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
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