On the peculiar nature of turbulence in planetary dynamos

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dc.creatorNataf, Henri-Claude
dc.creatorGagnière, Nadège
dc.date2008-05-12
dc.date2008-08-07
dc.date.accessioned2026-07-07T10:17:52Z
dc.date.available2026-07-07T10:17:52Z
dc.descriptionUnder the combined constraints of rapid rotation, sphericity, and magnetic field, motions in planetary cores get organized in a peculiar way. Classical hydrodynamic turbulence is not present, but turbulent motions can take place under the action of the buoyancy and Laplace forces. Laboratory experiments, such as the rotating spherical magnetic Couette DTS experiment in Grenoble, help us understand what motions take place in planetary core conditions.
dc.descriptionin press in Compte Rendu de l'Academie des Sciences
dc.identifierhttps://arxiv.org/abs/0805.1725
dc.identifierhttp://arxiv.org/abs/0805.1725
dc.identifierComptes Rendus Physique 9, 7 (2008) 702-710
dc.identifierdoi:10.1016/j.crhy.2008.07.009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/174003
dc.subjectGeophysics
dc.subjectFluid Dynamics
dc.titleOn the peculiar nature of turbulence in planetary dynamos
dc.typetext

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