Disk winds are powerful outflows of gas and dust that are observed in the vicinity of accretion disks around young stellar objects or active galactic nuclei. These winds are believed to play a crucial role in the evolution of these systems by removing excess angular momentum and material from the disk. Disk winds are thought to be driven by a combination of thermal pressure, magnetic fields, and radiation pressure, and they can have a significant impact on the surrounding environment by shaping the distribution of material and influencing the growth of the central object. Studying disk winds can provide valuable insights into the processes of star formation and black hole accretion.