Co-aligned HRI_Lyα image and SPICE integrated intensities showing the chromospheric/TR view of NOAA 12967 and the DH fine structure. The SPICE observations in the H-Lyβ, C III, N IV, O VI, and Ne VIII lines (ordered as function of temperature) are overplotted on the HRI_EUV image. The numbers in the top-left and middle panels mark the locations of the EUV bundles shown in Fig. 3 that have a clear counterpart in the HRI_Lyα image. The bundle marked by number 10 also has counterparts observed in the SPICE rasters.