The Solar Cycle is an approximately 11-year cycle during which the Sun's magnetic activity fluctuates, leading to variations in solar phenomena such as sunspots, solar flares, and coronal mass ejections. This cycle significantly impacts space weather and can influence satellite operations and communications on Earth. During periods of high solar activity, known as solar maximum, the Sun exhibits an increase in sunspots and solar storms. Conversely, during solar minimum, these activities decrease. Understanding the Solar Cycle is crucial for predicting space weather and its effects on technology and the Earth's atmosphere.