Fig. 6From: Solar events and solar wind conditions associated with intense geomagnetic stormsScatter plots of |min. Dst| and solar wind parameters: Bp, Bsp, Vp, Eyp, Eyi, and integration time of Ey. Solid line shows the LS fittings of |min. Dst| vs. Bsp, |min. Dst| vs. Eyp, and |min. Dst| vs. Eyi, respectivelyBack to article page