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Coherent Synchrotron Radiation studies at the A0 photoinjector

Coherent Synchrotron Radiation studies at the A0 photoinjector. Jayakar Charles Tobin Thangaraj & the A0 team. Outline of the talk. Introduction Coherent Synchrotron Radiation Detection and characterization of radiation Studies on the electron beam

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Coherent Synchrotron Radiation studies at the A0 photoinjector

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  1. Coherent Synchrotron Radiation studies at the A0 photoinjector Jayakar Charles Tobin Thangaraj & the A0 team

  2. Outline of the talk Introduction Coherent Synchrotron Radiation • Detection and characterization of radiation • Studies on the electron beam • Impact on accelerator operation Conclusions

  3. Coherent Synchrotron Radiation • Synchrotron radiation is the result of individual electrons that randomly emit photons when passing through a bending magnet. • Coherent synchrotron radiation (CSR) is produced when a group of electrons collectively emit photons in phase. This occurs when bunch length is shorter than radiation wavelength.

  4. Why is it important? • CSR induces an energy redistribution along the bunch. • This energy modulation inside the dipole may result in modulation of the transverse slopes which may increase the projected emittance in the bend plane R Coherent radiation forlr > sz R=Lo/q q

  5. Condition for coherent radiation

  6. The A0 beamline 3.9 GHz cavity (on/off) D4 D2 D3 XS4 1.3 GHz booster cavity Collecting Optics D1 Coherent Synchrotron light Pyrodetector =quadrupole =dipoles =diagnostics

  7. Long wavelength cutoff due to vacuum chamber

  8. CSR effect on the bunch is….

  9. CSR : Measurements • Power • Polarization • Angular Distribution • Using CSR as a bunchlength monitor

  10. What to expect ? Some estimates…

  11. Chirp maths: • We expect maximum CSR power around 40 deg off crest.

  12. CSR Power Vs RF Phase (bunchlength)

  13. Polarizer angle vs CSR

  14. CSR Angular distribution Ratio (Horizontal to vertical) = 4.6

  15. Bunch length measurement: ExperimentalSetup 3.9 GHz cavity (off) D4 D2 D3 XS4 1.3 GHz booster cavity Collecting Optics D1 Synchrotron light Martin - Puplett Interferometer =quadrupole =dipoles =diagnostics

  16. Bunch length measurement: Simulation Vs Experiment

  17. Studying the effects of CSR on the beam D4 D2 D3 D1 screen Skew quad =quadrupole =dipoles =diagnostics

  18. “Skewed” maths

  19. “Skewed” maths So, with skew quad on, (after cancelling x-dispersion), what we see on the screen is,

  20. Twin pulse 10.2 ps 3.1ps 2.6ps

  21. Twin pulse Profile @X24 vsSkewQuad

  22. Twin pulse Profile @X24 vsSkewQuad X Skew Quad off Y

  23. Skew quad diagnostic to resolve CSR effects Skew QUAD OFF Skew QUAD ON (a) (c) CSR ON CSR OFF (d) (b)

  24. Skew quad measurements at X24 Skew QUAD OFF Skew QUAD ON Charge 300pC X (pixels) Charge 600pC Charge 900pC Y (pixels)

  25. Operations

  26. Nominal operation: Minimum energy spread Pick 9-cell phase to cancel this term. If 9-cell phase is -1/R56, this term will vanish 3.9 GHz cavity ON D4 D2 D3 XS4 1.3 GHz booster cavity D1

  27. Pyroscan with and without RF chirp No chirp Chirp • Signal increases ~ by a factor of 2

  28. Interferometer measurement Bunch length reduction ~ 2

  29. Summary • Coherent synchrotron radiation has been measured at A0 for various different charges • Power, polarization and angular distribution of CSR have been measured. CSR diagnostics. • Skew quad has been used to look at CSR effects. • ‘Chirp mode’ with EEX shows pulse compression. Operational for diagnostics testing.

  30. Thanks to… • Randy Thurman-Keup • Amber Johnson • Jinhao Ruan • Alex Lumpkin • James Santucci • Helen Edwards • Mike Church • Philippe Piot • Yin-E Sun • Timothy Maxwell • All the A0 techs….

  31. Few references • M. Cornacchia and P. Emma, Phys. Rev. ST Accel. Beams 5, 084001 (2002). • J. Ruan, A. S. Johnson, A. H. Lumpkin, R. Thurman-Keup, H. Edwards, R. P. Fliller, T. Koeth, and Y.-E Sun, Phys. Rev. Lett. 106, 244801 (2011). • P. Emma, Z. Huang, and K.-J. Kim, and P. Piot, Phys. Rev. ST Accel. Beams 9, 100702 (2006). • Y. S. Derbenev, J. Rossbach, E. L. Saldin, and V. D. Shiltsev, DESY FEL Report No. TESLA-FEL 95-05, 1995 • K. Bertsche, P. Emma, O. Shevchenko “A simple, low cost longitudinal phase space diagnostic”, SLAC-PUB-13614

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