Wide angle fast speed lens with only 4 elementsDave Shafer
The document discusses the design of a wide angle fast speed lens with 4 elements and a 90 degree field of view at f/2.0 aperture. By using extensive aspherics, including a nearly zero power double-aspheric element, amazing lens designs can be achieved with very high image quality correction despite the simple design. While the initial designs are monochromatic, adding additional lens elements can provide color correction.
Cooke triplet lens with freeform surfacesDave Shafer
The document discusses optimizing a Cooke Triplet lens design for a strip field using freeform surfaces. It finds that with 10th order conventional aspherics on all surfaces, the design can be diffraction-limited over a 20 degree field at f/2.5. Replacing the aspherics with 10th order freeform surfaces and optimizing for a 20x1.5 degree strip field improves performance tenfold to a wavefront of 0.0040 waves rms. Narrowing the strip field to 20x0.5 degrees further improves performance to 0.0025 waves rms, showing the benefits of freeform surfaces for strip field designs.
Some odd and interesting monocentric designs 2005Dave Shafer
This document summarizes several monocentric optical designs created by David Shafer about 30 years ago. It begins by looking at fully monocentric designs like the Sutton ball lens and a theoretical "perfect do-nothing lens". It then discusses how monocentric designs have the same performance when used backwards or with shuffled surface orders. Several examples of monocentric catadioptric systems are provided, including some with refractive elements added. The document concludes by examining designs that combine monocentric and flat surfaces, such as the Dyson, Wynne-Dyson, and Rosch designs.
This document discusses various optical design tricks and techniques for designing optical systems using monocentric, nearly concentric, and concentric lens configurations. Some key points:
- Monocentric designs have no unique optical axis and forward and backward paths are indistinguishable. Nearly concentric lenses act as if located at their centers of curvature and can introduce spherical aberration.
- Monocentric systems have equivalent aberrations regardless of surface order. Concentric lenses in front of or behind the aperture stop are also equivalent.
- The Gabor telescope design has better higher-order performance than the Bouwers monocentric design. Nearly concentric lenses can simulate aspheric surfaces.
- Lens designs
A survey of some unusual telescope designs. One has a 20 meter diameter f/1.0 spherical primary mirror while others are suitable for amateur astronomers to make.
1) Optical design techniques include investigating multiple versions of simple designs to find the best one, as different versions can have tradeoffs in higher-order aberrations.
2) Stop shift theory is a useful technique for creating new designs by finding aperture stop positions that correct specific aberrations, such as lateral color, even if the final stop position is constrained.
3) Combining simple optical systems with useful properties, such as common axial color cancellation, is a way to develop new complex corrected designs like the CMO (catadioptric, mirror, objective) type.
Extreme pixels per volume optical designDave Shafer
The surprising benefits are shown of superimposing a diffractive surface on top of an aspheric surface to get very high performance designs with a very narrow spectral bandwidth. The combination on the same surface allows independent control of a ray's direction and phase..
A method is described of designing cell phone lenses that automatically results in much smoother surfaces without the usual very "wiggly" aspheric shapes.
Wide angle fast speed lens with only 4 elementsDave Shafer
The document discusses the design of a wide angle fast speed lens with 4 elements and a 90 degree field of view at f/2.0 aperture. By using extensive aspherics, including a nearly zero power double-aspheric element, amazing lens designs can be achieved with very high image quality correction despite the simple design. While the initial designs are monochromatic, adding additional lens elements can provide color correction.
Cooke triplet lens with freeform surfacesDave Shafer
The document discusses optimizing a Cooke Triplet lens design for a strip field using freeform surfaces. It finds that with 10th order conventional aspherics on all surfaces, the design can be diffraction-limited over a 20 degree field at f/2.5. Replacing the aspherics with 10th order freeform surfaces and optimizing for a 20x1.5 degree strip field improves performance tenfold to a wavefront of 0.0040 waves rms. Narrowing the strip field to 20x0.5 degrees further improves performance to 0.0025 waves rms, showing the benefits of freeform surfaces for strip field designs.
Some odd and interesting monocentric designs 2005Dave Shafer
This document summarizes several monocentric optical designs created by David Shafer about 30 years ago. It begins by looking at fully monocentric designs like the Sutton ball lens and a theoretical "perfect do-nothing lens". It then discusses how monocentric designs have the same performance when used backwards or with shuffled surface orders. Several examples of monocentric catadioptric systems are provided, including some with refractive elements added. The document concludes by examining designs that combine monocentric and flat surfaces, such as the Dyson, Wynne-Dyson, and Rosch designs.
This document discusses various optical design tricks and techniques for designing optical systems using monocentric, nearly concentric, and concentric lens configurations. Some key points:
- Monocentric designs have no unique optical axis and forward and backward paths are indistinguishable. Nearly concentric lenses act as if located at their centers of curvature and can introduce spherical aberration.
