Solar Magnetism

Solar magnetism arises from the movement of charged particles within the Sun's interior, creating complex magnetic fields through a process called the solar dynamo. These magnetic fields influence the solar surface, leading to phenomena such as sunspots, solar flares, and prominences. Sunspots are dark, cooler areas with intense magnetic activity, while solar flares are sudden energy releases caused by magnetic reconnection. Overall, solar magnetism shapes the Sun’s behavior and impacts space weather, which can affect satellite communications, power grids, and even Earth's climate.