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SUPFDV007 |
Magnetic Field Penetration of Niobium Thin Films Produced by the ARIES Collaboration |
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- D.A. Turner
Cockcroft Institute, Lancaster University, Lancaster, United Kingdom
- G. Burt, K.D. Dumbell, O.B. Malyshev, R. Valizadeh
Cockcroft Institute, Warrington, Cheshire, United Kingdom
- G. Burt
Lancaster University, Lancaster, United Kingdom
- E. Chyhyrynets, C. Pira
INFN/LNL, Legnaro (PD), Italy
- T. Junginger
TRIUMF, Vancouver, Canada
- T. Junginger
UVIC, Victoria, Canada
- S.B. Leith, M. Vogel
University Siegen, Siegen, Germany
- O.B. Malyshev, R. Valizadeh
STFC/DL/ASTeC, Daresbury, Warrington, Cheshire, United Kingdom
- A. Medvids, P. Onufrijevs
Riga Technical University, Riga, Latvia
- R. Ries
Slovak Academy of Sciences, Institute of Electrical Engineering, Bratislava, Slovak Republic
- E. Seiler
IEE, Bratislava, Slovak Republic
- A. Sublet
CERN, Meyrin, Switzerland
- J.T.G. Wilson
STFC/DL, Daresbury, Warrington, Cheshire, United Kingdom
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Superconducting (SC) thin film coatings on Cu substrates are already widely used as an alternative to bulk Nb SRF structures. Using Cu allows improved thermal stability compared to Nb due to having a greater thermal conductivity. Niobium thin film coatings also reduce the amount of Nb required to produce a cavity. The performance of thin film Nb cavities is not as good as bulk Nb cavities. The H2020 ARIES WP15 collaboration studied the impact of substrate polishing and the effect produced on Nb thin film depositions. Multiple samples were produced from Cu and polished with various techniques. The polished Cu substrates were then coated with a Nb film at partner institutions. These samples were characterised with surface characterisation techniques for film morphology and structure. The SC properties were studied with 2 DC techniques, a vibrating sample magnetometer (VSM) and a magnetic field penetration (MFP) facility. The results conclude that both chemical polishing and electropolishing produce the best DC properties in the MFP facility. A comparison between the VSM and the MFP facility can be made for 10 micron thick samples, but not for 3 micron thick samples.
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Poster SUPFDV007 [1.064 MB]
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DOI • |
reference for this paper
※ doi:10.18429/JACoW-SRF2021-SUPFDV007
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About • |
Received ※ 21 June 2021 — Accepted ※ 28 October 2021 — Issue date ※ 09 April 2022 |
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MOPFAV002 |
Commissioning of the UKRI STFC Daresbury Vertical Test Facility for Jacketed SRF Cavities |
308 |
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- A.J. May, A.E.T. Akintola, A.R. Bainbridge, R.K. Buckley, G. Collier, P.A. Corlett, K.D. Dumbell, M.J. Ellis, S. Hitchen, P.C. Hornickel, G. Hughes, C.R. Jenkins, P.A. McIntosh, K.J. Middleman, A.J. Moss, N. Pattalwar, S.M. Pattalwar, M.D. Pendleton, P.A. Smith, A.E. Wheelhouse, AAJ. White, S. Wilde
STFC/DL/ASTeC, Daresbury, Warrington, Cheshire, United Kingdom
- M.D. Hancock, J. Hathaway, C. Hodgkinson, G. Jones, M. Lowe, D.A. Mason, G. Miller, J. Mutch, A. Oates, P. Sollars, J.T.G. Wilson
STFC/DL, Daresbury, Warrington, Cheshire, United Kingdom
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A novel vertical test facility has been developed at the STFC Daresbury Laboratory. The VTF is designed to test 3 jacketed SRF cavities in a horizontal configuration in a single cool-down run at 2 K. Cavities were tested at low power levels for HOMs and passband modes, and Q vs E field measurements at high power levels. The specification requires an unloaded Q of 5·109 at a field gradient of 19.9 MV/m. The cavities are cooled with superfluid helium filled into their individual helium jackets. This reduces the liquid helium consumption by more than 70% in comparison with the conventional facilities operational elsewhere. The facility will be used to conduct a 2-year program to qualify 84 high-beta SRF cavities for the European Spallation Source as part of the UK’s in-kind contribution. This paper reports on the commissioning program, along with a detailed discussion of the RF and cryogenic operations and performance of the facility.
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DOI • |
reference for this paper
※ doi:10.18429/JACoW-SRF2021-MOPFAV002
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About • |
Received ※ 21 June 2021 — Revised ※ 12 July 2021 — Accepted ※ 21 August 2021 — Issue date ※ 20 October 2021 |
Cite • |
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