
A technique that adjusts optical components in real time to improve image or signal quality.Adaptive optics is a technology that corrects distortions in optical systems in real time, allowing images or signals to be captured with clarity that would otherwise be impossible. It is most famously used in ground-based astronomy to counteract the blurring effect of Earth's atmosphere, but it also plays a role in medical imaging, laser communications, and even vision correction. The core idea is to measure how light is being disturbed and then apply a compensating adjustment before the light is recorded.
The concept was first proposed by Horace Babcock in 1953, but practical systems were only developed decades later, initially for military applications and then for astronomy in the 1990s.
The system typically uses a wavefront sensor to measure the distortion of incoming light, a deformable mirror or other adjustable optical element to apply corrections, and a control loop that updates the corrections many times per second. When light enters the system, the sensor detects how its wavefront deviates from an ideal shape, and the mirror is deformed to flatten that wavefront, effectively canceling out the distortion. In biological applications, such as imaging deep into tissue, the same principle is used to correct for scattering and aberrations caused by the sample itself.
Adaptive optics is used in large telescopes to produce sharper images of celestial objects, in retinal imaging to see individual photoreceptor cells in the eye, and in laser communication systems to maintain signal quality over long atmospheric paths.
The deformable mirrors used in adaptive optics can change their shape thousands of times per second, with surface adjustments as small as a few nanometers.




















