Atomic Emission Spectroscopy

Total Page:16

File Type:pdf, Size:1020Kb

Atomic Emission Spectroscopy Chapter 9 - Atomic Emission Spectroscopy Consider Figure 9.1 and the discussion of Boltzmann distribution in Chapters 2 and 7. Before continuing in this chapter, speculate on why a flame is an excellent atomizer for use in atomic absorption but is a poor atomizer for use in atomic emission. Since the signal in AES is the result of relaxation from the excited state, the intrinsic LOD of AES is a function of the population density of the excited state. The flame in AAS is not nearly as hot as the sources used in AES. Use of a flame for AES would have a significant negative impact on the LOD of AES. Thinking in terms of quantum mechanic phenomena and instrumentation, list some similarities and differences between molecular absorption and molecular luminescence spectroscopic methods (see Figure 9.1). This is an open ended question so the instructor may need to adjust expectations accordingly. Because students were asked to discuss quantum mechanic phenomena, the students should not go into details outlining the similarities in instrumentation. Similarities Differences Both measure transitions between electronic UV-vis spectroscopy involves absorption of a quantum states photon while Luminescence involves the emission of a photon. Both techniques have relatively broad spectra as the result of superimposed vibrational and In UV-vis spectroscopy, the detector is measuring rotational states upon each electronic state power from an external source. In luminescence (vibronic). spectroscopy, the detector is measuring power as the excited state analyte molecules relax to the Both techniques involve photon energies that ground state. reside in the “UV-vis” portion of the EM spectrum. Use the Boltzmann distribution equation to calculate the percentage of magnesium atoms that are in the excited state (electronic transition from 3s to 3p, λ = 285.2 nm) under the conditions of (a) an air–acetylene flame at 2,955 K and (b) a plasma at 6,955 K. Assume that ge/gg = 3. Students are encouraged to review Example 9.1. The Boltzman distribution equation is ∆E Ne ge (− ) = e kT Ng gg … and −34 8 푚 ℎ푐 (6.626 푋 10 퐽푠)(2.99 푋 10 ⁄푠) ∆퐸 = = = 6.95 푋 10−19퐽 휆 285.2 푋 10−9푚 Therefore in the air-acetylene flame the population ratio would be, −19 ∆E 6.95 푋 10 퐽 Ne ge (− ) −[ −23 −1 ] = e kT = (3)푒 (1.38065 푥 10 퐽∙퐾 )(2,995퐾) = 1.506 푋 10−7 Ng gg And the percentage of magnesium atoms in the excited state at 2,995K would be 1.506 X 10-5 %. A more compact way of expressing this number would be to say that 0.1506 ppm of the magnesium atoms would be in the excited state at 2,995K. If we changed the atomizer to a plasma torch at 6,955K the population ratio would be −19 ∆E 6.95 푋 10 퐽 Ne ge (− ) −[ −23 −1 ] = e kT = (3)푒 (1.38065 푥 10 퐽∙퐾 )(6,955퐾) = 2.16 푋 10−3 Ng gg And the percentage of magnesium atoms in the excited state at 6,955K would be 0.216 %. A more compact way of expressing this number would be to say that 2160 ppm of the magnesium atoms would be in the excited state at 2,995K The Saha ionization equation allows us to estimate the ratio of gas phase atoms that will be ionized (ni) relative to the number of neutral atoms (n0 = ntotal – ni) under certain conditions. Assuming that the partial pressure of Mg atoms in the atomizer is 10-5 atm, ge/gg = 3, and the volume of the flame or plasma is 2.0 cm3, calculate the percentage of Mg atoms that will be ionized under the two atomizer conditions given in Problem 9.3. The first ionization energy of magnesium is 737.7 kJ/mol. 2 We can begin by calculating the Saha ratio (ni /n0) in general terms. We will first need to calculate the given ionization energy (737.7 kJ/mol) in terms of joules per atom: 737.7 푘퐽 1000 퐽 푚표푙 -18 퐸 = 푥 푥 = 1.2250 x 10 J/atom 푚표푙 푘퐽 6.022 푥 1023 푎푡표푚푠 1.225 x 10−18J 2 E −( ) n 2 −( i ) 3 2 −23 J i 21 k T 21 −3 (1.381 x 10 )(2955 K) = (2.41 x 10 )T3 ∙ e b = (2.41 x 10 m K2)(2955 K)3 ∙ e K n0 = 3.51103 x 1013 m-3 From the units, we see that this is a ratio calculated for a volume of 1 cubic meter (that is, per m3 or -3 times m ). If this were a direct ratio (that is, simply