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CA II K Line Profile of the Truly Quiet Sun

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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

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