DOCSLIB.ORG

Introduction to Synchrotron Radiation

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Introduction to Synchrotron Radiation Introduction to Synchrotron Radiation Frederico Alves Lima International School on Laser-Beam Interactions Centro Nacional de Pesquisa em Energia e Materiais - CNPEM UFRN - Natal, Brazil Laboratório Nacional de Luz Síncrotron - LNLS September 2016 Outline ✓ Tools for structural analysis ✓ History of X-rays ✓ Synchrotron Radiation ✓ LNLS & SIRIUS: Synchrotron Radiation in Brazil Why do we need to study “structure” Structure Dynamics - X-ray crystallography - Laser spectroscopy - electron microscopy - NMR - atomic force microscopy - Time-resolved diffraction & XAS - electron diffraction - Time-resolved PES - X-ray absorption spectroscopy - NMR Manganite: atomic motion coupled by charge and orbital order Graphene Fullerene Layer-selective spin dynamics in Nanotube magnetic multilayers Photosystem II Rotating hydrated Mb molecule What are the length scales involved ? http://www.newgrounds.com/portal/view/525347 The Electromagnetic Spectrum Electromagnetic wave ➟ Light! Orthogonal and alternating electric and magnetic fields that propagate into space. Set of equations describing how electric and magnetic fields are generated and altered by each other and by charges and currents. Maxwell’s equation of electromagnetism James Clerk Maxwell The Electromagnetic Spectrum 700 nm 400 nm X-ray ➟ proper tool to investigate atoms. History of X-rays In the evening of Nov. 8th 1895 Wilhem Röntgen first detected x-rays He found that when running a high-voltage discharge tube enclosed in thick black cardboard which excluded all visible light, in his darkened room, a paper plate covered on one side with barium platinocyanide would fluoresce, even when it was as far as 2 m from the discharge tube. ➟ X-rays! He soon discovered that these ‘x-rays’ also stained photographic plates and latter demonstrated that objects of different thicknesses showed different degrees of transparency. First x-ray photograph of a human hand with a ring… probably from his wife! Synchrotron Radiation We need an extremely bright source of x-rays ➟ Synchrotron F divergence flux brightness Ω F / S ⌦ source area S · Synchrotrons are very bright because the source size and divergence are very small. But why is that? Synchrotron Radiation Accelerated electric charge ➟ electromagnetic radiation In the non-relativistic case, the dominant emission from an electric charge is dipolar. ∆!0 Maxwell’s equation !0 The emitted power and spectrum are proportional do the acceleration, was given by the Larmor formula. Acceleration is usually a function of t, resulting in a certain distribution of the emitted energy. antenna Synchrotron Radiation Decelerated electric charge ➟ Bremsstrahlung radiation (Non-relativistic) charges colliding with a target also emit radiation with a dominant dipolar contribution. X-ray spectrum of a Silver target (anode) as a function of the voltage. Note the different emission lines and also the Bremsstrahlung radiation. X-ray tube Synchrotron Radiation Relativistic limit + acceleration ➟ synchrotron radiation Relativistic electrons can be accelerated by a magnetic F~ = q(E~ + ~v B~ ) field through the Lorentz force ⇥ Emitted radiation cone has an angular opening depending on " 1 the Lorentz factor γ = , that is: ✓ mc2 ⇠ γ ✓ Synchrotron source Synchrotron Radiation: bending magnets Magnetic field used to change the propagation direction of electric charges in movement The critical energy of radiation emitted by bending magnets depends on the energy of the accelerated electrons. Synchrotron Radiation: insertion devices Alternating magnetic poles make electric charges 'wiggle' Wiggler Undulator http://photon-science.desy.de/research/studentsteaching/primers/synchrotron_radiation/index_eng.html Insertion devices in reality How