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Fig. 4 | Earth, Planets and Space

Fig. 4

From: Relativistic electron flux growth during storm and non-storm periods as observed by ARASE and GOES satellites

Fig. 4

The electron fluxes on GOES-13, solar wind parameters, indexes of geomagnetic activity on 1–30 September 2017. The variations of GOES-13 electron fluxes with energy E > 2 MeV (first panel), with energy E = 475 keV (second panel), with energy E = 40 keV (third panel); SYM-H index, AE-index; OMNI solar wind velocity V, OMNI solar wind density N; ULF power index, VLF power intensity (0.7–4.54 kHz) according to Arase satellite on 1–30 September 2017. The green line on variations of SYM-H index is non-storm interval, red line is storm interval

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