WEOB —  Seeded FEL   (24-Aug-11   10:30—12:00)
Chair: M. Ferrario, INFN/LNF, Frascati (Roma), Italy
Paper Title Page
WEOBI1
FEL Commissioning at FERMI@Elettra  
 
  • E. Allaria, P. Craievich, S. Di Mitri, W.M. Fawley, L. Fröhlich, G. Penco, C. Spezzani, M. Trovò
    ELETTRA, Basovizza, Italy
  • G. De Ninno, S. Spampinati
    University of Nova Gorica, Nova Gorica, Slovenia
  • L. Giannessi
    ENEA C.R. Frascati, Frascati (Roma), Italy
 
  The FERMI@Elettra Free Electron Laser (FEL) produced the first coherent photons in December 2010 at the end of the first commissioning phase. Starting from February 2011 the commissioning has continued, leading to an improvement of the FEL performance. In agreement with to the design, FEL-1, the first of the two FERMI free electron lasers, has been producing coherent FEL pulses in the 60 to 20 nm wavelength range. Benefits of the seeded scheme adopted for FERMI have been immediately evident also in the case of a non-optimized electron beam.  
slides icon Slides WEOBI1 [4.528 MB]  
 
WEOB3
Seeding Experiments at SPARC  
 
  • M. Labat, F. Briquez, M.-E. Couprie
    SOLEIL, Gif-sur-Yvette, France
  • D. Alesini, M. Bellaveglia, M. Castellano, E. Chiadroni, G. Di Pirro, A. Drago, M. Ferrario, L. Ficcadenti, A. Gallo, G. Gatti, A. Ghigo, E. Pace, B. Spataro, C. Vaccarezza
    INFN/LNF, Frascati (Roma), Italy
  • A. Bacci, V. Petrillo, A.R. Rossi, L. Serafini
    Istituto Nazionale di Fisica Nucleare, Milano, Italy
  • M. Bougeard, B. Carré, D. Garzella
    CEA/DSM/DRECAM/SPAM, Gif-sur-Yvette, France
  • A. Cianchi
    Università di Roma II Tor Vergata, Roma, Italy
  • F. Ciocci, G. Dattoli, M. Del Franco, L. Giannessi, A. Petralia, M. Quattromini, C. Ronsivalle, E. Sabia, I.P. Spassovsky, V. Surrenti
    ENEA C.R. Frascati, Frascati (Roma), Italy
  • L. Cultrera
    CLASSE, Ithaca, New York, USA
  • D. Filippetto
    LBNL, Berkeley, California, USA
  • F. Frassetto, L. P. Poletto
    LUXOR, Padova, Italy
  • G. Lambert
    LOA, Palaiseau, France
  • G. Marcus, J.B. Rosenzweig
    UCLA, Los Angeles, California, USA
  • M. Migliorati, A. Mostacci, L. Palumbo
    Rome University La Sapienza, Roma, Italy
  • J.V. Rau
    ISM-CNR, Rome, Italy
  • M. Serluca
    INFN-Roma, Roma, Italy
  • C. Vicario
    PSI, Villigen PSI, Switzerland
 
  The SPARC FEL amplifier has been configured as a single stage HGHG FEL with a modulator and a radiator operating at the second harmonic. The HGHG cascade has been seeded with harmonics generated in a gas cell where a Ti:Sa laser pulse of 120 fs of duration is converted into higher harmonics. The cascaded FEL configuration obtained by tuning the undulator gaps has been studied by varying the number of modulators and radiators to optimize the conversion efficiency. The process of harmonic generation in a free electron laser operating in superradiant regime has been also analysed. Harmonic generation is expected to be efficient because of the quasi steady-state distribution of the e-beam phase space predicted in this regime. Harmonics up to the 11th have been experimentally observed.  
slides icon Slides WEOB3 [5.198 MB]  
 
WEOB4
Demonstration of High Harmonics from Echo-enabled Harmonic Generation with Small Energy Modulation  
 
  • D. Xiang
    SLAC, Menlo Park, California, USA
 
  Funding: This work was supported by the US DOE under Contract No. DE-AC02-76SF00515.
5th harmonic from EEHG has been observed at SLAC's NLCTA [1], yet with energy modulation amplitudes about 80 times larger than beam slice energy spread. While the experiment demonstrated that long-term memory of phase space correlations could be preserved, it was incapable of providing insight into the underlying physics of EEHG that high harmonics can be generated with small energy modulation. Here we report generation of the 7th harmonic from EEHG technique in realistic scenarios where the laser energy modulation is comparable to the beam slice energy spread. The experiment demonstrates the supreme up-frequency conversion efficiency of EEHG technique and indicates that scaling to X-ray wavelength may be possible.
[1] D. Xiang et al., Phys. Rev. Lett, 105, 114801 (2010).
 
slides icon Slides WEOB4 [0.981 MB]