Nobel Prize In Physics 1952 edward mills purcell Button 1/2 of prize Button USA Button born 1912, died 1997Button CA Harvard University, Cambridge, Massachusetts, USA http://www.cpenet.org.cn/cpe_resource/nobel/nobel1952.html
Extractions: American physicists Edward Mills Purcell and Harold Ewan discover electromagnetic radiation from interstellar hydrogen at a radio wavelength of 21 cm. Purcell and Felix Bloch independently develop the analytical technique of magnetic resonance spectroscopy for which both receive the 1952 Nobel Prize for physics. British-born American astronomer Eleanor Margaret Burbidge, Geoffrey Burbidge, American nuclear physicist William Alfred Fowler and English astronomer, cosmologist and astrophysicist Fred Hoyle show how stars create heavy elements. Margaret Burbidge, known for her work on the composition of the interior of stars, will direct the Greenwich Royal Observatory 1972-1973. Fowler will share a 1983 Nobel Prize for research on the evolution of stars. Hoyle proposes that eleven elements, including the heaviest, are produced from hydrogen.
Electron Magnetic Resonance Felix Bloch and edward mills purcell were awarded the Nobel Prize for Physics in1952 for their development of new methods for nuclear magnetic precision http://www.chm.bris.ac.uk/emr/History/bloch.htm
Extractions: The first successful nuclear magnetic resonance experiments in solid (parrafin wax) and liquid phases (water) were carried out independently at the end of 1945 respectively by Purcell, Torrey and Pound and by Bloch, Hansen and Packard. Felix Bloch is now remembered largely for his macroscopic phenomenological description of the magnetic properties of the atomic nucleus. This allowed him to develop a theory of nuclear induction which is particularly well suited to the study of transient effects, at the same time it is broadly consistent with a quantum theoretical treatment for systems in a steady state. Bloch's method was to derive expressions for the real and imaginary parts of the nuclear magnetic susceptibility. The Bloch Equations must still be studied by every serious student of NMR or EMR, they apply as well to the nucleus as to the electron. In recent years they have achieved even more prominence with the development of NMR based medical scanners (MRI)- see the selective slice simulation applet Felix Bloch and Edward Mills Purcell were awarded the Nobel Prize for Physics in 1952 "for their development of new methods for nuclear magnetic precision measurements and discoveries in connection therewith" Zavoisky was overlooked, and EMR missed out!
Nobel Prize Winners In Physics purcell, edward mills, USA, Harvard University, Cambridge, MA, * 1912. for theirdevelopment of new methods for nuclear magnetic precision measurements http://www.slcc.edu/schools/hum_sci/physics/whatis/nobel.html
Extractions: Nobel Prize Winners in Physics R~NTGEN, WILHELM CONRAD, Germany, Munich University,* 1845, + 1923: "in recognition of the extraordinary services he has rendered by the discovery of the remarkable rays subsequently named after him". The prize was awarded jointly to: LORENTZ, HENDRIK ANTOON, the Netherlands, Leyden University, * 1853, + 1928; and ZEEMAN, PIETER, the Netherlands, Amsterdam University, * 1865, + 1943: "in recognition of the extraordinary service they rendered by their researches into the influence of magnetism upon radiation phenomena". The prize was divided, one half being awarded to: BECQUEREL, ANTOINE HENRI, France, äcole Polytechnique, Paris, * 1852, + 1908: "in recognition of the extraordinary services he has rendered by his discovery of spontaneous radioactivity"; the other half jointly to: CURIE, PIERRE, France, äcole municipale de physique et de chimie industrielles, (Municipal School of Industrial Physics and Chemistry), Paris, * 1859, + 1906; and his wife CURIE, MARIE, n»e SKLODOWSKA, France, * 1867 (in Warsaw, Poland), + 1934: "in recognition of the extraordinary services they have rendered by their joint researches on the radiation phenomena discovered by Professor Henri Becquerel".
Radar purcell.gif (6314 bytes) edward mills purcell (19121997) grew up in a smallIllinois town where his father managed the local office of the telephone http://www.ee.umd.edu/~taylor/Electrons6.htm
Extractions: A Thumbnail History of Electronics VI. Radar R obert Alexander Watson-Watt (1892-1973), a descendant of James Watt, received a degree in Electrical Engineering from the University of St. Andrews, Scotland and in 1915 began a career in the British civil service, He patented his first radio location device, a device for locating atmospheric discharges, in 1919. In 1935, he received his eleventh radio-location patent, a device for detecting and locating an approaching aircraft. In the following years he was the leader of the intensive development of aircraft radio-location, the secret weapon of the Battle of Britain. In 1937, before the war began, Watson-Watt and his wife undertook the dangerous task of traveling disguised as ordinary tourists through Germany, searching for signs of German radar stations. A lfred Lee Loomis (1887-1975), a graduate of Yale and Harvard Law School, was called "the last of the great amateurs of science". Loomis made a fortune on Wall Street and used his wealth to play host at his estate to famous physicists and to finance a private electronics laboratory; he had already built a working low-power CW radar for aircraft detection when the British brought the magnetron to the U.S. in 1940. In the following months, Loomis helped found the Radiation Laboratory and became head of the Microwave Committee of the National Defense Research Committee. In 1940, Loomis conceived the idea of a precision long-range radio navigation system, Loran. By 1942, the first Loran system, operating at 1.95 MHz, was operating along the East Coast and was used to direct surface vehicles the location of aircraft attacking submarines. Loomis is also credited for conceiving the conical scan system for automatic radar tracking of targets.
Everything Quests: The Nobel Prize Winners@Everything2.com edward mills purcell. edward M. purcell. edward M. purcell s life shines as anexample of the good one man can bring to humanity through his research. http://www.everything2.com/index.pl?node_id=1469898
Nat' Academies Press, Biographical Memoirs V.78 (2000) 166181, edward mills purcell, pp. 182-205, Reed Clark Rollins, pp. 206-221,Stanley Schachter, pp. 222-235, Glenn Theodore Seaborg, pp. http://www.nap.edu/openbook/030907035X/html/
Extractions: Openbook Linked Table of Contents Front Matter, pp. i-viii Robert Cooley Elderfield, pp. 1-15 Gertrude B. Elion, pp. 16-29 Edward Vaughan Evarts, pp. 30-43 Edward C. Franklin, pp. 44-63 Clifford Grobstein, pp. 64-93 Jerome Clarke Hunsaker, pp. 94-107 Philip F. Low, pp. 108-127 Robert Franklin Mehl, pp. 128-145 Robert Sanderson Mulliken, pp. 146-165 William D. Phillips, pp. 166-181 Edward Mills Purcell, pp. 182-205 Reed Clark Rollins, pp. 206-221 Stanley Schachter, pp. 222-235 Glenn Theodore Seaborg, pp. 236-257 George Frederick Sprague, pp. 258-275 Robert Julius Trumpler, pp. 276-297 George Wald, pp. 298-317 John C. Warner, pp. 318-333 Jerome Bert Wiesner, pp. 334-353 Alfred P. Wolf, pp. 354-367
Nat' Academies Press, Biographical Memoirs V.78 (2000) Biographical Memoirs VOLUME 78 edward mills purcell August 30, 1912March 7,1997 BY ROBERT V. POUND edward mills purcell, Nobel laureate for physics in http://www.nap.edu/books/030907035X/html/182.html
