dorsal/arxiv
View SchemaMagnetic field induced by elliiptical instability in a rotating tidally distorded sphere
| Authors | P. Le Gal, L. Lacaze, S. Le Dizès |
|---|---|
| Categories | |
| ArXiv ID | physics/0511226 |
| URL | https://arxiv.org/abs/physics/0511226 |
| DOI | 10.1088/1742-6596/14/1/004 |
| Journal | Journal of Physics: conference Series 14 (2005) 30-34 |
Abstract
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.
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"abstract": "It is usually believed that the geo-dynamo of the Earth or more generally of\nother planets, is created by the convective fluid motions inside their molten\ncores. An alternative to this thermal or compositional convection can however\nbe found in the inertial waves resonances generated by the eventual precession\nof these planets or by the possible tidal distorsions of their liquid cores. We\nwill review in this paper some of our experimental works devoted to the\nelliptical instability and present some new results when the experimental fluid\nis a liquid metal. We show in particular that an imposed magnetic field is\ndistorted by the spin- over mode generated by the elliptical instability. In\nour experiment, the field is weak (20 Gauss) and the Lorenz force is negligible\ncompared to the inertial forces, therefore the magnetic field does not modify\nthe fluid flow and the pure hydrodynamics growth rates of the instability are\nrecovered through magnetic measurements.",
"arxiv_id": "physics/0511226",
"authors": [
"P. Le Gal",
"L. Lacaze",
"S. Le Diz\u00e8s"
],
"categories": [
"physics.flu-dyn"
],
"doi": "10.1088/1742-6596/14/1/004",
"journal_ref": "Journal of Physics: conference Series 14 (2005) 30-34",
"title": "Magnetic field induced by elliiptical instability in a rotating tidally distorded sphere",
"url": "https://arxiv.org/abs/physics/0511226"
},
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