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Stiffening an off-axis beam compressor mount for improved oerformance

机译:加强离轴光束压缩机的安装座,以提高性能

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The Navy Prototype Optical Interferometer (NPOI) near Flagstaff, Arizona, makes use of separate smaller optical elements spaced along a Y-array and used simultaneously to simulate an equivalent single large telescope. The instrument is useful in generating and upgrading existing astronomical catalogues and investigating synthetic aperture optical imaging techniques. The NPOI is a joint collaboration between the US Naval Observatory and Naval Research Laboratory in collaboration with the Lowell Observatory. Stellar radiation (visible light) reflects off 35 cm diameter flat mirrors, also known as siderostats, toward a tilt-tip mirror, which reflects a 12 cm diameter beam through a multi-reflection relay transport system. To maximize the reflective area of the siderostat optics and achieve an increase by a factor of 8.5 in light collecting area, a beam compressor is to be installed between the siderostat and fast tip/tilt mirror. However, the present configuration of a prototype beam compressor mount (BCM) vibrates at unacceptable amplitudes, which makes it nearly impossible to optically align the mirrors. This paper presents the results of finite element analyses conducted to quantify the design limitations of the prototype beam compressor mount. The analyses indicated that the current configuration is too soft, with very low fundamental frequencies, which verified the difficulties encountered during alignment tests. Based on these results, design modifications have been proposed to increase the overall structural stiffness of the mount and increase its fundamental frequency of vibration. These modifications will mechanically stabilize the structure for the alignment of the optics, and allow integration of the compressor into the interferometer. The interferometer will then have the capability to capture more light from each siderostat and allow observations of fainter stellar targets. More generally, the results can be useful as a guide for engineers and scientists involved in the design of similar optomechanical structures.
机译:亚利桑那州弗拉格斯塔夫附近的海军原型光学干涉仪(NPOI)利用沿Y阵列隔开的单独的较小光学元件,同时用于模拟等效的单个大型望远镜。该仪器可用于生成和升级现有的天文目录,以及研究合成孔径光学成像技术。 NPOI是美国海军天文台和海军研究实验室与洛厄尔天文台的联合合作。恒星辐射(可见光)从直径为35厘米的平面镜(也称为侧视镜)反射向倾斜镜,后者通过多反射中继传输系统反射直径为12厘米的光束。为了使侧视镜光学系统的反射面积最大化,并在聚光区实现8.5倍的增加,在侧视镜和快速倾斜/倾斜镜之间应安装光束压缩器。但是,原型光束压缩器安装架(BCM)的当前配置会以不可接受的幅度振动,这使得几乎不可能光学对齐反射镜。本文介绍了有限元分析的结果,以量化原型束流压缩机安装座的设计局限性。分析表明,当前配置太软,基频非常低,这证明了对准测试期间遇到的困难。根据这些结果,提出了一些设计修改方案,以增加安装座的总体结构刚度并增加其基本振动频率。这些修改将机械地稳定用于光学器件对准的结构,并允许将压缩机集成到干涉仪中。然后,干涉仪将能够捕获来自每个恒光调节器的更多光,并能够观察到较暗的恒星目标。更一般地,该结果对于参与类似光机结构设计的工程师和科学家可能是有用的指南。

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