Chapter 18.
Matrix Methods in paraxial optics Chapter 18.
Matrix Methods in paraxial optics
< Cardinal points (planes) >
Focal (F) points (planes)
• EFL: Effective Focal Length (or simply “focal length”)
• FFL: Front Focal Length
• BFL: Back Focal Length Principal (H) surface (planes) Nodal (N) points (planes)
< Matrix methods to find the cardinal points in paraxial optics >
Ray-transfer matrix
• Translation Matrix
• Reflection Matrix
• Refraction Matrix
• Lens Matrix
• Mirror Matrix
Complex optical systems Complex optical systems
Thick lenses, combinations of lenses etc..
Thick lenses, combinations of lenses etc..
tt
n
n
LLn n n n ’ ’
Consider case where
Consider case where tt is not negligible. is not negligible.
We would like to maintain our Gaussian We would like to maintain our Gaussian imaging relation
imaging relation
R P n R
s n n s
n
L
2 1
1 ) 1
' ' (
'
But where do we measure
But where do we measure s, s
s, s
’’
; f, f; f, f
’’
from? How do we determinefrom? How do we determine
PP
?? We try to develop a formalism that can be used with any system!!
We try to develop a formalism that can be used with any system!!
We need to define cardinal points (planes) :
focal (F), principal (H), and nodal (N) points (planes)
Example: Focal Lengths & Principal Planes
generalized optical system (e.g. thick lens, multi-element system)
EFL: Effective Focal Length (or simply “focal length”) FFL: Front Focal Length
BFL: Back Focal Length
FP: Focal Point/Plane
PS: Principal Surface/Plane
The significance of principal planes
object
multi-element optical system
lateral hold, where f= (EFL)
Utility of principal planes Utility of principal planes
H
H
22ƒ’ƒ’
FF22 H
H
11ƒƒ FF11
s s’
n
n
LLn n n n ’ ’
hh
h’h’
Suppose
Suppose s, s s, s’ ’, f, f , f, f’ ’ all measured from H all measured from H
11and H and H
22… …
' 1 '
f f
s s
' '
f f
n n 1 1 1
if '
' n n
s s f
Cardinal points and planes:
1st Focal points (F1)Cardinal points and planes:
1st Focal points (F1)제 1 초점 (first focal point, object side focal point): F
1 무한대에 상이 생기는 축 상 물체 점
상 측에서 광 축과 평행하게 입사한 광선이 모이는 점, 또는, 모이는 것처럼 보이는 점.
u'k=0
1 k
...
F1
u'k=0
1 k
...
F1
Cardinal points and planes:
2nd Focal points (F2)Cardinal points and planes:
2nd Focal points (F2). . .
F'
1 k (마지막 면)
u =01
F'
1 k
u =0
1제 2 초점 (second focal point, image side focal point) : F
2 무한대에 있는 축 상 물체 점의 상점
광축과 평행하게 입사한 광선이 모이는 점(실상), 또는, 모이는 것처럼 보이는 점(허상)
F2
F2
1st Principal planes (PP
1) and points(H
1) 1st Principal planes (PP
1) and points(H
1)
n n
LLn n n’ n ’
H
H
11ƒƒ FF11
PPPP11
제 1 주요면 (물체측 주요면) : PP1
-상측에서 광축과 평행하게 입사한 광선을 물체측에서 보아 굴절되는 것처럼 보이는 가상면.
제1 주요점 (물체측 주요점 ): H1 – 제1 주요면과 광축의 교점.
2nd principal planes (PP
2) and points (H
2) 2nd principal planes (PP
2) and points (H
2)
n n
LLn n n’ n ’
H
H
22ƒ’ƒ’
FF22
PPPP22
제 2 주요면 (상측 주요면) : PP2
- 물체측에서 광축과 평행하게 입사한 광선을 상측에서 보아 굴절되는 것처럼 보이는 가상면.
제2 주요점 (상측 주요점 ): H2 - 제2 주요면과 광축의 교점.
