Файл: Ersoy O.K. Diffraction, Fourier optics, and imaging (Wiley, 2006)(ISBN 0471238163)(427s) PEo .pdf

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MATRIX REPRESENTATION OF MERIDIONAL RAYS

129

(b) y2 and y1 are related by

y1

y2 ¼ f þ myy1

When y1 equals zero, we get

y2 ¼ myy1

Hence, my is the magnification factor of angles of rays starting from and converging to the optical axis.

EXAMPLE 8.13 Consider a positive lens. A parallel ray bundle that passes through the lens converges to a focused point behind the lens. This point is called the rear focal point or the second focal point of the lens. The plane passing through the rear focal point and perpendicular to the optical axis is called the rear focal plane or the second focal plane.

Consider the point in front of a positive lens such that the rays emerging from the point become a parallel bundle once they pass through the lens. This point is called the front focal point or the first focal point of the lens. The focal points and focal planes are visualized in Figures 8.17 and 8.18.

Figure 8.17. The rear focal point and the rear focal plane of a positive lens.

Figure 8.18. The front focal point and the front focal plane of a positive lens. Determine the ray-transfer matrix between the front and rear focal planes of a positive lens.

130

 

GEOMETRICAL OPTICS

 

 

 

Rear Focal Plane

Figure 8.19. The rear focal point and the rear focal plane of a negative lens.

Front Focal

Point

Front Focal Plane

Figure 8.20. The front focal point and the front focal plane of a negative lens.

Solution: In this case, d1 and d2 equal f. Hence, M becomes

 

 

 

 

 

2

 

d

 

 

 

d d

2

3

 

 

 

 

 

 

 

 

 

1

2

 

 

d1 þ d2

1

 

01

 

f

 

 

M

 

f

f

 

 

 

8:6-9

 

¼

6

 

f

1

f

 

7

¼

4

 

 

0

5

ð Þ

 

 

 

 

 

 

6

1

 

d1

7

2 f

3

 

 

4

 

 

 

 

 

 

 

 

5

 

 

 

 

 

 

 

EXAMPLE 8.14 The focal points and focal planes of a negative lens can be similarly defined. This is shown in Figures 8.19 and 8.20.

Note that the front and rear focal points and focal planes are the reverse of the front and rear focal points and focal planes of a positive lens. The ray-transfer matrix between the two planes can be shown to be also given by Eq. (8.6-9).

8.7THICK LENSES

A thick lens can be analyzed just like a thin lens by defining two principal planes. Consider the front focal point of a thick lens as shown in Figure 8.21. By definition, the rays emerging from this point exit the lens as a parallel bundle. An incident ray on the lens intersect with the existing ray from the lens projected backwards at a


THICK LENSES

131

Figure 8.21. (a) P1: first principal plane, (b) P2: second principal plane.

certain point. The plane passing through this point and perpendicular to the optical axis is called the first principal plane.

By definition, a parallel bundle of rays passing through a lens converge to the second focal point of the lens. An incident ray on the lens projected forward into the lens intersect the ray emerging towards the second focal point of the lens at a certain point. The plane passing through this point and perpendicular to the optical axis is called the second principle plane.

The ray-transfer matrix between the two principle planes of a thick lens can be shown to be the same as the regular ray-transfer matrix, namely,

 

2

1 1

0

3

M ¼

1

 

 

f

 

4

 

5

Consequently, the focal points, the focal length, and the imaging distances are as shown in Figure 8.22. The focal length is defined as the distance of a principle plane from the corresponding focal point. The two focal lengths are the same.

Figure 8.22. Object, image, principal and focal planes, focal lengths, and object and image distances in a thick lens.

132 GEOMETRICAL OPTICS

EXAMPLE 8.15 Show that the distances d1 and d2 between two conjugate planes satisfy the lens law.

Solution: The ray-transfer matrix between the two planes is given by

 

 

 

2

1

 

f

0

3

 

 

M ¼

1 d

 

 

1

1

 

1 d

0 12

 

 

 

0 11

 

 

 

4

 

 

 

 

5

 

 

This is the same ray-transfer matrix discussed in Example 8.11. Hence, the imaging condition is given by

1 ¼ 1 þ 1 f d1 d2

8.8 ENTRANCE AND EXIT PUPILS OF AN OPTICAL SYSTEM

An optical system typically contains a number of physical apertures. One of these apertures causes the most severe limitation for the system. It will be called the effective physical aperture.

