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dc.contributor.authorLantos, P.en
dc.contributor.authorAlissandrakis, C. E.en
dc.date.accessioned2015-11-24T18:28:53Z-
dc.date.available2015-11-24T18:28:53Z-
dc.identifier.issn0273-1177-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16200-
dc.rightsDefault Licence-
dc.titleEvolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengthsen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryhttp://dx.doi.org/10.1016/0273-1177(95)00332-9-
heal.identifier.secondaryhttp://www.sciencedirect.com/science/article/pii/0273117795003329-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1995-
heal.abstractThe Nan?ay Radioheliograph provides maps of the quiet solar corona around 160 MHz. In addition to coronal holes, localized emission sources and quiet sun, an unresolved component can be detected on the disk. The so-called coronal plateau corresponds to the K-corona dense regions observed on the limb and is thus located at the base of the interplanetary plasma sheet. Its evolution is studied from 1980 to 1986, during the declining phase of the cycle 21.en
heal.journalNameAdvances in Space Researchen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)



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