Fig. 2.
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Examples of selected lines. Shown here are Fe I lines around λ525 nm from the N59 model. Top: synthetic spectra at solar disk center, μ = 1; bottom: μ = 0.41. The clean lines selected for detailed analysis are shown in red: strong, medium, and weak labeled A, B, and C, respectively. The lines become noticeably broader toward the limb.
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