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Phys. Rev. E 80, 035302(R) (2009) [4 pages]

From reversing to hemispherical dynamos

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Basile Gallet and François Pétrélis
Laboratoire de Physique Statistique de l’Ecole Normale Supérieure, UMR CNRS 8550, 24 Rue Lhomond, 75231 Paris Cedex 5, France

Received 1 May 2009; published 28 September 2009

We show that hemispherical dynamos can result from weak equatorial symmetry breaking of the flow in the interior of planets and stars. Using a model of spherical dynamo, we observe that the interaction between a dipolar and a quadrupolar mode can localize the magnetic field in only one hemisphere when the equatorial symmetry is broken. This process is shown to be related to the one that is responsible for reversals of the magnetic field. These seemingly very different behaviors are thus understood in a unified framework.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevE.80.035302
DOI:
10.1103/PhysRevE.80.035302
PACS:
47.65.−d, 52.65.Kj, 91.25.Cw