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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/123456789/17075
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dc.contributor.authorHillaris, A.en
dc.contributor.authorPetousis, V.en
dc.contributor.authorMitsakou, E.en
dc.contributor.authorVassillou, C.en
dc.contributor.authorMoussas, X.en
dc.contributor.authorPolygiannakis, J.en
dc.contributor.authorPreka-Papadema, P.en
dc.contributor.authorCaroubalos, C.en
dc.contributor.authorAlissandrakis, C.en
dc.contributor.authorTsitsipis, P.en
dc.contributor.authorKontogeorgos, A.en
dc.contributor.authorBougeret, J. L.en
dc.contributor.authorDumas, G.en
dc.date.accessioned2015-11-24T18:35:17Z-
dc.date.available2015-11-24T18:35:17Z-
dc.identifier.issn0273-1177-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17075-
dc.rightsDefault Licence-
dc.subjectsun : coronal mass ejectionsen
dc.subjectsun : flaresen
dc.subjectsun : activityen
dc.subjectsun : x-raysen
dc.subjectx-ray-characteristicsen
dc.subjectradio-burstsen
dc.subjectcmesen
dc.titleSolar flares with and without SOHO/LASCO coronal mass ejections and type II shocksen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryDOI 10.1016/j.asr.2005.11.003-
heal.identifier.secondary<Go to ISI>://000202988200029-
heal.identifier.secondaryhttp://ac.els-cdn.com/S0273117705013992/1-s2.0-S0273117705013992-main.pdf?_tid=7a1c192c6b5c4e66de796a6214d8353c&acdnat=1334133568_29cc80a809cebcca504fbfc611fa4d67-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2006-
heal.abstractWe analyse of a set of radio rich (accompanied by type IV or II bursts) solar flares and their association with SOHO/LASCO Coronal Mass Ejections in the period 1998-2000. The intensity, impulsiveness and energetics of these events are investigated. We find that, on the average, flares associated both with type IIs and CMEs are more impulsive and more energetic than flares associated with type Its only (without CME reported), as well as flares accompanied by type IV continua but not type II shocks. From the last two classes, flares with type II bursts (without CMEs reported) are the shortest in duration and the most impulsive. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.en
heal.journalNameAdvances in Space Researchen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
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