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MOPAB142 |
A Compact, Low-Field, Broadband Matching Section for Externally-Powered X-Band Dielectric-Loaded Accelerating Structures |
495 |
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- Y. Wei, C.P. Welsch
The University of Liverpool, Liverpool, United Kingdom
- H. Bursali
Sapienza University of Rome, Rome, Italy
- N. Catalán Lasheras, S. Gonzalez Anton, A. Grudiev, R. Wegner, Y. Wei
CERN, Meyrin, Switzerland
- B.T. Freemire, C.-J. Jing
Euclid TechLabs, Solon, Ohio, USA
- J. Sauza-Bedolla
Lancaster University, Lancaster, United Kingdom
- Y. Wei, C.P. Welsch
Cockcroft Institute, Warrington, Cheshire, United Kingdom
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It has been technically challenging to efficiently couple external radiofrequency (RF) power to cylindrical dielectric-loaded accelerating (DLA) structures. This is especially true when the DLA structure has a high dielectric constant. This contribution presents a novel design of a matching section for coupling the RF power from a circular waveguide to an X-band DLA structure with a dielectric constant εr=16.66 and a loss tangent \tanθ = 3.43× 10-5. It consists of a very compact dielectric disk with a width of 2.035 mm and a tilt angle of 60 degrees, resulting in a broadband coupling at a low RF field which has the potential to survive in the high-power environment. To prevent a sharp dielectric corner break, a 45-degree chamfer is added. Moreover, a microscale vacuum gap, caused by metallic clamping between the thin coating and the outer thick copper jacket, is studied in detail. Based on simulation studies, a prototype of the DLA structure with the matching sections was fabricated. Results from preliminary bench measurements and their comparison with design values will also be discussed.
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Poster MOPAB142 [2.617 MB]
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-MOPAB142
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About • |
paper received ※ 11 May 2021 paper accepted ※ 21 May 2021 issue date ※ 19 August 2021 |
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MOPAB344 |
Machine Learning Models for Breakdown Prediction in RF Cavities for Accelerators |
1068 |
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- C. Obermair, A. Apollonio, T. Cartier-Michaud, N. Catalán Lasheras, L. Felsberger, W.L. Millar, W. Wuensch
CERN, Geneva, Switzerland
- C. Obermair, F. Pernkopf
TUG, Graz, Austria
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Radio Frequency (RF) breakdowns are one of the most prevalent limits in RF cavities for particle accelerators. During a breakdown, field enhancement associated with small deformations on the cavity surface results in electrical arcs. Such arcs degrade a passing beam and if they occur frequently, they can cause irreparable damage to the RF cavity surface. In this paper, we propose a machine learning approach to predict the occurrence of breakdowns in CERN’s Compact LInear Collider (CLIC) accelerating structures. We discuss state-of-the-art algorithms for data exploration with unsupervised machine learning, breakdown prediction with supervised machine learning, and result validation with Explainable-Artificial Intelligence (Explainable AI). By interpreting the model parameters of various approaches, we go further in addressing opportunities to elucidate the physics of a breakdown and improve accelerator reliability and operation.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-MOPAB344
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About • |
paper received ※ 20 May 2021 paper accepted ※ 16 July 2021 issue date ※ 11 August 2021 |
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MOPAB370 |
X-Band RF Spiral Load Optimization for Additive Manufacturing Mass Production |
1143 |
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- H. Bursali
Sapienza University of Rome, Rome, Italy
- N. Catalán Lasheras, R.L. Gerard, A. Grudiev, O. Gumenyuk, P. Morales Sanchez, B. Riffaud
CERN, Geneva, Switzerland
- J. Sauza-Bedolla
Lancaster University, Lancaster, United Kingdom
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The CLIC main linac uses X-band traveling-wave normal conducting accelerating structures. The RF power not used for beam acceleration nor dissipated in the resistive wall is absorbed in two high power RF loads that should be as compact as possible to minimize the total footprint of the machine. In recent years, CERN has designed, fabricated and successfully tested several loads produced by additive manufacturing. With the current design, only one load can be produced in the 3D printing machine at a time. The aim of this study is optimizing the internal cross-section of loads in order to create a stackable design to increase the number of produced parts per manufacturing cycle and thus decrease the unit price. This paper presents the new design with an optimization of the internal vacuum part of the so-called RF spiral load. In this case, RF and mechanical designs were carried out in parallel. The new cross section has showed good RF reflection reaching less than -30 dB in simulations. The final load is now ready to be manufactured and high-power tested. This new load will not only provide cost saving but also faster manufacturing for mass production.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-MOPAB370
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About • |
paper received ※ 18 May 2021 paper accepted ※ 26 May 2021 issue date ※ 23 August 2021 |
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TUPAB076 |
High-Gradient Breakdown Studies of an X-Band Accelerating Structure Operated in the Reversed Taper Direction |
1543 |
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- X.W. Wu, N. Catalán Lasheras, A. Grudiev, G. McMonagle, I. Syratchev, W. Wuensch
CERN, Meyrin, Switzerland
- M. Boronat
IFIC, Valencia, Spain
- A. Castilla, A.V. Edwards, W.L. Millar
Lancaster University, Lancaster, United Kingdom
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The results of high-gradient tests of a tapered X-band traveling-wave accelerator structure powered in reversed direction are presented. Powering the tapered structure from the small aperture, normally output, at the end of the structure provides unique conditions for the study of gradient limits. This allows high fields in the first cell for a comparatively low input power and a field distribution that rapidly falls off along the length of the structure. A maximum gradient of 130 MV/m in the first cell at a pulse length of 100 ns was reached for an input power of 31.9 MW. Details of the conditioning and operation at high-gradient are presented. Various breakdown rate measurements were conducted at different power levels and rf pulse widths. The structure was standard T24 CLIC test structure and was tested in Xbox-3 at CERN.
