3d Hybrid Simulation of the Martian Plasma Environment and Comparison With Rosetta Flyby Data

Details 3d Hybrid Simulation of the Martian Plasma Environment and Comparison With Rosetta Flyby Data 3d Hybrid Simulation of the Martian Plasma Environment and Comparison With Rosetta Flyby Data

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..758b&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Computer Science

Scientific paper

The interaction of the solar wind with theMartian magnetosphere is simulated by a 3d hybrid code model. This approach is applied as the gyroradii of the solar wind protons are in the range of several hundred kilometers and therefore they are comparable to the characteristic scale of the subsolar ionospheric interaction region. Characteristic boundaries as bow shock and ion composition boundary are identified and they are compared with Mars flyby measurements of the Rosetta spacecraft.

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