Application of the Regional Atmospheric Modeling System to the Martian Atmosphere

Mathematics – Logic

Scientific paper

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Atmospheric Chemistry, Atmospheric Models, Planetary Cores, Earth Core, Planetary Atmospheres, Meteorological Parameters, Mars Atmosphere, Wind Direction, Three Dimensional Flow, Thermodynamics, Substitutes, Rotation, Reaction Kinetics, Impingement, Craters

Scientific paper

The core dynamics of the Regional Atmospheric Modeling System (RAMS), a widely used and powerful mesoscale Earth model, is adapted to the Martian Atmosphere and applied in the study of aeolian surface features. In particular, research efforts focused on the substitution of Martian planetary and atmospheric properties such as rotation rate, and thermodynamic constants in place of hard-wired Earth properties. Application of the model was restricted to three-dimensional flow impinging upon impact craters, and the search for plausible wind patterns that could produce the so-called light and dark streaks downwind of topographic barriers.

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