Article ID Journal Published Year Pages File Type
9599362 Journal of Quantitative Spectroscopy and Radiative Transfer 2005 14 Pages PDF
Abstract
Most probable values of Coster-Kronig (CK) transition probabilities (S12, S13, S14, S15, S1,67, S23, S24, S2,67, S34, S35, S35, S3,67, S45 and S4,67) and Ni subshell fluorescence yields (N1, N2, N3, N4, N5 and N67) have been determined by using least-squares fitted to obtain the polynomials, which is plotted by using the McGuire's values (Phys Rev A 9(5) (1974) 1840), representing them as a function of atomic number. The Sij represents the N subshell vacancy transitions from ith subshell to jth subshell. The obtained values of Ni subshell fluorescence yields-N1, N2, N3, N4, N5, N67, and CK transition probabilities-S12, S13, S14, S15, S1,67, S23, S24, S2,67, S34, S35, S35, S3,67, S45 and S46 are presented.
Related Topics
Physical Sciences and Engineering Chemistry Spectroscopy
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