(12) United States Patent (10) Patent No.: US 6,266,191 B1 Abe (45) Date of Patent: *Jul

Total Page:16

File Type:pdf, Size:1020Kb

(12) United States Patent (10) Patent No.: US 6,266,191 B1 Abe (45) Date of Patent: *Jul USOO6266 191B1 (12) United States Patent (10) Patent No.: US 6,266,191 B1 Abe (45) Date of Patent: *Jul. 24, 2001 (54) DIFFRACTIVE-REFRACTIVE ACHROMATIC 5,568,325 10/1996 Hirando et al. ...................... 359/785 LENS 5,790,321 * 8/1998 Goto ............ ... 359/571 5,818,632 * 10/1998 Stephenson . ... 359/566 (75) Inventor: Tetsuya Abe, Hokkaido (JP) 5,949.577 * 9/1999 Ogata ................................... 359/570 (73) Assignee: Asahi Kogaku Kogyo Kabushiki * cited by examiner Kaisha, Tokyo (JP) Primary Examiner Audrey Chang (*) Notice: This patent issued on a continued pros ASSistant Examiner Jennifer Winstedt ecution application filed under 37 CFR (74) Attorney, Agent, or Firm-Greenblum & Bernstein 1.53(d), and is subject to the twenty year P.L.C. patent term provisions of 35 U.S.C. (57) ABSTRACT 154(a)(2). A diffractive-refractive achromatic lens includes a refractive Subject to any disclaimer, the term of this lens System exhibiting longitudinal chromatic aberration patent is extended or adjusted under 35 that is Substantially proportional to wavelength Such that the U.S.C. 154(b) by 0 days. back focus of the refractive lens System decreaseS as the wavelength becomes shorter and a diffractive grating for (21) Appl. No.: 09/244,077 correcting the longitudinal chromatic aberration of the refractive lens System. The refractive lens having Such a (22) Filed: Feb. 4, 1999 chromatic aberration includes a positive lens having rela (30) Foreign Application Priority Data tively Small dispersion and a negative lens having relatively large dispersion. Further, the following condition (1) should Feb. 5, 1998 (JP) ................................................. 1O-O24789 be satisfied: (51) Int. Cl." .............................. G02B 27/44; G02B 5/18 (52) U.S. Cl. ........................... 359/566; 359/565; 359/569 0.005<ff-0.2 (58) Field of Search ..................................... 359/795, 566, where 359/569, 570, 571, 565, 16 f is a focal length of the entire lens System, and (56) References Cited f, is a focal length of the positive diffractive grating. U.S. PATENT DOCUMENTS 4,190.324 2/1980 Arai ..................................... 359/789 17 Claims, 15 Drawing Sheets U.S. Patent Jul. 24, 2001 Sheet 1 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 2 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 3 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 4 of 15 US 6,266,191 B1 þ'1:NA U.S. Patent Jul. 24, 2001 Sheet 5 of 15 US 6,266,191 B1 2'!:NA 0"|0- % U.S. Patent Jul. 24, 2001 Sheet 6 of 15 US 6,266,191 B1 0"|0- % ENIT–p ENIT-6··· ENIT-O---- U.S. Patent Jul. 24, 2001 Sheet 7 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 8 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 9 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 10 Of 15 US 6,266,191 B1 0"|0- % ENIT-?)– ENIT-6······· ENIT-O---- U.S. Patent Jul. 24, 2001 Sheet 11 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 12 Of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 13 of 15 US 6,266,191 B1 NOILHO1S?0 Z'OZIO U.S. Patent Jul. 24, 2001 Sheet 14 of 15 US 6,266,191 B1 U.S. Patent Jul. 24, 2001 Sheet 15 of 15 US 6,266,191 B1 G08013008'9|+808'0|+w06914 US 6,266,191 B1 1 2 DIFFRACTIVE-REFRACTIVE ACHROMATIC persion and a negative lens having relatively large disper LENS sion. Further, the following condition (1) should be satisfied: BACKGROUND OF THE INVENTION 0.005<ff-0.2 (1) The present invention relates to an achromatic lens to be where used as a collimator lens, or an objective lens for a telescope. f is a focal length of the entire lens System, and Particularly, the present invention relates to a diffractive refractive achromatic lens that includes a refractive lens f, a is focal length of the positive diffractive grating. System provided with a diffractive grating. Preferably, the diffractive grating may be designed So that Conventionally, an achromatic lens has been well known the following condition (2) is satisfied: and used as a collimator lens or an objective lens. An example of the achromatic lens employs two thin lenses: one being a lens having large positive power that is made from crown glass having relatively low dispersion; and the other 15 where being a lens having Small negative power that is made from P and P are diffractive coefficients of second and fourth flint glass having relatively high dispersion. The resultant orders when the diffractive grating is expressed by the power is therefore positive, while the dispersion is neutral following optical path difference function d(h) ized. Since optical