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Article information
2004 , Volume 9, Special issue, p.53-58
Denisenko V.V., Erkaev N.V.
Mathematical simulation of the Earth's magnetosphere
The set of the designed mathematical models of the physical processes in the near space is presented. These processes are the results of the solar wind interaction with the Earth's magnetic field. The models are designed in frame of magnetic gas dynamics. The main geophysical results are described.
Classificator Msc2000:- *76W05 Magnetohydrodynamics and electrohydrodynamics
- 86A25 Geo-electricity and geomagnetism
Keywords: ideal MHD model, solar wind, model of magnetosheath flow, magnetic barrier
Author(s):
Denisenko Valery Vasilyevich
Dr. , Senior Scientist
Position: Leading research officer
Office: Institut Computing Simulation of SB RAS
Address: 660036, Russia, Krasnoyarsk, Akademgorodok
Phone Office: (391) 249 57 41
E-mail: denisen@icm.krasn.ru
Erkaev Nikolai Vasilievich
Dr. , Professor
Position: General Scientist
Office: Institut Computing Simulation of SB RAS
Address: 660036, Russia, Krasnoyarsk, Akademgorodok 50/44
Phone Office: (3912) 49 57 41
E-mail: erkaev@icm.krasn.ru
SPIN-code: 1471-5166
Bibliography link:
Denisenko V.V., Erkaev N.V. Mathematical simulation of the Earth's magnetosphere // Computational technologies. 2004. V. 9. Special issue. P. 53-58
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