Charged particle dynamics in the combined field of two rotating magnetic dipoles: A numerical investigation of the parametric effect on the equatorial motions

Kalvouridis, TJ

dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:29:58Z
dc.date.available	2014-03-01T01:29:58Z
dc.date.issued	2009	en
dc.identifier.issn	0273-1177	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/19426
dc.subject	Charged particles	en
dc.subject	Magnetic dipoles	en
dc.subject.classification	Engineering, Aerospace	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Geosciences, Multidisciplinary	en
dc.subject.classification	Meteorology & Atmospheric Sciences	en
dc.subject.other	Charged particles	en
dc.subject.other	Dynamics	en
dc.subject.other	Magnetic fields	en
dc.subject.other	Magnetic materials	en
dc.subject.other	Magnetism	en
dc.subject.other	Center of masses	en
dc.subject.other	Charged particle dynamics	en
dc.subject.other	Circular orbits	en
dc.subject.other	Equatorial planes	en
dc.subject.other	Magnetic dipoles	en
dc.subject.other	Newtonians	en
dc.subject.other	Numerical investigations	en
dc.subject.other	Parametric effects	en
dc.subject.other	Parametric variations	en
dc.subject.other	Particle motions	en
dc.subject.other	Problem parameters	en
dc.subject.other	Magnetic bubbles	en
dc.title	Charged particle dynamics in the combined field of two rotating magnetic dipoles: A numerical investigation of the parametric effect on the equatorial motions	en
heal.type	journalArticle	en
heal.identifier.primary	10.1016/j.asr.2008.10.022	en
heal.identifier.secondary	http://dx.doi.org/10.1016/j.asr.2008.10.022	en
heal.language	English	en
heal.publicationDate	2009	en
heal.abstract	In this contribution we study some aspects of the dynamics of a charged particle in the field produced by two magnetic dipoles that rotate in circular orbits around their common center of mass under their mutual Newtonian attraction. More precisely, we numerically investigate the evolution of the regions of the particle motion on the equatorial plane of each dipole and we explore their parametric variation. We focus our investigation on those problem parameters that are related with the magnetic fields and the masses of the primaries. The obtained preliminary results show that for each particular set of the above parameters and for certain values of energy these regions are bounded, and therefore the motion of the particle is confined inside them. (C) 2008 COSPAR. Published by Elsevier Ltd. All rights reserved.	en
heal.publisher	ELSEVIER SCI LTD	en
heal.journalName	Advances in Space Research	en
dc.identifier.doi	10.1016/j.asr.2008.10.022	en
dc.identifier.isi	ISI:000263388300007	en
dc.identifier.volume	43	en
dc.identifier.issue	3	en
dc.identifier.spage	377	en
dc.identifier.epage	384	en