ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
Introduction to Atomic Emission Spectrometry
Lisa Goldstone, Odile Hirsch*
Jobin Yvon, Inc., 3880 Park Avenue, Edison, NJ 08820
* Jobin Yvon SAS, 16-18, rue du Canal, 91165 Longjumeau, Cedex, France
Keywords: atomic emission, sample preparation, analysis
1 Principle of atomic emission
For a liquid sample, the atomization process can
be illustrated as follows.  
1.1 General information
A  given  atom  has  a  large  number  of  possible
energy levels. An emission spectrum is produced
by  an  electronic  transition  from  a  high  energy
level En to a lower energy level Em. The accept-
able  transitions  are  given  by  the  quantum
mechanics  selection  rules.  A  quantity  of  energy
Q  is  transferred  to  an  atom  by  collision  with
another  particle,  resulting  in  excitation  of  the
atom.  An  electron  from  an  outer  layer  of  the
atom  is  excited  to  a  higher  energy  level.
Following  this  electron  excitation,  the  electron
returns,  in  one  or  several  stages,  to  its  original
energy level.
The  atomic  emission  technique  measures  the
energy lost by an atom passing from an excited
state  to  a  lower  energy  state.  The  energy  is
released  in  the  form  of  light  rays  with  a  wave-
length  l  ,  or  more  specifically,  in  the  form  of  a
photon with a frequency v carrying energy h x v. 
Figure 1: Energy transition
The  atomic  emission  spectrum  is  composed  of
discrete  spectral  lines.  The  number  of  photons
emitted is proportional to the number of atoms of
the  element  present.  To  be  excited,  the  sample
must be atomized, meaning dissociated into free
ions or atoms.
Figure 2: Transformation of sample
Depending on the species excited, the lines
have different types:
* emission from an atom: line I
* emission from an ion once ionized: line II
* emission from an ion twice ionized : line III
Lines I and II are frequently observed; lines III are
rarely observed in the plasma and lines of a high-
er  degree  are  not  observed.  This  is  due  to  the
energies involved.
1.2 Plasma
The  emission  phenomena  takes  place  in  a  plas-
ma. A plasma is an electrically neutral highly ion-
ize ionized gas. The gas used is typically argon.
1.2.1 Plasma creation
An  argon  flow  travels  through  a  crystal  tube
inside a solenoid. The lines of force, generated by
the magnetic fields, are directed along the axis of
the solenoid inside the tube and take the form of
an ellipse on the outside.
ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
2.1 Introduction
As  discussed  previously,  an  atom  subjected  to  a
plasma  emits  characteristic  photons.  This  property
makes
it  possible  to  perform  a  qualitative
analysis. The number of photons emitted is propor-
tional to the number of atoms of the considered ele-
ment. This is the basis of the quantitative analysis.
2.2 Qualitative analysis
A  qualitative  analysis  consists  of  searching  for  the
elements  in  an  unknown  sample.JY.  The  lines
recorded  reveal  the  presence  of  an  element.  An
approximate quantification can also be performed.
To select the lines, see the wavelength tables. Note
that experience will play a major role in interpreting
the spectra. This semi-quantitative analysis can be
performed  very  rapidly  using  the  JY  Win-IMAGE
option. 
2.3 Quantitative analysis
The quantitative analysis links the energy emitted to
the  number  of  atoms  contained  in  the  sample.
Atomic  emission  is  not  an  absolute  method.  The
relation existing between the intensity emitted by a
line and the concentration of the associated element
must be calculated: this is called the line calibration
curve. The advantage of ICP-OES is that these cali-
bration  curves  are,  in  most  cases,  linear  to  several
orders of concentration. Great care must be taken in
calculating these curves as they will determine the
ultimate accuracy of the analysis.
2
An electrical discharge is created to arc the plasma
by partially ionising the gas in the torch.
2 Analysis
The  electrons  produced  are  subjected  to  the  mag-
netic  field  induced  and  circulate  along  the  axis  of
the crystal tube describing annular circuits. Induced
or  eddy  currents  are  thus  produced.  The  electron
path is stopped by collision, resulting in heating and
ionisation of the other gas atoms. The plasma is self
maintaining and continous.
