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Chubar, O.V.

Paper Title Page
WEOD03 Spatial Characterization of FEL Self-Amplified Spontaneous Emission 702
 
  • P. Mercère, R. Bachelard, M.-E. Couprie, M. Idir
    SOLEIL, Gif-sur-Yvette
  • S. Bucourt, G. Dovillaire, X. Levecq
    Imagine Optic, Orsay
  • O.V. Chubar
    BNL, Upton, Long Island, New York
  • J. Gautier, G. Lambert, P. Zeitoun
    LOA, Palaiseau
  • T. Hara, A. Higashiya, T. Ishikawa, M. Nagasono, M. Yabashi
    RIKEN/SPring-8, Hyogo
  • H. Kimura, H. Ohashi
    JASRI/SPring-8, Hyogo-ken
 
 

The VUV Self-Amplified Spontaneous Emission of the SPring-8 Compact SASE Source (SCSS) Test Accelerator is characterized at different stages of amplification up to saturation [1]. Experimental measurements are performed by use of a VUV Hartmann wavefront sensor. This kind of sensor gives access to both intensity and phase profiles of the incoming beam. We characterize the mode selection when approaching the saturation regime of the FEL. Optical quality of the saturated SASE radiation is measured to be better than Lambda/5 PV and Lambda/22 rms (Lambda = 61.5 nm) depending on the machine optimization. Moreover, pointing of the beam as well as spatial structure, size and position of the source are retrieved and their shot-to-shot fluctuations investigated. Analytical [2] and numerical calculations [3], using SRW and GENESIS codes, show good agreement with the experimental measurements. All these elements are of crucial importance for a better understanding and optimization of the FEL and of course for user applications requiring a stable focused beam on their samples. We are grateful to the SCSS Test Accelerator Operation Group at RIKEN for continuous support in the course of the studies


[1] R. Bachelard et al., "Wavefront and Transverse Structure of the FEL Self-Amplified Spontaneous Emission", to be submitted
[2] M. Xie, NIMA 445, 59(2000)
[3] O. Chubar et al., Proc. EPAC-98, 1177(1998)

 

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