Theoretical Effect of Coma and Spherical Aberrations Translation
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Quaternion Zernike Spherical Polynomials
MATHEMATICS OF COMPUTATION Volume 84, Number 293, May 2015, Pages 1317–1337 S 0025-5718(2014)02888-3 Article electronically published on August 29, 2014 QUATERNION ZERNIKE SPHERICAL POLYNOMIALS J. MORAIS AND I. CAC¸ AO˜ Abstract. Over the past few years considerable attention has been given to the role played by the Zernike polynomials (ZPs) in many different fields of geometrical optics, optical engineering, and astronomy. The ZPs and their applications to corneal surface modeling played a key role in this develop- ment. These polynomials are a complete set of orthogonal functions over the unit circle and are commonly used to describe balanced aberrations. In the present paper we introduce the Zernike spherical polynomials within quater- nionic analysis ((R)QZSPs), which refine and extend the Zernike moments (defined through their polynomial counterparts). In particular, the underlying functions are of three real variables and take on either values in the reduced and full quaternions (identified, respectively, with R3 and R4). (R)QZSPs are orthonormal in the unit ball. The representation of these functions in terms of spherical monogenics over the unit sphere are explicitly given, from which several recurrence formulae for fast computer implementations can be derived. A summary of their fundamental properties and a further second or- der homogeneous differential equation are also discussed. As an application, we provide the reader with plot simulations that demonstrate the effectiveness of our approach. (R)QZSPs are new in literature and have some consequences that are now under investigation. 1. Introduction 1.1. The Zernike spherical polynomials. The complex Zernike polynomials (ZPs) have long been successfully used in many different fields of optics. -
Chapter 3 (Aberrations)
Chapter 3 Aberrations 3.1 Introduction In Chap. 2 we discussed the image-forming characteristics of optical systems, but we limited our consideration to an infinitesimal thread- like region about the optical axis called the paraxial region. In this chapter we will consider, in general terms, the behavior of lenses with finite apertures and fields of view. It has been pointed out that well- corrected optical systems behave nearly according to the rules of paraxial imagery given in Chap. 2. This is another way of stating that a lens without aberrations forms an image of the size and in the loca- tion given by the equations for the paraxial or first-order region. We shall measure the aberrations by the amount by which rays miss the paraxial image point. It can be seen that aberrations may be determined by calculating the location of the paraxial image of an object point and then tracing a large number of rays (by the exact trigonometrical ray-tracing equa- tions of Chap. 10) to determine the amounts by which the rays depart from the paraxial image point. Stated this baldly, the mathematical determination of the aberrations of a lens which covered any reason- able field at a real aperture would seem a formidable task, involving an almost infinite amount of labor. However, by classifying the various types of image faults and by understanding the behavior of each type, the work of determining the aberrations of a lens system can be sim- plified greatly, since only a few rays need be traced to evaluate each aberration; thus the problem assumes more manageable proportions. -
Higher-Order Wavefront Aberration and Letter-Contrast Sensitivity In
Eye (2008) 22, 1488–1492 & 2008 Macmillan Publishers Limited All rights reserved 0950-222X/08 $32.00 www.nature.com/eye 1 1 2 2 CLINICAL STUDY Higher-order C Okamoto , F Okamoto , T Samejima , K Miyata and T Oshika1 wavefront aberration and letter-contrast sensitivity in keratoconus Abstract Keywords: keratoconus; wavefront aberration; higher-order aberration; contrast sensitivity; Aims To evaluate the relation between letter-contrast sensitivity higher-order aberration of the eye and contrast sensitivity function in eyes with keratoconus. Methods In 22 eyes of 14 patients with Introduction keratoconus (age 30.578.4 years, means7SD) and 26 eyes of 13 normal controls (age Keratoconus is a