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Fig. 1 | Earth, Planets and Space

Fig. 1

From: Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations

Fig. 1

Example distribution of the simulated IPS data. IPS g-value estimated by the SUSANOO projected onto the sky-plane. White circles and red lines indicate elongation and position angle range of the radio source used for the forecasting, respectively. The symbols indicate the IPS g-value observed by SWIFT from 01:00 UT to 02:00 UT. Crosses indicate all observed radio sources and diamonds indicate radio sources with the following g-values: 2.0 < g (red), 1.5 < g < 2.0 (green), and 1.2 < g < 1.5 (blue)

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