#!/usr/bin/env python # -*- coding: utf-8 -*- """Spectral feature extraction""" import numpy as np import scipy import scipy.signal import scipy.fftpack from .. import util from .. import filters from ..util.exceptions import ParameterError from ..util.decorators import deprecate_positional_args from ..core.convert import fft_frequencies from ..core.audio import zero_crossings from ..core.spectrum import power_to_db, _spectrogram from ..core.constantq import cqt, hybrid_cqt from ..core.pitch import estimate_tuning __all__ = [ "spectral_centroid", "spectral_bandwidth", "spectral_contrast", "spectral_rolloff", "spectral_flatness", "poly_features", "rms", "zero_crossing_rate", "chroma_stft", "chroma_cqt", "chroma_cens", "melspectrogram", "mfcc", "tonnetz", ] # -- Spectral features -- # @deprecate_positional_args def spectral_centroid( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, freq=None, win_length=None, window="hann", center=True, pad_mode="constant", ): """Compute the spectral centroid. Each frame of a magnitude spectrogram is normalized and treated as a distribution over frequency bins, from which the mean (centroid) is extracted per frame. More precisely, the centroid at frame ``t`` is defined as [#]_:: centroid[t] = sum_k S[k, t] * freq[k] / (sum_j S[j, t]) where ``S`` is a magnitude spectrogram, and ``freq`` is the array of frequencies (e.g., FFT frequencies in Hz) of the rows of ``S``. .. [#] Klapuri, A., & Davy, M. (Eds.). (2007). Signal processing methods for music transcription, chapter 5. Springer Science & Business Media. Parameters ---------- y : np.ndarray [shape=(..., n,)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] audio sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None (optional) spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. freq : None or np.ndarray [shape=(d,) or shape=(d, t)] Center frequencies for spectrogram bins. If `None`, then FFT bin center frequencies are used. Otherwise, it can be a single array of ``d`` center frequencies, or a matrix of center frequencies as constructed by `librosa.reassigned_spectrogram` win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length ``win_length`` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame `t` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. Returns ------- centroid : np.ndarray [shape=(..., 1, t)] centroid frequencies See Also -------- librosa.stft : Short-time Fourier Transform librosa.reassigned_spectrogram : Time-frequency reassigned spectrogram Examples -------- From time-series input: >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> cent = librosa.feature.spectral_centroid(y=y, sr=sr) >>> cent array([[1768.888, 1921.774, ..., 5663.477, 5813.683]]) From spectrogram input: >>> S, phase = librosa.magphase(librosa.stft(y=y)) >>> librosa.feature.spectral_centroid(S=S) array([[1768.888, 1921.774, ..., 5663.477, 5813.683]]) Using variable bin center frequencies: >>> freqs, times, D = librosa.reassigned_spectrogram(y, fill_nan=True) >>> librosa.feature.spectral_centroid(S=np.abs(D), freq=freqs) array([[1768.838, 1921.801, ..., 5663.513, 5813.747]]) Plot the result >>> import matplotlib.pyplot as plt >>> times = librosa.times_like(cent) >>> fig, ax = plt.subplots() >>> librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax) >>> ax.plot(times, cent.T, label='Spectral centroid', color='w') >>> ax.legend(loc='upper right') >>> ax.set(title='log Power spectrogram') """ # input is time domain:y or spectrogram:s # S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) if not np.isrealobj(S): raise ParameterError( "Spectral centroid is only defined " "with real-valued input" ) elif np.any(S < 0): raise ParameterError( "Spectral centroid is only defined " "with non-negative energies" ) # Compute the center frequencies of each bin if freq is None: freq = fft_frequencies(sr=sr, n_fft=n_fft) if freq.ndim == 1: # reshape for broadcasting freq = util.expand_to(freq, ndim=S.ndim, axes=-2) # Column-normalize S return np.sum(freq * util.normalize(S, norm=1, axis=-2), axis=-2, keepdims=True) @deprecate_positional_args def spectral_bandwidth( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", freq=None, centroid=None, norm=True, p=2, ): """Compute p'th-order spectral bandwidth. The spectral bandwidth [#]_ at frame ``t`` is computed by:: (sum_k S[k, t] * (freq[k, t] - centroid[t])**p)**(1/p) .. [#] Klapuri, A., & Davy, M. (Eds.). (2007). Signal processing methods for music transcription, chapter 5. Springer Science & Business Media. Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] audio sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None (optional) spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length ``win_length`` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If ``False``, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. freq : None or np.ndarray [shape=(d,) or shape=(..., d, t)] Center frequencies for spectrogram bins. If `None`, then FFT bin center frequencies are used. Otherwise, it can be a single array of ``d`` center frequencies, or a matrix of center frequencies as constructed by `librosa.reassigned_spectrogram` centroid : None or np.ndarray [shape=(..., 1, t)] pre-computed centroid frequencies norm : bool Normalize per-frame spectral energy (sum to one) p : float > 0 Power to raise deviation from spectral centroid. Returns ------- bandwidth : np.ndarray [shape=(..., 1, t)] frequency bandwidth for each frame Examples -------- From time-series input >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> spec_bw = librosa.feature.spectral_bandwidth(y=y, sr=sr) >>> spec_bw array([[1273.836, 1228.873, ..., 2952.357, 3013.68 ]]) From spectrogram input >>> S, phase = librosa.magphase(librosa.stft(y=y)) >>> librosa.feature.spectral_bandwidth(S=S) array([[1273.836, 1228.873, ..., 2952.357, 