July 23, 2007Open Access

On magnetic instabilities and dynamo action in stellar radiation zones

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Resumen

Context.We examine the MHD instabilities arising in the radiation zone of a differentially rotating star, in which a poloidal field of fossil origin is sheared into a toroidal field.

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Zahn et al. (Mon,) studied this question.

synapsesocial.com/papers/69dcbeff7873f5f05b133a64 https://doi.org/https://doi.org/10.1051/0004-6361:20077653

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