Lecture 3: Optical Transfer Function Flashcards

(53 cards)

1
Q

period

A

d_0 = 1/f_0

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2
Q

width D where D/d_0

A

> > 1

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3
Q

diffracted amplitude

A

fourier transform of A(x)

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4
Q

diffracted order at

A

x=0 +/- Z_0 λ/d

where z_0 is the object distance

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5
Q

objects can be decomposed into

A

its fourier components
these are not transmitted perfectly to the image

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6
Q

high spatial frequencies are filtered out (removed) at

A

the system’s aperture

leads to loss of resolution and contrast in the image

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7
Q

another perspective

A

Two small patches separated by s
Interference of two sources (c.f. Young’s slits)
point sources centred on +/- s/2

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8
Q

aperture function for point sources centred on +/- s/2

A

A(x)=δ(x-s/2)+δ(x+s/2)

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9
Q

spatial frequency in image

A

fi=s/zi lambda

zi=image distance

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10
Q

what if spacing corresponds to diffraction orders and let zi=z0=z

A

spatial frequency in image fi=f0

also di=d0

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11
Q

For a particular spatial frequency to be present in the image, the aperture must

A

be large enough to accommodate the spacing between the 0th and 1st diffracted orders, s=lambda z f0, of the corresponding spatial frequency in the object.

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12
Q

Spatial frequency only resolved if

A

diffraction orders corresponding
to that frequency pass through the aperture of system.

otherwise info about frequency is lsot

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13
Q

minimum requirement for spatial frequency to be resolved

A

at least two orders to be supported
by the system

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14
Q

Structure of object resolved if

A

first diffraction order
propagates through the optical system

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15
Q

Fidelity of the image increases with

A

the number of diffraction orders propagating through the optical system

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16
Q

Object can be considered to be made up of

A

many point sources
image of each is spread out

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17
Q

Image is convolution of

A

the geometrical image with
the Point Spread Intensity

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18
Q

Actual image is the convolution of

A

the ideal image predicted by
geometrical optics with the Point Spread Intensity

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19
Q

Start with Image Amplitude and Image Intensity as functions of spatial coordinates. Image amplitude:

A

Convolution of Point Spread Amplitude with Geometrical Amplitude,

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20
Q

Start with Image Amplitude and Image Intensity as functions of spatial coordinates. Image intensity

A

Convolution of Point Spread Intensity with Geometrical Intensity

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21
Q

Fourier transform of convolution is

A

the product of the Fourier transforms

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22
Q

fourier transform of product is

A

convolution of the fourier transforms

23
Q

spatial angular frequency

A

kx=2pifx

in radians per metre

24
Q

Image intensity is the convolution of

A

the geometric image intensity with the Point Spread
Intensity

25
get frequency content of image
take fourier transform
26
fourier transform of intensity
frequency spectrum of image = optical transfer function x frequency spectrum of geometrical image
27
filtering/degradation of system attributed to
H(kx,ky)
28
H(kx,ky) transmits
low spatial frequencies
29
H(kx,ky) attenuates
high spatial frequencies
30
H (optical transfer function) describes how
optical system filters or modifies spatial frequencies that would otherwise contribute to the image
31
magnitude of OTF |H| corresponds to
contrast modulation transfer function (MTF)
32
Phase of OTF, arg(H) corresponds to
distortion ie a shift in position phase transfer function (PTF)
33
atmospheric turbulence
* Pockets of air with different temperatures, densities and refractive indices * Corrugated wavefronts * Dominant cause of aberrations for large-scale telescopes
34
atmospheric turbulence: airy
small aperture short exposure
35
atmospheric turbulence: speckle
large aperture short exposure
36
atmospheric turbulence: time average
large aperture long exposure
37
atmospheric turbulence: telescope
well-defined static analytical
38
atmospheric turbulence: atmosphere
random changing statistical
39
convolution
(f⊗g)(z)
40
cross-correlation
(f★g)(z)
41
auto-correlation
(f★f)(z)
42
power spectrum=
fourier transform of autocorrelation
43
fourier transform of power=
autocorrelation of amplitude spectrum
44
amplitude transfer function (ATF)
H(fx,fy)= F{h}
45
optical transfer function
H(fx,fy) = F{|h|^2} / normalisation
46
aurtocorrelation of ATF, what are p and q?
spatial frequency variables
47
H(fx,fy)≡
scaled version of aperture / pupil function
48
autocorrelation of pupil, H(f'x,f'y)=
area of overlap / total overlap
49
With Fourier Optics we can understand
how an optical system filters frequencies present within the object
50
the optical transfer function expresses
how that frequency content in filtered at the aperture of the optical system
51
atmospheric turbulence requires a
statistical description
52
the optical transfer function can also be understood to be the
autocorrelation of the pupil function
53