Lecture 2 Flashcards

1
Q

angular resolution (formula)

A

α = 1.22 λ/D

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2
Q

resolution improves with

A

scale

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3
Q

Fraunhofer diffraction

A

plane-parallel waves incident upon aperture

viewed in far field L&raquo_space; D^2/λ

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4
Q

2D Fourier transform of aperture

A

Up ∝ ∫ ( ∫ A )A(x,y) exp(-i(xkx+yky)dxdy

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5
Q

A single-slit is modelled mathematically as

A

a step function

A(x) = { 1 , -a < x < a
{ 0 , elsewhere

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6
Q

Intensity in a single slit is proportional to

A

|Up|^2

the modulus of the fourier aperture function squared

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7
Q

Bessel functions

A

Up = Uo [ 2J1(kα) / kα ]

first zeros for kα = 1.22 π

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8
Q

Geometrical optics

A

Image formed of object at point of convergence rays.

Consider object to be made up of many individual point sources.

One-to-one mapping

Spacing in the image plane governed by the magnification of the system

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9
Q

Image formation

A

When imaging an object at infinity, the image plane is simply the focal plane

Mapping between incident angle and position on focal plane

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10
Q

Point Spread Function (formula)

A

I(α) = Ig * I(PSF)

I(α) = image intensity

Ig = geometrical image intensity

I(PSF) = point spread function intensity

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11
Q

Point spread function (formula in words)

A

actual image is the convolution of the ideal image predicted by geometrical optics with the point spread function intensity

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12
Q

U(PSF) =

A

Uo [ 2J1(πDα/λ) / (πDα/λ) ]

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13
Q

I(PSF) =

A

Io [ 2J1(πDα/λ) / (πDα/λ) ]^2

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14
Q

diffraction limit

A

effects of aberrations are negligible, said to be diffraction limited

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15
Q

Resolution - Strehl Ratio (formula)

A

S = I(PSF)(0) / I(airy)(0)

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16
Q

encircled energy

A

integrate PSF intensity within a circle of a given radius and compare to that of ideal PSF

17
Q

Strehl Ratio (definition)

A

is the ratio of intensity at the centre of the PSF peak with that expected in the ideal case (Airy disc)

18
Q

aberrations reduce

A

peak intensity of PSF

19
Q

Point spread function tells us

A

how the light from a source spreads out in an image

20
Q

for an ideal telescope the PSF is simply the

A

airy pattern

21
Q

use the expression for the point spread function to obtain the Rayleigh
criterion expression.

A

kα = 1.22π

(2π/λ D/2) sinα = 1.22π

angular separation of first zero:

sinα ≈ α = 1.22λ /D