Please use this identifier to cite or link to this item:
https://physrep.ff.bg.ac.rs/handle/123456789/926
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Redžić, Dragan | en_US |
dc.contributor.author | Eldakli, M. S.A. | en_US |
dc.contributor.author | Redžić, M. D. | en_US |
dc.date.accessioned | 2022-07-12T17:29:37Z | - |
dc.date.available | 2022-07-12T17:29:37Z | - |
dc.date.issued | 2011-01-01 | - |
dc.identifier.issn | 1937-8726 | - |
dc.identifier.uri | https://physrep.ff.bg.ac.rs/handle/123456789/926 | - |
dc.description.abstract | The 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.ispartof | Progress In Electromagnetics Research M | en_US |
dc.title | An extension of the Kelvin image theory to the conducting Heaviside ellipsoid | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.2528/PIERM11051504 | - |
dc.identifier.scopus | 2-s2.0-79959866215 | - |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/79959866215 | - |
dc.relation.volume | 18 | en_US |
dc.relation.firstpage | 233 | en_US |
dc.relation.lastpage | 246 | en_US |
item.grantfulltext | none | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | No Fulltext | - |
crisitem.author.orcid | 0000-0003-2745-0418 | - |
Appears in Collections: | Journal Article |
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