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6/12/2014 Seminar – The Atmospheric Circulation of Pluto and Trition as Predicted by a General Circulation Model

Published on June 12, 2014

Speaker:Angela Zalucha (SETI Institute)
Date:6/12
Time:4:00pm
Location:SPSC N248

Seminar Abstract:

A variety of previous studies have investigated the 1D vertical temperature-pressure profiles of Pluto and Triton’s atmospheres, while another class of models has investigated the bulk north-south transport of volatiles on these worlds.  However, only recently have modern, 3D general circulation models (GCMs) been applied to Pluto and Triton.

GCMs are global models that solve for the primitive equations of the atmosphere and surface simultaneously, and can be used to predict surface, subsurface, and atmospheric temperature; atmospheric pressure; the three components of atmospheric flow; and surface ice thickness and extent in a physically consistent way.  Most importantly from a meteorological standpoint, is that GCMs are the best tool for predicting atmospheric circulation, since this property is difficult to measure remotely.