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10. Electromagnetic Wave Propagation

Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

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Page 1: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

10. Electromagnetic WavePropagation

Page 2: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

1

10.2 WAVE IN GENERAL

u/

eEE

)3.10(0Et

E

)c2.10()utz(g)utz(fEEE

)b2.10()utz(gE

)a2.10()utz(fE

)1.10(0z

Eu

t

E

tjs

s2

2s

2

2

22

2

2

Page 3: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

2

tj

2

22

2

2

2

2

2

22

2

22

2

2

2

2

2

22

22

2

2

e~B,E

1cwhere

0E~

cE~

0t

E

c

1E

0t

EE

0B~

cB~

0t

B

c

1B

0t

BB

BB)

B(

t

B

t

EB

t

BE

Jt

EB

𝛻 × 𝛻 × u = 𝛻(𝛻 ∙ u) − 𝛻2u

Page 4: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

3

참고: Vector identity (벡터 항등식)

𝛻 ∙ φu = φ𝛻 ∙ u + u ∙ 𝛻φ

𝛻 × φu = φ𝛻 × u + 𝛻φ × u

𝛻 ∙ u × v = v ∙ 𝛻 × u − u ∙ 𝛻 × v

𝛻 × u × v = v ∙ 𝛻u − u ∙ 𝛻v + v ∙ 𝛻u − v ∙ 𝛻u

𝛻 u ∙ v = u ∙ 𝛻v + v ∙ 𝛻u + u × (𝛻 × v) +v × (𝛻 × u)

𝛻 × 𝛻φ = 0

𝛻 ∙ 𝛻 × u = 0

𝛻 × 𝛻 × u = 𝛻(𝛻 ∙ u) − 𝛻2u

𝛻 ∙ 𝛻φ1 × 𝛻φ2 = 0

a × b × c = (a ∙ c)b − (b ∙ a) c

a × b ∙ c × d = a ∙ c ∙ b ∙ d − a ∙ d ∙ b ∙ c

Page 5: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

4

(a) Traveling Wave.

𝐇 = 𝐇𝐢𝟎 𝐜𝐨𝐬 (βz−ω𝐭) 𝐚𝐱.

(b) Standing Wave.

𝐇 = 𝟐𝐇𝐢𝟎 𝐜𝐨𝐬 (βz)cos(ω𝐭) 𝐚𝐱.

Hx = Acos βz − ωtβz − ωt = c

vφ ≡dz

dt=

ω

β← Phase velocity

H

0 z

z

z

0

0

ωt=0

ωt=π/2

ωt=π

H

0z

z

z

0

0

ωt=0

ωt=π/2

ωt=π

Page 6: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

5

)b6.10(fu

)a6.10(uT

)ztcos(A

or

)5.10()ztsin(AE

)c4.10(BeAeE

)b4.10(BeE

)a4.10(AeE

)zt(j)zt(j

)zt(j

)zt(j

ejωt를 생각하면틀린 것은 아니나 불편.cos 이 편하다.

Page 7: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

6

)9.10(udt

dz

constantzt

)8.10(2

)c7.10(2

f

1T

)b7.10(u

)a7.10(f2

Page 8: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

7

Fig 10.1 E(z,t)=A·sin(ωt-βz)의 그림.

2

2

f

1T

u

f2

)ztsin(AE

E

z

(a) constant t

A

-A

λ

0

λλ

2

2

E

t

(b) constant z

A

-A

T

0

TT

2

3T

2

Page 9: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

8

Fig 10.2 E(z,t)=A·cos(ωt-βz)의 그림.

P는 +z 방향으로 u의 속도로 이동.

udt

dz

ttanconszt

)ztcos(AE

PH

0 z

z

z

0

0

ωt=0

ωt=π/2

ωt=π

Page 10: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

9

Table 10.1 Electromagnetic spectrum

EM Phenomena Examples od Uses Approximate Frequency Range

Cosmic rays

Gamma rays

X-rays

자외선가시광선적외선Microwaves

Radio waves

Physics, astronomy

Cancer therapy

X-ray examination

Sterilization

Human vision

Photography

Radar, microwave relays,

satellite communication

UHF TV

VHF TV, FM radio

Short-wave radio

AM radio

1014 GHz and above

1010~1013 GHz

108~109 GHz

106~108 GHz

105~106 GHz

103~104 GHz

3~300 GHz

470~806 MHz

54~216 MHz

3~26 MHz

535~1605 KHz

Page 11: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

10

)9.10(udt

dz

)8.10(2

)c7.10(2

f

1T

)b7.10(u

)a7.10(f2

예제 10.1 전장 E = 50 cos ωt + x/λ ay volt/m = 50 cos 108t + βx ay volt/m 가 주어졌다.

(a) wave의 진행 방향(b) β를 계산하고 λ/2 만큼의 거리를 진행하는 동안 걸리는 시간을 구하라.(c) t=0, T/4, T/2에서의 wave를 그려라.

(a) wave의 진행 방향: −ax 방향.시간이 지났을 때 동일 phase인 지점은 –ax 에 있다.

(b) β를 계산하고 λ/2 만큼의 거리를 진행하는 동안 걸리는 시간을 구하라.

sec1022/

f

1xt

m3

1

103

10

c

8

1

8

8

(c) t=0, T/4, T/2에서의 wave를 그려라.

Page 12: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

11Fig 10.3 For Example 10.1;

wave travels alongax.

(c) t=0, T/4, T/2에서의 wave를 그려라.

2

f

1T)c7.10(

2/Ttforxcos50

x2

2cos50E

4/Ttforx2/cos50

x4

2cos50E

0tforxcos50E

xtcos50E

y

y

y

y

-50

λ 2λ-λ-2λ

50

y

x

-50

0 λ 2λ-λ-2λ

50

y

x

50cosβx

0

-50

λ 2λ-λ-2λ

50

y

x0

50cos(βx+π/2)

50cos(βx+π)

(a) t=0

(c) t=T/2

(b) t=T/4

u

Page 13: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

12

10.3 Wave Propagation in Lossy Dielectrics

)14.10(E)j(H

E)j(

Et

E

Jt

EH

)13.10(HjE

t

HE

)12.10(0H

)11.10(0E

ss

ss

s

s

)18.10()j(j

)17.10(0EE

0E)j(jE

E)j(j

HjE

E

E)E(E

)16.10(A)A(A

)15.10(HjE

2

s2

s2

ss2

s

ss2

s2

s2

ss

2

ss

Space charge ρ=0

J ≠ 𝟎

Page 14: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

13

ss

ss

s

s

tjs

tjs

tjs

tjs

tjs

tjs

E)j(H)14.10(

HjE)13.10(

0H)12.10(

0E)11.10(

)eE)(j()eH(

)eH(j)eE(

0)eH(

0)eE(

t

EEH

t

HE

0H

0E

참고:

Vector identity

𝛻 ∙ φu = φ𝛻 ∙ u + u ∙ 𝛻φ

𝛻 × φu = φ𝛻 × u + 𝛻φ × u

𝛻 ∙ u × v = v ∙ 𝛻 × u − u ∙ 𝛻 × v

𝛻 × u × v = v ∙ 𝛻u − u ∙ 𝛻v + v ∙ 𝛻u − v ∙ 𝛻u

𝛻 u ∙ v = u ∙ 𝛻v + v ∙ 𝛻u + u × (𝛻 × v) +v × (𝛻 × u)

𝛻 × 𝛻φ = 0

𝛻 ∙ 𝛻 × u = 0

𝛻 × 𝛻 × u = 𝛻(𝛻 ∙ u) − 𝛻2u

𝛻 ∙ 𝛻φ1 × 𝛻φ2 = 0

a × b × c = (a ∙ c)b − (b ∙ a) c

a × b ∙ c × d = a ∙ c ∙ b ∙ d − a ∙ d ∙ b ∙ c

Page 15: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

14

)18.10()j(j

)19.10(0HH

0H)j(jH

H)j(j

E)j(H

H

H)H(H

A)A(A

E)j(H

)18.10()j(j

)17.10(0EE

2

s2

s2

ss2

s

ss2

s2

s2

ss

2

ss

2

s2

s2

ss HjE)13.10(

Page 16: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

15

)24.10(112

)23.10(112

)21.10(]Re[

)22.10()2()(

2j

)20.10(j

j

)18.10()j(j

2

2

2222

2222222222

222

2

2

Page 17: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

16

)30.10()aeeRe(H)t,z(H

0)z(Hdz

d

a)eeRe(E

)29.10(a)ztcos(eEt)(z,E

)28.10(eEeE(z)E

)27.10(0)z(Edz

d

)26.10(0)z(E)(

)25.10(a)z(EE

y)zt(jz

o

ys2

2

2

x)zt(jz

o

xz

0

z0

z0s

xs2

2

2

s22

xxss

α: “+α”는 물리적 문제 때문에해가 될 수 없음.

