Solar chromospheric structures observed in UV resonance lines: A multivariate analysis approach

dc.contributor.authorPatsourakos, Spirosen
dc.contributor.authorBocchialini, Karineen
dc.contributor.authorVial, Jean-Claudeen
dc.date.accessioned2015-11-24T18:35:18Z
dc.date.available2015-11-24T18:35:18Z
dc.identifier.issn1251-8069-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17079
dc.rightsDefault Licence-
dc.subjectSunen
dc.subjectchromosphereen
dc.subjectradiative transferen
dc.subjectmultivariate methodsen
dc.subjectSoleilen
dc.subjectchromosph?reen
dc.subjecttransfert du rayonnementen
dc.subjectm?thodes multivariablesen
dc.titleSolar chromospheric structures observed in UV resonance lines: A multivariate analysis approachen
heal.abstractWe present the results of a statistical analysis carried out from a data base of six solar chromospheric emission lines recorded simultaneously and with high spectral resolution. An empirical and a clustering method for separating the different solar structure contributions have been used and been found to be in good agreement. Mean profiles corresponding to the different populations have been built. Correlations of different parameters for each profile allowed us to deduce different properties of the solar chromosphere, such as the existence of magnetic canopies and downflows in active regions.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.primaryhttp://dx.doi.org/10.1016/S1251-8069(98)80202-9-
heal.identifier.secondaryhttp://www.sciencedirect.com/science/article/pii/S1251806998802029-
heal.journalNameComptes Rendus de l'Acad?mie des Sciences - Series IIB - Mechanics-Physics-Chemistry-Astronomyen
heal.journalTypepeer reviewed-
heal.publicationDate1998-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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