The reversed field pinch (RFP) is a highly-sheared nearly force-free magnet
ic field configuration, which is almost entirely self-generated, via a dyna
mo process. A still open question is the level of turbulence entailed by th
e dynamo and how it could be mitigated in order to improve plasma confineme
nt. The paper addresses the issue, first discussing the properties of the m
agnetic profiles of RFX in relation to other RFPs, then analysing some tran
sient enhanced confinement modes which suggest that the improved confinemen
t is due to a reduced dynamo action.