Population processes of 3p/4/4s levels of Fe X

Details Population processes of 3p/4/4s levels of Fe X Population processes of 3p/4/4s levels of Fe X

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..665m&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 15, 1980, p. 665-677.

Astronomy and Astrophysics

Astrophysics

17

Atomic Energy Levels, Iron, Line Spectra, Metallic Plasmas, Plasma Spectra, Transition Probabilities, Cosmic Plasma, Rydberg Series

Scientific paper

Lines emitted from levels of the 3s(2)3p(4)4s configuration to the ground levels 3s(2)3p(5) of Fe X are observed in both solar and laboratory plasma. Their relative intensities are five to six times stronger than those calculated assuming that the coronal equation is valid. Additional population processes - cascades from the 3s(2)3p(4)np configurations, radiative and dielectronic recombinations from Fe XI - have been included. Furthermore, the intensity of the unresolved satellite lines has been added to the line intensity. The intensities of lines emitted from the 3s(2)3p(4)4s levels are then reproduced with an accuracy of a factor 2.

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