Hartmann wavefront sensing Beamline alignment

MARX. Miroirs Actifs Rayons X pour micro et nanofocalisation X-ray Active Optics for micro and nanofocalisation

MARX Miroirs Actifs Rayons X pour micro et nanofocalisation X-ray Active Optics for micro and nanofocalisation Outline Goal of the MARX Project : To develop an X-ray active mirrors for micro or nano focalisation

Adaptive Optics for LIGO

Adaptive Optics for LIGO Justin Mansell Ginzton Laboratory LIGO-G990022-39-M Motivation Wavefront Sensor Outline Characterization Enhancements Modeling Projections Adaptive Optics Results Effects of Thermal

OPAL. SpotOptics. AUTOMATED WAVEFRONT SENSOR Single and double pass O P A L

Spotptics The software people for optics UTMTED WVEFRNT SENSR Single and double pass ccurate metrology of standard and aspherical lenses ccurate metrology of spherical and flat mirrors =0.3 to =60 mm F/1

X-ray mirror metrology using SCOTS/deflectometry Run Huang a, Peng Su a*, James H. Burge a and Mourad Idir b

X-ray mirror metrology using SCOTS/deflectometry Run Huang a, Peng Su a*, James H. Burge a and Mourad Idir b a College of Optical Sciences, the University of Arizona, Tucson, AZ 85721, U.S.A. b Brookhaven

SpotOptics. The software people for optics OPAL O P A L

Spotptics The software people for optics UTMTED WVEFRNT SENSR ccurate metrology of standard and aspherical lenses (single pass) ccurate metrology of spherical and flat mirrors (double pass) =0.3 to =50

Optical Components for Laser Applications. Günter Toesko - Laserseminar BLZ im Dezember

Günter Toesko - Laserseminar BLZ im Dezember 2009 1 Aberrations An optical aberration is a distortion in the image formed by an optical system compared to the original. It can arise for a number of reasons

CHARA Collaboration Review New York 2007 CHARA Telescope Alignment

CHARA Telescope Alignment By Laszlo Sturmann Mersenne (Cassegrain type) Telescope M2 140 mm R= 625 mm k = -1 M1/M2 provides an afocal optical system 1 m input beam and 0.125 m collimated output beam Aplanatic

Investigation of a Next Generation Piezo Bimorph Mirror

Investigation of a Next Generation Piezo Bimorph Mirror Simon Alcock 1, Ioana Nistea 1, John Sutter 1, Kawal Sawhney 1, Jean-Jacques Fermé 2, Christophe Thellier 2, Luca Peverini 2 1 Optics & Metrology

Characterisation of a novel super-polished bimorph mirror

Characterisation of a novel super-polished bimorph mirror Kawal Sawhney 1, Simon Alcock 1, Hongchang Wang 1, John Sutter 1 and Riccardo Signorato 2 1 Diamond Light Source Ltd. UK 2 BASC, D-51429 Bergisch

3.0 Alignment Equipment and Diagnostic Tools:

3.0 Alignment Equipment and Diagnostic Tools: Alignment equipment The alignment telescope and its use The laser autostigmatic cube (LACI) interferometer A pin -- and how to find the center of curvature

PROCEEDINGS OF SPIE. Measurement of low-order aberrations with an autostigmatic microscope

PROCEEDINGS OF SPIE SPIEDigitalLibrary.org/conference-proceedings-of-spie Measurement of low-order aberrations with an autostigmatic microscope William P. Kuhn Measurement of low-order aberrations with

1.1 Singlet. Solution. a) Starting setup: The two radii and the image distance is chosen as variable.

1 1.1 Singlet Optimize a single lens with the data λ = 546.07 nm, object in the distance 100 mm from the lens on axis only, focal length f = 45 mm and numerical aperture NA = 0.07 in the object space.

