大地测量学与导航

一种亮星识别算法及其在天文定向中的应用

  • 詹银虎 ,
  • 郑勇 ,
  • 张超 ,
  • 李铸洋 ,
  • 张中凯
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  • 信息工程大学导航与空天目标工程学院, 河南 郑州 450001
詹银虎(1986—),男,博士生,研究方向为天文导航. E-mail:oscardad@163.com

收稿日期: 2013-04-20

  修回日期: 2014-07-30

  网络出版日期: 2015-04-01

基金资助

国家自然科学基金(10878025)

Bright-star Recognition Algorithm and Its Application in Astronomical Azimuth Determination

  • ZHAN Yinhu ,
  • ZHENG Yong ,
  • ZHANG Chao ,
  • LI Zhuyang ,
  • ZHANG Zhongkai
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  • College of Navigation and Aerospace Engineering, Information Engineering University, Zhengzhou 450001, China

Received date: 2013-04-20

  Revised date: 2014-07-30

  Online published: 2015-04-01

Supported by

The National Natural Science Foundation of China(No.10878025)

摘要

基于全站仪对任意亮星的观测采样,提出了一种利用高度角序列和水平角速率进行联合匹配的任意亮星识别算法.通过引入天体地平坐标计算程序,算法可正确辨别行星和恒星.本文分析了任意亮星高度角和水平角速率的观测误差和计算误差,以此给出了匹配阈值条件的设定依据,并在此基础上制定了有效的匹配策略.仿真计算及实际观测试验均表明,该算法具有100%的识别成功率,远优于现有算法.将此算法应用于任意亮星天文定向,定向结果的内符合精度达到2",外部检核精度达到1.6".采用多颗任意亮星进行定向,可有效减弱由测站位置误差引入的定向系统误差,提高绝对定向精度.本文提出的天文定向适用于多云及雾霾天气.

本文引用格式

詹银虎 , 郑勇 , 张超 , 李铸洋 , 张中凯 . 一种亮星识别算法及其在天文定向中的应用[J]. 测绘学报, 2015 , 44(3) : 257 -263 . DOI: 10.11947/j.AGCS.2015.20130557

Abstract

A novel bright-star identification algorithm is presented using the time series of vertical angle and horizontal angle velocity observed by the total station. The algorithm can distinguish planets from the starry background with automatically computing for the horizontal coordinates of the observed target. Based on the investigation of measurement errors, the matching thresholds and the effective matching strategy are given. Tests results with simulated and actual measurements show that the success rate of identification can be up to 100%, which is much higher than the existing algorithm. Then the identification algorithm is applied to the astronomical azimuth determination with the measurements of some bright stars and planets and the resulting precision and accuracy are 1.6" and 2.0", respectively. Finally, it is pointed that multi-star observations can improve the accuracy of the astronomical orientation by effectively removing the impact of errors of station coordinates. The presented orientation method can be extended to cloudy or haze weather when only few visible bright stars can be observed.

