National Library of Energy BETA

Sample records for mar ket-based rates

  1. HEART RATE AND BLOOD PRESSURE VARIABILITY UNDER MOON, MARS AND ZERO GRAVITY CONDITIONS DURING PARABOLIC FLIGHTS

    E-Print Network [OSTI]

    HEART RATE AND BLOOD PRESSURE VARIABILITY UNDER MOON, MARS AND ZERO GRAVITY CONDITIONS DURING), studied via the heart rate variability (HRV) and blood pressure variability (BPV). HRV and BPV were predominant during reduced gravity. For the mean heart rate, a non-monotonic relation was found, which can

  2. HEART RATE AND BLOOD PRESSURE VARIABILITY UNDER MOON, MARS AND ZERO GRAVITY CONDITIONS DURING PARABOLIC FLIGHTS

    E-Print Network [OSTI]

    via the heart rate variability (HRV) and blood pressure variability (BPV). HRV and BPV were assessed in this study to assess the heart rate variability (HRV) and blood pres- sure variability (BPV). Due to gravity between the HRV and BPV, and the gravity level. In studies from the Laboratory Experi- mental Cardiology

  3. Emissions Trading and Air Toxics Emissions: RECLAIM and Toxics Regulation in the South Coast Air Basin

    E-Print Network [OSTI]

    Cohen, Nancy J.

    1993-01-01

    Emissions Trading and Air Toxics Emissions: RECLAIM anda mar- ket-based emissions trading program called theimpacts cre- ated by emissions trading programs that affect

  4. RATES

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

    and PACI Final FRN for Rate Order No. WAPA-139 - Notice of Order Temporarily Extending Formula Rates for Power, Transmission and Ancillary Services (PDF - 49K) Final FRN for Rate...

  5. RATES

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

    - 392K) Final FRN for Rate Order No. WAPA-139 - Notice of Order Temporarily Extending Formula Rates for Power, Transmission and Ancillary Services (PDF - 49K) Final FRN for Rate...

  6. RATES

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

    - Washoe Project, Stampede Division FERC Order Approving Extension of Non-Firm Power Formula Rate - Rate Order No. WAPA-160 (Sept. 5, 2013) (PDF - 22K) Notice of Extension of...

  7. Water for future Mars astronauts?

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

    Water for future Mars astronauts? Water for future Mars astronauts? Within its first three months on Mars, NASA's Curiosity Rover saw a surprising diversity of soils and sediments...

  8. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Grutter, Alexandra "Lexa"

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser 1 Published January 11 Parasite removal rates is dependent on the rates at which par- asites are removed by cleaner fish and added through colonization-Research 1996 Resale of full article not permitted #12;Mar Ecol Prog Ser 130:61-70, 1996 of daily consumption

  9. Gamma Radiation Dose Rate in Air due to Terrestrial Radionuclides in Southern Brazil: Synthesis by Geological Units and Lithotypes Covered by the Serra do Mar Sul Aero-Geophysical Project

    SciTech Connect (OSTI)

    Bastos, Rodrigo O.; Appoloni, Carlos R. [Applied Nuclear Physics Laboratory-Department of Physics-CCE State University of Londrina Campus Universitario-Rodovia Celso Garcia Cid s/n, Cx. Postal 6001, CEP 86051-990, Londrina, PR (Brazil); Pinese, Jose P. P. [Department of Geosciences-CCE State University of Londrina Campus Universitario-Rodovia Celso Garcia Cid s/n, Cx. Postal 6001, CEP 86051-990, Londrina, PR (Brazil)

    2008-08-07

    The absorbed dose rates in air due to terrestrial radionuclides were estimated from aerial gamma spectrometric data for an area of 48,600 km{sup 2} in Southern Brazil. The source data was the Serra do Mar Sul Aero-Geophysical Project back-calibrated in a cooperative work among the Geological Survey of Brazil, the Geological Survey of Canada, and Paterson, Grant and Watson Ltd. The concentrations of eU (ppm), eTh (ppm) and K (%) were converted to dose rates in air (nGy{center_dot}h{sup -1}) by accounting for the contribution of each element's concentration. Regional variation was interpreted according to lithotypes and a synthesis was performed according to the basic geological units present in the area. Higher values of total dose were estimated for felsic igneous and metamorphic rocks, with average values varying up to 119{+-}24 nGy{center_dot}h{sup -1}, obtained by Anitapolis syenite body. Sedimentary, metasedimentary and metamafic rocks presented the lower dose levels, and some beach deposits reached the lowest average total dose, 18.5{+-}8.2 nGy{center_dot}h{sup -1}. Thorium gives the main average contribution in all geological units, the highest value being reached by the nebulitic gneisses of Atuba Complex, 71{+-}23 nGy{center_dot}h{sup -1}. Potassium presents the lowest average contribution to dose rate in 53 of the 72 units analyzed, the highest contribution being obtained by intrusive alkaline bodies (28{+-}12 nGy{center_dot}h{sup -1}). The general pattern of geographic dose distribution respects well the hypotheses on geo-physicochemical behavior of radioactive elements.

  10. The Planet Mars Mars is noticeable

    E-Print Network [OSTI]

    Walter, Frederick M.

    Evidence for Water Sedimentary layerings with salt residues #12;Sedi- mentary Rocks #12;Ingredients Mars has (or had): ·Running water on the surface ·Tectonic activity Could it have supported life? #12;The

  11. Localized precipitation and runoff on Mars

    E-Print Network [OSTI]

    Kite, Edwin S; Rafkin, Scot; Manga, Michael; Dietrich, William E

    2010-01-01

    We use the Mars Regional Atmospheric Modeling System (MRAMS) to simulate lake storms on Mars, finding that intense localized precipitation will occur for lake size >=10^3 km^2. Mars has a low-density atmosphere, so deep convection can be triggered by small amounts of latent heat release. In our reference simulation, the buoyant plume lifts vapor above condensation level, forming a 20km-high optically-thick cloud. Ice grains grow to 200 microns radius and fall near (or in) the lake at mean rates up to 1.5 mm/hr water equivalent (maximum rates up to 6 mm/hr water equivalent). Because atmospheric temperatures outside the surface layer are always well below 273K, supersaturation and condensation begin at low altitudes above lakes on Mars. In contrast to Earth lake-effect storms, lake storms on Mars involve continuous precipitation, and their vertical velocities and plume heights exceed those of tropical thunderstorms on Earth. Convection does not reach above the planetary boundary layer for lakes O(10^2) mbar. In...

  12. MARS OBSERVER Mission Failure

    E-Print Network [OSTI]

    Rhoads, James

    of Mars Observer Mission Failure.. ................... D-12 a. Most Probable Cause: Leakage of NT0 Through Check Valves .................................................................. D-14 b. Potential Cause: Pressure Regulator Failure....................... D-28 c. Potential Cause: Failure of a Pyro Valve Charge

  13. Mars mission safety

    SciTech Connect (OSTI)

    Buden, D. (EG G Idaho, Idaho Falls (USA))

    1989-06-01

    Precautions that need to be taken to assure safety on a manned Mars mission with nuclear thermal propulsion are briefly considered. What has been learned from the 1955 SNAP-10A operation of a nuclear reactor in space and from the Rover/NERVA project is reviewed. The ways that radiation hazards can be dealt with at various stages of a Mars mission are examined.

  14. Powering Mars Rovers

    ScienceCinema (OSTI)

    Stewert, Robin;

    2013-05-28

    INL scientists are doing their best to help solve our energy problems here on Earth. But did you know the lab is playing a key role in the exploration of other worlds, too? Meet INL Engineer Robin Stewart helps build and test generators that power NASA missions to Pluto and Mars. You can learn more about INL projects at http://www.facebook.com/idahonationallaboratory.

  15. What to Pack for Mars

    E-Print Network [OSTI]

    De Weck, Olivier L.

    De Weck, O.L. “What to Pack for Mars.” Spectrum, IEEE 46.6 (2009): 39. © 2009 Institute of Electrical and Electronics Engineers

  16. MAR Background Report MAR Background Report: Indigenous Protest in Brazil

    E-Print Network [OSTI]

    Milchberg, Howard

    MAR Background Report MAR Background Report: Indigenous Protest in Brazil Hundreds of indigenous people demonstrated at the National Congress in Brasilia, capital of Brazil, following the announcement in the 1990s in the midst of extensive protests in Brazil and around the world. On February 8, an indigenous

  17. New Mexico to Mars

    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 shinesSolarNew scholarship supports returningNew Mexico to Mars Community

  18. Mars as a comet: Solar wind interaction on a large scale

    E-Print Network [OSTI]

    Holmstrom, Mats

    2015-01-01

    Looking at the Mars-solar wind interaction on a larger spatial scale than the near Mars region, the planet can be seen as an ion source interacting with the solar wind, in many ways like a comet, but with a smaller ion source region. Here we study the interaction between Mars and the solar wind using a hybrid model (particle ions and fluid electrons). We find that the solar wind is disturbed by Mars out to 100 Mars radii downstream of the planet, and beyond. On this large scale it is clear that the escaping ions can be classified into two different populations. A polar plume of ions picked-up by the solar wind, and a more fluid outflow of ions behind the planet. The outflow increases linear with the production up to levels of observed outflow rates, then the escape levels off for higher production rates.

  19. The Mars Microphone: Ready to Go by Greg Delory

    E-Print Network [OSTI]

    California at Berkeley, University of

    and David Juergens of the Jet Propulsion Laboratory, who proposed to the Planetary Society that a sound mass, power, volume, or data­rate adjustments on the lander. Friedman and Society President Carl Sagan Sciences Laboratory. Are There Sounds on Mars? Given that sound waves need an atmospheric medium through

  20. The Mars Microphone: Ready to Go by Greg Delory

    E-Print Network [OSTI]

    California at Berkeley, University of

    and David Juergens of the Jet Propulsion Laboratory, who proposed to the Planetary Society that a sound mass, power, volume, or data-rate adjustments on the lander. Friedman and Society President Carl Sagan Sciences Laboratory. Are There Sounds on Mars? Given that sound waves need an atmospheric medium through

  1. LOCALIZED PRECIPITATION, LAKE-EFFECT STORMS, AND EROSION ON MARS.

    E-Print Network [OSTI]

    LOCALIZED PRECIPITATION, LAKE-EFFECT STORMS, AND EROSION ON MARS. Edwin. S. Kite*, Earth], this hypothesis has never been modeled. We report numerical tests of localized precipitation using MRAMS ephemeral lakes. For a given vapor injection rate or lake surface temperature, localized precipitation

  2. An earth image simulation and tracking system for the Mars Laser Communication Demonstration

    E-Print Network [OSTI]

    Balster, Stephanie Karen

    2005-01-01

    In this thesis I created an Earth-image simulation and investigated Earth-tracking algorithms for the Mars Laser Communication Demonstration (MLCD). The MLCD mission will demonstrate the feasibility of high-data-rate laser ...

  3. Mars Surveyor Program '01 Mars Environmental Compatibility Assessment wet chemistry lab

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    Mars Surveyor Program '01 Mars Environmental Compatibility Assessment wet chemistry lab: A sensor Department of Chemistry, Tufts University, Medford, Massachusetts, USA Michael H. Hecht, Sabrina M. Grannan] The Mars Environmental Compatibility Assessment (MECA) instrument was designed, built, and flight qualified

  4. Earth plus Mars: Los Alamos National

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

    plus Mars: Los Alamos National Lab partners with Spain and France June 26, 2015 Earth plus Mars: Los Alamos National Lab partners with Spain and France New Mexico's role in the...

  5. Mars `Curiosity' has ORNL tech

    E-Print Network [OSTI]

    Pennycook, Steve

    thermoelectric generator, the Multi-Mission Radioisotope Thermoelectric Generator." ORNL's iridium alloy clad Radioisotope Thermoelectric Generator were produced at ORNL. (Image courtesy of NASA.) Table of Contents Mars involved with the development of this generator for several years." Key components of the probe's Multi-Mission

  6. European Space Agency European Mars Science and Exploration Conference: Mars Express & ExoMars

    E-Print Network [OSTI]

    Withers, Paul

    flares (and/or plumes), seismic shaking and crater excavation [7]. These effects have been modelled between the different instruments, require no hardware modification or space qualification of "soft-landing; and seismic detection of impact event clusters correlated with Mars' passage through low- speed meteoroid

  7. MAR flow mapping of Analytical Chemistry Operations (Preliminary Report)

    SciTech Connect (OSTI)

    Barr, Mary E. [Los Alamos National Laboratory; Farish, Thomas J. [Los Alamos National Laboratory

    2012-06-13

    The recently released Supplemental Directive, NA-1 SD 1027, updates the radionuclide threshold values in DOE-STD-1027-92 CN1 to reflect the use of modern parameters for dose conversion factors and breathing rates. The directive also corrects several arithmetic errors within the original standard. The result is a roughly four-fold increase in the amount of weapons-grade nuclear material allowed within a designated radiological facility. Radiological laboratory space within the recently constructed Radiological Laboratory Office and Utility Building (RLUOB) is slated to house selected analytical chemistry support activities in addition to small-scale actinide R&D activities. RLUOB is within the same facility operations envelope as TA-55. Consolidation of analytical chemistry activities to RLUOB and PF-4 offers operational efficiency improvements relative to the current pre-CMRR plans of dividing these activities between RLUOB, PF-4, and CMR. RLUOB is considered a Radiological Facility under STD-1027 - 'Facilities that do not meet or exceed Category 3 threshold criteria but still possess some amount of radioactive material may be considered Radiological Facilities.' The supplemental directive essentially increases the allowable material-at-risk (MAR) within radiological facilities from 8.4 g to 38.6 g for {sup 239}Pu. This increase in allowable MAR provides a unique opportunity to establish additional analytical chemistry support functions in RLUOB without negatively impacting either R&D activities or facility operations. Individual radiological facilities are tasked to determine MAR limits (up to the Category 3 thresholds) appropriate to their operational conditions. This study presents parameters that impact establishing MAR limits for RLUOB and an assessment of how various analytical chemistry support functions could operate within the established MAR limits.

  8. Computer Architecture (13 Mar 2008)

    E-Print Network [OSTI]

    Park, Seung-Jong "Jay"

    1 Computer Architecture (CSC-3501) Lecture 15 1 Lecture 15 (13 Mar 2008) Seung-Jong Park (Jay) http://www.csc.lsu.edu/~sjpark CSC3501 - S.J. Park Announcement 2 CSC3501 - S.J. Park 4.14 Real World Architectures MARIE shares many features with modern architectur es but it is not an accurate depiction of them. In the following slides

  9. Nuclear technologies for Moon and Mars exploration

    SciTech Connect (OSTI)

    Buden, D.

    1991-01-01

    Nuclear technologies are essential to successful Moon and Mars exploration and settlements. Applications can take the form of nuclear propulsion for transport of crews and cargo to Mars and the Moon; surface power for habitats and base power; power for human spacecraft to Mars; shielding and life science understanding for protection against natural solar and cosmic radiations; radioisotopes for sterilization, medicine, testing, and power; and resources for the benefits of Earth. 5 refs., 9 figs., 3 tabs.

  10. THE MARS ENVIRONMENTAL COMPATIBILITY ASSESSMENT (MECA) WET CHEMISTRY EXPERIMENT ON THE MARS '01 LANDER

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    THE MARS ENVIRONMENTAL COMPATIBILITY ASSESSMENT (MECA) WET CHEMISTRY EXPERIMENT ON THE MARS '01 of Chemistry, TuftsUniversity, Medford, MA, 02155 4 Mineral Processing Department, West Virginia University, Morgantown, WV, 26507 Introduction. The Mars Environmental Compatibility Assessment (MECA) is an instrument

  11. MAVEN overview MAVEN is a NASA Mars Scout mission designed to orbit Mars

    E-Print Network [OSTI]

    Mojzsis, Stephen J.

    MAVEN overview MAVEN is a NASA Mars Scout mission designed to orbit Mars and explore the state-Boulder professor and LASP research scientist, leads the project on behalf of NASA. Jakosky worked with a national of primary mission Mission description: MAVEN is a NASA Mars Scout mission carrying eight instruments

  12. 2011 MARS Refresher Presentation (2 of 3)

    ScienceCinema (OSTI)

    None

    2011-10-06

    Information sessions that shall outline the general principles of the 2011 annual Merit, Appraisal and Recognition Scheme (MARS). Presentation will be given in English.

  13. 2010 MARS Refresher Presentation (3 of 3)

    ScienceCinema (OSTI)

    None

    2011-10-06

    Information sessions that shall outline the general principles of the 2010 annual Merit, Appraisal and Recognition Scheme (MARS). Presentation will be given in English.

  14. NASA agreements advance Mars exploration, Los Alamos Rover instrument...

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

    NASA agreements advance Mars exploration NASA agreements advance Mars exploration, Los Alamos Rover instrument a key component Los Alamos National Laboratory is coordinating with...

  15. Los Alamos laser selected for 2020 Mars mission

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

    Los Alamos laser selected for 2020 Mars mission Los Alamos laser selected for 2020 Mars mission SuperCam builds upon the successful capabilities demonstrated aboard the Curiosity...

  16. The 2013 MAVEN Mission To Mars

    E-Print Network [OSTI]

    Of Martian Atmosphere Turn-off of the Martian magnetic field allowed turn-on of solar-EUV and solar · Spacecraft Dry Mass: 903 kg max · Power: 1135 W at Mars Aphelion MAG (2) "Gull-Wing" Solar Arrays LPW (2 latitude and local solar time · One-Earth-year mission allows thorough coverage of near-Mars space #12

  17. Mar

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

    Livermore, CA 94550, USA 10 Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA 11 Jet Propulsion Laboratory, California Institute of Technol- ogy,...

  18. The MAVEN mission to Mars and my role in it

    E-Print Network [OSTI]

    Withers, Paul

    of the environmental requirements for the occurrence of life: · Liquid water · Access to the biogenic elements · Source With Mars #12;Overarching Question: Did Mars Ever Have Life? Mars appears to meet or have met all of energy to drive metabolism Did Mars ever have life? How did any life interact with its planetary

  19. 02/02 NASA JSC Astrobiology: Fingerprints of Life Searching for Life: Mars Critters 1 Mars Critters

    E-Print Network [OSTI]

    Waliser, Duane E.

    to handle the constant radiation on the surface of Mars. Also the dominant gas in the Mars atmosphere Destination: Mars. In groups or as individuals, students will use their knowledge of Mars and living organisms up various art supplies at each table for either individual work or small group work. This activity

  20. Radiation dose estimates for typical piloted NTR lunar and Mars mission engine operations

    SciTech Connect (OSTI)

    Schnitzler, B.G. (EG and G Idaho, Inc., Idaho Falls, ID (United States)); Borowski, S.K. (National Aeronautics and Space Administration, Cleveland, OH (United States). Lewis Research Center)

    1991-01-01

    The natural and manmade radiation environments to be encountered during lunar and Mars missions are qualitatively summarized. The computational methods available to characterize the radiation environment produced by an operating nuclear propulsion system are discussed. Mission profiles and vehicle configurations are presented for a typical all-propulsive, fully reusable lunar mission and for a typical all-propulsive Mars mission. Estimates of crew location biological doses are developed for all propulsive maneuvers. Post-shutdown dose rates near the nuclear engine are estimated at selected mission times. 15 refs., 4 figs.

  1. Solar discrepancies : Mars exploration and the curious problem of inter-planetary time

    E-Print Network [OSTI]

    Mirmalek, Zara Lenora

    2008-01-01

    Monterey, California. Solar Discrepancies: Mars explorationCALIFORNIA, SAN DIEGO Solar discrepancies: Mars explorationOF THE DISSERTATION Solar discrepancies: Mars exploration

  2. Mars Rover's ChemCam Instrument gets

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

    last week to install the new software on Mars. "We think we will actually have better quality images and analyses with this new software than the original," said Wiens. The...

  3. The Mission of the Mars Exploration Rovers

    ScienceCinema (OSTI)

    Grant, John [Smithsonian Institution, Washington, D.C., United States

    2010-01-08

    The Mars Exploration Rover mission was expected to last 3 months, but has continued for more than 4 years. The major science results from both rovers will be summarized.

  4. The surface of Mars : morphology and process

    E-Print Network [OSTI]

    Aharonson, Oded, 1973-

    2002-01-01

    The goal of this work is a quantitative description of the morphology of the surface of Mars, in order to constrain the nature of processes acting during the ancient past through today. Emphasis is placed on linking geometric ...

  5. Adaptive control for Mars atmospheric flight 

    E-Print Network [OSTI]

    Restrepo, Carolina Isabel

    2009-05-15

    The new vision for space exploration will focus on sending humans to the moon and eventually to Mars. This endeavor presents new challenges that are critically di?erent from the past experience with robotic missions to ...

  6. Microbial iron reduction on Earth and Mars 

    E-Print Network [OSTI]

    Nixon, Sophie Louise

    2014-11-27

    The search for life beyond Earth is the driving force behind several future missions to Mars. An essential task in the lead-up to these missions is a critical assessment of the habitability for, and feasibility of, life. ...

  7. Rate Schedules

    Broader source: Energy.gov [DOE]

    One of the major responsibilities of Southeastern is to design, formulate, and justify rate schedules. Repayment studies prepared by the agency determine revenue requirements and appropriate rate...

  8. Remote sensing of surface pressure on Mars with the Mars Express/OMEGA spectrometer

    E-Print Network [OSTI]

    Spiga, Aymeric

    - surement of surface pressure from orbit, as is done for temperature or water vapor [Smith, 2006]. [4Remote sensing of surface pressure on Mars with the Mars Express/OMEGA spectrometer: 2 November 2006; revised 6 July 2007; accepted 7 August 2007; published 30 August 2007. [1] Surface pressure

  9. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    written consent of the publisher #12;Mar Ecol Prog Ser 280: 261­273, 2004 cific mesoscale oceanographic

  10. Mars mission laser tool heads to JPL

    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 toMSDS onBudget ||EnergyMark Holecek |MarkMarsMars

  11. Tuesday, March 24, 2009 MARS: GROUND ICE AND CLIMATE CHANGE

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Tuesday, March 24, 2009 MARS: GROUND ICE AND CLIMATE CHANGE 1:30 p.m. Waterway Ballroom 1 Chairs.-B. Fastook J. L. Deciphering the Late Amazonian Climate History of Mars: Assessing Obliquity Predictions climate history of Mars; extended periods of consistently high or low obliquity are unlikely during

  12. Humans to Mars Fifty Years of Mission Planning,

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Humans to Mars Fifty Years of Mission Planning, 1950--2000 David S. F. Portree Monographs in Aerospace History #21 NASA SP-2001-4521 Humans to Mars Fifty Years of Mission Planning, 1950--2000 David S. F. Portree #12;Humans to Mars Fifty Years of Mission Planning, 1950­2000 by David S. F. Portree NASA

  13. Recent MARS15 Developments, New Features and Event Generator Modes

    E-Print Network [OSTI]

    McDonald, Kirk

    Recent MARS15 Developments, New Features and Event Generator Modes Fermilab Accelerator Physics-28, 2013 Nikolai Mokhov 8 MARS15 EXCLUSIVE EVENT GENERATORS Improved Cascade-Exciton Model code, CEM03. Mokhov, "CEM03.03 and LAQGSM03.03 Event Generators for the MCNP6, MCNPX and MARS15 Transport Codes", LANL

  14. Interior Structure and Seasonal Mass Redistribution of Mars from Radio

    E-Print Network [OSTI]

    Manga, Michael

    Interior Structure and Seasonal Mass Redistribution of Mars from Radio Tracking of Mars Pathfinder. Analysis of radio tracking measurements from the Vi- king landers has determined the normal- ized polar. The precession is driven by the gravita- tional torque of the sun acting on Mars' oblate figure

  15. Thursday, March 16, 2006 MARS: SEDIMENTS AND GEOCHEMISTRY

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Thursday, March 16, 2006 MARS: SEDIMENTS AND GEOCHEMISTRY 8:30 a.m. Crystal Ballroom A Chairs: N. J of the Proposed Hypotheses for the Origin of Sediments at the Opportunity Landing Site on Mars [#1869] The MER Athena Team interpretation that sediments at the Opportunity Landing Site on Mars are altered eolian

  16. Lidar on the Phoenix mission to Mars James Whiteway,1

    E-Print Network [OSTI]

    Duck, Thomas J.

    Lidar on the Phoenix mission to Mars James Whiteway,1 Michael Daly,2 Allan Carswell,3 Thomas Duck,4 from the surface of Mars as part of the Phoenix mission. This will measure the height profile, and C. Cook (2008), Lidar on the Phoenix mission to Mars, J. Geophys. Res., 113, E00A08, doi:10

  17. Risk Management, Mar 2012 Risk Management

    E-Print Network [OSTI]

    Risk Management, Mar 2012 Risk Management Conditions of Volunteer Service (Please send completed form to the Office of Risk Management) riskmanagement@uoregon.edu Fax: 541-346-7008 As a volunteer Tort Claims Act, ORS 30.260-300, and Oregon Department of Administrative Services Risk Management

  18. Project Management in NASA Mars Climate Orbiter

    E-Print Network [OSTI]

    Rhoads, James

    by the Mars Climate Orbiter Mishap Investigation Board F. Recurring Themes From Failure Investigations and Control Center Navigation and Control Center Goddard Space Flight Center Goddard Space Flight Center Merwarth NASA/GSFC-retired Expert in ground operations & flight software development Moshe F. Rubinstein

  19. The MAVEN Mission: Exploring Mars' Climate

    E-Print Network [OSTI]

    Mojzsis, Stephen J.

    at launch ·Spacecraft Dry Mass: 810 kg at launch ·Power: 1135 W at Mars Aphelion MAG (2) "Gull-Wing" Solar Us to Understand Escape of Atmospheric Gases to Space #12;The Solar Wind is Able to Strip Off Gas-Related Proper1es and Processes LPW MAG STATIC Sun, Solar Wind, Solar Storms SWIA EUV

  20. Product specification Supersedes data 1998 Mar 24

    E-Print Network [OSTI]

    Ida, Nathan

    DATA SHEET Product specification Supersedes data 1998 Mar 24 2000 Jun 13 DISCRETE SEMICONDUCTORS KMZ51 Magnetic field sensor M3D495 #12;2000 Jun 13 2 Philips Semiconductors Product specification output voltage 8 -Iflip flip coil handbook, halfpage 41 58 MGD827 pin 1 index Hext Fig.1 Simplified

  1. Temporal Variability of Waves at the Proton Cyclotron Frequency Upstream from Mars: Implications for Mars Distant Hydrogen Exosphere

    E-Print Network [OSTI]

    Bertucci, Cesar; Chaufray, Jean-Yves; Gomez, Daniel; Mazelle, Christian; Delva, Magda; Modolo, Ronan; Gonzalez-Galindo, Francisco; Brain, David Andrew

    2013-01-01

    We report on the temporal variability of the occurrence of waves at the local proton cyclotron frequency upstream from the Martian bow shock from Mars Global Surveyor observations during the first aerobraking and science phasing orbit periods. Observations at high southern latitudes during minimum-to-mean solar activity show that the wave occurrence rate is significantly higher around perihelion southern summer solstice and lower around the same hemisphere's spring and autumn equinoxes. A similar trend is observed in the hydrogen (H) exospheric density profiles over the Martian South Pole obtained from a model including UV thermospheric heating effects. In spite of the complexity in the ion pick-up and plasma wave generation and evolution processes, these results support the idea that variations in the occurrence of waves could be used to study the temporal evolution of the distant Martian H corona and its coupling with the thermosphere at altitudes currently inaccessible to direct measurements.

  2. Impact inducted surface heating by planetesimals on early Mars

    E-Print Network [OSTI]

    Maindl, T I; Lammer, H; Güdel, M; Schäfer, C; Speith, R; Odert, P; Erkaev, N V; Kislyakova, K G; Pilat-Lohinger, E

    2014-01-01

    We investigate the influence of impacts of large planetesimals and small planetary embryos on the early Martian surface on the hydrodynamic escape of an early steam atmosphere that is exposed to the high soft X-ray and EUV flux of the young Sun. Impact statistics in terms of number, masses, velocities, and angles of asteroid impacts onto the early Mars are determined via n-body integrations. Based on these statistics, smoothed particle hydrodynamics (SPH) simulations result in estimates of energy transfer into the planetary surface material and according surface heating. For the estimation of the atmospheric escape rates we applied a soft X-ray and EUV absorption model and a 1-D upper atmosphere hydrodynamic model to a magma ocean-related catastrophically outgassed steam atmosphere with surface pressure values of 52 bar H2O and 11 bar CO2. The estimated impact rates and energy deposition onto an early Martian surface can account for substantial heating. The energy influx and conversion rate into internal ener...

  3. Microsoft Word - ex1b-ITER-mar07.doc

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

    PATENT RIGHTS - ACQUISITION BY THE GOVERNMENT - ITER (Mar 2007) (a) Definitions. (1) "Invention", as used in this clause, means any invention or discovery which is or may be...

  4. Dose calculations using MARS for Bremsstrahlung beam stops and collimators in APS beamline stations.

    SciTech Connect (OSTI)

    Dooling, J.; Accelerator Systems Division

    2010-11-01

    The Monte Carlo radiation transport code MARS is used to model the generation of gas bremsstrahlung (GB) radiation from 7-GeV electrons which scatter from residual gas atoms in undulator straight sections within the Advanced Photon Source (APS) storage ring. Additionally, MARS is employed to model the interactions of the GB radiation with components along the x-ray beamlines and then determine the expected radiation dose-rates that result. In this manner, MARS can be used to assess the adequacy of existing shielding or the specifications for new shielding when required. The GB radiation generated in the 'thin-target' of an ID straight section will consist only of photons in a 1/E-distribution up to the full energy of the stored electron beam. Using this analytical model, the predicted GB power for a typical APS 15.38-m insertion device (ID) straight section is 4.59 x 10{sup -7} W/nTorr/mA, assuming a background gas composed of air (Z{sub eff} = 7.31) at room temperature (293K). The total GB power provides a useful benchmark for comparisons between analytical and numerical approaches. We find good agreement between MARS and analytical estimates for total GB power. The extended straight section 'target' creates a radial profile of GB, which is highly peaked centered on the electron beam. The GB distribution reflects the size of the electron beam that creates the radiation. Optimizing the performance of MARS in terms of CPU time per incident trajectory requires the use of a relatively short, high-density gas target (air); in this report, the target density is {rho}L = 2.89 x 10{sup -2} g/cm{sup 2} over a length of 24 cm. MARS results are compared with the contact dose levels reported in TB-20, which used EGS4 for radiation transport simulations. Maximum dose-rates in 1 cc of tissue phantom form the initial basis for comparison. MARS and EGS4 results are approximately the same for maximum 1-cc dose-rates and attenuation in the photon-dominated regions; for thicker targets, however, the dose-rate no longer depends only on photon attenuation, as photoneutrons (PNs) begin to dominate. The GB radiation-induced photoneutron measurements from four different metals (Fe, Cu, W, and Pb) are compared with MARS predictions. The simulated dose-rates for beamline 6-ID are approximately 3-5 times larger than the measured values, whereas those for beamline 11-ID are much closer. Given the uncertainty in local values of pressure and Z, the degree of agreement between MARS and the PN measurements is good. MARS simulations of GB-induced radiation in and around the FOE show the importance of using actual pressure and gas composition (Z{sub eff}) to obtain accurate PN dose. For a beam current of 300 mA, extrapolating pressure data measured in previously published studies predicts an average background gas pressure of 27 nTorr. An average atomic number of Z{sub eff} = 4.0 is obtained from the same studies. In addition, models of copper masks presently in use at the APS are included. Simulations show that inclusion of exit masks make significant differences in both the radiation spatial distribution within the FOE, as well as the peak intensity. Two studies have been conducted with MARS to assess shielding requirements. First, dose levels in contact with the outside wall of the FOE are examined when GB radiation strikes Pb or W beam stops of varying transverse size within the FOE. Four separate phantom regions are utilized to measure the dose, two at beam elevation and two at the horizontal beam position. The first two phantoms are used for scoring FOE dose along the outside and back walls, horizontally; the second two collect dose on the roof and vertically on the back wall. In all cases, the beam stop depth is maintained at 30 cm. Inclusion of front end (FE) exit masks typically cause a 1-2 order-of-magnitude increase in the dose-rates relative to the case with no masks. Masks place secondary bremsstrahlung sources inside the FOE, and therefore they must be shielded appropriately. The MARS model does not fully account for all shielding present

  5. Mars Rover finds changing rocks, surprising scientists

    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 toMSDS onBudget ||EnergyMark Holecek |MarkMars Rover

  6. Mars Curiosity rover talks in May

    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 would likeUniverseIMPACTThousandReport)PriceHistoricEnergyApril 25,4MarioMarkMars Curiosity

  7. Mars Rover's ChemCam Instrument gets

    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 would likeUniverseIMPACTThousandReport)PriceHistoricEnergyApril 25,4MarioMarkMars

  8. Communiqu de presse Lyon, le 20 mars 2014

    E-Print Network [OSTI]

    Dellandréa, Emmanuel

    Communiqué de presse Lyon, le 20 mars 2014 3 000 étudiants pour la 32ème édition du Challenge Centrale Lyon Ce weekend du 22 et 23 mars 2014, l'école Centrale Lyon (Ecully) accueille sur son campus

  9. EWO Meeting, Mar. 2008, Pittsburgh, PA Risk Management

    E-Print Network [OSTI]

    Grossmann, Ignacio E.

