Abstract
Density-limit discharges in the W7-AS stellarator, with constant line-integrated density and a duration of up to 2 s, were studied at three values of the toroidal magnetic field (B = 0.8, 1.25 and 2.5 T). The central factor governing the physics of the density limit in stellarators was shown to be the decreasing net power to the plasma when the centrally-peaked radiated power density profile exceeds that of the deposited power density. The process was further accelerated by the peaking of electron density under these conditions. In discharges with B = 2.5 T, simulations of the centrally-peaked radiation power density profiles could be shown to be due to peaked impurity density profiles.
| Original language | English |
|---|---|
| Pages (from-to) | 603-627 |
| Number of pages | 25 |
| Journal | Plasma Physics and Controlled Fusion |
| Volume | 42 |
| Issue number | 6 |
| DOIs | |
| State | Published - Jun 2000 |
| Externally published | Yes |