Fig. 3
Synthetic NLTE spectral lines of oxygen (solid lines) compared with the observed solar spectrum (dots) from Kurucz et al. (1984). Left: forbidden line at 630.0 nm, Centre: infrared triplet at 777 nm, Right: infrared line at 845 nm. All synthetic spectral line profiles were computed using solar oxygen abundance of A(O) = 8.71.
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