chronic, non-inflammatory 29.276.7 years), ocular higher-order wavefront disease of the cornea associated with aberration for a 6-mm pupil was measured progressive thinning and anterior protrusion of with the Hartmann-Schack aberrometer the central cornea.1,2 Irregular astigmatism is (KR-9000 PW, Topcon). The root mean square often the first and most apparent clinical finding (RMS) of third- and fourth-order Zernike in keratoconus, and this is evidenced by a coefficients was used to represent higher-order distortion of the corneal image as noted with aberrations. The letter-contrast sensitivity was the placido disc, retinoscope, keratometer, examined using the CSV-1000LV contrast chart keratoscope, and computerized (Vector Vision). videokeratograph. Previous studies using Results In the keratoconus group, the videokeratography have quantitatively 1 Department of letter-contrast sensitivity showed significant demonstrated that corneal irregular Ophthalmology, Institute of correlation with third-order (Spearman’s astigmatism is significantly greater in eyes with Clinical Medicine, University correlation coefficient ¼À0.736, 0.001) 3–6 of Tsukuba, Ibaraki, Japan r Po keratoconus than in normal eyes. -
Correction of the Eye's Wave Aberration
Adaptive Optics for Vision Science and Astronomy ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** A. Quirrenbach Correction of the Eye’s Wave Aberration Yasuki Yamauchi∗, David R. Williams∗,, Jason Porter∗,, and Antonio Guirao∗,† ∗ Center for Visual Science, University of Rochester, Rochester, New York, 14627, USA The Institute of Optics, University of Rochester, Rochester, New York, 14627, USA † Laboratorio de Optica, Universidad de Murcia, Campus de Espinardo (Edificio C), 30071 Murcia, SPAIN 1. Introduction We have seen in the previous two chapters that the human eye is not a perfect optical system and contains a host of different aberrations. If the eye’s opti- cal quality is poor, i.e. if the images formed on the retina are blurred or have low contrast, vision will be deficient even if the rest of the visual system were perfect. Several methods to improve the optics of the human eye have been proposed and developed, the earliest written reports of which originated at least 700 years ago. Spectacles that corrected defocus were invented as early as the 13th century (Willoughby Cashell, 1971; Rubin, 1986) while spectacles that cor- rected defocus and astigmatism were conceived in the 19th century (Helmholtz, 1924). Since then, there has been relatively little work on exploring techniques to correct additional aberrations in the eye. In 1961, Smirnov suggested that it might be possible to manufacture customized contact lenses that would com- pensate for the higher order aberrations found in individual eyes. Recently, technological advances in measuring and compensating for the aberrations of the human eye have made it possible to provide the eye with unprecedented optical quality (Liang et al., 1997). -
Spherical Aberration ¥ Field Angle Effects (Off-Axis Aberrations) Ð Field Curvature Ð Coma Ð Astigmatism Ð Distortion
Astronomy 80 B: Light Lecture 9: curved mirrors, lenses, aberrations 29 April 2003 Jerry Nelson Sensitive Countries LLNL field trip 2003 April 29 80B-Light 2 Topics for Today • Optical illusion • Reflections from curved mirrors – Convex mirrors – anamorphic systems – Concave mirrors • Refraction from curved surfaces – Entering and exiting curved surfaces – Converging lenses – Diverging lenses • Aberrations 2003 April 29 80B-Light 3 2003 April 29 80B-Light 4 2003 April 29 80B-Light 8 2003 April 29 80B-Light 9 Images from convex mirror 2003 April 29 80B-Light 10 2003 April 29 80B-Light 11 Reflection from sphere • Escher drawing of images from convex sphere 2003 April 29 80B-Light 12 • Anamorphic mirror and image 2003 April 29 80B-Light 13 • Anamorphic mirror (conical) 2003 April 29 80B-Light 14 • The artist Hans Holbein made anamorphic paintings 2003 April 29 80B-Light 15 Ray rules for concave mirrors 2003 April 29 80B-Light 16 Image from concave mirror 2003 April 29 80B-Light 17 Reflections get complex 2003 April 29 80B-Light 18 Mirror eyes in a plankton 2003 April 29 80B-Light 19 Constructing images with rays and mirrors • Paraxial rays are used – These rays may only yield approximate results – The focal point for a spherical mirror is half way to the center of the sphere. – Rule 1: All rays incident parallel to the axis are reflected so that they appear to be coming from the focal point F. – Rule 2: All rays that (when extended) pass through C (the center of the sphere) are reflected back on themselves. -
