- •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
334 |
Lenses in Which Stop Position Is a Degree of Freedom |
12.4 ACHROMATIC LANDSCAPE LENSES
12.4.1 The Chevalier Type
In this type, a flint-in-front lens of slightly meniscus shape is used, with stop in front and the concave side facing the distant object.
As an example we will use the following glasses:
(a)Flint: nd ¼ 1.62360, V ¼ 36.75, Dn ¼ 0.01697
(b)Crown: nd ¼ 1.52122, V ¼ 62.72, Dn ¼ 0.00831
For a focal length of 10, we find using Eq. (5-4)
ca ¼ 0:2269; cb ¼ þ0:4634
Assuming an equiconcave flint as a starter and establishing suitable thicknesses (actually those used here were too thick), we solve the last radius by the D – d method and find the focal length to be 10.515. After scaling down to a focal length of 10 we have
c |
d |
n |
|
|
|
0.1189 |
0.28 |
1.62360 |
|
||
0.1189 |
|
|
0.3424 |
0.56 |
1.52122 |
|
|
with f 0 ¼ 10.00, l0 ¼ 10.4510, LA0 ( f/15) ¼ –0.162, Petzval sum ¼ 0.0667. We next trace a set of oblique rays through the upper half of the lens at 20
to locate the stop position for zero coma (Figure 12.8). This gives the values shown in the table on the next page.
H′
3.58
3.57
3.56 |
|
|
|
|
|
|
|
|
L |
|
–3 |
–2 |
–1 |
0 |
|||||||
|
|
|||||||||
Figure 12.8 The H0 – L curve of a Chevalier achromat (20 ).
12.4 Achromatic Landscape Lenses |
335 |
||
|
|
|
|
|
L |
H 0 |
|
0 |
3.579278 |
|
|
1.0 |
3.566382 |
|
|
2.0 |
3.577830 |
|
|
|
3.0 |
3.576493 |
|
The inflection point of this graph is at L ¼ –1.67, and because the graph is S-shaped, the tangential field will obviously be backward-curving (see Section 12.1.2). Performing Coddington traces at several obliquities produces data for Figure 12.9 (see Table 12.5).
Unfortunately, it is not possible to flatten the tangential field in a lens of this type at the same time as eliminating the coma. The concave front face and the dispersive interface both contribute overcorrected astigmatism of about the same amount, and bending the lens merely increases one contribution while reducing the other. Using modern barium crown glass with a flint of the same index, one could make an achromatic lens that would behave like a simple landscape lens so far as the monochromatic aberrations are concerned, with the interface then being merely a buried surface. Another possibility is to depart
30°
20°
10°
–0.5 |
0 |
0.5 |
1 |
1.5 |
Figure 12.9 Astigmatism of a Chevalier achromat. The sagittal field is the solid curve and the tangential field is the dashed curve.
Table 12.5
Astigmatism and Distortion for Lens Shown in Figure 12.9
Field (deg) |
0 |
0 |
Distortion (%) |
Xs |
Xt |
||
30 |
0.341 |
1.325 |
4.18 |
20 |
0.134 |
0.394 |
1.84 |
10 |
0.043 |
0.079 |
0.46 |
336 |
Lenses in Which Stop Position Is a Degree of Freedom |
from strict achromatism by weakening the cemented interface, but the high cost of such a lens over that of a single element would be scarcely justified.
12.4.2 The Grubb Type
In 1857 Thomas Grubb2 made a lens that he called the aplanat, consisting of a meniscus-shaped crown-in-front achromat. The spherical aberration was virtually corrected by the strong cemented interface, and as a result the user had to accept either the coma or the field curvature since both could not be corrected together. The Grubb lens eventually led to the “Rapid Rectilinear” design discussed in Section 12.5.1.
