Email this article Numerical Modeling of the General Circulation of the Atmosphere of Titan at Equinox
- Authors: Mingalev I.V.1, Rodin A.V.2,3, Orlov K.G.1
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Affiliations:
- Polar Geophysical Institute, Russian Academy of Sciences
- Moscow Institute of Physics and Technology
- Space Research Institute, Russian Academy of Sciences
- Issue: Vol 53, No 4 (2019)
- Pages: 278-293
- Section: Article
- URL: https://journals.rcsi.science/0038-0946/article/view/171357
- DOI: https://doi.org/10.1134/S0038094619040051
- ID: 171357
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Abstract
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.
About the authors
I. V. Mingalev
Polar Geophysical Institute, Russian Academy of Sciences
Author for correspondence.
Email: mingalev_i@pgia.ru
Russian Federation, Apatity, Murmansk oblast, 184209
A. V. Rodin
Moscow Institute of Physics and Technology; Space Research Institute, Russian Academy of Sciences
Email: mingalev_i@pgia.ru
Russian Federation, Dolgoprudny, Moscow oblast, 141701; Moscow, 117997
K. G. Orlov
Polar Geophysical Institute, Russian Academy of Sciences
Email: mingalev_i@pgia.ru
Russian Federation, Apatity, Murmansk oblast, 184209
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