National Library of Energy BETA

Sample records for belt public power

  1. Dotiki saves money and time with power tool and belt fasteners

    SciTech Connect (OSTI)

    Bargo, K.

    2009-11-15

    The use of a Hilti power tool to improve belt splice installations to minimise downtime is described. 3 photos.

  2. 3MTM Air-MateTM Belt Mounted High Efficiency Powered Air Purifying Respirator (PAPR)

    E-Print Network [OSTI]

    Acton, Scott

    3MTM Air-MateTM Belt Mounted High Efficiency Powered Air Purifying Respirator (PAPR) Welcome and thank you for choosing the 3MTM Air-MateTM Belt Mounted High Efficiency Powered Air Purifying Respirator text #12;Double click picture to start video Click button to view video text #12;3MTM Air-MateTM Belt

  3. Work Force Planning for Public Power Utilities

    E-Print Network [OSTI]

    Work Force Planning for Public Power Utilities: Ensuring Resources to Meet Projected.............................................................................20 #12;ii Work Force Planning for Public Power Utilities #12;1 Work Force Planning for Public Power as a result of the aging work force; and · Public power utilities need to do more to plan for their future

  4. Wheat Belt Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop IncIowa (Utility Company)Idaho)VosslohWest Plains ElectricElectricCountyWhat

  5. NREL: Water Power Research - Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines lightGeospatial ToolkitSMARTSWorkingManagement ModelsPublications Access

  6. Public speaking arouses implicit power motivation 1 Running head: Public speaking arouses implicit power motivation

    E-Print Network [OSTI]

    Schultheiss, Oliver C.

    Public speaking arouses implicit power motivation 1 Running head: Public speaking arouses implicit power motivation Public speaking in front of an unreceptive audience increases implicit power motivation: Oliver.Schultheiss@fau.de #12;Public speaking arouses implicit power motivation 2 Abstract The present

  7. Third-Party Financing and Power Purchase Agreements for Public...

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

    & Publications Third Party Financing and Power Purchasing Agreements for Public Sector PV Projects Third-Party Financing and Power Purchase Agreements for Public Sector PV...

  8. Belt conveyors for bulk materials. 6th ed.

    SciTech Connect (OSTI)

    NONE

    2007-07-01

    The 16 chapters are entitled: Belt conveyor general applications economics; Design considerations; Characteristics and conveyability of bulk materials; Capacities, belt widths and speeds; Belt conveyor idlers; Belt tension and power engineering; Belt selection; Pulleys and shafts; Curves; Steep angle conveying; Belt cleaners and accessories; Transfer points; Conveyor motor drives and controls; Operation, maintenance and safety; Belt takeups; and Emerging technologies. 6 apps.

  9. Replace V-Belts with Notched or Synchronous Belt Drives

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

    A properly designed belt power-transmission system offers high efficiency and low noise, requires no lubrication, and presents low maintenance requirements. However, certain...

  10. SLH Timing Belt Powertrain

    SciTech Connect (OSTI)

    Schneider, Abe

    2014-04-09

    The main goal of this proposal was to develop and test a novel powertrain solution for the SLH hydroEngine?, a low-cost, efficient low-head hydropower technology. Nearly two-thirds of U.S. renewable electricity is produced by hydropower (EIA 2010). According to the U.S. Department of Energy; this amount could be increased by 50% with small hydropower plants, often using already-existing dams (Hall 2004). There are more than 80,000 existing dams, and of these, less than 4% generate power (Blankinship 2009). In addition, there are over 800 irrigation districts in the U.S., many with multiple, non-power, low-head drops. These existing, non-power dams and irrigation drops could be retrofitted to produce distributed, baseload, renewable energy with appropriate technology. The problem is that most existing dams are low-head, or less than 30 feet in height (Ragon 2009). Only about 2% of the available low-head hydropower resource in the U.S. has been developed, leaving more than 70 GW of annual mean potential low-head capacity untapped (Hall 2004). Natel Energy, Inc. is developing a low-head hydropower turbine that operates efficiently at heads less than 6 meters and is cost-effective for deployment across multiple low-head structures. Because of the unique racetrack-like path taken by the prime-movers in the SLH, a flexible powertrain is required. Historically, the only viable technological solution was roller chain. Despite the having the ability to easily attach blades, roller chain is characterized by significant drawbacks, including high cost, wear, and vibration from chordal action. Advanced carbon-#12;fiber-reinforced timing belts have been recently developed which, coupled with a novel belt attachment system developed by Natel Energy, result in a large reduction in moving parts, reduced mass and cost, and elimination of chordal action for increased fatigue life. The work done in this project affirmatively addressed each of the following 3 major uncertainties concerning a timing-belt based hydroEngine ?powertrain: 1. Can a belt handle the high torques and power loads demanded by the SLH? (Yes.) 2. Can the SLH blades be mounted to belt with a connection that can withstand the loads encountered in operation? (Yes.) 3. Can the belt, with blade attachments, live through the required cyclic loading? (Yes.) The research adds to the general understanding of sustainable small hydropower systems by using innovative system testing to develop and demonstrate performance of a novel powertrain solution, enabling a new type of hydroelectric turbine to be commercially developed. The technical effectiveness of the methods investigated has been shown to be positive through an extensive design and testing process accommodating many constraints and goals, with a major emphasis on high cycle fatigue life. Economic feasibility of the innovations has been demonstrated through many iterations of design for manufacturability and cost reduction. The project is of benefit to the public because it has helped to develop a solution to a major problem -- despite the large available potential for new low-head hydropower, high capital costs and high levelized cost of electricity (LCOE) continue to be major barriers to project development. The hydroEngine? represents a significant innovation, leveraging novel fluid mechanics and mechanical configuration to allow lower-cost turbine manufacture and development of low head hydropower resources.

  11. Idaho Public Utilities Commission Approves Neal Hot Springs Power...

    Open Energy Info (EERE)

    Idaho Public Utilities Commission Approves Neal Hot Springs Power Purchase Agreement Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: Idaho Public...

  12. Howard Baker Center for Public Policy Nuclear Power Conference...

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

    Howard Baker Center for Public Policy Nuclear Power Conference Howard Baker Center for Public Policy Nuclear Power Conference October 4, 2007 - 3:14pm Addthis Remarks as Prepared...

  13. ForPeerReview PUBLIC ACCEPTANCE OF OFFSHORE WIND POWER

    E-Print Network [OSTI]

    Firestone, Jeremy

    ForPeerReview PUBLIC ACCEPTANCE OF OFFSHORE WIND POWER PROJECTS IN THE UNITED STATES Journal: Wind, Andrew; Minerals Management Service Keywords: offshore wind power, public opinion, social acceptancePeerReview 1 PUBLIC ACCEPTANCE OF OFFSHORE WIND POWER PROJECTS IN THE UNITED STATES Jeremy Firestone*, Willett

  14. NREL: Concentrating Solar Power Research - Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on771/6/14 Contact:News ReleasesChemicalPilotData andPublications

  15. Perennial Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc Jump to:Newberg,Energy LLC Jump to:3 ofAltosPenoyerPerennial Public Power Dist

  16. NEBRASKA PUBLIC POWER DISTRICT CUSTOMER MEETING ON ENERGY ALTERNATIVES

    E-Print Network [OSTI]

    customers value solar power? ..................................................................20 CumulativeNEBRASKA PUBLIC POWER DISTRICT CUSTOMER MEETING ON ENERGY ALTERNATIVES SUMMARY OF RESULTS August 19 megawatts of wind power would you like to see NPPD build by the year 2010

  17. QER- Comment of Large Public Power Council 1

    Broader source: Energy.gov [DOE]

    Attached are the Comments of the Large Public Power Council on the QER. Please feel to contact me if you have any questions.

  18. Omaha Public Power District- Commercial Energy Efficiency Rebate Programs

    Office of Energy Efficiency and Renewable Energy (EERE)

    Omaha Public Power District (OPPD) offers incentives for commercial and industrial customers to install energy-efficient heat pumps and replace/retrofit existing lighting systems. The Commercial...

  19. Appendix S-50 - Power Purchase Agreement (PPA) - Public Utilities...

    Open Energy Info (EERE)

    Appendix S-50 - Power Purchase Agreement (PPA) - Public Utilities Commission Jump to: navigation, search OpenEI Reference LibraryAdd to library PermittingRegulatory Guidance -...

  20. Wind Power Siting: Public Acceptance and Land Use

    Wind Powering America (EERE)

    by the Alliance for Sustainable Energy, LLC. Wind Power Siting: Public Acceptance and Land Use Suzanne Tegen WINDExchange Webinar June 17, 2015 2 Overview * Current NREL Research *...

  1. Synchronous and Cogged Fan Belt Performance Assessment

    SciTech Connect (OSTI)

    Cutler, D.; Dean, J.; Acosta, J.

    2014-02-01

    The GSA Regional GPG Team commissioned the National Renewable Energy Laboratory (NREL) to perform monitoring of cogged V-belts and synchronous belts on both a constant volume and a variable air volume fan at the Byron G. Rodgers Federal Building and U.S. Courthouse in Denver, Colorado. These motor/fan combinations were tested with their original, standard V-belts (appropriately tensioned by an operation and maintenance professional) to obtain a baseline for standard operation. They were then switched to the cogged V-belts, and finally to synchronous belts. The power consumption by the motor was normalized for both fan speed and air density changes. This was necessary to ensure that the power readings were not influenced by a change in rotational fan speed or by the power required to push denser air. Finally, energy savings and operation and maintenance savings were compiled into an economic life-cycle cost analysis of the different belt options.

  2. Custer Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LISTStar EnergyLawler,CoalConcordiaConsumerLEDS TierCristalinoCuivre RiverRuralPublic

  3. Michigan Public Power Agency | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource HistoryScenariosMarysville MtMedical Area TotalWindMicheln Jump to:Michigan Public

  4. Electric power plant emissions and public health

    SciTech Connect (OSTI)

    O'Connor, A.B.; Roy, C.

    2008-02-15

    The generation of electric power is one important source of pollutants such as mercury, sulfur dioxide, nitrogen oxides, and fine particulate matter that can affect the respiratory, cardiovascular, and central nervous systems and cause pregnancy complications. But protecting people from environmental health hazards has become increasingly complex. Air pollutants are often invisible and travel many miles virtually undetected. Nurses can play a critical role in preventive strategies, as well as in the national debate on energy production and dependence on fossil fuels.

  5. Nebraska Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo, Maryland:NPI Ventures Ltd Jump to:InformationNdunga Geothermal Power

  6. Norris Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc Jump to:Newberg, Oregon: EnergyNongqishi Electric PowerHandels GmbHNorris

  7. Laterally bendable belt conveyor

    DOE Patents [OSTI]

    Peterson, William J. (Coraopolis, PA)

    1985-01-01

    An endless, laterally flexible and bendable belt conveyor particularly adapted for coal mining applications in facilitating the transport of the extracted coal up- or downslope and around corners in a continuous manner is disclosed. The conveying means includes a flat rubber belt reinforced along the middle portion thereof along which the major portion of the belt tension is directed so as to cause rotation of the tubular shaped belt when trammed around lateral turns thus preventing excessive belt bulging distortion between adjacent belt supports which would inhibit belt transport. Pretension induced into the fabric reinforced flat rubber belt by conventional belt take-up means supports the load conveyed when the belt conveyor is making lateral turns. The carrying and return portions of the belt are supported and formed into a tubular shape by a plurality of shapers positioned along its length. Each shaper is supported from above by a monorail and includes clusters of idler rollers which support the belt. Additional cluster rollers in each shaper permit the belt supporting roller clusters to rotate in response to the belt's operating tension imposed upon the cluster rollers by induced lateral belt friction forces. The freely rotating roller clusters thus permit the belt to twist on lateral curves without damage to itself while precluding escape of the conveyed material by effectively enclosing it in the tube-shaped, inner belt transport length.

  8. Review of Historical and Modern Utilization of Wind Power Publications Department

    E-Print Network [OSTI]

    Review of Historical and Modern Utilization of Wind Power Publications Department publications Review of Historical and Modern Utilization of Wind Power Per Dannemand Andersen, Ph.D. Content INTRODUCTION THE HISTORY OF WIND POWER q Wind Power in Denmark APPLICATIONS OF WIND POWER WIND POWER

  9. February 10, 2010 - Public Power Open Session | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: AlternativeCommunication3-EDepartmentExerciseCarbon4 LDRDFebruary 10, 2010 - Public Power Open

  10. Belt Vision Inspection System

    Broader source: Energy.gov [DOE]

    Mining operations rely on conveyor belts to move mined material from the working face of the mine to a processing plant. When a conveyor belt breaks or stops for unscheduled maintenance, production...

  11. QER- Comment of American Public Power Association 1

    Broader source: Energy.gov [DOE]

    Attached are the American Public Power Association 's (APPA) statement for the April 11 QER public meeting, Duane Highley's statement for the same meeting since we reference it, and Sue Kelly's (APPA President & CEO) testimony from last Thursday's (April 10) Senate Energy and Natural Resources Committee hearing entitled "Keeping the Lights On – Are We Doing Enough to Ensure the Reliability and Security of the US Electric Grid?" since her testimony covers everything in regards to this meeting. Thank you in advance for your consideration of our attached documents for the QER. Please let me know if you have any questions. Best, Seth Seth Voyles Director, Government Relations 1875 Connecticut Ave., NW, Suite 1200, Washington, D.C. 20009-5715 www.publicpower.org

  12. McCook Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo, Maryland: Energy Resources Jump to: navigation, search EquivalentEnergyMcConePublic Power

  13. Loup River Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LISTStar2-0057-EAInvervarLeeds, UnitedLibertyLiteHuixinEnergyLorain-MedinaPublic Power

  14. M.P. BELT DETERIORATION. ACCELERATOR STRUCTURE. BELT CAPABILITY

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1375 M.P. BELT DETERIORATION. ACCELERATOR STRUCTURE. BELT CAPABILITY M. LETOURNEL Centre de.P. belt deterioration is proposed. It takes into account the strain of discharge to which the belt is submitted following the combination, first of a too high belt charge density in addition to the machine

  15. Congressional panel makes recommendations on belt safety

    SciTech Connect (OSTI)

    Fiscor, S.

    2007-12-15

    The Mine Improvement and New Emergency Response Act of 2006 (MINER Act) called for a Technical Study Panel to present a review and make recommendations on the use of belt air and the composition and fire retardant properties of belt materials in underground coal mining. In October 2007 the Panel released 20 recommendations publicly. These are presented in the article. Many recommendations encouraged the MSHA to enforce existing laws of maintenance and fire protection or example more vigorously. Maybe the biggest change recommended was that the industry should adopt the Belt Evaluation Laboratory Test (BELT) standard proposed in 1992. Another important recommendation was one that would help eliminate hazards associated with point feeding. 1 photo.

  16. The Gould Belt

    E-Print Network [OSTI]

    Bobylev, V V

    2015-01-01

    This review is devoted to studies of the Gould belt and the Local system. Since the Gould belt is the giant stellar-gas complex closest to the sun, its stellar component is characterized, along with the stellar associations and diffuse clusters, cold atomic and molecular gas, high-temperature coronal gas, and dust contained in it. Questions relating to the kinematic features of the Gould belt are discussed and the most interesting scenarios for its origin and evolution are examined.

  17. The Possible Belts for Extrasolar Planetary Systems

    E-Print Network [OSTI]

    Ing-Guey Jiang; M. Duncan; D. N. C. Lin

    2006-10-30

    More than 100 extrasolar planets have been discovered since 1990s. Different from the solar system, these planets' orbital eccentricities cover a huge range from 0 to 0.7. Incidently, the first Kuiper Belt Object was discovered in 1992. Thus, an interesting and important question will be whether extrasolar planetary systems could have structures like Kuiper Belt or asteroid belt. We investigate the stability of these planetary systems with different orbital eccentricities by the similar procedures in Rabl & Dvorak (1988) and Holman & Wiegert (1999). We claim that most extrasolar planetary systems can have their own belts at the outer regions. However, we find that the orbits with high--eccentricity is very powerful in depletion of these populations.

  18. Binaries in the Kuiper Belt

    E-Print Network [OSTI]

    Noll, KS; Grundy, WM; Chiang, EI; Margot, J-L; Kern, SD

    2007-01-01

    The relative sizes of Kuiper Belt binaries. Bull. Amer. As-density for binary Kuiper belt object (26308) 1998 SM 165 .the satellite of Kuiper Belt object 2003 EL 61 . Astrophys.

  19. Public Opinions of Building Additional High-Voltage Electric Power Lines

    E-Print Network [OSTI]

    Tesfatsion, Leigh

    Public Opinions of Building Additional High-Voltage Electric Power Lines A Report to the National-Voltage Electric Power Lines: A Report to the National Science Foundation and the Electric Power Research Center to build new power lines. Residents living in counties with planned routes for new transmission lines

  20. VALUING PUBLIC PREFERENCES FOR OFFSHORE WIND POWER: A CHOICE EXPERIMENT APPROACH

    E-Print Network [OSTI]

    Firestone, Jeremy

    VALUING PUBLIC PREFERENCES FOR OFFSHORE WIND POWER: A CHOICE EXPERIMENT APPROACH by Andrew D. Krueger All Rights Reserved #12;ii VALUING PUBLIC PREFERENCES FOR OFFSHORE WIND POWER: A CHOICE EXPERIMENT thank you for your perspective on offshore renewable energy regulation. As committee members, your

  1. Setting Confidence Belts

    E-Print Network [OSTI]

    Byron P. Roe; Michael B. Woodroofe

    2000-10-13

    We propose using a Bayes procedure with uniform improper prior to determine credible belts for the mean of a Poisson distribution in the presence of background and for the continuous problem of measuring a non-negative quantity $\\theta$ with a normally distributed measurement error. Within the Bayesian framework, these belts are optimal. The credible limits are then examined from a frequentist point of view and found to have good frequentist and conditional frequentist properties.

  2. Microsoft PowerPoint - Public Information Forum Presentation...

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

    14 1 Transmission & Ancillary Services Formula Rates Public Information Forums November 19, 2014 - Omaha, NE November 20, 2014 - Fargo, ND Introductions * Lloyd Linke - Operations...

  3. Microsoft PowerPoint - Final CLWR SEIS PUBLIC SCOPING PRESENTATION...

    National Nuclear Security Administration (NNSA)

    for the Production of Tritium in a Commercial Light Water Commercial Light Water Reactor Public Scoping Meeting October 20 2011 October 20, 2011 National Nuclear Security...

  4. Belt conveyor apparatus

    DOE Patents [OSTI]

    Oakley, David J. (Richland, WA); Bogart, Rex L. (Kennewick, WA)

    1987-01-01

    A belt conveyor apparatus according to this invention defines a conveyance path including a first pulley and at least a second pulley. An endless belt member is adapted for continuous travel about the pulleys and comprises a lower portion which engages the pulleys and an integral upper portion adapted to receive objects therein at a first location on said conveyance path and transport the objects to a second location for discharge. The upper belt portion includes an opposed pair of longitudinally disposed crest-like members, biased towards each other in a substantially abutting relationship. The crest-like members define therebetween a continuous, normally biased closed, channel along the upper belt portion. Means are disposed at the first and second locations and operatively associated with the belt member for urging the normally biased together crest-like members apart in order to provide access to the continuous channel whereby objects can be received into, or discharged from the channel. Motors are in communication with the conveyance path for effecting the travel of the endless belt member about the conveyance path. The conveyance path can be configured to include travel through two or more elevations and one or more directional changes in order to convey objects above, below and/or around existing structures.

  5. QER- Comment of American Public Power Association 3

    Broader source: Energy.gov [DOE]

    Attached are APPA’s comments for the Second public QER meeting. I have tried to submit these before too, so please send me a confirmation e-mail. Thanks in advance for your consideration of my request.

  6. Third Party Financing and Power Purchasing Agreements for Public Sector PV Projects

    Office of Energy Efficiency and Renewable Energy (EERE)

    Provides information on third-party financing and Power Purchase Agreements for public sector PV projects presented at the TAP Web Seminar on May 27, 2009, includes economic and legal information.

  7. KUIPER BELT OBJECTS David Jewitt

    E-Print Network [OSTI]

    Jewitt, David C.

    KUIPER BELT OBJECTS David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 BELT OBJECTS Dec 24 1998 Send Proofs to: David Jewitt Institute for Astronomy, 2680 Woodlawn Drive for Annual Reviews of Earth and Planetary Science. #12; Annual Reviews: Kuiper Belt Page 2 CONTENTS Abstract

  8. Energy Policy 35 (2007) 15841598 Public opinion about large offshore wind power: Underlying factors

    E-Print Network [OSTI]

    Firestone, Jeremy

    2007-01-01

    Energy Policy 35 (2007) 1584­1598 Public opinion about large offshore wind power: Underlying opinion regarding offshore wind power based on a survey of residents near a proposed development off Cape, the first offshore wind proposal in North America, in Nantucket Sound (MA, USA) has generated a strong

  9. Carbon Dioxide Footprint of the Northwest Power System Comments submitted by Grant County Public Utility District

    E-Print Network [OSTI]

    Carbon Dioxide Footprint of the Northwest Power System Comments submitted by Grant County Public paper: Carbon Dioxide Footprint of the Northwest Power System, dated September 13, 2007. The Grant done a very thorough job of assessing the current and future carbon dioxide footprints of the Northwest

  10. Burt County Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION JEnvironmentalBowerbank, Maine: EnergyEnergyOhio:InformationBurnham, Illinois:BurrCounty Public

  11. Microsoft PowerPoint - Secondary Revenue Public Process.pptx

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on darkMicroorganismsnowReport ARM ScienceCORPS a

  12. Public Power & Utility, Inc. (New Jersey) | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc Jump to:Newberg,Energy LLCALLETE Inc dEAPrysmian Jump to:OpenEIPublic Power

  13. Sandia National Laboratories: Z Pulsed Power Facility: Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust, High-ThroughputUpcoming Release of(LVOC) Working at the LVOC LVOC

  14. Valuing Public Preferences for Offshore Wind Power Andrew D. Krueger, University of Delaware, College of Marine and Earth Studies

    E-Print Network [OSTI]

    Firestone, Jeremy

    Valuing Public Preferences for Offshore Wind Power Andrew D. Krueger, University of Delaware in Massachusetts, New York, Delaware, and Texas. For Delaware, offshore wind power is currently the only cost public opposition, regulatory obstacles, and lack of incentives. Table 1: Delaware Offshore Wind Power

  15. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy Public UtilityAreaGCPCC's

  16. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy Public

  17. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook Chapters and Other

  18. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook Chapters and

  19. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook Chapters

  20. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook ChaptersLos Alamos

  1. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook ChaptersLos

  2. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook ChaptersLosSensors

  3. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook

  4. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook Directed

  5. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergy PublicBook DirectedFundamental

  6. 2A New Belt for the Van Allen Belts! Soon after launch, NASA's Van Allen

    E-Print Network [OSTI]

    2A New Belt for the Van Allen Belts! Soon after launch, NASA's Van Allen Probes detected a new Third Belt in the Van Allen Radiation Belts that encircle Earth. Located between the Inner and Outer Belts, which have been known to scientists for decades, the third belt is very temporary. It only

  7. Publications

    E-Print Network [OSTI]

    $author.value

    Rodrigo Bañuelos. MathScinet Publications and other (September 2013) · Link to Publications on MathScinet. RECENT PUBLICATIONS To Appear/In press:.

  8. Drive Alive: Teen Seat Belt Survey Program

    E-Print Network [OSTI]

    2010-01-01

    Traffic Safety Facts – Seat Belt Use in 2009 – OverallTraffic Safety Facts – Seat Belt Use in 2008 – DemographicClick-it-or-Ticket Safety Belt Initiative Telephone Survey.

  9. Impacts of Minnesota's Primary Seat Belt Law

    E-Print Network [OSTI]

    Minnesota, University of

    Impacts of Minnesota's Primary Seat Belt Law Frank Douma Center" Six Policies Strongly Supported By Research · Primary seat belt laws · SobrietyMcal Insights of Portland, Maine #12;Primary Seat Belt Laws "Allowing law

  10. Corn Belt Energy Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LISTStar EnergyLawler,CoalConcordiaConsumer ConnectionCoral Power LLC Place:PowerBelt

  11. IR Kuiper Belt Constraints

    E-Print Network [OSTI]

    Teplitz, V L; Anderson, J D; Rosenbaum, D C; Scalise, R J; Wentzler, P; Teplitz, Vigdor L.; Anderson, John D.; Rosenbaum, Doris; Scalise, Randall J.; Wentzler, Paul

    1999-01-01

    We compute the temperature and IR signal of particles of radius $a$ and albedo $\\alpha$ at heliocentric distance $R$, taking into account the emissivity effect, and give an interpolating formula for the result. We compare with analyses of COBE DIRBE data by others (including recent detection of the cosmic IR background) for various values of heliocentric distance, $R$, particle radius, $a$, and particle albedo, $\\alpha$. We then apply these results to a recently-developed picture of the Kuiper belt as a two-sector disk with a nearby, low-density sector (40belt IR spectra for various parameter v...

  12. Other Kuiper Belts

    E-Print Network [OSTI]

    M. Jura

    2003-11-28

    When a main sequence star evolves into a red giant and its Kuiper Belt Object's (KBO's) reach a temperature of about 170 K, the dust released during the rapid ice-sublimation of these cometary bodies may lead to a detectable infrared excess at 25 microns, depending upon the mass of the KBO's. Analysis of IRAS data for 66 first ascent red giants with 200 L(Sun) < L < 300 L(Sun) within 150 pc of the Sun provides an upper limit to the mass in KBO's at 45 AU orbital radius that is usually less than about 0.1 M(Earth). With improved infrared data, we may detect systems of KBO's around first ascent red giants that are analogs to our Solar System's KBO's.

  13. Publications

    E-Print Network [OSTI]

    $author.value

    Publications listed in Math Reviews as of September 17, 2013. See also "Other Publications" below. [1], Antonin Chambolle, Stacey E. Levine, and Bradley J.

  14. Publications

    E-Print Network [OSTI]

    $author.value

    Richard C Penney. Publications listed in MathSciNet .... Home · Assignments.txt · Publications. Department of Mathematics, Purdue University 150 N. University ...

  15. Silicon Valley Power and Oklahoma Municipal Power Authority Win 2014 Public

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LIST OF APPLICABLE DIRECTIVES Pursuant toPower Wind Awards | Department of Energy

  16. Public goods and private interests: Understanding non-residential demand for green power

    SciTech Connect (OSTI)

    Wiser, Ryan H.; Fowlie, Meredith; Holt, Edward A.

    2001-01-01

    This article presents the results of the first large-scale mail survey of non-residential green power customers in the United States. The survey explored the motivations, attitudes, and experiences of 464 business, non-profit, and public-sector customers that have voluntarily opted to purchase - and frequently pay a premium for - renewable electricity. Results of this study should be of value to marketers interested in targeting these customer segments, to policy makers interested in fostering and understanding non-residential demand for green power, and to academics pondering the motivations for firms to engage in such voluntary environmental initiatives.

  17. Re-Examining first principles of regulation: NRG power marketing, LLC v. Maine public utilities Commission

    SciTech Connect (OSTI)

    Haskell, Mark R.

    2010-03-15

    Maine PUC and Morgan Stanley have resolved some of the key issues facing the energy industry. The Supreme Court has plainly and directly in both cases reaffirmed the central role that private contracts play in the energy industry and set terms to balance the need to secure long-term investment with the public interest that lies at the heart of the Federal Power Act. (author)

  18. Impact of Public Policy and Societal Risk Perception on U.S. Civilian Nuclear Power Plant Construction

    E-Print Network [OSTI]

    Ford, David N.

    Impact of Public Policy and Societal Risk Perception on U.S. Civilian Nuclear Power Plant permit applications for 26 new nuclear power reactors. However, the previous generation of U.S. civilian of nuclear plants. Results point to the critical role societal perceptions of nuclear power risk play

  19. Chaos on the conveyor belt

    E-Print Network [OSTI]

    Bulcsú Sándor; Ferenc Járai-Szabó; Tamás Tél; Zoltán Néda

    2013-04-18

    The dynamics of a spring-block train placed on a moving conveyor belt is investigated both by simple experiments and computer simulations. The first block is connected by spring to an external static point, and due to the dragging effect of the belt the blocks undergo complex stick-slip dynamics. A qualitative agreement with the experimental results can only be achieved by taking into account the spatial inhomogeneity of the friction force on the belt's surface, modeled as noise. As a function of the velocity of the conveyor belt and the noise strength, the system exhibits complex, self-organized critical, sometimes chaotic dynamics and phase transition-like behavior. Noise induced chaos and intermittency is also observed. Simulations suggest that the maximum complexity of the dynamical states is achieved for a relatively small number of blocks, around five.

  20. D. Belt 4:30

    E-Print Network [OSTI]

    chenjk

    2007-08-16

    MA 152 – Online Homework iLrn/ThomsonNOW Course Key Code – for Registration & Getting Started. D. Belt 4:30. Note: This system used to be called iLrn, but ...

  1. The impact of main belt asteroids on infrared--submillimetre photometry and source counts

    E-Print Network [OSTI]

    Cs. Kiss; A. Pal; Th. G. Mueller; P. Abraham

    2007-11-28

    > Among the components of the infrared and submillimetre sky background, the closest layer is the thermal emission of dust particles and minor bodies in the Solar System. This contribution is especially important for current and future infrared and submillimetre space instruments --like those of Spitzer, Akari and Herschel -- and must be characterised by a reliable statistical model. > We describe the impact of the thermal emission of main belt asteroids on the 5...1000um photometry and source counts, for the current and future spaceborne and ground-based instruments, in general, as well as for specific dates and sky positions. > We used the statistical asteroid model (SAM) to calculate the positions of main belt asteroids down to a size of 1km, and calculated their infrared and submillimetre brightness using the standard thermal model. Fluctuation powers, confusion noise values and number counts were derived from the fluxes of individual asteroids. > We have constructed a large database of infrared and submillimetre fluxes for SAM asteroids with a temporal resolution of 5 days, covering the time span January 1, 2000 -- December 31, 2012. Asteroid fluctuation powers and number counts derived from this database can be obtained for a specific observation setup via our public web-interface. > Current space instruments working in the mid-infrared regime (Akari and Spitzer Space Telescopes) are affected by asteroid confusion noise in some specific areas of the sky, while the photometry of space infrared and submillimetre instruments in the near future (e.g. Herschel and Planck Space Observatories) will not be affected by asteroids. Faint main belt asteroids might also be responsible for most of the zodiacal emission fluctuations near the ecliptic.

  2. Publications

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

    Earthquake Engineering and Structural Dynamics Engineering Institute Publications-Earthquake Engineering and Structural Dynamics Contact Institute Director Charles Farrar (505)...

  3. Emergency Power Facility Assessment Tool (EPFAT) Following disasters that disrupt the commercial power service, generators are often required at critical public facilities,

    E-Print Network [OSTI]

    US Army Corps of Engineers

    plants, hospitals, wastewater treatment plants and shelters. The U.S. Army Corps of Engineers (USACE power service, generators are often required at critical public facilities, such as water treatment) 295-7745 (Primary) · Emergency Power SME (724) 459-4709 (Alternate) Key Web Links: · An EPFAT Tutorial

  4. Publications

    E-Print Network [OSTI]

    $author.value

    A new book published by World Scientific: Applications of Epidemiological Models to Public Health Policymaking--The role of heterogeneity in model predictions.

  5. Publications

    E-Print Network [OSTI]

    Please check my webpage: http://www.math.purdue.edu/~mdd/. Home · Publications. Department of Mathematics, Purdue University 150 N. University Street, ...

  6. Publications

    E-Print Network [OSTI]

    Publications. PHD Thesis (2012); Convergence of Space-Time Discrete Dynamics to Anisotropic Motion by Mean Curvature (with N.K. Yip) submitted, 2014.

  7. Publications

    E-Print Network [OSTI]

    Publications. 1. A compact embedding theorem for a class of degenerate Sobolev spaces. Rendiconti Sem. Mat. Univ. Polit. Torino, 49(3); 399-420, 1991. 2.

  8. THE COLLISIONAL DIVOT IN THE KUIPER BELT SIZE DISTRIBUTION

    SciTech Connect (OSTI)

    Fraser, Wesley C. [Division of Geological and Planetary Sciences, California Institute of Technology, MC 150-21, 1200 E. California Blvd. Pasadena, CA 91125 (United States)

    2009-11-20

    This paper presents the results of collisional evolution calculations for the Kuiper Belt starting from an initial size distribution similar to that produced by accretion simulations of that region-a steep power-law large object size distribution that breaks to a shallower slope at r approx 1-2 km, with collisional equilibrium achieved for objects r approx< 0.5 km. We find that the break from the steep large object power law causes a divot, or depletion of objects at r approx 10-20 km, which, in turn, greatly reduces the disruption rate of objects with r approx> 25-50 km, preserving the steep power-law behavior for objects at this size. Our calculations demonstrate that the roll-over observed in the Kuiper Belt size distribution is naturally explained as an edge of a divot in the size distribution; the radius at which the size distribution transitions away from the power law, and the shape of the divot from our simulations are consistent with the size of the observed roll-over, and size distribution for smaller bodies. Both the kink radius and the radius of the divot center depend on the strength scaling law in the gravity regime for Kuiper Belt objects. These simulations suggest that the sky density of r approx 1 km objects is approx10{sup 6}-10{sup 7} objects per square degree. A detection of the divot in the size distribution would provide a measure of the strength of large Kuiper Belt objects, and constrain the shape of the size distribution at the end of accretion in the Kuiper Belt.

  9. 1. THE RADIATION BELTS The outer zone radiation belts consist of energetic elec-

    E-Print Network [OSTI]

    Elkington, Scot R.

    1. THE RADIATION BELTS The outer zone radiation belts consist of energetic elec- trons trapped in the geomagnetic field. The dynamics of the belts are dictated by the global and local electric and mag- netic, A Review of ULF Interactions with Radiation Belt Electrons Scot R. Elkington Laboratory for Atmospheric

  10. 1 The Main Asteroid Belt Carolyn Crow: NASA's Dawn Mission The Main Asteroid Belt

    E-Print Network [OSTI]

    Waliser, Duane E.

    1 The Main Asteroid Belt Carolyn Crow: NASA's Dawn Mission The Main Asteroid Belt Written to the main asteroid belt to visit two of the largest protoplanets, Vesta and Ceres. Using sunlight, a mere accomplished by a spacecraft before. What compelled astronomers to send Dawn to the asteroid belt and what does

  11. Corn Belt Power Coop | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (Utility Company)| Open(Evans,Oregon:Volcano, Hawaii | OpenCorinna,CorixCorn

  12. THE KUIPER BELT AND THE PRIMORDIAL EVOLUTION

    E-Print Network [OSTI]

    Brown, Michael E.

    THE KUIPER BELT AND THE PRIMORDIAL EVOLUTION OF THE SOLAR SYSTEM A. MORBIDELLI Observatoire de la C. Morbidelli & Brown Abstract. We discuss the structure of the Kuiper belt as it can be inferred from the #12 inclinations and colors{ which clearly show that the belt has lost its pristine structure of a dynamically cold

  13. Conveyer-Belt Alphabet Erik D. Demaine

    E-Print Network [OSTI]

    Demaine, Erik

    Conveyer-Belt Alphabet Erik D. Demaine Martin L. Demaine Bel´en Palop Mathematics is often pursued, and the mathematics, font design, and puzzles that resulted. Conveyer-Belt Problem Suppose we are given several move), and the band as a conveyer belt or rubber band, modeled as a stretchable closed loop

  14. Conveyer Belt Puzzle Font Erik D. Demaine

    E-Print Network [OSTI]

    Demaine, Erik

    Conveyer Belt Puzzle Font Erik D. Demaine Martin L. Demaine Bel´en Palop (a) Input (b) Goal Figure 1: Conveyer belt open problem. Suppose you have a bunch of circular gears glued to a table (disks in the plane), as in Figure 1a. When can you wrap a conveyer belt (or elastic band) around them so

  15. THE KUIPER BELT: OVERVIEW David Jewitt

    E-Print Network [OSTI]

    Jewitt, David C.

    THE KUIPER BELT: OVERVIEW David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI in November 1998 #12;THE KUIPER BELT: OVERVIEW David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA The study of the Kuiper Belt has emerged as one of the leading subjects

  16. FROM KUIPER BELT OBJECT TO COMETARY NUCLEUS

    E-Print Network [OSTI]

    Jewitt, David C.