Objective distance, image distance Objective distance, image distance
물체거리 (object distance)
: 제1 주요면에서 물체까지의 거리 s = HO
상거리 (image distance)
: 제2 주요면에서 상면까지의 거리 s’ = H’O’
l l'
1 k
H H'
h h
P P'
u1 u'k
o o'
s s’
n1 n'1
h1 A1= H1= H'1
u'1 u1
l1
l'1 면의 물체거리
면의 상거리 o
1 2
* 면에서 물체까지의 거리 l1, l2 등과는 다름.
l1
l2
Effective focal length & back focal length Effective focal length & back focal length
1 k...
u1=0
h1
hk
F' u'k
Ak H'
A1 H
bfl f'b
efl, f' fb
f
F u1
h1
hk
u'k=0
유효 초점거리(effective focal length, efl): f'
- 제2 주요점에서 제2초점까지의 거리 : efl = f’ = H’F’
후 초점거리(back focal length, bfl): f‘
b-광학계의 마지막 면의 정점에서 제2 초점까지의 거리 : bfl = f’b = AkF’
제2 주요면의 위치 = bfl - efl
efl, f’
bfl, f’b
Front focal length = Working distance of a lens Front focal length = Working distance of a lens
물체측 초점거리(Object side focal length): f
- 제1 주요점에서 제1 초점까지의 거리 : f = HF
앞 초점거리(front focal length): f
b = 작동거리 (working distance)- 제1면의 정점에서 제1초점까지의 거리 : fb = A1F
제1 주요면의 위치 : f
b - f1 k...
u1=0
h1
hk
F' u'k
Ak H'
A1 H
bfl f'b
efl, f' fb
f
F u1
h1
hk
u'k=0
efl, f’
bfl, f’b
f fb
Utility of principal planes Utility of principal planes
H
H
22ƒ’ƒ’
FF22 H
H
11ƒƒ FF11
s s’
n
n
LLn n n n ’ ’
hh
h’h’
Suppose
Suppose s, s s, s’ ’, f, f , f, f’ ’ all measured from H all measured from H
11and H and H
22… …
' 1 '
f f
s s
' '
f f
n n 1 1 1
if '
' n n
s s f
Nodal points (N
1, N
2) and Nodal planes (NP
1, NP
2) Nodal points (N
1, N
2) and Nodal planes (NP
1, NP
2)
n n n’ n ’
N N
22NPNP22
N N
11NPNP11
n n
LL절점(nodal point : N
1, N2) 광학계는 입사각과 출사각이 같은 광선이 1개 존재.
제1절점:이 광선을 물체측에서 보아 입사하는 것처럼 보이는 점.
제2절점:이 광선을 상측에서 보아 출사하는 것처럼 보이는 점.
Nodal point (N) and optical center (c) Nodal point (N) and optical center (c)
N' u N
u' c
1 2
광심(optical center : C) :
절점(nodal point)을 정의하는 하나의 광선 (입사각과 출사각이 같은 광선)이 실제로 광 축과 교차하는 점.
Nodal point 의 성질
i) 제1절점으로 입사한 광선은 제2절점에서 출사 (제1절점 - 광심 (C) - 제2절점) ii) 제1절점으로 입사한 광선은 입사각과 출사각이 같다.
iii) 상측 매질의 굴절률과 물체측 매질의 굴절률이 같으면 절점과 주요점은 같다.
N1 = H1 , N2 = H2
iv) 제2절점을 기준으로 광학계를 회전시키면 상의 위치는 변화하지 않는다.
F'
N2 N1 F'
C
Cardinal planes of simple systems Thin lens
Cardinal planes of simple systems Thin lens
s P n s
n '
'
Principal planes, nodal planes, Principal planes, nodal planes, coincide at center
coincide at center VV
H, H H, H’’ V’V’
V’ V ’ and V coincide and and V coincide and
is obeyed.
is obeyed.
