Sunspots are dark, cooler areas on the sun's surface caused by magnetic activity, appearing in groups and indicating magnetic field fluctuations. Solar flares are intense bursts of radiation that occur near sunspots, releasing energy and particles into space. Prominences are large, loop-like structures of plasma that extend from the sun's surface, often associated with solar flares and sunspots, and can last for days to weeks. Each type of solar activity has distinct characteristics in terms of appearance, duration, and associated magnetic phenomena.
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