Skip to main content
Log in

Concerning isothermal self-similar blast waves

II: Two-dimensional flow and its stability

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

Abstract

We investigate the two-dimensional self-similar flow behind a blast wave from a line explosion in a medium whose density varies with distance asr −ω with the assumption that the flow is isothermal. If ω<0, a continuous solution passing through the origin and the shock does not exist. If 16/9>ω>0, no critical points exist and a continuous solution passing through both the origin and the shock is shown to exist. If 16/9<ω, two new critical points appear. To be physically acceptable the flow must by-pass both critical points. We show that a continuous solution passing through both the origin and the shock and by-passing both critical points exists in this case. If ω≥2 no physically acceptable solution exists since the mass behind the shock is infinite. The dependence of the solutions which have zero flow velocity at the origin on the parameter ω is analytic for ω>0 so that interpolation between neighboring values of ω is permitted.

We investigate the stability of these isothermal blast waves to two-dimensional but non-self-similar perturbations. If 0<ω<4/3, the solutions are shown to be linearly unstable against short wavelength perturbations near the origin. If 2>ω>1, the self-similar solutions are shown to be globally unstable in a fully non-linear sense; while if 1>ω>0 the solutions are globally unstable unless the solution curves cross the shock with a normalized velocity of precisely (2/ω)1/2.

Thus, for 2>ω>0 the solutions are always unstable somewhere (globally for certain in 2>ω>1; locally in a WKB sense near the origin in 0<ω<4/3). Since there is no characteristic time scale in the system, the local WKB instability near the origin grows as a power law in time rather than exponentially.

The existence of these instabilities implies that initial perturbations do not decay and the system does not tend to a self-similar form.

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

  • Lerche, I.: 1978,Astrophys. Space Sci. 53, 21.

    Google Scholar 

  • Parker, E. N.: 1963,Interplanetary Dynamical Processes Interscience, New York.

    Google Scholar 

  • Sedov, L.: 1959,Similarity and Dimensional Methods in Mechanics, Academic Press, New York.

    Google Scholar 

  • Solinger, A., Rappaport, S. and Buff, J.: 1975,Astrophys. J. 201, 381.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Lerche, I. Concerning isothermal self-similar blast waves. Astrophys Space Sci 53, 39–54 (1978). https://doi.org/10.1007/BF00645902

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00645902

Keywords

Navigation