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Official Publication of the Optometric Historical Society
Official Publication of the Optometric Historical Society Hindsight: Journal of Optometry History publishes material on the history of optometry and related topics. As the official publication of the Optometric Historical Society, Hindsight: Journal of Optometry History supports the purposes and functions of the Optometric Historical Society. The purposes of the Optometric Historical Society, according to its by-laws, are: ● to encourage the collection and preservation of materials relating to the history of optometry, ● to assist in securing and documenting the recollections of those who participated in the development of optometry, ● to encourage and assist in the care of archives of optometric interest, ● to identify and mark sites, landmarks, monuments, and structures of significance in optometric development, and ● to shed honor and recognition on persons, groups, and agencies making notable contributions toward the goals of the society. Officers and Board of Trustees of the Optometric Historical Society (with years of expiration of their terms on the Board in parentheses): President: John F. Amos (2015), email address: [email protected] Vice-President: Alden Norm Haffner (2014) Secretary-Treasurer: Chuck Haine (2016) Trustees: Jerry Abrams (2013) Arol Augsburger (2013) Irving Bennett (2016) Jay M. Enoch (2014) Morton Greenspoon (2015) Alfred Rosenbloom (2015) The official publication of the Optometric Historical Society, published quarterly since its beginning, was previously titled: Newsletter of the Optometric Historical Society, 1970-1991 (volumes 1-22), and Hindsight: Newsletter of the Optometric Historical Society, 1992-2006 (volumes 23-37). Use of the current title, Hindsight: Journal of Optometry History, began in 2007 with volume 38, number 1. On the cover: An image of the Chambers-Inskeep Ophthalmometer when it was introduced in 1899, from the May 24, 1899 issue of Jewelers Review (volume 32, page 652). -
Telescopes and Binoculars
Continuing Education Course Approved by the American Board of Opticianry Telescopes and Binoculars National Academy of Opticianry 8401 Corporate Drive #605 Landover, MD 20785 800-229-4828 phone 301-577-3880 fax www.nao.org Copyright© 2015 by the National Academy of Opticianry. All rights reserved. No part of this text may be reproduced without permission in writing from the publisher. 2 National Academy of Opticianry PREFACE: This continuing education course was prepared under the auspices of the National Academy of Opticianry and is designed to be convenient, cost effective and practical for the Optician. The skills and knowledge required to practice the profession of Opticianry will continue to change in the future as advances in technology are applied to the eye care specialty. Higher rates of obsolescence will result in an increased tempo of change as well as knowledge to meet these changes. The National Academy of Opticianry recognizes the need to provide a Continuing Education Program for all Opticians. This course has been developed as a part of the overall program to enable Opticians to develop and improve their technical knowledge and skills in their chosen profession. The National Academy of Opticianry INSTRUCTIONS: Read and study the material. After you feel that you understand the material thoroughly take the test following the instructions given at the beginning of the test. Upon completion of the test, mail the answer sheet to the National Academy of Opticianry, 8401 Corporate Drive, Suite 605, Landover, Maryland 20785 or fax it to 301-577-3880. Be sure you complete the evaluation form on the answer sheet. -
Articles Articles
