Abstract
The dependence of theoretical eigenfrequencies of five minute oscillation modes on the parameters that determine model solar envelopes has been investigated. It was found that the p mode frequencies are quite strongly correlated with the depth of the convection zone. Comparison of theory with observation suggests that the solar convection zone is about 200,000 km deep.
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Berthomieu, G., Cooper, A.J., Gough, D.O., Osaki, Y., Provost, J., Rocca, A. (1980). Sensitivity of five minute eigenfrequencies to the structure of the sun. In: Hill, H.A., Dziembowski, W.A. (eds) Nonradial and Nonlinear Stellar Pulsation. Lecture Notes in Physics, vol 125. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-09994-8_29
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DOI: https://doi.org/10.1007/3-540-09994-8_29
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