Radioactivity and X-Rays
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© in This Web Service Cambridge University
Cambridge University Press 978-1-107-64247-8 - Fellows of Trinity College, Cambridge Compiled by H. McLeod Innes Index More information FELLOWS 1561 AND LATER Peter Kapitza 1925 Charles Alfred Coulson 1934 Francis Crawford Burkitt 26 Douglas Edward Lea 34 Alexander Pearce Higgins 26 John Enoch Powell 34 Robert Mantle Rattenbury 26 Eduard David Mortier Fraenkel 34 Llewellyn Hilleth Thomas 26 Hans Arnold Heilbronn 35 James Cochran Stevenson Arthur John Terence Dibben Runciman 27, 32 Wisdom 35 Francis Henry Sandbach 27 Hugh Cary Gilson 35 Arthur Geoffrey Neale Cross 27 Nathaniel Mayer Victor Reginald Pepys Winnington- Rothschild 35 Ingram 28 David Arthur Gilbert Hinks 35 Norman Adrian de Bruyne 28 Harry Work Melville 35 William Leonard Edge 28 Alan Lloyd Hodgkin 36 Carl Frederick Abel Pantin 29 Thomas Thomson Paterson 36 Maurice Black 29, 34 Arthur Dale Trendall (el. 1936) 37 Norman Feather 29, 36 Arthur Christopher Moule 37 John Arthur Gaunt 29 Maurice Henry Lecorney Harold Douglas Ursell 29 Pryce (el. 1936) 37 Arthur Harold John Knight 30 Gerald Salmon Gough 37 John Waddingham Brunyate 30 Douglas William Logan 37 Louis Harold Gray 30 Clement Henry Bamford 37 Raymond Edward Alan Victor Gordon Kiernan 37 Christopher Paley 30 Douglas Malcolm Aufrere Patrick Du Val 30 Leggett 37 Abram Samoilovitch John Sinclair Morrison 37 Besicovitch 30 William Albert Hugh Rushton 38 Ludwig Josef Johann John Michal Kenneth Vyvyan 38 Wittgenstein 30, 39 Denis John Bauer 38 Frederick George Mann 31 Eric Russell Love 38 Laurence Chisholm Young 31 William Charles Price 38 Harold Scott Macdonald Coxeter 31 Michael Grant 38 Walter Hamilton 31 Piero Sraffa 39 Anthony Frederick Blunt 32 Gordon Leonard Clark 39 Harold Davenport 32 Mark Gillachrist Marlborough Glenn Allan Millikan (el. -
Stable Isotopes of Cobalt Properties of Cobalt
Stable Isotopes of Cobalt Isotope Z(p) N(n) Atomic Mass Natural Abundance Nuclear Spin Co-59 27 32 58.93320 100.00% 7/2- Cobalt was discovered in 1735 by Georg Brandt. Its name derives from the German word kobald, meaning "goblin" or "evil spirit." Minerals containing cobalt were used by the early civilizations of Egypt and Mesopotamia for coloring glass deep blue. Cobalt oxide is used today to add a pink or blue color to glass. It is also an important trace element in soils and necessary for animal nutrition. The most important modern use of cobalt is in the manufacture of various wear-resistant and superalloys. Its alloys have shown high resistance to corrosion and oxidation at high temperatures. Radioactive Cobalt-60 is used in radiography and in the sterilization of food. A silvery-white, shining, hard, ductile, somewhat malleable metal, cobalt is also ferromagnetic, with permeability two-thirds that of iron. It has exceptional magnetic properties in alloys. It is attached by dilute hydrochloric and sulfuric acids. It corrodes readily in air, and it has unusual coordinating properties, especially the trivalent ion. It is noncombustible except in powder form. Cobalt occurs in two allotropic modifications over a wide range of temperatures: the crystalline close-packed- hexagonal form is known as the alpha form, which turns into the beta (or gamma) form above 417 ºC. In finely powdered form, cobalt ignites spontaneously in air. Reactions with acetylene and bromine pentafluoride proceed to incandescence and can become violent. The metal is moderately toxic by ingestion. Inhalation of dusts can damage lungs. -
Glossary Derived From: Human Research Program Integrated Research Plan, Revision A, (January 2009)
