Three-dimensional magnetohydrodynamic description of the process of collision of a solar wind shock wave and the Earth’s bow shock-Reference-Cited by-同舟云学术

Three-dimensional magnetohydrodynamic description of the process of collision of a solar wind shock wave and the Earth’s bow shock

Published:2009-12 Issue:6 Volume:44 Page:917-930
ISSN:0015-4628
Container-title:Fluid Dynamics
language:en
Short-container-title:Fluid Dyn

Author:

Pushkar E. A.

Publisher

Pleiades Publishing Ltd

Subject

Fluid Flow and Transfer Processes,General Physics and Astronomy,Mechanical Engineering

Link

http://link.springer.com/content/pdf/10.1134/S0015462809060155.pdf

Reference28 articles.

1. J.R. Spreiter and A.Y. Alksne, “Plasma Flow around the Magnetosphere,” Rev. Geophys. 7, No. 1–2, 11–69 (1969).

2. V.G. Pivovarov and N.V. Erkaev, Interaction of the Solar Wind with the Earth’s Magnetosphere (Nauka, Novosibirsk, 1978) [in Russian].

3. E.N. Parker, Cosmical Magnetic Field (Clarendon Press, Oxford, 1979; Nauka, Moscow, 1982).

4. V.A. Sergeev and N.A. Tsyganenko, Earth’s Magnetosphere (Nauka, Moscow, 1980) [in Russian].

5. 5. M. Sonders, “Earth’s Magnetosphere,” in E.R. Priest and A.W. Hood (Eds.), Advances in Solar System Magnetohydrodynamics (Cambridge University Press, Cambridge etc., 1991), pp. 366–409.

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