The symplectic character of the three-dimensional magnetic-binary problem

Kalvouridis, T; Mavraganis, A; Pangalos, C

dc.contributor.author	Kalvouridis, T	en
dc.contributor.author	Mavraganis, A	en
dc.contributor.author	Pangalos, C	en
dc.date.accessioned	2014-03-01T01:06:13Z
dc.date.available	2014-03-01T01:06:13Z
dc.date.issued	1983	en
dc.identifier.issn	0004-640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9238
dc.subject	symplectic matrix	en
dc.subject	Three Dimensional	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.title	The symplectic character of the three-dimensional magnetic-binary problem	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00651670	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00651670	en
heal.language	English	en
heal.publicationDate	1983	en
heal.abstract	The authors' purpose is to generalize in this paper the symplectic character of the particle motions in the three-dimensional magnetic-binary problem. By adopting the classical electrodynamical formulation they find out the general form of the symplectic matrix as well as some relations between the variations of an orbit, which way be used to check the accuracy of any numerical work related to the orbits investigation. © 1983 D. Reidel Publishing Company.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/BF00651670	en
dc.identifier.isi	ISI:A1983RV68400004	en
dc.identifier.volume	96	en
dc.identifier.issue	2	en
dc.identifier.spage	255	en
dc.identifier.epage	259	en