Lord Rutherford (1871–1937): the Newton of the Atom and the Winner
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Cathode Rays 89 Cathode Rays
Cathode Rays 89 Cathode Rays Theodore Arabatzis C The detection of cathode rays was a by-product of the investigation of the discharge of electricity through rarefied gases. The latter phenomenon had been studied since the early eighteenth century. By the middle of the nineteenth century it was known that the passage of electricity through a partly evacuated tube produced a glow in the gas, whose color depended on its chemical composition and its pressure. Below a certain pressure the glow assumed a stratified pattern of bright and dark bands. During the second half of the nineteenth century the discharge of electricity through gases became a topic of intense exploratory experimentation, primarily in Germany [21]. In 1855 the German instrument maker Heinrich Geißler (1815– 1879) manufactured improved vacuum tubes, which made possible the isolation and investigation of cathode rays [23]. In 1857 Geissler’s tubes were employed by Julius Pl¨ucker (1801–1868) to study the influence of a magnet on the electrical dis- charge. He observed various complex and striking phenomena associated with the discharge. Among those phenomena were a “light which appears about the negative electrode” and a fluorescence in the glass of the tube ([9], pp. 122, 130). The understanding of those phenomena was advanced by Pl¨ucker’s student and collaborator, Johann Wilhelm Hittorf (1824–1914), who observed that “if any ob- ject is interposed in the space filled with glow-light [emanating from the negative electrode], it throws a sharp shadow on the fluorescent side” ([5], p. 117). This effect implied that the “rays” emanating from the cathode followed a straight path. -
Rutherford's Nuclear World: the Story of the Discovery of the Nuc
Rutherford's Nuclear World: The Story of the Discovery of the Nuc... http://www.aip.org/history/exhibits/rutherford/sections/atop-physic... HOME SECTIONS CREDITS EXHIBIT HALL ABOUT US rutherford's explore the atom learn more more history of learn about aip's nuclear world with rutherford about this site physics exhibits history programs Atop the Physics Wave ShareShareShareShareShareMore 9 RUTHERFORD BACK IN CAMBRIDGE, 1919–1937 Sections ← Prev 1 2 3 4 5 Next → In 1962, John Cockcroft (1897–1967) reflected back on the “Miraculous Year” ( Annus mirabilis ) of 1932 in the Cavendish Laboratory: “One month it was the neutron, another month the transmutation of the light elements; in another the creation of radiation of matter in the form of pairs of positive and negative electrons was made visible to us by Professor Blackett's cloud chamber, with its tracks curled some to the left and some to the right by powerful magnetic fields.” Rutherford reigned over the Cavendish Lab from 1919 until his death in 1937. The Cavendish Lab in the 1920s and 30s is often cited as the beginning of modern “big science.” Dozens of researchers worked in teams on interrelated problems. Yet much of the work there used simple, inexpensive devices — the sort of thing Rutherford is famous for. And the lab had many competitors: in Paris, Berlin, and even in the U.S. Rutherford became Cavendish Professor and director of the Cavendish Laboratory in 1919, following the It is tempting to simplify a complicated story. Rutherford directed the Cavendish Lab footsteps of J.J. Thomson. Rutherford died in 1937, having led a first wave of discovery of the atom. -
Former Fellows Biographical Index Part
Former Fellows of The Royal Society of Edinburgh 1783 – 2002 Biographical Index Part Two ISBN 0 902198 84 X Published July 2006 © The Royal Society of Edinburgh 22-26 George Street, Edinburgh, EH2 2PQ BIOGRAPHICAL INDEX OF FORMER FELLOWS OF THE ROYAL SOCIETY OF EDINBURGH 1783 – 2002 PART II K-Z C D Waterston and A Macmillan Shearer This is a print-out of the biographical index of over 4000 former Fellows of the Royal Society of Edinburgh as held on the Society’s computer system in October 2005. It lists former Fellows from the foundation of the Society in 1783 to October 2002. Most are deceased Fellows up to and including the list given in the RSE Directory 2003 (Session 2002-3) but some former Fellows who left the