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Mixing and Transport of Angular Momentum in the Solar Interior

Conference paper

Abstract

The observational indicators of mixing in the solar radiative interior, and the known mechanisms for mixing are reviewed critically. It is concluded that the three most important indicators, Li-depletion, the neutrino discrepancy and the internal rotation, probably each have a different, rather than a common origin. The low internal rotation is interpreted as a strong evidence for the presence of a weak magnetic field in the core of the sun.

Keywords

Rotation Rate Convection Zone Differential Rotation Meridional Circulation Shear Instability 
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 Berlin Heidelberg 1987

Authors and Affiliations

  1. 1.Institut für AstrophysikMax-Planck-Institut für Physik und AstrophysikGarchingFed. Rep. of Germany

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