Glossary derived from: Human Research Program Integrated Research Plan, Revision A, (January 2009). National Aeronautics and Space Administration, Johnson Space Center, Houston, Texas 77058, pages 232-280. Report No. 153: Information Needed to Make Radiation Protection Recommendations for Space Missions Beyond Low-Earth Orbit (2006). National Council on Radiation Protection and Measurements, pages 309-318. Reprinted with permission of the National Council on Radiation Protection and Measurements, http://NCRPonline.org . Managing Space Radiation Risk in the New Era of Space Exploration (2008). Committee on the Evaluation of Radiation Shielding for Space Exploration, National Research Council. National Academies Press, pages 111-118. -A- AAPM: American Association of Physicists in Medicine. absolute risk: Expression of excess risk due to exposure as the arithmetic difference between the risk among those exposed and that obtaining in the absence of exposure. absorbed dose (D): Average amount of energy imparted by ionizing particles to a unit mass of irradiated material in a volume sufficiently small to disregard variations in the radiation field but sufficiently large to average over statistical fluctuations in energy deposition, and where energy imparted is the difference between energy entering the volume and energy leaving the volume. The same dose has different consequences depending on the type of radiation delivered. Unit: gray (Gy), equivalent to 1 J/kg. ACE: Advanced Composition Explorer Mission, launched in 1997 and orbiting the L1 libration point to sample energetic particles arriving from the Sun and interstellar and galactic sources. It also provides continuous coverage of solar wind parameters and solar energetic particle intensities (space weather). When reporting space weather, it can provide an advance warning (about one hour) of geomagnetic storms that can overload power grids, disrupt communications on Earth, and present a hazard to astronauts. -
Royal Society of Chemistry Input to the Ad Hoc Nuclear
ROYAL SOCIETY OF CHEMISTRY INPUT TO THE AD HOC NUCLEAR RESEARCH AND DEVELOPMENT ADVISORY BOARD The Royal Society of Chemistry (RSC) was pleased to hear of the instigation of the Ad Hoc Nuclear Research and Development Advisory Board (the Board) following the findings of the House of Lords Science and Technology Committee Inquiry ‘Nuclear Research and Development Capabilities’.1,2 The RSC is the largest organisation in Europe for advancing the chemical sciences. Supported by a network of 47,000 members worldwide and an internationally acclaimed publishing business, its activities span education and training, conferences and science policy, and the promotion of the chemical sciences to the public. This document represents the views of the RSC. The RSC has a duty under its Royal Charter "to serve the public interest" by acting in an independent advisory capacity, and it is in this spirit that this submission is made. To provide input to the Board the RSC has performed a wide consultation with the chemical science community, including members of both our Radiochemistry and Energy Sector Interest Groups and also our Environment Sustainability and Energy Division. September 2012 The Role of Chemistry in a Civil Nuclear Strategy 1 Introduction Chemistry and chemical knowledge is essential in nuclear power generation and nuclear waste management. It is essential that a UK civil nuclear strategy recognises the crucial role that chemistry plays, both in research and innovation and in the development of a strong skills pipeline. As the RSC previously articulated in our response to the House of Lords Inquiry, 3 nuclear power is an important component of our current energy mix. -
Peer Review Draft Synthesis and Assessment Product 4.2 Thresholds