Articles Articles ALEXI BAKER “Precision,” “Perfection,” and the Reality of British Scientific Instruments on the Move During the 18th Century Résumé Abstract On représente souvent les instruments scientifiques Early modern British “scientific” instruments, including du 18e siècle, y compris les chronomètres de précision, precision timekeepers, are often represented as static, comme des objets statiques, à l’état neuf et complets en pristine, and self-contained in 18th-century depictions eux-mêmes dans les descriptions des débuts de l’époque and in many modern museum displays. In reality, they moderne et dans de nombreuses expositions muséales were almost constantly in physical flux. Movement and d’aujourd’hui. En réalité, ces instruments se trouvaient changing and challenging environmental conditions presque constamment soumis à des courants physiques. frequently impaired their usage and maintenance, Le mouvement et les conditions environnementales especially at sea and on expeditions of “science” and difficiles et changeantes perturbaient souvent leur exploration. As a result, individuals’ experiences with utilisation et leur entretien, en particulier en mer et mending and adapting instruments greatly defined the lors d’expéditions scientifiques et d’exploration. Ce culture of technology and its use as well as later efforts sont donc les expériences individuelles de réparation at standardization. et d’adaptation des instruments qui ont grandement contribué à définir la culture de la technologie. In 1769, the astronomer John Bradley finally the calculation of the distance between the Earth reached the Lizard peninsula in Cornwall and the Sun. Bradley had not needed to travel with his men, instruments, and portable tent as far as many of his Transit counterparts, but observatory after a stressful journey. -
A Newly-Discovered Accurate Early Drawing of M51, the Whirlpool Nebula
Journal of Astronomical History and Heritage , 11(2), 107-115 (2008). A NEWLY-DISCOVERED ACCURATE EARLY DRAWING OF M51, THE WHIRLPOOL NEBULA William Tobin 6 rue Saint Louis, 56000 Vannes, France. E-mail: [email protected] and J.B. Holberg Lunar and Planetary Laboratory, University of Arizona, 1541 East University Boulevard, Tucson, AZ 85721, U.S.A. E-mail: [email protected] Abstract: We have discovered a lost drawing of M51, the nebula in which spiral structure was first discovered by Lord Rosse. The drawing was made in April 1862 by Jean Chacornac at the Paris Observatory using Léon Foucault’s newly-completed 80-cm silvered-glass reflecting telescope. Comparison with modern images shows that Chacornac’s drawing was more accurate with respect to gross structure and showed fainter details than any other nineteenth century drawing, although its superiority would not have been apparent at the time without nebular photography to provide a standard against which to judge drawing quality. M51 is now known as the Whirlpool Nebula, but the astronomical appropriation of ‘whirlpool’ predates Rosse’s discovery. Keywords: reflecting telescopes, nebulae, spiral structure, Léon Foucault, Lord Rosse, M51, Whirlpool Nebula 1 REFLECTING TELESCOPES AND SPIRAL STRUCTURE The French physicist Léon Foucault (1819–1868) is the father of the reflecting telescope in its modern form, with large, optically-perfect, metallized glass or ceramic mirrors. Foucault achieved this breakthrough while working as ‘physicist’ at the Paris Observatory in the late 1850s. The largest telescope that he built (Foucault, 1862) had a silvered-glass, f/5.6 primary mirror of 80-cm diameter in a Newtonian configura- tion (see Figure 1). -
Philosophical Transactions (A)
INDEX TO THE PHILOSOPHICAL TRANSACTIONS (A) FOR THE YEAR 1889. A. A bney (W. de W.). Total Eclipse of the San observed at Caroline Island, on 6th May, 1883, 119. A bney (W. de W.) and T horpe (T. E.). On the Determination of the Photometric Intensity of the Coronal Light during the Solar Eclipse of August 28-29, 1886, 363. Alcohol, a study of the thermal properties of propyl, 137 (see R amsay and Y oung). Archer (R. H.). Observations made by Newcomb’s Method on the Visibility of Extension of the Coronal Streamers at Hog Island, Grenada, Eclipse of August 28-29, 1886, 382. Atomic weight of gold, revision of the, 395 (see Mallet). B. B oys (C. V.). The Radio-Micrometer, 159. B ryan (G. H.). The Waves on a Rotating Liquid Spheroid of Finite Ellipticity, 187. C. Conroy (Sir J.). Some Observations on the Amount of Light Reflected and Transmitted by Certain 'Kinds of Glass, 245. Corona, on the photographs of the, obtained at Prickly Point and Carriacou Island, total solar eclipse, August 29, 1886, 347 (see W esley). Coronal light, on the determination of the, during the solar eclipse of August 28-29, 1886, 363 (see Abney and Thorpe). Coronal streamers, observations made by Newcomb’s Method on the Visibility of, Eclipse of August 28-29, 1886, 382 (see A rcher). Cosmogony, on the mechanical conditions of a swarm of meteorites, and on theories of, 1 (see Darwin). Currents induced in a spherical conductor by variation of an external magnetic potential, 513 (see Lamb). 520 INDEX. -
