Mars regional atmospheric modeling system

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[1]. MRAMS, developed by Scot Rafkin and Timothy Michaels, is derived from the Regional Atmospheric Modeling System (RAMS), developed by William Cotton and Roger Pielke, to study atmospheric circulations on the Earth[2].

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[3], the Phoenix Scout Mission, and the Mars Science Laboratory have used MRAMS to study a variety of atmospheric circulations.

References

  1. ^ 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.
  2. ^ 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.
  3. ^ Rafkin, S. C. R. and T. I. Michaels, 2003: Meterological predictions for 2003 Mars Exploration Rover high-priority landing sites. J. Geophys. Res, 108 No. E12,10.1029/2002JE002027


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