I. Introduction
Helical Magneto Cumulative Generators (MCGs) have been the subject of extensive study for nearly half a century. It is thought that these types of devices, while capable of amplifying energy significant amounts, have yet to maximize their potential performance due to intrinsic flux losses. While several theories exist as to the cause of the flux loss, insufficient studies on generic MCGs are available to be able to pinpoint its exact nature. The interest in the flux loss associated with and overall performance of helical MCGs prompted their study as part of a Multi University Research Initiative (MURI).