Effect of the parameters of the medium on the reduction of models of highly ionized atoms

Details Effect of the parameters of the medium on the reduction of models of highly ionized atoms Effect of the parameters of the medium on the reduction of models of highly ionized atoms

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cajph..54.1426n&link_type=abstract

Canadian Journal of Physics, vol. 54, July 15, 1976, p. 1426-1432. In French.

Physics

Atomic Energy Levels, Electron Density (Concentration), Ion Recombination, Iron, Solar Corona, Temperature Distribution, Atmospheric Models, Ground State, Ionic Reactions, Linear Equations, Mathematical Models, Population Theory, Solar Electrons, Statistical Analysis

Scientific paper

Twenty different models, formed by different combinations of energy levels, of the Fe XI ion of the solar corona were considered under the assumption that the coronal medium is defined by two basic parameters: temperature and electron density. For each of these models, the relative populations of the ground state of the ion were calculated and linear equations of stationary statistical equilibrium were solved by reducing each of the models considered to an equivalent model of smaller dimension.

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