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Fig. 1 | Earth, Planets and Space

Fig. 1

From: The problem of the acceleration of electrons of the outer radiation belt and magnetospheric substorms

Fig. 1

Solar wind parameters and geomagnetic indexes for the geomagnetic storm on 8–9 October 2012. From top to bottom: the solar wind velocity, number density, dynamic pressure, and three components of the interplanetary magnetic field (a), the Dst (blue curve) and Dst* (red curve) corrected by dynamic pressure Dst indexes (b); from top to bottom: the Dst (blue curve) and SYM-H (red curve), AL (red curve), AU (blue curve), and PC (PC north—blue curve, Pc south—red curve) indexes (c)

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