On the turbulent sources of the solar dynamo

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dc.creatorPipin, V. V.
dc.creatorSeehafer, N.
dc.date2008-12-08
dc.date.accessioned2026-07-07T12:10:14Z
dc.date.available2026-07-07T12:10:14Z
dc.descriptionWe 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.
dc.description7th Int. PAMIR Conf. on Fundamental and Applied MHD (Giens, France, 2008)
dc.identifierhttps://arxiv.org/abs/0812.1466
dc.identifierhttp://arxiv.org/abs/0812.1466
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/209875
dc.subjectAstrophysics
dc.titleOn the turbulent sources of the solar dynamo
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