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dc.contributor.authorHerrera García, Sixto 
dc.contributor.authorPazó Bueno, Diego Santiago 
dc.contributor.authorFernández Fernández, Jesús (matemático) 
dc.contributor.authorRodríguez Díaz, Miguel Ángel 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2013-02-12T09:50:52Z
dc.date.available2013-02-12T09:50:52Z
dc.date.issued2011-10
dc.identifier.issn1600-0870
dc.identifier.issn0280-6495
dc.identifier.otherFIS2009-12964-C05-05
dc.identifier.otherCGL2007-64387/CLI
dc.identifier.otherCGL2010-21869
dc.identifier.otherCGL2010-22158-C02-01
dc.identifier.urihttp://hdl.handle.net/10902/1628
dc.description.abstractThe preparation of perturbed initial conditions to initialize an ensemble of numerical weather forecasts is a crucial task in current ensemble prediction systems (EPSs). Perturbations are added in the places where they are expected to grow faster, in order to provide an envelope of uncertainty along with the deterministic forecast. This work analyses the influence of large-scale spatial patterns on the growth of small perturbations. Therefore, we compare Lyapunov vector (LV) definitions, used in the initialization of state-of-the-art EPSs, with the so-called characteristic LVs. We test the dynamical behaviour of these LVs in the two-scale Lorenz’96 system. We find that the commonly used definitions of LVs include non-intrinsic and spurious effects due to their mutual orthogonality. We also find that the spatial locations where the small-scale perturbations are growing are ‘quantized’ by the large-scale pattern. This ‘quantization’ enhances the artificial disposition of the LVs, which is only avoided using the characteristic LVs, an unambiguous basis which may also be of great use in realistic models for assessing or initializing EPSs.es_ES
dc.description.sponsorshipThe authors thank two anonymous referees for their constructive remarks. We also thank Tony Owen for a revision of the manuscript. The authors are grateful to the Spanish Ministry of Science and Innovation (FIS2009-12964-C05-05, CGL2007-64387/CLI, CGL2010-21869 and CGL2010-22158-C02-01 grants) for partial support of this work. D.P. acknowledges support by CSIC under the Junta de Ampliación de Estudios Programme (JAE-Doc).
dc.format.extent13 p.es_ES
dc.language.isoenges_ES
dc.publisherInternational Meteorological Institute in Stockholmes_ES
dc.rightsAtribución-NoComercial 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc/3.0/es/
dc.sourceTellus A: Dynamic Meteorology and Oceanography, 2011, 63 (5), 978–990es_ES
dc.titleThe role of large-scale spatial patterns in the chaotic amplification of perturbations in a Lorenz’96 modeles_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1111/j.1600-0870.2011.00545.x
dc.type.versionpublishedVersiones_ES


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Atribución-NoComercial 3.0 EspañaExcepto si se señala otra cosa, la licencia del ítem se describe como Atribución-NoComercial 3.0 España