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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2653
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dc.contributor.authorKariyappa, R-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2008-07-14T05:51:04Z-
dc.date.available2008-07-14T05:51:04Z-
dc.date.issued1994-06-
dc.identifier.citationSolar Physics, Vol. 152, No. 1, pp. 139 - 144en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2653-
dc.description.abstractFrom a large sample of the Kodaikanal spectroheliograms in the Ca II K line we have studied the variations in the intensity of the network elements over two solar cycles and have estimated their contribution to the overall variability seen in the disk-averaged K line profiles. The relative contribution of the network elements and the bright points to the K-emission are of the order of 25% and 15% respectively. We have shown that the area of the network elements is anti-correlated with the solar activity, and it increases by about 24% during the solar minimum compared to the maximum period.en
dc.format.extent523499 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/abs/1994SoPh..152..139Ken
dc.relation.urihttp://www.springerlink.com/content/w6jk4l518p200154/en
dc.subjectCalciumen
dc.subjectK Linesen
dc.subjectLine Shapeen
dc.subjectNetwork Analysisen
dc.subjectPhotosphereen
dc.subjectSolar Activityen
dc.subjectCorrelation Coefficientsen
dc.subjectPeriodic Variationsen
dc.subjectSolar Cyclesen
dc.titleVariability of the solar chromospheric network over the solar cycleen
dc.typeArticleen
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