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ETEN05 Electromagnetic Wave PropagationLecture 6: Oblique propagation, beams, and
FDTD
Daniel Sjoberg
Department of Electrical and Information Technology
September 18, 2009
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
Oblique propagation
I So far, we have chosen the z direction as the propagationdirection.
I We shall see how this generalizes, and how to describe wavepropagation when the preferred direction is not the purepropagation direction.
I Understanding of this situation helps analyzing reflection onsurfaces at different angles.
I It also helps analyzing more general wave types than planewaves (today we look at beams).
Daniel Sjoberg, Department of Electrical and Information Technology
Numerical methods
Some problems are too complicated to do by hand, such as apacemaker in the human body. Numerical methods help.
Daniel Sjoberg, Department of Electrical and Information Technology
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
Generalized propagation factor
For a wave propagating in an arbitrary direction, the propagationfactor is generalized as
e−jkz → e−jk·r
Assuming this as the only spatial dependence, the nabla operatorcan be replaced by −jk since
∇(e−jk·r) = −jk(e−jk·r)
Writing the fields as E(r) = E0e−jk·r, Maxwell’s equations forisotropic media can then be written{
−jk ×E0 = −jωµH0
−jk ×H0 = jωεE0⇒
{k ×E0 = ωµH0
k ×H0 = −ωεE0
Daniel Sjoberg, Department of Electrical and Information Technology
Properties of the solutions
Eliminating the magnetic field, we find
k × (k ×E0) = −ω2εµE0
This shows that E0 does not have any components parallel to k,and the BAC-CAB rule implies k× (k×E0) = −E0(k · k). Thus,
k2 = k · k = ω2εµ
It is further clear that E0, H0 and k constitute a right-handedtriple since k ×E0 = ωµH0, or
H0 =k
ωµ
k
k×E0 =
1ηk ×E0
Daniel Sjoberg, Department of Electrical and Information Technology
Preferred direction
What happens when k is not along the z-direction (which could bethe normal to a plane surface)?
I There are then two preferred directions, k and z.
I These span a plane, the plane of incidence.
I It is natural to specify the polarizations with respect to thatplane.
I When the H-vector is orthogonal to the plane of incidence,we have transverse magnetic polarization (TM).
I When the E-vector is orthogonal to the plane of incidence, wehave transverse electric polarization (TE).
Daniel Sjoberg, Department of Electrical and Information Technology
TM and TE polarization
From these figures it is clear that the transverse impedance is
ηTM =ExHy
=A cos θ
1ηA
= η cos θ
ηTE = −EyHx
=B
1ηB cos θ
=η
cos θ
Daniel Sjoberg, Department of Electrical and Information Technology
Interpretation of transverse wave vector
The transverse wave vector kt = kxx corresponds to the angle ofincidence θ as
kx = k sin θ
This interpretation holds also for the vector kt in the fundamentaleigenvalue equation
β
k0
(Et
η0Ht
)=(
0 −z × Iz × I 0
)·[(εtt ξtt
ζtt µtt
)−A(kt)
]︸ ︷︷ ︸
=W
·(Et
η0Ht
)
in the completely general bianisotropic case. The transverseimpedance is
Et = Zr · (η0Ht × z), η0Zr = η cos θxx+η
cos θyy︸ ︷︷ ︸
isotropic case
Daniel Sjoberg, Department of Electrical and Information Technology
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
The plane wave monster
So far we have treated plane waves, which have a seriousdrawback:
I Due to the infinite extent of e−jβz in the xy-plane, the planewave has infinite energy.
However, the plane wave is a useful object with which we can buildother, more physically reasonable, solutions.
Daniel Sjoberg, Department of Electrical and Information Technology
Finite extent in the xy-plane
We can represent a field distribution with finite extent in thexy-plane using a Fourier transform:
Et(r, ω) =1
(2π)2
∞∫∫−∞
Et(kt, ω)e−jkt·r−jβz dkx dky
Et(kt, ω) =
∞∫∫−∞
Et(r, ω)ejkt·r dx dy
Defining the (square of the) total wavenumber ask2 = |kt|2 + β2 = k2
x + k2y + β2 = ω2εµ implies
β = (k2 − |kt|2)1/2
Daniel Sjoberg, Department of Electrical and Information Technology
Initial distribution
Assume a Gaussian distribution in the plane z = 0
Et(x, y, z = 0, ω) = A(ω)e−(x2+y2)/(2b2),
The transform is itself a Gaussian
Et(kt) = A(ω)2πb2e−(k2x+k2
y)b2/2
Daniel Sjoberg, Department of Electrical and Information Technology
Paraxial approximation
The field in z ≥ 0 is then
Et(r) =12πAb2
∞∫∫−∞
e−(k2x+k2
y)b2/2−j(kxx+kyy)−jβz dkx dky
The exponential makes the main contribution to come from aregion close to kt ≈ 0. This justifies the paraxial approximation
β = (k2 − |kt|2)1/2 = k(1− |kt|2/k2)1/2
= k
(1− 1
2|kt|2
k2+ O(|kt|4/k4)
)= k − |kt|2
2k+ · · ·
Daniel Sjoberg, Department of Electrical and Information Technology
Computing the field
Inserting the paraxial approximation in the Fourier integral implies
Et(r) ≈12πAb2
∞∫∫−∞
e−(k2x+k2
y)( b2
2−j z
2k)−j(kxx+kyy)−jkz dkx dky
= · · · = A
1− jξ(z, ω)e−(x2+y2)/(2F 2)−jkz
where F 2(z, ω) = b2 − jz/2k = b2(1− jξ(z, ω)) and ξ = z/(kb2) isa real quantity.
