The 3s2 1S0-3s3p 3P1 magnesium sequence intercombination lines from ScX to MoXXXI observed in the PLT tokamak
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Cited by (35)
Wavelengths and E1, E2, M1, and M2 line strengths in Nb XXX
2024, Journal of Quantitative Spectroscopy and Radiative TransferExcitation energies, lifetimes, and transition data for Zr XXIX
2023, Journal of Quantitative Spectroscopy and Radiative TransferCitation Excerpt :A number of Zr XXIX lines have been identified in plasma [3–9]. The wavelengths of the 3s2 1S0-3s3p 3Po1 and 3s2 1S0-3s3p 1Po1 transitions of Zr XXIX have been measured in the Princeton Large Torus (PLT) tokamak discharges by Finkenthal et al. [3]. Besides the resonance line 3s2 1S0-3s3p 1Po1, the two lines 3s3p 1Po1-3s3d 1D2 and 3s3p 3Po2-3s3d 3D3 have been identified with a laser-produced plasma and measured with an uncertainty of ± 0.015 Å by Reader [4].
Investigation of extreme ultraviolet radiation of highly charged Mo ions from a laser-produced plasma
2021, Journal of Quantitative Spectroscopy and Radiative TransferCitation Excerpt :Spectral data from such ions are part of a rich burgeoning field of substantial applications in absorption spectroscopy [8], fusion research [9], plasma diagnostics [10], and it is also being suitable as a bright source of continuum radiation in the soft and hard x-ray region [11]. Specifically, for the highly-charged Mo ions, the spectra have of great attention because of their use for plasma diagnostics in fusion research [12–16]. Like zirconium [5], it acts as a getter for oxygen; it is also being considered as intrinsic impurities in magnetic confinement devices (MCD) and as a material for use in the interior of tokamaks [15].
Energy levels and oscillator strengths for Mg-like copper
2015, Journal of Quantitative Spectroscopy and Radiative TransferAtomic data and spectral line intensities for Ni XVII
2011, Atomic Data and Nuclear Data TablesCitation Excerpt :Lines from Ni XVII have been observed on a number of occasions in the past, both in the laboratory and in solar plasmas. Laboratory measurements from many different devices provided line wavelengths [7–15] and level lifetimes [16–19]. A host of calculations have been performed to determine the radiative transition rates of an increasingly larger number of energy levels [20–26], but calculations of collisional excitation rates have been surprisingly scarce.
Isoelectronic behavior of resonant and intercombination lines in MgI-like ions
1996, Journal of Electron Spectroscopy and Related Phenomena
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Present address: Racah Institute of Physics, The Hebrew University, Jerusalem, Israel.