β: 편의에 의해 “–β” 만 채택.

j)20.10(

)j(j)18.10( 2

z

x

y

E

Page 18: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

17

)31.10(H

Ej

HjEE)j(

HjeeHj

eeE)j(z

E

aeeEt)(z,E

Hjaz

E

00E

z00

aaa

E

HjE)13.10(

0

0

ooo

y)zt(jz

o

)zt(jzo

x

x)zt(jz

o

syxs

xs

zyx

s

ss

j)20.10(

j22

)32.10(impedancewave:j

j

j

j

j

j

j

)31.10(H

E

2

22

2

0

0

Page 19: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

18

)32.10(impedance:j

j

)31.10()30.10()29.10(E

H

)30.10()aeeRe(H)t,zH(

)29.10(a)ztcos(eEt)(z,E

)28.10(eEeE(z)E

00

y)zt(jz

o

xz

0

z0

z0s

고유

0HH)19.10( s2

s2

j)20.10(

)j(j)18.10(

0)z(Edz

d)27.10(

0EE)17.10(

2

xs2

2

2

s2

s2

ss

ss

E)j(H)14.10(

HjE)13.10(

Page 20: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

19

Fig 10.5 시간 t=0와 t=Δt에서 +z 방향으로 진행하는 E의 x 성분: 화살표는

E의 순시 값을 나타낸다.

x

z

t=0

t=Δt

Δt

e−αz ∗ cos(βz − ωt)

Page 21: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

20

)34.10(a)ztcos(eE

aeeE

aeee

E

aeeE

H

yz0

y)zt(jz0

y)zt(jz

j0

y)zt(jz0

)33.10(

2tan

1)32.10(

e

j

j

41

2

j

η도 complex

Page 22: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

21

ss

ss

s

s

tjs

tjs

tjs

tjs

tjs

tjs

E)j(H)14.10(

HjE)13.10(

0H)12.10(

0E)11.10(

)eE)(j()eH(

)eH(j)eE(

0)eH(

0)eE(

t

EEH

t

HE

0H

0E

Page 23: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

22

)37.10(2tan

e

)(

j

j

j

ej

j)32.10(

2

2j2

22

22

j

jσωμ

Re

Im

η 2

2θη=θ

ω2με

Page 24: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

23

(10.35)dB 686.8elog20 Np 1

output:o,input:i

:V

Vlog20 dBins

10

i

o10

정의전압이득의

)37.10()2(tan

: 손실 Tangent

- Np/m: 감쇄율의 단위- 1 neper 감쇄는 e-1 만큼 줄어든 것.

- 1 neper 감쇄가 일어난 길이를 δ라고 정의 한다.

- 매우 작으면 무손실 유전체- 매우 크면 양도체

1 neper 증가

𝐇 = 𝟏𝟎𝐞−𝛂𝐱 𝐜𝐨𝐬 𝛚𝐭 − 𝐱/𝟐 𝐚𝐲 𝐀/𝐦

감쇄율 𝛂의 단위는 Np/m

Page 25: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

24

)37.10(tanEj

E

J

J

s

s

ds

cs

tanθ (손실 Tangent)

- 매우 작으면 무손실 유전체- 매우 크면 양도체

)2(tan)37.10(

Fig 10.6 Loss angle of

a lossy medium.

sEj

sE

jσωμ

Re

Im

η 2

2θη=θ

ω2με

ss

2

2j2

22

22

j

00

E)j(H

)37.10(2tan

e

)(

j

j

j

ej

j)32.10(

EH)31.10(

Page 26: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

25

)41.10(tan

)b40.10(j

)a40.10(j1

)39.10(Ej

Ej

1j

E)j(H

)38.10()37.10(&)33.10(from2

c

c

sc

s

ss

Page 27: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

26

예제 10.2 손실 유전체가 특정한 각속도 ω에서 wave impedance 𝛈 = 200ejπ/6 Ω 이다.

𝐇 = 𝟏𝟎𝐞−𝛂𝐱 𝐜𝐨𝐬 𝛚𝐭 − 𝐱/𝟐 𝐚𝐲 𝐀/𝐦 일 때 𝐄와 α를 구하라.

)aeee2000Re(E

e2000E

e200H

E

aa

aaaaaa

a

a)aa(aa

aaa

aaa

HEP

aa

aawave

Etjx6/j

6/j0

6/j

0

0

zE

zyxHkE

E

yyEyx

yEx

HEk

yH

xk

진행방향

진행 방향

y

z

x

aE aH

ak

j)20.10(

j)18.10( 22

Page 28: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

27

예제 10.2 손실 유전체가 특정한 각속도 ω에서 200ejπ/6 Ω의 wave impedance를 갖는다.

𝐇 = 𝟏𝟎𝐞−𝛂𝐱 𝐜𝐨𝐬 𝛚𝐭 − 𝐱/𝟐 𝐚𝐲 𝐀/𝐦 일 때 𝐄와 α를 구하라.

m32/1

2

1m/Np

32

1

3

360tan2tan3/1

11

11

112

)24.10(

112

)23.10(

o

2/1

2

2

2

2

)37.10(2tan

e

)(

j

j

j

ej

j)32.10(

EH)31.10(

)2(tan)37.10(

112

)24.10(

112

)23.10(

j)20.10(

j)18.10(

2

2j2

22

22

j

00

2

2

22

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28

10.4 Plane Waves in Lossless Dielectrics

)44.10(0

)b43.10(22

f

u

c1

u

)a43.10(0

)42.10(

0

ro

ro

112

)24.10(

112

)23.10(

2

2

𝐄와 𝐇는 위상이 같다. σ=0

je

j

j)32.10(

)9.10(udt

dz

)8.10(2

)c7.10(2

f

1T

)b7.10(u

)a7.10(f2

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29

10.5 Plane Waves in Free Space

)47.10(377120

10014436/10

104

)b46.10(2

c1

u

)a46.10(c/

0

)45.10(

0

2

9

7

0

00

00

00

o

o

)49.10(aaa

)b48.10(a)ztcos(E

a)ztcos(HH

)a48.10(a)ztcos(EE

kHE

y0

0

y0

x0

y)zt(jz0

x)zt(jz

0

aeeE

H

aeeEE

𝐚𝐇

𝐚𝐤

𝐚𝐄

𝐳𝐲

𝐱

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30

Fig 10.7 Plots of 𝐄 and 𝐇. The arrows

indicate instantaneous values

kHE

y)zt(jz0

x)zt(jz

0

aaa(10.49)

aeeE

H

aeeEE

𝐚𝐇

𝐚𝐤

𝐚𝐄

𝐳𝐲

𝐱 x

y

E = E0cos(−βz)ax

H = H0cos(−βz)ay

(b) at t=0

x

y

z

E = E0cos(−βz)ax

H = H0cos(−βz)ay

𝐚𝐤

(a) at t=0

Page 32: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

31

10.6 Plane Waves in Good Conductors

2tan)37.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

j

2

2

)52.10(45

)b51.10(2

,2

u

)a51.10(f2/

)50.10(

ro

o

주어진 전장에서 전하를축적할 수 있는 능력.의미 없음.

Page 33: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

32

)55.10(j1

e21

)b54.10(depthskin:f

1

)a54.10(1

)b53.10(a)4/ztcos(eE

H

)a53.10(a)ztcos(eEE

4/j

yzo

xz

o

yz0 a)ztcos(e

EH)34.10(

f2/)a51.10(

45)52.10(

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33

Fig 10.8 Illustration of skin depth. Fig 10.9 Skin depth at high frequencies.

δ

a

z

E0

0.368E0

δ

0

x

e−αz

𝐞−𝛂𝐳𝐜𝐨𝐬(𝛚𝐭 − 𝛃𝐳)

δ = 1/α

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34

표 10.2 구리의 표피 깊이.

