The thermal structure of Titan's atmosphere from Cassini radio occultations

Details The thermal structure of Titan's atmosphere from Cassini radio occultations The thermal structure of Titan's atmosphere from Cassini radio occultations

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ttt..work...51f&link_type=abstract

Through Time; A Workshop On Titan's Past, Present and Future, NASA Goddard Space Flight Center, April 6th - 8th, 2010. Edited b

Physics

Scientific paper

Temperatures in Titan's troposphere and stratosphere obtained from Cassini radio occultations at low and high latitudes will be presented. Emphasis will be on the structure of the lower stratosphere at high northern latitudes in winter, where a region of reduced static stability represents the transition between the troposphere, where radiative relaxation times are long and seasonal changes are muted, and the upper stratosphere and mesosophere, where the relaxation times are are shorter and seasonal variations are large. The nature of the atmospheric boundary layer above Titan's surface will also be described.

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