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Model-Based Wavefront Control for CCAT

机译:基于模型的CCAT波前控制

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摘要

The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into 162 individual segments, each of which is provided with 3 positioning actuators. CCAT will be equipped with innovative Imaging Displacement Sensors (IDS) - inexpensive optical edge sensors - capable of accurately measuring all segment relative motions. These measurements are used in a Kalman-filter-based Optical State Estimator to estimate wavefront errors, permitting use of a minimum-wavefront controller without direct wavefront measurement. This controller corrects the optical impact of errors in 6 degrees of freedom per segment, including lateral translations of the segments, using only the 3 actuated degrees of freedom per segment. The edge sensors do not measure the global motions of the Primary and Secondary Mirrors. These are controlled using a gravity-sag look-up table. Predicted performance is illustrated by simulated response to errors such as gravity sag.
机译:25米孔径的CCAT亚毫米波望远镜将具有一个主镜,该主镜分为162个独立的部分,每个部分都配备了3个定位致动器。 CCAT将配备创新的成像位移传感器(IDS)-廉价的光学边缘传感器-能够精确测量所有段的相对运动。这些测量用于基于卡尔曼滤波器的光学状态估计器中,以估计波前误差,从而允许使用最小波前控制器,而无需直接进行波前测量。该控制器仅使用每个分段的3个激活的自由度,就可以校正每个分段6个自由度中的误差的光学影响,包括分段的横向平移。边缘传感器不测量主镜和次镜的整体运动。这些通过重力下垂查找表进行控制。通过对诸如重力垂度之类的误差的模拟响应来说明预测的性能。

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