电邮这篇文章 Numerical Modeling of the General Circulation of the Atmosphere of Titan at Equinox
- 作者: Mingalev I.V.1, Rodin A.V.2,3, Orlov K.G.1
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隶属关系:
- Polar Geophysical Institute, Russian Academy of Sciences
- Moscow Institute of Physics and Technology
- Space Research Institute, Russian Academy of Sciences
- 期: 卷 53, 编号 4 (2019)
- 页面: 278-293
- 栏目: Article
- URL: https://journals.rcsi.science/0038-0946/article/view/171357
- DOI: https://doi.org/10.1134/S0038094619040051
- ID: 171357
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详细
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.
作者简介
I. Mingalev
Polar Geophysical Institute, Russian Academy of Sciences
编辑信件的主要联系方式.
Email: mingalev_i@pgia.ru
俄罗斯联邦, Apatity, Murmansk oblast, 184209
A. Rodin
Moscow Institute of Physics and Technology; Space Research Institute, Russian Academy of Sciences
Email: mingalev_i@pgia.ru
俄罗斯联邦, Dolgoprudny, Moscow oblast, 141701; Moscow, 117997
K. Orlov
Polar Geophysical Institute, Russian Academy of Sciences
Email: mingalev_i@pgia.ru
俄罗斯联邦, Apatity, Murmansk oblast, 184209
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