Paper
17 October 1997 Correcting for amplitude effects in laser beam propagation through the turbulent atmosphere using a two-deformable-mirror technique
Michael C. Roggemann, David J. Lee
Author Affiliations +
Abstract
A two deformable mirror concept for correcting amplitude effects in laser beam projection through the turbulent atmosphere is presented. This system uses a deformable mirror and a Fourier transforming mirror to adjust the amplitude of the wave front in the telescope pupil. A second deformable mirror is used to correct the phase of the wave front before it leaves the aperture. The phase applied to the deformable mirror used for controlling the beam amplitude is obtained using a technique based on the Fienup phase retrieval algorithm. One dimensional simulation results are presented which indicate that the average on-axis energy is improved by 15% or more on average, and the 90% encircled energy radius can be reduced by up to 30% on average.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael C. Roggemann and David J. Lee "Correcting for amplitude effects in laser beam propagation through the turbulent atmosphere using a two-deformable-mirror technique", Proc. SPIE 3126, Adaptive Optics and Applications, (17 October 1997); https://doi.org/10.1117/12.279041
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KEYWORDS
Deformable mirrors

Atmospheric propagation

Phase retrieval

Wavefronts

Scintillation

Mirrors

Wave propagation

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