On the turbulent sources of the solar dynamo

Details On the turbulent sources of the solar dynamo On the turbulent sources of the solar dynamo

2008-12-08

arxiv.org/abs/0812.1466v1

Astronomy and Astrophysics

Astrophysics

7th Int. PAMIR Conf. on Fundamental and Applied MHD (Giens, France, 2008)

Scientific paper

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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