Measuring Higher Order Optical Aberrations of the Human Eye: Techniques and Applications
Brazilian Journal of Medical and Biological Research (2002) 35: 1395-1406 Optical aberrations of the human eye 1395 ISSN 0100-879X Measuring higher order optical aberrations of the human eye: techniques and applications L. Alberto V. Carvalho1, 1Grupo de Óptica, Instituto de Física de São Carlos, Universidade de São Paulo, J.C. Castro1 and São Carlos, SP, Brasil L. Antonio V. Carvalho2 2Departamento de Matemática, Universidade Estadual de Maringá, Maringá, PR, Brasil Abstract Correspondence In the present paper we discuss the development of wave-front, an Key words L. Alberto V. Carvalho instrument for determining the lower and higher optical aberrations of · Optical aberrations Grupo de Óptica, IFSC, USP the human eye. We also discuss the advantages that such instrumenta- · Corneal topography 13560-900 São Carlos, SP tion and techniques might bring to the ophthalmology professional of · Zernike polynomials Brasil the 21st century. By shining a small light spot on the retina of subjects · Refractive surgery E-mail: [email protected] and observing the light that is reflected back from within the eye, we are able to quantitatively determine the amount of lower order aberra- Research partially supported by FAPESP (Nos. 01/03132-8 and tions (astigmatism, myopia, hyperopia) and higher order aberrations 00/06810-4). L. Antonio V. Carvalho (coma, spherical aberration, etc.). We have measured artificial eyes is partially supported by CNPq with calibrated ametropia ranging from +5 to -5 D, with and without (No. 304041/85-8). 2 D astigmatism with axis at 45º and 90º. We used a device known as the Hartmann-Shack (HS) sensor, originally developed for measuring the optical aberrations of optical instruments and general refracting surfaces in astronomical telescopes. -
Wavefront Sensing for Adaptive Optics MARCOS VAN DAM & RICHARD CLARE W.M
Wavefront sensing for adaptive optics MARCOS VAN DAM & RICHARD CLARE W.M. Keck Observatory Acknowledgments Wilson Mizner : "If you steal from one author it's plagiarism; if you steal from many it's research." Thanks to: Richard Lane, Lisa Poyneer, Gary Chanan, Jerry Nelson Outline Wavefront sensing Shack-Hartmann Pyramid Curvature Phase retrieval Gerchberg-Saxton algorithm Phase diversity Properties of a wave-front sensor Localization: the measurements should relate to a region of the aperture. Linearization: want a linear relationship between the wave-front and the intensity measurements. Broadband: the sensor should operate over a wide range of wavelengths. => Geometric Optics regime BUT: Very suboptimal (see talk by GUYON on Friday) Effect of the wave-front slope A slope in the wave-front causes an incoming photon to be displaced by x = zWx There is a linear relationship between the mean slope of the wavefront and the displacement of an image Wavelength-independent W(x) z x Shack-Hartmann The aperture is subdivided using a lenslet array. Spots are formed underneath each lenslet. The displacement of the spot is proportional to the wave-front slope. Shack-Hartmann spots 45-degree astigmatism Typical vision science WFS Lenslets CCD Many pixels per subaperture Typical Astronomy WFS Former Keck AO WFS sensor 21 pixels 2 mm 3x3 pixels/subap 200 μ lenslets CCD relay lens 3.15 reduction Centroiding The performance of the Shack-Hartmann sensor depends on how well the displacement of the spot is estimated. The displacement is usually estimated using the centroid (center-of-mass) estimator. x I(x, y) y I(x, y) s = sy = x I(x, y) I(x, y) This is the optimal estimator for the case where the spot is Gaussian distributed and the noise is Poisson. -
Total, Corneal, and Internal Ocular Optical Aberrations in Patients with Keratoconus
