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Dr. P. K. Mani 
BCKV
E – energy difference between two levels; 
h – Plank’s constant, 6.626068 × 10-34 m2kg/s; 
c – speed of light, 299 792 458 m/s; 
λ – wavelenght, nm 
Ion 
Emission 
Atom 
Emission
Atomic Emission Spectrometry (AES) 
In this method, a sample is normally excited 
by the thermal energy of a flame, argon plasma 
or an electrical discharge. The atoms in the 
sample absorb thermal energy, causing the 
excitation of the outer orbital electrons. 
As the excited state is short lived, the excited 
atoms return back to the ground state after a 
very short lifetime (typically10-6 to 10-9 s). 
This is accompanied by the emission of EMR, 
normally in the form of light in the UV-VIS 
region. 
The wavelength of the emitted radiation and 
its intensity provide the qualitative and 
quantitative information about the analyte. 
The atomic emission spectroscopy employing 
flame as a means of excitation is called ffllaammee 
pphhoottoommeettrryy oorr ffllaammee eemmiissssiioonn ssppeeccttrroossccooppyy 
((FFEESS))..
PRINCIPLE OF FLAME PHOTOMETRY 
For a few elements, such as the alkali metals Na and K, an air/ 
acetylene flame is hot enough not only to produce ground state atoms, 
but to raise some of the atoms to an excited electronic state. The 
radiant energy emitted when the atoms return to the ground state is 
proportional to the concentration and is the basis of flame emission 
spectroscopy. i.e., at 589 nm, Na -------> Na* (energy from flame) 
Na* -------> Na + hn (at 589 nm)
Within the flame, there are many more atoms in the ground state than 
in the excited state. For Zn, for instance, in a 2000K flame, there are 
7.3 X 1015 atoms in the ground state for every excited atom. 
The alkali metals are elements with unocuppied atomic orbitals of 
low enough energy to be sufficiently populated by a flame. 
For the element sodium, two inner shells are completely filled and 
there is one electron in the outer third shell. 
This electron is said to be in an s orbital. However, the remaining 
orbitals of the third shell and all the orbitals of the fourth, fifth and sixth 
shells, etc., are empty. When the outer electron of sodium is in the s 
orbital the atom is said to be in the “ground state” or the “unexcited 
state”. If the atom absorbs radiation the electron undergoes a transition 
to one of the empty orbitals at the higher energy levels.
Inductively coupled plasmas 
By definition, a plasma is an electrical conducting gaseous mixture 
containing a significant concentration of cations and electrons. (The 
concentrations of the two are such that the net charge approaches zero.) In the 
argon plasma employed for emission analyses, argon ions and electrons are 
the principal conducting species, although cations from the sample will also 
be present in lesser amounts. 
Argon ions, once formed in a plasma, are capable of absorbing 
sufficient power from an external source to maintain the temperature at 
a level at which further ionization sustains the plasma indefinitely; 
temperatures as great as 10,000 K are encountered. 
A plasma is an ionized gas that is macroscopically neutral (i.e. 
with the same number of positive particles (ions) and negative 
particles (electrons)). If a monoatomic gas, X, is used, a plasma can 
be described by the following equilibrium: 
Ar : 1s22s22p63s23p23p23p2 
x 
y 
z 
[Ne]3s23px 
23py 
23pz 
2
The gas that is used to generate the plasma (plasma gas) is Argon. 
Like any noble gas, 
Argon is a mono atomic element with a high ionization energy (15.76 
eV), and is chemically inert. 
Consequently: 
(i)a simple spectrum is emitted by argon in contrast to a flame where 
primarily molecular spectra are observed; 
(ii) argon has the capability to excite and ionize most of the elements of 
the Periodic Table; 
(iii) no stable compounds are formed between argon and the analytes.
The plasma acts as reservoir of energy provided by the radio frequency 
field, and transfers this energy to an analyte, M. 
the atomization of a sample is a relatively long process (of the order of a 
few ms), while ionization and excitation are very fast processes. 
