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.

Astronomers uncover why some solar eruptions die

A team of scientists has recorded one of the most detailed views ever of a failed solar eruption, a powerful blast from the sun that never broke free. Their work is published in the journal Nature Astronomy.

NASA missions track record-breaking radio burst from sun

When NASA scientists first observed a particular radio burst from the sun in August 2025, there was nothing unusual about it. But then the radio burst kept going. Typically, solar radio bursts like these last a few hours ...

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