Shri G.S. Institute of Technology and Science, Indore-456 003.
A self-similar theoretical model of propagation of strong plane shock waves in an inhomogeneous, magneto-radiative, self-gravitating atmosphere in the direction of decreasing density is considered. The results discussed depend upon the variations of the flow variables which are displayed graphically and the influences of the gravitation and radiation flux have been studied.
X
Lagrangian coordinate
ΔScale height
ρ*Arbitrary reference density
tTime
αSimilarity exponent
mMass Lagrangian coordinate
MTotal mass ahead of the gas
ηSimilarity variable
KPlanck mean absorption coefficient
Plane shock wave, gravitation, radiation flux, magneto-radiative shock waves, exponentially decreasing medium, wave propagation, fluid flow