2021
DOI: 10.15372/aoo20210710
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Numerical simulation of dynamical adaptive phase correction of turbulent radiation distortions and estimation of their temporal characteristics with the help of Shack-Hartmann wavefront sensor

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Cited by 3 publications
(4 citation statements)
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“…When creating, adjusting, and testing adaptive optical systems used in astronomy and vision systems in a turbulent atmosphere [2][3][4][5][6][7][8], the problem of estimating the effect of noise on measurements obtained on the stand of a tracking adaptive optical system becomes relevant [9,10].…”
Section: Introductionmentioning
confidence: 99%
“…When creating, adjusting, and testing adaptive optical systems used in astronomy and vision systems in a turbulent atmosphere [2][3][4][5][6][7][8], the problem of estimating the effect of noise on measurements obtained on the stand of a tracking adaptive optical system becomes relevant [9,10].…”
Section: Introductionmentioning
confidence: 99%
“…Numerical studies on the efficiency of phase correction of turbulent distortions of a laser beam depending on the speed of adaptive systems [11], with using of corrector to compensate for rapidly changing small-scale aberrations of laser beams [12] or of monomorphic mirror simulation [13] should also be carried out taking into account the repeatability of atmospheric parameters.…”
Section: Introductionmentioning
confidence: 99%
“…The beam formed by the system passes over the electric heating element (11), which forms its turbulent distortions, and enters the beam-splitting cube (19), where it branches and one branch enters the stand output through the scaling optics (20), from where it is directed to the input of the tuned (tested) optical systems. The other branch of the received beam passes through a light filter (33), a lens (34) and forms an image on the video camera of the stand (35).…”
Section: Introductionmentioning
confidence: 99%
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