Interferometric image fusion: interferometry in space

R. Lyon, J. Dorband, G. Solyar, U. Ranawake
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Abstract

Image fusion and information extraction from multiple spacecraft can occur after each image is sampled and digitized. A more tantalizing, but difficult, approach would be to optically phase multiple spacecraft flying in formation. Phasing of multiple spacecraft allows for coherent addition of imagery resulting in an optical system with a synthetic aperture as large as distance between the spacecraft. Thus, space based optical imaging systems approaching 100's of meters could theoretically be achieved; ultimately allowing for resolution of the solar disks of stars and resolution of extra-solar planets around these stars. The methods and techniques for systems of this type, as well as a number of optical testbeds for proof of principle and validation of the methods are currently under study at NASA Goddard Space Flight Center. In this work we give an overview of the underlying principles, the technology required and the state of development of the various testbeds involved.
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干涉图像融合:空间干涉测量
对每幅图像进行采样和数字化处理后,可以实现多航天器图像的融合和信息提取。一种更诱人但更困难的方法是光学相位多个航天器在编队中飞行。多个航天器的相位允许图像的相干添加,从而形成一个光学系统,其合成孔径与航天器之间的距离一样大。因此,空间光学成像系统接近100米理论上可以实现;最终使恒星的太阳盘和围绕这些恒星的太阳系外行星的分辨率得以实现。美国宇航局戈达德太空飞行中心目前正在研究这种类型系统的方法和技术,以及一些用于证明原理和验证方法的光学试验台。在这项工作中,我们概述了基本原理,所需的技术以及所涉及的各种试验台的开发状态。
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