Atmospheric Excitation of Mars Polar Motion

Details Atmospheric Excitation of Mars Polar Motion Atmospheric Excitation of Mars Polar Motion

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1803k&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1803

Physics

Scientific paper

The rotation of Mars is not constant and present irregularities with
time. Those are mostly associated with the atmosphere, and the
condensation/sublimation of the icecaps. We have estimated the
amplitudes of the two polar motion normal modes, i.e. the Chandler
wobble and the Inner Core wobble.

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