    FROM KUIPER BELT OBJECT TO COMETARY NUCLEUS David Jewitt Institute for Astronomy, 2680 Woodlawn body populations are related through a common origin in the Kuiper Belt, notably the Centaurs, the Jupiter Family Comets and certain dead-comets. But does primitive material from the Kuiper Belt survive

  17. The Kuiper Belt Harold F. Levison

    E-Print Network [OSTI]

    Levison, Harold F.

    The Kuiper Belt Harold F. Levison Department of Space Sciences Southwest Research Institute Perspective 2. Basic Orbital Dynamics 3. Observations of Kuiper Belt and Related Objects 4. Physical Observations of Trans-Neptunian Objects 5. The Long-Term Stability of Orbits in the Kuiper Belt 6. The Sizes

  18. A BOOSTER SEAT positions the seat belt

    E-Print Network [OSTI]

    A BOOSTER SEAT positions the seat belt so that it fits properly over the stronger parts of your movement during a crash. A SEAT BELT should lie across the upper thighs and be snug across the shoulder; read the vehicle owner's manual on how to install the car seat using the seat belt or LATCH system

  19. Creating Artificial Radiation Belts in the Lab

    E-Print Network [OSTI]

    Mauel, Michael E.

    Creating Artificial Radiation Belts in the Lab or "Some Observations of Hot Plasma Trapped Jeff #12;Outline · The Earth's radiation belts and ring current · Fast-electron interchange instability) fusion. #12;#12;"Artificial Radiation Belts" Van Allen kissing Explorer 4 "good bye" before it's launch

  20. Sun Belt Press Conference September 1, 2015

    E-Print Network [OSTI]

    Hutchens, John

    1 Sun Belt Press Conference September 1, 2015 Remarks by CCU President David A. DeCenzo Good the Sun Belt's invitation to become its 12th member beginning July 1, 2016. We are excited and honored Sun Belt staff as we embark upon this exciting journey. I also want to take this opportunity to thank

  1. THE KUIPER BELT: OVERVIEW David Jewitt

    E-Print Network [OSTI]

    Jewitt, David C.

    THE KUIPER BELT: OVERVIEW David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI in November 1998 #12; THE KUIPER BELT: OVERVIEW David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA The study of the Kuiper Belt has emerged as one of the leading subjects

  2. DYNAMICS OF THE KUIPER BELT RENU MALHOTRA

    E-Print Network [OSTI]

    Levison, Harold F.

    DYNAMICS OF THE KUIPER BELT RENU MALHOTRA Lunar and Planetary Institute MARTIN DUNCAN Queen of the Kuiper Belt is re­ viewed here. Numerical results on long term orbital evolution and dynamical mechanisms underlying the transport of objects out of the Kuiper Belt are discussed. Scenarios about the origin

  3. Simulation Worksheet: Kuiper Belt Interactions Instructor Guidelines

    E-Print Network [OSTI]

    Farritor, Shane

    Simulation Worksheet: Kuiper Belt Interactions Instructor Guidelines The goal of this activity is for students to understand that there are possible orbits in the outer solar system where Kuiper Belt Objects interaction with the asteroid belt and the Kirkwood Gaps. This worksheet makes use of simulations contained

  4. Certification Program SIX SIGMA GREEN BELT

    E-Print Network [OSTI]

    Bandyopadhyay, Antar

    Certification Program for SIX SIGMA GREEN BELT 20th to 24th January 2015 at Kolkata. Copies of certificates for proof of Domicile 5. A participant will be declared as certified Green Belt a Green Belt Certificate. 6. Any candidate failing to qualify the exam will be given another chance

  5. Impacts of Minnesota's Primary Seat Belt Law

    E-Print Network [OSTI]

    Levinson, David M.

    March 2012 Impacts of Minnesota's Primary Seat Belt Law Authors: Frank Douma Nebiyou Tilahun of Minnesota's Primary Seat Belt Law March 2012 6. 7. Author(s) 8. Performing Organization Report No. Frank. Abstract (Limit: 250 words) In the spring of 2009, the Minnesota Legislature changed the state's seat belt

  6. Tracking the Reliability of the U.S. Electric Power System: An Assessment of Publicly Available Information Reported to State Public Utility Commissions

    SciTech Connect (OSTI)

    LaCommare, Kristina H.; Eto, Joseph H.

    2008-10-10

    Large blackouts, such as the August 14-15, 2003 blackout in the northeasternUnited States and Canada, focus attention on the importance of reliable electric service. As public and private efforts are undertaken to improve reliability and prevent power interruptions, it is appropriate to assess their effectiveness. Measures of reliability, such as the frequency and duration of power interruptions, have been reported by electric utilities to state public utility commissions for many years. This study examines current state and utility practices for collecting and reporting electricity reliability information and discusses challenges that arise in assessing reliability because of differences among these practices. The study is based primarily on reliability information for 2006 reported by 123 utilities to 37 state public utility commissions.

  7. The role of public policy in emerging green power markets: an analysis of marketer preferences

    E-Print Network [OSTI]

    Wiser, Ryan

    1999-01-01

    13 Green Power Market Facilitation Efforts . . . . . . . .Development of Green Power Markets . . . . . . . . . . . . .to the Development of the Green Power Market: Survey

  8. MICROWAVE EMISSION FROM THE EDGEWORTH-KUIPER BELT AND THE ASTEROID BELT CONSTRAINED FROM THE WILKINSON MICROWAVE ANISOTROPY PROBE

    SciTech Connect (OSTI)

    Ichikawa, Kazuhide; Fukugita, Masataka [Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582 (Japan)

    2011-08-01

    Objects in the Edgeworth-Kuiper Belt and the main asteroid belt should emit microwaves that may give rise to extra anisotropy signals in the multipole of the cosmic microwave background (CMB) experiment. Constraints are derived from the absence of positive detection of such anisotropies for l {approx}< 50, meaning the total mass of Edgeworth-Kuiper Belt objects is smaller than 0.2 M{sub +}. This limit is consistent with the mass extrapolated from the observable population with the size of a {approx}> 15 km, assuming that the small-object population follows the power law in size dN/da {approx} a{sup -q} with the canonical index expected for collisional equilibrium, q {approx_equal} 3.5, with which 23% of the mass is ascribed to objects smaller than are observationally accessible down to grains. A similar argument applied to the main asteroid belt indicates that the grain population should not increase more quickly than q {approx_equal} 3.6 toward smaller radii, if the grain population follows the power law that continues to observed asteroids with larger radii. Both cases are at or only slightly above the limit that can be physically significant, implying the importance of further tightening the CMB anisotropy limit, which may be attained with observation at higher radio frequencies.

  9. Tampa Electric Company, Polk Power Station Unit No. 1, preliminary public design report

    SciTech Connect (OSTI)

    1994-06-01

    This preliminary Public Design Report (PDR) provides design information about Tampa Electric Company`s Polk Power Station Unit No. 1, which will demonstrate in a commercial 250 MW unit the benefits of the integration of oxygen-blown, entrained-flow coal gasification with advanced combined cycle technology. This project is partially funded by the US Department of Energy (DOE) under Round III of its Clean Coal Technology (CCT) Program under the provisions of Cooperative Agreement between DOE and Tampa Electric Company, novated on March 5,1992. The project is highlighted by the inclusion of a new hot gas cleanup system. DOE`s project management is based at its Morgantown Energy Technology Center (METC) in West Virginia. This report is preliminary, and the information contained herein is subject to revision. Definitive information will be available in the final PDR, which will be published at the completion of detailed engineering.

  10. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.Theory ofDid youOxygen Generation | CenterPressthisPublication Policy Publication

  11. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.Theory ofDid youOxygen Generation | CenterPressthisPublication Policy Publication

  12. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-RichProton Delivery and Removal in [Ni(P R 2PublicPublications

  13. Puget Sound Reinforcement Project : Planning for Peak Power Needs : Scoping Report, Part A, Summary of Public Comments.

    SciTech Connect (OSTI)

    United States. Bonneville Power Administration.

    1990-07-01

    This report summarizes public participation in the environmental scoping process for the Puget Sound Reinforcement Project, a Bonneville Power Administration (BPA) and Puget Sound area utilities study of voltage stability in northwestern Washington state. The environmental scoping phase of the Puget Sound project consisted of a series of public meetings and a public comment period. The content of these meetings is summarized in 2.0, Public Involvement. In 3.0, Comment Summary, the report summarizes comments received via meetings, mail and phone. The report ends with a description of the next steps in the project. Chapter 4.0, describes the decision process to be used by BPA and area utilities. Chapter 5.0 describes opportunities for public participation in decisions to be made about the future reliability of Puget Sound's electricity supply.

  14. Analysis of the rotational properties of Kuiper belt objects

    E-Print Network [OSTI]

    Pedro Lacerda; Jane Luu

    2006-01-12

    We use optical data on 10 Kuiper Belt objects (KBOs) to investigate their rotational properties. Of the 10, three (30%) exhibit light variations with amplitude delta_m >= 0.15 mag, and 1 out of 10 (10%) has delta_m >= 0.40 mag, which is in good agreement with previous surveys. These data, in combination with the existing database, are used to discuss the rotational periods, shapes, and densities of Kuiper Belt objects. We find that, in the sampled size range, Kuiper Belt objects have a higher fraction of low amplitude lightcurves and rotate slower than main belt asteroids. The data also show that the rotational properties and the shapes of KBOs depend on size. If we split the database of KBO rotational properties into two size ranges with diameter larger and smaller than 400 km, we find that: (1) the mean lightcurve amplitudes of the two groups are different with 98.5% confidence, (2) the corresponding power-law shape distributions seem to be different, although the existing data are too sparse to render this difference significant, and (3) the two groups occupy different regions on a spin period vs. lightcurve amplitude diagram. These differences are interpreted in the context of KBO collisional evolution.

  15. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    Renewable Energy Power Purchase Agreements. ” Journal ofit is the dynamic of power purchase agreement negotiationsbuy and sell sides of power purchase agreements (PPA), and

  16. Public goods and private interests: Understanding non-residential demand for green power

    E-Print Network [OSTI]

    Wiser, Ryan H.; Fowlie, Meredith; Holt, Edward A.

    2001-01-01

    Understanding Non-Residential Demand for Green PowerUnderstanding Non-Residential Demand for Green Power Vining,Understanding Non-Residential Demand for Green Power Kasius,

  17. Public goods and private interests: Understanding non-residential demand for green power

    E-Print Network [OSTI]

    Wiser, Ryan H.; Fowlie, Meredith; Holt, Edward A.

    2001-01-01

    Residential Demand for Green Power References Andreoni, J.Approach to Marketing Green Power. ” Research Report No. 8.Residential Demand for Green Power Vining, J. , Linn, N. ,

  18. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    Chen. (2007). “Should a coal-fired power plant be replacedof Regulatory Uncertainty for Coal-Fired Power Plants. ”in alternative coal-fired power plant technologies. ” Energy

  19. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    2007). “Should a coal-fired power plant be replaced orUncertainty for Coal-Fired Power Plants. ” Environmentalin alternative coal-fired power plant technologies. ” Energy

  20. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-RichProton Delivery and Removal in [Ni(P R 2Public

  1. Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-RichProton Delivery and Removal in [Ni(PLee » Publications

  2. Seat Belt Use Policy Outline the policy regarding use of seat belt in University of Michigan (U-M) vehicles.

    E-Print Network [OSTI]

    Kirschner, Denise

    Seat Belt Use Policy Objective Outline the policy regarding use of seat belt in University belt when operating a U-M vehicle. 2. Operators are also required to ensure that all occupants are adhering to the seat belt use laws when operating a U-M vehicle. 3. State of Michigan seat belt laws

  3. Summary of Information Presented at an NRC-Sponsored Low-Power Shutdown Public Workshop, April 27, 1999, Rockville, Maryland

    SciTech Connect (OSTI)

    Wheeler, Timothy A.; Whitehead, Donnie W.; Lois, Erasmia

    1999-07-01

    This report summarizes a public workshop that was held on April 27, 1999, in Rockville, Maryland. The workshop was conducted as part of the US Nuclear Regulatory Commission's (NRC) efforts to further develop its understanding of the risks associated with low power and shutdown operations at US nuclear power plants. A sufficient understanding of such risks is required to support decision-making for risk-informed regulation, in particular Regulatory Guide 1.174, and the development of a consensus standard. During the workshop the NRC staff discussed and requested feedback from the public (including representatives of the nuclear industry, state governments, consultants, private industry, and the media) on the risk associated with low-power and shutdown operations.

  4. Orbits, masses, and evolution of main belt triple (87) Sylvia

    E-Print Network [OSTI]

    Fang, J; Margot, JL; Margot, JL; Rojo, P

    2012-01-01

    D. 2008, Binaries in the Kuiper Belt, ed. Barucci, M. A. ,Brozovic et al. 2009), main belt triples Kleopatra (DescampsMASSES, AND EVOLUTION OF MAIN BELT TRIPLE (87) SYLVIA J ULIA

  5. Orbits, Masses, and Evolution of Main Belt Triple (87) Sylvia

    E-Print Network [OSTI]

    Fang, Julia; Margot, Jean-Luc; Rojo, Patricio

    2012-01-01

    D. 2008, Binaries in the Kuiper Belt, ed. Barucci, M. A. ,Brozovic et al. 2009), main belt triples Kleopatra (DescampsMASSES, AND EVOLUTION OF MAIN BELT TRIPLE (87) SYLVIA J ULIA

  6. Binary Objects in the Kuiper Belt and Outlying Centaurs: Simulations

    E-Print Network [OSTI]

    Binary Objects in the Kuiper Belt and Outlying Centaurs: Simulations Stephan Kolassa kolassa Abstract. Two exchange reaction scenarios to account for the characteristics of Kuiper belt binaries, Websites and Programs . . . . . . . . . . . . . . . . . . . . . . 10 2 Binary Objects in the Kuiper Belt 11

  7. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    on U.S. Wind Power Installation, Cost, and Performanceon U.S. Wind Power Installation, Cost, and Performancenot returned). Higher wind supply costs; Greater reliance on

  8. IEEE TRANSACTIONS ON WIRELESS COMMUNICATIONS, ACCEPTED FOR PUBLICATION 1 An Auction Approach to Distributed Power

    E-Print Network [OSTI]

    Tao, Meixia "Melissa"

    much power to reserve for its own transmission, how much power to purchase from other users, and how to Distributed Power Allocation for Multiuser Cooperative Networks Yuan Liu, Student Member, IEEE, Meixia Tao goal is to design an optimal distributed power allocation algorithm that enables user cooperation

  9. LIFAC demonstration at Richmond Power and Light Whitewater Valley Unit No. 2. Final report, Volume 1 - public design

    SciTech Connect (OSTI)

    NONE

    1998-02-01

    This report discusses the demonstration of LIFAC sorbent injection technology at Richmond Power and Light`s (RP&L) Whitewater Valley Unit No. 2 under the auspices of the U.S. Department of Energy`s (DOE) Clean Coal Technology Program. LIFAC is a sorbent injection technology capable of removing 75 to 85 percent of a power plant`s SO{sub 2} emissions using limestone at calcium to sulfur molar ratios of between 2 and 2.5. The site of the demonstration is a coal-fired electric utility power plant located in Richmond, Indiana. The project is being conducted by LIFAC North American (LIFAC NA), a joint venture partnership of Tampella Power Corporation and ICF Kaiser Engineers, in cooperation with DOE, RP&L, and several other organizations including the Electric Power Research Institute (EPRI), the State of Indiana, and Black Beauty Coal Company. The purpose of Final Report Volume 1: Public Design is to consolidate, for public use, all design and cost information regarding the LIFAC Desulfurization Facility at the completion of construction and startup.

  10. Empire of the Imagination: The Power of Public Fictions in Ovid's 'Reader Response' to Augustan Rome

    E-Print Network [OSTI]

    Pandey, Nandini B.

    2011-01-01

    gain in wealth and power upon annexing Egypt. 71 The poetsEgypt – Actium being quite an anticlimactic skirmish, except that it removed Augustus’ last true competitor for power.

  11. COLOR DEPENDENCE IN THE SIZE DISTRIBUTION OF MAIN BELT ASTEROIDS REVISITED

    SciTech Connect (OSTI)

    August, Tyler M.; Wiegert, Paul A.

    2013-06-15

    The size distribution of the asteroid belt is examined with 16956 main belt asteroids detected in data taken from the Canada-France-Hawaii Telescope Legacy Survey in two filters (g' and r'). The cumulative H (absolute magnitude) distribution is examined in both filters, and both match well to simple power laws down to H = 17, with slopes in rough agreement with those reported the literature. This implies that disruptive collisions between asteroids are gravitationally dominated down to at least this size, and probably sub-kilometer scales. The slopes of these distributions appear shallower in the outer belt than the inner belt, and the g' distributions appear slightly steeper than the r'. The slope shallowing in the outer belt may reflect a real compositional difference: the inner asteroid belt has been suggested to consist mostly of stony and/or metallic S-type asteroids, whereas carbonaceous C-types are thought to be more prevalent further from the Sun. No waves are seen in the size distribution above H = 15. Since waves are expected to be produced at the transition from gravitationally-dominated to internal strength-dominated collisions, their absence here may imply that the transition occurs at sub-kilometer scales, much smaller than the H = 17 (diameter {approx} 1.6 km) cutoff of this study.

  12. Green, Black, Lean Six Sigma and Master Black Belt Certifications

    E-Print Network [OSTI]

    Grissino-Mayer, Henri D.

    Green, Black, Lean Six Sigma and Master Black Belt Certifications Green BeLt CertifiCation Candidates may choose from three Green Belts offered: 1) Lean (one week of coursework) 2) Lean Six Sigma (two weeks of coursework) 3) Six Sigma (two weeks of coursework) Green Belt certification is a two

  13. BELT CHARGING SYSTEM M. LETOURNEL and J.-C. OBERLIN

    E-Print Network [OSTI]

    Boyer, Edmond

    1383 BELT CHARGING SYSTEM M. LETOURNEL and J.-C. OBERLIN Centre de Recherches Nucléaires courroie et de déterminer également les possibilités. Abstract. 2014 In M.P. accelerators belts have encountered some difficulties mainly about the belt life time. In the belt charging system, parameters

  14. Electric filter with movable belt electrode

    DOE Patents [OSTI]

    Bergman, W.

    1983-09-20

    A method and apparatus for removing airborne contaminants entrained in a gas or airstream includes an electric filter characterized by a movable endless belt electrode, a grounded electrode, and a filter medium sandwiched there between. Inclusion of the movable, endless belt electrode provides the driving force for advancing the filter medium through the filter, and reduces frictional drag on the filter medium, thereby permitting a wide choice of filter medium materials. Additionally, the belt electrode includes a plurality of pleats in order to provide maximum surface area on which to collect airborne contaminants. 4 figs.

  15. Electric filter with movable belt electrode

    DOE Patents [OSTI]

    Bergman, Werner (Pleasanton, CA)

    1983-01-01

    A method and apparatus for removing airborne contaminants entrained in a gas or airstream includes an electric filter characterized by a movable endless belt electrode, a grounded electrode, and a filter medium sandwiched therebetween. Inclusion of the movable, endless belt electrode provides the driving force for advancing the filter medium through the filter, and reduces frictional drag on the filter medium, thereby permitting a wide choice of filter medium materials. Additionally, the belt electrode includes a plurality of pleats in order to provide maximum surface area on which to collect airborne contaminants.

  16. A Public-Private-Academic Partnership to Advance Solar Power Forecasting

    Broader source: Energy.gov [DOE]

    The University Corporation for Atmospheric  Research (UCAR) will develop a solar power forecasting system that advances the state of the science through cutting-edge research.

  17. Statewide Estimate of 2012 Safety Belt Use in Texas

    E-Print Network [OSTI]

    Statewide Estimate of 2012 Safety Belt Use in Texas All Passenger Vehicles Passenger Cars Pickups Front Seat--Estimated Safety Belt Use 94.04 94.88 91.71 Driver--Estimated Safety Belt Use 94.66 95.56 92.10 Passenger--Estimated Safety Belt Use 91.05 91.74 82.11 #12;2012 Safety Belt Use in 18 Texas Cities #12

  18. The Compositional Structure of the Asteroid Belt

    E-Print Network [OSTI]

    DeMeo, Francesca E; Walsh, Kevin J; Chapman, Clark R; Binzel, Richard P

    2015-01-01

    The past decade has brought major improvements in large-scale asteroid discovery and characterization with over half a million known asteroids and over 100,000 with some measurement of physical characterization. This explosion of data has allowed us to create a new global picture of the Main Asteroid Belt. Put in context with meteorite measurements and dynamical models, a new and more complete picture of Solar System evolution has emerged. The question has changed from "What was the original compositional gradient of the Asteroid Belt?" to "What was the original compositional gradient of small bodies across the entire Solar System?" No longer is the leading theory that two belts of planetesimals are primordial, but instead those belts were formed and sculpted through evolutionary processes after Solar System formation. This article reviews the advancements on the fronts of asteroid compositional characterization, meteorite measurements, and dynamical theories in the context of the heliocentric distribution of...

  19. A study of binary Kuiper Belt objects

    E-Print Network [OSTI]

    Kern, Susan Diane

    2006-01-01

    About 105 bodies larger than 100km in diameter (Jewitt 1998) reside in the Kuiper Belt, beyond the orbit of Neptune. Since 1992 observational surveys have discovered over one thousand of these objects, believed to be fossil ...

  20. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    L.T. and P. Kraske (2003). “Renewable Energy Power PurchaseInvestments in Renewable Energy: The Role of Policy Design47. Wiser, R. (1997). “Renewable energy finance and project

  1. Practitioner Perspectives Matter: Public Policy and Private Investment in the U.S. Electric Power Sector

    E-Print Network [OSTI]

    Barradale, Merrill Jones

    2010-01-01

    R. (1997). “Renewable energy finance and project ownership:e.g. , “Finance and investment in wind energy in theEnergy Power Purchase Agreements. ” Journal of Structured and Project Finance

  2. Stroke Belt Initiative 1National Heart, Lung, and Blood Institute Stroke Belt Initiative

    E-Print Network [OSTI]

    Shen, Jun

    Stroke Belt Initiative 1National Heart, Lung, and Blood Institute Stroke Belt Initiative NATIONAL HEART, LUNG, AND BLOOD INSTITUTE Project Accomplishments and Lessons Learned Overview Cerebrovascular to those living in other regions of the country. The National Heart, Lung, and Blood Institute (NHLBI

  3. IDENTIFYING COLLISIONAL FAMILIES IN THE KUIPER BELT

    SciTech Connect (OSTI)

    Marcus, Robert A.; Ragozzine, Darin; Murray-Clay, Ruth A.; Holman, Matthew J., E-mail: rmarcus@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)

    2011-05-20

    The identification and characterization of numerous collisional families-clusters of bodies with a common collisional origin-in the asteroid belt has added greatly to the understanding of asteroid belt formation and evolution. More recent study has also led to an appreciation of physical processes that had previously been neglected (e.g., the Yarkovsky effect). Collisions have certainly played an important role in the evolution of the Kuiper Belt as well, though only one collisional family has been identified in that region to date, around the dwarf planet Haumea. In this paper, we combine insights into collisional families from numerical simulations with the current observational constraints on the dynamical structure of the Kuiper Belt to investigate the ideal sizes and locations for identifying collisional families. We find that larger progenitors (r {approx} 500 km) result in more easily identifiable families, given the difficulty in identifying fragments of smaller progenitors in magnitude-limited surveys, despite their larger spread and less frequent occurrence. However, even these families do not stand out well from the background. Identifying families as statistical overdensities is much easier than characterizing families by distinguishing individual members from interlopers. Such identification seems promising, provided the background population is well known. In either case, families will also be much easier to study where the background population is small, i.e., at high inclinations. Overall, our results indicate that entirely different techniques for identifying families will be needed for the Kuiper Belt, and we provide some suggestions.

  4. Satellites of the largest Kuiper belt objects

    E-Print Network [OSTI]

    M. E. Brown; M. A. van Dam; A. H. Bouchez; D. Le Mignant; R. D. Campbell; J. C. Y. Chin; A. Conrad; S. K. Hartman; E. M. Johansson; R. E. Lafon; D. L. Rabinowitz; P. J. Stomski, Jr.; D. M. Summers; C. A. Trujillo; P. L. Wizinowich

    2005-10-03

    We have searched the four brightest objects in the Kuiper belt for the presence of satellites using the newly commissioned Keck Observatory Laser Guide Star Adaptive Optics system. Satellites are seen around three of the four objects: Pluto (whose satellite Charon is well-known), 2003 EL61, and 2003 UB313. The object 2005 FY9, the brightest Kuiper belt object after Pluto, does not have a satellite detectable within 0.4 arcseconds with a brightness of more than 0.5% of the primary. The presence of satellites to 3 of the 4 brightest Kuiper belt objects is inconsistent with the fraction of satellites in the Kuiper belt at large at the 99.1% confidence level, suggesting a different formation mechanism for these largest KBO satellites. The satellites of 2003 EL61 and 2003 UB313, with fractional brightnesses of 5% and 2% of their primaries, respectively, are significantly fainter relative to their primaries than other known Kuiper belt object satellites, again pointing to possible differences in their origin.

  5. Title 30 Chapter 5 Powers and Duties of Department of Public Service and

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page| Open Energy Information Serbia-EnhancingEt Al., 2013)Open EnergyTinox Jump to:,11 Protection of2CFRenergyTitlePublic

  6. Microsoft PowerPoint - xxDraft SEIS PUBLIC MEETING PRESENTATION 9 sep 2014 [Compatibility Mode]

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal GasAdministration Medal01 Sandia NationalSecurityNuclearH-canyon |I6 Page 2Public

  7. Kinematic Peculiarities of Gould Belt Stars

    E-Print Network [OSTI]

    Vadim V. Bobylev

    2005-12-22

    We analyzed the space velocities of Gould Belt stars younger than 125 Myr located at heliocentric distances Belt by assuming the existence of a single kinematic center whose direction was found to be the following: $l_\\circ=128^\\circ$ and $R_\\circ=150$ pc. The linear velocities reach their maximum at a distance of $\\approx300$ pc from the center and are -6 km s$^{-1}$ for the rotation (whose direction coincides with the Galactic rotation) and +4 km s$^{-1}$ for the expansion. The stellar rotation model used here is shown to give a more faithful description of the observed velocity field than the linear model based on the Oort constants $A_G$ and $B_G$. We present evidence that the young clusters $\\beta$ Pic, Tuc/HorA, and TWA belong to the Gould Belt structure.

  8. Pulsar radiation belts and transient radio emission

    E-Print Network [OSTI]

    Q. Luo; D. B. Melrose

    2007-04-22

    It is proposed that radiation belts similar to the ones in the planetary magnetosphere can exist for a pulsar with a relatively long period and a strong magnetic field. In the belts located in the closed field line region near the light cylinder relativistic pairs are trapped and maintained at a density substantially higher than the local Goldreich-Julian corotation density. The trapped plasma can be supplied and replenished by either direct injection of relativistic pairs from acceleration of externally-supplied particles in a dormant outer gap or in situ ionization of the accreted neutral material in the trapping region. The radiation belts can be disrupted by waves that are excited in the region as the result of plasma instabilities or emitted from the surface due to starquakes or stellar oscillations. The disruption can cause an intermittent particle precipitation toward the star producing radio bursts. It is suggested that such bursts may be seen as rotating radio transients (RRATs).

  9. International Space Environment Conference 2001 Radiation Belt Science and Technology

    E-Print Network [OSTI]

    Chan, Anthony Arthur

    International Space Environment Conference 2001 Radiation Belt Science and Technology July 23 devoted to advancing our understanding of Earth's space environment and its effects on technology-27, 2001, Queenstown, New Zealand The International Space Environment Conference 2001: Radiation Belt

  10. Stored energy in conveyor belts - managing the risks

    SciTech Connect (OSTI)

    Goldbeck, L.J.

    2006-11-15

    Employees need to know the dangers of working around conveyors. Safety training on belt tension is discussed. 3 figs.

  11. Microsoft PowerPoint - NA-RP_Public_Workshop_April-2013.ppt

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on darkMicroorganismsnow widelySmall Ice CrystalsHighMorgantown

  12. Microsoft PowerPoint - Revised Public Information Opportunities 5-10-07.ppt

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on darkMicroorganismsnow widelySmallBPARegulating Energy

  13. Poludnista Dorsa, Venus: History and context of a deformation belt

    E-Print Network [OSTI]

    Hansen, Vicki

    Poludnista Dorsa, Venus: History and context of a deformation belt D. A. Young and V. L. Hansen is combined with altimetry data test models of deformation belt evolution in Venus's lowlands. Poludnista Dorsa, a complex 2000-km-long deformation belt, is highly segmented and broadly time transgressive. Long

  14. Visible and Infrared Photometry of Fourteen Kuiper Belt Objects

    E-Print Network [OSTI]

    Davies, John Keith

    Visible and Infrared Photometry of Fourteen Kuiper Belt Objects John K. Davies Joint Astronomy\\GammaJ colors of 14 Kuiper Belt objects using new infrared (J) data combined, in most cases, with simultaneous. Kuiper Belt objects exhibit a wide range of V\\GammaJ colors but there is no correlation with heliocentric

  15. Gears and Belt Drives for Non-Uniform Transmission

    E-Print Network [OSTI]

    Nawratil, Georg

    Gears and Belt Drives for Non-Uniform Transmission Hellmuth Stachel Abstract Ordinarily, gears and belt drives are used for uniform transmission of rotations between parallel axes. Here we focus. Concerning belt drives, we study their relation to tooth profiles and focus on `strict' cases which work

  16. Forming the Kuiper Belt by the Outward Transport of Objects

    E-Print Network [OSTI]

    Levison, Harold F.

    Forming the Kuiper Belt by the Outward Transport of Objects During Neptune's Migration Harold F la C^ote d'Azur, Nice, France To appear in Nature #12;Page 2 The `dynamically cold Kuiper belt unless the cold Kuiper belt originally contained tens of Earth-masses of solids. While several mechanisms

  17. Thesis Proposal Electromagnetic Ion Cyclotron (EMIC) Waves for Radiation Belt

    E-Print Network [OSTI]

    de Weck, Olivier L.

    Thesis Proposal Electromagnetic Ion Cyclotron (EMIC) Waves for Radiation Belt Remediation particles of the Van Allen belts coming from cosmic rays, solar storms, high altitude nuclear explosions regions, as well as an obstacle to exploration and development of space technologies. The "Radiation Belt

  18. Setting confidence belts Byron P. Roe and Michael B. Woodroofe

    E-Print Network [OSTI]

    Woodroofe, Michael B.

    Setting confidence belts Byron P. Roe and Michael B. Woodroofe Department of Physics (B credible belts for the mean of a Poisson distribution in the presence of a background the Bayesian framework, these belts are optimal. The credible limits are then examined from a frequentist point

  19. THE KUIPER BELT AND ITS PRIMORDIAL SCULPTING A. MORBIDELLI

    E-Print Network [OSTI]

    Brown, Michael E.

    THE KUIPER BELT AND ITS PRIMORDIAL SCULPTING A. MORBIDELLI Observatoire de la Côte d'Azur, Nice the structure of the Kuiper belt as it can be inferred from the first decade of observations. In particular, we that the belt has lost its pristine structure of a dynamically cold proto- planetary disk. Understanding how

  20. Bulk Acoustic Resonator Based on Piezoelectric ZnO Belts

    E-Print Network [OSTI]

    Wang, Zhong L.

    Bulk Acoustic Resonator Based on Piezoelectric ZnO Belts Brent A. Buchine, William L. Hughes, F, a bulk acoustic resonator based on ZnO belts is demonstrated. This device shows a great deal of promise-like geometry, making them ideal candidates as SMR, FBAR, and beam resonators.13 However, handling belts can

  1. Forming the Kuiper Belt by the Outward Transport of Objects

    E-Print Network [OSTI]

    Levison, Harold F.

    Forming the Kuiper Belt by the Outward Transport of Objects During Neptune's Migration Harold F + Observatoire de la Câ??ote d'Azur, Nice, France To appear in Nature #12; Page 2 The `dynamically cold Kuiper belt unless the cold Kuiper belt originally contained tens of Earth­masses of solids. While several mechanisms

  2. Gears and belt drives for non-uniform transmission

    E-Print Network [OSTI]

    Nawratil, Georg

    Gears and belt drives for non-uniform transmission Hellmuth Stachel stachel of gearing 2. Non-uniform belt drives 3. On the existence of strict non-uniform belt drives EUCOMES08. Finsterwalder's principle of gearing The driving wheel 1 rotates about O1 through 1, the out-put wheel 2 rotates

  3. THE PLANE OF THE KUIPER BELT Michael E. Brown

    E-Print Network [OSTI]

    Brown, Michael E.

    THE PLANE OF THE KUIPER BELT Michael E. Brown Division of Geological and Planetary Sciences of the Kuiper belt. The derived plane has an inclination with respect to the ecliptic of 1 .86 and an ascending node of 81 .6, with a 1 error in pole position of the plane of 0 .37. The plane of the Kuiper belt

  4. The largest Kuiper belt objects Michael E. Brown

    E-Print Network [OSTI]

    Brown, Michael E.

    The largest Kuiper belt objects Michael E. Brown California Institute of Technology ABSTRACT While for the first decade of the study of the Kuiper belt, a gap existed between the sizes of the relatively small and faint Kuiper belt objects (KBOs) that were being studied and the largest known KBO, Pluto, recent years

  5. Statistical Methods for Detecting Stellar Occultations by Kuiper Belt Objects

    E-Print Network [OSTI]

    Rice, John

    Statistical Methods for Detecting Stellar Occultations by Kuiper Belt Objects: the Taiwanese in the Kuiper Belt, by measuring the rate of occultations of stars by these objects, using an array of three of the solar system. This belt is the source of most short­period comets, those with periods of 200 years

  6. Certification Program SIX SIGMA GREEN BELT at Kolkata

    E-Print Network [OSTI]

    Bandyopadhyay, Antar

    Certification Program for SIX SIGMA GREEN BELT at Kolkata 20th to 24th January 2015. A participant will be declared as certified Green Belt only after passing the GB certification test with minimum 70% marks, and a candidate will be issued a Green Belt Certificate. 11. Any candidate failing

  7. Colors of Kuiper Belt objects : the relationship between KBO colors and Kuiper Belt plane inclination

    E-Print Network [OSTI]

    Kane, Julia Frances

    2006-01-01

    A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt. These objects, thought to be the progenitors of short period comets, could provide a sample of primordial material in ...

  8. Six Sigma Black Belts Fight For Quality

    E-Print Network [OSTI]

    Vardeman, Stephen B.

    Six Sigma Black Belts Fight For Quality Ron Scott Ross Finnestad Rodney Kalsow IE 361 mini-paper 9/22/00 #12;Six Sigma is a breakthrough management strategy that is revolutionizing the world's top corporations. So what is Six Sigma? "It is a business process that allows companies to drastically improve

  9. Leinhardt et al.: Collisions in the Kuiper Belt 195 Physical Effects of Collisions in the Kuiper Belt

    E-Print Network [OSTI]

    Stewart, Sarah T.

    Leinhardt et al.: Collisions in the Kuiper Belt 195 195 Physical Effects of Collisions in the Kuiper Belt Zoë M. Leinhardt and Sarah T. Stewart Harvard University Peter H. Schultz Brown University Collisions are a major modification process over the history of the Kuiper belt. Recent work illuminates

  10. Cogeneration and Small Power Production Quarterly Report to the California Public Utilities Commission First Quarter 1984

    SciTech Connect (OSTI)

    1984-01-01

    At the end of the First Quarter of 1984, the number of signed contracts and letter agreements for cogeneration and small power production projects was 322, with a total estimated nominal capacity of 2,643 MW. Of these totals, 215 projects, capable of producing 640 MW, are operational. A map indicating the location of operational facilities under contract with PG and E is provided. Developers of cogeneration, solid waste, or biomass projects had signed 110 contracts with a potential of 1,467 MW. In total, 114 contracts and letter agreements had been signed with projects capable of producing 1,508 MW. PG and E also had under active discussion 35 cogeneration projects that could generate a total of 425 MW to 467 MW, and 11 solid waste or biomass projects with a potential of 94 MW to 114 MW. One contract had been signed for a geothermal project, capable of producing 80 MW. There were 7 solar projects with signed contracts and a potential of 37 MW, as well as 5 solar projects under active discussion for 31 MW. Wind farm projects under contract numbered 32, with a generating capability of 848 MW. Also, discussions were being conducted with 18 wind farm projects, totaling 490 MW. There were 101 wind projects of 100 kW or less with signed contracts and a potential of 1 MW, as well as 6 other small wind projects under active discussion. There were 64 hydroelectric projects with signed contracts and a potential of 148 MW, as well as 75 projects under active discussion for 316 MW. In addition, there were 31 hydroelectric projects, with a nominal capacity of 187 MW, that Pg and E was planning to construct.

