Field and Wave Electromagnetic
Chapter7 Chapter7
The time varying fields and Maxwell’s equation
The time varying fields and Maxwell’s equation
Introduction (1) Introduction (1)
Time static fields
0, ,
E D ρ D εE
∇× = ∇i = =
1) Electrostatic
2) Magnetostatic
0, , 1
B H J H B
E D B H
∇i = ∇× = = μ not
2) Magnetostatic
) and are not related to and for time st
e E D B H atic cases
not
e) and are not related to and for time static cases
Example)
( )
E J E
E σ
⇒ =
⇒
A static field in a conducting medium steady current.
give rises to a static magnetic field:Ampere's law. But field can be completely determined from the static electric charge or potential distributions
⇒magnetic field is a consequence
Introduction (2) Introduction (2)
Time varying fields Time varying fields
and are properly related to and
1) modify equation fundamental postulate leading to Faraday's law
E D B H
∇ ×E →
&
2) then modify the ∇ ×H equation to be consiste
) 0
nt with the equation of continuity cf J for static. but J for time varying
t
ρ
∇ = ∇ = −∂
i i ∂
3) ∇iD =
ρ
and ∇iB = 0 never changes.Faraday’s Law Faraday s Law
Michael Faraday⇒1831, experimental law ⇒ postulate Michael Faraday 1831, experimental law postulate
Definition : the quantitative relationship between the induced emf and the rate of change of flux linkage
⇒ ⇒
Fundamental postulate for Electromagnetic Induction
Non-conservative field cannot be expressed as the gradient of a scalar potential
E B
t
∇× = −∂ ⇒
∂
as the gradient of a scalar potential
C S
E dl B dS
t
= − ∂
∫
i∫
∂ i
A Stationary Circuit in a Time Varying Magnetic Field (1) A Stationary Circuit in a Time Varying Magnetic Field (1)
d ∂ d ∂
∫ ∫ ( , since stationary 0)
C S
d d
E dl B ds ds
dt t dt t
∂ ∂
= − → =
∂ ∂
∫ i ∫ i ∵
11 2
Right hand rule (counter clock wise)
2
, 1 d , d 0
emf v E dl
dt dt
Φ Φ
=
∫
i = − >Assume
dt dt
A Stationary Circuit in a Time Varying Magnetic Field (2) A Stationary Circuit in a Time Varying Magnetic Field (2)
: emf induced in circuit with contour C Define v ∫ E dl : emf induced in circuit with contour C Define v = ∫
CE dl i
1
2
~
2 1
l t ti f d i i t i th di ti f i ht h d l
2 1
( 0)
v
E dl = E dl E = = E dl = V V = V
∫ i ∫ i ∵ ∫ i
: electromagnetive force driving current in the direction of right hand rule Meaning of contour integral
inside contour
Field between the terminal in the gap
1 2 12
1
( 0)
2right hand
E dl = E dl E = = − E dl = − = V V V
⇒
∫ i ∫ i ∵ ∫ i
inside contour
ca n be replaced with voltage source. But polarity of v V =
12depends on the change of the flux linkage
the change of the flux linkage
A Stationary Circuit in a Time Varying Magnetic Field (3) A Stationary Circuit in a Time Varying Magnetic Field (3)
∂B
0 . 12 0
[ ]
B v i e V
t
B ds S Wb
∂ > <
∂ Φ =
∫
ie.g) then (current is in the direction of left hand rule)
Define : magnetic flux crossing surface [ ]
SB ds S Wb
v d
dt Φ =
= − Φ ⇒
∫
iDefine : magnetic flux crossing surface
then This is valid even in the absense of a physical closed circuit
note The emf induced in a stationary loop caused by a time-varying magnetic field is a transformer emf
Ex 7 1) A Circular Loop of N Turns of Conducting Wire Ex 7-1) A Circular Loop of N Turns of Conducting Wire
(πr) i
A i l l f N t 0
2
cos( ) sin 2
i ) ( 2 ) ) 2
B zB r wt
b
B d B r t d f π d
π
π φ
=
Φ
∫ ∫
b∫
A circular loop of N turns,
Find the emf induced in the loop
sol) each turn ( 0
0 2
0
cos sin ) ( 2 ) ) 2
2
8 1) sin
SB ds zB wt z rdr cf d
b
b B wt
π φ π
π π
Φ = =
= −
∫
i∫
0 i∫
sol) each turn = (
( 2
z
2
