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city_retrofit/venv/lib/python3.7/site-packages/matplotlib/mlab.py

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Add virtual environment to the git repository, this isn't 100% right but it's practical at this development point
2020-06-16 10:34:17 -04:00
"""
Numerical python functions written for compatibility with MATLAB
commands with the same names. Most numerical python functions can be found in
the `numpy` and `scipy` libraries. What remains here is code for performing
spectral computations.
Spectral functions
-------------------
`cohere`
Coherence (normalized cross spectral density)
`csd`
Cross spectral density using Welch's average periodogram
`detrend`
Remove the mean or best fit line from an array
`psd`
Power spectral density using Welch's average periodogram
`specgram`
Spectrogram (spectrum over segments of time)
`complex_spectrum`
Return the complex-valued frequency spectrum of a signal
`magnitude_spectrum`
Return the magnitude of the frequency spectrum of a signal
`angle_spectrum`
Return the angle (wrapped phase) of the frequency spectrum of a signal
`phase_spectrum`
Return the phase (unwrapped angle) of the frequency spectrum of a signal
`detrend_mean`
Remove the mean from a line.
`detrend_linear`
Remove the best fit line from a line.
`detrend_none`
Return the original line.
`stride_windows`
Get all windows in an array in a memory-efficient manner
`stride_repeat`
Repeat an array in a memory-efficient manner
`apply_window`
Apply a window along a given axis
"""
import csv
import inspect
from numbers import Number
import numpy as np
import matplotlib.cbook as cbook
from matplotlib import docstring
def window_hanning(x):
'''
Return x times the hanning window of len(x).
See Also
--------
window_none : Another window algorithm.
'''
return np.hanning(len(x))*x
def window_none(x):
'''
No window function; simply return x.
See Also
--------
window_hanning : Another window algorithm.
'''
return x
@cbook.deprecated("3.2")
def apply_window(x, window, axis=0, return_window=None):
'''
Apply the given window to the given 1D or 2D array along the given axis.
Parameters
----------
x : 1D or 2D array or sequence
Array or sequence containing the data.
window : function or array.
Either a function to generate a window or an array with length
*x*.shape[*axis*]
axis : integer
The axis over which to do the repetition.
Must be 0 or 1. The default is 0
return_window : bool
If true, also return the 1D values of the window that was applied
'''
x = np.asarray(x)
if x.ndim < 1 or x.ndim > 2:
raise ValueError('only 1D or 2D arrays can be used')
if axis+1 > x.ndim:
raise ValueError('axis(=%s) out of bounds' % axis)
xshape = list(x.shape)
xshapetarg = xshape.pop(axis)
if np.iterable(window):
if len(window) != xshapetarg:
raise ValueError('The len(window) must be the same as the shape '
'of x for the chosen axis')
windowVals = window
else:
windowVals = window(np.ones(xshapetarg, dtype=x.dtype))
if x.ndim == 1:
if return_window:
return windowVals * x, windowVals
else:
return windowVals * x
xshapeother = xshape.pop()
otheraxis = (axis+1) % 2
windowValsRep = stride_repeat(windowVals, xshapeother, axis=otheraxis)
if return_window:
return windowValsRep * x, windowVals
else:
return windowValsRep * x
def detrend(x, key=None, axis=None):
'''
Return x with its trend removed.
Parameters
----------
x : array or sequence
Array or sequence containing the data.
key : {'default', 'constant', 'mean', 'linear', 'none'} or function
Specifies the detrend algorithm to use. 'default' is 'mean', which is
the same as `detrend_mean`. 'constant' is the same. 'linear' is
the same as `detrend_linear`. 'none' is the same as
`detrend_none`. The default is 'mean'. See the corresponding
functions for more details regarding the algorithms. Can also be a
function that carries out the detrend operation.
axis : integer
The axis along which to do the detrending.
See Also
--------
detrend_mean : Implementation of the 'mean' algorithm.
detrend_linear : Implementation of the 'linear' algorithm.
detrend_none : Implementation of the 'none' algorithm.
'''
if key is None or key in ['constant', 'mean', 'default']:
return detrend(x, key=detrend_mean, axis=axis)
elif key == 'linear':
return detrend(x, key=detrend_linear, axis=axis)
elif key == 'none':
return detrend(x, key=detrend_none, axis=axis)
elif callable(key):
x = np.asarray(x)
if axis is not None and axis + 1 > x.ndim:
raise ValueError(f'axis(={axis}) out of bounds')
if (axis is None and x.ndim == 0) or (not axis and x.ndim == 1):
return key(x)
# try to use the 'axis' argument if the function supports it,
# otherwise use apply_along_axis to do it
try:
return key(x, axis=axis)
except TypeError:
return np.apply_along_axis(key, axis=axis, arr=x)
else:
raise ValueError(
f"Unknown value for key: {key!r}, must be one of: 'default', "
f"'constant', 'mean', 'linear', or a function")
@cbook.deprecated("3.1", alternative="detrend_mean")
def demean(x, axis=0):
'''
Return x minus its mean along the specified axis.
