The technique of driving steady Hall currents in plasmas using a transverse oscillating magnetic field is studied numerically under the approximation of negligible ion flow. The authors model a uniformly dense and resistive spherical plasma bounded by an insulating wall and immersed in a uniform magnetic field which has both an oscillating component (of frequency Omega ) and an orthogonal constant 'vertical' component. The authors formulate the (3-D time-dependent) problem in terms of a spatial expansion in vector spherical harmonics and a temporal expansion in Fourier harmonics.