S VI line ratios in the sun

Details S VI line ratios in the sun S VI line ratios in the sun

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..279k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 279-284. SERC-supported research.

Physics

9

Electron Transitions, Line Spectra, Solar Spectra, Sulfur, Coronal Holes, Emission Spectra, Solar Spectrometers, Stellar Composition

Scientific paper

R-matrix calculations of electron impact excitation rates in S VI have been used to obtain the theoretical temperature sensitive emission lines ratios I(712.8-A)/I(944.5-A) and I(712.8-A)/I(933.4-A). It is found that the 944.5-A transition may be blended with lines from species with relatively low ionization potentials. It is suggested that the 712.8-A transition may be similarly blended.

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