    EWO Meeting, Mar. 2008, Pittsburgh, PA Risk Management Risk Management for Chemical Supply Chain, PA Risk Management Chemical Supply chain: an integrated network of business units for the supply #12;Page 3EWO Meeting, Mar. 2008, Pittsburgh, PA Risk Management Motivation Introduction · Objective

  10. Selection and Technology Evaluation of Moon/Mars Transportation Architectures

    E-Print Network [OSTI]

    de Weck, Olivier L.

    Selection and Technology Evaluation of Moon/Mars Transportation Architectures Gergana A. Bounova of Technology, Cambridge, MA 02139 Our purpose is to evaluate and select from a large family of Moon-Mars transportation architectures by integrating a general architecture network model with vehicle computa- tional

  11. Oceanography Vol.18, No.1, Mar. 2005 65 OCEANOGRAPHY

    E-Print Network [OSTI]

    Yen, Jeannette

    Oceanography Vol.18, No.1, Mar. 2005 65 WOMEN IN OCEANOGRAPHY AU TO B I O G R A PH I C A L S K E TC H E S O F Oceanography Vol.18, No.1, Mar. 2005 65 This article has been published in Oceanography, Volume 18, Number 1, a quarterly journal of The Oceanography Society. Copyright 2005 by The Oceanography

  12. The Global Topography of Mars and Implications for Surface

    E-Print Network [OSTI]

    Hauck II, Steven A.

    The Global Topography of Mars and Implications for Surface Evolution David E. Smith,1 * Maria T- accuracy global map of the topography of Mars. Dominant features include the low northern hemisphere-wavelength effect that has been shaped by an internal mechanism. The topography of Tharsis consists of two broad

  13. Simulations of the Mars ionosphere during a solar flare

    E-Print Network [OSTI]

    Withers, Paul

    .05.23 08:00-10:00 Spring AGU Meeting 2006, Acapulco, Mexico #12;Increased fluxes of X-rays during solarSimulations of the Mars ionosphere during a solar flare Paul Withers, Joei Wroten, Michael Mendillo simulations of the Mars ionosphere driven by temporally-varying solar fluxes, concentrating on 15 and 26 April

  14. CRISM: Exploring the Geology of Mars Tech Splash Open Music

    E-Print Network [OSTI]

    CRISM: Exploring the Geology of Mars Tech Splash Open Music Exploring the geology of Mars Marineris simply pulled apart, we would expect the geology on the North and South side of the canyon that make up the rocks. Using the CRISM data we can put together a very simplistic geologic profile

  15. Regionally compartmented groundwater flow on Mars Keith P. Harrison1

    E-Print Network [OSTI]

    Harrison, Keith

    Regionally compartmented groundwater flow on Mars Keith P. Harrison1 and Robert E. Grimm1 Received] Groundwater flow on Mars likely contributed to the formation of several types of morphologic and mineralogic of groundwater flow required for their formation. For groundwater simulation purposes, a global Martian aquifer

  16. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Krug, Patrick J.

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 312: 149­159, 2006 Published April 24 therefore have limited time to locate and colonize a suitable adult habitat. Domi- nant spatial competitors consent of the publisher #12;Mar Ecol Prog Ser 312: 149­159, 2006 energy reserves, they became `desperate

  17. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Denny, Mark

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 522: 127­143, 2015 doi: 10.3354/meps11117 on experimental plates colonized by natural microalgae. Limpet species found higher on the shore had lower peak without written consent of the publisher #12;Mar Ecol Prog Ser 522: 127­143, 2015 In the rocky intertidal

  18. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Pawlik, Joseph

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 368: 137­143, 2008 doi: 10.3354/meps07615 and reproduction, thereby also enhancing their ability to colonize open space. As for some plant communities without written consent of the publisher #12;Mar Ecol Prog Ser 368: 137­143, 2008 primary limiting

  19. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Shima, Jeff

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 472: 239­248, 2013 doi: 10.3354/meps10015 in the system via a range of mechanisms, including competition-colonization tradeoffs (Levins & Culver 1971 holder(s). It may be distributed to interested individuals on request. #12;Mar Ecol Prog Ser 472: 239

  20. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Stachowicz, Jay

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 398: 69­80, 2010 doi: 10.3354/meps08341 surfaces for colonization that adequately compensate for the primary substrate it exploits, its high consent of the publisher #12;Mar Ecol Prog Ser 398: 69­80, 2010 Rodriguez 2006, Heiman et al. 2008

  1. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 262: 19­25, 2003 Published November 7 blocked access to ice-free terrain for breeding. The first colonization of Ross Island in East Mc;Mar Ecol Prog Ser 262: 19­25, 2003 guins (Baroni &

  2. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Pawlik, Joseph

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 465: 111­117, 2012 doi: 10.3354/meps09904. laevis neither affected the frequency of colonization of Montastraea annularis by boring sponges, nor individuals on request. #12;Mar Ecol Prog Ser 465: 111­117, 2012 tem are altered. These context

  3. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Love, Milton

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 344: 245­256, 2007 doi: 10.3354/meps06929 findings suggest that trophic pathways on other types of artificial structures colonized by exotic species · Artificial reef Resale or republication not permitted without written consent of the publisher #12;Mar Ecol

  4. Real-time graphic displays in Mars. [AVLIS process

    SciTech Connect (OSTI)

    Treadway, T.

    1985-12-01

    Real-time diagnostic data of the AVLIS process is displayed in the form of a two-dimensional plot on selected monitors in the Mars Control Room. Each Mars workstation contains a HP2622 terminal for computer interface to the experiment and a Raster Technologies graphic controller driving a Conrac high resolution color monitor for graphics output.

  5. Remote Terrestrial Sites as Operational/Logistics Analogs for Moon/Mars Bases: the Haughton Mars Project

    E-Print Network [OSTI]

    de Weck, Olivier L.

    Remote Terrestrial Sites as Operational/Logistics Analogs for Moon/Mars Bases: the Haughton Mars coordinating the logistics and resupply of far-flung planetary bases. A number of logistics methods have been terrestrial logistics methods were tested in the context of (analog) planetary exploration. A comprehensive

  6. A Flow-Channel Analysis for the Mars Hopper

    SciTech Connect (OSTI)

    W. Spencer Cooley

    2013-02-01

    The Mars Hopper is an exploratory vehicle designed to fly on Mars using carbon dioxide from the Martian atmosphere as a rocket propellant. The propellent gasses are thermally heated while traversing a radioisotope ther- mal rocket (RTR) engine’s core. This core is comprised of a radioisotope surrounded by a heat capacitive material interspersed with tubes for the propellant to travel through. These tubes, or flow channels, can be manu- factured in various cross-sectional shapes such as a special four-point star or the traditional circle. Analytical heat transfer and computational fluid dynamics (CFD) anal- yses were performed using flow channels with either a circle or a star cross- sectional shape. The nominal total inlet pressure was specified at 2,805,000 Pa; and the outlet pressure was set to 2,785,000 Pa. The CO2 inlet tem- perature was 300 K; and the channel wall was 1200 K. The steady-state CFD simulations computed the smooth-walled star shape’s outlet temper- ature to be 959 K on the finest mesh. The smooth-walled circle’s outlet temperature was 902 K. A circle with a surface roughness specification at 0.01 mm gave 946 K and at 0.1 mm yielded 989 K. The The effects of a slightly varied inlet pressure were also examined. The analytical calculations were based on the mass flow rates computed in the CFD simulations and provided significantly higher outlet temperature results while displaying the same comparison trends. Research relating to the flow channel heat transfer studies was also done. Mathematical methods to geometrically match the cross-sectional areas of the circle and star, along with a square and equilateral triangle, were derived. A Wolfram Mathematica 8 module was programmed to analyze CFD results using Richardson Extrapolation and calculate the grid convergence index (GCI). A Mathematica notebook, also composed, computes and graphs the bulk mean temperature along a flow channel’s length while the user dynam- ically provides the input variables, allowing their effects on the temperature to be more easily observed.

  7. Widespread Excess Ice in Arcadia Planitia, Mars

    E-Print Network [OSTI]

    Bramson, Ali M; Putzig, Nathaniel E; Sutton, Sarah; Plaut, Jeffrey J; Brothers, T Charles; Holt, John W

    2015-01-01

    The distribution of subsurface water ice on Mars is a key constraint on past climate, while the volumetric concentration of buried ice (pore-filling versus excess) provides information about the process that led to its deposition. We investigate the subsurface of Arcadia Planitia by measuring the depth of terraces in simple impact craters and mapping a widespread subsurface reflection in radar sounding data. Assuming that the contrast in material strengths responsible for the terracing is the same dielectric interface that causes the radar reflection, we can combine these data to estimate the dielectric constant of the overlying material. We compare these results to a three-component dielectric mixing model to constrain composition. Our results indicate a widespread, decameters-thick layer that is excess water ice ~10^4 km^3 in volume. The accumulation and long-term preservation of this ice is a challenge for current Martian climate models.

  8. Mixed convection and heat management in the Mars gravity biosatellite

    E-Print Network [OSTI]

    Marsh, Jesse B. (Jesse Benjamin)

    2007-01-01

    The Mars Gravity Biosatellite will house fifteen mice in a low Earth orbit satellite spinning about its longitudinal axis. The satellite's payload thermal control system will reject heat through the base of the payload ...

  9. Infrared Brightness Temperature of Mars, 1983-2103

    E-Print Network [OSTI]

    E. L. Wright

    2007-03-25

    The predicted infrared brightness temperature of Mars using the 1976 model of Wright is tabulated here for the period 1983 to 2103. This model was developed for far-infrared calibration, and is still being used for JCMT calibration.

  10. Geomorphometric analysis of Hebes Chasma, Mars, using the GRASS GIS. 

    E-Print Network [OSTI]

    Harrison, Samantha

    This research addressed the local scale geomorphometric analysis of the Hebes Chasma region on Mars, utilising a new 50 m/pixel digital terrain model derived from stereo imagery. A secondary aspect of the research addressed the role of GIS...

  11. Design of spacecraft for exploration of the Moon and Mars

    E-Print Network [OSTI]

    Epps, Brenden P

    2006-01-01

    In this thesis, I develop the conceptual design of the spacecraft required for human-Lunar and human-Mars exploration. The requirements for these vehicles are derived in the context of the NASA Concept Exploration & ...

  12. First phase beamlines at CLS PROPOSED & UNDER REVIEW (Mar 2001)

    E-Print Network [OSTI]

    Hitchcock, Adam P.

    First phase beamlines at CLS PROPOSED & UNDER REVIEW (Mar 2001) X-ray Emission Alex Moewes (U. Sask 27 June 2000 27 June 2000 27-Feb 2001 27-Feb 2001 27-Feb 2001 #12;

  13. Integrated navigation architecture analysis for Moon and Mars exploration

    E-Print Network [OSTI]

    Chabot, Thomas

    2005-01-01

    The new solar system exploration objectives announced in January 2004 have the goal of sending humans back to the Moon by the year 2020 in preparation for human exploration of Mars. Advanced, but cost effective, surface ...

  14. A Mars-back approach to lunar surface operations

    E-Print Network [OSTI]

    Kleinwaks, Howard Neil

    2005-01-01

    The Vision for Space Exploration initiated a new space exploration program and called for a long term national commitment to space exploration starting with a return to the Moon and continuing with the exploration of Mars ...

  15. SpiritMars Exploration Rovers National Aeronautics and

    E-Print Network [OSTI]

    Murdo" panorama, captured by the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit. From April, exposed bright underlying material. This bright material is evidence of sulfur-rich salty minerals

  16. Geophysical evolution of planetary interiors and surfaces : Moon & Mars

    E-Print Network [OSTI]

    Evans, Alexander Joseph

    2013-01-01

    The interiors and surfaces of the terrestrial planetary bodies provide us a unique opportunity to gain insight into planetary evolution, particularly in the early stages subsequent to accretion. Both Mars and the Moon are ...

  17. Testing the Early Mars H2-CO2 Greenhouse Hypothesis with a 1-D Photochemical Model

    E-Print Network [OSTI]

    Batalha, Natasha; Ramirez, Ramses; Kasting, James

    2015-01-01

    A recent study by Ramirez et al. (2014) demonstrated that an atmosphere with 1.3-4 bar of CO2 and H2O, in addition to 5-20% H2, could have raised the mean annual and global surface temperature of early Mars above the freezing point of water. Such warm temperatures appear necessary to generate the rainfall (or snowfall) amounts required to carve the ancient martian valleys. Here, we use our best estimates for early martian outgassing rates, along with a 1-D photochemical model, to assess the conversion efficiency of CO, CH4, and H2S to CO2, SO2, and H2. Our outgassing estimates assume that Mars was actively recycling volatiles between its crust and interior, as Earth does today. H2 production from serpentinization and deposition of banded iron-formations is also considered. Under these assumptions, maintaining an H2 concentration of ~1-2% by volume is achievable, but reaching 5% H2 requires additional H2 sources or a slowing of the hydrogen escape rate below the diffusion limit. If the early martian atmosphere...

  18. Propulsion engineering study for small-scale Mars missions

    SciTech Connect (OSTI)

    Whitehead, J.

    1995-09-12

    Rocket propulsion options for small-scale Mars missions are presented and compared, particularly for the terminal landing maneuver and for sample return. Mars landing has a low propulsive {Delta}v requirement on a {approximately}1-minute time scale, but at a high acceleration. High thrust/weight liquid rocket technologies, or advanced pulse-capable solids, developed during the past decade for missile defense, are therefore more appropriate for small Mars landers than are conventional space propulsion technologies. The advanced liquid systems are characterize by compact lightweight thrusters having high chamber pressures and short lifetimes. Blowdown or regulated pressure-fed operation can satisfy the Mars landing requirement, but hardware mass can be reduced by using pumps. Aggressive terminal landing propulsion designs can enable post-landing hop maneuvers for some surface mobility. The Mars sample return mission requires a small high performance launcher having either solid motors or miniature pump-fed engines. Terminal propulsion for 100 kg Mars landers is within the realm of flight-proven thruster designs, but custom tankage is desirable. Landers on a 10 kg scale also are feasible, using technology that has been demonstrated but not previously flown in space. The number of sources and the selection of components are extremely limited on this smallest scale, so some customized hardware is required. A key characteristic of kilogram-scale propulsion is that gas jets are much lighter than liquid thrusters for reaction control. The mass and volume of tanks for inert gas can be eliminated by systems which generate gas as needed from a liquid or a solid, but these have virtually no space flight history. Mars return propulsion is a major engineering challenge; earth launch is the only previously-solved propulsion problem requiring similar or greater performance.

  19. Economic Development Benefits of the Mars Hill Wind Farm, Wind Powering America Rural Economic Development, Case Study (Fact Sheet)

    SciTech Connect (OSTI)

    Not Available

    2009-06-01

    This case study summarizes the economic development benefits of the Mars Hill Wind Farm to the community of Mars Hill, Maine. The Mars Hill Wind Farm is New England's first utility-scale wind farm.

  20. FRN and Rate Schedules

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

    Doing Business Skip navigation links Financial Information Financial Public Processes Asset Management Cost Verification Process Rate Cases BP-16 Rate Case OS-14 Rate Case FRN...

  1. FRN & Rate Schedules

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

    Doing Business Skip navigation links Financial Information Financial Public Processes Asset Management Cost Verification Process Rate Cases BP-16 Rate Case OS-14 Rate Case FRN...

  2. A quantitative comparison of rates of phagocytosis and digestion of apoptotic cells by macrophages from normal

    E-Print Network [OSTI]

    Keshet, Leah

    A quantitative comparison of rates of phagocytosis and digestion of apoptotic cells by macrophages head: Phagocytosis and digestion by NOD mice macrophages Corresponding author: Leah Edelstein, thus quantifying kinetics of uptake and digestion of apoptotic cells in both mouse strains (Mar´ee et

  3. Chlorite Dissolution Rates

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

    Carroll, Susan

    2013-07-01

    Spreadsheets provides measured chlorite rate data from 100 to 300C at elevated CO2. Spreadsheet includes derived rate equation.

  4. Chlorite Dissolution Rates

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

    Carroll, Susan

    Spreadsheets provides measured chlorite rate data from 100 to 300C at elevated CO2. Spreadsheet includes derived rate equation.

  5. An Independent Assessment of the Technical Feasibility of the Mars One Mission Plan

    E-Print Network [OSTI]

    Do, Sydney

    In mid-2012, the Mars One program was announced, aiming to build the first human settlement on the surface of Mars. Following a series of precursor missions to develop and deploy key technologies, the first crewed mission ...

  6. The Asymmetric TimeVariable Rings of Mars Douglas P. Hamilton

    E-Print Network [OSTI]

    Hamilton, Douglas P.

    from along Mars' vernal equinox (the intersection between Mars' orbital and equatorial planes­fated Phobos­2 mission, noted that strong solar wind disturbances in the plasma and magnetic fields

  7. Preservation of Martian Organic and Environmental Records: Final Report of the Mars Biosignature Working Group

    E-Print Network [OSTI]

    Summons, Roger Everett

    The Mars Science Laboratory (MSL) has an instrument package capable of making measurements of past and present environmental conditions. The data generated may tell us if Mars is, or ever was, able to support life. However, ...

  8. Engine placement for manned descent at Mars considering single engine failures

    E-Print Network [OSTI]

    York, Stephen P. (Stephen Patrick)

    2006-01-01

    Previous missions to Mars have landed masses of approximately I metric ton on the surface. Vehicles large enough to support humans on the flight to Mars and land them safely on the surface are closer to 100 metric tons, a ...

  9. Amino acid biosignatures : implications for the detection of extinct or extant microbial communities on Mars

    E-Print Network [OSTI]

    Aubrey, Andrew D.

    2008-01-01

    colonization in impact- generated hydrothermal sulphate deposits, Haughton impact structure, and implications for sulphates on Mars.colonization in impact- generated hydrothermal sulphate deposits, Haughton impact structure, and implications for sulphates on Mars.

  10. Amino Acid Biosignatures - Implications for the Detection of Extinct or Extant Microbial Communities on Mars

    E-Print Network [OSTI]

    Aubrey, Andrew D

    2008-01-01

    colonization in impact- generated hydrothermal sulphate deposits, Haughton impact structure, and implications for sulphates on Mars.colonization in impact- generated hydrothermal sulphate deposits, Haughton impact structure, and implications for sulphates on Mars.

  11. North polar stratigraphy and the paleo-erg of Mars Shane Byrne and Bruce C. Murray

    E-Print Network [OSTI]

    Byrne, Shane

    North polar stratigraphy and the paleo-erg of Mars Shane Byrne and Bruce C. Murray Division: Surface materials and properties; KEYWORDS: Mars, polar, geology, history, stratigraphy, dune 1

  12. Space weather effects on the Mars ionosphere due to solar flares and meteors

    E-Print Network [OSTI]

    Withers, Paul

    Space weather effects on the Mars ionosphere due to solar flares and meteors P. Withers (1), M observed two aspects of space weather at Mars. Following solar flares of both moderate to strong magnitude

  13. Gone with the Wind ON_Mars (GOWON): A Wind-Driven Networked System of Mobile Sensors on Mars

    E-Print Network [OSTI]

    Davoodi, Faranak; Murphy, Neil; Mischna, Michael; Nesnas, Issa; Nikzad, Shouleh

    2012-01-01

    We propose a revolutionary way of studying the surface of Mars using a wind-driven network of mobile sensors- Gone with the Wind ON_Mars (GOWON). GOWON is a scalable architecture that will allow in-situ mapping of a wide range of phenomena, exploiting existing capabilities, but radically improving our ability to study Mars. GOWON has the following characteristics: 1.it consists of a dynamic wireless network of many compact mobile sensors. 2.the mobile sensors (called moballs) are spherically-shaped and wind-driven; they are lightweight and bouncy. 3. moballs communicate with each other and earth through a satellite system orbiting Mars. There is also peer-to-peer communication between the moballs, creating a network of shared data, computing, and tasks. Motivation and Rationale Thanks to earlier exploration missions to Mars we now have a much better understanding of many of the natural characteristics of the red planet. We now know that there is an abundance of wind (with average speeds of 10 m/s and much hig...

  14. Chemical study of secondary metabolites from selected strains of the actinomycete clade MAR 4

    E-Print Network [OSTI]

    Espindola, Ana Paula Domingues de Mello

    2008-01-01

    pathways present in all member of the group makes the MAR 4 group unusual among both marine and terrestrial

  15. Mirror Advanced Reactor Study (MARS): executive summary and overview

    SciTech Connect (OSTI)

    Logan, B.G.; Perkins, L.J.; Gordon, J.D.

    1984-07-01

    Two self-consistent MARS configurations are discussed - a 1200-MWe commercial electricity-generating plant and a synguels-generating plant that produces hydrogen with an energy equivalent to 26,000 barrels of oil per day. The MARS machine emphasizes the attractive features of the tandem mirror concept, including steady-state operation, a small-diameter high-beta plasma, a linear central cell with simple low-maintenance blankets, low first-wall heat fluxes (<10 W/cm/sup 2/), no driven plasma currents or associated disruptions, natural halo impurity diversion, and direct conversion of end-loss charged-particle power. The MARS electric plant produces 2600 MW of fusion power in a 130-m-long central cell. Advanced tandem-mirror plasma-engineering concepts, a high-efficiency liquid lithium-lead (Li/sub 17/Pb/sub 83/) blanket, and efficient direct electrical conversion of end loss power combine to produce a high net plant efficiency of 36%. With a total capital cost of $2.9 billion (constant 1983 dollars), the MARS electric plant produces busbar electricity at approx. 7 cents/kW-hour. The MARS synfuels plant produces 3500 MW of fusion power in a 150-m-long central cell. A helium-gas-cooled silicon carbide pebble-bed blanket provides high-temperature (1000/sup 0/C) heat to a thermochemical water-splitting cycle and the resulting hydrogen is catalytically converted to methanol for distribution. With a total capital cost of $3.6 billion (constant 1983 dollars), the synfuels plant produces methanol fuel at about $1.7/gal. The major features of the MARS reactor include sloshing-ion thermal barrier plugs for efficient plasma confinement, a high efficiency blanket, high-field (24-T) choke cells, drift pumping for trapped plasma species, quasi-optical electron-cyclotron resonant heating (ECRH) systems, and a component gridless direct converter.

  16. A nonsteady one-dimensional theoretical model of Mars' neutral atmospheric composition between 30 and 200 km

    SciTech Connect (OSTI)

    Rodrigo, R.; Garcia-Alvarez, E.; Lopez-Gonzalez, M.J.; Lopez-Moreno, J.J. (Instituto de Astrofisica de Andalucia, Granada (Spain))

    1990-08-30

    There has been a big advance in the knowledge of the composition of the atmosphere of the planet Mars since its exploration by different missions in the 1970s, and this will be deeply increased in the following years as the upcoming programs to Mars develop. In this context, the authors have elaborated a model of the Mars' neutral atmosphere including the following compounds: O({sup 3}P), O({sup 1}D), O{sub 2}, O{sub 3}, H, H{sub 2}, OH, H{sub 2}O, HO{sub 2}, H{sub 2}O{sub 2}, CO, and CO{sub 2}, between 30 and 200 km of altitude. The model is carried out for middle latitudes in equinox conditions and with moderate solar activity and provides the day-to-night evolution of the atmosphere. The scarcity of observations corresponding to the nightside of the planet has made it necessary to calculate the atmospheric temperature profile based on the available observations and on theoretical estimations. The model includes a detailed treatment of both the photochemical and the dynamical processes. In this sense, the most recent values of the reaction rates and photodissociation cross sections have been used, and a new height profile of the eddy diffusion coefficient has been computed which is able to explain the vertical distribution of carbon monoxide. The concentration profiles obtained show, in general, a very good agreement with the available experimental measurements.

  17. The radiation stability of glycine in solid CO2 - in situ laboratory measurements with applications to Mars

    E-Print Network [OSTI]

    Gerakines, P A

    2015-01-01

    The detection of biologically important, organic molecules on Mars is an important goal that may soon be reached. However, the current small number of organic detections at the Martian surface may be due to the harsh UV and radiation conditions there. It seems likely that a successful search will require probing the subsurface of Mars, where penetrating cosmic rays and Solar energetic particles dominate the radiation environment, with an influence that weakens with depth. Toward the goal of understanding the survival of organic molecules in cold radiation-rich environments on Mars, we present new kinetics data on the radiolytic destruction of glycine diluted in frozen carbon dioxide. Rate constants were measured in situ with infrared spectroscopy, without additional sample manipulation, for irradiations at 25, 50, and 75 K with 0.8-MeV protons. The resulting half-lives for glycine in CO2-ice are compared to previous results for glycine in H2O-ice and show that glycine in CO2-ice is much less stable in a radia...

  18. Mars Rover's ChemCam Instrument gets sharper vision

    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 would likeUniverseIMPACTThousandReport)PriceHistoricEnergyApril 25,4MarioMarkMarsMars Rover's

  19. Mars Science Laboratory on Saturday, Los Alamos National Laboratory researchers

    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 would likeUniverseIMPACTThousandReport)PriceHistoricEnergyApril 25,4MarioMarkMarsMars

  20. Thursday, March 26, 2009 POSTER SESSION II: MARS: DUNES, DUST, AND WIND

    E-Print Network [OSTI]

    Rathbun, Julie A.

    mainly from the experimental work are presented. Segura T. L. Colaprete A. Global Modeling of Impact-induced Greenhouse Warming on Early Mars [#1056] We have modeled the climate effects of impacts on early Mars. Aeolian Dunes as Ground Truth for GCM and Mesoscale Modeling on Mars [#1212] Aeolian dunes preserve

  1. Assessment of architectural options for surface power generation and energy storage on human Mars missions

    E-Print Network [OSTI]

    de Weck, Olivier L.

    Assessment of architectural options for surface power generation and energy storage on human Mars power Nuclear Solar power Architectures a b s t r a c t The provision of power for human Mars surface analysis of surface power generation and energy storage architectures for human Mars surface missions

  2. Localized gravity/topography admittance and correlation spectra on Mars: Implications for

    E-Print Network [OSTI]

    Simons, Mark

    Localized gravity/topography admittance and correlation spectra on Mars: Implications for regional] From gravity and topography data collected by the Mars Global Surveyor spacecraft we calculate gravity/topography of an elastic/plastic shell. In regions of high topography on Mars (e.g., the Tharsis rise and associated shield

  3. 23 mars 2015CNRS I INSIS I Muriel Ilous La communication

    E-Print Network [OSTI]

    van Tiggelen, Bart

    23 mars 2015CNRS I INSIS I Muriel Ilous La communication à l'INSIS 1 #12;23 mars 2015CNRS I INSIS I Muriel Ilous Muriel Ilous, responsable communication Valérie Pierre, chargée de la communication workshops 2 Le service communication de l'INSIS #12;23 mars 2015CNRS I INSIS I Muriel Ilous La Direction de

  4. TTF/VUV-FEL meeting, 21. Mar 06 SaseFelPhotonDiagnostics

    E-Print Network [OSTI]

    TTF/VUV-FEL meeting, 21. Mar 06 SaseFelPhotonDiagnostics Gas Monitor Detector Electronics from charged particles to digital value Fini Jastrow, TTF/VUV-FEL meeting, 21. Mar 06 #12;TTF/VUV-FEL meeting, 21. Mar 06 SaseFelPhotonDiagnostics The Detector Ion Current Measurement Electron Pulse Measurement

  5. Surface runoff features on Mars: Testing the carbon dioxide formation hypothesis

    E-Print Network [OSTI]

    Nimmo, Francis

    materials and properties; KEYWORDS: Mars, gullies, seepage, runoff, carbon dioxide, water Citation: StewartSurface runoff features on Mars: Testing the carbon dioxide formation hypothesis Sarah T. Stewart1, S. T., and F. Nimmo, Surface runoff features on Mars: Testing the carbon dioxide formation

  6. Results from the Mars Phoenix Lander Robotic Arm experiment R. E. Arvidson,1

    E-Print Network [OSTI]

    Volpe, Richard

    Results from the Mars Phoenix Lander Robotic Arm experiment R. E. Arvidson,1 R. G. Bonitz,2 M. L; revised 8 June 2009; accepted 24 June 2009; published 2 October 2009. [1] The Mars Phoenix Lander. (2009), Results from the Mars Phoenix Lander Robotic Arm experiment, J. Geophys. Res., 114, E00E02, doi

  7. The MECA Wet Chemistry Laboratory on the 2007 Phoenix Mars Scout Lander

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    The MECA Wet Chemistry Laboratory on the 2007 Phoenix Mars Scout Lander Samuel P. Kounaves,1] To analyze and interpret the chemical record, the 2007 Phoenix Mars Lander includes four wet chemistry cells on the 2007 Phoenix Mars Scout Lander, J. Geophys. Res., 114, E00A19, doi:10.1029/2008JE003084. 1

  8. Localized precipitation and runoff on Mars Edwin S. Kite,1,2

    E-Print Network [OSTI]

    Localized precipitation and runoff on Mars Edwin S. Kite,1,2 Timothy I. Michaels,3 Scot Rafkin,3) to simulate lake storms on Mars, finding that intense localized precipitation will occur for lake size 103 km2 on Mars involve continuous precipitation, and their vertical velocities and plume heights exceed those

  9. The Mars Hopper: a radioisotope powered, impulse driven, long-range, long-lived mobile platform for exploration of Mars

    SciTech Connect (OSTI)

    Steven D. Howe; Robert C. O'Brien; William Taitano; Doug Crawford; Nathan Jerred; Spencer Cooley; John Crapeau; Steve Hansen; Andrew Klein; James Werner

    2011-02-01

    Planetary exploration mission requirements are becoming more demanding. Due to the increasing cost, the missions that provide mobile platforms that can acquire data at multiple locations are becoming more attractive. Wheeled vehicles such as the MER rovers have proven extremely capable but have very limited range and cannot traverse rugged terrain. Flying vehicles such as balloons and airplanes have been proposed but are problematic due to the very thin atmospheric pressure and the strong, dusty winds present on Mars. The Center for Space Nuclear Research has designed an instrumented platform that can acquire detailed data at hundreds of locations during its lifetime - a Mars Hopper. The Mars Hopper concept utilizes energy from radioisotopic decay in a manner different from any existing radioisotopic power sources—as a thermal capacitor. By accumulating the heat from radioisotopic decay for long periods, the power of the source can be dramatically increased for short periods. The platform will be able to "hop" from one location to the next every 5-7 days with a separation of 5-10 km per hop. Preliminary designs show a platform that weighs around 52 kgs unfueled which is the condition at deployment. Consequently, several platforms may be deployed on a single launch from Earth. With sufficient lifetime, the entire surface of Mars can be mapped in detail by a couple dozen platforms. In addition, Hoppers can collect samples from all over the planet, including gorges, mountains and crevasses, and deliver them to a central location for eventual pick-up by a Mars Sample Return mission. The status of the Mars Hopper development project at the CSNR is discussed.

  10. Strategies for autonomous rovers at Mars Martha S. Gilmore1

    E-Print Network [OSTI]

    Mjolsness, Eric

    , characterize the landing site and test geological hypothesis autonomously. Future missions to Mars will contain history, 3) the identification of resources and 4) the geological and geophysical history of the planet is the characterize the selected sites in detail using lander and mobile systems as is planned for the 2003

  11. Voyage de presse 26 et 27 mars 2015 -Lyon

    E-Print Network [OSTI]

    van Tiggelen, Bart

    Voyage de presse 26 et 27 mars 2015 - Lyon DOSSIER DE PRESSE Année internationale de la lumière nanotechnologies de Lyon 5 > Nanophotonique > Photovoltaïque Photosynthèse, micro-algues et biocarburants 9 L'Institut de recherches sur la catalyse et l'environnement de Lyon 10 > Photochimie atmosphérique L

  12. Wednesday, March 14, 2007 MARS TECTONICS AND CRUSTAL DICHOTOMY

    E-Print Network [OSTI]

    Rathbun, Julie A.

