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239 lines
13 KiB
239 lines
13 KiB
1 year ago
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# !/usr/bin/env python3
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# -*- coding: utf-8 -*-
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#
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# Copyright 2016-2099 Ailemon.net
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#
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# This file is part of ASRT Speech Recognition Tool.
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#
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# ASRT is free software: you can redistribute it and/or modify
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# it under the terms of the GNU General Public License as published by
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# the Free Software Foundation, either version 3 of the License, or
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# (at your option) any later version.
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# ASRT is distributed in the hope that it will be useful,
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# but WITHOUT ANY WARRANTY; without even the implied warranty of
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# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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# GNU General Public License for more details.
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#
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# You should have received a copy of the GNU General Public License
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# along with ASRT. If not, see <https://www.gnu.org/licenses/>.
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# ============================================================================
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# calculate filterbank features. Provides e.g. fbank and mfcc features for use in ASR applications
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# Author: James Lyons 2012
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"""
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@author: nl8590687
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ASRT语音识别声学特征基础库模块，一些基础函数实现
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"""
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from __future__ import division
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import numpy
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from scipy.fftpack import dct
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from .sigproc import preemphasis, framesig, powspec
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def calculate_nfft(samplerate, winlen):
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"""Calculates the FFT size as a power of two greater than or equal to
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the number of samples in a single window length.
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Having an FFT less than the window length loses precision by dropping
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many of the samples; a longer FFT than the window allows zero-padding
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of the FFT buffer which is neutral in terms of frequency domain conversion.
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:param samplerate: The sample rate of the signal we are working with, in Hz.
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:param winlen: The length of the analysis window in seconds.
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"""
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window_length_samples = winlen * samplerate
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nfft = 1
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while nfft < window_length_samples:
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nfft *= 2
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return nfft
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def mfcc(signal, samplerate=16000, winlen=0.025, winstep=0.01, numcep=13,
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nfilt=26, nfft=None, lowfreq=0, highfreq=None, preemph=0.97, ceplifter=22, appendEnergy=True,
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winfunc=lambda x: numpy.ones((x,))):
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"""Compute MFCC features from an audio signal.
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:param signal: the audio signal from which to compute features. Should be an N*1 array
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:param samplerate: the sample rate of the signal we are working with, in Hz.
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:param winlen: the length of the analysis window in seconds. Default is 0.025s (25 milliseconds)
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:param winstep: the step between successive windows in seconds. Default is 0.01s (10 milliseconds)
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:param numcep: the number of cepstrum to return, default 13
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:param nfilt: the number of filters in the filterbank, default 26.
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:param nfft: the FFT size. Default is None, which uses the calculate_nfft function to choose the smallest size that does not drop sample data.
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:param lowfreq: lowest band edge of mel filters. In Hz, default is 0.
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:param highfreq: highest band edge of mel filters. In Hz, default is samplerate/2
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:param preemph: apply preemphasis filter with preemph as coefficient. 0 is no filter. Default is 0.97.
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:param ceplifter: apply a lifter to final cepstral coefficients. 0 is no lifter. Default is 22.
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:param appendEnergy: if this is true, the zeroth cepstral coefficient is replaced with the log of the total frame energy.
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:param winfunc: the analysis window to apply to each frame. By default no window is applied. You can use numpy window functions here e.g. winfunc=numpy.hamming
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:returns: A numpy array of size (NUMFRAMES by numcep) containing features. Each row holds 1 feature vector.
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"""
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nfft = nfft or calculate_nfft(samplerate, winlen)
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feat, energy = fbank(signal, samplerate, winlen, winstep, nfilt, nfft, lowfreq, highfreq, preemph, winfunc)
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feat = numpy.log(feat)
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feat = dct(feat, type=2, axis=1, norm='ortho')[:, :numcep]
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feat = lifter(feat, ceplifter)
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if appendEnergy: feat[:, 0] = numpy.log(energy) # replace first cepstral coefficient with log of frame energy
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return feat
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def fbank(signal, samplerate=16000, winlen=0.025, winstep=0.01,
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nfilt=26, nfft=512, lowfreq=0, highfreq=None, preemph=0.97,
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winfunc=lambda x: numpy.ones((x,))):
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"""Compute Mel-filterbank energy features from an audio signal.
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:param signal: the audio signal from which to compute features. Should be an N*1 array
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:param samplerate: the sample rate of the signal we are working with, in Hz.
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:param winlen: the length of the analysis window in seconds. Default is 0.025s (25 milliseconds)
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:param winstep: the step between successive windows in seconds. Default is 0.01s (10 milliseconds)
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:param nfilt: the number of filters in the filterbank, default 26.
