Abstract

The pyramid wavefront sensor (PWFS) is the currently preferred design for adaptive optics (AO) systems for extremely large telescopes, as focal plane wavefront sensing bears potential for a large intrinsic sensitivity gain when compared to Shack–Hartmann (SH) sensors. Yet, obtaining a high quality pyramidal prism and a model-consistent assembly remains a critical design factor. We demonstrate that the traditional gradient sensing controller is extremely sensitive to prism shape defects and assembly misalignments. We show that even optimal registration of quadrants on the detector may be insufficient to prevent misalignment induced performance loss through a theoretical analysis of the impact of detection plane quadrants sampling errors and individual translations, which may be induced by a variety of mechanical defects. These misalignments displace wavefront information to terms not included in the conventional gradient-like slopes maps and high spatial frequencies become invisible to the sole X− and Y− axis differences. We introduce expanded space control (ESC) for quad-cell signal by generalizing output measurements of the PWFS and demonstrate its insensitivity to misalignment-induced information loss, therefore dramatically relaxing machining and alignment constraints for PWFS engineering. This work presents the theoretical developments leading to ESC design, along with validating performance and robustness results, both in end-to-end numerical simulations and on a PWFS demonstrator bench at LESIA.

Highlights

  • This paper presents novel research about pyramid wavefront sensor (PWFS; Ragazzoni 1996) control, conducted within the MICADO SCAO module (Davies et al 2010; Clénet et al 2014) development at LESIA

  • This paper presents a possible improvement to PWFS control, called expanded space control (ESC)

  • It is expected that using an XYGlob. measurement method, misalignment significantly affects the sensing ability of the PWFS for input phase spatial frequencies at a −45◦ angle, and corresponding speckles should persist in the long exposure point spread function (PSF)

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Summary

Introduction

This paper presents novel research about pyramid wavefront sensor (PWFS; Ragazzoni 1996) control, conducted within the MICADO SCAO module (Davies et al 2010; Clénet et al 2014) development at LESIA. Knowledge of modulation impact (Ragazzoni et al 2002b), signal normalization, edge-diffracted photons usage (Vérinaud 2004), theoretical models (Shatokhina 2014; Fauvarque et al 2016a,b), optimal modal control (Gendron & Léna 1994; Korkiakoski et al 2008a; Deo et al 2018), or phase reconstruction algorithms do not yet converge into a unique, well-established set of operation guidelines.

Measurements of the pyramid wavefront sensor
Misalignments of pyramid quadrants
Pixel selection and misalignment distributions
Definition
Simulated impact on real AO systems
Misalignment figure of merit
Experimental setup and protocols
Comparing measurement methods for a perfect PWFS
Misalignment impact on end-to-end performance
Conclusions
Preselected reference quadrant method
Findings
Optimal method
Full Text
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