dc.contributor.author | Hallerberg, Sarah | |
dc.contributor.author | Pazó Bueno, Diego Santiago | |
dc.contributor.author | López Martín, Juan Manuel | |
dc.contributor.author | Rodríguez Díaz, Miguel Ángel | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2023-04-21T12:47:02Z | |
dc.date.available | 2023-04-21T12:47:02Z | |
dc.date.issued | 2010-06 | |
dc.identifier.issn | 1539-3755 | |
dc.identifier.issn | 1550-2376 | |
dc.identifier.issn | 2470-0045 | |
dc.identifier.issn | 2470-0053 | |
dc.identifier.other | FIS2009-12964-C05-05 | es_ES |
dc.identifier.other | CGL2007-64387/CLI | es_ES |
dc.identifier.uri | https://hdl.handle.net/10902/28563 | |
dc.description.abstract | Bred 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.sponsorship | Financial 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.extent | 7 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | American Physical Society | es_ES |
dc.rights | ©2010 The American Physical Society | es_ES |
dc.source | Physical Review E - Statistical, Nonlinear, and Soft Matter Physics, 2010, 81(6), 066204 | es_ES |
dc.title | Logarithmic bred vectors in spatiotemporal chaos: structure and growth | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1103/PhysRevE.81.066204 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1103/PhysRevE.81.066204 | |
dc.type.version | publishedVersion | es_ES |