光束组合器是光学综合孔径望远镜阵重要技术组成部分之一。
Beam combiner is the key part of optical aperture synthesis telescope array.
光学综合孔径成像技术是高分辨率光学成像技术方法之一，它实现并应用于天文观测研究。
Optical aperture synthesis imaging technology is one of optical imaging technology methods for high observation resolution.
闭合相位技术、U _ V覆盖技术和像重构技术是光学综合孔径干涉成像的三个关键技术。
Closure phase technology, U-V coverage technology and image reconstruction technology are three key technologies for optical synthesis aperture image.
闭合相位技术、U - V覆盖技术和像重构技术是光学综合孔径干涉成像的三个关键技术。
Closure phase technology, U-V coverage technology and image reconstruction technology are three key technologies for optical aperture synthesis image.
从惠更斯—菲涅耳原理出发，根据光学综合成像像面干涉的实际情况，建立了符合实际的光学综合孔径像面干涉数学模型；
According to image plane interference status of optical aperture synthesis(OAS) and Huyges Fresnel theory, a mathematical method is set up which fits with the true condition.
由多个小口径成像系统通过特殊排列综合而成的光学稀疏孔径系统是实现高分辨率天文目标成像观测的一种新方法。
Optical sparse-aperture system can be designed to obtain high resolution in astronomical object imaging. It is a particular array synthesized by several small filled imaging systems.
初步的实验结果验证了综合孔径辐射计光学实时信号处理的可行性及系统设计的正确性。
The primary experiment results validate that feasibility of real-time signal processing for synthetic aperture microwave radiometer and the correctness of the system design.
初步的实验结果验证了综合孔径辐射计光学实时信号处理的可行性及系统设计的正确性。
The primary experiment results validate that feasibility of real-time signal processing for synthetic aperture microwave radiometer and the correctness of the system design.
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