt in traditional Li-ion electrolytes lead to ionic concentration

  16. YIA6 - Potash > Young Investigator Program > Research > The Energy

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

    Materials Center at Cornell Liquid Power: Utilizing Redox Active Liquids as Active Material in Redox Flow Batteries Rebecca Potash (Abruña) and Samanvaya Srivastava (Archer) are researching a new spin on RFBs. Redox flow batteries (RFB) are currently gaining attention for large-scale grid load-leveling applications. Contemporary technology is based primarily on aqueous salt electrode solutions that are limited by low operating salt concentrations, limiting the energy density of the cell.

  17. BUOYANT MAGNETIC LOOPS IN A GLOBAL DYNAMO SIMULATION OF A YOUNG SUN

    SciTech Connect (OSTI)

    Nelson, Nicholas J.; Toomre, Juri; Brown, Benjamin P.; Brun, Allan Sacha

    2011-10-01

    The current dynamo paradigm for the Sun and Sun-like stars places the generation site for strong toroidal magnetic structures deep in the solar interior. Sunspots and starspots on Sun-like stars are believed to arise when sections of these magnetic structures become buoyantly unstable and rise from the deep interior to the photosphere. Here, we present the first three-dimensional global magnetohydrodynamic (MHD) simulation in which turbulent convection, stratification, and rotation combine to yield a dynamo that self-consistently generates buoyant magnetic loops. We simulate stellar convection and dynamo action in a spherical shell with solar stratification, but rotating three times faster than the current solar rate. Strong wreaths of toroidal magnetic field are realized by dynamo action in the convection zone. By turning to a dynamic Smagorinsky model for subgrid-scale turbulence, we here attain considerably reduced diffusion in our simulation. This permits the regions of strongest magnetic field in these wreaths to rise toward the top of the convection zone via a combination of magnetic buoyancy instabilities and advection by convective giant cells. Such a global simulation yielding buoyant loops represents a significant step forward in combining numerical models of dynamo action and flux emergence.

  18. Indoor risk factors for cough and their relation to wheeze and sensitization in Chilean young adults

    SciTech Connect (OSTI)

    Potts, J.F.; Rona, R.J.; Oyarzun, M.J.; Amigo, H.; Bustos, P.

    2008-04-15

    We assessed the effects of indoor risk factors, including smoking, on different types of cough and on cough and wheeze in combination. Our sample was composed of 1232 men and women residing in a semi-rural area of Chile. We used a standardized questionnaire, sensitization to 8 allergens, and bronchial hyperresponsiveness to methacholine to assess cough and wheeze characteristics. Information was gathered on dampness, mold, ventilation, heating, housing quality, smoking, and environmental tobacco smoke exposure. Most exposures were associated with cough alone or cough in combination with wheeze. Smoking, past smoking, and environmental tobacco smoke exposure were strongly associated with dry cough and wheeze. The use of coal for heating was associated with dry cough. Leaks, mold, and lack of kitchen ventilation were associated with cough and wheeze. Nocturnal cough and productive cough were associated with specific types of sensitization, but dry cough was not. Productive cough was associated with hyperresponsiveness to methacholine. Several different types of indoor exposures, including environmental tobacco smoke exposure, are important contributors to morbidity associated with cough and wheeze. A vigorous preventive strategy designed to lower exposures to indoor risk factors would lower rates of respiratory morbidity.

  19. The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane...

    Office of Scientific and Technical Information (OSTI)

    Information Service, Springfield, VA at www.ntis.gov. Authors: Barman, T S ; Macintosh, B A ; Konopacky, Q M ; Marois, C Publication Date: 2011-05-31 OSTI Identifier:...

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

    Broader source: Energy.gov [DOE]

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

  1. NETL-Regional University Alliance Researcher to Receive Nation’s Highest Award for Young Scientists

    Broader source: Energy.gov [DOE]

    Dr. Brian Anderson, a research fellow of the NETL-Regional University Alliance and associate professor of chemical engineering at West Virginia University, was recognized during a special event at U.S. Department of Energy Headquarters April 14 for receiving the highest honor the U.S. government can bestow on an outstanding scientist in the early stages of his research career.

  2. America's Home Energy Education Challenge: Teaching Kids to Save Energy and

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

    Money | Department of Energy The deadline to register for the Home Energy Education Challenge is November 15. The deadline to register for the Home Energy Education Challenge is November 15. Linda Silverman Senior Advisor, Tech-to-Market Office Daniel Boff Intern, Office of Energy Efficiency and Renewable Energy Energy Education Resources Find lesson plans, science projects, and other activities that can be done in the classroom or at home to prepare K-12 students for a greener future Find

  3. NERSC Announces Winners of Inaugural HPC Achievement Awards

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

    Announces Winners of Inaugural HPC Achievement Awards NERSC Announces Winners of Inaugural HPC Achievement Awards February 14, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 XBD201009 01166 03 NERSC's Cray XE6 "Hopper" The Department of Energy's National Energy Research Scientific Computing Center (NERSC) announced the winners of their inaugural High Performance Computing (HPC) Achievement Awards on Wednesday at the annual NERSC User Group meeting at the Lawrence Berkeley

  4. NERSC Contributes to Science Magazine's Breakthroughs of the Year

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

    Science Magazine's Breakthroughs of the Year NERSC Contributes to Science Magazine's Breakthroughs of the Year January 14, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 sciencebreakthrough.jpg Every year, Science magazine editors and staff sift through numerous scientific accomplishments and ultimately crown one "Breakthrough of the Year." Of the top 10 finalists for 2012, Lawrence Berkeley National Laboratory (Berkeley Lab) computational researchers were major contributors to

  5. NERSC Intern Wins Award for Computing Achievement

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

    Intern Wins Award for Computing Achievement NERSC Intern Wins Award for Computing Achievement March 27, 2013 Linda Vu, lvu@lbl.gov, +1 510 495 2402 ncwit1 Stephanie Cabanela, a student intern in the National Energy Research Scientific Computing Center's (NERSC) Operation Technologies Group was honored with the Bay Area Affiliate National Center for Women and Information Technology (NCWIT) Aspirations in Computing award on Saturday, March 16, 2013 in a ceremony in San Jose, CA. The award honors

  6. NERSC Signs Supercomputing Agreement with Cray

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (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 pr@cray.com +1 206 701 2123 The Department of Energy's National Energy Research Scientific Computing Center (NERSC) announced today that Cray will install its next-generation supercomputer computing system. Consisting of products and services, the multi-year, multi-phase project is valued at more than $40 million. It

  7. NERSC Supercomputers Help Explain the Last Big Freeze

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

    NERSC Supercomputers Help Explain the Last Big Freeze NERSC Supercomputers Help Explain the Last Big Freeze January 31, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 meltwaterroutes.jpg This image shows the different routes that the meltwater could have taken to the ocean. (A. Condron, U. Mass, Amherst.) Scientists suspect that about 13,000 years ago, a catastrophic injection of freshwater into the North Atlantic "conveyor," which transports warm tropical water northward,

  8. Spotlight: Bryant Roybal

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

    Spotlight: Bryant Roybal Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Spotlight: Bryant Roybal Champion chile and a recipe March 1, 2015 Bryant Roybal and his ingredient Bryant Roybal and his ingredient Contact Linda Anderman Email Champion chile New Mexico's first green chile stew champion, Bryant Roybal, is proud to add first prize at the First Annual Great Bowls of Fire Chili Cookoff on February 14, 2015, to

  9. Special Feature: Energy - The Spark that Ignited DOE Supercomputing

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

    Energy - The Spark that Ignited DOE Supercomputing Special Feature: Energy - The Spark that Ignited DOE Supercomputing Scientific Computing for Energy Independence and a Clean Energy Future September 16, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 1280px-OREGONSODD-EVENPLANREDUCEDTHELINESATGASSTATIONSDURINGTHEFUELCRISISINTHEFALLANDWINTEROF1973-74....-NARA-555498.jpg Oregon's odd-even plan reduced the lines at gas stations during the fuel crisis in the fall and winter of 1973-74. This

  10. Supercomputers Capture Turbulence in the Solar Wind

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

    Capture Turbulence in the Solar Wind Supercomputers Capture Turbulence in the Solar Wind Berkeley Lab visualizations could help scientists forecast destructive space weather December 16, 2013 Linda Vu, +1 510 495 2402, lvu@lbl.gov eddies1.jpg This visualization zooms in on current sheets revealing the "cascade of turbulence" in the solar wind occurring down to electron scales. This is a phenomenon common in fluid dynamics-turbulent energy injected at large eddies is transported to

  11. Supercomputers Help a Catalyst Reach its Full Potential

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

    Help a Catalyst Reach its Full Potential Supercomputers Help a Catalyst Reach its Full Potential Placing Protons Prevents Wasteful Profligate Reactions April 23, 2013 Contact: Linda Vu, lvu@lbl.gov +1 510 495 2402 protondeliverystory.jpg While one configuration (endo/endo) of a popular nickel catalyst can produce thousands of hydrogen molecules a second, the other forms that place the proton farther from the center are slower and less efficient. Chemical reactions facilitated by catalysts are