Various ionization and excitation processes have been suggested resulting 
from the presence of species that are obtained during the plasma generation. 
The major species are not only the argon ions, Ar, and the electrons, e, but 
also the excited argon atoms, Ar*,with the special case of the metastable 
levels, Arm
The hf field is produced by a rf generator and accelerates the electrons. 
These electrons will ionize the plasma gas: 
the kinetic energy of the projectile 
electron must be greater than the 
ionization potential of the bound 
electron to be ionized 
Then, through the process of radiative recombination, the argon ions 
are recombined with electrons to lead to excited argon atoms and to a 
significant background: 
This background is mainly produced by the process of radiative 
recombination in the ultraviolet (UV) region, while bremsstrahlung 
must also be taken into consideration in the visible part of the spectrum . 
Except for the resonance lines that are located at 106.7 nm and 104.8 
nm, there are no argon atomic lines below 300 nm.
In addition to ionization and excitation, beta particles may also transfer 
energy by a process called Bremsstrahlung. As negative beta particles 
approach the positively charged nucleus of an atom, some are slowed down and 
pulled into a new direction (like the gravitational pull of the earth on a 
satellite). As the electrons are slowed down some energy is released in the 
form of X-rays called Bremsstrahlung. These X-rays are more penetrating 
than the beta particles and may require more shielding. Plastic is commonly 
used to shield beta particles because low density materials result in less 
production of Bremsstrahlung
Electron ionization (EI, formerly known as electron impact) is an ionization 
method in which energetic electrons interact with gas phase atoms or 
molecules to produce ions. 
where M is the analyte molecule being ionized, e− is the electron and 
M+• is the resulting ion. 
Radiative recombination (RR) is a non-resonant, one step 
recombination process in which a free electron recombines with an 
ion, emitting excess energy in the form of a photon:
The Penning ionization process, in which a metastable atom or 
molecule A* collides with another atom or molecule B, to leave A 
unexcited and B+ as an ion, 
is one member of a class of irreversible energy conversion processes 
in which irreversibility is due to the loss of an electron into its 
continuum. 
Penning ionization refers to the interaction between a gas-phase excited-state 
atom or molecule G* and a target molecule M resulting in the formation 
of a radical molecular cation M+●, an electron e−, and a neutral gas 
molecule G 
Penning ionization occurs when the target molecule has an ionization 
potential lower than the internal energy of the excited-state atom
Two laws are used to describe equilibrium in a plasma: 
the Boltzmann law to describe the equilibrium between the population of the 
various levels within the same ionization state, including both excited and 
ground states, and 
the Saha law to describe the equilibrium between the population of two 
successive ionization states. 
If we consider the population nm and nk of the excited level Em 
and Ek, respectively, their ratio can be given by the 
Boltzmann law:
The Saha Equation 
In 1920, Meghnad Saha derived an equation for the relative number of 
atoms in each ionization state. Here, just present the result: 
Note: 
3/2 
i 
This Edepends on the number density of electrons, n. This is 
ebecause as the number of free electrons increases, it is more 
likely that they can recombine with an atom and lower the 
ionization state. 
The Boltzmann factor exp(-/kT) means it is more difficult 
to ionize atoms with high ionization potentials
 For a gas at a high enough temperature, the thermal collisions of the 
atoms will ionize some of the atoms. One or more of the electrons that 
are normally bound to the atom in orbits around the atomic nucleus will be 
ejected from the atom and will form an electron gas that co-exists with 
the gas of atomic ions and neutral atoms. This state of matter is called a 
plasma. 
 The Saha equation describes the degree of ionization of this plasma as 
a function of the temperature, density, and ionization energies of the 
atoms. 
 The Saha equation only holds for weakly ionized plasmas for which 
the Debye length is large. This means that the “screening” of the 
coulomb charge of ions and electrons by other ions and electrons is 
negligible. The subsequent lowering of the ionization potentials and the 
“cutoff” of the partition function is therefore also negligible.
