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Matlab Analyze Spectrum

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From the author

Analyze signal spectra in MATLAB using nonparametric and parametric estimators. Use when computing frequency content, PSD, power spectrum, spectral peaks, bandwidth, or streaming spectral analysis. Covers pspectrum, pwelch, periodogram, pmtm, pburg, pmusic, rootmusic, plomb, poctave, spectrumAnalyzer, dsp.SpectrumEstimator. TRIGGER: FFT, PSD, power spectrum, spectral analysis, frequency content, bandwidth measurement, spectral leakage, window selection, streaming spectrum, periodicity, resolve close frequencies, multitaper. DO NOT TRIGGER: filter design, spectrogram/time-frequency, audio features.
— the description by MathWorks

AutoGineer summary

Written by AutoGineer from the skill’s own files, not by the author

This skill provides a structured approach to spectral analysis in MATLAB, covering both batch and streaming data processing. It guides users through selecting the appropriate estimator (e.g., pspectrum, pwelch, periodogram, pmtm, pburg) based on signal characteristics like length, uniformity, and spectral content. The skill emphasizes best practices such as proper window selection, unit normalization, and the use of built-in measurement functions for peak detection, bandwidth, and power estimation, while discouraging manual FFT implementations.

What it does

  • Recommends spectral estimators based on signal length and character
  • Provides workflows for batch and streaming spectral analysis
  • Automates peak detection, bandwidth measurement, and power calculation
  • Offers guidance on window selection and leakage control
  • Supports advanced techniques like multitaper and parametric estimation
  • Ensures correct unit normalization and dB conversion

When to use it

  • When computing frequency content, PSD, or power spectrum
  • When analyzing signal periodicity or resolving close frequencies
  • When performing real-time streaming spectral analysis
  • When comparing frequency content between two signals
  • When measuring band power or occupied bandwidth

Advantages

  • Reduces errors by using built-in, calibrated functions
  • Provides clear decision trees for estimator selection
  • Standardizes spectral visualization and measurement
  • Includes verification steps like Parseval's theorem
  • Handles complex scenarios like non-uniform sampling

Usage examples

“How do I compute the PSD of a long signal in MATLAB?”
The agent will recommend using pwelch for low-variance PSD estimation, providing code to set segment length and windowing for optimal resolution.
“I need to find the dominant frequency peaks in my signal.”
The agent will guide you to use findpeaks on the spectral output, including advice on setting prominence and distance thresholds.
“How can I perform real-time spectral analysis?”
The agent will direct you to use spectrumAnalyzer or dsp.SpectrumEstimator from the DSP System Toolbox for frame-by-frame processing.
“Which window should I use to resolve two close frequencies?”
The agent will suggest using a Hann or Kaiser window and explain the trade-off between main-lobe width and sidelobe suppression.

Install

  1. Download the skill as a ZIP:

    https://autogineer.com/agent-skills/matlab/matlab-analyze-spectrum/download
  2. Unzip it into the cross-client skills folder of your project:

    mkdir -p .agents/skills && unzip matlab-analyze-spectrum.zip -d .agents/skills

Documentation by MathWorks

Analyze Signal Spectra in MATLAB

Compute, visualize, and extract measurements from signal spectra using Signal Processing Toolbox. Choose the right spectral estimator, avoid common FFT pitfalls, and use built-in measurement functions instead of reinventing them.

When to Use

  • Computing frequency content of a signal (FFT, periodogram, PSD, power spectrum)

  • Estimating power spectral density (Welch, periodogram, parametric)

  • Comparing frequency content of two signals (cross-spectrum, coherence)

  • Finding spectral peaks (dominant frequencies, harmonics)

  • Measuring bandwidth, band power, or occupied bandwidth

  • Visualizing frequency-domain data

  • Streaming (real-time, frame-by-frame) spectral analysis with spectrumAnalyzer, dsp.SpectrumEstimator, dsp.CrossSpectrumEstimator

When NOT to Use

  • Designing or applying filters -- use matlab-design-digital-filter

  • Time-frequency/spectrogram analysis (including spectrumAnalyzer spectrogram ViewType, STFT, reassignment, CWT) -- use the time-frequency analysis skill (TBD)

  • Audio-specific features (MFCC, pitch, auditory models) -- use Audio Toolbox

  • Control system frequency response (Bode, Nyquist) -- use Control System Toolbox

Workflow

  1. Batch or streaming? -- Determine if data is already in workspace (batch) or arrives frame-by-frame (streaming). See below.

