Research news on coronal mass ejection

A coronal mass ejection (CME) is a large-scale eruptive solar phenomenon in which magnetized plasma from the Sun’s corona is expelled into interplanetary space, typically associated with magnetic reconnection in active regions or filament eruptions. CMEs involve the release of up to ~10¹⁶ g of plasma embedded in coherent magnetic flux rope structures and can attain speeds from a few hundred to over 2,000 km/s. Propagating through the heliosphere, they drive interplanetary shocks, restructure the solar wind and heliospheric magnetic field, and, upon interacting with planetary magnetospheres, can induce strong geomagnetic disturbances.

NASA's PUNCH sharpens solar storm forecasting in first test

Using continuous imagery from NASA's PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, scientists predicted the near-Earth arrival of a solar eruption to within 30 minutes in an initial proof-of-concept test. ...

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