Paper |
Title |
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WEPRB001 |
The Effect of the SLED Installation on Extracted and Lost Beam at the Australian Synchrotron Linac. |
2794 |
SUSPFO001 |
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- P.J. Giansiracusa, T.G. Lucas, R.P. Rassool, M. Volpi
The University of Melbourne, Melbourne, Victoria, Australia
- M.J. Boland
University of Saskatchewan, Saskatoon, Canada
- M.J. Boland
CLS, Saskatoon, Saskatchewan, Canada
- M.P. Lafky
AS - ANSTO, Clayton, Australia
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A recent upgrade to the high power RF network of the linac at the Australian Synchrotron included a SLED Type 1 Pulse Compressor allowing for the operation of its 100 MeV linac using a single klystron. We explore the effects of the SLED installation on the properties of the beam extracted from the linac with a particular focus on the energy spread and bunch train profile. Additionally, the optical fibre beam loss monitor (oBLM), also recently commissioned, was employed to provide shot-by-shot feedback on loss location and intensity to investigate the change in beam losses.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB001
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About • |
paper received ※ 15 May 2019 paper accepted ※ 20 May 2019 issue date ※ 21 June 2019 |
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WEPRB059 |
Dark Current Analysis at CERN’s X-band Facility |
2944 |
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- D. Banon-Caballero, M. Boronat, V. Sánchez Sebastián, A. Vnuchenko
IFIC, Valencia, Spain
- N. Catalán Lasheras, S. Pitman, M. Widorski, W. Wuensch, V. del Pozo Romano
CERN, Meyrin, Switzerland
- A. Faus-Golfe
LAL, Orsay, France
- B. Gimeno
UVEG, Burjasot (Valencia), Spain
- T.G. Lucas, M. Volpi
The University of Melbourne, Melbourne, Victoria, Australia
- W.L. Millar
Lancaster University, Lancaster, United Kingdom
- J. Paszkiewicz
University of Oxford, Oxford, United Kingdom
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Dark current is particularly relevant during operation in high-gradient linear accelerators. Resulting from the capture of field emitted electrons, dark current produces additional radiation that needs to be accounted for in experiments. In this paper, an analysis of dark current is presented for four accelerating structures that were tested and conditioned in CERN’s X-band test facility for CLIC. The dependence on power, and therefore on accelerating gradient, of the dark current signals is presented. The Fowler-Nordheim equation for field emission seems to be in accordance with the experimental data. Moreover, the analysis shows that the current intensity decreases as a function of time due to conditioning, but discrete jumps in the dark current signals are present, probably caused by breakdown events that change the emitters’ location and intensity.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB059
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About • |
paper received ※ 10 May 2019 paper accepted ※ 22 May 2019 issue date ※ 21 June 2019 |
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WEPRB064 |
High Power Conditioning of X-Band Variable Power Splitter and Phase Shifter |
2964 |
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- V. del Pozo Romano, H. Bursali, N. Catalán Lasheras, A. Grudiev, S. Pitman, I. Syratchev
CERN, Geneva, Switzerland
- C. Serpico
Elettra-Sincrotrone Trieste S.C.p.A., Basovizza, Italy
- M. Volpi
The University of Melbourne, Melbourne, Victoria, Australia
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The three X-band test facilities currently at CERN aim at qualifying CLIC structures prototypes but are also exten- sively used to qualify X-band components operation at high power. In order to upgrade one of the facilities from a single test line to a double test line facility, a high power variable splitter and variable phase shifter have been designed and manufactured at CERN. They have been power tested, first in a dedicated test and also in their final configuration, to en- sure stable power operation before installing them together with an accelerating structure. In this paper, we broadly describe the RF and mechanical design, manufacturing and low power measurements agreement with simulations. We report the high power qualification of both components and their suitability to be used in existing and planned X-band facilities.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2019-WEPRB064
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About • |
paper received ※ 10 May 2019 paper accepted ※ 22 May 2019 issue date ※ 21 June 2019 |
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