Fig. 12From: Statistical analysis of geomagnetic field intensity differences between ASM and VFM instruments onboard Swarm constellationPower spectral density. Comparison between the PSD of the magnetic disturbance field (\(\Delta F\)) with characterizes the magnetic data corrected by the Sun-driven disturbance (0408 version) and the PDF of the VFM electronic unit temperature (\(T_{\mathrm{EU}}\)). Data here considered are recorded onboard Swarm B satellite from January 13, 2015, to June 29, 2015Back to article page