  2. Preliminary analysis -- When user provides data, run diagnostics to inform technique selection (see below)

  3. Pre-process -- Check for NaN/gaps (use plomb for non-uniform data). Apply detrend(x) only if DC/trend visibly distorts the spectrum

  4. Choose output type -- PSD, power spectrum, amplitude spectrum, or octave bands (see below)

  5. Choose estimator -- Use preliminary analysis results + Estimator Selection below

  6. Compute spectrum -- Use the chosen function with explicit Fs (if available)

  7. Visualize -- Plot with proper axis labels (Hz, dB or linear units)

  8. Extract metrics -- Use findpeaks, bandpower, obw, powerbw. See references/peak-detection.md

  9. Verify -- Parseval's theorem, known tone levels. See references/power-from-spectrum.md

Batch vs Streaming

Determine the processing mode before choosing tools:

IndicatorModeTools
Entire signal in workspace (vector/matrix)Batchpwelch, pspectrum, periodogram, pburg, etc.
Data arrives frame-by-frame (sensor, ADC, real-time loop)StreamingspectrumAnalyzer, dsp.SpectrumEstimator, dsp.CrossSpectrumEstimator
Need live-updating spectrum displayStreamingspectrumAnalyzer (ViewType: spectrum)
Need spectrum values for real-time decisionsStreamingdsp.SpectrumEstimator (returns numeric output each frame)

If streaming: See references/streaming-spectral-analysis.md for System object APIs, properties, and patterns. DSP System Toolbox is required.

The rest of this skill covers batch processing. For streaming, the reference file provides full guidance including the batch-to-streaming mapping table.

Preliminary Data Analysis

When the user provides signal data (variable, file, or description), run diagnostic checks before recommending a technique. See references/preliminary-analysis.md for full code.

Quick checks (run in order — stop early if decisive):

  1. Sampling type — Fs given → uniform. Time vector with small jitter (<5%) → pspectrum(x,t) (resamples internally). Large jitter or truly non-uniform → plomb

  2. Data quality — NaN/Inf, DC offset, trend → preprocess first

  3. Length — <128: parametric only. 128–1024: periodogram/pburg. >10k: pwelch preferred

  4. Spectral character — Run periodogram (Hann), compute spectral flatness + peak count + strongest peak width:

    • Flatness >0.3 → wideband → pwelch (peaks are just noise fluctuations)

    • Flatness <0.1, strongest peak narrow (width < 10×df) → tonal → periodogram(...,'power') or rootmusic

    • Flatness <0.1, strongest peak wide (width ≥ 10×df) → wideband-structured (chirps, shaped bands) → pwelch + obw

    • Flatness 0.1–0.3, peaks present → mixed → pwelch + findpeaks

  5. AR fitness — Fit AR models with arburg, track prediction error vs order. If error plateaus <10% at low order → pburg is strong candidate

  6. Tone count — If tonal: count peaks with findpeaks, cross-check with eigenvalue drop. Known count + resolution-limited → rootmusic(x,2*nTones,Fs)

Report findings to the user before computing the spectrum:

Preliminary Analysis:
- Sampling: uniform at [Fs] Hz
- Duration: [X] s ([N] samples), resolution: [df] Hz
- Spectral character: [wideband/tonal/mixed]
- AR fit: [quality] (order [N], residual [X]%)
Recommendation: [estimator] because [justification]

Output Type Selection

User's GoalOutput TypeFunction / Option
Compare to a standard or another signal (length-independent)PSD (power/Hz)pwelch (default), periodogram
Read amplitude of a specific tonePower spectrum → sqrtpspectrum(x,Fs) (default); periodogram(x,w,N,Fs,'power') or pwelch(x,w,[],[],Fs,'power') for explicit control
Measure total power in a bandPSD then integrate, or use bandpowerbandpower(x,Fs,[fLow fHigh])
Octave-band levels (acoustics, vibration)Fractional-octave spectrumpoctave(x,Fs,'BandsPerOctave',3)
Detect frequencies in nearly-uniform data (small jitter)Power spectrumpspectrum(x,t) — resamples internally
Detect frequencies in non-uniform/gapped dataLomb-Scargleplomb(x,t)

PSD vs Power Spectrum: PSD (power/Hz) is resolution-independent — broadband noise stays flat when you change parameters. Power spectrum (power/bin) is tone-friendly — peak height equals true tone power. Use PSD for noise characterization and specs (g²/Hz, dBm/Hz); use power spectrum for reading tone amplitudes. Convert: PS = PSD × RBW where RBW = enbw(win)*Fs/segLen.