Parameters
----------
x : array or sequence
Array or sequence containing the data
Can have any dimensionality
axis : integer
The axis along which to take the mean. See numpy.mean for a
description of this argument.
See Also
--------
detrend_mean : Same as `demean` except for the default *axis*.
'''
return detrend_mean(x, axis=axis)
def detrend_mean(x, axis=None):
'''
Return x minus the mean(x).
Parameters
----------
x : array or sequence
Array or sequence containing the data
Can have any dimensionality
axis : integer
The axis along which to take the mean. See numpy.mean for a
description of this argument.
See Also
--------
detrend_linear : Another detrend algorithm.
detrend_none : Another detrend algorithm.
detrend : A wrapper around all the detrend algorithms.
'''
x = np.asarray(x)
if axis is not None and axis+1 > x.ndim:
raise ValueError('axis(=%s) out of bounds' % axis)
return x - x.mean(axis, keepdims=True)
def detrend_none(x, axis=None):
'''
Return x: no detrending.
Parameters
----------
x : any object
An object containing the data
axis : integer
This parameter is ignored.
It is included for compatibility with detrend_mean
See Also
--------
detrend_mean : Another detrend algorithm.
detrend_linear : Another detrend algorithm.
detrend : A wrapper around all the detrend algorithms.
'''
return x
def detrend_linear(y):
'''
Return x minus best fit line; 'linear' detrending.
Parameters
----------
y : 0-D or 1-D array or sequence
Array or sequence containing the data
axis : integer
The axis along which to take the mean. See numpy.mean for a
description of this argument.
See Also
--------
detrend_mean : Another detrend algorithm.
detrend_none : Another detrend algorithm.
detrend : A wrapper around all the detrend algorithms.
'''
# This is faster than an algorithm based on linalg.lstsq.
y = np.asarray(y)
if y.ndim > 1:
raise ValueError('y cannot have ndim > 1')
# short-circuit 0-D array.
if not y.ndim:
return np.array(0., dtype=y.dtype)
x = np.arange(y.size, dtype=float)
C = np.cov(x, y, bias=1)
b = C[0, 1]/C[0, 0]
a = y.mean() - b*x.mean()
return y - (b*x + a)
def stride_windows(x, n, noverlap=None, axis=0):
'''
Get all windows of x with length n as a single array,
using strides to avoid data duplication.
.. warning::
It is not safe to write to the output array. Multiple
elements may point to the same piece of memory,
so modifying one value may change others.
Parameters
----------
x : 1D array or sequence
Array or sequence containing the data.
n : integer
The number of data points in each window.
noverlap : integer
The overlap between adjacent windows.
Default is 0 (no overlap)
axis : integer
The axis along which the windows will run.
References
----------
`stackoverflow: Rolling window for 1D arrays in Numpy?
<http://stackoverflow.com/a/6811241>`_
`stackoverflow: Using strides for an efficient moving average filter
<http://stackoverflow.com/a/4947453>`_
'''
if noverlap is None:
noverlap = 0
if noverlap >= n:
raise ValueError('noverlap must be less than n')
if n < 1:
raise ValueError('n cannot be less than 1')
x = np.asarray(x)
if x.ndim != 1:
raise ValueError('only 1-dimensional arrays can be used')
if n == 1 and noverlap == 0:
if axis == 0:
return x[np.newaxis]
else:
return x[np.newaxis].transpose()
if n > x.size:
raise ValueError('n cannot be greater than the length of x')
# np.lib.stride_tricks.as_strided easily leads to memory corruption for
# non integer shape and strides, i.e. noverlap or n. See #3845.
noverlap = int(noverlap)
n = int(n)
step = n - noverlap
if axis == 0:
shape = (n, (x.shape[-1]-noverlap)//step)
strides = (x.strides[0], step*x.strides[0])
else:
shape = ((x.shape[-1]-noverlap)//step, n)
strides = (step*x.strides[0], x.strides[0])
return np.lib.stride_tricks.as_strided(x, shape=shape, strides=strides)
@cbook.deprecated("3.2")
def stride_repeat(x, n, axis=0):
'''
Repeat the values in an array in a memory-efficient manner. Array x is
stacked vertically n times.
.. warning::
It is not safe to write to the output array. Multiple
elements may point to the same piece of memory, so
modifying one value may change others.
Parameters
----------
x : 1D array or sequence
Array or sequence containing the data.
n : integer
The number of time to repeat the array.
axis : integer
The axis along which the data will run.
References
----------
`stackoverflow: Repeat NumPy array without replicating data?
