Visual utility for the localization of corona-accelerated nuclei

The proton prediction system developed by Smart and Shea (1979) provides the approximate magnitude of the fluxes of solar-flare-ejected protons in the vicinity of the Earth. A system is described that extends Smart and Shea's work, in that it predicts fluxes of such protons at arbitrary points of the inner heliosphere near the plane of the solar equator. It has interactive graphical components that enhance the user's overall perception of a flare's effects upon the solar system, while also providing precise user-requested data. The flux predictions of the system agree well with proton fluxes as measured by various spacecraft. Results are given. A database of flare events is maintained and can be used for a retroactive analysis when it is desired to know the magnitudes of potential proton fluxes due to a previous flare. (Author)