Cluster Dynamics of Planetary Waves

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dc.creatorKartashova, Elena
dc.creatorL'vov, Victor S.
dc.date2008-01-22
dc.date2008-11-05
dc.date.accessioned2026-07-07T10:15:14Z
dc.date.available2026-07-07T10:15:14Z
dc.descriptionThe dynamics of nonlinear atmospheric planetary waves is determined by a small number of independent wave clusters consisting of a few connected resonant triads. We classified the different types of connections between neighboring triads that determine the general dynamics of a cluster. Each connection type corresponds to substantially different scenarios of energy flux among the modes. The general approach can be applied directly to various mesoscopic systems with 3-mode interactions, encountered in hydrodynamics, astronomy, plasma physics, chemistry, medicine, etc.
dc.description6 pages, 3 figs, EPL, published
dc.identifierhttps://arxiv.org/abs/0801.3374
dc.identifierhttp://arxiv.org/abs/0801.3374
dc.identifierEPL 83: 50012 (2008)
dc.identifierdoi:10.1209/0295-5075/83/50012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173113
dc.subjectChaotic Dynamics
dc.titleCluster Dynamics of Planetary Waves
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