Differential X-ray pulsar aided celestial navigation for Mars exploration

被引:35
|
作者
Ning, Xiaolin [1 ]
Gui, Mingzhen [1 ]
Fang, Jiancheng [1 ]
Liu, Gang [1 ]
机构
[1] Beihang Univ, Sch Instrument Sci & Optoelect Engn, Beijing 100191, Peoples R China
基金
中国国家自然科学基金;
关键词
Autonomous navigation; Mars exploration; Celestial navigation; X-ray pulsar-based navigation; Unscented Kalman filter; INTEGRATED NAVIGATION; SYSTEM;
D O I
10.1016/j.ast.2016.10.032
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Celestial navigation (CeleNav) has been successfully used for position determination-in many Mars exploration missions. Traditional CeleNav usually uses star angle as measurement, which is a function of spacecraft's position. Its accuracy is affected by the distance between the spacecraft and the Mars. X-ray pulsar-based navigation (XNAV) is a feasible autonomous method which can provide highly accurate distance measurements. However, single pulsar navigation system is unobservable and its navigational performance is influenced by the corresponding systematic biases caused by the pulsar directional error and the spacecraft-borne clock error. For the complementary of the CeleNav and the XNAV, the differential X-ray pulsar aided CeleNav method is proposed, which adopts the time-differenced X-ray pulsar measurement to eliminate the major part of systematic biases and improve the navigation accuracy. Simulations demonstrate the feasibility and effectiveness of this method. (C) 2016 Elsevier Masson SAS. All rights reserved.
引用
收藏
页码:36 / 45
页数:10
相关论文
共 50 条
  • [41] Space experiments on X-ray pulsar navigation: Progress and prospects
    Zheng W.
    Wang Y.
    Jiang K.
    Wang Y.
    Hangkong Xuebao/Acta Aeronautica et Astronautica Sinica, 2024, 45 (06):
  • [42] Performance of the detection system for X-ray pulsar based navigation
    Sheng, Li-Zhi
    Zhao, Bao-Sheng
    Zhou, Feng
    Wang, Peng
    Song, Juan
    Liu, Yong-An
    Shen, Jing-Shi
    Hu, Hui-Jun
    Ma, Xiao-Fei
    Zhao, B.-S. (open@opt.ac.cn), 2013, Chinese Optical Society (42): : 1071 - 1076
  • [43] Selection of MCP for array X-ray pulsar navigation detector
    State Key Laboratory of Transient Optics and Photonics, Xi'an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi'an
    710119, China
    不详
    100049, China
    Guangxue Jingmi Gongcheng, 2 (402-407):
  • [44] A simulation experiment system for X-ray pulsar based navigation
    Hu Hui-Jun
    Zhao Bao-Sheng
    Sheng Li-Zhi
    Yan Qiu-Rong
    ACTA PHYSICA SINICA, 2011, 60 (02)
  • [45] Analysis in x-ray pulsar navigation phase ambiguity resolution
    Mao, Yue
    Song, Xiao-Yong
    Yuhang Xuebao/Journal of Astronautics, 2009, 30 (02): : 510 - 514
  • [46] Application of STEKF in X-ray Pulsar Based Autonomous Navigation
    Du, Jian
    Fei, Bao-jun
    Liu, Ying
    Xiao, Yu
    2012 INTERNATIONAL WORKSHOP ON INFORMATION AND ELECTRONICS ENGINEERING, 2012, 29 : 4369 - 4373
  • [47] Profile Bias' Influence in X-ray Pulsar Based Navigation
    Zhang, Dapeng
    Zheng, Wei
    Wang, Yidi
    Zhang, Lu
    SELECTED PAPERS OF THE PHOTOELECTRONIC TECHNOLOGY COMMITTEE CONFERENCES HELD NOVEMBER 2015, 2016, 9796
  • [48] A Novel Celestial Aided Time-Differenced Pulsar Navigation Method Against Ephemeris Error of Jupiter for Jupiter Exploration
    Gui, Mingzhen
    Ning, Xiaolin
    Ma, Xin
    Zhang, Jie
    IEEE SENSORS JOURNAL, 2019, 19 (03) : 1127 - 1134
  • [49] Pulsar-based navigation results: data processing of the x-ray pulsar navigation-I telescope
    Huang, Liangwei
    Shuai, Ping
    Zhang, Xinyuan
    Chen, Shaolong
    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS, 2019, 5 (01)
  • [50] Effect of Ephemeris on Pulsar Timing and Navigation Accuracy Based on X-ray Pulsar Navigation-I Data
    Deng, Yongtao
    Jin, Shuanggen
    UNIVERSE, 2022, 8 (07)