Cardinal planes of simple systems Spherical refracting surface
Cardinal planes of simple systems Spherical refracting surface
n n n n ’ ’
Gaussian imaging formula Gaussian imaging formula obeyed, with all distances obeyed, with all distances measured from V
measured from V VV
s P n s
n '
'
Combination of two systems:
e.g. two spherical interfaces, two thin lenses … Combination of two systems:
e.g. two spherical interfaces, two thin lenses …
n n
22n n
HH
11 HH
11’’ n n ’ ’
HH
22 HH
22’’
H
H
tt’’
y y
Y Y
d d
ƒ ƒ
tt’ ’ ƒ ƒ
11’ ’
F
F
’’
FF
11’’
1. Consider F
1. Consider F’’ and Fand F11’’
h h ’ ’
Find
Find h h’ ’
Combination of two systems:
Combination of two systems:
n n
22n n n’ n ’
H
H
11’’
HH
11H
H
22 HH
22’’
HH
y y Y Y
d d ƒ ƒ
1. Consider F and F 1. Consider F and F22
F
F
22ƒ ƒ
22h h
F
F
Find
Find h h
Summary Summary
H
H
11’’
H
H
11 HH
22 HH
22’’
HH
H’H
’ƒ ƒ h h h h ’ ’ ƒ’ ƒ’
F
F
FF
’’
d d
n n
22n n n n ’ ’
Summary Summary
2 2 1 2
1
2 1
1 2 2
2 1
2 1
2 2
1 2
,
' '
' '
' '
'
' ' '
' '
n P d P
P P
P or
f n f
f dn f
n f
n f
n
n n P
d P H
f H d f
h
n n P
d P H
f H d f
h
Hecht, 6.1, p.214
Thick Lens Thick Lens
n n
22R R
11R R
22H
H
11,H,H
11’’
HH
22,H,H
22’’
In air n = n
In air n = n ’ ’ =1 =1 Lens, n
Lens, n
22= 1.5 = 1.5
R R
11= - = - R R
22= 10 cm = 10 cm d = 3 cm
d = 3 cm Find
Find ƒ ƒ
11, , ƒ ƒ
22, , ƒ ƒ , h and h , h and h ’ ’ Construct the
Construct the
principal planes, H, principal planes, H, H H ’ ’ of the entire of the entire
system system
n n n n ’ ’
Principal planes for thick lens (n 2 =1.5) in air Principal planes for thick lens (n 2 =1.5) in air
Equi Equi - - convex or convex or equi equi - - concave and moderately thick concave and moderately thick
P P
11= P = P
22≈ ≈ P/2 P/2
' d 3 h
h
1 2
2 2
' f
f n
h d
f f n
h d
H H H’ H ’ H H H’ H ’
Principal planes for thick lens (n 2 =1.5) in air Principal planes for thick lens (n 2 =1.5) in air
Plano
Plano - - convex or convex or plano plano - - concave lens with R concave lens with R
22= =
P P
22= 0 = 0
d h
h
3 ' 2
0
1 2
2 2
' f
f n
h d
f f n
h d
H H H’ H ’ H H H H ’ ’
Principal planes for thick lens (n=1.5) in air Principal planes for thick lens (n=1.5) in air
For meniscus lenses, the principal planes move For meniscus lenses, the principal planes move
outside the lens outside the lens
R R
22= 3R = 3R
11(H (H ’ ’ reaches the first surface) reaches the first surface)
P Same for all lenses Same for all lenses
1 2
2 2
' f
f n
h d
f f n
h d
H H H’ H ’ H H H H ’ ’ H H H’ H ’
H H H’ H ’
Examples: Two thin lenses in air Examples: Two thin lenses in air
2 2
f d f P
d P
h
ƒ ƒ
11ƒ ƒ
22d d
H
H
11’’
H
H
11 HH
22 HH
22’’
n = n
n = n
2 2= n’ = n ’ = 1 = 1 Want to replace H
Want to replace H
ii, H , H
ii’ ’ with H, H’ with H, H ’
1
'
1f d f P
d P
h
h h h h ’ ’
H H H’ H ’
Examples: Two thin lenses in air Examples: Two thin lenses in air
ƒ ƒ
11ƒ ƒ
22d d
n = n
n = n
2 2= n’ = n ’ = 1 = 1
2 1 2
1
2 2 1 2
1
1 1
1 ,
f f
d f
f f
or
n P d P
P P
P
H H H’ H ’
F F F F ’ ’
ƒ ƒ ƒ’ ƒ’ s s f
1 '
1 1
s’ s ’
s s
Two separated lenses in air Two separated lenses in air
If f
If f
11’ ’ =2f =2f
22’ ’
d = 0.5 d = 0.5 f f
22’ ’
H H H’ H ’
F’ F ’ F F
f’ f ’
d = d = f f
22’ ’
H H H H ’ ’
F’ F ’ F F
f’ f ’
Two separated lenses in air Two separated lenses in air
f f
11’ ’ =2f =2f
22’ ’
d = 2 d = 2 f f
22’ ’
H H H’ H ’
F’ F ’ F F
f’ f ’
d = 3 d = 3f f
22’ ’
Principal points at Principal points at
e.g. Astronomical telescope e.g. Astronomical telescope
Two separated lenses in air Two separated lenses in air
f f
11’ ’ =2f =2f
22’ ’
d = 5 d = 5 f f
22’ ’
f’ f ’
e.g. Compound microscope e.g. Compound microscope
H H
F’ F ’ F F
H’ H ’
Two separated lenses in air Two separated lenses in air
f f
11’ ’ = = - - 2f 2f
22’ ’
d = d = - - f f
22’ ’
e.g. Galilean telescope e.g. Galilean telescope
Principal points at
Principal points at
Two separated lenses in air Two separated lenses in air
f f
11’ ’ = = - - 2f 2f
22’ ’
d = d = - - 1.5 1.5 f f
22’ ’
e.g. Telephoto lens e.g. Telephoto lens
H H H H ’ ’
F’ F ’
f’ f ’
F F
우와아~ !!! 복잡하다.