Figure 3 : Magnetic field
1.2.2 Plasma gas
The gas generally used is argon, which like all rare
gases, is monatomic, chemically inert and has a high
ionisation  energy  (15.6  eV).  A  certain  number  of
advantages are provided by argon:
– Emission of a relatively simple spectrum producing
little spectral interference in emission spectrometry,
– Capacity to atomise, ionise and excite most of the
elements of the periodic table,
–  Absence  of  formation  of  stable  composites
between argon and elements,
– Lower cost than that of other rare gases as it is the
most widely available (1 % in air).
Its  only  limitation  is  its  low  thermal  conductivity
compared to that of molecular gases such as nitro-
gen or oxygen. During heating, the argon ions trans-
fer energy to the atoms present in the sample solu-
tions.
ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
Repeatability:  Represents  the  fluctuations  of  the
signal during a single reading under the same meas-
urement conditions.
Reproducibility:  Represents  the  fluctuations  of  the
signal  when  one  of  the  measurement  parameters
has varied.
Robustness: Capacity of plasma to accept different
changes  without  significant  variation  in  element
concentration.  These  changes  can  come  from  the
matrix,  the  analytical  parameters  or  the  environ-
ment.
Sensitivity:  Slope  of  the  calibration  line;  signal
intensity versus concentration.
Uncertainty: Estimation within which the true value
is located.
2.4.1 Repeatability, reproducibility and accuracy
These  three  terms  are  often  understood  to  mean
the same thing. Repeatability and reproducibility are
expressed as a relative standard deviation. The only
difference is the fact that for reproducibility, one of
the  parameters  has  varied.  Accuracy  is  a  principle
that  can  be  difficult  to  measure.  It  is  evaluated
using  certified  reference  materials.  It  mainly
depends  on  the  calibration  curve  and  the  prepara-
tion of the samples.
The  repeatability  and  accuracy  concepts  can  be
summarised using a target. The true value being the
center of the target.
Figure 4: Calibration line
2.4 Analytical performance
An emission spectrometer provides a large number
of  analytical  performance  features:  accuracy,
repeatability, reproducibility, selectivity, robustness,
sensitivity, detection limit, linearity, dynamic range
…
The main terms are defined below:
Accuracy:  The  accuracy  of  an  instrument  is  its
capacity to give results that are free of systematic
error, meaning having a good degree of exactitude.
The  accuracy  is  evaluated  by  the  difference
between  the  measured  mean  value  and  the  true
value of element concentration.
Blank: Matrix without analytes
Detection  limit:  Smallest  concentration  which  can
be detected with certainty with respect to a blank
Error: Deviation  between  the  mean  value  and  the
true value
Fidelity:  Capacity  of  an  instrument  to  give  good
repeatability.
Long term stability: Equivalent to repeatability over
a long period of time (several hours).
Figure 5: Repeatability and Accuracy
Precision: Corresponds to  repeatability  and  repro-
ducibility.
Quantification limit: Concentration corresponding to
a given repeatability (for example 5%).
In figure 5 the second case is better than the third,
even  though  the  result  seems  bad  (high  relative
standard deviation).
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ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
2.4.2 Detection limits (LOD), Quantification limit
(LOQ)
expressed in multiples of standard deviation.
Figure 8 shows the influence of the coefficient k on
the percentage of error.
Here, we assume that  the fluctuation  of the  spec-
tral  background  follows  a  Gaussian  distribution
defined by its standard deviation.
Figure 6: Gaussian distribution of spectral back-
ground distribution fluctuations
The  detection  limit  is  derived  from  the  signal  that
will  be  statistically  possible  to  extract  from  the
background.  This  comes  down  to  stating  the  fol-
lowing question: does a measurement point belong
to the background or to the signal?
k  corresponds  to  a  safety  coefficient.  The  higher
the k, the easier it will be to differentiate a signal
point from a background point.
Figure 8: Smallest detectable signal XL
IUPAC recommends applying k = 3. The percent-
age of error is then 13%.
Three equivalent formulas are used to express the
detection limit:
(CL., concentration limit) :
(1) CL = 3 C SB /S
(2) CL = 3 C RSDB/SBR
(3) CL = 3 BEC RSDB
Where,
S = net signal of solution
C = concentration of solution measured.
sB = standard deviation of blank
RSDB = standard deviation relative to blank
SBR = signal to background ratio
BEC = Background Equivalent Concentration
Formula (2) is mainly used for plasma optimisation.
Formula (3) is used to calculate the detection limits
for a given matrix following a calibration.
The  Background  Equivalent  Concentration  (BEC)  is
represented  on  the  figure  9.  It  corresponds  to  the
concentration  for  which  the  signal  is  equal  to  the
background (S = B or SBR = 1).