Puntino. Shack-Hartmann wavefront sensor for optimizing telescopes. The software people for optics

Puntino Shack-Hartmann wavefront sensor for optimizing telescopes 1 1. Optimize telescope performance with a powerful set of tools A finely tuned telescope is the key to obtaining deep, high-quality astronomical

Proposed Adaptive Optics system for Vainu Bappu Telescope

Proposed Adaptive Optics system for Vainu Bappu Telescope Essential requirements of an adaptive optics system Adaptive Optics is a real time wave front error measurement and correction system The essential

WaveMaster IOL. Fast and accurate intraocular lens tester

WaveMaster IOL Fast and accurate intraocular lens tester INTRAOCULAR LENS TESTER WaveMaster IOL Fast and accurate intraocular lens tester WaveMaster IOL is a new instrument providing real time analysis

Experience of synchrotron sources and optics modelling at Diamond Light Source

Experience of synchrotron sources and optics modelling at Diamond Light Source Lucia Alianelli Outline Microfocus MX beamline optics design (Principal Beamline Scientist G. Evans) Surface and interface

CHARA AO Calibration Process

CHARA AO Calibration Process Judit Sturmann CHARA AO Project Overview Phase I. Under way WFS on telescopes used as tip-tilt detector Phase II. Not yet funded WFS and large DM in place of M4 on telescopes

Lecture 4: Geometrical Optics 2. Optical Systems. Images and Pupils. Rays. Wavefronts. Aberrations. Outline

Lecture 4: Geometrical Optics 2 Outline 1 Optical Systems 2 Images and Pupils 3 Rays 4 Wavefronts 5 Aberrations Christoph U. Keller, Leiden University, keller@strw.leidenuniv.nl Lecture 4: Geometrical

Optics of Wavefront. Austin Roorda, Ph.D. University of Houston College of Optometry

Optics of Wavefront Austin Roorda, Ph.D. University of Houston College of Optometry Geometrical Optics Relationships between pupil size, refractive error and blur Optics of the eye: Depth of Focus 2 mm

Sequential Ray Tracing. Lecture 2

Sequential Ray Tracing Lecture 2 Sequential Ray Tracing Rays are traced through a pre-defined sequence of surfaces while travelling from the object surface to the image surface. Rays hit each surface once

Structure in out-of-focus beams of X-ray focusing mirrors: Causes and possible solutions. Fiona Rust Department of Physics, University of Bath

Structure in out-of-focus beams of X-ray focusing mirrors: Causes and possible solutions John Sutter, Simon Alcock, Kawal Sawhney Diamond Light Source Ltd Fiona Rust Department of Physics, University of

Lecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.

Lecture 2: Geometrical Optics Outline 1 Geometrical Approximation 2 Lenses 3 Mirrors 4 Optical Systems 5 Images and Pupils 6 Aberrations Christoph U. Keller, Leiden Observatory, keller@strw.leidenuniv.nl

Design of null lenses for testing of elliptical surfaces

Design of null lenses for testing of elliptical surfaces Yeon Soo Kim, Byoung Yoon Kim, and Yun Woo Lee Null lenses are designed for testing the oblate elliptical surface that is the third mirror of the

Lecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.

Lecture 2: Geometrical Optics Outline 1 Geometrical Approximation 2 Lenses 3 Mirrors 4 Optical Systems 5 Images and Pupils 6 Aberrations Christoph U. Keller, Leiden Observatory, keller@strw.leidenuniv.nl

WaveMaster IOL. Fast and Accurate Intraocular Lens Tester

WaveMaster IOL Fast and Accurate Intraocular Lens Tester INTRAOCULAR LENS TESTER WaveMaster IOL Fast and accurate intraocular lens tester WaveMaster IOL is an instrument providing real time analysis of

Breakout Session 3: Mirror Update. 2007/4/ /22 Peter M. Stefan LCLS Facility Advisory Committee (FAC) Meeting

Breakout Session 3: Mirror Update 2007/4/16-17 1/22 Peter M. Stefan LCLS Facility Advisory Committee (FAC) Meeting stefan@slac.stanford.edu Breakout Session 3: Mirror Update Overall Offset Mirror System

The Aberration Structure of the Keratoconic Eye

The Aberration Structure of the Keratoconic Eye Geunyoung Yoon, Ph.D. Department of Ophthalmology Center for Visual Science Institute of Optics Department of Biomedical Engineering University of Rochester

VATT Optical Performance During 98 Oct as Measured with an Interferometric Hartmann Wavefront Sensor

VATT Optical Performance During 98 Oct as Measured with an Interferometric Hartmann Wavefront Sensor S. C. West, D. Fisher Multiple Mirror Telescope Observatory M. Nelson Vatican Advanced Technology Telescope

Explanation of Aberration and Wavefront

Explanation of Aberration and Wavefront 1. What Causes Blur? 2. What is? 4. What is wavefront? 5. Hartmann-Shack Aberrometer 6. Adoption of wavefront technology David Oh 1. What Causes Blur? 2. What is?

