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Theoretical solar models

Published online by Cambridge University Press:  25 May 2016

J. Provost
J. Provost*
Affiliation:
Département Cassini, UMR CNRS 6529, OCA, BP 229, 06304 Nice CEDEX 4, France

Abstract

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In the last two decades the large amount of accurate helioseismic data has open a new possibility to sound the stellar interiors and to test the stellar evolution theory. This has particularly impulsed a critical reexamination of the basic assumptions and physical inputs in solar modelling. The present status of theoretical solar models is presented and discussed in relation with the observational constraints: helioseismology, lithium depletion and measured neutrino fluxes.

Type
Part II: Internal structure and rotation. Seismic inversions
Information
Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 121 - 136
Copyright
Copyright © Kluwer 1997 

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