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26 Radio Engineering for Wireless Communication and Sensor Applications

electromagnetic shield made of pure copper of thickness of 4 mm (= 6 skin depths) provides an attenuation of about 20 log (1/e )6 6 × 8.68 dB 50 dB.

In a general case, each field component can be solved from the general Helmholtz equation:

2E i

+

2E i

+

2E i

g

2

E i = 0, i = x , y , z

(2.70)

x 2

y 2

z 2

 

 

 

 

 

 

 

The solution is found by using the separation of variables. By assuming that

E i = f (x ) g ( y ) h (z ),

f

+

g

+

h

 

g2

= 0

(2.71)

f

 

g

 

h

 

 

 

 

 

 

where the double prime denotes the second derivative. The first three terms of this equation are each a function of one independent variable. As the sum of these terms is constant (g2 ), each term must also be constant. Therefore, (2.71) can be divided into three independent equations of form f /f gx2 = 0, which have solutions as shown previously.

2.5 Polarization of a Plane Wave

Electromagnetic fields are vector quantities, which have a direction in space. The polarization of a plane wave refers to this orientation of the electric field vector, which may be a fixed orientation (a linear polarization) or may change with time (a circular or elliptical polarization).

The electric field of a plane wave can be presented as a sum of two orthogonal components

E = (E 1 ux + E 2 uy ) e jkz

(2.72)

where ux and uy are the unit vectors in the x and y direction, respectively. In a general case this represents an elliptically polarized wave. The polarization ellipse shown in Figure 2.6(a) is characterized by the axial ratio Emax /Emin , tilt angle t , and direction of rotation. The direction of rotation, as seen in

Fundamentals of Electromagnetic Fields

27

 

 

 

 

 

 

 

 

 

 

 

 

Figure 2.6 Polarization of a plane wave: (a) elliptic; (b) linear; (c) clockwise circular; and

(d) counterclockwise circular.

the direction of propagation and observed in a plane perpendicular to the direction of propagation, is either clockwise (right-handed) or counterclockwise (left-handed).

Special cases of an elliptic polarization are the linear polarization, Figure 2.6(b), and circular polarization, Figure 2.6(c, d). If E1 0 and E2 = 0, we have a wave polarized linearly in the x direction. If both E1 and E2 are nonzero but real and the components are in the same phase, we have a linearly polarized wave, the polarization direction of which is in angle

t = arctan (E2 /E1 )

(2.73)

In the case of circular polarization, the components have equal amplitudes and a 90° phase difference, that is, E1 = ±jE2 = E0 (E0 real), and the electric field is

E = E0 (ux j uy ) e jkz

(2.74)

or

 

E = E0 (ux + j uy ) e jkz

(2.75)

28 Radio Engineering for Wireless Communication and Sensor Applications

The former represents a clockwise, circularly polarized wave, and the latter a counterclockwise, circularly polarized wave. In the time domain the circularly polarized wave can be presented as (clockwise)

E(z , t ) = E0 [ux cos (vt kz ) + uy cos (vt kz p /2)] (2.76)

and (counterclockwise)

E(z , t ) = E0 [ux cos (vt kz ) uy cos (vt kz p /2)] (2.77)

At z = 0, (2.76) and (2.77) are reduced to

E(t ) = E0 [ux cos vt ± uy cos (vt p/2)]

(2.78)

2.6 Reflection and Transmission at a Dielectric Interface

Let us consider a plane wave that is incident at a planar interface of two lossless media, as illustrated in Figure 2.7. The wave comes from medium 1, which is characterized by e1 and m 1 , to medium 2 with e 2 and m2 . The planar interface is at z = 0. The angle of incidence is u 1 and the propagation vector k1 is in the xz -plane. Part E1from the incident field is reflected at an angle u 1and part E2 is transmitted through the interface and leaves at an angle of u2 .

Figure 2.7 Reflection and transmission of a plane wave in case of an oblique incidence at an interface of two lossless media: (a) parallel polarization, and (b) perpendicular polarization.

Fundamentals of Electromagnetic Fields

29

According to the boundary conditions, the tangential components of the electric and magnetic field are equal on both sides of the interface in each point of plane z = 0. This is possible only if the phase of the incident, reflected, and transmitted waves change equally in the x direction, in other words, the phase velocities in the x direction are the same, or

v 1

 

=

v 1

=

v 2

 

(2.79)

sin u

1

sin u

sin u

 

 

 

1

 

 

2

where v 1 and v 2 (vi = v/k i ) are the wave velocities in medium 1 and 2, respectively. From (2.79) it follows

u1′ = u1

(2.80)

which means the angle of incidence and angle of reflection are equal, and the angle of propagation of the transmitted wave is obtained from

sin u2

=

m1 e1

(2.81)

sin u1

m2 e 2

 

Let us assume in the following that m1 = m 2 = m 0 , which is valid in most cases of interest in practice. Then (2.81), which is called Snell’s law, can be rewritten as

sin u2

=

e1

=

er1

n 1

 

 

 

 

 

 

=

 

 

(2.82)

sin u 1

e2

er2

n 2

where n 1 = er1 and n 2 = er2 are the refraction indices of the materials. The reflection and transmission coefficients depend on the polarization of the incident wave. Important special cases are the so-called parallel and

perpendicular polarizations; see Figure 2.7. The parallel polarization means that the electric field vector is in the same plane with k1 and the normal n of the plane, that is, the field vector is in the xz -plane. The perpendicular polarization means that the electric field vector is perpendicular to the plane described previously, that is, it is parallel to the y -axis. The polarization of an arbitrary incident plane wave can be thought to be a superposition of the parallel and perpendicular polarizations.

In the case of the parallel polarization, the condition of continuity of the tangential electric field is

30 Radio Engineering for Wireless Communication and Sensor Applications

E 1 cos u1 + E 1cos u1′ = E 2 cos u2

(2.83)

which leads, with the aid of (2.80) and (2.82), to

 

 

 

 

 

 

 

 

 

 

 

 

 

e1

2

 

 

 

(E 1 + E 1) cos u 1 = E 2 1

 

sin

 

u1

(2.84)

e2

 

The magnetic field has only a component in the y direction. The continuity of the tangential magnetic field leads to

(E 1 E 1)

 

= E 2

 

(2.85)

e 1

e 2

From (2.84) and (2.85) we can solve for the parallel polarization the reflection and transmission coefficients, r || and t || , respectively:

 

E 1

 

 

 

 

e 2

 

sin2 u1

e2

 

cos u1

 

 

 

 

 

 

 

 

 

 

r || =

=

e 1

 

 

 

 

 

 

 

 

e1

(2.86)

E 1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e 2

sin2 u1

 

+

e2

cos u1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e 1

 

 

 

 

 

 

 

 

 

e1

 

 

 

 

 

2

 

e2

cos u 1

 

 

 

 

 

 

 

 

 

 

t || =

E 2

 

=

e1

(2.87)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

E 1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e 2

sin2 u1

+

e2

cos u 1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e1

 

 

 

 

 

 

 

e 1

 

When the angle of incidence is 90°, that is, when the incident wave approaches perpendicularly to the surface, it holds for r and t that

1 + r = t

(2.88)

In case of the perpendicular polarization, the boundary conditions lead

to

 

E 1 + E 1′ = E 2

(2.89)

(E 1 E 1)

 

cos u1 = E 2

 

cos u2

(2.90)

e1

e 2

from which we can solve for the perpendicular polarization