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Title: Modeling an unmitigated thermal quench event in a large field magnet in a DEMO reactor

Journal Article · · Fusion Engineering and Design
 [1]
  1. Idaho National Lab. (INL), Idaho Falls, ID (United States)

The superconducting magnet systems of future fusion reactors, such as a Demonstration Power Plant (DEMO), will produce magnetic field energies in the 10 s of GJ range. The release of this energy during a fault condition could produce arcs that can damage the magnets of these systems. The public safety consequences of such events must be explored for a DEMO reactor because the magnets are located near the DEMO's primary radioactive confinement barrier, the reactor's vacuum vessel (VV). Great care will be taken in the design of DEMO's magnet systems to detect and provide a rapid field energy dump to avoid any accidents conditions. During an event when a fault condition proceeds undetected, the potential of producing melting of the magnet exists. If molten material from the magnet impinges on the walls of the VV, these walls could fail, resulting in a pathway for release of radioactive material from the VV. A model is under development at Idaho National Laboratory (INL) called MAGARC to investigate the consequences of this accident in a large toroidal field (TF) coil. Recent improvements to this model are described in this paper, along with predictions for a DEMO relevant event in a toroidal field magnet.

Research Organization:
Idaho National Laboratory (INL), Idaho Falls, ID (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Grant/Contract Number:
AC07-05ID14517
OSTI ID:
1193685
Alternate ID(s):
OSTI ID: 1467758
Report Number(s):
INL/JOU-15-33174; PII: S0920379615001659; TRN: US1500532
Journal Information:
Fusion Engineering and Design, Vol. 98-99; Conference: 28. Symposium on Fusion Technology (SOFT-28), San Sebastian (Spain), 29 Sep - 3 Oct 2014; ISSN 0920-3796
Publisher:
ElsevierCopyright Statement
Country of Publication:
United States
Language:
English

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