Height profile of water vapor concentration on Mars

Statistics – Computation

Scientific paper

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Atmospheric Moisture, Mars Atmosphere, Vertical Distribution, Water Vapor, Atmospheric Boundary Layer, Atmospheric Turbulence, Diurnal Variations, Turbulent Diffusion, Turbulent Mixing

Scientific paper

The problem of water vapor mixing in the lower atmosphere of Mars is solved for different values of the turbulent diffusion coefficient, under conditions when condensation and adsorption occur on the surface of the planet for more than half a day. The distribution of water vapor is represented as consisting of two components: (1) one characterized by uniform mixing in the atmosphere up to the condensation level, and (2) the other characterized by excess water content in the near-surface region of the atmosphere. Computational results agree well with experimental data from Mars probe observations for a turbulent diffusion coefficient of 3 x 10 to the 6th sq cm/s.

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