On the magnitude and distribution of halo currents during disruptions on MAST
On the magnitude and distribution of halo currents during disruptions on MAST
复制标题
关于 MAST 中断期间晕流的大小和分布
DOI:
10.1088/0741-3335/49/4/007
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发表时间:
2007
影响因子:
2.2
通讯作者:
D. Taylor
中科院分区:
文献类型:
--
作者:
G. Counsell;R. Martín;T. Pinfold;D. Taylor
Recent results from MAST in which all halo current paths are monitored suggest that, during disruptions, the plasma responsible for the generation of halo current acts more as a voltage source than a current source. As a result the resistance of the current path along which the halo current must flow has a profound impact on the magnitude of the current. This may provide opportunities for directing the current away from sensitive components in future devices such as ITER. Analysis of data from over 3800 disruptions shows that the halo currents on MAST are relatively benign, having a peak value less than 25% of the pre-disruption plasma current with a rather symmetric distribution near the centre column (average toroidal peaking factor ∼1.1). The low peaking factor favourably reduces the tilting/bending forces in the region of the centre column, which has limited space for bulky supports.