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ANALYSIS

89

Interchanging orders of integration, this can be written as

 

 

 

 

Uðx; zrÞ ¼

ð

 

ð

dfx0ðe j2pfx0xejkz0r pk2 4p2fx02

 

 

 

 

1

2 M

 

 

 

 

 

1

4

M

 

 

 

 

 

 

 

Q

 

ej2pfxxe jz0r pk2 4p2fx2 2R sin c 2Rfx

 

3T x; zr dx

 

 

 

 

dfx

 

 

 

 

 

Q

 

Þ&Þ

7

ð

Þ

 

 

 

ð

½

ð

5

 

 

 

 

 

 

 

 

 

 

It is observed that the sin c function above mixes the plane wave components in the original object wave. This means that each plane wave component in the original object wave is truncated by the aperture (-R,R) and therefore ‘‘spreads’’ by diffraction.

EXAMPLE 6.2 When M ¼ Q ¼ 1=l, show that T ðx; zrÞ can be exactly recovered from Uðx0; z0Þ by forward propagation of U ðx0;z0Þ instead of inverse propagation. Solution: Suppose that forward propagation from the plane z ¼ z0 to z ¼ 2z0 zr is carried out. As

2z0 zr z0 ¼ z0r

the forward propagation equation is given by

 

 

 

 

Q

 

1

 

 

 

 

 

 

 

Q

 

1

 

 

 

Uðx; 2z0 zrÞ ¼

ð dfx

ð

 

U ðx0; z0Þe j2pfxx0 ejz0r pk2 4p2fx2 ej2pfxxdx0

 

Rearranging orders of integration results in

 

 

 

U x; 2z0

zr

2 Q

1 U x0; z0

 

ej2pfxx0 e jz0r pk2 4p2fx2 e j2pfxxdx03 dfx T

x; 0

ð

Þ ¼

6 Q 1

 

ð

 

Þ

 

7

¼ ð Þ

ð

ð

 

 

 

5

 

 

4

 

 

 

 

 

 

 

 

In other words, the original image can be reconstructed by back space propagation of the recorded wave or forward propagation of the complex conjugate of the recorded wave.


7

Wide-Angle Near and Far Field Approximations for Scalar Diffraction

7.1INTRODUCTION

Approximations for computing forward and inverse diffraction integrals are of vital significance in many areas involving wave propagation. As discussed in Chapters 4 and 5, approximations such as the Fresnel approximation, the Fraunhofer approximation, and the more rigorous angular spectrum method (ASM) all involve the Fourier transform, its discrete counterpart, the discrete Fourier transform, and its fast computational routine, the fast Fourier transform (FFT).

The Fresnel approximation is valid at reasonable distances from the input plane whereas the Fraunhofer approximation is valid in the far field. The ASM is a rigorous solution of the Helmholtz equation; its numerical implementation is usually done with the FFT, and possibly other digital signal processing algorithms, with their related approximations [Mellin and Nordin, 2001; Shen and Wang, 2006].

When the sizes of the diffracting apertures are less than the wavelength, scalar diffraction theory yields nonnegligible errors, and other numerical methods such as the finite difference time domain (FDTD) method and the finite element method (FEM) may become necessary to use [Kunz, 1993; Taflove and Hagness, 2005]. However, these methods are not practical with large scale simulations as compared with methods utilizing the FFT. With diffracting aperture sizes of the order of the wavelength used and in the near field, the ASM has been found to give satisfactory results [Mellin and Nordin, 2001]. With the ASM, one disadvantage is that the input and output plane sizes are the same. The output plane size is usually desired to be considerably larger than the input plane size in most applications, and this can be done with the ASM only by repeatedly using the ASM in short distances and additionally using filtering schemes to make the output size progressively larger.

The Fresnel, Fraunhofer approximations, and the ASM can be considered to be valid in practice at small angles of diffraction. It is desirable to have approximate methods that are valid at wide angles of diffraction in the near field as well as the far field and also based on the Fourier integral to be implemented with the FFT so that

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

Copyright # 2007 John Wiley & Sons, Inc.

90

A REVIEW OF FRESNEL AND FRAUNHOFER APPROXIMATIONS

91

large scale computations can be carried out in a reasonable amount of time and storage. Even if the spatial frequencies are sampled such that the FFT cannot be used, the Fourier integral representation is still desirable as it is separable in the two variables of integration, reducing 4-D tensor operations to 2-D matrix operations.

