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CHE. 331
Chapter 10
Atomic Emission Spectroscopy.
History and Theory of Atomic Absorption Spectroscopy As the name implies, atomic absorption is the absorption of light by free atoms. An atomic absorption spectrophotometer is an instrument that uses this principle to analyze the concentration of metals in solution. The versatility of atomic absorption an analytical technique (Instrumental technique) has led to the development of commercial instruments. In all, a total of 68 metals can be analyzed. Advantages of AA · Determination of 68 metals · Ability to make ppb determinations on major components of a sample · Precision of measurements by flame are better than 1% rsd. There are few other instrumental methods that offer this precision so easily. · AA analysis is subject to little interference. · Most interference that occurs have been well studied and documented. · Sample preparation is simple (often involving only dissolution in an acid) · Instrument easy to tune and operate Kirchoff and Bunsen's Experiment Between 1859 to 1861, Gustav Kirchoff (Prussian physicist), with his colleague Robert Tunsen, a German chemist, at the University of Heidelberg demonstrated that every element gives off a characteristic color when heated in incandescence. The apparatus used for their classic experiment is shown here. Applying this new research tool, they discovered the element cesium and rubidium. Kirchoff - Absorbance & Emission Line Kirchoff and Bunsen not only identified various characteristic spectra, but they established the relationship between the emission spectra and the absorption spectra thus explaining the presence of the dark lines in the solar spectra.
Ground State Atom With that brief history of the development of the atomic absorption procedure and Varian atomic absorption instruments, we will now examine the atomic theory that explains how an atomic absorption signal is generated. In order to understand the atomic absorption process one must first understand the structure of the atom and its orbitals. The atom consists of the central core, or nucleus, made up of positively charged protons and neutral neutrons. Surrounding the nucleus in precisely defined energy orbitals are the electrons. All neutral atoms have an equal number of protons in the nucleus. This means that each element has a unique number of electrons and protons, The outermost electrons are known as the valence electrons and atomic spectroscopy involves energy changes in these valence electrons. Beer - Lambert Law The relationship that converts the intensity of the light beam to concentration is called the Beer - Lambert Law or simply Beer' s law. Beer' s Law states that the absorbance, A, is equal to the molar absorptivity or extinction coefficient, a. times the path length over which the measurement is made. b, times the concentration of the analyte, c. For a given set of conditions, the molar absorptivity, a, is a constant. The path length of the determination, b, is also a constant. Therefore, the absorbance is equal to a constant times the concentration. A = abc = Kc, where A = absorbance a = absorptivity constant, b = sample thickness path length, c = concentration K = a constant If this expression is plotted, a curve of absorbance versus concentration is drawn, Beer's Law predicts that a straight line will result. In practice we find that deviation from the linear calibration is observed at higher concentrations. Normal Absorbance The important thing to remember in the use of Beer' s Law is that A refers to absorbance, not absorption. Absorbance is defined by the equation: A = log (lo/1), where A = absorbance
significant concentration of cations and electrons. The concentration of the two are such that the net charge approaches zero. Argon plasmas are used most often for nonflame AES. The high temperatures that are achieved in argon plasmas cause more efficient excitation of atoms and ions than is achieved with flames. As a result, the intensities of the emitted lines are greater and more spectral lines are observed. Three types of high-temperature plasmas are encountered and these are: 1) the inductively coupled plasma (ICP), (2) the direct current plasma (DCP), and (the microwave induced plasma (MIP). The most important of these plasmas is the inductively coupled plasma (ICP). The Inductively Coupled Plasma Source. The figure below is a shematic of a typical inductively coupled plasma source called a torch. It consists of three concentric quartz tubes through which streams of argon gas flow. Depending upon the torch design, the total rate of argon consumption is 5 to 20 l/min. Surrounding the top of this tube is a water-cooled induction coil that is powered by a radio frequency generator, which is capable of producing 0.5 to 2kW of power at about 27 or 41MHz.