Total, Corneal, and Internal Ocular Optical Aberrations in Patients With Keratoconus Zuzana Schlegel, MD; Yara Lteif, MD; Harkaran S. Bains; Damien Gatinel, MD, PhD he front corneal surface is a major refracting com- ABSTRACT ponent of the eye and is considerably distorted in 1 PURPOSE: To measure and compare total, corneal, and T patients with keratoconus. Asymmetric corneal internal ocular aberrations using combined wavefront protrusion is the primary cause of irregular astigmatism in analysis and corneal topography in eyes with keratoco- keratoconus.2 This deformity affects both the anterior and nus and eyes with normal corneas. posterior corneal surfaces.3-5 Recent studies have investigated the contribution of the posterior surface to the overall corneal METHODS: This prospective study comprised eyes of optical performance by analyzing data obtained with slit- patients with keratoconus and myopic patients seeking 6 7 refractive surgery. Patients diagnosed with keratoconus scanning or Scheimpfl ug topography. Signifi cantly larger and with a classifi cation of “normal” or “keratoconus” amounts of posterior corneal aberrations and higher compen- on the NIDEK Corneal Navigator corneal disease screen- sation effects were observed in keratoconic eyes compared ing software were selected for inclusion in this study. to normal eyes.6,7 Both the posterior corneal aberrations and The normal group comprised eyes with a “normal” clas- crystalline lens aberrations contribute to the internal aberra- sifi cation with 99% similarity. In the normal group, only one eye per patient was randomly selected based on tion component. a randomization schedule. Corneal, internal, and total Recent studies have found that in pre-presbyopic patients, wavefront measurements were provided by the NIDEK the magnitude of higher order aberrations for the cornea or OPD-Scan II. -
Lab #5 Shack-Hartmann Wavefront Sensor
EELE 482 Lab #5 Lab #5 Shack-Hartmann Wavefront Sensor (1 week) Contents: 1. Summary of Measurements 2 2. New Equipment and Background Information 2 3. Beam Characterization of the HeNe Laser 4 4. Maximum wavefront tilt 4 5. Spatially Filtered Beam 4 6. References 4 Shack-Hartmann Page 1 last edited 10/5/18 EELE 482 Lab #5 1. Summary of Measurements HeNe Laser Beam Characterization 1. Use the WFS to measure both beam radius w and wavefront radius R at several locations along the beam from the HeNe laser. Is the beam well described by the simple Gaussian beam model we have assumed? How do the WFS measurements compare to the chopper measurements made previously? Characterization of WFS maximum sensible wavefront gradient 2. Tilt the wavefront sensor with respect to the HeNe beam while monitoring the measured wavefront tilt. Determine the angle beyond which which the data is no longer valid. Investigation of wavefront quality after spatial filtering and collimation with various lenses 3. Use a single-mode fiber as a spatial filter. Characterize the beam emerging from the fiber for wavefront quality, and then measure the wavefront after collimation using a PCX lens and a doublet. Quantify the aberrations of these lenses. 2. New Equipment and Background Information 1. Shack-Hartmann Wavefront Sensor (WFS) The WFS uses an array of microlenses in front of a CMOS camera, with the camera sensor located at the back focal plane of the microlenses. Locally, the input beam will look like a portion of a plane wave across the small aperture of the microlens, and the beam will come to a focus on the camera with the center position of the focused spot determined by the local tilt of the wavefront. -
Visual Effect of the Combined Correction of Spherical and Longitudinal Chromatic Aberrations
Visual effect of the combined correction of spherical and longitudinal chromatic aberrations Pablo Artal 1,* , Silvestre Manzanera 1, Patricia Piers 2 and Henk Weeber 2 1Laboratorio de Optica, Centro de Investigación en Optica y Nanofísica (CiOyN), Universidad de Murcia, Campus de Espinardo, 30071 Murcia, Spain 2AMO Groningen, Groningen, The Netherlands *[email protected] Abstract: An instrument permitting visual testing in white light following the correction of spherical aberration (SA) and longitudinal chromatic aberration (LCA) was used to explore the visual effect of the combined correction of SA and LCA in future new intraocular lenses (IOLs). The LCA of the eye was corrected using a diffractive element and SA was controlled by an adaptive optics instrument. A visual channel in the system allows for the