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A Rao–Blackwellized Particle Filter for Adaptive Beamforming With Strong Interference

机译:Rao-Blackwellized粒子滤波器用于强干扰自适应波束形成

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摘要

A particle filter approach is proposed for adaptive narrowband beamforming in the presence of strong interference and uncertain steering vector of interest signal. From the viewpoint of subspace decomposition, we first describe the known subspace projection beamformer as an orthogonal component of the steering vector that is perpendicular to the interference space. Then a Rao–Blackwellized particle filter algorithm is designed to estimate the subspace projection beamforming weights. All steps including the important sampling, weight updating, resampling and analytical computation have been discussed in detail. Finally, the overall adaptive beamforming algorithm is summarized and the computational complexity analysis is presented. The main contribution of this paper is to apply and formulate Rao–Blackwellized particle filtering to estimate the distribution over the subspace projection beamforming weights. Different from other two particle-filter-based beamformers proposed by Li and Chandrasekar, it is a STI-based method with unknown source steering vector. The sampled state variables are the signal power, noise power and a model parameter for beamformer weights transition; the marginalized analytical state variables are the subspace projection beamforming weights; and the measurements are a series of constructed signal samples by using the estimated projection operator and random noise loading. Numerical simulations show that the proposed beamformer outperforms linearly constrained minimum variance, subspace projection, Bayesian and other two particle-filter-based beamformers. After convergence, it has similar performance to the optimal max-SINR beamformer which uses the true steering vector and ideal interference-plus-noise covariance matrix.
机译:提出了一种在强干扰和感兴趣信号的转向矢量不确定的情况下用于自适应窄带波束形成的粒子滤波方法。从子空间分解的观点出发,我们首先将已知的子空间投影波束形成器描述为与干扰空间垂直的转向矢量的正交分量。然后设计了Rao-Blackwellized粒子滤波算法来估计子空间投影波束成形权重。详细讨论了所有步骤,包括重要的采样,权重更新,重采样和分析计算。最后,总结了整体自适应波束成形算法,并进行了计算复杂度分析。本文的主要贡献是应用和制定了Rao-Blackwellized粒子滤波算法,以估计子空间投影波束成形权重的分布。与Li和Chandrasekar提出的其他两种基于粒子滤波器的波束形成器不同,它是一种基于STI的方法,具有未知的源导向向量。采样的状态变量是信号功率,噪声功率和波束成形器权重过渡的模型参数。边缘化分析状态变量是子空间投影波束成形权重;通过使用估计的投影算子和随机噪声加载,测量结果是一系列构造的信号样本。数值模拟表明,所提出的波束形成器优于线性约束的最小方差,子空间投影,贝叶斯和其他两个基于粒子滤波的波束形成器。收敛后,它的性能与使用真实导引向量和理想干扰加噪声协方差矩阵的最佳max-SINR波束形成器相似。

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