glass has dispersion Such that refractive indeX thereof increases with decreasing wavelength of light, a positive refractive lens has longitudinal chromatic aberra where tion where a back focus of the lens decreases as wavelength h is a height from the optical axis, and becomes shorter. The achromatic doublet corrects the chro 2 is a design wavelength of the diffractive grating. matic aberration of the positive lens by using a negative lens 25 Embodiments described in this specification includes that has opposite chromatic aberration. three groups. In a first group of the embodiments, the The conventional achromatic doublet is designed for refractive lens System includes a non-achromatic doublet. In correcting the longitudinal chromatic aberration with respect the Second and third groups of embodiments, the refractive to two different wavelengths, e.g., F-line (486 nm) and lens System consists of a combination of a refractive ach C-line (656 nm). That is, the light beams of F-line and C-line romatic lens and an additional lens. In each case, the are focused on Substantially the same focal point. diffractive grating could be formed on one Surface of the However, light beams having wavelengths except the C refractive lenses or provided as a separate diffractive ele and F-lines are not focused on the same focal point. ment. Particularly, the back focus of the doublet becomes remark In the first group of the embodiments, the doublet should ably larger in a range shorter than F-line. This remaining 35 have longitudinal chromatic aberration Such that the back focus of the refractive lens System decreases as the wave chromatic aberration is called as Secondary Spectrum. length becomes shorter. In Such a case, it is preferable that If the normal optical glasses are used for constituting the the refractive lens System Satisfies the following condition conventional type of the achromatic lens, it is impossible to correct the Secondary Spectrum Sufficiently. Because refrac (3); 40 tive index of glass increases as wavelength becomes shorter 1 (3) as described, while increasing degree of the flint glass is 0.02 larger than that of the crown glass in Short wavelength range. Then the chromatic aberration of the doublet is overcor rected (backfocus becomes too long) in the range shorter where than F-line. 45 In order to Suppress the Secondary Spectrum of the lon f is a focal length of the refractive lens System, gitudinal chromatic aberration with the conventional type of f is a focal length of an i-th lens of the refractive lens the achromatic lens, fluorite or anomalous dispersion glass System counted from the object Side, should be used. However, these materials are too expensive. v is an Abbe number of the i-th lens of the refractive lens 50 System counted from the object Side, and SUMMARY OF THE INVENTION m is a total number of lenses of the refractive lens System. It is therefore an object of the present invention to provide In the Second and third groups of the embodiments, the an achromatic lens, which is capable of correcting the refractive achromatic lens is corrected in chromatic aberra Secondary Spectrum of the longitudinal chromatic aberration 55 tion at two different wavelengths and an additional refractive without using expensive material Such as the fluorite or lens generates longitudinal chromatic aberration Such that anomalous dispersion glass. the back focus of the refractive lens System decreases as the For the above object, according to the present invention, wavelength becomes shorter. In Such a case, it is preferable there is provided a diffractive-refractive achromatic lens that that the refractive achromatic lens Satisfies the following includes a refractive lens System exhibiting longitudinal 60 condition (4), chromatic aberration that is Substantially proportional to wavelength such that the back focus of the refractive lens 1 (4) System decreases as the wavelength becomes shorter, and a positive diffractive grating for correcting the longitudinal fiXT, chromatic aberration of the refractive lens System. 65 The refractive lens System having Such a chromatic aber where ration includes a positive lens having relatively Small dis f is a focal length of the refractive achromatic lens, US 6,266,191 B1 3 4 f is a focal length of an i-th lens of the refractive FIGS. 2A through 2D are graphs showing Spherical achromatic lens counted from the object Side, aberration, lateral chromatic aberration, astigmatism and v is an Abbe number of the i-th lens of the refractive distortion, respectively, of the lens in FIG. 1; achromatic lens counted from the object Side, and FIG. 3 is a lens diagram of the diffractive-refractive m is a total number of lenses of the refractive achromatic achromatic lens according to a Second embodiment; lens.
