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- W139987488 abstract "We present the first numerical model of the Titan atmosphere based on GCM with non-hydrostatic dynamical core. The model is set on the triangular mesh with uniform density and covers altitude range from the surface to 550 km. Gas dynamics equations are solved by semi-Lagrangian method that allows for conservation of mass, momentum and energy with high accuracy. Radiation block of the model is based on TGM model[1] and interactively takes into account optical properties of aerosols. The model is integrated with time step of 6 sec on the 16-processor server with shared memory. The resulting meteorological fields demonstrate superrotation with zonal velocity up to 120 m/s, expected for a slowly rotating planet with dense atmosphere. The remarkable difference from conventional hydrostatic GCMs is the enhanced vertical velocities reaching few m/s above the tropopause. A strong wave-1 tidal feature is responsible for decrease of zonal velocity at the altitude of thermal inversion at 7080 km, consistent with observations." @default.
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- W139987488 date "2009-09-01" @default.
- W139987488 modified "2023-09-24" @default.
- W139987488 title "Simulations of tholin haze in the Titan atmosphere with non-hydrostatic General Circulation Model" @default.
- W139987488 hasPublicationYear "2009" @default.
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