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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Math. Comput. Appl. 2001, 6(3), 177-188; https://doi.org/10.3390/mca6030177
Published: 1 December 2001
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.
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MDPI and ACS Style
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. https://doi.org/10.3390/mca6030177
AMA Style
Ganguly A, Shinde S. Propagation of Cylindrical Magneto-Gasdynamic Shock Wave with Varying Energy in a Rotating, Gravitating, Non-Uniform Atmosphere. Mathematical and Computational Applications. 2001; 6(3):177-188. https://doi.org/10.3390/mca6030177
Chicago/Turabian StyleGanguly, Ashok, and Shilpa Shinde. 2001. "Propagation of Cylindrical Magneto-Gasdynamic Shock Wave with Varying Energy in a Rotating, Gravitating, Non-Uniform Atmosphere" Mathematical and Computational Applications 6, no. 3: 177-188. https://doi.org/10.3390/mca6030177
