Optics Flashcards

(33 cards)

1
Q

Fermats principle of least time

A

The optical path length of the ray between two points is stationary with respect to small changes of the path

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2
Q

Light travels in _ in uniform medium

A

Straight lines

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3
Q

Law of relfection

A

The reflected ray lies in the plane of incidence, with the angle of reflection equal to the angle of incidence

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4
Q

Law of refraction

A

The refracted ray lies in the plane of incidence, with the angle of refraction related to the angle incidence by Snells law.

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5
Q

Positive R means

A

C is to the right of the lens

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6
Q

Negative R means

A

Its to the left

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7
Q

Positive lenses

A

Thicker in the middle than the edges. f is positive. (Bulge out more than they cave in). Always tries to make rays converge more than they did to start with

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8
Q

Real images form

A

After the lens

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9
Q

Virtual images form

A

Before the lens

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10
Q

Negative lenses

A

Thinner in the middle than the edges, they ‘cave in’ more than they ‘bulge out’ . Makes rays diverge more than they did to start with

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11
Q

Chromatic abberation

A

Focal length depends on refractive index, which depends on wavelength, so different colours get focused at different points, leading to fringing

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12
Q

Spherical aberration

A

Spherical lenses deviate from the “thin and paraxial” approximation. Light further from axis is focused closer to the lens than light closer to the axis, so light is not focused at a single point

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13
Q

Chromatic aberration mitigation

A

Use curved mirrors instead of lenses

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14
Q

Spherical aberration mitigation

A

‘Aspheric’ lenses

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15
Q

Superposition Principle

A

The disturbance, at any point in a linear medium is the algebraic sum of the separate constituent waves

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16
Q

Coherence

A

Two waves are coherent if they have:
-a well defined (relatively stable) relative phase
- have the same frequency, and
-split off from the same source
-delay between waves must be small compared to coherence time

17
Q

Interferometers

A

An experiment of device that makes use of interference. Light from a single source is split into two or more waves that are made to interfere.

18
Q

Types of interferometer

A

Wavefront-division interferometer
Amplitude division interferometer

19
Q

Types of Amplitude division interferometers

A

Michelson, Mach-Zehnder, Sagnac

20
Q

Fabry perot interferometer

A

A precisely parallel pair of such mirrors, with a cavity of width d between

21
Q

Finesse measures

A

The interferometer’s performance as a spectrometer

22
Q

Full width half maximum (FWHM)

A

The width between where the transmission is half its maximum value

23
Q

Free spectral range. (FSR )

A

Separation between fringes

24
Q

Huygens Fresnel Principle

A

Every point on a wavefront serves as a source of secondary wavelets. The disturbance at a point beyond is the superposition of all these wavelets

25
Far field
When L is much greater than h^2/lambda (Fraunhofer condition) and the derivation of I(theta) is reliable
26
Near field
Reverse the inequality in the fraunhofer condition and the pattern is the geometrical shadow
27
Fresnel zone
In between the near field and far field
28
Rayleigh criterion
Two incoherent point sources are just resolved if the centre of one’s Airy disc falls on the first minimum of the other’s
29
Double slit relationships
Large feature d determines the small feature: fringes. Small feature h determines large feature: diffraction envelope.
30
Diffraction orders
Sharp peaks in the interference pattern of N slits
31
Blazing grating
Adding a saw tooth pattern in the grating to shift the envelope so that its peak lies near the wavelength dependent first order instead of the wavelength independent zeroth order
32
Aperture function
The wave function just after the aperturem
33
Paraxial
Small angles close to axis