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Frequency-Domain COLA Constraints

Recall that for error-free OLA processing, we required the constant-overlap-add (COLA) window constraint:

$\displaystyle \sum_m w(n-mR) = \hbox{constant}
$

Thanks to the PSF, we may now express the COLA constraint in the frequency domain:

$\displaystyle \zbox {w\in\hbox{\sc Cola}(R) \;\Leftrightarrow\; W(\omega_k) = 0, \quad \vert k\vert = 1,2, \dots, R-1}
$

In other terms,
$\textstyle \parbox{0.8\textwidth}{A window $w$\ gives constant overlap-add at
h...
...dow transform $W$\ is \emph{zero at
all harmonics of the frame rate} $2\pi/R$.}$

Notation:

$\displaystyle \zbox {w \in \hbox{\sc Cola}(R) \quad \Leftrightarrow \quad W \in \hbox{\sc Nyquist}(2\pi/R)} \protect$ (9.5)

The ``Nyquist($ \Omega_R$)'' property for a function $ W$ simply means that $ W$ is zero at all nonzero multiples of $ \Omega_R$ (all harmonics of the frame rate here).

We may also refer to (8.5) as the ``weak COLA constraint'' in the frequency domain. It gives necessary and sufficient conditions for perfect reconstruction in overlap-add FFT processors. However, when the short-time spectrum is being modified, these conditions no longer apply, and a stronger COLA constraint is preferable.



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written by Julius Orion Smith III
Julius Smith's background is in electrical engineering (BS Rice 1975, PhD Stanford 1983). He is presently Professor of Music and Associate Professor (by courtesy) of Electrical Engineering at Stanford's Center for Computer Research in Music and Acoustics (CCRMA), teaching courses and pursuing research related to signal processing applied to music and audio systems. See http://ccrma.stanford.edu/~jos/ for details.


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