Variability of the solar chromospheric network over the solar cycle

dc.contributor.author	Kariyappa, R
dc.contributor.author	Sivaraman, K. R
dc.date.accessioned	2008-07-14T05:51:04Z
dc.date.available	2008-07-14T05:51:04Z
dc.date.issued	1994-06
dc.identifier.citation	Solar Physics, Vol. 152, No. 1, pp. 139 - 144	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/2653
dc.description.abstract	From 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.extent	523499 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994SoPh..152..139K	en
dc.relation.uri	http://www.springerlink.com/content/w6jk4l518p200154/	en
dc.subject	Calcium	en
dc.subject	K Lines	en
dc.subject	Line Shape	en
dc.subject	Network Analysis	en
dc.subject	Photosphere	en
dc.subject	Solar Activity	en
dc.subject	Correlation Coefficients	en
dc.subject	Periodic Variations	en
dc.subject	Solar Cycles	en
dc.title	Variability of the solar chromospheric network over the solar cycle	en
dc.type	Article	en