- •Lens Design Fundamentals
- •Contents
- •Preface to the Second Edition
- •Preface to the First Edition
- •A Special Tribute to Rudolf Kingslake
- •1.1. Relations Between Designer and Factory
- •1.1.1 Spherical versus Aspheric Surfaces
- •1.1.2 Establishment of Thicknesses
- •1.1.3 Antireflection Coatings
- •1.1.4 Cementing
- •1.1.5 Establishing Tolerances
- •1.1.6 Design Tradeoffs
- •1.2. The Design Procedure
- •1.2.1 Sources of a Likely Starting System
- •1.2.2 Lens Evaluation
- •1.2.3 Lens Appraisal
- •1.2.4 System Changes
- •1.3. Optical Materials
- •1.3.1 Optical Glass
- •1.3.2 Infrared Materials
- •1.3.3 Ultraviolet Materials
- •1.3.4 Optical Plastics
- •1.4. Interpolation of Refractive Indices
- •1.4.1 Interpolation of Dispersion Values
- •1.4.2 Temperature Coefficient of Refractive Index
- •1.5. Lens Types to be Considered
- •2.1. Introduction
- •2.1.1 Object and Image
- •2.1.2 The Law of Refraction
- •2.1.3 The Meridional Plane
- •2.1.4 Types of Rays
- •2.1.5 Notation and Sign Conventions
- •2.2. Graphical Ray Tracing
- •2.3. Trigonometrical Ray Tracing at a Spherical Surface
- •2.3.1 Program for a Computer
- •2.4. Some Useful Relations
- •2.4.1 The Spherometer Formula
- •2.4.2 Some Useful Formulas
- •2.4.3 The Intersection Height of Two Spheres
- •2.4.4 The Volume of a Lens
- •2.5. Cemented Doublet Objective
- •2.6. Ray Tracing at a Tilted Surface
- •2.6.1 The Ray Tracing Equations
- •2.6.2 Example of Ray Tracing through a Tilted Surface
- •2.7. Ray Tracing at an Aspheric Surface
- •3.1. Tracing a Paraxial Ray
- •3.1.1 The Standard Paraxial Ray Trace
- •3.1.2 The (y – nu) Method
- •3.1.3 Inverse Procedure
- •3.1.4 Angle Solve and Height Solve Methods
- •3.1.6 Paraxial Ray with All Angles
- •3.1.7 A Paraxial Ray at an Aspheric Surface
- •3.1.9 Matrix Approach to Paraxial Rays
- •3.2. Magnification and the Lagrange Theorem
- •3.2.1 Transverse Magnification
- •3.2.2 Longitudinal Magnification
- •3.3. The Gaussian Optics of a Lens System
- •3.3.1 The Relation between the Principal Planes
- •3.3.2 The Relation between the Two Focal Lengths
- •3.3.3 Lens Power
- •3.3.4 Calculation of Focal Length
- •3.3.5 Conjugate Distance Relationships
- •3.3.6 Nodal Points
- •3.3.7 Optical Center of Lens
- •3.3.8 The Scheimpflug Condition
- •3.4. First-Order Layout of an Optical System
- •3.4.1 A Single Thick Lens
- •3.4.2 A Single Thin Lens
- •3.4.3 A Monocentric Lens
- •3.4.4 Image Shift Caused by a Parallel Plate
- •3.4.5 Lens Bending
- •3.4.6 A Series of Separated Thin Elements
- •3.4.7 Insertion of Thicknesses
- •3.4.8 Two-Lens Systems
- •3.5. Thin-Lens Layout of Zoom Systems
- •3.5.1 Mechanically Compensated Zoom Lenses
- •3.5.2 A Three-Lens Zoom
- •3.5.4 A Four-Lens Optically Compensated Zoom System
- •3.5.5 An Optically Compensated Zoom Enlarger or Printer
- •Endnotes
- •4.1. Introduction
- •4.2. Symmetrical Optical Systems
- •4.3. Aberration Determination Using Ray Trace Data
- •4.3.1 Defocus
- •4.3.2 Spherical Aberration
- •4.3.3 Tangential and Sagittal Astigmatism
- •4.3.4 Tangential and Sagittal Coma
- •4.3.5 Distortion
- •4.3.6 Selection of Rays for Aberration Computation
- •4.3.7 Zonal Aberrations
