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Solar equilibrium models and physical processes governing the solar internal structure

  • M. Gabriel
Part II Physical Processes in Modeling the Sun
Part of the Lecture Notes in Physics book series (LNP, volume 367)

Abstract

In the first part of the paper, the uncertainties on the fundamental data and on the input physics relevant for the computation of the internal structure of the Sun are reviewed. In the second part, I present several tests done in order to compute a solar model with a relative accuracy of 3 x 10−5. I also propose a modification of the difference method which allows to achieve the required accuracy with a relatively low number of mesh points.

Keywords

Mesh Point Solar Model Monthly Notice Convective Envelope Standard Solar Model 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag 1990

Authors and Affiliations

  • M. Gabriel
    • 1
  1. 1.Institut d'Astrophysique de l'Université de LiègeLIEGEBelgium

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