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dc.contributor.authorDrago, F. C.en
dc.contributor.authorAlissandrakis, C. E.en
dc.contributor.authorBentley, R. D.en
dc.contributor.authorPhilips, A. T.en
dc.date.accessioned2015-11-24T18:40:32Z-
dc.date.available2015-11-24T18:40:32Z-
dc.identifier.issn0038-0938-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17635-
dc.rightsDefault Licence-
dc.subjecta missionen
dc.subjectwavelengthsen
dc.subjectresolutionen
dc.subjecttelescopeen
dc.subjectemissionen
dc.subjectradioen
dc.subjectloopsen
dc.titleMicrowave, soft and hard X-ray observations of solar flares - A self-consistent model of the flare siteen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000077322300012-
heal.identifier.secondaryhttp://www.springerlink.com/content/jw6147703256410k/fulltext.pdf-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1998-
heal.abstractHigh-resolution microwave observations of several flares performed with the Westerbork Synthesis Radio Telescope (WRST) on 3 and 3 July 1993 are compared with Yuhkoh observations in the soft and hard X-ray domain. Only for one flare, among the six analyzed, was the hard X-ray spectrum between 20 and 200 keV available from the Wide Bragg Spectrometer, supplying the energy spectrum of non-thermal particles responsible for this radiation and for the radio emission. A complete model of this flare is derived which accounts for all available observations in the X-ray and radio wavelengths.en
heal.journalNameSolar Physicsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

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