Performance enhancement of X-ray pulsar navigation using autonomous optical sensor

被引:23
作者
Xiong Kai [1 ]
Wei Chunling [1 ]
Liu Liangdong [1 ]
机构
[1] Beijing Inst Control Engn, Sci & Technol Space Intelligent Control Lab, Beijing 100190, Peoples R China
基金
北京市自然科学基金;
关键词
Autonomous navigation; X-ray pulsar; Optical navigation; Phase estimation; Spacecraft; ORBIT DETERMINATION; RELATIVE NAVIGATION; PHASE ESTIMATION; STARLIGHT; ALGORITHM; SYSTEM; FILTER; MODEL;
D O I
10.1016/j.actaastro.2016.08.007
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
This paper develops an integrated navigation method based on the X-ray pulsar navigation (XNAV) system and an autonomous optical navigation system for spacecrafts. The X-ray pulsar navigation is implemented by using the difference between the measured and predicated pulse arrival time, which is calculated by comparing an observed pulse profile with a standard pulse profile. A problem arises from the X-ray signal processing in that the spacecraft's orbit information, which may be unknown, is required to construct the observed pulse profile. The effect of the spacecraft orbit error on the accuracy of the pulse TOA (time of arrival) difference determination is analyzed. It is specified that the performance of the XNAV system may be degraded in the presence of large orbit error. In order to improve the navigation accuracy, an integrated navigation scheme is presented by fusing the measurement information of a X-ray detector and an ultraviolet optical sensor. The XNAV/optical integrated navigation system is effective to mitigate the effect of the spacecraft orbit error. The superiority of the presented scheme is illustrated through numerical simulations. (C) 2016 IAA. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:473 / 484
页数:12
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