Flame Atomic absorption spectroscopy (FAAS)
First, the liquid solvent is evaporated, leaving the dry sample. Then, the solid sample is vaporized to a gas and mixed as an aerosol with combustible gases like acetylene and air or acetylene and nitrous oxide. Lastly, the compounds of the sample are broken into free atoms by using a flame of temperature from 2100 to 2800 degree C. Atoms of the element of interest (in this case, lead) will be reduced to its atomic state.
Radiation of 283.3nm is sent through using a hollow cathode lamp. A beam of light from the lamp is focused through the flame. The cathode of the lamp is made from the same element being determined. The beam passes through the flame into a monochromator and then a detector. The monochromator consists of mirrors which help to separate the beam from any background noise and light.
Free, unexcited atoms at ground-state of the element absorb light at a specific wavelength, and the reduction of light energy detected is the quantitative measure of the concentration of the element in the sample.
An example of a detector is the photomultiplier, which is an extremely sensitive detector for UV light and visible light. It can detect the amount of reduction of light intensity due to absorption by the analyte, and this can be directly related to the amount of the element in the sample.
This diagram shows how the photomultiplier works:
Light enters the photomultiplier tube and strikes the photocathode layer. This causes electrons to be emitted.
The electrons will be directed towards the electron multiplier. The electron multiplier is made up of many electrodes, called dynodes. The dynodes all have different voltages, where each dynode has a higher positive voltage than the previous one. This is so that electrons can be multiplied.
The photoelectrons are electrostatically accelerated towards the first dynode because it is positive. They hit the first dynode with greater energy than when they left the photocathode. More low energy electrons are released, which are in turn attracted to the greater positive field of the next dynode, and they are similarly accelerated by the positive field of the next dynode. This process keeps repeating and electrons will keep hitting dynodes and releasing more electrons until they are collected at the anode.
The accumulation of charge hitting the anode results in a sharp current peak, amount of light transmitted can be measured and thus the amount of light absorbed by the analyte can thus be determined.
http://www.galbraith.com/spectroscopy.htm
http://www.radio-electronics.com/info/data/thermionic-valves/photomultiplier/what-is-a-photomultiplier-basics.php
http://www.et-enterprises.com/photomultipliers/understanding-photomultipliers