Abstract:The vast Moon surface, lower thermal environment, predictable orbit, and long distance of Earth-Moon centroid have provided long-term, large-scale, unique, stable, and many other advantages for Moon-based Earth observation, including the synthetic aperture radar interferometry. Compared with the space-borne method, the Moon-based cross-track interferometry (MB-CTI) that works in one transmitter dual-receiver mode undoubtedly not only has larger coverage at single gaze but also has stable baseline. Relatively s… Show more
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