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Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
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1

Contributors 7:2  

E-Print Network (OSTI)

CONTRIBUTORS Lome Cappe is an architect with the city ofOntario Association of Architects and the Royal Architec-Richard Gilbert an architect and artist, is professor at the

1991-01-01T23:59:59.000Z

2

CONTRIBUTORS (*)  

E-Print Network (OSTI)

This is a preprint of a paper intended for presentation at a scientific meeting. Because of the provisional nature of its content and since changes of substance or detail may have to be made before publication, the preprint is made available on the understanding that it will not be cited in the literature or in any way be reproduced in its present form. The views expressed and the statements made remain the responsibility of the named author(s); the views do not necessarily reflect those of the government of the designating Member State(s) or of the designating organization(s). In particular, neither the IAEA nor any other organization or body sponsoring this meeting can be held responsible for any material reproduced in this preprint. Topic: EX/1-4Ra

E. Joffrin; J. Hobirk; M. Brix; P. Buratti; C. D. Challis; F. Crisanti; C. Giroud; M. Gryaznevitch; T. C. Hender; F. Imbeaux; T. Luce; P. Mantica; D. C. Mcdonald; S. D. Pinches; S. Saarelma; A. C. C. Sips; F. Villone

2008-01-01T23:59:59.000Z

3

[Contributors  

E-Print Network (OSTI)

Joanna Dvila naci en Humacao, Puerto Rico. En sus estudiosel Universidad de Puerto Rico, Recinto de Ro Piedras. Ende la Repblica Dominicana y Puerto Rico. MESTER, VOL. XXXVI

Mester, [No author

2007-01-01T23:59:59.000Z

4

Centro De Energias Renovables (CER): A Major OpenEI Contributor | OpenEI  

Open Energy Info (EERE)

Centro De Energias Renovables (CER): A Major OpenEI Contributor Centro De Energias Renovables (CER): A Major OpenEI Contributor Home > Groups > OpenEI Community Central Graham7781's picture Submitted by Graham7781(1992) Super contributor 18 March, 2010 - 12:25 imported OpenEI OpenEI continues to expand and grow, and recently a new partnership between the Centro De Energias Renovables (CER) in Santiago, Chile and the international group at the National Renewable Energy Laboratory (NREL) in Golden, Colorado has led to the creation of a Latin American gateway on OpenEI.org, where users in Spanish-speaking countries can upload their data. The CER is focused on developing and growing the Latin American community around OpenEI by holding training sessions, and communicating with NREL's international group and community building team on ways to improve the

5

Contributors to the Dictionary of Algorithms and Data ...  

Science Conference Proceedings (OSTI)

Contributors to the Dictionary of Algorithms, Data Structures, and Classical Computer Science problems, with some contact information. NIST. ...

2013-11-08T23:59:59.000Z

6

Using Analogy to Acquire Commonsense Knowledge from Human Contributors  

E-Print Network (OSTI)

The goal of the work reported here is to capture the commonsense knowledge of non-expert human contributors. Achieving this goal will enable more intelligent human-computer interfaces and pave the way for computers to ...

Chklovski, Timothy

2003-02-12T23:59:59.000Z

7

OE Contributors Named IEEE Fellows | Department of Energy  

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

Contributors Named IEEE Fellows Contributors Named IEEE Fellows OE Contributors Named IEEE Fellows February 29, 2012 - 3:51pm Addthis Two Electric Power Research Institute (EPRI) executives who have worked with OE-funded projects were recently named fellows of the Institute of Electrical and Electronics Engineers (IEEE). Dr. Ram Adapa, technical leader for transmission systems, and Mark McGranaghan, vice president of Power Delivery & Utilization for EPRI were recognized for their contributions to IEEE fields of interest. Dr. Ram Adapa was recognized for leadership in direct current and flexible AC transmission systems. Dr. Adapa, through his technical leadership and innovative research ideas, has contributed significantly to the advancement of high-voltage direct current transmission and flexible AC transmission

8

Office of Electricity Delivery & Energy Reliability Contributors |  

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

Office of Electricity Delivery & Energy Reliability » Office of Office of Electricity Delivery & Energy Reliability » Office of Electricity Delivery & Energy Reliability Contributors Office of Electricity Delivery & Energy Reliability Contributors June 20, 2012 David Ortiz, OE-40 David Ortiz is Deputy Assistant Secretary for Energy Infrastructure Modeling and Analysis (EIMA) in the Department of Energy's Office of Electrici April 25, 2013 Eric Lightner June 22, 2011 Henry S. Kenchington, OE-50 Mr. Henry (Hank) Kenchington is Deputy Assistant Secretary (DAS) for the Advanced Grid Integration Division in the Department of Energy's Office of Electricity Delivery and Energy Reliability. He is responsible for the strategic management of the $3.4 billion Smart Grid Investment Grant program funded under the American Recovery and Reinvestment Act of 2009 to

9

Bulletin of Tibetology: Volume 3 Number 2 : Cover, contents, contributors  

E-Print Network (OSTI)

, Waterloo Lutheran University and University of Waterloo (Canada); presently Professor of Geography, University of Kentucky (USA). NALINAKSHA DUTT Vice-President: Namgyal Institute of Tibeto logy; President: Asiatic Society, Calcutta 1958-60; formerly... '1. CONTRIBUTORS IN THIS ISSUE- PRADYUMNA P. KARAN Authority on Himalayan geography; visited several times and written on Bhutan, Sikkim and Nepal ; formerly Lecturer in Geography, Patna University (India) and Visiting Profe&sor at University of Manitoba...

Namgyal Institute of Tibetology

1966-07-21T23:59:59.000Z

10

Ian Foster Named One of the Top Three Contributors to Computer...  

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

Foster Named One of the Top Three Contributors to Computer Science August 16, 2007 Tweet EmailPrint Argonne researcher Ian Foster has been named one of the top three contributors...

11

Accident sequence precursor events with age-related contributors  

SciTech Connect

The Accident Sequence Precursor (ASP) Program at ORNL analyzed about 14.000 Licensee Event Reports (LERs) filed by US nuclear power plants 1987--1993. There were 193 events identified as precursors to potential severe core accident sequences. These are reported in G/CR-4674. Volumes 7 through 20. Under the NRC Nuclear Plant Aging Research program, the authors evaluated these events to determine the extent to which component aging played a role. Events were selected that involved age-related equipment degradation that initiated an event or contributed to an event sequence. For the 7-year period, ORNL identified 36 events that involved aging degradation as a contributor to an ASP event. Except for 1992, the percentage of age-related events within the total number of ASP events over the 7-year period ({approximately}19%) appears fairly consistent up to 1991. No correlation between plant ape and number of precursor events was found. A summary list of the age-related events is presented in the report.

Murphy, G.A.; Kohn, W.E.

1995-12-31T23:59:59.000Z

12

Super Heavy Element Discovery | ornl.gov  

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

Super Heavy Element Discovery SHARE Super Heavy Element Discovery The location of the Transactinides (super-heavy elements) shown on the Periodic Table. ORNL is internationally...

13

US ITER is a strong contributor in plan to enhance international...  

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

American Fusion News Category: U.S. ITER Link: US ITER is a strong contributor in plan to enhance international sharing of prime ITER real estate...

14

Double-super-connected digraphs  

Science Conference Proceedings (OSTI)

A strongly connected digraph D is said to be super-connected if every minimum vertex-cut is the out-neighbor or in-neighbor set of a vertex. A strongly connected digraph D is said to be double-super-connected if every minimum vertex-cut is both the out-neighbor ... Keywords: Cartesian product, Double-super-connected, Lexicographic product, Line digraphs, Super-connected

Juan Liu; Jixiang Meng; Zhao Zhang

2010-05-01T23:59:59.000Z

15

(SUPER) W Algebras from Non Abelian (SUPER) Toda Theories  

E-Print Network (OSTI)

A classification of (super) $W$ algebras arising from non Abelian Toda and super Toda theories is presented. This classification is based on the $Sl(2)$ or $OSp(1|2)$ sub(super)algebras of the simple Lie (super)algebra underlying the model. This allows to compute the conformal spin content of each $W$ (super)algebra. {\\em Based on two lectures given by L. Frappat and E. Ragoucy at the\\\\ XIX International Colloquium on Group Theoretical Methods in Physics\\\\ Salamanca (Spain), June 29 - July 4, 1992}

Frappat, L; Sorba, Paul

1992-01-01T23:59:59.000Z

16

EUROv Super Beam Studies  

Science Conference Proceedings (OSTI)

Neutrino Super Beams use conventional techniques to significantly increase the neutrino beam intensity compared to the present neutrino facilities. An essential part of these facilities is an intense proton driver producing a beam power higher than a MW. The protons hit a target able to accept the high proton beam intensity. The produced charged particles are focused by a system of magnetic horns towards the experiment detectors. The main challenge of these projects is to deal with the high beam intensity for many years. New high power neutrino facilities could be build at CERN profiting from an eventual construction of a high power proton driver. The European FP7 Design Study EUROv, among other neutrino beams, studies this Super Beam possibility. This paper will give the latest developments in this direction.

Dracos, Marcos [IPHC, Universite de Strasbourg, CNRS/IN2P3, F-67037 Strasbourg (France)

2011-10-06T23:59:59.000Z

17

JGI - Prokaryote Super Program  

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

Prokaryote Super Program Prokaryote Super Program While the sequencing and assembly strategies for the Microbial Genomics and Metagenomics Programs are quite different, the scientific goals of the two programs are very much aligned with an underlying common objective to understand the structure and function of microorganisms and microbial communities with mission relevance to the Department of Energy. To achieve this, scientists in the program are pursuing the sequencing of nucleic acids from both individual microbes and entire communities of organisms. This combined approach offers unique opportunities to the scientific community, but also requires coordinated activities between metagenomic and individual microbial genome sequence generation and data analysis. To capitalize on these emerging opportunities, JGI recently merged the two

18

Super Storm Sandy  

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

Super Storm Sandy Super Storm Sandy JOHN DAVIS: Heavy rain, high winds, and surging waters pummeled the eastern seaboard in November of 2012 as hurricane Sandy chewed up the east coast leaving in its wake a swath of loss and destruction. In advance of this "storm of the century" the demand for gasoline spiked as thousands were forced to evacuate and many others stocked up on their fuel for their portable generators. After the storm passed, power outages and a crippled delivery infrastructure let to gas shortages that lasted for weeks hindering cleanup efforts and paralyzing entire cities. Atlantic City, NJ took a heavy toll in physical damage with numerous homes and boardwalk attractions damaged beyond repair. But, thanks to a program that began in 2009 the city?s recovery began more quickly than most. Atlantic City's

19

Los Alamos National Laboratory again top contributor to United Way of Santa  

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

LANL top contributor LANL top contributor Los Alamos National Laboratory again top contributor to United Way of Santa Fe County Employees and LANS, LLC donated $113,000 to the United Way of Santa Fe County's giving campaign. July 1, 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 multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. 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 multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. Contact Steve Sandoval

20

SuperB Progress Report: Detector  

SciTech Connect

This report describes the present status of the detector design for SuperB. It is one of four separate progress reports that, taken collectively, describe progress made on the SuperB Project since the publication of the SuperB Conceptual Design Report in 2007 and the Proceedings of SuperB Workshop VI in Valencia in 2008.

Grauges, E.; /Barcelona U., ECM; Donvito, G.; Spinoso, V.; /INFN, Bari /Bari U.; Manghisoni, M.; Re, V.; Traversi, G.; /INFN, Pavia /Bergamo U., Ingengneria Dept.; Eigen, G.; Fehlker, D.; Helleve, L.; /Bergen U.; Carbone, A.; Di Sipio, R.; Gabrielli, A.; Galli, D.; Giorgi, F.; Marconi, U.; Perazzini, S.; Sbarra, C.; Vagnoni, V.; Valentinetti, S.; Villa, M.; Zoccoli, A.; /INFN, Bologna /Bologna U. /Caltech /Carleton U. /Cincinnati U. /INFN, CNAF /INFN, Ferrara /Ferrara U. /UC, Irvine /Taras Shevchenko U. /Orsay, LAL /LBL, Berkeley /UC, Berkeley /Frascati /INFN, Legnaro /Orsay, IPN /Maryland U. /McGill U. /INFN, Milan /Milan U. /INFN, Naples /Naples U. /Novosibirsk, IYF /INFN, Padua /Padua U. /INFN, Pavia /Pavia U. /INFN, Perugia /Perugia U. /INFN, Perugia /Caltech /INFN, Pisa /Pisa U. /Pisa, Scuola Normale Superiore /PNL, Richland /Queen Mary, U. of London /Rutherford /INFN, Rome /Rome U. /INFN, Rome2 /Rome U.,Tor Vergata /INFN, Rome3 /Rome III U. /SLAC /Tel Aviv U. /INFN, Turin /Turin U. /INFN, Padua /Trento U. /INFN, Trieste /Trieste U. /TRIUMF /British Columbia U. /Montreal U. /Victoria U.

2012-02-14T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

US ITER is a strong contributor in plan to enhance international sharing of  

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

US ITER is a strong contributor in plan to enhance international sharing of US ITER is a strong contributor in plan to enhance international sharing of prime ITER real estate By Lynne Degitz, US ITER March 28, 2013 Tweet Widget Facebook Like Google Plus One PPPL's Russell Feder, left, and David Johnson developed key features for a modular approach to housing the extensive diagnostic systems that will be installed on the ITER tokamak. (Photo by Elle Starkman/PPPL Office of Communications) PPPL's Russell Feder, left, and David Johnson developed key features for a modular approach to housing the extensive diagnostic systems that will be installed on the ITER tokamak. Gallery: Diagram of an equatorial port plug shows the three vertical diagnostic shield modules with detachable first wall blocks. The modular approach has many advantages including efficient design collaboration, easier maintenance and the possibility for future upgrades to the ITER diagnostic systems.

22

SOWFA + Super Controller User's Manual  

DOE Green Energy (OSTI)

SOWFA + Super Controller is a modification of the NREL's SOWFA tool which allows for a user to apply multiturbine or centralized wind plant control algorithms within the high-fidelity SOWFA simulation environment. The tool is currently a branch of the main SOWFA program, but will one day will be merged into a single version. This manual introduces the tool and provides examples such that a user can implement their own super controller and set up and run simulations. The manual only discusses enough about SOWFA itself to allow for the customization of controllers and running of simulations, and details of SOWFA itself are reported elsewhere Churchfield and Lee (2013); Churchfield et al. (2012). SOWFA + Super Controller, and this manual, are in alpha mode.

Fleming, P.; Gebraad, P.; Churchfield, M.; Lee, S.; Johnson, K.; Michalakes, J.; van Wingerden, J. W.; Moriarty, P.

2013-08-01T23:59:59.000Z

23

Washington, D.C.Abandoned Mine Site Characterization and Cleanup Handbook Contributors  

E-Print Network (OSTI)

(Handbook) is the result of the collective efforts and contributions of a number of individuals. During the earliest days of Handbook development, Mike Bishop of EPA Region 8 lead the effort to develop a Superfund Mine Waste Reference Document for EPA project managers working on mine site cleanup. That effort evolved into the Handbook in recognition of the many regulatory and non-regulatory mechanisms that are used today to manage the characterization and cleanup of mines sites. Users are encouraged to consider the information presented in the Handbook against the backdrop of site specific environmental and regulatory factors. The Handbook has been developed as a source of information and ideas for project managers involved in the characterization and cleanup of inactive mine sites. It is not guidance or policy. The list that follows acknowledges the efforts of writers, reviewers, editors, and other contributors that made development of the Handbook possible. It is always a bit risky to develop a list of contributors because it is inevitable

Attn Of; Nick Ceto; Shahid Mahmud; Fred Macmillan; Brad Bradley; Shawn Ghose; Mark Doolan; Mike Bishop; Matt Cohn; Carol Russ; Jim Dunn; Elisabeth Evans; Holly Fliniau; Eva Hoffman; Sonya Pennock; Mike Holmes; Andy Lensink; Ken Wangerud; Sara Weinstock; Chris Weis; Patti Collins; Ken Greenberg; Mike Hingerty; Nick Ceto; Bruce Duncan; Earl Liverman; Roseanne Lorenzana; Patty Mcgrath; Don Metheny

2000-01-01T23:59:59.000Z

24

Polarimetery for SuperB  

SciTech Connect

We provide an overview description of a Compton polarimeter for measuring electron beam polarization near the IR in the Low Energy Ring of SuperB. The polarimeter is designed to achieve 1.0% accuracy. A scheme for measuring the electron beam polarization at SuperB near the IR has been described. The Compton polarimeter has been designed to fit into the existing lattice of the SuperB ring and results in a Compton IP measuring the polarization located where the beam is almost longitudinal with opposite helicity to that at the IR. The polarization at the IR is expected to be determined with an accuracy of {approx}1% from the measurement at the Compton IP provided the beam direction at the electron-positron interaction region and the Compton IP are well known and the beam energy is measured to better than 20 MeV. Detailed detector studies are needed to study resolution and acceptance effects on detector analyzing powers, and to determine sensitivity to beam and machine parameters.

Sullivan, Michael; /SLAC; Field, R.; /SLAC; Moffeit, Kenneth; /SLAC; Nosochkov, Yuri; /SLAC; Wienands, Ulrich; /SLAC; Wittmer, Walter; /SLAC; Woods, Mike; /SLAC

2012-07-06T23:59:59.000Z

25

Super Projects (Arkansas) | Department of Energy  

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

Super Projects (Arkansas) Super Projects (Arkansas) Super Projects (Arkansas) < Back Eligibility Construction Industrial Installer/Contractor Investor-Owned Utility Savings Category Alternative Fuel Vehicles Hydrogen & Fuel Cells Buying & Making Electricity Water Home Weatherization Solar Program Info State Arkansas Program Type Bond Program Provider Department of Economic Develoment A 2004 amendment to the state constitution authorizes the state to attract super projects by issuing bonds to fund a project's infrastructure, limited to 5% of the net general revenues during the most recent fiscal year. Super projects are defined as ones that create at least 500 new jobs and invest more than $500 million. Examples of the type of projects that might meet the criteria for a super project and have infrastructure needs

26

Super Wi-Fi is Super for Energy Too | Department of Energy  

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

Super Wi-Fi is Super for Energy Too Super Wi-Fi is Super for Energy Too Super Wi-Fi is Super for Energy Too September 24, 2010 - 11:45am Addthis Super Wi-Fi is Super for Energy Too Nick Sinai Senior Advisor to the U.S. Chief Technology Officer, White House Office of Science and Technology Policy What does this mean for me? By integrating broadband into the emerging Smart Grid, consumers will have revolutionized communication with their utility -- they will have detailed information on their energy use that will help inform them how they can save on their electric bills. Editor's Note: Cross-posted from the National Broadband Plan blog, which deals with how broadband technology will integrate into the smart grid. We at the FCC are very excited about yesterday's order to free up the unused "white spaces" spectrum between television channels, intended to

27

SuperProtonic | Open Energy Information  

Open Energy Info (EERE)

search Name SuperProtonic Place Pasadena, California Zip 91101 Product Established to market and commercialize the solid acid fuel cell (SAFC) technology developed and patented by...

28

DOE SuperTruck Program Benefits Analysis  

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

in the project's technical scope development, information collection, and analysis. He also served as the key technical contact point for the SuperTruck development...

29

Super Gabor frames on discrete periodic sets  

Science Conference Proceedings (OSTI)

Due to its potential applications in multiplexing techniques such as time division multiple access and frequency division multiple access, superframe has interested some mathematicians and engineering specialists. In this paper, we investigate super ... Keywords: 42C40, Discrete Zak transform, Discrete periodic sets, Gabor dual, Super Gabor frame, Superframe

Yun-Zhang Li; Qiao-Fang Lian

2013-05-01T23:59:59.000Z

30

Big Data, New Physics and Geospatial Super-Food  

Science Conference Proceedings (OSTI)

Big Data, New Physics and Geospatial Super-Food. Purpose: As ... amazing. As it turns out, geospatial data are analytic super-food. ...

2011-10-25T23:59:59.000Z

31

Convection feedbacks in a super-parameterization GCM  

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

and Goddard super-parameterization GCM (SP-GCM) simulate a super-active Asian summer monsoon with unrealistically enhanced levels of precipitation. The underlying physical...

32

Columbia Water & Light - Commercial Super Saver Loans | Department...  

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

Commercial Super Saver Loans Columbia Water & Light - Commercial Super Saver Loans Eligibility Commercial Fed. Government Industrial Nonprofit State Government Savings For Heating...

33

Columbia Water & Light - Residential Super Saver Loans | Department...  

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

Super Saver Loans Columbia Water & Light - Residential Super Saver Loans Eligibility Multi-Family Residential Residential Savings For Home Weatherization Commercial Weatherization...

34

Introduction to Measurement & Verification for DOE Super ESPC...  

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

in energy performance contracts is required in federal contracts such as the Super Energy Savings Performance Contracts (Super ESPCs). Since energy savings are "guaranteed,"...

35

The SuperCDMS Experiment  

SciTech Connect

Modest improvements in the level and/or discrimination of backgrounds are needed to keep backgrounds negligible during the three phases of SuperCDMS. By developing production designs that require only modest testing, detector production rates may be improved sufficiently to allow an exposure of 500 ton d within a reasonable time and budget. Overall, the improvement estimates described above are conservative. Previous development efforts have shown that some areas prove easier and provide larger factors while others prove more difficult. The conservative estimates together with the broad approach reduce the risk and give us confidence that we will succeed, providing the surest way to probe to WIMP-nucleon cross sections of 10{sup -46} cm{sup 2}.

Schnee, Richard W.; Akerib, D.S.; Attisha, M.J.; Bailey, C.N.; Baudis, L.; Bauer, Daniel A.; Brink, P.L.; Brusov, P.P.; Bunker, R.; Cabrera, B.; Caldwell, D.O.; Chang, C.L.; Cooley, J.; Crisler, M.B.; Cushman, P.; Denes, P.; Dragowsky, M.R.; Duong, L.; Filippini, J.; Gaitskell, R.J.; Golwala, S.R.; /Case Western Reserve U. /Brown U. /Florida U. /Fermilab /Stanford U., Phys. Dept. /UC, Santa Barbara /Minnesota U. /LBL, Berkeley /UC, Berkeley /Caltech /Colorado U., Denver /NIST, Boulder /Santa Clara U.

2005-02-01T23:59:59.000Z

36

SuperB Progress Report for Physics  

SciTech Connect

SuperB is a high luminosity e{sup +}e{sup -} collider that will be able to indirectly probe new physics at energy scales far beyond the reach of any man made accelerator planned or in existence. Just as detailed understanding of the Standard Model of particle physics was developed from stringent constraints imposed by flavour changing processes between quarks, the detailed structure of any new physics is severely constrained by flavour processes. In order to elucidate this structure it is necessary to perform a number of complementary studies of a set of golden channels. With these measurements in hand, the pattern of deviations from the Standard Model behavior can be used as a test of the structure of new physics. If new physics is found at the LHC, then the many golden measurements from SuperB will help decode the subtle nature of the new physics. However if no new particles are found at the LHC, SuperB will be able to search for new physics at energy scales up to 10-100 TeV. In either scenario, flavour physics measurements that can be made at SuperB play a pivotal role in understanding the nature of physics beyond the Standard Model. Examples for using the interplay between measurements to discriminate New Physics models are discussed in this document. SuperB is a Super Flavour Factory, in addition to studying large samples of B{sub u,d,s}, D and {tau} decays, SuperB has a broad physics programme that includes spectroscopy both in terms of the Standard Model and exotica, and precision measurements of sin{sup 2} {theta}{sub W}. In addition to performing CP violation measurements at the {Upsilon}(4S) and {phi}(3770), SuperB will test CPT in these systems, and lepton universality in a number of different processes. The multitude of rare decay measurements possible at SuperB can be used to constrain scenarios of physics beyond the Standard Model. In terms of other precision tests of the Standard Model, this experiment will be able to perform precision over-constraints of the unitarity triangle through multiple measurements of all angles and sides. This report extends and updates the studies presented in both the SuperB Conceptual Design Report in 2007 and the Proceedings of SuperB Workshop VI in Valencia in 2008. Together, these three documents detail the Physics case of the SuperB Project.

O'Leary, B.; /Aachen, Tech. Hochsch.; Matias, J.; Ramon, M.; /Barcelona, IFAE; Pous, E.; /Barcelona U.; De Fazio, F.; Palano, A.; /INFN, Bari; Eigen, G.; /Bergen U.; Asgeirsson, D.; /British Columbia U.; Cheng, C.H.; Chivukula, A.; Echenard, B.; Hitlin, D.G.; Porter, F.; Rakitin, A.; /Caltech; Heinemeyer, S.; /Cantabria Inst. of Phys.; McElrath, B.; /CERN; Andreassen, R.; Meadows, B.; Sokoloff, M.; /Cincinnati U.; Blanke, M.; /Cornell U., Phys. Dept.; Lesiak, T.; /Cracow, INP /DESY /Zurich, ETH /INFN, Ferrara /Frascati /INFN, Genoa /Glasgow U. /Indiana U. /Mainz U., Inst. Phys. /Karlsruhe, Inst. Technol. /KEK, Tsukuba /LBL, Berkeley /UC, Berkeley /Lisbon, IST /Ljubljana U. /Madrid, Autonoma U. /Maryland U. /MIT /INFN, Milan /McGill U. /Munich, Tech. U. /Notre Dame U. /PNL, Richland /INFN, Padua /Paris U., VI-VII /Orsay, LAL /Orsay, LPT /INFN, Pavia /INFN, Perugia /INFN, Pisa /Queen Mary, U. of London /Regensburg U. /Republica U., Montevideo /Frascati /INFN, Rome /INFN, Rome /INFN, Rome /Rutherford /Sassari U. /Siegen U. /SLAC /Southern Methodist U. /Tel Aviv U. /Tohoku U. /INFN, Turin /INFN, Trieste /Uppsala U. /Valencia U., IFIC /Victoria U. /Wayne State U. /Wisconsin U., Madison

2012-02-14T23:59:59.000Z

37

Super Energy Saver Heat Pump with Dynamic Hybrid Phase Change ...  

Super Energy Saver Heat Pump with Dynamic Hybrid Phase Change Material United States Patent Application

38

Columbia Water & Light- Commercial Super Saver Loans  

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

Columbia Water & Light (CWL) provides Commercial Super Saver Loans, which allow C&I rate customers to replace a furnace along with a new central air conditioner or heat pump with an...

39

Columbia Water & Light- Residential Super Saver Loans  

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

The Columbia Water & Light (CWL) Home Performance Super Saver Loan allows Columbia residents to finance energy improvements to homes with affordable, low interest loans with five to ten year...

40

WEB PUBLISHING APPLICATION FORM: REGISTRATION AS OPENTEXT CMS CONTRIBUTOR This form should be printed and completed by members of staff of the University who wish to  

E-Print Network (OSTI)

WEB PUBLISHING APPLICATION FORM: REGISTRATION AS OPENTEXT CMS CONTRIBUTOR This form should of entering and updating web information using OpenText CMS [Content Management System]. A contributor may only edit an existing web site and create or edit content ready for approval. If you require to approve

Howie, Jim

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Argonne OutLoud: Rise of the Super Smart Supercomputer | Argonne National  

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

Rise of the Super Smart Supercomputer Rise of the Super Smart Supercomputer Rise of the Super Smart Supercomputer lecture 1 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 1 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 2 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 3 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 4 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 5 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture 6 of 13 Rise of the Super Smart Supercomputer lecture Rise of the Super Smart Supercomputer lecture

42

JGI - Prokaryotic Super Program Advisory Committee Meeting  

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

Prokaryotic Super Program Advisory Committee Meeting Prokaryotic Super Program Advisory Committee Meeting Members Cameron Currie, University of Wisconsin Ed DeLong, MIT Jed Fuhrman, University of Southern California George Garrity, MSU Steve Hallam, University of British Columbia Bob Landick, Great Lakes Bioenergy Research Center Folker Meyer, Argonne National Laboratory Nancy Moran, Yale University Mary Ann Moran, University of Georgia Karen Nelson, JCVI Rich Roberts, NEB Doug Rusch, J. Craig Venter Institute Ramunas Stepanauskas, Bigelow Laboratory for Ocean Sciences Niels van der Lelie, RTI Phil Hugenholtz, University of Queensland Home > About Us > JGI Management > Prokaryotic Super Program Advisory Committee Meeting UC logo DOE logo Contact Us Credits Disclaimer Access KeysAccessibility/Section 508 ©1997-2013 The Regents of the University of California Page Last Updated

43

Super-tasks, accelerating Turing machines and uncomputability  

Science Conference Proceedings (OSTI)

Accelerating Turing machines are devices with the same computational structure as Turing machines (TM), but able to perform super-tasks. We ask whether performing super-tasks alone produces more computational power; for example, whether accelerating ... Keywords: Thomson's paradox, accelerating Turing machines, halting problem, super-task

Oron Shagrir

2004-06-01T23:59:59.000Z

44

Federal Energy Management Program: Regional Super ESPC Saves Energy and  

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

Regional Super Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center to someone by E-mail Share Federal Energy Management Program: Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center on Facebook Tweet about Federal Energy Management Program: Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center on Twitter Bookmark Federal Energy Management Program: Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center on Google Bookmark Federal Energy Management Program: Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center on Delicious Rank Federal Energy Management Program: Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center on Digg Find More places to share Federal Energy Management Program:

45

DOE Webcast: GTI Super Boiler Technology  

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

Webcast Webcast GTI Super Boiler Technology by Dennis Chojnacki, Senior Engineer by Curt Bermel, Business Development Mgr. R&D > November 20, 2008 November 20, 2008 2 November 20, 2008 2 WHO WE ARE Gas Technology Institute >Leading U.S. research, development, and training organization serving the natural gas industry and energy markets ─ An independent, 501c (3) not-for-profit Serving the Energy Industry Since 1941 > Over 1,000 patents > Nearly 500 products commercialized November 20, 2008 3 November 20, 2008 3 Super Boiler Background > U.S. industrial and commercial steam boilers ─ Consume over 6 quads of natural gas per year ─ Wide range of steam uses from process steam to space heating > Installed base of steam boilers ─ Largely over 30 years old

46

Solar Neutrinos with Super-Kamiokande  

E-Print Network (OSTI)

The discrepancy of the measured solar neutrino flux compared to the predictions of the standard solar model may be explained by the neutrino flavor oscillation hypothesis. A more direct and less model-dependent test of this hypothesis is a measurement of the distortion of the shape of the solar neutrino energy spectrum. Super-Kamiokande studies the energy spectrum of recoil electrons from solar neutrino scattering in water above 5.5 MeV.

Smy, M B

1999-01-01T23:59:59.000Z

47

Vibration Budget for SuperB  

Science Conference Proceedings (OSTI)

We present a vibration budget for the SuperB accelerator. We include ground motion data, motion sensitivity of machine components, and beam feedback system requirements. The SuperB accelerator design attains at least 50 times higher than current B-factories due to smaller beam sizes and a crabbed waist crossing angle scheme at the IP (interaction point). The beam size (1{sigma}) at the IP will be about 10 {micro}m (horizontal) by 40 nm (vertical). These small beam sizes will make the luminosity very sensitive to mechanical vibration and electrical noise. Relative vertical misalignment of the two beams at the IP by only 8 nm will result in a 1% reduction in luminosity. The corresponding horizontal alignment tolerance of is 250x looser (2 {micro}m). The vertical beam angle at the IP for a 1% luminosity loss is fairly loose at 200 {micro}rad, and the horizontal beam angle tolerance is looser still. We will focus on vertical beam position at the IP, since this presents the greatest alignment challenge. The values presented here are for a closed orbit with tunes near a half-integer in the SuperB v.12 lattice.

Bertsche, K; Wittmer, W.; /SLAC; Bolzon, B.; Brunetti, L.; Jeremie, A.; /Annecy, LAPP; Esposito, M.; Tomassini, S.; /Frascati

2011-04-05T23:59:59.000Z

48

SuperB Technical Design Report  

E-Print Network (OSTI)

In this Technical Design Report (TDR) we describe the SuperB detector that was to be installed on the SuperB e+e- high luminosity collider. The SuperB asymmetric collider, which was to be constructed on the Tor Vergata campus near the INFN Frascati National Laboratory, was designed to operate both at the Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1} and at the tau/charm production threshold with a luminosity of 10^{35} cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100 larger than present B Factories, would allow investigation of new physics effects in rare decays, CP Violation and Lepton Flavour Violation. This document details the detector design presented in the Conceptual Design Report (CDR) in 2007. The R&D and engineering studies performed to arrive at the full detector design are described, and an updated cost estimate is presented. A combination of a more realistic cost estimates and the unavailability of funds due of the global economic climate led to a formal cancelation of the project on Nov 27, 2012.

SuperB Collaboration; M. Baszczyk; P. Dorosz; J. Kolodziej; W. Kucewicz; M. Sapor; A. Jeremie; E. Grauges Pous; G. E. Bruno; G. De Robertis; D. Diacono; G. Donvito; P. Fusco; F. Gargano; F. Giordano; F. Loddo; F. Loparco; G. P. Maggi; V. Manzari; M. N. Mazziotta; E. Nappi; A. Palano; B. Santeramo; I. Sgura; L. Silvestris; V. Spinoso; G. Eigen; J. Zalieckas; Z. Zhuo; L. Jenkovszky; G. Balbi; M. Boldini; D. Bonacorsi; V. Cafaro; I. D'Antone; G. M. Dallavalle; R. Di Sipio; F. Fabbri; L. Fabbri; A. Gabrielli; D. Galli; P. Giacomelli; V. Giordano; F. M. Giorgi; C. Grandi; I. Lax; S. Lo Meo; U. Marconi; A. Montanari; G. Pellegrini; M. Piccinini; T. Rovelli; N. Semprini Cesari; G. Torromeo; N. Tosi; R. Travaglini; V. M. Vagnoni; S. Valentinetti; M. Villa; A. Zoccoli; J. -F. Caron; C. Hearty; P. F. -T. Lu; T. S. Mattison; J. A. McKenna; R. Y. -C. So; M. Yu. Barnyakov; V. E. Blinov; A. A. Botov; V. P. Druzhinin; V. B. Golubev; S. A. Kononov; E. A. Kravchenko; E. B. Levichev; A. P. Onuchin; S. I. Serednyakov; D. A. Shtol; Y. I. Skovpen; E. P. Solodov; A. Cardini; M. Carpinelli; D. S. -T. Chao; C. H. Cheng; D. A. Doll; B. Echenard; K. Flood; J. Hanson; D. G. Hitlin; P. Ongmongkolkul; F. C. Porter; R. Y. Zhu; N. Randazzo; E. De La Cruz Burelo; Y. Zheng; P. Campos; M. De Silva; A. Kathirgamaraju; B. Meadows; B. Pushpawela; Y. Shi; M. Sokoloff; G. Lopez Castro; V. Ciaschini; P. Franchini; F. Giacomini; A. Paolini; G. A. Calderon Polania; S. Laczek; P. Romanowicz; B. Szybinski; M. Czuchry; L. Flis; D. Harezlak; J. Kocot; M. Radecki; M. Sterzel; T. Szepieniec; T. Szymocha; P. Wjcik; M. Andreotti; W. Baldini; R. Calabrese; V. Carassiti; G. Cibinetto; A. Cotta Ramusino; F. Evangelisti; A. Gianoli; E. Luppi; R. Malaguti; M. Manzali; M. Melchiorri; M. Munerato; C. Padoan; V. Santoro; L. Tomassetti; M. M. Beretta; M. Biagini; M. Boscolo; E. Capitolo; R. de Sangro; M. Esposito; G. Felici; G. Finocchiaro; M. Gatta; C. Gatti; S. Guiducci; S. Lauciani; P. Patteri; I. Peruzzi; M. Piccolo; P. Raimondi; M. Rama; C. Sanelli; S. Tomassini; P. Fabbricatore; D. Delepine; M. A. Reyes Santos; M. Chrzaszcz; R. Grzymkowski; P. Knap; J. Kotula; T. Lesiak; J. Ludwin; J. Michalowski; B. Pawlik; B. Rachwal; M. Stodulski; J. Wiechczynski; M. Witek; L. Zawiejski; M. Zdybal; V. Y. Aushev; A. Ustynov; N. Arnaud; P. Bambade; C. Beigbeder; F. Bogard; M. Borsato; D. Breton; J. Brossard; L. Burmistrov; D. Charlet; V. Chaumat; O. Dadoun; M. El Berni; J. Maalmi; V. Puill; C. Rimbault; A. Stocchi; V. Tocut; A. Variola; S. Wallon; G. Wormser; F. Grancagnolo; E. Ben-Haim; S. Sitt; M. Baylac; O. Bourrion; J. -M. Deconto; Y. Gomez Martinez; N. Monseu; J. -F. Muraz; J. -S. Real; C. Vescovi; R. Cenci; A. Jawahery; D. Roberts; E. W. Twedt; R. Cheaib; D. Lindemann; S. Nderitu; P. Patel; S. H. Robertson; D. Swersky; A. Warburton; E. Cuautle Flores; G. Toledo Sanchez; P. Biassoni; L. Bombelli; M. Citterio; S. Coelli; C. Fiorini; V. Liberali; M. Monti; B. Nasri; N. Neri; F. Palombo; F. Sabatini; A. Stabile; A. Berra; A. Giachero; C. Gotti; D. Lietti; M. Maino; G. Pessina; M. Prest; J. -P. Martin; M. Simard; N. Starinski; P. Taras; A. Drutskoy; S. Makarychev; A. V. Nefediev; A. Aloisio; S. Cavaliere; G. De Nardo; M. Della Pietra; A. Doria; R. Giordano; A. Ordine; S. Pardi; G. Russo; C. Sciacca; I. I. Bigi; C. P. Jessop; W. Wang; M. Bellato; M. Benettoni; M. Corvo; A. Crescente; F. Dal Corso; U. Dosselli; C. Fanin; A. Gianelle; S. Longo; M. Michelotto; F. Montecassiano; M. Morandin; R. Pengo; M. Posocco; M. Rotondo; G. Simi; R. Stroili; L. Gaioni; A. Manazza; M. Manghisoni; L. Ratti; V. Re; G. Traversi; S. Zucca; S. Bizzaglia; M. Bizzarri; C. Cecchi; S. Germani; M. Lebeau; P. Lubrano; E. Manoni; A. Papi; A. Rossi; G. Scolieri; G. Batignani; S. Bettarini; G. Casarosa; A. Cervelli; A. Fella; F. Forti; M. Giorgi; L. Lilli; A. Lusiani; B. Oberhof; A. Paladino; F. Pantaleo; E. Paoloni; A. L. Perez Perez; G. Rizzo; J. Walsh; A. Fernndez Tllez; G. Beck; M. Berman; A. Bevan; F. Gannaway; G. Inguglia; A. J. Martin; J. Morris; V. Bocci; M. Capodiferro; G. Chiodi; I. Dafinei; N. V. Drenska; R. Faccini; F. Ferroni; C. Gargiulo; P. Gauzzi; C. Luci; R. Lunadei; G. Martellotti; F. Pellegrino; V. Pettinacci; D. Pinci; L. Recchia; D. Ruggeri; A. Zullo; P. Camarri; R. Cardarelli; C. De Santis; A. Di Ciaccio; V. Di Felice; F. Di Palma; A. Di Simone; L. Marcelli; R. Messi; D. Moricciani; R. Sparvoli; S. Tammaro; P. Branchini; A. Budano; S. Bussino; M. Ciuchini; F. Nguyen; A. Passeri; F. Ruggieri; E. Spiriti; F. Wilson; I. Leon Monzon; J. R. Millan-Almaraz; P. L. M. Podesta-Lerma; D. Aston; B. Dey; A. Fisher; P. D. Jackson; D. W. G. S. Leith; S. Luitz; D. MacFarlane; M. McCulloch; S. Metcalfe; A. Novokhatski; S. Osier; R. Prepost; B. Ratcliff; J. Seeman; M. Sullivan; J. Va'vra; U. Wienands; W. Wisniewski; B. D. Altschul

2013-06-24T23:59:59.000Z

49

SuperB Technical Design Report  

E-Print Network (OSTI)

In this Technical Design Report (TDR) we describe the SuperB detector that was to be installed on the SuperB e+e- high luminosity collider. The SuperB asymmetric collider, which was to be constructed on the Tor Vergata campus near the INFN Frascati National Laboratory, was designed to operate both at the Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1} and at the tau/charm production threshold with a luminosity of 10^{35} cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100 larger than present B Factories, would allow investigation of new physics effects in rare decays, CP Violation and Lepton Flavour Violation. This document details the detector design presented in the Conceptual Design Report (CDR) in 2007. The R&D and engineering studies performed to arrive at the full detector design are described, and an updated cost estimate is presented. A combination of a more realistic cost estimates and the unavailability of funds due of the global economic ...

Baszczyk, M; Kolodziej, J; Kucewicz, W; Sapor, M; Jeremie, A; Pous, E Grauges; Bruno, G E; De Robertis, G; Diacono, D; Donvito, G; Fusco, P; Gargano, F; Giordano, F; Loddo, F; Loparco, F; Maggi, G P; Manzari, V; Mazziotta, M N; Nappi, E; Palano, A; Santeramo, B; Sgura, I; Silvestris, L; Spinoso, V; Eigen, G; Zalieckas, J; Zhuo, Z; Jenkovszky, L; Balbi, G; Boldini, M; Bonacorsi, D; Cafaro, V; D'Antone, I; Dallavalle, G M; Di Sipio, R; Fabbri, F; Fabbri, L; Gabrielli, A; Galli, D; Giacomelli, P; Giordano, V; Giorgi, F M; Grandi, C; Lax, I; Meo, S Lo; Marconi, U; Montanari, A; Pellegrini, G; Piccinini, M; Rovelli, T; Cesari, N Semprini; Torromeo, G; Tosi, N; Travaglini, R; Vagnoni, V M; Valentinetti, S; Villa, M; Zoccoli, A; Caron, J -F; Hearty, C; Lu, P F -T; Mattison, T S; McKenna, J A; So, R Y -C; Barnyakov, M Yu; Blinov, V E; Botov, A A; Druzhinin, V P; Golubev, V B; Kononov, S A; Kravchenko, E A; Levichev, E B; Onuchin, A P; Serednyakov, S I; Shtol, D A; Skovpen, Y I; Solodov, E P; Cardini, A; Carpinelli, M; Chao, D S -T; Cheng, C H; Doll, D A; Echenard, B; Flood, K; Hanson, J; Hitlin, D G; Ongmongkolkul, P; Porter, F C; Zhu, R Y; Randazzo, N; Burelo, E De La Cruz; Zheng, Y; Campos, P; De Silva, M; Kathirgamaraju, A; Meadows, B; Pushpawela, B; Shi, Y; Sokoloff, M; Castro, G Lopez; Ciaschini, V; Franchini, P; Giacomini, F; Paolini, A; Polania, G A Calderon; Laczek, S; Romanowicz, P; Szybinski, B; Czuchry, M; Flis, L; Harezlak, D; Kocot, J; Radecki, M; Sterzel, M; Szepieniec, T; Szymocha, T; Wjcik, P; Andreotti, M; Baldini, W; Calabrese, R; Carassiti, V; Cibinetto, G; Ramusino, A Cotta; Evangelisti, F; Gianoli, A; Luppi, E; Malaguti, R; Manzali, M; Melchiorri, M; Munerato, M; Padoan, C; Santoro, V; Tomassetti, L; Beretta, M M; Biagini, M; Boscolo, M; Capitolo, E; de Sangro, R; Esposito, M; Felici, G; Finocchiaro, G; Gatta, M; Gatti, C; Guiducci, S; Lauciani, S; Patteri, P; Peruzzi, I; Piccolo, M; Raimondi, P; Rama, M; Sanelli, C; Tomassini, S; Fabbricatore, P; Delepine, D; Santos, M A Reyes; Chrzaszcz, M; Grzymkowski, R; Knap, P; Kotula, J; Lesiak, T; Ludwin, J; Michalowski, J; Pawlik, B; Rachwal, B; Stodulski, M; Wiechczynski, J; Witek, M; Zawiejski, L; Zdybal, M; Aushev, V Y; Ustynov, A; Arnaud, N; Bambade, P; Beigbeder, C; Bogard, F; Borsato, M; Breton, D; Brossard, J; Burmistrov, L; Charlet, D; Chaumat, V; Dadoun, O; Berni, M El; Maalmi, J; Puill, V; Rimbault, C; Stocchi, A; Tocut, V; Variola, A; Wallon, S; Wormser, G; Grancagnolo, F; Ben-Haim, E; Sitt, S; Baylac, M; Bourrion, O; Deconto, J -M; Martinez, Y Gomez; Monseu, N; Muraz, J -F; Real, J -S; Vescovi, C; Cenci, R; Jawahery, A; Roberts, D; Twedt, E W; Cheaib, R; Lindemann, D; Nderitu, S; Patel, P; Robertson, S H; Swersky, D; Warburton, A; Flores, E Cuautle; Sanchez, G Toledo; Biassoni, P; Bombelli, L; Citterio, M; Coelli, S; Fiorini, C; Liberali, V; Monti, M; Nasri, B; Neri, N; Palombo, F; Sabatini, F; Stabile, A; Berra, A; Giachero, A; Gotti, C; Lietti, D; Maino, M; Pessina, G; Prest, M; Martin, J -P; Simard, M; Starinski, N; Taras, P; Drutskoy, A; Makarychev, S; Nefediev, A V; Aloisio, A; Cavaliere, S; De Nardo, G; Della Pietra, M; Doria, A; Giordano, R; Ordine, A; Pardi, S; Russo, G; Sciacca, C; Bigi, I I; Jessop, C P; Wang, W; Bellato, M; Benettoni, M; Corvo, M; Crescente, A; Corso, F Dal; Dosselli, U; Fanin, C; Gianelle, A; Longo, S; Michelotto, M; Montecassiano, F; Morandin, M; Pengo, R; Posocco, M; Rotondo, M; Simi, G; Stroili, R; Gaioni, L; Manazza, A; Manghisoni, M; Ratti, L; Re, V; Traversi, G; Zucca, S; Bizzaglia, S; Bizzarri, M; Cecchi, C; Germani, S; Lebeau, M; Lubrano, P; Manoni, E; Papi, A; Rossi, A; Scolieri, G; Batignani, G; Bettarini, S; Casarosa, G; Cervelli, A; Fella, A; Forti, F; Giorgi, M; Lilli, L; Lusiani, A; Oberhof, B; Paladino, A; Pantaleo, F; Paoloni, E; Perez, A L Perez; Rizzo, G; Walsh, J; Tllez, A Fernndez; Beck, G; Berman, M; Bevan, A; Gannaway, F; Inguglia, G; Martin, A J; Morris, J; Bocci, V; Capodiferro, M; Chiodi, G; Dafinei, I; Drenska, N V; Faccini, R; Ferroni, F; Gargiulo, C; Gauzzi, P; Luci, C; Lunadei, R; Martellotti, G; Pellegrino, F; Pettinacci, V; Pinci, D; Recchia, L; Ruggeri, D; Zullo, A; Camarri, P; Cardarelli, R; De Santis, C; Di Ciaccio, A; Di Felice, V; Di Palma, F; Di Simone, A; Marcelli, L; Messi, R; Moricciani, D; Sparvoli, R; Tammaro, S; Branchini, P; Budano, A; Bussino, S; Ciuchini, M; Nguyen, F; Passeri, A; Ruggieri, F; Spiriti, E; Wilson, F; Monzon, I Leon; Millan-Almaraz, J R; Podesta-Lerma, P L M; Aston, D; Dey, B; Fisher, A; Jackson, P D; Leith, D W G S; Luitz, S; MacFarlane, D; McCulloch, M; Metcalfe, S; Novokhatski, A; Osier, S; Prepost, R; Ratcliff, B; Seeman, J; Sullivan, M; Va'vra, J; Wienands, U; Wisniewski, W; Altschul, B D; Purohit, M V; Baudot, J; Ripp-Baudot, I; Cirrone, G A P; Cuttone, G; Bezshyyko, O; Dolinska, G; Soffer, A

2013-01-01T23:59:59.000Z

50

Green Supers Graduate Prepared to Make NYC More Energy Efficient |  

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

Green Supers Graduate Prepared to Make NYC More Energy Efficient Green Supers Graduate Prepared to Make NYC More Energy Efficient Green Supers Graduate Prepared to Make NYC More Energy Efficient May 26, 2011 - 5:15pm Addthis Victor Nazario speaks at the 1,000 Green Supers graduation ceremony in New York City. | Courtesy of SEIU32BJ Victor Nazario speaks at the 1,000 Green Supers graduation ceremony in New York City. | Courtesy of SEIU32BJ Lindsey Geisler Lindsey Geisler Public Affairs Specialist, Office of Public Affairs Earlier this week, Secretary Chu delivered the graduation address for the Green Supers program in New York City. The 40-hour program teaches building superintendents everything they need to know about green building operations and maintenance. Victor Nazario, part of this first class of graduates who also spoke at the

51

The Mechanism Interpretation by Energetic Band Diagram of Super ...  

