Boian Andonov Hristov, Prof. (Ph.D) Bulgarian Academy of Sciences

Slides:



Advertisements
Similar presentations
Geometrical theory of aberration for off-axis reflecting telescope and its applications Seunghyuk Chang SSG13.
Advertisements

Consider Refraction at Spherical Surfaces:
1 Complex math basics material from Advanced Engineering Mathematics by E Kreyszig and from Liu Y; Tian Y; “Succinct formulas for decomposition of complex.
Chapter 2 Propagation of Laser Beams
Nonlinear Optics Lab. Hanyang Univ. Chapter 2. The Propagation of Rays and Beams 2.0 Introduction Propagation of Ray through optical element : Ray (transfer)
 Light can take the form of beams that comes as close
Lenses in the Paraxial Limit
Gaussian Beam Propagation Code
Chapter 32Light: Reflection and Refraction. Electromagnetic waves can have any wavelength; we have given different names to different parts of the wavelength.
Light: Geometric Optics
Reflective Optics Chapter 25. Reflective Optics  Wavefronts and Rays  Law of Reflection  Kinds of Reflection  Image Formation  Images and Flat Mirrors.
Aperture Pupil (stop) Exit Pupil Entrance Pupil.
Geometric Optics of thick lenses and Matrix methods
Optics 1----by Dr.H.Huang, Department of Applied Physics
Aberrations  Aberrations of Lenses  Analogue to Holographic Model  Aberrations in Holography  Implications in the aberration equations  Experimental.
International Conference on Industrial and Applied Mathematics Zurich, Switzerland, July 2007 Shekhar Guha United States Air Force Research Laboratory.
Fig Reflection of an object (y) from a plane mirror. Lateral magnification m = y ’ / y © 2003 J. F. Becker San Jose State University Physics 52 Heat.
1 Optics for Astrometry: a quick introduction William F. van Altena Yale University Basic Astrometric Methods Yale University July 18-22, 2005.
Copyright © 2009 Pearson Education, Inc. Chapter 32 Light: Reflection and Refraction.
Lenses We will only consider “thin” lenses where the thickness of the lens is small compared to the object and image distances. Eugene Hecht, Optics, Addison-Wesley,
Optical Center Eugene Hecht, Optics, Addison-Wesley, Reading, MA, 1998.
Fiber Optics Defining Characteristics: Numerical Aperture Spectral Transmission Diameter.
C F V Light In Side S > 0 Real Object Light Out Side S ’ > 0 Real Image C This Side, R > 0 S < 0 Virtual Object S ’ < 0 Virtual Image C This Side, R
CS223b, Jana Kosecka Rigid Body Motion and Image Formation.
Image Formation III Chapter 1 (Forsyth&Ponce) Cameras “Lenses”
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science Mirrors and Lenses.
One Mark Questions. Choose the Correct Answer 1.If p is true and q is false then which of the following is not true? (a) ~ p is true (b) p  q is true.
Pat Arnott, ATMS 749 Atmospheric Radiation Transfer CH4: Reflection and Refraction in a Homogenous Medium.
Sebastian Thrun CS223B Computer Vision, Winter Stanford CS223B Computer Vision, Winter 2005 Lecture 2 Lenses and Camera Calibration Sebastian Thrun,
3/4/ PHYS 1442 – Section 004 Lecture #18 Monday March 31, 2014 Dr. Andrew Brandt Chapter 23 Optics The Ray Model of Light Reflection; Image Formed.
1. Two long straight wires carry identical currents in opposite directions, as shown. At the point labeled A, is the direction of the magnetic field left,
Focusing of Light in Axially Symmetric Systems within the Wave Optics Approximation Johannes Kofler Institute for Applied Physics Johannes Kepler University.
Geometrical Optics Chapter 24 + Other Tidbits 1. On and on and on …  This is a short week.  Schedule follows  So far, no room available for problem.
Yi-Chin Fang, Institute of Electro-Optical Engineering, National Kaohsiung First Univ. of Science and Technology Improvements of Petzval Field Curvature.
Doc.: IEEE /0431r0 Submission April 2009 Alexander Maltsev, Intel CorporationSlide 1 Polarization Model for 60 GHz Date: Authors:
Thin Lenses A lens is an optical device consisting of two refracting surfaces The simplest lens has two spherical surfaces close enough together that we.
Prof. Charles A. DiMarzio Northeastern University Fall 2003 July 2003
Matrix methods, aberrations & optical systems
Image Formation III Chapter 1 (Forsyth&Ponce) Cameras “Lenses” Guido Gerig CS-GY 6643, Spring 2016 (slides modified from Marc Pollefeys, UNC Chapel Hill/
Today’s agenda: Plane Mirrors. You must be able to draw ray diagrams for plane mirrors, and be able to calculate image and object heights, distances, and.
Spherical Aberration. Rays emanating from an object point that are incident on a spherical mirror or lens at different distances from the optical axis,
July © Chuck DiMarzio, Northeastern University ECEG105/ECEU646 Optics for Engineers Course Notes Part 4: Apertures, Aberrations Prof.
Optics Geometric Optics1 CHAPTER 2 GEOMETRIC OPTICS.
Lab 2 Alignment.
Level 2 Certificate Further Mathematics 8360 Route Map
Geometric Optics Figure Mirrors with convex and concave spherical surfaces. Note that θr = θi for each ray.
Chapter 32Light: Reflection and Refraction
Applied Electricity and Magnetism
HW #4, Due Sep. 21 Ch. 2: P28, PH8, PH16 Ch. 3: P3, P5.
Chapter 22/23.
Geometric Optics Ray Model assume light travels in straight line
Phys102 Lecture 21/22 Light: Reflection and Refraction
Chapter 7: Matrices and Systems of Equations and Inequalities
Spherical Mirrors: concave and convex mirrors.
Find sec 5π/4.
Linear Algebra Lecture 3.
Text Reference: Chapter 32.1 through 32.2
Mirrors, Plane and Spherical Spherical Refracting Surfaces
CH4: Reflection and Refraction in a Homogenous Medium.
PHANTOM GRAPHS PART 2 Philip Lloyd Epsom Girls Grammar School
Light, Reflection, & Mirrors
UNIVERSITY OF ILLINOIS AT URBANA-CHAMPAIGN
Chaper 6 Image Quality of Optical System
Linear Algebra Lecture 20.
LIGHT: Geometric Optics
PROF. KAPARE A.K. SUBMITTED BY- DEPARTMENT OF PHYSICS
DR MOHAMAD HALIM ABD. WAHID School of Microelectronic Engineering
Antenna Theory Chapter.4.7.4~4.8.1 Antennas
Light, Reflection, & Mirrors
Presentation transcript:

Boian Andonov Hristov, Prof. (Ph.D) Bulgarian Academy of Sciences 4th International Conference on Photonics July 28029,2016 Berlin, Germany Exact analytical aberration theory of centered optical systems containing conic surfaces Boian Andonov Hristov, Prof. (Ph.D) Bulgarian Academy of Sciences

Exact Analytical Aberration Theory of Centered Optical Systems Containing Conic Surfaces To achieve: Precise analytical correction of individual aberrations; Exact calculation of the system constructive parameters, such as surface radiuses and conic constants, axial thicknesses, etc.; Correct pictures of the aberrations space distribution in the whole object space and the whole image space of the optical system.

Conic radiuses coefficient- 𝝉 𝒋 1 - angle of incidence (𝜺 𝒋 ); 2 - angle of refraction or reflection (𝜺 𝒋 ′ ); 3 – slope of the surface normal ( 𝝋 𝒋 ) ; 4 – angle between refracted ray and z-axes ( 𝒘 𝒋+𝟏 ) ; 5 – angle between incident ray and z-axes ( 𝒘 𝒋 ). 𝒓 𝒕𝒋 = 𝒓 𝒔𝒋 𝟑 𝒓 𝟎𝒋 𝟐 ; 𝒓 𝟎𝒋 = 𝝉 𝒋 𝒓 𝒔𝒋 ; 𝒓 𝒕 = 𝒓 𝒔𝒋 𝝉 𝒋 𝟐 = 𝒓 𝟎𝒋 𝝉 𝒋 𝟑 ; 𝝉 𝒋 = 1+ K j sin 2 φ j .