Aplea for Reflectors
A PLEA FOR REFLECTORS Pedro RÉ http://pedroreastrophotography.com/ In 1867 John Browing (c1833-1925)1 published a trade catalogue entitled “A Plea for Reflectors: Being a Description of the New Astronomical Telescopes with Silvered-Glass Specula; And Instructions for adjusting and Using Them”. This catalogue had six editions that were published until 18762. Browning describes his range of reflecting telescopes, how to use them and compares these with achromatic refractors of comparable apertures. It also contains numerous details of its extensive range of glass silvered specula, eyepieces, micrometres, barometers and microscopes (Figure 1). The back of the booklet contains testimonials from satisfied customers, many of them distinguished amateurs and professionals. By publishing “A Plea for Reflectors”, J. Browning & Co. became one of the first to mass produce telescopes for the amateur (Figure 2). The popularity of the Newtonian reflector as the instrument of choice for the amateur astronomer followed the pioneering work of George Henry With (1827-1904). With began making silvered-glass mirrors in the early 1860's following his retirement as schoolmaster at the Blue Coat School, Hereford. With did not actually make telescopes. His principal customer was John Browning, the London instrument maker well-known for his spectroscopes and telescopes. Browning's business flourished to circa 1905, possibly first starting at 1 Norfolk Street, Strand circa 1866. The firm had their 'factory' in Vine Street EC3 (1872-76) and Southampton Street north off the Strand (1877-82) and William Street (1887). The shop was at 111 Minories (near Tower Hill) working under the name Spencer, Browning and Co. -
The Herschels and Their Astronomy
The Herschels and their Astronomy Mary Kay Hemenway 24 March 2005 outline • William Herschel • Herschel telescopes • Caroline Herschel • Considerations of the Milky Way • William Herschel’s discoveries • John Herschel Wm. Herschel (1738-1822) • Born Friedrich Wilhelm Herschel in Hanover, Germany • A bandboy with the Hanoverian Guards, later served in the military; his father helped him to leave Germany for England in 1757 • Musician in Bath • He read Smith's Harmonies, and followed by reading Smith's Optics - it changed his life. Miniature portrait from 1764 Discovery of Uranus 1781 • William Herschel used a seven-foot Newtonian telescope • "in the quartile near zeta Tauri the lowest of the two is a curious either Nebulous Star or perhaps a Comet” • He called it “Georgium Sidus" after his new patron, George Ill. • Pension of 200 pounds a year and knighted, the "King's Astronomer” -- now astronomy full time. Sir William Herschel • Those who had received a classical education in astronomy agreed that their job was to study the sun, moon, planets, comets, individual stars. • Herschel acted like a naturalist, collecting specimens in great numbers, counting and classifying them, and later trying to organize some into life cycles. • Before his discovery of Uranus, Fellows of the Royal Society had contempt for his ignorance of basic procedures and conventions. Isaac Newton's reflecting telescope 1671 William Herschel's 20-foot, 1783 Account of some Observations tending to investigate the Construction of the Heavens Philosophical Transactions of the Royal Society of London (1784) vol. 74, pp. 437-451 In a former paper I mentioned, that a more powerful instrument was preparing for continuing my reviews of the heavens. -
James Short and John Harrison: Personal Genius and Public Knowledge