  11. Cogeneration and Small Power Production Quarterly Report to the California Public Utilities Commission Fourth Quarter 1983

    SciTech Connect (OSTI)

    1983-01-01

    At the end of 1983, the number of signed contracts and letter agreements for cogeneration and small power production projects was 305, with a total estimated nominal capacity of 2,389 MW. Of these totals, 202 projects, capable of producing 566 MW, are operational (Table A). A map indicating the location of operational facilities under contract with PG and E is provided as Figure A. Developers of cogeneration, solid waste, or biomass projects had signed 101 contracts with a potential of 1,408 MW. In total, 106 contracts and letter agreements had been signed with projects capable of producing 1,479 MW. PG and E also had under active discussion 29 cogeneration projects that could generate a total of 402 MW to 444 MW, and 13 solid waste or biomass projects with a potential of 84 MW to 89 MW. One contract had been signed for a geothermal project, capable of producing 80 MW. There were 7 solar projects with signed contracts and a potential of 37 MW, as well as 3 solar projects under active discussion for 31 MW. Wind farm projects under contract numbered 28, with a generating capability of 618 MW. Also, discussions were being conducted with 14 wind farm projects, totaling 365 MW. There were 100 wind projects of 100 kW or less with signed contracts and a potential of 1 MW, as well as 8 other small wind projects under active discussion. There were 59 hydroelectric projects with signed contracts and a potential of 146 MW, as well as 72 projects under active discussion for 169 MW. In addition, there were 31 hydroelectric projects, with a nominal capacity of 185 MW, that PG and E was planning to construct. Table B displays the above information. In tabular form, in Appendix A, are status reports of the projects as of December 31, 1983.

  12. Cogeneration and Small Power Production Quarterly Report to the California Public Utilities Commission. Second Quarter 1984

    SciTech Connect (OSTI)

    1984-01-01

    At the end of the Second Quarter of 1984, the number of signed contracts and letter agreements for cogeneration and small power production projects was 334, with total estimated nominal capacity of 2,876 MW. Of these totals, 232 projects, capable of producing 678 MW, are operational (Table A). A map indicating the location of operational facilities under contract with PG and E is provided as Figure A. Developers of cogeneration projects had signed 80 contracts with a potential of 1,161 MW. Thirty-three contracts had been signed for solid waste/biomass projects for a total of 298 MW. In total, 118 contracts and letter agreements had been signed with cogeneration, solid waste, and biomass projects capable of producing 1,545 MW. PG and E also had under active discussion 46 cogeneration projects that could generate a total of 688 MW to 770 MW, and 13 solid waste or biomass projects with a potential of 119 MW to 139 MW. One contract had been signed for a geothermal project, capable of producing 80 MW. Two geothermal projects were under active discussion for a total of 2 MW. There were 8 solar projects with signed contracts and a potential of 37 MW, as well as 4 solar projects under active discussion for 31 MW. Wind farm projects under contract numbered 34, with a generating capability of 1,042 MW, Also, discussions were being conducted with 23 wind farm projects, totaling 597 MW. There were 100 wind projects of 100 kW or less with signed contracts and a potential of 1 MW, as well as 7 other small wind projects under active discussion. There were 71 hydroelectric projects with signed contracts and a potential of 151 MW, as well as 76 projects under active discussion for 505 MW. In addition, there were 18 hydroelectric projects, with a nominal capacity of 193 MW, that PG and E was planning to construct. Table B displays the above information. Appendix A displays in tabular form the status reports of the projects as of June 30, 1984.

  13. HIGH ECLIPTIC LATITUDE SURVEY FOR SMALL MAIN-BELT ASTEROIDS

    SciTech Connect (OSTI)

    Terai, Tsuyoshi [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Takahashi, Jun; Itoh, Yoichi, E-mail: tsuyoshi.terai@nao.ac.jp [Center for Astronomy, University of Hyogo, 407-2 Nishigaichi, Sayo-cho, Sayo-gun, Hyogo 679-5313 (Japan)

    2013-11-01

    Main-belt asteroids have been continuously colliding with one another since they were formed. Their size distribution is primarily determined by the size dependence of asteroid strength against catastrophic impacts. The strength scaling law as a function of body size could depend on collision velocity, but the relationship remains unknown, especially under hypervelocity collisions comparable to 10 km s{sup –1}. We present a wide-field imaging survey at an ecliptic latitude of about 25° for investigating the size distribution of small main-belt asteroids that have highly inclined orbits. The analysis technique allowing for efficient asteroid detections and high-accuracy photometric measurements provides sufficient sample data to estimate the size distribution of sub-kilometer asteroids with inclinations larger than 14°. The best-fit power-law slopes of the cumulative size distribution are 1.25 ± 0.03 in the diameter range of 0.6-1.0 km and 1.84 ± 0.27 in 1.0-3.0 km. We provide a simple size distribution model that takes into consideration the oscillations of the power-law slope due to the transition from the gravity-scaled regime to the strength-scaled regime. We find that the high-inclination population has a shallow slope of the primary components of the size distribution compared to the low-inclination populations. The asteroid population exposed to hypervelocity impacts undergoes collisional processes where large bodies have a higher disruptive strength and longer lifespan relative to tiny bodies than the ecliptic asteroids.

  14. THE CANADA-FRANCE ECLIPTIC PLANE SURVEY-L3 DATA RELEASE: THE ORBITAL STRUCTURE OF THE KUIPER BELT

    SciTech Connect (OSTI)

    Kavelaars, J. J.; Jones, R. L.; Murray, I. [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC V9E 2E7 (Canada); Gladman, B. J.; Petit, J.-M.; Van Laerhoven, C. [Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia, Vancouver, BC (Canada); Parker, Joel Wm.; Bieryla, A. [Space Science and Engineering Division, Southwest Research Institute, 1050 Walnut Street, Suite 400, Boulder, CO 80302 (United States); Nicholson, P.; Margot, J. L. [Cornell University, Space Sciences Building, Ithaca, NY 14853 (United States); Rousselot, P.; Mousis, O. [Institut UTINAM, CNRS-UMR 6213, Observatoire de Besancon, BP 1615, 25010 Besancon Cedex (France); Scholl, H. [Observatoire de la Cote d'Azur, BP 4229, Boulevard de l'Observatoire, F-06304 Nice Cedex 4 (France); Marsden, B. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Benavidez, P.; Campo Bagatin, A. [Departamento de Fisica, Ingenieria de Sistemas y Teoria de la Senal, E.P.S.A., Universidad de Alicante, Apartado de Correos 99, Alicante 03080 (Spain); Doressoundiram, A. [LESIA, Observatoire de Paris, 92195 Meudon Principal Cedex (France); Veillet, C. [Canada-France-Hawaii Telescope Corporation, P.O. Box 1597, Kamuela, HI 96743 (United States)

    2009-06-15

    We report the orbital distribution of the trans-Neptunian comets discovered during the first discovery year of the Canada-France Ecliptic Plane Survey (CFEPS). CFEPS is a Kuiper Belt object survey based on observations acquired by the Very Wide component of the Canada-France-Hawaii Telescope Legacy Survey (LS-VW). The first year's detections consist of 73 Kuiper Belt objects, 55 of which have now been tracked for three years or more, providing precise orbits. Although this sample size is small compared to the world-wide inventory, because we have an absolutely calibrated and extremely well-characterized survey (with known pointing history) we are able to de-bias our observed population and make unbiased statements about the intrinsic orbital distribution of the Kuiper Belt. By applying the (publically available) CFEPS Survey Simulator to models of the true orbital distribution and comparing the resulting simulated detections to the actual detections made by the survey, we are able to rule out several hypothesized Kuiper Belt object orbit distributions. We find that the main classical belt's so-called 'cold' component is confined in semimajor axis (a) and eccentricity (e) compared to the more extended 'hot' component; the cold component is confined to lower e and does not stretch all the way out to the 2:1 resonance but rather depletes quickly beyond a = 45 AU. For the cold main classical belt population we find a robust population estimate of N(H{sub g} < 10) = 50 {+-} 5 x 10{sup 3} and find that the hot component of the main classical belt represents {approx}60% of the total population. The inner classical belt (sunward of the 3:2 mean-motion resonance) has a population of roughly 2000 trans-Neptunian objects with absolute magnitudes H{sub g} < 10, and may not share the inclination distribution of the main classical belt. We also find that the plutino population lacks a cold low-inclination component, and so, the population is somewhat larger than recent estimates; our analysis shows a plutino population of N(H{sub g} < 10){approx} 25{sup +25} {sub -12} x 10{sup 3}compared to our estimate of the size of main classical Kuiper Belt population of N(H{sub g} < 10) {approx} (126{sup +50} {sub -46}) x 10{sup 3}.

  15. Accepted for publication in Energy Policy Greenhouse-gas Emissions from Solar Electric-and Nuclear Power: A Life-cycle

    E-Print Network [OSTI]

    Accepted for publication in Energy Policy Greenhouse-gas Emissions from Solar Electric- and Nuclear., 2002). However, all anthropogenic means of energy production, including solar and nuclear, generate Power: A Life-cycle Study Vasilis M. Fthenakis1,2, * and Hyung Chul Kim1 1 Energy Sciences

  16. The Kuiper Belt Luminosity Function from m(R)=21 to 26

    E-Print Network [OSTI]

    W. C. Fraser; JJ Kavelaars; M. J. Holman; C. J. Pritchet; B. J Gladman; T. Grav; R. L. Jones; J. MacWilliams; J. -M. Petit

    2008-02-17

    We have performed an ecliptic imaging survey of the Kuiper belt with our deepest and widest field achieving a limiting flux of m(g') = 26.4, with a sky coverage of 3.0 square-degrees. This is the largest coverage of any other Kuiper belt survey to this depth. We detect 72 objects, two of which have been previously observed. We have improved the Bayesian maximum likelihood fitting technique presented in Gladman et al. (1998) to account for calibration and sky density variations and have used this to determine the luminosity function of the Kuiper belt. Combining our detections with previous surveys, we find the luminosity function is well represented by a single power-law with slope alpha = 0.65 +/- 0.05 and an on ecliptic sky density of 1 object per square-degree brighter than m(R)=23.42 +/- 0.13. Assuming constant albedos, this slope suggests a differential size-distribution slope of 4.25 +/- 0.25, which is steeper than the Dohnanyi slope of 3.5 expected if the belt is in a state of collisional equilibrium. We find no evidence for a roll-over or knee in the luminosity function and reject such models brightward of m(R) ~ 24.6.

  17. The Kuiper Belt and Other Debris Disks

    E-Print Network [OSTI]

    David Jewitt; Amaya Moro-Martín; Pedro Lacerda

    2008-08-24

    We discuss the current knowledge of the Solar system, focusing on bodies in the outer regions, on the information they provide concerning Solar system formation, and on the possible relationships that may exist between our system and the debris disks of other stars. Beyond the domains of the Terrestrial and giant planets, the comets in the Kuiper belt and the Oort cloud preserve some of our most pristine materials. The Kuiper belt, in particular, is a collisional dust source and a scientific bridge to the dusty "debris disks" observed around many nearby main-sequence stars. Study of the Solar system provides a level of detail that we cannot discern in the distant disks while observations of the disks may help to set the Solar system in proper context.

  18. Kuiper Belt evolution due to dynamical friction

    E-Print Network [OSTI]

    A. Del Popolo; E. Spedicato; M. Gambera

    1999-05-04

    In this paper we study the role of dynamical friction on the evolution of a population of large objects ($m>10^{22}$ g) at heliocentric distances $>70$ AU in the Kuiper Belt. We show that the already flat distribution of these objects must flatten further due to non-spherically symmetric distribution of matter in the Kuiper Belt. Moreover the dynamical drag, produced by dynamical friction, causes objects of masses $\\geq 10^{24} g$ to lose angular momentum and to fall through more central regions in a timescale $\\approx 10^9 yr$. This mechanism is able to transport inwards objects of the size of Pluto, supposing it was created beyond 50 AU, according to a Stern & Colwell's (1997b) suggestion.

  19. QUAOAR: A ROCK IN THE KUIPER BELT

    SciTech Connect (OSTI)

    Fraser, Wesley C.; Brown, Michael E. [Division of Geological and Planetary Sciences, California Institute of Technology, MC 150-21. 1200 E. California Blvd. Pasadena, CA 91125 (United States)

    2010-05-10

    Here we report Wide-Field Planetary Camera 2 observations of the Quaoar-Weywot Kuiper Belt binary. From these observations, we find that Weywot is on an elliptical orbit with an eccentricity of 0.14 {+-} 0.04, a period of 12.438 {+-} 0.005 days, and a semimajor axis of 1.45 {+-} 0.08 x 10{sup 4} km. The orbit reveals a surprisingly high-Quaoar-Weywot system mass of (1.6 {+-} 0.3) x 10{sup 21} kg. Using the surface properties of the Uranian and Neptunian satellites as a proxy for Quaoar's surface, we reanalyze the size estimate from Brown and Trujillo. We find, from a mean of available published size estimates, a diameter for Quaoar of 890 {+-} 70 km. We find Quaoar's density to be {rho} = 4.2 {+-} 1.3gcm{sup -3}, possibly the highest density in the Kuiper Belt.

  20. Chaotic Diffusion of Resonant Kuiper Belt Objects

    E-Print Network [OSTI]

    Matthew S. Tiscareno; Renu Malhotra

    2009-07-06

    We carried out extensive numerical orbit integrations to probe the long-term chaotic dynamics of the two strongest mean motion resonances of Neptune in the Kuiper belt, the 3:2 (Plutinos) and 2:1 (Twotinos). Our primary results include a computation of the relative volumes of phase space characterized by large- and small-resonance libration amplitudes, and maps of resonance stability measured by mean chaotic diffusion rate. We find that Neptune's 2:1 resonance has weaker overall long-term stability than the 3:2 -- only ~15% of Twotinos are projected to survive for 4 Gyr, compared to ~27% of Plutinos, based on an extrapolation from our 1-Gyr integrations. We find that Pluto has only a modest effect, causing a ~4% decrease in the Plutino population that survives to 4 Gyr. Given current observational estimates, and assuming an initial distribution of particles proportional to the local phase space volume in the resonance, we conclude that the primordial populations of Plutinos and Twotinos formerly made up more than half the population of the classical and resonant Kuiper Belt. We also conclude that Twotinos were originally nearly as numerous as Plutinos; this is consistent with predictions from early models of smooth giant planet migration and resonance sweeping of the Kuiper Belt, and provides a useful constraint for more detailed models.

  1. STUDY CITIES IN THE TEXAS SAFETY BELT OBSERVATIONAL SURVEY CONDUCTED BY TEXAS TRANSPORTATION INSTITUTE

    E-Print Network [OSTI]

    STUDY CITIES IN THE TEXAS SAFETY BELT OBSERVATIONAL SURVEY CONDUCTED BY TEXAS TRANSPORTATION INSTITUTE #12;2010 SAFETY BELT USE BY CITY #12;2010 Safety Belt Use In the 18 Texas Cities City Total N Observed % Restrained Total Driver N % Belt Use Total Passenger N % Belt Use Abilene Amarillo Austin

  2. Water Power Program: Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on DeliciousMathematics And Statistics » USAJobs SearchAMERICA'S FUTURE.Projects at ArmyusingPeer Reviews WaterAbout

  3. Statewide Estimate of 2011 Safety Belt Use in Texas

    E-Print Network [OSTI]

    Statewide Estimate of 2011 Safety Belt Use in Texas All Passenger Vehicles Passenger Cars Pickups Front Seat--Estimated Safety Belt Use Standard Error Lower 95% confidence limit Upper 95% confidence limit 93.68 2.31 89.15 98.21 94.67 2.28 90.20 99.14 90.81 2.33 86.24 95.38 Driver--Estimated Safety Belt

  4. New compounds will help coal operators comply with BELT standards

    SciTech Connect (OSTI)

    NONE

    2009-04-15

    US coal producers will soon have a new set of conveyor belting standards, which are currently proposed as a rulemaking by the Mine Safety and Health Administration (MSHA), to bring higher levels of resistance to propagation of fire by a secondary source. The new test being put into effect is known as a Belt Evaluation Laboratory Test (BELT). The article, submitted by Fenner Dunlop, discusses the company's testing procedures and the development of conveyors to comply with regulations. 2 photos.

  5. Geologic Setting of the Central Alaskan Hot Springs Belt: Implications...

    Open Energy Info (EERE)

    the Central Alaskan Hot Springs Belt: Implications for Geothermal Resource Capacity and Sustainable Energy Production Jump to: navigation, search OpenEI Reference LibraryAdd to...

  6. Magnetic refrigeration apparatus with belt of ferro or paramagnetic material

    DOE Patents [OSTI]

    Barclay, J.A.; Stewart, W.F.; Henke, M.D.; Kalash, K.E.

    1986-04-03

    A magnetic refrigerator operating in the 12 to 77 K range utilizes a belt which carries ferromagnetic or paramagnetic material and which is disposed in a loop which passes through the center of a solenoidal magnet to achieve cooling. The magnetic material carried by the belt, which can be blocks in frames of a linked belt, can be a mixture of substances with different Curie temperatures arranged such that the Curie temperatures progressively increase from one edge of the belt to the other. This magnetic refrigerator can be used to cool and liquefy hydrogen or other fluids.

  7. Magnetic refrigeration apparatus with belt of ferro or paramagnetic material

    DOE Patents [OSTI]

    Barclay, John A. (Madison, WI); Stewart, Walter F. (Marshall, WI); Henke, Michael D. (Los Alamos, NM); Kalash, Kenneth E. (Los Alamos, NM)

    1987-01-01

    A magnetic refrigerator operating in the 12 to 77K range utilizes a belt which carries ferromagnetic or paramagnetic material and which is disposed in a loop which passes through the center of a solenoidal magnet to achieve cooling. The magnetic material carried by the belt, which can be blocks in frames of a linked belt, can be a mixture of substances with different Curie temperatures arranged such that the Curie temperatures progressively increase from one edge of the belt to the other. This magnetic refrigerator can be used to cool and liquefy hydrogen or other fluids.

  8. COLORS OF INNER DISK CLASSICAL KUIPER BELT OBJECTS

    SciTech Connect (OSTI)

    Romanishin, W. [Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 (United States); Tegler, S. C. [Department of Physics and Astronomy, Northern Arizona University, Flagstaff, AZ 86011 (United States); Consolmagno, G. J., E-mail: wromanishin@ou.ed, E-mail: Stephen.Tegler@nau.ed, E-mail: gjc@specola.v [Vatican Observatory, Specola Vaticana, V-00120 (Vatican City State, Holy See)

    2010-07-15

    We present new optical broadband colors, obtained with the Keck 1 and Vatican Advanced Technology telescopes, for six objects in the inner classical Kuiper Belt. Objects in the inner classical Kuiper Belt are of interest as they may represent the surviving members of the primordial Kuiper Belt that formed interior to the current position of the 3:2 resonance with Neptune, the current position of the plutinos, or, alternatively, they may be objects formed at a different heliocentric distance that were then moved to their present locations. The six new colors, combined with four previously published, show that the ten inner belt objects with known colors form a neutral clump and a reddish clump in B-R color. Nonparametric statistical tests show no significant difference between the B-R color distribution of the inner disk objects compared to the color distributions of Centaurs, plutinos, or scattered disk objects. However, the B-R color distribution of the inner classical Kuiper Belt Objects does differ significantly from the distribution of colors in the cold (low inclination) main classical Kuiper Belt. The cold main classical objects are predominately red, while the inner classical belt objects are a mixture of neutral and red. The color difference may reveal the existence of a gradient in the composition and/or surface processing history in the primordial Kuiper Belt, or indicate that the inner disk objects are not dynamically analogous to the cold main classical belt objects.

  9. The formation of the Kuiper belt by the outward transport of

    E-Print Network [OSTI]

    Morbidelli, Alessandro

    .............................................................. The formation of the Kuiper belt ............................................................................................................................................................................. The `dynamically cold Kuiper belt' consists of objects on low- inclination orbits between ,40 and ,50 AU from size unless the cold Kuiper belt originally contained tens of Earth masses of solids. Although several

  10. The albedo, size, and density of binary Kuiper Belt object (47171) 1999 TC36

    E-Print Network [OSTI]

    2006-01-01

    2005. The formation of Kuiper-belt binaries through exchangeand Density of Binary Kuiper Belt Object (47171) 1999 TC 36emission of the binary Kuiper Belt Object (47171) 1999 TC 36

  11. Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope

    E-Print Network [OSTI]

    2007-01-01

    in the scattered Kuiper Belt. Astrophys. J. , 635, L97-L100.al. (2002). The binary Kuiper-belt object 1998 WW31. Nature,2005). The high-albedo Kuiper Belt object (55565) 2002 AW

  12. Euclid Asteroseismology and Kuiper Belt Objects

    E-Print Network [OSTI]

    Gould, A; Stello, D

    2015-01-01

    Euclid, which is primarily a dark-energy/cosmology mission, may have a microlensing component, consisting of perhaps four dedicated one-month campaigns aimed at the Galactic bulge. We show that such a program would yield excellent auxilliary science, including asteroseimology detections for about 100,000 giant stars, and detection of about 1000 Kuiper Belt Objects (KBOs), down to 2--2.5 mag below the observed break in the KBO luminosity function at I ~26. For the 400 KBOs below the break, Euclid will measure accurate orbits, with fractional period errors <~ 2.5%.

  13. SunBelt Biofuels | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page| Open Energy Information Serbia-Enhancing CapacityVectren)Model for the EntireOpenSumpter,Energy GroupSunBelt Biofuels

  14. A POSSIBLE DIVOT IN THE SIZE DISTRIBUTION OF THE KUIPER BELT'S SCATTERING OBJECTS

    SciTech Connect (OSTI)

    Shankman, C.; Gladman, B. J. [Department of Physics and Astronomy, University of British Columbia, 6224 Agriculture Road, Vancouver, BC V6T 1Z1 (Canada); Kaib, N. [Department of Physics and Astronomy, Queens University (Canada); Kavelaars, J. J. [National Research Council of Canada, Victoria, BC V9E 2E7 (Canada); Petit, J. M. [Institut UTINAM, CNRS-Universite de Franche-Comte, Besancon (France)

    2013-02-10

    Via joint analysis of a calibrated telescopic survey, which found scattering Kuiper Belt objects, and models of their expected orbital distribution, we explore the scattering-object (SO) size distribution. Although for D > 100 km the number of objects quickly rise as diameters decrease, we find a relative lack of smaller objects, ruling out a single power law at greater than 99% confidence. After studying traditional ''knees'' in the size distribution, we explore other formulations and find that, surprisingly, our analysis is consistent with a very sudden decrease (a divot) in the number distribution as diameters decrease below 100 km, which then rises again as a power law. Motivated by other dynamically hot populations and the Centaurs, we argue for a divot size distribution where the number of smaller objects rises again as expected via collisional equilibrium. Extrapolation yields enough kilometer-scale SOs to supply the nearby Jupiter-family comets. Our interpretation is that this divot feature is a preserved relic of the size distribution made by planetesimal formation, now ''frozen in'' to portions of the Kuiper Belt sharing a ''hot'' orbital inclination distribution, explaining several puzzles in Kuiper Belt science. Additionally, we show that to match today's SO inclination distribution, the supply source that was scattered outward must have already been vertically heated to the of order 10 Degree-Sign .

  15. The absolute magnitude distribution of Kuiper Belt objects

    SciTech Connect (OSTI)

    Fraser, Wesley C. [Herzberg Institute of Astrophysics, 5071 West Saanich Road, Victoria, BC V9E 2E7 (Canada); Brown, Michael E. [Division of Geological and Planetary Sciences, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Morbidelli, Alessandro [Laboratoire Lagrange, UMR7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, BP 4229, F-06304 Nice (France); Parker, Alex [Department of Astronomy, University of California at Berkeley, Berkeley, CA 94720 (United States); Batygin, Konstantin, E-mail: wesley.fraser@nrc.ca [Institute for Theory and Computation, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS 51, Cambridge, MA 02138 (United States)

    2014-02-20

    Here we measure the absolute magnitude distributions (H-distribution) of the dynamically excited and quiescent (hot and cold) Kuiper Belt objects (KBOs), and test if they share the same H-distribution as the Jupiter Trojans. From a compilation of all useable ecliptic surveys, we find that the KBO H-distributions are well described by broken power laws. The cold population has a bright-end slope, ?{sub 1}=1.5{sub ?0.2}{sup +0.4}, and break magnitude, H{sub B}=6.9{sub ?0.2}{sup +0.1} (r'-band). The hot population has a shallower bright-end slope of, ?{sub 1}=0.87{sub ?0.2}{sup +0.07}, and break magnitude H{sub B}=7.7{sub ?0.5}{sup +1.0}. Both populations share similar faint-end slopes of ?{sub 2} ? 0.2. We estimate the masses of the hot and cold populations are ?0.01 and ?3 × 10{sup –4} M {sub ?}. The broken power-law fit to the Trojan H-distribution has ?{sub 1} = 1.0 ± 0.2, ?{sub 2} = 0.36 ± 0.01, and H {sub B} = 8.3. The Kolmogorov-Smirnov test reveals that the probability that the Trojans and cold KBOs share the same parent H-distribution is less than 1 in 1000. When the bimodal albedo distribution of the hot objects is accounted for, there is no evidence that the H-distributions of the Trojans and hot KBOs differ. Our findings are in agreement with the predictions of the Nice model in terms of both mass and H-distribution of the hot and Trojan populations. Wide-field survey data suggest that the brightest few hot objects, with H{sub r{sup ?}}?3, do not fall on the steep power-law slope of fainter hot objects. Under the standard hierarchical model of planetesimal formation, it is difficult to account for the similar break diameters of the hot and cold populations given the low mass of the cold belt.

  16. Tolerance of combined salinity and O2 deficiency in Hordeum marinum accessions from the grain-belt of Western Australia

    E-Print Network [OSTI]

    Malik1,2,3, AI; English1,2, JP; Shepherd1,4, KA; Islam2,5, AKMR; Colmer1,2, TD

    2009-01-01

    accessions from the grain-belt of Western Australia forcollected from the grain-belt of Western Australia. Single

  17. Visible and infrared photometry of Kuiper Belt objects: searching for evidence of trends

    E-Print Network [OSTI]

    Sheppard, Scott S.

    Visible and infrared photometry of Kuiper Belt objects: searching for evidence of trends Neil Mc. © 2003 Elsevier Science (USA). All rights reserved. Keywords: Kuiper Belt objects; Photometry; Infrared

  18. Best Practices for Rural Traffic Safety Georgia's Experience in Increasing Rural Safety Belt Use Rates

    E-Print Network [OSTI]

    Minnesota, University of

    Best Practices for Rural Traffic Safety Georgia's Experience in Increasing Rural Safety Belt Use Enforcement Efforts ­ Checkpoints ­ Messages regarding Seat Belts ­ Messages regarding Rural SB Use

  19. Radiation belt electrons respond to multiple solar wind inputs

    E-Print Network [OSTI]

    Radiation belt electrons respond to multiple solar wind inputs E. J. Rigler,1 M. Wiltberger,1 and D is clearly valuable from a practical standpoint, but the latter helps build confidence in any physical on the fractional or percent variance of radiation belt electron flux that can be attributed to each different solar

  20. Young Stellar Objects in the Gould Belt

    E-Print Network [OSTI]

    Dunham, Michael M; Evans, Neal J; Broekhoven-Fiene, Hannah; Cieza, Lucas; Di Francesco, James; Gutermuth, Robert A; Harvey, Paul M; Hatchell, Jennifer; Heiderman, Amanda; Huard, Tracy; Johnstone, Doug; Kirk, Jason M; Matthews, Brenda C; Miller, Jennifer F; Peterson, Dawn E; Young, Kaisa E

    2015-01-01

    We present the full catalog of Young Stellar Objects (YSOs) identified in the 18 molecular clouds surveyed by the Spitzer Space Telescope "cores to disks" (c2d) and "Gould Belt" (GB) Legacy surveys. Using standard techniques developed by the c2d project, we identify 3239 candidate YSOs in the 18 clouds, 2966 of which survive visual inspection and form our final catalog of YSOs in the Gould Belt. We compile extinction corrected SEDs for all 2966 YSOs and calculate and tabulate the infrared spectral index, bolometric luminosity, and bolometric temperature for each object. We find that 326 (11%), 210 (7%), 1248 (42%), and 1182 (40%) are classified as Class 0+I, Flat-spectrum, Class II, and Class III, respectively, and show that the Class III sample suffers from an overall contamination rate by background AGB stars between 25% and 90%. Adopting standard assumptions, we derive durations of 0.40-0.78 Myr for Class 0+I YSOs and 0.26-0.50 Myr for Flat-spectrum YSOs, where the ranges encompass uncertainties in the ado...

  1. The Dynamical Evolution of the Asteroid Belt

    E-Print Network [OSTI]

    Morbidelli, Alessandro; O'Brien, David P; Minton, David A; Bottke, William F

    2015-01-01

    The asteroid belt is the leftover of the original planetesimal population in the inner solar system. However, currently the asteroids have orbits with all possible values of eccentricities and inclinations compatible with long-term dynamical stability, whereas the initial planetesimal orbits should have been quasi-circular and almost co-planar. The total mass in the asteroid population is a small fraction of that existing primordially. Also, asteroids with different chemical/mineralogical properties are not ranked in an orderly manner with mean heliocentric distance as one could expect from the existence of a radial gradient of the temperature in the proto-planetary disk, but they are partially mixed. These properties show that the asteroid belt has been severely sculpted by one or a series of processes during its lifetime. This paper reviews the processes that have been proposed so far, discussing the properties that they explain and the problems that they are confronted with. Emphasis is paid to the interpl...

  2. WATER ICE IN THE KUIPER BELT

    SciTech Connect (OSTI)

    Brown, M. E.; Fraser, W. C. [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Schaller, E. L., E-mail: mbrown@caltech.edu [NASA Dryden Aircraft Operations Facility, Palmdale, CA 93550 (United States)

    2012-06-15

    We examine a large collection of low-resolution near-infrared spectra of Kuiper Belt objects (KBOs) and centaurs in an attempt to understand the presence of water ice in the Kuiper Belt. We find that water ice on the surface of these objects occurs in three separate manners: (1) Haumea family members uniquely show surfaces of nearly pure water ice, presumably a consequence of the fragmentation of the icy mantle of a larger differentiated proto-Haumea; (2) large objects with absolute magnitudes of H < 3 (and a limited number to H = 4.5) have surface coverings of water ice-perhaps mixed with ammonia-that appears to be related to possibly ancient cryovolcanism on these large objects; and (3) smaller KBOs and centaurs which are neither Haumea family members nor cold-classical KBOs appear to divide into two families (which we refer to as 'neutral' and 'red'), each of which is a mixture of a common nearly neutral component and either a slightly red or very red component that also includes water ice. A model suggesting that the difference between neutral and red objects due to formation in an early compact solar system either inside or outside, respectively, of the {approx}20 AU methanol evaporation line is supported by the observation that methanol is only detected on the reddest objects, which are those which would be expected to have the most of the methanol containing mixture.

  3. Abstract of Doctoral Dissertation in "Engineering and Public Policy, EPP" Retrospectiveand Prospective Analysis of Incentives for Wind Power in

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    Prospective Analysis of Incentives for Wind Power in Author: Ivonne Peña (pena.ivonne@gmail.com) 2014 IST main parts: a first introductory section, a retrospective study of wind power in Portugal and a prospective analysis of the Portuguese wind power sector. The introductory section is a brief overview

  4. Accepted for publication in Wireless Networks, Special Issue on Multiuser Detection in Wireless Communications Adaptive Power Control and MMSE Interference

    E-Print Network [OSTI]

    Yates, Roy

    with an acceptable quality of service while minimizing the total transmitter power. Multiuser detection on the other communication systems, iterative power control is used to provide each user with an acceptable level and interference. In [10], a framework was given for uplink power control for cellular radio systems. Variations

  5. Accurately specifying storm-time ULF wave radial diffusion in the radiation belts

    E-Print Network [OSTI]

    Dimitrakoudis, Stavros; Balasis, Georgios; Papadimitriou, Constantinos; Anastasiadis, Anastasios; Daglis, Ioannis A

    2015-01-01

    Ultra-low frequency (ULF) waves can contribute to the transport, acceleration and loss of electrons in the radiation belts through inward and outward diffusion. However, the most appropriate parameters to use to specify the ULF wave diffusion rates are unknown. Empirical representations of diffusion coefficients often use Kp; however, specifications using ULF wave power offer an improved physics-based approach. We use 11 years of ground-based magnetometer array measurements to statistically parameterise the ULF wave power with Kp, solar wind speed, solar wind dynamic pressure and Dst. We find Kp is the best single parameter to specify the statistical ULF wave power driving radial diffusion. Significantly, remarkable high energy tails exist in the ULF wave power distributions when expressed as a function of Dst. Two parameter ULF wave power specifications using Dst as well as Kp provide a better statistical representation of storm-time radial diffusion than any single variable alone.

  6. Piezoelectric and Semiconducting Coupled Power Generating Process of a

    E-Print Network [OSTI]

    Wang, Zhong L.

    observation of piezoelectric generation from a single ZnO wire/belt for illustrating a fundamental process of the electric generator relies on the unique coupling of piezoelectric and semiconducting dual properties of ZnPiezoelectric and Semiconducting Coupled Power Generating Process of a Single ZnO Belt

  7. INCLINATION MIXING IN THE CLASSICAL KUIPER BELT

    SciTech Connect (OSTI)

    Volk, Kathryn; Malhotra, Renu, E-mail: kvolk@lpl.arizona.edu [Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721 (United States)

    2011-07-20

    We investigate the long-term evolution of the inclinations of the known classical and resonant Kuiper Belt objects (KBOs). This is partially motivated by the observed bimodal inclination distribution and by the putative physical differences between the low- and high-inclination populations. We find that some classical KBOs undergo large changes in inclination over gigayear timescales, which means that a current member of the low-inclination population may have been in the high-inclination population in the past, and vice versa. The dynamical mechanisms responsible for the time variability of inclinations are predominantly distant encounters with Neptune and chaotic diffusion near the boundaries of mean motion resonances. We reassess the correlations between inclination and physical properties including inclination time variability. We find that the size-inclination and color-inclination correlations are less statistically significant than previously reported (mostly due to the increased size of the data set since previous works with some contribution from inclination variability). The time variability of inclinations does not change the previous finding that binary classical KBOs have lower inclinations than non-binary objects. Our study of resonant objects in the classical Kuiper Belt region includes objects in the 3:2, 7:4, 2:1, and eight higher-order mean motion resonances. We find that these objects (some of which were previously classified as non-resonant) undergo larger changes in inclination compared to the non-resonant population, indicating that their current inclinations are not generally representative of their original inclinations. They are also less stable on gigayear timescales.

  8. SCHOLARLY PUBLICATIONS Scholarly PublicationS

    E-Print Network [OSTI]

    2012 SCHOLARLY PUBLICATIONS #12;#12;Scholarly PublicationS 2012 #12;Editor: caroline brandt Publications 2012 1 contents Introduction

  9. The Warped Plane of the Classical Kuiper Belt

    E-Print Network [OSTI]

    Eugene Chiang; Hyomin Choi

    2008-06-02

    By numerically integrating the orbits of the giant planets and of test particles over a period of four billion years, we follow the evolution of the location of the midplane of the Kuiper belt. The Classical Kuiper belt conforms to a warped sheet that precesses with a 1.9 Myr period. The present-day location of the Kuiper belt plane can be computed using linear secular perturbation theory: the local normal to the plane is given by the theory's forced inclination vector, which is specific to every semimajor axis. The Kuiper belt plane does not coincide with the invariable plane, but deviates from it by up to a few degrees in stable zones. For example, at a semimajor axis of 38 AU, the local Kuiper belt plane has an inclination of 1.9 deg and a longitude of ascending node of 149.9 deg when referred to the mean ecliptic and equinox of J2000. At a semimajor axis of 43 AU, the local plane has an inclination of 1.9 deg and a nodal longitude of 78.3 deg. Only at infinite semimajor axis does the Kuiper belt plane merge with the invariable plane, whose inclination is 1.6 deg and nodal longitude is 107.7 deg. A Kuiper belt object keeps its inclination relative to the Kuiper belt plane nearly constant, even while the latter plane departs from the trajectory predicted by linear theory. The constancy of relative inclination reflects the undamped amplitude of free oscillation. Current observations of Classical Kuiper belt objects are consistent with the plane being warped by the giant planets alone, but the sample size will need to increase by a few times before confirmation exceeds 3-sigma in confidence. In principle, differences between the theoretically expected plane and the observed plane could be used to infer as yet unseen masses orbiting the Sun, but carrying out such a program would be challenging.

