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


Дәйексөз келтіру

Толық мәтін

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Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

I. Mingalev

Polar Geophysical Institute, Russian Academy of Sciences

Хат алмасуға жауапты Автор.
Email: mingalev_i@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

A. Rodin

Moscow Institute of Physics and Technology; Space Research Institute, Russian Academy of Sciences

Email: mingalev_i@pgia.ru
Ресей, Dolgoprudny, Moscow oblast, 141701; Moscow, 117997

K. Orlov

Polar Geophysical Institute, Russian Academy of Sciences

Email: mingalev_i@pgia.ru
Ресей, Apatity, Murmansk oblast, 184209

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© Pleiades Publishing, Inc., 2019