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.
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Spruit, H.C. (1987). Mixing and Transport of Angular Momentum in the Solar Interior. In: Hillebrandt, W., Meyer-Hofmeister, E., Thomas, HC. (eds) Physical Processes in Comets, Stars and Active Galaxies. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-72640-8_8
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DOI: https://doi.org/10.1007/978-3-642-72640-8_8
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