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Earth, Planets and Space
Figure 6 | Earth, Planets and Space

Figure 6

From: High-latitude GPS phase scintillation and cycle slips during high-speed solar wind streams and interplanetary coronal mass ejections: a superposed epoch analysis

Figure 6

The cumulative PDFs in the ‘cusp’ for days -1 and 0. Probability of the phase scintillation occurrence for (a) slow and fast solar wind on days just before and after CIRs (n = 108) and (b) days just before and after ICMEs (Dst < -30 nT; n = 40). The overall probabilities for each case (solid lines) are bracketed by a pair of curves (broken lines) for data corresponding to low and high (below and above median) values of the mean solar wind velocity, V (dashed lines), magnetic field magnitude, |B| (dash-dot line), and standard deviation of IMF B Z component, σ Bz (dotted line).

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