Oblique incidence: Interface between dielectric mediaamanogawa.com/archive/docs/EM13.pdfOblique...
Transcript of Oblique incidence: Interface between dielectric mediaamanogawa.com/archive/docs/EM13.pdfOblique...
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 165
Oblique incidence: Interface between dielectric media Consider a planar interface between two dielectric media. A plane wave is incident at an angle from medium 1. The interface plane defines the boundary between the media. The plane of incidence contains the propagation vector and is both perpendicular to the interface plane and to the phase planes of the wave.
θi θrβ
Plane of incidence
Interface plane
Medium 1ε1 = εr1 εo µ1 = µr1 µo
Medium 2ε2 = εr2 εo µ2 = µr2 µo
Phase plane
θt
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 166
There are two elementary orientations (polarizations) for the electromagnetic fields: Perpendicular Polarization
The electric field is perpendicular to the plane of incidence and the magnetic field is parallel to the plane of incidence.
The fields are configured as in the Transverse Electric (TE) modes.
Parallel Polarization
The magnetic field is perpendicular to the plane of incidence and the electric field is parallel to the plane of incidence.
The fields are configured as in the Transverse Magnetic (TM) modes.
Any plane wave with general field orientation can be obtained by superposition of two waves with perpendicular and parallel polarization.
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 167
Perpendicular (TE) polarization
Medium 1 ε1 = εr1 εo µ1 = µr1 µo
z
x
y
iE
iβxβ
zβ
iθ
×
×
rθ×
rE
iH
rH rβ
× tHtE
tθ
tβ
Medium 2 ε2 = εr2 εo µ2 = µr2 µo
Incident wave
Reflectedwave
Transmitted wave
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 168
The electric field phasors for the perpendicular polarization, with reference to the system of coordinates in the figure, are given by
The propagation vector components in medium 1 are expressed as
i
r
t
ˆE
ˆE
ˆE
ix iz
rx rz
tx t z
j x j zyi y
j x j zyr y
j x j zyt y
E e i
E e i
E e i
β β
β β
β β
− ⋅ − ⋅
− ⋅ − ⋅
− ⋅ − ⋅
=
=
=
2 21 1 1
1 1
2 21
1 1
cos sin
cos sin
i ix iz
ix i iz i
r rx rz
rx r rz r
β β β β ω µ ε
β β θ β β θ
β β β β
β β θ β β θ
= + = =
= =
= + =
= − =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 169
The propagation vector components in medium 2 are expressed as
The magnetic field components can be obtained as
2 22 2 2
2 2cos sint tx tz
tx t tz t
β β β β ω µ ε
β β θ β β θ
= + = =
= =
( )
( )
( )
ii
1 1
rr
1 1
tt
2 2
E ˆ ˆH sin cos
E ˆ ˆH sin cos
E ˆ ˆH sin cos
ix iz
rx rz
tx tz
j x j zyiii x i z
j x j zyrrr x r z
j x j zyttt x t z
Ei i e
Ei i e
Ei i e
β β
β β
β β
β θ θωµ η
β θ θωµ η
β θ θωµ η
− −
− −
− −
×= = − +
×= = − +
×= = − +
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 170
Assuming that the amplitude of the incident electric field is given, to completely specify the problem we need to find the amplitude of reflected and transmitted electric field. The boundary condition at the interface (x = 0) states that the tangential electric field must be continuous. Because of the perpendicular polarization, the tangential field is also the total field The relation above must be valid for any choice of “z” and we must have (phase conservation law)
The first equality indicates that the reflected angle is the same as the incident angle.
