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- W1985304851 abstract "The strong x-ray line emission of n = 4→n = 3 and n = 5→n = 3 transitions of Ni-like Au has been investigated under a coronal plasma condition. A complete set of atomic data, including energy level, transition probability and collision strength, has been obtained to simulate the emission spectra. Under a typical coronal equilibrium (electron temperature of 2500 eV and density of 1.0×1015), the predicted strongest line is due to the transition of (3d3/2−14f5/2)1 → (3d10)0. Extensive studies show that the relative intensity is insensitive to temperature and density over a wide plasma condition." @default.
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- W1985304851 date "2005-07-29" @default.
- W1985304851 modified "2023-09-27" @default.
- W1985304851 title "X-Ray Emission Spectra of Ni-Like Gold Ions under Coronal Plasma Condition" @default.
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- W1985304851 doi "https://doi.org/10.1088/0256-307x/22/8/042" @default.
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