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dc.contributor.authorHallerberg, Sarah
dc.contributor.authorPazó Bueno, Diego Santiago 
dc.contributor.authorLópez Martín, Juan Manuel 
dc.contributor.authorRodríguez Díaz, Miguel Ángel 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-04-21T12:47:02Z
dc.date.available2023-04-21T12:47:02Z
dc.date.issued2010-06
dc.identifier.issn1539-3755
dc.identifier.issn1550-2376
dc.identifier.issn2470-0045
dc.identifier.issn2470-0053
dc.identifier.otherFIS2009-12964-C05-05es_ES
dc.identifier.otherCGL2007-64387/CLIes_ES
dc.identifier.urihttps://hdl.handle.net/10902/28563
dc.description.abstractBred vectors are a type of finite perturbation used in prediction studies of atmospheric models that exhibit spatially extended chaos. We study the structure, spatial correlations, and the growth rates of logarithmic bred vectors (which are constructed by using a given norm). We find that, after a suitable transformation, logarithmic bred vectors are roughly piecewise copies of the leading Lyapunov vector. This fact allows us to deduce a scaling law for the bred vector growth rate as a function of its amplitude. In addition, we relate growth rates with the spectrum of Lyapunov exponents corresponding to the most expanding directions. We illustrate our results with simulations of the Lorenz 1996 model.es_ES
dc.description.sponsorshipFinancial support from the Ministerio de Ciencia e Innovación (Spain) under Projects No. FIS2009-12964-C05-05 and No. CGL2007-64387/CLI is acknowledged. D.P. acknowledges support by CSIC under the Junta de Ampliación de Estudios Programme (JAE-Doc).es_ES
dc.format.extent7 p.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rights©2010 The American Physical Societyes_ES
dc.sourcePhysical Review E - Statistical, Nonlinear, and Soft Matter Physics, 2010, 81(6), 066204es_ES
dc.titleLogarithmic bred vectors in spatiotemporal chaos: structure and growthes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1103/PhysRevE.81.066204es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1103/PhysRevE.81.066204
dc.type.versionpublishedVersiones_ES


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