Antoine Strugarek, Allan Sacha Brun, J. P. Zahn
Abstract
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Context. The reason for the observed thinness of the solar tachocline is still not well understood. One of the explanations that have been proposed is that a primordial magnetic field renders the rotation uniform in the radiation zone.
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Context. The reason for the observed thinness of the solar tachocline is still not well understood. One of the explanations that have been proposed is that a primordial magnetic field renders the rotation uniform in the radiation zone.
Key concepts: Convection zone, Radiation zone, Tachocline, Differential rotation, Physics, Convection, Rotation (mathematics), Geophysics