Relaxed equilibrium configurations to model fossil fields

Author: Duez V.   Mathis S.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|517|issue|A58-A58

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.517, Iss.issue, 2010-08, pp. : A58-A58

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Abstract

Context. The understanding of fossil fields' origin, topology, and stability is one of the corner stones of the stellar magnetism theory. On one hand, since they survive on secular time scales, they may modify the structure and the evolution of their host stars. On the other hand, they must have a complex stable structure since it has been demonstrated that the simplest purely poloidal or toroidal fields are unstable on dynamical time scales. In this context, the only stable configuration found today is the one resulting from a numerical simulation by Braithwaite and collaborators who studied the evolution of an initial stochastic magnetic field, which is found to relax on a mixed stable configuration (poloidal and toroidal) that seems to be in equilibrium and then diffuses.