to produce Synchrotron radiation? Synchrotron Radiation Main components: - LINAC: linear accelerator - Booster - Storage ring - Beamlines Where are the synchrotron sources? http://www.lightsources.org/ Synchrotron Radiation: Optics Synchrotron Radiation: stored electrons Stored electrons are in dynamic equilibrium inside the lattice Concrete wall shielding Front-end Bending magnet Insertion device RF cavity restores the energy lost each turn. It also generates a potential well in the storage ring which is responsible for packing the electrons in “bunches”. Synchrotron radiation is intrinsically pulsed Resonant RF cavity Experiments exploiting temporal resolution! X-ray Free-Electron Lasers Resonant condition: The slippage between the electromagnetic wave and a given electron, while the electron advances by one undulator period must be equal to the field wavelength. ➟ ⇥0 2 ⇥rad = 2 (1 + Keff /2) Micro-bunching 2γ Keff =0.934λradBeff SASE - Self Amplified Spontaneous Emission Long undulators are needed as the saturation of the micro-bunching effect is a function of the length. X-ray Free-Electron Lasers The result is a tremendous increase in the peak brilliance! X-ray FEL’s generate laser-like radiation: coherent x-rays and with ultrafast temporal duration (femtosecond pulses!) Ultrafast dynamics Single-molecule diffraction Coherent imaging/scattering Investigation of Small quantum systems Non-linear X-ray Matter under extreme conditions et cetera Completely new science could be done at XFELs! Interaction of X-rays with Matter How does electromagnetic radiation interact with matter? - Scatter - Diffraction - Absorption - … We make use of these phenomena to design experiments that help us to elucidate the properties of matter. - Small/Wide Angle X-ray Scattering - X-ray Diffraction - X-ray Absorption Spectroscopy Structural characterization using x-rays Scattering sample Int q Structural characterization using x-rays Diffraction �istal histidine ligand heme �istal histidine proximal histidine ligand heme proximal histidine http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/bragg.html Structural characterization using x-rays Absorption X-RAYS 0 An x-ray photon is absorbed by an atom ejected an electron, I / I which then propagates in the material using the excess energy. 1 Z 1.4 1.2 1.0 0.8 0.6 Norm. [a.u.]µ(E) 0.4 0.2 7.105 7.110 7.115 7.120 0.0 7.1 7.2 7.3 7.4 7.5 7.6 X-ray energy [keV] Synchrotron Radiation Around the World Brazil has one such light source operating since 1997! CNPEM - LNLS & SIRIUS LNLS: research and development using LNNano: research on nano(materials) synchrotron radiation CTBE: research on ethanol production LNBio: research on biosciences SIRIUS% Synchrotron Radiation LNLS Synchrotron Radiation in Brazil Laboratório Nacional de Luz Síncrotron: LNLS - One out of the 4 labs (LNLS, LNNano, LNBio & CTBE) of the CNPEM - 18 beamlines operating http://lnls.cnpem.br/ LNLS User community Other States São Paulo Other countries In 1997 In 2013 100 proposals 400 proposals 180 users 1200 users 18 beamlines 7 beamlines http://lnls.cnpem.br CNPEM: areas of actuation - Synchrotron Light Source operation and development - Material’s science - Molecular biology - NMR spectroscopy - Mass spectrometry - Electron microscopy & Scanning probe microscopy - Mechanical microfabrication - Chemical synthesis - Engineering (scientific instrumentation) - Bioethanol research - etc Summary ✓ CNPEM is a multi-disciplinary research center with cutting edge equipment and staff ✓ Structure & dynamics are important to determine how materials function ✓ X-rays are suitable to study atomic scale ✓ Synchrotron light ➟ indispensable scientific & technologic tool ✓ To produce SR we need accelerated relativistic charges (e-) ✓ The SR has very special characteristics - Hight brightness - Very collimamated - (Almost) continuum spectrum Thank you.
