Evan Balster wrote:
...

To that end:  A handy, cheap algorithm for approximating the power-weighted 
spectral
centroid -- a signal's "mean frequency" -- which is a good heuristic for 
perceived sound
brightness <https://en.wikipedia.org/wiki/Brightness#Brightness_of_sounds>.  In 
spite of
its simplicity, ...
Hi,

Always interesting to learn a few more tricks, and thanks to Ethan's explanation I get there are certain statistical ideas involved. I wonder however where those ideas in practice lead to, because of a number of assumptions, like the "statistical variance" of a signal. I get that a self correlation of a signal in some normal definition gives an idea of the power, and that you could take it that you compute power per frequency band. But what does it mean when you talk about variance ? Mind you I know the general theoretics up to the quantum mechanics that worked on these subjects long ago fine, but I wonder what the understanding here is?

Some have remarked about the analysis of a signal into ground frequency and harmonics that it might be hard to summarize and make an ordinal measure for "brightness" as a one dimensional quantity, I mean of you look at a number of peaks in a frequency graph, how do you sum up the frequency of the signal, if there is one, and the meaning of the various harmonics in the spectrum, if they are to be taken as a measure of the brightness? So a trick is fine, though I do not completely understand the meaning of a brightness measure for frequency analysis.

Of course to determine a statistical measure about a spectrum, either based on sampled signals or (where the analysis comes from and is only generally correct for signal from - to + inf) on a continuous signal, and based either on a Fourier integral/summation or a Fast Fourier analysis (with certain analysis length and frequency bin accuracy), you could use the general big numbers theorem and presume there's a mean and a variance. It would be nice to at least make credible why this is an ok analysis, because a lot of signals are far from Gaussian distributed in the sense of the frequency spectrum.

T.


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