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installed required libs
2021-02-17 12:26:31 +05:30
"""Tools for spectral analysis.
"""
import numpy as np
from scipy import fft as sp_fft
from . import signaltools
from .windows import get_window
from ._spectral import _lombscargle
from ._arraytools import const_ext, even_ext, odd_ext, zero_ext
import warnings
__all__ = ['periodogram', 'welch', 'lombscargle', 'csd', 'coherence',
'spectrogram', 'stft', 'istft', 'check_COLA', 'check_NOLA']
def lombscargle(x,
y,
freqs,
precenter=False,
normalize=False):
"""
lombscargle(x, y, freqs)
Computes the Lomb-Scargle periodogram.
The Lomb-Scargle periodogram was developed by Lomb [1]_ and further
extended by Scargle [2]_ to find, and test the significance of weak
periodic signals with uneven temporal sampling.
When *normalize* is False (default) the computed periodogram
is unnormalized, it takes the value ``(A**2) * N/4`` for a harmonic
signal with amplitude A for sufficiently large N.
When *normalize* is True the computed periodogram is normalized by
the residuals of the data around a constant reference model (at zero).
Input arrays should be 1-D and will be cast to float64.
Parameters
----------
x : array_like
Sample times.
y : array_like
Measurement values.
freqs : array_like
Angular frequencies for output periodogram.
precenter : bool, optional
Pre-center measurement values by subtracting the mean.
normalize : bool, optional
Compute normalized periodogram.
Returns
-------
pgram : array_like
Lomb-Scargle periodogram.
Raises
------
ValueError
If the input arrays `x` and `y` do not have the same shape.
Notes
-----
This subroutine calculates the periodogram using a slightly
modified algorithm due to Townsend [3]_ which allows the
periodogram to be calculated using only a single pass through
the input arrays for each frequency.
The algorithm running time scales roughly as O(x * freqs) or O(N^2)
for a large number of samples and frequencies.
References
----------
.. [1] N.R. Lomb "Least-squares frequency analysis of unequally spaced
data", Astrophysics and Space Science, vol 39, pp. 447-462, 1976
.. [2] J.D. Scargle "Studies in astronomical time series analysis. II -
Statistical aspects of spectral analysis of unevenly spaced data",
The Astrophysical Journal, vol 263, pp. 835-853, 1982
.. [3] R.H.D. Townsend, "Fast calculation of the Lomb-Scargle
periodogram using graphics processing units.", The Astrophysical
Journal Supplement Series, vol 191, pp. 247-253, 2010
See Also
--------
istft: Inverse Short Time Fourier Transform
check_COLA: Check whether the Constant OverLap Add (COLA) constraint is met
welch: Power spectral density by Welch's method
spectrogram: Spectrogram by Welch's method
csd: Cross spectral density by Welch's method
Examples
--------
>>> import matplotlib.pyplot as plt
First define some input parameters for the signal:
>>> A = 2.
>>> w = 1.
>>> phi = 0.5 * np.pi
>>> nin = 1000
>>> nout = 100000
>>> frac_points = 0.9 # Fraction of points to select
Randomly select a fraction of an array with timesteps:
>>> r = np.random.rand(nin)
>>> x = np.linspace(0.01, 10*np.pi, nin)
>>> x = x[r >= frac_points]
Plot a sine wave for the selected times:
>>> y = A * np.sin(w*x+phi)
Define the array of frequencies for which to compute the periodogram:
>>> f = np.linspace(0.01, 10, nout)
Calculate Lomb-Scargle periodogram:
>>> import scipy.signal as signal
>>> pgram = signal.lombscargle(x, y, f, normalize=True)
Now make a plot of the input data:
>>> plt.subplot(2, 1, 1)
>>> plt.plot(x, y, 'b+')
Then plot the normalized periodogram:
>>> plt.subplot(2, 1, 2)
>>> plt.plot(f, pgram)
>>> plt.show()
"""
x = np.asarray(x, dtype=np.float64)
y = np.asarray(y, dtype=np.float64)
freqs = np.asarray(freqs, dtype=np.float64)
assert x.ndim == 1
assert y.ndim == 1
assert freqs.ndim == 1
if precenter:
pgram = _lombscargle(x, y - y.mean(), freqs)
else:
pgram = _lombscargle(x, y, freqs)
if normalize:
pgram *= 2 / np.dot(y, y)
return pgram
def periodogram(x, fs=1.0, window='boxcar', nfft=None, detrend='constant',
return_onesided=True, scaling='density', axis=-1):
"""
Estimate power spectral density using a periodogram.
Parameters
----------
x : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to 'boxcar'.
nfft : int, optional
Length of the FFT used. If `None` the length of `x` will be
used.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
scaling : { 'density', 'spectrum' }, optional
Selects between computing the power spectral density ('density')
where `Pxx` has units of V**2/Hz and computing the power
spectrum ('spectrum') where `Pxx` has units of V**2, if `x`
is measured in V and `fs` is measured in Hz. Defaults to
'density'
axis : int, optional
Axis along which the periodogram is computed; the default is
over the last axis (i.e. ``axis=-1``).
Returns
-------
f : ndarray
Array of sample frequencies.
Pxx : ndarray
Power spectral density or power spectrum of `x`.
Notes
-----
.. versionadded:: 0.12.0
See Also
--------
welch: Estimate power spectral density using Welch's method
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
>>> np.random.seed(1234)
Generate a test signal, a 2 Vrms sine wave at 1234 Hz, corrupted by
0.001 V**2/Hz of white noise sampled at 10 kHz.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 2*np.sqrt(2)
>>> freq = 1234.0
>>> noise_power = 0.001 * fs / 2
>>> time = np.arange(N) / fs
>>> x = amp*np.sin(2*np.pi*freq*time)
>>> x += np.random.normal(scale=np.sqrt(noise_power), size=time.shape)
Compute and plot the power spectral density.
>>> f, Pxx_den = signal.periodogram(x, fs)
>>> plt.semilogy(f, Pxx_den)
>>> plt.ylim([1e-7, 1e2])
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('PSD [V**2/Hz]')
>>> plt.show()
If we average the last half of the spectral density, to exclude the
peak, we can recover the noise power on the signal.
>>> np.mean(Pxx_den[25000:])
0.00099728892368242854
Now compute and plot the power spectrum.
>>> f, Pxx_spec = signal.periodogram(x, fs, 'flattop', scaling='spectrum')
>>> plt.figure()
>>> plt.semilogy(f, np.sqrt(Pxx_spec))
>>> plt.ylim([1e-4, 1e1])
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('Linear spectrum [V RMS]')
>>> plt.show()
The peak height in the power spectrum is an estimate of the RMS
amplitude.
>>> np.sqrt(Pxx_spec.max())
2.0077340678640727
"""
x = np.asarray(x)
if x.size == 0:
return np.empty(x.shape), np.empty(x.shape)
if window is None:
window = 'boxcar'
if nfft is None:
nperseg = x.shape[axis]
elif nfft == x.shape[axis]:
nperseg = nfft
elif nfft > x.shape[axis]:
nperseg = x.shape[axis]
elif nfft < x.shape[axis]:
s = [np.s_[:]]*len(x.shape)
s[axis] = np.s_[:nfft]
x = x[tuple(s)]
nperseg = nfft
nfft = None
return welch(x, fs=fs, window=window, nperseg=nperseg, noverlap=0,
nfft=nfft, detrend=detrend, return_onesided=return_onesided,
scaling=scaling, axis=axis)
def welch(x, fs=1.0, window='hann', nperseg=None, noverlap=None, nfft=None,
detrend='constant', return_onesided=True, scaling='density',
axis=-1, average='mean'):
r"""
Estimate power spectral density using Welch's method.
