Modeling the Middle and Upper Atmosphere of Mars for Late 2003 to Early 2004

Details Modeling the Middle and Upper Atmosphere of Mars for Late 2003 to Early 2004 Modeling the Middle and Upper Atmosphere of Mars for Late 2003 to Early 2004

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusm.p21f..02c&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #P21F-02

Physics

5400 Planetology: Solid Surface Planets, 5405 Atmospheres: Composition And Chemistry, 5409 Atmospheres: Structure And Dynamics, 5435 Ionospheres (2459)

Scientific paper

We have created a new Mars GCM that extends from about 14 km above the planetary surface to altitudes of about 300km, thus coupling the lower and upper atmospheres. The model includes Mars-appropriate dynamics, chemistry, and energetics. Some preliminary results for a dust-free tide-free atmosphere are presented, showing temperature and composition profiles, electron density distributions, and global wind patterns for late 2003 to early 2004. The simulations are validated against measurements of neutral density, temperature, and electron density.

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