Examples of EBs and QSEBs in dataset 2 which targeted active region AR 11778 near the limb. The SST field is rotated over −59 deg from solar (X,Y). The full-field overview at left was taken with the blue (λ = 3953.7 Å) wide-band (FWHM 10 Å) camera. The axis divisions are arcsec from the lower-left corner. The four regions of interest A–D are shown enlarged as Hα-wing and blue wide-band cutout pairs at right, with corresponding arcsec coordinates. Regions A and B are in quiet areas, regions C and D sample the active region. Ellerman features are visible as bright flames in the Hα wings, respectively as smaller and weaker QSEBs in A and B and as larger and brighter EBs in C and D. Their relative brightness enhancements can be judged from the darkness of the surrounding granulation because each cutout panel is independently greyscaled. They are invisible in the blue wide-band images at right, in contrast to facular striations which are visible in both diagnostics, although appearing darker in Hα from the greyscaling needed to accommodate the bright Ellerman flames.