Dr. G. Mirjalili, physics Dept. Yazd University Applied optics Wave fronts
Dr. G. Mirjalili, physics Dept. Yazd University
Applied optics
Wave fronts
Dr. G. Mirjalili, physics Dept. Yazd University
Geometrical OpticsIn describing the propagation of
light as a wave we need to understand:
wavefronts: a surface passing through points of a wave that have the same phase and amplitude.
rays: a ray describes the direction of wave propagation. A ray is a vector perpendicular to the wavefront.
Dr. G. Mirjalili, physics Dept. Yazd University
Wavefronts• We can chose to associate
the wavefronts with the instantaneous surfaces where the wave is at its maximum.
• Wavefronts travel outward from the source at the speed of light: c.
• Wavefronts propagate perpendicular to the local wavefront surface.
Dr. G. Mirjalili, physics Dept. Yazd University
Light Rays
• The propagation of the wavefronts can be described by light rays.
• In free space, the light rays travel in straight lines, perpendicular to the wavefronts.
Dr. G. Mirjalili, physics Dept. Yazd University
The ray approximation in geometric optics
• Geometric optics: The study of the propagation of light.
• Ray approximation: In the ray approximation, we assume that a wave moving through a medium travels in a straight line in the direction of its rays.
Dr. G. Mirjalili, physics Dept. Yazd University
Huygens’ principle Huygens’ principle
Every point of a wave front may be considered the source of secondarywavelets that spread out in all directions with a speed equal to the speedof propagation of the wave.
Plane waves
Dr. G. Mirjalili, physics Dept. Yazd University
• At t = 0, the wave front is indicated by the plane AA’
• The points are representative sources for the wavelets
• After the wavelets have moved a distance st, a new plane BB’ can be drawn tangent to the wavefronts
Huygens’ principle (cont’d) Huygens’ principle for plane wave
Dr. G. Mirjalili, physics Dept. Yazd University
• The inner arc represents part of the spherical wave
• The points are representative points where wavelets are propagated
• The new wavefront is tangent at each point to the wavelet
Huygens’ principle (cont’d) Huygens’ principle for spherical wave (cont’d)
Dr. G. Mirjalili, physics Dept. Yazd University
• The law of reflection can be derived from Huygen’s Principle
• AA’ is a wave front of incident light
• The reflected wave front is CD
Huygens’ principle (cont’d) Huygens’ principle for law of reflection
• Triangle ADC is congruent to
triangle AA’C
• Angles 1 = 1’
• This is the law of reflection
Dr. G. Mirjalili, physics Dept. Yazd University
• In time t, ray 1 moves from A to B and ray 2 moves from A’ to C
• From triangles AA’C and ACB, all the ratios in the law of refraction can be found:
n1 sin 1 = n2 sin 2
Huygens’ principle (cont’d) Huygens’ principle for law of refraction
22
11
2
2
1
1
2211
,,sinsin
sin;sin
n
cv
n
cv
tvtv
tvtv
AC
Dr. G. Mirjalili, physics Dept. Yazd University
Reflection
• Reflection: When a light ray traveling in one medium encounters a boundary with another medium, part of the incident light is reflected.– Specular reflection: Reflection of light from a
smooth surface, where the reflected rays are all parallel to each other.
– Diffuse reflection: Reflection from any rough surface, where the reflected rays travel in random directions.
– we use the term reflection to mean specular reflection.
Dr. G. Mirjalili, physics Dept. Yazd University
Reflection and refraction
Reflection (cont’d)
Dr. G. Mirjalili, physics Dept. Yazd University
The Law of reflection
• Law of reflection: The angle of reflection equals the angle of incidence: 1
’ = 1.• Some definitions:
– Normal: The normal is a line drawn perpendicular to the surface at the point where the incident ray strikes.
– Angle of reflection and incidence: Measured from the normal to the reflected and incident rays, respectively.
Dr. G. Mirjalili, physics Dept. Yazd University
Example : The double-reflected light ray
• Two mirrors make an angle of 120° with each other. A ray is incident on mirror M1 at an angle of 65° to the normal. Find the direction of the ray after it is reflected from mirror M2.
