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We define the intensity S, as the rate. of energy flow per unit area: ... Intensity of light at a distance r is S = P / 4pr2. Example: ... – PowerPoint PPT presentation

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1
Chapter 34
  • (continued)
  • The Laws of Electromagnetism
  • Maxwells Equations
  • Displacement Current
  • Electromagnetic Radiation

2
The Electromagnetic Spectrum
infra -red
ultra -violet
Radio waves
g-rays
m-wave
x-rays
3
Maxwells Equations of Electromagnetismin Vacuum
(no charges, no masses)
4
Plane Electromagnetic Waves
Ey
Bz
Notes Waves are in Phase, but fields
oriented at 900. k2p/l. Speed of wave is
cw/k ( fl) At all times EcB.
c
x
5
Plane Electromagnetic Waves
Ey
Bz
x
Note sin(wt-kx) -sin(kx-wt) ? notations are
interchangeable. sin(wt-kx) and sin(kx-wt)
represent waves traveling towards x, while
sin(wtkx) travels towards -x.
6
Energy in Electromagnetic Waves
  • Electric and magnetic fields contain energy,
    potential energy stored in the field uE and uB
  • uE ½ ?0 E2 electric field energy density
  • uB (1/?0) B2 magnetic field energy density
  • The energy is put into the oscillating fields by
    the sources that generate them.
  • This energy can then propagate to locations far
    away, at the velocity of light.

7
Energy in Electromagnetic Waves
Energy per unit volume is u uE uB
B
dx
area A
E
c
propagation direction
8
Energy in Electromagnetic Waves
Energy per unit volume is u uE uB Thus
the energy, dU, in a box of area A and length dx
is
B
dx
area A
E
c
propagation direction
9
Energy in Electromagnetic Waves
Energy per unit volume is u uE uB Thus
the energy, dU, in a box of area A and length dx
is Let the length dx equal cdt. Then all of
this energy leaves the box in time dt. Thus
energy flows at the rate
B
dx
area A
E
c
propagation direction
10
Energy Flow in Electromagnetic Waves
B
Rate of energy flow
dx
area A
E
c
propagation direction
11
Energy Flow in Electromagnetic Waves
B
Rate of energy flow
dx
area A
E
We define the intensity S, as the rate of energy
flow per unit area
c
propagation direction
12
Energy Flow in Electromagnetic Waves
B
Rate of energy flow
dx
area A
E
We define the intensity S, as the rate of energy
flow per unit area
c
propagation direction
Rearranging by substituting EcB and BE/c, we
get,
13
The Poynting Vector
B
In general, we find S (1/?0) E x B S
is a vector that points in the direction of
propagation of the wave and represents the rate
of energy flow per unit area. We call this the
Poynting vector. Units of S are Jm-2 s-1, or
Watts/m2.
dx
area A
E
propagation direction
14
The Inverse-Square Dependence of S
A point source of light, or any radiation,
spreads out in all directions
Power, P, flowing through sphere is same for
any radius.
Source
15
ExampleAn observer is 1.8 m from a point light
source whose average power P 250 W. Calculate
the rms fields in the position of the observer.
Intensity of light at a distance r is S P
/ 4pr2
16
ExampleAn observer is 1.8 m from a point light
source whose average power P 250 W. Calculate
the rms fields in the position of the observer.
Intensity of light at a distance r is S P
/ 4pr2
17
ExampleAn observer is 1.8 m from a point light
source whose average power P 250 W. Calculate
the rms fields in the position of the observer.
Intensity of light at a distance r is S P
/ 4pr2
18
Wave Momentum and Radiation Pressure
Momentum and energy of a wave are related by,
p U / c. Now, Force d p /dt
(dU/dt)/c pressure (radiation) Force / unit
area P (dU/dt) / (A c) S / c Radiation
Pressure ?
19
Example Serious proposals have been made to
sail spacecraft to the outer solar system using
the pressure of sunlight. How much sail area must
a 1000 kg spacecraft have if its acceleration is
to be 1 m/s2 at the Earths orbit? Make the sail
reflective.
Can ignore gravity. Need Fma(1000kg)(1
m/s2)1000 N This comes from pressure FPA, so
AF/P. Here P is the radiation pressure of
sunlight Suns power 4 x 1026 W, so
Spower/(4pr2) gives S (4 x 1026 W) /
(4p(1.5x1011m)2 ) 1.4kW/m2. Thus the pressure
due to this light, reflected, is P
2S/c 2(1400W/m2) / 3x108m/s
9.4x10-6N/m2 Hence A1000N / 9.4x10-6N/m2
1.0x108 m2 100 km2
20
Polarization
The direction of polarization of a wave is the
direction of the electric field. Most light is
randomly polarized, which means it contains a
mixture of waves of different polarizations.
Polarization direction
21
Polarization
A polarizer lets through light of only one
polarization
E
Transmitted light has its E in the direction of
the polarizers transmission axis.
E0
E
q
E E0 cosq hence, S S0 cos2q -
Maluss Law
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