Inner-shell photoexcitation of Fe XV and Fe XVI

R. Kisielius; A. Hibbert; G. J. Ferland; M. E. Foord; S. J. Rose; P. A.M. Van Hoof; F. P. Keenan

doi:10.1046/j.1365-8711.2003.06801.x

Inner-shell photoexcitation of Fe XV and Fe XVI

R. Kisielius, A. Hibbert, G. J. Ferland, M. E. Foord, S. J. Rose, P. A.M. Van Hoof, F. P. Keenan

Physics And Astronomy

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

6 Scopus citations

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 1s²2s²2p⁶3s ²-1s²2s²2p⁵3l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s²2s ²2p⁶3s-1s²2s²2p ⁵3l3l′ (l and l′ = s,p or d) in Fe XVI, 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
DOIs	https://doi.org/10.1046/j.1365-8711.2003.06801.x
State	Published - Sep 21 2003

Keywords

Atomic data
Line: formation
X-rays: general

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1046/j.1365-8711.2003.06801.x

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 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (l and l′ = s,p or d) in Fe XVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed.",

keywords = "Atomic data, Line: formation, X-rays: general",

author = "R. Kisielius and A. Hibbert and Ferland, {G. J.} and Foord, {M. E.} and Rose, {S. J.} and {Van Hoof}, {P. A.M.} and Keenan, {F. P.}",

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language = "English",

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TY - JOUR

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

AU - Kisielius, R.

AU - Hibbert, A.

AU - Ferland, G. J.

AU - Foord, M. E.

AU - Rose, S. J.

AU - Van Hoof, P. A.M.

AU - Keenan, F. P.

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 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (l and l′ = s,p or d) in Fe XVI, 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 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (l and l′ = s,p or d) in Fe XVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed.

KW - Atomic data

KW - Line: formation

KW - X-rays: general

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VL - 344

SP - 696

EP - 706

IS - 3

ER -

Inner-shell photoexcitation of Fe XV and Fe XVI

Abstract

Keywords

ASJC Scopus subject areas

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