Entrance and

Exit Pupils

(a)

Entrance Pupil

Exit Pupil

(b)

Exit Pupil

(c)

Figure 8.23. (a) Entrance pupil ¼ exit pupil, (b) Exit pupil ¼ physical pupil, (c) Entrance pupil ¼ exit pupil.


ENTRANCE AND EXIT PUPILS OF AN OPTICAL SYSTEM

133

The entrance pupil of the system is the image of the effective physical aperture when looking from the object space. The exit pupil of the system is the image of the effective physical aperture when looking from the image space.

In order to clarify these concepts, consider Figure 8.23. In part (a), the effective physical aperture is on the plane of the lens. In this case, the entrance and exit pupils coincide, and are the same as the effective physical aperture. In part (b), the effective physical aperture is the same as the exit pupil. Its image seen from the object side is a virtual image, which is the entrance pupil. In part (c), the effective physical aperture is the same as the entrance pupil. Its image seen from the image space is a virtual image, which is the exit pupil.

In considering diffraction effects, it is the exit pupil that effectively limits the wave field passing through the optical system. As far as diffraction is concerned, the lens system has the exit pupil as its aperture, and Fraunhofer diffraction can be used to study diffraction effects on the image plane. For this purpose, the distance on the optical axis is the distance from the exit pupil to the image plane.

9

Fourier Transforms and Imaging with Coherent Optical Systems

9.1INTRODUCTION

In this chapter, the uses of lenses to form the Fourier transform or the image of an incoming coherent wave are discussed. Both issues are discussed from the point of view of diffraction.

Imaging can also be discussed from the point of view of geometrical optics using rays as discussed in Chapter 8. The results obtained with diffraction are totally consistent with those of geometrical optics.

This chapter consists of seven sections. Section 9.2 discusses phase transformation with a thin lens, using its physical geometry. The phase function obtained is used in Section 9.3 to show how lenses form an output field, which is related to the Fourier transform of the input field in various geometries. This leads to the linear filtering interpretation of imaging in Section 9.4.

The theory discussed up to this point is illustrated with phase contrast microscopy in Section 9.5 and scanning confocal microscopy in Section 9.6. The last section highlights operator algebra for complex optical systems.

9.2PHASE TRANSFORMATION WITH A THIN LENS

A lens consists of an optically dense material in which the phase velocity is less than the velocity in air. The thickness of the lens is modulated so that a desired phase modulation is achieved at the aperture of the lens.

A thin lens has three important parameters: n, the material index of refraction by which factor the phase velocity is reduced, R1 and R2, which are the radii of the two circular faces of the lens, as shown in Figure 9.1. If the material is glass, n is approximately 1.5. By convention, as rays travel from left to right, each convex surface hit by rays has positive radius of curvature and each concave surface has

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

Copyright # 2007 John Wiley & Sons, Inc.

134

PHASE TRANSFORMATION WITH A THIN LENS

135

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 9.1. The three parts of a thin lens.

negative radius of curvature. A thin lens has the property that a ray enters and exits the lens at about the same (x,y) coordinates.

The three parameters discussed about can be combined in a single parameter called f, the focal length, by

f ¼

ðn 1Þ R1

R2

ð9:2-1Þ

 

1

1

 

1

f is positive or negative, depending on R1 and R2. For example, a double-convex lens has positive f whereas a double-concave lens has negative f. In the following discussion, f will be assumed to be positive.

The phase transformation of a perfect lens can be written as

tðx; yÞ ¼ ejkt0 e j

k

ðx2þy2Þ

ð9:2-2Þ

2f

where t0 is the maximum thickness of the lens. Since ejkt0 gives a constant phase change, it can be neglected. Equation (9.2-2) will be derived below. The finite extent of the lens aperture can be taken into account by defining a pupil function P(x,y):

Pðx; yÞ ¼

1

inside the lens aperture

ð9:2-3Þ

0

otherwise

In order to drive Eq. (9.2-2), the lens is considered in three parts as shown in Figure 9.1. The thickness ðx; yÞ at a location (x,y) can be shown to be [Goodman, 2004]

 

 

 

 

 

 

"

 

s #

 

 

 

"

 

s #

 

 

 

 

x; y

t

 

R

 

1

 

1

 

 

x2 þ y2

þ

R

 

