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

被引:0
作者
Alkhimova, M. A. [1 ]
Makarov, S. S. [1 ]
Skobelev, I. Yu. [1 ]
Ryazantsev, S. N. [1 ]
Filippov, E. D. [1 ]
机构
[1] Russian Acad Sci, Joint Inst High Temp, Moscow 125412, Russia
关键词
X-ray spectroscopy; high power laser matter interaction; magnetic reconnection; laboratory astrophysics; CURRENT SHEETS; LASER-PULSES; PLASMA; ACCELERATION; SPECTROMETER; SPECTROSCOPY; CONFINEMENT; DYNAMICS; DENSITY; FLARES;
D O I
10.1134/S1063772924700331
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 <10(18) W/cm(2). 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.
引用
收藏
页码:345 / 355
页数:11
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