Extension of a Martian general circulation model to thermospheric altitudes: UV heating and photochemical models

Author:

González-Galindo F.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference66 articles.

1. Photodissociation in the atmosphere of Mars: Impact of high resolution, temperature-dependent CO2 cross-section measurements;Anbar;J. Geophys. Res.,1993

2. Towards a global model of the Martian atmosphere;Angelats i Coll

3. The Mars Thermospheric LMD General Circulation Model: First comparisons with MGS aerobraking data;Angelats i Coll

4. Upper atmosphere of Mars up to 120 km: Mars Global Surveyor accelerometer data analysis with the LMD general circulation model;Angelats i Coll;J. Geophys. Res.,2004

5. The first Mars thermospheric general circulation model: The Martian atmosphere from the ground to 240 km;Angelats i Coll;Geophys. Res. Lett.,2005

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