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Development of an On-Line Fuel Failure Monitoring System For
DEVELOPMENT OF AN ON-LINE FUEL FAILURE MONITORING SYSTEM FOR CANDU REACTORS DEVELOPPEMENT D'UN SYSTEME DE SURVEILLANCE EN LIGNE POUR DES RUPTURES DE GAINES DES REACTEURS CANDU A Thesis Submitted to the Division of Graduate Studies of the Royal Military College of Canada by Stephen Jason Livingstone, BSc, MSc Sub-Lieutenant In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy March 2012 ©This thesis may be used within the Department of National Defence but copyright for open publication remains the property of the author. Library and Archives Bibliotheque et Canada Archives Canada Published Heritage Direction du Branch Patrimoine de I'edition 395 Wellington Street 395, rue Wellington Ottawa ON K1A0N4 Ottawa ON K1A 0N4 Canada Canada Your file Votre reference ISBN: 978-0-494-83407-7 Our file Notre reference ISBN: 978-0-494-83407-7 NOTICE: AVIS: The author has granted a non L'auteur a accorde une licence non exclusive exclusive license allowing Library and permettant a la Bibliotheque et Archives Archives Canada to reproduce, Canada de reproduire, publier, archiver, publish, archive, preserve, conserve, sauvegarder, conserver, transmettre au public communicate to the public by par telecommunication ou par Plnternet, preter, telecommunication or on the Internet, distribuer et vendre des theses partout dans le loan, distrbute and sell theses monde, a des fins commerciales ou autres, sur worldwide, for commercial or non support microforme, papier, electronique et/ou commercial purposes, in microform, autres formats. paper, electronic and/or any other formats. The author retains copyright L'auteur conserve la propriete du droit d'auteur ownership and moral rights in this et des droits moraux qui protege cette these. -
小型飛翔体/海外 [Format 2] Technical Catalog Category
小型飛翔体/海外 [Format 2] Technical Catalog Category Airborne contamination sensor Title Depth Evaluation of Entrained Products (DEEP) Proposed by Create Technologies Ltd & Costain Group PLC 1.DEEP is a sensor analysis software for analysing contamination. DEEP can distinguish between surface contamination and internal / absorbed contamination. The software measures contamination depth by analysing distortions in the gamma spectrum. The method can be applied to data gathered using any spectrometer. Because DEEP provides a means of discriminating surface contamination from other radiation sources, DEEP can be used to provide an estimate of surface contamination without physical sampling. DEEP is a real-time method which enables the user to generate a large number of rapid contamination assessments- this data is complementary to physical samples, providing a sound basis for extrapolation from point samples. It also helps identify anomalies enabling targeted sampling startegies. DEEP is compatible with small airborne spectrometer/ processor combinations, such as that proposed by the ARM-U project – please refer to the ARM-U proposal for more details of the air vehicle. Figure 1: DEEP system core components are small, light, low power and can be integrated via USB, serial or Ethernet interfaces. 小型飛翔体/海外 Figure 2: DEEP prototype software 2.Past experience (plants in Japan, overseas plant, applications in other industries, etc) Create technologies is a specialist R&D firm with a focus on imaging and sensing in the nuclear industry. Createc has developed and delivered several novel nuclear technologies, including the N-Visage gamma camera system. Costainis a leading UK construction and civil engineering firm with almost 150 years of history. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Study of Macromolecule-Mineral Interactions on Nuclear Related Materials
Study of macromolecule-mineral interactions on nuclear related materials by Lygia Eleftheriou Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Supervised by: Prof John Harding Dr Maria Romero-González The University of Sheffield Faculty of Engineering Department of Materials Science and Engineering September 2016 Declaration The work described within this thesis has been completed under the supervision of Prof J. Harding and Dr M. Romero-González at the University of Sheffield between September 2012 and September 2016. This thesis along with the work described here has been completed by the author with some exceptions indicated clearly at the relevant chapters. These include: (1) the construction of ceria models for the computational work that was completed by Dr Colin Freeman and Dr Shaun Hall (described in chapter 5), (2) the purification of peptidoglycan completed by Dr Stephane Mesnage (described in chapter 4) and (3) the electron microscopy analysis completed by Dr Mohamed Merroun (described in chapter 2). Lygia Eleftheriou September 2016 Acknowledgements I would like to express my sincere gratitude to my supervisors Dr Maria Romero González and Prof John Harding for all their support during the past four years. This work would not have been possible without their endless encouragement, guidance and advice. I would also like to thank Dr Colin Freeman, Dr Shaun Hall and Riccardo Innocenti Malini for all the hours they spent trying to make things work and all their help with the computational part of this project. In addition, I would like to thank Dr Simon Thorpe, Dr Stephane Mesnage and Mr Robert Hanson for their help with the analytical methods of this project. -
