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Resolving fringe ambiguities of a wide-field Michelson interferometer using visibility measurements of a noncollimated laser beam

机译:使用非准直激光束的可见性测量来解决宽视场迈克尔逊干涉仪的条纹模糊性

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An actively stabilized interferometer with a constant optical path difference is a key element in long-term astronomical observation, and resolving interference fringe ambiguities is important to produce high-precision results for the long term. We report a simple and reliable method of resolving fringe ambiguities of a wide-field Michelson interferometer by measuring the interference visibility of a noncollimated single-frequency laser beam. Theoretical analysis shows that the interference visibility is sensitive to a subfringe phase shift, and a wide range of beam arrangements is suitable for real implementation. In an experimental demonstration, a Michelson interferometer has an optical path difference of 7 mm and a converging monitoring beam has a numerical aperture of 0.045 with an incidental angle of 17 deg. The resolution of visibility measurements corresponds to approx1/16 fringe in the interferometer phase shift. The fringe ambiguity-free region is extended over a range of approx100 fringes.
机译:具有恒定光程差的有源稳定干涉仪是长期天文观测的关键因素,解决干涉条纹的歧义对于长期获得高精度结果很重要。我们报告了一种简单可靠的方法,通过测量非准直单频激光束的干扰可见度来解决宽视场迈克尔逊干涉仪的条纹模糊性。理论分析表明,干扰可见度对亚条纹相移很敏感,并且宽范围的光束布置都适合实际实现。在实验演示中,迈克尔逊干涉仪的光程差为7 mm,会聚的监视光束的数值孔​​径为0.045,入射角为17度。可见性测量的分辨率对应于干涉仪相移中的大约1/16条纹。无条纹的模糊区域扩展到大约100个条纹的范围。

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