@Xray Yes, exactly! Adaptive optics is used to compensate for star twinkle (scintillation) caused by atmospheric turbulence. It corrects light in real time using wavefront sensors and deformable mirrors, resulting in sharper and clearer images. This system is especially useful in large ground-based telescopes, allowing them to achieve resolutions comparable to space telescopes. For example, the Very Large Telescope (VLT) at the European Southern Observatory (ESO), the Keck Telescopes in Hawaii, and the Magellan Telescopes in the U.S. utilize advanced adaptive optics systems for high-resolution observations.
Also, receiving such a comment from the founder of the program is truly an honor for me. Knowing that my work on adaptive optics has been examined in such detail further boosts my motivation. Thank you!