How is the suns magnetic behavior associated with its activity cycle?

The Sun's magnetic behavior is closely linked to its 11-year solar activity cycle, characterized by fluctuations in sunspot numbers, solar flares, and coronal mass ejections. During periods of high solar activity, the Sun's magnetic field becomes more complex and intense, leading to increased sunspots and eruptions. Conversely, during solar minimum, the magnetic field is more stable and sunspots are fewer. This cycle is driven by the dynamo effect in the Sun's interior, where the movement of electrically conductive plasma generates and sustains its magnetic field.