Exact transformations from the object to the image space in a single conic surface In the sagittal planes: 𝒛 𝒔𝒋 ′ = 𝒓 𝒔𝒋 𝒑 𝒋 𝒛 𝒔𝒋 + 𝒓 𝒔𝒋 𝟐 𝑸 𝒋 𝒎 𝒋 𝒛 𝒔𝒋 + 𝒓 𝒔𝒋 𝝁 𝒋 = 𝒓 𝒔𝒋 𝒂 𝒋 𝒛 𝒔𝒋 + 𝒃 𝒋 𝒄 𝒋 𝒛 𝒔𝒋 + 𝒅 𝒋 , 𝑸 𝒋 ≡𝟎, 𝐆 𝐣 = 𝐚 𝐣 𝟎 𝐜 𝐣 𝐝 𝐣 = 𝐫 𝐬𝐣 𝐩 𝐣 𝟎 𝐦 𝐣 𝐫 𝐬𝐣 𝛍 𝐣 . Here 𝒑 𝒋 , 𝝁 𝒋 , 𝒎 𝒋 are exact functions depending on the real values of the following parameters: 𝒏 𝒋 , 𝒏 𝒋+𝟏 , 𝜺 𝒋 , 𝝋 𝒋 , 𝒘 𝒋+𝟏 𝒂𝒏𝒅 𝒘 𝒋 . In the tangential planes: 𝒛 𝒕𝒋 ′ = 𝒓 𝒔𝒋 𝒑 𝒋 𝒕 𝒛 𝒔𝒋 + 𝒓 𝒔𝒋 𝟐 𝑸 𝒋 𝒕 𝝉 𝒋 𝟐 𝒎 𝒋 𝒛 𝒕𝒋 + 𝒓 𝒔𝒋 𝝁 𝒋 𝒕 = 𝒓 𝒔𝒋 𝒂 𝒋 𝒕 𝒛 𝒕𝒋 + 𝒃 𝒋 𝒕 𝒄 𝒋 𝒕 𝒛 𝒕𝒋 + 𝒅 𝒋 𝒕 , 𝐆 𝐣 𝐭 = 𝐚 𝐣 𝐭 𝐛 𝐣 𝐭 𝐜 𝐣 𝐭 𝐝 𝐣 𝐭 = 𝐫 𝐬𝐣 𝐩 𝐣 𝐭 𝐐 𝐣 𝐭 𝛕 𝐣 𝟐 𝐦 𝐣 𝐫 𝐬𝐣 𝛍 𝐣 𝐭 . Here 𝒑 𝒋 𝒕 , 𝝁 𝒋 𝒋 𝒕 , 𝑸 𝒋, 𝒕 𝒂𝒏𝒅 𝒎 𝒋 are exact functions depending on the real values of parameters: 𝒏 𝒋 , 𝒏 𝒋+𝟏 , 𝜺 𝒋 , 𝝋 𝒋 , 𝒘 𝒋 , 𝝉 𝒋 𝟐 , 𝒂𝒏𝒅 𝒘 𝒋+𝟏 . In the paraxial region: 𝒛 𝟎𝒋 ′ = 𝒓 𝒔𝒋 𝒑 𝒋 𝟎 𝒛 𝟎𝒋 + 𝒓 𝒔𝒋 𝟐 𝑸 𝒋 𝟎 𝝉 𝒋 𝟐 𝒎 𝒋 𝟎 𝒛 𝟎𝒋 + 𝒓 𝒋 𝝁 𝒋 = 𝐫 𝐬𝐣 𝐚 𝒋 𝟎 𝐳 𝟎𝐣 + 𝐛 𝒋 𝟎 𝐜 𝒋 𝟎 𝐳 𝟎𝐣 + 𝐝 𝒋 𝟎 , 𝑮 𝒋 𝟎 = 𝒂 𝒋 𝟎 𝒃 𝒋 𝟎 𝒄 𝒋 𝟎 𝒅 𝒋 𝟎 = 𝒓 𝒔𝒋 𝒑 𝒋 𝟎 𝑸 𝒋 𝟎 𝒎 𝒋 𝟎 𝒓 𝒔𝒋 𝝁 𝒋 𝟎 . Here 𝒑 𝒋 𝟎 , 𝝁 𝒋 𝒋 𝟎 , 𝑸 𝒋, 𝟎 𝒎 𝒋 𝟎 are exact functions depending on t he real values of parameters: 𝒏 𝒋 , 𝒏 𝒋+𝟏 , 𝜺 𝒋 , 𝝋 𝒋 , 𝒘 𝒋 , 𝝉 𝒋 , 𝒂𝒏𝒅 𝒘 𝒋+𝟏 . 𝑸 𝒋 𝟎 = 𝒒 𝒋𝟑 𝝉 𝒋 𝟑 + 𝒒 𝒋𝟐 𝝉 𝒋 𝟐 + 𝒒 𝒋𝟏 𝝉+ 𝒒 𝒋𝟎 𝝉 𝒋 + 𝐜𝐨𝐬 𝝋 𝒋 𝟐 . In the saggital planes the image distance is bilinear function of the object distance. It is related to a matrix of this type. It can be proved that coefficient Q is always identical 0. “Rsj” is the well-known abcd matrix formalism in the paraxial theory. I prove that in sagittal planes it is similar. Here p.mi.m are…….. Patameters shown in the previous slide. We use identical transforamationa for tangential planes and paraxial regions.

