THE GOAL OF THIS PROPOSAL IS TO INVESTIGATE THE ROLE OF PLASMA WAVES IN THE ACCELERATION LOSS AND SCATTERING OF ELECTRONS IN THE JOVIAN MAGNETOSPHERE ALONG AURORAL FIELD LINES AND PARTICULARLY RELATED TO THE FILLING OF THE RADIATION BELTS. TO ACCOMPLISH THIS WE WILL DETERMINE THE GLOBAL DISTRIBUTION OF PLASMA WAVE INTENSITY LEVELS AND CONDUCT DIFFUSIVE MODELING.