Theoretical intensity ratios for the UV lines of MG VII, SI IX and S XI

Details Theoretical intensity ratios for the UV lines of MG VII, SI IX and S XI Theoretical intensity ratios for the UV lines of MG VII, SI IX and S XI

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..423m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Aug. 1978, p. 423-437. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

70

Line Spectra, Luminous Intensity, Solar Atmosphere, Solar Spectra, Ultraviolet Spectra, Electron Density (Concentration), Forbidden Transitions, Magnesium, Silicon, Solar Corona, Sulfur

Scientific paper

Energy levels, oscillator strengths, and electron collision strengths have been computed for the configurations 2s2 2p2, 2s 2p3, 2p4 of Mg VII, Si IX, and S XI. Level populations for the ground configuration and theoretical intensity ratios for the UV lines are tabulated for electron densities and temperatures appropriate to the solar atmosphere. The identification of the Mg VII, Si IX, and S XI UV lines is discussed.

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