Solar Oblateness and the Abundance of Lithium in the Sun

Physics

Scientific paper

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Scientific paper

The Goldreich-Schubert thermally driven turbulence extending to the deep interiors of solar-type stars which exhibit rotational slowing is precluded by spectroscopic observations showing the presence of lithium and beryllium. These observations, similar observations of the sun, the solar-wind torque, and the solar oblateness are consistent with a model for which such a turbulence is terminated at the surface of a rapidly rotating core containing 95% of the star's mass.

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