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The solar cycle is an approximately 11-year period of fluctuations in the Sun's activity, most notably in the number and size of sunspots and solar prominences. This cycle is driven by changes in the Sun's magnetic fields.123

The period of highest solar activity within this cycle is known as the solar maximum. During solar maximum, phenomena like coronal mass ejections (CMEs) occur more frequently and intensely. These CMEs are large eruptions of plasma from the Sun's corona that can impact Earth, causing space weather events such as geomagnetic storms. The solar cycle also influences the Sun's magnetic polarities, which reverse approximately every 11 years, leading to a full magnetic cycle of 22 years.341

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