)0 i z rz tzj z j z j zyi yr ytE e E e ex Eβ β β− − −
+ ==
iz rz tzβ β β= =
1 1sin siniz rz i r i rβ β β θ β θ θ θ= ⇒ = ⇒ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 171
The second equality provides the transmitted angle
Since we have also the boundary condition for the electric field becomes
1 11
2 2sin sint i
µ εθ θ
µ ε−
⇒ =
Snell's Law
i z rz tzj z j z j ze e eβ β β− − −= =
yi yr ytE E E+ =
1 2sin siniz tz i tβ β β θ β θ= ⇒ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 172
The tangential magnetic field must also be continuous at the interface. This applies in our case to the z−components
Solution of the system of boundary equations gives
1 1 2
1
2
cos cos cos
coscos
y i y r y ti i t
ty
z i z r z t
i y r y ti
E E E
E E
H H H
E
θ θ θη η η
η θη θ
− =
⇒ −
+ =
=
2 1
2 1
cos cos( )cos cos
yr i t
yi i t
EE
Eη θ η θη θ η θ⊥
−Γ = =
+Reflection coefficient
2
2 1
2 cos( )cos cos
yt i
yi i t
EE
Eη θτ
η θ η θ⊥ = =+
Transmission coefficient
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 173
For the magnetic field, we can define the reflection coefficient as
In terms of electric field, the magnetic field components are
The reflection coefficient for the magnetic field is then
1 2
2 1
cos cos( ) ( )cos cos
y r t i
y i i t
EH E
Eη θ η θη θ η θ⊥ ⊥
− −Γ = = −Γ =
+
1
1
cos cos
cos cos
yrzr i r i
yizi i i i
EH H
EH H
θ θη
θ θη
−= = −
= =
( ) zr rzi i
H HHH H⊥Γ = = −
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 174
The transmission coefficient is defined as
The magnetic field components are
The transmission coefficient for the magnetic field is then
( ) t
i
HHH
τ⊥ =
112 2 1
2 cos( ) ( )cos cos
t i
i i t
HH EH
η θητ τη η θ η θ⊥ ⊥= = =
+
2
1
y tt
y ii
EH
EH
η
η
=
=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 175
Parallel (TM) polarization
Medium 1 ε1 = εr1 εo µ1 = µr1 µo
z
x
y
iEiβ
xβ
zβ
iθ
×
×
rθ×
rE
iH
rH
rβ
× tH
tEtθ
tβ
Medium 2 ε2 = εr2 εo µ2 = µr2 µo
Incident wave
Reflectedwave
Transmitted wave
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 176
The magnetic field phasors for the parallel polarization are given by
and the electric field components can be obtained as
i
r
t
ˆH
ˆH
ˆH
ix iz
rx rz
tx t z
j x j zyi y
j x j zyr y
j x j zyt y
H e i
H e i
H e i
β β
β β
β β
− ⋅ − ⋅
− ⋅ − ⋅
− ⋅ − ⋅
=
=
=
( )
( )
( )
ii 1
1
rr 1
1
tt 2
2
H ˆ ˆE sin cos
H ˆ ˆE sin cos
H ˆ ˆE sin cos
ix iz
rx rz
tx tz
j x j ziyi i x i z
j x j zryr r x r z
j x j ztyt t x t z
H i i e
H i i e
H i i e
β β
β β
β β
β η θ θωεβ η θ θωε
β η θ θωε
− −
− −
− −
×= − = −
×= − = +
×= − = −
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 177
Also for parallel polarization one can verify that the same relationships between angles apply, as found earlier for the perpendicular polarization, including Snell’s law
We have again two boundary conditions at the interface. One condition is for continuity of the tangential magnetic field
yi yr ytH H H+ =
1 11
2 2sin sin
i r
t i
θ θ
µ εθ θ
µ ε−
=
=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 178
A second condition is for continuity of the tangential electric field
From the equations provided by the boundary conditions we obtain the reflection and transmission coefficients for the magnetic field of a wave with parallel polarization as
1 1 2
2
1
cos cos cos
coscos
zi
i yi i yr t yt
tyi yr y
i
zr zt
t
H H H
H H H
E E E
η θ η θ η θ
η θη θ
− + = −
⇒ − =
+ =
1 2
1 2
1
1 2
cos cos( )cos cos
