On the turbulent sources of the solar dynamo

V. V. Pipin; N. Seehafer

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arXiv · 0812.1466

On the turbulent sources of the solar dynamo

V. V. Pipin·N. Seehafer

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Abstract

We revisit the possible turbulent sources of the solar dynamo. Studying axisymmetric mean-field dynamo models, we find that the large-scale poloidal magnetic field could be generated not only by the famous alpha effect, but also by the Omega x J and shear-current effects. The inclusion of these additional turbulent sources alleviates several of the known problems of solar mean-field dynamo models.

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V. V. Pipin, N. Seehafer. 2008-12-08. On the turbulent sources of the solar dynamo. https://arxiv.org/abs/0812.1466

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