We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.

Durham Research Online
You are in:

On-sky results for adaptive optics control with data-driven models on low-order modes.

Sinquin, Baptiste and Prengere, Léonard and Kulcsár, Caroline and Raynaud, Henri-Francois and Gendron, Eric and Osborn, James and Basden, Alastair and Conan, Jean-Marc and Bharmal, Nazim and Bardou, Lisa and Staykov, Lazar and Morris, Tim and Buey, Tristan and Chemla, Fanny and Cohen, Matthieu (2020) 'On-sky results for adaptive optics control with data-driven models on low-order modes.', Monthly notices of the Royal Astronomical Society., 498 (3). pp. 3228-3240.


Dedicated tip-tilt loops are commonly implemented on adaptive optics (AO) systems. In addition, a number of recent high-performance systems feature tip-tilt controllers which are more efficient than the integral action controller. In this context, Linear Quadratic Gaussian (LQG) tip-tilt regulators based on stochastic models identified from AO telemetry have demonstrated their capacity to effectively compensate for the cumulated effects of atmospheric disturbance, windshake and vibrations. These tip-tilt LQG regulators can also be periodically re-tuned during AO operations, thus allowing to track changes in the disturbances’ temporal dynamics. This paper investigates the potential benefit of extending the number of low-order modes to be controlled using models identified from AO telemetry. The global stochastic dynamical model of a chosen number of turbulent low-order modes is identified through data-driven modelling from wavefront sensor measurements. The remaining higher modes are modelled using priors with autoregressive models of order 2. The loop is then globally controlled using the optimal LQG regulator build from all these models. Our control strategy allows for combining a dedicated tip-tilt loop with a deformable mirror that corrects for the remaining low-order modes and for the higher orders altogether, without resorting to mode decoupling. Performance results are obtained through evaluation of the Strehl ratio computed on H-band images from the scientific camera, or in replay mode using on-sky AO telemetry recorded in July 2019 on the CANARY instrument.

Item Type:Article
Full text:(VoR) Version of Record
Download PDF
Publisher Web site:
Publisher statement:This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Date accepted:18 August 2020
Date deposited:06 October 2020
Date of first online publication:26 August 2020
Date first made open access:06 October 2020

Save or Share this output

Look up in GoogleScholar