Recommended publications
  • The Plumbers Telescope-English
    240.BLT KLAUS HÜNIG than 10mm. Use sandpaper to smooth the hole and then roughen the inside of the plug The Plumber’s Telescope to provide a good base for the glue. Remove Kit for an astronomical refracting telescope with Put a small amount of glue evenly all dust and loose plastic bits. 30x magnification, fromusing any 40mm local drain DIY pipes store around the inner side of the end with the Step 8: tags, again without drops or strings. Apply a generous amount of glue onto the Push the eyepiece into the holder from disk holding the eyepiece and fit it into the the tag side and slide it into place by socket plug so that the hole in the disk sits pushing it onto the work surface so it is centrally over the hole in the plug. Again flush with the six tags. take care that no glue gets onto the surface of the lens. After the glue has set, push the plug into the second push-fit coupling. This •Achromatic objective lens, finishes the construction of the eyepiece Ø 40mm, f +450mm holder. •Colour corrected Plössl eyepiece, 15mm, f +15mm Step 5: D. The final assembly Ø Open the 11mm central hole in Part C Step 9: •Tripod adapter (without tripod) Remove the rubber seal from the open end of (blind) using a sharp knife and then •Indestructible HT tubing Shopping list for the DIY store: remove the part from the cardboard. the eyepiece holder. Then fit the eyepiece Fold the six tags backwards and glue the holder on the open end of the objective lens •Shows Moon craters, phases tube.
    [Show full text]
  • Buying a Home Microscope
    Buying a Home Microscope The process of ecological restoration requires many tools. I initially learned about prescribed burns, pumper units, backpack sprayers, and Parsnip Predators. But there are 2 other tools that I’ve found important in my quest to learn more about all aspects of ecological restoration, a camera and a microscope! I imagine my journey through restoring prairies, savannas, woodlands, and wetlands began in about the same as many others…learning about the plants and learning techniques for managing the plants. I dove into this head first! I began taking photos of every aspect of the plants that I could. I wanted photos of stems, leaves, petals, stamens, sepals, and seeds. I wanted photos of each plant through their growth stages from seedlings, to vegetation, to flowering, to senescence. The more photos I took and the more I learned, the bigger the picture of the restoration became. I realized there were many aspects working together to make this restoration successful. There was the soil and its ecosystem and processes and there were the insects, the birds, the mammals, the reptiles, the amphibians, and the fungi to consider. The biggest question that niggled at me was how could I possibly create a management plan when the only aspect of the land I knew about were the plants. Well, I also knew a great deal about the birds and their relationship to the plants, but I needed to know much more. I began studying the other aspects!! And once I was through the mammals, reptiles, and amphibians, the subjects started getting smaller and smaller and smaller.
