Abstract
The point-source, spherical magnetogasdynamics shock wave moving into a constant density γ-law gas is considered in the limit of infinite shock strength, from the point of view of the Richtmyer-Von Neumann viscosity technique. Numerical solutions of this problem has been obtained in viscous and non-viscous regions. A similarity solution of this problem is shown to exist. We have shown that field variables change rapidly when the magnetic field is imposed in both the viscous and the non-viscous regions.
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Supported by CSIR, New DeIhi under the grant No. 7157/287/81-DMR-I.
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Verma, B.G., Srivastava, R.C. & Singh, V.K. Spherical shock waves in viscous magnetogasdynamics. Astrophys Space Sci 111, 253–263 (1985). https://doi.org/10.1007/BF00649969
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DOI: https://doi.org/10.1007/BF00649969