NASA NTRS · 19820031109
Recombination coefficients for iron ions
Abstract
Radiative recombination coefficients for all Fe ions are calculated by use of the Milne relation of detailed balance. Analytic fits are made to the dielectronic recombination rates computed by Jacobs (1977) and the Burgess general formula (1965). Higher level rates are treated hydrogenically by a quantum defect method based on the energies of the levels. Recombination coefficients for Fe I to Fe 26 are listed.
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Woods, D. T., Shull, J. M., Sarazin, C. L.. 1981-10-01. Recombination coefficients for iron ions. https://ntrs.nasa.gov/citations/19820031109
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