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Comparing the Emission Spectra of U and Th Hollow Cathode Lamps and a New U Line-List
Astronomy & Astrophysics manuscript no. HCL_U_Th_Ull_S2018 c ESO 2018 October 1, 2018 Comparing the emission spectra of U and Th hollow cathode lamps and a new U line-list L. F. Sarmiento1,⋆, A. Reiners1, P. Huke1, F. F. Bauer1, E. W. Guenter2,3, U. Seemann1, and U. Wolter4 1 Institut für Astrophysik, Georg-August-Universität Göttingen, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany 2 Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany 3 Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife, Spain 4 Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany Received , 22 February 2018; accepted , 5 June 2018 ABSTRACT Context. Thorium hollow cathode lamps (HCLs) are used as frequency calibrators for many high resolution astronomical spectro- graphs, some of which aim for Doppler precision at the 1 m/s level. Aims. We aim to determine the most suitable combination of elements (Th or U, Ar or Ne) for wavelength calibration of astronomical spectrographs, to characterize differences between similar HCLs, and to provide a new U line-list. Methods. We record high resolution spectra of different HCLs using a Fourier transform spectrograph: (i) U-Ne, U-Ar, Th-Ne, and Th-Ar lamps in the spectral range from 500 to 1000 nm and U-Ne and U-Ar from 1000 to 1700 nm; (ii) we systematically compare the number of emission lines and the line intensity ratio for a set of 12 U-Ne HCLs; and (iii) we record a master spectrum of U-Ne to create a new U line-list. Results. Uranium lamps show more lines suitable for calibration than Th lamps from 500 to 1000 nm. -
Mössbauer Spectroscopy 9.1 Recoil Free Resonance Absorption
Chapter 9, page 1 9 Mössbauer Spectroscopy 9.1 Recoil free resonance absorption Robert Wood published in 1905 an article "Resonance Radiation of Sodium Vapor" (see Literature) and reported that if a bulb containing pure sodium vapor was illuminated by light from a sodium flame, the vapor emitted a yellow light which spectroscopic analysis showed to be identical with the exciting light, in other words, the two D lines. Sodium is liquid above 98 °C, boiling point 883 °C, thus a remarkable vapor pressure exists, if sodium is heated by the Fig. 9.1: Wood's apparatus for the Bunsen burner above 200 °C. Wood used the name resonance radiation of the sodium "resonance radiation" for the effect of identical D lines. absorbed radiation and fluorescence radiation. Now we use the term "resonance absorption" instead. Since 1900 γ-rays were known as a highly energetic monochromatic radiation, but the anticipated γ-ray resonance fluorescence failed to occur. Werner Kuhn succeeded in publishing such an experiment that don't work and argued in 1929: "The (third) influence, reducing the absorption, arises from the emission process of the γ-rays. The emitting atom will suffer recoil due to the projection of the γ-ray. The wavelength of the radiation is therefore shifted to the red; the emission line is displaced relative to the absorption line.... It is thus possible that by a large γ-shift, the whole emission line is brought out of the absorption region”. (see Literature, Kuhn) Intensity In the case of γ-radiation the atoms suffer recoil, which is not significant for radiation in the visible range, were the recoil energy is small compared with the linewidth of the h δν1/2 radiation (times h), see Fig. -
Stark Broadening of Spectral Lines in Plasmas
atoms Stark Broadening of Spectral Lines in Plasmas Edited by Eugene Oks Printed Edition of the Special Issue Published in Atoms www.mdpi.com/journal/atoms Stark Broadening of Spectral Lines in Plasmas Stark Broadening of Spectral Lines in Plasmas Special Issue Editor Eugene Oks MDPI • Basel • Beijing • Wuhan • Barcelona • Belgrade Special Issue Editor Eugene Oks Auburn University USA Editorial Office MDPI St. Alban-Anlage 66 4052 Basel, Switzerland This is a reprint of articles from the Special Issue published online in the open access journal Atoms (ISSN 2218-2004) in 2018 (available at: https://www.mdpi.com/journal/atoms/special issues/ stark broadening plasmas) For citation purposes, cite each article independently