Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203.1269b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, June 1983, p. 1269-1280. Research supported by the
Astronomy and Astrophysics
Astronomy
58
Autoionization, Electron Impact, Ion Charge, Ionic Collisions, Ionization Cross Sections, Nonequilibrium Plasmas, Argon Plasma, Atomic Energy Levels, Atomic Excitations, Born Approximation, Coulomb Collisions, Electron Energy, Ion Beams, Ionization Coefficients, Metal Ions, Strongly Coupled Plasmas
Scientific paper
The procedure suggested by Burgess et al. (1977) to allow for inner-shell excitation and auto-ionization is used with an empirical formula similar in form to that of Lotz (1968) and is compared with a wide range of crossed-beam experimental data for ions having a charge greater than or equal to 2. The general formula obtained for the total ionization cross section, and the corresponding rate coefficient, represents the experimental data to within + or - 23 percent rms deviation. Even though the formula is consistent with the earlier formulas of Seaton (1964, valid only near threshold) and Lotz, it gives a significantly smaller rms deviation through the consistent inclusion of auto-ionization effects. For simple ions, comparisons with much more elaborate quantal calculations are found to be satisfactory. In addition, comparisons are made with the simplified ECIP formula (Burgess, 1964; Burgess and Summers, 1976).
Burgess Andrew
Chidichimo Marita C.
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