Microphysics and Radiative Effect of Water Ice Clouds on Mars: Modeling with the LMD/GCM and insights from the OMEGA/MEx Data Set

Details Microphysics and Radiative Effect of Water Ice Clouds on Mars: Modeling with the LMD/GCM and insights from the OMEGA/MEx Data Set Microphysics and Radiative Effect of Water Ice Clouds on Mars: Modeling with the LMD/GCM and insights from the OMEGA/MEx Data Set

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9013m&link_type=abstract

Third International Workshop on The Mars Atmosphere: Modeling and Observations, held November 10-13, 2008 in Williamsburg, Virgi

Computer Science

Scientific paper

Radiatively active water ice clouds of varying effective radius have
been implemented in the LMD/GCM. Resulting water cycle has been compared
to the TES/MGS observations, and to cloud particle size and NIR opacity
retrieved from the OMEGA/MEx data set.

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