as indicated on the article page online and as indicated below: LastName, A.A.; LastName, B.B.; LastName, C.C. Article Title. Journal Name Year, Article Number, Page Range. ISBN 978-3-03897-455-0 (Pbk) ISBN 978-3-03897-456-7 (PDF) Cover image courtesy of Eugene Oks. c 2018 by the authors. Articles in this book are Open Access and distributed under the Creative Commons Attribution (CC BY) license, which allows users to download, copy and build upon published articles, as long as the author and publisher are properly credited, which ensures maximum dissemination and a wider impact of our publications. The book as a whole is distributed by MDPI under the terms and conditions of the Creative Commons license CC BY-NC-ND. Contents About the Special Issue Editor ...................................... vii Preface to ”Stark Broadening of Spectral Lines in Plasmas” ..................... ix Eugene Oks Review of Recent Advances in the Analytical Theory of Stark Broadening of Hydrogenic Spectral Lines in Plasmas: Applications to Laboratory Discharges and Astrophysical Objects Reprinted from: Atoms 2018, 6, 50, doi:10.3390/atoms6030050 ................... -
Quantitative Analysis of Cerium-Gallium Alloys Using a Hand-Held Laser Induced Breakdown Spectroscopy Device
atoms Article Quantitative Analysis of Cerium-Gallium Alloys Using a Hand-Held Laser Induced Breakdown Spectroscopy Device Ashwin P. Rao 1 , Matthew T. Cook 2 , Howard L. Hall 2,3 and Michael B. Shattan 1,* 1 Air Force Institute of Technology, 2950 Hobson Way, WPAFB, OH 45433, USA 2 Institute for Nuclear Security, University of Tennessee, Knoxville, TN 37996, USA 3 Department of Nuclear Engineering, University of Tennessee, Knoxville, TN 37996, USA * Correspondence: michael.shattan@afit.edu Received: 26 July 2019; Accepted: 20 August 2019; Published: 22 August 2019 Abstract: A hand-held laser-induced breakdown spectroscopy device was used to acquire spectral emission data from laser-induced plasmas created on the surface of cerium-gallium alloy samples with Ga concentrations ranging from 0–3 weight percent. Ionic and neutral emission lines of the two constituent elements were then extracted and used to generate calibration curves relating the emission line intensity ratios to the gallium concentration of the alloy. The Ga I 287.4-nm emission line was determined to be superior for the purposes of Ga detection and concentration determination. A limit of detection below 0.25% was achieved using a multivariate regression model of the Ga I 287.4-nm line ratio versus two separate Ce II emission lines. This LOD is considered a conservative estimation of the technique’s capability given the type of the calibration samples available and the low power (5 mJ per 1-ns pulse) and resolving power (l/Dl = 4000) of this hand-held device. Nonetheless, the utility of the technique is demonstrated via a detailed mapping analysis of the surface Ga distribution of a Ce-Ga sample, which reveals significant heterogeneity resulting from the sample production process. -
Emission Mössbauer Spectroscopy at ISOLDE/CERN
Emission Mössbauer Spectroscopy at ISOLDE/CERN Torben Esmann Mølholt ISOLDE Seminar, 25. Nov. 2015 Outline Experimental setup at ISOLDE Brief on the Mössbauer spectroscopy technique Examples and Results Future/ongoing measurements 2 Acknowledgements The Mössbauer collaboration at ISOLDE/CERN, >30 active members with new members (2014) from China, Russia, Bulgaria, Austria, Spain: Four experiments Existing members New members 2014 (IS-501, IS-576, IS-578, I-161) 3 Emission Mössbauer Spectroscopy at ISOLDE/CERN http://e-ms.web.cern.ch/ GLM (GPS) LA1-2 (HRS) 4 119In RILIS 2014 2015 57Mn 119 RILIS In 15 μSi/h - 57Mn 10 μSi/h - RILIS 5 μSi/h - 0 μSi/h - 5 Mössbauer Experimental setup Implantation chamber Incoming 60 keV beam Sample Faraday cup Be window Mössbauer drive with resonance detector Container: 25 mbar acetone • Intensity (~1×108 atoms/s) • High statistics spectrum (5 – 10 min.) •On-line (short lived) •Collections for Off-line (long lived) 6 •Hours - days Mössbauer Experimental setup Sample holder •Temperature range 90 – 700 K • Measurements at different emission angles • Applied magnetic field (Bext ≤ 0.6 T) 7 Mössbauer Experimental setup Sample holder • Quenching: Implant at high temperature Measure at low temperature (off-line) 8 Mössbauer Experimental setup Resonance detector - G. Weyer, Mössbauer Eff. Meth., 10 (1976) 301 PPAD: Parallel Plate Avalanche Detector - Single line resonance detector. 0.1 cps (~0.1 µCi) – 50k cps (~500 mCi) 9 Mössbauer spectroscopy technique 10 40-60 keV Ion-implantation of Mössbauer Probe Emission -
