Introduction to galactic dynamos

dc.creatorShukurov, Anvar
dc.date2004-11-27
dc.date.accessioned2026-07-07T02:16:03Z
dc.date.available2026-07-07T02:16:03Z
dc.descriptionA review of galactic magnetic fields is given with emphasis on simple analytical solutions of relevant equations and detailed comparison with observations. It is shown that mean-field dynamo theory, in its simplest form, is in a remarkably good agreement with observations of galactic magnetic fields. It is argued that the disc-halo connection can play crucial role in the nonlinear evolution of regular magnetic fields in spiral galaxies by driving flux of magnetic helicity from the disc, thus supporting healthy dynamo action.
dc.description58 pages, 8 figures; to be published in "Mathematical Aspects of Natural Dynamos", EDP Press
dc.identifierhttps://arxiv.org/abs/astro-ph/0411739
dc.identifierhttp://arxiv.org/abs/astro-ph/0411739
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8644
dc.subjectAstrophysics
dc.titleIntroduction to galactic dynamos
dc.typetext

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