Plane Wave Spectrum Method
� Plane Wave Spectrum Method
� Solve the source-less Maxwell’s equations with the constrain of the boundary conditions
� Plane Waves are naturally eigenmodes
� Other functions also possible, e.g. Gaussian beams
Source-less Maxwell’s Equations
� Source-less Maxwell’s Equations
� In most region of concern, we may have boundaries, but usually we do not have charges, or current
HjE ωµ−=×∇
EjH ωε=×∇
0=⋅∇ E
0=⋅∇ H
Homogeneous Wave Equation
� Homogeneous Wave Equation
� A result from source-less Maxwell’s Equation
� Free space
� No boundaries
� Plane waves are the eigenmodes
� Waveguide
� Boundary conditions
� Waveguide modes (e.g. COMSOL®)
022 =+∇ EkE 022 =+∇ HkH
Free space propagation
� Superposition of all plane waves
� Decompose the plane wave spectrum at z=0
� Add the propagation phase reaching z=z
� Sum all the plane wave components
( ) ( ) ( )∫∫
−−±+=
= βαβα βαβα ddeeEzyxE zkjyxj
z
222
0,,,
z=0z=z
(x,y)
k
kz
Fourier Transform relations
� Superposition of all plane waves
� At z=0
� Decompose the plane wave spectrum
� Spatial function E(x,y) and Spatial Spectrum function E(α,β) is a 2-D Fourier Transform Pair
( ) ( ) ( )∫∫
−−±+=
= βαβα βαβα ddeeEzyxE zkjyxj
z
222
0,,,
( ) ( ) ( )∫∫
+=
== βαβα βα ddeEzyxE yxj
z 0,0,,
( ) ( ) ( )∫∫
+−=
== dxdyezyxEE yxj
z
βα
πβα 0,,
4
1,
20
Use of Fourier Transform Tables
( ) ( ) ( )∫∫
+=
== βαβα βα ddeEzyxE yxj
z 0,0,,
� Be careful where to put 2π
( ) ( ) ( )∫∫
+−=
== dxdyezyxEE yxj
z
βα
πβα 0,,
4
1,
20
Limit of Imaging Resolution
� Visible part of spectrum
� Propagation modes, will reach the image plane
� Evanescent waves
� Will not reach the image plane
� Limit of Imaging Resolution� The finest detail that can be observed in an optical
image is limited by the highest spatial frequency in the planewave spectrum
� roughly equal to the wavelength of the light used to produce that image. (Why?)
� If near field evanescent waves is detected, better image resolution can be attained, e.g., Scanning near-field microscopy
0222 >−− βαk zkje222 βα −−±
0222 <−− βαk
Aperture stop
� The Fourier transform of a multiplication is a convolution
( ) ( ) ( )−+ === 0,,,0,, inctrans zyxEyxAzyxE
( ) ( ) ( ) βαβαββααβα ′′′′′−′−= ∫∫ ddEAE ,,, inctrans
• For a single plane wave incident
( ) ( )00inc ,, ββααδβα −−=E
( ) ( ) ( )( )00
00trans
,
,,,
ββαα
βαββααδββααβα
−−=
′′−′−′′−′−= ∫∫A
ddAE
Aperture stop
� A single plane wave incident on an aperture gives rise to an entire spectrum of plane waves, whose spectral contents are determined by the Fourier transform of the aperture function.
� Including both propagating modes and
� Evanescent waves, which are of paramount importance for super-resolution imaging.
( ) ( )00trans ,, ββααβα −−= AE
• For a single plane wave incident
( ) ( )00inc ,, ββααδβα −−=E
Thin Lens with finite size
� A finite size thin lens can be treated as the same size aperture stop followed by an ideal (infinitely large) thin lens.
� Each plane wave spectral component after the aperture stop focuses into a point at the back focal plane. (Why?)
� Where?
For the spectral component E(α,β), where is the focused point after a thin lens of focal length f?
Thin Lens with finite size
� A finite size thin lens can be treated as the same size aperture stop followed by an ideal (infinitely large) thin lens.
� Each plane wave spectral component after the aperture stop focuses into a point at the back focal plane. (Why?)
( ) ( ) 2
00trans ,, ββααεε −−=−− EyxI yx
0αε =f
k x0β
ε=
fk y
Thin Lens Imaging: Plane-Wave Spectrum method
� A source d0 distance away from the thin lens,
( ) ( ) ( ) βαβα βα ddeEyxE yxj +∫∫= ,, objobj
( ) ( ) 0222
,, objinc dkjeEE βαβαβα −−−=
At thin lens,
� Field distribution at the back focal plane
( ) ( ) ( ) 222220 1obj ,,, yxfjkfyfxjkd ee
f
ky
f
kxEfzyxE ++−−−−
==
� Field distribution at the back focal plane
( ) ( ) ( ) 222220 1obj ,,, yxfjkfyfxjkd ee
f
ky
f
kxEfzyxE ++−−−−
==
( ) ( ) ( )
( ) ( )( )22020
222220
2
1,
yxfdf
kfdk
yxfkfyfxkdyx
+−++−≈
++−−−−=φ
� Paraxial approximation
( ) ( ) ( )( )2202
0 2obj ,,,yxfd
f
kj
fdjk eef
ky
f
kxEfzyxE
+−+−
==
Back focal plane field and Paraxial Approximation
Lens Law: Plane-Wave Spectrum method
� Field distribution at the back focal plane
� Lens Law
( ) ( ) ( )( )2202
0 2obj ,,,yxfd
f
kj
fdjk eef
ky
f
kxEfzyxE
+−+−
==
( )( )22022
yxfdf
kj
e+−
is a quadratic phase front, will focus to a point
fd
fL
−=
0
2
away from the back focal plane.