2 cos( )cos cos
yr i t
yi i t
yt i
yi i t
HH
H
HH
H
η θ η θη θ η θ
η θτη θ η θ
−Γ = =
+
= =+
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 179
The reflection coefficient for the electric field is defined as
The tangential components of the electric field can be expressed in terms of magnetic field as
The reflection coefficient for the electric field is
( ) zr rzi i
E EEE E
Γ = = −
2 1
1 2
cos cos( ) ( )cos cos
zr yr t i
zi yi i t
E HE H
E Hη θ η θη θ η θ
−Γ = = − = −Γ =
+
1
1
cos cos
cos coszr r i i yr
zi i i i yi
E E H
E E H
θ η θ
θ η θ
= =
= − = −
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 180
The transmission coefficient for the electric field is defined as
The electric field components are given by
The transmission coefficient for the electric field becomes
2 21 1
1 221 1 2 1 2
( ) ( )
2 cos 2 coscos cos cos cos
ytt
i yi
i i
i t i t
HEE HE H
η ητ τη η
η θ η θηη η θ η θ η θ η θ
= = =
= =+ +
( ) t
i
EE
Eτ =
2
1
t yt
i yi
E H
E H
η
η
=
=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 181
Considerable simplifications are possible for the common case of nonmagnetic dielectric media with
First of all, Snell’s law becomes
or, equivalently
Snell’s law provides then a useful recipe to express the reflection and transmission coefficients only with angles, thus eliminating the explicit dependence on medium impedance.
1 2 oµ µ µ= =
1 11 1 12 2 2
sin sin sin sint i iµ ε εθ θ θµ ε ε
− − = =
)2 21 1
sin (sin
i
t
n nn
θ εθ ε
= = = index of refraction
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 182
After some trigonometric manipulations, we obtain the following table of simplified coefficients for electric and magnetic field
( )( )( )( )
( )
( ) ( )
1
2
1
2
2sin cos( ) ( )sin
2sin cos( ) ( )
sin( ) ( )
sint
sin cos
an( ) ( )
tan
i t
i t
i t
t i
i t
i
t
t
i
i t i t
E H
E H
E
E H
H
ε θ θτ τθ θε
ε
θ θθ θ
θ θτ τ
θ θθ θ
θ θ θ θε
⊥ ⊥
⊥ ⊥
−Γ = −Γ = −
+
−Γ
= =+
= =+ −
= −Γ = −+
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 183
Power flow The time-average power flow normal to the interface must be continuous. We can express this as
We define the reflection and transmission coefficients for the time-average power as
2
2
21
2 2
coscos
r
i
t t
ii
ERE
ETE
θηη θ
= =
= =
reflected power
incident power
transmitted power
incident power
2 22
1 1 2
1 1 1cos cos cos2 2 2i tr
i i tE EEθ θ θη η η
− =
− =
incident p reflected power ower transmitted p ower
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 184
The following conversion formulas relate power and electric field coefficients
Note that reflection and transmission coefficients for the time-average power are always real positive quantities. The following power conservation condition is always verified
Since the power flow normal to the interface is considered, the results obtained above apply equally to perpendicular and parallel polarization.
2
2 12
( )
cos( )cos
t
i
R E
T E θητη θ
= Γ
=
1R T+ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 185
Non−magnetic perfect dielectric media
From Snell’s law
2 1Case ε ε>
Medium 1 ε1 = εr1 εo µ1 = µo
z
x
y
iβiθ
×
iθrβ
tθtβ
Medium 2 ε2 = εr2 εo µ2 = µo
2 11 2sin sin ii ttε θ ε θ ε ε θ θ> ⇒ <=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 186
Since θ t < θ i there is always a transmitted (refracted) beam.
The transmission coefficients are always positive
⇒ transmitted and incident wave are in phase at the boundary.