ni/no), it would not matter, but since the numerator of the ratio term we calculated is squared, we need to adjust to the volume of the flame: 2 13 3 ni 3.51103 x 10 m 3 7 ( ) = 3 x ( ) x 2.0 cm = 7.0221 x 10 n0 flame m 100 cm ni To get the percentage of ionized Mg atoms, we need x 100%. Since n0 is the number of unionized nt Mg atoms, we know that n0 = nt – ni, where nt is the total number of Mg atoms in the flame. We are given that the partial pressure of Mg in the flame is 10-5 atm, and we will treat this as an exact number to find nt – note that we need to distinguish between the nt as defined here (number of Mg atoms) vs. “n” as a common unit for moles, which we can designate as nt,moles −5 PV (10 atm)(0.0020 L) -11 nt,moles = = L∙atm = 8.24785 x 10 mol Mg atoms RT (0.08206 )(2955 K) mol∙K 23 −11 6.022 x 10 atoms 13 n = 8.24785 x 10 mol Mg atoms x = 4.96686 x 10 atoms total t mol We can derive a quadratic expression to allow us to extract ni: 2 2 ni 7 ni = 7.0221 x 10 so n0 = 7 n0 7.0221 x 10 2 ni also, n0 = nt - ni so = n − n 7.0221 x 107 t i 2 7 7 then ni = (7.0221 x 10 )nt − (7.0221 x 10 )ni 2 7 13 7 and ni = (7.0221 x 10 )(4.96686 x 10 ) − (7.0221 x 10 )ni 2 21 7 ni = (3.4878 x 10 ) − (7.0221 x 10 )ni 2 7 21 and finally ni + (7.0221 x 10 )ni − (3.4878 x 10 ) = 0 −푏 ± √−푏+4푎푐 10 We then use the quadratic equation ( ) to find ni = 5.9022 x 10 ions. 2푎 So percentage of ionized Mg atoms 10 푛푖 5.9022 푥 10 푥 100% = 13 푥 100% = 0.12% ionized at 2955 K 푛푡 4.96686 푥 10 We can follow the same procedure to find that 99.74% Mg atoms would be expected to be ionized at 6955 K. Instructors should follow this interesting result up with discussion introduced in Problem 9.5. The Saha equation does not take into account environment – it is based solely on the relationship between temperature and ionization energy. The inherently electron-rich, reducing environment of both the flame and the plasma prevents ionization at the level predicted by the Saha equation. In AES, one of the concerns of using too hot of a source is the generation of atomic ions instead of atomic atoms. The plasma source used in AES is much hotter than the atomizers used in AAS, yet we do not observe an overwhelming abundance of atomic ions in the sample spectrum. Speculate on why this is true (Hint: Think about the definition of and physical composition of plasma). A plasma is an energized atomic vapor resulting in a “soup” of free electrons and free cationic ions. The very high concentration of free electrons in the plasma result in the reduction of analyte cations generated during the atomization process. Find the cost per volume for a tank of high-purity argon in your area. What is the cost per minute of using (a) an ICP-AES and (b) a DCP-AES? The answer to this question will vary depending upon the price the student finds. This problem can also be a little tricky because the student will need to convert the volume of the gas from the volume of the pressurized cylinder to volume of argon at one atmosphere of pressure. A typical cylinder is 30 liters (often referred to as the water volume) and is purchased with a pressure typically near 2000 psi. Assuming constant temperature, if the new argon tank was pressurized to 2000 psi the pressure at one atmosphere (14.7 psi) would be found using P1V1=P2V2. Solving for V2 we obtain, 푃1푉1 2000푝푠 푋 30퐿 푉2 = = = 4081퐿 푃2 14.7푝푠 A typical ICP torch consumes 12 liters/min of argon so a typical argon tank will last approximately 4081퐿⁄ 340 푚푛 푡푎푛푘 = 12퐿 푡푎푛푘 ⁄푚푛 Assuming a price of $300/tank, an ICP torch costs $300⁄ 푡푎푛푘 = $0.88⁄ 340푚푛 푚푛 ⁄푡푎푛푘 A typical DCP torch consumes between 5 & 8 liters/min of argon. If we assume the high end of this range, an argon tank will last 4081퐿⁄ 510 푚푛 푡푎푛푘 = 8퐿 푡푎푛푘 ⁄푚푛 For a cost of $300⁄ 푡푎푛푘 = $0.59⁄ 510푚푛 푚푛 ⁄푡푎푛푘 You are the financial manager of an analytical laboratory that uses atomic emission to conduct environmental analysis. Assuming you run the instrument continuously for 6 hours on each workday, how much would you spend on argon each year (using your values from Problem 9.6)? Be sure to clearly indicate all assumptions you make to estimate the number of workdays each year.
