Cylindrical Magneto-Hydrodynamic Model of Shock Waves with Radiation Heat Flux in Non-Uniform Rotating Atmosphere
نویسندگان
چکیده
منابع مشابه
The Emergence of Spherical Magneto-gas Dynamic Strong Shock with Radiation near the Surface of a Star with a Rotating , Gravitating, Non-uniform Atmosphere
Department of Applied Mathematics and Computational Science, 1 Shri G. S. Institute of Technology and Science, Indore (M.P.) – 452003, INDIA 2 Jawaharlal Institute of Technology, Borawan (Khargone) -451228, INDIA E-mail : [email protected] Abstract The propagation of a strong magneto-gas dynamic, rotating and gravitating shock wave originating in a stellar interior is considere...
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ژورنال
عنوان ژورنال: Mathematical and Computational Applications
سال: 2002
ISSN: 2297-8747
DOI: 10.3390/mca7030287