Modelling of self-similar cylindrical shock wave in radiating magnetogasdynamics. I
type: Item
instance of: scholarly article
title: Modelling of self-similar cylindrical shock wave in radiating magnetogasdynamics. I
zbMATH Open document ID: 0608.76112
DOI: 10.1007/BF00637760
author: B. George
published in: Astrophysics and Space Science
publication date: 1986-01-01T00:00:00Z
review text: Self-similar flows of a perfect gas behind a cylindrical blast wave with radiation heat flux in the presence of an azimuthal magnetic field have been investigated. The effects of radiation flux and magnetic field together on the other flow variables have been studied in the region of interest. The magnetic field and density distribution vary as an inverse power of radial distance from the axis of symmetry. The electrical conductivity of the gas is taken to be infinite. The total energy of the flow between the inner expanding surface and the shock is assumed to be constant. We also have supposed the gas to be grey and opaque and the shock to be transparent and isothermal.
Mathematics Subject Classification ID: 76X05
Mathematics Subject Classification ID: 76L05
Mathematics Subject Classification ID: 85A05
zbMATH DE Number: 3984885
zbMATH Keywords: Self-similar flows
zbMATH Keywords: perfect gas
zbMATH Keywords: cylindrical blast wave
zbMATH Keywords: radiation heat flux
zbMATH Keywords: azimuthal magnetic field
zbMATH Keywords: radiation flux
zbMATH Keywords: electrical conductivity
MaRDI profile type: Publication
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description: scientific article; zbMATH DE number 3984885