Magnetogasdynamic exponential shock wave in a self-gravitating, rotational axisymmetric non-ideal gas under the influence of heat-conduction and radiation heat-flux
DOI10.1007/s11587-021-00563-7OpenAlexW3127131781WikidataQ115602053 ScholiaQ115602053MaRDI QIDQ6196240
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Publication date: 14 March 2024
Published in: Ricerche di Matematica (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s11587-021-00563-7
shock wavegravitationrotating mediumnon-ideal gaspiston problemmagnetogasdynamicheat transfer effects
Shock waves and blast waves in fluid mechanics (76L05) General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Diffusive and convective heat and mass transfer, heat flow (80A19)
Cites Work
- Collision of an interplanetary shock wave with the Earth's bow shock. Hydrodynamic parameters and magnetic field
- Self-similar solutions in the theory of flare-ups in novae. I
- Flow behind an exponential shock wave in a rotational axisymmetric non-ideal gas with conduction and radiation heat flux
- Propagation of an exponential shock wave in a rotational axisymmetric isothermal or adiabatic flow of a self-gravitating non-ideal gas under the influence of axial or azimuthal magnetic field
- Effect of Radiation on Shock Wave Behavior
- Effects of internal heat transfer on the structure of self-similar blast waves
- Equatorial propagation of axisymmetric magnetohydrodynamic shocks
- A self-similar solution for blast waves with transport properties
- Similarity solution for a spherical shock wave in a non‐ideal gas under the influence of gravitational field and monochromatic radiation with increasing energy
- The ‘piston problem’ with thermal radiation
- Self-similar piston problems with radiative heat transfer
- Strong cylindrical shocks in a rotating gas
- Cylindrical Shock Waves Produced by Instantaneous Energy Release
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