One of the main results of the Wendelstein 7-AS stellarator (major radius
2 m, average plasma radius 0.18 m, magnetic field 2.5 T, low shear) is the
achievement of the H-mode confinement in ECR- and NBI-heated plasmas. There
is a strong dependence on the external rotational transform; the H-mode
confinement can be found only in a narrow window close to ι = 1/2.
Viscous damping and the interaction with a neutral background are the only
damping mechanisms proposed so far, which inhibit the poloidal shear flow.
Viscous damping is computed using collisional and weakly collisionless
approximations (plateau regime). Large values of the poloidal viscosity are
found on rational magnetic surfaces, while in the neighbourhood of
low-order rational surfaces the viscosity is very small. Islands provide a
mechanism for enhanced momentum transport in the radial direction, which
leads to an effective shear viscosity. In Wendelstein 7-AS islands exist on
the `natural' rational surfaces with ι = 5/9,5/10,5/11,....
Furthermore, a next generation of islands exist on ι = 10/19,10/21.
Experimental results in Wendelstein 7-AS confirm the hypothesis that the
H-mode only can arise if none of these islands exist in the plasma. The
regions of rotational transform predicted by this hypothesis roughly agree
with those of the experiment.
The extrapolation towards Wendelstein 7-X
shows that a similar case is expected there. Numerical calculations of
islands are made in vacuum fields; the evolution of the islands with rising
plasma pressure is unknown. Finally a qualitative model of H-mode
development is discussed.