Development of Gamma-Ray Diagnostics for ITER
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Design of Neutron and Gamma Ray Diagnostics for the Start-Up Phase of the DTT Tokamak
46th EPS Conference on Plasma Physics P5.1105 Design of neutron and gamma ray diagnostics for the start-up phase of the DTT tokamak M. Angelone 1, D. Rigamonti 2, M Tardocchi 2, F. Causa 2, S. Fiore 1, L. C. Giacomelli 2, G. Gorini 3,2 , F. Moro 1, M. Nocente 3,2 , M. Osipenko 4, M. Pillon 1, , M. Ripani 4, R. Villari 1 1ENEA, Centro Ricerche Frascati, Frascati, Italy 2Istituto per la Scienza e Tecnologia dei Plasmi, CNR, Milan, Italy 3Dipart. di Fisica “G. Occhialini”, Università degli Studi di Milano-Bicocca, Milano, Italy 4Istituto Nazionale di Fisica Nucleare, Genova, Italy e-mail : [email protected] Abstract The Divertor Tokamak Test (DTT) facility, which is under design for construction in Frascati (Italy), will produce neutron yield up to 1.3*10 17 n/s at full power (H-mode scenario). This calls for an accurate design and selection of the 2.5 MeV neutron diagnostic systems and detectors which can give the comprehensive exploitation of the high neutron fluxes. Measurements of 14 MeV neutrons (which are about 1% of the total neutron yield) coming from the triton burn-up will also be performed. DTT will reach its best performances after a preliminary phase , needed to assess and improve the machine parameters. Here we present the neutron and gamma-ray diagnostics systems which are under design for the initial start-up phase of DTT. The design work benefits from the experience gathered by the community on high power tokamak such as JET. These systems, also called day-1 diagnostics, are: i) Neutron flux monitors which measure the 2.5 and 14 MeV neutron yield s, ii) Neutron/Gamma camera for the reconstruction of the neutron and gamma ray emission profile of the plasma , iii) Hard x-ray monitors for measurements of the bremsstrahlung radiation produced by runway electrons in the 1-40 MeV energy range 1.0 Introduction The Divertor Tokamak Test (DTT) facility, which is under design for construction in Frascati (Italy), will produce neutron yield up to 1.3*10 17 n/s at full power (H-mode scenario). -
R-Process Elements from Magnetorotational Hypernovae
r-Process elements from magnetorotational hypernovae D. Yong1,2*, C. Kobayashi3,2, G. S. Da Costa1,2, M. S. Bessell1, A. Chiti4, A. Frebel4, K. Lind5, A. D. Mackey1,2, T. Nordlander1,2, M. Asplund6, A. R. Casey7,2, A. F. Marino8, S. J. Murphy9,1 & B. P. Schmidt1 1Research School of Astronomy & Astrophysics, Australian National University, Canberra, ACT 2611, Australia 2ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia 3Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, AL10 9AB, UK 4Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 5Department of Astronomy, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden 6Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany 7School of Physics and Astronomy, Monash University, VIC 3800, Australia 8Istituto NaZionale di Astrofisica - Osservatorio Astronomico di Arcetri, Largo Enrico Fermi, 5, 50125, Firenze, Italy 9School of Science, The University of New South Wales, Canberra, ACT 2600, Australia Neutron-star mergers were recently confirmed as sites of rapid-neutron-capture (r-process) nucleosynthesis1–3. However, in Galactic chemical evolution models, neutron-star mergers alone cannot reproduce the observed element abundance patterns of extremely metal-poor stars, which indicates the existence of other sites of r-process nucleosynthesis4–6. These sites may be investigated by studying the element abundance patterns of chemically primitive stars in the halo of the Milky Way, because these objects retain the nucleosynthetic signatures of the earliest generation of stars7–13. -
Experimental Γ Ray Spectroscopy and Investigations of Environmental Radioactivity
