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Waveguides - ieeetsu

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www.ece.rutgers.edu/∼orfanidi/ewa 273<br />

274 Electromagnetic Waves & Antennas – S. J. Orfanidis – June 21, 2004<br />

Although these expressions look different, they are actually equal, W e ′ = W m ′ . Indeed,<br />

using the property β 2 /k 2 c + 1 = (β2 + k 2 c )/k2 c = k2 /k 2 c = ω2 /ω 2 c and the relationships<br />

between the constants in (8.7.1), we find:<br />

µ ( |H 1 | 2 +|H 0 | 2) = µ ( |H 0 | 2 β2<br />

k 2 +|H 0 | 2) = µ|H 0 | 2 ω2<br />

c<br />

ωc<br />

2 = µ η |E 0| 2 = ɛ|E 2 0 | 2<br />

The equality of the electric and magnetic energies is a general property of waveguiding<br />

systems. We also encountered it in Sec. 2.3 for uniform plane waves. The total<br />

energy density per unit length will be:<br />

The field expressions (8.4.3) were derived assuming the boundary conditions for<br />

perfectly conducting wall surfaces. The induced surface currents on the inner walls of<br />

the waveguide are given by J s = ˆn × H, where the unit vector ˆn is ±ˆx and ±ŷ on the<br />

left/right and bottom/top walls, respectively.<br />

The surface currents and tangential magnetic fields are shown in Fig. 8.8.1. In particular,<br />

on the bottom and top walls, we have:<br />

W ′ = W ′ e + W′ m = 2W′ e = 1 4 ɛ|E 0| 2 ab (8.7.5)<br />

According to the general relationship between flux, density, and transport velocity<br />

given in Eq. (1.5.2), the energy transport velocity will be the ratio v en = P T /W ′ . Using<br />

Eqs. (8.7.4) and (8.7.5) and noting that 1/ηɛ = 1/ √ µɛ = c, we find:<br />

√<br />

v en = P T<br />

W ′ = c 1 − ω2 c<br />

(energy transport velocity) (8.7.6)<br />

ω 2<br />

This is equal to the group velocity of the propagating mode. For any dispersion<br />

relationship between ω and β, the group and phase velocities are defined by<br />

v gr = dω<br />

dβ ,<br />

v ph = ω β<br />

(group and phase velocities) (8.7.7)<br />

For uniform plane waves and TEM transmission lines, we have ω = βc, so that v gr =<br />

v ph = c. For a rectangular waveguide, we have ω 2 = ω 2 c + β2 c 2 . Taking differentials of<br />

both sides, we find 2ωdω = 2c 2 βdβ, which gives:<br />

√<br />

v gr = dω<br />

dβ = βc2<br />

ω<br />

= c 1 − ω2 c<br />

ω 2 (8.7.8)<br />

where we used Eq. (8.1.10). Thus, the energy transport velocity is equal to the group<br />

velocity, v en = v gr . We note that v gr = βc 2 /ω = c 2 /v ph ,or<br />

Fig. 8.8.1<br />

Currents on waveguide walls.<br />

J s =±ŷ × H =±ŷ × (ˆx H x + ẑH z )=±(−ẑ H x + ˆx H z )=±(−ẑ H 1 sin k c x + ˆx H 0 cos k c x)<br />

Similarly, on the left and right walls:<br />

J s =±ˆx × H =±ˆx × (ˆx H x + ẑH z )=∓ŷ H z =∓ŷ H 0 cos k c x<br />

At x = 0 and x = a, this gives J s =∓ŷ(±H 0 )= ŷ H 0 . Thus, the magnitudes of the<br />

surface currents are on the four walls:<br />

{<br />

|J s | 2 |H0 | 2 , (left and right walls)<br />

=<br />

|H 0 | 2 cos 2 k c x +|H 1 | 2 sin 2 k c x, (top and bottom walls)<br />

The power loss per unit z-length is obtained from Eq. (8.2.8) by integrating |J s | 2<br />

around the four walls, that is,<br />

P ′ loss = 2 1 2 R s<br />

∫ a<br />

0<br />

|J s | 2 dx + 2 1 2 R s<br />

∫ b<br />

0<br />

|J s | 2 dy<br />

v gr v ph = c 2 (8.7.9)<br />

The energy or group velocity satisfies v gr ≤ c, whereas v ph ≥ c. Information transmission<br />

down the guide is by the group velocity and, consistent with the theory of<br />

relativity, it is less than c.<br />

8.8 Power Attenuation<br />

In this section, we calculate the attenuation coefficient due to the ohmic losses of the<br />

conducting walls following the procedure outlined in Sec. 8.2. The losses due to the<br />

filling dielectric can be determined from Eq. (8.2.5).<br />

∫ a<br />

(<br />

= R s |H0 | 2 cos 2 k c x +|H 1 | 2 sin 2 k c x ) ∫ b<br />

dx + R s |H 0 | 2 dy<br />

0<br />

0<br />

a (<br />

= R s |H0 | 2 +|H 1 | 2) + R s b|H 0 | 2 = R sa (<br />

|H0 | 2 +|H 1 | 2 + 2b 2<br />

2<br />

a |H 0| 2)<br />

Using |H 0 | 2 +|H 1 | 2 =|E 0 | 2 /η 2 from Sec. 8.7, and |H 0 | 2 = (|E 0 | 2 /η 2 )ωc/ω 2 2 , which<br />

follows from Eq. (8.4.2), we obtain:<br />

P ′ loss = R sa|E 0 |<br />

(1 2<br />

+ 2b )<br />

ω 2 c<br />

2η 2 a ω 2<br />

The attenuation constant is computed from Eqs. (8.2.9) and (8.7.4):

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