주파수 (Hz) 10 60 100 500 104 108 1010

표피 깊이 (mm) 20.8 8.6 6.6 2.99 0.66 6.6x10-3 6.6x10-4

구리의 경우 𝛔 = 𝟓. 𝟖 × 𝟏𝟎𝟕 𝐒/𝐦𝛍 = 𝛍𝟎

𝟏𝟎. 𝟓𝟒𝐛 𝛅 = 𝟏/ 𝛑𝐟𝛍𝛔 = 𝟔𝟔. 𝟏 / 𝐟 (단위는 mm)

Fig 10.9 Skin depth at high frequencies.

δ

a

)b54.10(depthskin:f

1

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35

)57.10(w

R

wR

)56.10(f1

R

)16.5(S

R

sac

s

dc

Surface or Skin Resistance:

Sheet 인 경우의단위 폭, 단위 길이 당 저항.

j1e2

1)55.10(

depthskin:f

1)b54.10(

EH)31.10(

4/j

oo

w

δ

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36

1

2j1

)57.10(w

RVIw

V

w

IEH

1

VE

w

IH

EH)31.10(

w

I

)a~(2

I

)ba(2

I

)a0(a2

I

H)29.7(

ac0

0o

o

oo

2

과소평가는

aI

-I

a

b

ρz

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37

예제 10.3 η=60π, μr=1, H = −0.1 cos ωt − z ax + 0.5 sin ωt − z ay A/m 인 무손실 매질에서

εr , ω, 𝐄 를 계산하라.

sec/rad105.1

1103

24

c

4

60120

)44.10(

j

j)32.10(

1,0,0

8

8

rr00

r

r

r

r

0

0

무손실매질

)44.10(0

)b43.10(22

f

u

c1

u

)a43.10(0

)42.10(

0

ro

ro

매질무손실

Page 39: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

38xy

x2

2020

xyzHkE

y1

1010

HEk

yxzHkE

E202

E101

21

y2

x121

a)ztsin(30a)ztcos(6E

a)ztsin(30E

30)5.0(60HE

a)aa()aa(a

a)ztcos(6E

6)1.0(60HE

aaawhere

a)aa()aa(a

a)ztsin(EE

a)ztcos(EEwhereEEE

a)ztsin(5.0H

)a)(ztcos(1.0HwhereHHH

1

22

11

2

1

방법

sec/rad105.1

1103

24

c

4

60120

)44.10(

j

j)32.10(

1,0,0

8

8

rr00

r

r

r

r

0

0

무손실매질

예제 10.3 η=60π, μr=1, H = −0.1 cos ωt − z ax + 0.5 sin ωt − z ay A/m 인 무손실 매질에서

εr , ω, 𝐄 를 계산하라.

𝐚𝐇

𝐚𝐤

𝐚𝐄

𝐳𝐲

𝐱

𝐚𝐄

𝐚𝐤

𝐚𝐇

𝐳𝐲

𝐱

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39

yx

y8

9x8

9

y10

x20

y10x20

y10x20

y10x20

yx

xy

yx

zyx

yx

zyx

a)ztcos(30a)ztsin(6E

a)ztcos(

105.136

104

10/1a)ztsin(

105.136

104

2/1

a)ztcos(H

a)ztsin(H

dta)ztsin(Ha)ztcos(H1

dtH1

E

a)ztsin(Ha)ztcos(H

a)]ztcos(H[z

a)]ztsin(H[z

az

Ha

z

H

0)z(H)z(H

z00

aaa

0)z(H)z(H

zyx

aaa

H

dtH1

E

t

E

t

EEH

2

방법

𝐇 = −𝟎. 𝟏 𝐜𝐨𝐬 𝛚𝐭 − 𝐳 𝐚𝐱 + 𝟎. 𝟓 𝐬𝐢𝐧 𝛚𝐭 − 𝐳 𝐚𝐲

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40

예제 10.4 매질 내에서 전파되는 균일 평면파가

𝐄 = 𝟐𝐞−𝛂𝐳 𝐬𝐢𝐧 𝟏𝟎𝟖𝐭 − 𝛃𝐳 𝐚𝐲 = 𝐄𝟎𝐞−𝛂𝐳𝐞−𝐣𝛑/𝟐𝐞𝐣(𝛚𝐭−𝛃𝐳)𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦 이다.

εr=1, μr=20, σ=3 S/m일 때 α, β, 𝐇를 구하라.

)a(eeee

E

a)ztsin(eHH

e

4

2233932tan

3

800

4.612

)a51.10(

13393

10

2E

x)zt(j2/jz

4/j0

Hz

0

4/j

8

0

전도체

tan)41.10(

4/j0

j0

00 e

1Ee

1E

EH

xyzEkH aaaaaa

sds EjJ

ss EJ

112

)24.10(

112

)23.10(

2

2

2tan)37.10(

ej

j)32.10(

j

𝐚𝐇

𝐚𝐤

𝐚𝐄

𝐳𝐲

𝐱

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41

)ztcos(j)ztsin(

)ztsin(j)ztcos(j

)ztsin(j)ztcos(2

sinj2

cos

ee

e

)ztsin(

)ztsin()2/sin()ztcos()2/cos()zt2/cos(

)zt(j)2/(j

)zt2/(j

112

)24.10(

112

)23.10(

2

2

예제 10.4 매질 내에서 전파되는 균일 평면파가

𝐄 = 𝟐𝐞−𝛂𝐳 𝐬𝐢𝐧 𝟏𝟎𝟖𝐭 − 𝛃𝐳 𝐚𝐲 = 𝐄𝟎𝐞−𝛂𝐳𝐞−𝐣𝛑/𝟐𝐞𝐣(𝛚𝐭−𝛃𝐳)𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦 이다.

εr=1, μr=20, σ=3 S/m일 때 α, β, 𝐇를 구하라.

Im

Re

j

2/

Page 43: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

42

xz0

z0

x)2/4/zt(jz0

xzt2/jz

4/j0

Hz

0

a)4/ztsin(eE

H

)2/4/ztcos(eE

aeeE

)a(eeee

E

a)ztsin(eHH

)a(eeee

E

a)ztsin(eHH

e

4

2233932tan

3

800

4.612

)a51.10(

13393

x)zt(j2/jz

4/j0

Hz

0

4/j

전도체

예제 10.4 매질 내에서 전파되는 균일 평면파가

𝐄 = 𝟐𝐞−𝛂𝐳 𝐬𝐢𝐧 𝟏𝟎𝟖𝐭 − 𝛃𝐳 𝐚𝐲 = 𝐄𝟎𝐞−𝛂𝐳𝐞−𝐣𝛑/𝟐𝐞𝐣(𝛚𝐭−𝛃𝐳)𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦 이다.

εr=1, μr=20, σ=3 S/m일 때 α, β, 𝐇를 구하라.

𝐚𝐇

𝐚𝐤

𝐚𝐄

𝐳𝐲

𝐱

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43

예제 10.5 평면파 𝐄 = 𝐄𝟎 𝐬𝐢𝐧 𝟏𝟎𝟖𝐭 − 𝛃𝐳 𝐚𝐱 V/m 가 진공에서 양도체로 입사 된다.

도체 내의 전류 밀도 J 를 구하라.

j1)j1(j

/1for1

))z(J(0B

BeAeJ

0Jz

J

EJ0JJ

/1)a54.10(

j)20.10(

)j(j)18.10(

0EE)17.10(

sx

zzsx

sx2

2sx

2

s2

s2

2

s2

s2

양도체

)zt10(j/zsxx

t10j)j1(zsxx

)j1(zsx

)j1(zsx

8

8

ee)0(JJ

ee)0(JJ

e)0(J

AeJ

112

)24.10(

112

)23.10(

2

2

Page 45: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

44

)57.10(w

R

wR

)56.10(f1

R

)16.5(S

R

sac

s

dc

예제 10.6 다음 동축 cable에서 a=2 mm, b=6 mm, t=1 mm인 경우 직류가 흐를 때와100 MHz 교류가 흐를 때 cable 저항을 계산하라. 길이는 L=2 m 이다.

σ = 5.8 × 107 S/m μr = 1

m4.548RRR

1384.0f

b2b2w

RR

41.0f

a2a2w

RR

m587.3RRR

m8429.0]b)tb[(S

R

m744.2aS

R

RRR

i0ac

so

si

i0dc

22o

2i

innerouter

경우교류인

경우직류인

AC 저항이 훨씬 크다.

