Classe « Axes »
Signature de la méthode specgram
def specgram(self, x, NFFT=None, Fs=None, Fc=None, detrend=None, window=None, noverlap=None, cmap=None, xextent=None, pad_to=None, sides=None, scale_by_freq=None, mode=None, scale=None, vmin=None, vmax=None, *, data=None, **kwargs)
Description
specgram.__doc__
Plot a spectrogram.
Compute and plot a spectrogram of data in *x*. Data are split into
*NFFT* length segments and the spectrum of each section is
computed. The windowing function *window* is applied to each
segment, and the amount of overlap of each segment is
specified with *noverlap*. The spectrogram is plotted as a colormap
(using imshow).
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data.
Fs : float, default: 2
The sampling frequency (samples per time unit). It is used to calculate
the Fourier frequencies, *freqs*, in cycles per time unit.
window : callable or ndarray, default: `.window_hanning`
A function or a vector of length *NFFT*. To create window vectors see
`.window_hanning`, `.window_none`, `numpy.blackman`, `numpy.hamming`,
`numpy.bartlett`, `scipy.signal`, `scipy.signal.get_window`, etc. If a
function is passed as the argument, it must take a data segment as an
argument and return the windowed version of the segment.
sides : {'default', 'onesided', 'twosided'}, optional
Which sides of the spectrum to return. 'default' is one-sided for real
data and two-sided for complex data. 'onesided' forces the return of a
one-sided spectrum, while 'twosided' forces two-sided.
pad_to : int, optional
The number of points to which the data segment is padded when performing
the FFT. This can be different from *NFFT*, which specifies the number
of data points used. While not increasing the actual resolution of the
spectrum (the minimum distance between resolvable peaks), this can give
more points in the plot, allowing for more detail. This corresponds to
the *n* parameter in the call to fft(). The default is None, which sets
*pad_to* equal to *NFFT*
NFFT : int, default: 256
The number of data points used in each block for the FFT. A power 2 is
most efficient. This should *NOT* be used to get zero padding, or the
scaling of the result will be incorrect; use *pad_to* for this instead.
detrend : {'none', 'mean', 'linear'} or callable, default: 'none'
The function applied to each segment before fft-ing, designed to remove
the mean or linear trend. Unlike in MATLAB, where the *detrend* parameter
is a vector, in Matplotlib is it a function. The :mod:`~matplotlib.mlab`
module defines `.detrend_none`, `.detrend_mean`, and `.detrend_linear`,
but you can use a custom function as well. You can also use a string to
choose one of the functions: 'none' calls `.detrend_none`. 'mean' calls
`.detrend_mean`. 'linear' calls `.detrend_linear`.
scale_by_freq : bool, default: True
Whether the resulting density values should be scaled by the scaling
frequency, which gives density in units of Hz^-1. This allows for
integration over the returned frequency values. The default is True for
MATLAB compatibility.
mode : {'default', 'psd', 'magnitude', 'angle', 'phase'}
What sort of spectrum to use. Default is 'psd', which takes the
power spectral density. 'magnitude' returns the magnitude
spectrum. 'angle' returns the phase spectrum without unwrapping.
'phase' returns the phase spectrum with unwrapping.
noverlap : int, default: 128
The number of points of overlap between blocks.
scale : {'default', 'linear', 'dB'}
The scaling of the values in the *spec*. 'linear' is no scaling.
'dB' returns the values in dB scale. When *mode* is 'psd',
this is dB power (10 * log10). Otherwise this is dB amplitude
(20 * log10). 'default' is 'dB' if *mode* is 'psd' or
'magnitude' and 'linear' otherwise. This must be 'linear'
if *mode* is 'angle' or 'phase'.
Fc : int, default: 0
The center frequency of *x*, which offsets the x extents of the
plot to reflect the frequency range used when a signal is acquired
and then filtered and downsampled to baseband.
cmap : `.Colormap`, default: :rc:`image.cmap`
xextent : *None* or (xmin, xmax)
The image extent along the x-axis. The default sets *xmin* to the
left border of the first bin (*spectrum* column) and *xmax* to the
right border of the last bin. Note that for *noverlap>0* the width
of the bins is smaller than those of the segments.
**kwargs
Additional keyword arguments are passed on to `~.axes.Axes.imshow`
which makes the specgram image. The origin keyword argument
is not supported.
Returns
-------
spectrum : 2D array
Columns are the periodograms of successive segments.
freqs : 1-D array
The frequencies corresponding to the rows in *spectrum*.
t : 1-D array
The times corresponding to midpoints of segments (i.e., the columns
in *spectrum*).
im : `.AxesImage`
The image created by imshow containing the spectrogram.
See Also
--------
psd
Differs in the default overlap; in returning the mean of the
segment periodograms; in not returning times; and in generating a
line plot instead of colormap.
magnitude_spectrum
A single spectrum, similar to having a single segment when *mode*
is 'magnitude'. Plots a line instead of a colormap.
angle_spectrum
A single spectrum, similar to having a single segment when *mode*
is 'angle'. Plots a line instead of a colormap.
phase_spectrum
A single spectrum, similar to having a single segment when *mode*
is 'phase'. Plots a line instead of a colormap.
Notes
-----
The parameters *detrend* and *scale_by_freq* do only apply when *mode*
is set to 'psd'.
.. note::
In addition to the above described arguments, this function can take
a *data* keyword argument. If such a *data* argument is given,
the following arguments can also be string ``s``, which is
interpreted as ``data[s]`` (unless this raises an exception):
*x*.
Objects passed as **data** must support item access (``data[s]``) and
membership test (``s in data``).
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