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 |
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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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E. ; Zanozina, E. M.</creator><creatorcontrib>Civiš, S. ; Ferus, M. ; Chernov, V. E. ; Zanozina, E. M.</creatorcontrib><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.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>DOI: 10.1051/0004-6361/201321052</identifier><language>eng</language><publisher>EDP Sciences</publisher><subject>atomic data ; Infrared ; Infrared radiation ; Lists ; Magnesium ; methods: laboratory ; Orbitals ; Oscillator strengths ; Spectra ; techniques: spectroscopic ; Wavenumber</subject><ispartof>Astronomy and astrophysics (Berlin), 2013-06, Vol.554, p.1-6</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c398t-27231eb57f6b0fb0e1e9dc98afd22802cb8ed274ebc128a00571cc692f2eb9db3</citedby><cites>FETCH-LOGICAL-c398t-27231eb57f6b0fb0e1e9dc98afd22802cb8ed274ebc128a00571cc692f2eb9db3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,3725,27923,27924</link.rule.ids></links><search><creatorcontrib>Civiš, S.</creatorcontrib><creatorcontrib>Ferus, M.</creatorcontrib><creatorcontrib>Chernov, V. 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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. 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M.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Civiš, S.</au><au>Ferus, M.</au><au>Chernov, V. E.</au><au>Zanozina, E. M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Infrared transitions and oscillator strengths of Ca and Mg</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2013-06-01</date><risdate>2013</risdate><volume>554</volume><spage>1</spage><epage>6</epage><pages>1-6</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><abstract>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.</abstract><pub>EDP Sciences</pub><doi>10.1051/0004-6361/201321052</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
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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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