  We take a three dimensional Euclidian metric in toroidal coordinates and
consider the corresponding Laplace equation. The simplest solution of this
equation is taken. Based on this we build a Weyl space-time. This space-time is
transformed to cylindrical coordinates. It is shown by using Mathematica that
Weyl equations in cylindrical coordinates are satisfied. Geodesic motion is
considered along the symmetric axis as well as along the radii of the
singularity, which is the cause of the space time.