    [Show full text]
  • Evolution of Eyepieces
    EVOLUTION of the ASTRONOMICAL EYEPIECE PREFACE In wri tin g this monograph about In the late 1960’s, when I was Head of astronomical eyepieces Chris Lord has th e Optical Departmen t of carried out a sign al se rvice for Astronomical Equipment Ltd., I would astronomers, be they amateur or pro- take any available new eyepiece to fessional. Horace Dall who would dismantle it and produce a detailed optical pre- Information on eyepieces is difficult to scription. These test reports were not obtain as it is well scattered. Much published, as Selby had done - he did that was available in the first half of however write an article suitable for this century seems to have leant heav- th e non- specialist in the 1963 ily on the articles Optics & T elescopes Yearbook of Astron omy. A sli ghtly in the 9th Edi tio n of t he mo dified versio n appeared in t he Encyclopaedia Britannica c1892! All Journal of the British Astronomical we seemed to read before the 1950’s Association, 1969. He would design w e re descriptions of Huyghenian ; and make specialist eyepieces when Ramsden; Kellner; Orthoscopic, and, the need arose. His extensive note- p e rhaps, solid eyepieces. In 1953 books are now in an archive in the Horace S elby, writing i n Amateur Science Museum. There are rich pick- Telescope Making: B ook Thre e ings there for some future historian of brought out a paper in which he gave science. Since Horace Dall died in detailed descriptions of more tha n 1986 development of eyepieces has forty different eyepieces - many of gone on apace, greatly aided by the which h ad been used durin g the computer revolution.
    [Show full text]
  • Optical Theory Simplified: 9 Fundamentals to Becoming an Optical Genius APPLICATION NOTES
    LEARNING – UNDERSTANDING – INTRODUCING – APPLYING Optical Theory Simplified: 9 Fundamentals To Becoming An Optical Genius APPLICATION NOTES Optics Application Examples Introduction To Prisms Understanding Optical Specifications Optical Cage System Design Examples All About Aspheric Lenses Optical Glass Optical Filters An Introduction to Optical Coatings Why Use An Achromatic Lens www.edmundoptics.com OPTICS APPLICATION EXAMPLES APPLICATION 1: DETECTOR SYSTEMS Every optical system requires some sort of preliminary design. system will help establish an initial plan. The following ques- Getting started with the design is often the most intimidating tions will illustrate the process of designing a simple detector step, but identifying several important specifications of the or emitter system. GOAL: WHERE WILL THE LIGHT GO? Although simple lenses are often used in imaging applications, such as a plano-convex (PCX) lens or double-convex (DCX) in many cases their goal is to project light from one point to lens, can be used. another within a system. Nearly all emitters, detectors, lasers, and fiber optics require a lens for this type of light manipula- Figure 1 shows a PCX lens, along with several important speci- tion. Before determining which type of system to design, an fications: Diameter of the lens (D1) and Focal Length (f). Figure important question to answer is “Where will the light go?” If 1 also illustrates how the diameter of the detector limits the the goal of the design is to get all incident light to fill a detector, Field of View (FOV) of the system, as shown by the approxi- with as few aberrations as possible, then a simple singlet lens, mation for Full Field of View (FFOV): (1.1) D Figure 1: 1 D θ PCX Lens as FOV Limit FF0V = 2 β in Detector Application ƒ Detector (D ) 2 or, by the exact equation: (1.2) / Field of View (β) -1 D FF0V = 2 tan ( 2 ) f 2ƒ For detectors used in scanning systems, the important mea- sure is the Instantaneous Field of View (IFOV), which is the angle subtended by the detector at any instant during scan- ning.
