The time-dependent,single-fluid,dissipative magnetohydrodynamic equations are solved in helical coordinates (r,+), where + =8-kz, k= Ag L and L is the periodicity length in the z-direction. The two-dimensional nume•rical calculations simulate theta pinches which have an £= 1 helical field added to them. Given the applied magnetic fields and the initial state of the plasma, we study the time evolution of the system. The plasma is found to experience two kinds of oscillations, occurring on different time scales. These are the radial compression oscillations, and the slower helical osci-1lations of the plasma column. The plasma motion is followed until these oscillations disappear and an equilibrium is nearly reached. Hence given the amplitude and the rise time of the applied magnetic fields, our calculations allow us to relate the initial state of a cold, homogeneous plasma to its final equilibrium state where it is heated and compressed. Furthermore, using the parameters of various experiments, we evaluate the amount of plasma helical distortion..Analytical. expressions for this quantity, in terms of physical parameters, are all obtained with the assumption that the helical distortion ,(normalized to the. plasma 3 radius) is small compared to unity. This assumption being violated in most * experiments, we consider the regime where , r. 1. This experimentally interesting case has to be solved numerically. Our numerical results are then iii I am very grateful to my wife, Muriel, f or her extreme encouragement, her patience and moral support. I also acknowledge many useful discussions with Dr. H. C. Lui in the early stages of4his work.