摘要
为了研究激光相干阵列在全大气层湍流中的成像能力,在全相位闭合等方法的基础上,利用HV57模型中的大气折射率结构常数来标定大气相干长度,通过当地风速和光路高度等参数计算了实验所在地等效整层大气湍流的水平传输距离,研制了Ф1.5 m等效孔径的激光相干发射阵列,对1.2 km远处物体进行了成像实验,成像分辨率达到了亚角秒级。验证了激光相干阵列成像系统对大气湍流影响的抑制作用和成像能力,可为未来研制实体激光相干阵列成像系统提供理论与技术支撑。
In order to study laser array in the whole atmosphere turbulence coherent imaging ability,on the basis of all phase method such as closure,the atmospheric refractive index structure constant of HV57 model is used to calibrate the atmospheric coherence length,through the local wind speed and light road height to calculate the experimental parameters,such as local equivalent whole layer of the atmospheric turbulence level transmission distance.A laser coherent emission array with a diameter of 1.5 m equivalent aperture is developed,and the imaging experiment of a 1.2 km distant object is carried out.The imaging resolution reaches sub-arcsecond level.It is verified that the laser coherent array imaging system can suppress the influence of atmospheric turbulence and provide theoretical and technical support for the development of solid laser coherent array imaging system in the future.
作者
张羽
李治国
刘辉
陈明徕
罗秀娟
马彩文
张怀利
ZHANG Yu;LI Zhiguo;LIU Hui;CHEN Minglai;LUO Xiujuan;MA Caiwen;ZHANG Huaili(Xi′an Institute of Optics and Precision Mechanics,Chinese Academy of Science,Xi′an 710119,China;Key Lab of Space Precision Measurement Technology,Chinese Academy of Science,Xi′an 710119,China;University of Chinese Academy of Science,Beijing 100084,China;Pilot National Laboratory for marine science and technology,Qingdao,Shandong 266200,China;Space Engineering University,Beijing 101499,China)
出处
《光子学报》
EI
CAS
CSCD
北大核心
2021年第12期49-59,共11页
Acta Photonica Sinica
基金
国家自然科学基金青年基金(No.61505248)。
关键词
激光相干阵列
傅里叶望远
主动照明成像
大气湍流
图像重构
Laser coherent array
Fourier telescope
Active illumination imaging
Atmospheric turbulence
Image reconstruction