Focusing X-ray beams below 50 nm using bent multilayers. O. Hignette Optics group. European Synchrotron Radiation Facility (FRANCE) Outline

Focusing X-ray beams below 50 nm using bent multilayers O. Hignette Optics group European Synchrotron Radiation Facility (FRANCE) Outline Graded multilayers resolution limits 40 nanometers focusing Fabrication

12.4 Alignment and Manufacturing Tolerances for Segmented Telescopes

330 Chapter 12 12.4 Alignment and Manufacturing Tolerances for Segmented Telescopes Similar to the JWST, the next-generation large-aperture space telescope for optical and UV astronomy has a segmented

OPTINO. SpotOptics VERSATILE WAVEFRONT SENSOR O P T I N O

Spotptics he software people for optics VERSALE WAVEFR SESR Accurate metrology in single and double pass Lenses, mirrors and laser beams Any focal length and diameter Large dynamic range Adaptable for

Paper Synopsis. Xiaoyin Zhu Nov 5, 2012 OPTI 521

Paper Synopsis Xiaoyin Zhu Nov 5, 2012 OPTI 521 Paper: Active Optics and Wavefront Sensing at the Upgraded 6.5-meter MMT by T. E. Pickering, S. C. West, and D. G. Fabricant Abstract: This synopsis summarized

Aberrations and adaptive optics for biomedical microscopes

Aberrations and adaptive optics for biomedical microscopes Martin Booth Department of Engineering Science And Centre for Neural Circuits and Behaviour University of Oxford Outline Rays, wave fronts and

Solution of Exercises Lecture Optical design with Zemax Part 6

2013-06-17 Prof. Herbert Gross Friedrich Schiller University Jena Institute of Applied Physics Albert-Einstein-Str 15 07745 Jena Solution of Exercises Lecture Optical design with Zemax Part 6 6 Illumination

Fabrication of 6.5 m f/1.25 Mirrors for the MMT and Magellan Telescopes

Fabrication of 6.5 m f/1.25 Mirrors for the MMT and Magellan Telescopes H. M. Martin, R. G. Allen, J. H. Burge, L. R. Dettmann, D. A. Ketelsen, W. C. Kittrell, S. M. Miller and S. C. West Steward Observatory,

Exercise 1 - Lens bending

Exercise 1 - Lens bending Most of the aberrations change with the bending of a lens. This is demonstrated in this exercise. a) Establish a lens with focal length f = 100 mm made of BK7 with thickness 5

Testing an off-axis parabola with a CGH and a spherical mirror as null lens

Testing an off-axis parabola with a CGH and a spherical mirror as null lens Chunyu Zhao a, Rene Zehnder a, James H. Burge a, Hubert M. Martin a,b a College of Optical Sciences, University of Arizona 1630

Review of Basic Principles in Optics, Wavefront and Wavefront Error

Review of Basic Principles in Optics, Wavefront and Wavefront Error Austin Roorda, Ph.D. University of California, Berkeley Google my name to find copies of these slides for free use and distribution Geometrical

Why is There a Black Dot when Defocus = 1λ?

Why is There a Black Dot when Defocus = 1λ? W = W 020 = a 020 ρ 2 When a 020 = 1λ Sag of the wavefront at full aperture (ρ = 1) = 1λ Sag of the wavefront at ρ = 0.707 = 0.5λ Area of the pupil from ρ =

Ron Liu OPTI521-Introductory Optomechanical Engineering December 7, 2009

Synopsis of METHOD AND APPARATUS FOR IMPROVING VISION AND THE RESOLUTION OF RETINAL IMAGES by David R. Williams and Junzhong Liang from the US Patent Number: 5,777,719 issued in July 7, 1998 Ron Liu OPTI521-Introductory

MMTO Technical Memorandum #03-1

MMTO Technical Memorandum #03-1 Fall 2002 f/9 optical performance of the 6.5m MMT analyzed with the top box Shack-Hartmann wavefront sensor S. C. West January 2003 Fall 2002 f/9 optical performance of

Large-Area Interference Lithography Exposure Tool Development

Large-Area Interference Lithography Exposure Tool Development John Burnett 1, Eric Benck 1 and James Jacob 2 1 Physical Measurements Laboratory, NIST, Gaithersburg, MD, USA 2 Actinix, Scotts Valley, CA