0
8 1) cos
N
d Nb
v N B wt
dt
π π
∴ ⇒ Φ
∴ = − Φ = − −
N-turns
( [V]
2
y b
x
Transformers (1) Transformers (1)
mmf
j j k k
j k
N I = ℜ Φ
∑ ∑
mmf
1, 2 1, , 2
number of turns and the currents : the reluctance of the magnetic circuit
N N i i ⇒ ℜ
N1 1 N2 2 ℜΦ
1 1 2 2 :
(where : mmf in the positive direction, mmf in the negative direction) N i N i
N i N i
l
∴ − = ℜΦ
ℜ = ℜ =
μ
Transformers (2) Transformers (2)
)
a Ideal transformer
1 2
1 1 2 2
2 1
)
) a
i N N i N i
i N cf
μ → ∞ = ⇒ =
Ideal transformer
,
Faraday's law
1 1
) cf
v N d dt d
= Φ Φ
Φ Faraday s law
( No negative sign, careful of sign of flux )
v N
2 2
v N d dt
= Φ
(But flux is in the reverse direction) 1 1
2 2
v N
v N
N
∴ =
⎛ ⎞
effective load seen by the source connected to primary winding
1 2 2
1 2 1
1
1 2 2
2
( )eff L
N v
v N N
R R
i N N
i
⎛ ⎞
⎜ ⎟ ⎛ ⎞
⎝ ⎠
= = ⎛ ⎞ = ⎜⎝ ⎟⎠
⎜ ⎟
2 1
2 1 1
2
( )eff L
N
Z N Z
N
⎜ ⎟
⎝ ⎠
⎛ ⎞
∴ = ⎜ ⎟
⎝ ⎠ Impedance transformation
⎝ 2 ⎠
Transformers (3) Transformers (3)
) Real transformer b
1 1 2 2
) Real transformer
b
N i N i l
s
s s
μ
μ μ
− = Φ
2 2
1 1 1 1 2 2 2 2 1 2 1 2 2
1 2 1 2
1 1 12 2 12 2
( ), ( )
,
1 s s
N N i N N i N N N i N i
l l
di di di di
v L L v L L
dt dt dt dt
μ μ
⇒ Λ = Φ = − Λ = Φ = −
= − = −
∵
2 2
1 1 , 2 2, 12 1 2)
(where
For an ideal tran
dt dt dt dt
s s s
L N L N L N N
l l l
μ μ μ
= = =
sformer ⇒No leakage flux ∴L L L
For an ideal tran 12 1 2
12 1 2 , 1 :
sformer No leakage flux
For a real transformer ( coefficient of coupling)
L L L
L k L L k k
⇒ ∴ =
∴ = <
Transformers (4) Transformers (4)
Equivalent ci rcui t Equivalent ci rcui t
1, 2 : :
winding resistance
leakage inductive reactance R R
X X1, 2 : :
:
leakage inductive reactance
power loss due to hysteresis and eddy current
nonlinear inductive reactance due to the nonlinear magnetization behavior of the ferro
c c
X X R X
magnetic core of the ferromagnetic core
A Moving Conductor in a Static Magnetic Field A Moving Conductor in a Static Magnetic Field
Fm =qu×B F qu B
F F
×
→
→
→
Charge Seperation
Coulomb force of an attraction
and will balance each other to be in equilibrium.
m e
F F
F F
→
∴
∫
and will balance each other to be in equilibrium.
Magnetic force per unit charge
2
21 1
, ,
( )
m m
F F
u B V E dl E
q q
V u B dl
= × = − ⋅ = −
∴ = × ⋅
∫
∫
The emf g
' ( )
V =
∫
C u×B dl⋅ →enerated around the closed loop is flux cutting emf
Ex 6 5) A Metal Bar Sliding Over Conducting Rails Ex 6-5) A Metal Bar Sliding Over Conducting Rails
B = zBˆ 0 constant u
0 1 2
,
( )
C
B zB u
V V V u B dl
=
= − =
∫
× ⋅ constanta)
1' 2' 0
0
ˆ ˆ ˆ
(xu zB ) (ydl) uB h
= × ⋅
= −
∫
2
0 2 ( 0 )
, l
V uB h
I P I R
R R
= = =
b)
1'
ˆ 0
Fm = I
∫
dl × = −B xIB h c) mechanical power0
m 2'
I
∫
( : n
2 2 2
0
)
m m
dl u B h
P F u F u
∴ = ⋅ = − ⋅ = R
egative direction to
m m
R
A Moving Circuit in a Time Varying Magnetic Field (1) A Moving Circuit in a Time Varying Magnetic Field (1)
( )
F =q E( + ×u B)
', '
Fm q E u B
E E E u B
+ ×
= + ×
To an observer moving with C,
the force on q can be interpreted as caused by an electric field
' ( )
C S C
E dl B ds u B dl
t
⋅ = − ∂ + × ⋅ →
∫ ∫
∂∫
General form of Faraday lawthe emf induced
B motional emf in the moving due to the motion frame of reference of the circuit in
transformer emf due to the time
i i variation
A Moving Circuit in a Time Varying Magnetic Field (2) A Moving Circuit in a Time Varying Magnetic Field (2)
The time rate of chage of magnetic flux,
2 2 1 1
0
lim 1 ( ) ( )
S
S S
t
d d
dt dt B ds
B t t ds B t ds
Δ → t
Φ = ⋅
⎡ + Δ ⋅ − ⋅ ⎤
⎢ ⎥
⎣ ⎦
Δ
∫
∫ ∫
=
( )
2 1
( ) ( ) . . .
