Аннотация:A stationary solution is obtained for the dynamo equations of a central magnetic field in the presence of a linear velocity field where a liquid particle is stretched into a filament in the direction of the z axis. In the absence of central turbulence helicity, the magnetic field is distributed along the z axis in the form of a filament with a Gaussian profile. In spiral turbulence, an azimuthal magnetic field component is generated in addition to the longitudinal field. The magnetic field is distributed in the form of a spiral whose pitch and twist direction vary with distance from the z axis.