https://doi.org/10.1140/epjd/s10053-024-00891-x
Regular Article
High-resolution laboratory measurements of M-shell Fe EUV line emission using EBIT-I
1
Columbia Astrophysics Laboratory, Columbia University, 10027, New York, NY, USA
2
Lawrence Livermore National Laboratory, 94550, Livermore, CA, USA
3
Space Science Laboratory, University of California, Berkeley, 94720, Berkeley, CA, USA
Received:
14
February
2024
Accepted:
21
June
2024
Published online:
29
July
2024
Solar physicists routinely utilize observations of Ar-like Fe IX and Cl-like Fe X emission to study a variety of solar structures. However, unidentified lines exist in the Fe IX and Fe X spectra, greatly impeding the spectroscopic diagnostic potential of these ions. Here, we present measurements using the Lawrence Livermore National Laboratory EBIT-I electron beam ion trap in the wavelength range 238–258 Å. These studies enable us to unambiguously identify the charge state associated with each of the observed lines. This wavelength range is of particular interest because it contains the Fe IX density diagnostic line ratio 241.74 Å/244.91 Å, which is predicted to be one of the best density diagnostics of the solar corona, as well as the Fe X 257.26 Å magnetic-field-induced transition. We compare our measurements to the Fe IX and Fe X lines tabulated in CHIANTI v10.0.1, which is used for modeling the solar spectrum. In addition, we have measured previously unidentified Fe X lines that will need to be added to CHIANTI and other spectroscopic databases.
© The Author(s) 2024
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