  Current spacecraft missions such as Wind and ACE can be used to determine
magnetic correlation functions in the solar wind. Data sets from these missions
can, in principle, also be used to compute so-called Eulerian correlation
functions. These temporal correlations are essential for understanding the
dynamics of solar wind turbulence. In the current article we calculate these
dynamical correlations by using well-established methods. These results are
very useful for a comparison with Eulerian correlations obtained from space
craft missions.