measurement of visual acuity (VA) and contrast sensitivity (CS) at 6 c/deg in three subjects, for the four different conditions resulting from the combination of the presence or absence of LCA and SA. In the cases where SA is present, the average SA value found in pseudophakic patients is induced. Improvements in VA were found when SA alone or combined with LCA were corrected. For CS, only the combined correction of SA and LCA provided a significant improvement over the uncorrected case. The visual improvement provided by the correction of SA was higher than that from correcting LCA, while the combined correction of LCA and SA provided the best visual performance. This suggests that an aspheric achromatic IOL may provide some visual benefit when compared to standard IOLs. ©2010 Optical Society of America OCIS codes: (330.0330) Vision, color, and visual optics; (330.4460) Ophthalmic optics and devices; (330.5510) Psycophysics; (220.1080) Active or adaptive optics. -
Wavefront Parameters Recovering by Using Point Spread Function
Wavefront Parameters Recovering by Using Point Spread Function Olga Kalinkina[0000-0002-2522-8496], Tatyana Ivanova[0000-0001-8564-243X] and Julia Kushtyseva[0000-0003-1101-6641] ITMO University, 197101 Kronverksky pr. 49, bldg. A, Saint-Petersburg, Russia [email protected], [email protected], [email protected] Abstract. At various stages of the life cycle of optical systems, one of the most important tasks is quality of optical system elements assembly and alignment control. The different wavefront reconstruction algorithms have already proven themselves to be excellent assistants in this. Every year increasing technical ca- pacities opens access to the new algorithms and the possibilities of their appli- cation. The paper considers an iterative algorithm for recovering the wavefront parameters. The parameters of the wavefront are the Zernike polynomials coef- ficients. The method involves using a previously known point spread function to recover Zernike polynomials coefficients. This work is devoted to the re- search of the defocusing influence on the convergence of the algorithm. The method is designed to control the manufacturing quality of optical systems by point image. A substantial part of the optical systems can use this method with- out additional equipment. It can help automate the controlled optical system ad- justment process. Keywords: Point Spread Function, Wavefront, Zernike Polynomials, Optimiza- tion, Aberrations. 1 Introduction At the stage of manufacturing optical systems, one of the most important tasks is quality of optical system elements assembly and alignment control. There are various methods for solving this problem, for example, interference methods. However, in some cases, one of which is the alignment of the telescope during its operation, other control methods are required [1, 2], for example control by point image (point spread function) or the image of another known object. -
Topic 3: Operation of Simple Lens
V N I E R U S E I T H Y Modern Optics T O H F G E R D I N B U Topic 3: Operation of Simple Lens Aim: Covers imaging of simple lens using Fresnel Diffraction, resolu- tion limits and basics of aberrations theory. Contents: 1. Phase and Pupil Functions of a lens 2. Image of Axial Point 3. Example of Round Lens 4. Diffraction limit of lens 5. Defocus 6. The Strehl Limit 7. Other Aberrations PTIC D O S G IE R L O P U P P A D E S C P I A S Properties of a Lens -1- Autumn Term R Y TM H ENT of P V N I E R U S E I T H Y Modern Optics T O H F G E R D I N B U Ray Model Simple Ray Optics gives f Image Object u v Imaging properties of 1 1 1 + = u v f The focal length is given by 1 1 1 = (n − 1) + f R1 R2 For Infinite object Phase Shift Ray Optics gives Delta Fn f Lens introduces a path length difference, or PHASE SHIFT. PTIC D O S G IE R L O P U P P A D E S C P I A S Properties of a Lens -2- Autumn Term R Y TM H ENT of P V N I E R U S E I T H Y Modern Optics T O H F G E R D I N B U Phase Function of a Lens δ1 δ2 h R2 R1 n P0 P ∆ 1 With NO lens, Phase Shift between , P0 ! P1 is 2p F = kD where k = l with lens in place, at distance h from optical, F = k0d1 + d2 +n(D − d1 − d2)1 Air Glass @ A which can be arranged to|giv{ze } | {z } F = knD − k(n − 1)(d1 + d2) where d1 and d2 depend on h, the ray height.