Diagnostic Studies of Ion Beam Formation in Inductively Coupled Plasma Mass Spectrometry with the Collision Reaction Interface Jeneé L
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Excitation Temperature, Degree of Ionization of Added Iron Species, and Electron Density in an Exploding Thin Film Plasma
SpectmchimiccrACIO. Vol. MB. No. II. Pp.10814096. 1981. 0584-8547/81/111081-16SIZ.CNI/O Printedin Great Britain. PerpmonPress Ltd. Excitation temperature, degree of ionization of added iron species, and electron density in an exploding thin film plasma S. Y. SUH* and R. D. SACKS Department of Chemistry, University of Michigan, Ann Arbor, Ml 48109, U.S.A. (Received 7 April 1981) Abstract-Time and spatially resolved spectra of a cylindrically symmetric exploding thin film plasma were obtained with a rotating mirror camera and astigmatic imaging. These spectra were deconvoluted to obtain relative spectral emissivity profiles for nine Fe(H) and two Fe(I) lines. The effective (electronic) excitation temperature at various positions in the plasma and at various times during the first current halfcycle was computed from the Fe(H) emissivity values using the Boltzmann graphical method. The Fe(II)/Fe(I) emissivity ratios together with the temperature were used to determine the degree of ionization of Fe. Finally, the electron density was estimated from the Saha equilibrium. Electronic excitation temperatures range from lO,OOO-15,OOOKnear the electrode surface at peak discharge current to 700&10.000K at 6-10 mm above the electrode surface at the first current zero. Corresponding electron densities range from 10’7-10u cm-’ at peak current to 10’~-10’6cm-3 near zero current. Error propagation and criteria for thermodynamic equilibrium are discussed. 1. IN-~R~DU~~ION THE HIGH-TEMPERATURE plasmas produced by the rapid electrical vaporization of Ag thin films recently have been used as atomization cells and excitation sources for the direct determination of selected elements in micro-size powder samples [ 11. -
Discussion of the Surface Science of Quasicrystals Patricia Thiel
Discussion of the Surface Science of Quasicrystals Patricia Thiel To cite this version: Patricia Thiel. Discussion of the Surface Science of Quasicrystals. Philosophical Magazine, Taylor & Francis, 2008, 88 (13-15), pp.2123-2129. 10.1080/14786430802186973. hal-00513904 HAL Id: hal-00513904 https://hal.archives-ouvertes.fr/hal-00513904 Submitted on 1 Sep 2010 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Philosophical Magazine & Philosophical Magazine Letters For Peer Review Only Discussion of the Surface Science of Quasicrystals Journal: Philosophical Magazine & Philosophical Magazine Letters Manuscript ID: TPHM-08-Mar-0086.R1 Journal Selection: Philosophical Magazine Date Submitted by the 30-Apr-2008 Author: Complete List of Authors: Thiel, Patricia; Iowa State University, Department of Chemistry Keywords: quasicrystals, surface physics Keywords (user supplied): quasicrystals, surface physics http://mc.manuscriptcentral.com/pm-pml Page 1 of 15 Philosophical Magazine & Philosophical Magazine Letters 1 2 3 Discussion of the Surface Science of Quasicrystals 4 5 6 7 8 Patricia A. Thiel 9 10 11 Ames Laboratory and Department of Chemistry, Iowa State University 12 13 Ames, IA 50011 USA 14 For Peer Review Only 15 16 17 18 19 20 Abstract. -
The Avs 67Th International Symposium & Exhibition
THE AVS 67TH INTERNATIONAL SYMPOSIUM & EXHIBITION On behalf of the AVS, we invite you to submit an abstract to the AVS 67th International Symposium and Exhibition, which will be held October 24 – 29, 2021 in Charlotte, North Carolina. The AVS Symposium is the premier forum for the presentation and discussion of the science and technology of materials, interfaces, and processing. This year, the Symposium’s theme is “Advances in Interfacial Science for Energy and The Environment.” The challenges facing the development and implementation of new energy sources and solutions to outstanding environmental problems have never been more