Page 2: 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.

Scientists use AI to interpret the sun's acoustic heartbeat

A new AI-based approach that can "hear" inside the sun could give vital signs of the solar disturbances that have significant effects in near-Earth space and on human activities. The solar cycle is an approximate 11-year ...

ESA's Proba 3 is unlocking secrets of the solar wind

It has been a dream of astronomers and solar scientists for ages. A new mission gives solar researchers a powerful new tool in their arsenal: on-demand, total solar eclipses. Launched in 2024, The European Space Agency's ...

NASA probe data suggests a more complex sun's magnetic engine

A Southwest Research Institute-led study found that protons and heavy ions react differently to solar magnetic reconnection events, revealing a more complex magnetic engine powering the solar wind. Magnetic reconnection converts ...

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