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Mechanics of Magnetostrictive Thin Film Deformation and its Application in Active X-ray Optics.

机译:磁致伸缩薄膜变形的力学及其在有源X射线光学中的应用。

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摘要

High quality imaging system of telescopes in astronomy requires innovations to remove or correct the mid-spatial frequency (MSF) ripples on the mirror surface of lightweight optics. When the telescope is sent to the space, its launch mass is the key point to limit its collecting area. Therefore, the lightweight optics (100-150 mum thick electroplated nickel/cobalt, or 200-400 mum thick glass) is considered to be employed. However, the surface profile of the thin optical surface can't be polished to extremely high accuracy. Instead, the profile is expected to be corrected by applying voltage or magnetic field to drive the coating of smart materials (piezo or magnetostrictive materials) on the back side of the mirrors. During the process, the surface profile correction by the local stress on the 2-d surface is challenging. Both the measurements and the theoretical prediction of the surface profiles after correction are investigated.;As a first step in the development of tools to predict the deformation of the coated glass strip samples (20x5x0.1 mm), one commercial magnetically smart material (MSM) was deposited on the samples by the magnetron sputtering method. One experimental setup was established to measure the deflections of these coated samples under an external magnetic field by Zygo NewView white light interferometry (WLI). These deflections agreed well with the results from the developed analytical and numerical analysis under various magnetic field strengths.;In the further research, more efforts were made to analyze the full three-dimensional deformation behavior of MSM thin films on a square glass sample (50x50x0.2 mm). With the magnetic field applied, the 2-d surface profile of the coated glass sample was measured by WLI. To better study the deformation of the sample coated with MSMs, a finite element method (FEM) and a theoretical model were developed to predict the deformation of the sample with local misfit strains. The results calculated form the FEM and the theoretical model agreed well with the experimental results.;Finally, some work was done on the NiCo substrate coated with MSMs to preliminarily verify its capability to hold the deformation after the external magnetic field was removed.
机译:天文望远镜的高质量成像系统需要创新,以消除或校正轻型光学镜面表面上的中空频率(MSF)波纹。当望远镜送入太空时,其发射质量是限制其收集区域的关键。因此,可以考虑使用轻巧的光学元件(100-150微米厚的电镀镍/钴或200-400微米厚的玻璃)。但是,薄的光学表面的表面轮廓无法抛光到极高的精度。相反,期望通过施加电压或磁场以驱动反射镜背面上的智能材料(压电或磁致伸缩材料)涂层来校正轮廓。在此过程中,通过二维表面上的局部应力进行表面轮廓校正非常具有挑战性。校正后对表面轮廓的测量和理论预测都进行了研究;作为开发用于预测涂层玻璃带样品(20x5x0.1 mm)变形的工具的第一步,一种商业磁性智能材料(MSM)通过磁控溅射法将)沉积在样品上。建立了一种实验装置,以通过Zygo NewView白光干涉仪(WLI)在外部磁场下测量这些涂层样品的变形。这些挠度与在各种磁场强度下进行的分析和数值分析得出的结果吻合得很好。在进一步的研究中,做出了更多的努力来分析方形玻璃样品(50x50x0)上MSM薄膜的完整三维变形行为。 .2毫米)。施加磁场后,通过WLI测量镀膜玻璃样品的二维表面轮廓。为了更好地研究涂有MSM的样品的变形,建立了有限元方法(FEM)和理论模型来预测具有局部失配应变的样品的变形。通过有限元法和理论模型计算得到的结果与实验结果吻合良好。最后,对涂覆有MSM的NiCo基体进行了一些工作,以初步验证其在去除外部磁场后能够保持变形的能力。

著录项

  • 作者

    Wang, Xiaoli.;

  • 作者单位

    Northwestern University.;

  • 授予单位 Northwestern University.;
  • 学科 Mechanical engineering.;Mechanics.;Optics.
  • 学位 Ph.D.
  • 年度 2016
  • 页码 165 p.
  • 总页数 165
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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