Fig. 9From: Predictions of the geomagnetic secular variation based on the ensemble sequential assimilation of geomagnetic field models by dynamo simulationsSame as Fig. 4, but for predictions of the axial dipole \(g_1^0\) and \(h_5^3\) coefficients and their SV after the assimilation of COV-OBS and Kalmag until the year 2020. The green star now shows the IGRF-13Back to article page