In this chapter, a new set of approximations having such features is discussed. The approximations are based on the Taylor expansion around the radial distance of a point on the output plane from the origin. With these approximations, what makes possible to utilize the FFT is semi-irregular sampling at the output plane. Semiirregular sampling means sampling is first done in a regular array, and the array points are subsequently perturbed to satisfy the FFT conditions.

Some interesting results will be related to the similarity of the proposed approximation to the Fresnel approximation even though the new approximation is valid in the near field and at wide angles whereas the Fresnel approximation is not. This is believed to be one reason why the Fresnel approximation has often been used in the near field in many applications. The results obtained in such studies are actually valid at the output sampling points perturbed in position, as discussed in this paper.

This chapter consists of eight sections. Section 7.2 is a review of Fresnel and Fraunhofer approximations previously discussed in Chapter 5. Section 7.3 introduces the new methods with the radial set of approximations. Section 7.4 provides further higher order improvements and error analysis. Section 7.5 shows how the method can be used in inverse diffraction and iterative optimization applications. Section 7.6 provides numerical simulation examples in 2-D and 3-D geometries. Section 7.7 is about how to increase accuracy by centering input and output plane apertures around some center coordinates and possibly also using smaller subareas in large scale simulations. Section 7.8 covers conclusions.

7.2 A REVIEW OF FRESNEL AND FRAUNHOFER APPROXIMATIONS

The first Rayleigh–Sommerfeld diffraction integral can be written as

Uðx; y; zÞ ¼ j1l

ðð

Uðx; y; 0Þ rz2 e jkrdxdy

ð7:2-1Þ

 

 

1

 

 

 

 

 

 

1

 

 

 

 

where Uðx; y; 0Þ is the input field, Uðx0; y0; zÞ is the output field, k is the wave number equal to 2p=l, l is the wavelength, and r is the radius vector length from the point ðx; y; 0Þ to the point ðx0; y0; zÞ. In general, z is often large enough to approximate z=r2 by 1=z. Then, Eq. (7.2-1) becomes

 

 

 

Uðx; y; zÞ ¼ jlz

ðð

Uðx; y; 0Þe jkrdxdy

ð7:2-2Þ

 

 

 

1

1

 

 

 

 

 

 

1

 

 

The constant term

1

 

will be neglected in the rest of the chapter.

 

jlz

 

 

 

 

 

 


92

WIDE-ANGLE NEAR AND FAR FIELD APPROXIMATIONS

In the Fresnel approximation commonly used in diffraction problems, the radius vector length is approximated by the Taylor’s series expansion with two terms [Mezouari and Harvery, 2003; Southwell, 1981; Steane and Rutt, 1989]:

q

 

 

þ

g

 

ð

 

Þ

r ¼ z2 þ ðx0 xÞ2 þ ðy0 yÞ2

 

z 1

 

2

 

 

7:2-3

 

where

 

 

 

 

 

 

 

 

 

 

g

¼

ðx0 xÞ2 þ ðy0 yÞ2

 

 

 

 

ð

7:2-4

Þ

 

z2

 

 

 

 

 

 

The magnitude of the maximum phase error Emax in radians is estimated by the next term in the Taylor series as

Emax

1

ð7:2-5Þ

8 zg2k

The Fresnel approximation is not sufficiently good in problems where Emax is larger than, say, 1 radian. However, this condition has often been relaxed in various applications because good results have been generally obtained. This was partially explained by using the method of stationary phase [Goodman]. In this chapter, another explanation for these results is provided.