Welch's method [1]_ computes an estimate of the power spectral
density by dividing the data into overlapping segments, computing a
modified periodogram for each segment and averaging the
periodograms.
Parameters
----------
x : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window.
nperseg : int, optional
Length of each segment. Defaults to None, but if window is str or
tuple, is set to 256, and if window is array_like, is set to the
length of the window.
noverlap : int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 2``. Defaults to `None`.
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
scaling : { 'density', 'spectrum' }, optional
Selects between computing the power spectral density ('density')
where `Pxx` has units of V**2/Hz and computing the power
spectrum ('spectrum') where `Pxx` has units of V**2, if `x`
is measured in V and `fs` is measured in Hz. Defaults to
'density'
axis : int, optional
Axis along which the periodogram is computed; the default is
over the last axis (i.e. ``axis=-1``).
average : { 'mean', 'median' }, optional
Method to use when averaging periodograms. Defaults to 'mean'.
.. versionadded:: 1.2.0
Returns
-------
f : ndarray
Array of sample frequencies.
Pxx : ndarray
Power spectral density or power spectrum of x.
See Also
--------
periodogram: Simple, optionally modified periodogram
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
Notes
-----
An appropriate amount of overlap will depend on the choice of window
and on your requirements. For the default Hann window an overlap of
50% is a reasonable trade off between accurately estimating the
signal power, while not over counting any of the data. Narrower
windows may require a larger overlap.
If `noverlap` is 0, this method is equivalent to Bartlett's method
[2]_.
.. versionadded:: 0.12.0
References
----------
.. [1] P. Welch, "The use of the fast Fourier transform for the
estimation of power spectra: A method based on time averaging
over short, modified periodograms", IEEE Trans. Audio
Electroacoust. vol. 15, pp. 70-73, 1967.
.. [2] M.S. Bartlett, "Periodogram Analysis and Continuous Spectra",
Biometrika, vol. 37, pp. 1-16, 1950.
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
>>> np.random.seed(1234)
Generate a test signal, a 2 Vrms sine wave at 1234 Hz, corrupted by
0.001 V**2/Hz of white noise sampled at 10 kHz.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 2*np.sqrt(2)
>>> freq = 1234.0
>>> noise_power = 0.001 * fs / 2
>>> time = np.arange(N) / fs
>>> x = amp*np.sin(2*np.pi*freq*time)
>>> x += np.random.normal(scale=np.sqrt(noise_power), size=time.shape)
Compute and plot the power spectral density.
>>> f, Pxx_den = signal.welch(x, fs, nperseg=1024)
>>> plt.semilogy(f, Pxx_den)
>>> plt.ylim([0.5e-3, 1])
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('PSD [V**2/Hz]')
>>> plt.show()
If we average the last half of the spectral density, to exclude the
peak, we can recover the noise power on the signal.
>>> np.mean(Pxx_den[256:])
0.0009924865443739191
Now compute and plot the power spectrum.
>>> f, Pxx_spec = signal.welch(x, fs, 'flattop', 1024, scaling='spectrum')
>>> plt.figure()
>>> plt.semilogy(f, np.sqrt(Pxx_spec))
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('Linear spectrum [V RMS]')
>>> plt.show()
The peak height in the power spectrum is an estimate of the RMS
amplitude.
>>> np.sqrt(Pxx_spec.max())
2.0077340678640727
If we now introduce a discontinuity in the signal, by increasing the
amplitude of a small portion of the signal by 50, we can see the
corruption of the mean average power spectral density, but using a
median average better estimates the normal behaviour.
>>> x[int(N//2):int(N//2)+10] *= 50.
>>> f, Pxx_den = signal.welch(x, fs, nperseg=1024)
>>> f_med, Pxx_den_med = signal.welch(x, fs, nperseg=1024, average='median')
>>> plt.semilogy(f, Pxx_den, label='mean')
>>> plt.semilogy(f_med, Pxx_den_med, label='median')
>>> plt.ylim([0.5e-3, 1])
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('PSD [V**2/Hz]')
>>> plt.legend()
>>> plt.show()
"""
freqs, Pxx = csd(x, x, fs=fs, window=window, nperseg=nperseg,
noverlap=noverlap, nfft=nfft, detrend=detrend,
return_onesided=return_onesided, scaling=scaling,
axis=axis, average=average)
return freqs, Pxx.real
def csd(x, y, fs=1.0, window='hann', nperseg=None, noverlap=None, nfft=None,
detrend='constant', return_onesided=True, scaling='density',
axis=-1, average='mean'):
r"""
Estimate the cross power spectral density, Pxy, using Welch's
method.
Parameters
----------
x : array_like
Time series of measurement values
y : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` and `y` time series. Defaults
to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window.
nperseg : int, optional
Length of each segment. Defaults to None, but if window is str or
tuple, is set to 256, and if window is array_like, is set to the
length of the window.
noverlap: int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 2``. Defaults to `None`.
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
scaling : { 'density', 'spectrum' }, optional
Selects between computing the cross spectral density ('density')
where `Pxy` has units of V**2/Hz and computing the cross spectrum
('spectrum') where `Pxy` has units of V**2, if `x` and `y` are
measured in V and `fs` is measured in Hz. Defaults to 'density'
axis : int, optional
Axis along which the CSD is computed for both inputs; the
default is over the last axis (i.e. ``axis=-1``).
average : { 'mean', 'median' }, optional
Method to use when averaging periodograms. Defaults to 'mean'.
.. versionadded:: 1.2.0
Returns
-------
f : ndarray
Array of sample frequencies.
Pxy : ndarray
Cross spectral density or cross power spectrum of x,y.
See Also
--------
periodogram: Simple, optionally modified periodogram
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
welch: Power spectral density by Welch's method. [Equivalent to
csd(x,x)]
coherence: Magnitude squared coherence by Welch's method.
Notes
--------
By convention, Pxy is computed with the conjugate FFT of X
multiplied by the FFT of Y.
If the input series differ in length, the shorter series will be
zero-padded to match.
An appropriate amount of overlap will depend on the choice of window
and on your requirements. For the default Hann window an overlap of
50% is a reasonable trade off between accurately estimating the
signal power, while not over counting any of the data. Narrower
windows may require a larger overlap.
.. versionadded:: 0.16.0
References
----------
.. [1] P. Welch, "The use of the fast Fourier transform for the
estimation of power spectra: A method based on time averaging
over short, modified periodograms", IEEE Trans. Audio
Electroacoust. vol. 15, pp. 70-73, 1967.
.. [2] Rabiner, Lawrence R., and B. Gold. "Theory and Application of
Digital Signal Processing" Prentice-Hall, pp. 414-419, 1975
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
Generate two test signals with some common features.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 20
>>> freq = 1234.0
>>> noise_power = 0.001 * fs / 2
>>> time = np.arange(N) / fs
>>> b, a = signal.butter(2, 0.25, 'low')
>>> x = np.random.normal(scale=np.sqrt(noise_power), size=time.shape)
>>> y = signal.lfilter(b, a, x)
>>> x += amp*np.sin(2*np.pi*freq*time)
>>> y += np.random.normal(scale=0.1*np.sqrt(noise_power), size=time.shape)
Compute and plot the magnitude of the cross spectral density.
