近距离谱源功率估计的基本算法

S. D. Silverstein
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引用次数: 2

摘要

一种基于样本协方差特征结构划分为近似信号子空间和噪声子空间的新算法。这些波动效应是用随机摄动理论技术计算的。这些结果表明,MUSIC零谱的矩可以用源信噪比和快照数的线性泛函来近似。理论预测与模拟结果基本一致。一个有特色的仿真演示了由亚瑞利分辨率空间频率分隔的三个源的准确功率估计,其中0 dB信噪比的弱源夹在两个40和20 dB的大源之间。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A fundamental algorithm for the power estimation of closely separated spectral sources
A new algorithm is based upon division of the eigenstructure of the sample covariance into approximate signal and noise subspaces due to fluctuations caused by finite data samples. These fluctuation effects are calculated using stochastic perturbation theoretic techniques. These results show that the moments of the MUSIC null spectrum can be approximated by linear functionals of the source SNR and the number of snapshots. All theoretical predictions are in accord with the simulation results. A featured simulation demonstrates accurate source power estimates for three sources separated by sub-Rayleigh resolution spatial frequencies with a weak source of 0 dB SNR sandwiched between two much larger sources of 40 and 20 dB.<>
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