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Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration
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Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Dec 20, 2015

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Page 1: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Atomic Emission - AES

Thermal excitation M → M*

Radiative decay to lower energy level M* → M + h

Emission signal directly proportional to concentration

Page 2: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Holy Grail of Atomic Spectroscopy

For one sample:

The ability to measure all elements at all ranges of concentration at one time.

Page 3: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Excitation Source

The atoms are excited by energy provided by the source.

The energy created by a flame can excite only a few atoms, e.g. alkali metals

Other atoms (especially non-metals) need much higher energy - plasma

If you only have a flame instrument, you can use AES for alkali metals (and a few others), otherwise you should use AAS to achieve good detection limits.

Page 4: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Types of high energy analytical plasmas

DC Arc 4000-5000 K

HV Spark 40,000

Direct Current Plasma 6000-10,000

Inductively Coupled Plasma (ICP) 6000-8000

Microwave Induced Plasma (MIP) electrodeless

5000-7000

Capacitively Coupled Microwave Plasma (CMP) electrode

5000-7000

Page 5: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

PlasmasIonized gas that is electrically neutral

Very high temperature and energy

Contains ions, electrons, neutral atoms & molecules

Page 6: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Inductively Coupled Plasmas

Up to 20 mL/min Ar flow

Annual cost of several thousand dollars

Ionized Ar flow, sustained in a torch by the RF field generated by induction coils.

Page 7: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Characteristics of Plasma AES

Sufficient energy to excite all elements

Capable of doing solids, liquids, or gases-sample introduction via nebulizer, ETV, laser ablation, others

Tolerant to variety of solvents and solutions

Simultaneous multielement analysis

Large Linear Dynamic Range (LDR)

Low LOD

Page 8: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

ICP-AES spectrum

Page 9: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

ICP AES Calibration CurveIf you can interpret

your spectrum, you can get great quantitative results.

Calibration curve is plotted as log/log, because the LDR spans several orders of magnitude.

Page 10: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Internal Standard

An internal standard is used to compensate for various random (and even systematic) errors.

A big random error in plasma emission spectroscopy is power/intensity fluctuations of the plasma.

Reasoning: fluctuations effect on analyte will be the same as the effect on the internal standard.

Page 11: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Quantitative Analysis - Calibration with Internal Standard

Internal standard must be something not present in your standards or sample (in this example, Y)

The signal plotted is the ratio:

Intensity ratio = Analyte signal Yttrium signal

Page 12: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

Homework problemy = 4.2781x + 7.1758

0

50

100

150

200

250

300

350

400

450

500

0 20 40 60 80 100 120

Cu concentration (ppm)

intensity ratio

y = 0.7619x + 1.0441

0

0.5

1

1.5

2

2.5

3

-0.5 0 0.5 1 1.5 2 2.5

log concentration (ppm)

log intensity ratio

linear-linear plot log-log plot

When your LDR spans more than 2 orders of magnitude, it can be helpful to do a log-log plot so you can see your data points better.

Page 13: Atomic Emission - AES Thermal excitation M → M* Radiative decay to lower energy level M* → M + h Emission signal directly proportional to concentration.

ICPAdvantages

Analysis of solutions or dissolved solids

LDR spans several orders of magnitude

Detection limits in the parts per billion range

Multielement analysis: Determine up to 70 elements in two minutes per sample

Disadvantages

ionization leads to complex spectra

need high resolution monochromator

Expensive

Plasma source leads to messy background - fluctuations