Polarisation Flashcards

1
Q

What is a longitudinal wave?

A

motion is along the direction of propagation

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2
Q

What is a transverse wave?

A

motion is transverse (perpendicular) to the direction of motion

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3
Q

Light is a 3d vector field, if it propagates along the z axis what is happening in the rest of the field?

A

the electric and magnetic fields will be confined to the x-y plane forming a 2d vector field

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4
Q

How are the magnetic and electric fields related

A

B(z,t) = 1/cE(z,t)

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5
Q

What is the condition under which we can neglect the light’s magnetic force compared to its electric force

A

the charge’s velocity must be much less than the speed of light

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6
Q

what do you call a surface over which a plane wave is constant?

A

a wavefront

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7
Q

What can we say about a plane wave

A
  • it is of infinite extent
  • in planes perpendicular to the propagation, the phase of the wave (and the field) is constant
  • all the electric field vectors in this plane are in phase
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8
Q

What are the formulae for linearly polarised light

A

Ḛ𝑥 (𝑧, 𝑡) = Re{Ḛ0 cos(a) exp[ 𝑖(𝑘𝑧 − 𝜔𝑡)]}
Ḛ𝑦 (𝑧, 𝑡) = Re{Ḛ0 sin(a) exp[ 𝑖(𝑘𝑧 − 𝜔𝑡)]}

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9
Q

Why are the components of linearly polarised light always in phase?

A

The complex amplitude is the same for each component

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10
Q

what are the formulae for circular polarisation?

A

Ḛ𝑥 (𝑧, 𝑡) = Re{Ḛ0 exp[ 𝑖(𝑘𝑧 − 𝜔𝑡)]}
Ḛ𝑦 (𝑧, 𝑡) = Re{−(or +)𝑖Ḛ0 exp[ 𝑖(𝑘𝑧 − 𝜔𝑡)]}

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11
Q

What is the phase shift between components of circularly polarised light?

A

90 degrees

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12
Q

Looking along k, what direction does right circularly polarised light rotate?

A

counterclockwise

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13
Q

Looking along k, what direction does left circularly polarised light rotate?

A

clockwise

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14
Q

What do you get if you combine RCPL and LCPL of the same amplitude

A

linearly polarised light

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15
Q

What yields elliptically polarised light?

A

unequal arbitrary relative phase components

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16
Q

what are the formulae for elliptically polarised light?

A

𝐸𝑥 (𝑧, 𝑡) = Re{Ḛ0𝑥 exp[ 𝑖(𝑘𝑧 − 𝜔𝑡)]}
𝐸𝑦 (𝑧, 𝑡) = Re{Ḛ0𝑦 exp[ 𝑖(𝑘𝑧 − 𝜔𝑡 − 𝜃)]}

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17
Q

When is light unpolarised?

A

When phases of x and y polarisations fluctuate
they vary on a timescale lower than 1/omega but faster than we can measure

18
Q

What is a jones vector?

A

A 2d vector containing the two complex amplitudes which defines the polarisation state of a field.

19
Q

What is the general form of a jones vector?

A

E = |Ex|
|Ey|

20
Q

What con it be useful to consider for Jones vectors?

A

the relative values
E/Ex = | 1 |
|Ey/Ex|

21
Q

For RCP what is Ey/Ex

A

-i

22
Q

For LCP what is Ey/Ex

A

+i

23
Q

Linear general jones jector

A

sin(a)
cos(a)

24
Q

Circular general jones vector

A

1
+-i

25
Q

Elliptical general jones vector

A

A
B+-iC

26
Q

How can you calculate the polarisation of a beam after it has passed through an optical component?

A

Et = A.Ei where A is a 2x2 matrix for the component

27
Q

what is the matrix for a horizontal polariser?

A

1 0
0 0

28
Q

what is the matrix for a vertical linear polariser?

A

0 0
0 1

29
Q

what is the matrix for a quarter wave plate with the fast axis horizontal and how can it be changed if the fast axis is vertical?

A

exp(ipi/4) 1 0
0 i
change to -i

30
Q

what is the matrix for a homogeneous circular polariser right and how can it be changed for left?

A

1/2 1 i
-i 1
swap the signs on the i’s

31
Q

what is the jones vector representing the polarisation state of UPL

A

1 |
|Ay/Ax exp(𝜃𝑥 (𝑡) − 𝜃𝑦 (𝑡))|

32
Q

What is Malus’ Law

A

A^2=A0^2cos^2(𝜃)

33
Q

What happens at the polarising angle 𝜃p

A

reflected light is completely polarised orthogonal to plane of incidence
it is perpendicular to the refracted ray

34
Q

What is Brewster’s Law?

A

tan𝜃p = nb/na

35
Q

what happens when the reflected and refracted beams are at 90 degrees?

A

polarisation is parallel
reflection coefficient goes to zero
because no scattering can occur due to dipole emission pattern

36
Q

How do you derive Brewster’s Law

A
  • start with snell’s law
  • the incident angle plus the transmitted angle = 90
  • nisin(𝜃i) = ntcos(𝜃i)
37
Q

Why does the Brewster angle effect happen?

A

at 𝜃p dipole radiators in n2 emit a characteristic patter and when the refracted and reflected rays are perpendicular there can be no emission of parallel polarised light along the dipole axis (reflected ray)

38
Q

What are the Fresnel equations?

A

analysing the incidence of light at a boundary allows calculation of the reflectivity and transmission of light at the interface

39
Q

What orientation do transverse electric waves have their electric fields with respect to the plane of incidence and the media boundary?

A
  • perpendicular to the plane of incidence
  • parallel to the boundary
40
Q

when does the Rtm go through zero

A

at brewster angle