t
B t t B t B t t H O T t
d B ds
⎣ ⎦
Δ
+ Δ = +∂ Δ +
∂
∴ ⋅ =
cf) Taylor's series
2 1
lim 1 . . .
B ds B ds B ds H O T
∂ ⋅ + ⎡⎢⎣ ⋅ − ⋅ + ⎤⎥⎦
∫
B ds∫ ∫ ∫
∴ dt
2 1
2 1
0
3
lim . . .
S S ds t S B ds S B ds H O T
t t
dS dl u t
+Δ → ⎢⎣ + ⎥⎦
∂ Δ
Δ
= × Δ
∫ ∫ ∫ ∫
assuming side surface S as the area swept out by the conductor in time t3
f om di e gence theo em
2 2 1 1
S S
B dv B ds B ds B ds
∇ ⋅ = ⋅ − ⋅ + ⋅
∫
V∫ ∫
from divergence theorem
3 3
2 1 ( )
S
B ds B ds t u B dl
∴ ⋅ − ⋅ = −Δ × ⋅
∫
∫
2 2∫
1 1∫
( )( )
' '
S S C
S S C
B ds B ds t u B dl
d B
B ds ds u B dl
dt t
d d
V E dl B d
∴ Δ ×
∴ ⋅ = ∂ ⋅ − × ⋅
∂
Φ
∫ ∫ ∫
∫ ∫ ∫
∫ ∫
' '
C S
d d
V E dl B ds
dt dt
∴ =
∫
i = −∫
⋅ = − ΦMaxwell’s Equation (1) Maxwell s Equation (1)
static Time varying
0
∇× = E B
E ∂
∇× = −
∂ ,
D ρ D ε E
∇ i = = t
D ρ
∂
∇ i =
0, H J
B B μ H
∇× =
∇ i = =
0 H J D
t B
∇× = + ∂
∂
∇ B 0
∇ i =
Maxwell’s Equation (2) Maxwell s Equation (2)
Note ① Continuity equation 0
J
J ρ
∇ =
∇ ∂ i
Note Continuity equation ①
: for steady state current : time varying current
J t
ρ
ρ
∇ = −
∂
∂ i
②
: time varying current Vector identity
( H ) 0 J J
t ρ
∇ ∇× = = ∇ ⇒ ∇ = − ∂
∂
∴
i i i
contradiction
( ) 0 D
H J ∂ ρ ⎛ J ∂ ⎞ ρ D
∇ ∇× i = = ∇ + i = ∇ i ⎜ + ⎟ where = ∇ i
Displacement current density. [A/m2]
Time varying electric field and induced magnetic field→coupling
∴
( H ) 0 J J D
t t
H J D
ρ
∇ ∇× = = ∇ + = ∇ ⎜ + ⎟ = ∇
∂ ⎝ ∂ ⎠
∇× = + ∂
∂
i i i , where i
Time varying electric field and induced magnetic field→coupling
( )
t
F q E u B
∂
= + ×
Cf) Lorentz force equation,
Integral Form of Maxwell’s Equation Integral Form of Maxwell s Equation
→
Cf) Differential form Point function
E B S C
t
→
∇× = − ∂ ⇒
∂
Cf) Differential form Point function
Apply stokes's theorem over open surface with contour
( )
S S
E ds B ds
t
∇× = − ∂
∫ i ∫ ∂ i
c s
B d
E dl ds
t dt
∂ Φ
= − = −
∫ i ∫ ∂ i
① : Faraday's law
∂ D
② H
c s
s
dl I D ds t
D ρ D ds Q
= + ∂
∂
∇ = ⇒ =
∫ ∫
∫
i i
i i
③
: Ampere's circuital law : Gauss law
∫
sEx 7 5 Ex. 7-5
(a) Displacement current = conduction current
dv
→
(a) Displacement current conduction current 1 conduction current current on the wire.