- Monocentric systems have equivalent aberrations regardless of surface order. Concentric lenses in front of or behind the aperture stop are also equivalent.
- The Gabor telescope design has better higher-order performance than the Bouwers monocentric design. Nearly concentric lenses can simulate aspheric surfaces.
- Lens designs
A survey of some unusual telescope designs. One has a 20 meter diameter f/1.0 spherical primary mirror while others are suitable for amateur astronomers to make.
1) Optical design techniques include investigating multiple versions of simple designs to find the best one, as different versions can have tradeoffs in higher-order aberrations.
2) Stop shift theory is a useful technique for creating new designs by finding aperture stop positions that correct specific aberrations, such as lateral color, even if the final stop position is constrained.
3) Combining simple optical systems with useful properties, such as common axial color cancellation, is a way to develop new complex corrected designs like the CMO (catadioptric, mirror, objective) type.
Extreme pixels per volume optical designDave Shafer
The surprising benefits are shown of superimposing a diffractive surface on top of an aspheric surface to get very high performance designs with a very narrow spectral bandwidth. The combination on the same surface allows independent control of a ray's direction and phase..
A method is described of designing cell phone lenses that automatically results in much smoother surfaces without the usual very "wiggly" aspheric shapes.
More of a new family of freeform mirror telescopesDave Shafer
The document discusses new families of telescope designs with two or three mirrors and multiple reflections between the mirrors. These designs can achieve good correction for spherical aberration, coma, and astigmatism with just two or three mirrors. Some key points:
- Four families of two-mirror designs exist with three reflections between the mirrors. Tilting and shaping the mirrors as aspheres allows for unobscured designs.
- Three-mirror designs with four reflections between the mirrors can also produce flat, anastigmatic images with compact packaging. Different sequences of reflections off the three mirrors are possible.
- While these multiple reflection designs open up new possibilities, conventional three-mirror freeform designs may still
A modification of the Double-Gauss design with two diffractive surfaces is described with very enhanced performance. The key is an interaction between the aberrations of the two diffractive surfaces and the aberrations of a curved substrate lens.
The document discusses how early lens design progress was hindered by slow hand calculations and lack of modern materials. It provides examples of simple lens designs that were possible even pre-computer but had limited applications without modern technologies. The document emphasizes that while computers have advanced design capabilities, fundamental design ideas and theories are more important. It provides several examples of innovative lens designs the author developed through conceptual thinking alone. The document cautions against overuse of new technologies like freeform surfaces and metasurfaces without consideration of conventional design alternatives.
New catadioptric design type fast speed and wide fieldDave Shafer
A very simple catadioptric design is described that is capable of providing fast speed, like f/1.0, over a telecentric 65 degree field diameter with excellent aberration correction and an external pupil
The biblical Exodus - what really happened?Dave Shafer
An attempt to explain by natural causes most of the events of the biblical Exodus as If they had actually happened. Whether or not they did happen is not relevant to this presentation.
1) The document describes a proposed design for an unobscured astronomical camera with a 22 degree field of view and f/2 speed, to be used for a new large telescope in Hawaii.
2) It explores starting with an existing 5-mirror spherical design that was used on space missions, but determines a 3-mirror freeform aspheric design may be better.
3) The document presents an example 3-mirror freeform aspheric design that meets the requirements, with all mirrors tilted and shaped as aspheres to produce an unobscured 22 degree field of view at f/2.
One example is given of a fast speed wide angle telescope design that uses freeform aspherics to give great performance gains compared to conventional aspherics
Modified freeform offner, august 11, 2021Dave Shafer
An Offner 1.0X relay system can be given a greatly increased field size with good aberration correction by adding to the design two 45 degree flat fold mirrors that are given some freeform aspheric deformation.
Broad band catadioptric design with long working distanceDave Shafer
A broad spectral band high NA catadioptric design is developed that has a long working distance. The design is developed from first principles and the evolution of the design shows what the process of lens design is like.
A zoom lens design method, july 3, 2013Dave Shafer
This document describes the steps taken to design a compact zoom lens with a focal length range of 8-30mm and constant f-number of 2.8. The design process began with a simple monochromatic design using aspherics, which was then optimized. Aspheric lenses were replaced one by one with equivalent spherical doublets. Groups were achromatized separately, first the moving groups and then the fixed groups. The final design was fully color corrected but unable to focus close objects. The designer may need to backtrack to an earlier monochromatic design stage to solve the focusing issue before continuing color correction.
The power of negative thinking in optical designDave Shafer
This document discusses optical lens design. It begins with an overview of the talk, which will review previous material and introduce new ideas. The document then discusses challenges with correcting aberrations in highly optimized designs. It provides examples of triplet lens designs and compares their performance based on third-order assumptions versus ray-tracing optimization. The document introduces new compact lens designs that achieve wide angles and fast speeds using no vignetting. It shows examples achieving various specifications like being diffraction limited or having specific fields of view and focal lengths.