Extractions: Openbook Linked Table of Contents Front Matter, pp. i-viii Robert Cooley Elderfield, pp. 1-15 Gertrude B. Elion, pp. 16-29 Edward Vaughan Evarts, pp. 30-43 Edward C. Franklin, pp. 44-63 Clifford Grobstein, pp. 64-93 Jerome Clarke Hunsaker, pp. 94-107 Philip F. Low, pp. 108-127 Robert Franklin Mehl, pp. 128-145 Robert Sanderson Mulliken, pp. 146-165 William D. Phillips, pp. 166-181 Edward Mills Purcell, pp. 182-205 Reed Clark Rollins, pp. 206-221 Stanley Schachter, pp. 222-235 Glenn Theodore Seaborg, pp. 236-257 George Frederick Sprague, pp. 258-275 Robert Julius Trumpler, pp. 276-297 George Wald, pp. 298-317 John C. Warner, pp. 318-333 Jerome Bert Wiesner, pp. 334-353 Alfred P. Wolf, pp. 354-367
IFMBE News: January 2004 and edward mills purcell was awarded a Nobel Prize in Physics in 1952. edward purcell was also investigating the interaction of an NMR machine in http://ifmbe-news.iee.org/ifmbe-news/jan2004/editorial.html
Extractions: In 2003, the Nobel Prize in Physiology or Medicine was awarded jointly to Paul C Lauterbur and Peter Mansfield for their discoveries concerning "magnetic resonance imaging" . As a biomedical engineer and, if you allow me, a scientist, I was glad and proud that these two excellent researchers and scientists received this prize, generally considered as the most important in the world of science, for their contribution to medical science through their pioneering work that includes a lot of basic science and engineering knowledge. Their efforts resulted in one of the probably most complicated, but also most useful non-invasive devices ever developed for the research of living tissue. Biomedical engineering is an interdisciplinary field of science that increases knowledge in engineering, medicine and biology, and contributes to human health and wellbeing through activities such as research, development and applications, that integrate engineering with biomedical and basic life sciences but also with clinical practice. Therefore, I must mention that, in addition to the Nobel Prize in Medicine, this year is rich with awards to scientists whose field of interest and discoveries are very close to biomedical engineering. The decision of the Royal Swedish Academy of Sciences to award the Nobel Prize in Chemistry in 2003 "for discoveries concerning channels in cell membranes"
EXPLORIT Science Center 1912, purcell, edward mills. 1912, RMS Titanic. 1912, Seaborg, Glen Theodore.1912, Turing, Alan Mathison. 1912, Wu, ChienShiun http://www.explorit.org/book/BOSDscientists.html
Extractions: useful resource today Birth Year Last Name Other names 15th Century da Vinci Leonardo Copernicus Nicolas 16th Century Fuchs Leonhart Mercator Gerardus Vesalius Andreas Gilbert William Brahe Tycho Bacon Francis Galilei Galileo Kepler Johannes Harvey William 17th Century Fermat Pierre de Torricelli Evangelista Grimaldi Francesco Maria Picard Jean Pascal Blaise Sydenham Thomas Boyle Robert Malpighi Marcello Ray John Huygens Christiaan Leeuwenhoek Antony van Wren Christopher Hooke Robert Steno Nicolaus Newton Isaac Flamsteed John Papin Denis Lancisi Giovanni Maria Halley Edmund Newcomen Thomas Hales Stephen Reaumur Rene Antoine Ferchault de Taylor Brook Fahrenheit Gabriel Maupertius Pierre Louis Moreau de Bernoulli Daniel 18th Century Celsius Anders Artedi Petrus Chatelet Emilie du Franklin Benjamin Euler Leonhard Linnaeus Carl Vaucanson Jacques de D'Alembert Jean le Rond Agnesi Maria Gaetana Macquer Pierre Joseph Hutton James Boulton Matthew Spallanzani Lazarro Wedgewood Josiah Cavendish Henry Darwin Erasmus Arkwright Richad Wilcke Johan Carl Priestley Joseph Bergman Torbern Olaf Watt James Galvani Luigi Herschel William Withering William Young Arthur Scheele Carl Wilhelm Cartwright Edmund Klaproth Martin Heinrich Lavoisier Antoine Laurent Lamarck Jean Baptiste Montgolfier Jacques-Etienne Volta Alessandro Charles Jacques Alexandre Cesar Curtis William Monge Gaspard Delambre Jean Baptiste Joseph Jenner Edward Herschel Caroline Fourcroy Antoine Francoise de Chaptal Jean Antoine Claude Telford Thomas Whitney Eli Dalton John Malthus
Low Temperature Physics, Superconductivity (high And Low Tc), Etc. 1952 Felix Bloch Nuclear magnetic precision methods edward mills purcell 1953Frits Zernike Phasecontrast microscope 1954 Max Born Fundamental research http://www.faqs.org/faqs/physics-faq/part1/section-21.html
Extractions: Usenet FAQs Search Web FAQs ... RFC Index 1] The Theory of Quantum Liquids, by D. Pines and P. Nozieres 2] Superconductivity of Metals and Alloys, P. G. DeGennes A classic introduction. 3] Theory of Superconductivity, J. R. Schrieffer 4] Superconductivity, M. Tinkham 5] Experimental techniques in low-temperature physics / by Guy K. White. This is considered by many as a "bible" for those working in experimental low temperature physics. Thanks to the contributors who made this compilation possible, including, but not limited to olivers@physics.utoronto.ca cpf@alchemy.ithaca.NY.US glowboy@robot.nuceng.ufl.edu jgh1@iucf.indiana.edu , p675cen@mpifr-bonn. mpg.de, ted@physics.Berkeley.EDU Jeremy_Caplan@postoffice.brown.edu baez@ucrmath.UCR.EDU greason@ptdcs2.intel.com ... roberts@alpha.brooks.af.mil , rev@NBSENH.BITNET, cotera@aspen.uml.edu panetta@cithe503.cithep.caltech.edu johncobb@emx.cc.utexas.edu , exunikh @exu.ericsson.se, bergervo@prl.philips.nl
MSN Encarta - Purcell, Edward Mills Translate this page purcell, edward mills (Taylorville, Illinois 1912 Cambridge, Massachusets 1997),fisico statunitense Trova altre informazioni su purcell, edward mills http://it.encarta.msn.com/encyclopedia_981528868/Purcell_Edward_Mills.html
SETI Article: SETI Horn Of Plenty purcell, edward mills and Harold I. Ewen, Observations of a line in the galacticradio spectrum. Nature 168356, 1951. Silver, Samuel, Microwave Antenna http://www.setileague.org/articles/horn.htm
Extractions: Executive Director, The SETI League, Inc. Presented at , Trenton NJ USA, April 2003 ABSTRACT The parabolic reflector has, since the days of Reber, been the antenna of choice for amateur radio astronomers. Project Argus participants are no exception, typically employing discarded backyard satellite TV dishes of three to five meters in diameter. Such antennas perform well, but their size, as well as complications of municipal zoning restrictions, preclude their use by many a potential Argonaut. This article presents construction and performance details of an alternative Argus antenna, a portable waveguide horn reminiscent of the one used by Ewen in 1951 to first detect the 21 cm radiation signature of interstellar hydrogen. Producing +19 to +21 dBi of gain across the 1200 - 1700 MHz band, the SETI Horn of Plenty rises to the challenge of mapping galactic hydrogen. It also performs well in monitoring the Sun, the Moon, natural radio sources in Cygnus, Cassiopeia, Taurus, and Sagittarius, and (maybe, some day) in detecting ETI. INTRODUCTION Project Argus, a major scientific endeavor of the nonprofit SETI League, Inc., is an attempt to coordinate a global network of amateur radio telescopes in conducting an all-sky survey for microwave emissions of intelligent extraterrestrial origin. Though the holy grail of SETI (the Search for Extra-Terrestrial Intelligence) remains the detection of unambiguous evidence of other technological civilizations in the cosmos, Project Argus participants are also applying their amateur radio telescopes to the challenges of studying natural astrophysical phenomena through their microwave emissions.