<http://stackoverflow.com/a/5568169>`_
'''
if axis not in [0, 1]:
raise ValueError('axis must be 0 or 1')
x = np.asarray(x)
if x.ndim != 1:
raise ValueError('only 1-dimensional arrays can be used')
if n == 1:
if axis == 0:
return np.atleast_2d(x)
else:
return np.atleast_2d(x).T
if n < 1:
raise ValueError('n cannot be less than 1')
# np.lib.stride_tricks.as_strided easily leads to memory corruption for
# non integer shape and strides, i.e. n. See #3845.
n = int(n)
if axis == 0:
shape = (n, x.size)
strides = (0, x.strides[0])
else:
shape = (x.size, n)
strides = (x.strides[0], 0)
return np.lib.stride_tricks.as_strided(x, shape=shape, strides=strides)
def _spectral_helper(x, y=None, NFFT=None, Fs=None, detrend_func=None,
window=None, noverlap=None, pad_to=None,
sides=None, scale_by_freq=None, mode=None):
'''
This is a helper function that implements the commonality between the
psd, csd, spectrogram and complex, magnitude, angle, and phase spectrums.
It is *NOT* meant to be used outside of mlab and may change at any time.
'''
if y is None:
# if y is None use x for y
same_data = True
else:
# The checks for if y is x are so that we can use the same function to
# implement the core of psd(), csd(), and spectrogram() without doing
# extra calculations. We return the unaveraged Pxy, freqs, and t.
same_data = y is x
if Fs is None:
Fs = 2
if noverlap is None:
noverlap = 0
if detrend_func is None:
detrend_func = detrend_none
if window is None:
window = window_hanning
# if NFFT is set to None use the whole signal
if NFFT is None:
NFFT = 256
if mode is None or mode == 'default':
mode = 'psd'
cbook._check_in_list(
['default', 'psd', 'complex', 'magnitude', 'angle', 'phase'],
mode=mode)
if not same_data and mode != 'psd':
raise ValueError("x and y must be equal if mode is not 'psd'")
# Make sure we're dealing with a numpy array. If y and x were the same
# object to start with, keep them that way
x = np.asarray(x)
if not same_data:
y = np.asarray(y)
if sides is None or sides == 'default':
if np.iscomplexobj(x):
sides = 'twosided'
else:
sides = 'onesided'
cbook._check_in_list(['default', 'onesided', 'twosided'], sides=sides)
# zero pad x and y up to NFFT if they are shorter than NFFT
if len(x) < NFFT:
n = len(x)
x = np.resize(x, NFFT)
x[n:] = 0
if not same_data and len(y) < NFFT:
n = len(y)
y = np.resize(y, NFFT)
y[n:] = 0
if pad_to is None:
pad_to = NFFT
if mode != 'psd':
scale_by_freq = False
elif scale_by_freq is None:
scale_by_freq = True
# For real x, ignore the negative frequencies unless told otherwise
if sides == 'twosided':
numFreqs = pad_to
if pad_to % 2:
freqcenter = (pad_to - 1)//2 + 1
else:
freqcenter = pad_to//2
scaling_factor = 1.
elif sides == 'onesided':
if pad_to % 2:
numFreqs = (pad_to + 1)//2
else:
numFreqs = pad_to//2 + 1
scaling_factor = 2.
if not np.iterable(window):
window = window(np.ones(NFFT, x.dtype))
if len(window) != NFFT:
raise ValueError(
"The window length must match the data's first dimension")
result = stride_windows(x, NFFT, noverlap, axis=0)
result = detrend(result, detrend_func, axis=0)
result = result * window.reshape((-1, 1))
result = np.fft.fft(result, n=pad_to, axis=0)[:numFreqs, :]
freqs = np.fft.fftfreq(pad_to, 1/Fs)[:numFreqs]
if not same_data:
# if same_data is False, mode must be 'psd'
resultY = stride_windows(y, NFFT, noverlap)
resultY = detrend(resultY, detrend_func, axis=0)
resultY = resultY * window.reshape((-1, 1))
resultY = np.fft.fft(resultY, n=pad_to, axis=0)[:numFreqs, :]
result = np.conj(result) * resultY
elif mode == 'psd':
result = np.conj(result) * result
elif mode == 'magnitude':
result = np.abs(result) / np.abs(window).sum()
elif mode == 'angle' or mode == 'phase':
# we unwrap the phase later to handle the onesided vs. twosided case
result = np.angle(result)
elif mode == 'complex':
result /= np.abs(window).sum()
if mode == 'psd':
# Also include scaling factors for one-sided densities and dividing by
# the sampling frequency, if desired. Scale everything, except the DC
# component and the NFFT/2 component:
# if we have a even number of frequencies, don't scale NFFT/2
if not NFFT % 2:
slc = slice(1, -1, None)
# if we have an odd number, just don't scale DC
else:
slc = slice(1, None, None)
result[slc] *= scaling_factor
# MATLAB divides by the sampling frequency so that density function
# has units of dB/Hz and can be integrated by the plotted frequency
# values. Perform the same scaling here.
if scale_by_freq:
result /= Fs
# Scale the spectrum by the norm of the window to compensate for
# windowing loss; see Bendat & Piersol Sec 11.5.2.
result /= (np.abs(window)**2).sum()
else:
# In this case, preserve power in the segment, not amplitude
result /= np.abs(window).sum()**2
t = np.arange(NFFT/2, len(x) - NFFT/2 + 1, NFFT - noverlap)/Fs
if sides == 'twosided':
# center the frequency range at zero
freqs = np.concatenate((freqs[freqcenter:], freqs[:freqcenter]))
result = np.concatenate((result[freqcenter:, :],
result[:freqcenter, :]), 0)
elif not pad_to % 2:
# get the last value correctly, it is negative otherwise
freqs[-1] *= -1
# we unwrap the phase here to handle the onesided vs. twosided case
if mode == 'phase':
result = np.unwrap(result, axis=0)
return result, freqs, t
def _single_spectrum_helper(x, mode, Fs=None, window=None, pad_to=None,
sides=None):
'''
This is a helper function that implements the commonality between the
complex, magnitude, angle, and phase spectrums.