1) The document describes several simple mirror systems that have unusual optical characteristics despite using few elements.
2) Many of the designs use multiple reflections off of spherical or aspheric surfaces to correct aberrations like astigmatism.
3) Unexpected solutions are found, such as designs that correct third-order spherical aberration using a single reflective surface.
Highlights of my 48 years in optical designDave Shafer
the art ASML
machines can
print circuit
features on
chips that are
only a few
dozen atoms
wide.
Dave Shafer has had a long career in optical design spanning 48 years. Some highlights include:
1) As a young boy, he was fascinated by optics and did experiments with magnifying glasses and homemade microscopes.
2) He studied optics in college in the 1960s when there were only two undergraduate optics programs worldwide.
3) Over his career, he has designed optics for applications like military reconnaissance, medical imaging, laser fusion experiments, lithography steppers, and space telescopes.
4) He started his own optical design consulting business
A recent article shows the use of a curved image in a three mirror freeform design and the performance benefits that brings. Here I duplicate their results but get better image quality without their "fancy" surface description or a toric image. surface
Dennis gabor's catadioptric design and some new variationsDave Shafer
A variety of optical designs are developed and discussed, inspired by Gabor's very simple and largely unknown design. Some are extremely high NA (0.999!!!) with a wide field of view and diffraction-limited correction.
More of a new family of freeform mirror telescopesDave Shafer
The document discusses new families of telescope designs with two or three mirrors and multiple reflections between the mirrors. These designs can achieve good correction for spherical aberration, coma, and astigmatism with just two or three mirrors. Some key points:
- Four families of two-mirror designs exist with three reflections between the mirrors. Tilting and shaping the mirrors as aspheres allows for unobscured designs.
- Three-mirror designs with four reflections between the mirrors can also produce flat, anastigmatic images with compact packaging. Different sequences of reflections off the three mirrors are possible.
- While these multiple reflection designs open up new possibilities, conventional three-mirror freeform designs may still
A modification of the Double-Gauss design with two diffractive surfaces is described with very enhanced performance. The key is an interaction between the aberrations of the two diffractive surfaces and the aberrations of a curved substrate lens.
The document discusses how early lens design progress was hindered by slow hand calculations and lack of modern materials. It provides examples of simple lens designs that were possible even pre-computer but had limited applications without modern technologies. The document emphasizes that while computers have advanced design capabilities, fundamental design ideas and theories are more important. It provides several examples of innovative lens designs the author developed through conceptual thinking alone. The document cautions against overuse of new technologies like freeform surfaces and metasurfaces without consideration of conventional design alternatives.
New catadioptric design type fast speed and wide fieldDave Shafer
A very simple catadioptric design is described that is capable of providing fast speed, like f/1.0, over a telecentric 65 degree field diameter with excellent aberration correction and an external pupil
The biblical Exodus - what really happened?Dave Shafer
An attempt to explain by natural causes most of the events of the biblical Exodus as If they had actually happened. Whether or not they did happen is not relevant to this presentation.
1) The document describes a proposed design for an unobscured astronomical camera with a 22 degree field of view and f/2 speed, to be used for a new large telescope in Hawaii.
2) It explores starting with an existing 5-mirror spherical design that was used on space missions, but determines a 3-mirror freeform aspheric design may be better.
3) The document presents an example 3-mirror freeform aspheric design that meets the requirements, with all mirrors tilted and shaped as aspheres to produce an unobscured 22 degree field of view at f/2.
One example is given of a fast speed wide angle telescope design that uses freeform aspherics to give great performance gains compared to conventional aspherics
Modified freeform offner, august 11, 2021Dave Shafer
An Offner 1.0X relay system can be given a greatly increased field size with good aberration correction by adding to the design two 45 degree flat fold mirrors that are given some freeform aspheric deformation.
Broad band catadioptric design with long working distanceDave Shafer
A broad spectral band high NA catadioptric design is developed that has a long working distance. The design is developed from first principles and the evolution of the design shows what the process of lens design is like.
A zoom lens design method, july 3, 2013Dave Shafer
This document describes the steps taken to design a compact zoom lens with a focal length range of 8-30mm and constant f-number of 2.8. The design process began with a simple monochromatic design using aspherics, which was then optimized. Aspheric lenses were replaced one by one with equivalent spherical doublets. Groups were achromatized separately, first the moving groups and then the fixed groups. The final design was fully color corrected but unable to focus close objects. The designer may need to backtrack to an earlier monochromatic design stage to solve the focusing issue before continuing color correction.