3013.68 ]]) Using variable bin center frequencies >>> freqs, times, D = librosa.reassigned_spectrogram(y, fill_nan=True) >>> librosa.feature.spectral_bandwidth(S=np.abs(D), freq=freqs) array([[1274.637, 1228.786, ..., 2952.4 , 3013.735]]) Plot the result >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> times = librosa.times_like(spec_bw) >>> centroid = librosa.feature.spectral_centroid(S=S) >>> ax[0].semilogy(times, spec_bw[0], label='Spectral bandwidth') >>> ax[0].set(ylabel='Hz', xticks=[], xlim=[times.min(), times.max()]) >>> ax[0].legend() >>> ax[0].label_outer() >>> librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax[1]) >>> ax[1].set(title='log Power spectrogram') >>> ax[1].fill_between(times, np.maximum(0, centroid[0] - spec_bw[0]), ... np.minimum(centroid[0] + spec_bw[0], sr/2), ... alpha=0.5, label='Centroid +- bandwidth') >>> ax[1].plot(times, centroid[0], label='Spectral centroid', color='w') >>> ax[1].legend(loc='lower right') """ S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) if not np.isrealobj(S): raise ParameterError( "Spectral bandwidth is only defined " "with real-valued input" ) elif np.any(S < 0): raise ParameterError( "Spectral bandwidth is only defined " "with non-negative energies" ) # centroid or center? if centroid is None: centroid = spectral_centroid( y=y, sr=sr, S=S, n_fft=n_fft, hop_length=hop_length, freq=freq ) # Compute the center frequencies of each bin if freq is None: freq = fft_frequencies(sr=sr, n_fft=n_fft) if freq.ndim == 1: deviation = np.abs( np.subtract.outer(centroid[..., 0, :], freq).swapaxes(-2, -1) ) else: deviation = np.abs(freq - centroid) # Column-normalize S if norm: S = util.normalize(S, norm=1, axis=-2) return np.sum(S * deviation ** p, axis=-2, keepdims=True) ** (1.0 / p) @deprecate_positional_args def spectral_contrast( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", freq=None, fmin=200.0, n_bands=6, quantile=0.02, linear=False, ): """Compute spectral contrast Each frame of a spectrogram ``S`` is divided into sub-bands. For each sub-band, the energy contrast is estimated by comparing the mean energy in the top quantile (peak energy) to that of the bottom quantile (valley energy). High contrast values generally correspond to clear, narrow-band signals, while low contrast values correspond to broad-band noise. [#]_ .. [#] Jiang, Dan-Ning, Lie Lu, Hong-Jiang Zhang, Jian-Hua Tao, and Lian-Hong Cai. "Music type classification by spectral contrast feature." In Multimedia and Expo, 2002. ICME'02. Proceedings. 2002 IEEE International Conference on, vol. 1, pp. 113-116. IEEE, 2002. Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] audio sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None (optional) spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. freq : None or np.ndarray [shape=(d,)] Center frequencies for spectrogram bins. If `None`, then FFT bin center frequencies are used. Otherwise, it can be a single array of ``d`` center frequencies. fmin : float > 0 Frequency cutoff for the first bin ``[0, fmin]`` Subsequent bins will cover ``[fmin, 2*fmin]`, `[2*fmin, 4*fmin]``, etc. n_bands : int > 1 number of frequency bands quantile : float in (0, 1) quantile for determining peaks and valleys linear : bool If `True`, return the linear difference of magnitudes: ``peaks - valleys``. If `False`, return the logarithmic difference: ``log(peaks) - log(valleys)``. Returns ------- contrast : np.ndarray [shape=(..., n_bands + 1, t)] each row of spectral contrast values corresponds to a given octave-based frequency Examples -------- >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> S = np.abs(librosa.stft(y)) >>> contrast = librosa.feature.spectral_contrast(S=S, sr=sr) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> img1 = librosa.display.specshow(librosa.amplitude_to_db(S, ... ref=np.max), ... y_axis='log', x_axis='time', ax=ax[0]) >>> fig.colorbar(img1, ax=[ax[0]], format='%+2.0f dB') >>> ax[0].set(title='Power spectrogram') >>> ax[0].label_outer() >>> img2 = librosa.display.specshow(contrast, x_axis='time', ax=ax[1]) >>> fig.colorbar(img2, ax=[ax[1]]) >>> ax[1].set(ylabel='Frequency bands', title='Spectral contrast') """ S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) # Compute the center frequencies of each bin if freq is None: freq = fft_frequencies(sr=sr, n_fft=n_fft) freq = np.atleast_1d(freq) if freq.ndim != 1 or len(freq) != S.shape[-2]: raise ParameterError( "freq.shape mismatch: expected " "({:d},)".format(S.shape[-2]) ) if n_bands < 1 or not isinstance(n_bands, (int, np.integer)): raise ParameterError("n_bands must be a positive integer") if not 0.0 < quantile < 1.0: raise ParameterError("quantile must lie in the range (0, 1)") if fmin <= 0: raise ParameterError("fmin must be a positive number") octa = np.zeros(n_bands + 2) octa[1:] = fmin * (2.0 ** np.arange(0, n_bands + 1)) if np.any(octa[:-1] >= 0.5 * sr): raise ParameterError( "Frequency band exceeds Nyquist. " "Reduce either fmin or n_bands." ) # shape of valleys and peaks based on spectrogram shape = list(S.shape) shape[-2] = n_bands + 1 valley = np.zeros(shape) peak = np.zeros_like(valley) for k, (f_low, f_high) in enumerate(zip(octa[:-1], octa[1:])): current_band = np.logical_and(freq >= f_low, freq <= f_high) idx = np.flatnonzero(current_band) if k > 0: current_band[idx[0] - 1] = True if k == n_bands: current_band[idx[-1] + 1 :] = True sub_band = S[..., current_band, :] if k < n_bands: sub_band = sub_band[..., :-1, :] # Always take at least one bin from each side idx = np.rint(quantile * np.sum(current_band)) idx = int(np.maximum(idx, 1)) sortedr = np.sort(sub_band, axis=-2) valley[..., k, :] = np.mean(sortedr[..., :idx, :], axis=-2) peak[..., k, :] = np.mean(sortedr[..., -idx:, :], axis=-2) if linear: return peak - valley else: return power_to_db(peak) - power_to_db(valley) @deprecate_positional_args def spectral_rolloff( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", freq=None, roll_percent=0.85, ): """Compute roll-off frequency. The roll-off frequency is defined for each frame as the center frequency for a spectrogram bin such that at least roll_percent (0.85 by default) of the energy of the spectrum in this frame is contained in this bin and the bins below. This can be used to, e.g., approximate the maximum (or minimum) frequency by setting roll_percent to a value close to 1 (or 0). Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] audio sampling rate of ``y`` S : np.ndarray [shape=(d, t)] or None (optional) spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. freq : None or np.ndarray [shape=(d,) or shape=(..., d, t)] Center frequencies for spectrogram bins. If `None`, then FFT bin center frequencies are used. Otherwise, it can be a single array of ``d`` center frequencies, .. note:: ``freq`` is assumed to be sorted in increasing order roll_percent : float [0 < roll_percent < 1] Roll-off percentage. Returns ------- rolloff : np.ndarray [shape=(..., 1, t)] roll-off frequency for each frame Examples -------- From time-series input >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> # Approximate maximum frequencies with roll_percent=0.85 (default) >>> librosa.feature.spectral_rolloff(y=y, sr=sr) array([[2583.984, 3036.182, ..., 9173.145, 9248.511]]) >>> # Approximate maximum frequencies with roll_percent=0.99 >>> rolloff = librosa.feature.spectral_rolloff(y=y, sr=sr, roll_percent=0.99) >>> rolloff array([[ 7192.09 , 6739.893, ..., 10960.4 , 10992.7 ]]) >>> # Approximate minimum frequencies with roll_percent=0.01 >>> rolloff_min = librosa.feature.spectral_rolloff(y=y, sr=sr, roll_percent=0.01) >>> rolloff_min array([[516.797, 538.33 , ..., 764.429, 764.429]]) From spectrogram input >>> S, phase = librosa.magphase(librosa.stft(y)) >>> librosa.feature.spectral_rolloff(S=S, sr=sr) array([[2583.984, 3036.182, ..., 9173.145, 9248.511]]) >>> # With a higher roll percentage: >>> librosa.feature.spectral_rolloff(y=y, sr=sr, roll_percent=0.95) array([[ 3919.043, 3994.409, ..., 10443.604, 10594.336]]) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots() >>> librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax) >>> ax.plot(librosa.times_like(rolloff), rolloff[0], label='Roll-off frequency (0.99)') >>> ax.plot(librosa.times_like(rolloff), rolloff_min[0], color='w', ... label='Roll-off frequency (0.01)') >>> ax.legend(loc='lower right') >>> ax.set(title='log Power spectrogram') """ if not 0.0 < roll_percent < 1.0: raise ParameterError("roll_percent must lie in the range (0, 1)") S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) if not np.isrealobj(S): raise ParameterError( "Spectral rolloff is only defined " "with real-valued input" ) elif np.any(S < 0): raise ParameterError( "Spectral rolloff is only defined " "with non-negative energies" ) # Compute the center frequencies of each bin if freq is None: freq = fft_frequencies(sr=sr, n_fft=n_fft) # Make sure that frequency can be broadcast if freq.ndim == 1: # reshape for broadcasting freq = util.expand_to(freq, ndim=S.ndim, axes=-2) total_energy = np.cumsum(S, axis=-2) # (channels,freq,frames) threshold = roll_percent * total_energy[..., -1, :] # reshape threshold for broadcasting threshold = np.expand_dims(threshold, axis=-2) ind = np.where(total_energy < threshold, np.nan, 1) return np.nanmin(ind * freq, axis=-2, keepdims=True) @deprecate_positional_args def spectral_flatness( *, y=None, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", amin=1e-10, power=2.0, ): """Compute spectral flatness Spectral flatness (or tonality coefficient) is a measure to quantify how much noise-like a sound is, as opposed to being tone-like [#]_. A high spectral flatness (closer to 1.0) indicates the spectrum is similar to white noise. It is often converted to decibel. .. [#] Dubnov, Shlomo "Generalization of spectral flatness measure for non-gaussian linear processes" IEEE Signal Processing Letters, 2004, Vol. 11. Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. S : np.ndarray [shape=(..., d, t)] or None (optional) pre-computed spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If `False`, then frame `t` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. amin : float > 0 [scalar] minimum threshold for ``S`` (=added noise floor for numerical stability) power : float > 0 [scalar] Exponent for the magnitude spectrogram. e.g., 1 for energy, 2 for power, etc. Power spectrogram is usually used for computing spectral flatness. Returns ------- flatness : np.ndarray [shape=(..., 1, t)] spectral flatness for each frame. The returned value is in [0, 1] and often converted to dB scale. Examples -------- From time-series input >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> flatness = librosa.feature.spectral_flatness(y=y) >>> flatness array([[0.001, 0. , ..., 0.218, 0.184]], dtype=float32) From spectrogram input >>> S, phase = librosa.magphase(librosa.stft(y)) >>> librosa.feature.spectral_flatness(S=S) array([[0.001, 0. , ..., 0.218, 0.184]], dtype=float32) From power spectrogram input >>> S, phase = librosa.magphase(librosa.stft(y)) >>> S_power = S ** 2 >>> librosa.feature.spectral_flatness(S=S_power, power=1.0) array([[0.001, 0. , ..., 0.218, 0.184]], dtype=float32) """ if amin <= 0: raise ParameterError("amin must be strictly positive") S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, power=1.0, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) if not np.isrealobj(S): raise ParameterError( "Spectral flatness is only defined " "with real-valued input" ) elif np.any(S < 0): raise ParameterError( "Spectral flatness is only defined " "with non-negative energies" ) S_thresh = np.maximum(amin, S ** power) gmean = np.exp(np.mean(np.log(S_thresh), axis=-2, keepdims=True)) amean = np.mean(S_thresh, axis=-2, keepdims=True) return gmean / amean @deprecate_positional_args def rms( *, y=None, S=None, frame_length=2048, hop_length=512, center=True, pad_mode="constant", ): """Compute root-mean-square (RMS) value for each frame, either from the audio samples ``y`` or from a spectrogram ``S``. Computing the RMS value from audio samples is faster as it doesn't require a STFT calculation. However, using a spectrogram will give a more accurate representation of energy over time because its frames can be windowed, thus prefer using ``S`` if it's already available. Parameters ---------- y : np.ndarray [shape=(..., n)] or None (optional) audio time series. Required if ``S`` is not input. Multi-channel is supported. S : np.ndarray [shape=(..., d, t)] or None (optional) spectrogram magnitude. Required if ``y`` is not input. frame_length : int > 0 [scalar] length of analysis frame (in samples) for energy calculation hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. center : bool If `True` and operating on time-domain input (``y``), pad the signal by ``frame_length//2`` on either side. If operating on spectrogram input, this has no effect. pad_mode : str Padding mode for centered analysis. See `numpy.pad` for valid values. Returns ------- rms : np.ndarray [shape=(..., 1, t)] RMS value for each frame Examples -------- >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> librosa.feature.rms(y=y) array([[1.248e-01, 1.259e-01, ..., 1.845e-05, 1.796e-05]], dtype=float32) Or from spectrogram input >>> S, phase = librosa.magphase(librosa.stft(y)) >>> rms = librosa.feature.rms(S=S) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> times = librosa.times_like(rms) >>> ax[0].semilogy(times, rms[0], label='RMS Energy') >>> ax[0].set(xticks=[]) >>> ax[0].legend() >>> ax[0].label_outer() >>> librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax[1]) >>> ax[1].set(title='log Power spectrogram') Use a STFT window of constant ones and no frame centering to get consistent results with the RMS computed from the audio samples ``y`` >>> S = librosa.magphase(librosa.stft(y, window=np.ones, center=False))[0] >>> librosa.feature.rms(S=S) >>> plt.show() """ if y is not None: if center: padding = [(0, 0) for _ in range(y.ndim)] padding[-1] = (int(frame_length // 2), int(frame_length // 2)) y = np.pad(y, padding, mode=pad_mode) x = util.frame(y, frame_length=frame_length, hop_length=hop_length) # Calculate power power = np.mean(np.abs(x) ** 2, axis=-2, keepdims=True) elif S is not None: # Check the frame length if S.shape[-2] != frame_length // 2 + 1: raise ParameterError( "Since S.shape[-2] is {}, " "frame_length is expected to be {} or {}; " "found {}".format( S.shape[-2], S.shape[-2] * 2 - 2, S.shape[-2] * 2 - 1, frame_length ) ) # power spectrogram x = np.abs(S) ** 2 # Adjust the DC and sr/2 component x[..., 0, :] *= 0.5 if frame_length % 2 == 0: x[..., -1, :] *= 0.5 # Calculate power power = 2 * np.sum(x, axis=-2, keepdims=True) / frame_length ** 2 else: raise ParameterError("Either `y` or `S` must be input.") return np.sqrt(power) @deprecate_positional_args def poly_features( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", order=1, freq=None, ): """Get coefficients of fitting an nth-order polynomial to the columns of a spectrogram. Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] audio sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None (optional) spectrogram magnitude n_fft : int > 0 [scalar] FFT window size hop_length : int > 0 [scalar] hop length for STFT. See `librosa.stft` for details. win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame `t` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. order : int > 0 order of the polynomial to fit freq : None or np.ndarray [shape=(d,) or shape=(..., d, t)] Center frequencies for spectrogram bins. If `None`, then FFT bin center frequencies are used. Otherwise, it can be a single array of ``d`` center frequencies, or a matrix of center frequencies as constructed by `librosa.reassigned_spectrogram` Returns ------- coefficients : np.ndarray [shape=(..., order+1, t)] polynomial coefficients for each frame. ``coefficients[..., 0, :]`` corresponds to the highest degree (``order``), ``coefficients[..., 1, :]`` corresponds to the next highest degree (``order-1``), down to the constant term ``coefficients[..., order, :]``. Examples -------- >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> S = np.abs(librosa.stft(y)) Fit a degree-0 polynomial (constant) to each frame >>> p0 = librosa.feature.poly_features(S=S, order=0) Fit a linear polynomial to each frame >>> p1 = librosa.feature.poly_features(S=S, order=1) Fit a quadratic to each frame >>> p2 = librosa.feature.poly_features(S=S, order=2) Plot the results for comparison >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=4, sharex=True, figsize=(8, 8)) >>> times = librosa.times_like(p0) >>> ax[0].plot(times, p0[0], label='order=0', alpha=0.8) >>> ax[0].plot(times, p1[1], label='order=1', alpha=0.8) >>> ax[0].plot(times, p2[2], label='order=2', alpha=0.8) >>> ax[0].legend() >>> ax[0].label_outer() >>> ax[0].set(ylabel='Constant term ') >>> ax[1].plot(times, p1[0], label='order=1', alpha=0.8) >>> ax[1].plot(times, p2[1], label='order=2', alpha=0.8) >>> ax[1].set(ylabel='Linear term') >>> ax[1].label_outer() >>> ax[1].legend() >>> ax[2].plot(times, p2[0], label='order=2', alpha=0.8) >>> ax[2].set(ylabel='Quadratic term') >>> ax[2].legend() >>> librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax[3]) """ S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) # Compute the center frequencies of each bin if freq is None: freq = fft_frequencies(sr=sr, n_fft=n_fft) if freq.ndim == 1: # If frequencies are constant over frames, then we only