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measures how well the time-domain signal x ( t ) can be approximated by counterclock-
wise rotating phasors. Similarly, the magnitude of the CR-TFD, normalized by the
time- and frequency-marginals of the HR-TFD, measures how well the time-domain
signal x ( t ) can be approximated by clockwise rotating phasors. This suggests that the
distribution of coherence (rather than energy or power) over time and frequency is a
fundamental descriptor of a nonstationary signal.
Finally we point out that, if x ( t ) is WSS, the estimator x f ( t ) simplifies to
( f )e j2 π ft
x f ( t )
=
d
ξ
(9.98)
for all t , which has already been shown in Section 8.4.2 . Furthermore, since WSS
analytic signals are proper, the conjugate-linear estimator is identically zero: x f ( t )
0
for all t . Hence, WSS analytic signals can be estimated only from counterclockwise
rotating phasors, whereas nonstationary improper analytic signals may also be estimated
from clockwise rotating phasors.
=
9.3.2
Kernel estimators
The Rihaczek distribution is a mathematical expectation. As a practical matter, it must
be estimated. Because such an estimator is likely to be implemented digitally, we present
it for a time series x [ k ]. We require that our estimator be a bilinear function of x [ k ] that
is covariant with respect to shifts in time and frequency. Estimators that satisfy these
properties constitute Cohen's class. 10 (Since we want to perform time- and frequency-
smoothing, we do not expect our estimator to have the correct time- and frequency-
marginals.) The discrete-time version of Cohen's class is
V xx [ k
] x [ k
m ]e j µθ ,
)
=
x [ k
+
m
+ µ
]
φ
[ m
+
(9.99)
m
µ
where m is a global and
µ
a local time variable. The choice of the dual-time kernel
] determines the properties of the HR-TFD estimator V xx [ k
φ
). Omitting the
conjugation in ( 9.99 ) gives an estimator of the CR-TFD. It is our objective to design
a suitable kernel
[ m
φ
[ m
]. A factored kernel that preserves the spirit of the Rihaczek
distribution is
w 3 [ m ]
φ
[ m
]
= w 1 [ m
+ µ
]
w 2 [
µ
]
.
(9.100)
In practice, the three windows
w 1 ,
w 2 , and
w 3 might be chosen real and even. By
inserting ( 9.100 )into( 9.99 ), we obtain
m ] π
π
m w 3 [ m ] x [ k
)e j m ( θ ω ) d
ω
V xx [ k
)
=
+
W 2 (
ω
) F 1 [ k
ω
π .
(9.101)
2
Here W 2 (
ω
) is the discrete-time Fourier transform (DTFT) of
w 2 [
µ
] and F 1 is the
short-time Fourier transform (STFT) of x [ k ] using window
w 1 , defined as
n w 1 [ n ] x [ n
k ]e j n θ .
F 1 [ k
)
=
+
(9.102)
 
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