smat是一种测量TMT主镜支架支撑点机械载荷的工具

J. Nijenhuis, N. van der Heiden, W. Jonker
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引用次数: 1

摘要

TMT将是一个由492个部分组成主镜的望远镜。每个部分都由高度复杂的部分支持组件(SSA)支持,每个部分都将使用称为smat的工具进行验收测试。该工具将安装在每个SSA的顶部,并提供应用于其27个支撑点的负载分布。由于机械公差,这些载荷将略有变化,这是完全可以接受的,并且可以使用有限元分析进行预测。然而,制造误差和寄生刚度的贡献可能导致不可接受的偏差。这是应该避免的。本文将描述smart的功能。该工具的设计使得可以在任何位置测量分段支撑载荷。在SSA中,实施了21个翘曲线束(WH)来主动补偿表面形状误差(SFE)。在使用smart时,还可以验证这些WH是否正常工作。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
SMATT, a tool that measures the mechanical loads on the support points of the TMT primary mirror supports
TMT will be a telescope with 492 segments making up the primary mirror. Each of these segments is supported with a highly sophisticated Segment Support Assembly (SSA) and each of them is to be tested for acceptance using a tool called SMATT. This tool will be mounted on top of each SSA and provides the load distribution applied to its 27 support points. These loads will vary slightly due to mechanical tolerances which is perfectly acceptable and can be predicted using FE-analysis. However manufacturing errors and parasitic stiffness contributions may cause unacceptable deviations. This should be avoided. The article will describe the functioning of SMATT. The tool is designed such that the segment support loads can be measured in any position. In the SSA, 21 Warping Harnesses (WH) are implemented to actively compensate for Surface Form Errors (SFE). These WH can also be verified for proper functioning when using SMATT.
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