Abstract
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.
Original language | English |
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Pages (from-to) | 382-390 |
Number of pages | 9 |
Journal | Astrophysical Journal |
Volume | 463 |
Issue number | 1 PART I |
DOIs | |
Publication status | Published - 1996 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science