Oscillator strengths for optically allowed transitions in carbon-like ions

Details Oscillator strengths for optically allowed transitions in carbon-like ions Oscillator strengths for optically allowed transitions in carbon-like ions

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90..281a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Feb. 1984, p. 281-290. Research supported by the Science and Engineering Research Counc

Astronomy and Astrophysics

Astrophysics

7

Atomic Excitations, Carbon, Isoelectronic Sequence, Optical Transition, Oscillator Strengths, Astrophysics, Configuration Interaction, Electron States, Wave Functions

Scientific paper

Using configuration interaction wavefunctions, the excitation thresholds for the twelve lowest terms arising from the configurations 1s22s22p2, 1s22s2p3, and 1s22p4 of Mg VII have been calculated. The same wavefunctions have been used to calculate the oscillator strengths for the optically allowed transitions in Mg VII. Combining these results with earlier published values for O III, Ne V, Si IX, Ca XV, and Fe XXI, oscillator strengths for other ions in the carbon isoelectronic sequence (F through Ni) have been predicted. The predicted values are found to be slightly lower when compared with the available published results.

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