need to fit once fitter = np.vectorize( lambda y: np.polyfit(freq, y, order), signature="(f,t)->(d,t)" ) coefficients = fitter(S) else: # Otherwise, we have variable frequencies, and need to fit independently fitter = np.vectorize( lambda x, y: np.polyfit(x, y, order), signature="(f),(f)->(d)" ) # We have to do some axis swapping to preserve layout # otherwise, the new dimension gets put at the end instead of the penultimate position coefficients = fitter(freq.swapaxes(-2, -1), S.swapaxes(-2, -1)).swapaxes( -2, -1 ) return coefficients @deprecate_positional_args def zero_crossing_rate(y, *, frame_length=2048, hop_length=512, center=True, **kwargs): """Compute the zero-crossing rate of an audio time series. Parameters ---------- y : np.ndarray [shape=(..., n)] Audio time series. Multi-channel is supported. frame_length : int > 0 Length of the frame over which to compute zero crossing rates hop_length : int > 0 Number of samples to advance for each frame center : bool If `True`, frames are centered by padding the edges of ``y``. This is similar to the padding in `librosa.stft`, but uses edge-value copies instead of zero-padding. **kwargs : additional keyword arguments See `librosa.zero_crossings` .. note:: By default, the ``pad`` parameter is set to `False`, which differs from the default specified by `librosa.zero_crossings`. Returns ------- zcr : np.ndarray [shape=(..., 1, t)] ``zcr[..., 0, i]`` is the fraction of zero crossings in frame ``i`` See Also -------- librosa.zero_crossings : Compute zero-crossings in a time-series Examples -------- >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> librosa.feature.zero_crossing_rate(y) array([[0.044, 0.074, ..., 0.488, 0.355]]) """ # check if audio is valid util.valid_audio(y, mono=False) if center: padding = [(0, 0) for _ in range(y.ndim)] padding[-1] = (int(frame_length // 2), int(frame_length // 2)) y = np.pad(y, padding, mode="edge") y_framed = util.frame(y, frame_length=frame_length, hop_length=hop_length) kwargs["axis"] = -2 kwargs.setdefault("pad", False) crossings = zero_crossings(y_framed, **kwargs) return np.mean(crossings, axis=-2, keepdims=True) # -- Chroma --# @deprecate_positional_args def chroma_stft( *, y=None, sr=22050, S=None, norm=np.inf, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", tuning=None, n_chroma=12, **kwargs, ): """Compute a chromagram from a waveform or power spectrogram. This implementation is derived from ``chromagram_E`` [#]_ .. [#] Ellis, Daniel P.W. "Chroma feature analysis and synthesis" 2007/04/21 http://labrosa.ee.columbia.edu/matlab/chroma-ansyn/ Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time series. Multi-channel is supported. sr : number > 0 [scalar] sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None power spectrogram norm : float or None Column-wise normalization. See `librosa.util.normalize` for details. If `None`, no normalization is performed. n_fft : int > 0 [scalar] FFT window size if provided ``y, sr`` instead of ``S`` hop_length : int > 0 [scalar] hop length if provided ``y, sr`` instead of ``S`` win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. tuning : float [scalar] or None. Deviation from A440 tuning in fractional chroma bins. If `None`, it is automatically estimated. n_chroma : int > 0 [scalar] Number of chroma bins to produce (12 by default). **kwargs : additional keyword arguments Arguments to parameterize chroma filters. See `librosa.filters.chroma` for details. Returns ------- chromagram : np.ndarray [shape=(..., n_chroma, t)] Normalized energy for each chroma bin at each frame. See Also -------- librosa.filters.chroma : Chroma filter bank construction librosa.util.normalize : Vector normalization Examples -------- >>> y, sr = librosa.load(librosa.ex('nutcracker'), duration=15) >>> librosa.feature.chroma_stft(y=y, sr=sr) array([[1. , 0.962, ..., 0.143, 0.278], [0.688, 0.745, ..., 0.103, 0.162], ..., [0.468, 0.598, ..., 0.18 , 0.342], [0.681, 0.702, ..., 0.553, 1. ]], dtype=float32) Use an energy (magnitude) spectrum instead of power spectrogram >>> S = np.abs(librosa.stft(y)) >>> chroma = librosa.feature.chroma_stft(S=S, sr=sr) >>> chroma array([[1. , 0.973, ..., 0.527, 0.569], [0.774, 0.81 , ..., 0.518, 0.506], ..., [0.624, 0.73 , ..., 0.611, 0.644], [0.766, 0.822, ..., 0.92 , 1. ]], dtype=float32) Use a pre-computed power spectrogram with a larger frame >>> S = np.abs(librosa.stft(y, n_fft=4096))**2 >>> chroma = librosa.feature.chroma_stft(S=S, sr=sr) >>> chroma array([[0.994, 0.873, ..., 0.169, 0.227], [0.735, 0.64 , ..., 0.141, 0.135], ..., [0.6 , 0.937, ..., 0.214, 0.257], [0.743, 0.937, ..., 0.684, 0.815]], dtype=float32) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> img = librosa.display.specshow(librosa.amplitude_to_db(S, ref=np.max), ... y_axis='log', x_axis='time', ax=ax[0]) >>> fig.colorbar(img, ax=[ax[0]]) >>> ax[0].label_outer() >>> img = librosa.display.specshow(chroma, y_axis='chroma', x_axis='time', ax=ax[1]) >>> fig.colorbar(img, ax=[ax[1]]) """ S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, power=2, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) if tuning is None: tuning = estimate_tuning(S=S, sr=sr, bins_per_octave=n_chroma) # Get the filter bank chromafb = filters.chroma( sr=sr, n_fft=n_fft, tuning=tuning, n_chroma=n_chroma, **kwargs ) # Compute raw chroma raw_chroma = np.einsum("cf,...ft->...ct", chromafb, S, optimize=True) # Compute normalization factor for each frame return util.normalize(raw_chroma, norm=norm, axis=-2) @deprecate_positional_args def chroma_cqt( *, y=None, sr=22050, C=None, hop_length=512, fmin=None, norm=np.inf, threshold=0.0, tuning=None, n_chroma=12, n_octaves=7, window=None, bins_per_octave=36, cqt_mode="full", ): r"""Constant-Q chromagram Parameters ---------- y : np.ndarray [shape=(..., n,)] audio time series. Multi-channel is