Lines in special positions display special behavior. The weak Fe I 393.2627 and Fe I 396.7421 lines are superposed onto the extended absorption wings of the Ca II H & K lines and get their formation heights lifted through combining their opacities with those of the H&K line wings. The leftmost column shows their appearance in solar spectrum atlases (Kitt Peak full-disk, Jungfraujoch disk center). With vertical bisectors, the line cores are remarkably symmetric in both the nonmagnetic (center) and magnetic 240 mT = 2400 G case (right).