Apply circuit theorem
1 c 1 0 cos
C
i C dv C V t
dt ω ω
= =
2 Displacement cur
∂D rent. Reminding
1
H J D t
C A
μ ε d
∇× = + ∂
∂
=
Assuming the area A, plate separation d, permitivity , then Assume is uniform in the dielectric (ignoriE
0 i
vc V
E D E t
ng fringing effects) then
0
0 1 0
, sin
cos cos
c
D C
A
E D E t
d d
D A
i ds V t C V t i
t d
ε ε ω
ε ω ω ω ω
= = =
= ∂ = = =
∫
∂ i
Ex 7 5 Ex. 7-5
(b) Magnetic field intensity reminding Ampere's law
, C S
D D
H J H dl I ds
t t
∂ ∂
∇× = + = +
∂
∫
i∫
∂ i(b) Magnetic field intensity reminding Ampere s law
0 2
D =
∫
H dli =π
r①
②
①
surface S1 with ring C surface S2 with ring C
H
0, 2
D =
∫
C H dli =π
r①
1 0 cos
C
H
H
I J ds i C V t
φ
φ
ω ω
⇒
=
∫
i = =( Symmetry around the wire along the contour C) constant
1 0
1 0
cos
, cos
S C
d
J ds i C V t
I i Hφ C V t
ω ω
ω ω
= ∴ =
∫
② no conduction current, but displacement current
, cos
I id Hφ
ω ω
t∴
π
Potential Functions (1) Potential Functions (1)
0 ( ) 0
A
B A B
B A
= ∇×
∇ i ∇ ∇× i Vector magnetic potential,
(Solenoidal nature of )
Vector identity 0, ( ) 0
( )
B A
B A
E E A E
∇ = ∇ ∇× =
⎛ ⎞
∂ ∂ ∂
∇× ∴∇× ∇× ⇒ ∇× ⎜ +
i i
Vector identity Recall Faraday's law
▷
⎟ 0
Curl free( )
E E A E
t t t
∇× = − ∂ ∴∇× = − ∂ ∇× ⇒ ∇× ⎜ ⎝ + ∂ ⎠
0
( V ) 0
⎟ =
∇× ∇ = Vector identity
d d f l
▷
[ / ]
E V
A A
E V E V V m
t t
= −∇
∂ ∂
+ = −∇ = −∇ −
∂ ∂
and reminding for electromagnetics for time varying i.e)
t t
∂ ∂
Potential Functions (2) Potential Functions (2)
∂ A A 0
E V
t
E ρ
→ ∂ = ∴ = −∇
Cf) Static ∂
Time varying is induced by charge distribution and time varying J
B A E B
→
magnetic field time varying current,
l d d l d
▷ ,
1
B A E B
V
∴
=
also depends on are coupled
▷
▷
0' '
0
', '
4
v4
vdv A J dv
R R
μ ρ
πε ∫ = π ∫ : From the static condition
0
2 2
V ρ A μ
0J
∇ = − ∇ = −
These are solution of poisson equation
and
0ε
Potential Functions (3) Potential Functions (3)
J
R ρ
Quasi-static fields
- and vary slowly with time
- the range of interest R is small compared to the wavelength R
- the range of interest is small compared to the wavelength cf) Frequency is high, and is large compared to wavelength : time-retardation effect must be included.
