Current sheets are thin, elongated structures in plasma that contain intense currents and magnetic fields. They are commonly observed in plasma physics environments, such as in the Earth's magnetosphere, solar wind, and laboratory experiments. Current sheets play a crucial role in the dynamics of plasma systems, as they can generate instabilities, drive magnetic reconnection, and contribute to the overall energy transport in the system. Understanding the formation and behavior of current sheets is essential for studying a wide range of phenomena in space and laboratory plasmas.