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Simulation of Full Field Correction with Two Deformable Mirror Adaptive Optics

Li You

Open publisher page 1 citations

Abstract

WT5”BZ]One key step for full field correction is to match the main laser amplitude distribution with beacon amplitude distribution on deformable mirror 2 in two deformable mirror adaptive optics. Amplitude and phase corrections for turbulence are studied based on Y G wavefront retrieval algorithms. The results show that full field corrections can improve Strehl ratio by a factor of 1.27 to 2.50 compared with phase only correction. For a distance of 10m between deformable mirror 1 and deformable mirror 2, the factor is from 1.13 to 1.50. [WT5”HZ]

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What this paper is about

WT5”BZ]One key step for full field correction is to match the main laser amplitude distribution with beacon amplitude distribution on deformable mirror 2 in two deformable mirror adaptive optics. Amplitude and phase corrections for turbulence are studied based on Y G wavefront retrieval algorithms. The results show that full field corrections can improve Strehl ratio by a factor of 1.27 to 2.50 compared with phase only correction. For a distance of 10m between deformable mirror 1 and deformable mirror 2, the factor is from 1.13 to 1.50. [WT5”HZ]

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Available abstract

WT5”BZ]One key step for full field correction is to match the main laser amplitude distribution with beacon amplitude distribution on deformable mirror 2 in two deformable mirror adaptive optics. Amplitude and phase corrections for turbulence are studied based on Y G wavefront retrieval algorithms. The results show that full field corrections can improve Strehl ratio by a factor of 1.27 to 2.50 compared with phase only correction. For a distance of 10m between deformable mirror 1 and deformable mirror 2, the factor is from 1.13 to 1.50. [WT5”HZ]

Key concepts: Strehl ratio, Deformable mirror, Adaptive optics, Wavefront, Physics, Optics, Amplitude, Phase (matter)

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