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dc.contributor.authorMaffione, Nicolás P.-
dc.contributor.authorDarriba, Luciano A.-
dc.contributor.authorCincotta, Pablo M.-
dc.contributor.authorGiordano, Claudia M.-
dc.date.accessioned2019-11-25T14:14:53Z-
dc.date.available2019-11-25T14:14:53Z-
dc.date.issued2011-11-
dc.identifier.citationMaffione, Nicolás P., Darriba, Luciano A., Cincotta, Pablo M. y Giordano, Claudia M. (2011). A comparison of different indicators of chaos based on the deviation vectors: application to symplectic mappings. Springer; Celestial Mechanics and Dynamical Astronomy; 111; 285-307es_ES
dc.identifier.issn0923-2958es_ES
dc.identifier.issn1572-9478es_ES
dc.identifier.urihttps://rid.unrn.edu.ar/jspui/handle/20.500.12049/3764-
dc.description.abstractThe aim of this research work is to compare the reliability of several variational indicators of chaos in mappings. The Lyapunov Indicator; the Mean Exponential Growth factor of Nearby Orbits (MEGNO); the Smaller Alignment Index (SALI); the Fast Lyapunov Indicator (FLI); the Dynamical Spectra of stretching numbers and the corresponding Spectral Distance and the Relative Lyapunov Indicator (RLI), which is based on the evolution of the difference between two close orbits, have been included. The experiments presented herein allow us to reliably suggest a group of chaos indicators to analyze a general mapping. We show that a package composed of the FLI and the RLI (to analyze the phase portrait globally) and the MEGNO and the SALI (to analyze orbits individually) is good enough to make a description of the systems’ dynamics.es_ES
dc.format.extentp. 285-307es_ES
dc.format.mediumdigitales_ES
dc.language.isoenes_ES
dc.publisherSpringeres_ES
dc.titleA comparison of different indicators of chaos based on the deviation vectors: application to symplectic mappingses_ES
dc.typeArticuloes_ES
dc.rights.licensehttps://creativecommons.org/licenses/by-nc-sa/4.0/es_ES
dc.description.filiationFil: Maffione, Nicolás P. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. IALP-UNLP-CONICET; Argentina.es_ES
dc.description.filiationFil: Darriba, Luciano A. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. IALP-UNLP-CONICET; Argentina.es_ES
dc.description.filiationFil: Cincotta, Pablo M. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. IALP-UNLP-CONICET; Argentina.es_ES
dc.description.filiationFil: Giordano, Claudia M. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. IALP-UNLP-CONICET; Argentina.es_ES
dc.subject.keywordChaos Indicatorses_ES
dc.subject.keywordMappingses_ES
dc.subject.keywordDynamical Systemses_ES
dc.subject.keywordMEGNOes_ES
dc.subject.keywordSALIes_ES
dc.subject.keywordFLIes_ES
dc.subject.keywordRLIes_ES
dc.subject.keywordSticky Chaotic Orbitses_ES
dc.type.versioninfo:eu-repo/semantics/acceptedVersiones_ES
dc.origin.lugarDesarrolloUniversidad Nacional de La Plataes_ES
dc.origin.lugarDesarrolloIALP-UNLP-CONICETes_ES
dc.relation.journalissue111es_ES
dc.description.reviewtruees_ES
dc.description.resumenThe aim of this research work is to compare the reliability of several variational indicators of chaos in mappings. The Lyapunov Indicator; the Mean Exponential Growth factor of Nearby Orbits (MEGNO); the Smaller Alignment Index (SALI); the Fast Lyapunov Indicator (FLI); the Dynamical Spectra of stretching numbers and the corresponding Spectral Distance and the Relative Lyapunov Indicator (RLI), which is based on the evolution of the difference between two close orbits, have been included. The experiments presented herein allow us to reliably suggest a group of chaos indicators to analyze a general mapping. We show that a package composed of the FLI and the RLI (to analyze the phase portrait globally) and the MEGNO and the SALI (to analyze orbits individually) is good enough to make a description of the systems’ dynamics.es_ES
dc.identifier.doihttps://doi.org/10.1007/s10569-011-9373-z-
dc.relation.journalTitleCelestial Mechanics and Dynamical Astronomyes_ES
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