1

 

1

 

x2 þ y2

ð

9:2-4

Þ

 

R12

 

R22

ð

 

Þ ¼ 0

 

1

 

 

 

 

2

 

 

 

where t0 is the total thickness of the lens. This expression is simplified by using paraxial approximation stated by

si

 

 

 

 

 

i

ð

 

Þ

1

 

x2 þ y2

 

1

 

x2

þ y2

 

9:2-5

 

R

 

 

 

2R2

 

 

 

 

 

 

 

 

 

 


136 FOURIER TRANSFORMS AND IMAGING WITH COHERENT OPTICAL SYSTEMS

where Ri is R1 or R2. Then, the thickness function becomes

 

 

 

x; y

 

t

 

x2 þ y2

 

1

 

1

 

 

9:2-6

 

Þ ¼

0

 

 

 

R1

R2

ð

Þ

ð

 

2

 

 

The phase transformation yðx; yÞ by the lens is expressed as

 

 

 

yðx; yÞ ¼ kn ðx; yÞ þ kðt0 ðx; yÞÞ

ð9:2-7Þ

¼ kt0 þ kðn 1Þ ðx; yÞ

 

 

 

Using Eqs. (9.2-1) and (9.2-6), Eq. (9.2-7) becomes

 

 

 

 

 

 

 

 

k

 

 

 

 

 

 

 

 

yðx; yÞ ¼ kt0

 

ðx2 þ y2Þ

ð9:2-8Þ

2f

Equation (9.2-8) leads to Eq. (9.2-2).

9.3FOURIER TRANSFORMS WITH LENSES

In Section 5.4, the Fraunhofer region was observed to be very far from the initial plane for reasonable aperture sizes. This limitation is removed with the use of a lens. Three separate cases will be discussed depending upon whether the initial wave field is incident on the lens, in front of the lens or behind the lens.

9.3.1Wave Field Incident on the Lens

This geometry is shown in Figure 9.2.

Suppose the wave field incident on the lens is U(x, y, 0). The wave field behind the lens becomes

U0ðx; y; 0Þ ¼ Uðx; y; 0ÞPðx; yÞe j

k

ðx2þy2Þ

ð9:3-1Þ

2f

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 9.2. The geometry for input placed against the lens.


FOURIER TRANSFORMS WITH LENSES

137

This complex amplitude can be substituted in Eq. (5.2-13), the Fresnel diffraction formula, to find the wave field at z ¼ f , the focal plane. If the focal plane coordinates are ðxf ; yf ; f Þ, the result is given by

Uðxf ; yf ; f Þ ¼ e j 2kf ðxf2þyf2Þ ðð U0

ðx; y; 0ÞPðx; yÞe j2pðfxxþfyyÞdxdy

ð9:3-2Þ

1

 

 

 

 

1

 

 

 

 

where constant terms are neglected, and the

spatial

frequencies are fx ¼ xf =lf ,

fy ¼ xf =lf . Equation (9.3-2) shows

that the

output

complex amplitude

is the

Fraunhofer diffraction pattern of the input complex amplitude within the pupil function of the lens.

9.3.2Wave Field to the Left of the Lens

This geometry is shown in Figure 9.3.

Consider Uðx1; y1; d1Þ, a wave field at the plane z ¼ d1, d1 > 0. Its angular spectrum Aðfx; fy; d1Þ and the angular spectrum Aðfx; fy; 0 Þ of U(x, y, 0) are related by

Aðfx; fy; 0 Þ ¼ Aðfx; fy; d1Þe jpld1ðfx2þfy2Þ

ð9:3-3Þ

If U(x, y, 0) has an extent less than the extent of P(x,y), Eq. (9.3-2) can be

written as

 

Uðxf ; yf ; f Þ ¼ Aðfx; fy; 0Þe j

k

ðxf2þyf2Þ

ð9:3-4Þ

2f

or, using Eq. (9.3-3),

 

Uðxf ; yf ; f Þ ¼ Aðfx; fy; d1Þe j

k

ð1

d1

Þðxf2þyf2Þ

ð9:3-5Þ

2f

f

When d1 ¼ f > 0, the phase factor becomes unity such that

 

 

Uðxf ; yf ; f Þ ¼ Að fx; fy; f Þ

ð9:3-6Þ

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Figure 9.3. The geometry for input placed to the left of the lens.