PHY2049 Summer 2011

• The following clicker numbers are no longer going to be counted. They have not been registered.

420441 461211 462681

497478 625833• Exam 2 (Ch. 28-33) is scheduled for

Monday July 11 during class times.

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Chapter 34

One of the most important uses of the basic laws governing light is the production of images. Images are critical to a variety of fields and industries ranging from entertainment, security, and medicine

In this chapter we define and classify images, and then classify several basic ways in which they can be produced.

Images

34-

3

A clear sheet of polaroid is placed on top of a similar sheet so that their polarizing axes make an angle of 30◦ with each other. The ratio of the intensity of emerging light to incident unpolarized light is:

A. 1/4 B. 1/3 C. 1/2 D. 3 /4 E. 3 /8

4

Image: a reproduction derived from light

Real Image: light rays actually pass through image, really exists in space (or on a screen for example) whether you are looking or not

Virtual Image: no light rays actually pass through image. Only appear to be coming from image. Image only exists when rays are traced back to perceived location of source

Two Types of Images

34-

object lensreal image

object mirror virtual image

5

Light travels faster through warm air warmer air has smaller index of refraction than colder air refraction of light near hot surfaces

For observer in car, light appears to be coming from the road top ahead, but is really coming from sky.

A Common Mirage

34-

Fig. 34-1

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Plane mirror is a flat reflecting surface.

Plane Mirrors, Point Object

34-

Fig. 34-2

Fig. 34-3

Ib Ob

Identical triangles

Plane Mirror: i pSince I is a virtual image i < 0

7

Each point source of light in the extended object is mapped to a point in the image

Plane Mirrors, Extended Object

34-

Fig. 34-4 Fig. 34-5

8

Your eye traces incoming rays straight back, and cannot know that the rays may have actually been reflected many times

Plane Mirrors, Mirror Maze

34-

Fig. 34-6

1

23

4

56

78

9

12

34

56

78

9

9

Plane mirror Concave Mirror1. Center of Curvature C:

in front at infinity in front but closer2. Field of view

wide smaller3. Image

i=p |i|>p 4. Image height

image height = object height image height > object height

34-Fig. 34-7

Plane mirror Convex Mirror1. Center of Curvature C:

in front at infinity behind mirror and closer2. Field of view

wide larger3. Image

i=p |i|<p 4. Image height

image height = object height image height < object height

Spherical Mirrors, Making a Spherical Mirror

concave

plane

convex

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Spherical Mirrors, Focal Points of Spherical Mirrors

34-

Fig. 34-8

concave convex

Spherical Mirror:1

2f r

r > 0 for concave (real focal point)r < 0 for convex (virtual focal point)

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Start with rays leaving a point on object, where they intersect, or appear to intersect marks the corresponding point on the image.

Images from Spherical Mirrors

34-

Fig. 34-9

Real images form on the side where the object is located (side to which light is going). Virtual images form on the opposite side.

Spherical Mirror:1 1 1

p i f Lateral Magnification:

'hm

h

Lateral Magnification:i

mp

12

Locating Images by Drawing Rays

34-

Fig. 34-10

1. A ray parallel to central axis reflects through F2. A ray that reflects from mirror after passing through F, emerges parallel to central axis3. A ray that reflects from mirror after passing through C, returns along itself4. A ray that reflects from mirror after passing through c is reflected symmetrically about the

central axis

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Proof of the magnification equation

34-

Fig. 34-10

Similar triangles (are angles same)

, ,

(magnification)

de cd decd i ca p m

ab ca abi

mp

14

Spherical Refracting Surfaces

34-

Fig. 34-11

Real images form on the side of a refracting surface that is opposite the object (side to which light is going). Virtual images form on the same side as the object.

Spherical Refracting Surface: 1 2 2 1n n n n

p i r

When object faces a convex refracting surface r is positive. When it faces a concave surface, r is negative. CAUTION: Reverse of of mirror sign convention!

1534-

Fig. 34-13

Converging lens

Diverging lens

Thin Lens:1 1 1

f p i Thin Lens in air:

1 2

1 1 11n

f r r

Lens only can function if the index of the lens is different than that of its surrounding medium

Thin Lenses

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Images from Thin Lenses

34-

Fig. 34-14

Real images form on the side of a lens that is opposite the object (side to which light is going). Virtual images form on the same side as the object.

