Fig. 6From: Observing Earth’s magnetic environment with the GRACE-FO missionGF1 (top) or GF2 (bottom) conjunctions with Swarm B. Panel 1: Kp and Dst indices, panel 2: magnetic local time of conjunction, panel 3: intra-satellite distance, panel 4: quasi-dipole latitude of conjunction, and panels 5–7: difference between magnetic residuals of GF1 or GF2 and Swarm BBack to article page