A. Tauheed, Y. N. Joshi, V. Kaufman, J. Sugar, and E. H. Pinnington, "Analysis of the 5s25p2–(5s5p3 + 5s25p5d + 5s25p6s) transitions of four-times ionized xenon (Xe v)," J. Opt. Soc. Am. B 10, 561-565 (1993)
The spectrum of xenon was photographed in the range 350–2000 Å with 3-m normal-incidence and 10.7-m normal-incidence spectrographs. The source used in both cases was a gas-triggered spark. The Xe v spectrum was distinguished by observation of spectral changes with variation of spark current. The 5s25p2–(5s5p3 + 5s25p5d + 5s25p6s) transition array of Xe v was identified and analyzed. Calculations were carried out to assist in the analysis and to help us to interpret the results. An earlier analysis was revised and extended, and 73 lines are now classified. A value for the ionization energy of 436 700 ± 400 cm−1 was determined.
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.
You do not have subscription access to this journal. Equations are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Visually estimated relative plate blackening.
Blended with C iii line.
Blended with O iv line.
Blended with Xe vii line (see Ref. 7).
Blended with Xe iv line (see Ref. 11).
Blended with O iii line.
Table 2
Energy Levels of the Ground Configuration 5s25p2 of Xe v
Standard deviation, which is [∑ (obs. value − fitted value)2/(n − m)]1/2, where n is the number of known levels and m is the number of free parameters.
Table 4
Observed Energy Levels of 5s5p3, 5s25p5d, and 5s25p6s Configuration of Xe v
Experimental minus calculated level in inverse centimeters.
The two highest percentages are given.
Calculated value from fitted-parameter calculation.
Third-largest component.
Table 5
Energy Parameter Values (cm−1) of the 5s5ps, 5s25p5d, 5s25p6s, 5s25p6d, and 5s25p7s Configurations of Xe v
Visually estimated relative plate blackening.
Blended with C iii line.
Blended with O iv line.
Blended with Xe vii line (see Ref. 7).
Blended with Xe iv line (see Ref. 11).
Blended with O iii line.
Table 2
Energy Levels of the Ground Configuration 5s25p2 of Xe v
Standard deviation, which is [∑ (obs. value − fitted value)2/(n − m)]1/2, where n is the number of known levels and m is the number of free parameters.
Table 4
Observed Energy Levels of 5s5p3, 5s25p5d, and 5s25p6s Configuration of Xe v
Experimental minus calculated level in inverse centimeters.
The two highest percentages are given.
Calculated value from fitted-parameter calculation.
Third-largest component.
Table 5
Energy Parameter Values (cm−1) of the 5s5ps, 5s25p5d, 5s25p6s, 5s25p6d, and 5s25p7s Configurations of Xe v