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Sun / Heat transfer / Physical quantities / Electron / Corona / Thermal conduction / Magnetohydrodynamics / Plasma / Solar wind / Physics / Space plasmas / Plasma physics


Heating of the solar wind with electron and proton effects Ben Breech∗, Steven R. Cranmer†, William H. Matthaeus∗∗ , Justin C. Kasper† and Sean Oughton‡ ∗ NASA Goddard Space Flight Center, 8800 Greenbelt Ro
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Document Date: 2010-11-08 18:10:12


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Hamilton / Cambridge / London / Newark / /

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W. C. Feldman S. P. / E. E. Scime A. E. / /

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New Zealand / /

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USD / /

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University of Delaware / Smithsonian Astrophysical Observatory / Bartol Research Institute / American Institute of Physics / Goddard Space Flight Center / University of Waikato / /

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turbulence model solutions / electron temperature solution / energy containing scale / gas pressure / temperature solutions / internal energy equations / electron solution / proton solution / power law / normalized energy difference / internal energy content / straightforward algebraic solution / energy-containing scale / electron temperature solutions / energy / Model solutions / power-law function / /

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University of Waikato / American Institute of Physics / African Union / National Science Foundation / Harvard / Department of Physics and Astronomy / National Aeronautics and Space Administration / Department of Mathematics / NASA Goddard Space Flight Center / Smithsonian Center for Astrophysics / Bartol Research Institute / Smithsonian / ON PP / University of Delaware / Goddard Space Flight Center / /

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Sean Oughton / L. Sorriso-Valvo / V / William H. Matthaeus / Steven R. Cranmer / Ben Breech / L. Kohl / Justin C. Kasper / Coulomb / /

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model / MHD turbulence transport model for the solar wind / /

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Maryland / Delaware / Massachusetts / /

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ATM / /

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http /

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