EM Waves: Lecture Notes on Electromagnetic Waves, Study notes of Geology

A set of lecture notes on electromagnetic waves. It covers topics such as the properties of em waves, their velocity, the poynting vector, energy density, polarization, and the effect of polarizing sheets on the intensity of em waves.

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Uploaded on 07/28/2009

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Lecture 32
Chapter 34
Electromagnetic Waves
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Lecture 32

Chapter 34

Electromagnetic Waves

Review

ï^

EM Waves ññ Wavelengths of 10

8

to

10

-

16

meters (10-

24

Hz)

ñ Traveling wave of both

E

and

B

fields

ñ

E

field is

⊥⊥⊥⊥

B

field

ñ Wave moves in direction

⊥⊥⊥⊥

to both

E

and

B

fields

ñ

E

and

B

vary sinusoidally

with same frequency ñ At large distances fields

are in phase

B

E

r

r

×

)

sin(

t

kx

E

E

m

ω −

=

)

sin(

t

kx

B

B

m

ω −

=

Review

ï^

Poynting vector,

S

ñ rate of

energy transported per unitarea ï^

Instantaneous energy flow rate ï^

Defined intensity

I

to be time

averaged value of

S

2

0

rms

avg

E
c
S
I

μ

ave

ave

avg

powerarea

area

time

energy

S I^

  

  

  

  

=

/

B

E

S

r

r

r^

×

EB

S

0

=

EM Waves (12)

ï^

Problem ñ Isotropic point light source as powerof 250 W. You are 1.8 meters away. Calculatethe rms values of the

E

and

B

fields.

ï^

To find

E

rms

need

ï^

Find intensity

I

from

2

0 1

rms E

c

I

μ

=

2

r

P

I^

s π

(^02)

0

4

c r P

Ic

E

s

rms

π

μ

μ

=

=

m V

E

rms

2

8

8

×
×

π

EM Waves (14)

ï^

Look at sizes of

E

rms

and

B

rms

ï^

This is why most instruments measure

E

ï^

Does not mean that

E

component is stronger

than

B

component in EM wave

ñ Canít compare different units ï^

Average energies are equal for

E

and

B

T

B

rms

7

10

(^6). 1

×

=

m

V

E

rms

/

(^1).

48

EM Waves (15)

ï^

The energy density of electric field,

u

E^

is equal

to energy density of magnetic field,

u

B

B

c

E

=

2 0 1 2

E

u

E

ε

=

2 2 0 1 2

2

0 1 2

)

(^

B c

cB

u

E

ε

ε

=

=

0

1 ε^0

μ

c

2 0

2 0 0 0

ε^

B
B

u

E^

2 0 2

B^ μ

u

B^

B

E

u

u

=

EM Waves (17)

ï^

Just defined intensity,

I

as power

per unit area

A

so power is

ï^

Change in energy is amount ofpower

P

in time

t

ï^

Want force of radiation on object ï^

For total absorption ï^

Find force is

I

A

P

t

IA

t

P

U

p^ t

F

∆ ∆

U c

p

IA^ c

t

c

t

IA

t

c

U

p t

F

EM Waves (18)

ï^

For total reflection back along original path ï^

Express in terms of radiation

pressure

p

r^

which is force/area

ï^

SI unit is N/m

2

called pascal

Pa

U c

p

IA c

t c

t

IA

t c

U

p t

F

2

2

2

=

=

∆ ∆

=

∆ ∆

F^ A

p

r^

=

I c

p

r^

=

I c

p

r

2

ï^

Total absorption

ï^

Total reflection

EM Waves (20)

ï^

Source emits EM waveswith random planes ofoscillation (

E

field changes

direction) is unpolarizedñ Example, light bulb or Sun ï^

Resolve

E

field into

components ï^

Draw unpolarized light assuperposition of 2 polarizedwaves with

E

fields

to

each other

EM Waves (21)

ï^

Transform unpolarizedlight into polarized byusing a polarizing sheet ï^

Sheet contains longmolecules embeddedin plastic which wasstretched to align themolecules in rows ï^

E

field component || to polarizing direction of sheet is passed (transmitted), but

component is absorbed

EM Waves (23)

ï^

For polarized light, resolve Einto components ï^

Transmitted || component is ï^

Use definition of intensity ï^

Cosine-squared rule: Intensity ofpolarized wave changes as cos

2 θθθθ

θ 2

0

cos I

I^

=

θ

cos E

E

y^

=

θ

θ

μ

μ

2 0 2 2 0 2 0

cos

cos

I
E

c

E

c

I^

EM Waves (24)

ï^

Have 2 polarizing sheetsñ First one called polarizerñ Second one called analyzer ï^

Intensity of unpolarizedlight going throughpolarizer is ï^

Light is now polarized andintensity of light afteranalyzer is given by

2

0

cos I

I

=

0

1 2

I

I^

=

EM Waves (26)

ï^

Look at relative orientation of polarizationdirection between the 2 sheets. ï^

What is the intensity if the sheets areÖñ Polarized || ñ all light passesñ Polarized

⊥⊥⊥⊥

to each other ñ no light passes

ñ For angles in between ñ get more light if closer to ||

a,d,b,c