typed op• データ種: signal → image
• 呼び出し: fullseye.apply(img, "tb_spectrogram", a=0.5, b=0.5) (2-D は 1 画像 + 2 スカラつまみ a,b∈[0,1] のモデル)
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.
Typed bridge of the 1d op `spectrogram into the 2-D evolution registry: the same implementation, called under the op(v, a, b) convention. a drives rate (default 1) and b drives win` (default 256).
• サンプルデータ カタログ(DL URL / ライセンス) — 2-D は skimage.data(BSD/public)+ 合成、3-D は実データ源(Stanford/PDS 等)の DL URL。
• 演算子の来歴・参考文献 — この op 族の元になった研究/手法の出典。
• (まだありません)
image を入力に取れる)identity · gaussian · mean_box · bilateral · unsharp · median · min_filter · max_filter
typed)tb_points_to_voxel · tb_estimate_point_normals · tb_iss_keypoints · tb_angle_3points · tb_project_points · tb_render_point_depth · tb_statistical_outlier_removal · tb_radius_outlier_removal
*Provenance: ops.py — 2D 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.