J. F. Seely, U. Feldman, C. M. Brown, M. C. Richardson, D. D. Dietrich, and W. E. Behring, "Transitions in Na-like and Mg-like ions of In, Sb, I, and Cs," J. Opt. Soc. Am. B 5, 785-788 (1988)
The spectra of highly charged ions of the elements In, Sb, I, and Cs have been recorded by using a 3-m grazing-incidence spectrograph at the University of Rochester’s Laboratory for Laser Energetics. Transitions in the Na i and Mg i isoelectronic sequences have been identified. Wavelengths in the range 7–100 Å were measured to an accuracy of ± 0.02 Å, and energy levels were derived from the measured wavelengths.
You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
You do not have subscription access to this journal. Figure files are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
You do not have subscription access to this journal. Article tables are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Intensities based on visual estimates of plate darkening.
Wavelengths predicted by Reader et al.1
Wavelengths calculated by the present authors using Grant’s program.7,8
Table 2
Wavelengths (in Angstroms) and Classification of Spectral Lines for Mg-like Ions
Intensities based on visual estimates of plate darkening.
Wavelengths predicted by Ivanova et al.9
Wavelengths calculated by the present authors using Grant’s program.7,8
Energies calculated by the present authors using Grant’s program.7,8
Energy based on the measured 3p2P3/2 energy and the calculated 3p2P1/2–2P3/2 splitting.
Intensities based on visual estimates of plate darkening.
Wavelengths predicted by Reader et al.1
Wavelengths calculated by the present authors using Grant’s program.7,8
Table 2
Wavelengths (in Angstroms) and Classification of Spectral Lines for Mg-like Ions
Intensities based on visual estimates of plate darkening.
Wavelengths predicted by Ivanova et al.9
Wavelengths calculated by the present authors using Grant’s program.7,8
Energies calculated by the present authors using Grant’s program.7,8
Energy based on the measured 3p2P3/2 energy and the calculated 3p2P1/2–2P3/2 splitting.
Add to BibSonomy