Estimator Selection

Decision tree (simple → specialized):

  1. Just want to see what frequencies are present? → pspectrum(x,Fs)

  2. Need a smooth, low-variance PSD? → pwelch (favored for long signals — segment averaging reduces variance) or periodogram (short signal, cannot segment)

  3. Need accurate tone amplitude from peaks? → periodogram(x,win,N,Fs,'power') then sqrt

  4. Need octave-band levels (acoustics, vibration)? → poctave(x,Fs,'BandsPerOctave',3)

  5. Comparing two signals at each frequency? → mscohere (related?) / cpsd (shared content + phase)

  6. Data is nearly uniform (small jitter)? → pspectrum(x,t) (resamples internally). Truly non-uniform or large gaps? → plomb(x,t)

  7. Need to resolve sinusoids closer than Fs/N? → rootmusic / pmusic (must know # of sinusoids)

  8. Short data, want low-variance PSD without segmenting? → pmtm (multitaper — uses orthogonal DPSS tapers on full record; no AR assumption)

  9. Short data, want smooth sidelobe-free PSD? → pburg (assumes signal is AR-like)

Quick reference table:

GoalFunctionWhen to use
Quick look at frequency contentpspectrumDefault -- good defaults, tune Leakage (0–1) for resolution vs sidelobes
Single-sided amplitude spectrumperiodogram with 'power'Need amplitude per bin
PSD with low variancepwelchLong signals — averaging segments reduces variance; preferred when signal is long enough to segment
PSD of short signal, low variancepmtmMultitaper — uses full record with orthogonal DPSS tapers; no segmentation needed
PSD of short signalperiodogramToo short to segment; high variance (single window)
Resolve closely-spaced sinusoidspmusic, rootmusicKnown # of sinusoids, super-resolution
Smooth PSD of short AR-like datapburgNo sidelobes; NOT for resolving tones

Default: Start with pspectrum. Drop to pwelch/periodogram for explicit control. Never use manual FFT unless user explicitly asks — redirect to built-in functions.

pspectrum vs pwelch: pspectrum outputs power spectrum (Kaiser beta=20, ~76% overlap). pwelch defaults to PSD. They match within ~0.2 dB using equivalent parameters. See references/pspectrum-equivalence.md for exact mapping. Resolution control in pspectrum: Use FrequencyResolution (Hz) to set target resolution directly, or Leakage (0–1) to control the resolution/sidelobe trade-off indirectly. TimeResolution is spectrogram-only — do NOT use it for power spectrum. Leakage parameter: pspectrum(x,Fs,Leakage=L) where L ∈ [0,1] — 0 = minimum leakage (max sidelobe suppression, widest main lobe), 1 = maximum leakage (rectangular window, best resolution), default 0.5.

Nonparametric vs Parametric: Use nonparametric (FFT-based) when signal is long or spectral shape is unknown. Use parametric when data is short, signal matches an AR model, or you need super-resolution. See references/estimator-comparison.md for detailed trade-offs.

Window Selection

GoalWindowWhy
General-purpose PSDHannGood balance, 50% overlap optimal
Detect weak tone near strong toneBlackman-Harris or Kaiser (beta≥10)Low sidelobes (-92 dB)
Resolve two close frequenciesHann or Kaiser (beta=5)Narrow main lobe
Accurate amplitude measurementFlat Top~0.01 dB scalloping loss
Tunable trade-offKaiser(N,beta)Single parameter controls curve

Key rule: Higher sidelobe suppression costs wider main lobe. Only suppress as much as dynamic range requires. See references/spectral-windows.md for ENBW values and overlap guidelines.

