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Fraunhofer Diffraction: Circular aperture

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Title: Fraunhofer Diffraction: Circular aperture


1
Fraunhofer Diffraction Circular aperture
  • Wed. Nov. 27, 2002

2
Fraunhofer diffraction from a circular aperture
?
y
?
P
r
x
?
Lens plane
3
Fraunhofer diffraction from a circular aperture
Path length is the same for all rays ro
Do x first looking down
Why?
?
4
Fraunhofer diffraction from a circular aperture
Do integration along y looking from the side
?
P
R
?
y0
ro
?
?
-R
r ro - ysin?
5
Fraunhofer diffraction from a circular aperture
Let
Then
6
Fraunhofer diffraction from a circular aperture
The integral
where J1(?) is the first order Bessell function
of the first kind.
7
Fraunhofer diffraction from a circular aperture
  • These Bessell functions can be represented as
    polynomials
  • and in particular (for p 1),

8
Fraunhofer diffraction from a circular aperture
  • Thus,
  • where ? kRsin? and Io is the intensity when ?0

9
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,

10
Fraunhofer diffraction from a circular aperture
The central Airy disc contains 85 of the light
11
Fraunhofer diffraction from a circular aperture
D
?
sin? 1.22?/D
12
Diffraction limited focussing
  • sin? 1.22?/D
  • The width of the Airy disc
  • W 2fsin? ? 2f ? 2f(1.22?/D) 2.4 f?/D
  • W 2.4(f)? gt ? f gt 1
  • Cannot focus any wave to spot with dimensions lt ?

f
D
?
?
13
Fraunhofer diffraction and spatial resolution
  • Suppose two point sources or objects are far away
    (e.g. two stars)
  • Imaged with some optical system
  • Two Airy patterns
  • If S1, S2 are too close together the Airy
    patterns will overlap and become indistinguishable

S1
?
S2
14
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,
  • e.g. telescope D 10 cm ? 500 X 10-7 cm
  • e.g. eye D 1mm ?min 5 X 10-4 rad

15
Polarization
16
Matrix treatment of polarization
  • Consider a light ray with an instantaneous
    E-vector as shown

y
Ey
x
Ex
17
Matrix treatment of polarization
  • Combining the components
  • The terms in brackets represents the complex
    amplitude of the plane wave

18
Jones Vectors
  • The state of polarization of light is determined
    by
  • the relative amplitudes (Eox, Eoy) and,
  • the relative phases (? ?y - ?x )
  • of these components
  • The complex amplitude is written as a two-element
    matrix, the Jones vector

19
Jones vector Horizontally polarized light
The arrows indicate the sense of movement as the
beam approaches you
  • The electric field oscillations are only along
    the x-axis
  • The Jones vector is then written,
  • where we have set the phase ?x 0, for
    convenience

The normalized form is
20
Jones vector Vertically polarized light
  • The electric field oscillations are only along
    the y-axis
  • The Jones vector is then written,
  • Where we have set the phase ?y 0, for
    convenience

The normalized form is
21
Jones vector Linearly polarized light at an
arbitrary angle
  • If the phases are such that ? m? for m 0,
    ?1, ?2, ?3,
  • Then we must have,
  • and the Jones vector is simply a line inclined
    at an angle ? tan-1(Eoy/Eox)
  • since we can write

?
The normalized form is
22
Jones vector and polarization
  • In general, the Jones vector for the arbitrary
    case
  • is an ellipse

y
Eoy
b
a
?
x
Eox
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