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基于渥拉斯顿棱镜的单路实时偏振成像系统设计

许洁 刘飞 刘杰涛 王娇阳 韩平丽 周淙浩 邵晓鹏

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基于渥拉斯顿棱镜的单路实时偏振成像系统设计

许洁, 刘飞, 刘杰涛, 王娇阳, 韩平丽, 周淙浩, 邵晓鹏

A design of real-time unipath polarization imaging system based on Wollaston prism

Xu Jie, Liu Fei, Liu Jie-Tao, Wang Jiao-Yang, Han Ping-Li, Zhou Cong-Hao, Shao Xiao-Peng
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  • 针对非实时成像中动态场景偏振探测产生的虚假偏振信息问题, 充分利用渥拉斯顿棱镜(Wollaston Prism, WP)的分光特性, 设计了一种新型实时偏振成像系统. 采用像方远心望远透镜系统、准直透镜系统并设计匹配的成像镜系统, 在单探测器阵列上同时获取偏振态相互垂直的两幅偏振图像. 通过全系统联动设计与优化, 系统的调制传递函数(modulation transfer function, MTF)在截止频率处不小于0.55, 全系统弥散斑均方根半径(root-mean-square, RMS)小于5.3 m, 即小于探测器像元尺寸, 满足成像设计要求. 仿真结果证明该成像系统可有效解决传统分振幅偏振成像系统的实时性差的不足, 分孔径偏振成像系统的能量利用率和分辨率低的问题以及偏振焦平面方法中光路串扰的缺陷, 应用前景广阔.
    A real-time polarization imaging system employing the Wollaston prism and a single charge-coupled device(CCD) chip covering a wavelength range of 400 nm-650 nm is proposed to avoid the false polarization information from dynamic scenes in non-real-time polarization detection imaging method. An architecture consisting of telescope lens, collimation lens, Wollaston prism, the imaging lens and a single CCD chip is employed in the system. The telescope lens is used to focus the incoming light on an intermediate image. And after collimation, the beam is angularly separated by the Wollaston prism. Two beams corresponding to ordinary light and extraordinary light are subsequently focused on the CCD plane via the imaging lens. The telescope lens is designed to have a telecentric structure in the imaging space, and the invert of which is used as the collimation lens, the completely symmetrical structure design is used to reduce the influence of aberrations. More abundant details from this system can be obtained by using matched image post-processing strategy, which is beneficial to high-quality target detection with enhanced working distance and improved environment adaptability. After joint-designing and optimization, the system modulation transfer function (MTF) value at cut-off frequency is higher than 0.55, and the root-mean-square (RMS) radius of the system is less than 5.3 m, which is smaller than the pixel size of the CCD detector. Additionally, the lateral chromatic aberration of the system is much smaller than the diameter of airy disk, and the absolute values of all kinds of aberrations are kept smaller than 0.02 at the same time. The calculation results show that all the aberrations are mostly corrected. The system imaging is numerically modeled and analyzed, and it is demonstrated that two intensity images with perpendicular polarization states appear adjacently on the CCD plane simultaneously in the imaging simulation. One image is formed with the fraction of the backscattered light polarized parallelly to the incident light, and the other with light polarized orthogonally to the incidence, indicating that the expected design is accomplished. Compared with the traditional amplitude-split polarization imaging system, the proposed real-time polarization imaging system shows that the improved performance for real-time detection with promoted power efficiency, spatial resolution, and the light crosstalk in focal plane is well handled. Moreover, the joint design of the whole system can compensate for the distortion aberration in the vertical direction of the CCD detector, which means that a further improvement of image quality can be expected. The proposed system has a promising perspective in the fields of underwater imaging detection, astronomical observation, remote sensing, biological tissues inspection, and environmental monitoring.
      通信作者: 邵晓鹏, xpshao@xidian.edu.cn
    • 基金项目: 国家自然科学基金(批准号: 61575154)和中国国防科技预研项目(批准号: 90406150009)资助的课题.
      Corresponding author: Shao Xiao-Peng, xpshao@xidian.edu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 61575154) and the National Defense Foundation of China (Grant No. 90406150009).
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  • [1]

    Cao X, Roy G, Roy N, Bernier R 2009 Appl. Opt. 48 004130

    [2]

    He H H, Zeng N, Liao R, Ma H 2015 Prog. Biochem. Biophys. 42 419 (in Chinese) [何宏辉, 曾楠, 廖然, 马辉 2015 生物化学与生物物理进展 42 419]

    [3]

    Makita S, Yasuno Y, Endo T, Itoh M, Yatagai T 2006 Appl. Opt. 45 001142

    [4]

    Zeng N, Jiang X, Gao Q, He Y H, Ma H 2009 Appl. Opt. 48 006734

    [5]

    Langlois M, Dohlen K, Augereau J C, Mouillet D, Boccaletti A, Schmid H M 2010 Proc. of SPIE 7735 857049

    [6]

    Han J F, Yang K C, Xia M, Sun L Y, Cheng Z, Liu H, Ye J W 2015 Appl. Opt. 54 003294

    [7]

    Liu F, Shao X P, Xiang L B, Gao Y, Han P L, Wang L 2015 Chin. Phys. Lett 32 114203

    [8]

    Liu F, Cao L, Shao X P, Han P L, Xiang L B 2015 Appl. Opt. 54 008116

    [9]

    Mu T K, Zhang C M, Li Q W, Wei Y T, Chen Q Y, Ja C L 2007 Opt. Express 15 005827

    [10]

    Matchko R M, Gerhart G R 2008 Opt. Eng. 47 016001

    [11]

    Li C L, Sun X B, Wang H, Wei W, Shu C M 2014 Acta Opt. Sin. 34 0412004 (in Chinese) [李翠丽, 孙晓兵, 王涵, 韦玮, 舒存铭2014 光学学报34 0412004]

    [12]

    Yuan Y L, Zheng X B, Wu H Y, Meng F G, Kang Q, Chen L G, Li J J, Zou P 2014 Acta Opt. Sin. 34 1223001 (in Chinese) [袁银麟, 郑小兵, 吴浩宇, 孟凡刚, 康晴, 陈立刚, 李健军, 邹鹏2014 光学学报34 1223001]

    [13]

    He H C, Ji Y Q, Zhou J K 2013 Acta Opt. Sin. 33 0622005 (in Chinese) [贺虎成, 季轶群, 周建康2013 光学学报33 0622005]

    [14]

    Lindlein N, Quabis S, Peschel U, Leuchs G 2007 Opt. Express 15 5827

    [15]

    Zhao J S 2013 Infrared Technology 35 0743 (in Chinese) [赵劲松 2013 红外技术 35 0743]

    [16]

    Weijers A L, Brug H V, Frankena H J 1998 Appl. Opt. 37 005150

    [17]

    Bnire A, Alouini M, Goudail F, Dolfi D 2009 Appl. Opt. 48 005764

    [18]

    Zhu H C, Nan Y J, Yun M J 2012Acta Opt. Sin. 32 0623002 (in Chinese) [朱化凤, 南玉杰, 云茂金 2012 光学学报 32 0623002]

    [19]

    Sun J X, Pan G Q, Liu Y 2013 Acta Phys. Sin. 62 094203 (in Chinese) [孙金霞, 潘国庆, 刘英 2013 物理学报 62 094203]

    [20]

    Wu Z Y, Zhang Q C 2011 Acta Opt. Sin. 31 0412011 (in Chinese) [吴启云, 张启灿 2011 光学学报 31 0412011]

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出版历程
  • 收稿日期:  2016-01-30
  • 修回日期:  2016-04-27
  • 刊出日期:  2016-07-05

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