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High-bandwidth tip-tilt vibration compensation in telescope systems

机译:望远镜系统的高带宽尖端倾斜振动补偿

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Mechanical vibrations resulting from wind, ground vibrations and actuator imperfections lower the performance of optical telescope systems used for astronomical applications, as well as free-space optical communication. This paper proposes a high-bandwidth tip-tilt compensation system for optical telescopes, in order to reduce the influence of these vibrations. A typical, high precision, motorized telescope system is used as a base for this evaluation. By utilization of a tip-tilt sensor, the resulting tip-tilt errors are measured and analyzed in the frequency domain. A fast steering mirror integrated into the optical path allows to compensate for the measured tip-tilt errors. The performance of the fast steering mirror based system is compared to the original, uncompensated system, as well as to a compensation loop, which uses the telescope mount to counteract measured errors. Experiments demonstrate a significant reduction of the tip-tilt errors due to vibrations by a factor of 5 (altitude axis) and by a factor of 4.6 (azimuth axis) utilizing a compensation bandwidth of up to 810 Hz.
机译:风力,地面振动和执行器缺陷产生的机械振动降低了用于天文应用的光学望远镜系统的性能,以及自由空间光学通信。本文提出了一种用于光学望远镜的高带宽尖端补偿系统,以减少这些振动的影响。典型的高精度电动望远镜系统用作该评估的基础。通过利用尖端倾斜传感器,在频域中测量并分析产生的尖端倾斜误差。集成到光路中的快速转向镜允许补偿测量的尖端倾斜误差。将基于快速转向镜的系统的性能与原始的,未偿付的系统以及使用望远镜安装件抵消测量误差的补偿环比较。实验表明,由于振动,通过5(高度轴)的振动和4.6(方位角轴)的振动,利用高达810Hz的补偿带宽来显着降低尖端倾斜误差。

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