Standard solar model

D. B. Guenther, P. Demarque, Y. C. Kim, M. H. Pinsonneault

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Abstract

A set of solar models have been constructed, each based on a single modification to the physics of a reference solar model. In addition, a model combining several of the improvements has been calculated to provide a "best" solar model. Improvements were made to the nuclear reaction rates, the equation of state, the opacities, and the treatment of the atmosphere. The impact on both the structure and the frequencies of the low-l p-modes of the model to these improvements are discussed. We find that the combined solar model, which is based on the best physics available to us (and does not contain any ad hoc assumptions), reproduces the observed oscillation spectrum (for low-l) within the errors associated with the uncertainties in the model physics (primarily opacities).

Original languageEnglish
Pages (from-to)373-393
Number of pages21
JournalAstrophysical Journal
Volume387
Issue number1
Publication statusPublished - 1992 Jan 1

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All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Guenther, D. B., Demarque, P., Kim, Y. C., & Pinsonneault, M. H. (1992). Standard solar model. Astrophysical Journal, 387(1), 373-393.