3-D, 3-species, MHD studies of the Interaction of the Solar Wind with Mars.

Details 3-D, 3-species, MHD studies of the Interaction of the Solar Wind with Mars. 3-D, 3-species, MHD studies of the Interaction of the Solar Wind with Mars.

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm12a0838m&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SM12A-0838

Physics

2780 Solar Wind Interactions With Unmagnetized Bodies, 5421 Interactions With Particles And Fields, 5435 Ionospheres (2459)

Scientific paper

We used our 3-species, 3-D, adaptive, MHD code to study the interaction of the solar wind with Mars, using a realistic magnetic field model, which is based on the MGS results. We studied the influence of the remnant, crustal magnetic field on the location and shape of the bowshock and ionopause. We also calculated the ion escape fluxes, for the different conditions considered and find them to be consistent with the measured values.

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