In general, the ICP is not in true thermodynamic equilibrium 
because the various processes that are occurring in the plasma are 
individually not in equilibrium. Therefore, the ICP cannot be 
characterized by a single equilibrium temperature. The Saha equation 
can be used to make a reasonable estimate of the degree of ionization: 
3/2 
where ni, na, and ne are the number densities of ions, atoms, and free 
electrons, respectively; m is the electron mass; Za and Zi are partition 
functions; Ei is the ionization potential; and T is the temperature. 
Using this equation, Houk (1986) calculated the degree of ionization of 
elements for a plasma temperature of 7500 K and an electron density of 
10l5 cm-3.
PLASMA FORMATION : 
Inductively coupled plasmas are formed by coupling energy 
produced by a RF generator to the plasma support gas with an 
electromagnetic field. The field is produced by applying an RF power 
(typically 700-1500 W) to an antenna (load coil) constructed from 3- 
mm-diameter copper tubing wrapped in a two- or three-turn 3-cm-diameter 
coil, positioned around the quartz torch assembly designed 
to configure and confine the plasma. 
An alternating current field is created that oscillates at the 
frequency of the tuned RF generator. 
The plasma is initiated by the addition of a few "seed” electrons, 
generated from the spark of a Tesla coil or a piezoelectric starter, to 
the flowing support gas in the vicinity of the load coil. 
After the plasma is initiated it is sustained by a process known as 
inductive coupling.
As these seed electrons are accelerated by the electromagnetic RF field, 
collisions with neutral gas atoms create the ionized medium of the 
plasma. The mean free path of accelerated electrons in atmospheric 
pressure argon gas is about1 μm before a collision occurs with an argon 
atom. These collisions produce additional electrons. This cascading 
effect creates and sustains the plasma. 
Once the gas is ionized, it is self-sustaining as long as RF power is 
applied to the load coil. The ICP has the appearance of an intensely 
bright fireball-shaped discharge.
Inductively Coupled Plasma Spectroscopy
A photograph of the ICP torch
SScchheemmaattiicc vviieeww ooff aann IICCPP.. 
Induction 
coil 
Magnetic 
field 
Manning T.J. and Grow W.P., 1997
Plasma Generation 
 The ICP is generated by coupling the energy from a radio frequency 
generator into a suitable gas via a magnetic field which is induced through 
a two- or three-turn, water -cooled copper coil. 
 The radiofrequency energy is normally supplied at a frequency of 27.12 
MHz, delivering forward power at between 500 and 2000 W. 
 Two gas flows, usually argon, flow in a tangential manner through the 
outer tubes of a concentric, three-tube quartz torch which is placed axially 
in the copper coil. 
 Because the outer and intermediate gases flow tangentially (i.e. they 
swirl around as they pass through the torch), the plasma is continually 
revolving and has a 'weak spot' at the centre of its base, through which the 
inner gas flow, containing the sample, can be introduced.
 When the gas is seeded with electrons, usually by means of a spark, the 
electrons accelerate in the magnetic field and reach energies 
sufficient to ionize gaseous atoms in the field. 
 Subsequent collisions with other gaseous atoms causes further 
ionization and so on, so that the plasma becomes self-sustaining. This 
occurs almost instantaneously. 
 The magnetic field causes the ions and electrons to flow in the 
horizontal plane of the coil, thereby heating the neutral argon by 
collisional energy exchange, and a hot fireball is produced. 
 The hottest part of the ICP has a temperature between 8000 and 10000 
K, which is the temperature of the surface of the Sun, though the 
analytically useful region is in the tail-flame with a temperature between 
5000 and 6000 K.
ICP-AES: Plasma 
Inductively Coupled Plasma Source
Advantages of an ICP source 
1. The analytes are confined to a narrow region. 
2. The plasma provides simultaneous excitation of many elements. 
3. The analyst is not limited to analytical lines involving ground state 
transitions but can select from first or even second ionization state lines. 
