Abstract
An approximate analytical solution for self-similar flow behind a spherically-symmetric magnetogasdynamic strong shock wave is investigated using the method of Laumbach and Probstein (1969). The total energy of flow is taken to be dependent on the shock radius obeying a power law. The shock is propagating into a perfect gas at rest with non-uniform density and magnetic field.
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Singh, J.B. An approximate analytical solution of the self-similar flow with frozen-in magnetic field, I. Astrophys Space Sci 95, 291–298 (1983). https://doi.org/10.1007/BF00653635
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DOI: https://doi.org/10.1007/BF00653635