Fig. 9From: A statistical analysis of Pc1–2 waves at a near-cusp station in AntarcticaULF dependence on AE and solar wind density. The UT distribution of the events for disturbed geomagnetic conditions (black line) and high SW densities (red line). The vertical lines at approximately 08 UT and 20 UT indicate the magnetic midnight and noon, respectivelyBack to article page