Potential Vorticity, Angular Momentum and Inertial Instabilities in the Martian Atmospheric Circulation from Assimilated Analyses of MGS/TES

Details Potential Vorticity, Angular Momentum and Inertial Instabilities in the Martian Atmospheric Circulation from Assimilated Analyses of MGS/TES Potential Vorticity, Angular Momentum and Inertial Instabilities in the Martian Atmospheric Circulation from Assimilated Analyses of MGS/TES

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1447.9104r&link_type=abstract

Third International Workshop on The Mars Atmosphere: Modeling and Observations, held November 10-13, 2008 in Williamsburg, Virgi

Physics

Scientific paper

Data based on re-analyses of the MGS/TES observations have been used to
map distributions of potential vorticity and axial absolute angular
momentum. Distribution of angular momentum and potential vorticity are
closely related to the zonal-mean circulation.

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