Atomic calculation for Fe XXIII, UV, and X-ray lines

Details Atomic calculation for Fe XXIII, UV, and X-ray lines Atomic calculation for Fe XXIII, UV, and X-ray lines

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103..324b&link_type=abstract

Astronomy and Astrophysics, vol. 103, no. 2, Nov. 1981, p. 324-330. Research supported by the Science Research Council.

Astronomy and Astrophysics

Astrophysics

31

Atomic Spectra, Iron, Line Spectra, Solar Flares, Ultraviolet Spectra, X Ray Spectra, Collision Parameters, Electron Energy, Electron Scattering, Ion Scattering, Proton Scattering, Solar Spectra, Transition Probabilities, Wavelengths

Scientific paper

Electron-ion scattering data have been obtained for the configurations 22, 2s2p, 2p2, 2s3s, 2s3p, and 2s3d of Fe XXIII in the "distorted wave" approximation. Oscillator and collision strengths are compared with other calculations. Wavelengths for various UV and X-ray lines are compared with laboratory measurements. New identifications are given for recent solar spectra based on intensity estimates. A line at 11.737 Å is identified as the strongest Fe XXIII line in the solar X-ray spectrum.

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