Skip to main content
Log in

An exact similarity solution for a spherical shock wave in a magneto-radiative gas

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

An exact similarity solution for a spherical magneto-gas dynamic shock wave is obtained in the case when the loss of energy due to radiation escape is significant. The total energy of the shock wave is not constant but decreases with time. We have shown that due to the magnetic field, the radiation flux changes considerably.

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

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Verma, B.G., Vishwakarma, J.P. An exact similarity solution for a spherical shock wave in a magneto-radiative gas. Astrophys Space Sci 58, 139–147 (1978). https://doi.org/10.1007/BF00645381

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00645381

Keywords

Navigation