It is *NOT* meant to be used outside of mlab and may change at any time.
'''
cbook._check_in_list(['complex', 'magnitude', 'angle', 'phase'], mode=mode)
if pad_to is None:
pad_to = len(x)
spec, freqs, _ = _spectral_helper(x=x, y=None, NFFT=len(x), Fs=Fs,
detrend_func=detrend_none, window=window,
noverlap=0, pad_to=pad_to,
sides=sides,
scale_by_freq=False,
mode=mode)
if mode != 'complex':
spec = spec.real
if spec.ndim == 2 and spec.shape[1] == 1:
spec = spec[:, 0]
return spec, freqs
# Split out these keyword docs so that they can be used elsewhere
docstring.interpd.update(Spectral=inspect.cleandoc("""
Fs : scalar
The sampling frequency (samples per time unit). It is used
to calculate the Fourier frequencies, freqs, in cycles per time
unit. The default value is 2.
window : callable or ndarray
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. The
default is `window_hanning`. 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'}
Specifies which sides of the spectrum to return. Default gives the
default behavior, which returns one-sided for real data and both
for complex data. 'onesided' forces the return of a one-sided
spectrum, while 'twosided' forces two-sided.
"""))
docstring.interpd.update(Single_Spectrum=inspect.cleandoc("""
pad_to : int
The number of points to which the data segment is padded when
performing the FFT. 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 the length of the
input signal (i.e. no padding).
"""))
docstring.interpd.update(PSD=inspect.cleandoc("""
pad_to : int
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
The number of data points used in each block for the FFT.
A power 2 is most efficient. The default value is 256.
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, optional
Specifies 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.
"""))
@docstring.dedent_interpd
def psd(x, NFFT=None, Fs=None, detrend=None, window=None,
noverlap=None, pad_to=None, sides=None, scale_by_freq=None):
r"""
Compute the power spectral density.
The power spectral density :math:`P_{xx}` by Welch's average
periodogram method. The vector *x* is divided into *NFFT* length
segments. Each segment is detrended by function *detrend* and
windowed by function *window*. *noverlap* gives the length of
the overlap between segments. The :math:`|\mathrm{fft}(i)|^2`
of each segment :math:`i` are averaged to compute :math:`P_{xx}`.
If len(*x*) < *NFFT*, it will be zero padded to *NFFT*.
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data
%(Spectral)s
%(PSD)s
noverlap : integer
The number of points of overlap between segments.
The default value is 0 (no overlap).
Returns
-------
Pxx : 1-D array
The values for the power spectrum `P_{xx}` (real valued)
freqs : 1-D array
The frequencies corresponding to the elements in *Pxx*
References
----------
Bendat & Piersol -- Random Data: Analysis and Measurement Procedures, John
Wiley & Sons (1986)
See Also
--------
specgram
`specgram` differs in the default overlap; in not returning the mean of
the segment periodograms; and in returning the times of the segments.
magnitude_spectrum : returns the magnitude spectrum.
csd : returns the spectral density between two signals.
"""
Pxx, freqs = csd(x=x, y=None, NFFT=NFFT, Fs=Fs, detrend=detrend,
window=window, noverlap=noverlap, pad_to=pad_to,
sides=sides, scale_by_freq=scale_by_freq)
return Pxx.real, freqs
@docstring.dedent_interpd
def csd(x, y, NFFT=None, Fs=None, detrend=None, window=None,
noverlap=None, pad_to=None, sides=None, scale_by_freq=None):
"""
Compute the cross-spectral density.
The cross spectral density :math:`P_{xy}` by Welch's average
periodogram method. The vectors *x* and *y* are divided into
*NFFT* length segments. Each segment is detrended by function
*detrend* and windowed by function *window*. *noverlap* gives
the length of the overlap between segments. The product of
the direct FFTs of *x* and *y* are averaged over each segment
to compute :math:`P_{xy}`, with a scaling to correct for power
loss due to windowing.
If len(*x*) < *NFFT* or len(*y*) < *NFFT*, they will be zero
padded to *NFFT*.
Parameters
----------
x, y : 1-D arrays or sequences
Arrays or sequences containing the data
%(Spectral)s
%(PSD)s
noverlap : integer
The number of points of overlap between segments.
The default value is 0 (no overlap).
