Self-similar solution for the flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with magnetic field

DOI10.1016/j.cjph.2019.02.007OpenAlexW2911853136WikidataQ115578511 ScholiaQ115578511MaRDI QIDQ6199539

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Publication date: 21 March 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cjph.2019.02.007

zbMATH Keywords

self-similar solutionshock waverotating mediummagnetogasdynamicsnon-ideal gasinterstellar mediumadiabatic and isothermal flows

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76Lxx) Magnetohydrodynamics and electrohydrodynamics (76Wxx) Rotating fluids (76Uxx)

Cites Work

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• Equatorial propagation of axisymmetric magnetohydrodynamic shocks
• Self-similar adiabatic flow headed by a magnetogasdynamic cylindrical shock wave in a rotating non-ideal gas
• Analytic solutions for the one-dimensional compressible Euler equation with heat conduction closed with different kind of equation of states
• Strong cylindrical shocks in a rotating gas

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