L

ab

t

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45

표 10.2 구리의 표피 깊이.

주파수 (Hz) 10 60 100 500 104 108 1010

표피 깊이 (mm) 20.8 8.6 6.6 2.99 0.66 6.6x10-3 6.6x10-4

구리의 경우 𝛔 = 𝟓. 𝟖 × 𝟏𝟎𝟕 𝐒/𝐦𝛍 = 𝛍𝟎

𝟏𝟎. 𝟓𝟒𝐛 𝛅 = 𝟏/ 𝛑𝐟𝛍𝛔 = 𝟔𝟔. 𝟏 / 𝐟 (단위는 mm)

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46

10.7 Power and The Poynting Vector

t

)H(

2t

)E(

2E)HE(

)61.10(t

)H(

2t

HH)E(H

)60.10(t

EEE)HE()E(H

)59.10(t

)E(

2E

t

EJE)H(E

)H(E)E(H)HE(

)b58.10(t

EE

t

EJH

)a58.10(t

HE

222

2

2

22

𝛻 ∙ u × v = v ∙ 𝛻 × u − u ∙ 𝛻 × v

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47

참고: Vector identity (벡터 항등식)

𝛻 ∙ φu = φ𝛻 ∙ u + u ∙ 𝛻φ

𝛻 × φu = φ𝛻 × u + 𝛻φ × u

𝛻 ∙ u × v = v ∙ 𝛻 × u − u ∙ 𝛻 × v

𝛻 × u × v = v ∙ 𝛻u − u ∙ 𝛻v + v ∙ 𝛻u − v ∙ 𝛻u

𝛻 u ∙ v = u ∙ 𝛻v + v ∙ 𝛻u + u × (𝛻 × v) +v × (𝛻 × u)

𝛻 × 𝛻φ = 0

𝛻 ∙ 𝛻 × u = 0

𝛻 × 𝛻 × u = 𝛻(𝛻 ∙ u) − 𝛻2u

𝛻 ∙ 𝛻φ1 × 𝛻φ2 = 0

a × b × c = (a ∙ c)b − (b ∙ a) c

a × b ∙ c × d = a ∙ c ∙ b ∙ d − a ∙ d ∙ b ∙ c

Page 49: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

48

)63.10(dvEdvH2

1E

2

1

t-Sd)HE(

)62.10(dvEdvH2

1E

2

1

tdv)HE(

Et

)H(

2t

)E(

2)HE(

v2

v22

S

v2

v22

v

222

Total powerleaving the volume

저장된전장, 자장 energy

Ohmic powerdissipated= -

(10.49)aaa

(10.65)HEp:VectorPoynting

HEk

(10.64)

Page 50: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

49

Fig 10.10 Illustration of power

balance for EM fields.

v2

v22

SdvEdvH

2

1E

2

1

t-Sd)HE()63.10(

Total powerleaving the volume

저장된전장, 자장 energy

Ohmic powerdissipated

= -

Page 51: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

50

)70.10(SdpP

)69.10(acose2

E)z(p

)68.10(HERe2

1

)67.10(dt)t,z(pT

1)z(p

)66.10(a )z2t2cos(cose2

E

a )ztcos()ztcos(eE

)t,z(p

a)ztcos(eE

)t,z(H

a)ztcos(eE)t,z(E

aeeE

)t,z(H

aeeE)t,z(E

e

S aveave

zz2

20

ave

ss

T

0ave

zz2

20

zz2

20

yz0

xz

0

y)zt(jz0

x)zt(jz

0

j

𝐚𝐄𝐚𝐤

𝐚𝐇

𝐳𝐲

𝐱

v2

v22

SdvEdvH

2

1E

2

1

t-Sd)HE()63.10(

Total powerleaving the volume

저장된전장, 자장 energy

Ohmic powerdissipated

= -

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51

tan 1 cot

sin cos

cscsec

2

22

secd

tand

sind

cosd

cosd

sind

tantan1

tantan)tan(

sincos)2cos(

sinsincoscos)cos(

cossin2)2sin(

sincoscossin)sin(

참고

cos)z2t2cos(2

1

)ztcos()ztcos(

)cos()cos(2

1coscos

coscos2)cos()cos(

sinsincoscos)cos(

sinsincoscos)cos(

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52

)68.10(]HERe[2

1

]HEHE[4

1

)67.10(dt)t,z(pT

1p

]eHEHEHEeHE[4

1

]HH[]EE[4

1]HERe[p

]eHeH[2

1]HH[

2

1]HRe[

]eEeE[2

1]EE[

2

1]ERe[

eH)t,z(H

eE)t,z(E

*ss

*sss

*s

T

0ave

t2j*s

*s

*sss

*s

t2jss

**

tjs

tjs

*

tjs

tjs

*

tjs

tjs

)aa(2

1]aRe[

cba

bca

j1a

j1a

*

참고

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53

7.9810

59.14c

c

102

8.0

00

)a(

2

2

r

r0r0

0r

0

7

매질비자성

매질무손실

예제 10.7 무손실 비자성 매질에서 𝐄 = 𝟒𝐬𝐢𝐧 𝟐𝝅 × 𝟏𝟎𝟕𝐭 − 𝟎. 𝟖𝐱 𝐚𝐳 𝐕/𝐦 이다. 다음을 구하라

(a) εr , η(b) wave에 전달 되는 time-average power(c) 평면 2x+y=5의 100 cm2 되는 면을 통과하는 총 전력.

112

)24.10(

112

)23.10(

2

2

je

j

j)32.10(

2/)]2cos(1[sin

sin21

sincos)2cos(

)sin()sin(

)cos()cos()cos(

2

2

22

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54

W5.724

5

)0,1,2(01.0)0,0,1(81

aSpSdpP

5

)0,1,2(a

)c(

m/mWa81

a2

EdtP

T

1p

a)xt(sinE

HEp

)b(

naveaveave

n

2x

x

20T

oave

x2

20

j

2

2

ej

j)32.10(

112

)24.10(

112

)23.10(

2/)]2cos(1[sin

sin21

sincos)2cos(

)sin()sin(

)cos()cos()cos(

2

2

22

𝐚𝐤

𝐚𝐄

𝐚𝐇

𝐳𝐲

𝐱

예제 10.7 비자성 매질에서 𝐄 = 𝟒𝐬𝐢𝐧 𝟐𝝅 × 𝟏𝟎𝟕𝐭 − 𝟎. 𝟖𝐱 𝐚𝐳 𝐕/𝐦 이다. 다음을 구하라

(a) εr , η(b) wave에 전달 되는 time-average power(c) 평면 2x+y=5의 100 cm2 되는 면을 통과하는 총 전력.

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55

10.8 Reflection of a Plane Wave at Normal Incidence

Incident wave :

Reflected Wave :

H

HEk

2

s2

s2

a/EH

aaa

j)20.10(

)j(j)18.10(

0EE)17.10(

)72.10(ae

EaeH)z(H

aeeE)z(E

)71.10(aeE)z(E

yz

1

ioy

ziois

x)zt(jz

ioi

xz

iois

11

11

1

)74.10(aeE

)a(eH)z(H

)73.10(aeE)z(EIf

yz

1

ro

yz

rors

xz

rors

1

1

1

𝐚𝐤

𝐳𝐲

𝐱𝐚𝐄

𝐚𝐇

𝐚𝐤

𝐳𝐲

𝐱𝐚𝐄

𝐚𝐇

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56

Fig 10.11 A plane wave incident normallyon an interface between two different media.