( )
( ) ( )
1
2
1
2
2sin cos( ) ( ) 0sin
2sin cos( ) ( ) 0sin cos
t i
i t
t i
i t i t
E H
E H
ε θ θτ τθ θε
ε θ θτ τθ θ θ θε
⊥ ⊥= = >+
= = >+ −
× ×
ytE
yiE ziH
ztH( ) yt
yi
EE
Eτ⊥ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 187
Perpendicular polarization
The reflection coefficient for the electric field is always negative
The reflection coefficient for the magnetic field is always positive
( )( )
( )( )
sin sin( ) ( )
sin sini t i t
i t i tE H
θ θ θ θθ θ θ θ⊥ ⊥− −
Γ = − Γ =+ +
and have always phase difference of 180yi yrE E °
and are always in phasezi zrH H
( ) yr
yi
EE
E⊥Γ = × yrEyiE ziH zrH( ) zr
zi
HH
H⊥Γ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 188
Parallel polarization ( )( )
( )( )
tan tan( ) ( )
tan tani t i t
i t i tE H
θ θ θ θθ θ θ θ− −
Γ = − Γ =+ +
( )
( )
When and have phase difference of 180 and are in phase
When an
90d are in phase
and have phase differenc
tan
e o
9
0
f 180
0 nta 0
zi zr
yi yr
zi z
i t i
r
yi y
t
t i
r
i tE EH H
E EH H
θ
θ
θ θ θ
θ θ θ
+ > °
⇒
°
⇒
+ < ° +
+ <
°
>
×yrHyiHziE zrE×
×yrHyiHziE zrE
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 189
( )90 taWhen ni t i tθ θ θ θ+ = ° +⇒ →∞ the reflection coefficients vanish (TOTAL TRANSMISSION)
For
90 and cos s
(Brewster angle)in
it
t
Bi
B
θ θθ θθ θ
⇒
⇒ =
= ° =+
From Snell’s law
( )( )
( )( )
tan tan( ) 0 ; ( ) 0
tan tani t i t
i t i tE H
θ θ θ θθ θ θ θ− −
Γ = − → Γ = →+ +
121
21
sin sin tansin co
ns
taB BB
t BB
θ θ εθ θθ ε
εεθ
−= = = ⇒ =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 190
From Snell’s law
2 1Case ε ε<
Medium 1 ε1 = εr1 εo µ1 = µo
z
x
y
iβiθ
×
iθrβ
tθtβMedium 2 ε2 = εr2 εo
µ2 = µo
2 11 2sin sin ii ttε θ ε θ ε ε θ θ< ⇒ >=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 191
For angles of incidence such that
we have for perpendicular polarization
( )( )
( )( )
( )( )
( )( )
sin sin( ) 0
sin sin
sin sin( )
and are always in phase
and have always phase differenc
0sin sin
e of 180
i t t i
i t i t
i t t i
i t i
yi yr
zi zr
t
E
H
E
H
E
H
θ θ θ θθ θ θ θ
θ θ θ θθ θ θ θ
⊥
⊥
− −Γ = − = >
+ +
− −Γ = = − <
+ +
°
sin 1tθ <
×yrEyiE ziH zrH
×
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 192
For parallel polarization ( )( )
( )( )
( )( )
( )( )
tan tan( )
tan tan
tan tan( )
tan tan
i t t i
i t i t
i t t i
i t i t
E
H
θ θ θ θ
θ θ θ θ
θ θ θ θ
θ θ θ θ
− −Γ = − =
+ +
− −Γ = = −
+ +
( )
( )
When and are in phase and have phase difference of 180
When an
90d have phase difference of 180
and a
tan
re
9
0
in ph
0 0
e
an
as
t
zi zr
yi yr
zi z
i
i
r
yi yr
t
t i t
i t
E EH H
E EH H
θ θ θ
θ
θ
θ θ θ+ <
+ > ° +
⇒°
⇒
+
°
°
>
<
×yrHyiHziE zrE×
×yrHyiHziE zrE
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 193
( )90 taWhen ni t i tθ θ θ θ+ = ° +⇒ →∞ Also in this case the reflection coefficients vanish and we have TOTAL TRANSMISSION
Total transmission occurs again, for parallel polarization only, at the Brewster angle
( )( )
( )( )
tan tan( ) 0 ; ( ) 0
tan tant i t i
i t i tE H
θ θ θ θθ θ θ θ− −
Γ = → Γ = − →+ +
1 21
tani Bεθ θε
−= =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 194
When
we have a limit condition for TOTAL REFLECTION, valid for both polarizations. This particular angle of incidence is called
2 21 1
sin sin sin 01 9i t t tε εθ θ θε ε
θ⇒ = ⇒ == = °
1 21
sini cεθ θε
−= = critical angle
90tθ = °
cθ
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 195
For angles of incidence beyond the critical angle The negative sign is selected, in order to obtain the proper wave vector in medium 2, as shown later.