For the elements Ba, Be, Mg, Sr, Ti, and V, the ion lines provide the best 
detection limits. 
4. The high temperature of the plasma ensures the complete breakdown of 
chemical compounds (even refractory compounds) and impedes the formation 
of other interfering compounds, thus virtually eliminating matrix effects. 
5. The ICP torch provides a chemically inert atmosphere and an optically thin 
emission source. 
6. Excitation and emission zones are spatially separated : this results in a low 
background. 
7. Low background, combined with a high S/N ratio of analyte emission, 
results in low detection limits, typically in the parts-per-billion range.
list of some of the most beneficial characteristics of the ICP source.
Additional information
Inductively Coupled Plasma Source 
A plasma is a hot, partially ionized 
gas. It contains relatively high 
concentrations of ions and electrons. 
Argon ions, once formed in a plasma, are 
capable of absorbing sufficient power from 
an external source to maintain the 
temperature at a level at which further 
ionization sustains the plasma indefinitely. 
The plasma temperature is about 10 000 K. 
After Manning T.J. and Grow W.P., 1997 
ICP-AES: Plasma
The main ionization processes are: 
the charge-transfer ionization, 
the electron-impact ionization 
the Penning ionization, 
while the main excitation processes for the analyte atom are: 
the electron impact excitation, 
And the 
ion–electron radiative recombination,
Ar 1s22s22p63s23px 
23py 
23pz 
2 [Ne]3s23px 
23py 
23pz 
2 
Ionization states 
Consider an atom in an ionization state r, for example a carbon ion 
with only 3 electrons (C IV) when normally it would have six in its 
neutral state. In its ground state, 2 electrons would occupy its n = 1 
state and 1 would occupy its n = 2 state. 
This atom can be raised to the next higher ionization state (C V) 
with the ejection of the latter electron if a collision or photon 
provides the appropriate energy, the ionization potential, 
Such a transition is indicated as Transition 1 in Fig. 2. It takes the 
atom from the ground state of the r ionization state to the ground 
state of the r+1 ionization state. The ejected electron will take on any 
excess energy p the exciting photon may have had beyond r. The 
photon energy would be
In Transition 2 the energy of the 
exciting photon would be 
if the final momentum of 
the ejected electron is 
p2/2m. 
In Transition 1 the photon 
energy would be 
Energy states of an atom in two ionizations states. The r+1 state has one less 
bound electron less than the r state. In the r+1 state, that electron is free.
More generally, the transition can initiate in any energy state of 
the original ion and terminate in any energy state of the final 
ion as illustrated by Transition 2 of Fig. 2. The 
energy of the exciting photon would be 
if the final momentum of the ejected electron is p2/2m.
d5 means 
d8 means 
Mn 1s22s22p63s23p63d54s2 
Fe 1s22s22p63s23p63d64s2 
Co 1s22s22p63s23p63d74s2 
Ni 1s22s22p63s23p63d84s2 
Cu 1s22s22p63s23p63d104s1 
Zn 1s22s22p63s23p63d104s2 
A transition element is defined as one which has partially filled d orbitals 
either in the element or any of its compounds. Zinc (at the right-hand end 
of the d-block) always has a completely full 3d level (3d10) and so doesn't 
count as a transition element.
3 power sources have been employed in argon plasma spectroscopy. 
(i)dc electrical source capable of maintaining a current of several 
amperes between electrodes immersed in a stream of argon. The 
second and third utilize powerful 
(ii)radio-frequency and 
(iii)microwave-frequency fields through which the argon flows. 
Of the three, the radio-frequency, or inductively coupled plasma 
(ICP), source appears to offer the greatest advantage in terms of 
sensitivity and freedom from interference. 
On the other hand, the dc plasma source (DCP) has the virtue of 
simplicity and lower cost. 
