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A Micromachined Deformable Mirror for Adaptive Optics

机译:用于自适应光学的微机械变形镜

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摘要

The application of adaptive optics in astronomy requires increasingly compact deformable optical components with a high density of actuators, able to provide strokes of several micrometers. The main problem of the use of adaptive optics in more mainstream areas is the cost, the size and consequently the weight of the system. This paper presents the design and the results obtained with the deformable mirror under development. The system will have a continuous reflective membrane of 1 cm~2 driven by 64 closing gap actuators operating in contact. In the following this type of actuators is called "zipping actuators". Applying 100 V to some 800 μm wide zipping actuators results in an electrostatic force of 100 μN and a mirror displacement of 6 μm. Recent tests of the electric behaviour show linearity between applied tension and resulting displacement as well as a good reproducibility. We also present analysis and results obtained on silicon or polymer (BCB) membranes which have to be attached on the actuator array. A preliminary assembled component made of one actuator sealed to a 5 um thick polymer 5 x 5 mm~2 (BCB) membrane has demonstrated the feasibility of deforming such a small membrane by 3 μm, which is very promising.
机译:自适应光学器件在天文学中的应用需要具有高密度致动器的,越来越紧凑的可变形光学组件,该致动器能够提供几微米的行程。在更主流的领域中使用自适应光学器件的主要问题是系统的成本,尺寸和重量。本文介绍了正在开发中的可变形反射镜的设计和获得的结果。该系统将具有1 cm〜2的连续反射膜,该反射膜由64个闭合间隙致动器以接触方式驱动。在下文中,这种类型的致动器称为“拉链致动器”。将100 V电压施加到大约800μm宽的拉链致动器上,会产生100μN的静电力和6μm的镜面位移。最近对电性能的测试表明,施加的张力与所产生的位移之间具有线性关系,并具有良好的可重复性。我们还介绍了必须附着在执行器阵列上的硅或聚合物(BCB)膜的分析结果。由一个致动器密封到5 um厚的聚合物5 x 5 mm〜2(BCB)膜制成的预组装组件已证明将这种小膜变形3μm的可行性,这是非常有希望的。

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