Direct Numerical Simulation of structural vacillation in the transition to geostrophic turbulence

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dc.creatorRandriamampianina, Anthony
dc.creatorMaubert, Pierre
dc.creatorFruh, Wolf-Gerrit
dc.creatorRead, Peter L.
dc.date2007-11-28
dc.date.accessioned2026-07-07T08:45:54Z
dc.date.available2026-07-07T08:45:54Z
dc.descriptionThe onset of small-scale fluctuations around a steady convection pattern in a rotating baroclinic annulus filled with air is investigated using Direct Numerical Simulation. In previous laboratory experiments of baroclinic waves, such fluctuations have been associated with a flow regime termed Structural Vacillation which is regarded as the first step in the transition to fully-developed geostrophic turbulence.
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/0711.4574
dc.identifierhttp://arxiv.org/abs/0711.4574
dc.identifierDans Stratified and Rotating Flows Symposium, Congres Francais de Mecanique - Congres Francais de Mecanique, Grenoble : France (2007)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143108
dc.subjectGeophysics
dc.subjectChaotic Dynamics
dc.titleDirect Numerical Simulation of structural vacillation in the transition to geostrophic turbulence
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