Experimental oscillator strengths for resonance transitions in aluminum-like sulfur, S IV

Details Experimental oscillator strengths for resonance transitions in aluminum-like sulfur, S IV Experimental oscillator strengths for resonance transitions in aluminum-like sulfur, S IV

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...327..502r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 327, April 1, 1988, p. 502-506. Research supported by the Naturvetenskaplig

Astronomy and Astrophysics

Astrophysics

16

Electron Energy, Electron Transitions, Oscillator Strengths, Positive Ions, Sulfur, Transition Probabilities, Aluminum, Electron Density (Concentration), Solar Atmosphere, Voyager Project

Scientific paper

The beam-foil technique has been used to determine experimental oscillator strengths for the resonance transitions from the 3s3p2 2S, 2P, and 3s24s 2S terms in S IV. Accurate lifetimes for these terms are obtained. The results are 0.25±0.01 ns for 3p2 2S, 0.076±0.01 ns for 3p2 2P, and 0.16±0.01 ns for 4s 2S. Significant discrepancies with recent theoretical calculations are observed.

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