Jovian Proton and Heavy Ion Models for Spacecraft Design

This presentation will review the results of the latest modeling at the Jet Propulsion Laboratory of the high energy proton and ion environments at Jupiter. The existing models of the proton and ion environments at Jupiter have been revised and extended from the original 12 jovian radii out to 50 jovian radii using the latest Galileo data. In addition to the physical significance of these particle populations, the new models will be important in the evaluation and design of solar arrays at Jupiter as they can affect the radiation damage to the solar array cells and cover glass. The new models represent an important update to the tools currently being used to study the effects of the jovian environment on spacecraft. These models (part of the GIRE family of electron and proton models) are currently used worldwide to describe that jovian environment and are the main tools used by NASA to determine the effects of this environment on spacecraft systems and instruments. The update to be presented is the first significant revision (extending the proton and ion models from 12 Rj to 50 Rj) to the GIRE proton environment since 1983 and fills an important gap in our understanding.