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Consider again the Fourier transform of a complex Gaussian in
(10.27):
 |
(11.33) |
Setting
gives
 |
(11.34) |
The log magnitude Fourier transform is given by
 |
(11.35) |
and the phase is
 |
(11.36) |
Note that both log-magnitude and (unwrapped) phase are
parabolas in
.
In practice, it is simple to estimate the curvature at a
spectral peak using parabolic interpolation:
We can write
Note that the window ``amplitude-rate''
is always positive.
The ``chirp rate''
may be positive (increasing frequency) or
negative (downgoing chirps). For purposes of chirp-rate estimation,
there is no need to find the true spectral peak because the curvature
is the same for all
. However, curvature estimates are
generally more reliable near spectral peaks, where the signal-to-noise
ratio is typically maximum.
In practice, we can form an estimate of
from the known FFT
analysis window (typically ``close to Gaussian'').
Subsections
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