Test particle E x B radial flux surface excursions are reduced during
the H-mode. Particle transport is reduced by a factor of 10 in the H-m
ode, but energy confinement increases are small. In the H-mode the evo
lution of poloidally resolved turbulent statistics are not explained b
y published theory. Turbulent momentum transport leads to a concentrat
ion of poloidal momentum within the transport barrier, and compressibi
lity leads to poloidal shock-like phenomena. The electron distribution
functions may be modified by this shock, leading to kinetic instabili
ties. A physics-based understanding of the H-mode must therefore inclu
de toroidal effects combined with an adequate treatment of particle or
bits, plasma compressibility and associated kinetic effects, and at le
ast a two-species model of turbulent transport. The results suggest th
at rapid poloidal core-plasma rotation could form core transport barri
ers without reliance on fluid shear or reversed magnetic shear effects
.