Fig. 19.
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Search for relations between radial velocities of Fe I lines of different strengths at 520 nm (Fig. 2) and photometric Strömgren indices in integrated sunlight, as computed over the small simulation area of the N59 model (for the actual Sun, divide the numerical values by a factor of ∼150−200). The rows show (from top down) the weak, medium, and strong lines.
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