Figure  7:  Detection  of  a  point  among  the  back-
ground noise
The Figure 7 represents the overlap of the fluctua-
tions of background B and signal S as a function of
the  deviation  between  the  two  mean  values,
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ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
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2.4.3 Robustness
Depending  on  the  composition  of  the  matrix,  the
same concentration of an element will not give the
same signal.For example, 5 ppm of Mg in water or
in NaCl 10 g/L does not give the same net intensi-
ty.
Figure 9 : Background Equivalent Concentration
(BEC)
BEC is the absolute value of the ordinate of the ori-
gin  of  the  calibration  curve  when  no  background
correction  is  applied.  If  a  background  correction  is
applied, use formula (2).
For the detection limit, RSD is expressed:
RSD =
/1(
k
2)
Therefore, for k = 3, RSD = 47%.
To  define  the  quantification  limit,  you  define  the
maximum desired RSD, for example 5 or 10%.
RSD = 10%, for LOQ = 4.5 LOD
RSD = 5%, for LOQ = 10 LOD
RSD = 2% for LOQ = 30 LOD
Generally, the minimum LOQ used = 3 LOD.
The detection limit is an estimation.
The quantification limit is a measurement.
The detection limit can be calculated in water or in
a  special  matrix.  It  is  very  important  to  know  the
detection  and  quantification  limits  for  each  of  the
applications.
Figure 10: Influence of matrix
To minimize this difference, the most robust plasma
possible must be used. The robustness can be eval-
uated by the ratio between two lines (an ionic line
and  an  atomic  line).  For  this  purpose,  we  use  the
ratio provided by two Magnesium lines:
Mg II 280 nm/ Mg I 285 nm.
The higher the ratio, the more robust is the plasma.
A plasma is robust when the ratio of magnesium is
greater than 6. In this case, the plasma is in ther-
modynamic equilibrium.
3 Sample Preparation
The samples are usually introduced into the plasma
in solution form but solids, finely divided, can also
be used. Care should be taken in obtaining a solu-
tion of a solid sample since there is a risk of loss of
element,  or  contamination.  The  final  solution
obtained  by  the  analyst  depends  on  the  nature  of
the sample and the concentration of elements to be
determined.
Two main types of sample preparation are used for
ICP analysis:
– Acid Digestion.
– Dry attack.
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ICP OPTICAL EMISSION SPECTROSCOPY
TECHNICAL NOTE 12
3.1 Acid Digestion
3.3 Remarks
Acids, whether singly or in a mixture, use their oxi-
dising  or  reducing  properties.  Care  must  be  taken
with  respect  to  possible  loss  of  volatile  elements.
For example, loss of As, Se, Sn in the form of chlo-
ride in the presence of HCl. Creation of precipitates
of Ca, Ba, Pb also represents a possible error in the
presence  of  H2SO4.  Open  and  closed  microwave
systems are increasingly used in laboratories.
3.2 Dry attack
Alkaline  fusion  is  often  used,  as  well  as  high-tem-
perature  calcination  (450  –  600  °C)  with  acid
recovery of ashes. Care must be taken with respect
to contaminants introduced by the reagents. Losses
by  volatilisation  and  insolubilisation  can  be  more
than negligible.
– Whatever the type of solution, the quantity of acid
or flux must be as low as possible to ensure mini-
mum perturbation of the plasma. Certain acids are
preferable  to  others  as  they  perturb  the  plasma
less.
Order  of  preference  (from  more  favorable  to  least
favourable): HNO3, HCl, HCLO4, H2SO4, H3PO4.
–  Caution,  HF  requires  a  specific  sample  introduc-
tion system.
– Na has a high depressive effect on sensitivity.
– The presence of hydrofluoric acid can result in the
formation  of  Ca,  Mg  Mn…  fluoride  precipitates.
This occurs frequently during mineralization of geo-
logical  products,  even  after  evaporation  of  the
hydrofluoric acid. This can be avoided by adding a
few drops of boric acid.
In the USA:
Jobin Yvon Inc.
3880 Park Avenue
Edison, NJ 08820
Tel: 1-732-494-8660
Fax: 1-732-494-8796
E-mail:
emission@jyhoriba.com
1-877-JYHORIBA
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Jobin Yvon S.A.S.
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91165 Longjumeau Cedex
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FAX:  (81) 75 321 5725
www.horiba.com
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Other Countries: Contact JY
S.A.S.
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