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深空探测器接近段自适应滤波方法研究

宁晓琳 李卓 黄盼盼 杨雨青

空间科学学报2017,Vol.37Issue(3):322-331,10.
空间科学学报2017,Vol.37Issue(3):322-331,10.DOI:10.11728/cjss2017.03.322

深空探测器接近段自适应滤波方法研究

Comparison of Adaptive Filter for Celestial Navigation during Approach Phase

宁晓琳 1李卓 1黄盼盼 2杨雨青1

作者信息

  • 1. 北京航空航天大学仪器科学与光电工程学院 北京100191
  • 2. School of Civil and Environmental Engineering, University of New South Wales, Sydney 2052, Australia
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摘要

Abstract

Celestial navigation is an autonomous navigation method for deep space mission,which has been wildly researched.In celestial navigation,nonlinear Kalman filters such as Unscented Kalman Filter (UKF) are usually used.However,for traditional nonlinear Kalman filter,the system model errors should be Gaussian noise and their statistical characteristics should be known.However,the information is usually unknown and the system model errors are usually time-varying in real system.Hence,many adaptive filters have been studied to solve this problem.In this paper,three adaptive filters based on adjusting the predicted state covariance matrix are compared by simulation.Before this,the system model errors of celestial navigation are also analyzed for the approach phase.

关键词

天文导航/自适应滤波/深空探测接近段

Key words

Celestial navigation/Adaptive filter/Approach phase

分类

天文与地球科学

引用本文复制引用

宁晓琳,李卓,黄盼盼,杨雨青..深空探测器接近段自适应滤波方法研究[J].空间科学学报,2017,37(3):322-331,10.

基金项目

国家自然科学基金项目资助(61233005,61503013) (61233005,61503013)

空间科学学报

OA北大核心CSCDCSTPCD

0254-6124

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