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Fabrication processes for MEMS deformable mirrors in the next generation telescope instruments.

机译:下一代望远镜仪器中MEMS可变形反射镜的制造工艺。

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摘要

This dissertation advances three critical technology areas at the frontier of research for micro electro-mechanical systems (MEMS) deformable minors (DMs) needed for next generation telescopes (NGTs). High actuator-count MEMS deformable minors are needed for future ground-based large astronomical telescopes. Scaling up the current MEMS DMs to unprecedented numbers of independent actuators---up to 10,000 on a single DM---will require new electrical connection architecture for the actuators in order to replace the wire-bonded scheme that has been used to date. A through-wafer via interconnection fabrication process for MEMS DMs is developed to offer a path to transform the frontier of high actuator count MEMS micromirrors.;In a class of NGTs instrument known as the Multi-Object Adaptive Optics (MOAO), the correction made by the DM of the wavefront phase error over the entire telescope field view is not accessible to the sensing unit. To achieve compensation, precise, single step "open-loop" commands must be developed for the DM. Due to the nonlinear relationship between applied voltage and actuation displacement at each actuator, and the mechanical coupling among actuators through the mirror membrane, such open-loop control is a formidable task. A combination of mirror surface modeling and sparse actuator empirical calibration is used to demonstrate open-loop control of MEMS deformable minors to the accuracy of closed-loop control over the entire available DM stroke. Shapes at the limit of achievable minor spatial frequencies with up to 2.5microm amplitudes have been achieved within 20nm RMS error accuracy of closed-loop control. The calibration of a single actuator to be used for predicting shapes results in an additional 14nm RMS surface error compared to parallel calibration of all actuators in the deformable minor.;The ubiquitous reflective coatings for MEMS deformable minors are gold and aluminum. Emerging adaptive optics application require broadband optical coatings usable from the near visible to near infrared, i.e. silver. Many of the reflective coatings of interest have high stress resulting in added curvature on deformable mirror. A thick epitaxial polysilicon MEMS mirror that can tolerate thicker reflective coatings with higher stresses has been fabricated. A thin film deposition process to counteract the stress in the reflective coating was also developed. The deformable mirror has low stress (∼10 nm flatness), high reflectivity (>95%), 1024 actuated segments, that is usable over a wavelength range from visible to IR with a protective layer for the silver coating and stress-reducing layer between the silver and mirror layer to obtain the desired flatness.
机译:本文在下一代望远镜(NGT)所需的微机电系统(MEMS)可变形镜(DM)的研究前沿推进了三个关键技术领域。未来的地面大型天文望远镜需要高致动器数的MEMS可变形镜。将当前的MEMS DM扩展到空前数量的独立执行器-在单个DM上最多可达到10,000-将需要用于执行器的新电连接架构,以取代迄今使用的引线键合方案。开发了用于MEMS DM的晶圆通孔互连制造工艺,以提供一条途径来转变高致动器数MEMS微镜的前沿。在一种称为多目标自适应光学(MOAO)的NGT类仪器中,进行了校正DM无法检测整个望远镜视野范围内的波前相位误差。为了实现补偿,必须为DM开发精确的单步“开环”命令。由于每个致动器上施加的电压与致动位移之间的非线性关系,以及致动器之间通过镜膜的机械耦合,这种开环控制是一项艰巨的任务。镜面建模和稀疏执行器经验性校准的结合用于演示MEMS变形镜的开环控制,以达到整个可用DM行程的闭环控制精度。在闭环控制的20nm RMS误差精度内,可达到的最小空间频率极限为2.5μm。与可变形镜中的所有致动器的平行校准相比,用于预测形状的单个致动器的校准会导致额外的14nm RMS表面误差。MEMS可变形镜的无处不在的反射涂层是金和铝。新兴的自适应光学应用需要使用从近可见光到近红外的宽带光学镀膜,即银。许多令人关注的反射涂层具有高应力,导致可变形反射镜上的曲率增加。已经制造了可以耐受较高应力的较厚反射涂层的厚外延多晶硅MEMS镜。还开发了一种薄膜沉积工艺来抵消反射涂层中的应力。可变形反射镜具有低应力(平坦度约为10 nm),高反射率(> 95%),1024个驱动段,可在从可见光到IR的波长范围内使用,并具有用于银涂层的保护层和介于两者之间的应力减小层银和镜面层以获得所需的平整度。

著录项

  • 作者

    Diouf, Alioune.;

  • 作者单位

    Boston University.;

  • 授予单位 Boston University.;
  • 学科 Engineering Mechanical.;Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 2010
  • 页码 163 p.
  • 总页数 163
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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