Simulation of the Titan atmosphere with the non-hydrostatic general circulation model

Details Simulation of the Titan atmosphere with the non-hydrostatic general circulation model Simulation of the Titan atmosphere with the non-hydrostatic general circulation model

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1692r&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1692

Physics

Scientific paper

We apply non-hydrostatic, gas-dynamics general circulation model to simulate the dynamics of Titan atmosphere. The model is coupled with the detailed microphysical model of tholin aerosols. Simulations reproduce zonal superrotation with a maximum velocity up to 200-240 m/sec in the jet core between 200 and 300 km altitude and wave-2 features in zonal aerosol distribution.

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