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intro
uv-visible spectroscopy is based on molecular interactions
measures electronic transition of atoms
used for quantitative elemental analysis
transition occurs in the visible region and are measured by absorption or emission
samples must be atomised by heating
sample atomisation
sample solution —> nebuliser (removal of solvent from aerosol) —> plasma, flame or electric heating (desolvation, liquefaction, vaporisation, atomisation)
after atomisation
to persons AES a much higher temperature is required as atoms need to be in an excited state
AES is very temperature dependant and instruments designed to protect flame from draughts
elements with low ionisation potential are ideal for AES analysis
range of elements can be increased by hotter flames
flame temp can increase by using higher flow rates or different gas mixtures
plasma AES instrumentation
flames have limited temperature —> limited elemental range
plasma sources overcome this limitation
plasma generated by energising argon gas
plasma = ionised, electrically natural gas
temperatures up to 10,000 degrees
most common source: inductively couple plasma
ICP-AES advantages
very high temp = all elements atomised
multi element, simultaneous or sequential analysis
requires less sample
inert argon atmosphere —> chemical interferences
stable signals and similar operating conditions for many elements
low background emission —> low detection limits
wide linear range (10³ - 10^6)
excellent precision
requires calibration with multi element standards
atomic absorption spectroscopy - instrumentation
found state atoms absorb characteristic wavelength
energy source - hollow cathode lamp
each element requires its own lamp
multiple lamps may be mounted but elements analysed individually
instrumentation costly due to lamps
AAS - disadvantages
large dilution of analyte —> low sensitivity
high sample consumption
flame conditions optimised for each element
minimising these problems
use long path burners to increase absorption path length
replace flames with graphite furnace —> EAAS
electrothermal atomic absorption
uses electrically heated graphite tube
sample retained longer and in smaller volume —> higher sensitivity
very small samples size
EAAS - heating stages
drying, charring, atomisation
conditions must be optimised of specific analyte and sample matrix
matrix. modifies added to prevent analyte loss during charring
atomic spectroscopy interferences
common due to high temperatures
produce reactive species and promote chemical reactions that can arise from the fuel and oxidant used
less severe in plasma
two main types - spectral interference, chemical interference
spectral interference - flam background
broad absorption from molecular species
reduced using background connection
spectral interference - overlapping lines
emission from another element at similar wavelength
minimise by changing wavenelgth or remove impurity
chemical interference - refractory compound formation
anions in the sample can form stable, non volatile compounds with the analyte
reduced AAS signal because atoms are no longer free to absorb radiation
overcome by adding releasing agents
chemical interference - ionisation interference
easily ionised elements released electrons that suppress analyte ionisation
reduces signal intensity
minimised by adding ionised element to both samples and standards to keep the effect constant
chemical interference - use of organic solvents
water can increase background absorption and lower sensitivity
organic solvents improve atomisation efficiency
benefits include increased rate of aspiration, finer aerosols, faster evaporation, better combustion
AS sample preparation
must be in solution form, solids aired to constant weight
preparation varies by sample type
plant materials - wet oxidation, extraction, titration
biologic samples - protein preparation or ashing
tissues - dry washing, acid extraction
metals - acid digestion and filtration
quantitative analysis
beer Lambert, measurements done in triplicate
standards run first to check calibration
AES is linear; ASS often quadratic