Adapting the pyramid wavefront sensor for pupil fragmentation of the ELT class telescopes
Nicolas Levraud (LAM, OAA), Vincent Chambouleyron (LAM), Olivier, Fauvarque (IFREMER), Mahawa Ciss\'e (LAM), Jean-Fran\c{c}ois Sauvage (LAM),, Beno\^it Neichel (LAM), Charlotte Bond (UK ATC), Enrico Pinna (OAA), Simone, Esposito (OAA), Noah Schwartz (UK ATC), Thierry Fusco (LAM)

TL;DR
This paper proposes a modified pyramid wavefront sensor scheme with spatial filtering to effectively detect and correct pupil fragmentation and petal modes in ELT telescopes, enhancing their adaptive optics performance.
Contribution
It introduces a double path wavefront sensor scheme with spatial filtering to measure and correct both turbulence and petal modes caused by pupil fragmentation in ELT telescopes.
Findings
The spatial structure of petal modes affects pyramid wavefront sensor sensitivity.
A double path wavefront sensor scheme can measure turbulence and petal modes simultaneously.
The proposed scheme restores the full spatial resolution of ELT adaptive optics.
Abstract
The next generation of Extremely Large Telescope (24 to 39m diameter) will suffer from the so-called "pupil fragmentation" problem. Due to their pupil shape complexity (segmentation, large spiders ...), some differential pistons may appear between some isolated part of the full pupil during the observations. Although classical AO system will be able to correct for turbulence effects, they will be blind to this specific telescope induced perturbations. Hence, such differential piston, a.k.a petal modes, will prevent to reach the diffraction limit of the telescope and ultimately will represent the main limitation of AO-assisted observation with an ELT. In this work we analyse the spatial structure of these petal modes and how it affects the ability of a Pyramid Wavefront sensor to sense them. Then we propose a variation around the classical Pyramid concept for increasing the WFS…
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