  10. From the Kuiper Belt to JupiterFamily Comets: The Spatial Distribution of Ecliptic Comets

    E-Print Network [OSTI]

    Levison, Harold F.

    From the Kuiper Belt to Jupiter­Family Comets: The Spatial Distribution of Ecliptic Comets Harold F particles as they evolve from Neptune­encountering orbits in the Kuiper belt for up to 1 Gyr or until, that originated in the Kuiper belt. This conclusion assumes that the rate of objects leaving the Kuiper belt has

  11. Rayleigh-Taylor instability, lithospheric dynamics, surface topography at convergent mountain belts, and gravity anomalies

    E-Print Network [OSTI]

    Kraus, Mary

    Rayleigh-Taylor instability, lithospheric dynamics, surface topography at convergent mountain belts sign. For the range of wavelengths appropriate for convergent mountain belts (~150­600 km), calculated for wave numbers relevant to mountain belts. For essentially all mountain belts, however, measured free

  12. Master of Science in Engineering and Technology Management Louisiana Tech University Six Sigma Black Belt Certification

    E-Print Network [OSTI]

    Selmic, Sandra

    Black Belt Certification A Louisiana Tech University Six Sigma Black Belt certification can be obtained, STAT 507 Design and Analysis of Experiments, and INEN 557 Six Sigma Black Belt Project with a B the Louisiana Tech University Six Sigma Black Belt certification. INEN 514 is offered in the fall and spring

  13. GREENGATE AND FABREEKA BELT PERFORMANCE IN A 3.5 MV TANDEM

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1413 GREENGATE AND FABREEKA BELT PERFORMANCE IN A 3.5 MV TANDEM F. CRISTOFORI Istituto di Fisica of belts used in the 3.5 MV Tandem of C.I.S.E. REVUE DE PHYSIQUE APPLIQUÃ?E TOME 12, OCTOBRE 1977, PAGE belts. Unfortunately there is little information regarding the performance of these belts

  14. MODELING THE EFFECTS OF BELT COMPLIANCE, BACKLASH, AND SLIP ON WEB TENSION AND NEW METHODS FOR

    E-Print Network [OSTI]

    Pagilla, Prabhakar R.

    MODELING THE EFFECTS OF BELT COMPLIANCE, BACKLASH, AND SLIP ON WEB TENSION AND NEW METHODSQuest Information and Learning Company. #12;MODELING THE EFFECTS OF BELT COMPLIANCE, BACKLASH, AND SLIP ON WEB and analysis of the belt compliance 13 2.1 Belt-pulley transmission system

  15. The small numbers of large Kuiper Belt objects

    SciTech Connect (OSTI)

    Schwamb, Megan E. [Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, National Taiwan University. No. 1, Sec. 4, Roosevelt Rd, Taipei 10617, Taiwan (China); Brown, Michael E.; Fraser, Wesley C., E-mail: mschwamb@asiaa.sinica.edu.tw [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States)

    2014-01-01

    We explore the brightness distribution of the largest and brightest (m(R) < 22) Kuiper Belt Objects (KBOs). We construct a luminosity function of the dynamically excited or hot Kuiper Belt (orbits with inclinations >5°) from the very brightest to m(R) = 23. We find for m(R) ? 23, a single slope appears to describe the luminosity function. We estimate that ?12 KBOs brighter than m(R) ? 19.5 are present in the Kuiper Belt today. With nine bodies already discovered this suggests that the inventory of bright KBOs is nearly complete.

  16. Kinematics of the Gould Belt Based on Open Clusters

    E-Print Network [OSTI]

    Vadim V. Bobylev

    2006-10-15

    We have redetermined kinematic parameters of the Gould Belt using currently available data on the motion of nearby young (log t Belt center: Ro=150 pc and lo=128 degrees. The whole structure is shown to move relative to the local standard of rest at a velocity of 10.7+-0.7 km/s in the direction l=274+-4degrees and b=-1+-3 degrees. Using the derived rotation velocity, we have estimated the virial mass of the Gould Belt to be 1.5E6 Solar mass.

  17. Risk-informed public safety policy for seismic events in the vicinity of a nuclear power plant

    E-Print Network [OSTI]

    Afolayan Jejeloye, Olubukola

    2002-01-01

    Nuclear Power Plants (NPPs) are potentially vulnerable to accidents, which can either be internally or externally initiated. External events include natural events like tornadoes, hurricanes, and earthquakes. The purpose ...

  18. Physical effects of collisions in the Kuiper belt

    E-Print Network [OSTI]

    Zoe M. Leinhardt; Sarah T. Stewart; Peter H. Schultz

    2007-05-27

    Collisions are a major modification process over the history of the Kuiper Belt. Recent work illuminates the complex array of possible outcomes of individual collisions onto porous, volatile bodies. The cumulative effects of such collisions on the surface features, composition, and internal structure of Kuiper Belt Objects are not yet known. In this chapter, we present the current state of knowledge of the physics of cratering and disruptive collisions in KBO analog materials. We summarize the evidence for a rich collisional history in the Kuiper Belt and present the range possible physical modifications on individual objects. The question of how well present day bodies represent primordial planetesimals can be addressed through future studies of the coupled physical and collisional evolution of Kuiper Belt Objects.

  19. MAIN-BELT COMET P/2012 T1 (PANSTARRS)

    E-Print Network [OSTI]

    Hsieh, Henry H.

    We present initial results from observations and numerical analyses aimed at characterizing the main-belt comet P/2012 T1 (PANSTARRS). Optical monitoring observations were made between 2012 October and 2013 February using ...

  20. Nanomaterial modifications on conductivity of coal conveyer belt

    SciTech Connect (OSTI)

    Zhang, J.C.; Zhang, Y.G.; Wang, T.T.; Yang, L.F.; Liu, S.M.; Yang, D.H.; Zhang, M.; Gao, X. [Zhongyuan University of Technology, Zhengzhou (China)

    2008-08-15

    By analyzing the macro electrical properties and the microscopic structure from SEM of nanomaterials modified mine transmission belt samples. The influences of the filling process of inorganic nano particle-filled rubber and PVC polymer on the physical properties of coal transmission belt is reviewed, as well as PTC and NTC effect on the stability of the physical properties and stability of materials. Influence of nano-materials and polymer materials for rubber and temperature changes in the plastic filled refining process. Crosslinker and major filler changes in the amount and filled plastic chain time on the conductivity of coal conveyer belt is studied. Influence of cure temperature. Cure time on the mechanical performance is studied. The microscopic mechanism of macro conductivity change of conveyer belt is discussed.

  1. New Horizons Science Photos from NASA's Pluto-Kuiper Belt Mission

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    DOE provided the power supply for NASA's New Horizons Mission, a mission to the Pluto and Charon, a double-planet system, and the Kuiper Belt. There are 61 science photos posted on the New Horizons website, along with mission photos, spacecraft images, launch photos, posters and renderings that are both scientific and artistic. Dates range from June of 2006 to February of 2008. The images can be searched by keywords, by date, or by subject topic. They can also be browsed as an entire list. Each image has a detailed description.

  2. Publication List Publications

    E-Print Network [OSTI]

    Egenhofer, Max J.

    Publication List #12;Publications List authors, title, (complete) source, date Reverse Location Date #12;An Impressive Publication List 1-2 refereed articles per year Increased publication activities in the last year 1-2 journal articles First author on 50% of the publications Publications

  3. Collisional Velocities and Rates in Resonant Planetesimal Belts

    E-Print Network [OSTI]

    Martina Queck; Alexander V. Krivov; Miodrag Sremcevic; Philippe Thebault

    2007-07-23

    We consider a belt of small bodies around a star, captured in one of the external or 1:1 mean-motion resonances with a massive perturber. The objects in the belt collide with each other. Combining methods of celestial mechanics and statistical physics, we calculate mean collisional velocities and collisional rates, averaged over the belt. The results are compared to collisional velocities and rates in a similar, but non-resonant belt, as predicted by the particle-in-a-box method. It is found that the effect of the resonant lock on the velocities is rather small, while on the rates more substantial. The collisional rates between objects in an external resonance are by about a factor of two higher than those in a similar belt of objects not locked in a resonance. For Trojans under the same conditions, the collisional rates may be enhanced by up to an order of magnitude. Our results imply, in particular, shorter collisional lifetimes of resonant Kuiper belt objects in the solar system and higher efficiency of dust production by resonant planetesimals in debris disks around other stars.

  4. Forming the Cold Classical Kuiper Belt in a light Disk

    E-Print Network [OSTI]

    Shannon, Andrew; Lithwick, Yoram

    2015-01-01

    Large Kuiper Belt Objects are conventionally thought to have formed out of a massive planetesimal belt that is a few thousand times its current mass. Such a picture, however, is incompatible with multiple lines of evidence. Here, we present a new model for the conglomeration of Cold Classical Kuiper belt objects, out of a solid belt only a few times its current mass, or a few percent of the solid density in a Minimum Mass Solar Nebula. This is made possible by depositing most of the primordial mass in grains of size centimetre or smaller. These grains collide frequently and maintain a dynamically cold belt out of which large bodies grow efficiently: an order-unity fraction of the solid mass can be converted into large bodies, in contrast to the ~0.1% efficiency in conventional models. Such a light belt may represent the true outer edge of the Solar system, and it may have effectively halted the outward migration of Neptune. In addition to the high efficiency, our model can also produce a mass spectrum that pe...

  5. Replace V-Belts with Notched or Synchronous Belt Drives | Department of

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustmentsShirleyEnergyTher i nAandSummary From: v2.7 Multiple< Back<<Energy Belt drives

  6. SCHOLARLY PUBLICATIONS Scholarly PublicationS

    E-Print Network [OSTI]

    2013 SCHOLARLY PUBLICATIONS #12;Scholarly PublicationS 2013 #12;Editor: Mark hayman academic' notes: #12;THE PETROLEUM INSTITUTE | Scholarly Publications 2013 1 contents Introduction

  7. Angle stations in or for endless conveyor belts

    DOE Patents [OSTI]

    Steel, Alan (Glasgow, GB6)

    1987-04-07

    In an angle station for an endless conveyor belt, there are presented to each incoming run of the belt stationary curved guide members (18, 19) of the shape of a major segment of a right-circular cylinder and having in the part-cylindrical portion (16 or 17) thereof rectangular openings (15) arranged in parallel and helical paths and through which project small freely-rotatable rollers (14), the continuously-changing segments of the curved surfaces of which projecting through said openings (15) are in attitude to change the direction of travel of the belt (13) through 90.degree. during passage of the belt about the part-cylindrical portion (16 or 17) of the guide member (18 or 19). The rectangular openings (15) are arranged with their longer edges lengthwise of the diagonals representing the mean of the helix but with those of a plurality of the rows nearest to each end of the part-cylindrical portion (16 or 17) slightly out of axial symmetry with said diagonals, being slightly inclined in a direction about the intersections (40) of the diagonals of the main portion of the openings, to provide a "toe-in" attitude in relation to the line of run of the endless conveyor belt.

  8. Structure of Possible Long-lived Asteroid Belts

    E-Print Network [OSTI]

    N. W. Evans; S. A. Tabachnik

    2002-04-24

    High resolution simulations are used to map out the detailed structure of two long-lived stable belts of asteroid orbits in the inner Solar system. The Vulcanoid belt extends from 0.09 to 0.20 astronomical units (au), though with a gaps at 0.15 and 0.18 au corresponding to de-stabilising mean motion resonances with Mercury and Venus. As collisional evolution proceeds slower at larger heliocentric distances, kilometre-sized or larger Vulcanoids are most likely to be found in the region between 0.16 and 0.18 au. The optimum location in which to search for Vulcanoids is at geocentric ecliptic longitudes roughly between 9 and 10 degrees. Dynamically speaking, the Earth-Mars belt between 1.08-1.28 au is an extremely stable repository for asteroids on nearly circular orbits. It is interrupted at 1.21 au due to the 3:4 commensurability with the Earth, while secular resonances with Saturn are troublesome beyond 1.17 au. These detailed maps of the fine structure of the belts can be used to plan search methodologies. Strategies for detecting members of the belts are discussed, including the use of infrared wide-field imaging with VISTA, and forthcoming European Space Agency satellite missions like GAIA and BepiColombo.

  9. JOVIAN EARLY BOMBARDMENT: PLANETESIMAL EROSION IN THE INNER ASTEROID BELT

    SciTech Connect (OSTI)

    Turrini, D.; Coradini, A.; Magni, G., E-mail: diego.turrini@ifsi-roma.inaf.it [Istituto di Astrofisica e Planetologia Spaziali, INAF-IAPS, Via Fosso del Cavaliere 100, 00133, Rome (Italy)

    2012-05-01

    The asteroid belt is an open window on the history of the solar system, as it preserves records of both its formation process and its secular evolution. The progenitors of the present-day asteroids formed in the Solar Nebula almost contemporary to the giant planets. The actual process producing the first generation of asteroids is uncertain, strongly depending on the physical characteristics of the Solar Nebula, and the different scenarios produce very diverse initial size-frequency distributions (SFDs). In this work, we investigate the implications of the formation of Jupiter, plausibly the first giant planet to form, on the evolution of the primordial asteroid belt. The formation of Jupiter triggered a short but intense period of primordial bombardment, previously unaccounted for, which caused an early phase of enhanced collisional evolution in the asteroid belt. Our results indicate that this Jovian Early Bombardment caused the erosion or the disruption of bodies smaller than a threshold size, which strongly depends on the SFD of the primordial planetesimals. If the asteroid belt was dominated by planetesimals less than 100 km in diameter, the primordial bombardment would have caused the erosion of bodies smaller than 200 km in diameter. If the asteroid belt was instead dominated by larger planetesimals, the bombardment would have resulted in the destruction of bodies as big as 500 km.

  10. Development of Molten-Salt Heat Transfer Fluid Technology for Parabolic Trough Solar Power Plants - Public Final Technical Report

    SciTech Connect (OSTI)

    Grogan, Dylan C. P.

    2013-08-15

    Executive Summary This Final Report for the "Development of Molten-Salt Heat Transfer Fluid (HTF) Technology for Parabolic Trough Solar Power Plants” describes the overall project accomplishments, results and conclusions. Phase 1 analyzed the feasibility, cost and performance of a parabolic trough solar power plant with a molten salt heat transfer fluid (HTF); researched and/or developed feasible component options, detailed cost estimates and workable operating procedures; and developed hourly performance models. As a result, a molten salt plant with 6 hours of storage was shown to reduce Thermal Energy Storage (TES) cost by 43.2%, solar field cost by 14.8%, and levelized cost of energy (LCOE) by 9.8% - 14.5% relative to a similar state-of-the-art baseline plant. The LCOE savings range met the project’s Go/No Go criteria of 10% LCOE reduction. Another primary focus of Phase 1 and 2 was risk mitigation. The large risk areas associated with a molten salt parabolic trough plant were addressed in both Phases, such as; HTF freeze prevention and recovery, collector components and piping connections, and complex component interactions. Phase 2 analyzed in more detail the technical and economic feasibility of a 140 MWe,gross molten-salt CSP plant with 6 hours of TES. Phase 2 accomplishments included developing technical solutions to the above mentioned risk areas, such as freeze protection/recovery, corrosion effects of applicable molten salts, collector design improvements for molten salt, and developing plant operating strategies for maximized plant performance and freeze risk mitigation. Phase 2 accomplishments also included developing and thoroughly analyzing a molten salt, Parabolic Trough power plant performance model, in order to achieve the project cost and performance targets. The plant performance model and an extensive basic Engineering, Procurement, and Construction (EPC) quote were used to calculate a real levelized cost of energy (LCOE) of 11.50¢/kWhe , which achieved the Phase 2 Go/No Go target of less than 0.12¢/kWhe. Abengoa Solar has high confidence that the primary risk areas have been addressed in the project and a commercial plant utilizing molten salt is economically and technically feasible. The strong results from the Phase 1 and 2 research, testing, and analyses, summarized in this report, led Abengoa Solar to recommend that the project proceed to Phase 3. However, a commercially viable collector interconnection was not fully validated by the end of Phase 2, combined with the uncertainty in the federal budget, forced the DOE and Abengoa Solar to close the project. Thus the resources required to construct and operate a molten salt pilot plant will be solely supplied by Abengoa Solar.

  11. EIA publications directory, 1992

    SciTech Connect (OSTI)

    Not Available

    1993-06-24

    This directory contains abstracts and ordering information for EIA publications. The abstracts are arranged by broad subject category such as coal, petroleum, natural gas, and electric power. A comprehensive subject index, a title index, and a report number index are included. Each entry gives the title, report number, publication frequency, date, number of pages, and ordering information. Publication began with the 1979 edition.

  12. Early Proterozoic transcontinental orogenic belts in the United States

    SciTech Connect (OSTI)

    Van Schmus, W.R. . Dept. of Geology); Bickford, M.E. . Dept. of Geology); Condie, K.C. . Dept. Geoscience)

    1993-02-01

    It has been recognized for many years that Early Proterozoic orogenic rocks in the western US range from 1.8 to 1.6 Ga, with a general distribution such that 1.8 to 1.7 Ga rocks underlie Colorado, northern Arizona, and northern New Mexico and 1.7 to 1.6 Ga rocks underlie southern Arizona and southern New Mexico. Recent U-Pb geochronologic and Sm-Nd isotopic studies by a variety of research groups have refined crustal history in the western region and have extended knowledge eastward into the buried midcontinent basement. As a result, the authors propose that 1.8 Ga to 1.6 Ga crust of the US by divided into two distinct, but overlapping, orogenic belts: a 1.8 to 1.7 Ga Inner Accretionary Belt and a 1.7 to 1.6 Ga Outer Tectonic Belt. The Inner Accretionary Belt (IAB) comprises rock suites with compositions and isotopic signatures compatible with origin as juvenile crustal terranes formed as oceanic or off-shore and related terranes that were accreted to southern Laurentia between 1.8 and 1.6 Ga. The IAB includes the Yavapai Province of Arizona, Early Proterozoic basement of Colorado and southern Wyoming, and the basement of Nebraska. The Mojave Province of California may be part of this belt, although it also includes components derived from older Proterozoic or Archean crust. Extension of the IAB eastward from Nebraska is uncertain at present, although coeval rocks that may be eastern manifestations of this 1.8 to 1.7 Ga orogenesis occur in Wisconsin (1.76 Ga granite-rhyolite suite), Ontario (Killarney granite), Labrador (Makkovic Province) and southern Greenland (Ketilidian orogen). The Outer Tectonic Belt (OTB) comprises rock suites which have compositions, structures, and isotopic signature compatible with origin in continental margin tectonic settings between 1.7 and 1.6 Ga.

  13. Page 1 of 4 Fig. 1. Wireless system for bladder volume monitoring. The belt is

    E-Print Network [OSTI]

    Chiao, Jung-Chih

    Page 1 of 4 Fig. 1. Wireless system for bladder volume monitoring. The belt is worn at the waist of the patient. In this conceptual drawing, the belt is moved upward in order to show the implant location

  14. Applications of an Electrostatic High-Voltage Tether to Radiation Belt Remediation

    E-Print Network [OSTI]

    Applications of an Electrostatic High-Voltage Tether to Radiation Belt Remediation by Christopher F.1.1 Magnetic Mirrors and the Van Allen Belts........................... 10 1.1.2 The Loss Cone

  15. THE SURFACE COMPOSITION OF LARGE KUIPER BELT OBJECT 2007 OR10

    E-Print Network [OSTI]

    Brown, M. E.

    We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice. While most objects in the Kuiper belt with water ice absorption ...

  16. Land regeneration for the 21st Century in the Mersey Belt

    E-Print Network [OSTI]

    Newlands Land regeneration for the 21st Century in the Mersey Belt objectives Newlands (New in the Mersey Belt to support the social and economic regeneration of the area (phase one 2003-2009); improving

  17. Detection of methane on Kuiper Belt Object (50000) Quaoar

    E-Print Network [OSTI]

    E. L. Schaller; M. E. Brown

    2007-10-18

    The near-infrared spectrum of (50000) Quaoar obtained at the Keck Observatory shows distinct absorption features of crystalline water ice, solid methane and ethane, and possibly other higher order hydrocarbons. Quaoar is only the fifth Kuiper belt object on which volatile ices have been detected. The small amount of methane on an otherwise water ice dominated surface suggests that Quaoar is a transition object between the dominant volatile-poor small Kuiper belt objects (KBOs) and the few volatile-rich large KBOs such as Pluto and Eris.

  18. Mantle conveyor beneath the Tethyan collisional belt Thorsten W. Becker a,

    E-Print Network [OSTI]

    Becker, Thorsten W.

    into Eurasia, creating the Bitlis­Zagros collisional belt during the spreading of the Red Sea-Gulf of Aden

  19. Cogeneration and Small Power Production Quarterly Report to the California Public Utilities Commission Third Quarter - September 1982

    SciTech Connect (OSTI)

    1982-09-01

    In the Third Quarter of 1982, the number of signed contracts and committed projects rose from 148 to 173, with a total estimated nominal capacity of these projects of 922 MW. Of this nominal capacity, about 168 MW is operational, and the balance is under contract for development. Of the 173 signed contracts and committed projects, 61 were cogeneration and solid waste projects with a potential of 643 MW. PG and E also had under active discussion 28 cogeneration projects that could generate a total of 968 MW to 1,049 MW, and 10 solid waste projects with a potential of 90 MW to 95 MW. Wind projects under contract number 84, with a generating capability of 85 MW. Also, discussions are being conducted with 17 wind projects, totaling 83 MW. There are 23 hydroelectric projects with signed contracts and a potential of 95 MW, as well as 63 projects under active discussion for 169 MW. In addition, there are 25 hydroelectric projects, with a nominal capacity of 278 MW, that PG and E is constructing or planning to construct. Five contracts have been signed with projects, using other types of electric power generation, capable of producing 100 MW.

  20. Structure of Earth's outer radiation belt inferred from long-term electron flux dynamics

    E-Print Network [OSTI]

    Vassiliadis, Dimitrios

    mapped the radiation-belt structure by quantifying the electron flux variability over the entire radialStructure of Earth's outer radiation belt inferred from long-term electron flux dynamics D September 2003; published 15 October 2003. [1] We map the spatial structure of the electron belts over

  1. Re-examining the main asteroid belt as the primary source of ancient lunar craters

    E-Print Network [OSTI]

    Richardson Jr., James E.

    Re-examining the main asteroid belt as the primary source of ancient lunar craters David A. Minton craters on the ancient lunar highlands were derived from the main asteroid belt in such a way, postulates that a destabilized contiguous inner extension of the main asteroid belt produced a bombardment

  2. Sculpting the Kuiper Belt by a Stellar Encounter: Constraints from the Oort Cloud and Scattered Disk

    E-Print Network [OSTI]

    Levison, Harold F.

    Sculpting the Kuiper Belt by a Stellar Encounter: Constraints from the Oort Cloud and Scattered belt's outer edge (Melita et al: 2002). Thus, we restrict our study to encounters that could have; solar system: general; Oort cloud 1. Introduction Since its discovery in 1992, the Kuiper belt has

  3. High connectivity across the fragmented chemosynthetic ecosystems of the deep Atlantic Equatorial Belt: efficient

    E-Print Network [OSTI]

    Borges, Rita

    Belt: efficient dispersal mechanisms or questionable endemism? SARA TEIXEIRA,* KARINE OLU,* CAROLE Equatorial Belt (AEB). Here, we combined genetic data (COI) from several taxa to assess the possible distributions in overlooked parts of the deep sea. Keywords: Atlantic equatorial belt, chemosynthetic habitats

  4. Forward: Final Version 2007 January 31 Forward to the University of Arizona Kuiper Belt Book

    E-Print Network [OSTI]

    Jewitt, David C.

    Forward: Final Version 2007 January 31 Forward to the University of Arizona Kuiper Belt Book Only belt since 1992. Those of us whose research has "helped the tree grow", a group which includes most a privilege and what a thrill it is to be able to do science this way. The Kuiper belt is amazing in its

  5. Red-belted clearwing Synanthedon myopaeformis Michigan State University's invasive species factsheets

    E-Print Network [OSTI]

    Isaacs, Rufus

    Red-belted clearwing Synanthedon myopaeformis Michigan State University's invasive species State University IPM Program and M. Philip of Michigan Department of Agriculture. The red-belted. Michigan risk maps for exotic plant pests. Other common names small red-belted clearwing, apple clearwing

  6. Discovery of very large amplitude whistler-mode waves in Earth's radiation belts

    E-Print Network [OSTI]

    California at Berkeley, University of

    Discovery of very large amplitude whistler-mode waves in Earth's radiation belts C. Cattell,1 J. R January 2008. [1] During a passage through the Earth's dawn-side outer radiation belt, whistler-mode waves of magnitude larger than previously observed for whistlers in the radiation belt. Although the peak frequency

  7. Optimal Deployment and Efficient Movement of Mobile Sensor Nodes for Long Belt Coverage

    E-Print Network [OSTI]

    Optimal Deployment and Efficient Movement of Mobile Sensor Nodes for Long Belt Coverage Han Xu is a triangle lattice placement. However, what is the optimal placement in a long belt scenario has not been with shifted node strips for complete belt coverage. We prove its optimality in terms of the lowest node

  8. Outer radiation belt boundary location relative to the magnetopause: Implications for magnetopause shadowing

    E-Print Network [OSTI]

    California at Berkeley, University of

    Outer radiation belt boundary location relative to the magnetopause: Implications for magnetopause fluxes of the outer radiation belt often decrease rapidly in response to solar wind disturbances. If the MPS is essential for outer radiation belt electron losses, a close relationship between the outer edge

  9. Large Kuiper Belt Objects: The Mauna Kea 8k CCD Survey

    E-Print Network [OSTI]

    Jewitt, David C.

    Large Kuiper Belt Objects: The Mauna Kea 8k CCD Survey David Jewitt Institute for Astronomy, 2680 1998 January 14 #12; Large Kuiper Belt Objects Page 2 Abstract We describe a large­area ecliptic survey designed to assess the sky­plane surface density of bright Kuiper Belt Objects. We used a 8192 x 8192 pixel

  10. The energization of relativistic electrons in the outer Van Allen radiation belt

    E-Print Network [OSTI]

    Loss, Daniel

    LETTERS The energization of relativistic electrons in the outer Van Allen radiation belt YUE CHEN online: 1 July 2007; doi:10.1038/nphys655 The origin and dynamics of the Van Allen radiation belts is one. These observations represent an important step towards a more complete physical understanding of radiation belt

  11. CONTROL OF A SHAKING BELT CONVEYOR BY A NOVEL APPLICATION OF FLOQUETLYAPUNOV

    E-Print Network [OSTI]

    Spiteri, Raymond J.

    CONTROL OF A SHAKING BELT CONVEYOR BY A NOVEL APPLICATION OF FLOQUET­LYAPUNOV THEORY Raymond J­orientation of workpieces for grasping by a robot is by means of a shaking belt conveyor. Control of small per­ turbations INTRODUCTION A shaking belt conveyor was proposed in [1] to achieve the self­orientation of workpieces in flexi

  12. Geophys. Res. Lett., 17, 3265, 1998. The Global Response of Relativistic Radiation Belt

    E-Print Network [OSTI]

    Reeves, Geoffrey D.

    Geophys. Res. Lett., 17, 3265, 1998. 1 The Global Response of Relativistic Radiation Belt Electrons of the radiation belts at Lª4, however, there was a single enhancement followed by a gradual decay. Radial profiles electron fluxes increased simultaneously at Lª4-6. (2) During the passage of the cloud the radiation belts

  13. The Kuiper Belt As An Evolved Circumstellar David C. Jewitt 1

    E-Print Network [OSTI]

    Jewitt, David C.

    The Kuiper Belt As An Evolved Circumstellar Disk David C. Jewitt 1 Institute for Astronomy­ called Kuiper Belt is a repository of the solar system's most primitive (volatile­rich) matter with orbital semi­ major axes greater than Neptune's 30 AU) have been discovered. Widely known as Kuiper Belt

  14. Submitted to ApJ; preprint: Jan 11, 2011. Inclination Mixing in the Classical Kuiper Belt

    E-Print Network [OSTI]

    Malhotra, Renu

    Submitted to ApJ; preprint: Jan 11, 2011. Inclination Mixing in the Classical Kuiper Belt Kathryn clas- sical and resonant Kuiper belt objects. This is partially motivated by the ob- served bimodal Kuiper belt undergo large changes in inclination (i > 5 ) over gigayear timescales, which means

  15. Radial distributions of equatorial phase space density for outer radiation belt electrons

    E-Print Network [OSTI]

    California at Berkeley, University of

    Radial distributions of equatorial phase space density for outer radiation belt electrons D. L throughout the outer radiation belt using data from the Solid State Telescopes on THEMIS-D. We estimate for the relativistic and non-relativistic populations. Specifically, the PSD distribution of outer belt relativistic

  16. Johnston et al. 1 Preliminary U-Pb Geochronology of the Tugela Terrane, Natal Belt, eastern

    E-Print Network [OSTI]

    Johnston, Stephen T.

    Johnston et al. 1 Preliminary U-Pb Geochronology of the Tugela Terrane, Natal Belt, eastern South of the Mesoproterozoic Natal belt of eastern South Africa. The Tugela terrane consists of a west-plunging structural granitoid suite. Introduction Mesoproterozoic orogenic belts are common to most continental fragments

  17. LANDSLIDE-DRIVEN EROSION AND TOPOGRAPHIC EVOLUTION OF ACTIVE MOUNTAIN BELTS

    E-Print Network [OSTI]

    Weissel, Jeffrey K.

    LANDSLIDE-DRIVEN EROSION AND TOPOGRAPHIC EVOLUTION OF ACTIVE MOUNTAIN BELTS N. HOVIUS* Department a crucial role in the erosion and topographic evolution of active mountain belts. They drive the expansion from active mountain belts. Here, we illustrate these points with observations from the Southern Alps

  18. Incorporating spectral characteristics of Pc5 waves into three-dimensional radiation belt

    E-Print Network [OSTI]

    Elkington, Scot R.

    Incorporating spectral characteristics of Pc5 waves into three-dimensional radiation belt modeling frequency range on radiation belt electrons in a compressed dipole magnetic field is examined-dimensional radiation belt modeling and the diffusion of relativistic electrons, J. Geophys. Res., 110, A03215, doi:10

  19. Comparison of two approaches to automated PI controller tuning for an industrial weigh belt feeder

    E-Print Network [OSTI]

    Collins, Emmanuel

    Comparison of two approaches to automated PI controller tuning for an industrial weigh belt feeder, are applied to an industrial weigh belt feeder that has significant nonlinearities. Both methods do; Weigh belt feeder 1. Introduction Automated controller tuning is of significant in- terest to control

  20. New Directions in Polyvanadate Chemistry:From Cages and Clusters to Baskets, Belts, Bowls, and Barrels

    E-Print Network [OSTI]

    Yaghi, Omar M.

    New Directions in Polyvanadate Chemistry:From Cages and Clusters to Baskets, Belts, Bowls recently ex- panded beyond classical cage/cluster structures to include hitherto unknown basket, belt, bowl 3.14] The belt-shaped [v,0,,]16-anion D is found in 4,['] where it encircles an [*I Prof. W. G

  1. On the Size-Dependence of the Inclination Distribution of the Main Kuiper Belt

    E-Print Network [OSTI]

    Levison, Harold F.

    On the Size-Dependence of the Inclination Distribution of the Main Kuiper Belt Harold F. Levison We present a new analysis of the currently available orbital elements for the known Kuiper belt objects. In the non-resonant, main Kuiper belt we #12;nd a statistically signi#12;cant relationship

  2. High-temperature deformation in the Neoproterozoic transpressional Ribeira belt, southeast Brazil

    E-Print Network [OSTI]

    Bascou, Jérôme

    High-temperature deformation in the Neoproterozoic transpressional Ribeira belt, southeast Brazil; accepted 12 December 2001 Abstract The Neoproterozoic Ribeira belt is subdivided in two domains of anastomosing transcurrent shear zones parallel to the belt. This contrast is interpreted as reflecting

  3. A planetary system as the origin of structure in Fomalhaut's dust belt

    E-Print Network [OSTI]

    Kalas, Paul G.

    A planetary system as the origin of structure in Fomalhaut's dust belt Paul Kalas1 , James R resolution of 0.5 AU. The dust is distributed in a belt 25 AU wide, with a very sharp inner edge at a radial distance of 133 AU, and we measure an offset of 15 AU between the belt's geometric centre and Fomalhaut

  4. Invited Review for Asteroids/Comets/Meteors 1996 The Dynamical Structure of the Kuiper Belt

    E-Print Network [OSTI]

    Levison, Harold F.

    Invited Review for Asteroids/Comets/Meteors 1996 The Dynamical Structure of the Kuiper Belt H 1 , which was the first of over 30 Kuiper Belt objects with radii ¸ 100--200 km that have now been discovered by groundbased observations. When 1992 QB 1 was discovered, the Kuiper Belt was instantly

  5. LONG-TERM DYNAMICS AND THE ORBITAL INCLINATIONS OF THE CLASSICAL KUIPER BELT OBJECTS

    E-Print Network [OSTI]

    Brown, Michael E.

    LONG-TERM DYNAMICS AND THE ORBITAL INCLINATIONS OF THE CLASSICAL KUIPER BELT OBJECTS Marc J in the region of the classical Kuiper belt (41 AU a 47 AU) to explore the role of dynamical instabilities in sculpting the inclination distribution of the classical Kuiper belt objects (KBOs). We find

  6. THE DESIGN OF THE AUTOMATIC CONTROL SYSTEM OF THE GRIPPING-BELT SPEED IN

    E-Print Network [OSTI]

    Boyer, Edmond

    THE DESIGN OF THE AUTOMATIC CONTROL SYSTEM OF THE GRIPPING-BELT SPEED IN LONG-ROOTSTALK TRADITIONAL.R.China, Tel:13836641830, Email:hjxlcj2006@sina.com Abstract This article aims to design a kind of gripping-belt computer as a core combined with fuzzy PID control algorithm. The system can adjust the gripping-belt speed

  7. A FAUNISTIC SURVEY OF NATIVE BEES IN THE MISSISSIPPI BLACK BELT PRAIRIE

    E-Print Network [OSTI]

    Ray, David

    A FAUNISTIC SURVEY OF NATIVE BEES IN THE MISSISSIPPI BLACK BELT PRAIRIE SURVEY OF NATIVE BEES IN THE MISSISSIPPI BLACK BELT PRAIRIE By Beverly A. McGee Smith of Study: A FAUNISTIC SURVEY OF NATIVE BEES IN THE MISSISSIPPI BLACK BELT

  8. SAID/SAPSrelated VLF waves and the outer radiation belt boundary

    E-Print Network [OSTI]

    Santolik, Ondrej

    SAID/SAPSrelated VLF waves and the outer radiation belt boundary Evgeny Mishin,1 Jay Albert,1 for the alteration of the outer radiation belt boundary during (sub)storms. Citation: Mishin, E., J. Albert, and O. Santolik (2011), SAID/SAPSrelated VLF waves and the outer radiation belt boundary, Geophys. Res. Lett., 38

  9. EXPLORATION OF THE KUIPER BELT BY HIGH-PRECISION PHOTOMETRIC STELLAR OCCULTATIONS: FIRST RESULTS

    E-Print Network [OSTI]

    Roques, Françoise

    EXPLORATION OF THE KUIPER BELT BY HIGH-PRECISION PHOTOMETRIC STELLAR OCCULTATIONS: FIRST RESULTS F detected are caused by Kuiper Belt objects beyond 100 AU from the Sun and hence are the farthest known objects in the solar system. These detections show that the Kuiper Belt is much more extended than

  10. Tectonic and petrologic evolution of the Kodiak batholith and the trenchward belt, Kodiak Island, AK: Contact

    E-Print Network [OSTI]

    Wang, Yang

    and the trenchward belt, Kodiak Island, AK: Contact fault juxtaposition? David W. Farris1 Received 4 March 2009; revised 23 December 2010; accepted 9 March 2010; published 20 July 2010. [1] Two forearc magmatic belts exist in Kodiak Island, the granitic Kodiak batholith and the basaltic trenchward belt. Both are part

  11. EVIDENCE FOR A COLOR DEPENDENCE IN THE SIZE DISTRIBUTION OF MAIN-BELT ASTEROIDS Paul Wiegert

    E-Print Network [OSTI]

    Wiegert, Paul

    EVIDENCE FOR A COLOR DEPENDENCE IN THE SIZE DISTRIBUTION OF MAIN-BELT ASTEROIDS Paul Wiegert ($1 km) main-belt asteroids with the 3.6 m Canada-France-Hawaii Telescope. We observed in two filters axis, the difference between the filters in the inner belt is found to be somewhat less pronounced than

  12. The size of the auroral belt during magnetic storms N. Yokoyama1

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    The size of the auroral belt during magnetic storms N. Yokoyama1 , Y. Kamide1 , and H. Miyaoka2 1 and the Dst index, changes in the size of the auroral belt during magnetic storms are studied. It is found that the equatorward boundary of the belt at midnight expands equatorward, reaching its lowest latitude about one hour

  13. Late Cenozoic partitioning of oblique plate convergence in the Zagros fold-and-thrust belt (Iran)

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Late Cenozoic partitioning of oblique plate convergence in the Zagros fold-and-thrust belt (Iran 2 May 2006. [1] The NW trending Zagros fold-and-thrust belt is affected by two major dextral faults operating at the rear of the belt has become partitioned along the newly formed Main Recent Fault

  14. Response of highenergy protons of the inner radiation belt to large magnetic storms

    E-Print Network [OSTI]

    California at Berkeley, University of

    Response of highenergy protons of the inner radiation belt to large magnetic storms Hong Zou,1 belt are found during the large storms. Similar loss events were also measured by the HEO3 satellite. The modeling results based on the stormtime geomagnetic field model (TS04c) and the radiation belt model (AP8

  15. Environment and Planning b: Planning and Design Fringe-belt analysis in France

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Environment and Planning b: Planning and Design Fringe-belt analysis in France : A Conzenian University Estelle.ducom@paris4.sorbonne.fr - 1 - halshs-00203109,version1-9Jan2008 #12;Fringe-belt analysis in France : A Conzenian approach to urban renewal Abstract : This study is based on the fringe-belt model

  16. Toward Application of an Active Fence for Object Detection, Manipulation and Alignment on Conveyer Belt

    E-Print Network [OSTI]

    Belt Andon Salvarinov Shahram Payandeh Experimental Robotics Laboratory (ERL), School of Engineering This paper presents a novel approach for orienting an object on conveyer belt utilizing an Active Fence for each incoming randomly oriented object . Object alignment on conveyor belt by passive fences [2] is one

  17. Evolution of the Namaqua-Natal Belt, southern Africa A geochronological and isotope geochemical review

    E-Print Network [OSTI]

    Patterson, William P.

