Solar storms could be forecast by monitoring cosmic rays
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Using incidental data collected by the BepiColombo mission, an international research team has made the first detailed measurements of how coronal mass ejections (CMEs) reduce cosmic-ray intensity at varying distances from the Sun. Led by Gaku Kinoshita at the University of Tokyo, the team hopes that their approach could help improve the accuracy of space weather forecasts following CMEs.
CMEs are dramatic bursts of plasma originating from the Sun's outer atmosphere. In particularly violent events, this plasma can travel through interplanetary space, sometimes interacting with Earth's magnetic field to produce powerful geomagnetic storms.



