The role of kinetic helicity in small-scale fast dynamo action is inve
stigated by employing a simple statistical model for the underlying fl
ow with statistics that are Gaussian distributed, temporally delta-cor
related and spatially homogeneous and isotropic. In order to focus on
small-scale dynamo action we restrict our attention to flows possessin
g no net kinetic helicity. With the help of a diagrammatic technique a
nd a numerical calculation we show that the dynamo growth rate is inde
pendent of the kinetic helicity as the magnetic Reynolds number R-m --
> infinity. It is indicated that the latter enhances the growth of the
magnetic energy only for finite R-m. (C) 1997 Elsevier Science B.V.