The advantage in the Fresnel approximation is that the variables are separable so that the integral in Eq. (7.2-2) can be written as a Fourier integral. For example, Eq. (7.2-4) is rewritten as

g

¼

v w

2ðx0 x þ y0yÞ

 

z2

þ

z2

 

z2

where

v ¼ x20 þ y20

w ¼ x2 þ y2

ð7:2-6Þ

ð7:2-7Þ

ð7:2-8Þ

Then, with the help of Eq. (7.2-3), Eq. (7.2-2) can be approximated as a Fourier integral by

ðð

Uðx0; y0; zÞ ¼ e jk2vz u0ðx; yÞe jkz ðx0xþy0yÞdxdy ð7:2-9Þ

where

u0ðx; yÞ ¼ uðx; yÞe jk

w

ð7:2-10Þ

2z


THE RADIAL SET OF APPROXIMATIONS

93

Equation (7.2-9) becomes a Fourier integral by writing it as

ðð

Uðx0; y0; zÞ ¼ e jk2vz u0ðx; yÞe j2pðfxxþfyyÞdxdy

where the spatial frequencies fx and fy are defined by

fx ¼ xs lz

fy ¼ ys lz

where xs equals x0, and ys equals y0 at this point.

In the Fraunhofer approximation, the condition z w allows u0ðx; yÞ

that Eq. (7.2-9) becomes

 

Uðx0; y0; zÞ ¼ e jk2vz

ðð uðx; yÞe jkz ðx0xþy0yÞdxdy

ð7:2-11Þ

ð7:2-12Þ

ð7:2-13Þ

uðx; yÞ so

ð7:2-14Þ

Equation (7.2-9) can be evaluated with the fast Fourier transform [Brigham, 1974] by letting

xs ¼ mx 0x; ys ¼ my 0y;

x¼ nx x;

y¼ ny y;

lz

0x x ¼ Mx

0y y ¼ lz My

mx ¼ integer

ð7:2-15Þ

my ¼ integer

ð7:2-16Þ

nx ¼ integer

ð7:2-17Þ

ny ¼ integer

ð7:2-18Þ

 

ð7:2-19Þ

 

ð7:2-20Þ

where Mx and My are the number of samples in the x- and y-directions, respectively. In any other approximation, it is necessary to keep Eqs. (7.2-19) and (7.2-20) valid if FFT is to be used.

7.3THE RADIAL SET OF APPROXIMATIONS

In many applications such as those involving digital holography and diffractive optical elements, the coordinates ðx; y; 0Þ are usually much smaller than the object coordinates ðx0; y0; zÞ. Then, Eq. (7.2-3) will be written as

 

¼

 

ð

 

Þ

r

 

r0p1 þ h

 

7:3-1

 


94 WIDE-ANGLE NEAR AND FAR FIELD APPROXIMATIONS

where

¼ q

ð

 

Þ

 

 

r0

 

 

z2 þ x02 þ y02

 

7:3-2

 

h

 

w

 

2ðx0x þ y0yÞ

 

7:3-3

 

¼ r02

r02

ð

Þ

 

 

In order to be able to use the Fourier transform, Eq. (7.3-3) is to be approximated by

h

 

w

 

2ðx0x þ y0yÞ

7:3-4

 

¼ z2

r02

Þ

 

ð

The simplest radial set of approximations is obtained by approximating the radial distance r as

r

 

r

 

w2

 

xx0 þ yy0

7:3-5

 

0 þ

2z

 

Þ

 

 

r0

ð

Equations (7.3-4) and (7.3-5) are also valid when x; y; x0, and y0 are sufficiently smaller than z (sufficiency conditions will be more clear later). Equation (7.3-5) is further improved in the next section. In order to obtain a Fourier transform relationship with the diffraction integral given by Eq. (7.2-9 ), the following is defined:

x0 ¼

xs

r0

ð7:3-6Þ

z

y0 ¼

ys

r0

ð7:3-7Þ

z

where ðxs; ysÞ is the regular output sampling point. The simultaneous solution of Eqs. (7.3-6) and (7.3-7) is given by

 

 

 

 

 

x0 ¼ Cðxs; ysÞxs

 

 

 

ð7:3-8Þ

 

 

 

 

 

y0 ¼ Cðxs; ysÞys

 

 

 

ð7:3-9Þ

where

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

C

x

; y

sÞ ¼

1

 

xs2

þ ys2

 

21

ð

7:3-10

Þ

 

 

 

 

 

 

 

 

 

z2

 

 

 

 

ð

s

 

 

 

 

 

2

z

 

w as in the

Fraunhofer

approximation, the

term involving

When

 

w in Eq. (7.3-5) is skipped. The resulting approximations will be referred to as the near field approximation (NFA) and the far field approximation (FFA) below. The general case covering both NFA and FFA will be referred to as NFFA.