signal opsignal → image2dimport fullseye as fs; fs.ledger.spectrogram(x, rate=1.0, win=256, hop=None) (実装を直接呼ぶなら import dsp; dsp.spectrogram(x, rate=1.0, win=256, hop=None)、台帳から引くなら ops1d.get("spectrogram"))fullseye.ledger.spectrogram(...) は宣言 out 型 image2d の値だけを返す(本体は補助情報も返す)。捨てられた側が要るときは fullseye.ledger.spectrogram.raw(...)、または dsp.spectrogram を直接呼ぶ。
(freqs, times, S) — S が本体STFT magnitude spectrogram -> (freqs, times, S) with S shape
(n_freqs, n_frames). Hann-windowed; hop defaults to win//2.
Same raw convention as :func:spectrum, but a different divisor. Each
column is the unnormalised |rfft(frame * hann(win))|, so it is not an
amplitude either — and dividing by 2/win is wrong here, because the
Hann window has already thrown away part of the signal. The correct one-sided
amplitude conversion divides by the window’s coherent gain::
w = np.hanning(win)
amp = S * (2.0 / w.sum()) # bins 1 .. win/2-1; DC / Nyquist: 1/w.sum()
Measured on a unit sine at a bin centre (rate = 16000 Hz, 1000 Hz,
amplitude exactly 1.0, win = 256): the raw column peak is
63.7497786196906; * 2/win gives 0.49804514546633283 (too small by
exactly the Hann coherent gain sum(w)/win = 0.498046875), while
* 2/sum(w) gives 0.9999965273676957. Only the second one is the
amplitude that was actually in the signal.
Peak positions, frame-to-frame ratios and any dB difference are unaffected
by either factor. This function returns magnitudes only — the phase is
discarded, so it cannot be inverted; use acoustics.stft / acoustics.istft
for a round-trip.
py -3.11 examples/acoustic_condition_monitoring.pyimage2d を入力に取れる)—
signal)lowpass · highpass · bandpass · envelope · rms · resample · spectrum · zero_crossing_rate
Provenance: dsp.py — ONED operator registry. この per-op ノートは tools/opdocs.py md が自動生成(手編集しない)。
© 2026 Kazufumi Furuse — Fullseye operator documentation. Licensed under Apache-2.0.