>>> f, Pxy = signal.csd(x, y, fs, nperseg=1024)
>>> plt.semilogy(f, np.abs(Pxy))
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('CSD [V**2/Hz]')
>>> plt.show()
"""
freqs, _, Pxy = _spectral_helper(x, y, fs, window, nperseg, noverlap, nfft,
detrend, return_onesided, scaling, axis,
mode='psd')
# Average over windows.
if len(Pxy.shape) >= 2 and Pxy.size > 0:
if Pxy.shape[-1] > 1:
if average == 'median':
Pxy = np.median(Pxy, axis=-1) / _median_bias(Pxy.shape[-1])
elif average == 'mean':
Pxy = Pxy.mean(axis=-1)
else:
raise ValueError('average must be "median" or "mean", got %s'
% (average,))
else:
Pxy = np.reshape(Pxy, Pxy.shape[:-1])
return freqs, Pxy
def spectrogram(x, fs=1.0, window=('tukey', .25), nperseg=None, noverlap=None,
nfft=None, detrend='constant', return_onesided=True,
scaling='density', axis=-1, mode='psd'):
"""
Compute a spectrogram with consecutive Fourier transforms.
Spectrograms can be used as a way of visualizing the change of a
nonstationary signal's frequency content over time.
Parameters
----------
x : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg.
Defaults to a Tukey window with shape parameter of 0.25.
nperseg : int, optional
Length of each segment. Defaults to None, but if window is str or
tuple, is set to 256, and if window is array_like, is set to the
length of the window.
noverlap : int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 8``. Defaults to `None`.
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
scaling : { 'density', 'spectrum' }, optional
Selects between computing the power spectral density ('density')
where `Sxx` has units of V**2/Hz and computing the power
spectrum ('spectrum') where `Sxx` has units of V**2, if `x`
is measured in V and `fs` is measured in Hz. Defaults to
'density'.
axis : int, optional
Axis along which the spectrogram is computed; the default is over
the last axis (i.e. ``axis=-1``).
mode : str, optional
Defines what kind of return values are expected. Options are
['psd', 'complex', 'magnitude', 'angle', 'phase']. 'complex' is
equivalent to the output of `stft` with no padding or boundary
extension. 'magnitude' returns the absolute magnitude of the
STFT. 'angle' and 'phase' return the complex angle of the STFT,
with and without unwrapping, respectively.
Returns
-------
f : ndarray
Array of sample frequencies.
t : ndarray
Array of segment times.
Sxx : ndarray
Spectrogram of x. By default, the last axis of Sxx corresponds
to the segment times.
See Also
--------
periodogram: Simple, optionally modified periodogram
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
welch: Power spectral density by Welch's method.
csd: Cross spectral density by Welch's method.
Notes
-----
An appropriate amount of overlap will depend on the choice of window
and on your requirements. In contrast to welch's method, where the
entire data stream is averaged over, one may wish to use a smaller
overlap (or perhaps none at all) when computing a spectrogram, to
maintain some statistical independence between individual segments.
It is for this reason that the default window is a Tukey window with
1/8th of a window's length overlap at each end.
.. versionadded:: 0.16.0
References
----------
.. [1] Oppenheim, Alan V., Ronald W. Schafer, John R. Buck
"Discrete-Time Signal Processing", Prentice Hall, 1999.
Examples
--------
>>> from scipy import signal
>>> from scipy.fft import fftshift
>>> import matplotlib.pyplot as plt
Generate a test signal, a 2 Vrms sine wave whose frequency is slowly
modulated around 3kHz, corrupted by white noise of exponentially
decreasing magnitude sampled at 10 kHz.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 2 * np.sqrt(2)
>>> noise_power = 0.01 * fs / 2
>>> time = np.arange(N) / float(fs)
>>> mod = 500*np.cos(2*np.pi*0.25*time)
>>> carrier = amp * np.sin(2*np.pi*3e3*time + mod)
>>> noise = np.random.normal(scale=np.sqrt(noise_power), size=time.shape)
>>> noise *= np.exp(-time/5)
>>> x = carrier + noise
Compute and plot the spectrogram.
>>> f, t, Sxx = signal.spectrogram(x, fs)
>>> plt.pcolormesh(t, f, Sxx, shading='gouraud')
>>> plt.ylabel('Frequency [Hz]')
>>> plt.xlabel('Time [sec]')
>>> plt.show()
Note, if using output that is not one sided, then use the following:
>>> f, t, Sxx = signal.spectrogram(x, fs, return_onesided=False)
>>> plt.pcolormesh(t, fftshift(f), fftshift(Sxx, axes=0), shading='gouraud')
>>> plt.ylabel('Frequency [Hz]')
>>> plt.xlabel('Time [sec]')
>>> plt.show()
"""
modelist = ['psd', 'complex', 'magnitude', 'angle', 'phase']
if mode not in modelist:
raise ValueError('unknown value for mode {}, must be one of {}'
.format(mode, modelist))
# need to set default for nperseg before setting default for noverlap below
window, nperseg = _triage_segments(window, nperseg,
input_length=x.shape[axis])
# Less overlap than welch, so samples are more statisically independent
if noverlap is None:
noverlap = nperseg // 8
if mode == 'psd':
freqs, time, Sxx = _spectral_helper(x, x, fs, window, nperseg,
noverlap, nfft, detrend,
return_onesided, scaling, axis,
mode='psd')
else:
freqs, time, Sxx = _spectral_helper(x, x, fs, window, nperseg,
noverlap, nfft, detrend,
return_onesided, scaling, axis,
mode='stft')
if mode == 'magnitude':
Sxx = np.abs(Sxx)
elif mode in ['angle', 'phase']:
Sxx = np.angle(Sxx)
if mode == 'phase':
# Sxx has one additional dimension for time strides
if axis < 0:
axis -= 1
Sxx = np.unwrap(Sxx, axis=axis)
# mode =='complex' is same as `stft`, doesn't need modification
return freqs, time, Sxx
def check_COLA(window, nperseg, noverlap, tol=1e-10):
r"""
Check whether the Constant OverLap Add (COLA) constraint is met
Parameters
----------
window : str or tuple or array_like
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg.
nperseg : int
Length of each segment.
noverlap : int
Number of points to overlap between segments.
tol : float, optional
The allowed variance of a bin's weighted sum from the median bin
sum.
Returns
-------
verdict : bool
`True` if chosen combination satisfies COLA within `tol`,
`False` otherwise
See Also
--------
check_NOLA: Check whether the Nonzero Overlap Add (NOLA) constraint is met
stft: Short Time Fourier Transform
istft: Inverse Short Time Fourier Transform
Notes
-----
In order to enable inversion of an STFT via the inverse STFT in
`istft`, it is sufficient that the signal windowing obeys the constraint of
"Constant OverLap Add" (COLA). This ensures that every point in the input
data is equally weighted, thereby avoiding aliasing and allowing full
reconstruction.
Some examples of windows that satisfy COLA:
- Rectangular window at overlap of 0, 1/2, 2/3, 3/4, ...
- Bartlett window at overlap of 1/2, 3/4, 5/6, ...
- Hann window at 1/2, 2/3, 3/4, ...
- Any Blackman family window at 2/3 overlap
- Any window with ``noverlap = nperseg-1``
A very comprehensive list of other windows may be found in [2]_,
wherein the COLA condition is satisfied when the "Amplitude
Flatness" is unity.
.. versionadded:: 0.19.0
References
----------
.. [1] Julius O. Smith III, "Spectral Audio Signal Processing", W3K
Publishing, 2011,ISBN 978-0-9745607-3-1.
