Transition Energies, Oscillator Strengths, and Transition Probabilities of High-lying 1P O and 1D E States of Neon-like Ions

Details Transition Energies, Oscillator Strengths, and Transition Probabilities of High-lying 1P O and 1D E States of Neon-like Ions Transition Energies, Oscillator Strengths, and Transition Probabilities of High-lying 1P O and 1D E States of Neon-like Ions

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...468..445d&link_type=abstract

Astrophysical Journal v.468, p.445

Astronomy and Astrophysics

Astronomy

8

Atomic Data, Atomic Processes

Scientific paper

Transition energies, oscillator strengths, and transition probabilities for the high-lying dipolar and quadrupolar excitations up to principal quantum number n = 4 have been calculated for the first few members of the Ne isoelectronic sequence using the time-dependent coupled Hartree-Fock (TDCHF) theory. These data are very useful for the spectral diagnostics of solar, stellar, and laboratory plasma. Most of the data for high-lying transitions are new. For low-lying transitions, results agree well with the existing theoretical and experimental data.

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