- •4.3.8 Tangential and Sagittal Zonal Astigmatism
- •4.3.9 Tangential and Sagittal Zonal Coma
- •4.3.10 Higher-Order Contributions
- •4.4. Calculation of Seidel Aberration Coefficients
- •Endnotes
- •5.1. Introduction
- •5.2. Spherochromatism of a Cemented Doublet
- •5.2.4 Secondary Spectrum
- •5.2.5 Spherochromatism
- •5.3. Contribution of a Single Surface to the Primary Chromatic Aberration
- •5.4. Contribution of a Thin Element in a System to the Paraxial Chromatic Aberration
- •5.5. Paraxial Secondary Spectrum
- •5.7.1 Secondary Spectrum of a Dialyte
- •5.7.2 A One-Glass Achromat
- •5.8. Chromatic Aberration Tolerances
- •5.8.1 A Single Lens
- •5.8.2 An Achromat
- •5.9. Chromatic Aberration at Finite Aperture
- •5.9.1 Conrady’s D – d Method of Achromatization
- •5.9.3 Tolerance for the D – d Sum
- •5.9.5 Paraxial D – d for a Thin Element
- •Endnotes
- •6.1. Surface Contribution Formulas
- •6.1.1 The Three Cases of Zero Aberration at a Surface
- •6.1.2 An Aplanatic Single Element
- •6.1.3 Effect of Object Distance on the Spherical Aberration Arising at a Surface
- •6.1.4 Effect of Lens Bending
- •6.1.6 A Two-Lens Minimum Aberration System
- •6.1.7 A Four-Lens Monochromat Objective
- •6.2. Zonal Spherical Aberration
- •6.3. Primary Spherical Aberration
- •6.3.1 At a Single Surface
- •6.3.2 Primary Spherical Aberration of a Thin Lens
- •6.4. The Image Displacement Caused by a Planoparallel Plate
- •6.5. Spherical Aberration Tolerances
- •6.5.1 Primary Aberration
- •6.5.2 Zonal Aberration
- •Endnotes
- •7.1. The Four-Ray Method
- •7.2. A Thin-Lens Predesign
- •7.2.1 Insertion of Thickness
- •7.2.2 Flint-in-Front Solutions
- •7.3. Correction of Zonal Spherical Aberration
- •7.4. Design Of an Apochromatic Objective
- •7.4.1 A Cemented Doublet
- •7.4.2 A Triplet Apochromat
- •7.4.3 Apochromatic Objective with an Air Lens
- •Endnotes
- •8.1. Passage of an Oblique Beam through a Spherical Surface
- •8.1.1 Coma and Astigmatism
- •8.1.2 Principal Ray, Stops, and Pupils
- •8.1.3 Vignetting
- •8.2. Tracing Oblique Meridional Rays
- •8.2.1 The Meridional Ray Plot
- •8.3. Tracing a Skew Ray
- •8.3.1 Transfer Formulas
- •8.3.2 The Angles of Incidence
- •8.3.3 Refraction Equations
- •8.3.4 Transfer to the Next Surface
- •8.3.5 Opening Equations
- •8.3.6 Closing Equations
- •8.3.7 Diapoint Location
- •8.3.8 Example of a Skew-Ray Trace
- •8.4. Graphical Representation of Skew-Ray Aberrations
- •8.4.1 The Sagittal Ray Plot
- •8.4.2 A Spot Diagram
- •8.4.3 Encircled Energy Plot
- •8.4.4 Modulation Transfer Function
- •8.5. Ray Distribution from a Single Zone of a Lens
- •Endnotes
- •9.1. The Optical Sine Theorem
- •9.2. The Abbe Sine Condition
- •9.2.1 Coma for the Three Cases of Zero Spherical Aberration
- •9.3. Offense Against the Sine Condition
- •9.3.1 Solution for Stop Position for a Given OSC
- •9.3.2 Surface Contribution to the OSC
- •9.3.3 Orders of Coma
- •9.3.4 The Coma G Sum
- •9.3.5 Spherical Aberration and OSC
- •9.4. Illustration of Comatic Error
- •Endnotes
- •10.1. Broken-Contact Type
- •10.2. Parallel Air-Space Type
- •10.3. An Aplanatic Cemented Doublet
- •10.4. A Triple Cemented Aplanat
- •10.5. An Aplanat with A Buried Achromatizing Surface
