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Geomagnetic storms occur when solar activity disturbs Earth’s magnetosphere. Key causes include:
- Coronal Mass Ejections (CMEs): Massive bursts of solar plasma and magnetic field released into space.
- High-Speed solar wind streams (HSS): Faster-than-normal streams of solar wind from coronal holes.
- Solar flares: Sudden flashes of brightness often associated with CMEs.
When these reach Earth, they inject energy into the magnetosphere, leading to geomagnetic storms.
The sun's magnetic field undergoes a periodic reversal, flipping its polarity in an approximately 11-year cycle. This process is associated with various solar phenomena, such as sunspots, flares, and coronal mass ejections (CME) ↗.
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