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Shock Waves Propagation in the Turbulent Interplanetary Plasma

Published online by Cambridge University Press:  12 April 2016

I.V. Chashei  and
V.I. Shishov
I.V. Chashei
Affiliation:
Lebedev Physical Institute, Leninski pr. 53, 117924 Moscow, Russia
V.I. Shishov
Affiliation:
Lebedev Physical Institute, Leninski pr. 53, 117924 Moscow, Russia

Abstract

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Effect of turbulence on interplanetary shock waves propagation is considered. It is shown that background turbulence results in the additional shock wave deceleration which may be comparable with the deceleration due to plasma sweeping. The turbulent deceleration is connected with the energy losses due to the strong turbulence amplification behind the moving shock front.

Keywords

Interplanetary PlasmaShock WavesTurbulence
Type
Origin of Solar and Interplanetary Transients
Information
International Astronomical Union Colloquium , Volume 154: Solar and Interplanetary Transients , 1996 , pp. 23 - 28
Copyright
Copyright © Kluwer 1997

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