Forced stationary planetary waves in Mars's winter atmosphere.

Details Forced stationary planetary waves in Mars's winter atmosphere. Forced stationary planetary waves in Mars's winter atmosphere.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jats...53..428h&link_type=abstract

Journal of Atmospheric Science, Vol. 53, No. 3, p. 428 - 448

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Mars Atmosphere: Dynamics

Scientific paper

Mariner 9 and Viking spacecraft observations provided evidence for planetary-scale, wavelike disturbances in the Mars winter atmosphere. Possible sources of the wave activity are dynamical instabilities, for example, barotropic and/or baroclinic instabilities. Other candidate sources are forced, quasi-stationary planetary waves - waves that arise-predominantly via zonally asymmetric surface properties. The authors attempt to model aspects of the wave activity, focusing on forced planetary waves in representative wintertime atmospheres for Mars, by applying a spherical linear primitive equations model.

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