  Fluid models that approximate kinetic effects have received attention
recently in the modelling of large scale plasmas such as planetary
magnetospheres. In three-dimensional reconnection, both reconnection itself and
current sheet instabilities need to be represented appropriately. We show that
a heat flux closure based on pressure gradients enables a ten moment fluid
model to capture key properties of the lower-hybrid drift instability (LHDI)
within a reconnection simulation. Characteristics of the instability are
examined with kinetic and fluid continuum models, and its role in the
three-dimensional reconnection simulation is analysed. The saturation level of
the electromagnetic LHDI is higher than expected which leads to strong kinking
of the current sheet. Therefore, the magnitude of the initial perturbation has
significant impact on the resulting turbulence.
