Full field-of-view comparison between physical quantities in the chromosphere as determined from the NLTE inversion (left) and the original 3D snapshot (right). From top to bottom: temperature, line-of-sight velocity, B_z, |B_x| and |B_y|. The line profiles were degraded with an instrumental profile of FWHM = 50 mÅ before carrying out the inversion. In the velocity panel, upflows have positive sign.