Key Functions

FunctionPurpose
pspectrumPower spectrum with automatic defaults; Leakage parameter (0–1) controls resolution vs sidelobe suppression
periodogramPSD or power spectrum via single-window DFT
pwelchPSD via Welch's averaged periodogram
pmtmPSD via Thomson's multitaper method (DPSS/Slepian tapers)
cpsdCross power spectral density
mscohereMagnitude-squared coherence (0 to 1)
pburg / pyulearAR PSD (Burg / Yule-Walker)
pmusic / peigPseudospectrum (MUSIC / eigenvector)
rootmusicFrequency estimation via root-MUSIC
findpeaksLocate spectral peaks
refinepeaksSub-bin peak frequency/amplitude refinement (use after findpeaks)
bandpowerPower in a frequency band
obw / powerbwOccupied bandwidth / 3-dB power bandwidth
meanfreq / medfreqMean / median frequency of spectrum
sfdrSpurious free dynamic range
toiThird-order intercept point (two-tone intermodulation)
spectralFlatnessSpectral flatness (0=tonal, 1=white noise)
spectralCrestSpectral peak-to-mean ratio
spectralKurtosisSpectral kurtosis (transient/non-stationarity detection)
poctaveFractional-octave spectrum
plombLomb-Scargle periodogram (non-uniform data)
spectralEntropySpectral entropy (replaces deprecated pentropy)
spectrumAnalyzerLive streaming spectrum/spectrogram display (DSP System Toolbox)
dsp.SpectrumEstimatorStreaming PSD/PS with numeric output (DSP System Toolbox)
dsp.CrossSpectrumEstimatorStreaming cross-spectrum between two signals (DSP System Toolbox)

Patterns

Convention reminders (apply to ALL code below):

  • pow2db(x) for dB — NEVER 10*log10(x)

  • detrend(x) only when DC offset or trend is clearly an issue (e.g., large DC spike dominates spectrum)

Single-Sided Amplitude Spectrum
Fs = 1000;
N = length(x);
win = hann(N);

% periodogram with 'power' gives single-sided power per bin
% NFFT=N keeps df=Fs/N ([] defaults to nextpow2 which shifts grid)
[pxx,f] = periodogram(x,win,N,Fs,'power');
ampSpectrum = sqrt(pxx);  % power → RMS amplitude

figure
plot(f,ampSpectrum)
xlabel("Frequency (Hz)")
ylabel("Amplitude (RMS)")
title("Single-Sided Amplitude Spectrum")

Key points:

  • Window correction handled automatically by periodogram

  • Frequency resolution is always Fs/N — zero-padding only interpolates

  • For manual FFT: multiply by 2/N for single-sided amplitude, do NOT double DC

PSD with Welch's Method
Fs = 44100;
% x = detrend(x);  % uncomment if DC/trend distorts low-frequency estimates
segmentLength = round(Fs * 0.05);  % 50 ms → df = 20 Hz
win = hann(segmentLength);

[pxx,f] = pwelch(x,win,round(0.5*segmentLength),[],Fs);

figure
plot(f,pow2db(pxx))
xlabel("Frequency (Hz)")
ylabel("PSD (dB/Hz)")
title("Power Spectral Density (Welch)")
grid on

Key points:

  • Segment length sets resolution: df = Fs / segmentLength

  • More segments = lower variance but coarser resolution (trade-off)

  • 50% overlap with Hann is optimal

Spectral Peak Detection

See references/peak-detection.md for noise-floor-relative thresholds and harmonic detection.

[pxx,f] = pwelch(x,hann(1024),[],[],Fs);
pxxDB = pow2db(pxx);

[peaks,locs] = findpeaks(pxxDB,f, ...
    MinPeakHeight=-20, ...
    MinPeakDistance=50, ...
    MinPeakProminence=10);

figure
plot(f,pxxDB)
hold on
plot(locs,peaks,"rv",MarkerFaceColor="r")
hold off
xlabel("Frequency (Hz)")
ylabel("Power/Frequency (dB/Hz)")
legend("PSD","Peaks")
Band Power and Bandwidth

See references/spectral-measurements.md for full details including PSD input, power spectrum + rbw input, and spectral entropy.

Fs = 1000;
pTotal = bandpower(x,Fs,[0 Fs/2]);
pBand = bandpower(x,Fs,[50 150]);
fracPower = pBand / pTotal;

bw = obw(x,Fs);       % 99% occupied bandwidth
pbw = powerbw(x,Fs);  % 3-dB bandwidth (narrowband/resonance signals only)
Fractional-Octave Spectrum (poctave)

See references/poctave-api.md for full syntax, common mistakes, and octave smoothing pattern.

