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Adaptive optics test bench for predictive wavefront correction

机译:自适应光学测试台,用于预测波前校正

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摘要

We describes the status of AO test bench, which is developing at the Adaptive optics Lab, V.E. Zuev Institute ofAtmospheric Optics of the Siberian Branch of the Russian Academy of Sciences (IAO SB RAS), Tomsk, Russia tosimulate predictive algorithms of wavefront adaptive correction. The description of the optical and mechanical design,components AO bench, and the working principle and first experimental results are presented. The current AO test benchconsists of laser source, two deformable mirrors with 59 actuators and 56 mm diameter (Visionica Ltd., Russia), twotip/tilt mirrors (IAO SB RAS, Russia), Shack-Hartmann Wavefront Sensor (WFS), which we specially designed, and ascience camera for the evaluation of the performance. The user derived aberrations are introduced using a onedeformable mirror and corrected by another deformable mirror. The tip/tilt mirrors are used for predictive control of thelow-order wavefront aberrations related such as vibrations.
机译:我们描述了AO光学测试台的状态,该测试台是在V.E的自适应光学实验室开发的。祖夫研究所 俄罗斯科学院西伯利亚分院(IAO SB RAS)的大气光学 模拟波前自适应校正的预测算法。光学和机械设计的说明, 介绍了AO工作台的组件,并介绍了其工作原理和首次实验结果。当前的AO测试台 包括激光源,两个带有59个促动器和56毫米直径的可变形反射镜(俄罗斯维尼察有限公司),两个 倾斜/倾斜镜(IAO SB RAS,俄罗斯),我们专门设计的Shack-Hartmann波前传感器(WFS)和 科学相机的性能评估。用户导出的像差使用一个引入 可变形镜,并由另一个可变形镜校正。倒车镜/倾斜镜用于对车窗的预测控制 与低阶波前像差有关,例如振动。

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