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Kawasaki, S.; Kobayashi, T.; Sakamoto, K.; Kishimoto, Y.; Watanabe, A.; Musyoki, S.; Oda, H.; Tokuda, S.; Nakamura, Y.
Beams 92: Proceedings. Volume 1: Invited papers, pulsed power1993
Beams 92: Proceedings. Volume 1: Invited papers, pulsed power1993
AbstractAbstract
[en] An experiment of Raman mm wave FEL was carried out using a planar focusing wiggler and an additional axial magnetic field. An IREB (0.9 MeV, 2 kA, 100 ns) was generated by a field emission gun driven with inductive acceleration units and flowed into the wiggler. The beam transmission up to 85% through the whole wiggler length(1.5 m) was realized at its best, though the axial magnetic field was kept very low. The particle orbits in the wiggler were to be in the open-quotes group Iclose quotes. There appeared a pattern showing effect of higher modes of the resonance between the electron cyclotron frequency in the axial field and the frequency associated with the wiggler field. The results were compared with the simulation made by a newly developed code. Strong superradiant emission was found in several sharp peaks with a very narrow width, separated by 6-8 GHz in the frequency spectrum in the range between 30-65 GHz. The radiation power as well as the spectrum were correlated to the radial distribution of the particles in the cross section of the beam. At the amplifier mode of the FEL operation, rf pulse of 45 GHz was injected at the entrance of the wiggler, and amplified along the beam flowing in the wiggler from the power level of 100 W at the input, to finally 6 MW at the saturated state, at a spatial growth rate of 50-56 db/m. The amplification process observed was also consistent with the analyses by 3D simulations
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Mosher, D.; Cooperstein, G. (Naval Research Lab., Washington, DC (United States)) (eds.); Maryland Univ., College Park, MD (United States); 704 p; 1993; p. 255-262; 9. international conference on high power particle beams; Washington, DC (United States); 25-29 May 1992; Also available from OSTI as DE94014783; NTIS; US Govt. Printing Office Dep
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