librosa.stft
- librosa.stft(y, *, n_fft=2048, hop_length=None, win_length=None, window='hann', center=True, dtype=None, pad_mode='constant', out=None)[source]
Short-time Fourier transform (STFT).
The STFT represents a signal in the time-frequency domain by computing discrete Fourier transforms (DFT) over short overlapping windows.
This function returns a complex-valued matrix D such that
np.abs(D[..., f, t])
is the magnitude of frequency binf
at framet
, andnp.angle(D[..., f, t])
is the phase of frequency binf
at framet
.
The integers
t
andf
can be converted to physical units by means of the utility functionsframes_to_samples
andfft_frequencies
.- Parameters:
- ynp.ndarray [shape=(…, n)], real-valued
input signal. Multi-channel is supported.
- n_fftint > 0 [scalar]
length of the windowed signal after padding with zeros. The number of rows in the STFT matrix
D
is(1 + n_fft/2)
. The default value,n_fft=2048
samples, corresponds to a physical duration of 93 milliseconds at a sample rate of 22050 Hz, i.e. the default sample rate in librosa. This value is well adapted for music signals. However, in speech processing, the recommended value is 512, corresponding to 23 milliseconds at a sample rate of 22050 Hz. In any case, we recommend settingn_fft
to a power of two for optimizing the speed of the fast Fourier transform (FFT) algorithm.- hop_lengthint > 0 [scalar]
number of audio samples between adjacent STFT columns.
Smaller values increase the number of columns in
D
without affecting the frequency resolution of the STFT.If unspecified, defaults to
win_length // 4
(see below).- win_lengthint <= n_fft [scalar]
Each frame of audio is windowed by
window
of lengthwin_length
and then padded with zeros to matchn_fft
. Padding is added on both the left- and the right-side of the window so that the window is centered within the frame.Smaller values improve the temporal resolution of the STFT (i.e. the ability to discriminate impulses that are closely spaced in time) at the expense of frequency resolution (i.e. the ability to discriminate pure tones that are closely spaced in frequency). This effect is known as the time-frequency localization trade-off and needs to be adjusted according to the properties of the input signal
y
.If unspecified, defaults to
win_length = n_fft
.- windowstring, tuple, number, function, or np.ndarray [shape=(n_fft,)]
Either:
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
Defaults to a raised cosine window (‘hann’), which is adequate for most applications in audio signal processing.
- centerboolean
If
True
, the signaly
is padded so that frameD[:, t]
is centered aty[t * hop_length]
.If
False
, thenD[:, t]
begins aty[t * hop_length]
.Defaults to
True
, which simplifies the alignment ofD
onto a time grid by means oflibrosa.frames_to_samples
. Note, however, thatcenter
must be set to False when analyzing signals withlibrosa.stream
.- dtypenp.dtype, optional
Complex numeric type for
D
. Default is inferred to match the precision of the input signal.- pad_modestring or function
If
center=True
, this argument is passed to np.pad for padding the edges of the signaly
. By default (pad_mode="constant"
),y
is padded on both sides with zeros.Note
Not all padding modes supported by
numpy.pad
are supported here. wrap, mean, maximum, median, and minimum are not supported.Other modes that depend at most on input values at the edges of the signal (e.g., constant, edge, linear_ramp) are supported.
If
center=False
, this argument is ignored.- outnp.ndarray or None
A pre-allocated, complex-valued array to store the STFT results. This must be of compatible shape and dtype for the given input parameters.
If out is larger than necessary for the provided input signal, then only a prefix slice of out will be used.
If not provided, a new array is allocated and returned.
- Returns:
- Dnp.ndarray [shape=(…, 1 + n_fft/2, n_frames), dtype=dtype]
Complex-valued matrix of short-term Fourier transform coefficients.
If a pre-allocated out array is provided, then D will be a reference to out.
If out is larger than necessary, then D will be a sliced view: D = out[…, :n_frames].
See also
istft
Inverse STFT
reassigned_spectrogram
Time-frequency reassigned spectrogram
Notes
This function caches at level 20.
Examples
>>> y, sr = librosa.load(librosa.ex('trumpet')) >>> S = np.abs(librosa.stft(y)) >>> S array([[5.395e-03, 3.332e-03, ..., 9.862e-07, 1.201e-05], [3.244e-03, 2.690e-03, ..., 9.536e-07, 1.201e-05], ..., [7.523e-05, 3.722e-05, ..., 1.188e-04, 1.031e-03], [7.640e-05, 3.944e-05, ..., 5.180e-04, 1.346e-03]], dtype=float32)
Use left-aligned frames, instead of centered frames
>>> S_left = librosa.stft(y, center=False)
Use a shorter hop length
>>> D_short = librosa.stft(y, hop_length=64)
Display a spectrogram
>>> import matplotlib.pyplot as plt >>> fig, ax = plt.subplots() >>> img = librosa.display.specshow(librosa.amplitude_to_db(S, ... ref=np.max), ... y_axis='log', x_axis='time', ax=ax) >>> ax.set_title('Power spectrogram') >>> fig.colorbar(img, ax=ax, format="%+2.0f dB")