Experimental investigation of the origin of the Ti Kα″ satellites

N. Shigeoka, H. Oohashi, T. Tochio, Y. Ito, T. Mukoyama, A. M. Vlaicu, S. Fukushima

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Abstract

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.

Original languageEnglish
Article number052505
Pages (from-to)052505-1-052505-5
JournalPhysical Review A - Atomic, Molecular, and Optical Physics
Volume69
Issue number5 A
DOIs
Publication statusPublished - May 2004

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

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    Shigeoka, N., Oohashi, H., Tochio, T., Ito, Y., Mukoyama, T., Vlaicu, A. M., & Fukushima, S. (2004). Experimental investigation of the origin of the Ti Kα″ satellites. Physical Review A - Atomic, Molecular, and Optical Physics, 69(5 A), 052505-1-052505-5. [052505]. https://doi.org/10.1103/PhysRevA.69.052505