Society by resignation or were removed from the roll are still living. HISTORY OF THE PROJECT Information on the Fellowship has been kept by the Society in many ways – unpublished sources include Council and Committee Minutes, Card Indices, and correspondence; published sources such as Transactions, Proceedings, Year Books, Billets, Candidates Lists, etc. All have been examined by the compilers, who have found the Minutes, particularly Committee Minutes, to be of variable quality, and it is to be regretted that the Society’s holdings of published billets and candidates lists are incomplete. The late Professor Neil Campbell prepared from these sources a loose-leaf list of some 1500 Ordinary Fellows elected during the Society’s first hundred years. He listed name and forenames, title where applicable and national honours, profession or discipline, position held, some information on membership of the other societies, dates of birth, election to the Society and death or resignation from the Society and reference to a printed biography. -
Front Matter (PDF)
PROCEEDINGS OF THE OYAL SOCIETY OF LONDON Series A CONTAINING PAPERS OF A MATHEMATICAL AND PHYSICAL CHARACTER. VOL. LXXXV. LONDON: P rinted for THE ROYAL SOCIETY and S old by HARRISON AND SONS, ST. MARTIN’S LANE, PRINTERS IN ORDINARY TO HIS MAJESTY. N ovember, 1911. LONDON: HARRISON AND SONS, PRINTERS IN ORDINARY TO HTS MAJESTY, ST. MARTIN’S LANE. CONTENTS --- 0 0 ^ 0 0 ----- SERIES A. VOL. LXXXV. No. A 575.—March 14, 1911. P AG-E The Chemical Physics involved in the Precipitation of Free Carbon from the Alloys of the Iron-Carbon System. By W. H. Hatfield, B. Met. (Sheffield University). Communicated by Prof. W. M. Hicks, F.R.S. (Plates 1—5) ................... .......... 1 On the Fourier Constants of a Function. By W. H. Young, Se.D., F.R.S................. 14 The Charges on Ions in Gases, and some Effects that Influence the Motion of Negative Ions. By Prof. John S. Townsend, F.R.S............................................... 25 On the Energy and Distribution of Scattered Rontgen Radiation. By J. A. Crowtlier, M.A., Fellow of St. John's College, Cambridge. Com municated by Prof. Sir J. J. Thomson, F.R.S...........................*.............................. 29 The Origin of Magnetic Storms. By Arthur Schuster, F.R.S...................................... 44 On the Periodicity of Sun-spots. By Arthur Schuster, F.R.S..................................... 50 The Absorption Spectx*a of Lithium and Caesium. By Prof. P. V. Bevan, M.A., Royal Holloway College. Communicated by Sir J. J. Thomson, F.R.S.............. 54 Dispersion in Vapours of the Alkali Metals. By Prof. P. V. Bevan, M.A., Royal Holloway College. -
1 Ethers, Religion and Politics In
ORE Open Research Exeter TITLE Ethers, religion and politics in late-Victorian physics: beyond the Wynne thesis AUTHORS Noakes, Richard JOURNAL History of Science DEPOSITED IN ORE 16 June 2008 This version available at http://hdl.handle.net/10036/30065 COPYRIGHT AND REUSE Open Research Exeter makes this work available in accordance with publisher policies. A NOTE ON VERSIONS The version presented here may differ from the published version. If citing, you are advised to consult the published version for pagination, volume/issue and date of publication ETHERS, RELIGION AND POLITICS IN LATE-VICTORIAN PHYSICS: BEYOND THE WYNNE THESIS RICHARD NOAKES 1. INTRODUCTION In the past thirty years historians have demonstrated that the ether of physics was one of the most flexible of all concepts in the natural sciences. Cantor and Hodge’s seminal collection of essays of 1981 showed how during the eighteenth and nineteenth centuries British and European natural philosophers invented a range of ethers to fulfil diverse functions from the chemical and physiological to the physical and theological.1 In religious discourse, for example, Cantor identified “animate” and spiritual ethers invented by neo-Platonists, mystics and some Anglicans to provide a mechanism for supporting their belief in Divine immanence in the cosmos; material, mechanistic and contact-action ethers which appealed to atheists and Low Churchmen because such media enabled activity in the universe without constant and direct Divine intervention; and semi-spiritual/semi-material ethers that appealed to dualists seeking a mechanism for understanding the interaction of mind and matter. 2 The third type proved especially attractive to Oliver Lodge and several other late-Victorian physicists who claimed that the extraordinary physical properties of the ether made it a possible mediator between matter and spirit, and a weapon in their fight against materialistic conceptions of the cosmos. -