The microwave induced plasma source (MIP) is not widely used 
for analysis
• If we confine ourselves to a discussion of an argon ICP then we can say 
that it consists mainly of the following species:
ICPES , analytical, P KMani, BCKV

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ICPES , analytical, P KMani, BCKV

  • 1. Dr. P. K. Mani BCKV
  • 2. E – energy difference between two levels; h – Plank’s constant, 6.626068 × 10-34 m2kg/s; c – speed of light, 299 792 458 m/s; λ – wavelenght, nm Ion Emission Atom Emission
  • 3. Atomic Emission Spectrometry (AES) In this method, a sample is normally excited by the thermal energy of a flame, argon plasma or an electrical discharge. The atoms in the sample absorb thermal energy, causing the excitation of the outer orbital electrons. As the excited state is short lived, the excited atoms return back to the ground state after a very short lifetime (typically10-6 to 10-9 s). This is accompanied by the emission of EMR, normally in the form of light in the UV-VIS region. The wavelength of the emitted radiation and its intensity provide the qualitative and quantitative information about the analyte. The atomic emission spectroscopy employing flame as a means of excitation is called ffllaammee pphhoottoommeettrryy oorr ffllaammee eemmiissssiioonn ssppeeccttrroossccooppyy ((FFEESS))..
  • 4. PRINCIPLE OF FLAME PHOTOMETRY For a few elements, such as the alkali metals Na and K, an air/ acetylene flame is hot enough not only to produce ground state atoms, but to raise some of the atoms to an excited electronic state. The radiant energy emitted when the atoms return to the ground state is proportional to the concentration and is the basis of flame emission spectroscopy. i.e., at 589 nm, Na -------> Na* (energy from flame) Na* -------> Na + hn (at 589 nm)
  • 5. Within the flame, there are many more atoms in the ground state than in the excited state. For Zn, for instance, in a 2000K flame, there are 7.3 X 1015 atoms in the ground state for every excited atom. The alkali metals are elements with unocuppied atomic orbitals of low enough energy to be sufficiently populated by a flame. For the element sodium, two inner shells are completely filled and there is one electron in the outer third shell. This electron is said to be in an s orbital. However, the remaining orbitals of the third shell and all the orbitals of the fourth, fifth and sixth shells, etc., are empty. When the outer electron of sodium is in the s orbital the atom is said to be in the “ground state” or the “unexcited state”. If the atom absorbs radiation the electron undergoes a transition to one of the empty orbitals at the higher energy levels.
  • 6.
  • 7. Inductively coupled plasmas By definition, a plasma is an electrical conducting gaseous mixture containing a significant concentration of cations and electrons. (The concentrations of the two are such that the net charge approaches zero.) In the argon plasma employed for emission analyses, argon ions and electrons are the principal conducting species, although cations from the sample will also be present in lesser amounts. Argon ions, once formed in a plasma, are capable of absorbing sufficient power from an external source to maintain the temperature at a level at which further ionization sustains the plasma indefinitely; temperatures as great as 10,000 K are encountered. A plasma is an ionized gas that is macroscopically neutral (i.e. with the same number of positive particles (ions) and negative particles (electrons)). If a monoatomic gas, X, is used, a plasma can be described by the following equilibrium: Ar : 1s22s22p63s23p23p23p2 x y z [Ne]3s23px 23py 23pz 2
  • 8. The gas that is used to generate the plasma (plasma gas) is Argon. Like any noble gas, Argon is a mono atomic element with a high ionization energy (15.76 eV), and is chemically inert. Consequently: (i)a simple spectrum is emitted by argon in contrast to a flame where primarily molecular spectra are observed; (ii) argon has the capability to excite and ionize most of the elements of the Periodic Table; (iii) no stable compounds are formed between argon and the analytes.
