Optical-Radar Imaging Of Scale Models For Studies In Asteroid Astronomy

During the past five years, delay-Doppler radar has become the primary technique for studying the structure of Earth-crossing asteroids. None of these objects has yet been visited by spacecraft, so ground-truth test cases are lacking. A laboratory system is described that provides optical-radar images at 0.1-mm resolution. These data are analogous to the highest-resolution asteroid radar images currently available and provided realistic test cases for developing signal-processing techniques. The system can be thought of as a 1/188,000 scale model of the Arecibo radar, or a 1/52,800 scale model of the Goldstone radar. (C) 1995 Optical Society of America


Published in:
Optics Letters, 20, 2327-2329
Year:
1995
Laboratories:




 Record created 2010-11-25, last modified 2018-03-17

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