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Conceptual design of 1.5m aperture vertical collimator assembly with short tube and long focus

机译:1.5m孔径短直管长焦准直器组件的概念设计

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In order to evaluate and test the image quality of large aperture telescope, the most directly method is adopting the collimator and test the telescope system with full aperture. Changchun Institute of Optics, Fine Mechanics and Physics (CIOMP) commenced developing the large aperture collimator for interferometric and image quality testing of meter scale optical systems under cryogenic, vacuum conditions. The aperture of the collimator which has been on the conceptual design phase is 1.5m diameter, and the optical configuration is Cassegrain, the focus is 50m. The material of reaction bonded Silicon Carbide (RB-SiC) produced by CIOMP will be used as the primary mirror substrate. And the figure accuracy of the primary mirror will be polished better than 15nm (RMS). The collimator will be working in a vacuum chamber and face down vertically to the unit under test. The application requirements, specification requirements, and some key technology are demonstrated and analysed with finite element analysis (FEA) in the paper. The feasibility, error budget, and hazards evaluation of the collimator are fulfilled by the FEA results. It demonstrated that the conceptual design meet the requirements of the 1.5m aperture vertical collimator, and could achieve the high accuracy requirements of the wavefront for the beam of light in the vacuum chamber, which the wavefront error should less than 32nm(RMS). Mechanical alignment errors induced by thermal and structural perturbations are monitored with an auto-focusing system to enable focus compensation. The ambient temperature of the collimator in chamber are controlled allowing testing while the chamber shrouds and test unit are brought to cryogenic temperatures. With the high accuracy of the wavefront, the collimator could test the image resolution, modulation transfer functions (MTFs), point spread functions (PSFs), encircled energy, wavefront error, best focus, etc. for optical systems. And the conceptual design could be consulted to other large aperture collimators.
机译:为了评估和测试大光圈望远镜的图像质量,最直接的方法是采用准直仪并测试全光圈望远镜系统。长春光学精密机械与物理研究所(CIOMP)开始开发用于在低温,真空条件下对米级光学系统进行干涉和图像质量测试的大孔径准直仪。处于概念设计阶段的准直仪的孔径为1.5m直径,光学配置为Cassegrain,焦点为50m。 CIOMP生产的反应结合碳化硅(RB-SiC)的材料将用作主镜基板。而且主镜的图形精度将被抛光好于15nm(RMS)。准直仪将在真空室中工作,并垂直向下面对被测设备。通过有限元分析(FEA)对应用需​​求,规范需求和一些关键技术进行了演示和分析。准直器的可行性,错误预算和危害评估由FEA结果完成。结果表明,该概念设计满足1.5m孔径垂直准直仪的要求,可以达到真空室内光束对波前的高精度要求,其波前误差应小于32nm(RMS)。由热和结构扰动引起的机械对准误差可通过自动聚焦系统进行监控,以实现聚焦补偿。控制腔室内准直仪的环境温度,以便在将腔室护罩和测试单元置于低温状态下进行测试。借助波前的高精度,准直仪可以测试光学系统的图像分辨率,调制传递函数(MTF),点扩展函数(PSF),环绕能量,波前误差,最佳聚焦等。并且可以向其他大口径准直仪咨询概念设计。

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