3-D motions in the field of two rotating oblate magnetic dipoles

Kalvouridis, T

dc.contributor.author	Kalvouridis, T	en
dc.date.accessioned	2014-03-01T02:51:31Z
dc.date.available	2014-03-01T02:51:31Z
dc.date.issued	2008	en
dc.identifier.issn	0094243X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/35531
dc.subject	Restricted three-body problem	en
dc.subject	Sturmer's problem	en
dc.title	3-D motions in the field of two rotating oblate magnetic dipoles	en
heal.type	conferenceItem	en
heal.identifier.primary	10.1063/1.2993625	en
heal.identifier.secondary	http://dx.doi.org/10.1063/1.2993625	en
heal.publicationDate	2008	en
heal.abstract	The systematic study of the motion of charged particles in an electromagnetic field started with Stornier and its model at the beginning of the 20th century. Since then, many new models have been proposed. One of these is the so-called magnetic-binary problem or alternatively the problem of two rotating dipoles which combines the restricted three-body problem and the initial idea of Störmer. In this work we shall consider that the two primaries of the system are oblate spheroids and we shall try to reveal the mechanism of the evolution of the zero-velocity surfaces that limit the three-dimensional motions of the particle. © 2008 American Institute of Physics.	en
heal.journalName	AIP Conference Proceedings	en
dc.identifier.doi	10.1063/1.2993625	en
dc.identifier.volume	1043	en
dc.identifier.spage	142	en
dc.identifier.epage	146	en