Recommended publications
  • Atomic and Molecular Laser-Induced Breakdown Spectroscopy of Selected Pharmaceuticals
    Article Atomic and Molecular Laser-Induced Breakdown Spectroscopy of Selected Pharmaceuticals Pravin Kumar Tiwari 1,2, Nilesh Kumar Rai 3, Rohit Kumar 3, Christian G. Parigger 4 and Awadhesh Kumar Rai 2,* 1 Institute for Plasma Research, Gandhinagar, Gujarat-382428, India 2 Laser Spectroscopy Research Laboratory, Department of Physics, University of Allahabad, Prayagraj-211002, India 3 CMP Degree College, Department of Physics, University of Allahabad, Pragyagraj-211002, India 4 Physics and Astronomy Department, University of Tennessee, University of Tennessee Space Institute, Center for Laser Applications, 411 B.H. Goethert Parkway, Tullahoma, TN 37388-9700, USA * Correspondence: [email protected]; Tel.: +91-532-2460993 Received: 10 June 2019; Accepted: 10 July 2019; Published: 19 July 2019 Abstract: Laser-induced breakdown spectroscopy (LIBS) of pharmaceutical drugs that contain paracetamol was investigated in air and argon atmospheres. The characteristic neutral and ionic spectral lines of various elements and molecular signatures of CN violet and C2 Swan band systems were observed. The relative hardness of all drug samples was measured as well. Principal component analysis, a multivariate method, was applied in the data analysis for demarcation purposes of the drug samples. The CN violet and C2 Swan spectral radiances were investigated for evaluation of a possible correlation of the chemical and molecular structures of the pharmaceuticals. Complementary Raman and Fourier-transform-infrared spectroscopies were used to record the molecular spectra of the drug samples. The application of the above techniques for drug screening are important for the identification and mitigation of drugs that contain additives that may cause adverse side-effects. Keywords: paracetamol; laser-induced breakdown spectroscopy; cyanide; carbon swan bands; principal component analysis; Raman spectroscopy; Fourier-transform-infrared spectroscopy 1.
    [Show full text]
  • ADVANCED SPECTROMETER Introduction
    ADVANCED SPECTROMETER Introduction In principle, a spectrometer is the simplest of scientific very sensitive detection and precise measurement, a real instruments. Bend a beam of light with a prism or diffraction spectrometer is a bit more complicated. As shown in Figure grating. If the beam is composed of more than one color of 1, a spectrometer consists of three basic components; a light, a spectrum is formed, since the various colors are collimator, a diffracting element, and a telescope. refracted or diffracted to different angles. Carefully measure The light to be analyzed enters the collimator through a the angle to which each color of light is bent. The result is a narrow slit positioned at the focal point of the collimator spectral "fingerprint," which carries a wealth of information lens. The light leaving the collimator is therefore a thin, about the substance from which the light emanates. parallel beam, which ensures that all the light from the slit In most cases, substances must be hot if they are to emit strikes the diffracting element at the same angle of inci- light. But a spectrometer can also be used to investigate cold dence. This is necessary if a sharp image is to be formed. substances. Pass white light, which contains all the colors of The diffracting element bends the beam of light. If the beam the visible spectrum, through a cool gas. The result is an is composed of many different colors, each color is dif- absorption spectrum. All the colors of the visible spectrum fracted to a different angle. are seen, except for certain colors that are absorbed by the gas.
    [Show full text]
  • Spectrum 100 Series User's Guide
    MOLECULAR SPECTROSCOPY SPECTRUM 100 SERIES User’s Guide 2 . Spectrum 100 Series User’s Guide Release History Part Number Release Publication Date L1050021 A October 2005 Any comments about the documentation for this product should be addressed to: User Assistance PerkinElmer Ltd Chalfont Road Seer Green Beaconsfield Bucks HP9 2FX United Kingdom Or emailed to: [email protected] Notices The information contained in this document is subject to change without notice. Except as specifically set forth in its terms and conditions of sale, PerkinElmer makes no warranty of any kind with regard to this document, including, but not limited to, the implied warranties of merchantability and fitness for a particular purpose. PerkinElmer shall not be liable for errors contained herein for incidental consequential damages in connection with furnishing, performance or use of this material. Copyright Information This document contains proprietary information that is protected by copyright. All rights are reserved. No part of this publication may be reproduced in any form whatsoever or translated into any language without the prior, written permission of PerkinElmer, Inc. Copyright © 2005 PerkinElmer, Inc. Trademarks Registered names, trademarks, etc. used in this document, even when not specifically marked as such, are protected by law. PerkinElmer is a registered trademark of PerkinElmer, Inc. Spectrum, Spectrum 100, and Spectrum 100N are trademarks of PerkinElmer, Inc. Spectrum 100 Series User’s Guide . 3 Contents Contents...............................................................................................