    Evolution of the Namaqua-Natal Belt, southern Africa ­ A geochronological and isotope geochemical Available online 10 July 2006 Abstract Juvenile crust formation within the Namaqua-Natal Belt occurred of the Mesoproterozoic evolution of the Namaqua-Natal Belt. Graben formation with associated extrusion of lavas

  18. PROCESSES OF URBAN CHANGE: PLANNING AND MONITORING STRATEGIES THROUGH THE APPLICATION OF THE FRINGE BELT

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    BELT MODEL TO NANTES AND RENNES (FRANCE). ESTELLE DUCOM Laboratoire RESO UMR CNRS 6590 Université Rennes 2 Haute Bretagne Estelle.ducom@uhb.fr Abstract : This study is based on the fringe belt model (fringe belts). Formerly at the edge of the built-up area, they are now embedded within it

  19. Recent widening of the tropical belt from global tropopause statistics: Sensitivities

    E-Print Network [OSTI]

    Birner, Thomas

    Recent widening of the tropical belt from global tropopause statistics: Sensitivities Thomas Birner 2010. [1] Several recent studies have shown evidence for a widening of the tropical belt over the past of the resulting widening trend of the tropical belt to these thresholds is investigated using four different

  20. THE SECULAR EVOLUTION OF THE PRIMORDIAL KUIPER BELT Joseph M. Hahn1

    E-Print Network [OSTI]

    Hahn, Joseph M.

    THE SECULAR EVOLUTION OF THE PRIMORDIAL KUIPER BELT Joseph M. Hahn1 Lunar and Planetary Institute to compute the secular evolution of a Kuiper Belt having a variety of masses, and it is shown that the early massive belt was very susceptible to the propagation of low-amplitude apsidal and nodal waves launched

  1. SCULPTING THE KUIPER BELT BY A STELLAR ENCOUNTER: CONSTRAINTS FROM THE OORT CLOUD AND SCATTERED DISK

    E-Print Network [OSTI]

    Morbidelli, Alessandro

    SCULPTING THE KUIPER BELT BY A STELLAR ENCOUNTER: CONSTRAINTS FROM THE OORT CLOUD AND SCATTERED et al. as the cause of the Kuiper belt's outer edge. Thus, we restrict our study to encounters system: formation -- solar system: general 1. INTRODUCTION Since its discovery in 1992, the Kuiper belt

  2. Radiation Belt Activity Indices and Solar Proton Event Alarm on the CRATERRE Project Web Site

    E-Print Network [OSTI]

    Radiation Belt Activity Indices and Solar Proton Event Alarm on the CRATERRE Project Web Site D--Two Radiation Belt Activity Indices, based on electron flux measurement >300 keV and >1.6 MeV, and one Solar updated. Index Terms- CRATERRE project, Radiation belts activity, Space environment I. INTRODUCTION

  3. UT College of Natural Sciences Mandatory Safety Belt Usage in College Vehicles

    E-Print Network [OSTI]

    Jefferys, William

    UT College of Natural Sciences Mandatory Safety Belt Usage in College Vehicles To help ensure concerning the use of safety belts will go into effect immediately. These rules supplement and extend those of the State of Texas and the University of Texas. The term "safety belts" refers to both lap and shoulder

  4. Contrasting the efficiency of radiation belt losses caused by ducted and nonducted whistlermode waves

    E-Print Network [OSTI]

    Cummer, Steven A.

    Contrasting the efficiency of radiation belt losses caused by ducted and nonducted whistlermode, nonducted VLF waves are much less effective in driving radiation belt pitch angle scattering. Citation. Parrot, and J.J. Berthelier (2010), Contrasting the efficiency of radiation belt losses caused by ducted

  5. Retention of canopy lichens after partial-cut harvesting in wet-belt interior cedarhemlock forests,

    E-Print Network [OSTI]

    Northern British Columbia, University of

    Retention of canopy lichens after partial-cut harvesting in wet-belt interior cedar­hemlock forests-growth cedar­hemlock forests of the interior wet-belt of British Columbia are rich in abundance and diversity a zone of high precipitation, the so-called interior wet- belt, which favours the development of lush wet

  6. Toward Application of an Active Fence for Object Detection, Manipulation and Alignment on Conveyer Belt

    E-Print Network [OSTI]

    Belt Andon Salvarinov Shahram Payandeh Experimental Robotics Laboratory ERL, School of Engineering This paper presents a novel approach for orienting an object on conveyer belt utilizing an Active Fence for each incoming randomly oriented object . Object alignment on conveyor belt by passive fences 2 is one

  7. THE MURCHISON GREENSTONE BELT, SOUTH AFRICA: ACCRETED1 SLIVERS WITH CONTRASTING METAMORPHIC CONDITIONS2

    E-Print Network [OSTI]

    Boyer, Edmond

    1 THE MURCHISON GREENSTONE BELT, SOUTH AFRICA: ACCRETED1 SLIVERS WITH CONTRASTING METAMORPHIC.09-2.92 Ga Murchison30 Greenstone Belt (MGB), located in South Africa's Kaapvaal Craton, and discusses deformation patterns observed throughout the belt. These patterns are explained by a N-S compressional36

  8. TIME-RESOLVED PHOTOMETRY OF KUIPER BELT OBJECTS: ROTATIONS, SHAPES, AND PHASE FUNCTIONS

    E-Print Network [OSTI]

    Jewitt, David C.

    TIME-RESOLVED PHOTOMETRY OF KUIPER BELT OBJECTS: ROTATIONS, SHAPES, AND PHASE FUNCTIONS Scott S are less spherical than their main-belt asteroid counterparts, indicating a higher specific angular measured phase darkening for seven Kuiper belt objects in the 0 to 2 phase-angle range. Unlike Pluto

  9. Solar, interplanetary, and magnetospheric parameters for the radiation belt energetic electron flux

    E-Print Network [OSTI]

    Vassiliadis, Dimitrios

    Solar, interplanetary, and magnetospheric parameters for the radiation belt energetic electron flux 2005. [1] In developing models of the radiation belt energetic electron flux, it is important identify its peaks in reference to the radial regions P0 (L = 3.1­4.0, inner edge of the outer belt), P1 (4

  10. ENVIRONMENTAL VARIABLES AFFECTING ANT (FORMICIDAE) COMMUNITY COMPOSITION IN MISSISSIPPI'S BLACK BELT

    E-Print Network [OSTI]

    Ray, David

    BELT AND FLATWOODS REGIONS By JoVonn Grady Hill A Thesis Submitted to the Faculty of Mississippi State COMPOSITION IN MISSISSIPPI'S BLACK BELT AND FLATWOODS REGIONS. By JoVonn Grady Hill Approved: Richard L. Brown (FORMICIDAE) COMMUNITY COMPOSITION IN MISSISSIPPI'S BLACK BELT AND FLATWOODS REGIONS Pages in Study: 72

  11. Metallogeny of precious and base metal mineralization in the Murchison Greenstone Belt, South Africa

    E-Print Network [OSTI]

    Boyer, Edmond

    1 Metallogeny of precious and base metal mineralization in the Murchison Greenstone Belt, South The 3.09-2.97 Ga Murchison Greenstone Belt is an important metallotect in the northern Kaapvaal Craton that the major styles of orogenic Au-Sb and the Cu-Zn VMS mineralization in the Murchison Greenstone Belt

  12. Holocene vegetation and fire dynamics in the supra-mediterranean belt of the Nebrodi Mountains

    E-Print Network [OSTI]

    Bern, Universität

    Holocene vegetation and fire dynamics in the supra-mediterranean belt of the Nebrodi Mountains, a small lake in the supra-mediterranean belt in the Nebrodi Mountains of Sicily (Italy). The data suggest from Sicily. In the thermo-mediterranean belt (i.e. broadleaved evergreen wood- lands

  13. Belt-parallel mantle flow beneath a halted continental collision: The Western Alps Guilhem Barruol a,

    E-Print Network [OSTI]

    Demouchy, Sylvie

    Belt-parallel mantle flow beneath a halted continental collision: The Western Alps Guilhem Barruol belts, is a particularly important objective of "mantle tectonics" that may bring a depth extent a coherent picture of upper mantle anisotropy beneath the belt. The large-scale anisotropy pattern

  14. Solar, interplanetary, and magnetospheric parameters for the radiation belt energetic electron flux

    E-Print Network [OSTI]

    California at Berkeley, University of

    Solar, interplanetary, and magnetospheric parameters for the radiation belt energetic electron flux, and A. J. Klimas (2005), Solar, interplanetary, and magnetospheric parameters for the radiation belt 2005. [1] In developing models of the radiation belt energetic electron flux, it is important

  15. On the Dynamics of Resonant Kuiper Belt Objects

    E-Print Network [OSTI]

    Ing-Guey Jiang; Li-Chin Yeh

    2007-01-29

    We propose a new mechanism of drag-induced resonant capture, which can explain the resonant Kuiper Belt Objects in a natural way. A review and comparison with the traditional mechanism of sweeping capture by the migrating Neptune will be given.

  16. A HYPOTHESIS FOR THE COLOR DIVERSITY OF THE KUIPER BELT

    SciTech Connect (OSTI)

    Brown, M. E.; Fraser, W. C. [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Schaller, E. L., E-mail: mbrown@caltech.edu [NASA Dryden Aircraft Operations Facility, Palmdale, CA 93550 (United States)

    2011-10-01

    We propose a chemical and dynamical process to explain the surface colors of the Kuiper belt. In our hypothesis, the initial bulk compositions of the bodies themselves can be quite diverse-as is seen in comets-but the early surface compositions are set by volatile evaporation after the objects are formed. Strong gradients in surface composition, coupled with UV and particle irradiation, lead to the surface colors that are seen today. The objects formed in the inner part of the primordial belt retain only H{sub 2}O and CO{sub 2} as the major ice species on their surfaces. Irradiation of these species plausibly results in the dark neutrally colored centaurs and Kuiper belt objects (KBOs). Object formed further in the disk retain CH{sub 3}OH, which has been shown to lead to brighter redder surfaces after irradiation, as seen in the brighter redder centaurs and KBOs. Objects formed at the current location of the cold classical Kuiper belt uniquely retain NH{sub 3}, which has been shown to affect irradiation chemistry and could plausibly lead to the unique colors of these objects. We propose observational and experimental tests of this hypothesis.

  17. Pioneer Anomaly and the Kuiper Belt mass distribution

    E-Print Network [OSTI]

    O. Bertolami; P. Vieira

    2006-06-18

    Pioneer 10 and 11 were the first probes sent to study the outer planets of the Solar System and Pioneer 10 was the first spacecraft to leave the Solar System. Besides their already epic journeys, Pioneer 10 and 11 spacecraft were subjected to an unaccounted effect interpreted as a constant acceleration toward the Sun, the so-called Pioneer anomaly. One of the possibilities put forward for explaining the Pioneer anomaly is the gravitational acceleration of the Kuiper Belt. In this work we examine this hypothesis for various models for the Kuiper Belt mass distribution. We find that the gravitational effect due to the Kuiper Belt cannot account for the Pioneer anomaly. Furthermore, we have also studied the hypothesis that drag forces can explain the the Pioneer anomaly; however we conclude that the density required for producing the Pioneer anomaly is many orders of magnitude greater than those of interplanetary and interstellar dust. Our conclusions suggest that only through a mission, the Pioneer anomaly can be confirmed and further investigated. If a mission with these aims is ever sent to space, it turns out, on account of our results, that it will be also a quite interesting probe to study the mass distribution of the Kuiper Belt.

  18. Effective Conveyor Belt Inspection for Improved Mining Productivity

    SciTech Connect (OSTI)

    Chris Fromme

    2006-06-01

    This document details progress on the project entitled ''Effective Conveyor Belt Inspection for Improved Mining Productivity'' during the period from November 15, 2004 to May 14, 2004. Highlights include fabrication of low-cost prototype hardware, acquisition of infrared thermal data, and initial design of a Smart-Camera based system.

  19. Effective Conveyor Belt Inspection for Improved Mining Productivity

    SciTech Connect (OSTI)

    Chris Fromme

    2006-06-01

    This document details progress on the project entitled ''Effective Conveyor Belt Inspection for Improved Mining Productivity'' during the period from November 15, 2004 to May 14, 2004. Highlights include fabrication of an improved LED lightbar, fabrication of a line-scan sensor head for the Smart-Camera based prototype, and development of prototype vulcanized splice detection algorithms.

  20. PRECIPITATION OF RADIATION BELT ELECTRONS BY LIGHTNING-GENERATED

    E-Print Network [OSTI]

    PRECIPITATION OF RADIATION BELT ELECTRONS BY LIGHTNING-GENERATED MAGNETOSPHERICALLY REFLECTING-order model to estimate the L-shell dependence of the precipitation flux of energetic electrons driven by MR L-shell extent) peak in the precipitation signature can result due to the focusing of the whistler

  1. MAIN-BELT COMET P/2008 R1 (GARRADD)

    SciTech Connect (OSTI)

    Jewitt, David; Yang Bin; Haghighipour, Nader [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)], E-mail: jewitt@ifa.hawaii.edu, E-mail: yangbin@ifa.hawaii.edu, E-mail: nader@ifa.hawaii.edu

    2009-05-15

    We present a study of the newly discovered main-belt comet P/2008 R1 (Garradd), an object with the dynamical characteristics of an asteroid and the physical characteristics of a comet. Photometry sets a limit to the effective radius of the nucleus at r{sub e} < 0.7 km (red geometric albedo 0.05 assumed). The coma shows a secular fading in our data caused by the escape of dust particles from the near-nucleus environment. The optical reflection spectrum is a nearly neutral continuum devoid of gaseous emission lines, from which we derive a limit to the cyanide (CN) radical production rate of Q {sub CN}< 1.4 x 10{sup 23} s{sup -1} and infer a mass-loss rate <1.5 kg s{sup -1} at the time of our observations. Unlike the first-reported main-belt comets, P/2008 R1 is not dynamically stable. The nearby 8:3 mean-motion resonance with Jupiter induces dynamical instability on timescales 20-30 Myr. Hence, we conclude that P/2008 R1 has recently arrived from a more stable source elsewhere. The high Tisserand parameter of the orbit (in fact, with T{sub J} = 3.216 it is the highest of any comet) points to a source in the asteroid belt itself, instead of in the Kuiper belt (putative source of the Jupiter family comets). We infer that P/2008 R1 is an icy body from the outer asteroid belt in which sublimation has been triggered by rising temperatures resulting from a decreasing perihelion distance.

  2. Electron Acceleration and Loss in the Earth'sElectron Acceleration and Loss in the Earth's Radiation Belts: The Contribution of WaveRadiation Belts: The Contribution of Wave--

    E-Print Network [OSTI]

    Chan, Anthony Arthur

    's Radiation Belts: The Contribution of WaveRadiation Belts: The Contribution of Wave-- particle.Horne@bas.ac.ukR.Horne@bas.ac.uk Tutorial, GEM, Telluride, Colorado, 25 June 2002 Outline ·· RelevanceRelevance ·· Radiation belt variabilityRadiation belt variability ·· Existing theoriesExisting theories ·· Evidence for wave

  3. On auroral dynamics observed by HF radar: 1. Equatorward edge of the afternoon-evening diuse luminosity belt

    E-Print Network [OSTI]

    Boyer, Edmond

    luminosity belt M. Uspensky1,4 , P. Eglitis1,2 , H. Opgenoorth1,2 , G. Starkov3 , T. Pulkkinen1 , R. Pellinen luminosity belt (SEEL) and the ionospheric footprint of the inner boundary of the electron plasma sheet wave scattering belt and the intense irregular- ity curtains which include the visual auroral belt

  4. Why Democracy Is Public: The American Dream Beats the Nightmare

    E-Print Network [OSTI]

    Lakoff, George

    2011-01-01

    dams, sewers, and a power grid, agencies to monitor disease,mains, sewers, and the power grid; public agencies that

  5. Publications Received

    E-Print Network [OSTI]

    Mester, [No author

    1988-01-01

    No. (Spring, 1988) Publications Received Alianza Editorial (1 (Winter/Spring 1986). Publications Received International

  6. Publications Received

    E-Print Network [OSTI]

    Mester, [No author

    1991-01-01

    Publications Received Agua. 1 (enero 1991). ¡Aha! Hispanicmismáticos. ) XL:222-227. Publications Received Oribatejo:

  7. 1 Public Policy and Public Administration PUBLIC POLICY AND PUBLIC

    E-Print Network [OSTI]

    Vertes, Akos

    1 Public Policy and Public Administration PUBLIC POLICY AND PUBLIC ADMINISTRATION Through its Trachtenberg School of Public Policy and Public Administration, Columbian College of Arts and Sciences offers the Master of Public Policy, Master of Public Administration, and the Doctor of Philosophy in the field

  8. Offering Songs, Festive Songs, Processional Songs mGar-gLu, Khro-Glu, Phebsnga: Khang Lhamo, Yandol & Pema Dolma Music: Ri di ngak me ri la, 'The belt on the boots'

    E-Print Network [OSTI]

    Blumenthal, Katey

    Translation of title The belt on the boots Description (to be used in archive entry) A song about festive dress and customs. Genre or type (i.e. epic, song, ritual) ‘khro glu (festive song) Medium (i.e. reel to reel, web-based file, DVD) Digital... Level of public access (fully closed, fully open) Fully open for web streaming Notes and context (include reference to any related documentation, such as photographs) "This belt is really long on the boots. If we use it on the waist it's short. You...

  9. Publications | NISAC

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergyPublications

  10. Gravity interpretation of the northern Overthrust Belt, Idaho and Wyoming 

    E-Print Network [OSTI]

    Silver, Wendy Ilene

    1979-01-01

    GRAVITY INTERPRETATION OF THE NORTHERN OVERTHRUST BELT, IDAHO AND 'vlYOMING A Thesis by IJENDY ILENE SILVER Submitted to the Graduate College of Texas ARM University in partial fulfillment of the requirements for the deoree of MASTER... OF SCIFNCE December 1979 Major Subject: Geology GRAVITY INTERPRETATION OF THE NORTHERN OVERTHRUST lIELT, . IDAHO AND NYOMING A Thesis by NENDY ILEI'lE 5!, LVER Approved as to style and content by: (Chairman of Committee (Hea o epartment (i~1embe...

  11. The Origin and Evolution of the Asteroid Main Belt

    E-Print Network [OSTI]

    Philip R. Bidstrup; Henning Haack; Anja C. Andersen; Rene Michelsen; John Leif Jorgensen

    2005-11-11

    Using a fully autonomous spacecraft - Bering - we propose to detect and study sub-km asteroids from an orbit within the asteroid Main Belt. The main purpose of the proposed Bering mission is to detect a statistically significant sample of an expected population of approximately 10^(10) main belt asteroids in the size range 1 m to 1 km. These asteroids are too faint to be observed using Earth-based telescopes. Sub-km asteroids can be detected from spacecraft at close range but due to the high relative velocities and the long communication times this requires a fully autonomous spacecraft. Using theoretical estimates of the distribution and abundance of sub-km asteroids we find that the Bering mission would detect approximately 6 new sub-km asteroids per day. With an expected lifetime for the mission of a few years we expect to detect and study several thousand sub-km asteroids. Results from the Bering mission would allow us to: 1) Provide further links between groups of meteorites and their parent asteroids. 2) Constrain the cratering rate at planetary surfaces and thus allow significantly improved cratering ages for terrains on Mars and other planets. 3) Constrain processes that transfer small asteroids from orbits in the main belt to the inner Solar System.

  12. Detection of Small Kuiper Belt Objects by Stellar Occultations

    E-Print Network [OSTI]

    R. Stevenson

    2007-12-10

    Knowledge of the Kuiper Belt is currently limited to those objects that can be detected directly. Objects with diameters less than $\\sim$10km reflect too little light to be detected. These smaller bodies could contain most of the mass in the Kuiper Belt while the abundance of these bodies may constrain the distribution of mass. The overall size distribution of bodies within the Kuiper Belt can also be inferred from the relative abundances of sub-km and larger bodies. Stellar occultations are already used to study dark objects in the Solar System, such as asteroids or planetary rings. Occultation by a KBO of a size comparable to, or larger than, that of the Fresnel Scale will result in Fresnel diffraction. Detection of diffraction effects requires fast multiple-star photometry, which will be conducted in July 2007 using the Orthogonal Parallel Transfer Imaging Camera (OPTIC) mounted on the University of Hawaii 2.2m telescope on Mauna Kea. This paper details how knowledge of the mass and structure of the outer Solar System may be obtained through the detection of serendipitous stellar occultations.

  13. Recent Publications

    E-Print Network [OSTI]

    Students, DCRP

    2002-01-01

    Journal 1 6 (2002) RECENT PUBLICATIONS Department of CityRedevelopment. Recent Publications Professional ReportsREAL World. Recent Publications Won g, Jeann ie. Building a

  14. Publications Received

    E-Print Network [OSTI]

    Mester, [No author

    1988-01-01

    Vol. xvii. No. 2 (Fali, Publications Received Anales de lafor Afro-American Studies Publications, 1987. Morris, C.Essays in Memory Publications Received of Federico García

  15. Publications Received

    E-Print Network [OSTI]

    Mester, [No author

    1992-01-01

    xxi. No. (Spring, ¡992) Publications Received ¡Aha! HispanicTemporal. Gávea-Brown Publications, Center for Portuguesenoviembre/diciembre 1991). Publications Received Shalom: A

  16. EIA Publications Directory 1993

    SciTech Connect (OSTI)

    Not Available

    1994-07-18

    This directory contains abstracts and ordering information for EIA publications released in the above time period. The abstracts are arranged by broad subject category such as coal, petroleum, natural gas, and electric power. A comprehensive subject index, a title index, and a report number index are included. Each entry gives the title, report number, publication frequency, date, number of pages, and ordering information.

  17. INITIAL PLANETESIMAL SIZES AND THE SIZE DISTRIBUTION OF SMALL KUIPER BELT OBJECTS

    SciTech Connect (OSTI)

    Schlichting, Hilke E. [UCLA, Department of Earth and Space Science, 595 Charles E. Young Drive East, Los Angeles, CA 90095 (United States); Fuentes, Cesar I.; Trilling, David E., E-mail: hilke@ucla.edu [Department of Physics and Astronomy, Northern Arizona University, P.O. Box 6010, Flagstaff, AZ 86011 (United States)

    2013-08-01

    The Kuiper Belt is a remnant from the early solar system and its size distribution contains many important constraints that can be used to test models of planet formation and collisional evolution. We show, by comparing observations with theoretical models, that the observed Kuiper Belt size distribution is well matched by coagulation models, which start with an initial planetesimal population with radii of about 1 km, and subsequent collisional evolution. We find that the observed size distribution above R {approx} 30 km is primordial, i.e., it has not been modified by collisional evolution over the age of the solar system, and that the size distribution below R {approx} 30 km has been modified by collisions and that its slope is well matched by collisional evolution models that use published strength laws. We investigate in detail the resulting size distribution of bodies ranging from 0.01 km to 30 km and find that its slope changes several times as a function of radius before approaching the expected value for an equilibrium collisional cascade of material strength dominated bodies for R {approx}< 0.1 km. Compared to a single power-law size distribution that would span the whole range from 0.01 km to 30 km, we find in general a strong deficit of bodies around R {approx} 10 km and a strong excess of bodies around 2 km in radius. This deficit and excess of bodies are caused by the planetesimal size distribution left over from the runaway growth phase, which left most of the initial mass in small planetesimals while only a small fraction of the total mass is converted into large protoplanets. This excess mass in small planetesimals leaves a permanent signature in the size distribution of small bodies that is not erased after 4.5 Gyr of collisional evolution. Observations of the small Kuiper Belt Object (KBO) size distribution can therefore test if large KBOs grew as a result of runaway growth and constrained the initial planetesimal sizes. We find that results from recent KBO occultation surveys and the observed KBO size distribution can be best matched by an initial planetesimal population that contained about equal mass per logarithmic mass bin in bodies ranging from 0.4 km to 4 km in radius. We further find that we cannot match the observed KBO size distribution if most of the planetesimal mass was contained in bodies that were 10 km in radius or larger simply because their resulting size distribution cannot be sufficiently depleted over 4.5 Gyr to match observations.

  18. Data From HANE-Generated Radiation Belts and the Origin of Diffusion Theory

    SciTech Connect (OSTI)

    Winske, Dan [Los Alamos National Laboratory

    2012-07-16

    In this presentation we briefly review some of the published data regarding the artificial radiation belts produced by the Starfish and R2 high altitude nuclear explosions in 1962. The data showed slow temporal variations of the belts in altitude (L) and pitch angle ({alpha}) that could be modeled as a diffusion process. That early work formed the basis for more complex radiation belt diffusion models that are in use at present.

  19. Publications Received

    E-Print Network [OSTI]

    Mester, [No author

    1992-01-01

    No. 2 (Fali. 1992) xxi. Publications Received Aha! HispanicDias, Erika. kok, 1988. Publications Received East and West

  20. PowerPoint Presentation

    Office of Environmental Management (EM)

    the public's investment in wind technologies to improve the performance and lower the cost of wind power. TARGETS: * Reduce vehicle petroleum use by 1 billion gallonsyear by...

  1. Gould Belt Kinematics on the Base of the Open Clusters and Ob-Associations

    E-Print Network [OSTI]

    Vadim V. Bobylev; Anisa T. Bajkova

    2006-08-12

    The kinematic parameters of the Gould Belt are redetermined using modern data on the motion of nearby young ($\\log tBelt centre: $l_\\circ=128^\\circ$ and $R_\\circ=150$ pc. It is shown that the whole structure of the Gould Belt is moving relative to the local standard of rest with a velocity of $10.7\\pm0.7$ km s$^{-1}$ in the direction towards $l=274\\pm4^\\circ$, $b=-1\\pm3^\\circ$. Using the rotation velocity, we obtained the virial estimation of the Gould Belt mass as $1.5\\times 10^6 M_\\odot$.

  2. Structure and anisotropy of the Mexico subduction zone based on Rayleigh-wave analysis and implications for the geometry of the Trans-Mexican Volcanic Belt

    E-Print Network [OSTI]

    Stubailo, I; Beghein, C; Davis, PM

    2012-01-01

    across the central Mexican volcanic belt at 100 W: Spatialcentral Trans-Mexican volcanic belt, Chem. Geol. , 244(3–4),Trans-Mexican volcanic belt: Slab detachment in a subduction

  3. UNBIASED INCLINATION DISTRIBUTIONS FOR OBJECTS IN THE KUIPER BELT

    SciTech Connect (OSTI)

    Gulbis, A. A. S. [South African Astronomical Observatory, P.O. Box 9, Observatory, 7935 Cape Town (South Africa); Elliot, J. L.; Adams, E. R. [Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139-4307 (United States); Benecchi, S. D. [Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719 (United States); Buie, M. W. [Department of Space Studies, Southwest Research Institute, 1050 Walnut Street 400, Boulder, CO 80302 (United States); Trilling, D. E. [Department of Physics and Astronomy, Northern Arizona University, P.O. Box 6010, Flagstaff, AZ 86011 (United States); Wasserman, L. H., E-mail: amanda@saao.ac.z, E-mail: jle@mit.ed, E-mail: era@mit.ed, E-mail: lhw@lowell.ed, E-mail: susank@psi.ed, E-mail: buie@boulder.swri.ed, E-mail: David.Trilling@nau.ed [Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001 (United States)

    2010-08-15

    Using data from the Deep Ecliptic Survey (DES), we investigate the inclination distributions of objects in the Kuiper Belt. We present a derivation for observational bias removal and use this procedure to generate unbiased inclination distributions for Kuiper Belt objects (KBOs) of different DES dynamical classes, with respect to the Kuiper Belt plane. Consistent with previous results, we find that the inclination distribution for all DES KBOs is well fit by the sum of two Gaussians, or a Gaussian plus a generalized Lorentzian, multiplied by sin i. Approximately 80% of KBOs are in the high-inclination grouping. We find that Classical object inclinations are well fit by sin i multiplied by the sum of two Gaussians, with roughly even distribution between Gaussians of widths 2.0{sup +0.6}{sub -0.5}{sup 0} and 8.1{sup +2.6}{sub -2.1}{sup 0}. Objects in different resonances exhibit different inclination distributions. The inclinations of Scattered objects are best matched by sin i multiplied by a single Gaussian that is centered at 19.1{sup +3.9}{sub -3.6}{sup 0} with a width of 6.9{sup +4.1}{sub -2.7}{sup 0}. Centaur inclinations peak just below 20{sup 0}, with one exceptionally high-inclination object near 80{sup 0}. The currently observed inclination distribution of the Centaurs is not dissimilar to that of the Scattered Extended KBOs and Jupiter-family comets, but is significantly different from the Classical and Resonant KBOs. While the sample sizes of some dynamical classes are still small, these results should begin to serve as a critical diagnostic for models of solar system evolution.

  4. Two new basaltic asteroids in the Outer Main Belt?

    E-Print Network [OSTI]

    R. Duffard; F. Roig

    2008-01-14

    The identification of basaltic asteroids in the asteroid Main Belt and the description of their surface mineralogy is necessary to understand the diversity in the collection of basaltic meteorites. Basaltic asteroids can be identified from their visible reflectance spectra and are classified as V-type in the usual taxonomies. In this work, we report visible spectroscopic observations of two candidate V-type asteroids, (7472) Kumakiri and (10537) 1991 RY16, located in the outer Main Belt (a > 2.85 UA). These candidate have been previously identified by Roig and Gil-Hutton (2006, Icarus 183, 411) using the Sloan Digital Sky Survey colors. The spectroscopic observations have been obtained at the Calar Alto Observatory, Spain, during observational runs in November and December 2006. The spectra of these two asteroids show the steep slope shortwards of 0.70 microns and the deep absorption feature longwards of 0.75 microns that are characteristic of V-type asteroids. However, the presence of a shallow but conspicuous absorption band around 0.65 microns opens some questions about the actual mineralogy of these two asteroids. Such band has never been observed before in basaltic asteroids with the intensity we detected it. We discuss the possibility for this shallow absorption feature to be caused by the presence of chromium on the asteroid surface. Our results indicate that, together with (1459) Magnya, asteroids (7472) Kumakiri and (10537) 1991 RY16 may be the only traces of basaltic material found up to now in the outer Main Belt.

  5. Los Alamos provides HOPE for radiation belt storm probes

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home Room NewsInformationJesse BergkampCentermillion to local UnitedtoHOPE for radiation belt storm

  6. First ultraviolet reflectance measurements of several Kuiper Belt objects, Kuiper Belt object satellites, and new ultraviolet measurements of A Centaur

    SciTech Connect (OSTI)

    Stern, S. A.; Schindhelm, E.; Cunningham, N. J.

    2014-05-01

    We observed the 2600-3200 Å (hereafter, mid-UV) reflectance of two Kuiper Belt Objects (KBOs), two KBO satellites, and a Centaur, using the Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS). Other than measurements of the Pluto system, these constitute the first UV measurements obtained of KBOs, and KBO satellites, and new HST UV measurements of the Centaur 2060 Chiron. We find significant differences among these objects, constrain the sizes and densities of Haumea's satellites, and report the detection of a possible spectral absorption band in Haumea's spectrum near 3050 Å. Comparisons of these objects to previously published UV reflectance measurements of Pluto and Charon are also made here.

  7. Adiabatic effects on radiation belt electrons at low altitude Weichao Tu1,2

    E-Print Network [OSTI]

    Li, Xinlin

    Adiabatic effects on radiation belt electrons at low altitude Weichao Tu1,2 and Xinlin Li1] The stormtime adiabatic effects of radiation belt electrons mirroring at low altitude are not analogous to those of equatorially mirroring electrons. During the main phase of a geomagnetic storm the adiabatic effects

  8. Modeling the radiation belt electrons with radial diffusion driven by the solar wind

    E-Print Network [OSTI]

    Li, Xinlin

    Modeling the radiation belt electrons with radial diffusion driven by the solar wind A. B. Barker1 October 2005. [1] On the basis of the correlation between the solar wind and radiation belt electron fluxes, we develop a model to simulate the MeV electron phase space density variations from L = 3 to L

  9. Master of Science in Engineering and Technology Management Louisiana Tech University Six Sigma Black Belt Certification

    E-Print Network [OSTI]

    Selmic, Sandra

    Master of Science in Engineering and Technology Management Louisiana Tech University Six Sigma Black Belt Certification A Louisiana Tech University Six Sigma Black Belt certification can be obtained by successfully completing INEN 514 Statistical Analysis for Six Sigma, ENGR 566 Six Sigma and Quality Control

  10. Precambrian Research 136 (2005) 2750 The Wadi Mubarak belt, Eastern Desert of Egypt

    E-Print Network [OSTI]

    Fritz, Harald

    2005-01-01

    Precambrian Research 136 (2005) 27­50 The Wadi Mubarak belt, Eastern Desert of Egypt, Graz, Austria b Mansoura University, Faculty of Science, Geology Department, El Mansoura, Egypt c February 2003; accepted 3 September 2004 Abstract The Wadi Mubarak belt in Egypt strikes west­east (and

  11. Are energetic electrons in the solar wind the source of the outer radiation belt?

    E-Print Network [OSTI]

    Li, Xinlin

    . Mewaldt6 Abstract. Using data from WIND, SAMPEX (Solar, Anomalous, and Magnetospheric Particle Explorer the outer radiation belt electrons. Al- though lower energy electrons in the solar wind could be a seedAre energetic electrons in the solar wind the source of the outer radiation belt? Xinlin Li,1 D. N

  12. Jumping Neptune Can Explain the Kuiper Belt Kernel

    E-Print Network [OSTI]

    Nesvorny, David

    2015-01-01

    The Kuiper belt is a population of icy bodies beyond the orbit of Neptune. A particularly puzzling and up-to-now unexplained feature of the Kuiper belt is the so-called `kernel', a concentration of orbits with semimajor axes a~44 AU, eccentricities e~0.05, and inclinations ibelt kernel can be explained if Neptune's otherwise smooth migration was interrupted by a discontinuous change of Neptune's semimajor axis when Neptune reached ~28 AU. Before the discontinuity happened, planetesimals located at ~40 AU were swept into Neptune's 2:1 resonance, and were carried with the migrating resonance outwards. The 2:1 resonance was at ~44 AU when Neptune reached ~28 AU. If Neptune's semimajor axis changed by fraction of AU at this point, perhaps because Neptune was scattered off of another planet, the 2:1 population would have been released at ~44 AU, and would remain there to this day. We show that the orbital distribution of bodies produced in this model provides a good match to...

