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Shack–Hartmann wavefront sensor
Type of optical instrument
Type of optical instrument


A Shack–Hartmann (or Hartmann–Shack) wavefront sensor (SHWFS) is an optical instrument used for characterizing an imaging system. It is a wavefront sensor commonly used in adaptive optics systems. It consists of an array of lenses (called lenslets) of the same focal length. Each is focused onto a photon sensor (typically a CCD array or CMOS array
The design of this sensor improves upon an array of holes in a mask that had been developed in 1904 by Johannes Franz Hartmann as a means of tracing individual rays of light through the optical system of a large telescope, thereby testing the quality of the image. |editor1-first=F. Dow |editor1-last=Smith
Shack–Hartmann sensors are used in astronomy to measure telescopes and in medicine to characterize eyes for corneal treatment of complex refractive errors. |name-list-style=amp | volume = 17 | hdl-access = free |name-list-style=amp | publisher = Springer Recently, Pamplona et al. |url-status = dead |hdl-access= free
References
References
- (August 2019). "Accounting for focal shift in the Shack–Hartmann wavefront sensor". Optics Letters.
- (August 2019). "Centroid error due to non-uniform lenslet illumination in the Shack–Hartmann wavefront sensor". Optics Letters.
- Scheiner, "Oculus, sive fundamentum opticum", Innsbruck 1619
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