  12. Supernova Hunting with Supercomputers

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

    Supernova Hunting with Supercomputers Supernova Hunting with Supercomputers Berkeley researchers provide "roadmap" and tools for finding and studying Type Ia supernovae in their natural habitat May 20, 2015 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov sn-star.jpg Simulation of the expanding debris from a supernova explosion (shown in red) running over and shredding a nearby star (shown in blue). Image credit: Daniel Kasen, Berkeley Lab/ UC Berkeley Type Ia supernovae are famous for

  13. Throwing a Lifeline to Scientists Drowning in Data

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

    Throwing a Lifeline to Scientists Drowning in Data Throwing a Lifeline to Scientists Drowning in Data New topological technique helps scientists 'see' and search large data sets August 1, 2013 Contact: Linda Vu, lvu@lbl.gov, (510) 495-2402 New computational techniques developed at Lawrence Berkeley National Laboratory (Berkeley Lab) may help save scientists from drowning in their own data. Computational scientists at the Lab have figured out how to streamline the analysis of enormous scientific

  14. Back to school

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

    Kurt's Column Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Back to school LANL supports students in a number of ways, including the Science Education Community Service Time program, our annual school-supply drive, and LANL Laces. August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The biggest thing we can do for our

  15. Beware of migrating animals

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

    Beware of Migrating Animals Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Beware of migrating animals Keep an eye out for wildlife on roadways and in recreational areas, and take extra caution while driving or hiking. November 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Those who encounter injured and or aggressive

  16. Science on Tap - Next Generation Rocket Propellants

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

    Science on Tap - Next Generation Rocket Propellants Science on Tap - Next Generation Rocket Propellants WHEN: Dec 17, 2015 5:30 PM - 7:00 PM WHERE: UnQuarked Wine Room 145 Central Park Square, Los Alamos, NM 87544, USA SPEAKER: Bryce Tappan, Los Alamos National Laboratory CONTACT: Linda Anderman (505) 665-9196 CATEGORY: Bradbury INTERNAL: Calendar Login Science on Tap happens every third Thursday Event Description Science On Tap happens every third Thursday of the month, featuring a new topic

  17. Supercomputer decommissioning

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

    Supercomputer decommissioning Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Roadrunner supercomputer: Rest in pieces Decommissioning a classified computer into hardware "mulch." May 1, 2013 The Roadrunner supercomputer broke the petaflop barrier The Roadrunner supercomputer broke the petaflop barrier. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email

  18. TRANSPORTATION WORKING GROUP (TWG) MEETING Clark County Government Center, Training Room 3

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

    July 28, 2011 at 1 p.m. Present: Brok Armantrout, Boulder City Community Development Department Richard Arnold, Tribal Representative Kathy Bienenstein, Nevada Site Specific Advisory Board Nohemi Brewer, National Nuclear Security Administration Nevada Site Office (NNSA/NSO) Daniel Burns, Nevada Division of Emergency Management Jhon Carilli, NNSA/NSO Linda Cohn, NNSA/NSO Frank Di Sanza, NNSA/NSO Ken Elgan, Esmeralda County Sheriff Sandy Enyeart, Science Applications International Corporation

  19. Trillion Particle Simulation on Hopper Honored with Best Paper

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

    Trillion Particle Simulation on Hopper Honored with Best Paper Trillion Particle Simulation on Hopper Honored with Best Paper Berkeley Lab Researchers Bridge Gap to Exascale May 31, 2013 Contact: Linda Vu, lvu@lbl.gov, (510) 495-2402 VPIC1.jpg Image by Oliver Rubel, Berkeley Lab. An unprecedented trillion-particle simulation, which utilized more than 120,000 processors and generated approximately 350 terabytes of data, pushed the performance capability of the National Energy Research Scientific

  20. Teacher training for fuel cell challenge coming in September

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

    Teacher Training For Fuel Cell Challenge Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Teacher training for fuel cell challenge coming in September The teacher training will take place on two Saturdays in September. August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email While the exact dates have not yet been finalized,

  1. What Are the Computational Keys to Future Scientific Discoveries?

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

    What are the Computational Keys to Future Scientific Discoveries? What Are the Computational Keys to Future Scientific Discoveries? NERSC Develops a Data Intensive Pilot Program to Help Scientists Find Out August 23, 2012 Linda Vu,lvu@lbl.gov, +1 510 495 2402 ALS.jpg Advanced Light Source at the Lawrence Berkeley National Laboratory. (Photo by: Roy Kaltschmidt, Berkeley Lab) A new camera at the hard x-ray tomography beamline of Lawrence Berkeley National Laboratory's (Berkeley Lab's) Advanced

  2. Shadi Dayeh: UCSD

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

    Shadi Dayeh: UCSD Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Shadi Dayeh: UCSD Former postdoc now an Associate Professor with the Jacobs School of Engineering at UC San Diego. June 20, 2014 Shadi Dayeh Shadi Dayeh Contact Linda Anderman Email Shadi Dayeh Dayeh growing nanowires in a Lab glove box Shadi Dayeh is currently an assistant professor with the Department of Electrical and Computer Engineering with the

  3. $165,000 awarded to regional businesses by LANS

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

    $165,000 Awarded to Regional Businesses Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit $165,000 awarded to regional businesses by LANS The companies are Mustomo, Inc.; IX Power; Synfolia; and Tape-Ease. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Los Alamos National Security, LLC invests $1 million per year in

  4. Robert Jilek: Pellion Technologies

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

    Robert Jilek: Pellion Technologies Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Robert Jilek: Pellion Technologies Senior research scientist at eastern energy storage startup September 3, 2014 Robert Jilek Robert Jilek Contact Linda Anderman Email Robert Jilek Jilek is currently with Pellion Technologies Bob Jilek is currently spending part of his time in a management role at Pellion Technologies in the Cambridge

  5. Bubbles Help Break Energy Storage Record for Lithium Air-Batteries

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

    Bubbles Help Break Energy Storage Record for Lithium Air-Batteries Bubbles Help Break Energy Storage Record for Lithium Air-Batteries Foam-base graphene keeps oxygen flowing in batteries that holds promise for electric vehicles January 25, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Using a new approach, the team built a graphene membrane for use in lithium-air batteries, which could, one day, replace conventional batteries in electric vehicles. Resembling coral, this porous graphene material

  6. Protecting the environment into the future

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

    Protecting the Environment Into the Future Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Protecting the environment into the future Last year, the Lab recycled 47 percent of its solid, non-hazardous waste by placing it in the recycling containers. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The Lab's

  7. Quality Teaching in Northern New Mexico

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    Quality Teaching in Northern New Mexico Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Quality Teaching in Northern New Mexico A personal message from the Community Programs Office Director February 1, 2014 Kurt Steinhaus, Community Programs Office Director Kurt Steinhaus, Community Programs Office Director Contacts Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman

  8. Assets in Action Community Award nominations open until December 17

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

    Assets in Action Community Award Nominations Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Assets in Action Community Award nominations open until December 17 If you know people who support building a strong community for youth in Los Alamos, nominate them for an Assets in Action Community Award. January 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community

  9. At the intersection of past and future-The Lab's archives

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

    The Lab's Archives Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit At the intersection of past and future-The Lab's archives The Archives staff typically handle about 60 requests a month for everything from Freedom of Information Act queries to calls from journalists and television producers. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs

  10. 2013 Community Commitment plan approved

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    Community Commitment Plan Approved Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit 2013 Community Commitment plan approved The plan provides funding from LANS' management fee to invest in regional education, economic development, and charitable giving programs. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The

  11. Potential partnerships and funding from a variety of sources

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

    Potential partnerships and funding from a variety of sources Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Potential partnerships and funding from a variety of sources Find a funding opportunity from our current opportunities. June 20, 2014 Potential partnerships Find a funding opportunity from our current opportunities. Contact Linda Anderman Email An evolving list of funding opportunities. See attachments and

  12. Potential partnerships and funding from a variety of sources

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

    Potential partnerships and funding from a variety of sources Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Potential partnerships and funding from a variety of sources Find a funding opportunity from current opportunities. November 1, 2014 Potential partnerships Find a funding opportunity from current opportunities. Contact Linda Anderman Email An evolving list of funding opportunities. See attachments and links

  13. Potential partnerships and funding from a variety of sources

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

    Potential partnerships and funding from a variety of sources Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Potential partnerships and funding from a variety of sources Find a funding opportunity from current opportunities. September 1, 2015 Potential partnerships and funding from a variety of sources Find a funding opportunity from current opportunities. Contact Linda Anderman Email An evolving list of funding

