Wideband source localization by space-time MUSIC subspace estimation

E. D. D. Claudio, G. Jacovitti
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引用次数: 4

Abstract

Accurate estimation of the direction of arrivals (DOAs) of multiple wideband signal sources by sensor arrays is of paramount importance in recent developments of Ultra-Wide Band (UWB) and MIMO communication systems, acoustic applications, ultrasound, beside classical radar and sonar sensing. The array model changes with frequency. Narrowband analysis is not suited for short duration and, more in general, non-stationary sources. Most existing wideband direction finding algorithms are based on sensor output channelization (frequency binning) and neglect correlations among frequency bins, intra-bin finite bandwidth effects and spectral leakage that may create ghost sources during signal subspace estimation and impair the consistency of DOA estimators at high signal to noise (SNR) ratios. In this paper, a minimum leakage MUSIC-based estimator of subband signal subspaces from the space-time array covariance is introduced. Resulting subspace estimates can be fed to any frequency domain Maximum Likelihood (ML), Weighted Subspace Fitting (WSF) or focusing algorithm for final DOA estimation. Realistic simulations demonstrate the superior performance of the new estimator in difficult environments.
基于空时MUSIC子空间估计的宽带源定位
通过传感器阵列准确估计多个宽带信号源的到达方向(DOAs)在超宽带(UWB)和MIMO通信系统、声学应用、超声波以及经典雷达和声纳传感的最新发展中具有至关重要的意义。阵列模型随频率变化。窄带分析不适合短持续时间,更一般地说,不适合非平稳源。大多数现有的宽带测向算法都是基于传感器输出信道化(频率分频),忽略了频箱之间的相关性、频箱内有限带宽效应和频谱泄漏,这些因素可能会在信号子空间估计过程中产生幽灵源,并损害高信噪比下DOA估计器的一致性。提出了一种基于空时阵协方差的最小泄漏music子带信号子空间估计方法。由此产生的子空间估计可以输入到任何频域最大似然(ML)、加权子空间拟合(WSF)或聚焦算法中进行最终的DOA估计。仿真结果表明,该估计器在复杂环境下具有良好的性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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