, A , D ( , )
B A E V H J B H D E
t t μ ε
∂ ∂
= ∇× = −∇ − ∇× = + = =
∂ ∂
From the equations
t t
A J V A
t t
μ με
∂ ∂
⎛ ⎞
∂ ∂
∇×∇× = + ⎜ −∇ − ⎟
∂ ⎝ ∂ ⎠
⎝ ⎠
Recalling vec
( )
2A A A
∇×∇× = ∇ ∇ i − ∇ tor identity
Potential Functions (4) Potential Functions (4)
V
2A
∂ ∂
⎛ ⎞
2
2 2
2
( ) V A
A A J
t t
A V
A J A
μ με με
με μ με
∂ ∂
⎛ ⎞
∴∇ ∇ − ∇ = − ∇ ⎜ ⎝ ∂ ⎟ ⎠ − ∂
∂ ⎛ ∂ ⎞
∇ + ∇ ∇ + ⎜ ⎟
i
A
2J A
t t
A B A
με μ με
∇ − ∂ = − + ∇ ∇ + ⎜ ⎝ ∂ ⎟ ⎠
∇× = ∇
i
i
- we only designated but we are free to choose
- vector will b A A A
V V
∇× ∇
∂ ∂
e specified by giving and i
0 , 0 0
V V
A A
t t
με ∂ ∂
∇ + = = ∴∇ =
∂ ∂
i i
- let for static
Lorentz gauge for potentials g g p
Potential Functions (5) Potential Functions (5)
0, 0
0
V A
t t
A
∂ ∂
= =
∂ ∂
∴∇ i = cf) For static,
2
A μ
0J
∇ = −
then vector poisson equation
2
A
∂
- Then nonhomogeneous wave equation for vector potential becomes
2
2
A A
με ∂ t
∇ − = −
∂ μ J : Vector potential wave equation
Potential Functions(6) Potential Functions(6)
A , A
E V D V
t ρ ε ⎛ t ⎞ ρ
∂ ∂
= −∇ − ∂ ∇ i = ⇒ −∇ i ⎜ ⎝ ∇ + ∂ ⎟ ⎠ = Scalar potential wave equation
∨
2
( ) ,
t t
V A A V
t t
ρ με
ε
∂ ⎝ ∂ ⎠
∂ ∂
∴∇ + ∇ = − ∇ = −
∂ i i ∂
2 2
2
V V
t με ρ
ε
∴ ∇ − ∂ = −
∂
Boundary Condition (1) Boundary Condition (1)
Electric field's boundary condition
⊙
c s s v
E dl B ds D ds dv
t ρ
= − ∂ =
∫
i∫
∂ i∫
i∫
Electric field s boundary condition
... ...
⊙
0 0 0
B ds h S
∂ → Δ → →
∫
iFrom equation
when since area
0 0, 0
s ds h S
t → Δ → →
∫
∂when since area ∴ E1t = E2t (E1tΔ −w E2tΔ =w 0)
Boundary Condition (2) Boundary Condition (2)
From equation
1 2 2 1 2 1 2
( ) ( )
( )
sD ds D n D n S n D D S s S
n D D D D
ρ
ρ ρ
= + Δ = − Δ = Δ
∴ − = − =
∫
i i i ii From equation
2 ( 1 2) s , 2n 1n s
n D D D D
H
ρ ρ
∴ i = =
Magnetic field's boundary conditions
D
dl ⎛J ∂ ⎞ ds
= ⎜ + ⎟
∫
i∫
i1 2 1 2
2 1 2
( )
. ) ( )
c s
sn t t sn
dl J ds
t
H w H w J w H H J
i e n H H J
⎜ ⎟
⎝ ∂ ⎠
∴ Δ + −Δ = Δ − =
× − =
∫ ∫
i i
,
2 1 2
2
. ) ( ) s
s
i e n H H J
n J
×
cf) & are perpendicular to each other
Boundary Condition (3) Boundary Condition (3)
t )
H note)
The tangential component of the field is discontinuous across an interface where a free surface current exists
if both media have finite conductivity, currents are defined by volume current density
1t 2t
H H
→
→ =
current density
surface currents do not exists
i e) discontinuous only for interface with an ideal perfect conductor or super i.e) discontinuous only for interface with an ideal perfect conductor or super conductor.
∇iB = 0 ∴ B1n = B2n
Interface Between Two Lossless Linear Media Interface Between Two Lossless Linear Media
ε μ
→
Linear media permitivity : ε permeability : μ σ
→
→
Linear media permitivity : , permeability : Lossless =0
J
Sρ
→
→ Assume, at interface, no free charge
S=0
no surface currents =0
1 1 1
1t 2t
D
t,
1t 2tB
tE = E ⇒ = ε H = H ⇒ = μ
11 2 1 2
2 2 2
t t
,
t tt t
E E H H
D ε B
⇒ ⇒
2
1n 2n 1 1n 2 2n
,
1n 2n 1 1n 2 2nD D E E B B H H
μ
ε ε μ μ
= ⇒ = = ⇒ =
Interface between a Dielectric and Perfect Conductor (1) Interface between a Dielectric and Perfect Conductor (1)
→
Good conductor perfect conductor
( ) ( )
E
E D B H
→
⇒
Good conductor perfect conductor
Interior of perfect conductor (surface charge only) : are zero in the interior of a conductor
( , ) ( , )
,
E D B H
E D
⇒ are zero in the interior of a conductor
cf) In static case, may be zero, but H , may not be zero. B
2
0,
20,
20,
20
E = H = D = B =
Interface between a Dielectric and Perfect Conductor (2) Interface between a Dielectric and Perfect Conductor (2)
0 0
E1 E2
2 1 2 2
1 1
0, 0
( ) , 0
, 0 0
t t
s t
t sn sn t
E E
n H H J H
H J J H
= =
× − = =
= = → =
if
2 1 2 2 1
1 2
( ) , 0,
0, 0
s n n s
n n
n D D D D
B B
n
ρ ρ
− = = =
= =
i
note) n2 : outward normal from medium2 note)
E
: outward normal from medium2
At an interface between a dielectric and a perfect conductor
i l t d i t f (i t ) th d t f
1
1 1
1 s n
E
E E ρ
= = ε
: is normal to and points away from(into) the conductor surface
: is tangential to the interface with a magnitude of
Wave Equation and Their Solutions (1) Wave Equation and Their Solutions (1)
2 A
2 ∂
2 2 2
2
A A J
t V V
t
με μ
με ρ
ε
∇ − ∂ = −
∂
∇ − ∂ = −
∂ Wave equation :
2
( ) t
t t
ε
ρ ν
∂
Δ ′ i
Solution :
Assume an elemental point charge at time , located at the
i i f th di t
origin of the coordinates.
