Infrared transitions and oscillator strengths of Ca and Mg

Aims. While solar spectra contain a lot of Ca I and Mg I infrared (IR) lines, no laboratory-measured spectra of these atoms have been reported for wavenumbers below 2000 cm-1. This study reports Ca I spectra in the 1300–4500 cm-1 range and Mg I spectra in the 1300–4500 cm-1 range. Methods. We perfor...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2013-06, Vol.554, p.1-6
Hauptverfasser: Civiš, S., Ferus, M., Chernov, V. E., Zanozina, E. M.
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creator Civiš, S.
Ferus, M.
Chernov, V. E.
Zanozina, E. M.
description Aims. While solar spectra contain a lot of Ca I and Mg I infrared (IR) lines, no laboratory-measured spectra of these atoms have been reported for wavenumbers below 2000 cm-1. This study reports Ca I spectra in the 1300–4500 cm-1 range and Mg I spectra in the 1300–4500 cm-1 range. Methods. We performed a time-resolved Fourier transform infrared spectroscopy study of a plasma created by the laser ablation of MgF2 and CaF2 targets in a vacuum. The oscillator strengths (f-values) were calculated using quantum defect theory (QDT), which shows good agreement with the available experimental and theoretical results. Results. We report several Ca I and Mg I IR lines that have not been measured previously in laboratory. The recorded spectra allow the excitation energies of some Ca I and Mg I states with high orbital momentum (l = 4,5) to be determined. We also provide a long list of QDT-calculated f-values for Ca I and Mg I in the range of 800–9000 cm-1.
doi_str_mv 10.1051/0004-6361/201321052
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source Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; EZB-FREE-00999 freely available EZB journals
subjects atomic data
Infrared
Infrared radiation
Lists
Magnesium
methods: laboratory
Orbitals
Oscillator strengths
Spectra
techniques: spectroscopic
Wavenumber
title Infrared transitions and oscillator strengths of Ca and Mg
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