Magneto-hydro-dynamic limits in spherical tokamaks
Autor: | T. C. Hender, R. J. Akers, C. M. Roach, S.J. Allfrey, Mikhail Gryaznevich, M. K. Bevir, M. J. Walsh, K. G. McClements, R. J. Buttery, Laurent Villard, C. Ribeiro, M. P. S. Nightingale, Ohjin Kwon, S. E. Sharapov, D. C. Robinson, A. Sykes, L. Appel, I. Jenkins, S. Medvedev, Romualdo Martín |
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Rok vydání: | 1999 |
Předmět: | |
Zdroj: | Scopus-Elsevier |
ISSN: | 1089-7674 1070-664X |
Popis: | The operational limits observed in spherical tokamaks, notably the small tight aspect ratio tokamak (START) device [A. Sykes et al., Nucl. Fusion 32, 694 (1992)], are consistent with those found in conventional aspect ratio tokamaks. In particular the highest β achieved (∼40%) is consistent with an ideal magneto-hydro-dynamic (MHD) Troyon type limit, the upper limit on density is well described by the Greenwald density (πa2ne/Ip∼1) and the normalized current (Ip/aBt) is limited such that q95≳2. Stability calculations indicate scope for increasing both normalized β and normalized current beyond the values so far achieved, although wall stabilization is generally needed for low-n modes. In double null configurations current terminating disruptions occur at each of the operational boundaries, though the current quench tends to be slow at the density limit and disruptions at high β may be due to the low q. In early limiter START discharges, before the divertor coils were installed, disruptions rarely occurred. Instead internal reconnection events which have all the characteristics of a disruption except the current quench occurred. These various disruptive behaviors are explained in terms of a model in which helicity is conserved during the disruption. Due to the low toroidal field beam ions in START, and α particles in a ST power plant, are super-Alfvenic. This gives the possibility for toroidal Alfven eigenmodes (TAEs) to occur and such modes are frequently observed in START neutral beam injection (NBI) discharges, but seem to be benign. The features of these observed TAEs are shown to be in agreement with MHD calculations. |
Databáze: | OpenAIRE |
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