Fig. 3From: Relativistic electron flux growth during storm and non-storm periods as observed by ARASE and GOES satellitesThe 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 intervalBack to article page