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Article

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

by
Shilpa Shinde
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
Published: 1 August 2006
Versions Notes

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

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MDPI and ACS Style

Shinde, S. Propagation of Cylindrical Shock Waves in a Non-Uniform Rotating Stellar Atmosphere under the Action of Monochromatic Radiation and Gravitation. Math. Comput. Appl. 2006, 11, 95-102. https://doi.org/10.3390/mca11020095

AMA Style

Shinde S. Propagation of Cylindrical Shock Waves in a Non-Uniform Rotating Stellar Atmosphere under the Action of Monochromatic Radiation and Gravitation. Mathematical and Computational Applications. 2006; 11(2):95-102. https://doi.org/10.3390/mca11020095

Chicago/Turabian Style

Shinde, Shilpa. 2006. "Propagation of Cylindrical Shock Waves in a Non-Uniform Rotating Stellar Atmosphere under the Action of Monochromatic Radiation and Gravitation" Mathematical and Computational Applications 11, no. 2: 95-102. https://doi.org/10.3390/mca11020095

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