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B¨ornstein-Landolt

VIII/1A1 Series New

Table 3.1.4 continued.

Integrals

Formula

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Restrictions

Ref.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Fraunhofer

EFra(x, y, z) =

i exp (i kz) p

A

E(x , y , 0) exp

 

i 2π

xx + yy

d x

d y

(3.1.40)

a2

1

[99Bor]

far-field

λ z

λd

[68Goo]

 

 

 

 

 

λz

 

 

 

 

 

 

 

 

 

 

approximation,

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

[96For]

refers to

with the additional phase term

 

 

 

 

 

 

 

 

 

 

 

[97For]

Fig. 3.1.8

 

 

 

 

 

 

 

 

 

 

 

[86Sta]

p =

 

 

 

 

 

 

 

 

 

b2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

2

λ z

2

 

for

 

λz

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

i π x

 

+ y

 

otherwise

 

 

 

 

 

 

 

 

 

 

exp

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Plane-wave representation (also: angular-spectrum representation), refers to

Figs. 3.1.8 and 3.1.9

2-D Fourier transform (see remark on (3.1.40)) of the source distribution Es in plane z = 0:

rSP > λ0

[91Sal]

A0(fx, fy ) =

 

∞ ∞

Es(x , y , 0) exp

i 2 π (fxx

+ fy y

)

d x d y

,

 

 

 

 

 

(3.1.41)

[78Loh]

 

 

 

 

 

 

 

[97For]

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

[86Sta]

 

 

−∞ −∞

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

[99Bor]

propagation of plane waves with the spatial frequencies fx and fy along the z-direction by distance z:

 

exp {−i 2 π (fxx + fy y} exp i 2 π (fxx + fy y +

 

12 − fx2 − fy2 z) ,

 

 

 

(3.1.42)

 

addition of plane waves at distance z:

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

E(x, y, z) 2

2

0 x y

x

 

y

 

 

x y

x

y

 

 

fx

+fy

<1

A (f , f ) exp

 

i 2 π

f x + f y +

 

f 2 f 2 z

d f

d f

,

(3.1.43)

 

=

 

 

 

 

 

12

 

 

equivalent to (3.1.34) [97For]

Far field in the focal plane of a lens, refers to

Fig. 3.1.9

EP(x, y) = λf

 

∞ ∞

ES(x , y ) exp

i 2 π λf

x

+ λf y dx

dy

,

 

 

 

i p

 

 

 

 

 

 

 

x

 

 

y

 

 

 

 

 

−∞ −∞

 

 

 

 

 

 

 

 

 

 

 

 

 

(x

2

+

y2) (d

 

f )

 

 

 

 

 

 

 

 

p = exp i π

 

 

 

 

 

 

 

 

 

 

 

 

 

 

λ f 2

 

 

 

 

 

 

 

 

d, f λ

[91Sal]

(3.1.44)

(3.1.45)

131] .p .Ref

optics Linear 1.3

87


88

 

 

3.1.4 Di raction

 

 

[Ref. p. 131

x

Plane wave

 

x

Field ES (x’,y’)

Lens

x

 

 

 

 

Plane wave

 

Convergent wave

 

 

 

 

 

 

z

 

x

= sin

1

 

 

Field EP (x,y)

 

x

 

 

 

 

 

 

d

 

f

x = 1/fx

 

 

z

 

 

 

 

 

 

a

 

 

b

 

 

 

Fig. 3.1.9. (a) Spatial frequencies of a plane wave with propagation direction Θx with respect to the

plane x = 0 (and Θy analogously) are fx and fy with Θx = sin1(λfx) ≈ λfx and Θy = sin1(λfy ) ≈ λfy

(: paraxial approximation). (b) Generation of the far field in the focal plane of a lens: The Fourier

transformation (d = f ) is changed by an additional phase term for d = f with d: distance, f : focal length.

(3.1.40): Fraunhofer’s approximation

Fresnel number :

NF = a2/λz .

(3.1.46)

Validity of Fraunhofer’s approximation: NF 1 .

p = 1 (parabolic phase): the intensity of di racted light is the square of the modulus of the Fourier transform of E(x, y, 0) only.

– Additional condition with second Fresnel number NF = b2/λz 1 :

E(x, y, z) is the Fourier transform of E(x, y, 0) in dependence on the spatial frequencies fx (x/z)/λ ≈ Θxand fy (y/z)/λ ≈ Θy .

Di erent conventions on the spatial Fourier transform F (fx) of a spatial distribution f (x) :

The convention of the plane-wave structure exp(i kx − i ω t) is connected with the determination of F (fx) by

F (fx) = d x f (x) ei 2π fxx

−∞

[68Goo, 68Pap, 78Loh, 78Gas, 93Sto, 05Hod].

– The plane-wave structure exp(i ω t − i kx) can be combined with

F (fx) = d x f (x) ei 2π fxx

−∞

[71Col, 73Men, 92Lug], but

F (fx) = d x f (x) ei 2π fxx

−∞

is defined also in [88Kle, 91Sal, 95Wil, 96Ped].

Landolt-B¨ornstein

New Series VIII/1A1


Ref. p. 131]

3.1 Linear optics

89

 

 

 

Di erent approximations in (3.1.37) and (3.1.38):

rSP ≈ r0 + 2xξ − ξ2 + 2yη − η2

2r0

[99Bor, 68Pap, 78Gra] with r0 from Fig. 3.1.8 versus

rSP ≈ z + 2xx − x 2 + 2yy − y 2

2z

(references on lasers: [86Sie, 05Hod], optoelectronics: [68Goo, 72Mar, 91Sal]) for grating di raction: The sine of the di raction angle sin Θx = x/r0 is derived from principle and not by a postpositive reasoning of the paraxial range x/z = tan Θx sin Θx. x/z should be “translated” into sin Θx for better approximation.

