Figure 4From: Pc5 geomagnetic fluctuations in response to solar wind excitation and their relationship with relativistic electron fluxes in the outer radiation belt The SW and geomagnetic time series during March to May 2006. (top panel) The SW speed. (bottom panel) The Pc5 power at TNB (black) and AQU (red) of the IMF strength (magenta) and SW dynamic pressure (blue). The time series have been converted to zero mean and unitary variance. The most relevant SW speed peaks are indicated by vertical dashed lines.Back to article page