Non-ideal effects on the solar equation of state

Details Non-ideal effects on the solar equation of state Non-ideal effects on the solar equation of state

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..499b&link_type=abstract

"in "Helio- and Asteroseismology at the Dawn of the Millennium", SOHO10/GONG2000 Workshop, Santa Cruz de Tenerife, October 2-6,

Statistics

Computation

Solar Interior, Equation Of State, Sun: Non-Ideal Effects, Sun'S Interior

Scientific paper

This paper presents a simple and efficient equation of state which can be used for quick and accurate computation of the thermodynamic functions of partly ionized and weakly coupled plasmas (Bi, Di Mauro and Christensen-Dalsgaard 2000). Based on the free energy minimization method, the improvement of the equation of state includes a detailed account of the physical processes of non-ideal effects consisting of electron degeneracy, Coulomb coupling and pressure ionization. The non-ideal corrections to the equation of state are calculated under solar interior conditions. The result reveals that the contribution is quite significant, and hence modifies the thermodynamic properties of the plasma substantially.

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