Fe i 5434 Å profiles for the atmospheres from numerical simulations by Asplund et al. (2000). The solid line and rhombs: from granule (GR) with infinite spectral resolution and after convolving with FPI spectrometer curve and Hamming smoothing, respectively; dashed and asterisks: the same for intergranular (IGR) area; crosses: average observed profile scaled to the average of the calculated intensities in the wings.