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X-ray Telescope Mirror Mounting and Deformation Reduction Using ThermoYield Actuators and Mirror Geometry Changes

机译:使用Thermoyield执行器和镜面几何变化,X射线望远镜镜安装和变形减少

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Recently, the X-ray optics community has been developing technology' for high angular resolution, large collecting area X-ray telescopes such as the Lynx mission concept. To meet the high collecting area requirements of such telescope concepts, research is being conducted on thin, segmented optics. The precision mounting posts that fixture and align segmented optics must be the correct length to sub-micron accuracy to satisfy the angular resolution goals of such a concept. Mirror distortion caused by adhesive shrinkage at mount points on the mirror surface also needs to be controlled to micron-radian tolerances. We report on two solutions to these problems. Set-and-forget adjustable length optical mounting posts have been developed to control mirror spacer length. The actuator consists of a metal cylinder with a cylindrical neck cut halfway along the length. To change the length of this actuator, an axial force is applied and the neck is momentarily heated to the plastic deformation temperature via resistive heating. All of the plastic deformation that occurs becomes permanent after cooling. Both compression and expansion of these actuators has been demonstrated in steps ranging from 6 nm to several microns. This paper will describe an experimental setup, show, and discuss data. Additionally, a stress relief technique to reduce mirror distortion caused by shrinkage of the adhesive bond to the actuator is proposed and demonstrated by modelling.
机译:最近,X射线光学界一直在开发技术'用于高角度分辨率,大收集区域X射线望远镜,如Lynx任务概念。为了满足这种望远镜概念的高收集区域要求,正在进行研究薄,分段的光学。夹具和对齐分段光学器件的精密安装柱必须是亚微米精度的正确长度,以满足这种概念的角度分辨率。在镜面上的安装点处的粘合剂收缩引起的镜像也需要控制到微米 - 弧度公差。我们向这些问题报告了两个解决方案。已经开发出设定和忘记可调节的长度光学安装柱以控制镜子间隔长度。致动器由金属圆筒组成,金属缸沿着长度的半径切割圆柱形颈部。为了改变该致动器的长度,施加轴向力,并且颈部通过电阻加热暂时地加热到塑性变形温度。发生冷却后发生的所有塑性变形都是永久性的。这些致动器的压缩和扩展都已在6nm到几微米的步骤中证明。本文将描述实验设置,显示和讨论数据。另外,提出了一种通过建模提出并通过粘合剂与致动器收缩引起的镜子变形来降低镜子变形的应力浮雕技术。

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