Large-Scale Internal Magnetic Field of the Sun
The behaviour of the magnetic field during the formation and evolution of the Sun is investigated. It is shown that an internal poloidal magnetic field of the order of 104 – 105 G near the core of the Sun may be compatible with differential rotation and with torsional waves, travelling along the magnetic field lines (Dudorov et al., 1989).
KeywordsMagnetic Field Line Convection Zone Differential Rotation Toroidal Magnetic Field Torsional Wave
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