Adaptive optics systems use a combination of wavefront sensors and deformable mirrors to relay information to a computer for adjusting a telescope's mirror. The wavefront sensors detect distortions in the incoming light caused by atmospheric turbulence, while the computer processes this data to calculate the necessary adjustments. The deformable mirror then changes its shape in real-time to correct these distortions, resulting in clearer images. This technology enhances the resolution of telescopes, allowing for more detailed observations of celestial objects.
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