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A CFAR Detection Algorithm for X-ray Pulsar Signal Based on Time-Frequency Entropy

机译:基于时频熵的X射线脉冲星信号CFAR检测算法

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摘要

Focusing on the X-ray pulsar signal detection in high background noise, a class of CFAR detection algorithms is proposed based on time-frequency entropy (TFE). Firstly, the definition of the pulsar signal TFE is given, moreover, the TFE difference of signal and noise is verified by theoretical derivation from the view of energy distribution. Then the distribution characteristic of TFE of pulsar signal is analyzed theoretically. The theoretical analysis result is further verified by Monte Carlo method. We detect the observation signal based on CFAR with the test statistic designed by TFE. We have also verified the effectiveness of this method by simulation experiment. The simulation results show that the time-frequency Renyi entropy detection algorithm based on ST generates the optimal detection performance.
机译:针对高背景噪声中的X射线脉冲星信号检测,提出了一种基于时频熵(TFE)的CFAR检测算法。首先给出了脉冲星信号TFE的定义,并从能量分布的角度通过理论推导验证了信号和噪声的TFE差异。然后从理论上分析了脉冲星信号的TFE的分布特性。理论分析结果通过蒙特卡洛方法进一步验证。我们使用TFE设计的测试统计量,基于CFAR来检测观测信号。我们还通过仿真实验验证了该方法的有效性。仿真结果表明,基于ST的时频Renyi熵检测算法产生了最优的检测性能。

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