우와아 우와아 ~ !!! ~ !!! 복잡하다 복잡하다 . .
HH11’’
HH11 HH22 HH22’’
HH H’H’
ƒ
ƒ ƒ’ƒ’
h
h hh’’
FF FF’’
d d nn22
nn n’n’
렌즈 렌즈 2 2 개가 개가 있는 있는 경우도 경우도 힘들다 힘들다 . .
좋은 좋은 방법이 방법이 없을까 없을까 ? ?
H H11’’ H
H11 HH22 HH22’’ HH H’H’
ƒ
ƒ ƒ’ƒ’
hh h’h’
FF F’F’
dd n n22 n
n n’n’
H H11’’ H
H11 HH22 HH22’’ H
H H’H’
ƒƒ hh hh’’ ƒ’ƒ’
FF FF’’
dd n n22 n
n nn’’
3 3 개 개 이상 이상 있으면 있으면 ? ? 못하겠다 못하겠다 . .
포기 포기 ? ?
Matrix Methods in paraxial optics Matrix Methods in paraxial optics
• Development of systematic methods of analyzing optical systems with numerous elements
• Matrices for analyzing the translation, refraction, and reflection of optical rays
• Matrices for thick and thin lenses, optical systems with numerous elements
Matrix Method Matrix Method
1 1 2
2
y D
C
B A
y
1 1
2
1 1
2
D Cy
B Ay
y
ABCD Matrix
What is the ray-transfer matrix What is the ray-transfer matrix
tan
sin
How to use the ray-transfer matrices
How to use the ray-transfer matrices
How to use the ray-transfer matrices How to use the ray-transfer matrices
translation refraction translation translation
Translation Matrix Translation Matrix
0 0
1 1 0
0 0
1
1 1
0 1 0 1
y y
y L x x
( yo, o)
( y1, 1 )
L
1 0
y
1y
0L tan
0y
0L
0
1 0 0
1 0 0
1
0 1
y y L
y
Refraction Matrix Refraction Matrix
' :
1 1
Paraxial Snell s Law n n
y n y n y y n n
R n R n R R R n y n
1
01 0
: 0
1 1 : 0
y y
y y Concave surface R
n n
Convex surface R
R n n
y=y’
y
R
y y
R R
n n'
Reflection Matrix Reflection Matrix
:
2
1 0
2 1
1 0 2 1 Law of Reflection
y y
R R R y
y y
R y
y y
R
y=y’
y y y
R R R
Thick Lens Matrix I Thick Lens Matrix I
0 0
1
1
0 0
1
1
1 0
: L
L L
y y
Refraction at first surface y n n n M
n R n
2 1 1
2
2 1 1
1 2 : 1
0 1
y t y y
Translation from st surface to nd surface M
3 2 2
3
3 2 2
2
1 0
: y L L y y
Refraction at second surface n n n M
n R n
Thick Lens Matrix II Thick Lens Matrix II
1
2
1
1
2 1 1 2
: 1
1 0
1
1 1
L
L L
L L
L
L L
L
L L
L L L L
L L
Assuming n n
t n n t n
n R n
M n n n
n n n
n R n
n R n
t n n t n
n R n
t n n
n n n n n n
n R n R n R n R t
2 1
1 0 1 0
1
L L 0 1 L
L L
M n n n t n n n
n R n n R n
3 2 1
:
Thick lens matrix M M M M
Thin Lens Matrix Thin Lens Matrix
2 1
1 2
:
1 0
1 1
1
1 1 1
1 0
1 1
L
L
Thin lens matrix
M n n
n R R
n n
but f n R R
M
f
The thin lens matrix is found by setting t = 0:
nL
Summary of Matrix Methods Summary of Matrix Methods
0
System Ray-Transfer Matrix System Ray-Transfer Matrix
Introduction to Matrix Methods in Optics, A.