Computer Generated Holograms for Optical Testing

Computer Generated Holograms for Optical Testing Dr. Jim Burge Associate Professor Optical Sciences and Astronomy University of Arizona jburge@optics.arizona.edu 520-621-8182 Computer Generated Holograms

EUV projection optics and active mirror development at SAGEM

EUV projection optics and active mirror development at SAGEM R. Geyl,, M. Boutonne,, J.L. Carel,, J.F. Tanné, C. Voccia,, S. Chaillot,, J. Billet, Y. Poulard, X. Bozec SAGEM, Etablissement de St Pierre

Challenges of Optics for High Repetition Rate XFEL Source

Challenges of Optics for High Repetition Rate XFEL Source Liubov Samoylova, European XFEL GmbH ACTOP11, DIAMOND, April 5 th, 2011 2 European XFEL photon transport system - overview X-ray optics for XFEL:

ΘΘIntegrating closedloop adaptive optics into a femtosecond laser chain

Θ ΘΘIntegrating closedloop adaptive optics into a femtosecond laser chain www.imagine-optic.com The Max Planck Institute of Quantum Optics (MPQ) has developed an Optical Parametric Chirped Pulse Amplification

Ion Beam Figuring precision optics for synchrotron radiation sources L. PEVERINI, J. J. FERME & C. du JEU

www.thalesgroup.com Ion Beam Figuring precision optics for synchrotron radiation sources L. PEVERINI, J. J. FERME & C. du JEU Thales SESO S.A.S., Aix en Provence, 13593, France email: luca.peverini@fr.thalesgroup.com

Photon Diagnostics. FLASH User Workshop 08.

Photon Diagnostics FLASH User Workshop 08 Kai.Tiedtke@desy.de Outline What kind of diagnostic tools do user need to make efficient use of FLASH? intensity (New GMD) beam position intensity profile on the

Cardinal Points of an Optical System--and Other Basic Facts

Cardinal Points of an Optical System--and Other Basic Facts The fundamental feature of any optical system is the aperture stop. Thus, the most fundamental optical system is the pinhole camera. The image

Subjective Image Quality Metrics from The Wave Aberration

Subjective Image Quality Metrics from The Wave Aberration David R. Williams William G. Allyn Professor of Medical Optics Center For Visual Science University of Rochester Commercial Relationship: Bausch

Industrial quality control HASO for ensuring the quality of NIR optical components

Industrial quality control HASO for ensuring the quality of NIR optical components In the sector of industrial detection, the ability to massproduce reliable, high-quality optical components is synonymous

Collimation Tester Instructions

Description Use shear-plate collimation testers to examine and adjust the collimation of laser light, or to measure the wavefront curvature and divergence/convergence magnitude of large-radius optical

Manufacture of 8.4 m off-axis segments: a 1/5 scale demonstration

Manufacture of 8.4 m off-axis segments: a 1/5 scale demonstration H. M. Martin a, J. H. Burge a,b, B. Cuerden a, S. M. Miller a, B. Smith a, C. Zhao b a Steward Observatory, University of Arizona, Tucson,

Advanced Lens Design

Advanced Lens Design Lecture 3: Aberrations I 214-11-4 Herbert Gross Winter term 214 www.iap.uni-jena.de 2 Preliminary Schedule 1 21.1. Basics Paraxial optics, imaging, Zemax handling 2 28.1. Optical systems

ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof. Charles A. DiMarzio Northeastern University Fall 2008

ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof. Charles A. DiMarzio Northeastern University Fall 2008 July 2003+ Chuck DiMarzio, Northeastern University 11270-04-1

Aberration Theory and Prototype Mirror Experiments

Aberration Theory and Prototype Mirror Experiments Bruce Holenstein, Rich Mitchell, Dylan Holenstein 2010-2011 Alt-Az Initiative Hawaii Conference on Light Bucket Astronomy 1 Some Light Bucket Aberration

Better Imaging with a Schmidt-Czerny-Turner Spectrograph

Better Imaging with a Schmidt-Czerny-Turner Spectrograph Abstract For years, images have been measured using Czerny-Turner (CT) design dispersive spectrographs. Optical aberrations inherent in the CT design

Predicting the Performance of Space Coronagraphs. John Krist (JPL) 17 August st International Vortex Workshop