Returns
-------
Pxy : 1-D array
The values for the cross spectrum `P_{xy}` before scaling (real valued)
freqs : 1-D array
The frequencies corresponding to the elements in *Pxy*
References
----------
Bendat & Piersol -- Random Data: Analysis and Measurement Procedures, John
Wiley & Sons (1986)
See Also
--------
psd : equivalent to setting ``y = x``.
"""
if NFFT is None:
NFFT = 256
Pxy, freqs, _ = _spectral_helper(x=x, y=y, NFFT=NFFT, Fs=Fs,
detrend_func=detrend, window=window,
noverlap=noverlap, pad_to=pad_to,
sides=sides, scale_by_freq=scale_by_freq,
mode='psd')
if Pxy.ndim == 2:
if Pxy.shape[1] > 1:
Pxy = Pxy.mean(axis=1)
else:
Pxy = Pxy[:, 0]
return Pxy, freqs
@docstring.dedent_interpd
def complex_spectrum(x, Fs=None, window=None, pad_to=None,
sides=None):
"""
Compute the complex-valued frequency spectrum of *x*. Data is padded to a
length of *pad_to* and the windowing function *window* is applied to the
signal.
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data
%(Spectral)s
%(Single_Spectrum)s
Returns
-------
spectrum : 1-D array
The values for the complex spectrum (complex valued)
freqs : 1-D array
The frequencies corresponding to the elements in *spectrum*
See Also
--------
magnitude_spectrum
Returns the absolute value of this function.
angle_spectrum
Returns the angle of this function.
phase_spectrum
Returns the phase (unwrapped angle) of this function.
specgram
Can return the complex spectrum of segments within the signal.
"""
return _single_spectrum_helper(x=x, Fs=Fs, window=window, pad_to=pad_to,
sides=sides, mode='complex')
@docstring.dedent_interpd
def magnitude_spectrum(x, Fs=None, window=None, pad_to=None,
sides=None):
"""
Compute the magnitude (absolute value) of the frequency spectrum of
*x*. Data is padded to a length of *pad_to* and the windowing function
*window* is applied to the signal.
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data
%(Spectral)s
%(Single_Spectrum)s
Returns
-------
spectrum : 1-D array
The values for the magnitude spectrum (real valued)
freqs : 1-D array
The frequencies corresponding to the elements in *spectrum*
See Also
--------
psd
Returns the power spectral density.
complex_spectrum
This function returns the absolute value of `complex_spectrum`.
angle_spectrum
Returns the angles of the corresponding frequencies.
phase_spectrum
Returns the phase (unwrapped angle) of the corresponding frequencies.
specgram
Can return the complex spectrum of segments within the signal.
"""
return _single_spectrum_helper(x=x, Fs=Fs, window=window, pad_to=pad_to,
sides=sides, mode='magnitude')
@docstring.dedent_interpd
def angle_spectrum(x, Fs=None, window=None, pad_to=None,
sides=None):
"""
Compute the angle of the frequency spectrum (wrapped phase spectrum) of
*x*. Data is padded to a length of *pad_to* and the windowing function
*window* is applied to the signal.
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data
%(Spectral)s
%(Single_Spectrum)s
Returns
-------
spectrum : 1-D array
The values for the angle spectrum in radians (real valued)
freqs : 1-D array
The frequencies corresponding to the elements in *spectrum*
See Also
--------
complex_spectrum
This function returns the angle value of `complex_spectrum`.
magnitude_spectrum
Returns the magnitudes of the corresponding frequencies.
phase_spectrum
Returns the phase (unwrapped angle) of the corresponding frequencies.
specgram
Can return the complex spectrum of segments within the signal.
"""
return _single_spectrum_helper(x=x, Fs=Fs, window=window, pad_to=pad_to,
sides=sides, mode='angle')
@docstring.dedent_interpd
def phase_spectrum(x, Fs=None, window=None, pad_to=None,
sides=None):
"""
Compute the phase of the frequency spectrum (unwrapped angle spectrum) of
*x*. Data is padded to a length of *pad_to* and the windowing function
*window* is applied to the signal.
Parameters
----------
x : 1-D array or sequence
Array or sequence containing the data
%(Spectral)s
%(Single_Spectrum)s
Returns
-------
spectrum : 1-D array
The values for the phase spectrum in radians (real valued)
freqs : 1-D array
The frequencies corresponding to the elements in *spectrum*
See Also
--------
complex_spectrum
This function returns the phase value of `complex_spectrum`.
magnitude_spectrum
Returns the magnitudes of the corresponding frequencies.
angle_spectrum
Returns the angle (wrapped phase) of the corresponding frequencies.
specgram
Can return the complex spectrum of segments within the signal.
"""
return _single_spectrum_helper(x=x, Fs=Fs, window=window, pad_to=pad_to,
sides=sides, mode='phase')
@docstring.dedent_interpd
def specgram(x, NFFT=None, Fs=None, detrend=None, window=None,
noverlap=None, pad_to=None, sides=None, scale_by_freq=None,
mode=None):
"""
Compute 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.
Parameters
----------
x : array-like
1-D array or sequence.
