Final data products (from left to right: continuum intensity, I_c, magnetic field strength, B, magnetic field inclination, γ, magnetic field azimuth, ϕ and LOS velocity, v_LOS) after on-board data analysis. The inversion code used is a software version of the one to be used in flight. Upper row: simulated high resolution channel data results. The original data come from the Swedish 1 m Solar Telescope (Scharmer et al. 2003) in the Observatorio de La Palma (Canary Islands) in 2012. Lower row: simulated full disc data results. The original images have been taken with the Helioseismic Magnetic Imager (HMI; see Scherrer et al. 2012) on the Solar Dynamics Observatory (SDO) with a resolution of 1 arcsec (December 2, 2011).