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Optics Lecture Notes: Total Internal Reflection, Polarization, and Geometric Optics, Slides of Electrical Engineering

A set of lecture notes covering various topics in optics, including total internal reflection, polarization, and geometric optics. The notes discuss the concepts of incident, reflected, and refracted rays, as well as the properties of unpolarized and polarized light. The document also includes formulas for the brewster angle and the calculation of the intensity of light passing through two polarizers.

Typology: Slides

2012/2013

Uploaded on 08/20/2013

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4/11/12 1
Total Internal Reflection
incident
ray reflected
ray
refracted
ray
2!
1!
!
GLASS
AIR
n2
n1
LECTURE 24: Light
Text Reference: Chapter 32.1 through 32.2
4/11/12 3
Unpolarized Light Project onto the y, z
axes:
4/11/12 4
Linear Polarization (LP): Intensity Reduction
UP
(unpolarized light)
TA
LP
E1
!
E2
!
I=I0!
I1= !
I2= !
TA
LP
n
ˆ
TWO polarizers produce LP light. What is the intensity?
pf3
pf4
pf5

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Download Optics Lecture Notes: Total Internal Reflection, Polarization, and Geometric Optics and more Slides Electrical Engineering in PDF only on Docsity!

4/11/12 1

Total Internal Reflection

incident

ray

reflected

ray

refracted

ray

 2!  1!^ !

GLASS

n 2 AIR

n 1

LECTURE 24: Light

Text Reference: Chapter 32.1 through 32. 4/11/12 3

Unpolarized Light Project onto the y , z

axes:

4/11/12 4

Linear Polarization (LP): Intensity Reduction

UP

(unpolarized light)

TA

LP

E 1 !

E 2

I = I 0 ! I 1 = I 2 =

TA

LP

n ˆ

TWO polarizers produce LP light. What is the intensity?

4/11/12 5

Cross Polarizers (DEMO 7B-22)

I 0

cos

I 0

Vary

4/11/12 6

Polarization by Reflection

partially polarized

reflecting

surface

eyeball

Polaroid sun glass: eliminates glare If i = B, then reflected light will be fully polarized. i + B = 90o n 1 sin B = n 2 sin(90- B) n 1 sin B = n 2 cos B  B = arctan (n 2 /n 1 ) n 1 ~ 1 B = arctan (n 2 ) Brewster’s Law (1812) Brewster Angle AtB light has only perpendicular components. 4/11/12 7

Stress Distributions (DEMO 7B-22)

Stress rotates the polarization.

4/11/12 8

Geometric Optics

In situations in which the length scales are >> than

the light’s wavelength, lights propagates as rays

incident

ray

reflected

^ ray

1^  r

n 1

refracted

ray

 2^ n^2

Reflection:

Refraction:

θ i =θ r

n 1 sin θ 1 = n 2 sin θ 2

4/11/12 13

Focal Points of Spherical Mirrors DEMO

7A-

Concave: Parallel rays close to central axis reflect through a common point F. Convex: The extensions of the reflected rays pass through a common point behind the mirror. Sign Convention: r & f are positive for concave mirror. r & f are negative for convex mirror. 4/11/12^14 Images from Spherical Mirrors (b) O at the focal point: *image is ambiguous (a) O is inside the focal point: *image appears behind the mirror *same orientation (c) O is outside the focal point: *image is inverted & in front of the mirror

DEMO

7A-

4/11/12 15

Spherical Mirrors

  • Real images form on the same side of a mirror as the object.
  • Virtual images form on the opposite side. 1 s + 1 s ' = 1 f

For a spherical mirror

4/11/12 16

Magnification

Size of an object or image is measured to the mirror’s central axis & is called the image height, h’. h - height of object h’ - height of image Magnification produced by a mirror: m^ =^ h ' h m = s ' s For Spherical mirror: 1 s

1 s ' = 1 fs ' = fs sf m = − s ' sm = − f sf For plane mirror: s ' = − s m = + 1

4/11/12 17

Example

  • How tall must a vertical mirror be for MJ to be able to see his full height?
  • Simple trigonometry tells you that the mirror must be half the height of MJ h e f ! ! 2 ( ) 2 ( ) 2 2 he ef h MJ Hmirror ac ab bc ab^ he bc^ ef
  • = = = + = = = a b c 4/11/12 18

Location of Images by Drawing Rays

Use with next slide. 4/11/12 19

Location of Images by Drawing Rays

For concave mirrors: You can graphically locate the image of any off-axis point of the object by drawing a ray diagram with any two of four special rays through the point:

  1. A ray that is parallel to the central axis reflects through the focal point F.
  2. A ray that reflects from the mirror after passing through the focal point emerges parallel to the central axis.
  3. A ray that reflects from the mirror after passing through the center of curvature C returns along itself.
  4. A ray that reflects from the mirror at its intersection with the central axis is reflected symmetrically about that axis. 4/11/12 20

Summary

  • Equations for mirrors :

when the following sign conventions are used:

Mirror Type Object Location Image Location Image Type Image Orientation Sign of f r s’ m Plane Anywhere Opposite side of mirror from object Virtual Same orientation as object Concave Inside F Opposite side of mirror from object Virtual Same orientation as object Concave Outside F Same side as object Real Inverted Convex Anywhere Opposite side of mirror from object Virtual Same orientation as object 1 s

1 s ′ = 1 f M = − ss