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Optimized Setup for Active Compensation of Distortions for Interferometric Techniques onboard the International Space Station

机译:针对国际空间站上的干涉技术进行畸变的主动补偿的优化设置

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The main part of the Fluid Science Laboratory (FSL) that is under development for the Columbus Orbital Facility is the Optical Diagnosis Module (ODM). It provides quantitative measurements of fluid science experiments with the help of different interferometric techniques. The assembly of these methods is based on a Mach-Zehnder-Interferometer. Because of the employment on the FSL the design of this interferometer has several requirements regarding volume, mass, modularity, operational needs and especially an environment with thermal and mechanical distortions of the interferometer. At BIAS an interferometer was designed that detects the misalignment due to external distortions and compensates it. The design is based on a simplified Hartmann-Sensor and detects wavefront tilt and curvature errors. The active compensation of these errors is realized by piezoelectric driven optical components and operates in realtime but cannot compensate the curvature errors completely. In this paper we describe the construction of a modified setup that compensates wavefront tilt and curvature errors in a temperature range from 15℃ to 35℃ sufficiently for the planned applications. The new design is substantial simpler and hence the passive stability is better as well. The results of thermal tests with the new setup are demonstrated and show the enhanced stability of the new actively stabilized interferometer.
机译:哥伦布轨道设施正在开发的流体科学实验室(FSL)的主要部分是光学诊断模块(ODM)。它借助不同的干涉测量技术提供了流体科学实验的定量测量。这些方法的组装基于马赫曾德尔干涉仪。由于在FSL上的使用,该干涉仪的设计对体积,质量,模块性,操作需求,特别是在干涉仪的热和机械变形的环境方面有一些要求。在BIAS,设计了一种干涉仪,用于检测由于外部畸变引起的未对准并进行补偿。该设计基于简化的Hartmann传感器,可检测波前倾斜和曲率误差。这些误差的主动补偿是通过压电驱动的光学组件实现的,并且可以实时运行,但无法完全补偿曲率误差。在本文中,我们描述了一种经过改进的装置的构造,该构造可以充分补偿计划应用中在15℃至35℃温度范围内的波前倾斜和曲率误差。新设计实质上更简单,因此被动稳定性也更好。演示了使用新设置的热测试结果,并显示了新型有源稳定干涉仪的增强稳定性。

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