脉冲星
航天器
导航系统
物理
能见度
美国宇航局深空网络
卫星
X射线脉冲星
转化(遗传学)
深空探测
计算机科学
轨道(动力学)
职位(财务)
遥感
计算机视觉
天文
航空航天工程
光学
地质学
工程类
基因
经济
财务
化学
生物化学
作者
Jinyuan Wu,Zhaohua Yang,Ningning Yang
标识
DOI:10.1177/0959651812455896
摘要
An autonomous and secure navigation system is needed for the spacecraft in future deep space missions. X-ray pulsar offers the possibility of autonomous navigation anywhere in the solar system. This article introduces an analysis of the spacecraft autonomous navigation system accuracy, utilizing signals emitted from the X-ray pulsars. Based on the principle of the X-ray navigation, visibility of X-ray pulsar on L1 sun-observation orbit was simulated. The influence of the geometry distribution and the pulsar angle position error was analyzed. Error sources of the navigation system were listed, including the measurement error of the X-ray detector, transformation error of time-of-arrival (TOA), and the navigation calculation error, and the simulations of their parts were shown.
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