Geomagnetic Storms

Geomagnetic storms are disturbances in Earth’s magnetosphere caused by changes in the solar wind, particularly during solar activity such as coronal mass ejections (CMEs) or solar flares. These storms occur when charged particles from the sun interact with Earth’s magnetic field, leading to variations in the magnetic environment. The intensity and effects of geomagnetic storms can vary, impacting technologies such as satellite operations, communication systems, and power grids. They can also produce spectacular natural displays such as auroras near the polar regions. Monitoring geomagnetic storms is crucial for understanding space weather and mitigating potential impacts on human activities and infrastructure.