Comparing Estimates of the Mg II Index at Solar Minimum from 1961 through 1981 with the Observed Mg II Index from 1978 to Present

Astronomy and Astrophysics – Astronomy

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Scientific paper

Using a solar spectral irradiance model which estimates the spectrum in an 18 nm region around the Mg II h and k lines at 280 nm we have estimated the Mg II index. This model uses observed active region, quiet Sun, and sunspot spectra as well as center-to-limb variation results from the HRTS-9 rocket as empirical inputs. To determine the location of these features on a given day, the model uses Ca II K images. This paper presents preliminary estimates of the Mg II index during the 1961 to 1981 time period and compares these values to those determined from observations from 1978 to present.

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