- •10.6. The Matching Principle
- •Endnotes
- •11.1. Astigmatism and the Coddington Equations
- •11.1.1 The Tangential Image
- •11.1.2 The Sagittal Image
- •11.1.3 Astigmatic Calculation
- •11.1.5 Astigmatism for the Three Cases of Zero Spherical Aberration
- •11.1.6 Astigmatism at a Tilted Surface
- •11.2. The Petzval Theorem
- •11.2.1 Relation Between the Petzval Sum and Astigmatism
- •11.2.2 Methods for Reducing the Petzval Sum
- •11.3. Illustration of Astigmatic Error
- •11.4. Distortion
- •11.4.1 Measuring Distortion
- •11.4.2 Distortion Contribution Formulas
- •11.4.3 Distortion When the Image Surface Is Curved
- •11.5. Lateral Color
- •11.5.1 Primary Lateral Color
- •11.6. The Symmetrical Principle
- •11.7. Computation of the Seidel Aberrations
- •11.7.1 Surface Contributions
- •11.7.2 Thin-Lens Contributions
- •11.7.3 Aspheric Surface Corrections
- •11.7.4 A Thin Lens in the Plane of an Image
- •Endnotes
- •12.1.1 Distortion
- •12.1.2 Tangential Field Curvature
- •12.1.3 Coma
- •12.1.4 Spherical Aberration
- •12.2. Simple Landscape Lenses
- •12.2.1 Simple Rear Landscape Lenses
- •12.2.2 A Simple Front Landscape Lens
- •12.3. A Periscopic Lens
- •12.4. Achromatic Landscape Lenses
- •12.4.1 The Chevalier Type
- •12.4.2 The Grubb Type
- •12.5. Achromatic Double Lenses
- •12.5.1 The Rapid Rectilinear
- •12.5.3 Long Telescopic Relay Lenses
- •12.5.4 The Ross “Concentric” Lens
- •Endnotes
- •13.1. The Design of a Dagor Lens
- •13.2. The Design of an Air-Spaced Dialyte Lens
- •13.4. Double-Gauss Lens with Cemented Triplets
- •13.5. Double-Gauss Lens with Air-spaced Negative Doublets
- •Endnotes
- •14.1. The Petzval Portrait Lens
- •14.1.1 The Petzval Design
- •14.1.2 The Dallmeyer Design
- •14.2. The Design of a Telephoto Lens
- •14.3. Lenses to Change Magnification
- •14.3.1 Barlow Lens
- •14.3.2 Bravais Lens
- •14.4. The Protar Lens
- •14.5. Design of a Tessar Lens
- •14.5.1 Choice of Glass
- •14.5.2 Available Degrees of Freedom
- •14.5.3 Chromatic Correction
- •14.5.4 Spherical Correction
- •14.5.5 Correction of Coma and Field
- •14.5.6 Final Steps
- •14.6. The Cooke Triplet Lens
- •14.6.2 The Thin-Lens Predesign of the Bendings
- •14.6.3 Calculation of Real Aberrations
- •14.6.4 Triplet Lens Improvements
- •Endnotes
- •15.1. Comparison of Mirrors and Lenses
- •15.2. Ray Tracing a Mirror System
- •15.3. Single-Mirror Systems
- •15.3.1 A Spherical Mirror
- •15.3.2 A Parabolic Mirror
- •15.3.3 An Elliptical Mirror
- •15.3.4 A Hyperbolic Mirror
- •15.4. Single-Mirror Catadioptric Systems
- •15.4.1 A Flat-Field Ross Corrector
- •15.4.2 An Aplanatic Parabola Corrector
- •15.4.3 The Mangin Mirror
- •15.4.4 The Bouwers–Maksutov System
- •15.4.5 The Gabor Lens
- •15.4.6 The Schmidt Camera
- •15.4.7 Variable Focal-Range Infrared Telescope
- •15.4.8 Broad-Spectrum Afocal Catadioptric Telescope
- •15.4.9 Self-Corrected Unit-Magnification Systems
- •15.5. Two-Mirror Systems
- •15.5.1 Two-Mirror Systems with Aspheric Surfaces
- •15.5.2 A Maksutov Cassegrain System
- •15.5.3 A Schwarzschild Microscope Objective
- •15.5.4 Three-Mirror System
- •15.6. Multiple-Mirror Zoom Systems
- •15.6.2 All-Reflective Zoom Optical Systems
