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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1579
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dc.contributor.authorSivaraman, K. R-
dc.contributor.authorGupta, S. S-
dc.contributor.authorKariyappa, R-
dc.date.accessioned2007-05-10T09:11:22Z-
dc.date.available2007-05-10T09:11:22Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 659-661en
dc.identifier.urihttp://hdl.handle.net/2248/1579-
dc.description.abstractWe have derived a mean disc averaged K line profile from observations at the Kodaikanal Solar Tower Telescope on days when sun was relatively very quiet during the years 1985-86. This mean profile would represent the K-line profile of a truly quiet sunen
dc.format.extent141979 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar cycleen
dc.subjectQuiet Sunen
dc.titleWhat is a quiet sun CaII K line profile?en
dc.typeArticleen
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