The power of negative thinking in optical designDave Shafer
This document discusses optical lens design. It begins with an overview of the talk, which will review previous material and introduce new ideas. The document then discusses challenges with correcting aberrations in highly optimized designs. It provides examples of triplet lens designs and compares their performance based on third-order assumptions versus ray-tracing optimization. The document introduces new compact lens designs that achieve wide angles and fast speeds using no vignetting. It shows examples achieving various specifications like being diffraction limited or having specific fields of view and focal lengths.
1) The document describes several simple mirror systems that have unusual optical characteristics despite using few elements.
2) Many of the designs use multiple reflections off of spherical or aspheric surfaces to correct aberrations like astigmatism.
3) Unexpected solutions are found, such as designs that correct third-order spherical aberration using a single reflective surface.
Highlights of my 48 years in optical designDave Shafer
the art ASML
machines can
print circuit
features on
chips that are
only a few
dozen atoms
wide.
Dave Shafer has had a long career in optical design spanning 48 years. Some highlights include:
1) As a young boy, he was fascinated by optics and did experiments with magnifying glasses and homemade microscopes.
2) He studied optics in college in the 1960s when there were only two undergraduate optics programs worldwide.
3) Over his career, he has designed optics for applications like military reconnaissance, medical imaging, laser fusion experiments, lithography steppers, and space telescopes.
4) He started his own optical design consulting business
A recent article shows the use of a curved image in a three mirror freeform design and the performance benefits that brings. Here I duplicate their results but get better image quality without their "fancy" surface description or a toric image. surface
Dennis gabor's catadioptric design and some new variationsDave Shafer
A variety of optical designs are developed and discussed, inspired by Gabor's very simple and largely unknown design. Some are extremely high NA (0.999!!!) with a wide field of view and diffraction-limited correction.
Lens designs with extreme image quality featuresDave Shafer
A variety of lens designs is described which have some image quality feature which is extreme - like an extremely wide spectral bandwidth or extremely high resolution.
Attention Eyecare Professionals.
Discover the New Breakthrough in Eyewear. Intellect progressive lens was developed by a team of scientists and CSC Group is now the exclusive manufacturer and distributor in the United States. View this slideshow to learn more about the Patient Benefits and Features.
Schmidt's three lens corrector for a spherical mirrorDave Shafer
Schmidt's aspheric plate in a Schmidt telescope design can be replaced by a group of three spherical lenses, as Schmidt himself showed, but he died before he could publish anything on this. Here I show many alternate versions to Schmidt's design.
This is the term project report for an Optical Mount project for MCHE 1940: Mechanical Engineering Design Studio
& Professional Practice, University of Georgia, Freshman Year
The project aimed to design new locking wheels for baby chairs that would lock when a baby is placed in the chair and unlock when the baby is removed. Three design solutions were developed using TRIZ and the Acclaro DFSS tool. Solution 3 was selected as the optimal design using a Pugh matrix. The design incorporated rubber, pins, a base, springs, rings, plates, wheels, and an axle. Validation testing found the design worked as intended within 60 working hours. A patent application was also prepared to protect the intellectual property.
Freeform aspheric telescope with an external pupilDave Shafer
A 4 mirror telescope design with freeform aspherics is described which has a distant external front pupil, for those situations that require this. It is unobscured and has a 10 degree diameter field at f/3.0 on an unvignetted flat image.
For the full video of this presentation, please visit:
https://www.embedded-vision.com/platinum-members/embedded-vision-alliance/embedded-vision-training/videos/pages/may-2017-embedded-vision-summit-gehlhar
For more information about embedded vision, please visit:
http://www.embedded-vision.com
Jessica Gehlhar, Vision Solutions Engineer at Edmund Optics, presents the "Introduction to Optics for Embedded Vision" tutorial at the May 2017 Embedded Vision Summit.
This talk provides an introduction to optics for embedded vision system and algorithm developers. Gehlhar begins by presenting fundamental imaging lens specifications and quality metrics. She explains key parameters and concepts such as field of view, f number, working f number, NA (numerical aperture), focal length, working distance, depth of field, depth of focus, resolution, MTF (modulation transfer function), distortion, keystoning, and telecentricity and their relationships. Optical design basics and trade-offs introduced include design types, aberrations, aspheres, pointing accuracy, sensor matching, color and protective coatings, filters, temperature and environmental considerations, and their relation to sensor artifacts.
She also explores manufacturing considerations, including testing the optical components and imaging lenses in a product, and the industrial optics used for a wide range of manufacturing tests. Depending on requirements, a wide variety of tests and calibrations may be performed. These tests and calibrations become important with designs that include technologies such as multi-camera, 3D, color and NIR (near-infrared).
A freeform aspheric version of the classic Dyson design gives much improved aberration correction and makes for designs that are fast speed and have a large field size, especially large rectangular strip fields
1. Margarita Andreou designed a mechanical apparatus to precisely hold ultrasound probes and resolution phantoms to reproducibly measure ultrasound imaging resolution.
