On the semiclassical perturbation Stark shifts of Ar II spectral lines

被引：1

作者：

Hamdi, R. ^{[1
,2
]}

Ben Nessib, N. ^{[3
]}

Sahal-Brechot, S. ^{[4
]}

Dimitrijevic, M. S. ^{[4
,5
]}

机构：

[1] Umm Al Qura Univ, Dept Phys, Deanship Joint First Year, Mecca, Saudi Arabia

[2] Univ Carthage, Grp Rech Phys Atom & Astrophys, Fac Sci Bizerte, Tunis, Tunisia

[3] King Saud Univ, Dept Phys & Astron, Coll Sci, POB 2455, Riyadh 11451, Saudi Arabia

[4] Univ PSL, Sorbonne Univ, Observ Paris, LERMA,CNRS, F-92190 Meudon, France

[5] Astron Observ, Volgina 7, Belgrade 11060, Serbia

来源：

CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO | 2020年 / 50卷 / 01期

关键词：

atomic data; atomic processes; line: formation; TRANSITION-PROBABILITIES; WIDTHS; ARGON; IONS; ELECTRONS;

D O I：

10.31577/caosp.2020.50.1.128

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present in this paper Stark shifts as a function of temperature for 20 spectral lines of Ar II belonging to 4p - 4d transition array. Calculations are made using semiclassical perturbation approach in impact approximation. Atomic data used in this calculation are carried out using Hartree-Fock method with relativistic corrections. Singly charged argon (Ar II) spectral lines are observed in many astrophysical plasmas. Ar II spectral lines are also important for laboratory plasmas and laser physics and technology.

引用

页码：128 / 138

页数：11

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