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Spark OES - Trinity College Dublin

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<strong>Spark</strong> Optical Emission Spectroscopy<br />

Analytical<br />

Workshop 2012<br />

Dr Heath Bagshaw – CMA, <strong>Trinity</strong> <strong>College</strong> <strong>Dublin</strong>


Why Use <strong>Spark</strong> <strong>OES</strong> Analysis?<br />

• Quick, reliable and reproducible analysis technique<br />

• Can analyse wide range of elements<br />

• Usually used for metals\alloy analysis, such as :-<br />

Steel, cast iron and high alloyed steels<br />

Non-ferrous metals and their alloys<br />

AI: wrought alloys, casting alloys, etc.<br />

Cu: bronze, brass, cupronickel, etc.<br />

Mg, Zn alloys, solders<br />

Nitrogen in steel<br />

P in aluminium<br />

Ultra low carbon analysis<br />

Elements such as Se, La, Te, etc.<br />

• Good limit of detection for most materials - generally less then 50 ppm although 10<br />

ppm detection limits are typical.<br />

• Higher resolution spectrometers (using PMTs) have limits of detection of


Colours - Flame Testing<br />

• When an element is burned it burns with a distinct colour –<br />

Barium Strontium Potassium<br />

• These colours are due to the emission spectrum of the element.<br />

Analytical<br />

Workshop 2012


Analytical<br />

Workshop 2012<br />

Basic Theory


• The emitted radiation\light is split using a prism or diffraction grating to produce a<br />

spectrum.<br />

More Basic Theory<br />

Analytical<br />

Workshop 2012


Basics cont<br />

• modern equipment uses a slightly different set up:-<br />

• A diffraction grating is used to produce the spectrum and mirrors focus the radiation<br />

onto detectors.<br />

Analytical<br />

Workshop 2012


Emission Spectra<br />

• In the case of optical emission spectroscopy the EM radiation is in the visible\optical<br />

region of the EMS which we see as different colours depending on the<br />

wavelength\energy of the emitted photon.<br />

• The energy of a photon and it’s wavelength are related by the following equation:-<br />

E = hc<br />

Analytical<br />

Workshop 2012<br />

λ<br />

where h is Planck's constant (6.626 × 10 -34 joules) and c is the<br />

speed of light (2.998 × 10 8 m/s).


Examples of Emission Spectra<br />

Emission spectrum of H<br />

Emission spectrum of Fe<br />

Analytical<br />

Workshop 2012


The System<br />

Sample<br />

‘sparked’ to<br />

produce a<br />

‘burn’<br />

Emitted Light<br />

Polychromatic light<br />

CCD measures the<br />

light intensity at<br />

each wavelength<br />

Diffraction Grating,<br />

Produces a<br />

dispersion spectrum<br />

Computer<br />

Calculation of results<br />

Comparison to Standards<br />

Data output and storage<br />

Analytical<br />

Workshop 2012


The Spectrometer (Schematic)<br />

• The diffraction grating Is like a concave mirror with lines ruled on it.<br />

• Modern Gratings have up to 4000 rules/mm.<br />

Entrance Slit<br />

130 – 800 nm<br />

Grating<br />

• The incoming light is reflected and diffracted, producing the spectrum<br />

Analytical<br />

Workshop 2012


The Spectrometer (Real)<br />

Entrance Slit<br />

130 – 800 nm<br />

• The CCD chips simultaneously detect all incident light and determine the intensity of<br />

each wavelength.<br />

Analytical<br />

Workshop 2012


The Sample<br />

• Generally speaking the sample is metallic, flat and freshly ground.<br />

• The sample is clamped in place and ‘sparked’ to generate a spectrum<br />

– this leaves ‘burn’ marks on the sample:-<br />

‘Burn’ marks<br />

Sample<br />

• If the sample does not ‘burn’ correctly spurious results can be produced.<br />

• Poor burning can be caused by poor grinding and rough\uneven surfaces.<br />

Analytical<br />

Workshop 2012


Analysis<br />

• The Intensity of an emission line (colour) is proportional to concentration – allows<br />

measurement of ‘how much’ of each element is present.<br />

• A number of standards are run first to set up a calibration curve, these take into<br />

account any matrix matching difficulties (i.e. overlap of elements in some materials).<br />

Take the example of Fe<br />

Requires six standards to correctly calibrate the instrument<br />

for Fe analysis.<br />

Analytical<br />

Workshop 2012


Analysis Continued<br />

• Once calibration is completed numerous samples can be analysed.<br />

• The sample is simply clamped into place, ‘sparked’ and a spectrum collected.<br />

• The spectrometer collects the intensity of light at all wavelengths and compares this<br />

to the values for the calibration standard. This gives an accurate value of the elements<br />

present in the sample.<br />

• Multiple sparks are collected until concordant results are obtained within an<br />

acceptable standard deviation.<br />

• Further samples of the same alloy type can then be analysed.<br />

• Different alloys require re-calibration before analysis can occur.<br />

Analytical<br />

Workshop 2012


System Types<br />

• <strong>Spark</strong> Optical Emission Spectrometers come in all shapes and sizes for a multitude of<br />

uses.<br />

• Foundry\steel making applications – usually floor standing to analyse composition of<br />

metals during production – quality control.<br />

• Portable units often used in manufacturing plants to assess<br />

metal composition.<br />

• Portable units to analyse large immovable materials<br />

• Hand held units to assist in scrap sorting<br />

• The smaller the unit the less accuracy In the measurements<br />

– so convenience over quality – still useful as analysis can be<br />

Performed anywhere.

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