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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Format: | Article |
Language: | English |
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Astronomical Observatory, Department of Astronomy, Belgrade
2000-01-01
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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. |
first_indexed | 2024-12-14T21:47:40Z |
format | Article |
id | doaj.art-44b6e894e34a48fdbfc725bfbe2fb4dc |
institution | Directory Open Access Journal |
issn | 1450-698X 1820-9289 |
language | English |
last_indexed | 2024-12-14T21:47:40Z |
publishDate | 2000-01-01 |
publisher | Astronomical Observatory, Department of Astronomy, Belgrade |
record_format | Article |
series | Serbian Astronomical Journal |
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 |
work_keys_str_mv | AT djenizes measuredcalculatedandpredictedstarkwidthsofthesinglyionizedcnofnesipsclandarspectrallines |