Nobel Prizes Indeed the first Director General, Felix Bloch, was awarded the 1952 Nobel prizewith edward mills purcell, for their development of new methods for nuclear http://public.web.cern.ch/Public/Content/Chapters/AboutCERN/Achievements/NobelPr
Extractions: Home Search SiteMap Contact Us ... One dream of CERN's founders , to achieve European eminence in 'big' science, was realised in 1984, when Carlo Rubbia and Simon Van der Meer received the physics Nobel Prize for 'their decisive contributions to the large project which led to the discovery of the field particles W and Z, communicators of the weak interaction The project was a magnificently executed scheme to collide protons and antiprotons in the existing Super Proton Synchrotron . The experimental results confirmed the unification of weak and electromagnetic forces, the electroweak theory of the Standard Model Less than a decade later, Georges Charpak , a CERN physicist since 1959, received the 1992 physics Nobel for 'his invention and development of particle detectors, in particular the multiwire proportional chamber , a breakthrough in the technique for exploring the innermost parts of matter' . Charpak's multiwire proportional chamber, invented in 1968, and his subsequent developments launched the era of fully electronic particle detection. Charpak's detectors are already used for biological research and could eventually replace photographic recording in applied radio-biology. The increased recording speeds translate into faster scanning and lower body doses in medical diagnostic tools based on radiation or particle beams. The Laboratory not only attracts Nobel Prizes but also Nobel Laureates . Indeed the first Director General
Kalender Translate this page edward mills purcell 84 Jahre, Vereinigte Staaten Physiker (09.12.2001) Inhaltsuchen oben *30 Aug 1912 Taylorville/IL. +7 Mrz 1997 Cambridge/MA. http://www.info-kalender.de/kal/k000830.htm
Index Who S Who In Iowa - 1940 Those For Clinton County, Iowa Byron Russel purcell, John edward purcell, William edward Reid, Lloyd William George David Rich, edward mills Rich, Maurice Eugene Sr. Riedesel, http://ftp.rootsweb.com/pub/usgenweb/ia/clinton/history/index/1940ww.txt.txt
Extractions: Index: Who's Who in Iowa - 1940: those for Clinton County, Iowa Contributed for use in USGenWeb Archives by Annette Lucas ClintonRoots@aol.com Elaine Meis (email: EMEIS@aol.com) has a copy of Who's Who in Iowa 1940, and would be willing to do lookups for people. Here's a list of the people who have bios in Clinton County: Allen, Carl Sperry Armstrong, Charles A. Armstrong, Roscoe Whalen Baade, Henry Babock, Otis Warfield Barker, Arthur Platt Barnard, Thomas Harvie Bather, Leo Herbert Beauchamp, Oda Walter Beeby, Charles William Beil, Reuben Henry Bell, Charles L. Bell, Robert Reid Below, Walter Charles Bickelhaupt, Grover Earl Bloom Joseph A. Book, J. Don Bowerrsox, Fred C. Bragonier, Howard Edgar Buechner, Carl Albert Bulow, Harry Ferdinand Burke, J.C. Buxton, Frank William Buxton, Perry Thomas Cady, Edwin Glen Carroll, William Henry Cartensen, Detlef Christ Chase, Charles Perry Clapp, A.M. Clark, John Calhoun Clark, Lewis Samuel Clarke, Michael J. Claussen, George Collis, Oliver Dallyn Coman, Stephen Conway Cook, Ward W. Corson, George Edward Cummings, William Langdon Curtis, Eugene Judson Curtis, George Lewis Curtis, George Martin Dake, Morgan H. Delaney, Emett Patrick DeMoss, Emmett Murray Derflinger, Lloyd Jackson Dettner, Herman W. Dodge, Ray Dulany, G. William III Dulany, George William Jr. Dunk, Jacob J. Eastland, Warren Charles Eberhart, William E. Jr. Eggers, Walter William Ekstrand, Clarence Albin Ellis, Frank Wolcott Ellison, George M. Ewing, Edwin Finefield, Harvey Francis Floerchinger, John Yvo Franklin, Albert Earl Fulmer, Harrison Clark Gane, Albert Ernest Gault, Andrew William Gmelin, Max Rudolph Guenther, Clayton Arnold Guenther, Henry Halbach, Edward Christian Hancock, Courtland Young Hannaher, Leo Patrick Hansen, Alfred Wilhelm Hansen, Ferdinand George Harrington, Frank Lee Harrington, James Spencer Heiberg, E.C. Henningsen, Otto H. Heusinkveld, Henry John Jr. Higbee, Claude Olen Hobart, Harrison Hughitt Hoffman, Charles Augustus Holleran, Frank Louis Holleran, Paul Burghardt Horstmann, Gustave Adolph Howes, John William Howes, Richard Newton Hoxsey, Thomas Tristram Hullinger, John Dudley Hummelgaard, Simon Thomas Huston, William Robinson Irwin, Harold Leonard Iten, Frank Joseph Iten, Louis Conrad Iten, Louis Franklin Iten, William Harry Jackson, Edward F. Jacobs, Roy Henry Jacobsen, Marvin J. Jacobsen, William Sebastian Jaeger, Henry Bernhard Jaenicke, Kurt Jefferies, Lyle Maynard Johannsen, Emil Johnson, Arthur William Johnson, Carroll Franklin Jowett, John Russell Judd, William Nelson Juhl, Soren Nissen Kaack, Harry Frederick Kamler, Paul Frank Kearney, James Francis King, William Norval Kirby, Adrian Mayo Kleeberger, Fred Reed Kramer, Henry George Krenz, Albert Krukow, Ewald Emil Kruse, Kermit George Kynett, Laurence Edward Ladd, Ernest Everett Ladehoff, Arthur Detlef Ladehoff, Mrs. Leona Lagomarcino, Richard Andrew Lahann, Sophie Dorothea Lohmann, August Carl Lundgren, Donald Albert Luse, Ralph Frank Lyon, Morton McCarthy, John Thomas McCullough, William Armstrong McEleney, Leo Patrick McKinley, Leslie Samuel McLane, Thomas I. McPherson, Donald Beach Machael, Eugene Maegerlein, Marcus C. Maloney, T. Emmett Martin, Hobart Earle Martindale, Edward Lowry Maxheim, John F. Sr. Maxheim, Vincent J. Mayer, Earl Franklin Mayer, Stanley Messer, Oliver Leonard Meyer, Archie Edward Miller, Earnest Leander Minor, Ralph Mockridge,William R. Mona, Fred W. Morgan, Jasper William Moriarty, John James Morris, Walter David Jr. Moses, Oliver Seymour Mueller, John Frederick Muhs, Charles Murphy, Thomas Vincent Myers, George Nantz, Orville Wright Needle, Haskell Cahn Nelson, Grant Newell Nissen, John Henry Nyquist, A. Edward Oakes, William Thomas Ogden, David Batchelder Ogden, Frank Edmond O'Neil, James Wendell Oyaas, Einar Bernhardt Pape, Dillwynne N. Pape, Floyd N. Pape, Harry F.L. Pascal, Aylett Le Varia Pascal, Percival Purcell Paulsen, William Herman Peckham, George Taylor Jr. Peckosh, Frank Stanley Peters, Henry C. Peters, Sample Rex Petersen, Alfred Emil Petersen, Peter Hems Peterson, Lloyd Leonard Petty, Oliver Perry Pinney, Byron Russel Purcell, John Edward Purcell, William Edward Reid, Lloyd William Reynolds, George David Rich, Edward Mills Rich, Maurice Eugene Sr. Riedesel, Mrs. Augusta Matilda Riedesel, Elmer Vinton Ringuette, Arthur Lynzal Root, Aurelius Clark Ross, Arthur James Rowland, Maud Romaine Scanlan, George Cyril Schell, Mayard Marr Schlect, Emil Julian Schlotfeldt, Robert Bruce Schneider, Captain Frank William Schneider, Captain George Henry Schuster, Lester James Schuyler, Andrew Livingston Seaman, Dwight Scott Seaman, Halleck Wager Shannon, Cecil Wesley Sharar, Paul Byron Shelstad, Martin John Shuh, Lewis Edwin Siegmund, Paul Siegmund, William Ferdinand Sino, Henry Andrew Slocum, King Darwin Smith, Carl James Smith, George A. Smith, Geoge Morris Smith, Harold Alexander Smith, Herbert Lyle Smith, William Thomas Roy Snyder, Dean Clifford Sorenson, Victor Valentine Stenzel, Martin Carl Stewart, John Brayton Sr. Stoddard, Carrol Nevin Stoner, Rex Richard Sugg, Herbert Reid Sutherland, Lillian Alberta Sutton, Merrit Leofwin Tallman, Roy Elmer Towle, Charles Curtis Towle, Henry Stewart Townsend, Bruce Troeger, Edward Irving Tucker, Charles Francis Van Allen, Frederick Holmes Van Allen, John Bevier Volckmann, Herman J. Volckmann, William J.C. Wagner, Roscoe C. Wagner, Walter Christy Walker, William Henry Ward, Frank J. Warner, Edward Martin White, Lee Francis Whitley, Roy Sumner Whitney, Milton E. Wilkinson, Herbert Ellery Wilson, Frank Eugene Wilson, George E. Wohlenbert, Louis H. Wolfe, John Loyola Work, Ernest Otto Yourd, William John ************************************************************************ USGENWEB ARCHIVES NOTICE: These electronic pages may NOT be reproduced in any format for profit or presentation by any other organization or persons. Persons or organizations desiring to use this material, must obtain the written consent of the contributor, or the legal representative of the submitter, and contact the listed USGenWeb archivist with proof of this consent. The submitter has given permission to the USGenWeb Archives to store the file permanently for free access. http://www.rootsweb.com/~usgenweb ***********************************************************************
