米级望远镜高对比度自适应光学系统

M. Mateen, O. Reynolds, M. Eickhoff
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引用次数: 0

摘要

本文介绍了星火光学靶场米级望远镜Castor正在建造的自然导星(NGS)自适应光学(AO)系统的最新情况。我们提出了一系列可变参数的辐射测量案例研究,如光源亮度、Shack-Hartmann子孔径数量、AO和Track环路帧率和带宽。我们通过对比来衡量系统性能,并调整误差预算以允许在明亮恒星附近检测昏暗物体。我们提出了不同AO组件之间的波段划分,如轨道传感器、波前传感器、计分相机和科学相机。我们展示了不同的配置,允许在昏暗的对象和明亮的对象跟踪之间切换。介绍了光学光学系统的光机械设计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
High contrast adaptive optics system for meter class telescopes
This paper provides a status update on the Natural Guidestar (NGS) Adaptive Optics (AO) system being built for Castor, the meter class telescope at the Starfire Optical Range. We present a radiometric case study for a range of variable parameters such as source brightness, number of Shack-Hartmann sub-apertures, AO and Track loop frame rate and bandwidth. We gauge system performance by contrast and adapt the error budget to allow detection of a dim object near a bright star. We present wave band splits between the different AO components such as track sensor, wavefront sensor, scoring camera, and science camera. We show the different configurations that allow to switch between dim object and bright object tracking. The opto-mechanical design of the AO system is also presented.
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