%(Spectral)s
%(PSD)s
noverlap : int, optional
The number of points of overlap between blocks. The default
value is 128.
mode : str, optional
What sort of spectrum to use, default is 'psd'.
'psd'
Returns the power spectral density.
'complex'
Returns the complex-valued frequency spectrum.
'magnitude'
Returns the magnitude spectrum.
'angle'
Returns the phase spectrum without unwrapping.
'phase'
Returns the phase spectrum with unwrapping.
Returns
-------
spectrum : array-like
2-D array, columns are the periodograms of successive segments.
freqs : array-like
1-D array, frequencies corresponding to the rows in *spectrum*.
t : array-like
1-D array, the times corresponding to midpoints of segments
(i.e the columns in *spectrum*).
See Also
--------
psd : differs in the overlap and in the return values.
complex_spectrum : similar, but with complex valued frequencies.
magnitude_spectrum : similar single segment when mode is 'magnitude'.
angle_spectrum : similar to single segment when mode is 'angle'.
phase_spectrum : similar to single segment when mode is 'phase'.
Notes
-----
detrend and scale_by_freq only apply when *mode* is set to 'psd'.
"""
if noverlap is None:
noverlap = 128 # default in _spectral_helper() is noverlap = 0
if NFFT is None:
NFFT = 256 # same default as in _spectral_helper()
if len(x) <= NFFT:
cbook._warn_external("Only one segment is calculated since parameter "
"NFFT (=%d) >= signal length (=%d)." %
(NFFT, len(x)))
spec, freqs, t = _spectral_helper(x=x, y=None, NFFT=NFFT, Fs=Fs,
detrend_func=detrend, window=window,
noverlap=noverlap, pad_to=pad_to,
sides=sides,
scale_by_freq=scale_by_freq,
mode=mode)
if mode != 'complex':
spec = spec.real # Needed since helper implements generically
return spec, freqs, t
@docstring.dedent_interpd
def cohere(x, y, NFFT=256, Fs=2, detrend=detrend_none, window=window_hanning,
noverlap=0, pad_to=None, sides='default', scale_by_freq=None):
r"""
The coherence between *x* and *y*. Coherence is the normalized
cross spectral density:
.. math::
C_{xy} = \frac{|P_{xy}|^2}{P_{xx}P_{yy}}
Parameters
----------
x, y
Array or sequence containing the data
%(Spectral)s
%(PSD)s
noverlap : integer
The number of points of overlap between blocks. The default value
is 0 (no overlap).
Returns
-------
The return value is the tuple (*Cxy*, *f*), where *f* are the
frequencies of the coherence vector. For cohere, scaling the
individual densities by the sampling frequency has no effect,
since the factors cancel out.
See Also
--------
:func:`psd`, :func:`csd` :
For information about the methods used to compute :math:`P_{xy}`,
:math:`P_{xx}` and :math:`P_{yy}`.
"""
if len(x) < 2 * NFFT:
raise ValueError(
"Coherence is calculated by averaging over *NFFT* length "
"segments. Your signal is too short for your choice of *NFFT*.")
Pxx, f = psd(x, NFFT, Fs, detrend, window, noverlap, pad_to, sides,
scale_by_freq)
Pyy, f = psd(y, NFFT, Fs, detrend, window, noverlap, pad_to, sides,
scale_by_freq)
Pxy, f = csd(x, y, NFFT, Fs, detrend, window, noverlap, pad_to, sides,
scale_by_freq)
Cxy = np.abs(Pxy) ** 2 / (Pxx * Pyy)
return Cxy, f
def _csv2rec(fname, comments='#', skiprows=0, checkrows=0, delimiter=',',
converterd=None, names=None, missing='', missingd=None,
use_mrecords=False, dayfirst=False, yearfirst=False):
"""
Load data from comma/space/tab delimited file in *fname* into a
numpy record array and return the record array.
If *names* is *None*, a header row is required to automatically
assign the recarray names. The headers will be lower cased,
spaces will be converted to underscores, and illegal attribute
name characters removed. If *names* is not *None*, it is a
sequence of names to use for the column names. In this case, it
is assumed there is no header row.
- *fname*: can be a filename or a file handle. Support for gzipped
files is automatic, if the filename ends in '.gz'
- *comments*: the character used to indicate the start of a comment
in the file, or *None* to switch off the removal of comments
- *skiprows*: is the number of rows from the top to skip
- *checkrows*: is the number of rows to check to validate the column
data type. When set to zero all rows are validated.
- *converterd*: if not *None*, is a dictionary mapping column number or
munged column name to a converter function.
- *names*: if not None, is a list of header names. In this case, no
header will be read from the file
- *missingd* is a dictionary mapping munged column names to field values
which signify that the field does not contain actual data and should
be masked, e.g., '0000-00-00' or 'unused'
- *missing*: a string whose value signals a missing field regardless of
the column it appears in
- *use_mrecords*: if True, return an mrecords.fromrecords record array if
any of the data are missing
- *dayfirst*: default is False so that MM-DD-YY has precedence over
DD-MM-YY. See
http://labix.org/python-dateutil#head-b95ce2094d189a89f80f5ae52a05b4ab7b41af47
for further information.
