Stellar magnetic fields, according to theory, are caused within the convective zone of the star. The convective circulation of the conducting plasma functions like a . This activity destroys the star's primordial magnetic field, then generates a dipolar magnetic field. As the star undergoes differential rotation—rotating at different rates for various latitudes—the magnetism is wound into a toroidal field of "flux ropes" that become wrapped around the star. The fields can become highly conce. [pdf]
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