  13. Thermal Stress and Reliability for Advanced Power Electronics...

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

    & Publications Thermal Stress and Reliability for Advanced Power Electronics and Electric Machines Power Electronic Thermal System Performance and Integration Thermal...

  14. These works have been submitted to the IEEE for possible publication in the IEEE Transactions on Power Systems. Copyright may be transferred without notice,

    E-Print Network [OSTI]

    of producers and a lack of sufficient energy storage [3]. The ability to identify generators with market power of excess capacity, contractual arrangements, the process for establishing prices, and the ease of market to acknowledge the support of the Power Systems Engineering Research Center (PSERC) and the U.S. Department

  15. inverter. He is the author or co-author of more than 300 publica-tions in his research fields including the book `Control in Power

    E-Print Network [OSTI]

    Simões, Marcelo Godoy

    Power Electronics Society NEWSLETTER 19 Induction Generators for Small Wind Energy Systems M. GodoyW, the induction generator is favored for small hydro and wind power plants. More recently, with the widespread use that enabled people to move away from large urban concentrations, and growing concerns with the environment led

  16. WHY SMALL IS BEAUTIFUL AND HOW TO DETECT ANOTHER 10 BILLION SMALL MAIN BELT ASTEROIDS. Henning Haack1

    E-Print Network [OSTI]

    Andersen, Anja C.

    WHY SMALL IS BEAUTIFUL ­ AND HOW TO DETECT ANOTHER 10 BILLION SMALL MAIN BELT ASTEROIDS. Henning. Introduction: Estimates of the size distribution of main belt asteroids suggest that there is a population- tant sub-kilometer asteroids in the main belt. Long intergration times cannot be used unless the object

  17. PUBLISHED ONLINE: 29 JANUARY 2012 | DOI: 10.1038/NPHYS2185 Explaining sudden losses of outer radiation belt

    E-Print Network [OSTI]

    Loss, Daniel

    of outer radiation belt electrons during geomagnetic storms Drew L. Turner1,2 *, Yuri Shprits1,2,3 , Michael Hartinger1 and Vassilis Angelopoulos1,2 The Van Allen radiation belts were first discovered in 1958 by the Explorer series of spacecraft1 . The dynamic outer belt consists primarily of relativistic

  18. Title: Prompt Creation of New Radiation Belts Cluster: Cross-Theme Theory and Data Analysis/SECTP

    E-Print Network [OSTI]

    Lotko, William

    Title: Prompt Creation of New Radiation Belts Cluster: Cross-Theme Theory and Data Analysis/SECTP Contributor: William Lotko/Dartmouth College · Radiation belt genesis via shock-induced magnetospheric compression The unexpected creation of new electron and proton radiation belts during the March 24, 1991

  19. ApJ, in press; this version: March 01, 2011 Secular resonance sweeping of the main asteroid belt during

    E-Print Network [OSTI]

    Malhotra, Renu

    ApJ, in press; this version: March 01, 2011 Secular resonance sweeping of the main asteroid belt a remnant asteroid belt to survive, we de- rive a lower limit on Saturn's migration speed of 0.15 AU My-1 during the era that the 6 resonance swept through the inner asteroid belt (semimajor axis range 2

  20. Deformation zone `jumps' in a young convergent setting; the Lengguru fold-and-thrust belt, New Guinea Island

    E-Print Network [OSTI]

    Nicolas, Chamot-Rooke

    Deformation zone `jumps' in a young convergent setting; the Lengguru fold-and-thrust belt, New The Lengguru fold-and-thrust belt in West Papua (Indonesia) has all the characteristics of a young orogen buttress. The construction of these two wedges is younger than 11 Myr. The structures of the Lengguru belt

  1. GEOLOGY | Volume 43 | Number 7 | www.gsapubs.org 1 Foreland basin stratigraphic control on thrust belt evolution

    E-Print Network [OSTI]

    Fay, Noah

    belt evolution James B. Chapman and Peter G. DeCelles Department of Geosciences, University of Arizona on thrust belt architecture have not been fully evalu- ated. Mechanical properties of typical foreland basin stratigraphic successions influence the structural development of fold-thrust belts in predictable ways

  2. Bering a deep space mission to study the origin and evolution of the asteroid belt Philip Bidstrup1

    E-Print Network [OSTI]

    Andersen, Anja C.

    Bering ­ a deep space mission to study the origin and evolution of the asteroid belt Philip. An estimated population of approximately 1010 main belt asteroids in the size range 1 m to 1 km are too faint of the fragments are perturbed out of the main belt and fall on Earth as meteorites. The young surfaces and minimal

  3. 2015 EPO No. 14 Belt-Conveyor Scale Systems (Rev 09/14) DRAFT Page 1 of 12

    E-Print Network [OSTI]

    2015 EPO No. 14 Belt-Conveyor Scale Systems (Rev 09/14) DRAFT Page 1 of 12 Examination Procedure Outline for Belt-Conveyor Scale Systems Introduction It is recommended that this outline be followed as minimum criteria for examining belt-conveyor scale systems. This document has been prepared as a guide

  4. Why do continents break-up parallel to ancient orogenic belts? A. Vauchez*, G. Barruol and A. Tommasi?

    E-Print Network [OSTI]

    Barruol, Guilhem

    Why do continents break-up parallel to ancient orogenic belts? A. Vauchez*, G. Barruol and A belts Ocean-opening through rifting and continent break-up is frequently related to the occurrence Atlantic oceans provide spectacularexamples of parallelism be- tween rifts and older orogenic belts

  5. to appear in Astrophysical Journal (Letters) An Analysis of the Statistics of the HST Kuiper Belt Object

    E-Print Network [OSTI]

    Brown, Michael E.

    to appear in Astrophysical Journal (Letters) An Analysis of the Statistics of the HST Kuiper Belt Belt objects in the HST data of Cochran et al. (1995), in which they report the discovery al. The detection of such a population of Halley­sized Kuiper Belt objects with these data

  6. 0036-1445/81.'"2301-0005 $01.00/0 f^MATICAL REMARKS ON THE VAN ALLEN RADIATION BELT

    E-Print Network [OSTI]

    Knill, Oliver

    0036-1445/81.'"2301-0005 $01.00/0 f^MATICAL REMARKS ON THE VAN ALLEN RADIATION BELT: A SURVEY radiation belt, were seemingly i vv j . {severai vears. sd, some of these particles were observed to have center or "adiabatic" approximation.) Under these circumstances, it was #12;THE VAN ALLEN RADIATION BELT

  7. hal-00193179,version1-4Dec2007 Origin of the Structure of the Kuiper Belt during a Dynamical

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    hal-00193179,version1-4Dec2007 Origin of the Structure of the Kuiper Belt during a Dynamical explore the origin and orbital evolution of the Kuiper belt in the frame- work of a recent model would stop migrating at its currently observed location. As a result, the Kuiper belt would have

  8. Tectonics of the Middle Triassic intracontinental Xuefengshan Belt, South China: new insights from structural and chronological constraints on the basal

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Tectonics of the Middle Triassic intracontinental Xuefengshan Belt, South China: new insights-012-0780-5 #12;2 Abstract: In orogenic belts, a basal décollement zone often develops at depth to accommodate Xuefengshan Belt of South China, such a décollement zone is exposed in the core of anticlines formed

  9. P-and S-Wave Receiver Function Images of Crustal Imbrication beneath the Cheyenne Belt in Southeast Wyoming

    E-Print Network [OSTI]

    Dueker, Ken

    P- and S-Wave Receiver Function Images of Crustal Imbrication beneath the Cheyenne Belt estimation to constrain the crustal structure across the Archean­Proterozoic Cheyenne belt suture of Proterozoic lower crust across the Chey- enne belt. Both P and S-wave receiver function images delineate

  10. Title: Prompt Creation of New Radiation Belts Cluster: Cross-Theme Theory and Data Analysis/SECTP

    E-Print Network [OSTI]

    Lotko, William

    Title: Prompt Creation of New Radiation Belts Cluster: Cross-Theme Theory and Data Analysis-pushing code for radiation belt particles in a global MHD simulation of the solar wind/SECTP Contributor: William Lotko/Dartmouth College · Radiation belt genesis via shock-induced magnetospheric

  11. CNEEC - Publications

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

    CNEEC archival journal publications CNEEC maintains two lists of publications, one devoted to research solely supported by funding from the CNEEC EFRC and another containing...

  12. Offshore Resource Assessment and Design Conditions Public Meeting...

    Office of Environmental Management (EM)

    Resource Assessment and Design Conditions Public Meeting More Documents & Publications Marine and Hydrokinetic Energy Projects 2014 Water Power Peer Review Report Before the...

  13. MAIN-BELT COMET P/2012 T1 (PANSTARRS)

    SciTech Connect (OSTI)

    Hsieh, Henry H.; Kaluna, Heather M.; Yang Bin; Haghighipour, Nader; Micheli, Marco; Denneau, Larry; Jedicke, Robert; Kleyna, Jan; Veres, Peter; Wainscoat, Richard J.; Ansdell, Megan; Elliott, Garrett T.; Keane, Jacqueline V.; Meech, Karen J.; Riesen, Timm E.; Sonnett, Sarah; Novakovic, Bojan; Fitzsimmons, Alan; Moskovitz, Nicholas A.; Sheppard, Scott S.; and others

    2013-07-01

    We present initial results from observations and numerical analyses aimed at characterizing the main-belt comet P/2012 T1 (PANSTARRS). Optical monitoring observations were made between 2012 October and 2013 February using the University of Hawaii 2.2 m telescope, the Keck I telescope, the Baade and Clay Magellan telescopes, Faulkes Telescope South, the Perkins Telescope at Lowell Observatory, and the Southern Astrophysical Research Telescope. The object's intrinsic brightness approximately doubles from the time of its discovery in early October until mid-November and then decreases by {approx}60% between late December and early February, similar to photometric behavior exhibited by several other main-belt comets and unlike that exhibited by disrupted asteroid (596) Scheila. We also used Keck to conduct spectroscopic searches for CN emission as well as absorption at 0.7 {mu}m that could indicate the presence of hydrated minerals, finding an upper limit CN production rate of Q{sub CN} < 1.5 Multiplication-Sign 10{sup 23} mol s{sup -1}, from which we infer a water production rate of Q{sub H{sub 2O}}<5 Multiplication-Sign 10{sup 25} mol s{sup -1}, and no evidence of the presence of hydrated minerals. Numerical simulations indicate that P/2012 T1 is largely dynamically stable for >100 Myr and is unlikely to be a recently implanted interloper from the outer solar system, while a search for potential asteroid family associations reveals that it is dynamically linked to the {approx}155 Myr old Lixiaohua asteroid family.

  14. RADIATION BELTS AND SUBSTORM PARTICLE INJECTIONS Department of Aerospace Engineering Sciences and LASP, University of Colorado, Boulder, CO 80303-7814, USA

    E-Print Network [OSTI]

    Li, Xinlin

    1 RADIATION BELTS AND SUBSTORM PARTICLE INJECTIONS Xinlin Li Department of Aerospace Engineering belt particles in the Earth's magnetosphere is briefly reviewed, with a focus on the radiation belt energies are presented and the acceleration mecha- nisms for radiation belt electrons are discussed. 1

  15. THE DUST ENVIRONMENT OF MAIN-BELT COMET P/2012 T1 (PANSTARRS)

    SciTech Connect (OSTI)

    Moreno, F.; Pozuelos, F. [Instituto de Astrofisica de Andalucia, CSIC, Glorieta de la Astronomia s/n, E-18008 Granada (Spain); Cabrera-Lavers, A.; Vaduvescu, O.; Licandro, J., E-mail: fernando@iaa.es [Instituto de Astrofisica de Canarias, c/Via Lactea s/n, E-38200 La Laguna, Tenerife (Spain)

    2013-06-20

    The Main-Belt Comet P/2012 T1 (PANSTARRS) has been imaged using the 10.4 m Gran Telescopio Canarias and the 4.2 m William Herschel Telescope at six epochs in the period from 2012 November to 2013 February, with the aim of monitoring its dust environment. The dust tails' brightness and morphology are best interpreted in terms of a model of sustained dust emission spanning four to six months. The total dust mass ejected is estimated at {approx}6-25 Multiplication-Sign 10{sup 6} kg. We assume a time-independent power-law size distribution function, with particles in the micrometer to centimeter size range. Based on the quality of the fits to the isophote fields, an anisotropic emission pattern is favored against an isotropic one, in which the particle ejection is concentrated toward high latitudes ({+-}45 Degree-Sign to {+-}90 Degree-Sign ) in a high-obliquity object (I = 80 Degree-Sign ). This seasonally driven ejection behavior, along with the modeled particle ejection velocities, are in remarkable agreement to those we found for P/2010 R2 (La Sagra).

  16. A long-lived relativistic electron storage ring embedded in Earth's Outer Van Allen belt

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Baker, D. N.; Kanekal, S. G.; Hoxie, V. C.; Henderson, M. G.; Li, X.; Spence, H. E.; Elkington, S. R.; Friedel, R. H. W.; Goldstein, J.; Hudson, M. K.; et al

    2013-02-28

    Since their discovery over 50 years ago, the Earth’s Van Allen radiation belts are thought to consist of two distinct zones of trapped, highly energetic charged particles. The outer zone is comprised predominantly of mega-electron volt (MeV) electrons that wax and wane in intensity on time scales ranging from hours to days depending primarily on external forcing by the solar wind. Thus, the spatially separated inner zone is comprised of commingled high-energy electrons and very energetic positive ions (mostly protons), the latter being stable in intensity levels over years to decades. In situ energy-specific and temporally resolved spacecraft observations revealmore »an isolated third ring, or torus, of high-energy (E > 2 MeV) electrons that formed on 2 September 2012 and persisted largely unchanged in the geocentric radial range of 3.0 to ~3.5 Earth radii for over four weeks before being disrupted (and virtually annihilated) by a powerful interplanetary shock wave passage.« less

  17. Power Electronic Thermal System Performance and Integration ...

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

    May 18-22, 2009 -- Washington D.C. ape13bennion.pdf More Documents & Publications Power Electronic Thermal System Performance and Integration Integrated Power Module...

  18. EA-196-D Minnesota Power | Department of Energy

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

    Minnesota Power Order authorizing Minnesota Power to export electric energy to Canada. EA-196-D Minnesota Power (CN).pdf More Documents & Publications Application to Export...

  19. Superconducting Power Generation

    E-Print Network [OSTI]

    Mario Rabinowitz

    2003-02-20

    The superconducting ac generator has the greatest potential for large-scale commercial application of superconductivity that can benefit the public. Electric power is a vital ingredient of modern society, and generation may be considered to be the vital ingredient of a power system. This articles gives background, and an insight into the physics and engineering of superconducting power generation.

  20. Wind Power

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

    Wind Power Bioenergy Power Systems Wind Power Wind Power Main Page Outreach Programs Image Gallery FAQs Links Software Hydro Power INL Home Wind Power Introduction The Wind Power...

  1. MEASURING THE ABUNDANCE OF SUB-KILOMETER-SIZED KUIPER BELT OBJECTS USING STELLAR OCCULTATIONS

    SciTech Connect (OSTI)

    Schlichting, Hilke E. [Department of Earth and Space Science, UCLA, 595 Charles East Young Drive East, Los Angeles, CA 90095 (United States); Ofek, Eran O.; Gal-Yam, Avishay [Faculty of Physics, Weizmann Institute of Science, P.O. Box 26, Rehovot 76100 (Israel); Sari, Re'em [Racah Institute of Physics, Hebrew University, Jerusalem 91904 (Israel); Nelan, Edmund P.; Livio, Mario [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Wenz, Michael [Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Muirhead, Philip [Department of Astronomy, California Institute of Technology, MC 130-33, Pasadena, CA 91125 (United States); Javanfar, Nikta, E-mail: hilke@ucla.edu [Department of Physics, Physics Engineering and Astronomy, Queen's University, 99 University Avenue, Kingston, Ontario K7L 3N6 (Canada)

    2012-12-20

    We present here the analysis of about 19,500 new star hours of low ecliptic latitude observations (|b| {<=} 20 Degree-Sign ) obtained by the Hubble Space Telescope's Fine Guidance Sensors over a time span of more than nine years, which is in addition to the {approx}12, 000 star hours previously analyzed by Schlichting et al. Our search for stellar occultations by small Kuiper Belt Objects (KBOs) yielded one new candidate event corresponding to a body with a 530 {+-} 70 m radius at a distance of about 40 AU. Using bootstrap simulations, we estimate a probability of Almost-Equal-To 5% that this event is due to random statistical fluctuations within the new data set. Combining this new event with the single KBO occultation reported by Schlichting et al. we arrive at the following results: (1) the ecliptic latitudes of 6. Degree-Sign 6 and 14. Degree-Sign 4 of the two events are consistent with the observed inclination distribution of larger, 100-km-sized KBOs. (2) Assuming that small, sub-kilometer-sized KBOs have the same ecliptic latitude distribution as their larger counterparts, we find an ecliptic surface density of KBOs with radii larger than 250 m of N(r > 250 m) = 1.1{sup +1.5}{sub -0.7} Multiplication-Sign 10{sup 7} deg{sup -2}; if sub-kilometer-sized KBOs have instead a uniform ecliptic latitude distribution for -20 Degree-Sign < b < 20 Degree-Sign then N(r > 250 m) = 4.4{sup +5.8}{sub -2.8} Multiplication-Sign 10{sup 6} deg{sup -2}. This is the best measurement of the surface density of sub-kilometer-sized KBOs to date. (3) Assuming the KBO size distribution can be well described by a single power law given by N(> r){proportional_to}r{sup 1-q}, where N(> r) is the number of KBOs with radii greater than r, and q is the power-law index, we find q = 3.8 {+-} 0.2 and q = 3.6 {+-} 0.2 for a KBO ecliptic latitude distribution that follows the observed distribution for larger, 100-km-sized KBOs and a uniform KBO ecliptic latitude distribution for -20 Degree-Sign < b < 20 Degree-Sign , respectively. (4) Regardless of the exact power law, our results suggest that small KBOs are numerous enough to satisfy the required supply rate for the Jupiter family comets. (5) We can rule out a single power law below the break with q > 4.0 at 2{sigma}, confirming a strong deficit of sub-kilometer-sized KBOs compared to a population extrapolated from objects with r > 45 km. This suggests that small KBOs are undergoing collisional erosion and that the Kuiper Belt is a true analog to the dust producing debris disks observed around other stars.

  2. Structure and evolution of the active fold and thrust belt of southwestern Taiwan using GPS geodesy 

    E-Print Network [OSTI]

    Hickman, John Bibb

    1999-01-01

    Using GPS and published geologic data, we have crographics. investigated the current deformation rates and local kinematic relationships for the southern region of the Taiwan fold-thrust belt. The GPS measurements suggest complex motions across...

  3. Evaluation of the orogenic belt hypothesis for the formation of the Thaumasia Highlands, Mars

    E-Print Network [OSTI]

    , 2002, Borraccini et al., 2007] or continentalscale salt tectonics [Montgomery et al., 2009; Dohm et al., 2001], an orogenic belt produced by an ancient period of plate tectonics or large scale

  4. The Role of Climate in the Deformation of a Fold and Thrust Belt 

    E-Print Network [OSTI]

    Steen, Sean Kristian

    2012-02-14

    Theory and experiment show that the rate and geographic distribution of erosion control the rate and pattern of deformation in collisional mountain belts. Enhanced erosion reduces the mass of material that must be moved up and over ramps...

  5. Migration of matter from the Edgeworth-Kuiper and main asteroid belts to the Earth

    E-Print Network [OSTI]

    S. I. Ipatov

    2002-05-16

    A considerable portion of near-Earth objects could have come from the trans-Neptunian belt. Some of them have aphelia deep inside Jupiter's orbit during more than 1 Myr.

  6. Thrust belt architecture of the central and southern Western Foothills of Taiwan 

    E-Print Network [OSTI]

    Rodriguez-Roa, Fernando Antonio

    2009-05-15

    A structural model of the central and southern Western Foothills Fold and Thrust Belt (WFFTB) was constructed from serial balanced cross sections. The cross sections are constrained by published surface and subsurface geologic data...

  7. Shaping mobile belts by small-scale convection Claudio Faccenna1,2

    E-Print Network [OSTI]

    Becker, Thorsten W.

    ­Dinarides­Hellenides, and further to the east joining the Bitlis­Zagros zone. Most of these fast anomalies are not connected). For example, the collision along the Zagros­Bitlis belt induced the westward motion of Anatolia

  8. The Electric Field and Waves Instruments on the Radiation Belt Storm Probes Mission

    E-Print Network [OSTI]

    Wygant, J. R.

    The Electric Fields and Waves (EFW) Instruments on the two Radiation Belt Storm Probe (RBSP) spacecraft (recently renamed the Van Allen Probes) are designed to measure three dimensional quasi-static and low frequency ...

  9. De-biased populations of Kuiper Belt objects from the Deep Ecliptic Survey

    E-Print Network [OSTI]

    Adams, Elisabeth Rose

    The Deep Ecliptic Survey (DES) was a survey project that discovered hundreds of Kuiper Belt objects from 1998 to 2005. Extensive follow-up observations of these bodies has yielded 304 objects with well-determined orbits ...

  10. Water Ice on the Satellite of Kuiper Belt Object 2003 EL61

    E-Print Network [OSTI]

    K. M Barkume; M. E. Brown; E. L. Schaller

    2006-01-24

    We have obtained a near infrared spectrum of the brightest satellite of the large Kuiper Belt Object, 2003 EL61. The spectrum has absorption features at 1.5 and 2.0 microns, indicating that water ice is present on the surface. We find that the satellite's absorption lines are much deeper than water ice features typically found on Kuiper Belt Objects. We argue that the unusual spectrum indicates that the satellite was likely formed by impact and not by capture.

  11. Mechanical characteristics of folds in Upper Cretaceous strata in the Disturbed Belt of northwestern Montana 

    E-Print Network [OSTI]

    Gilbert, Pat Kader

    1974-01-01

    MECHANICAL CHARACTERISTICS OF FOLDS IN UPPER CRETACEOUS STRATA IN THE DISTURBED BELT OF NORTHWESTERN MONTANA A Thesis by PAT KADER GILBERT Submitted to the Graduate College of Texas A&M University in partial fulfillment of the requirements... for the degree of MASTER OF SCIENCE May 1974 Major Subject: Geology MECHANICAL CHARACTERISTICS OF FOLDS IN UPPER CRETACEOUS STRATA IN THE DISTURBED BELT OF NORTHWESTERN MONTANA A Thesis by PAT KADER GILBERT Approved as to style and content by: (Chairman...

  12. Public Outreach 

    E-Print Network [OSTI]

    Roberts, J.

    2011-01-01

    REGION REGIONAL PUBLIC TRANSPORTATION COORDINATION PLAN PREPARED FOR THE TEXAS DEPARTMENT OF TRANSPORTATION NOVEMBER 2006 REGIONAL PUBLIC TRANSPORTATION COORDINATION PLAN NOVEMBER 2006 PAGE 1 Table of Contents... ....................................................................4 History of Regional Coordination of Public Transportation ..............................10 REGIONAL SERVICE COORDINATION PLANNING........................................................10 Lead Agency...

  13. Biomechanical caracterisation of lumbar belt by full-field techniques: Preliminary results

    E-Print Network [OSTI]

    Bonnaire, Rebecca; Calmels, Paul; Convert, Reynald

    2013-01-01

    In France, 50% of the population per year is suffering from low back pain. Lumbar belt are frequently proposed as a part of the treatment of this pathology. However mechanical ways of working of this medical device is not clearly understood, but abdominal pressure is often related. So an optical method was developed in this study to measure strain in lumbar belt and trunk interface and to derive a pressure estimation. Optical method consisted of coupling fringe projection and digital image correlation (DIC). Measurement has been carried out on the right side of a manikin wearing a lumbar belt. Average strain is 0.2 and average pressure is 1 kPa. Continuation of this study will be comparison of strain and pressure in different areas of lumbar belt (left side, front and back) and comparison of different lumbar belts. Results will be used in a finite elements model to determine lumbar belt impact in intern body. In long term, this kind of study will be done on human.

  14. Power the world's powers the world's economy.

    E-Print Network [OSTI]

    Power the world's economy BUSINESS #12;powers the world's economy. Put yourself in the driver. · A buyer, merchandiser, planner or manager in a retail operation. · The manager of a restaurant or food materials firm. · A marketer promoting a business, nonprofit organization or public agency. · A small

  15. Wind Power Today, 2010, Wind and Water Power Program (WWPP)

    SciTech Connect (OSTI)

    Not Available

    2010-05-01

    Wind Power Today is an annual publication that provides an overview of the wind energy research conducted by the U.S. Department of Energy Wind and Water Power Program.

  16. Volatile Loss and Classification of Kuiper Belt Objects

    E-Print Network [OSTI]

    Johnson, R E; Young, L A; Volkov, A N; Schmidt, C

    2015-01-01

    Observations indicate that some of the largest Kuiper Belt Objects (KBOs) have retained volatiles in the gas phase, which implies the presence of an atmosphere that can affect their reflectance spectra and thermal balance. Volatile escape rates driven by solar heating of the surface were estimated by Schaller and Brown (2007) (SB) and Levi and Podolak (2009)(LP) using Jeans escape from the surface and a hydrodynamic model respectively. Based on recent molecular kinetic simulations these rates can be hugely in error (e.g., a factor of $\\sim 10^{16}$ for the SB estimate for Pluto). In this paper we estimate the loss of primordial N$_2$ for several large KBOs guided by recent molecular kinetic simulations of escape due to solar heating of the surface and due to UV/EUV heating of the upper atmosphere. For the latter we extrapolate simulations of escape from Pluto (Erwin et al. 2013) using the energy limited escape model recently validated for the KBOs of interest by molecular kinetic simulations (Johnson et al. 2...

  17. Planar resonant periodic orbits in Kuiper belt dynamics

    E-Print Network [OSTI]

    George Voyatzis; Thomas Kotoulas

    2005-02-28

    In the framework of the planar restricted three body problem we study a considerable number of resonances associated to the Kuiper Belt dynamics and located between 30 and 48 a.u. Our study is based on the computation of resonant periodic orbits and their stability. Stable periodic orbits are surrounded by regular librations in phase space and in such domains the capture of trans-Neptunian object is possible. All the periodic orbits found are symmetric and there is evidence for the existence of asymmetric ones only in few cases. In the present work first, second and third order resonances are under consideration. In the planar circular case we found that most of the periodic orbits are stable. The families of periodic orbits are temporarily interrupted by collisions but they continue up to relatively large values of the Jacobi constant and highly eccentric regular motion exists for all cases. In the elliptic problem and for a particular eccentricity value of the primary bodies the periodic orbits are isolated. The corresponding families, where they belong to, bifurcate from specific periodic orbits of the circular problem and seem to continue up to the rectilinear problem. Both stable and unstable orbits are obtained for each case. In the elliptic problem the unstable orbits found are associated with narrow chaotic domains in phase space. The evolution of the orbits, which are located in such chaotic domains, seems to be practically regular and bounded for long time intervals.

  18. First results from the Herschel Gould Belt Survey in Taurus

    E-Print Network [OSTI]

    Kirk, J M; Palmeirim, P; Andre, Ph; Griffin, M J; Hargrave, P J; Konyves, V; Bernard, J P; Nutter, D J; Sibthorpe, B; Di Francesco, J; Abergel, A; Arzoumanian, D; Benedettini, M; Bontemps, S; Elia, D; Hennemann, M; Hill, T; Men'shchikov, A; Motte, F; Nguyen-Luong, Q; Peretto, N; Pezzuto, S; Rygl, K L J; Sadavoy, S I; Schisano, E; Schneider, N; Testi, L; White, G

    2013-01-01

    The whole of the Taurus region (a total area of 52 sq. deg.) has been observed by the Herschel SPIRE and PACS instruments at wavelengths of 70, 160, 250, 350 and 500 {\\mu}m as part of the Herschel Gould Belt Survey. In this paper we present the first results from the part of the Taurus region that includes the Barnard 18 and L1536 clouds. A new source-finding routine, the Cardiff Source-finding AlgoRithm (CSAR), is introduced, which is loosely based on CLUMPFIND, but that also generates a structure tree, or dendrogram, which can be used to interpret hierarchical clump structure in a complex region. Sources were extracted from the data using the hierarchical version of CSAR and plotted on a mass-size diagram. We found a hierarchy of objects with sizes in the range 0.024-2.7 pc. Previous studies showed that gravitationally bound prestellar cores and unbound starless clumps appeared in different places on the mass-size diagram. However, it was unclear whether this was due to a lack of instrumental dynamic range ...

  19. Initial highlights from the Herschel Gould Belt survey

    E-Print Network [OSTI]

    André, Ph; Bontemps, S; Könyves, V; Motte, F; Schneider, N; Didelon, P; Minier, V; Saraceno, P; Ward-Thompson, D; Di Francesco, J; White, G; Molinari, S; Testi, L; Abergel, A; Griffin, M; Henning, Th; Royer, P; Merín, B; Vavrek, R; Attard, M; Arzoumanian, D; Wilson, C D; Ade, P; Aussel, H; Baluteau, J -P; Benedettini, M; Bernard, J -Ph; Blommaert, J A D L; Cambrésy, L; Cox, P; Di Giorgio, A; Hargrave, P; Hennemann, M; Huang, M; Kirk, J; Krause, O; Launhardt, R; Leeks, S; Pennec, J Le; Li, J Z; Martin, P; Maury, A; Olofsson, G; Omont, A; Peretto, N; Pezzuto, S; Prusti, T; Roussel, H; Russeil, D; Sauvage, M; Sibthorpe, B; Sicilia-Aguilar, A; Spinoglio, L; Waelkens, C; Woodcraft, A; Zavagno, A

    2010-01-01

    We summarize the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the 'science demonstration phase' of Herschel. Our 70-500 micron images taken in parallel mode with the SPIRE and PACS cameras reveal a wealth of filamentary structure, as well as numerous dense cores embedded in the filaments. Between ~ 350 and 500 prestellar cores and ~ 45-60 Class 0 protostars can be identified in the Aquila field, while ~ unbound starless cores and no protostars are observed in the Polaris field. The prestellar core mass function (CMF) derived for the Aquila region bears a strong resemblance to the stellar initial mass function (IMF), already confirming the close connection between the CMF and the IMF with much better statistics than earlier studies. Comparing and contrasting our Herschel results in Aquila and Polaris, we propose an observationally-driven scenario for core formation according to which complex networks of long, thin filaments form first within molecul...

  20. The Gould Belt 'MISFITS' Survey: The Real Solar Neighborhood Protostars

    E-Print Network [OSTI]

    Heiderman, Amanda

    2015-01-01

    We present an HCO$^{+}$ J=3-2 survey of Class 0+I and Flat SED young stellar objects (YSOs) found in the Gould Belt clouds by surveys with Spitzer. Our goal is to provide a uniform Stage 0+I source indicator for these embedded protostar candidates. We made single point HCO$^{+}$ J = 3-2 measurements toward the source positions at the CSO and APEX of 546 YSOs (89% of the Class 0+I + Flat SED sample). Using the criteria from van Kempen et al. (2009), we classify sources as Stage 0+I or bona fide protostars and find that 84% of detected sources meet the criteria. We recommend a timescale for the evolution of Stage 0+I (embedded protostars) of 0.54 Myr. We find significant correlations of HCO$^{+}$ integrated intensity with ${\\alpha}$ and $T_{bol}$ but not with $L_{bol}$. The detection fraction increases smoothly as a function of ${\\alpha}$ and $L_{bol}$, while decreasing smoothly with $T_{bol}$. Using the Stage 0+I sources tightens the relation between protostars and high extinction regions of the cloud; 89% of ...

  1. Kuiper belt structure around nearby super-Earth host stars

    E-Print Network [OSTI]

    Kennedy, Grant M; Marmier, Maxime; Greaves, Jane S; Wyatt, Mark C; Bryden, Geoffrey; Holland, Wayne; Lovis, Christophe; Matthews, Brenda C; Pepe, Francesco; Sibthorpe, Bruce; Udry, Stéphane

    2015-01-01

    We present new observations of the Kuiper belt analogues around HD 38858 and HD 20794, hosts of super-Earth mass planets within 1 au. As two of the four nearby G-type stars (with HD 69830 and 61 Vir) that form the basis of a possible correlation between low-mass planets and debris disc brightness, these systems are of particular interest. The disc around HD 38858 is well resolved with Herschel and we constrain the disc geometry and radial structure. We also present a probable JCMT sub-mm continuum detection of the disc and a CO J=2-1 upper limit. The disc around HD 20794 is much fainter and appears marginally resolved with Herschel, and is constrained to be less extended than the discs around 61 Vir and HD 38858. We also set limits on the radial location of hot dust recently detected around HD 20794 with near-IR interferometry. We present HARPS upper limits on unseen planets in these four systems, ruling out additional super-Earths within a few au, and Saturn-mass planets within 10 au. We consider the disc st...

  2. MAIN-BELT COMET 238P/READ REVISITED

    SciTech Connect (OSTI)

    Hsieh, Henry H.; Meech, Karen J.; Pittichova, Jana, E-mail: hsieh@ifa.hawaii.edu, E-mail: meech@ifa.hawaii.edu, E-mail: jana@ifa.hawaii.edu [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

    2011-07-20

    We present a series of observations of the return of activity in main-belt comet (MBC) 238P/Read. Using data obtained in 2010 July and August when 238P appeared to be largely inactive, we find best-fit IAU phase function parameters of H = 19.05 {+-} 0.05 mag, corresponding to a nucleus radius of r{sub n} {approx} 0.4 km (assuming an albedo of p{sub R} = 0.05), and G = -0.03 {+-} 0.05. Observations from 2010 September onward show a clear rise in activity, causing both a notable change in visible morphology and increasing photometric excesses beyond what would be expected based on bare nucleus observations. By the end of the observing period reported on here, the dust mass in the coma shows indications of reaching a level comparable to that observed in 2005, but further observations are highly encouraged once 238P again becomes observable from Earth in mid-2011 to confirm whether this level of activity is achieved, or if the comet shows a noticeable drop in activity strength compared with 2005. Comet 238P is now the second MBC (after 133P/Elst-Pizarro) observed to exhibit recurrent activity, providing strong corroboration for the conclusion that it is a true comet whose active episodes are driven by sublimation of volatile ice.

  3. Grenville foreland thrust belt hidden beneath the eastern US midcontinent

    SciTech Connect (OSTI)

    Hauser, E.C. (Cornell Univ., Ithaca, NY (United States))

    1993-01-01

    Grenville foreland thrust structures are observed beneath the eastern US midcontinent on COCORP (Consortium for Continental Reflection Profiling) line OH-1 and a short seismic line in southwest Ohio. These structures represent the first evidence for a significant Grenville foreland thrust belt preserved in eastern North America. On the COCORP lines, the structures include a thrust ramp anticline and an associated asymmetric syncline. The Grenville front tectonic zone appears to truncate these foreland structures, indicating a later, second phase expressed as a deeply penetrating, out-of-sequence thrust zone associated with the main uplift of the Grenville province on the east. A short, shallow seismic line in southwestern Ohio reveals an east-dipping sequence of prominently layered rocks that may lie above a footwall ramp to a deeper Grenville thrust fault. A drill hole into the less reflective top of this dipping sequence encountered unmetamorphosed sedimentary rocks like those increasingly reported from other drill holes in southwestern Ohio and adjacent states. Although possibly part of a late Precambrian (Keweenawan ) rift, these clastic sedimentary rocks may instead preserve evidence of a heretofore unrecognized Grenville foreland basin in eastern North America. Alternatively these Precambrian sedimentary rocks together with an underlying, but yet undrilled, strongly layered sequence may correlate with similarly layered rocks observed on COCORP and industrial seismic lines within the Middle Proterozoic granite-rhyolite province to the west in Indiana and Illinois and indicate that unmetamorphosed sedimentary material is an important constituent of the granite-rhyolite province. 25 refs., 6 figs.

  4. Dynamical implantation of objects in the Kuiper Belt

    SciTech Connect (OSTI)

    Brasil, P. I. O.

