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Fig. 1


Magnetogram (upper panel) and Ca II K images (middle panel and lower panel) taken by SST/CHROMIS of the quiet Sun near the disk center (μ = 1.0). Upper panel: vertical magnetic field obtained from Milne–Eddington inversion with Fe I taken by SST/CRISP is shown. The color bar range is [ − 300, 300 G]. Middle panel: red wing position at Δ λ = +1409 mÅ is indicated. Lower panel: line center position at Δ λ = 0 mÅ is indicated. The white square outlines the region that we compare with our simulations (see Fig. 13).

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