Predicting the Performance of Space Coronagraphs John Krist (JPL) 17 August 2016 1 st International Vortex Workshop Determine the Reality of a Coronagraph through End-to-End Modeling Use End-to-End modeling

FIRST INDIRECT X-RAY IMAGING TESTS WITH AN 88-mm DIAMETER SINGLE CRYSTAL

FERMILAB-CONF-16-641-AD-E ACCEPTED FIRST INDIRECT X-RAY IMAGING TESTS WITH AN 88-mm DIAMETER SINGLE CRYSTAL A.H. Lumpkin 1 and A.T. Macrander 2 1 Fermi National Accelerator Laboratory, Batavia, IL 60510

Optics for next generation light sources

Optics for next generation light sources Anton Barty Centre for Free Electron Laser Science Hamburg, Germany Key issues Optical specifications Metrology (mirror surfaces) Metrology (wavefront, focal spot)

Optical Design with Zemax for PhD

Optical Design with Zemax for PhD Lecture 7: Optimization II 26--2 Herbert Gross Winter term 25 www.iap.uni-jena.de 2 Preliminary Schedule No Date Subject Detailed content.. Introduction 2 2.2. Basic Zemax

Fabrication and alignment of 10X-Schwarzschild optics for F2X experiments

Fabrication and alignment of 10X-Schwarzschild optics for F2X experiments a, Michael Shumway b,e, Lou Marchetti d, Donald Phillion c, Regina Soufli c, Manish Chandhok a, Michael Goldstein a, and Jeff Bokor

"SIMPLE MEASUREMENT, ADVANCED RESULTS"

"SIMPLE MEASUREMENT, ADVANCED RESULTS" 1 Phasics offers the most innovative solutions for lens and objectives quality control in R&D and production. Relying on a unique wavefront technology, the quadriwave

Big League Cryogenics and Vacuum The LHC at CERN

Big League Cryogenics and Vacuum The LHC at CERN A typical astronomical instrument must maintain about one cubic meter at a pressure of

Nature Methods: doi: /nmeth Supplementary Figure 1. Schematic of 2P-ISIM AO optical setup.

Supplementary Figure 1 Schematic of 2P-ISIM AO optical setup. Excitation from a femtosecond laser is passed through intensity control and shuttering optics (1/2 λ wave plate, polarizing beam splitting

Breadboard adaptive optical system based on 109-channel PDM: technical passport

F L E X I B L E Flexible Optical B.V. Adaptive Optics Optical Microsystems Wavefront Sensors O P T I C A L Oleg Soloviev Chief Scientist Röntgenweg 1 2624 BD, Delft The Netherlands Tel: +31 15 285 15-47

Fabrication and testing of large free-form surfaces Jim H. Burge

Fabrication and testing of large free-form surfaces Jim H. Burge College of Optical Sciences + Steward Observatory University of Arizona Tucson, AZ 85721 Introduction A tutorial on Fabrication and testing

System Architecting: Defining Optical and Mechanical Tolerances from an Error Budget

System Architecting: Defining Optical and Mechanical Tolerances from an Error Budget Julia Zugby OPTI-521: Introductory Optomechanical Engineering, Fall 2016 Overview This tutorial provides a general overview

Wavefront Sensing In Other Disciplines. 15 February 2003 Jerry Nelson, UCSC Wavefront Congress

Wavefront Sensing In Other Disciplines 15 February 2003 Jerry Nelson, UCSC Wavefront Congress QuickTime and a Photo - JPEG decompressor are needed to see this picture. 15feb03 Nelson wavefront sensing

Lens Design I Seminar 1

Xiang Lu, Ralf Hambach Friedrich Schiller University Jena Institute of Applied Physics Albert-Einstein-Str 15 07745 Jena Lens Design I Seminar 1 Warm-Up (20min) Setup a single, symmetric, biconvex lens

Difrotec Product & Services. Ultra high accuracy interferometry & custom optical solutions

Difrotec Product & Services Ultra high accuracy interferometry & custom optical solutions Content 1. Overview 2. Interferometer D7 3. Benefits 4. Measurements 5. Specifications 6. Applications 7. Cases

Lens Design I Seminar 5

Y. Sekman, X. Lu, H. Gross Friedrich Schiller University Jena Institute of Applied Physics Albert-Einstein-Str 15 07745 Jena Lens Design I Seminar 5 Exercise 5-1: PSF scaling (Homework) To check the Airy

