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Mathematical and Computational Applications is published by MDPI from Volume 21 Issue 1 (2016). Articles in this Issue were published by another publisher in Open Access under a CC-BY (or CC-BY-NC-ND) licence. Articles are hosted by MDPI on mdpi.com as a courtesy and upon agreement with the previous journal publisher.
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Math. Comput. Appl. 2006, 11(2), 95-102; https://doi.org/10.3390/mca11020095

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
Published: 1 August 2006
PDF [179 KB, uploaded 30 March 2016]

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
This is an open access article distributed under the Creative Commons Attribution License (CC BY 3.0).
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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.

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