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HANKEL TRANSFORMS

23

Thus, the 2-D FT of a circularly symmetric function is itself circularly symmetric and is given by Eq. (2.8-7). This relation is called the Hankel transform of zero order or the Fourier-Bessel transform.

It can be easily shown that the inverse Hankel transform of zero order is given by the same type of integral as

1

 

 

 

uðrÞ ¼ 2p ð0

UðrÞJ0ð2prrÞrdr

ð2:8-8Þ

 

 

 

 

EXAMPLE 2.5 Derive Eq. (2.8-5).

 

 

 

Solution: x, y and fx, fy are given by

 

 

 

x ¼ r cos y

 

y ¼ r sin y

 

fx ¼ r cos f

fy ¼ r sin f

 

Equation (2.8-2) becomes

2p

1

 

Uðr; fÞ ¼ ð0

dy ð0

uðr; yÞe j2prrðcos y cos fþsin y sin fÞJdr

where J is the Jacobian given by

 

 

@x

 

@x

 

 

 

 

 

 

 

@y

 

 

cos y

J

 

@r

 

 

 

 

 

@r

 

@y

 

 

 

 

 

 

 

 

 

 

 

 

@y

 

@y

 

sin y

 

¼

 

¼

 

 

 

 

 

 

 

 

r sin y ¼ r r cos y

ð2:8-9Þ

ð2:8-10Þ

where j j indicates determinant. Substituting J ¼ r in Eq. (2.8-9) gives the desired result.

EXAMPLE 2.6 (a) Find the Hankel transform of the cylinder function cylðrÞ defined by

 

 

 

1

0 r <

1

 

 

 

 

 

>

 

 

 

 

 

 

 

2

 

 

 

 

 

8

 

 

 

 

 

>

 

 

 

 

 

 

 

 

 

 

 

 

>

 

 

 

1

 

 

 

 

 

 

 

 

<

 

 

 

 

 

 

 

 

 

cyl r

Þ ¼

>

1

r

¼

1

 

ð

2:8-11

Þ

ð

>

2

 

2

 

 

 

 

>

 

 

 

 

 

 

 

 

 

 

 

 

>

 

 

 

 

 

 

 

 

 

 

 

 

>

 

 

 

 

 

 

 

 

 

 

 

 

>

 

 

 

 

 

 

 

 

 

 

 

 

:

 

 

 

 

 

 

 

 

 

 

 

 

>

0

r >

2

 

 

 

 

 

 

(b) Find the Hankel transform of cylðr=DÞ.


24 LINEAR SYSTEMS AND TRANSFORMS

Solution: (a) Let

uðrÞ ¼ cylðrÞ

Then

 

1

 

 

 

 

 

 

 

 

 

 

UðrÞ ¼ 2p ð uðrÞJ0ð2prrÞrdr

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

 

1=2

 

 

 

 

 

 

 

 

 

 

 

ð

 

 

 

 

 

 

 

 

 

 

¼ 2p J0ð2prrÞrdr

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

The Bessel function of the first kind of first order is given by [Erdelyi]

 

 

 

 

 

 

1=2

 

 

 

 

 

 

J1ðprÞ ¼ 4pr

ð0

J0ð2prrÞrdr

ð2:8-12Þ

Hence,

 

 

 

 

 

 

 

 

 

 

 

 

 

U

ðrÞ ¼

 

J1ðprÞ

 

 

 

 

 

 

 

 

2r

 

 

 

The sombrero function sombðrÞ is defined by

 

 

 

somb

r

Þ ¼

2J1ðprÞ

ð

2:8-13

Þ

 

pr

 

ð

 

 

 

UðrÞ is related to sombðrÞ by

 

 

p

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

UðrÞ ¼

 

sombðrÞ

 

 

 

4

 

 

 

(b) We have

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

D=2

 

 

 

 

 

 

 

U0ðrÞ ¼ 2p ð0

 

J0ð2prrÞrdr

 

 

 

Let r0 ¼ r=D. Then, dr ¼ Ddr0, and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1=2

 

 

 

 

 

 

 

 

 

U0ðrÞ ¼ 2pD2

 

ð0

 

r0J0ð2prDrÞdr0

 

 

 

2

 

 

 

 

 

 

 

D2p

 

 

 

¼ D UðrÞ ¼

 

 

sombðDrÞ

 

 

 

 

4

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 


3

Fundamentals of Wave Propagation

3.1INTRODUCTION

In this chapter and Chapter 4, waves are considered in 3-D, in general. However, in some applications such as in integrated optics in which propagation of waves on a surface is often considered, 2-D waves are of interest. For example, see Chapter 19 on dense wavelength division multiplexing. Two-dimensional equations are simpler because one of the space variables, say, y is omitted from the equations. Hence, the results discussed in 3-D in what follows can be easily reduced to the 2-D counterparts.

