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Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium

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Abstract

Strong cylindrical magnetogasdynamic shock waves in rotating interplanetary medium has been studied and an analytic solution for their propagation has been obtained. Using characteristic method and considering the effect of Coriolis force, we have shown that magnetic field has significant effect on the velocity of the shock wave.

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Authors and Affiliations

  1. Department of Mathematics, Gorakhpur University, Gorakhpur, U.P., India

    B. G. Verma, R. C. Srivastava & V. K. Singh

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  1. B. G. Verma
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  2. R. C. Srivastava
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  3. V. K. Singh
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Verma, B.G., Srivastava, R.C. & Singh, V.K. Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium. Astrophys Space Sci 103, 95–98 (1984). https://doi.org/10.1007/BF00650047

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  • DOI: https://doi.org/10.1007/BF00650047

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