Dopplershifts in the solar transition region

dc.contributor.authorGontikakis, C.en
dc.contributor.authorDara, H. C.en
dc.contributor.authorAlissandrakis, C. E.en
dc.contributor.authorZachariadis, T. G.en
dc.contributor.authorVial, J. C.en
dc.date.accessioned2015-11-24T18:30:00Z
dc.date.available2015-11-24T18:30:00Z
dc.identifier.issn1432-0746-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16326
dc.rightsDefault Licence-
dc.subjectsun : transition regionen
dc.subjectline formationen
dc.subjectcoronal diagnostic spectrometeren
dc.subjectultraviolet emission-linesen
dc.subjectquiet-sun connectionen
dc.subjectlate-type starsen
dc.subjectspectrograph observationsen
dc.subjectobserved redshiftsen
dc.subjectsumer observationsen
dc.subjectactive-regionen
dc.subjectc-iven
dc.subjectchromosphereen
dc.titleDopplershifts in the solar transition regionen
heal.abstractWe study the dynamics of the quiet sun transition region, using observations obtained with the SOHO CDS/NIS and SUMER spectrographs. We examine the morphology of the network as a function of temperature and we compare the intensity features with those of the dopplergrams. The velocity distributions have a different behaviour for the bright features which outline the network and the dark ones, located in the internetwork. A redshift and a smaller standard deviation are observed for the bright feature distributions relative to the dark ones. It should be mentioned that the internetwork is also statistically redshifted, with the exception of the He I line. Velocity distributions from different lines are compared.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.secondary<Go to ISI>://000171486600033-
heal.journalNameAstronomy & Astrophysicsen
heal.journalTypepeer reviewed-
heal.languageen-
heal.publicationDate2001-
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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