Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....83..380b&link_type=abstract
Astronomy and Astrophysics, vol. 83, no. 3, Mar. 1980, p. 380-382. Research supported by the Science Research Council.
Astronomy and Astrophysics
Astrophysics
38
Atomic Energy Levels, Electron Transitions, Iron, Solar Flares, Toroidal Plasmas, Electron Density (Concentration), Electron Scattering, Plasma Spectra, Solar Spectra, Tokamak Devices, Ultraviolet Spectra
Scientific paper
New atomic data are tabulated for Fe(+19). The electron collision strengths are calculated using the 'distorted wave' approximation and results are presented for several energies of the exciting electron. The populations of the ground levels are calculated as a function of electron density under conditions appropriate to solar flares and tokamak plasmas. Theoretical intensity ratios are tabulated for the UV lines.
Bhatia Anand K.
Mason Harris E.
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