Haze Transport in Titan's Stratosphere

Details Haze Transport in Titan's Stratosphere Haze Transport in Titan's Stratosphere

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1683b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1683

Physics

Fluid Dynamics

Scientific paper

We continue development of a new Titan General Circulation Model (GCM) using the Flexible Modeling System (FMS) dynamical core from the Geophysical Fluid Dynamics Laboratory (GFDL). The FMS core is state-of-the-art and conserves angular momentum better than other existing dynamical cores which is especially important for modeling Titan's thick atmosphere. Furthermore, an aerosol microphysics package has been developed and linked to the core model. This microphysics is based on the modified version of the Community and Radiation Model for Atmospheres (CARMA) used to study haze and cloud physical processes in Titan's atmosphere [1], [2]. The model also uses a radiative transfer package that is based on the correlated-k two-stream model of [3].

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