Identification of Topographically-controlled Thermal Tidal Modes in the Martian Upper Atmosphere

Details Identification of Topographically-controlled Thermal Tidal Modes in the Martian Upper Atmosphere Identification of Topographically-controlled Thermal Tidal Modes in the Martian Upper Atmosphere

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3069w&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3069

Computer Science

Scientific paper

We use classical theory to identify the main tidal modes. The dominance
of wave-2 and wave-3 in the zonal structure is consistent with the good
overlap between the meridional profiles of solar heating and wave-2 and
wave-3 components of topography.

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