“…An abundance of such echoes is a critical factor for producing reliable convection maps. It has been established that the rate of echo detection with the SuperDARN radars varies with radar location, time of day, season and solar cycle (e.g., Milan et al, 1997;Ruohoniemi and Greenwald, 1997;Koustov et al, 2004;Kane et al, 2012). It has been reported that solar illumination conditions (Bristow et al, 2011), interplanetary magnetic field (IMF) magnitude and orientation (Ballatore et al, 2000), occurrence of magnetic storms (Kumar et al, 2011), and substorms (Wild and Grocott, 2008) affect echo detection.…”