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Numerical Study on Radiation Trapping of He I Resonance Lines in Arc Plasma Under High-Gas Pressures

In high-gas pressure helium arc plasmas, a forbidden line (1s 1S-2p 3P : 59.1 nm) as well as the resonance lines 1s 1S-np 1P lines of He I have been observed. The intensity ratio of the 1s 1S-2p 1P line of He I to forbidden line calculated from the Einstein A coefficients (NIST database) is ∼10−7, w...

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Bibliographic Details
Published in:Plasma and Fusion Research 2021/02/10, Vol.16, pp.2401012-2401012
Main Authors: KAWAZOME, Hayato, ISLAM, Md Anwarul, NAMBA, Shinichi
Format: Article
Language:English
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Summary:In high-gas pressure helium arc plasmas, a forbidden line (1s 1S-2p 3P : 59.1 nm) as well as the resonance lines 1s 1S-np 1P lines of He I have been observed. The intensity ratio of the 1s 1S-2p 1P line of He I to forbidden line calculated from the Einstein A coefficients (NIST database) is ∼10−7, whereas the value obtained experimentally was as small as ∼20. The reason for the discrepancy between the experiment and database can be interpreted from that the photoabsorption (self-absorption) of the resonance lines 1s 1S-np 1P lines can cause the drastic change in radiative processes in high-pressure plasmas. In order to validate our interpretation on this mismatch, we investigated the influence of self-absorption of the resonance lines 1s 1S-np 1P lines by numerical simulations. The simulation code calculated the photoabsorption process by He atom along a line-of-sight by using coupled rate equations incorporated with the radiation trapping effect. As a result, the simulation yielded the line intensity ratio of 25 because of the strong self-absorption.
ISSN:1880-6821
1880-6821
DOI:10.1585/pfr.16.2401012