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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/926
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dc.contributor.authorRedžić, Draganen_US
dc.contributor.authorEldakli, M. S.A.en_US
dc.contributor.authorRedžić, M. D.en_US
dc.date.accessioned2022-07-12T17:29:37Z-
dc.date.available2022-07-12T17:29:37Z-
dc.date.issued2011-01-01-
dc.identifier.issn1937-8726-
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/926-
dc.description.abstractThe Kelvin image theory for a conducting sphere is extended to the case of a conducting oblate spheroid in uniform motion along its axis of revolution (a Heaviside ellipsoid) using the well-known method provided by Special Relativity. The results derived are checked in various ways.en_US
dc.relation.ispartofProgress In Electromagnetics Research Men_US
dc.titleAn extension of the Kelvin image theory to the conducting Heaviside ellipsoiden_US
dc.typeArticleen_US
dc.identifier.doi10.2528/PIERM11051504-
dc.identifier.scopus2-s2.0-79959866215-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/79959866215-
dc.relation.volume18en_US
dc.relation.firstpage233en_US
dc.relation.lastpage246en_US
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.orcid0000-0003-2745-0418-
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