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Abstracts Brochure - CERN

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THOPA01<br />

THOPA02<br />

THOPA03<br />

29-Jun-06 11:30 - 12:30 THOPA — Synchrotron Light Sources and FELs<br />

THOPA — Synchrotron Light Sources and FELs<br />

Formation of Electron Bunches for Harmonic Cascade X-ray Free Electron Lasers<br />

M. Cornacchia, S. Di Mitri, G. Penco (ELETTRA) P. Emma, G.V.<br />

Stupakov (SLAC) A. Zholents (LBNL)<br />

A relatively long electron bunch is required<br />

for an operation of harmonic cascade free<br />

electron lasers (FELs). This is because they<br />

repeatedly employ a principle when the ra-<br />

diation produced in one cascade by one group of electrons proceeds ahead and interacts with other electrons from<br />

the same electron bunch in the next cascade. An optical laser is used to seed the radiation in the first cascade. Understandably<br />

the length of the electron bunch in this situation must accommodate the length of the x-ray pulse multiplied<br />

by a number of cascades plus a time jitter between the arrival time of the electron bunch and a seed laser pulse. Thus<br />

a variation of the peak current along the electron bunch as well as slice energy spread and emittance may affect the<br />

performance of the FEL. In this paper we analyze all possible sources affecting the distributions and interplay between<br />

them and show how desirable distributions can be produced. Results are illustrated with simulations using particle<br />

tracking codes.<br />

Status of the SCSS Test Accelerator and XFEL Project in Japan<br />

Construction of the SCSS* 250 MeV test ac-<br />

T. Shintake, T. Ishikawa, H. Kitamura (RIKEN Spring-8 Harima) celerator was completed in October 2005, and<br />

the beam commissioning was started in November<br />

2005. The first light at visible wavelength, which is the spontaneous radiation from undulator, was observed<br />

right after machine commissioning. We expect the first SASE beam around 60 nm in 2006. The purpose of the test<br />

accelerator is to assemble all hardware components in a real machine, and check their performance, reliability and<br />

stability. It is also very important to build all control software and link to the main frame to see system performance.<br />

All experience will provide feedback to 8 GeV XFEL design, whose construction will start in April 2006.<br />

*http://www-xfel.spring8.or.jp<br />

An Integrated Femtosecond Timing Distribution System for XFELs<br />

J. Kim, J. Burnham, dc. Cheever, J. Chen, F.X. Kaertner (MIT) M.<br />

Ferianis (ELETTRA) F.O. Ilday (Bilkent University) F. Ludwig, H.<br />

Schlarb, A. Winter (DESY)<br />

Tightly synchronized lasers and rf-systems<br />

with timing jitter in the few femtoseconds<br />

range are an important component of future<br />

x-ray free electron laser facilities. In this paper,<br />

we present an optical-rf phase detector<br />

that is capable of extracting an rf-signal from an optical pulse stream without amplitude-to-phase conversion. Extraction<br />

of a microwave signal with less than 10 fs timing jitter (from 1 Hz to 10 MHz) from an optical pulse stream<br />

is demonstrated. Scaling of this component to sub-femtosecond resolution is discussed. Together with low noise<br />

mode-locked lasers, timing-stabilized optical fiber links and compact optical cross-correlators, a flexible femtosecond<br />

timing distribution system with potentially sub-10 fs precision over distances of a few kilometres can be constructed.<br />

Experimental results on both synchronized rf and laser sources will be presented.<br />

*A. Winter et al. "Synchronization of Femtosecond Pulses", Proceedings of FEL 2005.**J. Kim et al. "Large-Scale<br />

Timing Distribution and RF-Synchronization for FEL Facilities", Proc. of FEL 2004.<br />

378 Chair: A.F. Wrulich (PSI, Villigen)

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