Diffraction Flashcards

1
Q

What is diffraction?

A

The process where light spreads when it passes through a narrow aperture.

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2
Q

When is light diffracted?

A

If the physical size of the aperture is comparable to, or smaller than, the wavelength of the light

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3
Q

What is Fraunhofer Diffraction?

A

Waves incident on and leaving the aperture can be considered plane

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4
Q

What is Fresnel Diffraction?

A

Waves incident on and leaving the aperture can NOT be considered plane

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5
Q

What is the geometry for observing Fraunhofer diffraction?

A
  • Large distances between S(source) and screen and also the screen and L(second screen)
    ^ Too big of a system over come by:
    OR
  • Two lenses to produce incoming and outgoing plane waves ( diffraction pattern is produced in focal plane of second lens) – at a distance f from L
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6
Q

What are the steps of calculating Fraunhofer diffraction produced by an (1D) aperture?

A
  • Write f(x) (describes the transmission of light through the screen)
  • Calculate the Fourier transform of f(x) to give F(kx)
  • Calculate |F(kx)|^2
    Substitute kx =2Ο€sintheta/lambda
    Replace sintheta with x/f

Fraunhofer diffraction by a single long square slit:
𝐼(π‘₯)=𝐼_0 sinc ^2 (πœ‹π‘€x/π‘“πœ†)
Fraunhofer diffraction by a single long triangle slit:
𝐼(π‘₯)=𝐼_0 sinc ^4 (πœ‹π‘€x/π‘“πœ†)

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7
Q

How do we get a aperture that has a variable value?

A

Systems with transmission functions intermediate between one and zero
For example using glass with filter, if it is very thin it will partial transmit light. Used in photography

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8
Q

What does the diffraction depend on?

A
  • Depends on the size of the aperture.
  • aperture size&raquo_space; wavelength
  • light travels in a straight line with no diffraction as a result we get geometrical optics and shadows etc
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9
Q

What is the width of the central peak of the diffraction pattern by a single slit?

A

Ξ”x=2sΞ»/w ( s or f )
Example 15

Ξ”x -the separation between fringes 
s - the separation between screens 
f - distance to screen L when a lens is used
Ξ» - wavelength
w - the slit width
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10
Q

What are the steps of calculating Fraunhofer diffraction produced by an (2D) aperture?

A
  • Write f(x) (describes the transmission of light through the screen)
  • Calculate the Fourier transform of f(x) to give F(kx)= 𝐹(π‘˜_π‘₯,π‘˜_𝑦)=1/√2πœ‹ 1/√2πœ‹ ∫(βˆ’βˆž)^(+∞)∫(βˆ’βˆž)^(+∞)𝑓(π‘₯,𝑦)𝑒^(βˆ’π‘–π‘˜_π‘₯ π‘₯) 𝑒^(βˆ’π‘–π‘˜_𝑦 𝑦) dπ‘₯d𝑦 (In 2D)
  • Calculate |F(kx)|^2
    Substitute kx =2pisintheta/lambda
    Replace sintheta with x/f
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11
Q

What are the equations for the diffraction by a rectangular aperture?

A
Ξ”x=2sΞ»/wx
Ξ”y=2sΞ»/wy
( s turns into f for a lens)
Ξ”x - the spot size (the diameter of the central maxima of diffraction pattern) 
s - the separation between screens 
Ξ» - wavelength
w - the slit width/size of the aperture
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12
Q

What are the equations for the diffraction by a circular aperture?

A

Ξ”x =~2.44Ξ»s/D
( s turns into f for a lens)
Ξ”x - the spot size (the diameter of the central maxima of diffraction pattern)
s - the separation between screens
f - focal length/distance to screen L when a lens is used
Ξ» - wavelength
w - the slit width

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13
Q

What are the effects of diffraction on spatial resolution of a telescope?

A

Diffraction as light passes through a telescope may prevent closely spaced objects from being separately resolved.

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14
Q

What are the equations for the diffraction by two very narrow slits?

