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JOURNALS // Optics and Spectroscopy // Archive

Optics and Spectroscopy, 2022 Volume 130, Issue 7, Pages 996–1003 (Mi os1783)

This article is cited in 1 paper

Spectroscopy and physics of atoms and molecules

Low pressure DBD in He–Ne mixture. Spectroscopy of the afterglow

V. A. Ivanov

Saint Petersburg State University, 198504 St. Petersburg, Russia

Abstract: The paper considers the possibility of using a low-pressure dielectric barrier discharge (DBD) as a plasma source for the active medium of a He-Ne laser. The results of a spectroscopic study of the decay stage of a DBD plasma of a cylindrical configuration with a pronounced inverse population of the upper level of the $2p^55s$ configuration, which makes the line of 632.8 nm one of the brightest in the visible region of the spectrum, are presented. It is shown that in the early stage of the DBD afterglow, the distribution of the populations over the $2p^55s$ and $2p^54d$ levels of the neon atom is due to the excitation transfer mechanism Νε$(2^1S_0)$ + Ne $\to$ He$(1^1S_0)$ + Ne$^*$. In the late afterglow with the departure of helium atoms Νε$(2^1S_0)$, emission in the visible region of the spectrum is formed mainly by transitions from levels of the $2p^53p$ configuration, the population of which is associated with Νε$(2^3S_1)$ atoms. At this stage, the population of the $2p^55s$ and $2p^54d$ states by electron-ion recombination processes is ineffective and does not lead to the formation of population inversion. As an optimal solution in terms of the 632.8 nm line brightness in the afterglow, it is proposed to use a discharge with electrodes along the outer surface of a cylindrical discharge tube, initiated at frequencies that exclude the recombination stage of the afterglow.

Keywords: elementary processes, barrier discharge, inverse population, afterglow, helium-neon plasma, excitation transfer.

Received: 24.12.2021
Revised: 13.02.2022
Accepted: 06.04.2022

DOI: 10.21883/OS.2022.07.52718.3076-21


 English version:
Optics and Spectroscopy, 2023, 131:7, 519–526

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© Steklov Math. Inst. of RAS, 2025