    . * Murray J. B. van Wyk de Vries B. Troll V. R. Flank Terrace Architecture of Martian Shield Volcanoes and regional stresses can influence terrace architecture. 10:00 a.m. Searls M. L. * Phillips R. J. Tectonics of Utopia Basin, Mars: Results from Finite Element Loading Models [#1965] We use a finite element model

  13. Periodic bedrock ridges on Mars David R. Montgomery,1

    E-Print Network [OSTI]

    Montgomery, David R.

    Periodic bedrock ridges on Mars David R. Montgomery,1 Joshua L. Bandfield,1 and Scott K. Becker1 to be widespread [Carr, 1981; Greeley et al., 1992; Malin and Edgett, 2001]. Although wind-streamlined yardangs interpreted as sedimentary forms [McCauley et al., 1972; Cutts and Smith, 1973; Carr, 1981; Greeley et al

  14. NASA/TP--2006214196 Haughton-Mars Project Expedition 2005

    E-Print Network [OSTI]

    de Weck, Olivier L.

    NASA/TP--2006­214196 Haughton-Mars Project Expedition 2005 Final Report Prof. Olivier de Weck: Press F1 key (Windows) or Help key (Mac) for help January 2006 #12;NASA STI Program ... in Profile Since its founding, NASA has been dedicated to the advancement of aeronautics and space science. The NASA

  15. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Sponaugle, Su

    of 28.5°C) or the interference of mesoscale advection processes. When 4 cohorts that settled during the passage of mesoscale eddies were omitted from the analysis, 61% of the varia- tion in recruitment due to mesoscale oceanographic circulation. Photos: Evan D'Alessandro OPENPEN ACCESSCCESS #12;Mar Ecol

  16. Mar./Apr. 2002 Winter Losses, Again Organic Beekeeping Conf.

    E-Print Network [OSTI]

    Ishida, Yuko

    Mar./Apr. 2002 Winter Losses, Again Organic Beekeeping Conf. Diagnosing and Treating Nosema is extremely hard to see, because the bees look OK while the stored food reserves in their bodies just aren of the honey bee midgut stimulate germination. The organism penetrates a midgut cell and grows by absorbing

  17. Friday, March 27, 2009 MARS: DUNES, DUST, AND WIND

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Friday, March 27, 2009 MARS: DUNES, DUST, AND WIND 8:30 a.m. Waterway Ballroom 1 Chairs: Lori Fenton Steve Metzger 8:30 a.m. Chojnacki M. * Moersch J. E. Valles Marineris Dune Fields: Thermophysical Properties, Morphology, and Provenance [#2486] We examined 25 dune fields in Valles Marineris to identify

  18. Mars Exploration Rover Mobility and Robotic Arm Operational Performance

    E-Print Network [OSTI]

    Mars Exploration Rover Mobility and Robotic Arm Operational Performance Edward Tunstel, Mark California Institute of Technology Pasadena, CA, 91109 USA tunstel@robotics.jpl.nasa.gov Abstract - Increased they should operate. The purpose of this paper is to describe an actual instance of a practical human-robot

  19. Science Results from the Mars Exploration Rover Mission

    ScienceCinema (OSTI)

    Squyres, Steven [Cornell University, Ithaca, New York, United States

    2010-09-01

    One of the most important scientific goals of the mission was to find and identify a variety of rocks and soils that provide evidence of the past presence of water on the planet. To obtain this information, Squyres is studying the data obtained on Mars by several sophisticated scientific instruments.

  20. DU 27 AU 29 MARS SYMPOSIUM Innovation for the management

    E-Print Network [OSTI]

    Jeanjean, Louis

    DU 27 AU 29 MARS SYMPOSIUM Innovation for the management of echinococcosis-2014 (ImE-2014) Nouveaux hospitalier universitaire de Besançon) ; Centre national de référence échinococcose alvéolaire, Centre hospitalier régional universitaire de Besançon LIEU Chambre de commerce et d'industrie du Doubs, 46 avenue

  1. VOL. 35, NO. 1 SOUTHWESTERN ENTOMOLOGIST MAR. 2009 SCIENTIFIC NOTE

    E-Print Network [OSTI]

    Tomberlin, Jeff

    VOL. 35, NO. 1 SOUTHWESTERN ENTOMOLOGIST MAR. 2009 SCIENTIFIC NOTE Observations on the Oriental and is restricted to the southern U.S. We observed the arrival and colonization of blow flies on a decaying domestic to colonize decomposing remains in the U.S. (Byrd and Butler 1996). The first flies attracted to the chickens

  2. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Koehl, Mimi

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 479: 47­62, 2013 doi: 10.3354/meps10193 larvae, which are trans- ported by ambient currents and colonize new sur- faces. The recruitment. 1994, Schiel 2004, Edwards & Stachowicz 2011). To colonize a surface, a larva must be transported

  3. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Pawlik, Joseph

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 224: 103­114, 2001 Published December 19 process: solitary larvae first colonize a suitable but previously uninhabited sub- stratum; gregarious the conditions under which larvae of a gregarious species colonize new habitats. We first confirmed

  4. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Pawlik, Joseph

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 224: 115­131, 2001 Published December 19 substrata. Previous investigations with barnacles and polychaetes have suggested that the colonization for the initiation of monospecific aggregations of fouling marine invertebrates. KEY WORDS: Colonization · Gregarious

  5. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Pawlik, Joseph

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Published November 2 Defenses of Caribbean sponges.Pawlik* Biological Sciences and Center for Marine Science Research. University of North Carolina at Wilmington. Analyses of ash content, tensile strength, protein, carbohydrate, and lipid content, and total energy

  6. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 382: 211­219, 2009 doi: 10.3354/meps07997 Published April 30 INTRODUCTION Seabirds play critical roles in the transfer of energy and nutrients within marine ecosystems and also between marine and terrestrial ecosystems. Despite decades of intensive study

  7. Radio tracking of Phoenix during its landing on Mars

    E-Print Network [OSTI]

    Withers, Paul

    Radio tracking of Phoenix during its landing on Mars Paul Withers Center for Space Physics, Boston University (withers@bu.edu) MEX/VEX Radio Science Meeting 2010.03.18-19 Bonn, Germany #12;Phoenix atmospheric for a-aero using known quantities Re-arrange: #12;Next steps · Find f(t) for Phoenix direct

  8. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Thomas, David D.

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 311: 273­283, 2006 Published April 13 scales in biodiversity-based research: challenges and solutions for marine systems Shahid Naeem York, New York 10027, USA ABSTRACT: As in terrestrial biodiversity, human influences over marine

  9. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Queensland, University of

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 295: 201­213, 2005 Published June 23 INTRODUCTION Due to the ongoing direct depletion of the world's marine resources as well as the indirect effects of fish- ing, no-take marine reserves are being promoted as an ecosystem-level management tool. No

  10. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Camassa, Roberto

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 487: 185­200, 2013 doi: 10.3354/meps10387 Published July 30 INTRODUCTION Marine snow plays a critical role in the marine car- bon cycle, as a dominant, Kiørboe 2011). Knowledge of the vertical distribution of marine aggregates in the water column, as well

  11. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Morel, François M. M.

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 236: 37­43, 2002 Published July 3 the CO2 responses of marine phytoplankton despite the established importance of these organisms poten- tially limit the growth of large marine diatoms (Riebe- sell et al. 1993), while recent field

  12. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Rolán-Alvarez, Emilio

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 357: 175­184, 2008 doi: 10.3354/meps07278 will affect only some regions of the genome. An additional difficulty in the marine environment variation in the marine environment remains insufficiently understood (Avise 2004). Natural populations

  13. MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser

    E-Print Network [OSTI]

    Queensland, University of

    MARINE ECOLOGY PROGRESS SERIES Mar Ecol Prog Ser Vol. 253: 25­38, 2003 Published May 15 INTRODUCTION Marine protected areas are riding the wave of ocean governance reform (Kelleher 1997, Allison et component for the ecologically sustainable use of marine resources. Where such reform processes are grounded

  14. 2004 Rate Adjustments

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

    for Transmission and Ancillary Services Federal Register Notice -- Rate Order WAPA-141: Notice of Extension of Formula Rates for Transmission and Ancillary Services If you have any...

  15. Rate Schedule CPP-2

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

    points established by contract, in accordance with approved policies and procedures. Formula Rate: The formula rate for CPP includes three components: Component 1: The customer...

  16. Our Sun. V. A Bright Young Sun Consistent with Helioseismology and Warm Temperatures on Ancient Earth and Mars

    E-Print Network [OSTI]

    I. -Juliana Sackmann; Arnold I. Boothroyd

    2002-10-05

    The relatively warm temperatures required on early Earth and Mars have been difficult to account for via warming from greenhouse gases. We tested whether this problem can be resolved for both Earth and Mars by a young Sun that is brighter than predicted by the standard solar model. We computed high-precision solar evolutionary models with slightly increased initial masses of M_i = 1.01 to 1.07 M_sun; for each mass, we considered three different mass loss scenarios. We then tested whether these models were consistent with the current high-precision helioseismic observations. The relatively modest mass loss rates in these models are consistent with observational limits from young stars and estimates of the past solar wind obtained from lunar rocks, and do not significantly affect the solar lithium depletion. For appropriate initial masses, all three mass loss scenarios are capable of yielding a solar flux 3.8 Gyr ago high enough to be consistent with water on ancient Mars. We find that all of our mass-losing solar models are consistent with the helioseismic observations. The early solar mass loss of a few percent does indeed leave a small fingerprint on the Sun's internal structure. However, for helioseismology to significantly constrain early solar mass loss would require higher accuracy in the observed solar parameters and input physics, namely, by a factor of about 3 for the observed solar surface composition, and a factor of 2 for the solar interior opacities, the pp nuclear reaction rate, and the diffusion constants for gravitational settling.

  17. Extension of the quantum-kinetic model to lunar and Mars return physics

    SciTech Connect (OSTI)

    Liechty, D. S.; Lewis, M. J.

    2014-02-15

    The ability to compute rarefied, ionized hypersonic flows is becoming more important as missions such as Earth reentry, landing high-mass payloads on Mars, and the exploration of the outer planets and their satellites are being considered. A recently introduced molecular-level chemistry model, the quantum-kinetic, or Q-K, model that predicts reaction rates for gases in thermal equilibrium and non-equilibrium using only kinetic theory and fundamental molecular properties, is extended in the current work to include electronic energy level transitions and reactions involving charged particles. Like the Q-K procedures for neutral species chemical reactions, these new models are phenomenological procedures that aim to reproduce the reaction/transition rates but do not necessarily capture the exact physics. These engineering models are necessarily efficient due to the requirement to compute billions of simulated collisions in direct simulation Monte Carlo (DSMC) simulations. The new models are shown to generally agree within the spread of reported transition and reaction rates from the literature for near equilibrium conditions.

  18. Piloted Mars mission planning: NEP technology and power levels

    SciTech Connect (OSTI)

    George, J.A.; Hack, K.J.; Dudzinski, L.A.; Gefert, L.P. (NASA Lewis Research Center, 21000 Brookpark Rd., M.S. AAC-2, Cleveland, Ohio 44135 (United States)); Gilland, J.H. (Sverdrup Technology, Inc., NASA Lewis Research Center, 21000 Brookpark Rd., M.S. AAC-2, Cleveland, Ohio 44135 (United States))

    1993-01-10

    This paper examines the strong interrelationship between assumed technology and mission performance requirements for NEP. Recent systems analysis efforts by NASA, DOE, and various contractors are used to project achievable system performance as a function of technological sophistication for two piloted Mars mission applications. Specific mass regimes for each collection of technologies are presented as a function of power level for piloted applications. Low thrust mission analyses are presented which relate these system performance projections to achievable mission performance. Mission performance maps'' are constructed which link prime mission figures-of-merit of time and initial mass with system requirements on power level and specific mass, and hence technology. Both opposition and conjunction class piloted Mars missions are presented for the 2016 opportunity, analogous to those proposed in the 90-Day Study'' and Synthesis'' architecture studies. Mass and time breakdowns are presented for 10 MWe piloted and 5 MWe cargo point designs.

  19. Reducing the risk to Mars: The gas core nuclear rocket

    SciTech Connect (OSTI)

    Howe, S.D.; DeVolder, B.; Thode, L.; Zerkle, D.

    1998-12-31

    The next giant leap for mankind will be the human exploration of Mars. Almost certainly within the next thirty years, a human crew will brave the isolation, the radiation, and the lack of gravity to walk on and explore the Red planet. However, because the mission distances and duration will be hundreds of times greater than the lunar missions, a human crew will face much greater obstacles and a higher risk than those experienced during the Apollo program. A single solution to many of these obstacles is to dramatically decrease the mission duration by developing a high performance propulsion system. The gas-core nuclear rocket (GCNR) has the potential to be such a system. The authors have completed a comparative study of the potential impact that a GCNR could have on a manned Mars mission. The total IMLEO, transit times, and accumulated radiation dose to the crew will be compared with the NASA Design Reference Missions.

  20. Nuclear Design of the HOMER-15 Mars Surface Fission Reactor

    SciTech Connect (OSTI)

    Poston, David I.

    2002-07-01

    The next generation of robotic missions to Mars will most likely require robust power sources in the range of 3 to 20 kWe. Fission systems are well suited to provide safe, reliable, and economic power within this range. The goal of this study is to design a compact, low-mass fission system that meets Mars surface power requirements, while maintaining a high level of safety and reliability at a relatively low cost. The Heat pipe Power System (HPS) is one possible approach for producing near-term, low-cost, space fission power. The goal of the HPS project is to devise an attractive space fission system that can be developed quickly and affordably. The primary ways of doing this are by using existing technology and by designing the system for inexpensive testing. If the system can be designed to allow highly prototypic testing with electrical heating, then an exhaustive test program can be carried out quickly and inexpensively, and thorough testing of the actual flight unit can be performed - which is a major benefit to reliability. Over the past 4 years, three small HPS proof-of-concept technology demonstrations have been conducted, and each has been highly successful. The Heat pipe-Operated Mars Exploration Reactor (HOMER) is a derivative of the HPS designed especially for producing power on the surface of Mars. The HOMER-15 is a 15-kWt reactor that couples with a 3-kWe Stirling engine power system. The reactor contains stainless-steel (SS)-clad uranium nitride (UN) fuel pins that are structurally and thermally bonded to SS/sodium heat pipes. Fission energy is conducted from the fuel pins to the heat pipes, which then carry the heat to the Stirling engine. This paper describes conceptual design and nuclear performance the HOMER-15 reactor. (author)

  1. ChemCam Rock Laser for the Mars Science Laboratory

    ScienceCinema (OSTI)

    LANL

    2009-09-01

    Los Alamos has a long history of space-related instr... Los Alamos has a long history of space-related instruments, tied primarily to its role in defense-related treaty verification. Space-based detectors have helped determine the differences between signals from lightning bolts and potential nuclear explosions. LANL-developed gamma-ray detection instruments first revealed the existence of what we now know as gamma-ray bursts, an exciting area of astrophysical research. And the use of LANL instruments on varied space missions continues with such products as the ChemCam rock laser for NASA, shown here. The Engineering Model of the ChemCam Mars Science Laboratory rover instrument arrived at NASA's Jet Propulsion Laboratory on February 6, 2008. ChemCam will use imaging and laser-induced breakdown spectroscopy (LIBS) to determine rock and soil compositions on Mars, up to 9 meters from the rover. The engineering model is being integrated into the rover test bed for the development and testing of the rover software. The actual flight model components are concurrently being assembled at Los Alamos and in Toulouse, France, and will be delivered to JPL in July. The Mars Science Laboratory is scheduled to launch in 2009. Animations courtesy of JPL/NASA.

  2. ChemCam rock laser for Mars Science Laboratory "Curiosity"

    ScienceCinema (OSTI)

    Wiens, Roger

    2014-08-12

    Los Alamos has a long history of space-related instruments, tied primarily to its role in defense-related treaty verification. Space-based detectors have helped determine the differences between signals from lightning bolts and potential nuclear explosions. LANL-developed gamma-ray detection instruments first revealed the existence of what we now know as gamma-ray bursts, an exciting area of astrophysical research. And the use of LANL instruments on varied space missions continues with such products as the ChemCam rock laser for NASA, shown here. The Engineering Model of the ChemCam Mars Science Laboratory rover instrument arrived at NASA's Jet Propulsion Laboratory on February 6, 2008. The Flight Model was shipped in August, 2010 for installation on the rover at JPL. ChemCam will use imaging and laser-induced breakdown spectroscopy (LIBS) to determine rock and soil compositions on Mars, up to 9 meters from the rover. The engineering model is being integrated into the rover test bed for the development and testing of the rover software. The actual flight model components were concurrently assembled at Los Alamos and in Toulouse, France. The Mars Science Laboratory is scheduled to launch in 2011. Animations courtesy of JPL/NASA.

  3. Lesson 22 Related Rates

    E-Print Network [OSTI]

    2013-10-11

    Oct 11, 2013 ... A spherical weather balloon is being inflated with helium at a rate of 82 cubic meters per minute. Find the rate at which its radius is increasing.

  4. Naughton's related rates problems

    E-Print Network [OSTI]

    dominic

    2013-02-25

    Related rates (1). (1) Oil spills from a rupture container in a circular pattern whose radius increases at a rate of 2 ft/s. How fast is the area of the oil spill increasing ...

  5. DEVELOPMENT AND DEPLOYMENT OF THE MOBILE ARM RETRIEVAL SYSTEM (MARS) - 12187

    SciTech Connect (OSTI)

    BURKE CA; LANDON MR; HANSON CE

    2011-11-08

    Washington River Protection Solutions (WRPS) is developing and deploying Mobile Arm Retrieval System (MARS) technologies solutions to support retrieval of radioactive and chemical waste from underground single shell storage tanks (SST) located at the Hanford Site, which is near Richland, Washington. WRPS has developed the MARS using a standardized platform that is capable of deploying multiple retrieval technologies. To date, WRPS, working with their mentor-protege company, Columbia Energy and Environmental Services (CEES), has developed two retrieval mechanisms, MARS-Sluicing (MARS-S) and MARS-Vacuum (MARS-V). MARS-S uses pressurized fluids routed through spray nozzles to mobilize waste materials to a centrally located slurry pump (deployed in 2011). MARS-V uses pressurized fluids routed through an eductor nozzle. The eductor nozzle allows a vacuum to be drawn on the waste materials. The vacuum allows the waste materials to be moved to an in-tank vessel, then extracted from the SST and subsequently pumped to newer and safer double shell tanks (DST) for storage until the waste is treated for disposal. The MARS-S system is targeted for sound SSTs (i.e., non leaking tanks). The MARS-V is targeted for assumed leaking tanks or those tanks that are of questionable integrity. Both versions of MARS are beinglhave been developed in compliance with WRPS's TFC-PLN-90, Technology Development Management Plan [1]. TFC-PLN-90 includes a phased approach to design, testing, and ultimate deployment of new technologies. The MARS-V is scheduled to be deployed in tank 241-C-105 in late 2012.

  6. DEVELOPMENT AND DEPLOYMENT OF THE MOBILE ARM RETRIEVAL SYSTEM (MARS) - 12187

    SciTech Connect (OSTI)

    BURKE CA; LANDON MR; HANSON CE

    2012-01-30

    Washington River Protection Solutions (WRPS) is developing and deploying Mobile Arm Retrieval System (MARS) technologies solutions to support retrieval of radioactive and chemical waste from underground single shell storage tanks (SST) located at the Hanford Site, which is near Richland, Washington. WRPS has developed the MARS using a standardized platform that is capable of deploying multiple retrieval technologies. To date, WRPS, working with their mentor-protege company, Columbia Energy and Environmental Services (CEES), has developed two retrieval mechanisms, MARS-Sluicing (MARS-S) and MARS-Vacuum (MARS-V). MARS-S uses pressurized fluids routed through spray nozzles to mobilize waste materials to a centrally located slurry pump (deployed in 2011). MARS-V uses pressurized fluids routed through an eductor nozzle. The eductor nozzle allows a vacuum to be drawn on the waste materials. The vacuum allows the waste materials to be moved to an in-tank vessel, then extracted from the SST and subsequently pumped to newer and safer double shell tanks (DST) for storage until the waste is treated for disposal. The MARS-S system is targeted for sound SSTs (i.e., non leaking tanks). The MARS-V is targeted for assumed leaking tanks or those tanks that are of questionable integrity. Both versions of MARS are being/have been developed in compliance with WRPS's TFC-PLN-90, Technology Development Management Plan. TFC-PLN-90 includes a phased approach to design, testing, and ultimate deployment of new technologies. The MARS-V is scheduled to be deployed in tank 241-C-105 in late 2012.

  7. Development and Deployment of the Mobile Arm Retrieval System (MARS) - 12187

    SciTech Connect (OSTI)

    Burke, Christopher A.; Landon, Matthew R. [Washington River Protection Solutions, Richland, Washington 99352 (United States); Hanson, Carl E. [AREVA Federal Services, Richland, Washington 99352 (United States)

    2012-07-01

    Washington River Protection Solutions (WRPS) is developing and deploying Mobile Arm Retrieval System (MARS) technologies solutions to support retrieval of radioactive and chemical waste from underground single shell storage tanks (SST) located at the Hanford Site, which is near Richland, Washington. WRPS has developed the MARS using a standardized platform that is capable of deploying multiple retrieval technologies. To date, WRPS, working with their mentor-protege company, Columbia Energy and Environmental Services (CEES), has developed two retrieval mechanisms, MARS-Sluicing (MARS-S) and MARS-Vacuum (MARS-V). MARS-S uses pressurized fluids routed through spray nozzles to mobilize waste materials to a centrally located slurry pump (deployed in 2011). MARS-V uses pressurized fluids routed through an eductor nozzle. The eductor nozzle allows a vacuum to be drawn on the waste materials. The vacuum allows the waste materials to be moved to an in-tank vessel, then extracted from the SST and subsequently pumped to newer and safer double shell tanks (DST) for storage until the waste is treated for disposal. The MARS-S system is targeted for sound SSTs (i.e., non leaking tanks). The MARS-V is targeted for assumed leaking tanks or those tanks that are of questionable integrity. Both versions of MARS are being/have been developed in compliance with WRPS's TFC-PLN-90, Technology Development Management Plan [1]. TFC-PLN-90 includes a phased approach to design, testing, and ultimate deployment of new technologies. The MARS-V is scheduled to be deployed in tank 241-C-105 in late 2012. (authors)

  8. Fluid Core Size of Mars from Detection of the Solar Tide

    E-Print Network [OSTI]

    Manga, Michael

    Lovenumber,hasbeen obtained from an analysis of Mars Global Surveyor radio tracking. The observed k2 of 0.153 0.017 is large) tracking data, Smith et al. (5, 6) reported a solution for the tidal Love number k2 of 0.055 0.008, which deformation of the figure of Mars by the gravitational pull of the Sun and hence a less rigid Mars (7). We

  9. Analysis of organic molecules using the Mars Organic Analyzer, a portable, automated microfabricated capillary electrophoresis instrument

    E-Print Network [OSTI]

    Stockton, Amanda Michelle

    2010-01-01

    utilizes subcritical water extraction and the Mars Organiceither by subcritical water extraction 115 or by sublimationwater. Subcritical Water Extraction / Reaction Protocol. A

  10. HYDROGEN PEROXIDE DETECTED ON MARS IAU Circular 8254 9 December 2003

    E-Print Network [OSTI]

    Atreya, Sushil

    HYDROGEN PEROXIDE DETECTED ON MARS IAU Circular 8254 9 December 2003 Central Bureau. Wong, University of Michigan, report: "On June 20, we made an unambiguous detection of hydrogen

  11. Space weather effects on the Mars ionosphere due to solar flares and

    E-Print Network [OSTI]

    Withers, Paul

    Space weather effects on the Mars ionosphere due to solar flares and meteors Paul Withers1, Michael in the ionospheric response to these aspects of space weather. #12;

  12. Mar/Apr 2013 Subscription Information SuperBoost Heat Exhaustion

    E-Print Network [OSTI]

    Ishida, Yuko

    1 Mar/Apr 2013 of formerly strong honey bee colon- ies, and easily observable decreases in bumble bee sightings, correlated

  13. Resonant thermonuclear reaction rate

    SciTech Connect (OSTI)

    Haubold, H.J.; Mathai, A.M.

    1986-08-01

    Basic physical principles for the resonant and nonresonant thermonuclear reaction rates are applied to find their standard representations for nuclear astrophysics. Closed-form representations for the resonant reaction rate are derived in terms of Meijer's G-italic-function. Analytic representations of the resonant and nonresonant nuclear reaction rates are compared and the appearance of Meijer's G-italic-function is discussed in physical terms.

  14. LCC Guidance Rates

    Office of Energy Efficiency and Renewable Energy (EERE)

    Notepad text file provides the LCC guidance rates in a numbered format for the various regions throughout the U.S.

  15. Planning Considerations Related to the Organic Contamination of Martian Samples and Implications for the Mars 2020 Rover

    E-Print Network [OSTI]

    Sessions, A. L.

    Data gathered during recent NASA missions to Mars, particularly by the Rovers Spirit, Opportunity, and Curiosity, have provided important insights into the past history and habitability of the Red Planet. The Mars science ...

  16. 19Bulletin Infirmier du Cancer Vol.6-n1-janvier-fvrier-mars 2006 SOR savoir patient

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    19Bulletin Infirmier du Cancer Vol.6-n°1-janvier-février-mars 2006 SOR savoir patient A fin de;20Bulletin Infirmier du Cancer Vol.6-n°1-janvier-février-mars 2006 SOR savoir patient mandations pour la

  17. New Mars exhibit at the Bradbury Science Museum

    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 shinesSolarNew scholarship supports returning students New LANLNewNew Mars Exhibit

  18. MHK Projects/Del Mar Landing | 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 HistoryScenarios Towards 2050 JumpCoos Bay OPT Wave Park <EnergyMar Landing

  19. Mars Rover's ChemCam Instrument gets sharper vision

    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 toMSDS onBudget ||EnergyMark Holecek |MarkMars

  20. Biagioli, Mario, Galileo's System of Patronage , History of Science, 28:1=79 (1990:Mar.) p.1 Biagioli, Mario, Galileo's System of Patronage , History of Science, 28:1=79 (1990:Mar.) p.1

    E-Print Network [OSTI]

    Biagioli, Mario, Galileo's System of Patronage , History of Science, 28:1=79 (1990:Mar.) p.1 #12;Biagioli, Mario, Galileo's System of Patronage , History of Science, 28:1=79 (1990:Mar.) p.1 #12;Biagioli, Mario, Galileo's System of Patronage , History of Science, 28:1=79 (1990:Mar.) p.1 #12;Biagioli, Mario

  1. Mars at very low obliquity: Atmospheric collapse and the fate of M. A. Kreslavsky1

    E-Print Network [OSTI]

    Head III, James William

    : Kreslavsky, M. A., and J. W. Head (2005), Mars at very low obliquity: Atmospheric collapse and the fateMars at very low obliquity: Atmospheric collapse and the fate of volatiles M. A. Kreslavsky1 and J. W. Head Department of Geological Sciences, Brown University, Providence, Rhode Island, USA Received

  2. MARS15 study of the Energy Production Demonstrator Model for Megawatt

    E-Print Network [OSTI]

    McDonald, Kirk

    MARS15 study of the Energy Production Demonstrator Model for Megawatt proton beams in the 0.5 ­ 120 Targetry Workshop HPT5, Fermilab #12;Energy Production Demonstrator MARS15 Model · Solid targets · R= 60 cm · Energy Production/Materials Testing · LAQGSM/CEM generators were usedU-nat, 3 GeV, Energy deposition, Ge

  3. Solar flux variability of Mars' exosphere densities and temperatures Jeffrey M. Forbes,1

    E-Print Network [OSTI]

    Forbes, Jeffrey

    Solar flux variability of Mars' exosphere densities and temperatures Jeffrey M. Forbes,1 Frank G, the response of Mars' exosphere to long-term solar change is established and compared to that of Earth conditions) change only 36­50% as much as those at Earth as solar activity increases from solar minimum

  4. Oceanography Vol. 19, No. 1, Mar. 200664 Hybrid ModelFOR COASTAL SIMULATIONS

    E-Print Network [OSTI]

    Fringer, Oliver B.

    Oceanography Vol. 19, No. 1, Mar. 200664 Hybrid ModelFOR COASTAL SIMULATIONS A DVA N C E S I N CO M Oceanography Vol. 19, No. 1, Mar. 200664 ThisarticlehasbeenpublishedinOceanography,Volume19,Number1,aquarterlyjournalofTheOceanographySociety.Copyright2006byTheOceanography

  5. Thursday, March 16, 2006 POSTER SESSION II: MARS SPECTROSCOPY AND REMOTE SENSING

    E-Print Network [OSTI]

    Rathbun, Julie A.

    ] Exposure of sulfates to a low pressure (0.01 Torr) carbon dioxide-rich atmosphere, and intense UVThursday, March 16, 2006 POSTER SESSION II: MARS SPECTROSCOPY AND REMOTE SENSING 7:00 p.m. Fitness of Mars [#1885] Currently, the same infrared remote sensing data sets are interpreted as pointing both

  6. A comparison of methods used to estimate the height of sand dunes on Mars

    E-Print Network [OSTI]

    Bourke, Mary C.

    A comparison of methods used to estimate the height of sand dunes on Mars M.C. Bourke a,b,, M bodies is difficult. We assess four methods that can be used to estimate the height of aeolian dunes of which were not previously available for dunes on Mars. They include dune height, width, length, surface

  7. Dunes on Mars, `Venus', Earth, and subaqueous ripples: a scaling law for their elementary size

    E-Print Network [OSTI]

    Claudin, Philippe

    Dunes on Mars, `Venus', Earth, and subaqueous ripples: a scaling law for their elementary size P@pmmh.espci.fr Dunes and bedforms are observed in considerably di- verse environments: aeolian dunes of sand as well as snow, dunes under water, but also dunes on Mars or Titan. Summarising our work published in [1], we

  8. Mars Global Digital Dune Database and initial science results Rosalyn K. Hayward,1

    E-Print Network [OSTI]

    Bourke, Mary C.

    Mars Global Digital Dune Database and initial science results Rosalyn K. Hayward,1 Kevin F. Mullins 20 November 2007. [1] A new Mars Global Digital Dune Database (MGD3 ) constructed using Thermal of the geographic distribution of moderate- to large-size dune fields (area >1 km2 ) that will help researchers

  9. Fuel-optimal Earth-Mars trajectories using low-thrust exhaust-modulated plasma propulsion 

    E-Print Network [OSTI]

    Nah, Ren Sang

    1999-01-01

    orbit about Mars within a fixed time frame. The trajectory and spacecraft parameters have been chosen to simulate the outbound leg of a planned human mission to Mars in the year of 2014. The optimizations involve both planar and three-dimensional...

