Evolution of surface changes and weather on Titan in the wake of the Fall 2010 equatorial storm

Details Evolution of surface changes and weather on Titan in the wake of the Fall 2010 equatorial storm Evolution of surface changes and weather on Titan in the wake of the Fall 2010 equatorial storm

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1186t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1186

Physics

Scientific paper

We have continued to monitor Titan frequently (at least a few times per month), but to date no significant cloud activity has been observed since Fall 2010. This lack of clouds may indicate that the outbreak removed enough CH4 from the atmosphere and the lapse rate stabilized sufficiently that activity will not resume until the onset of convection at midnorthern latitudes later in the spring.

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