    [Show full text]
  • New Light on the Invention of the Achromatic Telescope Objective”
    Remarks to the Article: “New Light on the Invention of the Achromatic Telescope Objective” Igor Nesterenko FRIB/NSCL, Michigan State University, East Lansing, MI 48824, USA Budker Institute of Nuclear Physics, Novosibirsk, 630090, RUSSIA (corresponding author, e-mail: [email protected]) Abstract The article analysis was carried out within the confines of the replication project of the telescope, which was used by Mikhail Lomonosov at observation the transit of Venus in 1761. At that time he discovered the Venusian atmosphere. It is known that Lomonosov used Dollond’s 4.5 feet long achromatic telescope. The investigation revealed significant faults in the description of the approximation method, which most likely was used by J. Dollond & Son during manufacturing of the early achromatic lenses. Introduction In the article [1] R. Willach described the research of the four early achromatic lenses. Two doublet lenses were made by Dollond: one is flint-forward type and other lens is crown-forward type. The others two doublet lenses (both flint-forward type) were made by James Ayscough and by Joseph Linnell1. The flint-forward doublets are classified as a first early achromatic lenses in comparison with crown-forward type. The optical parameters of the examined flint-forward doublets are collected in the Table 1. For calculation and comparison of the optical systems, Zemax-EE software was used. Table 1. Optical parameters of the flint-forward achromatic lenses Maker D F R1 R2 tflint Glass tair R3 R4 tcrown Glass Name (mm) (mm) (mm) (mm) (mm) Name (mm) (mm) (mm) (mm) Name Dollond 32.0 773 -1826 190 2.8 E18_F1 0.0 193 -262 3.7 E18_C1 Linnell 24.5 492 -83000 99 1.9 E18_F2 0.3 136 -132 4.0 E18_C2 Ayscough 32.0 790 -803 168 1.1 E18_F3 0.2 220 -171 3.5 E18_C3 The measured refractive indexes of the glasses from the investigated achromatic doublets at the different wavelengths are described in Table 2.
    [Show full text]
  • Design and Construction of a Refracting Telescope C
    31102 C. I. Onah and C. M. Ogudo/ Elixir Materials Science 80 (2015) 31102-31108 Available online at www.elixirpublishers.com (Elixir International Journal) Materials Science Elixir Materials Science 80 (2015) 31102-31108 Design and construction of a refracting telescope C. I. Onah * and C. M. Ogudo Department of Physics, Federal University of Technology, Owerri, Nigeria. ARTICLE INFO ABSTRACT Article history: Most people see the telescope as the things for the movies, the science geeks and the rich Received: 29 August 2014; and affluent, but are these feelings for real? This paper on the design and construction of an Received in revised form: optical refracting telescope which is aimed at producing a low cost and portable telescope 28 February 2015; with less or no aberration effects using the materials we see around us every day goes a long Accepted: 14 March 2015; way to answer the question that the telescope is for everybody that loves astronomy. Overall implementation of this work involves knowledge of the physics of optics; lenses to be Keywords precise. As a case study I used a double convex lens and the eyepiece of a microscope for Telescope, the construction of the mini refractor telescope, my hypothesis is that using a double convex Astronomy and General Physics. is better than using a Plano-convex because the two curved surfaces will cancel out the aberration effect of the individual sides. The resultant telescope was tested during the night and during the day and was used to focus objects at a distance of about 50m from the person with less aberration effect.
    [Show full text]
  • 502-20 Chromatic Effects
    20-1 I and Instrumentation Design Optical OPTI-502 © Copyright 2019 John E. Greivenkamp E. John 2019 © Copyright Section 20 Chromatic Effects 20-2 I and Instrumentation Design Optical OPTI-502 Chromatic Aberration Greivenkamp E. John 2019 © Copyright For a thin lens: 1 nCC1 f 12 Since the index changes with wavelength, so will the focal length. z 1 2 3 Where do Red, Green (or Yellow) and Blue focus? n Because of the higher index for Blue or F light, Blue light is bent more and the Blue focus is closest to the lens. The foci corresponding to the F, d and C wavelengths are not evenly spaced due to the shape of the F d C dispersion curve. 20-3 I and Instrumentation Design Optical OPTI-502 Axial or Longitudinal Chromatic Aberration Greivenkamp E. John 2019 © Copyright Axial chromatic aberration or axial color is a variation of the system focal length with wavelength. FdC z f f = fd FC nCCnCC F 1112 C 12 nnCCFC12 11F C nn ffCF f FC nCCd 1 12 CF CF nd 1 ff f 2 n 1 CF 2 CF d d CF d ddnCC1 12 nnF C dd11f ffCF f 2 d dd FC 20-4 I and Instrumentation Design Optical OPTI-502 Axial Chromatic Aberration - Continued Greivenkamp E. John 2019 © Copyright FCf CF 1 d F cFC FC ddf f f ff f d f 1 CF CF ffCF f Since Abbe numbers are typically 30-70, the longitudinal chromatic aberration of a singlet is 1.5-3% of the focal length.
