The imaging of Earth-orbiting objects using large aperture telescopes equipped with adaptive optics is a critical component of Space Situational Awareness. Unfortunately, due to limitations in the adaptive optics, compensation of the wave-front distortions imparted by the Earth's turbulent atmosphere is incomplete. Achieving the quality of imagery necessary for high confidence monitoring of the near space environment, therefore requires the use of image restoration methods to remove the unconnected component ...
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