Using the Gerchberg-Saxton algorithm to reconstruct non-modulated pyramid wavefront sensor measurements
Vincent Chambouleyron, Aditya Sengupta, Ma\"issa Salama, Maaike A.M, van Kooten, Benjamin L. Gerard, Sebastiaan Y. Haffert, Sylvain Cetre, Daren, Dillon, Renate Kupke, Rebecca Jensen-Clem, Phil Hinz, Bruce Macintosh

TL;DR
This paper introduces a novel iterative reconstruction method using the Gerchberg-Saxton algorithm to invert non-modulated pyramid wavefront sensor signals, significantly enhancing their dynamic range for adaptive optics applications.
Contribution
It presents a new inversion technique for nPWFS signals based on reciprocity and the Gerchberg-Saxton algorithm, improving dynamic range in AO systems.
Findings
The method increases the dynamic range of nPWFS reconstructions.
It performs well in simulations and laboratory tests.
The technique is now the standard inversion method at SEAL.
Abstract
Adaptive optics (AO) is a technique to improve the resolution of ground-based telescopes by correcting, in real-time, optical aberrations due to atmospheric turbulence and the telescope itself. With the rise of Giant Segmented Mirror Telescopes (GSMT), AO is needed more than ever to reach the full potential of these future observatories. One of the main performance drivers of an AO system is the wavefront sensing operation, consisting of measuring the shape of the above mentioned optical aberrations. Aims. The non-modulated pyramid wavefront sensor (nPWFS) is a wavefront sensor with high sensitivity, allowing the limits of AO systems to be pushed. The high sensitivity comes at the expense of its dynamic range, which makes it a highly non-linear sensor. We propose here a novel way to invert nPWFS signals by using the principle of reciprocity of light propagation and the Gerchberg-Saxton…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Wireless Communication Technologies · Optical Systems and Laser Technology
