Paper
7 July 2000 New approach to Rayleigh guide beacons
Michael Lloyd-Hart, Stuart M. Jefferies, E. Keith Hege, James Roger P. Angel
Author Affiliations +
Abstract
We present analysis and numerical simulations of a new method to sense atmospheric wavefront distortion in real time with Rayleigh beacons. Multiple range-gated images of a single pulse from the laser are used to determine each phase map, providing an advantage over other methods in that photon noise is substantially reduced for a given brightness of the beacon. A laser at about 350 nm projects collimated pulses of light adjacent to the telescope. Rayleigh-scattered light from each pulse is recorded through the full telescope aperture in a sequence of video frames, each a few microseconds long. Images are captured as the pulse approaches and passes through the height at which the camera is focused. Phase diversity is thus naturally introduced between the frames. An iterative algorithm is used to extract the pupil-plane phases from the recorded intensity distributions. We anticipate that such beacons are likely to be valuable in future advanced systems for adaptive optics on very large telescopes with multiple laser beacons and deformable mirrors that aim to provide a large corrected field of view by tomography of the atmospheric turbulence.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael Lloyd-Hart, Stuart M. Jefferies, E. Keith Hege, and James Roger P. Angel "New approach to Rayleigh guide beacons", Proc. SPIE 4007, Adaptive Optical Systems Technology, (7 July 2000); https://doi.org/10.1117/12.390334
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CITATIONS
Cited by 4 scholarly publications.
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KEYWORDS
Telescopes

Sensors

Pulsed laser operation

Wavefront sensors

Adaptive optics

Rayleigh guide stars

Wavefronts

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