Inner-shell photoexcitation of Fe XV and Fe XVI
Data(s) |
21/09/2003
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Resumo |
The configuration-interaction method as implemented in the computer code CIV3 is used to determine energy levels, electric dipole radiative transition wavelengths, oscillator strengths and transition probabilities for inner-shell excitation of transitions in Fe XV and Fe XVI. Specifically, transitions are considered of the type 1s(2) 2s(2) 2p(6) 3s(2) -1s(2) 2s(2) 2p(5) 3l3l' 3l" (l, l' and l" = s,p or d) in FeXV and 1s(2) 2s(2) 2p(6) 3s- 1s(2) 2s(2) 2p(5) 3l3l' (l and l' = s,p or d) in FeXVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed. |
Identificador |
http://www.scopus.com/inward/record.url?scp=0142260959&partnerID=8YFLogxK |
Idioma(s) |
eng |
Direitos |
info:eu-repo/semantics/restrictedAccess |
Fonte |
Keenan , F , Kisielius , R , Hibbert , A , Ferland , G J , Foord , M E , Rose , S J & Van Hoof , P A M 2003 , ' Inner-shell photoexcitation of Fe XV and Fe XVI ' Monthly Notices of the Royal Astronomical Society , vol 344 , no. 3 , pp. 696-706 . |
Palavras-Chave | #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science |
Tipo |
article |