Empirical mode decomposition pulsar signal denoising method based on predicting of noise mode cell

被引:5
作者
Wang Wen-Bo [1 ,2 ]
Wang Xiang-Li [3 ]
机构
[1] Wuhan Univ Sci & Technol, Sch Sci, Wuhan 430065, Peoples R China
[2] State Key Lab Remote Sensing Sci, Beijing 100101, Peoples R China
[3] Wuhan Univ Technol, Sch Comp Sci & Technol, Wuhan 430063, Peoples R China
基金
中国国家自然科学基金;
关键词
pulsar signal denoising; empirical mode decomposition; noise mode cell predicting; local mean square error;
D O I
10.7498/aps.62.209701
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In order to improve the de-noising effect of the pulsar signal, an empirical mode decomposition (EMD) denoising algorithm based on the prediction of noise mode cell is put forward. The core steps of the proposed method is as follows: firstly, the noisy pulsar signal is decomposed into a group intrinsic mode function (IMF) by EMD, and the noise mode cell is predicted according to the IMF coefficients statistics and local minimum mean square error criteria. The selected noise mode cells are set to be zero. Then the IMF which has been processed according to noise mode cell prediction is denoised by optimal mode cell proportion shrinking, for removing the noise and retaining the signal details. The experimental results show that compared with the Sure Shrink wavelet threshold algorithm, Bayes Shrink wavelet threshold algorithm and the EMD mode cell proportion shrinking algorithm, the proposed method performs well in removing the pulsar signal noise and retaining the signal details information. The proposed method can achieve a higher signal-to-noise, the lower root mean square error, error of the peak position, relative error of the peak value and phase error.
引用
收藏
页数:10
相关论文
共 25 条
  • [1] Adaptive wavelet thresholding for image denoising and compression
    Chang, SG
    Yu, B
    Vetterli, M
    [J]. IEEE TRANSACTIONS ON IMAGE PROCESSING, 2000, 9 (09) : 1532 - 1546
  • [2] Adapting to unknown smoothness via wavelet shrinkage
    Donoho, DL
    Johnstone, IM
    [J]. JOURNAL OF THE AMERICAN STATISTICAL ASSOCIATION, 1995, 90 (432) : 1200 - 1224
  • [3] [杜念文 Du Nianwen], 2007, [电子测量与仪器学报, Journal of Electronic Measurement and Instrument], V21, P15
  • [4] A differentiable thresholding function and an adaptive threshold selection technique for pulsar signal denoising
    Gao Guo-Rong
    Liu Yan-Ping
    Pan Qiong
    [J]. ACTA PHYSICA SINICA, 2012, 61 (13)
  • [5] X-RAY PHASE-RESOLVED SPECTROSCOPY OF PSRs B0531+21, B1509-58, AND B0540-69 WITH RXTE
    Ge, M. Y.
    Lu, F. J.
    Qu, J. L.
    Zheng, S. J.
    Chen, Y.
    Han, D. W.
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2012, 199 (02)
  • [6] On the difference between empirical mode decomposition and wavelet decomposition in the nonlinear time series
    Gong, ZQ
    Zou, MW
    Gao, XQ
    Dong, WJ
    [J]. ACTA PHYSICA SINICA, 2005, 54 (08) : 3947 - 3957
  • [7] A simulation experiment system for X-ray pulsar based navigation
    Hu Hui-Jun
    Zhao Bao-Sheng
    Sheng Li-Zhi
    Yan Qiu-Rong
    [J]. ACTA PHYSICA SINICA, 2011, 60 (02)
  • [8] [胡慧君 HU HuiJun], 2011, [中国科学. 物理学, 力学, 天文学, Scientia Sinica Physica, Mechanica & Astronomica], V41, P1015
  • [9] The empirical mode decomposition and the Hilbert spectrum for nonlinear and non-stationary time series analysis
    Huang, NE
    Shen, Z
    Long, SR
    Wu, MLC
    Shih, HH
    Zheng, QN
    Yen, NC
    Tung, CC
    Liu, HH
    [J]. PROCEEDINGS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1998, 454 (1971): : 903 - 995
  • [10] JI PY, 2008, CHINESE PHYS B, V17, P356