Magnetic field induced by elliptical instability in a rotating tidally distorded sphere

Patrice Le Gal (1) , Laurent Lacaze (1) , Stéphane Le Dizès (1)

1 IRPHE - Institut de Recherche sur les Phénomènes Hors Equilibre

It is usually believed that the geo-dynamo of the Earth or more generally of other planets, is created by the convective fluid motions inside their molten cores. An alternative to this thermal or compositional convection can however be found in the inertial waves resonances generated by the eventual precession of these planets or by the possible tidal distorsions of their liquid cores. We will review in this paper some of our experimental works devoted to the elliptical instability and present some new results when the experimental fluid is a liquid metal. We show in particular that an imposed magnetic field is distorted by the spin- over mode generated by the elliptical instability. In our experiment, the field is weak (20 Gauss) and the Lorenz force is negligible compared to the inertial forces, therefore the magnetic field does not modify the fluid flow and the pure hydrodynamics growth rates of the instability are recovered through magnetic measurements.

Domaines: Dynamique des Fluides [physics.flu-dyn]

Patrice Le Gal, Laurent Lacaze, Stéphane Le Dizès. Magnetic field induced by elliptical instability in a rotating tidally distorded sphere. Journal of Physics: Conference Series, 2005, 14, pp.30-34. ⟨10.1088/1742-6596/14/1/004⟩. ⟨hal-00014489⟩