Meridional trend of thermal emission and cooling rate in the Venus cloud layer

Details Meridional trend of thermal emission and cooling rate in the Venus cloud layer Meridional trend of thermal emission and cooling rate in the Venus cloud layer

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1278l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1278

Physics

Scientific paper

Through a great depth of more than 20 km and global coverage, the Venus cloud layer plays an important role in the radiative energy balance. The Venus Express (VEx) observations showed that the cloud top properties significantly change with latitudes. Here we use the structure of the upper cloud derived from the joint analysis of the VeRa and VIRTIS observations to calculate the outgoing thermal flux and cooling rates and discuss the cloud effects.

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