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SUPERBOX is known as a very efficient particle‐mesh code with highly‐resolving sub‐grids. Nevertheless, the height of a typical galactic disc is small compared to the size of the whole system. Consequently, the numerical resolution in  z  direction, i. e. vertically with respect to the plane of the disc, remains poor. Here, we present a new version of SUPERBOX that allows for a considerably higher resolution along  z . The improved code is applied to investigate disc heating by the in‐fall of a galaxy satellite. We describe the improvement and communicate our results. As an important application we discuss the disruption of a dwarf galaxy within a disc‐bulge‐halo galaxy that consists of some 10 6  particles. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

High resolution in z ‐direction: The simulation of disc‐bulge‐halo galaxies using the particle‐mesh code SUPERBOX