Computes the estimated power and frequency around a peak in the power spectrum of a time-domain signal. Details
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Power Spectrum is the power spectrum of a time domain signal. Power Spectrum is the output of the Auto Power Spectrum VI. Refer to Auto Power Spectrum VI for more information about this VI. | ||||
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peak frequency is the frequency (usually in Hertz) of the frequency peak around which you want to estimate the frequency and power. The default is -1. If you do not wire this parameter, the VI automatically searches for the maximum peak in the power spectrum array and estimates the frequency and power around it. | ||||
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window constants contains the window constants of the window that was used to compute the power spectrum. The default values are set to those of the uniform window (no window).
window constants is usually the output of the Scaled Time Domain Window VI.
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df is the line frequency interval of the input spectrum. The default is 1.0. You need this input only when you use the spectral density output formats (the last four display unit selections). | ||||
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span is the number of frequency lines (bins) around the peak to be included in the peak frequency and power estimation. The default is 7, which means that the power in three frequency lines before the peak frequency line, the peak frequency line itself, and three frequency lines after the peak are included in the estimation. This is adequate for most windows. | ||||
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est frequency peak is the estimated frequency of the peak in the input Power Spectrum.
est frequency peak is computed as
for j = i - span/2, i + span/2, where i = peak index, Power Spectrum (j) = power in bin j, and df = frequency bin width. |
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est power peak is the estimated power of the peak in the input Power Spectrum.
est power peak is computed as
for j = i span/2, i + span/2, where i = peak index, Power Spectrum (j) = power in bin j, and ENBW = equivalent noise bandwidth of the window. |
With the Power & Frequency Estimate VI, you can achieve good frequency estimates for measured frequencies that lie between frequency lines on the spectrum. The Power & Frequency Estimate VI makes corrections for the window function you use.