Physics
Scientific paper
Jun 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230..627j&link_type=abstract
Astrophysical Journal, Part 1, vol. 230, June 1, 1979, p. 627-638. NASA-Navy-supported research.
Physics
73
Gas Ionization, Radiative Recombination, Rarefied Plasmas, Solar Corona, Solar Physics, Bremsstrahlung, Dielectric Properties, Magnesium, Neon, Sulfur
Scientific paper
Results of detailed and systematic calculations are presented for the total dielectronic recombination rate coefficients for the ions of Ne, Mg, and S in a low-density predominantly hydrogen plasma. The new recombination rates are used to calculate solar corona ionization-equilibrium distributions of the ions. The most important effect of dielectronic recombination for ions in corona equilibrium is found to be a shift in the maximum-abundance temperatures toward higher temperatures, which are in some cases reduced from those predicted on the basis of the simple Burgess formula.
Blaha M.
Davis Jared
Jacobs Verne L.
Rogerson J. E.
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