Science Museum Group Journal James Short and John Harrison: personal genius and public knowledge Journal ISSN number: 2054-5770 This article was written by Jim Bennett 10-09-2014 Cite as 10.15180; 140209 Research James Short and John Harrison: personal genius and public knowledge Published in Autumn 2014, Issue 02 Article DOI: http://dx.doi.org/10.15180/140209 Abstract The instrument maker James Short, whose output was exclusively reflecting telescopes, was a sustained and consistent supporter of the clock and watch maker John Harrison. Short’s specialism placed his work in a tradition that derived from Newton’s Opticks, where the natural philosopher or mathematician might engage in the mechanical process of making mirrors, and a number of prominent astronomers followed this example in the eighteenth century. However, it proved difficult, if not impossible, to capture and communicate in words the manual skills they had acquired. Harrison’s biography has similarities with Short’s but, although he was well received and encouraged in London, unlike Short his mechanical practice did not place him at the centre of the astronomers’ agenda. Harrison became a small part of the growing public interest in experimental demonstration and display, and his timekeepers became objects of exhibition and resort. Lacking formal training, he himself came to be seen as a naive or intuitive mechanic, possessed of an individual and natural ‘genius’ for his work – an idea likely to be favoured by Short and his circle, and appropriate to Short’s intellectual roots in Edinburgh. The problem of capturing and communicating Harrison’s skill became acute once he was a serious candidate for a longitude award and was the burden of the specially appointed ‘Commissioners for the Discovery of Mr Harrison’s Watch’, whose members included Short. -
Back Matter (PDF)
[ 395 ] INDEX TO THE PHILOSOPHICAL TRANSACTIONS, S e r ie s A, V o l . 193. A. Abney (W. de W.). The Colour Sensations in Terms of Luminosity, 259. Atmospheric electricity—experiments in connection with precipitation (Wilson), 289. Bakebian Lectube. See Ewing and Kosenhain. C. Colour-blind, neutral points in spectra found by (Abney), 259. Colour sensations in terms of luminosity (Abney), 259. Condensation nuclei, positively and negatively charged ions as (W ilson), 289. Crystalline aggregates, plasticity in (Ewing and Rosenhain), 353. D. Dawson (H. M.). See Smithells, Dawson, and Wilson VOL. CXCIII.— Ao : S F 396 INDEX. Electric spark, constitution of (Schuster and Hemsalech), 189; potential—variation with pressure (Strutt), 377. Electrical conductivity of flames containing vaporised salts (Smithells, Dawson, and Wilson), 89. Electrocapillary phenomena, relation to potential differences between‘solutions (Smith), 47. Electrometer, capillary, theory of (Smith), 47. Ewing (J. A.) and Rosenhain (W.). The Crystalline Structure of Metals.—Bakerian Lecture, 353. F. Filon (L. N. G ). On the Resistance to Torsion of certain Forms of Shafting, with special Reference to the Effect of Keyways, 309. Flames, electrical conductivity of, and luminosity of salt vapours in (Smithells, Dawson, and Wilson), 89. G. Gravity balance, quartz thread (Threlfall and Pollock), 215. H. Hemsalech (Gustav). See Schuster and Hemsalech. Hertzian oscillator, vibrations in field of (Pearson and Lee), 159. Hysteresis in the relation of extension to stress exhibited by overstrained iron (Muir), 1. I. Ions, diffusion into gases, determination of coefficient (Townsend), 129. Ions positively and negatively charged, as condensation nuclei (Wilson), 289. Iron, recovery of, from overstrain (Muir), 1. -
“Precision,” “Perfection,” and the Reality of British Scientific Instruments on the Move During the 18Th Century Alexi Baker
Document generated on 09/29/2021 11:28 a.m. Material Culture Review “Precision,” “Perfection,” and the Reality of British Scientific Instruments on the Move During the 18th Century Alexi Baker Volume 74-75, 2012 Article abstract Early modern British “scientific” instruments, including precision timekeepers, URI: https://id.erudit.org/iderudit/mcr74_75art01 are often represented as static, pristine, and self-contained in 18th-century depictions and in many modern museum displays. In reality, they were almost See table of contents constantly in physical flux. Movement and changing and challenging environmental conditions frequently impaired their usage and maintenance, especially at sea and on expeditions of “science” and exploration. As a result, Publisher(s) individuals’ experiences with mending and adapting instruments greatly defined the culture of technology and its use as well as later efforts at standardization. National Museums of Canada ISSN 