important. The AVS 67th Annual Symposium will highlight the emergent science and technology of materials and techniques for environmental applications and energy transformation. AVS 67 will be an ideal forum for presentation and discussion of your latest results and will provide many opportunities to connect with other engineers and scientists. A sampling of sessions that encompass this theme include: • Electronic and Photonic Devices for Energy Conversion and Storage • Bioenergy and Biomass Conversion • 2D Materials for Electrochemical, Energy, and Environmental Applications • Structural Characterization of Energy Materials • Analysis of Surfaces and Interfaces Related to Energy and the Environment • Astrochemistry and Surfaces for Space and Extreme Environments • Vacuum Technology for Fusion Research • Hybrid Nanomaterials Based on Biologically-Inspired Approaches • Advances in Heterogeneous Electrocatalysis • Atomic Layer Processing: Integration of Deposition and Etching for Advanced Material Processing • Environmental Interfaces • Catalysis at the Metal Oxide Interface • Pushing the Boundaries of Energy Transfer in Materials • MEMS Technology for Energy and Environment • Energy Efficient Nanoelectronics • Plasma-Engineered Materials and Interfaces for the Environment • Electronic Interfaces and Contacts In addition, we will feature programming on innovative topical areas. -
MRS Materials Connections
RESEARCH/RESEARCHERS ness of the TeSW-prepared p-Si is very thin ing orientation. Some recent studies have such efforts for PZN-PT. In the August and the rms roughness is only 1.6 nm. reported frictional differences, or aniso- issue of the Journal of the American Ceramic The researchers also performed a con- tropy, less than a factor of 3 for incom- Society (p. 2310; DOI: 10.111/j.1551- trolled experiment of p-Si formation using mensurate crystal surfaces when there 2916.2005.00391.x), G. Deng and col- NaOH etchant at various pH levels, but were periodicity differences. leagues from the Shanghai Institute of they observed no efficient PL emission To measure the frictional effects due to Ceramics, China, have reported their suc- from any of the NaOH-prepared samples. periodicity alone and not to other factors cess in synthesizing pure perovskite The researchers pointed out that the such as chemical differences, the re- ceramics of PZN-PZT, as an alternative to reproducibility appeared to be a problem searchers worked with decagonal quasi- PZN-PT, near their MPB. The researchers for the photoetched p-Si synthesis tech- crystals of an aluminum-nickel-cobalt (Al- have observed much higher piezoelectric nique. They point out that others have Ni-Co) alloy. Stacked planes of Al-Ni-Co and electromechanical coupling coeffi- suggested that the preexisting state of the crystals exhibit both tenfold and twofold cients for their newly synthesized mate- Si surface plays a decisive role in deter- rotational symmetry. By cutting a single rial than those reported earlier. -
Ionization Balance in EBIT and Tokamak Plasmas N
Ionization balance in EBIT and tokamak plasmas N. J. Peacock, R. Barnsley, M. G. O’Mullane, M. R. Tarbutt, D. Crosby et al. Citation: Rev. Sci. Instrum. 72, 1250 (2001); doi: 10.1063/1.1324755 View online: http://dx.doi.org/10.1063/1.1324755 View Table of Contents: http://rsi.aip.org/resource/1/RSINAK/v72/i1 Published by the American Institute of Physics. Related Articles Bragg x-ray survey spectrometer for ITER Rev. Sci. Instrum. 83, 10E126 (2012) Novel energy resolving x-ray pinhole camera on Alcator C-Mod Rev. Sci. Instrum. 83, 10E526 (2012) Measurement of electron temperature of imploded capsules at the National Ignition Facility Rev. Sci. Instrum. 83, 10E121 (2012) South pole bang-time diagnostic on the National Ignition Facility (invited) Rev. Sci. Instrum. 83, 10E119 (2012) Temperature diagnostics of ECR plasma by measurement of electron bremsstrahlung Rev. Sci. Instrum. 