作者单位
摘要
四川师范大学物理与电子工程学院, 四川 成都 610068
采用空域滤波方法和海洋湍流功率谱, 编制了海洋湍流中扩展物体漫反射光成像的模拟仿真程序, 研究了成像质量与海洋湍流参数和接收孔径之间的关系。研究发现, 随着海水湍流功率谱中由温度引起的海水折射率变化与由盐度变化引起的海水折射率变化的比率的增大, 海水温度方差耗散率的增大, 以及单位质量海水动能耗散率的减小, 海洋湍流的可见参数减小, 成像质量变差。该数值模拟方法为研究海洋湍流中扩展物体的漫反射光成像提供了一种可行、正确的方法。
海洋光学 湍流介质中成像 海洋湍流 漫反射 扩展物体 数值模拟 
中国激光
2017, 44(11): 1105001
Author Affiliations
Abstract
Key Laboratory of Space Laser Communication and Detection Technology, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai 201800, China
We present a tabletop-scale spotlight-mode down-looking synthetic aperture imaging ladar (DL SAIL) demonstrator, which is performed by a collimator with 10 m focal length to simulate the far-field optical field. A specular-point target and a diffuse-reflection target have been used for resolution analysis and 2D imaging, respectively. The experimental result is in agreement with the theoretical design. The experiment setup is capable of simulating a real application scenario for further study. This Letter is focused on the proposition and implementation of spotlight-mode DL SAIL.
100.2000 Digital image processing 100.3010 Image reconstruction techniques 110.0115 Imaging through turbulent media 280.6730 Synthetic aperture radar 
Chinese Optics Letters
2015, 13(9): 091001
Changhui Rao 1,2Lei Zhu 1,2,*Xuejun Rao 1,2Lanqiang Zhang 1,2[ ... ]Zhiyong Wang 1,2,3
Author Affiliations
Abstract
1 The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China
2 The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
3 University of Chinese Academy of Sciences, Beijing 100049, China
A second generation solar adaptive optics (AO) system is built and installed at the 1-m New Vacuum Solar Telescope (NVST) of the Fuxian Solar Observatory (FSO) in 2015. The AO high-order correction system consists of a 151-element deformable mirror (DM), a correlating Shack–Hartmann (SH) wavefront sensor (WFS) with a 3500 Hz frame rate, and a real-time controller. The system saw first light on Mar. 16, 2015. The simultaneous high-resolution photosphere and chromosphere images with AO are obtained. The on-sky observational results show that the contrast and resolution of the images are apparently improved after the wavefront correction by AO.
010.1080 Active or adoptive optics 110.1080 Active or adoptive optics 110.0115 Imaging through turbulent media 
Chinese Optics Letters
2015, 13(12): 120101

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