THE NOBEL PRIZE IN PHYSICS 1901 RÖNTGEN, WILHELM CONRAD, Germany FELIX, USA, Stanford University, Stanford, CA, * 1905 (in Zürich, Switzerland),+ 1983; and purcell, edward mills, USA, Harvard University, Cambridge, http://felix.unife.it/Root/d-General/d-Physics/t-Nobel-prizes-physics
Extractions: THE NOBEL PRIZE IN PHYSICS 1901 RÖNTGEN, WILHELM CONRAD, Germany, Munich University, * 1845, + 1923: "såsom ett erkännande av den utomordentliga förtjänst han inlagt genom upptäckten av de egendomliga strålar, som sedermera uppkallats efter honom"; "in recognition of the extraordinary services he has rendered by the discovery of the remarkable rays subsequently named after him". THE NOBEL PRIZE IN PHYSICS 1902 The prize was awarded jointly to: LORENTZ, HENDRIK ANTOON, the Netherlands, Leyden University, * 1853, + 1928; and ZEEMAN, PIETER, the Netherlands, Amsterdam University, * 1865, + 1943: "såsom ett erkännande av den utomordentliga förtjänst de inlagt genom sina undersökningar över magnetismens inflytande på strålningsfenomenen"; "in recognition of the extraordinary service they rendered by their researches into the influence of magnetism upon radiation phenomena". THE NOBEL PRIZE IN PHYSICS 1903 The prize was divided, one half being awarded to: BECQUEREL, ANTOINE HENRI, France, École Polytechnique, Paris, * 1852, + 1908: "såsom ett erkännande av den utomordentliga förtjänst han inlagt genom upptäckten av den spontana radioaktiviteten"; "in recognition of the extraordinary services he has rendered by his discovery of spontaneous radioactivity"; the other half jointly to: CURIE, PIERRE, France, École municipale de physique et de chimie industrielles, (Municipal School of Industrial Physics and Chemistry), Paris, * 1859, + 1906; and his wife CURIE, MARIE, née SKLODOWSKA, France, * 1867 (in Warsaw, Poland), + 1934: "såsom ett erkännande av den utomordentliga förtjänst de inlagt genom sina gemensamt utförda arbeten rörande de av Professor Henri Becquerel upptäckta strålningsfenomenen"; "in recognition of the extraordinary services they have rendered by their joint researches on the radiation phenomena discovered by Professor Henri Becquerel". THE NOBEL PRIZE IN PHYSICS 1904 RAYLEIGH, Lord (JOHN WILLIAM STRUTT), Great Britain, Royal Institution of Great Britain, London, * 1842, + 1919: "för hans undersökningar rörande de viktigaste gasernas täthet samt hans i sammanhang med dessa undersökningar gjorda upptäckt av argon"; "for his investigations of the densities of the most important gases and for his discovery of argon in connection with these studies". THE NOBEL PRIZE IN PHYSICS 1905 LENARD, PHILIPP EDUARD ANTON, Germany, Kiel University, * 1862 (in Pressburg, then Hungary), + 1947: "för hans arbeten över katodstrålarna"; "for his work on cathode rays". THE NOBEL PRIZE IN PHYSICS 1906 THOMSON, Sir JOSEPH JOHN, Great Britain, Cambridge University, * 1856, + 1940: "såsom ett erkännande av den stora förtjänst han inlagt genom sina teoretiska och experimentella undersökningar över elektricitetens gång genom gaser"; "in recognition of the great merits of his theoretical and experimental investigations on the conduction of electricity by gases". THE NOBEL PRIZE IN PHYSICS 1907 MICHELSON, ALBERT ABRAHAM , U.S.A., Chicago University, * 1852 (in Strelno, then Germany), + 1931: "för hans optiska precisionsinstrument och hans därmed utförda spektroskopiska och metrologiska undersökningar"; "for his optical precision instruments and the spectroscopic and metrological investigations carried out with their aid". THE NOBEL PRIZE IN PHYSICS 1908 LIPPMANN, GABRIEL, France, Sorbonne University, Paris,* 1845 (in Hollerich, Luxembourg), + 1921: "för hans på interferensfenomenet grundade metod att fotografiskt återgiva färger"; "for his method of reproducing colours photographically based on the phenomenon of interference". THE NOBEL PRIZE IN PHYSICS 1909 The prize was awarded jointly to: MARCONI, GUGLIELMO, Italy, Marconi Wireless Telegraph Co. Ltd., London, Great Britain, * 1874, +1937; and BRAUN, CARL FERDINAND, Germany, Strasbourg University, Alsace (then Germany), * 1850, + 1918: "såsom ett erkännande av deras förtjänster om den trådlösa telegrafiens utveckling"; "in recognition of their contributions to the development of wireless telegraphy". THE NOBEL PRIZE IN PHYSICS 1910 VAN DER WAALS, JOHANNES DIDERIK, the Netherlands, Amsterdam University, * 1837, + 1923: "för hans arbeten angående gasers och vätskors tillståndsekvation"; "for his work on the equation of state for gases and liquids". THE NOBEL PRIZE IN PHYSICS 1911 WIEN, WILHELM, Germany, Würzburg University, * 1864, + 1928: "för hans upptäckter angående värmestrålningens lagar"; "for his discoveries regarding the laws governing the radiation of heat". THE NOBEL PRIZE IN PHYSICS 1912 DALÉN, NILS GUSTAF, Sweden, Swedish Gas-Accumulator Co., Lidingö-Stockholm, * 1869, + 1937: "för hans uppfinningar av självverkande regulatorer att i kombination med gasaccumulatorer användas till belysning av fyrar och lysbojar"; "for his invention of automatic regulators for use in conjunction with gas accumulators for illuminating lighthouses and buoys". THE NOBEL PRIZE IN PHYSICS 1913 KAMERLINGH-ONNES, HEIKE, the Netherlands, Leyden University * 1853, + 1926: "i anledning av hans undersökningar över kroppars egenskaper vid låga temperaturer, vilka bland annat lett till framställningen av flytande helium"; "for his investigations on the properties of matter at low temperatures which led, inter alia to the production of liquid helium". THE NOBEL PRIZE IN PHYSICS 1914 VON LAUE, MAX, Germany, Frankfurt-on-the Main University, * 1879, + 1960: "för hans upptäckt av röntgenstrålarnas diffraktion i kristaller"; "for his discovery of the diffraction of X-rays by crystals". THE NOBEL PRIZE IN PHYSICS 1915 The prize was awarded jointly to: BRAGG, Sir WILLIAM HENRY, Great Britain, London University, * 1862, + 1942; and his son BRAGG, Sir WILLIAM LAWRENCE, Great Britain, Victoria University, Manchester, * 1890 (in Adelaide, Australia), + 1971: "för deras förtjänster om utforskandet av kristallstrukturer medelst röntgenstrålar"; "for their services in the analysis of crystal structure by means of X-rays". THE NOBEL PRIZE IN PHYSICS 1916 Reserved. THE NOBEL PRIZE IN PHYSICS 1917 The prize money for 1916 was allocated to the Special Fund of this prize section. The prize for 1917: Reserved. THE NOBEL PRIZE IN PHYSICS 1918 The prize for 1917: BARKLA, CHARLES GLOVER, Great Britain, Edinburgh University, * 1877, + 1944: "för hans upptäckt av den karakteristiska röntgenstrålningen hos elementen"; "for his discovery of the characteristic Röntgen radiation of the elements". The prize for 1918: Reserved. THE NOBEL PRIZE IN PHYSICS 1919 The prize for 1918: PLANCK, MAX KARL ERNST LUDWIG, Germany, Berlin University, * 1858, + 1947: "såsom ett erkännande av den förtjänst han genom upptäckten av elementarkvanta inlagt om fysikens utveckling"; "in recognition of the services he rendered to the advancement of Physics by his discovery of energy quanta". The prize for 1919: STARK, JOHANNES, Germany, Greifswald University, * 1874, + 1957: "för hans upptäckt av dopplereffekten hos kanalstrålar och av spektrallinjers uppdelning i elektriska fält"; "for his discovery of the Doppler effect in canal rays and the splitting of spectral lines in electric fields". THE NOBEL PRIZE IN PHYSICS 1920 GUILLAUME, CHARLES EDOUARD, Switzerland, Bureau International des Poids et Mesures (International Bureau of Weights and Measures), Sèvres, * 1861, + 1938: "såsom ett erkännande av den förtjänst han genom upptäckten av nickelstållegeringarnas anomalier inlagt om precisionsfysiken"; "in recognition of the service he has rendered to precision measurements in Physics by his discovery of anomalies in nickel steel alloys". THE NOBEL PRIZE IN PHYSICS 1921 Reserved. THE NOBEL PRIZE IN PHYSICS 1922 The prize for 1921: EINSTEIN, ALBERT, Germany and Switzerland, Kaiser-WilhelmInstitut (now Max-Planck-Institut) für Physik, Berlin, * 1879, + 1955: "för hans förtjänster om den teoretiska fysiken, särskilt hans upptäckt av lagen för den fotoelektriska effekten"; "for his services to Theoretical Physics, and especially for his discovery of the law of the photoelectric effect". The prize for 1922: BOHR, NIELS, Denmark, Copenhagen University, * 1885, + 1962: "för hans förtjänster om utforskandet av atomernas struktur och den från dem utgående strålningen"; "for his services in the investigation of the structure of atoms and of the radiation emanating from them". THE NOBEL PRIZE IN PHYSICS 1923 MILLIKAN, ROBERT ANDREWS, U.S.A., California Institute of Technology, Pasadena, CA, * 