Graphics Programs Reference
In-Depth Information
11.5.1. Sphere
Due to symmetry, waves scattered from a perfectly conducting sphere are
co-polarized (have the same polarization) with the incident waves. This means
that the cross-polarized backscattered waves are practically zero. For example,
if the incident waves were Left Circularly Polarized (LCP), then the backscat-
tered waves will also be LCP. However, because of the opposite direction of
propagation of the backscattered waves, they are considered to be Right Circu-
larly Polarized (RCP) by the receiving antenna. Therefore, the PP backscat-
tered waves from a sphere are LCP, while the OP backscattered waves are
negligible.
The normalized exact backscattered RCS for a perfectly conducting sphere
is a Mie series given by
∞
∑
krJ
n
k
()
nJ
n
k
()
σ
π
r
2
j
kr
----
(
n
1
--------
=
1
(
2
n
+
1
)
-----------------------------------------------------------
(11.27)
()
k
()
nH
n
()
k
()
krH
n
1
n
=
1
J
n
k
()
H
n
()
k
()
--------------------
where
r
is the radius of the sphere,
k
=
2πλ
⁄
,
λ
is the wavelength,
J
n
is the
H
n
()
spherical Bessel of the first kind of order n, and
is the Hankel function of
order n, and is given by
H
n
()
k
()
J
n
=
k
()
jY
n
+
k
()
(11.28)
is the spherical Bessel function of the second kind of order n. Plots of the
normalized perfectly conducting sphere RCS as a function of its circumference
in wavelength units are shown in
Figs. 11.16a
and
11.16b.
These plots can be
reproduced using the function
Ðrcs_sphere.mÑ
given in Listing 11.4 in Section
11.9.
Y
n
In Fig. 11.16, three regions are identified. First is the optical region (corre-
sponds to a large sphere). In this case,
σ
r
2
=
r
λ
»
(11.29)
Second is the Rayleigh region (small sphere). In this case,
σ 9π
r
2
k
(
4
≈
r
λ
«
(11.30)
The region between the optical and Rayleigh regions is oscillatory in nature
and is called the Mie or resonance region.
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