Atomic data for permitted resonance lines of atoms and ions from H to Si, and S, Ar, Ca, and Fe

D. A. Verner; E. M. Verner; G. J. Ferland

doi:10.1006/adnd.1996.0018

Atomic data for permitted resonance lines of atoms and ions from H to Si, and S, Ar, Ca, and Fe

D. A. Verner
, E. M. Verner
, G. J. Ferland

Research output: Contribution to journal › Article › peer-review

308 Scopus citations

Abstract

We list vacuum wavelengths, energy levels, statistical weights, transition probabilities, and oscillator strengths for permitted resonance spectral lines of all ions of 18 astrophysically important elements (H through Si, S, Ar, Ca, Fe). Using a compilation of experimental energy levels, we derived accurate wavelengths for 5599 lines of 1828 ground-term multiplets which have gf-values calculated in the Opacity Project. We recalculated the Opacity Project multiplet gf-values to oscillator strengths and transition probabilities of individual lines. For completeness, we added 372 resonance lines of Ne I, Ar I, Fe I, and Fe II ions which are not covered by the Opacity Project. Intercombination and forbidden lines are not included in the present compilation.

Original language	English
Pages (from-to)	1-180
Number of pages	180
Journal	Atomic Data and Nuclear Data Tables
Volume	64
Issue number	1
DOIs	https://doi.org/10.1006/adnd.1996.0018
State	Published - Sep 1996

Bibliographical note

Funding Information:
This work was supported by grants from the National Science Foundation (AST 93-19034) and NASA (NAGW 3315). We are grateful to M. J. Seaton for useful discussions on the Opacity Project data. We are also grate- ful to the Opacity Project team for their efforts to make the data available before publication through the TOPbase database. We acknowledge the use of the TOPbase 0.7 database installed by A. K. Pradhan at the Ohio State University. We thank K. T. Korista for helpful conversations. We are indebted to both referees for suggestions which improved the presentation of the tables.

Funding

This work was supported by grants from the National Science Foundation (AST 93-19034) and NASA (NAGW 3315). We are grateful to M. J. Seaton for useful discussions on the Opacity Project data. We are also grate- ful to the Opacity Project team for their efforts to make the data available before publication through the TOPbase database. We acknowledge the use of the TOPbase 0.7 database installed by A. K. Pradhan at the Ohio State University. We thank K. T. Korista for helpful conversations. We are indebted to both referees for suggestions which improved the presentation of the tables.

Funders	Funder number
National Science Foundation Arctic Social Science Program	AST 93-19034
National Science Foundation Arctic Social Science Program
National Aeronautics and Space Administration	NAGW 3315
National Aeronautics and Space Administration

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

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10.1006/adnd.1996.0018

Cite this

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title = "Atomic data for permitted resonance lines of atoms and ions from H to Si, and S, Ar, Ca, and Fe",

abstract = "We list vacuum wavelengths, energy levels, statistical weights, transition probabilities, and oscillator strengths for permitted resonance spectral lines of all ions of 18 astrophysically important elements (H through Si, S, Ar, Ca, Fe). Using a compilation of experimental energy levels, we derived accurate wavelengths for 5599 lines of 1828 ground-term multiplets which have gf-values calculated in the Opacity Project. We recalculated the Opacity Project multiplet gf-values to oscillator strengths and transition probabilities of individual lines. For completeness, we added 372 resonance lines of Ne I, Ar I, Fe I, and Fe II ions which are not covered by the Opacity Project. Intercombination and forbidden lines are not included in the present compilation.",

author = "Verner, \{D. A.\} and Verner, \{E. M.\} and Ferland, \{G. J.\}",

note = "Funding Information: This work was supported by grants from the National Science Foundation (AST 93-19034) and NASA (NAGW 3315). We are grateful to M. J. Seaton for useful discussions on the Opacity Project data. We are also grate- ful to the Opacity Project team for their efforts to make the data available before publication through the TOPbase database. We acknowledge the use of the TOPbase 0.7 database installed by A. K. Pradhan at the Ohio State University. We thank K. T. Korista for helpful conversations. We are indebted to both referees for suggestions which improved the presentation of the tables.",

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AU - Verner, D. A.

AU - Verner, E. M.

AU - Ferland, G. J.

N1 - Funding Information: This work was supported by grants from the National Science Foundation (AST 93-19034) and NASA (NAGW 3315). We are grateful to M. J. Seaton for useful discussions on the Opacity Project data. We are also grate- ful to the Opacity Project team for their efforts to make the data available before publication through the TOPbase database. We acknowledge the use of the TOPbase 0.7 database installed by A. K. Pradhan at the Ohio State University. We thank K. T. Korista for helpful conversations. We are indebted to both referees for suggestions which improved the presentation of the tables.

PY - 1996/9

Y1 - 1996/9

N2 - We list vacuum wavelengths, energy levels, statistical weights, transition probabilities, and oscillator strengths for permitted resonance spectral lines of all ions of 18 astrophysically important elements (H through Si, S, Ar, Ca, Fe). Using a compilation of experimental energy levels, we derived accurate wavelengths for 5599 lines of 1828 ground-term multiplets which have gf-values calculated in the Opacity Project. We recalculated the Opacity Project multiplet gf-values to oscillator strengths and transition probabilities of individual lines. For completeness, we added 372 resonance lines of Ne I, Ar I, Fe I, and Fe II ions which are not covered by the Opacity Project. Intercombination and forbidden lines are not included in the present compilation.

AB - We list vacuum wavelengths, energy levels, statistical weights, transition probabilities, and oscillator strengths for permitted resonance spectral lines of all ions of 18 astrophysically important elements (H through Si, S, Ar, Ca, Fe). Using a compilation of experimental energy levels, we derived accurate wavelengths for 5599 lines of 1828 ground-term multiplets which have gf-values calculated in the Opacity Project. We recalculated the Opacity Project multiplet gf-values to oscillator strengths and transition probabilities of individual lines. For completeness, we added 372 resonance lines of Ne I, Ar I, Fe I, and Fe II ions which are not covered by the Opacity Project. Intercombination and forbidden lines are not included in the present compilation.

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Atomic data for permitted resonance lines of atoms and ions from H to Si, and S, Ar, Ca, and Fe

Abstract

Bibliographical note

Funding

ASJC Scopus subject areas

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