83, 073111 (2012) Additional information on Rev. Sci. Instrum. Journal Homepage: http://rsi.aip.org Journal Information: http://rsi.aip.org/about/about_the_journal Top downloads: http://rsi.aip.org/features/most_downloaded Information for Authors: http://rsi.aip.org/authors Downloaded 08 Aug 2012 to 194.81.223.66. Redistribution subject to AIP license or copyright; see http://rsi.aip.org/about/rights_and_permissions REVIEW OF SCIENTIFIC INSTRUMENTS VOLUME 72, NUMBER 1 JANUARY 2001 Ionization balance in EBIT and tokamak plasmas N. J. Peacock,a) R. Barnsley,b) and M. G. O’Mullane Euratom/UKAEA Fusion Association, Culham Science Centre, Abingdon, Oxon OX14 3DB, United Kingdom M. R. Tarbutt, D. Crosby, and J. D. Silver The Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU, United Kingdom J. -
Minutes for the Basic Energy Sciences Advisory Committee Meeting July 29-30, 1998, Gaithersburg Hilton Hotel, Gaithersburg, Maryland
Minutes for the Basic Energy Sciences Advisory Committee Meeting July 29-30, 1998, Gaithersburg Hilton Hotel, Gaithersburg, Maryland BESAC members present: Boris Batterman Thomas Russell Jack Crow Zhi-Xun Shen Marye Anne Fox (Vice Chair) Sunil Sinha Jan Herbst Richard Smalley Linda Horton David Tirrell Franklin Orr Patricia Thiel Geraldine Richmond (Chair) BESAC members absent: Barbara Garrison Carolyn Meyers Robert Horsch Edel Wasserman Stephen Leone Conrad Williams Marsha Lester Also present: Jim Decker, Deputy Director, ER (Wednesday only) Patricia Dehmer, Associate Director, ER, OBES Martha Krebs, Director, ER (Wednesday afternoon only) Iran Thomas, Deputy Associate Director, ER, OBES and Director, Division of Materials Sciences, OBES July 29, 1998 Chair Geraldine Richmond opened the meeting at 8:30 a.m. She had each committee member introduce himself or herself. She then introduced Patricia Dehmer to provide an overview of the Department of Energy (DOE) and of the Office of Basic Energy Sciences (BES). In her preliminary remarks, Dehmer welcomed the members to the meeting and stressed the importance of this advisory committee, BESAC, pointing out that it produced outcomes as well as outputs. One outcome has been the Birgeneau Report that reviewed the major light-source initiatives; it will be the force in determining funding for those sources, and it has already become part of the vernacular on Capitol Hill. An output has been the analysis of the shutdown of the High-Flux Beam Reactor (HFBR). She pointed out that BESAC already has three charges for this year: to review the High Flux Isotope Reactor (HFIR), to conduct a workshop on fourth-generation light sources, and to conduct a workshop on complex systems. -
How the Saha Ionization Equation Was Discovered
How the Saha Ionization Equation Was Discovered Arnab Rai Choudhuri Department of Physics, Indian Institute of Science, Bangalore – 560012 Introduction Most youngsters aspiring for a career in physics research would be learning the basic research tools under the guidance of a supervisor at the age of 26. It was at this tender age of 26 that Meghnad Saha, who was working at Calcutta University far away from the world’s major centres of physics research and who never had a formal training from any research supervisor, formulated the celebrated Saha ionization equation and revolutionized astrophysics by applying it to solve some long-standing astrophysical problems. The Saha ionization equation is a standard topic in statistical mechanics and is covered in many well-known textbooks of thermodynamics and statistical mechanics [1–3]. Professional physicists are expected to be familiar with it and to know how it can be derived from the fundamental principles of statistical mechanics. But most professional physicists probably would not know the exact nature of Saha’s contributions in the field. Was he the first person who derived and arrived at this equation? It may come as a surprise to many to know that Saha did not derive the equation named after him! He was not even the first person to write down this equation! The equation now called the Saha ionization equation appeared in at least two papers (by J. Eggert [4] and by F.A. Lindemann [5]) published before the first paper by Saha on this subject. The story of how the theory of thermal ionization came into being is full of many dramatic twists and turns. -
