AST-143intermediate

Solar Flares & Coronal Mass Ejections: Physical Mechanisms

Solar flares and coronal mass ejections are major releases of energy from magnetically active regions on the Sun. Monitoring flares and CMEs helps forecast radiation hazards, satellite anomalies, radio disruptions, auroral activity, and geomagnetic storms.

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intermediate45 minFact checked

Solar Flares & Coronal Mass Ejections: Physical Mechanisms

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AST-142Solar Flares & Coronal Mass Ejections: Structures & Vocabulary→

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AST-144Solar Flares & Coronal Mass Ejections: Observation, Measurement & Evidence→

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Solar flares and coronal mass ejections are major releases of energy from magnetically active regions on the Sun.

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Solar plasma drags and twists magnetic fields as differential rotation and convective motions stress active regions.

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