基于自适应滤波器的脉冲星相对导航信号在线时延估计

A. A. Emadzadeh, C. G. Lopes, J. Speyer
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引用次数: 14

摘要

航天器的相对导航可以通过观测x射线源和间接确定航天器的相对位置来完成。在这种方法中,两个航天器锁定在一个已知的脉冲星上,该脉冲星向它们发射x射线波形,并以与航天器之间的距离成正比的不同时间延迟到达它们。通过观测不同脉冲星源在星系盘上的几何分布,可以确定航天器的相对惯性位置。我们的目标是通过检测信号之间的时间延迟估计(TDE)来估计它们的相对位置。尽管有几种离线TDE方法,如基本互相关(BCC)和广义互相关(GCC)技术,但在本工作中,我们将TDE描述为信道估计问题,并应用自适应滤波技术在线估计时延。使用自适应滤波器有一定的好处,特别是当信号统计等基础参数未知或随时间变化时。我们研究了不同的自适应算法,并展示了它们如何能够在降低计算复杂性和实时的情况下有效地提供准确的延迟估计。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Online time delay estimation of pulsar signals for relative navigation using adaptive filters
Relative navigation of spacecrafts may be accomplished by observing X-ray sources and indirectly determining the spacecraftspsila relative position. In this approach, two spacecrafts lock on a known pulsar which irradiates X-ray waveforms that reach them with a differential time delay that is proportional to the distance between the spacecrafts. By observing different pulsar sources geometrically distributed over the galactic disc, it is possible to determine the spacecraftspsila relative inertial position. Our goal is to estimate their relative position by Time Delay Estimation (TDE) between the detected signals. Although there are several off-line TDE methods, like the basic cross-correlation (BCC) and the generalized cross-correlation (GCC) techniques, in this work we formulate TDE as a channel estimation problem and apply adaptive filtering techniques to estimate the time delay online. There are certain benefits in using adaptive filters, especially when the underlying parameters like signalspsila statistics are unknown or change over time. We study different adaptive algorithms and show how they are able to efficiently deliver accurate delay estimates at reduced computational complexity and in real time.
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