Identification of a forbidden line in Kr xxiii

Benjamin, R. D.; Terry, J. L.; Moos, H. W.

doi:10.1103/physreva.36.4504

Cited by 5 publications

(2 citation statements)

References 15 publications

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“…The levels of the ground configuration 3s 2 3p2 are determined completely by measured and interpolated Ml lines. The following transitions have been measured: 3p o _ 3 P 1 1462.65 ± 0.03 A Benjamin et al [1987] 3P 1 -3P2 3840.9 ± 0.3 A 3p 1 _I Dz 853.8 ± 1.0 A The following was predicted by plotting the observed minus calculated M1 wavelength along the isoelectronic sequence: 3p l _Is o 537.2±0.3 A Sugar et al [1990] The above values were used to derive the energy levels of the 3s 2 3p2 configuration.…”

Section: Z=36mentioning

confidence: 96%

Energy Levels of Krypton, Kr I through Kr XXXVI

Sugar

Musgrove

1991

Journal of Physical and Chemical Reference Data

120

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The energy levels of the krypton atom, in all stages of ionization for which experimental data are available, have been compiled. No data has yet been published for Kr XI through Kr XVII. For H-like krypton very accurate· calculated level values are compiled. In all, data for 29 spectra are given. Experimental g-factors are included for Krl and Kr II. Calculated percentage compositions of levels are given for 12 ions. A value for the ionzation energy of each ion, either experimental or theoretical, is included.

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Section: Z=36mentioning

confidence: 96%

Energy Levels of Krypton, Kr I through Kr XXXVI

Sugar

Musgrove

1991

Journal of Physical and Chemical Reference Data

120

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“…These rarely include the confidence level, but it is reasonable to assume that they represent at least one standard deviation of the measurements. We have previously published such compilations [1][2][3][4][5][6][7][8][9] forTi, V, Cr, Mn, Fe, Co, Ni, Cu and Mo (Z- [22][23][24][25][26][27][28][29]42). The present compilation contains data for Kr V through Kr XXXVI, except for Kr XI through Kr XVII, for which no data have been 1578 SHIRAI, OKAZAKI, AND SUGAR published.…”

Section: Introductionmentioning

confidence: 99%

Spectral Data for Highly Ionized Krypton, Kr V through Kr X X X V I

Shirai

Okazaki

Sugar

1995

Journal of Physical and Chemical Reference Data

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Wavelengths, energy levels, ionization energies, line classifications, intensities and transition probabilities for Kr v through Kr XXXVI, with the exception of Kr XI through Kr XVII, are tabulated. No data have been published for Kr Xl through Kr XVII. These data are based on the energy levels compilation of Sugar and Musgrove [13]. Transition probabilities for selected M 1 lines have been reported and are quoted here. A short review of the line identifications and wavelength measurements is given for each stage of ionization. The literature has been surveyed through February 1995.

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Calculations of energy levels, transition rates, lifetimes and Landé g factors for silicon-like Kr XXIII

Wu,

Yan,

et al. 2024

Journal of Quantitative Spectroscopy and Radiative Transfer

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Identification of a forbidden line in Kr xxiii

Cited by 5 publications

References 15 publications

Energy Levels of Krypton, Kr I through Kr XXXVI

Energy Levels of Krypton, Kr I through Kr XXXVI

Spectral Data for Highly Ionized Krypton, Kr V through Kr X X X V I

Calculations of energy levels, transition rates, lifetimes and Landé g factors for silicon-like Kr XXIII

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