Digital Signal Processing Reference
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as the plug-in estimator. The optimal weight at
F
S
employs the MLE of
S
(i.e.,
w¼ w
ml
, where
w
ml
is given by (2.23)) and is hereafter denoted by
w
mle
.
B
EXAMPLE 2.9
Our simulation setting is as follows. A
k ¼
4 sensor ULA with
l=
2 spacing
received two (
d ¼
2) uncorrelated circular Gaussian signals of equal variance
s
s
with DOAs at
10
8
(SOI) and 15
8
(interferer). In the first setting (A), noise
n
has circular Gaussian distribution CN
k
(
s
n
I
), and in the second setting (B), noise
has circular Cauchy distribution CT
k
,1
(
s
n
I
). Note that the Cauchy distribution
does not have finite variance and
s
n
is the scale parameter of the distribution. In
both A and B, the SNR (dB) is defined using scale parameters as
10 log
10
[
s
s
=s
n
]
¼
15 dB. The number of snapshots is
n ¼
500.
Figure 2.8 depicts the estimated
w
-MVDR beampatterns for look direction
10
8
for settings A and B averaged over 100 realizations. Also plotted are the estimated
spectrums. The employed
M
-estimators are the SCM [i.e., HUB(1)], MLT(1) and
HUB(0.9). In the Gaussian noise case (setting A), the beampatterns are similar, in
Figure 2.8 Averaged w-MVDR beampatterns (a) and spectrums (b) for setting A and B
(n ¼ 500, SOI at 10
). In Gaussian noise, all estimators perform
comparably. In Cauchy noise, SCM fails, but robust HUB(0.9) and MLT(1) estimators
perform very well.
8
,
interferer at 15
8
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