Abstract
The results of a spectroscopic study of the conversion of acetylene and methane in a helium plasma jet produced by a direct current plasma torch are presented. The operating mode of the plasma torch corresponds to conditions that provide a high yield of carbon nanostructures. In the emission spectra recorded during the transverse observation of a 20-mm jet section following the outlet of the anode channel of the plasma torch, high-intensity Swan bands of the С2 molecule are the dominant component in the visible wavelength range. The spectra show atomic hydrogen lines of the HI Balmer series from Hα to Hε, numerous CI carbon lines from ultraviolet 247.9 nm to infrared 962–966 nm, and a number of HeI helium lines. The axial temperature values of the plasma jet were spectrally determined by the observed ionized carbon CII lines 283.7 nm, 392.0 and 426.7 nm. A joint analysis of the emission spectra and the mixture composition calculated in the Saha–Boltzmann approximation revealed the nature of the spatial heterogeneity of the studied He : C : H plasma jet. It is manifested by the difference in the electron temperature of the axial region of the jet, which is measured with ionized carbon lines CII (Te(0) = 12 000–14 000 K) from the vibrational and rotational temperatures of C2 molecules (TV = TR ≅ 5000 K) that emit intensely at the jet periphery. The electron density measured along the Hβ and Hγ line widths, which varies in the range of the observed jet region of ne = (4–2) × 1016 cm–3, corresponds to the ionization equilibrium in a plasma He : C : H mixture with an electron temperature close to Te measured by carbon-ion lines.
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Kramida A., Ralchenko Yu., Reader J. NIST ASD Team (2018). NIST Atomic Spectra Database (ver. 5.6.1). https://physics.nist.gov/asd [2019, June 12]. National Institute of Standards and Technology, Gaithersburg, MD. https://doi.org/10.18434/T4W30F
NIST Chemical Kinetics Database Standard Reference Database 17, Version 7.0 (Web Version), Release 1.6.8, Data Version 2017.07 (http://kinetics.nist.gov/kinetics).
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ACKNOWLEDGMENTS
We are grateful to our colleague M.A. Sargsyan for the participation in the experiment and discussion of results.
Funding
This study was supported by the Russian Foundation for Basic Research, project. nos. 18-08-00306 and 19-08-00081.
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Translated by L. Mosina
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Shavelkina, M.B., Amirov, R.K., Kavyrshin, D.I. et al. Spectroscopic Study of a Helium Plasma Jet with Hydrocarbon Additives. High Temp 58, 309–316 (2020). https://doi.org/10.1134/S0018151X20030165
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DOI: https://doi.org/10.1134/S0018151X20030165