Modeling of the Venus atmosphere with the non-hydrostatic general circulation model

Details Modeling of the Venus atmosphere with the non-hydrostatic general circulation model Modeling of the Venus atmosphere with the non-hydrostatic general circulation model

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1676m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1676

Physics

Scientific paper

A fully non-hydrostatic, gas-dynamics general circulation model of the Venus atmosphere is presented. Simulations demonstrate the development of superrotation in the deep undercloud atmosphere driven by the thermal tide. Polar vortices reproduced by the model in good agreement with observations presumably result from the interaction of superrotation with subsolar-antisolar circulation near the mesopause.

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