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Fig. 15 | Earth, Planets and Space

Fig. 15

From: Statistical analysis of geomagnetic field intensity differences between ASM and VFM instruments onboard Swarm constellation

Fig. 15

Comparison between \(T_{\mathrm{EU}}\) and \(\Delta F\) signals. From top to bottom Comparison between \(T_{\mathrm{EU}}\) (red line) and \(\Delta F\) (blue line) signals during a day in which the local time of the ascending node of Swarm B is about 12 (Swarm B orbits in the noon–midnight sector) and 18 (Swarm B orbits in the dawn–dusk sector), respectively

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