A Novel Celestial Aided Time-Differenced Pulsar Navigation Method Against Ephemeris Error of Jupiter for Jupiter Exploration

被引:14
作者
Gui, Mingzhen [1 ]
Ning, Xiaolin [1 ]
Ma, Xin [1 ]
Zhang, Jie [1 ]
机构
[1] Beihang Univ, Sch Instrumentat & Optoelect Engn, Beijing 100191, Peoples R China
基金
中国国家自然科学基金; 中国博士后科学基金;
关键词
Celestial navigation; pulsar navigation; Jupiter exploration; time difference; ephemeris error; X-RAY PULSARS; INTEGRATED NAVIGATION; PLANETARY EPHEMERIDES; SPACECRAFT; DIRECTION;
D O I
10.1109/JSEN.2018.2879355
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
Subjected to the current observation technology, the planetary ephemerides which are used to predict the positions of planets are not accurately known. For .Jupiter exploration, ephemeris error of Jupiter will greatly degrade the performance of navigation system. To improve the autonomous navigation performance, a novel celestial aided time-differenced pulsar navigation method against ephemeris error is proposed. Time-differenced time-of-arrival (TDTOA) is adopted as measurement to eliminate the system bias caused by the ephemeris error of Jupiter. Because TDTOA cannot work individually, the celestial measurement adopting Jupiter as near celestial body is added to provide the position information of the spacecraft with respect to Jupiter. Unscented kinematic and static filter is used as the navigation filter. Simulations demonstrate that the proposed method can acquire similar accuracy compared with the ideal scenario when there is no ephemeris error of Jupiter, which indicates that the impact of ephemeris error of Jupiter can be eliminated effectively by the proposed method. Moreover, the proposed method can acquire better navigation performance than using celestial measurements or TDTOA measurements individually.
引用
收藏
页码:1127 / 1134
页数:8
相关论文
共 33 条
[1]  
Bhaskara S. N., 2012, 2012 IEEE Power & Energy Society General Meeting. New Energy Horizons - Opportunities and Challenges, DOI 10.1109/PESGM.2012.6345694
[2]  
BHASKARAN S, 2002, AIAA AAS ASTR SPEC C
[3]  
Folkner W. M., 2009, 42178 IPN NASA
[4]  
Folkner W. M., 2014, 42196 IPN NASA
[5]  
Han ST, 2014, INT CONF SIGN PROCES, P2344, DOI 10.1109/ICOSP.2014.7015413
[6]  
Hanson J. E., 1996, SLACR809
[7]   High-Accuracy Synchronous Extraction Algorithm of Star and Celestial Body Features for Optical Navigation Sensor [J].
Jiang, Jie ;
Wang, Hao ;
Zhang, Guangjun .
IEEE SENSORS JOURNAL, 2018, 18 (02) :713-723
[8]   A new method for the nonlinear transformation of means and covariances in filters and estimators [J].
Julier, S ;
Uhlmann, J ;
Durrant-Whyte, HF .
IEEE TRANSACTIONS ON AUTOMATIC CONTROL, 2000, 45 (03) :477-482
[9]  
JULIER SJ, 1995, PROCEEDINGS OF THE 1995 AMERICAN CONTROL CONFERENCE, VOLS 1-6, P1628
[10]   X-ray Pulsar/Starlight Doppler Integrated Navigation for Formation Flight With Ephemerides Errors [J].
Liu, J. ;
Fang, J. C. ;
Ma, X. ;
Kang, Z. W. ;
Wu, J. .
IEEE AEROSPACE AND ELECTRONIC SYSTEMS MAGAZINE, 2015, 30 (03) :30-39