introduction to aberrations...opti 518 structural stop shifting parameter s’ is the distance from...
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Prof. Jose SasianOPTI 518
Introduction to aberrations
OPTI 518Lecture 14
Prof. Jose SasianOPTI 518
Topics
• Structural aberration coefficients• Examples
Prof. Jose SasianOPTI 518
Structural coefficients
Ж
Requires a focal systemAfocal systems can be treated with Seidel sums
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Structural stop shifting parameter
s’ is the distance from the rear principal plane to exit pupil
s is the distance from the front principal plane to entrance pupil
2
2 2P P Py y yS SЖ Ж
'
2 1 2 1 ' 2 'P Py y s sSЖ Y s n Y s n
1 / 2nu Y y
Using ω on we can express:
2P Py ySЖ
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Review of concepts
• Thin lens as the thickness tends to zero
• Shape of a lens and shape factor• Conjugate factor to quantify how the lens
is used. Related to transverse magnification
• Must know well first-order optics
1 2 1 2tn
Prof. Jose SasianOPTI 518
Shape and Conjugate factors
nu ' 1' 1
mYm
1 2 1 2
1 2 1 2
c c R RXc c R R
Lens bending concept
Prof. Jose SasianOPTI 518
Shape X
X=-1
X=0
X=-1.7
X=-3.5X=3.5
X=1.7
X=1
X=0
Prof. Jose SasianOPTI 518
Shape
X=0
X=0
X=-1X=-2X=-3
X=1X=2X=3
Prof. Jose SasianOPTI 518
Shape or bending factor X• Quantifies lens shape• Optical power of thin lens is maintained• Not defined for zero power, R1=R2
1 2 1 2
1 2 1 2
c c R RXc c R R
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Example:Refracting surface free from spherical aberration
Object at infinity Y=1
2 2 22 2 2 2
2 2 2 2 2 2
1 ' ' ' 1 2 2 2 112 ' ' ' 2 ' ' ' 'In n n n n n n nn n n n n n n n n n n n
44 3 4 3 4 3
23
1 1 14 4 '
PI P I P I P
yS y n K y y Kr n n
2 4 3 24 3
2 22 2
1 2 1 14 ' ' '' '
PI P
yn nS y K Kn n n nn n n n
22
20'InS Kn
Parabola for reflectionEllipse for air to glassHyperbola for glass to air
Prof. Jose SasianOPTI 518
Note
24 3 4 3 4 3
21 1 1 24 4 ''
I P I P P IS y y K y Kn nn n
The contribution to the structural coefficient from the aspheric cap is
22'Icap Kn n
For a reflecting surface is just the conic constant K
Prof. Jose SasianOPTI 518
Icap K
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Spherical MirrorA spherical mirror can be treated as a convex/concave
plano lens with n=-1. The plano surface acts as an unfoldingflat surface contributing no aberration.
2
1
11
000
I
II
III
IV
V
L
T
XYY
14
011401
A
BC
D
EF
n=-1
n=1 n=1
Prof. Jose SasianOPTI 518
Field curves
Prof. Jose SasianOPTI 518
Field curves
Rt~f/3.66Rm~f/2.66Rs~f/1.66Rp~f/0.66
Prof. Jose SasianOPTI 518
Thin lensSpherical aberration and coma
I II
Fourth-order
Prof. Jose SasianOPTI 518
Spherical aberration of a F/4 lens
•Asymmetry•For high index 4th order predicts well the aberration
Prof. Jose SasianOPTI 518
Thin lens spherical aberration
n=1.517
I
Y
X
Prof. Jose SasianOPTI 518
Thin lens coma aberration
n=1.517
II
X
Y
Prof. Jose SasianOPTI 518
This lensAplanatic solutions
X=4
Y=5n=1.5
' 1' 1
mYm
Prof. Jose SasianOPTI 518
Thin lensSpherical and coma @ Y=0
III
N=1.5N=2N=2.5N=3N=3.5N=4
Strong index dependence
Prof. Jose SasianOPTI 518
Thin lens special casesstop at lens
Prof. Jose SasianOPTI 518
Thin lens special cases stop at lens
Prof. Jose SasianOPTI 518
Thin lens special cases stop at lens
For double convex lens (CX)For double concave lens (CC)
Prof. Jose SasianOPTI 518
Thin lens special cases stop at lens
Prof. Jose SasianOPTI 518
Thin lens special cases stop at lens
Prof. Jose SasianOPTI 518
Achromatic doubletTwo thin lenses in contactThe stop is at the doublet
1 2
1 2
11
22
y y
1 2
21
1
12
2
1
YY
YY
Prof. Jose SasianOPTI 518
Achromatic doubletCorrection for chromatic change of focus
1 2
1 2
11 2
1 2
22 1
1 2
1
1
L
L
L
0L
For an achromatic doublet:
2,
,0
kP kk
L L ki P
yy
Prof. Jose SasianOPTI 518
Achromatic doubletCorrection for spherical aberration
3 2 2 3 2 21 1 1 1 1 1 1 1 1 2 2 2 2 2 2 2 2 2I A X B X Y CY D A X B X Y C Y D
43,
,0
kP kk
I I ki P
yy
For a given conjugate factor Y, spherical aberration is a functionOf the shape factors X1 and X2 . For a constant value of spherical
aberration we obtain a hyperbola as a function of X1 and X2.
