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ELG5106 Fourier Optics. Trevor Hall [email protected]. Fourier Optics . Diffraction. 2. Propagation between Planes in Free Space. x 2. y 2. y 1. x 1. k. x 3. x 3 =z. x 3 =0. 3. Plane Wave Expansion I. Evanescent wave. 4. Plane Wave Expansion II. 5. Plane Wave Expansion III. - PowerPoint PPT Presentation
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ELG5106 Fourier Optics
Trevor [email protected]
DIFFRACTIONFourier Optics
2
Propagation between Planes in Free Space
3
x1
x2
y1
y2
x3
x3=0 x3=z
k
022 k
Plane Wave Expansion I
213213221121
222
21
222
21213
222
21
22
21
2213
223
22
21
22
,exp,
: tosgeneralise ion thissuperpositby ,,
,,
)dependence exp(implicit wavegoing forward afor exp,0
dkdkxkkkxkxkikka
kkkkkkikkk
kkkkkkkkk
tikkkkiak
x
k.x
Evanescent wave
4
Plane Wave Expansion II
2122112121
21213221121221
322112132121
21221121321
3
exp,,ˆ
where
,exp,ˆ2
1,
then,,,,0,,,
:setting and
exp,0,,
:constant tivemultiplica awithin ansformFourier tr inversean toreduces this0at that Noting
dkdkxkxkixxukku
dkdkzkkkykykikkuyyv
zxyxyxyyvxxxxxu
dkdkxkxkikkaxxx
x
5
Plane Wave Expansion III
zkkikkkh
dkdkzkkkykykiyyh
dxdxxxuxyxyhyyv
dkdkdxdxzkkkxykxykixxuyyv
21321
212132211221
2121221121
212121322211121221
,exp,ˆ
,exp2
1,
,,,
,exp,2
1,
Explicity
Linear Shift Invariant System
Impulse Response /Point Spread Function
Spatial Frequency Response
6
Propagation as a filter
u v
022 k
1k
h2k
7
k0
1
unimodular phase function
exponential decay
Why is the angular spectrum of plane waves expansion rarely used?
kzqpqpi
qpqpm
dpdqmzyq
zypikyyh
kkd
kkd
kkkk
zy
kk
zy
kkikzkyyh
dkdkzkkkykykiyyh
1,1
1,1
exp2
,
or
,exp2
,
rewriten bemay
,exp2
1,
2222
2222
212
2
21
2121322112
2
21
212132211221
8
Oscillatory Integrals• We are left with the consideration of integrals of the form:
,,
exp
Ca
dppipaI
• If 0p
then the integrand is highly oscillatory and
,0I• If 0*
pp
then there is a contribution from the integrand in the neighbourhood of the stationary point p*
9
Stationary Phase Condition
The stationary phase condition corresponds to a ray from source point to observation point ( recall shift invariance)
00;00
1;,,
21
2211
mq
zy
pmp
zy
p
qpmqpmzyq
zypqp
1y
z
p
m3
2
3
1 ,kk
mq
kk
mp
10
Paraxial Approximation IIn a paraxial system rays are inclined at small angles to the optical axis. One may then make the paraxial approximation:
22
21
22
21
2221
21
2222
21
21
21
211
21
211
,,
21
2111
zyq
zyp
zy
zy
qpzyq
zyp
qpmzyq
zypqp
qpqpm
z
11
Paraxial Approximation II
22
21
22
21
2
2
2
22
2122
2
2
22
21
22
21
2
2
2
2
21
21
211expexp
21
21
211exp2
2
21
211expexp
2
21
211expexp
2
,exp2
,
zy
zyikzikz
zik
zy
zyi
ik
zy
zyidpdqqpik
zy
zyidpdq
zyq
zypik
dpdqqpikyyh
12
Fresnel Diffraction
212211
22
21
21
21
21
21
222
211
21
2121221121
exp21
211exp,
21
211exp
21
21
211exp,exp
21
,,,
dxdxyxyxzik
zx
zxikzxxu
zy
zyikz
zik
dxdxzxy
zxyikzxxuikz
zik
dxdxxxuxyxyhyyv
13
Up to a multiplicative quadratic phase factor (that is often neglected), the field at the observation plane is given by the Fourier transform of the field at the source plane multiplied by a quadratic phase factor.
Fraunhoffer Diffraction
2122112121 exp,, dxdxyxyxzikxxuyyv
14
If the source filed u has compact support (is zero outside some bounded aperture) and z is sufficiently large the variation of the quadratic phase factor over the support of u becomes negligible. The leading phase factor is also often neglected either because the region of interest in the observation plane subtends a sufficiently small angle with respect to the origin at the source plane or because it is the intensity only that is observed. The diffracted field distribution is then given by a Fourier transform of the field distribution in the source plane.
Notes• The oscillatory integral representation of the impulse response of this
optical system can be evaluated asymptotically without recourse to the paraxial approximation using the method of stationary phase.
• The magnitude but not the phase of the leading multiplicative phase factors of the Fresnel and Faunhoffer diffraction integrals may be evaluated by appealing to energy conservation – the integral over the source and observation planes of the field intensity must be equal.
• The choice of outgoing plane waves in the plane wave spectrum ensures that all three diffraction integrals (plane wave expansion, Fresnel & Fraunhoffer formulae satisfy the Sommerfeld radiation condition at infinity.