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Conceptual design and structural analysis for an 8.4 m telescope

机译:8.4 m望远镜的概念设计和结构分析

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摘要

This paper describes the conceptual design of the optics support structures of a telescope with a primary mirror of 8.4 m, the same size as a Large Binocular Telescope (LBT) primary mirror. The design goal is to achieve a structure for supporting the primary and secondary mirrors and keeping them joined as rigid as possible. With this purpose an optimization with several models was done. This iterative design process includes: specifications development, concepts generation and evaluation. Process included Finite Element Analysis (FEA) as well as other analytical calculations. Quality Function Deployment (QFD) matrix was used to obtain telescope tube and spider specifications. Eight spiders and eleven tubes geometric concepts were proposed. They were compared in decision matrixes using performance indicators and parameters. Tubes and spiders went under an iterative optimization process. The best tubes and spiders concepts were assembled together. All assemblies were compared and ranked according to their performance.
机译:本文介绍了具有8.4 m主镜的望远镜的光学支撑结构的概念设计,该主镜的尺寸与大型双筒望远镜(LBT)主镜相同。设计目标是要获得一种结构,用于支撑主镜和副镜,并使它们保持尽可能牢固的连接。为此,对几个模型进行了优化。此迭代设计过程包括:规范开发,概念生成和评估。过程包括有限元分析(FEA)以及其他分析计算。质量功能展开(QFD)矩阵用于获得望远镜筒和星形轮规格。提出了八只蜘蛛和十一只管的几何概念。使用绩效指标和参数在决策矩阵中对它们进行了比较。试管和蜘蛛进行了反复的优化过程。最好的管和蜘蛛的概念组装在一起。比较所有程序集并根据其性能对其进行排名。

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