Adaptive Optics
Adaptive optics (AO) is a technology used to improve the performance of optical systems by reducing the effect of wavefront distortions. It is used in astronomical telescopes and laser communication systems to remove the effects of atmospheric distortion, in microscopy, optical fabrication and in retinal imaging systems to reduce optical aberrations. Adaptive optics works by measuring the distortions in a wavefront and compensating for them with a device that corrects those errors such as a deformable mirror or a liquid crystal array. AO was first envisioned by Horace W. Babcock in 1953, and was also considered in Science Fiction, as in Poul Anderson's novel Tau Zero (1970), but it did not come into common usage until advances in computer technology during the 1990s made the technique practical.
Adaptive optics should not be confused with active optics, which works on a longer timescale to correct the primary mirror geometry.
Other methods can achieve resolving power exceeding the limit imposed by atmospheric seeing, such as speckle imaging, aperture synthesis, lucky imaging, and space telescopes, such as the Hubble Space Telescope.
Read more about Adaptive Optics: Tip–tilt Correction, In Retinal Imaging, Other Uses, Beam Stabilization
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