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・ Spectral concentration problem
・ Spectral correlation density
・ Spectral Database for Organic Compounds
・ Spectral density
・ Spectral density estimation
・ Spectral Dusk
・ Spectral edge frequency
・ Spectral efficiency
・ Spectral element method
・ Spectral energy distribution
・ Spectral envelope
・ Spectral estimation of multidimensional signals
・ Spectral evidence
・ Spectral expansion solution
・ Spectral flatness
Spectral flux
・ Spectral flux density
・ Spectral gap
・ Spectral Gene
・ Spectral Genomics
・ Spectral geometry
・ Spectral glide
・ Spectral graph theory
・ Spectral Hash
・ Spectral hole burning
・ Spectral imaging
・ Spectral index
・ Spectral induced polarisation
・ Spectral invariants
・ Spectral layout


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Spectral flux : ウィキペディア英語版
Spectral flux

Spectral flux is a measure of how quickly the power spectrum of a signal is changing, calculated by comparing the power spectrum for one frame against the power spectrum from the previous frame.〔 More precisely, it is usually calculated as the 2-norm (also known as the Euclidean distance) between the two normalised spectra.
Calculated this way, the spectral flux is not dependent upon overall power (since the spectra are normalised), nor on phase considerations (since only the magnitudes are compared).
The spectral flux can be used to determine the timbre of an audio signal, or in onset detection,〔 among other things.
==Variations==

Some implementations use the 1-norm rather than the 2-norm (i.e. the sum rather than the Euclidean distance).
Some implementations do not normalise the spectra.
For onset detection, increases in energy are important (not decreases), so some algorithms only include values calculated from bins in which the energy is increasing.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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