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The MICADO first light imager for the ELT: Relay Optics Opto-Mechanical design

机译:ELT的MICADO第一灯成像仪:继电器光学光学设计

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MICADO is the Multi-AO Imaging Camera for Deep Observations, a first light instrument for the Extremely Large Telescope (ELT). The instrument provides imaging, astrometric, spectroscopic and coronographic observing modes. MICADO will be assisted by a Single-Conjugate Adaptive Optics (SCAO) system and the Multi-conjugate Adaptive Optics RelaY (MAORY). The instrument will provide a narrow (19") and a wide (51") Field of View. MICADO can operate in the so-called stand-alone mode in the absence of MAORY with the SCAO correction alone. Here, we present the opto-mechanical design of the Relay Optics (RO), the optical system relaying the ELT focal plane to an accessible position for MICADO using the SCAO-only stand-alone observing mode. The RO consists of an optical bench made of carbon fiber reinforced plastic (CFRP), an optical assembly made of three flat mirrors with motorized piston-tip-tilt mounts and three additional powered mirrors of up to ~500 mm in diameter, the MICADO calibration assembly, and a cover to protect all opto-mechanical components on top of the bench. A 9-point whiffletree support, combined with a thermal compensation system is implemented for the critical mirrors. The static and the dynamic performance of the MICADO RO are investigated through a detailed Finite Element Model (FEM), the results are combined with a Zernike basis representation of the mirror surface deformations performed in Zemax for assessing the optical performance.
机译:蟋是多AO成像相机深观测,为特大望远镜(ELT)第一光仪器。该仪器提供成像,天文,光谱和coronographic观察模式。蟋将由单共轭自适应光学(SCAO)系统和多偶联物自适应光学中继(MAORY)进行辅助。该仪器将提供窄(19“)和宽(51”)视场。蟋可以在所谓的独立模式在没有MAORY的单独的SCAO校正操作。这里,我们提出的中继光学器件(RO),该光学系统使用SCAO仅单机观测模式中继ELT焦平面到可访问位置蟋的光机械设计。的RO包括由碳纤维制成的光具座的增强塑料(CFRP),光学组件由具有机动活塞尖端倾斜安装件3个平面镜和向上的三个附加动力反射镜5〜50毫米的直径,蟋校准组件,以及一个盖,以保护在工作台上的顶部所有光学机械组件。 9点whiffletree支撑,具有热补偿系统相结合是为临界反射镜实现。静态和蟋RO的动态性能通过一个详细的有限元模型(FEM)的调查,将结果与表面变形在Zemax中用于评估光学性能进行的反射镜的泽尼克基础表示结合。

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