=2
Dr. G. Mirjalili, physics Dept. Yazd University
Practical applications of reflection
• Retroreflection: If the angle between the two mirrors is 90°, the reflected beam will return to the source parallel to its original path.
Dr. G. Mirjalili, physics Dept. Yazd University
Refraction• Refraction: When a ray of light traveling through
a transparent medium encounters a boundary leading into another transparent medium, part of the ray enters the second medium. The part that enters the second medium is bent at the boundary and is said to be refracted.
• sin2 / sin1 = v2 / v1
1 and 2 are the angle of incidence and angle of refraction, respectively.
– v1 and v2 are the speed of the light in the first and second medium, respectively.
• The path of a light ray through a refracting surface is reversible. All rays and the
normal lie in the same plane.
Dr. G. Mirjalili, physics Dept. Yazd University
Reflection by plane surfacesr1 = (x,y,z)
x
y
r2 = (x,-y,z)
Law of Reflection
r1 = (x,y,z) → r2 = (x,-y,z)
Reflecting through (x,z) plane
x
y
zr2= (-x,y,z)
r3=(-x,-y,z)
r4=(-x-y,-z)
r1 = (x,y,z)
Dr. G. Mirjalili, physics Dept. Yazd University
n2
Refraction by plane interface& Total internal reflection
n1
n1 > n2
θC
P
θ1θ1
θ1 θ1
θ2
θ2
Snell’s law n1sinθ1=n2sinθ2
Dr. G. Mirjalili, physics Dept. Yazd University
Examples of prisms and total internal reflection
45o
45o
45o
45o
Totally reflecting prism
Porro Prism
Dr. G. Mirjalili, physics Dept. Yazd University
Total internal reflection
Total internal reflection
,sinsin 21
21 n
nSince 1sin 2 when .sin&1/ 11212 nnnn
When this happens, is 90o and is called critical angle. Furthermore2 1when , all the light is reflected (total internal reflection). crit 1
Dr. G. Mirjalili, physics Dept. Yazd University
Total internal reflection
Optical fibers
Dr. G. Mirjalili, physics Dept. Yazd University
Index of Refraction and Snell’s Law of Refraction
• Index of refraction n of a medium: n c/v– c = 3 x 108 m/s: speed of light in vacuum.– v: speed of light in the medium; v < c.– n > 1 for any medium and n = 1 for vacuum (or
approximately in air).• Snell’s law of refraction: n1sin1=n2sin2 • As light travels from one medium to another, its
frequency does not change but its wavelength does. 1n1 = 2n2, or 1/2 = v1/v2.
• Light slows on entering a medium – Huygens
• Also, if n → ∞ = 0
• i.e. light stops in its track !!!!!
Dr. G. Mirjalili, physics Dept. Yazd University
n1 = 1.5 n2 = 1.0
Reflections, Refractive offset
• Let’s consider a thick piece of glass (n = 1.5), and the light paths associated with it
– reflection fraction = [(n1 – n2)/(n1 + n2)]2
– using n1 = 1.5, n2 = 1.0 (air), R = (0.5/2.5)2 = 0.04 = 4%
incoming ray(100%)
96%
92% transmitted0.16%
4%
4%
8% reflected in tworeflections (front & back)
image looks displaceddue to jog
Dr. G. Mirjalili, physics Dept. Yazd University
Atmospheric Refraction and Sunsets
• Light rays from the sun are bent as they pass into the atmosphere
• It is a gradual bend because the light passes through layers of the atmosphere – Each layer has a slightly
different index of refraction
• The Sun is seen to be above the horizon even after it has fallen below it
Dr. G. Mirjalili, physics Dept. Yazd University
Mirages
• A mirage can be observed when the air above the ground is warmer than the air at higher elevations
• The rays in path B are directed toward the ground and then bent by refraction
• The observer sees both an upright and an inverted image
Dr. G. Mirjalili, physics Dept. Yazd University
Example: depth of a swimming pool
Pool depth s = 2m
person looks straight down.
the depth is judged by the apparent size of some object of length L at the bottom of the pool (tiles etc.)