Physics 111 Fall 2007 Radioactive Decay Problems Solutions
Physics 111 Fall 2007 Radioactive Decay Problems Solutions 3 1. The 1 H isotope of hydrogen, which is called tritium (because it contains three nucleons), has a half-life of 12.33 yr. It can be used to measure the age of objects up to about 100 yr. It is produced in the upper atmosphere by cosmic rays and brought to Earth by rain. As an application, determine approximately the age of a bottle of wine 3 1 whose 1 H radiation is about 10 that present in new wine. Because the tritium in water is being replenished, we assume that the amount is constant until the wine is made, and then it decays. We find the number of half-lives from N n = 1 ; N ()2 0 n 0.10 = 1 , or n log 2 = log 10 , which gives n = 3.32. ()2 () Thus the time is t = nT = 3.32 12.33 yr = 41 yr. 1 ()() 2 2. Strontium-90 is produced as a nuclear fission product of uranium in both reactors and atomic bombs. Look at its location in the periodic table to see what other elements it might be similar to chemically, and tell why you think it might be dangerous to ingest. It has too many neutrons, and it decays with a half-life of about 29 yr. How 90 long will we have to wait for the amount of 38 Sr on the Earth’s surface to reach 1% of its current level, assuming no new material is scattered about? Write down the decay reaction, including the daughter nucleus. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
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Perspective the Radioactivity of Atmospheric Krypton in 1949–1950
Proc. Natl. Acad. Sci. USA Vol. 94, pp. 7807–7810, July 1997 Perspective The radioactivity of atmospheric krypton in 1949–1950 Anthony Turkevich*, Lester Winsberg†, Howard Flotow‡, and Richard M. Adams§ Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439 Contributed by Anthony Turkevich, April 10, 1997 ABSTRACT The chemical element krypton, whose prin- Libby (in 1948; unpublished work) gave indications that these cipal source is the atmosphere, had a long-lived radioactive predictions were correct. The present report describes the content, in the mid-1940s, of less than 5 dpm per liter of technique that was used soon afterward to establish more krypton. In the late 1940s, this content had risen to values in precisely that atmospheric krypton in the late 1940s was much the range of 100 dpm per liter. It is now some hundred times more radioactive than it had been, and gives the results of some higher than the late 1940 values. This radioactivity is the early measurements of krypton samples isolated from the result of the dissolving of nuclear fuel for military and civilian atmosphere at that time.** purposes, and the release thereby of the fission product krypton-85 (half-life 5 10.71 years, fission yield 5 0.2%). The Measurement Technique present largest emitter of krypton-85 is the French reprocess- ing plant at Cap-de-la-Hague. The measurement technique that was used was influenced by those simultaneously being developed by Libby and Anderson It is generally known that the chemical element krypton, (9) to measure the radiocarbon content of samples of arche- isolated from the atmosphere in 1996, is radioactive. -
PROGRAM SCHEDULE (Oral Presentations)
PROGRAM SCHEDULE (Oral Presentations) ID Title Session Time Room Date Speaker Authors 40SS - Passive control systems: Equivalent static analysis for structures with Giada Gasparini, Michele Palermo, Luca Landi, 2030 analysis methods and designing 10:30 - 10:45 Vitacura Room (1) Monday, January 9th Michele Palermo added viscous dampers Stefano Silvestri, Tomaso Trombetti procedures 40SS - Passive control systems: A General Design Method for Buildings with JUAN CARLOS DE LA 1187 analysis methods and designing 10:45 - 11:00 Vitacura Room (1) Monday, January 9th JUAN C. DE LA LLERA, JUAN J. BESA Energy Dissipation Devices LLERA procedures IMPORTANCE OF DUCTILE CONFINEMENT IN 40SS - Passive control systems: Horacio J. Nangullasmu- 3327 REINFORCED CONCRETE FRAMES WITH analysis methods and designing 11:00 - 11:15 Vitacura Room (1) Monday, January 9th Horacio Nangullasmu, Arturo Tena Hernandez STRUCTURAL FUSES procedures 40SS - Passive control systems: NEW SEISMIC RESPONSE CONTROL SYSTEM 1652 analysis methods and designing 11:15 - 11:30 Vitacura Room (1) Monday, January 9th Taiki SAITO Taiki SAITO, Satoshi DENNO, Toshio Maekawa USING BLOCK AND TACKLE procedures 40SS - Passive control systems: Eccentric Lever Arm Amplification System for 3870 analysis methods and designing 11:30 - 11:45 Vitacura Room (1) Monday, January 9th Jose Almazan Jose Almazan, Nicolas Tapia, Juan Baquero Frictional Energy Dissipation Devices procedures Experimental Study on the Seismic Performance 40SS - Passive control systems: 1223 of Four-Tower High-rise with an isolated -
