Probe beam distortion in TBTS due to high gradient RF acceleration (first part: observations) CTF3/TBTS Logbook 17 May 2013 Wilfrid Farabolini – Alexej.

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Presentation transcript:

Probe beam distortion in TBTS due to high gradient RF acceleration (first part: observations) CTF3/TBTS Logbook 17 May 2013 Wilfrid Farabolini – Alexej Grudiev 29 May 20131CLIC RF meeting

Beam observed on MTV0790 Beam kicks during acceleration have been observed from a long time, especially when the beam is passing off-axis through the 12 GHz structures. In addition of beam kick it appears that the beam shape can also be distorted after the 12 GHz structure when powered. Horizontal beam kick when scanning the horizontal positions within the ACSs Non-accelerated (left) and accelerated (right) beam shapes observed on the straight line screen, 4.75 m downstream the ACS Hor. Position [mm] accelerated non accelerated 29 May 20132RF meeting [mm] Vert. Pos.

Beam transport settings 29 May 2013RF meeting3 Transverse envelope model The only used triplet Beam size check Structures position Screen position With all quads off: structure shadowed beam (here not perfectly aligned) 4.7 m7.6 m

For transverse kick measurements beam can off course be much better focused 29 May 2013RF meeting4 And also beam loading evidence with high bunch charge

Beam shape observation To fully observe beam shape distortion we have used a non focused beam that covers the full structure aperture (4.7 mm bore diameter on the output side). Large beam shadowed by the structure, non accelerated (left) and accelerated (right) Similar shape can be observed in the spectrum line on MTV830 when energy spread is low (here on deceleration crest) 29 May 20135RF meeting

Beam shape characterization The octupolar-like beam shape evolves with the accelerating gradient but also with the accelerating phase (phase between probe beam and 12 GHz RF) For very weak RF power (few MWs, uncertain phase) At zero-crossing (rising RF power side), 25 MW At zero-crossing (falling RF power side), 25 MW 29 May 20136RF meeting

Phase scan from -110 to -10 deg (poor linearity of the phase shifter in this range) Close to decelerating crest 29 May 20137RF meeting

For accelerating phase from 10 to 98 deg On accelerating crest Close to zero-crossing (left side of accelerating crest) 29 May 20138RF meeting

For accelerating phase from 118 to 218 deg On zero-crossing (right side of accelerating crest) 29 May 20139RF meeting

For accelerating phase from 238 to 318 deg On decelerating crest Close to zero-crossing (left side of accelerating crest) 29 May RF meeting

Energy gain and beam shape as function of accelerating phase The octupolar beam shape changes from positive to negative at the RF crest phases. Note: phase shifter is not linear in the lower 20 deg range (at 3 GHz) corresponding to 80 deg range at 12 GHz. 29 May RF meeting

Problem of the octopus shape on crests On crest phases, octupolar components should compensated one each other, so why we observe their addition on the screen ? Possible effect of multi bunch with phase jitter or of the bunch length (15 ps FWHM: 61 deg) ? 29 May 2013RF meeting12 15 ps On crest energy spectrum At zero crossing energy spectrum

Summary and follow-up We have observed an octupolar transverse effect on the beam during 12 GHz acceleration that should be explained with model (achieved by Alexej, see following talk). We have shown that this transverse effect evolves with the accelerating phase and is a fundamental mode of the structure (12 GHz). Many other parameters should also be investigated during a next run (bunch number, bunch length, phase between the 2 accelerating structures, RF power). 29 May RF meeting