基于可分离模糊核的复合运动模糊星图建模与仿真
[1] Bhaskaran S, Riedel J E, Synnott S P, et al. The deep space 1 autonomous navigation system: a post-flight analysis[C]//AIAA Astrodynamics Specialist Conference, 2000, 3935: 42.
[2] Van bezooijen R W H, Anderson K A, Ward D K. Performance of the AST-201 star tracker for the microwave anisotropy probe[C]//AIAA Guidance and Control Conference, 2002, 4582: 5-8.
[3] Pasetti A, Habinc S, Creasey R C. Dynamical binning for high angular rate star tracking[C]//Spacecraft Guidance, Navigation and Control Systems, 2000, 425: 255.
[4] Xiaojuan W, Xinlong W. Multiple blur of star image and the restoration under dynamic conditions[J]. Acta Astronautica, 2011, 68(11): 1903-1913.
[5] Shen J, Zhang G, Wei X. Simulation analysis of dynamic working performance for star trackers[J]. JOSA A, 2010, 27(12): 2638-2647.
[6] Fei X, Nan C, Zheng Y, et al. A novel approach based on MEMS-gyro′s data deep coupling for determining the centroid of star spot[J]. Mathematical Problems in Engineering, 2012, 2012(6): 55-9.
[7] Wang X, Yi T, Tang Q, et al. Simulation and analysis of vibration blurred images[C]//IEEE Wireless Communications Networking and Mobile Computing(WiCOM), 2010: 1-4.
[8] Zhang W, Quan W, Guo L. Blurred star image processing for star sensors under dynamic conditions[J]. Sensors, 2012, 12(5): 6712-6726.
[9] Sun T, Xing F, You Z, et al. Smearing model and restoration of star image under conditions of variable angular velocity and long exposure time[J]. Optics Express, 2014, 22(5): 6009-6024.
[10] 吴小娟, 王新龙.星图运动模糊及其复原方法[J].北京航空航天大学学报, 2011, 11(37): 23-31.
Wu Xiaojuan, Wang Xinlong. Motion blur of star image and restoration[J]. Journal of Beihang University, 2011, 11(37): 23-31. (in Chinese)
[11] 张钧萍, 林涛. 一种模拟 CCD 星图的方法[J]. 中国空间科学技术, 1999, 19(3): 46-50.
Zhang Junping, Lin Tao. A simulation method of CCD map[J]. China′s Space Science and Technology, 1999, 19(3): 46-50. (in Chinese)
[12] 全伟, 房建成. 高精度星图模拟及有效性验证新方法[J]. 光电工程, 2005, 32(7): 22-26.
[13] Whyte O, Sivic J, Zisserman A, et al. Non-uniform de blurring for shaken images[J]. International Journal of Computer Vision, 2012, 98(2): 168-186.
[14] Fang L, Liu H, Wu F, et al. Separable kernel for image deblurring[C]//IEEE Computer Vision and Pattern Recognition (CVPR), 2014, 369: 2885-2892.
[15] 庞涛, 程小平. 基于Radon变换的运动模糊图像参数估计[J]. 科学与技术工程, 2010, 22(2): 1671－1815.
Pang Tao, Cheng Xiaoping. The parameter estimation of motion blurred image based on Radon transform[J]. Science and Technology Project, 2010, 22(2): 1671－1815. (in Chinese)
[16] 田玉龙, 王广君, 房建成, 等. 基于局部熵的星敏感器星图提取方法[J]. 哈尔滨工业大学学报, 2005, 37(8): 1068-1070.
Tian Yulong, Wang Guangjun, Fan Jiancheng, et al. A new method of star image high precision extraction based on local entropy[J]. Journal of Harbin Industrial University, 2005, 37(8): 1068-1070. (in Chinese)
袁洪琳, 李帆, 于涛, 张存读, 赵建辉. 基于可分离模糊核的复合运动模糊星图建模与仿真[J]. 红外与激光工程, 2016, 45(11): 1126001. Yuan Honglin, Li Fan, Yu Tao, Zhang Cundu, Zhao Jianhui. Modeling and simulation of blurred star images by the complicated motion based on the separable kernel[J]. Infrared and Laser Engineering, 2016, 45(11): 1126001.
PDF全文