Load more

Recommended publications
  • Physics of Incoherent Synchrotron Radiation Kent Wootton SLAC National Accelerator Laboratory
    SLAC-PUB-17214 Physics of Incoherent Synchrotron Radiation Kent Wootton SLAC National Accelerator Laboratory US Particle Accelerator School Fundamentals of Accelerator Physics 23rd Jan 2018 Old Dominion University Norfolk, VA This work was supported by the Department of Energy contract DE-AC02-76SF00515. Circular accelerators – observation of SR in 1947 “A small, very bright, bluish- white spot appeared at the side of the chamber where the beam was approaching the observer. At lower energies, the spot changed color.” “The visible beam of “synchrotron radiation” was an immediate sensation. Charles E. Wilson, president of G.E. brought the whole Board of Directors to see it. During the next two years there were visits from six Nobel Prize winners.” J. P. Blewett, Nucl. Instrum. Methods Phys. Res., Sect. A, 266, 1 (1988). 2 Circular electron colliders – SR is a nuisance • “… the radiative energy loss accompanying the Source: Australian Synchrotron circular motion.” 4휋 푒2 훿퐸 = 훾4 3 푅 • Limits max energy • Damps beam size Source: CERN D. Iwanenko and I. Pomeranchuk, Phys. Rev., 65, 343 (1944). J. Schwinger, Phys. Rev., 70 (9-10), 798 (1946). 3 ‘Discovery machines’ and ‘Flavour factories’ • Livingston plot • Proton, electron colliders • Protons, colliding partons (quarks) • Linear colliders Linear colliders proposed Source: Australian Synchrotron 4 Future energy frontier colliders FCC-ee/ FCC/ SPPC d=32 km LEP/ Source: Fermilab 5 SR can be useful – accelerator light sources • Unique source of electromagnetic radiation • Wavelength-tunable •
    [Show full text]
  • Synchrotron Radiation R.P
    SYNCHROTRON RADIATION R.P. Walker Sincrotrone Trieste, Italy Abstract The basic properties of synchrotron radiation are described, and their relevance to the design of electron and proton rings is discussed. The development of specialized sources of synchrotron radiation is also considered. 1 . INTRODUCTION The electromagnetic radiation emitted by a charged particle beam in a circular accelerator is termed "synchrotron radiation" (SR) after its first visual observation nearly 50 years ago in the General Electric (G.E.) 70 MeV Synchrotron. The theoretical basis for understanding synchrotron radiation however goes back much further. Maxwell's equations (1873) made it clear that changing charge densities would radiate electromagnetic waves, and Hertz demonstrated these waves in 1887. The first more directly relevant development was the publication of Liénard's paper entitled "The electric and magnetic field produced by an electric charge concentrated at a point and in arbitrary motion" [1]. This work includes the energy loss formula for particles travelling on a circular path with relativistic velocities. Later, Schott published a detailed essay that included also the angular and frequency distribution of the radiation, as well as the polarization properties [2]. No further interest appears to have been taken in the topic until the early 1940's, when theoretical work in the Soviet Union showed that the energy loss may pose a limit on the maximum energy obtainable in the betatron [3]. Then in 1946 Blewett measured the energy loss due to SR in the G.E. 100 MeV betatron and found agreement with theory, but failed to detect the radiation after searching in the microwave region of the spectrum [4].
    [Show full text]
  • 2 Radiation Safety and Shielding
    ESH&Q Chapter 2: Radiation Safety and Shielding 2-21 2 RADIATION SAFETY AND SHIELDING 2.1 SHIELDING OBJECTIVES NSLS-II is subject to DOE radiation protection standards. The primary document that defines the DOE radiation protection standard is the Code of Federal Regulations, 10 CFR 835. In addition, the accelerator- specific safety requirements are set by DOE Order 420.2b, Safety of Accelerator Facilities. All radiation protection policies and guidelines at NSLS-II must be in compliance with these regulations along with the BNL Radiation Control Manual and other pertinent documents in the BNL Standards Based Management System. The maximum annual exposure limits to radiation workers and members of the public are limited in 10 CFR Part 835 to 5,000 mrem and 100 mrem, respectively. To keep radiation exposures well below regulatory limits, BNL maintains an annual administrative control level of 1,250 mrem for its workers and 5 mrem per year from any single facility to the public off-site. An additional control level of 25 mrem/year from NSLS-II operations is established for personnel working in non-NSLS-II facilities on site and for visitors and minors within the NSLS-II building. The dose to workers and beamline scientists from NSLS-II operations will be kept well below federal limits and within BNL administrative levels through shielding, operational procedures, and administrative controls. Shielding will be provided to reduce radiation levels during normal operation to less than 0.5 mrem/h and as low as reasonably achievable. Assuming an occupancy of 2,000 hours per year, this will reduce annual exposure to 1,000 mrem or less, in accordance with 10 CFR 835.1001.