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:param nfft: the FFT size. Default is 512.
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:param lowfreq: lowest band edge of mel filters. In Hz, default is 0.
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:param highfreq: highest band edge of mel filters. In Hz, default is samplerate/2
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:param preemph: apply preemphasis filter with preemph as coefficient. 0 is no filter. Default is 0.97.
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:param winfunc: the analysis window to apply to each frame. By default no window is applied. You can use numpy window functions here e.g. winfunc=numpy.hamming
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:returns: 2 values. The first is a numpy array of size (NUMFRAMES by nfilt) containing features. Each row holds 1 feature vector. The
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second return value is the energy in each frame (total energy, unwindowed)
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"""
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highfreq = highfreq or samplerate / 2
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signal = preemphasis(signal, preemph)
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frames = framesig(signal, winlen * samplerate, winstep * samplerate, winfunc)
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pspec = powspec(frames, nfft)
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energy = numpy.sum(pspec, 1) # this stores the total energy in each frame
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energy = numpy.where(energy == 0, numpy.finfo(float).eps, energy) # if energy is zero, we get problems with log
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fb = get_filterbanks(nfilt, nfft, samplerate, lowfreq, highfreq)
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feat = numpy.dot(pspec, fb.T) # compute the filterbank energies
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feat = numpy.where(feat == 0, numpy.finfo(float).eps, feat) # if feat is zero, we get problems with log
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return feat, energy
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def logfbank(signal, samplerate=16000, winlen=0.025, winstep=0.01,
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nfilt=26, nfft=512, lowfreq=0, highfreq=None, preemph=0.97,
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winfunc=lambda x: numpy.ones((x,))):
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"""Compute log Mel-filterbank energy features from an audio signal.
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:param signal: the audio signal from which to compute features. Should be an N*1 array
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:param samplerate: the sample rate of the signal we are working with, in Hz.
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:param winlen: the length of the analysis window in seconds. Default is 0.025s (25 milliseconds)
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:param winstep: the step between successive windows in seconds. Default is 0.01s (10 milliseconds)
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:param nfilt: the number of filters in the filterbank, default 26.
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:param nfft: the FFT size. Default is 512.
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:param lowfreq: lowest band edge of mel filters. In Hz, default is 0.
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:param highfreq: highest band edge of mel filters. In Hz, default is samplerate/2
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:param preemph: apply preemphasis filter with preemph as coefficient. 0 is no filter. Default is 0.97.
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:param winfunc: the analysis window to apply to each frame. By default no window is applied. You can use numpy window functions here e.g. winfunc=numpy.hamming
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:returns: A numpy array of size (NUMFRAMES by nfilt) containing features. Each row holds 1 feature vector.
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"""
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feat, energy = fbank(signal, samplerate, winlen, winstep, nfilt, nfft, lowfreq, highfreq, preemph, winfunc)
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return numpy.log(feat)
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def ssc(signal, samplerate=16000, winlen=0.025, winstep=0.01,
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nfilt=26, nfft=512, lowfreq=0, highfreq=None, preemph=0.97,
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winfunc=lambda x: numpy.ones((x,))):
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"""Compute Spectral Subband Centroid features from an audio signal.
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:param signal: the audio signal from which to compute features. Should be an N*1 array
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:param samplerate: the sample rate of the signal we are working with, in Hz.
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:param winlen: the length of the analysis window in seconds. Default is 0.025s (25 milliseconds)
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:param winstep: the step between successive windows in seconds. Default is 0.01s (10 milliseconds)
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:param nfilt: the number of filters in the filterbank, default 26.
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:param nfft: the FFT size. Default is 512.
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:param lowfreq: lowest band edge of mel filters. In Hz, default is 0.
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:param highfreq: highest band edge of mel filters. In Hz, default is samplerate/2
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:param preemph: apply preemphasis filter with preemph as coefficient. 0 is no filter. Default is 0.97.
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:param winfunc: the analysis window to apply to each frame. By default no window is applied. You can use numpy window functions here e.g. winfunc=numpy.hamming
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:returns: A numpy array of size (NUMFRAMES by nfilt) containing features. Each row holds 1 feature vector.
