C IV line ratios in the sun

Details C IV line ratios in the sun C IV line ratios in the sun

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...385..381k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 385, Jan. 20, 1992, p. 381-383. Research supported by Nuffield Foundation a

Astronomy and Astrophysics

Astrophysics

10

Electron Transitions, Emission Spectra, Line Spectra, Solar Atmosphere, Solar Spectra, Atomic Excitations, Electron Energy, Electron Impact, Solar Flares

Scientific paper

Theoretical electron temperature-sensitive emission-line ratios are calculated with R-matrix analysis of electron-impact excitation rates for transitions in C IV. Two of the emission-line ratios are found to agree with observational data on the sun taken with a slitless spectrograph aboard Skylab, and the two remaining lines have inaccuracies that can be attributed to blending of the 312.43 A line. The agreement between the observational and analytical data lends credence to the accuracy of the atomic data used in the analysis.

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