ESA SEPEM project: Peak flux and fluence model
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A new modelling methodology for the prediction of the solar proton environment a 1 AU is presented. This new method named Virtual Timelines is applied to the SEPEM Reference Event List derived from a long flu time series of space-based measurements to produce the SEPEM model for proton peak flux and fluence at 1 AU. There are several new components including the use of the Lévy distribution for time distributions and the accounting for the non-poin-like nature of SEP events.
CitationJiggens, P.T.A.; Gabriel, S.B.; Heynderickx, D.; Crosby, N.; Glover, A.; Hilgers, A. (2011). ESA SEPEM project: Peak flux and fluence model. , Proceedings of the European Conference on Radiation and its Effects on Components and Systems, RADECS, 549-564, DOI: 10.1109/RADECS.2011.6131436.