Matlab Toolbox Quick Reference Page 2

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Convert transfer function filter parameters to lattice
Real cepstrum and minimum phase reconstruction.
Compute an estimate of AR model parameters using
tf2latc
rceps
arcov
filter form.
the covariance method.
Convert digital filter transfer function data to second-
Compute an estimate of AR model parameters using
tf2sos
armcov
order sections form.
the modified covariance method.
Statistical Signal Processing and Spectral
Convert transfer function filter parameters to state-
Compute an estimate of AR model parameters using
tf2ss
aryule
Analysis
space form.
the Yule-Walker method.
Estimate magnitude squared coherence function
cohere
tf2zp
Convert transfer function filter parameters to zero-
ident
See the
System Identification Toolbox
between two signals.
pole-gain form.
documentation.
Compute the correlation coefficient matrix.
corrcoef
Convert digital filter zero-pole-gain parameters to
Identify continuous-time filter parameters from
zp2sos
invfreqs
second-order sections form.
Compute a data matrix for autocorrelation matrix
frequency response data.
corrmtx
estimation.
Convert zero-pole-gain filter parameters to state-
Identify discrete-time filter parameters from
zp2ss
invfreqz
space form.
Compute the covariance matrix.
frequency response data.
cov
Convert zero-pole-gain filter parameters to transfer
Estimate the cross spectral density (CSD) of two
Prony's method for time domain IIR filter design.
zp2tf
csd
prony
function form.
signals.
Compute a linear model using Steiglitz-McBride
stmcb
Estimate the power spectral density using the Burg
iteration.
pburg
method.
Windows
Estimate the power spectral density using the
pcov
covariance method.
Linear Prediction
Compute a Bartlett window.
bartlett
Estimate the pseudospectrum using the eigenvector
peig
Compute a Blackman window.
Convert an autocorrelation sequence to prediction
blackman
ac2poly
method.
polynomial.
Compute a rectangular window.
boxcar
Estimate the power spectral density (PSD) of a signal
periodogram
Convert an autocorrelation sequence to reflection
ac2rc
Compute a Chebyshev window.
using a periodogram.
chebwin
coefficients.
Compute a Hamming window.
Estimate the power spectral density using the
hamming
pmcov
Convert inverse sine parameters to reflection
is2rc
modified covariance method.
Compute the Hann (Hanning) window.
hann
coefficients.
Estimate the power spectral density using the
pmtm
Compute a Kaiser window.
Convert log area ratio parameters to reflection
kaiser
lar2rc
multitaper method (MTM).
coefficients.
Compute a triangular window.
triang
Estimate the power spectral density using MUSIC
pmusic
Compute the Levinson-Durbin recursion.
levinson
algorithm.
Compute linear prediction filter coefficients.
lpc
Plot power spectral density (PSD) data.
psdplot
Transforms
Convert line spectral frequencies to a prediction filter
lsf2poly
Estimate the power spectral density (PSD) of a signal
pwelch
coefficients.
czt
Chirp z-transform.
using Welch's method.
Convert a prediction filter polynomial to an
poly2ac
Discrete cosine transform (DCT).
dct
Estimate the power spectral density using the Yule-
pyulear
autocorrelation sequence.
Walker AR method.
Discrete Fourier transform matrix.
dftmtx
Convert prediction filter coefficients to line spectral
poly2lsf
Estimate frequency and power content using the
rooteig
Compute the one-dimensional fast Fourier transform.
frequencies.
fft
eigenvector method.
Compute the two-dimensional fast Fourier transform.
fft2
Convert a prediction filter polynomial to reflection
poly2rc
Estimate frequency and power content using the root
rootmusic
coefficients.
Rearrange the outputs of the FFT functions.
MUSIC algorithm.
fftshift
Convert reflection coefficients to an autocorrelation
rc2ac
Compute the discrete-time analytic signal using the
Estimate the transfer function from input and output.
hilbert
tfe
sequence.
Hilbert transform.
Estimate the cross-correlation function.
xcorr
Convert reflection coefficients to inverse sine
rc2is
Inverse discrete cosine transform.
idct
Estimate the two-dimensional cross-correlation.
parameters.
xcorr2
ifft
One-dimensional inverse fast Fourier transform.
Estimate the cross-covariance function (equal to
Convert reflection coefficients to log area ratio
xcov
rc2lar
Two-dimensional inverse fast Fourier transform.
mean-removed cross-correlation).
parameters.
ifft2
Convert reflection coefficients to a prediction filter
rc2poly
polynomial.
Cepstral Analysis
Parametric Modeling
Compute the reverse Levinson-Durbin recursion.
rlevinson
Complex cepstral analysis.
cceps
Compute an estimate of AR model parameters using
Compute reflection coefficients from an
arburg
schurrc
the Burg method.
autocorrelation sequence.
Inverse complex cepstrum.
icceps

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