imaginary
12
2 21 22 1
sin sin 1
cos 1 sin sin
cos
, " "
i t i
t
t
c
t ij
εθ θε
ε εθ θ θε ε
θ
θ
θ
=
±
>
⇓
⇒ = >
⇒
= −
−
− − = −
choose
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 196
The reflection and transmission coefficients become complex 2
2 1
12
22 1
2 2 1
1 2 12
222 1
122
2
22 2 1
1
1
1
cos sin( ) ( )
cos sin
cos sin( ) ( )
cos sin
2cos( ) ( )cos sin
2 / cos( ) ( )cos sin
i
i
i i
i i
i i
i i
i
i
i i
jE H
j
jE
E Hj
E
H
Hj
j
θ θ ε ε
θ θ ε εε θ θ ε εεε θ θ ε εε
ε θτ τε θ θ ε ε
ε ε ε θτ τ εε θ θ ε ε
ε
⊥
⊥ ⊥
⊥+ −
Γ = −Γ =− −
− − −Γ = −Γ =
= =
= =
−
− −
−
−
−
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 197
If we consider the coefficients for time-average power flow, we have, for both polarizations This means that incident and reflected waves carry the same time-average power, and no power is transmitted to medium 2. But this does not mean that the field disappears in medium 2. The instantaneous power that enters medium 2 is eventually reflected back to medium 1. The electric field phasor of the transmitted wave has the form
2 2cos sintE t x t z t tj x j z j x j z
t tE e e E e eβ β β θ β θ− ⋅ − ⋅ − ⋅ − ⋅= =
( ) ( )*
011R E E
T R= Γ ⋅Γ =
= − =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 198
The wave vector components are
The field in medium 2 corresponds to a surface wave, moving along the z−direction and exponentially decaying (evanescent) along the x−direction
21 22 2
2 1
2 22 21 1
1 1
12 2 1
2
cos sin
sin sin
sin sin sin
t o i
o i i t
t o i i i z
j
j j j
ε εβ θ ω µ ε θε ε
ε εω µ ε θ β θ αε ε
εβ θ ω µ ε θ β θ βε
= − −
= − − = − − = −
= = =
( )tE i i zt tzj z j zj j x
t txE e e E eeβ βα α− ⋅ − ⋅− − − ⋅⋅= =
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 199
The surface wave moves parallel to the surface, with a phase velocity equal to the apparent phase velocity along z of the incident wave in medium 1
For the surface wave, planes of constant amplitude are parallel and planes of constant phase are normal to the interface. These planes do not coincide, therefore the surface wave is a nontransverse wave.
