Abstract
Narrow (Δλ<5 Å), intense quasicontinuum bands, appearing in emission spectra of highly ionized rare-earth elements between 70 and 100 Å, previously observed in tokamaks and laser-produced plasmas, have been obtained from a low-inductance vacuum spark. The bands shift toward shorter wavelengths with increasing atomic number Z. Using the unresolved transition array model, these bands are identified as primarily 4d-4f transitions in Rh i to Rb i–like ions, although the widths come out too large and the mean wavelengths are much too dependent on ionization stages. Detailed ab initio computations show that the interactions between the 444f and 44 configurations are responsible for the narrowing and the superposition of the transition arrays for the different ionization stages of a given element, in agreement with experimental data.
- Received 21 January 1987
DOI:https://doi.org/10.1103/PhysRevA.35.5051
©1987 American Physical Society