In the present paper the transport of impurities driven by trapped electron
(TE) mode turbulence is studied. Non-linear (NL) gyrokinetic simulations using
the code GENE are compared with results from quasilinear (QL) gyrokinetic
simulations and a computationally efficient fluid model. The main focus is on
model comparisons for electron temperature gra- dient driven turbulence
regarding the sign of the convective impurity velocity (pinch) and the impurity
density gradient R/LnZ (peaking factor) for zero impurity flux. In particular,
the scaling of the impurity peaking factors with impurity charge Z and with
driving temper- ature gradient is investigated and compared with the results
for Ion Temperature Gradient (ITG) driven turbulence. In addition, the impurity
peaking is compared to the main ion peaking obtained by a self-consistent fluid
calculation of the density gradients corresponding to zero particle fluxes.
For the scaling of the peaking factor with impurity charge Z, a weak
dependence is obtained from NL GENE and fluid simulations. The QL GENE results
show a stronger dependence for low Z impurities and overestimates the peaking
factor by up to a factor of two in this region. As in the case of ITG dominated
turbulence, the peaking factors saturate as Z increases, at a level much below
neoclassical predictions. However, the scaling with Z is weak or reversed as
compared to the ITG case.
The scaling of impurity peaking with the background temperature gradients is
found to be weak in the NL GENE and fluid simulations. The QL results are also
here found to significantly overestimate the peaking factor for low Z values.
For the parameters considered, the background density gradient for zero
particle flux is found to be slightly larger than the corresponding impurity
zero flux gradient.Comment: 23 pages, 13 figures. Submitted to AIP: Physics of Plasma
