2009
DOI: 10.1016/j.adt.2008.12.002
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Energy levels and spectral lines of tungsten, W III through W LXXIV

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Cited by 201 publications
(306 citation statements)
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“…Spectroscopic observations and further collisional data are becoming available now and are summarized in several contributions to the present Special Issue of ATOMS on "Atomic Data for Tungsten". Detailed information about energy levels of singly excited states in tungsten ions has been compiled by Kramida and Shirai [23][24][25] and can be found in the NIST Atomic Spectra Data Base [26].…”
Section: Introductionmentioning
confidence: 99%
“…Spectroscopic observations and further collisional data are becoming available now and are summarized in several contributions to the present Special Issue of ATOMS on "Atomic Data for Tungsten". Detailed information about energy levels of singly excited states in tungsten ions has been compiled by Kramida and Shirai [23][24][25] and can be found in the NIST Atomic Spectra Data Base [26].…”
Section: Introductionmentioning
confidence: 99%
“…Later on, an experimental observation of W VIII spectrum was performed by Veres et al [17] in emission of tokamak plasma but the low spectral resolution did not allow them to identify the observed broad peaks. However, using the weighted average energies of sub-configurations based on the 4f predicted by Kramida and Shirai [14]. The level identifications reported in [13] were supported by calculations performed using the pseudo-relativistic Hartree-Fock (HFR) method of Cowan [18] combined with a semi-empirical adjustment of the energy parameters.…”
Section: Available Atomic Data In W VIIImentioning
confidence: 99%
“…This lack of knowledge was underlined by Kramida and Shirai [14] who compiled all the classified energy levels and spectral lines of multiply ionized tungsten atoms from W 2+ to W 73+ . In this compilation, it was reminded that it was by the way uncertain whether the ground state of W VIII was 4f P°3/2, making this ion the only known case of p and f orbitals competing for the ground state, as previously noted by Sugar and Kaufman [15].…”
Section: Available Atomic Data In W VIIImentioning
confidence: 99%
“…This strong dependence reflects the charge distribution in the trap. For example, after the electron energy was changed from 630 eV to 675 eV, production of W 23+ became available because the ionization energy of W 22+ is 643 eV [18]. The lines at around 409 and 432 nm, appeared at 675 eV, are thus considered to be emission lines from W 23+ .…”
Section: Survey and Identification Of Previously Unreported Linesmentioning
confidence: 99%