The wavelength selector for an instrument that uses a plasma is a narrow-band pass monochromator. The wavelength of the monochromator as well as the other functions of the spectrometer are generally controlled by a microcomputer. Various detectors can be used including photomultiplier tubes and diode arrays. Several wavelengths can be simultaneously monitored or the wavelengths can be sequentially scanned. The readout devices that are used with the spectrometers include cathode-ray tubes, recorders, and line printers. Qualitative analysis is done using AES in the same manner in which it is done using FES. The spectrum of the analyte is obtained and compared with the atomic and ionic spectra of possible elements in the analyte. Generally an element is considered to be in the analyte if at least three intense lines can b matched with those from the spectrum of a known element. Quantitative analysis with a plasma can be done using either an atomic or an ionic line. Ionic lines are chosen for most analyses because they are usually more intense at the temperatures of plasmas than are the atomic lines. Interference that is encountered with plasmas can be grouped into the same categories as those that were encountered with AAS. Chemical interference owing to refractory compounds
Sketches of several common forms of graphite electrodes are shown in Figure. The cylindrical graphite electrodes typically have a diameter of 6.2mm and a length of 38mm. Electrical discharge occurs at the pointed end of the counter electrodes where the strength of the electrical field is maximum. Several types of sample electrodes are available. The pointed electrode can be a graphite rod on which the sample solution is coated and allowed to dry before analysis. It is also the usual design when the electrode is constructed from the analyte. Electrodes of that design are often used for steel or other metal samples. The electrode is a graphite-cup electrode. The sample (usually a powder) is placed in the cup in the top of the electrode. A drill bit is used to form the cup in the electrode. Often the neck of the electrode below the cup is narrowed in order to minimize conduction of heat away from the cup during the electrical discharge. In some electrodes the neck is of the same diameter as the remainder of the electrode. A porous-cup electrode is shown in Fig. 7-3f. It is used for solutions. Several milliliters of the solution are placed inside the electrode. The sample cavity in the electrode is prepared by drilling a hole to within about 3mm of the end of the graphite rod. The solution slowly seeps through the bottom of the electrode. The counter electrode is placed below the porous-cup electrode.
The rotating-disk electrode (Fig. 7-3g) is also used for solutions. The disk, which is about 1. cm in diameter. is mounted on an axle and dipped into the sample solution. As the disk is rotated a film of the solution is carried to the top of the disk. The counter electrode is placed above the rotating disk at the top of the electrode. In the rotating-platform electrode (Fig. 7-3h) the sample solution is placed on the top of the disk and allowed to drive. The disk is rotated during the assay. Both forms of electrodes are typically rotated at between 5 and '10 revolutions per minute (r/min). DC ARC. Electrical atomization/ ionization and subsequent excitation of the sample can be accomplished with either spark or are discharges. Commercial instruments often contain two or more of the electrical excitative sources. Of the several common types arcs and sparks. the de arc is the simplest. It uses a de potential that is between 10 and 50 V to cause an electrical discharge that corresponds to a current of between 1 and 5 A to flow between the counter and the sample electrode (Fig. 7-4). The temperature generated by the electrical discharge is about 4000 C at the anode and about 200C at the cathode. Between the electrodes the temperature is in the 4000 to 7000 C range. The sample electrode can be either the cathode or anode, but generally it is the anode. Temperatures that are achieved with the de arc are hotter than those achieved with most flames. The excitation of the sample is attributable to the combination of the high temperature and the electrical energy between the electrodes. Because different elements are vaporized and excited at different times, it is necessary to use the arc until the entire sample has been vaporized. In most instruments, the dc arc is started by applying a high-potential spark across the electrodes. After the arc has been started the spark can either be shut off or allowed to continue. The de arc yields intense emissive lines and consequently is often used for qualitative analysis. Because the de arc
The spark excitative source uses ac power an LC circuit, and a spark gap that is operated by a synchronous motor to cause a spark to jump between the electrodes. The spark gap operates in a manner similar to that of the spark gap. Distributor of an automobile. Its function is to ensure that the spark jumps between the electrodes only when the potential that is stored in the capacitor in the ac circuit is at a maximum. The motor rotation is synchronized to the frequency of alternation of the current. A sketch of a simple circuit (Feussner circuit) that can be used for a spark source is shown in Fig. 7-5. Several variations of the circuit are in use in different instruments. The potential after the step-up transformer in the circuit is between 10,000 and 50,000 V with a high-voltage source and about 1000 V with a medium voltage source. The spark is active for periods between 10 and 100ps and typically discharges at a rate of 120 to 180 times each second. Heating effects on the electrodes are minimized by the cooling that occurs between sparks. That leads to less fractional distillation of the sample from the electrode than is observed with the dc arc. The time required to obtain a spectrum with a spark is about 10s. The spark generally yields the most reproducible results and the highest precision of all of the spark and arc discharges. It is not as sensitive, however, as the de arc. Minimum concentrations that can be assayed with a spark are about 0.01 percent for solid metallic samples and about 1 Vtg/mL for solutions. Solid metallic samples are usually machined into a rod for use as the sample electrode. Normally the counter electrode is a pointed graphite or silver rod. Powders are pressed into pellets and inserted in the of the sample electrode. Liquids often are assayed with the aid of a porous-cup electrode. LASER MICROPROBE.
