Volume 410, Number 1, October IV 2003
|Page(s)||359 - 364|
|Section||Atomic, molecular, and nuclear data|
|Published online||17 November 2003|
Modeling of iron K lines: Radiative and Auger decay data for –*
NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USA
2 Centro de Física, Instituto Venezolano de Investigaciones Científicas (IVIC), PO Box 21827, Caracas 1020A, Venezuela
Corresponding author: T. R. Kallman, firstname.lastname@example.org
Accepted: 8 August 2003
A detailed analysis of the radiative and Auger de-excitation channels of K-shell vacancy states in Fe ii–Fe ix has been carried out. Level energies, wavelengths, A-values, Auger rates and fluorescence yields have been calculated for the lowest fine-structure levels populated by photoionization of the ground state of the parent ion. Different branching ratios, namely K/K, Kβ/Kα, KLM/KLL, KMM/KLL, and the total K-shell fluorescence yields, , obtained in the present work have been compared with other theoretical data and solid-state measurements, finding good general agreement with the latter. The K/K ratio is found to be sensitive to the excitation mechanism. From these comparisons it has been possible to estimate an accuracy of ~10% for the present transition probabilities.
Key words: atomic data / atomic processes / techniques: spectroscopic
© ESO, 2003
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