    2014-09-01

    Several models have been suggested in the past to describe the dynamical formation of hot Kuiper Belt objects (hereafter Hot Classicals or HCs for short). Here, we discuss a dynamical mechanism that allows orbits to evolve from the primordial planetesimal disk at ? 35 AU to reach the orbital region now occupied by HCs. We performed three different sets of numerical simulations to illustrate this mechanism. Two of these simulations were based on modern theories for the early evolution of the solar system (the Nice and jumping-Jupiter models). The third simulation was performed with the purpose of increasing the resolution at 41-46 AU. The common aspect of these simulations is that Neptune scatters planetesimals from ? 35 AU to >40 AU and then undergoes a long phase of slow residual migration. Our results show that to reach an HC orbit, a scattered planetesimal needs to be captured in a mean motion resonance (MMR) with Neptune where the perihelion distance rises due to the Kozai resonance (which occurs in MMRs even for moderate inclinations). Finally, while Neptune is still migrating, the planetesimal is released from the MMR on a stable HC orbit. We show that the orbital distribution of HCs expected from this process provides a reasonable match to observations. The capture efficiency and the mass deposited into the HC region appears to be sensitive to the maximum eccentricity reached by Neptune during the planetary instability phase. Additional work will be needed to resolve this dependency in detail.

  5. Power Plant Power Plant

    E-Print Network [OSTI]

    Stillwater Power Plant Wabuska Power Plant Casa Diablo Power Plant Glass Mountain Geothermal Area Lassen Geothermal Area Coso Hot Springs Power Plants Lake City Geothermal Area Thermo Geothermal Area Lakeview Geothermal Area Raft River Geothermal Area Cove Fort Power Plant Roosevelt Power Plant Borax Lake

  6. Wind Power Today

    SciTech Connect (OSTI)

    Not Available

    2006-05-01

    Wind Power Today is an annual publication that provides an overview of the wind energy research conducted by the U.S. Department of Energy Wind and Hydropower Technologies Program.

  7. The Insignificance of P-R Drag in Detectable Extrasolar Planetesimal Belts

    E-Print Network [OSTI]

    M. C. Wyatt

    2005-01-04

    This paper considers a simple model in which dust produced in a planetesimal belt migrates in toward the star due to P-R drag suffering destructive collisions with other dust grains on the way. Assuming the dust is all of the same size, the resulting surface density distribution can be derived analytically and depends only on the parameter eta0=5000tau*sqrt(Mstar/r)/beta; this parameter can be determined observationally with the hypothesis that beta=0.5. For massive belts in which eta0>>1 dust is confined to the planetesimal belt, while the surface density of more tenuous belts, in which eta0belts at different distances from different mass stars shows that the dust belts which have been detected to date should have eta0>>1; dust belts with eta010. This means that these disks are so massive that mutual collisions prevent dust from reaching the inner regions of these systems and P-R drag can be ignored when studying their dynamics. Models for the formation of structure in debris disks by the trapping of particles into planetary resonances by P-R drag should be reconsidered. However, since collisions do not halt 100% of the dust, this means that in the absence of planetary companions debris disk systems should be populated by small quantities of hot dust which may be detectable in the mid-IR. Even in disks with eta0<<1 the temperature of dust emission is shown to be a reliable tracer of the planetesimal distribution meaning that inner holes in the dust distribution imply a lack of colliding planetesimals in the inner regions.

  8. Publication Policy

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

    of experiments performed at the Facility. Vehicles for the publication may include: Journal articles Conference proceedings articles Books or book chapters Technical reports...

  9. ORBITS, MASSES, AND EVOLUTION OF MAIN BELT TRIPLE (87) SYLVIA

    SciTech Connect (OSTI)

    Fang, Julia; Margot, Jean-Luc [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Rojo, Patricio [Departamento de Astronomia, Universidad de Chile, Santiago (Chile)

    2012-08-15

    Sylvia is a triple asteroid system located in the main belt. We report new adaptive optics observations of this system that extend the baseline of existing astrometric observations to a decade. We present the first fully dynamical three-body model for this system by fitting to all available astrometric measurements. This model simultaneously fits for individual masses, orbits, and primary oblateness. We find that Sylvia is composed of a dominant central mass surrounded by two satellites orbiting at 706.5 {+-} 2.5 km and 1357 {+-} 4.0 km, i.e., about 5 and nearly 10 primary radii. We derive individual masses of 1.484{sup +0.016}{sub -0.014} Multiplication-Sign 10{sup 19} kg for the primary (corresponding to a density of 1.29 {+-} 0.39 g cm{sup -3}), 7.33{sup +4.7}{sub -2.3} Multiplication-Sign 10{sup 14} kg for the inner satellite, and 9.32{sup +20.7}{sub -8.3} Multiplication-Sign 10{sup 14} kg for the outer satellite. The oblateness of the primary induces substantial precession and the J{sub 2} value can be constrained to the range of 0.0985-0.1. The orbits of the satellites are relatively circular with eccentricities less than 0.04. The spin axis of the primary body and the orbital poles of both satellites are all aligned within about 2 deg of each other, indicating a nearly coplanar configuration and suggestive of satellite formation in or near the equatorial plane of the primary. We also investigate the past orbital evolution of the system by simulating the effects of a recent passage through 3:1 mean-motion eccentricity-type resonances. In some scenarios this allow us to place constraints on interior structure and past eccentricities.

  10. Hubble space telescope investigation of main-belt comet 133P/Elst-Pizarro

    SciTech Connect (OSTI)

    Jewitt, David; Ishiguro, Masateru; Weaver, Harold; Agarwal, Jessica; Mutchler, Max; Larson, Steven

    2014-05-01

    We report new observations of the prototype main-belt comet (active asteroid) 133P/Elst-Pizarro taken at high angular resolution using the Hubble Space Telescope. The object has three main components: (1) a point-like nucleus; (2) a long, narrow antisolar dust tail; and (3) a short, sunward anti-tail. There is no resolved coma. The nucleus has a mean absolute magnitude H{sub V} = 15.70 ± 0.10 and a light curve range ?V = 0.42 mag, the latter corresponding to projected dimensions 3.6 × 5.4 km (axis ratio 1.5:1) at the previously measured geometric albedo of 0.05 ± 0.02. We explored a range of continuous and impulsive emission models to simultaneously fit the measured surface brightness profile, width, and position angle of the antisolar tail. Preferred fits invoke protracted emission, over a period of 150 days or less, of dust grains following a differential power-law size distribution with index 3.25 ?q ? 3.5 and with a wide range of sizes. Ultra-low surface brightness dust projected in the sunward direction is a remnant from emission activity occurring in previous orbits, and consists of the largest (?cm-sized) particles. Ejection velocities of one-micron-sized particles are comparable to the ?1.8 m s{sup –1} gravitational escape speed of the nucleus, while larger particles are released at speeds less than the gravitational escape velocity. The observations are consistent with, but do not prove, a hybrid hypothesis in which mass loss is driven by gas drag from the sublimation of near-surface water ice, but escape is aided by centripetal acceleration from the rotation of the elongated nucleus. No plausible alternative hypothesis has been identified.

  11. Bio PowerBio Power The City of Gresham WastewaterThe City of Gresham Wastewater

    E-Print Network [OSTI]

    Prevedouros, Panos D.

    power=small scale turbinehydro power=small scale turbineMicroMicro--hydro power=small scale turbinehydro Power Micro-Hydro Power #12;Awards League of Oregon Cities 2006 Award of Excellence American PublicBio PowerBio Power The City of Gresham WastewaterThe City of Gresham Wastewater Treatment Plant

  12. THE SURFACE COMPOSITION OF LARGE KUIPER BELT OBJECT 2007 OR10

    SciTech Connect (OSTI)

    Brown, M. E.; Fraser, W. C. [Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 (United States); Burgasser, A. J., E-mail: aburgasser@ucsd.edu [Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093 (United States)

    2011-09-10

    We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice. While most objects in the Kuiper belt with water ice absorption this prominent have the optically neutral colors of water ice, 2007 OR10 is among the reddest Kuiper belt objects known. One other large Kuiper belt object-Quaoar-has similar red coloring and water ice absorption, and it is hypothesized that the red coloration of this object is due to irradiation of the small amounts of methane able to be retained on Quaoar. 2007 OR10, though warmer than Quaoar, is in a similar volatile retention regime because it is sufficiently larger that its stronger gravity can still retain methane. We propose, therefore, that the red coloration on 2007 OR10 is also caused by the retention of small amounts of methane. Positive detection of methane on 2007 OR10 will require spectra with higher signal to noise. Models for volatile retention on Kuiper belt objects appear to continue to do an excellent job reproducing all of the available observations.

  13. MAIN BELT ASTEROIDS WITH WISE/NEOWISE. I. PRELIMINARY ALBEDOS AND DIAMETERS

    SciTech Connect (OSTI)

    Masiero, Joseph R.; Mainzer, A. K.; Bauer, J. M.; Eisenhardt, P. R. M.; DeBaun, E.; Elsbury, D.; Gautier, T. IV; Gomillion, S.; Wilkins, A. [Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA 91109 (United States); Grav, T. IV [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Cutri, R. M.; Dailey, J. [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); McMillan, R. S. [Lunar and Planetary Laboratory, University of Arizona, Kuiper Space Science Building 92, Tucson, AZ 85721-0092 (United States); Spahr, T. B. [Minor Planet Center, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Skrutskie, M. F. [Department of Astronomy, University of Virginia, Charlottesville, VA 22903-0818 (United States); Tholen, D. [Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States); Walker, R. G. [Monterey Institute for Research in Astronomy, Monterey, CA (United States); Wright, E. L., E-mail: Joseph.Masiero@jpl.nasa.gov [UCLA Astronomy, Los Angeles, CA 90095-1547 (United States)

    2011-11-10

    We present initial results from the Wide-field Infrared Survey Explorer (WISE), a four-band all-sky thermal infrared survey that produces data well suited for measuring the physical properties of asteroids, and the NEOWISE enhancement to the WISE mission allowing for detailed study of solar system objects. Using a NEATM thermal model fitting routine, we compute diameters for over 100,000 Main Belt asteroids from their IR thermal flux, with errors better than 10%. We then incorporate literature values of visible measurements (in the form of the H absolute magnitude) to determine albedos. Using these data we investigate the albedo and diameter distributions of the Main Belt. As observed previously, we find a change in the average albedo when comparing the inner, middle, and outer portions of the Main Belt. We also confirm that the albedo distribution of each region is strongly bimodal. We observe groupings of objects with similar albedos in regions of the Main Belt associated with dynamical breakup families. Asteroid families typically show a characteristic albedo for all members, but there are notable exceptions to this. This paper is the first look at the Main Belt asteroids in the WISE data, and only represents the preliminary, observed raw size, and albedo distributions for the populations considered. These distributions are subject to survey biases inherent to the NEOWISE data set and cannot yet be interpreted as describing the true populations; the debiased size and albedo distributions will be the subject of the next paper in this series.

  14. Background & Publications

    E-Print Network [OSTI]

    Home Background & Projects Calendar Publications Staff Directory Station Videos Links Search to pit. Harvest is expected to continue through this week. Balaton fruit set is light, and harvest abandon some sweet cherry blocks. Brown MAES Home | Field Stations | Station Home | Publications | Fruit

  15. Background & Publications

    E-Print Network [OSTI]

    Home Background & Projects Calendar Publications Staff Directory Station Videos Links Search Home | Field Stations | Station Home | Publications | FruitNet Weekly Report GROWING DEGREE DAY is still relatively light, probably due to few wetting periods during early shoot growth. Sun scald

  16. NUCLEAR POWER in CALIFORNIA

    E-Print Network [OSTI]

    NUCLEAR POWER in CALIFORNIA: 2007 STATUS REPORT CALIFORNIA ENERGY COMMISSION October 2007 CEC-100 public workshops on nuclear power. The Integrated Energy Policy Report Committee, led by Commissioners, California Contract No. 700-05-002 Prepared For: California Energy Commission Barbara Byron, Senior Nuclear

  17. Using Intermediate-Luminosity Optical Transients (ILOTs) to reveal extended exo-solar Kuiper belt objects

    E-Print Network [OSTI]

    Bear, Ealeal

    2016-01-01

    We suggest that in the rare case of an Intermediate-Luminosity Optical Transient (ILOTs) event, evaporation of exo-solar Kuiper belt objects (ExoKBOs) at distances of d~500 - 10000AU from the ILOT can be detected. If the ILOT lasts for 1 month to a few years, enough dust might be ejected from the ExoKBOs for the IR emission to be detected. Because of the large distance of the ExoKBOs, tens of years will pass before the ILOT wind disperses the dust. We suggest that after an ILOT outburst there is a period of months to several years during which IR excess emission might hint at the existence of a Kuiper belt analog (ExoK-Belt).

  18. A RESOLVED MILLIMETER EMISSION BELT IN THE AU Mic DEBRIS DISK

    SciTech Connect (OSTI)

    Wilner, David J.; Andrews, Sean M.; MacGregor, Meredith A. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Meredith Hughes, A. [Department of Astronomy, 601 Campbell Hall, University of California, Berkeley, CA 94720 (United States)

    2012-04-20

    We present imaging observations at 1.3 mm of the debris disk surrounding the nearby M-type flare star AU Mic with beam size 3'' (30 AU) from the Submillimeter Array. These data reveal a belt of thermal dust emission surrounding the star with the same edge-on geometry as the more extended scattered light disk detected at optical wavelengths. Simple modeling indicates a central radius of {approx}35 AU for the emission belt. This location is consistent with the reservoir of planetesimals previously invoked to explain the shape of the scattered light surface brightness profile through size-dependent dust dynamics. The identification of this belt further strengthens the kinship between the debris disks around AU Mic and its more massive sister star {beta} Pic, members of the same {approx}10 Myr old moving group.

  19. Growth of asteroids, planetary embryos and Kuiper belt objects by chondrule accretion

    E-Print Network [OSTI]

    Johansen, Anders; Lacerda, Pedro; Bizzarro, Martin

    2015-01-01

    Chondrules are millimeter-sized spherules that dominate primitive meteorites (chondrites) originating from the asteroid belt. The incorporation of chondrules into asteroidal bodies must be an important step in planet formation, but the mechanism is not understood. We show that the main growth of asteroids can result from gas-drag-assisted accretion of chondrules. The largest planetesimals of a population with a characteristic radius of 100 km undergo run-away accretion of chondrules within ~3 Myr, forming planetary embryos up to Mars sizes along with smaller asteroids whose size distribution matches that of main belt asteroids. The aerodynamical accretion leads to size-sorting of chondrules consistent with chondrites. Accretion of mm-sized chondrules and ice particles drives the growth of planetesimals beyond the ice line as well, but the growth time increases above the disk life time outside of 25 AU. The contribution of direct planetesimal accretion to the growth of both asteroids and Kuiper belt objects is...

  20. KUIPER BELT OBJECT OCCULTATIONS: EXPECTED RATES, FALSE POSITIVES, AND SURVEY DESIGN

    SciTech Connect (OSTI)

    Bickerton, S. J. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); Welch, D. L. [Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1 (Canada); Kavelaars, J. J. [Herzberg Institute of Astrophysics, Victoria, BC V9E 2E7 (Canada)], E-mail: bick@astro.princeton.edu, E-mail: welch@physics.mcmaster.ca, E-mail: JJ.Kavelaars@nrc-cnrc.gc.ca

    2009-05-15

    A novel method of generating artificial scintillation noise is developed and used to evaluate occultation rates and false positive rates for surveys probing the Kuiper Belt with the method of serendipitous stellar occultations. A thorough examination of survey design shows that (1) diffraction-dominated occultations are critically (Nyquist) sampled at a rate of 2 Fsu{sup -1}, corresponding to 40 s{sup -1} for objects at 40 AU, (2) occultation detection rates are maximized when targets are observed at solar opposition, (3) Main Belt asteroids will produce occultations light curves identical to those of Kuiper Belt Objects (KBOs) if target stars are observed at solar elongations of: 116{sup 0} {approx}< {epsilon} {approx}< 125 deg., or 131 deg. {approx}< {epsilon} {approx}< 141 deg., and (4) genuine KBO occultations are likely to be so rare that a detection threshold of {approx}>7-8{sigma} should be adopted to ensure that viable candidate events can be disentangled from false positives.

  1. STIS CORONAGRAPHIC IMAGING OF FOMALHAUT: MAIN BELT STRUCTURE AND THE ORBIT OF FOMALHAUT b

    SciTech Connect (OSTI)

    Kalas, Paul; Graham, James R. [Astronomy Department, University of California, Berkeley, CA 94720 (United States); Fitzgerald, Michael P. [Department of Physics and Astronomy, UCLA, Los Angeles, CA (United States); Clampin, Mark [NASA Goddard Space Flight Center, Greenbelt, MD (United States)

    2013-09-20

    We present new optical coronagraphic data of Fomalhaut obtained with HST/STIS in 2010 and 2012. Fomalhaut b is recovered at both epochs to high significance. The observations include the discoveries of tenuous nebulosity beyond the main dust belt detected to at least 209 AU projected radius, and a ?50 AU wide azimuthal gap in the belt northward of Fomalhaut b. The two epochs of Space Telescope Imaging Spectrograph (STIS) photometry exclude optical variability greater than 35%. A Markov chain Monte Carlo analysis demonstrates that the orbit of Fomalhaut b is highly eccentric, with e = 0.8 ± 0.1, a = 177 ± 68 AU, and q = 32 ± 24 AU. Fomalhaut b is apsidally aligned with the belt and 90% of allowed orbits have mutual inclination ?36°. Fomalhaut b's orbit is belt crossing in the sky plane projection, but only 12% of possible orbits have ascending or descending nodes within a 25 AU wide belt annulus. The high eccentricity invokes a dynamical history where Fomalhaut b may have experienced a significant dynamical interaction with a hypothetical planet Fomalhaut c, and the current orbital configuration may be relatively short-lived. The Tisserand parameter with respect to a hypothetical Fomalhaut planet at 30 AU or 120 AU lies in the range 2-3, similar to highly eccentric dwarf planets in our solar system. We argue that Fomalhaut b's minimum mass is that of a dwarf planet in order for a circumplanetary satellite system to remain bound to a sufficient radius from the planet to be consistent with the dust scattered light hypothesis. In the coplanar case, Fomalhaut b will collide with the main belt around 2032, and the subsequent emergent phenomena may help determine its physical nature.

  2. Louisiana Tech University Six Sigma Green Belt Certification A Louisiana Tech University Six Sigma Greenbelt certification can be obtained by

    E-Print Network [OSTI]

    Selmic, Sandra

    Louisiana Tech University Six Sigma Green Belt Certification A Louisiana Tech University Six Sigma Sigma and ENGR 566 Six Sigma and Quality Control with a B or higher. The cost to take the two required courses is $1,180 per course for a total of $2,360 to complete the Six Sigma Green Belt certification

  3. Radio-Loud and Radio-Quiet Gamma-Ray Pulsars from the Galactic Plane and the Gould Belt

    SciTech Connect (OSTI)

    Gonthier, P. L.

    2005-03-17

    We present recent results of a pulsar population synthesis study in the polar cap model that includes the Parkes Multibeam Pulsar Survey, realistic beam geometries for radio and {gamma}-ray emission from neutron stars born in the Galactic disc as well as the local Gould Belt. We include nine radio surveys to normalize the simulated results from the Galactic disc to the number of radio pulsars observed by the group of selected surveys. In normalizing the contribution of the Gould Belt, we use results from a recent study that indicates a supernova rate in the Gould Belt of 3 to 5 times that of the local region of the Galactic plane leading to {approx}100 neutron stars born in the Gould Belt during the last 5 Myr. Our simulations include the dynamical evolution of the Gould Belt where neutron stars are produced in the plane of the Gould Belt during the past 5 Myr. We discuss the simulated numbers of radio-quiet (those below flux threshold of radio surveys) and radio-loud, {gamma}-ray pulsars from the Galactic disc and the Gould belt observed by {gamma}-ray telescopes EGRET, AGILE and GLAST. They suggest that about 35 of the unidentified EGRET sources could be (mostly radio-loud) {gamma}-ray pulsars with 2/3 of them born in the Galactic disc and 1/3 in the Gould Belt.

  4. Steady-State Impurity Control, Heat Removal and Tritium Recovery by Moving-Belt Plasma-Facing Components

    E-Print Network [OSTI]

    Tillack, Mark

    1 Steady-State Impurity Control, Heat Removal and Tritium Recovery by Moving-Belt Plasma-Z getter materials, heat removal and tritium recovery. In order to minimize MHD effects as well as induced is the application of "Moving-Belt Plasma-Facing Components" for steady-state impurity gettering, heat removal

  5. The Evidence for Slow Migration of Neptune from the Inclination Distribution of Kuiper Belt Objects

    E-Print Network [OSTI]

    Nesvorny, David

    2015-01-01

    Much of the dynamical structure of the Kuiper belt can be explained if Neptune migrated over several AU, and/or if Neptune was scattered to an eccentric orbit during planetary instability. An outstanding problem with the existing formation models is that the distribution of orbital inclinations they predicted is narrower than the one inferred from observations. Here we perform numerical simulations of Kuiper belt formation starting from an initial state with Neptune at 20 = 10 Myr and a_{N,0} 40 AU region, where the Cold Classicals presumably formed.

  6. MILLIMETER IMAGING OF THE {beta} PICTORIS DEBRIS DISK: EVIDENCE FOR A PLANETESIMAL BELT

    SciTech Connect (OSTI)

    Wilner, David J.; Andrews, Sean M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Hughes, A. Meredith [Department of Astronomy, 601 Campbell Hall, University of California, Berkeley, CA 94720 (United States)

    2011-02-01

    We present observations at 1.3 mm wavelength of the {beta} Pictoris debris disk with beam size 4.''3 x 2.''6 (83 x 50 AU) from the Submillimeter Array. The emission shows two peaks separated by {approx}7'' along the disk plane, which we interpret as a highly inclined dust ring or belt. A simple model constrains the belt center to 94 {+-} 8 AU, close to the prominent break in slope of the optical scattered light. We identify this region as the location of the main reservoir of dust-producing planetesimals in the disk.

  7. Geology of a portion of the northern Kings Mountain belt, North Carolina 

    E-Print Network [OSTI]

    Michie, Joanna

    1985-01-01

    GEOLOGY OF A PORTrON OP THE NORTHERN RINGS YOUNTAIN BELT NO&TH CAROLINA A Thesis by JOANNA NICHIF Submitted to the Graduate College of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Hay... lep5 Yaior Subiect: Geology GEOLOGY OF A PORTION OF THE NORTHERN KINGS MOUNTAIN BELT, NORTH CAROLINA A Thesis by JOANNA MICHIE Approved as to style and content by: David W. Mohr (Chairman of Committee) J. Robert Butler (Member) John H. pang...

  8. Electric power annual 1993

    SciTech Connect (OSTI)

    Not Available

    1994-12-08

    This report presents a summary of electric power industry statistics at national, regional, and state levels: generating capability and additions, net generation, fossil-fuel statistics, retail sales and revenue, finanical statistics, environmental statistics, power transactions, demand side management, nonutility power producers. Purpose is to provide industry decisionmakers, government policymakers, analysts, and the public with historical data that may be used in understanding US electricity markets.

  9. REVISED DRAFT OF ACCEPTED PAPER FOR ASME JOURNAL OF MECHANICAL DESIGN 1 Power Efficiency of the Rotational-to-Linear

    E-Print Network [OSTI]

    Amaral, Luis A.N.

    REVISED DRAFT OF ACCEPTED PAPER FOR ASME JOURNAL OF MECHANICAL DESIGN 1 Power Efficiency their efficiency to fixed ratio gear-trains. We also compare the overall power efficiency of the cobotic transmission architecture that can have minimal dis- sipation and trivial dynamics. Gear trains, timing belt

  10. EA-213-A Coral Power, LLC | Department of Energy

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

    Coral Power, LLC Order authorizing Coral Power, LLC to export electric energy to Canada. EA-213-A Coral Power, LLC More Documents & Publications EA-212-C Coral Power, LLC...

  11. GEOPHYSICAL RESEARCH LETTERS, VOL. 0, NO. 0, PAGES 0-0, M 0, 2001 Long Term Measurements of Radiation Belts by

    E-Print Network [OSTI]

    Li, Xinlin

    of Radiation Belts by SAMPEX and Their Variations Xinlin Li,1 D. N. Baker,1 S. G. Kanekal,1 M. Looper,2 M-altitude and polar- orbiting satellite, has provided a long-term global picture of the radiation belts since its launch on July 3, 1992. While the inner belt (L

  12. The Antarctic Circumpolar Productivity Belt Joint Institute for the Study of the Atmosphere and Ocean, University of Washington, Seattle, Washington, USA

    E-Print Network [OSTI]

    Follows, Mick

    The Antarctic Circumpolar Productivity Belt T. Ito Joint Institute for the Study of the Atmosphere in the Southern Ocean using a coupled, physical-biogeochemical-ecological model. The model captures a belt of enhanced export production, figuratively termed as the Antarctic Circumpolar Productivity Belt. As observed

  13. JOURNAL OF GEOPHYSICAL RESEARCH: SOLID EARTH, VOL. 118, 120, doi:10.1002/jgrb.50258, 2013 Lithospheric structure of an Archean craton and adjacent mobile belt

    E-Print Network [OSTI]

    Jones, Alan G.

    Lithospheric structure of an Archean craton and adjacent mobile belt revealed from 2-D and 3-D inversion; accepted 20 June 2013. [1] Archean cratons, and the stitching Proterozoic orogenic belts on their flanks-African orogenic belt due to thick sedimentary cover. We present the first lithospheric-scale geophysical study

  14. THE OUTER EDGE OF THE KUIPER BELT. J. M. Hahn, Lunar and Planetary Institute, Houston TX 77058, USA, (hahn@lpi.usra.edu).

    E-Print Network [OSTI]

    Hahn, Joseph M.

    THE OUTER EDGE OF THE KUIPER BELT. J. M. Hahn, Lunar and Planetary Institute, Houston TX 77058, USA, (hahn@lpi.usra.edu). One of the more curious features of the Kuiper Belt is the apparent dearth of Kuiper Belt Objects (KBOs) orbiting the Sun beyond 50 AU with modest eccentricities and incli- nations, e

  15. Journal of the Geological Society, London, Vol. 160, 2003, pp. 677685. Printed in Great Britain. Tectonic evolution of the NE Palmyride mountain belt, Syria

    E-Print Network [OSTI]

    . 677 Tectonic evolution of the NE Palmyride mountain belt, Syria: the Bishri crustal block GRAHAM BREW1 is a broad NE-plunging inverted basin located at the NE portion of the Palmyride mountain belt where that has driven the evolution of intracontinental Syria. Keywords: Palmyride mountain belt, Syria, seismic

  16. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 97, NO. BIO, PAGES 14,207-14,221, SEPTEMBER lO, 1992 On the Stability of Isostatically Compensated Mountain Belts

    E-Print Network [OSTI]

    Sandiford, Mike

    On the Stability of Isostatically Compensated Mountain Belts SHAOHUA ZHOU AND MICHAEL SANDIFORD Department of convergent mountain belts is invariably accompanied by an increase in grav- itational potential energy due of isostatically compensated mountain belts under the assumption that the strength of continental Iithosphere

  17. EXTREME KUIPER BELT OBJECT 2001 QG298 AND THE FRACTION OF CONTACT BINARIES Scott S. Sheppard and David C. Jewitt1

    E-Print Network [OSTI]

    Jewitt, David C.

    EXTREME KUIPER BELT OBJECT 2001 QG298 AND THE FRACTION OF CONTACT BINARIES Scott S. Sheppard ABSTRACT Extensive time-resolved observations of Kuiper belt object 2001 QG298 show a light curve of 0.04 (0.10) is assumed. This is the first known Kuiper belt object and only the third minor planet

  18. UPb Silurian age for a gabbro of the Platinum-bearing Belt of the Middle Urals (Russia): evidence for beginning of closure of the Uralian Ocean

    E-Print Network [OSTI]

    Demouchy, Sylvie

    U­Pb Silurian age for a gabbro of the Platinum-bearing Belt of the Middle Urals (Russia): evidence-bearing Belt of the Urals consists of a series of zoned ultramafic bodies obducted onto the passive continental that the Uralian Platinum-bearing Belt is best interpreted as remnants of an island-arc oceanic lithosphere

  19. Abstract, 2011 Advances in Earth Science Research Conference 2011 Petrogenesis of the Metavolcanic Rocks of the North Caribou Greenstone Belt: Implications for

    E-Print Network [OSTI]

    Rocks of the North Caribou Greenstone Belt: Implications for tectonic evolution of the Archean greenstone belt J. Duff1 , K. Hattori1 and D.A. Schneider1 1 Department of Earth Sciences, University with the presence of 3.0 Ga quartz arenite and a 3.45 Ga zircon. The North Caribou belt, approximately 10 km

  20. Source and tectono-metamorphic evolution of mafic and pelitic metasedimentary rocks from the central Quetico metasedimentary belt, Archean Superior Province

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    the central Quetico metasedimentary belt, Archean Superior Province of Canada Franck Vallia* , Stephane Abstract A study of the Jean Lake area of the Quetico metasedimentary belt, Superior Province, Canada to the Wabigoon subprovince to the north and Wawa greenstone belt to the south. The P-T-time path of this Archean

  1. ApJ, in press November 3, 2013 The density of mid-sized Kuiper belt object 2002 UX25 and the

    E-Print Network [OSTI]

    Brown, Michael E.

    ApJ, in press November 3, 2013 The density of mid-sized Kuiper belt object 2002 UX25 in the Kuiper belt, with measured den- sities of 1.5 g cm-3 and higher, from the coagulation of small bodies for diameters larger than 350 km. In the Kuiper belt, no density measurements have been made between 350 km

  2. Early Paleozoic tectonic evolution of the Xing-Meng Orogenic Belt: constraints from detrital zircon geochronology of western Erguna-Xing'an Block, North China

    E-Print Network [OSTI]

    Boyer, Edmond

    Early Paleozoic tectonic evolution of the Xing-Meng Orogenic Belt: constraints from detrital zircon,c,d , Faure Michelb,c,d a Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education is similar to those from adjacent blocks in the southeastern Central Asian Orogenic Belt. Taking previous

  3. THE SECULAR EVOLUTION OF THE PRIMORDIAL KUIPER BELT. J. M. Hahn, Lunar and Planetary Institute, Houston TX 77058, USA, (hahn@lpi.usra.edu).

    E-Print Network [OSTI]

    Hahn, Joseph M.

    THE SECULAR EVOLUTION OF THE PRIMORDIAL KUIPER BELT. J. M. Hahn, Lunar and Planetary Institute, Houston TX 77058, USA, (hahn@lpi.usra.edu). The Kuiper Belt is a vast swarm of comets orbiting at the Solar System's outer edge. This Belt is comprised of debris that was left over from the epoch of planet

  4. Reanalysis of Radiation Belt Electron Phase Space Density using the UCLA 1-D VERB code and Kalman filtering: Sensitivity to assumed

    E-Print Network [OSTI]

    Ghil, Michael

    Reanalysis of Radiation Belt Electron Phase Space Density using the UCLA 1-D VERB code and Kalman of improving current radiation belt models and achieving predictive capabilities. In the future data of radiation belt electron phase space density using the VERB code and a Kalman filter to the assumed location

  5. Electric power annual 1992

    SciTech Connect (OSTI)

    Not Available

    1994-01-06

    The Electric Power Annual presents a summary of electric utility statistics at national, regional and State levels. The objective of the publication is to provide industry decisionmakers, government policymakers, analysts and the general public with historical data that may be used in understanding US electricity markets. The Electric Power Annual is prepared by the Survey Management Division; Office of Coal, Nuclear, Electric and Alternate Fuels; Energy Information Administration (EIA); US Department of Energy. ``The US Electric Power Industry at a Glance`` section presents a profile of the electric power industry ownership and performance, and a review of key statistics for the year. Subsequent sections present data on generating capability, including proposed capability additions; net generation; fossil-fuel statistics; retail sales; revenue; financial statistics; environmental statistics; electric power transactions; demand-side management; and nonutility power producers. In addition, the appendices provide supplemental data on major disturbances and unusual occurrences in US electricity power systems. Each section contains related text and tables and refers the reader to the appropriate publication that contains more detailed data on the subject matter. Monetary values in this publication are expressed in nominal terms.

  6. "We will die and become science" : the production of invisibility and public knowledge about Chernobyl radiation effects in Belarus

    E-Print Network [OSTI]

    Kuchinskaya, Olga

    2007-01-01

    Public Opinion on Nuclear Power: A Constructionist Approach,1999. Red Atom: Russia’s Nuclear Power Program from Stalin1986. Chernobyl and nuclear power in the USSR. Basingstoke:

  7. Vermont Power Exchange, a power broker for QF sales

    SciTech Connect (OSTI)

    Schuyler, S.A.

    1988-01-01

    A power broker to handle QF sales - this is the unique approach taken by the Vermont Public Service Board to implement the Federal PURPA rules. In 1983, the Vermont Public Service Board used its rule making power to create a central purchasing agent which would buy power from QFs and redistribute it to the state's retail electric companies. This function is performed by Vermont Power Exchange, Inc., which is a private company which operates the system under contract with the Board. The result of this approach is the pooling of power from QFs for distribution to the state's retail electric utilities.

  8. Heavy Vehicle Essential Power Systems Workshop

    SciTech Connect (OSTI)

    Susan Rogers

    2001-12-12

    Essential power is a crosscutting technology area that addresses the efficient and practical management of electrical and thermal requirements on trucks. Essential Power Systems: any function on the truck, that is not currently involved in moving the truck, and requires electrical or mechanical energy; Truck Lights; Hotel Loads (HVAC, computers, appliances, lighting, entertainment systems); Pumps, starter, compressor, fans, trailer refrigeration; Engine and fuel heating; and Operation of power lifts and pumps for bulk fluid transfer. Transition from ''belt and gear driven'' to auxiliary power generation of electricity - ''Truck Electrification'' 42 volts, DC and/ or AC; All electrically driven auxiliaries; Power on demand - manage electrical loads; Benefits include: increased fuel efficiency, reduced emission both when truck is idling and moving down the road.

  9. Whitestone Power & Communications (TRL 1 2 3 System) - Whitestone...

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

    Poncelet RISEC Project 32poncwpcselvaggio.ppt More Documents & Publications Vortex Hydro Energy (TRL 5 6 System) - Advanced Integration of Power Take-Off in VIVACE Water Power...

  10. Combined Heat and Power Webinar | Department of Energy

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

    Power Webinar Combined Heat and Power Webinar 06092010CHP.pdf More Documents & Publications CHP: Connecting the Gap between Markets and Utility Interconnection and Tariff...

  11. Request for Information: Federal Government Power Purchase Agreements...

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

    request for information for federal government power purchase agreement (PPA) issues. pparfi.pdf More Documents & Publications Response Summary: Department of Energy Power...

  12. PLZT film capacitors for power electronics and energy storage...

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

    PLZT film capacitors for power electronics and energy storage applications Title PLZT film capacitors for power electronics and energy storage applications Publication Type Journal...

  13. NUCLEAR POWER REACTORS AND ASSOCIATED PLANTS; 05 NUCLEAR FUELS...

    Office of Scientific and Technical Information (OSTI)

    Title list of documents made publicly available, January 1-31, 1998 NONE 21 NUCLEAR POWER REACTORS AND ASSOCIATED PLANTS; 05 NUCLEAR FUELS; BIBLIOGRAPHIES; NUCLEAR POWER PLANTS;...

