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Article

Cylindrical Magneto-Hydrodynamic Model of Shock Waves with Radiation Heat Flux in Non-Uniform Rotating Atmosphere

by
Ashok Ganguly
* and
Shilpa Shinde
Department of Applied Mathematics, Shri G.S. Institute of Technology and Science, Indore (M.P.) 452003, India
*
Author to whom correspondence should be addressed.
Math. Comput. Appl. 2002, 7(3), 287-296; https://doi.org/10.3390/mca7030287
Published: 1 December 2002
Versions Notes

Abstract

A self similar, theoretical model of cylindrical magneto-hydrodynamics shock wave with radiation heat flux in non-uniform rotating atmosphere, in the rotating medium, in the presence of magnetic field, radiation and gravitation, has been developed. Subsequently, its comparison with the hydro dynamic case has been shown with the help of variations of flow variables with distance graphically. In case of density and radiation flux and mass a significant variation has been observed.
Keywords: Magneto-hydrodynamics shock wave; self similar motion; thermodynamic equilibrium Magneto-hydrodynamics shock wave; self similar motion; thermodynamic equilibrium

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MDPI and ACS Style

Ganguly, A.; Shinde, S. Cylindrical Magneto-Hydrodynamic Model of Shock Waves with Radiation Heat Flux in Non-Uniform Rotating Atmosphere. Math. Comput. Appl. 2002, 7, 287-296. https://doi.org/10.3390/mca7030287

AMA Style

Ganguly A, Shinde S. Cylindrical Magneto-Hydrodynamic Model of Shock Waves with Radiation Heat Flux in Non-Uniform Rotating Atmosphere. Mathematical and Computational Applications. 2002; 7(3):287-296. https://doi.org/10.3390/mca7030287

Chicago/Turabian Style

Ganguly, Ashok, and Shilpa Shinde. 2002. "Cylindrical Magneto-Hydrodynamic Model of Shock Waves with Radiation Heat Flux in Non-Uniform Rotating Atmosphere" Mathematical and Computational Applications 7, no. 3: 287-296. https://doi.org/10.3390/mca7030287

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