Fig. 6
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Very strong lines at solar disk center. Left: Mg I b2 and Na I D2 lines in the Jungfraujoch atlas. Center: synthetic profiles and bisectors for their line cores (corresponding to the boxes at left), and also the related Mg I b1 and Na I D1 lines for the nonmagnetic simulation. Right: 240 mT = 2400 G magnetic case. The effects of solar rotation and gravitational redshift are not included.
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