Introductory Raman Spectroscopy (Second Edition) Elsevier, 2003
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A Customized Stand-Alone Photometric Raman Sensor Applicable in Explosive Atmospheres: a Proof-Of-Concept Study
J. Sens. Sens. Syst., 7, 543–549, 2018 https://doi.org/10.5194/jsss-7-543-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. A customized stand-alone photometric Raman sensor applicable in explosive atmospheres: a proof-of-concept study Marcel Nachtmann1, Shaun Paul Keck1, Frank Braun1, Hanns Simon Eckhardt2, Christoph Mattolat2, Norbert Gretz3, Stephan Scholl4, and Matthias Rädle1 1Institute for Process Control and Innovative Energy Conversion, Mannheim University of Applied Sciences, Mannheim, 68163, Germany 2tec5 AG, Oberursel/Ts, 61440, Germany 3Medical Research Center, Medical Faculty Mannheim, Heidelberg University, Mannheim, 68167, Germany 4Institute for Chemical and Thermal Process Engineering, Technical University Braunschweig, Braunschweig, 38106, Germany Correspondence: Matthias Rädle ([email protected]) Received: 29 March 2018 – Revised: 12 September 2018 – Accepted: 14 September 2018 – Published: 12 October 2018 Abstract. This paper presents an explosion-proof two-channel Raman photometer designed for chemical pro- cess monitoring in hazardous explosive atmospheres. Due to its design, alignment of components is simplified and economic in comparison to spectrometer systems. Raman spectrometers have the potential of becoming an increasingly important tool in process analysis technologies as part of molecular-specific concentration monitor- ing. However, in addition to the required laser power, which restricts use in potentially explosive atmospheres, the financial hurdle is also high. Within the scope of a proof of concept, it is shown that photometric measure- ments of Raman scattering are possible. The use of highly sensitive detectors allows the required excitation power to be reduced to levels compliant for operation in potentially explosive atmospheres. -
Southwest Retort
SOUTHWEST RETORT SIXTY-NINTH YEAR OCTOBER 2016 Published for the advancement of Chemists, Chemical Engineers and Chemistry in this area published by The Dallas-Fort Worth Section, with the cooperation of five other local sections of the American Chemical Society in the Southwest Region. Vol. 69(2) OCTOBER 2016 Editorial and Business Offices: Contact the Editor for subscription and advertisement information. Editor: Connie Hendrickson: [email protected] Copy Editor: Mike Vance, [email protected] Business Manager: Danny Dunn: [email protected] The Southwest Retort is published monthly, September through May, by the Dallas-Ft. Worth Section of the American Chemical Society, Inc., for the ACS Sections of the Southwest Region. October 2016 Southwest RETORT 1 TABLE OF CONTENTS Employment Clearing House………….......3 Fifty Years Ago……………………….….....6 ARTICLES and COLUMNS Schulz Award Winner Gale Hunt………….7 And Another Thing……………………….11 Around the Area………………………….14 Letter from the Editor….…..……….........17 SPECIAL EVENTS National Chemistry Week…………………9 NEWS SHORTS Former pesticide ingredient found in dolphins, birds and fish……………………8 Coffee-infused foam removes lead from contaminated water………………………10 Snake venom composition could be related to hormones and diet……………………..13 Detecting blood alcohol content with an electronic skin patch………………...……16 INDEX OF ADVERTISERS Huffman Laboratories……………....……..4 Contact the DFW Section Vance Editing…..…………….…….……….4 General: [email protected] UT Arlington………………………………..4 Education: [email protected] ANA-LAB……………………...….…...……5 Elections: [email protected] Facebook: DFWACS Twitter: acsdfw October 2016 Southwest RETORT 2 EMPLOYMENT CLEARING HOUSE Job applicants should send name, email, and phone, along with type of position and geographical area desired; employers may contact job applicants directly. -
Input-Output Transfer Function Analysis of a Photometer Circuit Based on an Operational Amplifier
