The Vertical Structure of Martian Aerosols Explored Using a 3D Spherical Monte-Carlo Model and Observations at the Terminator by OMEGA

Details The Vertical Structure of Martian Aerosols Explored Using a 3D Spherical Monte-Carlo Model and Observations at the Terminator by OMEGA The Vertical Structure of Martian Aerosols Explored Using a 3D Spherical Monte-Carlo Model and Observations at the Terminator by OMEGA

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9059v&link_type=abstract

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

Physics

Scientific paper

We present a spherical model of radiative transfer through airborne
particles based on Monte-Carlo methods. We analyze OMEGA observations at
the day/night limit to study the vertical distribution of aerosols
(water ice layers, dust scale height).

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