Precise Attitude Determination of Ship Based on Star Sensor

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This paper analyses the attitude measured model and presents the attitude determination algorithm of space TT&C ship (space tracking, telemetry, and command ship) based on single star sensor. Considering lower precision of rolling angel for single star sensor, we proposed an algorithm by integrating attitude determination and redundancy measure to obtain high precision ship attitude data. Aiming at the circumstance of space TT&C ship, the factors that influence the precision of attitude measured data such as the number of star, atmosphere refraction correct and installation elevation are analyzed, which this can provide valuable references to the engineering design for star sensor used on space TT&C ship.

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995-1002

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August 2013

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© 2013 Trans Tech Publications Ltd. All Rights Reserved

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[1] Fang Jiancheng, Ning Xiaolin. The Principle of Celestial Navigation and its Application Beijing: Buaapress, (2006).

Google Scholar

[2] Liebe C. C. Accuracy Performance of Star Tracker-A tutorial. IEEE Transactions on Aerospace and Electronic Systems, 2002, 38(2): 557-59.

Google Scholar

[3] Hsiao F. H. ,Xu SD,Wu SL,et al. LQG Optimal Control of Discrete Stochastic Systems under Parametric and Noise Uncertainties. Journal of Franklin Institute,2006, 343 (3): 279-294.

DOI: 10.1016/j.jfranklin.2006.02.038

Google Scholar

[4] Ma Wenzhang. The Tutorial of Celestial Astronomy. Beijing : Normal Univ. press, (1995).

Google Scholar

[5] Zhen Wanbo, Xia liang,Hao Zhihang. Method Calculating of Satellitic Instantaneous Attitude based on Star Tracker[J]. Journal of Jilin University, 2003(1): 27-30.

Google Scholar

[6] Mortari D. Euler-q Algorithm for Attitude Determination from Vector Observation. Journal of Guidance, Control and Dynamics (S0731-5090). 1998, 21(2): 328-334.

DOI: 10.2514/2.4239

Google Scholar

[7] Markley F L. Attitude Determination Using Vector bserva- tion and the Singular Value Decomposition. Journal of the Astronautical Science(S0021-9142) . 1988, 36(3): 245-258.

Google Scholar

[8] Markley F L. Attitude Determination Using Vector bserva- tion:A Fast Optimal Matrix Algorithm. Journal of the Ast- ronautical Science (S0021-9142) . 1993, 41(2): 261-281.

Google Scholar

[9] Shuster M.D. and Oh S.D. Three-Axis Attitude Determina- tion from Vector Observations. Journal Guidence And Con- trol, AIAA 81-4003, 1981, 4(1): 70-77.

Google Scholar

[10] WANG Xiao-dong. Study on Wild-Field-of-View and High-Accuracy Star Sensor Technologies[D] . Changchun Institute of Optics, Fine Machine and Physics, Chinese Academy of Sciences, (2003).

Google Scholar

[11] Zhang Tongshuang,Zhong De-an etc. Dynamic Calibration Method of Attitude Error for Inertial Navigation System Based on RLS Algorithm[J] Telecommunication Engineering, 2011(8): 11-15.

Google Scholar

[12] Purple Observatory of Chinese Academy of Science. China Astronomical Almanac 2011[M]. Beijing: Sciences Press,(2010).

Google Scholar

[13] MAO Wei, YANG Lei, TIE Qiong-xian. On the Discussion of Astronomical Atmospheric Refraction[J]. ACTA Astronomica Sinica, 2008, 49(2): 216-222.

Google Scholar