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

Research output: Contribution to journalArticle

16 Citations (Scopus)

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
Pages (from-to)52505-52501
Number of pages5
JournalPhysical Review A
Volume69
Issue number5 A
DOIs
Publication statusPublished - May 2004

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excitation
spectrometers
energy

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics
  • Physics and Astronomy(all)

Cite this

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, 69(5 A), 52505-52501. https://doi.org/10.1103/PhysRevA.69.052505

Experimental investigation of the origin of the Ti Kα″ satellites. / Shigeoka, N.; Oohashi, H.; Tochio, T.; Ito, Y.; Mukoyama, T.; Vlaicu, A. M.; Fukushima, S.

In: Physical Review A, Vol. 69, No. 5 A, 05.2004, p. 52505-52501.

Research output: Contribution to journalArticle

Shigeoka, N, Oohashi, H, Tochio, T, Ito, Y, Mukoyama, T, Vlaicu, AM & Fukushima, S 2004, 'Experimental investigation of the origin of the Ti Kα″ satellites', Physical Review A, vol. 69, no. 5 A, pp. 52505-52501. https://doi.org/10.1103/PhysRevA.69.052505
Shigeoka, N. ; Oohashi, H. ; Tochio, T. ; Ito, Y. ; Mukoyama, T. ; Vlaicu, A. M. ; Fukushima, S. / Experimental investigation of the origin of the Ti Kα″ satellites. In: Physical Review A. 2004 ; Vol. 69, No. 5 A. pp. 52505-52501.
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