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  • 1
    Publication Date: 1991-08-09
    Description: Measurements of rotation rates and gravitational harmonics of Neptune made with the Voyager 2 spacecraft allow tighter constraints on models of the planet's interior. Shock measurements of material that may match the composition of Neptune, the so-calied planetary ;;ice,'' have been carried out to pressures exceeding 200 gigapascals (2 megabars). Comparison of shock data with inferred pressure-density profiles for both Uranus and Neptune shows substantial similarity through most of the mass of both planets. Analysis of the effect of Neptune's strong differential rotation on its gravitational harmonics indicates that differential rotation involves only the outermost few percent of Neptune's mass.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hubbard, W B -- Nellis, W J -- Mitchell, A C -- Holmes, N C -- Limaye, S S -- McCandless, P C -- New York, N.Y. -- Science. 1991 Aug 9;253(5020):648-51.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17772369" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2014-08-22
    Description: Liquid water has been known to occur beneath the Antarctic ice sheet for more than 40 years, but only recently have these subglacial aqueous environments been recognized as microbial ecosystems that may influence biogeochemical transformations on a global scale. Here we present the first geomicrobiological description of water and surficial sediments obtained from direct sampling of a subglacial Antarctic lake. Subglacial Lake Whillans (SLW) lies beneath approximately 800 m of ice on the lower portion of the Whillans Ice Stream (WIS) in West Antarctica and is part of an extensive and evolving subglacial drainage network. The water column of SLW contained metabolically active microorganisms and was derived primarily from glacial ice melt with solute sources from lithogenic weathering and a minor seawater component. Heterotrophic and autotrophic production data together with small subunit ribosomal RNA gene sequencing and biogeochemical data indicate that SLW is a chemosynthetically driven ecosystem inhabited by a diverse assemblage of bacteria and archaea. Our results confirm that aquatic environments beneath the Antarctic ice sheet support viable microbial ecosystems, corroborating previous reports suggesting that they contain globally relevant pools of carbon and microbes that can mobilize elements from the lithosphere and influence Southern Ocean geochemical and biological systems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Christner, Brent C -- Priscu, John C -- Achberger, Amanda M -- Barbante, Carlo -- Carter, Sasha P -- Christianson, Knut -- Michaud, Alexander B -- Mikucki, Jill A -- Mitchell, Andrew C -- Skidmore, Mark L -- Vick-Majors, Trista J -- WISSARD Science Team -- England -- Nature. 2014 Aug 21;512(7514):310-3. doi: 10.1038/nature13667.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Biological Sciences, Louisiana State University, Baton Rouge, Louisiana 70803, USA. ; Department of Land Resources and Environmental Science, Montana State University, Bozeman, Montana 59717, USA. ; Institute for the Dynamics of Environmental Processes - CNR, Venice, and Department of Environmental Sciences, Informatics and Statistics, Ca'Foscari University of Venice, Venice 30123, Italy. ; Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California San Diego, La Jolla, California 92093, USA. ; 1] Physics Department, St Olaf College, Northfield, Minnesota 55057, USA [2] Courant Institute of Mathematical Sciences, New York University, New York, New York 10012, USA (K.C.). ; Department of Microbiology, University of Tennessee, Knoxville, Tennessee 37996, USA. ; Department of Geography and Earth Sciences, Aberystwyth University, Aberystwyth SY23 3DB, UK. ; Department of Earth Science, Montana State University, Bozeman, Montana 59717, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25143114" target="_blank"〉PubMed〈/a〉
    Keywords: Antarctic Regions ; Aquatic Organisms/classification/genetics/*isolation & purification/metabolism ; Archaea/classification/genetics/isolation & purification/metabolism ; Bacteria/classification/genetics/isolation & purification/metabolism ; Carbon/metabolism ; *Ecosystem ; Geologic Sediments/chemistry/microbiology ; *Ice Cover/chemistry ; Lakes/chemistry/*microbiology ; Oceans and Seas ; Phylogeny
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 3
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1996-08-16
    Description: Electrical conductivities of molecular hydrogen in Jupiter were calculated by scaling electrical conductivities measured at shock pressures in the range of 10 to 180 gigapascals (0.1 to 1.8 megabars) and temperatures to 4000 kelvin, representative of conditions inside Jupiter. Jupiter's magnetic field is caused by convective dynamo motion of electrically conducting fluid hydrogen. The data imply that Jupiter should become metallic at 140 gigapascals in the fluid, and the electrical conductivity in the jovian molecular envelope at pressures up to metallization is about an order of magnitude larger than expected previously. The large magnetic field is produced in the molecular envelope closer to the surface than previously thought.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Nellis, W J -- Weir, S T -- Mitchell, A C -- New York, N.Y. -- Science. 1996 Aug 16;273(5277):936-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lawrence Livermore National Laboratory, University of California, Livermore, CA 94550, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/8688072" target="_blank"〉PubMed〈/a〉