Science Conference Proceedings (OSTI)

Composite Silicon Carbon Nano-fiber Anode for High Energy Advance Lithium .... of Super P Carbon Black and Silicon Carbide in Si-based Lithium Ion Batteries.

52

Example Measurement & Verification Plan for a Super ESPC Project  

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

Report features a comprehensive measurement and verification (M&V) plan for a fictitious super energy savings performance contract (ESPC) project.

53

Tungsten-Rhenium Super Alloy Development for Ultra High ...  

Science Conference Proceedings (OSTI)

Presentation Title, Tungsten-Rhenium Super Alloy Development for Ultra High Temperature Space Fission and Fusion Reactors. Author(s), Jonathan Webb,...

54

Super-Nanotubes: 'Remarkable' Spray-on Coating Combines ...  

Science Conference Proceedings (OSTI)

... have demonstrated a spray-on mixture of carbon nanotubes and ceramic ... of one strand of a new spray-on super-nanotube composite developed by ...

2013-04-17T23:59:59.000Z

55

Super Energy Saver Heat Pump - Energy Innovation Portal  

ORNL researchers developed a broad class of dynamic hybrid phase change materials and coupled them to residential heat pumps, inventing a super energy saver heat pump.

56

Matrix Market: Contributors  

Science Conference Proceedings (OSTI)

... Industry. Aerospatiale Cannes Boeing Computer Services Exxon General Electric Lockheed National Nuclear Corporation, Ltd. ...

2002-05-10T23:59:59.000Z

57

Microsoft Word - Contributors  

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

Information for beamline technique matrices provided Information for beamline technique matrices provided and/or compiled by: Major Technique Technique Compiled by Spectroscopy 01-01 Infrared Larry Carr, Lisa Miller, Eli Stavitski, Brookhaven National Laboratory 01-02 Photoemission Elio Vescovo, Brookhaven National Laboratory 02-01 Soft X-ray Spectroscopy Joe Dvorak, Brookhaven National Laboratory 02-02 Tender XAS Paul Northrup, Stony Brook University 03-01 EXAFS John Bargar, Stanford Linear Accelerator Center; Steve Heald, Argonne National Laboratory; Tony Lanzirotti, University of Chicago; Matt Newville, Argonne National Laboratory; Bruce Ravel, NIST, Sam Webb, Stanford Synchrotron Radiation Lightsource 04-01 Metrology Jeff Keister, Brookhaven National Laboratory

58

Contributors 9:2  

E-Print Network (OSTI)

City College. is a New York architect whose projects includeShe has worked with Roben A. M . Stern Architects, JohnsonBurgee Architects and Kox & Fowle Architects, and graduated

1994-01-01T23:59:59.000Z

59

Contributors 21:1  

E-Print Network (OSTI)

C. Allen, ASLA, is a landscape architect and a Professor ofArad was working as an architect for the New York Citycompetition, he joined Handel Architects, where he is now a

2009-01-01T23:59:59.000Z

60

Contributors 7:4  

E-Print Network (OSTI)

Robert Campbell is an architect and writer in Boston.plex project for Ratcliff Architects, where she is seniorAssociates Landscape Architects in Berkeley. H e explores

1992-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Contributors 19:2  

E-Print Network (OSTI)

is an urban designer, architect, and Assistant Professor inContributing Editor, is an architect and urban designeran urban designer, architect, and since 2004, a postdoctoral

2007-01-01T23:59:59.000Z

62

Contributors 7:1  

E-Print Network (OSTI)

t e r n is a practicing architect, teacher and writer. He isof Robert A. M . Stern Architects, professor at Columbiaof the American Institute of Architects. is a geographer and

1990-01-01T23:59:59.000Z

63

Student Fun Book Contributors  

E-Print Network (OSTI)

exhibit self-affine mound structures with a scaling exponent of 0.82 0.03 and a mound radius rc, resulting in broader mounds and a smaller root mean square surface roughness . This effect is most where some mounds grow laterally at the expense of their smaller neighbors, which die out. In contrast

Behmer, Spencer T.

64

Publication Information and Contributors  

Science Conference Proceedings (OSTI)

...D.B. Mitton University of North Dakota Bert Moniz DuPont William G. Moore National Electric Coil Max D. Moskal Mechanical and Materials

65

Publication Information and Contributors  

Science Conference Proceedings (OSTI)

...Hill Carpenter Technology Corporation Albert L. Hoffmanner Manufacturing Technologies William F. Hosford University of Michigan L.G. Housefield Pratt & Whitney Dennis Huffman The Timken Company (Retired) Warren H. Hunt, Jr. Aluminum Consultants

66

SUPER HIGH-SPEED MINIATURIZED PERMANENT MAGNET SYNCHRONOUS MOTOR  

E-Print Network (OSTI)

SUPER HIGH-SPEED MINIATURIZED PERMANENT MAGNET SYNCHRONOUS MOTOR by LIPING ZHENG B.S. Shanghai with the design of permanent magnet synchronous motors (PMSM) to operate at super-high speed with high efficiency the motor to have an efficiency reaching above 92%. This achieved efficiency indicated a significant

Wu, Shin-Tson

67

Solar neutrino measurements in Super-Kamiokande-I  

E-Print Network (OSTI)

The details of Super--Kamiokande--I's solar neutrino analysis are given. Solar neutrino measurement in Super--Kamiokande is a high statistics collection of $^8$B solar neutrinos via neutrino-electron scattering. The analysis method and results of the 1496 day data sample are presented. The final oscillation results for the data are also presented.

Super-Kamiokande Collaboration

2005-08-27T23:59:59.000Z

68

Toward a New Phenomenon: Super-Cerenkov Radiation  

E-Print Network (OSTI)

In this letter a new coherent gamma emission mechanism, called Super-Cerenkov radiation, is introduced. The SCR is expected to take place when the charged particle is moving in a medium with a phase velocity satisfying the super-coherent condition. The results on an experimental test of SCR in RICH detector are presented.

D. B. Ion; M. L. Ion

2004-02-26T23:59:59.000Z

69

Columbia Water and Light - Residential Super Saver Loans | Department of  

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

Residential Super Saver Loans Residential Super Saver Loans Columbia Water and Light - Residential Super Saver Loans < Back Eligibility Multi-Family Residential Residential Savings Category Home Weatherization Commercial Weatherization Heating & Cooling Commercial Heating & Cooling Cooling Sealing Your Home Design & Remodeling Windows, Doors, & Skylights Ventilation Heating Heat Pumps Appliances & Electronics Water Heating Solar Maximum Rebate $15,000 Program Info State Missouri Program Type Utility Loan Program Rebate Amount Home Performance Super Saver Loan: up to $15,000 Provider Columbia Water and Light The Columbia Water and Light (CWL) Home Performance Super Saver Loan allows Columbia residents to finance energy improvements to homes with affordable, low interest loans with five to ten year terms. If a Water and Light

70

DOE Subpoenas Maker of Super Power Showerhead | Department of Energy  

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

Subpoenas Maker of Super Power Showerhead Subpoenas Maker of Super Power Showerhead DOE Subpoenas Maker of Super Power Showerhead January 13, 2011 - 5:56pm Addthis Yesterday, the Department of Energy's Office of Enforcement issued a subpoena to Richard Graham of Long Beach, California seeking water efficiency information and sales records for the "Super Power Shower" in response to a complaint that it violates federal water conservation standards. The Super Power Shower is sold by Mr. Graham on www.gambling-systems.com and other websites, which declare that the showerhead uses 10 gallons of water per minute - four times the 2.5 gallon per minute maximum set by Congress in 1992. This action reflects the Department's commitment to enforce DOE's efficiency standards to ensure that all manufacturers play by the same rules and that consumers realize

71

DOE Subpoenas Maker of Super Power Showerhead | Department of Energy  

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

Subpoenas Maker of Super Power Showerhead Subpoenas Maker of Super Power Showerhead DOE Subpoenas Maker of Super Power Showerhead January 13, 2011 - 5:56pm Addthis Yesterday, the Department of Energy's Office of Enforcement issued a subpoena to Richard Graham of Long Beach, California seeking water efficiency information and sales records for the "Super Power Shower" in response to a complaint that it violates federal water conservation standards. The Super Power Shower is sold by Mr. Graham on www.gambling-systems.com and other websites, which declare that the showerhead uses 10 gallons of water per minute - four times the 2.5 gallon per minute maximum set by Congress in 1992. This action reflects the Department's commitment to enforce DOE's efficiency standards to ensure that all manufacturers play by the same rules and that consumers realize

72

Springfield Utility Board - Super Good Cents Manufactured Homes Rebate  

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

Springfield Utility Board - Super Good Cents Manufactured Homes Springfield Utility Board - Super Good Cents Manufactured Homes Rebate Program Springfield Utility Board - Super Good Cents Manufactured Homes Rebate Program < Back Eligibility Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Program Info State Oregon Program Type Utility Rebate Program Rebate Amount $600 Provider Springfield Utility Board The Springfield Utility Board offers a $600 incentive for the purchase of a Super Good Cents Manufactured Home. Super Good Cents Manufactured Homes offer improve comfort and efficiency. The incentive can be sent to the dealer or to the home buyer, depending on what the home buyer indicates on the application form. The [http://www.subutil.com/pdfs/sgcincentiveform.pdf

73

Carbon Film Electrodes For Super Capacitor Applications  

DOE Patents (OSTI)

A method for treating an organic polymer material, preferably a vinylidene chloride/vinyl chloride copolymer (Saran) to produce a flat sheet of carbon film material having a high surface area (.apprxeq.1000 m.sup.2 /g) suitable as an electrode material for super capacitor applications. The method comprises heating a vinylidene chloride/vinyl chloride copolymer film disposed between two spaced apart graphite or ceramic plates to a first temperature of about 160.degree. C. for about 14 hours to form a stabilized vinylidene chloride/vinyl chloride polymer film, thereafter heating the stabilized film to a second temperature of about 750.degree. C. in an inert atmosphere for about one hour to form a carbon film; and finally activating the carbon film to increase the surface area by heating the carbon film in an oxidizing atmosphere to a temperature of at least 750-850.degree. C. for between 1-6 hours.

Tan, Ming X. (Livermore, CA)

1999-07-20T23:59:59.000Z

74

Super Building Insulation by CO2 Foaming Process Research Project |  

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

Emerging Technologies » Super Building Insulation by CO2 Foaming Emerging Technologies » Super Building Insulation by CO2 Foaming Process Research Project Super Building Insulation by CO2 Foaming Process Research Project The Department of Energy is currently researching the development of building superinsulation through a carbon dioxide (CO2) foaming process. Project Description This project seeks to develop building super insulation through a carbon dioxide foaming process that does not use hydrofluorocarbons (HFCs), and which produces insulation with a high R-value. Project Partners Research is being undertaken between the Department of Energy and The Industrial Science & Technology Network. Project Goals The goal of this project is to develop advanced insulation without HFC, and to achieve a competitive processing cost for CO2 foaming technology.

75

Columbia Water and Light - Commercial Super Saver Loans | Department of  

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

Columbia Water and Light - Commercial Super Saver Loans Columbia Water and Light - Commercial Super Saver Loans Columbia Water and Light - Commercial Super Saver Loans < Back Eligibility Commercial Fed. Government Industrial Nonprofit State Government Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Heating Heat Pumps Appliances & Electronics Commercial Lighting Lighting Water Heating Solar Maximum Rebate $30,000 Program Info Start Date 06/01/2010 State Missouri Program Type Utility Loan Program Rebate Amount Up to $30,000 Provider Columbia Water and Light Columbia Water and Light (CWL) provides Commercial Super Saver Loans, which allow C&I rate customers to replace a furnace along with a new central air conditioner or heat pump with an efficiency rating 11 EER or greater for units 6 tons or larger. No prepayment penalties are enforced through the

76

Super-collimation in a rod-based photonic crystal  

E-Print Network (OSTI)

Super-collimation is the propagation of a light beam without spreading that occurs when the light beam is guided by the dispersion properties of a photonic crystal, rather than by defects in the photonic crystal. ...

Shih, Ta-Ming, Ph. D. Massachusetts Institute of Technology

2007-01-01T23:59:59.000Z

77

SuperShuttle Focus Fleet Study Interim Project Report, November...  

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

SuperShuttle's Boulder location. Five of the vans are dedicated compressed natural gas (CNG), five are bi-fuel CNGgasoline, and three are standard gasoline vans that are being...

78

Cause of super-thermal electron heating during magnetotail reconnection  

E-Print Network (OSTI)

[1] We present a candidate mechanism for the energization of super-thermal electrons during magnetic reconnection in the Earth's magnetotail. By analyzing in-situ measurements of electron distribution functions we characterize ...

Egedal-Pedersen, Jan

79

Y-12 and the super enriched Uranium 235?  

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

"super enriched Uranium 235" Ken Bernander called me to say that he had read in the newspaper about the 100 milligrams of uranium oxide that is 99.999% U-235. He was chuckling when...

80

An Indirect Search for WIMPs with Super-Kamiokande  

E-Print Network (OSTI)

A potential source of high energy neutrinos is the annihilation of Weakly Interacting Massive Particles (WIMPs) collecting in gravitational potential wells such as the centers of the Earth, the Sun, or the Galaxy. A search for such a WIMP annihilation signal using the Super-Kamiokande (Super-K) detector is presented. Super-K observes 1.1 upward through-going muons per day. These events are caused by high energy (typical E_nu ~ 100 GeV) nu_mu interactions in the rock under the detector, and are generally consistent with the expected flux from atmospheric neutrinos. No enhancement of the neutrino signal due to WIMP annihilation is seen, so upper limits on the possible flux of WIMPS are set. These limits are compared to those from other such indirect searches, and a model-independent method is used to compare the Super-K results with direct-detection WIMP experiments.

A. Habig; for the Super-Kamiokande Collaboration

2001-06-05T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

FACT SHEET: SUPER-EFFICIENT EQUIPMENT AND APPLICANCE DEPLOYMENT INITIATIVE  

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

FACT SHEET: SUPER-EFFICIENT EQUIPMENT AND APPLICANCE DEPLOYMENT INITIATIVE At the Clean Energy Ministerial in Washington, D.C. on July 19 th and 20 th , ministers pledged joint efforts to dramatically improve the energy efficiency of household appliances and other energy-using equipment - cutting energy waste, creating jobs, reducing pollution, and saving money for consumers around the world. The ministers launched the Super-efficient Equipment and Appliance Deployment (SEAD) Initiative, a

82

Solar neutrino analysis of Super-Kamiokande  

E-Print Network (OSTI)

Super-Kamiokande-IV data taking began in September of 2008, and with upgraded electronics and improvements to water system dynamics, calibration and analysis techniques, a clear solar neutrino signal could be extracted at recoil electron kinetic energies as low as 3.5 MeV. The SK-IV extracted solar neutrino flux between 3.5 and 19.5 MeV is found to be (2.36$\\pm$0.02(stat.)$\\pm$0.04(syst.))$\\times 10^6$ /(cm$^2$sec). The SK combined recoil electron energy spectrum favors distortions predicted by standard neutrino flavour oscillation parameters over a flat suppression at 1$\\sigma$ level. A maximum likelihood fit to the amplitude of the expected solar zenith angle variation of the elastic neutrino-electron scattering rate in SK, results in a day/night asymmetry of $-3.2\\pm1.1$(stat.)$\\pm$0.5(syst.)$%$. The 2.7 $\\sigma$ significance of non-zero asymmetry is the first indication of the regeneration of electron type solar neutrinos as they travel through Earth's matter. A fit to all solar neutrino data and KamLAND yields $\\sin^2 \\theta_{12} = 0.304 \\pm 0.013$, $\\sin^2 \\theta_{13} = 0.031^{+0.017}_{-0.015}$ and $\\Delta m^2_{21} = 7.45^{+0.20}_{-0.19} \\times 10^{-5} {\\rm eV}^2$.

Hiroyuki Sekiya; for the Super-Kamiokande Collaboration

2013-07-14T23:59:59.000Z

83

SuperB Progress Report for Accelerator  

Science Conference Proceedings (OSTI)

This report details the progress made in by the SuperB Project in the area of the Collider since the publication of the SuperB Conceptual Design Report in 2007 and the Proceedings of SuperB Workshop VI in Valencia in 2008. With this document we propose a new electron positron colliding beam accelerator to be built in Italy to study flavor physics in the B-meson system at an energy of 10 GeV in the center-of-mass. This facility is called a high luminosity B-factory with a project name 'SuperB'. This project builds on a long history of successful e+e- colliders built around the world, as illustrated in Figure 1.1. The key advances in the design of this accelerator come from recent successes at the DAFNE collider at INFN in Frascati, Italy, at PEP-II at SLAC in California, USA, and at KEKB at KEK in Tsukuba Japan, and from new concepts in beam manipulation at the interaction region (IP) called 'crab waist'. This new collider comprises of two colliding beam rings, one at 4.2 GeV and one at 6.7 GeV, a common interaction region, a new injection system at full beam energies, and one of the two beams longitudinally polarized at the IP. Most of the new accelerator techniques needed for this collider have been achieved at other recently completed accelerators including the new PETRA-3 light source at DESY in Hamburg (Germany) and the upgraded DAFNE collider at the INFN laboratory at Frascati (Italy), or during design studies of CLIC or the International Linear Collider (ILC). The project is to be designed and constructed by a worldwide collaboration of accelerator and engineering staff along with ties to industry. To save significant construction costs, many components from the PEP-II collider at SLAC will be recycled and used in this new accelerator. The interaction region will be designed in collaboration with the particle physics detector to guarantee successful mutual use. The accelerator collaboration will consist of several groups at present universities and national laboratories. In Italy these may include INFN Frascati and the University of Pisa, in the United States SLAC, LBNL, BNL and several universities, in France IN2P3, LAPP, and Grenoble, in Russia BINP, in Poland Krakow University, and in the UK the Cockcroft Institute. The construction time for this collider is a total of about four years. The new tunnel can be bored in about a year. The new accelerator components can be built and installed in about 4 years. The shipping of components from PEP-II at SLAC to Italy will take about a year. A new linac and damping ring complex for the injector for the rings can be built in about three years. The commissioning of this new accelerator will take about a year including the new electron and positron sources, new linac, new damping ring, new beam transport lines, two new collider rings and the Interaction Region. The new particle physics detector can be commissioned simultaneously with the accelerator. Once beam collisions start for particle physics, the luminosity will increase with time, likely reaching full design specifications after about two to three years of operation. After construction, the operation of the collider will be the responsibility of the Italian INFN governmental agency. The intent is to run this accelerator about ten months each year with about one month for accelerator turn-on and nine months for colliding beams. The collider will need to operate for about 10 years to provide the required 50 ab{sup -1} requested by the detector collaboration. Both beams as anticipated in this collider will have properties that are excellent for use as sources for synchrotron radiation (SR). The expected photon properties are comparable to those of PETRA-3 or NSLS-II. The beam lines and user facilities needed to carry out this SR program are being investigated.

Biagini, M.E.; Boni, R.; Boscolo, M.; Buonomo, B.; Demma, T.; Drago, A.; Esposito, M.; Guiducci, S.; Mazzitelli, G.; Pellegrino, L.; Preger, M.A.; Raimondi, P.; Ricci, R.; Rotundo, U.; Sanelli, C.; Serio, M.; Stella, A.; Tomassini, S.; Zobov, M.; /Frascati; Bertsche, K.; Brachman, A.; /SLAC /Novosibirsk, IYF /INFN, Pisa /Pisa U. /Orsay, LAL /Annecy, LAPP /LPSC, Grenoble /IRFU, SPP, Saclay /DESY /Cockroft Inst. Accel. Sci. Tech. /U. Liverpool /CERN

2012-02-14T23:59:59.000Z

84

Program on Technology Innovation: Functional Requirements of a Hydrogen-Electric SuperGrid: Two Scenarios - SuperSuburb and SuperTie  

Science Conference Proceedings (OSTI)

To effectively supply U.S. energy needs 3040 years in the future, EPRI has proposed a unique visionary concept called the Hydrogen Electric SuperGrid. The core concept of the SuperGrid is a "continental-scale" (for example, coast-to-coast), superconducting hydrogen-electric transmission system. Electricity and hydrogen would be supplied by advanced nuclear reactors, spaced along the transmission line corridor(s). The line would consist of a high-capacity, direct-current (dc), superconducting power transm...

2006-03-31T23:59:59.000Z

85

SuperB: A High-Luminosity Asymmetric e+e- Super Flavor Factory  

SciTech Connect

We discuss herein the exciting physics program that can be accomplished with a very large sample of heavy quark and heavy lepton decays produced in the very clean environment of an e{sup +}e{sup -} collider; a program complementary to that of an experiment such as LHCb at a hadronic machine. It then presents the conceptual design of a new type of e{sup +}e{sup -} collider that produces a nearly two-order-of-magnitude increase in luminosity over the current generation of asymmetric B Factories. The key idea is the use of low emittance beams produced in an accelerator lattice derived from the ILC Damping Ring Design, together with a new collision region, again with roots in the ILC final focus design, but with important new concepts developed in this design effort. Remarkably, SuperB produces this very large improvement in luminosity with circulating currents and wallplug power similar to those of the current B Factories. There is clear synergy with ILC R&D; design efforts have already influenced one another, and many aspects of the ILC Damping Rings and Final Focus would be operationally tested at SuperB. Finally, the design of an appropriate detector, based on an upgrade of BABAR as an example, is discussed in some detail. A preliminary cost estimate is presented, as is an example construction timeline.

Bona, M.; /et al.

2007-05-18T23:59:59.000Z

86

Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs  

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

L Prize(tm): The Race for Super L Prize(tm): The Race for Super Efficient Light Bulbs to someone by E-mail Share Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on Facebook Tweet about Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on Twitter Bookmark Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on Google Bookmark Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on Delicious Rank Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on Digg Find More places to share Solid-State Lighting: L Prize(tm): The Race for Super Efficient Light Bulbs on AddThis.com... Conferences & Meetings Presentations Publications Webcasts Videos Tools L Prize(tm): The Race for Super Efficient Light Bulbs

87

Recycling Energy Yields Super Savings | Department of Energy  

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

Recycling Energy Yields Super Savings Recycling Energy Yields Super Savings Recycling Energy Yields Super Savings April 23, 2010 - 4:34pm Addthis Joshua DeLung Recycling has been part of going green for a long time, but one company is going a step further by actually recycling energy that has already been used to power manufacturing plants. How do they do it? Recycled Energy Development implements proven technologies that help capture wasted heat and increase their energy efficiency. Dick Munson, senior vice president for public affairs at RED, says facilities that undertake such projects are generally able to cut their energy expenses by up to 20 percent. West Virginia Alloys, in Alloy, W.Va., is a silicon manufacturing plant that makes materials that end up in products such as solar cells and computer chips. In 2013, with help from

88

Top-secret super-secure vault declassified  

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

Top-secret super-secure vault declassified Top-secret super-secure vault declassified Top-secret super-secure vault declassified Located in Los Alamos canyon at Technical Area 41, the Tunnel Vault was built between 1948 and 1949. July 23, 2013 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 multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. 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 multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. Contact Kevin Roark Communications Office

89

Generalized Super-Cerenkov Radiations in Nuclear and Hadronic Media  

E-Print Network (OSTI)

Generalized Super-Cerenkov Radiations (SCR), as well as their SCR-signatures are investigated and classified. Two general SCR- coherence conditions are found as two natural extremes of the same spontaneous particles decay in (dielectric, nuclear or hadronic) media The main results on the quantum theory of the SCR-phenomena as well as the results of the first experimental test of the super-coherence conditions, obtained by using the experimental data from BNL are presented. The new concepts such as: SCR-gluons, SCR-W-bosons and SCR-Z-bosons, all three suggested by elementary particle classification, are introduced. The gluonic Super-Cerenkov-like radiation, first introduced here, is schematically described. The interpretation of some recent RHIC results as signature of the SCR-gluons is suggested.

D. B. Ion

2007-10-03T23:59:59.000Z

90

TRANSITION CROSSING FOR THE BNL SUPER NEUTRINO BEAM FACILITY.  

SciTech Connect

The super neutrino beam facility proposed at the Brookhaven National Laboratory requires proton beams to cross the transition energy in the AGS to reach 1 MW beam power at top energy. High intensity beams are accelerated at a fast repetition rate. Upon transition crossing, such high intensity bunches of large momentum spreads suffer from strong nonlinear chromatic effects and self-field effects. Using theoretical and experimental methods, we determine the impact of these effects and the effectiveness of transition-jump compensation schemes, and determine the optimum crossing scenario for the super neutrino beam facility.

WEI,J.TSOUPAS,N.

2004-07-05T23:59:59.000Z

91

SuperShuttle CNG Fleet Start-Up Experience  

DOE Green Energy (OSTI)

The Gas Research Institute (GRI) and the U.S. Department of Energy (DOE), along with several industry partners, are collaborating with SuperShuttle of Denver, Colorado, to evaluate natural gas vans added to the SuperShuttle fleet in 1999. Brand new (1999 model year) dedicated and bi-fuel compressed natural gas (CNG) vans manufactured by Ford Motor Company will be operated side-by-side with several similar gasoline vehicles in normal revenue service. Once the study is complete, DOE's National Renewable Energy Laboratory will analyze and compile the results for release.

Eudy, L.

1999-05-18T23:59:59.000Z

92

U.S. Department of Energy and SuperPower, Inc. Increase Energy...  

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

of Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's Electric Grid U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's...

93

Quantifying the economic and commercial potential of a high strength, low thermal coefficient super-alloy  

E-Print Network (OSTI)

Inspired by the importance of having a favourable sheathing material for superconducting wires, a high-strength, low thermal coefficient (CTE) super-alloy has been developed. Known as Incoloy 908, this super-alloy's material ...

Liew, Heng Lee Henry

2008-01-01T23:59:59.000Z

94

Model and Simulation of a Super-capacitor Braking Energy Recovery System for Urban Railway Vehicles  

Science Conference Proceedings (OSTI)

In this paper, a braking energy recovery system based on super-capacitor was presented. The method use super-capacitor and the conventional braking resistance constitute a new braking unit to realize the regenerative energy recovery, when braking, braking ... Keywords: Urban railway transportation, regeneration braking, super-capacitor, energy recovery, electric traction

Chen Xiao-li; Yang Jian; Fang Yu

2010-08-01T23:59:59.000Z

95

Nitriding of super alloys for enhancing physical properties  

DOE Patents (OSTI)

The invention teaches the improvement of certain super alloys by exposing the alloy to an atmosphere of elemental nitrogen at elevated temperatures in excess of 750/sup 0/C but less than 1150/sup 0/C for an extended duration, viz., by nitriding the surface of the alloy, to establish barrier nitrides of the order of 25 to 100 micrometers thickness. These barrier

Purohit, A.

1984-06-25T23:59:59.000Z

96

Research on a super-small-scale MHD power system  

Science Conference Proceedings (OSTI)

This paper describes a super-small-scale MHD power system, which can generate 4--10W pulse power with a plasma produced by an explosive or combustion as a working substance. Heat shielding material was made and tested, with the result that electrical insulation is desirable. This power generator can be used as an electrical power source of rocket or missile fuses.

He, Z.; Huam, L.Z.; Yao, F.G. (East China Inst. of Tech., Nanjing (China))

1994-03-01T23:59:59.000Z

97

Direct super-resolution and registration using raw CFA images  

Science Conference Proceedings (OSTI)

Super-resolution has been applied mainly to grayscale images, but producing a high-resolution color image using a single CCD sensor has not been investigated in detail until recently. This work aims at producing a high-resolution color image directly ...

Tomomasa Gotoh; Masatoshi Okutomi

2004-06-01T23:59:59.000Z

98

Constraint on super-luminal neutrinos from vacuum Cerenkov processes  

E-Print Network (OSTI)

We examine the Cerenkov-like emission of $e^+ e^-$ from muon super-luminal muon neutrinos assuming a quadratic energy dependence of the neutrino velocity arising from Lorentz violating interactions. We find that with the OPERA result for the neutrino-photon velocity difference, the decay length for the process $\

Subhendra Mohanty; Soumya Rao

2011-11-11T23:59:59.000Z

99

Super-iron Nanoparticles with Facile Cathodic Charge Transfer  

Science Conference Proceedings (OSTI)

Super-irons contain the + 6 valence state of iron. One advantage of this is that it provides a multiple electron opportunity to store additional battery charge. A decrease of particle size from the micrometer to the nanometer domain provides a higher surface area to volume ratio, and opportunity to facilitate charge transfer, and improve the power, voltage and depth of discharge of cathodes made from such salts. However, super-iron salts are fragile, readily reduced to the ferric state, with both heat and contact with water, and little is known of the resultant passivating and non-passivating ferric oxide products. A pathway to decrease the super-iron particle size to the nano-domain is introduced, which overcomes this fragility, and retains the battery capacity advantage of their Fe(VI) valence state. Time and power controlled mechanosynthesis, through less aggressive, dry ball milling, leads to facile charge transfer of super-iron nanoparticles. Ex-situ X-ray Absorption Spectroscopy is used to explore the oxidation state and structure of these iron oxides during discharge and shows the significant change in stability of the ferrate structure to lower oxidation state when the particle size is in the nano-domain.

M Farmand; D Jiang; B Wang; S Ghosh; D Ramaker; S Licht

2011-12-31T23:59:59.000Z

100

The Impact of SuperB on Flavor Physics  

SciTech Connect

This report provides a succinct summary of the physics programme of SuperB, and describes that potential in the context of experiments making measurements in flavour physics over the next 10 to 20 years. Detailed comparisons are made with Belle II and LHCb, the other B physics experiments that will run in this decade. SuperB will play a crucial role in defining the landscape of flavour physics over the next 20 years. SuperB is an approved high luminosity e{sup +}e{sup -} collider intended to search for indirect and some direct signs of new physics (NP) at low energy, while at the same time, enabling precision tests of the Standard Model (SM). This experiment will be built at a new laboratory on the Tor Vergata campus near Rome, Italy named after Nicola Cabibbo. The project has been described in a Conceptual Design Report, and more recently by a set of three white papers on the accelerator, detector, and physics programme. The main focus of the physics programme rests in the study of so-called Golden Modes, these are decay channels that provide access to measurements of theoretically clean observables that can provide both stringent constraints on models of NP, and precision tests of the SM. A number of ancillary measurements that remain important include those with observables that may not be theoretically clean, and those that can be used to provide stringent constraints on the SM but are not sensitive to NP. The remainder of this section introduces SuperB before discussing the golden modes for SuperB, precision CKM measurement modes, and an outline of the rest of this report.

Meadows, B.; Blanke, M.; Stocchi, A.; Drutskoy, A.; Cervelli, A.; Giorgi, M.; Lusiani, A.; Perez, A.; Walsh, J.; Hurth, T.; Bevan, A.; Silvestrini, L.; Ciuchini, M.; Tarantino, C.

2012-02-16T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

Photo of the Week: Inside the Super HILAC | Department of Energy  

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

Inside the Super HILAC Inside the Super HILAC Photo of the Week: Inside the Super HILAC August 29, 2013 - 2:55pm Addthis Super HILAC (Super Heavy Ion Linear Accelerator) was one of the first particle accelerators that could accelerate heavier elements to “atom-smashing” speeds. The device was built in 1972 and played a significant role in four decades of scientific research at Lawrence Berkeley National Laboratory. In addition to being the launchpad for a variety of major experiments, the Super HILAC was crucial in the discovery of five superheavy elements. In this photo, Lawrence Berkeley National Laboratory’s Bob Stevenson and Frank Grobelch are sitting inside the Super HILAC’s poststripper. The maze of piping behind them is meant to circulate cooling water through the accelerator. | Photo courtesy of Lawrence Berkeley National Laboratory.

102

Federal Energy Management Program: First Regional Super ESPC a Success on  

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

First Regional First Regional Super ESPC a Success on Kodiak Island, Alaska to someone by E-mail Share Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on Facebook Tweet about Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on Twitter Bookmark Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on Google Bookmark Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on Delicious Rank Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on Digg Find More places to share Federal Energy Management Program: First Regional Super ESPC a Success on Kodiak Island, Alaska on AddThis.com...

103

Power System Generation and Inter-Connection Planning Model (SUPER) | Open  

Open Energy Info (EERE)

Power System Generation and Inter-Connection Planning Model (SUPER) Power System Generation and Inter-Connection Planning Model (SUPER) Jump to: navigation, search Tool Summary Name: Power System Generation and Inter-Connection Planning Model (SUPER) Agency/Company /Organization: Latin American Energy Organization Sector: Energy Focus Area: Renewable Energy, Hydro Topics: Resource assessment Resource Type: Software/modeling tools Website: www.olade.org/superEn.html References: SUPER website [1] "This model is useful for multi-year electricity system planning studies, making it possible to analyze, optimize, simulate and develop hydrothermal power system expansion plans." References ↑ "SUPER website" Retrieved from "http://en.openei.org/w/index.php?title=Power_System_Generation_and_Inter-Connection_Planning_Model_(SUPER)&oldid=329

104

Job Tax Credit and Super Credit (Tennessee) | Department of Energy  

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

You are here You are here Home » Job Tax Credit and Super Credit (Tennessee) Job Tax Credit and Super Credit (Tennessee) < Back Eligibility Agricultural Commercial Construction Developer Fuel Distributor General Public/Consumer Industrial Investor-Owned Utility Municipal/Public Utility Rural Electric Cooperative Systems Integrator Utility Savings Category Alternative Fuel Vehicles Hydrogen & Fuel Cells Buying & Making Electricity Water Home Weatherization Solar Wind Program Info Funding Source Tennessee Department of Revenue State Tennessee Program Type Corporate Tax Incentive Personal Tax Incentives Provider Tennessee Department of Economic and Community Development The Job Tax Credit Program is a tax credit program for companies investing at least $500,000 and creating 25 new jobs in a 12-month period. The

105

CHEMISTRY OF SILICATE ATMOSPHERES OF EVAPORATING SUPER-EARTHS  

SciTech Connect

We model the formation of silicate atmospheres on hot volatile-free super-Earths. Our calculations assume that all volatile elements such as H, C, N, S, and Cl have been lost from the planet. We find that the atmospheres are composed primarily of Na, O{sub 2}, O, and SiO gas, in order of decreasing abundance. The atmospheric composition may be altered by fractional vaporization, cloud condensation, photoionization, and reaction with any residual volatile elements remaining in the atmosphere. Cloud condensation reduces the abundance of all elements in the atmosphere except Na and K. We speculate that large Na and K clouds such as those observed around Mercury and Io may surround hot super-Earths. These clouds would occult much larger fractions of the parent star than a closely bound atmosphere, and may be observable through currently available methods.

Schaefer, Laura; Fegley, Bruce, E-mail: laura_s@levee.wustl.ed, E-mail: bfegley@levee.wustl.ed [Planetary Chemistry Laboratory, McDonnell Center for the Space Sciences, Department of Earth and Planetary Sciences, Washington University in St. Louis, Saint Louis, MO 63130-4899 (United States)

2009-10-01T23:59:59.000Z

106

Hoisting Branch Conditions -- Improving Super-Scalar Processor Performance  

E-Print Network (OSTI)

. The performance and hardware complexity of super-scalar architectures is hindered by conditional branch instructions. When conditional branches are encountered in a program, the instruction fetch unit must rapidly predict the branch predicate and begin speculatively fetching instructions with no loss of instruction throughput. Speculative execution has a high hardware cost, is limited by dynamic branch prediction accuracies, and does not scale well for increasingly super-scalar architectures. The conditional branch bottleneck would be solved if we could somehow move branch condition evaluation far forward in the instruction stream and provide a new branch instruction that encoded both the source and target address of a branch. This paper summarizes the hardware extensions to support just such a Future Branch, then gives a compiler algorithm for hoisting branch evaluation across many blocks. The algorithm is applicable to other optimizations for parallelism, such as prefetching data. ...

Bill Appelbe; Reid Harmon; Scott Wills; Maurizio Vitale

1995-01-01T23:59:59.000Z

107

Wake Fields in the Super B Factory Interaction Region  

SciTech Connect

The geometry of storage ring collider interaction regions present an impedance to beam fields resulting in the generation of additional electromagnetic fields (higher order modes or wake fields) which affect the beam energy and trajectory. These affects are computed for the Super B interaction region by evaluating longitudinal loss factors and averaged transverse kicks for short range wake fields. Results indicate at least a factor of 2 lower wake field power generation in comparison with the interaction region geometry of the PEP-II B-factory collider. Wake field reduction is a consderation in the Super B design. Transverse kicks are consistent with an attractive potential from the crotch nearest the beam trajectory. The longitudinal loss factor scales as the -2.5 power of the bunch length. A factor of 60 loss factor reduction is possible with crotch geometry based on an intersecting tubes model.

Weathersby, Stephen; /SLAC; Novokhatski, Alexander; /SLAC

2011-06-02T23:59:59.000Z

108

SuperLig Ion Exchange Resin Swelling and Buoyancy Study  

Science Conference Proceedings (OSTI)

The objective of this study was to achieve a fundamental understanding of SuperLig resin swelling and shrinking characteristics, which lead to channeling and early breakthrough during loading cycles. The density of salt solution that causes resin floating was also determined to establish a limit for operation. Specific tests performed include (a) pH dependence, (b) ionic strength dependence and (c) buoyancy effect vs. simulant composition.

Hassan, N.M.

2000-07-27T23:59:59.000Z

109

ON THE STABILITY OF SUPER-EARTH ATMOSPHERES  

SciTech Connect

We investigate the stability of super-Earth atmospheres around M stars using a seven-parameter, analytical framework. We construct stability diagrams in the parameter space of exoplanetary radius versus semimajor axis and elucidate the regions in which the atmospheres are stable against the condensation of their major constituents, out of the gas phase, on their permanent nightside hemispheres. We find that super-Earth atmospheres that are nitrogen-dominated (Earth-like) occupy a smaller region of allowed parameter space, compared to hydrogen-dominated atmospheres, because of the dual effects of diminished advection and enhanced radiative cooling. Furthermore, some super-Earths which reside within the habitable zones of M stars may not possess stable atmospheres, depending on the mean molecular weight and infrared photospheric pressure of their atmospheres. We apply our stability diagrams to GJ 436b and GJ 1214b, and demonstrate that atmospheric compositions with high mean molecular weights are disfavored if these exoplanets possess solid surfaces and shallow atmospheres. Finally, we construct stability diagrams tailored to the Kepler data set, for G and K stars, and predict that about half of the exoplanet candidates are expected to harbor stable atmospheres if Earth-like conditions are assumed. We include 55 Cancri e and CoRoT-7b in our stability diagram for G stars.

Heng, Kevin [ETH Zuerich, Institute for Astronomy, Wolfgang-Pauli-Strasse 27, CH-8093, Zuerich (Switzerland); Kopparla, Pushkar [ETH Zuerich, Institute for Atmospheric and Climate Science, Universitaetstrasse 16, CH-8092, Zuerich (Switzerland)

2012-07-20T23:59:59.000Z

110

Current Status of the SuperWASP Project  

E-Print Network (OSTI)

We present the current status of the SuperWASP project, a Wide Angle Search for Planets. SuperWASP consists of up to 8 individual cameras using ultra-wide field lenses backed by high-quality passively cooled CCDs. Each camera covers 7.8 x 7.8 sq degrees of sky, for nearly 500 sq degrees of sky coverage. SuperWASP I, located in LaPalma, is currently operational with 5 cameras and is conducting a photometric survey of a large numbers of stars in the magnitude range ~7 to 15. The collaboration has developed a custom-built reduction pipeline and aims to achieve better than 1 percent photometric precision. The pipeline will also produce well sampled light curves for all the stars in each field which will be used to detect: planetary transits, optical transients, and track Near-Earth Objects. Status of current observations, and expected rates of extrasolar planetary detections will be presented. The consortium members, institutions, and further details can be found on the web site at: http://www.superwasp.org.

D. J. Christian; D. L. Pollacco; W. I. Clarkson; A. Collier Cameron; N. Evans; A. Fitzsimmons; C. A. Haswell; C. Hellier; S. T. Hodgkin; K. Horne; S. R. Kane; F. P. Keenan; T. A. Lister; A. J. Norton; R. Ryans; I. Skillen; R. A. Street; R. G. West; P. J. Wheatley

2004-10-31T23:59:59.000Z

111

Current Status of the SuperWASP Project  

E-Print Network (OSTI)

We present the current status of the SuperWASP project, a Wide Angle Search for Planets. SuperWASP consists of up to 8 individual cameras using ultra-wide field lenses backed by high-quality passively cooled CCDs. Each camera covers 7.8 x 7.8 sq degrees of sky, for nearly 500 sq degrees of sky coverage. SuperWASP I, located in LaPalma, is currently operational with 5 cameras and is conducting a photometric survey of a large numbers of stars in the magnitude range ~7 to 15. The collaboration has developed a custom-built reduction pipeline and aims to achieve better than 1 percent photometric precision. The pipeline will also produce well sampled light curves for all the stars in each field which will be used to detect: planetary transits, optical transients, and track Near-Earth Objects. Status of current observations, and expected rates of extrasolar planetary detections will be presented. The consortium members, institutions, and further details can be found on the web site at: http://www.superwasp.org.

Christian, D J; Clarkson, W I; Cameron, A C; Evans, N; Fitzsimmons, A; Haswell, C A; Hellier, C; Hodgkin, S T; Horne, K; Kane, S R; Keenan, F P; Lister, T A; Norton, A J; Ryans, R; Skillen, I; Street, R A; West, R G; Wheatley, P J

2004-01-01T23:59:59.000Z

112

Diffuse supernova neutrino background is detectable in Super-Kamiokande  

Science Conference Proceedings (OSTI)

The diffuse supernova neutrino background (DSNB) provides an immediate opportunity to study the emission of MeV thermal neutrinos from core-collapse supernovae. The DSNB is a powerful probe of stellar and neutrino physics, provided that the core-collapse rate is large enough and that its uncertainty is small enough. To assess the important physics enabled by the DSNB, we start with the cosmic star formation history of Hopkins and Beacom (2006) and confirm its normalization and evolution by cross-checks with the supernova rate, extragalactic background light, and stellar mass density. We find a sufficient core-collapse rate with small uncertainties that translate into a variation of {+-}40% in the DSNB event spectrum. Considering thermal neutrino spectra with effective temperatures between 4-6 MeV, the predicted DSNB is within a factor 4-2 below the upper limit obtained by Super-Kamiokande in 2003. Furthermore, detection prospects would be dramatically improved with a gadolinium-enhanced Super-Kamiokande: the backgrounds would be significantly reduced, the fluxes and uncertainties converge at the lower threshold energy, and the predicted event rate is 1.2-5.6 events yr{sup -1} in the energy range 10-26 MeV. These results demonstrate the imminent detection of the DSNB by Super-Kamiokande and its exciting prospects for studying stellar and neutrino physics.

Horiuchi, Shunsaku [Department of Physics, School of Science, University of Tokyo, Tokyo 113-0033 (Japan); Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio 43210 (United States); Department of Physics, Ohio State University, Columbus, Ohio 43210 (United States); Beacom, John F. [Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio 43210 (United States); Department of Physics, Ohio State University, Columbus, Ohio 43210 (United States); Department of Astronomy, Ohio State University, Columbus, Ohio 43210 (United States); Dwek, Eli [Observational Cosmology Lab, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771 (United States)

2009-04-15T23:59:59.000Z

113

Contributors to this issue - Springer  

Science Conference Proceedings (OSTI)

of Pilgrim (N.Y.) State Hospital since 1953. From 1958 to 1964 he was acting director. He received his M.D. from Wayne University Medical. School in 1931, and...

114

List of Authors and Contributors  

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

of Health, Bethesda, MD, USA P. Audebert, Laboratoire pour l'Utilisation des Lasers, Paris, France K. Bane, Stanford Linear Accelerator Center, Stanford, CA, USA I....

115

Contributors: Maria Balota, Crop Physiologist  

E-Print Network (OSTI)

-1200 Texasgulf Gypsum (Phosphogypsum) 50 1500-1800 ISG Resources, Inc. Peanut Maker (semi-granular) 71 1100

Liskiewicz, Maciej

116

Long-Lived Compounds Contributors  

E-Print Network (OSTI)

floating point values. However, to use these system calls you will need to use the mfc1 and mtc1 round down. However, for up to 20% extra credit, you can implement rounding (using the guard, round

Nassar, Ray

117

Stationary Source Division Principal Contributors  

E-Print Network (OSTI)

Publication does not signify that the contents reflect the views and policies of the Air Resources Board, nor does mention of trade names or commercial products constitute endorsement or recommendation for use. This Page Left Intentionally BlankAcknowledgments This report was prepared with the assistance and support from many individuals within the Air Resources Board. In addition, staff would like to acknowledge the assistance and cooperation that we have received from many individuals from other divisions and offices of the Air Resources Board, whose contributions throughout the development process have been invaluable. Finally, staff would like to acknowledge the significant contributions from the numerous State, federal, and internal governmental agencies that have provided assistance throughout the rulemaking process.

Alternative Fuels Branch; Richard Corey Chief; Kamal Ahuja; Ray Asregadoo; Michelle Buffington; Kevin Cleary; Hafizur Chowdhury; Susie Chung; James Duffy; Reza Lorestany; Carolyn Lozo; Ronald Oineza; Jose Saldana; Mike Scheible; Aubrey Sideco; Manisha Singh; Susan Solarz; Jing Yuan

2011-01-01T23:59:59.000Z

118

SuperGrid - The Next Steps: Synthesis Report Based on SuperGrid II Workshop, October 25-27, 2005  

Science Conference Proceedings (OSTI)

The "SuperGrid" represents a vision of an integrated system with the potential to play a major role in the provision of energy to the world in the latter decades of the 21st century. The core concept is a transcontinental energy spine consisting of a superconducting power transmission circuit integrated with a hydrogen pipeline and connected to nuclear power plants and other generating facilities sited in remote locations. The nuclear plants and the electricity/fuel delivery circuit would be constructed ...

2005-03-31T23:59:59.000Z

119

Lithium Super-Ionic Sulfide Carbon (LiSISC) Composite for Li-S ...  

Lithium Super-Ionic Sulfide Carbon (LiSISC) Composite for Li-S Batteries Note: The technology described above is an early stage opportunity. Licensing ...

120

The recent results of solar neutrino measuerments in Super-Kamiokande  

E-Print Network (OSTI)

The results of solar neutrino data from the first phase of Super-Kamiokande are presented. Super-Kamiokande can measure not only the solar neutrino flux but also its energy spectrum and its time variations such as day vs. night and seasonal differences. This information can severely restrict parameters of solar neutrino oscillation. From the combination of several experiments results with those of Super-K, the Large Mixing Angle solution is uniquely allowed at the 98.1 % confidence level; this global solar neutrino oscillation analysis is presented. The current status of the second phase of Super-Kamiokande is presented.

Yusuke Koshio

2003-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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121

Dynamic characteristics and wind-induced responses of a super tall building.  

E-Print Network (OSTI)

??This thesis describes a combined experimental and numerical investigation of wind effects on a super tall building, Di Wang Tower (325m high with 79 floors) (more)

Liu, Pengfei (???)

2007-01-01T23:59:59.000Z

122

LALP-08-045 Licensable Lead-Free Super-Thermite Electric Matches  

Licensable Technologies Lead-Free Super-Thermite Electric Matches An Equal Opportunity Employer / Operated by Los Alamos National Security LLC for DOE/NNSA

123

High-pressure science gets super-sized | Argonne National Laboratory  

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

leap forward with the discovery of a way to generate super high pressures without using shock waves whose accompanying heat turns solids to liquid. This discovery will allow...

124

ICME Modeling of a Super Vacuum Die Cast (SVDC) AZ91 ...  

Science Conference Proceedings (OSTI)

... of a super vacuum die cast (SVDC) AZ91 automotive shock tower component. .... PI-7: A Three-dimensional Lattice Boltzmann Model for Columnar Dendrite...

