MOMFBD-restored broadband image (top) at about λ600 nm of micro-pores (white square in the center in both images) in an EFR observed with the GFPI at 08:07 UT on 2008 August 7. Hα line-core intensity image corresponding to the broadband image (bottom). The white rectangle on the left outlines the region used for computing the average Hα quiet-Sun spectral profile. Crosses “✛” and alphabetic labels mark the locations of six contrast profiles plotted in Fig. 5. The black contours indicate the position of the micro-pores.