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Solar storms are powerful bursts of energy released from the Sun, often caused by solar flares or coronal mass ejections (CMEs). When these charged particles reach Earth, they interact with the magnetosphere, the protective magnetic field surrounding our planet.
The magnetosphere is a large, invisible shield created by Earth’s magnetic field. It deflects most of the solar wind, preventing harmful radiation from reaching the surface.
When a CME hits Earth, the magnetosphere compresses on the dayside and stretches on the nightside. This disturbance can trigger:
Strong solar storms can affect satellites, aviation, and communication systems. Monitoring agencies like NOAA and ESA track solar activity to provide early warnings.
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