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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/37912
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dc.contributor.authorYokoyama, T.-
dc.date.accessioned2014-05-20T15:28:00Z-
dc.date.accessioned2016-10-25T18:02:59Z-
dc.date.available2014-05-20T15:28:00Z-
dc.date.available2016-10-25T18:02:59Z-
dc.date.issued1996-01-01-
dc.identifierhttp://dx.doi.org/10.1007/BF00728350-
dc.identifier.citationCelestial Mechanics & Dynamical Astronomy. Dordrecht: Kluwer Academic Publ, v. 64, n. 3, p. 243-260, 1996.-
dc.identifier.issn0923-2958-
dc.identifier.urihttp://hdl.handle.net/11449/37912-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/37912-
dc.description.abstractA simple generalization of Wisdom's perturbative method, as originally proposed by Wisdom (1985), is obtained. Any number of resonant cosines can be handled and the method can also accommodate more involved disturbing functions. Averaged trajectories are easily obtained by drawing level curves of the action. Here, the method is first tested for simple models of 3:1 and 2:1 resonant problems. Comparisons with numerical integration and surface-section curves show very good agreements.en
dc.format.extent243-260-
dc.language.isoeng-
dc.publisherKluwer Academic Publ-
dc.sourceWeb of Science-
dc.subjectperturbative methodspt
dc.subjectchaospt
dc.subjectresonancept
dc.subjectadiabatic invariantpt
dc.subjectasteroidspt
dc.titleSimple generalization of Wisdom's perturbative methoden
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUNIV ESTADUAL PAULISTA,IGCE,DEMAC,CAIXA POSTAL 178,BR-13500 RIO CLARO,SP,BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,IGCE,DEMAC,CAIXA POSTAL 178,BR-13500 RIO CLARO,SP,BRAZIL-
dc.identifier.doi10.1007/BF00728350-
dc.identifier.wosWOS:A1996WB62500006-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofCelestial Mechanics & Dynamical Astronomy-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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