.. [2] G. Heinzel, A. Ruediger and R. Schilling, "Spectrum and
spectral density estimation by the Discrete Fourier transform
(DFT), including a comprehensive list of window functions and
some new at-top windows", 2002,
http://hdl.handle.net/11858/00-001M-0000-0013-557A-5
Examples
--------
>>> from scipy import signal
Confirm COLA condition for rectangular window of 75% (3/4) overlap:
>>> signal.check_COLA(signal.windows.boxcar(100), 100, 75)
True
COLA is not true for 25% (1/4) overlap, though:
>>> signal.check_COLA(signal.windows.boxcar(100), 100, 25)
False
"Symmetrical" Hann window (for filter design) is not COLA:
>>> signal.check_COLA(signal.windows.hann(120, sym=True), 120, 60)
False
"Periodic" or "DFT-even" Hann window (for FFT analysis) is COLA for
overlap of 1/2, 2/3, 3/4, etc.:
>>> signal.check_COLA(signal.windows.hann(120, sym=False), 120, 60)
True
>>> signal.check_COLA(signal.windows.hann(120, sym=False), 120, 80)
True
>>> signal.check_COLA(signal.windows.hann(120, sym=False), 120, 90)
True
"""
nperseg = int(nperseg)
if nperseg < 1:
raise ValueError('nperseg must be a positive integer')
if noverlap >= nperseg:
raise ValueError('noverlap must be less than nperseg.')
noverlap = int(noverlap)
if isinstance(window, str) or type(window) is tuple:
win = get_window(window, nperseg)
else:
win = np.asarray(window)
if len(win.shape) != 1:
raise ValueError('window must be 1-D')
if win.shape[0] != nperseg:
raise ValueError('window must have length of nperseg')
step = nperseg - noverlap
binsums = sum(win[ii*step:(ii+1)*step] for ii in range(nperseg//step))
if nperseg % step != 0:
binsums[:nperseg % step] += win[-(nperseg % step):]
deviation = binsums - np.median(binsums)
return np.max(np.abs(deviation)) < tol
def check_NOLA(window, nperseg, noverlap, tol=1e-10):
r"""
Check whether the Nonzero Overlap Add (NOLA) constraint is met
Parameters
----------
window : str or tuple or array_like
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg.
nperseg : int
Length of each segment.
noverlap : int
Number of points to overlap between segments.
tol : float, optional
The allowed variance of a bin's weighted sum from the median bin
sum.
Returns
-------
verdict : bool
`True` if chosen combination satisfies the NOLA constraint within
`tol`, `False` otherwise
See Also
--------
check_COLA: Check whether the Constant OverLap Add (COLA) constraint is met
stft: Short Time Fourier Transform
istft: Inverse Short Time Fourier Transform
Notes
-----
In order to enable inversion of an STFT via the inverse STFT in
`istft`, the signal windowing must obey the constraint of "nonzero
overlap add" (NOLA):
.. math:: \sum_{t}w^{2}[n-tH] \ne 0
for all :math:`n`, where :math:`w` is the window function, :math:`t` is the
frame index, and :math:`H` is the hop size (:math:`H` = `nperseg` -
`noverlap`).
This ensures that the normalization factors in the denominator of the
overlap-add inversion equation are not zero. Only very pathological windows
will fail the NOLA constraint.
.. versionadded:: 1.2.0
References
----------
.. [1] Julius O. Smith III, "Spectral Audio Signal Processing", W3K
Publishing, 2011,ISBN 978-0-9745607-3-1.
.. [2] G. Heinzel, A. Ruediger and R. Schilling, "Spectrum and
spectral density estimation by the Discrete Fourier transform
(DFT), including a comprehensive list of window functions and
some new at-top windows", 2002,
http://hdl.handle.net/11858/00-001M-0000-0013-557A-5
Examples
--------
>>> from scipy import signal
Confirm NOLA condition for rectangular window of 75% (3/4) overlap:
>>> signal.check_NOLA(signal.windows.boxcar(100), 100, 75)
True
NOLA is also true for 25% (1/4) overlap:
>>> signal.check_NOLA(signal.windows.boxcar(100), 100, 25)
True
"Symmetrical" Hann window (for filter design) is also NOLA:
>>> signal.check_NOLA(signal.windows.hann(120, sym=True), 120, 60)
True
As long as there is overlap, it takes quite a pathological window to fail
NOLA:
>>> w = np.ones(64, dtype="float")
>>> w[::2] = 0
>>> signal.check_NOLA(w, 64, 32)
False
If there is not enough overlap, a window with zeros at the ends will not
work:
>>> signal.check_NOLA(signal.windows.hann(64), 64, 0)
False
>>> signal.check_NOLA(signal.windows.hann(64), 64, 1)
False
>>> signal.check_NOLA(signal.windows.hann(64), 64, 2)
True
"""
nperseg = int(nperseg)
if nperseg < 1:
raise ValueError('nperseg must be a positive integer')
if noverlap >= nperseg:
raise ValueError('noverlap must be less than nperseg')
if noverlap < 0:
raise ValueError('noverlap must be a nonnegative integer')
noverlap = int(noverlap)
if isinstance(window, str) or type(window) is tuple:
win = get_window(window, nperseg)
else:
win = np.asarray(window)
if len(win.shape) != 1:
raise ValueError('window must be 1-D')
if win.shape[0] != nperseg:
raise ValueError('window must have length of nperseg')
step = nperseg - noverlap
binsums = sum(win[ii*step:(ii+1)*step]**2 for ii in range(nperseg//step))
if nperseg % step != 0:
binsums[:nperseg % step] += win[-(nperseg % step):]**2
return np.min(binsums) > tol
def stft(x, fs=1.0, window='hann', nperseg=256, noverlap=None, nfft=None,
detrend=False, return_onesided=True, boundary='zeros', padded=True,
axis=-1):
r"""
Compute the Short Time Fourier Transform (STFT).
STFTs can be used as a way of quantifying the change of a
nonstationary signal's frequency and phase content over time.
Parameters
----------
x : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window.
nperseg : int, optional
Length of each segment. Defaults to 256.
noverlap : int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 2``. Defaults to `None`. When
specified, the COLA constraint must be met (see Notes below).
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to `False`.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
boundary : str or None, optional
Specifies whether the input signal is extended at both ends, and
how to generate the new values, in order to center the first
windowed segment on the first input point. This has the benefit
of enabling reconstruction of the first input point when the
employed window function starts at zero. Valid options are
``['even', 'odd', 'constant', 'zeros', None]``. Defaults to
'zeros', for zero padding extension. I.e. ``[1, 2, 3, 4]`` is
extended to ``[0, 1, 2, 3, 4, 0]`` for ``nperseg=3``.
padded : bool, optional
Specifies whether the input signal is zero-padded at the end to
make the signal fit exactly into an integer number of window
segments, so that all of the signal is included in the output.
Defaults to `True`. Padding occurs after boundary extension, if
`boundary` is not `None`, and `padded` is `True`, as is the
default.
axis : int, optional
Axis along which the STFT is computed; the default is over the
last axis (i.e. ``axis=-1``).
Returns
-------
f : ndarray
Array of sample frequencies.
t : ndarray
Array of segment times.
Zxx : ndarray
STFT of `x`. By default, the last axis of `Zxx` corresponds
to the segment times.
See Also
--------
istft: Inverse Short Time Fourier Transform
check_COLA: Check whether the Constant OverLap Add (COLA) constraint
is met
check_NOLA: Check whether the Nonzero Overlap Add (NOLA) constraint is met
welch: Power spectral density by Welch's method.
spectrogram: Spectrogram by Welch's method.
csd: Cross spectral density by Welch's method.
