Flux transport solar dynamo models, current problems and possible solutions

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dc.creatorGuerrero, G.
dc.creatorPino, E. M. de Gouveia Dal
dc.date2008-12-05
dc.date.accessioned2026-07-07T12:09:49Z
dc.date.available2026-07-07T12:09:49Z
dc.descriptionThe sunspot solar cycle has been usually explained as the result of a dynamo process operating in the sun. This is a classical problem in Astrophysics that until the present is not fully solved. Here we discuss current problems and limitations with the solar dynamo modeling and their possible solutions using a kinematic dynamo model within the Babcock-Leighton approximation as a tool. In particular, we discuss the importance of the turbulent magnetic pumping versus the meridional flow circulation in the dynamo operation.
dc.descriptionTo appear in the proceedings of the Magnetic Field in the Universe 2 conference, Cozumel, Mexico, January 28th to February 1st, 2008
dc.identifierhttps://arxiv.org/abs/0812.1169
dc.identifierhttp://arxiv.org/abs/0812.1169
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/209757
dc.subjectAstrophysics
dc.titleFlux transport solar dynamo models, current problems and possible solutions
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