Standard solar model. II. g-modes

D. B. Guenther, P. Demarque, M. H. Pinsonneault, Yong Cheol Kim

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Abstract

We present the g-mode oscillation for a set of modern solar models. Each solar model is based on a single modification or improvement to the physics of a reference solar model. Improvements were made to the nuclear reaction rates, the equation of state, the opacities, and the treatment of the atmosphere. We estimate the error in the predicted g-mode periods associated with the uncertainties in the model physics and describe the specific sensitivities of the g-mode periods and their period spacings to the different model structures. In addition, we compare our models to a sample of published observations. We find remarkably good agreement between our "best" solar model and the observations of Hill & Gu.

Original languageEnglish
Pages (from-to)328-336
Number of pages9
JournalAstrophysical Journal
Volume392
Issue number1
DOIs
Publication statusPublished - 1992 Jun 10

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All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Guenther, D. B., Demarque, P., Pinsonneault, M. H., & Kim, Y. C. (1992). Standard solar model. II. g-modes. Astrophysical Journal, 392(1), 328-336. https://doi.org/10.1086/171432