  14. Preliminary Agenda

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

    Agenda INAUGURAL USER MEETING Center for Nanophase Materials Sciences Oak Ridge National Laboratory May 23-25, 2005 Pollard Technology Conference Center Oak Ridge, Tennessee Date Location Monday, May 23 MORNING 10:30 am Registration opens Pollard Lobby 11:30-1 pm Buffet Lunch available for all registered participants Pollard Lobby Monday, May 23 AFTERNOON 1 pm ORNL Welcome Jim Roberto, ORNL Deputy Director, Science and Technology Auditorium CNMS Welcome Linda Horton, CNMS Director Science at the

  15. Research & Technology Showcase in Albuquerque on September 12

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    Research & Technology Showcase In Albuquerque Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Research & Technology Showcase in Albuquerque on September 12 The event will include an overview of its economic development programs, examples of corporate applications, along with time for poster sessions and networking. September 1, 2012 dummy image Read our archives Contacts Editor Linda

  16. Accelerate program supports students as they establish careers

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

    Accelerate Program Supports Students Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Accelerate program supports students as they establish careers More than 60 students from six Northern New Mexico colleges meet business representatives to hone their professional readiness skills. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt

  17. Accelerating Advanced Material Development

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

    Materials Research in the Information Age Accelerating Advanced Material Development NERSC Science Gateway a 'Google of Material Properties' October 31, 2011 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Kristin Persson is one of the founding scientists behind the Materials Project, a computational tool aimed at taking the guesswork out of new materials discoveries, especially those aimed at energy applications like batteries. (Roy Kaltschmidt, LBNL) New materials are crucial to building a clean energy

  18. Next Big Idea coming September 14-15

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    Next Big Idea Coming September 14-15 Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Next Big Idea coming September 14-15 This event lets innovators and the public get together to share technology, art, research and development, and invention. August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email There are only a 100

  19. Northern New Mexico College scholarship dinner September 29

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

    Northern New Mexico College Scholarship Dinner Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Northern New Mexico College scholarship dinner September 29 In addition to recognizing scholarship recipients and donors, the evening will include a silent auction and student-performed entertainment. September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community

  20. Northern New Mexico companies benefit from economic development funds

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

    Northern New Mexico companies benefit from economic development funds Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Northern New Mexico companies benefit from economic development funds April 1, 2013 HydroBio satellite image shows irrigation status A HydroBio satellite image shows irrigation status. The company was awarded funds in 2012. Contact Editor Linda Anderman Email Community Programs

  1. Additional public meeting on plutonium disposition on September 18

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    Additional Public Meeting on Plutonium Disposition Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Additional public meeting on plutonium disposition on September 18 DOE has extended the public review and comment period for the Draft Surplus Plutonium Disposition (SPD) Supplemental Environmental Impact Statement (EIS). September 1, 2012 dummy image Read our archives Contacts Editor Linda

  2. After 70 years of service, taking action for the future

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    After 70 years of service, taking action for the future Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit After 70 years of service, taking action for the future April 1, 2013 Director Charlie McMillan Lab Director Charlie McMillan. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Welcome, everyone, to the latest edition of Connections. As we at the Laboratory

  3. Agnes Houser | Y-12 National Security Complex

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

    Agnes Houser Agnes Houser Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Agnes Houser A

  4. National Renewable Energy Laboratory

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

    RENEWABLE ENERGY AND ENERGY EFFICIENCY SCIENCE PROJECTS 1 SCIENCE PROECTS IN RENEWABLE ENERGY AND ENERGY EFFICIENCY A guide for Secondary School Teachers Authors and Acknowledgements: This second edition was produced at the National Renewable Energy Laboratory (NREL), through the laboratory's Office of Education Programs, under the leadership of the Manager, Dr. Cynthia Howell and guidance of the Program Coordinators, Matt Kuhn and Linda Lung. The contents are the result of contributions by a

  5. New Computer Codes Unlock the Secrets of Cleaner Burning Coal

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

    New Computer Codes Unlock the Secrets of Cleaner Burning Coal New Computer Codes Unlock the Secrets of Cleaner Burning Coal March 29, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 The Polk Power Station near Mulberry, Florida, is an Integrated Gasification Combined Cycle gasification plant. It is capable of generating 313 megawatts of electricity - 250 megawatts of which are supplied to the electric grid. The plant's gas cleaning technology removes more than 98 percent of the sulfur in coal,

  6. New Mexico Airlines begins Los Alamos/ Albuquerque flights April 8

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

    New Mexico Airlines begins Los Alamos/ Albuquerque flights April 8 Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit New Mexico Airlines begins Los Alamos/ Albuquerque flights April 8 Open House scheduled for April 5. April 1, 2013 New Mexico Airlines plane A New Mexico Airlines plane. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The service is available to

  7. New record for employee giving campaign

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

    New Record For Employee Giving Campaign Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit New record for employee giving campaign The Lab's annual employee giving campaign broke two records this year. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Employee contributions totaled more than $2.1 million, surpassing

  8. New tool helps reduce use of hazardous chemicals

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

    Tool Helps Reduce Use Of Hazardous Chemicals Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit New tool helps reduce use of hazardous chemicals The "Green Chemical Alternatives Purchasing Wizard," will begin to help employees choose the most benign substances possible for their work. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs

  9. Minutes

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

    » Minutes Minutes Minutes of the ERSUG/EXERSUG Meeting UCLA Faculty Center Jan 12-13, 1994 Wednesday, Jan 12, 1994 ----------------------- Morning Session --------------- Tom Kitchens: View from Washington ---------------------------------- Staff of OSC: Dave Nelson, John Cavallini, Fred Howes, Dan Hitchcock, George Seweryniak, Greg Chartrand, Bob Aiken, Wally Ermler, Gary Johnson, Jim Mcgraw, Linda Twenty, Melea Fogle, Jane Hiegel. Gary Johnson leaves in October. Gloomy expectations were

  10. Modeling Feat Sheds Light on Protein Channel's Function

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

    Modeling Feat Sheds Light on Protein Channel's Function Modeling Feat Sheds Light on Protein Channel's Function November 1, 2012 NERSC Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 nerscweb.png The ribosome (red-blue) in complex with the translocon channel (green), which is embedded in the cell membrane (yellow, white). Proteins that are inserted via the ribosome into the channel can either be laterally integrated into the cell membrane or secreted across the cell membrane (inset). (Image

  11. 2012-2013 EAC Membership Roster

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

    August 3, 2012 Electricity Advisory Committee 2012/2013 Membership Roster Richard Cowart Regulatory Assistance Project CHAIR Irwin Popowsky Pennsylvania Consumer Advocate VICE CHAIR William Ball Southern Company Linda Blair ITC Holdings Corporation Rick Bowen Alcoa Merwin Brown California Institute for Energy and Environment Ralph Cavanagh Natural Resources Defense Council The Honorable Paul Centolella Public Utilities Commission of Ohio David Crane NRG Energy, Inc. The Honorable Robert Curry

  12. HTWOS and System Planning Briefing to DOE-HQ

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

    Waste Operations Simulator (HTWOS): A System Planning Tool Ted Hohl Linda Bergmann Jeremy Belsher Tom Crawford Tony Waldo System Planning & Modeling September 11, 2013 Agenda  System Planning Process (12 min)  Hanford Tank Waste Operations Simulator Model (15 min)  Demonstration (30 minutes)  Q&A (25 min) 2 SYSTEM PLANNING PROCESS 3 Mission Flowsheet - Simplified Process Flow Diagram 4 System Planning Inputs How do system models guide System Planning 5 RPP System Plan Risk

  13. Happening Now

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

    Happening Now Happening Now From Nano Days and High-Tech Halloween to conversations with scientists, community events, and everything in between. This is the place to find out what's happening now @ the Bradbury. Contact Marketing, Communications and Event Planning Linda Anderman (505) 665-9196 Email Scientist in the Spotlight Join us at the Museum every second Saturday of the month from 11 AM to 1 PM for a program called Scientist in the Spotlight. This activity features Scientist Ambassadors

  14. Harvey Kite | Y-12 National Security Complex

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

    Harvey Kite Harvey Kite Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Harvey Kite Fondly

  15. Help local children get new shoes

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

    Help Local Children Get New Shoes Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Help local children get new shoes To help the program assist more children, consider a donation to the LANL Laces program. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Support for this program comes from contributions by Lab

  16. Helping make the holidays happier

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    Helping Make The Holidays Happier Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Helping make the holidays happier This year's LANL food drive collected enough donations to provide 11,600 meals for those in need. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The contributions by employees included 164 turkeys

  17. Gift tag drive benefits local children and seniors

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    Gift Tag Drive Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Gift tag drive benefits local children and seniors Each year, Lab employees and contractors work to make the holidays brighter for local children and seniors through its Holiday Gift Tag drive. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Individuals

  18. Gordon Fee, part 1 | Y-12 National Security Complex

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

    1 Gordon Fee, part 1 Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Gordon FeePart 1 |

  19. Gordon Fee, part 2 | Y-12 National Security Complex

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

    2 Gordon Fee, part 2 Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Gordon FeePart 1 |

  20. Graduate Research Fellowship Program deadlines begin November 13

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

    Graduate Research Fellowship Program Deadlines Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Graduate Research Fellowship Program deadlines begin November 13 The program is designed to recognize and support outstanding students pursuing research-based masters and doctoral degrees in its mission areas. November 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community