    Keywords: Electric Conductivity ; Helium ; *Hydrogen ; *Jupiter ; Magnetics ; Pressure ; Temperature
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 1988-05-06
    Description: Data from the Voyager II spacecraft showed that Uranus has a large magnetic field with geometry similar to an offset tilted dipole. To interpret the origin of the magnetic field, measurements were made of electrical conductivity and equation-of-state data of the planetary "ices" ammonia, methane, and "synthetic Uranus" at shock pressures and temperatures up to 75 gigapascals and 5000 K. These pressures and temperatures correspond to conditions at the depths at which the surface magnetic field is generated. Above 40 gigapascals the conductivities of synthetic Uranus, water, and ammonia plateau at about 20(ohm-cm)(-1), providing an upper limit for the electrical conductivity used in kinematic or dynamo calculations. The nature of materials at the extreme conditions in the interior is discussed.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Nellis, W J -- Hamilton, D C -- Holmes, N C -- Radousky, H B -- Ree, F H -- Mitchell, A C -- Nicol, M -- New York, N.Y. -- Science. 1988 May 6;240(4853):779-81.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17741451" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2012-05-26
    Description: Shortcomings in wheat yield predictions Nature Climate Change 2, 380 11042012 doi: 10.1038/nclimate1511 Mikhail A. Semenov Rowan A. C. Mitchell Andrew P. Whitmore Malcolm J. Hawkesford Martin A. J. Parry Peter R. Shewry Predictions of a 40–140% increase in wheat yield by 2050, reported in the UK Climate Change Risk Assessment, are based on a simplistic approach that ignores key factors affecting yields and hence are seriously misleading.
    Print ISSN: 1758-678X
    Electronic ISSN: 1758-6798
    Topics: Geosciences
    Published by Springer Nature
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  • 6
    Electronic Resource
    Electronic Resource
    [S.l.] : American Institute of Physics (AIP)
    Journal of Applied Physics 69 (1991), S. 2981-2986 
    ISSN: 1089-7550
    Source: AIP Digital Archive
    Topics: Physics
    Notes: Equation-of-state data and corresponding first-principles theory for the metals Al, Cu, Mo, and Pb are reported over the shock pressure range 0.4–2.4 TPa (4–24 Mbar). Strong shock waves were generated by nuclear explosions and a two-stage light-gas gun. The experimental data occur in the hot liquid-metal regime, where condensed-matter theory applies but with unusually large thermal components to the equation of state.
    Type of Medium: Electronic Resource
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  • 7
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: The dissociative phase transition of fluid nitrogen at pressures in the range 30–110 GPa (0.3–1.1 Mbar), temperatures in the range 4000–14 000 K, densities up to 3.5 g/cm3, and internal energies up to 1 MJ/mol was investigated by shock compression. Equation-of-state, shock-temperature, and electrical-conductivity experimental data are presented and analyzed in detail.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 93 (1990), S. 8235-8239 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: Shock temperature measurements have been performed on several materials which have relevance to the modeling of the outer planets. These materials are methane, ammonia and a mixture of water, ammonia, and isopropanol known as synthetic Uranus. Temperatures have been measured in these materials over the pressure range 33–76 GPa for which there also exists measurements of equation of state and electrical conductivity. The temperatures are found to agree well with available calculations, with small discrepancies between data and theory ascribed to energy absorbing processes such as dissociation and molecular ionization.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 88 (1988), S. 5042-5050 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: The electrical conductivity of shock-compressed liquid oxygen has been measured in the dynamic pressure range 18–43 GPa(180–430 Kbar). A double-shock equation-of-state point was also measured. The data and Hugoniot calculation, based on a chemical equilibrium model, indicate that liquid oxygen partially dissociates and forms a two-component conductive fluid. Details of the experimental design are given and the data are discussed in terms of electronic transport in disordered systems.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    College Park, Md. : American Institute of Physics (AIP)
    The Journal of Chemical Physics 95 (1991), S. 5268-5272 
    ISSN: 1089-7690
    Source: AIP Digital Archive
    Topics: Physics , Chemistry and Pharmacology
    Notes: Equation-of-state data were measured for liquid carbon dioxide and air shock-compressed to pressures in the range 28–71 GPa (280–710 kbar) using a two-stage light-gas gun. The experimental methods are described. The data indicate that shock-compressed liquid CO2 decomposes at pressures above 34 GPa. Liquid air dissociates above a comparable shock pressure, as does liquid nitrogen. Theoretical intermolecular potentials are derived for CO2 from the data. The calculated shock temperature for the onset of CO2 decomposition is 4500 K at a volume of 17 cm3/mol.
    Type of Medium: Electronic Resource
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