librosax.feature.spectral_contrast

spectral_contrast(*, y: Array | None = None, sr: float = 22050, S: Array | None = None, n_fft: int = 2048, hop_length: int = 512, win_length: int | None = None, window: str = 'hann', center: bool = True, pad_mode: str = 'constant', freq: Array | None = None, fmin: float = 200.0, n_bands: int = 6, quantile: float = 0.02, linear: bool = False) → Array[source]

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.

Parameters:

  • y – Audio time series. Multichannel is supported.

  • sr – Audio sampling rate

  • S – (optional) Pre-computed spectrogram magnitude

  • n_fft – FFT window size

  • hop_length – Hop length for STFT

  • win_length – Window length

  • window – Window function

  • center – If True, pad the signal

  • pad_mode – Padding mode

  • freq – Center frequencies for spectrogram bins. If None, FFT bin center frequencies are used.

  • fmin – Frequency cutoff for the first bin [0, fmin] Subsequent bins will cover [fmin, 2*fmin], [2*fmin, 4*fmin], etc.

  • n_bands – Number of frequency bands

  • quantile – Quantile for determining peaks and valleys

  • linear – If True, return the linear difference of magnitudes: peaks - valleys. If False, return the logarithmic difference: log(peaks) - log(valleys).

Returns:

Spectral contrast values [shape=(…, n_bands + 1, t)]

Return type:

jnp.ndarray