Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jqsrt..42..295r&link_type=abstract
Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 42, Oct. 1989, p. 295-302.
Astronomy and Astrophysics
Astronomy
16
Extreme Ultraviolet Radiation, Nitrogen, Oscillator Strengths, Oxygen, Sulfur, Ultraviolet Detectors, Calibrating, Plasma Diagnostics, Ultraviolet Astronomy
Scientific paper
Oscillator-strength determinations for EUV branching emissions of atomic oxygen, nitrogen and sulfur are reported. The transitions studied were excited using a beam-foil source and both branching ratios and radiative lifetimes were determined. Calculated transition-probability data for multiply-ionized neon and oxygen emissions were used to obtain an in situ relative sensitivity curve for the EUV detection system used. New oscillator strengths for NII, OII, SII, and SIII EUV branching emissions that terminate on metastable states of the respective ions are reported, together with new lifetime data for ionized sulfur emissions.
Cunningham Andrew J.
Rayburn L. A.
Ryan L. J.
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