supported. sr : number > 0 sampling rate of ``y`` C : np.ndarray [shape=(..., d, t)] [Optional] a pre-computed constant-Q spectrogram hop_length : int > 0 number of samples between successive chroma frames fmin : float > 0 minimum frequency to analyze in the CQT. Default: `C1 ~= 32.7 Hz` norm : int > 0, +-np.inf, or None Column-wise normalization of the chromagram. threshold : float Pre-normalization energy threshold. Values below the threshold are discarded, resulting in a sparse chromagram. tuning : float Deviation (in fractions of a CQT bin) from A440 tuning n_chroma : int > 0 Number of chroma bins to produce n_octaves : int > 0 Number of octaves to analyze above ``fmin`` window : None or np.ndarray Optional window parameter to `filters.cq_to_chroma` bins_per_octave : int > 0, optional Number of bins per octave in the CQT. Must be an integer multiple of ``n_chroma``. Default: 36 (3 bins per semitone) If `None`, it will match ``n_chroma``. cqt_mode : ['full', 'hybrid'] Constant-Q transform mode Returns ------- chromagram : np.ndarray [shape=(..., n_chroma, t)] The output chromagram See Also -------- librosa.util.normalize librosa.cqt librosa.hybrid_cqt chroma_stft Examples -------- Compare a long-window STFT chromagram to the CQT chromagram >>> y, sr = librosa.load(librosa.ex('nutcracker'), duration=15) >>> chroma_stft = librosa.feature.chroma_stft(y=y, sr=sr, ... n_chroma=12, n_fft=4096) >>> chroma_cq = librosa.feature.chroma_cqt(y=y, sr=sr) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True, sharey=True) >>> librosa.display.specshow(chroma_stft, y_axis='chroma', x_axis='time', ax=ax[0]) >>> ax[0].set(title='chroma_stft') >>> ax[0].label_outer() >>> img = librosa.display.specshow(chroma_cq, y_axis='chroma', x_axis='time', ax=ax[1]) >>> ax[1].set(title='chroma_cqt') >>> fig.colorbar(img, ax=ax) """ cqt_func = {"full": cqt, "hybrid": hybrid_cqt} if bins_per_octave is None: bins_per_octave = n_chroma elif np.remainder(bins_per_octave, n_chroma) != 0: raise ParameterError( "bins_per_octave={} must be an integer " "multiple of n_chroma={}".format(bins_per_octave, n_chroma) ) # Build the CQT if we don't have one already if C is None: C = np.abs( cqt_func[cqt_mode]( y, sr=sr, hop_length=hop_length, fmin=fmin, n_bins=n_octaves * bins_per_octave, bins_per_octave=bins_per_octave, tuning=tuning, ) ) # Map to chroma cq_to_chr = filters.cq_to_chroma( C.shape[-2], bins_per_octave=bins_per_octave, n_chroma=n_chroma, fmin=fmin, window=window, ) chroma = np.einsum("cf,...ft->...ct", cq_to_chr, C, optimize=True) if threshold is not None: chroma[chroma < threshold] = 0.0 # Normalize if norm is not None: chroma = util.normalize(chroma, norm=norm, axis=-2) return chroma @deprecate_positional_args def chroma_cens( *, y=None, sr=22050, C=None, hop_length=512, fmin=None, tuning=None, n_chroma=12, n_octaves=7, bins_per_octave=36, cqt_mode="full", window=None, norm=2, win_len_smooth=41, smoothing_window="hann", ): r"""Computes the chroma variant "Chroma Energy Normalized" (CENS) To compute CENS features, following steps are taken after obtaining chroma vectors using `chroma_cqt`: [#]_. 1. L-1 normalization of each chroma vector 2. Quantization of amplitude based on "log-like" amplitude thresholds 3. (optional) Smoothing with sliding window. Default window length = 41 frames 4. (not implemented) Downsampling CENS features are robust to dynamics, timbre and articulation, thus these are commonly used in audio matching and retrieval applications. .. [#] Meinard Müller and Sebastian Ewert "Chroma Toolbox: MATLAB implementations for extracting variants of chroma-based audio features" In Proceedings of the International Conference on Music Information Retrieval (ISMIR), 2011. Parameters ---------- y : np.ndarray [shape=(..., n,)] audio time series. Multi-channel is supported. sr : number > 0 sampling rate of ``y`` C : np.ndarray [shape=(d, t)] [Optional] a pre-computed constant-Q spectrogram hop_length : int > 0 number of samples between successive chroma frames fmin : float > 0 minimum frequency to analyze in the CQT. Default: `C1 ~= 32.7 Hz` norm : int > 0, +-np.inf, or None Column-wise normalization of the chromagram. tuning : float Deviation (in fractions of a CQT bin) from A440 tuning n_chroma : int > 0 Number of chroma bins to produce n_octaves : int > 0 Number of octaves to analyze above ``fmin`` window : None or np.ndarray Optional window parameter to `filters.cq_to_chroma` bins_per_octave : int > 0 Number of bins per octave in the CQT. Default: 36 cqt_mode : ['full', 'hybrid'] Constant-Q transform mode win_len_smooth : int > 0 or None Length of temporal smoothing window. `None` disables temporal smoothing. Default: 41 smoothing_window : str, float or tuple Type of window function for temporal smoothing. See `librosa.filters.get_window` for possible inputs. Default: 'hann' Returns ------- cens : np.ndarray [shape=(..., n_chroma, t)] The output cens-chromagram See Also -------- chroma_cqt : Compute a chromagram from a constant-Q transform. chroma_stft : Compute a chromagram from an STFT spectrogram or waveform. librosa.filters.get_window : Compute a window function. Examples -------- Compare standard cqt chroma to CENS. >>> y, sr = librosa.load(librosa.ex('nutcracker'), duration=15) >>> chroma_cens = librosa.feature.chroma_cens(y=y, sr=sr) >>> chroma_cq = librosa.feature.chroma_cqt(y=y, sr=sr) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True, sharey=True) >>> img = librosa.display.specshow(chroma_cq, y_axis='chroma', x_axis='time', ax=ax[0]) >>> ax[0].set(title='chroma_cq') >>> ax[0].label_outer() >>> librosa.display.specshow(chroma_cens, y_axis='chroma', x_axis='time', ax=ax[1]) >>> ax[1].set(title='chroma_cens') >>> fig.colorbar(img, ax=ax) """ if not ( (win_len_smooth is None) or (isinstance(win_len_smooth, (int, np.integer)) and win_len_smooth > 0) ): raise ParameterError( "win_len_smooth={} must be a positive integer or None".format( win_len_smooth ) ) chroma = chroma_cqt( y=y, C=C, sr=sr, hop_length=hop_length, fmin=fmin, bins_per_octave=bins_per_octave, tuning=tuning, norm=None, n_chroma=n_chroma, n_octaves=n_octaves, cqt_mode=cqt_mode, window=window, ) # L1-Normalization chroma = util.normalize(chroma, norm=1, axis=-2) # Quantize amplitudes QUANT_STEPS = [0.4, 0.2, 0.1, 0.05] QUANT_WEIGHTS = [0.25, 0.25, 0.25, 0.25] chroma_quant = np.zeros_like(chroma) for cur_quant_step_idx, cur_quant_step in enumerate(QUANT_STEPS): chroma_quant += (chroma > cur_quant_step) * QUANT_WEIGHTS[cur_quant_step_idx] if win_len_smooth: # Apply temporal smoothing win = filters.get_window(smoothing_window, win_len_smooth + 2, fftbins=False) win /= np.sum(win) # reshape for broadcasting win = util.expand_to(win, ndim=chroma_quant.ndim, axes=-1) cens = scipy.ndimage.convolve(chroma_quant, win, mode="constant") else: cens = chroma_quant # L2-Normalization return util.normalize(cens, norm=norm, axis=-2) @deprecate_positional_args def tonnetz(*, y=None, sr=22050, chroma=None, **kwargs): """Computes the tonal centroid features (tonnetz) This representation uses the method of [#]_ to project chroma features onto a 6-dimensional basis representing the perfect fifth, minor third, and major third each as two-dimensional coordinates. .. [#] Harte, C., Sandler, M., & Gasser, M. (2006). "Detecting Harmonic Change in Musical Audio." In Proceedings of the 1st ACM Workshop on Audio and Music Computing Multimedia (pp. 21-26). Santa Barbara, CA, USA: ACM Press. doi:10.1145/1178723.1178727. Parameters ---------- y : np.ndarray [shape=(..., n,)] or None Audio time series. Multi-channel is supported. sr : number > 0 [scalar] sampling rate of ``y`` chroma : np.ndarray [shape=(n_chroma, t)] or None Normalized energy for each chroma bin at each frame. If `None`, a cqt chromagram is performed. **kwargs Additional keyword arguments to `chroma_cqt`, if ``chroma`` is not pre-computed. Returns ------- tonnetz : np.ndarray [shape(..., 6, t)] Tonal centroid features for each frame. Tonnetz dimensions: - 0: Fifth x-axis - 1: Fifth y-axis - 2: Minor x-axis - 3: Minor y-axis - 4: Major x-axis - 5: Major y-axis See Also -------- chroma_cqt : Compute a chromagram from a constant-Q transform. chroma_stft : Compute a chromagram from an STFT spectrogram or waveform. Examples -------- Compute tonnetz features from the harmonic component of a song >>> y, sr = librosa.load(librosa.ex('nutcracker'), duration=10, offset=10) >>> y = librosa.effects.harmonic(y) >>> tonnetz = librosa.feature.tonnetz(y=y, sr=sr) >>> tonnetz array([[ 0.007, -0.026, ..., 0.055, 0.056], [-0.01 , -0.009, ..., -0.012, -0.017], ..., [ 0.006, -0.021, ..., -0.012, -0.01 ], [-0.009, 0.031, ..., -0.05 , -0.037]]) Compare the tonnetz features to `chroma_cqt` >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> img1 = librosa.display.specshow(tonnetz, ... y_axis='tonnetz', x_axis='time', ax=ax[0]) >>> ax[0].set(title='Tonal Centroids (Tonnetz)') >>> ax[0].label_outer() >>> img2 = librosa.display.specshow(librosa.feature.chroma_cqt(y=y, sr=sr), ... y_axis='chroma', x_axis='time', ax=ax[1]) >>> ax[1].set(title='Chroma') >>> fig.colorbar(img1, ax=[ax[0]]) >>> fig.colorbar(img2, ax=[ax[1]]) """ if y is None and chroma is None: raise ParameterError( "Either the audio samples or the chromagram must be " "passed as an argument." ) if chroma is None: chroma = chroma_cqt(y=y, sr=sr, **kwargs) # Generate Transformation matrix dim_map = np.linspace(0, 12, num=chroma.shape[-2], endpoint=False) scale = np.asarray([7.0 / 6, 7.0 / 6, 3.0 / 2, 3.0 / 2, 2.0 / 3, 2.0 / 3]) V = np.multiply.outer(scale, dim_map) # Even rows compute sin() V[::2] -= 0.5 R = np.array([1, 1, 1, 1, 0.5, 0.5]) # Fifths # Minor # Major phi = R[:, np.newaxis] * np.cos(np.pi * V) # Do the transform to tonnetz return np.einsum( "pc,...ci->...pi", phi, util.normalize(chroma, norm=1, axis=-2), optimize=True ) # -- Mel spectrogram and MFCCs -- # @deprecate_positional_args def mfcc( *, y=None, sr=22050, S=None, n_mfcc=20, dct_type=2, norm="ortho", lifter=0, **kwargs ): """Mel-frequency cepstral coefficients (MFCCs) .. warning:: If multi-channel audio input ``y`` is provided, the MFCC calculation will depend on the peak loudness (in decibels) across all channels. The result may differ from independent MFCC calculation of each channel. Parameters ---------- y : np.ndarray [shape=(..., n,)] or None audio time series. Multi-channel is supported.. sr : number > 0 [scalar] sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] or None log-power Mel spectrogram n_mfcc : int > 0 [scalar] number of MFCCs to return dct_type : {1, 2, 3} Discrete cosine transform (DCT) type. By default, DCT type-2 is used. norm : None or 'ortho' If ``dct_type`` is `2 or 3`, setting ``norm='ortho'`` uses an ortho-normal DCT basis. Normalization is not supported for ``dct_type=1``. lifter : number >= 0 If ``lifter>0``, apply *liftering* (cepstral filtering) to the MFCCs:: M[n, :] <- M[n, :] * (1 + sin(pi * (n + 1) / lifter) * lifter / 2) Setting ``lifter >= 2 * n_mfcc`` emphasizes the higher-order coefficients. As ``lifter`` increases, the coefficient weighting becomes approximately linear. **kwargs : additional keyword arguments Arguments to `melspectrogram`, if operating on time series input Returns ------- M : np.ndarray [shape=(..., n_mfcc, t)] MFCC sequence See Also -------- melspectrogram scipy.fftpack.dct Examples -------- Generate mfccs from a time series >>> y, sr = librosa.load(librosa.ex('libri1')) >>> librosa.feature.mfcc(y=y, sr=sr) array([[-565.919, -564.288, ..., -426.484, -434.668], [ 10.305, 12.509, ..., 88.43 , 90.12 ], ..., [ 2.807, 2.068, ..., -6.725, -5.159], [ 2.822, 2.244, ..., -6.198, -6.177]], dtype=float32) Using