2. An initial prototype had problems with setup and stability. A second design using optical rails for quick alignment was tested, showing fast, repeatable measurements.
3. Matlab software was created to automatically process images from the tests and calculate axial and lateral resolution values objectively. This helped ensure reproducible results without human subjectivity.
Progressive addition lenses (PALs) provide a gradual transition from distance to near vision without visible lines. PAL designs aim to maximize clear vision zones for distance, intermediate, and near viewing. Key design considerations include lens hardness, symmetry, prescription parameters, and lens surface asphericity. Modern PALs utilize advanced optical modeling and eye tracking technology to minimize distortions and provide natural vision across a wide range of viewing distances. While PALs offer continuous vision without lines, their transition zones may require more eye and head movement compared to single vision lenses.
This document provides information about progressive addition lenses (PALs), including their history, design, markings, fitting process, advantages, and disadvantages compared to bifocal lenses. Some key points:
- PALs were invented in the late 1950s and gradually increased in popularity as an alternative to bifocal lenses that provides clear vision from distance to near without visible lines.
- PAL designs can be "hard", with a rapid progression, or "soft" with a slower progression. Designs also differ in the size and location of distance, near, and intermediate zones.
- Fitting PALs properly requires selecting the right frame size and shape, measuring pupillary distance and fitting heights, and ver
This document provides information about pixels, pixel density, and scaling images across different displays. It begins with an overview of Steven Meyer's background in user experience design. It then discusses physical pixels and sub-pixels, and how color is represented at the pixel level. The document explains concepts like pixel pitch, resolution, pixels per inch, and how to calculate whether a display is a retina/high-dpi display. It also discusses challenges in scaling images across devices with different pixel densities like phones and monitors. The key point is that images need to be exported at the appropriate size to match physical sizes across devices and avoid blurriness from excessive scaling.
This document discusses various lens designs and technologies for high plus and minus lenses, progressive lenses, occupational lenses, and photochromic lenses. Key points include lens designs that can accommodate up to +/-16 diopters of power as well as up to 20 diopters of prism. Lens designs like freeform, franklin split, and presto are highlighted for their ability to control high prisms. Segmented lenses, digital surfaces, and specialty coatings are also covered.
This document summarizes standards and guidelines for ophthalmic lenses. It discusses markings that indicate lens properties like wavelength protection and tint density. Formulas are provided for determining appropriate base curves based on lens prescription, such as Vogel's formula. High powered lens designs are also outlined, including aspheric lenses for high plus powers and lenticular or myodisc designs for high minus powers to reduce edge thickness. Appropriate base curves are important for minimizing aberrations when viewing off-center.
The document discusses creative photography techniques used by top photographers to make their work stand out. It describes techniques using everyday household items like metal tubing, CDs, and prisms to create unique visual effects in camera without post-production editing. The ring of fire technique uses metal tubing in front of the lens and an external light source to add a circular flare around the subject. CDs can also add colorful light flares but are difficult to compose with. Prisming and other new techniques are helping move the field of photography forward in new ways.
Similar to Diffraction-limited pixels versus number of lens elements (20)
Aberration theory - A spectrum of design techniques for the perplexed - 1986.pdfDave Shafer
This document summarizes the design process for a Double-Gauss lens using aberration theory. It begins with the historical basis of two Gauss doublets back-to-back, then walks through building up a design from first principles using aberration theory. Key steps include: 1) Adding concentric surfaces to cancel astigmatism; 2) Adding an aplanatic/aplanatic shell to introduce Petzval curvature; 3) Adding a concentric/concentric shell to push the system to a telecentric exit pupil. This allows removing the final lens element far from the image. The result is a corrected Double-Gauss design arrived at through theoretical understanding rather than trial-and-error optimization.
1) Snakes played an important religious role in ancient Egypt and were depicted widely in art and iconography. When Moses was in Egypt, snake imagery would have been everywhere.
2) Some scholars propose that the Levite tribe, including Moses and Aaron, may have originated as Egyptian priests who followed Moses out of Egypt and had connections to snake handling and worship. References to snakes in the Bible may relate to this.
3) In the Bible, Moses was instructed by God to make a copper snake idol to cure snakebites, contradicting idol worship bans. This later developed into a snake cult in Jerusalem until being destroyed centuries later. Ancient Near Eastern snake cults and worship were common.
Georgia O'Keeffe was an American artist known for her paintings of flowers, landscapes, and cityscapes. She pioneered abstract painting in the early 20th century, creating non-representational works using only shapes, colors, and forms as early as 1915. Her early abstract paintings were prominently displayed by her husband Arthur Stieglitz at his 291 gallery, exposing the American public to this new style of art. O'Keeffe was influenced by Arthur Wesley Dow's principles of composition and abstraction, and she credited Arthur Dove as having the most significant impact on her development as a young artist moving her style towards abstraction.