参考文献

[1] WANG Anguo.Celestial Navigation Technique in the Background of Navigation War[J].Progress in Astronomy,2001,19(2):326-330.(王安国.导航战背景下的天文导航技术[J] .天文学进展,2001,19(2):326-330.)
[2] CHEN Junyong, YANG Yuanxi, WANG Min, et a1. Establishment of 2000 National Geodetic Control Network of China and It's Technological Progress[J]. ActaGeodatica et CartographiaSinica, 2007, 36(1):1-8. (陈俊勇,杨元喜,王敏,等.2000国家大地控制网的构建和它的技术进步[J].测绘学报, 2007, 36(1):1-8.)
[3] SUN Xiaochang,HUANG Fukan.Precision Calibration of Moving Platform Based Radar with Stars as Reference Marks [J].Journal of Astronautics,2002,23(3):29-33.(孙晓昶,皇甫堪.以恒星位置为基准的运动平台上测控雷达精度标校技术[J].宇航学报,2002,23(3):29-33.)
[4] LI Zhenghang, WEI Erhu, WANG Zhengtao.Space Geodesy[M].Wuhan: Wuhan University Press,2010.(李征航,魏二虎,王正涛.空间大地测量学[M].武汉:武汉大学出版社,2010.)
[5] HIRT C, BUERKI B. The Digital Zenith Camera-A New High-precision and Economic Astrogeodetic Observation System for Real-time Measurement of Defections of the Vertical [C] //Proceedings of the 3rd Meeting of the International Gravity and Geoid Commission of the International Association of Geodesy. Thessaloniki:[s.n.], 2002:161-166.
[6] WEI E, JIN S, ZHANG Q, et al. Autonomous Navigation of Mars Probe Using X-ray Pulsars: Modeling and Results[J]. Advances in Space Research, 2013, 51(5): 849-857.
[7] SUN Shouming. Study on Autonomous Navigation Method of Spacecraft Based on X-ray Pulsars [D].Changsha: National University of Defense Technology, 2011.(孙守明. 基于 X 射线脉冲星的航天器自主导航方法研究[D]. 长沙: 国防科学技术大学, 2011.)
[8] LAMBROU E, PANTAZIS G. Astronomical Azimuth Determination by the Hour Angle of Polaris Using Ordinary Total Stations[J]. Survey Review, 2008, 40(308): 164-172.
[9] BALODIMOS D, KORAKITIS R, LAMBROU E, et al. Fast and Accurate Determination of Astronomical Coordinates Φ, Λ and Azimuth, Using a Total Station and GPS Receiver[J]. Survey Review, 2003, 37(290): 269-275.
[10] ZHAN Yinhu,ZHANG Chao,WANG Yonghai.A New Method of Fast Orientation by Surveying the Constellation Stars[J].Beijing Surveying and Mapping,2012(4):11-13.(詹银虎,张超,王永海.利用特征星进行快速天文定向[J].北京测绘,2012(4):11-13.)
[11] ZHAN Yinhu,ZHANG Chao,HUA Yuesheng,et a1.Research on Fast Astro-geodetic Orientation by Observing Planets [J].Journal of Geomatics Science and Technology,2011,28(5):338-341.(詹银虎,张超,华跃升,等.利用行星进行快速天文定向[J].测绘科学技术学报,2011,28(5):338-341.)
[12] ZHAN Yinhu,ZHANG Chao,ZHENG Yong,et a1.A Fitting Algorithm of the Apparent Moon Center and Its Application on Fast Orientation [J].Acta Geodatica et Cartographia Sinica,2012,41(3):353-358.(詹银虎,张超,郑勇,等.月球视面中心拟合算法及其在测月快速定向中的应用[J].测绘学报,2012,41(3):353-358.)
[13] BUONOCORE B, VASSALLO A. Astronomical Determination of Azimuth and Latitude by Observation of Two Unknown Stars Without Time Measurement and Knowledge of Astronomy[J]. Survey Review, 1991, 31(242): 233-237.
[14] ZHANG Chao, ZHENG Yong, LI Changhui.Research of Astronomy Orientation by Using the Random Star[J].Science of Surveying and Mapping,2005,30(4): 30-32. (张超,郑勇,李长会.用任意星进行天文定向的研究[J]. 测绘科学, 2005, 30(4): 30-32.)
[15] LU Xiushan,FENG Zhunde,LIU Jimin.Analysis Theory on Ill-conditioned System with Application on Surveying[M].Beijing:Surveying and Mapping Press,2007.(卢秀山,冯遵德,刘纪敏.病态系统分析理论及其在测量中的应用[M].北京:测绘出版社,2007.)
[16] HANSEN P.Analysis of the Discrete Ill-posed Problems by Means of the L-curves[J].SIAM Review,1992,34:561-580.
[17] ZHANG Guangjun.Star identification [M].Beijing:National Defence Industry Press,2011.(张广军.星图识别[M].北京:国防工业出版社,2011.)
[18] JIANG Ming,YU Mingyan,WANG Jinxiang,et al.A Novel All-sky Autonomous Star Pattern Recognition Algorithm [J]. Journal of Astronautics, 2007, 28(4): 1020-1024.(蒋明,喻明艳,王进祥,等.一种新的全天自主星图识别算法[J]. 宇航学报, 2007, 28(4): 1020-1024.)
[19] XIA Yifei,JIN Wenjing. Impacts of the New Reference System on Astrometry[J]. Progress in Astronomy, 2004, 22(3): 200-207. (夏一飞,金文敬. 新参考系的引入对天体测量学的影响[J].天文学进展, 2004, 22(3): 200-207.)
[20] BANGERT J,PUATUA W, KAPLAN G, et al. User’s Guide to NOVAS Version C3.0[M].Washington:USA Naval Observatory,2009:31-32.
[21] JIN Shuanggen, ZHU Wenyao. International Terrestrial Reference Frame: Current Status and Its Future[J]. Progress in Astronomy, 2003, 21(3): 241-249.(金双根,朱文耀. 国际地球参考架:现状与未来[J].天文学进展,2003, 21(3):241-249.)
[22] WEI Erhu, LIU Jingnan, PAN Peijing. On Data Processing with Last Three Years of VLBI Observation[J].Geomatics and Information Science of Wuhan University, 2008,33(12):1275-1278.(魏二虎,刘经南,潘培鲸.近三年VLBI观测的数据处理及分析[J].武汉大学学报:信息科学版,2008,33(12):1275-1278.)
[23] LÜ Zhiping,QIAO Shubo.Foundation of Geodesy [M].Beijing:Surveying and Mapping Press,2010.(吕志平,乔书波.大地测量学基础 [M].北京:测绘出版社,2010.)
[24] XIA Yifei,HUANG Tianyi.Spherical Astronomy [M].Nanjing:Nanjing University Press,1995.(夏一飞,黄天衣.球面天文学 [M].南京:南京大学出版社,1995.)
[25] ZHANG Chao.System-level Development and Application Research on Astronomic Surveying System Based on Electronic Theodolites[D].Zhengzhou:Information Engineering University,2009.(张超.基于电子经纬仪的天文测量系统及应用研究[D].郑州:信息工程大学,2009.)
[26] ZHAN Yinhu.Theory and Technology Research on Fast Orientation Based on Celestial Bodies[D].Zhengzhou:Information Engineering University,2012.(詹银虎.基于自然天体的快速定向理论及技术研究[D].郑州:信息工程大学,2012.)

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