- •15.7. Summary
- •Endnotes
- •16.1. Design of a Military-Type Eyepiece
- •16.1.1 The Objective Lens
- •16.1.2 Eyepiece Layout
- •16.2. Design of an Erfle Eyepiece
- •16.3. Design of a Galilean Viewfinder
- •Endnotes
- •17.1. Finding a Lens Design Solution
- •17.1.1 The Case of as Many Aberrations as There Are Degrees of Freedom
- •17.1.2 The Case of More Aberrations Than Free Variables
- •17.1.3 What Is an Aberration?
- •17.1.4 Solution of the Equations
- •17.2. Optimization Principles
- •17.3. Weights and Balancing Aberrations
- •17.4. Control of Boundary Conditions
- •17.5. Tolerances
- •17.6. Program Limitations
- •17.7. Lens Design Computing Development
- •17.8. Programs and Books Useful for Automatic Lens Design
- •17.8.1 Automatic Lens Design Programs
- •17.8.2 Lens Design Books
- •Endnotes
- •Index
414 |
Unsymmetrical Photographic Objectives |
14.5.5 Correction of Coma and Field
To plot a double graph, we make a trial change of Dc1 ¼ –0.05 from System C and then restore everything to its original value (i.e., Setup D). We then return to Setup C and now change c3 by 0.05, which gives Setup E. These changes are shown in Figure 14.21. Following the usual procedure with a double graph, and making several small adjustments, we finally come up with Setup F:
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0.4126 |
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with f 0 ¼ 10, l0 ¼ 8.9344, LA0 |
( f/4.5) ¼ 0.0958, LZA ( f/6.4) ¼ –0.0258, OSC |
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( f/4.5) ¼ 0, Ptz ¼ 0.0250. The results are shown in Table 14.14.
The aberration graphs are shown plotted in Figure 14.22. As a check on the coma we next trace a number of oblique rays entering parallel to the principal ray at 17.19 and draw a meridional ray plot (Figure 14.23). It will be seen that the two ends of this graph sag somewhat, but the middle part of the curve is straight. This is an indication of the presence of negative higher-order coma, and it cannot be usefully corrected by the deliberate introduction of positive OSC. A much better method of removing it is to introduce some vignetting. If we limit the clear aperture of each surface to the diameter of the entering f/4.5 axial beam, we shall cut off the ends of the ray plot in Figure 14.23 to the marks
Table 14.14
Astigmatism and Distortion for Setup F
Field angle (deg) |
Xs0 |
Xt0 |
Distortion (%) |
29.74 |
0.1607 |
0.1303 |
1.42 |
25.61 |
0.0102 |
0.0871 |
0.92 |
21.42 |
0.0458 |
0.0305 |
0.56 |
17.19 |
0.0537 |
0.0020 |
0.32 |
14.5 Design of a Tessar Lens |
415 |
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Figure 14.22 Aberrations of Setup F. |
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3.10 |
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3.08 |
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3.06 |
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3.04 |
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3.02 |
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Figure 14.23 Meridional ray plot of Tessar Setup F. Rays SS are through top and bottom of the stop. Rays VV represent vignetted limiting rays.
