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Information for Physics 1201 Midterm 2 Wednesday, March 27

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My lecture slides are posted at<br />

http://www.physics.ohio-state.edu/~humanic/<br />

<strong>In<strong>for</strong>mation</strong> <strong>for</strong> <strong>Physics</strong> <strong>1201</strong> <strong>Midterm</strong> 2<br />

<strong>Wednesday</strong>, <strong>March</strong> <strong>27</strong><br />

1) Format: 10 multiple choice questions (each worth 5 points) and<br />

two show-work problems (each worth 25 points), giving 100 points<br />

total.<br />

2) Closed book and closed notes.<br />

3) Equations and constants will be provided on the midterm<br />

4) Covers the material in Chapters 21, 22, 23, and 24


Polarization<br />

Polarized light is produced by the scattering of unpolarized<br />

sunlight by molecules in the atmosphere.<br />

Molecules re-radiate sunlight.<br />

As you look at larger and larger<br />

angles with respect to the<br />

incident sunlight, the re-radiated<br />

light becomes more and more<br />

horizontally polarized.


Polaroid Sun Glasses<br />

Besides sunlight re-radiated from atmospheric molecules, there are<br />

other sources of horizontally polarized light that occur in nature, such<br />

as sunlight reflected from horizontal surfaces such as lakes.<br />

Polaroid sun glasses take advantage of this fact by using polarizers<br />

with their axes oriented vertically:<br />

è in addition to 1/2 of the unpolarized light which is already blocked by<br />

the polarizers, all of the horizontally polarized light is completely blocked,<br />

thus blocking out some of the reflected light which can confuse you<br />

during some outdoor activities (e.g. driving, piloting, fishing…….).


Polarization<br />

Another application using polarized glasses: watching 3-D movies.<br />

In a 3-D movie, two separate rolls of film are projected using a projector<br />

with two lenses, each with its own polarizer. The two polarizers are<br />

crossed. Viewers watch the action on-screen through glasses that have<br />

correspondingly crossed polarizers <strong>for</strong> each eye.<br />

IMAX movie projector Movie viewer using polarized glasses


Example. Partially polarized and partially unpolarized light.<br />

A light beam passes through a polarizer whose transmission axis makes<br />

angle θ with the vertical. The beam is partially polarized and<br />

partially unpolarized, and the average intensity of the incident light,<br />

S 0 , is the sum of the average intensity of the polarized light, S 0,polar ,<br />

and the average intensity of the unpolarized light, S 0,unpolar .<br />

As the polarizer is rotated clockwise, the intensity of the transmitted light<br />

has a minimum value of 2.0 W/m 2 when θ = 20.0 o and has a maximum<br />

value of 8.0 W/m 2 when the angle is θ = θ max .<br />

è Find a) S 0,unpolar , and b) S 0,polar .<br />

Incident light<br />

S 0 = S 0,polar + S 0,unpolar<br />

Transmitted light<br />

S = S polar + S unpolar


Incident light<br />

S 0 = S 0,polar + S 0,unpolar<br />

Transmitted light<br />

S = S polar + S unpolar<br />

a) Minimum transmitted intensity S = S min = 2.0 W/m 2 at θ = 20.0 o .<br />

S is minimum when S polar = 0 since S unpolar is not effected by θ.<br />

S unpolar = S min - S polar = 2.0 - 0 = 2.0 W/m 2<br />

S unpolar = ½ S 0,unpolar è S 0,unpolar = 2S unpolar = 2(2.0) = 4.0 W/m 2<br />

b) Maximum transmitted intensity S = S max = 8.0 W/m 2 occurs at θ max .<br />

S is maximum when S polar = S 0,polar (when θ = 20 o + 90 o = 110 o = θ max )<br />

S max = S 0,polar + S unpolor è S 0,polar = S max - S unpolar = 8.0 - 2.0 = 6.0 W/m 2


Polarization and the Reflection and Refraction of Light<br />

For air/water<br />

interface:<br />

θ p<br />

θ p<br />

n 1 =1.00, n 2 =1.33 ⇒ θ p = tan −1 1.33<br />

n 1 sinθ p = n 2 sinθ 2 ⇒ θ 2 = sin<br />

θ p +θ 2 = 90 o à Always true at θ p<br />

Reflected light is<br />

100% horizontally<br />

polarized at the<br />

polarizing angle, θ p<br />

Brewster’s law<br />

tanθ p = n 2<br />

n 1<br />

# &<br />

% ( = 53.1<br />

$ 1.00 '<br />

o<br />

−1 ( 1.00)sin53.1<br />

o<br />

)<br />

,<br />

+<br />

. = 36.9<br />

* 1.33 -<br />

o


Chapter 25<br />

Optical Instruments<br />

and the Eye


Cameras<br />

IMAGE FORMATION BY A CONVERGING LENS IN A CAMERA<br />

When the object is placed further than twice the focal length<br />

from the camera lens, the real image is inverted and smaller<br />

than the object on the film or ccd chip.


