基于模型强化学习的自适应光学控制实验室实验

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE
Jalo Nousiainen, Byron Engler, Markus Kasper, Chang Rajani, Tapio Helin, Cédric T. Heritier, Sascha P. Quanz, Adrian M. Glauser
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引用次数: 0

摘要

类地系外行星的直接成像是下一代地基望远镜最突出的科学驱动力之一。通常情况下,类地系外行星与其宿主恒星的角距很小,因此很难对其进行探测。因此,自适应光学(AO)系统的控制算法必须经过精心设计,以便将系外行星与主恒星产生的残余光区分开来。改进自适应光学系统控制的一个很有前途的研究方向是数据驱动控制方法,如强化学习(RL)。强化学习是机器学习研究领域的一个活跃分支,通过与环境的交互来学习对系统的控制。因此,RL 可以被看作是一种自动运行控制方法,其使用完全是一种交钥匙操作。特别是,基于模型的 RL 已被证明可以应对时间和错误注册错误。同样,它也被证明能适应非线性波前传感,同时在训练和执行方面也很高效。在这项工作中,我们实施了一种名为 "AO 策略优化"(PO4AO)的 RL 方法,并将其应用于欧洲南方天文台总部基于 GPU 的高阶自适应光学测试台(GHOST)。我们的实施允许训练与推理并行进行,这对于在天空运行至关重要。我们特别研究了该方法的预测和自校准方面。在运行 PyTorch 的 GHOST 上实现的新方法,除了硬件、流水线和 Python 接口延迟外,只引入了大约 700 μs 的延迟。我们为该方法的实现开源了文档齐全的代码,并明确了对 RTC 管道的要求。我们还讨论了该方法的重要超参数及其对该方法的影响。此外,本文还讨论了延迟的来源以及实现更低延迟的可能途径。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Laboratory experiments of model-based reinforcement learning for adaptive optics control
Direct imaging of Earth-like exoplanets is one of the most prominent scientific drivers of the next generation of ground-based telescopes. Typically, Earth-like exoplanets are located at small angular separations from their host stars, making their detection difficult. Consequently, the adaptive optics (AO) system’s control algorithm must be carefully designed to distinguish the exoplanet from the residual light produced by the host star. A promising avenue of research to improve AO control builds on data-driven control methods, such as reinforcement learning (RL). RL is an active branch of the machine learning research field, where control of a system is learned through interaction with the environment. Thus, RL can be seen as an automated approach to AO control, where its usage is entirely a turnkey operation. In particular, model-based RL has been shown to cope with temporal and misregistration errors. Similarly, it has been demonstrated to adapt to nonlinear wavefront sensing while being efficient in training and execution. In this work, we implement and adapt an RL method called policy optimization for AO (PO4AO) to the GPU-based high-order adaptive optics testbench (GHOST) test bench at ESO headquarters, where we demonstrate a strong performance of the method in a laboratory environment. Our implementation allows the training to be performed parallel to inference, which is crucial for on-sky operation. In particular, we study the predictive and self-calibrating aspects of the method. The new implementation on GHOST running PyTorch introduces only around 700 μs of in addition to hardware, pipeline, and Python interface latency. We open-source well-documented code for the implementation and specify the requirements for the RTC pipeline. We also discuss the important hyperparameters of the method and how they affect the method. Further, the paper discusses the source of the latency and the possible paths for a lower latency implementation.
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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