V R t
i i
Spherical coordinates.
depends only on . and because of spherical symmetry.
1 2 V
φ
∂ ⎛ ∂ ⎞ i
(No dependence on ) Except at the origin,
2V
2 ∂
2
1 V
R ∂∂R⎛⎜⎝R ∂∂R ⎞ −⎟⎠
με
V2 0 t
∂ =
∂
Wave Equation and Their Solutions (2) Wave Equation and Their Solutions (2)
New variable
( )
2 2
( , ) 1 ( , )
1 1 1
V R t U R t R
U U
=
∂ ⎛ ⎞ ⎡ ∂ ⎤ ∂
New variable
( )
2 2
2
2
2 2 2
1 1 1
,
1 1
U U
R U R t R U U R
R R R R R R
U U U U
U R R
R R R R R R R
∂ ⎛⎜ ⎞⎟= ⎡⎢− + ∂ ⎤⎥= − + ∂
∂ ⎝ ⎠ ⎣ ∂ ⎦ ∂
⎡ ⎤
∂ ⎡⎢− + ∂ ⎤⎥ = ⎢−∂ + ∂ + ∂ ⎥
∂ ⎣ ∂ ⎦ ⎣ ∂ ∂ ∂ ⎦
1
R ∂R ⎣ ∂R ⎦ R ⎣ ∂R ∂R ∂R ⎦
∴
2 2 1 22 2 ( , )2 2 ( , )2
0, 0
U U U R t U R t
R R R t R t
t R t R
με με
με με
∂ ∂ ∂ ∂
− = − =
∂ ∂ ∂ ∂
+
i.e)
Any function of ( ) or of ( ) will satisfy the differential
( )
t R t R
f t R
με με
με
− +
−
Any function of ( ) or of ( ) will satisfy the differential equation
is a wave equation which travels away from the origin
Wave Equation and Their Solutions (3) Wave Equation and Their Solutions (3)
( )
f ( R )
i ti hi h t l t th i i h i l
( , ) ( )
f t R
U R t f t R
με
με
+ →
∴ = −
is a wave equation which travels to the origin physical nonsense
( , ) ( )
( , ) ( )
f
R R t t
U R R t t f t t R R
μ
με
+ Δ + Δ
⎡ ⎤
+ Δ + Δ = ⎣ + Δ − + Δ ⎦
the function at at a later .
= f t( −R
με
)0
.