Transmitted wave :

𝐄𝐢

𝐚𝐤

𝐇𝐢

𝐳𝐲

𝐱

𝐌𝐞𝐝𝐢𝐮𝐦 𝟏 (𝛔𝟏, 𝛆𝟏, 𝛍𝟏) 𝐌𝐞𝐝𝐢𝐮𝐦 𝟐 (𝛔𝟐, 𝛆𝟐, 𝛍𝟐)

Transmitted Wave

Incident Wave

Reflected Wave

𝐄𝐭

𝐚𝐤

𝐇𝐭

𝐇𝐫

𝐚𝐤

𝐄𝐫

)76.10(aeE

aeH)z(H

)75.10(aeE)z(EIf

yz

2

toy

ztots

xz

tots

22

2

𝐚𝐤

𝐳𝐲

𝐱𝐚𝐄

𝐚𝐇

𝐚𝐤

𝐳𝐲

𝐱𝐚𝐄

𝐚𝐇

𝐚𝐤

𝐳𝐲

𝐱𝐚𝐄

𝐚𝐇

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57

ri1

ri1

HHH

EEE

t2

t2

HH

EE

𝐄𝐢

𝐚𝐤

𝐇𝐢

𝐳𝐲

𝐱

𝐌𝐞𝐝𝐢𝐮𝐦 𝟏 (𝛔𝟏, 𝛆𝟏, 𝛍𝟏) 𝐌𝐞𝐝𝐢𝐮𝐦 𝟐 (𝛔𝟐, 𝛆𝟐, 𝛍𝟐)

Transmitted Wave

Incident Wave

Reflected Wave

𝐄𝐭

𝐚𝐤

𝐇𝐭

𝐇𝐫

𝐚𝐤

𝐄𝐫

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58

)80.10(E2

E

)79.10(EE

0zat)78.10(

E)EE(

1 (0)H(0)H)0(H

)77.10(EEE (0)E(0)E)0(E

io12

2to

io12

12ro

2

toroio

1tri

toroiotri

연속성

𝐄𝐢

𝐚𝐤

𝐇𝐢

𝐳𝐲

𝐱

𝐌𝐞𝐝𝐢𝐮𝐦 𝟏 (𝛔𝟏, 𝛆𝟏, 𝛍𝟏) 𝐌𝐞𝐝𝐢𝐮𝐦 𝟐 (𝛔𝟐, 𝛆𝟐, 𝛍𝟐)

Transmitted Wave

Incident Wave

Reflected Wave

𝐄𝐭

𝐚𝐤

𝐇𝐭

𝐇𝐫

𝐚𝐤

𝐄𝐫

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59

0i12

10r0i0t

0i0i21

210r

0r210i21

0r0i20r0i1

0t0r0i

tri

0t20r0i1

HEk

H0t2H0r1H0i1

HEkHEk

E0tE0rE0i

tri

H2

HHH

HHH

H)(H)(

)H(H)H(H

HHH

(0)H(0)H)0(H

H)H(H

aaa

aHaHaH

aaaaaa

aEaEaE

(0)E(0)E)0(E

0zat

연속성

𝐄𝐢

𝐚𝐤

𝐇𝐢

𝐳𝐲

𝐱

𝐌𝐞𝐝𝐢𝐮𝐦 𝟏 (𝛔𝟏, 𝛆𝟏, 𝛍𝟏) 𝐌𝐞𝐝𝐢𝐮𝐦 𝟐 (𝛔𝟐, 𝛆𝟐, 𝛍𝟐)

Transmitted Wave

Incident Wave

Reflected Wave

𝐄𝐭

𝐚𝐤

𝐇𝐭

𝐇𝐫

𝐚𝐤

𝐄𝐫

Ht0 제거

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60

)83.10(

1 0 3.

. .2

1 .1

)b.82.10(EE

)a82.10(2

E

E

)(

)b.81.10(EE

)a81.10(E

E

)(

E2

E

EEE

H2

H

HHH

0i0t

12

2

io

to

0i0r

12

12

io

ro

0i12

20t

0i0i12

120r

0i12

120t2

0i10i121

210r1

복소수는와

투과계수

반사계수

𝐄𝐢

𝐚𝐤

𝐇𝐢

𝐳𝐲

𝐱

𝐌𝐞𝐝𝐢𝐮𝐦 𝟏 (𝛔𝟏, 𝛆𝟏, 𝛍𝟏) 𝐌𝐞𝐝𝐢𝐮𝐦 𝟐 (𝛔𝟐, 𝛆𝟐, 𝛍𝟐)

Transmitted Wave

Incident Wave

Reflected Wave

𝐄𝐭

𝐚𝐤

𝐇𝐭

𝐇𝐫

𝐚𝐤

𝐄𝐫

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61

)85.10(a zsinjE2

a)ee(E

)84.10(a )eEeE(EEE

x10i

xzjzj

0i

xz

roz

iorsis1

11

11

S

* 매질 1: Dielectric – 매질 2: Perfect Conductor

2

11

11

12

12

0i

0r

2

1

j

0

1E

E

0

roto

roio

xz

rors

xz

iois

EE)b82.10(

EE)b81.10(

aeE)z(E(10.73)

aeE)z(E(10.71)

1

1

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

2

j

2

2

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62

)cos()cos()sin()sin(2

)cos()cos()cos()cos(2

)sin()sin()cos()cos()cos(

)sin()sin()cos()cos()cos(

)86.10(a)tsin()zsin(E2E

a)ztcos(Ea)ztcos(E

ae)ee(EE

)85.10(a zsinjE2

a)ee(E

)84.10(a )eEeE(EEE

x10i1

x10ix10i

xtjzjzj

0i1

x10i

xzjzj

0i

xz

roz

iorsis1

11

11

11

S

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63

)87.10(a)tcos()zcos(E2

H

a)]ztcos()zt[cos(E

)]a)(ztcos(E)a)(ztcos(E[1

H

)86.10(a)tsin()zsin(E2E

a)ztcos(Ea)ztcos(EE

y11

0i1

y111

0i

y10iy10i1

1

x10i1

x10ix10i1

)cos()cos()sin()sin(2

)cos()cos()cos()cos(2

)sin()sin()cos()cos()cos(

)sin()sin()cos()cos()cos(

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64

Fig 10.12 Standing wave 𝐄 = 𝟐𝐄𝐢𝟎 𝐬𝐢𝐧 (βz)sin(ω𝐭) 𝐚𝐱.

The curves 0,1,2,3,4,... are, respectively,

at time t=0, T/8, T/4, 3T/8, T/2,... λ=2πβ1.

t=2

1, 3

0, 4, 8

5, 7

6

−λ

2

−λ−

2

σ1 = 0 σ2 = ∞

2Eio

−2Eio

x

z0

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65

그림 Traveling Wave는 위상의 이동이 있다.Standing Wave는 제자리에서 진동한다.

Phase velocity를 정의 할 수 없다 (𝐯𝛗 = 𝛚/𝛃).

(a) Traveling Wave.

𝐇 = 𝐇𝐢𝟎 𝐜𝐨𝐬 (βz−ω𝐭) 𝐚𝐱.

(b) Standing Wave.

𝐇 = 𝟐𝐇𝐢𝟎 𝐜𝐨𝐬 (βz)cos(ω𝐭) 𝐚𝐱.

H

0 z

z

z

0

0

ωt=0

ωt=π/2

ωt=π

H

0z

z

z

0

0

ωt=0

ωt=π/2

ωt=π

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66

x1iox1io

xtjzj

iozj

ioxtjzj

io1

zjio

zjio

zjio

zjio

zjio

zjio

zjio

zjio1

a)tcos()zcos(E2a)ztcos(E )1(

aeeEeEaeeE)1(E

eEeEeE)1(

eEeEeE)1(

eEeEE

j

0

0

111

111

111

11

S

* Dielectric – dielectric Interface

CASE. A: η1<η2

12

12

io

ro

2

j

2

2

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

Propagating Wave Standing Wave

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67

Propagating WaveStanding Wave

)9.10(udt

dz

)8.10(2

)c7.10(2

f

1T

)b7.10(u

)a7.10(f2

)89.10(,...2 ,1 ,0n , 4

)1n2(

2

)1n2(z

2)1n2(z

)88.10(,...2 ,1 ,0n ,2

nnz

nz

a)]ztcos(E )1()tcos()zcos(E2[E

11

min

min1

1

1max

max1

x1io1io1

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68

Fig 10.13 Standing wave due to reflection at an interface

between two lossless media; λ=2πβ1.

