A numerical code which solves evolution equations for the densities of each ionization level of oxygen and molybdenum is used for simulating the stationary state of T.F.R. discharges. The authors find that by using neo-classical (Pfirsch-Schluter) fluxes and anomalous 'spreading' fluxes, they obtain the positions of oxygen peaks inwardly displaced from those calculated using the coronal equilibrium model and in reasonable agreement with the experimental measurements. They find also reasonable agreement with the experiment for the emitted photons. In addition, the positions of the maxima of the molybdenum peaks are in agreement with both the coronal equilibrium model and the experimental observations.
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