Planar motions of a charged particle in a magnetic-binary system with spherical or oblate primaries

Kalvouridis, TJ

dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:10:06Z
dc.date.available	2014-03-01T01:10:06Z
dc.date.issued	1994	en
dc.identifier.issn	0923-2958	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/11316
dc.subject	Magnetic-binary problem	en
dc.subject	periodic orbits	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mathematics, Interdisciplinary Applications	en
dc.title	Planar motions of a charged particle in a magnetic-binary system with spherical or oblate primaries	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00692007	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00692007	en
heal.language	English	en
heal.publicationDate	1994	en
heal.abstract	In this paper we present for the first time simple symmetric motions in the planar magnetic-binary problem where both primaries are spherical bodies or oblate spheroids. From the study of this case it follows that there is a dense and complicated distribution of the families of such motions in the phase space. Our results also show that the orbital characteristics of the particle and the configuration of the phase space are appreciably affected by the oblateness of the primaries only if these parameters become sufficiently large. © 1994 Kluwer Academic Publishers.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Celestial Mechanics & Dynamical Astronomy	en
dc.identifier.doi	10.1007/BF00692007	en
dc.identifier.isi	ISI:A1994ND98200001	en
dc.identifier.volume	58	en
dc.identifier.issue	4	en
dc.identifier.spage	309	en
dc.identifier.epage	315	en