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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References
Allen, M. S., McAllister, H. C., and Jefferies, J. T.: 1978, High Resolution Atlas of the Solar Spectrum 2678–2931 A, Inst. Astron., U. Hawaii, Honolulu, Hawaii, 58 pp.
Avrett, E. H.: 1992, in R. F. Donnelly (ed.), Proc. of the Workshop on the Solar Electromagnetic Radiation Study for Solar Cycle 22, Space Environment Lab., NOAA ERL, Boulder, Colo., 20.
Donnelly, R. F.: 1991, J. Geomagnet. Geoelectr. 43, Suppl., 835.
Fredga, K.: 1971, Solar Phys. 21, 60.
Hall, L. A., and Anderson, G. P.: 1988, Ann. Geophys. 6, 531.
Heath, D. F. and Schlesinger, B. M.: 1986, J. Geophys. Res. 91, 8672.
Lemaire, P.: 1984, Adv. Space Res. 4, (8)29.
White, O. R. and Livingston, W. C.: 1981, Astrophys. J. 249, 798.
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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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DOI: https://doi.org/10.1007/BF01473185