Fig. 1
Six example events: numbers (a) 13, (b) 3, (c) 4, (d) 15, (e) 21, and (f) 20. Panels a–c and d–f: pertain toevents with clear/unclear presence of solar wind ions from April and May 2015, respectively.Subpanels:(1) magnetic field components in cometocentric solar equatorial (CSEQ) coordinates, (2)Blow in black and B0in blue, and (3) ΔB∕B0in black and relative change in LAP current ΔI∕I0in red.
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