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Decoupling control for position error and surface error of segmented primary mirror

机译:分段主镜的位置误差和表面误差的解耦控制

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Large-aperture segmented primary mirror has been widely used in high-resolution space telescopes. After deployment, position error and surface error of each segmented mirror will lead inacceptable wavefront errors together. A critical problem is how to decouple position error and surface error from exit-pupil wavefront aberrations. We proposed a decoupling control strategy based on sensitivity matrix retrieval method. The sensitivity matrix of segmented mirror is calculated by simulation method and a new type of orthogonal polynomials is recommended to fit wavefront aberrations in non-circular area. First we give a simulation example to show how to decouple position errors in each degree of freedom if there are no surface errors. Then a further simulation reveals the decoupling control process for position and surface errors. The low order aberrations are corrected by position control actuators and high order aberrations are corrected by figure control actuators.
机译:大孔径分段主镜已广泛用于高分辨率太空望远镜。部署后,每个分段镜的位置误差和表面误差将共同导致无法接受的波阵面误差。一个关键问题是如何使出射光波前像差与位置误差和表面误差脱钩。我们提出了一种基于灵敏度矩阵检索方法的解耦控制策略。通过仿真方法计算出分段镜的灵敏度矩阵,并推荐一种新型的正交多项式来拟合非圆形区域的波前像差。首先,我们给出一个仿真示例,以说明在没有表面误差的情况下如何在每个自由度上解耦位置误差。然后,进一步的仿真揭示了位置和表面误差的解耦控制过程。低阶像差由位置控制执行器校正,而高阶像差由图形控制执行器校正。

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