    [Show full text]
  • X-Ray Optics for Synchrotron Radiation Beamlines
    ESI2013: 3rd EIROforum School on Instrumentation An Introduction to Synchrotron Radiation Ray BARRETT X-ray Optics Group European Synchrotron Radiation Facility e-mail : barrett@esrf.fr Outline Part I Part II Introduction SR Research to synchrotron radiation (SR) Mostly Illustrated by examples from the ESRF 27 May 2013 ESI 2013: Synchrotron Radiation 2 Outline PART I Introduction to synchrotron radiation 1. Origin and physics 2. Historical evolution 3. Synchrotron radiation facilities 4. Three forms of synchrotron radiation 5. Sources and their operation 27 May 2013 ESI 2013: Synchrotron Radiation 3 What’s a synchrotron radiation source? • An extremely intense source of X-rays (also IR & EUV) • Typically produced by highly energetic electrons (or positrons) moving in a large circle in the synchrotron (or more usually Storage Ring). •Highly collimated X-rays are emitted tangentially to the storage ring and simultaneously serve multiple beamlines for scientific applications spanning physical, chemical and life sciences 27 May 2013 ESI 2013: Synchrotron Radiation 4 Origin of synchrotron radiation L. Shklovsky (1953) • Synchrotron radiation is electromagnetic energy emitted by charged particles (e.g., electrons and ions) that are moving at speeds close to that of light when their paths are altered, e.g. by a magnetic field. • It is thus termed because particles moving at such speeds in particle accelerators known as a synchrotrons produce electromagnetic radiation of this type. The Crab Nebula – a natural SR source CHANDRA (2001) 27 May 2013 ESI 2013: Synchrotron Radiation 5 Basic Principles Classical case Relativistic case v << c v ~ c orbit orbit Centripetal acceleration =1/ Isotropic emission Emission concentrated within a narrow forward cone E e mc2 Ee = 6 GeV (ESRF) mc2 = 511keV = 10-4 rad = a few 10-3 deg 27 May 2013 ESI 2013: Synchrotron Radiation 6 Man-made synchrotron radiation 1947 EVOLUTION 1930 First observation First particle of synchrotron accelerators radiation at General Electric First observation (USA).
    [Show full text]
  • Translational Research in FLASH Radiotherapy—From Radiobiological Mechanisms to in Vivo Results
    biomedicines Review Translational Research in FLASH Radiotherapy—From Radiobiological Mechanisms to In Vivo Results Loredana G. Marcu 1,2,* , Eva Bezak 2,3 , Dylan D. Peukert 4,5 and Puthenparampil Wilson 5,6 1 Faculty of Informatics & Science, Department of Physics, University of Oradea, 410087 Oradea, Romania 2 Cancer Research Institute and School of Health Sciences, University of South Australia, Adelaide, SA 5001, Australia; Eva.Bezak@unisa.edu.au 3 School of Physical Sciences, Department of Physics, University of Adelaide, North Terrace, Adelaide, SA 5005, Australia 4 School of Civil, Environmental & Mining Engineering, University of Adelaide, North Terrace, Adelaide, SA 5005, Australia; dylan.peukert@mymail.unisa.edu.au 5 STEM, University of South Australia, Adelaide, SA 5001, Australia; Puthenparampil.Wilson@unisa.edu.au 6 Department of Radiation Oncology, Royal Adelaide Hospital, Adelaide, SA 5000, Australia * Correspondence: loredana@marcunet.com Abstract: FLASH radiotherapy, or the administration of ultra-high dose rate radiotherapy, is a new radiation delivery method that aims to widen the therapeutic window in radiotherapy. Thus far, most in vitro and in vivo results show a real potential of FLASH to offer superior normal tissue sparing compared to conventionally delivered radiation. While there are several postulations behind the differential behaviour among normal and cancer cells under FLASH, the full spectra of radiobiological mechanisms are yet to be clarified. Currently the number of devices delivering FLASH dose rate is few and is mainly limited to experimental and modified linear accelerators. Nevertheless, FLASH research Citation: Marcu, L.G.; Bezak, E.; is increasing with new developments in all the main areas: radiobiology, technology and clinical Peukert, D.D.; Wilson, P.
