Quiet-Sun FOV observed by the SST on 6 June 2019. (a) CHROMIS WB image, (b) Hβ line core image, (c) LOS magnetic field (saturated at ±300 G) retrieved from ME inversions of the Fe I 6173 Å line observed with CRISP. The FOV for CRISP is smaller than that of CHROMIS, so that there is no overlap for 8 Mm at the left. (d) RP index map obtained from the k-means clustering algorithm applied to the Hβ line profiles showing all 100 RPs in shades of gray. The arrow in panel b shows the direction toward the nearest limb. An animation of this figure is available online.