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

Authors

  • 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

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Published

2014-01-29

How to Cite

Singh, J. B., & Ram, R. K. (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

License

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