Stark Widths of Na IV Spectral Lines
Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia
Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères—LERMA, Observatoire de Paris, 5 Place Jules Janssen, 92195 Meudon CEDEX, France
Department of Geography, Faculty of Natural Sciences and Mathematics, University of Kosovska Mitrovica, Ive Lole Ribara 29, 38220 Kosovska Mitrovica, Serbia
Edificio A. Einstein (C-2), Universidad de Córdoba, Campus de Rabanales, 14071 Córdoba, Spain
Current address: Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia.
These authors contributed equally to this work.
Author to whom correspondence should be addressed.
Academic Editor: Robert C. Forrey
Received: 16 August 2017 / Revised: 8 September 2017 / Accepted: 14 September 2017 / Published: 18 September 2017
Sodium is a very important element for the research and analysis of astrophysical, laboratory, and technological plasmas, but neither theoretical nor experimental data on Stark broadening of Na IV spectral lines are present in the literature. Using the modified semiempirical method of Dimitrijević and Konjević, here Stark widths have been calculated for nine Na IV transitions. Na IV belongs to the oxygen isoelectronic sequence, and we have calculated Stark widths belonging to singlets, triplets, and quintuplets, as well as with different parent terms. This is used to discuss similarities within one transition array with different multiplicities and parent terms. Additionally, calculated widths will be implemented in the STARK-B database (http://stark-b.obspm.fr
) which is also a part of the Virtual Atomic and Molecular Data Center (VAMDC—http://www.vamdc.org/
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MDPI and ACS Style
Dimitrijević, M.S.; Simić, Z.; Valjarević, A.; Yubero, C. Stark Widths of Na IV Spectral Lines. Atoms 2017, 5, 29.
Dimitrijević MS, Simić Z, Valjarević A, Yubero C. Stark Widths of Na IV Spectral Lines. Atoms. 2017; 5(3):29.
Dimitrijević, Milan S.; Simić, Zoran; Valjarević, Aleksandar; Yubero, Cristina. 2017. "Stark Widths of Na IV Spectral Lines." Atoms 5, no. 3: 29.
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