−λ

2

−λ−

2

σ1 = 0 σ2 = 0

Eio(1 + Γ)

x

z0

Eio(1 − Γ)

E1 for η2 > η1

E1 for η2 < η1

Page 70: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

69

1)83.10(

2

E

E)a82.10(

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

12

2

io

to

12

12

io

ro

2

j

2

2

x1iox1io

xtjzj

iozj

ioxtjzj

io1

zjio

zjio

zjio

zjio

zjio

zjio

zjio

zjio1

a)tsin()zsin(E2a)ztcos(E )1(

aeeEeEaeeE)1(E

eEeEeE)1(

eEeEeE)1(

eEeEE

j

0

0

111

111

111

11

S

Standing WavePropagating Wave

* Dielectric – dielectric Interface

CASE. B: η1>η2

Page 71: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

70

)92.10(slog 20 dBin s

)91.10(1s

1s

)1s1(

)90.10(1

1

H

H

E

Es

E

E)a81.10(

10

min1

max1

min1

max1

12

12

io

ro

* Standing Wave Ratio: s

x1io

x1io1

21

x1io

x1io1

21

a)tcos()zcos(E2

a)ztcos(E )1(E

a)tsin()zsin(E2

a)ztcos(E )1(E

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71

m/mVa)zt10cos(10E

10HE

aaaaaaaaa

2

3

444

c

0

120/

3

1

c

0

y18

0i

00i10i

HEkyzxkHE

0r

r

0

02

1rr002

2

0001

1

1

iii

예제 10.8 자유공간 (z≤0) 에서 𝐇𝐢 = 𝟏𝟎 𝐜𝐨𝐬 𝟏𝟎𝟖𝐭 − 𝛃𝐳 𝐚𝐱 𝐦𝐀/𝐦 인 평면파가 (z≥0) 인

무손실 매질 (ε=2ε0, μ=8μ0) 에 수직으로 입사된다.

반사파 𝐇𝐫 𝐄𝐫, 투과파 𝐇𝐭 𝐄𝐭를 구하라.

j

2

2

ej

j)32.10(

112

)24.10(

112

)23.10(𝐚𝐤

𝐚𝐄

𝐚𝐇𝐲𝐱

𝐳

𝐳𝐲

𝐱

(2) 무손실 유전체(𝛔𝟐 = 𝟎,𝟐𝛆𝟎, 𝟖𝛍𝟎)

(1) Free Space

(𝛔𝟏 = 𝟎, 𝛆𝟎, 𝛍𝟎)

Wave

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72

m/mAa)z3

4t10cos(

3

20H

aaafor

m/mVa)z3

4t10cos(

3

40

a)zt10cos(EE

3

41

E

E

x8

t

yEE

y8

0

E28

0tt

0i

0t

it

t

m/mAa)z3

1t10cos(

3

10H

m/mVa)z3

1t10cos(

3

10E

E3

1E

3

1

2

2

E

E

m/mVa)zt10cos(10E

23

40

1203

10

x8

r

y8

0r

0i0r

00

00

12

12

0i

0r

y18

0i

0222

0111

𝐚𝐤

𝐚𝐄 𝐚𝐇

𝐲𝐱

𝐳

𝐳𝐲

𝐱

(2) 무손실 유전체(𝛔𝟐 = 𝟎,𝟐𝛆𝟎, 𝟖𝛍𝟎)

(1) Free Space

(𝛔𝟏 = 𝟎, 𝛆𝟎, 𝛍𝟎)

Wave

1)83.10(

2

E

E)a82.10(

E

E)a81.10(

12

2

io

to

12

12

io

ro

𝐚𝐤𝐚𝐄

𝐚𝐇𝐲𝐱

𝐳

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73

y1i

HEk

yxzEkH

0

10i10i

H10i1i

2i1ii

r

y2i

x1i

a)ztcos(3

1H

)aaa(

aaaaaa

3

1

120

40EHwhere

a)ztcos(HH

HHH

airatm1for10006.1

a)ztsin(30E

a)ztcos(40E

)a(

111

1

예제 10.9 공기 중에 평면파가 다음과 같이 주어졌다.

𝐄𝐢 = 𝟒𝟎𝐜𝐨𝐬 𝛚𝐭 − 𝛃𝐳 𝐚𝐱 + 𝟑𝟎𝐬𝐢𝐧 𝛚𝐭 − 𝛃𝐳 𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦

(a) 𝐇𝐢 를 구하라.

(b) wave가 z=0에서 z 축에 놓인 완전도체판을 만날 때 반사되는 wave의 𝐄𝐫 과 𝐇𝐫 을 구하라.

(c) z≤0에서 총 전자기장 𝐄,𝐇는 얼마인가?(d) z≤0와 z≥0에서 time-average Poynting vector를 계산하라.

12010144

36

10

104

ej

j)32.10(

22

9

7

j

𝐚𝐤

𝐚𝐄

𝐚𝐇

𝐲𝐱

𝐳

𝐳𝐲

𝐱

(2) 초전도체(𝛔𝟐 = ∞)

(1) Free Space

(𝛔𝟏 = 𝟎, 𝛆𝟎, 𝛍𝟎)

Wave

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74

m/mAa)ztcos(3

1

a)ztsin(4

1

HHH

a)ztsin(4

1H

aaaaaa

aaa

4

1

120

30EHwhere

a)ztsin(HH

y

x

2i1ii

x2i

xyzEkH

HEk

0

20i20i

H20i2i

2

222

2

y2i

x1i

a)ztsin(30E

a)ztcos(40E

𝐚𝐤𝐚𝑯

𝐚𝐄

𝐲𝐱

𝐳

예제 10.9 공기 중에 평면파가 다음과 같이 주어졌다.

𝐄𝐢 = 𝟒𝟎𝐜𝐨𝐬 𝛚𝐭 − 𝛃𝐳 𝐚𝐱 + 𝟑𝟎𝐬𝐢𝐧 𝛚𝐭 − 𝛃𝐳 𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦

(a) 𝐇𝐢 를 구하라.

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75

m/Aa)ztsin(4

1a)ztcos(

3

1H

m/volta)ztsin(30

a)ztcos(40E

EEE

0,1

1

)b(

xyr

y

xr

0i0i0r

122

2

0HH

0EE

HHH

EEE

)c(

t2

t2

ri1

ri1

예제 10.9 공기 중에 평면파가 다음과 같이 주어졌다.

𝐄𝐢 = 𝟒𝟎𝐜𝐨𝐬 𝛚𝐭 − 𝛃𝐳 𝐚𝐱 + 𝟑𝟎𝐬𝐢𝐧 𝛚𝐭 − 𝛃𝐳 𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦

(b) wave가 z=0에서 z 축에 놓인 완전도체판을 만날 때 반사되는 wave의 Er 과 Hr 을 구하라.

(c) z≤0에서 총 전자기장 E,H는 얼마인가?

12

12

io

ro

E

E)a81.10(

je

j

j)32.10(

j)20.10(

)j(j)18.10( 2

1)83.10(

2

E

E)a82.10(

12

2

io

to

tan)41.10(

x

yi

y

xi

a)ztsin(4

1

a)ztcos(3

1H

a)ztsin(30

a)ztcos(40E

zz2

20

ave acose2

E)z(p)69.10(

120)32.10( 1

𝐚𝐤

𝐚𝐄𝐚𝐇

𝐲𝐱

𝐳

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76

j

2

2

ej

j)32.10(

112

)24.10(

112

)23.10(

𝐳𝐲

𝐱

(2) 초전도체(𝛔𝟐 = ∞)

(1) Free Space

(𝛔𝟏 = 𝟎, 𝛆𝟎, 𝛍𝟎)

Wave

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77

2z

1

20t

k1

2s2

ave2

2

z22

z22

z20rz

20i

1averaveik

1

2s1

ave

m/watt0a2

Ea

2

EP

0z

m/watt0

a)3040(a)3040(240

1

aEaE2

1PPa

2

EP

0z

)d(

12

12

io

ro

E

E)a81.10(

je

j

j)32.10(

j)20.10(

)j(j)18.10( 2

1)83.10(

2

E

E)a82.10(

12

2

io

to

2tantan)41.10(

zz2

20

ave acose2

E)z(p)69.10(

예제 10.9 공기 중에 평면파가 다음과 같이 주어졌다.