Cameras<br />

Example: Taking a picture of a flower vase with a ccd camera.<br />

A 0.500 m high flower vase is positioned 2.00 m in front of a ccd camera.<br />

The camera uses a converging lens whose focal length is 60.0 mm.<br />

(a) How far must the ccd be from the lens to have a sharp image?<br />

(b) Find the height of the image on the ccd.<br />

(c) If the lens diameter is 3.0 cm, find the f-stop of the lens.<br />

(d) If a properly exposed picture is taken with this f-stop with a shutter<br />

speed of 1/500 s, what f-stop is needed <strong>for</strong> a shutter speed of 1/125 s<br />

so that the picture is not overexposed?<br />

(a)<br />

(b)<br />

1<br />

d i<br />

= 1<br />

f<br />

− 1<br />

d o<br />

=<br />

1<br />

0.0600 m −<br />

d i = 0.0619 m = 61.9 mm<br />

h i = − d i<br />

d o<br />

h o = − 0.0619<br />

2.00<br />

1<br />

2.00 m<br />

=16.17 m−1<br />

0.500 = −0.0155 m = −15.5 mm


(c)<br />

f − stop =<br />

= 60 mm<br />

f<br />

Diameter of lens opening<br />

30 mm<br />

= 2.0 ⇒ f / 2<br />

= f<br />

D<br />

(d) For the picture not to be overexposed, we must reduce the lens area<br />

by the ratio of the shutter speeds, i.e.<br />

A final =<br />

!<br />

#<br />

"<br />

π D final<br />

2<br />

1 500<br />

1 125 Ainitial = 1<br />

4 Ainitial $<br />

&<br />

%<br />

2<br />

= 1<br />

f − stop final =<br />

!<br />

#<br />

4 π Dinitial " 2<br />

f<br />

D final<br />

= 2<br />

$<br />

&<br />

%<br />

2<br />

f<br />

D initial<br />

⇒ D final = 1<br />

2 D initial<br />

= 2( 2.0)<br />

= 4.0 ⇒ f / 4


The Human Eye<br />

ANATOMY


The Human Eye<br />

OPTICS<br />

The lens only contributes about 20-25% of the refraction, but its function<br />

is important.<br />

Normal eye near point, i.e. nearest point <strong>for</strong> com<strong>for</strong>table focusing, N = 25 cm<br />

Normal eye far point, i.e. farthest point <strong>for</strong> com<strong>for</strong>table focusing à ∞


The Human Eye<br />

NEARSIGHTEDNESS<br />

The lens creates an image of the distance object at the far point<br />

of the nearsighted eye.


The Human Eye<br />

Example: Eyeglasses <strong>for</strong> the Nearsighted Person<br />

A nearsighted person has a far point and near point located at only 10.0 cm<br />

and 8.0 cm, respectively, from the eye. Assuming that eyeglasses are to be<br />

worn 2.0 cm in front of the eye, find (a) the focal length needed <strong>for</strong> the lens<br />

of the glasses so the person can see distant objects and (b) the resulting<br />

location of the near point when the person is wearing these glasses.


The Human Eye<br />

(a)<br />

(b)<br />

do = ∞, di = −( 10.0 − 2.0)<br />

= −8.0 cm<br />

1<br />

f<br />

= 1<br />

d o<br />

+ 1<br />

d i<br />

= 1<br />

∞ +<br />

1<br />

−8.0<br />

( )<br />

di = −( 8.0 − 2.0)<br />

= −6.0 cm<br />

1<br />

d o<br />

= 1<br />

f<br />

− 1<br />

d i<br />

=<br />

1<br />

( −8.0)<br />

−<br />

∴ N = 24.0 + 2.0 = 26.0 cm<br />

= −<br />

1<br />

8.0 cm<br />

We want a virtual,<br />

upright image at the<br />

person’s near point<br />

We want a virtual,<br />

upright image at the<br />

person’s far point<br />

⇒ f = −8.0 cm<br />

f < 0, diverging lens<br />

1<br />

−6.0<br />

( ) = 0.0417 cm−1 ⇒ d o = 24.0 cm<br />

Close to the normal<br />

near point of 25 cm


The Human Eye<br />

FARSIGHTEDNESS<br />

The lens creates an image of the close object at the near point<br />

of the farsighted eye.