Frederic Mistral wrote a long love poem called "Mireille" about his native region of Provence, describing its traditions, culture, and dialects. Charles Gounod later adapted this poem into his 1864 opera of the same name. While Gounod's opera "Faust" has been performed thousands of times, his "Mireille" set in Provence is now rarely performed. The opera showcases aspects of Provençal culture described in Mistral's poem, such as the folk dance called the Farandole, and beliefs in witches and sylphs.
A wide angle fast speed unobscured freeform aspheric mirror design for the IR is shown to be enormous in size compared to an all refractive 3 element lens of germanium with conventional aspherics and better performance.
Schiefspiegler telescope with corrector lensesDave Shafer
This document contains contact information for David Shafer of David Shafer Optical Design and describes an unobscured 6 inch aperture f/10 telescope design from 1990. The design uses BK7 lenses and spherical mirrors to produce a diffraction limited image over a 1 degree flat field with no tilt at f/10 and has a length approximately equal to the focal length. It also references a simplified version of the design from a slideshare presentation that has a shorter length of half the focal length using tilted lenses and spherical mirrors with an optional fold flat.
A survey of some interesting Gregorian telescope designs includes some with all spherical surfaces as well as some with a 20 meter spherical f/1.0 primary mirror and sub-aperture corrector mirrors.
New optical system corrected for all third order aberrations for all conjugat...Dave Shafer
An afocal unit magnification optical system is described which is corrected for 3rd order spherical aberration, coma, astigmatism, Petzval and distortion for all conjugate distances
The document discusses the history of the invention of the achromatic lens, which corrects chromatic aberration by using two lenses made of different glass types with different dispersions. In the early 1700s, British mathematician Chester Hall figured out the formula to correct color this way but did not know if suitable glasses existed. He later discovered by accident that eyeglasses used two different glass types. Hall contracted with two opticians to secretly make prototype lenses to prove his theory, but both subcontracted the work to George Bass, who assembled the lenses and discovered they eliminated chromatic aberration. John Dolland overheard of this and patented the invention, becoming rich.
The document discusses how social isolation during the COVID-19 pandemic has disrupted normal routines and activities. While there is uncertainty about the future, this time provides an opportunity to spend more time on hobbies, help neighbors, and cooperate with each other. With cooperation and support of one another, people can work to reduce stress and have a more positive outlook despite challenges posed by the current situation.
By using a diffractive surface to provide most of the focusing power, combined with aspheric lenses, a simple fast speed wide angle design is possible with excellent image quality. But a very large amount of color limits the useful spectral bandwidth to a very small amount.
Determination of Equivalent Circuit parameters and performance characteristic...pvpriya2
Includes the testing of induction motor to draw the circle diagram of induction motor with step wise procedure and calculation for the same. Also explains the working and application of Induction generator
Tools & Techniques for Commissioning and Maintaining PV Systems W-Animations ...Transcat
Join us for this solutions-based webinar on the tools and techniques for commissioning and maintaining PV Systems. In this session, we'll review the process of building and maintaining a solar array, starting with installation and commissioning, then reviewing operations and maintenance of the system. This course will review insulation resistance testing, I-V curve testing, earth-bond continuity, ground resistance testing, performance tests, visual inspections, ground and arc fault testing procedures, and power quality analysis.
Fluke Solar Application Specialist Will White is presenting on this engaging topic:
Will has worked in the renewable energy industry since 2005, first as an installer for a small east coast solar integrator before adding sales, design, and project management to his skillset. In 2022, Will joined Fluke as a solar application specialist, where he supports their renewable energy testing equipment like IV-curve tracers, electrical meters, and thermal imaging cameras. Experienced in wind power, solar thermal, energy storage, and all scales of PV, Will has primarily focused on residential and small commercial systems. He is passionate about implementing high-quality, code-compliant installation techniques.
Blood finder application project report (1).pdfKamal Acharya
Blood Finder is an emergency time app where a user can search for the blood banks as
well as the registered blood donors around Mumbai. This application also provide an
opportunity for the user of this application to become a registered donor for this user have
to enroll for the donor request from the application itself. If the admin wish to make user
a registered donor, with some of the formalities with the organization it can be done.
Specialization of this application is that the user will not have to register on sign-in for
searching the blood banks and blood donors it can be just done by installing the
application to the mobile.
The purpose of making this application is to save the user’s time for searching blood of
needed blood group during the time of the emergency.
This is an android application developed in Java and XML with the connectivity of
SQLite database. This application will provide most of basic functionality required for an
emergency time application. All the details of Blood banks and Blood donors are stored
in the database i.e. SQLite.
This application allowed the user to get all the information regarding blood banks and
blood donors such as Name, Number, Address, Blood Group, rather than searching it on
the different websites and wasting the precious time. This application is effective and
user friendly.