- *yearfirst*: default is False so that MM-DD-YY has precedence over
YY-MM-DD. See
http://labix.org/python-dateutil#head-b95ce2094d189a89f80f5ae52a05b4ab7b41af47
for further information.
If no rows are found, *None* is returned
"""
if converterd is None:
converterd = dict()
if missingd is None:
missingd = {}
import dateutil.parser
import datetime
fh = cbook.to_filehandle(fname)
delimiter = str(delimiter)
class FH:
"""
For space-delimited files, we want different behavior than
comma or tab. Generally, we want multiple spaces to be
treated as a single separator, whereas with comma and tab we
want multiple commas to return multiple (empty) fields. The
join/strip trick below effects this.
"""
def __init__(self, fh):
self.fh = fh
def close(self):
self.fh.close()
def seek(self, arg):
self.fh.seek(arg)
def fix(self, s):
return ' '.join(s.split())
def __next__(self):
return self.fix(next(self.fh))
def __iter__(self):
for line in self.fh:
yield self.fix(line)
if delimiter == ' ':
fh = FH(fh)
reader = csv.reader(fh, delimiter=delimiter)
def process_skiprows(reader):
if skiprows:
for i, row in enumerate(reader):
if i >= (skiprows-1):
break
return fh, reader
process_skiprows(reader)
def ismissing(name, val):
"Should the value val in column name be masked?"
return val == missing or val == missingd.get(name) or val == ''
def with_default_value(func, default):
def newfunc(name, val):
if ismissing(name, val):
return default
else:
return func(val)
return newfunc
def mybool(x):
if x == 'True':
return True
elif x == 'False':
return False
else:
raise ValueError('invalid bool')
dateparser = dateutil.parser.parse
def mydateparser(x):
# try and return a datetime object
d = dateparser(x, dayfirst=dayfirst, yearfirst=yearfirst)
return d
mydateparser = with_default_value(mydateparser, datetime.datetime(1, 1, 1))
myfloat = with_default_value(float, np.nan)
myint = with_default_value(int, -1)
mystr = with_default_value(str, '')
mybool = with_default_value(mybool, None)
def mydate(x):
# try and return a date object
d = dateparser(x, dayfirst=dayfirst, yearfirst=yearfirst)
if d.hour > 0 or d.minute > 0 or d.second > 0:
raise ValueError('not a date')
return d.date()
mydate = with_default_value(mydate, datetime.date(1, 1, 1))
def get_func(name, item, func):
# promote functions in this order
funcs = [mybool, myint, myfloat, mydate, mydateparser, mystr]
for func in funcs[funcs.index(func):]:
try:
func(name, item)
except Exception:
continue
return func
raise ValueError('Could not find a working conversion function')
# map column names that clash with builtins -- TODO - extend this list
itemd = {
'return': 'return_',
'file': 'file_',
'print': 'print_',
}
def get_converters(reader, comments):
converters = None
i = 0
for row in reader:
if (len(row) and comments is not None and
row[0].startswith(comments)):
continue
if i == 0:
converters = [mybool]*len(row)
if checkrows and i > checkrows:
break
i += 1
for j, (name, item) in enumerate(zip(names, row)):
func = converterd.get(j)
if func is None:
func = converterd.get(name)
if func is None:
func = converters[j]
if len(item.strip()):
func = get_func(name, item, func)
else:
# how should we handle custom converters and defaults?
func = with_default_value(func, None)
converters[j] = func
return converters
# Get header and remove invalid characters
needheader = names is None
if needheader:
for row in reader:
if (len(row) and comments is not None and
row[0].startswith(comments)):
continue
headers = row
break
# remove these chars
delete = set(r"""~!@#$%^&*()-=+~\|}[]{';: /?.>,<""")
delete.add('"')
names = []
seen = dict()
for i, item in enumerate(headers):
item = item.strip().lower().replace(' ', '_')
item = ''.join([c for c in item if c not in delete])
if not len(item):
item = 'column%d' % i
item = itemd.get(item, item)
cnt = seen.get(item, 0)
if cnt > 0:
names.append(item + '_%d' % cnt)
else:
names.append(item)
seen[item] = cnt+1
else:
if isinstance(names, str):
names = [n.strip() for n in names.split(',')]
# get the converter functions by inspecting checkrows
converters = get_converters(reader, comments)
if converters is None:
raise ValueError('Could not find any valid data in CSV file')
# reset the reader and start over
fh.seek(0)
reader = csv.reader(fh, delimiter=delimiter)
process_skiprows(reader)
if needheader:
while True:
# skip past any comments and consume one line of column header
row = next(reader)
if (len(row) and comments is not None and
row[0].startswith(comments)):
continue
break
# iterate over the remaining rows and convert the data to date
# objects, ints, or floats as appropriate
rows = []
rowmasks = []
for i, row in enumerate(reader):
if not len(row):
continue
if comments is not None and row[0].startswith(comments):
continue
# Ensure that the row returned always has the same nr of elements
row.extend([''] * (len(converters) - len(row)))
rows.append([func(name, val)
for func, name, val in zip(converters, names, row)])
rowmasks.append([ismissing(name, val)
for name, val in zip(names, row)])
fh.close()
if not len(rows):
return None
if use_mrecords and np.any(rowmasks):
r = np.ma.mrecords.fromrecords(rows, names=names, mask=rowmasks)
else:
r = np.rec.fromrecords(rows, names=names)
return r
class GaussianKDE:
"""
Representation of a kernel-density estimate using Gaussian kernels.
