Change in the parameters of the anisotropic interplanetary plasma at the front of an MHD shock wave.

Computer Science

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Interplanetary Plasma: Shock Waves, Interplanetary Plasma: Magnetohydrodynamics

Scientific paper

The change in the parameters of the interplanetary plasma at the front of a magnetohydrodynamic shock wave is studied numerically using an open system of equations of dynamic consistency. The structure of the front is not studied. Possible variants of changes in the parameters of the plasma for weak and strong magnetic fields reflecting the environment in the solar-wind plasma and in the Earth's magnetosphere are studied. It is shown that under conditions of anisotropic pressure the change in the field at the shock wave front is smaller than in the isotropic case. The theoretical results are compared with the experimental data.

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