    [Show full text]
  • Dosimetry in Synchrotron Radiation Beam by Ionization Air Chambers
    ABSOLUTE AIR-KERMA MEASUREMENT IN A SYNCHROTRON RADIATION BEAM BY IONIZATION FREE-AIR CHAMBER M. Bovi(1), R.F. Laitano (1), M. Pimpinella(1), M. P. Toni(1), F. Arfelli (2), K. Casarin(3), D. Dreossi(3), R. H. Menk(3), E. Quai(3), G. Tromba(3), A. Vascotto(3) (1) Istituto Nazionale di Metrologia delle Radiazioni Ionizzanti, ENEA C R Casaccia, cp 2400 Roma, Italy. (2) Department of Physics, University and INFN, Trieste, Via A.Valerio 2, 34127 Trieste, Italy (3) Sincrotrone Trieste SCpA, Strada Statale S.S.14 km 163.5, 34012 Basovizza, Trieste, Italy Corresponding author (name and e-mail address): Maria Pia Toni, toni@casaccia.enea.it ABSTRACT A dosimetric procedure to assure the traceability to the air-kerma standard of the measurements performed in synchrotron radiation beams, was implemented at the “Istituto Nazionale di Metrologia delle Radiazioni Ionizzanti” of ENEA (INMRI-ENEA). To this purpose, absolute air-kerma measurements by the ENEA standard free-air chamber for low energy x-rays have been performed at the SYRMEP (SYnchrotron Radiation for Medical Physics) beamline of the ELETTRA light source in Trieste (Italy) where a program of clinical mammography based on phase contrast imaging has been developed in the framework of the SYRMA project (SYnchrotron Radiation for MAmmography). The synchrotron radiation beams to be characterized were monochromatic x-rays with energy in the range from 8 keV to 35 keV and the reference point for measurements corresponded to the centre of the breast when the patient lies on her support. The absolute air-kerma measurements were also used to calibrate two monitor chambers and an ionization free-air chamber specially designed and realized by ENEA to act as transfer standard in the synchrotron radiation beams.
    [Show full text]
  • Atoms, X-Rays and Synchrotron Radiation: (A. Balerna, LNF-INFN)
    Atoms, X-rays and Synchrotron Radiation Antonella Balerna DAΦNE-Light Facility INFN – Frascati National Laboratory INSPYRE 2017 – INternational School on modern PhYsics and Research 13-17 February 2017 INFN - Frascati National Laboratory Outline • Light • X-rays and Synchrotron radiation sources – X-rays and atoms – X-ray sources • Detectors Basic Principles – Interactions of x-rays with matter – XAFS: EXAFS and XANES • Gas Detectors – Ionization chambers • Conclusions Light Progress in science goes in parallel with the technical progress in producing and using light at different wavelengths to explore the physical world. Light Visible light is only a tiny slice of the electromagnetic spectrum. The entire electromagnetic spectrum of light is huge, spanning from gamma rays on one end to radio waves. Visible Light is the light we can see using our eyes. This tiny human spectrum encompasses a very specific range of wavelengths from about 380 nm to 780 nm. Physiologically we see these frequencies because the photoreceptors in our retinas are sensitive to them. When photons of light hit the photoreceptors this creates an electrochemical signal which is the first step in a fascinating process which ultimately results in us seeing colors. Light and waves Light travels as waves of energy. Waves of light have different wavelengths (the distance between the top of one wave and the top of the next). Different colors of visible light have different wavelengths. 1Å = 10-10 m λ (Å) Electromagnetic Spectrum From a macroscopic to a microscopic world… The wavelength (λ) and frequency (ν) of light are strictly related: the higher the frequency the shorter the wavelength! This is because all light waves move through vacuum at the same speed (c = speed of light) and the equation that relates wavelength and frequency for electromagnetic waves is: λν = c X-rays X-rays discovery While Wilhelm Roentgen was working on the effects of cathode rays during 1895, he discovered X-rays.
