Abstract
The dependence of adiabatic oscillations, particularly their frequencies, on the structure of the sun or other stars is analyzed, on the basis of asymptotic analysis and numerical computations. As a particular example I consider the effects of mixing in the solar core; mixing sufficiently strong to bring the computed neutrino flux into agreement with the observations appears to be inconsistent with the oscillation observations. I also discuss the effects of modifications to the upper, superadiabatic part of the convection zone.
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© 1986 D. Reidel Publishing Company, Dordrecht, Holland
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Christensen-Dalsgaard, J. (1986). Theoretical Aspects of Helio- and Asteroseismology. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_2
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DOI: https://doi.org/10.1007/978-94-009-4608-8_2
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