Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/16142
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dc.contributor.authorGeorgakilas, A. A.en
dc.contributor.authorDara, H.en
dc.contributor.authorZachariadis, T.en
dc.contributor.authorAlissandrakis, C. E.en
dc.contributor.authorKoutchmy, S.en
dc.date.accessioned2015-11-24T18:28:27Z-
dc.date.available2015-11-24T18:28:27Z-
dc.identifier.issn0038-0938-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16142-
dc.rightsDefault Licence-
dc.subjectcontrastsen
dc.subjectfaculaeen
dc.titleFine structure of the solar atmosphere from near-limb observations in three wavelengthsen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondary<Go to ISI>://A1997XL73000018-
heal.languageen-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1997-
heal.abstractWe analyze a time series of high-resolution observations near the limb, in the continuum, in the Mg b(1) line (-0.4 Angstrom off line center), and in the wings of H alpha (+0.75 Angstrom). The observations were obtained with a CCD camera at the Vacuum Tower telescope of the Sacramento Peak Observatory. We study the association of facular points, as they appear at different heights of the solar atmosphere (continuum, b(1) - 0.4 Angstrom, H alpha + 0.75 Angstrom) with the feet of fine dark mottles.en
heal.journalNameSolar Physicsen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)



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