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Published online by Cambridge University Press: 12 April 2016
The formulas for mean wavelengths and widths of Unresolved Transition Arrays (UTA)[1,2], have been extended to include spectator electrons and jj transitions. These were used to interpret several sorts of satellite spectra, e.g., 3d10 nℓq− −3d94fnq transitions in atoms Tm thru W from laser produced plasmas, and 3dm4s − 3dm−1 4p4s in Mo and Pd spectra. The Unresolved Character of the UTA will be discussed thanks to an evaluation of the number of lines in the array. This will be applied to 4d-4f transitions in Ionized Rare Earths.