Centroiding and extraction of tip/tilt information from nonlinear curvature wavefront sensor measurements

The nonlinear curvature wavefront sensor (nlCWFS) uses multiple (typically four) out-of-focus images to reconstruct the phase and amplitude of a propagating light beam. Because these images are located between the pupil and focal planes, they contain tip/tilt information. Rather than using a separate sensor to measure image locations, it would be beneficial to extract tip/tilt information directly and routinely as part of the reconstruction process. In the presence of atmospheric turbulence, recovering precise centroid offsets for each out-of-focus image becomes a dynamic process as image structure is altered by changing aberrations. We examine several tip/tilt extraction methods and compare their precision and accuracy using numerical simulations. With knowledge of the z-distance to each plane, we find that applying a best-fit linear model to multiple image centroid locations can offer fast and accurate tip/tilt (jitter) mode retrieval. We also develop a nonlinear tip/tilt extraction method that self-consistently uses the speckle field to compensate for jitter but find that algorithm latency precludes practical implementation. Simulations of closed-loop adaptive optics correction demonstrate that centroiding precisions may reach the diffraction limit despite using images with a finite region of interest that is purposefully defocused.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2025-01-16
DOI
https://doi.org/10.1117/1.jatis.11.1.019001
Primary Topic
Advanced Measurement and Metrology Techniques
Type
article
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article

Centroiding and extraction of tip/tilt information from nonlinear curvature wavefront sensor measurements

Stanimir Letchev, Justin R. Crepp, Connor Smith, Caleb G. Abbott
Journal of Astronomical Telescopes Instruments and Systems
Advanced Measurement and Metrology Techniques
article

Centroiding and extraction of tip/tilt information from nonlinear curvature wavefront sensor measurements

Stanimir Letchev, Justin R. Crepp, Connor Smith, Caleb G. Abbott
article en

Abstract

The nonlinear curvature wavefront sensor (nlCWFS) uses multiple (typically four) out-of-focus images to reconstruct the phase and amplitude of a propagating light beam. Because these images are located between the pupil and focal planes, they contain tip/tilt information. Rather than using a separate sensor to measure image locations, it would be beneficial to extract tip/tilt information directly and routinely as part of the reconstruction process. In the presence of atmospheric turbulence, recovering precise centroid offsets for each out-of-focus image becomes a dynamic process as image structure is altered by changing aberrations. We examine several tip/tilt extraction methods and compare their precision and accuracy using numerical simulations. With knowledge of the z-distance to each plane, we find that applying a best-fit linear model to multiple image centroid locations can offer fast and accurate tip/tilt (jitter) mode retrieval. We also develop a nonlinear tip/tilt extraction method that self-consistently uses the speckle field to compensate for jitter but find that algorithm latency precludes practical implementation. Simulations of closed-loop adaptive optics correction demonstrate that centroiding precisions may reach the diffraction limit despite using images with a finite region of interest that is purposefully defocused.

Journal of Astronomical Telescopes Instruments and SystemsVol. 11(01)
University of Notre Dame (US), Max Planck Institute for Astronomy (DE)
Openalex Percentile: Top 99%
Advanced Measurement and Metrology Techniques
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