Graphics Programs Reference
In-Depth Information
where
x
m
is the median of the random variable
x
, and
σ
is the standard devi-
ation of the random variable
ln
()
.
The Weibull distribution is used to model clutter at low grazing angles (less
than five degrees) for frequencies between and . The Weibull proba-
bility density function is determined by th
e
Weibull slope parameter
1
10
GHz
a
(often
tabulated) and a median scatter coefficient
σ
0
, and is given by
b
x
b
1
x
b
σ
0
f
()
=
--------------
exp
-----
;
x
≥
0
(6.45)
σ
0
where
b
=
1
⁄
a
is known as the shape parameter. Note that when
b
=
2
the
Weibull distribution becomes a Rayleigh distribution.
6.5. ÐMyRadarÑ Design Case Study - Visit 6
6.5.1. Problem Statement
Analyze the impact of ground clutter on ÐMyRadarÑ design case study.
Assume a Gaussian antenna pattern. Assume that the radar height is 5 meters.
Consider an antenna sidelobe level and a ground clutter coef-
ficient . What conclusions can you draw about the radarÓs
ability to maintain proper detection and track of both targets? Assume a radar
height
SL
=
20
dB
σ
0
=
15
dBsm
h
r
≥
5
m
.
6.5.2. A Design
From the design processes established in
Chapters 1
and
2,
it was determined
that the minimum single pulse SNR required to accomplish the design objec-
tives was when non-coherent integration (4 pulses) and cumula-
tive detection were used. Factoring in the surface clutter will degrade the SIR.
However, one must maintain
SNR
≥
4
dB
SIR
≥
4
dB
in order to achieve the desired prob-
ability of detection.
Figure 6.11
shows a plot of the clutter RCS versus range corresponding to
ÐMyRadarÑ
design requirements. This figure can be reproduced using the
MATLAB GUI
Ðclutter_rcs_guiÑ
with the following inputs:
Symbol
Va l u e
Units
sigma0
-15
dB
thetaE
11 (see page 45)
degrees
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