Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7416
Title: Variations in Ca-K line profiles and Ca-K line features as a function of latitude and solar cycle during the 20th century
Authors: Singh, J
Priyal, M
Sindhuja, G
Ravindra, B
Issue Date: Feb-2018
Publisher: Cambridge University Press
Citation: Proceedings of the International Astronomical Union, Vol. 340, pp. 23-26
Series/Report no.: International Astronomical Union Symposium; 340
Abstract: The analysis of the Ca-K line spectra as a function of latitude and integrated over the visible disk obtained during the period of 1989–2011 at the Kodaikanal Solar Tower Telescope shows that the FWHM of the K1 distribution at different latitudes varies by negligible amount at about 60° latitude whereas it varies significantly at other latitudes. Findings, especially the fewer variations in mid-latitude belts as compared to polar regions and complex variation in the shift in the activity around 60° latitude belt, will have important implications on the modeling of solar dynamos. Further, we have generated a uniform set of digitized Ca-K line images by selecting images considering the intensity distribution of the images corrected for the instrumental vignetting for the data obtained at Kodaikanal during the 20th century. Then, we have determined the percentage of plage and network areas by using the intensity and area threshold values.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7416
ISSN: 1743-9213
???metadata.dc.rights???: © International Astronomical Union
???metadata.dc.relation.uri???: http://dx.doi.org/10.1017/S1743921318001540
Appears in Collections:IIAP Publications



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