  1. Secure Wireless Tritium Air Monitoring Cart Development

    Office of Environmental Management (EM)

    Wireless Tritium Air Monitoring Cart Development PDRD Projects #SR13020, SR14058 Davie Shull and Joe Cordaro Research and Development Engineering Tritium Focus Group Meeting April 24, 2014 Acknowledgements * SRNL Team - Software Development * Matt Folsom * Joel Jones - Engineering Design * David McFall * Monica Phillips * Chad Sweeney - Electrical Fabrication * Kevin Tietze * Don Varble * George Graham - Drafting / Designer * Larry Feutral * Ken Meeler - Procurement * Linda Gray * Jim Buchanan -

  2. TEC/WG Tribal Topic Group

    Office of Environmental Management (EM)

    Conference Call December 6, 2005 Group Chair: Jay Jones (DOE/OCRWM) Participating TEC Tribal Topic Group Members: Kevin Clarke (DOE/RL), Kristen Ellis (DOE/CI), Lisa Gover (NTEC), Dan King (Oneida Nation), Corinne Macaluso (DOE/OCRWM), Ellen Ott (DOE/GC), Ted Repasky (CTUIR), Cathy Reynolds (DOE/GC), Lisa Sattler (CSG-MW) Herman Shorty (Navajo Nation), Linda Sikkema (NCSL), Christopher Wells (SSEB) DOE support contractors also participated in this call. Action Items: Responsible Party Action to

  3. How to See the Supernova Berkeley Lab Just Discovered | Department of

    Energy Savers [EERE]

    Energy See the Supernova Berkeley Lab Just Discovered How to See the Supernova Berkeley Lab Just Discovered September 1, 2011 - 10:12am Addthis Berkeley Lab scientist Peter Nugent discusses a recently discovered supernova that is closer to Earth - approximately 21 million light-years away - than any other of its kind in a generation. Linda Vu Skywatchers -- grab your binoculars and telescopes, and head for some clear dark skies. A new supernova has been discovered near the Big Dipper.

  4. SEPARATION OF HEAVY METALS: REMOVAL FROM INDUSTRIAL WASTEWATERS

    Office of Scientific and Technical Information (OSTI)

    SEPARATION OF HEAVY METALS: REMOVAL FROM INDUSTRIAL WASTEWATERS AND CONTAMINATED SOIL* Robert W. Peters + and Linda Shem Energy Systems Division Argonne National Laboratory 9700 South Cass Avenue Argonne, Illinois 60439 Abstract This paper reviews the applicable separation technologies relating to removal of heavy metals from solution and from soils in order to present the state-of-the-art in the field. Each technology is briefly described and typical operating conditions and technology

  5. Contacts for the Office of Standard Contract Management (GC-73) |

    Energy Savers [EERE]

    Department of Energy Standard Contract Management (GC-73) Contacts for the Office of Standard Contract Management (GC-73) David K. Zabransky, Director, Office of Standard Contract Management 202-586-9198 david.zabransky@hq.doe.gov Susan Smith, Supervisory Program Analyst Nuclear Waste Fund Activities Team 202-586-3213 susan.smith@hq.doe.gov Staff: Jackie Chestnut Linda Desell Vernita Galloway Sheila King George Riling Jim Zimmerman Connie Barton, Supervisory Nuclear Utility Specialist

  6. New DOE Office of Science support for CAMERA to develop computational

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

    mathematics for experimental facilities research New DOE Office of Science support for CAMERA to develop computational mathematics for experimental facilities research New DOE Office of Science support for CAMERA to develop computational mathematics for experimental facilities research September 22, 2015 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov newcameralogofinal Experimental science is evolving. With the advent of new technology, scientific facilities are collecting data at

  7. Vacancy announcements

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

    Vacancy announcements Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Vacancy announcements Join our team or tell a friend September 2, 2014 Vacancy announcements Vacancy announcements Contact Linda Anderman Email For the most up-to-date employment opportunities, go to our employment website. The jobs below were available as of the distribution date. Job title Organization R&D Engineer 2 for System Integration

  8. Volunteers needed for LANL Student Symposium August 7-8

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    Volunteers Needed For Student Symposium Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Volunteers needed for LANL Student Symposium August 7-8 Judges are needed at this year's student symposium, "Championing Scientific Careers." August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Judges are needed at this

  9. Researchers Discover a New Kind of Neutrino Transformation

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

    Researchers Discover a New Kind of Neutrino Transformation Researchers Discover a New Kind of Neutrino Transformation NERSC, ESnet and computational scientists help researchers discover how neutrinos flavor-shift as they travel at near light-speed March 8, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Daya Bay Neutrino Facility in China. Photo by: Roy Kaltschmidt, Lawrence Berkeley National Laboratory. Neutrinos, the wispy particles that flooded the universe in the earliest moments after the Big

  10. Researchers Model Impact of Aerosols Over California

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

    Researchers Model Impact of Aerosols Over California Researchers Model Impact of Aerosols Over California Research may clarify the effectiveness of regional pollution controls May 28, 2013 Contact: Linda Vu, lvu@lbl.gov, (510) 495-2404 LosAngelesSmogv1.jpg Smog over downtown Los Angeles. Aerosols are microscopic particles-like dust, pollen and soot-that ubiquitously float around in our atmosphere. Despite their tiny stature, these particles can have a huge impact on human health, climate and the

  11. Participants

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

    Participants Participants (Kneeling from left to right: C.S. Chang, Jeff Candy, Alex Friedman, Stephane Ethier, Zhihong Lin. Standing, left to right: Xianxu Tang, Richard Gerber, Harvey Wasserman, Alice Koniges, Brian Wirth, Kathy Yelick, Linda Sugiyama, Kai Germaschewski, Frank Tsung, Charlson Kim, Yukiko Sekine, Lee Berry, John Ludlow, John Mandrekas, Bill Tang, Doug McCune) Large Scale Computing and Storage Requirements for Fusion Energy Sciences An ASCR / FES / NERSC Workshop August 3-4,

  12. Peter Nugent Named Deputy for Scientific Engagement

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

    Peter Nugent Named Deputy for Scientific Engagement Peter Nugent Named Deputy for Scientific Engagement June 3, 2014 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov XBD201308-03524-01.jpg Peter Nugent working with 2013 summer student Kayla Mendel. Peter Nugent has been appointed Deputy for Scientific Engagement in Berkeley Lab's Computing Sciences. In his new role, Nugent will work with CRD and Computing Sciences leadership to develop and implement a strategy for engaging with other Berkeley Lab

  13. David Skinner Named NERSC Strategic Partnerships Lead

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

    David Skinner Named NERSC Strategic Partnerships Lead David Skinner Named NERSC Strategic Partnerships Lead January 24, 2014 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov XBD201102-00089.jpg David Skinner This month, the National Energy Research Scientific Computing Center (NERSC) created a new position-Strategic Partnerships Lead, to identify new science communities that can benefit from NERSC resources. David Skinner, former head of NERSC's Outreach Software and Programming Group (OSP), has

  14. Disordered Materials Hold Promise for Better Batteries

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

    Disordered materials hold promise for better batteries Disordered Materials Hold Promise for Better Batteries February 21, 2014 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov disorderedMAT.jpg Conventional layered lithium and transition metal cathode material (top) and the new disordered material studied by researchers at MIT (bottom) as seen through a scanning transmission electron microscope. Inset images show diagrams of the different structures in these materials. (In the disordered

  15. Frontiers in Science Archive

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

    Frontiers in Science Lectures » Frontiers in Science Archive Frontiers in Science Archive x LInda Anderman (505) 665-9196 Email The Frontiers in Science lecture series are a public service of the Los Alamos National Laboratory Fellows. Fellows are appointed by the Laboratory Director in recognition of sustained outstanding contributions and exceptional promise for continued professional achievement. All lectures are open to the public and free of charge. PAST LECTURES 2015 August Beyond Pluto:

  16. DRAFT ADVICE - UNACCEPTABLE PROGRAM IMPACTS UNDER FY 97 BUDGET

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

    John Iani, Regional Administrator U. S. Environmental Protection Agency, Region 10 1200 Sixth Avenue Seattle, WA 98101 Linda Hoffman, Director Washington State Department of Ecology P.O. Box 47600 Olympia, WA 98504-7600 Re: M-91 Change Package Dear Mssrs. Klein, Schepens, Iani and Ms. Hoffman, While the M-91-03-01 change package does not provide a comprehensive solution to Hanford's buried waste challenges, the Hanford Advisory Board (Board) believes the following items in the change package

  17. DRAFT ADVICE - UNACCEPTABLE PROGRAM IMPACTS UNDER FY 97 BUDGET

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

    John Iani, Regional Administrator U.S. Environmental Protection Agency, Region 10 1200 Sixth Avenue Seattle, WA 98101 Linda Hoffman, Director Washington State Department of Ecology P.O. Box 47600 Olympia, WA 98504-7600 Re: 300 Area Explanation of Significant Difference Dear Mssrs. Klein, Schepens, Iani and Ms. Hoffman, The Hanford Advisory Board (Board) is reviewing the Tri-Party Agreement (TPA) Agencies' proposed Explanation of Significant Difference (ESD) on the 300 Area cleanup. The cleanup