  • 9. The plasma acts as reservoir of energy provided by the radio frequency field, and transfers this energy to an analyte, M. the atomization of a sample is a relatively long process (of the order of a few ms), while ionization and excitation are very fast processes. Various ionization and excitation processes have been suggested resulting from the presence of species that are obtained during the plasma generation. The major species are not only the argon ions, Ar, and the electrons, e, but also the excited argon atoms, Ar*,with the special case of the metastable levels, Arm
  • 10. The hf field is produced by a rf generator and accelerates the electrons. These electrons will ionize the plasma gas: the kinetic energy of the projectile electron must be greater than the ionization potential of the bound electron to be ionized Then, through the process of radiative recombination, the argon ions are recombined with electrons to lead to excited argon atoms and to a significant background: This background is mainly produced by the process of radiative recombination in the ultraviolet (UV) region, while bremsstrahlung must also be taken into consideration in the visible part of the spectrum . Except for the resonance lines that are located at 106.7 nm and 104.8 nm, there are no argon atomic lines below 300 nm.
  • 11. In addition to ionization and excitation, beta particles may also transfer energy by a process called Bremsstrahlung. As negative beta particles approach the positively charged nucleus of an atom, some are slowed down and pulled into a new direction (like the gravitational pull of the earth on a satellite). As the electrons are slowed down some energy is released in the form of X-rays called Bremsstrahlung. These X-rays are more penetrating than the beta particles and may require more shielding. Plastic is commonly used to shield beta particles because low density materials result in less production of Bremsstrahlung
  • 12. Electron ionization (EI, formerly known as electron impact) is an ionization method in which energetic electrons interact with gas phase atoms or molecules to produce ions. where M is the analyte molecule being ionized, e− is the electron and M+• is the resulting ion. Radiative recombination (RR) is a non-resonant, one step recombination process in which a free electron recombines with an ion, emitting excess energy in the form of a photon:
  • 13. The Penning ionization process, in which a metastable atom or molecule A* collides with another atom or molecule B, to leave A unexcited and B+ as an ion, is one member of a class of irreversible energy conversion processes in which irreversibility is due to the loss of an electron into its continuum. Penning ionization refers to the interaction between a gas-phase excited-state atom or molecule G* and a target molecule M resulting in the formation of a radical molecular cation M+●, an electron e−, and a neutral gas molecule G Penning ionization occurs when the target molecule has an ionization potential lower than the internal energy of the excited-state atom
  • 14. Two laws are used to describe equilibrium in a plasma: the Boltzmann law to describe the equilibrium between the population of the various levels within the same ionization state, including both excited and ground states, and the Saha law to describe the equilibrium between the population of two successive ionization states. If we consider the population nm and nk of the excited level Em and Ek, respectively, their ratio can be given by the Boltzmann law:
  • 15. The Saha Equation In 1920, Meghnad Saha derived an equation for the relative number of atoms in each ionization state. Here, just present the result: Note: 3/2 i This Edepends on the number density of electrons, n. This is ebecause as the number of free electrons increases, it is more likely that they can recombine with an atom and lower the ionization state. The Boltzmann factor exp(-/kT) means it is more difficult to ionize atoms with high ionization potentials
  • 16.  For a gas at a high enough temperature, the thermal collisions of the atoms will ionize some of the atoms. One or more of the electrons that are normally bound to the atom in orbits around the atomic nucleus will be ejected from the atom and will form an electron gas that co-exists with the gas of atomic ions and neutral atoms. This state of matter is called a plasma.  The Saha equation describes the degree of ionization of this plasma as a function of the temperature, density, and ionization energies of the atoms.  The Saha equation only holds for weakly ionized plasmas for which the Debye length is large. This means that the “screening” of the coulomb charge of ions and electrons by other ions and electrons is negligible. The subsequent lowering of the ionization potentials and the “cutoff” of the partition function is therefore also negligible.