Fs = 44100;

% 1/3-octave with A-weighting (environmental noise)
[p,cf] = poctave(x,Fs,'BandsPerOctave',3,'Weighting','A','FrequencyLimits',[20 20000]);

% From existing PSD (no recomputation needed)
[pxx,f] = pwelch(x,[],[],[],Fs);
[p,cf] = poctave(pxx,Fs,f,'BandsPerOctave',3);

Key points:

  • Use 'BandsPerOctave',3 — do NOT use '1/3 octave' (invalid syntax)

  • Only valid types: 'power' (default), 'spectrogram' — NO 'psd' type

  • Can accept pre-computed PSD: poctave(pxx,Fs,f) avoids reprocessing

  • Output is always power — use pow2db(p) for dB display

Cross-Spectral Comparison
Fs = 1000;
segLen = 1024;
win = hann(segLen);

[pxy,f] = cpsd(x,y,win,segLen/2,[],Fs);
[cxy,f] = mscohere(x,y,win,segLen/2,[],Fs);

figure
tiledlayout(2,1)
nexttile
plot(f,pow2db(abs(pxy)))
ylabel("|CPSD| (dB)"); xlabel("Frequency (Hz)")
nexttile
plot(f,cxy)
ylabel("Coherence"); xlabel("Frequency (Hz)"); ylim([0 1])

Key points:

  • cpsd is complex — use abs for magnitude, angle for phase lag

  • Coherence ≈ 1: linearly related; ≈ 0: unrelated at that frequency

  • Use same win/overlap as pwelch for consistent resolution

Multitaper PSD (Thomson's Method)
Fs = 1000;
nw = 4;  % time-halfbandwidth product (default); resolution bandwidth = 2*nw*Fs/N
[pxx,f] = pmtm(x,nw,[],Fs);

plot(f,pow2db(pxx))
xlabel("Frequency (Hz)"); ylabel("PSD (dB/Hz)")

Key points:

  • Uses 2*nw-1 orthogonal DPSS (Slepian) tapers on the full record — no segmentation

  • Variance reduction without sacrificing frequency resolution (unlike Welch)

  • Resolution bandwidth = 2*nw*Fs/N — increase nw for smoother PSD (wider bandwidth), decrease for finer resolution

  • Ideal for short records where Welch can't segment, or when you need maximum spectral information from limited data

  • Output is true PSD — directly comparable to pwelch

  • Confidence intervals available: [pxx,f,pxxc] = pmtm(x,nw,[],Fs,ConfidenceLevel=0.95)

  • When to prefer over pwelch: short data, can't afford to segment, or need optimal bias-variance without AR assumptions

  • When to prefer over pburg: no prior knowledge that signal is AR-like; want a nonparametric estimate

Parametric PSD (Burg Method)
Fs = 1000;
modelOrder = 16;  % 2*numPeaks to 4*numPeaks
[pxx,f] = pburg(x,modelOrder,[],Fs);

plot(f,pow2db(pxx))
xlabel("Frequency (Hz)"); ylabel("PSD (dB/Hz)")

Key points:

  • Order too low = over-smoothed; too high = spurious peaks

  • Burg preferred over Yule-Walker (less biased for short data)

  • Output is true PSD — comparable to pwelch

Frequency Estimation with MUSIC
Fs = 1000;
nSinusoids = 2;
p = 2*nSinusoids;  % subspace dim: 2 per real sinusoid (pos + neg freq)

[pseudoSpectrum,f] = pmusic(x,p,1024,Fs);
freqEstimates = rootmusic(x,p,Fs);  % more accurate than reading peaks

Key points:

  • MUSIC output is a pseudospectrum, NOT a PSD — peak heights ≠ power

  • p = 2 × number of real sinusoids — using p = nSinusoids gives wrong results

  • rootmusic gives more accurate frequencies than reading pmusic peaks

  • Works best for sinusoids in white noise; short data OK if SNR adequate

Manual FFT-Based PSD (When User Insists)

Only when user explicitly needs manual FFT. See references/manual-fft-psd.md for windowed, power spectrum, and complex-valued variants.

Formula: psdx = (1/(Fs*N)) * abs(fft(x)(1:N/2+1)).^2, double interior bins only (not DC/Nyquist). Windowed: normalize by 1/(Fs*sum(win.^2)).

