Development of a Three Dimensional Non-Hydrostatic Model for Martian Atmosphere and a Numerical Simulation of Thermal Convection

Details Development of a Three Dimensional Non-Hydrostatic Model for Martian Atmosphere and a Numerical Simulation of Thermal Convection Development of a Three Dimensional Non-Hydrostatic Model for Martian Atmosphere and a Numerical Simulation of Thermal Convection

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9105o&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 develop a three dimensional non-hydrostatic model and perform a
numerical simulation of thermal convection in the martian atmosphere
without background wind and dust radiative heating.

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