RCC-Mrx Chairwoman CEA - Senior Expert in Design Codes and Standards for Mechanical Components
Shaping the rules for a sustainable nuclear technology How to introduce new materials in design codes Cécile PÉTESCH RCC-MRx chairwoman CEA - Senior Expert in design codes and standards for mechanical components SNETP FORUM 2021 Towards innovative R&D in civil nuclear fission AFCEN is ISO 9001:2015 certified © 2021 www.afcen.com | 1 Shaping the rules for a sustainable nuclear technology Design codes vs new material Why? Interest to connect R&D to standardisation What? Example of RCC-MRx code How? Difficulties to introduce a new material Conclusion SNETP FORUM 2021 Towards innovative R&D in civil nuclear fission AFCEN is ISO 9001:2015 certified © 2021 www.afcen.com | 2 Shaping the rules for a sustainable nuclear technology Design codes vs new material Why? Interest to connect R&D to standardisation What? Example of RCC-MRx code How? Difficulties to introduce a new material Conclusion SNETP FORUM 2021 Towards innovative R&D in civil nuclear fission AFCEN is ISO 9001:2015 certified © 2021 www.afcen.com | 3 Why? Codes and standards Modification request Material file Nuclear Industry New Material SNETP FORUM 2021 Towards innovative R&D in civil nuclear fission AFCEN is ISO 9001:2015 certified © 2021 www.afcen.com | 4 Why? Codes and standards DMRx Material file REGULATOR New Material SNETP FORUM 2021 Towards innovative R&D in civil nuclear fission AFCEN is ISO 9001:2015 certified © 2021 www.afcen.com | 5 Why? For innovative reactors, standardization is one way to reach a highest technology readiness level, giving a frame and a direction -
Accumulation and Mobility of Radionuclides in the Sellafield Near-Shore
Accumulation and Mobility of Radionuclides in the Sellafield Near-Shore A thesis submitted to the University of Manchester for the degree of Master of Science by Research in the Faculty of Engineering and Physical Sciences 2013 Daisy Ray School of Chemistry Contents Contents 2 List of Figures 5 Abstract 7 Declaration 8 Copyright 8 Chapter 1 Introduction 10 1.1. Overview 11 1.2. Thesis Structure 11 1.3. Nuclear Power 12 1.3.1 Early Development and Contemporary Demand 12 1.3.2. The UK Nuclear Legacy 13 1.4. The Nuclear Fuel Cycle 14 1.4.1. Mining and Milling of Uranium Ore 15 1.4.2. Purification and Fuel Fabrication 15 1.4.3. Reactor Operation 16 1.4.4. Spent Fuel Reprocessing 17 1.5. Sellafield 19 1.5.1. Operational History of Sellafield 19 1.6. Radionuclides in the Environment 20 1.6.1. Authorised Sellafield Discharges 21 2 1.7. The Chemistry of Select Actinides and Fission Products in Sellafield Effluents 23 1.7.1. Plutonium 23 1.7.2. Americium 26 1.7.3. Caesium 27 1.8. Biogeochemistry of the Natural Environment 27 1.8.1. Sorption 28 1.8.2. Incorporation/Precipitation 29 1.8.3. Redox Reactions 29 1.8.4. Bioturbation 30 1.8.5. Microbial Activity 31 1.9. Mechanism of Radionuclide Transportation 33 1.10. Project Aims 35 Chapter 2 Materials and Methods 37 2.1. Sample Collection 38 2.2. Major and Minor elemental analysis 39 2.3. Americium and Caesium Detection 40 2.3.1. -
Magnetic Field Generation in Planets and Satellites by Natural Nuclear Fission Reactors
Magnetic Field Generation in Planets and Satellites by Natural Nuclear Fission Reactors by J. Marvin Herndon Transdyne Corporation San Diego, CA 92131 USA 27 July 2007 Communications: [email protected] http://UnderstandEarth.com Keywords: Planetary Magnetic Field, Geomagnetism, Geomagnetic Field, Georeactor Abstract: One of the most fundamental problems in physics has been to understand the nature of the mechanism that generates the geomagnetic field and the magnetic fields of other planets and satellites. For decades, the dynamo mechanism, thought to be responsible for generating the geomagnetic field and other planetary magnetic fields, has been ascribed to convection in each planet’s iron-alloy core. Recently, I described the problems inherent in Earth-core convection and proposed instead that the geomagnetic field is produced by convection in the electrically conductive, fluid, fission-product sub-shell of a natural nuclear fission reactor at the center of the Earth, called the georeactor. Here I set forth in detail the commonality in the Solar System of the matter like that of the inside of the Earth, which is my basis for generalizing the concept of planetary magnetic field generation by natural planetocentric nuclear fission reactors. Introduction Currently active internally generated magnetic fields have been detected in six planets (Mercury, Earth, Jupiter, Saturn, Uranus, and Neptune) and in one satellite (Jupiter’s moon Ganymede). Magnetized surface areas of Mars and the Moon indicate the former existence of internally generated magnetic fields in those bodies. The purpose of this communication is to suggest that those magnetic fields arise from the same georeactor-type mechanism which I have suggested generates and powers the Earth’s magnetic field [1].