Example: Eyeglasses <strong>for</strong> the Farsighted Person<br />

A farsighted person has a near point located at 75.0 cm. from the eye.<br />

Assuming that eyeglasses are to be worn 2.0 cm in front of the eye,<br />

find the focal length needed <strong>for</strong> the lens of the glasses so the person’s<br />

near point with glasses is 25.0 cm.


do = 25.0 − 2.0 = 23.0 cm, di = −( 75.0 − 2.0)<br />

= −73.0 cm<br />

1<br />

f<br />

= 1<br />

d o<br />

+ 1<br />

d i<br />

f = 33.6 cm<br />

= 1<br />

23.0 +<br />

1<br />

−73.0<br />

( )<br />

f > 0, converging lens<br />

= 0.0298 cm−1<br />

We want a virtual,<br />

upright image at the<br />

person’s near point


The Human Eye<br />

THE REFRACTIVE POWER OF A LENS – THE DIOPTER<br />

Optometrists who prescribe correctional lenses and the opticians<br />

who make the lenses do not specify the focal length. Instead<br />

they use the concept of refractive power.<br />

Refractive<br />

power<br />

(in<br />

diopters)<br />

=<br />

f<br />

1<br />

( in meters)


Example: What refractive power, in diopters, would the optometrist<br />

prescribe <strong>for</strong> the lenses found in the last two examples, i.e. nearsighted<br />

and farsighted?<br />

Refractive power (in diopters) = P =<br />

Nearsighted example :<br />

f = −8.0 cm = −0.080 m<br />

P = 1<br />

f =<br />

1<br />

−0.080<br />

( )<br />

Farsighted example :<br />

f = 33.6 cm = 0.336 m<br />

P = 1<br />

f =<br />

1<br />

0.336<br />

= −12.5 D<br />

= +2.98 D<br />

1<br />

f in meters<br />

( )


Angular Magnification and the Magnifying Glass<br />

The size of the image on the retina determines how large<br />

an object appears to be.


Angular Magnification and the Magnifying Glass<br />

θ<br />

( in radians)<br />

=<br />

Angular size<br />

≈<br />

h<br />

d<br />

o<br />

o


Angular Magnification and the Magnifying Glass<br />

Example: A Penny and the Moon<br />

Compare the angular size of a penny held at arms length with that of<br />

the moon.<br />

Penny<br />

Moon<br />

θ ≈<br />

θ<br />

≈<br />

h<br />

d<br />

h<br />

d<br />

o<br />

o<br />

o<br />

o<br />

1.<br />

9 cm<br />

=<br />

71cm<br />

3.<br />

5×<br />

10<br />

=<br />

3.9×<br />

10<br />

=<br />

6<br />

8<br />

0.<br />

0<strong>27</strong><br />

m<br />

m<br />

=<br />

rad<br />

0.<br />

0090<br />

rad


Angular Magnification and the Magnifying Glass<br />

Angular magnification<br />

Special cases:<br />

Relaxed focus<br />

M<br />

=<br />

θʹ′<br />

θ<br />

di = −∞ ⇒ M ≈ N 1 %<br />

'<br />

& f<br />

Focus at N<br />

θ ' ≈ ho , θ ≈<br />

do ho N<br />

M ≈ h o d o<br />

h o N<br />

= N<br />

d o<br />

di = −N ⇒ M ≈ N 1 %<br />

'<br />

& f<br />

= N 1 #<br />

%<br />

$ f<br />

− 1<br />

−∞<br />

( )<br />

− 1<br />

−N<br />

( )<br />

(<br />

*<br />

)<br />

= N<br />

− 1<br />

d i<br />

(<br />

*<br />

)<br />

= N<br />

f<br />

&<br />

(<br />

'<br />

f +1


Example of a magnifying glass: A magnifying glass has a focal<br />

length of 9.5 cm. Find the magnification of the lens when used<br />

(a) with a relaxed eye, and (b) with the image at N=25 cm.<br />

f = 9.5 cm<br />

(a) M ≈ N<br />

f<br />

(b) M ≈ N<br />

f<br />

25<br />

=<br />

9.5 = 2.6 times d ( o = f = 9.5 cm)<br />

25<br />

+1=<br />

9.5 +1= 3.6 times d ( o = 6.9 cm)

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