Fig. 12From: Nighttime Pc3 pulsations: MM100 and MAGDAS observationsYearly averaged diurnal variation of Pc3 occurrence rate P for stations at \(L\approx 2\) (top panel), \(1.45<L<1.83\) (middle panel), and \(L\approx 1\) (bottom panel). H/D components are shown with solid/dashed lines. Colors correspond to different geomagnetic longitudesBack to article page