Rietmann St., Biela J., Sensor Design for a Current Measurement System with High Bandwidth and High
Sensor Design for a Current Measurement System with High Bandwidth and High Accuracy Based on the Faraday Effect St. Rietmann, J. Biela Power Electronic Systems Laboratory, ETH Zürich Physikstrasse 3, 8092 Zürich, Switzerland „This material is posted here with permission of the IEEE. Such permission of the IEEE does not in any way imply IEEE endorsement of any of ETH Zürich’s products or services. Internal or personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional pur- poses or for creating new collective works for resale or redistribution must be obtained from the IEEE by writing to [email protected]. By choosing to view this document you agree to all provisions of the copyright laws protecting it.” Sensor Design for a Current Measurement System with High Bandwidth and High RIETMANN Stefan Accuracy Based on the Faraday Effect Sensor Design for a Current Measurement System with High Bandwidth and High Accuracy Based on the Faraday Effect Stefan Rietman and Jurgen¨ Biela Laboratory for High Power Electronic Systems, ETH Zurich, Switzerland Keywords Current Sensor, Sensor, Transducer, Frequency-Domain Analysis Abstract This paper presents the design of the optical system of a current sensor with a wide bandwidth and a high accuracy. The principle is based on the Faraday effect, which describes the effect of magnetic fields on linearly polarized light in magneto-optical material. To identify suitable materials for the optical system the main requirements and specification are determined. A theoretical description of the optical system shows a maximal applicable magnetic field frequency due to the finite velocity of light inside the material. -
Production Scientifique 2004-2007
Production scientifique 2004-2007 Articles parus dans des revues internationales ou nationales avec comité de lecture 2004 • H. Bandulet, C. Labaune, K. Lewis and S. Depierreux, Thomson scattering study of the subharmonic decay of ion-acoustic waves driven by the Brillouin instability, Phys. Rev. Lett. 93, 035002 (2004) • S. Bastiani-Ceccotti, P. Audebert, V. Nagels-Silvert, J.P. Geindre, J.C. Gauthier, J.C. Adam, A. Héron and C. Chenais- Popovics, Time-resolved analysis of the x-ray emission of femtosecond-laser-produced plasmas in the 1.5-keV range, Appl. Phys. B 78, 905 (2004) • D. Batani, F. Strati, H. Stabile, M. Tomasini, G. Lucchini, A. Ravasio, M. Koenig, A. Benuzzi-Mounaix, H. Nishimura, Y. Ochi, J. Ullschmied, J. Skala, B. Kralikova, M. Pfeifer, C. Kadlec, T. Mocek, A. Prag, T. Hall, P. Milani, E. Barborini and P. Piseri, Hugoniot data for carbon at megabar pressures, Phys. Rev. Lett. 92, 065503 (2004) • A. Benuzzi-Mounaix, M. Koenig, G. Huse, B. Faral, N. Grandjouan, D. Batani, E. Henry, M. Tomasini, T. Hall and F. Guyot, Generation of a double shock driven by laser, Phys. Rev. E 70, 045401 (2004) • S. Bouquet, C. Stehlé, M. Koenig, J.P. Chièze, A. Benuzzi-Mounaix, D. Batani, S. Leygnac, X. Fleury, H. Merdji, C. Michaut, F. Thais, N. Grandjouan, T. Hall, E. Henry, V. Malka and J.P. Lafon, Observations of laser driven supercritical radiative shock precursors, Phys. Rev. Lett. 92, 225001 (2004) • P. Celliers, G. Collins, D. Hicks, M. Koenig, E. Henry, A. Benuzzi-Mounaix, D. Batani, D. Bradley, L. Da Silva, R. -
Structuraland Magnetic Properties of Er3fe5-Xalxo12 Garnets
