XFEL Beam Dynamics Meeting 31.03.2008 Bolko Beutner, DESY First results of micro-bunching and COTR experiments at FLASH Bolko Beutner, Winfried Decking,

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Presentation transcript:

XFEL Beam Dynamics Meeting Bolko Beutner, DESY First results of micro-bunching and COTR experiments at FLASH Bolko Beutner, Winfried Decking, Torsten Limberg, and Mathias Vogt, DESY XFEL Beam Dynamics Meeting

Bolko Beutner, DESY Contents Introduction Velocity bunching Experiments at FLASH First Results –microbunching –COTR Summary and Outlook

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Introduction Micobunching instabilities are predicted to have a strong effect on FEL like XFEL or 3 rd harm. FLASH – no experiments are done at FLASH so far… Velocity bunching can be used to simulate some beam properties of the 3 rd harm. System (linear long. Phase space) ACC23 as a “knob” to turn microbunching “on and off” Microbunch structure can be used for COTR studies M. Vogt

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Goals Microbuning Instability Observation of microbunch (~ 10 um) structure on the bunch with the THz spectrometer Observation of instbilities at LOLA Studies on possible beam break up Coherent Optical Transition Radiation COTR in “microbunching mode” (OTR screens / LOLA) COTR in standard compression (OTR screens) Charge dependence

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Machine Settings RF Gun Phi = degE_max = 44 MeV/mQ=1nC ACC1.C1 Phi = degE_max = MeV/m ACC1.C2-8 Phi = degE_max = MeV/m => = MeV BC2 rho = mtheta = deglim: 15-21deg => R56= 0.149=> I = A ACC2-3 Phi = -15 degE_max = MV/m=> = MeV BC3 rho = mtheta = 4.64 deglim: deg => R56= => I = A ACC4-6 Phi = 0 degE_max = MV/m=> ca. 680 MeV velocity bunching -> ASTRA/CSRTrack Simulations by M. Vogt

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Experiments at FLASH Setup of velocity bunching (including bunch length measurements) ACC23 phase scan in microbunching mode (vb on) –LOLA –THz –OTR18ACC7 Beam Focus on OTR screens in standard comprssion (vb off) –ACC1 phase scan BC2 compression / OTR10DBC2

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Velocity Bunching 3-Stab waveguide tuners are used to shift phase offsets of single cavitites Tuner positions are taken from pre- measured curves Q of the cavities are kept within reasonable limits by tuning of the middle stab position Final phase offsets differ slightly from the intended ones but are measured with the RF probes

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Streak Camera Sychrotron radiation from the 4 th dipole in BC2 is transported to TOSYLAB via an optical beamline. A Hamamatsu streak camera is used to measure synchrotron radiation pulse length and thus the bunch length. A 540 nm±40 nm wavelength filter was used suppress resolution limitation by optical dispersion. Resolution limit expected around 1 ps. time [ps]

XFEL Beam Dynamics Meeting Bolko Beutner, DESY VB Setup Bunch length measurements to set up velocity bunching Comparison with simulated bunch length data Working point set with respect to shortest bunch length Measurements Simulations Preliminary FWHM bunch length [ps]

XFEL Beam Dynamics Meeting Bolko Beutner, DESY 18ACC7 ACC23 phase scan in “microbunching mode” -6 deg -8 deg-10 deg -12 deg-14 deg-16 deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY 18ACC7 Strong intensity increase around 13 deg off crest in ACC23 Strong fluctuations Beam size determination is hard due to spiky structure

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Beam Breakup 13.3 deg in ACC23 – 100 shots

XFEL Beam Dynamics Meeting Bolko Beutner, DESY THz Spectra Phase scan ACC23 16deg -> 14 deg in ~0.1 deg steps Strongest contribution in 8-25um range deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY “Microbunching” ? ACC1.C1 vb mode ACC1.C2-C8 -2deg ACC23 scan Strong signals in predicted “microbunchig mode” 0deg -12deg -16deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY “no microbunching”? Structure in the 8-25um range Low intensity compared to the “microbunching mode” on crest On crest Only BC2 in vb mode On crest BC2 and BC3 in vb mode ACC1 -6deg Only BC2 in vb mode

XFEL Beam Dynamics Meeting Bolko Beutner, DESY VB on and off Similar structure with and without VB Strongest THz signal at ACC23 8 deg offcrest in non vb mode (~12 deg in vb mode) Maximum signal lower than in vb mode VB off VB on ACC23 8deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Spike of Tail ? Widening of beam spike Distortion of the whole bunch Strong machine jitter complicates analysis Not completely analysed yet….

XFEL Beam Dynamics Meeting Bolko Beutner, DESY COTR in standard compression? -1deg -8deg-11deg -12deg-13deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY COTR in standard compression? deg-11.75deg deg -12.5deg deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Fluctuations ACC1 phase deg

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Summary Increased spot size at “full compression” and a peak in maximum intensity

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Transverse Structure Bright spot horizontally separated from the beam centre  Spot size?  High intensity in narrow region

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Charge Dependence Charge dependence study of OTR/COTR radiation Sharp increase of total intensity in low charge regime More flat intensity for high bunch charges –higher transverse emittance –uncorr. energy spread Similar Fluctuations in all cases

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Summary Observation of strong THz signals in predicted “microbunching mode” Transverse beam breakup in “microbunching mode” COTR radiation in “microbunching mode” Indications for COTR in standard compression Studies on charge dependence of OTR/COTR radiation

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Next Steps Further data analysis –LOLA images –Detailed analysis of the THz spectra –More detailed image analysis Simulations –Start to end simulations with all known machine parameters during the measurements –Studies on transverse beam breakup

XFEL Beam Dynamics Meeting Bolko Beutner, DESY Thank you for your Attention and Special thanks to V. Ayvazyan, M. Huening, O. Grimm, B. Schmidt, S. Wesch, C. Behrens, H. Delsim-Hashemi.