Compute FFT resolution, bin spacing, and Nyquist values. Compare sample rate, length, padding, and windows. Interpret spectral detail correctly every time.
Use sample count or duration. If both are entered, duration updates the effective sample count from the chosen sample rate.
| Sample Rate (Hz) | Samples | Record Length (s) | True Resolution (Hz) | FFT Points | Displayed Bin Spacing (Hz) |
|---|---|---|---|---|---|
| 1000 | 1024 | 1.024 | 0.976563 | 1024 | 0.976563 |
| 1000 | 1024 | 1.024 | 0.976563 | 4096 | 0.244141 |
| 5000 | 2048 | 0.4096 | 2.441406 | 2048 | 2.441406 |
| 10000 | 8192 | 0.8192 | 1.220703 | 16384 | 0.610352 |
Δf = fs / N = 1 / T
True FFT frequency resolution depends on total record length. Here, fs is the sample rate, N is the number of acquired samples, and T is the observation time.
Displayed Bin Spacing = fs / NFFT
Zero padding changes displayed bin spacing by increasing NFFT, but it does not improve the actual ability to separate two close frequencies. The calculator also estimates window ENBW and main lobe width for better interpretation.
FFT frequency resolution is the smallest frequency spacing that your captured time record can meaningfully distinguish. It mainly depends on observation time, not on the plotting style of the spectrum.
No. Zero padding only creates more frequency samples between existing spectral bins. It smooths the plotted spectrum and improves interpolation, but the true resolving power still comes from the original record length.
A longer record means more observation time. Since resolution equals 1 divided by record length, extending capture time reduces the minimum distinguishable frequency spacing.
Nyquist frequency is half the sample rate. Frequencies above this limit fold back into the spectrum as aliases, so it defines the highest unambiguous frequency you can analyze.
Windows control spectral leakage. They trade amplitude accuracy, leakage suppression, and main lobe width. Some windows spread energy more, which can make closely spaced frequencies harder to separate.
Equivalent noise bandwidth estimates how much a chosen window broadens noise energy in frequency terms. It helps compare window effects beyond simple bin spacing.
For physical resolving ability, trust true frequency resolution based on record length. For plotted spectrum spacing and cursor steps, use displayed bin spacing based on FFT points.
Usually not reliably with a basic FFT alone. Separation depends on record length, signal-to-noise ratio, window choice, and whether advanced estimation methods are used.
Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.