Laboratory Calibrations of Fe xii–xiv Line-Intensity Ratios for Electron Density Diagnostics
Abstract
In this work, we have used an electron beam ion trap to measure electron-density-diagnostic line-intensity ratios for extreme ultraviolet lines from Fe xii, xiii, and xiv at wavelengths of ≈185–205 and 255–276 Å. These ratios can be used as density diagnostics for astrophysical spectra and are especially relevant to solar physics. We found that density diagnostics using the Fe xiii 196.53/202.04 and the Fe xiv 264.79/274.21 and 270.52A/274.21 line ratios are reliable using the atomic data calculated with the Flexible Atomic Code (FAC). On the other hand, we found a large discrepancy between the FAC theory and experiment for the commonly used Fe xii (186.85 + 186.88)/195.12 line ratio. These FAC theory calculations give results similar to the data tabulated in CHIANTI, which are commonly used to analyze solar observations. Our results suggest that the discrepancies seen between solar coronal density measurements using the Fe xii (186.85 + 186.88)/195.12 and Fe xiii 196.54/202.04 line ratios are likely due to issues with the atomic calculations for Fe xii.
- Authors:
-
- Columbia Univ., New York, NY (United States). Columbia Astrophysics Lab.
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Univ. of California, Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 1823217
- Report Number(s):
- LLNL-JRNL-791539
Journal ID: ISSN 0004-637X; 990650; TRN: US2215608
- Grant/Contract Number:
- AC52-07NA27344; NNX16AF10G
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 890; Journal Issue: 1; Journal ID: ISSN 0004-637X
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 74 ATOMIC AND MOLECULAR PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; Atomic spectroscopy; Atomic physics; Spectroscopy; Laboratory astrophysics; Solar corona
Citation Formats
Arthanayaka, Thusitha, Beiersdorfer, Peter, Brown, Gregory V., Gu, Ming Feng, Hahn, Michael, Hell, Natalie, Lockard, Tom, and Savin, Daniel W. Laboratory Calibrations of Fe xii–xiv Line-Intensity Ratios for Electron Density Diagnostics. United States: N. p., 2020.
Web. doi:10.3847/1538-4357/ab67b4.
Arthanayaka, Thusitha, Beiersdorfer, Peter, Brown, Gregory V., Gu, Ming Feng, Hahn, Michael, Hell, Natalie, Lockard, Tom, & Savin, Daniel W. Laboratory Calibrations of Fe xii–xiv Line-Intensity Ratios for Electron Density Diagnostics. United States. https://doi.org/10.3847/1538-4357/ab67b4
Arthanayaka, Thusitha, Beiersdorfer, Peter, Brown, Gregory V., Gu, Ming Feng, Hahn, Michael, Hell, Natalie, Lockard, Tom, and Savin, Daniel W. Thu .
"Laboratory Calibrations of Fe xii–xiv Line-Intensity Ratios for Electron Density Diagnostics". United States. https://doi.org/10.3847/1538-4357/ab67b4. https://www.osti.gov/servlets/purl/1823217.
@article{osti_1823217,
title = {Laboratory Calibrations of Fe xii–xiv Line-Intensity Ratios for Electron Density Diagnostics},
author = {Arthanayaka, Thusitha and Beiersdorfer, Peter and Brown, Gregory V. and Gu, Ming Feng and Hahn, Michael and Hell, Natalie and Lockard, Tom and Savin, Daniel W.},
abstractNote = {In this work, we have used an electron beam ion trap to measure electron-density-diagnostic line-intensity ratios for extreme ultraviolet lines from Fe xii, xiii, and xiv at wavelengths of ≈185–205 and 255–276 Å. These ratios can be used as density diagnostics for astrophysical spectra and are especially relevant to solar physics. We found that density diagnostics using the Fe xiii 196.53/202.04 and the Fe xiv 264.79/274.21 and 270.52A/274.21 line ratios are reliable using the atomic data calculated with the Flexible Atomic Code (FAC). On the other hand, we found a large discrepancy between the FAC theory and experiment for the commonly used Fe xii (186.85 + 186.88)/195.12 line ratio. These FAC theory calculations give results similar to the data tabulated in CHIANTI, which are commonly used to analyze solar observations. Our results suggest that the discrepancies seen between solar coronal density measurements using the Fe xii (186.85 + 186.88)/195.12 and Fe xiii 196.54/202.04 line ratios are likely due to issues with the atomic calculations for Fe xii.},
doi = {10.3847/1538-4357/ab67b4},
journal = {The Astrophysical Journal},
number = 1,
volume = 890,
place = {United States},
year = {Thu Feb 13 00:00:00 EST 2020},
month = {Thu Feb 13 00:00:00 EST 2020}
}
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Laboratory Measurements of Fe xxiv Line Emission: \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $3arrow 2$ \end{document} Transitions near Excitation Threshold
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