Atomic data for Fe XXII

Details Atomic data for Fe XXII Atomic data for Fe XXII

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.191..631m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 191, May 1980, p. 631-639. Research supported by the Science Research C

Astronomy and Astrophysics

Astronomy

43

Atomic Energy Levels, Iron, Line Spectra, Solar Flares, Solar Spectra, Electron Density Profiles, Electron Scattering, Population Theory, X Ray Spectra

Scientific paper

Intermediate coupling energy levels, oscillator strengths and electron collision strengths in the distorted wave approximation have been computed for Fe XXII. Results are tabulated for the configurations 2s22p, 2s 2p2, 2s23s, 2s23d, 2s 2p 3p, 2s24s, 2s24d, 2s 2p 4p. The level population of the excited level in the ground configuration is given as a function of electron density together with theoretical intensity ratios for the strongest transitions from the excited configurations. The theoretical results are compared to available solar flare observations. The intensity ratios observed correspond to electron densities of less than 10 to the 13 per cu cm.

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