1868, + 1953: "för hans arbeten rörande den elektriska enhetsladdningen samt den fotoelektriska effekten"; "for his work on the elementary charge of electricity and on the photoelectric effect". THE NOBEL PRIZE IN PHYSICS 1924 Reserved. THE NOBEL PRIZE IN PHYSICS 1925 The prize for 1924: SIEGBAHN, KARL MANNE GEORG, Sweden, Uppsala University, * 1886, + 1978: "för hans röntgenspektroskopiska upptäckter och forskningar"; "for his discoveries and researchin the field of X-ray spectroscopy". The prize for 1925: Reserved. THE NOBEL PRIZE IN PHYSICS 1926 The prize for 1925 was awarded jointly to: FRANCK, JAMES, Germany, Goettingen University, * 1882, + 1964; and HERTZ, GUSTAV, Germany, Halle University, * 1887, + 1975: "med anledning av deras upptäckt av lagarna för stöten mellan en elektron och en atom"; "for their discovery of the laws governing the impact of an electron upon an atom". The prize for 1926: PERRIN, JEAN BAPTISTE, France, Sorbonne University, Paris, * 1870, + 1942: "för hans arbeten rörande materiens diskontinuerliga struktur, särskilt för hans upptäckt av sedimentationsjämvikten"; "for his work on the discontinuous structure of matter, and especially for his discovery of sedimentation equilibrium". THE NOBEL PRIZE IN PHYSICS 1927 The prize was divided equally between: COMPTON, ARTHUR HOLLY, U.S.A., Chicago University, * 1892, + 1962: "för hans upptäckt av den efter honom benämnda effekten"; "for his discovery of the effect named after him"; and WILSON, CHARLES THOMSON REES, Great Britain, Cambridge University, * 1869 (in Glencorse, Scotland), + 1959: "för upptäckten av hans metod att genom ångkondensation göra elektriskt laddade partiklars banor iakttagbara"; "for his method of making the paths of electrically charged particles visible by condensation of vapour". THE NOBEL PRIZE IN PHYSICS 1928 Reserved. THE NOBEL PRIZE IN PHYSICS 1929 The prize for 1928: RICHARDSON, Sir OWEN WILLANS, Great Britain, London University, * 1879, + 1959: "för hans arbeten rörande termjonfenomenet och särskilt för upptäckten av den efter honom benämnda lagen"; "for his work on the thermionic phenomenon and especially for the discovery of the law named after him". The prize for 1929: DE BROGLIE, Prince LOUIS-VICTOR, France, Sorbonne University, Institut Henri Poincaré, Paris, * 1892, + 1987: "för upptäckten av elektronernas vågnatur"; "for his discovery of the wave nature of electrons". THE NOBEL PRIZE IN PHYSICS 1930 RAMAN, Sir CHANDRASEKHARA VENKATA, India, Calcutta University, * 1888, + 1970: "för hans arbeten angående ljusets diffusion och för upptäckten av den efter honom uppkallade effekten"; "for his work on the scattering of light and for the discovery of the effect named after him". THE NOBEL PRIZE IN PHYSICS 1931 Reserved. THE NOBEL PRIZE IN PHYSICS 1932 The prize money for 1931 was allocated to the Special Fund of this prize section. The prize for 1932: Reserved. THE NOBEL PRIZE IN PHYSICS 1933 The prize for 1932: HEISENBERG, WERNER, Germany, Leipzig University, * 1901, + 1976: "för uppställande av kvantmekaniken, vars användning bl.a. lett till upptäckten av vätets allotropa former"; "for the creation of quantum mechanics, the applica-tion of which has, inter alia, led to the discovery of the allotropic forms of hydrogen". The prize for 1933 was awarded jointly to: SCHRÖDINGER, ERWIN, Austria, Berlin University, Germany, * 1887, + 1961; and DIRAC, PAUL ADRIEN MAURICE, Great Britain, Cambridge University, * 1902, + 1984: "för upptäckandet av nya fruktbärande former av atomteorien"; "for the discovery of new productive forms of atomic theory". THE NOBEL PRIZE IN PHYSICS 1934 Reserved. THE NOBEL PRIZE IN PHYSICS 1935 The prize money for 1934 was with 1/3 allocated to the Main Fund and with 2/3 to the Special Fund of this prize section. The prize for 1935: CHADWICK, Sir JAMES, Great Britain, Liverpool University, * 1891, + 1974: "för upptäckten av neutronen"; "for the discovery of the neutron". THE NOBEL PRIZE IN PHYSICS 1936 The prize was divided equally between: HESS, VICTOR FRANZ, Austria, Innsbruck University, * 1883, + 1964: "för upptäckten av den kosmiska strålningen"; "for his discovery of cosmic radiation"; and ANDERSON, CARL DAVID, U.S.A., California Institute of Technology, Pasadena, CA, * 1905, + 1991: "för upptäckten av positronen"; "for his discovery of the positron". THE NOBEL PRIZE IN PHYSICS 1937 The prize was awarded jointly to: DAVISSON, CLINTON JOSEPH, U.S.A., Bell Telephone Laboratories, New York, NY, * 1881, + 1958; and THOMSON, Sir GEORGE PAGET, Great Britain, London Universi ty, * 1892, + 1975: "för den experimentella upptäckten av interferensfenomenet vid kristallers bestrålning med elektroner"; "for their experimental discovery of the diffraction of electrons by crystals". THE NOBEL PRIZE IN PHYSICS 1938 FERMI, ENRICO, Italy, Rome University, * 1901, + 1954: "för hans påvisande av nya radioaktiva grundämnen, framställda genom neutronbestrålning, och hans i anslutning därtill gjorda upptäckt av kärnreaktioner, åstadkomna genom långsamma neutroner"; "for his demonstrations of the existence of new radioactive elements produced by neutron irradiation, and for his related discovery of nuclear reactions brought about by slow neutrons". THE NOBEL PRIZE IN PHYSICS 1939 LAWRENCE, ERNEST ORLANDO, U.S.A., University of California, Berkeley, CA, * 1901, + 1958: "för uppfinningen av cyklotronen, dess utveckling och med densamma vunna resultat, särskilt beträffande artificiellt radioaktiva element"; "for the invention and development of the cyclotron and for results obtained with it, especially with regard to artifi cial radioactive elements". THE NOBEL PRIZE IN PHYSICS 1940 The prize money was with 1/3 allocated to the Main Fund and with 2/3 to the Special Fund of this prize section. THE NOBEL PRIZE IN PHYSICS 1941 The prize money was with 1/3 allocated to the Main Fund and with 2/3 to the Special Fund of this prize section. THE NOBEL PRIZE IN PHYSICS 1942 The prize money was with 1/3 allocated to the Main Fund and with 2/3 to the Special Fund of this prize section. THE NOBEL PRIZE IN PHYSICS 1943 Reserved. THE NOBEL PRIZE IN PHYSICS 1944 The prize for 1943: STERN, OTTO, U.S.A., Carnegie Institute of Technology, Pittsburg, PA, * 1888 (in Sorau, then Germany), + 1969: "för hans bidrag till utveckling av molekylstrålemetoden och upptäckten av protonens magnetiska moment"; "for his contribution to the development of the molecular ray method and his discovery of the magnetic moment of the proton". The prize for 1944: RABI, ISIDOR ISAAC, U.S.A., Columbia University, New York, NY, * 1898, (in Rymanow, then Austria-Hungary) + 1988: "för den av honom angivna resonansmetoden för registrering av atomkärnans magnetiska egenskaper"; "for his resonance method for recording the magnetic properties of atomic nuclei". THE NOBEL PRIZE IN PHYSICS 1945 PAULI, WOLFGANG, Austria, Princeton University, NJ, U.S.A., * 1900, + 1958: "för upptäckten av uteslutningsprincipen, även benämnd Pauliprincipen"; "for the discovery of the Exclusion Principle, also called the Pauli Principle". THE NOBEL PRIZE IN PHYSICS 1946 BRIDGMAN, PERCY WILLIAMS, U.S.A., Harvard University, Cambridge, MA, * 1882, + 1961: "för uppfinningen av en apparatur för åstadkommande av extremt höga tryck för de upptäckter han med densamma gjort inom området för de höga tryckens fysik"; "for the invention of an apparatus to produce extremely high pressures, and for the discoveries he made therewith in the field of high pressure physics". THE NOBEL PRIZE IN PHYSICS 1947 APPLETON, Sir EDWARD VICTOR, Great Britain, Department of Scientific and Industrial Research, London, * 1892, + 1965: "för hans arbeten rörande atmosfärens fysik, särskilt för upptäckten av det s.k. 