Abstract
Circularly polarized Alfvén waves give rise to an α-dynamo effect that can be exploited to drive parallel current. In a "laminar" magnetic the effect is weak and does not give rise to significant currents for realistic parameters (e.g., in tokamaks). However, in reversed-field pinches (RFPs) in which magnetic field in the plasma core is stochastic, a significant enhancement of the α effect occurs. Estimates of this effect show that it may be a realistic method of current generation in the present-day RFP experiments and possibly also in future RFP-based fusion reactors.
Original language | English (US) |
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Pages (from-to) | 553-555 |
Number of pages | 3 |
Journal | Physics of Plasmas |
Volume | 5 |
Issue number | 3 |
DOIs | |
State | Published - Mar 1998 |
All Science Journal Classification (ASJC) codes
- Condensed Matter Physics