Gerrard and J.
M. Burch
1 1
y
2 2
2 2
n n
y
System Ray-Transfer Matrix System Ray-Transfer Matrix
Any paraxial optical system, no matter how complicated, can be
represented by a 2x2 optical matrix. This matrix M is usually denoted
: system matrix A B
M C D
A useful property of this matrix is that
Det
0f
M AD BC n
n
where n0 and nf are the refractive indices of the initial and final media of the optical system
Det
01
f
M AD BC n
n
Usually, the medium will be air on both sides of the optical system and
Significance of system matrix elements
Significance of system matrix elements
The matrix elements of the system matrix can be analyzed
to determine the cardinal points and planes
of an optical system.0 0 f
f
y A B y
C D
Let’s examine the implications
when any of the four elements of the system matrix is equal to zero.
0 0
0 0
f f
y Ay B Cy D
D=0 : input plane = first focal plane
A=0 : output plane = second focal plane
B=0 : input and output planes correspond to conjugate planes C=0 : telescopic system
D=0 A=0
B=0 C=0
System Matrix with D=0 System Matrix with D=0
Let’s see what happens when D = 0.
0 0
0 0
0
0
f f
f f
y A B y
C
y Ay B Cy
When D = 0, the input plane for the optical system is the first (object) focal plane.
Ex) Two-Lens System : find the 1
stfocal plane Ex) Two-Lens System : find the 1
stfocal plane
f1 = +50 mm f2 = +30 mm
q = 100 mm
r s
Input
Plane Output
Plane
F1 F1 F2 F2
T1 R1 T2 R2 T3
1 1
2 1 1 2
1 1
1 0 1 1 0 1
1 1 1
1 1 1
1 1 1
0 1 0 1 0 1 1
1
q q r
r q
r f f
s q s
M r
f f f f r
f f
0
3 2 2 1 1
0
2 1
1 0 1 0
1 1 1
1 1
1 1
0 1 0 1 0 1
f f
y y s q r
M M T R T R T
f f
3 2 2 1 1
1 1
2 1 1 2 1 1
1 2 1 1 2 2 1 1
2 1 1 2 1 1
1 1
0 1 1 1 1
1 1
1 1 1
1 1 1
1 1
M T R T R T
q q r
r q
f f
s
q q r r
r q
f f f f f f
q s s q q r r q q r r
r q s
f f f f f f f f
q q r r
r q
f f f f f f
2 1 1
2 1 1
1 2
1 1 0
30 50 100 50 100 50 30 175
q r r
D r q
f f f
f f q f
r q f f
r mm
ƒ
ƒ11 ƒƒ22
d d HH H’H’
FF F’F’
ƒ
ƒ ƒ’ƒ’
s’s’ ss
h h rr
1 2
1 2 1 2 1 2
1 1 1
f f
d f
f f f f f f f d
2 2
f d f P d P
h
2 1 2 1
2 1 2
f d f f f d
r f h f
f f f d
< check! >
System Matrix with A=0, C=0 System Matrix with A=0, C=0
0 0 0
0 0
f
0
f f
f
y B y
C D
y B
Cy D
When A = 0, the output plane for the optical system is the output focal plane.
When C = 0, collimated light at the input plane is collimated light at the exit plane but the angle with the optical axis is different. This is a
telescopic arrangement, with a magnification of D = f/0.
0 0
0 0
0
0
f f f
f
y A B y
D y Ay B
D
0 0
0
0 0
0 f
0
f
f f
f
y A y
C D
y Ay
Cy D
m y A
y
When B = 0, the input and output planes are object and image planes, respectively, and the transverse magnification of the system m = A.
System Matrix with B=0 System Matrix with B=0
Conjugate planes