Sensors 2008, 8, 35-50 sensors ISSN 1424-8220 © 2008 by MDPI www.mdpi.org/sensors Input-output Transfer Function Analysis of a Photometer Circuit Based on an Operational Amplifier Wilmar Hernandez Department of Circuits and Systems in the EUIT de Telecomunicacion at the Universidad Politecnica de Madrid (UPM), Campus Sur UPM, Ctra. Valencia km 7, Madrid 28031, Spain Phone: +34913367830. Fax: +34913367829. E-mail: [email protected] Received: 22 December 2007 / Accepted: 7 January 2008 / Published: 9 January 2008 Abstract: In this paper an input-output transfer function analysis based on the frequency response of a photometer circuit based on operational amplifier (op amp) is carried out. Op amps are universally used in monitoring photodetectors and there are a variety of amplifier connections for this purpose. However, the electronic circuits that are usually used to carry out the signal treatment in photometer circuits introduce some limitations in the performance of the photometers that influence the selection of the op amps and other electronic devices. For example, the bandwidth, slew-rate, noise, input impedance and gain, among other characteristics of the op amp, are often the performance limiting factors of photometer circuits. For this reason, in this paper a comparative analysis between two photodiode amplifier circuits is carried out. One circuit is based on a conventional current- to-voltage converter connection and the other circuit is based on a robust current-to-voltage converter connection. The results are satisfactory and show that the photodiode amplifier performance can be improved by using robust control techniques. Keywords: photometer circuit, current-to-voltage converter connection, frequency response, robust control Sensors 2008, 8 36 1. -
Photoelectric Spectrophotometry by the Null Method'
. PHOTOELECTRIC SPECTROPHOTOMETRY BY THE NULL METHOD' By K. S. Gibson CONTENTS Page I. Introduction 325 II. Spectral transmission 329 1. Apparatus 329 2. Method 333 3 Errors and accuracy 337 III. Diffuse spectral reflection 348 IV. Other applications 350 V. Summary 352 I. INTRODUCTION Anyone who has had experience in trying to make spectro- photometric measurements of transmission or reflection in the blue and violet parts of the spectrum is well aware of the difficulty of obtaining reliable determinations in this region. Nearly all methods have relatively low sensitivity, or else are inaccurate for other reasons, from wave lengths 400 to 500 millimicrons (m/x). Radiometric methods, which are so suitable for infra-red work and which have been used also in the visible and even in the ultra- violet, are, nevertheless, not of the highest accuracy in these latter regions because of the relatively low radiant power of all sources used for this kind of work, the radiant power decreasing continuously with the wave length. It is very difficult to obtain accurate determinations below 500 m/x by the usual radiometric methods. Any visual method is limited in the blue and violet because of the combined low visibility of the human eye and the low radiant power of the sources used, except at the few wave lengths where monochromatic light of great intensity can be ob- tained, as from the mercury arc. The Hilger sector photometer method, which is the only photographic method of speed and reliability, also has its limitations for this region. Being such a 1 An abst-act of this paper was presented to the Optical Society of America at the Baltimore meet- ing, Dec, 27, 1918. -
Application of Filter Photometers in the Production of Ethylene and Propylene
Analytical Products Sales Engineering Application of Filter Photometers in the Production of Ethylene and Propylene SC7-66-403 Gary D. Brewer APPLICATION OF FILTER PHOTOMETERS IN THE PRODUCTION OF ETHYLENE AND PROPYLENE Gary D. Brewer Product Manager, Photometers ABB Inc. 843 N. Jefferson St. Lewisburg, WV 24901 KEYWORDS Photometer, Infrared Spectroscopy, IR, Near Infrared Spectroscopy, NIR, Ultraviolet Spectroscopy, UV, Ethylene, Propylene ABSTRACT There have been several successful applications of process filter photometers in ethylene plants throughout the world. The process of manufacturing ethylene is extremely fast; therefore, the continuous measurements provided by filter photometers allow for a fast response to process changes for better control and process optimization. The capability of the current generation of filter photometers to use several analytical wavelengths to compensate for spectral interferences have allowed their use in measurements that previously could not be done by photometers. The high reliability and simplicity of filter photometers make them a valuable tool in the process control of an olefins plant. Applications in the IR and NIR spectral regions in both the vapor and liquid phases will be discussed to demonstrate their capabilities and benefits in this manufacturing process. Applications that will be discussed include the measurement of acetylene and ethane at the acetylene converters and the measurement of methyl acetylene and propadiene (MAPD) at the MAPD converters can be measured on a single infrared photometer. Applications at the caustic wash tower and the measurement of carbon dioxide at the furnace decoke will also be discussed. INTRODUCTION Ethylene is one of the highest volume chemicals produced in the world. -