0316-1854 (print) 0000-0000 (digital) Explore this journal Cite this article Baker, A. (2012). “Precision,” “Perfection,” and the Reality of British Scientific Instruments on the Move During the 18th Century. Material Culture Review, 74-75, 14–29. All rights reserved © National Museums of Canada, 2011 This document is protected by copyright law. Use of the services of Érudit (including reproduction) is subject to its terms and conditions, which can be viewed online. https://apropos.erudit.org/en/users/policy-on-use/ This article is disseminated and preserved by Érudit. Érudit is a non-profit inter-university consortium of the Université de Montréal, Université Laval, and the Université du Québec à Montréal. Its mission is to promote and disseminate research. -
United Kingdom Was Originally Printed in 2003 but Contains Updates to Their Coordinate System Since Then
UNITED BY Clifford J. Mugnier, CP, CMS, FASPRS KINGDOM The Grids & Datums column has completed an exploration of every country on the Earth. For those who did not get to enjoy this world tour the first time,PE&RS is reprinting prior articles from the column. This month’s article on the United Kingdom was originally printed in 2003 but contains updates to their coordinate system since then. he United Kingdom includes England, Scotland, Wales, and Northern Ireland. TThe latter was included in a previous column on the entire island of Ireland (PE&RS, March 1999). Evidence from pre-Roman times includes Neolithic mound-tombs and henge monuments as well as Bronze Age Beaker culture tools, graves, and the famous StonehengeDelivered by Ingenta monument. Brythonic-speakingIP: 192.168.39.210Celtic peoples On: Tue, 28 Sep 2021 17:39:36 Copyright: American Society for Photogrammetry and Remote Sensing arrived during migrations of the first millennium B.C., according to Webster’s Geographical Dictionary. England has existed as a unified name engraved on the curved glass entrance doors, yet his entity since the 10th century. The union between vision of a national military survey wasn’t implemented un- England and Wales was begun in 1284 and til after his death in 1790. By then Europe was in turmoil, formalized in 1536. England and Scotland agreed and there were real fears that the French Revolution might to join as Great Britain in 1707 and with Ireland sweep across the English Channel. in 1801. The present name of Great Britain and Realizing the danger, the government ordered its defense Northern Ireland was adopted in 1927. -
Full History of The
London Mathematical Society Historical Overview Taken from the Introduction to The Book of Presidents 1865-1965 ADRIAN RICE The London Mathematical Society (LMS) is the primary learned society for mathematics in Britain today. It was founded in 1865 for the promotion and extension of mathematical knowledge, and in the 140 years since its foundation this objective has remained unaltered. However, the ways in which it has been attained, and indeed the Society itself, have changed considerably during this time. In the beginning, there were just nine meetings per year, twenty-seven members and a handful of papers printed in the slim first volume of the ’s Society Proceedings. Today, with a worldwide membership in excess of two thousand, the LMS is responsible for numerous books, journals, monographs, lecture notes, and a whole range of meetings, conferences, lectures and symposia. The Society continues to uphold its original remit, but via an increasing variety of activities, ranging from advising the government on higher education, to providing financial support for a wide variety of mathematically-related pursuits. At the head of the Society there is, and always has been, a President, who is elected annually and who may serve up to two years consecutively. As befits a prestigious national organization, these Presidents have often been famous mathematicians, well known and respected by the mathematical community of their day; they include Cayley and Sylvester, Kelvin and Rayleigh, Hardy and Littlewood, Atiyah and Zeeman.1 But among the names on the presidential role of honour are many people who are perhaps not quite so famous today, ’t have theorems named after them, and who are largely forgotten by the majority of who don modern-day mathematicians.