  • 17. In general, the ICP is not in true thermodynamic equilibrium because the various processes that are occurring in the plasma are individually not in equilibrium. Therefore, the ICP cannot be characterized by a single equilibrium temperature. The Saha equation can be used to make a reasonable estimate of the degree of ionization: 3/2 where ni, na, and ne are the number densities of ions, atoms, and free electrons, respectively; m is the electron mass; Za and Zi are partition functions; Ei is the ionization potential; and T is the temperature. Using this equation, Houk (1986) calculated the degree of ionization of elements for a plasma temperature of 7500 K and an electron density of 10l5 cm-3.
  • 18. PLASMA FORMATION : Inductively coupled plasmas are formed by coupling energy produced by a RF generator to the plasma support gas with an electromagnetic field. The field is produced by applying an RF power (typically 700-1500 W) to an antenna (load coil) constructed from 3- mm-diameter copper tubing wrapped in a two- or three-turn 3-cm-diameter coil, positioned around the quartz torch assembly designed to configure and confine the plasma. An alternating current field is created that oscillates at the frequency of the tuned RF generator. The plasma is initiated by the addition of a few "seed” electrons, generated from the spark of a Tesla coil or a piezoelectric starter, to the flowing support gas in the vicinity of the load coil. After the plasma is initiated it is sustained by a process known as inductive coupling.
  • 19. As these seed electrons are accelerated by the electromagnetic RF field, collisions with neutral gas atoms create the ionized medium of the plasma. The mean free path of accelerated electrons in atmospheric pressure argon gas is about1 μm before a collision occurs with an argon atom. These collisions produce additional electrons. This cascading effect creates and sustains the plasma. Once the gas is ionized, it is self-sustaining as long as RF power is applied to the load coil. The ICP has the appearance of an intensely bright fireball-shaped discharge.
  • 21. A photograph of the ICP torch
  • 22. SScchheemmaattiicc vviieeww ooff aann IICCPP.. Induction coil Magnetic field Manning T.J. and Grow W.P., 1997
  • 23. Plasma Generation  The ICP is generated by coupling the energy from a radio frequency generator into a suitable gas via a magnetic field which is induced through a two- or three-turn, water -cooled copper coil.  The radiofrequency energy is normally supplied at a frequency of 27.12 MHz, delivering forward power at between 500 and 2000 W.  Two gas flows, usually argon, flow in a tangential manner through the outer tubes of a concentric, three-tube quartz torch which is placed axially in the copper coil.  Because the outer and intermediate gases flow tangentially (i.e. they swirl around as they pass through the torch), the plasma is continually revolving and has a 'weak spot' at the centre of its base, through which the inner gas flow, containing the sample, can be introduced.
  • 24.  When the gas is seeded with electrons, usually by means of a spark, the electrons accelerate in the magnetic field and reach energies sufficient to ionize gaseous atoms in the field.  Subsequent collisions with other gaseous atoms causes further ionization and so on, so that the plasma becomes self-sustaining. This occurs almost instantaneously.  The magnetic field causes the ions and electrons to flow in the horizontal plane of the coil, thereby heating the neutral argon by collisional energy exchange, and a hot fireball is produced.  The hottest part of the ICP has a temperature between 8000 and 10000 K, which is the temperature of the surface of the Sun, though the analytically useful region is in the tail-flame with a temperature between 5000 and 6000 K.
  • 25. ICP-AES: Plasma Inductively Coupled Plasma Source
  • 26. Advantages of an ICP source 1. The analytes are confined to a narrow region. 2. The plasma provides simultaneous excitation of many elements. 3. The analyst is not limited to analytical lines involving ground state transitions but can select from first or even second ionization state lines. For the elements Ba, Be, Mg, Sr, Ti, and V, the ion lines provide the best detection limits. 4. The high temperature of the plasma ensures the complete breakdown of chemical compounds (even refractory compounds) and impedes the formation of other interfering compounds, thus virtually eliminating matrix effects. 5. The ICP torch provides a chemically inert atmosphere and an optically thin emission source. 6. Excitation and emission zones are spatially separated : this results in a low background. 7. Low background, combined with a high S/N ratio of analyte emission, results in low detection limits, typically in the parts-per-billion range.
