Detector Height (mm) Absorbance 2 494.5 Ni Fe Fe ـنـشـ 495.0 Wavelegnth (nm) Ni Fe Fe 494.5 495.0 Fe Wavelength (nm) 495.5 Fe Fe Cr (Fe+ Fe) C 496.0 Figure 2. Fraunhofer effect spectrum of the sun including the c band. 495.5 496.0

Principles of Instrumental Analysis
7th Edition
ISBN:9781305577213
Author:Douglas A. Skoog, F. James Holler, Stanley R. Crouch
Publisher:Douglas A. Skoog, F. James Holler, Stanley R. Crouch
Chapter16: An Introduction To Infrared Spectrometry
Section: Chapter Questions
Problem 16.14QAP
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The dark lines in the solar spectrum were discovered by Wollaston and cataloged by Fraunhofer in the early days of the 19th century. Some years later, Kirchhoff explained the appearance of the dark lines:  the sun was acting as a continuum light source and metals in the ground state in its atmosphere were absorbing characteristic narrow regions of the spectrum. This discovery eventually spawned atomic absorption spectrometry, which became a routine technique for chemical analysis in the mid-20th century. Laboratory-based atomic absorption spectrometers differ from the original observation of the Fraunhofer lines because they have always employed a separate light source and atomizer. This article describes a novel atomic absorption device that employs a single source, the tungsten coil, as both the generator of continuum radiation and the atomizer of the analytes. A 25-μL aliquot of sample is placed on the tungsten filament removed from a commercially available 150-W light bulb. The solution is dried and ashed by applying low currents to the coil in a three-step procedure. Full power is then applied to the coil for a brief period. During this time, the coil produces white light, which may be absorbed by any metals present in the atomization cloud produced by the sample. A high-resolution spectrometer with a charge-coupled device detector monitors the emission spectrum of the coil, which includes the dark lines from the metals. Detection limits are reported for seven elements:  5 pg of Ca (422.7 nm); 2 ng of Co (352.7 nm); 200 pg of Cr (425.4 nm); 7 pg of Sr (460.7 nm); 100 pg of Yb (398.8 nm); 500 pg of Mn (403.1 nm); and 500 pg of K (404.4 nm). Simultaneous multielement analyses are possible within a 4-nm spectral window. The relative standard deviations for the seven metals are below 8% for all metals except for Ca (10.7%), which was present in the blank at measurable levels. Analysis of a standard reference material (drinking water) resulted in a mean percent recovery of 91%. This report attempts to give an historical perspective on the development of a novel atomic spectrometer based on the Fraunhofer effect.

 

1. This paper attempted to atomize samples in a novel way, by putting them on the tungsten wire of a regular incandescent light bulb. List the most common methods of atomization in commercial AA instrumentation.

2. In Figure 2 above, the atomic spectrum is shown. Explain why atomic absorption bands are so narrow.

3. Why is it so critical to control temperature reproducibly in atomic absorption spectroscopy? Give at least three factors which will control flame temperature.

Detector Height (mm)
Absorbance
2
494.5
Ni
Fe
Fe
ـنـشـ
495.0
Wavelegnth (nm)
Ni Fe
Fe
494.5
495.0
Fe
Wavelength (nm)
495.5
Fe
Fe
Cr
(Fe+ Fe)
C
496.0
Figure 2. Fraunhofer effect spectrum of the sun
including the c band.
495.5
496.0
Transcribed Image Text:Detector Height (mm) Absorbance 2 494.5 Ni Fe Fe ـنـشـ 495.0 Wavelegnth (nm) Ni Fe Fe 494.5 495.0 Fe Wavelength (nm) 495.5 Fe Fe Cr (Fe+ Fe) C 496.0 Figure 2. Fraunhofer effect spectrum of the sun including the c band. 495.5 496.0
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