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BALANCING OPTICAL PATH LENGTHS IN BROADBAND FIBER INTERFEROMETERS

机译:宽带光纤干涉仪中的平衡光路长度

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A simple model is used to show that control of dispersion in an all-fiber stellar interferometer is feasible. From the results we assume that an interferometer control system is available in which both temperature and strain are used to balance the interferometer. Within the restriction of a single polarization mode, it is shown that vacuum path errors before the coupling of starlight into the fibers as well as fiber-length differences and environmental differences between two fibers can be corrected to high order. [References: 17]
机译:使用一个简单的模型可以证明在全光纤恒星干涉仪中控制色散是可行的。根据结果​​,我们假设可以使用干涉仪控制系统,其中温度和应变均用于平衡干涉仪。在单偏振模式的限制内,已表明可以将星光耦合到光纤之前的真空路径误差以及两个光纤之间的光纤长度差异和环境差异校正为高阶。 [参考:17]

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