'Appletonskiktet'"; "for his investigations of the physics of the upper atmosphere especially for the discovery of the so-called Appleton layer". THE NOBEL PRIZE IN PHYSICS 1948 BLACKETT, Lord PATRICK MAYNARD STUART, Great Britain, Victoria University, Manchester, * 1897, + 1974: "för hans utveckling av Wilsonmetoden och hans därmed gjorda upptäckter inom kärnfysiken och rörande den kosmiska strålningen"; "for his development of the Wilson cloud chamber method, and his discoveries therewith in the fields of nuclear physics and cosmic radiation". THE NOBEL PRIZE IN PHYSICS 1949 YUKAWA, HIDEKI, Japan, Kyoto Imperial University and Columbia University, New York, NY, U.S.A., * 1907, + 1981: "för hans på grundval av teoretiska arbeten rörande kärnkrafterna gjorda förutsägelse av mesonernas existens"; "for his prediction of the existence of mesons on the basis of theoretical work on nuclear forces". THE NOBEL PRIZE IN PHYSICS 1950 POWELL, CECIL FRANK, Great Britain, Bristol University, * 1903, + 1969: "för hans utveckling av den fotografiska metoden för studiet av kärnprocesser och hans därvid gjorda upptäckter rörande mesonerna"; "for his development of the photographic method of studying nuclear processes and his discoveries regarding mesons made with this method". THE NOBEL PRIZE IN PHYSICS 1951 The prize was awarded jointly to: COCKCROFT, Sir JOHN DOUGLAS, Great Britain, Atomic Energy Research Establishment, Harwell, Didcot, Berks., * 1897, + 1967; and WALTON, ERNEST THOMAS SINTON, Ireland, Dublin University, * 1903: "för deras pionjärarbete vid genomförandet av kärnomvandlingar medelst artificiellt accelererade partiklar"; "for their pioneer work on the transmutation of atomic nuclei by artificially acce lerated atomic particles". THE NOBEL PRIZE IN PHYSICS 1952 The prize was awarded jointly to: BLOCH, FELIX, U.S.A., Stanford University, Stanford, CA, * 1905 (in Zürich, Switzerland), + 1983; and PURCELL, EDWARD MILLS, U.S.A., Harvard University, Cambridge, MA, * 1912: "för deras utveckling av nya metoder för kärnmagnetiska precisionsmätningar och därmed gjorda upptäckter"; "for their development of new methods for nuclear magnetic precision measurements and discove ries in connection therewith". THE NOBEL PRIZE IN PHYSICS 1953 ZERNIKE, FRITS (FREDERIK), the Netherlands, Groningen University, * 1888, + 1966: "för den av honom angivna faskontrastmetoden, särskilt för hans uppfinning av faskontrastmikroskopet"; "for his demonstration of the phase contrast method, especially for his invention of the phase contrast microscope". THE NOBEL PRIZE IN PHYSICS 1954 The prize was divided equally between: BORN, MAX, Great Britain, Edinburgh University, * 1882 (in Breslau, then Germany), + 1970: "för hans grundläggande arbeten inom kvantmekaniken, särskilt hans statistiska tolkning av vågfunktionen"; "for his fundamental research in quantum mechanics, especially for his statistical interpretation of the wavefunction"; and BOTHE, WALTHER, Germany, Heidelberg University, Max-Planck Institut (former Kaiser-Wilhelm-Institut) für medizinische Forschung, Heidelberg, * 1891, + 1957: "för koincidensmetoden och hans därmed gjorda upptäckter"; "for the coincidence method and his discoveries made therewith". THE NOBEL PRIZE IN PHYSICS 1955 The prize was divided equally between: LAMB, WILLIS EUGENE, U.S.A., Stanford University, Stanford, CA, * 1913: "för hans upptäckter rörande finstrukturen i vätets spektrum"; "for his discoveries concerning the fine structure of the hydrogen spectrum"; and KUSCH, POLYKARP, U.S.A., Columbia University, New York, NY, * 1911 (in Blankenburg, then Germany), + 1993: "för hans precisionsbestämning av elektronens magnetiska moment"; "for his precision determination of the magnetic moment of the electron". THE NOBEL PRIZE IN PHYSICS 1956 The prize was awarded jointly, one third each, to: SHOCKLEY, WILLIAM, U.S.A., Semiconductor Laboratory of Beckman Instruments, Inc., Mountain View, CA, * 1910 (in London, Great Britain), + 1989; BARDEEN, JOHN, U.S.A., University of Illinois, Urbana, IL, * 1908, + 1991; and BRATTAIN, WALTER HOUSER, U.S.A., Bell Telephone Laboratories, Murray Hill, NJ, * 1902, + 1987: "för deras undersökningar över halvledare och upptäckt av transistor effekten"; "for their researches on semiconductors and their discovery of the transistor effect". THE NOBEL PRIZE IN PHYSICS 1957 The prize was awarded jointly to: YANG, CHEN NING, China, Institute for Advanced Study, Princeton, NJ, U.S.A., * 1922; and LEE, TSUNG-DAO, China, Columbia University, New York, NY, U.S.A., *1926: "för deras djupgående undersökning av de s.k. paritetslagarna, vilken har lett till viktiga upptäckter rörande elementarpartiklarna"; "for their penetratinginvestigation of the so-called parity laws which has led to important discoveries regarding the elementary partic les". THE NOBEL PRIZE IN PHYSICS 1958 The prize was awarded jointly to: CHERENKOV, PAVEL ALEKSEYEVICH, USSR, Physics Institute of USSR Academy of Sciences, Moscow, *1904, + 1990; FRANK, IL'JA MIKHAILOVICH, USSR, University of Moscow and Physics Institute of USSR Academy of Sciences, Moscow, * 1908, + 1990; and TAMM, IGOR YEVGENYEVICH, USSR, University of Moscow and Physics Institute of USSR Academy of Scien-ces, Moscow, * 1885, + 1971: "för upptäckten och tolkningen av Cherenkoveffekten"; "for the discovery and the interpretation of the Cherenkov effect". THE NOBEL PRIZE IN PHYSICS 1959 The prize was awarded jointly to: SEGRÈ, EMILIO GINO, U.S.A., University of California, Berkeley, CA, * 1905 (in Tivoli, Italy), + 1989; and CHAMBERLAIN, OWEN, U.S.A., University of California, Berkeley, CA, * 1920: "för deras upptäckt av antiprotonen"; "for their discovery of the antiproton". THE NOBEL PRIZE IN PHYSICS 1960 GLASER, DONALD A., U.S.A., University of California, Berkeley, CA, * 1926: "för uppfinningen av bubbelkammaren"; "for the invention of the bubble chamber". THE NOBEL PRIZE IN PHYSICS 1961 The prize was divided equally between: HOFSTADTER, ROBERT, U.S.A., Stanford University, Stanford, CA, * 1915, + 1990: "för hans banbrytande undersökningar över elektronspridningen mot atomkärnor och därvid gjorda upptäckter rörande nukleonernas struktur"; "for his pioneering studies of electron scattering in atomic nuclei and for his thereby achieved discoveries concerning the stucture of the nucleons"; and MÖSSBAUER, RUDOLF LUDWIG, Germany, Technische Hochschule, Munich, and California Institute of Technology, Pasadena, CA, U.S.A., * 1929: "för hans undersökningar rörande gammastrålningens resonansabsorption och därvid gjorda upptäckt av den efter honom benämnda effekten"; "for his researches concerning the resonance absorption of gamma radiation and his discovery in this connection of the effect which bears his name". THE NOBEL PRIZE IN PHYSICS 1962 LANDAU, LEV DAVIDOVICH, USSR, Academy of Sciences, Moscow, * 1908, + 1968: "för hans banbrytande teorier för kondenserad materia, särskilt flytande helium"; "for his pioneering theories for condensed matter, especially liquid helium". THE NOBEL PRIZE IN PHYSICS 1963 The prize was divided, one half being awarded to: WIGNER, EUGENE P., U.S.A., Princeton University, Princeton, NJ, * 1902 (in Budapest, Hungary), U 1995: "för hans insatser inom teorien för atomkärnorna och elementarpartiklarna, särskilt genom upptäckten och tillämpningen av fundamentala symmetriprinciper"; "for his contributions to the theory of the atomic nucleus and the elementary particles, particularly through the discovery and application of fundamental symmetry principles"; and the other half jointly to: GOEPPERT-MAYER, MARIA, U.S.A., University of California, La Jolla, CA, * 1906 (in Kattowitz, then Germany), + 1972; and JENSEN, J. HANS D., Germany, University of Heidelberg, * 1907, + 1973: "för deras upptäckter beträffande atomkärnornas skalstruktur"; "for their discoveries concerning nuclear shell structure". THE NOBEL PRIZE IN PHYSICS 1964 The prize was divided, one half being awarded to: TOWNES, CHARLES H., U.S.A., Massachusetts Institute of Technology (MIT) , Cambridge, MA, * 1915; and the other half jointly to: BASOV, NICOLAY GENNADIYEVICH, USSR, Lebedev Institute for Physics, Akademija Nauk, Moscow, * 1922; and PROKHOROV, ALEKSANDR MIKHAILOVICH, USSR, Lebedev Institute for Physics, Akademija Nauk, Moscow, * 1916: "för grundläggande arbeten inom kvantelektroniken, som lett till framställning av oscillatorer och förstärkare enligt maser-laserprincipen"; "for fundamental work in the field of quantum electronics, which has led to the construction of oscillators and amplifiers based on the maser-laser principle". THE NOBEL PRIZE IN PHYSICS 1965 The prize was awarded jointly to: TOMONAGA, SIN-ITIRO, Japan, Tokyo, University of Education, Tokyo, * 1906, + 1979; SCHWINGER, JULIAN, U.S.A., Harvard University, Cambridge, MA, * 1918, U 1994; and FEYNMAN, RICHARD P., U.S.A., California Institute of Technology, Pasadena, CA, * 1918, + 1988: "för deras fundamentala insats inom kvantelektrodynamiken, med djupgående konsekvenser för elementarpartikelfysiken"; "for their fundamental work in quantum electrodynamics, with deep-ploughing consequences for the physics of elementary particles". THE NOBEL PRIZE IN PHYSICS 1966 KASTLER, ALFRED, France, École Normale Supérieure, Université de Paris, * 1902, + 1984: "för upptäckt och utveckling av optiska metoder för studiet av hertzska resonanser i atomer"; "for the discovery and development of optical methods