  10. Yarkovsky-Driven Spreading of the Eureka Family of Mars Trojans Matija Cuk1

    E-Print Network [OSTI]

    Yarkovsky-Driven Spreading of the Eureka Family of Mars Trojans Matija ´Cuk1 , Apostolos A orbital grouping that was affected by a negative acceleration (i.e. one against the orbital motion above about 25 (Murray and Dermott, 1999). In our Solar System, only Jupiter, Neptune and Mars are known

  11. Tuesday, March 14, 2006 MARS: ANALOG STUDIES AND AEOLIAN DEPOSITION/EROSION

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Hyper-Arid Desert Analog to Mars: The Western Desert of Egypt [#2335] We are conducting transient electromagnetic and vertical electrical soundings of potential Mars analog sites to quantify the geoelectrical in the western desert of Egypt. 2:45 p.m. Quinn R. C. * Ehrenfreund P. Grunthaner F. J. Taylor C. L. Zent A. P

  12. CO2-SO2 clathrate hydrate formation on early Mars1 Eric Chassefirea,b

    E-Print Network [OSTI]

    Boyer, Edmond

    and maintained a global average surface temperature ~230 K. Because35 clathrates trap SO2 more favorably than CO2 as a possible greenhouse gas which worked together55 with CO2 to raise the surface temperature of early Mars1 CO2-SO2 clathrate hydrate formation on early Mars1 2 Eric Chassefièrea,b , Emmanuel Dartoisc

  13. The sulfur content of volcanic gases on Mars Fabrice Gaillard, a

    E-Print Network [OSTI]

    Boyer, Edmond

    The sulfur content of volcanic gases on Mars Fabrice Gaillard, a and Bruno Scaillet1, a a CNRS sulfur contents of the martian regolith and lack of detection of extensive carbonate deposits suggest that the latest geological events that shaped the landscapes of Mars were dominated by acidic waters possibly

  14. Mar Biol (2007) 150:509519 DOI 10.1007/s00227-006-0367-4

    E-Print Network [OSTI]

    2007-01-01

    Mar Biol (2007) 150:509­519 DOI 10.1007/s00227-006-0367-4 123 RESEARCH ARTICLE Phylogeography coast colonizing the Atlantic islands and the Mediterranean, promoting the evolu- tionary divergence, Avenida Astrofísico Francisco Sánchez s/n, 38206 La Laguna, Tenerife, Islas Canarias, Spain #12;510 Mar

  15. Mar Biol (2009) 156:14211432 DOI 10.1007/s00227-009-1182-5

    E-Print Network [OSTI]

    2009-01-01

    Mar Biol (2009) 156:1421­1432 DOI 10.1007/s00227-009-1182-5 123 ORIGINAL PAPER Phylogeography with a recent colonization from south- ern populations. The results showed signs of Pleistocene signatures-mail: sara_francisco@ispa.pt R. Castilho · M. Soares Centro de Ciências do Mar do Algarve, Campus de Gambelas

  16. Impact-induced hydrothermal activity on early Mars Oleg Abramov and David A. Kring

    E-Print Network [OSTI]

    Abramov, Oleg

    Impact-induced hydrothermal activity on early Mars Oleg Abramov and David A. Kring Lunar time for colonization of impact-induced hydrothermal systems by thermophilic organisms, provided they existed on early Mars. The habitable volume reaches a maximum of 6,000 km3 8,500 years after the impact

  17. Observations of atmospheric tides on Mars at the season and latitude of the Phoenix atmospheric entry

    E-Print Network [OSTI]

    Withers, Paul

    Observations of atmospheric tides on Mars at the season and latitude of the Phoenix atmospheric atmospheric entry of NASA's Phoenix Mars probe using Phoenix Atmospheric Structure Experiment (ASE) data atmospheric entry, Geophys. Res. Lett., 37, L24204, doi:10.1029/2010GL045382. 1. Introduction [2] Phoenix

  18. Wet Chemistry experiments on the 2007 Phoenix Mars Scout Lander mission: Data analysis and results

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    Wet Chemistry experiments on the 2007 Phoenix Mars Scout Lander mission: Data analysis and results performed using the Wet Chemistry Laboratories on the 2007 Phoenix Mars Scout Lander. One soil sample.36(±0.3) mM, respectively. Results indicate that the leached portion of soils at the Phoenix landing site

  19. The oxidationreduction potential of aqueous soil solutions at the Mars Phoenix landing site

    E-Print Network [OSTI]

    Kounaves, Samuel P.

    The oxidationreduction potential of aqueous soil solutions at the Mars Phoenix landing site Richard; revised 2 June 2011; accepted 3 June 2011; published 23 July 2011. [1] Results from the Mars Phoenix) of the Phoenix WCL Rosy Red sample soil solution. The measured Eh of the Rosy Red sample in the WCL aqueous test

  20. Dielectric signatures of adsorbed and salty liquid water at the Phoenix landing site, Mars

    E-Print Network [OSTI]

    Stillman, David E.

    Dielectric signatures of adsorbed and salty liquid water at the Phoenix landing site, Mars David E was measured by the Thermal and Electrical Conductivity Probe (TECP) on the Phoenix lander. We interpret liquid water at the Phoenix landing site, Mars, J. Geophys. Res., 116, E09005, doi:10.1029/2011JE003838

  1. Multipoint observations of coronal mass ejection and solar energetic particle events on Mars

    E-Print Network [OSTI]

    California at Berkeley, University of

    coupled with the WangSheeleyArge version 1.6 potential source surface model, using Solar and HeliosphericMultipoint observations of coronal mass ejection and solar energetic particle events on Mars and evolution of interplanetary coronal mass ejections (ICMEs) throughout the heliosphere. Using Mars Global

  2. ltima actualizacin 12-06-13 Nov Dic Ene Feb Mar Abr May Jun Jul Ago Sept Oct Nov

    E-Print Network [OSTI]

    Escolano, Francisco

    /Canadeka/Chineka Energias renovables 15Mar/15Jul continuamente abierta continuamente abierta continuamente abierta 14Febr/25

  3. Power Rate Cases (pbl/rates)

    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 mapSpeedingProgram Guidelines This document w w w.pv - te ch.orgPower PlantRates >

  4. Power Rates Announcements (pbl/rates)

    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 mapSpeedingProgram Guidelines This document w w w.pv - te ch.orgPower PlantRates >

  5. Rates Meetings and Workshops (pbl/rates)

    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 wouldMassR&D100 Winners * Impacts on GlobalRachel2RateCaseElements Sign In About | FY

  6. Previous Power Rates (rates/current)

    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-Rich Matrices in Hydrothermal PlumesPress1,Previous EventsRates

  7. The Phoenix Mars Lander Robotic Arm Robert Bonitz, Lori Shiraishi, Matthew Robinson, Joseph Carsten, Richard Volpe, Ashitey Trebi-Ollennu

    E-Print Network [OSTI]

    Volpe, Richard

    1 The Phoenix Mars Lander Robotic Arm Robert Bonitz, Lori Shiraishi, Matthew Robinson, Joseph,wilson,davis@honeybeerobotics.com Abstract--The Phoenix Mars Lander Robotic Arm (RA) has operated for 149 sols since the Lander touched down describes the design and operations of the RA as a critical component of the Phoenix Mars Lander necessary

  8. Unique Spectroscopy and Imaging of Mars with JWST

    E-Print Network [OSTI]

    Villanueva, Geronimo L; Clancy, Todd R; Encrenaz, Therese; Fouchet, Thierry; Hartogh, Paul; Lellouch, Emmanuel; Lopez-Valverde, Miguel A; Mumma, Michael J; Novak, Robert E; Smith, Michael D; Vandaele, Ann-Carine; Wolff, Michael J; Ferruit, Pierre; Milam, Stefanie N

    2015-01-01

    In this document, we summarize the main capabilities of the James Webb Space Telescope (JWST) for performing observations of Mars. The distinctive vantage point of JWST at the Sun-Earth Lagrange point (L2) will allow sampling the full observable disk, permitting the study of short-term phenomena, diurnal processes (across the East-West axis) and latitudinal processes between the hemispheres (including seasonal effects) with excellent spatial resolutions (0.07 arcsec at 2 {\\mu}m). Spectroscopic observations will be achievable in the 0.7-5 {\\mu}m spectral region with NIRSpec at a maximum resolving power of 2700, and with 8000 in the 1-1.25 {\\mu}m range. Imaging will be attainable with NIRCam at 4.3 {\\mu}m and with two narrow filters near 2 {\\mu}m, while the nightside will be accessible with several filters in the 0.5 to 2 {\\mu}m. Such a powerful suite of instruments will be a major asset for the exploration and characterization of Mars. Some science cases include the mapping of the water D/H ratio, investigatio...

  9. Mars mission performance enhancement with hybrid nuclear propulsion

    SciTech Connect (OSTI)

    Dagle, J.E.; Noffsinger, K.E. [Pacific Northwest Lab., Richland, WA (United States); Segna, D.R. [USDOE Richland Operations Office, WA (United States)

    1992-01-01

    Nuclear electric propulsion (NEP), compared with chemical and nuclear thermal propulsion (NTP), can effectively deliver the same mass to Mars using much less propellant, consequently requiring less mass delivered to Earth orbit. The lower thrust of NEP requires a spiral trajectory near planetary bodies, which significantly increases the travel time. Although the total travel time is long, the portion of the flight time spent during interplanetary transfer is shorter, because the vehicle is thrusting for much longer periods of time. This has led to the supposition that NEP, although very attractive for cargo missions, is not suitable for piloted missions to Mars. However, with the application of a hybrid application of a hybrid approach to propulsion, the benefits of NEP can be utilized while drastically reducing the overall travel time required. Development of a dual-mode system, which utilizes high-thrust NTP to propel the spacecraft from the planetary gravitational influence and low-thrust NEP to accelerate in interplanetary space, eliminates the spiral trajectory and results in a much faster transit time than could be obtained by either NEP or NTP alone. This results in a mission profile with a lower initial mass in low Earth orbit. In addition, the propulsion system would have the capability to provide electrical power for mission applications.

  10. Advanced hybrid nuclear propulsion Mars mission performance enhancement

    SciTech Connect (OSTI)

    Dagle, J.E.; Noffsinger, K.E.; Segna, D.R.

    1992-02-01

    Nuclear electric propulsion (NEP), compared with chemical and nuclear thermal propulsion (NTP), can effectively deliver the same mass to Mars using much less propellant, consequently requiring less mass delivered to Earth orbit. The lower thrust of NEP requires a spiral trajectory near planetary bodies, which significantly increases the travel time. Although the total travel time is long, the portion of the flight time spent during interplanetary transfer is shorter, because the vehicle is thrusting for much longer periods of time. This has led to the supposition that NEP, although very attractive for cargo missions, is not suitable for piloted missions to Mars. However, with the application of a hybrid approach to propulsion, the benefits of NEP can be utilized while drastically reducing the overall travel time required. Development of a dual-mode system, which utilizes high-thrust NTP to propel the spacecraft from the planetary gravitational influence and low-thrust NEP to accelerate in interplanetary space, eliminates the spiral trajectory and results in a much faster transit time than could be obtained by either NEP or NTP alone. This results in a mission profile with a lower initial mass in low Earth orbit. In addition, the propulsion system would have the capability to provide electrical power for mission applications.

  11. Sediment volume in the north polar sand seas of Mars

    SciTech Connect (OSTI)

    Lancaster, N.; Greeley, R. (Arizona State Univ., Tempe (USA))

    1990-07-10

    Data from studies of the cross-sectional area of terrestrial transverse dunes have been combined with maps of dune morphometry derived from Viking orbiter images to generate new estimates of sediment thickness and dune sediment volume in the north polar sand seas of Mars. A relationship between dune spacing and equivalent sediment thickness (EST) was developed from field data on Namibian and North American dunes and was applied to data on dune spacing and dune cover measured on Viking orbiter images to generate maps of dune sediment thickness for Martian north polar sand seas. There are four major sand seas in the north polar region of Mars, covering an area of 6.8 x 10{sup 5} km{sup 2}. Equivalent sediment thickness ranges between 0.5 and 6.1 m with a mean of 1.8 m. The sand seas contain a total of 1158 km{sup 3} of dune sediment, which may have been derived by erosion of polar layered deposits and concentrated in its present location by winds that change direction seasonally.

  12. Diagenesis and clay mineral formation at Gale Crater, Mars

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

    Bridges, J. C.; Schwenzer, S. P.; Leveille, R.; Westall, F.; Wiens, R. C.; Mangold, N.; Bristow, T.; Edwards, P.; Berger, G.

    2015-01-18

    The Mars Science Laboratory rover Curiosity found host rocks of basaltic composition and alteration assemblages containing clay minerals at Yellowknife Bay, Gale Crater. On the basis of the observed host rock and alteration minerals, we present results of equilibrium thermochemical modeling of the Sheepbed mudstones of Yellowknife Bay in order to constrain the formation conditions of its secondary mineral assemblage. Building on conclusions from sedimentary observations by the Mars Science Laboratory team, we assume diagenetic, in situ alteration. The modeling shows that the mineral assemblage formed by the reaction of a CO?-poor and oxidizing, dilute aqueous solution (Gale Portage Water)more »in an open system with the Fe-rich basaltic-composition sedimentary rocks at 10–50°C and water/rock ratio (mass of rock reacted with the starting fluid) of 100–1000, pH of ~7.5–12. Model alteration assemblages predominantly contain phyllosilicates (Fe-smectite, chlorite), the bulk composition of a mixture of which is close to that of saponite inferred from Chemistry and Mineralogy data and to that of saponite observed in the nakhlite Martian meteorites and terrestrial analogues. To match the observed clay mineral chemistry, inhomogeneous dissolution dominated by the amorphous phase and olivine is required. We therefore deduce a dissolving composition of approximately 70% amorphous material, with 20% olivine, and 10% whole rock component.« less

  13. Nuclear rockets: High-performance propulsion for Mars

    SciTech Connect (OSTI)

    Watson, C.W.

    1994-05-01

    A new impetus to manned Mars exploration was introduced by President Bush in his Space Exploration Initiative. This has led, in turn, to a renewed interest in high-thrust nuclear thermal rocket propulsion (NTP). The purpose of this report is to give a brief tutorial introduction to NTP and provide a basic understanding of some of the technical issues in the realization of an operational NTP engine. Fundamental physical principles are outlined from which a variety of qualitative advantages of NTP over chemical propulsion systems derive, and quantitative performance comparisons are presented for illustrative Mars missions. Key technologies are described for a representative solid-core heat-exchanger class of engine, based on the extensive development work in the Rover and NERVA nuclear rocket programs (1955 to 1973). The most driving technology, fuel development, is discussed in some detail for these systems. Essential highlights are presented for the 19 full-scale reactor and engine tests performed in these programs. On the basis of these tests, the practicality of graphite-based nuclear rocket engines was established. Finally, several higher-performance advanced concepts are discussed. These have received considerable attention, but have not, as yet, developed enough credibility to receive large-scale development.

  14. Effective Rate Period

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

    Regulation and Frequency Response DollarsKW-month 4.56 CV-RFS4 Spinning Reserve The formula rate for spinning reserve service is the price consistent with the California...

  15. Effective Rate Period

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

    and Frequency Response DollarsKW-month 3.98 4.17 CV-RFS4 Spinning Reserve The formula rate for spinning reserve service is the price consistent with the California...

  16. Effective Rate Period

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

    and Frequency Response DollarsKW-month 4.17 4.56 CV-RFS4 Spinning Reserve The formula rate for spinning reserve service is the price consistent with the California...

  17. 2012 Transmission Rate Schedules

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

    for HLH and LLH. 2. OTHER RATE PROVISIONS a. BPA Incremental Cost BPA's incremental cost will be based on an hourly energy index in the Pacific Northwest. If no adequate...

  18. On Thermonuclear Reaction Rates

    E-Print Network [OSTI]

    H. J. Haubold; A. M. Mathai

    1996-12-02

    Nuclear reactions govern major aspects of the chemical evolution od galaxies and stars. Analytic study of the reaction rates and reaction probability integrals is attempted here. Exact expressions for the reaction rates and reaction probability integrals for nuclear reactions in the case of nonresonant, modified nonresonant, screened nonresonant and resonant cases are given. These are expressed in terms of H-functions, G-functions and in computable series forms. Computational aspects are also discussed.

  19. Turnover Rates in Insular Biogeography: Effect of Immigration on Extinction Author(s): James H. Brown and Astrid Kodric-Brown

    E-Print Network [OSTI]

    Brown, James H.

    . Brown and Astrid Kodric-Brown Source: Ecology, Vol. 58, No. 2 (Mar., 1977), pp. 445-449 Published by, turnover rate is directly related to the distance between an island and the source of colonizing species: Arizona; biogeography; colonization; extinction; insular biogeography; island; turnover. INTRODUCTION More

  20. Calibrating the ChemCam LIBS for carbonate minerals on Mars

    SciTech Connect (OSTI)

    Wiens, Roger C; Clegg, Samuel M; Ollila, Ann M; Barefield, James E; Lanza, Nina; Newsom, Horton E

    2009-01-01

    The ChemCam instrument suite on board the NASA Mars Science Laboratory (MSL) rover includes the first LIBS instrument for extraterrestrial applications. Here we examine carbonate minerals in a simulated martian environment using the LIDS technique in order to better understand the in situ signature of these materials on Mars. Both chemical composition and rock type are determined using multivariate analysis (MVA) techniques. Composition is confirmed using scanning electron microscopy (SEM) techniques. Our initial results suggest that ChemCam can recognize and differentiate between carbonate materials on Mars.

  1. Propulsive options for a manned Mars transportation system

    SciTech Connect (OSTI)

    Braun, R.D.; Blersch, D.J.

    1989-01-01

    In this investigation, five potential manned Mars transportation systems are compared. These options include: (1) a single vehicle, chemically propelled (CHEM) option, (2) a single vehicle, nuclear thermal propulsion (NTP) option, (3) a single vehicle solar electric propulsion (SEP) option, (4) a single vehicle hybrid nuclear electric propulsion (NEP)/CHEM option, and (5) a dual vehicle option (NEP cargo spacecraft and CHEM manned vehicle). In addition to utilizing the initial vehicle weight in low-earth orbit as a measure of mission feasibility, this study addresses the major technological barriers each propulsive scenario must surpass. It is shown that instead of a single clearly superior propulsion system, each means of propulsion may be favored depending upon the specified program policy and the extent of the desired manned flight time. Furthermore, the effect which aerobraking and multiple transfer cycles have upon mission feasibility is considered. 18 refs.

  2. Modeling the variations of Dose Rate measured by RAD during the first MSL Martian year: 2012-2014

    E-Print Network [OSTI]

    Guo, Jingnan; Wimmer-Schweingruber, Robert F; Rafkin, Scot; Hassler, Donald M; Posner, Arik; Heber, Bernd; Koehler, Jan; Ehresmann, Bent; Appel, Jan K; Boehm, Eckart; Boettcher, Stephan; Burmeister, Soenke; Brinza, David E; Lohf, Henning; Martin, Cesar; Kahanpaeae, H; Reitz, Guenther

    2015-01-01

    The Radiation Assessment Detector (RAD), on board Mars Science Laboratory's (MSL) rover Curiosity, measures the {energy spectra} of both energetic charged and neutral particles along with the radiation dose rate at the surface of Mars. With these first-ever measurements on the Martian surface, RAD observed several effects influencing the galactic cosmic ray (GCR) induced surface radiation dose concurrently: [a] short-term diurnal variations of the Martian atmospheric pressure caused by daily thermal tides, [b] long-term seasonal pressure changes in the Martian atmosphere, and [c] the modulation of the primary GCR flux by the heliospheric magnetic field, which correlates with long-term solar activity and the rotation of the Sun. The RAD surface dose measurements, along with the surface pressure data and the solar modulation factor, are analysed and fitted to empirical models which quantitatively demonstrate} how the long-term influences ([b] and [c]) are related to the measured dose rates. {Correspondingly we ...

  3. Mars in the late Noachian : evolution of a habitable surface environment

    E-Print Network [OSTI]

    Johnson, Sarah Stewart

    2008-01-01

    This dissertation addresses whether simple life forms might have existed on Mars during the late Noachian epoch, and whether those life forms, or their traces, can be detected today. It begins by analyzing the ancient ...

  4. Comparative analysis of surface power system architectures for human Mars exploration

    E-Print Network [OSTI]

    Cooper, Chase Allen

    2009-01-01

    This thesis provides a comprehensive analysis of surface power generation and energy storage architectures for human Mars surface missions, including tracking and non-tracking photovoltaic power generation, nuclear fission ...

  5. Early Mars hydrology: Meridiani playa deposits and the sedimentary record of Arabia Terra

    E-Print Network [OSTI]

    Andrews-Hanna, Jeffrey C.

    The Meridiani Planum region of Mars has been identified as a region of past aqueous activity by a combination of orbital and in situ observations that revealed evidence for sulfate-rich dirty evaporites formed in a playa ...

  6. Design of power systems for extensible surface mobility systems on the Moon and Mars

    E-Print Network [OSTI]

    Hong, SeungBum, S.M. Massachusetts Institute of Technology

    2007-01-01

    This thesis presents the power system model description and sample studies for extensible surface mobility systems on the Moon and Mars. The mathematical model of power systems for planetary vehicles was developed in order ...

  7. Rover Technology Development and Infusion for the 2009 Mars Science Laboratory Mission

    E-Print Network [OSTI]

    Volpe, Richard

    Rover Technology Development and Infusion for the 2009 Mars Science Laboratory Mission Richard Volpe and Stephen Peters Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91103 email: {firstname.lastname}@jpl.nasa.gov Keywords: Spacecraft Autonomy, Planetary Robotics, Technology

  8. The Mars Gravity Biosatellite as an innovative partial gravity research platform

    E-Print Network [OSTI]

    Fulford-Jones, Thaddeus R. F

    2008-01-01

    The Mars Gravity Biosatellite is an unprecedented independent spaceflight platform for gravitational biology research. With a projected first launch after 2010, the low Earth orbit satellite will support a cohort of fifteen ...

  9. Constraining the average fill densities of Mars' lowlands and fluvial erosion of Titan's polar regions.

    E-Print Network [OSTI]

    Tewelde, Yodit

    2013-01-01

    Other than Earth, Mars and Titan are the only bodies in our Solar System where we have observed widespread fluvial activity. In this thesis I present two approaches for constraining the extent of multiple resurfacing ...

  10. Laser-Firing ChemCam Vital to Curiosity Rover's Tour of Mars...

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

    NASA's Curiosity rover. Image: NASAJPL-CaltechLANLCNESIRAP 4 of 4 A bright ball of plasma, produced by ChemCam's invisible laser beam striking a rock within the Mars sample...

  11. MARS IN A MINUTE: What Happens When the Sun Blocks our Signal?

    E-Print Network [OSTI]

    and Mars wind up on opposite sides of the sun. Thats called "solar conjunction." It's like being on either on other work... or take a well-deserved vacation! Solar conjunction lasts just a few weeks. Then its back

  12. Wednesday, March 14, 2007 MARS SEDIMENTS AND GEOCHEMISTRY: VIEW FROM THE SURFACE

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Golombek M. Parker T. Squyres S. W. Sullivan R. Structure and Sedimentology of the Western Margin of Erebus Crater, Meridiani Planum, Mars [#2235] The structure, stratigraphy and sedimentology of two outcrops

  13. Detailed stratigraphy and bed thickness of the Mars north and south polar layered deposits

    E-Print Network [OSTI]

    Limaye, Ajay B. S.

    The Mars polar layered deposits (PLD) likely hold an extensive record of recent climate during a period of high-amplitude orbit and obliquity cycles. Previous work has detected limited evidence for orbital signatures within ...

  14. STUDIES OF DUNE CHANGE ON MARS COMBINING MOC AND HIRISE IMAGES. M. C. , A. Philippoff1

    E-Print Network [OSTI]

    Bourke, Mary C.

    STUDIES OF DUNE CHANGE ON MARS COMBINING MOC AND HIRISE IMAGES. M. C. Bourke1 , A. Philippoff1 in the circumpolar sand seas (76.2°N, 95.3°E) found that two 20 m wide dome dunes disappeared and a third reduced its volume by 15% over 3.04 Mars years [1]. Here we report on the findings of an extended dune monitoring

  15. Rotational rate sensor

    DOE Patents [OSTI]

    Hunter, Steven L. (Livermore, CA)

    2002-01-01

    A rate sensor for angular/rotational acceleration includes a housing defining a fluid cavity essentially completely filled with an electrolyte fluid. Within the housing, such as a toroid, ions in the fluid are swept during movement from an excitation electrode toward one of two output electrodes to provide a signal for directional rotation. One or more ground electrodes within the housing serve to neutralize ions, thus preventing any effect at the other output electrode.

  16. Current Power Rates

    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 would like submit theCovalent Bonding in ActinideRail betweenProtectionCurrentJobPower-Rates

  17. Rate Case Elements

    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 wouldMassR&D100 Winners * Impacts on GlobalRachel2RateCaseElements Sign In About | Careers |

  18. Rate Design and Renewables

    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 wouldMassR&D100 Winners * Impacts on GlobalRachel2RateCaseElements Sign In About | Careers

  19. Solar X-ray Flare Hazards on the Surface of Mars

    E-Print Network [OSTI]

    David S. Smith; John M. Scalo

    2006-10-03

    Putative organisms on the Martian surface would be exposed to potentially high doses of ionizing radiation during strong solar X-ray flares. We extrapolate the observed flare frequency-energy release scaling relation to releases much larger than seen so far for the sun, an assumption supported by observations of flares on other solar- and subsolar-mass main sequence stars. We calculate the surficial reprocessed X-ray spectra using a Monte Carlo code we have developed. Biological doses from indirect genome damage are calculated for each parameterized flare spectrum by integration over the X-ray opacity of water. We estimate the mean waiting time for solar flares producing a given biological dose of ionizing radiation on Mars and compare with lethal dose data for a wide range of terrestrial organisms. These timescales range from decades for significant human health risk to 0.5 Myr for D. radiodurans lethality. Such doses require total flare energies of 10^33--10^38 erg, the lower range of which has been observed for other stars. Flares are intermittent bursts, so acute lethality will only occur on the sunward hemisphere during a sufficiently energetic flare, unlike low-dose-rate, extended damage by cosmic rays. We estimate the soil and CO_2 ice columns required to provide 1/e shielding as 4--9 g cm^-2, depending on flare mean energy and atmospheric column density. Topographic altitude variations give a factor of two variation in dose for a given flare. Life in ice layers that may exist ~ 100 g cm^-2 below the surface would be well protected.

  20. Radiological Contingency Planning for the Mars Science Laboratory Launch

    SciTech Connect (OSTI)

    Paul P. Guss

    2008-04-01

    This paper describes the contingency planning for the launch of the Mars Science Laboratory scheduled for the 21-day window beginning on September 15, 2009. National Security Technologies, LLC (NSTec), based in Las Vegas, Nevada, will support the U.S. Department of Energy (DOE) in its role for managing the overall radiological contingency planning support effort. This paper will focus on new technologies that NSTec’s Remote Sensing Laboratory (RSL) is developing to enhance the overall response capability that would be required for a highly unlikely anomaly. This paper presents recent advances in collecting and collating data transmitted from deployed teams and sensors. RSL is responsible to prepare the contingency planning for a range of areas from monitoring and assessment, sample collection and control, contaminated material release criteria, data management, reporting, recording, and even communications. The tools RSL has available to support these efforts will be reported. The data platform RSL will provide shall also be compatible with integration of assets and field data acquired with other DOE, National Space and Aeronautics and Space Administration (NASA), state, and local resources, personnel, and equipment. This paper also outlines the organizational structure for response elements in radiological contingency planning.

  1. Radiological Contingency Planning for the Mars Science Laboratory Launch

    SciTech Connect (OSTI)

    Paul Guss, Robert Augdahl, Bill Nickels, Cassandra Zellers

    2008-04-16

    This paper describes the contingency planning for the launch of the Mars Science Laboratory scheduled for the 21-day window beginning on September 15, 2009. National Security Technologies, LLC (NSTec), based in Las Vegas, Nevada, will support the U.S. Department of Energy (DOE) in its role for managing the overall radiological contingency planning support effort. This paper will focus on new technologies that NSTec’s Remote Sensing Laboratory (RSL) is developing to enhance the overall response capability that would be required for a highly unlikely anomaly. This paper presents recent advances in collecting and collating data transmitted from deployed teams and sensors. RSL is responsible to prepare the contingency planning for a range of areas from monitoring and assessment, sample collection and control, contaminated material release criteria, data management, reporting, recording, and even communications. The tools RSL has available to support these efforts will be reported. The data platform RSL will provide shall also be compatible with integration of assets and field data acquired with other DOE, National Aeronautics and Space Administration, state, and local resources, personnel, and equipment. This paper also outlines the organizational structure for response elements in radiological contingency planning.

  2. Reliability comparison of various nuclear propulsion configurations for Mars mission

    SciTech Connect (OSTI)

    Segna, D.R. [USDOE Richland Operations Office, WA (United States); Dagle, J.E. [Pacific Northwest Lab., Richland, WA (United States); Lyon, W.F. III [Westinghouse Hanford Co., Richland, WA (United States)

    1992-01-01

    Currently, trade-offs are being made among the various propulsion systems being considered for the Space Exploration Initiative (SEI) missions. It is necessary to investigate the reliability aspects as well as the efficiency, mass savings, and experience characteristics of the various configurations. Reliability is a very important factor for the SEI missions because of the long duration and because problems will be fixed onboard. The propulsion options that were reviewed consist of nuclear thermal propulsion (NTP), nuclear electric propulsion (NEP) and various configurations of each system. There were four configurations developed for comparison with the NTP as baselined in the Synthesis (1991): (1) NEP, (2) hybrid NEP/NTP, (3) hybrid with power beaming, and (4) NTP upper stage on the heavy lift launch vehicle (HLLV). The comparisons were based more or less on a qualitative review of complexity, stress levels and operations for each of the four configurations. Each configuration included a pressurized NEP and an NTP ascent stage propulsion system for the Mars mission.

  3. Energy Management Through Innovative Rates 

    E-Print Network [OSTI]

    Williams, M. L.

    1982-01-01

    of energy efficiency in the industrial sector and specific rate design alternatives for doing so....

  4. Exploring the Earth from Mars David T. Sandwell

    E-Print Network [OSTI]

    Sandwell, David T.

    orthogonal ridge/transform patterns, and a magnetic field that reverses at just the right rate to be recorded of kilometers (miles) across the mantle of the Earth at rates that are too slow to be observed without the aid further to claim that it is the optimal mechanism for the Earth to shed excess radiogenic heat produced

  5. Solar Rotation Effects on the Thermospheres of Mars and Earth

    E-Print Network [OSTI]

    Forbes, Jeffrey

    are determined by the efficiency with which ab- sorbed radiation is converted to heat, the rates of molecular and eddy heat conduction, and the rate of radiative cooling (3), particularly by CO2 at 15 mm (4. This dif- ferential rotation causes magnetic field lines to twist, resulting in the formation of active re

  6. National Utility Rate Database: Preprint

    SciTech Connect (OSTI)

    Ong, S.; McKeel, R.

    2012-08-01

    When modeling solar energy technologies and other distributed energy systems, using high-quality expansive electricity rates is essential. The National Renewable Energy Laboratory (NREL) developed a utility rate platform for entering, storing, updating, and accessing a large collection of utility rates from around the United States. This utility rate platform lives on the Open Energy Information (OpenEI) website, OpenEI.org, allowing the data to be programmatically accessed from a web browser, using an application programming interface (API). The semantic-based utility rate platform currently has record of 1,885 utility rates and covers over 85% of the electricity consumption in the United States.

  7. Mars atmospheric CO[subscript 2] condensation above the north and south poles as revealed by radio occultation, climate sounder, and laser ranging observations

    E-Print Network [OSTI]

    Hu, Renyu

    [1] We study the condensation of CO[subscript 2] in Mars' atmosphere using temperature profiles retrieved from radio occultation measurements from Mars Global Surveyor (MGS) as well as the climate sounding instrument onboard ...

  8. Bubble growth rates in boiling

    E-Print Network [OSTI]

    Griffith, P.

    1956-01-01

    The conditions determining the growth rate of a bubble on a surface in boiling are considered and a mathematical model framed in the light of these conditions. The growth rate is then calculated for bubbles growing under ...

  9. 2007 Wholesale Power Rate Schedules : 2007 General Rate Schedule Provisions.

    SciTech Connect (OSTI)

    United States. Bonneville Power Administration.

    2006-11-01

    This schedule is available for the contract purchase of Firm Power to be used within the Pacific Northwest (PNW). Priority Firm (PF) Power may be purchased by public bodies, cooperatives, and Federal agencies for resale to ultimate consumers, for direct consumption, and for Construction, Test and Start-Up, and Station Service. Rates in this schedule are in effect beginning October 1, 2006, and apply to purchases under requirements Firm Power sales contracts for a three-year period. The Slice Product is only available for public bodies and cooperatives who have signed Slice contracts for the FY 2002-2011 period. Utilities participating in the Residential Exchange Program (REP) under Section 5(c) of the Northwest Power Act may purchase Priority Firm Power pursuant to the Residential Exchange Program. Rates under contracts that contain charges that escalate based on BPA's Priority Firm Power rates shall be based on the three-year rates listed in this rate schedule in addition to applicable transmission charges. This rate schedule supersedes the PF-02 rate schedule, which went into effect October 1, 2001. Sales under the PF-07 rate schedule are subject to BPA's 2007 General Rate Schedule Provisions (2007 GRSPs). Products available under this rate schedule are defined in the 2007 GRSPs. For sales under this rate schedule, bills shall be rendered and payments due pursuant to BPA's 2007 GRSPs and billing process.

  10. Commercial Building Asset Rating Program

    Broader source: Energy.gov [DOE]

    Slides from a Commercial Building Initiative webinar outlining the Commercial Building Asset Rating Program on August 23, 2011.