Raman Spectroscopy Protocol
raman-prtkl4.doc 1/15 10.07.07 Raman Spectroscopy Comparison of Infrared Spectra with those gathered by Raman Spectroscopy of selected substances Protocol June 9th and 11th 1999, August 19th and 20th 1999, February 28th and 29th 2000 Headed by: Dr. M. Musso Handed in by : Pierre Madl (Mat-#: 9521584) Maricela Yip (Mat-#: 9424495) Salzburg, August 28th 2000 raman-prtkl4.doc 2/15 10.07.07 Introduction When radiation passes through a transparent medium, the species present scatter a fraction of the beam in all directions. In 1928, the Indian physicist C.V.Raman discovered that the wavelength of a small fraction of the radiation scattered by certain molecules differ from that of the incident beam; furthermore, the shifts in wavelength depend upon the chemical structure of the molecules responsible for scattering. The theory of Raman scattering, which now is well understood, shows that the phenomenon results from the same type of quantized vibrational changes that are associated with infrared (IR) absorption. Thus, the difference in wavelength between the incident and scattered radiation corresponds to wavelengths in the mid-infrared region. Indeed, Raman scattering spectrum and infrared spectrum for a given species often resemble one another quite closely. There are, however, enough differences between the kinds of groups that are infrared active and those that are Raman active to make the techniques complementary rather than competitive. For some problems, the infrared method is the superior tool, for others, the Raman procedure offers more useful spectra. An important advantage of Raman spectra over infrared lies in the fact that water does not cause interference; indeed, Raman spectra can be obtained form aqueous solutions. -
The CU 2-D-MAX-DOAS Instrument – Part 2: Raman Scattering Probability Measurements and Retrieval of Aerosol Optical Properties
Atmos. Meas. Tech., 9, 3893–3910, 2016 www.atmos-meas-tech.net/9/3893/2016/ doi:10.5194/amt-9-3893-2016 © Author(s) 2016. CC Attribution 3.0 License. The CU 2-D-MAX-DOAS instrument – Part 2: Raman scattering probability measurements and retrieval of aerosol optical properties Ivan Ortega1,2, Sean Coburn1,2, Larry K. Berg3, Kathy Lantz2,4, Joseph Michalsky2,4, Richard A. Ferrare5, Johnathan W. Hair5, Chris A. Hostetler5, and Rainer Volkamer1,2 1Department of Chemistry and Biochemistry, University of Colorado, Boulder, CO, USA 2Cooperative Institute for Research in Environmental Sciences (CIRES), Boulder, CO, USA 3Pacific Northwest National Laboratory, Richland, WA, USA 4Global Monitoring Division, Earth System Research Laboratory, NOAA, Boulder, CO, USA 5NASA Langley Research Center, Hampton, VA, USA Correspondence to: Rainer Volkamer ([email protected]) Received: 8 December 2015 – Published in Atmos. Meas. Tech. Discuss.: 18 January 2016 Revised: 12 July 2016 – Accepted: 13 July 2016 – Published: 23 August 2016 Abstract. The multiannual global mean of aerosol optical retrievals of AOD430 and g with data from a co-located depth at 550 nm (AOD550/ over land is ∼ 0.19, and that over CIMEL sun photometer, Multi-Filter Rotating Shadowband oceans is ∼ 0.13. About 45 % of the Earth surface shows Radiometer (MFRSR), and an airborne High Spectral AOD550 smaller than 0.1. There is a need for measurement Resolution Lidar (HSRL-2). The average difference (rela- techniques that are optimized to measure aerosol optical tive to DOAS) for AOD430 -
An Infrared Photon-Counting Photometer Based on the Edge-Illuminated Solid-State Photomultiplier