Conventions

  • Use pspectrum as default — redirect manual FFT users to built-in functions

  • Detrend when warranted — apply detrend(x) when DC/trend visibly dominates the spectrum or distorts low-frequency estimates; do not blindly detrend every signal

  • Label axes with units — "Frequency (Hz)", "PSD (dB/Hz)", "Amplitude (V)"

  • pow2db/db2pow for dB — never 10*log10(...) manually. See references/units-and-db.md for domain-specific reference levels

  • Frequency resolution is Fs/N — zero-padding only interpolates

  • Use built-in measurement functions — bandpower, obw, powerbw, findpeaks

  • Favor convenience plots — calling pwelch(x,[],[],[],Fs), pspectrum(x,Fs), pburg(x,order,[],Fs), etc. without output arguments generates a labeled plot automatically; prefer this over manual plotting when a quick visualization is needed

  • Write a script — when performing multi-step analysis, write the complete workflow as a .m script and run it with run_matlab_file, rather than executing code piecemeal across multiple evaluate_matlab_code calls. This produces a reviewable, reproducible artifact

Common Mistakes

MistakeCorrect Approach
fft(x) without windowApply hann(N) or similar
abs(fft(x)).^2 as "PSD"Use periodogram/pwelch; if manual, scale by 1/(Fs*N) and double interior only
Confusing PSD with power spectrumPSD = power/Hz; PS = power/bin
Zero-padded FFT = higher resolutionZero-padding interpolates, doesn't resolve
10*log10(pxx)Use pow2db
Manual integration for band powerUse bandpower(x,Fs,[fLow fHigh])
Comparing pspectrum to pwelch directlyDifferent units (PS vs PSD). See references/pspectrum-equivalence.md
Using pentropyDeprecated — use spectralEntropy instead
pspectrum(...,'TimeResolution',val) for power spectrumTimeResolution is spectrogram-only. Use 'FrequencyResolution',val or 'Leakage',val
obw(x,Fs,[],'Percentpower',pct)obw uses positional args, not name-value. Correct: obw(x,Fs,[fLow fHigh],pct) where pct is the 4th positional arg
Filter-bank tone power reads 1–3 dB lowTone is between bins — filter-bank has narrow pass-bands. Fix: coherent frame length (frameLen = Fs/df) so tones land on bin centers
snr(x,Fs) unstable for multi-tone with harmonic relationshipssnr classifies harmonics specially — 200 Hz = 2nd harmonic of 100 Hz causes inconsistent results. Use per-tone SNR from spectrum instead

Troubleshooting

See references/troubleshooting.md for detailed explanations and code examples.

  • "Two tones but only one peak" — Resolution limit (Fs/N) or sidelobe masking. Fix: more data, lower-sidelobe window (blackmanharris, kaiser(N,15)), or reassigned periodogram ([pxx,f,rpxx,fc] = periodogram(x,win,N,Fs,'reassigned') — 4-output syntax returns reassigned PSD and center-of-energy frequencies for sharper peak localization).

  • "Tone power is wrong" — Scalloping loss (tone between bins). Fix: flattopwin(N) for amplitude accuracy. Worst case: Hann loses 1.4 dB, Flat Top loses 0.01 dB.

Verification

Verify with Parseval's theorem — total power from spectrum should match time-domain. See references/power-from-spectrum.md for formulas.

pTime = sum(x.^2)/length(x);
pFreq = sum(pxx) * (f(2)-f(1));  % integrate PSD
assert(abs(pTime - pFreq)/pTime < 0.02,"Parseval check failed")

Copyright 2026 The MathWorks, Inc.


Files

references/spectral-measurements.md

Spectral Measurements

Built-in functions for extracting quantitative metrics from spectra. Use these instead of manual computation.

Band Power

Measure power in a specific frequency band.

% From time-domain signal
p = bandpower(x,Fs,[fLow fHigh]);

% From PSD (already computed)
p = bandpower(pxx,f,[fLow fHigh],'psd');

% Total signal power (equivalent to rms(x)^2 for zero-mean)
pTotal = bandpower(x,Fs,[0 Fs/2]);

% Relative band power (fraction of total)
relPower = bandpower(x,Fs,[fLow fHigh]) / bandpower(x,Fs,[0 Fs/2]);

Occupied Bandwidth

The frequency band containing a specified percentage (default 99%) of total power.

% 99% occupied bandwidth (default)
bw = obw(x,Fs);

% 95% occupied bandwidth
bw = obw(x,Fs,[0 Fs/2],95);

% With frequency bounds returned
[bw,fLow,fHigh,power] = obw(x,Fs);

% From power spectrum (not PSD) — must supply resolution bandwidth
[ps,f] = pwelch(x,win,[],[],Fs,'power');
rbw = enbw(win) * Fs / length(win);
bw = obw(ps,f,rbw);

Power Bandwidth

The 3-dB bandwidth -- frequency range where PSD is within 3 dB of the peak.

