Fig. 1From: Dependence of the high-latitude plasma irregularities on the auroral activity indices: a case study of 17 March 2015 geomagnetic stormVariations of the interplanetary and geomagnetic parameters during 15–20 March 2015 storm: the IMF Bz, Bx, and By components (Geocentric Solar Magnetospheric (GSM)), density, velocity, and dynamic pressure of the solar wind, and Sym-H index. Red line indicates the SSC timeBack to article page