Self-similar flows behind a spherical radiation-driven shock wave. II (Q1839175)

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scientific article; zbMATH DE number 3807272
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Self-similar flows behind a spherical radiation-driven shock wave. II
scientific article; zbMATH DE number 3807272

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    Self-similar flows behind a spherical radiation-driven shock wave. II (English)
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    1982
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    radiation-driven spherical shock
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    non-uniform atmosphere
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    optically thin ahead and thick behind the shock front
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    isentropic behind shock
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    time- dependent total energy content
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    self-similar blast wave model
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    propelling contact surface
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    quiet solar wind region
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    varying density distribution
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    azimuthal magnetic field
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    adiabatic and isothermal flows
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    solar flare activity
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    strong
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    erupting solar plasma
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