Real-time aimer based on special-shaped microlens and optical fiber bundle

Anzhi Wang, Jiabin Wang, Zhaoxu Gan, Yuxiang Yan, Shengjia Wang, Qi Yan, Tao Geng, Shuang Chen, Pengfei Wang, Weimin Sun
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Abstract

High precision alignment between the fiber core in the focal plane and the image of the target star is of great significance for the observation of multi-target telescopes. In this work, we propose and demonstrate a Special-shaped Micro-lens Aimer for Real-time Targeting, namely SMART, combining a special-shaped microlens and a fiber bundle to realize online alignment and improve the coupling efficiency of fibers. The platform in the center of the microlens transmits the starlight to the science fiber of the fiber bundle without changes in focal ratio. Six side micro-lenses couple leakage light to six feedback fibers and return misalignment signals. The structural parameters of SMART are well designed. Fresnel diffraction theory is applied to build a model for simulating the performance of SMART. In the SMART measurement, a pinhole with a diameter of 200 μm is used to imitate the effect of atmospheric turbulence during astronomical observations. Experimental results indicate that when the image spot is offset relative to the science fiber, the misaligned direction and displacement distance are identified by the signal of feedback fibers in SMART with a resolution of 0.02 mm and a detection range of 0.08 mm to 0.26 mm.
基于异形微透镜和光纤束的实时瞄准器
焦平面光纤纤芯与目标星图像之间的高精度对准对于多目标望远镜的观测具有重要意义。在这项工作中,我们提出并演示了一种用于实时瞄准的异形微透镜瞄准器,即 SMART,它将异形微透镜和光纤束结合在一起,实现了在线对准并提高了光纤的耦合效率。微透镜中心的平台将星光传输到光纤束的科学光纤,而不会改变焦比。六侧微透镜将漏光耦合到六根反馈光纤,并返回失准信号。SMART 的结构参数经过精心设计。菲涅尔衍射理论用于建立模拟 SMART 性能的模型。在 SMART 测量中,使用了一个直径为 200 μm 的针孔来模仿天文观测过程中的大气湍流效应。实验结果表明,当图像点相对于科学光纤发生偏移时,SMART 的反馈光纤信号可识别出错位方向和位移距离,分辨率为 0.02 毫米,检测范围为 0.08 毫米至 0.26 毫米。
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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