The Well-Known Bispectrum
The well-known bispectrum, which represents third-order spectral estimation, holds significant reference value in cosmological research.
Explore MATLAB source code curated for "双谱" with clean implementations, documentation, and examples.
The well-known bispectrum, which represents third-order spectral estimation, holds significant reference value in cosmological research.
This set of programs implements additive Gaussian noise removal through bispectral analysis and wavelet transforms. Key implementations include: 1. Bispectral analysis program for single variables calculating third-order cumulants and Fourier transforms 2. Autocorrelation function computation using inverse Fourier transform with proper normalization 3. Spectral analysis suite using FFT for preference spectrum, power spectrum, RMS spectrum, and logarithmic spectrum 4. Wavelet-based denoising pipeline for .wav audio signals with white noise removal 5. Comparative analysis framework evaluating multiple wavelet types and thresholding techniques on identical signals
MATLAB implementation of higher-order spectra analysis including bispectrum, featuring both direct and indirect methods for signal detection and time-delay estimation with enhanced algorithm descriptions.
Calculate and visualize time series biphase spectrum using 3D and 2D plots, essential for investigating nonlinear processes with code-driven implementation techniques