Self-Similar Flow Behind a Spherical Radiation-Driven Shock Wave in Magnetogasdynamics

  • J. B. Singh S.G.R. Postgraduate College, Jaunpur
  • R. K. Ram S.G.R. Postgraduate College, Jaunpur
DOI: https://doi.org/10.14429/dsj.34.6072
Keywords: Magnetogasdynamics, Adiabatic and Isothermal

Abstract

Adiabatic and isothermal self-similar flows behind a radiation-driven shock wave in the presence of magnetic field have been investigated by using the generalised method of Laumbach and Probstein for magnetogasdynamics. The density and magnetic field distributions of the gas ahead of the shock have beenassumed to be constant.

Author Biographies

J. B. Singh, S.G.R. Postgraduate College, Jaunpur
Department of Mathematics & Physics, S.G.R. Postgraduate College, Jaunpur
R. K. Ram, S.G.R. Postgraduate College, Jaunpur
Department of Mathematics & Physics, S.G.R. Postgraduate College, Jaunpur
Published
2014-01-29
How to Cite
Singh, J., & Ram, R. (2014). Self-Similar Flow Behind a Spherical Radiation-Driven Shock Wave in Magnetogasdynamics. Defence Science Journal, 34(3), 263-274. https://doi.org/10.14429/dsj.34.6072
Issue
Vol 34 No 3
Section
General Papers
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