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
Notes
-----
In order to enable inversion of an STFT via the inverse STFT in
`istft`, the signal windowing must obey the constraint of "Nonzero
OverLap Add" (NOLA), and the input signal must have complete
windowing coverage (i.e. ``(x.shape[axis] - nperseg) %
(nperseg-noverlap) == 0``). The `padded` argument may be used to
accomplish this.
Given a time-domain signal :math:`x[n]`, a window :math:`w[n]`, and a hop
size :math:`H` = `nperseg - noverlap`, the windowed frame at time index
:math:`t` is given by
.. math:: x_{t}[n]=x[n]w[n-tH]
The overlap-add (OLA) reconstruction equation is given by
.. math:: x[n]=\frac{\sum_{t}x_{t}[n]w[n-tH]}{\sum_{t}w^{2}[n-tH]}
The NOLA constraint ensures that every normalization term that appears
in the denomimator of the OLA reconstruction equation is nonzero. Whether a
choice of `window`, `nperseg`, and `noverlap` satisfy this constraint can
be tested with `check_NOLA`.
.. versionadded:: 0.19.0
References
----------
.. [1] Oppenheim, Alan V., Ronald W. Schafer, John R. Buck
"Discrete-Time Signal Processing", Prentice Hall, 1999.
.. [2] Daniel W. Griffin, Jae S. Lim "Signal Estimation from
Modified Short-Time Fourier Transform", IEEE 1984,
10.1109/TASSP.1984.1164317
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
Generate a test signal, a 2 Vrms sine wave whose frequency is slowly
modulated around 3kHz, corrupted by white noise of exponentially
decreasing magnitude sampled at 10 kHz.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 2 * np.sqrt(2)
>>> noise_power = 0.01 * fs / 2
>>> time = np.arange(N) / float(fs)
>>> mod = 500*np.cos(2*np.pi*0.25*time)
>>> carrier = amp * np.sin(2*np.pi*3e3*time + mod)
>>> noise = np.random.normal(scale=np.sqrt(noise_power),
... size=time.shape)
>>> noise *= np.exp(-time/5)
>>> x = carrier + noise
Compute and plot the STFT's magnitude.
>>> f, t, Zxx = signal.stft(x, fs, nperseg=1000)
>>> plt.pcolormesh(t, f, np.abs(Zxx), vmin=0, vmax=amp, shading='gouraud')
>>> plt.title('STFT Magnitude')
>>> plt.ylabel('Frequency [Hz]')
>>> plt.xlabel('Time [sec]')
>>> plt.show()
"""
freqs, time, Zxx = _spectral_helper(x, x, fs, window, nperseg, noverlap,
nfft, detrend, return_onesided,
scaling='spectrum', axis=axis,
mode='stft', boundary=boundary,
padded=padded)
return freqs, time, Zxx
def istft(Zxx, fs=1.0, window='hann', nperseg=None, noverlap=None, nfft=None,
input_onesided=True, boundary=True, time_axis=-1, freq_axis=-2):
r"""
Perform the inverse Short Time Fourier transform (iSTFT).
Parameters
----------
Zxx : array_like
STFT of the signal to be reconstructed. If a purely real array
is passed, it will be cast to a complex data type.
fs : float, optional
Sampling frequency of the time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window. Must match the window used to generate the
STFT for faithful inversion.
nperseg : int, optional
Number of data points corresponding to each STFT segment. This
parameter must be specified if the number of data points per
segment is odd, or if the STFT was padded via ``nfft >
nperseg``. If `None`, the value depends on the shape of
`Zxx` and `input_onesided`. If `input_onesided` is `True`,
``nperseg=2*(Zxx.shape[freq_axis] - 1)``. Otherwise,
``nperseg=Zxx.shape[freq_axis]``. Defaults to `None`.
noverlap : int, optional
Number of points to overlap between segments. If `None`, half
of the segment length. Defaults to `None`. When specified, the
COLA constraint must be met (see Notes below), and should match
the parameter used to generate the STFT. Defaults to `None`.
nfft : int, optional
Number of FFT points corresponding to each STFT segment. This
parameter must be specified if the STFT was padded via ``nfft >
nperseg``. If `None`, the default values are the same as for
`nperseg`, detailed above, with one exception: if
`input_onesided` is True and
``nperseg==2*Zxx.shape[freq_axis] - 1``, `nfft` also takes on
that value. This case allows the proper inversion of an
odd-length unpadded STFT using ``nfft=None``. Defaults to
`None`.
input_onesided : bool, optional
If `True`, interpret the input array as one-sided FFTs, such
as is returned by `stft` with ``return_onesided=True`` and
`numpy.fft.rfft`. If `False`, interpret the input as a a
two-sided FFT. Defaults to `True`.
boundary : bool, optional
Specifies whether the input signal was extended at its
boundaries by supplying a non-`None` ``boundary`` argument to
`stft`. Defaults to `True`.
time_axis : int, optional
Where the time segments of the STFT is located; the default is
the last axis (i.e. ``axis=-1``).
freq_axis : int, optional
Where the frequency axis of the STFT is located; the default is
the penultimate axis (i.e. ``axis=-2``).
Returns
-------
t : ndarray
Array of output data times.
x : ndarray
iSTFT of `Zxx`.
See Also
--------
stft: Short Time Fourier Transform
check_COLA: Check whether the Constant OverLap Add (COLA) constraint
is met
check_NOLA: Check whether the Nonzero Overlap Add (NOLA) constraint is met
Notes
-----
In order to enable inversion of an STFT via the inverse STFT with
`istft`, the signal windowing must obey the constraint of "nonzero
overlap add" (NOLA):
.. math:: \sum_{t}w^{2}[n-tH] \ne 0
This ensures that the normalization factors that appear in the denominator
of the overlap-add reconstruction equation
.. math:: x[n]=\frac{\sum_{t}x_{t}[n]w[n-tH]}{\sum_{t}w^{2}[n-tH]}
are not zero. The NOLA constraint can be checked with the `check_NOLA`
function.
An STFT which has been modified (via masking or otherwise) is not
guaranteed to correspond to a exactly realizible signal. This
function implements the iSTFT via the least-squares estimation
algorithm detailed in [2]_, which produces a signal that minimizes
the mean squared error between the STFT of the returned signal and
the modified STFT.
.. versionadded:: 0.19.0
References
----------
.. [1] Oppenheim, Alan V., Ronald W. Schafer, John R. Buck
"Discrete-Time Signal Processing", Prentice Hall, 1999.
.. [2] Daniel W. Griffin, Jae S. Lim "Signal Estimation from
Modified Short-Time Fourier Transform", IEEE 1984,
10.1109/TASSP.1984.1164317
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
Generate a test signal, a 2 Vrms sine wave at 50Hz corrupted by
0.001 V**2/Hz of white noise sampled at 1024 Hz.
>>> fs = 1024
>>> N = 10*fs
>>> nperseg = 512
>>> amp = 2 * np.sqrt(2)
>>> noise_power = 0.001 * fs / 2
>>> time = np.arange(N) / float(fs)
>>> carrier = amp * np.sin(2*np.pi*50*time)
>>> noise = np.random.normal(scale=np.sqrt(noise_power),
... size=time.shape)
>>> x = carrier + noise
Compute the STFT, and plot its magnitude
>>> f, t, Zxx = signal.stft(x, fs=fs, nperseg=nperseg)
>>> plt.figure()
>>> plt.pcolormesh(t, f, np.abs(Zxx), vmin=0, vmax=amp, shading='gouraud')
>>> plt.ylim([f[1], f[-1]])
>>> plt.title('STFT Magnitude')
>>> plt.ylabel('Frequency [Hz]')
>>> plt.xlabel('Time [sec]')
>>> plt.yscale('log')
>>> plt.show()
Zero the components that are 10% or less of the carrier magnitude,
then convert back to a time series via inverse STFT
>>> Zxx = np.where(np.abs(Zxx) >= amp/10, Zxx, 0)
>>> _, xrec = signal.istft(Zxx, fs)
Compare the cleaned signal with the original and true carrier signals.
