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- W1620785839 abstract "We have developed 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 stateof-the-art and actively maintained by GFDL; it conserves angular momentum better than other existing dynamical cores which is especially important for modeling Titan’s thick atmosphere. Furthermore, a basic 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 twostream model of [3])." @default.
- W1620785839 created "2016-06-24" @default.
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- W1620785839 date "2010-09-01" @default.
- W1620785839 modified "2023-09-23" @default.
- W1620785839 title "Simulations of Seasonal Haze Transport on Titan Using the FMS Core GCM" @default.
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