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

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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


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