TY - JOUR
T1 - Astronomical calibration and spatial registration of multi-sensor
AU - Zhang, Ting Hua
AU - Gao, Kun
AU - Ni, Guo Qiang
AU - Lu, Yan
N1 - Publisher Copyright:
© 2017, Science Press. All right reserved.
PY - 2017/6/1
Y1 - 2017/6/1
N2 - 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.
AB - 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.
KW - Astronomical calibration
KW - Attitude measurement
KW - Spatial registration
KW - Star image simulation
KW - Star pattern recognition
UR - http://www.scopus.com/inward/record.url?scp=85026436913&partnerID=8YFLogxK
U2 - 10.3788/OPE.20172506.1679
DO - 10.3788/OPE.20172506.1679
M3 - Article
AN - SCOPUS:85026436913
SN - 1004-924X
VL - 25
SP - 1679
EP - 1687
JO - Guangxue Jingmi Gongcheng/Optics and Precision Engineering
JF - Guangxue Jingmi Gongcheng/Optics and Precision Engineering
IS - 6
ER -