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

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

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsa31b..07m&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SA31B-07

Physics

2431 Ionosphere/Magnetosphere Interactions (2736), 2736 Magnetosphere/Ionosphere Interactions (2431), 2756 Planetary Magnetospheres (5443, 5737, 6033), 6225 Mars, 7833 Mathematical And Numerical Techniques (0500, 3200)

Scientific paper

The interaction of the solar wind with the Martian 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-Express data and the Mars flyby of the Rosetta spacecraft.

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