  11. Methane oxidation rates by AMS

    E-Print Network [OSTI]

    Pack, M; Heintz, M; ReeburGh, WS; Trumbore, SE; Valentine, DL; Xu, X

    2009-01-01

    second case. Number of cases Methane oxidation rates by AMSIn the marine environment methane (CH 4 ) oxidation consumes

  12. Formation of methane on Mars by fluid-rock interaction in the crust James R. Lyons,1

    E-Print Network [OSTI]

    Nimmo, Francis

    Formation of methane on Mars by fluid-rock interaction in the crust James R. Lyons,1 Craig Manning by magmatic degassing from a dike with only 50 ppm C. Atmospheric methane strongly suggests ongoing magmatism and hydrothermal alteration on Mars. Citation: Lyons, J. R., C. Manning, and F. Nimmo (2005), Formation of methane

  13. Sixth International Conference on Aeolian Research, Guelph, Canada. 2006 Barchan dune morphodynamics and linear dune formation on Mars

    E-Print Network [OSTI]

    Bourke, Mary C.

    Sixth International Conference on Aeolian Research, Guelph, Canada. 2006 Barchan dune morphodynamics and linear dune formation on Mars Mary C. Bourke, Planetary Science Institute, Tucson, mbourke@psi.edu Observations of sand dunes in satellite images indicate a wide variety of dune forms on Mars. Similar to Earth

  14. 1 Managed by UT-Battelle for the U.S. Department of Energy MERIT Videoconference 11 Mar 2009

    E-Print Network [OSTI]

    McDonald, Kirk

    1 Managed by UT-Battelle for the U.S. Department of Energy MERIT Videoconference 11 Mar 2009 · Containment encompasses nozzle tip #12;3 Managed by UT-Battelle for the U.S. Department of Energy MERIT Concept ORNL/VG Mar2009 Splash Mitigator #12;4 Managed by UT-Battelle for the U.S. Department of Energy

  15. Genetic signature of a recent invasion: The ragged sea hare Bursatella leachii in Mar Menor (SE Spain)

    E-Print Network [OSTI]

    Borges, Rita

    Genetic signature of a recent invasion: The ragged sea hare Bursatella leachii in Mar Menor (SE, Portugal b Departamento de Ciencias del Mar y Biología Aplicada, Universidad de Alicante, Campus de San hypothesis for the origin of invasions is that colonization by invasive species is most often associated

  16. Optimization Online - Convergence rate of a proximal multiplier ...

    E-Print Network [OSTI]

    Orlando Sarmiento

    2015-03-13

    Mar 13, 2015 ... ... solve a convex program with separable structure unified the works of Chen and Teboulle (PCPM method), Kyono and Fukushima (NPCPMM) ...

  17. Hydrothermal formation of Clay-Carbonate alteration assemblages in the Nili Fossae region of Mars

    E-Print Network [OSTI]

    Brown, Adrian J; Baldridge, Alice M; Crowley, James K; Bridges, Nathan T; Thomson, Bradley J; Marion, Giles M; Filho, Carlos R de Souza; Bishop, Janice L

    2014-01-01

    The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) has returned observations of the Nili Fossae region indicating the presence of Mg- carbonate in small (characterize these carbonate-bearing units. We applied absorption band mapping techniques to investigate a range of possible phyllosilicate and carbonate minerals that could be present in the Nili Fossae region. We also describe a clay-carbonate hydrothermal alteration mineral assemblage in the Archean Warrawoona Group of Western Australia that is a potential Earth analog to the Nili Fossae carbonate-bearing rock units. We discuss the geological and biological implications for hydrothermal processes on Noachian Mars.

  18. Don't look for little green men of Mars to be skinny-dipping in canals, but their dousing rods

    E-Print Network [OSTI]

    Eustice, Ryan

    water. In 2002 the Mars Odyssey Orbiter found large amounts of water ice below the surface of Mars blew away the top layer of soil, a layer of water ice was uncovered. One very exciting moment Mars science strategy "Follow the Water," Phoenix aimed to dig up and examine the water ice, to (1

  19. Wholesale Power Rate Schedules | Department of Energy

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

    Rate Schedules Wholesale Power Rate Schedules Wholesale Power Rate Schedules October 1, 2012 ALA-1-N Wholesale Power Rate Schedule Area: PowerSouth Energy Cooperative System:...

  20. PRINT ONLY: MARS Kress A. Head J. W. Marchant D. R.

    E-Print Network [OSTI]

    Rathbun, Julie A.

    larger glacial landsystems. López V. Tejero R. Ruiz J. Gómez-Ortiz D. The Elevation Range of the Possible of the manual counts in several adjacent diameter bins. Popa I. C. Salt Triggered Melting of Permafrost as an alternative cause for permafrost melting in chaos regions on Mars. This process, along with the fluid freezing

  1. Detecting sub-glacial aquifers in the north polar layered deposits with Mars Express/MARSIS

    E-Print Network [OSTI]

    Gurnett, Donald A.

    effects, local geothermal hot spots, or heat-generating glacial sliding. Ice cap basal melting mayDetecting sub-glacial aquifers in the north polar layered deposits with Mars Express/MARSIS W. M into the polar ice mass is modeled to determine the capability of the instrument to locate sub-glacial aquifers

  2. Carbon geochemistry of serpentinites in the Lost City Hydrothermal System (30N, MAR)

    E-Print Network [OSTI]

    Gilli, Adrian

    Massif (Mid-Atlantic Ridge, 30°N) was exam- ined to characterize carbon sources and speciation in oceanic. The speciation of carbon de- pends on the chemical and physical conditions prevailing in the reservoir, and itsCarbon geochemistry of serpentinites in the Lost City Hydrothermal System (30°N, MAR) Ade

  3. AN AUTOMATED ROVER COMMAND GENERATION PROTOTYPE FOR THE MARS 2003 MARIE CURIE ROVER

    E-Print Network [OSTI]

    Schaffer, Steven

    1 AN AUTOMATED ROVER COMMAND GENERATION PROTOTYPE FOR THE MARS 2003 MARIE CURIE ROVER Rob Sherwood.lastname@jpl.nasa.gov Abstract This paper discusses a proof-of-concept prototype for ground-based automatic generation) based planning and scheduling system will automatically generate a command sequence that will execute

  4. Joint and Conflat Leakage, March 2007 Tests P. Titus, MIT (Mar. 7,2007)

    E-Print Network [OSTI]

    McDonald, Kirk

    Joint and Conflat Leakage, March 2007 Tests P. Titus, MIT (Mar. 7,2007) · Problems feed closure valve that was "found equipment" · Cobbled together cryogenic system does not represent detected from the center terminal assembly. #12;Joint and Conflat Leakage, March 2007 Tests · During March

  5. Mesoscale Spectra of Mars's Atmosphere Derived from MGS TES Infrared Radiances TAKESHI IMAMURA

    E-Print Network [OSTI]

    and potential energy spectra as a function of horizontal wavenumber. Each spectrum has two different wave spectra of the atmospheric potential energy of Mars at mesoscales (wavelengths of 64­957 km) were obtained-scale ends, the spectra sometimes show prominent steepening with slopes from 2 to 3. The power peaks

  6. SALINE LAKES ON QINGHAI-TIBET PLATEAU AND SALTS ON MARS1 M. P. Zheng1

    E-Print Network [OSTI]

    SALINE LAKES ON QINGHAI-TIBET PLATEAU AND SALTS ON MARS1 M. P. Zheng1 , A. Wang2 , F. J. Kong1 , N of tectonically active belts of plateaus on the Earth [3]. The Qinghai-Tibet Plateau accounts for 1

  7. Wednesday, March 14, 2007 MARS SEDIMENTS AND GEOCHEMISTRY: THE MAP VIEW

    E-Print Network [OSTI]

    Rathbun, Julie A.

    the type of material. 2:30 p.m. Dromart G. * Quantin C. Broucke O. Stratigraphic Architectures in Southern Melas Basin, Valles Marineris, Mars [#1089] We report an identification of stratigraphic architectures the northern plains. 3:45 p.m. Pearce G. P. * Veillette D. Soare R. J. Ground Ice in Utopia Planitia: A Late

  8. Small-scale methane dispersion modelling for possible plume sources on the surface of Mars

    E-Print Network [OSTI]

    Strong, Kimberly

    Small-scale methane dispersion modelling for possible plume sources on the surface of Mars K. S 2012; published 11 October 2012. [1] Intense interest in the characteristics of a methane source Laboratory and future landers and orbiters will be tasked with understanding the sources of methane

  9. Joint Institute for Marine and Atmospheric Research (J/MAR) University of Hawaii, Honolulu, Hawaii 96822

    E-Print Network [OSTI]

    Joint Institute for Marine and Atmospheric Research (J/MAR) University of Hawaii, Honolulu, Hawaii 96822 Department of Oceanography, School of Ocean and Earth Science and Technology University of Hawaii, Honolulu. Hawaii 96822 Department of Oceanography, School of Ocean and Earth Science and Technology

  10. NASA/TP-2005-213164 Managing Lunar and Mars Mission

    E-Print Network [OSTI]

    Rathbun, Julie A.

    NASA/TP-2005-213164 Managing Lunar and Mars Mission Radiation Risks Part I: Cancer Risks, Uncertainties, and Shielding Effectiveness Francis A. Cucinotta NASA Lyndon B. Johnson Space Center Houston Division Houston, Texas July 2005 #12;THE NASA STI PROGRAM OFFICE . . . IN PROFILE Since its founding, NASA

  11. Chemical markers of possible hot spots on Mars Ah-San Wong and Sushil K. Atreya

    E-Print Network [OSTI]

    Atreya, Sushil

    not be ruled out. If outgassing does occur somewhere on Mars, water, carbon dioxide, sulfur species, methane that includes methane (CH4), sulfur dioxide (SO2), and hydrogen sulfide (H2S), starting with their current and the resulting new molecules may be detectable locally, either by remote sensing or in situ measurements. INDEX

  12. Atmosphere-crust coupling and carbon sequestration on the young Mars Professor Martin R. Lee1

    E-Print Network [OSTI]

    Guo, Zaoyang

    Atmosphere-crust coupling and carbon sequestration on the young Mars Professor Martin R. Lee1 *, Dr the idea that CO2 was `scrubbed' by precipitation of carbonate minerals within the planet's crust - a reaction termed `carbonation'. This project will seek evidence for carbonation by analysis of martian

  13. JOURNAL DE PHYSIQUE Colloque Cl, Suppl6ment au n03, Tome 49, Mars 1988

    E-Print Network [OSTI]

    Boyer, Edmond

    JOURNAL DE PHYSIQUE Colloque Cl, Suppl6ment au n03, Tome 49, Mars 1988 SOLAR PHYSICS FROM SPACELAB systematic observations of the solar atmosphere at high resolution and to measure specific global properties of the sun. The Solar Optical Universal Polarimeter recorded series of white light images with which

  14. The Fluid Mechanics of Arthropod Sniffing in Turbulent Odor Plumes M.A.R. Koehl

    E-Print Network [OSTI]

    Koehl, Mimi

    The Fluid Mechanics of Arthropod Sniffing in Turbulent Odor Plumes M.A.R. Koehl Department on the speed at which they are moved through the surrounding fluid. Therefore, antennule flicking of a hair-bearing arthropod antennule with the surrounding fluid affects the temporal patterns of odor

  15. arXiv:physics/0211010v225Mar2003 Citation Networks in High Energy Physics

    E-Print Network [OSTI]

    arXiv:physics/0211010v225Mar2003 Citation Networks in High Energy Physics S. Lehmann, B. Lautrup. The probability that a given paper in the SPIRES data base has k citations is well described by simple power laws are presented that both represent the data well, one which generates power laws and one which generates

  16. Meteorological predictions for the Beagle 2 mission to Mars Scot C. Randell Rafkin,1

    E-Print Network [OSTI]

    Rafkin, Scot C. R.

    circulations, but these are modulated by changes in the large-scale circulation. INDEX TERMS: 0343 Atmospheric Composition and Structure: Planetary atmospheres (5405, 5407, 5409, 5704, 5705, 5707); 6225 Planetology: Solar5 were used during the selection process for the Mars Exploration Rovers [Rafkin and Michaels, 2003

  17. A scaling law for aeolian dunes on Mars, Venus, Earth, and for subaqueous ripples

    E-Print Network [OSTI]

    Claudin, Philippe

    A scaling law for aeolian dunes on Mars, Venus, Earth, and for subaqueous ripples Philippe Claudin to a turbulent shear flow predicts that the wavelength at which the bed destabilises to form dunes should scale in water (subaqueous ripples), in air (aeolian dunes and fresh snow dunes), in a high pressure CO2 wind

  18. Can freezing cause floods on Mars? Chi-yuen Wang,1

    E-Print Network [OSTI]

    Manga, Michael

    Can freezing cause floods on Mars? Chi-yuen Wang,1 Michael Manga,1 and Jeffrey C. Hanna2 Received to examine freezing-induced pressurization as a mechanism for releasing groundwater. The results suggest that freezing of an aquifer of global extent under the optimal conditions, i.e., perfectly confined and with low

  19. OCTOBER 2013 IEEE CONTROL SYSTEMS MAGAZINE 27 RATNESh KuMAR

    E-Print Network [OSTI]

    Kumar, Ratnesh

    -control systems, and this work further provided entry into the field of formal verification of logi- cal (e for precision agriculture (IBM). » Licheng Jin worked on model predictive control of power sys-OCTOBER 2013 « IEEE CONTROL SYSTEMS MAGAZINE 27 RATNESh KuMAR Q. How did your education and career

  20. SPACE DAILY SPACE WAR TERRA DAILY MARS DAILY SPACE MART SPACE TRAVEL World's Smallest Universal Material

    E-Print Network [OSTI]

    Espinosa, Horacio D.

    SPACE DAILY SPACE WAR TERRA DAILY MARS DAILY SPACE MART SPACE TRAVEL NANO TECH World's Smallest, professor of mechanical Get Our Free Newsletters Via Email Space - War - Earth - Energy - China your email yes Search All Of Our Sites In One Search SpaceDaily - SpaceWar - TerraDaily Search Horacio D

  1. MH Vignal-Expos CEA-CESTA, 25 Mars 2004-Modlisation et simulations numriques

    E-Print Network [OSTI]

    Vignal, Marie-Hélène

    se détend. « Quand le plasma atteint l'anode, un arc est créé. #12;MH Vignal- Exposé CEA-CESTA, 25 de plasma entre deux électrodes P. Crispel, P. Degond, C. Parzani, M. H. Vignal Laboratoire MIP, CNRS Vignal- Exposé CEA-CESTA, 25 Mars 2004- 4Diodes à forts courants (2) « Diode à forts courants E Plasma

  2. hal-00125705,version4-21Mar2007 Connected allocation to Poisson points in R2

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    hal-00125705,version4-21Mar2007 Connected allocation to Poisson points in R2 Maxim Krikun March 21, the elements of Rd ­ sites, and we write L for the Lebesgue measure in R2 . An allocation of Rd to X with appetite [0, ] is a measurable function : Rd X {, } such that L-1 () for all X and L-1 () = 0. We

  3. Project EARTH-12-BW2: An experimental study of the accretion and differentiation of Mars

    E-Print Network [OSTI]

    Henderson, Gideon

    Project EARTH-12-BW2: An experimental study of the accretion and differentiation of Mars Supervisor: Professor B J Wood Recent research has shown that the Earth accreted and differentiated over a time period of 30-40 M.yr and that Earth became more oxidised as it grew. Stable continental crust

  4. Evaluation of melting process of the permafrost on Mars: Its implication for surface features

    E-Print Network [OSTI]

    Manga, Michael

    . The point of our simulation is incorporation of thermal convection in porous media, which has not been in the melted zone causes drastic change in heat transfer, which results in focusing in the growth of the melt surface features around the outflow channels. INDEX TERMS: 6225 Planetology: Solar System Objects: Mars

  5. Aust. J. Mar. Freshw. Res., 1984, 35, 119-28 Aromatic Hydrocarbons in Waters of

    E-Print Network [OSTI]

    Canberra, University of

    Aust. J. Mar. Freshw. Res., 1984, 35, 119-28 Aromatic Hydrocarbons in Waters of Port Phillip Bay of aromatic hydrocarbons in coastal waters, using solvent extraction and fluorescence emission analysis, shows and the Yarra River estuary. Introduction Pollution of the marine environment by petroleum hydrocarbons

  6. Groundwater-controlled valley networks and the decline of surface runoff on early Mars

    E-Print Network [OSTI]

    Harrison, Keith

    Groundwater-controlled valley networks and the decline of surface runoff on early Mars Keith P was dominated by valley networks created through a combination of groundwater processes and surface runoff evolution characterized by a weakening of surface runoff, leaving groundwater processes as the dominant

  7. Ancient groundwater flow in the Valles Marineris on Mars inferred from

    E-Print Network [OSTI]

    Treiman, Allan H.

    LETTERS Ancient groundwater flow in the Valles Marineris on Mars inferred from fault trace ridges e-mail: treiman@lpi.usra.edu Published online: XX Month XXXX; doi:10.1038/ngeoXXXX Groundwater of bedrock3­6 .2 Understanding groundwater flow is also important for assessing3 the possibility of past

  8. Detection of copiapite in the northern Mawrth Vallis region of Mars: Evidence of acid sulfate alteration

    E-Print Network [OSTI]

    Glotch, Timothy D.

    coatings in acid mine drainage environments or in association with acid sulfate soils. The pres- enceDetection of copiapite in the northern Mawrth Vallis region of Mars: Evidence of acid sulfate of jarosite and copiapite indicates the presence of acidic waters. Such acid waters could have contrib- uted

  9. Catal Espaol English Canons i talussos profunds en els MARS Mediterrani i Cantbric: des de la

    E-Print Network [OSTI]

    Martin, Daniel

    Recursos Marins Renovables de l'Institut de Ciències del Mar del CSIC a Barcelona i el GRC d'estudi de les transferències de matèria i energia en l'oceà i en processos físics del fons marí, en biologia transferències de matèria i energia cap l'ecosistema profund. Des del punt de vista biològic, al Cantàbric es

  10. Dr. John Slough "Rapid Manned Mars Mission with a Propagating Magnetic Wave

    E-Print Network [OSTI]

    Shepherd, Simon

    Dr. John Slough MSNW "Rapid Manned Mars Mission with a Propagating Magnetic Wave Plasma Accelerator" For man to venture forth into the solar system, a radically different propulsion system must be envisioned problem. This is accomplished by employing a travelling magnetic wave accelerator to accelerate

  11. Mars aerosol studies with the MGS TES emission phase function observations: Optical depths, particle

    E-Print Network [OSTI]

    Whitney, Barbara A.

    aerosol properties to date. TES solar band and infrared (IR) spectral EPF sequences are analyzed to obtain and scattering of radiation; 6225 Planetology: Solar System Objects: Mars; KEYWORDS: Martian atmosphere, aerosols, radiative forcing from atmo- spheric dust solar absorption and thermal emission was recognized as a primary

  12. OBSERVATIONS OF PLASMA WAVES NEAR MARS AND THEIR IMPLICATIONS FOR ATMOSPHERIC LOSS. J. R. Espley1

    E-Print Network [OSTI]

    California at Berkeley, University of

    NASA Goddard Space Flight Center, Greenbelt, MD Summary: We use data from over 500 pre- mapping orbits (and therefore climate change). We present in this work observations of magnetic oscillations of Mars Global Surveyor magnetome- ter data to present statistical results on the characteris- tics

  13. An alkaline spring system within the Del Puerto Ophiolite (California, USA): A Mars analog site

    E-Print Network [OSTI]

    Meyers, Stephen R.

    that could be used in the search for evidence of life on Mars. & 2008 Elsevier Ltd. All rights reserved. 1 life-bearing systems. Serpentinization, the reaction of water with mafic minerals such as olivine is associated with the precipitation of Mg­Ca carbonate cements. The carbonates may serve as a biosignature

  14. Organisation of the soil mantle in tropical southeastern Brazil (Serra do Mar)

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Organisation of the soil mantle in tropical southeastern Brazil (Serra do Mar) in relation-900 Sao Paulo ­ SP, Brazil And INRA-ENSA. Laboratoire des sciences du sol 65 rue de St Brieuc 35042 RennesORSTOM - Instituto de geociencias - DGG ­ USP C.P. 11 348 Cep: 05 422-970 Sao Paulo ­ SP, Brazil Correspondence

  15. HJB---Mar/94 Theory of Local Observables and KMS--Condition

    E-Print Network [OSTI]

    that locality and spectrum condition seem to be good for defining acceptable dynamics. If we use the theoryHJB--- Mar/94 Theory of Local Observables and KMS--Condition Dedicated to Bert Schroer is a theory of local observables then it will be shown that locality condition implies that there do not exist

  16. Italian Forest Certification System Seeks Re-Endorsement by PEFC MAR 03 2010 | INTERNATIONAL

    E-Print Network [OSTI]

    Italian Forest Certification System Seeks Re-Endorsement by PEFC MAR 03 2010 | INTERNATIONAL process of national systems seeking recognition by PEFC at international level. The current endorsement in the standard setting forum," said Antonio Brunori, Secretary General of PEFC Italy. "The year- long process

  17. Mar Biol (2008) 154:465474 DOI 10.1007/s00227-008-0941-z

    E-Print Network [OSTI]

    2008-01-01

    Mar Biol (2008) 154:465­474 DOI 10.1007/s00227-008-0941-z 123 RESEARCH ARTICLE Tropical Wshes diversity, even in the eastern basin, pointing to an ancient colonization event. This suggests that both may reXect the re-colonization of areas in the Atlantic by Wsh that survived the cold phases in rela

  18. Energetic particles detected by the Electron Reflectometer instrument on the Mars

    E-Print Network [OSTI]

    California at Berkeley, University of

    ) spacecraft from May of 1999 to the mission conclusion in November 2006. Originally designed to detect low Reflectometer instrument on the Mars Global Surveyor, 1999­2006, Space Weather, 10, S06003, doi:10.1029/2012SW on the terrestrial environment is well known, and include communications and power disruptions, damage or even

  19. ccsd-00021119,version1-17Mar2006 Light transport in cold atoms and thermal decoherence

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ccsd-00021119,version1-17Mar2006 Light transport in cold atoms and thermal decoherence G. Labeyrie, we investigate experimentally and the- oretically how coherent transport of light inside a cold motivated by astrophysical purposes, wave transport in opaque media was first analyzed through a detailed

  20. Compositions of subsurface ices at the Mars Phoenix landing site Selby Cull,1

    E-Print Network [OSTI]

    Skemer, Philip

    Compositions of subsurface ices at the Mars Phoenix landing site Selby Cull,1 Raymond E. Arvidson,1 25 October 2010; accepted 2 November 2010; published 22 December 2010. [1] NASA's Phoenix Lander that broke during Robotic Arm operations; and a darker icy deposit. Spectra from the Phoenix Surface Stereo

  1. Mar. Drugs 2015, 13, 3154-3181; doi:10.3390/md13053154 marine drugs

    E-Print Network [OSTI]

    Paré, Paul W.

    Mar. Drugs 2015, 13, 3154-3181; doi:10.3390/md13053154 marine drugs ISSN 1660-3397 www.mdpi.com/journal/marinedrugs Review Molecular Architecture and Biomedical Leads of Terpenes from Red Sea Marine Invertebrates Mohamed Costantino Received: 9 April 2015 / Accepted: 7 May 2015 / Published: 20 May 2015 Abstract: Marine

  2. Thursday, March 26, 2009 POSTER SESSION II: MARS ANALOGS: CHEMICAL AND PHYSICAL

    E-Print Network [OSTI]

    Rathbun, Julie A.

    . Experimental Study of the Kinetics of CO2 Hydrate Dissociation Under Simulated Martian Conditions [#1341] We performed an experimental study of the kinetics of CO2 hydrate dissociation under simulated martian and Implications for Mars: Current Knowledge and Gaps [#2187] Terrestrial concretion analogs indicate that small

  3. Mar. Drugs 2013, 11, 4370-4389; doi:10.3390/md11114370 marine drugs

    E-Print Network [OSTI]

    Eirin Lopez, Jose Maria

    Mar. Drugs 2013, 11, 4370-4389; doi:10.3390/md11114370 marine drugs ISSN 1660-3397 www.mdpi.com/journal/marinedrugs Review Bivalve Omics: State of the Art and Potential Applications for the Biomonitoring of Harmful Marine of the marine ecosystem, constitute very valuable commercial resources in aquaculture, and have been widely used

  4. Mar 24th 2011 | from the print edition 0 40Like Battery technology

    E-Print Network [OSTI]

    Braun, Paul

    Mar 24th 2011 | from the print edition 0 40Like Battery technology Highly charged A powerful experimental battery that can be recharged completely in minutes ENGINEERS have long dreamed of shortening the time it takes to recharge batteries. Currently, that can be hours. For applications like motor vehicles

  5. LMS SUBSCRIPTION RATES & NOTES 2014/15 SUBSCRIPTION RATES

    E-Print Network [OSTI]

    1 LMS SUBSCRIPTION RATES & NOTES 2014/15 SUBSCRIPTION RATES LMS membership subscription: £ US.00 Associate membership 16.00 32.00 Free membership (see note 2) Print only Online only Print & online* LMS, or are unemployed or otherwise in hardship. Contact membership@lms.ac.uk to enquire further. #12;LMS PUBLICATIONS 4

  6. LMS SUBSCRIPTION RATES & NOTES 2013/14 SUBSCRIPTION RATES

    E-Print Network [OSTI]

    1 LMS SUBSCRIPTION RATES & NOTES 2013/14 SUBSCRIPTION RATES LMS membership subscription: £ US.00 Associate membership 15.00 30.00 Free membership (see note 2) Print only Online only Print & online* LMS, or are unemployed or otherwise in hardship. Contact membership@lms.ac.uk to enquire further. #12;LMS PUBLICATIONS 4

  7. Upper Great Plains Rates information

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

    3, 2014 (112 KB .pdf) FRN Notice of Proposed Transmission and Ancillary Services Formula Rates November 3, 2014 (93 KB .pdf) SPP Membership Information Integrated System (IS)...

  8. Sustainable Building Rating Systems Summary

    SciTech Connect (OSTI)

    Fowler, Kimberly M.; Rauch, Emily M.

    2006-07-01

    The purpose of this document is to offer information that could be used to compare and contrast sustainable building rating systems.

  9. Liquid Metal Flow Can Be One Clue to Explain the Frequently Observed Fluid-Like Matters on Mars

    E-Print Network [OSTI]

    Jing Liu; Yunxia Gao; Huangde Li

    2013-10-07

    The frequently discovered flooding structure on Mars and other planets has long been an intriguing mystery remained un-disclosed so far. Considering that on Earth, quite a few low melting point liquid metals or their alloy can be candidates of fluid like matters, we proposed here that there might also exists certain liquid metal instead of water or methane alone on Mars or the like planets. Compared with water, such liquid metal would be much easier to stay at the Mars surface because of its low melting point however extremely high evaporation point. Along this theoretical route, quite a few observations on the fluid like matters in former space explorations can be well interpreted. Such hypothesis for the existence of liquid metal on Mars surface does not mean refuting the possibility of water on Mars. This new point would be helpful for planning further exploration of Mars in a sense according to the characters of liquid metal. It at least identifies one more target fluid towards either finding or denying life at outer space. Whether the planet could harbor life in some form or it reaffirms Mars as an important future destination for human exploration still needs serious but not just enthusiasm explorations.

  10. Mapping analysis of scaffold/matrix attachment regions (s/MARs) from two different mammalian cell lines

    SciTech Connect (OSTI)

    Pilus, Nur Shazwani Mohd; Ahmad, Azrin; Yusof, Nurul Yuziana Mohd [School of Bioscience and Biotechnology, Faculty of Science and Technology, Universiti Kebangsaan Malaysia, 43600 Bangi, Selangor (Malaysia); Johari, Norazfa [Department of Chemical and Process Engineering, Faculty of Engineering and Built Environment, Universiti Kebangsaan Malaysia, 43600 Bangi, Selangor (Malaysia)

    2014-09-03

    Scaffold/matrix attachment regions (S/MARs) are potential element that can be integrated into expression vector to increase expression of recombinant protein. Many studies on S/MAR have been done but none has revealed the distribution of S/MAR in a genome. In this study, we have isolated S/MAR sequences from HEK293 and Chinese hamster ovary cell lines (CHO DG44) using two different methods utilizing 2 M NaCl and lithium-3,5-diiodosalicylate (LIS). The isolated S/MARs were sequenced using Next Generation Sequencing (NGS) platform. Based on reference mapping analysis against human genome database, a total of 8,994,856 and 8,412,672 contigs of S/MAR sequences were retrieved from 2M NaCl and LIS extraction of HEK293 respectively. On the other hand, reference mapping analysis of S/MAR derived from CHO DG44 against our own CHO DG44 database have generated a total of 7,204,348 and 4,672,913 contigs from 2 M NaCl and LIS extraction method respectively.

  11. Nuclear electric propulsion: A better, safer, cheaper transportation system for human exploration of Mars

    SciTech Connect (OSTI)

    Clark, J.S.; George, J.A.; Gefert, L.P.; Doherty, M.P.; Sefcik, R.J.

    1994-03-01

    NASA has completed a preliminary mission and systems study of nuclear electric propulsion (NEP) systems for split-sprint' human exploration and related robotic cargo missions to Mars. This paper describes the study, the mission architecture selected, the NEP system and technology development needs, proposed development schedules, and estimated development costs. Since current administration policy makers have delayed funding for key technology development activities that could make Mars exploration missions a reality in the near future, NASA will have time to evaluate various alternate mission options, and it appears prudent to ensure that Mars mission plans focus on astronaut and mission safety, while reducing costs to acceptable levels. The split-sprint nuclear electric propulsion system offers trip times comparable to nuclear thermal propulsion (NTP) systems, while providing mission abort opportunities that are not possible with reference' mission architectures. Thus, NEP systems offer short transit times for the astronauts, reducing the exposure of the crew to intergalactic cosmic radiation. The high specific impulse of the NEP system, which leads to very low propellant requirements, results in significantly lower initial mass in low earth orbit' (IMLEO). Launch vehicle packaging studies show that the NEP system can be launched, assembled, and deployed, with about one less 240-metric-ton heavy lift launch vehicle (HLLV) per mission opportunity - a very Technology development cost of the nuclear reactor for an NEP system would be shared with the proposed nuclear surface power systems, since nuclear systems will be required to provide substantial electrical power on the surface of Mars. The NEP development project plan proposed includes evolutionary technology development for nuclear electric propulsion systems that expands upon SP-100 (Space Power - 100 kw(e)) technology that has been developed for lunar and Mars surface nuclear power.

  12. Innovative Rates Program. Final report

    SciTech Connect (OSTI)

    Not Available

    1982-06-21

    Title II of the Energy Conservation and Production Act (ECPA) as amended by the Public Utility Regulatory Policies Act (PURPA) provided financial assistance to state utility regulatory commissions, nonregulated electric utilities, and the Tennessee Valley Authority through the Innovative Rates Program. The financial assistance was to be used to plan or carry out electric utility regulatory rate reform initiatives relating to innovative rate structures that encourage conservation of energy, electric utility efficiency and reduced costs, and equitable rates to consumers. The Federal and local objectives of the project are described. Activities planned and accomplishments are summarized for the following: project management, data collection, utility bill evaluation, billing enclosure/mailing evaluation, media program evaluation, display evaluation, rate study sessions evaluation, speakers bureau evaluation, and individual customer contacts. A timetable/milestone chart and financial information are included. (MHR)

  13. Downloaded 23 Mar 2004 to 155.101.19.17. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp Downloaded 23 Mar 2004 to 155.101.19.17. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/c

    E-Print Network [OSTI]

    Simons, Jack

    Downloaded 23 Mar 2004 to 155.101.19.17. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 23 Mar 2004 to 155.101.19.17. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 23 Mar 2004

  14. Downloaded 13 Mar 2004 to 129.97.80.195. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp Downloaded 13 Mar 2004 to 129.97.80.195. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/c

    E-Print Network [OSTI]

    Le Roy, Robert J.