(3.1.41)–(3.1.43): Plane-wave spectrum or angular-spectrum representation (also Rayleigh- Sommerfeld-Debye di raction theory) [78Loh, 99Pau] is the plane-wave formulation of (3.1.34) [78Loh, 97For]. Application: see Fourier optics [68Goo, 83Ste, 93Sto].

(3.1.44), (3.1.45): Generation of the far field in the focal plane of a lens: d = f (object is outside the object-side focal plane) additional phase term p to the pure (inverse) Fourier transform (d = f ), similarly to (3.1.40).

Applications: generation of the spectrum of a function, possibility of mathematical operations in the Fourier-space with complex filtering masks, correlation and convolution.

Another important di raction theory

Di raction theory after Young, Maggi, Rubinowicz [66Rub, 99Pau]: The light in point P of Fig. 3.1.8 results from the unperturbed light and local waves, which are emitted by the edge of the aperture A. Therefore, a line integral is to be calculated [99Pau]. There is an equivalence with Fresnel-Kirchho ’s theory.

3.1.4.3 Time-dependent di raction theory

Two formulations of the time-dependent treatment of di raction are possible:

1.A general Fresnel-Kirchho ’s integral formula exists for time-dependent source functions in the aperture A, see [99Bor, 99Pau].

2.Used more often now [96Die, 99Pau]: The time-dependent source functions are decomposed into a superposition of monochromatic fields. The di racted field is calculated for every monochromatic component by the stationary di raction given above. The superposition of all di racted monochromatic components yields the time-dependent di racted field.

3.1.4.4 Fraunhofer di raction patterns

3.1.4.4.1 Rectangular aperture with dimensions 2a × 2b

In Fig. 3.1.10 the geometry of the di raction from a rectangular aperture 2a × 2b is shown. The x-part of the di raction pattern in Fig. 3.1.10 is given in Fig. 3.1.11. In Table 3.1.5 the zeros and maxima of the intensity distribution are listed.

Landolt-B¨ornstein

New Series VIII/1A1



90

 

 

3.1.4 Di raction

 

 

 

[Ref. p. 131

x ’

 

 

 

 

 

1.0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

x

 

intensity/

0.8

 

 

 

 

 

 

 

x

y

Normalized intensity

 

 

 

y ’

 

0.6

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

a

x

 

 

 

field

0.4

 

Normalized field

 

 

~ sin

 

 

 

 

 

 

z

 

 

Normalized

0.2

 

 

 

 

b

 

z

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Opaque screen

 

z

 

 

 

 

 

 

 

 

 

0

FWHM

 

 

 

 

 

 

 

 

 

 

 

 

 

Rectangular

 

Diffraction

 

 

0.2

 

 

 

 

 

 

pattern

 

 

 

 

 

 

 

 

aperture A

 

 

 

0

0.5

1.0

1.5

2.0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

x a/( d )

 

 

Fig. 3.1.10. Geometry of the di raction from a rectangular aperture 2a × 2b.

Fig. 3.1.11. x-part of the di raction pattern in Fig. 3.1.10. This is the di raction pattern of a slit. For more exact electromagnetic solutions of a slit see [61Hoe, p. 266].

Table 3.1.5. Zeros and maxima of the intensity distribution.

Number n

 

 

 

xa/λz

 

 

 

 

 

 

In/I0

 

 

 

 

 

 

 

 

 

0

 

 

 

0

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

FWHM

 

 

 

2 × 0.221

 

 

 

 

 

0.5

 

 

 

 

 

 

 

 

 

 

1

 

 

 

0.5

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

0.715

 

 

 

 

 

 

0.0472

 

 

 

 

 

 

 

 

 

2

 

 

 

1

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

1.230

 

 

 

 

 

 

0.0168

 

 

 

 

 

 

 

 

 

3

 

 

 

1.5

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

3

 

 

 

1.735

 

 

 

 

 

 

0.0083

 

 

 

 

 

 

 

 

 

4

 

 

 

2

 

 

 

 

 

 

 

0

 

 

 

 

 

 

 

 

 

 

 

4

 

 

 

2.239

 

 

 

 

 

 

0.0050

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Field distribution:

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

4 a b

E0 exp i k z

x2

+ y2

sinc

2 π a x

sinc

 

2 π b y

 

(3.1.47)

E(x, y, z) =

 

 

 

+

 

 

 

 

 

 

i λ z

 

2 z

 

λ z

λ z

with sinc(x) =

sin x

and

E0

the electric-field amplitude .

 

 

 

 

 

 

 

 

 

 

 

Intensity:

 

 

 

x

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

sinc2

 

 

.

 

 

 

 

 

 

 

I(x, y, z) = I(0, 0, z) sinc2

2

λ z

λ z

 

 

 

 

 

 

(3.1.48)

 

 

 

 

 

 

 

 

 

π a x

 

 

 

 

2 π b y

 

 

 

 

 

 

 

 

 

If the Fraunhofer di raction is observed in the focal plane, z has to be replaced by f .

3.1.4.4.2 Circular aperture with radius a

The circular aperture with radius a is discussed in [61Hoe, p. 453]. In Fig. 3.1.12 di raction by a circular aperture is shown. In Fig. 3.1.13a the di racted field and intensity and in Fig. 3.1.13b the encircled energy in the di raction plane with a circular screen are given. The zeros and maxima of intensity for di raction by a circular aperture are listed in Table 3.1.6.

Landolt-B¨ornstein

New Series VIII/1A1