  Fluid simulation of stellarator edge transport is difficult due to the
complexities of mesh generation; the stochastic edge and strong nonaxisymmetry
inhibit the use of field aligned coordinate systems. The recent implementation
of the Flux Coordinate Independent method for calculating parallel derivatives
in BOUT++ has allowed for more complex geometries. Here we present initial
results of nonaxisymmetric diffusion modelling as a step towards stellarator
turbulence modelling. We then present initial (non-turbulent) transport
modelling using the FCI method and compare the results with analytical
calculations. The prospects for future stellarator transport and turbulence
modelling are discussed.
