Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers

Traditional wavefront control in high-energy, high-intensity laser systems usually lacks real-time capability, failing to address dynamic aberrations. This limits experimental accuracy due to shot-to-shot fluctuations and necessitates long cool-down phases to mitigate thermal effects, particularly a...

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Main Authors: J. B. Ohland, N. Lebas, V. Deo, O. Guyon, F. Mathieu, P. Audebert, D. Papadopoulos
Format: Article
Language:English
Published: Cambridge University Press 2025-01-01
Series:High Power Laser Science and Engineering
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Online Access:https://www.cambridge.org/core/product/identifier/S2095471925000167/type/journal_article
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author J. B. Ohland
N. Lebas
V. Deo
O. Guyon
F. Mathieu
P. Audebert
D. Papadopoulos
author_facet J. B. Ohland
N. Lebas
V. Deo
O. Guyon
F. Mathieu
P. Audebert
D. Papadopoulos
author_sort J. B. Ohland
collection DOAJ
description Traditional wavefront control in high-energy, high-intensity laser systems usually lacks real-time capability, failing to address dynamic aberrations. This limits experimental accuracy due to shot-to-shot fluctuations and necessitates long cool-down phases to mitigate thermal effects, particularly as higher repetition rates become essential, for example, in inertial fusion research. This paper details the development and implementation of a real-time capable adaptive optics system at the Apollon laser facility. Inspired by astronomical adaptive optics, the system uses a fiber-coupled 905 nm laser diode as a pilot beam that allows for spectral separation, bypassing the constraints of pulsed lasers. A graphics processing unit-based controller, built on the open-source Compute And Control for Adaptive Optics framework, manages a loop comprising a bimorph deformable mirror and a high-speed Shack–Hartmann sensor. Initial tests showed excellent stability and effective aberration correction. However, integration into the Apollon laser revealed critical challenges unique to the laser environment that must be resolved to ensure safe operation with amplified shots.
format Article
id doaj-art-3a99bdf36bf249afb4e604ca65cd53f8
institution Kabale University
issn 2095-4719
2052-3289
language English
publishDate 2025-01-01
publisher Cambridge University Press
record_format Article
series High Power Laser Science and Engineering
spelling doaj-art-3a99bdf36bf249afb4e604ca65cd53f82025-08-20T03:45:15ZengCambridge University PressHigh Power Laser Science and Engineering2095-47192052-32892025-01-011310.1017/hpl.2025.16Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasersJ. B. Ohland0https://orcid.org/0000-0002-1328-2188N. Lebas1V. Deo2O. Guyon3F. Mathieu4P. Audebert5https://orcid.org/0000-0002-1330-3946D. Papadopoulos6https://orcid.org/0000-0001-7163-0761Laboratoire d’Utilisation des Lasers Intenses, Ecole Polytechnique, Palaiseau Cedex, France GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, GermanyLaboratoire d’Utilisation des Lasers Intenses, Ecole Polytechnique, Palaiseau Cedex, FranceSubaru Telescope, National Astronomical Observatory of Japan, National Institute of Natural Sciences, Hilo, HI, USASubaru Telescope, National Astronomical Observatory of Japan, National Institute of Natural Sciences, Hilo, HI, USA Astrobiology Center of NINS, Osawa, Mitaka, Tokyo, Japan Steward Observatory, University of Arizona, Tucson, AZ, USA College of Optical Sciences, University of Arizona, Tucson, AZ, USALaboratoire d’Utilisation des Lasers Intenses, Ecole Polytechnique, Palaiseau Cedex, FranceLaboratoire d’Utilisation des Lasers Intenses, Ecole Polytechnique, Palaiseau Cedex, FranceLaboratoire d’Utilisation des Lasers Intenses, Ecole Polytechnique, Palaiseau Cedex, FranceTraditional wavefront control in high-energy, high-intensity laser systems usually lacks real-time capability, failing to address dynamic aberrations. This limits experimental accuracy due to shot-to-shot fluctuations and necessitates long cool-down phases to mitigate thermal effects, particularly as higher repetition rates become essential, for example, in inertial fusion research. This paper details the development and implementation of a real-time capable adaptive optics system at the Apollon laser facility. Inspired by astronomical adaptive optics, the system uses a fiber-coupled 905 nm laser diode as a pilot beam that allows for spectral separation, bypassing the constraints of pulsed lasers. A graphics processing unit-based controller, built on the open-source Compute And Control for Adaptive Optics framework, manages a loop comprising a bimorph deformable mirror and a high-speed Shack–Hartmann sensor. Initial tests showed excellent stability and effective aberration correction. However, integration into the Apollon laser revealed critical challenges unique to the laser environment that must be resolved to ensure safe operation with amplified shots.https://www.cambridge.org/core/product/identifier/S2095471925000167/type/journal_articlebeam controladaptive opticsdynamic aberrationsstabilization
spellingShingle J. B. Ohland
N. Lebas
V. Deo
O. Guyon
F. Mathieu
P. Audebert
D. Papadopoulos
Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
High Power Laser Science and Engineering
beam control
adaptive optics
dynamic aberrations
stabilization
title Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
title_full Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
title_fullStr Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
title_full_unstemmed Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
title_short Apollon Real-Time Adaptive Optics: astronomy-inspired wavefront stabilization in ultraintense lasers
title_sort apollon real time adaptive optics astronomy inspired wavefront stabilization in ultraintense lasers
topic beam control
adaptive optics
dynamic aberrations
stabilization
url https://www.cambridge.org/core/product/identifier/S2095471925000167/type/journal_article
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