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Locating Images of Extended Objects by Drawing Rays

34-

Fig. 34-15

1. A ray initially parallel to central axis will pass through F22. A ray that initially passes through F1, will emerge parallel to central axis3. A ray that initially is directed toward the center of the lens will emerge from the lens

with no change in its direction (the two sides of the lens at the center are almost parallel)

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Two Lens System

34-

1. Let p1 be the distance of object O from Lens 1. Use equation and/or principle rays to determine the distance to the image of Lens 1, i1.

2. Ignore Lens 1, and use I1 as the object O2. If O2 is located beyond Lens 2, then use a negative object distance p1. Determine i2 using the equation and/or principle rays to locate the final image I2.

Lens 1 Lens 2

p1

OI1

i1

O2

p2

I2

i2

1 2The net magnification is: M m m

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A football field is about 100 meters long. The time for light to travel this distance is about:

A. 0.33x10-6 s B. 0.33 ms C. 33 minD. 3 hr E. 3 yr

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Optical Instruments, Simple Magnifying Lens

34-

Fig. 34-17

Can make an object appear larger (greater angular magnification) by simply bringing it closer to your eye. However, the eye cannot focus on objects closer that the near point pn~25 cmBIG & BLURRY IMAGE

A simple magnifying lens allows the object to be placed close by making a large virtual image that is far away.

'

and '25 cm

m

h h

f

Simple Magnifier:

25 cmm

f

Object at F1

2134-

Fig. 34-18

Optical Instruments, Compound Microscope

obob

ob ey

since and

25 cm magnification compounded (microscope)

i sm i s p f

p f

sM mm

f f

I close to F1’O close to F1

Mag. Lens

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Optical Instruments, Refracting Telescope

34-

Fig. 34-19

eyob ey

ob ob ey

ob

ey

' ' , ,

(telescope)

h hm

f f

fm

f

I close to F2 and F1’

Mag. Lens

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Three Proofs, The Spherical Mirror Formula

34-

Fig. 34-20

and 2

1

2

,

12

2

1 1 1

2

22

ac ac ac ac

cO p cC r

ac ac

CI i

f r

ac ac ac

p i

r f

pf i f

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Three Proofs, The Refracting Surface Formula

34-

Fig. 34-21

1 1 2 2

1 1 2 2 1 2

1 2

1 2

1 2 2 1

1 2 2

1 2 2 1

1

sin sin

if and are small

and

; ;

n n n n

ac ac acn n n

n n

n n

n

np

n

ac ac ac

p r i

n n n n

p i

i

r

r

2534-

Fig. 34-22

1 2 2 1

1 2

where 1 and

'' '

1 1 ; if small

1 1 Eq. 34-22

' ' '

1 1 Eq. 34-25

' '' ''

Eq. 34-22 Eq. 34

' '' ''1 1 1 1 1 1 1 1

1 1' '' ' '

-25' ' ''

n n n n

p i r

n n n

p i L

n nL

i L i r

n np i r r p

n n

p i r

n n

i r

i i

r

r

Three Proofs, The Thin Lens Formulas

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The time for a radar signal to travel to the Moon and back, a one-way distance of about 3.8 × 108 m, is:

A. 1.3 s B. 2.5 s C. 8 s D. 8minE. 1 × 106 s

Radio waves of wavelength 3 cm have a frequency of:

A. 1MHz B. 9MHz C. 100MHz D. 10, 000MHz E. 900MHz

The light intensity 10m from a point source is 1000W/m2. The intensity 100m from the samesource is:

A. 1000W/m2 B. 100W/m2 C. 10W/m2 D. 1W/m2

E. 0.1W/m2

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Light of uniform intensity shines perpendicularly on a totally absorbing surface, fully illuminating the surface. If the area of the surface is decreased:

A. the radiation pressure increases and the radiation force increasesB. the radiation pressure increases and the radiation force decreasesC. the radiation pressure stays the same and the radiation force increasesD. the radiation pressure stays the same and the radiation force decreasesE. the radiation pressure decreases and the radiation force decreases