Ground to exobase modeling of the Martian atmosphere using M-GITM

Details Ground to exobase modeling of the Martian atmosphere using M-GITM Ground to exobase modeling of the Martian atmosphere using M-GITM

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufm.p52a..08p&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #P52A-08

Other

[0343] Atmospheric Composition And Structure / Planetary Atmospheres, [0355] Atmospheric Composition And Structure / Thermosphere: Composition And Chemistry, [5405] Planetary Sciences: Solid Surface Planets / Atmospheres, [6225] Planetary Sciences: Solar System Objects / Mars

Scientific paper

A new non-hydrostatic 3D global circulation model called the Mars global ionosphere-thermosphere model (M-GITM) which simulates the Martian atmosphere from the ground to 300 km has recently been developed. Ultimately, the goal of this project is to begin to investigate the response of the Martian atmosphere to a wide range of conditions, including transient features launched from the sun and in the solar wind. M-GITM has been run under a wide range of solar and seasonal conditions to demonstrate that the simulated atmosphere is consistent with other models and observations. In addition, preliminary results are presented which are used to investigate the response of the system to a large solar flare.

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