We consider the microscopic sources of toroidal and poloidal flow in c
onfined magnetoplasmas and the effects of such flows on macroscopic st
ability, The central difficulty is satisfactory modelling of kinetic t
heory effects so as to permit their robust introduction into magnetohy
drodynamic (MHD) codes. It is tentatively concluded that poloidal rota
tion, but not toroidal, is responsible for the computed stabilization
and return to axisymmetry.