Stark broadening of Sn II spectral lines

IF 2.3 3区物理与天体物理 Q2 OPTICS

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2024-11-06 DOI:10.1016/j.jqsrt.2024.109241

Milan S. Dimitrijević , Magdalena D. Christova , Cristina Yubero , Sylvie Sahal-Bréchot

引用次数: 0

Abstract

Our objective is to provide reliable Stark broadening data for Sn II spectral lines needed for astrophysics, plasma physics, fusion research, and different plasmas in laboratory and technology. We used the semiclassical perturbation method for the calculation of Stark broadening parameters, full widths at half intensity maximum and shifts for 44 spectral lines of singly charged tin ion (Sn II), for collisions with electrons and protons. The obtained results have been compared with the existing experimental and theoretical results and used to demonstrate the influence of Stark broadening mechanism on spectral lines of Sn II in stellar atmospheres.

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锡 II 光谱线的斯塔克增宽

我们的目标是为天体物理学、等离子体物理学、核聚变研究以及实验室和技术中的不同等离子体提供可靠的锡离子（Sn II）光谱线的斯塔克展宽数据。我们采用半经典扰动法计算了单电荷锡离子（Sn II）与电子和质子碰撞时 44 条光谱线的斯塔克展宽参数、半强度最大值全宽和位移。所得结果与现有的实验和理论结果进行了比较，并用于证明斯塔克展宽机制对恒星大气中锡离子（Sn II）光谱线的影响。

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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来源期刊

Journal of Quantitative Spectroscopy & Radiative Transfer 物理-光谱学

CiteScore

5.30

自引率

21.70%

发文量

273

审稿时长

58 days

期刊介绍： Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer: - Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas. - Spectral lineshape studies including models and computational algorithms. - Atmospheric spectroscopy. - Theoretical and experimental aspects of light scattering. - Application of light scattering in particle characterization and remote sensing. - Application of light scattering in biological sciences and medicine. - Radiative transfer in absorbing, emitting, and scattering media. - Radiative transfer in stochastic media.