  18. Director testifies before Senate subcommittee

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    Director testifies before Senate subcommittee Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Director testifies before Senate subcommittee Future Laboratory budgets under consideration. June 1, 2013 Director Charlie McMillan during his remarks Director Charlie McMillan during his remarks Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Lab Director Charlie

  19. Chimayo Elementary school performs well in Fuel Cell Challenge

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

    Fuel Cell Challenge Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Chimayo Elementary school performs well in Fuel Cell Challenge A team from Chimayo Elementary School placed second overall in the competition, even though it was its first year in the event. January 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Los

  20. Chris Fresquez named Small Business leader

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

    Chris Fresquez Named Small Business Leader Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Chris Fresquez named Small Business leader Fresquez and his team support businesses within Northern New Mexico, including those in area pueblos. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email We want to support and grow

  1. Collaboration drives achievement in protein structure research

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

    Collaboration drives achievement in protein structure research Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Collaboration drives achievement in protein structure research By tracking down how bacterial defense systems work, the scientists can potentially fight infectious diseases and genetic disorders November 1, 2014 Thomas Terwilliger Thomas Terwilliger Contact Linda Anderman Email When a recent print issue of

  2. Coming up with platinum substitutes may be elemental

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

    Coming up with platinum substitutes may be elemental Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Coming up with platinum substitutes may be elemental Lab researchers are working with an abundant element to take their place: cobalt. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Initial findings by a Los

  3. H-02 Constructed Wetland Studies: Amphibians and Plants | SREL Research

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    H-02 Constructed Wetland Studies: Amphibians and Plants Amphibian Studies: Stacey Lance, David Scott, Wes Flynn, and Diana Soteropoulos Vegetation Surveys: Rebecca Sharitz, Linda Lee, and Paul Stankus The H-02 treatment wetland array associated with the H-Area facilities Buckets at sampling location Green treefrogs (Hyla cinerea) on planted bulrush stems Construction of the H-02 treatment wetlands adjacent to H-Area on the Savannah River Site (SRS) began during FY-2007. The Savannah River

  4. Ice Sheet Model Reveals Most Comprehensive Projections for West

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    Antarctica's Future Most Comprehensive Projections for West Antarctica's Future Revealed Ice Sheet Model Reveals Most Comprehensive Projections for West Antarctica's Future BISICLES Simulations Run at NERSC Help Estimate Ice Loss, Sea Level Rise August 18, 2015 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov IceSheet Retreat in the Amundsen Sea Embayment in 2154 (Credit: Cornford et al., The Cryosphere, 2015) A new international study is the first to use a high-resolution, large-scale

  5. BISICLES Captures Details of Retreating Antarctic Ice

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    BISICLES Captures Details of Retreating Antarctic Ice BISICLES Captures Details of Retreating Antarctic Ice March 30, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 Satellite observations suggest that the shrinking West Antarctic ice sheet is contributing to global sea level rise. But until recently, scientists could not accurately model the physical processes driving retreat of the ice sheet. Now, a new ice sheet model-called Berkeley-ISICLES (BISICLES)-is shedding light on these details.

  6. Bauer named Facilities, Infrastructure and Services head | Y-12 National

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    Security Complex Bauer named Facilities, ... Bauer named Facilities, Infrastructure and Services head Posted: August 27, 2012 - 1:01pm B&W Y-12 President and General Manager Chuck Spencer has named Linda Bauer as vice president of Facilities, Infrastructure and Services (FI&S). Bauer most recently served as senior vice president with Los Alamos Technical Associates, Inc. helping direct large-scale government and private endeavors, such as the Portsmouth Environmental Restoration

  7. Brian K. Kobilka and G-protein-coupled Receptors (GPCR)

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    Brian K. Kobilka and G-protein-coupled Receptors (GPCR) Resources with Additional Information Brian K. Kobilka Credit: Linda A. Cicero Stanford News Service 'Thanks in part to research performed at the U.S. Department of Energy's (DOE) Argonne National Laboratory, the 2012 Nobel Prize in Chemistry was awarded today to Americans Brian Kobilka and Robert Lefkowitz for their work on G-protein-coupled receptors. G-protein-coupled receptors, or GPCRs, are a large family of proteins embedded in a

  8. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar Los Alamos 70th anniversary events and a fundraiser for LANL Laces. April 1, 2013 Bradbury Science Museum Exciting 70th anniversary activities will take place at the Bradbury Science Museum all year. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Take advantage of all the great

  9. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar 70th anniversary talk, scholarship deadline, parenting conference June 1, 2013 Istvan Hargittai and James D. Watson in 2010 in the Watsons' home in New York City Istvan Hargittai and James D. Watson in 2010 in the Watsons' home in New York City Contact Editor Linda Anderman Email Community Programs Office Kurt

  10. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar Talks on science, history, fun with robots and renewable energy resources for small business August 1, 2013 New Frontiers in Science talk in August in four locations New Frontiers in Science talk in August in four locations Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman

  11. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar Talks on the Cold War and explosives September 1, 2013 New Frontiers in Science talk in August in four locations One of the talks this month will highlight the Lab's history and contributions regarding explosives Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email Talk on

  12. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar New Frontiers in Science talk and museum activities November 1, 2013 The Bradbury Science Museum at night The Lab celebrates 50 years in space Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email Big bang survival topic of the next Frontiers in Science talk In early

  13. For your calendar

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    For your calendar Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit For your calendar MidSchoolMath, climate change talk, Innovation Summit and Bradbury activities March 1, 2014 New Frontiers in Science talk in August in four locations National math teacher's conference in Santa Fe Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email MidSchoolMath National

  14. Four seasons of giving

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    Kurt's Column Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Four seasons of giving We value a culture of giving and appreciate our employees' on-going volunteerism throughout Northern New Mexico and even nationwide. January 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email We value a culture of giving and appreciate our

  15. Fourth Friday Cancelled due to Thanksgiving Holidays

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    Fourth Friday Cancelled due to Thanksgiving Holidays Fourth Friday Cancelled due to Thanksgiving Holidays WHEN: Nov 27, 2015 10:00 AM - 5:00 PM WHERE: Bradbury Science Museum 1350 Central Ave, Los Alamos, NM 87544, USA CONTACT: Linda Anderman (505) 665-9196 CATEGORY: Bradbury INTERNAL: Calendar Login Fourth Fridays Downtown Event Description Fourth Fridays Downtown will not take place during the weeks of Thanksgiving and Christmas. The Los Alamos Creative District sponsors Fourth Fridays, an

  16. Fourth Fridays - Museum Open Late

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    Fourth Fridays - Museum Open Late Fourth Fridays - Museum Open Late WHEN: Jan 22, 2016 10:00 AM - 6:00 PM WHERE: Bradbury Science Museum 1350 Central Ave, Los Alamos, NM 87544 USA CONTACT: Linda Anderman (505) 665-9196 CATEGORY: Bradbury INTERNAL: Calendar Login Fourth Fridays in Downtown Los Alamos Event Description The museum will be open late until 6 p.m. every Fourth Friday offering extended access to exhibits, special programming, and activities. The Los Alamos Creative District is

  17. Francesco Grilli: Karlsruhe Institute of Technology

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    Francesco Grilli: Karlsruhe Institute of Technology Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Francesco Grilli: Karlsruhe Institute of Technology High-temperature superconductors January 1, 2015 Francesco Grilli Francesco Grilli Contact Linda Anderman Email Peter Hosemann Francesco Grilli now at Karlsruhe Institute of Technology After graduating with his Ph.D. from the Swiss Federal Institute of Technology in

  18. Free film screening at Bradbury Science Museum September 7

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    Free Film Screening At Bradbury Science Museum Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Free film screening at Bradbury Science Museum September 7 There will be a special screening of the film "The Biggest Story Problem: Why America's Students are Failing at Math." September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt

  19. Expanding Your Horizons scheduled for March 2

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    Expanding Your Horizons Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues 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

  20. After 5 Years, NERSC's Franklin Retires

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    After 5 Years, NERSC's Franklin Retires After 5 Years, NERSC's Franklin Retires May 4, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 Franklin Cray XT4 supercomputer: Franklin Cray XT4 supercomputer -- a massively parallel processor (MPP) system. Photo: Roy Kaltschmidt/LBNL. This week, the Department of Energy's National Energy Research Scientific Computing Center (NERSC) retired one of its most scientifically prolific supercomputers to date-a Cray XT4 named Franklin, in honor of the United States'

