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

Published 3 Nov 2023 in physics.optics, astro-ph.IM, and physics.ins-det | (2311.01716v1)

Abstract: Here 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 such as low wind effect (LWE), Zernike modes and Kolmogorov phase maps. The aberrated wavefronts were experimentally simulated using a Spatial Light Modulator (SLM) with combinations of different phase maps in both the linear regime (average incident RMS wavefront error (WFE) of 0.88 rad) and in the non-linear regime (average incident RMS WFE of 1.5 rad). Results were analysed using a NN to determine the transfer function of the relationship between the incident wavefront error (WFE) at the input modes at the multimode input of the PL and the intensity distribution output at the multicore fibre outputs end of the PL. The root mean square error (RMSE) of the reconstruction of petal and LWE modes were just $2.87\times10{-2}$ rad and $2.07\times10{-1}$ rad respectively, in the non-linear regime. The reconstruction RMSE for Zernike combinations ranged from $5.67\times10{-2}$ rad to $8.43\times10{-1}$ 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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