  14. Analysis of Heavy Oil Recovery by Thermal EOR in a Meander Belt: From Geological

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Analysis of Heavy Oil Recovery by Thermal EOR in a Meander Belt: From Geological to Reservoir- zation of fluvial meandering reservoirs and petrophysical properties are required for uncertainty Modeling R. Deschamps*, N. Guy, C. Preux and O. Lerat 1 IFP Energies nouvelles, 1-4 avenue de Bois

  15. Quantification of the precipitation loss of radiation belt electrons observed by SAMPEX

    E-Print Network [OSTI]

    Li, Xinlin

    Click Here for Full Article Quantification of the precipitation loss of radiation belt electrons/PET observations, the rates and the spatial and temporal variations of electron loss to the atmosphere in the Earth and pitch angle diffusion. The measured electrons by SAMPEX can be distinguished as trapped, quasi trapped

  16. A nonstorm time enhancement of relativistic electrons in the outer radiation belt

    E-Print Network [OSTI]

    Li, Xinlin

    A nonstorm time enhancement of relativistic electrons in the outer radiation belt Quintin Schiller (based on the Dst index), relativistic electron fluxes were enhanced over 2.5 orders of magnitude Electron Ion Spectrometer (MagEIS), onboard the Van Allen Probes; Relativistic Electron and Proton

  17. Pitch angle distribution analysis of radiation belt electrons based on Combined Release and Radiation Effects Satellite

    E-Print Network [OSTI]

    Li, Xinlin

    Pitch angle distribution analysis of radiation belt electrons based on Combined Release and Radiation Effects Satellite Medium Electrons A data J. L. Gannon,1 X. Li,1 and D. Heynderickx2 Received 13 the Medium Electrons A instrument on the Combined Release and Radiation Effects Satellite (CRRES), a survey

  18. Heavy oil reservoirs in the Tulare Fold Belt, Cymric-McKittrick fields, Kern County, California

    SciTech Connect (OSTI)

    Farley, T. (Chevron U.S.A., Bakersfield, CA (USA))

    1990-05-01

    The Tulare fold belt is a series of asymmetric, generally northeast-verging anticlines and synclines in the Pliocene-Pleistocene Tulare Formation that trend northwestward through the Cymric-McKittrick fields. Anticlines within the deformed belt generally originated as fault propagation folds above decollements, the most important of which is the regional decollement on top of the Amnicola sand, the basal Tulare unit. The Amnicola decollement is the northeast subsurface extension of the McKittrick thrust, a low-angle fault that has displaced the Miocene Antelope shale over the Pliocene San Joaquin Formation and locally over the Tulare Formation. The Amnicola decollement is itself deformed by folding related to a younger, deeper decollement near the base of the San Joaquin Formation that merges westward with the Amnicola decollement and defines a zone of faulting associated with the McKittrick thrust Heavy oil reservoirs in the Tulare Formation are currently undergoing active development by thermal recovery techniques. In general, the geometry of heavy oil reservoirs is determined by location within the Tulare fold belt combined with the position of a subhorizontal fluid level trap that forms the updip limit of fluid-saturated rock Reservoir geometry is complicated by complex local structure, discontinuous stratigraphy, and partial depletion of heavy oil reservoirs by fluid withdrawal due to gravity drainage. Proper resolution of fold geometry, fault geometry, and position of the fluid level trap is crucial to the design and monitoring of thermal recovery projects within the Tulare fold belt.

  19. Analysis of radiation belt energetic electron phase space density using THEMIS SST measurements: Crosssatellite calibration

    E-Print Network [OSTI]

    California at Berkeley, University of

    Laboratory (LANL) satellite LANL01A synchronous orbit particle analyzer (SOPA) for a half year period SOPA instrument, the THEMIS SST underestimates the electron fluxes within a factor of 2 for the 40 and the SOPA measurements from the LANL01A and 1989­048 satellites, we analyze the response of radiation belt

  20. Numerical investigation of deformation mechanics in fold-and-thrust belts: Influence of rheology

    E-Print Network [OSTI]

    Kaus, Boris

    -and-thrust belts related to convergence tectonics develop by scraping off a rock sequence along a weaker basal décollement often formed by water-saturated shale layers or low-viscosity salt horizons. A two friction angles as the cover sequence. Model salt layers behave linear viscous, due to a lower viscosity

  1. Terrestrial Planet Formation Constrained by Mars and the Structure of the Asteroid Belt

    E-Print Network [OSTI]

    Izidoro, André; Morbidelli, Alessandro; Winter, Othon C

    2015-01-01

    Reproducing the large Earth/Mars mass ratio requires a strong mass depletion in solids within the protoplanetary disk between 1 and 3 AU. The Grand Tack model invokes a specific migration history of the giant planets to remove most of the mass initially beyond 1 AU and to dynamically excite the asteroid belt. However, one could also invoke a steep density gradient created by inward drift and pile-up of small particles induced by gas-drag, as has been proposed to explain the formation of close-in super Earths. Here we show that the asteroid belt's orbital excitation provides a crucial constraint against this scenario for the Solar System. We performed a series of simulations of terrestrial planet formation and asteroid belt evolution starting from disks of planetesimals and planetary embryos with various radial density gradients and including Jupiter and Saturn on nearly circular and coplanar orbits. Disks with shallow density gradients reproduce the dynamical excitation of the asteroid belt by gravitational s...

  2. A spectroscopic comparison of HED meteorites and V-type asteroids in the inner Main Belt

    E-Print Network [OSTI]

    Moskovitz, Nicholas A.

    V-type asteroids in the inner Main Belt (a < 2.5 AU) and the HED meteorites are thought to be genetically related to one another as collisional fragments from the surface of the large basaltic Asteroid 4 Vesta. We investigate ...

  3. School Name Team Name Coach/Teacher Bloomfield HS Van Allen Belts Jason McCaughey

    E-Print Network [OSTI]

    Devoret, Michel H.

    School Name Team Name Coach/Teacher Bloomfield HS Van Allen Belts Jason Mc Rangers Peter Schmitt Mauro Sheridan Middle School Apple Sue Brown Mercy HS Quanta Buff Bachenheimer Millbrook School Spooky Action Somerset Waters Naugatuck HS Gone Fission Marc Pardee

  4. Adaptive Linear Prediction of Radiation Belt Electrons Using the Kalman Filter

    E-Print Network [OSTI]

    to changes in solar wind bulk speed using linear prediction filters [Baker et al., 1990; Vassiliadis et alAdaptive Linear Prediction of Radiation Belt Electrons Using the Kalman Filter E.J. Rigler, D improvement in zero-time-lag electron log-flux "predictions" relative to models that are based on time

  5. Method for determining molten metal pool level in twin-belt continuous casting machines

    DOE Patents [OSTI]

    Kaiser, Timothy D. (Colchester, VT); Daniel, Sabah S. (Pittsburgh, PA); Dykes, Charles D. (Milton, VT)

    1989-03-21

    A method for determining level of molten metal in the input of a continuous metal casting machine having at least one endless, flexible, revolving casting belt with a surface which engages the molten metal to be cast and a reverse, cooled surface along which is directed high velocity liquid coolant includes the steps of predetermining the desired range of positions of the molten metal pool and positioning at least seven heat-sensing transducers in bearing contact with the moving reverse belt surface and spaced in upstream-downstream relationship relative to belt travel spanning the desired pool levels. A predetermined temperature threshold is set, somewhat above coolant temperature and the output signals of the transducer sensors are scanned regarding their output signals indicative of temperatures of the moving reverse belt surface. Position of the molten pool is determined using temperature interpolation between any successive pair of upstream-downstream spaced sensors, which follows confirmation that two succeeding downstream sensors are at temperature levels exceeding threshold temperature. The method accordingly provides high resolution for determining pool position, and verifies the determined position by utilizing full-strength signals from two succeeding downstream sensors. In addition, dual sensors are used at each position spanning the desired range of molten metal pool levels to provide redundancy, wherein only the higher temperature of each pair of sensors at a station is utilized.

  6. GEOSPATIAL DECISION SUPPORT FOR SEED COMPANIES IN THE CORN BELT Marcus E. Tooze1

    E-Print Network [OSTI]

    Reichenbach, Stephen E.

    agroecological regions where Golden Harvest's suite of corn hybrids were bested adapted in the western Corn Belt qualities and root zone water-holding capacities, reducing risks to drought events. A toolkit of ESRI Arc Harvest brand products, outlined a series of issues within their business model to improve acreage

  7. METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1

    E-Print Network [OSTI]

    Brown, Michael E.

    METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1 K. M. Barkume,1 G. A indicates the clear presence of ethane, an expected product of UV photolysis of methane. No evidence for N2 of 2005 FY9 that leads to large methane grains, abundant sites for ethane formation through UV photolysis

  8. Frontline Earth Science Research @ St Andrews The Rise and Fall of Mountain Belts

    E-Print Network [OSTI]

    Brierley, Andrew

    1 Frontline Earth Science Research @ St Andrews (FRESH) The Rise and Fall of Mountain Belts 18 and for controlling the tectonics of mountain building by Z ZZ- dZ ZZ tween tectonics and anatexis and establish (28-23 Ma) suite comprises anastamosing sheets of foli- ated two-mica, garnet-bearing granite

  9. Variations in ground surface temperature histories in the Thompson Belt, Manitoba, Canada: environment and climate changes

    E-Print Network [OSTI]

    Long, Bernard

    history (GSTH) obtained by the inversion of Pipe Mine temperature profiles suggests that a recent (50Variations in ground surface temperature histories in the Thompson Belt, Manitoba, Canada recherche en ge´ochimie et ge´odynamique, Universite´ du Que´bec a` Montre´al, C.P. 8888, succ. ``Centre

  10. Deformation regime variations in an arcuate transpressional orogen (Ribeira belt, SE Brazil) imaged by anisotropy of

    E-Print Network [OSTI]

    Bascou, Jérôme

    Deformation regime variations in an arcuate transpressional orogen (Ribeira belt, SE Brazil) imaged Paulo, Brazil b Laboratoire de Tectonophysique, Universite´ de Montpellier II CNRS, Montpellier, France Instituto de Geocie^ncias, Universidade Federal de Minas Gerais, Minas Gerais, Brazil Received 23 September

  11. Seismic imaging of the lithospheric structure of the Zagros mountain belt (Iran)

    E-Print Network [OSTI]

    Hatzfeld, Denis

    Seismic imaging of the lithospheric structure of the Zagros mountain belt (Iran) ANNE PAUL1*, DENIS International Institute of Earthquake Engineering and Seismology, Tehran, Iran 3 Institute for Advanced Studies in Basic Sciences (IASBS), PO Box 45195-1159, Zanjan, Iran *Corresponding author (e-mail: Anne

  12. AN ASTEROID BELT INTERPRETATION FOR THE TIMING VARIATIONS OF THE MILLISECOND PULSAR B1937+21

    SciTech Connect (OSTI)

    Shannon, R. M.; Cordes, J. M. [Astronomy Department, Cornell University, Ithaca, NY 14853 (United States)] [Astronomy Department, Cornell University, Ithaca, NY 14853 (United States); Metcalfe, T. S. [Space Science Institute, 4750 Walnut Street Suite 205, Boulder, CO 80301 (United States)] [Space Science Institute, 4750 Walnut Street Suite 205, Boulder, CO 80301 (United States); Lazio, T. J. W. [Jet Propulsion Laboratory, California Institute of Technology, M/S 138-308, Pasadena, CA 91109 (United States)] [Jet Propulsion Laboratory, California Institute of Technology, M/S 138-308, Pasadena, CA 91109 (United States); Cognard, I.; Desvignes, G.; Theureau, G. [LPC2E/CNRS-Universite d'Orleans, Orleans, F-45071, Cedex 2 (France)] [LPC2E/CNRS-Universite d'Orleans, Orleans, F-45071, Cedex 2 (France); Janssen, G. H.; Purver, M. B.; Stappers, B. W. [University of Manchester and Jodrell Bank Observatory, Manchester, M13 9PL (United Kingdom)] [University of Manchester and Jodrell Bank Observatory, Manchester, M13 9PL (United Kingdom); Jessner, A.; Kramer, M.; Lazaridis, K., E-mail: ryan.shannon@csiro.au, E-mail: cordes@astro.cornell.edu [Max-Planck-Institut fuer Radioastonomie, Bonn, D-53121 (Germany)

    2013-03-20

    Pulsar timing observations have revealed companions to neutron stars that include other neutron stars, white dwarfs, main-sequence stars, and planets. We demonstrate that the correlated and apparently stochastic residual times of arrival from the millisecond pulsar B1937+21 are consistent with the signature of an asteroid belt having a total mass {approx}< 0.05 M{sub Circled-Plus }. Unlike the solar system's asteroid belt, the best fit pulsar asteroid belt extends over a wide range of radii, consistent with the absence of any shepherding companions. We suggest that any pulsar that has undergone accretion-driven spin-up and subsequently evaporated its companion may harbor orbiting asteroid mass objects. The resulting timing variations may fundamentally limit the timing precision of some of the other millisecond pulsars. Observational tests of the asteroid belt model include identifying periodicities from individual asteroids, which are difficult; testing for statistical stationarity, which becomes possible when observations are conducted over a longer observing span; and searching for reflected radio emission.

  13. NEPTUNE ON TIPTOES: DYNAMICAL HISTORIES THAT PRESERVE THE COLD CLASSICAL KUIPER BELT

    SciTech Connect (OSTI)

    Wolff, Schuyler [Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218 (United States); Dawson, Rebekah I.; Murray-Clay, Ruth A., E-mail: swolff@pha.jhu.edu, E-mail: rdawson@cfa.harvard.edu, E-mail: rmurray-clay@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

    2012-02-20

    The current dynamical structure of the Kuiper Belt was shaped by the orbital evolution of the giant planets, especially Neptune, during the era following planet formation when the giant planets may have undergone planet-planet scattering and/or planetesimal-driven migration. Numerical simulations of this process, while reproducing many properties of the Belt, fail to generate the high inclinations and eccentricities observed for some objects while maintaining the observed dynamically 'cold' population. We present the first of a three-part parameter study of how different dynamical histories of Neptune sculpt the planetesimal disk. Here we identify which dynamical histories allow an in situ planetesimal disk to remain dynamically cold, becoming today's cold Kuiper Belt population. We find that if Neptune undergoes a period of elevated eccentricity and/or inclination, it secularly excites the eccentricities and inclinations of the planetesimal disk. We demonstrate that there are several well-defined regimes for this secular excitation, depending on the relative timescales of Neptune's migration, the damping of Neptune's orbital inclination and/or eccentricity, and the secular evolution of the planetesimals. We model this secular excitation analytically in each regime, allowing for a thorough exploration of parameter space. Neptune's eccentricity and inclination can remain high for a limited amount of time without disrupting the cold classical belt. In the regime of slow damping and slow migration, if Neptune is located (for example) at 20 AU, then its eccentricity must stay below 0.18 and its inclination below 6 Degree-Sign .

  14. Distributed energy resources customer adoption modeling with combined heat and power applications

    E-Print Network [OSTI]

    Siddiqui, Afzal S.; Firestone, Ryan M.; Ghosh, Srijay; Stadler, Michael; Edwards, Jennifer L.; Marnay, Chris

    2003-01-01

    System Operator California Power Exchange California Energyand reliability photovoltaic power exchange Public Utilitiesaverage California Power Exchange (CalPX) prices for those

  15. De-biased populations of Kuiper belt objects from the deep ecliptic survey

    SciTech Connect (OSTI)

    Adams, E. R.; Benecchi, S. D. [Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719 (United States); Gulbis, A. A. S. [The Southern African Large Telescope and South African Astronomical Observatory, Cape Town, 7935 (South Africa); Elliot, J. L. [Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States); Buie, M. W. [Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238 (United States); Trilling, D. E. [Department of Physics and Astronomy, Northern Arizona University, S San Francisco Street, Flagstaff, AZ 86011 (United States); Wasserman, L. H. [Lowell Observatory, 1400 W. Mars Hill Road, Flagstaff, AZ 86001 (United States)

    2014-09-01

    The Deep Ecliptic Survey (DES) was a survey project that discovered hundreds of Kuiper Belt objects from 1998 to 2005. Extensive follow-up observations of these bodies has yielded 304 objects with well-determined orbits and dynamical classifications into one of several categories: Classical, Scattered, Centaur, or 16 mean-motion resonances with Neptune. The DES search fields are well documented, enabling us to calculate the probability on each frame of detecting an object with its particular orbital parameters and absolute magnitude at a randomized point in its orbit. The detection probabilities range from a maximum of 0.32 for the 3:2 resonant object 2002 GF {sub 32} to a minimum of 1.5 × 10{sup –7} for the faint Scattered object 2001 FU {sub 185}. By grouping individual objects together by dynamical classes, we can estimate the distributions of four parameters that define each class: semimajor axis, eccentricity, inclination, and object size. The orbital element distributions (a, e, and i) were fit to the largest three classes (Classical, 3:2, and Scattered) using a maximum likelihood fit. Using the absolute magnitude (H magnitude) as a proxy for the object size, we fit a power law to the number of objects versus H magnitude for eight classes with at least five detected members (246 objects). The Classical objects are best fit with a power-law slope of ? = 1.02 ± 0.01 (observed from 5 ? H ? 7.2). Six other dynamical classes (Scattered plus five resonances) have consistent magnitude distribution slopes with the Classicals, provided that the absolute number of objects is scaled. Scattered objects are somewhat more numerous than Classical objects, while there are only a quarter as many 3:2 objects as Classicals. The exception to the power law relation is the Centaurs, which are non-resonant objects with perihelia closer than Neptune and therefore brighter and detectable at smaller sizes. Centaurs were observed from 7.5 < H < 11, and that population is best fit by a power law with ? = 0.42 ± 0.02. This is consistent with a knee in the H-distribution around H = 7.2 as reported elsewhere. Based on the Classical-derived magnitude distribution, the total number of objects (H ? 7) in each class is: Classical (2100 ± 300 objects), Scattered (2800 ± 400), 3:2 (570 ± 80), 2:1 (400 ± 50), 5:2 (270 ± 40), 7:4 (69 ± 9), 5:3 (60 ± 8). The independent estimate for the number of Centaurs in the same H range is 13 ± 5. If instead all objects are divided by inclination into 'Hot' and 'Cold' populations, following Fraser et al., we find that ?{sub Hot} = 0.90 ± 0.02, while ?{sub Cold} = 1.32 ± 0.02, in good agreement with that work.

  16. Mark Walker Director of Public Affairs

    E-Print Network [OSTI]

    assistance from the Bonneville Power Administration, which has not raised its conservation budget. If othersMark Walker Director of Public Affairs Northwest Power and Conservation Council Dear Mr. Walker, I Northwest Power and Conservation Plan. According to your recent study, Â"A Retrospective Look

  17. Mark Walker Director of Public Affairs

    E-Print Network [OSTI]

    assistance from the Bonneville Power Administration, which has not raised its conservation budget. If othersMark Walker Director of Public Affairs Northwest Power and Conservation Council Dear Mr. Walker, I Power and Conservation Plan. That's great news! According to your recent study, "A Retrospective Look

  18. UNIRIB: Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservationBio-Inspired SolarAbout /Two0 - 19 Publications 1. Xie, Z.; Ma,UNIRIB Publications

  19. Publication Policy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.Theory ofDid youOxygen Generation | CenterPressthisPublication Policy Publication of

  20. Publications | NREL

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefieldSulfateSciTechtail.Theory ofDid youOxygen Generation |Publications The NREL Publications Database

  1. An Outer Planet Beyond Pluto and Origin of the Trans-Neptunian Belt Architecture

    E-Print Network [OSTI]

    Patryk Sofia Lykawka; Tadashi Mukai

    2007-12-13

    Trans-Neptunian objects (TNOs) are remnants of a collisionally and dynamically evolved planetesimal disk in the outer solar system. This complex structure, known as the trans-Neptunian belt (or Edgeworth-Kuiper belt), can reveal important clues about disk properties, planet formation, and other evolutionary processes. In contrast to the predictions of accretion theory, TNOs exhibit surprisingly large eccentricities, e, and inclinations, i, which can be grouped into distinct dynamical classes. Several models have addressed the origin and orbital evolution of TNOs, but none have reproduced detailed observations, e.g., all dynamical classes and peculiar objects, or provided insightful predictions. Based on extensive simulations of planetesimal disks with the presence of the four giant planets and massive planetesimals, we propose that the orbital history of an outer planet with tenths of Earth's mass can explain the trans-Neptunian belt orbital structure. This massive body was likely scattered by one of the giant planets, which then stirred the primordial planetesimal disk to the levels observed at 40-50 AU and truncated it at about 48 AU before planet migration. The outer planet later acquired an inclined stable orbit (>100 AU; 20-40 deg) because of a resonant interaction with Neptune (an r:1 or r:2 resonance possibly coupled with the Kozai mechanism), guaranteeing the stability of the trans-Neptunian belt. Our model consistently reproduces the main features of each dynamical class with unprecedented detail; it also satisfies other constraints such as the current small total mass of the trans-Neptunian belt and Neptune's current orbit at 30.1 AU. We also provide observationally testable predictions.

  2. Evidence for a colour dependence in the size distribution of main belt asteroids

    E-Print Network [OSTI]

    Paul Wiegert; David Balam; Andrea Moss; Christian Veillet; Martin Connors; Ian Shelton

    2006-11-09

    We present the results of a project to detect small (~1 km) main-belt asteroids with the 3.6 meter Canada-France-Hawaii Telescope (CFHT). We observed in 2 filters (MegaPrime g' and r') in order to compare the results in each band. Owing to the observational cadence we did not observe the same asteroids through each filter and thus do not have true colour information. However strong differences in the size distributions as seen in the two filters point to a colour-dependence at these sizes, perhaps to be expected in this regime where asteroid cohesiveness begins to be dominated by physical strength and composition rather than by gravity. The best fit slopes of the cumulative size distributions (CSDs) in both filters tend towards lower values for smaller asteroids, consistent with the results of previous studies. In addition to this trend, the size distributions seen in the two filters are distinctly different, with steeper slopes in r' than in g'. Breaking our sample up according to semimajor axis, the difference between the filters in the inner belt is found to be somewhat less pronounced than in the middle and outer belt, but the CSD of those asteroids seen in the r' filter is consistently and significantly steeper than in g' throughout. The CSD slopes also show variations with semimajor axis within a given filter, particularly in r'. We conclude that the size distribution of main belt asteroids is likely to be colour dependent at kilometer sizes and that this dependence may vary across the belt.

  3. Study of movement of the western and central belts of Peninsular Malaysia using GPS data analysis

    SciTech Connect (OSTI)

    Ramli, Siti Hafizah; Samsudin, Abdul Rahim [Geology Programme, School of Environmental and Natural Resource Sciences, Faculty of Science and Technology, Universiti Kebangsaan Malaysia, 43600 Bangi, Selangor (Malaysia)

    2014-09-03

    Since the large earthquakes in Sumatera and Nias, there were some tremors incidents at Bukit Tinggi. Therefore, a study on the earth’s crust movement and the effects of the earthquake in Indonesia on the tectonic blocks of Peninsular Malaysia have been carried out using GPS data analysis. GPS data from five MyRTKnet stations within Peninsular Malaysia have been analyzed to monitor the movement of two major tectonic blocks of Peninsular Malaysia which are the western belt represented by the Behrang (BEHR) and UPM Serdang (UPMS) stations and the central belt represented by Bentong (BENT), Jerantut (JRNT) and Temerloh (TLOH) stations. GPS data recorded from 2005 to 2010 were analysed based on horizontal and vertical displacements of the respective stations by using Trimble Business Centre (TBC) software. Based on the results of accumulated displacements of recorded GPS data from January 2006 to December 2013, it shows that the western belt which represented by UPMS has shifted 0.096m towards northwest with changes of ellipsoidal height of +0.030m while the central belt which represented by TLOH has shifted 0.080m towards northwest with changes of ellipsoidal height of ?0.015m. Meanwhile, BENT station which is located on the Bentong-Raub suture zone turns to its original position as well as JRNT station. However, BEHR station which are located in western belt do not show any movements. All of these movements may be due to the influence of reactive faults in the stations area stimulated by several large earthquakes that occurred in 2005 to 2010. Study on using the GPS data analysis and combine with integrated geophysical methods are necessary to understand in detail about the tectonic evolution of Peninsular Malaysia.

  4. EVIDENCE FROM THE ASTEROID BELT FOR A VIOLENT PAST EVOLUTION OF JUPITER'S ORBIT

    SciTech Connect (OSTI)

    Morbidelli, Alessandro; Brasser, Ramon [Departement Cassiopee, Universite de Nice-Sophia Antipolis, Observatoire de la Cote d'Azur, CNRS 4, 06304 Nice (France); Gomes, Rodney [Observatrio Nacional, Rua General Jos Cristino 77, CEP 20921-400, Rio de Janeiro, RJ (Brazil); Levison, Harold F. [Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302 (United States); Tsiganis, Kleomenis [Department of Physics, Aristotle University of Thessaloniki, 54 124 Thessaloniki (Greece)

    2010-11-15

    We use the current orbital structure of large (>50 km) asteroids in the main asteroid belt to constrain the evolution of the giant planets when they migrated from their primordial orbits to their current ones. Minton and Malhotra showed that the orbital distribution of large asteroids in the main belt can be reproduced by an exponentially decaying migration of the giant planets on a timescale of {tau} {approx} 0.5 Myr. However, self-consistent numerical simulations show that the planetesimal-driven migration of the giant planets is inconsistent with an exponential change in their semi-major axes on such a short timescale. In fact, the typical timescale is {tau} {>=} 5 Myr. When giant planet migration on this timescale is applied to the asteroid belt, the resulting orbital distribution is incompatible with the observed one. However, the planet migration can be significantly sped up by planet-planet encounters. Consider an evolution where both Jupiter and Saturn have close encounters with a Neptune-mass planet (presumably Uranus or Neptune itself) and where this third planet, after being scattered inward by Saturn, is scattered outward by Jupiter. This scenario leads to a very rapid increase in the orbital separation between Jupiter and Saturn which we show here to have only mild effects on the structure of the asteroid belt. This type of evolution is called a 'jumping-Jupiter' case. Our results suggest that the total mass and dynamical excitation of the asteroid belt before migration were comparable to those currently observed. Moreover, they imply that, before migration, the orbits of Jupiter and Saturn were much less eccentric than their current ones.

  5. Industrial Utility Webinar: Public Power Open Session

    SciTech Connect (OSTI)

    2010-02-10

    The Industrial Utility Webinars focus on providing utilities with information on how to develop sucessful energy efficeincy programs for industrial energy consumers.

  6. Roosevelt Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onRAPID/Geothermal/Exploration/ColoradoRemsenburg-Speonk, NewMichigan: EnergyRocklinRohm andNew Mexico:Dist Jump to:

  7. Omaha Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History ViewMayo, Maryland:NPI VenturesNewSt.Information Olinda LandfillShakthi Renergies Ltd OSRL

  8. Butler Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LISTStar Energy LLC JumpBiossenceBrunswick, Maine:IAEA CooperationSolar Strategy

  9. MSR Public Power Agency | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc Jump to: navigation, search Name: Lyon-Lincoln ElectricEarthMJMMAMSK

  10. Southern Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc JumpHeter BatterySolarfin JumpOpen EnergySoutheastern ElectricCAGenE

  11. Southwest Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop Inc JumpHeter BatterySolarfin JumpOpen EnergySoutheasternSouthsideLLCE P A

  12. Vinton Public Power Auth | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoop IncIowa (Utility Company)Idaho) JumpWinside, Nebraska (Utility

  13. Butler Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION JEnvironmentalBowerbank, Maine:Kansas: Energy Resources Jump to: navigation,Butler County Rural P P

  14. Cornhusker Public Power Dist | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (Utility Company)| Open(Evans,Oregon:Volcano, Hawaii |North

  15. Lafayette Public Power Auth | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource History ViewInformation Actions(Redirected

  16. Omaha Public Power District | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII Jump to:InformationInformation 6thOhmsettOklahoma: EnergyII

  17. February 10, 2010 - Public Power Open Session

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:FinancingPetroleum12, 2015Executive Order14, 20111,FYDepartment of5! ASSISTANT SECRETARY OF

  18. Energy Storage & Power Electronics 2008 Peer Review - Energy...

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

    Systems Security Publications Library Energy Storage Power Electronics Advanced Modeling Grid Research Transmission Reliability Renewable Energy Integration Small Business...

  19. Abuse Testing of High Power Batteries | Department of Energy

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

    roth.pdf More Documents & Publications Abuse Tolerance Improvement Abuse Testing of High Power Batteries USABC Program Highlights...

  20. INTERPRETING THE KUIPER BELT LUMINOSITY FUNCTION. J. M. Hahn, Lunar and Planetary Institute, Houston TX 77058-1113, USA,(hahn@lpi.jsc.nasa.gov), L. Brown, ColgateUniversity, HamiltonNY 13346, USA,(labrown@center.colgate.edu).

    E-Print Network [OSTI]

    Hahn, Joseph M.

    INTERPRETING THE KUIPER BELT LUMINOSITY FUNCTION. J. M. Hahn, Lunar and Planetary Institute,(labrown@center.colgate.edu). The Kuiper Belt luminosity function m, which is the number density of Kuiper Belt Objects (KBOs) observable that increases with distance. Although most treatments of the Kuiper Belt assume a primordial radial distribution

  1. Dynamical determination of the Kuiper Belt's mass from motions of the inner planets of the Solar System

    E-Print Network [OSTI]

    Lorenzo Iorio

    2006-11-08

    In this paper we dynamically determine the mass of the Kuiper Belt Objects by exploiting the latest observational determinations of the orbital motions of the inner planets of the Solar System. Our result, in units of terrestrial masses, is 0.033 +/- 0.115 by modelling the Classical Kuiper Belt Objects as an ecliptic ring of finite thickness. A two-rings model yields for the Resonant Kuiper Belt Objects a value of 0.018 +/- 0.063. Such figures are consistent with recent determinations obtained with ground and space-based optical techniques. Some implications for precise tests of Einsteinian and post-Einsteinian gravity are briefly discussed.

  2. Participants were asked to generate aloud either the object's common use (e.g., belt: to keep one's pants up) or an uncommon use for it (e.g., belt: to use as a tourniquet). Participants received the Forward Digit Span

    E-Print Network [OSTI]

    Thompson-Schill, Sharon

    Procedure Participants were asked to generate aloud either the object's common use (e.g., belt: to keep one's pants up) or an uncommon use for it (e.g., belt: to use as a tourniquet). Participants

  3. HERSCHEL-RESOLVED OUTER BELTS OF TWO-BELT DEBRIS DISKS AROUND A-TYPE STARS: HD 70313, HD 71722, HD 159492, AND F-TYPE: HD 104860

    SciTech Connect (OSTI)

    Morales, F. Y.; Bryden, G.; Werner, M. W. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Stapelfeldt, K. R., E-mail: Farisa@jpl.nasa.gov [NASA Goddard Space Flight Center, Exoplanets and Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771 (United States)

    2013-10-20

    We present dual-band Herschel/Photodetector Array Camera and Spectrometer imaging for four stars whose spectral energy distributions (SEDs) suggest two-ring disk architectures that mirror that of the asteroid-Kuiper Belt geometry of our own solar system. The Herschel observations at 100 ?m spatially resolve the cold/outer-dust component for each star-disk system for the first time, finding evidence of planetesimals at >100 AU, i.e., a larger size than assumed from a simple blackbody fit to the SED. By breaking the degeneracy between the grain properties and the dust's radial location, the resolved images help constrain the dust grain-size distribution for each system. Three of the observed stars are A-type and one solar-type. On the basis of the combined Spitzer/IRS+MIPS (5-70 ?m), the Herschel/PACS (100 and 160 ?m) dataset, and under the assumption of idealized spherical grains, we find that the cold/outer belts of the three A-type stars are well fit with a mixed ice/rock composition rather than pure rocky grains, while the debris around the solar-type star is consistent with either rock or ice/rock grains. For the solar-type star HD 104860, we find that the minimum grain size is larger than expected from the threshold set by radiative blowout. The A-type stars HD 71722 and HD 159492, on the other hand, require minimum grain sizes that are smaller than blowout for inner- and outer-ring populations. In the absence of spectral features for ice, we find that the behavior of the continuum can help constrain the composition of the grains (of icy nature and not pure rocky material) given the Herschel-resolved locations of the cold/outer-dust belts.

  4. WIND AND WATER POWER TECHNOLOGIES OFFICE

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

    AND WATER POWER TECHNOLOGIES OFFICE August 20, 2014 2 2013 Wind Technologies Market Report Purpose, Scope, and Data: * Publicly available annual report summarizing key trends in...

  5. Power Electronic Thermal System Performance and Integration ...

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

    More Documents & Publications Motor Thermal Control Thermal Stress and Reliability for Advanced Power Electronics and Electric Machines Integrated Vehicle Thermal Management...

  6. Transportation and Stationary Power Integration: Workshop Proceedings...

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

    Transportation and Stationary Power Integration Workshop held on October 27, 2008 in Phoenix, Arizona tspiproceedings.pdf More Documents & Publications U.S. DOE Hydrogen and...

  7. Mysterious electron stash found hidden among Van Allen belts

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on77 PAGEMissionStressMoveMuncrief Ames019 For moreMy FirstMyVan

  8. Drive train design, construction, and evaluation for a powered cart for third world farmers 

    E-Print Network [OSTI]

    Kittelson, David Andrew

    1986-01-01

    of the broader goal of developing a rugged, safe, and reliable 500 kg capacity vehicle that will cost the farmers less than USS 1000. The drive train includes a torque converter, a v-belt drive with a large plywood pulley, a chain drive, and a solid drive... DEDICATION. ACRNOWLEDGNENT. . LIST OF TABLES. iv vii i LIST OF FIGURES 1 INTRODUCTION. 2 REVIEW OF LITERATURE 2. 1 Power Source 2. 2 Preliminary Drive Options 2. 3 Belt Drives. 2. 4 Chain Drives 10 13 2. 5 Differentials vs. Solid Axles. . 2. 6...

  9. Public Lecture

    ScienceCinema (OSTI)

    None

    2011-10-06

    An outreach activity is being organized by the Turkish community at CERN, on 5 June 2010 at CERN Main Auditorium. The activity consists of several talks that will take 1.5h in total. The main goal of the activity will be describing the CERN based activities and experiments as well as stimulating the public's attention to the science related topics. We believe the wide communication of the event has certain advantages especially for the proceeding membership process of Turkey.

  10. NREL: Biomass Research - Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass map shines light on771/6/14 Contact:News ReleasesChemical andPublications NREL

  11. Small Business News, Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effect Photovoltaics -7541 *Impact NeutronSmall Business News, Publications Small

  12. Sandia Energy » Publications

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust, High-ThroughputUpcoming Release of the University of Minnesota's4thAssistsPublication in

  13. Publications | Argonne National Laboratory

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergyPublications by

  14. Publications | The Ames Laboratory

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeedingProgramExemptionsProtein DynamicsEnergyPublicationsInquiries

  15. Tools for Public Information

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorking With U.S.Week DayDr.Theories81 to 1990BeToo Crowded toTools for Public

  16. Public opinion and nuclear energy

    SciTech Connect (OSTI)

    Nealey, S.M.; Melber, B.D.; Rankin, W.L.

    1983-01-01

    Public acceptance of a nuclear power plant (NPP) built near one's residence has declined steadily since the early 1970's. Following the TMI accident, this acceptance decreased dramatically. There has been some attitude rebound, however, and through mid-1981, the % who supported continued NPP construction in USA was 5 to 10% more than those in opposition. Men's and women's attitudes are different and were differentially affected by the TMI accident. Beliefs and attitudes about specific nuclear power issues were explored using questionnaires. Reactor-safety concerns were found to be more important than nuclear-waste concerns. Nuclear fuel-supply considerations are believed to be a major advantage of nuclear power. The public was largely unaware of the breeder-reactor concept. The US public generally does not favor selling US reactors abroad. It also greatly underestimates how long it takes to build a NPP. Most people believed solar-generated electricity is cheapest. The public has little information or has misinformation about some areas of nuclear power. (DLC)

  17. BONNEVILLE POWER ADMINISTRATION FOR IMMEDIATE RELEASE

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

    publicly owned electric utilities have helped 473 industrial companies save enough energy to power nearly 60,000 homes for a year. PR 02 15 BONNEVILLE POWER ADMINISTRATION FOR...

  18. The Courts in American Public Culture

    E-Print Network [OSTI]

    Silbey, Susan S.

    In American public imagination, courts are powerful but also impotent. They are guardians of citizens' rights but also agents of corporate wealth; simultaneously the least dangerous branch and the ultimate arbiters of ...

  19. An evaluation of a weight-lifting belt and back injury prevention training class for fleet service clerks 

    E-Print Network [OSTI]

    Reddell, Cheryl Renee?

    1991-01-01

    AN EVALUATION OF A WEIGHT-LIFTING BELT AND BACK INJURY PREVENTION TRAINING CLASS FOR FLEET SERVICE CLERKS A Thesis by CHERYL RENEE REDDELL Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment... of the requirements for the degree of MASTER OF SCIENCE May 1991 Major Subject: Industrial Engineering AN EVALUATION OF A WEIGHT-LIFTING BELT AND BACK INJURY PREVENTION TRAINING CLASS FOR FLEET SERVICE CLERKS A Thesis by Cheryl Rene' Reddell Approved...

  20. Social Movements and Public Policy: Eggs, Chicken, and Theory

    E-Print Network [OSTI]

    Meyer, David S.

    2003-01-01

    D. McCarthy. 1987. Social Movements in an Organizational1998. Power in Movement: Social Movements and ContentiousBurstein, Paul. 1999. “Social Movements and Public Policy. ”