par Giesecke, André;Stefani, Frank;Gerbeth, Gunter;Nore, Caroline;Laguerre, Raphaël 
;Ribeiro, Adolfo;Guermond, Jean Luc;Plunian, Franck;Léorat, Jacques
Référence Geophysical and astrophysical fluid dynamics, 104, 2-3, page (249-271)
Publication Publié, 2010-04
;Ribeiro, Adolfo;Guermond, Jean Luc;Plunian, Franck;Léorat, JacquesRéférence Geophysical and astrophysical fluid dynamics, 104, 2-3, page (249-271)
Publication Publié, 2010-04
Article révisé par les pairs
| Résumé : | In an attempt to understand why the dominating magnetic field observed in the von-Kármán-sodium (VKS) dynamo experiment is axisymmetric, we investigate in the present article the ability of mean field models to generate axisymmetric eigenmodes in cylindrical geometries. An α-effect is added to the induction equation and we identify reasonable and necessary properties of the α distribution so that axisymmetric eigenmodes are generated. The parametric study is done with two different simulation codes. We find that simple distributions of α-effect, either concentrated in the disk neighborhood or occupying the bulk of the flow, require unrealistically large values of the parameter α to explain the VKS observations. © 2010 Taylor & Francis. |
