Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...259..869s&link_type=abstract
Astrophysical Journal, Part 1, vol. 259, Aug. 15, 1982, p. 869-879.
Astronomy and Astrophysics
Astronomy
20
Atomic Energy Levels, Chromosphere, Oxygen Spectra, Resonance Lines, Solar Atmosphere, Ultraviolet Astronomy, Atmospheric Models, H Lines, Late Stars, Lyman Beta Radiation, Photoionization, Ultraviolet Spectra
Scientific paper
Spectrum synthesis calculations are presented for the O I resonance triplet at 1304 A and the intercombination doublet at 1358 A for the solar atmosphere and several variants, allowing for triplet fluorescence by the Ly-beta emission of H I. Profiles, synthesized from a seven-level plus continuum O I atom are compared to observations taken with the high-resolution spectrometer on OSO 8. It is found that the O I triplet emission is dominated by the Ly-beta fluorescence and that the agreement between observations and profiles computed with current chromospheric models is much improved over earlier studies.
Shine Richard A.
Skelton Dennis L.
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