Radial-velocity shifts for ordinary lines (Table A.1). The gray circles are lines from the nonmagnetic simulation at solar disk center; the dark squares are for the full solar disk. The red triangles are from the magnetic model at disk center; the purple stars are magnetic full disk. Small symbols denote specific spectral lines, large symbols their total average. Line depth denotes absorption in units of the local continuum; weak lines thus carry small numbers. Each line’s average wavelength and line width measure is obtained from fitting the synthetic profiles to a symmetric five-parameter Gaussian-type function. The modeled lines are not affected by either solar rotation or gravitational redshift.