Waves and instability in the atmosphere of Mars: NASA planetary atmospheres program

Details Waves and instability in the atmosphere of Mars: NASA planetary atmospheres program Waves and instability in the atmosphere of Mars: NASA planetary atmospheres program

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990osuc.rept.....b&link_type=abstract

Final Report, 1 Jul. 1987 - 31 Dec. 1990 Oregon State Univ., Corvallis.

Mathematics

Atmospheric Heating, Atmospheric Models, Baroclinity, Flow Stability, Gravity Waves, Mars Atmosphere, Mathematical Models, Planetary Atmospheres, Polar Regions, Transport Properties, Vortices, Atmospheric Moisture, Dust

Scientific paper

A broad range of phenomena were addressed by the study including the following: (1) polar warming; (2) forced stationary waves; (3) gravity waves; (4) transient baroclinic eddies; and (5) radiative-dynamical instabilities. A variety of numerical models have been employed in these studies, as well as analytical approaches. Some of the most significant results from this work are very briefly summarized.

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