CHAPTER 3 Structural and Magnetic Properties of Er3Fe5-xAlxO12 Garnets Ibrahim Bsoul1,a, Khaled Hawamdeh1,b, Sami H. Mahmood2,c 1Physics Department, Al al-Bayt University, Mafraq 13040, Jordan 2Physics Department, The University of Jordan, Amman 11942, Jordan [email protected], [email protected], [email protected] Abstract Er3Fe5-xAlxO12 (0.0 ≤ x ≤ 0.8) garnets were prepared by ball milling and sintering at 1300ºC. Rietveld refinement of the samples revealed a garnet structure with Ia3d symmetry. The lattice parameter, cell volume, X-ray density and magnetization of the prepared garnets decreased with the increase of Al content (x). The coercivity of the garnets increased with x, but remained generally low, being below 20 Oe. Low temperature magnetic measurements versus temperature indicated that the magnetization of x = 0.0 exhibited a compensation temperature at ˗186º C, however, x = 0.8 exhibited a minimum at a higher temperature of ˗134º C. Keywords Rare Earth Iron Garnet; Structural Characteristics; Magnetic Properties; Compensation Temperature; Thermomagnetic curves. Contents 1. Introduction 2. Experimental procedures 3. Results and discussion 3.1 XRD measurements 3.2 Magnetic measurements 3.3 Temperature dependence of the magnetic properties 3.4 Low temperature measurements 4. Conclusions References 1. INTRODUCTION Ferrimagnetic garnets exemplified by yttrium iron garnet (YIG) was discovery in 1956, and received considerable interest due to their low dielectric losses and remarkable performance in microwave devices and magnetic bubbles for digital memories [1, 2], in addition to their importance in the field of fundamental magnetism. The garnets have a cubic crystal structure 3+ 3+ 3+ 2− 3+ with space group Ia3d and chemical formula {R3 }c[Fe2 ]a(Fe3 )d O12 , where R is a trivalent rare-earth ion occupying dodecahedral (c) sites, and Fe3+ ions occupy octahedral [a- sublattice] and tetrahedral (d-sublattice) sites in the garnet lattice. -
Glossary of Terms Absorption Line a Dark Line at a Particular Wavelength Superimposed Upon a Bright, Continuous Spectrum
Glossary of terms absorption line A dark line at a particular wavelength superimposed upon a bright, continuous spectrum. Such a spectral line can be formed when electromag- netic radiation, while travelling on its way to an observer, meets a substance; if that substance can absorb energy at that particular wavelength then the observer sees an absorption line. Compare with emission line. accretion disk A disk of gas or dust orbiting a massive object such as a star, a stellar-mass black hole or an active galactic nucleus. An accretion disk plays an important role in the formation of a planetary system around a young star. An accretion disk around a supermassive black hole is thought to be the key mecha- nism powering an active galactic nucleus. active galactic nucleus (agn) A compact region at the center of a galaxy that emits vast amounts of electromagnetic radiation and fast-moving jets of particles; an agn can outshine the rest of the galaxy despite being hardly larger in volume than the Solar System. Various classes of agn exist, including quasars and Seyfert galaxies, but in each case the energy is believed to be generated as matter accretes onto a supermassive black hole. adaptive optics A technique used by large ground-based optical telescopes to remove the blurring affects caused by Earth’s atmosphere. Light from a guide star is used as a calibration source; a complicated system of software and hardware then deforms a small mirror to correct for atmospheric distortions. The mirror shape changes more quickly than the atmosphere itself fluctuates. -
Arxiv:Cond-Mat/0404626V1
LA-UR-03-8735 Nuclear Magnetic Resonance Studies of δ-Stabilized Plutonium N. J. Curro Condensed Matter and Thermal Physics, Los Alamos National Laboratory, Los Alamos, NM 87545, [email protected] L. Morales Nuclear Materials and Technology Division, Los Alamos National Laboratory, Los Alamos, NM 87545 (Dated: July 14, 2018) Nuclear Magnetic Resonance studies of Ga stabilized δ-Pu reveal detailed information about the local distortions surrounding the Ga impurities as well as provides information about the local spin fluctuations experienced by the Ga nuclei. The Ga NMR spectrum is inhomogeneously broadened by a distribution of local electric field gradients (EFGs), which indicates that the Ga experiences local distortions from cubic symmetry. The Knight shift and spin lattice relaxation rate indicate that the Ga is dominantly coupled to the Fermi surface via core polarization, and is inconsistent with magnetic order or low frequency spin correlations. Introduction tuations of of the electron