Exact transformations from the object to the image space in an optical system of “k” centered conic surfaces 𝑔 𝑘 = 𝐺 𝑘 𝐺 𝑘−1 … 𝐺 𝑗 … 𝐺 2 𝐺 1 = 𝑎 𝑘 0 𝑐 𝑘 𝑑 𝑘 – sagittal matrix; 𝒂 𝒌 , 𝒄 𝒌 , 𝒅 𝒌 - sagittal matrix coefficients of the whole system; 𝑔 𝑘 𝑡 = 𝐺 𝑘 𝑡 𝐺 𝑘−1 𝑡 ,…, 𝐺 𝑗 𝑡 … 𝐺 2 𝑡 𝐺 1 𝑡 = 𝑎 𝑘 𝑡 𝑏 𝑘 𝑡 𝑐 𝑘 𝑡 𝑑 𝑘 𝑡 - tangential matrix; 𝒂 𝒕 𝒕 , 𝒃 𝒌 𝒕 , 𝒄 𝒌 𝒕 , 𝒅 𝒌 𝒕 tangential matrix coefficients of the whole system; 𝑔 𝑘 0 = 𝐺 𝑘 0 𝐺 𝑘−1 0 ,…, 𝐺 𝑗 0 ,…, 𝐺 2 0 𝐺 1 0 = 𝑎 𝑘 0 𝑏 𝑘 0 𝑐 𝑘 0 𝑑 𝑘 0 - paraxial matrix; 𝒂 𝒌 𝟎 , 𝒃 𝒌 𝟎 , 𝒄 𝒌 𝟎 , 𝒅 𝒌 𝟎 paraxial matrix coefficients of the whole system;

Relative parameters ( 𝒙 𝒋 ) and relative matrix coefficients: 𝒙 𝒋 = 𝒓 𝒔𝒋 𝒓 𝒔(𝒋+𝟏) ; 𝑨 𝒌 , 𝑩 𝒌 , 𝑪 𝒌 , 𝑫 𝒌 : - sagittal relative matrix coefficients; 𝑨 𝒌 𝒕 , 𝑩 𝒌 𝒕 , 𝑪 𝒌 𝒕 , 𝑫 𝒌 𝒕 : - tangential relative matrix coefficients; 𝑨 𝒌 𝟎 , 𝑩 𝒌 𝟎 , 𝑪 𝒌 𝟎 , 𝑫 𝒌 𝟎 : - paraxial relative matrix coefficients; 𝒂 𝒌 = 𝒓 𝒔𝒌 𝑨 𝒌 𝒋=𝟐 𝒌 𝒓 𝒔𝒋 ; 𝒃 𝒌 = 𝒓 𝒔𝟏 𝒓 𝒔𝒌 𝑩 𝒌 𝒋=𝟐 𝒌 𝒓 𝒔𝒋 ; 𝒄 𝒌 = 𝒓 𝒔𝒌 𝑪 𝒌 𝒋=𝟐 𝒌 𝒓 𝒔𝒋 ; 𝒅 𝒌 = 𝒓 𝒔𝟏 𝑫 𝒌 𝒋=𝟐 𝒌 𝒓 𝒔𝒋 .