Experimental γ Ray Spectroscopy and Investigations of Environmental Radioactivity BY RANDOLPH S. PETERSON 216 α Po 84 10.64h. 212 Pb 1- 415 82 0- 239 β- 01- 0 60.6m 212 1+ 1630 Bi 2+ 1513 83 α β- 2+ 787 304ns 0+ 0 212 α Po 84 Experimental γ Ray Spectroscopy and Investigations of Environmental Radioactivity Randolph S. Peterson Physics Department The University of the South Sewanee, Tennessee Published by Spectrum Techniques All Rights Reserved Copyright 1996 TABLE OF CONTENTS Page Introduction ....................................................................................................................4 Basic Gamma Spectroscopy 1. Energy Calibration ................................................................................................... 7 2. Gamma Spectra from Common Commercial Sources ........................................ 10 3. Detector Energy Resolution .................................................................................. 12 Interaction of Radiation with Matter 4. Compton Scattering............................................................................................... 14 5. Pair Production and Annihilation ........................................................................ 17 6. Absorption of Gammas by Materials ..................................................................... 19 7. X Rays ..................................................................................................................... 21 Radioactive Decay 8. Multichannel Scaling and Half-life ..................................................................... -
Radiation Quick Reference Guide Recommend Contacting Your State Fusion Center
Domestic Nuclear Detection Office If you encounter something suspicious follow your specific local protocols. Radiation Quick Reference Guide Recommend contacting your state fusion center. DNDO is available 24/7 to assist at 1-877-DNDO-JAC / 1-877-363-6522 JAC Information Line 202-254-7179 Email: [email protected] Nuclear Concerns/ Threats 1. Nuclear Weapon - a device that releases nuclear energy in an ex- Isotopes of Concern for use in RDDs - with common uses plosive manner. Uses Highly Enriched Uranium (HEU) and/or 1. Cobalt-60 – cancer treatment, level/ Plutonium. density gauge, teletherapy, radiography, 2. Improvised Nuclear Device (IND) - a nuclear weapon fabricated food sterilization/irradiation, by a terrorist organization or rogue nation. brachytherapy 2. Iridium-192 – Radiography/non- destructive testing, flaw detection, brachy- therapy “cancer seed”, skin cancer Cobalt 60 sources Uranium “superficial” brachytherapy Plutonium 3. Uranium a. Uranium exists naturally in the earth’s crust. Of the different “isotopes” of uranium, U-235 is the one required to produce a Iridium sentinel and nuclear weapon. gamma camera b. Natural uranium contains a small amount of U-235 (<1%) which Cesium Seeds must be separated in complex extraction processes to create HEU. The predominant uranium isotope is U-238. 3. Cesium-137 - Gauge/level gauge, industrial radiography, brachyther- c. Highly Enriched Uranium (HEU) refers to uranium usable in weap- apy/teletherapy, well logging/density gauges ons due to its enrichment in U-235. 4. Strontium-90 – Radioisotope thermoelectric generator (RTG), fis- d. Approximately 25 kg of HEU is required for a nuclear weapon. sion product, industrial gauges, medical treatment e. -
A New Gamma Camera for Positron Emission Tomography
INIS-mf—11552 A new gamma camera for Positron Emission Tomography NL89C0813 P. SCHOTANUS A new gamma camera for Positron Emission Tomography A new gamma camera for Positron Emission Tomography PROEFSCHRIFT TER VERKRIJGING VAN DE GRAAD VAN DOCTOR AAN DE TECHNISCHE UNIVERSITEIT DELFT, OP GEZAG VAN DE RECTOR MAGNIFICUS, PROF.DRS. P.A. SCHENCK, IN HET OPENBAAR TE VERDEDIGEN TEN OVERSTAAN VAN EEN COMMISSIE, AANGEWEZEN DOOR HET COLLEGE VAN DECANEN, OP DINSDAG 20 SEPTEMBER 1988TE 16.00 UUR. DOOR PAUL SCHOTANUS '$ DOCTORANDUS IN DE NATUURKUNDE GEBOREN TE EINDHOVEN Dit proefschrift is goedgekeurd door de promotor Prof.dr. A.H. Wapstra s ••I Sommige boeken schijnen geschreven te zijn.niet opdat men er iets uit zou leren, maar opdat men weten zal, dat de schrijver iets geweten heeft. Goethe Contents page 1 Introduction 1 2 Nuclear diagnostics as a tool in