Skip to main content
Log in

Magneto-radiative supersonic flow with variable specific heat

  • Published:
pure and applied geophysics Aims and scope Submit manuscript

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.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. D. H. Menzel, P. L. Bhatnagar andH. K. Sen,Stellar Interiors, Vol. 6 (1963), 77.

    Google Scholar 

  2. F. C. Auluck andJ. N. Tandon, Proc. Nat. Inst. Sci. (India), [32 A (4)] (1966), p. 404.

    Google Scholar 

  3. B. G. Verma, Pure and Applied Geophysics81 (1970), 124–129.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

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

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00875225

Keywords

Navigation