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BiBTeX citation export for SUSPB011: Magnetic Flux Expulsion in TRIUMF’s Multi-Mode Coaxial Cavities

@inproceedings{gregory:srf2023-mopmb023,
  author       = {R.R. Gregory and T. Junginger and P. Kolb and R.E. Laxdal and M.W. McMullin and Z.Y. Yao},
  title        = {{Magnetic Flux Expulsion in TRIUMF’s Multi-Mode Coaxial Cavities}},
% booktitle    = {Proc. SRF'23},
  booktitle    = {Proc. 21th Int. Conf. RF Supercond. (SRF'23)},
  pages        = {135--140},
  eid          = {MOPMB023},
  language     = {english},
  keywords     = {cavity, simulation, SRF, experiment, controls},
  venue        = {Grand Rapids, MI, USA},
  series       = {International Conference on RF Superconductivity},
  number       = {21},
  publisher    = {JACoW Publishing, Geneva, Switzerland},
  month        = {09},
  year         = {2023},
  issn         = {2673-5504},
  isbn         = {978-3-95450-234-9},
  doi          = {10.18429/JACoW-SRF2023-MOPMB023},
  url          = {https://jacow.org/srf2023/papers/mopmb023.pdf},
  abstract     = {{The external magnetic flux sensitivity of SRF cavities is an important characteristic of SRF accelerator design. Previous studies have shown that n-doped elliptical cavities are very sensitive to external fields, resulting in stringent requirements for residual field and cavity cool-down speed. Few such studies have been done on HWRs and QWRs. The impact of applied field direction and cool-down speed of flux expulsion for these cavities is poorly understood. This study explores the effect of these cool-down characteristics on TRIUMF¿s QWR using COMSOL ® simulations and experimental results. This study seeks to maximize the flux expulsion that occurs when a cavity is cooled down through its superconducting temperature. Flux expulsion is affected by the cool-down speed, temperature gradient, and orientation of the cavity relative to an applied magnetic field. It was found that for a vertically applied magnetic field the cool-down speed and temperature gradient did not have a significant effect on flux expulsion. Contrarily, a horizontal magnetic field can be nearly completely expelled by a fast, high temperature gradient cool-down.}},
}