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RIS citation export for TUPOTK045: Magnetic Field Mapping of 1.3 GHz Superconducting Radio Frequency Niobium Cavities

TY  - CONF
AU  - Parajuli, I.P.
AU  - Ciovati, G.
AU  - Delayen, J.R.
AU  - Gurevich, A.V.
ED  - Zimmermann, Frank
ED  - Tanaka, Hitoshi
ED  - Sudmuang, Porntip
ED  - Klysubun, Prapong
ED  - Sunwong, Prapaiwan
ED  - Chanwattana, Thakonwat
ED  - Petit-Jean-Genaz, Christine
ED  - Schaa, Volker R.W.
TI  - Magnetic Field Mapping of 1.3 GHz Superconducting Radio Frequency Niobium Cavities
J2  - Proc. of IPAC2022, Bangkok, Thailand, 12-17 June 2022
CY  - Bangkok, Thailand
T2  - International Particle Accelerator Conference
T3  - 13
LA  - english
AB  - Niobium is the material of choice to build superconducting radio frequency (SRF) cavities, which are fundamental building blocks of modern particle accelerators. These cavities require a cryogenic cool-down to ~2 - 4 K for optimum performance minimizing RF losses on the inner cavity surface. However, temperature-independent residual losses in SRF cavities cannot be prevented entirely. One of the significant contributor to residual losses is trapped magnetic flux. The flux trapping mechanism depends on different factors, such as surface preparations and cool-down conditions. We have developed a diagnostic magnetic field scanning system (MFSS) using Hall probes and anisotropic magneto-resistance sensors to study the spatial distribution of trapped flux in 1.3 GHz single-cell cavities. The first result from this newly commissioned system revealed that the trapped flux on the cavity surface might redistribute with increasing RF power. The MFSS was also able to capture significant magnetic field enhancement at specific cavity locations after a quench.
PB  - JACoW Publishing
CP  - Geneva, Switzerland
SP  - 1319
EP  - 1322
KW  - cavity
KW  - SRF
KW  - niobium
KW  - MMI
KW  - radio-frequency
DA  - 2022/07
PY  - 2022
SN  - 2673-5490
SN  - 978-3-95450-227-1
DO  - doi:10.18429/JACoW-IPAC2022-TUPOTK045
UR  - https://jacow.org/ipac2022/papers/tupotk045.pdf
ER  -