Файл: Ersoy O.K. Diffraction, Fourier optics, and imaging (Wiley, 2006)(ISBN 0471238163)(427s) PEo .pdf
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FRESNEL DIFFRACTION BY A SINUSOIDAL AMPLITUDE GRATING |
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The FTs of f(x,y) and g(x,y) are given by
Fðfx; fyÞ ¼ 1 dðfx; fyÞ þ m ½dðfx þ f0; fyÞ þ dðfx f0; fyÞ&
2 4
Gðfx; fyÞ ¼ D2 sin cðDfxÞ sin cðDfyÞ
The FT of U(x,y,0) is the convolution of Fðfx; fyÞ with Gðfx; fyÞ:
Uðx; y; 0Þ $ Fðfx; fyÞ Gðfx; fyÞ
where |
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Fðfx; fyÞ Gðfx; fyÞ |
2 ðsin c½Dðfx þ f0Þ& þ sin c½Dðfx f0Þ&Þ |
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¼ 2 sin cðDfyÞnhsin cðDfxÞ þ |
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D2 |
m |
Then, the wave field at z is given by
ð5:7-7Þ
ð5:7-8Þ
ð5:7-9Þ
io
ð5:7-10Þ
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ejkz |
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k 2 |
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ÞFð fx; fyÞ Gð fx; fyÞ |
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Uðx0; y0; zÞ ¼ |
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ej |
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ðx0 |
þy0 |
ð5:7-11Þ |
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2z |
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jlz |
where fx ¼ x0=lz and fy ¼ y0=lz.
5.8 FRESNEL DIFFRACTION BY A SINUSOIDAL AMPLITUDE GRATING
In order to compute Fresnel diffraction by a sinusoidal amplitude grating, we can use the convolution form of the diffraction integral given by Eq. (5.2-8). The transfer function of the system is rewritten here as
Hðfx; fyÞ ¼ ejkze jplzðfx2þfy2Þ |
ð5:8-1Þ |
where ejkz can be suppressed as it is a constant phase factor.
The Fourier transform of the transmittance function is given by Eq. (5.7-9). In order to simplify the computations, we will assume that the diffraction grating aperture is large so that the Fourier transform of the transmittance function of the grating can be approximated by Eq. (5.7-7). Then, the frequencies that contribute are given by
ðfx; fyÞ ¼ ð0; 0Þ; ð f0; 0Þ; ðf0; 0Þ
The propagated wave has the following Fourier transform:
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m |
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Uðx0; y0; zÞ $ |
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dðfx; fyÞ þ |
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½e jplzf0 |
dðfx f0; fyÞ þ e jplzf0 |
dðfx þ f0; fyÞ& ð5:8-2Þ |
2 |
4 |
80 |
FRESNEL AND FRAUNHOFER APPROXIMATIONS |
The inverse Fourier transform yields
Uðx0; y0; zÞ ¼ 12 þ m4 e jplzf02 ½ej2pf0x0 þ e j2pf0x0 &
ð5:8-3Þ
¼ 12 ½1 þ m e jplzf 02 cosð2pf0x0Þ&
The intensity of the wave is given by
Iðx0; y0; zÞ ¼ |
1 |
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þ 2mcos plzf02 cosð2pf0x0Þ þ m2 cos2ð2pf0x0Þ |
ð5:8-4Þ |
4 |
EXAMPLE 5.11 Determine the intensity of the diffraction pattern at a distance z that satisfies
2n
z ¼ n integers
lf02
Solution: Iðx0; y0; zÞ is given by
Iðx0; y0; zÞ ¼ 14 ½1 þ mcosð2pf0x0Þ&2
This is the image of the grating. Such images are called Talbot images or selfimages.
EXAMPLE 5.12 Repeat the previous example if
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¼ |
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ð2n þ 1Þ |
n integer |
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lf02 |
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Solution: Iðx0; y0; zÞ is given by
Iðx0; y0; zÞ ¼ 14 ½1 mcosð2pf0x0Þ&2
This is the image of the grating with a 180 spatial phase shift, referred to as contrast reversal. Such images are also called Talbot images.
FRAUNHOFER DIFFRACTION WITH A SINUSOIDAL PHASE GRATING |
81 |
EXAMPLE 5.13 Repeat the previous example if
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¼ |
2n 1 |
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n integer |
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2lf02 |
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Solution: Iðx0; y0; zÞ is given by |
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1 |
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m2 |
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m2 |
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Iðx0; y0; zÞ ¼ |
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1 þ |
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þ |
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cosð4pf0x0Þ |
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4 |
2 |
2 |
This is the image of the grating at twice the frequency, namely, 2f0. Such images are called Talbot subimages.
