实验室天体物理实验中对多充离子 X 射线 L 壳发射光谱的磁重联效应研究

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Reports Pub Date : 2024-07-27 DOI:10.1134/S1063772924700331
M. A. Alkhimova, S. S. Makarov, I. Yu. Skobelev, S. N. Ryazantsev, E. D. Filippov
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摘要

摘要 在本文中,我们展示了在实验室天体物理实验中应用具有高空间分辨率的 X 射线光谱来研究磁重联的情况,这些实验是利用纳秒和皮秒持续时间的激光设备,以中等激光密度(<1018 W/cm2)在目标上进行的。本文简要介绍了常用的实验方案。对 Ne 离子和类 F 铁离子(铁,Z = 26)的 L 壳光谱进行的原子动力学计算表明,测量对等离子体参数的变化具有很高的灵敏度。讨论了测量电子温度和激光等离子体密度的不同诊断方法的范围。结果表明,类 Ne 离子的跃迁是测量等离子体参数的通用工具,无论是在激光与目标相互作用的区域还是在重联区域都是如此。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Study of the Magnetic Reconnection Effect in a Laboratory Astrophysical Experiment on X-Ray L-Shell Emission Spectra of Multicharged Ions

In the paper, we demonstrate the application of X-ray spectroscopy with high spatial resolution to study magnetic reconnection in laboratory astrophysical experiments performed with nano- and pico-second duration laser facilities at a moderate laser density on the target of <1018 W/cm2. A brief overview of the commonly used experimental schemes is given. Atomic kinetic calculations for the L-shell spectra of Ne- and F‑like Fe ions (iron, Z = 26) demonstrate the high sensitivity of the measurements to changes in plasma parameters. The scope of the different diagnostic approaches to measure electron temperature and laser plasma density is discussed. It is shown that transitions in Ne-like ions are a universal tool for measuring plasma parameters, both in the region of laser interaction with the target and in the reconnection zone.

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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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