Fig. 3.From: An algorithm for deriving core magnetic field models from the Swarm data setDifferences from known misalignment angles as a function of time for each 30 day window after removal of outliers and underpopulated segments. Data gaps are interpolated. The γ angle, in particular on satellite C (highest orbit) shows largest differences. The horizontal dashed lines at 3 arcsecs are the Swarm threshold requirement standard deviation.Back to article page