Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines

In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the existing measured, calculated and predicted Stark width values was performed for ten singly ionized emitters: C, N, O, F, Ne Si, P, S, Cl and Ar in the lower lying 3s - 3p, 3p - 3d and 4s - 4p transitio...

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Main Author: Djeniže S.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2000-01-01
Series:Serbian Astronomical Journal
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2000/1450-698X0061015D.pdf
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author Djeniže S.
author_facet Djeniže S.
author_sort Djeniže S.
collection DOAJ
description In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the existing measured, calculated and predicted Stark width values was performed for ten singly ionized emitters: C, N, O, F, Ne Si, P, S, Cl and Ar in the lower lying 3s - 3p, 3p - 3d and 4s - 4p transitions. These emitters are present in many cosmic light sources. On the basis of the agreement between mentioned values 17 spectral lines from six singly ionized spectra have been recommended, for the first time, for plasma spectroscopy as spectral lines with reliable Stark width data. Critical analysis of the existing Stark width data is also given.
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spelling doaj.art-44b6e894e34a48fdbfc725bfbe2fb4dc2022-12-21T22:46:19ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892000-01-012000161152310.2298/SAJ0061015D1450-698X0061015DMeasured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral linesDjeniže S.0Faculty of Physics, BelgradeIn order to find reliable Stark width data, needed in plasma spectroscopy comparision between the existing measured, calculated and predicted Stark width values was performed for ten singly ionized emitters: C, N, O, F, Ne Si, P, S, Cl and Ar in the lower lying 3s - 3p, 3p - 3d and 4s - 4p transitions. These emitters are present in many cosmic light sources. On the basis of the agreement between mentioned values 17 spectral lines from six singly ionized spectra have been recommended, for the first time, for plasma spectroscopy as spectral lines with reliable Stark width data. Critical analysis of the existing Stark width data is also given.http://www.doiserbia.nb.rs/img/doi/1450-698X/2000/1450-698X0061015D.pdf
spellingShingle Djeniže S.
Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
Serbian Astronomical Journal
title Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
title_full Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
title_fullStr Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
title_full_unstemmed Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
title_short Measured, calculated and predicted Stark widths of the singly ionized C, N, O, F, Ne, Si, P, S, Cl and Ar spectral lines
title_sort measured calculated and predicted stark widths of the singly ionized c n o f ne si p s cl and ar spectral lines
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2000/1450-698X0061015D.pdf
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