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Shevchenko, O.A.

Paper Title Page
TUPP040 Predicted Parameters of the Second Stage of High Power Novosibirsk FEL
 
  • A.V. Kuzmin, O.A. Shevchenko, N. Vinokurov
    BINP SB RAS, Novosibirsk
 
 

The first stage of Novosibirsk high power terahertz FEL was successfully put into operation in 2003 [1]. The measured parameters of the FEL turned out to be in a good agreement with calculations [2]. The second and the third stages of the FEL are under construction now. The beam energy at the second stage will be about 20 MeV and the wavelength will change in the range 40-80 μm. In this paper we present the design parameters for the second stage FEL. The simulations were carried out with the help of 1-D code based on macroparticles. This code was previously used for the first stage simulations [2].

[1] Antokhin E.A. et al. NIM A528 (2004) p.15-18. [2] Kuzmin A.V., Shevchenko O.A., Vinokurov N.A. NIM A543 (2005) p.114-117.

 
   
WEOA003 First Lasing and Initial Operation of a Circularly Polarized Optical Klystron OK-5 FEL and a Variably Polarized Distributed Optical Klystron DOK-1 FEL at Duke 407
 
  • Y.K. Wu, J. Li, S. Mikhailov, V. Popov
    DU/FEL, Durham, North Carolina
  • N. Gavrilov, G. Kulipanov, O.A. Shevchenko, N. Vinokurov, P. Vobly
    BINP SB RAS, Novosibirsk
 
 

Funding: This work is supported by the U.S. AFOSR MFEL grant F49620-001-0370 and by U.S. DOE grant DE-FG05-91ER40665.

To improve the capability and performance of its light sources, the Duke FEL lab (DFELL) is upgrading its storage ring based FEL by replacing the existing linearly polarized OK-4 FEL with the next generation OK-5 FEL which is capable of delivering both linearly and circularly polarized light. To reduce and manage the risk associated with this project, the FEL upgrade is carried out in three phases. In the second phase of upgrade in 2005, two OK-5 wigglers are installed in a specially designed lattice where OK-4 wigglers remain, forming a distributed optical klystron FEL with hybrid wiggler magnets. In this paper, we report our commissioning experience of this distributed optical klystron FEL, including its first lasing in visible wavelengths and measured lasing spectra and power. We will also present our first experimental results on the FEL polarization manipulation using OK-4 and OK-5 wigglers. In addition, we report the performance enhancement of the Compton gamma-ray source driven by this FEL and initial FEL operation experience for user applications.