Prof. Jose SasianOPTI 518
Achromatic doubletCorrection for coma aberration
22
,, ,
0
kP kk
II II k k I ki P
yS
y
2 21 1 1 1 1 2 2 2 2 2II E X FY E X F Y
For a given conjugate factor Y and a constant amount of coma the graph of X1 and X2 is a straight line.
Prof. Jose SasianOPTI 518
Achromatic doubletAstigmatism aberration
2, , ,
0
2k
kIII III k k II k k I k
i
S S
1 21 1III
Astigmatism is independent of the relative lens powers, shape factors,or conjugate factors.
Prof. Jose SasianOPTI 518
Achromatic doublet
1 2
1 2IV n n
2 1
2 1
n n
Field curvature aberration
,0
kk
IV IV ki
0IV For an achromatic doublet there is no field curvature if
Prof. Jose SasianOPTI 518
Achromatic doubletDistortion and chromatic change of magnification
, ,0
k
T T k k L ki
S
2
2 3, , , , ,
0 ,
3 3k
PV V k k IV k III k k II k k I k
i P k
y S S Sy
00
V
T
Prof. Jose SasianOPTI 518
Cemented achromatic doublet
1 1 2 212 21
1 2
1 1 2 2
1 2
2 1
1 12 1 2 1
1 11 1
1 1
X Xc c
n n
X Xn n
X X
2 1
1 2
2 1
1 2
11
11
nn
nn
For achromat
For a cemented achromatic lens the graph of X1 and X2 is a straight line.
Prof. Jose SasianOPTI 518
Crown in front: BK7 and F8
Prof. Jose SasianOPTI 518
Flint in front: BK7 and F8
Prof. Jose SasianOPTI 518
Cemented achromatic doublet
Prof. Jose SasianOPTI 518
Cemented doublet solutions
Crown in front
Flint in front
Prof. Jose SasianOPTI 518
Doublets with no spherical aberration but with varying coma
Crown in front, no spherical aberration, F/5, f=100 mm, no chromatic aberration
Coma=0Coma=-10 waves Coma=10 waves
Prof. Jose SasianOPTI 518
Lister objective
Prof. Jose SasianOPTI 518
Lister objective• Two achromatic doublets that are spaced• Telecentric in image space• Normalized system
11100
A
A
IA
IB
Жyu
Prof. Jose SasianOPTI 518
Lister objective
The aperture stop is at the first lens.The system is telecentric
111
B
A B
B
yy
Prof. Jose SasianOPTI 518
Lister objective
Prof. Jose SasianOPTI 518
Condition for zero coma
22,
, ,0
2 2 2 2
2 2
2
2
0
1 0
1
kP kk
II II k k I ki P
II A A IIA B B IIB
IB
II B IIA B IIB
BIIA IIB
B
yS
y
y y
y y
yy
Prof. Jose SasianOPTI 518
Condition for zero astigmatism
2, , ,
0
2
2
1 0
1 1 0
2 02
12
2
1
kk
III III k k II k k I ki
III A B B IIB
III B B IIB
B B IIB
BIIB
BIIB
B
B BIIA
B
S S
y
y y
y y
y
yy
y y
y
, ,
2k P k P k
k
y yS
Ж
Prof. Jose SasianOPTI 518
Lister Objective
2
2 2
2 2
221
1
1 212123
3
IIB IIA
B BB
B B
B B
B B B
B
A
IIA
IIB
y yyy y
y y
y y y
y
Choose:
Prof. Jose SasianOPTI 518
1Petzval IV
Petzval
Cn
N-BK7 : Petzval radius -151.7 mm
Plano convex lens
Prof. Jose SasianOPTI 518
Wollaston meniscus lens
222 220/ 0.8PW W
• Artificially flattening the field• Periscopic lenses
Prof. Jose SasianOPTI 518
Periskop lens
• Principle of symmetry• No distortion
Prof. Jose SasianOPTI 518
1 2 1 2
1 2 1 2 1 2
1Petzval IV
Petzval
v vCn n v v n n
N-BAK1 and N-LLF6: Petzval radius -185 mm
N-BK7 : Petzval radius -151.7 mm
N-BK7 and N-F2: Petzval radius -139.99 mm (+139.99 for negative doublet)
Field curvature
• Old achromat• New achromat
Prof. Jose SasianOPTI 518
Chevalier landscape lens
222 220/ 0.8PW W • F/5 telescope doublet used in reverse
and with an aperture stop in front
Prof. Jose SasianOPTI 518
• F/8• Glass selection is keyto minimize spherical aberrationwhile artificially flattening the field
Rapid rectilinear
RMS spot size
Prof. Jose SasianOPTI 518
• Telecentric
Lister microscope objective
2 2 2 2II A A IIA B B IIBy y
2
21B
IIA IIBB
yy
12By
IIA IIB
1 1 0III B B IIBy y
0IA IB
* 22III III II IS S SS S S
Prof. Jose SasianOPTI 518
Lister microscope objectivePractical solution
• Two identical doublets• Spherical aberration and coma are corrected• Astigmatism is small• Telecentric• Less vignetting
• RMS wavefront error in waves
Prof. Jose SasianOPTI 518
Aplanatic concentric meniscus lens
• Optical speed is increased by an N factor
Prof. Jose SasianOPTI 518
Petzval portrait objective
222 220/ 0.8PW W
• Chromatic aberration and spherical aberrationcorrected at each doublet
• Positive coma in the first doublet corrected with negative coma of aberration of the second doublet
• Negative astigmatism introduced by the negative coma of the second doublet toartificially flatten the field of view.
f’=144 mm; F/3.7; FOV=+/- 16.5⁰.
