3D, Multi-fluid, MHD Calculations Of Plasma Escape From Mars

Details 3D, Multi-fluid, MHD Calculations Of Plasma Escape From Mars 3D, Multi-fluid, MHD Calculations Of Plasma Escape From Mars

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsm13a1670n&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SM13A-1670

Physics

2753 Numerical Modeling, 2780 Solar Wind Interactions With Unmagnetized Bodies, 6225 Mars

Scientific paper

We use our new multi-fluid, MHD model to calculate plasma escape from Mars. Our lower boundary is set at 100 km and we have a radial grid resolution of about 10 km in the ionosphere. We consider both photo and electron impact ionization, as well as charge exchange processes in calculating the escape fluxes, using a variety of solar and upstream conditions.

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