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Optimized setup for active compensation of distortions for interferometric techniques onboard the International Space Station

机译:国际空间站船上干涉技术的活动补偿优化设置

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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?C to 35?C 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:正在开发哥伦布轨道设施的流体科学实验室(FSL)的主要部分是光学诊断模块(ODM)。它提供了在不同干涉技术的帮助下提供了流体科学实验的定量测量。这些方法的组装基于Mach-Zehnder干涉仪。由于FSL上的就业,这种干涉仪的设计具有关于体积,质量,模块化,运营需求以及具有干涉仪的热和机械扭曲的环境的若干要求。在偏见时,干涉仪设计,以防止由于外部扭曲和补偿它。该设计基于简化的Hartmann传感器,并检测波前倾斜和曲率误差。通过压电驱动光学组件实现这些误差的主动补偿,并实时操作,但不能完全补偿曲率误差。在本文中,我们描述了修改的设置的构造,该改进的设置可以为计划的应用程序的温度范围内的波前倾斜和曲率误差补偿到35°C至35Ω·c。新的设计更简单,因此被动稳定性也更好。对新设置进行热试验结果并显示出新的主动稳定干涉仪的增强稳定性。

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