A high-precision and efficient adaptive alignment method for Cassegrain dual mirror optical system based on machine learning algorithms

Jian XIONG , Zhijing ZHANG , Xinhai YU , Qimuge SAREN , Taiyu SU , Erbo LI
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Abstract

The Cassegrain telescope is widely used in aerospace exploration equipment, characterized by compact structure, complex optical path, and high imaging quality. However, due to the difficulty in establishing an accurate correspondence between the relative pose and imaging quality of a multi mirror group with real machining errors, the current Cassegrain telescope assembly process is very difficult, with blind operation, time-consuming, and low accuracy. This article proposes a high-precision adaptive alignment method for Cassegrain dual mirror optical systems based on machine learning algorisms, and an experimental adaptive alignment system with uncoupled degrees of freedom is developed. Firstly, the overall architecture of the adaptive alignment method is proposed consists of detection, calculation and alignment modules. In the detection module, the Zernike polynomial coefficient of wavefront aberration of the optical system is detected online through the interferometer, meanwhile the pose coordinates of the secondary mirror is accurately fed back through a 6-DOF nanoscale micro mechanism. In the calculation module, machine learning algorithm is applied to build a nonlinear mapping model between the Zernike coefficient and the pose coordinates of the secondary mirror. In the alignment module, the pose coordinates of the secondary mirror can be forced to adjust to the target position. Then, during the real alignment process, the Zernike coefficient test data of the optical system alignment process is monitored in real time, and the nonlinear mapping model is employed to calculate the pose coordinates and then the misalignment of the secondary mirror. Finally, the alignment module is driven to execute the pose correction according to the calculated misalignment value, realizing a high-precision adjustment of the Cassegrain dual mirror optical system. Experimental results shows that the average alignment time cost can be dramatically reduced from around 7 days using the current manual alignment method to just 30 minutes using the proposed adaptive alignment method for achieving a current standard alignment accuracy of wavefront aberration root mean square (RMS) less than 0.1λ, which greatly improves the assembly efficiency. This study proposes a new method for high-precision and efficient alignment of optical systems based on artificial intelligence and contributes to the efficiency improvement for optical assembly.
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基于机器学习算法的卡塞格伦双镜光学系统高精度高效自适应对准方法
卡塞格伦望远镜广泛应用于航天探测设备,具有结构紧凑、光路复杂、成像质量高等特点。然而,由于多镜组的相对姿态与成像质量之间难以建立准确的对应关系,且存在实际加工误差,因此目前的卡塞格伦望远镜装配工艺难度大、盲目操作、耗时长、精度低。本文提出了一种基于机器学习算法的卡塞格伦双镜光学系统高精度自适应对准方法,并开发了一种非耦合自由度自适应对准实验系统。首先,自适应配准方法的总体结构由检测、计算和配准模块组成。在检测模块中,通过干涉仪在线检测光学系统波前像差的Zernike多项式系数,同时通过6-DOF纳米级微机构精确反馈副镜的姿态坐标。在计算模块中,应用机器学习算法建立 Zernike 系数与副镜姿态坐标之间的非线性映射模型。在对准模块中,副反射镜的姿态坐标可以强制调整到目标位置。然后,在实际对准过程中,实时监测光学系统对准过程的 Zernike 系数测试数据,并利用非线性映射模型计算姿态坐标,进而计算副反射镜的偏差。最后,根据计算出的偏差值驱动对准模块执行姿态校正,实现卡塞格伦双镜光学系统的高精度调整。实验结果表明,使用所提出的自适应对准方法,平均对准时间成本可从目前使用的人工对准方法的 7 天左右大幅降低到仅需 30 分钟,即可实现波前像差均方根(RMS)小于 0.1λ 的当前标准对准精度,从而大大提高了装配效率。本研究提出了一种基于人工智能的高精度、高效率光学系统对准新方法,有助于提高光学装配的效率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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