𝐄𝐢 = 𝟒𝟎𝐜𝐨𝐬 𝛚𝐭 − 𝛃𝐳 𝐚𝐱 + 𝟑𝟎𝐬𝐢𝐧 𝛚𝐭 − 𝛃𝐳 𝐚𝐲 𝐯𝐨𝐥𝐭/𝐦

(d) z≤0와 z≥0에서 time-average Poynting vector를 계산하라.

m/Aa)ztsin(4

1

a)ztcos(3

1H

m/Va)ztsin(30

a)ztcos(40E

x

yr

y

xr

x

yi

y

xi

a)ztsin(4

1

a)ztcos(3

1H

a)ztsin(30

a)ztcos(40E

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78

10.9 경사 입사 시 평면파의 반사

매질무손실 for ~

kkkk

)94.10(kkkk

)k,k,k(k

)93.10(eERe

)tzcos(a)trkcos(E)t,r(E

2z

2y

2x

22z

2y

2x

2

zyx

)trk(j0

x0

22k

1c

kv

kv

0t

rk

t

trk

k

k

j

2

2

ej

j)32.10(

k~

112

)24.10(

112

)23.10(

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79

EHk

HEkk

)d95.10(0Ek

)c95.10(0Hk

)b95.10(EHk

)a95.10(HEk

00

00

)trk(j0

)trk(j0

EHk

HEk

eHH

eEE

t

BE

t

EJ

t

EB

0B

E

매질무손실

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80

Ejt

E

Ekj

eE eE eE

z

y

x

a a a

EEE

zyx

aaa

E

k)k,k,k(zkykxkz

ay

ax

a)rk(

zkykxkrk

eEE

)z,y,x(r

)k,k,k(k

)tzkykxk(jz0

)tzkykxk(jy0

)tzkykxk(jx0

zyx

zyx

zyx

zyxzyxzyx

zyx

)trk(j0

zyx

zyxzyxzyx

참고

Page 82: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

81

)trk(j0

)trk(j0

)tzkykxk(jz0

)tzkykxk(jy0

)tzkykxk(jx0

zyx

)trk(j0

)trk(j0

)trk(j0

)trk(j0

eEjeHkj

eH eH eH

z

y

x

a a a

eEjeH

eHH

eEE

t

EH

zyxzyxzyx

00

00

)trk(j0

)trk(j0

EHk

HEk

eHH

eEE

t

BE

t

EJ

t

EB

0B

E

매질무손실

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82

)96.10(Ea

Ek1

H

kEkHk

)k,k,k(k

)b95.10(EHk

)a95.10(HEk

k

zyx

k

k

0

ej

j)32.10(

k~

112

)24.10(

112

)23.10(

j

2

2

𝐚𝐤

𝐚𝐄

𝐚𝐇

Page 84: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

83

)100.10(sinksink

)99.10(sinksink

kkkk.3

kkkk.2

.1

)tykxkcos(EE

)tykxkcos(EE

)tykxkcos(EE

)98.10()0z(E)0z(E)0z(E

)c97.10()tzkykxkcos(EE

)b97.10()tzkykxkcos(EE

)a97.10()tzkykxkcos(EE

ttii

rrii

ytyryiy

xtxrxix

tri

ttytx0tt

rryrx0rr

iiyix0ii

tri

ttztytx0tt

rrzryrx0rr

iiziyix0ii

Fig 10.15 평면파의 경사 입사.

(b) 𝐤 의 법선 및 접선 성분의 설명.

입사파, 투과파 반사파는 하나의

평면에 있다.

kz + k⊥

z

n(2) 매질

(σ2 = 0, 2ε2, μ2)(1) 매질

(σ1 = 0, ε1, μ1)

θtθi

θr

kr

ki

kt

a θi, θr, θt 의 설명

kiz = β1cosθi

θr

θi

kikisinθi

krz = β1cosθz

kr

krsinθr

ktz = kzcosθt

ktsinθtkt

θt

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84

tzrziz

yxtytx

yxryrx

yxiyixn

ytyryiy

xtxrxix

kBkAk

)0,k,k()0,k,k(

)0,k,k()0,k,k(

)0,k,k()0,k,k(k

kkkk.3

kkkk.2

원점에서 3 wave는 만난다.

𝐤𝐧과 𝐤𝐢𝐳로 이루어진 하나의 평면상에 있다

θr

z

n(2) 매질

(σ2 = 0, 2ε2, μ2)(1) 매질

(σ1 = 0, ε1, μ1)

θtθi

kr

ki

kt

Page 86: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

85

)b101.10(k

)a101.10(kk

k

k

for

)100.10(sinksink

)99.10(sinksink

222t

111ri

ttii

rrii

매질무손실

222

111

t2i1

22

11

1

2

t

i

i

t

ir

cn

:cnwhere

)104.10(sinnsinn

:k/u

Snellwhere

)103.10(u

u

k

k

sin

sin

)101.10()100.10(

)102.10(

)a101.10()99.10(

굴절률

위상속도

법칙의

Page 87: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

86

k

k

0

ej

j)32.10(

k~

112

)24.10(

112

)23.10(

j

2

2

Page 88: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

87

A. 평행편파 (Parallel Polarization)

(𝐄가 입사 평면에 평행: η2>η1기준)

222

y)coszsinx(j

2

0tts

)coszsinx(jztxt0tts

111

y)coszsinx(j

1

0rrs

)coszsinx(jzrxr0rrs

ii

y)coszsinx(j

1

0iis

)coszsinx(jzixi0iis

where

)b107.10(aeE

H

)a107.10(e)asina(cosEE

where

)b106.10(aeE

H

)a106.10(e)asina(cosEE

)coszsinxr(

)b105.10(aeE

H

)a105.10(e)asina(cosEE

tt2

tt2

ii1

ii1

ii1

ii1

𝐚𝐤

𝐚𝐄 𝐚𝐇

Fig 10.16 oblique incidence

with 𝐄 parallel to the planeof incidence.

θiEi

x

z

Er

kr

Hr

kiHi

kt

Et

Htθt

θr

Medium 1μ1, ε1

Medium 2μ2, ε2

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88

12

2

io

to

12

12

io

ro

2

j

2

2

2

E

E)a82.10(

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

tan 1 cot

sin cos

cscsec

2

22

secd

tand

sind

cosd

cosd

sind

tantan1

tantan)tan(

sincos)2cos(

sinsincoscos)cos(

cossin2)2sin(

sincoscossin)sin(

Page 90: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

89

)b110.10(EE

)a110.10(coscos

cos2

E

E

)b109.10(EE

)a109.10(coscos

coscos

E

E

Fresnel

)b108.10(E1

)EE(1

HHH

)a108.10(cosEcos)EE(

EEE

0i//0t

i1t2

i2

0i

0t//

0i//0r

i1t2

i1t2

0i

0r//

0t2

0r0i1

0t0r0i

t0ti0r0i

ri

0t0r0i

TanTanTan

TanTanTan

방정식

12

2

io

to

12

12

io

ro

ti

2

E

E)a82.10(

E

E)a81.10(

0

θiEi

x

z

Er

kr

Hr

kiHi

kt

Et

Htθt

θr

Medium 1μ1, ε1

Medium 2μ2, ε2

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90

)112.10(cos

cos1

)111.10()110.10()109.10(

)111.10(sin)u/u(1

sin1cos

i

t////

i22

12

t2

t

22

11

1

2

t

i

i

t

u

u

k

k

sin

sin)103.10(

i1t2

i2

0i

0t//

i1t2

i1t2

0i

0r//

coscos

cos2

E

E)110.10(

coscos

coscos

E

E)109.10(

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91

)114.10(n

ntan

for /1

1

)113.10()/(1

/1sin

)sin1()sin1(

coscos

)Brewster(

1

2

1

2B

01221

221

2112B

2

B22

1t22

2

B1t2

//

//

//

//

.0E

coscos

coscos

E

E)a109.10(

//Bi0r

i1t2

i1t2

0i

0r//

있다가각도되는

/1u

sin)u/u(1

sin1cos)111.10(

i22

12

t2

t

굴절률:cn

굴절률이 작은 곳에서 큰 곳으로 진행시반사되지 않고 모두 투과.

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92

B. 수직편파

(𝐄가 입사 평면에 수직)

Fig 10.17 oblique incidence

with 𝐄 perpendicular to the plane of incidence.

