ABSTRACT
Conventional centroid location algorithms are all in two dimensions. In order to solve the problem that the conventional centroid location algorithms are useless when the point spread function is smaller than the size of the detector, the research is about the centroid location algorithm in three dimensions based on big data. By using the time parameter to link the big data of energy received by the detector at different time, not only the single image but the time sequence images are used in the algorithm, based on the geometric theorem, the exact position at the special time is calculated out. It is sure that, the algorithm is very steady when the sample number is enough, that means the phase of the sample point is nothing, and the error of the position got by the algorithm is less than 0.06 pixel when the non-uniformity of the detectors is smaller than 5%, that is usually the upper limit of the non-uniformity of the detector.
- R. Abreu. Stellar attitude determination accuracy with multiple-star-tracking advanced star tracker. In Optical Engineering and Photonics in Aerospace Sensing, pages 216--227. International Society for Optics and Photonics, 1993.Google ScholarCross Ref
- J.-q. Bai, C.-g. Zhao, S.-f. Wang, and N. Sun. Adaptive wiener filtering noise reduction in infrared images {j}. Opto-Electronic Engineering, 11: 018, 2011.Google Scholar
- T. Bank. Characterizing a star tracker with built-in attitude estimation algorithms under the night sky. In AeroSense'97, pages 264--274. International Society for Optics and Photonics, 1997.Google ScholarCross Ref
- Y. Dong, F. Xing, and Z. You. Determination of the optical system parameters for a cmos aps based star sensor. Yuhang Xuebao/ Journal of Astronautics(China), 25(6):663--668, 2004.Google Scholar
- L. Guangrui. Research of sub-pixel location for star image based on gaussian distribution {j}. Optical Technique, 1: 57--61, 2011.Google Scholar
- C. E. Hannelore G. Hansen. Adaptive the threshold adjustment and control. In Proc. SPIE 1096, Signal and Data Processing of Small Targets 1989, 44. SPIE, 1989.Google ScholarCross Ref
- D. Hui. Angular velocity determination directly from star tracker measurements. Ship Electronic Engineering, 6: 022, 2011.Google Scholar
- Y. Jiahu, Z. Jianrong, and H. Shanjin. A study on detection sensitivity of navigation star sensor. Opto-Electronic Engineering, 26(6):1--6, 1999.Google Scholar
- M. Jiang, M.-y. Yu, J.-x. Wang, and F.-c. Lai. Obtaining method of star location for star sensor of high maneuverability. Microelectronics & Computer, 7:028, 2009.Google Scholar
- Z. Z. Jiang, C. R. Sheng, H. Q. Cheng, and L. W. Guo. Centroid of characteristic point image obtain in probe imaging vision coordinate measuring system. Optics and Precision Engineering, page 05, 1998.Google Scholar
- G. Ju. Autonomous star sensing, pattern identification, and attitude determination for spacecraft: an analytical and experimental study. 2001.Google Scholar
- W. Lei, S. Xiaowei, G. Deren, and L. Wei. Optimal attitude determination method based on star sensor. Computer Measurement & Control, 4:061, 2012.Google Scholar
- D.-m. Li, X.-w. Wang, and M. Guo. Image simulation of star sensor and movement characteristic analysis of background and target. Opto-Electronic Engineering, 4:010, 2009.Google Scholar
- X.-k. Li, Z.-h. Hao, J. Li, and G.-h. Zhou. The research on the method of the star's position determination of the star sensor {j}. Journal of Electron Devices, 4:007, 2004.Google Scholar
- Y.-f. LI and Z.-h. Hao. Research of hyper accuracy subpixel subdivision location algorithm for star image {j}. Optical Technique, 5:006, 2005.Google Scholar
- C. C. Liebe. Accuracy performance of star trackers-a tutorial. IEEE Transactions on Aerospace and Electronic Systems, pages 587--599, 2002.Google ScholarCross Ref
- J. Liu, S. Zheng, and J.-w. Tian. New star acquisition algorithm and optimization {j}. Opto-electronic Engineering, 2:000, 2005.Google Scholar
- C. Padgett and K. Kreutz-Delgado. A grid algorithm for autonomous star identification. Aerospace and Electronic Systems, IEEE Transactions on, 33(1):202--213, 1997.Google Scholar
- U. Schmidt. Autonomous star tracker based on active pixel sensors. In 5th International Conference on Space Optics, ESA SP-554, Toulouse, France, pages 355--358, 2004.Google Scholar
- W. M. Z. F. H. Shuang. Novel infrared dim and small target detection algorithm based on multi-scale gradient {j}. Acta Optica Sinica, 10:021, 2011.Google Scholar
- L.-l. Song, T. Zhang, B. Liang, and J. Yang. Attitude determination method based on star sensor. Journal of System Simulation, page S1, 2010.Google Scholar
- Z. Wanbo, X. Liang, and H. Zhihang. Method calculating of satellite instantaneous attitude based on star tracker {j}. Journal of Jilin University (Information Science Edition), 1: 27--30, 2003.Google Scholar
- D. Wang, Y. Han, and T. Sun. Star sub-pixel centroid calculation based on multi-step minimum energy difference method. In ISPDI 2013-Fifth International Symposium on Photoelectronic Detection and Imaging, pages 89075M--89075M. International Society for Optics and Photonics, 2013.Google ScholarCross Ref
- H. Wang, Z. Fei, and X. Wang. Precise simulation of star spots and centroid calculation based on gaussian distribution. Optics and Precision Engineering, 7:030, 2009.Google Scholar
- W. Wei and L. Enhai. Denoising algorithms to infrared star map of daytime star observation. Infrared and Laser Engineering, 7:049, 2013.Google Scholar
- L. XiaoKun and C. Guilin. Three-axis stability satellite radiometer of geostationary charge-ccd star sense of visible channel {j}. Science technology and engineering, 19: 4897--4899, 2007.Google Scholar
- J. Yan and Z. Dong. Method for ccd superresolved position measurement and capability analysis. Journal of Test and Measurement Technology, 20(3):189, 2006.Google Scholar
- L. Yan, Z. Xueqing, and Z. Wang. A star field identification method based on dsp. Ship Electronic Engineering, 5: 104--107, 2006.Google Scholar
- B. Zhang, J. Duan, and W. Jing. Ccd-based optical detection precision of angle measurement {j}. Journal of Changchun University of Science and Technology (Natural Science Edition), 4:016, 2010.Google Scholar
- H. Zhang, J.-h. Yuan, and E.-h. Liu. Ccd noise effects on position accuracy of star sensor. Infrared and Laser Engineering, 35(5):629, 2006.Google Scholar
- W. Zhengliang, T. Zhengqi, and A. Delong. Attitude determination for spacecraft based on star sensor. Modern Surveying and Mapping, 1: 17--18, 21, 2008.Google Scholar
Index Terms
- Centroid location algorithm in three dimensions based on big data
Recommendations
The Study of the Weighted Centroid Localization Algorithm Based on RSSI
WCSN '14: Proceedings of the 2014 International Conference on Wireless Communication and Sensor NetworkAiming at the wireless sensor network (WSN) positioning of the centroid localization algorithm with the problem of inaccurate positioning, this paper proposes an improved weighted centroid localization algorithm based on RSSI. This algorithm regard the ...
Research on Indoor Location Algorithm Based on WIFI
ISBDAI '18: Proceedings of the International Symposium on Big Data and Artificial IntelligenceWith the wide application of mobile Internet, location-based service demands are more and more extensive. In the indoor positioning technology, the location fingerprinting method based on WIFI is widely used because of its strong anti-interference ...
Comments