Stellar flares are sudden and intense bursts of increased electromagnetic radiation from the surface of a star, typically associated with magnetic disturbances. These events can occur on any type of star, but are most commonly observed on young and active stars with strong magnetic fields. Stellar flares can release significant amounts of energy in a short period of time, causing rapid increases in brightness across multiple wavelengths, from X-rays to radio waves. They can also produce high-energy particles and eject material into space. Research on stellar flares aims to better understand the physical processes behind these events, including the role of magnetic fields, plasma dynamics, and the impact on the star's atmosphere and surrounding environment. Studying stellar flares can provide insights into the fundamental properties of stars, their magnetic activity cycles, and the potential influences on planetary systems. This research also has implications for understanding the habitability of exoplanets around active stars.