125

SUPER-M: School and University Partnership for Educational Renewal in Mathematics  

E-Print Network (OSTI)

. Desirable qualifications for this positon include experience in high performance computing, knowledge in the area of high performance computing, please indicate this in your application. Eligibility: · SUPER

Olsen, Stephen L.

126

The Super-Radiant Mechanism, Doorway States, and Nuclear Reactions  

SciTech Connect

In 1954 the possibility of forming a 'super-radiant' (SR) state in a gas of atoms confined to a volume of a size smaller than the wave length of radiation was suggested by Dicke. The atoms, with two levels, are coupled through their common radiation field. This indirect coupling leads to a redistribution of decay widths among unstable intrinsic states. A strongly decaying SR state is created at the expense of the rest of the states of the system. The connection of this mechanism to the notion of doorway states in low-energy nuclear reactions is discussed and applications to well known nuclear physics phenomena are presented.

Auerbach, Naftali [School of Physics and Astronomy, Tel Aviv University, Tel Aviv, 69978 (Israel)

2010-11-24T23:59:59.000Z

127

Super multi-instantons in conformal chiral superspace  

Science Conference Proceedings (OSTI)

We reformulate self-dual supersymmetric theories directly in conformal chiral superspace, where superconformal invariance is manifest. The superspace can be interpreted as the generalization of the usual Atiyah-Drinfel`d-Hitchin-Manin (ADHM) twistors (the quaternionic projective line), the real projective light cone in six dimensions, or harmonic superspace, but can be reduced immediately to four-dimensional chiral superspace. As an exsample, we give the `t Hooft and ADHM multi-instanton constructions for self-dual super Yang-Mills theory. In both cases, all the parameters are represented as a single, irreducible, constant tensor.

Siegel, W. [Institute for Theoretical Physics, State University of New York, Stony Brook, New York 11794-3840 (United States)

1995-07-15T23:59:59.000Z

128

Cerenkov radiation from collisions of straight cosmic (super)strings  

E-Print Network (OSTI)

We consider Cerenkov radiation which must arise when randomly oriented straight cosmic (super)strings move with relativistic velocities without intercommutation. String interactions via dilaton, two-form and gravity (gravity being the dominant force in the ultra-relativistic regime) leads to formation of superluminal sources which generate Cerenkov radiation of dilatons and axions. Though the effect is of the second order in the couplings of strings to these fields, its total efficiency is increased by high dependence of the radiation rate on the Lorentz-factor of the collision.

Elena Melkumova; Dmitri Gal'tsov; Karim Salehi

2006-12-26T23:59:59.000Z

129

Super-light electromagnetic wave with longitudinal and transversal modes  

E-Print Network (OSTI)

The transformation converting equations invariant under Lorentz into the equations invariant under Galileo is obtained. On this basis: (1) the super-light electromagnetic wave with longitudinal and transversal modes is found out; (2) it is shown the wave velocity coincides with that of de Broglie's wave; (3) the connection between Maxwell's electrodynamics and Shredinger's equation is established; (4) structural elements of space are discovered and "a horizon of visibility" is found. It is shown Bell's inequalities and the principle of the light speed constancy are based on the SRT artifact and "Einstein's local realism" is determined by the wave referred above. Objectivity of results for quantum and classical objects is discussed

M. M. Kononenko

2007-08-20T23:59:59.000Z

130

Supernova Relic Neutrino Search at Super-Kamiokande  

E-Print Network (OSTI)

A new Super-Kamiokande (SK) search for Supernova Relic Neutrinos (SRNs) was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 SK result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on SRN flux are between 2.8 and 3.0 nu_e cm^-2 s^-1 > 16 MeV total positron energy (17.3 MeV E_nu).

The Super-Kamiokande Collaboration; :; K. Bays; T. Iida; K. Abe; Y. Hayato; K. Iyogi; J. Kameda; Y. Koshio; L. Marti; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; K. Ueno; K. Ueshima S. Yamada T. Yokozawa H. Kaji T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; L. K. Pik; K. Martens; M. Vagins; L. Labarga; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; W. R. Kropp; S. Mine; C. Regis; A. Renshaw; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; S. Cho; J. S. Jang; J. Y. Kim; I. T. Lim; J. Albert; K. Scholberg; C. W. Walter; R. Wendell; T. Wongjirad; T. Ishizuka; S. Tasaka; J. G. Learned; S. Matsuno; S. Smith; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; M. Ikeda; K. Matsuoka; A. Minamino; A. Murakami; T. Nakaya; Y. Fukuda; Y. Itow; G. Mitsuka; M. Miyake; T. Tanaka; J. Hignight; J. Imber; C. K. Jung; I. Taylor; C. Yanagisawa; A. Kibayashi; H. Ishino; S. Mino; M. Sakuda; T. Mori; H. Toyota; Y. Kuno; S. B. Kim; B. S. Yang; H. Okazawa; Y. Choi; K. Nishijima; M. Koshiba; Y. Totsuka; M. Yokoyama; Y. Heng; S. Chen; H. Zhang; Z. Yang; P. Mijakowski; K. Connolly; M. Dziomba; R. J. Wilkes

2011-11-21T23:59:59.000Z

131

New Low Emittance Lattice for the Super-B Accelerator  

SciTech Connect

New low emittance lattices have been designed for the asymmetric SuperB accelerator, aiming at a luminosity of 10{sup 36} cm{sup -2} s{sup -1}. Main optics features are two alternating arc cells with different horizontal phase advance, decreasing beam emittance and allowing at the same time for easy chromaticity correction in the arcs. Emittance can be further reduced by a factor of two for luminosity upgrade. Spin rotation schemes for the e{sup -} beam have been studied to provide longitudinal polarization at the IP, and implementation into the lattice is in progress.

Biagini, M.E.; Boscolo, M.; Raimondi, P.; Tomassini, S.; Zobov, M.; /Frascati; Seeman, J.; Sullivan, M.; Wienands, U.; Wittmer, W.; /SLAC; Bettoni, S.; /CERN; Paoloni, E.; /Pisa U. /INFN, Pisa; Bogomyagkov, A.; Koop, I.; Levichev, E.; Nikitin, S.; Piminov, P.; Shatilov, D.; /Novosibirsk, IYF

2011-10-21T23:59:59.000Z

132

From Characters to Quantum (Super)Spin Chains via Fusion  

E-Print Network (OSTI)

We give an elementary proof of the Bazhanov-Reshetikhin determinant formula for rational transfer matrices of the twisted quantum super-spin chains associated with the gl(K|M) algebra. This formula describes the most general fusion of transfer matrices in symmetric representations into arbitrary finite dimensional representations of the algebra and is at the heart of analytical Bethe ansatz approach. Our technique represents a systematic generalization of the usual Jacobi-Trudi formula for characters to its quantum analogue using certain group derivatives.

Vladimir Kazakov; Pedro Vieira

2007-11-15T23:59:59.000Z

133

Doorway States and the Super-Radiant Mechanism  

Science Conference Proceedings (OSTI)

A new approach to physics of doorway states in nuclear reactions is developed. It is argued that the coupling of intrinsic states to the continuum through special doorway state(s) may create the situation similar to the optical super-radiance, when the segregation of broad (short-lived) resonances and trapped (long-lived) states occurs. Necessary conditions are discussed, along with applications to isobaric analog states, single-particle resonances, giant resonances, and fission through a double-humped barrier. This pattern can be observed in other mesoscopic systems as well.

Auerbach, N. [School of Physics and Astronomy, Tel Aviv University, Tel Aviv, 69978 (Israel) and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States)

2008-04-04T23:59:59.000Z

134

Introduction to Measurement & Verification for DOE Super ESPC Projects  

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

Introduction to M&V Introduction to M&V Introduction to Measurement & Verification for DOE Super ESPC Projects June 2007 Federal Energy Management Program (FEMP) Office of Energy Efficiency and Renewable Energy U.S. Department of Energy This document was developed for the U.S. Department of Energy's Federal Energy Management Program by Nexant, Inc., and Lawrence Berkeley National Laboratory. This document is posted on FEMP's web site at http://www1.eere.energy.gov/femp/financing/superespcs_mvresources.html. Introduction to M&V Contents WHY MEASURE AND VERIFY? .................................................................................... 1 OVERVIEW OF M&V ...................................................................................................... 1

135

Tracking the Orbital and Super-orbital Periods of SMC X-1  

E-Print Network (OSTI)

The High Mass X-ray Binary (HMXB) SMC X-1 demonstrates an orbital variation of 3.89 days and a super-orbital variation with an average length of 55 days. As we show here, however, the length of the super-orbital cycle varies by almost a factor of two, even across adjacent cycles. To study both the orbital and super-orbital variation we utilize lightcurves from the Rossi X-ray Timing Explorer All Sky Monitor (RXTE-ASM). We employ the orbital ephemeris from Wojdowski et al. (1998) to obtain the average orbital profile, and we show that this profile exhibits complex modulation during non-eclipse phases. Additionally, a very interesting ``bounceback'' in X-ray count rate is seen during mid-orbital eclipse phases, with a softening of the emission during these periods. This bounceback has not been previously identified in pointed observations. We then define a super-orbital ephemeris (the phase of the super-orbital cycle as a function of date) based on the ASM lightcurve and analyze the trend and distribution of super-orbital cycle lengths. SMC X-1 exhibits a bimodal distribution of these lengths, similar to what has been observed in other systems (e.g., Her X-1), but with more dramatic changes in cycle length. There is some hint, but not conclusive evidence, for a dependence of the super-orbital cycle length upon the underlying orbital period, as has been observed previously for Her X-1 and Cyg X-2. Using our super-orbital ephemeris we are also able to create an average super-orbital profile over the 71 observed cycles, for which we witness overall hardening of the spectrum during low count rate times. We combine the orbital and super-orbital ephemerides to study the correlation between the orbital and super-orbital variations in the system.

Sarah Trowbridge; Michael A. Nowak; Joern Wilms

2007-07-31T23:59:59.000Z

136

Denver SuperShuttle CNG Fleet Evaluation; Evaluacion de la flotilla de GNC de la empresa SuperShuttle de Denver  

DOE Green Energy (OSTI)

A description of a joint effort between Denver SuperShuttle, the Gas Research Institute (GRI) and DOE that evaluated two types of bi-fuel and compressed natural gas.

LaRocque, T.

2001-10-01T23:59:59.000Z

137

SuperShuttle CNG Fleet Study Summary; Resumen de Estuidio de la Flotilla de GNC de la Empresa SuperShuttle  

DOE Green Energy (OSTI)

An account of the successful use of alternative fuels in a fleet of SuperShuttle passenger vans, which offer shared-rides between Boulder and Denver International Airport.

Eudy, L.

2001-10-01T23:59:59.000Z

138

Super-renormalizable or finite completion of the Starobinsky theory  

E-Print Network (OSTI)

The recent Planck data of Cosmic Microwave Background (CMB) temperature anisotropies support the Starobinsky theory in which the quadratic Ricci scalar drives cosmic inflation. We build up a multi-dimensional quantum consisted ultraviolet completion of the model in a phenomenological "bottom-up approach". We present the maximal class of theories compatible with unitarity and (super-)renormalizability or finiteness which reduces to the Starobinsky theory in the low-energy limit. The outcome is a maximal extension of the Krasnikov-Tomboulis-Modesto theory including an extra scalar degree of freedom besides the graviton field. The original theory was afterwards independently discovered by Biswas-Gerwick-Koivisto-Mazumdar starting from first principles. We explicitly show power counting super-renormalizability or finiteness (in odd dimensions) and unitarity (no ghosts) of the theory. Any further extension of the theory is non-unitary confirming the existence of at most one single extra degree of freedom, the scalaron. A mechanism to achieve the Starobinsky theory in string (field) theory is also investigated at the end of the paper.

Fabio Briscese; Leonardo Modesto; Shinji Tsujikawa

2013-08-06T23:59:59.000Z

139

Operation Pattern Recognition and Control for Super Capacitor Braking Energy Regeneration System of Micro EV  

Science Conference Proceedings (OSTI)

Super capacitor has some advantages of high charge-discharge rate, long life, simple structure and reliable performance, and it is especially suitable as braking energy renewable energy storage device for electric vehicle and hybrid electric vehicle. ... Keywords: Super capacitor, braking energy regeneration, micro EV, pattern recognition and control

Jinyu Qu; Liyan Liang; Zhongyu Yang

2009-12-01T23:59:59.000Z

140

Study on the Control Scheme of DFIG Wind Power System with Super Capacitors under Nonlinear Load  

Science Conference Proceedings (OSTI)

Wind energy is a kind of clean renewable energy resource with the characteristic of intermittent, fluctuant and stochastic, highly depends on the weather condition. The adoption of energy storage device based on super capacitors is an efficient way to ... Keywords: doubly fed induction generator, wind power, converter, super capacitors

Lingyun Wang; Li Huang; Jian Sun; Juan Meng

2012-05-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

An overview of SuperLU: Algorithms, implementation, and user interface  

Science Conference Proceedings (OSTI)

We give an overview of the algorithms, design philosophy, and implementation techniques in the software SuperLU, for solving sparse unsymmetric linear systems. In particular, we highlight the differences between the sequential SuperLU (including its ... Keywords: Sparse direct solver, distributed-memory computers, parallelism, scalability, supernodal factorization

Xiaoye S. Li

2005-09-01T23:59:59.000Z

142

Is There Evidence of Super Cycles in Oil Prices?* Abdel M. Zellou and John T. Cuddington**  

E-Print Network (OSTI)

since 2000 represents the early phase of a `super cycle' (SC) driven by the sustained rise in demand: is there evidence of super cycles in crude oil prices? On one hand, one might expect the strong demand associated, Colorado, USA, 30 October-2 November 2011. ** PhD candidate and William J. Coulter Professor of Mineral

143

Design of optimal digital controller for stable super-high-speed permanent-magnet synchronous  

E-Print Network (OSTI)

Design of optimal digital controller for stable super-high-speed permanent-magnet synchronous motor collaborative design scheme of a super-high-speed permanent-magnet synchronous motor (PMSM) and its digital controller is presented, which provides a low-cost but highly efficient motor system with guaranteed

Wu, Shin-Tson

144

SOLARCAP: Super Capacitor Buffering of Solar Energy for Self-Sustainable Field Systems  

E-Print Network (OSTI)

SOLARCAP: Super Capacitor Buffering of Solar Energy for Self-Sustainable Field Systems Amal Fahad of the conventional battery-based energy storage, this paper argues that the super capacitor buffering of solar energy (e.g., solar cells) and energy storage. Conventional rechargeable battery-based energy storage has

Shen, Kai

145

FDA Construction Project Serves as a Super ESPC Model | Department of  

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

FDA Construction Project Serves as a Super ESPC Model FDA Construction Project Serves as a Super ESPC Model FDA Construction Project Serves as a Super ESPC Model October 7, 2013 - 1:55pm Addthis The U.S. Food and Drug Administration (FDA) has initiated an $890 million energy-saving construction project at the site of its new headquarters-a 1940s-era Navy base in White Oak, Maryland. Using a wide range of energy efficiency measures and solar energy, it has led to one of the largest Super Energy Savings Performance Contracts (ESPC). Watch the video modules below to learn more about this successful Super ESPC project. And find out how you can apply the FDA's energy management performance model to your federal agency's construction or building renovation project. Related Links Learn more about the energy-efficient and renewable energy technologies

146

Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center |  

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

Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center Regional Super ESPC Saves Energy and Dollars at NASA Johnson Space Center October 7, 2013 - 1:57pm Addthis Space Shuttle Endeavour, 2002 The NASA Johnson Space Flight Center in Houston is well known for its achievements in the U.S. space program (this 2002 photo shows the Space Shuttle Endeavour on its way to the International Space Station). Overview NASA will save approximately $43 million in facility operations costs over the next 23 years at the Johnson Space Flight Center (JSC) in Houston, Texas, thanks to the largest delivery order signed to date under a Regional Super Energy Savings Performance Contract (Super ESPC). The U. S. Department of Energy's Federal Energy Management Program (FEMP) instituted

147

Super Cool Appliance Design Wins Student Competition | Department of Energy  

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

Cool Appliance Design Wins Student Competition Cool Appliance Design Wins Student Competition Super Cool Appliance Design Wins Student Competition August 23, 2012 - 2:44pm Addthis The winners of the Max Tech and Beyond competition -- a team of University of Maryland students -- designed and built a prototype for a wall unit air conditioner that showed more than 30 percent energy savings when tested in a lab. | Photo courtesy of Yunho Hwang, University of Maryland. The winners of the Max Tech and Beyond competition -- a team of University of Maryland students -- designed and built a prototype for a wall unit air conditioner that showed more than 30 percent energy savings when tested in a lab. | Photo courtesy of Yunho Hwang, University of Maryland. Rebecca Matulka Rebecca Matulka Digital Communications Specialist, Office of Public Affairs

148

Example Measurement & Verification Plan for a Super ESPC Project  

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

6.1 6.1 Example M&V Plan Example Measurement & Verification Plan for a Super ESPC Project February 2007 Federal Energy Management Program (FEMP) Office of Energy Efficiency and Renewable Energy U.S. Department of Energy This document was developed for the U.S. Department of Energy's Federal Energy Management Program by Nexant, Inc., and Lawrence Berkeley National Laboratory. This document is posted on FEMP's web site at www.eere.energy.gov/femp/financing/superespcs_mvresources.cfm. Comments should be sent to lwebster@nexant.com. 6.1 Example M&V Plan Contents 1. EXECUTIVE SUMMARY / M&V OVERVIEW AND PROPOSED SAVINGS CALCULATIONS ................................................................................................... 2 1.1

149

Short period eclipsing binary candidates identified using SuperWASP  

E-Print Network (OSTI)

We present light curves and periods of 53 candidates for short period eclipsing binary stars identified by SuperWASP. These include 48 newly identified objects with periods <2x10^4 seconds (~0.23d), as well as the shortest period binary known with main sequence components (GSC2314-0530 = 1SWASP J022050.85+332047.6) and four other previously known W UMa stars (although the previously reported periods for two of these four are shown to be incorrect). The period distribution of main sequence contact binaries shows a sharp cut-off at a lower limit of around 0.22d, but until now, very few systems were known close to this limit. These new candidates will therefore be important for understanding the evolution of low mass stars and to allow investigation of the cause of the period cut-off.

Norton, A J; Evans, T; West, R G; Wheatley, P J; Anderson, D R; Barros, S C C; Butters, O W; Cameron, A Collier; Christian, D J; Enoch, B; Faedi, F; Haswell, C A; Hellier, C; Holmes, S; Horne, K D; Lister, T A; Maxted, P F L; Parley, N; Pollacco, D; Simpson, E K; Skillen, I; Smalley, B; Southworth, J; Street, R A

2011-01-01T23:59:59.000Z

150

A note on super-hedging for investor-producers  

E-Print Network (OSTI)

We study the situation of an investor-producer who can trade on a financial market in continuous time and can transform some assets into others by means of a discrete time production system, in order to price and hedge derivatives on produced goods. This general framework covers the interesting case of an electricity producer who wants to hedge a financial position and can trade commodities which are also inputs for his system. This extends the framework of Bouchard and Nguyen (2011) to continuous time for concave and bounded production functions. We introduce the flexible concept of conditional sure profit along the idea of the no sure profit condition of Rasonyi (2009) and show that it allows one to provide a closedness property for the set of super-hedgeable claims in a very general setting. Using standard separation arguments, we then deduce a dual characterization of the latter.

Huu, Adrien Nguyen

2011-01-01T23:59:59.000Z

151

Solar neutrino measurements in Super-Kamiokande-II  

E-Print Network (OSTI)

The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time-variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity. The measured boron 8 total flux is 2.38 +/-0.05(stat.) +0.16-0.15(sys.) X 10^6 cm^-2 sec^-1 and the day-night difference is found to be -6.3 +/-4.2(stat.) +/-3.7(sys.) %. There is no evidence of systematic tendencies between the first and second phases.

The Super-Kamiokande collaboration

2008-03-30T23:59:59.000Z

152

Super Efficient Refrigerator Program (SERP) evaluation. Volume 1: Process evaluation  

Science Conference Proceedings (OSTI)

The Pacific Northwest National Laboratory (PNNL) conducted this study for the US Department of Energy (DOE) as part of the Super Efficient Refrigerator Program (SERP) Evaluation. This report documents the SERP formation and implementation process, and identifies preliminary program administration and implementation issues. The findings are based primarily on interviews with those familiar with the program, such as utilities, appliance manufacturers, and SERP administrators. These interviews occurred primarily between March and April 1995, when SERP was in the early stages of program implementation. A forthcoming report will estimate the preliminary impacts of SERP within the industry and marketplace. Both studies were funded by DOE at the request of SERP Inc., which sought a third-party evaluation of its program.

Sandahl, L.J.; Ledbetter, M.R.; Chin, R.I.; Lewis, K.S.; Norling, J.M.

1996-01-01T23:59:59.000Z

153

From super-charged nuclei to massive nuclear density cores  

Science Conference Proceedings (OSTI)

Due to e{sup +}e{sup -}-pair production in the field of supercritical (Z>>Z{sub cr}{approx_equal}170) nucleus an electron shell, created out of the vacuum, is formed. The distribution of the vacuum charge in this shell has been determined for super-charged nuclei Z{sub e}{sup 3} > or approx. 1 within the framework of the Thomas-Fermi equation generalized to the relativistic case. For Z{sub e}{sup 3}>>1 the electron shell penetrates inside the nucleus and almost completely screens its charge. Inside such nucleus the potential takes a constant value equal to V{sub 0} = -(3{pi}{sup 2}n{sub p}){sup 1/3}approx-2m{sub {pi}}c{sup 2}, and super-charged nucleus represents an electrically neutral plasma consisting of e, p and n. Near the edge of the nucleus a transition layer exists with a width {lambda}{approx_equal}{alpha}{sup -1/2}h-bar/m{sub {pi}}c{approx}15 fm, which is independent of Z(h-bar/m{sub {pi}}celectric field and surface charge are concentrated in this layer. These results, obtained earlier for hypothetical superheavy nuclei with Z{approx}A/2 or approx. 0.04(Z/A){sup 1/2}(m{sub Planck}/m{sub n}){sup 3} the Coulomb repulsion of protons, screened by relativistic electrons, can be balanced by gravitational forces. The overcritical electric fields E{approx}m{sup 2}{sub {pi}}c{sup 3}/eh-bar are present in the narrow transition layer near the core surface.

Popov, Vladimir [Institute of Theoretical and Experimental Physics 117218 Moscow (Russian Federation)

2010-03-24T23:59:59.000Z

154

First Regional Super ESPC a Success on Kodiak Island, Alaska | Department  

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

First Regional Super ESPC a Success on Kodiak Island, Alaska First Regional Super ESPC a Success on Kodiak Island, Alaska First Regional Super ESPC a Success on Kodiak Island, Alaska October 7, 2013 - 2:01pm Addthis Photo of new boiler at Kodiak Island facility The first delivery order included upgrades to the steam plant and boilers Jerry Reilley, ERI Services, Inc. Overview By taking a leadership role in a pilot program to streamline Federal financing and procurement for energy-saving projects, the Coast Guard is saving more than $220,000 a year in energy costs at their facility at Kodiak Island, Alaska. The project was the first under the Regional Super Energy Saving Performance Contract (ESPC) program run by the U.S. Department of Energy's Federal Energy Management Program (FEMP). Coast Guard staff completed $1.1 million of work, without needing Congressional appropriations, by

155

Major Recovery Act Project Completed at Hanford: Two New Super Cells Go  

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

Major Recovery Act Project Completed at Hanford: Two New Super Major Recovery Act Project Completed at Hanford: Two New Super Cells Go Into Service To Accept Contaminated Soil and Debris Months Ahead of Schedule and Millions Under Budget Major Recovery Act Project Completed at Hanford: Two New Super Cells Go Into Service To Accept Contaminated Soil and Debris Months Ahead of Schedule and Millions Under Budget February 23, 2011 - 12:00pm Addthis Media Contacts Cameron Hardy, DOE (509) 376-5365 Cameron.Hardy@rl.doe.gov Todd Nelson, Washington Closure (509) 372-9097 media@wch-rcc.com RICHLAND, WASH. - Two new super cells are going into service to expand disposal capacity for contaminated soil and debris at the Environmental Restoration Disposal Facility (ERDF), at the Department of Energy's (DOE) Hanford Site in southeastern Washington State.

156

Fine Tuning for Best-Value Super ESPC Deals Using the Responsibility Matrix  

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

Savings and Performance Guarantees Savings and Performance Guarantees That Work for You QUICK STUDY Fine Tuning for Best-Value Super ESPC Deals Using the Responsibility Matrix Super Energy Savings Performance Contracts (Super ESPCs) are a practical and flexible tool for obtaining energy improvements for federal facilities. While the overarching Super ESPC establishes general terms and conditions of the agree- ment between the agency and the energy service company (ESCO), the contract leaves broad latitude to custom-tailor a deal to suit the agency's own particular needs, priorities, and circumstances. The agency can precisely define the nature of the savings guarantee and how optimum performance of the energy conservation measures (ECMs) will be ensured through- out the life of the contract. A full aware-

157

SuperHILAC: Heavy-ion linear accelerator: Summary of capabilities, facilities, operations, and research  

Science Conference Proceedings (OSTI)

This report consists of a description of the accelerator facilities and a review of research programs being conducted there. Lists of SuperHILAC researchers and publications are also given.

McDonald, R.J. (ed.)

1987-09-01T23:59:59.000Z

158

Vids4Grids: Smart Meters and Super Cables | Department of Energy  

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

Grids: Smart Meters and Super Cables Grids: Smart Meters and Super Cables Vids4Grids: Smart Meters and Super Cables March 14, 2011 - 4:46pm Addthis This episode of Vids 4 Grids will take us to Itron's smart meter factory in West Union, SC where we will learn the role smart meters play in the Smart Grid. Deborah J. Buterbaugh Energy Project Specialist at National Energy Technology Laboratory What does this mean for me? Smart meters allow consumers to get real time information about their energy usage. Super cables help provide more reliable electricity to your home. In January we introduced you to the Vids4Grids project, a series of videos targeting students in high school and starting college. Through integration into curricula and online posting for open viewing, the project aims to increase awareness and create interest in power systems careers to help

159

Vids4Grids: Smart Meters and Super Cables | Department of Energy  

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

Vids4Grids: Smart Meters and Super Cables Vids4Grids: Smart Meters and Super Cables Vids4Grids: Smart Meters and Super Cables March 14, 2011 - 4:46pm Addthis This episode of Vids 4 Grids will take us to Itron's smart meter factory in West Union, SC where we will learn the role smart meters play in the Smart Grid. Deborah J. Buterbaugh Energy Project Specialist at National Energy Technology Laboratory What does this mean for me? Smart meters allow consumers to get real time information about their energy usage. Super cables help provide more reliable electricity to your home. In January we introduced you to the Vids4Grids project, a series of videos targeting students in high school and starting college. Through integration into curricula and online posting for open viewing, the project aims to increase awareness and create interest in power systems careers to help

160

LANL's Top-secret super-secure vault declassified | National Nuclear  

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

Top-secret super-secure vault declassified | National Nuclear Top-secret super-secure vault declassified | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > NNSA Blog > LANL's Top-secret super-secure vault declassified LANL's Top-secret super-secure vault declassified Posted By Office of Public Affairs NNSA Blog Down a remote canyon near Los Alamos National Laboratory lies a facility

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161

U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency  

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

and SuperPower, Inc. Increase Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's Electric Grid U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's Electric Grid February 21, 2008 - 11:29am Addthis $27 Million Project Demonstrates Advanced Superconductivity Technology ALBANY, NY- The U.S. Department of Energy (DOE) and SuperPower, Inc. today commemorated the Albany High-Temperature Superconducting (HTS) Cable Project, the world's first use of second-generation HTS wire on the grid. This 350-meter HTS cable runs between the Riverside and Menands Substations in Albany, New York. HTS cables encounter essentially no resistance in electricity flow, which increases efficiency by eliminating 7-10 percent of the energy losses of conventional copper-based cables. DOE's over $13.5

162

The Cal Poly Sustainable Power for Electrical Resources (SuPER) Project  

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

The Cal Poly Sustainable Power for Electrical Resources (SuPER) Project The Cal Poly Sustainable Power for Electrical Resources (SuPER) Project Speaker(s): James Harris Date: August 16, 2007 - 12:00pm Location: 90-3122 Seminar Host/Point of Contact: Anita Estner The Cal Poly sustainable power for electrical resources (SuPER) project has completed two years of development for a low-cost source of electrical power for the 2 billion people who do not have access. The overall goal of the Cal Poly SuPER system is to provide sustainable electrical power for a household unit over a 20-year life cycle for a total cost of $500. A prototype has been developed, and consists of a solar photovoltaic module source with battery storage, a standard DC output voltage, and a computer/digital control and status subsystem. The design is documented

163

An interactive super resolution coding approach of images and videos for enhanced user visualization  

Science Conference Proceedings (OSTI)

In this paper we propose an interactive super resolution coding technique to enhance user's visualization of received low resolution (LR) images. The proposed technique hides/embeds high frequencies and edges in the LR image, and constructs a high resolution ...

Gamal Fahmy

2011-12-01T23:59:59.000Z

164

The Cal Poly Sustainable Power for Electrical Resources (SuPER...  

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

electrical resources (SuPER) project has completed two years of development for a low-cost source of electrical power for the 2 billion people who do not have access. The overall...

165

U.S. Department of Energy and SuperPower, Inc. Increase Energy...  

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

Superconducting (HTS) Cable Project, the world's first use of second-generation HTS wire on the grid. U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency...

166

Development of multiplexing strategies for electron and super-resolution optical microscopy/  

E-Print Network (OSTI)

The aim of this work is to increase the multiplexing capabilities of electron and super resolution optical microscopy. This will be done through the development of molecular-scale barcodes that can be resolved in one of ...

Tillberg, Paul W

2013-01-01T23:59:59.000Z

167

Closed-String Tachyon Condensation and the Worldsheet Super-Higgs Effect  

E-Print Network (OSTI)

For example, in Type 0 string the- ory in the presence ofClosed-String Tachyon Condensation and the Worldsheet Super-of California. Closed-String Tachyon Condensation and the

Horava, Petr

2008-01-01T23:59:59.000Z

168

Fine Tuning for Best-Value Super ESPC Deals Using the Responsibility Matrix  

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

Savings and Performance Guarantees Savings and Performance Guarantees That Work for You QUICK STUDY Fine Tuning for Best-Value Super ESPC Deals Using the Responsibility Matrix Super Energy Savings Performance Contracts (Super ESPCs) are a practical and flexible tool for obtaining energy improvements for federal facilities. While the overarching Super ESPC establishes general terms and conditions of the agree- ment between the agency and the energy service company (ESCO), the contract leaves broad latitude to custom-tailor a deal to suit the agency's own particular needs, priorities, and circumstances. The agency can precisely define the nature of the savings guarantee and how optimum performance of the energy conservation measures (ECMs) will be ensured through- out the life of the contract. A full aware-

169

Super Hard and Slick Coatings Win R&D 100 Award  

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

Super Hard and Slick Coatings Win R&D 100 Award Super Hard and Slick Coatings Win R&D 100 Award Researchers from the U.S. Department of Energy's (DOE) Argonne National Laboratory received a R&D 100 award, as judged by R&D Magazine, in July 2009 for developing super hard and slick coating (SSC) for increased engine efficiency and component reliability. SSC is an important step towards increasing fuel efficiency in vehicles, which helps meet the administration's goals of reducing the Nation's dependence on foreign oil and decreasing greenhouse gas emissions. Argonne National Laboratory (ANL) began researching super slick coatings in 2005. The awards recognize the top scientific and technological innovations of the past year. ANL scientists have won 105 R&D 100 awards since they were first introduced in 1964.

170

U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency  

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

Department of Energy and SuperPower, Inc. Increase Energy Department of Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's Electric Grid U.S. Department of Energy and SuperPower, Inc. Increase Energy Efficiency in the Nation's Electric Grid February 21, 2008 - 11:46am Addthis $27 Million Project Demonstrates Advanced Superconductivity Technology ALBANY, NY- The U.S. Department of Energy (DOE) and SuperPower, Inc. today commemorated the Albany High-Temperature Superconducting (HTS) Cable Project, the world's first use of second-generation HTS wire on the grid. This 350-meter HTS cable runs between the Riverside and Menands Substations in Albany, New York. HTS cables encounter essentially no resistance in electricity flow, which increases efficiency by eliminating 7-10 percent of the energy losses of conventional copper-based cables. DOE's over $13.5

171

Solar neutrino results in Super-Kamiokande-III  

E-Print Network (OSTI)

The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results. With improved detector calibrations, a full detector simulation, and improved analysis methods, the systematic uncertainty on the total neutrino flux is estimated to be ?2.1%, which is about two thirds of the systematic uncertainty for the first phase of Super-Kamiokande. The observed 8B solar flux in the 5.0 to 20 MeV total electron energy region is 2.32+/-0.04 (stat.)+/-0.05 (sys.) *10^6 cm^-2sec^-1, in agreement with previous measurements. A combined oscillation analysis is carried out using SK-I, II, and III data, and the results are also combined with the results of other solar neutrino experiments. The best-fit oscillation parameters are obtained to be sin^2 {\\theta}12 = 0.30+0.02-0.01(tan^2 {\\theta}12 = 0.42+0.04 -0.02) and {\\Delta}m2_21 = 6.2+1.1-1.9 *10^-5eV^2. Combined with KamLAND results, the best-fit oscillation parameters are found to be sin^2 {\\theta}12 = 0.31+/-0.01(tan^2 {\\theta}12 = 0.44+/-0.03) and {\\Delta}m2_21 = 7.6?0.2*10^-5eV^2 . The 8B neutrino flux obtained from global solar neutrino experiments is 5.3+/-0.2(stat.+sys.)*10^6cm^-2s^-1, while the 8B flux becomes 5.1+/-0.1(stat.+sys.)*10^6cm^-2s^-1 by adding KamLAND result. In a three-flavor analysis combining all solar neutrino experiments, the upper limit of sin^2 {\\theta}13 is 0.060 at 95% C.L.. After combination with KamLAND results, the upper limit of sin^2 {\\theta}13 is found to be 0.059 at 95% C.L..

K. Abe; Y. Hayato; T. Iida; M. Ikeda; C. Ishihara; K. Iyogi; J. Kameda; K. Kobayashi; Y. Koshio; Y. Kozuma; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Ogawa; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; K. Ueno; K. Ueshima; H. Watanabe; S. Yamada; T. Yokozawa; S. Hazama; H. Kaji; T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; M. R. Vagins; L. Labarga; L. M Magro; F. Dufour; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; W. Wang; M. Goldhaber; K. Bays; D. Casper; J. P. Cravens; W. R. Kropp; S. Mine; C. Regis; A. Renshaw; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. Albert; R. Wendell; T. Wongjirad; K. Scholberg; C. W. Walter; T. Ishizuka; S. Tasaka; J. G. Learned; S. Matsuno; Y. Watanabe; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; H. Nishino; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; A. Minamino; T. Nakaya; Y. Fukuda; Y. Itow; G. Mitsuka; T. Tanaka; C. K. Jung; G. Lopez; C. McGrew; R. Terri; C. Yanagisawa; N. Tamura; H. Ishino; A. Kibayashi; S. Mino; T. Mori; M. Sakuda; H. Toyota; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; T. Ishizuka; H. Okazawa; Y. Choi; K. Nishijima; Y. Yokosawa; M. Koshiba; Y. Totsuka; M. Yokoyama; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; E. Thrane; R. J. Wilkes

2010-10-01T23:59:59.000Z

172

Super-Planckian Near-Field Thermal Emission with Phonon-Polaritonic Hyperbolic Metamaterials  

E-Print Network (OSTI)

We study super-Planckian near-field heat exchanges for multilayer hyperbolic metamaterials using exact S-matrix calculations. We investigate heat exchanges between two multilayer hyperbolic metamaterial structures. We show that the super- Planckian emission of such metamaterials can either come from the presence of surface phonon-polaritons modes or from a continuum of hyperbolic modes depending on the choice of composite materials as well as the structural configuration.

Biehs, Svend-Age; Messina, Riccardo; Ben-Abdallah, Philippe

2013-01-01T23:59:59.000Z

173

SuperShuttle CNG Fleet Evaluation--Final Report  

DOE Green Energy (OSTI)

The mission of the US Department of Energy's Office of Transportation Technologies is to promote the development and deployment of transportation technologies that reduce US dependence on foreign oil, while helping to improve the nation's air quality and promoting US competitiveness. In support of this mission, DOE has directed the National Renewable Energy Laboratory to conduct projects to evaluate the performance and acceptability of alternative fuel vehicles. NREL has undertaken several fleet study projects, which seek to provide objective real-world fleet experiences with AFVs. For this type of study we collect, analyze, and report on operational, cost, emissions, and performance data from AFVs being driven in a fleet application. The primary purpose of such studies is to make real-world information on AFVs available to fleet managers and other potential AFV purchasers. For this project, data was collected from 13 passenger vans operating in the Boulder/Denver, Colorado area. The study vehicles were all 1999 Ford E-350 passenger vans based at SuperShuttle's Boulder location. Five of the vans were dedicated CNG, five were bi-fuel CNG/gasoline, and three were standard gasoline vans that were used for comparison.

Eudy, L.

2000-12-07T23:59:59.000Z

174

Overview of the SuperNova/Acceleration probe (SNAP)  

SciTech Connect

The SuperNova/Acceleration Probe (SNAP) is a space-based experiment to measure the expansion history of the Universe and study both its dark energy and the dark matter. The experiment is motivated by the startling discovery that the expansion of the Universe is accelerating. A 0.7 square-degree imager comprised of 36 large format fully-depleted n-type CCD's sharing a focal plane with 36 HgCdTe detectors forms the heart of SNAP, allowing discovery and lightcurve measurements simultaneously for many supernovae. The imager and a high-efficiency low-resolution integral field spectrograph are coupled to a 2-m three mirror anastigmat wide-field telescope, which will be placed in a high-earth orbit. The SNAP mission can obtain high-signal-to-noise calibrated light-curves and spectra for over 2000 Type Ia supernovae at redshifts between z = 0.1 and 1.7. The resulting data set can not only determine the amount of dark energy with high precision, but test the nature of the dark energy by examining its equation of state. In particular, dark energy due to a cosmological constant can be differentiated from alternatives such as ''quintessence'', by measuring the dark energy's equation of state to an accuracy of {+-} 0.05, and by studying its time dependence.

galdering@lbl.gov

2002-07-29T23:59:59.000Z

175

SuperCDMS status from Soudan and plans for SNOLab  

SciTech Connect

Matter, as we know it, makes up less than 5% of the Universe. Various astrophysical observations have confirmed that one quarter of the Universe and most of the matter content in the Universe is made up of Dark Matter. The nature of Dark Matter is yet to be discovered and is one of the biggest questions in Physics. Particle Physics combined with astrophysical measurements of the abundance gives rise to a Dark Matter candidate called Weakly Interacting Massive Particle (WIMP). The low density of WIMPs in the galaxies and the extremely weak nature of the interaction with ordinary matter make detection of the WIMP an extraordinarily challenging task, with abundant fakes from various radioactive and cosmogenic backgrounds with much stronger electromagnetic interaction. The extremely weak nature of the WIMP interaction dictates detectors that have extremely low naturally occurring radioactive background, a large active volume (mass) of sensitive detector material to maximize statistics, a highly efficient detector based rejection mechanism for the dominant electromagnetic background and sophisticated analysis techniques to reject any residual background. This paper describes the status of the SuperCDMS experiment.

Sander, J.; Jastram, A.; Koch, K.; Mahapatra, R.; Prasad, K. [Department of Physics, Texas A and M University, College Station, TX 77843 (United States); Ahmed, Z.; Cornell, B.; Golwala, S. R.; Moore, D. C.; Nelson, R. [Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States); Anderson, A. J.; Figueroa-Feliciano, E.; Hertel, S. A.; Leman, S. W.; Mccarthy, K. A. [Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States); Arrenberg, S. [Physics Institute, University of Zrich, Winterthurerstr. 190, CH-8057 (Switzerland); Balakishiyeva, D.; Saab, T.; Welliver, B. [Department of Physics, University of Florida, Gainesville, FL 32611 (United States); Thakur, R. B. [Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States); and others

2013-05-23T23:59:59.000Z

176

2012 CERTS R&M Peer Review - Summary: Commercialization of the SuperOPF Framework - Hsiao-Dong Chiang  

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

Commercialization of the SuperOPF Framework: Phase 2 Commercialization of the SuperOPF Framework: Phase 2 Project Lead: Hsiao-Dong Chiang Co-investigators: Bin Wang, Patrick Causgrove, Ray Zimmerman 1. Project Objectives: The stochastic contingency-based security constrained AC Optimal Power Flow formulation behind the SuperOPF makes it very applicable to a variety of problems arising in power system planning and operations under deregulation. The ultimate goal of this project is to develop a commercial-grade SuperOPF in the context of co-optimization framework that correctly accounts for contingencies, ancillary services, static and dynamic constraints in determining both dispatch, price and operating reserve. This phase is focused on the following: (i) enhancing SuperOPF (into SuperOPF-VS

177

Super Boiler 2nd Generation Technology for Watertube Boilers  

Science Conference Proceedings (OSTI)

This report describes Phase I of a proposed two phase project to develop and demonstrate an advanced industrial watertube boiler system with the capability of reaching 94% (HHV) fuel-to-steam efficiency and emissions below 2 ppmv NOx, 2 ppmv CO, and 1 ppmv VOC on natural gas fuel. The boiler design would have the capability to produce >1500 F, >1500 psig superheated steam, burn multiple fuels, and will be 50% smaller/lighter than currently available watertube boilers of similar capacity. This project is built upon the successful Super Boiler project at GTI. In that project that employed a unique two-staged intercooled combustion system and an innovative heat recovery system to reduce NOx to below 5 ppmv and demonstrated fuel-to-steam efficiency of 94% (HHV). This project was carried out under the leadership of GTI with project partners Cleaver-Brooks, Inc., Nebraska Boiler, a Division of Cleaver-Brooks, and Media and Process Technology Inc., and project advisors Georgia Institute of Technology, Alstom Power Inc., Pacific Northwest National Laboratory and Oak Ridge National Laboratory. Phase I of efforts focused on developing 2nd generation boiler concepts and performance modeling; incorporating multi-fuel (natural gas and oil) capabilities; assessing heat recovery, heat transfer and steam superheating approaches; and developing the overall conceptual engineering boiler design. Based on our analysis, the 2nd generation Industrial Watertube Boiler when developed and commercialized, could potentially save 265 trillion Btu and $1.6 billion in fuel costs across U.S. industry through increased efficiency. Its ultra-clean combustion could eliminate 57,000 tons of NOx, 460,000 tons of CO, and 8.8 million tons of CO2 annually from the atmosphere. Reduction in boiler size will bring cost-effective package boilers into a size range previously dominated by more expensive field-erected boilers, benefiting manufacturers and end users through lower capital costs.

Mr. David Cygan; Dr. Joseph Rabovitser

2012-03-31T23:59:59.000Z

178

Superconducting Super Collider silicon tracking subsystem research and development  

SciTech Connect

The Alamos National Laboratory Mechanical Engineering and Electronics Division has been investigating silicon-based elementary particle tracking device technology as part of the Superconducting Super Collider-sponsored silicon subsystem collaboration. Structural, materials, and thermal issues have been addressed. This paper explores detector structural integrity and stability, including detailed finite element models of the silicon wafer support and predictive methods used in designing with advanced composite materials. The current design comprises a magnesium metal matrix composite (MMC) truss space frame to provide a sparse support structure for the complex array of silicon detectors. This design satisfies the 25-{mu}m structural stability requirement in a 10-Mrad radiation environment. This stability is achieved without exceeding the stringent particle interaction constraints set at 2.5% of a radiation length. Materials studies have considered thermal expansion, elastic modulus, resistance to radiation and chemicals, and manufacturability of numerous candidate materials. Based on optimization of these parameters, the MMC space frame will possess a coefficient of thermal expansion (CTE) near zero to avoid thermally induced distortions, whereas the cooling rings, which support the silicon detectors and heat pipe network, will probably be constructed of a graphite/epoxy composite whose CTE is engineered to match that of silicon. Results from radiation, chemical, and static loading tests are compared with analytical predictions and discussed. Electronic thermal loading and its efficient dissipation using heat pipe cooling technology are discussed. Calculations and preliminary designs for a sprayed-on graphite wick structure are presented. A hydrocarbon such as butane appears to be a superior choice of heat pipe working fluid based on cooling, handling, and safety criteria.

Miller, W.O.; Thompson, T.C.; Ziock, H.J. (Los Alamos National Lab., NM (USA)); Gamble, M.T. (Massachusetts Inst. of Tech., Cambridge, MA (USA). Dept. of Materials Science and Engineering)

1990-12-01T23:59:59.000Z

179

Information Resources: L Prize(tm): The Race for Super Efficient Light Bulbs  

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

L Prize(tm): The Race for Super Efficient Light Bulbs L Prize(tm): The Race for Super Efficient Light Bulbs This September 23, 2008 webcast provided an overview of the Bright Tomorrow Lighting Prize (L Prize) technology competition. The L Prize calls for super-efficient SSL products to replace two of the most common light bulbs used today: the 60-watt incandescent and the PAR-38 halogen reflector. Kelly Gordon, Pacific Northwest National Laboratory, kicked off the webcast with an overview of the competition requirements, evaluation process, and opportunities for promotion of the winning products. Mary Matteson Bryan, Pacific Gas & Electric, and Liesel Whitney-Schulte, Wisconsin Focus on Energy, followed with a look at the role of L Prize partners and plans for their organizations to support the winning products through demonstrations, education, promotions, and other collaborative efforts.

180

Calorimeter R&D for the SuperNEMO Double Beta Decay Experiment  

E-Print Network (OSTI)

SuperNEMO is a next-generation double beta decay experiment based on the successful tracking plus calorimetry design approach of the NEMO3 experiment currently running in the Laboratoire Souterrain de Modane (LSM). SuperNEMO can study a range of isotopes, the baseline isotopes are 82Se and possibly 150Nd. The total isotope mass will be 100-200 kg. A sensitivity to neutrinoless double beta decay half-life greater than 10e26 years can be reached which gives access to Majorana neutrino masses of 50-100 meV. One of the main challenges of the SuperNEMO R&D is the development of the calorimeter with an unprecedented energy resolution of 4% FWHM at 3 MeV (Qbb value of 82Se).

Matthew Kauer; for the SuperNEMO Collaboration

2008-07-14T23:59:59.000Z

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181

Analysis of Godiva-IV delayed-critical and static super-prompt-critical conditions  

SciTech Connect

Super-prompt-critical burst experiments were conducted on the Godiva-IV assembly at Los Alamos National Laboratory from the 1960s through 2005. Detailed and simplified benchmark models have been constructed for four delayed-critical experiments and for the static phase of a super-prompt-critical burst experiment. In addition, a two-dimensional cylindrical model has been developed for the super-prompt-critical condition. Criticality calculations have been performed for all of those models with four modern nuclear data libraries: ENDFIB-VI, ENDF/8-VII.0, JEFF-3.1 , and JENDL-3.3. Overall, JENDL-3.3 produces the best agreement with the reference values for k{sub eff}.

Mosteller, Russell D [Los Alamos National Laboratory; Goda, Joetta M [Los Alamos National Laboratory

2009-01-01T23:59:59.000Z

182

The Solar Neutrino Day/Night Effect in Super-Kamiokande  

E-Print Network (OSTI)

The time variation of the elastic scattering rate of solar neutrinos with electrons in Super-Kamiokande-I was fit to the day/night variations expected from active two-neutrino oscillations in the Large Mixing Angle region. Combining Super-Kamiokande measurements with other solar and reactor neutrino data, the mixing angle is determined as sin^2theta=0.276+0.033-0.026 and the mass squared difference between the two neutrino mass eigenstates as Delta m^2=7.1+0.6-0.5x10^-5eV^2. For the best fit parameters, a day/night asymmetry of -1.7+-1.6(stat)+1.3-1.2(syst)% was determined from the Super-Kamiokande data, which has improved statistical precision over previous measurements and is in excellent agreement with the expected value of -1.6%.

