On the Stark broadening of N VI spectral lines

被引：1
|
作者：
Christova, Magdalena D. [1 ]
Dimitrijevic, Milan S. [2 ,3 ]
Sahal-Brechot, Sylvie [3 ]
机构：
[1] Tech Univ Sofia, Dept Appl Phys, Sofia 1000, Bulgaria
[2] Astron Observ, Volgina 7, Belgrade 11060, Serbia
[3] Univ PSL, Sorbonne Univ, Observ Paris, CNRS,LERMA, F-92190 Meudon, France
来源：
CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO | 2023年 / 53卷 / 03期
关键词：
Stark broadening; spectral line shapes; atomic data; N VI; proton-boron fusion; IMPACT THEORY; ELECTRONS; IONS; COLLISIONS; SHIFTS;
D O I：
10.31577/caosp.2023.53.3.84
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Results for the Stark broadening parameters for spectral lines within one spectral series of N VI 2s-np (n = 2 - 4) triplet transitions are included. Plasma conditions of interest cover temperatures from 50 000 K to 2 000 000 K, perturber density is 10(17 )cm(-3), and electrons, and boron ions (B III, B IV, B V and B VI) are perturbers. These conditions correspond to those in laser driven plasma for proton boron fusion reaction. The contribution in Stark width and shift of different types of perturbers is analyzed. The width versus principal quantum number is presented.
引用
收藏
页码：84 / 93
页数：10
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