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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2895
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dc.contributor.authorSivaraman, K. R-
dc.contributor.authorGupta, S. S-
dc.contributor.authorKariyappa, R-
dc.date.accessioned2008-07-28T04:49:20Z-
dc.date.available2008-07-28T04:49:20Z-
dc.date.issued1996-01-
dc.identifier.citationSolar Physics, Vol. 163, No. 1, pp. 93 - 97en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2895-
dc.description.abstractWhile evaluating the chromospheric variability (solar cycle related or any other) using the Ca II K line (λ3933.684 Å) as an indicator, an essential prerequisite is the knowledge of the profile of a truly quiet Sun in the integrated light. Such a profile can serve as a bench mark over which enhancements can be measured, particularly when modelling variability. This paper describes how such a K-line profile has been derived for the quiet Sun using disc-integrated light.en
dc.format.extent465626 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996SoPh..163...93Sen
dc.subjectChromospheric variabilityen
dc.subjectK-line profileen
dc.subjectChromosphereen
dc.subjectCa II Ken
dc.subjectH - lineen
dc.titleCA II K Line Profile of the Truly Quiet Sunen
dc.typeArticleen
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