Emission Lines of Fe xiv, Fe xv, and Fe xvi in the Extreme Ultraviolet Region 40–100 Å

Author:

Lepson J. K.ORCID,Beiersdorfer P.ORCID,Brown G. V.ORCID,Liedahl D. A.

Abstract

Abstract We report on emission spectra of iron in the extreme ultraviolet recorded at an electron density of ∼1011 cm−3 on the Lawrence Livermore electron beam ion trap facility. We present a summary of the observed emission lines, including wavelengths and emission intensities, and present spectra of pure Fe xiv through Fe xvi emission derived from our measurements in the 40–100 Å wavelength range. We show that spectral models, especially the current version of CHIANTI v10.0, describe the M-shell emission from these three charge states of iron reasonably well, and we are able to verify several transitions in CHIANTI for the first time.

Funder

NASA ∣ SMD ∣ Heliophysics Division

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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