Michael Burghard Smy; for the Super-Kamiokande Collaboration

2003-10-31T23:59:59.000Z

183

Three-dimensional Q (super -1) model of the Coso Hot Springs known  

Open Energy Info (EERE)

Q (super -1) model of the Coso Hot Springs known Q (super -1) model of the Coso Hot Springs known geothermal resource area (in Coso geothermal area) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: Three-dimensional Q (super -1) model of the Coso Hot Springs known geothermal resource area (in Coso geothermal area) Details Activities (3) Areas (1) Regions (0) Abstract: Observations of teleseismic P waves above geothermal systems exhibit travel time delays and anomalously high seismic attenuation, which is extremely useful in estimating the thermal regime and the potential of the system. A regional telemetered network of sixteen stations was operated by the U.S. Geological Survey in the Coso Hot Springs Known Geothermal Resources Area (KGRA) for such studies from September 1975 to October 1976.

184

5 Super-Sized Solar Projects Transforming the Clean Energy Landscape |  

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

Super-Sized Solar Projects Transforming the Clean Energy Super-Sized Solar Projects Transforming the Clean Energy Landscape 5 Super-Sized Solar Projects Transforming the Clean Energy Landscape April 8, 2013 - 4:00pm Addthis The California Valley Solar Ranch has a capacity of 250 MW -- enough energy to power the equivalent of every home in San Luis Obispo County. | Photo courtesy of SunPower. The California Valley Solar Ranch has a capacity of 250 MW -- enough energy to power the equivalent of every home in San Luis Obispo County. | Photo courtesy of SunPower. Arial shot of the California Valley Solar Ranch in San Luis Obispo County. | Photo courtesy of SunPower. Arial shot of the California Valley Solar Ranch in San Luis Obispo County. | Photo courtesy of SunPower. The Alamosa Solar project in Colorado is the largest high-concentration solar facility in the world. | Photo courtesy of Cogentrix.

185

Post-Acceleration Study for Neutrino Super-beam at CSNS  

E-Print Network (OSTI)

A post-acceleration system based on the accelerators at CSNS (China Spallation Neutron Source) is proposed to build a super-beam facility for neutrino physics. Two post-acceleration schemes, one using superconducting dipole magnets in the main ring and the other using room-temperature magnets have been studied, both to achieve the final proton energy of 128 GeV and the beam power of 4 MW by taking 10% of the CSNS beam from the neutron source. The main design features and the comparison for the two schemes are presented. The CSNS super-beam facility will be very competitive in long-baseline neutrino physics studies, compared with other super-beam facilities proposed in the world.

Yang Wu; Jingyu Tang

2012-12-24T23:59:59.000Z

186

U.S. DRIVE Highlights of Technical Accomplishments 2011: Super Duty Diesel Truck with NOx Aftertreatment  

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

2011 U.S. DRIVE Highlight Advanced Combustion and Emission Control 2011 Super Duty Diesel Truck with NO x Aftertreatment Diesel engine aftertreatment: Minimizing NO x emissions with SCR. Ford's 2011 Super Duty diesel truck-which utilizes aftertreatment technology jointly developed by Ford and the U.S. Department of Energy (DOE)-deliv- ered a multitude of firsts for the company. It was the first Ford diesel engine developed entirely in-house, the first to operate on B20 (a blend of 20% biofuel, 80% petroleum diesel), and the first to comply with

187

Super-radiance in the sodium resonance lines from sodium iodide arc lamps  

Science Conference Proceedings (OSTI)

Super-radiance observed within the centers of the sodium resonance D lines emitted by arc lamps containing sodium iodide as additive in a high-pressure mercury plasma environment was studied by high-resolution emission spectroscopy. The spectral radiance of these self-reversed lines including super-radiance was simulated by considering a local enhancement of the source function due to the presence of an additional source of radiation near the arc wall. Causes of this hitherto unrecognized source of radiation are given.

Karabourniotis, D. [Department of Physics, Institute of Plasma Physics, University of Crete, 71003 Heraklion (Greece); Drakakis, E. [Department of Electrical Engineering, Technological Educational Institute, Heraklion (Greece)

2010-08-09T23:59:59.000Z

188

Search for Differences in Oscillation Parameters for Atmospheric Neutrinos and Antineutrinos at Super-Kamiokande  

E-Print Network (OSTI)

We present a search for differences in the oscillations of antineutrinos and neutrinos in the Super-Kamiokande -I, -II, and -III atmospheric neutrino sample. Under a two-flavor disappearance model with separate mixing parameters between neutrinos and antineutrinos, we find no evidence for a difference in oscillation parameters. Best fit antineutrino mixing is found to be at (dm2bar, sin2 2 thetabar) = (2.0x10^-3 eV^2, 1.0) and is consistent with the overall Super-K measurement.

Super-Kamiokande Collaboration; :; K. Abe; Y. Hayato; T. Iida; M. Ikeda; K. Iyogi; J. Kameda; Y. Koshio; Y. Kozuma; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; Y. Takeuchi; K. Ueno; K. Ueshima; H. Watanabe; S. Yamada; T. Yokozawa; C. Ishihara; H. Kaji; K. P. Lee; T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; K. Martens; M. R. Vagins; L. Labarga; L. M. Magro; F. Dufour; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; M. Goldhaber; K. Bays; W. R. Kropp; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. B. Albert; K. Scholberg; C. W. Walter; R. Wendell; T. M. Wongjirad; S. Tasaka; J. G. Learned; S. Matsuno; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; H. Nishino; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; A. Minamino; T. Nakaya; Y. Fukuda; Y. Itow; G. Mitsuka; T. Tanaka; C. K. Jung; I. Taylor; C. Yanagisawa; H. Ishino; A. Kibayashi; S. Mino; T. Mori; M. Sakuda; H. Toyota; Y. Kuno; S. B. Kim; B. S. Yang; T. Ishizuka; H. Okazawa; Y. Choi; K. Nishijima; M. Koshiba; M. Yokoyama; Y. Totsuka; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; R. J. Wilkes

2011-09-08T23:59:59.000Z

189

A robust super-efficiency data envelopment analysis model for ranking of provincial gas companies in Iran  

Science Conference Proceedings (OSTI)

Conventional super-efficiency data envelopment analysis (DEA) models require the exact information of inputs or outputs. However, in many real world applications this simple assumption does not hold. Stochastic super-efficiency is one of recent methods ... Keywords: Data envelopment analysis, Rank, Robust optimization, Uncertainty

S. J. Sadjadi; H. Omrani; S. Abdollahzadeh; M. Alinaghian; H. Mohammadi

2011-09-01T23:59:59.000Z

190

16000-64000 B pMTU experiments with simulation: The case for super jumbo frames at Supercomputing '05  

Science Conference Proceedings (OSTI)

This paper presents a case study including the results and preliminary simulations for a series of Ethernet-based Xnet ''super jumbo frame'' (SJF) experiments conducted prior to and at Supercomputing '05, for up-to-64000 B path MTU. As far as we are ... Keywords: Maximum transmission unit, Network protocols, Network testing, Networks, Path MTU, Super jumbo frames

W. Rutherford; L. Jorgenson; M. Siegert; P. Van Epp; L. Liu

2007-06-01T23:59:59.000Z

191

Fluctuation limits of the super-Brownian motion with a single point catalyst  

E-Print Network (OSTI)

We prove a fluctuating limit theorem of a sequence of super-Brownian motions over $\\mbb{R}$ with a single point catalyst. The weak convergence of the processes on the space of Schwarz distributions is established. The limiting process is an Ornstein-Uhlenbeck type process solving a Langevin type equation driven by a one-dimensional Brownian motion.

Li, Zenghu

2009-01-01T23:59:59.000Z

192

Request for Support for the Conference on Super Intense Laser Atom Physics  

Science Conference Proceedings (OSTI)

The Conference on Super Intense Laser Atom Physics (SILAP) was held in November 2003 in Dallas, Texas. The venue for the meeting was South Fork Ranch in the outskirts of Dallas. The topics of the meeting included high harmonic generation and attosecond pulse generation, strong field interactions with molecules and clusters, particle acceleration, and relativistic laser atom interactions.

Todd Ditmire

2004-10-21T23:59:59.000Z

193

Total System Cost Analysis of Master-Slave Multi-super-Hypercube DX-tree Architecture  

Science Conference Proceedings (OSTI)

In recent years the area of High Performance Computing (HPC) has received an outstanding support both from the users as well as the computer system designers. This support is mainly due to the increase of the complexity and density of the data processing ... Keywords: DX-Tree architecture, XTree architecture, cost analysis, high performance computing, super-hypercube architecture

Hamid Abachi

2013-07-01T23:59:59.000Z

194

Search of Kaonic Nuclear States at the SuperB factory  

E-Print Network (OSTI)

The search of nuclear bound states of anti-K in few-body nuclear systems such as K-pp, can be extended from the nuclear medium to the vacuum, using the glue-rich Y(1S) decays at B-factories. Here the possibility for such a measurement at the future SuperB factory is discussed.

S. Marcello; F. De Mori; A. Filippi

2012-10-10T23:59:59.000Z

195

Probing the Birth of Super Star Clusters: Implications for Massive Star Formation  

E-Print Network (OSTI)

Super Star Clusters are one of the most extreme star forming environments in the universe, and the most massive and dense of these may be proto globular clusters. Like individual massive stars, the earliest stages of super star cluster evolution are deeply obscured, and therefore our knowledge about their birth environments is currently very incomplete. However, the study of natal super star clusters has become somewhat of a cottage industry in recent years, and the sample of such objects has been growing rapidly with high-quality long-wavelength data now available from a number of observatories. The natal super star clusters identified in thermal-infrared and radio observations represent the youngest stage of massive star cluster evolution yet observed. Their properties appear to be similar to those of ultracompact HII regions in the Milky Way, but scaled up in total mass and luminosity. I will overview what we think we know about these objects based on existing observations, discuss their relationship to ultracompact HII regions, present new models of their spectral energy distributions based on 3-D simulations, and outline some of the most significant gaps in our current understanding.

Kelsey E. Johnson

2005-06-21T23:59:59.000Z

196

Super-resolution in medical imaging: an illustrative approach through ultrasound  

Science Conference Proceedings (OSTI)

The requirements for better resolution in all medical imaging modalities currently represent a very important and open challenge. Accurate measurement and visualization of structure in living tissues is intrinsically limited by the imaging system features. ... Keywords: AR model, medical imaging, multidimensional, super-resolution, ultrasound

D. Kouam; M. Ploquin

2009-06-01T23:59:59.000Z

197

Generative Models for Super-Resolution Single Molecule Microscopy Images of Biological Structures  

E-Print Network (OSTI)

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41 3.2 Conventional fluorescence image (A) and STORM reconstruction (B,C) of annular clathrin introduced by Ernst Abbe in 1873. Super-resolution (SR) imaging has led to various important studies the fluorescence of the molecules so that a subset of molecules are emitting at any given time and thus

198

Contracting practices for the underground construction of the Superconducting Super Collider  

SciTech Connect

This report was prepared by a specially appointed committee under the auspices of the National Academy of Sciences/National Research Council to address contracting and associated management issues essential to the successful execution of underground construction for the Superconducting Super Collider.

Not Available

1989-01-01T23:59:59.000Z

199

SuperLU_DIST: A scalable distributed-memory sparse direct solver for unsymmetric linear systems  

Science Conference Proceedings (OSTI)

We present the main algorithmic features in the software package SuperLU_DIST, a distributed-memory sparse direct solver for large sets of linear equations. We give in detail our parallelization strategies, with a focus on scalability issues, and demonstrate ... Keywords: Sparse direct solver, distributed-memory computers, parallelism, scalability, supernodal factorization

Xiaoye S. Li; James W. Demmel

2003-06-01T23:59:59.000Z

200

Super-Cerenkov Radiation: A new phenomenon useful for RICH Detectors  

E-Print Network (OSTI)

In this contribution the Super-Cerenkov radiation (SCR) as a new phenomenon which includes in a more general and exact form the usual Cerenkov effect is presented. The Super-Cerenkov effect at Cerenkov threshold in the radiators of RICH detectors is investigated. The results on the experimental test of the super- Cerenkov coherence conditions are presented. The SCR-predictions are verified experimentally with high accuracy chi/n_{dof}=1.47 by the data on the Cerenkov ring radii of electron, muon, pion and kaon, all measured with RICH detector. Moreover, it is shown that the Super-Cerenkov phenomenon can explain not only subthreshold CR but also the observed secondary rings (or anomalous Cerenkov radiation) observed at CERN SPS accelerator. The influence of medium on the particle propagation properties is also estimated and the refractive properties of electrons, muons, pions, in the radiator C4F10Ar are obtained. So, we proved that the refractive indices of the charged elementary particles in medium are also very important for the RICH detectors, especially at low and intermediate energies.

D. B. Ion; M. L. Ion

2004-12-11T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Implementation and optimization of a new super-resolution technique in PET imaging  

Science Conference Proceedings (OSTI)

Super-Resolution (SR) techniques are used in PET imaging to generate a high-resolution image by combining multiple low-resolution images that have been acquired from different points of view (POV). In this paper, we propose a new implementation of the ...

Guoping Chang; Tinsu Pan; John W. Clark; Osama R. Mawlawi

2009-06-01T23:59:59.000Z

202

Testing Non-Universal Neutrino Couplings with the Super-Kamiokande Solar Data  

Science Conference Proceedings (OSTI)

We present a phenomenological analysis of the non-universal flavor conserving neutrino couplings in the framework of non-standard neutrino interactions. We use the neutrino scattering off electrons in the Super-Kamiokande solar neutrino data. We show that it is possible to obtain constraints that are complementary to the current bounds.

Bolanos, A. [Departamento de Fisica, Centro de Investigacion y de Estudios Avanzados del IPN, Apartado Postal 14-740 07000 Mexico D F (Mexico)

2008-07-02T23:59:59.000Z

203

China: A Rising Scientific (Super-)Power & a Node Embedded in the Global Scientific  

E-Print Network (OSTI)

China: A Rising Scientific (Super-)Power & a Node Embedded in the Global Scientific Network Cong Cao, Ph.D. University of Nottingham Cong.cao@nottingham.ac.uk #12;· China as a Rising Scientific) #12;The Global Scientific Network (25 nations, 2004) #12;· China as a Node Embedded in the Global

Rambaut, Andrew

204

NIST Saha Database: Codes and Contributors  

Science Conference Proceedings (OSTI)

... Las Palmas, Spain. ATOMIC, CJFontes, P.Hakel, J.Abdallah, HLZhang, J.Colgan, M.Sherrill, S.Mazevet, LANL, USA. AVERROES_C1, ...

2013-07-16T23:59:59.000Z

205

Scale Dependence of Radar Rainfall Uncertainty: Initial Evaluation of NEXRADs New Super-Resolution Data for Hydrologic Applications  

Science Conference Proceedings (OSTI)

This study explores the scale effects of radar rainfall accumulation fields generated using the new super-resolution level II radar reflectivity data acquired by the Next Generation Weather Radar (NEXRAD) network of the Weather Surveillance Radar-...

Bong-Chul Seo; Witold F. Krajewski

2010-10-01T23:59:59.000Z

206

Empirical Assessment of Shareholder Incentive Mechanisms Designs under Aggressive Savings Goals: Case Study of a Kansas "Super-Utility"  

E-Print Network (OSTI)

period as the super-utilitys rate base continues togrowth Utility Budget Category Capital Expenditure Rate baseAnnual Growth Rate (%) N/A Motivating utilities to achieve

Cappers, Peter

2010-01-01T23:59:59.000Z

207

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star  

E-Print Network (OSTI)

The absolute magnitudes of Type IA supernovae. Astrophys. J.in a Sublu- o minous Type Ia Supernova: SpectropolarimetryL. Could There Be a Hole in Type Ia Super- novae? Astrophys.

2008-01-01T23:59:59.000Z

208

Cellular delivery and site-specific targeting of organic fluorophores for super-resolution imaging in living cells  

E-Print Network (OSTI)

Recent advances in super-resolution fluorescence microscopy have pushed the spatial resolution of biological imaging down to a few nanometers. The key element to the development of such imaging modality is synthetic organic ...

Uttamapinant, Chayasith

2013-01-01T23:59:59.000Z

209

Financial Impact of Energy Efficiency under a Federal Renewable Electricity Standard: Case Study of a Kansas "super-utility"  

E-Print Network (OSTI)

first-year 2012 cost for wind energy under a power purchaseCost Study of the 2015 Wind Challenge: An Assessment of Wind Energycosts, we assumed that the super-utility had a preference for wind energy.

Cappers, Peter

2010-01-01T23:59:59.000Z

210

SuperShuttle CNG Fleet Study Summary: Clean Cities Alternative Fuel Information Series, Alternative Fuel Case Study  

DOE Green Energy (OSTI)

An account of the successful use of alternative fuels in a fleet of SuperShuttle passenger vans, which offer shared-rides between Boulder and Denver International Airport.

Eudy, L.

2001-03-05T23:59:59.000Z

211

NREL: News Feature - Super-Efficient Cells Key to Low-Cost Solar Power  

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

Super-Efficient Cells Key to Low-Cost Solar Power Super-Efficient Cells Key to Low-Cost Solar Power February 16, 2011 This photo shows eight Amonix 7700 solar power generators, those in front tilted horizontally, those in the rear tilted near vertically. Each is a huge rectangle divided into hundreds of squares holding cells and lenses. Enlarge image The Amonix 7700 Concentrated Photovoltaic (CPV) Solar Power Generators are showcasing reliability and undergoing validation-of-performance measurements at the SolarTAC facility in Aurora, Colo. Credit: Dennis Schroeder In this photo, a man in an orange safety vest and hardhat is using a laptop, with large concentrated photovoltaic generators in the background. Enlarge image A technician at SolarTAC in Aurora, CO, enters some numbers into a laptop as he monitors validation of the Amonix 7700 Solar Power Generators.

212

Super-Tonks-Girardeau Gas of Spin-1/2 Interacting Fermions  

SciTech Connect

Fermi gases confined in tight one-dimensional waveguides form two-particle bound states of atoms in the presence of a strongly attractive interaction. Based on the exact solution of the one-dimensional spin-1/2 interacting Fermi gas, we demonstrate that a stable excited state with no pairing between attractive fermionic atoms can be realized by a sudden switch of interaction from the strongly repulsive regime to strongly attractive regime. Such a state is an exact fermionic analog of the experimentally observed super-Tonks-Girardeau state of bosonic Cesium atoms [Science 325, 1224 (2009)] and should be possible to be observed by the experiment. The frequency of the lowest breathing mode of the fermionic super-Tonks-Girardeau gas is calculated as a function of the interaction strength, which could be used as a detectable signature for the experimental observation.

Guan Liming; Chen Shu [Institute of Physics, Chinese Academy of Sciences, Beijing 100190 (China)

2010-10-22T23:59:59.000Z

213

The role of the tropical super greenhouse effect in heating the ocean surface  

SciTech Connect

Measurements made by a Fourier transform infrared (FTIR) spectroradiometer operating in the middle infrared (5 to 20 micrometers, with a spectral resolution of one inverse centimeter) imply that there is an anomalously large greenhouse effect over equatorial oceans that is caused by water vapor. As sea-surface temperature increased from 297 to 303 degrees kelvin, the net infrared cooling at the surface decreased by 30 to 50 watts per square meter. Thus, according to the FTIR data, the super greenhouse effect that has been inferred from satellite measurements contributes directly to radiative heating of the sea surface. The data demonstrate that most of this heating occurs in the middle infrared by means of the continuum emission window of water vapor and that tropical deep convection contributes substantially to this super greenhouse effect.

Lubin, D. (Univ. of California, San Diego, CA (United States))

1994-07-08T23:59:59.000Z

214

New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP)  

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

New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP) New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP) The Equation of the Universe PowerPoint Presentation The Cosmological Constant Slide 5 Hubble's Great Discovery - and Einstein's "biggest blunder" Slide 7 Slide 8 Slide 9 Slide 10 Slide 11 Slide 12 Slide 13 Slide 14 A Revolution in Cosmology Slide 16 Who Ordered That?! What we don't know Slide 19 Slide 20 Slide 21 Dark Energy Task Force Slide 23 Slide 24 Slide 25 Slide 26 Slide 27 "Standard-izable" Candles Slide 29 Slide 30 Slide 31 Slide 32 Slide 33 Slide 34 Slide 35 Slide 36 Slide 37 Slide 38 Slide 39 What is the Physical Mechanism for Type Ia SNe? Discovering Supernovae Slide 42 The Expansion History of the Universe Discovering Supernovae from Space Gravitational Weak Lensing Slide 46 Slide 47

215

CATEGORICAL EXCLUSION TO INSTALL EMSL SUPER-COMPUTER POWER INFRASTRUCTURE, PACIFIC NORTHWEST NATIONAL  

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

TO INSTALL EMSL SUPER-COMPUTER TO INSTALL EMSL SUPER-COMPUTER POWER INFRASTRUCTURE, PACIFIC NORTHWEST NATIONAL LABORATORY, RICHLAND, WASHINGTON Proposed Action: The U.S. Department of Energy (DOE) Pacific Northwest Site Office (PNSO) proposes to provide enhanced electrical service to the Environmental Molecular Sciences Laboratory (EMSL) to provide an increased power capacity for future facility computational developments. Location of Action: The electrical service would be installed underground via excavation in the lawn and gravel area between EMSL, room 1145, west toward the northeast comer of the Biological Sciences Facility (BSF), in Richland, Washington. The excavation would also extend north-south for about 450 feet along the property line between EMSL and BSF. Please refer to Figure 1.

216

Coordinate-Space Hartree-Fock-Bogoliubov Solvers for Super fluid Fermi  

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

Coordinate-Space Hartree-Fock-Bogoliubov Solvers for Super fluid Fermi Coordinate-Space Hartree-Fock-Bogoliubov Solvers for Super fluid Fermi Systems in Large Boxes Submitted by mkaczmar on March 29, 2013 - 12:53 Authors: Pei, J.C., Fann, G.I., Harrison, R.J., Nazarewicz, W., Hill, J., Galindo, D., Jia, J. The self-consistent Hartree-Fock-Bogoliubov problem in large boxes can be solved accurately in the coordinate space with the recently developed solvers HFB-AX (2D) and MADNESS-HFB (3D). This is essential for the description of superfluid Fermi systems with complicated topologies and significant spatial extend, such as fissioning nuclei, weakly-bound nuclei, nuclear matter in the neutron star rust, and ultracold Fermi atoms in elongated traps. The HFB-AX solver based on B-spline techniques uses a hybrid MPI and OpenMP programming model for parallel computation for

217

Revisiting the symmetric reactions for synthesis of super heavy nuclei of $Z\\geq $120  

E-Print Network (OSTI)

Extensive efforts have been made experimentally to reach nuclei in the super heavy mass region of Z = 110 and above with suitable choices of projectile and target nuclei. The cross sections for production of these nuclei are seen to be in the range of a few picobarn or less, and pose great experimental challenges. Theoretically, there have been extensive calculations for highly asymmetric (hot-fusion) and moderately asymmetric (cold-fusion) collisions and only a few theoretical studies are available for near symmetric collisions to estimate the cross sections for production of super-heavy nuclei. In the present article, we revisit the symmetric heavy ion reactions with suitable combinations of projectile and target nuclei in the rare-earth region, that will lead to compound systems with very low excitation energy and with better neutron-to-proton ratio for higher stability.

R. K. Choudhury; Y. K. Gupta

2012-11-19T23:59:59.000Z

218

Status and future of the CDMS experiment: CDMS-II to SuperCDMS  

SciTech Connect

The Cryogenic Dark Matter Search experiment (CDMS-II) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering interactions with the target nuclei. No Dark Matter signal has been observed so far, resulting in a limit on the spin-independent WIMP-nucleon elastic scattering cross-section with a minimum of 1.6x10{sup -43} cm{sup 2} at a WIMP mass of 60 GeV c{sup -2}. To increase the sensitivity, new one inch thick detectors have been developed which will be used in the SuperCDMS phase. SuperCDMS will be operated at SNOLAB with an expected sensitivity on the spin-independent WIMP-nucleon elastic scattering cross-section of 1x10{sup -45} cm{sup 2} at the 25 kg stage.

Bruch, T. [Physik Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich (Switzerland)

2007-11-20T23:59:59.000Z

219

Super-allowed beta-decay rates in 1d5/2 shell in Coriolis coupling model  

E-Print Network (OSTI)

The expression for super-allowed beta-decay transition rates have been derived within the context of Coriolis coupling model. The derived expressions, valid for the beta-decay between any two mirror nuclei, has been applied to calculate super-allowed beta-decay transition rates of 21Na, 21Mg, 21Al, and 21Si. The calculated rates agree well with the data and the calculations done using the shell model with configuration admixture.

M. Sultan Parvez; F. Bary Malik

2009-04-03T23:59:59.000Z

220

High-Efficiency Retrofit Lessons for Retail from a SuperTarget: Preprint  

SciTech Connect

The National Renewable Energy Laboratory partnered with Target under the Commercial Building Program to design and implement a retrofit of a SuperTarget in Thornton, CO. The result was a retrofit design that predicted 37% energy savings over ASHRAE Standard 90.1-2004, and 29% compared to existing (pre-retrofit) store consumption. The largest savings came from energy efficient lighting, energy efficient cooling systems, improved refrigeration, and better control of plug loads.

Langner, R.; Deru, M.; Hirsch, A.; Williams, S.

2013-02-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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221

Proposal for Optical Super-Focusing with a Metal-Dielectric Waveguide Array  

E-Print Network (OSTI)

In this paper, super-focusing using radiationless electromagnetic interference is extended to the visible regime. It is shown that the highest-order mode of a specifically designed metal-dielectric waveguide array can provide the rapidly oscillating source field for radiationless interference. Using finite-difference time-domain simulations, an example structure is demonstrated. This structure provides focusing to 0.21 of the optical wavelength at a distance of half the optical wavelength from the source.

Gordon, Reuven

2008-01-01T23:59:59.000Z

222

SOWFA Super-Controller: A High-Fidelity Tool for Evaluating Wind Plant Control Approaches  

DOE Green Energy (OSTI)

This paper presents a new tool for testing wind plant controllers in the Simulator for Offshore Wind Farm Applications (SOWFA). SOWFA is a high-fidelity simulator for the interaction between wind turbine dynamics and the fluid flow in a wind plant. The new super-controller testing environment in SOWFA allows for the implementation of the majority of the wind plant control strategies proposed in the literature.

Fleming, P.; Gebraad, P.; van Wingerden, J. W.; Lee, S.; Churchfield, M.; Scholbrock, A.; Michalakes, J.; Johnson, K.; Moriarty, P.

2013-01-01T23:59:59.000Z

223

Super-soft symmetry energy encountering non-Newtonian gravity in neutron stars  

E-Print Network (OSTI)

Considering the non-Newtonian gravity proposed in the grand unification theories, we show that the stability and observed global properties of neutron stars can not rule out the super-soft nuclear symmetry energies at supra-saturation densities. The degree of possible violation of the Inverse-Square-Law of gravity in neutron stars is estimated using an Equation of State (EOS) of neutron-rich nuclear matter consistent with the available terrestrial laboratory data.

De-Hua Wen; Bao-An Li; Lie-Wen Chen

2009-08-13T23:59:59.000Z

224

High intensity uranium beams from the superHILAC and the bevatron: final report  

Science Conference Proceedings (OSTI)

The two injectors formerly used at the SuperHILAC were a 750-kV air-insulated Cockcroft-Walton (EVE) and a 2.5-MV pressurized HV multiplier (ADAM). The EVE injector can deliver adequate intensities of ions up to mass 40 (argon). The ADAM injector can accelerate ions with lower charge-to-mass ratios, and they can produce beams of heavier ions. The intensity of these beams decreases as the mass number increases, with the lowest practical intensity being achieved with lead beams. Experience with the two existing injectors provided substantial help in defining the general requirements for a new injector which would provide ample beams above mass 40. The requirements for acceptance by the first tank of the SuperHILAC are a particle velocity ..beta.. = 0.0154 (corresponding to an energy of 113 keV/amu) and a charge-to-mass ratio of 0.046 or larger. Present ion source performance dictates an air-insulated Cockcroft-Walton as a pre-accelerator because of its easy accessibility and its good overall reliability. The low charge state ions then receive further acceleration and, if necessary, subsequent stripping to the required charge state before injection into the SuperHILAC. A low-beta linac of the Widereoe type has been built to perform this acceleration. The injector system described consists of a Cockcroft-Walton pre-injector, injection beam lines and isotope analysis, a low-velocity linear accelerator, and SuperHILAC control center modifications.

Not Available

1982-03-01T23:59:59.000Z

225

Noncommutative N=1 super Yang-Mills, the Seiberg-Witten map and UV divergences  

E-Print Network (OSTI)

Classically, the dual under the Seiberg-Witten map of noncommutative U(N), {\\cal N}=1 super Yang-Mills theory is a field theory with ordinary gauge symmetry whose fields carry, however, a \\theta-deformed nonlinear realisation of the {\\cal N}=1 supersymmetry algebra in four dimensions. For the latter theory we work out at one-loop and first order in the noncommutative parameter matrix \\theta^{\\mu\

C. P. Martin; C. Tamarit

2009-07-14T23:59:59.000Z

226

Highly Selective Membranes For The Separation Of Organic Vapors Using Super-Glassy Polymers  

DOE Patents (OSTI)

A process for separating hydrocarbon gases of low boiling point, particularly methane, ethane and ethylene, from nitrogen. The process is performed using a membrane made from a super-glassy material. The gases to be separated are mixed with a condensable gas, such as a C.sub.3+ hydrocarbon. In the presence of the condensable gas, improved selectivity for the low-boiling-point hydrocarbon gas over nitrogen is achieved.

Pinnau, Ingo (Palo Alto, CA); Lokhandwala, Kaaeid (Menlo Park, CA); Nguyen, Phuong (Fremont, CA); Segelke, Scott (Mountain View, CA)

1997-11-18T23:59:59.000Z

227

Spontaneous fission modes and lifetimes of super-heavy elements in the nuclear density functional theory  

E-Print Network (OSTI)

Lifetimes of super-heavy (SH) nuclei are primarily governed by alpha decay and spontaneous fission (SF). Here we study the competing decay modes of even-even SH isotopes with 108 cold fusion" and "hot fusion" reactions. The region of long-lived SH nuclei is expected to be centered on $^{294}$Ds with a total half-life of ?1.5 days.

A. Staszczak; A. Baran; W. Nazarewicz

2012-08-06T23:59:59.000Z

228

THEORETICAL TRANSIT SPECTRA FOR GJ 1214b AND OTHER 'SUPER-EARTHS'  

SciTech Connect

We present new calculations of transit spectra of super-Earths that allow for atmospheres with arbitrary proportions of common molecular species and haze. We test this method with generic spectra, reproducing the expected systematics and absorption features, then apply it to the nearby super-Earth GJ 1214b, which has produced conflicting observational data, leaving the questions of a hydrogen-rich versus hydrogen-poor atmosphere and the water content of the atmosphere ambiguous. We present representative transit spectra for a range of classes of atmosphere models for GJ 1214b. Our analysis supports a hydrogen-rich atmosphere with a cloud or haze layer, although a hydrogen-poor model with {approx}<10% water is not ruled out. Several classes of models are ruled out, however, including hydrogen-rich atmospheres with no haze, hydrogen-rich atmospheres with a haze of {approx}0.01 {mu}m tholin particles, and hydrogen-poor atmospheres with major sources of absorption other than water. We propose an observational test to distinguish hydrogen-rich from hydrogen-poor atmospheres. Finally, we provide a library of theoretical transit spectra for super-Earths with a broad range of parameters to facilitate future comparison with anticipated data.

Howe, Alex R.; Burrows, Adam S., E-mail: arhowe@astro.princeton.edu, E-mail: burrows@astro.princeton.edu [Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States)

2012-09-10T23:59:59.000Z

229

The Atmospheric Signatures of Super-Earths: How to Distinguish Between Hydrogen-Rich and Hydrogen-Poor Atmospheres  

E-Print Network (OSTI)

Extrasolar super-Earths (1-10 M$_{\\earth}$) are likely to exist with a wide range of atmospheres. Some super-Earths may be able to retain massive hydrogen-rich atmospheres. Others might never accumulate hydrogen or experience significant escape of lightweight elements, resulting in atmospheres more like those of the terrestrial planets in our Solar System. We examine how an observer could differentiate between hydrogen-rich and hydrogen-poor atmospheres by modeling super-Earth emission and transmission spectra, and we find that discrimination is possible by observing the transmission spectrum alone. An Earth-like atmosphere, composed of mostly heavy elements and molecules, will have a very weak transmission signal due to its small atmospheric scale height (since the scale height is inversely proportional to molecular weight). On the other hand, a large hydrogen-rich atmosphere reveals a relatively large transmission signal. The super Earth emission spectrum can additionally contrain the atmospheric composition and temperature structure. Super-Earths with massive hydrogen atmospheres will reveal strong spectral features due to water, whereas those that have lost most of their hydrogen (and have no liquid ocean) will be marked by CO$_2$ features and a lack of H$_2$O. We apply our study specifically to the low-mass planet orbiting an M star, Gl 581c ($M sin i$ = 5 M$_{\\earth}$), although our conclusions are relevant for super-Earths in general. The ability to distinguish hydrogen-rich atmospheres might be essential for interpreting mass and radius observations of planets in the transition between rocky super-Earths and Neptune-like planets.

E. Miller-Ricci; D. Sasselov; S. Seager

2008-08-13T23:59:59.000Z

230

First Principles Study of the Li[subscript 10]GeP[subscript 2]S[subscript 12] Lithium Super Ionic Conductor Material  

E-Print Network (OSTI)

The continued drive for high performance lithium batteries has imposed stricter requirements on the electrolyte materials. Solid electrolytes comprising lithium super ionic conductor materials exhibit good safety and ...

Mo, Yifei

231

Efficient identification of exoplanetary transit candidates from SuperWASP light curves  

E-Print Network (OSTI)

Transiting extrasolar planets constitute only a small fraction of the range of stellar systems found to display periodic, shallow dimmings in wide-field surveys employing small-aperture camera arrays. Here we present an efficient selection strategy for follow-up observations, derived from analysis of the light curves of a sample of 67 SuperWASP targets that passed the selection tests we used in earlier papers, but which have subsequently been identified either as planet hosts or as astrophysical false positives. We determine the system parameters using Markov-chain Monte Carlo analysis of the SuperWASP light curves. We use a constrained optimisation of chi-squared combined with a Bayesian prior based on the main-sequence mass and radius expected from the 2MASS J-H colour. The Bayesian nature of the analysis allows us to quantify both the departure of the host star from the main-sequence mass-radius relation and the probability that the companion radius is less than 1.5 Jupiter radii. When augmented by direct light curve analyses that detect binaries with unequal primary and secondary eclipses, and objects with aperture blends that are resolved by SuperWASP, we find that only 13 of the original 67 stars, including the three known planets in the sample, would qualify for follow-up. This suggests that planet discovery "hit rates" better than one-in-five should be achievable. In addition, the stellar binaries that qualify are likely to have astrophysically interesting stellar or sub-stellar secondaries.

A. Collier Cameron; D. M. Wilson; R. G. West; L. Hebb; X. -B. Wang; S. Aigrain; F. Bouchy; D. J. Christian; W. I. Clarkson; B. Enoch; M. Esposito; E. Guenther; C. A. Haswell; G. Hebrard; C. Hellier; K. Horne; J. Irwin; S. R. Kane; B. Loeillet; T. A. Lister; P. Maxted; M. Mayor; C. Moutou; N. Parley; D. Pollacco; F. Pont; D. Queloz; R. Ryans; I. Skillen; R. A. Street; S. Udry; P. J. Wheatley

2007-07-03T23:59:59.000Z

232

THE INFLUENCE OF PRESSURE-DEPENDENT VISCOSITY ON THE THERMAL EVOLUTION OF SUPER-EARTHS  

Science Conference Proceedings (OSTI)

We study the thermal evolution of super-Earths with a one-dimensional (1D) parameterized convection model that has been adopted to account for a strong pressure dependence of the viscosity. A comparison with a 2D spherical convection model shows that the derived parameterization satisfactorily represents the main characteristics of the thermal evolution of massive rocky planets. We find that the pressure dependence of the viscosity strongly influences the thermal evolution of super-Earths-resulting in a highly sluggish convection regime in the lower mantles of those planets. Depending on the effective activation volume and for cooler initial conditions, we observe with growing planetary mass even the formation of a conductive lid above the core-mantle boundary (CMB), a so-called CMB-lid. For initially molten planets our results suggest no CMB-lids but instead a hot lower mantle and core as well as sluggish lower mantle convection. This implies that the initial interior temperatures, especially in the lower mantle, become crucial for the thermal evolution-the thermostat effect suggested to regulate the interior temperatures in terrestrial planets does not work for massive planets if the viscosity is strongly pressure dependent. The sluggish convection and the potential formation of the CMB-lid reduce the convective vigor throughout the mantle, thereby affecting convective stresses, lithospheric thicknesses, and heat fluxes. The pressure dependence of the viscosity may therefore also strongly affect the propensity of plate tectonics, volcanic activity, and the generation of a magnetic field of super-Earths.

Stamenkovic, Vlada; Noack, Lena; Spohn, Tilman [Institute of Planetology, Westfaelische Wilhelms-Universitaet Muenster, Wilhelm-Klemm-Str. 10, 48149 Muenster (Germany); Breuer, Doris, E-mail: Vlada.Stamenkovic@dlr.de, E-mail: Lena.Noack@dlr.de, E-mail: Doris.Breuer@dlr.de, E-mail: Tilman.Spohn@dlr.de [Institute of Planetary Research, German Aerospace Center DLR, Rutherfordstrasse 2, 12489 Berlin (Germany)

2012-03-20T23:59:59.000Z

233

Ignition of a deuterium micro-detonation with a gigavolt super marx generator  

E-Print Network (OSTI)

The Centurion-Halite experiment demonstrated the feasibility of igniting a deuterium-tritium micro-explosion with an energy of not more than a few megajoule, and the Mike test, the feasibility of a pure deuterium explosion with an energy of more than 10^6 megajoule. In both cases the ignition energy was supplied by a fission bomb explosive. While an energy of a few megajoule, to be released in the time required of less than 10^-9 sec, can be supplied by lasers and intense particle beams, this is not enough to ignite a pure deuterium explosion. Because the deuterium-tritium reaction depends on the availability of lithium, the non-fusion ignition of a pure deuterium fusion reaction would be highly desirable. It is shown that this goal can conceivably be reached with a "Super Marx Generator", where a large number of "ordinary" Marx generators charge (magnetically insulated) fast high voltage capacitors of a second stage Marx generator, called a "Super Marx Generator", ultimately reaching gigavolt potentials with an energy output of 100 megajoule. An intense 10^7 Ampere-GeV proton beam drawn from a "Super Marx Generator" can ignite a deuterium thermonuclear detonation wave in a compressed deuterium cylinder, where the strong magnetic field of the proton beam entraps the charged fusion reaction products inside the cylinder. In solving the stand-off problem, the stiffness of a GeV proton beam permits to place the deuterium target at a comparatively large distance from the wall of a cavity confining the deuterium micro-explosion.

Friedwardt Winterberg

2008-12-01T23:59:59.000Z

234

Structural performance of the first SSC (Superconducting Super Collider) Design B dipole magnet  

Science Conference Proceedings (OSTI)

The first Design B Superconducting Super Collider (SSC) dipole magnet has been successfully tested. This magnet was heavily instrumented with temperature and strain gage sensors in order to evaluate its adherence to design constraints and design calculations. The instrumentation and associated data acquisition system allowed monitoring of the magnet during cooldown, warmup, and quench testing. This paper will focus on the results obtained from structural measurements on the suspension system during normal and rapid cooldowns and during quench studies at full magnet current. 4 refs., 9 figs.

Nicol, T.H.

1989-09-01T23:59:59.000Z

235

Performance evaluation and enhancement of SuperLU{_}DIST 2.0  

Science Conference Proceedings (OSTI)

We present the runtime comparison of the two versions of Super LU{_}DIST, using up to 128 processors of the IBM SP at NERSC. One version provides the global input interface, and another provides the distributed input interface. The comparison includes the total runtime of the solver with both 32-bit and 64-bit addressing modes, the time breakdown for different phases of the solver. We also present an in-depth comparison off our sparse matrix-vector multiplication methods in the context of iterative refinement. Finally, we describe our Fortran 90 interface that enhances the usability of the software.

Li, Xiaoye S.; Wang, Yu

2003-08-28T23:59:59.000Z

236

The Super Efficient Refrigerator Program: Case study of a Golden Carrot program  

Science Conference Proceedings (OSTI)

The work in this report was conducted by the Analytic Studies Division (ASD) of the National Renewable Energy Laboratory (NREL) for the U.S. Department of Energy Office of Energy Efficiency and Renewable Energy, Office of Building Technologies. This case study describes the development and implementation of the Super Efficient Refrigerator Program (SERP), which awarded $30 million to the refrigerator manufacturer that developed and commercialized a refrigerator that exceeded 1993 federal efficiency standards by at least 25%. The program was funded by 24 public and private utilities. As the first Golden Carrot program to be implemented in the United States, SERP was studied as an example for future `market-pull` efforts.

Eckert, J B

1995-07-01T23:59:59.000Z

237

GRB 070724B: the first Gamma Ray Burst localized by SuperAGILE and its Swift X-ray Afterglow  

E-Print Network (OSTI)

GRB 070724B is the first Gamma Ray Burst localized by SuperAGILE, the hard X-ray monitor aboard the AGILE satellite. The coordinates of the event were published $\\sim 19$ hours after the trigger. The Swift X-Ray Telescope pointed at the SuperAGILE location and detected the X-ray afterglow inside the SuperAGILE error circle. The AGILE gamma-ray Tracker and Minicalorimeter did not detect any significant gamma ray emission associated with GRB 070724B in the MeV and GeV range, neither prompt nor delayed. Searches of the optical afterglow were performed by the Swift UVOT and the Palomar automated 60-inch telescopes without any significant detection. Similarly the Very Large Array did not detect a radio afterglow. This is the first GRB event with a firm upper limit in the 100 MeV -- 30 GeV energy range, associated with an X-ray afterglow.

E. Del Monte; M. Feroci; L. Pacciani; Y. Evangelista; I. Donnarumma; P. Soffitta; E. Costa; I. Lapshov; F. Lazzarotto; M. Rapisarda; A. Argan; G. Barbiellini; M. Basset; A. Bulgarelli; P. Caraveo; A. Chen; G. Di Cocco; L. Foggetta; F. Fuschino; M. Galli; F. Gianotti; A. Giuliani; C. Labanti; P. Lipari; F. Longo; M. Marisaldi; F. Mauri; S. Mereghetti; A. Morselli; A. Pellizzoni; F. Perotti; P. Picozza; M. Prest; G. Pucella; M. Tavani; M. Trifoglio; A. Trois; E. Vallazza; S. Vercellone; V. Vittorini; A. Zambra; P. Romano; D. N. Burrows; G. Chincarini; N. Gehrels; V. La Parola; P. T. O'Brien; J. P. Osborne; B. Preger; C. Pittori; L. A. Antonelli; F. Verrecchia; P. Giommi; L. Salotti

2007-12-04T23:59:59.000Z

238

SuperIdentity: Fusion of Identity across Real and Cyber Domains  

Science Conference Proceedings (OSTI)

Under both benign and malign circumstances, people now manage a spectrum of identities across both real-world and cyber domains. Our belief, however, is that all these instances ultimately track back for an individual to reflect a single 'SuperIdentity'. This paper outlines the assumptions underpinning the SuperIdentity Project, describing the innovative use of data fusion to incorporate novel real-world and cyber cues into a rich framework appropriate for modern identity. The proposed combinatorial model will support a robust identification or authentication decision, with confidence indexed both by the level of trust in data provenance, and the diagnosticity of the identity factors being used. Additionally, the exploration of correlations between factors may underpin the more intelligent use of identity information so that known information may be used to predict previously hidden information. With modern living supporting the 'distribution of identity' across real and cyber domains, and with criminal elements operating in increasingly sophisticated ways in the hinterland between the two, this approach is suggested as a way forwards, and is discussed in terms of its impact on privacy, security, and the detection of threat.

Black, Sue; Creese, Sadie; Guest, Richard; Pike, William A.; Saxby, Steven; Stanton Fraser, Danae; Stevenage, Sarah; Whitty, Monica

2012-04-23T23:59:59.000Z

239

Effective slip in pressure-driven flow past super-hydrophobic stripes  

E-Print Network (OSTI)

Super-hydrophobic array of grooves containing trapped gas (stripes), have the potential to greatly reduce drag and enhance mixing phenomena in microfluidic devices. Recent work has focused on idealized cases of stick-perfect slip stripes, with limited guidance. Here, we analyze the experimentally relevant situation of a pressure-driven flow past striped slip-stick surfaces with arbitrary local slip at the gas sectors. We derive analytical formulas for maximal (longitudinal) and minimal (transverse) directional effective slip lengths that can be used for any surface slip fraction (validated by numerical calculations). By representing eigenvalues of the slip length-tensor, they allow us to obtain the effective slip for any orientation of stripes with respect to the mean flow. Our results imply that flow past stripes is controlled by the ratio of the local slip length to texture size. In case of a large (compared to the texture period) slip at the gas areas, surface anisotropy leads to a tensorial effective slip, by attaining the values predicted earlier for a perfect local slip. Both effective slip lengths and anisotropy of the flow decrease when local slip becomes of the order of texture period. In the case of small slip, we predict simple surface-averaged, isotropic flows (independent of orientation). These results provide a framework for the rational design of super-hydrophobic surfaces and devices.

Aleksey V. Belyaev; Olga I. Vinogradova

2009-12-08T23:59:59.000Z

240

Efficient identification of exoplanetary transit candidates from SuperWASP light curves  

E-Print Network (OSTI)

Transiting extrasolar planets constitute only a small fraction of the range of stellar systems found to display periodic, shallow dimmings in wide-field surveys employing small-aperture camera arrays. Here we present an efficient selection strategy for follow-up observations, derived from analysis of the light curves of a sample of 67 SuperWASP targets that passed the selection tests we used in earlier papers, but which have subsequently been identified either as planet hosts or as astrophysical false positives. We determine the system parameters using Markov-chain Monte Carlo analysis of the SuperWASP light curves. We use a constrained optimisation of chi-squared combined with a Bayesian prior based on the main-sequence mass and radius expected from the 2MASS J-H colour. The Bayesian nature of the analysis allows us to quantify both the departure of the host star from the main-sequence mass-radius relation and the probability that the companion radius is less than 1.5 Jupiter radii. When augmented by direct ...

Cameron, A Collier; West, R G; Hebb, L; Wang, X -B; Aigrain, S; Bouchy, F; Christian, D J; Clarkson, W I; Enoch, B; Esposito, M; Gnther, E; Haswell, C A; Hbrard, G; Hellier, C; Horne, K; Irwin, J; Kane, S R; Loeillet, B; Lister, T A; Maxted, P; Mayor, M; Moutou, C; Parley, N; Pollacco, D; Pont, F; Queloz, D; Ryans, R; Skillen, I; Street, R A; Udry, S; Wheatley, P J

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

More accurate and efficient bath spectral densities from super-resolution  

E-Print Network (OSTI)

Quantum transport and other phenomena are typically modeled by coupling the system of interest to an environment, or bath, held at thermal equilibrium. Realistic bath models are at least as challenging to construct as models for the quantum systems themselves, since they must incorporate many degrees of freedom that interact with the system on a wide range of timescales. Owing to computational limitations, the environment is often modeled with simple functional forms, with a few parameters fit to experiment to yield semi-quantitative results. Growing computational resources have enabled the construction of more realistic bath models from molecular dynamics (MD) simulations. In this paper, we develop a numerical technique to construct these atomistic bath models with better accuracy and decreased cost. We apply a novel signal processing technique, known as super-resolution, combined with a dictionary of physically-motivated bath modes to derive spectral densities from MD simulations. Our approach reduces the required simulation time and provides a more accurate spectral density than can be obtained via standard Fourier transform methods. Moreover, the spectral density is provided as a convenient closed-form expression which yields an analytic time-dependent bath kernel. Exciton dynamics of the Fenna-Matthews-Olsen light-harvesting complex are simulated with a second order time-convolutionless master equation, and spectral densities constructed via super-resolution are shown to reproduce the dynamics using only a quarter of the amount of MD data.