The laser microprobe uses a laser to vaporize a small section on the surface of a sample. The vaporized sample passes between two ac spark electrodes that excite the sample. The resulting emissive spectrum is recorded as with the other AES methods. The laser microprobe is ideally suited for examination of small areas on a surface. A microscope is used to focus the beam from the laser onto an area that is roughly 10 to 50vim in diameter. Often a pulsed laser is used. The electrodes are held in place about 25mm above the surface. The laser is fired between the electrodes. The two electrodes are sharply pointed rods that serve to control the location of the electric field during the discharges. A sketch of a laser microprobe. WAVELENGTH SELECTION AND DETECTION FOR AES. Arc and spark instruments normally contain non scanning monochromators. Either a series of slits is cut in the focal plane of the monochromator and a photomultiplier tube is placed behind each slit that corresponds to the wavelength of a line that is to be measured, or one or more photographic plates or pieces of film are placed on the focal of the monochromator. The instrument is a spectrometer if a photomultiplier tube or other photon detectors are used. It is a spectrograph if the detector is a photographic plate or film. Commercial spectrometers can contain as many as 90 exit slits. The analyst chooses the exit slits that correspond to the spectral lines that are to be measured and places a detector behind each chosen slit. For many analyses between 20 and 35 detectors are simultaneously used at different slits to simultaneously assay one element for each detector. Each detector is termed a channel. A spectrometer of that design is a direct reader or a direct-reading spectrometer. If the chosen slits are too close together to permit placement of a detector behind each, mirrors can be used behind the slits to reflect the radiation to the detectors. In a spectrograph the entire spectrum of the sample is simultaneously recorded. Each spectral line forms an image in the shape of the entrance slit to the monochromator on the film. Generally the entrance slit and the images are narrow rectangles. Measurement of the intensity of a particular spectral line is a requirement for quantitative analysis. Intensity measurements with films and plates are not as easily accomplished as they are
With direct readers quantitative analysis is straightforward. A channel is assigned for each element. The measured intensity of the spectral line is used with a working curve to quantitate the element in the sample. The wavelengths must be carefully chosen to prevent spectral interference. Typically precision obtained with direct readers are in the range of ±0.3 to 3 percent. When a photographic plate or film is used as the detector, the precision is not as good as that achieved with direct readers. In order to obtain accurate and precise results all of the experimental conditions must be carefully controlled. Variables such as exposure time, film type, and developing conditions particularly are important. Automated development of the film or plat is advisable, whenever possible, in order to minimize changes in the development process. With careful control of conditions, errors between 1 and 10 percent can be achieved using photographic detection. Regardless of the type of detection used for the assay, the precision of the results can be improved by matrix-matching the standards with the sample. Use of the internal-standard method also improves precision. Usually a working curve is prepared by plotting the ratio or logarithm of the ratio of intensity of the standard's line to the internal standard's line as a function of the logarithm of the concentration of the standard. The corresponding ratio for the analyte is obtained and the concentration determined from the working curve. In many cases the precision and accuracy of an analysis of a compound that contains organic components can be increased by washing the sample prior to the assay. Normally the sample is placed in a platinum or silica crucible and heated in a muffle furnace to 500'C. Ashing can also be done in a low-temperature oxygen plasma. The temperature should be sufficiently high to remove all traces of any organic matrix of the analyte, but it cannot be high enough to vaporize the assayed elements. The ashing process is similar to that performed in furnace cells during atomic absorption spectrophotometry. Internet References: www.anachem.umu.se/jumpstation.htm www.anachem.umu.se/cgi/jumpstation.exe?AtomicSpectroscopy www.anachem.umu.se/cgi/jumpstation.exe?OpticalMolecularSpectroscopy www.minyos.its.rmit.edu.au/~rcmfa/mstheory.html http://science.widener.edu/sub/ftir/intro_it.html
http://www.s-a-s.org/ http://www.chemsw.com http://www.scimedia.com/chem-ed/spec/atomic/aa.htm http://nercdg.org http://www.analyticon.com www.lcgmag.com/ www.lcms.com/ www.dq.fct.unl.pt/QOF/Chroma.html www-ssg.chem.utas.edu.au/ www.yahoo.com/science/chemistry/chromatography/ www.onlinegc.com http://www.aurora-instr.com http://www.chem.ufl.edu/~itl/3417_s98/spectroscopy/aes.htm http://www.rohan.sdsu.edu/staff/drjackm/chemistry/chemlink/analytic/analyt1.html http://www.cofc.edu/~deavorj/521/jpd521.htm http://www.scimedia.com/chem-ed/spec/atomic/aes.htm
