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On the Accuracy of Solar Modelling

Published online by Cambridge University Press:  12 April 2016

S. Turck-Chièze
S. Turck-Chièze*
Affiliation:
Service d’Astrophysique, C.E.N. Saclay, 91191 Gif sur Yvette, FRANCE

Abstract

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The confrontation between theoretical predictions and observations requires an estimate of the uncertainties of these predictions. Recent results on nuclear reaction rates and photospheric abundances are analysed, in a classical model framework. The role of opacities in the determination of the helium content, the neutrino fluxes prediction and the adiabatic sound speed is discussed. Comments on extra phenomena as mass loss, turbulent mixing and WIMPS are also presented, in the light of very recent seismological results.

Type
Part 1: Solar Modelling
Information
International Astronomical Union Colloquium , Volume 121: Inside the Sun , 1990 , pp. 125 - 132
Copyright
Copyright © Kluwer 1990

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