for studying hertzian resonances in atoms". THE NOBEL PRIZE IN PHYSICS 1967 BETHE, HANS ALBRECHT, U.S.A., Cornell University, Ithaca, NY, * 1906 (in Strasbourg, then Germany): "för hans insatser inom teorien för kärnreaktioner, särskilt hans upptäckter rörande energialstringen i stjärnorna"; "for his contributions to the theory ofnuclear reactions, especially his discoveries concerning the energy production in stars". THE NOBEL PRIZE IN PHYSICS 1968 ALVAREZ, LUIS W., U.S.A., University of California, Berkeley, CA, * 1911, + 1988: "för hans avgörande insatser inom elementarpartikelfysiken, särskilt upptäckten av ett stort antal resonanstillstånd, möjliggjord genom hans utveckling av tekniken med vätebubbelkammare och dataanalys"; "for his decisive contributions to elementary particle physics, in particular the discovery of a large number of resonance states, made possible through his development of the technique of using hydrogen bubble chamber and data analysis". THE NOBEL PRIZE IN PHYSICS 1969 GELL-MANN, MURRAY, U.S.A., California Institute of Technology, Pasadena, CA, * 1929: "för hans bidrag och upptäckter beträffande klassificeringen av elementarpartiklarna och deras växelverkan"; "for his contributions and discoveries concerning the classification of elementary particles and their interactions". THE NOBEL PRIZE IN PHYSICS 1970 The prize was divided equally between: ALFVÉN, HANNES, Sweden, Royal Institute of Technology, Stockholm, * 1908, U 1995: "för grundläggande insatser och upptäckter inom magnetohydrodynamiken med fruktbärande tillämpningar inom olika områden av plasmafysiken"; "for fundamental work and discoveries in magneto-hydrodynamics with fruitful applications in different parts of plasma physics"; and NÉEL, LOUIS, France, University of Grenoble, Grenoble, * 1904: "för grundläggande insatser och upptäckter rörande antiferromagnetism och ferrimagnetism som lett till betydelsefulla tillämpningar inom det fasta tillståndets fysik"; "for fundamental work and discoveries concerning antiferromagnetism and ferrimagnetism which have led to important applications in solid state physics". THE NOBEL PRIZE IN PHYSICS 1971 GABOR, DENNIS, Great Britain, Imperial College of Science and Technology, London, * 1900 (in Budapest, Hungary), + 1979: "för hans uppfinning och utveckling av den holografiska metoden"; "for his invention and development of the holographic method". THE NOBEL PRIZE IN PHYSICS 1972 The prize was awarded jointly to: BARDEEN, JOHN, U.S.A., University of Illinois, Urbana, IL, * 1908, + 1991; COOPER, LEON N., U.S.A., Brown University, Providence, RI, * 1930; and SCHRIEFFER, J. ROBERT, U.S.A., University of Pennsylvania, Philadelphia, PA, * 1931: "för den av dem gemensamt utvecklade teorien för supraledningsfenomenet, vanligen kallad BCS-teorien"; "for their jointly developed theory of superconductivity, usually called the BCS-theory". THE NOBEL PRIZE IN PHYSICS 1973 The prize was divided, one half being equally shared between: ESAKI, LEO, Japan, IBM Thomas J. Watson Research Center, Yorktown Heights, NY, U.S.A., * 1925; and GIAEVER, IVAR, U.S.A., General Electric Company, Schenectady, NY, * 1929 (in Bergen, Norway), "för deras experimentella upptäckter rörande tunnelfenomenet i halvledare, respektive supraledare"; "for their experimental discoveries regarding tunneling phenomena in semiconductors and superconductors, respectively", and the other half to: JOSEPHSON, BRIAN D., Great Britain, Cambridge University, Cambridge, * 1940: "för hans teoretiska förutsägelser av egenskaperna hos en supraström genom en tunnelbarriär, särskilt de fenomen vilka allmänt benämnas Josephson-effekterna"; "for his theoretical predictions of the properties of a supercurrent through a tunnel barrier, in particular those phenomena which are generally known as the Josephson effects". THE NOBEL PRIZE IN PHYSICS 1974 The prize was awarded jointly to: RYLE, Sir MARTIN, Great Britain, Cambridge University, Cambridge, * 1918, + 1984; and HEWISH, ANTONY, Great Britain, Cambridge University, Cambridge, * 1924: "för deras banbrytande arbeten inom radioastrofysiken: Ryle för hans observationer och uppfinningar, särskilt apertursyntestekniken, och Hewish för hans avgörande insatser vid upptäckten av pulsarerna"; "for their pioneering research in radio astrophysics: Ryle for his observations and inventions, in particular of the aperture synthesis technique, and Hewish for his decisive role in the discovery of pulsars". THE NOBEL PRIZE IN PHYSICS 1975 The prize was awarded jointly to: BOHR, AAGE, Denmark, Niels Bohr Institute, Copenhagen, * 1922; MOTTELSON, BEN, Denmark, Nordita, Copenhagen, * 1926 (in Chicago, U.S.A.); and RAINWATER, JAMES, U.S.A., Columbia University, New York, NY, * 1917, + 1986: "för upptäckten av sambandet mellan kollektiva rörelser och partikelrörelser i atomkärnor, samt den därpå baserade utvecklingen av teorien för atomkärnans struktur"; "for the discovery of the connection between collective motion and particle motion in atomic nuclei and the development of the theory of the structure of the atomic nucleus based on this connection". THE NOBEL PRIZE IN PHYSICS 1976 The prize was divided equally between: RICHTER, BURTON, U.S.A., Stanford Linear Accelerator Center, Stanford, CA, * 1931; TING, SAMUEL C. C., U.S.A., Massachusetts Institute of Technology (MIT), Cambridge, MA, (European Center for Nuclear Research, Geneva, Switzerland), * 1936: "för deras ledande insatser vid upptäckten av en tung elementarpartikel av nytt slag"; "for their pioneering work in the discovery of a heavy elementary particle of a new kind". THE NOBEL PRIZE IN PHYSICS 1977 The prize was divided equally between: ANDERSON, PHILIP W., U.S.A., Bell Laboratories, Murray Hill, NJ, * 1923; MOTT, Sir NEVILL F., Great Britain, Cambridge University, Cambridge, * 1905; and VAN VLECK, JOHN H., U.S.A., Harvard University, Cambridge, MA, * 1899, + 1980: "för deras grundläggande teoretiska insatser rörande elektronstrukturen i magnetiska och oordnade system"; "for their fundamental theoretical investigations of the electronic structure of magnetic and disordered systems". THE NOBEL PRIZE IN PHYSICS 1978 The prize was divided, one half being awarded to: KAPITSA, PYOTR LEONIDOVICH, USSR, Academy of Sciences, Moscow, * 1894, + 1984: "för hans grundläggande uppfinningar och upptäckter inom lågtemperaturfysiken"; "for his basic inventions and discoveries in the area of low-temperature physics"; and the other half divided equally between: PENZIAS, ARNO A., U.S.A., Bell Laboratories, Holmdel, NJ, * 1933 (in Munich, Germany); and WILSON, ROBERT W., U.S.A., Bell Laboratories, Holmdel, NJ, * 1936: "för deras upptäckt av den kosmiska bakgrunden av mikrovågor"; "for their discovery of cosmic microwave background radiation". THE NOBEL PRIZE IN PHYSICS 1979 The prize was divided equally between: GLASHOW, SHELDON L., U.S.A., Lyman Laboratory, Harvard University, Cambridge, MA, * 1932; SALAM, ABDUS, Pakistan, International Centre for Theoretical Physics, Trieste, and Imperial College of Science and Technology, London, Great Britain, * 1926; and WEINBERG, STEVEN, U.S.A., Harvard University, Cambridge, MA, * 1933: "för deras insatser inom teorin för förenad svag och elektromagnetisk växelverkan mellan elementar partiklar, innefattande bl.a. förutsägelsen av den svaga neutrala strömmen"; "for their contributions to the theory of the unified weak and electromagnetic interaction between elementary particles, including inter alia the prediction of the weak neutral current". THE NOBEL PRIZE IN PHYSICS 1980 The prize was divided equally between: CRONIN, JAMES, W., U.S.A., University of Chicago, Chicago, IL, * 1931; and FITCH, VAL L., U.S.A., Princeton University, Princeton, NJ, * 1923: "för upptäckten av brott mot fundamentala symmetriprinciper i neutrala K-mesoners sönderfall"; "for the discovery of violations of fundamental symmetry principles in the decay of neutral K-mesons". THE NOBEL PRIZE IN PHYSICS 1981 The prize was awarded by one half jointly to: BLOEMBERGEN, NICOLAAS, U.S.A., Harvard University, Cambridge, MA, * 1920 (in the Netherlands); and SCHAWLOW, ARTHUR L., U.S.A., Stanford University, Stanford, CA, * 1921: "för deras bidrag till utvecklingen av laserspektroskopien"; "for their contribution to the development of laser spectroscopy"; and the other half to: SIEGBAHN, KAI M., Sweden, Uppsala University, Uppsala, * 1918: "för hans bidrag till utvecklingen av den högupplösande elektronspektroskopien"; "for his contribution to the development of high- resolution electron spectroscopy". THE NOBEL PRIZE IN PHYSICS 