)b117.10(e)asinacos(E

H

)a117.10(aeEE

)b116.10(e)asina(cosE

H

)a116.10(aeEE

)b115.10(e)asinacos(E

H

)a115.10(aeEE

)coszsinx(jztxt

1

0tts

y)coszsinx(j

0tts

)coszsinx(jzrxr

1

0rrs

y)coszsinx(j

0rrs

)coszsinx(jzixi

1

0iis

y)coszsinx(j

0iis

tt2

tt2

rr1

rr1

ii1

ii1

θi

Hi

x

z

Hr

kr

Er

kiEi

kt

Ht

Et

θtθr

Medium 1μ1, ε1

Medium 2μ2, ε2

𝐚𝐤

𝐚𝐄 𝐚𝐇

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93

)121.10(1

)b120.10(EE

)a120.10(coscos

cos2

E

E

)b119.10(EE

)a119.10(coscos

coscos

E

E

Fresnel

)b118.10( cosE1

cos)EE(1

)a118.10(EEE

0i0t

t1i2

i2

0i

0t

0i0r

t1i2

t1i2

0i

0r

t0t2

i0r0i1

ri

0t0r0i

방정식

연속성

연속성

θi

Hi

x

z

Hr

kr

Er

kiEi

kt

Ht

Et

θtθr

Medium 1μ1, ε1

Medium 2μ2, ε2

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94

)123.10(tan

forsin

)122.10()/(

/1sin

sin Snell

)sin1()sin1(

coscos

0

)Brewster(

1

2B

2121

2B

221

1221B

2

t

t22

1B22

2

t1B2

제거의해법칙에의

θi

Hi

x

z

Hr

kr

Er

kiEi

kt

Ht

Et

θtθr

Medium 1μ1, ε1

Medium 2μ2, ε2

22

11

1

2

t

i

i

t

i22

12

t2

t

t1i2

t1i2

0i

0r

u

u

k

k

sin

sin)103.10(

Snell

/1u

sin)u/u(1

sin1cos)111.10(

coscos

coscos

E

E)a119.1(

법칙의

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95

예제 10.10 자유공간에서 진행하는 전자파의 전기장 성분이 다음과 같다.

𝐄𝐢 = 𝟏𝟎𝟎𝐞−𝐣(𝟎.𝟖𝟔𝟔𝐲+𝟎.𝟓𝐳)𝐚𝐱 𝐯𝐨𝐥𝐭/𝐦(a) ω와 λ.

(b) 자기장 성분.

(c) wave의 시평균 전력.

m283.6k

2

sec/rad103kc

2

c

f2

ck

1kkkk

5.0k,866.0k,0k

aeEE

)a(

8

00

2z

2y

2x

zyx

x)zkykxk(j

0szyx

2zy

zy

2

k

20

ssave

zz2

20

ave

)z5.0y866.0(jzy

rkjx87

zy

ssks

m/W)a631.6a49.11(

)a5.0a866.0()120(2

100

a2

E)HERe(

2

1P

acose2

E)z(p)69.10()c(

m/Ae)a23.0a133.0(

ea100)103)(104(

a5.0a866.0

Ek1

Ea1

H)96.10(

)b(

𝐚𝐤

𝐚𝐄 𝐚𝐇

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96

12

2

io

to

12

12

io

ro

2

j

2

2

2

E

E)a82.10(

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

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97

예제 10.11 자유공간에서 진행하는 전기장이 𝐄𝐢 = 𝟖𝐞𝐣(𝛚𝐭−𝟒𝐱−𝟑𝐳)𝐚𝐲 volt/m 인

균일 평면파가 𝛍𝐫=1, 𝛆𝐫=2.5, σ=0 인 유전체 (z ≥ 0) 에 입사 된다. 다음을 구하라.

(a) ω, wave의 편파 특성(b) 입사각(c) 반사 전기장(d) 투과 자기장

Fig 10.18 Propagation vectors of Example 10.11.

θi

krkrx

krz

kikix

kiz

θr

θtθi

ktx

kt

ktzθr

z

x

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98

sec/rad1015

c/5ka3a4k

)a(

8

00izxi

경계면 (z=0) 에 수직인 단위 vector 𝐚𝐳 와 𝐤 를 포함하는 평면은 y=상수인 xz-평면이

입사 평면이다. 𝐄𝐢 가 이 평면에 수직이기때문에수직편파이다.

13.51

5

3a

5

aaaacos

13.513

4

k

ktan

)b(

izzx

nki

iiz

ixi

예제 10.11 자유공간에서 진행하는 전기장이 𝐄𝐢 = 𝟖𝐞𝐣(𝛚𝐭−𝟒𝐱−𝟑𝐳)𝐚𝐲 volt/m 인

균일 평면파가 𝛍𝐫=1, 𝛆𝐫=2.5, σ=0 인 유전체 (z ≥ 0) 에 입사 된다. 다음을 구하라.

(a) ω, wave의 편파 특성 (b) 입사각 (c) 반사 전기장 (d) 투과 자기장

θi

krkrx

krz

kikix

kiz

θr

θtθi

ktx

kt

ktzθr

z

x

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99

m/Va)z3x4t1015cos(112.3E

112.3EE

389.0

4.238/

377

coscos

coscos

E

E

39.30

5.2

)13.53sin(sinsin

a3a4k

coskk

sinkk

akakk

a)rktcos(EE

)c(

y8

r

0i0r

2r02r02

01

t1i2

t1i2

0i

0r

t

o

i22

11t

zxr

rrrz

rrrx

zrzxrxr

yr0rr

반사전기장

ssks

22

11

1

2

t

i

i

t

12

2

io

to

12

12

io

ro

2

j

2

2

Ek1

Ea1

H)96.10(

u

u

k

k

sin

sin)103.10(

2

E

E)a82.10(

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

𝐄𝐢 = 𝟖𝐞𝐣(𝛚𝐭−𝟒𝐱−𝟑𝐳)𝐚𝐲

𝛉𝐢 = 𝟓𝟏. 𝟐𝟑𝐨

Page 101: Chapter 10 Electromagnetic Wave Propagation - … · 9 Table 10.1 Electromagnetic spectrum EM Phenomena Examples od Uses Approximate Frequency Range Cosmic rays Gamma rays X-rays

100m/mAa)z819.6x4t1015cos()a37.10a69.17(H

a)rktcos(888.4)4.238(906.7

a819.6a4

EaEk

1H

m/Va)z819.6x4t1015cos(888.4E

888.4EE

1

611.0coscos

cos2

E

E

a819.6a4k

819.6coskk

4sinkk

c/k

a)rktcos(EE

)d(

y8

zxt

yrzx

2

tktt

2t

y8

t

0i0t

t1i2

i2

0i

0t

zxt

tttz

tttx

2r2r222t

yr0tt

t

투과자기장 𝐄𝐢 = 𝟖𝐞𝐣(𝛚𝐭−𝟒𝐱−𝟑𝐳)𝐚𝐲

𝛉𝐢 = 𝟓𝟏. 𝟐𝟑𝐨

𝛉𝐭 = 𝟑𝟎.𝟑𝟗𝐨

ssks

22

11

1

2

t

i

i

t

12

2

io

to

12

12

io

ro

2

j

2

2

Ek1

Ea1

H)96.10(

u

u

k

k

sin

sin)103.10(

2

E

E)a82.10(

E

E)a81.10(

j)20.10(

)j(j)18.10(

ej

j)32.10(

112

)24.10(

112

)23.10(

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101

10.10 응용 note - microwave

Fig 10.19 Satellite communications configurations. (From W. Stallings, Data and Computer Communications, 5th ed. Upper

Saddle River, NJ: Prentice Hall, 1997, p. 90.)

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102

Fig 10.20 Microwave oven. (From N. Schlager, ed., How Products are made. Detroit: Gale Research, 1994, p. 289.)

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103

S-parameter

)130.10(ZZ

ZZwhere

)129.10(S1

SSS

a

b

port2matchingwhere

)128.10(0SS

)127.10(SS

)126.10(reciprocalSS

)125.10(a

a

SS

SS

b

b

:b

:awhere

)124.10(aSaSb

aSaSb

0L

0LL

L22

L211211

1

1i

2211

2211

2112

2

1

2221

1211

2

1

2221212

2121111

입력반사계수

회로망된

대칭

반사파

입사파

Fig 10.21 A two-port network.

LZ

gV

gZ

1a 2a

1b 2b

2221

1211

SS

SS

)132.10(ZZ

ZZwhere

)131.10(S1

SSS

a

b

0g

0gg

g11

g211222

0V2

20

g

출력반사계수

CgdT

rdsCgsT gmV1

V1

+

-

I1

V2

+

-

I2

Cds

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104

예제 10.12 2.5 GHz에서 동작하는 microwave transistor에서다음과 같은 S-parameter를 얻었다..

S11=0.85/-30o, S12=0.07/56o, S21=1.68/120o, S22=0.85/-40o, ZL=Z0=75 Ω

일 때 입력 반사 계수 Γi를 구하라.

o11i

0L

0LL

L22

L211211

1

1i

30/85.0S)129.10(

0ZZ

ZZ)130.10(

)129.10(S1

SSS

a

b