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Long-baseline optical fiber interferometer instruments and science

机译:长基线光纤干涉仪和科学

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Developments of fiber linked optical interferometer are reported. This interferometer is a part of MIRA-I.2 interferometer (Mitaka InfraRed and optical Array). MIRA-I.2 is an optical interferometer with a 30 meters long baseline. It consists of two 30cm siderostats, tip-tilt mirrors, vacuum pipes delay lines and detectors. We plan to use two 60 meters long polarization-maintaining fibers for arms of the interferometer, instead of vacuum pipes. The developments include dispersion and polarization compensation of fiber and fiber injection module. In laboratory experiments, dispersion compensation succeeded. The fringe visibility was 0.93 for wide-band, where the central wavelength of light was 700nm, and bandwidth was 200nm, while 0.95 with a He-Ne laser. We used BK7 glass wedge for dispersion compensation. About fiber injection module, basic optical design has completed. The results of our fiber interferometer could contribute to OHANA (Optical Hawaiian Array for Nanoradian Astronomy) project. We present new science targets, white dwarves and T Tauri stars, and an 800m delayline concept in CFHT for the project.
机译:报道了光纤连接光学干涉仪的发展。该干涉仪是MIRA-1.2干涉仪(三鹰红外和光学阵列)的一部分。 MIRA-1.2是一种光学干涉仪,基线长30米。它由两个30厘米的恒温器,倾斜镜,真空管延迟线和检测器组成。我们计划将两根60米长的偏振保持光纤用于干涉仪的支臂,而不是用于真空管。这些发展包括光纤和光纤注入模块的色散和偏振补偿。在实验室实验中,色散补偿成功。宽带的条纹可见度为0.93,其中光的中心波长为700nm,带宽为200nm,而氦氖激光器的条纹可见度为0.95。我们使用BK7玻璃楔进行色散补偿。关于光纤注入模块,基本的光学设计已经完成。我们的光纤干涉仪的结果可能有助于OHANA(纳米弧度天文光学夏威夷阵列)项目。我们为该项目提出了新的科学目标,白矮星和T Tauri星,以及CFHT中的800m延迟线概念。

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