The solar wind interaction with Mars and Venus.

Details The solar wind interaction with Mars and Venus. The solar wind interaction with Mars and Venus.

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....6150n&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #6150

Physics

Scientific paper

We have modified our multi-species, 3D, MHD model of the interaction of the solar wind with Mars and Venus. We have moved from a Cartesian coordinate system to a spherical one, in order to achieve better radial resolution and to achieve a better fit to the shape of the ionosphere-magnetosheath interface in our calculations. This is especially important in order to assess the role of the interaction processes on the ionosphere and the inner magnetosheath. We will be presenting the first results of these new calculations, which also include the effects of the crustal magnetic fields for the case of Mars.

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