Demonstration of a photonic lantern focal-plane wavefront sensor: measurement of atmospheric wavefront error modes and low wind effect in the nonlinear regime

We present a laboratory analysis of the use of a 19-core photonic lantern (PL) in combination with neural network (NN) algorithms as an efficient focal plane wavefront sensor (FP-WFS) for adaptive optics (AO), measuring wavefront errors (WFE) such as low wind effect (LWE), Zernike modes, and Kolmogorov phase maps. The aberrated wavefronts were experimentally simulated using a spatial light modulator with combinations of different phase maps in both the approximately linear regime (average incident RMS WFE of 0.88 rad) and in the nonlinear regime (average incident RMS WFE of 1.5 rad). Results were analyzed using an NN to determine the transfer function of the relationship between the incident WFE at the input modes at the multimode input of the PL and the intensity distribution output at the multicore fiber outputs end of the PL. The root mean square error (RMSE) of the reconstruction of petal and LWE modes were just 2.87×10−2 rad and 2.07×10−1 rad respectively, in the nonlinear regime. The reconstruction RMSE for Zernike combinations ranged from 5.67×10−2 rad to 8.43×10−1 rad, depending on the number of Zernike terms and incident RMS WFE employed. These results demonstrate the promising potential of PLs as an innovative FP-WFS in conjunction with NNs.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2024-10-07
DOI
https://doi.org/10.1117/1.jatis.10.4.049001
Citations
3
Primary Topic
Adaptive optics and wavefront sensing
Type
article
Field-Weighted Citation Impact
1.01
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article

Demonstration of a photonic lantern focal-plane wavefront sensor: measurement of atmospheric wavefront error modes and low wind effect in the nonlinear regime

Sergio G. Leon-Saval, Barnaby Norris, Christopher H. Betters, Wei Jin
3 citations
Journal of Astronomical Telescopes Instruments and Systems
Adaptive optics and wavefront sensing
1.01
article

Demonstration of a photonic lantern focal-plane wavefront sensor: measurement of atmospheric wavefront error modes and low wind effect in the nonlinear regime

Sergio G. Leon-Saval, Barnaby Norris, Christopher H. Betters, Wei Jin
article en
3 citations

Abstract

We present a laboratory analysis of the use of a 19-core photonic lantern (PL) in combination with neural network (NN) algorithms as an efficient focal plane wavefront sensor (FP-WFS) for adaptive optics (AO), measuring wavefront errors (WFE) such as low wind effect (LWE), Zernike modes, and Kolmogorov phase maps. The aberrated wavefronts were experimentally simulated using a spatial light modulator with combinations of different phase maps in both the approximately linear regime (average incident RMS WFE of 0.88 rad) and in the nonlinear regime (average incident RMS WFE of 1.5 rad). Results were analyzed using an NN to determine the transfer function of the relationship between the incident WFE at the input modes at the multimode input of the PL and the intensity distribution output at the multicore fiber outputs end of the PL. The root mean square error (RMSE) of the reconstruction of petal and LWE modes were just 2.87×10−2 rad and 2.07×10−1 rad respectively, in the nonlinear regime. The reconstruction RMSE for Zernike combinations ranged from 5.67×10−2 rad to 8.43×10−1 rad, depending on the number of Zernike terms and incident RMS WFE employed. These results demonstrate the promising potential of PLs as an innovative FP-WFS in conjunction with NNs.

Journal of Astronomical Telescopes Instruments and SystemsVol. 10(04)
The University of Sydney (AU)
Affordable and clean energy
Openalex Percentile: Top 24%
Adaptive optics and wavefront sensing
1.01
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