Thomas Markovich; Samuel M. Blau; John Parkhill; Christoph Kreisbeck; Jacob N. Sanders; Xavier Andrade; Aln Aspuru-Guzik

2013-07-16T23:59:59.000Z

242

Reactor Anti-Neutrino Oscillations and Gadolinium Loaded Super-Kamiokande Detector  

E-Print Network (OSTI)

We explore the potential of measuring the solar neutrino oscillation parameters in the proposed gadolinium loaded Super-Kamiokande (SK-Gd) detector. Gadolinium dissolved in water can detect neutrons much more efficiently than pure water. This imparts the detector the ability to observe electron type antineutrinos, transforming Super-Kamiokande into a huge reactor antineutrino detector with an event rate approximately 43 times higher than that observed in KamLAND. We simulate the reactor antineutrino data expected in this high statistics detector. We use these prospective data to study the precision with which the solar neutrino oscillation parameters, $\\Delta m^2_{\\odot}$ and $\\sin^2\\theta_{\\odot}$, can be determined i) with the SK-Gd detector, and ii) by combining the SK-Gd data with the global data on solar neutrino oscillations. For comparison and completeness the allowed regions of $\\Delta m^2_{\\odot}$ and $\\sin^2\\theta_{\\odot}$, expected to be obtained from the data of the solar neutrino and KamLAND experiments, are also presented.

Sandhya Choubey; S. T. Petcov

2004-04-12T23:59:59.000Z

243

POTENTIAL FOR HIGGS PHYSICS AT THE LHC AND SUPER-LHC.  

SciTech Connect

The expected sensitivity of the LHC experiments to the discovery of the Higgs boson and the measurement of its properties is presented in the context of both the standard model and the its minimal supersymmetric extension. Prospects for a luminosity-upgraded ''Super-LHC'' are also presented. If it exists, the LHC should discover standard model Higgs boson, measure its mass accurately, and make various measurements of its couplings, spin and CP properties. In the context of the CP-conserving MSSM, the LHC should be able to discover one or more Higgs bosons over the entire m{sub A}-tan {beta} plane, with two or more observable in many cases. The large number of channels available insure a robust discovery and offer many opportunities for additional measurements. Observation of H {yields} {mu}{mu}, measurement of the tri-linear Higgs self-coupling, and various search channels are statistics-limited, and only possible with a luminosity upgrade. A luminosity upgrade would substantially improve some of the coupling measurements and generally extend the sensitivity in the MSSM Higgs plane. Efforts are ongoing to understand the upgrade of the LHC to the Super-LHC.

CRANMER, K.S.

2005-12-12T23:59:59.000Z

244

Welding and weldability of directionally solidified single crystal nickel-base super-alloys  

DOE Green Energy (OSTI)

The objective of this CRADA project was to investigate the weldability of polycrystalline, directionally-solidified, and single-crystal, nickel-base super-alloys. These materials are used extensively in turbine engine components. The ability to weld these materials is highly desirable in that it would greatly facilitate component fabrication. Welding of these materials would also have the potential benefit of allowing for the repair of cracked or worn components. Specifically, the program had four objectives: (1) to evaluate the weldability of nickel-base super-alloys; (2) to characterize the solidification microstructure of the welds; (3) to evaluate the phase stability of the weldments during exposure to service conditions; and (4) to determine the mechanical properties of the welds. Westinghouse Electric Corporation was to supply material for the program, in both as-case and heat-treated form. This was to include commercially available as well as experimental alloys developed at Westinghouse. ORNL was to perform weldability tests on the materials using a variety of welding procedures.

vitek, j.m.

1996-09-01T23:59:59.000Z

245

The CMS Level-1 Trigger at LHC and Super-LHC  

E-Print Network (OSTI)

The Level-1 trigger of the CMS experiment at CERN has been designed to select proton-proton interactions whose final state includes signatures of new physics in the form of high transverse energy electrons, photons, jets, or high missing transverse energy. The Level-1 trigger system process data in a pipeline fashion at a rate of 40 MHz, has a design latency of 128 bunch crossings and an output rate of 100 KHz. The design of this system is presented with emphasis on the calorimeter triggers. After a long period of testing and validation of its performance the Level-1 trigger system has been installed and commissioned at the CMS experiment at CERN. Cosmic ray data and Monte Carlo events have been used to compare the actual performance of the trigger with expectations from off-line emulation models. Results from these studies are presented here. The limitations of this system to cope with future luminosity upgrades of the LHC, the Super-LHC, are discussed. The current CMS plan for a new CMS Level-1 trigger system at the Super-LHC is presented. The center point of the new system is a Level-1 tracking trigger which uses data from a new CMS silicon tracking detector.

C. Foudas

2008-10-22T23:59:59.000Z

246

Slowly fading super-luminous supernovae that are not pair-instability explosions  

E-Print Network (OSTI)

Super-luminous supernovae that radiate more than 10^44 ergs per second at their peak luminosity have recently been discovered in faint galaxies at redshifts of 0.1-4. Some evolve slowly, resembling models of 'pair-instability' supernovae. Such models involve stars with original masses 140-260 times that of the Sun that now have carbon-oxygen cores of 65-30 solar masses. In these stars, the photons that prevent gravitational collapse are converted to electron-positron pairs, causing rapid contraction and thermonuclear explosions. Many solar masses of 56Ni are synthesized; this isotope decays to 56Fe via 56Co, powering bright light curves. Such massive progenitors are expected to have formed from metal-poor gas in the early Universe. Recently, supernova 2007bi in a galaxy at redshift 0.127 (about 12 billion years after the Big Bang) with a metallicity one-third that of the Sun was observed to look like a fading pair-instability supernova. Here we report observations of two slow-to-fade super-luminous supernovae...

Nicholl, M; Jerkstrand, A; Inserra, C; McCrum, M; Kotak, R; Fraser, M; Wright, D; Chen, T -W; Smith, K; Young, D R; Sim, S A; Valenti, S; Howell, D A; Bresolin, F; Kudritzki, R P; Tonry, J L; Huber, M E; Rest, A; Pastorello, A; Tomasella, L; Cappellaro, E; Benetti, S; Mattila, S; Kankare, E; Kangas, T; Leloudas, G; Sollerman, J; Taddia, F; Berger, E; Chornock, R; Narayan, G; Stubbs, C W; Foley, R J; Lunnan, R; Soderberg, A; Sanders, N; Milisavljevic, D; Margutti, R; Kirshner, R P; Elias-Rosa, N; Morales-Garoffolo, A; Taubenberger, S; Botticella, M T; Gezari, S; Urata, Y; Rodney, S; Riess, A G; Scolnic, D; Wood-Vasey, W M; Burgett, W S; Chambers, K; Flewelling, H A; Magnier, E A; Kaiser, N; Metcalfe, N; Morgan, J; Price, P A; Sweeney, W; Waters, C

2013-01-01T23:59:59.000Z

247

DOENEWS: Address of John S. Herrington, Secretary of Energy, at the National symposium on the superconducting super collider in Denver, Colorado, December 3, 1987  

Science Conference Proceedings (OSTI)

In this address, the President's support for basic science is briefly discussed, and support for the Superconducting Super Collider in particular is emphasized. Perceived benefits of the Super Collider are discussed, including benefits to the world, training for scientists, maintaining American competitiveness. Federal support of science, including Congressional action, is discussed briefly. (LEW)

Herrington, J.S.

1987-12-01T23:59:59.000Z

248

Super Boiler: Packed Media/Transport Membrane Boiler Development and Demonstration  

Science Conference Proceedings (OSTI)

Gas Technology Institute (GTI) and Cleaver-Brooks developed a new gas-fired steam generation system???¢????????the Super Boiler???¢????????for increased energy efficiency, reduced equipment size, and reduced emissions. The system consists of a firetube boiler with a unique staged furnace design, a two-stage burner system with engineered internal recirculation and inter-stage cooling integral to the boiler, unique convective pass design with extended internal surfaces for enhanced heat transfer, and a novel integrated heat recovery system to extract maximum energy from the flue gas. With these combined innovations, the Super Boiler technical goals were set at 94% HHV fuel efficiency, operation on natural gas with boilers of similar steam output. To demonstrate these technical goals, the project culminated in the industrial demonstration of this new high-efficiency technology on a 300 HP boiler at Clement Pappas, a juice bottler located in Ontario, California. The Super Boiler combustion system is based on two stage combustion which combines air staging, internal flue gas recirculation, inter-stage cooling, and unique fuel-air mixing technology to achieve low emissions rather than external flue gas recirculation which is most commonly used today. The two-stage combustion provides lower emissions because of the integrated design of the boiler and combustion system which permit precise control of peak flame temperatures in both primary and secondary stages of combustion. To reduce equipment size, the Super Boiler's dual furnace design increases radiant heat transfer to the furnace walls, allowing shorter overall furnace length, and also employs convective tubes with extended surfaces that increase heat transfer by up to 18-fold compared to conventional bare tubes. In this way, a two-pass boiler can achieve the same efficiency as a traditional three or four-pass firetube boiler design. The Super Boiler is consequently up to 50% smaller in footprint, has a smaller diameter, and is up to 50% lower in weight, resulting in very compact design with reduced material cost and labor costs, while requiring less boiler room floor space. For enhanced energy efficiency, the heat recovery system uses a transport membrane condenser (TMC), a humidifying air heater (HAH), and a split-stage economizer to extract maximum energy from the flue gas. The TMC is a new innovation that pulls a major portion of water vapor produced by the combustion process from the flue gases along with its sensible and latent heat. This results in nearly 100% transfer of heat to the boiler feed water. The HAH improves the effectiveness of the TMC, particularly in steam systems that do not have a large amount of cold makeup water. In addition, the HAH humidifies the combustion air to reduce NOx formation. The split-stage economizer preheats boiler feed water in the same way as a conventional economizer, but extracts more heat by working in tandem with the TMC and HAH to reduce flue gas temperature. These components are designed to work synergistically to achieve energy efficiencies of 92-94% which is 10-15% higher than today???¢????????s typical firetube boilers.

Liss, William E; Cygan, David F

2013-04-17T23:59:59.000Z

249

Super Boiler: Packed Media/Transport Membrane Boiler Development and Demonstration  

SciTech Connect

Gas Technology Institute (GTI) and Cleaver-Brooks developed a new gas-fired steam generation system???¢????????the Super Boiler???¢????????for increased energy efficiency, reduced equipment size, and reduced emissions. The system consists of a firetube boiler with a unique staged furnace design, a two-stage burner system with engineered internal recirculation and inter-stage cooling integral to the boiler, unique convective pass design with extended internal surfaces for enhanced heat transfer, and a novel integrated heat recovery system to extract maximum energy from the flue gas. With these combined innovations, the Super Boiler technical goals were set at 94% HHV fuel efficiency, operation on natural gas with <5 ppmv NOx (referenced to 3%O2), and 50% smaller than conventional boilers of similar steam output. To demonstrate these technical goals, the project culminated in the industrial demonstration of this new high-efficiency technology on a 300 HP boiler at Clement Pappas, a juice bottler located in Ontario, California. The Super Boiler combustion system is based on two stage combustion which combines air staging, internal flue gas recirculation, inter-stage cooling, and unique fuel-air mixing technology to achieve low emissions rather than external flue gas recirculation which is most commonly used today. The two-stage combustion provides lower emissions because of the integrated design of the boiler and combustion system which permit precise control of peak flame temperatures in both primary and secondary stages of combustion. To reduce equipment size, the Super Boiler's dual furnace design increases radiant heat transfer to the furnace walls, allowing shorter overall furnace length, and also employs convective tubes with extended surfaces that increase heat transfer by up to 18-fold compared to conventional bare tubes. In this way, a two-pass boiler can achieve the same efficiency as a traditional three or four-pass firetube boiler design. The Super Boiler is consequently up to 50% smaller in footprint, has a smaller diameter, and is up to 50% lower in weight, resulting in very compact design with reduced material cost and labor costs, while requiring less boiler room floor space. For enhanced energy efficiency, the heat recovery system uses a transport membrane condenser (TMC), a humidifying air heater (HAH), and a split-stage economizer to extract maximum energy from the flue gas. The TMC is a new innovation that pulls a major portion of water vapor produced by the combustion process from the flue gases along with its sensible and latent heat. This results in nearly 100% transfer of heat to the boiler feed water. The HAH improves the effectiveness of the TMC, particularly in steam systems that do not have a large amount of cold makeup water. In addition, the HAH humidifies the combustion air to reduce NOx formation. The split-stage economizer preheats boiler feed water in the same way as a conventional economizer, but extracts more heat by working in tandem with the TMC and HAH to reduce flue gas temperature. These components are designed to work synergistically to achieve energy efficiencies of 92-94% which is 10-15% higher than today???¢????????s typical firetube boilers.

Liss, William E; Cygan, David F

2013-04-17T23:59:59.000Z

250

Super-strong interacting gravitons as a main engine of the universe without expansion or dark energy  

E-Print Network (OSTI)

The basic cosmological conjecture about the Dopplerian nature of redshifts may be false if gravitons are super-strong interacting particles. A quantum mechanism of classical gravity and the main features of a new cosmological paradigm based on it are described here.

Ivanov, M A

2004-01-01T23:59:59.000Z

251

Cover: PNNL's Photovoltaic array produces electricity for our super-computing facility and adjacent car charging stations. IN THIS REPORT  

E-Print Network (OSTI)

#12;Cover: PNNL's Photovoltaic array produces electricity for our super-computing facility agencies, universities, and industry. Interdisciplinary teams at PNNL address many of America's most: 143 kBtu/ft2 ) · At least 7.5% of electricity use from renewable sources by 2013 and thereafter

252

Super Bowl City Leads on Energy Efficient Forefront | Department of Energy  

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

Bowl City Leads on Energy Efficient Forefront Bowl City Leads on Energy Efficient Forefront Super Bowl City Leads on Energy Efficient Forefront February 2, 2013 - 11:30am Addthis New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity, equivalent to powering a small home. | Photo courtesy of SMG. New Orleans' Mercedes-Benz Superdome features more than 26,000 LED lights on the building's exterior. The system uses only 10 kilowatts of electricity, equivalent to powering a small home. | Photo courtesy of SMG. John Horst Public Affairs Specialist with the Office of Energy Efficiency and Renewable Energy While the Baltimore Ravens and San Francisco 49ers compete to hoist the Vince Lombardi trophy this weekend, eco-friendly fans and city leaders in

253

Electric dipole-forbidden nuclear transitions driven by super-intense laser fields  

E-Print Network (OSTI)

Electric dipole-forbidden transitions of nuclei interacting with super-intense laser fields are investigated considering stable isotopes with suitable low-lying first excited states. Different classes of transitions are identified, and all magnetic sublevels corresponding to the near-resonantly driven nuclear transition are included in the description of the nuclear quantum system. We find that large transition matrix elements and convenient resonance energies qualify nuclear M1 transitions as good candidates for the coherent driving of nuclei. We discuss the implications of resonant interaction of intense laser fields with nuclei beyond the dipole approximation for the controlled preparation of excited nuclear states and important aspects of possible experiments aimed at observing these effects.

Adriana Plffy; Jrg Evers; Christoph H. Keitel

2007-10-31T23:59:59.000Z

254

Super Energy Efficiency Design (S.E.E.D.) Home Evaluation  

SciTech Connect

This report describes the results of evaluation by the Alliance for Residential Building Innovation (ARBI) Building America team of the 'Super Energy Efficient Design' (S.E.E.D) home, a 1,935 sq. ft., single-story spec home located in Tucson, AZ. This prototype design was developed with the goal of providing an exceptionally energy efficient yet affordable home and includes numerous aggressive energy features intended to significantly reduce heating and cooling loads such as structural insulated panel (SIP) walls and roof, high performance windows, an ERV, an air-to-water heat pump with mixed-mode radiant and forced air delivery, solar water heating, and rooftop PV. Source energy savings are estimated at 45% over the Building America B10 Benchmark. System commissioning, short term testing, long term monitoring and detailed analysis of results was conducted to identify the performance attributes and cost effectiveness of the whole house measure package.

German, A.; Dakin, B.; Backman, C.; Weitzel, E.; Springer, D.

2012-12-01T23:59:59.000Z

255

Appendix C: DOE Super-ESPC Project Acceptance Guidelines and Checklist  

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

Guidelines, Checklist, and Contract Clauses for Government Acceptance Guidelines, Checklist, and Contract Clauses for Government Acceptance of DOE Super-ESPC Projects  ECM Installation: All ECMs are installed in accordance with plans, specifications, standards, and other contract documents (sometimes by the Contractor, often by a subcontractor and always over a period of months).  Inspection, start-up, testing and commissioning. All ECMs are inspected, brought on line, tested, and commissioned interactively with all related Government-owned or Contractor-installed ECMs. Again, the ECMs should be operating in accordance with the design, plans, specifications, standards and other contract documents and manufacturer's recommendations. Individual ECMs may go through start-up and testing, but all interrelated

256

In R&D, Super X-rays Mark Many Spots  

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

A New Gas Loading System for Diamond Anvil Cells at GSECARS A New Gas Loading System for Diamond Anvil Cells at GSECARS Sidorowicz Named "Supervisor of the Year" SESS 2007: The School for Environmental Sciences with Synchrotrons Art and Science A Breakthrough in Interface Science APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed In R&D, Super X-rays Mark Many Spots MARCH 11, 2008 Bookmark and Share Research and Design Magazine "The Advanced Photon Source (APS) at the U.S. Dept. of Energy's Argonne National Laboratory has been kept busy of late." That's the first sentence of R&D Magazine's recent overview of research results from the APS. The article highlights "a new ultrafast synchrotron x-ray full-field phase contrast imaging technique and used it to reveal

257

Type III Dyson Sphere of Highly Advanced Civilizations around a Super Massive Black Hole  

E-Print Network (OSTI)

We describe a new system for a society of highly advanced civilizations around a super massive black hole (SMBH), as an advanced Type III "Dyson Sphere", pointing out an efficient usage of energy for the advanced civilizations. SMBH also works as a sink for waste materials. Here we assume that Type III civilisations of Kardashev classification [1] form a galactic club [2] in a galaxy, and the energy from the SMBH will be delivered to the club members, forming an energy control system similar to power grids in our present society. The energy is probably transmitted by a sharp beam with coherent electro-magnetic waves, which provide a new concept for the search for extraterrestrial intelligence (SETI) via detection of such energy transmission signals. This expands the search window for other intelligences within the Universe.

Inoue, Makoto

2011-01-01T23:59:59.000Z

258

New periodic variable stars coincident with ROSAT sources discovered using SuperWASP  

E-Print Network (OSTI)

We present optical lightcurves of 428 periodic variable stars coincident with ROSAT X-ray sources, detected using the first run of the SuperWASP photometric survey. Only 68 of these were previously recognised as periodic variables. A further 30 of these objects are previously known pre-main sequence stars, for which we detect a modulation period for the first time. Amongst the newly identified periodic variables, many appear to be close eclipsing binaries, their X-ray emission is presumably the result of RS CVn type behaviour. Others are probably BY Dra stars, pre-main sequence stars and other rapid rotators displaying enhanced coronal activity. A number of previously catalogued pulsating variables (RR Lyr stars and Cepheids) coincident with X-ray sources are also seen, but we show that these are likely to be misclassifications. We identify four objects which are probable low mass eclipsing binary stars, based on their very red colour and light curve morphology.

A. J. Norton; P. J. Wheatley; R. G. West; C. A. Haswell; R. A. Street; A. Collier Cameron; D. J. Christian; B. Enoch; M. Gallaway; C. Hellier; K. Horne; J. Irwin; S. R. Kane; T. A. Lister; J. P. Nicholas; N. Parley; D. Pollacco; R. Ryans; I. Skillen; D. M. Wilson

2007-02-23T23:59:59.000Z

259

New periodic variable stars coincident with ROSAT sources discovered using SuperWASP  

E-Print Network (OSTI)

We present optical lightcurves of 428 periodic variable stars coincident with ROSAT X-ray sources, detected using the first run of the SuperWASP photometric survey. Only 68 of these were previously recognised as periodic variables. A further 30 of these objects are previously known pre-main sequence stars, for which we detect a modulation period for the first time. Amongst the newly identified periodic variables, many appear to be close eclipsing binaries, their X-ray emission is presumably the result of RS CVn type behaviour. Others are probably BY Dra stars, pre-main sequence stars and other rapid rotators displaying enhanced coronal activity. A number of previously catalogued pulsating variables (RR Lyr stars and Cepheids) coincident with X-ray sources are also seen, but we show that these are likely to be misclassifications. We identify four objects which are probable low mass eclipsing binary stars, based on their very red colour and light curve morphology.

Norton, A J; West, R G; Haswell, C A; Street, R A; Cameron, A C; Christian, D J; Enoch, B; Gallaway, M; Hellier, C; Horne, K; Irwin, J; Kane, S R; Lister, T A; Nicholas, J P; Parley, N; Pollacco, D; Ryans, R; Skillen, I; Wilson, D M

2007-01-01T23:59:59.000Z

260

Transmission function properties for multi-layered structures: Application to super-resolution  

E-Print Network (OSTI)

We discuss the properties of the transmission function in the k-space for a generic multi-layered structure. In particular we analytically demonstrate that a transmission greater than one in the evanescent spectrum (amplification of the evanescent modes) can be directly linked to the guided modes supported by the structure. Moreover we show that the slope of the phase of the transmission function in the propagating spectrum is inversely proportional to the ability of the structure to compensate the diffraction of the propagating modes. We apply these findings to discuss several examples where super-resolution is achieved thanks to the simultaneous availability of the amplification of the evanescent modes and the diffraction compensation of the propagating modes.

Mattiucci, Nadia; Scalora, Michael; Bloemer, Mark J; Sibilia, Concita

2009-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
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261

Super-Efficient Refrigerator Program (SERP) evaluation volume 2: Preliminary impact and market transformation assessment  

SciTech Connect

The Super Efficient Refrigerator Program (SERP) is a collaborative utility program intended to transform the market for energy-efficient and environmentally friendly refrigerators. It is one of the first examples of a large-scale {open_quotes}market transformation{close_quotes} energy efficiency program. This report documents the preliminary impact and market transformation evaluation of SERP ({open_quotes}the Program{close_quotes}). Pacific Northwest National Laboratory (PNNL) conducted this evaluation for the U.S. Department of Energy. This study focuses on the preliminary impact evaluation and market transformation assessment, but also presents limited process evaluation information. It is based on interviews with refrigerator dealers and manufacturers, interviews with utility participants, industry data, and information from the Program administrators. Results from this study complement those from prior process evaluation also conducted by PNNL. 42 refs., 5 figs., 4 tabs.

Lee, A.D.; Conger, R.L.

1996-08-01T23:59:59.000Z

262

Holographic thermalization in N=4 Super Yang-Mills theory at finite coupling  

E-Print Network (OSTI)

We investigate the behavior of the energy momentum tensor correlators in holographic N=4 Super Yang-Mills plasma, taking finite coupling corrections into account. In the thermal limit we determine the flow of the quasinormal modes as a function of the 't Hooft coupling. Then we use a specific model of holographic thermalization to study the deviation of the spectral density from its thermal limit in an out-of-equilibrium situation. The main focus lies on the thermalization pattern with which the plasma constituents approach their thermal distribution as the coupling constant decreases from the infinite coupling limit. All obtained results point towards a weakening of the usual top-down thermalization pattern.

Stricker, Stefan A

2013-01-01T23:59:59.000Z

263

The Gardner category and nonlocal conservation laws for N=1 Super KdV  

Science Conference Proceedings (OSTI)

The nonlocal conserved quantities of the N=1 Super KdV are obtained using a Gardner map. A fermionic substitution semigroup and the resulting Gardner category are defined and several propositions concerning their algebraic structure are obtained. This algebraic framework makes it possible to define general transformations between different nonlinear SUSY differential equations. A SUSY ring extension is then introduced to deal with the nonlocal conserved quantities of SKdV. The algebraic version of the nonlocal conserved quantities is solved in terms of the exponential function applied to the D{sup -1} of the local conserved quantities of SKdV. Finally the same formulas are shown to work for rapidly decreasing superfields.

Andrea, S.; Restuccia, A.; Sotomayor, A. [Departamento de Matematicas, Universidad Simon Bolivar (Venezuela); Departamento de Fisica, Universidad Simon Bolivar (Venezuela); Departamento de Ciencias Basicas, Unexpo, Luis Caballero Mejias, Caracas (Venezuela)

2005-10-01T23:59:59.000Z

264

VOLATILE TRANSPORT INSIDE SUPER-EARTHS BY ENTRAPMENT IN THE WATER-ICE MATRIX  

SciTech Connect

Whether volatiles can be entrapped in a background matrix composing planetary envelopes and be dragged via convection to the surface is a key question in understanding atmospheric fluxes, cycles, and composition. In this paper, we consider super-Earths with an extensive water mantle (i.e., water planets), and the possibility of entrapment of methane in their extensive water-ice envelopes. We adopt the theory developed by van der Waals and Platteeuw for modeling solid solutions, often used for modeling clathrate hydrates, and modify it in order to estimate the thermodynamic stability field of a new phase called methane filled ice Ih. We find that in comparison to water ice VII the filled ice Ih structure may be stable not only at the high pressures but also at the high temperatures expected at the core-water mantle transition boundary of water planets.

Levi, A.; Podolak, M. [Department of Geophysics and Planetary Science, Tel Aviv University, Tel Aviv 69978 (Israel); Sasselov, D., E-mail: amitlevi.planetphys@gmail.com [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2013-05-20T23:59:59.000Z

265

DETECTION OF A LOW-ECCENTRICITY AND SUPER-MASSIVE PLANET TO THE SUBGIANT HD 38801  

Science Conference Proceedings (OSTI)

We report the detection of a large mass planet orbiting around the K0 metal-rich subgiant HD38801 (V = 8.26) by precise radial velocity (RV) measurements from the Subaru Telescope and the Keck Telescope. The star has a mass of 1.36 M{sub sun} and a metallicity of [Fe/H] = +0.26. The RV variations are consistent with a circular orbit with a period of 696.0 days and a velocity semiamplitude of 200.0 m s{sup -1}, which yield a minimum mass for the companion of 10.7 M{sub JUP} and a semimajor axis of 1.71 AU. Such super-massive objects with very low eccentricities and periods of hundreds of days are uncommon among the ensemble of known exoplanets.

Harakawa, Hiroki; Ida, Shigeru; Hori, Yasunori [Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Sato, Bun'ei [Global Edge Institute, Tokyo Institute of Technology, 2-12-1-S6-6 Ookayama, Meguro-ku, Tokyo 152-8550 (Japan); Fischer, Debra A. [Department of Physics and Astronomy, San Francisco State University, San Francisco, CA 94132 (United States); Omiya, Masashi [Department of Physics, Tokai University, 1117 Kitakaname, Hiratsuka, Kanagawa 259-1292 (Japan); Johnson, John A. [Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States); Marcy, Geoffrey W.; Howard, Andrew W. [Department of Astronomy, University of California, Berkeley, CA 94720 (United States); Toyota, Eri, E-mail: harakawa@geo.titech.ac.j [Kobe Science Museum, 7-7-6 Minatojima-Nakamachi, Chuo-ku, Kobe, Hyogo 650-0046 (Japan)

2010-05-20T23:59:59.000Z

266

Neutrino Magnetic Moments, Flavor Mixing, and the Super-Kamiokande Solar Data  

Science Conference Proceedings (OSTI)

We find that magnetic neutrino-electron scattering is unaffected by oscillations for vacuum mixing of Dirac neutrinos with only diagonal moments and for Majorana neutrinos with two flavors. For Mikheyev-Smirnov-Wolfenstein mixing, these cases are again obtained, though the effective moments can depend on the neutrino energy. Thus, e.g., the magnetic moments measured with {nu}(bar sign){sub e} from a reactor and {nu}{sub e} from the Sun could be different. With minimal assumptions, we find a new limit on {mu}{sub {nu}} using the 825-d Super-Kamiokande solar neutrino data: |{mu}{sub {nu}}|{<=}1.5x10{sup -} {sup 10}{mu}{sub B} at 90% CL, comparable to the existing reactor limit. (c) 1999 The American Physical Society.

Beacom, J. F.; Vogel, P.

1999-12-20T23:59:59.000Z

267

Evaluation of the Super Efficient Refrigerator Program (SERP) in the Bonneville Power Administration service territory  

Science Conference Proceedings (OSTI)

The Super Efficient Refrigerator Program (SERP) is a collaborative utility program intended to transform the market for energy-efficient and environmentally friendly refrigerators. it is one of the first examples of large-scale {open_quotes}market transformation{close_quotes} energy efficiency program. This report documents the evaluation of SERP ({open_quotes}the Program{close_quotes}) in the Bonneville Power Administration`s (Bonneville`s) service territory. Pacific Northwest National Laboratory (PNNL) conducted this evaluation for Bonneville. This study includes the process evaluation, preliminary impact evaluation, and market transformation assessment. It is based on site visits and interviews with refrigerator dealers and manufacturers, industry data, and Bonneville information. Results from this study are compared with those from a parallel study that examines the Program across the 24 participating utilities.

Lee, A.D.; Conger, R.L.

1996-06-01T23:59:59.000Z

268

Constraining the Leading Weak Axial Two-body Current by SNO and Super-K  

E-Print Network (OSTI)

We analyze the Sudbury Neutrino Observatory (SNO) and Super-Kamiokande (SK) data on charged current (CC), neutral current (NC) and neutrino electron elastic scattering (ES) reactions to constrain the leading weak axial two-body current parameterized by L_1A. This two-body current is the dominant uncertainty of every low energy weak interaction deuteron breakup process, including SNO's CC and NC reactions. Our method shows that the theoretical inputs to SNO's determination of the CC and NC fluxes can be self-calibrated, be calibrated by SK, or be calibrated by reactor data. The only assumption made is that the total flux of active neutrinos has the standard ^8B spectral shape (but distortions in the electron neutrino spectrum are allowed). We show that SNO's conclusion about the inconsistency of the no-flavor-conversion hypothesis does not contain significant theoretical uncertainty, and we determine the magnitude of the active solar neutrino flux.

Jiunn-Wei Chen; Karsten M. Heeger; R. G. Hamish Robertson

2002-10-24T23:59:59.000Z

269

Can the Super-Kamiokande Atmospheric Data Predict the Solar Neutrino Deficit?  

E-Print Network (OSTI)

In this Letter we show that the evidence for neutrino oscillations from the Super-Kamiokande atmospheric neutrino data fully determines the 3x3 neutrino-oscillations mixing matrix and predicts an energy independent solar neutrino deficit at the level of 45%. This corresponds to a ratio of measured to predicted neutrino flux of R_e^{Solar} = 0.55, in good agreement with the experimental results. We achieve this result within the framework of a minimal, three-generations neutrino mixing, with mass squared differences of dM^2 = 0.45 eV^2 and dm^2 = O(10^-3) eV^2. The mixing matrix derived here is characterized by the mixing angles theta = 35.1, beta = 5.5, and psi = 23.3, and a vanishing CP-violating phase, delta = 0.

Stancu, I

1999-01-01T23:59:59.000Z

270

In vitro adsorption of sodium pentobarbital by SuperChar, USP and Darco G-60 activated charcoals  

SciTech Connect

This study was designed to examine the in vitro adsorption of sodium pentobarbital by three activated charcoals. Solutions of sodium pentobarbital (20 mM) were prepared in distilled water and in 70% sorbitol (w/v). Radiolabeled (/sup 14/C) sodium pentobarbital was added to each solution to serve as a concentration marker. Two ml of each drug solution was added to test tubes containing 40 mg of either Darco G-60, USP, or SuperChar activated charcoal. The drug-charcoal mixtures were incubated at 37 degrees C for O, 2.5, 5, 7.5 or 10 min. Equilibrium, indicated by a constant percentage of drug bound for two consecutive time periods, was established immediately for the aqueous mixtures and for Darco G-60 in sorbitol. The time to equilibrium was prolonged for USP (2.5 min) and SuperChar (5 min) in the presence of sorbitol. In the second series of experiments, solutions of sodium pentobarbital (1.25 to 160 mM) were prepared in either distilled water or sorbitol. Amount of drug bound by 10 to 320 mg of activated charcoal within a 10 min incubation period was determined. Scatchard analysis determined maximum binding capacity (Bmax) and dissociation constants (Kd) for each activated charcoal. In water, Bmax (mumoles/gm) was greatest for SuperChar (1141), followed by USP (580) and Darco G-60 (381), while the Kd's did not differ. Sorbitol did not change the Bmax or Kd of USP or Darco G-60, but the additive significantly decreased the Bmax (717) and increased the Kd for SuperChar (3.3 to 10.1 mM). The results suggest that relative binding capacity of activated charcoal is directly proportional to surface area, and that sorbitol significantly reduces sodium pentobarbital binding to SuperChar.

Curd-Sneed, C.D.; Parks, K.S.; Bordelon, J.G.; Stewart, J.J.

1987-01-01T23:59:59.000Z

271

WIMS/PANTHER analysis of UO{sub 2}/MOX cores using embedded super-cells  

Science Conference Proceedings (OSTI)

This paper describes a method of analysing PWR UO{sub 2}MOX cores with WIMS/PANTHER. Embedded super-cells, run within the reactor code, are used to correct the standard methodology of using 2-group smeared data from single assembly lattice calculations. In many other codes the weakness of this standard approach has been improved for MOX by imposing a more realistic environment in the lattice code, or by improving the sophistication of the reactor code. In this approach an intermediate set of calculations is introduced, leaving both lattice and reactor calculations broadly unchanged. The essence of the approach is that the whole core is broken down into a set of 'embedded' super-cells, each extending over just four quarter assemblies, with zero leakage imposed at the assembly mid-lines. Each supercell is solved twice, first with a detailed multi-group pin-by-pin solution, and then with the standard single assembly approach. Correction factors are defined by comparing the two solutions, and these can be applied in whole core calculations. The restriction that all such calculations are modelled with zero leakage means that they are independent of each other and of the core-wide flux shape. This allows parallel pre-calculation for the entire cycle once the loading pattern has been determined, in much the same way that single assembly lattice calculations can be pre-calculated once the range of fuel types is known. Comparisons against a whole core pin-by-pin reference demonstrates that the embedding process does not introduce a significant error, even after burnup and refuelling. Comparisons against a WIMS reference demonstrate that a pin-by-pin multi-group diffusion solution is capable of capturing the main interface effects. This therefore defines a practical approach for achieving results close to lattice code accuracy, but broadly at the cost of a standard reactor calculation. (authors)

Knight, M.; Bryce, P. [EDF Energy, Barnett Way, Barnwood, Gloucester (United Kingdom); Hall, S. [Advanced Modelling and Computation Group, Imperial College, London (United Kingdom)

2012-07-01T23:59:59.000Z

272

A POSSIBLE CARBON-RICH INTERIOR IN SUPER-EARTH 55 Cancri e  

SciTech Connect

Terrestrial planets in the solar system, such as the Earth, are oxygen-rich, with silicates and iron being the most common minerals in their interiors. However, the true chemical diversity of rocky planets orbiting other stars is yet unknown. Mass and radius measurements are used to constrain the interior compositions of super-Earths (exoplanets with masses of 1-10 M{sub Circled-Plus }), and are typically interpreted with planetary interior models that assume Earth-centric oxygen-rich compositions. Using such models, the super-Earth 55 Cancri e (mass 8 M{sub Circled-Plus }, radius 2 R{sub Circled-Plus }) has been suggested to bear an interior composition consisting of Fe, silicates, and an envelope ({approx}> 10% by mass) of supercritical water. We report that the mass and radius of 55 Cancri e can also be explained by a carbon-rich solid interior made of Fe, C, SiC, and/or silicates and without a volatile envelope. While the data allow Fe mass fractions of up to 40%, a wide range of C, SiC, and/or silicate mass fractions are possible. A carbon-rich 55 Cancri e is also plausible if its protoplanetary disk bore the same composition as its host star, which has been reported to be carbon-rich. However, more precise estimates of the stellar elemental abundances and observations of the planetary atmosphere are required to further constrain its interior composition. The possibility of a C-rich interior in 55 Cancri e opens a new regime of geochemistry and geophysics in extraterrestrial rocky planets, compared to terrestrial planets in the solar system.

Madhusudhan, Nikku [Department of Physics and Department of Astronomy, Yale University, New Haven, CT 06511 (United States); Lee, Kanani K. M. [Department of Geology and Geophysics, Yale University, New Haven, CT 06511 (United States); Mousis, Olivier, E-mail: Nikku.Madhusudhan@yale.edu [Universite de Franche-Comte, Institut UTINAM, CNRS/INSU, UMR 6213, Observatoire des Sciences de l'Univers THETA, CP 1615, F-25010 Besancon Cedex (France)

2012-11-10T23:59:59.000Z

273

Evaluation of the Super ESPC Program: Level 2 -- Recalculated Cost Savings  

SciTech Connect

This report presents the results of Level 2 of a three-tiered evaluation of the U.S. Department of Energy Federal Energy Management Program's Super Energy Savings Performance Contract (Super ESPC) Program. Level 1 of the analysis studied all of the Super ESPC projects for which at least one Annual Measurement & Verification (M&V) Report had been produced by April 2006. For those 102 projects in aggregate, we found that the value of cost savings reported by the energy service company (ESCO) in the Annual M&V Reports was 108% of the cost savings guaranteed in the contracts. We also compared estimated energy savings (which are not guaranteed, but are the basis for the guaranteed cost savings) to the energy savings reported by the ESCO in the Annual M&V Report. In aggregate, reported energy savings were 99.8% of estimated energy savings on the basis of site energy, or 102% of estimated energy savings based on source energy. Level 2 focused on a random sample of 27 projects taken from the 102 Super ESPC projects studied in Level 1. The objectives were, for each project in the sample, to: repeat the calculations of the annual energy and cost savings in the most recent Annual M&V Report to validate the ESCO's results or correct any errors, and recalculate the value of the reported energy, water, and operations and maintenance (O&M) savings using actual utility prices paid at the project site instead of the 'contract' energy prices - the prices that are established in the project contract as those to be used by the ESCO to calculate the annual cost savings, which determine whether the guarantee has been met. Level 3 analysis will be conducted on three to five projects from the Level 2 sample that meet validity criteria for whole-building or whole-facility data analysis. This effort will verify energy and cost savings using statistical analysis of actual utility use, cost, and weather data. This approach, which can only be used for projects meeting particular validity criteria, is described in Shonder and Florita (2003) and Shonder and Hughes (2005). To address the first objective of the Level 2 analysis, we first assembled all the necessary information, and then repeated the ESCOs' calculations of reported annual cost savings. Only minor errors were encountered, the most common being the use of incorrect escalation rates to calculate utility prices or O&M savings. Altogether, our corrected calculations of the ESCO's reported cost savings were within 0.6% of the ESCOs' reported cost savings, and errors found were as likely to favor the government as they were the ESCO. To address the second objective, we gathered data on utility use and cost from central databases maintained by the Department of Defense and the General Services Administration, and directly from some of the sites, to determine the prices of natural gas and electricity actually paid at the sites during the periods addressed by the annual reports. We used these data to compare the actual utility costs at the sites to the contract utility prices. For natural gas, as expected, we found that prices had risen much faster than had been anticipated in the contracts. In 17 of the 18 projects for which the comparison was possible, contract gas prices were found to be lower than the average actual prices being paid. We conclude that overall in the program, the estimates of gas prices and gas price escalation rates used in the Super ESPC projects have been conservative. For electricity, it was possible to compare contract prices with the actual (estimated) marginal prices of electricity in 20 projects. In 14 of these projects, the overall contract electricity price was found to be lower than the marginal price of electricity paid to the serving utility. Thus it appears that conservative estimates of electricity prices and escalation rates have been used in the program as well. Finally we calculated the value of the reported energy savings using the prices of utilities actually paid by the sites instead of the contract

Shonder, John A [ORNL; Hughes, Patrick [ORNL

2009-04-01T23:59:59.000Z

274

Evaluation of the Super ESPC Program: Level 2 -- Recalculated Cost Savings  

SciTech Connect

This report presents the results of Level 2 of a three-tiered evaluation of the U.S. Department of Energy Federal Energy Management Program's Super Energy Savings Performance Contract (Super ESPC) Program. Level 1 of the analysis studied all of the Super ESPC projects for which at least one Annual Measurement & Verification (M&V) Report had been produced by April 2006. For those 102 projects in aggregate, we found that the value of cost savings reported by the energy service company (ESCO) in the Annual M&V Reports was 108% of the cost savings guaranteed in the contracts. We also compared estimated energy savings (which are not guaranteed, but are the basis for the guaranteed cost savings) to the energy savings reported by the ESCO in the Annual M&V Report. In aggregate, reported energy savings were 99.8% of estimated energy savings on the basis of site energy, or 102% of estimated energy savings based on source energy. Level 2 focused on a random sample of 27 projects taken from the 102 Super ESPC projects studied in Level 1. The objectives were, for each project in the sample, to: repeat the calculations of the annual energy and cost savings in the most recent Annual M&V Report to validate the ESCO's results or correct any errors, and recalculate the value of the reported energy, water, and operations and maintenance (O&M) savings using actual utility prices paid at the project site instead of the 'contract' energy prices - the prices that are established in the project contract as those to be used by the ESCO to calculate the annual cost savings, which determine whether the guarantee has been met. Level 3 analysis will be conducted on three to five projects from the Level 2 sample that meet validity criteria for whole-building or whole-facility data analysis. This effort will verify energy and cost savings using statistical analysis of actual utility use, cost, and weather data. This approach, which can only be used for projects meeting particular validity criteria, is described in Shonder and Florita (2003) and Shonder and Hughes (2005). To address the first objective of the Level 2 analysis, we first assembled all the necessary information, and then repeated the ESCOs' calculations of reported annual cost savings. Only minor errors were encountered, the most common being the use of incorrect escalation rates to calculate utility prices or O&M savings. Altogether, our corrected calculations of the ESCO's reported cost savings were within 0.6% of the ESCOs' reported cost savings, and errors found were as likely to favor the government as they were the ESCO. To address the second objective, we gathered data on utility use and cost from central databases maintained by the Department of Defense and the General Services Administration, and directly from some of the sites, to determine the prices of natural gas and electricity actually paid at the sites during the periods addressed by the annual reports. We used these data to compare the actual utility costs at the sites to the contract utility prices. For natural gas, as expected, we found that prices had risen much faster than had been anticipated in the contracts. In 17 of the 18 projects for which the comparison was possible, contract gas prices were found to be lower than the average actual prices being paid. We conclude that overall in the program, the estimates of gas prices and gas price escalation rates used in the Super ESPC projects have been conservative. For electricity, it was possible to compare contract prices with the actual (estimated) marginal prices of electricity in 20 projects. In 14 of these projects, the overall contract electricity price was found to be lower than the marginal price of electricity paid to the serving utility. Thus it appears that conservative estimates of electricity prices and escalation rates have been used in the program as well. Finally we calculated the value of the reported energy savings using the prices of utilities actually paid by the sites instead of the contract prices. In 16 of the 22 projects (

Shonder, John A [ORNL; Hughes, Patrick [ORNL

2009-04-01T23:59:59.000Z

275

Search for the QCD critical point in nuclear collisions at 158A GeV at the CERN Super Proton Synchrotron (SPS)  

E-Print Network (OSTI)

Pion production in nuclear collisions at the Super Proton Synchrotron (SPS) is investigated with the aim to search, in a restricted domain of the phase diagram, for power laws in the behavior of correlations that are ...

Roland, Christof E.

276

Discovery and Characterization of Transiting Super Earths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope  

E-Print Network (OSTI)

Doppler and transit surveys are finding extrasolar planets of ever smaller mass and radius, and are now sampling the domain of super Earths (13R?). Recent results from the Doppler surveys suggest that discovery of a ...

Seager, Sara

277

"FEMP Support Through Initial Proposal Review for Contractor-Identified Super ESPC Project"  

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

3 3 " "FEMP Support Through Initial Proposal Review for Contractor-Identified Super ESPC Project" "Task #","Task Title","Work Scope","Deliverable","Agency Requirements" " " "Phase One Activities - Project Planning" "1-1","Energy Potential Assessment","FEMP Services will analyze all available information to determine if Agency specified project site is a good candidate for ESPC. FEMP Services will provide recommendations as needed to improve project economics for Super ESPC/recommend other project implementation strategies","Telecon advice and recommendations","Agency will provide site data requested by FEMP Services staff. Typical data requested is 1-2 years of monthly utility bill, past audits, building list and maintenance records, facility condition assessments."

278

The Minimum-Mass Extrasolar Nebula: In-Situ Formation of Close-In Super-Earths  

E-Print Network (OSTI)

Close-in super-Earths, with radii R = 2-5 R_Earth and orbital periods P < 100 days, orbit more than half, and perhaps nearly all Sun-like stars in the universe. We use this omnipresent population to construct the minimum-mass extrasolar nebula (MMEN), the circumstellar disk of solar-composition solids and gas from which such planets formed, if they formed near their current locations and did not migrate. In a series of back-of-the-envelope calculations, we demonstrate how in-situ formation in the MMEN is fast, efficient, and can reproduce many of the observed properties of close-in super-Earths, including their gas-to-rock fractions. Testable predictions are discussed.

Chiang, E

2012-01-01T23:59:59.000Z

279

Effects of Resin Particle Size and Solution Temperature on SuperLig(R) 644 Resin Performance with AN-105 Simulate  

DOE Green Energy (OSTI)

The performance of the SuperLig(R) 644 resin loading and elution was evaluated at 25, 35, and 45 degree C using a single-column containing 2.25 g of oven-dry, hydrogen form of SuperLig(R) 664 resin. A simulated Envelope A solution was used to mimic the composition of low-activity waste solution from Tank 241-AN-105 supernate in the Hanford Site waste tank. The simulant was spiked with small quantities of trace metals (cadmium, chromium, iron, and lead) to evaluate the effects of these metals on cesium sorption. The results from column tests performed at 25, 35, and 45 degree C showed that more than 100 BVs of simulated Envelope A solution could be processed at each temperature before 50 percent breakthrough of the cesium occurred.

Nash, C.A.

2003-07-15T23:59:59.000Z

280

ON THE IMPACT OF SUPER RESOLUTION WSR-88D DOPPLER RADAR DATA ASSIMILATION ON HIGH RESOLUTION NUMERICAL MODEL FORECASTS  

SciTech Connect

Assimilation of radar velocity and precipitation fields into high-resolution model simulations can improve precipitation forecasts with decreased 'spin-up' time and improve short-term simulation of boundary layer winds (Benjamin, 2004 & 2007; Xiao, 2008) which is critical to improving plume transport forecasts. Accurate description of wind and turbulence fields is essential to useful atmospheric transport and dispersion results, and any improvement in the accuracy of these fields will make consequence assessment more valuable during both routine operation as well as potential emergency situations. During 2008, the United States National Weather Service (NWS) radars implemented a significant upgrade which increased the real-time level II data resolution to 8 times their previous 'legacy' resolution, from 1 km range gate and 1.0 degree azimuthal resolution to 'super resolution' 250 m range gate and 0.5 degree azimuthal resolution (Fig 1). These radar observations provide reflectivity, velocity and returned power spectra measurements at a range of up to 300 km (460 km for reflectivity) at a frequency of 4-5 minutes and yield up to 13.5 million point observations per level in super-resolution mode. The migration of National Weather Service (NWS) WSR-88D radars to super resolution is expected to improve warning lead times by detecting small scale features sooner with increased reliability; however, current operational mesoscale model domains utilize grid spacing several times larger than the legacy data resolution, and therefore the added resolution of radar data is not fully exploited. The assimilation of super resolution reflectivity and velocity data into high resolution numerical weather model forecasts where grid spacing is comparable to the radar data resolution is investigated here to determine the impact of the improved data resolution on model predictions.

Chiswell, S

2009-01-11T23:59:59.000Z

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281

An Integrated Refrigeration, Humidity Control and HVAC Solution for Supermarkets: Field Demonstration at a Wal-Mart SuperCenter  

Science Conference Proceedings (OSTI)

This report describes a systematic approach to developing an energy efficient and cost effective solution for refrigeration, humidity control, indoor air quality, and space heating and cooling for large retail super centers. The report also presents the results of a field demonstration using a newly developed integrated system that achieved significant energy savings and other benefits compared to the state-of-the-art system.

