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NASA NTRS · 20150000165

Atomic Decay Data for Modeling K Lines of Iron Peak and Light Odd-Z Elements*

Abstract

Complete data sets of level energies, transition wavelengths, A-values, radiative and Auger widths and fluorescence yields for K-vacancy levels of the F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn isonuclear sequences have been computed by a Hartree-Fock method that includes relativistic corrections as implemented in Cowan's atomic structure computer suite. The atomic parameters for more than 3 million fine-structure K lines have been determined. Ions with electron number N greater than 9 are treated for the first time, and detailed comparisons with available measurements and theoretical data for ions with N less than or equal to 9 are carried out in order to estimate reliable accuracy ratings.

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BibTeXRIS

Palmeri, P., Quinet, P., Mendoza, C., Bautista, M. A., Garcia, J., Witthoeft, M. C., Kallman, T. R.. 2012-06-25. Atomic Decay Data for Modeling K Lines of Iron Peak and Light Odd-Z Elements*. https://ntrs.nasa.gov/citations/20150000165

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