    Downloaded 13 Mar 2004 to 129.97.80.195. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 13 Mar 2004 to 129.97.80.195. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 13 Mar 2004

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    E-Print Network [OSTI]

    Radin, Charles

    Downloaded 23 Mar 2004 to 146.6.139.170. Redistribution subject to AIP license or copyright, see http://jmp.aip.org/jmp/copyright.jsp #12;Downloaded 23 Mar 2004 to 146.6.139.170. Redistribution subject to AIP license or copyright, see http://jmp.aip.org/jmp/copyright.jsp #12;Downloaded 23 Mar 2004

  16. ALGORITHMIC CLASSIFICATION OF DRAINAGE NETWORKS ON MARS AND ITS RELATION TO MARTIAN GEOLOGICAL UNITS. T. F. Stepinski1

    E-Print Network [OSTI]

    Vilalta, Ricardo

    ALGORITHMIC CLASSIFICATION OF DRAINAGE NETWORKS ON MARS AND ITS RELATION TO MARTIAN GEOLOGICAL locations covering 16 major geological units. The classification is quantitative and objective with an existing division into geological units. A morphological interpretation for this emergent classification

  17. arXiv:cond-mat/0503226v19Mar2005 Two Superconducting Phases in the d = 3 Hubbard Model

    E-Print Network [OSTI]

    Gozuacik, Devrim

    arXiv:cond-mat/0503226v19Mar2005 Two Superconducting Phases in the d = 3 Hubbard Model: Phase. The strong-coupling phase, on the other hand, has characteristics of BEC-type superconductivity, including

  18. Enhancing the science return of Mars missions via sample preparation, robotic surface exploration and in orbit fuel production

    E-Print Network [OSTI]

    Lamamy, Julien-Alexandre, 1978-

    2004-01-01

    The future of Mars exploration is challenging from multiple points of view. To enhance their science return, future surface probes will most likely be equipped with complex Sample Preparation And Transfer (SPAT) facilities. ...

  19. SEASONAL SNOWMELT VERSUS IMPACT-TRIGGERED RUNOFF IN MARS' GEOLOGIC RECORD OF SURFACE LIQUID WATER. E. S. Kite1

    E-Print Network [OSTI]

    on Early Mars is retreat of water ice to planetary cold traps. (Melt- ing is also suppressed at low, forcing seasonal melting (Fig. 1b). Strong sensitivity to orbital forcing, plus the knowledge

  20. QUANTITATIVE ANALYSES OF TERRESTRIAL CRATER DEPOSITS: CONSTRAINING FORMATION AND SEDIMENT TRANSPORT PROCESSES ON MARS. M. S. Ramsey1

    E-Print Network [OSTI]

    Ramsey, Michael

    PROCESSES ON MARS. M. S. Ramsey1 and D. A. Crown2 , 1 Department of Geology and Planetary Science, University of Pittsburgh, Pittsburgh, PA, 15260, ramsey@ivis.eps.pitt.edu, 2 Planetary Science Institute

  1. HiRISE observations of gas sublimation-driven activity in Mars' southern polar regions: I. Erosion of the surface

    E-Print Network [OSTI]

    Byrne, Shane

    complete mar- tian southern spring. In some areas of the surface, beneath the conformal coating of seasonal' Antarctic circle. The capability of the MRO spacecraft to roll off-nadir and image features at different

  2. IX Encontro de tecnologia em Acstica Submarina IX ETAS Instituto de Estudos do Mar Almirante Paulo Moreira

    E-Print Network [OSTI]

    Jesus, Sérgio M.

    IX Encontro de tecnologia em Acústica Submarina ­ IX ETAS Instituto de Estudos do Mar Almirante properties variability is analysed using the Doppler spread function. #12;IX Encontro de tecnologia em

  3. Received 28 Jun 2013 | Accepted 5 Mar 2014 | Published 1 Apr 2014 The Vibrio cholerae type VI secretion system

    E-Print Network [OSTI]

    MacMillan, Andrew

    ARTICLE Received 28 Jun 2013 | Accepted 5 Mar 2014 | Published 1 Apr 2014 The Vibrio cholerae type, toxigenic V. cholerae passes through the gastric acid barrier, expresses TCP, secretes CT and colonizes

  4. Rate Adjustments and Public Involvement

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

    Letter to South Texas Electric Coop., Inc requesting an extension of the existing rate formula FalconAmistad WAPA-143 FERC Approval FalconAmistad Published WAPA-143 Falcon...

  5. Tier 2 Vintage Rate Workshop

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

    period FY2015 through 2028. Customers have a diversification right to limit the amount of power they purchase at the Load Growth rate in future years with notice provided by...

  6. Asset Prices and Exchange Rates

    E-Print Network [OSTI]

    Pavlova, Anna

    2003-08-01

    This paper develops a simple two-country, two-good model, in which the real exchange rate, stock and bond prices are jointly determined. The model predicts that ...

  7. Asset Prices and Exchange Rates

    E-Print Network [OSTI]

    Pavlova, Anna

    2004-11-30

    This paper develops a simple two-country, two-good model, in which the real exchange rate, stock and bond prices are jointly determined. The model predicts that stock market prices are correlated ...

  8. High repetition rate fiber lasers

    E-Print Network [OSTI]

    Chen, Jian, Ph. D. Massachusetts Institute of Technology

    2009-01-01

    This thesis reports work in high repetition rate femtosecond fiber lasers. Driven by the applications including optical arbitrary waveform generation, high speed optical sampling, frequency metrology, and timing and frequency ...

  9. High compression rate text summarization

    E-Print Network [OSTI]

    Branavan, Satchuthananthavale Rasiah Kuhan

    2008-01-01

    This thesis focuses on methods for condensing large documents into highly concise summaries, achieving compression rates on par with human writers. While the need for such summaries in the current age of information overload ...

  10. FIRST STEP IN THEORETICAL APPROACH IN STUDY OF MARS AND TITAN ATMOSPHERES WITH AN INDUCTIVELY COUPLED PLASMA TORCH

    E-Print Network [OSTI]

    with the titan atmosphere (CH4-N2) unlike the Mars atmosphere (CO2-N2). We observe the creation of solid], one can obtain the molar fraction versus temperature. The composition of Mars is assumed to be 97% CO22, CO2 - , N2O, N2O3, N2O4, N2O5, N2O+, N3, NCN, NO2, NO2 - , NO3, O3 and the electrons

  11. Modeling the variations of Dose Rate measured by RAD during the first MSL Martian year: 2012-2014

    E-Print Network [OSTI]

    Jingnan Guo; Cary Zeitlin; Robert F. Wimmer-Schweingruber; Scot Rafkin; Donald M. Hassler; Arik Posner; Bernd Heber; Jan Koehler; Bent Ehresmann; Jan K. Appel; Eckart Boehm; Stephan Boettcher; Soenke Burmeister; David E. Brinza; Henning Lohf; Cesar Martin; H. Kahanpaeae; Guenther Reitz

    2015-07-13

    The Radiation Assessment Detector (RAD), on board Mars Science Laboratory's (MSL) rover Curiosity, measures the {energy spectra} of both energetic charged and neutral particles along with the radiation dose rate at the surface of Mars. With these first-ever measurements on the Martian surface, RAD observed several effects influencing the galactic cosmic ray (GCR) induced surface radiation dose concurrently: [a] short-term diurnal variations of the Martian atmospheric pressure caused by daily thermal tides, [b] long-term seasonal pressure changes in the Martian atmosphere, and [c] the modulation of the primary GCR flux by the heliospheric magnetic field, which correlates with long-term solar activity and the rotation of the Sun. The RAD surface dose measurements, along with the surface pressure data and the solar modulation factor, are analysed and fitted to empirical models which quantitatively demonstrate} how the long-term influences ([b] and [c]) are related to the measured dose rates. {Correspondingly we can estimate dose rate and dose equivalents under different solar modulations and different atmospheric conditions, thus allowing empirical predictions of the Martian surface radiation environment.

  12. Modeling the variations of Dose Rate measured by RAD during the first MSL Martian year: 2012-2014

    E-Print Network [OSTI]

    Jingnan Guo; Cary Zeitlin; Robert F. Wimmer-Schweingruber; Scot Rafkin; Donald M. Hassler; Arik Posner; Bernd Heber; Jan Koehler; Bent Ehresmann; Jan K. Appel; Eckart Boehm; Stephan Boettcher; Soenke Burmeister; David E. Brinza; Henning Lohf; Cesar Martin; H. Kahanpaeae; Guenther Reitz

    2015-09-21

    The Radiation Assessment Detector (RAD), on board Mars Science Laboratory's (MSL) rover Curiosity, measures the {energy spectra} of both energetic charged and neutral particles along with the radiation dose rate at the surface of Mars. With these first-ever measurements on the Martian surface, RAD observed several effects influencing the galactic cosmic ray (GCR) induced surface radiation dose concurrently: [a] short-term diurnal variations of the Martian atmospheric pressure caused by daily thermal tides, [b] long-term seasonal pressure changes in the Martian atmosphere, and [c] the modulation of the primary GCR flux by the heliospheric magnetic field, which correlates with long-term solar activity and the rotation of the Sun. The RAD surface dose measurements, along with the surface pressure data and the solar modulation factor, are analysed and fitted to empirical models which quantitatively demonstrate} how the long-term influences ([b] and [c]) are related to the measured dose rates. {Correspondingly we can estimate dose rate and dose equivalents under different solar modulations and different atmospheric conditions, thus allowing empirical predictions of the Martian surface radiation environment.

  13. Comparison of Space Propulsion Methods for a Manned Mission to Mars

    E-Print Network [OSTI]

    Guerra, A G C; Gil, P J S

    2015-01-01

    We undertake a comparison of the latest developments in propulsion technologies, for a manned mission to Mars. The main objective is to assess the possibility of reducing travel time keeping the mass at departure within bounds. For the sake of comparison we used representative systems of different state of the art or proposed technologies, from the chemical engine to the "Pure Electro-Magnetic Thrust" (PEMT) concept, using a nuclear engine proposed by Rubbia. A mission architecture is suggested, based on existing mission proposals to Mars, to estimate the mass budget that influences the performance of the propulsion system. The trajectory of the spacecraft is determined by a numerical integration of the equations of motion and a partial optimization procedure, for the interplanetary phase with continuous thrust, and by conics and instant manoeuvres in the regions of influence of the departure and arrival planets. Pareto curves of the duration of the mission and time of flight versus mass of mission are drawn....

  14. A LANL Scientist's Dream Takes Off to Zap Rocks on Mars

    ScienceCinema (OSTI)

    Wiens, Roger

    2012-08-02

    Roger Wiens, with a team of 40 people at Los Alamos National Laboratory and the collaboration of the French space institute IRAP, created ChemCam, a laser spectrometer and telescope device aboard the Curiosity rover. ChemCam will blast rocks from as far as 7 meters, vaporize bits of their surfaces, and spectroscopically determine their chemical composition, aiding in the search for life on Mars, and making this scientist's boyhood dream a reality.

  15. ChemCam for Mars Science Laboratory rover, undergoing pre-flight testing

    ScienceCinema (OSTI)

    None

    2014-08-12

    Los Alamos National Laboratory and partners developed a laser instrument, ChemCam, that will ride on the elevated mast of the Mars Science Laboratory rover Curiosity. The system allows Curiosity to "zap" rocks from a distance, reading their chemical composition through spectroscopic analysis. In this video, laboratory shaker-table testing of the instrument ensures that all of its components are solidly attached and resistant to damage from the rigors of launch, travel and landing.

  16. The Mars thermosphere. 2. General circulation with coupled dynamics and composition

    SciTech Connect (OSTI)

    Bougher, S.W. (Univ. of Arizona, Tucson (USA)); Roble, R.G.; Ridley, E.C.; Dickinson, R.E. (National Center for Atmospheric Research, Boulder, CO (USA))

    1990-08-30

    The National Center for Atmospheric Research thermospheric general circulation model (TGCM) for the Earth's thermosphere has been modified to examine the three-dimensional structure and circulation of the upper mesosphere and thermosphere of Mars (MTGCM). The computational framework and major processes unique to a CO{sub 2} thermosphere are similar to those utilized in a recent Venus TGCM. Solar EUV, UV, and IR heating alone combine to drive the Martian winds above {approximately}100 km. An equinox version of the code is used to examine the Mars global dynamics and structure for two specific observational periods spanning a range of solar activity: Viking 1 (July 1976) and Mariner 6-7 (August-September 1969). The MTGCM is then modified to predict the state of the Mars thermosphere for various combinations of solar and orbital conditions. Calculations show that no nightside cryosphere of the type observed on Venus is obtained on the Mars nightside. Instead, planetary rotation significantly modifies the winds and the day-to-night contrast in densities and temperatures, giving a diurnal behavior similar to the Earth under quiet solar conditions. Maximum exospheric temperatures are calculated near 1,500 LT ({le} 305 K), with minimum values at 0500 LT ({le} 175 K). The global temperature distribution is strongly modified by nightside adiabatic heating (subsidence) and dayside cooling (upwelling). The global winds also affect vertical density distributions; vertical eddy diffusion much weaker than used in previous one-dimensional models is required to maintain observed Viking profiles. A solar cycle variation in dayside exospheric temperatures of {approximately}195-305 K is simulated by the Viking and Mariner runs.

  17. Development of a propulsion system and component test facility for advanced radioisotope powered Mars Hopper platforms

    SciTech Connect (OSTI)

    Robert C. O'Brien; Nathan D. Jerred; Steven D. Howe

    2011-02-01

    Verification and validation of design and modeling activities for radioisotope powered Mars Hopper platforms undertaken at the Center for Space Nuclear Research is essential for proof of concept. Previous research at the center has driven the selection of advanced material combinations; some of which require specialized handling capabilities. The development of a closed and contained test facility to forward this research is discussed within this paper.

  18. 125 total creditsMar. 15, 2013 (offered Fall/Spring)

    E-Print Network [OSTI]

    Carver, Jeffrey C.

    125 total creditsMar. 15, 2013 CH 101 General Chemistry 4 cr ECE 121 or ENGR 111 1 cr (offered Fall to Linear Algebra 3 cr ECE 285 Prog. for ECE 3 cr (offered Fall/Spring) CS 150 Programming I 2 cr PH106 cr (offered Fall/Spring) CS 351 CS Programming III 2 cr ECE380 Digital Logic 4 cr (offered Fall

  19. 125 total creditsMar. 15, 2013 (offered Fall/Spring)

    E-Print Network [OSTI]

    Carver, Jeffrey C.

    125 total creditsMar. 15, 2013 CH 101 General Chemistry 4 cr ECE 121 or ENGR 111 1 cr (offered Fall to Linear Algebra 3 cr ECE 285 Prog. for ECE 3 cr (offered Fall/Spring) CS 150 Programming I 2 cr PH106 cr (offered Fall/Spring) CS 351 CS Programming III 2 cr ECE 380 Digital Logic 4 cr (offered Fall

  20. Coal Transportation Rate Sensitivity Analysis

    Reports and Publications (EIA)

    2005-01-01

    On December 21, 2004, the Surface Transportation Board (STB) requested that the Energy Information Administration (EIA) analyze the impact of changes in coal transportation rates on projected levels of electric power sector energy use and emissions. Specifically, the STB requested an analysis of changes in national and regional coal consumption and emissions resulting from adjustments in railroad transportation rates for Wyoming's Powder River Basin (PRB) coal using the National Energy Modeling System (NEMS). However, because NEMS operates at a relatively aggregate regional level and does not represent the costs of transporting coal over specific rail lines, this analysis reports on the impacts of interregional changes in transportation rates from those used in the Annual Energy Outlook 2005 (AEO2005) reference case.

  1. Fast repetition rate (FRR) flasher

    DOE Patents [OSTI]

    Kolber, Z.; Falkowski, P.

    1997-02-11

    A fast repetition rate (FRR) flasher is described suitable for high flash photolysis including kinetic chemical and biological analysis. The flasher includes a power supply, a discharge capacitor operably connected to be charged by the power supply, and a flash lamp for producing a series of flashes in response to discharge of the discharge capacitor. A triggering circuit operably connected to the flash lamp initially ionizes the flash lamp. A current switch is operably connected between the flash lamp and the discharge capacitor. The current switch has at least one insulated gate bipolar transistor for switching current that is operable to initiate a controllable discharge of the discharge capacitor through the flash lamp. Control means connected to the current switch for controlling the rate of discharge of the discharge capacitor thereby to effectively keep the flash lamp in an ionized state between successive discharges of the discharge capacitor. Advantageously, the control means is operable to discharge the discharge capacitor at a rate greater than 10,000 Hz and even up to a rate greater than about 250,000 Hz. 14 figs.

  2. MEDICAL RATES for Active Employees

    E-Print Network [OSTI]

    New Mexico, University of

    -time, your base salary is calculated on the full-time equivalent. For example, if you are at an appointment percentage of 50% and earn $12,000 per year, your base salary is $24,000 and UNM would contribute 40%. UNM Health-Bi-Weekly Rates Annualized Salary $34,999 and below Annualized Salary $35,000 - $49,999 Annualized

  3. Fast repetition rate (FRR) flasher

    DOE Patents [OSTI]

    Kolber, Zbigniew (Shoreham, NY); Falkowski, Paul (Stony Brook, NY)

    1997-02-11

    A fast repetition rate (FRR) flasher suitable for high flash photolysis including kinetic chemical and biological analysis. The flasher includes a power supply, a discharge capacitor operably connected to be charged by the power supply, and a flash lamp for producing a series of flashes in response to discharge of the discharge capacitor. A triggering circuit operably connected to the flash lamp initially ionizes the flash lamp. A current switch is operably connected between the flash lamp and the discharge capacitor. The current switch has at least one insulated gate bipolar transistor for switching current that is operable to initiate a controllable discharge of the discharge capacitor through the flash lamp. Control means connected to the current switch for controlling the rate of discharge of the discharge capacitor thereby to effectively keep the flash lamp in an ionized state between Successive discharges of the discharge capacitor. Advantageously, the control means is operable to discharge the discharge capacitor at a rate greater than 10,000 Hz and even up to a rate greater than about 250,000 Hz.

  4. THE MARS HOPPER: AN IMPULSE DRIVEN, LONG RANGE, LONG-LIVED MOBILE PLATFORM UTILIZING IN-SITU MARTIAN RESOURCES

    SciTech Connect (OSTI)

    Robert C. O'Brien; Mark McKay; Brian Gross; JOnathan Webb

    2001-09-01

    The requirements for performance by planetary exploration missions are increasing. Landing at a single location to take data is no longer sufficient. Due to the increasing cost, the missions that provide mobile platforms that can acquire data at displaced locations are becoming more attractive. Landers have also had limited range due to power limitations, limited lifetime of subsystems and the inability to negotiate rough terrain. The Center for Space Nuclear Research has designed an instrumented platform that can acquire detailed data at hundreds of locations during its lifetime - a Mars Hopper. The Mars Hopper concept utilizes energy from radioisotopic decay in a manner different from any existing radioisotopic power sources—as a thermal capacitor. By accumulating the heat from radioisotopic decay for long periods, the power of the source can be dramatically increased for short periods. Thus, a radioisotopic thermal rocket (RTR) is possible. The platform will be able to “hop” from one location to the next every 5-7 days with a separation of 5-10 km per hop. Each platform will weigh around 50 kgs unfueled which is the condition at deployment. Consequently, several platforms may be deployed on a single launch from Earth. With a lifetime estimated at 5-7 years, the entire surface of Mars can be mapped in detail by a couple dozen platforms. In addition, Hoppers can collect samples and deliver them to the Mars Science Laboratory for more detailed analysis. The design and performance of the Mars Hopper will be discussed.

  5. Electric Rate Alternatives to Cogeneration 

    E-Print Network [OSTI]

    Sandberg, K. R. Jr.

    1988-01-01

    ALTERNATIVES TO COGENERATION" K. R. SANDBERG, JR. INDUSTRIAL ACCOUNTS MANAGER - TEXAS GULF STATES UTILITIES COMPANY BEAUMONT, TEXAS ABSTRACT This paper discusses electric rate slternatives to cogeneration for the industrisl customer and attempts... electricity to municipalities and rural electric cooperatives in both Texas and Louisiana. In Baton Rouge. GSU supplies steam and electricity to a large industrial customer through a cogeneration facility that the company has had in operation since...

  6. Cooling rate, heating rate and aging effects in glassy water

    E-Print Network [OSTI]

    Nicolas Giovambattista; H. Eugene Stanley; Francesco Sciortino

    2004-03-03

    We report a molecular dynamics simulation study of the properties of the potential energy landscape sampled by a system of water molecules during the process of generating a glass by cooling, and during the process of regenerating the equilibrium liquid by heating the glass. We study the dependence of these processes on the cooling/heating rates as well as on the role of aging (the time elapsed in the glass state). We compare the properties of the potential energy landscape sampled during these processes with the corresponding properties sampled in the liquid equilibrium state to elucidate under which conditions glass configurations can be associated with equilibrium liquid configurations.

  7. WP-07 Power Rate Case (rates/ratecases)

    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 /Two0Photos and Videos Videos Re-EntryApproval OMB No.:Rates

  8. October 1996 - September 2001 Wholesale Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power are

  9. October 2001 - March 2002 Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power

  10. October 2001 - September 2006 Wholesale Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power1 -

  11. October 2002 - March 2003 Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power1

  12. October 2003 - March 2004 Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power13 -

  13. October 2004 - March 2005 Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power13

  14. October 2005 - March 2006 Power Rates (rates/previous)

    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 mapSpeeding access toOctober 1996 - September 2001 The rates BPA charges for power135

  15. WP-07 Rate Case Workshops (rates/meetings)

    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 WithTelecentricN A 035(92/02) nerg *415,Rates > Meetings &

  16. Rate Schedule CV-SPR4

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

    that is available immediately to serve load and is synchronized with the power system. Formula Rate: The formula rate for spinning reserve includes three components: Component 1:...

  17. Rate Schedule CV-SUR4

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

    within the first 10 minutes to take load and is synchronized with the power system. Formula Rate: The formula rate for supplemental reserve service includes three components:...

  18. Rate Schedule COTP-T3

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

    and system control and dispatch service needed to support the transmission service. Formula Rate: The formula rate for COTP firm and non-firm PTP transmission service includes...

  19. Rate Schedule CV-NWT5

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

    and system control and dispatch service needed to support the transmission service. Formula Rate: The formula rate for CVP NITS includes three components: Component 1: The NITS...

  20. Rate Schedule PACI-T3

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

    and system control and dispatch service needed to support the transmission service. Formula Rate: The formula rate for PACI firm and non-firm transmission includes three...

  1. Rate Schedule CV-RFS4

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

    load and for maintaining scheduled interconnection frequency at 60-cycles per second. Formula Rate: The formula rate for regulation includes three components: Component 1: Annual...

  2. Rate Schedule CV-EID4

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

    that is established in the service agreement or Interconnected Operations Agreements. Formula Rate: The formula rate for EI service includes three components: Component 1: EI...

  3. Mars north polar dunes: possible formation from low-density sediment aggregates

    SciTech Connect (OSTI)

    Saunders, R.S.; Blewett, D.T.

    1987-10-01

    Low-density aggregates, composed of submicron clay aerosols, have been formed experimentally as the sublimation residues of masses of dust-nucleated ice. These ice-dust mixtures are possible analogues of materials of Martian north polar deposits. Low-density (0.002 g/cm/sup 3/) spheroidal pellets formed from these materials in wind tunnel experiments have been examined as possible candidates for forming north polar dunes on Mars. It is shown that these particles move like sand grains under conditions of saltation and, given a sufficient supply, would be capable of forming the dunes observed in the north circumpolar erg.

  4. MHK ISDB/Instruments/AirMar G2183 GPS Antenna | 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 View NewTexas:Montezuma, Arizona:Oregon:LowellMHK ISDB/Instruments/ACM-WAVE-PLUSMHKMHKMHKMHKAirMar

  5. ChemCam on Mars (Technical Report) | SciTech Connect

    Office of Scientific and Technical Information (OSTI)

    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 MunicipalTechnical Report: Achievements ofCOMPOSITION OF VAPORS FROM BOILINGChemCam on Mars Citation

  6. GEOPHYSICAL RESEARCH LETTERS, VOL. 40, 16, doi:10.1002/grl.50415, 2013 The importance of pickup oxygen ion precipitation to the Mars upper

    E-Print Network [OSTI]

    Johnson, Robert E.

    by the fields in the solar wind. Ion precipitation and their impact on the Mars atmosphere has been extensively oxygen ion precipitation to the Mars upper atmosphere under extreme solar wind conditions Xiaohua Fang,1 to very important when upstream solar wind conditions vary from normal to extreme. The atmospheric

  7. Nomad rover field experiment, Atacama desert, Chile 2. Identification of paleolife evidence using a robotic vehicle: Lessons and recommendations for a Mars sample return mission

    E-Print Network [OSTI]

    Cabrol, N. A.; Bettis III, E. A.; Glenister, B. F.; Chong, G.; Herrera, C.; Jensen, A.; Pereira, M.; Stoker, R.; Grin, E. A.; Landheim, R.; Thomas, G.; Golden, Jennifer E.; Saville, K.; Ludvigson, Gregory A.; Witzke, B.

    2001-04-25

    69-G81, 1970. Ramirez, C. F., and M. Gardeweg, Carta geo16gica de Chile, region de Antofagasta, scale 1:250,000, Serv. Nac. de Geol. y Mineria Chile, 1982. Squyres, S. W., et al., The Athena Mars Rover Science Payload, paper presented at Mars...

  8. Mars And Beyond: Human Spaceflight at the Museum of Science Boston Joseph Paul Cohen at the University of Massachuestts Boston, and Julia Sable at the Museum of Science Boston, and

    E-Print Network [OSTI]

    Ding, Wei

    on the Apollo and Orion missions, space suits, Mars settlement, and 3D printing (a technique for making needed

  9. Power Rates Study Final Proposal

    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 mapSpeedingProgram Guidelines This document w w w.pv - te ch.orgPower PlantRates >5

  10. Rate Schedules | 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: Alternative FuelsofProgram: Report Appendices |ProjectKnow Your PowerWeatherize »Rain orRate

  11. Downloaded 22 Mar 2001 to 157.182.50.14. Redistribution subject to AIP copyright, see http://ojps.aip.org/chaos/chocr.jsp Downloaded 22 Mar 2001 to 157.182.50.14. Redistribution subject to AIP copyright, see http://ojps.aip.org/chaos/chocr.jsp

    E-Print Network [OSTI]

    Showalter, Kenneth

    Downloaded 22 Mar 2001 to 157.182.50.14. Redistribution subject to AIP copyright, see http://ojps.aip.org/chaos/chocr.jsp #12;Downloaded 22 Mar 2001 to 157.182.50.14. Redistribution subject to AIP copyright, see http://ojps.aip.org/chaos/chocr.jsp #12;Downloaded 22 Mar 2001 to 157.182.50.14. Redistribution subject to AIP copyright, see http

  12. Downloaded 08 Mar 2002 to 129.7.12.23. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/japo/japcr.jsp Downloaded 08 Mar 2002 to 129.7.12.23. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/japo/japcr

    E-Print Network [OSTI]

    Economou, Demetre J.

    Downloaded 08 Mar 2002 to 129.7.12.23. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/japo/japcr.jsp #12;Downloaded 08 Mar 2002 to 129.7.12.23. Redistribution subject to AIP license or copyright, see to AIP license or copyright, see http://ojps.aip.org/japo/japcr.jsp #12;Downloaded 08 Mar 2002 to 129

  13. What Is the Right Rate? Loan Rates and Demand | Department of...

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

    What Is the Right Rate? Loan Rates and Demand What Is the Right Rate? Loan Rates and Demand Better Buildings Neighborhood Program Financing Peer Exchange Call: "What is the Right...

  14. Combined Retrieval, Microphysical Retrievals and Heating Rates

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

    Feng, Zhe

    2013-02-22

    Microphysical retrievals and heating rates from the AMIE/Gan deployment using the PNNL Combined Retrieval.

  15. Combined Retrieval, Microphysical Retrievals and Heating Rates

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

    Feng, Zhe

    Microphysical retrievals and heating rates from the AMIE/Gan deployment using the PNNL Combined Retrieval.

  16. A low-alpha nuclear electric propulsion system for lunar and Mars missions

    SciTech Connect (OSTI)

    Coomes, E.P.; Dagle, J.E.

    1992-01-01

    The advantages of using electric propulsion are well-known in the aerospace community. The high specific impulse and, therefore, lower propellant requirements make it a very attractive propulsion option for the Space Exploration Initiative (SEI). Recent studies have shown that nuclear electric propulsion (NEP) is not only attractive for the transport of cargo but that fast piloted missions to Mars are possible as well, with alphas on the order of 7.5 kg/kW. An advanced NEP system with a specific power (alpha) of 2.5 kg/kW or less would significantly enhance the manned mission option of NEP by reducing the trip time even further. This paper describes an advanced system that combines the PEGASUS Drive with systems of the Rotating Multimegawatt Boiling Liquid Metal (RMBLR) power system that was developed as part of the DOE multimegawatt program and just recently declassified. In its original configuration, the PEGASUS Drive was a 10-MWe propulsion system. The RMBLR was a 20-MW electric system. By combining the two, a second-generation PEGASUS Drive can be developed with an alpha less than 2.5 kg/kW. This paper will address the technology advancements incorporated into the PEGASUS Drive, the analysis of a fast piloted mission and an unmanned cargo transport Mars mission, and the integration of laser power beaming to provide surface power.

  17. Extensibility of the fission surface power (FSP) system from the moon to Mars

    SciTech Connect (OSTI)

    Poston, David Irvin

    2011-01-28

    Fission reactors have great near-term potential to power human and robotic missions/outposts on the surface of the Moon and Mars (and potentially other planets, moons, and asteroids). The ability to provide a power-rich environment that is independent of solar intensity, nights, dust storms, etc., is of significant (perhaps enabling) importance to the further expansion of humans into our solar system. NASA's Reference Fission Surface Power (FSP) System is a 40 kWe system that has been primarily designed for lunar applications. This paper examines the extensibility of the FSP design and technology for potential missions on Mars. Possible impacts include the effects of changes in heat sink, gravity, day-night cycles, mission transit time, communication delay, and the chemistry of the regolith and atmosphere. One of the biggest impacts might be differences in the potential utilization of in-situ materials for shielding. Another major factor is that different missions will likely require different performance requirements, e.g. power, lifetime and mass. This paper concludes that the environmental differences between potential mission locations will not require significant changes in design and technologies, unless performance requirements for a specific mission are substantially different than those adopted for the FSP The primary basis for this conclusion is that the FSP has been designed with robust materials and design margins.

  18. A scaling law for aeolian dunes on Mars, Venus, Earth, and for subaqueous ripples

    E-Print Network [OSTI]

    Philippe Claudin; Bruno Andreotti

    2006-08-07

    The linear stability analysis of the equations governing the evolution of a flat sand bed submitted to a turbulent shear flow predicts that the wavelength $\\lambda$ at which the bed destabilises to form dunes should scale with the drag length $L_{\\rm drag} = \\frac{\\rho_s}{\\rho_f} d$. This scaling law is tested using existing and new measurements performed in water (subaqueous ripples), in air (aeolian dunes and fresh snow dunes), in a high pressure CO$_2$ wind tunnel reproducing conditions close to the Venus atmosphere and in the low pressure CO$_2$ martian atmosphere (martian dunes). A difficulty is to determine the diameter of saltating grains on Mars. A first estimate comes from photographs of aeolian ripples taken by the rovers Opportunity and Spirit, showing grains whose diameters are smaller than on Earth dunes. In addition we calculate the effect of cohesion and viscosity on the dynamic and static transport thresholds. It confirms that the small grains visualised by the rovers should be grains experiencing saltation. Finally, we show that, within error bars, the scaling of $\\lambda$ with $L_{\\rm drag}$ holds over almost five decades. We conclude with a discussion on the time scales and velocities at which these bed instabilities develop and propagate on Mars.

  19. Interactive Evolution of Multiple Water-Ice Reservoirs on Mars: Insights from Hydrogen Isotope Compositions

    E-Print Network [OSTI]

    Kurokawa, Hiroyuki; Sato, Masahiko

    2015-01-01

    Remote sensing data from orbiter missions have proposed that ground ice may currently exist on Mars, although the volume is still uncertain. Recent analyses of Martian meteorites have suggested that the water reservoirs have at least three distinct hydrogen isotope compositions (D/H ratios): primordial and high D/H ratios, which are approximately the same and six times that of ocean water on Earth, respectively, and a newly identified intermediate D/H ratio, which is approximately two to three times higher than that in ocean water on Earth. We calculate the evolution of the D/H ratios and the volumes of the water reservoirs on Mars by modeling the exchange of hydrogen isotopes between multiple water reservoirs and the atmospheric escape. The D/H ratio is slightly higher in the topmost thin surface-ice layer than that in the atmosphere because of isotopic fractionation by sublimation, whereas the water-ice reservoir just below the exchangeable topmost surface layer retains the intermediate D/H signature found ...