>>> plt.figure()
>>> plt.plot(time, x, time, xrec, time, carrier)
>>> plt.xlim([2, 2.1])
>>> plt.xlabel('Time [sec]')
>>> plt.ylabel('Signal')
>>> plt.legend(['Carrier + Noise', 'Filtered via STFT', 'True Carrier'])
>>> plt.show()
Note that the cleaned signal does not start as abruptly as the original,
since some of the coefficients of the transient were also removed:
>>> plt.figure()
>>> plt.plot(time, x, time, xrec, time, carrier)
>>> plt.xlim([0, 0.1])
>>> plt.xlabel('Time [sec]')
>>> plt.ylabel('Signal')
>>> plt.legend(['Carrier + Noise', 'Filtered via STFT', 'True Carrier'])
>>> plt.show()
"""
# Make sure input is an ndarray of appropriate complex dtype
Zxx = np.asarray(Zxx) + 0j
freq_axis = int(freq_axis)
time_axis = int(time_axis)
if Zxx.ndim < 2:
raise ValueError('Input stft must be at least 2d!')
if freq_axis == time_axis:
raise ValueError('Must specify differing time and frequency axes!')
nseg = Zxx.shape[time_axis]
if input_onesided:
# Assume even segment length
n_default = 2*(Zxx.shape[freq_axis] - 1)
else:
n_default = Zxx.shape[freq_axis]
# Check windowing parameters
if nperseg is None:
nperseg = n_default
else:
nperseg = int(nperseg)
if nperseg < 1:
raise ValueError('nperseg must be a positive integer')
if nfft is None:
if (input_onesided) and (nperseg == n_default + 1):
# Odd nperseg, no FFT padding
nfft = nperseg
else:
nfft = n_default
elif nfft < nperseg:
raise ValueError('nfft must be greater than or equal to nperseg.')
else:
nfft = int(nfft)
if noverlap is None:
noverlap = nperseg//2
else:
noverlap = int(noverlap)
if noverlap >= nperseg:
raise ValueError('noverlap must be less than nperseg.')
nstep = nperseg - noverlap
# Rearrange axes if necessary
if time_axis != Zxx.ndim-1 or freq_axis != Zxx.ndim-2:
# Turn negative indices to positive for the call to transpose
if freq_axis < 0:
freq_axis = Zxx.ndim + freq_axis
if time_axis < 0:
time_axis = Zxx.ndim + time_axis
zouter = list(range(Zxx.ndim))
for ax in sorted([time_axis, freq_axis], reverse=True):
zouter.pop(ax)
Zxx = np.transpose(Zxx, zouter+[freq_axis, time_axis])
# Get window as array
if isinstance(window, str) or type(window) is tuple:
win = get_window(window, nperseg)
else:
win = np.asarray(window)
if len(win.shape) != 1:
raise ValueError('window must be 1-D')
if win.shape[0] != nperseg:
raise ValueError('window must have length of {0}'.format(nperseg))
ifunc = sp_fft.irfft if input_onesided else sp_fft.ifft
xsubs = ifunc(Zxx, axis=-2, n=nfft)[..., :nperseg, :]
# Initialize output and normalization arrays
outputlength = nperseg + (nseg-1)*nstep
x = np.zeros(list(Zxx.shape[:-2])+[outputlength], dtype=xsubs.dtype)
norm = np.zeros(outputlength, dtype=xsubs.dtype)
if np.result_type(win, xsubs) != xsubs.dtype:
win = win.astype(xsubs.dtype)
xsubs *= win.sum() # This takes care of the 'spectrum' scaling
# Construct the output from the ifft segments
# This loop could perhaps be vectorized/strided somehow...
for ii in range(nseg):
# Window the ifft
x[..., ii*nstep:ii*nstep+nperseg] += xsubs[..., ii] * win
norm[..., ii*nstep:ii*nstep+nperseg] += win**2
# Remove extension points
if boundary:
x = x[..., nperseg//2:-(nperseg//2)]
norm = norm[..., nperseg//2:-(nperseg//2)]
# Divide out normalization where non-tiny
if np.sum(norm > 1e-10) != len(norm):
warnings.warn("NOLA condition failed, STFT may not be invertible")
x /= np.where(norm > 1e-10, norm, 1.0)
if input_onesided:
x = x.real
# Put axes back
if x.ndim > 1:
if time_axis != Zxx.ndim-1:
if freq_axis < time_axis:
time_axis -= 1
x = np.rollaxis(x, -1, time_axis)
time = np.arange(x.shape[0])/float(fs)
return time, x
def coherence(x, y, fs=1.0, window='hann', nperseg=None, noverlap=None,
nfft=None, detrend='constant', axis=-1):
r"""
Estimate the magnitude squared coherence estimate, Cxy, of
discrete-time signals X and Y using Welch's method.
``Cxy = abs(Pxy)**2/(Pxx*Pyy)``, where `Pxx` and `Pyy` are power
spectral density estimates of X and Y, and `Pxy` is the cross
spectral density estimate of X and Y.
Parameters
----------
x : array_like
Time series of measurement values
y : array_like
Time series of measurement values
fs : float, optional
Sampling frequency of the `x` and `y` time series. Defaults
to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window.
nperseg : int, optional
Length of each segment. Defaults to None, but if window is str or
tuple, is set to 256, and if window is array_like, is set to the
length of the window.
noverlap: int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 2``. Defaults to `None`.
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
axis : int, optional
Axis along which the coherence is computed for both inputs; the
default is over the last axis (i.e. ``axis=-1``).
Returns
-------
f : ndarray
Array of sample frequencies.
Cxy : ndarray
Magnitude squared coherence of x and y.
See Also
--------
periodogram: Simple, optionally modified periodogram
lombscargle: Lomb-Scargle periodogram for unevenly sampled data
welch: Power spectral density by Welch's method.
csd: Cross spectral density by Welch's method.
Notes
--------
An appropriate amount of overlap will depend on the choice of window
and on your requirements. For the default Hann window an overlap of
50% is a reasonable trade off between accurately estimating the
signal power, while not over counting any of the data. Narrower
windows may require a larger overlap.
.. versionadded:: 0.16.0
References
----------
.. [1] P. Welch, "The use of the fast Fourier transform for the
estimation of power spectra: A method based on time averaging
over short, modified periodograms", IEEE Trans. Audio
Electroacoust. vol. 15, pp. 70-73, 1967.
.. [2] Stoica, Petre, and Randolph Moses, "Spectral Analysis of
Signals" Prentice Hall, 2005
Examples
--------
>>> from scipy import signal
>>> import matplotlib.pyplot as plt
Generate two test signals with some common features.
