Stark broadening parameters for 6s 4F - 6p 4(D, F, G)o supermultiplet of singly ionized Hafnium

Stark broadening parameters -line widths and shifts -are of interest in stellar spectroscopy as well as in laboratory and technological plasmas.Stark widths and shifts have been calculated for 28 Hf II transitions using plasma electron density of 10 17 cm -3 and temperature from 5000K to 80000K as parameters.The calculations were performed according to the simplified modified semiempirical (SMSE) method.

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Publication Details

Journal
Contributions of the Astronomical Observatory Skalnaté Pleso
Published
2025-02-01
DOI
https://doi.org/10.31577/caosp.2025.55.2.69
Primary Topic
Laser-induced spectroscopy and plasma
Type
article
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article

Stark broadening parameters for 6s 4F - 6p 4(D, F, G)o supermultiplet of singly ionized Hafnium

Z. Simić, M. S. Dimitrijević, N. Sakan
Contributions of the Astronomical Observatory Skalnaté Pleso
Laser-induced spectroscopy and plasma
article

Stark broadening parameters for 6s 4F - 6p 4(D, F, G)o supermultiplet of singly ionized Hafnium

Z. Simić, M. S. Dimitrijević, N. Sakan
article en

Abstract

Stark broadening parameters -line widths and shifts -are of interest in stellar spectroscopy as well as in laboratory and technological plasmas.Stark widths and shifts have been calculated for 28 Hf II transitions using plasma electron density of 10 17 cm -3 and temperature from 5000K to 80000K as parameters.The calculations were performed according to the simplified modified semiempirical (SMSE) method.

Contributions of the Astronomical Observatory Skalnaté PlesoVol. 55(2)
Openalex Percentile: Top 96%
Laser-induced spectroscopy and plasma
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Stark broadening parameters for 6s 4F - 6p 4(D, F, G)o supermultiplet of singly ionized Hafnium — Z. Simić, M. S. Dimitrijević, et al. · Contributions of the Astronomical Observatory Skalnaté Pleso (2025) | TGRS Research Map | TGRS