Solar O I 1304-A triplet line profiles

Details Solar O I 1304-A triplet line profiles Solar O I 1304-A triplet line profiles

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....9719519g&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. A12, p. 19,519-19,525.

Physics

12

Atomic Energy Levels, Line Shape, Oxygen Atoms, Oxygen Spectra, Solar Atmosphere, Oso, Solar Cycles, Solar Maximum Mission

Scientific paper

Estimates were made of the full-disk line profiles of the solar O I resonant triplet at 1304 A, using data from the SMM and the Orbiting Solar Observatory 8 for the time period 1975-1985. The observed line profiles are parameterized using a nonlinear least squares fit of the data by a simple empirical representation of the general line shape. The derived full-disk line shape parameters may be used, in combination with an appropriate value for the line-integrated full-disk solar flux, in the analysis of planetary or cometary O I 1304-A observations under any solar conditions.

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