Download Propagation of waves

Fraunhofer Diffraction:
Multiple slits & Circular aperture
Mon. Nov. 25, 2002
1
Diffraction from an array of N slits, separated by a distance a and of width b
y=(N-1)a + b

y=(N-1)a
y=3a+b
y=3a
y=2a+b
y=2a
y=a+b
y=a

P


a
y=b
y=0

2
Diffraction from an array of N slits

It can be shown that,
 sin 
I P  I o 
 

where,
b
  k sin 
2
2
  sin N 
 

  sin  
2
a
  k sin 
2
3
Diffraction and interference for N slits
The diffraction term
 Minima for sin  = 0
  = p = k(b/2)sin 
 or, sin = p(/b)
The interference term
 Amplitude due to N coherent
sources
 Can see this by adding N phasors
that are 2 out of phase. See
Hecht Problem 10.2
sin 

sin N
Io
sin 
4
Interference term
Maxima occur at  = m (m = 0,1, 2, 3, ..)
 To see this use L’Hopital’s rule _______
 Thus maxima occur at sin  = m/a
 This is the same result we have derived
for Young’s double slit
 Intensity of principal maxima, I = N2Io
 i.e. N times that due to one slit

5
Interference term

Minima occur for  = /N, 2/N, … (N-1)/N

and when we add m
For example, _______________________
Thus principal maxima have a width determined
by zeros on each side
Since  = (/)a sin  = /N
The angular width is determined by




sin  = /(Na)

Thus peaks are N times narrower than in a
single slit pattern (also a > b)
6
Interference term





Subsidiary or Secondary Maximum
Now between zeros must have secondary
maxima
Assume these are approximately midway
sin N
2N

Then first at [ m+3/(2N) ]
sin 
3
Then it can be shown that
 4  2
I 
N I o  0.045I max
2 
9



7
Single slit envelope

Now interference term or pattern is
modulated by the diffraction term
 sin 

 






2
which has zeros at =(b/)sin=p
or, sin  = p/b
But, sin = m/a locate the principal
maxima of the interference pattern
8
Single slit envelope
Thus at a given angle a/b=m/p
 Then suppose a/b = integer
 For example, a = 3b
 Then m = 3, 6, 9, interference maxima are
missing

9
Diffraction gratings
Composed of systems with many slits per
unit length – usually about 1000/mm
 Also usually used in reflection
 Thus principal maxima vary sharp
 Width of peaks Δ = (2/N)
 As N gets large the peak gets very narrow
 For example, _________________

10
Diffraction gratings
Resolution
 Imagine trying to resolve two wavelengths
 1  2
 Assume resolved if principal maxima of
one falls on first minima of the other
 See diagram___________

11
Diffraction gratings







m1 = a sin 
m2 = a sin ’
But must have
a sin 
 m
1
a sin  ' 
1
  m  
2
N

Thus m(2 - 1 )= a (sin’ - sin) = (1/N)
Or mΔ =/N
Resolution, R =  /Δ = mN
E.g.
12
Fraunhofer diffraction from a circular aperture

y
x

P
r

E P  C  e dxdy
ikr
Lens plane
13
Fraunhofer diffraction from a circular aperture
Do x first – looking down
Path length is the same
for all rays = ro
Why?


R2  y2
 R y
2
2
EP  C  eikr 2 R 2  y 2 dy
14
Fraunhofer diffraction from a circular aperture
Do integration along y – looking from the side

P
+R

y=0

-R
ro

r = ro - ysin
15
Fraunhofer diffraction from a circular aperture
R
EP  2Ceikro
 iky sin
e

R 2  y 2 dy
R
Let
Then
y

R
  kR sin 
  
ky sin   k R  
 kR 
R2  y2 
R 2  2 R 2  R 1  2
Rd  dy
(1)
(2)
(3)
16
Fraunhofer diffraction from a circular aperture
1
EP  2Ce
ikro
R
2
e
i
1   d
2
1
1
The integral
e

1
i
J1  
1  d 

2
where J1() is the first order Bessell function of the first kind.
17
Fraunhofer diffraction from a circular aperture

These Bessell functions can be represented as
polynomials:
2k  p
k 



1
 2 



J P    
k!k  p !
k 0

and in particular (for p = 1),
  
  
  
2
2
2
2 J1  



 1




2!
2!3!
3!4!
2
4
6
18
Fraunhofer diffraction from a circular aperture

Thus,
 2 J1   
I  Io 

  

2
where  = kRsin and Io is the intensity when =0
19
Fraunhofer diffraction from a circular aperture
 Now



•
the zeros of J1() occur at,
= 0, 3.832, 7.016, 10.173, …
= 0, 1.22, 2.23, 3.24, …
=kR sin = (2/) sin
Thus zero at
sin  = 1.22/D, 2.23 /D, 3.24 /D, …
20
Fraunhofer diffraction from a circular aperture
2J1  
1.0

 2 J1   
 



0.5
-10
-8
-6
-4
-2
0
2
4
6
8
2
10
The central Airy disc contains 85% of the light

21
Fraunhofer diffraction from a circular aperture
D

sin = 1.22/D
22
Diffraction limited focussing
6
8
10
Cannot focus any wave to spot with dimensions < 
2
0
-2
-4


0.5
D
4
f
1.0


W = 2fsin  2f  = 2f(1.22/D) = 2.4 f/D
W = 2.4(f#) > 
f# > 1
-6

sin = 1.22/D
The width of the Airy disc
8

23
Fraunhofer diffraction and spatial resolution

If S1, S2 are too close together the Airy patterns will overlap and
become indistinguishable
4 0
-6-10
-4 -8
-2 -6
0 -4
2 -2
0.5
0.5
S2

1.0
S1
1.0
6 2
8 4
10 6

8



Suppose two point sources or objects are far away (e.g.
two stars)
Imaged with some optical system
Two Airy patterns
10

24
Fraunhofer diffraction and spatial resolution


Assume S1, S2 can just be resolved when
maximum of one pattern just falls on minimum
(first) of the other
Then the angular separation at lens,
 min

e.g. telescope D = 10 cm  = 500 X 10-7 cm
 min

1.22

D
5 X 10 5

 5 X 10 6 rad
10
e.g. eye D ~ 1mm min = 5 X 10-4 rad
25