An Infrared Photon-counting Photometer Based on the Edge-illuminated Solid-State Photomultiplier Dae-Sik Moon1234, Stephen S. Eikenberry54, and Giovanni G. Fazio6 1Division of Physics, Mathematics and Astronomy, Caltech, MC 103–33, Pasadena, CA 91125; 2Robert A. Millikan Fellow; 3Space Radiation Laboratory, Caltech, MC 220–47, Pasadena, CA 91125; 4Department of Astronomy, Cornell University, Ithaca, NY 14853; 5Department of Astronomy, University of Florida, Gainesville, FL 32611; 6Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA ABSTRACT We present the design, construction, and test observations of a new infrared (IR) photon-counting photometer for astronomy based on the edge-illuminated solid-state photomultiplier (EISSPM). The EISSPM has a photon- counting capability over the 0.4–28 µm range with a nanosecond-scale intrinsic detector time resolution. Its quantum efficiency (QE) peaks ≥ 30 % in the near-IR, which is much higher than the previous SSPM with back illumination. After characterizing the dark noise of the EISSPM at its operational temperature range, we develop an EISSPM-based IR photon-counting photometer for astronomical observations. This includes the design and construction of a full optical, cryo-mechanical, and electronics system as well as the software for operating the instrument on telescopes. We report the results of our test observations of the Crab Nebula pulsar using this new instrument on the Palomar Hale 5-m telescope with 10-µs time resolution. Keywords: infrared, instrumentation, detectors, photometers 1. INTRODUCTION A photon-counting capability with > 100 Hz sampling rate (and potentially up to ∼106 Hz sampling rate) has diverse interesting applications in modern astronomy, involving both observational and technological aspects. -
Sphinx: the Solar Photometer in X-Rays
Solar Phys DOI 10.1007/s11207-012-0201-8 SphinX: The Solar Photometer in X-Rays Szymon Gburek · Janusz Sylwester · Miroslaw Kowalinski · Jaroslaw Bakala · Zbigniew Kordylewski · Piotr Podgorski · Stefan Plocieniak · Marek Siarkowski · Barbara Sylwester · Witold Trzebinski · Sergey V. Kuzin · Andrey A. Pertsov · Yurij D. Kotov · Frantisek Farnik · Fabio Reale · Kenneth J.H. Phillips Received: 10 April 2012 / Accepted: 19 November 2012 © Springer Science+Business Media Dordrecht 2012 Abstract Solar Photometer in X-rays (SphinX) was a spectrophotometer developed to ob- serve the Sun in soft X-rays. The instrument observed in the energy range ≈ 1–15 keV with resolution ≈ 0.4 keV. SphinX was flown on the Russian CORONAS–PHOTON satellite placed inside the TESIS EUV and X telescope assembly. The spacecraft launch took place on 30 January 2009 at 13:30 UT at the Plesetsk Cosmodrome in Russia. The SphinX exper- iment mission began a couple of weeks later on 20 February 2009 when the first telemetry dumps were received. The mission ended nine months later on 29 November 2009 when data transmission was terminated. SphinX provided an excellent set of observations dur- ing very low solar activity. This was indeed the period in which solar activity dropped to the lowest level observed in X-rays ever. The SphinX instrument design, construction, and operation principle are described. Information on SphinX data repositories, dissemination methods, format, and calibration is given together with general recommendations for data users. Scientific research areas in which SphinX data find application are reviewed. S. Gburek () · J. Sylwester · M. Kowalinski · J. Bakala · Z. Kordylewski · P. Podgorski · S. -
Euclid Near Infrared Spectro Photometer Instrument Concept and First Test Results at the End of Phase B
CORE Metadata, citation and similar papers at core.ac.uk Provided by NORA - Norwegian Open Research Archives Euclid Near Infrared Spectro Photometer instrument concept and first test results at the end of phase B Thierry Maciaszek, Ctr. National d'Études Spatiales, and Observatoire Astronomique de Marseille-Provence (France); Anne Ealet, Ctr. de Physique des Particules de Marseille (France); Knud Jahnke, Max-Planck-Institut für Astronomie (Germany); Eric Prieto, Observatoire Astronomique de Marseille-Provence (France); Rémi Barbier, Institut de Physique Nucléaire de Lyon (France); Yannick Mellier, Institut d'Astrophysique de Paris (France), and Commissariat à l'Énergie Atomique (France); Anne Costille, Franck Ducret, Christophe Fabron, Jean-Luc Gimenez, Robert Grange, Laurent Martin, Christelle Rossin, Tony Pamplona, Pascal Vola, Observatoire Astronomique de Marseille-Provence (France); Jean Claude Clémens, Ctr de Physique des Particules de Marseille (France); Gérard Smadja, Institut de Physique Nucléaire de Lyon (France); Jérome Amiaux, Jean Christophe Barrière, Michel Berthe, Commissariat à l'Énergie Atomique (France); Adriano De Rosa, Enrico Franceschi, Gianluca Morgante, Massimo Trifoglio, Luca Valenziano INAF - IASF Bologna (Italy); Carlotta Bonoli, Favio Bortoletto, Maurizio D'Alessandro, INAF - Osservatorio Astronimico di Padova (Italy); Leonardo Corcione, Sebastiano Ligori, INAF - Osservatorio Astronomico di Torino (Italy); Bianca Garilli, Marco Riva, INAF - IASF Milano (Italy); Frank Grupp, Carolin Vogel, Max-Planck-Institut für extraterrestrische Physik (Germany); Felix Hormuth, Gregor Seidel, Stefanie Wachter, Max-Planck-Institut für Astronomie (Germany); Jose Javier. Diaz, Instituto de Astrofisica de Canarias (Spain); Ferran Grañena, Cristobal Padilla, Institut de Física d’Altes Energies (IFAE) (Spain); Rafael Toledo, Universidad Politécnica de Cartagena (Spain); Per B. Lilje, University of Oslo; Bjarte G. -