    [Show full text]
  • Aberration Control in Antique Telescope Objectives
    The University of Arizona Aberration Control in Antique Telescope Objectives A Master’s Report by Samuel R. Driscoll In partial fulfillment for the degree of Master of Science in the College of Optical Sciences May 2015 1 The University of Arizona ABSTRACT College of Optical Sciences Master of Science by Samuel Driscoll The development and implementation of achromatic objective lenses in refracting telescopes had a significant impact on image quality and understanding of aberrations in the 18th and 19th centuries. It is common for non-rotationally symmetric errors to be polished into the surfaces of the elements of a telescope objective during the optical manufacturing process. Astigmatism is the most common type of manufacturing error, resulting in a reduction of image quality. Certain achromatic doublets and triplets from the early-mid 1800s have been found to be “clocked” to restrict elements from rotating when mounted in their cells. This paper summarizes different tests performed on these refracting telescope objectives to determine the reasoning behind clocking these lenses and to show how astigmatism was controlled in these telescope objectives. 2 ACKNOWLEDGEMENTS I would like to personally thank many of those who greatly supported and guided me through the completion of this report. Most notably is my advisor, Dr. John Greivenkamp who gave me the inspiration and motivation necessary to succeed in my journey. In addition to Dr. Greivenkamp, I would like to recognize David Steed and the Museum of Optics for their help in procuring and identifying the unique telescope objective, which are the focus of this report. I also would like to acknowledge the other members of my review committee, Dr.
    [Show full text]
  • F/2.8, Its the Following Three Optical Established
    ..... .... Expanding Horizons In Photography Canon's Ultrahigh-Performance L-Series FD Lenses The Ideal Achievement of Canon's Comprehensive Optical Engineering Capabilities necessary. However, in caused by the different remaining in a lens are To eliminate this objectionable because aspherical lenses are A superb camera body is a practice, it is extremely wa velengths of the incident called "residual" aberrations. feature, asphericallenses designed to compensate for prerequisite for taking difficult to create lenses that light. All these aberrations Distinctive expressive have varying curvatures image disto rtion through the quality pictures. However, can approach the "ideal" in influence each o ther in nuances, such as softly which permit all incident use of ideal lens shapes. no matter how superb it may performance. Major obstacles complex ways and affect the out-of-fo cus images, are rays to fo cus at one point. Fo r Asphericallens elements also be, the camera body alone in achieving this include ( I ) image-forming performances produced by these residual example, t he FD 8Smm contribute to re ducing the does not suffice. It requires drawbacks attributable to the of lenses. Aberrations aberrations. f/l.2l short-telephoto lens, overall le ns size. For example, equally superb matching spherical c urvatur~ s of the featuring an extremely large the FD 14mm f/2.Sl uses an interchangeable lenses. elements, (2) pro blems fll.2 maximum aperture, asphericallens element wi th Canon's'\.! I tra-high­ ari sing fro m lens materials, Spherical aberrations are uses an aspherical element an extremely accurate performance l-series FD and (3) problems caused by Spherical aberrations, visible caused by spherical ele ments as its second element.
