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Fig. 3 | Earth, Planets and Space

Fig. 3

From: On some features characterizing the plasmasphere–magnetosphere–ionosphere system during the geomagnetic storm of 27 May 2017

Fig. 3

Solar wind parameters between 25 May and 2 June 2017 observed by WIND (at first Lagrangian point), in UT: a proton density, b proton velocity, c proton temperature, d pressure, e IMF intensity, fh IMF x, y, z components in the GSE coordinate system. The vertical black dashed line indicates the arrival of the interplanetary shock, on 27 May 2017 at 14:41 UT. The green area beyond is the ICME sheath, while the red area corresponds to the magnetic cloud (ejecta interval)

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