Front Matter (PDF)
PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON Series A CONTAINING PAPERS OF A MATHEMATICAL AND PHYSICAL CHARACTER. VOL. G LONDON: P rinted for THE ROYAL SOCIETY and Sold by HARRISON AND SONS, Ltd., ST. MARTIN’S LANE,. PRINTERS in ordinary to h is m a jesty . March, 1922. LONDON : HARRISON AND SONS, LTD., PRINTERS IN ORDINARY TO HIS MAJESTY, ST. MARTIN^ LANE. CONTENTS ---------------- SERIES A. VOL. C. i PAGE Minutes of Meetings, November 3, 1021—February 23, 1922 .................................. i No. A 702.—October 4, 1921. On the Velocity of Sound in Gases at High Temperatures, and the Ratio of the Specific Heats. By Harold B. Dixon, C.B.E., F.R.S., Colin Campbell, D.Sc., and A. Parker, D.Sc....................................................................................................... 1 The Ratio of the Specific Heats of Air and of Carbon Dioxide. By J. R. Partington, D.Sc. Communicated by Dr. J. A. Harker, F.R.S............................ 27 On the Currents induced in a Conductor by the Passage of a Mass of Magnetic Material over it. By E. S. Bieler, M.Sc., 1851 Scholar of McGill University. Communicated by Sir E. Rutherford, F.R.S. (Plate 1 ) ............. ................ 1.......... 50 On some New Formuke for the Numerical Calculation of the Mutual Induction of Coaxial Circles. By Louis V. King, D.Sc., Macdonald Professor of Physics, McGill University, Montreal. Communicated by Prof. A. S. Eve, F.R.S......... 60 Gaseous Combustion at High Pressures. Part II.—The Explosion of Hydrogen-Air and Carbon Monoxide-Air Mixtures. By William A rthur Bone, D.Sc., Ph.D., F.R.S.,'and the late William Arthur Haward, M.Sc., Salters’Research Fellow.. -
Guides to the Royal Institution of Great Britain: 1 HISTORY
Guides to the Royal Institution of Great Britain: 1 HISTORY Theo James presenting a bouquet to HM The Queen on the occasion of her bicentenary visit, 7 December 1999. by Frank A.J.L. James The Director, Susan Greenfield, looks on Front page: Façade of the Royal Institution added in 1837. Watercolour by T.H. Shepherd or more than two hundred years the Royal Institution of Great The Royal Institution was founded at a meeting on 7 March 1799 at FBritain has been at the centre of scientific research and the the Soho Square house of the President of the Royal Society, Joseph popularisation of science in this country. Within its walls some of the Banks (1743-1820). A list of fifty-eight names was read of gentlemen major scientific discoveries of the last two centuries have been made. who had agreed to contribute fifty guineas each to be a Proprietor of Chemists and physicists - such as Humphry Davy, Michael Faraday, a new John Tyndall, James Dewar, Lord Rayleigh, William Henry Bragg, INSTITUTION FOR DIFFUSING THE KNOWLEDGE, AND FACILITATING Henry Dale, Eric Rideal, William Lawrence Bragg and George Porter THE GENERAL INTRODUCTION, OF USEFUL MECHANICAL - carried out much of their major research here. The technological INVENTIONS AND IMPROVEMENTS; AND FOR TEACHING, BY COURSES applications of some of this research has transformed the way we OF PHILOSOPHICAL LECTURES AND EXPERIMENTS, THE APPLICATION live. Furthermore, most of these scientists were first rate OF SCIENCE TO THE COMMON PURPOSES OF LIFE. communicators who were able to inspire their audiences with an appreciation of science. -
December 4, 1954 NATURE 1037
