We investigate the kinematic dynamo properties of interacting vortex tubes. These flows are of great importance in geophysical and astrophysical fluid dynamics: for al a r g er a n g eo fs ystems, turbulence is dominated by such coherent structures. We obtain a dynamically consistent 2 1 2 -dimensional velocity field of the form (u(x, y, t),v(x, y, t),w(x, y, t)) by solving the z-independent Navier-Stokes equations in the presence of helical forcing. This system naturally forms vortex tubes via an inverse cascade. It has chaotic Lagrangian properties and is therefore a candidate for fast dynamo action. The kinematic dynamo properties of the flow are calculated by determining the growth rate of a small-scale seed field. The growth rate is found to have a complicated dependence on Reynolds number Re and magnetic Reynolds number Rm, but the flow continues to act as a dynamo for large Re and Rm. Moreover the dynamo is still efficient even in the limit Re ≫ Rm,p r o v i ding Rm is large enough, because of the formation of coherent structures.