Still from an animation of the inversion results for the time series of the quiet Sun. Leftmost panel: 2D maps of the H-index for eight repetitions scanning the same area of 2′′ × 61′′. Time increases left to right. The scan step of the spectra shown in the other panels is always located at the very left border at 0′′. Second and third panels: observed and best-fit Ca spectra. Fourth panel: temperature stratifications along the slit corresponding to the best-fit spectra. Fifth panel: co-spatial and simultaneous Stokes V spectra at 630 nm. Sixth panel: 2D maps of the polarity of the Stokes V signal for eight repetitions scanning the same area. Seventh panel: 2D maps of the LOS velocity of the Fe i line at 630.15 nm for eight repetitions of scanning the same area.