No. 4440 December 4, 1954 NATURE 1037 COPLEY MEDALLISTS, 1915-54 is that he never ventured far into interpretation or 1915 I. P. Pavlov 1934 Prof. J. S. Haldane prediction after his early studies in fungi. Here his 1916 Sir James Dewar 1935 Prof. C. T. R. Wilson interpretation was unfortunate in that he tied' the 1917 Emile Roux 1936 Sir Arthur Evans word sex to the property of incompatibility and 1918 H. A. Lorentz 1937 Sir Henry Dale thereby led his successors astray right down to the 1919 M. Bayliss W. 1938 Prof. Niels Bohr present day. In a sense the style of his work is best 1920 H. T. Brown 1939 Prof. T. H. Morgan 1921 Sir Joseph Larmor 1940 Prof. P. Langevin represented by his diagrams of Datura chromosomes 1922 Lord Rutherford 1941 Sir Thomas Lewis as packets. These diagrams were useful in a popular 1923 Sir Horace Lamb 1942 Sir Robert Robinson sense so long as one did not take them too seriously. 1924 Sir Edward Sharpey- 1943 Sir Joseph Bancroft Unfortunately, it seems that Blakeslee did take them Schafer 1944 Sir Geoffrey Taylor seriously. To him they were the real and final thing. 1925 A. Einstein 1945 Dr. 0. T. Avery By his alertness and ingenuity and his practical 1926 Sir Frederick Gow 1946 Dr. E. D. Adrian sense in organizing the Station for Experimental land Hopkins 1947 Prof. G. H. Hardy Evolution at Cold Spring Harbor (where he worked 1927 Sir Charles Sherring- 1948 . A. V. Hill Prof in 1942), ton 1949 Prof. G. -
THE ETHICAL DILEMMA of SCIENCE and OTHER WRITINGS the Rockefeller Institute Press
THE ETHICAL DILEMMA OF SCIENCE AND OTHER WRITINGS The Rockefeller Institute Press IN ASSOCIATION WITH OXFORD UNIVERSITY PRESS NEW YORK 1960 @ 1960 BY THE ROCKEFELLER INSTITUTE PRESS ALL RIGHTS RESERVED BY THE ROCKEFELLER INSTITUTE PRESS IN ASSOCIATION WITH OXFORD UNIVERSITY PRESS Library of Congress Catalogue Card Number 60-13207 PRINTED IN THE UNITED STATES OF AMERICA CONTENTS CHAPTER ONE The Ethical Dilemma of Science Living mechanism 5 The present tendencies and the future compass of physiological science 7 Experiments on frogs and men 24 Scepticism and faith 39 Science, national and international, and the basis of co-operation 45 The use and misuse of science in government 57 Science in Parliament 67 The ethical dilemma of science 72 Science and witchcraft, or, the nature of a university 90 CHAPTER TWO Trailing One's Coat Enemies of knowledge 105 The University of London Council for Psychical Investigation 118 "Hypothecate" versus "Assume" 120 Pharmacy and Medicines Bill (House of Commons) 121 The social sciences 12 5 The useful guinea-pig 127 The Pure Politician 129 Mugwumps 131 The Communists' new weapon- germ warfare 132 Independence in publication 135 ~ CONTENTS CHAPTER THREE About People Bertram Hopkinson 1 39 Hartley Lupton 142 Willem Einthoven 144 The Donnan-Hill Effect (The Mystery of Life) 148 F. W. Lamb 156 Another Englishman's "Thank you" 159 Ivan P. Pavlov 160 E. D. Adrian in the Chair of Physiology at Cambridge 165 Louis Lapicque 168 E. J. Allen 171 William Hartree 173 R. H. Fowler 179 Joseph Barcroft 180 Sir Henry Dale, the Chairman of the Science Committee of the British Council 184 August Krogh 187 Otto Meyerhof 192 Hans Sloane 195 On A. -
Center for History of Physics Newsletter, Spring 2008
One Physics Ellipse, College Park, MD 20740-3843, CENTER FOR HISTORY OF PHYSICS NIELS BOHR LIBRARY & ARCHIVES Tel. 301-209-3165 Vol. XL, Number 1 Spring 2008 AAS Working Group Acts to Preserve Astronomical Heritage By Stephen McCluskey mong the physical sciences, astronomy has a long tradition A of constructing centers of teaching and research–in a word, observatories. The heritage of these centers survives in their physical structures and instruments; in the scientific data recorded in their observing logs, photographic plates, and instrumental records of various kinds; and more commonly in the published and unpublished records of astronomers and of the observatories at which they worked. These records have continuing value for both historical and scientific research. In January 2007 the American Astronomical Society (AAS) formed a working group to develop and disseminate procedures, criteria, and priorities for identifying, designating, and preserving structures, instruments, and records so that they will continue to be available for astronomical and historical research, for the teaching of astronomy, and for outreach to the general public. The scope of this charge is quite broad, encompassing astronomical structures ranging from archaeoastronomical sites to modern observatories; papers of individual astronomers, observatories and professional journals; observing records; and astronomical instruments themselves. Reflecting this wide scope, the members of the working group include historians of astronomy, practicing astronomers and observatory directors, and specialists Oak Ridge National Laboratory; Santa encounters tight security during in astronomical instruments, archives, and archaeology. a wartime visit to Oak Ridge. Many more images recently donated by the Digital Photo Archive, Department of Energy appear on page 13 and The first item on the working group’s agenda was to determine through out this newsletter. -
