5 - Diffr/Thin Film/Scatter/Polar Flashcards
Describe scatter + types (2)
Bending of waves around obstacles
Fraunhofer: far-field
Fresnel: near-field
Diffraction and resolution ability
Resolution is limited by diffraction
As light passes thru a circular aperture, it creates an Airy disk
-larger for smaller apertures
-2 objects cannot be distinguished when the 2 corresponding Airy disks overlap
—mathematically = Rayleigh’s criteria
How we estimate pt’s expected VA thru pinhole
Rayleigh’s criteria: sinθr = (1.22λ)/d
Rayleigh’s criteria for pinhole: assumes λ of 555nm, θ corresponds to MAR, d is pinhole diameter in milimeters, we rewrite Rayleigh’s as:
MAR = 2.33/d (mm)
*d of 2.3 = 20/20 vision
Recall:
MAR: (Snellen fraction)^-1
-units arc minutes
Anti-glare coatings
AR = thin film that creates destructive interference between 2 reflecting light waves
We choose the film so that nL > nF > 1 (lens > film > 1)
Minimum film thickness providing destructive interference for anti-glare coatings equation
d = λ/(4nf)
Thickness = wavelength of light/(4*index of refr of film)
If not specified, assume 555nm for wavelength
Optical thickness equations (2)
OT = (d)(nf) = (thickness of film)*(index of refr of film)
OT = λ/4
*second one is much more helpful!
Ideal thin film equation (film material that minimizes reflection)
nf = √(n1nL)
Index of film = √((index of initial medium)*(index of lens material used))
Initial medium usually air
Describe Rayleigh scattering and give equation
Particles that cause are much SMALLER than the wavelength of light = WAVELENGTH-DEPENDENT
-gives sky blue color, sunsets red
I ∝ 1/(λ^4)
Intensity of scattered light = 1/(wavelength to the fourth)
Describe Tyndall scattering
Particles that cause are much LARGER than the wavelength of light and is PURELY DUE TO GEOMETRIC OPTICS = WAVELENGTH-INDEPENDENT
-gives clouds white color
Light consists of oscillating (2) field vectors, both perpendicular to the direction of travel.
Polarization allows us to talk about the shape that __ vector traces out in that plane.
E (electric) + B (magnetic)
E
Describe linearly polarized light
Oscillations of the E vector (in time) all fall on a line
The magnitude of E is changing, but direction is constant
Describe circularly polarized light
Oscillations of the E vector (in time) trace out a circle
The E vector is rotating, but its magnitude is constant
Mathematically due to addition of 2 linearly polarized waves of EQUAL AMPLITUDE and a phase difference of θ = π/2
Describe elliptically polarized light
Oscillations of E vector (in time) trace out an ellipse
The E vector is rotating AND changing in magnitude
Mathematically due to addition of 2 linearly polarized waves of DIFFERENT AMPLITUDE and a phase difference of θ = π/2
Describe Brewster’s law
Reflection changes the state of polarization of light
Directly applied in polarized sunglasses
-in particular, made to reduce glare arising from horizontal surfaces
Polarizers
- absorption axis
- transmission axis
AA: parallel to the wire grid, E field components parallel to the AA are not transmitted
TA: perpendicular to the wire grid, E field components parallel to the TA are transmitted