5.9 FRAUNHOFER DIFFRACTION WITH A SINUSOIDAL PHASE GRATING
As with the sinusoidal amplitude grating, with an incident plane wave on the grating, the transmission function for a sinusodial phase grating is given by
m |
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y |
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Uðx; y; 0Þ ¼ ej2 sinð2pf0xÞrect |
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rect |
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ð5:9-1Þ |
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D |
D |
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U(x,y,0) can be written as |
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Uðx; y; 0Þ ¼ f ðx; yÞgðx; yÞ |
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ð5:9-2Þ |
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where |
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f ðx; yÞ ¼ ejm2 sinð2pf0xÞ |
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ð5:9-3Þ |
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x |
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y |
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gðx; yÞ ¼ rect |
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rect |
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ð5:9-4Þ |
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D |
D |
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The analysis can be simplified by use of the following identity:
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X |
m |
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ej2pf0kx |
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ej |
2 sinð2pf0xÞ ¼ k¼ 1 Jk |
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ð5:9-5Þ |
where Jkð Þ is the Bessel function of the first kind of order k. Using the above identity, the FT of f(x,y) is given by
X |
m |
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dð fx kf0; fyÞ |
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Fðfx; fyÞ ¼ k¼ 1 Jk |
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ð5:9-6Þ |
82 FRESNEL AND FRAUNHOFER APPROXIMATIONS
The FT of U(x,y,0) is given by |
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Uðx; y; 0Þ $ Fðfx; fyÞ Gðfx; fyÞ |
ð5:9-7Þ |
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where |
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X |
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m |
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sinc½Dðfx kf0Þ& sincðDfyÞ |
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Fðfx1; fyÞ Gðfx; fyÞ ¼ D2 k¼ 1 Jk |
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ð5:9-8Þ |
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Then, |
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ejkz |
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k |
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2 |
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Uðx0; y0; zÞ ¼ |
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ej |
2z |
ðx0þy0ÞFð fx; fyÞ Gð fx; fyÞ |
ð5:9-9Þ |
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jlz |
It is observed that sinusoidal amplitude grating in Section 5.7 has three orders of energy concentration due to three sin c functions, which do not significantly overlap if the grating frequency is much greater than 2/D. In contrast, the sinusoidal phase grating has many orders of energy concentration. Whereas the central order is dominant in the amplitude grating, the central order may vanish in the phase grating when J0ðm=2Þ equals 0.
5.10DIFFRACTION GRATINGS MADE OF SLITS
Sometimes diffraction gratings are made of slits. A two-slit example is shown in Figure 5.9, where b is the slit width, and f is the diffraction angle as shown in this figure.
The intensity of the wave field coming from the grating in the Fraunhofer region can be shown to be
I |
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2I |
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sinðkbf=2Þ |
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2 |
1 |
cos |
k |
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kd |
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5:10-1 |
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ðfÞ ¼ |
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þ |
fÞ& |
ð |
Þ |
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kbf=2 |
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0 |
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½ þ |
ð |
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d
b b
φ
Figure 5.9. A two-slit diffraction grating.
DIFFRACTION GRATINGS MADE OF SLITS |
83 |
where is the difference of the optical path lengths between the rays of two adjacent slits and I0 is the initial intensity of the beam.
When there are N parallel slits, the intensity in the Fraunhofer region can be shown to be
I |
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2I |
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sinðkbf=2Þ |
2 |
sinðNkdf=2Þ |
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2 |
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5:10-2 |
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ðfÞ ¼ |
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ð |
Þ |
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kbf=2 |
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sinðkdf=2Þ |
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The second factor above equals N cosðpNmÞ= cosðpmÞ when the grating equation d sin f ¼ ml is satisfied.
6
Inverse Diffraction
6.1INTRODUCTION
Inverse diffraction involves recovery of the image of an object whose diffraction pattern is measured, for example, on a plane. In the case of the Fresnel and Fraunhofer approximations, the inversion is straightforward. In the very near field, the angular spectrum representation can be used, but then there are some technical issues that need to be addressed.
The geometry to be used in the following sections is shown in Figure 6.1. The observation plane and the measurement plane are assumed to be at z ¼ z0 and z ¼ zr, respectively. Previously, zr was chosen equal to 0. The distance between the two planes is denoted by z0r. The medium is assumed to be homogeneous. The problem is to determine the field at z ¼ z0, assuming it is known at z ¼ zr.
Like all inverse problems, the inverse diffraction problem is actually difficult if evanescent waves are to be incorporated into the solution [Vesperinas, 1991]. Then, the inverse diffraction problem involves a singular kernel [Shewell, Wolf, 1968]. When the evanescent waves are avoided as discussed in the succeeding sections, the problem is well behaved.
This chapter consists of four sections. Section 2 is on inversion of the Fresnel and Fraunhofer approximations. Section 6.3 describes the inversion of the angular spectrum representation. Section 6.4 discusses further analysis of the results of Section 6.3.
6.2 INVERSION OF THE FRESNEL AND FRAUNHOFER REPRESENTATIONS
The Fresnel diffraction is governed by Eq. (5.2-13). As the integral is a Fourier transform, its inversion is given by
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je jkz0r |
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k |
2 |
2 |
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1 1 |
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k |
2 |
2 |
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2p |
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Uðx; y; zrÞ ¼ |
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e j |
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ðx |
þy |
Þ |
ð ð |
Uðx0; y0; z0Þe j |
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ðx0 |
þy0 |
Þej |
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ðx0xþy0yÞdx0dy0 |
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2z0r |
2z0r |
lz0r |
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lz |
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1 1 |
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ð6:2-1Þ
Diffraction, Fourier Optics and Imaging, by Okan K. Ersoy
Copyright # 2007 John Wiley & Sons, Inc.
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