OUR PROJECT PROVIDES A COMPREHENSIVE PICTURE OF THE FLOW OF MATERIAL AND ENERGY ACROSS LARGE DISTANCES IN THE JOVIAN MAGNETOSPHERE INCLUDING ITS ULTIMATE SOURCES AND SINKS. WE SEEK TO ANSWER FUNDAMENTAL QUESTIONS IN JOVIAN MAGNETOSPHERIC PHYSICS WHICH ULTIMATELY ADVANCE OUR UNDERSTANDING OF MASS TRANSPORT AND ENERGY DEPOSITION IN MAGNETIZED PLASMAS. BY ARCHIVING OUR DATA WITH NASA'S PLANETARY DATA SYSTEM WE LEAVE A LEGACY FOR FUTURE PLANETARY SCIENTISTS TO STUDY THE DYNAMIC PLASMA ENVIRONMENTS OF GIANT PLANET MAGNETOSPHERES.