Light: Basic principles
Dr Yoonchan Jeong
School of Electrical Engineering, Seoul National University
Office: 302-523 (temporary), Tel: +82 (0)2 880 1623, Fax: +82 (0)2 873 9953 Email: [email protected]
2
n = 1.406 (centre) n = 1.386 (edge)
n = 1. 337
n = 1. 336
Human eyes are not like a monochrometer!
Not everyone sees the same colours!
Eye optics degeneracy, variations in cone pigments, and different
psychological experience
Retina photoreceptors:
• Cones (s, m, l): sensitive to colours
• Rods: not sensitive to colours, dark- adapted
s m l
Visible: 400 ~ 700 nm
Human eye & colour vision
• Photopic vision:
– Perceived brightness with colours (cones)
– Most sensitive at 555 nm:
683 lm/W
– Perceived brightness is different with colours even with the same optical power!
– More important to displays
• Scotopic vision:
– Dark adapted (rods)
– Most sensitive at 507 nm:
1700 lm/W
Brightness perception
Laser safety
CLASS 1 LASER PRODUCT LASER RADIATION
DO NOT VIEW DIRECTLY WITH OPTICAL INSTRUMENTS CLASS 1M LASER PRODUCT
LASER RADIATION
DO NOT STARE INTO BEAM CLASS 2 LASER PRODUCT
LASER RADIATION
DO NOT STARE INTO BEAM OR VIEW DIRECTLY WITH OPTICAL INSTRUMENTS CLASS 2M LASER PRODUCT
LASER RADIATION
AVOID DIRECT EYE EXPOSURE CLASS 3R LASER PRODUCT
LASER RADIATION
AVOID EXPOSURE TO BEAM CLASS 3B LASER PRODUCT
LASER RADIATION
AVOID EYE OR SKIN EXPOSURE TO DIRECT OR SCATTERED RADIATION CLASS 4 LASER PRODUCT
e.g. 0.39 mW @600 nm
1 mW @400 - 700 nm
0.5 W 5 mW
all lasers with beam power higher than class 3B
Protective eyewear required !
Frequency
(Hz)
Wavelength
(m)
1THz
1GHz
1MHz
1kHz
21cm H line
h
Photon energy (eV)
1MeV
1keV
h
Photon energy
(J)
-RAYS
X-RAYS ULTRAVIOLET
1020
1027
1022
101 4
101 2
109
106
103
106
103
101
106
101 1
LIGHT INFRARED
MICROWAVES
RADIOFREQUENCY
UHF VHF TV
Radar FM Radio Broadcast
Power Lines
Outer electrons Eye Arcs
1eV 100 1nm 1Å
1cm 1m
1km 1013
1010
109
102
100
102
103
105
1mm 106
101 5 19
10 1018
10
1014
MICROSCOPIC
SOURCE DETECTION
ARTTIFICIAL GENERATION Atomic
nuclei Inner electrons Inner and Outer electrons Molecular vibrations
and rotations Electron spin
Nuclear spin
Geiger and scintillation Ionization
chamber Photoelectric Photomultiplie
r Bolometer Thermopile
Crystal Electronic
circuits
Accelerators X-ray tubes Synchrotrons
Lasers Sparks Lamps Hot bodies Magnetron Klystron Travelling-wave
tube Electronic
circuits AC generators
Electromagnetic-Photon Spectrum
Visible Light (400 nm ~ 700 nm)
Maxwell’s Equations
Maxwell’s Equations
Constitutive Equations
0
0
B D
D J H
E B
t
t
Faraday’s law Ampère’s law Gauss’s lawNo free magnetic monopole (?)
M H
H B
P E E
D
o o
m m
(
on
2, m m
o)
Isotropic and non-magneticWave Equations
Wave Equations
Plane Wave
Phase Velocity
0 ,
0 2
2 2
2 2
2
t t
H H
E m E m (Homogeneous and no source)
m
ei(tkr), k
s m c
t k
o o
/ 10 997930
. 1 2
1 , v
constant,
8 p
m
m
k r
) ,
( ) , ( .
.g f x t f x x t t
e
Boundary Conditions
Continuity Relations
0
0
B D
D J H
E B
t
t
Tangential Comp.Tangential Comp.
Normal Comp.
Normal Comp.
K H
H
n( 2 1)
(D2 D1) n
0 ) ( 2 1
B B n
0 ) ( 2 1
E E
n
1 2
n
1 2
C
Reflection and Refraction
Ei Hi ki
Er Hr
kr qi qr
qt Et Ht kt
Plane of Incidence ni
nt
Hi Ei ki
Hr Er
kr qi qr
qt Ht Et kt
Plane of Incidence ni
nt
P-Polarization (TM) S-Polarization (TE)
Snell’s Law
t t
i
i n
n sin
q
sinq
Field continuity of tangential components0 10 20 30 40 50 60 70 80 90 0.0
0.2 0.4 0.6 0.8 1.0
ni < nt
ni = 1, nt = 1.5 P-Polarization S-Polarization
Reflectivity
Incident Angle qi [deg]
Brewster
angle 0 10 20 30 40 50 60 70 80 90
0.0 0.2 0.4 0.6 0.8 1.0
ni > nt
ni = 1.5, nt = 1 P-Polarization S-Polarization
Reflectivity
Incident Angle qi [deg]
Critical angle
Brewster Angle and Critical Angle
Brewster Angle Critical Angle
Reflectivity
) ( tan
1i t
B
n
n q
2
q
q
i t
) ( sin
1i t
c
n
n q
,
q
2 t t
i n
nFor P-polarization Total internal reflection
Polarization and Anisotropy
Constitutive Relation for Electrical Field
P E E
D
o
Biaxial Uniaxial
Isotropic
n n
n
n n
n
n n
n
n n
n
z y
x
z y
x
z y
x
z y
x o
2 2
2
0 0
0 0
0 0
with
k Surface Index Ellipsoid Double Refraction
Dispersion
Natural Dispersion RAINBOW
White light
Prism
Material Dispersion
White light which is a mixture of colors is separated into its different wavelengths.
Refractive index
n
is inherently a function of wavelength.Recall Snell’s law!
t t
i
i n
n sin
q
sinq
Scattering
Rayleigh Scattering
- When an electromagnetic radiation hits a particle whose diameter is smaller than the wavelength of the radiation
- Short wavelength is scattered more than long wavelength
Mie Scattering
- When an electromagnetic radiation hits a particle whose diameter is similar or greater than the wavelength of the radiation
- Roughly independent of wavelength
Phenomenon
- Interaction between an electro- magnetic radiation and small particles or molecules
- Different wavelengths get
deflected in different directions.
4
~ 1
Source: http://www.vislab.usyd.edu.au/photonics/
Scattering
Rayleigh scattering Mie scattering
No scattering
Diffraction and Interference
Diffraction
A wave such as light is bent when it passes an edge or through an
aperture. The aperture or the edge acts as a radiating point (Huygens–
Fresnel principle).
This effect increases as the physical dimension of the aperture is close to the wavelength of the wave.
Constructive Interference
Destructive Interference
Interference by Multiple Reflection
Fabry-Perot Interferometer
q m nd cos 2
Constructive interference (100 % transmission)