AI Article Synopsis

  • Optical aberrations in telescopes prevent them from achieving their best possible clarity, but these can be corrected using deformable mirrors guided by real-time data about the aberrations from images.
  • Current methods for detecting these aberrations depend on potentially flawed physical models, which can hinder the correction process.
  • This study proposes a new approach using model-free reinforcement learning to improve the estimation and correction of aberrations using phase diversity images, showing effective performance even under various conditions and noise levels.

Article Abstract

Optical aberrations prevent telescopes from reaching their theoretical diffraction limit. Once estimated, these aberrations can be compensated for using deformable mirrors in a closed loop. Focal plane wavefront sensing enables the estimation of the aberrations on the complete optical path, directly from the images taken by the scientific sensor. However, current focal plane wavefront sensing methods rely on physical models whose inaccuracies may limit the overall performance of the correction. The aim of this study is to develop a data-driven method using model-free reinforcement learning to automatically perform the estimation and correction of the aberrations, using only phase diversity images acquired around the focal plane as inputs. We formulate the correction problem within the framework of reinforcement learning and train an agent on simulated data. We show that the method is able to reliably learn an efficient control strategy for various realistic conditions. Our method also demonstrates robustness to a wide range of noise levels.

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Source
http://dx.doi.org/10.1364/OE.529415DOI Listing

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