Physics
Scientific paper
Jul 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002soph..208...91d&link_type=abstract
Solar Physics, v. 208, Issue 1, p. 91-111 (2002).
Physics
10
Scientific paper
In the past few years new calculations of the ionization and recombination rates have been published. The new Fe ionization equilibrium for these new rates is available for a Maxwellian distribution. Therefore the updated Fe ionization equilibrium for the non-thermal κ-distribution with an enhanced number of particles in the high-energy tail is presented. Results for the various deviations from a Maxwellian distribution are given in tabular form and these are compared with previous ones. A method for the determination of an energy distribution different from the Maxwellian one is suggested.
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