Computed profiles of the solar C I multiplets at 1561 and 1657 A

Details Computed profiles of the solar C I multiplets at 1561 and 1657 A Computed profiles of the solar C I multiplets at 1561 and 1657 A

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345.1104m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 1104-1113. Research supported by the Smithsonian Ins

Astronomy and Astrophysics

Astrophysics

10

Carbon, Chromosphere, Fine Structure, Line Spectra, Solar Spectra, Frequency Distribution, Skylab 1, Spectral Energy Distribution, Spectrum Analysis, Ultraviolet Spectra, Ultraviolet Spectrometers

Scientific paper

A nine-level atomic model is presented for C I lines synthesis in the sun. All the atomic parameters are based on recent experimental and theoretical data. Profiles of the multiplets at 1561 and 1657 A are computed from a model of the solar chromosphere. The sensitivity of the results to changes in the atomic parameters is examined. Partial frequency redistribution must be included in these lines to obtain agreement between calculated and observed profiles.

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