Here we present a study on the dynamics of plane symmetric gravitational collapse in the presence of charge. We consider both adiabatic as well as non-adiabatic flows of viscous fluid. The Einstein and Maxwell field equations are formulated for general plane symmetric space-time in the interior. Junction conditions between the interior and exterior regions are derived. For the adiabatic case, spacetime for the exterior is taken as plane Reissner-Nordstrom while for the non- adiabatic case, it is described by plane symmetric charged Vaidya spacetime. Using Misner and Sharp ...