s`is reduced distance
L
Dr. G. Mirjalili, physics Dept. Yazd University
L
21
2
1
21
tan)(tan
'tan
tan
sinsin
sss
s
L
ss
Ls
L
na
for small angles: tan ->sin
.504
1)2(
1
sin)(sin
sin)(sin
11
21
cmmn
nss
nsss
sss
a
a
a
Dr. G. Mirjalili, physics Dept. Yazd University
Example: Flat refracting surface
• The image formed by a flat refracting surface is on the same side of the surface as the object– The image is virtual– The image forms between
the object and the surface– The rays bend away from
the normal since n1 > n2
sn
ns
s
n
s
n
1
221 ''
L
)sinsin( '
sinsin'
1for sintan
tantan'tan||,tan|'|
221121
21
2121
nnsnsn
ss
ssLsLs
s’
s
Dr. G. Mirjalili, physics Dept. Yazd University
• Light is refracted twice – once entering and once leaving. • Since n decreases for increasing , a spectrum emerges...
Analysis: (60 glass prism in air)
1 2
4
n2 = 1.5
n1 = 1 60
sin 1 = n2 sin 2
n2 sin 3 = sin 4
3
3 = 90 - = 90 - 2 3 = 60 - 2
Example: 1 = 30
o
oo
o
9.76sin5.1sin
5.40)60(
5.195.1
)30sin(sin
31
4
23
12
o = o
Prism example
Dr. G. Mirjalili, physics Dept. Yazd University
Prisms
Applications of prism
• A prism and the total reflection can alter the direction of travel of a light beam.“Diversion, Deviation”
• All hot low-pressure gases emit their own characteristic spectra. A prism spectrometer is used to identify gases.“Dispersion”
Dr. G. Mirjalili, physics Dept. Yazd University
Dispersion &Deviation
Little dispersion
High deviation
High dispersion
Low
deviation
n1 n2
n1<n2
Dr. G. Mirjalili, physics Dept. Yazd University
Angular Dispersion
A hollow 600 prism is filled with carbon disulfide, whose index of refraction for blue is 1.652, for red light is 1.618 what is angular dispersion
2
1sin
)(2
1sin
0
n
n prism
n1=1.652 n2=1.618
1=51.380 2=48.00
1-2 =3.380 angular dispersion
Dr. G. Mirjalili, physics Dept. Yazd University
Deviation & wavenumber in prism
• Deviation angle &
b+nt1+d=c+nt2+e
b+(n+ n)t1+d+a D=c+ (n+ n)t2+e
nt1+a D=n t2
D/ =(t2-t1)/a
A
B
A`b
c
d
e
t1
t2
A``
aD
a
dD/dn = (t2-t1)/a
dD/dn =t/a
dD/d=(dD/dn)(dn/d)=(t/a) (dn/d)
(dn/d)=?
Dr. G. Mirjalili, physics Dept. Yazd University
Deviation angle &
n = A+B/2
dn/d = -2B/3
dD/d = t/a dn/ddD/d = t/a(-2B/3)
Dr. G. Mirjalili, physics Dept. Yazd University
Dispersive power & Abbe`s nunber
1
D
cf
n
nnDispersive power
numbersAbbenn
n
Cf
D `1
Low dispersion, low refractive index
Dr. G. Mirjalili, physics Dept. Yazd University
Refractive indices of Crown and flint glasses
Fraunhofer line
color (nm) n crown n flint
F
D
C
Blue
Yellow
Red
486.1
589.3
656.3
1.5293
1.5230
1.55204
1.7378
1.7200
1.7130
Crown =59 flint=29
Dr. G. Mirjalili, physics Dept. Yazd University
Dispersing prisms
• Achromatic prism:
• Deviates light but gives no dispersion
1
2
Dispersion for 1 and 2 is zero
Dr. G. Mirjalili, physics Dept. Yazd University
Dispersing prisms
• Direct-vision prism
1
2
Direct vision for wavelength
Dr. G. Mirjalili, physics Dept. Yazd University
example• Assume that 140 is the apex angle of a crown glass prism. What
should be the apex angle of a flint prism:(a)-if the combination of both is to be achromatic for blue and red?(b)-if the prism is to have no deviation for yellow?Solution (a)
F = 1(nf - 1)
C = 1(nc- 1) → f - c = 1 (nf - nc) mean dispersion of prism
For the combination to be achromatic,
(1)(n1f - n1c) + (2)(n2f - n2c)=0
(14)(1.5293-1.5204)+ (2)(1.7378-1.7130)=0
2= -50
Dr. G. Mirjalili, physics Dept. Yazd University
Example (cont.)
