Summary
Formulae for stagnation conditions and for the one dimensional flow through shock waves considering variable specific heat have been derived in the presence of magnetic field and radiation effects. These formulae have been compared with those for constant specific heat to obtain correction factors in order to make them valid for reasonably high Mach numbers.
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References
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B. G. Verma, Pure and Applied Geophysics81 (1970), 124–129.
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Verma, B.G., Srivastava, S.K. Magneto-radiative supersonic flow with variable specific heat. PAGEOPH 93, 91–99 (1972). https://doi.org/10.1007/BF00875225
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DOI: https://doi.org/10.1007/BF00875225