  20. Nuclear Risk Assessment for the Mars 2020 Mission Environmental Impact Statement

    SciTech Connect (OSTI)

    Clayton, Daniel J.; Bignell, John; Jones, Christopher A.; Rohe, Daniel P.; Flores, Gregg J.; Bartel, Timothy J.; Gelbard, Fred; Le, San; Morrow, Charles W.; Potter, Donald L.; Young, Larry W.; Bixler, Nathan E.; Lipinski, Ronald J.

    2014-01-01

    In the summer of 2020, the National Aeronautics and Space Administration (NASA) plans to launch a spacecraft as part of the Mars 2020 mission. One option for the rover on the proposed spacecraft uses a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) to provide continuous electrical and thermal power for the mission. An alternative option being considered is a set of solar panels for electrical power with up to 80 Light-Weight Radioisotope Heater Units (LWRHUs) for local component heating. Both the MMRTG and the LWRHUs use radioactive plutonium dioxide. NASA is preparing an Environmental Impact Statement (EIS) in accordance with the National Environmental Policy Act. The EIS will include information on the risks of mission accidents to the general public and on-site workers at the launch complex. This Nuclear Risk Assessment (NRA) addresses the responses of the MMRTG or LWRHU options to potential accident and abort conditions during the launch opportunity for the Mars 2020 mission and the associated consequences. This information provides the technical basis for the radiological risks of both options for the EIS.

  1. Property:OpenEI/UtilityRate/DemandRateStructure/Tier4Rate | Open Energy

    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,AltFuelVehicle2 JumpPublicationDate Jump to:InformationEnergyInformation Rate Jump

  2. mar015

    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-effectWorkingLosThe 26th AnnualHistoryM aterialsmFUSE: Functionmanaging the` [ ` [

  3. 05Mar09 ANALYSISIn crisis, GE finds its deep bench not so magical By James B. Kelleher

    E-Print Network [OSTI]

    Kuzmanovic, Aleksandar

    05Mar09 ANALYSISIn crisis, GE finds its deep bench not so magical By James B. Kelleher CHICAGO, March 5 (Reuters) Crotonville, we have a problem. The travails of General Electric Co GE and expensive training program credited with creating those managers. In recent weeks, GE executives have

  4. Flow in seagrass canopies: The influence of patch width Mark S. Fonseca*, M.A.R. Koehl

    E-Print Network [OSTI]

    Koehl, Mimi

    Flow in seagrass canopies: The influence of patch width Mark S. Fonseca*, M.A.R. Koehl Department published on the inter- action of seagrass canopies with flowing water has been derived from laboratory flume studies. The few studies that have been conducted all point to similar patterns of flow alteration

  5. arXiv:1103.0628v1[astro-ph.IM]3Mar2011 Bivariate least squares linear regression

    E-Print Network [OSTI]

    Masci, Frank

    arXiv:1103.0628v1[astro-ph.IM]3Mar2011 Bivariate least squares linear regression: towards a unified squares linear regression, the classical ap- proach pursued for functional models in earlier attempts are regression lines in the general case of correlated errors in X and in Y for heteroscedastic data

  6. NASA's newest Mars orbiter is a spacecraft designed to find out what the planet is made of,

    E-Print Network [OSTI]

    water and shallow buried ice and study the radiation environment. The surface of Mars has long been more fuel. Science Goals The orbiter mission will study and globally map the elemental composition measurements of the planet's radiation environ- ment that can be used to evaluate the potential health risks

  7. ccsd-00001341(version1):23Mar2004 Hanbury-Brown Twiss correlations to probe the population

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ccsd-00001341(version1):23Mar2004 Hanbury-Brown Twiss correlations to probe the population the first study of the statistics of GHz photons in quantum circuits, using Hanbury- Brown and Twiss experiment of Hanbury-Brown and Twiss (HBT)[1], consisted in two detec- tors correlating the power

  8. Talk to Inside-Outside Workshop, Senate House, Londond 10 Mar 2010 Workshop: Inside and Outside of Computers and Minds

    E-Print Network [OSTI]

    Sloman, Aaron

    Talk to Inside-Outside Workshop, Senate House, Londond 10 Mar 2010 Workshop: Inside and Outside with capabilities matching those of orangutans, corvids, human toddlers, and probably many other animals · will need. · We now, as a result of a great deal of work on hardware, software, firmware, and CS theory, know how

  9. Development of the Variable Atmosphere Testing Facility for Blow-Down Analysis of the Mars Hopper Prototype

    SciTech Connect (OSTI)

    Nathan D. Jerred; Robert C. O'Brien; Steven D. Howe; James E. O'Brien

    2013-02-01

    Recent developments at the Center for Space Nuclear Research (CSNR) on a Martian exploration probe have lead to the assembly of a multi-functional variable atmosphere testing facility (VATF). The VATF has been assembled to perform transient blow-down analysis of a radioisotope thermal rocket (RTR) concept that has been proposed for the Mars Hopper; a long-lived, long-ranged mobile platform for the Martian surface. This study discusses the current state of the VATF as well as recent blow-down testing performed on a laboratory-scale prototype of the Mars Hopper. The VATF allows for the simulation of Mars ambient conditions within the pressure vessel as well as to safely perform blow-down tests through the prototype using CO2 gas; the proposed propellant for the Mars Hopper. Empirical data gathered will lead to a better understanding of CO2 behavior and will provide validation of simulation models. Additionally, the potential of the VATF to test varying propulsion system designs has been recognized. In addition to being able to simulate varying atmospheres and blow-down gases for the RTR, it can be fitted to perform high temperature hydrogen testing of fuel elements for nuclear thermal propulsion.

  10. British Geomorphological Research Group, Annual Meeting, Oxford, 2003. An analysis and classification of 'barchan' dunes on Mars.

    E-Print Network [OSTI]

    Bourke, Mary C.

    and classification of 'barchan' dunes on Mars. Bourke, M.C., and Balme, M. School of Geography and the Environment, University of Oxford, Oxford, OX1 3TB, UK. Mary.bourke@geog.ox.ac.uk Martian sand dunes have the potential and morphodynamics. Recognition of the characteristics of both recent and ancient dunes is the first step towards

  11. Recent aeolian dune change on Mars M.C. Bourke a,b,, K.S. Edgett c

    E-Print Network [OSTI]

    Bourke, Mary C.

    Recent aeolian dune change on Mars M.C. Bourke a,b,, K.S. Edgett c , B.A. Cantor c a Planetary 2007 Abstract Previous comparisons of Martian aeolian dunes in satellite images have not detected any change in dune form or position. Here, we show dome dunes in the north polar region that shrank

  12. arXiv:0903.3329v1[cs.LG]19Mar2009 Optimal Policies Search for Sensor Management

    E-Print Network [OSTI]

    Del Moral , Pierre

    complex sensor(s)-based systems which supply the decision centers with an increasing amount of data) Radar to propose management scheme during the detection step. In [7]­[9] an information-based approacharXiv:0903.3329v1[cs.LG]19Mar2009 Optimal Policies Search for Sensor Management : Application

  13. The solar wind interaction with Mars: Recent progress and future directions The Sun has a powerful influence on planetary atmospheres.

    E-Print Network [OSTI]

    California at Berkeley, University of

    Editorial The solar wind interaction with Mars: Recent progress and future directions The Sun has field, because the solar wind can interact directly with the upper atmo- sphere. Neutral particles in the upper atmosphere are ionized by solar photons and through interactions with solar wind charged particles

  14. Problems #7, Math 311, Dr. M. Bohner. Mar 19, 2003. Due Apr 2, 1 pm. 138. Let A =

    E-Print Network [OSTI]

    Bohner, Martin

    Problems #7, Math 311, Dr. M. Bohner. Mar 19, 2003. Due Apr 2, 1 pm. 138. Let A = a b b c . Show by f(x, y, z) = (x2 +2y2 )e-(x2+y2) +zez . 147. In order to produce a box we have two materials

  15. On the Semiclassical Jacobi Algorithm \\Lambda Mar'ia T. C'amara and Domingo Gim'enez y

    E-Print Network [OSTI]

    Giménez, Domingo

    Chapter 1 On the Semiclassical Jacobi Algorithm \\Lambda Mar'ia T. C'amara and Domingo Gim'enez y Abstract In this paper a new Jacobi method to solve the symmetric eigenvalue problem is presented Jacobi methods. By combining this method with an adequate threshold strategy a reduction in the execution

  16. MGS MAG/ER observations at the magnetic pileup boundary of Mars: draping enhancement and low frequency waves

    E-Print Network [OSTI]

    California at Berkeley, University of

    MGS MAG/ER observations at the magnetic pileup boundary of Mars: draping enhancement and low Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA Received 26 November 2002; received in revised form 19 March 2003; accepted 24 April 2003 Abstract The magnetic pileup boundary (MPB) is a sharp

  17. Received 7 Dec 2013 | Accepted 11 Feb 2014 | Published 4 Mar 2014 Radial-arrayed rotary electrification for high

    E-Print Network [OSTI]

    Wang, Zhong L.

    ARTICLE Received 7 Dec 2013 | Accepted 11 Feb 2014 | Published 4 Mar 2014 Radial-arrayed rotary of Materials Science and Engineering, Georgia Institute of Technology, Atlanta, Georgia 30332, USA (TEG) for producing energy from rotary surfaces with unprece- dented performance. Enabled by a design

  18. Received 5 Mar 2014 | Accepted 11 Jul 2014 | Published 18 Aug 2014 Sea surface temperature contributes to marine

    E-Print Network [OSTI]

    Benton, Michael

    ARTICLE Received 5 Mar 2014 | Accepted 11 Jul 2014 | Published 18 Aug 2014 Sea surface temperature,3 & Michael J. Benton1 During the Mesozoic and Cenozoic, four distinct crocodylomorph lineages colonized most probably ectothermic reptiles, these lineages colonized the marine realm and diversified during

  19. Received 2 Oct 2014 | Accepted 2 Feb 2015 | Published 12 Mar 2015 IL-23-mediated mononuclear phagocyte crosstalk

    E-Print Network [OSTI]

    ARTICLE Received 2 Oct 2014 | Accepted 2 Feb 2015 | Published 12 Mar 2015 IL-23-mediated mononuclear phagocyte crosstalk protects mice from Citrobacter rodentium-induced colon immunopathology Tegest that colonic CX3CR1þ mononuclear phagocytes are critical inducers of the innate response to Citrobacter

  20. Bull Mar Sci. 90(3):781794. 2014 http://dx.doi.org/10.5343/bms.2013.1056

    E-Print Network [OSTI]

    Durako, Michael J.

    Bull Mar Sci. 90(3):781­794. 2014 http://dx.doi.org/10.5343/bms.2013.1056 781Bulletin of Marine.e., it rapidly colonizes disturbance or gap areas, but does not hold its ground; Kenworthy 1997, Dean and Durako

  1. Stratigraphy and structure of interior layered deposits in west Candor Chasma, Mars, from High Resolution Stereo Camera (HRSC) stereo

    E-Print Network [OSTI]

    Utrecht, Universiteit

    Stratigraphy and structure of interior layered deposits in west Candor Chasma, Mars, from High the stratigraphy of two adjacent mounds. Layering tends to dip in the same direction as the local topographic slope rotations. The stratigraphy of two adjacent mounds correlates, but the thicknesses of the units differ. Most

  2. Pre-4.0 billion year weathering on Mars constrained by RbSr geochronology on meteorite ALH84001

    E-Print Network [OSTI]

    Johnson, Clark M.

    Pre-4.0 billion year weathering on Mars constrained by Rb­Sr geochronology on meteorite ALH84001 Accepted 24 October 2012 Editor: T. Elliott Available online 22 November 2012 Keywords: geochronology Sr crystallization age of this meteorite has been debated, where initial Sm­Nd geochronology by Nyquist et al. (1995

  3. arXiv:1003.1143v1[nucl-th]4Mar2010 Nuclear energy density functional from chiral

    E-Print Network [OSTI]

    Weise, Wolfram

    arXiv:1003.1143v1[nucl-th]4Mar2010 Nuclear energy density functional from chiral pion energy density functional approach is the many-body method of choice in order to calculate the properties nuclear energy density functional [10, 11, 12] focusses less on the fitting of experimental data

  4. Cloning, expression, crystallization and preliminary X-ray analysis of a putative multiple antibiotic resistance repressor protein (MarR) from Xanthomonas campestris

    SciTech Connect (OSTI)

    Tu, Zhi-Le; Li, Juo-Ning; Chin, Ko-Hsin; Chou, Chia-Cheng; Lee, Cheng-Chung; Shr, Hui-Lin; Lyu, Ping-Chiang; Gao, Fei Philip; Wang, Andrew H.-J.; Chou, Shan-Ho

    2005-07-01

    A putative repressor for the multiple antibiotic resistance operon from a plant pathogen X. campestris pv. campestris has been overexpressed in E. coli, purified and crystallized. The crystals diffracted to 2.3 Å with good quality. The multiple antibiotic resistance operon (marRAB) is a member of the multidrug-resistance system. When induced, this operon enhances resistance of bacteria to a variety of medically important antibiotics, causing a serious global health problem. MarR is a marR-encoded protein that represses the transcription of the marRAB operon. Through binding with salicylate and certain antibiotics, however, MarR can derepress and activate the marRAB operon. In this report, the cloning, expression, crystallization and preliminary X-ray analysis of XC1739, a putative MarR repressor protein present in the Xanthomonas campestris pv. campestris, a Gram-negative bacterium causing major worldwide disease of cruciferous crops, are described. The XC1739 crystals diffracted to a resolution of at least 1.8 Å. They are orthorhombic and belong to space group P2{sub 1}2{sub 1}2{sub 1}, with unit-cell parameters a = 39.5, b = 54.2 and c = 139.5 Å, respectively. They contain two molecules in the asymmetric unit from calculation of the self-rotation function.

  5. Variable-Rate State Gasoline Taxes

    E-Print Network [OSTI]

    Ang-Olson, Jeffrey; Wachs, Martin; Taylor, Brian D.

    2000-01-01

    J Bradshaw, "SLate ’F~es’ Gasoline Tax So ~t Wdl Rise," TheVarlable-Rate State Gasoline Taxers Jeffrey Ang-Olson MartinVariable-Rate State Gasoline Taxes Jeffrey Ang-Olson

  6. Rate Schedule CV-TPT7

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

    or receipt, adjusted for losses, and delivered to points as agreed to by the parties. Formula Rate: The formula rate for transmission of Western's power by others includes three...

  7. Fluorescence Assay for Polymerase Arrival Rates

    E-Print Network [OSTI]

    Che, Austin

    2003-08-31

    To engineer complex synthetic biological systems will require modular design, assembly, and characterization strategies. The RNA polymerase arrival rate (PAR) is defined to be the rate that RNA polymerases arrive at a ...

  8. Fluorescence assay for polymerase arrival rates

    E-Print Network [OSTI]

    Che, Austin, 1979-

    2004-01-01

    To engineer complex synthetic biological systems will require modular design, assembly, and characterization strategies. The RNA polymerase arrival rate (PAR) is defined to be the rate that RNA polymerases arrive at a ...

  9. Energy Efficiency Interest Rate Reduction Program

    Broader source: Energy.gov [DOE]

    For new and existing home purchases that are rated 6 Star or 5 Star Plus, applicants are eligible for an interest rate reduction for the first $200,000 of the loan amount, with a blended interest...

  10. Rate Setting for Small Water Systems 

    E-Print Network [OSTI]

    Dozier, Monty; Theodori, Gene L.; Jensen, Ricard

    2007-03-28

    Knowing how to set the proper rate for water service is a challenge for small water systems. They must generate enough revenue to remain solvent, but offer affordable service. This publication describes the various types of rates and explains...

  11. Home Energy Ratings and Building Performance 

    E-Print Network [OSTI]

    Gardner, J.C.

    2008-01-01

    climate as they affect the rating score of a proposed or completed structure. The rating is used to determine the most cost effective mechanical systems, building envelope design including window and door types, effect of various roofing materials...

  12. Difference in the wind speeds required for initiation versus continuation of sand transport on Mars: Implications for dunes and dust storms

    E-Print Network [OSTI]

    Kok, Jasper F

    2010-01-01

    Much of the surface of Mars is covered by dunes, ripples, and other features formed by the blowing of sand by wind, known as saltation. In addition, saltation loads the atmosphere with dust aerosols, which dominate the Martian climate. We show here that saltation can be maintained on Mars by wind speeds an order of magnitude less than required to initiate it. We further show that the resulting hysteresis effect causes saltation to occur for much lower wind speeds than previously thought. These findings have important implications for the formation of dust storms, sand dunes, and ripples on Mars.

  13. Spontaneous Emission Rate Enhancement Using Optical Antennas

    E-Print Network [OSTI]

    Kumar, Nikhil

    2013-01-01

    of  Spontaneous  Emission  in  a  Semiconductor  nanoLED,”  emission  rate  enhancement  using  the  Fluorescent  Emission  by  Lattice   Resonances  in  

  14. Simulation of the output power of copper bromide lasers by the MARS method

    SciTech Connect (OSTI)

    Iliev, I P; Voynikova, D S; Gocheva-Ilieva, S G

    2012-04-30

    The dependence of the output power of CuBr lasers (operating at wavelengths of 510.6 and 578.2 nm) on ten input physical parameters has been statistically analysed based on a large amount of experimental data accumulated for these lasers. Regression models have been built using the flexible nonparametric method of multivariate adaptive regression splines (MARS) to describe both linear and nonlinear local dependences. These models cover more than 97% initial data with an error comparable with the experimental error; they are applied to estimate and predict the output powers of both existing and future lasers. The advantage of the models constructed for estimating laser parameters over the standard parametric methods of multivariate factor and regression analysis is demonstrated.

  15. Improving the performance of MARS reservoir simulator on Cray-2 supercomputer

    SciTech Connect (OSTI)

    Li, K.G.; Dogru, A.H.; McDonald, A.E.; Merchant, A.R.; Al-Mulhem, A.A.; Al-Ruwaili, S.B.; Sobh, N.A.; Al-Sunaidi, H.A.

    1995-10-01

    The computational efficiency of a reservoir simulator-MARS-that is heavily used in Saudi Aramco, was significantly enhanced by improving the vectorization, parallelization and a key algorithm of the simulator. In particular, a state-of-the-art parallel linear equation solver was developed and implemented in the simulator. This new solver ran three to five times faster than the existing solvers. With the new solver and the other improvements in the simulator, the optimized code ran 1.3 to 1.8 times faster than the original code on a single processor and more than four times faster on four processors of Cray-2 supercomputer for typical Saudi Aramco reservoir models. This translates into great savings for the company since it, in effect, creates additional computational resources at no additional cost and improves the reservoir engineer`s productivity by shortening the job turnaround time.

  16. Construction and Testing of a Low-power Cryostat for MARS

    SciTech Connect (OSTI)

    Aalseth, Craig E.; Caggiano, Joseph A.; Day, Anthony R.; Fast, James E.; Fuller, Erin S.

    2007-10-01

    A low-power cryostat was designed and built for the Multi-sensor Airborne Radiation Survey (MARS) project for the purpose of housing a close-packed high-purity germanium (HPGe) detector array of 14 HPGe detectors. The power consumption of the cold mass in the cryostat was measured to be 4.07(11) watts, sufficient for 5.5 days of continuous operation using only 8 liters of liquid nitrogen. Temperatures throughout the cryostat were measured by platinum resistance temperature detectors. These measurements were used to determine the emissivity of the copper used in the floating radiation shield and outer cryostat wall, which was constructed using chemically cleaned and passivated copper metal. Using a PNNL-developed passivation process, an emissivity of 2.5(3)% was achieved for copper.

  17. Thermal creep assisted dust lifting on Mars: Wind tunnel experiments for the entrainment threshold velocity

    E-Print Network [OSTI]

    Küpper, Markus

    2015-01-01

    In this work we present laboratory measurements on the reduction of the threshold friction velocity necessary for lifting dust if the dust bed is illuminated. Insolation of a porous soil establishes a temperature gradient. At low ambient pressure this gradient leads to thermal creep gas flow within the soil. This flow leads to a sub-surface overpressure which supports lift imposed by wind. The wind tunnel was run with Mojave Mars Simulant and air at 3, 6 and 9 mbar, to cover most of the pressure range at martian surface levels. Our first measurements imply that the insolation of the martian surface can reduce the entrainment threshold velocity between 4 % and 19 % for the conditions sampled with our experiments. An insolation activated soil might therefore provide additional support for aeolian particle transport at low wind speeds.

  18. Downloaded 14 Mar 2006 to 171.64.124.26. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp Downloaded 14 Mar 2006 to 171.64.124.26. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/c

    E-Print Network [OSTI]

    Downloaded 14 Mar 2006 to 171.64.124.26. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 14 Mar 2006 to 171.64.124.26. Redistribution subject to AIP license or copyright, see http

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    E-Print Network [OSTI]

    Umstadter, Donald

    Downloaded 19 Mar 2003 to 141.213.19.32. Redistribution subject to AIP license or copyright, see.213.19.32. Redistribution subject to AIP license or copyright, see http://proceedings.aip.org/proceedings/cpcr.jsp #12;Downloaded 19 Mar 2003 to 141.213.19.32. Redistribution subject to AIP license or copyright, see http

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    E-Print Network [OSTI]

    Berry, R. Stephen

    Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp #12;Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http

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    E-Print Network [OSTI]

    Sprott, Julien Clinton

    Downloaded 29 Mar 2004 to 128.104.223.199. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://pof.aip.org/pof/copyright.jsp #12;Downloaded 29 Mar 2004 to 128.104.223.199. Redistribution subject to AIP license or copyright, see http

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    E-Print Network [OSTI]

    Berthier, Ludovic

    Downloaded 06 Mar 2009 to 128.135.186.78. Redistribution subject to AIP license or copyright; see.135.186.78. Redistribution subject to AIP license or copyright; see http://proceedings.aip.org/proceedings/cpcr.jsp #12;Downloaded 06 Mar 2009 to 128.135.186.78. Redistribution subject to AIP license or copyright; see http

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    E-Print Network [OSTI]

    Berry, R. Stephen

    Downloaded 15 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 15 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http

  4. Downloaded 22 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp Downloaded 22 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http://jap.aip.org/j

    E-Print Network [OSTI]

    Berry, R. Stephen

    Downloaded 22 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp #12;Downloaded 22 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http

  5. Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/j

    E-Print Network [OSTI]

    Berry, R. Stephen

    Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp #12;Downloaded 20 Mar 2004 to 128.135.233.250. Redistribution subject to AIP license or copyright, see http

  6. Kiwifruitsize influences softening rate during storage

    E-Print Network [OSTI]

    Crisosto, Carlos H.

    Kiwifruitsize influences softening rate during storage Carlos H. Crisosto o David Garner D Katia)at 32*F for 16 weeks. Un- der both storage conditions,large fruit had a slower rate of softening than fruit size and the rate of softening under air and CA conditions will help cold storage managerssafely

  7. An analysis of international grain freight rates 

    E-Print Network [OSTI]

    Jonnala, Sneha Latha

    1999-01-01

    decreasing rate as shipment quantity increases. Highest rates were associated with the berth term followed by the free discharge and free-in-and-out terms. The ships with U.S. flags were found to charge higher rates when compared to ships with foreign flags...

  8. The evolution of the cosmic SN rate

    E-Print Network [OSTI]

    Enrico Cappellaro; Maria Teresa Botticella; Laura Greggio

    2007-06-09

    We briefly review the contribution of SN rate measurements to the debate on SN progenitor scenarios. We find that core collapse rates confirms the rapid evolution of the star formation rate with redshift. After accounting for the dispersion of SN Ia measurements and uncertainty of the star formation history, the standard scenarios for SN Ia progenitors appear consistent with all observational constraints.

  9. The Mars Hopper: Development, Simulation and Experimental Validation of a Radioisotope Exploration Probe for the Martian Surface

    SciTech Connect (OSTI)

    Nathan D. Jerred; Spencer Cooley; Robert C. O'Brien; Steven D. Howe; James E. O'Brien

    2012-09-01

    An advanced exploration probe has been proposed by the Center for Space Nuclear Research (CSNR) to acquire detailed data from the Martian surface and subsurface, ‘hop’ large distances to multiple sites in short periods of time and perform this task repeatedly. Although several similar flying vehicles have been proposed utilizing various power sources and complex designs, e.g. solar-electric and chemical-based, the CSNR’s Mars Hopper is based on a radioisotope thermal rocket (RTR) concept. The Mars Hopper’s design relies on the high specific energies [J/kg] of radioisotopes and enhances their low specific power [W/kg] through the use of a thermal capacitance material to store thermal energy over time. During operation, the RTR transfers the stored thermal energy to a flowing gas, which is then expanded through a converging-diverging nozzle, producing thrust. Between flights, the platform will have ample time to perform in-depth science at each location while the propellant tanks and thermal capacitor recharge. Recharging the propellant tanks is accomplished by sublimation freezing of the ambient CO2 atmosphere with a cryocooler, followed by heating and pressurization to yield a liquid storage state. The proposed Mars Hopper will undergo a ballistic flight, consuming the propellant in both ascent and descent, and by using multiple hopper platforms, information can be gathered on a global scale, enabling better resource resolution and providing valuable information for a possible Mars sample-return mission. The CSNR, collaborating with the Idaho National Laboratory (INL) and three universities (University of Idaho, Utah State University and Oregon State University), has identified key components and sub-systems necessary for the proposed hopper. Current project activities include the development of a lab-scale prototypic Mars Hopper and test facility, along with computational fluid dynamics (CFD)/thermal-hydraulic models to yield a better understanding of the heat transfer process and complex nature of turbulent CO2 flow. Laboratory experimentation will aid design iterations and the development of both tethered and free-flying terrestrial hoppers that utilize an electrically heated core. The knowledge base acquired from these activities will refine the Mars Hopper’s future performance and optimize the RTR core components prior to constructing the final design.

  10. Managing by passion, professionalism and performance : the MBP³ model : an alternative management framework developed for the Instituto de Ciencias Terra-Mar (ICTM)

    E-Print Network [OSTI]

    Coelho, Alexandre C. (Alexandre Costa)

    2007-01-01

    The objective of this thesis is to develop a new, tailor-made and innovative managerial framework for the Instituto de Ciencias Terra-Mar (ICTM). The ICTM is a multi-functional science and technology institute dedicated ...

  11. APPLIED AND ENVIRONMENTAL MICROBIOLOGY, Mar. 2011, p. 16911697 Vol. 77, No. 5 0099-2240/11/$12.00 doi:10.1128/AEM.02240-10

    E-Print Network [OSTI]

    Cotty, Peter J.

    APPLIED AND ENVIRONMENTAL MICROBIOLOGY, Mar. 2011, p. 1691­1697 Vol. 77, No. 5 0099 contact and prior to either germ tube emergence or host colonization. This suggests the timing of host

  12. ANTIMICROBIAL AGENTS AND CHEMOTHERAPY, Mar. 2011, p. 10361044 Vol. 55, No. 3 0066-4804/11/$12.00 doi:10.1128/AAC.01319-10

    E-Print Network [OSTI]

    ANTIMICROBIAL AGENTS AND CHEMOTHERAPY, Mar. 2011, p. 1036­1044 Vol. 55, No. 3 0066 antiviral response to colonize its host cells (23). Therefore, an alternative approach to inhibiting HCV

  13. JOURNAL OF BACTERIOLOGY, Mar. 2009, p. 19411950 Vol. 191, No. 6 0021-9193/09/$08.00 0 doi:10.1128/JB.00601-08

    E-Print Network [OSTI]

    Chattopadhyay, Sujay

    JOURNAL OF BACTERIOLOGY, Mar. 2009, p. 1941­1950 Vol. 191, No. 6 0021-9193/09/$08.00 0 doi:10 commensal colonization of mucosal surfaces in humans and other animals (1). Several studies have reported K

  14. doi:10.1152/ajpregu.00824.2005 291:307-314, 2006. First published Mar 23, 2006;Am J Physiol Regulatory Integrative Comp Physiol

    E-Print Network [OSTI]

    Murphy, Anne Z.

    doi:10.1152/ajpregu.00824.2005 291:307-314, 2006. First published Mar 23, 2006;Am J Physiol the vmr in both groups without affecting colonic compliance. However, morphine was sig- nificantly more

  15. Crazy Engineering Mars Helicopter Transcript Hey guys! We've all seen these RC helicopters before. They're everywhere. They're

    E-Print Network [OSTI]

    Crazy Engineering Mars Helicopter Transcript Hey guys! We've all seen these RC helicopters before to put a helicopter on Mars? If I'm the rover right now, I can't really see the terrain behind me. But if I had a helicopter with a camera on it, all of a sudden, I can see a whole lot more. If our rover

  16. United States Patent [19] [11] Patent Number: 4,817,182 Adelson et al. [45] Date of Patent: Mar. 28, 1989

    E-Print Network [OSTI]

    Adelson, Edward

    United States Patent [19] [11] Patent Number: 4,817,182 Adelson et al. [45] Date of Patent: Mar. 28; 364/723-725, 728 [56] References Cited U.S. PATENT DOCUMENTS 4,455,649 6/1984 Esteban et al for the secceeding analysis procedure. 9 Claims, 4 Drawing Sheets #12;U.S. Patent Mar. 28, 1989 Sheet 1 of 4 4

  17. Wind measurements in Mars' middle atmosphere at equinox and solstice: IRAM Plateau de Bure interferometric CO observations

    E-Print Network [OSTI]

    Moreno, R; Encrenaz, T; Forget, F; Chassefière, E; Hourdin, F; Guilloteau, S; Guilloteau, St\\'{e}phane

    2007-01-01

    Characterizing the Martian atmosphere is an essential objective to understand its meteorology and its climate. The lower atmosphere (< 40 km) and middle atmosphere (40-80 km) of Mars appear dynamically coupled at much higher levels than in the case of the Earth. The vertical extension of the weather phenomena is considerable with for example Hadley's cells reaching the top of the neutral atmosphere (120 km). The circulation in the middle atmosphere modifies the meteorology of the lower atmosphere, affecting the transport and climatic processes Observations of the CO rotational lines at millimeter (mm) wavelengths (Clancy et al 1990) have strongly contributed in the study of the vertical distribution of this compound and the thermal profile in the atmosphere of Mars over 0-70 km. Singledish observations of the CO Doppler lineshift have allowed direct wind measurements in the martian middle atmosphere near 50 km altitude (Lellouch et al 1991), but at a low spatial resolution (12'') enabling only an essential...

  18. CM-1-H Wholesale Power Rate Schedule

    Broader source: Energy.gov [DOE]

    Availability:This rate schedule shall be available to the South Mississippi Electric Power Association, Municipal Energy Agency of Mississippi, and Mississippi Delta Energy Agency (hereinafter...

  19. Rating the energy performance of buildings

    E-Print Network [OSTI]

    Olofsson, Thomas; Meier, Alan; Lamberts, Roberto

    2004-01-01

    T. , (1998), Building Energy Measurement and PerformanceRating a building’s energy performance is becoming anrating of energy performance of buildings. Modern existing

  20. BPA proposes rate increase to bolster

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

    the proposed wholesale power rate increase is reduced revenue expectations from surplus power sales. Market prices have been, and are forecast to continue to be, suppressed...

  1. Confronting the Graduation Rate Crisis in Texas

    E-Print Network [OSTI]

    Losen, Daniel; Orfield, Gary; Balfanz, Robert

    2006-01-01

    of minority students in Texas attend these schools, comparedfourths of the high schools in Texas where graduation is notthe Graduation Rate Crisis in Texas By Daniel Losen, Gary

  2. Photovoltaic Degradation Rates -- An Analytical Review

    SciTech Connect (OSTI)

    Jordan, D. C.; Kurtz, S. R.

    2012-06-01

    As photovoltaic penetration of the power grid increases, accurate predictions of return on investment require accurate prediction of decreased power output over time. Degradation rates must be known in order to predict power delivery. This article reviews degradation rates of flat-plate terrestrial modules and systems reported in published literature from field testing throughout the last 40 years. Nearly 2000 degradation rates, measured on individual modules or entire systems, have been assembled from the literature, showing a median value of 0.5%/year. The review consists of three parts: a brief historical outline, an analytical summary of degradation rates, and a detailed bibliography partitioned by technology.

  3. Method of controlling fusion reaction rates

    DOE Patents [OSTI]

    Kulsrud, R.M.; Furth, H.P.; Valeo, E.J.; Goldhaber, M.

