Energy levels, lifetimes and branch fractions for Fe xi

We present transition energies, probabilities and branching ratios for the electric dipole allowed (E1) and forbidden (M1, E2, M2) lines of the 3s23p4, 3s3p5 and 3s23p33d configurations of Fe xi. Large-scale multiconfiguration Dirac–Fock wavefunctions are applied to include the effects of relativity, correlation and rearrangement of the electron density consistently within the same (computational) model. From the transition probabilities, lifetimes of the 46 lowest-lying excited levels are derived, and the prospects for experimental verification are discussed. An M2 transition is identified in the solar extreme ultraviolet spectrum.

[1]  Stephan Fritzsche,et al.  REOS99: A revised program for transition probability calculations including relativistic, correlation, and relaxation effects , 2000 .

[2]  P. Beiersdorfer,et al.  Visible-range spectroscopy and a lifetime measurement on Kr22+ in an electron beam ion trap , 2000 .

[3]  Stephan Fritzsche,et al.  CALCULATED LEVEL ENERGIES, TRANSITION PROBABILITIES, AND LIFETIMES FOR PHOSPHORUS-LIKE IONS OF THE IRON GROUP IN THE 3s3p4AND 3s23p23dCONFIGURATIONS☆ , 1998 .

[4]  L. Malinovský,et al.  An Analysis of the Solar Extreme-Ultraviolet Between 50 and 300 A , 1973 .

[5]  B. Fawcett Improved oscillator strength calculations for Ti VI and Fe X , 1991 .

[6]  Stephan Fritzsche,et al.  Branching ratios and lifetimes for the low-lying levels of Fe xx , 1999 .

[7]  J. Schmitt,et al.  The extreme ultraviolet coronal spectrum of the solar-type star chi[SUP]1[/SUP] Orionis , 1994 .

[8]  V. Kaufman,et al.  Resonance transitions in the Mg i and Ar i isoelectronic sequences from Cu to Mo , 1987 .

[9]  Stephen Wilson,et al.  Methods in Computational Chemistry , 1987 .

[10]  Werner M. Neupert,et al.  Extreme ultraviolet spectrum of a solar active region from SERTS , 1994 .

[11]  J. Drake,et al.  Stellar Coronal Abundances. II. The First Ionization Potential Effect and Its Absence in the Corona of Procyon , 1995 .

[12]  Stephan Fritzsche,et al.  Calculated level energies, transition probabilities, and lifetimes of silicon-like ions , 1998 .

[13]  É. Biémont,et al.  Forbidden Transitions in 3p4 and 4p4 Configurations , 1986 .

[14]  E. B. Saloman,et al.  Energy levels and transition probabilities in the ground-state configuration of sulfur like ions , 1989 .

[15]  Atomic Data for Permitted Resonance Lines of Atoms and Ions from H to Si, and S, Ar, Ca, and Fe , 1996, atom-ph/9604003.

[16]  K. Dere Spectral lines observed in solar flares between 171 and 630 angstroms , 1978 .

[17]  G. Gwinner,et al.  Magnetic dipole transition rates in B-like and F-like titanium ions measured at a heavy-ion storage ring , 1999 .

[18]  U. Feldman,et al.  Solar spectroscopy in the far-ultraviolet-X-ray wavelength regions - Status and prospects , 1988 .

[19]  P. H. Heckmann,et al.  Beam-foil measurements on intercombination transitions in Cl-like ions of elements Mn through Zn , 1993 .

[20]  B. Fawcett Calculated wavelengths, oscillator strengths, and energy levels for allowed 3-3 and 3–4 transitions for ions in the P-like isoelectronic sequence between P I and Ni XIV , 1987 .

[21]  E. Träbert Solar EUV line identifications from delayed beam‐foil spectra , 1998 .

[22]  G. Brueckner,et al.  The high-resolution solar spectrum, 1175-1710 Å , 1986 .

[23]  W. E. Behring,et al.  A Coronal Spectrum in the 500-1610 Å Wavelength Range Recorded at a Height of 21,000 Kilometers above the West Solar Limb by the SUMER Instrument on Solar and Heliospheric Observatory , 1997 .

[24]  Jack Sugar,et al.  Spectral Data and Grotrian Diagrams for Highly Ionized Iron, Fe VIII‐XXVI , 1990 .

[25]  Stephen M. Shafroth,et al.  Accelerator-based atomic physics : techniques and applications , 1997 .

[26]  B. Fricke,et al.  Comment on the Lifetimes of the 3s3p6 2S1/2 Level for Chlorine-like Ions , 1999 .

[28]  R. Isler,et al.  Solar identifications of Fe X-Fe XIV based on comparison with beam-foil, tokamak and laser-produced plasma spectra , 1993 .