The Atmospheric General Circulation of Synchronously Rotating Planets: Dependence on Planetary Rotation Rate

Details The Atmospheric General Circulation of Synchronously Rotating Planets: Dependence on Planetary Rotation Rate The Atmospheric General Circulation of Synchronously Rotating Planets: Dependence on Planetary Rotation Rate

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1364n&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1364

Physics

Scientific paper

We numerically investigate general circulation of moist atmosphere on synchronously rotating planets to examine the dependence of the atmospheric structure on planetary rotation rate. Three representative surface temperature patterns associated with different structure of heat transport appear. However, total amount of energy transport from dayside to nightside has only weak dependence on planetary rotation rate.

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