medical science; principles and applications 2.1 The position of nuclear diagnostics in medical science 2 2.2 The detection of radiation in nuclear diagnostics: 5 standard techniques 2.3 Positron emission tomography 7 2.4 Positron emitting isotopes 9 2.5 Examples of radiodiagnostic studies with PET 11 2.6 Comparison of PET with other diagnostic techniques 12 3 Detectors for positron emission tomography 3.1 The absorption d 5H keV annihilation radiation in solids 15 3.2 Scintillators for the detection of annihilation radiation 21 3.3 The detection of scintillation light 23 3.4 Alternative ways to detect annihilation radiation 28 3-5 Determination of the point of annihilation: detector geometry, -
Gamma Cameras
OECD Health Statistics 2021 Definitions, Sources and Methods Gamma cameras Number of Gamma cameras. A Gamma camera (including Single Photon Emission Computed Tomography, SPECT) is used for a nuclear medicine procedure in which the camera rotates around the patient to register gamma rays emission from an isotope injected to the patient's body. The gathered data are processed by a computer to form a tomographic (cross-sectional) image. Inclusion - SPECT-CT systems using image fusion (superposition of SPECT and CT images). Sources and Methods Australia Source of data: Department of Health. Unpublished data from Location Specific Position Number register. Reference period: Years reported are financial years 1st July to 31st June (e.g. data for 2012 are as at 30th June 2012). Coverage: Data from 2008 onwards represent the number of units approved for billing to Medicare only. Units may be removed from one location and re-registered in another location. Austria Source of data: Austrian Federal Ministry of Social Affairs, Health, Care and Consumer Protection / Gesundheit Österreich GmbH, Monitoring of medical technology development. Reference period: 31st December. Coverage: - Included are all Gamma cameras units in hospitals as defined by the Austrian Hospital Act (KAKuG) and classified as HP.1 according to the System of Health Accounts (OECD). - The ambulatory sector is included (HP.3). Belgium Source of data: Federal Service of Public Health, DGGS “Organisation of health provisions”; Ministry of the Flemish community and Ministry of the French community. Coverage: - Ambulatory care providers (HP.3): Data on high-tech equipment in cabinets of ambulatory care providers are not available. -
3 Gamma-Ray Detectors
3 Gamma-Ray Detectors Hastings A Smith,Jr., and Marcia Lucas S.1 INTRODUCTION In order for a gamma ray to be detected, it must interact with matteu that interaction must be recorded. Fortunately, the electromagnetic nature of gamma-ray photons allows them to interact strongly with the charged electrons in the atoms of all matter. The key process by which a gamma ray is detected is ionization, where it gives up part or all of its energy to an electron. The ionized electrons collide with other atoms and liberate many more electrons. The liberated charge is collected, either directly (as with a proportional counter or a solid-state semiconductor detector) or indirectly (as with a scintillation detector), in order to register the presence of the gamma ray and measure its energy. The final result is an electrical pulse whose voltage is proportional to the energy deposited in the detecting medhtm. In this chapter, we will present some general information on types of’ gamma-ray detectors that are used in nondestructive assay (NDA) of nuclear materials. The elec- tronic instrumentation associated with gamma-ray detection is discussed in Chapter 4. More in-depth treatments of the design and operation of gamma-ray detectors can be found in Refs. 1 and 2. 3.2 TYPES OF DETECTORS Many different detectors have been used to register the gamma ray and its eneqgy. In NDA, it is usually necessary to measure not only the amount of radiation emanating from a sample but also its energy spectrum. Thus, the detectors of most use in NDA applications are those whose signal outputs are proportional to the energy deposited by the gamma ray in the sensitive volume of the detector. -
