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ECE 107: Electromagnetism Set 7: Dynamic fields
Instructor: Prof. Vitaliy Lomakin Department of Electrical and Computer Engineering
University of California, San Diego, CA 92093
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Maxwell’s equations • Maxwell’s equations
• Goals of this chapter – To “close the loop” between dynamics and statics – To explain effects introduced by time variations – To extend some results from static to dynamics
t∂∇× = −∂BE
t∂∇× = +∂DH J
ρ∇⋅ =D
0∇⋅ =B
12 2 1
12 2 1
12 2 1
12 2 1
ˆ ( ) 0ˆ ( )ˆ ( )ˆ ( ) 0
s
s
ρ× − =⋅ − =× − =⋅ − =
n E En D Dn H H Jn B B
εµ
==
D EB H
E ⋅d l∫ = − ddt
B ⋅ds∫∫H ⋅d l∫ = d
dtD ⋅ds∫∫ + I
D ⋅ds∫∫ = Q
B ⋅ds∫∫ = 0
εµ
==
D EB H
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Faraday’s law • Faraday’s law: • Magnetic flux: • Electromotive force voltage: • induces currents in a wire
loop. The currents produce the flux that opposes the inducing flux (Lenz’s law)
• allows for transformers, generators, motors, etc.! Its existence is a foundation of Electromagnetics
E ⋅d l
C∫ = − ddt
B ⋅dsS∫∫
SdΦ = ⋅∫∫ B s
emf S
d dV ddt dtΦ= − = − ⋅∫∫ B s
emfV
emfV
• Transformers: – Current à mutual flux – Flux à voltage
– Energy conservation à
Faraday’s law (2)
I1V1 = I2V2
⇒ I1I2
= N2
N1
V1 = −N1dΦdt, V2 = −N2
dΦdt
⇒ V1V2
= N1N2
• Electric generator: – Rotating loop in a magnetic field à EMF
• Electric motor: – Opposite to the generator – An AC current is sent to the coil in
a constant magnetic field à coil spins
Faraday’s law (2)
• Eddy currents: – Time varying magnetic field à Electric field à (Eddy) current
• Examples: – Eddy current waist separator – Eddy current break – Transcranial magnetic stimulation
Faraday’s law (2)
∇×E = − ∂B
∂t⇒ J =σE
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Ampere’s law • Ampere’s law: • Displacement current: • Displacement current density: • Displacement current is required to establish
consistent equations of Electromagnetics. Its introduction resulted in Maxwell’s equations
• To explain its importance, consider a capacitor under an ac voltage.
H ⋅d l
C∫ = I + ddt
D ⋅dsS∫∫
d dS S
dI d ddt
= ⋅ = ⋅∫∫ ∫∫J s D s
dddt
= DJ
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Charge-current continuity relation • Start with the Ampere’s law • Apply divergence
• Continuity relation:
• The amount of charge change equals the current needed to compensate the change
• For statics – The current and charge are independent – Kirchhoff’s current law
t∂∇× = +∂DH J
∇⋅(∇× H) =0 (vector identity)
= ∇⋅ ∂D∂t
+∇⋅J ⇒∇⋅J = − ∂∂t
∇⋅D =ρvGauss law
⇒∇⋅Jv = − ∂∂t
ρv
⇒ Jv ⋅dsS∫∫ = − ∂
∂tρvV∫∫∫ ⇒ I = − ∂
∂tQ
Jv ⋅ds
S∫∫ = 0⇒ 0ii I =∑
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Complex permittivity (1) • Modified Ampere’s law
– Ampere’s law – Constitutive relation – Current
– Modified Ampere’s law
• Complex permittivity • Loss tangent
jω∇× = +H D Jε=D E
J = Jcconductivity
Jc=σE
+ Ji impressedgiven source
⇒∇× H = jωεE+ Jc + Ji⇒∇× H = jωεE+σE+ Ji
⇒∇× H = jω ε − jσω
⎛⎝⎜
⎞⎠⎟
εc
E+ Ji
| | jc c
j j e δσε ε ε ε εω
−′ ′′= − = − =
tan ( )δ ε ε σ ωε′′ ′= =
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Complex permittivity (2) • Maxwell’s equations in conducting media
– Differential equations
– Boundary conditions
– Continuity relation
∇× E = − jωµ H∇× H = jωεc
E+ Ji∇⋅ D = ρi∇⋅ B = 0
n12 × ( E2 − E1) = 0n12 ⋅(εc2
E2 − εc11E1) = ρis
n12 × ( H2 − H1) = J is
n12 ⋅(µ2H2 − µ1
H1) = 0
i isjωρ∇⋅ = −J
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Electromagnetic potentials (1) • Fields radiated in free space by a charge
distribution and current distribution (recall that and are related )
1
Vt
µ= ∇×
∂= −∇ −∂
H A
AE
V (R,t)
retartedpotential
= 14πε
ρv ( t − ′R vp
retardation due to causality
)
′R′V
∫∫∫ d ′v
A(R,t) = µ4π
Jv (t − ′R vp )
′R′V
∫∫∫ d ′v
( , )v tJ r( , )v tρ r
v v tρ∇⋅ = −∂ ∂Jvρ vJ
83 10pv c m s= = ×
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Electromagnetic potentials (2) • Frequency domain fields radiated by a charge
distribution and current distribution (recall that and are related )
⇒H = 1
µ∇× A
E = −∇ V − jω A
V (R) = 14πε
ρve− jk ′R
′R′V
∫∫∫ d ′v
A(R) = µ4π
Jve− jk ′R
′R′V
∫∫∫ d ′v
Jv
ρv (r)
2 wavenumberp
kvω π
λ= = −
ρv ∇⋅ Jv = − jω ρv
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Radiation from a short dipole (1) • Consider an electric dipole • Its time derivative results in
current
• When then is uniform • Physically, the dipole is
represented by two wires • Vector potential
ˆql=p z
ddt
p = Il z ⇒ jω p = Il z
l λ= I
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• Expressions for the radiated fields
• When the expressions reduce to the expression due to a static dipole with
• Magnetic field is present only in the dynamic case • No electric field is in the direction, hence the
field is TM to z • The short dipole is one of the simplest antennas
⇒
0ω →( )p Il jω=
ϕ
η0 =µ0
ε0
= 120π
characteristic impedance of free space
Radiation from a short dipole (2)
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• Far field approximation: or – The terms can be neglected – Far field approximation fields
– Characteristics of far field fields of ANY antenna § Relation between E and H is simply through the impedance
of free space similar to the case of transmission lines § The phase behavior is like for TLs with z replaced by R § The field decays but only as (compare to decay
for a static charge and decay for an electric dipole)
R λ kR12 3~1 ( ) ,1 ( )kR kR
1 R 21 R31 R
Radiation from a short dipole (3)