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Prof. Jose Sasian OPTI 518 1 Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations
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Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Jan 20, 2020

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Page 1: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

1

Introduction to aberrations

OPTI 518

Lecture 15

Pupil aberrations

Page 2: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Page 3: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Pupil mismatch

System’s Aexit pupil

System’s B entrance pupil

Zero-order matchFirst-order matchThird-order mismatch

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Prof. Jose SasianOPTI 518

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Some references• T. Smith, “The changes in aberrations when the object

and stop are moved,” Trans. Opt. Soc. 23, 139-153, 1921/1922

• C. C. Wynne, “Primary aberrations and conjugate change,” Proc. Phys. Soc. Lond. 65 b, 429-437 (1952)

• J. Sasian, Interpretation of pupil aberrations in imaging systems, SPIE V. 6342-634206 (2006)

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Prof. Jose SasianOPTI 518

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Object-image systemPupil-pupil system

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Prof. Jose SasianOPTI 518

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Pupil aberration function

000 200 111 020

22040 131 222

2

220 311 400

,W H W W H H W H W

W W H W H

W H H W H H H W H H

000 200 111 020

2 2

040 131 222

2220 311 400

,W H W W W H W H H

W H H W H H H W H

W H H W H W

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Prof. Jose SasianOPTI 518

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Pupil aberrations• Object-image interchange role with entrance-and exit pupils• The chief ray becomes the marginal ray, and the marginal ray

becomes the chief ray. Lagrange invariant changes sign• Image and pupil aberrations are connected

Page 8: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Prof. Jose SasianOPTI 518

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Some interesting “shift”relationships

, , ,H H PPW H W H S W H

, , ,PP HW H W H S W H

Ж

Page 10: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Geometry for derivation

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Prof. Jose SasianOPTI 518

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The displacement vector at the entrance pupil

040 131

222 220 311

4 21 1,2 2

H

W H H H W H H H HW H

Ж Ж W H W H W

51 ,H W H OЖ

Page 12: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Beam deformation at pupil

040 131

222 220 311

4 21 1,2 2

H

W H H H W H H H HW H

Ж Ж W H W H W

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Prof. Jose SasianOPTI 518

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Pupil aberration consequences

• Can now determine aberration change upon object shift

• Spherical aberration of the pupil• Coma of the pupil• Astigmatism and field curvature of the

pupil• Extrinsic sixth-order aberrations• Bow-Sutton conditions

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Effects from pupil aberrations• Kidney bean effect. This is a partial obscuration in the

form of a kidney bean caused by pupil spherical aberration

• Loss of telecentricity in relay systems. The chief slope varies as a function of the field of view.

• Vignetting. Spherical aberration of the pupil can lead to light vignetting.

• Pupil walking. Notably in fish eye lenses.• Slyusarev effects. Due to pupil coma, the exit pupil

changes size impacting the relative illumination• Pupil Apodization

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Pupil walking

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Prof. Jose SasianOPTI 518

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Kidney bean effect

Chief rays

Off-axis clipping aperture(eye iris)

From pupil spherical aberration

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Loss of telecentricity

Chief rays Spherical aberrationof the exit

pupil

Entrancepupil

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Change in relative illumination

• Vignetting• Image distortion• Cosine to the fourth law• Pupil distortion• Coatings

Page 19: Introduction to aberrations - University of Arizona...Introduction to aberrations OPTI 518 Lecture 15 Pupil aberrations. Prof. Jose Sasian OPTI 518 2. Prof. Jose Sasian OPTI 518 3

Prof. Jose SasianOPTI 518

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Effects from pupil coma

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Bow-Sutton conditions

See Kingslake’s lens design fundamentalsNew edition with Barry Johnson

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Bow-Sutton Conditions• Since the lens is symmetrical ubar’=ubar• Thus Coma pupil = image distortion• A unit magnification the system is fully symmetrical for the stop and

for the image systems and so, Coma pupil = image distortion=0• When the object moves at other conjugate coma of the pupil

according to stop shift equations is,• New pupil coma=old pupil coma + pupil spherical aberration *

y/ybar.• The old coma is zero, thus,• New pupil coma=pupil spherical aberration * y/ybar.• Therefore if pupil spherical aberration is zero then the new pupil

coma is zero.• And therefore image distortion is zero.• ubar’=ubar, still holds for the second conjugate

2

131 31112

W W Ж u 131 131

*040

yW W Wy

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Object shift equations

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Formulas

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Invariance of aberrations

No primary aberrations independently of stop position or conjugate!Negative unit magnification system

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Chromatic pupil aberrations

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Summary

• Optical systems are formed by concatenating one system to the next

• The exit pupil of one system becomes the entrance pupil for the next system

• Every pupil mismatch leads to light loss, aberration, or other effect.

• Pupil aberrations are also important