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Poster TUPAB076 [1.077 MB]
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-TUPAB076
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About • |
paper received ※ 19 May 2021 paper accepted ※ 12 July 2021 issue date ※ 12 August 2021 |
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WEPAB038 |
Commissioning of a New X-Band, Low-Noise LLRF System |
2683 |
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- A.V. Edwards, M. Boronat Arevalo, N. Catalán Lasheras, G. McMonagle
CERN, Meyrin, Switzerland
- A.C. Dexter
Cockcroft Institute, Lancaster University, Lancaster, United Kingdom
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To increase beam energy in the CLEAR facility at CERN and study the CLIC accelerating structure prototype in operating conditions, the first X-band test facility at CERN was upgraded in 2020. Both, the acquisition and software systems at X-band test stand 1 (Xbox1) were upgraded to exhibit low phase noise which is relevant to klystron based CLIC and to the use of crab cavities in the beam delivery system. The new LLRF uses down-conversion which necessitates a local oscillator which can be produced by two different methods. The first is a PLL, a commonly used technique which has been previously employed at the other X-band facilities at CERN. The second is a novel application of a single sideband up-convertor. The up-convertor system has demonstrated reduced phase noise when compared with the PLL. The commissioning of the new system began in late 2020 with the conditioning of a 50 MW Klystron. Measurements of the quality of the new LLRF will be shown. These will compare the PLL and up-convertor with particular attention on the quality of the phase measurements. Also, a preliminary study of phase shifts in the waveguide network due to temperature changes will be presented.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-WEPAB038
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About • |
paper received ※ 13 May 2021 paper accepted ※ 05 July 2021 issue date ※ 20 August 2021 |
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WEPAB374 |
The Southern Hemisphere’s First X-Band Radio-Frequency Test Facility at the University of Melbourne |
3588 |
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- M. Volpi, R.P. Rassool, S.L. Sheehy, G. Taylor, S.D. Williams
The University of Melbourne, Melbourne, Victoria, Australia
- M.J. Boland
CLS, Saskatoon, Saskatchewan, Canada
- M.J. Boland
University of Saskatchewan, Saskatoon, Canada
- N. Catalán Lasheras, S. Gonzalez Anton, G. McMonagle, S. Stapnes, W. Wuensch
CERN, Meyrin, Switzerland
- R.T. Dowd, K. Zingre
AS - ANSTO, Clayton, Australia
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The first Southern Hemisphere X-band Laboratory for Accelerators and Beams (X-LAB) is under construction at the University of Melbourne, and it will operate CERN X-band test stand containing two 12GHz 6MW klystron amplifiers. By power combination through hybrid couplers and the use of pulse compressors, up to 50 MW of peak power can be sent to any of 2 test slots at pulse repetition rates up to 400 Hz. The test stand is dedicated to RF conditioning and testing CLIC’s high gradient accelerating structures beyond 100 MV/m. It will also form the basis for developing a compact accelerator for medical applications, such as radiotherapy and compact light sources. Australian researchers working as part of a collaboration between the University of Melbourne, international universities, national industries, the Australian Synchrotron -ANSTO, Canadian Light Source and the CERN believe that creating a laboratory for novel accelerator research in Australia could drive technological and medical innovation.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-WEPAB374
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About • |
paper received ※ 18 May 2021 paper accepted ※ 06 July 2021 issue date ※ 30 August 2021 |
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WEPAB416 |
Industrialization Study of the Accelerating Structures for a 380 GeV Compact Linear Collider |
3674 |
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- A. Magazinik
Tampere University, Tampere, Finland
- N. Catalán Lasheras
CERN, Meyrin, Switzerland
- S. Mäkinen
Tampere University of Technology, Tampere, Finland
- J. Sauza-Bedolla
Lancaster University, Lancaster, United Kingdom
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The LHC at CERN will continue its operation for approximately 20 years. In parallel, diverse studies are conducted for the design of a future large-scale accelerator. One of the options is the Compact Linear Collider (CLIC) who aims to provide a very high accelerating gradient (100 MV/m) achieved by using normal conducting radiofrequency (RF) cavities operating in the X-band range (12 GHz). Each accelerating structure is a challenging component involving ultra-precise machining and diffusion bonding techniques. The first stage of CLIC operates at a collision energy of 380 GeV with an accelerator length of 11 km, consisting of 21630 accelerating structures. Even though the prototypes have shown a mature and ready to build concept, the present number of qualified suppliers is limited. Therefore, an industrialization study was done through a technical survey with hi-tech companies. The aim is to evaluate current capabilities, to ensure the necessary manufacturing yield, schedule, and cost for mass production. This paper presents the results of the industrialization study for 12 GHz accelerating structures for CLIC 380 GeV, highlighting the principal challenges towards mass production.
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DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-IPAC2021-WEPAB416
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About • |
paper received ※ 19 May 2021 paper accepted ※ 22 June 2021 issue date ※ 14 August 2021 |
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