Walls of Resonance: Institutional History and the Buildings of the University of Manchester
Walls of resonance: institutional history and the buildings of the University of Manchester James Sumner Corrected pre-print draft, October 2012. Lacks images which appeared in the final version. If citing this work formally, please use the version published: Studies in History and Philosophy of Science, Part A, 44(4), December 2013, 700-715, doi 10.1016/j.shpsa.2013.07.014. Why talk about walls? A wide range of research since the 1990s has focused on the material and spatial character of laboratories, museums, hospitals and other sites of science. Historians, geographers, ethnographers and others have traced how spatial arrangement and presentation have been influenced by, and have themselves influenced, the character of research, teaching, and communication with external audiences of various kinds.1 This paper addresses specifically how these insights may be used to let buildings stand for ideas – how the history of an institution or a discipline (known, for the most part, from established documentary sources) may be articulated through its material fabric. Over the past few years, I have led walking tours around the University of Manchester campus for a variety of audiences including undergraduate and graduate students, adult learners enrolled on the University’s former Courses for the Public programme, and members of the public attending events advertised as part of the annual Manchester Science Festival. Related work, developed with my colleagues at the Centre for the History of Science, Technology and Medicine, includes site-based historical survey articles for resources such as the British Society for the History of Science Travel Guide.2 The University has recently endorsed activity in this area through the appointment of Professor John Pickstone as advisor to the institution on its history and heritage. -
How Liquid Helium and Superconductivity Came to Us
IEEE/CSC & ESAS EUROPEAN SUPERCONDUCTIVITY NEWS FORUM (ESNF), No. 16, April 2011 Heike Kamerlingh Onnes and the Road to Liquid Helium Dirk van Delft, Museum Boerhaave – Leiden University e-mail: [email protected] Abstract – I sketch here the scientific biography of Heike Kamerlingh Onnes, who in 1908 was the first to liquefy helium and in 1911 discovered superconductivity. A son of a factory owner, he grew familiar with industrial approaches, which he adopted and implemented in his scientific career. This, together with a great talent for physics, solid education in the modern sense (unifying experiment and theory) proved indispensable for his ultimate successes. Received April 11, 2011; accepted in final form April 19, 2011. Reference No. RN19, Category 11. Keywords – Heike Kamerligh Onnes, helium, liquefaction, scientific biography I. INTRODUCTION This paper is based on my talk about Heike Kamerlingh Onnes (HKO) and his cryogenic laboratory, which I gave in Leiden at the Symposium “Hundred Years of Superconductivity”, held on April 8th, 2011, the centennial anniversary of the discovery. Figure 1 is a painting of HKO from 1905, by his brother Menso, while Figure 2 shows his historically first helium liquefier, now on display in Museum Boerhaave of Leiden University. Fig. 1. Heike Kamerling Onnes (HKO), 1905 painting by his brother Menso. 1 IEEE/CSC & ESAS EUROPEAN SUPERCONDUCTIVITY NEWS FORUM (ESNF), No. 16, April 2011 Fig. 2. HKO’s historical helium liquefier (last stage), now in Museum Boerhaave, Leiden. I will address HKO’s formative years, his scientific mission, the buiding up of a cryogenic laboratory as a direct consequence of this mission, add some words about the famous Leiden school of instrument makers, the role of the Leiden physics laboratory as an international centre of low temperature research, to end with a conclusion.