MG I as a probe of the solar chromosphere - The atomic model

Details MG I as a probe of the solar chromosphere - The atomic model MG I as a probe of the solar chromosphere - The atomic model

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...330.1008m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 330, July 15, 1988, p. 1008-1021.

Astronomy and Astrophysics

Astrophysics

48

Atomic Collisions, Atomic Energy Levels, Atomic Spectra, Chromosphere, Magnesium, Solar Atmosphere, Einstein Equations, Ionization Cross Sections, Opacity, Photoionization, Photosphere, Scattering Cross Sections, Solar Flares

Scientific paper

The authors present a complete atomic model for Mg I line synthesis, where all the atomic parameters are based on recent experimental and theoretical data. It is studied how the computed profiles at 4571 Å and 5173 Å are influenced by the choice of these parameters and the number of levels included in the model atom. The authors also present observed profiles of the λ5173 Å b2 line and theoretical profiles for comparison based on a recent atmospheric model for the average quiet Sun.

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