Characterisation of plasma breakdown at JET with a carbon and ITER-like wall

TitleCharacterisation of plasma breakdown at JET with a carbon and ITER-like wall
Publication TypeJournal Article
Year of Publication2013
AuthorsP.C de Vries, A.C.C. Sips, H.T Kim, P.J Lomas, F. Maviglia, R. Albanese, I. Coffey, E. Joffrin, M. Lehnen, A. Manzanares, M. O'Mulane, I. Nunes, G.J van Rooij, F.G Rimini, M.F Stamp, JET-EFDA Contributors
JournalNuclear Fusion
Volume53
Number5
Pagination053003
Abstract

The recent installation of a full metal, ITER-like, first wall provided the opportunity to study the impact of the plasma-facing materials on plasma initiation or breakdown. This study for the first time presents a full experimental characterisation of tokamak breakdown at JET, using all discharges since 2008, covering both operations with a main chamber carbon and a beryllium ITER-like main chamber wall. It was found that the avalanche phase was unaffected by the change in wall material. However, changes in out-gassing by the wall and lower carbon levels resulted in better controlled density and significantly lower radiation during the burn-through phase with the ITER-like wall. Breakdown failures, that usually developed with a carbon wall during the burn-through phase (especially after disruptions) were absent with the ITER-like wall. These observations match with the results obtained from a new model of plasma burn-through that includes plasma–surface interactions (Kim et al 2012 Nucl. Fusion 52 [http://dx.doi.org/10.1088/0029-5515/52/10/103016] 103016 ). This shows that chemical sputtering of carbon is the determining factor for the impurity content, and hence also radiation, during the burn-through phase for operations with a carbon wall. As seen experimentally, with a beryllium main wall, the plasma surface effects predicted by the model do not raise the radiation levels much above those expected for pure deuterium plasmas. With the ITER-like wall, operation with higher pre-fill pressures, and thus higher breakdown densities, was possible, which helped maintaining the density after breakdown.

URLhttp://www.euro-fusionscipub.org/wp-content/uploads/2014/11/EFDP12030.pdf
DOI10.1088/0029-5515/53/5/053003
Division

FP

Department

PDG

PID

fa61ed1b3df72e37f95ab821a0e68852

Alternate TitleNucl. Fusion
LabelOA

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