    1983-05-09

    This invention relates to a method of controlling the reaction rates in a nuclear fusion reactor; and more particularly, to the use of polarized nuclear fuel.

  4. Use of High-Power Brayton Nuclear Electric Propulsion (NEP) for a 2033 Mars Round-Trip Mission

    SciTech Connect (OSTI)

    McGuire, Melissa L. [Space Propulsion and Mission Analysis Office (Code: PBM), NASA Glenn Research Center, MS 500-103, 21000 Brookpark Rd., Cleveland, Ohio 44135 (United States); Martini, Michael C.; Packard, Thomas W. [Space Propulsion and Mission Analysis Office (Code: PBM), NASA Glenn Research Center, MS 500-103, 21000 Brookpark Rd., Cleveland, Ohio 44135 (United States); Analex Corporation, 1100 Apollo Drive, Brook Park, OH 44142 (United States); Weglian, John E. [Space Propulsion and Mission Analysis Office (Code: PBM), NASA Glenn Research Center, MS 500-103, 21000 Brookpark Rd., Cleveland, Ohio 44135 (United States); Ohio Aerospace Institute, 22800 Cedar Point Rd., Brook Park, OH 44142 (United States); Gilland, James H. [Ohio Aerospace Institute, 22800 Cedar Point Rd., Brook Park, OH 44142 (United States)

    2006-01-20

    The Revolutionary Aerospace Systems Concepts (RASC) team, led by the NASA Langley Research Center, is tasked with exploring revolutionary new approaches to enabling NASA to achieve its strategic goals and objectives in future missions. This paper provides the details from the 2004-2005 RASC study of a point-design that uses a high-power nuclear electric propulsion (NEP) based space transportation architecture to support a manned mission to Mars. The study assumes a high-temperature liquid-metal cooled fission reactor with a Brayton power conversion system to generate the electrical power required by magnetoplasmadynamic (MPD) thrusters. The architecture includes a cargo vehicle with an NEP system providing 5 MW of electrical power and a crewed vehicle with an NEP system with two reactors providing a combined total of 10 MW of electrical power. Both vehicles use a low-thrust, high-efficiency (5000 sec specific impulse) MPD system to conduct a spiral-out of the Earth gravity well, a low-thrust heliocentric trajectory, and a spiral-in at Mars with arrival late in 2033. The cargo vehicle carries two moon landers to Mars and arrives shortly before the crewed vehicle. The crewed vehicle and cargo vehicle rendezvous in Mars orbit and, over the course of the 60-day stay, the crew conducts nine-day excursions to Phobos and Deimos with the landers. The crewed vehicle then spirals out of Martian orbit and returns via a low-thrust trajectory to conduct an Earth flyby. The crew separates from the vehicle prior to Earth flyby and aerobrakes for a direct-entry landing.

  5. Origin of upper Bell Canyon Reservoir Sandstones (Guadalupian), El Mar and Paduca Fields, Southeast New Mexico and West Texas 

    E-Print Network [OSTI]

    Weinmeister, Marcus Paul

    1978-01-01

    and into the Delaware Basin. A turbidite origin is supported by the ordered sequence of sedimentary structures of the sandstones and stratigraphic evidence which shows that Upper Bell Canyon sedimentation occurred in a water depth of at least 1500 ft. Texture... units, Paduca field. 32 Frequency of bed divisions in Ramsey Sandstone cores. 43 ix LIST OF FIGURES Figure Page Regional map of Delaware Basin showing structure on top of Bell Canyon Formation and locations of Paduca and El Mar fields. North...

  6. Microsoft PowerPoint - 15.1025_Bosco_PM Workshop Mar15_2010 | Department of

    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 DeliciousMathematicsEnergyInterested Parties - WAPAEnergy May 28Mar [Compatibility Mode] |HUMAN

  7. Optimal Rate Allocation in Overlay Content Distribution

    E-Print Network [OSTI]

    Li, Baochun

    Optimal Rate Allocation in Overlay Content Distribution Chuan Wu and Baochun Li Department. This paper addresses the optimal rate allocation problem in overlay content distribution for efficient, these scenarios reflect the contrast between elastic and streaming content distribution, with either per

  8. China's High Savings Rates Rick Harbaugh

    E-Print Network [OSTI]

    Martins, Emília

    the highest in the world. That savings would grow in a country emerging from poverty is not necessarilyChina's High Savings Rates Rick Harbaugh Prepared for conference on "The Rise of China Revisited Abstract Since the early 1980s China has witnessed a rapid increase in its national savings rate to one

  9. Heat release rate markers for premixed combustion

    E-Print Network [OSTI]

    Nikolaou, Zacharias M.; Swaminathan, Nedunchezhian

    2014-06-16

    The validity of the commonly used flame marker for heat release rate (HRR) visualization, namely the rate of the reaction OH + CH2O ? HCO + H2O is re-examined. This is done both for methane–air and multi-component fuel–air mixtures for lean...

  10. Variable word rate N-grams 

    E-Print Network [OSTI]

    Gotoh, Yoshihiko; Renals, Steve

    The rate of occurrence of words is not uniform but varies from document to document. Despite this observation, parameters for conventional N-gram language models are usually derived using the assumption of a constant word rate. In this paper we...

  11. Method of controlling fusion reaction rates

    DOE Patents [OSTI]

    Kulsrud, Russell M. (Princeton, NJ); Furth, Harold P. (Princeton, NJ); Valeo, Ernest J. (Princeton Junction, NJ); Goldhaber, Maurice (Bayport, NY)

    1988-01-01

    A method of controlling the reaction rates of the fuel atoms in a fusion reactor comprises the step of polarizing the nuclei of the fuel atoms in a particular direction relative to the plasma confining magnetic field. Fusion reaction rates can be increased or decreased, and the direction of emission of the reaction products can be controlled, depending on the choice of polarization direction.

  12. Resonances and the thermonuclear reaction rate

    E-Print Network [OSTI]

    M. S. Hussein; M. Ueda; A. J. Sargeant; M. P. Pato

    2003-07-21

    We present an approximate analytic expression for thermonuclear reaction rate of charged particles when the cross section contains a single narrow or wide resonance described by a Breit-Wigner shape. The resulting expression is uniformly valid as the effective energy and resonance energy coalesce. We use our expressions to calculate the reaction rate for $^{12}$C(p,$\\gamma$)$^{13}$N.

  13. Polycyclic Aromatic Hydrocarbon Biodegradation Rates: A

    E-Print Network [OSTI]

    Peters, Catherine A.

    Polycyclic Aromatic Hydrocarbon Biodegradation Rates: A Structure-Based Study K R I S T I N E H . W structure in determining the biodegradation rates of polycyclic aromatic hydrocarbons (PAHs). Laboratory. Introduction Polycyclic aromatic hydrocarbons (PAHs) are a class of organic pollutants that are commonly found

  14. Cadmium Biosorption Rate in Protonated Sargassum Biomass

    E-Print Network [OSTI]

    Volesky, Bohumil

    Cadmium Biosorption Rate in Protonated Sargassum Biomass J I N B A I Y A N G A N D B O H U M I L V Sargassum fluitans biomass was accompanied by the release of hydrogen protons from the biomass. The uptake the overall biosorption rate of cadmium ions in flat seaweed biomass particles. The overall biosorption

  15. N-body simulations of oligarchic growth of Mars: Implications for Hf-W chronology

    E-Print Network [OSTI]

    Morishima, Ryuji; Samuel, Henri

    2013-01-01

    Dauphas and Pourmand (2011) [Nature 473, 489--492] estimated the accretion timescale of Mars to be 1.8 $^{+0.9}_{-1.0}$ Myr from the W isotopes of martian meteorites. This timescale was derived assuming perfect metal-silicate equilibration between the impactor and the target's mantle. However, in the case of a small impactor most likely only a fraction of the target's mantle is involved in the equilibration, while only a small part of the impactor's core equilibrates in the case of a giant impact. We examined the effects of imperfect equilibration using results of high-resolution $N$-body simulations for the oligarchic growth stage. These effects were found to be small as long as a planetary embryo has a deep liquid magma ocean during its accretion. The effect due to partial involvement of the target's mantle in equilibration is small due to the low metal-silicate partition coefficient for W suggested from the low Hf/W ratio of the martian mantle. The effect due to partial involvement of the impactor's core i...

  16. 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...

  17. Benchmarking Heavy Ion Transport Codes FLUKA, HETC-HEDS MARS15, MCNPX, and PHITS

    SciTech Connect (OSTI)

    Ronningen, Reginald Martin [Michigan State University; Remec, Igor [Oak Ridge National Laboratory; Heilbronn, Lawrence H. [University of Tennessee-Knoxville

    2013-06-07

    Powerful accelerators such as spallation neutron sources, muon-collider/neutrino facilities, and rare isotope beam facilities must be designed with the consideration that they handle the beam power reliably and safely, and they must be optimized to yield maximum performance relative to their design requirements. The simulation codes used for design purposes must produce reliable results. If not, component and facility designs can become costly, have limited lifetime and usefulness, and could even be unsafe. The objective of this proposal is to assess the performance of the currently available codes � PHITS, FLUKA, MARS15, MCNPX, and HETC-HEDS � that could be used for design simulations involving heavy ion transport. We plan to access their performance by performing simulations and comparing results against experimental data of benchmark quality. Quantitative knowledge of the biases and the uncertainties of the simulations is essential as this potentially impacts the safe, reliable and cost effective design of any future radioactive ion beam facility. Further benchmarking of heavy-ion transport codes was one of the actions recommended in the �Report of the 2003 RIA R&D Workshop".

  18. Design, qualification and operation of nuclear rockets for safe Mars missions

    SciTech Connect (OSTI)

    Buden, D.; Madsen, W.W.; Olson, T.S. (EG and G Idaho, Inc., Idaho Falls, ID (United States)); Redd, L.R. (USDOE Idaho Field Office, Idaho Falls, ID (United States))

    1993-01-01

    Nuclear thermal propulsion modules planned for use on crew missions to Mars improve mission reliability and overall safety of the mission. This, as well as all other systems, are greatly enhanced if the system specifications take into account safety from design initiation, and operational considerations are well thought through and applied. For instance, the use of multiple engines in the propulsion module can lead to very high system safety and reliability. Operational safety enhancements may include: the use of multiple perigee burns, thus allowing time to ensure that all systems are functioning properly prior to departure from Earth orbit; the ability to perform all other parts of the mission in a degraded mode with little or no degradation of the mission; and the safe disposal of the nuclear propulsion module in a heliocentric orbit out of the ecliptic plane. The standards used to qualify nuclear rockets are one of the main cost drivers of the program. Concepts and systems that minimize cost and risk will rely on use of the element and component levels to demonstrate technology readiness and validation. Subsystem or systems testing then is only needed for verification of performance. Also, these will be the safest concepts because they will be more thoroughly understood and the safety margins will be well established and confirmed by tests.

  19. Design, qualification and operation of nuclear rockets for safe Mars missions

    SciTech Connect (OSTI)

    Buden, D.; Madsen, W.W.; Olson, T.S. [EG and G Idaho, Inc., Idaho Falls, ID (United States); Redd, L.R. [USDOE Idaho Field Office, Idaho Falls, ID (United States)

    1993-04-01

    Nuclear thermal propulsion modules planned for use on crew missions to Mars improve mission reliability and overall safety of the mission. This, as well as all other systems, are greatly enhanced if the system specifications take into account safety from design initiation, and operational considerations are well thought through and applied. For instance, the use of multiple engines in the propulsion module can lead to very high system safety and reliability. Operational safety enhancements may include: the use of multiple perigee burns, thus allowing time to ensure that all systems are functioning properly prior to departure from Earth orbit; the ability to perform all other parts of the mission in a degraded mode with little or no degradation of the mission; and the safe disposal of the nuclear propulsion module in a heliocentric orbit out of the ecliptic plane. The standards used to qualify nuclear rockets are one of the main cost drivers of the program. Concepts and systems that minimize cost and risk will rely on use of the element and component levels to demonstrate technology readiness and validation. Subsystem or systems testing then is only needed for verification of performance. Also, these will be the safest concepts because they will be more thoroughly understood and the safety margins will be well established and confirmed by tests.

  20. Measuring Degradation Rates Without Irradiance Data

    SciTech Connect (OSTI)

    Pulver, S.; Cormode, D.; Cronin, A.; Jordan, D.; Kurtz, S.; Smith, R.

    2011-02-01

    A method to report PV system degradation rates without using irradiance data is demonstrated. First, a set of relative degradation rates are determined by comparing daily AC final yields from a group of PV systems relative to the average final yield of all the PV systems. Then, the difference between relative and absolute degradation rates is found from a statistical analysis. This approach is verified by comparing to methods that utilize irradiance data. This approach is significant because PV systems are often deployed without irradiance sensors, so the analysis method described here may enable measurements of degradation using data that were previously thought to be unsuitable for degradation studies.

  1. Considerations for How to Rate CPV

    SciTech Connect (OSTI)

    Kurtz, S.; Miller, M.; Marion, B.; Emery, K.; McConnell, R.; Surendran, S.; Kimber, A.

    2011-02-01

    The concentrator photovoltaic (CPV) industry is introducing multiple products into the marketplace, but, as yet, the; community has not embraced a unified method for assessing a nameplate rating. The choices of whether to use 850,; 900, or 1000 W/m2 for the direct-normal irradiance and whether to link the rating to ambient or cell temperature will; affect how CPV modules are rated and compared with other technologies. This paper explores the qualitative and; quantitative ramifications of these choices using data from two multi-junction CPV modules and two flat-plate; modules.

  2. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility RateUtility Rate

  3. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtilityRateUtility Rate

  4. Cooling rate, heating rate, and aging effects in glassy water Nicolas Giovambattista,1

    E-Print Network [OSTI]

    Sciortino, Francesco

    Cooling rate, heating rate, and aging effects in glassy water Nicolas Giovambattista,1 H. Eugene of water molecules during the process of generating a glass by cooling, and during the process on the cooling/heating rates as well as on the role of aging (the time elapsed in the glass state). We compare

  5. Does Growth Rate Determine the Rate of Metabolism in Shorebird Chicks Living in the Arctic?

    E-Print Network [OSTI]

    Williams, Jos. B.

    primarily of greater metabolic inten- sities of heat-generating tissues. The maximum temperature gradient500 Does Growth Rate Determine the Rate of Metabolism in Shorebird Chicks Living in the Arctic/22/2007; Electronically Published 7/13/2007 ABSTRACT We measured resting and peak metabolic rates (RMR and PMR

  6. Dependence of Up-scaled Reaction Rate on Flow Rate in Porous Media

    E-Print Network [OSTI]

    New York at Stoney Brook, State University of

    to inherent heterogeneities in structure, mineral placement and fluid velocity in rock, bulk reaction rates1 Dependence of Up-scaled Reaction Rate on Flow Rate in Porous Media D. Kim · W. B. Lindquist model simulations of anorthite and kaolinite reactions in two sandstone pore networks under acidic

  7. Contractor Rating and Feedback Systems | Department of Energy

    Energy Savers [EERE]

    Rating and Feedback Systems Contractor Rating and Feedback Systems Better Buildings Residential Workforce Business Partners Peer Exchange Call Series: Contractor Rating and...

  8. Tier 2 Vintage Rate Workshop II

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

    Rates. These are intended to be based on specific resource costs for customers that need power to be based on specific resource types (e.g., renewable) or that want to know more...

  9. Rate Schedule CV-F13

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

    for the entire FY. The PRR is allocated to FP Customers and BR Customers based on formula rates, as adjusted for Hourly Exchange (HE), FP true-up calculation, and midyear...

  10. Regularization of Tunneling Rates with Quantum Chaos

    E-Print Network [OSTI]

    Pecora, Louis M; Wu, Dong-Ho

    2012-01-01

    We study tunneling in various shaped, closed, two-dimensional, flat potential, double wells by calculating the energy splitting between symmetric and anti-symmetric state pairs. For shapes that have regular or nearly regular classical behavior (e.g. rectangular or circular) the tunneling rates vary greatly over wide ranges often by several orders of magnitude. However, for well shapes that admit more classically chaotic behavior (e.g. the stadium, the Sinai billiard) the range of tunneling rates narrows, often by orders of magnitude. This dramatic narrowing appears to come from destabilization of periodic orbits in the regular wells that produce the largest and smallest tunneling rates and causes the splitting vs. energy relation to take on a possibly universal shape. It is in this sense that we say the quantum chaos regularizes the tunneling rates.

  11. Essays on exchange rates and electricity demand

    E-Print Network [OSTI]

    Li, Xiangming, 1966-

    1999-01-01

    This thesis examines two important issues in economic development: exchange rates and electricity demand and addresses methodological issues of using time series and panel data analysis to investigate important policy ...

  12. Uncertainty Analysis for Photovoltaic Degradation Rates (Poster)

    SciTech Connect (OSTI)

    Jordan, D.; Kurtz, S.; Hansen, C.

    2014-04-01

    Dependable and predictable energy production is the key to the long-term success of the PV industry. PV systems show over the lifetime of their exposure a gradual decline that depends on many different factors such as module technology, module type, mounting configuration, climate etc. When degradation rates are determined from continuous data the statistical uncertainty is easily calculated from the regression coefficients. However, total uncertainty that includes measurement uncertainty and instrumentation drift is far more difficult to determine. A Monte Carlo simulation approach was chosen to investigate a comprehensive uncertainty analysis. The most important effect for degradation rates is to avoid instrumentation that changes over time in the field. For instance, a drifting irradiance sensor, which can be achieved through regular calibration, can lead to a substantially erroneous degradation rates. However, the accuracy of the irradiance sensor has negligible impact on degradation rate uncertainty emphasizing that precision (relative accuracy) is more important than absolute accuracy.

  13. Dynamic Line Rating: Research and Policy Evaluation

    SciTech Connect (OSTI)

    Jake P. Gentle; Kurt S. Myers; Michael R. West

    2014-07-01

    Dynamic Line Rating (DLR) is a smart grid technology that allows the rating of electrical conductors to be increased based on local weather conditions. Overhead lines are conventionally given a conservative rating based on worst case scenarios. We demonstrate that observing the conditions in real time leads to additional capacity and safer operation. This paper provides a report of a pioneering scheme in the United States of America in which DLR has been applied. Thereby, we demonstrate that observing the local weather conditions in real time leads to additional capacity and safer operation. Secondly, we discuss limitations involved. In doing so, we arrive at novel insights which will inform and improve future DLR projects. Third, we provide a policy background and discussion to clarify the technology’s potential and identifies barriers to the imminent adoption of dynamic line rating systems. We provide suggestions for regulatory bodies about possible improvements in policy to encourage adoption of this beneficial technology.

  14. Extratropical Lapse Rates in Very Hot Climates 

    E-Print Network [OSTI]

    Zamora, Ryan Alexander

    2013-07-02

    circulation in progressively warmer climate states. As a tool to assess the stability of the atmosphere, we calculate a thermodynamic variable called saturation potential vorticity (P*), which has the property of being identically zero wherever lapse rates...

  15. Negotiating Rates and Contracts for Qualifying Facilities 

    E-Print Network [OSTI]

    Collier, S. E.

    1986-01-01

    . This paper describes the key issues involved in the development of purchase rates, as well as supplemental power services, and contract terms and conditions. Attention is given to special issues such as wheeling, losses, and regulatory proceedings. A general...

  16. PSNC Energy (Gas)- Green Building Rate Discount

    Office of Energy Efficiency and Renewable Energy (EERE)

    This discounted rate is available to commercial customers whose building meets the U.S. Green Building Council’s Leadership in Energy and Environmental Design (LEED) certification or equivalent. To...

  17. Extended range radiation dose-rate monitor

    DOE Patents [OSTI]

    Valentine, Kenneth H. (Knoxville, TN)

    1988-01-01

    An extended range dose-rate monitor is provided which utilizes the pulse pileup phenomenon that occurs in conventional counting systems to alter the dynamic response of the system to extend the dose-rate counting range. The current pulses from a solid-state detector generated by radiation events are amplified and shaped prior to applying the pulses to the input of a comparator. The comparator generates one logic pulse for each input pulse which exceeds the comparator reference threshold. These pulses are integrated and applied to a meter calibrated to indicate the measured dose-rate in response to the integrator output. A portion of the output signal from the integrator is fed back to vary the comparator reference threshold in proportion to the output count rate to extend the sensitive dynamic detection range by delaying the asymptotic approach of the integrator output toward full scale as measured by the meter.

  18. Calibration and Rating of Photovoltaics: Preprint

    SciTech Connect (OSTI)

    Emery, K.

    2012-06-01

    Rating the performance of photovoltaic (PV) modules is critical to determining the cost per watt, and efficiency is useful to assess the relative progress among PV concepts. Procedures for determining the efficiency for PV technologies from 1-sun to low concentration to high concentration are discussed. We also discuss the state of the art in primary and secondary calibration of PV reference cells used by calibration laboratories around the world. Finally, we consider challenges to rating PV technologies and areas for improvement.

  19. Intraclass Price Elasticity & Electric Rate Design 

    E-Print Network [OSTI]

    Gresham, K. E.

    1987-01-01

    beyond this becomes more elastic as usage increases. In the book "Innovative Electric, Rates," John Chamberlin and Charles Dickson utilize an economic model to test conservation programs. This model utilizes intrac1ass price elasticities and has a.... Utilities must rely on customer data and intuition to estimate customer response to rate changes. These methods have several downfalls. First, the customer data may not reflect customer behavior in an economic downturn. Second, the data may not exactly...

  20. Solar Models and NACRE thermonuclear reaction rates

    E-Print Network [OSTI]

    P. Morel; B. Pichon; J. Provost; G. Berthomieu

    1999-07-27

    Using the most recent updated physics, calibrated solar models have been computed with the new thermonuclear reaction rates of NACRE, the recently available European compilation. Comparisons with models computed with the reaction rates of Caughlan & Fowler (\\cite{cf88}) and of Adelberger et al. (\\cite{a98}) are made for global structure, expected neutrinos fluxes, chemical composition and sound speed profiles, helioseismological properties of p-modes and g-modes.

  1. Rating of Mixed Split Residential Air Conditioners 

    E-Print Network [OSTI]

    Domanski, P. A.

    1988-01-01

    require that manufac- turers derive cooling ratings for unitary systems by testing a sample of sufficient size to meet certain specified statistical confidence levels. For split unitary systems comprising an outdoor unit and an indoor coil assembly...(95), SEER, and recommended indoor volumetric flow rate of air, are publicly available. The procedure also assumee that the matched indoor section is available for inspection and evaluation of the indoor coil capacity and the indoor fan power...

  2. Radiation Leukemogenesis at Low Dose Rates

    SciTech Connect (OSTI)

    Weil, Michael; Ullrich, Robert

    2013-09-25

    The major goals of this program were to study the efficacy of low dose rate radiation exposures for the induction of acute myeloid leukemia (AML) and to characterize the leukemias that are caused by radiation exposures at low dose rate. An irradiator facility was designed and constructed that allows large numbers of mice to be irradiated at low dose rates for protracted periods (up to their life span). To the best of our knowledge this facility is unique in the US and it was subsequently used to study radioprotectors being developed for radiological defense (PLoS One. 7(3), e33044, 2012) and is currently being used to study the role of genetic background in susceptibility to radiation-induced lung cancer. One result of the irradiation was expected; low dose rate exposures are ineffective in inducing AML. However, another result was completely unexpected; the irradiated mice had a very high incidence of hepatocellular carcinoma (HCC), approximately 50%. It was unexpected because acute exposures are ineffective in increasing HCC incidence above background. This is a potential important finding for setting exposure limits because it supports the concept of an 'inverse dose rate effect' for some tumor types. That is, for the development of some tumor types low dose rate exposures carry greater risks than acute exposures.

  3. Feasibility of Ground Testing a Moon and Mars Surface Power Reactor in EBR-II

    SciTech Connect (OSTI)

    Sheryl Morton; Carl Baily; Tom Hill; Jim Werner

    2006-02-01

    Ground testing of a surface fission power system would be necessary to verify the design and validate reactor performance to support safe and sustained human exploration of the Moon and Mars. The Idaho National Laboratory (INL) has several facilities that could be adapted to support a ground test. This paper focuses on the feasibility of ground testing at the Experimental Breeder Reactor II (EBR-II) facility and using other INL existing infrastructure to support such a test. This brief study concludes that the INL EBR-II facility and supporting infrastructure are a viable option for ground testing the surface power system. It provides features and attributes that offer advantages to locating and performing ground testing at this site, and it could support the National Aeronautics and Space Administration schedules for human exploration of the Moon. This study used the initial concept examined by the U.S. Department of Energy Inter-laboratory Design and Analysis Support Team for surface power, a lowtemperature, liquid-metal, three-loop Brayton power system. With some facility modification, the EBR-II can safely house a test chamber and perform long-term testing of the space reactor power system. The INL infrastructure is available to receive and provide bonded storage for special nuclear materials. Facilities adjacent to EBR-II can provide the clean room environment needed to assemble and store the test article assembly, disassemble the power system at the conclusion of testing, and perform posttest examination. Capability for waste disposal is also available at the INL.

  4. Mars Mission Analysis Trades Based on Legacy and Future Nuclear Propulsion Options

    SciTech Connect (OSTI)

    Joyner, Russell [Pratt and Whitney Rocketdyne, West Palm Beach, Florida (United States); Lentati, Andrea [Georgia Institute of Technology, Atlanta, Georgia (United States); Cichon, Jaclyn [University of Florida, Gainesville, Florida (United States)

    2007-01-30

    The purpose of this paper is to discuss the results of mission-based system trades when using a nuclear thermal propulsion (NTP) system for Solar System exploration. The results are based on comparing reactor designs that use a ceramic-metallic (CERMET), graphite matrix, graphite composite matrix, or carbide matrix fuel element designs. The composite graphite matrix and CERMET designs have been examined for providing power as well as propulsion. Approaches to the design of the NTP to be discussed will include an examination of graphite, composite, carbide, and CERMET core designs and the attributes of each in regards to performance and power generation capability. The focus is on NTP approaches based on tested fuel materials within a prismatic fuel form per the Argonne National Laboratory testing and the ROVER/NERVA program. NTP concepts have been examined for several years at Pratt and Whitney Rocketdyne for use as the primary propulsion for human missions beyond earth. Recently, an approach was taken to examine the design trades between specific NTP concepts; NERVA-based (UC)C-Graphite, (UC,ZrC)C-Composite, (U,Zr)C-Solid Carbide and UO2-W CERMET. Using Pratt and Whitney Rocketdyne's multidisciplinary design analysis capability, a detailed mission and vehicle model has been used to examine how several of these NTP designs impact a human Mars mission. Trends for the propulsion system mass as a function of power level (i.e. thrust size) for the graphite-carbide and CERMET designs were established and correlated against data created over the past forty years. These were used for the mission trade study. The resulting mission trades presented in this paper used a comprehensive modeling approach that captures the mission, vehicle subsystems, and NTP sizing.

  5. Utility Rate Structures and the Impact of Energy Efficiency and...

    Energy Savers [EERE]

    FL Energy Efficiency Calculations * Rates: most common are energy only rates, or a demand rate (kVa or kW) * Demand Rate - Can't use the average cost per kWh for calculations -...

  6. FITCH RATES ENERGY NORTHWEST, WA'S ELECTRIC REV RFDG BONDS 'AA...

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

    FITCH RATES ENERGY NORTHWEST, WA'S ELECTRIC REV RFDG BONDS 'AA'; OUTLOOK STABLE Fitch Ratings-Austin-22 September 2015: Fitch Ratings assigns its 'AA' rating to the following bonds...

  7. Galvanic corrosion of aluminum-matrix composites. Technical report No. 2, 1 Mar-31 Dec 90

    SciTech Connect (OSTI)

    Hihara, L.H.; Latanision, R.M.

    1991-02-01

    Galvanic-corrosion rates of Al-matrix composites were high in aerated chloride-containing solutions. Oxygen reduction was found to be the primary cathodic reaction. Aluminum corroded by pitting. The type of noble constituent (i.e., graphite, SiC, or TiB{sub 2}) also affected galvanic-corrosion rates. For example, results indicated that the galvanic-corrosion rate of Al should be about 30 times greater when coupled to graphite than when coupled to SiC or TiB{sub 2}. In dearated solutions, galvanic corrosion was negligible even if chlorides were present. The galvanic-corrosion rates were determined using the zero-resistance ammeter technique and from potentiodynamic polarization diagrams of ultrapure Al, 6061-T6 Al, graphite fiber, SiC, TiB2, and a commercial graphite fiber/6061-T6 Al metal-matrix composite.

  8. Microsoft Word - BWCS Scorecard Third period FY 2014 Mar 9 2015...

    Office of Environmental Management (EM)

    by the material processed fee rate for the period, which happens to be 67Metric Ton. BWCS processed 22,596 MT of DUF 6 . The fee associated with this is 1,513,932. The Total...

  9. Incorporation of a Helical Tube Heat Transfer Model in the MARS Thermal Hydraulic Systems Analysis Code for the T/H Analyses of the SMART Reactor

    SciTech Connect (OSTI)

    Young Jin Lee; Bub Dong Chung; Jong Chull Jo; Hho Jung Kim; Un Chul Lee

    2004-07-01

    SMART is a medium sized integral type advanced pressurized water reactor currently under development at KAERI. The steam generators of SMART are designed with helically coiled tubes and these are designed to produce superheated steam. The helical shape of the tubes can induce strong centrifugal effect on the secondary coolant as it flows inside the tubes. The presence of centrifugal effect is expected to enhance the formation of cross-sectional circulation flows within the tubes that will increase the overall heat transfer. Furthermore, the centrifugal effect is expected to enhance the moisture separation and thus make it easier to produce superheated steam. MARS is a best-estimate thermal-hydraulic systems analysis code with multi-phase, multi-dimensional analysis capability. The MARS code was produced by restructuring and merging the RELAP5 and the COBRA-TF codes. However, MARS as well as most other best-estimate systems analysis codes in current use lack the detailed models needed to describe the thermal hydraulics of helically coiled tubes. In this study, the heat transfer characteristics and relevant correlations for both the tube and shell sides of helical tubes have been investigated, and the appropriate models have been incorporated into the MARS code. The newly incorporated helical tube heat transfer package is available to the MARS users via selection of the appropriate option in the input. A performance analysis on the steam generator of SMART under full power operation was carried out using the modified MARS code. The results of the analysis indicate that there is a significant improvement in the code predictability. (authors)

  10. Analytical Improvements in PV Degradation Rate Determination

    SciTech Connect (OSTI)

    Jordan, D. C.; Kurtz, S. R.

    2011-02-01

    As photovoltaic (PV) penetration of the power grid increases, it becomes vital to know how decreased power output may affect cost over time. In order to predict power delivery, the decline or degradation rates must be determined accurately. For non-spectrally corrected data several complete seasonal cycles (typically 3-5 years) are required to obtain reasonably accurate degradation rates. In a rapidly evolving industry such a time span is often unacceptable and the need exists to determine degradation rates accurately in a shorter period of time. Occurrence of outliers and data shifts are two examples of analytical problems leading to greater uncertainty and therefore to longer observation times. In this paper we compare three methodologies of data analysis for robustness in the presence of outliers, data shifts and shorter measurement time periods.

  11. Nuclear weak interaction rates in primordial nucleosynthesis

    E-Print Network [OSTI]

    George M. Fuller; Christel J. Smith

    2010-09-01

    We calculate the weak interaction rates of selected light nuclei during the epoch of Big Bang Nucleosynthesis (BBN), and we assess the impact of these rates on nuclear abundance flow histories and on final light element abundance yields. We consider electron and electron antineutrino captures on 3He and 7Be, and the reverse processes of positron capture and electron neutrino capture on 3H and 7Li. We also compute the rates of positron and electron neutrino capture on 6He. We calculate beta and positron decay transitions where appropriate. As expected, the final standard BBN abundance yields are little affected by addition of these weak processes, though there can be slight alterations of nuclear flow histories. However, non-standard BBN scenarios, e.g., those involving out of equilibrium particle decay with energetic final state neutrinos, may be affected by these processes.

  12. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility Rate Home > Utility Rate

  13. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility Rate Home >Utility Rate

  14. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility Rate Home >

  15. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility Rate Home

  16. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility Rate HomeUtility

  17. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility Rate

  18. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtility RateUtility

  19. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtilityRate Home >

  20. Utility Rate | OpenEI Community

    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 JEnvironmental Jump to:EA EISTJThin FilmUnited States:UserLaborUtility RateUtilityRate Home