Graphics Programs Reference
In-Depth Information
Thus, the
H ρ
expressions for the three regions defined in Fig. 11.30 become
1
I
H
=−
a vJ
(
k
ρ
) s(
v
ϕ α
) in(
v
ϕ α
)
ρ
nv
1
0
j
ωµρ
n
=
0
1
(11.93)
(
)
II
H
=−
(2)
ρ ϕα ϕα
cos (
v
)sin (
v
)
vbJ k
()
ρ
+
cH
()
k
ρ
0
nv
n v
j
ωµρ
n
=
0
1
III
H
=−
d
vH
(2)
( s(
k
ρ
v
ϕ α
in(
v
ϕ α
)
ρ
n
0
j
ωµρ
v
n
=
0
11.6.1. Far Scattered Field
In region III, the scattered field may be found as the difference between the
total and incident fields. Thus, using Eqs. (11.68) and (11.69) and considering
the far field condition (
ρ∞
) we get
2
j
III
i
s
jkρ
v
EEE
=+=
e
dj
sin
v φα v φα
(
− −
) sin
(
)
z
z
z
n
0
πkρ
n
=
0
(11.94)
11
E
ωȺ
2
j
H
=−
z
(
)
i
jkρ
+
jkρ
cos
φ φ
EI
=−
0
e
e
0
0
ρ
j
ωµρ φ
z
e
4
πkρ
Note that
d n
can be written as
ωȺI
%
(11.95)
d
=−
0
4
e
d
n
n
where
(
)
(
)
(
)
(
)
(
)
kJ
k a
J
ka Y
YkaJ kρ
+
K
v
1
v
ν
0
ν
v
0
(
)
(
)
(
)
(
)
(
)
kJ
ka
Y ka J
JkaY ρ
π
dj παβ
4
%
1
v
1
ν
v
0
v
ν
0
(11.96)
=
n
2
−−
() ()() () ()()
2
2
kH
ka J
k a
k H
ka J
k a
ν
v
1
1
ν
v
1
Substituting Eq. (11.95) into Eq. (11.94), the scattered field
f ()
is
 
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