Figure 10From: High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysisThe cumulative PDFs for MC and non-MC ICMEs. Probability of the phase scintillation occurrence in the ‘nightside auroral zone’ (top panels) and in the ‘cusp’ (bottom panels) for (a, c) non-MC (n = 13) and (b, d) MC (n = 27) events.Back to article page