AST Lab exercise: aberrations

AST2210 - Lab exercise: aberrations 1 Introduction This lab exercise will take you through the most common types of aberrations. 2 Chromatic aberration Chromatic aberration causes lens to have dierent

Use of Computer Generated Holograms for Testing Aspheric Optics

Use of Computer Generated Holograms for Testing Aspheric Optics James H. Burge and James C. Wyant Optical Sciences Center, University of Arizona, Tucson, AZ 85721 http://www.optics.arizona.edu/jcwyant,

Be aware that there is no universal notation for the various quantities.

Fourier Optics v2.4 Ray tracing is limited in its ability to describe optics because it ignores the wave properties of light. Diffraction is needed to explain image spatial resolution and contrast and

Lens Design II. Lecture 3: Aspheres Herbert Gross. Winter term

Lens Design II Lecture 3: Aspheres 6-- Herbert Gross Winter term 6 www.iap.uni-jena.de Preliminar Schedule 9.. Aberrations and optimiation Repetition 6.. Structural modifications Zero operands, lens splitting,

Chapter 3 Mirrors. The most common and familiar optical device

Chapter 3 Mirrors The most common and familiar optical device Outline Plane mirrors Spherical mirrors Graphical image construction Two mirrors; The Cassegrain Telescope Plane mirrors Common household mirrors:

Inverted-COR: Inverted-Occultation Coronagraph for Solar Orbiter

Inverted-COR: Inverted-Occultation Coronagraph for Solar Orbiter OATo Technical Report Nr. 119 Date 19-05-2009 by: Silvano Fineschi Release Date Sheet: 1 of 1 REV/ VER LEVEL DOCUMENT CHANGE RECORD DESCRIPTION

EE119 Introduction to Optical Engineering Fall 2009 Final Exam. Name:

EE119 Introduction to Optical Engineering Fall 2009 Final Exam Name: SID: CLOSED BOOK. THREE 8 1/2 X 11 SHEETS OF NOTES, AND SCIENTIFIC POCKET CALCULATOR PERMITTED. TIME ALLOTTED: 180 MINUTES Fundamental

High contrast imaging lab

High contrast imaging lab Ay122a, November 2016, D. Mawet Introduction This lab is an introduction to high contrast imaging, and in particular coronagraphy and its interaction with adaptive optics sytems.

ADVANCED OPTICS LAB -ECEN Basic Skills Lab

ADVANCED OPTICS LAB -ECEN 5606 Basic Skills Lab Dr. Steve Cundiff and Edward McKenna, 1/15/04 Revised KW 1/15/06, 1/8/10 Revised CC and RZ 01/17/14 The goal of this lab is to provide you with practice

Vision Research at. Validation of a Novel Hartmann-Moiré Wavefront Sensor with Large Dynamic Range. Wavefront Science Congress, Feb.

Wavefront Science Congress, Feb. 2008 Validation of a Novel Hartmann-Moiré Wavefront Sensor with Large Dynamic Range Xin Wei 1, Tony Van Heugten 2, Nikole L. Himebaugh 1, Pete S. Kollbaum 1, Mei Zhang

Manufacturing, testing and alignment of Sentinel-2 MSI telescope mirrors

Manufacturing, testing and alignment of Sentinel-2 MSI telescope mirrors P. Gloesener, F. Wolfs, F. Lemagne, C. Flebus AMOS Angleur, Belgium pierre.gloesener@amos.be P. Gloesener, F. Wolfs, F. Lemagne,

The Design, Fabrication, and Application of Diamond Machined Null Lenses for Testing Generalized Aspheric Surfaces

The Design, Fabrication, and Application of Diamond Machined Null Lenses for Testing Generalized Aspheric Surfaces James T. McCann OFC - Diamond Turning Division 69T Island Street, Keene New Hampshire

Coherent Laser Measurement and Control Beam Diagnostics

Coherent Laser Measurement and Control M 2 Propagation Analyzer Measurement and display of CW laser divergence, M 2 (or k) and astigmatism sizes 0.2 mm to 25 mm Wavelengths from 220 nm to 15 µm Determination

ABSTRACT. Keywords: Computer-aided alignment, Misalignments, Zernike polynomials, Sensitivity matrix 1. INTRODUCTION

