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Solar minimum

 Home Physics Concepts in physics Physical phenomena Stellar phenomena Solar phenomena
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Solar minimum refers to a period of lowest solar activity in the approximately 11-year solar cycle, during which the Sun's output of solar radiation and solar phenomena, such as sunspots, solar flares, and coronal mass ejections, are at their lowest levels. During these times, the Sun exhibits fewer sunspots, which are dark regions on its surface associated with magnetic activity.

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