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A function related to cross-correlation
is the coherence function
, defined in terms of power
spectral densities and the cross-spectral
density by
In practice, these quantities can be estimated by averaging
,
and
over successive signal blocks. Let
denote time averaging
across frames as in Eq. (E.3)
of §E.3
above Then the time average of
, for example, is given by
where
is the DFT of the
th
block of time data
, and
is the total
number of time blocks available. In this notation, an estimate of the coherence,
the sample coherence function
, may be defined by
The magnitude-squared coherence
is a real function between 0 and
which gives a measure of correlation
between
and
at each frequency
(DFT bin
number
). For example, imagine that
is produced from
via an LTI
filtering operation:
Then the coherence function in each frame is
and the magnitude-squared coherence function is simply
On the other hand, when
and
are uncorrelated
(e.g.,
is a noise process not
derived from
), the coherence converges to zero at
all frequencies.
A common use for the coherence function is in the validation of input/output
data collected in an acoustics experiment for purposes of system
identification. For example,
might be a known signal which is input to an unknown system, such as a
reverberant room, say, and
is the recorded response of the
room. Ideally, the coherence should be
at all frequencies.
However, if the microphone is situated at a null
in the room response for some frequency, it may record mostly noise at that
frequency. This will be indicated in the measured coherence by a significant dip
below
.
Continuous/Discrete Fourier Transforms
Welch's Method for Power Spectrum Estimation
Signal Processing Analysis Contents
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Contents
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``Mathematics of the Discrete
Fourier Transform (DFT)'', by Julius O. Smith III, (online
book).
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Copyright © 2003-08-28 by Julius O. Smith III
Center for Computer Research in Music and
Acoustics (CCRMA), Stanford
University
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