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首页> 外文期刊>The Astrophysical journal >RECOMBINATION X-RAY LINE FORMATION OF IRON L-SHELL IONS IN LOW-TEMPERATURE PLASMAS
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RECOMBINATION X-RAY LINE FORMATION OF IRON L-SHELL IONS IN LOW-TEMPERATURE PLASMAS

机译:低温等离子体中铁L壳离子的重组X射线线形成

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摘要

In low-temperature plasmas, X-ray line emission is dominated by radiative cascades following recombination and photoexcitation, with a negligible contribution from collisional excitation. In this paper, we present theoretical line formation rate coefficients for all n → 2 (3 ≤ n ≤ 5) transitions of Fe XVII-XXIV in the temperature range between 1 and 500 eV. Both radiative recombination (RR) and ΔN = 0 dielectronic recombination (DR) are taken into account. In addition, the rate coefficients for radiative recombination continua onto n = 2 and 3 states of Fe XVII-XXIV are tabulated. The total RR rate coefficients of Fe XVIII-XXV and total ΔN = 0 DR rate coefficients of Fe XVIII-XXIV are presented as well, and compared with existing experimental measurements and theoretical calculations.
机译:在低温等离子体中,复合和光激发后,辐射级联控制着X射线线的发射,而碰撞激发的贡献可忽略不计。在本文中,我们介绍了Fe XVII-XXIV在1至500 eV之间的温度范围内的所有n→2(3≤n≤5)转变的理论线形成速率系数。辐射复合(RR)和ΔN= 0双电子复合(DR)都被考虑在内。此外,将Fe XVII-XXIV的n = 2和3个态的辐射复合连续体的速率系数制成表格。还给出了Fe XVIII-XXV的总RR率系数和Fe XVIII-XXIV的总ΔN= 0 DR率系数,并将其与现有的实验测量结果和理论计算进行了比较。

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  • 来源
    《The Astrophysical journal》 |2003年第1期|p.1249-1254|共6页
  • 作者

    M. F. Gu;

  • 作者单位

    Center for Space Research, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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