Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/16973
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dc.contributor.authorSyntelis, P.en
dc.contributor.authorGontikakis, C.en
dc.contributor.authorGeorgoulis, M. K.en
dc.contributor.authorAlissandrakis, C. E.en
dc.contributor.authorTsinganos, K.en
dc.date.accessioned2015-11-24T18:34:37Z-
dc.date.available2015-11-24T18:34:37Z-
dc.identifier.issn0038-0938-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16973-
dc.rightsDefault Licence-
dc.subjectActive regionsen
dc.subjectStructureen
dc.subjectVelocity fielden
dc.subjectMagnetic fieldsen
dc.titleStudy of the Three-Dimensional Shape and Dynamics of Coronal Loops Observed by Hinode/EISen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primary10.1007/s11207-012-0026-5-
heal.identifier.secondaryhttp://dx.doi.org/10.1007/s11207-012-0026-5-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2012-
heal.publisherSpringer Netherlandsen
heal.journalNameSolar Physicsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)



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