The dissipative effect of thermal radiation loss in high-temperature dense plasmas
arXiv:astro-ph/9711002 · doi:10.1088/0022-3727/29/8/024
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.
4 pages, 1 postscript figure included; RevTeX3.0, epsf.tex needed