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  5. Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)
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Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/17484
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dc.contributor.authorKontogeorgos, A.en
dc.contributor.authorTsitsipis, P.en
dc.contributor.authorMoussas, X.en
dc.contributor.authorPreka-Papadema, G.en
dc.contributor.authorHillaris, A.en
dc.contributor.authorCaroubalos, C.en
dc.contributor.authorAlissandrakis, C.en
dc.contributor.authorBougeret, J. L.en
dc.contributor.authorDumas, G.en
dc.date.accessioned2015-11-24T18:39:41Z-
dc.date.available2015-11-24T18:39:41Z-
dc.identifier.issn0038-6308-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17484-
dc.rightsDefault Licence-
dc.subjectspecial issue wsef sunen
dc.subjectsolar radio burstsen
dc.subjectsolar flaresen
dc.subjectradio spectrographen
dc.subjectfibers pulsationsen
dc.subjectcoronal loop oscillationsen
dc.subjectsolar radio pulsationsen
dc.subjectfine-structuresen
dc.subjectiv bursten
dc.subjectoscillationsen
dc.subjectparametersen
dc.subjectradiationen
dc.titleObserving the sun at 20-650 mhz at thermopylae with artemisen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDOI 10.1007/s11214-006-7492-8-
heal.identifier.secondary<Go to ISI>://000239927800017-
heal.identifier.secondaryhttp://www.springerlink.com/content/43944jn2g34l2v8l/fulltext.pdf-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2006-
heal.abstractFine structure of type IV radio solar bursts with a great variety and complexity often give much information in different ways and enable estimation of various coronal characteristics. In this work, we expose our new method for fine structure revealing and separation of two basic kinds of type IV fine structure, as fibers and pulsations. We also estimate frequency drift of fibers from dynamic spectra, clean from continuous background, with a prototype method using 2-D Fourier transform and we estimate periodicities of fibers as well as pulsations with continuous wavelet transform. Working with the last method we found periodicities close to 3 min umbral oscillations and 5 min global solar oscillations.en
heal.journalNameSpace Science Reviewsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
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