Figure 2From: Stochastic forecasting of the geomagnetic field from the COV-OBS.x1 geomagnetic field model, and candidate models for IGRF-12Prediction errors (nT) as function of geomagnetic latitude for intensity (F) and vector (B b ,B ⊥,B 3) data. Oersted (black), CHAMP (red), Sac-C (yellow), and Swarm (cyan) observations.Back to article page