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The helicity constraint in spherical shell dynamos
Authors:A Brandenburg  P J Käpylä  D Mitra  D Moss  R Tavakol
Institution:1. NORDITA, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden

Observatory, University of Helsinki, PO Box 14, FI-00014 University of Helsinki, Finland;2. School of Mathematical Sciences, Queen Mary, University of London, Mile End Road, London E1 4NS, UK;3. School of Mathematics, University of Manchester, Oxford Road, Manchester M13 9PL, UK

Abstract:The motivation for considering distributed large scale dynamos in the solar context is reviewed in connection with the magnetic helicity constraint. Preliminary accounts of 3-dimensional direct numerical simulations (in spherical shell segments) and simulations of 2-dimensional mean field models (in spherical shells) are presented. Interesting similarities as well as some differences are noted. (© 2007 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
Keywords:magnetohydrodynamics (MHD)  turbulence
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