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The solar Ca II K index and the Mg II core-to-wing ratio

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Abstract

The 1 Å index of the solar Ca II K line is compared with the core-to-wing ratio of satellite measurements of the Mg II h and k lines. The correlation coefficient r = 0.976 for the Nimbus-7 Mg II ratio during solar cycle 21 andr = 0.99 for the NOAA9 Mg II ratio in cycle 22. Linear regression analysis for the full dynamic range of both data sets is used to combine the Nimbus-7 and NOAA9 Mg II data. These relations permit the ground-based Ca K index to estimate the solar UV flux.

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Donnelly, R.F., White, O.R. & Livingston, W.C. The solar Ca II K index and the Mg II core-to-wing ratio. Sol Phys 152, 69–76 (1994). https://doi.org/10.1007/BF01473185

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