12 1sin
pp pz p
i
vv v vθ
= = >
i cθ θ>
x
Et
Constant amplitude planes
Constant phase planes
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 200
If you consider a beam incident on the interface, it is found that the power is totally reflected but after penetrating for some distance into medium 2. The reflected beam emerges displaced by a distance D (called Goos-Hänchen shift, discovered in 1947) From experiments, the displacement is found to be
2 22 2
11
2 20.52 0.52sin t
i
D π πε εαεβ θ
ε
≈ =−
i cθ θ>D
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 201
Examples:
?Bθ =
Medium 1
o
o
air µ µ
ε ε
=
=
{80 microwaves
Medium
1.8 optic
2
al
o
o
o
water µ µ
εε
ε
=
=
1
1
tan 80 83.6 microwaves
tan 1.8 53.3 opticalB
B
θ
θ
−
−
= ≅ °
= ≅ °
1 21
tanBεθε
−=
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 202
At the Brewster angle
Verification with Snell’s law
906.38 microwaves36.7 optical
i t B t
t
θ θ θ θ
θ
+ = + = °
°⇒ ≅ °
1 2
1
2
sin sin
6.38 microwavessinsin36.7 optical
B t
Bt
ε θ ε θ
θθε
−
=
°= ≅ °
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 203
?Bθ =
Medium 2
o
o
air µ µ
ε ε
=
=
{80 microwaves
Medium
1.8 optic
1
al
o
o
o
water µ µ
εε
ε
=
=
1 21
tanBεθε
−=
1
1
1tan 6.38 microwaves801tan 36.7 optical
1.8
B
B
θ
θ
−
−
= ≅ °
= ≅ °
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 204
At the Brewster angle
Verification with Snell’s law
9083.6 microwaves53.3 optical
i t B t
t
θ θ θ θ
θ
+ = + = °
°⇒ ≅ °
1 2
1 2
sin sin
83.6 microwavessinsin53.3 optical
B t
Bt
o
ε θ ε θ
θ εθ
ε−
=
°= ≅ °
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 205
The total reflection angle does not exist since
?cθ =
Medium 1
o
o
air µ µ
ε ε
=
=
{80 microwaves
Medium
1.8 optic
2
al
o
o
o
water µ µ
εε
ε
=
=
1 21
sincεθε
−=
2 1ε ε>
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 206
?cθ =
Medium 2
o
o
air µ µ
ε ε
=
=
{80 microwaves
Medium
1.8 optic
1
al
o
o
o
water µ µ
εε
ε
=
=
1 21
sincεθε
−=
1
1
1sin 6.4193 microwaves801sin 48.19 optical
1.8
c
c
θ
θ
−
−
= ≅ °
= ≅ °
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 207
Consider a perpendicularly polarized wave. Find the Brewster angle and the critical angle:
60iθ = °
Medium 2
o
o
air µ µ
ε ε
=
=
Medium 1
4
o
o
µ µ
ε ε
=
=
1 1
1 1
1 1tan tan 26.5654 2
1 1sin sin 304 2
B
c
θ
θ
− −
− −
= = ≈ °
= = = °
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 208
Find the components of the incident propagation vector and of the x-component of the transmitted propagation vector in terms of
o o oβ ω µ ε=
choose " "
1
1
2 2
2 2
2cos 4 cos602
3sin 4 sin 60 2 32
3
3 2
oix i o o o
iz i o o o o
tx t tz t o tz iz o
tx o o o tj j
ββ β θ ω µ ε β
β β θ ω µ ε β β
β β β β β β β β
β β β β α
−
= = ° = =
= = ° = =
= − = = =
= ± − = − = −
Electromagnetic Fields
© Amanogawa, 2006 – Digital Maestro Series 209
In the second medium, find the distance at which the field strength is 1/e of that at the interface
What is the value of the magnitude of the reflection coefficient at the interface?
The reflection coefficient is a complex quantity when the incident angle exceeds the critical angle. Because of total reflection we know that it must be
since the time-average power reflection coefficient is
1 12t o
dα β
= =
( ) 1E⊥Γ =
2( ) 1R E⊥= Γ =