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COMPUTATIONAL MORPHOGENESIS OF TRUSS STRUCTURES - APPLICATION TO TELESCOPE STRUCTURE

机译:桁架结构的计算形态发生学-在望远结构中的应用

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摘要

Larger astronomical telescopes are required for research of deeper and darker space. Weight reduction techniques for telescopes are necessary to build them cost-effectively as well as constructionwise. However, it is not easy to design such a structure, because various tilt (elevation) angles caused by rotation of the optical support structure (OSS) of the telescope for astronomical observations result in a large change in the external load. In this paper, the scheme of multi-objective optimal design for truss structures for telescopes is proposed and demonstrated in an actually constructed 3.8 m telescope. The requirements of both weight minimization and homologous deformation are simultaneously satisfied by using SPEA2 as a multi-objective optimal method, where standard deviation of nodal displacements is adopted to evaluate homologous deformation.
机译:研究更深和更暗的空间需要使用更大的天文望远镜。望远镜的减重技术对于经济高效地建造它们是必不可少的。但是,设计这样的结构并不容易,因为用于天文观测的望远镜的光学支撑结构(OSS)的旋转引起的各种倾斜(仰角)导致外部载荷的较大变化。提出并在实际建造的3.8 m望远镜中对望远镜的桁架结构进行多目标优化设计。通过使用SPEA2作为多目标最优方法,同时满足重量最小化和同源变形的要求,其中采用节点位移的标准偏差来评估同源变形。

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