1 1
limt
if t R
R R
t t u
με
με
Δ →με
Δ = Δ
Δ = ⇒ Δ = =
Δ Δ
: velocity of propagation
0
( , ) 1
t t t
V R t f t R
R u
με
Δ →με
Δ Δ
⎛ ⎞
= ⎜⎝ − ⎟⎠
f t R u
⎛ − ⎞
⎜ ⎟
⎝ ⎠
Determine
Wave Equation and Their Solutions (4) Wave Equation and Their Solutions (4)
( )t ρ Δν Recall potential function induced by a static point charge ( ) at
( ) ' '
t t R v
t v R u
ρ ν
ρ ρ
Δ
⎛ − ⎞Δ
⎜ ⎟
Δ ⎛ ⎞ ⎝ ⎠
Recall potential function induced by a static point charge at the origin
( ) ( ) ,
4 4
1
t v R u
V R f t
R u
t R u ρ
πε πε
ρ
Δ ⎛ ⎞ ⎝ ⎠
Δ = Δ ⎜⎝ − ⎟⎠=
⎛ − ⎞
⎜ ⎟
⎝ ⎠
∫
'
( , ) 1 '
4 v
V R t u dv
πε ⎝ R ⎠
∴ =
∫
:
R t
⎛ R⎞ Retarded scalar potential Scalar potential at a distance from the source at time
t R u
⎛ ⎞
→Depends on the value of charge distribution at an earlier time ⎜⎝ − ⎟⎠ Retarded vector potential
⎛ RR⎞
⎛ ⎞
Source Free Wave Equation Source Free Wave Equation
If the wave is in a simple (linear isotropic and homogeneous)
H , E
E H
t t
ε μ σ
μ ∂ ε ∂
∇× = − ∇× =
∂ ∂
If the wave is in a simple (linear, isotropic and homogeneous) non conducting medium. i.e) , ( =0)
0 ,
t t
E H
∂ ∂
∇i = ∇i
2
= 0 From vector identity
2
( ) 2
) ( ) ( ) ( ) ( )
E H E
t t
cf A B C B A C C A B B A C A B C
μ ∂ με ∂
∇×∇× = − ∇× = −
∂ ∂
× × = i − i = i − i
2 2
2
( E) ( )E E
E με E
∇ ∇ − ∇ ∇ = −∇
∴∇ − ∂
i i
2 12
0 if
t = με = u
∂
2 2
2 2
2 2 2 2
1 1
0, 0
E H
E H
u t u t
∂ ∂
∇ − = ∇ − =
∂ ∂
: Homogeneous vector wave equation
Time Harmonic Fields Time Harmonic Fields
Maxwell's equations Maxwell s equations
- linear differential equations
- sinusoidal time variation of source functions at given frequency ,
- are sinusoidal with the same frequency E H
Ti h i d i id l
Time harm →
→
onic steady state sinusoidal Phasors : Amplitude and phase information
independent of time e
j tω→ independent of time
cf) : time dependent factor
Time Harmonic Electromagnetics (1) Time Harmonic Electromagnetics (1)
Vector phasors of field vectors : depend on space coordinates ( , , ; ) Re ( , , ) ,
( ) :
E x y z t E x y z e
j tE x y z
⎡
ω⎤
= ⎣ ⎦
Vector phasors of field vectors : depend on space coordinates
where ( , , ) : vector phasor : complex quantity ( , , ; ) Re
E x y z
E x y z t j E
t ω
∂ =
∂
where vector phasor : complex quantity ⎡ ⎣ ( , , ) x y z e
j tω⎤ ⎦
( , , ) :
( , , )
( , , ; ) Re
j tj E x y z
E x y z
E x y z t dt e
j
ω
ω
ω
⎡ ⎤
= ⎢ ⎥
⎣ ⎦
∫
where vector phasor
( , , )
j E x y z
j
ω ω
⎣ ⎦
where : vector phasor
2
( )
2 2
, , 1
j j
t ω t ω j
ω
∂ ⇒ ∂ ⇒ ⇒
∂ ∂ ∫
i.e)
Time Harmonic Electromagnetics (2) Time Harmonic Electromagnetics (2)
Maxwell's equations
,
, ,
E H ρ J
Maxwell's equations
Vector field phasors ( )
Source phasors ( ) Simple (linear, isotropic and homogeneous) media ,
,
E j H H J j E
E H
ωμ ωε
ρ ε
∇× = − ∇× = +
∇i = ∇i
0
ej tω
⎫⎪
= ⎬⎪⎭ Assuming
ε
2 2
V A
V k V ρ
⎭
∇ + = − ⎫⎪
⎬
Time harmonic wave equation for and
Non-homogeneous helmholtz's equations
2 2
2 2 k , k :
A k A J u
εμ ω με ω με ω
⎪⎬ = = =
∇ + = − ⎪⎭
where wave-number
Time Harmonic Electromagnetics (3) Time Harmonic Electromagnetics (3)
∂22 ∂
2
2 2 2
2
) A V 0 0
cf A J A A j V
t t
V V
t
με μ με ωμε
με ρ
ε
∂ ∂
∇ − = − ∇ + = ⇒ ∇ + =
∂ ∂
∇ − ∂ = −
∂
i i
( )
2 2
2 2 2
0 t
E E
t H
ε με
∂
∇ − ∂ =
∂
∂
2 H
H με ∂
∇ −
2
( )
0
1 1
j t R j R
u u
t
ω ω
ρ − ρ −
∂ = Phasor solution
' '
'
1 1
( , ) ' ( ) '
4 4
( ) 1 '
4
u u
j t j t
v v
jkR
v
e e
V R t dv V R e dv e
R R
V R e dv
R
ω ω
ρ ρ
πε πε
ρ πε
−
= ⇒ = ⋅
⎧ =
⎪⎪⎨
∫ ∫
∫
[V]
E p essions fo the eta ded scala and
'
4
( ) '
4
jkR
v
R
A R Je dv
R πε
μ π
−
⎪⎨
⎪ =
⎪⎩
∫
[Wb/m]
Expressions for the retarded scalar and vector potentials due to time harmonic sources
Time Harmonic Electromagnetics (4) Time Harmonic Electromagnetics (4)
2 2
kR k R
1 .... :
2
2 2
,
jkR k R
e jkR
k f u f
u u
ω π π λ
λ
− = − − +
= = = =
cf) Taylor series expansion.
