Abstract
Similarity solutions describing the flow of a perfect gas behind cylindrical shock waves with radiation heat flux are investigated. The total energy of the expanding wave has been supposed to remain constant. The solution, however, is only applicable to a gaseous medium where the undisturbed pressure falls as the inverse square of the distance from the line of explosion.
Similar content being viewed by others
References
Lin, S. C.: 1954,J. Appl. Phys. 25, 54.
Ray, G. Deb: 1957,Proc. Nat. Inst. Sci. India 23A, 420.
Rogers, M. H.: 1958,Quart. J. Mech. Appl. Math.,11, 411.
Sakurai, A.: 1955,J. Phys. Soc. Japan 10, 827.
Singh J. B. and Vishwakarma, P. R.: 1983,Astrophys. Space Sci. 93 423.
Wang, K. C.: 1966,Phys. Fluid 9, 1922.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Singh, J.B. Self-similar cylindrical shock waves with radiation heat flux. Astrophys Space Sci 102, 263–268 (1984). https://doi.org/10.1007/BF00650174
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650174