X-Ray Spectroscopy 2012
DOI: 10.5772/28882
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Analysis of the K Satellite Lines in X-Ray Emission Spectra

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“…The Ka 1 and Ka 2 lines, often just called Ka lines, refer to the radiative decay of a K-shell (1s orbital) vacancy being filled with an electron from the L 2 L 3 -shells (2p orbitals) [157]. Thus, it is dipole allowed having the highest transition probability for a 1s vacancy, leading the brightest emission in K-edge XES [154].…”
Section: Xes Backgroundmentioning
confidence: 99%
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“…The Ka 1 and Ka 2 lines, often just called Ka lines, refer to the radiative decay of a K-shell (1s orbital) vacancy being filled with an electron from the L 2 L 3 -shells (2p orbitals) [157]. Thus, it is dipole allowed having the highest transition probability for a 1s vacancy, leading the brightest emission in K-edge XES [154].…”
Section: Xes Backgroundmentioning
confidence: 99%
“…One can extend the transition rules to include also the molecular orbitals which are created by the hybridisation between the local atomic orbitals and the ligand's orbitals (see Table 2 bottom) [164]. These inter-atomic transitions will then yield information about the molecular electronic structure and the ligands involved [100,149,155,157,165,162]. Therefore we will in the following shortly introduce the so-called satellite emissions, which have first been reported by Sommerfeld and Wentzel in the early 1920s as spark lines in the X-ray spectrum [45,52,166,167].…”
Section: Xes Backgroundmentioning
confidence: 99%
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