Radial velocities showing lack of correlation with several plausibly anticipated fluctuations in various line parameters. No correlations were found here, except a hint of a line depth dependence in the strongest lines. The measures for line depth, width, and shape are normalized to 100% for the averages over the simulation sequence. The calculations are for integrated sunlight from the small simulation area of the N59 model (for the actual Sun, divide the lineshift values by a factor of ∼150−200).