首页> 外文会议>Workshop on Integrated Modeling of Telescopes, Feb 5-7, 2002, Lund, Sweden >Modeling and Analysis of LAMOST Primary Mirror Support Structure
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Modeling and Analysis of LAMOST Primary Mirror Support Structure

机译:LAMOST主镜支撑结构建模与分析

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The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) is a national large scientific project in China at the beginning of this century. It is an unconventional designed modern optical telescope and has the both large field of view and large aperture. The spherical primary mirror M_B in LAMOST is a segmented mirror with 37 sub-mirrors. The M_B will be supported by a very stable truss structure and the mirror surface will be kept in a high optical accuracy. This paper presents the work on the finite element model of the truss structure of M_B and gives the results of static and dynamic analysis with this model especially for the optimization of the higher stiffness and the lighter weight.
机译:大天空区多目标光纤光谱望远镜(LAMOST)是本世纪初在中国的一项国家大型科学项目。它是非常规设计的现代光学望远镜,具有大视野和大光圈。 LAMOST中的球面主镜M_B是具有37个子镜的分段镜。 M_B将由非常稳定的桁架结构支撑,并且镜面将保持较高的光学精度。本文介绍了M_B桁架结构的有限元模型的工作,并给出了使用该模型进行静态和动态分析的结果,尤其是为了优化较高的刚度和减轻重量。

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