Congratulations to the New 25 Year Club Members of 2010
CONGRATULATIONS TO THE NEW 25 YEAR CLUB MEMBERS OF 2010 TWENTY-FIVE YEAR HONOREES The following persons completed 25 years of employment at ISU during the calendar year of 2008. New members being welcomed to this honored organization are: DIVISION OF THE PRESIDENT Cindy Van Loon Human Resource Services DIVISION OF ACADEMIC AFFAIRS COLLEGE OF AGRICULTURE & LIFE SCIENCES Dennis Garvey Animal Science Catherine Good Ag Exp Stn Administration Martha Jeffrey Animal Science Danny Johnson Animal Science Randy Killorn Agronomy Susan Lamont Animal Science Robert Martin Ag Education Sally Medford IA State Research Farms Pamela Mundt Agronomy Donna Nelson Animal Science Jonathan Sandor Agronomy Ann Shuey Animal Science Jeffrey Thorson Animal Science Helene Uhlenhopp Agronomy COLLEGE OF BUSINESS Ronald Ackerman Business Graduate Program Farhad Choobineh Log Operation & Mis Mark Power Finance Jenison Stoehr Log Operations and MIS COLLEGE OF DESIGN Clare Cardinal-Pett Architecture COLLEGE OF ENGINEERING Robert Abendroth Civ/Con/ Env Engineering Linda Edson Chemical & Bio Engineering Jeffrey Eichorn Ind/ Manufacturing Systems Engineering Scott Schlorholtz Materials Science and Engineering Martha Selby Materials Science and Engineering Terry Wipf Civ/Con/Env Eng COLLEGE OF HUMAN SCIENCES Marcia Rosenbusch Curriculum/ Instruction COLLEGE OF LIBERAL ARTS & SCIENCES Barbara Blakely English Michael Duffy Economics Sally Gleason Chemistry Kristy Goodale Mathematics Margaret Graham English J Arne Hallam Economics Paul Hollander Chemistry Margaret Holmgren Philosophy/ -
1 Introduction
i i Karl-Heinz Spatschek: High Temperature Plasmas — Chap. spatscheck0415c01 — 2011/9/1 — page 1 — le-tex i i 1 1 Introduction A plasma is a many body system consisting of a huge number of interacting (charged and neutral) particles. More precisely, one defines a plasma as a quasineu- tral gas of charged and neutral particles which exhibits collective behavior. In many cases, one considers quasineutral gases consisting of charged particles, namely electrons and positively charged ions of one species. Plasmas may contain neutral atoms. In this case, the plasma is called partially or incompletely ionized. Other- wise the plasma is said to be completely or fully ionized. The term plasma is not limited to the most common electron–ion case. One may have electron–positron plasmas, quark-gluon plasmas, and so on. Semiconductors contain plasma con- sisting of electrons and holes. Most of the matter in the universe occurs in the plasma state. It is often said that 99% of the matter in the universe is in the plasma state. However, this estimate may not be very accurate. Remember the discussion on dark matter. Nevertheless, the plasma state is certainly dominating the universe. Modern plasma physics emerged in 1950s, when the idea of thermonuclear re- actor was introduced. Fortunately, modern plasma physics completely dissociated from weapons development. The progression of modern plasma physics can be retraced from many monographs, for example, [1–15]. In simple terms, plasmas can be characterized by two parameters, namely, charged particle density n and temperature T. The density varies over roughly 28 6 34 3 orders of magnitude, for example, from 10 to 10 m . -
Lecture 8: Statistical Equilibria, Saha Equation
