CA II K Line Profile of the Truly Quiet Sun

Details CA II K Line Profile of the Truly Quiet Sun CA II K Line Profile of the Truly Quiet Sun

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..163...93s&link_type=abstract

Solar Physics, Volume 163, Issue 1, pp.93-97

Physics

2

Scientific paper

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.

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