Electromagnetic (EM) waves will be of main concern. They are generated when a time-varying electric field Eðr; tÞ produces a time-varying field Hðr; tÞ. EM waves propagate through unguided media such as free space or air and in guided media such as an optical fiber or the medium between the earth’s surface and the ionosphere. In this chapter, we will be mainly concerned with unbounded media.

Spherical waves result when a source such as an antenna emits EM energy as shown in Figure 3.1(a). At a far away distance from the source, the spherical wave appears like a plane wave with uniform properties at all points of the wavefront, as seen in Figure 3.1(b). Another example would be an electric dipole directed along the z-axis, located at the origin, and oscillating with the circular frequency w. It generates electric and magnetic fields with a complicated expression, but far from the origin where the fields look like plane waves. A perfect plane wave does not exist physically, but it is a component that is very useful in modeling all kinds of waves.

Waves propagate in a medium. In the case of optical waves, the optical medium is characterized by a quantity n called the refractive index. It is the ratio of the speed of light in free space to that of the speed of light in the medium. The medium is homogeneous if n is constant, otherwise, it is inhomogeneous. In this chapter, we will assume that the medium is homogeneous.

The chapter consists of seven sections. How waves come about and some of their fundamental properties are discussed in Section 3.2. The fundamental properties of EM waves and the Kirchoff equations that characterize them are discussed in Section 3.3. The phasor representation is reviewed in Section 3.4. Wave equations,

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

Copyright # 2007 John Wiley & Sons, Inc.

25

26

FUNDAMENTALS OF WAVE PROPAGATION

Source

(a)

Propagation

Direction

(b)

Figure 3.1. (a) Spherical wave generated by a source; (b) plane wave with uniform properties along the direction of propagation.

the wave equation in a source free medium as well as the plane wave solution with wave number and direction cosines, are described in Section 3.5. Wave equations in phasor representation in a charge-free medium are discussed in Section 3.6. Plane waves are fundamental components of EM waves. They are described in more detail in Section 3.7, including their polarization properties.

3.2WAVES

Nature is rich in a large variety of waves, such as electromagnetic, acoustical, water, and brain waves. A wave can be considered as a disturbance of some kind that can travel with a fixed velocity and is unchanged in form from point to point.

Let uðx; tÞ denote a 1-D wave in the x-direction in a homogeneous medium. If v is its velocity, uðx; tÞ satisfies

uðx; tÞ ¼ uðx vt; 0Þ

ð3:2-1Þ

if it is traveling to the right and

uðx; tÞ ¼ uðx þ vt; 0Þ

ð3:2-2Þ

if it is traveling to the left.

Assuming the wave is traveling to the left, let s be given by

s ¼ x þ vt

ð3:2-3Þ


WAVES

27

Then, the following can be computed:

 

 

 

@u

¼

@u

 

 

 

 

 

 

 

@x

 

@s

 

 

 

 

 

 

 

 

 

 

 

@2u

¼

@2u

 

 

 

 

 

 

 

@x2

 

@s2

 

 

 

 

 

 

 

@u

 

@s @u

 

@u

 

 

 

 

¼

 

 

 

 

 

 

¼ v

 

 

 

 

 

@t

 

@t @s

@s

 

 

@2u

¼ v2

@2u

 

 

@t2

@s2

 

 

 

 

Hence,

 

 

 

 

 

 

 

 

 

 

 

 

 

@2uðx; tÞ

 

 

 

1 @2uðx; tÞ

 

 

 

@x2

 

¼

v2

 

 

@t2

ð3:2-4Þ

ð3:2-5Þ

This equation is known as the nondispersive wave equation. A particular solution, which is also a solution for all other wave equations, is the simple harmonic solution given by

x

ðx; tÞ ¼ A cosðkðx þ vtÞÞ ¼ A cosðkx þ wtÞ ¼ A cos 2p l þ ft ; ð3:2-6Þ

where o ¼ 2pf and k ¼ 2p=l. l is the wavelength, f is the time frequency, 1=l is the spatial frequency, and o and k are the corresponding angular frequencies. k is also known as the wave number. ðx; tÞ given by Eq. (3.2-6), is also known as the 1-D plane wave.

Because of mathematical ease, Eq. (3.2-6) is often written as

uðx; tÞ ¼ Re½AejðkxþotÞ&

ð3:2-7Þ

or simply as

 

 

 

 

 

 

u

x; t

Þ ¼

AejðkxþotÞ

ð

3:2-8

Þ

ð

 

 

 

‘‘real part’’ being understood from the content. We reassert that the wave number k is the radian spatial frequency along the x-direction. It can also be written as

k ¼ 2pfx

ð3:2-9Þ

where fx is the spatial frequency in the x-direction in cycles/unit length. Substituting Eq. (3.2-8) into Eq. (3.2-5) gives

v ¼

o

ð3:2-10Þ

k