    [Show full text]
  • A Brilliant Light for Science
    A BRILLIANT LIGHT FOR SCIENCE Located in Grenoble, THE MOST INTENSE A benchmark for science and innovation France, the European SYNCHROTRON Synchrotron Supported by 21 partner countries, the ESRF Radiation Facility LIGHT SOURCE IN THE is the most intense source of synchrotron (ESRF) is a WORLD light. Inaugurated in 1994, the ESRF shining light on is an international centre of excellence for fundamental research with a strong the international A unique research facility commitment to applied and industrial research scene. Imagine a source that produces X-rays 100 research. Every year, the ultra- billion times brighter than the X-rays used With its 43 highly specialised experimental intense X-ray beams in hospitals, X-rays that allow us to fathom stations, known as “beamlines”, produced at the ESRF the structure of matter down to the minutest each equipped with state-of-the-art attract thousands of detail, at the atomic level. Imagine no further! instrumentation, the ESRF offers scientists X-rays with these outstanding properties research scientists an extremely powerful research tool that is really do exist. They can be found at the ESRF, constantly being upgraded. from both academic where they are produced by the high-energy institutions and electrons that race around the institute’s Its strength also lies in bringing together in industry. emblematic “storage ring”, an accelerator of one facility multidisciplinary teams involving impressive proportions. some of the world’s best scientists, engineers and technicians. Working like a giant microscope, the ESRF offers unparalleled opportunities to explore Every year, thousands of scientists come to materials and living matter.
    [Show full text]
  • Synchrotron Radiation
    Synchrotron Radiation The synchrotron radiation, the emission of very relativistic and ultrarelativistic electrons gyrating in a magnetic field, is the process which dominates much of high energy astrophysics. It was originally observed in early betatron experiments in which electrons were first accelerated to ultrarelativistic energies. This process is responsible for the radio emission from the Galaxy, from supernova remnants and extragalactic radio sources. It is also responsible for the non-thermal optical and X-ray emission observed in the Crab Nebula and possibly for the optical and X-ray continuum emission of quasars. The word non-thermal is used frequently in high energy astrophysics to describe the emission of high energy particles. This an unfortunate terminology since all emission mechanisms are ‘thermal’ in some sense. The word is conventionally taken to mean ‘continuum radiation from particles, the energy spectrum of which is not Maxwellian’. In practice, continuum emission is often referred to as ‘non-thermal’ if it cannot be described by the spectrum of thermal bremsstrahlung or black-body radiation. 1 Motion of an Electron in a Uniform, Static Magnetic field We begin by writing down the equation of motion for a particle of rest mass m0, charge ze and Lorentz factor γ = (1 − v2/c2)−1/2 in a uniform static magnetic field B. d (γm0v) = ze(v × B) (1) dt We recall that the left-hand side of this equation can be expanded as follows: d dv 3 (v · a) m0 (γv) = m0γ + m0γ v (2) dt dt c2 because the Lorentz factor γ should be written γ = (1 − v · v/c2)−1/2.
    [Show full text]
  • Speciation, Techniques and Facilities for Radioactive Materials at Synchrotron Light Sources
    Nuclear Science NEA/NSC/DOC(2009)15 Speciation, techniques and facilities for radioactive materials at synchrotron light sources Actinide XAS 2008 Proceedings of the 5th workshop Saint-Aubin, France 15-17 July 2008 © OECD 2009 NUCLEAR ENERGY AGENCY Organisation for Economic Co-operation and Development ORGANISATION FOR ECONOMIC CO-OPERATION AND DEVELOPMENT The OECD is a unique forum where the governments of 30 democracies work together to address the economic, social and environmental challenges of globalisation. The OECD is also at the forefront of efforts to understand and to help governments respond to new developments and concerns, such as corporate governance, the information economy and the challenges of an ageing population. The Organisation provides a setting where governments can compare policy experiences, seek answers to common problems, identify good practice and work to co-ordinate domestic and international policies. The OECD member countries are: Australia, Austria, Belgium, Canada, the Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Iceland, Ireland, Italy, Japan, Korea, Luxembourg, Mexico, the Netherlands, New Zealand, Norway, Poland, Portugal, the Slovak Republic, Spain, Sweden, Switzerland, Turkey, the United Kingdom and the United States. The Commission of the European Communities takes part in the work of the OECD. OECD Publishing disseminates widely the results of the Organisation’s statistics gathering and research on economic, social and environmental issues, as well as the conventions, guidelines and standards agreed by its members. This work is published on the responsibility of the Secretary-General of the OECD. The opinions expressed and arguments employed herein do not necessarily reflect the official views of the Organisation or of the governments of its member countries.
