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Adiabatic Spherical Shock Waves in Rotating Magnetized Ideal Gas: Weak-Field Approximation
¹ Department of Physics, Bareilly College, Bareilly, India ² Department of Physics, K.S. Saket (P.G.) College, Ayodhya, India ³ Department of Physics, K.G.K. (P.G.) College, Moradabad, India ⁴ Department of Computer Science and Engineering, Future University, Bareilly, U. P., India
Published Online: November-December 2025
Pages: 70-77
Cite this article
↗ https://www.doi.org/10.59256/ijsreat.20250506012
Adiabatic propagation of spherical magneto hydrodynamic shock waves in an ideal gas has been carried out by the well-known CCW method under the impact of solid body rotation of medium. The effect of constant axial weak magnetic field of the phenomenon is estimated for the converging strong shock with constant angular velocity. Neglecting the flow behind the shock front the analytical expressions for shock velocity, shock strength, pressure and particle velocity just behind the shock front have been derived and discussed with the graphs and tables. The results accomplished here have been compared with dose for normal shock wave and earlier results
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