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Title of Thesis
Investigation of Plasma Parameteers in Ne-N2
Mixture Discharge with 13.56 MH2RF Generator |
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Author(s)
Najeeb-ur-Rehman |
Institute/University/Department
Details Department of Physics / Quaid-i-Azam University,
Islamabad |
Session 2009 |
Subject Physics |
Number of Pages 162 |
Keywords (Extracted from title, table of contents and
abstract of thesis) Positive, Second, Energy, Electrons,
Intensites, Generator, Temperature, Power, Parameteers,
Investigation, Pressure, Emission, Plasma, Sequences, Measured |
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Abstract Non-LTE Ne-N2 (Local
thermal equilibrium) mixture plasma is characterized to evaluate the
electron temperature (Te) and Excitation temperature (Texc). The
investigated plasma is of density range (109 to 1010 cm-3), thus it
belongs to corona balance. Optical emission spectroscopy (OES) is
used to calculate the electron temperature and excitation
temperature. Ne-I lines are employed to calculate the electron
temperature and excitation temperature. The effective principal
quantum numbers ‘ k p ’ of the selected Ne-I lines, are less than 7
for the above mentioned density range, which confirm that the corona
balance is the most probable balance. Modified Boltzmann plot is
employed to estimate the electron temperature, whereas simple
Boltzmann plot is used to calculate the excitation temperature.
Langmuir probe has also been used to measure the plasma parameters
e.g., electron temperature (Te), electron number density (ne),
plasma potential (Vp) and electron energy distribution function (EEDF).
Electron temperature (Te) measured from Ne-I lines, by employing
modified Boltzmann plot technique, is also compared with Langmuir
probe results. In both techniques the trend is same i.e., electron
temperature increases with increase in Ne % and RF power in the
mixture and it decreases with increase in filling pressure. It is
also observed that electron temperature (Te) measured with Langmuir
probe is slightly greater than electron temperature (Te) measured
with modified Boltzmann plot method. Generally, excitation
temperature (Texc) is greater than electron temperature (Te).This
fact is also observed in the characterization of the Ne-N2 mixture
plasma.
EEDFs in Ne-N2 mixture plasma are measured as a function of Ne %,
filling pressure and RF power. It is observed that the tails of the
EEDF gain height and extend towards the higher energy with increase
in Ne %, which confirms that population of high energy electrons
increases with increase in Ne % in the mixture. Electron number
density (ne) is also calculated and results show that ‘ne’ decreases
with Ne %. Optical emission spectroscopy (OES) is used to
investigate the effect of neon mixing on the vibrational temperature
of second positive ( 3 ,ν ′→ 3 ,ν ′′) 2 u g N C Π B Π and first
negative ( Σ+ ν ′→ Σ+ ν ′′) + 2 , 2 , 2 u g N B X system of nitrogen
plasma generated by 13.56 MHz RF generator. The relative changes in
vibrational population of ( 3 ) 2 u N C Π and Σ+ + N (B 2 u ) 2
states with neon mixing are monitored by measuring the emission
intensities of second positive and first negative system of nitrogen
molecules. Vibrational temperature is calculated for the sequences
Δν = 0, -1 and -2, that follows the Boltzmann distribution. It is
found that electron temperature as well as vibrational temperature
of second positive and first negative system can be raised
significantly by mixing of neon in the nitrogen plasma.Vibrational
temperature of second positive system is raised up to 0.67 eV at 90
% neo whereas for first negative system it is raised up to 0.78 eV
at 0.5 mbar pressure and 250 watt RF power. It is also found that
vibrational temperature increases with the gas pressure up to 0.5
mbar.The over population of the levels of ( 3 , ) N2 C Πu ν ′ states
with neon mixing are monitored by measuring the emission intensities
of second positive system of nitrogen molecules. Since, over
populations of levels of ( 3 , ) N2 C Πu ν ′ e.g., 1 and 4, effect
the calculus of vibrational temperature of ( 3 , ) N2 C Πu ν ′
state, therefore, a linearization process is employed to such
distributions allowing us to calculate the vibrational temperature
of the ( 3 , ) N2 C Πu ν ′ state. Vibration temperature ( ν T )
measured from different linear adjust gives different value of ‘ ν T
’, which in turns reflects the effect of over population of levels
of ( 3 , ) N2 C Πu ν ′ state. |
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