Simulation of Water Cycle With a Martian Weather Research and Forecast Model

Details Simulation of Water Cycle With a Martian Weather Research and Forecast Model Simulation of Water Cycle With a Martian Weather Research and Forecast Model

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufm.p21e..08i&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #P21E-08

Physics

5210 Planetary Atmospheres, Clouds, And Hazes (0343), 6225 Mars

Scientific paper

The water cycle in the Martian atmosphere is influenced by exchange with the subsurface, condensation on the surface, mixing between the boundary layer and the free atmosphere, large-scale horizontal mixing of air masses and precipitation as water ice particles. We have installed a water cycle model with microphysics processes into the Martian Weather Research and Forecast (WRF) model. It treats subsurface water diffusion and adsorptive / condensational exchange, surface ice formation and diffusive mixing in the atmosphere. Formed water ice particles in the atmosphere are transformed by advection, diffusion and sedimentation. We will present the spatial and diurnal variation of water including cloud/fog formation.

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