>>> fs = 10e3
>>> N = 1e5
>>> amp = 20
>>> freq = 1234.0
>>> noise_power = 0.001 * fs / 2
>>> time = np.arange(N) / fs
>>> b, a = signal.butter(2, 0.25, 'low')
>>> x = np.random.normal(scale=np.sqrt(noise_power), size=time.shape)
>>> y = signal.lfilter(b, a, x)
>>> x += amp*np.sin(2*np.pi*freq*time)
>>> y += np.random.normal(scale=0.1*np.sqrt(noise_power), size=time.shape)
Compute and plot the coherence.
>>> f, Cxy = signal.coherence(x, y, fs, nperseg=1024)
>>> plt.semilogy(f, Cxy)
>>> plt.xlabel('frequency [Hz]')
>>> plt.ylabel('Coherence')
>>> plt.show()
"""
freqs, Pxx = welch(x, fs=fs, window=window, nperseg=nperseg,
noverlap=noverlap, nfft=nfft, detrend=detrend,
axis=axis)
_, Pyy = welch(y, fs=fs, window=window, nperseg=nperseg, noverlap=noverlap,
nfft=nfft, detrend=detrend, axis=axis)
_, Pxy = csd(x, y, fs=fs, window=window, nperseg=nperseg,
noverlap=noverlap, nfft=nfft, detrend=detrend, axis=axis)
Cxy = np.abs(Pxy)**2 / Pxx / Pyy
return freqs, Cxy
def _spectral_helper(x, y, fs=1.0, window='hann', nperseg=None, noverlap=None,
nfft=None, detrend='constant', return_onesided=True,
scaling='density', axis=-1, mode='psd', boundary=None,
padded=False):
"""
Calculate various forms of windowed FFTs for PSD, CSD, etc.
This is a helper function that implements the commonality between
the stft, psd, csd, and spectrogram functions. It is not designed to
be called externally. The windows are not averaged over; the result
from each window is returned.
Parameters
---------
x : array_like
Array or sequence containing the data to be analyzed.
y : array_like
Array or sequence containing the data to be analyzed. If this is
the same object in memory as `x` (i.e. ``_spectral_helper(x,
x, ...)``), the extra computations are spared.
fs : float, optional
Sampling frequency of the time series. Defaults to 1.0.
window : str or tuple or array_like, optional
Desired window to use. If `window` is a string or tuple, it is
passed to `get_window` to generate the window values, which are
DFT-even by default. See `get_window` for a list of windows and
required parameters. If `window` is array_like it will be used
directly as the window and its length must be nperseg. Defaults
to a Hann window.
nperseg : int, optional
Length of each segment. Defaults to None, but if window is str or
tuple, is set to 256, and if window is array_like, is set to the
length of the window.
noverlap : int, optional
Number of points to overlap between segments. If `None`,
``noverlap = nperseg // 2``. Defaults to `None`.
nfft : int, optional
Length of the FFT used, if a zero padded FFT is desired. If
`None`, the FFT length is `nperseg`. Defaults to `None`.
detrend : str or function or `False`, optional
Specifies how to detrend each segment. If `detrend` is a
string, it is passed as the `type` argument to the `detrend`
function. If it is a function, it takes a segment and returns a
detrended segment. If `detrend` is `False`, no detrending is
done. Defaults to 'constant'.
return_onesided : bool, optional
If `True`, return a one-sided spectrum for real data. If
`False` return a two-sided spectrum. Defaults to `True`, but for
complex data, a two-sided spectrum is always returned.
scaling : { 'density', 'spectrum' }, optional
Selects between computing the cross spectral density ('density')
where `Pxy` has units of V**2/Hz and computing the cross
spectrum ('spectrum') where `Pxy` has units of V**2, if `x`
and `y` are measured in V and `fs` is measured in Hz.
Defaults to 'density'
axis : int, optional
Axis along which the FFTs are computed; the default is over the
last axis (i.e. ``axis=-1``).
mode: str {'psd', 'stft'}, optional
Defines what kind of return values are expected. Defaults to
'psd'.
boundary : str or None, optional
Specifies whether the input signal is extended at both ends, and
how to generate the new values, in order to center the first
windowed segment on the first input point. This has the benefit
of enabling reconstruction of the first input point when the
employed window function starts at zero. Valid options are
``['even', 'odd', 'constant', 'zeros', None]``. Defaults to
`None`.
padded : bool, optional
Specifies whether the input signal is zero-padded at the end to
make the signal fit exactly into an integer number of window
segments, so that all of the signal is included in the output.
Defaults to `False`. Padding occurs after boundary extension, if
`boundary` is not `None`, and `padded` is `True`.
Returns
-------
freqs : ndarray
Array of sample frequencies.
t : ndarray
Array of times corresponding to each data segment
result : ndarray
Array of output data, contents dependent on *mode* kwarg.
Notes
-----
Adapted from matplotlib.mlab
.. versionadded:: 0.16.0
"""
if mode not in ['psd', 'stft']:
raise ValueError("Unknown value for mode %s, must be one of: "
"{'psd', 'stft'}" % mode)
boundary_funcs = {'even': even_ext,
'odd': odd_ext,
'constant': const_ext,
'zeros': zero_ext,
None: None}
if boundary not in boundary_funcs:
raise ValueError("Unknown boundary option '{0}', must be one of: {1}"
.format(boundary, list(boundary_funcs.keys())))
# If x and y are the same object we can save ourselves some computation.
same_data = y is x
if not same_data and mode != 'psd':
raise ValueError("x and y must be equal if mode is 'stft'")
axis = int(axis)
# Ensure we have np.arrays, get outdtype
x = np.asarray(x)
if not same_data:
y = np.asarray(y)
outdtype = np.result_type(x, y, np.complex64)
else:
outdtype = np.result_type(x, np.complex64)
if not same_data:
# Check if we can broadcast the outer axes together
xouter = list(x.shape)
youter = list(y.shape)
xouter.pop(axis)
youter.pop(axis)
try:
outershape = np.broadcast(np.empty(xouter), np.empty(youter)).shape
except ValueError as e:
raise ValueError('x and y cannot be broadcast together.') from e
if same_data:
if x.size == 0:
return np.empty(x.shape), np.empty(x.shape), np.empty(x.shape)
else:
if x.size == 0 or y.size == 0:
outshape = outershape + (min([x.shape[axis], y.shape[axis]]),)
emptyout = np.rollaxis(np.empty(outshape), -1, axis)
return emptyout, emptyout, emptyout
if x.ndim > 1:
if axis != -1:
x = np.rollaxis(x, axis, len(x.shape))
if not same_data and y.ndim > 1:
y = np.rollaxis(y, axis, len(y.shape))
# Check if x and y are the same length, zero-pad if necessary
if not same_data:
if x.shape[-1] != y.shape[-1]:
if x.shape[-1] < y.shape[-1]:
pad_shape = list(x.shape)
pad_shape[-1] = y.shape[-1] - x.shape[-1]
x = np.concatenate((x, np.zeros(pad_shape)), -1)
else:
pad_shape = list(y.shape)
pad_shape[-1] = x.shape[-1] - y.shape[-1]
y = np.concatenate((y, np.zeros(pad_shape)), -1)
if nperseg is not None: # if specified by user
nperseg = int(nperseg)
if nperseg < 1:
raise ValueError('nperseg must be a positive integer')
# parse window; if array like, then set nperseg = win.shape
win, nperseg = _triage_segments(window, nperseg, input_length=x.shape[-1])
if nfft is None:
nfft = nperseg
elif nfft < nperseg:
raise ValueError('nfft must be greater than or equal to nperseg.')
else:
nfft = int(nfft)
if noverlap is None:
noverlap = nperseg//2
else:
noverlap = int(noverlap)
if noverlap >= nperseg:
raise ValueError('noverlap must be less than nperseg.')
