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The dissipative effect of thermal radiation loss in high-temperature dense plasmas

L. H. Li, H. Q. Zhang

astro-pharXiv:astro-ph/9711002

Abstract

A dynamical model based on the two-fluid dynamical equations with energy generation and loss is obtained and used to investigate the self-generated magnetic fields in high-temperature dense plasmas such as the solar core. The self-generation of magnetic fields might be looked at as a self-organization-type behavior of stochastic thermal radiation fields, as expected for an open dissipative system according to Prigogine's theory of dissipative structures.

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