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Fig. 3 | Earth, Planets and Space

Fig. 3

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

Fig. 3

The electron fluxes on Arase, indexes of geomagnetic activity, solar wind parameters on 10 May 2017–10 June 2017. Variations of electron fluxes on Arase with energy E = 60 keV (first panel), with energy E = 700 keV (second panel), with energy E = 1 MeV (third panel); SYM-H* index, AE-index; Bz-component of the IMF, solar wind velocity V, solar wind density N according to the OMNI database on 10 May–10 June 2017. The green line on variations of SYM-H* index is non-storm interval, red line is storm interval

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