spin S relax the nuclei so fast that their signal is rendered invisible. On the other hand, The investigavtion of the low temperature properties the hyperfine coupling to the nuclei of the secondary el- of plutonium and its compounds has experienced a re- ement (Al, Ga or In) are typically one to three orders of naissance in recent years, and several important experi- magnitude smaller, so by measuring the secondary nuclei ments have revealed unusual correlated electron behavior one can gain considerable insight into the spin dynamics [1, 2, 3]. The 5f electrons in elemental plutonium are on of the system. the boundary between localized and itinerant behavior, One of the challenges facing band theorists calculating so that slight perturbations in the Pu-Pu spacing can give the electronic structure of δ-Pu is the role of the sec- rise to dramatic changes in the ground state character. -
Faraday Rotator Based on TSAG Crystal with <001> Orientation
Vol. 24, No. 14 | 11 Jul 2016 | OPTICS EXPRESS 15486 Faraday rotator based on TSAG crystal with <001> orientation 1* 2 2 RYO YASUHARA, ILYA SNETKOV, ALEKSEY STAROBOR, ЕVGENIY 2 2 MIRONOV, AND OLEG PALASHOV 1National Institute for Fusion Science, 322-6, Oroshi-cho, Toki, Gifu 509-5292, Japan 2Institute of Applied Physics of the Russian Academy of Sciences, 46 Ulyanov Street, Nizhny Novgorod, 603950, Russia *[email protected] Abstract: A Faraday isolator (FI) for high-power lasers with kilowatt-level average power and 1-µm wavelength was demonstrated using a terbium scandium aluminum garnet (TSAG) with its crystal axis aligned in the <001> direction. Furthermore, no compensation scheme for thermally induced depolarization in a magnetic field was used. An isolation ratio of 35.4 dB (depolarization ratio γ of 2.9 × 10−4) was experimentally observed at a maximum laser power of 1470 W. This result for room-temperature FIs is the best reported, and provides a simple, practical solution for achieving optical isolation in high-power laser systems. ©2016 Optical Society of America OCIS codes: (160.3820) Magneto-optical materials; (140.6810) Thermal effects. References and links 1. D. J. Gauthier, P. Narum, and R. W. Boyd, “Simple, compact, high-performance permanent-magnet Faraday isolator,” Opt. Lett. 11(10), 623–625 (1986). 2. R. Wynands, F. Diedrich, D. Meschede, and H. R. Telle, “A compact tunable 60dB Faraday optical isolator for the near infrared,” Rev. Sci. Instrum. 63(12), 5586–5590 (1992). 3. S. Banerjee, K. Ertel, P. D. Mason, P. J. Phillips, M. Siebold, M. Loeser, C. -
Pulsed Laser Deposition of High-Quality Μm-Thick YIG Films on YAG
Pulsed laser deposition of high-quality μm-thick YIG films on YAG A. Sposito,1,* T. C. May-Smith,1 G. B. G. Stenning,2 P. A. J. de Groot,2 and R. W. Eason1 1Optoelectronics Research Centre, University of Southampton, SO17 1BJ, Southampton, United Kingdom 2Physics and Astronomy, University of Southampton, SO17 1BJ, Southampton, United Kingdom *[email protected] Abstract: We report the epitaxial growth of high-quality μm-thick yttrium iron garnet (YIG) films on yttrium aluminium garnet (YAG) substrates by pulsed laser deposition (PLD). The effects of substrate temperature and oxygen pressure on composition, crystallinity, optical transmission and ferromagnetic resonance (FMR) linewidth have been investigated. An FMR linewidth as low as 1.75 mT at 6 GHz was achieved by depositing YIG on YAG substrates with (100) orientation at a substrate temperature of ~1600 K and with oxygen pressure of ~1 Pa. ©2013 Optical Society of America OCIS codes: (160.3820) Magneto-optical materials; (310.1860) Deposition and fabrication. References and links 1. R. W. Eason, Pulsed Laser Deposition of Thin Films – Applications-led Growth of Functional Materials (Wiley Interscience, 2007). 2. N. A. Vainos, C. Grivas, C. Fotakis, R. W. Eason, A. A. Anderson, D. S. Gill, D. P. Shepherd, M. Jelinek, J. Lancok, and J. Sonsky, “Planar laser waveguides of Ti:sapphire, Nd:GGG and Nd:YAG grown by pulsed laser deposition,” Appl. Surf. Sci. 127-129, 514–519 (1998). 3. H. Dötsch, N. Bahlmann, O. Zhuromskyy, M. Hammer, L. Wilkens, R. Gerhardt, P. Hertel, and A. F. Popkov, “Applications of magneto-optical waveguides in integrated optics: review,” J.