Fig. 9From: Statistical analysis of geomagnetic field intensity differences between ASM and VFM instruments onboard Swarm constellationVariance. Comparison between the variance associated with each IMF k obtained decomposing \(\Delta F_{\mathrm{P}}\) and \(\Delta F_{\mathrm{C}}\) plotted as a function of the associated mean frequency \(< f_k>\) for all the three Swarm satellitesBack to article page