2004-04-20T23:59:59.000Z

282

L{sup p} Theory for Super-Parabolic Backward Stochastic Partial Differential Equations in the Whole Space  

SciTech Connect

This paper is concerned with semi-linear backward stochastic partial differential equations (BSPDEs for short) of super-parabolic type. An L{sup p}-theory is given for the Cauchy problem of BSPDEs, separately for the case of p Element-Of (1,2] and for the case of p Element-Of (2,{infinity}). A comparison theorem is also addressed.

Du Kai, E-mail: kdu@fudan.edu.cn; Qiu, Jinniao, E-mail: 071018032@fudan.edu.cn; Tang Shanjian, E-mail: sjtang@fudan.edu.cn [Fudan University, Department of Finance and Control Sciences, School of Mathematical Sciences, and Laboratory of Mathematics for Nonlinear Sciences (China)

2012-04-15T23:59:59.000Z

283

Comment on "Search for periodic modulations of the solar neutrino flux in Super-Kamiokande" by J. Yoo et al  

E-Print Network (OSTI)

We comment on a recent article by Yoo et al. that presents an analysis of Super-Kamiokande 10-day and 5-day data, correcting certain errors in that article. We also point out that, in using the Lomb-Scargle method of power spectrum analysis, Yoo et al. ignore much of the relevant data. A likelihood analysis, that can take account of all of the relevant data, yields evidence indicative of modulation by solar processes.

P. A. Sturrock; D. O. Caldwell; J. D. Scargle; G. Walther; M. S. Wheatland

2004-03-23T23:59:59.000Z

284

STRUCTURE OF THE INNER JET OF OJ287 FROM VLBA DATA AT 15 GHz IN SUPER-RESOLUTION MODE  

Science Conference Proceedings (OSTI)

In this work we show the results obtained from the Very Long Baseline Array data at 15 GHz of OJ287 in super-resolution mode. The data showed a jet configuration in the form of a 'fork' where superluminal components emerge via stationary components at the northwest and the southeast close to the core to form parallel trajectories along the southwest direction in the plane of sky. This agrees with a source structure of an extended, broad morphology of OJ287.

Tateyama, Claudio E. [CEA-Instituto Nacional de Pesquisas Espaciais (INPE), Av. dos Astronautas 1758, 12201-970 Sao Jose dos Campos, SP, Brazil. (Brazil)] [CEA-Instituto Nacional de Pesquisas Espaciais (INPE), Av. dos Astronautas 1758, 12201-970 Sao Jose dos Campos, SP, Brazil. (Brazil)

2013-04-01T23:59:59.000Z

285

The Injection System of the INFN-SuperB Factory Project: Preliminary Design  

Science Conference Proceedings (OSTI)

The ultra high luminosity B-factory (SuperB) project of INFN requires a high performance and reliable injection system, providing electrons at 4 GeV and positrons at 7 GeV, to fulfil the very tight requirements of the collider. Due to the short beam lifetime, continuous injection of electron and positron bunches in both LER and HER rings is necessary to maintain an high average luminosity. Polarized electrons are required for experiments and must be delivered by the injection system, due to the beam lifetime shorter than the ring polarization build-up: they will be produced by means of a SLAC-SLC polarized gun. The emittance and the energy spread of the e{sup -}/e{sup +} beams are reduced in a 1 GeV Damping Ring (DR) before injection in the main rings. Two schemes for positron production are under study, one with e{sup -}/e{sup +} conversion at low energy (conversion at 6 GeV and a recirculation line to bring the positrons back to the DR. Acceleration through the Linac is provided by a 2856 MHz RF system made of travelling wave (TW), room temperature accelerating structures.

Boni, Roberto; /INFN, Rome; Guiducci, Susanna; /INFN, Rome; Preger, Miro; /INFN, Rome; Raimondi, Pantaleo; /INFN, Rome; Chance, Antoine; /Saclay; Dadoun, Olivier; /Orsay, LAL; Poirier, Freddy; /Orsay, LAL; Variola, Alessandro; /Orsay, LAL; Seeman, John; /SLAC

2012-07-05T23:59:59.000Z

286

Studies of Nucleon Form Factors with 12 GeV CEBAF and SuperBigBite  

SciTech Connect

The elastic electromagnetic form factors are among the most fundamental quantities that describe the ground-state structure of the proton and neutron. Precision data of the form factors over a wide kinematical range provide a powerful test of current theories of hadron structure. A number of experiments aiming to measure the electric and magnetic elastic form factors of the neutron, G{sub E}{sup n} and G{sub M}{sup n}, and proton, G{sub E}{sup p}, at very high momentum transfer, up to the range of Q{sup 2} = 10-14 (GeV/c){sup 2}, are planned to be carried out with the future 11 GeV electron beam of the upgraded CEBAF at Jefferson Lab. These experiments will determine the nucleon form factors with unprecedented precision to Q{sup 2}-values up to three times higher than those of existing data. We review the approved proposals and the conceptual design of a new spectrometer, SuperBigBite, that will be used in these and other future experiments at Jefferson Lab.

Jens-Ole Hansen

2012-04-01T23:59:59.000Z

287

The Nature of the Atmosphere of the Transiting Super-Earth GJ 1214b  

E-Print Network (OSTI)

The newly discovered planet GJ 1214b is the first known transiting super-Earth requiring a significant atmosphere to explain its observed mass and radius. Models for the structure of this planet predict that it likely possesses a H-He envelope of at least 0.05% of the total mass of the planet. However, models without a significant H-He atmosphere are not entirely ruled out by the available data. Here we explore a range of possible atmospheres for the planet, ranging from solar composition gas, to pure CO_2 or water (steam). We present transmission and emission spectra for each of these cases. We find that, if GJ 1214b possesses a hydrogen-rich atmosphere as expected, then the primary transit depth for such an atmosphere would vary at a level of up to 0.3% as a function of wavelength, relative to the background light of its M-dwarf host star. Observations at this level of precision are potentially obtainable with current space-based instrumentation. Successful detection of the transmission signature of this pl...

Miller-Ricci, E

2010-01-01T23:59:59.000Z

288

WAITING TIMES OF QUASI-HOMOLOGOUS CORONAL MASS EJECTIONS FROM SUPER ACTIVE REGIONS  

Science Conference Proceedings (OSTI)

Why and how do some active regions (ARs) frequently produce coronal mass ejections (CMEs)? These are key questions for deepening our understanding of the mechanisms and processes of energy accumulation and sudden release in ARs and for improving our space weather prediction capability. Although some case studies have been performed, these questions are still far from fully answered. These issues are now being addressed statistically through an investigation of the waiting times of quasi-homologous CMEs from super ARs in solar cycle 23. It is found that the waiting times of quasi-homologous CMEs have a two-component distribution with a separation at about 18 hr. The first component is a Gaussian-like distribution with a peak at about 7 hr, which indicates a tight physical connection between these quasi-homologous CMEs. The likelihood of two or more occurrences of CMEs faster than 1200 km s{sup -1} from the same AR within 18 hr is about 20%. Furthermore, the correlation analysis among CME waiting times, CME speeds, and CME occurrence rates reveals that these quantities are independent of each other, suggesting that the perturbation by preceding CMEs rather than free energy input is the direct cause of quasi-homologous CMEs. The peak waiting time of 7 hr probably characterizes the timescale of the growth of the instabilities triggered by preceding CMEs. This study uncovers some clues from a statistical perspective for us to understand quasi-homologous CMEs as well as CME-rich ARs.

Wang Yuming; Liu Lijuan; Shen Chenglong; Liu Rui; Ye Pinzhong; Wang, S., E-mail: ymwang@ustc.edu.cn [CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, Anhui 230026 (China)

2013-02-01T23:59:59.000Z

289

Super-hot (T > 30 MK) Thermal Plasma in Solar Flares  

E-Print Network (OSTI)

The Sun offers a convenient nearby laboratory to study the physical processes of particle acceleration and impulsive energy release in magnetized plasmas that occur throughout the universe, from planetary magnetospheres to black hole accretion disks. Solar flares are the most powerful explosions in the solar system, releasing up to 10^32-10^33 ergs over only 100-1,000 seconds, accelerating electrons up to hundreds of MeV and heating plasma to tens of MK. The accelerated electrons and the hot plasma each contain tens of percent of the total flare energy, indicating an intimate link between particle acceleration, plasma heating, and flare energy release. The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) observes the X-ray emission from these processes from ~3 keV to ~17 MeV with unprecedented spectral, spatial, and temporal resolution. RHESSI observations show that "super-hot" (>30 MK) plasma temperatures are achieved almost exclusively by intense, GOES X-class flares and appear to be strictly a...

Caspi, Amir

2011-01-01T23:59:59.000Z

290

Born's Rule as Signature of a Super-Classical Current Algebra  

E-Print Network (OSTI)

We present a new tool for calculating the interference patterns and particle trajectories of a double-, three- and N-slit system on the basis of an emergent sub-quantum theory developed by our group throughout the last years. The quantum itself is considered as an emergent system representing an off-equilibrium steady state oscillation maintained by a constant throughput of energy provided by a classical zero-point energy field. We introduce the concept of a "relational causality" which allows for evaluating structural interdependences of different systems levels, i.e. in our case of the relations between partial and total probability density currents, respectively. Combined with the application of 21st century classical physics like, e.g., modern nonequilibrium thermodynamics, we thus arrive at a "super-classical" theory. Within this framework, the proposed current algebra directly leads to a new formulation of the guiding equation which is equivalent to the original one of the de Broglie-Bohm theory. By proving the absence of third order interferences in three-path systems it is shown that Born's rule is a natural consequence of our theory. Considering the series of one-, double-, or, generally, of N-slit systems, with the first appearance of an interference term in the double slit case, we can explain the violation of Sorkin's first order sum rule, just as the validity of all higher order sum rules. Moreover, the Talbot patterns and Talbot distance for an arbitrary N-slit device can be reproduced exactly by our model without any quantum physics tool.

Siegfried Fussy; Johannes Mesa Pascasio; Herbert Schwabl; Gerhard Groessing

2013-08-27T23:59:59.000Z

291

SUPER-AGB-AGB EVOLUTION AND THE CHEMICAL INVENTORY IN NGC 2419  

Science Conference Proceedings (OSTI)

We follow the scenario of formation of second-generation stars in globular clusters by matter processed by hot bottom burning (HBB) in massive asymptotic giant branch (AGB) stars and super-AGB stars (SAGB). In the cluster NGC 2419 we assume the presence of an extreme population directly formed from the AGB and SAGB ejecta, so we can directly compare the yields for a metallicity Z = 0.0003 with the chemical inventory of the cluster NGC 2419. At such a low metallicity, the HBB temperatures (well above 10{sup 8} K) allow a very advanced nucleosynthesis. Masses {approx}6 M{sub Sun} deplete Mg and synthesize Si, going beyond Al, so this latter element is only moderately enhanced; sodium cannot be enhanced. The models are consistent with the observations, although the predicted Mg depletion is not as strong as in the observed stars. We predict that the oxygen abundance must be depleted by a huge factor (>50) in the Mg-poor stars. The HBB temperatures are close to the region where other p-capture reactions on heavier nuclei become possible. We show that high potassium abundance found in Mg-poor stars can be achieved during HBB by p-captures on the argon nuclei, if the relevant cross section(s) are larger than listed in the literature or if the HBB temperature is higher. Finally, we speculate that some calcium production is occurring owing to proton capture on potassium. We emphasize the importance of a strong effort to measure a larger sample of abundances in this cluster.

Ventura, Paolo; D'Antona, Francesca; Carini, Roberta [INAF-Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio (Italy); Di Criscienzo, Marcella [INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Napoli (Italy); D'Ercole, Annibale [INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna (Italy); Vesperini, Enrico, E-mail: paolo.ventura@oa-roma.inaf.it [Department of Astronomy, Indiana University, Bloomington (United States)

2012-12-20T23:59:59.000Z

292

A SUPER-EARTH ORBITING THE NEARBY SUN-LIKE STAR HD 1461  

Science Conference Proceedings (OSTI)

We present precision radial velocity (RV) data that reveal a Super-Earth mass planet and two probable additional planets orbiting the bright nearby G0V star HD 1461. Our 12.8 years of Keck High Resolution Echelle Spectrometer precision RVs indicate the presence of a 7.4 M{sub +} planet on a 5.77 day orbit. The data also suggest, but cannot yet confirm, the presence of outer planets on low-eccentricity orbits with periods of 446.1 and 5017 days, and projected masses (Msin i) of 27.9 and 87.1 M{sub +}, respectively. Test integrations of systems consistent with the RV data suggest that the configuration is dynamically stable. We present a 12.2 year time series of photometric observations of HD 1461, which comprise 799 individual measurements, and indicate that it has excellent long-term photometric stability. However, there are small amplitude variations with periods comparable to those of the suspected second and third signals in the RVs near 5000 and 446 days, thus casting some suspicion on those periodicities as Keplerian signals. If the 5.77 day companion has a Neptune-like composition, then its expected transit depth is of order dapprox0.5 mmag. The geometric a priori probability of transits is approx8%. Phase folding of the ground-based photometry shows no indication that transits of the 5.77 day companion are occurring, but high-precision follow-up of HD 1461 during upcoming transit phase windows will be required to definitively rule out or confirm transits. This new system joins a growing list of solar-type stars in the immediate galactic neighborhood that are accompanied by at least one Neptune (or lower) mass planets having orbital periods of 50 days or less.

Rivera, Eugenio J.; Vogt, Steven S.; Laughlin, Gregory; Meschiari, Stefano [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Butler, R. Paul [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015-1305 (United States); Henry, Gregory W. [Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209 (United States)

2010-01-10T23:59:59.000Z

293

A Search for Nucleon Decay via $n \\rightarrow \\bar? ?^{0}$ and $p \\rightarrow \\bar? ?^{+}$ in Super-Kamiokande  

E-Print Network (OSTI)

We present the results of searches for nucleon decay via bound neutron to antineutrino plus pizero and proton to antineutrino plus piplus using data from a combined 172.8 kiloton-years exposure of Super-Kamiokande-I, -II, and -III. We set lower limits on the partial lifetime for each of these modes. For antineutrino pizero, the partial lifetime is >1.1x10^{33} years; for antineutrino piplus, the partial lifetime is >3.9x10^{32} years at 90% confidence level.

Super-Kamiokande Collaboration; :; K. Abe; Y. Hayato; T. Iida; K. Iyogi; J. Kameda; Y. Koshio; Y. Kozuma; Ll. Marti; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; K. Ueno; K. Ueshima; S. Yamada; T. Yokozawa; C. Ishihara; H. Kaji; T. Kajita; K. Kaneyuki; K. P. Lee; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; M. Goldhaber; K. Bays; W. R. Kropp; S. Mine; C. Regis; A. Renshaw; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. B. Albert; K. Scholberg; C. W. Walter; R. Wendell; T. M. Wongjirad; T. Ishizuka; S. Tasaka; J. G. Learned; S. Matsuno; S. N. Smith; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; M. Ikeda; A. Minamino; T. Nakaya; Y. Fukuda; Y. Itow; G. Mitsuka; T. Tanaka; C. K. Jung; G. D. Lopez; I. Taylor; C. Yanagisawa; H. Ishino; A. Kibayashi; S. Mino; T. Mori; M. Sakuda; H. Toyota; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; H. Okazawa; Y. Choi; K. Nishijima; M. Koshiba; M. Yokoyama; Y. Totsuka; K. Martens; J. Schuemann; M. R. Vagins; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; E. Thrane; R. J. Wilkes

2013-05-19T23:59:59.000Z

294

ATMOSPHERIC RETRIEVAL FOR SUPER-EARTHS: UNIQUELY CONSTRAINING THE ATMOSPHERIC COMPOSITION WITH TRANSMISSION SPECTROSCOPY  

SciTech Connect

We present a retrieval method based on Bayesian analysis to infer the atmospheric compositions and surface or cloud-top pressures from transmission spectra of exoplanets with general compositions. In this study, we identify what can unambiguously be determined about the atmospheres of exoplanets from their transmission spectra by applying the retrieval method to synthetic observations of the super-Earth GJ 1214b. Our approach to inferring constraints on atmospheric parameters is to compute their joint and marginal posterior probability distributions using the Markov Chain Monte Carlo technique in a parallel tempering scheme. A new atmospheric parameterization is introduced that is applicable to general atmospheres in which the main constituent is not known a priori and clouds may be present. Our main finding is that a unique constraint of the mixing ratios of the absorbers and two spectrally inactive gases (such as N{sub 2} and primordial H{sub 2}+ He) is possible if the observations are sufficient to quantify both (1) the broadband transit depths in at least one absorption feature for each absorber and (2) the slope and strength of the molecular Rayleigh scattering signature. A second finding is that the surface pressure or cloud-top pressure can be quantified if a surface or cloud deck is present at low optical depth. A third finding is that the mean molecular mass can be constrained by measuring either the Rayleigh scattering slope or the shapes of the absorption features, thus enabling one to distinguish between cloudy hydrogen-rich atmospheres and high mean molecular mass atmospheres. We conclude, however, that without the signature of molecular Rayleigh scattering-even with robustly detected infrared absorption features (>10{sigma})-there is no reliable way to tell from the transmission spectrum whether the absorber is a main constituent of the atmosphere or just a minor species with a mixing ratio of X{sub abs} < 0.1%. The retrieval method leads us to a conceptual picture of which details in transmission spectra are essential for unique characterizations of well-mixed exoplanet atmospheres.

Benneke, Bjoern; Seager, Sara, E-mail: bbenneke@mit.edu [Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)

2012-07-10T23:59:59.000Z

295

The SuperWASP wide-field exoplanetary transit survey: Candidates from Fields 23hr < RA < 03hr  

E-Print Network (OSTI)

Photometric transit surveys promise to complement the currently known sample of extra-solar planets by providing additional information on the planets and especially their radii. Here we present extra-solar planet (ESP) candidates from one such survey called, the Wide Angle Search for Planets (WASP) obtained with the SuperWASP wide-field imaging system. Observations were taken with SuperWASP-North located in La Palma during the April to October 2004 observing season. The data cover fields between 23hr and 03hr in RA at declinations above +12. This amounts to over $\\approx$400,000 stars with V magnitudes 8 to 13.5. For the stars brighter than 12.5, we achieve better than 1 percent photometric precision. Here we present 41 sources with low amplitude variability between $\\approx$ 1 and 10 mmag, from which we select 12 with periods between 1.2 and 4.4 days as the most promising extrasolar planet candidates. We discuss the properties of these ESP candidates, the expected fraction of transits recovered for our sample, and implications for the frequency and detection of hot-Jupiters.

D. J. Christian; D. L. Pollacco; I. Skillen; R. A. Street; F. P. Keenan; W. I. Clarkson; A. Collier Cameron; S. R. Kane; T. A. Lister; R. G. West; R. Enoch; A. Evans; A. Fitzsimmons; C. A. Haswell; C. Hellier; S. T. Hodgkin; K. Horne; J. Irwin; A. J. Norton; J. Osborne; R. Ryans; P. J. Wheatley; D. M. Wilson

2006-08-07T23:59:59.000Z

296

Review of Methods of Power-Spectrum Analysis as Applied to Super-Kamiokande Solar Neutrino Data  

E-Print Network (OSTI)

To help understand why different published analyses of the Super-Kamiokande solar neutrino data arrive at different conclusions, we have applied six different methods to a standardized problem. The key difference between the various methods rests in the amount of information that each processes. A Lomb-Scargle analysis that uses the mid times of the time bins and ignores experimental error estimates uses the least information. A likelihood analysis that uses the start times, end times, and mean live times, and takes account of the experimental error estimates, makes the greatest use of the available information. We carry out power-spectrum analyses of the Super-Kamiokande 5-day solar neutrino data, using each method in turn, for a standard search band (0 to 50 yr-1). For each method, we also carry out a fixed number (10,000) of Monte-Carlo simulations for the purpose of estimating the significance of the leading peak in each power spectrum. We find that, with one exception, the results of these calculations are compatible with those of previously published analyses. (We are unable to replicate Koshio's recent results.) We find that the significance of the peaks at 9.43 yr-1 and at 43.72 yr-1 increases progressively as one incorporates more information into the analysis procedure.

P. A. Sturrock

2004-08-02T23:59:59.000Z

297

Bulletin of Tibetology: Volume 22 Number 2 : Cover, contents, contributors  

E-Print Network (OSTI)

, INDIA ME TAG: DRUKPA TSESH! 11 July 1986 Price per capy R& 10/- 7/86 PRINTED At THE HIMAUNDIA PHOTO OFFSET NAM NAMROAD, GANCTOK PUBUSH.ED BY DIRECTOR, SlKlUMRBSEARCH INsmurE OF ftBETOLOGY, CANCTOIC - 737101 BllClUM . CONTENTS AGAIN:ON ATISA...

Namgyal Institute of Tibetology

1986-01-01T23:59:59.000Z

298

Nuclear Criticality as a Contributor to Gamma Ray Burst Events  

E-Print Network (OSTI)

Most gamma ray bursts are able to be explained using supernovae related phenomenon. Some measured results still lack compelling explanations and a contributory cause from nuclear criticality is proposed. This is shown to have general properties consistent with various known gamma ray burst properties. The galactic origin of fast rise exponential decay gamma ray bursts is considered a strong candidate for these types of events.

Robert Bruce Hayes

2013-01-15T23:59:59.000Z

299

Invasive plant species as potential bioenergy producers and carbon contributors.  

Science Conference Proceedings (OSTI)

Current cellulosic bioenergy sources in the United States are being investigated in an effort to reduce dependence on foreign oil and the associated risks to national security and climate change (Koh and Ghazoul 2008; Demirbas 2007; Berndes et al. 2003). Multiple sources of renewable plant-based material have been identified and include agricultural and forestry residues, municipal solid waste, industrial waste, and specifically grown bioenergy crops (Demirbas et al. 2009; Gronowska et al. 2009). These sources are most commonly converted to energy through direct burning, conversion to gas, or conversion to ethanol. Annual crops, such as corn (Zea Mays L.) and sorghum grain, can be converted to ethanol through fermentation, while soybean and canola are transformed into fatty acid methyl esters (biodiesel) by reaction with an alcohol (Demirbas 2007). Perennial grasses are one of the more viable sources for bioenergy due to their continuous growth habit, noncrop status, and multiple use products (Lewandowski el al. 2003). In addition, a few perennial grass species have very high water and nutrient use efficiencies producing large quantities of biomass on an annual basis (Dohleman et al. 2009; Grantz and Vu 2009).

Young, S.; Gopalakrishnan, G.; Keshwani, D. (Energy Systems); (Univ. of Nebraska)

2011-03-01T23:59:59.000Z

300

THE AGS-BASED SUPER NEUTRINO BEAM FACILITY CONCEPTUAL DESIGN REPORT  

Science Conference Proceedings (OSTI)

After more than 40 years of operation, the AGS is still at the heart of the Brookhaven hadron accelerator complex. This system of accelerators presently comprises a 200 MeV linac for the pre-acceleration of high intensity and polarized protons, two Tandem Van der Graaffs for the pre-acceleration of heavy ion beams, a versatile Booster that allows for efficient injection of all three types of beams into the AGS and, most recently, the two RHIC collider rings that produce high luminosity heavy ion and polarized proton collisions. For several years now, the AGS has held the world intensity record with more than 7 x 10{sup 13} protons accelerated in a single pulse. The requirements for the proton beam for the super neutrino beam are summarized and a schematic of the upgraded AGS is shown. Since the present number of protons per fill is already close to the required number, the upgrade is based on increasing the repetition rate and reducing beam losses (to avoid excessive shielding requirements and to maintain activation of the machine components at workable level). It is also important to preserve all the present capabilities of the AGS, in particular its role as injector to RHIC. The AGS Booster was built not only to allow the injection of any species of heavy ion into the AGS but to allow a fourfold increase of the AGS intensity. It is one-quarter the circumference of the AGS with the same aperture. However, the accumulation of four Booster loads in the AGS takes about 0.6 s, and is therefore not well suited for high average beam power operation. To minimize the injection time to about 1 ms, a 1.2 GeV linac will be used instead. This linac consists of the existing warm linac of 200 MeV and a new superconducting linac of 1.0 GeV. The multi-turn H{sup -} injection from a source of 30 mA and 720 {micro}s pulse width is sufficient to accumulate 9 x 10{sup 13} particle per pulse in the AGS[10]. The minimum ramp time of the AGS to full energy is presently 0.5 s; this must be upgraded to 0.2 s to reach the required repetition rate of 2.5 Hz. The required upgrade of the AGS power supply, the rf system, and other rate dependent accelerator issues is discussed. The design of the target/horn configuration is shown. The material selected for the proton target is a Carbon-Carbon composite. It is a 3-dimensional woven material that exhibits extremely low thermal expansion for temperatures up to 1000 C; for higher temperatures it responds like graphite. This property is important for greatly reducing the thermo-elastic stresses induced by the beam, thereby extending the life of the target. The target consists of a 80 cm long cylindrical rod of 12 mm diameter. The target intercepts a 2 mm rms proton beam of 10{sup 14} protons/pulse. The total energy deposited as heat in the target is 7.3 kJ with peak temperature rise of about 280 C. Heat will be removed from the target through forced convection of helium gas across its outside surface. The extracted proton beam uses an existing beamline at the AGS, but is then directed to a target station atop a constructed earthen hill. The target is followed by a downward slopping pion decay channel. This vertical arrangement keeps the target and decay pipe well above the water table in this area. The 11.3 degrees slope aims the neutrino beam at a water Cerenkov neutrino detector to be located in the Homestake mine at Lead, South Dakota. A 3-dimensional view of the beam transport line, target station, and decay tunnel is provided.

WENG,W.T.; DIWAN,M.; RAPARIA,D.

2004-10-08T23:59:59.000Z

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301

Super Models, Old King Coal II, & Civil Disobedience For fellow technocrats: "Climate simulations for 1880-2003 with GISS modelE", to appear soon  

E-Print Network (OSTI)

Super Models, Old King Coal II, & Civil Disobedience Model: For fellow technocrats: "Climate" was a guise, using prurient interest to gain attention. Sorry! "Old King Coal II" and "Civil Disobedience" are accurate headings. Old King Coal II: Thanks for comments/suggestions re my "Old King Coal" e-mail. Main

Hansen, James E.

302

Comparison of the Recently proposed Super Marx Generator Approach to Thermonuclear Ignition with the DT Laser Fusion-Fission Hybrid Concept by the Lawrence Livermore National Laboratory  

E-Print Network (OSTI)

The recently proposed Super Marx generator pure deuterium micro-detonation ignition concept is compared to the Lawrence Livermore National Ignition Facility (NIF) Laser DT fusion-fission hybrid concept (LiFE) [1]. In a Super Marx generator a large number of ordinary Marx generators charge up a much larger second stage ultra-high voltage Marx generator, from which for the ignition of a pure deuterium micro-explosion an intense GeV ion beam can be extracted. A typical example of the LiFE concept is a fusion gain of 30, and a fission gain of 10, making up for a total gain of 300, with about 10 times more energy released into fission as compared to fusion. This means a substantial release of fission products, as in fusion-less pure fission reactors. In the Super Marx approach for the ignition of a pure deuterium micro-detonation a gain of the same magnitude can in theory be reached [2]. If feasible, the Super Marx generator deuterium ignition approach would make lasers obsolete as a means for the ignition of ther...

Winterberg, Friedwardt

2009-01-01T23:59:59.000Z

303

Power-Spectrum Analyses of Super-Kamiokande Solar Neutrino Data: Variability and its Implications for Solar Physics and Neutrino Physics  

E-Print Network (OSTI)

There have been conflicting claims as to whether or not power-spectrum analysis of the Super-Kamiokande solar neutrino data yields evidence of variability. Comparison of these claims is complicated by the fact that the relevant articles may use different datasets, different methods of analysis, and different procedures for significance estimation. The purpose of this article is to clarify the role of power spectrum analysis. To this end, we analyze only the Super-Kamiokande 5-day dataset, and we use a standard procedure for significance estimation proposed by the Super-Kamiokande collaboration. We then analyze this dataset, with this method of significance estimation, using six methods of power spectrum analysis. We find that the significance of the principal peak in the power spectrum (that at 9.43 yr-1with a depth of modulation of 7%) shows a clear correlation with the amount and relevance of the information being processed, as would be expected if there were a real signal in the data. The significance level reaches 99.3% for one method of analysis. We discuss, in terms of sub-dominant processes, possible neutrino-physics interpretations of the apparent variability of the Super-Kamiokande measurements, and we suggest steps that could be taken to resolve the question of variability of the solar neutrino flux.

P. A. Sturrock; D. O. Caldwell; J. D. Scargle; M. S. Wheatland

2005-01-21T23:59:59.000Z

304

The Superconducting Horizontal Bend Magnet for the Jefferson Lab's 11 GeV/c Super High Momentum Spectrometer  

SciTech Connect

A collaboration between NSCL and Jlab has developed the reference design and coil winding for Jlab's Super High Momentum Spectrometer (SHMS) horizontal bend magnet. A warm iron ??C?? type superferric dipole magnet will bend the 12 GeV/c particles horizontally by 3?? to allow the SHMS to reach angles as low as 5.5??. This requires an integral field strength of up to 2.1 T.m. The major challenges are the tight geometry, high and unbalanced forces and a required low fringe field in primary beam path. A coil design based on flattened SSC Rutherford cable that provides a large current margin and commercially available fiberglass prepreg epoxy tape has been developed. A complete test coil has been wound and will be cold tested. This paper present the modified magnet design includes coil forces, coil restraint system and fringe field. In addition, coil properties, quench calculations and the full mechanical details are also presented.

S. Chouhan, J. DeKamp, A. Zeller, P. Brindza, S. Lassiter, M. Fowler, E. Sun

2010-06-01T23:59:59.000Z

305

Power-spectrum analysis of Super-Kamiokande solar neutrino data, taking into account asymmetry in the error estimates  

E-Print Network (OSTI)

The purpose of this article is to carry out a power-spectrum analysis (based on likelihood methods) of the Super-Kamiokande 5-day dataset that takes account of the asymmetry in the error estimates. Whereas the likelihood analysis involves a linear optimization procedure for symmetrical error estimates, it involves a nonlinear optimization procedure for asymmetrical error estimates. We find that for most frequencies there is little difference between the power spectra derived from analyses of symmetrized error estimates and from asymmetrical error estimates. However, this proves not to be the case for the principal peak in the power spectra, which is found at 9.43 yr-1. A likelihood analysis which allows for a "floating offset" and takes account of the start time and end time of each bin and of the flux estimate and the symmetrized error estimate leads to a power of 11.24 for this peak. A Monte Carlo analysis shows that there is a chance of only 1% of finding a peak this big or bigger in the frequency band 1 - 36 yr-1 (the widest band that avoids artificial peaks). On the other hand, an analysis that takes account of the error asymmetry leads to a peak with power 13.24 at that frequency. A Monte Carlo analysis shows that there is a chance of only 0.1% of finding a peak this big or bigger in that frequency band 1 - 36 yr-1. From this perspective, power spectrum analysis that takes account of asymmetry of the error estimates gives evidence for variability that is significant at the 99.9% level. We comment briefly on an apparent discrepancy between power spectrum analyses of the Super-Kamiokande and SNO solar neutrino experiments.

P. A. Sturrock; J. D. Scargle

2006-01-30T23:59:59.000Z

306

PLANETESIMAL FORMATION AT THE BOUNDARY BETWEEN STEADY SUPER/SUB-KEPLERIAN FLOW CREATED BY INHOMOGENEOUS GROWTH OF MAGNETOROTATIONAL INSTABILITY  

Science Conference Proceedings (OSTI)

We have studied formation of planetesimals at a radial pressure bump in a protoplanetary disk created by radially inhomogeneous magnetorotational instability (MRI), through three-dimensional resistive MHD simulations including dust particles. In our previous papers, we showed that the inhomogeneous MRI developing in non-uniform structure of magnetic field or magnetic resistivity can transform the local gas flow in the disk to a quasi-steady state with local rigid rotation that is no longer unstable against the MRI. Since the outer part of the rigid rotation is super-Keplerian flow, a quasi-static pressure bump is created and dust concentration is expected there. In this paper, we perform simulations of the same systems, adding dust particles that suffer gas drag and modulate gas flow via the back-reaction of the gas drag (dust drag). We use {approx}O(10{sup 7}) super-particles, each of which represents {approx}O(10{sup 6})-O(10{sup 7}) dust particles with sizes of centimeter to meter. We have found that the dust drag suppresses turbulent motion to decrease the velocity dispersion of the dust particles while it broadens the dust concentrated regions to limit peaky dust concentration, compared with the simulation without the dust drag. We found that the positive effect for the gravitational instability (GI), reduction in the velocity dispersion, dominates over the negative one, suppression in particle concentration. For meter-size particles with the friction time {tau}{sub f} {approx_equal} 1/{Omega}, where {Omega} is Keplerian frequency, the GI of the dust particles that may lead to planetesimal formation is expected. For such a situation, we further introduced the self-gravity of dust particles to the simulation to demonstrate that several gravitationally bound clumps are actually formed. Through analytical arguments, we found that planetesimal formation from meter-sized dust particles is possible at {approx}5 AU, if dust spatial density is a few times larger than that in the minimum mass solar nebula.

Kato, M. T.; Ida, S. [Department of Earth and Planetary Science, Tokyo Institute of Technology, Ookayama 2-1-12-I2-10, Meguro-ku, Tokyo (Japan); Fujimoto, M., E-mail: ida@geo.titech.ac.jp [Institute of Space and Astronomical Science, Japan Aerospace Exploration Agency, Yoshinodai 3-1-1 Sagamihara, Kanagawa (Japan)

2012-03-01T23:59:59.000Z

307

WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE  

E-Print Network (OSTI)

We have detected radial-velocity variations in two objects that were identified as being likely host stars of transiting exoplanets in the 2004 SuperWASP wide-field transit survey. Using the newly-commissioned radial-velocity spectrograph SOPHIE at the Observatoire de Haute-Provence, we found that both objects exhibit reflex orbital radial-velocity variations with amplitudes characteristic of planetary-mass companions and in-phase with the photometric orbits. Line-bisector studies rule out faint blended binaries as the cause of either the radial-velocity variations or the transits. We perform preliminary spectral analyses of the host stars, which together with their radial-velocity variations and fits to the transit light curves, yield estimates of the planetary masses and radii. WASP-1b and WASP-2b have orbital periods of 2.52 and 2.15 days respectively. Given mass estimates for their F7V and K1V primaries we derive planet masses 0.80 to 0.98 and 0.81 to 0.95 times that of Jupiter respectively. WASP-1b appea...

Cameron, A C; Hbrard, G; Maxted, P; Pollacco, D; Pont, F; Skillen, I; Smalley, B; Street, R A; West, R G; Wilson, D M; Aigrain, S; Christian, D J; Clarkson, W I; Enoch, B; Evans, A; Fitzsimmons, A; Gillon, M; Haswell, C A; Hebb, L; Hellier, C; Hodgkin, S T; Horne, K; Irwin, J; Kane, S R; Keenan, F P; Loeillet, B; Lister, T A; Mayor, M; Moutou, C; Norton, A J; Osborne, J; Parley, N; Queloz, D; Ryans, R; Triaud, A; Udry, S; Wheatley, P J

2006-01-01T23:59:59.000Z

308

The Variation of the Solar Neutrino Fluxes over Time in the Homestake, GALLEX(GNO) and Super-Kamiokande Experiments  

E-Print Network (OSTI)

Using the records of the fluxes of solar neutrinos from the Homestake, GALLEX (GNO), and Super-Kamiokande experiments, their statistical analyses were performed to search for whether there existed a time variation of these fluxes. The results of the analysis for the three experiments indicate that these fluxes are varying quasi-biennially. This means that both efficiencies of the initial p-p and the pp-III reactions of the proton-proton chain are varying quasi-biennially together with a period of about 26 months. Since this time variation prospectively generated by these two reactions strongly suggests that the efficiency of the proton-proton chain as the main energy source of the Sun has a tendency to vary quasi-biennially due to some chaotic or non-linear process taking place inside the gravitationally stabilized solar fusion reactor. It should be, however, remarked that, at the present moment, we have no theoretical reasoning to resolve this mysterious result generally referred to as the quasi-biennial periodicity in the time variation of the fluxes of solar neutrinos. There is an urgent need to search for the reason why such a quasi-biennial periodicity is caused through some physical process as related to nuclear fusion deep inside the Sun.

K. Sakurai; H. J. Haubold; T. Shirai

2011-11-22T23:59:59.000Z

309

Review of project definition studies of possible on-site uses of superconducting super collider assets and facilities. Final report  

Science Conference Proceedings (OSTI)

This document reports on the results of a peer review and evaluation of studies made of potential uses of assets from the terminated Superconducting Super Collider (SSC) project. These project definition studies focused on nine areas of use of major assets and facilities at the SSC site near Waxahachie, Texas. The studies were undertaken as part of the effort to maximize the value of the investment made in the SSC and were supported by two sets of grants, one to the Texas National Research Laboratory Commission (TNRLC) and the second to various universities and other institutions for studies of ideas raised by a public call for expressions of interest. The Settlement Agreement, recently signed by the Department of Energy (DOE) and TNRLC, provides for a division of SSC property. As part of the goal of maximizing the value of the SSC investment, the findings contained in this report are thus addressed to officials in both the Department and TNRLC. In addition, this review had several other goals: to provide constructive feedback to those doing the studies; to judge the benefits and feasibility (including funding prospects) of the projects studied; and to help worthy projects become reality by matching projects with possible funding sources.

NONE

1994-12-01T23:59:59.000Z

310

Atmospheric neutrino oscillation analysis with sub-leading effects in Super-Kamiokande I, II, and III  

E-Print Network (OSTI)

We present a search for non-zero theta_{13} and deviations of sin^2 theta_{23} from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande -I, -II, and -III. No distortions of the neutrino flux consistent with non-zero theta_{13} are found and both neutrino mass hierarchy hypotheses are in agreement with the data. The data are best fit at Delta m^2 = 2.1 x 10^-3 eV^2, sin^2 theta_{13} = 0.0, and sin^2 theta_{23} =0.5. In the normal (inverted) hierarchy theta_{13} and Delta m^2 are constrained at the one-dimensional 90% C.L. to sin^2 theta_{13} < 0.04 (0.09) and 1.9 (1.7) x 10^-3 < Delta m^2 < 2.6 (2.7) x 10^-3 eV^2. The atmospheric mixing angle is within 0.407 <= sin^2 theta_{23} <= 0.583 at 90% C.L.

Super-Kamiokande Collaboration; :; R. Wendell; C. Ishihara; K. Abe; Y. Hayato; T. Iida; M. Ikeda; K. Iyogi; J. Kameda; K. Kobayashi; Y. Koshio; Y. Kozuma; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Ogawa; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; Y. Takeuchi; K. Ueno; K. Ueshima; H. Watanabe; S. Yamada; T. Yokozawa; S. Hazama; H. Kaji; T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; M. R. Vagins; F. Dufour; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; W. Wang; M. Goldhaber; K. Bays; D. Casper; J. P. Cravens; W. R. Kropp; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. Albert; M. Fechner; K. Scholberg; C. W. Walter; S. Tasaka; J. G. Learned; S. Matsuno; Y. Watanabe; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; H. Nishino; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; A. Minamino; T. Nakaya; Y. Fukuda; Y. Itow; G. Mitsuka; T. Tanaka; C. K. Jung; G. Lopez; C. McGrew; C. Yanagisawa; N. Tamura; H. Ishino; A. Kibayashi; S. Mino; T. Mori; M. Sakuda; H. Toyota; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; T. Ishizuka; H. Okazawa; Y. Choi; K. Nishijima; Y. Yokosawa; M. Koshiba; M. Yokoyama; Y. Totsuka; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; E. Thrane; R. J. Wilkes

2010-02-18T23:59:59.000Z

311

Cryogenic system design of 11 GEV/C super high momentum spectrometer superconducting magnets at Jefferson Lab  

SciTech Connect

The design of the cryogenic system for the 11 GeV/c Super High Momentum Spectrometer (SHMS) is presented. A description of the cryogenic control reservoir and the cryogenic transfer line is given. Details of the cryogenic control reservoirs, cryogenic transfer lines, and pressure piping are summarized. Code compliance is ensured through following the requirements of the ASME Pressure Vessel Code and Pressure Piping Code. An elastic-plastic-analysis-based combined safety factor approach is proposed to meet the low stress requirement of ASME 2007 Section VIII, Division 2 so that Charpy V-notch (CVN) impact testing can be avoided through analysis. Material toughness requirements in ASME 2007 Section VIII, Division 2 are adopted as CVN impact testing rules of stainless steel 304 piping at 4.2 K and 77 K. A formula-based combined safety factor approach for pressure piping is also proposed to check whether the impact testing can be avoided due to low stress. Analysis and calculation have shown that no CVN impact testing of base metal and heat affected zones is required for the helium reservoir, nitrogen reservoir, and their relevant piping. Total heat loads to liquid helium and liquid nitrogen are studied also. The total heat load to LHe for SHMS is estimated to be 137 W, and the total load to LN2 is calculated to be 420 W.

Eric Sun, Paul Brindza, Steven Lassister, Mike Fowler

2012-07-01T23:59:59.000Z

312

Solar Neutrino Rates, Spectrum, and its Moments : an MSW Analysis in the Light of Super-Kamiokande Results  

E-Print Network (OSTI)

We re-examine MSW solutions of the solar neutrino problem in a two flavor scenario taking (a) the results on total rates and the electron energy spectrum from the 1117-day SuperKamiokande (SK) data and (b) those on total rates from the Chlorine and Gallium experiments. We find that the SMA solution gives the best fit to the total rates data from the different experiments. One new feature of our analysis is the use of the moments of the SK electron spectrum in a $\\chi^2$ analysis. The best-fit to the moments is broadly in agreement with that obtained from a direct fit to the spectrum data and prefers a $\\Delta m^2$ comparable to the SMA fit to the rates but the required mixing angle is larger. In the combined rate and spectrum analysis, apart from varying the normalization of the $^8$B flux as a free parameter and determining its best-fit value we also obtain the best-fit parameters when correlations between the rates and the spectrum data are included and the normalization of the $^8$B flux held fixed at its SSM value. We observe that the correlations between the rates and spectrum data are important and the goodness of fit worsens when these are included. In either case, the best-fit lies in the LMA region.

Srubabati Goswami; Debasish Majumdar; Amitava Raychaudhuri

2000-03-16T23:59:59.000Z

313

Broadband Transmission Spectroscopy of the super-Earth GJ 1214b suggests a Low Mean Molecular Weight Atmosphere  

E-Print Network (OSTI)

We used WIRCam on CFHT to observe four transits of the super-Earth GJ 1214b in the near-infrared. For each transit we observed in two bands nearly-simultaneously by rapidly switching the WIRCam filter wheel back and forth for the duration of the observations. By combining all our J-band (~1.25 microns) observations we find a transit depth in this band of 1.338\\pm0.013% - a value consistent with the optical transit depth reported by Charbonneau and collaborators. However, our best-fit combined Ks-band (~2.15 microns) transit depth is deeper: 1.438\\pm0.019%. Formally our Ks-band transits are deeper than the J-band transits observed simultaneously by a factor of 1.072\\pm0.018 - a 4-sigma discrepancy. The most straightforward explanation for our deeper Ks-band depth is a spectral absorption feature from the limb of the atmosphere of the planet; for the spectral absorption feature to be this prominent the atmosphere of GJ 1214b must have a large scale height and a low mean molecular weight. That is, it would have ...

Croll, Bryce; Jayawardhana, Ray; Kempton, Eliza Miller-Ricci; Fortney, Jonathan J; Murray, Norman; Neilson, Hilding

2011-01-01T23:59:59.000Z

314

Review of project definition studies of possible on-site uses of superconducting super collider assets and facilities  

SciTech Connect

This document reports on the results of a peer review and evaluation of studies made of potential uses of assets from the terminated Superconducting Super Collider (SSC) project. These project definition studies focused on nine areas of use of major assets and facilities at the SSC site near Waxahachie, Texas. The studies were undertaken as part of the effort to maximize the value of the investment made in the SSC and were supported by two sets of grants, one to the Texas National Research Laboratory Commission (TNRLC) and the second to various universities and other institutions for studies of ideas raised by a public call for expressions of interest. The Settlement Agreement, recently signed by the Department of Energy (DOE) and TNRLC, provides for a division of SSC property. As part of the goal of maximizing the value of the SSC investment, the findings contained in this report are thus addressed to officials in both the Department and TNRLC. In addition, this review had several other goals: to provide constructive feedback to those doing the studies; to judge the benefits and feasibility (including funding prospects) of the projects studied; and to help worthy projects become reality by matching projects with possible funding sources.

1994-12-01T23:59:59.000Z

315

REVISITING {rho}{sup 1} CANCRI e: A NEW MASS DETERMINATION OF THE TRANSITING SUPER-EARTH  

SciTech Connect

We present a mass determination for the transiting super-Earth {rho}{sup 1} Cancri e based on nearly 700 precise radial velocity (RV) measurements. This extensive RV data set consists of data collected by the McDonald Observatory planet search and published data from Lick and Keck observatories. We obtained 212 RV measurements with the Tull Coude Spectrograph at the Harlan J. Smith 2.7 m Telescope and combined them with a new Doppler reduction of the 131 spectra that we have taken in 2003-2004 with the High-Resolution Spectrograph (HRS) at the Hobby-Eberly Telescope for the original discovery of {rho}{sup 1} Cancri e. Using this large data set we obtain a five-planet Keplerian orbital solution for the system and measure an RV semi-amplitude of K = 6.29 {+-} 0.21 m s{sup -1} for {rho}{sup 1} Cnc e and determine a mass of 8.37 {+-} 0.38 M {sub Circled-Plus }. The uncertainty in mass is thus less than 5%. This planet was previously found to transit its parent star, which allowed them to estimate its radius. Combined with the latest radius estimate from Gillon et al., we obtain a mean density of {rho} = 4.50 {+-} 0.20 g cm{sup -3}. The location of {rho}{sup 1} Cnc e in the mass-radius diagram suggests that the planet contains a significant amount of volatiles, possibly a water-rich envelope surrounding a rocky core.

Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Barnes, Stuart I. [McDonald Observatory, University of Texas at Austin, Austin, TX 78712 (United States); Robertson, Paul; Brugamyer, Erik J.; Caldwell, Caroline; Gullikson, Kevin [Department of Astronomy, University of Texas at Austin, Austin, TX 78712 (United States); Wittenmyer, Robert A., E-mail: mike@astro.as.utexas.edu [Department of Astrophysics and Optics, School of Physics, University of New South Wales, Sydney (Australia)

2012-11-01T23:59:59.000Z

316

WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE  

E-Print Network (OSTI)

We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219-0005465 (GSC 02265-00107 = WASP-1) and USNO-B1.0 0964-0543604 (GSC 00522-01199 = WASP-2). Both stars were identified as being likely host stars of transiting exoplanets in the 2004 SuperWASP wide-field transit survey. Using the newly-commissioned radial-velocity spectrograph SOPHIE at the Observatoire de Haute-Provence, we found that both objects exhibit reflex orbital radial-velocity variations with amplitudes characteristic of planetary-mass companions and in-phase with the photometric orbits. Line-bisector studies rule out faint blended binaries as the cause of either the radial-velocity variations or the transits. We perform preliminary spectral analyses of the host stars, which together with their radial-velocity variations and fits to the transit light curves, yield estimates of the planetary masses and radii. WASP-1b and WASP-2b have orbital periods of 2.52 and 2.15 days respectively. Given mass estimates for their F7V and K1V primaries we derive planet masses 0.80 to 0.98 and 0.81 to 0.95 times that of Jupiter respectively. WASP-1b appears to have an inflated radius of at least 1.33 R_Jup, whereas WASP-2b has a radius in the range 0.65 to 1.26 R_Jup.

