The Flat Top window

The Flat Top window is a specialized window function designed for highly accurate amplitude measurements in the frequency domain. Unlike other windows that optimize for spectral resolution or leakage, the Flat Top window is optimized for amplitude accuracy, making it ideal for FFT-based measurements where knowing the exact amplitude of a frequency component is more important than distinguishing closely spaced frequencies. Its frequency response has an extremely flat passband, which minimizes the amplitude error that occurs when a signal frequency falls between FFT bins (scalloping loss).

\[ w(n) = a_0 - a_1 \cos\left(\frac{2\pi n}{N-1}\right) + a_2 \cos\left(\frac{4\pi n}{N-1}\right) - a_3 \cos\left(\frac{6\pi n}{N-1}\right) + a_4 \cos\left(\frac{8\pi n}{N-1}\right), \quad 0 \le n \le N-1 \]

Typical coefficients for the 5-term Flat Top window are:

\[ a_0 = 0.21557895, \quad a_1 = 0.41663158, \quad a_2 = 0.277263158, \quad a_3 = 0.083578947, \quad a_4 = 0.006947368 \]

These coefficients are carefully chosen to create a frequency response that is nearly flat across the width of each FFT bin, ensuring that the measured amplitude is accurate to within ±0.01 dB regardless of where the signal frequency falls within the bin.

Time-Domain Effect: The Flat Top window (blue) shows significantly stronger tapering than the Hann window (orange), with more aggressive attenuation toward the edges. This reflects its design priority: amplitude accuracy over resolution.
Frequency-Domain Comparison: The Flat Top window (blue) shows a very wide main lobe and excellent side lobe suppression below -90 dB. However, the key feature is invisible in this plot: the passband is extremely flat, ensuring amplitude measurement accuracy of ±0.01 dB regardless of frequency offset within the bin.

The Flat Top window's defining characteristic is not visible in a standard magnitude spectrum plot. Its unique property is the flatness of the main lobe – the region near the peak is deliberately shaped to have minimal amplitude variation. When a signal frequency falls exactly between two FFT bins, most windows introduce an amplitude error (scalloping loss) of up to 1.5 dB (Hann) or 0.8 dB (Hamming). The Flat Top window reduces this error to less than 0.01 dB, making it the industry standard for precision amplitude measurements.

The Flat Top window achieves this by using five cosine terms and carefully optimized coefficients. The wide main lobe (approximately 3.5-4.0 times wider than the rectangular window) is the price paid for this amplitude accuracy. Side lobe suppression is excellent, typically below -90 dB, but the primary purpose is amplitude fidelity, not leakage reduction.

Use Case: Precision Amplitude Measurements in Calibration and Test Equipment

The Flat Top window is the standard choice for applications where accurate amplitude measurement is critical, such as spectrum analyzer calibration, audio analyzer THD (total harmonic distortion) measurements, and vibration analysis for machine condition monitoring. When measuring harmonic distortion, the fundamental frequency may be 60-100 dB stronger than the harmonics. The Flat Top window ensures that the measured amplitude of the fundamental is accurate, which is essential for calculating correct distortion percentages.

Practical example: In audio test equipment measuring amplifier distortion, a 1 kHz sine wave is applied, and the spectrum is analyzed for harmonics at 2 kHz, 3 kHz, etc. The fundamental may drift slightly due to oscillator instability. With a Hann window, this drift would cause amplitude variations in the measured fundamental, leading to inconsistent distortion readings. The Flat Top window's flat passband ensures that even if the fundamental moves within the FFT bin, its measured amplitude remains stable, producing repeatable distortion measurements.

Trade-offs and Limitations

The Flat Top window has several significant trade-offs:

  • Very wide main lobe: Approximately 3.5-4.0 times wider than the rectangular window (compared to 1.44x for Hann). This makes it impossible to distinguish closely spaced frequencies.
  • Poor frequency resolution: Two signals that are close in frequency will appear as a single merged peak.
  • High scalloping loss compensation: The flat passband comes at the cost of reduced peak amplitude (typically -0.5 dB to -1.0 dB), requiring calibration or correction.
  • Longer FFTs needed: To achieve adequate frequency resolution, longer FFT sizes (e.g., 8192 or 16384 points) are often required when using a Flat Top window.
  • Not for general use: If you don't need high amplitude accuracy, a Flat Top window is usually the wrong choice due to its poor resolution.

Conclusion

The Flat Top window is the window of choice when amplitude accuracy is the primary requirement. Its unique design produces a frequency response that is flat across each FFT bin, reducing amplitude measurement error (scalloping loss) to less than ±0.01 dB – compared to ±1.5 dB for the Hann window. However, this comes at a severe cost: the main lobe is 3.5-4.0 times wider than the rectangular window, making it unsuitable for resolving closely spaced frequencies. For applications like audio distortion analysis, spectrum analyzer calibration, and precision vibration measurement, the Flat Top window is indispensable. For general spectral analysis where frequency resolution matters, choose a different window.

See also:

  • Window function
  • Spectral leakage
  • Flat Top window