% Default (3-dB down from peak)
bw = powerbw(x,Fs);

% Custom reference level (6-dB bandwidth)
bw = powerbw(x,Fs,[],6);

% With bounds
[bw,fLow,fHigh] = powerbw(x,Fs);

% From power spectrum (not PSD) — must supply resolution bandwidth
[ps,f] = pwelch(x,win,[],[],Fs,'power');
rbw = enbw(win) * Fs / length(win);
bw = powerbw(ps,f,rbw);

Spectral Peaks

Find dominant frequencies, harmonics, and interference tones.

% Compute PSD first
[pxx,f] = pwelch(x,hann(1024),[],[],Fs);
pxxDB = pow2db(pxx);

% Find peaks with constraints
[peakPowers,peakFreqs] = findpeaks(pxxDB,f, ...
    MinPeakHeight=-30, ...       % ignore below -30 dB
    MinPeakDistance=20, ...      % at least 20 Hz apart
    MinPeakProminence=6, ...     % must stand out by 6 dB
    NPeaks=10, ...              % return at most 10 peaks
    SortStr="descend");          % strongest first
Harmonic Detection Pattern
f0 = peakFreqs(1);  % fundamental
nHarmonics = 5;
harmonicFreqs = f0 * (1:nHarmonics);
tolerance = 5;  % Hz

foundHarmonics = false(1,nHarmonics);
for k = 1:nHarmonics
    foundHarmonics(k) = any(abs(peakFreqs - harmonicFreqs(k)) < tolerance);
end

Spectral Entropy

Measure spectral complexity/randomness (0 = pure tone, 1 = white noise).

Use spectralEntropy (introduced R2019a). The older pentropy is deprecated and will be removed.

% Scalar entropy of the whole signal
se = spectralEntropy(x,Fs,Instantaneous=false);

% Time-varying spectral entropy (default)
[se,t] = spectralEntropy(x,Fs);

% Limit frequency range
se = spectralEntropy(x,Fs,Range=[50 400]);

Note: spectralEntropy requires column-vector input (x(:)).

Lomb-Scargle Detection Thresholds (plomb)

plomb can return power-level thresholds for given detection probabilities via the Pd name-value pair. Use this to assess statistical significance of spectral peaks in non-uniformly sampled data.

% Return thresholds for 50%, 90%, 99% detection probability
[pxx,f,pth] = plomb(x,t,[],'psd',Pd=[0.5 0.9 0.99]);

% Plot with significance line
figure
plot(f,pxx)
hold on
yline(pth(3),'--r',Label="99% detection")
hold off
xlabel("Frequency (Hz)")
ylabel("PSD")
title("Lomb-Scargle with Detection Threshold")

Key points:

  • pth is a vector with one threshold per requested probability

  • Works with 'psd', 'power', or 'normalized' spectrum types

  • With 'normalized' output, thresholds follow an exponential distribution under the null hypothesis (no signal)

Reassigned Periodogram

Reassignment sharpens spectral peaks by moving energy from each bin to its center-of-energy frequency. Useful for closely-spaced tones or chirps.

% Reassigned periodogram: returns both reassigned and standard PSD + center freqs
[rpxx,f,pxx,fc] = periodogram(x,hann(N),N,Fs,'reassigned');

% fc contains the center-of-energy frequency for each bin
% rpxx is the reassigned PSD (energy redistributed to true frequencies)

% Also works with 'power' output
[rps,f,ps,fc] = periodogram(x,hann(N),N,Fs,'power','reassigned');

Key points:

  • Output has 4 arguments: [reassigned, f, standard, center_freqs]

  • fc (center-of-energy frequencies) tells you where energy truly lives within each bin

  • Reassignment sharpens peaks but can create artifacts in noisy spectra

  • Only available for periodogram, not pwelch

Mean and Median Frequency

Scalar descriptors of the spectral "center of mass." Useful for characterizing where spectral energy is concentrated.

% Mean frequency (power-weighted average frequency)
fMean = meanfreq(x,Fs);

% Median frequency (frequency that divides power in half)
fMed = medfreq(x,Fs);

% From PSD (already computed)
fMean = meanfreq(pxx,f);
fMed = medfreq(pxx,f);

% Restrict to a band
fMean = meanfreq(x,Fs,[100 500]);

% From power spectrum (not PSD) — supply resolution bandwidth
[ps,f] = pwelch(x,win,[],[],Fs,'power');
rbw = enbw(win) * Fs / length(win);
fMean = meanfreq(ps,f,rbw);

Key points:

  • meanfreq = power-weighted centroid; sensitive to spectral tails

  • medfreq = frequency splitting total power 50/50; robust to outlier energy

  • Both accept time-domain signals or pre-computed PSD/power spectrum

Signal-to-Noise Ratio (from spectrum)

% SNR of a sinusoidal signal in noise
r = snr(x,Fs);

% SNR with known signal frequency
r = snr(x,Fs,f0);

% Total harmonic distortion
thd_value = thd(x,Fs);

% SINAD (signal-to-noise-and-distortion)
s = sinad(x,Fs);

Spurious Free Dynamic Range (SFDR)

Distance (dB) between fundamental and the largest spurious component.