or ( )( ) 20 ffdfdi =−−
which is the lens law. (compare to ).fdd i
111
0
=+
Spectrum at the image plane
� Field distribution at the back focal plane
( ) ( ) ( )( )2202
0 2obj ,,,yxfd
f
kj
fdjk eef
yk
f
xkEfzyxE
′+′−+−
′′==′′
kfd
x
i −′
=′−α
(x’,y’)(x,y)
f di
kfd
y
i −′
=′− β
• each point on the back focal planecorresponds to a specific direction,i.e., spectral content of image plane.
( )fzyxE =′′ ,, give rise to the spectrum of the image plane
Spectrum and field at the image plane
� Spectrum at image plane
( )
′′=′′
f
yk
f
xkEE ,, objβα k
fd
x
i −′
=′−α kfd
y
i −′
=′− β
recall at object plane f
yk
f
xk ′=
′= βα ,
therefore using the magnification factorf
fdM i −−=
′=
′=
ββ
αα
� Field at image plane
( ) ( ) ( )∫∫ ′′′′== ′+′ βαβα βα ddeEdzyxE ii yxj
iii ,,,
( ) ( ) ( )∫∫
+== βαβα βα ddeEM
dzyxE Myxjiii
ii,1
,, obj2
Image of extended objects
( )( ) ( )( ) ( )
i
iyx
d
kjyx
d
kj
i
jkd
ii dka
dkaJaee
d
eAyxPSF
iii
i
ρρπ
π1222
0 24
,222
020
0
+−+−−
=
� Point spread function (for circular lens)
� Field/Image at the image plane z=di
( )( )( ) ( )
( ) ( )00
1200
220
20
20
0
22
,24
, dydxdka
dkaJeyxEae
d
eAyxE
i
iyx
d
kjyx
d
kj
i
jkd
ii
iii
i
∫∫+−+−−
=ρρπ
π
( ) ( )20
20 MyyMxx ii +++=ρfor 0ddM i=
Image of extended objects
( ) ( ) ( ) 000000 ,,, dydxMyyMxxPSFyxOyxI iiii ∫∫ −−=
( )( )( ) ( )
( ) ( )00
1200
220
20
20
0
22
,24
, dydxdka
dkaJeyxEae
d
eAyxE
i
iyx
d
kjyx
d
kj
i
jkd
ii
iii
i
∫∫+−+−−
=ρρπ
π
( ) ( )20
20 MyyMxx ii +++=ρfor 0ddM i=
In general:
is a convolution of object field and the PSF in spatial domain,therefore in plane-wave spectral domain
( ) ( ) ( )βαβαβα ,,, PSFOI =
The Optical Transfer Function (OTF)
� For imaging with incoherent light source, the power PSF is
( ) ( ) 2,, yxPSFyxPPSF =
� Optical Transfer Function (OTF) is the Fourier transform of PPSF
( ) ( ) 2, .., yxPSFTFOTF =βα
for ( ) ( ) ( )∫∫
+= βαβα βα ddeyxPSFPSF yxj,,
( ) ( ) ( ) βαβαββααβα ′′′′′+′+= ∫∫ ddPSFPSFOTF ,,, *
is the complex autocorrelation of spectral domain PSF. (Why?)
The Modulation Transfer Function (MTF)
� MTF is the magnitude of OTF
( ) ( )βαβα ,, OTFMTF =
� Example: MTF of an ideal lens
( )yxA , ( ) ( )βαβα ,, PSFA =
Example: MTF of an ideal lens
( ) ( ) ( ) βαβαββααβα ′′′′′+′+= ∫∫ ddPSFPSFOTF ,,, *
( ) ( )
∆−∆−∆=
∆−∆−∆=
∆−==∆
−−2
122
12
222shaded
1cos2
1cos2
sin222
aaaa
aa
aa
aaaaAMTF
ππ
πφφπ
Example: MTF of an ideal lens
� Another way to calculate
( )( ) ( )( ) ( )
i
iyx
d
kjyx
d
kj
i
jkd
ii dka
dkaJaee
d
eAyxPSF
iii
i
ρρπ
π1222
0 24
,222
020
0
+−+−−
=
( ) ( ) ( )( )2
2122
2
022
4,
i
i
iii
dka
dkaJa
d
AyxPSF
ρρπ
π=
( ) ( ) ( )( )
( )yxj
i
i
i
edka
dkaJdda
d
AOTF βα
ρρϕρρπ
πβα +−
∫∫= 2
2122
2
0 24
,
( ) ( )( ) ( )∫∝ θρ
ρρρβα sin, 0
21 kJ
dka
dkaJdOTF
i
i
Figure-of-Merit (FOM) of Lens
� Lens FOM measures how well real lens approximates the ideal lens.
� phase front aberration
� PSF
� MTF
� Strehl ratio
� The ratio of the area under the MTF curve of the lens to that of an ideal lens.
� The ratio of the on-axis PPSF(x=0,y=0) of the lens to that of an ideal lens.
( ) PPSF .., TFOTF =βαsince
( ) ( ) βαβα ddOTFyx ∫∫=== ,0,0PPSF