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"""
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highfreq = highfreq or samplerate / 2
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signal = preemphasis(signal, preemph)
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frames = framesig(signal, winlen * samplerate, winstep * samplerate, winfunc)
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pspec = powspec(frames, nfft)
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pspec = numpy.where(pspec == 0, numpy.finfo(float).eps, pspec) # if things are all zeros we get problems
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fb = get_filterbanks(nfilt, nfft, samplerate, lowfreq, highfreq)
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feat = numpy.dot(pspec, fb.T) # compute the filterbank energies
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R = numpy.tile(numpy.linspace(1, samplerate / 2, numpy.size(pspec, 1)), (numpy.size(pspec, 0), 1))
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return numpy.dot(pspec * R, fb.T) / feat
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def hz2mel(hz):
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"""Convert a value in Hertz to Mels
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:param hz: a value in Hz. This can also be a numpy array, conversion proceeds element-wise.
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:returns: a value in Mels. If an array was passed in, an identical sized array is returned.
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"""
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return 2595 * numpy.log10(1 + hz / 700.)
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def mel2hz(mel):
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"""Convert a value in Mels to Hertz
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:param mel: a value in Mels. This can also be a numpy array, conversion proceeds element-wise.
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:returns: a value in Hertz. If an array was passed in, an identical sized array is returned.
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"""
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return 700 * (10 ** (mel / 2595.0) - 1)
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def get_filterbanks(nfilt=20, nfft=512, samplerate=16000, lowfreq=0, highfreq=None):
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"""Compute a Mel-filterbank. The filters are stored in the rows, the columns correspond
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to fft bins. The filters are returned as an array of size nfilt * (nfft/2 + 1)
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:param nfilt: the number of filters in the filterbank, default 20.
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:param nfft: the FFT size. Default is 512.
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:param samplerate: the sample rate of the signal we are working with, in Hz. Affects mel spacing.
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:param lowfreq: lowest band edge of mel filters, default 0 Hz
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:param highfreq: highest band edge of mel filters, default samplerate/2
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:returns: A numpy array of size nfilt * (nfft/2 + 1) containing filterbank. Each row holds 1 filter.
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"""
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highfreq = highfreq or samplerate / 2
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assert highfreq <= samplerate / 2, "highfreq is greater than samplerate/2"
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# compute points evenly spaced in mels
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lowmel = hz2mel(lowfreq)
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highmel = hz2mel(highfreq)
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melpoints = numpy.linspace(lowmel, highmel, nfilt + 2)
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# our points are in Hz, but we use fft bins, so we have to convert
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# from Hz to fft bin number
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bin = numpy.floor((nfft + 1) * mel2hz(melpoints) / samplerate)
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fbank = numpy.zeros([nfilt, nfft // 2 + 1])
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for j in range(0, nfilt):
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for i in range(int(bin[j]), int(bin[j + 1])):
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fbank[j, i] = (i - bin[j]) / (bin[j + 1] - bin[j])
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for i in range(int(bin[j + 1]), int(bin[j + 2])):
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fbank[j, i] = (bin[j + 2] - i) / (bin[j + 2] - bin[j + 1])
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return fbank
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def lifter(cepstra, L=22):
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"""Apply a cepstral lifter the the matrix of cepstra. This has the effect of increasing the
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magnitude of the high frequency DCT coeffs.
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:param cepstra: the matrix of mel-cepstra, will be numframes * numcep in size.
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:param L: the liftering coefficient to use. Default is 22. L <= 0 disables lifter.
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"""
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if L > 0:
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nframes, ncoeff = numpy.shape(cepstra)
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n = numpy.arange(ncoeff)
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lift = 1 + (L / 2.) * numpy.sin(numpy.pi * n / L)
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return lift * cepstra
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else:
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# values of L <= 0, do nothing
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return cepstra
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def delta(feat, N):
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"""Compute delta features from a feature vector sequence.
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:param feat: A numpy array of size (NUMFRAMES by number of features) containing features. Each row holds 1 feature vector.
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:param N: For each frame, calculate delta features based on preceding and following N frames
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:returns: A numpy array of size (NUMFRAMES by number of features) containing delta features. Each row holds 1 delta feature vector.
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"""
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if N < 1:
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raise ValueError('N must be an integer >= 1')
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NUMFRAMES = len(feat)
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denominator = 2 * sum([i ** 2 for i in range(1, N + 1)])
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delta_feat = numpy.empty_like(feat)
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padded = numpy.pad(feat, ((N, N), (0, 0)), mode='edge') # padded version of feat
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for t in range(NUMFRAMES):
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delta_feat[t] = numpy.dot(numpy.arange(-N, N + 1),
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padded[t: t + 2 * N + 1]) / denominator # [t : t+2*N+1] == [(N+t)-N : (N+t)+N+1]
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return delta_feat
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