Level populations and line intensity ratios for transitions between the 1s2 2s2 2p2 and 1s2 2s 2p3 configurations of carbon-like ions

Details Level populations and line intensity ratios for transitions between the 1s2 2s2 2p2 and 1s2 2s 2p3 configurations of carbon-like ions Level populations and line intensity ratios for transitions between the 1s2 2s2 2p2 and 1s2 2s 2p3 configurations of carbon-like ions

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apjs...61..699a&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 61, Aug. 1986, p. 699-717. SERC-supported research.

Astronomy and Astrophysics

Astrophysics

23

Astrophysics, Atomic Energy Levels, Ion Density (Concentration), Line Spectra, Transition Probabilities, Carbon, Cosmic Plasma, Electron Energy, Magnesium, Nebulae, Neon, Silicon, Tables (Data), Wave Functions

Scientific paper

The transition probabilities for transitions between the 1s22s22p2 and 1s22s2p3 configurations of carbon-like ions have been calculated using configuration interaction wave functions in the CIV3 program. Using these values together with the experimental threshold energies and earlier reported R-matrix data for the effective collision strengths, populations of the lowest 15 excited levels of the carbon-like ions are calculated. The results are tabulated at a series of electron temperatures and densities for Ne V, Mg VII, and Si IX.

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