Distributed versus tachocline dynamos

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dc.creatorBrandenburg, Axel
dc.date2005-12-29
dc.date.accessioned2026-07-07T06:49:15Z
dc.date.available2026-07-07T06:49:15Z
dc.descriptionArguments are presented in favor of the idea that the solar dynamo may operate not just at the bottom of the convection zone, i.e. in the tachocline, but it may operate in a more distributed fashion in the entire convection zone. The near-surface shear layer is likely to play an important role in this scenario.
dc.description4 pages, 2 figures, in Solar activity: exploration, understanding and prediction, ed: H. Lundstedt, ESA, ESTEC Noordwijk
dc.identifierhttps://arxiv.org/abs/astro-ph/0512638
dc.identifierhttp://arxiv.org/abs/astro-ph/0512638
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104270
dc.subjectAstrophysics
dc.titleDistributed versus tachocline dynamos
dc.typetext

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