设置在月球的巨大的光学干涉法望远镜阵列，将探测太阳系周围其他星球，而且对它们的环境特征和是否具备生存条件进行分析。
Very large optical interferometry telescope arrays on the Moon will not only detect planets around other stars, but also analyze their atmospheres and characterize their habitability.
这是利用望远镜展示名为“牛顿圈”的光学效应，折射光线彼此干涉，形成了这些条纹。
This is the view through a telescope demonstrating the optical effect known as Newton's Rings, whereby reflected light rays interfere with one another and produce a pattern.
使用一种名为电子实时甚长基干涉测量法(e -VLBI)的技术，多个望远镜可以同时观测同一个目标。
Using an astronomical technique called electronic, real-time Very Long Baseline Interferometry, or e-VLBI, participating telescopes will observe the same object simultaneously.
天文学家使用欧洲南方天文台位于智利的超大规模望远镜干涉仪对一个年轻的星体对象(YSO)进行了红外线观察，名为IRAS13481- 6124。
Astronomers used the Very Large Telescope Interferometer of the European Southern Observatory in Chile to make infrared observations of a young stellar object (YSO) called IRAS 13481-6124.
天文学家使用欧洲南方天文台位于智利的超大规模望远镜干涉仪对一个年轻的星体对象(YSO)进行了红外线观察，名为IRAS13481 - 6124。
Astronomers used the Very Large Telescope Interferometer of the European Southern Observatory in Chile to make infrared observations of a young stellar object (YSO) called.
例如，这台叫做空间干涉任务执行者的天文望远镜，将在下一个十年的早些时候发射，这台望远镜由一系列30英尺的望远镜阵列组成。
For example, the Space Interferometry Mission (SIM), to be launched early in the next decade, consists of multiple telescopes placed along a 30 foot structure.
在近红外波段，自适应光学和干涉术已在大望远镜上获得成功。
In near Infrared waveband the adaptive optics and interferometry have been used in large telescopes successfully.
望远镜技术和光干涉技术的结合是提高望远镜分辨率的方法之一。
Combination of optical interference technology with telescope technology is one of the ways to raise the resolution of a telescope.
针对大口径望远镜拼接式主镜，提出一种基于迈克耳孙干涉原理的低相干光源干涉检测系统。
The concrete structure of the interferometric detection system with the low-coherence source was presented, and the detection principle of the interferometric detection system was narrated.
针对大口径望远镜拼接式主镜，提出一种基于迈克耳孙干涉原理的低相干光源干涉检测系统。
The concrete structure of the interferometric detection system with the low-coherence source was presented, and the detection principle of the interferometric detection system was narrated.
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