Digital Twins Computer Networking Paper Presentation.pptxaryanpankaj78
A Digital Twin in computer networking is a virtual representation of a physical network, used to simulate, analyze, and optimize network performance and reliability. It leverages real-time data to enhance network management, predict issues, and improve decision-making processes.
Build the Next Generation of Apps with the Einstein 1 Platform.
Rejoignez Philippe Ozil pour une session de workshops qui vous guidera à travers les détails de la plateforme Einstein 1, l'importance des données pour la création d'applications d'intelligence artificielle et les différents outils et technologies que Salesforce propose pour vous apporter tous les bénéfices de l'IA.
smart pill dispenser is designed to improve medication adherence and safety f...
Diffraction-limited pixels versus number of lens elements
1. Diffraction-limited pixels versus number of lens elements
David Shafer
David Shafer Optical Design
Fairfield, CT 06824
#203-259-1431
shaferlens@sbcglobal.net
2. For any optical design with a given
focal length there is some product
of the pupil diameter D and the
full field angle A for which he
design can be made diffraction-
limited over the whole field.
1) For a 100 mm focal length design what is the maximum number of diffraction-limited
pixels possible with a one-element design, a two-element design, a three element
design, etc. D is the pupil diameter in mm and A is the full field angle in degrees
2) What is the ratio of the maximum number of pixels divided by the number of
elements? And how does that change?
3. 100 mm focal length
Monochromatic at .55u
Only BK7 glass lenses
No aspherics
Real image on flat surface
.07 waves r.m.s. or better over field
Distortion not relevant
Non-zero center and edge thickness
and edge gaps to next lens.
Real stop can be inside glass
No vignetting
Design Problem Groundrules
4. For any design where the product of D and A gives
diffraction-limited performance over the whole field
both D and A can usually be changed by +/- 20% or
sometimes a lot more, to give the same D x A product,
and the reoptimized performance will still stay
diffraction-limited. There is a “sweet spot” within that
range where the D x A product is maximized.
There are two good single element designs, one
with a front aperture stop and one with a rear stop.
The sweet spot for the D x A product is near 190 for
the rear stop design and that is better than the 140
value of the front stop design. The first has a sweet
spot that does better with a larger D value while the
front stop does better with a large field A.
Not to same scale
D x A = 140
D x A = 190
5. D x A = 430
D x A = 415
With two lenses there are again two solutions, now
according to if the negative power is in front of or in
back of the aperture stop. Both designs have nearly
the same sweet spot combination of the optimum
choice for the pupil diameter D and the full field
angle A (in degrees), and they have nearly the same
value for the D X A product.
The best single lens value for D x A is 190. Here
with two lenses the value of D x A divided by the
number of lenses is 430/2 = 215, which is very close
to the single lens value. The number of pixels is an
area number and goes with the square of D x A, but
we will first just be looking at how D x A changes with
the number of lenses, not the squared value.
The two plots here are to the same scale and you
can see the design lengths differ.
6. D x A = 680
D x A = 528
Not to same scale
With three lenses there are again two best
solutions. The lesser of the two is much longer and
has a front external aperture stop. Now here is the
data so far.
Number of lenses Best D x A value Best value/ number of lenses
1 190 190
2 430 215
3 680 227
7. D x A = 1010
D x A = 770
Not to same scale
D x A = 700
With 4 lenses we know from the Monochromatic
Quartet IODC contest that the best design form is the
one shown on the upper left here and the 2nd best
form is shown below that. With 4 lenses and the
important extra variables from the glass thickness
there are several discrete good solution regions. With
5 and 6 lenses there are a large number of local
minima and it is hard to know if the best has been
found. Here D x A divided by 4 lenses gives 252
Front exterior stop design
8. D x A = 1400
For 5 lenses I have several quite different
configurations, one shown below, and there
are probably a few more good ones, but this
one here on the left is the best so far.
What is most interesting is the trend here
of D x A divided by the number of lenses.
Clearly that number has to eventually turn
around and decline for some value, not yet
reached, of the number of lenses. And D x A
also has to also slow down in its growth.
Number of lenses Best D x A value Best value/ number of lenses
1 190 190
2 430 215
3 680 227
4 1010 252
5 1550 310
D x A = 1550
9. D x A = 1800
It is interesting that this 6 lens design here
shows that, like the previous designs, the
highest “sweet spot” value for the D x A
product occurs when the field angle A is
increased but the D value does not change
much. This design here and the best 5 lens
design sort of look like a “ball lens” with a
field flattening lens at the image. It has a 90
degree field for A. Further improvements in
D x A will probably need a larger aperture D.
Number of lenses Best D x A value Best value/ number of lenses
1 190 190
2 430 215
3 680 227
4 1010 252
5 1550 310
6 1800 300
There is a lot of work involved in trying to find the
best 6 lens design and I can’t tell for sure if this one
here is it. If it is, then the numbers here are starting
to maybe turn around in value. But finding the best
7 lens design has not been done yet to show that
trend, if it is true. So I tried that next.