    [Show full text]
  • Experiment 2 Radiation in the Visible Spectrum Emission Spectra Can Be
    Experiment 2 Radiation in the Visible Spectrum Emission spectra can be a unique fingerprint of an atom or molecule. The photon energies and wavelengths are directly related to the allowed quantum energy states of the system. In the following experiments we will examine the radiation given off by sources radiating in the visible region. We will be using a spectrometer produced by Ocean Optics. Light enters the spectrometer via a fiber optic cable. Inside the spectrometer a diffraction grating diffracts the different frequencies onto a CCD. The CCD basically ”counts” the photons according to wavelength. The data is transferred via a usb port to a PC. The Ocean Optics software displays the spectrum as counts versus wavelength. We will examine the spectra given off by the following sources: incandescent light filament, hydrogen, helium, various light emitting diodes and a laser pointer. You will also be given an unknown gas discharge tube and will need to identify the gas via its spectral emissions Pre Lab 1) Obtain a spectrum for hydrogen, mercury, sodium and neon gas emissions. The spectrum must contain an accurate listing of major emission lines (in nm), not simply a color photo of the emission. 2) Make yourself familiar with the manual for the spectrometer and the software. These are available via the following links: http://www.oceanoptics.com/technical/hr4000.pdf http://www.oceanoptics.com/technical/SpectraSuite.pdf These documents are also available on Black Board. 3) How does the Ocean Optics spectrometer work? In your answer list its three main components and describe what each component does.
    [Show full text]
  • Electrochemical Characterization and Determination of Tramadol Drug Using Graphite Pencil Electrode
    Anal. Bioanal. Electrochem., Vol. 8, No. 1, 2016, 78-91 Analytical & Bioanalytical Electrochemistry 2016 by CEE www.abechem.com Full Paper Electrochemical Characterization and Determination of Tramadol drug using Graphite Pencil Electrode Deepa G. Patil, Naveen M. Gokavi, Atmanand M. Bagoji and Sharanappa T. Nandibewoor P.G. Department of Studies in Chemistry, Karnatak University, Dharwad – 580003, India * Corresponding Author, Tel.: +918362215286; Fax: +918362747884 E-Mail: [email protected] Received: 1 October 2015 / Received in revised form: 23 December 2015 / Accepted: 28 December 2015 / Published online: 15 February 2016 Abstract- Electrochemical oxidation of tramadol at pencil graphite electrode has been investigated using cyclic, differential pulse and square wave voltammetric techniques. In pH 9.2 phosphate buffer, tramadol showed an irreversible oxidation peak at 0.77 V. The dependence of the current on pH, concentration and scan rate was investigated to optimize the experimental conditions for the determination of tramadol. Differential pulse voltammetry was further exploited as a sensitive method for the detection of tramadol. Under optimized conditions, the concentration range and detection limit were 1.0×10−7 to 1.5×10−6 M and 0.38 ×10−8 M, respectively. The proposed method was applied to determine the tramadol assay in pharmaceutical samplesArchive and human biological fluids suchof as urine SID as a real sample. Keywords- Voltammetry, Tramadol, Pencil, pH, Electrochemical, Tablet 1. INTRODUCTION Drug analysis is an important tool for drug quality control. Hence, the development of simple, sensitive and rapid method is of great importance. Tramadol(TRA),(1R,2R)-2- [(dimethylamino)methyl]-1-(3methoxyphenyl) cyclohexanol (Scheme 1), is a synthetic monoamine uptake inhibitor and centrally acting analgesic, used for treating moderate to severe pain and it appears to have actions at the µ-opioid receptor as well as the www.SID.ir Anal.