Daniel Sjoberg, Department of Electrical and Information Technology
Beam width
The power density of the beam is proportional to
e−(x2+y2)Re(1/F 2)
and the beam width is then
B(z) =1√
Re 1F 2
= · · · = bξ√
1 + ξ−2
where ξ = z/(kb2). For large z, the beam width is
B(z)→ bξ(z) =z
kb, z →∞
Daniel Sjoberg, Department of Electrical and Information Technology
Beam width
The beam angle θb is characterized by
tan θb =B(z)z
=1kb
Small initial width compared to wavelength implies large angle.Daniel Sjoberg, Department of Electrical and Information Technology
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
Finite difference approximation
To make numerical simulations, we approximate the derivatives inthe wave equation
∂2E
∂z2− 1c2∂2E
∂t2= 0
with finite differences (where the field is evaluated in grid pointsE|nr = E(r∆z, n∆t):
E|nr+1 − 2E|nr + E|nr−1
(∆z)2− 1c2E|n+1
r − 2E|nr + E|n−1r
(∆t)2= 0
We expect the error in the approximation to decrease as ∆z and∆t become small.
Daniel Sjoberg, Department of Electrical and Information Technology
Time stepping
By solving for the field at time step n+ 1, we find
E|n+1r = 2E|nr − E|n−1
r +(c∆t
∆z
)2
(E|nr+1 − 2E|nr + E|nr−1)
Thus, the solution at time t can be found if the solution at twoprevious time steps is known.
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
jjj jj
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
j
jj jj
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
jj
j jj
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
jjj j
j
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
jjj jj
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Leap frog stencil
-
6
0
0
z
t
∆z
∆t
r∆z
n∆t
b b b b b b bb b b b b b bb b b b b b bb b b b b b bb b b b b b b
jjj jj
Initial conditions: E|0r = fr and E|1r = gr (known functions).Boundary conditions: E|n0 = 0 and E|nR = 0 (metal walls).
Daniel Sjoberg, Department of Electrical and Information Technology
Dispersion relation
A harmonic wave propagating through the lattice can be written
ejωn∆t−jkr∆z
Inserting this into the difference approximation we obtain
ejωn∆t−jkr∆z
(e−jk∆z − 2 + ejk∆z
(∆z)2− 1c2
ejω∆t − 2 + e−jω∆t
(∆t)2
)= 0
which can be rewritten as(sin
ω∆t
2
)2
=(c∆t
∆z
)2(sin
k∆z
2
)2
This relates the spatial frequency k to the temporal frequency ω,and is called the dispersion relation.
Daniel Sjoberg, Department of Electrical and Information Technology
Time step and stability: R = c∆t/∆z
R = 1: Magic time step, ω = ±ck, no dispersion.
R < 1: Stable solution, ω 6= ±ck, different frequencies travel withdifferent speed (lower than c).
R > 1: Unstable solution, growing exponentially.
Daniel Sjoberg, Department of Electrical and Information Technology
Example: square wave
R = 1
R < 1
R > 1
Daniel Sjoberg, Department of Electrical and Information Technology
Example: smooth wave
Daniel Sjoberg, Department of Electrical and Information Technology
Time and frequency
Even though FDTD solves problem in the time domain, the resultscan be transformed to the frequency domain. A common situationis the computation of resonance frequencies in a cavity:
I Discretize the cavity with finite differences.
I Set up PEC boundary conditions.
I Give random data as initialization in order to excite allfrequencies.
I Run simulation for a long time.
I Fourier transform the field, sampled at a point.
I The resulting spikes correspond to the resonances of thecavity.
Daniel Sjoberg, Department of Electrical and Information Technology
Outline
1 Introduction
2 Oblique propagation
3 Paraxial approximation: beams
4 Finite differences in the time domain: FDTD
5 Conclusions
Daniel Sjoberg, Department of Electrical and Information Technology
Conclusions
I Oblique propagation with respect to some preferred directionz generates a plane of incidence.
I The TM and TE polarizations are natural decompositions ofthe fields.
I A beam can be composed by many plane waves travellingalmost parallel to the axis.
I The beam broadens as it propagates. Narrow beam, largeangle.
I FDTD is a simple numerical scheme for time domain.
I It is vital to choose a smaller discretization in time than infrequency. The relation between time and space determinesthe numerical dispersion.
Daniel Sjoberg, Department of Electrical and Information Technology
Next week
I Three lectures next week, lots to read!
I Overall theme is pulse propagation and dispersion.
I The second handin is distributed on Tuesday, and will dealwith numerical experiments.
Daniel Sjoberg, Department of Electrical and Information Technology