Issue |
A&A
Volume 649, May 2021
|
|
---|---|---|
Article Number | A70 | |
Number of page(s) | 7 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/202140354 | |
Published online | 12 May 2021 |
Focal-plane-assisted pyramid wavefront sensor: Enabling frame-by-frame optical gain tracking
1
Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France
e-mail: vincent.chambouleyron@lam.fr
2
DOTA, ONERA, Université Paris Saclay, 91123 Palaiseau, France
3
IFREMER, Laboratoire Detection, Capteurs et Mesures (LDCM), Centre Bretagne, ZI de la Pointe du Diable, CS 10070, 29280 Plouzane, France
Received:
15
January
2021
Accepted:
1
March
2021
Aims. With its high sensitivity, the pyramid wavefront sensor (PyWFS) is becoming an advantageous sensor for astronomical adaptive optics (AO) systems. However, this sensor exhibits significant non-linear behaviours leading to challenging AO control issues.
Methods. In order to mitigate these effects, we propose to use in addition to the classical pyramid sensor a focal plane image combined with a convolutive description of the sensor to fast track the PyWFS non-linearities, the so-called optical gains (OG).
Results. We show that this additional focal plane imaging path only requires a small fraction of the total flux while representing a robust solution to estimating the PyWFS OG. Finally, we demonstrate the gain that our method brings with specific examples of bootstrapping and handling non-common path aberrations.
Key words: instrumentation: adaptive optics / telescopes
© V. Chambouleyron et al. 2021
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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