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A statistical and physical mechanisms-based interference and noise model for array observations

机译:基于统计和物理机制的阵列观测的干扰和噪声模型

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摘要

A statistical noise model is developed from mathematical modeling of the physical mechanisms that generate noise in communication receivers employing antenna arrays. Such models have been lacking for cases where the antenna observations may be statistically dependent from antenna to antenna. The model is developed by generalizing an approach for single antenna cases suggested by Middleton (1967, 1974, 1976, 1977). The model derived here is applicable to a wide variety of physical situations. The focus is primarily on problems defined by Middleton to be Class A interference. The number of noise sources in a small region of space is assumed to be Poisson distributed, and the emission times are assumed to be uniformly distributed over a long time interval. Finally, an additive Gaussian background component is included to represent the thermal noise that is always present in real receivers.
机译:从对在采用天线阵列的通信接收器中产生噪声的物理机制进行数学建模,可以开发出统计噪声模型。对于天线观测值可能在统计上因天线而异的情况,缺少这种模型。该模型是通过对Middleton(1967,1974,1976,1977)建议的单天线情况的方法进行概括而开发的。此处导出的模型适用于多种物理情况。重点主要放在由Middleton定义为A类干扰的问题上。在小空间区域内的噪声源的数量被假定为泊松分布,并且发射时间被假定为在长的时间间隔上均匀分布。最后,还包括一个加性高斯背景分量,以表示实际接收器中始终存在的热噪声。

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