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arXiv · 1911.13121

Analysis of the C$_2$ (d$^3\Pi_g$-a$^3\Pi_u$) Swan bands as a thermometric probe in CO$_2$ microwave plasmas

Emile Carbone·Federico D'Isa·Ante Hecimovic·Ursel Fantz
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Abstract

The optical emission spectra of high pressure CO$_2$ microwave plasmas are usually dominated by the C$_2$ Swan bands. In this paper, the use of the C$_2$ Swan bands for estimating the gas temperature in CO$_2$ microwave plasmas is assessed. State by state fitting is employed to check the correctness of assuming a Boltzmann distribution for the rotational and vibrational distribution functions and, within statistical and systematic uncertainties, the C$_2$ Swan band can be fitted accurately with a single temperature for rotational and vibrational levels. The processes leading to the production of the C$_2$ molecule and particularly its d$^3\Pi_g$ state are briefly reviewed as well as collisional relaxation times of the latter. It is concluded that its rotational temperature can be associated to the gas temperature of the CO$_2$ microwave plasma and the results are moreover cross-checked by adding a small amount of N$_2$ in the discharge and measuring the CN violet band system. The 2.45~GHz plasma source is analyzed in the pressure range 180-925~mbar, for input microwave powers ranging from 0.9 - 3 kW and with gas flow rates of 5-100~L/min. An intense C$_2$ Swan bands emission spectrum can be measured only when the plasma is operated in contracted regime. A unique temperature of about 6000 $\pm$ 500 K is obtained for all investigated conditions. A spectroscopic database is constructed using the recent compilation and calculations by Brooke et al. \cite{BROOKE201311} of the line strengths and molecular constants for the C$_2$ (d$^3\Pi_g$-a$^3\Pi_u$) Swan bands system and made available as Supplementary Material in a format compatible with the open source MassiveOES software.

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Emile Carbone, Federico D'Isa, Ante Hecimovic, Ursel Fantz. 2019-11-29. Analysis of the C$_2$ (d$^3\Pi_g$-a$^3\Pi_u$) Swan bands as a thermometric probe in CO$_2$ microwave plasmas. https://doi.org/10.1088/1361-6595%2Fab74b4

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