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
收藏
页码：128 / 138
页数：11
相关论文
共 50 条
  • [41] Stark broadening of neutral germanium spectral lines
    Dimitrijevic, MS
    Jovanovic, P
    Simic, Z
    ASTRONOMY & ASTROPHYSICS, 2003, 410 (02): : 735 - 739
  • [42] Stark Widths of Spectral Lines of Neutral Neon
    Dimitrijevic, Milan S.
    Simic, Zoran
    Kovacevic, Andjelka
    Valjarevic, Aleksandar
    Sahal-Brechot, Sylvie
    JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 2015, 36 (04) : 643 - 659
  • [43] Stark broadening of Pb IV spectral lines
    Hamdi, Rafik
    Ben Nessib, Nabil
    Dimitrijevic, Milan S.
    Sahal-Brechot, Sylvie
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 431 (02) : 1039 - 1047
  • [44] Stark broadening of Fe V spectral lines: 4s-4p transitions
    Hamdi, Rafik
    Ben Nessib, Nabil
    Sahal-Brechot, Sylvie
    Dimitrijevic, Milan S.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 504 (01) : 1320 - 1330
  • [45] Stark broadening of several Bi IV spectral lines of astrophysical interest
    Colon, C.
    Moreno-Diaz, C.
    de Andres-Garcia, I.
    Alonso-Medina, A.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 470 (02) : 2179 - 2189
  • [46] Stark broadening of Si II spectral lines: comparison with experimental results
    Dimitrijevi, M. S.
    Christova, M. D.
    Sahal-Brechot, S.
    CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO, 2022, 52 (03): : 25 - 34
  • [47] STARK SHIFTS OF SINGLY-IONIZED NITROGEN SPECTRAL-LINES
    DJENIZE, S
    SRECKOVIC, A
    LABAT, J
    ASTRONOMY & ASTROPHYSICS, 1992, 253 (02) : 632 - 634
  • [48] Experimental Stark widths and shifts of triply ionized sulfur spectral lines
    Djenize, S
    Sreckovic, A
    Jelisavcic, M
    Bukvic, S
    ASTRONOMY & ASTROPHYSICS, 2002, 389 (03) : 1086 - 1089
  • [49] Experimental Stark parameters of Cr II spectral lines
    Manrique, J.
    Aguilera, J. A.
    Aragon, C.
    XXII INTERNATIONAL CONFERENCE ON SPECTRAL LINE SHAPES (ICSLS 2014), 2014, 548
  • [50] Irregularities of Stark parameters of Xe II spectral lines
    Pelaez, R. J.
    Djurovic, S.
    Cirisan, M.
    Aparicio, J. A.
    Mar, S.
    JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 2009, 42 (12)
12345