Solar Rotation

Solar rotation refers to the rotation of the Sun around its own axis. Unlike a solid object, the Sun is a massive ball of hot plasma, so different parts rotate at different speeds. The equator takes about 25 days to complete one rotation, while the poles take about 35 days. This differential rotation affects solar phenomena like sunspots, solar flares, and the solar magnetic field. Understanding solar rotation is crucial for studying solar dynamics and its impact on space weather, which can influence satellite operations and communications on Earth.