The shell model approach to the rotating turbulence

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dc.creatorReshetnyak, M.
dc.creatorSteffen, B.
dc.date2003-11-03
dc.date.accessioned2026-07-07T05:50:22Z
dc.date.available2026-07-07T05:50:22Z
dc.descriptionApplications of the shell model of turbulence to the case of rapidly rotating bodies are considered. Starting from the classical GOY model we introduce the Coriolis force and obtain a $\sim k^{-2}$ spectrum for 3D hydrodynamical turbulence for the free decay regime as well for the regime with external forcing. Additional modifications of the GOY model providing a realistic form of the helicity are proposed.
dc.identifierhttps://arxiv.org/abs/physics/0311001
dc.identifierhttp://arxiv.org/abs/physics/0311001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/85694
dc.subjectFluid Dynamics
dc.subjectGeophysics
dc.titleThe shell model approach to the rotating turbulence
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