1982 WILSON, KENNETH G., U.S.A., Cornell University, Ithaca, NY, * 1936: "för hans teori för kritiska fenomen vid fasomvandlingar"; "for his theory for critical phenomena in connection with phase transitions". THE NOBEL PRIZE IN PHYSICS 1983 The prize was awarded by one half to: CHANDRASEKHAR, SUBRAMANYAN, U.S.A., University of Chicago, Chicago, IL, * 1910 (in Lahore, India): "för hans teoretiska studier av de fysikaliska processer, som är av betydelse för stjärnornas struktur och utveckling"; "for his theoretical studies of the physical processes of importance to the structure and evolution of the stars". and by the other half to: FOWLER, WILLIAM A., U.S.A., California Institute of Technology, Pasadena, CA, * 1911, U 1995: "för hans teoretiska och experimentella studier av de kärnreaktioner, som är av betydelse för de kemiska elementens bildning i universum"; "for his theoretical and experimental studies of the nuclear reactions of importance in the formation of the chemical elements in the universe". THE NOBEL PRIZE IN PHYSICS 1984 The prize was awarded jointly to: RUBBIA, CARLO, Italy, CERN, Geneva, Switzerland, * 1934; and VAN DER MEER, SIMON, the Netherlands, CERN, Geneva, Switzerland, * 1925: "för deras avgörande insatser i det stora projekt, som lett till upptäckten av fältpartiklarna W och Z, förmedlare av svag växelverkan"; "for their decisive contributions to the large project, which led to the discovery of the field particles W and Z, communicators of weak interaction". THE NOBEL PRIZE IN PHYSICS 1985 VON KLITZING, KLAUS, Federal Republic of Germany, Max-PlanckInstitute for Solid State Research, Stuttgart, * 1943: "för upptäckten av den kvantiserade Halleffekten"; "for the discovery of the quantized Hall effect". THE NOBEL PRIZE IN PHYSICS 1986 The prize was awarded by one half to: RUSKA, ERNST, Federal Republic of Germany, Fritz- Haber-Institut der Max-Planck-Gesellschaft, Berlin, * 1906, + 1988: "för hans fundamentala elektronoptiska arbeten och konstruktionen av det första elektronmikroskopet"; "for his fundamental work in electron optics, and for the design of the first electron microscope". and the other half jointly to: BINNIG, GERD, Federal Republic of Germany, IBM Zürich Research Laboratory, Rüschlikon, Switzerland, * 1947; and ROHRER, HEINRICH, Switzerland, IBM Zürich Research Laboratory, Rüschlikon, Switzerland, * 1933: "för deras konstruktion av sveptunnelmikroskopet"; "for their design of the scanning tunneling microscope". THE NOBEL PRIZE IN PHYSICS 1987 The prize was awarded jointly to: BEDNORZ, J. GEORG, Federal Republic of Germany, IBM Research Laboratory, Rüschlikon, Switzerland, * 1950; and MÜLLER, K. ALEXANDER, Switzerland, IBM Research Laboratory, Rüschlikon, Switzerland, * 1927: "för deras banbrytande upptäckt av supraledning i keramiska material"; "for their important breakthrough in the discovery of superconductivity in ceramic materials". THE NOBEL PRIZE IN PHYSICS 1988 The prize was awarded jointly to: LEDERMAN, LEON M., U.S.A., Fermi National Accelerator Laboratory, Batavia, IL, * 1922; SCHWARTZ, MELVIN, U.S.A., Digital Pathways, Inc., Mountain View, CA, * 1932; and STEINBERGER, JACK, U.S.A., CERN, Geneva, Switzerland, * 1921 (in Bad Kissingen, FRG): "för metoden med neutrinostrålar och påvisandet av leptonernas dubblettstruktur genom upptäckten av myonneutrinon"; "for the neutrino beam method and the demonstration of the doublet structure of the leptons through the discovery of the muon neutrino". THE NOBEL PRIZE IN PHYSICS 1989 The prize was awarded by one half to: RAMSEY, NORMAN F., U.S.A., Harvard University, Cambridge, MA, * 1915: "för uppfinningen av metoden med separerade oscillerande fält och dess användning i vätemasern och andra atomklockor"; "for the invention of the separated oscillatory fields method and its use in the hydrogen maser and other atomic clocks". and the other half jointly to: DEHMELT, HANS G., U.S.A., University of Washington, Seattle, WA, * 1922 (in Görlitz, Germany); and PAUL, WOLFGANG, Federal Republic of Germany, University of Bonn, Bonn, * 1913, U 1993: "för utvecklingen av jonfälletekniken"; "for the development of the ion trap technique". THE NOBEL PRIZE IN PHYSICS 1990 The prize was awarded jointly to: FRIEDMAN, JEROME I., U.S.A., Massachusetts Institute of Technology, Cambridge, MA, * 1930; KENDALL, HENRY W., U.S.A., Massachusetts Institute of Technology, Cambridge, MA, * 1926; and TAYLOR, RICHARD E., Canada, Stanford University, Stanford, CA, U.S.A., * 1929: "för deras banbrytande undersökningar rörande starkt inelastisk spridning av elektroner mot protoner och bundna neutroner, vilka haft en avgörande betydelse för utvecklingen av kvarkmodellen inom partikelfysiken"; "for their pioneering investigations concerning deep inelastic scattering of electrons on protons and bound neutrons, which have been of essential importance for the development of the quark model in particle physics". THE NOBEL PRIZE IN PHYSICS 1991 de GENNES, PIERRE-GILLES, France, Collège de France, Paris, * 1932: "för upptäckten att metoder, som utvecklats för att beskriva ordning i enkla system, kan generaliseras till att gälla mer komplicerade former av materia, särskilt flytande kristaller och polymerer"; "for discovering that methods developed for studying order phenomena in simple systems can be generalized to more complex forms of matter, in particular to liquid crystals and polymers". THE NOBEL PRIZE IN PHYSICS 1992 CHARPAK, GEORGES, France, École Supérieure de Physique et Chimie, Paris and CERN, Geneva, Switzerland, * 1924 ( in Poland): "för hans uppfinning och utveckling av partikeldetektorer, särskilt flertrådsproportionalkammaren"; "for his invention and development of particle detectors, in particular the multiwire proportional chamber". THE NOBEL PRIZE IN PHYSICS 1993 The prize was awarded jointly to: HULSE, RUSSELL A., U.S.A., Princeton University, Princeton, NJ, * 1950, and TAYLOR Jr., JOSEPH H., U.S.A., Princeton University, Princeton, NJ, * 1941: "för upptäckten av en ny typ av pulsar, en upptäckt som öppnat nya möjligheter för studiet av gravitationen"; "for the discovery of a new type of pulsar, a discovery that has opened up new possibilities for the study of gravitation". THE NOBEL PRIZE IN PHYSICS 1994 The prize was awarded "för pionjärinsatser vid utvecklingen av neutronspridningsmetoder för studier av kondenserad materia"; "for pioneering contributions to the development of neutron scattering techniques for studies of condensed matter" by one half to: BROCKHOUSE, BERTRAM N., Canada, McMaster University, Hamilton, Ontario, * 1918: "för utveckling av neutronspektroskopin"; "for the development of neutron spectroscopy" and by the other half to: SHULL, CLIFFORD G., U.S.A., Massachusetts Institute of Technology, Cambridge, MA, * 1915: "för utveckling av neutrondiffraktionstekniken"; "for the development of the neutron diffraction technique".
St. John's 1885-86 [QRS] Pearce Aubyn, agent coastal steamer, house Rennie s Mill road Pearson Eli,engineer, 15 West street purcell edward, sanitary department, 23 Maxse street http://genealogy.nlpubliclibraries.ca/directories/1885/pages/stjohns-opq.htm
Asbestos Lawyers Brayton Purcell: Asbestos Lung Cancer Case Brayton purcell, Lawyers for People, specializing in asbestos and personal edward Jones was first exposed to asbestos while working at a steel mill in http://www.braytonlaw.com/news/verdicts/2003jones.htm
Extractions: Our Court Record Trial Verdicts Appeals For Our Clients Practice Areas Our Court Record In the News ... Trial Verdicts San Francisco Jury Awards Over $5 Million San Francisco, CA Edward Jones was first exposed to asbestos while working at a steel mill in Colorado when he was 16 years old. He was involved in the cleanup of insulation debris during piping and furnace repairs. He joined the United States Navy in 1950, serving as an apprentice machinist and machinist mate on the USS Juneau during the Korean War and aboard various other vessels until the early 1960s. Mr. Jones maintained and repaired equipment, including valves, pumps, turbines and auxiliary equipment during these early years of his Navy career. He was routinely exposed to insulation, packing and gaskets containing asbestos. In 1978, Mr. Jones retired from the Navy as an officer in the shipbuilding division and received an honorable discharge. He then worked with Lockheed Shipbuilding in Washington state until 1985 supervising the construction of Navy submarine tenders. During this period, he was intermittently exposed to asbestos from the use of asbestos packing and gaskets.