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bundles / scipy 1.17.1 / scipy / signal / _spectral_py / spectrogram

function

scipy.signal._spectral_py:spectrogram

source: /scipy/signal/_spectral_py.py :975

Signature

def   spectrogram ( x fs = 1.0 window = ('tukey_periodic', 0.25) nperseg = None noverlap = None nfft = None detrend = constant return_onesided = True scaling = density axis = -1 mode = psd )

Summary

Compute a spectrogram with consecutive Fourier transforms (legacy function).

Extended Summary

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 periodic 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.

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.

Array API Standard Support

spectrogram is not in-scope for support of Python Array API Standard compatible backends other than NumPy.

See dev-arrayapi for more information.

Examples

import numpy as np
from scipy import signal
from scipy.fft import fftshift
import matplotlib.pyplot as plt
rng = np.random.default_rng()
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 = rng.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()
fig-85b0eb49babb5fa9.png
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()
fig-d33de0e9cb3ee714.png

See also

ShortTimeFFT

Newer STFT/ISTFT implementation providing more features, which also includes a ~ShortTimeFFT.spectrogram method.

csd

Cross spectral density by Welch's method.

lombscargle

Lomb-Scargle periodogram for unevenly sampled data

periodogram

Simple, optionally modified periodogram

welch

Power spectral density by Welch's method.

Aliases

  • scipy.signal.spectrogram

Referenced by