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Analysis of Field-of-View of Optical Aperture Synthesis Imaging Interferometry

机译:光学孔径合成成像干涉仪的视场分析

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Interferometric imaging systems measure the complex visibility, which is the Fourier transform of the source brightness distribution, according to the van Cittert-Zernike theorem. Both the amplitude and phase of the visibility are needed to produce images of a complex object structure by Fourier inversion. In this paper, by using the generalized imaging theory of a diffraction-limited incoherent imaging system, the pinhole model and the circular aperture model of the interferometry are presented and derived. The approximate condition, which should be followed by optical aperture synthesis imaging interferometry, is obtained by comparing two models. Based on this condition, the angle of field-of-view (FOV) in the object space is analyzed and determined. At the good approximation, the FOV is about one-sixth of an Airy disk of a elementary aperture diffraction. Also the computer simulation results are presented and match the theoretical results very well. This suggests that the extremely high image resolution can be achieved in the interferometric imaging systems, but it generally has a very small field of view. Such imaging systems are suitable only for the astronomical application.
机译:根据van Cittert-Zernike定理,干涉成像系统可测量复杂的可见度,这是光源亮度分布的傅立叶变换。能见度的幅度和相位都需要通过傅立叶反演来产生复杂物体结构的图像。本文利用衍射极限非相干成像系统的广义成像理论,提出并推导了干涉测量的针孔模型和圆孔模型。通过比较两个模型,可以获得近似条件,随后应进行光学孔径合成成像干涉测量。基于此条件,分析并确定对象空间中的视角(FOV)。以良好的近似值,FOV约为基本孔径衍射的艾里斑的六分之一。并给出了计算机仿真结果,并与理论结果非常吻合。这表明在干涉成像系统中可以实现极高的图像分辨率,但是通常具有非常小的视野。这样的成像系统仅适用于天文应用。

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