Abstract
A self-similar flow of a perfect gas behind a strong shock driven out by a propelling contact discontinuity surface moving with time according to an exponential law in the presence of axial component of the magnetic field is investigated. The flow between the shock and the inner-expanding surface is assumed to be isothermal. The infinite electrically conductive and uniform medium has been taken into consideration.
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Christer, A. H. and Helliwell, J. B.: 1969,J. Fluid Mech. 39, 705.
Greenspan, H. P.: 1962,Fluids 5, 255.
Grover, R. and Hardy, J. W.: 1966,Astrophys. J. 143, 48.
Gusev, V. N.: 1957, TSAGI Rep., BNI.
Hayes, W. D.: 1968,Fluid Mech. 32, 305.
Laumbach, D. D. and Probstein, R. F.: 1970,Phys. Fluids 13, 1178.
Pai, S. I.: 1958,Proc. Fourth Cong. Theor. Appl. Mech. 89.
Ranga Rao, M. P. and Ramana, B. V.: 1976,J. Math. Phys. Sci. 10, 465.
Verma, B. G. and Singh, J. B.: 1979,Astrophys. Space Sci. 63, 253.
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Singh, J.B., Vishwakarma, P.R. Unsteady isothermal flow of a gas behind an exponential shock in magnetogasdynamics. Astrophys Space Sci 95, 111–116 (1983). https://doi.org/10.1007/BF00661161
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DOI: https://doi.org/10.1007/BF00661161