% From time-domain signal
r = sfdr(x,Fs);

% With minimum spur distance (ignore spurs within 100 Hz of fundamental)
r = sfdr(x,Fs,100);

% From power spectrum
[ps,f] = periodogram(x,hann(N),N,Fs,'power');
r = sfdr(ps,f,'power');

% Get spur frequency and power
[r,spurPow,spurFreq] = sfdr(x,Fs);

Third-Order Intercept (TOI/OIP3)

Measures third-order intermodulation distortion in a two-tone signal.

% From time-domain two-tone signal
oip3 = toi(x,Fs);

% Full output: fundamental + intermod powers and frequencies
[oip3,fundPow,fundFreq,imodPow,imodFreq] = toi(x,Fs);

% From PSD
[pxx,f] = pwelch(x,[],[],[],Fs);
oip3 = toi(pxx,f,'psd');

Key points:

  • Input must be a two-tone signal (two sinusoids)

  • Returns OIP3 in dBW (or dB relative to input units)

  • Intermodulation products appear at 2*f1-f2 and 2*f2-f1

Spectral Shape Descriptors

Scalar statistics describing the shape of the power spectrum. All accept time-domain signals (with windowed STFT internally) or pre-computed spectra.

% Spectral flatness: ratio of geometric to arithmetic mean (0=tonal, 1=white noise)
flatness = spectralFlatness(x,Fs);

% Spectral crest: peak-to-mean ratio (high=tonal, low=flat/noise-like)
crest = spectralCrest(x,Fs);

% Spectral skewness: asymmetry of the spectral distribution
skew = spectralSkewness(x,Fs);

% Spectral kurtosis: peakedness/tailedness of spectral distribution
kurt = spectralKurtosis(x,Fs);

% With confidence threshold for non-stationarity detection (requires Scaled=false)
[kurt,~,~,threshold] = spectralKurtosis(x,Fs,Scaled=false,ConfidenceLevel=0.95);

% Restrict frequency range
flatness = spectralFlatness(x,Fs,Range=[100 4000]);

% From frequency-domain input (pre-computed spectrum + freq vector)
flatness = spectralFlatness(pxx,f);

Key points:

  • All require column-vector input (x(:)) — a row vector is treated as multi-channel with length 1 per channel.

  • These return time-varying values by default (one per frame). Use Instantaneous=false (for spectralEntropy) or process the full signal as one window to get a scalar.

  • spectralFlatness ≈ same concept as Wiener entropy; use to distinguish tonal vs broadband signals

  • spectralKurtosis is useful for detecting transients/non-stationarity in vibration signals; values exceeding the confidence threshold indicate non-Gaussian frequency content. ConfidenceLevel requires Scaled=false

  • All share the same name-value interface: Window, OverlapLength, FFTLength, Range, SpectrumType

Summary Table

MeasurementFunctionInputOutput
Power in bandbandpowerSignal or PSD + freq rangeWatts (linear)
99% bandwidthobwSignal + FsHz
3-dB bandwidthpowerbwSignal + FsHz
Mean frequencymeanfreqSignal or PSD + FsHz
Median frequencymedfreqSignal or PSD + FsHz
Peak frequenciesfindpeaksPSD in dB + freq vectordB, Hz
Spectral entropyspectralEntropySignal + Fs0-1 (normalized)
Spectral flatnessspectralFlatnessSignal or spectrum + Fs0-1
Spectral crestspectralCrestSignal or spectrum + Fsratio
Spectral skewnessspectralSkewnessSignal or spectrum + Fsunitless
Spectral kurtosisspectralKurtosisSignal or spectrum + Fsunitless
SNRsnrSignal + FsdB
THDthdSignal + FsdB
SINADsinadSignal + FsdB
SFDRsfdrSignal or spectrum + FsdB
TOI (OIP3)toiTwo-tone signal or PSD + FsdBW

Copyright 2026 The MathWorks, Inc.


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