1 Peer Review Draft 2 Synthesis and Assessment Product 4.2 3 Thresholds of Change in Ecosystems 4 Authors: Daniel B. Fagre (lead author), Colleen W. Charles, Craig 5 D. Allen, Charles Birkeland, F. Stuart Chapin, III, Peter M. 6 Groffman, Glenn R. Guntenspergen, Alan K. Knapp, A. David 7 McGuire, Patrick J. Mulholland, Debra P.C. Peters, Daniel D. 8 Roby, and George Sugihara 9 Contributing authors: Brandon T. Bestelmeyer, Julio L. 10 Betancourt, Jeffrey E. Herrick, and Douglas S. Kenney 11 U.S. Climate Change Science Program 12 Draft 5.0 SAP 4.2 9/26/2008 1 1 Table of Contents 2 Executive Summary............................................................................................................ 5 3 Introduction................................................................................................................... 5 4 Definitions.....................................................................................................................5 5 Development of Threshold Concepts............................................................................ 6 6 Principles of Thresholds ............................................................................................... 7 7 Case Studies.................................................................................................................. 8 8 Potential Management Responses............................................................................... 10 9 Recommendations...................................................................................................... -
Cherenkov Radiation
TheThe CherenkovCherenkov effecteffect A charged particle traveling in a dielectric medium with n>1 radiates Cherenkov radiation B Wave front if its velocity is larger than the C phase velocity of light v>c/n or > 1/n (threshold) A β Charged particle The emission is due to an asymmetric polarization of the medium in front and at the rear of the particle, giving rise to a varying electric dipole momentum. dN Some of the particle energy is convertedγ = 491into light. A coherent wave front is dx generated moving at velocity v at an angle Θc If the media is transparent the Cherenkov light can be detected. If the particle is ultra-relativistic β~1 Θc = const and has max value c t AB n 1 cosθc = = = In water Θc = 43˚, in ice 41AC˚ βct βn 37 TheThe CherenkovCherenkov effecteffect The intensity of the Cherenkov radiation (number of photons per unit length of particle path and per unit of wave length) 2 2 2 2 2 Number of photons/L and radiation d N 4π z e 1 2πz 2 = 2 1 − 2 2 = 2 α sin ΘC Wavelength depends on charge dxdλ hcλ n β λ and velocity of particle 2πe2 α = Since the intensity is proportional to hc 1/λ2 short wavelengths dominate dN Using light detectors (photomultipliers)γ = sensitive491 in 400-700 nm for an ideally 100% efficient detector in the visibledx € 2 dNγ λ2 d Nγ 2 2 λ2 dλ 2 2 11 1 22 2 d 2 z sin 2 z sin 490393 zz sinsinΘc photons / cm = ∫ λ = π α ΘC ∫ 2 = π α ΘC 2 −− 2 = α ΘC λ1 λ1 dx dxdλ λ λλ1 λ2 d 2 N d 2 N dλ λ2 d 2 N = = dxdE dxdλ dE 2πhc dxdλ Energy loss is about 104 less hc 2πhc than 2 MeV/cm in water from € -
*Revelle, Roger Baltimore 18, Maryland
NATIONAL ACADEMY OF SCIENCES July 1, 1962 OFFICERS Term expires President-Frederick Seitz June 30, 1966 Vice President-J. A. Stratton June 30, 1965 Home Secretary-Hugh L. Dryden June 30, 1963 Foreign Secretary-Harrison Brown June 30, 1966 Treasurer-L. V. Berkner June 30, 1964 Executive Officer Business Manager S. D. Cornell G. D. Meid COUNCIL *Berkner L. V. (1964) *Revelle, Roger (1965) *Brown, Harrison (1966) *Seitz, Frederick (1966) *Dryden, Hugh L. (1963) *Stratton, J. A. (1965) Hutchinson, G. Evelyn (1963) Williams, Robley C. (1963) *Kistiakowsky, G. B. (1964) Wood, W. Barry, Jr. (1965) Raper, Kenneth B. (1964) MEMBERS The number in parentheses, following year of election, indicates the Section to which the member belongs, as follows: (1) Mathematics (8) Zoology and Anatomy (2) Astronomy (9) Physiology (3) Physics (10) Pathology and Microbiology (4) Engineering (11) Anthropology (5) Chemistry (12) Psychology (6) Geology (13) Geophysics (7) Botany (14) Biochemistry Abbot, Charles Greeley, 1915 (2), Smithsonian Institution, Washington 25, D. C. Abelson, Philip Hauge, 1959 (6), Geophysical Laboratory, Carnegie Institution of Washington, 2801 Upton Street, N. W., Washington 8, D. C. Adams, Leason Heberling, 1943 (13), Institute of Geophysics, University of Cali- fornia, Los Angeles 24, California Adams, Roger, 1929 (5), Department of Chemistry and Chemical Engineering, University of Illinois, Urbana, Illinois Ahlfors, Lars Valerian, 1953 (1), Department of Mathematics, Harvard University, 2 Divinity Avenue, Cambridge 38, Massachusetts Albert, Abraham Adrian, 1943 (1), 111 Eckhart Hall, University of Chicago, 1118 East 58th Street, Chicago 37, Illinois Albright, William Foxwell, 1955 (11), Oriental Seminary, Johns Hopkins University, Baltimore 18, Maryland * Members of the Executive Committee of the Council of the Academy. -
