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Simulations for the HXRSS experiment with the 40 pC beam

Simulations for the HXRSS experiment with the 40 pC beam. S. Spampinati, J.Wu, T.Raubenhaimer Future light source March , 2012. Presentation aims. Comments on simulations vs experiments Derive model of pulse evolution in SASE and seeded undulator from experimental observation

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Simulations for the HXRSS experiment with the 40 pC beam

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  1. Simulations for the HXRSS experiment with the 40 pC beam S. Spampinati, J.Wu, T.Raubenhaimer Future light source March, 2012

  2. Presentation aims • Comments on simulations vs experiments • Derive model of pulse evolution in SASE and seeded undulator from experimental observation • Benchmark with start to end simulations • Try ideal simulations model to match with experiment • Try to understand seeding efficiency and match with simulations • Focus on • Pulse characteristic in the SASE undulator • Pulse characteristic in the seeded undulator • Seed used power

  3. Comments on simulations vs experiments • Start to end simulation are a guidance • Some beam parameter (current beam profile) can be measured, even if indirectly, to confirm simulations • Only few accelerator configurations and beams can be simulated completely • Accelerator and beam change from shift to shift and from shot to shot • Ideal models can be used to catch physics

  4. Measurements of current of fs beam profile beam energy spectrometer (Z.Huang, K.Bane, Y.Ding, and P Emma,Phys. Rev. ST Accel. Beams 13, 092801 (2010) ) • The beam measured is not exactly the beam in the undulator but 1-1 correspondence exists • The beam profile change from shot to shot 24/1/2012 R. Iverson, H. Loos, Z. Huang, H.-D. Nuhn, Y. Ding, J. Wu, S. SpampinatiT.O. Raubenheimer,

  5. Pulse in the SASE undulator • Measured quantity: 2.5m gain lengthand ≈20 µJ at crystal • Short length with low energy: short pulse length • Back extrapolation of measured power: Considering a shot noise power of some KW the pulse length should be shorter then fs • Start to end simulation confirm very short pulse formation • 3.7 m gain length, energy ≈5µJ. Than we try simulations with a beam more bright

  6. SASE undulator (U 3-15) with a more brighterbeam • Beam parameter: energy spread 4 MeV, emittance 0.40. • Energy at crystal ~20µJ in very narrow pulses, gain length 3.1 m

  7. Evolution of the pulse in the seeded undulator Seed energy Letargy • Energy along seeded undulator (active length on x) • Fitting the data with exponential curve • gain length can be short like 3.5 m • 3.5 lethargy length • Amplified energy is around 1 nJ considering interaction from the start • If the seed peak power is of the order of MW the FEL pulse length • is <= 1fs (is gain length measurement in the seeded part correct?)

  8. Evolution of the pulse in the seeded undulator (continue) • experimental spectral relative bandwidth FWHM 8-5*10^-5 • (FWHM PULSE DURATION)* (FWHM PULSE DURATION)=0.44 • 2.8-4*fs FWHM pulse duration for a Gaussian Fourier transform pulse • Lasing from a small part of the beam or chirp on the FEL pulse. • FEL pulse longer then 2.8 fs Then considering a gain length of 3.5 m the seed power is more like 0.2-0.3 MW. This level of power prevent • saturation even for such short gain length. • FEL pulse in the second undulator is longer than the SASE in the first • undulator

  9. Seeded undulator start to end simulation Different colors for different tapering • For the optimum detuning of the second undulator the core starts • to contribute to the pulse energy and this produce the shorter gain length • Gain length 5 m • Starting from 2MW seed power production of ≈250µJ

  10. Simulation with high current beam • Wakes in the undulator no chirp • Gain length 5 m • Lasing on all the beam • Same detuning of the second undulator for narrow spectrum maximum energy • Seems very difficult to have gain length shorter than 5m

  11. Lasing from horns in the SASE undulators. Then the core starts to lase • even if the horns still dominate • High current in the horn reduces gain length in the SASE undulator. • It seems, from the experiments, that the Horns are very bright • Shorter Gain length in the experiment shorter than the simulated one • The shorter seed gain length observed in the experiments (<5m) requires a seed power below 0.2 MW • Gain length ≈ 5m is more compatible with MW level seed power

  12. END

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