A MATRIX ISOLATION SPECTROSCOPIC INVESTIGATION of the REACTION PRODUCTS of TRANSITION METAL CENTRES with ETHENE and WATER By
A MATRIX ISOLATION SPECTROSCOPIC INVESTIGATION OF THE REACTION PRODUCTS OF TRANSITION METAL CENTRES WITH ETHENE AND WATER by MATTHEW G. K. THOMPSON A thesis submitted to the Department of Chemistry in conformity with the requirements for the degree of Doctor of Philosophy Queen’s University Kingston, Ontario, Canada November 2007 Copyright © Matthew Gary Karl Thompson, 2007 Abstract The reaction products of thermally generated atomic V with ethene and ethene isotopomers have been investigated by matrix isolation ultraviolet visible and Fourier transform infrared (FTIR) spectroscopy. When V is deposited into matrices of pure Ar, evidence for V and V2 are present in the UV-visible absorption spectra. Addition of trace amounts of ethene results in the elimination of absorptions due to V2 on deposition, likely due to the formation of … V (C2H4) van der Waals complexes on matrix condensation. Irradiation of matrices containing V and trace C2H4 in Ar, with light corresponding to atomic V electronic excitations, eliminates all UV-visible absorptions due to atomic V in the matrix. Infrared analysis of matrices containing V and C2H4 give evidence for a new product on deposition, consistent with a kinetically formed H-V-C2H3 isomer. Following further irradiation of the matrix, several new products of C-H bond insertion by the metal atom, including additional H-V-C2H3 conformational 2 isomers, and H2V(η -C2H2) products are observed in the infrared spectrum. Additionally, the formation of ethane is evident as a major product immediately following deposition of V + C2H4 + H2O in Ar. The formation of this product is consistent with alkene insertion into the V-H bond of an H-V-OH intermediate, followed by a photo-induced elimination to give C2H6. -
Basics of Atomic Absorption Photometer
(Hitachi High-Technologies) Technical Note: Atomic Absorption Photometer Basics of Atomic Absorption Photometer Hitachi High-Technologies Corporations Copyright© 2007, Hitachi High-Technologies Corporation 1 (Hitachi High-Technologies) Technical Note: Atomic Absorption Photometer 1. Atomic Absorption Photometer Q “What does an atomic absorption photometer measure?” A: It is a system which mainly measures the concentration of metallic elements (quantitative analysis). Q “What are metallic elements?” A: They are elements corresponding to metallic elementary substances. For example, calcium, which is an ingredient in our bones, or sodium and potassium, which are contained in alkali drinking water are metallic elements. The metallic elements which can be measured are shown in the following periodic table. z Sixty-nine elements can be analyzed. z The elements which can be measured are shaded. z The peripheral equipment which needs to be prepared varies by element. Please refer to the supplemental data for details. Q “What concentrations can it measure?” A: It can measure from ppm to ppb. Q “Just a moment. What are ppm and ppb?” A: These are units indicating concentration, similar to percent. The ‘m’ and ‘b’ in ppm and ppb stand for million and billion, respectively. That is, 1% means 1/100, ppm means 1/million and ppb means 1/billion. To illustrate simply, 1% would mean one person in 100 people, while 1 ppm would be one person in one million people. Do you understand? Please see the following concentration conversion table. Generally a measurement sample is a solution specimen. Solution concentration units 1% = 1/100 = 10-2 1 ppm = 1/1,000,000 = 10-6 = 0.0001% 1 ppm = 1 mg/L= 1 µg/mL 1 ppb = 0.001 ppm = 10-9 1 ppt = 0.001 ppb = 10-12 = 1/trillion 1 ppb = 1 µg/L =1 ng/mL 1 ppt = 1 ng/L =1 pg/mL 1 (Hitachi High-Technologies) Technical Note: Atomic Absorption Photometer 2.