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Fig. 1 | Earth, Planets and Space

Fig. 1

From: Relationship between large-scale ionospheric field-aligned currents and electron/ion precipitations: DMSP observations

Fig. 1

(Top panel) The variation of solar flux, F10.7 (gray) and P10.7 (black), from 2009 to the end of 2016. (middle panel) The altitude evolutions of DMSP F-16 (black), F-17 (blue), F-18 (red), and Swarm A (green). (bottom panel) The local time evolutions of the four satellites, separately for ascneding (thick-solid) and descending (thin-dotted) nodes. The light-orange shaded area represents the period of available particle energy flux data from DMSP

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