Figure 6From: Pc5 geomagnetic fluctuations in response to solar wind excitation and their relationship with relativistic electron fluxes in the outer radiation belt The relativistic electron flux and the Pc5 power. (top) The relativistic electron flux (>600 keV) at geosynchronous orbit (magenta) and the geomagnetic power at TNB (black). (bottom) The cross-correlation of the E > 600 keV (solid) and E > 2 MeV (dashed) electron flux with the Pc5 power at TNB (black), AQU (red), and GOES 12 (green) during 2007 to 2008, together with the 95% confidence levels (dashed, gray lines).Back to article page