Inner-shell photoexcitation of Fe XV and Fe XVI

Francis Keenan; Romas Kisielius; Alan Hibbert; G.J. Ferland; M.E. Foord; S.J. Rose; P.A.M. Van Hoof

Inner-shell photoexcitation of Fe XV and Fe XVI

Francis Keenan
, Romas Kisielius
, Alan Hibbert
, G.J. Ferland
, M.E. Foord
, S.J. Rose
, P.A.M. Van Hoof

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

Abstract

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.

Original language	English
Pages (from-to)	696-706
Number of pages	11
Journal	Monthly Notices of the Royal Astronomical Society
Volume	344
Issue number	3
Publication status	Published - 21 Sept 2003

ASJC Scopus subject areas

Space and Planetary Science

Cite this

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title = "Inner-shell photoexcitation of Fe XV and Fe XVI",

abstract = "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.",

author = "Francis Keenan and Romas Kisielius and Alan Hibbert and G.J. Ferland and M.E. Foord and S.J. Rose and \{Van Hoof\}, P.A.M.",

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volume = "344",

pages = "696--706",

journal = "Monthly Notices of the Royal Astronomical Society",

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TY - JOUR

T1 - Inner-shell photoexcitation of Fe XV and Fe XVI

AU - Keenan, Francis

AU - Kisielius, Romas

AU - Hibbert, Alan

AU - Ferland, G.J.

AU - Foord, M.E.

AU - Rose, S.J.

AU - Van Hoof, P.A.M.

PY - 2003/9/21

Y1 - 2003/9/21

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/0142260959

M3 - Article

SN - 0035-8711

VL - 344

SP - 696

EP - 706

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

Inner-shell photoexcitation of Fe XV and Fe XVI

Abstract

ASJC Scopus subject areas

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