nstep = nperseg - noverlap
# Padding occurs after boundary extension, so that the extended signal ends
# in zeros, instead of introducing an impulse at the end.
# I.e. if x = [..., 3, 2]
# extend then pad -> [..., 3, 2, 2, 3, 0, 0, 0]
# pad then extend -> [..., 3, 2, 0, 0, 0, 2, 3]
if boundary is not None:
ext_func = boundary_funcs[boundary]
x = ext_func(x, nperseg//2, axis=-1)
if not same_data:
y = ext_func(y, nperseg//2, axis=-1)
if padded:
# Pad to integer number of windowed segments
# I.e make x.shape[-1] = nperseg + (nseg-1)*nstep, with integer nseg
nadd = (-(x.shape[-1]-nperseg) % nstep) % nperseg
zeros_shape = list(x.shape[:-1]) + [nadd]
x = np.concatenate((x, np.zeros(zeros_shape)), axis=-1)
if not same_data:
zeros_shape = list(y.shape[:-1]) + [nadd]
y = np.concatenate((y, np.zeros(zeros_shape)), axis=-1)
# Handle detrending and window functions
if not detrend:
def detrend_func(d):
return d
elif not hasattr(detrend, '__call__'):
def detrend_func(d):
return signaltools.detrend(d, type=detrend, axis=-1)
elif axis != -1:
# Wrap this function so that it receives a shape that it could
# reasonably expect to receive.
def detrend_func(d):
d = np.rollaxis(d, -1, axis)
d = detrend(d)
return np.rollaxis(d, axis, len(d.shape))
else:
detrend_func = detrend
if np.result_type(win, np.complex64) != outdtype:
win = win.astype(outdtype)
if scaling == 'density':
scale = 1.0 / (fs * (win*win).sum())
elif scaling == 'spectrum':
scale = 1.0 / win.sum()**2
else:
raise ValueError('Unknown scaling: %r' % scaling)
if mode == 'stft':
scale = np.sqrt(scale)
if return_onesided:
if np.iscomplexobj(x):
sides = 'twosided'
warnings.warn('Input data is complex, switching to '
'return_onesided=False')
else:
sides = 'onesided'
if not same_data:
if np.iscomplexobj(y):
sides = 'twosided'
warnings.warn('Input data is complex, switching to '
'return_onesided=False')
else:
sides = 'twosided'
if sides == 'twosided':
freqs = sp_fft.fftfreq(nfft, 1/fs)
elif sides == 'onesided':
freqs = sp_fft.rfftfreq(nfft, 1/fs)
# Perform the windowed FFTs
result = _fft_helper(x, win, detrend_func, nperseg, noverlap, nfft, sides)
if not same_data:
# All the same operations on the y data
result_y = _fft_helper(y, win, detrend_func, nperseg, noverlap, nfft,
sides)
result = np.conjugate(result) * result_y
elif mode == 'psd':
result = np.conjugate(result) * result
result *= scale
if sides == 'onesided' and mode == 'psd':
if nfft % 2:
result[..., 1:] *= 2
else:
# Last point is unpaired Nyquist freq point, don't double
result[..., 1:-1] *= 2
time = np.arange(nperseg/2, x.shape[-1] - nperseg/2 + 1,
nperseg - noverlap)/float(fs)
if boundary is not None:
time -= (nperseg/2) / fs
result = result.astype(outdtype)
# All imaginary parts are zero anyways
if same_data and mode != 'stft':
result = result.real
# Output is going to have new last axis for time/window index, so a
# negative axis index shifts down one
if axis < 0:
axis -= 1
# Roll frequency axis back to axis where the data came from
result = np.rollaxis(result, -1, axis)
return freqs, time, result
def _fft_helper(x, win, detrend_func, nperseg, noverlap, nfft, sides):
"""
Calculate windowed FFT, for internal use by
scipy.signal._spectral_helper
This is a helper function that does the main FFT calculation for
`_spectral helper`. All input validation is performed there, and the
data axis is assumed to be the last axis of x. It is not designed to
be called externally. The windows are not averaged over; the result
from each window is returned.
Returns
-------
result : ndarray
Array of FFT data
Notes
-----
Adapted from matplotlib.mlab
.. versionadded:: 0.16.0
"""
# Created strided array of data segments
if nperseg == 1 and noverlap == 0:
result = x[..., np.newaxis]
else:
# https://stackoverflow.com/a/5568169
step = nperseg - noverlap
shape = x.shape[:-1]+((x.shape[-1]-noverlap)//step, nperseg)
strides = x.strides[:-1]+(step*x.strides[-1], x.strides[-1])
result = np.lib.stride_tricks.as_strided(x, shape=shape,
strides=strides)
# Detrend each data segment individually
result = detrend_func(result)
# Apply window by multiplication
result = win * result
# Perform the fft. Acts on last axis by default. Zero-pads automatically
if sides == 'twosided':
func = sp_fft.fft
else:
result = result.real
func = sp_fft.rfft
result = func(result, n=nfft)
return result
def _triage_segments(window, nperseg, input_length):
"""
Parses window and nperseg arguments for spectrogram and _spectral_helper.
This is a helper function, not meant to be called externally.
Parameters
----------
window : string, tuple, or ndarray
If window is specified by a string or tuple and nperseg is not
specified, nperseg is set to the default of 256 and returns a window of
that length.
If instead the window is array_like and nperseg is not specified, then
nperseg is set to the length of the window. A ValueError is raised if
the user supplies both an array_like window and a value for nperseg but
nperseg does not equal the length of the window.
nperseg : int
Length of each segment
input_length: int
Length of input signal, i.e. x.shape[-1]. Used to test for errors.
Returns
-------
win : ndarray
window. If function was called with string or tuple than this will hold
the actual array used as a window.
nperseg : int
Length of each segment. If window is str or tuple, nperseg is set to
256. If window is array_like, nperseg is set to the length of the
6
window.
"""
# parse window; if array like, then set nperseg = win.shape
if isinstance(window, str) or isinstance(window, tuple):
# if nperseg not specified
if nperseg is None:
nperseg = 256 # then change to default
if nperseg > input_length:
warnings.warn('nperseg = {0:d} is greater than input length '
' = {1:d}, using nperseg = {1:d}'
.format(nperseg, input_length))
nperseg = input_length
win = get_window(window, nperseg)
else:
win = np.asarray(window)
if len(win.shape) != 1:
raise ValueError('window must be 1-D')
if input_length < win.shape[-1]:
raise ValueError('window is longer than input signal')
if nperseg is None:
nperseg = win.shape[0]
elif nperseg is not None:
if nperseg != win.shape[0]:
raise ValueError("value specified for nperseg is different"
" from length of window")
return win, nperseg
def _median_bias(n):
"""
Returns the bias of the median of a set of periodograms relative to
the mean.
See Appendix B from [1]_ for details.
Parameters
----------
n : int
Numbers of periodograms being averaged.
Returns
-------
bias : float
Calculated bias.
References
----------
.. [1] B. Allen, W.G. Anderson, P.R. Brady, D.A. Brown, J.D.E. Creighton.
"FINDCHIRP: an algorithm for detection of gravitational waves from
inspiraling compact binaries", Physical Review D 85, 2012,
:arxiv:`gr-qc/0509116`
"""
ii_2 = 2 * np.arange(1., (n-1) // 2 + 1)
return 1 + np.sum(1. / (ii_2 + 1) - 1. / ii_2)