光学 精密工程, 2017, 25 (6): 1679, 网络出版: 2017-07-10   

多传感器的天文标定与空间配准

Astronomical calibration and spatial registration of multi-sensor
作者单位
1 北京理工大学 光电学院, 北京 100081
2 装备学院 光电装备系, 北京 101416
3 北京理工大学 光电学院, 北京 10008
摘要
为了实现共平台的多个空间观测成像系统的空间配准, 对多个相机进行天文标定和姿态测量, 提出一种基于星图模拟的星图识别和姿态解算算法。首先, 建立共平台的多传感器天文观测模型, 并产生模拟星图, 将星点之间的特征转换为图像特征; 其次, 根据四边形对角线的共线不变性特征, 对相机观测星图和模拟星图进行特征匹配, 提取相机内参数的初始值; 然后, 利用星点坐标矩阵奇异值不变性, 自动匹配剩余星点并求解姿态矩阵的初始值; 最后, 对相机内参数和姿态矩阵进行非线性优化求解。实验结果表明, 在未精确标定光学系统内外参数的情况下, 星点正确识别率大于97.4%, 相机像元角分辨率为3.9"×3.4", 最后计算得出的投影误差低于1个像素, 满足多传感器空间观测系统空间配准的精度和鲁棒性要求。
Abstract
In order to achieve the spatial registration of multi-sensor on the same platform for astronomical observation, a camera calibration and attitude measurement algorithm was proposed based on the star image simulation which includes four steps. Firstly, according to star observation model and star catalogue, the simulated star image was produced in order to transform constellation features into image features. Then, based on the invariant collinearity of quadrilateral diagonal, image features between the observed star map and the simulated star image were matched, consequently, the initial values of the camera parameters could be extracted. Through using the singular value decomposition method, all the remaining control points were matched automatically and the attitudes of cameras were calculated. Finally, a complicated nonlinear optimization on camera intrinsic parameters and attitude matrix was required for this algorithm. The experimental result indicates that the re-projection error between different cameras is better than 1 pixel, and the correct recognition rate is more than 97.4% when the calibrations of optical system parameters are imprecise. This method can meet the requirements of accuracy and robust in registration of multi-sensor astronomical observation system.
参考文献

[1] SMITH A M S, HEBB L, COLLIER C A, et al. A SuperWASP search for additional transiting planets in 24 known systems [J]. Monthly Notices of Royal Astronomical Society, 2009, 398(4): 1827-1834.

[2] 王鸣浩, 陈涛, 王建立, 等. 捆绑式望远镜图像信噪比测量及分析[J]. 光学 精密工程, 2009, 17(1): 92-97.

    WANG M H, CHEN T, WANG J L, et al.. Measurement and analysis of image SNR in binding style telescope [J]. Opt. Precision Eng., 2009, 17(1): 92-97. (in Chinese)

[3] 徐树奎, 张军, 涂丹,等. 一种多分辨率混合相机系统标定方法[J]. 小型微型计算机系统, 2012, 33(9): 2073-2078.

    XU SH K, ZHANG J, TU D, et al.. A calibration technology for multi-resolution hybrid camera system [J]. Journal of Chinese Computer Systems, 2012, 33(9): 2073-2078. (in Chinese)

[4] LIU Z, ZHANG G, WEI Z. A global calibration method for multi-sensor vision system [C]. International Symposium on Instrumentation and Control Technology. USA: International Society for Optics and Photonics, 2008: 37-40.

[5] KIM S, SHIN J, PAIK J. Auto calibration for multiple camera-based surveillance system [J]. Ieek Proc. Korea-Japan Joint Workshop on Frontiers of Computer Vision. 2005, 1(34): 1-9.

[6] 张磊, 何昕, 魏仲慧,等. 基于星图识别的空间目标快速天文定位[J]. 光学 精密工程, 2014, 22(11): 3074-3080.

    ZHNAG L, HE X, WEI ZH H, et al.. Fast celestial positioning for space objects based on star identification [J]. 2014, 22(11): 3074-3080. (in Chinese)

[7] 戴东凯, 王省书, 胡春生,等. 基于天文观测的相机标定及姿态测量技术研究[J]. 光学学报, 2012(3): 100-104.

    DAI D K, WANG X SH, HU CH SH, et al.. Camera calibration and attitude measurement technology based on astronomical observation [J]. Acta Optica Sinica, 2012(3): 100-104. (in Chinese)

[8] 张广军. 星图识别[M]. 北京: 国防工业出版社, 2011.

    ZHANG G J. Star identification [M]. Beijing: National defense industry press, 2011. (in Chinese)

[9] 樊巧云, 陆壮志, 魏新国,等. 基于惯性比特征的三角形星图识别算法[J]. 红外与激光工程, 2012, 41(10): 2838-2843.

    FAN Q Y, LU ZH ZH, WEI X G, et al.. Triangle star identification algorithm based on inertia ratio [J]. Infrared and Laser Engineering, 2012,41(10): 2838-2843. (in Chinese)

[10] 林涛, 周建林, 等. 四边形全天自主星图识别算法[J]. 宇航学报, 2000, 21(2): 82-85.

    LIN T, ZHOU J L, et al.. All-sky automated quaternary star pattern recognition [J]. Journal of Astron Autics, 2000,21(2): 82-85. (in Chinese)

[11] 王玮. 图像仿射不变特征提取及匹配技术研究[D]. 长沙: 国防科学技术大学, 2013.

    WANG W. Image affine invariant feature extraction and matching [D]. Changsha: Graduate school of national university of defense technology, 2013. (in Chinese)

[12] JUANG J N, KIM H Y, JUNKINS J L. An Efficient and Robust Singular Value Method for Star Pattern Recognition and Attitude Determination [J]. Advances in the Astronautical Sciences, 2003, 115(1): 211-220.

[13] 王海涌, 林浩宇, 周文睿. 星光观测蒙气差补偿技术[J]. 光学学报, 2011, 31(11): 7-12.

    WANG H Y, LIN H Y, ZHOU W R. Technology of atmospheric refraction compensation in starlight observation [J]. Acta Optica Sinica, 2011,31(11): 100-104. (in Chinese)

张廷华, 高昆, 倪国强, 卢岩. 多传感器的天文标定与空间配准[J]. 光学 精密工程, 2017, 25(6): 1679. ZHANG Ting-Hua, GAO Kun, NI Guo-Qiang, LU Yan. Astronomical calibration and spatial registration of multi-sensor[J]. Optics and Precision Engineering, 2017, 25(6): 1679.

本文已被 2 篇论文引用
被引统计数据来源于中国光学期刊网
引用该论文: TXT   |   EndNote

相关论文

加载中...

关于本站 Cookie 的使用提示

中国光学期刊网使用基于 cookie 的技术来更好地为您提供各项服务,点击此处了解我们的隐私策略。 如您需继续使用本网站,请您授权我们使用本地 cookie 来保存部分信息。
全站搜索
您最值得信赖的光电行业旗舰网络服务平台!