2008
DOI: 10.3788/aos20082806.1197
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Synthetic-Aperture Ladar (Ⅱ): Spatial Phase Biased Telescope for Transmitting Antenna

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Cited by 3 publications
(3 citation statements)
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“…The three target points of simulation are shown in Fig.2: the coordinates of the points in the target plane are (5,5), (0, 0), (-5, -5), and the coordinates in the vertical plane are (3.535, 5, 3.535), (0, 0, 0), (-3.535, -5, -3.535). The delay times of the points are 0.158μs, 0.156μs, 0.154μs.…”
Section: Simulationmentioning
confidence: 99%
“…The three target points of simulation are shown in Fig.2: the coordinates of the points in the target plane are (5,5), (0, 0), (-5, -5), and the coordinates in the vertical plane are (3.535, 5, 3.535), (0, 0, 0), (-3.535, -5, -3.535). The delay times of the points are 0.158μs, 0.156μs, 0.154μs.…”
Section: Simulationmentioning
confidence: 99%
“…Pro. Liren Liu analyzed the optical characters of SAIL in space domain, and redefined the imaging azimuth and range resolutions in terms of the idea of optical imaging by a lens [6][7][8][9][10][11][12] . Directed by these analyses, we designed a multi-purpose SAIL demonstrator based on free-space optics to experimentally investigate and theoretically analyze the beam diffraction properties, antenna function, imaging resolution and signal processing algorithm of SAIL, besides, a laboratory-scaled SAIL system were built to verify the principle of design, and a primary experimental results were given [13] .…”
Section: Introductionmentioning
confidence: 99%
“…Liren Liu analyzed the optical characters of SAIL in space domain, and redefined the imaging azimuth and range resolutions in terms of the idea of optical imaging by a lens. [5][6][7][8][9][10] In this research, a synthetic aperture imaging ladar (SAIL) demonstrator is designed and being fabricated to experimentally investigate and theoretically analyze the beam diffraction properties, antenna function, imaging resolution and signal processing algorithm of SAIL. Such a multi-purpose SAIL demonstrator has the following design features: (1) A unified structure of telescope antenna has a big telescope of φ300mm aperture followed by a circulated duplex of a tunable secondary telescope to transmit an illuminating wavefront of needed spatial quadratic phase and of a defocused 4-f receiver to compensate the wavefront aberration of echo for a correct and efficient heterodyne detection, thus by tuning the secondary telescope not only the far-filed but also the near-field diffraction can be physically realized.…”
Section: Introductionmentioning
confidence: 99%