'
2 1 1, ( ) 1 '
4
jkR
v
u u
if kR R e V R dv
R
λ
π ρ
λ πε
= ⇒ − = =
∫
⇒then static potential
Procedure for determining the electric and magnetic fields due to Procedure for determining the electric and magnetic field
( ) ( )
V R A R
s due to time harmonic charge and current distributions
1. Find phasors and
( ) )
( )
E R V j A cf E V A
t
B R A
ω
∂= −∇ − = −∇ −
∂
= ∇×
2. Find phasors
Source free Fields in Simple Media (1) Source-free Fields in Simple Media (1)
Source free fields in simple media
E j H
H j E
ωμ ωε
⎧∇× = −
⎪∇× =
⎪⎨
Source free fields in simple media
0
0 E
H
⎨∇ =
⎪⎪∇ =
⎩ i
i
2 2
2 2 2 2
0 0 E k E
H k H k
ω με
⎧∇ + =
⎪⎨
∇ + = =
⎪⎩
and Homogeneous vector Helmholtz’s equation
⎩
μ
PrinciplE
e of duality : Source free Maxwell's equations in a simple media are invariant under the linear transformation
' , ' E ,
E
η
H Hη μ
η ε
= = − =
Source free Fields in Simple Media (2) Source-free Fields in Simple Media (2)
0
( )
J E
H j E j E j E
σ σ
σ ωε ω ε σ ωε
≠ ⇒ =
⎛ ⎞
∴∇× = + = ⎜ + ⎟ =
If simple medium is conducting i.e)
( ) c
c
H j E j E j E
j j
σ ωε ω ε ωε
ω ε ε σ
ω
∴∇× + ⎜ + ⎟
⎝ ⎠
= −
and [F/m] : complex permitivity
⋅
cf) out of phase polariza
⋅ →
tion : power loss to overcome a fractional damping mechanism caused by the inertia the charged particle
finite conductivity ohmic losses
' j '' ε ε ε
→
= −
te co duct ty o c osses Complex permitivity
[F/m] where ε '' : out of phase polarization and finite conductivity
c j
ε =ε ε
[F/m] , where : out of phase polarization and finite conductivityε
Source free Fields in Simple Media (3) Source-free Fields in Simple Media (3)
Complex permeability : out of phase component of magnetization
' '', ''
'
μ μ jμ μ μ
μ μ
= −
∴ =
Complex permeability : out of phase component of magnetization where ' for ferromagnetic materials
Complex wavenumber
( ' '')
c c
k =ω με =ω μ ε − jε Complex wavenumber
: in a lossy dielectric
Loss tangent
tan '' ,
'
''
c c
ε σ
δ δ
ε ωε ε
⎧ = ≅
⎪⎪⎨
⎪
where : loss angle
loss tangent ε ' σ ωε
⎪⎪⎩loss tangent Good conductor & Good insulator
: Good conductor σ ωε
: Good insulator
Source free Fields in Simple Media (4) Source-free Fields in Simple Media (4)
π
∂
Cf) Electric hertz vector, ,
A V
t
A
με ∂π π
= = −∇
∂
⎧ ∂
⎪
i
: combine the vector and scalar potential and satisfy the Lorentz condition
0 E V A
t A V
με t
= −∇ −∂
⎪⎪ ∂
⎨ ∂
⎪∇ + =
⎪ ∂
⎩ i
combine continuity equation
0, ,
J
J J P P
t t
ρ
ρ ρ
∂ ∂
∇ + = = = −∇
∂ ∂
i i
with and
2
t t
π P
∂ ∂
∂
Single vector equation
2π με ∂ π P
∇ − = −
The electromagnetic spectrum
The electromagnetic spectrum