Solar Storm

A solar storm, also known as a geomagnetic storm, refers to a temporary disturbance in the Earth’s magnetosphere caused by solar wind and solar energetic particles emitted by the Sun. These storms typically occur as a result of solar flares or coronal mass ejections (CMEs), which release large amounts of plasma and magnetic fields into space. When this charged particle influx interacts with the Earth’s magnetic field, it can lead to various phenomena, including increased auroras (Northern and Southern Lights), disruptions in satellite communications, navigation systems, and power grids. Solar storms can vary in intensity and duration, and understanding them is important for protecting technology and infrastructure on Earth.