Nuclear Power
No.59 z iii "Ill ~ 2 er0 Ill Ill 0 Nuclear Family Pia nning p3 Chernobyl Broadsheet ·, _ I. _ . ~~~~ George Pritchar d speaks CONTENTS COMMENT The important nuclear development since the Nuclear Family Planning 3 last SCRAM Journal was the Government's The CEGB's plans, and the growing opposition, after Sizewell B by go ahead for Sizewell B: the world's first HUGH RICHARDS. reactor order since Chernobyl, and Britain's News 4-6 first since the go ahead was given to Torness Accidents Will Happen 1 and Heysham 2 in 1978. Of great concern is Hinkley Seismic Shocker 8-9 the CEGB's announced intention to build "a A major article on seismic safety of nuclear plants in which JAMES small fanilty• of PWRs, starting with Hinkley GARRETT reveals that Hinkley Point C. At the time of the campaign In the Point sits on a geological fault. south west to close the Hinkley A Magnox Trouble at Trawsfynydd 10-11 station, and .a concerted push in Scotland to A summary of FoE's recent report on increasing radiation levels from prevent the opening of Torness, another Trawsfynydd's by PATRICK GREEN. nuclear announcement is designed to divide Pandora's POX 12 and demoralise the opposition. But, it should The debate over plutonium transport make us more determined. The article on the to and from Dounreay continues by facing page gives us hope: the local PETE MUTTON. authorities on Severnside are joining forces CHERNOBYL BROADSHEET to oppose Hinkley C, and hopefully they will Cock-ups and Cover-ups work closely with local authorities in other "Sacrificed to • • • Nuclear Power" threatened areas - Lothian Region, The Soviet Experience Northumberland, the County Council Coalition "An Agonising Decision• 13 against waste dumping and the Nuclear Free GEORGE PRITCHARD explains why Zones - to formulate a national anti-nuclear he left Greenpeoce and took a job strategy. -
Annual Report 1951 National Bureau of Standards
Annual Report 1951 National Bureau of Standards Miscellaneous Publication 204 UNITED STATES DEPARTMENT OF COMMERCE Charles Sawyer, Secretary NATIONAL BUREAU OF STANDARDS A. V. Astint, Director Annual Report 1951 National Bureau of Standards For sale by the Superintendent of Documents, U. S. Government Printing Office Washington 2 5, D. C. Price 50 cents CONTENTS Page 1. General Review 1 2. Electricity 16 Beam intensification in a high-voltage oscillograph 17, Low-temperature dry cells 17, High-rate batteries 17, Battery additives 18. 3. Optics and Metrology 18 The kinorama 19, Measurement of visibility for aircraft 20, Antisubmarine aircraft searchlights 20, Resolving power chart 20, Refractivity 21, Thermal expansivity of aluminum alloys 21. 4. Heat and Power . 21 Thermodynamic properties of materials 22, Synthetic rubber and other high polymers 23, Combustors for jet engines 24, Temperature and composition of flames 25, Engine "knock" 25, Low-temperature physics 26, Medical physics instrumentation 28. 5. Atomic and Radiation Physics 28 Atomic standard of length 29, Magnetic moment of the proton 29, Spectra of artificial elements 31, Photoconductivity of semiconductors 31, Radiation detecting instruments 32, Protection against radiation 32, X-ray equipment 33, Atomic and molecular ions 35, Electron physics 35, Tables of nuclear data 35, Atomic energy levels 36. 6. Chemistry 36 Radioactive carbohydrates 36, Dextran as a substitute for blood plasma 37, Acidity and basicity in organic solvents 37, Interchangeability of fuel gases 38, Los Angeles "smog" 39, Infrared spectra of alcohols 39, Electrodeposi- tion 39, Development of analytical methods 40, Physical constants 42. 7. Mechanics 42 Turbulent flow 43, Turbulence at supersonic speeds 43, Dynamic properties of materials 43, High-frequency vibrations 44, Hearing loss 44, Physical properties by sonic methods 44, Water waves 46, Density currents 46, Precision weighing 46, Viscosity of gases 46, Evaporated thin films 47. -
