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Figure 3 | Earth, Planets and Space

Figure 3

From: Pc5 geomagnetic fluctuations in response to solar wind excitation and their relationship with relativistic electron fluxes in the outer radiation belt

Figure 3

The correlation between the IMF and SW parameters and the geomagnetic field fluctuation power. The cross-correlation, through the years 2006 to 2010, of the SW speed (cyan), IMF strength (magenta), and SW dynamic pressure (blue) fluctuation power with the Pc5 power at TNB (top panels), AQU (middle panels), and GOES 12 (bottom panels), together with the 95% confidence levels (dashed, gray lines). In each panel, the horizontal axis indicates the lag in hours.

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