• (b) for the direct-vision prism
1=1(n1D-1)
2=2(n2D-1)
1(n1D-1)= 2(n2D-1)
14(1.5230-1)= 2(1.7200-1)
2=10.20
Dr. G. Mirjalili, physics Dept. Yazd University
Image manipulation by reflection prisms
Right angle prism
Dr. G. Mirjalili, physics Dept. Yazd University
Image manipulation by reflection prisms
Dove prism
Dr. G. Mirjalili, physics Dept. Yazd University
Dispersion
Dispersion
• The index of refraction of a material depends on wavelength as shown on the right. This is called dispersion.
• It is also true that, although the speed of light in vacuum does not depends on wavelength, in a material, wave speed depends on wavelength.
Dr. G. Mirjalili, physics Dept. Yazd University
Diversion & dispersion
Examples
Dr. G. Mirjalili, physics Dept. Yazd University
Resolving power of a prism
+
d
b
Ts
FT+TW=nb
FT+ Tw - s= (n- n) b
s=b n
s=b (dn/d)
=s/d=(b/d)(dn/d)
F
d W
n
= /d
/d = (b/d)(dn/d)
()min= /b(dn/d)
R=/()min= b(dn/d)
Dr. G. Mirjalili, physics Dept. Yazd University
Resolving power of a prism (example)
• A prism made from flint glass with a base of 5 cm. find the resolving power of the prism at =550 nm.
• solution
n/=(nf-nD)/(f-D)= (1.7328-1.7205)/(486-587)=-1.9x10 -4 nm -1
R = b(dn/d) = (0.05x10 9nm)(-1.9x10 -4 nm -1) = 5971
()min=/R =5500A0/5971 ≈ 1 A0
Dr. G. Mirjalili, physics Dept. Yazd University
•Exercises
Dr. G. Mirjalili, physics Dept. Yazd University
ExercisesExample
Solution
m
n
A
A
The prism shown in the figure has a refractiveindex of 1.66, and the angles A are 25.00 . Twolight rays m and n are parallel as they enterthe prism. What is the angle between themthey emerge?
.6.44)00.1
0.25sin66.1(sin)
sin(sinsinsin 11
b
aabbbaa n
nnn
Therefore the angle below the horizon isand thus the angle between the two emerging beams is
,6.190.256.440.25 b.2.39
Dr. G. Mirjalili, physics Dept. Yazd University
ExercisesExample
Light is incident in air at an angle on the upper surface of a transparentplate, the surfaces of the plate beingplane and parallel to each other. (a)Prove that (b) Show that thisis true for any number of different parallelplates. (c) Prove that the lateral displacementD of the emergent beam is given by therelation:
where t is the thickness of the plate. (d) A ray of light is incident at an angleof 66.00 on one surface of a glass plate 2.40 cm thick with an index ofrefraction 1.80. The medium on either side of the plate is air. Find the lateralDisplacement between the incident and emergent rays.
P
Q
n
n’
n
t
d
a
'a
b
'b
.'aa
,cos
)sin('
'
b
batd
Dr. G. Mirjalili, physics Dept. Yazd University
ExercisesProblem
Solution
P
Q
n
n’
n
t
d
a
'a
b
'b(a)For light in air incident on a parallel-faced
plate, Snell’s law yields:
(b) Adding more plates just adds extra steps in the middle of the above equation that always cancel out. The requirement of parallel faces ensures that the angle and the chain of equations can continue.(c) The lateral displacement of the beam can be calculated using geometry:
(d)
.sinsinsinsin'sin'sin ''''aaaaabba nnnn
'nn
.cos
)sin(
cos),sin(
'
'
''
b
ba
bba
td
tLLd
L
.62.15.30cos
)5.300.66sin()40.2(
5.30)80.1
0.66sin(sin)
'
sin(sin 11'
cmcm
d
n
n ab