State-Of-The-Art Mobile Radiation Detection Systems for Different Scenarios
sensors Review State-of-the-Art Mobile Radiation Detection Systems for Different Scenarios Luís Marques 1,* , Alberto Vale 2 and Pedro Vaz 3 1 Centro de Investigação da Academia da Força Aérea, Academia da Força Aérea, Instituto Universitário Militar, Granja do Marquês, 2715-021 Pêro Pinheiro, Portugal 2 Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal; [email protected] 3 Centro de Ciências e Tecnologias Nucleares, Instituto Superior Técnico, Universidade de Lisboa, Estrada Nacional 10 (km 139.7), 2695-066 Bobadela, Portugal; [email protected] * Correspondence: [email protected] Abstract: In the last decade, the development of more compact and lightweight radiation detection systems led to their application in handheld and small unmanned systems, particularly air-based platforms. Examples of improvements are: the use of silicon photomultiplier-based scintillators, new scintillating crystals, compact dual-mode detectors (gamma/neutron), data fusion, mobile sensor net- works, cooperative detection and search. Gamma cameras and dual-particle cameras are increasingly being used for source location. This study reviews and discusses the research advancements in the field of gamma-ray and neutron measurements using mobile radiation detection systems since the Fukushima nuclear accident. Four scenarios are considered: radiological and nuclear accidents and emergencies; illicit traffic of special nuclear materials and radioactive -
Sources of Gamma Radiation in a Reactor Core Matts Roas
AE-19 Sources of gamma radiation in a reactor core Matts Roas AKTIEBOLAGET ATOMENERGI STOCKHOLM • S\\ HDJtN • 1959 AE-19 ERRATUM The spectrum in Fig. 3 has erroneously been normalized to 7. 4 MeV/capture. The correct spectrum can be found by mul- tiplying the ordinate by 0. 64. AE-19 Sources of gamma radiation in a reactor core Matts Roos Summary: - In a thermal reactor the gamma ray sources of importance for shielding calculations and related aspects are 1) fission, 2) decay of fission products, 3) capture processes in fuel, poison and other materials, 4) inelastic scattering in the fuel and 5) decay of capture products. The energy release and the gamma ray spectra of these sources have been compiled or estimated from the latest information available, and the results are presented in a general way to permit 235 application to any thermal reactor, fueled with a mixture of U and 238 U • As an example the total spectrum and the spectrum of radiation escaping from a fuel rod in the Swedish R3-reactor are presented. Completion of manuscript April 1959 Printed Maj 1959 LIST OF CONTENTS Page Introduction ........... 1 1. Prompt fis sion gamma rays i 2. Fission product gamma rays 2 3. Uranium capture gamma rays 4 O -2 Q 4. U inelastic scattering gamma rays 5 5. Gamma rays from capture in poison, construction materials and moderator .....*•»..•........ 8 6. Gamma rays from disintegration of capture products. 8 7. Total gamma spectra. Application to the Swedish R3 -reactor 9 SOURCES OF GAMMA RADIATION IN A REACTOR CORE. -
Slow Neutrons and Secondary Gamma Ray Distributions in Concrete Shields Followed by Reflecting Layers
oo A. R. E. A. E. A. / Rep. 318 w ARAB REPUBLIC OF EGYPT ATOMIC ENERGY AUTHORITY REACTOR AND NEUTRON PHYSICS DEPART SLOW NEUTRONS AND SECONDARY GAMMA RAY DISTRIBUTIONS IN CONCRETE SHIELDS FOLLOWED BY REFLECTING LAYERS BY A.S. MAKARI.OUS, Y;I. SWILEM, Z. AWWAD AND T. BAYOMY 1993 INFORMATION AND DOCUMENTATION CENTER ATOMIC ENERGY POST OFFICE CAIRO, A.R;I:. VOL 2 7 id Q 7 AREAEA/Rep.318 ARAB REPUBLIC OF EGYPT ATOMIC ENERGY AUTHORITY REACTOR AND NEUTRON PHYSICS DEPART, SLOW NEUTRONS AND SECONDARY GAMMA RAY DISTRIBUTIONS IN CONCRETE SHIELDS FOLLOWED BY REFLECTING LAYERS BY A,S.M\KARIOUS, Y.I.SWILEM, 2.AWWAD AND T.BAYOMY INFORMATION AND DUCUMENTATICN CENTER ATOMIC ENERGY POST OFFICE CAIRO, A.R«E. CONTENTS x Page ABSTRACT *<,..».»••... i INTRODUCTION . *« . *.*,...... 1 EXPERIMENTAL DETAILS ••»*«•««»« • • a • » « •»»«*««* *»»*«•»»»«»<>• — RESULTS AND DISCUSSION ..,.••+ .*.....