10. Next there was a surprise. I found a
pretty good 7 lens design and after a lot
of work on it the design slowly moved
to a place where one lens could be
removed with no performance penalty.
The result was a better 6 lens design
than what is shown in the previous
slide. With more work on that it
became clear that another lens could
come out and the result is this new 5
lens design shown here, with better
performance than my best 5 lens
design shown earlier, and also shown at
the bottom left here. It is also a little
better than the earlier best 6 lens
design. The new 5 lens design is much
larger in size than the old one.
D x A = 1840
D x A = 1550
These are two
very different
solution regions,
especially for the
first lens shape
11. D x A = 2024
After a lot of searching I found what
seems to be the best 6 lens design and
glass path is a very important part of the
solution. There are several good solutions
and it is hard to move from one to another.
This is not a practical design, in this 100
mm focal length, because of all the glass.
It is a very “relaxed” design with gentle
bending of the rays. All of the designs
shown so far have distortion (not a lot) and
that helps performance.
Here is the revised data, with the new 5
and 6 element results. There is a big jump
going from 4 to 5 lenses and it looks like
maybe at six lenses the trend is starting to
slow down. The best D x A values still
occur with a slow speed and a large field,
which is 90 degrees here.
Number of lenses Best D x A value Best value/ number
of lenses
1 190 190
2 430 215
3 680 227
4 1010 252
5 1840 368
6 2024 337
12. D x A = 2230
The best 7 lens design I could
find, after a lot of work, is
basically the 6 lens design with
one split lens. It looks like the
entrance pupil keeps moving
closer to the front as the
number of lenses increases.
This lens is the end of the line
for this study. I can not find an
8 lens design that is better
except by just a little bit.
The design has very gentle
bending of the rays.
Very many attempts were made to add a lens to this design but
it looks like this particular configuration is pretty much exhausted
now, or that it is in a very deep local minimum where nothing can
improve it. That is common among very “relaxed” designs.
13. Number of lenses Best D x A value Best value/ number of lenses
1 190 190
2 430 215
3 680 227
4 1010 252
5 1840 368
6 2025 337
7 2230 319
8 ? ?
The D x A value is proportional to the
diameter of the image, measured in Airy
disks. The total number of Airy disks
would be the square of that and is a
measure of how much information the
designs can transmit. Usually the
performance drops off very quickly as
soon as you get even slightly outside of
the optimized field diameter so there is
very little useful information outside of
that. So the square of D x A does
accurately indicate the total amount of
information transfer by the design.
It looks like the effect of adding additional lenses
has started to decline, which it must eventually do.
But it might be that some new design configuration
can be found that breaks away from the designs
shown here of 4,5,6, and 7 lenses, which have a
similar type of configuration. But I have looked long
and hard for that and have not found something
new that is better than what is covered here.
14. Discussion
This is a very artificial design problem in several ways. But by limiting the scope of it the
difficulty of finding optimum designs is reduced to a reasonable level. No cemented lenses are
allowed and an index break across a cemented surface is a very powerful design tool, like in
monocentric ball lenses. But that would expand the scope of the problem too much. Having
all the lenses be low index BK7 is also a restriction which hurts potential performance. I have
limited the length to be 4X the focal length and all of these more complex designs, with close
to 90 degree fields, want to be at least that long. And not allowing any vignetting removes a
way to extend the field size while cutting off bad rays. But within these various constraints I
think that the results given here have some validity and predictive value.
Not requiring distortion correction makes a big difference in the wide angle performance
and allows for lens configurations that maximize the D x A product but have considerable
distortion at 90 degree fields. The D x A product is easiest to improve by increasing A, the field
angle, and not D, the aperture diameter. That is because higher-order aperture aberrations
are mostly a higher polynomial degree than higher-order field angle dependency and
therefore increase the fastest.
15. The optimum designs for the D x A product all have very gentle ray bendings
and are “relaxed” designs. It turns out that designs like that are very difficult to
optimize. The low-order derivatives of the parameters are very “weak” because
of the way the rays are bent gradually from surface to surface. That makes it hard
for an optimization program to work well. It is also very hard to find out how to
add a lens to a “relaxed” design to improve the performance.
In this study here I was not able to find an 8 lens design that is more than
slightly better than the best 7 lens design, and that 7 lens design is not as
improved as I would like compared to the 6 lens design. Going to longer lengths,
higher index glass, cemented lenses, Merte surfaces, etc. would change this but
without that it looks like I am stuck at 7 lenses. It is hard to see how the
configuration could be any different, for the best wide angle form, from what we
have here – an inverse form with front negative power, long length, and a
negative field flattener at the image.
More discussion
16. If anyone wants to take on the 8 lens design problem and gets something
good I would love to hear about it, at shaferlens@sbcglobal.net.