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INTERFEROMETRIC IMAGE ACQUISITION AND RECONSTRUCTION

机译:干涉仪图像采集和重建

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摘要

To obtain an image of an exo-solar planet, a space-borne interferometric imaging system consisting of free-flying spacecraft (telescopes) is considered. A brief account of the underlying mathematics of image synthesis via interferometry is reviewed. A measure of image quality is adopted based on the estimated image and the Modulation Transfer Function (MTF) of the entire formation. The coordination of the formation is required to execute optimal formational maneuvers that correlate to a coverage problem; in which the resolution disc in the spatial frequency plane must be entirely covered via coverage discs that represent the mutual light measurements from pairs of telescopes. We formulate and find the necessary conditions of optimality for the coverage task via the coordinated maneuvers of the spacecraft formation. Minimum time bounds for achieving complete coverage are found. Finally, given the relative position data of the formation and using the measure of image quality to redirect the spacecraft maneuvers, we address the problem of accounting for the regions that are not completely covered in the resolution disc. We show the feasibility of using signal processing techniques to account for these regions of attenuation rather than have the formation reposition itself in order to achieve complete coverage.
机译:为了获得太阳系外行星的图像,考虑了由自由飞行的航天器(望远镜)组成的星载干涉成像系统。简要介绍了通过干涉法进行图像合成的基本数学方法。基于估计的图像和整个编队的调制传递函数(MTF),采用图像质量度量。需要进行编队协调才能执行与覆盖问题相关的最佳编队演习。其中必须通过覆盖圆盘完全覆盖空间频率平面中的分辨率圆盘,该覆盖圆盘代表来自望远镜对的互光测量值。我们通过航天器编队的协调演算来制定并找到覆盖任务的最优必要条件。找到实现完全覆盖的最小时间范围。最后,给定地层的相对位置数据并使用图像质量度量来重定向航天器操纵,我们解决了解决分辨率盘中未完全覆盖的区域的问题。我们展示了使用信号处理技术解决衰减的这些区域的可行性,而不是为了重新实现覆盖范围本身而对地层进行重新定位。

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