1976
DOI: 10.1088/0031-8949/14/6/005
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Structure hyperfine de la transition 2S1/2-2P1/2 de Hg II (γ=194,2 nm)

Abstract: The hyperfine structure of the 194.2 nm line of Hg II has been studied by Fabry-Pérot interferometry. The A-factors for the odd isotopes have been determined for the levels 2 S 1/2 and 2 P 1/2 and the shifts for the different isotopes in the natural mercury line have been measured.

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Cited by 27 publications
(11 citation statements)
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“…The Sqy2 (F = 1) state is detected by exciting the Szyq (F = 1)~Pqy2 (F = 0) transition with laser 1. ting has been measured by microwave resonance methods to be 40.507 347 996 9(3) GHz [24]. The Piyz hyperfine splitting has been measured by Fabry-Perot interferometry to be 6.955(90) GHz [25). The natural linewidth of the Piyz state is about 70 MHz [26,27].…”
Section: Amentioning
confidence: 99%
“…The Sqy2 (F = 1) state is detected by exciting the Szyq (F = 1)~Pqy2 (F = 0) transition with laser 1. ting has been measured by microwave resonance methods to be 40.507 347 996 9(3) GHz [24]. The Piyz hyperfine splitting has been measured by Fabry-Perot interferometry to be 6.955(90) GHz [25). The natural linewidth of the Piyz state is about 70 MHz [26,27].…”
Section: Amentioning
confidence: 99%
“…Additional isotope shifts were given by Shorthill and Fowles [6]. Accurate interferometric measurements for 4 lines of Hg II were reported by Burns and Adams [7], and the detailed structure of the 1942 Ð line was studied using Fabry-Perot interferometry by Guern et al [8] and using laser spectroscopy by Hemmati, Bergquist, and Itano [9].…”
Section: Introductionmentioning
confidence: 93%
“…The levels reported at 92566 cm À1 , 104036 cm À1 , 106612 cm À1 , and 110603 cm À1 were rejected as spurious, and the J values of the levels at 97094 cm À1 , 100859 cm À1 , and 111172 cm À1 were revised. Three undesignated AEL levels at 106086 cm À1 , 106213 cm À1 , and 121960 cm À1 were found 5d 10 7p 2 P 3/2 -5d 10 7d 2 D 3/2 5d 10 7d 2 D 5/2 -5d 10 7f 2 F 7/2 5d 10 7p 2 P 1/2 -5d 10 8s 2 S 1/2 5d 10 8p 2 P 1/2 -5d 10 9d 2 D 3/2 5d 10 7s 2 S 1/2 -5d 10 7p 2 P 1/2 5d 10 8p 2 P 3/2 -5d 10 9d 2 D 5/2 5d 9 6s6p ( 2 D 3/2 , 1 P 1 ) 5/2 -5d 10 5g 2 G 7/2 5d 10 5f 2 F 7/2 -5d 10 5g 2 G 9/2 5d 10 7s 2 S 1/2 -5d 9 6s6p ( 2 D 5/2 , 1 P 1 ) 3/2 5d 10 5f 2 F 5/2 -5d 10 (7) 3.8 (7) 8.6 (7) 5.9 (7) 1.6 (8) 7.2 (8) 2.9 (7) 4.1 (8) a Wavelengths shorter than 2000 Ð are in vacuum. Wavelengths longer than 2000 Ð are in standard air.…”
Section: D 9 6s6p Con¢gurationmentioning
confidence: 99%
“…The nuclear magnetic moments are taken from [22] unless noted otherwise. The results for the last [23,24], 137 Ba + [25][26][27], 201 Hg + [28], 210 Fr (µ = 4.38(5)µB ) [29,30], 211 Ra + (µ = 0.878(4)µB ) and 213 Ra + (µ = 0.613(2)µB ) [31][32][33]. Theory values for Cs and Fr are from [20].…”
Section: Introductionmentioning
confidence: 99%