Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..777k&link_type=abstract
Astrophysical Journal, vol. 199, Aug. 1, 1975, pt. 1, p. 777-780.
Astronomy and Astrophysics
Astrophysics
8
Abundance, Electron Transitions, Ion Density (Concentration), Line Spectra, Solar Spectra, Fine Structure, Gas Ionization, Neon, Solar X-Rays, Transition Probabilities, X Ray Spectra
Scientific paper
Subordinate 2p(5)4d-2p(5)3p transitions in the neon-like ions from Ca XI through Ni XIX are identified. Such transitions between excited levels have not previously been reported for ionization stages higher than Al IV, although the resonance lines are known through Zn XXI in the neon isoelectronic sequence. Measurement of the solar flux in such transitions may aid in establishing the relative importance of the several cascade processes giving rise to the observed Fe XVII resonance lines.
Behring William E.
Cohen Lawrence
Kastner Sidney O.
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