Exact aberration functions and space distribution Field aberrations: astigmatism, sagittal curvature, tangential curvature, field curvature, distortion, sagittal coma, tangential coma). On-axes aberrations: paraxial chromatism, spherical aberration, OPD or wave aberration and Abbe’s sine condition) ∆𝒛 𝒌 ′ 𝒓 𝒔𝒌 = 𝑼 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑼 𝟎 𝑽 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑽 𝟎 - bilinear function to 𝑧 0 for: the distortion, on-axes spherical aberration, OPD and Abbe’s sine condition; Here 𝑈 1 , 𝑈 0 are linear functions to every 𝑥 𝑗 and cubic functions to every 𝜏 𝑗 ; ∆𝒛 𝒌 ′ 𝒓 𝒔𝒌 = 𝑼 𝟐 𝒛 𝟎 𝟐 𝒓 𝒔𝟏 𝟐 + 𝑼 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑼 𝟎 𝑽 𝟐 𝒛 𝟎 𝟐 𝒓 𝒔𝟏 𝟐 + 𝑽 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑽 𝟎 - quadratic-fractional function to 𝑧 0 for: the image astigmatism, sagittal curvature, tangential curvature and paraxial chromatism; Here 𝑈 2 , 𝑈 1 𝑎𝑛𝑑 𝑈 0 are quadratic functions to every 𝑥 𝑗 and cubic functions to every 𝜏 𝑗 ; ∆𝒛 𝒌 ′ 𝒓 𝒔𝒌 = 𝑼 𝟑 𝒛 𝟎 𝟑 𝒓 𝒔𝟏 𝟑 + 𝑼 𝟐 𝒛 𝟎 𝟐 𝒓 𝒔𝟏 𝟐 + 𝑼 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑼 𝟎 𝑽 𝟑 𝒛 𝟎 𝟑 𝒓 𝒔𝟏 𝟑 + 𝑽 𝟐 𝒛 𝟎 𝟐 𝒓 𝒔𝟏 𝟐 + 𝑽 𝟏 𝒛 𝟎 𝒓 𝒔𝟏 + 𝑽 𝟎 - cubic fractional function for: the field curvature, tangential coma and sagittal coma; Here 𝑈 3 , 𝑈 2 , 𝑈 1 , 𝑈 0 are cubic functions to every 𝑥 𝑗 and 𝜏 𝑗 ; Space distribution: zero points and zero surfaces; vertical and horizontal asymptotes

General aberration theorems for a centered optical system containing conic surfaces Discriminants of aberrations: 𝑫 𝒂𝒔𝒕 = 𝑼 𝟏 𝟐 −𝟒 𝑼 𝟐 𝑼 𝟎 ; Theorem for the paraxial achromatic points: In every centered optical system containing conic surfaces for every two wavelengths on the optical axis: a) there are two paraxial achromatic points if the paraxial chromatic discriminant is greater than zero; b) there is one achromatic point if the paraxial chromatic discriminant is zero; c) there is no achromatic point if the paraxial chromatic discriminant is less than zero; d) there is an endless set of achromatic points if all the three paraxial chromatic coefficients, 𝑼 𝟐 , 𝑼 𝟏 , 𝑼 𝟎 are zero. (Ref: HRISTOV, B. Exact Analytical Theory of Aberrations of Centered Optical Systems. OPTICAL REVIEW Vol. 20, No. 5 (2013) 395–419).  Theorems for the field aberrations: distortion, astigmatism, sagittal curvature, tangential curvature, field curvature, sagittal coma and tangential coma. General theorem: When the object space and image space are homogeneous and the object space is aberration-free, no more than one surface in general can be perfectly imaged by a centered optical system containing conic surfaces. (Ref: HRISTOV, B. Development Of Optical Design Algorithms On The Base Of The Exact (All Orders) Geometrical Aberration Theory, Proc. SPIE 8167 (2011) 12.)

Exact analytical correction of individual aberrations and simultaneous correction By solving one linear equation to the arbitrary chosen relative parameter ( 𝑥 𝑗 ), or one cubic equation to the arbitrary chosen conic radius coefficient ( 𝜏 𝑗 ) on-axes spherical aberration, distortion, OPD, or satisfaction of Abbe’s sine condition become corrected each one separately. By solving one quadratic equation to the arbitrary chosen relative parameter ( 𝑥 𝑗 ), or one cubic equation to the arbitrary chosen conic radius coefficient ( 𝜏 𝑗 ) astigmatism, or sagittal curvature, or tangential curvature, or paraxial chromatism become corrected each one separately. By solving one cubic equation to the arbitrary chosen relative parameter ( 𝑥 𝑗 ), or one cubic equation to the arbitrary chosen conic radius coefficient ( 𝜏 𝑗 ) field curvature, or tangential coma, or sagittal coma become corrected each one separately For simultaneous correction of aberrations we use Sylvester’s matrices by excluding unknown parameters to find exactly all existing solutions.

EXAMPLE

THANK YOU For contacts: Email address: bhristov@abv.bg