Computer-Aided Alignment for High Precision Lens LI Lian, FU XinGuo, MA TianMeng, WANG Bin The institute of optical and electronics, the Chinese Academy of Science, Chengdu 6129, China ABSTRACT Computer-Aided

October 7, Peter Cheimets Smithsonian Astrophysical Observatory 60 Garden Street, MS 5 Cambridge, MA Dear Peter:

October 7, 1997 Peter Cheimets Smithsonian Astrophysical Observatory 60 Garden Street, MS 5 Cambridge, MA 02138 Dear Peter: This is the report on all of the HIREX analysis done to date, with corrections

http://goldberg.lbl.gov 1 To EUV or not to EUV? That is the question. Do we need EUV interferometry and EUV optical testing? 17 Things you need to know about perfecting EUV optics. 2 The main things you

Simulation of Zernike Aberrations in optical systems. Michael Koch, July 5, 2018

Simulation of Zernike Aberrations in optical systems Michael Koch, astroelectronic@t-online.de July 5, 2018 This paper is about three related questions: 1. In a Newton telescope we have two mirrors. It's

Optical Engineering 421/521 Sample Questions for Midterm 1

Optical Engineering 421/521 Sample Questions for Midterm 1 Short answer 1.) Sketch a pechan prism. Name a possible application of this prism., write the mirror matrix for this prism (or any other common

Design and Manufacture of 8.4 m Primary Mirror Segments and Supports for the GMT

Design and Manufacture of 8.4 m Primary Mirror Segments and Supports for the GMT Introduction The primary mirror for the Giant Magellan telescope is made up an 8.4 meter symmetric central segment surrounded

X-ray generation by femtosecond laser pulses and its application to soft X-ray imaging microscope

X-ray generation by femtosecond laser pulses and its application to soft X-ray imaging microscope Kenichi Ikeda 1, Hideyuki Kotaki 1 ' 2 and Kazuhisa Nakajima 1 ' 2 ' 3 1 Graduate University for Advanced

Pantoscopic tilt induced higher order aberrations characterization using Shack Hartmann wave front sensor and comparison with Martin s Rule.

Research Article http://www.alliedacademies.org/ophthalmic-and-eye-research/ Pantoscopic tilt induced higher order aberrations characterization using Shack Hartmann wave front sensor and comparison with

Hartmann Wavefront Analyzer

Hartmann Wavefront Analyzer Installation & Setup Guide Ophir-Spiricon Inc. 60 West 1000 North Logan, UT 84321 For Sales, Service or Technical Support Phone (435)753-3729 Fax (435)753-5231 Email service@ophir-spiricon.com

Lens Design I. Lecture 3: Properties of optical systems II Herbert Gross. Summer term

Lens Design I Lecture 3: Properties of optical systems II 205-04-8 Herbert Gross Summer term 206 www.iap.uni-jena.de 2 Preliminary Schedule 04.04. Basics 2.04. Properties of optical systrems I 3 8.04.

CaSSIS. Colour and Stereo Surface Imaging System. L. Gambicorti & CaSSIS team

CaSSIS Colour and Stereo Surface Imaging System & CaSSIS team CaSSIS on Exomars TGO l l Introduction CaSSIS: stereo-colour camera Telescope and Optical configuration Best focus on ground CaSSIS integration

AgilEye Manual Version 2.0 February 28, 2007

AgilEye Manual Version 2.0 February 28, 2007 1717 Louisiana NE Suite 202 Albuquerque, NM 87110 (505) 268-4742 support@agiloptics.com 2 (505) 268-4742 v. 2.0 February 07, 2007 3 Introduction AgilEye Wavefront

SpotOptics. The software people for optics L E N T I N O LENTINO

Spotptics he software people for optics AUMAD WAVFR SSR Accurate Metrology of standard and aspherical lenses =0.3 to =20 mm F/1 to F/15 Accurate motor for z-movement Accurate XY and tilt stages for easy

DETERMINING CALIBRATION PARAMETERS FOR A HARTMANN- SHACK WAVEFRONT SENSOR

DETERMINING CALIBRATION PARAMETERS FOR A HARTMANN- SHACK WAVEFRONT SENSOR Felipe Tayer Amaral¹, Luciana P. Salles 2 and Davies William de Lima Monteiro 3,2 Graduate Program in Electrical Engineering -