Evaluation of self-absorption effect of He I resonance line by measurement of forbidden emission in helium arc jet plasma

Author:

Shigesada Ryo1,Islam Md. Anwarul1ORCID,Kawazome Hayato2ORCID,Okuda Kosuke1ORCID,Sunada Yuta1,Yanagi Ohshi1ORCID,Sumino Masato1ORCID,Hatta Kazuho1,Tamura Naoki34ORCID,Yamasaki Kotaro1ORCID,Kawata Jun2ORCID,Namba Shinichi1ORCID

Affiliation:

1. Graduate School of Advanced Science and Engineering, Hiroshima University, Higashihiroshima, Hiroshima 739-8527, Japan

2. Department of Information Engineering, National Institute of Technology (KOSEN), Kagawa College, Mitoyo, Kagawa 769-1192, Japan

3. National Institute for Fusion Science, Toki, Gifu 509-5292, Japan

4. The Graduate University for Advanced Studies (SOKENDAI), Toki, Gifu 509-5292, Japan

Abstract

We have proposed a new method to estimate the optical escape factor (OEF) in high-density helium (He) plasma. Plasma with an electron temperature of ca. 3 eV and density of 5 × 1013 cm−3 was generated by a cascaded arc discharge and rapidly cooled by the introduction of additional He gas, which resulted in a transition from ionizing to recombining plasma. With an increase in the gas pressure, the plasma became optically thick, and the He I forbidden line (spin-exchange intercombination line, 1 1S-2 3P: 59.1 nm) with resonance lines were simultaneously observed using a vacuum ultraviolet spectrometer. Comparison of the intensity ratio of the He I 58.4 nm resonance line to the forbidden emission with those by determined from the collisional-radiative model considering the self-absorption enabled the successful estimation of the OEF. The OEF was decreased with the ambient He gas pressure and was 6.6 × 10−4 and 3.5 × 10−5 for He gas pressures of 1.59 and 20.22 Pa, respectively.

Funder

KAKENHI

Murata Science Foundation

National Institute of Fisheries Science

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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