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

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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

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