Image-based wavefront correction using model-free Reinforcement Learning
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arXiv
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| Main Authors: | , , , , |
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| Format: | Preprint |
| Published: |
2024
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| _version_ | 1866929400607408128 |
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| author | Gutierrez, Yann Mazoyer, Johan Mugnier, Laurent M. Herscovici-Schiller, Olivier Abeloos, Baptiste |
| author_facet | Gutierrez, Yann Mazoyer, Johan Mugnier, Laurent M. Herscovici-Schiller, Olivier Abeloos, Baptiste |
| contents | 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. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2406_18143 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Image-based wavefront correction using model-free Reinforcement Learning Gutierrez, Yann Mazoyer, Johan Mugnier, Laurent M. Herscovici-Schiller, Olivier Abeloos, Baptiste Optics Instrumentation and Methods for Astrophysics 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. |
| title | Image-based wavefront correction using model-free Reinforcement Learning |
| topic | Optics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2406.18143 |