a different hop length and HTK-style Mel frequencies >>> librosa.feature.mfcc(y=y, sr=sr, hop_length=1024, htk=True) array([[-5.471e+02, -5.464e+02, ..., -4.446e+02, -4.200e+02], [ 1.361e+01, 1.402e+01, ..., 9.764e+01, 9.869e+01], ..., [ 4.097e-01, -2.029e+00, ..., -1.051e+01, -1.130e+01], [-1.119e-01, -1.688e+00, ..., -3.442e+00, -4.687e+00]], dtype=float32) Use a pre-computed log-power Mel spectrogram >>> S = librosa.feature.melspectrogram(y=y, sr=sr, n_mels=128, ... fmax=8000) >>> librosa.feature.mfcc(S=librosa.power_to_db(S)) array([[-559.974, -558.449, ..., -411.96 , -420.458], [ 11.018, 13.046, ..., 76.972, 80.888], ..., [ 2.713, 2.379, ..., 1.464, -2.835], [ 2.712, 2.619, ..., 2.209, 0.648]], dtype=float32) Get more components >>> mfccs = librosa.feature.mfcc(y=y, sr=sr, n_mfcc=40) Visualize the MFCC series >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots(nrows=2, sharex=True) >>> img = librosa.display.specshow(librosa.power_to_db(S, ref=np.max), ... x_axis='time', y_axis='mel', fmax=8000, ... ax=ax[0]) >>> fig.colorbar(img, ax=[ax[0]]) >>> ax[0].set(title='Mel spectrogram') >>> ax[0].label_outer() >>> img = librosa.display.specshow(mfccs, x_axis='time', ax=ax[1]) >>> fig.colorbar(img, ax=[ax[1]]) >>> ax[1].set(title='MFCC') Compare different DCT bases >>> m_slaney = librosa.feature.mfcc(y=y, sr=sr, dct_type=2) >>> m_htk = librosa.feature.mfcc(y=y, sr=sr, dct_type=3) >>> fig, ax = plt.subplots(nrows=2, sharex=True, sharey=True) >>> img1 = librosa.display.specshow(m_slaney, x_axis='time', ax=ax[0]) >>> ax[0].set(title='RASTAMAT / Auditory toolbox (dct_type=2)') >>> fig.colorbar(img, ax=[ax[0]]) >>> img2 = librosa.display.specshow(m_htk, x_axis='time', ax=ax[1]) >>> ax[1].set(title='HTK-style (dct_type=3)') >>> fig.colorbar(img2, ax=[ax[1]]) """ if S is None: # multichannel behavior may be different due to relative noise floor differences between channels S = power_to_db(melspectrogram(y=y, sr=sr, **kwargs)) M = scipy.fftpack.dct(S, axis=-2, type=dct_type, norm=norm)[..., :n_mfcc, :] if lifter > 0: # shape lifter for broadcasting LI = np.sin(np.pi * np.arange(1, 1 + n_mfcc, dtype=M.dtype) / lifter) LI = util.expand_to(LI, ndim=S.ndim, axes=-2) M *= 1 + (lifter / 2) * LI return M elif lifter == 0: return M else: raise ParameterError( "MFCC lifter={} must be a non-negative number".format(lifter) ) @deprecate_positional_args def melspectrogram( *, y=None, sr=22050, S=None, n_fft=2048, hop_length=512, win_length=None, window="hann", center=True, pad_mode="constant", power=2.0, **kwargs, ): """Compute a mel-scaled spectrogram. If a spectrogram input ``S`` is provided, then it is mapped directly onto the mel basis by ``mel_f.dot(S)``. If a time-series input ``y, sr`` is provided, then its magnitude spectrogram ``S`` is first computed, and then mapped onto the mel scale by ``mel_f.dot(S**power)``. By default, ``power=2`` operates on a power spectrum. Parameters ---------- y : np.ndarray [shape=(..., n)] or None audio time-series. Multi-channel is supported. sr : number > 0 [scalar] sampling rate of ``y`` S : np.ndarray [shape=(..., d, t)] spectrogram n_fft : int > 0 [scalar] length of the FFT window hop_length : int > 0 [scalar] number of samples between successive frames. See `librosa.stft` win_length : int <= n_fft [scalar] Each frame of audio is windowed by `window()`. The window will be of length `win_length` and then padded with zeros to match ``n_fft``. If unspecified, defaults to ``win_length = n_fft``. window : string, tuple, number, function, or np.ndarray [shape=(n_fft,)] - a window specification (string, tuple, or number); see `scipy.signal.get_window` - a window function, such as `scipy.signal.windows.hann` - a vector or array of length ``n_fft`` .. see also:: `librosa.filters.get_window` center : boolean - If `True`, the signal ``y`` is padded so that frame ``t`` is centered at ``y[t * hop_length]``. - If `False`, then frame ``t`` begins at ``y[t * hop_length]`` pad_mode : string If ``center=True``, the padding mode to use at the edges of the signal. By default, STFT uses zero padding. power : float > 0 [scalar] Exponent for the magnitude melspectrogram. e.g., 1 for energy, 2 for power, etc. **kwargs : additional keyword arguments Mel filter bank parameters. See `librosa.filters.mel` for details. Returns ------- S : np.ndarray [shape=(..., n_mels, t)] Mel spectrogram See Also -------- librosa.filters.mel : Mel filter bank construction librosa.stft : Short-time Fourier Transform Examples -------- >>> y, sr = librosa.load(librosa.ex('trumpet')) >>> librosa.feature.melspectrogram(y=y, sr=sr) array([[3.837e-06, 1.451e-06, ..., 8.352e-14, 1.296e-11], [2.213e-05, 7.866e-06, ..., 8.532e-14, 1.329e-11], ..., [1.115e-05, 5.192e-06, ..., 3.675e-08, 2.470e-08], [6.473e-07, 4.402e-07, ..., 1.794e-08, 2.908e-08]], dtype=float32) Using a pre-computed power spectrogram would give the same result: >>> D = np.abs(librosa.stft(y))**2 >>> S = librosa.feature.melspectrogram(S=D, sr=sr) Display of mel-frequency spectrogram coefficients, with custom arguments for mel filterbank construction (default is fmax=sr/2): >>> # Passing through arguments to the Mel filters >>> S = librosa.feature.melspectrogram(y=y, sr=sr, n_mels=128, ... fmax=8000) >>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots() >>> S_dB = librosa.power_to_db(S, ref=np.max) >>> img = librosa.display.specshow(S_dB, x_axis='time', ... y_axis='mel', sr=sr, ... fmax=8000, ax=ax) >>> fig.colorbar(img, ax=ax, format='%+2.0f dB') >>> ax.set(title='Mel-frequency spectrogram') """ S, n_fft = _spectrogram( y=y, S=S, n_fft=n_fft, hop_length=hop_length, power=power, win_length=win_length, window=window, center=center, pad_mode=pad_mode, ) # Build a Mel filter mel_basis = filters.mel(sr=sr, n_fft=n_fft, **kwargs) return np.einsum("...ft,mf->...mt", S, mel_basis, optimize=True)