stft — ACOUSTICS transform op

資料種類:signaltable

呼叫:import acoustics; acoustics.stft(x, rate, win=256, hop=None, window='hann', nfft=None, scaling='none')(或 opsacoustics.get("stft"))

用法

保留相位且可逆的短時傅立葉變換。

> 以下的詳細說明為原文 —— 摘要與標題已翻譯。

:func:dsp.spectrogram returns magnitudes, which is all a display needs and

strictly less than an analysis needs: a magnitude spectrogram cannot be

turned back into a signal, so there is no path in :mod:dsp that filters or

modifies a signal in the time-frequency plane and comes back. This is that

path, and the test of it is that the round trip is exact.

Returns a dict (the transform plus everything :func:istft needs to undo

it):

`spectra`

complex128 `(n_freqs, n_frames)`, same orientation as

:func:dsp.spectrogram.

`freqs, times`

bin centre frequencies in Hz and frame start times in seconds. Frame

time 0.0 is the first *original* sample, so the leading pad does not

shift the time axis.

**`times[0]` is therefore negative**, and that is the consequence of

the sentence above rather than an error: the first frames start inside

the leading pad. Measured on 1.0 s at 16 kHz with `win=256, hop=128`,

`times[0] = -0.016000 and times[-1] = 1.000000`, a span 1.6 %

wider than the record. Do not hand `times[0] and times[-1]`

straight to a plot's time extent — the picture then claims a

time-frequency surface wider than the recording, whose outermost columns

are half-empty frames. Use `times[interior]`, whose first value is

exactly `0.000000`, for anything that has to line up with the signal.

`rate, win, hop, nfft, length, pad_left, scale`,

`scaling, window, window_values`

the geometry, kept so the inverse needs no arguments.

`nola_min`

the smallest value of the squared-window overlap sum over the original

samples. Reconstruction divides by this sum, so a value of zero means

some sample is not reconstructible; it is refused up front rather than

producing a hole.

`interior`

boolean mask over frames, true for the frames that lie **entirely inside

the original signal**. The transform pads by a full window at each end so

that inversion is exact, and the frames straddling that pad see part

zeros — they are correct as coefficients but they are not representative,

and any statistic averaged over *all* frames is therefore biased low.

Measured on 16384 samples of unit-variance white noise, win = 1024,

hop = 512: the `"density"` spectrum integrates to 0.9073 over all 35

frames and to 0.9933 over the 31 interior ones (the signal's own variance

is 0.9923). :func:spectral_kurtosis uses this mask for exactly that

reason — a half-empty frame looks impulsive.

Normalisation is explicit, because a windowed spectrum has no single

natural amplitude and a plausible-looking dB number is the usual result of

leaving it implicit. `scaling` selects a real factor applied to every

coefficient, recorded as `scale and divided out again by :func:istft`:

• `"none" (default) — the raw rfft` of the windowed frame.

• `"amplitude"2 / sum(w). A sinusoid of amplitude A` sitting on

a bin centre then reads `|Z| = A`. Measured on a 1 kHz, amplitude-0.7

tone at 16 kHz with a 256-sample periodic Hann, over the interior frames:

`|Z|` ranges 0.699999999999999 to 0.700000000000001.

DC and Nyquist read twice their amplitude under this convention (they are

not two-sided), which is the standard caveat and is not corrected for.

• `"density"sqrt(2 / (rate * sum(w**2))), so |Z|**2` is a

single-sided power spectral density in units^2/Hz. Measured on 16384

samples of white noise at 16 kHz (win 1024, hop 512): the PSD integrates

to 0.9933 over the interior frames against the record's own variance

0.9923, and to 0.9073 if the pad frames are included — see `interior`.

Raises `ValueError`: non-1-D / non-finite / complex / masked input,

`rate <= 0, a string or bool rate, hop outside [1, win]`,

`nfft < win`, an unknown window, an all-zero window, a transform over

:data:MAX_STFT_ELEMENTS, and a window/hop pair whose squared overlap sum

touches zero (NOLA violated — the round trip would be silently lossy).

詳細使用指南

acoustic_condition_monitoring 族使用指南

參考(範例資料・文獻)

• 範例資料目錄(下載 URL / 授權) —— 2-D 用 skimage.data(BSD/公有領域)加合成圖,3-D 給出真實資料源(Stanford/PDS 等)的下載 URL。

• 運算子來歷與參考文獻 —— 該運算子族所依據的研究/方法出處。

• 演算法的正典(作者・年份)與用途見上面的族使用指南

可執行的範例(實際呼叫該運算子並已驗證的樣例)

acoustic_condition_monitoringpy -3.11 examples/acoustic_condition_monitoring.py

型別可銜接的下一個運算子(可接受 table 作為輸入)

istft

同類別(transform)

istft · stft_cola_check


*Provenance: acoustics.py — ACOUSTICS 運算子登記表。本條目由 tools/opdocs.py md 自動產生(請勿手動編輯)。*

© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.