Expected intensities of solar neon-like ions

Details Expected intensities of solar neon-like ions Expected intensities of solar neon-like ions

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96...11b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, March 1985, p. 11-26.

Physics

5

Atomic Energy Levels, Emission Spectra, Forbidden Transitions, Gas Density, Neon, Solar Spectra, Abundance, Heavy Ions, Lyman Spectra, Quadrupoles, Solar Activity, Solar Flares

Scientific paper

A study of the expected intensities of the stronger solar neon-like ion emission lines, some not yet observed, is carried out to compare with the observational situation. The potential usefulness of the 2p53s(3P2) - 2p6 forbidden line as a density diagnostic is discussed and new electric quadrupole lines in the soft X-ray range are noted. "Observability diagrams" are presented as a convenient overview of the known and unobserved lines. The S VII resonance lines appear to have anomalous intensities.

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