Seismology of the Standard Solar Model: Tests of Diffusion and the OPAL and MHD Equations of State

Details Seismology of the Standard Solar Model: Tests of Diffusion and the OPAL and MHD Equations of State Seismology of the Standard Solar Model: Tests of Diffusion and the OPAL and MHD Equations of State

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...463..382g&link_type=abstract

Astrophysical Journal v.463, p.382

Astronomy and Astrophysics

Astronomy

34

Atomic Data, Equation Of State, Magnetohydrodynamics: Mhd, Sun: Interior, Sun: Oscillations

Scientific paper

The OPAL equation-of-state tables and the MHD equation-of-state tables are utilized in the calculation of new standard solar models that also include helium diffusion. The structure of the models and their l = 0-100 p-mode oscillation spectra are compared. The p-mode frequencies of the standard solar model are dramatically and nearly identically affected by the inclusion of these detailed equation-of-state formulations. The sensitivities of the p-mode frequencies to other physical uncertainties, in particular the surface conditions, are also discussed.

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