  1. Aided by Simulations, Scientists Observe Atomic Collapse State

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    Atomic Collapse State Observed Aided by Simulations, Scientists Observe Atomic Collapse State Quantum Mechanics Prediction Confirmed in Graphene Using NERSC's Hopper April 26, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 Michael Crommie runs the research group that made the discovery. He holds joint appointments with Berkeley Lab and UC Berkeley. (Photo by Roy Kaltschmidt) Scientists have finally confirmed a 70 year-old prediction in quantum mechanics-that electrons in super-heavy atoms

  2. Staff | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Scientific User Facilities (SUF) Division SUF Home About Staff Dr. James B. Murphy What's New User Facilities Projects Accelerator & Detector Research Science Highlights Principal Investigators' Meetings BES Home About Staff Print Text Size: A A A FeedbackShare Page Name Title Research Area of Responsibility Dr. James Murphy Division Director Scientific User Facilities Ms. Linda Cerrone Support Specialist Ms. Rocio Meneses Program Assistant Operations Dr. Peter Lee Program Manager X-ray and

  3. Multidisciplinary team aids understanding of Hepatitis C virus and possible

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    cure Multidisciplinary team aids understanding of Hepititus C virus Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Multidisciplinary team aids understanding of Hepatitis C virus and possible cure Computer simulations model cellular development. March 1, 2013 Centers for Disease Control World Map of Hepititus C Centers for Disease Control World Map of Hepatitis C. Contacts Editor Linda

  4. Multiple organizations build interagency fire center at LANL

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    Interagency Fire Center At LANL Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Multiple organizations build interagency fire center at LANL The facility is expected to significantly enhance the current fire-fighting capabilities of the partnering agencies. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The new

  5. NERSC 2013 Annual Report

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    3 Annual Report National Energy Research Scientific Computing Center 2013 Annual Report Ernest Orlando Lawrence Berkeley National Laboratory 1 Cyclotron Road, Berkeley, CA 94720-8148 This work was supported by the Director, Office of Science, Office of Advanced Scientific Computing Research of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. Cover Image Credits: front cover, left to right: Linda Sugiyama, Massachusetts Institute of Technology; IceCube Collaboration; David

  6. NERSC Helps Develop Next-Gen Batteries

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    NERSC Helps Develop Next-Gen Batteries NERSC Helps Develop Next-Gen Batteries A genomics approach to materials research could speed up advancements in battery performance December 18, 2012 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 XBD201110-01310.jpg Kristin Persson To reduce the United States' reliance on foreign oil and lower consumer energy costs, the Department of Energy (DOE) is bringing together five national laboratories, five universities and four private firms to revolutionize

  7. NREL Enters Wind Energy Research Partnership in Hawaii - News Releases |

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

    NREL NREL Enters Wind Energy Research Partnership in Hawaii April 1, 2008 The U.S. Department of Energy's National Renewable Energy Laboratory (NREL) has signed a memorandum of understanding with UPC Wind to establish a Remote Research Affiliate Partner Site at UPC Wind's Kaheawa Wind Farm on Maui. It is the first such partner site for the National Renewable Energy Laboratory's wind technology program outside of its base in Colorado. Hawaii Gov. Linda Lingle announced the collaborative

  8. Learning From Photosynthesis to Create Electricity

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    Scientists Studying Photosynthesis to Generate Electricity Learning From Photosynthesis to Create Electricity Researchers use NERSC supercomputers to investigate photosynthetic materials May 15, 2012 NERSC Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 TACC Contact: Adam Dubrow, aarondubrow@tacc.utexas.edu A triad molecule (left) is rendered in bond representation. Carbon atoms are in cyan; nitrogen in blue; hydrogen in white. Image credit: Margaret Cheung. Solar power could transform the

  9. Martin Karplus Wins Nobel Prize in Chemistry

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    Home » News & Publications » NERSC News » Center News » Martin Karplus Wins Nobel Prize in Chemistry Martin Karplus Wins Nobel Prize in Chemistry October 9, 2013 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov Karplus605v1.jpg Martin Karplus On Wednesday, the Nobel Prize in Chemistry was awarded to three scientists for pioneering methods in computational chemistry that have brought a deeper understanding of complex chemical structure and reactions in biochemical systems. These methods

  10. Meraculous: Deciphering the 'Book of Life' With Supercomputers

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    Meraculous: Deciphering the 'Book of Life' With Supercomputers Meraculous: Deciphering the 'Book of Life' With Supercomputers Novel Berkeley Algorithms and Computational Techniques Speed Up Genome Assembly, from Months to Minutes June 1, 2015 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov Genomev1.jpg Human Chromosomes. Credit: Jane Ades, NHGRI Genomes are like the biological owner's manual for all living things. Cells read DNA instantaneously, getting instructions necessary for an organism to

  11. OSTI, US Dept of Energy, Office of Scientific and Technical Information |

    Office of Scientific and Technical Information (OSTI)

    Speeding access to science information from DOE and Beyond Champions of Change: Open Science by Linda McBrearty on Tue, Jul 2, 2013 OSTI's involvement in public access is accelerating! The week of June 24th, 2013, The White House recognized Champions of Change: Open Science at an event in the Eisenhower Executive Office Building. OSTI's Director Walt Warnick was invited to nominate individuals who had been instrumental in championing public access to open science. As a result of Walt's

  12. OSTI, US Dept of Energy, Office of Scientific and Technical Information |

    Office of Scientific and Technical Information (OSTI)

    Speeding access to science information from DOE and Beyond Connects with Universities Nationwide by Linda McBrearty on Fri, Oct 23, 2009 One of OSTI's founding missions is to support education. From the early 1960s when OSTI provided educational materials on the atom and published the booklet called "Understanding the Atom" we have been committed to education. While information in OSTI databases can be used by teachers, students and parents for Kindergarten through High School,

  13. Introducing the new look of "Connections"

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    Introducing the new look of "Connections" Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit "Connections" gets new look and feel based on your feedback Changed to serve you better for mobile and tablet reading. March 1, 2013 Mobile view enhances user experience Responsive mobile view enhances user experience. Contacts Editor Linda Anderman Email Community Programs Office Kurt

  14. Izabela Stroe: Worcester Polytechnic Institute

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    Izabela Stroe: Worcester Polytechnic Institute Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Izabela Stroe: Worcester Polytechnic Institute Former postdoc, now collaborator November 1, 2014 Izabela Stroe Izabela Stroe Contact Linda Anderman Email Izabela Stroe Izabela Stroe now at Worcester Polytechnic Institute Izabela Stroe's history with the Lab dates back to 2001 and over the years she's been a summer student,

  15. Jack Rains | Y-12 National Security Complex

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

    Jack Rains Jack Rains Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Jack Rains Recalls

  16. Jefferson Lab adds three popular presentations to Fall Science Series

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    line-up | Jefferson Lab adds three popular presentations to Fall Science Series line-up October 9, 2002 Three popular presentations have been added to Jefferson Lab's Fall Science Series schedule. Each one promises to be a stimulating, educational foray into scientific topics, says Linda Ware, Lab Public Affairs manager. On Wednesday Oct. 23, Sean M. Carroll from the University of Chicago's Center for Cosmological Physics, brings to the Lab his discussion of "Dark Energy and the

  17. Clot Busting Simulations Test Potential Stroke Treatment

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    Clot Busting Simulations Test Potential Stroke Treatment Clot Busting Simulations Test Potential Stroke Treatment September 24, 2013 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov Calvariasetup.jpg The array transducer in position above the calvaria (skull). Shown are the ends of the array elements above the computational model of the skull. Researchers are using computer simulations to investigate how ultrasound and tiny bubbles injected into the bloodstream might break up blood clots,

  18. Elmer Brummitt | Y-12 National Security Complex

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    Elmer Brummitt Elmer Brummitt Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Elmer

  19. Empty Bowl Project needs volunteers and attendees

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    Empty Bowl Project Needs Volunteers and Attendees Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Empty Bowl Project needs volunteers and attendees Volunteers are needed during the evening of March 15 to help set up the kitchen and on March 16 to assist cleanup. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email In

  20. Espanola Public School teachers strengthen skills during summer session

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    Espanola Public School Teachers Strengthen Skills Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Espanola Public School teachers strengthen skills during summer session Elementary- through high-school teachers attended a workshop designed to help them better understand and teach earth and space science. September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email

  1. Donald Raby | Y-12 National Security Complex

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

    Donald Raby Donald Raby Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Donald Raby Don's

  2. Donate used career clothes to help others through October 15

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    Donate Used Career Clothes to Help Others Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Donate used career clothes to help others through October 15 Accelerate is currently accepting donations of gently used business clothing to help men and women transition into the workforce. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt

  3. Dorothy Coker | Y-12 National Security Complex

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    Dorothy Coker Dorothy Coker Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Dorothy Coker

  4. Early Childhood Experiences Conference on October 30

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    Early Childhood Experiences Conference Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Early Childhood Experiences Conference on October 30 Los Alamos National Laboratory Foundation's First Born Program presents "Understanding Early Childhood Experiences as a Primary Public Health Concern." October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community

