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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. 2001, 6(3), 177-188; https://doi.org/10.3390/mca6030177

Propagation of Cylindrical Magneto-Gasdynamic Shock Wave with Varying Energy in a Rotating, Gravitating, Non-Uniform Atmosphere

Department of Applied Mathematics, Shri G.S. Institute of Technology and Science, Indore (M.P.) 452 003, India
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Published: 1 December 2001
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Abstract

A self similar, theoretical model of propagation of cylindrical magneto-gasdynamic shock wave with varying energy in a non-uniform atmosphere, in the interplanetary region, in the presence of rotation and gravitation, has been developed. Subsequently, its comparison with the gas dynamic case has been shown with the help of variations of flow variables with distance graphically. It is seen that the presence of magnetic field generates very high energy at the instant of explosion and its absence in gasdynamic model makes the variation of energy docile.
Keywords: Magneto-gasdynamic shock wave; self similar motion; thermodynamic equilibrium Magneto-gasdynamic shock wave; self similar motion; thermodynamic equilibrium
This is an open access article distributed under the Creative Commons Attribution License (CC BY 3.0).
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Ganguly, A.; Shinde, S. Propagation of Cylindrical Magneto-Gasdynamic Shock Wave with Varying Energy in a Rotating, Gravitating, Non-Uniform Atmosphere. Math. Comput. Appl. 2001, 6, 177-188.

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