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Yagishita, A.

Paper Title Page
MOOAI7 First Observation of the 61.5 nm Seeded FEL at the SCSS Test Accelerator 13
 
  • T. Togashi, K. Fukami, S. Matsubara, H. Ohashi, H. Tomizawa, T. Watanabe
    JASRI/SPring-8, Hyogo-ken
  • M. Aoyama, K. Yamakawa
    JAEA/Kansai, Kyoto
  • M.-E. Couprie
    SOLEIL, Gif-sur-Yvette
  • T. Hara, T. Hatsui, T. Ishikawa, T.K. Kameshima, H. Kitamura, N. Kumagai, M. Nagasono, Y. Otake, T. Shintake, H. Tanaka, T. Tanaka, K. Togawa, M. Yabashi
    RIKEN/SPring-8, Hyogo
  • A. Iwasaki, T. Okino, S. Owada, T. Sato, K. Yamanouchi
    The University of Tokyo, Tokyo
  • F. Kannari
    Keio University, Kanagawa-ken
  • K. Midorikawa, E. Takahashi
    RIKEN, Saitama
  • H. Nakano
    NTT Corp., Kanagawa-ken
  • A. Yagishita
    KEK, Tsukuba
 
 

A seeded FEL is the most promised way to generate fully coherent radiation in a short-wavelength region. After the improvement of the laser and HHG system at the SCSS test accelerator, we have succeeded the amplification of the seed, for the first time, in the plateau region. The wavelength of the seed is 61.5 nm, which is the 13th harmonic of a Ti:Sa laser, and clear intensity increase and spectral narrowing by the FEL was observed. Although there still remains room for optimization of the transverse matching and synchronization of the seed, this result leads to realization of a fully coherent light source to users in VUV and soft x-ray regions.

 

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