Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/16141
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dc.contributor.authorZachariadis, T. G.en
dc.contributor.authorGeorgakilas, A. A.en
dc.contributor.authorKoutchmy, S.en
dc.contributor.authorAlissandrakis, C. E.en
dc.date.accessioned2015-11-24T18:28:26Z-
dc.date.available2015-11-24T18:28:26Z-
dc.identifier.issn0038-0938-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16141-
dc.rightsDefault Licence-
dc.subjectevolutionen
dc.titleFine structure of the solar chromosphere: Arch-shaped mottlesen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://000078944000004-
heal.identifier.secondaryhttp://www.springerlink.com/content/t552333u52992861/fulltext.pdf-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1999-
heal.abstractWe analyze a time series of high resolution observations near the solar limb, obtained in H alpha and the Mg bl line. We identified arch-shaped dark mottles, which are thin, faint H alpha structures observable under very good seeing conditions, best seen in H alpha + 0.75 Angstrom. Their mean length is about 15", their mean height about 6'' and indicative lifetimes is of the order of 5 min. They show negative (away from the observer) line-of-sight velocities. A possible interpretation is that material flows from the apex towards the feet of the arches.en
heal.journalNameSolar Physicsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) - ΦΥΣ

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