Fig. 3From: Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observationsTime variation of the SUSANOO-estimated (the background) and observed (symbols) IPS g values on September 9, 2017. Simulations (columns from the left): RUN1, RUN2, RUN3 and RUN4. Time (rows from the top: 0:00 UT, 1:00 UT, 2:00 UT and 3:00 UT)Back to article page