刘劲, 马杰, 田金文. 基于小波和双谱的脉冲星信号识别[J]. 信息与控制, 2009, 38(2): 249-252.
引用本文: 刘劲, 马杰, 田金文. 基于小波和双谱的脉冲星信号识别[J]. 信息与控制, 2009, 38(2): 249-252.
LIU Jin, MA Jie, TIAN Jin-wen. Pulsar Signal Recognition Based on Wavelet and Bispectra[J]. INFORMATION AND CONTROL, 2009, 38(2): 249-252.
Citation: LIU Jin, MA Jie, TIAN Jin-wen. Pulsar Signal Recognition Based on Wavelet and Bispectra[J]. INFORMATION AND CONTROL, 2009, 38(2): 249-252.

基于小波和双谱的脉冲星信号识别

Pulsar Signal Recognition Based on Wavelet and Bispectra

  • 摘要: 为了提高脉冲星光信号识别效果,提出了一种基于小波变换和双谱分析的脉冲星信号识别算法.首先,本文提出了一种小波域双谱的概念,即对信号进行小波分解后再计算各级小波系数的双谱.然后,采用主分量分析(PCA)提取低频系数的双谱特征;根据最大类间误差平方和准则,用选择双谱的方法抽取高频系数的双谱特征,这些双谱特征构成特征向量.最后,采用最小距离分类器对脉冲星信号进行分类.实验结果表明了该脉冲星信号识别算法在识别效果和特征降维方面的有效性.

     

    Abstract: In order to improve the recognition effect of pulsar optical signals,an algorithm based on wavelet transform and bispectra analysis for pulsar signal recognition is proposed.First,the concept of bispectra in wavelet domain is proposed, namely,the bispectra of wavelet coefficients is calculated after signal is decomposed by wavelet transform.Then,the bispectral features of low frequency coefficients are extracted by PCA(principal component analysis),and those of high frequency coefficients are extracted by selected bispectra,according to the criterion of the maximal square sum of inter-cluster error. The bispectral features constitute feature vector.Finally,the minimum distance classifier is used to classify pulsar signals. The effectiveness of this algorithm in both pulsar signal recognition and feature dimensionality reduction is illustrated with some experimental results.

     

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