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High-gradient C-band linac for a compact x-ray free-electron laser facility

Authors :
T. Inagaki
C. Kondo
H. Maesaka
T. Ohshima
Y. Otake
T. Sakurai
K. Shirasawa
T. Shintake
Source :
Physical Review Special Topics. Accelerators and Beams, Vol 17, Iss 8, p 080702 (2014)
Publication Year :
2014
Publisher :
American Physical Society, 2014.

Abstract

An electron linac using a C-band rf frequency, 5.712 GHz, has enabled us to obtain an acceleration gradient of more than 35 MV/m reliably. A C-band accelerator system has been developed and constructed for the compact x-ray FEL facility, SACLA, in order to fit within the available site length at SPring-8, and to reduce construction costs. An accelerator unit consists of two 1.8 m-long accelerator structures, a cavity-type rf pulse compressor and a 50 MW pulsed klystron. In order to achieve a compact rf source and to obtain extremely stable rf fields in the accelerator structures, an oil-filled, high-voltage pulse modulator combined with an extremely stable, inverter-type, high voltage charger was developed. SACLA uses 64 sets of these accelerator units in order to achieve a final beam energy of 8.5 GeV. After rf conditioning for 1 700 hours, the maximum acceleration gradient achieved was 38 MV/m. The typical trip rate for each accelerator unit at 35 MV/m and 30 pps is about once per day. Dark current from the accelerator structures is less than 5 pC, which causes a negligible effect on the beam monitors. The phase and amplitude stability of the rf fields were measured to be 0.03 degree and 0.01% rms, respectively, which is sufficient for the XFEL operation of SACLA. Since the first beam commissioning in 2011, the C-band accelerator has demonstrated fairly stable performance under continuous operation for 20 000 hours.

Details

Language :
English
ISSN :
10984402
Volume :
17
Issue :
8
Database :
Directory of Open Access Journals
Journal :
Physical Review Special Topics. Accelerators and Beams
Publication Type :
Academic Journal
Accession number :
edsdoj.69f1ab635c3e4e878d788d348909ce85
Document Type :
article
Full Text :
https://doi.org/10.1103/PhysRevSTAB.17.080702