  5. Eastport Customs Brokers Win Small Business Award | Jefferson Lab

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    Eastport Customs Brokers Win Small Business Award Cynthia Keppel Jefferson Lab Chief Operating Officer Mike Dallas presents Eastport Customs Brokers, Inc., with the Jefferson Science Associates Outstanding Small Business Subcontractor award for 2011. Accepting the award is Eastport Customs' co-owner Linda Jennings (from left), associate Patricia L. Smith, and co-owner Margaret Adams. Jefferson Lab photo NEWPORT NEWS, VA, June 26, 2012 - Jefferson Science Associates, the management and operations

  6. Ed Bailey | Y-12 National Security Complex

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    Ed Bailey Ed Bailey Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Ed Bailey A close

  7. Effective Teaching Conference on October 11-12

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    Effective Teaching Conference Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Effective Teaching Conference on October 11-12 Los Alamos National Laboratory Foundation's 15th annual conference on education will feature Harry K. Wong and Rosemary Wong as keynote speakers. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus

  8. ARM - Field Participants

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    Field Participants Campaign Details News Field Participants Resources Status and Actions ARM Data Discovery Browse Data Field Participants Alexander, Liz Pacific Northwest National Laboratory/EMSL (509) 376-1576 Andrews, Betsy NOAA/Cooperative Institute for Environmental Research (303) 497-5171 Berg, Larry Pacific Northwest National Laboratory (509) 375-3916 Berkowitz, Carl Pacific Northwest National Laboratory (509) 372-6183 Bowerman, Linda Brookhavan National Laboratory (631) 344-5576 Chen, Qi

  9. Frontiers in Science Lectures

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    Frontiers in Science Lectures Frontiers in Science Lectures x Linda Anderman (505) 665-9196 Email The Frontiers in Science lecture series are a public service of the Los Alamos National Laboratory Fellows. Fellows are appointed by the Laboratory Director in recognition of sustained outstanding contributions and exceptional promise for continued professional achievement. All lectures are open to the public and free of charge. LATEST LECTURE Hacking Photosynthesis: Growing Plants to Power Our

  10. Jim Bailey | Y-12 National Security Complex

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    Jim Bailey Jim Bailey Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Jim Bailey Gives a

  11. Naomi Brummit | Y-12 National Security Complex

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

    Naomi Brummit Naomi Brummit Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Naomi Brummitt

  12. Nathan Henry | Y-12 National Security Complex

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

    Nathan Henry Nathan Henry Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Nathan Henry A

  13. A Massive Stellar Burst Before the Supernova

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    A Massive Stellar Burst Before the Supernova A Massive Stellar Burst Before the Supernova February 6, 2013 Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402 An automated supernova hunt is shedding new light on the death sequence of massive stars-specifically, the kind that self-destruct in Type IIn supernova explosions. Digging through the Palomar Transient Factory (PTF) data archive housed at the Department of Energy's National Energy Research Scientific Computing Center (NERSC) at Lawrence

  14. A Roadmap for Engineering Piezoelectricity in Graphene

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    Roadmap for Engineering Piezoelectricity in Graphene A Roadmap for Engineering Piezoelectricity in Graphene Doping this 'Miracle Material' May Lead to New Array of Nanoscale Devices, Simulations Reveal February 23, 2012 Linda Vu, lvu@lbl.gov, +1 510 495 2402 This illustration shows lithium atoms (red) doped on graphene (black hexagons) and generating electricity. Graphic courtesy of Mitchell Ong, Stanford University. Some scientists refer to graphene as the "miracle material" of the

  15. A Standard for Neuroscience Data

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    A Standard for Neuroscience Data A Standard for Neuroscience Data Berkeley Lab researchers have developed a computational framework for standardizing neuroscience data worldwide December 16, 2014 Contact: Linda Vu, +1 510 495 2402, lvu@lbl.gov Neural1.jpg Image Credit: Wikimedia Commons Thanks to standardized image file formats-like JPEG, PNG or TIFF-which store information every time you take a digital photo, you can easily share selfies and other pictures with anybody connected to a computer,

  16. Larry Case | Y-12 National Security Complex

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    Larry Case Larry Case Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Larry Case Jack

  17. Learn about Lab research at this year's LDRD Day on October 23

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    Learn About Lab Research At LDRD Day Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Learn about Lab research at this year's LDRD Day on October 23 Attendees will be able to view more than 30 posters that highlight current Laboratory research and vote for their favorite one. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt

  18. Looking forward to 2014

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    Looking forward to 2014 Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Looking forward to 2014 A personal message from the Community Programs Office December 1, 2013 Kurt Steinhaus, Community Programs Office Director Kurt Steinhaus, Community Programs Office Director Contacts Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email While 2013 was a very successful

  19. Los Alamos High School team wins 2013 New Mexico Science Bowl

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    High School team wins New Mexico Science Bowl Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos High School team wins 2013 New Mexico Science Bowl Team heads to national competition in Washington, D.C. March 1, 2013 Los Alamos High School wins regional Science Bowl. Los Alamos High School wins regional Science Bowl. Contacts Editor Linda Anderman Email Community Programs Office Kurt

  20. Los Alamos Middle School team wins regional MathCounts competition

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    Los Alamos Middle School team wins Regional MathCounts competition Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos Middle School wins regional MathCounts event Competes against 60 other middle schools for the title. March 1, 2013 Los Alamos Middle School won the regional MathCounts competition. Los Alamos Middle School won the regional MathCounts competition. Contacts Editor Linda

  1. Los Alamos Public Schools recommended for accreditation

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    Los Alamos Schools Recommended For Accreditation Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos Public Schools recommended for accreditation Los Alamos Public Schools has taken the unusual step of working to obtain accreditation for its entire district. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email We

  2. Los Alamos STEM Challenge registration due April 12

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    Los Alamos STEM Challenge registration due April 12 Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos STEM Challenge registration due April 12 Submission deadline April 30. April 1, 2013 Two students at work on a laptop Videos, posters, apps and essays are all possible submissions for the upcoming STEM Challenge for students. Contact Editor Linda Anderman Email Community Programs Office

  3. Los Alamos physicist Hockaday honored for national security contributions

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    Los Alamos physicist Hockaday honored for national security contributions Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Los Alamos physicist Hockaday honored for national security contributions Hockaday earned a 2014 fellowship from the AAAS and also a Distinguished Alumni Award from the NMSU Alumni Association January 1, 2015 Mary Hockaday Mary Hockaday Contact Linda Anderman Email Associate Director for

  4. Los Alamos scientists advance biomass fuel production

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    Los Alamos scientists advance biomass fuel production Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Los Alamos scientists advance biomass fuel production Adapting biomass waste molecules for energy production May 1, 2013 Lab research can yield energy from non-food biomass Lab research can yield energy from non-food biomass Contact Editor Linda Anderman Email Community Programs Office Kurt

  5. Louis Freels | Y-12 National Security Complex

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    Louis Freels Louis Freels Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Louis Freels A

  6. Lowe's "Toolbox for Education" grant applications due by October 12

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    Lowe's "Toolbox for Education" Grant Applications Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lowe's "Toolbox for Education" grant applications due by October 12 Five million dollars is available for the 2012-13 school year. September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Over the past

  7. John Rice Irwin, part 1 | Y-12 National Security Complex

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    1 John Rice Irwin, part 1 Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript John Rice

  8. John Rice Irwin, part 2 | Y-12 National Security Complex

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

    2 John Rice Irwin, part 2 Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript John Rice

  9. Join our highlighted LinkedIn discussion

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    Join our highlighted LinkedIn discussion Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Join our highlighted LinkedIn discussion What experiences have alumni had in software releases and deployments at different institutions? March 1, 2015 Robert Jilek Robert Jilek Contact Linda Anderman Email alumni LinkedIn Join us for a variety of discussions on the Lab's LinkedIn Alumni page What experiences have alumni had in

  10. Join our highlighted LinkedIn discussion

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

    Join our highlighted LinkedIn discussion Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Join our highlighted LinkedIn discussion Congratulations to LANL's Claudia Mora for being selected president elect of the Geological Society of America! July 1, 2015 Claudia Mora Claudia Mora Contact Linda Anderman Email alumni LinkedIn Join us for a variety of discussions on the Lab's LinkedIn Alumni page Congratulations to

  11. Katharine Page: Atomic-level insights for better materials

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    Katharine Page: Atomic-level insights for better materials Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Katharine Page: Atomic-level insights for better materials Page's research supports materials' advances that could have wide-ranging impact, investigating, manipulating and manufacturing nano-particles. May 1, 2014 Katherine Page Katherine Page Contact Linda Anderman Email A Love for Science Impassioned by

  12. Katherine Lovejoy: FDA

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    Katherine Lovejoy: FDA Alumni Link: Opportunities, News and Resources for Former Employees Latest Issue:September 2015 all issues All Issues » submit Katherine Lovejoy: FDA Former postdoc now at the Food and Drug Administration June 20, 2014 Katherine Lovejoy Katherine Lovejoy Contact Linda Anderman Email Katherine Lovejoy now with the Food and Drug Administration's Center for Tobacco Products Katherine Lovejoy Katherine Lovejoy is currently a chemist with the Food and Drug Administration's