•...•.. 4 ACKNOWLEDGEMENTS ...,.......•..<...»,..>......... 10 REFERENCES „...»,«.**»» 11 ABSTRACT Slow neutrons and secondary gamma r>ay distributions in concrete shields with and without a reflecting layer behind the concrete shield have been investigated first in case of' using a bare reactor beam and then on using & B.C filtered beam. The total and capture secondary gair-m-a ray coefficient (B^and B^) , the ratio of the reflected (Thermal neutron (S ) the ratio of the secondary gamma rays caused by reflected neutrons to those caused by transmitted neutrons ( and the effect of inserting a blocking l&yer (a B^C layer) between the concrete shield and the reflector on the sup- pression of the produced secondary gamma rays have been investigated, It was found that the presence of the reflector layer behind the concrete shield reflects sor/so thermal neutrons back to the concrete shields end so it increases the number of thermal neutrons at the interface between the concrete shield and the reflector. -
Radiation and Radionuclide Measurements at Radiological and Nuclear Emergencies
Radiation and radionuclide measurements at radiological and nuclear emergencies. Use of instruments and methods intended for clinical radiology and nuclear medicine. Ören, Ünal 2016 Document Version: Publisher's PDF, also known as Version of record Link to publication Citation for published version (APA): Ören, Ü. (2016). Radiation and radionuclide measurements at radiological and nuclear emergencies. Use of instruments and methods intended for clinical radiology and nuclear medicine. Lund University: Faculty of Medicine. Total number of authors: 1 Creative Commons License: Other General rights Unless other specific re-use rights are stated the following general rights apply: Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the public portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the public portal Read more about Creative commons licenses: https://creativecommons.org/licenses/ Take down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. LUND UNIVERSITY PO Box 117 221 00 Lund +46 46-222 00 00 Download date: 24. Sep. 2021 Radiation and radionuclide measurements at radiological and nuclear emergencies Use of instruments and methods intended for clinical radiology and nuclear medicine Ünal Ören DOCTORAL DISSERTATION by due permission of the Faculty of Medicine, Lund University, Sweden. -
Gamma-Ray Bursts and Magnetars
GAMMA-RAY BURSTS AND MAGNETARS How USRA scientists helped make major advancements in high-energy astrophysics. During the 1960s, the second Administrator Frank J. Kerr (1918 - 2000) of the University of NASA, James E. Webb, sought a university- of Maryland was appointed by USRA to based organization that could serve the manage its programs in astronomy and needs of NASA as well as the space research astrophysics. Kerr was a highly-regarded radio community. In particular, Webb sought to astronomer, originally from Australia. He had have university researchers assist NASA in been the Director of the Astronomy Program the planning and execution of large, complex at the University projects. The result of Webb’s vision was of Maryland, the Universities Space Research Association and at the time (USRA), which was incorporated as a non- of his USRA proft association of research universities on appointment 12 March 1969. in 1983, he was Provost of As described in the previous essay, USRA’s the Division of frst major collaboration with NASA was the Physical and Apollo Exploration of the Moon. The vehicle Mathematical by which USRA assisted NASA and the space Sciences and research community was the Lunar Science Engineering at Institute, later renamed the Lunar and the University. Frank Kerr Planetary Institute. In support of Another major project was undertaken in MSFC and NRL, USRA brought astronomers 1983, when USRA began to support NASA to work closely with NASA researchers in in the development of the Space Telescope the development of instrumentation and Project at NASA’s Marshall Space Flight the preparation for analyses of data for Center (MSFC).