    [Show full text]
  • Orbitrap Fusion Tribrid Mass Spectrometer
    MASS SPECTROMETRY Product Specifications Thermo Scientific Orbitrap Fusion Tribrid Mass Spectrometer Unmatched analytical performance, revolutionary MS architecture The Thermo Scientific™ Orbitrap Fusion™ mass spectrometer combines the best of quadrupole, Orbitrap, and linear ion trap mass analysis in a revolutionary Thermo Scientific™ Tribrid™ architecture that delivers unprecedented depth of analysis. It enables life scientists working with even the most challenging samples—samples of low abundance, high complexity, or difficult-to-analyze chemical structure—to identify more compounds faster, quantify them more accurately, and elucidate molecular composition more thoroughly. • Tribrid architecture combines quadrupole, followed by ETD or EThCD for glycopeptide linear ion trap, and Orbitrap mass analyzers characterization or HCD followed by CID • Multiple fragmentation techniques—CID, for small-molecule structural analysis. HCD, and optional ETD and EThCD—are available at any stage of MSn, with The ultrahigh resolution of the Orbitrap mass subsequent mass analysis in either the ion analyzer increases certainty of analytical trap or Orbitrap mass analyzer results, enabling molecular-weight • Parallelization of MS and MSn acquisition determination for intact proteins and confident to maximize the amount of high-quality resolution of isobaric species. The unsurpassed data acquired scan rate and resolution of the system are • Next-generation ion sources and ion especially useful when dealing with complex optics increase system ease of operation and robustness and low-abundance samples in proteomics, • Innovative instrument control software metabolomics, glycomics, lipidomics, and makes setup easier, methods more similar applications. powerful, and operation more intuitive The intuitive user interface of the tune editor The Orbitrap Fusion Tribrid MS can perform and method editor makes instrument calibration a wide variety of analyses, from in-depth and method development easier.
    [Show full text]
  • Standard Methods for the Examination of Water and Wastewater
    Standard Methods for the Examination of Water and Wastewater Part 1000 INTRODUCTION 1010 INTRODUCTION 1010 A. Scope and Application of Methods The procedures described in these standards are intended for the examination of waters of a wide range of quality, including water suitable for domestic or industrial supplies, surface water, ground water, cooling or circulating water, boiler water, boiler feed water, treated and untreated municipal or industrial wastewater, and saline water. The unity of the fields of water supply, receiving water quality, and wastewater treatment and disposal is recognized by presenting methods of analysis for each constituent in a single section for all types of waters. An effort has been made to present methods that apply generally. Where alternative methods are necessary for samples of different composition, the basis for selecting the most appropriate method is presented as clearly as possible. However, samples with extreme concentrations or otherwise unusual compositions or characteristics may present difficulties that preclude the direct use of these methods. Hence, some modification of a procedure may be necessary in specific instances. Whenever a procedure is modified, the analyst should state plainly the nature of modification in the report of results. Certain procedures are intended for use with sludges and sediments. Here again, the effort has been to present methods of the widest possible application, but when chemical sludges or slurries or other samples of highly unusual composition are encountered, the methods of this manual may require modification or may be inappropriate. Most of the methods included here have been endorsed by regulatory agencies. Procedural modification without formal approval may be unacceptable to a regulatory body.
    [Show full text]
  • Mass Spectrometer
    CLASSICAL CONCEPT REVIEW 6 Mass Spectrometer One of several devices currently used to measure the charge-to-mass ratio q m of charged atoms and molecules is the mass spectrometer. The mass spectrometer is used to find the charge-to-mass ratio of ions of known charge by measuring> the radius of their circular orbits in a uniform magnetic field. Equation 3-2 gives the radius of R for the circular orbit of a particle of mass m and charge q moving with speed u in a magnetic field B that is perpendicular to the velocity of the particle. Figure MS-1 shows a simple schematic drawing of a mass spectrometer. Ions from an ion source are accelerated by an electric field and enter a uniform magnetic field produced by an electromagnet. If the ions start from rest and move through a poten- tial DV, their kinetic energy when they enter the magnetic field equals their loss in potential energy, qDV: B out 1 mu2 = qDV MS-1 2 R The ions move in a semicircle of radius R given by Equation 3-2 and exit through a P P narrow aperture into an ion detector (or, in earlier times, a photographic plate) at point 1 u 2 P2, a distance 2R from the point where they enter the magnet. The speed u can be eliminated from Equations 3-2 and MS-1 to find q m in terms of DV, B, and R. The + + q result is Source > – + q 2DV ∆V = 2 2 MS-2 m B R MS-1 Schematic drawing of a mass spectrometer.