Parameters
----------
dataset : array-like
Datapoints to estimate from. In case of univariate data this is a 1-D
array, otherwise a 2-D array with shape (# of dims, # of data).
bw_method : str, scalar or callable, optional
The method used to calculate the estimator bandwidth. This can be
'scott', 'silverman', a scalar constant or a callable. If a
scalar, this will be used directly as `kde.factor`. If a
callable, it should take a `GaussianKDE` instance as only
parameter and return a scalar. If None (default), 'scott' is used.
Attributes
----------
dataset : ndarray
The dataset with which `gaussian_kde` was initialized.
dim : int
Number of dimensions.
num_dp : int
Number of datapoints.
factor : float
The bandwidth factor, obtained from `kde.covariance_factor`, with which
the covariance matrix is multiplied.
covariance : ndarray
The covariance matrix of *dataset*, scaled by the calculated bandwidth
(`kde.factor`).
inv_cov : ndarray
The inverse of *covariance*.
Methods
-------
kde.evaluate(points) : ndarray
Evaluate the estimated pdf on a provided set of points.
kde(points) : ndarray
Same as kde.evaluate(points)
"""
# This implementation with minor modification was too good to pass up.
# from scipy: https://github.com/scipy/scipy/blob/master/scipy/stats/kde.py
def __init__(self, dataset, bw_method=None):
self.dataset = np.atleast_2d(dataset)
if not np.array(self.dataset).size > 1:
raise ValueError("`dataset` input should have multiple elements.")
self.dim, self.num_dp = np.array(self.dataset).shape
if bw_method is None:
pass
elif cbook._str_equal(bw_method, 'scott'):
self.covariance_factor = self.scotts_factor
elif cbook._str_equal(bw_method, 'silverman'):
self.covariance_factor = self.silverman_factor
elif isinstance(bw_method, Number):
self._bw_method = 'use constant'
self.covariance_factor = lambda: bw_method
elif callable(bw_method):
self._bw_method = bw_method
self.covariance_factor = lambda: self._bw_method(self)
else:
raise ValueError("`bw_method` should be 'scott', 'silverman', a "
"scalar or a callable")
# Computes the covariance matrix for each Gaussian kernel using
# covariance_factor().
self.factor = self.covariance_factor()
# Cache covariance and inverse covariance of the data
if not hasattr(self, '_data_inv_cov'):
self.data_covariance = np.atleast_2d(
np.cov(
self.dataset,
rowvar=1,
bias=False))
self.data_inv_cov = np.linalg.inv(self.data_covariance)
self.covariance = self.data_covariance * self.factor ** 2
self.inv_cov = self.data_inv_cov / self.factor ** 2
self.norm_factor = (np.sqrt(np.linalg.det(2 * np.pi * self.covariance))
* self.num_dp)
def scotts_factor(self):
return np.power(self.num_dp, -1. / (self.dim + 4))
def silverman_factor(self):
return np.power(
self.num_dp * (self.dim + 2.0) / 4.0, -1. / (self.dim + 4))
# Default method to calculate bandwidth, can be overwritten by subclass
covariance_factor = scotts_factor
def evaluate(self, points):
"""Evaluate the estimated pdf on a set of points.
Parameters
----------
points : (# of dimensions, # of points)-array
Alternatively, a (# of dimensions,) vector can be passed in and
treated as a single point.
Returns
-------
values : (# of points,)-array
The values at each point.
Raises
------
ValueError : if the dimensionality of the input points is different
than the dimensionality of the KDE.
"""
points = np.atleast_2d(points)
dim, num_m = np.array(points).shape
if dim != self.dim:
raise ValueError("points have dimension {}, dataset has dimension "
"{}".format(dim, self.dim))
result = np.zeros(num_m)
if num_m >= self.num_dp:
# there are more points than data, so loop over data
for i in range(self.num_dp):
diff = self.dataset[:, i, np.newaxis] - points
tdiff = np.dot(self.inv_cov, diff)
energy = np.sum(diff * tdiff, axis=0) / 2.0
result = result + np.exp(-energy)
else:
# loop over points
for i in range(num_m):
diff = self.dataset - points[:, i, np.newaxis]
tdiff = np.dot(self.inv_cov, diff)
energy = np.sum(diff * tdiff, axis=0) / 2.0
result[i] = np.sum(np.exp(-energy), axis=0)
result = result / self.norm_factor
return result
__call__ = evaluate
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