A. Collier Cameron; F. Bouchy; G. Hebrard; P. Maxted; D. Pollacco; F. Pont; I. Skillen; B. Smalley; R. A. Street; R. G. West; D. M. Wilson; S. Aigrain; D. J. Christian; W. I. Clarkson; B. Enoch; A. Evans; A. Fitzsimmons; M. Fleenor; M. Gillon; C. A. Haswell; L. Hebb; C. Hellier; S. T. Hodgkin; K. Horne; J. Irwin; S. R. Kane; F. P. Keenan; B. Loeillet; T. A. Lister; M. Mayor; C. Moutou; A. J. Norton; J. Osborne; N. Parley; D. Queloz; R. Ryans; A. H. M. J. Triaud; S. Udry; P. J. Wheatley

2006-09-25T23:59:59.000Z

317

RAPID COOLING OF THE NEUTRON STAR IN THE QUIESCENT SUPER-EDDINGTON TRANSIENT XTE J1701-462  

SciTech Connect

We present Rossi X-Ray Timing Explorer and Swift observations made during the final three weeks of the 2006-2007 outburst of the super-Eddington neutron star (NS) transient XTE J1701-462, as well as Chandra and XMM-Newton observations covering the first {approx_equal}800 days of the subsequent quiescent phase. The source transitioned quickly from active accretion to quiescence, with the luminosity dropping by over 3 orders of magnitude in {approx_equal}13 days. The spectra obtained during quiescence exhibit both a thermal component, presumed to originate in emission from the NS surface, and a non-thermal component of uncertain origin, which has shown large and irregular variability. We interpret the observed decay of the inferred effective surface temperature of the NS in quiescence as the cooling of the NS crust after having been heated and brought out of thermal equilibrium with the core during the outburst. The interpretation of the data is complicated by an apparent temporary increase in temperature {approx_equal}220 days into quiescence, possibly due to an additional spurt of accretion. We derive an exponential decay timescale of {approx_equal}120{sup +30}{sub -20} days for the inferred temperature (excluding observations affected by the temporary increase). This short timescale indicates a highly conductive NS crust. Further observations are needed to confirm whether the crust is still slowly cooling or has already reached thermal equilibrium with the core at a surface temperature of {approx_equal}125 eV. The latter would imply a high equilibrium bolometric thermal luminosity of {approx_equal}5 x 10{sup 33}ergs{sup -1} for an assumed distance of 8.8 kpc.

Fridriksson, Joel K.; Lewin, Walter H. G. [Department of Physics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States); Homan, Jeroen [MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States); Wijnands, Rudy; Altamirano, Diego; Degenaar, Nathalie [Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Science Park 904, 1098 XH, Amsterdam (Netherlands); Mendez, Mariano [Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV, Groningen (Netherlands); Cackett, Edward M. [Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109 (United States); Brown, Edward F. [Department of Physics and Astronomy, National Superconducting Cyclotron Laboratory, and Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI 48824 (United States); Belloni, Tomaso M., E-mail: joelkf@mit.ed [INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate (Italy)

2010-05-01T23:59:59.000Z

318

THE SUPER LITHIUM-RICH RED GIANT RAPID ROTATOR G0928+73.2600: A CASE FOR PLANET ACCRETION?  

Science Conference Proceedings (OSTI)

We present the discovery of a super lithium-rich K giant star, G0928+73.2600. This red giant (T {sub eff} = 4885 K and log g = 2.65) is a fast rotator with a projected rotational velocity of 8.4 km s{sup -1} and an unusually high lithium abundance of A(Li) = 3.30 dex. Although the lack of a measured parallax precludes knowing the exact evolutionary phase, an isochrone-derived estimate of its luminosity places the star on the Hertzsprung-Russell diagram in a location that is not consistent with either the red bump on the first ascent of the red giant branch or with the second ascent on the asymptotic giant branch, the two evolutionary stages where lithium-rich giant stars tend to cluster. Thus, even among the already unusual group of lithium-rich giant stars, G0928+73.2600 is peculiar. Using {sup 12}C/{sup 13}C as a tracer for mixing-more mixing leads to lower {sup 12}C/{sup 13}C-we find {sup 12}C/{sup 13}C = 28, which is near the expected value for standard first dredge-up mixing. We can therefore conclude that 'extra' deep mixing has not occurred. Regardless of the ambiguity of the evolutionary stage, the extremely large lithium abundance and the rotational velocity of this star are unusual, and we speculate that G0928+73.2600 has been enriched in both lithium and angular momentum from a sub-stellar companion.

Carlberg, Joleen K.; Majewski, Steven R.; Rood, Robert T. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325 (United States); Smith, Verne V.; Cunha, Katia, E-mail: jkm9n@virginia.ed [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States)

2010-11-01T23:59:59.000Z

319

Superdeformed nuclei: Shells-vs-liquid drop, pairing-vs-thermal excitations, triaxial-vs-octupole shapes, super-superdeformation  

SciTech Connect

Mechanisms influencing the behavior of superdeformed nuclei are studied using several well established nuclear structure techniques. In particular: pairing, thermal excitation, shell and liquid-drop mechanisms are considered. The effects of quadrupole and hexadecapole (both axial and non-axial), and octupole deformation degrees of freedom are studied. Most of the results are illustrated using the case of /sup 152/Dy nucleus in which a superdeformed band extending up to I approx. 60 h-bar has been found in experiment. Some comparisons between /sup 152/Dy and the nuclei in the neighborhood are given. Calculations show that pairing ''de-aligns'' typically 6 to 8 units of angular momentum, as compared to the corresponding rigid rotation. This takes place for spins extending up to the highest limit, and thus diminishes the effective moments of inertia. Predicted octupole shape susceptibility is extremely large, significantly stronger than the susceptibilities known in the ground-states of many Actinide nuclei. Consequences of this result for the near-constancy of the dynamical moments of inertia are pointed out. Nuclear level densities calculated in function of spin, excitation energy and deformation explain the ''unusual'' side feeding pattern of the /sup 152/Dy superdeformed states. Predictions of super-superdeformed nuclear states (axis ratio varying between 2:1 and 3:1 or more) are given and exemplified for Erbium nuclei. Finally, the problem of superdeformation stability and the influence of increased collective inertia on a barrier penetration are examined. An analytical expression for the effective inertia parameter is obtained and its derivation outlined. 35 refs., 9 figs.

Dudek, J.

1987-01-01T23:59:59.000Z

320

Abstract Nuclear Instruments and Methods in Physics Research A 559 (2006) 411413 The SuperCDMS proposal for dark matter detection  

E-Print Network (OSTI)

Presently the CDMS-II collaborations Weakly Interacting Massive Particle (WIMP) search at the Soudan Underground Laboratory sets the most stringent exclusion limits of any WIMP cold dark matter direct-detection experiment. To extend our reach further, to WIMP-nucleon cross-sections in the range 10 46 10 44 cm2, we propose SuperCDMS, which would take advantage of a very deep site. One promising site is the recently approved SNOLab facility in Canada. In this paper we will present our overall program and focus on

D. S. Akerib A; M. J. Attisha B; C. N. Bailey A; L. Baudis C; D. A. Bauer D; J. Cooley E; M. B. Crisler D; P. Cushman G; P. Denes H; M. R. Dragowsky A; L. Duong G; D. Holmgren D; M. E. Huber K; K. D. Irwin L; A. Lu H; R. Mahapatra F; P. Meunier I; N. Mirabolfathi I; H. Nelson F; R. W. Ogburn E; E. Ramberg D; A. Reisetter G; T. Saab C; B. Sadoulet H; Er F; D. N. Seitz I; B. Serfass I; R. W. Schnee A; K. M. Sundqvist I; J. -p. F. Thompson B; S. Yellin F; J. Yoo D; B. A. Young M

2005-01-01T23:59:59.000Z

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321

Cold collisions of highly rotationally excited CO{sub 2} with He: The prospects for cold chemistry with super-rotors  

SciTech Connect

Building on recent advances in ultrafast lasers and methods to slow molecules, an experiment is proposed to produce translationally cold CO{sub 2} super-rotors (j{approx}200) by combining an optical centrifuge with helium-buffer-gas cooling. Quantum mechanical calculations of the complex scattering length for He-CO{sub 2} collisions demonstrate that the efficiency of rotational quenching decreases rapidly with increasing rotational excitation j in the ultracold regime. Extrapolating to helium cryogenic temperatures, rotational quenching is predicted to remain inefficient up to {approx}1 K, allowing for the possible creation of a beam of translationally cold, rotationally hot molecules.

Al-Qady, W. H.; Forrey, R. C.; Yang, B. H.; Stancil, P. C.; Balakrishnan, N. [Department of Physics and Astronomy and the Center for Simulational Physics, University of Georgia, Athens, Georgia 30602 (United States); Department of Physics, The Pennsylvania State University, Berks Campus, Reading, Pennsylvania 19610 (United States); Department of Physics and Astronomy and the Center for Simulational Physics, University of Georgia, Athens, Georgia 30602 (United States); Department of Chemistry, University of Nevada-Las Vegas, Las Vegas, Nevada 89154 (United States)

2011-11-15T23:59:59.000Z

322

Supercomputers: Super-polluters?  

E-Print Network (OSTI)

energy efficiency while maintaining computing performance and reliability requires effective systems integration

Mills, Evan

2008-01-01T23:59:59.000Z

323

SUPER HARD SURFACED POLYMERS  

SciTech Connect

High energy ion beam surface treatments were applied to a selected group of polymers. Of the six materials in the present study, four were thermoplastics (polycarbonate, polyethylene, polyethylene terephthalate, and polystyrene) and two were thermosets (epoxy and polyimide). The particular epoxy evaluated in this work is one of the resins used in formulating fiber reinforced composites for military helicopter blades. Measures of mechanical properties of the near surface regions were obtained by nanoindentation hardness and pin on disk wear. Attempts were also made to measure erosion resistance by particle impact. All materials were hardness tested. Pristine materials were very soft, having values in the range of approximately 0.1 to 0.5 GPa. Ion beam treatment increased hardness by up to 50 times compared to untreated materials. For reference, all materials were hardened to values higher than those typical of stainless steels. Wear tests were carried out on three of the materials, PET, PI and epoxy. On the ion beam treated epoxy no wear could be detected, whereas the untreated material showed significant wear.

Mansur, Louis K [ORNL; Bhattacharya, R [UES, Incorporated, Dayton, OH; Blau, Peter Julian [ORNL; Clemons, Art [ORNL; Eberle, Cliff [ORNL; Evans, H B [UES, Incorporated, Dayton, OH; Janke, Christopher James [ORNL; Jolly, Brian C [ORNL; Lee, E H [Consultant, Milpitas, CA; Leonard, Keith J [ORNL; Trejo, Rosa M [ORNL; Rivard, John D [ORNL

2010-01-01T23:59:59.000Z

324

Supercomputers: Super-polluters?  

E-Print Network (OSTI)

and controlling operating cost, energy efficiency has been anew levels of energy efficiency and first- cost savings.and Energy Efficiency Survey. ranges of environmental conditions setby ASHRAE represents a low cost

Mills, Evan

2008-01-01T23:59:59.000Z

325

Supercomputers: Super-polluters?  

E-Print Network (OSTI)

where petaflop high-performance computing (HPC) systems areJournal of High Performance Computing Applications (Together Efficient high-performance computing requires not

Mills, Evan

2008-01-01T23:59:59.000Z

326

Synthesis of super-dense phase of aluminum under extreme pressure and temperature conditions created by femtosecond laser pulses in sapphire  

SciTech Connect

We describe synthesis of a new super-dense phase of aluminum under extreme pressure and temperature conditions created by laser-induced microexplosions in sapphire. Micro explosions in sub-micrometer sized regions of sapphire were induced by tightly-focused femtosecond laser pulses with a temporal length of {approx} 100 fs and an energy of {approx} 100 nJ. Fast, explosive expansion of photogenerated high-density plasma created strong heating and pressure transients with peak temperature and pressure of {approx} 105 K and 10 TPa, respectively. Partial decomposition of sapphire in the shock-compressed sapphire led to formation of nanocrystalline bcc-Al phase, which is different from ambient fcc-Al phase, and was permanently preserved by fast quenching. The existence of super-dense bcc-Al phase was confirmed using X-ray diffraction technique. This is the first observation of bcc-Al phase, which so far has been only predicted theoretically, and a demonstration that laser-induced micro explosions technique enables simple, safe and cost-efficient access to extreme pressures and temperatures without the tediousness typical to traditional techniques that use diamond anvil cells, gas guns, explosives, or megajoule-class lasers.

Mizeikis, Vygantas; Vailionis, Arturas; Gamaly, Eugene G.; Yang, Wenge; Rode, Andrei V.; Juodkazis, Saulius (Swinburne); (Shizuoka); (Stanford); (CIW); (ANU)

2012-06-26T23:59:59.000Z

327

Disbursement of $65 million to the State of Texas for construction of a Regional Medical Technology Center at the former Superconducting Super Collider Site, Waxahachie, Texas  

SciTech Connect

As part of a settlement agreement between the US DOE and the State of Texas, DOE proposes to transfer $65 million of federal funds to the Texas National Research Laboratory Commission (TNLRC) for construction of the Regional Medical Technology Center (RMTC) to be located in Ellis County, Texas. The RMTC would be a state-of-the-art medical facility for proton cancer therapy, operated by the State of Texas in conjunction with the University of Texas Southwestern Medical Center. The RMTC would use the linear accelerator assets of the recently terminated DOE Superconducting Super Collider Project to accelerate protons to high energies for the treatment of cancer patients. The current design provides for treatment areas, examination rooms, support laboratories, diagnostic imaging equipment, and office space as well as the accelerators (linac and synchrotron) and beam steering and shaping components. The potential environmental consequences of the proposed action are expected to be minor.

NONE

1995-05-01T23:59:59.000Z

328

Closure Report for Corrective Action Unit 118: Area 27 Super Kukla Facility, Nevada Test Site, Nevada with ROTC 1, Revision 0  

SciTech Connect

This CR provides documentation and justification for the closure of CAU 118 without further corrective action. This justification is based on process knowledge and the results of the investigative and closure activities conducted in accordance with the CAU 118 SAFER Plan: Streamlined Approach for Environmental Restoration (SAFER) Plan for CAU 118: Area 27 Super Kukla Facility, Nevada Test Site, Nevada (NNSA/NSO, 2006). The SAFER Plan provides information relating to site history as well as the scope and planning of the investigation. This CR also provides the analytical and radiological survey data to confirm that the remediation goals were met as specified in the CAU 118 SAFER Plan (NNSA/NSO, 2006). The Nevada Division of Environmental Protection (NDEP) approved the CAU 118 SAFER Plan (Murphy, 2006), which recommends closure in place with use restrictions (URs).

Mark Burmeister

2007-09-01T23:59:59.000Z

329

Conceptual design report for a superconducting coil suitable for use in the large solenoid detector at the SSC (Superconducting Super Collider)  

Science Conference Proceedings (OSTI)

The conceptual design of a large superconducting solenoid suitable for a magnetic detector at the Superconducting Super Collider (SSC) was done at Fermilab. The magnet will provide a magnetic field of 1.7 T over a volume 8 m in diameter by 16 m long. The particle-physics calorimetry will be inside the field volume and so the coil will be bath cooled and cryostable; the vessels will be stainless steel. Predictability of performance and the ability to safely negotiate all probable failure modes, including a quench, are important items of the design philosophy. Our conceptual design of the magnet and calorimeter has convinced us that this magnet is a reasonable extrapolation of present technology and is therefore feasible. The principal difficulties anticipated are those associated with the very large physical dimensions and stored energy of the magnet. 5 figs.

Fast, R.W.; Grimson, J.H.; Krebs, H.J.; Kephart, R.D.; Theriot, D.; Wands, R.H.

1989-09-15T23:59:59.000Z

330

Convergence Studies of Thermal and Electromagnetic Transient Quench Analysis of 11 GeV Super High Momentum Spectrometer Superconducting Magnets in Jefferson Lab  

Science Conference Proceedings (OSTI)

This paper presents results of convergence studies of transient thermal and electromagnetic quench analysis of five Super High Momentum Spectrometer (SHMS) superconducting magnets: HB, Q1, Q2, Q3, and Dipole, using Vector Fields Quench analysis codes. The convergence of the hot spot temperature and solution solve times were used to investigate the effects of element types, mesh densities, and tolerance criteria. The comparisons between tetrahedral elements and hexahedral elements was studied, and their advantages and disadvantages were discussed. Based on the results of convergence studies, a meshing guideline for coils is presented. The impact of iteration tolerance to the hot spot temperature was also explored, and it is found that tight tolerances result in extremely long solve times with only marginal improvements in the results.

Eric Sun, Paul Brindza, Steve Lassiter, Mike Fowler, E. Xu

2010-11-01T23:59:59.000Z

331

Day-night asymmetry of high and low energy solar neutrino events in Super-Kamiokande and in the Sudbury Neutrino Observatory  

E-Print Network (OSTI)

In the context of solar neutrino oscillations among active states, we briefly discuss the current likelihood of Mikheyev-Smirnov-Wolfenstein (MSW) solutions to the solar neutrino problem, which appear to be currently favored at large mixing, where small Earth regeneration effects might still be observable in Super-Kamiokande (SK) and in the Sudbury Neutrino Observatory (SNO). We point out that, since such effects are larger at high (low) solar neutrino energies for high (low) values of the mass square difference \\delta m^2, it may be useful to split the night-day rate asymmetry in two separate energy ranges. We show that the difference \\Delta of the night-day asymmetry at high and low energy may help to discriminate the two large-mixing solutions at low and high \\delta m^2 through a sign test, both in SK and in SNO, provided that the sensitivity to \\Delta can reach the (sub)percent level.

G. L. Fogli; E. Lisi; D. Montanino; A. Palazzo

2000-08-01T23:59:59.000Z

332

LEDS | OpenEI Community  

Open Energy Info (EERE)

LEDS Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 16 November, 2012 - 11:23 LEDS the focus of Monday's 10 a.m. Town Hall Meeting LEDS Town Hall meeting...

333

tagging API | OpenEI Community  

Open Energy Info (EERE)

tagging API Home Graham7781's picture Submitted by Graham7781(1982) Super contributor 15 February, 2013 - 16:25 Reegle mentions OpenEI in video on new Content Pool API data energy...

334

Energy.gov | OpenEI Community  

Open Energy Info (EERE)

picture Submitted by Graham7781(1982) Super contributor 1 October, 2012 - 09:32 White House Energy Datapalooza live on Whitehouse.gov Datapalooza Energy data Energy.gov OpenEI...

335

Whitehouse.gov | OpenEI Community  

Open Energy Info (EERE)

picture Submitted by Graham7781(1982) Super contributor 1 October, 2012 - 09:32 White House Energy Datapalooza live on Whitehouse.gov Datapalooza Energy data Energy.gov OpenEI...

336

carbon | OpenEI Community  

Open Energy Info (EERE)

carbon Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 9 January, 2014 - 13:12 Suburbs offset Low Carbon Footprint of major U.S. Cities carbon cities CO2...

337

Vehicles Data Challenge | OpenEI Community  

Open Energy Info (EERE)

Vehicles Data Challenge Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 13 December, 2012 - 14:40 The Apps for Vehicles Challenge has begun contest data...

338

American Clean Skies Foundation | OpenEI Community  

Open Energy Info (EERE)

American Clean Skies Foundation Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 2 October, 2012 - 14:01 Nominations open for 250,000 Multimedia Clean...

339

PMU | OpenEI Community  

Open Energy Info (EERE)

PMU Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 10:09 DOE Report Describes Progress in the Deployment of Synchrophasor Technologies...

340

regulatory | OpenEI Community  

Open Energy Info (EERE)

regulatory Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 5 August, 2013 - 14:18 Geothermal Regulatory Roadmap featured on NREL Now geothermal NREL...

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341

recovery act | OpenEI Community  

Open Energy Info (EERE)

recovery act Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 10:09 DOE Report Describes Progress in the Deployment of Synchrophasor...

342

SGIG | OpenEI Community  

Open Energy Info (EERE)

SGIG Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 10:09 DOE Report Describes Progress in the Deployment of Synchrophasor Technologies...

343

DOE Report Describes Progress in the Deployment of Synchrophasor...  

Open Energy Info (EERE)

Graham7781's blog Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 10:09 OpenEI PMU recovery act SGIG Smart Grid The U.S. Department of...

344

New report from White House outlines largest problems facing...  

Open Energy Info (EERE)

Graham7781's blog Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 13:21 energy grid OpenEI President Smart Grid United States White House On...

345

Water power | OpenEI Community  

Open Energy Info (EERE)

Water power Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 28 March, 2013 - 15:16 OpenEI launches new Water Power Gateway and Community Forum community...

346

WPA | OpenEI Community  

Open Energy Info (EERE)

picture Submitted by Graham7781(1992) Super contributor 30 January, 2013 - 11:55 Wind Powering America Guidebook officially launched on OpenEI guidebook OpenEI wind powering...

347

fossil fuels | OpenEI Community  

Open Energy Info (EERE)

fossil fuels Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 July, 2013 - 14:37 Four new publications help advance renewable energy development energy...

348

google hangout | OpenEI Community  

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google hangout Home Graham7781's picture Submitted by Graham7781(1982) Super contributor 21 February, 2013 - 16:32 Energy Secretary Steven Chu to host DOE's first google hangout at...

349

guidebook | OpenEI Community  

Open Energy Info (EERE)

guidebook Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 30 January, 2013 - 10:55 Wind Powering America Guidebook officially launched on OpenEI guidebook...

350

SDG&E Customers Can Connect Home Area Network Devices With Smart...  

Open Energy Info (EERE)

SDG&E Customers Can Connect Home Area Network Devices With Smart Meters Home > Groups > Utility Rate Graham7781's picture Submitted by Graham7781(1992) Super contributor 16...

351

Las Vegas | OpenEI Community  

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Las Vegas Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 23 January, 2013 - 13:57 The Consumer Electronics Show round-up CES electronics home automation...

352

Smartgrid | OpenEI Community  

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Smartgrid Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 January, 2013 - 11:09 SDG&E Customers Can Connect Home Area Network Devices With Smart Meters...

353

Smart Meters | OpenEI Community  

Open Energy Info (EERE)

Smart Meters Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 January, 2013 - 11:09 SDG&E Customers Can Connect Home Area Network Devices With Smart...

354

legislation | OpenEI Community  

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legislation Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 2 January, 2013 - 12:53 Key energy efficiency measures signed into law by President Obama...

355

contest | OpenEI Community  

Open Energy Info (EERE)

contest Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 13 December, 2012 - 14:40 The Apps for Vehicles Challenge has begun contest data fuel efficiency...

356

GTO | OpenEI Community  

Open Energy Info (EERE)

GTO Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 26 April, 2013 - 11:05 OpenEI Showcased in Geothermal Exploration Best Practices Workshop DOE...

357

download | OpenEI Community  

Open Energy Info (EERE)

download Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 March, 2013 - 10:23 Quarterly Smart Grid Data available for download on OpenEI data download...

358

CES | OpenEI Community  

Open Energy Info (EERE)

CES Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 23 January, 2013 - 13:57 The Consumer Electronics Show round-up CES electronics home automation Las...

359

electricity | OpenEI Community  

Open Energy Info (EERE)

electricity Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 21 November, 2013 - 12:53 NREL releases 2012 Renewable Energy Data Book 2012 data book...

360

Generation of warm dense matter and strongly coupled plasmas using the High Radiation on Materials facility at the CERN Super Proton Synchrotron  

E-Print Network (OSTI)

A dedicated facility named High Radiation on Materials (HiRadMat) is being constructed at CERN to study the interaction of the 450 GeV protons generated by the Super Proton Synchrotron (SPS) with fixed solid targets of different materials. The main purpose of these future experiments is to study the generation and propagation of thermal shock waves in the target in order to assess the damage caused to the equipment, including collimators and absorbers, in case of an accident involving an uncontrolled release of the entire beam at a given point. Detailed numerical simulations of the beam-target interaction of several cases of interest have been carried out. In this paper we present simulations of the thermodynamic and the hydrodynamic response of a solid tungsten cylindrical target that is facially irradiated with the SPS beam with nominal parameters. These calculations have been carried out in two steps. First, the energy loss of the protons is calculated in the solid target using the FLUKA code (Fasso et al....

Tahir, N A; Brugger, M; Assmann, R; Shutov, A; Lomonosov, I V; Gryaznov, V; Piriz, A R; Udrea, S; Hoffmann, D H H; Fortov, V E; Deutsch, C

2009-01-01T23:59:59.000Z

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361

False-alarm probability in relation to over-sampled power spectra, with application to Super-Kamiokande solar neutrino data  

E-Print Network (OSTI)

The term "false-alarm probability" denotes the probability that at least one out of M independent power values in a prescribed search band of a power spectrum computed from a white-noise time series is expected to be as large as or larger than a given value. The usual formula is based on the assumption that powers are distributed exponentially, as one expects for power measurements of normally distributed random noise. However, in practice one typically examines peaks in an over-sampled power spectrum. It is therefore more appropriate to compare the strength of a particular peak with the distribution of peaks in over-sampled power spectra derived from normally distributed random noise. We show that this leads to a formula for the false-alarm probability that is more conservative than the familiar formula. We also show how to combine these results with a Bayesian method for estimating the probability of the null hypothesis (that there is no oscillation in the time series), and we discuss as an example the application of these procedures to Super-Kamiokande solar neutrino data.

Peter A. Sturrock; Jeffrey D. Scargle

2010-06-03T23:59:59.000Z

362

Evaluation of the adequacy of using few-group lattice-homogenized properties for the diffusion analysis of the super critical water reactor  

SciTech Connect

Two issues may affect the accuracy of computed core reactivities and flux/power distributions for the Super Critical Water Reactor (SCWR) core with traditional core-analysis code RFSP: one is the two-energy-group neutron-diffusion theory; the other is the generation of lattice-homogenized properties with the lattice code based on the single-lattice-cell model without considering the effects of the environment. These two issues are not SCWR specific; however their effect may be more significant for SCWR. It has been illustrated that the lattice-homogenized properties calculated with the single-lattice-cell model is not sufficiently accurate for heterogeneous core configurations such as ACR-1000 checkerboard-voiding and core-reflector interface when adjacent channels experience significant spectrum interaction. To evaluate the adequacy of using two-group neutron-diffusion theory with single-lattice-based lattice properties for the analysis of the SCWR core, a 2-D SCWR benchmark problem was setup with the reference solution provided by the continuous-energy Monte-Carlo code SERPENT. The assessment shows that the traditional two-group neutron-diffusion theory with the single-lattice-cell- based lattice properties is not sufficient to capture either the spectral change or the environment effect for the SCWR core. The solution of the eight-group neutron-diffusion equation with the multicell- based lattice properties is considered appropriate for the analysis of the d SCWR core. (authors)

Shen, W. [Candu Energy Inc., 2285 Speakman Dr., Mississauga, ON L5B 1K (Canada)

2012-07-01T23:59:59.000Z

363

A Very Intense Neutrino Super Beam Experiment for Leptonic CP Violation Discovery based on the European Spallation Source Linac: A Snowmass 2013 White Paper  

E-Print Network (OSTI)

Very intense neutrino beams and large neutrino detectors will be needed in order to enable the discovery of CP violation in the leptonic sector. We propose to use the proton linac of the European Spallation Source currently under construction in Lund, Sweden to deliver, in parallel with the spallation neutron production, a very intense, cost effective and high performance neutrino beam. The baseline program for the European Spallation Source linac is that it will be fully operational at 5 MW average power by 2022, producing 2 GeV 2.86 ms long proton pulses at a rate of 14 Hz. Our proposal is to upgrade the linac to 10 MW average power and 28 Hz, producing 14 pulses/s for neutron production and 14 pulses/s for neutrino production. Furthermore, because of the high current required in the pulsed neutrino horn, the length of the pulses used for neutrino production needs to be compressed to a few $\\mu$s with the aid of an accumulator ring. A long baseline experiment using this Super Beam and a megaton underground Water Cherenkov detector located in existing mines 300-600 km from Lund will make it possible to discover leptonic CP violation at 5 $\\sigma$ significance level in up to 50% of the leptonic Dirac CP-violating phase range. This experiment could also determine the neutrino mass hierarchy at a significance level of more than 3 $\\sigma$ if this issue will not already have been settled by other experiments by then. The mass hierarchy performance could be increased by combining the neutrino beam results with those obtained from atmospheric neutrinos detected by the same large volume detector. This detector will also be used to measure the proton lifetime, detect cosmological neutrinos and neutrinos from supernova explosions. Results on the sensitivity to leptonic CP violation and the neutrino mass hierarchy are presented.

E. Baussan; M. Blennow; M. Bogomilov; E. Bouquerel; J. Cederkall; P. Christiansen; P. Coloma; P. Cupial; H. Danared; C. Densham; M. Dracos; T. Ekelof; M. Eshraqi; E. Fernandez Martinez; G. Gaudiot; R. Hall-Wilton; J. -P. Koutchouk; M. Lindroos; R. Matev; D. McGinnis; M. Mezzetto; R. Miyamoto; L. Mosca; T. Ohlsson; H. Ohman; F. Osswald; S. Peggs; P. Poussot; R. Ruber; J. Y. Tang; R. Tsenov; G. Vankova-Kirilova; N. Vassilopoulos; E. Wildner; J. Wurtz

2013-09-26T23:59:59.000Z

364

Streamlined Approach for Environmental Restoration (SAFER) Plan for Corrective Action Unit 118: Area 27 Super Kukla Facility, Nevada Test Site, Nevada, Rev. No.: 1  

SciTech Connect

This Streamlined Approach for Environmental Restoration (SAFER) plan addresses closure for Corrective Action Unit (CAU) 118, Area 27 Super Kukla Facility, identified in the ''Federal Facility Agreement and Consent Order''. Corrective Action Unit 118 consists of one Corrective Action Site (CAS), 27-41-01, located in Area 27 of the Nevada Test Site. Corrective Action Site 27-41-01 consists of the following four structures: (1) Building 5400A, Reactor High Bay; (2) Building 5400, Reactor Building and access tunnel; (3) Building 5410, Mechanical Building; and (4) Wooden Shed, a.k.a. ''Brock House''. This plan provides the methodology for field activities needed to gather the necessary information for closing the CAS. There is sufficient information and process knowledge from historical documentation and site confirmation data collected in 2005 and 2006 to recommend closure of CAU 118 using the SAFER process. The Data Quality Objective process developed for this CAU identified the following expected closure option: closure in place with use restrictions. This expected closure option was selected based on available information including contaminants of potential concern, future land use, and assumed risks. There are two decisions that need to be answered for closure. Decision I is to determine the nature of contaminants of concern in environmental media or potential source material that could impact human health or the environment. Decision II is to determine whether or not sufficient information has been obtained to confirm that closure objectives were met. This decision includes determining whether the extent of any contamination remaining on site has been defined, and whether actions have been taken to eliminate exposure pathways.

David Strand

2006-09-01T23:59:59.000Z

365

Super Star Cluster NGC1705-1: A Local Analogue to the Birthsite of Long-duration Gamma-ray Bursts  

E-Print Network (OSTI)

Recent observations suggest that global properties of the host galaxies for long-duration gamma-ray bursts (GRBs) are particularly well-suited for creating the massive star progenitors of these GRBs. Motivated by the hypothesis that massive young star clusters located in metal-poor, low-metallicity galaxies are a natural birthsite for GRB progenitors, we present a comparison study of the ISM properties along the sightline toward the super star cluster, NGC1705-1, and those in distant GRB hosts. Using the same set of metal transitions in the UV and applying known ISM structures in NGC1705, we find that NGC1705-1 resembles distant GRB host galaxies in its high neutral gas column, low molecular gas fraction, low metallicity, alpha-element enhancement,and low dust depletion. The lack of molecular gas is due to the enhanced UV radiation field in the starburst environment, consistent with the expectations for GRB progenitors. In addition, the known presence of dense neutral gas clouds at rnatural reservoir of C^+, Si^+, and Fe^+ ions that may be subsequently excited by the afterglow UV radiation field to produce excited lines commonly seen in GRB host ISM. We further argue that the apparent offset in the velocity profiles of low- and high-ionization transitions from absorption-line observations alone already offers important clues for related starburst episodes in GRB host galaxies. Our study shows that a statistical comparison between the ISM around star clusters and high-redshift GRB progenitors is important for identifying the key physical parameters that facilitate the formation of GRBs.

Hsiao-Wen Chen; J. X. Prochaska; Joshua S. Bloom

2007-06-15T23:59:59.000Z

366

US ITER is a strong contributor in plan to enhance international...  

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

By Lynne Degitz, US ITER March 28, 2013 Tweet Widget Facebook Like Google Plus One PPPL's Russell Feder, left, and David Johnson developed key features for a modular approach to...

367

ii AUTHORS AND CONTRIBUTORS Future of Toxicity Testing Workgroup Co-Chairs  

E-Print Network (OSTI)

Recycled/Recyclable Printed with vegetable-based ink on paper that contains a minimum of 50 % post-consumer fiber and is processed chlorine free. DISCLAIMER Mention of trade names or commercial products does not constitute endorsement or recommendation for use. Notwithstanding any use of mandatory language such as "must " and "require " in this document with regard to or to reflect scientific practices, this document does not

Science Policy Council; Michael Firestone; Health Protection; Environmental Education

2009-01-01T23:59:59.000Z

368

A Meteorological Analysis of Important Contributors to the 19992005 Canadian Prairie Drought  

Science Conference Proceedings (OSTI)

Drought is a complex natural hazard that is endemic to the Canadian prairies. The 19992005 Canadian prairie drought, which had great socioeconomic impacts, was meteorologically unique in that it did not conform to the traditional persistent ...

Lisa M. Hryciw; Eyad H. Atallah; Shawn M. Milrad; John R. Gyakum

2013-10-01T23:59:59.000Z

369

Dust in the polar region as a major contributor to the IR emission of AGN  

E-Print Network (OSTI)

(abridged) It is generally assumed that the distribution of dust on parsec scales forms a geometrically- and optically-thick entity in the equatorial plane around the accretion disk and broad-line region - dubbed "dust torus" - that emits the bulk of the sub-arcsecond-scale IR emission and gives rise to orientation-dependent obscuration. Here we report detailed interferometry observations of the unobscured (type 1) AGN in NGC 3783 that allow us to constrain the size, elongation, and direction of the mid-IR emission with high accuracy. The mid-IR emission is characterized by a strong elongation toward position angle PA -52 deg, closely aligned with the polar axis (PA -45 deg). We determine half-light radii along the major and minor axes at 12.5 {\\mu}m of (4.23 +/- 0.63) pc x (1.42 +/- 0.21) pc, which corresponds to intrinsically-scaled sizes of (69.4 +/- 10.8) rin x (23.3 +/- 3.5) rin for the inner dust radius of rin = 0.061 pc as inferred from near-IR reverberation mapping. This implies an axis ratio of 3:1, ...

Hoenig, Sebastian F; Tristram, Konrad R W; Prieto, M Almudena; Gandhi, Poshak; Asmus, Daniel; Antonucci, Robert; Burtscher, Leonard; Duschl, Wolfgang J; Weigelt, Gerd

2013-01-01T23:59:59.000Z

370

Wind power is a rapidly growing con-tributor to worldwide energy supplies and  

E-Print Network (OSTI)

the U.S., represent- ing nearly one-third of the total installed wind energy capacity in the country for wind turbine siting and wind source prediction. Ironically, PPM has hired 3TIER to provide wind energy and operates wind farms in Ireland, Scotland, England, Wales and the United States. With the recent extension

371

Bulletin of Tibetology: Volume 25 Number 3 Number 3 : Cover, contents, contributors  

E-Print Network (OSTI)

-40 and 1946- 50) and Chungking (1942-44); for severa1 terms professor in Tibetan -:language and History at University of Washing ton, Seattie, USA; recipient of the GaId Meda1 of the Roya1 Centra1 Asian Society, UK; Fe-.llow, KeMe Ca:I1ege, Oxford; Fe...

Namgyal Institute of Tibetology

1989-01-01T23:59:59.000Z

372

Examining Internal and External Contributors to Greenland Climate Variability Using CCSM3  

Science Conference Proceedings (OSTI)

Greenland climate variability is connected to internal and external sources of global climate variability in six millennium simulations using Community Climate System Model 3. Simulation forcings are consistent with the PaleoClimate Model Inter-...

Heather J. Andres; W. R. Peltier

373

Interior of an off-campus apartment. Photo: Michael Diamond Contributor: Amanda Lanyon-LeSage  

E-Print Network (OSTI)

. Water and heat are included in rent, and residents are responsible for paying electricity. Free laundry of your own parking space! You really don't need a car to get into campus since the #80 Metro bus provides

Wisconsin at Madison, University of

374

Feed and Farm Supply Store Managers' Perceptions of Employee Training as a Contributor to Competitive Advantage  

E-Print Network (OSTI)

The purpose of this study was to assess the perception held by managers of feed and farm supply stores in Texas regarding the contribution of employee training to the competitiveness of the firm, determine if managers of feed and farm supply stores perceive that employee training can improve their competitive strength, and to determine if they will invest in employee training in order to gain a competitive advantage. The objectives of this study include: describe the operating environment of feed and farm supply stores in Texas; describe feed and farm supply store managers? perception of employee training?s contribution to their firm?s competitive advantage; identify barriers to employee training in feed and farm supply stores; determine Internet availability and potential use for employee training in feed and farm supply stores; and describe the willingness of feed and farm supply store managers to engage in employee training delivered via the Internet. This study employed a descriptive and correlational research design. A selfadministered questionnaire was used to collect data from a sample frame of 305 feed and farm supply stores randomly selected from 1,487 stores in Texas. These stores operate in a demanding, competitive environment that is changing at a rapid pace. They perceive that employee training improves customer satisfaction, contributes to business growth, improves productivity, and increases profits. The skills needed by their employees are increasing and they need training in sales, communication skills, technical knowledge, time management, retail merchandising, marketing, and business management to help the business stay competitive. Barriers to training include not being able to see immediate results, cost, difficulties created when key employees are not on the job, travel distances to attend training, and a lack of training programs relevant to their needs. Over 80 percent of these stores have both computers and Internet access. Managers will allow employees to use these resources for training purposes, encourage participation in online training, and allow their employees to participate in training during business hours. It is recommended that Internet based training programs be developed in sales, communication skills, technical knowledge, time management, retail merchandising, and business management for these small agribusinesses.

Springfield, Henry C., III

2008-12-01T23:59:59.000Z

375

Bulletin of Tibetology: Volume 35 Number 3 Number 3 : Cover, contents, contributors  

E-Print Network (OSTI)

, Department of Ecdessiastical Affairs, Government of Sikkim, Gangtok, Sikkim . Prof. Parameshwar Giri Yogi: Obtained Acharya degree in Pali Buddhism and Post Graduate Diploma in Archaeology and Mumem Science. He is also a member of Board of Study, Sangkai...

Namgyal Institute of Tibetology

1999-10-31T23:59:59.000Z

376

SuperComputing | Mathematics | ORNL  

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

Discrete Math Kinetic Theory Linear Algebra Solvers Uncertainty Quantification National Security Systems Modeling Engineering Analysis Behavioral Sciences Geographic Information Science and Technology Quantum Information Science Supercomputing and Computation Home | Science & Discovery | Supercomputing and Computation | Research Areas | Mathematics SHARE Mathematics The Computational Mathematics activities include the developing and deploying computational and applied mathematical capabilities for modeling, simulating, and predicting complex phenomena of importantance to the Department of Energy (DOE). A particular focus is on developing novel scalable algorithms for exploiting novel high performance computing resources for scientific discovery as well as decision-sciences.

377

SuperComputing | Materials | ORNL  

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

Theory Institute Polymer-based Multicomponent Materials Molecular Dynamics Molecular Mechanics Course Grained Models Mathematics National Security Systems Modeling Engineering...

378

Energy usage in super markets  

SciTech Connect

The supermarket industry used 450 billion Btu's of energy each day, enough to heat 2 million homes. But more important than the overall energy usage is what energy is costing the supermarket operator; in many cases energy costs exceed rent. This special research report is designed to help the supermarket management determine if their stores are excessive energy users and to provide valuable data for planning remodels and new stores. The report is presented in five sections. The first two sections, General Observations and Monthly Electrical Usage and Demand Power, can easily be used by all supermarket operators. The third and fourth sections contain more detailed statistics that will be valuable to industry people who want to analyze energy usage more thoroughly. The statistics in section 1-4 are reported for various geographic regions and store sizes. Section five is the sample distribution which provides an insight into what other stores are using for refrigeration, lighting, etc. The information in this report is average for a typical supermarket and should be used only as that when compared to a specific supermarket facility.

Gerke, E.

1976-01-01T23:59:59.000Z

379

Integrated modeling of CO2 storage and leakage scenarios including transitions between super- and sub-critical conditions, and phase change between liquid and gaseous CO2  

SciTech Connect

Storage of CO{sub 2} in saline aquifers is intended to be at supercritical pressure and temperature conditions, but CO{sub 2} leaking from a geologic storage reservoir and migrating toward the land surface (through faults, fractures, or improperly abandoned wells) would reach subcritical conditions at depths shallower than 500-750 m. At these and shallower depths, subcritical CO{sub 2} can form two-phase mixtures of liquid and gaseous CO{sub 2}, with significant latent heat effects during boiling and condensation. Additional strongly non-isothermal effects can arise from decompression of gas-like subcritical CO{sub 2}, the so-called Joule-Thomson effect. Integrated modeling of CO{sub 2} storage and leakage requires the ability to model non-isothermal flows of brine and CO{sub 2} at conditions that range from supercritical to subcritical, including three-phase flow of aqueous phase, and both liquid and gaseous CO{sub 2}. In this paper, we describe and demonstrate comprehensive simulation capabilities that can cope with all possible phase conditions in brine-CO{sub 2} systems. Our model formulation includes: (1) an accurate description of thermophysical properties of aqueous and CO{sub 2}-rich phases as functions of temperature, pressure, salinity and CO{sub 2} content, including the mutual dissolution of CO{sub 2} and H{sub 2}O; (2) transitions between super- and subcritical conditions, including phase change between liquid and gaseous CO{sub 2}; (3) one-, two-, and three-phase flow of brine-CO{sub 2} mixtures, including heat flow; (4) non-isothermal effects associated with phase change, mutual dissolution of CO{sub 2} and water, and (de-) compression effects; and (5) the effects of dissolved NaCl, and the possibility of precipitating solid halite, with associated porosity and permeability change. Applications to specific leakage scenarios demonstrate that the peculiar thermophysical properties of CO{sub 2} provide a potential for positive as well as negative feedbacks on leakage rates, with a combination of self-enhancing and self-limiting effects. Lower viscosity and density of CO{sub 2} as compared to aqueous fluids provides a potential for self-enhancing effects during leakage, while strong cooling effects from liquid CO{sub 2} boiling into gas, and from expansion of gas rising towards the land surface, act to self-limit discharges. Strong interference between fluid phases under three-phase conditions (aqueous - liquid CO{sub 2} - gaseous CO{sub 2}) also tends to reduce CO{sub 2} fluxes. Feedback on different space and time scales can induce non-monotonic behavior of CO{sub 2} flow rates.

Pruess, K.

2011-05-15T23:59:59.000Z

380

OpenEI | OpenEI Community  

Open Energy Info (EERE)

OpenEI OpenEI Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 09:09 DOE Report Describes Progress in the Deployment of Synchrophasor Technologies for Improved Grid Operations OpenEI PMU recovery act SGIG Smart Grid Graham7781's picture Submitted by Graham7781(1992) Super contributor 5 August, 2013 - 13:18 Geothermal Regulatory Roadmap featured on NREL Now geothermal NREL OpenEI regulatory roadmap Navigating the complex system of federal and state regulations to secure project approvals is one of the biggest hurdles geothermal power developers

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381

Smart Grid | OpenEI Community  

Open Energy Info (EERE)

Smart Grid Smart Grid Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 09:09 DOE Report Describes Progress in the Deployment of Synchrophasor Technologies for Improved Grid Operations OpenEI PMU recovery act SGIG Smart Grid Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 March, 2013 - 10:23 Quarterly Smart Grid Data available for download on OpenEI data download OpenEI quarterly Smart Grid Smartgrid.gov SmartGrid.gov is a resource for information about the Smart Grid and government-sponsored Smart Grid projects. The information on SmartGrid.gov

382

Graham7781's blog | OpenEI Community  

Open Energy Info (EERE)

Graham7781's blog Graham7781's blog Home > Blogs Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Graham7781's picture Submitted by Graham7781(1992) Super contributor 15 August, 2013 - 09:09 DOE Report Describes Progress in the Deployment of Synchrophasor Technologies for Improved Grid Operations OpenEI PMU recovery act SGIG Smart Grid Graham7781's picture Submitted by Graham7781(1992) Super contributor 5 August, 2013 - 13:18 Geothermal Regulatory Roadmap featured on NREL Now geothermal NREL OpenEI regulatory roadmap Navigating the complex system of federal and state regulations to secure project approvals is one of the biggest hurdles geothermal power developers

383

imported | OpenEI Community  

Open Energy Info (EERE)

imported imported Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 24 July, 2012 - 09:48 Visualizing OpenEI Data imported OpenEI Want to create a visualization like the one on the new OpenEI front page? There are several online tools that make organizing and visualizing data free and easy. Graham7781's picture Submitted by Graham7781(1992) Super contributor 18 July, 2012 - 10:02 New OpenEI Homepage imported OpenEI OpenEI has gotten a makeover, and we couldn't help gush over how nice we think we look. Graham7781's picture Submitted by Graham7781(1992) Super contributor 10 July, 2012 - 14:04 S & P Opines on Securitizing Distributed Generation imported OpenEI Article originally published at NREL's Renewable Energy Project Finance website Graham7781's picture

384

ECO2M: A TOUGH2 Fluid Property Module for Mixtures of Water, NaCl, and CO2, Including Super- and Sub-Critical Conditions, and Phase Change Between Liquid and Gaseous CO2  

SciTech Connect

ECO2M is a fluid property module for the TOUGH2 simulator (Version 2.0) that was designed for applications to geologic storage of CO{sub 2} in saline aquifers. It includes a comprehensive description of the thermodynamics and thermophysical properties of H{sub 2}O - NaCl - CO{sub 2} mixtures, that reproduces fluid properties largely within experimental error for temperature, pressure and salinity conditions in the range of 10 C {le} T {le} 110 C, P {le} 600 bar, and salinity from zero up to full halite saturation. The fluid property correlations used in ECO2M are identical to the earlier ECO2N fluid property package, but whereas ECO2N could represent only a single CO{sub 2}-rich phase, ECO2M can describe all possible phase conditions for brine-CO{sub 2} mixtures, including transitions between super- and sub-critical conditions, and phase change between liquid and gaseous CO{sub 2}. This allows for seamless modeling of CO{sub 2} storage and leakage. Flow processes can be modeled isothermally or non-isothermally, and phase conditions represented may include a single (aqueous or CO{sub 2}-rich) phase, as well as two-and three-phase mixtures of aqueous, liquid CO{sub 2} and gaseous CO{sub 2} phases. Fluid phases may appear or disappear in the course of a simulation, and solid salt may precipitate or dissolve. TOUGH2/ECO2M is upwardly compatible with ECO2N and accepts ECO2N-style inputs. This report gives technical specifications of ECO2M and includes instructions for preparing input data. Code applications are illustrated by means of several sample problems, including problems that had been previously solved with TOUGH2/ECO2N.

Pruess, K.

2011-04-01T23:59:59.000Z

385

Renewable Energy: A Significant Contributor? Achieving the Goal of 30% Transportation Fuels from Biomass by 2030 (Presentation)  

DOE Green Energy (OSTI)

Presented by Dan Arvizu at the 10th Annual Green Chemistry & Engineering Conference on June 29, 2006 in Washington, D.C.

Arvizu, D.

2006-06-29T23:59:59.000Z

386

Motor Oil Analysis It is helpful when investigating the composition and source of pollution that possible contributors have been sufficiently  

E-Print Network (OSTI)

Motor Oil Analysis It is helpful when investigating the composition and source of pollution various oils, fuels, et cetera. Patrick Ferree ­ under the guidance of Anita Johnson ­ prepared samples of motor oil via atomization onto Teflon filters, and analyzed these samples using a Fourier transform

Russell, Lynn

387

INTENDED TO IMPROVE THE UNDERSTANDING OF OPERATIONAL TERMS. SPECIAL THANKS TO THE FOLLOWING CONTRIBUTORS FOR MAKING POSSIBLE  

E-Print Network (OSTI)

One or more conditions of the original document may affect the quality of the image, such as: Discolored pages Faded or light ink Binding intrudes into the text This has been a co-operative project between the NOAA Central Library and the Climate Database Modernization Program, National Climate Data Center (NCDC). To view the

The Compilation; Of This; Booklet Robert; A. Mccoy; Roy Crockett; Alfonso Diazdelcastillo

2009-01-01T23:59:59.000Z

388

Supercomputers: Super-polluters? Datacenters Journal  

E-Print Network (OSTI)

includes: · Free Cooling - Free cooling is the use of outside air- or water-side cooling via cooling towers and $112.7 million. These values are for the IT equipment only, i.e. excluding cooling. 1 Wehner, M, L--would not be unusual for a contemporary supercomputing facility. Meanwhile, rising cooling demand is driving the up

Lee, Jason R.

