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 |