Fig. 3.From: Simultaneous observation of the electron acceleration and ion deceleration over lunar magnetic anomaliesElectrons and ions over magnetic anomalies observed at ~25 km altitude. Format is the same as Fig. 1. The propagation time of the solar wind IMF measured by ACE shown in Panel (i) is 43 minutes. Magnetically reflected solar wind ions were observed by IMA when Kaguya flew over magnetic anomalies during the time period indicated by a blue box.Back to article page