Atomic decay data for modeling K lines of iron peak and light odd-Z elements

作者:Palmeri P*; Quinet P; Mendoza C; Bautista M A; Garcia J; Witthoeft M C; Kallman T R
来源:ASTRONOMY %26 ASTROPHYSICS, 2012, 543: A44.
DOI:10.1051/0004-6361/201219438

摘要

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%26apos;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 %26gt; 9 are treated for the first time, and detailed comparisons with available measurements and theoretical data for ions with N %26lt;= 9 are carried out in order to estimate reliable accuracy ratings.

  • 出版日期2012-7