Numerical Modeling of the General Circulation of the Atmosphere of Titan at Equinox

Numerical Modeling of the General Circulation of the Atmosphere of Titan at Equinox

A new model of the general circulation of the atmosphere of Titan is discussed. This model is based on numerical grid integration of the complete equations of gas dynamics with a fine spatial resolution. The relaxation approximation is used to calculate the power of radiation heating and cooling the...

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Veröffentlicht in:Solar system research 2019-07, Vol.53 (4), p.278-293
Hauptverfasser: Mingalev, I. V., Rodin, A. V., Orlov, K. G.
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Astronomy
Astrophysics and Astroparticles
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Physics
Physics and Astronomy
Planetology
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container_title Solar system research
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creator Mingalev, I. V.
Rodin, A. V.
Orlov, K. G.
description A new model of the general circulation of the atmosphere of Titan is discussed. This model is based on numerical grid integration of the complete equations of gas dynamics with a fine spatial resolution. The relaxation approximation is used to calculate the power of radiation heating and cooling the atmospheric gas. The results of simulation of the general atmospheric circulation of Titan at equinox with this model are presented and analyzed.
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subjects Astronomy
Astrophysics and Astroparticles
Astrophysics and Cosmology
Observations and Techniques
Physics
Physics and Astronomy
Planetology
title Numerical Modeling of the General Circulation of the Atmosphere of Titan at Equinox
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