A
Fridge spacing:
Ξ”x =Ξ»s/d (s or f)
s - the separation between screens 
f - distance to screen L when a lens is used
Ξ» - wavelength
d - the separation between slits 
Ξ”x -the separation between fringes
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15
Q

What are the equations for the diffraction by two slits of non-zero width?

A

𝐼(π‘₯)=𝐼_0 sinc ^2 (πœ‹π‘€/π‘“πœ† π‘₯) cos^2⁑(πœ‹π‘‘/πœ†π‘“ π‘₯)
First term - Diffraction by a single slit
Second term - Diffraction by two
very narrow slits

IGNORING THE FIRST TERM
Intense maxima occur when denominator term is zero which gives Ξ”x =Ξ»s/d, we maximise d by choosing the one at the very end d = N-1/2 * centre of slit spacing

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16
Q

What is the consequence of diffraction by two slits of non-zerowidth?

A

Missing bright fridges in the diffraction pattern (missing orders)

17
Q

What are the equations for diffraction by an array of N identical slits?

A

𝐼(π‘₯)=𝐼_0sinc^2 (πœ‹π‘€x/πœ†π‘“) (sin⁑(π‘π‘‘πœ‹x/πœ†π‘“)/sin⁑(π‘‘πœ‹x/πœ†π‘“ )^2

First Term - Diffraction by a single slit
Second Term - Diffraction by a N very narrow slits

IGNORING THE FIRST TERM
Intense maxima occur when denominator term is zero this gives the diffraction equation

Weaker maxima occur when numerator equals one

18
Q

What is the diffraction equation and what does it tell us?

A

𝑑 sinβ‘πœƒ=π‘›πœ†
(for large N)
Tells us the angles where intense light is diffracted.

19
Q

What is the equation for the angular width of the main maxima of the diffracted light?

A

Ξ”πœƒ=πœ† 2πœ‹/(π‘‘πœ‹ cosβ‘πœƒ )𝑁

20
Q

What is the equation for the number of diffraction orders produced by a diffraction grating?

A

nmax= d/πœ†

n must be integer it must take the next lowest whole number

21
Q

What is the Rayleigh criterion for spectral resolution?

A

When the maxima of one wavelength coincides with the first minima of the second wavelength

22
Q

What is the equation for the spectral resolving power?

A

πœ†/Ξ”πœ†
πœ† - average wavelength
Ξ”πœ† - the difference between two wavelength

23
Q

What is a diffraction grating and why is it used?

A

A structure consisting of a large number of slits (e.g. N>100)

used to split light consisting of many wavelengths into the wavelength components

24
Q

What is the equation for the spectral resolving power for a diffraction grating?

A
πœ†/Ξ”πœ†=𝑛𝑁
n - diffraction order
N - slit number
πœ† - average wavelength
Ξ”πœ† - the difference between two wavelength
25
Q

What are the consequences of diffraction?

A

When light of wavelength passes through the aperture of a telescope of diameter D and if the focal length is f then the angular and spatial widths of the maximum of the resultant diffraction pattern are

Ξ”πœƒβ‰ˆ2.44 πœ†/𝐷, Δπ‘₯β‰ˆ2.44 πœ†π‘“/𝐷

If light from two closely spaced objects enters a telescope the spread in their images that results from diffraction may prevent them from being separated – spatially resolved

There will be a minimum angular separation that two objects can have such that the telescopes shows them as being separate – this is the angular resolution of the system

26
Q

What is the equation for the size of an image if diffraction is IGNORED and not ignored?

A

Ξ”π‘₯ = Ξ±f
Ξ± - angular power
f - focal length

Ξ”π‘₯β‰ˆ2.44 πœ†π‘“/𝐷
πœ† - wavelength
𝑓 - focal length
D - diameter

If 2nd effect&raquo_space; 1st so just use 2nd effect

27
Q

What is the angular resolution of an optical system/resolving power of a telescope?

A

Ξ” Ξ± = 1.22πœ†/𝐷

Ξ” Ξ± - resolving power
D - input aperture diameter
πœ† - imaging light of wavelength

28
Q

What is the equation for the maximum distance an optical system can resolve light?

A

Ξ” Ξ± = x/d

x- separation
d - min distance
Ξ± - angular resolving power (minimum angular separation between two points)