  • 27. list of some of the most beneficial characteristics of the ICP source.
  • 29. Inductively Coupled Plasma Source A plasma is a hot, partially ionized gas. It contains relatively high concentrations of ions and electrons. Argon ions, once formed in a plasma, are capable of absorbing sufficient power from an external source to maintain the temperature at a level at which further ionization sustains the plasma indefinitely. The plasma temperature is about 10 000 K. After Manning T.J. and Grow W.P., 1997 ICP-AES: Plasma
  • 30. The main ionization processes are: the charge-transfer ionization, the electron-impact ionization the Penning ionization, while the main excitation processes for the analyte atom are: the electron impact excitation, And the ion–electron radiative recombination,
  • 31. Ar 1s22s22p63s23px 23py 23pz 2 [Ne]3s23px 23py 23pz 2 Ionization states Consider an atom in an ionization state r, for example a carbon ion with only 3 electrons (C IV) when normally it would have six in its neutral state. In its ground state, 2 electrons would occupy its n = 1 state and 1 would occupy its n = 2 state. This atom can be raised to the next higher ionization state (C V) with the ejection of the latter electron if a collision or photon provides the appropriate energy, the ionization potential, Such a transition is indicated as Transition 1 in Fig. 2. It takes the atom from the ground state of the r ionization state to the ground state of the r+1 ionization state. The ejected electron will take on any excess energy p the exciting photon may have had beyond r. The photon energy would be
  • 32. In Transition 2 the energy of the exciting photon would be if the final momentum of the ejected electron is p2/2m. In Transition 1 the photon energy would be Energy states of an atom in two ionizations states. The r+1 state has one less bound electron less than the r state. In the r+1 state, that electron is free.
  • 33. More generally, the transition can initiate in any energy state of the original ion and terminate in any energy state of the final ion as illustrated by Transition 2 of Fig. 2. The energy of the exciting photon would be if the final momentum of the ejected electron is p2/2m.
  • 34. d5 means d8 means Mn 1s22s22p63s23p63d54s2 Fe 1s22s22p63s23p63d64s2 Co 1s22s22p63s23p63d74s2 Ni 1s22s22p63s23p63d84s2 Cu 1s22s22p63s23p63d104s1 Zn 1s22s22p63s23p63d104s2 A transition element is defined as one which has partially filled d orbitals either in the element or any of its compounds. Zinc (at the right-hand end of the d-block) always has a completely full 3d level (3d10) and so doesn't count as a transition element.
  • 35. 3 power sources have been employed in argon plasma spectroscopy. (i)dc electrical source capable of maintaining a current of several amperes between electrodes immersed in a stream of argon. The second and third utilize powerful (ii)radio-frequency and (iii)microwave-frequency fields through which the argon flows. Of the three, the radio-frequency, or inductively coupled plasma (ICP), source appears to offer the greatest advantage in terms of sensitivity and freedom from interference. On the other hand, the dc plasma source (DCP) has the virtue of simplicity and lower cost. The microwave induced plasma source (MIP) is not widely used for analysis
  • 36. • If we confine ourselves to a discussion of an argon ICP then we can say that it consists mainly of the following species:

Editor's Notes

  1. In the absence of analyte atoms, water and sample matrix components, the predominant species will be Ar, Ar+ and e-, although the others are important when considering analyte ionization mechanisms. The RF energy used to sustain the plasma is only coupled into the outer region of the plasma, so these species are primarily formed in this region and are thermally transferred to the centre. This is known as the skin effect. The depth to which the RF energy will couple into the plasma gas is called the skin depth, and is determined by the frequency of the RF energy and the nature of the plasma gas. One desirable consequence of the skin effect is that the ICP is much more energetic in the outer region, which makes it optically thin. This means that emission from the centre will not be re-absorbed by unexcited atoms in the outer regions, such as occurs with flames. This lack of self-absorption means that ICP-AES has a large linear dynamic range.