    [Show full text]
  • Thin Lensesand Chromatic Aberrations
    PHYSICS CONNECTIONS | Introductory Physics Theory Applied to Real-World Problems Thin Lenses and Chromatic Aberrations by Dwight E. Neuenschwander Professor of Physics, Southern Nazarene University, Bethany, OK As SPS gears up to participate in the 2015 UNESCO (United Nations Educational, Imagine you, a physicist, have been hired as an Scientific, and Cultural Organization) Year of Light and Light-Related Technologies, optical engineer for a camera manufacturing we are reminded of the old proverb that says, “The eyes are the window to the company. You have been given the task of soul.” If through the window to your soul you look closely at a small purple dot on designing a system of lenses that will make red a white background, it appears blue in the center surrounded by red. Move farther light and blue light come to a focus at the same out, and the dot appears red in the center surrounded by blue.[1] I do not know spot. Of course, there are other colors in the what this means for the soul, but for optics it means that the lens in the human eye spectrum besides red and blue. But by building exhibits chromatic aberration. This effect occurs when the index of refraction of the a compound lens that focuses onto the same spot lens material varies with the wavelength of light. Such dispersion separates light into light from opposite ends of the visible spectrum, a rainbow when passing through a prism and causes interesting challenges for the you will have made an important step toward designers of refractive optical systems.
    [Show full text]
  • Design of Custom Achromatic Lenses Used for Optical Image Relay System for the OSU Petawatt Class Laser Amplifier Chain
    Design of Custom Achromatic Lenses Used For Optical Image Relay System For The OSU Petawatt Class Laser Amplifier Chain Thesis Presented in Partial Fulfillment of the Requirements for Graduation with Research Distinction in Engineering Physics in the College of Engineering at The Ohio State University By Aakash Patel The Oho State University 2012 Thesis Committee: Professor Linn D. Van Woerkom, Advisor Professor Richard E. Hughes Copyright by Aakash Patel 2012 Abstract The Science Center for the Advanced Research on Lasers and Engineered Targets (SCARLET) laser system of the High Energy Density Physics research group at the Ohio State University is built to study laser-matter interactions at very high intensities. Ultrashort pulses are needed to generate such high intensities. Ultrashort pulses require large bandwidths. The SCARLET laser system is undergoing a major upgrade and part of the new system is a Keplerian telescope that relays the laser pulses. The function of the telescope is to magnify the pulse profile while relaying the image in its most intact form possible. The aberrations created by the lenses of the telescope need to be minimized in order to preserve the image quality. In this kind of application, the adverse effects of the thickness of the lenses and chromatic aberrations become apparent because of the broad spectrum. In order to focus all wavelengths (770 nm to 850 nm) at the same point and re-collimate them, custom designed multi-element lenses needed to be used. After learning about achromats, aberrations and principles used to minimize the aberrations, lens design software OSLO was used for computer aided ray-tracing and analysis of optical performance.
    [Show full text]
  • Optics: How to Build a Beam Expander
    Optics Technical Note # 1 Optical Components Optics: How to Build a Beam Expander Beam expansion or reduction is a common application requirement in most labs using lasers or light sources and optics. There are many ready made beam expanders available on the market, but often they are not available in the required expansion ratio or spectral range. And, for students, or those working within a tight budget, the plug and play solution may not be the answer. Luckily, building a beam expander from off-the-shelf components is easily accomplished and can be fit into most budgets. The quality of the output is dependant only on the input beam and the component optics used. To create a beam expansion unit, it is important to know a few simple optical relationships, as well as what your input to output beam diameter ratio requirement is. Simple beam expanders, sometimes referred to as telescopes, in their most basic forms generally consist of two lenses. The first lens should have a diameter larger than the maximum expected input diameter of the incoming light source. For example, if the diameter of the incoming beam is 10mm, a 12mm diameter lens will do a nice job with a little room to spare. The input beam is assumed to be collimated. The diameter of the output lens should be larger than the desired exit beam diameter. For a 3x expansion ratio with a 10mm maximum input beam diameter, an output lens of greater than 30mm in diameter is required. The useable diameter of a lens is usually specified at approximately 80% of the actual lens diameter, a minimum lens diameter of 37.5mm would be required.
    [Show full text]