Real-time solar flare monitoring and X-ray flux data
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Solar flares are sudden bursts of radiation from the Sun's surface, classified by their X-ray brightness. Large flares can trigger geomagnetic storms and enhance aurora activity.
M-class and X-class flares can produce coronal mass ejections (CMEs) that reach Earth 1-3 days later, potentially triggering strong geomagnetic storms and spectacular aurora displays. However, not all flares produce CMEs, and CME direction matters—they must be Earth-directed to affect our planet.
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