A numerical model of convective motion in the atmosphere of Mars

Details A numerical model of convective motion in the atmosphere of Mars A numerical model of convective motion in the atmosphere of Mars

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993avest..27...85v&link_type=abstract

Astronomicheskij Vestnik (ISSN 0320-930X), vol. 27, no. 2, p. 85-95

Astronomy and Astrophysics

Astronomy

Convective Flow, Mars (Planet), Mars Atmosphere, Mathematical Models, Planetary Meteorology, Flow Stability, Navier-Stokes Equation, Rayleigh Number, Viscous Fluids, Wind (Meteorology)

Scientific paper

Based on the Navier-Stokes equations for a compressed viscous gas, a two-dimensional numerical model of heat convection with a vertical wind shift is constructed. The cases of convection rolls, which are longitudinal and transversal with respect to the wind, are considered. For different Rayleigh numbers, the conditions for stability of the roll structures are determined. They may prove useful for studying the dynamics of the Martian atmosphere for the Aerostat component of the mission Mars-94.

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