Magnetogasdynamic shock waves in a rotating gas with exponentially varying density

DOI10.5402/2012/168315zbMath1360.76118OpenAlexW2120587176WikidataQ58689940 ScholiaQ58689940MaRDI QIDQ454471

J. P. Vishwakarma, G. Nath

Publication date: 8 October 2012

Published in: ISRN Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.5402/2012/168315

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) General theory of rotating fluids (76U05)

Related Items (2)

The propagation of strong cylindrical shock wave in a rotating axisymmetric non‐ideal gas with radiation heat flux ⋮ Lie group of invariance technique for analyzing propagation of strong shock wave in a rotating non‐ideal gas with azimuthal magnetic field

Cites Work

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• Propagation of spherical shock waves in stars
• On the propagation of shock waves through regions of non-uniform area or flow
• Propagation of shock waves in a dusty gas with heat conduction, radiation heat flux and exponentially varying density
• Predictions of Variable-Energy Blast Waves
• Strong cylindrical shocks in a rotating gas
• Similarity solutions for cylindrical blast waves in magnetogasdynamics

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