Influence of atmospheric dynamics on the CO2 ice cloud formation on Mars studied with a general circulation model

Details Influence of atmospheric dynamics on the CO2 ice cloud formation on Mars studied with a general circulation model Influence of atmospheric dynamics on the CO2 ice cloud formation on Mars studied with a general circulation model

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..333k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.333

Physics

Scientific paper

Although CO2 ice clouds on Mars have been observed in the low- and mid-latitude mesosphere, they form in the winter polar regions and create the seasonal polar caps upon sedimentation. We have implemented a CO2 ice cloud formation scheme into our Mars General Circulation Model (MGCM) to investigate the cloud formations and its relation with the atmospheric dynamical processes.

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