14–17 Sept 2015
MCEC
Australia/Melbourne timezone

Fully Intensity and Timing Jitter Compensated Ultra-Fast Experiments at Accelerator-Driven Photonsources at High Repetition Rates

14 Sept 2015, 15:00
20m
MCEC

MCEC

1 Convention Centre Place, South Wharf VIC 3006, Australia
Contributed Oral Time Resolved Diagnostics and Synchronization MOCLA

Speaker

Sergey Kovalev (HZDR)

Description

Timing jitter and power instabilities are crucial parameters which greatly reduce the applicability of accelerator driven light sources for time-resolved experiments. In this contribution we present a technique that allows achieving few 10 fs time-resolution in experiments operating at cw repetition rates of up to 100 kHz by employing high repetition rate data acquisition. The method employs a fs-level arrival time monitor based on electro-optic sampling* ** of residual pulses from a coherent diffraction radiator and a fast THz detector allowing for pulse to pulse detection of arrival time and pump intensity. The monitor can operate at high repetition rates cw (presently up to a few 100 kHz) and low electron bunch charges (sub pC). The prototype device has been tested at the quasi CW SRF accelerator (ELBE) by performing an ultra-fast THz driven magnetization dynamics experiment***. Our method has high potential to provide few fs level timing on next generation large scale X-ray photon sources based on high repetition rate electron accelerators such as LCLSII. A demonstrator aiming at operation up to 4.7 MHz is under development for the European X-FEL. Footnotes * Z. Jiang, X. C. Zhang, IEEE Journal of Quantum Electronics, 36, 1214, 2000 ** I. Wilke et al., Phys. Rev. Lett., 88, 124801, 2002. *** S. Kovalev et. al., under review (2015).

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