* 22III III II IS S SS S S
Prof. Jose SasianOPTI 518
Concentric lens
• Use of new glasses• Reduced Petzval sum• Nearly flat field• Surfaces nearly concentric• Limited by spherical aberration
due to strong curvatures.
1 2 1 2
1 2 1 2 1 2
1Petzval IV
Petzval
v vCn n v v n n
N-BAK1 and N-LLF6: Petzval radius -185 mm
Prof. Jose SasianOPTI 518
Anastigmatic lens
• Corrected for spherical aberration, coma, astigmatism, and field curvature• Distortion is negligible• Combination of an old achromat and a new achromat
RMS spot size
Prof. Jose SasianOPTI 518
Anastigmatic lens
• Corrected for spherical aberration, coma, astigmatism, and field curvature• Distortion is negligible• Combination of an old achromat and a new achromat
RMS spot size
Prof. Jose SasianOPTI 518
Telephoto lens
• Corrected for spherical aberration, coma, astigmatism, and field curvature• Distortion is not corrected• Telephoto ratio=TTL/f
Telephoto lens with BK7 and SF5 glasses. f’=100 mm, F/4, FOV=+/- 6.2⁰, TTL/F=0.8.
2
131 31112
W W Ж u
* 22III III II IS S SS S S
* 2 2III III B IIIB BS S Ж Ж
A B
Prof. Jose SasianOPTI 518
Telephoto lens
• Corrected for spherical aberration, coma, astigmatism, and field curvature• Distortion is also corrected
Telephoto lens with BK7 and F6 glasses. f’=100 mm, F/4, FOV=+/- 6.2⁰, TTL/F=0.8
Prof. Jose SasianOPTI 518
Reverse telephoto lens
• Corrected for spherical aberration, coma, astigmatism, and field curvature• Distortion is small ~-1.5%• Large back focal length/distance
Reverse telephoto lens with BK7 and SF5 glasses. f’=100 mm, BFL=200 mm, TTL= 324 mm, FOV=+/-12⁰, F/4
Prof. Jose SasianOPTI 518
Ray diffractive law (1D)
Prof. Jose SasianOPTI 518
Grating linear phase change
sin ' sin mn I n Id
sin ' sin my n I y yn I yd
Prof. Jose SasianOPTI 518
Diffractive opticshigh-index model
1/d
Prof. Jose SasianOPTI 518
Diffractive opticshigh-index model
1/d
Prof. Jose SasianOPTI 518
Diffractive lens (n very large @ X=0)
A=0B=0C=3D=1E=0F=2
23 1I Y
2II Y 1III
0IV
0V 1
Ldiffractive
0T
Prof. Jose SasianOPTI 518
Mirror Systems
'
2 1 2 1 ' 2 'P Py y s sSЖ Y s n Y s n
Prof. Jose SasianOPTI 518
Two mirror afocal system
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Two mirror systems111
PyЖ
2
2
2
2
/ 1 11/
111
2 111
P
M ML
y yMLML
SML
MYM
1
1
1
1
/ 1/ 1
00
Py y
SY
2
2
2
2
1
yLy
yMy
Prof. Jose SasianOPTI 518
Two mirror systems
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Prof. Jose SasianOPTI 518
Schmidt camera
Prof. Jose SasianOPTI 518
Merssene afocal systemAnastigmatic
Confocal paraboloids
Prof. Jose SasianOPTI 518
Paul-Baker systemAnastigmatic-Flat field
AnastigmaticParabolic primarySpherical secondary and tertiaryCurved fieldTertiary CC at secondary
Anastigmatic, Flat fieldParabolic primaryElliptical secondary Spherical tertiaryTertiary CC at secondary
Prof. Jose SasianOPTI 518
Meinel’s two stage optics concept (1985)
Large DeployableReflector
Second stage correctsfor errors of first stage;fourth mirror is at the
exit pupil.
Prof. Jose SasianOPTI 518
Aplanatic, Anastigmatic, Flat-field, Orthoscopic (free from distortion, rectilinear, JS 1987)
Spherical primary telescope.The quaternary mirror is near the exit pupil. Spherical aberration and
Coma are then corrected with a single aspheric surface. The Petzval sum is zero.If more aspheric surfaces are allowed then more aberrations
can be corrected.
Prof. Jose SasianOPTI 518
Summary
• Structural coefficients• Basic treatment• Analysis of simple systems