Observation and Line Analysis of Tungsten, Molybdenum and Copper Spectra at 20-150Å Emitted from Experimental Advanced Superconducting Tokamak (EAST) Plasma
Complex spectra of tungsten (W) and molybdenum (Mo) unresolved transition arrays (W-UTA and Mo-UTA) are frequently observed with isolated W, Mo and copper (Cu) lines at 20-150Å wavelength range in EAST plasmas with limiter configuration. The high-Z impurity ions of W, Mo and Cu enter the plasma through an unavoidable plasma-wall interaction at inboard Mo first wall and outboard W/Cu limiter. The spectra were observed with a fast-time-response extreme ultraviolet (EUV) spectrometer and line identification was carefully performed referring our previous works. As a result, W-UTA at 46-64Å and Mo-UTA at 68-96Å are found to be composed of W27+-W45+ and Mo16+-Mo30+ ions, respectively. The Cu spectra from Cu10+-Cu13+ ions are also found in wavelength range of 135-150 Å. In the analysis radial profiles of the impurity spectra are taken into account in determining the charge state in addition to the time behavior.
Authors
- S. Morita (ORCID: https://orcid.org/0000-0003-4139-7721)
- Yunxin Cheng (ORCID: https://orcid.org/0000-0002-9195-2757)
- Ailan Hu
- D. M. Mitnik (ORCID: https://orcid.org/0000-0003-0193-0958)
- Wenmin Zhang (ORCID: https://orcid.org/0009-0000-9980-6765)
- Chao Zhou (ORCID: https://orcid.org/0000-0003-1185-9964)
- Jiale Chen (ORCID: https://orcid.org/0000-0003-1781-9744)
- Ling Zhang (ORCID: https://orcid.org/0000-0002-8778-8704)
- Haiqing Liu (ORCID: https://orcid.org/0000-0001-6892-358X)
Institutions
- University of Science and Technology of China (CN)
- Chinese Academy of Sciences (CN)
- National Institute for Fusion Science (JP)
- Institute of Astronomy and Space Physics (AR)
Publication Details
- Journal
- Plasma and Fusion Research
- Published
- 2025-01-22
- DOI
- https://doi.org/10.1585/pfr.20.2402011
- Primary Topic
- X-ray Spectroscopy and Fluorescence Analysis
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China
- Chinese Academy of Sciences