Published 2013
| Version v1
Miscellaneous
Quench limits in the next generation of magnets
- 1. European Organization for Nuclear Research, Geneva (Switzerland)
Description
Several projects around the planet aim at building a new generation of superconducting magnets for particle accelerators, relying on Nb3Sn conductor, with peak fields in the range of 10-15 T. In this paper we give an overview of the main challenges for protecting this new generation of magnets. The cases of isolated short magnets, in which the energy can be extracted on an external dump resistor, and chain of long magnets, which have to absorb their stored energy and have to rely on quench heaters, are discussed. We show that this new generation of magnets can pose special challenges, related to both the large current density and to the energy densities. (author)
Availability note (English)
Available on-line: http://cds.cern.ch/record/1643430/files/arXiv:1401.3931.pdfAdditional details
Identifiers
Publishing Information
- ISBN
- 978-92-9083-394-9
- Imprint Title
- Proceedings of Workshop on Accelerator Magnet, Superconductor, Design and Optimization
- Imprint Pagination
- 90 p.
- Series
- CERN Yellow Reports Series
- Journal Page Range
- p. 10-16
- ISSN
- 0007-8328
- Report number
- CERN--2013/006
Conference
- Title
- Workshop on Accelerator Magnet, Superconductor, Design and Optimization
- Dates
- 15-16 Jan 2013
- Place
- Geneva (Switzerland)
INIS
- Country of Publication
- European Organization for Nuclear Research (CERN)
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 47109267
- Subject category
- S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference, Non-conventional Literature
- Descriptors DEI
- ACCELERATORS; CERN; NIOBIUM COMPOUNDS; QUENCHING; SUPERCONDUCTING MAGNETS; TIN COMPOUNDS
- Descriptors DEC
- ELECTRICAL EQUIPMENT; ELECTROMAGNETS; EQUIPMENT; INTERNATIONAL ORGANIZATIONS; MAGNETS; REFRACTORY METAL COMPOUNDS; SUPERCONDUCTING DEVICES; TRANSITION ELEMENT COMPOUNDS
Optional Information
- Copyright
- Copyright (c) 2013 CERN