  13. Kay Bailey | Y-12 National Security Complex

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    Bailey Kay Bailey Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Kay Bailey Housekeeper

  14. Kay Steed | Y-12 National Security Complex

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

    Steed Kay Steed Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Kay Steed Secretary to Jack

  15. Keeping comets and asteroids at bay

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    Keeping Comets And Asteroids At Bay Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Keeping comets and asteroids at bay Every two years, experts from around the globe convene at the Planetary Defense Conference. August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Every two years, experts from around the globe convene at

  16. Keeping terrorists from putting us in the dark

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    Keeping terrorists from putting us in the dark Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Keeping terrorists from putting us in the dark Lab research helps keep electrical grid secure. April 1, 2013 Power lines Lab research helps protect the grid. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email While there is potential that terrorists could target the

  17. Ken Bernander | Y-12 National Security Complex

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    Bernander Ken Bernander Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Ken Bernander Tells

  18. Ken Sommerfeld | Y-12 National Security Complex

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

    Sommerfeld Ken Sommerfeld Oral History Videos Speakers INTRODUCTION Ed Bailey Jim Bailey Kay Bailey Ken Bernander Willard Brock Wilma Brooks Elmer Brummitt Naomi Brummitt Blake Case Larry Case Patrick Case Dorothy Coker Gordon Fee Linda Fellers Louis Freels Marie Guy Nathan Henry Agnes Houser John Rice Irwin Harvey Kite Charlie Manning Alice Piercey Donald Raby Jack Rains Ray Smith Ken Sommerfeld Kay Steed Bill Wilcox Beverly Woods more ... Options Hide Chapters Show Transcript Ken Sommerfeld

  19. LANL assists with resource and job event in Espanola

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    Resource and Job Event In Espanola Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit LANL assists with resource and job event in Espanola The event was designed to help attendees meet potential employers, discover new employment resources, and increase expertise in job-search skills and resume development. November 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email

  20. LANL sets waste shipping record for fourth consecutive year

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    LANL Sets Waste Shipping Record Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit LANL sets waste shipping record for fourth consecutive year The Laboratory has transported more than 1,000 shipments to WIPP since that facility opened in 1999. September 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Our goal this fiscal year

  1. Lab celebrates Earth Day

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    Lab celebrates Earth Day Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lab celebrates Earth Day Multiple activities focus on environmental protection. May 1, 2013 A team from Industrial Hygiene and Safety during the Great Garbage Grab A team from Industrial Hygiene and Safety during the Great Garbage Grab. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Great

  2. Lab makes understanding the complexity of wind power "A breeze"

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    Understanding the Complexity of Wind Power Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lab makes understanding the complexity of wind power "A breeze" Loren Toole has been working with a group of ranchers and other landowners in eastern New Mexico to help them evaluate their renewable energy resources. October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman

  3. Lab sets new record for waste volume removed

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    Lab Sets New Record for Waste Volume Removed Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lab sets new record for waste volume removed The Transuranic Waste Program has met its commitment to ship 800 cubic meters of TRU waste to the Waste Isolation Pilot Plant during fiscal year 2012. November 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office

  4. Lab subcontractor a major asset to Northern New Mexico

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    Lab Subcontractor Major Asset To Northern New Mexico Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lab subcontractor a major asset to Northern New Mexico Adelante Consulting, Inc. holds Laboratory contracts for environmental work and supports more than 30 regional nonprofit organizations. August 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs

  5. Lab transitions employee giving campaigns

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    Lab transitions employee giving campaigns Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit Lab transitions employee giving campaigns This year's theme: "I Give Because..." November 1, 2013 Employee Giving Logo The theme for this year's employee giving campaigns Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email During the past seven years

  6. Site Map

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    Home » Site Map Site Map Home About Overview NERSC Mission Contact us Staff Center Leadership Sudip Dosanjh Sudip Dosanjh: Select Publications Jeff Broughton Katie Antypas Richard Gerber Publications John Shalf Center Administration James Craw Norma Early Jeff Grounds Betsy MacGowan Zaida McCunney Kerri Peyovich Lynn Rippe David Tooker Center Communications Jon Bashor Kathy Kincade Linda Vu Margie Wylie Advanced Technologies Nicholas Wright Brian Austin Research Projects Christopher Daley Glenn

  7. Staff > Scientific Advisory Board > The Energy Materials Center at Cornell

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    Scientific Advisory Board List Image Michelle Buchanan Oak Ridge National Laboratory List Image Gary Calabrese Corning Inc. List Image Thomas Mallouk Pennsylvania State University List Image Mark Mathias General Motors - Fuel Cell Research List Image Linda Nazar University of Waterloo List Image Bart Riley A123 Systems List Image Eugene Smotkin Northeastern University List Image Esther Takeuchi Stony Brook University List Image M. Stanley Whittingham Binghamton University List Image Piotr

  8. Upcoming Seminars | Savannah River Ecology Laboratory

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    Upcoming Seminars Seminars will be held at the Savannah River Ecology Laboratory, Bldg. 737-A, in the Cypress Room, at 3:30 PM. Snacks will be provided at 3:15. DATE SPEAKER TITLE 3:30 PM Thursday, March 17, 2016 Dan Quinn, MS Candidate, SREL/Warnell School of Forestry and Natural Resources, UGA Head-starting as a conservation tool for Gopher Tortoises (Gopherus polyphemus) SREL seminar committee: Dr. Gary Mills (chair), Margaret Wead, Linda Lee, Wes Flynn

  9. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues 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

  10. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In Other News Help us make Connections better! October 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Help us make Connections better! Periodically, we like to get feedback on this publication so we can make it even better and more useful to you. Well, that

  11. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In Other News Richard Marquez Leadership and Service Award established at NNMC; Lab employees recognized for Mars Rover contribution; Connections survey feedback results. November 1, 2012 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Richard Marquez Leadership and

  12. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In Other News New Lab program reinforces safety behavior; Laboratory Fellows announced. January 1, 2013 dummy image Read our archives Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email Chuck, Steven, and Mikhail have made exceptional contributions in their fields and to national security. New Lab

  13. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In Other News Community Leaders survey results; NNSA orders security enhancements; Scientists awarded Fellowships from APS. February 1, 2013 dummy image Read our archives. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The American Physical Society recognized 10 Laboratory scientists for

  14. In Other News

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    In Other News Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In Other News Lecture on Sandia Lab history; LANL Foundation personnel changes. March 1, 2013 Rebbecca Ullrich is Sandia National Laboratories' historian Rebbecca Ullrich is Sandia National Laboratories' historian. Contacts Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email The Bradbury Science Museum's next

  15. In other news

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    In other news Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In other news Environmental sustainability, Science Bowl winners and new Pinterest site. April 1, 2013 The Lab's Pinterest site The Lab's Pinterest site. Contact Editor Linda Anderman Email Community Programs Office Kurt Steinhaus Email 2013 Site Sustainability Plan released The Lab looked 50 years into the future to write a strategy

  16. In other news

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    In other news Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In other news Connections has a new title, winners of the Robot Rodeo, local firm gets large grant and new kits available for regional teachers July 1, 2013 A new STEM teacher kit is being distributed throughout the region A new STEM teacher kit is being distributed throughout the region Contact Editor Linda Anderman Email Community

  17. In other news

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    In other news Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In other news Readers' survey, protecting Lab bird residents and major media mentions December 1, 2013 Community Connections readers' survey Please participate in our readers' survey Contacts Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email Community Connections readers survey - please let your voice

  18. In other news

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    In other news Community Connections: Your link to news and opportunities from Los Alamos National Laboratory Latest Issue:Mar. 2016 all issues All Issues » submit In other news Science Cinema, crowdfunding and giving programs wrap up February 1, 2014 Crowdsourcing class at UNM-LA The Bradbury Science Museum in Los Alamos Contact Community Programs Office Director Kurt Steinhaus Email Editor Linda Anderman Email Lab supports local business through crowdfunding class A recent crowdfunding course

  19. Changes in Vegetation at the Monticello, Utah, Disposal Site | Department

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

    of Energy Changes in Vegetation at the Monticello, Utah, Disposal Site Changes in Vegetation at the Monticello, Utah, Disposal Site Changes in Vegetation at the Monticello, Utah, Disposal Site Linda Sheader and Marilyn Kastens PDF icon Changes in Vegetation at the Monticello, Utah, Disposal Site More Documents & Publications Study of Factors Affecting Shrub Establishment on the Monticello, Utah, Disposal Cell Cover Monitoring the Performance of an Alternative Landfill Cover at the

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

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    CNSM UEC Meeting Minutes 26 Sept 08 Meeting of the CNMS User Executive Committee September 26, 2008 Room 214, ORNL Visitor Center (bldg 5200) Present: Yoke Khin Yap (Chair), Haiping Cheng (Vice-Chair), David Bucknall (secretary), Tony Hmelo, Alamgir Karim, 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). Apologies: Mark Dadmun, Cheol Park  The meeting was called to order at