Dielectronic satellite spectra for highly charged helium-like ions. VI - Iron spectra with improved inner-shell and helium-like excitation rates

Astronomy and Astrophysics – Astrophysics

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Atomic Excitations, Atomic Theory, Electron Transitions, Electronic Spectra, Ion Production Rates, Iron, Solar Flares, Atomic Spectra, Collisional Plasmas, Electron Energy, Electron Orbitals, Electron Recombination, Helium Ions, Resonance Lines, Tokamak Devices

Scientific paper

The atomic theory developed through earlier papers in this series is extended in order to improve the understanding of iron solar flare spectra in the region 1.85-1.88 Å. The new work concerns impact excitation by distorted wave theory for the inner- shell Fe xxiv transitions and the 1 S2 - 1 s 2l transitions in Fe XXV. In addition, rates are evaluated for contributions to the Fe XXV lines from cascade, radiative recombination, dielectronic recombination, and inner-shell ionization of Fe XXIV. The results will be applicable to any plasma with a density below 1015 cm-3, and are therefore of use in Tokamak devices as well as in astrophysics.

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