- •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
Chapter 14
Unsymmetrical Photographic
Objectives
14.1 THE PETZVAL PORTRAIT LENS
This ancient lens was the first photographic objective to be deliberately designed rather than being put together by an empirical selection of lenses out of a box. It consists of two fairly thin achromats spaced widely apart with a central stop.1 It has excellent correction for spherical aberration and coma, but because the Petzval sum is uncorrected, the angular field is limited by astigmatism to about 12 to 15 from the axis. Modified forms of the Petzval lens are still used, mainly for the projection of 16 and 8 mm movie films and other projection devices, although if a negative field flattener is added close to the image plane the lens becomes a true anastigmat, and in this form it has been used as a long-focal-length lens for aerial reconnaissance purposes.
The front component of the original Petzval design of 1839 was an ordinary f/5 telescope doublet. It is possible that Petzval attempted to assemble two identical lenses symmetrically about a central stop, in order to raise the aperture to f/3.5 for use with the slow daguerreotype plates of the time, but the aberrations were so bad that he had to separate the two elements in the rear component and bend them independently to correct the spherical aberration and coma. Later, in 1860, J. H. Dallmeyer turned the rear component around,2 with the crown element leading, and he thus obtained a lens that was better than the Petzval design near the middle of the field, but the inevitable uncorrected astigmatism was so great that the two designs are virtually indistinguishable. In 1878 F. von Voigtla¨nder3 found that by suitably bending the front component of the Dallmeyer type he could cement the rear component also, and it is this last arrangement that is used today as a small projection lens of high aperture.
Copyright # 2010, Elsevier Inc. All rights reserved. |
379 |
DOI: 10.1016/B978-0-12-374301-5.00018-8
380 |
Unsymmetrical Photographic Objectives |
14.1.1 The Petzval Design
In designing a Petzval portrait lens it is customary to make both doublets of the same diameter and to mount the stop approximately midway between them. If the front doublet consists of the familiar form with an equiconvex crown, this stop position has the effect of making the tangential field of the front component somewhat backward-curving, and to correct this requires a positive rear component somewhat weaker than the front component. To correct the spherical aberration as well as the OSC and to flatten the tangential field, we find that we must select glass types having a rather large V difference; with the refractive indices used by Petzval, 1.51 and 1.57, a V difference of at least 18 is required. In the present examples the following Schott glasses are used:
(a)Crown: K-1, ne ¼ 1.51173, nF – nC ¼ 0.00824, Ve ¼ 62.10
(b)Flint: LF-6, ne ¼ 1.57046, nF – nC ¼ 0.01325, Ve ¼ 43.05
The V difference is 19.05.
The Front Component
For the front component we adopt a thin-lens focal length of 10 and a clear aperture of 1.8. This aperture may have to be adjusted later after the actual focal length of the system has been determined. For this front lens, the thin-lens formulas give ca ¼ 0.63706 and cb ¼ –0.30618. Assuming an equiconvex crown, our front component is as follows:
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0.31853
0.4 1.51173
0.31853
0.12 1.57046
(D – d) 0.086680
Assuming an air space of 2.6, the 10 principal ray enters at Lpr ¼ 2.054 and crosses the axis midway between the two lenses.
The Petzval Rear Component
For a Petzval-type rear component, we may start with the arbitrary Setup that follows:
14.1 The Petzval Portrait Lens |
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with f 0 ¼ 6.1898, l0 ¼ 3.9286, LA0 ( f/3.44) ¼ 0.0005, OSC ( f/3.44) ¼ 0.001944. The focal length and aberration data given here are calculated for the complete system. The space between the two rear elements was determined so that they would be in edge contact at a diameter of 1.8. As the design proceeds this separation must be recalculated for each Setup to maintain the edge–contact condition.
The best way to correct the spherical aberration and coma is to bend the two rear elements separately and plot a double graph as shown in Figure 14.1. The graph data are
(a)Original Setup A: LA0 ¼ 0.000449, OSC ¼ 0.001944
(b)Bend flint by 0.02 for Setup B: LA0 ¼ 0.024885, OSC ¼ 0.004688
(c)From Setup B, bend crown by 0.02 to obtain Setup C: LA0 ¼ 0.010455, OSC ¼ 0.001965
OSC
0.004
Bend
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Figure 14.1 Double graph for rear component of Petzval portrait lens ( f 0 ¼ 6.2).
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Unsymmetrical Photographic Objectives |
Extrapolating in the usual way, and because the graphs are remarkably straight, we quickly reach the aplanatic form (Setup D):
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with f 0 ¼ 6.2206, l0 ¼ 3.9233, LA0 ( f/3.46) ¼ –0.0009, OSC ( f/3.46) ¼ –0.00003. The fields along the computed 10 principal ray were Xs0 ¼ –0.0597, Xt0 ¼ –0.0123.
To move the fields backward, we must weaken the entire rear component. A few trials indicate that cc should be reduced by 0.025, and after recorrecting the spherical and chromatic aberrations and the OSC we obtain the following solution (Setup E):
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with f 0 ¼ 6.4012, l0 ¼ 4.0408, LA0 ( f/3.56) ¼ 0.0030, LZA ( f/5) ¼ –0.0021, OSC ( f/3.56) ¼ –0.00002, Ptz (10) ¼ 0.0811. The results are shown in Table 14.1. These aberrations are plotted in Figure 14.2.
The final check on our system is made by drawing a meridional ray plot at 10 obliquity, which is shown in Figure 14.3a. The abscissas are the height of each ray at the stop with the height of the marginal ray at the stop being shown on the graph ordinate. However, because of vignetting at the front and rear surfaces,
Table 14.1
Astigmatism and Distortion for Setup E
Field (deg) |
Xs0 |
Xt0 |
Distortion (%) |
15 |
0.1034 |
0.1551 |
0.32 |
10 |
0.0571 |
0.0007 |
0.11 |
14.1 The Petzval Portrait Lens |
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Figure 14.2 |
Aberrations of Setup E ( f 0 ¼ 6.4): (a) longitudinal spherical aberration and (b) |
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(b) 1.18 |
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–0.8 |
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Figure 14.3 Ray plots for Petzval objectives at 10 : (a) Ray plot with rear elements in close contact; (b) Ray plot with air-spaced rear elements.
which are assumed to have a free aperture of 1.8, only a part of the graph is valid. The upper and lower vignetted rays are indicated by VV, whereas the limiting rays through the top and bottom of the stop are marked SS on this graph. It should be noted particularly that the middle of the curve is straight and level as a result of the good correction of OSC and the flat tangential field at 10 , but
