Chester - Chesnell- Whitham method has been applied to study the propagation of strong spherical shock in the heat radiating atmosphere having uniform density distribution. Neglecting the effect of overtaking disturbances the analytical expressions for shock velocity, shock strength, particle velocity and pressure have been obtained using Bhowmick conditions. The results obtained here are compared with those for non-radiating heat atmosphere.
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R. Yadav; R. K. ; M. K. Gangwar, "Spherical shock in heat radiating atmosphere", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 1, Page Number 47-50, 2018Copy the following to cite this URL:
R. Yadav; R. K. ; M. K. Gangwar, "Spherical shock in heat radiating atmosphere", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 1, Page Number 47-50, 2018Available from: http://ultraphysicalsciences.org/paper/1357/
