Inner-shell photoexcitation of Fe XV and Fe XVI


Autoria(s): Keenan, Francis; Kisielius, Romas; Hibbert, Alan; Ferland, G.J.; Foord, M.E.; Rose, S.J.; Van Hoof, P.A.M.
Data(s)

21/09/2003

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://pure.qub.ac.uk/portal/en/publications/innershell-photoexcitation-of-fe-xv-and-fe-xvi(44d273eb-b36b-47a0-aca2-3565a9e4abff).html

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