Propagation of Cylindrical Shock Waves in a Non-Uniform Rotating Stellar Atmosphere under the Action of Monochromatic Radiation and Gravitation

Shilpa Shinde

doi:10.3390/mca11020095

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Article

1 August 2006

Propagation of Cylindrical Shock Waves in a Non-Uniform Rotating Stellar Atmosphere under the Action of Monochromatic Radiation and Gravitation

Department of Applied Mathematics and Computational Sciences Shri G. S. Institute of Technology and Science 23, Park Road, Indore-452003, India

Math. Comput. Appl.2006, 11(2), 95-102;https://doi.org/10.3390/mca11020095

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Abstract

A self-similar, theoretical model of propagation of cylindrical shock wave in a magneto- gas dynamic rotating non-uniform atmosphere in the presence of monochromatic radiation and gravitation, is considered. The result discussed depends upon the variations of the flow variables behind the shock, which are displayed graphically. A special case is considered in presence and absence of gravitation along with rotation to observe the influence of gravitation.

Keywords:

Magneto-gas dynamic shock wave; Self similar motion; Monochromaticradiation

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