NASA NTRS · 20050156931
Model for Solar Proton Risk Assessment
Abstract
A statistical model for cumulative solar proton event fluences during space missions is presented that covers both the solar minimum and solar maximum phases of the solar cycle. It is based on data from the IMP and GOES series of satellites that is integrated together to allow the best features of each data set to be taken advantage of. This allows fluence-energy spectra to be extended out to energies of 327 MeV.
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Xapos, M. A., Stauffer, C., Gee, G. B., Barth, J. L., Stassinopoulos, E. G., McGuire, R. E.. 2004-01-01. Model for Solar Proton Risk Assessment. https://ntrs.nasa.gov/citations/20050156931
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