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Mars regional atmospheric modeling system
The Mars Regional Atmospheric Modeling System (MRAMS) is a computer program that simulates the circulations of the Martian atmosphere at regional and local scales.〔Rafkin, S. C. R., Haberle, R. M., and T. I. Michaels, 2001: The Mars Regional Atmospheric Modeling System (MRAMS): Model description and selected simulations. Icarus, 151, 228-256.〕 MRAMS, developed by Scot Rafkin and Timothy Michaels, is derived from the Regional Atmospheric Modeling System (RAMS) developed by William R. Cotton and Roger A. Pielke to study atmospheric circulations on the Earth.〔Pielke, R. A.; Cotton, W. R.; Walko, R. L.; Tremback, C. J.; Lyons, W. A.; Grasso, L. D.; Nicholls, M. E.; Moran, M. D.; Wesley, D. A.; Lee, T. J.; Copeland, J. H., 1992: A comprehensive meteorological modeling system: RAMS Meteorology and Atmospheric Physics, vol. 49, issue 1-4, pp. 69-91.〕
Key features of MRAMS include a non-hydrostatic, fully compressible dynamics, explicit bin dust, water, and carbon dioxide ice atmospheric physics model, and a fully prognostic regolith model that includes carbon dioxide deposition and sublimation. Several Mars exploration projects, including the Mars Exploration Rovers,〔Rafkin, S. C. R. and T. I. Michaels, 2003: Meteorological predictions for 2003 Mars Exploration Rover high-priority landing sites. J. Geophys. Res, 108 No. E12,10.1029/2002JE002027〕 the Phoenix Scout Mission, and the Mars Science Laboratory have used MRAMS to study a variety of atmospheric circulations.
==References==
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