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  4. Anomaly detection based quench detection system for cw operation of srf cavities

Anomaly detection based quench detection system for cw operation of srf cavities

Publikationstyp
Conference Paper
Date Issued
2022-09-23
Sprache
English
Author(s)
Martino, Gianluca
Eingebettete Systeme E-13
Bellandi, Andrea
Deutsches Elektronen-Synchrotron DESY
Eichler, Annika
Deutsches Elektronen-Synchrotron DESY
Branlard, Julien
Deutsches Elektronen-Synchrotron DESY
Schlarb, Holger
Deutsches Elektronen-Synchrotron DESY
Doolittle, Lawrence R.
Aderhold, Sebastian
Hoobler, Sonya
Nelson, Janice A.
Porter, Ryan D.
Zacarias, L.
Benwell, Andrew L.
Gonnella, Dan A.
Ratti, Alessandro
Fey, Görschwin
Eingebettete Systeme E-13
TORE-URI
https://hdl.handle.net/11420/47750
Start Page
776
End Page
778
Citation
31st International Linear Accelerator Conference, LINAC 2022
Contribution to Conference
31st International Linear Accelerator Conference, LINAC 2022
Publisher DOI
10.18429/JACoW-LINAC2022-THPOPA15
Scopus ID
2-s2.0-85171257323
ISSN
22260366
ISBN of container
978-3-95450-215-8
Superconducting radio frequency (SRF) cavities are used in modern particle accelerators to take advantage of their very high quality factor (Q). A higher Q means that a higher RF field can be sustained, and a higher acceleration can be produced in the cavity for length unity. However, in certain situations, e.g., too high RF field, the SRF cavities can experience quenches that risk creating damage due to the rapid increase in the heat load. This is especially negative in continuous wave (CW) operation due to the impossibility of the system to recover during the off-load period. The design goal of a quench-detection system is to protect the system without being a limiting factor during the operation. In this paper, we compare two different classification approaches for improving a quench detection system. We perform tests using traces recorded from LCLS-II and show that the ARSENAL classifier outperforms a CNN classifier in terms of accuracy.
DDC Class
600: Technology
Funding(s)
Helmholtz Graduate School for the Structure of Matter - Phase 1
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