389

Characteristics and Identification of Super- Effective Thermal ...  

Science Conference Proceedings (OSTI)

... diffusion flames. The earliest such calculation we have identified is that of Hahn and Wendt that was published in 1981. [87 ...

2007-03-13T23:59:59.000Z

390

Super Energy Saver Ground Source Heat Pump  

Source: US Energy Information Administration . 11 Managed by UT-Battelle for the U.S. Department of Energy ... GSHPs are very energy efficient, and the market is

391

Acceleration methods for image super-resolution  

E-Print Network (OSTI)

, Atlanta, GA, USA (2000) 43­49 18. Franchi, D., Belardinelli, A., Palagi, G., Ripoli, A., Bedini, R.: New

Cooperstock, Jeremy R.

392

Fabrication and Characterization of Super Strong Cellulose ...  

Science Conference Proceedings (OSTI)

Pros and cons, depending on the problems studied, are discussed. ... Investigation on Modified Humic Substances Based Binders for Iron Ore Agglomeration.

393

Super-Index of Mathematical Encyclopedia - CECM  

E-Print Network (OSTI)

... Eisenstein Conjecture Eisenstein Series Elation Elder's Theorem Election Early Results Electric Motor Curve Elementary Proof Elevator Paradox...

394

Carbon film electrodes for super capacitor applications  

DOE Patents (OSTI)

A microporous carbon film for use as electrodes in energy strorage devices is disclosed, which is made by the process comprising the steps of: (1) heating a polymer film material consisting essentially of a copolymer of polyvinylidene chloride and polyvinyl chloride in an inert atmosphere to form a carbon film; and (2) activating said carbon film to form said microporous carbon film having a density between about 0.7 g/cm.sup.2 and 1 g/cm.sup.2 and a gravimetric capacitance of about between 120 F/g and 315 F/g.

Tan, Ming X. (Livermore, CA)

1999-01-01T23:59:59.000Z

395

Available Technologies: Super High Rate Sputter Deposition  

Andre Anders of Berkeley Lab has developed a very high deposition rate magnetron sputtering wherein the surface of a target and the race track zone area of the ...

396

Microstructure of Super-duplex Stainless Steels  

E-Print Network (OSTI)

in duplex stainless steels by solution heat treatment at or above ferritisation tem- peratures, specimens were quenched into iced water after different holding times at 1300 QC. The results are discussed in the chapters that follow. In another series...

Sharafi, Shahriar

1993-12-07T23:59:59.000Z

397

Composite, nanostructured, super-hydrophobic material - Energy ...  

Hydrogen and Fuel Cell; Hydropower, Wave and Tidal; Industrial Technologies; Solar Photovoltaic; Solar Thermal; Startup America; ... July 27, 2004: Government Interests:

398

Super-hydrophobic fluorine containing aerogels  

Science Conference Proceedings (OSTI)

An aerogel material with surfaces containing fluorine atoms which exhibits exceptional hydrophobicity, or the ability to repel liquid water. Hydrophobic aerogels are efficient absorbers of solvents from water. Solvents miscible with water are separated from it because the solvents are more volatile than water and they enter the porous aerogel as a vapor across the liquid water/solid interface. Solvents that are immisicble with water are separated from it by selectively wetting the aerogel. The hydrophobic property is achieved by formulating the aerogel using fluorine containing molecules either directly by addition in the sol-gel process, or by treating a standard dried aerogel using the vapor of fluorine containing molecules.

Coronado, Paul R. (Livermore, CA); Poco, John F. (Livermore, CA); Hrubesh, Lawrence W. (Pleasanton, CA)

2007-05-01T23:59:59.000Z

399

Frequency scaling of linear super-colliders  

SciTech Connect

The development of electron-positron linear colliders in the TeV energy range will be facilitated by the development of high-power rf sources at frequencies above 2856 MHz. Present S-band technology, represented by the SLC, would require a length in excess of 50 km per linac to accelerate particles to energies above 1 TeV. By raising the rf driving frequency, the rf breakdown limit is increased, thereby allowing the length of the accelerators to be reduced. Currently available rf power sources set the realizable gradient limit in an rf linac at frequencies above S-band. This paper presents a model for the frequency scaling of linear colliders, with luminosity scaled in proportion to the square of the center-of-mass energy. Since wakefield effects are the dominant deleterious effect, a separate single-bunch simulation model is described which calculates the evolution of the beam bunch with specified wakefields, including the effects of using programmed phase positioning and Landau damping. The results presented here have been obtained for a SLAC structure, scaled in proportion to wavelength.

Mondelli, A.; Chernin, D.; Drobot, A.; Reiser, M.; Granatstein, V.

1986-06-01T23:59:59.000Z

400

SuperComputing | Energy Science | ORNL  

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

Energy Storage Future Technology Knowledge Discovery Materials Mathematics National Security Systems Modeling Engineering Analysis Behavioral Sciences Geographic Information...

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

Super Duty Diesel Truck with NOx Aftertreatment  

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

A profile of a Ford-Energy Department program to develop a three-stage aftertreatment technology, which cleans the vehicle exhaust emissions.

402

Bioenergy - Super microbe | ornl.gov  

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

microbe A newly discovered microbe may offer a cost-effective solution that makes biofuel production more efficient. Researchers have found an anaerobic bacterium called...

403

Super Separator | Princeton Plasma Physics Lab  

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

Join Our Mailing List A Collaborative National Center for Fusion & Plasma Research Search form Search Search Home About Overview Learn More Visiting PPPL History...

404

Composite, nanostructured, super-hydrophobic material  

DOE Patents (OSTI)

A hydrophobic disordered composite material having a protrusive surface feature includes a recessive phase and a protrusive phase, the recessive phase having a higher susceptibility to a preselected etchant than the protrusive phase, the composite material having an etched surface wherein the protrusive phase protrudes from the surface to form a protrusive surface feature, the protrusive feature being hydrophobic.

D' Urso, Brian R. (Clinton, TN); Simpson, John T. (Clinton, TN)

2007-08-21T23:59:59.000Z

405

Super-high density laser fusion CTR  

SciTech Connect

From sixth European conference on controlled fusion and plasma physics; Moscow, USSR (30 Jul 1973). A basic discussion of laser-induced fusion is presented. Implosion development and applications are described. Implosion and thermonuclear physics are discussed in some detail along with laser technology, laser fusion reactors, and fusion energy conversion. (MOW)

Thiessen, A.; Zimmerman, G.; Weaver, T.; Emmett, J.; Nuckolls, J.; Wood, L.

1973-09-01T23:59:59.000Z

406

Development of Super-high Sensitivity Radon Detector for the Super-Kamiokande Detector  

E-Print Network (OSTI)

samples of standard radon water produced by the radon water making system, which takes account produced by the radon water making system. 13 #12; Diluted Rn water[mBq=m 3 ] 700L C.F[cpd/(mBq=m 3 )] 70L-high sensitivity radon detector for water which works as a real-time monitor of the radon concentration in water

Takeuchi, Yasuo

407

NREL | OpenEI Community  

Open Energy Info (EERE)

NREL NREL Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 5 August, 2013 - 13:18 Geothermal Regulatory Roadmap featured on NREL Now geothermal NREL OpenEI regulatory roadmap Navigating the complex system of federal and state regulations to secure project approvals is one of the biggest hurdles geothermal power developers face-but not if they've got a map outlining every twist and turn. Graham7781's picture Submitted by Graham7781(1992) Super contributor 26 June, 2013 - 09:17 NREL's Energy Databus storing big energy data campus databus energy meter data NREL OpenEI Tool The Energy Databus began as a project aimed at addressing campus energy consumption and tracking issues at NREL. Now, with the ability to store large amounts of data, some of which measured by the second, along with

408

United States | OpenEI Community  

Open Energy Info (EERE)

United States United States Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Sfomail's picture Submitted by Sfomail(48) Member 17 May, 2013 - 12:03 Commercial and Residential Hourly Load Data Now Available on OpenEI! building load building load data commercial load data dataset datasets electric load data load data load profile OpenEI residential load TMY3 United States Load data Image source: NREL Files: application/zip icon System Advisor Model Tool for Downloading Load Data Graham7781's picture Submitted by Graham7781(1992) Super contributor 29 October, 2012 - 14:46 East Coast Utilities prepare for Hurricane Sandy

409

REEGLE | OpenEI Community  

Open Energy Info (EERE)

REEGLE REEGLE Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 15 February, 2013 - 15:25 Reegle mentions OpenEI in video on new Content Pool API data energy OpenEI REEEP REEGLE structured tagging API Reegle and OpenEI share the vision that easy access to energy information will help drive future developments in clean energy development. Graham7781's picture Submitted by Graham7781(2002) Super contributor 27 November, 2012 - 10:41 LOD Workshop Wrap-up courtesy of REEGLE LOD NREL OpenEI REEEP REEGLE Dubbed as the first "Linked Open Data" workshop, last week REEEP and NREL ran a clean energy workshop in Washington, D.C. to discuss the enormous potential of LOD in supporting the transition to a cleaner energy economy. Syndicate content 429 Throttled (bot load)

410

Town Hall meeting | OpenEI Community  

Open Energy Info (EERE)

Town Hall meeting Town Hall meeting Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 November, 2012 - 11:23 LEDS the focus of Monday's 10 a.m. Town Hall Meeting LEDS Town Hall meeting What: OpenEI's town hall meeting is a half-hour open forum for discussions on energy topics with NREL's OpenEI team. Find out how your fellow researchers, students, teachers and energy professionals are using energy data, maps and tools. Graham7781's picture Submitted by Graham7781(1992) Super contributor 19 September, 2012 - 13:40 Town Hall Meeting October 1st, 2012 OpenEI Town Hall meeting What: OpenEI's town hall meeting is a half-hour open forum for discussions on energy topics with NREL's OpenEI team. Find out how your fellow researchers, students, teachers and energy professionals are using energy

411

White House | OpenEI Community  

Open Energy Info (EERE)

White House White House Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Graham7781's picture Submitted by Graham7781(1992) Super contributor 30 August, 2012 - 15:16 Historic Fuel Standards auto fuel efficiency obama standards vehicle White House On Tuesday, Ray Lahood, Secretary of the U.S. Department of Transportation, and Lisa P. Jackson, Environmental Protection Agency Administrator, unveiled the joint effort, along with the Obama Administration, to create record fuel standards for vehicles built between 2017 and 2025. Syndicate content 429 Throttled (bot load) Error 429 Throttled (bot load)

412

fuel efficiency | OpenEI Community  

Open Energy Info (EERE)

fuel efficiency fuel efficiency Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 13 December, 2012 - 14:40 The Apps for Vehicles Challenge has begun! contest data fuel efficiency launch Obama Administration OpenEI Vehicles Data Challenge **Update: Visit the Apps for Vehicles page for all the information you need on the challenge.** Graham7781's picture Submitted by Graham7781(1992) Super contributor 30 August, 2012 - 15:16 Historic Fuel Standards auto fuel efficiency obama standards vehicle White House On Tuesday, Ray Lahood, Secretary of the U.S. Department of Transportation, and Lisa P. Jackson, Environmental Protection Agency Administrator, unveiled the joint effort, along with the Obama Administration, to create record fuel standards for vehicles built between 2017 and 2025.

413

obama | OpenEI Community  

Open Energy Info (EERE)

obama obama Home Graham7781's picture Submitted by Graham7781(1992) Super contributor 27 June, 2013 - 12:39 President Obama presents new Climate Action Plan Climate Action Plan obama OpenEI President President Obama layed out his much anticipated Climate Action Plan tuesday. The President's plan calls for major actions that the administration believes will mitigate the environmental and economic costs of climate change. Obama's six Climate Action Initiatives: 1. Phasing out Fossil Fuels Graham7781's picture Submitted by Graham7781(1992) Super contributor 30 August, 2012 - 15:16 Historic Fuel Standards auto fuel efficiency obama standards vehicle White House On Tuesday, Ray Lahood, Secretary of the U.S. Department of Transportation, and Lisa P. Jackson, Environmental Protection Agency Administrator,

414

President | OpenEI Community  

Open Energy Info (EERE)

59 59 Varnish cache server Home Groups Community Central Green Button Applications Developer Utility Rate FRED: FRee Energy Database More Public Groups Private Groups Features Groups Blog posts Content Stream Documents Discussions Polls Q & A Events Notices My stuff Energy blogs 429 Throttled (bot load) Error 429 Throttled (bot load) Throttled (bot load) Guru Meditation: XID: 2142234959 Varnish cache server President Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 16 August, 2013 - 12:21 New report from White House outlines largest problems facing United States energy grid energy grid OpenEI President Smart Grid United States White House Graham7781's picture Submitted by Graham7781(2002) Super contributor 27 June, 2013 - 12:39 President Obama presents new Climate Action Plan

415

energy efficiency | OpenEI Community  

Open Energy Info (EERE)

energy efficiency energy efficiency Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 2 January, 2013 - 12:53 Key energy efficiency measures signed into law by President Obama energy efficiency legislation OpenEI President Obama President Obama recently signed into law the American Energy Manufacturing Technical Corrections Act, a piece of legislation that includes provisions that are aimed at aggressively moving clean energy and energy efficiency forward. For a more in-depth article, visit Smartgridnews.com Graham7781's picture Submitted by Graham7781(2002) Super contributor 12 December, 2012 - 11:30 FOA aimed at growing expansive database of Renewable Energy and Energy Efficiency Incentives and Policies DOE energy efficiency FOA funding opportunity Renewable Energy

416

LOD | OpenEI Community  

Open Energy Info (EERE)

LOD LOD Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 27 November, 2012 - 10:41 LOD Workshop Wrap-up courtesy of REEGLE LOD NREL OpenEI REEEP REEGLE Dubbed as the first "Linked Open Data" workshop, last week REEEP and NREL ran a clean energy workshop in Washington, D.C. to discuss the enormous potential of LOD in supporting the transition to a cleaner energy economy. Jweers's picture Submitted by Jweers(83) Contributor 10 October, 2012 - 08:20 LOD Workshop Invitation Event linked open data LOD Open Data workshop Update the invitation (attached). It now features a link to the public facing wiki page.Upload Files: application/pdf icon LOD Workshop Invitation Jweers's picture Submitted by Jweers(83) Contributor 8 October, 2012 - 15:42 LOD Workshop Invitation

417

Super Sensitive Gas Detector Goes Down the Nanotubes  

Science Conference Proceedings (OSTI)

... When cells are under stress, they blow off steam by releasing minute amounts of nitrogen oxides and other toxic gases. ...

2012-10-10T23:59:59.000Z

418

Thermodynamic and transport property modeling in super critical water  

E-Print Network (OSTI)

Supercritical water oxidation (SCWO) is a thermally-based, remediation and waste-treatment process that relies on unique property changes of water when water is heated and pressurized above its critical point. Above its ...

Kutney, Michael C. (Michael Charles)

2005-01-01T23:59:59.000Z

419

FINAL REPORT ON THE EXPERIMENTAL SUPER, CONDUCTING SYNCHROTRON (ESCAR)  

E-Print Network (OSTI)

operating costs for electrical power, LN feed, maintenance,distribution, refrigerator, electrical power supplies, andhad substantial electrical power, control and instrumentat:

Lambertson, G.R.

2011-01-01T23:59:59.000Z

420

STARTUP DESIGN FEATURES FOR SUPER RITI AL POWER ONVERSION SYSTEMS ...  

owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energys National Nuclear Security Administration. SAND # 2011-6954P TE HNOLOGY

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While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Method for making carbon super capacitor electrode materials  

DOE Patents (OSTI)

A method for making near-net-shape, monolithic carbon electrodes for energy storage devices. The method includes the controlled pyrolysis and activation of a pressed shape of methyl cellulose powder with pyrolysis being carried out in two stages; pre-oxidation, preferably in air at a temperature between 200.degree.-250.degree. C., followed by carbonization under an inert atmosphere. An activation step to adjust the surface area of the carbon shape to a value desirable for the application being considered, including heating the carbon shape in an oxidizing atmosphere to a temperature of at least 300.degree. C., follows carbonization.

Firsich, David W. (Dayton, OH); Ingersoll, David (Albuquerque, NM); Delnick, Frank M. (Dexter, MI)

1998-01-01T23:59:59.000Z

422

Applied Super Conductor Group, Oxide Molecular Beam Epitaxy Group,  

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

AEMG Homepage AEMG Homepage Site Details Homepage Research Publications Presentations Facilities How to Contact Us Other Information Basic Energy Sciences Directorate Links BNL Site Index Can't View PDFs? Advanced Energy Materials Group Applied Superconductivity The applied superconductivity research (past funded by DOE Office of Electricity Delivery and Energy Reliability) is related to modernization of the U.S. power grid. One direction of the modernization is replacement of normal metal (copper, aluminum) transmission lines with High Temperature Superconducting (HTS) cables. Our group concentrates its effort on studying fundamental thermodynamics of nucleation and texture development of thick YBCO layers. High-performance YBCO layer is a critical element of modern second generation (2G) HTS wire.

423

NIST Super-Sensors to Measure 'Signature' of Inflationary ...  

Science Conference Proceedings (OSTI)

... 10 billion times hotter than the energies attainable by ... the early distributions of matter and energy that evolved into the stars and galaxies of ...

2011-11-02T23:59:59.000Z

424

Investigation of Super-Hydrophobic Coatings with Hierarchical ...  

Science Conference Proceedings (OSTI)

The wettability of the modified surfaces was studied by contact angle method and .... Preparation and Characterization on Cellulose Nanofiber Film Preparation...

425

The Effect of Composition on the Shape Memory and Super ...  

Science Conference Proceedings (OSTI)

Development of a SMA-Based Drive Unit for Prehension Orthoses to Support Disabled People Effect of H in Metals and Alloys: An Application to bcc W and NiTi...

426

Tropical Intraseasonal Oscillation, Super Cloud Clusters, and Cumulus Convection Schemes  

Science Conference Proceedings (OSTI)

A new framework for interpreting the origin of the tropical intraseasonal oscillation (TISO), which avoids the speed and scale selection problems in the previous theories, is proposed in this study. In this interpretation TISO is viewed as an ...

Winston C. Chao; Shian-Jiann Lin

1994-05-01T23:59:59.000Z

427

DEPARTMENT OF ENERGY'S SUPER ENERGY SAVINGS PERFORMANCE CONTRACTS...  

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

is facing the most serious energy supply situation since the 1970s. And, current forecasts suggest that the demand for energy is increasing. As one of the largest energy...

428

GE-MOV Varistor The Super Alpha Varistor  

Science Conference Proceedings (OSTI)

... Where explosive environments may be encountered such as in the oil refinery industry, considerable savings can be achieved by eliminating the ...

2013-05-17T23:59:59.000Z

429

Microsoft Word - 2 21 08 DOE-SuperPower.doc  

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

the grid. This 350-meter HTS cable runs between the Riverside and Menands Substations in Albany, New York. HTS cables encounter essentially no resistance in electricity flow,...

430

Super-Index of Encyclopedia of Integer Sequences - CECM  

E-Print Network (OSTI)

... Endomorphism patterns Energy function Engel expansion Enneagonal ... Greatest minimal norm Greedy algorithm Green function Green's function...

431

Automatic prediction of solar flares and super geomagnetic storms.  

E-Print Network (OSTI)

??Space weather is the response of our space environment to the constantly changing Sun. As the new technology advances, mankind has become more and more (more)

Song, Hui

2008-01-01T23:59:59.000Z

432

Super Energy Saver Heat Pump - Oak Ridge National Laboratory  

pump, enables load shifting, and saves electricity Fulfills many attributes recommended for residential and commercial heating and cooling

433

Method for making carbon super capacitor electrode materials  

DOE Patents (OSTI)

A method is described for making near-net-shape, monolithic carbon electrodes for energy storage devices. The method includes the controlled pyrolysis and activation of a pressed shape of methyl cellulose powder with pyrolysis being carried out in two stages; pre-oxidation, preferably in air at a temperature between 200--250 C, followed by carbonization under an inert atmosphere. An activation step to adjust the surface area of the carbon shape to a value desirable for the application being considered, including heating the carbon shape in an oxidizing atmosphere to a temperature of at least 300 C, follows carbonization. 1 fig.

Firsich, D.W.; Ingersoll, D.; Delnick, F.M.

1998-07-07T23:59:59.000Z

434

Energy storage in carbon nanotube super-springs  

E-Print Network (OSTI)

A new technology is proposed for lightweight, high density energy storage. The objective of this thesis is to study the potential of storing energy in the elastic deformation of carbon nanotubes (CNTs). Prior experimental ...

Hill, Frances Ann

2008-01-01T23:59:59.000Z

435

Super-Index of Ramanujan, Modular Equations, and Approximations ...  

E-Print Network (OSTI)

... Fonctions Elliptiques Forcade R.W. Fourier analysis fundamental region ... Gosper W. Gregory's series Guilloud Handbook of Mathematical Functions...

436

Solar neutrinos results and oscillation analysis from SuperKamiokande  

E-Print Network (OSTI)

. Actually different solar neutrino oscillation solutions require the different energy dependece. In addition of the deviation from the expected energy spectrum not only show the definit evidence of the solar neutrino measure the energy spectrum and the time dependence of the solar neu­ trino flux, (day/night or seasonal

Tokyo, University of

437

Method of cleaning plastics using super and subcritical media  

DOE Patents (OSTI)

A method for treating a plastic, such as polyethylene or polypropylene, to remove at least a portion of at least one contaminant includes combining the plastic with a supercritical medium, such as carbon dioxide or sulfur hexafluoride, whereby at least a portion of the contaminant dissolves in the supercritical medium. Alternatively, the plastic can be combined with a suitable liquid medium, such as carbon dioxide or liquid sulfur hexafluoride. At least a portion of the medium, containing the dissolved contaminant, is separated from the plastic, thereby removing at least a portion of the contaminant from the plastic.

Sawan, Samuel P. (Tyngsborough, MA); Spall, W. Dale (Los Alamos, NM); Talhi, Abdelhafid (Nashua, NH)

1998-05-26T23:59:59.000Z

438

Research Support Facility - A Model of Super Efficiency (RSF...  

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

for the U.S. Green Building Council's Leadership in Energy and Environmental Design (LEED) Platinum rating. With 19 percent of the primary energy in the United States consumed...

439

ORNL and SuperPower Sign Superconducting Wire Agreement  

for more efficient transmission of electricity. ... line networks; and increase power-transmission capacity. Second-generation (2G) wires made by

440

Adaptive Multiple Super Fast Simulated Annealing for Stochastic ...  

Science Conference Proceedings (OSTI)

Integrating Advanced Materials Simulation Techniques into an Automated Data Analysis Workflow at the Spallation Neutron Source Intersecting Slip for...

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Ranges of Atmospheric Mass and Composition of Super Earth Exoplanets  

E-Print Network (OSTI)

Terrestrial-like exoplanets may obtain atmospheres from three primary sources: Capture of nebular gases, degassing during accretion, and degassing from subsequent tectonic activity. Here we model degassing during accretion to estimate the range of atmospheric mass and composition on exoplanets ranging from 1 to 30 Earth masses. We use bulk compositions drawn from primitive and differentiated meteorite compositions. Degassing alone can create a wide range of masses of planetary atmospheres, ranging from less than a percent of the planet's total mass up to ~6 mass% of hydrogen, ~20 mass% of water, and/or ~5 mass% of carbon compounds. Hydrogen-rich atmospheres can be outgassed as a result of oxidizing metallic iron with water, and excess water and carbon can produce atmospheres through simple degassing. As a byproduct of our atmospheric outgassing models we find that modest initial water contents (10 mass% of the planet and above) create planets with deep surface liquid water oceans soon after accretion is complete.

L. Elkins-Tanton; S. Seager

2008-08-13T23:59:59.000Z

442

Super-Galilean conformal algebra in AdS/CFT  

Science Conference Proceedings (OSTI)

Galilean conformal algebra (GCA) is an Inoenue-Wigner (IW) contraction of a conformal algebra, while Newton-Hooke string algebra is an IW contraction of an Anti-de Sitter (AdS) algebra, which is the isometry of an AdS space. It is shown that the GCA is a boundary realization of the Newton-Hooke string algebra in the bulk AdS. The string lies along the direction transverse to the boundary, and the worldsheet is AdS{sub 2}. The one-dimensional conformal symmetry so(2,1) and rotational symmetry so(d) contained in the GCA are realized as the symmetry on the AdS{sub 2} string worldsheet and rotational symmetry in the space transverse to the AdS{sub 2} in AdS{sub d+2}, respectively. It follows from this correspondence that 32 supersymmetric GCAs can be derived as IW contractions of superconformal algebras, psu(2,2|4), osp(8|4), and osp(8*|4). We also derive less supersymmetric GCAs from su(2,2|2), osp(4|4), osp(2|4), and osp(8*|2)

Sakaguchi, Makoto [Okayama Institute for Quantum Physics, 1-9-1 Kyoyama, Okayama 700-0015 (Japan)

2010-04-15T23:59:59.000Z

443

Conformal supergravity, twistors, and the super-BMS group  

SciTech Connect

The asymptotic symmetry group of General Relativity is the Bondi-Metzner-Sachs (BMS) group. We find the appropriate supergeneralization of this group for supergravity. The analysis is carried out using properties of the twistor equation and is valid for any space-time dimension.

Awada, M.A.; Gibbons, G.W.; Shaw, W.T.

1986-10-01T23:59:59.000Z

444

Studsvik Super-Ramp-II: 9 x 9 Project  

Science Conference Proceedings (OSTI)

Establishing the pellet-cladding interaction (PCI) failure threshold for 9 x 9 lattice fuel is an important part of demonstrating the suitability of the new design since 9 x 9 lattice fuel was introduced for BWRs to reduce PCI-related fuel failures. In an international program with EPRI participation, the failure threshold of 9 x 9 fuel designs has been determined through ramp testing of fuel rod segments in a test reactor in Sweden.

1992-01-01T23:59:59.000Z

445

NETL: Pilot Test of a Nanoporous, Super-hydrophobic Membrane...  

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

HFC, while a CO2 selective solvent, Hitachi's advanced H3-1, flows on the other side. Carbon dioxide permeates through the hollow fiber membrane pores and is chemically...

446

Super sensitive UV detector using polymer functionalized nanobelts  

SciTech Connect

An ultraviolet light sensor includes an elongated metal oxide nanostructure, a layer of an ultraviolet light-absorbing polymer, a current source and a current detector. The elongated metal oxide nanostructure has a first end and an opposite second end. The layer of an ultraviolet light-absorbing polymer is disposed about at least a portion of the metal oxide nanostructure. The current source is configured to provide electrons to the first end of the metal oxide nanostructure. The current detector is configured to detect an amount of current flowing through the metal oxide nanostructure. The amount of current flowing through the metal oxide nanostructure corresponds to an amount of ultraviolet light impinging on the metal oxide nanostructure.

Wang, Zhong L; Lao, Changshi; Zhou, Jun

2012-10-23T23:59:59.000Z

447

Optimization Online - Projections Onto Super-Half-Spaces for ...  

E-Print Network (OSTI)

Aug 25, 2008 ... Our algorithmic scheme includes the classical projection method and Fukushima's subgradient projection method as special cases. Keywords:...

448

LANL's Top-secret super-secure vault declassified | National...  

National Nuclear Security Administration (NNSA)

version Facebook Twitter Youtube Flickr NNSA Blog October 2013 (1) September 2013 (18) August 2013 (17) July 2013 (20) June 2013 (19) May 2013 (25) April 2013 (17) March 2013...

449

Search for GUT Monopoles at Super-Kamiokande  

E-Print Network (OSTI)

GUT monopoles captured by the Sun's gravitation are expected to catalyze proton decays via the Callan-Rubakov process. In this scenario, protons, which initially decay into pions, will ultimately produce \

The Super-Kamiokande Collaboration; :; K. Ueno; K. Abe; Y. Hayato; T. Iida; K. Iyogi; J. Kameda; Y. Koshio; Y. Kozuma; M. Miura; S. Moriyama; M. Nakahata; S. Nakayama; Y. Obayashi; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takenaga; K. Ueshima; S. Yamada; T. Yokozawa; K. Martens; J. Schuemann; M. Vagins; C. Ishihara; H. Kaji; T. Kajita; K. Kaneyuki; T. McLachlan; K. Okumura; Y. Shimizu; N. Tanimoto; E. Kearns; M. Litos; J. L. Raaf; J. L. Stone; L. R. Sulak; K. Bays; W. R. Kropp; S. Mine; C. Regis; A. Renshaw; M. B. Smy; H. W. Sobel; K. S. Ganezer; J. Hill; W. E. Keig; J. S. Jang; J. Y. Kim; I. T. Lim; J. B. Albert; K. Scholberg; C. W. Walter; R. Wendell; T. Wongjirad; T. Ishizuka; S. Tasaka; J. G. Learned; S. Matsuno; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nishikawa; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; M. Ikeda; A. Minamino; T. Nakaya; L. Labarga; Ll. Marti; Y. Fukuda; Y. Itow; G. Mitsuka; T. Tanaka; C. K. Jung; G. Lopez; I. Taylor; C. Yanagisawa; H. Ishino; A. Kibayashi; S. Mino; T. Mori; M. Sakuda; H. Toyota; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; H. Okazawa; Y. Choi; K. Nishijima; M. Koshiba; Y. Totsuka; M. Yokoyama; S. Chen; Y. Heng; Z. Yang; H. Zhang; D. Kielczewska; P. Mijakowski; K. Connolly; M. Dziomba; E. Thrane; R. J. Wilkes

2012-03-05T23:59:59.000Z

450

SUPER COOL TIPS FOR BEING GREEN AT LSU  

E-Print Network (OSTI)

of the road NOT on the sidewalk (i.e. Bike like a car) Bikes have all the same rights and responsibilities as a car. Lock your bike to a bike rack. DO NOT lock it to a tree, guardrail, or lamppost. The Office. Place your computer in a power save mode to save electricity and money. The EPA recommends setting your

451

Spray-On Super Nanotubes - Materials Technology @ TMS  

Science Conference Proceedings (OSTI)

Apr 25, 2013 ... This new coating material consists of multiwall carbon nanotubes and a ceramic made of silicon, boron, carbon, and nitrogen. Boron boosts the...

452

Ultrafast photo-acoustic spectroscopy of super-cooled liquids  

E-Print Network (OSTI)

Picosecond laser ultrasonic techniques for acoustic wave generation and detection were adapted to probe longitudinal and transverse acoustic waves in liquids at gigahertz frequencies. The experimental effort was designed ...

Klieber, Christoph

2010-01-01T23:59:59.000Z

453

Crabbed Waist Collisions in DAFNE and Super-B Design  

Science Conference Proceedings (OSTI)

The new idea of increasing the luminosity of a collider with crab waist collisions and first experimental results from the DA{Phi}NE {Phi}-Factory at LNF, Frascati, using this concept are presented. Consequences for the design of future factories will be discussed. An outlook to the performance reach with crab waist collisions is given, with emphasis on future B Factories.

Raimondi, P.; Alesini, D.; Biagini, M.E.; Biscari, C.; Boni, R.; Boscolo, M.; Bossi, F.; Buonomo, B.; Clozza, A.; Delle Monache, G.O.; Demma, T.; Di Pasquale, E.; Di Pirro, G.; Drago, A.; Gallo, A.; Ghigo, A.; Guiducci, S.; Ligi, C.; Marcellini, F.; Mazzitelli, Giovanni; Milardi, C.; /Frascati /Orsay, LAL /CERN /Rome III U. /Rome U. /Novosibirsk, IYF /KEK, Tsukuba /INFN, Pisa /INFN, Cosenza /SLAC /Frascati

2011-11-02T23:59:59.000Z

454

Super energy saver heat pump with dynamic hybrid phase change ...  

The at least one outdoor heat exchanger has a phase change material in thermal communication ... Building Energy Efficiency; ... Solar Thermal; Startup America;

455

LANL's Top-secret super-secure vault declassified | National...  

National Nuclear Security Administration (NNSA)

the United States Senate Committee on Armed Services Sep 17, 2013 NNSA, Republic of Korea Ministry Agree to Minimize Use of HEU in Nuclear Reactors Sep 3, 2013 NNSA Conducts...

456

FINAL REPORT ON THE EXPERIMENTAL SUPER, CONDUCTING SYNCHROTRON (ESCAR)  

E-Print Network (OSTI)

4. Thermal insulation region in helium refrigerator cold boxthermal insulation of the magnet cryostats is similar to that of the refrigerator cold

Lambertson, G.R.

2011-01-01T23:59:59.000Z

457

LANL's Top-secret super-secure vault declassified | National...  

National Nuclear Security Administration (NNSA)

LANL declassified the vault this week. BLOG: 1.usa.gov18CVf6K VIDEO: bit.ly169ebnB Facebook Twitter Youtube Flickr Headlines Oct 22, 2013 Workshop Focuses on Combating Illicit...

458

Fusion hierarchies for N = 4 superYang-Mills theory  

E-Print Network (OSTI)

We employ the analytic Bethe Anzats to construct eigenvalues of transfer matrices with finite-dimensional atypical representations in the auxiliary space for the putative long-range spin chain encoding anomalous dimensions of all composite single-trace gauge invariant operators of the maximally supersymmetric Yang-Mills theory. They obey an infinite fusion hierarchy which can be reduced to a finite set of integral relations for a minimal set of transfer matrices. This set is used to derive a finite systems of functional equations for eigenvalues of nested Baxter polynomials.

A. V. Belitsky

2008-03-13T23:59:59.000Z

459

Researh On Microstructures and Properties of 780MPa Grade Super ...  

Science Conference Proceedings (OSTI)

Analysis of Residence Time Distribution (RTD) of Fluid Flows in a Four Strand Delta-shaped Tundish Operating Under Isothermal and Non-isothermal...

460

Ranking the Susceptibility to Hydrogen-assisted Cracking in Super ...  

Science Conference Proceedings (OSTI)

Thus, SDSS welds are exposed to hydrogen charging to under CP. There have been reported hydrogen assisted cracking (HAC) failures in SDSS welds during...

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Columbia Water & Light - Commercial Super Saver Loans (Missouri...  

Open Energy Info (EERE)

Low Emission Development Strategies Oil & Gas Smart Grid Solar U.S. OpenLabs Utilities Water Wind Page Actions View form View source History View New Pages Recent Changes All...

462

Columbia Water & Light - Residential Super Saver Loans (Missouri...  

Open Energy Info (EERE)

Low Emission Development Strategies Oil & Gas Smart Grid Solar U.S. OpenLabs Utilities Water Wind Page Actions View form View source History View New Pages Recent Changes All...

463

BNL VERY LONG BASELINE EXPERIMENT WITH A SUPER NEUTRINO BEAM.  

SciTech Connect

An upgrade to the BNL AGS could produce a very intense proton source at a relatively low cost. This proton source could produce a conventional neutrino beam with a very significant flux at large distances from the laboratory. In this paper we examine the possibility of using this neutrino beam for a very long baseline oscillation experiment where a 500 kiloton water Cherenkov detector is situated at the Homestake mine in South Dakota. We study the physics potential of a high intensity neutrino oscillation experiment with a 2540 km baseline and a peak neutrino energy of {approx}1 GeV.

KAHN,S.A.

2003-11-18T23:59:59.000Z

464

Super Phos esters: the key to higher-performance products  

Science Conference Proceedings (OSTI)

Robert L. Reierson, winner of the 2012 Samuel Rosen Memorial Award recognizing accomplishments in surfactant chemistry, describes how phosphation process control makes it possible to systematically design and adjust product compositions to deliver maximum

465

Example Measurement & Verification Plan for a Super ESPC Project  

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

in Table 1-1. Table 1-1: Proposed Annual Savings Summary ECM Electric energy savings (kWhyr) Electric demand savings (kW-yr)* Natural gas savings (therms) Water savings...

466

SuperShuttle Reservation Confirmation Thank you Axel Brandenburg. Your reservation with SuperShuttle has been saved.  

E-Print Network (OSTI)

a 3.5 cent per gallon surcharge on fuel credit card transactions to cover the cost of the fuel card N/A N/A 779.00 New for FY 09: * Due to the volatility of fuel prices, the mileage rates for the rental fleet may be adjusted quarterly to reflect current fuel prices. * We will begin charging a per

Brandenburg, Axel

467

energy | OpenEI Community  

Open Energy Info (EERE)

energy energy Home Future of Condition Monitoring for Wind Turbines Description: Research into third party software to aid in the development of better CMS in order to raise turbine efficiency We endeavor to build new software over existing SCADA and sensor data to simplify and ameliorate the existing condition/health monitoring of deployed wind turbines. We are seeking partners and contributors to aid in our search for real data sets in order to test our hypothesis! energy software turbine Wind Graham7781's picture Submitted by Graham7781(1992) Super contributor 26 June, 2013 - 09:17 NREL's Energy Databus storing big energy data campus databus energy meter data NREL OpenEI Tool The Energy Databus began as a project aimed at addressing campus energy consumption and tracking issues at NREL. Now, with the ability to store

468

OpenEI Building Social Media Networks | OpenEI Community  

Open Energy Info (EERE)

Building Social Media Networks Building Social Media Networks Home > Groups > OpenEI Community Central Graham7781's picture Submitted by Graham7781(1992) Super contributor 16 February, 2010 - 14:44 imported OpenEI As OpenEI continues to expand and grow thanks to contributions from users, so grows the OpenEI social media network. Multiple social media outlets are employed by OpenEI to help further grow a dynamic community of contributors. This community is vital to the success of OpenEI. Here are the social media outlets being used by OpenEI. We encourage that everyone join in the discussion. OpenEI Blog: The blog is the 'home' of our social media links. It is the place to find articles of information about what's going on at OpenEI.org. It is also the place to link to other social media outlets.

469

Suburbs offset Low Carbon Footprint of major U.S. Cities | OpenEI Community  

Open Energy Info (EERE)

Suburbs offset Low Carbon Footprint of major U.S. Cities Suburbs offset Low Carbon Footprint of major U.S. Cities Home > Blogs > Graham7781's blog Graham7781's picture Submitted by Graham7781(2002) Super contributor 9 January, 2014 - 13:12 carbon cities CO2 emissions OpenEI suburbs US New research from the University of California-Berkeley shows that those who live in cities in the United States have significantly smaller per-capita carbon footprints than their suburban counterparts. The difference is such that suburban dwellers essentially offset the low carbon footprints of urban dwellers. Vehicle emissions accounted for the biggest contributor to carbon dioxide, accounted by longer commutes to work, school, and shopping. The data, balancing 37 factors such as weather, income, home size, shows that those dwelling in major cities have a carbon footprint about 50 percent below the

470

NETL Engineer Uses OpenEI to Publicize Energy R&D | OpenEI Community  

Open Energy Info (EERE)

NETL Engineer Uses OpenEI to Publicize Energy R&D NETL Engineer Uses OpenEI to Publicize Energy R&D Home > Groups > OpenEI Community Central Graham7781's picture Submitted by Graham7781(1992) Super contributor 18 February, 2010 - 10:01 imported OpenEI Justin Weber believes in the power of open energy information. He's using OpenEI to publicize energy R&D at the National Energy Technology Laboratory (NETL)-where he works as a mechanical engineer-and encouraging others within NETL to do so as well. Justin learned about OpenEI from Secretary of Energy Chu's December 2009 press release. Soon, he became one of OpenEI's earliest and most active contributors. He has added information about NETL and several of its R&D areas: National Energy Technology Laboratory Chemical Looping Energy Storage Compressed Air Energy Storage

471

OECD | OpenEI Community  

Open Energy Info (EERE)

OECD OECD Home Graham7781's picture Submitted by Graham7781(2002) Super contributor 16 July, 2013 - 14:37 Four new publications help advance renewable energy development energy scenarios fossil fuels OECD OpenEI policy Renewable Energy Four publications giving guidance to policy and decision makers on particular challenges facing renewable energy deployment were released yesterday. As renewable energy becomes more competitive with fossil fuels in OECD countries, reports of this nature can go a long way to supporting more and more development. The four new reports in short: Wzeng's picture Submitted by Wzeng(50) Contributor 8 August, 2012 - 12:37 New Gapminder Visualizations Added! EIA Energy data Gapminder OECD OpenEI SEDS Visualization Graph OpenEI now features some cool new Gapminder Visualizations for users to

472

Slide 1  

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

Secure Planning and Secure Planning and Operations of Systems with Stochastic Sources, Energy Storage and Active Demand Ray Zimmerman, Carlos Murillo-Sánchez, Bob Thomas CERTS Review, Cornell University August 6-7, 2013 Other Contributors * Input scenario creation and analysis - C. Lindsay Anderson (Cornell) - Amandeep Gupta (Cornell) - Jung Mo (Cornell) - Tim Mount (Cornell) - Laurie Tupper (Cornell) * Simulation environment and testing - Daniel Muñoz-Álvarez (Cornell) - Wooyoung Jeon (Cornell) - Alberto Lamadrid (Lehigh) * MATPOWER - Shrirang Abhyankar (Argonne) - Alexander J. Flueck (IIT) - Daniel Molzahn (U Wisc/Madison) - MATPOWER user base (worldwide) 2 Outline * Overview of Tools * MATPOWER * SuperOPF Planning Tool * Multiperiod SuperOPF (2 nd gen) - especially storage model

473

Power Politics: The Political Economy of Russia's Electricity Sector Liberalization  

E-Print Network (OSTI)

2002 and Burgansky, "Hydro Power: Super-Profits or Super-Burgansky, Alexander. "Hydro Power: Super-Profits or Super-Alexander Burgansky, "Hydro Power: Super-Profits or Super-

Wenle, Susanne Alice

2010-01-01T23:59:59.000Z

474

What can super-parameterization teach us about the tropical climate system?  

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

Presented by... Presented by... Dr. David Randall Professor of Atmospheric Science, Colorado State University Director of the Center for Multiscale Modeling of Atmospheric Processes Chief Editor of the Journal of Advances in Modeling Earth Systems (JAMES) Coordinating Lead Author for the Fifth Assessment of the Intergovernmental Panel on Climate Change (IPCC) Awards:  NASA's Medal for Exceptional Scientific Achievement  Meisinger Award of the American Meteorological Society  NASA's Medal for Distinguished Public Service  Colorado State University for Scholarship Impact, Research, and Graduate Advising Fellow of:  The American Meteorological Society,

475

NETL: Pilot Test of a Nanoporous, Super-hydrophobic Membrane Contactor  

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

Pilot Scale Evaluation of an Advanced Carbon Sorbent-Based Process for Post-combustion CO2 Capture Pilot Scale Evaluation of an Advanced Carbon Sorbent-Based Process for Post-combustion CO2 Capture Project No.: DE-FE00013123 SRI is incorporating an advanced carbon capture sorbent-based process in a 1 MWe slipstream pilot plant that will reduce the parasitic plant load by using a CO2 capture sorbent requiring a reduced amount of steam. The process is based on advanced carbon sorbents having a low heat of adsorption, high CO2 adsorption capacity, and excellent selectivity. Design and performance data will be produced by testing the sorbent using the slipstream from an operating pulverized coal (PC)-fired boiler under realistic conditions and continuous long-term operation. The acquired data will be used for further development and commercialization of the process.

476

Structure and Elastic Properties of Ni3Al Based Super Alloys under ...  

Science Conference Proceedings (OSTI)

Influence of Different Cooling Structure on Surface Crack of HSLA Steel Plate by ... of Si3N4-SiC Heat Absorption Ceramic Material Used for Tower Type Solar...

477

First LIGO search for gravitational wave bursts from cosmic (super)strings  

Science Conference Proceedings (OSTI)

We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LIGO data from the fourth science run (S4) which took place in February and March 2005. No gravitational waves were detected in 14.9 days of data from times when all three LIGO detectors were operating. We interpret the result in terms of a frequentist upper limit on the rate of gravitational wave bursts and use the limits on the rate to constrain the parameter space (string tension, reconnection probability, and loop sizes) of cosmic string models. Many grand unified theory-scale models (with string tension G{mu}/c{sup 2}{approx_equal}10{sup -6}) can be ruled out at 90% confidence for reconnection probabilities p{<=}10{sup -3} if loop sizes are set by gravitational back reaction.

Abbott, B. P.; Abbott, R.; Adhikari, R.; Anderson, S. B.; Araya, M.; Armandula, H.; Aso, Y.; Ballmer, S.; Barton, M. A.; Betzwieser, J.; Billingsley, G.; Black, E.; Blackburn, J. K.; Bork, R.; Boschi, V.; Brooks, A. F.; Cannon, K. C.; Cardenas, L.; Cepeda, C.; Chalermsongsak, T. [LIGO-California Institute of Technology, Pasadena, California 91125 (United States)] (and others)

2009-09-15T23:59:59.000Z

478

PROJECTED CONSTRAINTS ON THE COSMIC (SUPER)STRING TENSION WITH FUTURE GRAVITATIONAL WAVE DETECTION EXPERIMENTS  

SciTech Connect

We present projected constraints on the cosmic string tension, G{mu}/c {sup 2}, that could be achieved by future gravitational wave detection experiments and express our results as semi-analytic relations of the form G{mu}({Omega}{sub gw} h {sup 2})/c {sup 2}, to allow for direct computation of the tension constraints for future experiments. These results can be applied to new constraints on {Omega}{sub gw} h {sup 2} as they are imposed. Experiments operating in different frequency bands probe different parts of the gravitational wave spectrum of a cosmic string network and are sensitive to different uncertainties in the underlying cosmic string model parameters. We compute the gravitational wave spectra of cosmic string networks based on the one-scale model, covering all the parameter space accessed by each experiment that is strongly dependent on the birth scale of loops relative to the horizon, {alpha}. The upper limits on the string tension avoid any assumptions on the model parameters. We perform this investigation for Pulsar Timing Array experiments of different durations, as well as ground-based and space-borne interferometric detectors.

Sanidas, Sotirios A.; Battye, Richard A.; Stappers, Benjamin W., E-mail: sotiris.sanidas@gmail.com, E-mail: rbattye@jb.man.ac.uk, E-mail: ben.stappers@manchester.ac.uk [Jodrell Bank Centre for Astrophysics, University of Manchester, Manchester, M13 9PL (United Kingdom)

2013-02-10T23:59:59.000Z

479

Super-hot (T > 30 MK) Thermal Plasma in Solar Flares  

E-Print Network (OSTI)

Solar X-ray Spectrometer SolarSoftWare (IDL package) soft X-SolarViews.org) ena. (Image credit: SolarViews.org) servations of such a

Caspi, Amir

2010-01-01T23:59:59.000Z

480

Scheduling the SSC (Superconducting Super Collider) construction as of March 1990  

SciTech Connect

The scheduling of the construction activities for the SSC Project involves two major concurrent emphases on design, construction, installation, and test. These two major activities include the completion of the construction project by the end of FY98 and industrially produced magnet tests by the end of FY92. Scheduling of the construction activities is further complicated by the fact that the baseline cost and schedule is still under review and negotiation with the Department of Energy and the currently anticipated funding for FY91 is somewhat less than originally requested. However, with the above limitations, the schedules presented herein are the most current at this time.

Kozman, T.

1990-07-01T23:59:59.000Z

Note: This page contains sample records for the topic "graham77811987 super contributor" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

ACTIVE CATHODES FOR SUPER-HIGH POWER DENSITY SOLID OXIDE FUEL CELLS THROUGH SPACE CHARGE EFFECTS  

DOE Green Energy (OSTI)

This report summarizes the work done during the eleventh quarter of the project. Conductivity relaxation experiments were conducted on porous La{sub 0.5}Sr{sub 0.5}CoO{sub (3-{delta})} (LSC50) samples over a temperature range from 350 to 750 C, and over an oxygen partial pressure, p{sub O{sub 2}}, switch between 0.04 and 0.06 atm in order to determine the surface exchange coefficient, k{sub chem}. The normalized conductivity data could be fitted to a first order kinetic equation. The time constant decreased with decreasing temperature between {approx}750 and {approx}450 C, but sharply increased with decreasing temperature between 450 and 350 C. The corresponding k{sub chem} was estimated using three models: (a) A porous body model wherein it is assumed that the kinetics of surface exchange is the slowest. (b) Solution to the diffusion equation assuming the particles can be approximated as spheres. (c) Solution to the diffusion equation assuming the particles can be approximated as cylinders. The values of k{sub chem} ob