12.4.3 A“New Achromat” Landscape Lens
Since the cemented interface in the “old” Chevalier achromat has the effect of overcorrecting the astigmatism at high obliquities, it is evident that we could reverse the effect if we were to use a crown glass of higher refractive index than the flint glass (a “new achromat”). Furthermore, this combination of refractive indices has the effect of reducing the Petzval sum, but it will be accompanied by a large increase in the spherical aberration.
The design procedure for a new achromat is entirely different from that for an old achromat, because now we leave the achromatizing to the end and solve the outside radii of curvature for Petzval sum and focal length. We select refractive indices such that there are a variety of dispersive powers available for achromatizing after the design is completed. Two typical refractive indices meeting this requirement are
(a)Flint: 1.5348 (available V numbers from 45.7 to 48.7)
(b)Crown: 1.6156 (available V numbers from 54.9 to 58.8)
As a first guess we will aim for a Petzval sum of 0.03 on a focal length of 10. We must also guess at a likely interface radius and lens thicknesses. This gives the following as a starting system.
c |
d |
n |
|
|
|
0.551
0.1 1.5348
0.164
0.4 1.6156
0.5687
12.4 Achromatic Landscape Lenses |
337 |
with f 0 ¼ 9.9998, l0 ¼ 10.8865, Petzval sum ¼ 0.030. The large thickness helps to reduce the Petzval sum without using very strong elements (see “A Thick Meniscus” in Section 11.2.2).
In plotting the H 0 L graph, we use a larger obliquity angle than before because new achromats tend to cover an exceptionally wide field. The graph shown in Figure 12.10 represents the curve for 25 , and we see that the inflection falls at L ¼ –0.326. The astigmatic field curves are also shown and indicate that they suffer higher-order astigmatic and Petzval terms. As was mentioned in Section 11.2.1, the longitudinal distance from the Petzval surface to the tangential focal line is three times as great as the corresponding sagittal astigmatism when considering primary (Seidel) aberrations.
In a like manner, when the secondary or fifth-order Petzval occurs, the
longitudinal distance from the secondary Petzval surface to the tangential focal line is five times as great as the corresponding sagittal astigmatism.3,4,5
The field focus locations can be written as
zt ¼ ½ð3AST3 þ PTZ3ÞH2 þ ð5AST5 þ PTZ5ÞH4&=u0
H′
4.53
4.52
L
–0.6 |
–0.4 |
–0.2 |
0 |
40°
30°
20°
10°
0
–0.5 0 0.5
Figure 12.10 Tentative design of a new-achromat lens. The sagittal field is the solid curve and the tangential field is the dashed curve.
338 |
Lenses in Which Stop Position Is a Degree of Freedom |
and |
|
|
zs ¼ ½ðAST3 þ PTZ3ÞH2 þ ðAST5 þ PTZ5ÞH4&=u0: |
It is evident that the collective interface should be made stronger to move the field inward, and a smaller Petzval sum would also be desirable. Hence for our next attempt we try c2 ¼ 0.25 and Petzval sum ¼ 0.027. The changes listed in the following table give the system that is shown in Figure 12.11.
c |
d |
n |
|
|
|
0.5777 |
0.1 |
1.5348 |
|
||
0.25 |
|
|
0.57795 |
0.4 |
1.6156 |
|
|
with f 0 ¼ 9.99996, l0 ¼ 10.91516, Petzval sum ¼ 0.027, LA0 ( f/15) ¼ –0.50, and stop position ¼ –0.102. The astigmatic and distortion behavior are shown in Table 12.6.
Assuming that this is acceptable, the last step is the selection of real glasses for achromatism. A few trials, using the D – d method, indicate that the following Schott glasses would be excellent:
(a)LLF1: ne ¼ 1.55099, Dn ¼ 0.01198, V ¼ 45.47
(b)N-SK4: ne ¼ 1.61521, Dn ¼ 0.01046, V ¼ 58.37
40°
30°
20°
10°
–0.5 |
0 |
0.5 |
1.0 |
Figure 12.11 Astigmatism of a new achromat, later form. The sagittal field is the solid curve and the tangential field is the dashed curve.