VV shown, and we shall thus remove almost the entire higher-order coma without seriously reducing the image illumination. Figure 14.24 shows the lens apertures so reduced and the path of the limiting oblique rays VV.
The astigmatic fields shown in Figure 14.22 cross rather too high and the field is a little backward-curving. We shall therefore return to the double graph of Figure 14.21 and establish a new aim point at OSC ¼ 0 and Xt0 ¼ –0.04, which is by chance very close to Setup E. After making several small adjustments in c1 and c3, and of course correcting the spherical aberration each time by c5 and the Petzval sum by d20 , we arrive at the following solution G:
416 |
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Unsymmetrical Photographic Objectives |
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with f 0 ¼ 10, l0 ¼ 8.925977, Ptz ¼ 0.025, LA0 |
( f/4.5) ¼ 0.1029, LZA ( f/6.4) |
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¼ –0.0216, OSC ( f/4.5) ¼ 0, |
(D – d) Dn ¼ –0.00001096, lateral color |
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HF0 – HC0 (17 ) ¼ –0.00031. ThePresults are shown in Table 14.15. The fields |
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and aberration are shown plotted in Figure 14.25. |
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Figure 14.24 Vignetting in Setup F, 17 beam. |
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Table 14.15 |
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Astigmatism and Distortion for Setup G |
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Field (deg) |
Xs0 |
Xt0 |
Distortion (%) |
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29.64 |
0.1224 |
0.0283 |
1.18 |
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0.0148 |
0.0064 |
0.77 |
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21.38 |
0.0619 |
0.0257 |
0.47 |
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17.16 |
0.0635 |
0.0430 |
0.27 |
14.5 Design of a Tessar Lens |
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Figure 14.25 Aberrations of Tessar Setup G. |
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14.5.6 Final Steps |
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We must now study the effect of changing the cemented interface c6. This was arbitrarily set at 0.45, and we will next repeat the entire design with c6 ¼ 0.325. The resulting lens is decidedly different from the previous design, as shown in the following table:
c |
d |
n |
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0.328 |
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0.4 |
1.61128 |
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with f 0 ¼ 10, l0 ¼ 9.20712, LA0 ( f/4.5) ¼ 0.08714, LZA ( f/6.4) ¼ –0.03475, OSC ( f/4.5) ¼ 0, P (D – d) Dn ¼ –0.0000707, lateral color (17 ) ¼ –0.00121. The results are shown in Table 14.16.
These aberrations are shown in Figure 14.26. The field is a little narrower than before but quite satisfactory. It should be noted that both of the color aberrations
418 Unsymmetrical Photographic Objectives
Table 14.16
Astigmatism and Distortion for Second Tessar System
Field (deg) |
Xs0 |
Xt0 |
Distortion (%) |
25.41 |
0.0408 |
0.0905 |
þ0.12 |
21.38 |
0.0244 |
0.0198 |
0.04 |
17.22 |
0.0413 |
0.0157 |
0.06 |
30°
T S
20 |
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Z
10
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0.1 0.2 |
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–0.1 0 |
Figure 14.26 Aberrations of second Tessar system.
are negative; to rectify this requires a small increase in the V number of the glass used for the rear crown element, say to SK-1, which has ne ¼ 1.61282 and Ve ¼ 56.74, or SK-19 with ne ¼ 1.61597 and Ve ¼ 57.51. The lens designer should always be mindful of the impact glass choice can have on a design.
The chief matter requiring study is the meridional ray plot in Figure 14.27, which should be compared with the previous graph in Figure 14.23. It is immediately clear that the change from c6 ¼ 0.325 to 0.45 has had the effect of raising the lower end of the curve and depressing the upper end. That is, strengthening c6 has introduced some undercorrected oblique spherical aberration to the existing negative higher-order coma, with an improvement in the overall quality of the lens. The lower end of the curve needs cutting off more than the upper end, but obviously we cannot cut it back beyond the marginal ray aperture.
The best way to improve this Tessar is to raise the refractive indices, preferably above 1.6 in all elements. It is doubtful if changing the thicknesses would have any significant effect.
