It is shown that the magnetic current-driven (`kink-type') instability produces flow and field patterns with helicity and even with α-effect but only if the magnetic background field possesses non-vanishing current helicity B. curl B by itself. Fields with positive large-scale current helicity lead to negative small-scale kinetic helicity. The resulting α-effect is positive. These results are very strict for cylindric setups without z-dependence of the background fields. The sign rules also hold for the more complicated cases in spheres where the toroidal fields are the result of the action of differential rotation (induced from fossil poloidal fields) at least for the case that the global rotation is switched off after the onset of the instability.
Advances in Plasma Astrophysics
- Pub Date:
- June 2011
- magnetic instability;
- radiation zone;
- Astrophysics - Solar and Stellar Astrophysics
- 6 pages, 6 figures, submitted to Proceedings of IAU Symp. 274: Advances in Plasma Astrophysics