Self-similar flows behind a spherical radiation-driven shock wave. II
type: Item
instance of: scholarly article
title: Self-similar flows behind a spherical radiation-driven shock wave. II
zbMATH Open document ID: 0511.76121
DOI: 10.1007/BF00653465
author: J. B. Singh
author: R. N. Lal Srivastava
published in: Astrophysics and Space Science
publication date: 1982-01-01T00:00:00Z
Mathematics Subject Classification ID: 76X05
Mathematics Subject Classification ID: 76L05
Mathematics Subject Classification ID: 85A20
Mathematics Subject Classification ID: 85A25
zbMATH DE Number: 3807272
zbMATH Keywords: radiation-driven spherical shock
zbMATH Keywords: non-uniform atmosphere
zbMATH Keywords: optically thin ahead and thick behind the shock front
zbMATH Keywords: isentropic behind shock
zbMATH Keywords: time- dependent total energy content
zbMATH Keywords: self-similar blast wave model
zbMATH Keywords: propelling contact surface
zbMATH Keywords: quiet solar wind region
zbMATH Keywords: varying density distribution
zbMATH Keywords: azimuthal magnetic field
zbMATH Keywords: adiabatic and isothermal flows
zbMATH Keywords: solar flare activity
zbMATH Keywords: strong
zbMATH Keywords: erupting solar plasma
MaRDI profile type: Publication
cites work: Self-similar flows with increasing energy. III: Radiation-driven shock wave
full work available at URL: https://doi.org/10.1007/bf00653465
OpenAlex ID: W1994308975
description: scientific article; zbMATH DE number 3807272