The solar interior - radial structure, rotation, solar activity cycle

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dc.creatorBrandenburg, Axel
dc.date2007-03-28
dc.date.accessioned2026-07-07T08:26:27Z
dc.date.available2026-07-07T08:26:27Z
dc.descriptionSome basic properties of the solar convection zone are considered and the use of helioseismology as an observational tool to determine its depth and internal angular velocity is discussed. Aspects of solar magnetism are described and explained in the framework of dynamo theory. The main focus is on mean field theories for the Sun's magnetic field and its differential rotation.
dc.description45 pages, 17 figures, to appear in Handbook of Solar-Terrestrial Environment, eds. Y. Kamide & A. C.-L. Chian, Springer
dc.identifierhttps://arxiv.org/abs/astro-ph/0703711
dc.identifierhttp://arxiv.org/abs/astro-ph/0703711
dc.identifierin Handbook of Solar-Terrestrial Environment, ed. Y. Kamide & A. C.-L. Chian, Springer, pp. 27-54 (2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/136942
dc.subjectAstrophysics
dc.titleThe solar interior - radial structure, rotation, solar activity cycle
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