CA II K Line Profile of the Truly Quiet Sun

dc.contributor.author	Sivaraman, K. R
dc.contributor.author	Gupta, S. S
dc.contributor.author	Kariyappa, R
dc.date.accessioned	2008-07-28T04:49:20Z
dc.date.available	2008-07-28T04:49:20Z
dc.date.issued	1996-01
dc.identifier.citation	Solar Physics, Vol. 163, No. 1, pp. 93 - 97	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/2895
dc.description.abstract	While 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.extent	465626 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996SoPh..163...93S	en
dc.subject	Chromospheric variability	en
dc.subject	K-line profile	en
dc.subject	Chromosphere	en
dc.subject	Ca II K	en
dc.subject	H - line	en
dc.title	CA II K Line Profile of the Truly Quiet Sun	en
dc.type	Article	en