Statistical Equilibria: Saha Equation We are now going to consider the statistics of equilibrium. Specifically, suppose we let a system stand still for an extremely long time, so that all processes can come into balance. We then measure the fraction of particles that are in each of several states (e.g., if we have a pure hydrogen gas, we might want to know the ionization fraction). How can we compute this fraction? We’ll take a look at this in several different ways. We will then step back and ask ourselves when these equilibrium formulae do not apply. This is important! To paraphrase Clint Eastwood, “An equation’s got to know its limitations”. In virtually all astronomical problems we deal with approximations, so we always need a sense of when those approximations fail. This serves a double purpose: it keeps us from making errors, but it also keeps us from applying too complex an approach to a simple problem. Let’s start out with a simple case. We consider a column of isothermal gas (temperature T ) in a constant gravitational acceleration g. Each molecule has mass m. If we can treat this like an ideal gas, Ask class: how do we figure out how the pressure vary with height h? An ideal gas has pressure P = nkT , where n is the number density. In equilibrium the pressure gradient balances the weight of the gas, so dP/dh = −ρg. Using ρ = nm = P m/kT and the constancy of T , we have dP/dh = −(mg/kT )P , so P = P0 exp(−mgh/kT ), where P0 is defined as the pressure at h = 0. -
Example 1 Nicotinic Acid Is a Monoprotic Acid
Weak acids and bases Example 1 Nicotinic acid is a monoprotic acid. A solution that is 0.012 M in nicotinic acid has a pH of 3.39. What is the acid ionization constant (Ka)? What is the degree of ionization of nicotinic acid in this solution? Solution When we say the solution is 0.012 M, this refers to how the solution is prepared. The solution is made up by adding 0.012 mol of substance to enough water to give a liter of solution. Once the solution is prepared, some molecules ionize, so the actual concentration is somewhat less than 0.012 M. - + We start with 0.012 M of acid (HNic) before ionization, i.e. [Nic ]=0 before ionization. The H3O concentration at the start is that from the self-ionization of water. It is usually much smaller than that obtained from the acid (unless the solution is extremely dilute or Ka is quite small), so you can write + + – [H3O ] = ~ 0 (meaning approximately zero). If x mol HNic ionizes, x mol each of H3O and Nic is formed, leaving (0.012 - x) mol HNic in solution. You can summarize the situation in the table: + – Concentration (M) HNic(aq) + H2O(l) <==> H3O (aq) + Nic (aq) Starting 0.012 ~0 0 Change -x +x +x Equilibrium 0.012 - x x x The equilibrium-constant equation is + – [H3O ][Nic ] Ka = [HNic] When you substitute the expressions for the equilibrium concentrations, you get x2 Ka = (0.012 - x) The value of x equals the numerical value of the molar hydronium-ion concentration, and can be obtained from the pH of the solution. -
Lecture Notes in Physics Introduction to Plasma Physics
Lecture Notes in Physics Introduction to Plasma Physics Michael Gedalin ii Contents 1 Basic definitions and parameters 1 1.1 What is plasma . 1 1.2 Debye shielding . 2 1.3 Plasma parameter . 4 1.4 Plasma oscillations . 5 1.5 ∗Ionization degree∗ ............................ 5 1.6 Summary . 6 1.7 Problems . 7 2 Plasma description 9 2.1 Hierarchy of descriptions . 9 2.2 Fluid description . 10 2.3 Continuity equation . 10 2.4 Motion (Euler) equation . 11 2.5 State equation . 12 2.6 MHD . 12 2.7 Order-of-magnitude estimates . 14 2.8 Summary . 14 2.9 Problems . 15 3 MHD equilibria and waves 17 3.1 Magnetic field diffusion and dragging . 17 3.2 Equilibrium conditions . 18 3.3 MHD waves . 19 3.4 Alfven and magnetosonic modes . 22 3.5 Wave energy . 23 3.6 Summary . 24 3.7 Problems . 24 iii CONTENTS 4 MHD discontinuities 27 4.1 Stationary structures . 27 4.2 Discontinuities . 28 4.3 Shocks . 29 4.4 Why shocks ? . 31 4.5 Problems . 32 5 Two-fluid description 33 5.1 Basic equations . 33 5.2 Reduction to MHD . 34 5.3 Generalized Ohm’s law . 35 5.4 Problems . 36 6 Waves in dispersive media 37 6.1 Maxwell equations for waves . 37 6.2 Wave amplitude, velocity etc. 38 6.3 Wave energy . 40 6.4 Problems . 44 7 Waves in two-fluid hydrodynamics 47 7.1 Dispersion relation . 47 7.2 Unmagnetized plasma . 49 7.3 Parallel propagation . 49 7.4 Perpendicular propagation . 50 7.5 General properties of the dispersion relation .