We describe plasma profiles evolution during pulsed poloidal current drive experiments performed with the RFX reversed field pinch device. With external drive of edge poloidal current, magnetic fluctuations are reduced suggesting a concomitant reduction of the spontaneous dynamo action. The electron temperature profile is seen to peak in the plasma core, consistently with a reduction of the heat conductivity due to a substantial decrease of MHD dynamo fluctuations. Our results also indicate that the magnetic turbulence due to these fluctuations, which dominates heat transport in the core of the reverse field pinch configuration, does not drive an appreciable heat flux at the edge.[S0031-9007(98)08371-9] PACS numbers: 52.55. Hc, 52.25.Fi, 52.25.Gj, 52.35.Py A growing body of experimental and theoretical work is indicating that in the reverse field pinch (RFP) configuration [1] for magnetic confinement of a thermonuclear plasma a large fraction of the energy losses is due to transport mechanisms linked to MHD turbulence. In fact, magnetic fluctuations are intrinsic to the RFP, since the configuration is usually maintained by a strong dynamo mechanism, which converts part of the energy externally supplied by the toroidal transformer to the poloidal magnetic field component B u into energy associated with the toroidal component B f . This process regenerates toroidal magnetic flux lost by resistive diffusion.Many of the mechanisms (see [2], and references therein, and [3,4]) proposed to explain the dynamo are based on the nonlinear interaction of global, low-m resistive MHD modes resonant inside the toroidal field reversal surface. According to the most developed theory, the MHD dynamo (see [2] for a review), they produce coherent magnetic fieldb and velocityỹ fluctuations which combine to generate an electromotive electric field, E d ͗ỹ 3b͘. This dynamo electric field is found in three-dimensional numerical simulations [5-7] and has been directly measured [8]. Magnetic fluctuations in the RFP are then intimately connected to the dynamo, and in standard conditions they are somewhat unavoidable. This leads to the stochasticization of the magnetic field lines over a large part of the core plasma and, as a consequence, thermal isolation is only provided by a thin layer located at the plasma edge. The mechanism controlling the edge energy transport in a RFP is still a matter of debate, as there are not yet definite conclusions on whether electrostatic or magnetic turbulence is mostly responsible for it. Recent measurements [9][10][11] have shown the existence of a strongly sheared plasma flow in the edge region of a RFP discharge, suggesting a quenching of turbulent transport with a mechanism similar to the one identified in tokamaks [12].Reducing the impact of magnetic turbulence on transport has become one of the major challenges of RFP research. In particular, external poloidal current drive has been proposed as a tool for improving confinement properties of the RFP configuration by alleviating the need of the dyna...