The origin of the Ti Kα″ satellite was discussed. A Johann-type spectrometer on the BL15XU undulator beam line of SPring-8 at excitation energies between 4996 and 7000 eV was used for the purpose. It was found that at an excitation energy of 5010 eV, the intensity of the Kα″ satellite exhibited a jump from 0% to ∼1% in a range of 10 eV. The results show that the Kα″ satellite originated from a 3p spectator hole.
|Journal||Physical Review A - Atomic, Molecular, and Optical Physics|
|Issue number||5 A|
|Publication status||Published - May 2004|
ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics