NON-EQUILIBRIUM MODELING OF THE FE XVII 3C/3D LINE RATIO IN AN INTENSE X-RAY FREE-ELECTRON LASER EXCITED PLASMA

被引：15

作者：

Loch, S. D. ^{[1
]}

Ballance, C. P. ^{[1
]}

Li, Y. ^{[1
]}

Fogle, M. ^{[1
]}

Fontes, C. J. ^{[2
]}

机构：

[1] Auburn Univ, Auburn, AL 36849 USA

[2] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2015年 / 801卷 / 01期

关键词：

atomic data; atomic processes; line: formation; plasmas; X-rays: general; ATOMIC DATA;

D O I：

10.1088/2041-8205/801/1/L13

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Recent measurements using an X-ray Free Electron Laser (XFEL) and an Electron Beam Ion Trap at the Linac Coherent Light Source facility highlighted large discrepancies between the observed and theoretical values for the Fe XVII 3C/3D line intensity ratio. This result raised the question of whether the theoretical oscillator strengths may be significantly in error, due to insufficiencies in the atomic structure calculations. We present time-dependent spectral modeling of this experiment and show that non-equilibrium effects can dramatically reduce the predicted 3C/3D line intensity ratio, compared with that obtained by simply taking the ratio of oscillator strengths. Once these non-equilibrium effects are accounted for, the measured line intensity ratio can be used to determine a revised value for the 3C/3D oscillator strength ratio, giving a range from 3.0 to 3.5. We also provide a framework to narrow this range further, if more precise information about the pulse parameters can be determined. We discuss the implications of the new results for the use of Fe XVII spectral features as astrophysical diagnostics and investigate the importance of time-dependent effects in interpreting XFEL-excited plasmas.

引用

页数：5

共 13 条

[1] ATOMIC DATA AND SPECTRAL-LINE INTENSITIES FOR NE-LIKE FE-XVII [J].