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FRESNEL DIFFRACTION BY A SINUSOIDAL AMPLITUDE GRATING

79

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

 

Fðfx; fyÞ Gðfx; fyÞ

2 ðsin c½Dðfx þ f0Þ& þ sin c½Dðfx f0Þ&Þ

¼ 2 sin cðDfyÞnhsin cðDfxÞ þ

 

D2

m

Then, the wave field at z is given by

ð5:7-7Þ

ð5:7-8Þ

ð5:7-9Þ

io

ð5:7-10Þ

 

ejkz

 

k 2

2

ÞFð fx; fyÞ Gð fx; fyÞ

 

Uðx0; y0; zÞ ¼

 

ej

 

ðx0

þy0

ð5:7-11Þ

 

2z

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:

 

1

 

m

2

2

 

Uðx0; y0; zÞ $

 

dðfx; fyÞ þ

 

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

1

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

z

¼

 

ð2n þ 1Þ

n integer

lf02

 

 

 

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

z

¼

2n 1

 

n integer

 

 

2lf02

 

 

 

 

Solution: Iðx0; y0; zÞ is given by

 

 

 

 

 

 

 

 

1

 

m2

 

m2

Iðx0; y0; zÞ ¼

 

1 þ

 

þ

 

cosð4pf0x0Þ

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

x

y

 

Uðx; y; 0Þ ¼ ej2 sinð2pf0xÞrect

 

rect

 

 

ð5:9-1Þ

D

D

U(x,y,0) can be written as

 

 

 

 

 

 

 

Uðx; y; 0Þ ¼ f ðx; yÞgðx; yÞ

 

 

ð5:9-2Þ

where

 

 

 

 

 

 

 

f ðx; yÞ ¼ ejm2 sinð2pf0xÞ

 

 

 

 

 

 

ð5:9-3Þ

 

x

 

 

y

 

 

 

gðx; yÞ ¼ rect

 

rect

 

 

 

 

ð5:9-4Þ

D

D

 

 

The analysis can be simplified by use of the following identity:

 

m

X

m

 

 

 

1

ej2pf0kx

 

ej

2 sinð2pf0xÞ ¼ k¼ 1 Jk

2

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

 

 

1

dð fx kf0; fyÞ

 

Fðfx; fyÞ ¼ k¼ 1 Jk

2

ð5:9-6Þ


82 FRESNEL AND FRAUNHOFER APPROXIMATIONS

The FT of U(x,y,0) is given by

 

 

 

 

 

 

 

 

Uðx; y; 0Þ $ Fðfx; fyÞ Gðfx; fyÞ

ð5:9-7Þ

where

 

 

 

 

 

 

 

 

X

 

 

 

m

 

 

 

1

 

 

 

sinc½Dðfx kf0Þ& sincðDfyÞ

 

Fðfx1; fyÞ Gðfx; fyÞ ¼ D2 k¼ 1 Jk

2

ð5:9-8Þ

Then,

 

 

 

 

 

 

 

 

 

 

ejkz

 

k

2

2

 

Uðx0; y0; zÞ ¼

 

 

ej

2z

ðx0þy0ÞFð fx; fyÞ Gð fx; fyÞ

ð5:9-9Þ

 

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

 

2I

 

 

sinðkbf=2Þ

 

2

1

cos

k

 

kd

 

 

5:10-1

 

ðfÞ ¼

 

 

þ

fÞ&

ð

Þ

 

kbf=2

 

 

 

0

 

½ þ

ð

 

 

 

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

 

2I

 

 

sinðkbf=2Þ

2

sinðNkdf=2Þ

 

2

 

5:10-2

 

ðfÞ ¼

 

 

ð

Þ

 

kbf=2

 

 

 

 

0

sinðkdf=2Þ

 

 

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

 

je jkz0r

 

k

2

2

 

1 1

 

k

2

2

 

2p

 

Uðx; y; zrÞ ¼

 

e j

 

ðx

þy

Þ

ð ð

Uðx0; y0; z0Þe j

 

ðx0

þy0

Þej

 

ðx0xþy0yÞdx0dy0

 

2z0r

2z0r

lz0r

lz

 

 

 

 

 

 

 

1 1

 

 

 

 

 

 

 

ð6:2-1Þ

Diffraction, Fourier Optics and Imaging, by Okan K. Ersoy

Copyright # 2007 John Wiley & Sons, Inc.

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