    [Show full text]
  • Opacity and Emissivity in Spectral Lines (Cont)
    PHYS 7810 / COLLAGE2021: Solar Spectral Line Diagnostics Lecture 05: Opacity and Emissivity in Spectral Lines (cont) Ivan Milic (CU Boulder) ; ivan.milic (at) colorado.edu Plan for today: ● On Tuesday we entered the discussion talking about emissivity and deriving an expression ● Today we are first going to do the same for opacity (but much faster) ● Then we are going to investigate some relationships between the two ● And to analyze, through equations how each physical parameter (T, p, v, B), influences opacity/emissivity. Once again, this is equation that includes it all This whole equation tells us how the things behave on big scales. (dl is geometrical length, and light propagates over very large distances inside of astrophysical objects. These two coefficients, on the other side, depend on specific physics of emission and absorption. We talk about them now Emissivity due to spectral line transitions ● This is only due to bound-bound processes, other sources would look differently ● Finding the number density of the atoms that are in the upper energy state (population of the upper level) will be the most cumbersome task. ● Also, line emission/absorption profile (often the same) contains many dependencies The absorption coefficient (opacity) ● We can have a very similar story here: ● The intensity should have units of inverse length. What if we relate it somehow to number density of absorption events (absorbers?) ● This is more “classical” than the previous argument, but it very intuitively tells us what opacity depends on! Let’s write
    [Show full text]
  • Research Article Electron Density from Balmer Series Hydrogen Lines
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Crossref Hindawi Publishing Corporation International Journal of Spectroscopy Volume 2016, Article ID 7521050, 9 pages http://dx.doi.org/10.1155/2016/7521050 Research Article Electron Density from Balmer Series Hydrogen Lines and Ionization Temperatures in Inductively Coupled Argon Plasma Supplied by Aerosol and Volatile Species Jolanta Borkowska-Burnecka, WiesBaw gyrnicki, Maja WeBna, and Piotr Jamróz Chemistry Department, Division of Analytical Chemistry and Chemical Metallurgy, Wroclaw University of Technology, Wybrzeze Wyspianskiego 27, 50-370 Wroclaw, Poland Correspondence should be addressed to Wiesław Zyrnicki;˙ [email protected] Received 29 October 2015; Revised 15 February 2016; Accepted 1 March 2016 Academic Editor: Eugene Oks Copyright © 2016 Jolanta Borkowska-Burnecka et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Electron density and ionization temperatures were measured for inductively coupled argon plasma at atmospheric pressure. Different sample introduction systems were investigated. Samples containing Sn, Hg, Mg, and Fe and acidified with hydrochloric or acetic acids were introduced into plasma in the form of aerosol, gaseous mixture produced in the reaction of these solutions with NaBH4 and the mixture of the aerosol and chemically generated gases. The electron densities measured from H ,H,H,andH lines on the base of Stark broadening were compared. The study of the H Balmer series line profiles showed that the values from H and H were well consistent with those obtained from H which was considered as a common standard line for spectroscopic 15 15 −3 measurement of electron density.
    [Show full text]
  • Atomic Spectroscopy
    Atomic Spectroscopy Reference Books: 1) Analytical Chemistry by Gary D. Christian 2) Principles of instrumental Analysis by Skoog, Holler, Crouch 3) Fundamentals of Analytical Chemistry by Skoog 4) Basic Concepts of analytical Chemistry by S. M. Khopkar We consider two types of optical atomic spectrometric methods that use similar techniques for sample introduction and atomization. The first is atomic absorption spectrometry (AAS), which for half a century has been the most widely used method for the determination of single elements in analytical samples. The second is atomic fluorescence spectrometry (AFS), which since the mid-1960s has been studied extensively. By contrast to the absorption method, atomic fluorescence has not gained widespread general use for routine elemental analysis. Thus, although several instrument makers have in recent years begun to offer special- purpose atomic fluorescence spectrometers, the vast majority of instruments are still of the atomic absorption type. Sample Atomization Techniques We first describe the two most common methods of sample atomization encountered in AAS and AFS, flame atomization, and electrothermal atomization. We then turn to three specialized atomization procedures used in both types of spectrometry. Flame Atomization In a flame atomizer, a solution of the sample is nebulized by a flow of gaseous oxidant, mixed with a gaseous fuel, and carried into a flame where atomization occurs. As shown in Figure, a complex set of interconnected processes then occur in the flame. The first step is desolvation, in which the solvent evaporates to produce a finely divided solid molecular aerosol. The aerosol is then volatilized to form gaseous molecules. Dissociation of most of these molecules produces an atomic gas.
    [Show full text]
  • 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.
    [Show full text]