Updated System of S <sc>i</sc> Levels Using Fourier Transform Infrared Spectroscopy in the Range from 800 to 11,000 cm-1

被引:1
|
作者
Civis, S. [1 ]
Kramida, A. [2 ]
Zanozina, E. M. [1 ]
Kubista, J. [1 ]
Kubelik, P. [1 ]
Ferus, M. [1 ]
Chernov, V. E. [3 ]
机构
[1] Acad Sci Czech Republ, J Heyrovsky Inst Phys Chem, Dolejskova 3, Prague 8, Czech Republic
[2] Natl Inst Stand & Technol, Gaithersburg, MD 20899 USA
[3] Voronezh State Univ, Voronezh 394018, Russia
来源
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2024年 / 274卷 / 02期
基金
俄罗斯科学基金会;
关键词
FTIR LABORATORY MEASUREMENT; OSCILLATOR-STRENGTHS; ATOMIC SULFUR; TRANSITION-PROBABILITIES; PLANETARY-NEBULAE; NEUTRAL SULFUR; ENERGY-LEVELS; RYDBERG STATES; GIANT PLANETS; I SPECTRA;
D O I
10.3847/1538-4365/ad6904
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this study we report on high-precision laboratory measurements of transition wavenumbers for 172 atomic sulfur lines in the infrared region 800-11,000 cm(-1) using Fourier transform spectroscopy techniques. Our analysis includes 96 lines that have not been previously measured in the laboratory. We also correct several sulfur energy-level measurements reported in earlier studies. These refined measurements are important for a range of scientific disciplines, such as astrophysics, atmospheric chemistry, and combustion plasma physics. We have used the combined list of all observed lines to derive a refined set of sulfur energy levels. For about half of all nonautoionizing levels, the uncertainties have been reduced by a factor between 2 and 23. From the newly measured nonpenetrating (high-l) Rydberg levels we have also obtained the first ionization energy of the S atom, IE = 83,559.170(11) cm(-1), which is more accurate than the currently recommended value by 2 orders of magnitude. Our analysis has led to a significantly more accurate result than the earlier set of Ritz wavelengths with observed intensities reduced to a common uniform scale and an extended list of recommended transition probabilities.
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页数:20
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