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
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.
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.
Multiple solutions in very simple optical designsDave Shafer
Several optical design examples show how multiple solutions can exist even in very simple systems. Time spent in looking for them is often more useful then simply optimizing the first solution that you find, which may not be the best of the alternates..
A high performance design is described that uses freeform aspherics to give an unobscured reflective telescope with a 22 degree field of view at f/2.0 on a flat image with no vignetting. The entrance pupil is out in front of the system, one focal length in front, and that is very difficult to achieve.
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
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.
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.
Multiple solutions in very simple optical designsDave Shafer
Several optical design examples show how multiple solutions can exist even in very simple systems. Time spent in looking for them is often more useful then simply optimizing the first solution that you find, which may not be the best of the alternates..
A high performance design is described that uses freeform aspherics to give an unobscured reflective telescope with a 22 degree field of view at f/2.0 on a flat image with no vignetting. The entrance pupil is out in front of the system, one focal length in front, and that is very difficult to achieve.
Freeform aspherics in telescope design, #2Dave Shafer
An example is given of a three mirror wide angle fast speed telescope design using freeform aspherics, showing how it evolved from a design with conventional aspherics
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.
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 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.
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.
Freeform aspherics in telescope design, #2Dave Shafer
An example is given of a three mirror wide angle fast speed telescope design using freeform aspherics, showing how it evolved from a design with conventional aspherics
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.
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 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.
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.
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.
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
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.
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
Online aptitude test management system project report.pdfKamal Acharya
The purpose of on-line aptitude test system is to take online test in an efficient manner and no time wasting for checking the paper. The main objective of on-line aptitude test system is to efficiently evaluate the candidate thoroughly through a fully automated system that not only saves lot of time but also gives fast results. For students they give papers according to their convenience and time and there is no need of using extra thing like paper, pen etc. This can be used in educational institutions as well as in corporate world. Can be used anywhere any time as it is a web based application (user Location doesn’t matter). No restriction that examiner has to be present when the candidate takes the test.
Every time when lecturers/professors need to conduct examinations they have to sit down think about the questions and then create a whole new set of questions for each and every exam. In some cases the professor may want to give an open book online exam that is the student can take the exam any time anywhere, but the student might have to answer the questions in a limited time period. The professor may want to change the sequence of questions for every student. The problem that a student has is whenever a date for the exam is declared the student has to take it and there is no way he can take it at some other time. This project will create an interface for the examiner to create and store questions in a repository. It will also create an interface for the student to take examinations at his convenience and the questions and/or exams may be timed. Thereby creating an application which can be used by examiners and examinee’s simultaneously.
Examination System is very useful for Teachers/Professors. As in the teaching profession, you are responsible for writing question papers. In the conventional method, you write the question paper on paper, keep question papers separate from answers and all this information you have to keep in a locker to avoid unauthorized access. Using the Examination System you can create a question paper and everything will be written to a single exam file in encrypted format. You can set the General and Administrator password to avoid unauthorized access to your question paper. Every time you start the examination, the program shuffles all the questions and selects them randomly from the database, which reduces the chances of memorizing the questions.
Understanding Inductive Bias in Machine LearningSUTEJAS
This presentation explores the concept of inductive bias in machine learning. It explains how algorithms come with built-in assumptions and preferences that guide the learning process. You'll learn about the different types of inductive bias and how they can impact the performance and generalizability of machine learning models.
The presentation also covers the positive and negative aspects of inductive bias, along with strategies for mitigating potential drawbacks. We'll explore examples of how bias manifests in algorithms like neural networks and decision trees.
By understanding inductive bias, you can gain valuable insights into how machine learning models work and make informed decisions when building and deploying them.
We have compiled the most important slides from each speaker's presentation. This year’s compilation, available for free, captures the key insights and contributions shared during the DfMAy 2024 conference.
Literature Review Basics and Understanding Reference Management.pptxDr Ramhari Poudyal
Three-day training on academic research focuses on analytical tools at United Technical College, supported by the University Grant Commission, Nepal. 24-26 May 2024
NO1 Uk best vashikaran specialist in delhi vashikaran baba near me online vas...Amil Baba Dawood bangali
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Harnessing WebAssembly for Real-time Stateless Streaming PipelinesChristina Lin
Traditionally, dealing with real-time data pipelines has involved significant overhead, even for straightforward tasks like data transformation or masking. However, in this talk, we’ll venture into the dynamic realm of WebAssembly (WASM) and discover how it can revolutionize the creation of stateless streaming pipelines within a Kafka (Redpanda) broker. These pipelines are adept at managing low-latency, high-data-volume scenarios.
KuberTENes Birthday Bash Guadalajara - K8sGPT first impressionsVictor Morales
K8sGPT is a tool that analyzes and diagnoses Kubernetes clusters. This presentation was used to share the requirements and dependencies to deploy K8sGPT in a local environment.
HEAP SORT ILLUSTRATED WITH HEAPIFY, BUILD HEAP FOR DYNAMIC ARRAYS.
Heap sort is a comparison-based sorting technique based on Binary Heap data structure. It is similar to the selection sort where we first find the minimum element and place the minimum element at the beginning. Repeat the same process for the remaining elements.
Mirror corrector for a 10 meter fast speed parabola
1. Dave Shafer
David Shafer Optical Design
Fairfield, CT 06824
203-259-1431
shaferlens@sbcglobal.net
Simple mirror corrector for a huge fast speed parabolic mirror
2. The aberration theory behind this very
simple design is explained in my
Slideshare post at
https://www.slideshare.net/operacrazy/gregorian-telescope-designs
It is remarkable that the extremely high level of
correction (on a slightly curved image surface) of this
huge very fast f/.7 speed parabolic mirror is
accomplished with just three subaperture corrector
elements – the small conic secondary mirror (a pure
conic, easily testable at its foci) only 10% of the
diameter of the big primary mirror, and two tiny (in
relative size) low order aspheric mirrors near the
intermediate image.