Named Units of Measurement
Dr. John Andraos, http://www.careerchem.com/NAMED/Named-Units.pdf 1 NAMED UNITS OF MEASUREMENT © Dr. John Andraos, 2000 - 2013 Department of Chemistry, York University 4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to [email protected] http://www.chem.yorku.ca/NAMED/ Atomic mass unit (u, Da) John Dalton 6 September 1766 - 27 July 1844 British, b. Eaglesfield, near Cockermouth, Cumberland, England Dalton (1/12th mass of C12 atom) Dalton's atomic theory Dalton, J., A New System of Chemical Philosophy , R. Bickerstaff: London, 1808 - 1827. Biographical References: Daintith, J.; Mitchell, S.; Tootill, E.; Gjersten, D ., Biographical Encyclopedia of Dr. John Andraos, http://www.careerchem.com/NAMED/Named-Units.pdf 2 Scientists , Institute of Physics Publishing: Bristol, UK, 1994 Farber, Eduard (ed.), Great Chemists , Interscience Publishers: New York, 1961 Maurer, James F. (ed.) Concise Dictionary of Scientific Biography , Charles Scribner's Sons: New York, 1981 Abbott, David (ed.), The Biographical Dictionary of Scientists: Chemists , Peter Bedrick Books: New York, 1983 Partington, J.R., A History of Chemistry , Vol. III, Macmillan and Co., Ltd.: London, 1962, p. 755 Greenaway, F. Endeavour 1966 , 25 , 73 Proc. Roy. Soc. London 1844 , 60 , 528-530 Thackray, A. in Gillispie, Charles Coulston (ed.), Dictionary of Scientific Biography , Charles Scribner & Sons: New York, 1973, Vol. 3, 573 Clarification on symbols used: personal communication on April 26, 2013 from Prof. O. David Sparkman, Pacific Mass Spectrometry Facility, University of the Pacific, Stockton, CA. Capacitance (Farads, F) Michael Faraday 22 September 1791 - 25 August 1867 British, b. -
Sterns Lebensdaten Und Chronologie Seines Wirkens
Sterns Lebensdaten und Chronologie seines Wirkens Diese Chronologie von Otto Sterns Wirken basiert auf folgenden Quellen: 1. Otto Sterns selbst verfassten Lebensläufen, 2. Sterns Briefen und Sterns Publikationen, 3. Sterns Reisepässen 4. Sterns Züricher Interview 1961 5. Dokumenten der Hochschularchive (17.2.1888 bis 17.8.1969) 1888 Geb. 17.2.1888 als Otto Stern in Sohrau/Oberschlesien In allen Lebensläufen und Dokumenten findet man immer nur den VornamenOt- to. Im polizeilichen Führungszeugnis ausgestellt am 12.7.1912 vom königlichen Polizeipräsidium Abt. IV in Breslau wird bei Stern ebenfalls nur der Vorname Otto erwähnt. Nur im Emeritierungsdokument des Carnegie Institutes of Tech- nology wird ein zweiter Vorname Otto M. Stern erwähnt. Vater: Mühlenbesitzer Oskar Stern (*1850–1919) und Mutter Eugenie Stern geb. Rosenthal (*1863–1907) Nach Angabe von Diana Templeton-Killan, der Enkeltochter von Berta Kamm und somit Großnichte von Otto Stern (E-Mail vom 3.12.2015 an Horst Schmidt- Böcking) war Ottos Großvater Abraham Stern. Abraham hatte 5 Kinder mit seiner ersten Frau Nanni Freund. Nanni starb kurz nach der Geburt des fünften Kindes. Bald danach heiratete Abraham Berta Ben- der, mit der er 6 weitere Kinder hatte. Ottos Vater Oskar war das dritte Kind von Berta. Abraham und Nannis erstes Kind war Heinrich Stern (1833–1908). Heinrich hatte 4 Kinder. Das erste Kind war Richard Stern (1865–1911), der Toni Asch © Springer-Verlag GmbH Deutschland 2018 325 H. Schmidt-Böcking, A. Templeton, W. Trageser (Hrsg.), Otto Sterns gesammelte Briefe – Band 1, https://doi.org/10.1007/978-3-662-55735-8 326 Sterns Lebensdaten und Chronologie seines Wirkens heiratete. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,