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Solar constraints

Published online by Cambridge University Press:  04 August 2017

Janine Provost
Janine Provost*
Affiliation:
Observatoire de Nice, B.P. 139, 06003 Nice-Cedex, France

Abstract

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Accurate tests of the theory of stellar structure and evolution are available from the Sun's observations. The solar constraints are reviewed, with a special attention to the recent progress in observing global solar oscillations. Each constraint is sensitive to a given region of the Sun. The present solar models (standard, low Z, mixed) are discussed with respect to neutrino flux, low and high degree five-minute oscillations and low degree internal gravity modes. It appears that actually there do not exist solar models able to fully account for all the observed quantities.

Information

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984, pp. 47 - 65
Copyright
Copyright © Reidel 1984 

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