    [Show full text]
  • SEC-00109, Petition Evaluation Report, Los Alamos National
    SEC Petition Evaluation Report Petition SEC-00109 Report Rev Number: Addendum Report Submittal Date: April 24, 2017 Subject Expert(s): Christopher Miles Site Expert(s): N/A Petition Administrative Summary Petition Under Evaluation Petition Number: SEC-00109 Petition Type: 83.13 Petition Receipt Date: April 3, 2008 Qualification Date: May 29, 2008 DOE/AWE Facility Name: Los Alamos National Laboratory (LANL) Petition Class Class Evaluated by NIOSH: Service Support Workers (which includes, but is not limited to, security guards, firefighters, laborers, custodians, carpenters, plumbers, electricians, pipefitters, sheet metal workers, ironworkers, welders, maintenance workers, truck drivers, delivery persons, rad technicians, and area work coordinators) who worked in any operational Technical Areas with a history of radioactive material use at the Los Alamos National Laboratory from January 1, 1996 through December 31, 2005. NIOSH-Proposed Class(es) to be None Added to the SEC: Related Petition Summary Information SEC Petition Tracking Numbers SEC-00051 (83.13) and Petition Types SEC-00061 (83.14) SEC-00109 (83.13) SEC-00170 (83.14) DOE/AWE Facility Name: Los Alamos National Laboratory (LANL) Petition Status: SEC-00051: Class added to the SEC for Mar. 15, 1943 through Dec. 31, 1975 SEC-00061: Class added to the SEC for Sep. 1, 1944 through Jul. 18, 1963 SEC-00109: Class added to the SEC for Jan. 1, 1976 through Dec. 31, 1995 SEC-00170: Class added to the SEC for Mar. 15, 1943 through Dec. 31, 1975 Related Evaluation Report Information Report Title: SEC Petition Evaluation Report for Petition SEC-00051 SEC Petition Evaluation Report for Petition SEC-00061 SEC Petition Evaluation Report for Petition SEC-00109, Rev.
    [Show full text]
  • The Morphology of the Anomalous Microwave Emission in the Planck 2015 Data Release
    Prepared for submission to JCAP The Morphology of the Anomalous Microwave Emission in the Planck 2015 data release S. von Hauseggera;1 H. Liua;b aThe Niels Bohr Institute and Discovery Center, Blegdamsvej 17, 2100 Copenhagen Ø, Denmark bThe Key laboratory of Particle and Astrophysics, Institute of High Energy Physics, CAS, China E-mail: s.vonhausegger@nbi.dk, liuhao@nbi.dk Abstract. We calculate weighted mosaic correlations between the recently published Planck 2015 foreground maps - both anomalous microwave emission (AME) maps, free-free emission, synchrotron radiation and thermal dust emission. The weighting coefficients are constructed taking account of the signal-to-error ratio given by the data product. Positive correlation is found for AME compared with thermal dust emission as well as synchrotron radiation. We find AME and free-free emission tending to be anti-correlated, however, when investigating different scales, their relationship appears to be more complex. We argue that dust particles responsible for AME are pushed out of hot zones in the interstellar medium (ISM). Keywords: CMBR experiments arXiv:1507.05171v1 [astro-ph.CO] 18 Jul 2015 1Corresponding author. Contents 1 Introduction1 2 The Component Maps2 3 Mosaic Correlation3 3.1 Weighted Mosaic Correlation4 3.2 Weights5 3.3 Assessment of correlations.5 4 K-maps for AME and synchrotron, free-free and dust emission maps7 4.1 Unweighted correlations8 4.2 Weighted correlations 10 4.3 Comparison of weighted and unweighted results 12 5 Conclusion 12 A Additional Figures 15 1 Introduction Following the release of the PLANCK full mission data, cosmology and astro-particle physics are confronted with major challenges concerning the verification of the theories of inflation[1– 4].
    [Show full text]